P. S. Barklem¹ - N. Christlieb² - T. C. Beers³ - V. Hill ⁴ - M. S. Bessell⁵ - J. Holmberg ^6,7,8 - B. Marsteller ³ - S. Rossi ⁹ - F.-J. Zickgraf ² - D. Reimers²

1 - Department of Astronomy and Space Physics, Uppsala University, Box 515, 751-20 Uppsala, Sweden
2 - Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany
3 - Department of Physics and Astronomy and JINA: Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, MI 48824, USA
4 - GEPI, Observatoire de Paris Meudon, 92125 Meudon Cedex, France
5 - Research School of Astronomy and Astrophysics, Australian National University, Cotter Rd, Weston ACT 2611, Australia
6 - Tuorla Observatory, Väisäläntie 20, 21500 Piikkiö, Finland
7 - Astronomical Observatory, NBIfAFG, Juliane Meries Vej 30, 2100 Copenhagen, Denmark
8 - Nordic Optical Telescope Scientific Association, Apartado 474, 38700 Santa Cruz de La Palma, Spain
9 - Departamento de Astronomia, IAG, Universidade de São Paulo, Rua do Matão 1226, 05508-900 São Paulo - SP, Brazil

Abstract
We present the results of analysis of "snapshot'' spectra of 253 metal-poor halo stars $-3.8\leq {\rm [Fe/H]} \leq -1.5$ obtained in the HERES survey. The snapshot spectra have been obtained with VLT/UVES and have typically $S/N\sim 54$ per pixel (ranging from 17 to 308), $R\sim20~ 000$ , $\lambda = 3760$ -4980 Å. This sample represents the major part of the complete HERES sample of 373 stars; however, the CH strong content of the sample is not dealt with here.

The spectra are analysed using an automated line profile analysis method based on the Spectroscopy Made Easy (SME) codes of Valenti & Piskunov. Elemental abundances of moderate precision (absolute rms errors of order 0.25 dex, relative rms errors of order 0.15 dex) have been obtained for 22 elements, C, Mg, Al, Ca, Sc, Ti, V, Cr, Mn, Fe, Co, Ni, Zn, Sr, Y, Zr, Ba, La, Ce, Nd, Sm, and Eu, where detectable. Of these elements, 14 are usually detectable at the 3 $\sigma$ confidence level for our typical spectra. The remainder can be detected in the least metal-poor stars of the sample, spectra with higher than average S/N, or when the abundance is enhanced.

Among the sample of 253 stars, disregarding four previously known comparison stars, we find 8 r-II stars and 35 r-I stars. The r-II stars, including the two previously known examples CS 22892-052 and CS 31082-001, are centred on a metallicity of ${\rm [Fe/H]} = -2.81$ , with a very small scatter, on the order of 0.16 dex. The r-I stars are found across practically the entire metallicity range of our sample. We also find three stars with strong enhancements of Eu which are s-process rich. A significant number of new very metal-poor stars are confirmed: 49 stars with ${\rm [Fe/H]}<-3$ and 181 stars with $-3<{\rm [Fe/H]}<-2$ . We find one star with ${\rm [Fe/H]}<-3.5$ .

We find the scatter in the abundance ratios of Mg, Ca, Sc, Ti, Cr, Fe, Co, and Ni, with respect to Fe and Mg, to be similar to the estimated relative errors and thus the cosmic scatter to be small, perhaps even non-existent. The elements C, Sr, Y, Ba and Eu, and perhaps Zr, show scatter at ${\rm [Fe/H]} \la -2.5$ significantly larger than can be explained from the errors in the analysis, implying scatter which is cosmic in origin. Significant scatter is observed in abundance ratios between light and heavy neutron-capture elements at low metallicity and low levels of r-process enrichment.

Key words: stars: abundances - stars: population II - Galaxy: abundances - Galaxy: evolution - Galaxy: halo

1 Introduction

The Hamburg/ESO R-process Enhanced Star (HERES) survey has been described in the preceding paper in this series (Christlieb et al. 2004, hereafter Paper I). In this survey, "snapshot'' spectra of 373 very metal-poor stars, here meaning with ${\rm [Fe/H]} \leq -1.5$ as judged from medium resolution spectra, have been obtained with VLT2-UVES, with the main goal of finding stars enhanced in the r-process elements through detection of strong Eu II lines. Though the snapshot spectra are of what would generally be considered low quality for abundance analysis (typically $S/N\sim 54$ , $R\sim20~ 000$ , $\lambda = 3760$ -4980 Å), they contain a wealth of information and abundances may be derived for a significant number of elements with moderate precision (absolute rms errors of order 0.25 dex, relative errors of order 0.15 dex). Modern surveys of metal-poor stars, such as the ESO "First Stars'' Large programme (Cayrel et al. 2004; Hill et al. 2002, and references therein), now obtain significantly better quality spectra for of the order of 70 stars, yet just a decade ago spectra of similar quality to our snapshot spectra were typical for studies of very metal-poor stars (e.g. McWilliam et al. 1995a,b). While high precision (better than 0.1 dex) is expected to be needed to discern detailed patterns in abundance distributions which might serve as diagnostics of early nucleosynthesis (e.g. Karlsson & Gustafsson 2001), the large number of stars observed in the HERES survey offers the possibility to investigate more general trends in metal-poor star abundances in a previously unexplored statistical regime. In particular, the scatter in abundance distributions may provide insights into mixing and the diversity of supernovae at early epochs. The study of Norris et al. (2001), which investigated such scatter, drawing from different surveys in the literature, had of order 70 stars in this metallicity regime. This project provides a homogeneously analysed sample of several hundred stars.

In this paper we analyse a total of 253 of the spectra using an automated spectrum analysis technique based on the Spectroscopy Made Easy (SME) codes by Valenti & Piskunov (1996). In Sect. 2 the sample, observations, and choice of initial stellar parameters will be described. In Sect. 3 the automated analysis technique and codes are described, including the line list, detection classification and error analysis, and the method is tested through comparisons with previously studied stars and tests of the robustness of the method. The results are presented in Sect. 4, including the new interesting stars found in the survey. In Sect. 5, we discuss general trends in the results and other interesting features to emerge. Finally, in Sect. 6 we present our conclusions and discuss possible uses for the data set.

**Table 1:** The sample. The entire table is available only electronically. Coordinates of the HES stars (prefix HE) have been derived from the Digitized Sky Survey I and are accurate to 1 $^{\prime \prime }$ ; the coordinates of the HK survey stars (prefix CS) are from identifications of the sources in the 2MASS All Sky Release. Barycentric radial velocities $v_{\rm rad}$ were measured from the snapshot spectra and are accurate to a few km s^-1.
Star	$\alpha(2000.0)$	$\delta(2000.0)$	$v_{\rm rad}$
			[km s^-1]
CS 22175-007	02 17 26.6	-09 00 45	-18.3
CS 22186-023	04 19 45.5	-36 51 35	51.9
CS 22186-025	04 24 32.8	-37 09 02	-122.6
CS 22886-042	22 20 25.8	-10 23 20	-220.6
CS 22892-052	22 17 01.6	-16 39 27	14.5
CS 22945-028	23 31 13.5	-66 29 57	388.9
CS 22957-013	23 55 49.0	-05 22 52	-213.5
CS 22958-083	02 15 42.7	-53 59 56	175.6
CS 22960-010	22 08 25.3	-44 53 56	49.2
CS 29491-069	22 31 02.1	-32 38 36	-375.5
$\vdots$	$\vdots$	$\vdots$	$\vdots$
HE 2338-1618	23 40 36.2	-16 01 28	-219.4
HE 2345-1919	23 47 55.4	-19 02 37	119.4
HE 2347-1254	23 50 09.8	-12 37 50	-43.5
HE 2347-1334	23 50 26.9	-13 17 39	-54.8
HE 2347-1448	23 49 58.3	-14 32 16	-165.1

2 Observations and sample

The target selection for HERES and observational details have been described in Sect. 3 of Paper I. The spectra were obtained with the ESO-VLT2 and UVES, and cover a wavelength range of 3760-4980 Å, and have an average signal-to-noise ratio of $S/N\sim 54$ per pixel over the spectral range, though some spectra have S/N as low as 17 and as high as 308. A 2 $^{\prime \prime }$ slit is employed giving a minimum resolving power of $R\approx 20~000$ , though typically the resolving power is seeing limited and thus slightly better. As mentioned in Paper I, the pipeline-reduced spectra are employed, corrected to the stellar rest frame. The sample of analysed stars is given in the electronic Table 1 with coordinates and barycentric radial velocities. The final stellar parameters of the sample are presented in Table 2, together with the abundances for convenience, and are plotted in Fig. 1. The [Fe/H] distribution for the sample from the final analysis is shown in Fig. 2. Though observations of adequate quality have been obtained for 373 stars, not all are analysed in this paper. Spectra showing strong molecular carbon features cannot be analysed by our current method, and thus 72 such spectra from the survey are not included in this sample for this reason. These spectra are, however, of great interest and it is planned that they will be analysed separately in future. Further, some stars which turned out to be too Fe-rich ( ${\rm [Fe/H]}>-1.5$ ) or too cool for our analysis method (<4200 K), or are suspected to be spectroscopic binaries or rotators, were also removed from the sample. For a small number of stars, we have not yet obtained adequate photometry and they are also removed from the sample. Thus, the final sample of stars analysed in this work presented in Tables 1 and 2 contains 253 stars.

2.1 Photometry and effective temperatures

To begin our analysis we require as accurate as possible estimates of the effective temperatures of HERES targets. This is particularly the case since, as noted below, the snapshot spectra we obtain are not generally of sufficiently high quality to derive precise spectroscopic temperature estimates. Hence, over the course of the past few years, we have obtained broadband $BVR_{\rm C}I_{\rm C}$ (where the subscript "C'' indicates the Cousins system) observations for as many HERES targets as possible, using the ESO/Danish 1.5 m telescope on La Silla and the DFOSC instrument. The observing and reduction techniques for this data are described in Beers et al. (2005, in preparation). We also make use of near-infrared ${\it JHK}$ photometry from the 2MASS Point Source Catalog (Cutri et al. 2003). The complete set of available photometry for stars in the HERES sample will be published in Beers et al. (2005, in preparation), a compilation of photometry for more than 1500 metal-poor stars and horizontal-branch candidates. The adopted reddening is taken from the maps of Schlegel et al. (1998), adjusted to account for distance. Note, all but the brightest giants of our sample lie outside the reddening layer and thus for most stars the full reddening is applied. The reddening data will also be presented in Beers et al.

Temperature estimates are obtained on the scale of Alonso et al. (1999). Note that, while the majority of the colour calibrations of Alonso et al. require measurements on the Johnson system, the near-IR colours J-H and J-K are on the TCS system (the photometric system at the 1.54 m Carlos Sanchez telescope; Arribas & Martinez-Roger 1987). Thus we first have to apply several transformations of our observed colours. We follow the prescription described by Sivarani et al. (2004). In performing our transformations, and for carrying out the Alonso et al. estimates of effective temperature, we made use of a program kindly provided to us by Sivarani. In order to arrive at a final "best estimate'' of the effective temperatures for our HERES pilot sample stars, we take a straight average of the derived estimates from different colour criteria, after trimming off the highest and lowest estimates for each star. The estimated effective temperatures, for the colours we had available, are provided in Table 2. Although errors in the determinations of temperature for individual colours arising from photometric errors can range from 50-100 K (for the optical colours), and up to several hundred K for the near-IR colours (owing to the generally larger errors in the 2MASS photometry), we conservatively estimate that our final determination of effective temperature has an absolute rms error of 100 K. We note that our photometry is incomplete, i.e. we do not have measurements of all colours for every star, and this incompleteness, together with the trimming in the averaging procedure, means there is an error introduced due to differences in the temperature scales from different colour criteria. Since the incompleteness is effectively random, this should lead only to a slight increase in random scatter. This has been considered in our error estimates. The error due to uncertain reddening (see discussion below) was also considered. We plan to obtain improved photometric estimates of $T_{\rm eff}$ for stars of particular interest on the HERES program (for instance, those noted to be r- and/or s-process enhanced) by measuring more precise ${\it JHK}$ photometry in the near future.

As will be discussed in Sect. 3.5.1, our temperatures are found to be systematically warmer than those found in the literature for the stars where comparisons can be made. This discrepancy was traced primarily to the use of different reddening maps. In this work, the maps of Schlegel et al. (1998) have been employed, while in the past most workers have used the maps of Burstein & Heiles (1982). We computed reddenings and effective temperatures using both maps and find systematic differences as seen in Fig. 3, the results using the maps of Burstein & Heiles being cooler than those found using Schlegel et al. by $70\pm58$ K. We have chosen to use the Schlegel et al. estimates, which have superior spatial resolution and are thought to have a better determined zero point. We note, however, that Arce & Goodman (1999) have pointed out that the Schlegel et al. maps may overestimate the reddening values when E(B-V) exceeds about 0.15 mag, though none of the stars considered here exceed that value (see also Beers et al. 2002 for further discussion).

It should be noted that while the HERES target selection aims at a cutoff of B-V>0.5, a number of warmer stars which turned out to be bluer than our targeted cutoff have also been included due to incorrect estimated B-V colours from the HES prism plates.

As will be described later in Sect. 3.3, we compute individual abundances for all Fe lines and thus can compare our adopted temperature scale with that implied by excitation equilibrium. Given the lines available to us, the spectroscopic data are not of sufficient quality to determine precise excitation temperatures, but one can make a comparison of the average temperature scale. Figure 4 plots the histogram of slopes of the best fit to the Fe I line abundances against excitation. On average the distribution is skewed towards negative slopes, indicating that our temperature scale is on average warmer than would be obtained from excitation equilibrium. Such trends have been noted in previous works on metal-poor giants and dwarfs, for example by Norris et al. (2001) and Cohen et al. (2004).

2.2 Other atmospheric parameters

Estimates of the metallicity, [Fe/H], which serve as initial guesses for our automated analysis, are derived from the medium-resolution spectra obtained during the course of the large-scale campaign to identify suitable targets for the HERES program (see Paper I), in combination with available B-V and J-K photometry. Estimates of [Fe/H] were obtained from the calibration of the Ca II K-line index, KP, along with the B-V colour, described by Beers et al. (1999). For most stars this calibration should be accurate to on the order of 0.2 dex, given spectra and photometry of suitable quality. In addition, we carried out a new calibration, making use of available J-K colours, and a newly-trained artificial neural network procedure (see Snider et al. 2001), to provide an alternative initial estimate of [Fe/H]. This latter step was taken because the HERES targets include objects that are known to be carbon-enhanced; the strong CH G-bands in these objects could possibly perturb the B-V colours used in the Beers et al. calibration. We take the average of the two determinations as our initial guess for [Fe/H]. The differences between the adopted initial guess and the final [Fe/H] values from the automated analysis of the high-resolution spectra are plotted in Fig. 5, and application of robust methods (see, e.g., Beers et al. 1990) to the set of differences in the initial and final metallicity determinations yield estimates of the mean offset and standard deviation of +0.04 dex and 0.27 dex, respectively. The mean estimated relative error for the high-resolution abundance determinations of [Fe/H] is 0.12 dex (see Sect. 3.4 and Table 2), indicating that the medium-resolution estimates have relative errors of about 0.24 dex. Note that the [Fe/H] estimates for the worst outliers were often based on rather noisy medium-resolution spectra.

An initial estimate of the surface gravity, $\log g$ , is also required, which is refined in the automated analysis. For stars on the subgiant and giant-branch stages of evolution, it is well known that $\log g$ correlates very well with effective temperature. Hence, in order to obtain a first-pass estimate of surface gravity we used the reported temperatures and surface gravities by Honda et al. (2004) to derive the regression relation:

As will be described in the next section, a 1D analysis is employed and turbulent line broadening is modelled via the classical microturbulence $\xi$ and macroturbulence $v_{\rm macro}$ parameters. These parameters are derived from the spectrum. Initial guesses of $\xi=1.8$ km s^-1 and $v_{\rm macro}=1.5$ km s^-1 were employed. The final values of $\xi$ derived from the spectrum are given in Table 2 and plotted in Fig. 7, showing the usual correlation with gravity. Note that the stars lying above the main trend, around $\log g \sim 2$ are the red horizontal branch stars (see Fig. 1).

3 Automated spectrum analysis

3.1 Analysis code

Software for automated analysis of the spectrum has been developed, based on the Spectroscopy Made Easy (SME) package by Valenti & Piskunov (1996). SME consists of three components: a spectrum synthesis component written in C++, a parameter optimisation component written in IDL, and a user interface written in IDL. In this work we make use of the first two components. Our developed software is written in IDL, and essentially provides an alternative interface to the parameter optimisation component, which in turn calls the spectrum synthesis component. We also made some minor adaptations and improvements to the SME codes, the most important of which are discussed below. The new interface software takes our input data and provides it to the parameter optimisation component without any need for user interaction. The input data in this case consist of a pipeline-reduced count spectrum with corresponding measurement error spectrum (corrected to the stellar rest frame), initial guess stellar atmosphere parameters and abundances (see Sect. 3.3), and a list of spectral features with corresponding atomic or molecular data (see Sect. 3.2). The main tasks of the new interface software are, in a completely automated fashion, to extract relevant spectral regions appropriate for the line list, to identify continuum points and normalise the spectra relative to the continuum, to make small adjustments (within the error of the wavelength calibration) to line central wavelengths such that they match the observed line centres, and to reject lines polluted by artifacts such as cosmic ray hits. The continuum points are identified by an automated procedure where for each spectral region required for the analysis, the continuum is determined for a wide region, including the desired spectral region and 7 Å on each side by iteratively fitting a low order polynomial to the count spectrum and discarding points more than one standard deviation below the fitted line in the subsequent iteration, thereby converging to the continuum high points. Cosmic ray hits are identified by being significantly above this fit.

Given the input data in the correct form, the SME parameter optimisation code can then solve for any desired model parameters. The parameter optimisation code uses the Marquardt algorithm (Marquardt 1963; Press et al. 1992) to obtain estimates of the parameters, through minimising the $\chi^2$ statistic comparing model and observed spectra.

The spectrum synthesis assumes LTE and a 1D plane-parallel model of the atmosphere, where turbulence is modelled through the classical microturbulence and macroturbulence parameters. Note that in recent versions of SME, molecular line formation is supported (see Valenti et al. 1998), and for speed the radiative transfer is solved using a Feautrier scheme (e.g. Mihalas 1978) not a Runge-Kutta scheme (cf. Valenti & Piskunov 1996). The original spectrum synthesis code did not account for scattering in the source function, i.e. continuous scattering is treated as absorption and thus $S_\nu = B_\nu$ . Rayleigh scattering by neutral hydrogen can be an important contributor to continuous opacity particularly in the ultraviolet for metal-poor stars, especially giants, and thus it is important to treat continuous scattering correctly in the source function (e.g. Griffin et al. 1982). It should be computed as $S_\nu = (1-\epsilon_\nu) J_\nu + \epsilon_\nu B_\nu$ where $\epsilon_\nu$ is the photon thermalisation probability given by $\kappa_\nu/(\kappa_\nu+\sigma_\nu)$ where $\kappa_\nu$ is the absorption coefficient (including line absorption) and $\sigma_\nu$ is the continuum scattering coefficient. This has been implemented into the SME spectrum synthesis code, where the mean intensity $J_\nu$ has been solved using the perturbation technique of Cannon (1971). Further minor improvements included correction of Thorium partition functions (see Paper I), and the ability to handle data for line broadening by neutral hydrogen collisions from the Anstee, Barklem & O'Mara theory (see Sect. 3.2).

A grid of 1D, plane-parallel, LTE models covering the stellar atmosphere parameter space of the stars of interest, namely low metallicity F, G, and K stars from the main sequence to the giant stage, was computed using the 1997 MARCS code (Asplund et al. 1997; Gustafsson et al. 1975). All models use scaled solar abundances with the exception of the alpha-elements, which are enhanced by 0.4 dex. Throughout this paper solar abundances means those of Grevesse & Sauval (1998), except C which is taken from Allende Prieto et al. (2002). Microturbulence in the line blanketing of 2 km s^-1 was adopted as most of our stars are giants (see Fig. 7). This should not have a great effect in metal-poor stars in any case. This model grid was incorporated into SME, allowing SME to solve for atmospheric parameters, where specific models are obtained by interpolation.

In Sect. 3.3 we will describe how we apply this code. First we describe the adopted line list.

3.2 Line list

A list of spectral lines and corresponding atomic and molecular data, suitable for our sample of stars, observational data, and analysis technique is required. For our automated line profile analysis technique, spectral windows where the model and observed spectrum are to be compared need also to be defined.

The lines and spectral windows used are listed in Tables A.1-A.5 in Appendix A, along with comments on each element. Note that in order to avoid the cores of strong lines, any wavelength points in the chosen spectral windows where the observed flux is less than 0.5 of the continuum are automatically rejected. The line list and windows were, for the most part, built by selecting suitable lines from previous studies, particularly McWilliam et al. (1995a,b), Norris et al. (1996), and Sneden et al. (1996). As our technique is automated, our aim is to build a line list which requires either no adjustment from star to star, or possibly a small amount of adjustment that can be automated based on criteria that are known in advance of the analysis, such as stellar temperature. We must therefore be more selective than in interactive analyses. One must keep in mind, however, the need to have as many lines as possible to provide better statistics, which is particularly important for low-quality spectra. Ideally we would like to choose lines which for all stars of the type we are examining are unblended, or which are partially blended in such a way that they can be used if an appropriate comparison window is chosen that neglects the blended part of the line (usually one wing of the line).

Our first step for selecting the lines was to apply all candidate lines to an automated abundance analysis of four stars viewed to be extreme cases of possible blending for metal-poor stars. We used HD 20, moderately r-process enhanced, which is one of the most metal-rich of our stars, non-carbon-enhanced; CS 31082-001, an r-process enhanced, non-carbon-enhanced star; CS 22892-052 an r-process enhanced, carbon-enhanced star; and HE 0338-3945, an r- and s-process enhanced, carbon-enhanced star. Based on examination of the four spectra we chose appropriate spectral windows for each line, rejecting lines where a suitable window for all four stars could not be easily chosen. We then performed an abundance analysis of each star and rejected lines which were not well fit by the derived abundance with respect to the majority of lines of that element, indicating most likely an unresolved blend, or possibly poor atomic data. Special attention was paid to lines that were blended in the carbon-enhanced stars, but not in the carbon-normal stars. We chose to only make use of these lines for the carbon-normal stars, as described below. These lines are marked with an asterisk in the line list. To err on the side of caution, we also used some other very carbon-enhanced stars in the sample, which we deemed too carbon-rich for our present method, to indicate other lines which could be blended by carbon features. Finally, the line list and windows were refined based on testing using the complete sample.

We empirically determined that the lines noted above to be blended in the carbon-enhanced stars, could be safely applied in stars where the G band has a depth not greater than 0.6 of the continuum flux. Further, in the warmer stars some chosen lines lie in the wings of high Balmer lines. Thus, we empirically derived a scheme for application of the line list to a given star. The list is applied to all stars with the following adjustments:

While the employed spectral lines were chosen from the above mentioned previous studies, we compiled our own atomic data for these lines, though often guided by these works. In particular, we attempted to update the data. The adopted oscillator strengths are discussed for each element in Appendix A. The VALD database (Kupka et al. 1999) and NIST Atomic Spectra Database (see also Wiese et al. 1969; Wiese & Martin 1980; Martin et al. 1988; Fuhr et al. 1988) were used extensively, particularly for wavelengths and excitation energies. Radiative broadening, Stark broadening and collisional broadening by neutral hydrogen are included, though the data have not been presented in the tables; they may be obtained from the authors on request. Radiative broadening is taken in all cases from VALD, which is supplied from the calculations by Kurucz (1995). Collisional broadening by neutral hydrogen is, where possible, described by the Anstee, Barklem and O'Mara theory (e.g. Anstee & O'Mara 1991; Barklem et al. 2000 and references therein). In the absence of such calculations the data are taken from VALD which again originates from Kurucz (1995) using the van der Waals theory (Unsöld 1955) with a detailed calculation of the long range interaction constant C₆. In the absence of data from both of these sources the classical van der Waals theory is used, where C₆ is estimated by the usual Unsöld approximation. In both the last two cases we apply an enhancement of a factor of 2. Stark broadening is taken from VALD where available, which often originates from Kurucz (1995). We note that since the lines are typically weak, collisional mechanisms are generally not important, except in a few lines which attain significant strength (e.g. the strongest lines of Mg, Sr and Ba).

Where possible we have considered the hyperfine structure of spectral lines. Hyperfine structure is typically seen in elements with odd atomic numbers. Though Sr and Ba have even atomic numbers, in the solar system they have non-negligible abundances of isotopes with odd atomic masses, and thus hyperfine structure must be considered in these elements also. Isotopic mixtures and splitting have been considered in Sr, Ba and Eu. In all other elements the dominating natural isotope is assumed (or equivalently in the case of even atomic numbers that isotopes with even atomic masses dominate and they have negligible isotope shift). Details of adopted hyperfine structure and isotopic ratios are discussed for each element in Appendix A where it is considered. Hyperfine structure and isotopic splitting have been omitted from the tables for compactness. They may be obtained on request from the authors.

3.3 Procedure

We now describe the procedure used for analysis of the spectra. The goal is to determine the required stellar atmosphere parameters and abundances from the spectra in the best possible way. In Sect. 3.1 a code was described which can analyse a given spectrum to obtain best estimates of chosen model parameters. While the code can in principal analyse the entire set of spectral lines and obtain all desired stellar parameters and abundances simultaneously in one step, this is not done, since for cases with many free model parameters such a procedure is susceptible to errors if strong dual dependencies of the model spectra on parameters exists. Thus, our procedure, like traditional analyses, separates the determination of stellar parameters using appropriate spectral features from the determination of abundances as we now describe.

First, the $T_{\rm eff}$ from Sect. 2.1 is adopted and held fixed throughout. We experimented with refining $T_{\rm eff}$ from the spectra (essentially excitation equilibrium of Fe I), but found that the spectra are not of sufficiently high quality given the spectral features available to us. Thus we need to solve for the atmosphere parameters surface gravity $\log g$ , microturbulence $\xi$ , macroturbulence $v_{\rm macro}$ , and metallicity [Fe/H]. Once these parameters are known we then solve for the individual abundances. All stars are assumed to be slow rotators; we adopt $v \sin i = 1$ km s^-1 for all stars, and this has no effect on the final abundances. Since the resolving power of observations can vary from star to star, we fix the instrumental broadening at a value R=50 000, significantly higher than expected and allow the derived macroturbulence to compensate for the difference. Thus our derived $v_{\rm macro}$ includes both the macroturbulence and a degree of the instrumental profile.

Our basic procedure is broken into three steps. In the first two steps we employ only the Fe and Ti lines of our list. In the first step initial estimates of $T_{\rm eff}$ , $\log g$ , [Fe/H], $\xi$ and $v_{\rm macro}$ as described in Sects. 2.1 and 2.2 are adopted. The initial guess Ti abundance is chosen to be a scaled solar value based on the [Fe/H] initial guess. We then solve for the Fe and Ti abundances, $\log \epsilon_{\rm Fe}$ and $\log \epsilon_{\rm Ti}$ to obtain better initial estimates of these parameters before solving for the remaining stellar parameters.

The second step repeats the first, but now $\log g$ , $\xi$ and $v_{\rm macro}$ are also free parameters. The minimisation to solve for $\log g$ is in essence equivalent to performing an ionisation equilibrium procedure for Fe and Ti. The resultant parameters ( $\log g$ , $\xi$ , $v_{\rm macro}$ , [Fe/H], $\log \epsilon_{\rm Ti}$ ) are then adopted and held fixed for stage three, the analysis of lines of elements other than Fe and Ti in the list, where the only free parameters are the elemental abundances. All the remaining elements are considered separately, as this is most computationally efficient. Solar abundances scaled by [Fe/H] are adopted as initial guesses, which was found usually to be satisfactory; on rare occasions where convergence was not achieved this could be solved by searching for an initial guess which resulted in convergence. Note that in all steps, the single abundance which gives the best global fit to the spectrum is derived. It is also worth noting that we adopt scaled solar abundances for all elements which we do not analyse, except O which we assume enhanced by +0.4 dex; these abundances enter the molecular equilibrium and continuous opacity calculations.

An additional stage is performed for checking purposes. In this stage we analyse the Fe and Ti line list keeping all parameters fixed to those derived in the above stages except the abundance which may now vary from line to line (in SME this can be achieved in practice by fixing the abundance and solving for $\log gf$ for each line, and observing the change from the $\log gf$ -value in the line list). This permits us to check for trends with excitation and ionisation stage, which might warn of deficiencies in the adopted model.

Three further steps are then performed which are required for the error analysis, the details of which will be described below in Sect. 3.4 and in Appendix B. However, for the error analysis we will require partial derivatives describing the dependence of each abundance on $T_{\rm eff}$ , $\log g$ and $\xi$ . Thus we solve for all abundances with fixed stellar parameters except that $T_{\rm eff}$ , $\log g$ and $\xi$ are offset by 100 K, 0.3 dex and 0.2 km s^-1 in each step respectively. We note that these last three steps increase computing time significantly (they comprise more than 1/2 of the computing time). However, we view the error analysis as important enough to justify this increase.

It is worthwhile to make some comment on computing times. With the large number of molecular lines, isotopic and hyperfine components, our line list results in approximately 900 individual line components to be included in the spectrum synthesis, which is where the vast majority of computation is used. Model convergence typically requires approximately 3.5N+13 model spectrum calculations, where N is the number of free parameters (Valenti & Piskunov 1996). This means for the main abundance step (step 3) we require of the order of 15 model spectrum calculations of the complete spectrum. This is repeated three additional times for the error calculations. With a modern workstation typical computation times per star are of the order of 2-3 hours.

3.4 Elemental detections and errors

A first important step before assigning an error to a derived abundance is to determine if there is in fact a reliable detection. A Gaussian is fit to each line and the approximate equivalent width W is determined. Following Norris et al. (2001), the error in W is then computed as $\sigma_W = \lambda\sqrt{n}/(R[S/N])$ where R is the resolving power, n the number of pixels integrated to obtain W, and S/N the signal to noise ratio per pixel. In all cases we adopted R=20000 and adopted the full-width of the fitted Gaussian measured in pixels for n. By then computing $m= W/\sigma_W$ we classify a $m\sigma$ detection of the line. For each element we count the number of lines detected at the $3\sigma$ level or better. If the element has at least one line detected at the $3\sigma$ level we assign the abundance as a detection. Otherwise the element is regarded as undetected, and the derived abundance discarded. Due to the possibility of weak blending, even in high quality spectra, it was further required that a line must be deeper than 10% of the continuum flux for a valid detection. Due to decreased likelihood of blending in the redder parts of the spectrum, we relaxed this condition to 5% for lines redder than 4500 Å. A similar detection scheme was used for CH bands, though W and n for the considered band must be estimated by a different technique.

As one of the main goals of this work is to look at abundance scatter at low metallicities, and given the relatively low quality of the data, it is vital to have error estimates which are as accurate as possible to distinguish real scatter from that due to uncertainties. Thus, we have put significant effort into obtaining realistic error estimates.

**Table 3:** Comparison of our final stellar parameters with those adopted in the literature for the comparison stars. $T_{\rm eff}$ derived with the reddening maps of Burstein & Heiles (1982) instead of Schlegel et al. (1998) are also given for comparison.
Star	This work	Literature	Reference/note
	$T_{\rm eff}$	$\log g$	[Fe/H]	$\xi$	$T_{\rm eff}$	$\log g$	[Fe/H]	$\xi$
	[K]	[cm s^-2]		[km s^-1]	[K]	[cm s^-2]		[km s^-1]
HD 20	5445	2.39	-1.58	2.30	5351				Alonso et al. (1999)
					5475	2.8	-1.4	2.0	Burris et al. (2000)
					5375	2.41	-1.4	1.90	Fulbright & Johnson (2003)
	5416								Using Burstein & Heiles (1982)
HD 221170	4648	1.57	-2.14	2.22	4410				Alonso et al. (1999)
					4425	1.0	-2.0	1.5	Burris et al. (2000)
					4500	0.9	-2.1	2.75	Fulbright (2000)
					4475	1.15	-2.2	2.40	Fulbright & Johnson (2003)
	4548								Using Burstein & Heiles (1982)
CS 22186-025	4985	1.70	-2.87	2.14	4900	1.5	-3.0	2.0	Cayrel et al. (2004)
	4887								Using Burstein & Heiles (1982)
CS 22892-052	4884	1.81	-2.95	1.67	4800	1.5	-3.1	1.95	Sneden et al. (2003)
	4843								Using Burstein & Heiles (1982)
CS 31082-001	4922	1.90	-2.78	1.88	4825	1.5	-2.9	1.8	Hill et al. (2002)
	4874								Using Burstein & Heiles (1982)

Usually in analyses of stellar spectra, systematic errors are expected to dominate. This is not necessarily the case here. For elements with a small number of spectral features, the low S/N means that random measurement errors can be significant. However, for elements with a significant number of spectral features, e.g. Fe, measurement errors are in fact quite small, and systematic errors will dominate.

Our method for calculating errors in abundances and abundance ratios is detailed in Appendix B. First, we should emphasise that we make a distinction between absolute and relative errors. In our discussion we will refer to the uncertainty in the absolute abundance or abundance ratio as the absolute error, and the uncertainty in the relative abundance between stars, that is from star to star, as the relative error. Appendix B provides a formalism for calculation of both absolute and relative errors; however, throughout this paper, unless otherwise stated we discuss the relative error. This is of most interest as we are interested in distributions of abundances. The main difference between absolute errors and relative errors is that some systematic sources of error are presumed to cancel in the latter, in particular, errors in oscillator strengths and some part of the errors incurred from modelling uncertainties such as LTE and 1D. We note however, that as our sample covers such a large stellar parameter space, the cancellation of errors from the modelling will be only partial.

The error estimates include contributions from uncertainties in the observations, atomic and molecular data, continuum fitting, stellar parameters, model atmospheres and inherent assumptions in the spectrum modelling such as LTE and 1D. We have included as many sources of error as possible, however, some of these uncertainties are difficult to estimate quantitatively, particularly those related to the model atmospheres and modelling assumptions. Our abundances and error estimates are provided with the explicit understanding that they are based on traditional 1D LTE models and spectrum synthesis. Corrections for 3D and non-LTE effects often should be applied by the user. For example, it is known that the resonance line of Al is subject to strong deviations from LTE (e.g. Baumüller & Gehren 1997). While corrections for cases such as Al where only a single line is employed are relatively straight forward, we point out that for other elements one needs to consider the correction to the best fit to all spectral features used here.

3.5 Tests of the automated method

Before presenting the results for the sample, we present the results of some tests on our automated method. In particular, we compare our results where possible with the literature, and perform test calculations to assess the robustness of the automated method at low S/N.

3.5.1 Comparison stars

Five stars, namely HD 20, HD 221170, CS 22186-025, CS 22892-052 and CS 31082-001, which have been studied in detail with better quality observational material by others, were included in our pilot sample. Four of these were included in the sample for the specific purpose of use as comparison stars, while CS 22186-025 has been recently observed as part of the ESO First Stars programme (Cayrel et al. 2004). We now present a comparison of our results with some of the literature studies. For CS 22186-025, CS 22892-052, and CS 31082-001, we compare with the studies of Cayrel et al., Sneden et al. (2003), and Hill et al. (2002), respectively. For HD 20 and HD 221170 there are a number of different studies which have included these stars. For the purpose of clarity, for the abundances of these two stars we chose to concentrate our comparison on just one study, that of Burris et al. (2000), which includes both these stars and has reasonable overlap with our work in terms of the elements analysed.

First, in Table 3 we compare our stellar parameters for these stars with those used in the literature. Our temperatures are seen to be systematically warmer than those found in the literature for the comparison stars by of order 100 K. As mentioned in Sect. 2.1, and has been noted by other authors for individual stars (e.g. Hill et al. 2002, Sneden et al. 2003), the reddening maps of Schlegel et al. (1998) give larger reddenings than those of Burstein & Heiles (1982). As shown in Fig. 3 this leads to systematic differences in $T_{\rm eff}$ , of around 100 K. In Table 3 we also quote our temperatures using the lower reddenings of Burstein & Heiles. These temperatures agree well with the literature within error (of order $\pm 100$ K). The remaining parameters agree reasonably well, given the typical absolute error bars of $\sigma_{\log g} \sim 0.35$ dex, $\sigma_{\rm [Fe/H]}\sim 0.10$ dex, and $\sigma_\xi \sim 0.15$ km s^-1. Considering the effect of the systematic offset in $T_{\rm eff}$ we see, in line with expectations, that it usually leads to slightly higher $\log g$ values (+100 K $\rightarrow$ +0.2 dex), and slightly higher metallicities (+100 K $\rightarrow$ +0.1 dex).

To demonstrate the quality of the stellar parameter solutions, Fig. 8 plots abundances derived for individual Fe and Ti lines (the checking step of the procedure) against lower level excitation potential and wavelength of the line. Lines of the neutral and singly ionised species are distinguished in the plots, and thus it is clearly seen that the derived $\log g$ values satisfy ionisation equilibrium for both Fe and Ti. The plots against excitation potential, particularly for Fe, demonstrate that our spectra are not of sufficiently high quality to specify $T_{\rm eff}$ with the required precision as seen from the large scatter in the plot for CS 22186-025 which has $S/N\sim 32$ . The plots show our temperatures are reasonably consistent with excitation equilibrium (noting of course that one may question the validity of 1D LTE excitation equilibria); however, as discussed in Sect. 2.1 we find that on average excitation equilibria would give a cooler temperature scale. Finally, the plots against line wavelength indicate no significant systematic effects in the bluer lines due to blending or continuum placement. We also checked for significant trends with line strength and found none. Similar results were obtained for all stars in the sample.

Figure 9 compares abundances for our comparison stars with results from the literature. The results show generally reasonable agreement within error, thus supporting not only our method for obtaining abundances, but our error estimates as well. For CS 22892-052 and CS 31082-001 there is a systematic offset which is a result of our slightly warmer temperatures. This is clearly demonstrated by Fig. 10, where we compare results for CS 22892-052 and CS 31082-001 where we have reanalysed the spectra adopting the temperatures used in the relevant literature work. The remaining small differences are likely attributable to use of different lines and atomic data, particularly oscillator strengths and hyperfine structure.

The differences for HD 20 and HD 221170 are not improved by adopting temperatures used by Burris et al. (2000), which originate from Pilachowski et al. (1996). For HD 20, our temperature is already in reasonable agreement with that of Burris et al., yet we obtain systematically lower abundances by of the order of 0.3 dex. We reanalysed the spectrum adopting the stellar parameters of Burris et al., and the new comparison shown in Fig. 11 shows a significant improvement. Thus, the main reasons for the differences are our significantly higher microturbulence and lower gravity. We found no evidence of a significant trend of Fe abundance with line strength or ionisation stage to indicate our microturbulence or gravity solutions are in error. In spite of the fact that our stellar parameters for HD 221170 differ significantly from those adopted in Burris et al., the abundances are in reasonable agreement, probably due to compensation of the $T_{\rm eff}$ , $\log g$ and microturbulence differences. Note that this star has a large colour excess $E(B-V)\approx 0.12$ in our sample, and a large discrepancy with the Burstein & Heiles maps (see Fig. 3).

While these systematic offsets, of order 0.1-0.2 dex, are present and attributed to differences in stellar parameters, perhaps the most important result is the scatter in the difference, as this indicates the accuracy with which the abundance pattern in a given star is reproduced. We find for all comparisons scatter of 0.1 to 0.15 dex. Thus we conclude that the relative abundance patterns are accurate to of order 0.15 dex, within our quoted error bars.

3.5.2 Robustness at low S/N

Since most of our comparison stars are relatively bright, the spectra are usually of higher S/N than is typical for this project. The lowest quality comparison star spectrum is that of CS 22186-025, which has on average $S/N\approx 32$ per pixel. As some of our spectra are of even lower quality, it is important to ascertain what effect S/N has on our results. It should be pointed out that, provided our detection classification method and error estimates are reasonable, the pertinent issues are: (a) what is the minimum precision in abundances that is useful, and (b) what S/N is necessary to achieve it.

**Table 4:** Comparison of results for CS 31082-001 using spectra with degraded S/N. The difference from our results using the original spectrum $S/N\approx 90$ in Table 2 is quoted, with the relative error in the derived abundance for the degraded S/N in parentheses. A blank means a non-detection (below 3 $\sigma$ ) at this S/N for this star.
Parameter	$\Delta$ Parameter
	S/N = 30	20	15	10
$\log g$	+0.01 (0.26)	+0.05 (0.27)	-0.08 (0.26)	0.00 (0.34)
$\xi$	-0.04 (0.18)	-0.07 (0.18)	-0.08 (0.18)	-0.16 (0.20)
$\log\epsilon({\rm C})$	-0.02 (0.20)	-0.10 (0.20)	-0.07 (0.20)	-0.19 (0.22)
$\log\epsilon({\rm Mg})$	-0.04 (0.12)	-0.06 (0.12)	-0.02 (0.12)	-0.02 (0.13)
$\log\epsilon({\rm Al})$	-0.19 (0.19)	-0.14 (0.30)	--	--
$\log\epsilon({\rm Ca})$	-0.02 (0.12)	-0.04 (0.12)	-0.06 (0.11)	-0.06 (0.14)
$\log\epsilon({\rm Sc})$	-0.02 (0.17)	0.00 (0.18)	-0.09 (0.19)	--
$\log\epsilon({\rm Ti})$	-0.03 (0.16)	-0.02 (0.16)	-0.04 (0.16)	--
$\log\epsilon({\rm V})$	--	--	--	--
$\log\epsilon({\rm Cr})$	-0.06 (0.17)	-0.09 (0.19)	--	--
$\log\epsilon({\rm Mn})$	-0.07 (0.16)	-0.11 (0.18)	-0.03 (0.19)	--
$\log\epsilon({\rm Fe})$	-0.02 (0.13)	0.00 (0.12)	-0.02 (0.13)	0.00 (0.15)
$\log\epsilon({\rm Co})$	-0.05 (0.16)	--	--	--
$\log\epsilon({\rm Ni})$	-0.08 (0.20)	-0.09 (0.23)	-0.21 (0.25)	--
$\log\epsilon({\rm Zn})$	--	--	--	--
$\log\epsilon({\rm Sr})$	+0.01 (0.15)	+0.01 (0.17)	0.00 (0.19)	-0.07 (0.23)
$\log\epsilon({\rm Y})$	-0.04 (0.18)	-0.03 (0.19)	--	--
$\log\epsilon({\rm Zr})$	-0.04 (0.18)	--	--	--
$\log\epsilon({\rm Ba})$	-0.04 (0.15)	-0.03 (0.16)	+0.05 (0.16)	+0.01 (0.21)
$\log\epsilon({\rm La})$	-0.02 (0.18)	--	--	--
$\log\epsilon({\rm Ce})$	--	--	--	--
$\log\epsilon({\rm Nd})$	-0.02 (0.19)	--	--	--
$\log\epsilon({\rm Sm})$	--	--	--	--
$\log\epsilon({\rm Eu})$	-0.01 (0.18)	-0.01 (0.19)	-0.15 (0.19)	--

To investigate this we took the spectrum of CS 31082-001, which has $S/N\approx 90$ , and degraded it to lower S/N values by multiplying with appropriate Poisson noise and rescaling so that count numbers are consistent with the noise level. These spectra were then run through the entire automated spectrum analysis process completely independently from the original spectrum. The differences in derived atmosphere parameters (noting the model [Fe/H] is determined by the Fe abundance) and abundances for four degraded spectra compared to the original spectrum are given in Table 4, along with the relative error bar for that derived parameter. First, we note that almost every difference reported was less than our computed error bar for the degraded spectrum, giving confidence in our estimated errors. Secondly, the differences are generally reasonable for most elements, less than 0.1 dex. However, it is immediately obvious that for most elements there is a systematic trend towards slight underestimation of the abundances. We attribute this systematic trend to systematically lower continuum placement, which is to be expected, since at low S/N it is impossible to distinguish weak lines from continuum. Therefore, there should be a natural trend towards the continuum being placed too low, and thus underestimation of abundances, as the weak lines make the continuum appear slightly lower. This problem could perhaps be circumvented if one a priori defined continuum regions from higher quality spectra to be used for normalising the spectra; however such a procedure would be dependent on the similarity of the spectra. As noted, the error in the abundance at this S/N is much larger in any case.

Based on these results, we conclude that our method seems to be reasonably robust even at S/N as low as 15 for elements with a large number of lines, such as Fe and Ti. However, as one expects, detections for a number of elements cannot be made at such low S/N for stars of this metallicity. Elements with a small number of lines which are still detectable at low S/N at this metallicity, for example Mg, Ca and Ni, are less robust, but at S/N>15 the induced error usually does not appear to exceed of order 0.1 dex.

3.5.3 Example fits to spectra

Examples of portions of the spectra, and fits to the data obtained, are shown in Fig. 12 for an r-process enhanced star HE 1127-1143. The example was chosen to be representative of the sample; it is a giant star with $S/N\sim 49$ , typical for the sample.

4 Results

The derived stellar parameters and elemental abundances for the sample are presented in Table 2. Below, we note and discuss objects of particular interest found in the sample. In the next section we will discuss the more general behaviour of the abundances and implications for understanding the chemical evolution of the Galactic halo.

It is worth emphasising that some care must be taken in interpreting the results presented here involving elements which are not always, or even usually, detected in our spectra, which may lead to selection effects. Fourteen elements, C, Mg, Al, Ca, Sc, Ti, Cr, Mn, Fe, Co, Ni, Sr, Y and Ba, are almost always detectable at the 3 $\sigma$ level in the spectra. Another eight elements are analysed, V, Zn, Zr, La, Ce, Nd, Sm and Eu, which can usually only be detected in the spectra of the least metal-poor stars of our sample, spectra with higher than usual S/N, if the abundance is enhanced, or a combination of these factors. Thus, particular care must be taken in interpreting results involving these eight elements as the data are incomplete.

4.1 Objects of interest

The complete sample consists of 253 stars, of which four were comparison stars already known to be r-process enhanced metal-poor stars. Among the remainder we have identified a number of interesting objects, which we will now summarise. For the discussion in this subsection (Sect. 4.1) we consider only the 249 other stars as "the sample''. Though CS 22186-025 has been recently observed by Cayrel et al. (2004) it is included in our statistics as it had not been observed at the time of selection.

First, this work adds significantly to the number of confirmed very metal-poor stars. The [Fe/H] distribution for the sample is shown in Fig. 2. The sample contains 49 stars with ${\rm [Fe/H]}<-3$ , and 181 stars with $-3<{\rm [Fe/H]}<-2$ . Only 12 stars are currently known with ${\rm [Fe/H]}<-3.5$ (Beers & Christlieb 2005) and we find just one new star in this regime, HE 1300+0157 with ${\rm [Fe/H]}=-3.76\pm0.18$ . This star is at the base of the giant branch ( $T_{\rm eff}\sim 5400$ K, $\log g \sim 3.4$ ) and is carbon enhanced with ${\rm [C/Fe]} \sim 1.2$ .

The main goal of the HERES survey is to identify r-process enhanced stars, to address questions about the r-process. We were able to detect both Eu and Ba at the $3\sigma$ level in 62 stars in the sample. Of these, 57 are judged to be "pure'' r-process stars, as they have ${\rm [Ba/Eu]}<0$ , see Fig. 13. In Paper I we made the distinction between r-I and r-II stars, $0.3 \leq {\rm [Eu/Fe]} \leq 1.0$ and ${\rm [Eu/Fe]} > 1.0$ respectively (and ${\rm [Ba/Eu]}<0$ in both cases), on the basis that previous work had suggested a bimodal distribution of [Eu/Fe] with a lack of stars found in the range between 1.0 and 1.5. A histogram of detected [Eu/Fe], is plotted in Fig. 14; however, due to the significant incompleteness of the Eu abundances and the detection bias towards high [Eu/Fe], only the high [Eu/Fe] side of this distribution is reliable, and thus this plot gives little information about the cosmic distribution. We will return to the question of the distribution of r-process enhancement in Sect. 5.3. Following this classification system, of these 57 stars, eight are r-II stars ( ${\rm [Eu/Fe]} > 1.0$ ) which are listed in Table 5 (two of which were announced in Paper I), and 35 are r-I stars ( $0.3 \leq {\rm [Eu/Fe]} \leq 1.0$ ), while 14 do not have r-process enhancement ( ${\rm [Eu/Fe]} < 0.3$ ). This implies a frequency of around 3% and >14% for r-II and r-I stars respectively among metal-poor stars ( ${\rm [Fe/H]}<-1.5$ ). It must be borne in mind that these frequencies are dependent on detection in our spectra, and thus are certainly lower limits, particularly for r-I stars. For example, at the lowest metallicities, an r-I star would often not be detectable with our typical spectra.

The abundance patterns for the neutron-capture elements for the eight r-II stars are shown in Fig. 15, along with the scaled solar system r-process abundances, demonstrating that these elements follow this pattern in these stars. In fact, all 57 pure r-process stars, as judged from Ba/Eu, follow the pattern quite well for Ba and heavier elements. The lighter neutron-capture elements, Sr, Y and Zr, tend to deviate from the solar-r-process pattern in stars of lower r-process enrichment, which will be discussed in Sect. 5.4. The scaled solar system s- and r-process abundances used throughout this paper are based on the s-process fractions from the stellar model of Arlandini et al. (1999), the assumption that the remainder of neutron-capture elements are produced by the r-process, and meteoritic abundances from Grevesse & Sauval (1998). We chose the Arlandini et al. (1999) fractions over those of Burris et al. (2000) for our comparisons, since we found consistently better agreement with Y abundances in the pure r-process stars. The abundance patterns are otherwise very similar for the other neutron-capture elements considered here.

**Table 5:** New r-II and s-II objects. Quoted error estimates are relative errors. N3 is defined in the caption to Table 2.
Star	$T_{\rm eff}$	$\log g$	[Fe/H]	N3	[C/Fe]	N3	[Ba/Fe]	N3	[Eu/Fe]	N3	[Ba/Eu]
	[K]	[cm s^-2]
r-II stars
CS 29491-069	5103	2.45	$-2.81\pm 0.13$	46	$0.18 \pm 0.17$	1	$0.34 \pm 0.19$	1	$1.06\pm 0.15$	2	$-0.71\pm 0.17$
CS 29497-004	5013	2.23	$-2.81\pm 0.13$	42	$0.22 \pm 0.18$	1	$1.21 \pm 0.15$	1	$1.62\pm 0.15$	4	$-0.41\pm 0.17$
HE 0430-4901	5296	3.12	$-2.72\pm 0.12$	46	$0.09 \pm 0.18$	1	$0.50 \pm 0.20$	1	$1.16\pm 0.17$	3	$-0.65\pm 0.17$
HE 0432-0923	5131	2.64	$-3.19\pm 0.13$	41	$0.24 \pm 0.17$	1	$0.72 \pm 0.18$	1	$1.25\pm 0.15$	2	$-0.53\pm 0.16$
HE 1127-1143	5224	2.64	$-2.73\pm 0.14$	46	$0.54 \pm 0.17$	1	$0.63 \pm 0.19$	1	$1.08\pm 0.15$	3	$-0.45\pm 0.18$
HE 1219-0312	5140	2.40	$-2.81\pm 0.12$	44	$-0.08 \pm 0.19$	1	$0.51 \pm 0.25$	1	$1.41\pm 0.17$	3	$-0.91\pm 0.21$
HE 2224+0143	5198	2.66	$-2.58\pm 0.12$	54	$0.35 \pm 0.17$	1	$0.59 \pm 0.18$	1	$1.05\pm 0.15$	4	$-0.46\pm 0.16$
HE 2327-5642	5048	2.22	$-2.95\pm 0.12$	50	$0.43 \pm 0.19$	1	$0.66 \pm 0.19$	1	$1.22\pm 0.17$	4	$-0.56\pm 0.17$
s-II stars
HE 0131-3953	5928	3.83	$-2.71\pm 0.11$	22	$2.45 \pm 0.18$	1	$2.20 \pm 0.16$	2	$1.62\pm 0.19$	2	$0.58\pm 0.18$
HE 0338-3945	6162	4.09	$-2.41\pm 0.13$	23	$2.07 \pm 0.16$	1	$2.41 \pm 0.15$	2	$1.89\pm 0.16$	2	$0.51\pm 0.16$
HE 1105+0027	6132	3.45	$-2.42\pm 0.13$	34	$2.00 \pm 0.17$	1	$2.45 \pm 0.16$	2	$1.81\pm 0.16$	4	$0.64\pm 0.19$

The eight r-II stars are all giants with $T_{\rm eff}\sim 5100$ K, and have a quite narrow range in metallicity, $-3.2 \leq {\rm [Fe/H]} \leq -2.6$ . The r-II stars, including the two previously known examples CS 22892-052 and CS 31082-001, are centred on a metallicity of ${\rm [Fe/H]} = -2.81$ , with a very small scatter, on the order of 0.16 dex. Note, we find one r-II star with ${\rm [Fe/H]}<-3$ among 49 stars in our sample, a frequency of 2%, and 7 r-II stars among 118 stars in the range $-3<{\rm [Fe/H]}<-2.5$ , a frequency of 6%. This perhaps indicates that r-II stars are more rare at ${\rm [Fe/H]}<-3$ ; further study in a larger sample with better spectra would be desirable to resolve this question more definitively. All eight r-II stars have quite normal C/Fe abundances, the largest being ${\rm [C/Fe]} \sim 0.5$ , noting of course that the present sample is biased towards CH weak stars. The low C abundances mean that these stars are all candidates for studies of the actinide elements, particularly Th and U, in such stars. CS 22892-052 remains a unique object as the only r-II star known with ${\rm [C/Fe]}\sim 1$ .

The majority of the r-I stars are also giants, however, four such stars are unevolved (i.e. not yet on the giant branch $T_{\rm eff} > 5500$ K, $\log g > 3$ ), namely HE 0341-4024, HE 0534-4615, HE 0538-4515 and HE 2301-4024. As seen in Fig. 17 the r-I stars span the range $-3.4 \leq {\rm [Fe/H]} \leq -1.5$ , practically the entire metallicity range of our sample. We note that the four unevolved stars all have ${\rm [Fe/H]} \geq -2.1$ , but that there is a selection effect at work here; the Eu II lines observed will be weaker in unevolved stars than in evolved stars with the same abundances, and thus our survey preferentially detects Eu in giant stars. Our survey is also biased towards cool giants as described in Paper I.

Five stars in which both Eu and Ba were detected are found to be s-process rich as judged from their having ${\rm [Ba/Eu]}>0.5$ . All five are carbon-enhanced, and three are strongly Eu enhanced with ${\rm [Eu/Fe]} > 1.0$ . The three stars with ${\rm [Ba/Eu]}>0.5$ and ${\rm [Eu/Fe]} > 1.0$ , are listed in Table 5. A number of similar stars are known; e.g. Hill et al. (2000), Aoki et al. (2002b) and Cohen et al. (2003). We shall refer to these stars as "s-II'' stars, though we note that whether the neutron-capture elements in such stars are produced predominantly by the s-process or by both the s- and r-processes is a matter of current debate (e.g. Johnson & Bolte 2004). We note that these three stars all have large C enhancements ${\rm [C/Fe]}>1.5$ , and are unevolved. It must be borne in mind, however, that since this sample is limited to the stars with spectra only weakly polluted by CH features, we were only able to analyse the warmest strongly C enhanced stars. The complete HERES sample contains 72 CH strong stars which were not analysed here, among which there will be a large number of s-process rich stars. As we will discuss in the next section, a further such s-II star is suspected based on other abundances, but is not confirmed as Eu is detected at below the 3 $\sigma$ level.

The remaining two s-process rich stars with ${\rm [Ba/Eu]}>0.0$ yet more normal Eu enhancement ( ${\rm [Eu/Fe]}<0.6$ ) have abundance patterns of neutron-capture elements which are reasonably well matched by a scaled solar s-process abundance pattern. Figure 16 shows the abundance patterns for the three s-II stars. In these cases the Ba, La, Ce and Nd abundances can be well reproduced by a scaled solar-system s-process abundance pattern. The Sr and Y abundances, however, are much lower. We notice, however, that these abundances are consistent with the scaled solar system r-process abundance pattern normalised to Eu. On the other hand, the s-process is expected to be skewed towards heavier elements in metal-poor environments (e.g. Busso et al. 1999). A summary of suggested possible production scenarios for the s-process rich metal-poor stars has been recently given by Johnson & Bolte (2004). As stated by those authors, to distinguish different scenarios more strongly, measurements of as many heavy elements as possible are needed, and studies of these stars using better observational material will be the subject of future work as part of the HERES survey.

5 Discussion

5.1 Abundance trends and scatter with metallicity

We now discuss the general behaviour of the abundances, particularly trends and scatter in abundance ratios of interest. The abundance ratio trends of [X/Fe] with [Fe/H] and [X/Mg] with [Mg/H] have been plotted in Figs. 17 and 18 respectively for elements with a reasonable number of detections. The estimated $1\sigma$ scatter in the y-variable is shown, following the definition for the scatter used by Karlsson & Gustafsson (2005), such that at a given x-coordinate 32% of the stars lie outside the $1\sigma$ scatter lines, 16% above and below. In practice, this has been computed for a given x-coordinate by taking the n nearest stars in the x-variable, where n is the lesser of n=50 or $n_{\rm stars}/3$ , with $n_{\rm stars}$ being the number of stars in the diagram. The results are smoothed over the average width of bins containing n stars to remove transient behaviour caused by outliers. In Table 6 we compare the mean measured scatter in [X/Fe] and [X/Mg], across the range of [Fe/H] and [Mg/H] respectively, with the average error estimates. The minimum and maximum measured scatters are also reported to give an indication of the range of variation with [Fe/H] and [Mg/H].

**Table 6:** Comparison of measured scatter in Figs. 17 and 18 with relative errors in the abundance ratios. For each plot we report the minimum, mean and maximum measured $1\sigma$ scatter $\sigma _{\rm meas}$ across the range of [Fe/H] or [Mg/H], which is compared to the average relative error in the abundance ratio $\sigma ^{\rm rel}$ . The ratio of the mean measured scatter to the estimated error $\langle \sigma_{\rm meas} \rangle /\sigma^{\rm rel}$ is reported in the last column.
	min( $\sigma _{\rm meas}$ )	$\langle \sigma_{\rm meas} \rangle$	max( $\sigma _{\rm meas}$ )	$\sigma ^{\rm rel}$	$\langle \sigma_{\rm meas} \rangle /\sigma^{\rm rel}$
[C/Fe]	0.22	0.32	0.53	0.18	1.73
[Mg/Fe]	0.07	0.09	0.12	0.15	0.59
[Al/Fe]	0.17	0.20	0.21	0.17	1.13
[Ca/Fe]	0.08	0.09	0.10	0.15	0.59
[Sc/Fe]	0.09	0.11	0.13	0.16	0.69
[Ti/Fe]	0.08	0.09	0.12	0.15	0.61
[V/Fe]	0.06	0.09	0.11	0.15	0.60
[Cr/Fe]	0.10	0.12	0.14	0.16	0.72
[Mn/Fe]	0.13	0.16	0.21	0.16	1.03
[Co/Fe]	0.10	0.11	0.13	0.16	0.71
[Ni/Fe]	0.12	0.14	0.17	0.18	0.80
[Zn/Fe]	0.08	0.15	0.19	0.15	1.01
[Sr/Fe]	0.19	0.32	0.59	0.19	1.71
[Y/Fe]	0.21	0.25	0.32	0.17	1.47
[Zr/Fe]	0.13	0.19	0.23	0.16	1.18
[Ba/Fe]	0.37	0.50	0.69	0.18	2.77
[Eu/Fe]	0.21	0.37	0.62	0.16	2.34
[C/Mg]	0.24	0.35	0.51	0.18	1.89
[Al/Mg]	0.15	0.19	0.23	0.18	1.03
[Ca/Mg]	0.07	0.08	0.09	0.15	0.56
[Sc/Mg]	0.10	0.11	0.12	0.18	0.60
[Ti/Mg]	0.08	0.09	0.11	0.17	0.55
[V/Mg]	0.12	0.13	0.14	0.16	0.79
[Cr/Mg]	0.12	0.15	0.19	0.18	0.84
[Mn/Mg]	0.17	0.21	0.30	0.17	1.26
[Fe/Mg]	0.08	0.10	0.14	0.15	0.63
[Co/Mg]	0.11	0.13	0.16	0.17	0.79
[Ni/Mg]	0.15	0.17	0.19	0.19	0.88
[Zn/Mg]	0.09	0.18	0.26	0.15	1.16
[Sr/Mg]	0.18	0.29	0.55	0.21	1.41
[Y/Mg]	0.23	0.25	0.30	0.19	1.36
[Zr/Mg]	0.15	0.22	0.29	0.17	1.27
[Ba/Mg]	0.33	0.48	0.60	0.20	2.40
[Eu/Mg]	0.22	0.39	0.60	0.18	2.18

For Mg, Ca, Sc, Ti, Cr, Fe, Co, and Ni, the measured scatters are slightly less than the scatters expected from the typical estimated relative error in the abundance ratios, suggesting that our computed errors overestimate the real relative error. Bearing in mind the difficulties in accurately calculating the errors, this suggests that the cosmic scatter is small (or even non-existent) at these metallicities. These results are in line with previous results for smaller samples with smaller uncertainties for some of these elements, such as the studies by Arnone et al. (2005), Cayrel et al. (2004) and Cohen et al. (2004). It should be noted that in all these elements, apparent outliers may perhaps be explained simply by the errors in the analysis; in a sample of 253 stars outliers due to random errors are expected. In particular, examining the outliers we noted that they often showed trends in the abundances derived from individual Fe I lines with excitation that were at the edge of the distribution of such slopes for the entire sample (see Fig. 4), and occur in elements where particularly temperature sensitive spectral features have been employed, such as Co and Ni. Thus, we believe that more often than not for these elements, the outliers are more likely due to errors in the analysis, such as $T_{\rm eff}$ being in error, than indicative of any real over- or under-abundance of the element in question.

The results for Al, V, Mn and Zn are less clear. In the case of Al, the scatters are marginally larger than the typical error bars; however, we note the Al abundances are based on a single line and are very sensitive to the S/N of the spectrum (see Table 4). Further, this line is known to be subject to deviations from LTE. Both these facts may lead to increased scatter in the derived abundances. In the cases of V and Zn, the number of detections is small and the abundances for these elements are based on quite weak features and are therefore susceptible to overestimation due to unresolved blends. For Mn, the scatter at low metallicity does marginally exceed the error estimates, with the hint of a "bump'' of Mn enhanced stars at around ${\rm [Fe/H]}\sim -3$ . A similar feature is suggested by the results of Cayrel et al. (2004).

The elements C, Sr, Y, Ba and Eu, and perhaps Zr, show scatter at low metallicities, ${\rm [Fe/H]} \la -2.5$ and ${\rm [Mg/H]} \la -2.2$ , significantly larger than can be explained from the errors in the analysis, implying the scatter is cosmic in origin. At higher metallicities the scatter among the non-C-rich stars, does not greatly exceed that expected from the errors in the analysis, but perhaps indicates some cosmic scatter. Note, the scatter in [Ba/Fe] and [Ba/Mg], and to a lesser degree Sr and Y, at higher [Fe/H] and [Mg/H] is affected by C-enhanced stars which have high Ba/Fe and Ba/Mg ratios, see Fig. 28. The scatter at low metallicity seems, in most cases, to be increasing monotonically with decreasing metallicity. Similar results have been found, for example, by McWilliam et al. (1995b), McWilliam (1998), Norris et al. (2001), and Burris et al. (2000). The results of Norris et al. (2001) suggested the existence of a larger scatter in [Sr/Fe] than for [Ba/Fe] at the lowest [Fe/H]. We do not find this result; the scatters are of comparable magnitude. Note that in contrast to the results for lighter elements discussed above, the cases of under-abundances and over-abundances of these elements with respect to the general trends are sometimes significant.

In summary, among the stars without strong C enhancement, at about ${\rm [Fe/H]} \ga -2.5$ or equivalently ${\rm [Mg/H]} \ga -2.2$ , our analysis indicates that the cosmic scatter in all abundance ratios is small. This implies that at around this level of enrichment the Galactic halo was reasonably well mixed. At lower metallicities C, Sr, Y, Ba and Eu all show evidence for real cosmic scatter, while the results for the remaining elements still admit only a small amount of cosmic scatter within the errors of our analysis. This dichotomy implies that while the lack of scatter in these elements at ${\rm [Fe/H]} \ga -2.5$ might be explained by a well mixed Galactic halo, the small scatter at ${\rm [Fe/H]} \la -2.5$ has a different explanation. One possibilty is suggested by the stochastic models of metal-poor enrichment by Karlsson & Gustafsson (2005). The small scatter among the most metal-poor stars may be tentatively explained by cosmic selection effects in contributing supernova masses, and a relatively narrow range of masses of gas the newly synthesised elements mix with (so called mixing masses). Alternatively, as suggested by Arnone et al. (2005), the scatter in C, Sr, Y, Ba and Eu at these metallicities might be explained by the addition of sources of these elements which produce negligible amounts of the other elements such as Mg and Fe, such as low mass supernovae of type II.

5.2 Carbon

The work of Bromm & Loeb (2003) suggests that halo stars with low C abundances, ${\rm [C/H]}\sim-3.5$ according to their model, and low oxygen abundances, are probably true second generation stars. In Fig. 19 we plot the [C/H] values for our sample, identifying evolved (on the giant branch or red horizontal branch) and unevolved stars (all others). Though we do not have oxygen abundances, we see the majority of stars lie above the -3.5 level. It would be interesting to obtain O abundances for the stars lying near or below ${\rm [C/H]}\sim-3.5$ to identify likely second generation stars among this sample.

5.3 Heavy neutron-capture elements, Ba-Eu

Figure 13, which we used earlier as a measure of r- vs. s-process enrichment, plots [Ba/Eu] against Fe and C abundances. The plots show a clear separation between two groupsin the halo, a separation which correlates with C enrichment. This distinction was first seen in McWilliam (1998), though with fewer stars. The scatter among the pure r-process stars is consistent with the observational uncertainties and we thus conclude that the cosmic scatter in Ba/Eu among pure r-process halo stars is small. This implies that the Ba/Eu abundances produced by the r-process in the early Galaxy are universal. Taking the weighted mean (weights are based on absolute errors), we find for the pure r-process stars analysed in this work $\langle {\rm [Ba/Eu]} \rangle = -0.58 \pm 0.03$ , where the quoted error is the weighted standard deviation. The solar system r-process abundance ratio, based on the data from Arlandini et al. (1999), is -0.65. Our result seems to be in disagreement with that found at low metallicities by Truran et al. (2002), who compiled data from a number of studies, and found a large scatter in Ba/Eu. They noted the difficulties in analysing Ba in metal-poor spectra due to dependence on hyperfine and isotopic structure and microturbulence. This is particularly problematic when combining data from different studies. Our data on the other hand are homogeneously analysed, but the Eu abundances are incomplete and biased towards stars with strong r-process enhancement.

It has been suggested (e.g. Burris et al. 2000; Truran et al. 2002; Simmerer et al. 2004) that La may be a better alternative as a tracer of the s-process enrichment. Unfortunately, as the lines available to us are typically weak, La is often undetected in our low S/N spectra according to our detection criteria. When plotting [La/Eu] vs. [Fe/H], Fig. 20, we see no trend or significant scatter. Among the pure r-process stars $\langle {\rm [La/Eu]} \rangle = -0.40 \pm 0.05$ . The solar system r-process abundance ratio is -0.38.

As mentioned in Sect. 4.1, the distribution of r-process enhancement in the early Galaxy is of great interest. This is usually traced by [Eu/Fe], but our data are incomplete due to the inability to reliably detect low Eu abundances in our snapshot spectra. One may, however, try to reconstruct the r-process enhancement by instead using the Ba abundances, which are practically complete due to the ease of detecting the Ba II resonance line at 4554 Å. Following Raiteri et al. (1999) and Burris et al. (2000), where possible we attempt to reconstruct the r-process-only contribution to Ba. We define the ratio ${\rm [Ba/Fe]}_{r-{\rm process}} = \log ( N_{{\rm Ba},r} / N_{\rm Fe} )_\star - \log (N_{{\rm Ba},r} / N_{\rm Fe})_{\rm\odot}$ , where $N_{{\rm Ba},r}$ indicates the r-process-only Ba abundance. Note, the zero point of the scale is set at the solar r-process-only Ba abundance, not the total solar Ba abundance. For the pure r-process stars, ${\rm [Ba/Fe]}_{r-{\rm process}} = {\rm [Eu/Fe]}$ , since the Ba/Eu r-process ratio is fixed at the solar r-process-only ratio and Eu is produced practically entirely by the r-process. Previous studies indicate that the main s-process does not become important until ${\rm [Fe/H]} \ga -2.5$ , e.g. Burris et al. and Truran et al. (2002). Thus we assume that at lower metallicities all Ba in non-C-rich stars is produced by the r-process. That is, for stars with ${\rm [C/Fe]}<0.3$ and ${\rm [Fe/H]}<-2.5$ , ${\rm [Ba/Fe]}_{r-\rm process} = {\rm [Ba/Fe]} + 0.721$ . Those stars that are not pure r-process stars with higher C enrichment and higher metallicity are disregarded.

The results for ${\rm [Ba/Fe]}_{r-{\rm process}}$ are plotted against [Fe/H] in Fig. 21. Note, since we can only estimate ${\rm [Ba/Fe]}_{r\rm -process}$ in stars with ${\rm [Fe/H]} > -2.5$ if Eu is detected, there is an observational bias here; we will miss stars with low r-process enhancements at ${\rm [Fe/H]} > -2.5$ . The results of Burris et al., which cover this metallicity regime and are much more complete, indicate the scatter in the region $-2.5 <{\rm [Fe/H]}<-1.5$ is larger than seen in our results. They find stars in this regime with ${\rm [Eu/Fe]}$ ranging from as low as $\sim$ -0.4 (significantly lower than in our data) to as high as $\sim$ 0.8 (similar to our data). In any case, even accounting for the fact that this bias leads to an underestimation of the scatter at ${\rm [Fe/H]} > -2.5$ , the scatter at ${\rm [Fe/H]}<-2.5$ in our data is significantly larger than seen at higher metallicity in the results of Burris et al. If we consider only the upper envelope of the abundance distribution, which should be well defined by our sample, there is an rapid transition from a maximum value of [Eu/Fe] of $\sim$ 1.0 to $\sim$ 1.7 at ${\rm [Fe/H]} \sim -2.5$ . Thus, Fig. 21 and the occurrence of r-II stars only at ${\rm [Fe/H]}<-2.5$ , suggests the r-II stars are extreme cases of a wide range of r-process enrichment in the early, chemically inhomogeneous Galaxy. Note, the cutoff of ${\rm [Eu/Fe]}=1.0$ between r-I and r-II is suggested by the maximum enrichment levels at higher metallicity.

5.4 Light neutron-capture elements, Sr, Y and Zr

The production of light neutron-capture elements (particularly Sr, Y, Zr) versus heavy neutron-capture elements (such as Ba, Eu), has become a topic of interest due to evidence of production of the former without significant production of the latter, e.g. McWilliam (1998), Burris et al. (2000), Truran et al. (2002), Travaglio et al. (2004) and Aoki et al. (2005). Figures 22 and 23 plot [Sr/Ba] and [Sr/Eu] against Fe and C abundances. Significant scatter is seen in Sr/Ba at low metallicity, as found by McWilliam and Burris et al. In both cases, Sr/Ba and Sr/Eu, even among the pure r-process stars, a significant amount of scatter is seen at ${\rm [Fe/H]}<-2.5$ . For Sr/Ba, the scatter appears to increase quite uniformly with decreasing [Fe/H], the data showing quite clear upper and lower boundaries, apart from a small number of outliers which are usually C enhanced. Sr/Eu shows similar tendencies when the s-process rich stars are disregarded, though not as clearly due to the smaller number of stars. The r-II stars all have similar Sr/Ba and Sr/Eu ratios, which are always among lowest of the non-C-enhanced stars. For Sr/Ba the weighted mean of the results for r-II stars, is $\langle {\rm [Sr/Ba]} \rangle_{\rm r-II} = -0.44 \pm 0.08$ , and for Sr/Eu $\langle {\rm [Sr/Eu]} \rangle_{\rm r-II} = -0.98 \pm 0.09$ . The solar system r-process values are -0.24 and -0.89 respectively.

Truran et al. (2002) examined the variation of Sr/Ba with r-process enrichment, as traced by Ba/Fe and Eu/Fe. Figure 24 shows Sr/Ba with Ba/Fe, and Fig. 25 shows Sr/Eu with Eu/Fe. We find similar results; however, with our large and homogeneously analysed sample the scatter is well defined, and we see a trend for decreasing scatter in Sr/Ba and Sr/Eu with increasing r-process enrichment.

Similar plots are shown for Y/Ba in Figs. 26 and 27. The results are similar to those for Sr/Ba, in particular, increasing scatter in Y/Ba with decreasing metallicity and decreasing heavy r-process enrichment, and similar Y/Ba among the r-II stars. For the r-II stars we find $\langle {\rm [Y/Ba]} \rangle_{\rm r-II} = -0.47 \pm 0.08$ ; the solar system r-process value is ${\rm [Y/Ba]} = -0.48$ .

Figures 22, 24, 26 and 27 identify two stars of interest, two metal-poor stars with ${\rm [Sr,Y/Ba]} \la -1$ which are not carbon-rich or overly Ba-rich, which are HE 0305-4520 ( ${\rm [C/Fe]}\sim +0.3$ , ${\rm [Sr/Fe]}\sim -0.7$ , ${\rm [Y/Fe]}\sim -0.4$ , ${\rm [Ba/Fe]}\sim +0.6$ ) and HE 2156-3130 ( ${\rm [C/Fe]}\sim +0.7$ , ${\rm [Sr/Fe]}\sim -0.9$ , ${\rm [Y/Fe]}\sim -0.9$ , ${\rm [Ba/Fe]}\sim +0.5$ ), the latter being the more metal-poor of the two. These stars perhaps warrant further study.

We note that Figs. 22 and 24 show 6 stars with similar Sr/Ba ratios and similar C/H and Fe/H to the stars identified as s-process-rich stars. These stars also stand out clearly in a plot of [Ba/Fe] vs. [C/Fe], see Fig. 28, occupying a similar region of the plot as the s-process-rich stars. As Eu has not been detected at the 3 sigma level according to our criteria they have not been classified in terms of the likely neutron-capture processes that have contributed to the heavy elements. It is interesting to look at these stars in more detail. We find that all these stars appear to be s-process-rich stars based on Eu abundances obtained, though we emphasise the abundances are not 3 sigma detections and thus not completely reliable. HE 1430-1123, the star with the lowest [Sr/Ba] of the six, and thus more closely associated with the s-II stars in Fig. 22, appears also to be a s-II star as we determine ${\rm [Eu/Fe]}\sim 1.4$ . The other five stars, HE 0231-4016, HE 0430-4404, HE 2150-0825, HE 2227-4044, and HE 2240-0412, which seem more closely associated with the remaining mildly Eu enhanced s-process-rich stars in Fig. 22, appear to be similar stars with ${\rm [Eu/Fe]}\sim 0.7\leftrightarrow 1.0$ .

Figure 28 also identifies a number of mildly carbon-enhanced stars without enhancement of neutron-capture elements, a class of objects identified by Aoki et al. (2002a). The five objects with ${\rm [C/Fe]}>0.8$ and ${\rm [Ba/Fe]}<0.2$ are, from largest [C/Fe] to smallest, HE 1351-1049, HE 1300-0641, HE 1330-0354, HE 1300-2201, and HE 1124-2335.

6 Conclusions

We have analysed snapshot spectra of a sample of 253 metal-poor stars, deriving abundances for 22 elements, where detectable, using an automated technique based on SME by Valenti & Piskunov (1996). The technique has been shown to give results in agreement with previous work within errors, when one considers differences in temperature scale. For our particular case (namely resolving power, spectral coverage and line list) the technique has been shown to be quite robust (at around the 0.1 dex level) even for S/N as low as 15. Our error estimates and comparisons with studies in the literature show the derived elemental abundances to be of moderate precision, relative and absolute errors of order 0.15 and 0.25 dex respectively. This work has dealt with the CH weak content of the sample. The CH strong content will also be examined as part of the HERES programme. It would be interesting to obtain additional spectra for (the most interesting of) these stars, particularly covering the Eu II lines at 6437 and 6645 Å.

Our main goal here has been to identify stars of interest, particularly those enhanced in r-process elements. We identified 8 new r-II stars, 35 r-I stars and 3 s-process rich stars with strong Eu enhancement. Notably, the r-II stars were found only in a rather narrow metallicity range, $-3.2\la{\rm [Fe/H]}\la-2.6$ . These interesting stars should be investigated in more detail, and such work is underway as part of the HERES project large programme. The spectra obtained will be of much higher quality, in terms of S/N, resolving power, and spectral coverage. The higher quality data, together with a careful manual spectrum analysis, will naturally permit abundances and stellar parameters to be obtained with higher precision and abundances for additional elements to be obtained. It will also be possible to obtain isotopic ratios for some elements. Ideally, such analyses should be performed with reference to deviations from the assumptions of LTE and 1D model atmospheres.

The results presented here provide a database of confirmed metal-poor stars, including a number of new r-process and s-process rich stars, which may be used for selection of stars for further studies. The results also provide a homogeneous database of moderate precision abundances for comparison with Galactic chemical evolution models. We stress that such comparisons must consider the limitations of our data set, most importantly the selection effects arising from the significant incompleteness of the data for some elements, but also the precision of the abundances and the assumptions of the modelling such as LTE and the use of 1D model atmospheres.

We investigated trends and scatter in some measured abundance ratios of interest. Among the stars without strong C enhancement, at about ${\rm [Fe/H]} \ga -2.5$ we find that the cosmic scatter in any abundance ratio is small (perhaps even non-existent), implying that at around this level of enrichment the Galactic halo was reasonably well mixed. At lower metallicities C, Sr, Y, Ba and Eu, and perhaps Zr, show evidence for cosmic scatter, while the results for the Mg, Ca, Sc, Ti, Cr, Fe, Co and Ni still indicate at most small cosmic scatter within the errors of our analysis. Due to the difficulties in accurately estimating errors, and thus disentangling the observational and modelling uncertainties from the real cosmic scatter, we conclude that to determine the magnitude of the scatter in the cases where it is small will require high precision studies of a large number of stars.

References

7 Online Material

Appendix A: Line list

The lines and spectral windows used are listed in Tables A.1-A.5. The most important atomic and molecular data, wavelength $\lambda$ , excitation potential $\chi$ , and $\log gf$ , are tabulated. Line broadening data used may be obtained from the authors on request. Below we briefly comment on line selection issues and data sources for each element.

First, it is worth commenting on Si which is notably omitted from our analysis. Our spectra include two Si lines, at 3905 and 4102 Å. The $\lambda$ 4102 line lies in the wing of H $\delta$ and thus presents a considerable challenge for automated analysis. The $\lambda$ 3905 line is known to be blended by CH lines (e.g. Cayrel et al. 2004). Even with known CH lines from the lists of Plez & Jorrisen (see below) included in the synthesis, our Si abundances were found to differ from the literature values (see Sect. 3.5.2), which are usually based on the $\lambda$ 4102 line, and the difference was seen to correlate with carbon-enhancement. We have reasonable agreement with the literature for CS 22186-025 which has $\rm [C/Fe]\sim-0.7$ , while we have mild disagreement for CS 31082-001 which has $\rm [C/Fe]\sim 0.2$ and strong disagreement for CS 22892-052 which has ${\rm [C/Fe]}\sim 1$ . This suggests that the $\lambda$ 3905 line may be affected by further blends of features involving C, and thus we chose to omit Si from our analysis.

**Table A.1:** Molecular line data for A-X system of the CH molecule near 4310 Å from Plez & Jorissen. The spectral windows employed for this molecular band are defined with respect to an arbitrary $\lambda$ and span from $\lambda +d\lambda _{\rm blue}$ to $\lambda +d\lambda _{\rm red}$ .
Species	$\lambda$	$\chi$	$\log gf$	d $\lambda_{\rm blue}$	d $\lambda_{\rm red}$
	[Å]	[eV]		[mÅ]	[mÅ]
CH	4310.150			-100	2300
CH	4310.038	0.096	-3.183
CH	4310.090	0.096	-1.412
CH	4310.110	0.096	-1.474
CH	4310.149	0.431	-3.202
CH	4310.162	0.096	-3.025
CH	4310.203	0.431	-1.443
CH	4310.220	0.431	-1.505
CH	4310.272	0.431	-3.039
CH	4310.404	0.096	-3.183
CH	4310.430	0.408	-1.581
CH	4310.458	0.096	-1.412
CH	4310.504	0.432	-3.202
CH	4310.508	0.408	-2.966
CH	4310.556	0.432	-1.443
CH	4310.679	0.072	-1.550
CH	4310.729	0.408	-1.581
CH	4310.757	0.072	-2.952
CH	4310.807	0.408	-2.966
CH	4310.811	0.408	-3.155
CH	4310.889	0.408	-1.508
CH	4310.937	0.388	-1.677
CH	4310.969	1.107	-2.269
CH	4310.991	0.072	-1.550
CH	4311.045	0.388	-2.879
CH	4311.069	0.072	-2.952
CH	4311.075	0.408	-3.155
CH	4311.075	0.072	-3.136
CH	4311.084	0.987	-4.123
CH	4311.145	0.987	-4.123
CH	4311.153	0.408	-1.508
CH	4311.153	0.388	-1.677
CH	4311.153	0.072	-1.477
CH	4311.196	1.108	-3.922
CH	4311.196	1.108	-2.229
CH	4311.261	0.388	-2.879
CH	4311.328	0.371	-1.805
CH	4311.348	0.072	-3.136
CH	4311.394	0.388	-3.105
CH	4311.426	0.072	-1.477
CH	4311.473	0.371	-1.805
CH	4311.476	0.371	-2.771
CH	4311.502	0.388	-1.587
CH	4311.502	0.051	-1.646
CH	4311.545	1.108	-2.269
CH	4311.547	0.347	-2.386
CH	4311.567	0.357	-2.002
CH	4311.580	0.388	-3.105
CH	4311.592	0.347	-2.386
CH	4311.612	0.051	-2.865
CH	4311.618	0.662	-2.054
CH	4311.618	0.662	-2.054
CH	4311.621	0.371	-2.771
CH	4311.655	0.357	-2.002
CH	4311.688	0.388	-1.587
CH	4311.722	1.108	-3.923
CH	4311.727	0.051	-1.646
CH	4311.729	1.108	-2.229
CH	4311.776	0.357	-2.632
CH	4311.837	0.051	-2.866
CH	4311.861	0.347	-2.432
CH	4311.863	0.357	-2.632
CH	4311.897	0.371	-3.052
CH	4311.906	0.347	-2.432
CH	4311.978	0.051	-3.085
CH	4312.017	0.371	-3.052
CH	4312.045	0.371	-1.688
CH	4312.088	0.051	-1.557
CH	4312.153	0.033	-1.773
CH	4312.164	0.371	-1.688
CH	4312.172	0.051	-3.085
CH	4312.280	0.051	-1.557
CH	4312.304	0.033	-1.773
CH	4312.304	0.033	-2.759
CH	4312.317	0.358	-3.007
CH	4312.386	0.358	-3.007
CH	4312.456	0.033	-2.759
CH	4312.527	0.358	-1.831
CH	4312.594	0.358	-1.831
CH	4312.594	0.019	-1.969
CH	4313.620			-200	200
CH	4313.377	0.020	-2.985
CH	4313.446	0.020	-2.985
CH	4313.590	0.020	-1.800
CH	4313.660	0.020	-1.800
CH	4313.876	0.009	-3.033
CH	4313.906	0.009	-3.033

**Table A.2:** Molecular line data for A-X system of the CH molecule near 4363 Å from Plez & Jorissen. The spectral window employed for this molecular band is defined with respect to two arbitrary wavelengths $\lambda$ and span from $\lambda +d\lambda _{\rm blue}$ to $\lambda +d\lambda _{\rm red}$ .
Species	$\lambda$	$\chi$	$\log gf$	d $\lambda_{\rm blue}$	d $\lambda_{\rm red}$
	[Å]	[eV]		[mÅ]	[mÅ]
CH	4363.300			-1000	3700
CH	4362.021	1.247	-4.054
CH	4362.061	1.247	-1.976
CH	4362.172	1.247	-1.943
CH	4362.202	0.777	-1.982
CH	4362.204	1.247	-4.149
CH	4362.255	0.777	-3.284
CH	4362.531	0.777	-1.917
CH	4362.549	0.557	-1.749
CH	4362.551	0.557	-3.392
CH	4362.697	0.777	-1.982
CH	4362.749	0.557	-1.705
CH	4362.750	0.777	-3.285
CH	4362.985	0.777	-1.917
CH	4363.086	0.227	-3.380
CH	4363.087	0.227	-1.716
CH	4363.162	1.248	-4.055
CH	4363.186	1.248	-1.976
CH	4363.242	1.248	-1.943
CH	4363.276	1.248	-4.149
CH	4363.291	0.227	-1.673
CH	4363.461	0.558	-1.749
CH	4363.463	0.558	-3.392
CH	4363.605	0.558	-1.705
CH	4364.034	0.228	-3.380
CH	4364.036	0.228	-1.716
CH	4364.114	1.289	-4.093
CH	4364.167	1.289	-1.947
CH	4364.181	0.228	-1.673
CH	4364.253	1.289	-1.916
CH	4364.295	1.289	-4.181
CH	4365.416	1.290	-4.093
CH	4365.450	1.290	-1.947
CH	4365.477	1.290	-1.916
CH	4365.522	1.290	-4.181
CH	4365.929	0.987	-3.729
CH	4366.010	0.987	-3.729
CH	4366.230	0.987	-3.828
CH	4366.312	0.987	-3.828
CH	4366.398	0.597	-3.426
CH	4366.407	0.597	-1.699
CH	4366.482	0.268	-3.414
CH	4366.497	0.268	-1.666
CH	4366.520	1.333	-4.129
CH	4366.573	0.597	-1.659
CH	4366.588	1.333	-1.920
CH	4366.647	1.333	-1.892
CH	4366.663	0.268	-1.627
CH	4366.699	1.333	-4.211
CH	4366.897	0.805	-1.903
CH	4366.928	0.987	-3.495
CH	4366.930	0.805	-3.326
CH	4366.991	0.987	-3.495
CH	4367.172	0.805	-1.848

**Table A.3:** Data for atomic lines for species lighter than Fe. The spectral window employed for the line is from $\lambda +{\rm d}\lambda _{\rm blue}$ to $\lambda +{\rm d}\lambda _{\rm red}$ . Lines which are removed in carbon-enhanced stars are marked with asterisks in the wavelength column.
Species	$\lambda$	$\chi$	$\log gf$	d $\lambda_{\rm blue}$	d $\lambda_{\rm red}$	Refs.
	[Å]	[eV]		[mÅ]	[mÅ]
Mg I	3829.355	2.707	-0.208	-150	100	WSM69
Mg I	3832.304	2.710	0.270	-300	200	WSM69
Mg I	3838.292	2.715	0.490	-230	150	WSM69
Mg I	*4057.505	4.346	-0.890	-120	100	FF75
Mg I	*4167.271	4.346	-0.710	-250	200	FF75
Mg I	4571.096	0.000	-5.393	-300	300	WSM69
Mg I	4702.990	4.330	-0.380	-300	300	FF75
Al I	3961.529	0.014	-0.336	-200	170	WM80
Ca I	4226.728	0.000	0.244	-150	400	WM80
Ca I	*4283.011	1.886	-0.224	-120	300	WM80
Ca I	*4289.367	1.879	-0.304	-120	170	WM80
Ca I	4318.652	1.890	-0.207	-120	120	WM80
Ca I	*4425.437	1.879	-0.358	-300	300	WM80
Ca I	*4434.957	1.886	-0.005	-300	50	WM80
Ca I	4454.780	1.898	0.258	-50	200	WM80
Ca I	4455.887	1.899	-0.526	-300	300	WM80
Ca I	4578.551	2.521	-0.558	-200	100	WM80
Sc II	4246.837	0.315	0.240	-350	250	LD89
Sc II	*4314.095	0.618	-0.100	-250	70	LD89
Sc II	*4400.399	0.605	-0.540	-150	200	LD89
Sc II	4415.563	0.595	-0.670	-180	300	LD89
Sc II	4670.417	1.357	-0.580	-150	50	LD89
Ti I	3989.759	0.021	-0.140	-200	100	GBP89, BPSL82
Ti I	3998.636	0.048	0.000	-250	150	GBP89, BPSL82
Ti I	4533.249	0.848	0.530	-150	300	GBP89, BMPS82
Ti I	4534.776	0.836	0.340	-300	300	GBP89, BMPS82
Ti I	4656.469	0.000	-1.290	-300	300	GBP89, BPSL82
Ti I	*4681.909	0.048	-1.020	-300	150	GBP89, BPSL82
Ti II	*4337.915	1.080	-0.960	-150	150	PTP01
Ti II	*4394.051	1.221	-1.780	-100	300	PTP01
Ti II	*4395.850	1.243	-1.930	-200	100	PTP01
Ti II	*4417.719	1.165	-1.190	-200	300	PTP01
Ti II	4443.794	1.080	-0.720	-300	250	PTP01
Ti II	4468.507	1.131	-0.600	-150	300	RHLPS94
Ti II	*4470.857	1.165	-2.020	-250	150	PTP01
Ti II	4501.273	1.116	-0.770	-300	300	PTP01
Ti II	4563.761	1.221	-0.690	-300	300	PTP01
Ti II	4571.968	1.572	-0.320	-300	150	PTP01
Ti II	4589.958	1.237	-1.620	-300	300	RHLPS94
V I	*4379.230	0.301	0.550	-150	150	DKKWZ85
V I	*4389.976	0.275	0.270	-150	150	DKKWZ85
V II	*3951.960	1.480	-0.784	-150	60	BGFML89
Cr I	4254.332	0.000	-0.114	-150	200	see MFW88
Cr I	*4274.796	0.000	-0.231	-200	100	see MFW88
Cr I	*4289.716	0.000	-0.361	-150	100	see MFW88
Mn I	4030.763	0.000	-0.470	-150	250	BBPS84
Mn I	4033.060	0.000	-0.618	-200	150	BBPS84
Mn I	*4034.492	0.000	-0.811	-150	300	BBPS84
Mn I	4754.040	2.282	-0.086	-200	200	BBPS84
Mn I	4823.496	2.319	0.144	-100	200	BBPS84

**Table A.4:** Data for atomic lines of Fe. The spectral window employed for the line is from $\lambda +{\rm d}\lambda _{\rm blue}$ to $\lambda +{\rm d}\lambda _{\rm red}$ . Lines which are removed in carbon-enhanced stars are marked with asterisks in the wavelength column.
Species	$\lambda$	$\chi$	$\log gf$	d $\lambda_{\rm blue}$	d $\lambda_{\rm red}$	Refs.
	[Å]	[eV]		[mÅ]	[mÅ]
Fe I	*3856.372	0.052	-1.286	-200	400	OWLWB91
Fe I	*3859.911	0.000	-0.710	-400	350	OWLWB91
Fe I	3865.523	1.011	-0.950	-250	250	OWLWB91
Fe I	*3878.018	0.958	-0.896	-300	100	OWLWB91
Fe I	4005.242	1.557	-0.583	-150	150	OWLWB91
Fe I	4045.812	1.485	0.284	-100	150	OWLWB91
Fe I	4063.594	1.558	0.062	-100	300	OWLWB91
Fe I	4071.738	1.608	-0.008	-100	300	OWLWB91
Fe I	4114.445	2.831	-1.303	-250	250	OWLWB91
Fe I	4132.058	1.608	-0.675	-300	100	OWLWB91
Fe I	4143.868	1.557	-0.511	-200	300	OWLWB91
Fe I	*4175.636	2.845	-0.827	-150	300	OWLWB91
Fe I	*4187.039	2.449	-0.514	-150	200	OWLWB91
Fe I	*4199.095	3.047	0.156	-200	300	OWLWB91
Fe I	4202.029	1.485	-0.689	-200	150	OWLWB91
Fe I	4222.213	2.449	-0.914	-300	200	OWLWB91
Fe I	4227.426	3.332	0.266	-150	150	OWLWB91
Fe I	*4233.603	2.482	-0.579	-150	100	OWLWB91
Fe I	*4250.120	2.469	-0.380	-100	300	OWLWB91
Fe I	4250.787	1.557	-0.713	-300	300	OWLWB91
Fe I	4260.474	2.400	0.077	-150	200	OWLWB91
Fe I	*4271.154	2.449	-0.337	-300	100	OWLWB91
Fe I	*4271.761	1.485	-0.173	-150	300	OWLWB91
Fe I	4282.403	2.176	-0.779	-250	150	OWLWB91
Fe I	*4325.762	1.608	0.006	-250	100	OWLWB91
Fe I	*4375.930	0.000	-3.031	-150	300	OWLWB91
Fe I	*4383.545	1.485	0.208	-300	300	OWLWB91
Fe I	*4404.750	1.557	-0.147	-250	200	OWLWB91
Fe I	*4415.123	1.608	-0.621	-300	200	OWLWB91
Fe I	*4430.614	2.223	-1.728	-250	250	OWLWB91
Fe I	*4442.339	2.198	-1.228	-300	300	OWLWB91
Fe I	4443.194	2.858	-1.043	-100	250	OWLWB91
Fe I	4447.717	2.223	-1.339	-300	300	OWLWB91
Fe I	4489.739	0.121	-3.899	-300	200	OWLWB91
Fe I	4494.563	2.198	-1.143	-300	300	OWLWB91
Fe I	4528.614	2.176	-0.887	-100	300	OWLWB91
Fe I	4602.941	1.485	-2.208	-300	300	OWLWB91
Fe I	*4736.773	3.211	-0.752	-200	200	OWLWB91
Fe I	4872.137	2.882	-0.567	-300	300	OWLWB91
Fe I	4890.755	2.876	-0.394	-350	350	OWLWB91
Fe I	4891.492	2.852	-0.112	-300	300	OWLWB91
Fe I	4918.994	2.845	-0.342	-350	350	OWLWB91
Fe I	4920.503	2.832	0.068	-400	100	OWLWB91
Fe I	4938.814	2.875	-1.077	-300	200	OWLWB91
Fe I	4939.687	0.859	-3.252	-250	300	OWLWB91
Fe II	*4178.862	2.583	-2.443	-100	200	SSK04
Fe II	4233.172	2.583	-1.809	-150	200	SSK04
Fe II	4416.828	2.778	-2.540	-240	300	M83
Fe II	4508.289	2.856	-2.318	-300	300	BBKAP91
Fe II	4515.343	2.844	-2.362	-100	300	SSK04
Fe II	4520.224	2.807	-2.550	-200	300	M83
Fe II	*4541.524	2.856	-2.990	-100	200	M83
Fe II	*4555.893	2.828	-2.250	-150	100	SSK04
Fe II	4583.839	2.807	-1.740	-250	300	SSK04
Fe II	4923.927	2.891	-1.206	-400	400	SSK04

**Table A.5:** Data for atomic lines of species heavier than Fe. The spectral window employed for the line is from $\lambda +{\rm d}\lambda _{\rm blue}$ to $\lambda +{\rm d}\lambda _{\rm red}$ . Lines which are removed in carbon-enhanced stars are marked with asterisks in the wavelength column.
Species	$\lambda$	$\chi$	$\log gf$	d $\lambda_{\rm blue}$	d $\lambda_{\rm red}$	Refs.
	[Å]	[eV]		[mÅ]	[mÅ]
Co I	*3842.046	0.923	-0.770	-200	100	CSSTW82
Co I	*3845.461	0.923	0.010	-150	150	CSSTW82
Co I	3894.073	1.049	0.090	-50	200	NKWL99
Co I	3995.302	0.922	-0.140	-250	250	NKWL99
Co I	4118.767	1.049	-0.470	-100	200	NKWL99
Co I	4121.311	0.922	-0.300	-250	250	NKWL99
Ni I	3775.565	0.423	-1.408	-200	200	BBPL89
Ni I	3783.524	0.423	-1.304	-70	300	HS80
Ni I	3807.138	0.423	-1.220	-200	150	BBPL89
Ni I	3858.292	0.423	-0.951	-300	100	BBPL89
Zn I	*4722.163	4.030	-0.390	-300	300	BG80
Zn I	4810.537	4.078	-0.170	-300	300	BG80
Sr I	*4607.327	0.000	0.283	-300	100	MB87
Sr II	4077.709	0.000	0.158	-150	100	PBL95
Sr II	4215.519	0.000	-0.155	-300	200	PBL95
Y II	3774.331	0.130	0.210	-250	150	HLGBW82
Y II	*3788.694	0.104	-0.070	-150	300	HLGBW82
Y II	3818.314	0.130	-0.980	-300	150	HLGBW82
Y II	3950.352	0.104	-0.490	-200	300	HLGBW82
Y II	*4398.013	0.130	-1.000	-250	150	HLGBW82
Y II	4883.684	1.084	0.070	-200	200	HLGBW82
Zr II	*4161.213	0.713	-0.720	-300	130	BGHL81
Zr II	4208.985	0.713	-0.460	-200	200	BGHL81
Zr II	4317.299	0.713	-1.380	-300	300	BGHL81
Ba II	4130.645	2.722	0.560	-150	300	G67
Ba II	4554.000	0.000	0.163	-500	220	G67
La II	*3988.515	0.403	0.210	-300	300	LBS01
La II	3995.745	0.173	-0.060	-250	150	LBS01
La II	4086.709	0.000	-0.070	-200	200	LBS01
La II	4123.218	0.321	0.130	-300	180	LBS01
La II	*4322.503	0.173	-0.930	-300	150	LBS01
La II	*4333.753	0.173	-0.060	-300	100	LBS01
Ce II	3999.237	0.295	0.232	-100	300	VALD95
Ce II	4073.474	0.478	0.320	-150	150	SMPCBA96
Ce II	*4083.222	0.701	0.240	-150	200	SMPCBA96
Ce II	4120.827	0.320	-0.240	-300	300	SMPCBA96
Ce II	*4127.364	0.684	0.240	-300	70	SMPCBA96
Ce II	4222.597	0.122	-0.180	-150	150	GS94
Ce II	*4418.780	0.864	0.310	-200	150	SMPCBA96
Ce II	4486.909	0.295	-0.360	-300	300	GS94
Ce II	4562.359	0.478	0.330	-300	300	GS94
Ce II	4628.161	0.516	0.260	-300	300	GS94
Nd II	*4018.823	0.064	-0.850	-300	120	DLSC03
Nd II	4021.327	0.321	-0.100	-200	200	DLSC03
Nd II	4061.085	0.471	0.550	-300	300	DLSC03
Nd II	4069.265	0.064	-0.570	-200	300	DLSC03
Nd II	*4109.448	0.321	0.350	-150	150	DLSC03
Nd II	4232.374	0.064	-0.470	-200	200	DLSC03
Nd II	*4358.161	0.321	-0.160	-200	150	DLSC03
Nd II	4446.384	0.205	-0.350	-300	300	DLSC03
Nd II	*4462.979	0.559	0.040	-300	300	DLSC03
Sm II	3896.972	0.041	-0.578	-100	200	BGHL89
Sm II	4068.324	0.434	-0.710	-150	150	BGHL89
Sm II	*4318.936	0.277	-0.270	-150	150	BGHL89
Sm II	4499.475	0.248	-1.010	-200	200	BGHL89
Sm II	4519.630	0.544	-0.432	-300	300	BGHL89
Sm II	4537.954	0.485	-0.230	-300	300	BGHL89
Sm II	4577.688	0.248	-0.775	-300	300	BGHL89
Sm II	*4642.232	0.378	-0.520	-150	150	BGHL89
Eu II	3819.670	0.000	0.510	-150	300	LWDS01
Eu II	3907.110	0.207	0.170	-150	200	LWDS01
Eu II	4129.720	0.000	0.220	-150	400	LWDS01
Eu II	*4205.040	0.000	0.210	-50	200	LWDS01

Appendix B: Error estimates

Our method for estimating error propagation is similar to the approach devised by McWilliam et al. (1995b), but modified to suit our abundance analysis method. The important difference is that our approach fits the spectral features of a given element globally rather than fitting individual lines. Further, as discussed in Sect. 3.4, we will make a distinction between absolute (the uncertainty in the absolute abundance) and relative (the uncertainty in the relative abundance between stars) error estimates. First, we develop the formalism quite generally, and later specify the difference between the calculations for these two types of errors.

We consider the propagation of errors in model atmosphere parameters $T_{\rm eff}$ , $\log g$ , $\xi$ . For low metallicity models of the type used here, typical errors in metallicity have negligible effect on the model structure and can be neglected. Errors due to propagation of uncertainties in $\log gf$ , observational error, continuum placement and spectrum modelling uncertainties are also considered. For compactness, in the following discussion we define the abundance parameter $\varepsilon\equiv\log\epsilon$ . Assuming the behaviour of the considered abundance with small changes in these parameters can be approximated by a first-order Taylor expansion, i.e. that the abundance $\varepsilon\equiv\log\epsilon$ varies approximately linearly with changes in parameters on scales of the parameter uncertainties, we obtain (e.g. McWilliam et al. 1995b; Taylor 1982) for the variance in the abundance

We adopt $\sigma_{T,\xi}=0$ and $\sigma_{\log g,\xi}=-0.02$ following McWilliam et al. (1995b). We obtained similar estimates for these quantities from our own numerical experiments for a subsample of stars representative of the complete sample. Based on these experiments we adopted $\sigma_{T,\log g}=+22$ . Thus, the expression for the total variance becomes

Now it simply remains to specify each variance (or standard deviation). The input variances, however, will depend on whether we wish to estimate the absolute error or the relative error.

B.1 Relative error estimates

The relative error estimates are of interest for comparison of abundances within the sample. In particular, we wish to estimate the amount of abundance scatter which should be attributed to uncertainties in the data and analysis.

**Table B.1:** Assigned average values of $\sigma_{\log gf}$ for each element.
Element	$\sigma_{\log gf}$	Element	$\sigma_{\log gf}$
C	0.10	Ni	0.03
Mg	0.07	Zn	0.10
Al	0.11	Sr	0.10
Ca	0.11	Y	0.03
Sc	0.04	Zr	0.03
Ti	0.05	Ba	0.03
V	0.05	La	0.03
Cr	0.05	Ce	0.10
Mn	0.06	Nd	0.03
Fe	0.03	Sm	0.05
Co	0.10	Eu	0.03

First, from Sect. 2.1, we adopt $\sigma_T=100$ K. If the measurement errors in the observed data are normally distributed, the formal random errors in derived spectrum modelling parameters due to this measurement error are given by the SME optimisation routine from the estimated covariance matrix, which is the inverse of the curvature matrix at the solution (see e.g. Press et al 1992). These errors represent the propagation of the random observational uncertainties in each point in the spectrum (dominated by photon noise) to the relevant parameter and is computed by the parameter optimisation procedure. Such contributions are obtained for $\sigma_{\varepsilon}({\rm obs})$ , $\sigma_{\log g}$ and $\sigma_{\xi}$ ; these random components of $\sigma_{\log g}$ and $\sigma_{\xi}$ are usually quite small, around 0.05 dex and 0.05 km s^-1, while $\sigma_{\varepsilon}({\rm obs})$ varies significantly from element to element. To this random component of $\sigma_{\log g}$ we add 0.22 dex reflecting the error due to uncertainty in $T_{\rm eff}$ , and to the random component of $\sigma_{\xi}$ we add 0.1 km s^-1 reflecting the error due to uncertainty in $\log g$ . These numbers are based on the numerical experiments for a representative subsample which were mentioned above.

As mentioned above, errors arise due to uncertainties in the spectrum modelling, for example, assumptions of 1D geometry or LTE. The contributions of these errors to relative errors in abundances would be expected to cancel if all the stars were identical; however, across our sample, which covers a wide range of stellar atmosphere parameters, we can only expect partial cancellation. Thus, such uncertainties will lead to a degree of scatter in any quantity derived from the spectrum, arising from differences in modelling errors from star to star. The relative component of $\sigma_{\varepsilon}({\rm model})$ has been estimated at 0.1 dex. This is simply an order-of-magnitude estimate based on indications from 3-D modelling, (e.g. Asplund 2004,2005) and non-LTE spectrum modelling (e.g. Korn et al. 2003; Asplund 2005). However it should be noted this quantity should vary with element and employed spectral feature. We have neglected any relative error in $\log g$ and $\xi$ which might arise from modelling uncertainties.

Since the relevant continuum points are located close to lines employed in the analysis, they will have very similar error bars to the points in the line, and thus the sensitivity of the abundance to continuum placement errors will be essentially identical to that for the points in the line. Thus we expect that the error due to uncertainty in the continuum placement can be approximated by $\sigma_{\varepsilon}({\rm cont})\approx\sigma_{\varepsilon}({\rm obs})/\sqrt{m}$ , where the $1/\sqrt{m}$ factor accounts for the fact that we typically have m times more independent pixels to define the continuum than the line. Based on inspection of spectra we adopt m=5 for all elements except carbon, where we adopt m=1 since it is determined from wide molecular bands. The estimates for m approximately account for possible correlations between pixels introduced by very weak lines. The uncertainty in $\log gf$ will not contribute to relative errors, and thus we adopt $\sigma_{\log gf}=0$ .

B.2 Absolute error estimates

While relative errors are generally of most interest, it is also important to have some estimate of the absolute error in our obtained abundances. The calculation of absolute errors follows that of the relative errors with a few changes which we now list.

The main differences arise in the modelling uncertainties, as there is no cancellation as in the relative error case. To $\sigma_{\log g}$ and $\sigma_{\xi}$ we add an additional 0.1 dex and 0.1 km s^-1 respectively to account for modelling uncertainties. We estimate $\sigma_{\varepsilon}({\rm model})$ at 0.15 dex. Further, the errors $\sigma_{\log gf}$ must be included in the absolute errors. Since our procedure globally fits the spectral lines of a given element, the value for $\sigma_{\log gf}$ should be representative of the typical error for the chosen spectral lines. In Table B.1 we provide an estimated average uncertainty for each element with reference to the original literature, which are adopted for $\sigma_{\log gf}$ .

B.3 Errors in abundance ratios

We are often interested in elemental abundance ratios. Following McWilliam et al. (1995b), if the abundances $\varepsilon_A$ and $\varepsilon_B$ are expressed in logarithms such that $\varepsilon_{A/B}=\varepsilon_A-\varepsilon_B$ , the variance in the abundance ratio $\varepsilon_{A/B}$ is given by

where $\sigma_{A}^2$ and $\sigma_{B}^2$ are the variance in $\varepsilon_A$ and $\varepsilon_B$ respectively and $\sigma_{A,B}$ is the covariance of $\varepsilon_A$ and $\varepsilon_B$ given by

**Table 1F:** Coordinates of the HES stars (prefix HE) have been derived from the Digitized Sky Survey I and are accurate to 1 $^{\prime \prime }$ ; the coordinates of the HK survey stars (prefix CS) are from identifications of the sources in the 2MASS All Sky Release. Barycentric radial velocities $v_{\rm rad}$ were measured from the snapshot spectra and are accurate to a few km s^-1.
Star	$\alpha(2000.0)$	$\delta(2000.0)$	$v_{\rm rad}$
			[km s^-1]
CS 22175-007	02 17 26.6	-09 00 45	-18.3
CS 22186-023	04 19 45.5	-36 51 35	51.9
CS 22186-025	04 24 32.8	-37 09 02	-122.6
CS 22886-042	22 20 25.8	-10 23 20	-220.6
CS 22892-052	22 17 01.6	-16 39 27	14.5
CS 22945-028	23 31 13.5	-66 29 57	388.9
CS 22957-013	23 55 49.0	-05 22 52	-213.5
CS 22958-083	02 15 42.7	-53 59 56	175.6
CS 22960-010	22 08 25.3	-44 53 56	49.2
CS 29491-069	22 31 02.1	-32 38 36	-375.5
CS 29491-109	22 25 01.1	-32 14 41	160.1
CS 29497-004	00 28 06.9	-26 03 04	105.1
CS 29510-058	02 21 46.5	-24 01 58	153.1
CS 30308-035	20 45 54.1	-44 50 29	-51.8
CS 30315-001	23 37 38.8	-26 21 53	110.3
CS 30315-029	23 34 26.6	-26 42 14	-169.2
CS 30337-097	22 01 21.5	-30 57 57	-108.7
CS 30339-041	00 23 12.9	-37 01 26	-19.3
CS 30343-063	21 45 17.5	-37 22 18	-59.4
CS 31060-047	00 08 07.8	-15 54 03	106.1
CS 31062-041	00 35 03.0	-15 54 29	-173.0
CS 31072-118	05 08 53.5	-59 18 21	145.8
CS 31082-001	01 29 31.1	-16 00 45	139.4
HD 20	00 05 15.3	-27 16 18	-57.5
HD 221170	23 29 28.8	+30 25 57	-120.7
HE 0005-0002	00 08 06.8	+00 14 09	-65.4
HE 0008-3842	00 10 56.0	-38 26 10	128.9
HE 0017-4838	00 19 48.3	-48 21 24	26.8
HE 0018-1349	00 20 52.4	-13 32 29	-161.7
HE 0023-4825	00 25 50.3	-48 08 27	-21.5
HE 0029-1839	00 32 07.7	-18 22 36	-97.8
HE 0037-2657	00 39 51.7	-26 41 31	-279.0
HE 0039-4154	00 41 43.3	-41 37 58	128.9
HE 0043-2845	00 45 55.8	-28 29 16	16.4
HE 0044-2459	00 46 35.8	-24 43 02	-160.0
HE 0044-4023	00 46 29.4	-40 07 23	346.2
HE 0045-2430	00 47 40.5	-24 14 02	144.5
HE 0049-5700	00 52 06.8	-56 44 37	59.8
HE 0051-2304	00 53 51.5	-22 47 55	-135.6
HE 0054-0657	00 57 20.7	-06 41 00	51.3
HE 0057-4541	00 59 59.2	-45 24 54	13.4
HE 0104-4007	01 06 56.0	-39 51 52	200.8
HE 0104-5300	01 06 51.8	-52 44 11	185.8
HE 0105-6141	01 07 38.0	-61 25 17	3.8
HE 0109-0742	01 11 47.0	-07 26 32	-24.1
HE 0109-3711	01 11 38.4	-36 55 17	-1.0
HE 0111-1454	01 13 49.1	-14 38 23	-85.2
HE 0121-2826	01 23 37.2	-28 10 27	-2.0
HE 0131-2740	01 33 25.8	-27 25 28	51.7
HE 0131-3953	01 33 36.4	-39 37 52	67.5
HE 0143-1135	01 46 10.2	-11 20 10	-223.1
HE 0143-4108	01 45 19.9	-40 53 37	55.5
HE 0143-4146	01 45 18.0	-41 31 48	-16.3
HE 0157-3335	02 00 00.2	-33 21 23	-175.2
HE 0200-0955	02 03 16.2	-09 40 48	73.6
HE 0202-2204	02 04 50.0	-21 50 10	108.2
HE 0231-4016	02 33 44.3	-40 03 44	180.8
HE 0240-0807	02 42 57.6	-07 54 35	-98.8
HE 0240-6105	02 42 06.2	-60 53 03	153.0
HE 0243-0753	02 46 14.1	-07 40 53	-13.0
HE 0243-5238	02 45 36.2	-52 25 58	112.3
HE 0244-4111	02 45 57.4	-40 59 08	214.3
HE 0248+0039	02 50 59.0	+00 51 32	48.9
HE 0249-0126	02 51 39.7	-01 14 33	15.1
HE 0256-1109	02 59 10.1	-10 58 01	-132.3
HE 0300-0751	03 03 04.0	-07 39 42	155.5
HE 0305-4520	03 07 02.1	-45 09 00	135.3
HE 0308-1154	03 11 09.8	-11 43 20	13.4
HE 0315+0000	03 17 39.0	+00 11 04	-120.8
HE 0316+0214	03 19 09.2	+02 24 54	-161.0
HE 0317-4640	03 18 56.2	-46 29 27	9.3
HE 0323-4529	03 25 30.1	-45 19 31	180.6
HE 0328-1047	03 30 45.2	-10 37 10	-75.0
HE 0330-4004	03 32 07.3	-39 54 51	227.0
HE 0330-4144	03 32 16.1	-41 34 49	134.2
HE 0331-4939	03 32 41.8	-49 29 10	273.4
HE 0333-4001	03 35 25.7	-39 51 48	-162.3
HE 0336-3829	03 38 31.7	-38 20 15	-109.1
HE 0337-5127	03 39 13.0	-51 18 16	75.4
HE 0338-3945	03 39 54.9	-39 35 44	177.7
HE 0339-4027	03 40 49.6	-40 17 36	22.0
HE 0340-3430	03 42 04.7	-34 20 50	228.1
HE 0340-5355	03 41 34.6	-53 46 17	317.5
HE 0341-4024	03 43 07.9	-40 15 30	211.8
HE 0344+0139	03 47 15.7	+01 49 03	-232.9
HE 0347-1819	03 49 18.4	-18 10 40	-4.8
HE 0353-6024	03 53 59.5	-60 15 16	178.8
HE 0400-2917	04 02 06.4	-29 08 47	296.8
HE 0401-0138	04 03 49.8	-01 30 03	137.4
HE 0417-0821	04 19 31.4	-08 14 19	-8.5
HE 0430-4404	04 31 38.1	-43 57 49	201.5
HE 0430-4901	04 31 31.1	-48 54 42	208.7
HE 0432-0923	04 34 25.6	-09 16 50	-66.5
HE 0436-4008	04 38 11.0	-40 03 01	185.7
HE 0441-4343	04 43 20.4	-43 38 20	165.0
HE 0442-1234	04 44 51.7	-12 28 46	253.4
HE 0447-4858	04 49 01.0	-48 53 35	88.5
HE 0450-4705	04 51 33.4	-47 00 03	-6.3
HE 0454-4758	04 55 26.7	-47 53 42	240.5
HE 0501-5139	05 02 48.1	-51 35 36	199.3
HE 0501-5644	05 02 35.3	-56 40 20	70.8
HE 0512-3835	05 13 59.5	-38 31 55	276.2
HE 0513-4557	05 15 12.1	-45 54 10	51.2
HE 0516-3820	05 18 12.9	-38 17 33	153.5
HE 0517-1952	05 19 18.7	-19 49 13	42.2
HE 0519-5525	05 19 59.1	-55 22 41	377.4
HE 0520-1748	05 22 25.8	-17 46 08	1.3
HE 0524-2055	05 27 04.4	-20 52 42	255.3
HE 0534-4615	05 35 52.9	-46 13 36	280.4
HE 0538-4515	05 39 46.1	-45 13 34	59.2
HE 0547-4539	05 49 13.7	-45 39 04	488.8
HE 0858-0016	09 01 32.3	-00 28 02	48.6
HE 0926-0508	09 28 55.3	-05 21 39	191.0
HE 0938+0114	09 40 43.0	+01 00 37	-56.6
HE 0951-1152	09 54 17.4	-12 06 14	353.9
HE 1006-2218	10 09 00.7	-22 33 29	-19.6
HE 1015-0027	10 17 35.7	-00 42 24	96.8
HE 1044-2509	10 47 16.5	-25 25 17	386.7
HE 1052-2548	10 55 20.6	-26 04 47	230.4
HE 1054-0059	10 56 47.7	-01 15 29	234.0
HE 1059-0118	11 02 03.4	-01 34 15	296.6
HE 1100-0137	11 02 55.5	-01 53 41	318.1
HE 1105+0027	11 07 49.5	+00 11 38	77.0
HE 1120-0153	11 22 43.2	-02 09 36	228.4
HE 1122-1429	11 25 06.6	-14 46 04	152.0
HE 1124-2335	11 27 27.0	-23 52 06	180.4
HE 1126-1735	11 28 51.4	-17 51 44	281.9
HE 1127-1143	11 29 50.5	-12 00 13	228.5
HE 1128-0823	11 30 44.3	-08 39 56	200.2
HE 1131+0141	11 34 32.1	+01 24 41	267.7
HE 1132+0125	11 34 46.7	+01 09 01	92.0
HE 1132+0204	11 34 51.0	+01 47 27	238.2
HE 1135+0139	11 38 09.8	+01 22 44	11.0
HE 1135-0344	11 38 21.0	-04 01 24	-167.4
HE 1148-0037	11 51 15.0	-00 54 11	-36.6
HE 1207-2031	12 09 50.8	-20 47 43	113.3
HE 1210+0048	12 13 27.8	+00 32 10	110.4
HE 1210-1956	12 12 50.9	-20 12 58	123.3
HE 1212-0127	12 15 18.3	-01 43 56	279.4
HE 1214-1819	12 17 01.5	-18 35 55	180.3
HE 1215+0149	12 17 43.1	+01 32 32	124.5
HE 1217-0540	12 19 53.7	-05 57 15	151.2
HE 1219-0312	12 21 34.1	-03 28 40	163.6
HE 1221-0522	12 24 07.7	-05 39 11	48.6
HE 1221-1948	12 23 47.7	-20 04 46	31.6
HE 1222-0200	12 25 29.4	-02 17 24	226.8
HE 1222-0336	12 24 52.4	-03 53 06	-198.5
HE 1225+0155	12 28 04.8	+01 38 32	99.4
HE 1225-0515	12 28 12.4	-05 31 40	61.5
HE 1230-1724	12 32 57.0	-17 41 27	99.1
HE 1243-1425	12 46 28.1	-14 41 34	41.8
HE 1245-1616	12 47 56.8	-16 32 44	141.9
HE 1246-1344	12 49 20.2	-14 00 42	47.9
HE 1247-2114	12 50 05.1	-21 30 47	75.7
HE 1248-1800	12 51 28.0	-18 16 30	280.7
HE 1249-2932	12 52 18.4	-29 48 57	-13.3
HE 1249-3121	12 52 05.1	-31 37 44	218.7
HE 1251-0104	12 53 52.1	-01 20 36	195.1
HE 1252+0044	12 55 22.1	+00 28 00	395.5
HE 1252-0117	12 54 59.8	-01 33 35	225.7
HE 1254+0009	12 57 12.9	-00 06 41	168.5
HE 1256-0228	12 58 38.4	-02 44 18	30.4
HE 1256-0651	12 59 13.1	-07 07 18	120.1
HE 1259-0621	13 01 51.1	-06 37 14	130.6
HE 1300+0157	13 02 56.3	+01 41 51	73.6
HE 1300-0641	13 03 34.1	-06 57 21	67.9
HE 1300-0642	13 03 23.3	-06 58 23	-16.4
HE 1300-2201	13 03 17.3	-22 17 38	-62.8
HE 1300-2431	13 03 00.1	-24 47 12	308.1
HE 1305-0331	13 07 58.9	-03 47 41	-38.4
HE 1311-1412	13 13 42.0	-14 28 24	195.3
HE 1314-3036	13 17 29.2	-30 51 51	34.6
HE 1320-1339	13 22 44.1	-13 55 31	172.1
HE 1330-0354	13 33 10.7	-04 10 05	35.3
HE 1330-0607	13 32 56.6	-06 22 31	-32.4
HE 1332-0309	13 34 38.0	-03 24 53	200.3
HE 1333-0340	13 35 51.5	-03 55 49	-114.6
HE 1335+0135	13 37 53.9	+01 20 26	121.0
HE 1337+0012	13 40 02.7	-00 02 18	441.7
HE 1337-0453	13 39 58.3	-05 08 32	79.3
HE 1343-0640	13 46 09.1	-06 55 46	62.1
HE 1345-0206	13 48 16.0	-02 21 47	124.7
HE 1351-1049	13 53 57.1	-11 04 24	285.4
HE 1413-1954	14 16 04.7	-20 08 54	-100.4
HE 1419-1759	14 22 17.7	-18 13 30	201.4
HE 1421-2006	14 23 50.5	-20 20 11	3.8
HE 1430+0053	14 33 16.5	+00 40 49	-107.4
HE 1430-0026	14 33 16.2	-00 39 49	50.6
HE 1430-1123	14 33 33.7	-11 37 08	93.4
HE 1431-2142	14 34 06.7	-21 55 16	-165.0
HE 1500-1628	15 02 56.6	-16 40 07	23.5
HE 2133-1432	21 36 22.6	-14 19 20	-129.0
HE 2134+0001	21 37 08.2	+00 15 04	48.0
HE 2139-1851	21 42 29.5	-18 37 51	-91.6
HE 2143+0030	21 46 12.0	+00 44 46	-76.2
HE 2145-3025	21 48 43.3	-30 11 08	131.4
HE 2150-0825	21 53 00.2	-08 11 19	-63.3
HE 2151-2858	21 54 01.7	-28 44 20	-89.7
HE 2153-2719	21 56 04.1	-27 04 49	-111.8
HE 2154-2838	21 57 43.7	-28 24 31	-16.9
HE 2155+0136	21 57 37.7	+01 50 20	-248.2
HE 2156-3130	21 59 05.8	-31 16 12	269.8
HE 2158-3112	22 01 21.4	-30 57 57	-110.0
HE 2200-2030	22 03 02.6	-20 15 58	89.7
HE 2201-0637	22 03 44.6	-06 22 42	114.0
HE 2204-1703	22 07 12.0	-16 49 10	-11.7
HE 2206-2245	22 09 09.4	-22 30 17	-210.5
HE 2216-0621	22 18 46.1	-06 06 50	52.5
HE 2216-1548	22 19 30.5	-15 33 36	-271.0
HE 2217-0706	22 20 18.0	-06 51 17	-93.3
HE 2217-1523	22 20 33.8	-15 08 34	79.5
HE 2219-0713	22 22 15.8	-06 58 34	-111.8
HE 2221-4150	22 24 47.3	-41 35 38	40.2
HE 2222-4156	22 25 28.6	-41 40 57	-126.0
HE 2224+0143	22 27 23.0	+01 58 33	-112.3
HE 2224-4103	22 27 48.2	-40 48 25	-60.7
HE 2226-4102	22 29 04.3	-40 46 53	96.0
HE 2227-4044	22 30 19.2	-40 29 13	103.9
HE 2228-3806	22 31 02.6	-37 50 41	179.0
HE 2229-4153	22 32 49.0	-41 38 25	-139.6
HE 2231-0622	22 34 20.2	-06 06 30	-428.8
HE 2234-0521	22 36 37.7	-05 06 05	-177.8
HE 2238-2152	22 41 10.3	-21 36 19	-22.2
HE 2240-0412	22 42 58.1	-03 56 33	-163.7
HE 2242-1930	22 45 17.3	-19 14 52	-22.5
HE 2243-0151	22 46 08.9	-01 35 55	-47.4
HE 2244-1503	22 47 25.9	-14 47 30	148.1
HE 2247-3705	22 50 29.5	-36 49 17	143.6
HE 2248-3345	22 51 44.6	-33 29 25	145.4
HE 2250-2132	22 53 40.3	-21 16 24	-207.6
HE 2252-4157	22 55 34.1	-41 41 29	-94.5
HE 2252-4225	22 54 58.6	-42 09 19	-333.7
HE 2258-3456	23 00 59.8	-34 40 42	-229.0
HE 2259-3407	23 02 15.6	-33 51 11	-13.6
HE 2301-4024	23 04 13.9	-40 08 21	-221.7
HE 2301-4126	23 03 50.2	-41 10 27	252.2
HE 2304-4153	23 07 05.5	-41 37 30	-33.9
HE 2311+0129	23 14 21.4	+01 45 24	-149.0
HE 2314-1554	23 17 01.2	-15 37 49	72.8
HE 2319-0852	23 22 17.3	-08 36 17	-121.6
HE 2325-0755	23 27 59.5	-07 39 12	-237.0
HE 2326+0038	23 28 56.9	+00 54 35	-40.9
HE 2327-5642	23 30 37.2	-56 26 14	282.1
HE 2329-3702	23 32 18.0	-36 45 59	71.7
HE 2333-1358	23 35 48.5	-13 41 31	96.7
HE 2334-0604	23 37 28.6	-05 47 56	-18.5
HE 2335-5958B	23 38 19.4	-59 42 05	210.7
HE 2338-1311	23 41 08.3	-12 55 10	-84.0
HE 2338-1618	23 40 36.2	-16 01 28	-219.4
HE 2345-1919	23 47 55.4	-19 02 37	119.4
HE 2347-1254	23 50 09.8	-12 37 50	-43.5
HE 2347-1334	23 50 26.9	-13 17 39	-54.8
HE 2347-1448	23 49 58.3	-14 32 16	-165.1

**Table 2F:** Derived stellar atmosphere parameters and elemental abundances for the sample. For each star we report the average signal-to-noise ratio per pixel for the whole observed spectrum, the stellar parameters with their respective relative and absolute r.m.s. error estimates, $\sigma^\mathrm{rel}$ and $\sigma^\mathrm{abs}$ , then for each element X the abundance $\log \epsilon_\mathrm{X}$ and its relative and absolute r.m.s. error estimates $\sigma_{\log\epsilon_\mathrm{X}}$ , [X/Fe] and its relative and absolute r.m.s. error estimates $\sigma_\mathrm{[X/Fe]}$ . N gives the number of features of the element used in each star, noting that this varies from star to star as certain features may be automatically rejected if the star has a strong G band, if the feature is near a Balmer line in warmer stars (see Sect. 3.2), or if they are determined to be affected by a cosmic ray hit or bad pixel. N3 then gives the number of those features classified as 3 $\sigma$ detections. In the case of CH bands we simply classify detections and non-detections with 1 and 0 respectively. In the case of a non-detection, this is signified by an abundance of -9.99 and error of 0.00.
Star	S/N_av	T_eff	$\sigma_{T_\mathrm{eff}}$	$\log g$	$\sigma_{\log g}^\mathrm{rel}$	$\sigma_{\log g}^\mathrm{abs}$	[Fe/H]	$\sigma_\mathrm{[Fe/H]}^\mathrm{rel}$	$\sigma_\mathrm{[Fe/H]}^\mathrm{abs}$	$\xi$	$\sigma_\xi^\mathrm{rel}$	$\sigma_\xi^\mathrm{abs}$	$\log\epsilon_\mathrm{C}$	$\sigma_{\log\epsilon_\mathrm{C}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{C}}^\mathrm{abs}$	[C/Fe]	$\sigma_\mathrm{[C/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[C/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{Mg}$	$\sigma_{\log\epsilon_\mathrm{Mg}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{Mg}}^\mathrm{abs}$	[Mg/Fe]	$\sigma_\mathrm{[Mg/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[Mg/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{Al}$	$\sigma_{\log\epsilon_\mathrm{Al}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{Al}}^\mathrm{abs}$	[Al/Fe]	$\sigma_\mathrm{[Al/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[Al/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{Ca}$	$\sigma_{\log\epsilon_\mathrm{Ca}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{Ca}}^\mathrm{abs}$	[Ca/Fe]	$\sigma_\mathrm{[Ca/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[Ca/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{Sc}$	$\sigma_{\log\epsilon_\mathrm{Sc}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{Sc}}^\mathrm{abs}$	[Sc/Fe]	$\sigma_\mathrm{[Sc/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[Sc/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{Ti}$	$\sigma_{\log\epsilon_\mathrm{Ti}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{Ti}}^\mathrm{abs}$	[Ti/Fe]	$\sigma_\mathrm{[Ti/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[Ti/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{V}$	$\sigma_{\log\epsilon_\mathrm{V}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{V}}^\mathrm{abs}$	[V/Fe]	$\sigma_\mathrm{[V/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[V/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{Cr}$	$\sigma_{\log\epsilon_\mathrm{Cr}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{Cr}}^\mathrm{abs}$	[Cr/Fe]	$\sigma_\mathrm{[Cr/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[Cr/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{Mn}$	$\sigma_{\log\epsilon_\mathrm{Mn}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{Mn}}^\mathrm{abs}$	[Mn/Fe]	$\sigma_\mathrm{[Mn/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[Mn/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{Fe}$	$\sigma_{\log\epsilon_\mathrm{Fe}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{Fe}}^\mathrm{abs}$	[Fe/Fe]	$\sigma_\mathrm{[Fe/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[Fe/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{Co}$	$\sigma_{\log\epsilon_\mathrm{Co}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{Co}}^\mathrm{abs}$	[Co/Fe]	$\sigma_\mathrm{[Co/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[Co/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{Ni}$	$\sigma_{\log\epsilon_\mathrm{Ni}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{Ni}}^\mathrm{abs}$	[Ni/Fe]	$\sigma_\mathrm{[Ni/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[Ni/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{Zn}$	$\sigma_{\log\epsilon_\mathrm{Zn}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{Zn}}^\mathrm{abs}$	[Zn/Fe]	$\sigma_\mathrm{[Zn/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[Zn/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{Sr}$	$\sigma_{\log\epsilon_\mathrm{Sr}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{Sr}}^\mathrm{abs}$	[Sr/Fe]	$\sigma_\mathrm{[Sr/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[Sr/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{Y}$	$\sigma_{\log\epsilon_\mathrm{Y}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{Y}}^\mathrm{abs}$	[Y/Fe]	$\sigma_\mathrm{[Y/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[Y/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{Zr}$	$\sigma_{\log\epsilon_\mathrm{Zr}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{Zr}}^\mathrm{abs}$	[Zr/Fe]	$\sigma_\mathrm{[Zr/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[Zr/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{Ba}$	$\sigma_{\log\epsilon_\mathrm{Ba}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{Ba}}^\mathrm{abs}$	[Ba/Fe]	$\sigma_\mathrm{[Ba/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[Ba/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{La}$	$\sigma_{\log\epsilon_\mathrm{La}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{La}}^\mathrm{abs}$	[La/Fe]	$\sigma_\mathrm{[La/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[La/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{Ce}$	$\sigma_{\log\epsilon_\mathrm{Ce}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{Ce}}^\mathrm{abs}$	[Ce/Fe]	$\sigma_\mathrm{[Ce/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[Ce/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{Nd}$	$\sigma_{\log\epsilon_\mathrm{Nd}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{Nd}}^\mathrm{abs}$	[Nd/Fe]	$\sigma_\mathrm{[Nd/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[Nd/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{Sm}$	$\sigma_{\log\epsilon_\mathrm{Sm}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{Sm}}^\mathrm{abs}$	[Sm/Fe]	$\sigma_\mathrm{[Sm/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[Sm/Fe]}^\mathrm{abs}$	N	N3	$\log\epsilon_\mathrm{Eu}$	$\sigma_{\log\epsilon_\mathrm{Eu}}^\mathrm{rel}$	$\sigma_{\log\epsilon_\mathrm{Eu}}^\mathrm{abs}$	[Eu/Fe]	$\sigma_\mathrm{[Eu/Fe]}^\mathrm{rel}$	$\sigma_\mathrm{[Eu/Fe]}^\mathrm{abs}$	N	N3
		[K]		[cm s^-2]						[km s^-1]
CS 22175-007	31	5108	100	2.46	0.26	0.36	-2.81	0.13	0.18	1.67	0.14	0.24	5.77	0.19	0.26	0.19	0.18	0.27	1	1	5.15	0.12	0.18	0.37	0.15	0.24	7	4	2.54	0.17	0.25	-1.12	0.18	0.26	1	1	3.87	0.12	0.20	0.31	0.15	0.25	9	5	0.49	0.18	0.23	0.13	0.16	0.25	5	3	2.56	0.17	0.22	0.34	0.15	0.24	17	8	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.52	0.17	0.24	-0.35	0.16	0.24	3	3	1.84	0.17	0.22	-0.74	0.16	0.23	5	3	4.69	0.13	0.18	0.00	0.14	0.22	55	35	2.35	0.15	0.22	0.24	0.15	0.24	6	4	3.70	0.20	0.30	0.25	0.19	0.28	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.33	0.20	0.30	0.16	0.19	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.15	0.21	0.25	-0.47	0.18	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
CS 22186-023	55	5066	100	2.19	0.24	0.34	-2.72	0.13	0.18	1.58	0.11	0.21	5.97	0.19	0.25	0.30	0.18	0.27	1	1	4.99	0.12	0.18	0.14	0.15	0.23	7	6	2.78	0.15	0.24	-0.97	0.16	0.26	1	1	3.77	0.12	0.20	0.13	0.15	0.25	9	7	0.46	0.17	0.23	0.01	0.15	0.24	5	4	2.44	0.16	0.21	0.15	0.15	0.23	17	14	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.68	0.16	0.25	-0.27	0.15	0.25	3	3	2.27	0.15	0.21	-0.39	0.15	0.23	5	3	4.78	0.13	0.18	0.00	0.14	0.22	55	50	2.33	0.16	0.22	0.13	0.15	0.24	6	5	3.56	0.17	0.28	0.03	0.17	0.27	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.10	0.19	0.30	-0.14	0.18	0.29	3	2	-0.89	0.18	0.23	-0.41	0.15	0.24	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.52	0.19	0.23	-0.93	0.16	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
CS 22186-025	32	4985	100	1.70	0.26	0.36	-2.87	0.14	0.19	2.14	0.13	0.23	4.83	0.20	0.27	-0.68	0.19	0.29	1	1	4.99	0.12	0.18	0.28	0.15	0.24	7	3	2.60	0.21	0.27	-1.00	0.21	0.29	1	1	3.75	0.12	0.20	0.26	0.15	0.25	9	3	0.44	0.18	0.23	0.14	0.16	0.24	5	4	2.40	0.15	0.20	0.26	0.14	0.23	17	9	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.35	0.16	0.23	-0.44	0.15	0.23	3	3	1.85	0.16	0.21	-0.67	0.15	0.23	5	3	4.63	0.14	0.19	0.00	0.14	0.22	55	36	2.26	0.15	0.22	0.21	0.15	0.24	6	4	3.12	0.19	0.25	-0.26	0.18	0.25	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.20	0.25	0.35	-0.29	0.23	0.33	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.59	0.24	0.31	0.16	0.21	0.30	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
CS 22886-042	39	4881	100	1.85	0.25	0.35	-2.68	0.12	0.18	1.84	0.12	0.22	5.72	0.19	0.26	0.01	0.19	0.28	1	1	5.13	0.12	0.18	0.23	0.15	0.23	7	6	2.70	0.17	0.26	-1.10	0.18	0.27	1	1	3.90	0.12	0.20	0.22	0.14	0.25	9	7	0.50	0.17	0.23	0.01	0.16	0.25	5	4	2.50	0.16	0.21	0.16	0.15	0.24	17	13	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.64	0.17	0.26	-0.35	0.17	0.25	3	3	2.20	0.15	0.21	-0.51	0.15	0.23	5	3	4.82	0.12	0.18	0.00	0.14	0.22	55	47	2.34	0.14	0.21	0.10	0.15	0.24	6	5	3.46	0.19	0.28	-0.11	0.19	0.27	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.13	0.20	0.30	-0.16	0.19	0.29	3	2	-0.68	0.18	0.23	-0.25	0.16	0.25	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.67	0.24	0.31	-0.12	0.22	0.30	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
CS 22892-052	46	4884	100	1.81	0.26	0.36	-2.95	0.14	0.19	1.67	0.12	0.22	6.44	0.19	0.26	1.00	0.18	0.28	1	1	4.75	0.13	0.19	0.12	0.15	0.24	5	5	2.79	0.16	0.26	-0.72	0.18	0.28	1	1	3.63	0.12	0.20	0.22	0.15	0.25	5	3	0.20	0.17	0.22	-0.01	0.15	0.24	3	2	2.12	0.15	0.20	0.05	0.14	0.22	11	8	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	2.25	0.17	0.25	-0.47	0.17	0.25	1	1	1.77	0.12	0.20	-0.67	0.15	0.23	4	2	4.55	0.14	0.19	0.00	0.14	0.22	35	27	1.99	0.15	0.22	0.02	0.15	0.24	4	4	3.39	0.20	0.29	0.09	0.18	0.27	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	1	0	0.63	0.16	0.23	0.61	0.15	0.24	2	2	-0.26	0.18	0.23	0.45	0.15	0.24	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.37	0.16	0.21	1.19	0.15	0.23	2	1	-0.76	0.18	0.23	1.02	0.16	0.24	3	3	-9.99	0.00	0.00	-9.99	0.00	0.00	7	0	-0.31	0.19	0.23	1.14	0.16	0.24	5	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-0.90	0.18	0.23	1.54	0.15	0.24	3	3
CS 22945-028	31	5126	100	2.55	0.26	0.36	-2.66	0.13	0.18	1.53	0.14	0.24	5.93	0.19	0.26	0.21	0.18	0.27	1	1	5.24	0.13	0.18	0.32	0.15	0.23	7	4	2.83	0.18	0.26	-0.97	0.19	0.28	1	1	4.03	0.11	0.20	0.33	0.15	0.25	9	6	0.47	0.18	0.23	-0.04	0.16	0.25	5	2	2.57	0.16	0.21	0.22	0.15	0.24	17	8	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.77	0.18	0.26	-0.24	0.17	0.25	3	3	2.18	0.18	0.23	-0.55	0.16	0.24	5	3	4.84	0.13	0.18	0.00	0.14	0.22	55	38	2.39	0.16	0.22	0.14	0.15	0.25	6	4	3.61	0.22	0.30	0.02	0.21	0.29	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.37	0.21	0.30	0.06	0.20	0.29	3	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.66	0.23	0.28	-0.13	0.20	0.28	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
CS 22957-013	35	4904	100	1.96	0.25	0.35	-2.64	0.14	0.19	1.79	0.12	0.22	5.85	0.19	0.26	0.10	0.17	0.27	1	1	5.11	0.11	0.18	0.17	0.16	0.24	7	5	2.89	0.20	0.26	-0.94	0.20	0.28	1	1	3.91	0.12	0.20	0.19	0.15	0.25	9	7	0.59	0.18	0.23	0.06	0.15	0.24	5	4	2.54	0.15	0.21	0.16	0.14	0.22	17	13	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.49	0.18	0.26	-0.54	0.16	0.25	3	3	2.25	0.16	0.22	-0.50	0.15	0.23	5	3	4.86	0.14	0.19	0.00	0.14	0.22	55	44	2.46	0.16	0.23	0.18	0.15	0.24	6	5	3.52	0.21	0.30	-0.09	0.19	0.28	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.06	0.20	0.31	-0.27	0.19	0.30	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.06	0.21	0.27	-0.54	0.18	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
CS 22958-083	32	5101	100	2.40	0.26	0.36	-2.79	0.12	0.18	1.50	0.13	0.23	6.24	0.20	0.26	0.64	0.18	0.27	1	1	5.19	0.12	0.18	0.40	0.15	0.23	7	6	2.80	0.17	0.26	-0.88	0.19	0.28	1	1	3.89	0.12	0.20	0.32	0.15	0.24	9	6	0.41	0.19	0.24	0.03	0.17	0.26	5	3	2.52	0.16	0.21	0.29	0.15	0.24	17	10	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.78	0.17	0.27	-0.10	0.17	0.27	3	3	2.33	0.16	0.22	-0.27	0.16	0.24	5	3	4.71	0.12	0.18	0.00	0.14	0.22	55	37	2.41	0.16	0.22	0.28	0.15	0.24	6	5	3.74	0.19	0.29	0.28	0.19	0.29	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.12	0.21	0.31	-0.06	0.21	0.31	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.65	0.19	0.24	-0.99	0.17	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
CS 22960-010	35	5737	100	4.85	0.25	0.35	-2.65	0.12	0.17	1.53	0.17	0.27	6.56	0.17	0.24	0.82	0.16	0.25	1	1	5.18	0.13	0.19	0.25	0.15	0.24	7	1	2.90	0.14	0.21	-0.92	0.15	0.25	1	1	3.97	0.12	0.20	0.27	0.14	0.24	9	3	0.69	0.18	0.23	0.17	0.17	0.27	5	1	2.57	0.16	0.21	0.20	0.16	0.26	17	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.89	0.15	0.20	-0.13	0.15	0.23	3	3	2.46	0.15	0.20	-0.28	0.15	0.24	5	3	4.85	0.12	0.17	0.00	0.14	0.22	55	29	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	3.53	0.16	0.21	-0.06	0.16	0.24	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
CS 29491-069	57	5103	100	2.45	0.24	0.34	-2.81	0.13	0.18	1.54	0.12	0.22	5.76	0.19	0.25	0.18	0.17	0.27	1	1	5.05	0.11	0.18	0.28	0.15	0.24	7	6	2.64	0.14	0.23	-1.03	0.15	0.25	1	1	3.84	0.12	0.20	0.29	0.15	0.25	9	8	0.37	0.17	0.22	0.00	0.15	0.24	5	4	2.42	0.16	0.21	0.20	0.14	0.23	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.58	0.16	0.24	-0.29	0.15	0.24	3	3	2.01	0.17	0.22	-0.57	0.15	0.23	5	3	4.69	0.13	0.18	0.00	0.14	0.22	55	46	2.28	0.16	0.22	0.16	0.15	0.24	6	5	3.40	0.18	0.26	-0.05	0.16	0.25	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.23	0.18	0.27	0.07	0.16	0.27	3	2	-0.57	0.18	0.23	0.00	0.15	0.24	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.34	0.22	0.29	0.34	0.19	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.24	0.18	0.23	1.06	0.15	0.24	4	2
CS 29491-109	50	4736	100	1.50	0.24	0.34	-2.90	0.15	0.19	1.82	0.12	0.22	5.30	0.20	0.27	-0.19	0.16	0.27	1	1	4.98	0.12	0.18	0.30	0.15	0.24	7	6	2.74	0.16	0.25	-0.83	0.17	0.30	1	1	3.71	0.11	0.20	0.25	0.15	0.26	9	8	0.25	0.17	0.22	-0.02	0.15	0.23	5	4	2.32	0.15	0.20	0.20	0.15	0.23	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.40	0.15	0.25	-0.37	0.15	0.29	3	3	1.77	0.15	0.21	-0.72	0.15	0.25	5	3	4.60	0.15	0.19	0.00	0.14	0.22	55	51	2.06	0.15	0.22	0.04	0.14	0.25	6	5	3.20	0.17	0.27	-0.15	0.17	0.31	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.31	0.21	0.31	-0.38	0.20	0.33	3	2	-1.19	0.18	0.23	-0.53	0.15	0.23	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.69	0.20	0.24	-0.92	0.16	0.24	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
CS 29497-004	39	5013	100	2.23	0.24	0.34	-2.81	0.13	0.18	1.62	0.13	0.23	5.80	0.19	0.26	0.22	0.18	0.27	1	1	5.08	0.12	0.18	0.31	0.15	0.24	7	6	2.62	0.16	0.25	-1.04	0.17	0.26	1	1	3.83	0.12	0.20	0.28	0.15	0.25	9	6	0.41	0.18	0.22	0.05	0.15	0.24	5	4	2.42	0.16	0.21	0.21	0.14	0.23	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.51	0.18	0.26	-0.35	0.17	0.25	3	2	2.18	0.18	0.24	-0.40	0.16	0.24	5	3	4.69	0.13	0.18	0.00	0.14	0.22	55	42	2.35	0.16	0.22	0.24	0.15	0.24	6	5	3.48	0.19	0.29	0.05	0.18	0.28	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.73	0.15	0.22	0.57	0.15	0.24	3	2	0.08	0.18	0.23	0.66	0.16	0.24	6	4	0.73	0.18	0.22	0.94	0.15	0.24	3	1	0.53	0.13	0.19	1.21	0.15	0.22	2	1	-0.43	0.18	0.23	1.21	0.15	0.25	6	5	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-0.02	0.19	0.23	1.29	0.15	0.25	9	2	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-0.68	0.18	0.23	1.62	0.15	0.24	4	4
CS 29510-058	38	5108	100	2.32	0.24	0.34	-2.61	0.12	0.18	1.62	0.12	0.22	6.18	0.19	0.25	0.40	0.18	0.27	1	1	5.23	0.12	0.18	0.26	0.15	0.24	7	6	2.86	0.18	0.25	-1.00	0.18	0.27	1	1	4.04	0.11	0.20	0.29	0.15	0.25	9	7	0.48	0.18	0.23	-0.08	0.16	0.25	5	4	2.63	0.16	0.21	0.23	0.15	0.23	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.90	0.17	0.27	-0.16	0.17	0.26	3	3	2.26	0.16	0.22	-0.52	0.15	0.23	5	3	4.89	0.12	0.18	0.00	0.14	0.22	55	43	2.46	0.16	0.22	0.15	0.15	0.24	6	5	3.48	0.19	0.28	-0.16	0.18	0.27	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.53	0.17	0.25	0.17	0.16	0.26	3	2	-0.35	0.19	0.23	0.02	0.16	0.25	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.49	0.24	0.30	-0.01	0.21	0.29	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
CS 30308-035	32	4806	100	1.78	0.27	0.37	-3.35	0.13	0.18	1.64	0.14	0.24	5.08	0.20	0.27	0.04	0.19	0.29	1	1	4.24	0.13	0.19	0.01	0.15	0.23	7	3	2.10	0.16	0.24	-1.01	0.17	0.26	1	1	3.12	0.12	0.20	0.12	0.15	0.25	9	1	-0.28	0.17	0.22	-0.09	0.16	0.24	5	2	1.67	0.16	0.21	0.00	0.15	0.23	17	6	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.78	0.16	0.22	-0.53	0.15	0.23	3	3	1.39	0.17	0.21	-0.64	0.15	0.23	5	3	4.15	0.13	0.18	0.00	0.14	0.22	55	28	1.73	0.16	0.22	0.17	0.15	0.24	6	1	3.15	0.21	0.29	0.26	0.20	0.28	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-1.19	0.23	0.31	-0.81	0.21	0.31	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
CS 30315-001	37	4565	100	1.14	0.25	0.35	-2.98	0.11	0.17	1.99	0.12	0.22	4.93	0.22	0.28	-0.50	0.21	0.29	1	1	4.99	0.12	0.18	0.38	0.14	0.23	7	5	2.54	0.20	0.29	-0.97	0.22	0.30	1	1	3.65	0.11	0.20	0.25	0.14	0.24	9	7	0.28	0.17	0.22	0.08	0.16	0.25	5	4	2.21	0.16	0.21	0.16	0.16	0.24	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.08	0.16	0.25	-0.62	0.17	0.25	3	3	2.04	0.13	0.20	-0.39	0.15	0.23	5	3	4.53	0.11	0.17	0.00	0.14	0.22	55	51	2.13	0.15	0.22	0.18	0.16	0.25	6	5	3.40	0.20	0.30	0.12	0.20	0.29	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.32	0.17	0.24	0.32	0.17	0.26	3	2	-0.65	0.17	0.22	0.08	0.17	0.26	6	4	0.08	0.17	0.22	0.44	0.17	0.26	3	1	-1.66	0.19	0.24	-0.82	0.18	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
CS 30315-029	38	4541	100	1.07	0.25	0.35	-3.33	0.12	0.18	2.06	0.13	0.23	4.63	0.21	0.28	-0.43	0.20	0.29	1	1	4.67	0.12	0.19	0.42	0.15	0.23	7	5	2.54	0.15	0.26	-0.59	0.18	0.29	1	1	3.33	0.12	0.20	0.30	0.15	0.25	9	4	-0.19	0.16	0.21	-0.03	0.15	0.23	5	4	1.87	0.15	0.20	0.18	0.15	0.23	17	11	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.82	0.15	0.22	-0.52	0.15	0.24	3	3	1.21	0.15	0.21	-0.85	0.15	0.23	5	3	4.17	0.12	0.18	0.00	0.14	0.22	55	41	1.67	0.14	0.21	0.08	0.15	0.24	6	4	2.72	0.18	0.27	-0.19	0.18	0.26	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.55	0.25	0.35	-0.19	0.22	0.33	3	2	-1.31	0.18	0.23	-0.21	0.16	0.25	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.79	0.24	0.32	0.42	0.22	0.30	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-2.10	0.18	0.23	0.72	0.16	0.25	4	3
CS 30337-097	44	4865	100	1.81	0.24	0.34	-2.73	0.13	0.18	1.88	0.12	0.22	5.64	0.20	0.26	-0.02	0.18	0.28	1	1	5.13	0.11	0.18	0.29	0.15	0.23	7	6	3.17	0.16	0.25	-0.57	0.17	0.27	1	1	3.79	0.12	0.20	0.17	0.15	0.25	9	7	0.51	0.17	0.22	0.07	0.15	0.24	5	4	2.40	0.15	0.20	0.11	0.14	0.23	17	13	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.58	0.16	0.25	-0.36	0.16	0.25	3	3	2.30	0.12	0.20	-0.36	0.14	0.23	5	3	4.77	0.13	0.18	0.00	0.14	0.22	55	49	2.27	0.13	0.21	0.09	0.14	0.24	6	6	3.35	0.18	0.28	-0.16	0.17	0.26	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.09	0.19	0.30	-0.15	0.18	0.29	3	2	-0.89	0.13	0.19	-0.39	0.15	0.23	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.32	0.20	0.25	-0.72	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
CS 30339-041	37	5478	100	2.10	0.26	0.36	-2.20	0.12	0.18	2.23	0.13	0.23	5.77	0.19	0.26	-0.41	0.21	0.30	1	1	5.67	0.11	0.17	0.29	0.15	0.24	7	7	3.20	0.17	0.25	-1.07	0.18	0.27	1	1	4.48	0.12	0.20	0.33	0.15	0.25	9	8	1.12	0.18	0.23	0.15	0.16	0.24	5	4	3.11	0.16	0.21	0.29	0.15	0.23	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.12	0.17	0.24	-0.34	0.16	0.24	3	3	2.64	0.15	0.21	-0.54	0.16	0.23	5	3	5.29	0.12	0.18	0.00	0.14	0.22	55	47	2.78	0.15	0.21	0.07	0.16	0.25	6	5	4.00	0.18	0.26	-0.04	0.17	0.25	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.91	0.21	0.31	0.14	0.19	0.29	3	2	-0.11	0.18	0.23	-0.14	0.17	0.24	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	0.04	0.21	0.27	0.12	0.19	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
CS 30343-063	40	4412	100	0.83	0.25	0.35	-2.95	0.12	0.18	2.26	0.11	0.21	4.75	0.22	0.28	-0.67	0.20	0.28	1	1	5.06	0.12	0.19	0.45	0.15	0.23	7	6	2.84	0.22	0.30	-0.66	0.21	0.29	1	1	3.63	0.11	0.20	0.24	0.14	0.24	9	8	0.19	0.16	0.21	-0.01	0.15	0.24	5	4	2.21	0.14	0.19	0.16	0.14	0.23	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.07	0.29	0.33	-0.63	0.25	0.30	3	3	1.78	0.20	0.24	-0.63	0.18	0.25	5	3	4.53	0.12	0.18	0.00	0.14	0.22	55	51	1.77	0.19	0.25	-0.17	0.17	0.26	6	5	3.45	0.08	0.38	0.17	0.15	0.37	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.05	0.21	0.28	-0.04	0.19	0.28	3	1	-0.79	0.18	0.22	-0.06	0.16	0.25	6	5	-0.11	0.17	0.22	0.27	0.16	0.25	3	1	-1.74	0.21	0.26	-0.90	0.19	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
CS 31060-047	30	4749	100	1.55	0.26	0.36	-2.72	0.12	0.18	2.00	0.13	0.23	5.41	0.20	0.27	-0.26	0.20	0.29	1	1	5.11	0.12	0.18	0.25	0.15	0.23	7	5	2.64	0.23	0.30	-1.11	0.23	0.31	1	1	3.76	0.12	0.20	0.12	0.15	0.25	9	5	0.53	0.17	0.22	0.08	0.16	0.25	5	4	2.46	0.16	0.21	0.16	0.15	0.23	17	13	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.53	0.18	0.27	-0.42	0.17	0.26	3	3	2.42	0.15	0.20	-0.25	0.15	0.23	5	3	4.78	0.12	0.18	0.00	0.14	0.22	55	43	2.32	0.16	0.23	0.12	0.16	0.25	6	5	3.78	0.23	0.33	0.25	0.22	0.30	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.11	0.22	0.31	-0.13	0.20	0.30	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.61	0.19	0.23	-1.02	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
CS 31062-041	37	4915	100	1.83	0.26	0.36	-2.67	0.14	0.19	1.84	0.13	0.23	6.20	0.20	0.26	0.49	0.19	0.29	1	1	5.23	0.12	0.19	0.33	0.16	0.25	5	5	2.94	0.16	0.25	-0.86	0.18	0.28	1	1	3.92	0.12	0.20	0.24	0.15	0.25	5	3	0.66	0.17	0.22	0.17	0.15	0.23	3	2	2.48	0.15	0.20	0.14	0.14	0.22	11	10	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	2.42	0.20	0.29	-0.57	0.19	0.28	1	1	2.08	0.15	0.22	-0.64	0.15	0.23	4	2	4.82	0.14	0.19	0.00	0.14	0.22	35	30	2.24	0.17	0.23	-0.00	0.15	0.25	4	4	3.49	0.21	0.30	-0.08	0.18	0.28	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	1	0	-0.10	0.23	0.33	-0.39	0.20	0.30	2	2	-0.95	0.19	0.24	-0.52	0.16	0.24	4	1	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.94	0.22	0.27	-0.39	0.18	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	7	0	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0
CS 31072-118	53	4606	100	1.25	0.24	0.34	-3.06	0.12	0.17	2.02	0.12	0.22	4.82	0.21	0.27	-0.50	0.19	0.28	1	1	4.84	0.12	0.19	0.33	0.14	0.23	7	6	2.59	0.14	0.25	-0.81	0.17	0.28	1	1	3.45	0.12	0.20	0.16	0.14	0.24	9	7	0.16	0.17	0.22	0.06	0.15	0.24	5	4	2.28	0.15	0.20	0.32	0.15	0.23	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.14	0.15	0.24	-0.47	0.15	0.25	3	3	1.62	0.14	0.22	-0.71	0.15	0.23	5	3	4.44	0.12	0.17	0.00	0.14	0.22	55	51	1.91	0.15	0.22	0.05	0.15	0.24	6	5	3.37	0.14	0.28	0.19	0.15	0.28	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.26	0.22	0.33	-0.17	0.20	0.32	3	2	-1.14	0.18	0.23	-0.32	0.16	0.24	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.97	0.18	0.22	-1.04	0.16	0.24	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
CS 31082-001	90	4922	100	1.90	0.23	0.33	-2.78	0.14	0.19	1.88	0.11	0.21	5.83	0.19	0.26	0.22	0.18	0.28	1	1	5.16	0.10	0.18	0.36	0.16	0.25	7	7	2.89	0.13	0.23	-0.80	0.15	0.26	1	1	3.91	0.11	0.20	0.33	0.15	0.25	9	8	0.51	0.17	0.23	0.12	0.14	0.23	5	5	2.49	0.15	0.20	0.25	0.14	0.22	17	16	1.24	0.15	0.19	0.02	0.15	0.23	3	2	2.53	0.15	0.23	-0.36	0.14	0.23	3	3	2.03	0.15	0.21	-0.58	0.14	0.23	5	3	4.72	0.14	0.19	0.00	0.14	0.22	55	54	2.32	0.15	0.22	0.18	0.14	0.24	6	6	3.60	0.16	0.27	0.13	0.15	0.25	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.72	0.15	0.22	0.53	0.14	0.24	3	2	0.02	0.18	0.23	0.56	0.15	0.23	6	6	0.71	0.17	0.22	0.89	0.14	0.23	3	2	0.53	0.14	0.19	1.18	0.14	0.22	2	2	-0.43	0.18	0.22	1.18	0.14	0.23	6	5	-0.14	0.18	0.24	1.06	0.15	0.25	10	8	0.02	0.18	0.23	1.30	0.15	0.23	9	9	-0.27	0.18	0.23	1.50	0.15	0.24	8	3	-0.61	0.18	0.22	1.66	0.15	0.23	4	4
HD 20	113	5445	100	2.39	0.22	0.32	-1.58	0.14	0.20	2.30	0.11	0.21	6.47	0.18	0.24	-0.34	0.17	0.27	1	1	6.17	0.11	0.18	0.17	0.15	0.24	7	6	4.07	0.12	0.23	-0.82	0.14	0.25	1	1	5.02	0.12	0.20	0.24	0.15	0.25	9	9	1.71	0.18	0.23	0.12	0.14	0.24	5	5	3.64	0.15	0.21	0.20	0.14	0.22	17	17	2.39	0.15	0.20	-0.03	0.14	0.23	3	3	3.87	0.17	0.26	-0.22	0.15	0.24	3	3	3.45	0.14	0.19	-0.36	0.14	0.23	5	5	5.92	0.14	0.20	0.00	0.14	0.22	55	54	3.42	0.15	0.22	0.08	0.14	0.24	6	6	4.58	0.18	0.28	-0.09	0.16	0.25	4	4	3.03	0.13	0.20	0.01	0.14	0.25	2	2	1.51	0.15	0.22	0.12	0.14	0.24	3	2	0.62	0.17	0.22	-0.04	0.14	0.23	6	6	1.40	0.17	0.22	0.38	0.14	0.24	3	2	0.86	0.15	0.20	0.31	0.13	0.23	2	2	-0.08	0.17	0.22	0.33	0.14	0.24	6	5	0.25	0.18	0.24	0.25	0.14	0.26	10	5	0.26	0.18	0.23	0.34	0.14	0.24	9	8	0.01	0.18	0.23	0.58	0.14	0.25	8	2	-0.27	0.18	0.23	0.80	0.14	0.24	4	4
HD 221170	51	4648	100	1.57	0.24	0.34	-2.14	0.15	0.20	2.22	0.11	0.21	5.68	0.22	0.27	-0.55	0.17	0.26	1	1	5.72	0.11	0.18	0.30	0.16	0.24	7	5	3.94	0.13	0.23	-0.37	0.16	0.26	1	1	4.48	0.12	0.21	0.27	0.15	0.25	9	9	1.24	0.17	0.22	0.22	0.14	0.23	5	5	3.10	0.16	0.22	0.24	0.14	0.23	17	17	1.93	0.17	0.21	0.08	0.14	0.22	3	3	3.29	0.22	0.30	-0.23	0.17	0.26	3	3	3.03	0.15	0.20	-0.20	0.14	0.23	5	5	5.35	0.15	0.20	0.00	0.14	0.22	55	53	3.05	0.18	0.27	0.29	0.15	0.25	6	6	3.94	0.19	0.29	-0.16	0.17	0.26	4	4	2.61	0.13	0.20	0.16	0.15	0.25	2	2	0.77	0.15	0.22	-0.05	0.15	0.24	3	1	0.04	0.18	0.23	-0.04	0.14	0.24	6	6	0.80	0.17	0.22	0.35	0.14	0.24	3	2	0.35	0.15	0.20	0.38	0.15	0.23	2	1	-0.60	0.17	0.22	0.39	0.14	0.24	6	5	-0.25	0.17	0.24	0.32	0.14	0.26	10	5	-0.16	0.18	0.23	0.49	0.14	0.24	9	7	-0.47	0.18	0.23	0.67	0.14	0.24	8	1	-0.80	0.17	0.22	0.85	0.14	0.24	4	4
HE 0005-0002	67	4726	100	1.58	0.25	0.35	-3.09	0.11	0.17	1.82	0.11	0.21	5.50	0.20	0.27	0.17	0.20	0.29	1	1	4.93	0.11	0.18	0.42	0.15	0.23	7	7	2.97	0.15	0.26	-0.43	0.18	0.27	1	1	3.65	0.11	0.20	0.36	0.14	0.24	9	8	0.20	0.17	0.22	0.09	0.16	0.25	5	4	2.13	0.16	0.21	0.18	0.16	0.24	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.92	0.16	0.22	-0.68	0.16	0.24	3	3	2.00	0.16	0.35	-0.33	0.24	0.37	5	3	4.44	0.11	0.17	0.00	0.14	0.22	55	53	2.03	0.15	0.22	0.17	0.16	0.25	6	6	3.26	0.18	0.28	0.08	0.18	0.28	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.10	0.18	0.27	0.19	0.18	0.28	3	2	-0.78	0.18	0.23	0.04	0.17	0.26	6	6	-0.02	0.18	0.22	0.45	0.17	0.26	3	2	-0.91	0.21	0.28	0.02	0.20	0.28	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0008-3842	67	4327	100	0.65	0.23	0.33	-3.35	0.11	0.18	2.39	0.12	0.22	4.17	0.21	0.28	-0.89	0.22	0.30	1	1	4.58	0.13	0.19	0.33	0.15	0.24	7	5	2.30	0.17	0.26	-0.84	0.19	0.27	1	1	2.98	0.12	0.20	-0.05	0.15	0.26	9	6	-0.15	0.15	0.20	0.01	0.15	0.24	5	4	1.66	0.15	0.20	-0.03	0.15	0.24	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.64	0.19	0.25	-0.70	0.19	0.26	3	3	1.22	0.11	0.24	-0.84	0.14	0.24	5	3	4.17	0.11	0.18	0.00	0.14	0.22	55	52	1.53	0.17	0.23	-0.06	0.18	0.26	6	6	2.75	0.27	0.32	-0.16	0.26	0.31	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-1.86	0.18	0.26	-1.50	0.18	0.27	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-2.95	0.18	0.22	-1.75	0.17	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0017-4838	42	5149	100	2.23	0.29	0.39	-3.23	0.13	0.18	1.81	0.14	0.24	4.87	0.25	0.31	-0.29	0.24	0.33	1	1	4.60	0.12	0.19	0.25	0.16	0.24	7	3	2.35	0.16	0.23	-0.89	0.17	0.26	1	1	3.40	0.12	0.20	0.27	0.15	0.25	9	3	0.17	0.18	0.23	0.23	0.16	0.25	5	3	2.15	0.17	0.22	0.36	0.15	0.24	17	8	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.06	0.16	0.21	-0.37	0.15	0.23	3	3	1.58	0.17	0.21	-0.58	0.16	0.23	5	3	4.27	0.13	0.18	0.00	0.14	0.22	55	34	2.01	0.15	0.22	0.32	0.15	0.25	6	4	3.18	0.18	0.24	0.17	0.17	0.24	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.42	0.22	0.31	0.68	0.20	0.30	3	2	-0.65	0.19	0.24	0.34	0.17	0.25	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.88	0.20	0.24	-0.78	0.17	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0018-1349	35	5719	100	4.62	0.26	0.36	-2.26	0.12	0.18	1.73	0.20	0.30	6.49	0.18	0.24	0.36	0.17	0.26	1	1	5.62	0.11	0.17	0.30	0.15	0.24	7	2	3.25	0.15	0.23	-0.95	0.17	0.26	1	1	4.32	0.12	0.20	0.23	0.14	0.25	9	6	0.95	0.18	0.23	0.05	0.18	0.28	5	2	2.96	0.15	0.20	0.21	0.16	0.26	17	7	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.32	0.15	0.22	-0.09	0.16	0.24	3	3	2.85	0.16	0.22	-0.28	0.17	0.25	5	3	5.23	0.12	0.18	0.00	0.14	0.22	55	38	2.90	0.16	0.22	0.25	0.16	0.26	6	3	4.00	0.17	0.24	0.01	0.18	0.25	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.65	0.18	0.25	-0.06	0.18	0.28	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	0.34	0.20	0.24	0.47	0.19	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0023-4825	42	5816	100	3.63	0.26	0.36	-2.06	0.12	0.18	1.45	0.14	0.24	6.64	0.17	0.23	0.31	0.17	0.26	1	1	5.74	0.11	0.17	0.22	0.15	0.23	7	4	3.40	0.16	0.24	-1.01	0.18	0.27	1	1	4.56	0.12	0.20	0.26	0.15	0.24	9	7	1.14	0.18	0.23	0.03	0.16	0.26	5	4	3.27	0.15	0.20	0.31	0.15	0.24	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.61	0.16	0.24	-0.00	0.16	0.25	3	3	2.88	0.16	0.21	-0.45	0.16	0.24	5	3	5.44	0.12	0.18	0.00	0.14	0.22	55	47	2.98	0.15	0.22	0.12	0.15	0.25	6	4	4.19	0.20	0.27	-0.01	0.19	0.27	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.89	0.19	0.27	-0.02	0.18	0.28	3	2	0.13	0.19	0.23	-0.05	0.17	0.26	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	0.01	0.22	0.27	-0.06	0.20	0.28	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0029-1839	70	5010	100	2.19	0.24	0.34	-2.50	0.12	0.18	1.67	0.12	0.22	6.21	0.19	0.25	0.31	0.18	0.27	1	1	5.08	0.12	0.18	-0.00	0.15	0.23	7	7	2.97	0.15	0.26	-1.00	0.17	0.27	1	1	3.97	0.12	0.20	0.11	0.14	0.24	9	7	0.28	0.17	0.22	-0.39	0.15	0.25	5	4	2.39	0.16	0.21	-0.13	0.15	0.24	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.04	0.16	0.27	-0.13	0.16	0.26	3	3	2.02	0.16	0.22	-0.87	0.15	0.23	5	3	5.00	0.12	0.18	0.00	0.14	0.22	55	53	2.39	0.16	0.22	-0.03	0.15	0.24	6	6	3.28	0.18	0.26	-0.47	0.17	0.25	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.50	0.16	0.25	0.03	0.16	0.25	3	2	-0.64	0.18	0.23	-0.38	0.16	0.25	6	3	0.23	0.18	0.22	0.13	0.16	0.25	3	1	-1.67	0.19	0.23	-1.30	0.16	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0037-2657	69	4982	100	2.21	0.26	0.36	-3.22	0.13	0.18	1.80	0.12	0.22	5.48	0.19	0.26	0.31	0.17	0.27	1	1	4.63	0.12	0.18	0.27	0.15	0.23	7	5	2.41	0.14	0.23	-0.84	0.15	0.25	1	1	3.46	0.12	0.20	0.32	0.15	0.25	9	7	0.08	0.18	0.23	0.13	0.16	0.24	5	4	2.02	0.16	0.21	0.22	0.15	0.23	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.06	0.16	0.22	-0.38	0.15	0.23	3	3	1.48	0.16	0.21	-0.69	0.15	0.23	5	3	4.28	0.13	0.18	0.00	0.14	0.22	55	44	1.94	0.16	0.22	0.24	0.15	0.24	6	5	3.00	0.16	0.23	-0.03	0.16	0.24	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.89	0.21	0.30	-0.64	0.19	0.29	3	2	-1.50	0.19	0.23	-0.52	0.16	0.25	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-2.18	0.19	0.23	-1.09	0.16	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0039-4154	70	4735	100	1.55	0.25	0.35	-3.38	0.11	0.17	2.01	0.12	0.22	4.89	0.20	0.27	-0.14	0.20	0.29	1	1	4.77	0.12	0.18	0.55	0.15	0.23	7	7	2.67	0.13	0.23	-0.44	0.15	0.26	1	1	3.23	0.11	0.20	0.23	0.15	0.25	9	7	0.04	0.17	0.22	0.23	0.16	0.25	5	4	1.79	0.16	0.21	0.13	0.15	0.24	17	13	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.70	0.15	0.21	-0.61	0.15	0.23	3	3	1.11	0.19	0.23	-0.92	0.18	0.26	5	3	4.14	0.11	0.17	0.00	0.14	0.22	55	47	1.87	0.16	0.22	0.31	0.16	0.25	6	6	2.84	0.16	0.23	-0.06	0.16	0.24	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.63	0.21	0.32	-0.24	0.20	0.31	3	2	-1.49	0.18	0.23	-0.38	0.17	0.26	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.18	0.19	0.26	0.05	0.18	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0043-2845	66	5517	100	4.42	0.25	0.35	-2.91	0.13	0.18	1.17	0.16	0.26	5.68	0.19	0.25	0.19	0.17	0.26	1	1	4.97	0.12	0.18	0.29	0.15	0.23	7	2	2.73	0.14	0.22	-0.83	0.16	0.25	1	1	3.65	0.12	0.20	0.20	0.14	0.24	9	6	0.33	0.18	0.23	0.06	0.16	0.26	5	2	2.36	0.16	0.21	0.24	0.15	0.25	17	8	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.66	0.14	0.20	-0.10	0.15	0.23	3	3	1.79	0.17	0.21	-0.70	0.15	0.24	5	3	4.59	0.13	0.18	0.00	0.14	0.22	55	37	2.37	0.16	0.22	0.36	0.15	0.25	6	4	3.35	0.16	0.21	0.00	0.16	0.23	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.71	0.19	0.25	-0.77	0.17	0.28	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0044-2459	62	5242	100	2.92	0.26	0.36	-3.28	0.13	0.18	1.55	0.14	0.24	5.56	0.19	0.26	0.45	0.18	0.27	1	1	4.65	0.11	0.20	0.34	0.17	0.26	7	4	2.30	0.14	0.22	-0.89	0.15	0.25	1	1	3.35	0.11	0.20	0.27	0.15	0.25	9	3	0.11	0.18	0.23	0.22	0.16	0.25	5	2	2.07	0.16	0.21	0.33	0.15	0.24	17	9	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.91	0.16	0.20	-0.48	0.15	0.23	3	3	1.12	0.17	0.21	-0.99	0.16	0.24	5	3	4.22	0.13	0.18	0.00	0.14	0.22	55	37	1.95	0.15	0.22	0.31	0.15	0.24	6	4	2.93	0.15	0.21	-0.04	0.15	0.22	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-1.96	0.19	0.25	-1.65	0.17	0.27	3	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0044-4023	39	5694	100	3.26	0.26	0.36	-2.56	0.13	0.18	1.49	0.14	0.24	6.23	0.18	0.24	0.40	0.17	0.27	1	1	5.26	0.12	0.18	0.24	0.15	0.23	7	2	2.86	0.15	0.23	-1.05	0.17	0.26	1	1	4.02	0.12	0.20	0.22	0.15	0.25	9	4	0.44	0.18	0.23	-0.17	0.16	0.25	5	2	2.63	0.14	0.20	0.17	0.15	0.23	17	6	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.88	0.17	0.22	-0.23	0.16	0.23	3	3	2.17	0.16	0.20	-0.66	0.15	0.23	5	3	4.94	0.13	0.18	0.00	0.14	0.22	55	37	2.50	0.16	0.22	0.14	0.15	0.25	6	3	3.54	0.22	0.26	-0.15	0.19	0.26	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.34	0.24	0.33	-0.06	0.21	0.31	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.78	0.20	0.24	-0.35	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0045-2430	59	5377	100	3.25	0.24	0.34	-1.77	0.12	0.18	1.67	0.12	0.22	6.54	0.18	0.24	-0.09	0.16	0.25	1	1	5.77	0.11	0.18	-0.04	0.14	0.23	7	6	3.61	0.14	0.23	-1.09	0.16	0.26	1	1	4.68	0.11	0.20	0.09	0.14	0.24	9	9	1.30	0.17	0.22	-0.10	0.16	0.26	5	5	3.29	0.16	0.21	0.04	0.15	0.25	17	17	2.16	0.16	0.20	-0.07	0.15	0.24	3	3	3.82	0.14	0.24	-0.09	0.16	0.24	3	3	3.37	0.14	0.19	-0.25	0.14	0.23	5	5	5.73	0.12	0.18	0.00	0.14	0.22	55	52	3.00	0.15	0.22	-0.15	0.15	0.25	6	6	4.00	0.17	0.26	-0.48	0.18	0.26	4	4	2.81	0.14	0.21	-0.02	0.14	0.26	2	1	0.46	0.20	0.30	-0.75	0.20	0.30	3	2	-0.13	0.18	0.23	-0.61	0.16	0.27	6	3	0.93	0.18	0.23	0.10	0.16	0.27	3	1	0.03	0.21	0.27	-0.34	0.20	0.28	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-0.93	0.18	0.23	0.33	0.15	0.27	4	3
HE 0049-5700	42	5952	100	4.08	0.26	0.36	-2.41	0.12	0.18	1.63	0.15	0.25	6.38	0.18	0.24	0.39	0.17	0.26	1	1	5.55	0.12	0.18	0.37	0.15	0.23	7	4	3.09	0.15	0.22	-0.98	0.16	0.25	1	1	4.33	0.12	0.20	0.37	0.14	0.25	9	7	0.89	0.18	0.23	0.12	0.16	0.26	5	2	2.95	0.16	0.21	0.33	0.15	0.24	17	7	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.08	0.15	0.21	-0.19	0.15	0.23	3	3	2.34	0.16	0.20	-0.66	0.15	0.24	5	3	5.10	0.12	0.18	0.00	0.14	0.22	55	37	2.59	0.16	0.22	0.07	0.16	0.25	6	1	3.62	0.12	0.18	-0.23	0.17	0.24	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.66	0.20	0.29	0.08	0.19	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.69	0.19	0.24	-0.42	0.17	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0051-2304	47	4537	100	1.22	0.25	0.35	-2.41	0.12	0.19	1.97	0.13	0.23	5.31	0.20	0.26	-0.64	0.20	0.28	1	1	5.45	0.11	0.19	0.30	0.15	0.24	7	5	3.33	0.17	0.26	-0.70	0.18	0.27	1	1	4.12	0.12	0.21	0.20	0.15	0.25	9	8	0.80	0.18	0.24	0.07	0.17	0.26	5	5	2.77	0.17	0.23	0.18	0.16	0.24	17	17	1.39	0.17	0.21	-0.18	0.17	0.24	3	3	2.72	0.48	0.56	-0.51	0.43	0.52	3	3	2.43	0.17	0.22	-0.52	0.17	0.24	5	5	5.06	0.12	0.19	0.00	0.14	0.22	55	53	2.42	0.20	0.27	-0.07	0.19	0.27	6	6	3.63	0.24	0.34	-0.18	0.22	0.30	4	4	2.32	0.13	0.20	0.16	0.15	0.26	2	2	0.46	0.17	0.23	-0.07	0.17	0.25	3	1	-0.40	0.18	0.23	-0.20	0.16	0.26	6	6	0.35	0.17	0.22	0.19	0.16	0.26	3	2	-0.37	0.23	0.31	-0.07	0.20	0.29	2	1	-1.37	0.17	0.22	-0.10	0.16	0.26	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-1.00	0.18	0.23	-0.07	0.17	0.27	9	2	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.75	0.18	0.22	0.17	0.16	0.27	4	4
HE 0054-0657	32	5908	100	4.40	0.26	0.36	-2.00	0.11	0.18	1.56	0.18	0.28	6.68	0.17	0.23	0.29	0.17	0.26	1	1	5.81	0.11	0.17	0.23	0.15	0.24	7	3	3.67	0.15	0.24	-0.80	0.18	0.27	1	1	4.47	0.12	0.20	0.10	0.15	0.25	9	7	1.06	0.18	0.23	-0.11	0.18	0.28	5	2	3.17	0.16	0.21	0.15	0.17	0.26	17	7	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.69	0.16	0.24	0.01	0.17	0.25	3	3	3.00	0.15	0.21	-0.39	0.16	0.24	5	3	5.50	0.11	0.18	0.00	0.14	0.22	55	39	3.13	0.16	0.22	0.21	0.17	0.26	6	3	4.32	0.17	0.25	0.07	0.18	0.26	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.92	0.19	0.27	-0.05	0.19	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	0.05	0.20	0.25	-0.08	0.21	0.29	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0057-4541	75	5083	100	2.55	0.24	0.34	-2.32	0.11	0.18	1.67	0.12	0.22	6.26	0.21	0.26	0.17	0.19	0.27	1	1	5.53	0.12	0.18	0.25	0.14	0.23	7	5	3.31	0.13	0.24	-0.85	0.16	0.25	1	1	4.30	0.11	0.20	0.24	0.14	0.24	9	9	0.93	0.18	0.23	0.07	0.16	0.26	5	5	2.87	0.16	0.21	0.16	0.15	0.24	17	17	1.66	0.16	0.20	-0.03	0.15	0.24	3	3	3.08	0.17	0.26	-0.28	0.17	0.25	3	3	2.75	0.15	0.20	-0.33	0.15	0.23	5	5	5.19	0.11	0.18	0.00	0.14	0.22	55	53	2.70	0.16	0.23	0.09	0.16	0.25	6	6	3.77	0.16	0.26	-0.17	0.17	0.25	4	4	2.43	0.14	0.21	0.14	0.14	0.26	2	1	0.72	0.14	0.23	0.06	0.15	0.24	3	2	-0.14	0.19	0.24	-0.07	0.16	0.27	6	6	0.64	0.18	0.22	0.35	0.15	0.26	3	2	-0.29	0.20	0.28	-0.11	0.19	0.28	2	1	-0.91	0.18	0.23	0.22	0.15	0.27	6	4	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-0.53	0.18	0.23	0.28	0.16	0.26	9	2	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.17	0.18	0.23	0.62	0.15	0.27	4	4
HE 0104-4007	48	5154	100	2.64	0.26	0.36	-3.30	0.13	0.18	1.72	0.14	0.24	5.59	0.19	0.26	0.50	0.18	0.28	1	1	4.49	0.11	0.20	0.21	0.16	0.25	7	3	2.14	0.15	0.22	-1.03	0.16	0.25	1	1	3.41	0.12	0.20	0.36	0.15	0.25	9	3	0.17	0.18	0.23	0.31	0.16	0.24	5	4	2.11	0.15	0.21	0.40	0.15	0.23	17	10	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.93	0.16	0.21	-0.44	0.15	0.23	3	2	1.43	0.17	0.21	-0.66	0.15	0.23	5	3	4.20	0.13	0.18	0.00	0.14	0.22	55	35	2.02	0.16	0.22	0.40	0.15	0.24	6	4	3.02	0.17	0.23	0.07	0.16	0.23	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-1.31	0.20	0.26	-0.98	0.17	0.27	3	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.81	0.19	0.24	-0.64	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0104-5300	52	4732	100	1.43	0.27	0.37	-3.42	0.11	0.19	1.99	0.13	0.23	5.07	0.20	0.28	-0.01	0.27	0.34	1	1	4.52	0.13	0.19	0.25	0.19	0.27	7	5	2.31	0.16	0.24	-0.85	0.21	0.29	1	1	3.27	0.12	0.20	0.22	0.18	0.27	9	4	-0.20	0.17	0.22	-0.06	0.23	0.31	5	4	1.90	0.16	0.21	0.18	0.21	0.29	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.83	0.16	0.22	-0.53	0.21	0.27	3	3	1.13	0.16	0.21	-0.95	0.22	0.29	5	3	4.19	0.11	0.19	0.00	0.14	0.22	55	42	1.74	0.16	0.22	0.12	0.22	0.30	6	5	3.07	0.18	0.26	0.13	0.22	0.28	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.93	0.20	0.30	-0.60	0.24	0.32	3	2	-1.32	0.18	0.23	-0.25	0.23	0.31	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-2.70	0.19	0.23	-1.52	0.25	0.33	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0105-6141	66	5218	100	2.83	0.24	0.34	-2.55	0.13	0.18	1.66	0.13	0.23	6.04	0.20	0.25	0.20	0.17	0.26	1	1	5.36	0.12	0.18	0.33	0.15	0.23	7	7	3.26	0.14	0.24	-0.67	0.16	0.26	1	1	4.14	0.12	0.20	0.33	0.14	0.24	9	8	0.83	0.18	0.23	0.20	0.16	0.25	5	4	2.78	0.16	0.22	0.31	0.15	0.24	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.91	0.17	0.25	-0.22	0.16	0.25	3	3	2.34	0.16	0.22	-0.50	0.16	0.23	5	3	4.95	0.13	0.18	0.00	0.14	0.22	55	52	2.55	0.16	0.22	0.18	0.15	0.24	6	6	3.62	0.17	0.26	-0.08	0.17	0.26	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.40	0.18	0.27	-0.03	0.17	0.28	3	2	-0.49	0.19	0.24	-0.18	0.16	0.26	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.24	0.21	0.27	0.17	0.19	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.36	0.18	0.23	0.68	0.16	0.26	4	3
HE 0109-0742	44	5315	100	1.85	0.26	0.36	-2.53	0.12	0.18	2.19	0.13	0.23	5.72	0.19	0.26	-0.14	0.20	0.30	1	1	5.36	0.12	0.18	0.30	0.15	0.23	7	5	3.01	0.17	0.25	-0.94	0.18	0.27	1	1	4.07	0.12	0.20	0.23	0.15	0.25	9	8	0.68	0.18	0.23	0.03	0.16	0.24	5	4	2.71	0.29	0.37	0.21	0.25	0.35	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.90	0.17	0.24	-0.24	0.16	0.24	3	3	2.23	0.15	0.20	-0.64	0.15	0.23	5	3	4.98	0.12	0.18	0.00	0.14	0.22	55	47	2.52	0.15	0.21	0.12	0.15	0.25	6	5	3.58	0.18	0.24	-0.15	0.16	0.24	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.42	0.23	0.32	-0.03	0.21	0.30	3	2	-0.67	0.18	0.23	-0.39	0.17	0.25	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.56	0.22	0.28	-0.16	0.20	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0109-3711	17	6156	100	3.91	0.30	0.40	-1.91	0.13	0.18	1.60	0.18	0.28	6.79	0.18	0.26	0.31	0.20	0.29	1	1	-9.99	0.00	0.00	-9.99	0.00	0.00	7	0	-9.99	0.00	0.00	-9.99	0.00	0.00	1	0	4.87	0.12	0.20	0.42	0.15	0.25	9	1	1.38	0.18	0.23	0.12	0.17	0.26	5	1	3.49	0.16	0.22	0.38	0.16	0.24	17	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.70	0.20	0.26	-0.06	0.19	0.26	3	1	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	5.59	0.13	0.18	0.00	0.14	0.22	55	14	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0111-1454	82	4632	100	1.05	0.24	0.34	-2.99	0.13	0.18	2.36	0.11	0.21	5.18	0.20	0.27	-0.22	0.19	0.28	1	1	4.94	0.12	0.18	0.35	0.15	0.23	7	6	2.94	0.13	0.24	-0.54	0.17	0.27	1	1	3.53	0.12	0.20	0.16	0.15	0.25	9	8	0.21	0.16	0.21	0.04	0.15	0.23	5	5	2.26	0.14	0.19	0.24	0.14	0.22	17	17	1.03	0.15	0.19	0.02	0.15	0.23	3	2	2.40	0.12	0.22	-0.27	0.14	0.24	3	3	2.19	0.13	0.20	-0.21	0.14	0.23	5	5	4.51	0.13	0.18	0.00	0.14	0.22	55	54	2.06	0.14	0.22	0.14	0.15	0.24	6	6	3.40	0.14	0.26	0.14	0.15	0.26	4	4	2.29	0.13	0.20	0.68	0.14	0.24	2	2	-0.15	0.20	0.31	-0.13	0.19	0.30	3	1	-1.07	0.18	0.22	-0.31	0.15	0.24	6	4	-0.22	0.18	0.22	0.17	0.15	0.24	3	1	-1.56	0.18	0.23	-0.69	0.16	0.23	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-2.54	0.18	0.23	-0.06	0.15	0.24	4	1
HE 0121-2826	46	4955	100	1.99	0.26	0.36	-2.97	0.12	0.18	1.68	0.12	0.22	5.97	0.20	0.27	0.54	0.19	0.28	1	1	5.04	0.11	0.19	0.43	0.15	0.24	7	6	2.64	0.16	0.25	-0.87	0.18	0.27	1	1	3.75	0.12	0.20	0.36	0.15	0.25	9	8	0.24	0.18	0.23	0.04	0.16	0.25	5	4	2.31	0.16	0.21	0.25	0.15	0.23	17	13	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.44	0.16	0.24	-0.26	0.16	0.24	3	3	1.73	0.16	0.22	-0.70	0.16	0.23	5	3	4.53	0.12	0.18	0.00	0.14	0.22	55	45	2.15	0.16	0.22	0.19	0.15	0.25	6	6	3.13	0.17	0.25	-0.16	0.17	0.24	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.27	0.18	0.27	0.27	0.17	0.27	3	2	-0.66	0.19	0.23	0.06	0.17	0.25	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.39	0.20	0.24	-0.56	0.18	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0131-2740	28	5351	100	3.03	0.28	0.38	-3.08	0.13	0.18	1.62	0.15	0.25	5.66	0.19	0.26	0.35	0.18	0.27	1	1	4.87	0.12	0.19	0.37	0.16	0.25	7	3	2.70	0.18	0.24	-0.69	0.18	0.27	1	1	3.61	0.12	0.20	0.33	0.15	0.25	9	1	0.26	0.18	0.23	0.16	0.17	0.25	5	1	2.21	0.15	0.21	0.27	0.15	0.24	17	4	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.31	0.17	0.22	-0.28	0.15	0.23	3	3	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	4.42	0.13	0.18	0.00	0.14	0.22	55	19	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	3.27	0.19	0.24	0.10	0.18	0.25	4	1	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0131-3953	52	5928	100	3.83	0.29	0.39	-2.71	0.11	0.17	1.06	0.15	0.25	8.16	0.16	0.24	2.45	0.18	0.27	1	1	5.21	0.12	0.18	0.30	0.15	0.24	5	2	2.84	0.14	0.21	-0.96	0.16	0.26	1	1	4.05	0.12	0.20	0.37	0.15	0.25	5	3	1.08	0.19	0.24	0.59	0.19	0.27	3	1	2.47	0.16	0.22	0.13	0.17	0.26	11	5	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	2.78	0.16	0.21	-0.21	0.17	0.24	1	1	2.18	0.16	0.20	-0.53	0.17	0.25	4	2	4.82	0.11	0.17	0.00	0.14	0.22	35	22	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0	3.29	0.16	0.20	-0.28	0.17	0.24	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	0.75	0.18	0.27	0.46	0.18	0.28	2	2	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	1.66	0.13	0.18	2.20	0.16	0.23	2	2	0.43	0.18	0.23	1.94	0.19	0.27	3	2	0.83	0.19	0.26	1.93	0.19	0.29	7	1	0.58	0.19	0.24	1.76	0.20	0.28	5	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-0.55	0.19	0.24	1.62	0.19	0.28	3	2
HE 0143-1135	43	5629	100	4.53	0.24	0.34	-2.13	0.12	0.18	1.42	0.16	0.26	6.49	0.19	0.24	0.23	0.17	0.26	1	1	5.78	0.12	0.18	0.33	0.14	0.24	7	4	3.70	0.12	0.23	-0.64	0.15	0.25	1	1	4.49	0.13	0.21	0.26	0.14	0.25	9	8	1.21	0.17	0.22	0.17	0.17	0.28	5	4	3.12	0.16	0.21	0.24	0.16	0.26	17	10	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.51	0.13	0.21	-0.02	0.15	0.23	3	3	3.07	0.15	0.20	-0.19	0.16	0.24	5	3	5.37	0.12	0.18	0.00	0.14	0.22	55	46	2.92	0.16	0.22	0.13	0.16	0.26	6	4	4.03	0.15	0.22	-0.09	0.17	0.24	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.64	0.15	0.22	-0.20	0.16	0.26	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.08	0.20	0.24	-0.07	0.19	0.29	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0143-4108	70	5121	100	2.41	0.24	0.34	-2.62	0.12	0.18	1.51	0.12	0.22	5.93	0.18	0.25	0.16	0.18	0.27	1	1	4.98	0.10	0.18	0.02	0.15	0.24	7	7	2.75	0.15	0.23	-1.10	0.16	0.26	1	1	3.75	0.12	0.20	0.00	0.14	0.25	9	8	0.45	0.17	0.22	-0.10	0.15	0.25	5	3	2.69	0.16	0.21	0.28	0.15	0.23	17	15	1.52	0.15	0.20	0.14	0.15	0.24	3	2	2.95	0.17	0.27	-0.10	0.16	0.26	3	3	2.83	0.13	0.19	0.06	0.14	0.23	5	4	4.88	0.12	0.18	0.00	0.14	0.22	55	54	2.51	0.16	0.22	0.21	0.15	0.24	6	6	3.87	0.16	0.28	0.23	0.17	0.27	4	4	2.72	0.13	0.20	0.74	0.14	0.25	2	2	-0.59	0.22	0.31	-0.94	0.20	0.30	3	2	-1.30	0.18	0.23	-0.92	0.16	0.25	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	-1.67	0.19	0.23	-1.18	0.16	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0143-4146	45	4799	100	1.50	0.26	0.36	-2.94	0.13	0.18	2.03	0.13	0.23	5.55	0.20	0.27	0.11	0.19	0.28	1	1	5.04	0.12	0.19	0.41	0.15	0.23	7	7	2.92	0.19	0.29	-0.61	0.21	0.30	1	1	3.67	0.12	0.20	0.25	0.15	0.25	9	7	0.60	0.18	0.23	0.38	0.16	0.25	5	5	2.43	0.16	0.21	0.36	0.15	0.23	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.52	0.17	0.26	-0.20	0.16	0.26	3	3	2.31	0.14	0.22	-0.13	0.15	0.24	5	3	4.55	0.13	0.18	0.00	0.14	0.22	55	49	2.26	0.16	0.22	0.28	0.15	0.24	6	6	3.34	0.20	0.29	0.03	0.19	0.28	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.60	0.23	0.34	-0.62	0.22	0.32	3	2	-1.37	0.19	0.23	-0.66	0.17	0.25	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.61	0.19	0.24	-0.79	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0157-3335	81	4775	100	1.62	0.24	0.34	-3.08	0.14	0.19	1.86	0.12	0.22	5.09	0.20	0.27	-0.22	0.18	0.29	1	1	4.90	0.11	0.18	0.40	0.16	0.24	7	7	2.85	0.14	0.25	-0.54	0.16	0.27	1	1	3.50	0.12	0.20	0.22	0.15	0.25	9	8	0.17	0.17	0.22	0.08	0.14	0.23	5	3	2.21	0.16	0.21	0.27	0.14	0.22	17	16	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.15	0.15	0.23	-0.44	0.14	0.23	3	3	1.40	0.16	0.21	-0.91	0.15	0.23	5	3	4.42	0.14	0.19	0.00	0.14	0.22	55	52	2.00	0.15	0.22	0.17	0.15	0.24	6	6	3.21	0.15	0.26	0.04	0.16	0.26	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.06	0.19	0.30	0.06	0.18	0.29	3	2	-0.96	0.17	0.21	-0.12	0.15	0.23	6	3	-0.16	0.18	0.22	0.33	0.15	0.24	3	1	-1.36	0.20	0.25	-0.41	0.16	0.24	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0200-0955	39	5216	100	2.57	0.26	0.36	-2.46	0.13	0.19	1.79	0.14	0.24	6.34	0.19	0.26	0.41	0.18	0.27	1	1	5.45	0.11	0.18	0.34	0.16	0.24	7	6	3.07	0.17	0.26	-0.93	0.18	0.27	1	1	4.19	0.12	0.20	0.30	0.15	0.25	9	8	0.75	0.14	0.20	0.04	0.15	0.23	5	4	2.73	0.16	0.21	0.17	0.15	0.23	17	14	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.02	0.19	0.27	-0.19	0.17	0.26	3	3	2.56	0.16	0.22	-0.36	0.16	0.23	5	3	5.03	0.13	0.19	0.00	0.14	0.22	55	48	2.62	0.16	0.23	0.16	0.15	0.24	6	5	3.58	0.20	0.27	-0.20	0.18	0.26	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.14	0.24	0.33	-0.36	0.22	0.31	3	2	-0.54	0.19	0.24	-0.32	0.17	0.26	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.02	0.21	0.25	-0.68	0.18	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0202-2204	82	5280	100	1.65	0.22	0.32	-1.98	0.14	0.19	2.47	0.12	0.22	7.57	0.17	0.24	1.16	0.17	0.28	1	1	5.59	0.13	0.19	-0.01	0.15	0.23	5	3	3.94	0.14	0.25	-0.55	0.16	0.27	1	1	4.64	0.12	0.20	0.26	0.15	0.25	5	5	1.15	0.16	0.22	-0.04	0.14	0.23	3	3	2.98	0.16	0.21	-0.06	0.14	0.22	11	10	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	3.29	0.18	0.27	-0.40	0.16	0.25	1	1	3.08	0.13	0.19	-0.33	0.15	0.23	4	4	5.52	0.14	0.19	0.00	0.14	0.22	35	34	2.97	0.14	0.21	0.03	0.15	0.24	4	4	4.31	0.19	0.28	0.04	0.16	0.25	4	4	2.65	0.17	0.23	0.03	0.16	0.26	1	1	1.56	0.16	0.23	0.57	0.15	0.24	2	1	0.67	0.18	0.24	0.41	0.15	0.23	4	4	1.09	0.17	0.22	0.47	0.15	0.23	2	1	1.55	0.16	0.20	1.41	0.14	0.22	2	2	0.55	0.18	0.30	1.36	0.25	0.34	3	3	0.90	0.20	0.27	1.30	0.16	0.26	7	7	0.54	0.18	0.23	1.02	0.15	0.23	5	5	0.06	0.18	0.23	1.03	0.15	0.24	6	4	-0.98	0.18	0.22	0.49	0.15	0.24	3	3
HE 0231-4016	39	5972	100	3.59	0.28	0.38	-2.08	0.13	0.18	1.67	0.15	0.25	7.67	0.16	0.23	1.36	0.17	0.27	1	1	5.72	0.11	0.17	0.22	0.15	0.24	7	4	3.30	0.17	0.24	-1.09	0.18	0.26	1	1	4.64	0.12	0.20	0.36	0.15	0.25	9	8	1.08	0.18	0.23	-0.01	0.17	0.25	5	3	3.19	0.16	0.22	0.25	0.15	0.24	17	9	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.48	0.17	0.24	-0.11	0.16	0.24	3	3	3.03	0.16	0.20	-0.28	0.16	0.23	5	3	5.42	0.13	0.18	0.00	0.14	0.22	55	42	2.72	0.16	0.22	-0.12	0.16	0.25	6	2	4.03	0.16	0.22	-0.14	0.17	0.24	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	1.56	0.15	0.23	0.67	0.16	0.25	3	2	0.88	0.16	0.22	0.72	0.16	0.23	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.52	0.16	0.21	1.47	0.16	0.23	2	2	0.31	0.23	0.27	1.22	0.20	0.28	6	3	1.03	0.18	0.25	1.53	0.17	0.27	10	1	0.77	0.19	0.24	1.35	0.17	0.26	9	2	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0240-0807	50	4729	100	1.54	0.24	0.34	-2.68	0.11	0.18	1.96	0.12	0.22	5.37	0.20	0.26	-0.35	0.20	0.29	1	1	5.20	0.12	0.18	0.30	0.15	0.23	7	6	3.05	0.16	0.26	-0.75	0.18	0.27	1	1	3.83	0.12	0.20	0.15	0.14	0.25	9	8	0.62	0.18	0.23	0.13	0.16	0.26	5	5	2.71	0.22	0.35	0.36	0.29	0.37	17	17	1.27	0.16	0.20	-0.06	0.16	0.24	3	2	2.64	0.18	0.28	-0.35	0.18	0.26	3	3	2.20	0.15	0.21	-0.51	0.16	0.24	5	3	4.82	0.11	0.18	0.00	0.14	0.22	55	51	2.27	0.15	0.23	0.03	0.16	0.25	6	5	3.92	0.20	0.32	0.35	0.20	0.29	4	4	2.17	0.14	0.21	0.24	0.15	0.26	2	1	0.20	0.21	0.30	-0.10	0.20	0.29	3	1	-0.56	0.17	0.22	-0.13	0.16	0.25	6	5	0.25	0.17	0.22	0.33	0.16	0.26	3	2	-0.34	0.29	0.34	0.21	0.25	0.33	2	1	-1.28	0.18	0.22	0.23	0.16	0.26	6	4	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-0.72	0.18	0.23	0.45	0.17	0.26	9	1	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.43	0.18	0.22	0.73	0.16	0.26	4	4
HE 0240-6105	73	4720	100	1.26	0.25	0.35	-3.23	0.12	0.18	2.15	0.12	0.22	4.91	0.19	0.27	-0.25	0.18	0.29	1	1	4.65	0.12	0.18	0.30	0.14	0.23	7	5	2.57	0.15	0.24	-0.67	0.16	0.27	1	1	3.29	0.11	0.19	0.17	0.15	0.25	9	7	0.05	0.17	0.22	0.11	0.15	0.24	5	4	2.12	0.15	0.20	0.33	0.15	0.23	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.00	0.15	0.21	-0.44	0.15	0.23	3	3	1.76	0.15	0.21	-0.40	0.15	0.23	5	3	4.27	0.12	0.18	0.00	0.14	0.22	55	52	1.97	0.15	0.22	0.28	0.15	0.24	6	6	3.23	0.17	0.27	0.21	0.16	0.27	4	3	2.16	0.14	0.20	0.80	0.15	0.25	2	1	0.10	0.20	0.29	0.36	0.18	0.29	3	2	-0.85	0.17	0.22	0.14	0.16	0.24	6	4	-0.05	0.17	0.22	0.58	0.16	0.24	3	2	-1.78	0.20	0.24	-0.68	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0243-0753	71	5066	100	2.29	0.24	0.34	-2.49	0.14	0.19	1.77	0.12	0.22	6.19	0.20	0.26	0.29	0.17	0.27	1	1	5.31	0.11	0.18	0.23	0.15	0.24	7	6	3.51	0.13	0.24	-0.47	0.16	0.26	1	1	4.10	0.12	0.20	0.23	0.15	0.25	9	8	0.87	0.19	0.24	0.19	0.15	0.24	5	5	2.79	0.16	0.21	0.26	0.14	0.23	17	17	1.58	0.15	0.20	0.07	0.15	0.23	3	3	2.99	0.17	0.27	-0.19	0.16	0.26	3	3	2.66	0.14	0.19	-0.24	0.14	0.23	5	5	5.01	0.14	0.19	0.00	0.14	0.22	55	54	2.69	0.16	0.23	0.26	0.15	0.24	6	6	3.85	0.17	0.28	0.09	0.16	0.27	4	4	2.38	0.14	0.21	0.27	0.14	0.25	2	1	0.10	0.21	0.32	-0.38	0.19	0.30	3	2	-0.74	0.18	0.23	-0.48	0.15	0.24	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.38	0.18	0.22	-1.01	0.15	0.23	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0243-5238	60	5085	100	2.35	0.26	0.36	-3.04	0.12	0.18	1.64	0.13	0.23	5.75	0.19	0.26	0.40	0.18	0.28	1	1	4.87	0.11	0.18	0.33	0.15	0.24	7	6	2.40	0.14	0.22	-1.03	0.16	0.25	1	1	3.64	0.12	0.20	0.32	0.15	0.25	9	7	0.22	0.19	0.24	0.09	0.16	0.25	5	4	2.21	0.16	0.21	0.23	0.15	0.24	17	13	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.34	0.16	0.22	-0.29	0.15	0.23	3	3	1.61	0.17	0.21	-0.75	0.16	0.23	5	3	4.46	0.12	0.18	0.00	0.14	0.22	55	45	2.12	0.16	0.22	0.24	0.15	0.24	6	6	3.20	0.18	0.25	-0.01	0.17	0.25	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.11	0.22	0.33	-0.04	0.20	0.31	3	2	-0.92	0.19	0.23	-0.12	0.17	0.25	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.21	0.20	0.24	-0.31	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0244-4111	46	5624	100	3.39	0.26	0.36	-2.56	0.12	0.17	1.38	0.14	0.24	6.08	0.18	0.24	0.25	0.17	0.26	1	1	5.36	0.11	0.17	0.34	0.14	0.23	7	5	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	4.18	0.11	0.20	0.37	0.15	0.24	9	7	0.71	0.18	0.23	0.10	0.17	0.26	5	4	2.77	0.16	0.21	0.30	0.15	0.24	17	11	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.92	0.17	0.23	-0.19	0.16	0.24	3	3	2.26	0.16	0.20	-0.57	0.15	0.23	5	3	4.94	0.12	0.17	0.00	0.14	0.22	55	42	2.61	0.15	0.22	0.25	0.15	0.24	6	4	3.69	0.18	0.25	-0.00	0.18	0.26	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.26	0.22	0.31	-0.16	0.21	0.31	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.75	0.20	0.24	-0.32	0.18	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0248+0039	52	5199	100	2.57	0.25	0.35	-2.53	0.12	0.18	1.75	0.13	0.23	5.96	0.19	0.25	0.09	0.18	0.27	1	1	5.31	0.11	0.18	0.26	0.15	0.24	7	6	3.16	0.16	0.25	-0.78	0.17	0.26	1	1	4.10	0.12	0.20	0.27	0.14	0.24	9	8	0.78	0.18	0.23	0.14	0.16	0.25	5	4	2.73	0.16	0.22	0.24	0.15	0.24	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.76	0.17	0.25	-0.38	0.16	0.25	3	3	2.24	0.17	0.23	-0.62	0.16	0.24	5	3	4.97	0.12	0.18	0.00	0.14	0.22	55	53	2.52	0.16	0.22	0.13	0.15	0.25	6	6	3.51	0.19	0.26	-0.21	0.18	0.25	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.19	0.21	0.31	-0.25	0.20	0.30	3	2	-0.58	0.19	0.23	-0.29	0.17	0.25	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.66	0.21	0.26	-0.26	0.19	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0256-1109	16	5891	100	4.04	0.34	0.44	-2.73	0.13	0.18	1.69	0.24	0.34	6.33	0.19	0.26	0.67	0.19	0.28	1	1	5.32	0.13	0.19	0.47	0.16	0.24	7	1	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	3.89	0.13	0.20	0.25	0.16	0.25	9	1	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	-9.99	0.00	0.00	-9.99	0.00	0.00	17	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	4.77	0.13	0.18	0.00	0.15	0.22	54	5	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0300-0751	33	5280	100	2.97	0.26	0.36	-2.27	0.13	0.19	1.61	0.15	0.25	6.22	0.20	0.25	0.10	0.17	0.26	1	1	5.51	0.12	0.18	0.19	0.15	0.23	7	6	3.58	0.19	0.27	-0.62	0.20	0.29	1	1	4.40	0.13	0.21	0.30	0.15	0.24	9	8	1.07	0.18	0.23	0.17	0.17	0.26	5	4	3.06	0.17	0.22	0.30	0.16	0.25	17	13	1.90	0.17	0.21	0.17	0.16	0.25	3	1	3.12	0.19	0.28	-0.28	0.19	0.27	3	3	2.75	0.16	0.22	-0.37	0.16	0.24	5	3	5.23	0.13	0.19	0.00	0.14	0.22	55	47	2.85	0.17	0.23	0.20	0.16	0.25	6	5	3.95	0.20	0.30	-0.03	0.20	0.29	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.83	0.17	0.25	0.13	0.17	0.26	3	2	0.03	0.19	0.24	0.06	0.17	0.27	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.11	0.26	0.31	0.02	0.24	0.31	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-0.99	0.19	0.23	0.77	0.17	0.27	4	3
HE 0305-4520	56	4817	100	1.56	0.25	0.35	-2.91	0.13	0.18	2.02	0.13	0.23	5.80	0.19	0.26	0.33	0.18	0.28	1	1	4.87	0.13	0.18	0.20	0.14	0.23	7	6	2.79	0.23	0.28	-0.77	0.21	0.29	1	1	3.67	0.12	0.20	0.23	0.15	0.25	9	8	0.49	0.18	0.23	0.23	0.16	0.24	5	5	2.30	0.16	0.21	0.19	0.15	0.23	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.29	0.14	0.24	-0.47	0.15	0.24	3	3	1.88	0.16	0.22	-0.60	0.15	0.23	5	3	4.59	0.13	0.18	0.00	0.14	0.22	55	51	2.19	0.16	0.22	0.18	0.15	0.24	6	5	3.46	0.19	0.29	0.12	0.18	0.28	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.60	0.23	0.33	-0.66	0.21	0.31	3	2	-1.05	0.13	0.20	-0.38	0.17	0.25	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.20	0.21	0.27	0.59	0.19	0.27	2	1	-1.45	0.18	0.23	0.29	0.16	0.25	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0308-1154	34	4984	100	2.05	0.27	0.37	-2.82	0.13	0.18	1.69	0.14	0.24	5.95	0.21	0.27	0.38	0.19	0.28	1	1	5.38	0.12	0.19	0.62	0.15	0.23	7	6	3.17	0.24	0.31	-0.48	0.25	0.33	1	1	4.03	0.12	0.20	0.49	0.15	0.25	9	8	0.85	0.19	0.24	0.51	0.17	0.26	5	4	2.50	0.17	0.22	0.30	0.16	0.24	17	15	1.50	0.16	0.20	0.32	0.16	0.23	3	1	2.76	0.17	0.28	-0.09	0.17	0.28	3	3	1.87	0.17	0.22	-0.70	0.16	0.24	5	3	4.68	0.13	0.18	0.00	0.14	0.22	55	44	2.18	0.16	0.23	0.08	0.15	0.24	6	5	3.62	0.23	0.33	0.20	0.22	0.32	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-1.78	0.20	0.27	-1.93	0.18	0.28	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0315+0000	43	5013	100	2.11	0.26	0.36	-2.73	0.13	0.19	1.72	0.13	0.23	5.84	0.19	0.26	0.18	0.18	0.28	1	1	5.11	0.12	0.18	0.26	0.15	0.24	7	7	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	3.91	0.12	0.20	0.28	0.15	0.25	9	7	0.57	0.18	0.23	0.13	0.16	0.24	5	4	2.56	0.16	0.21	0.26	0.15	0.23	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.71	0.19	0.28	-0.23	0.18	0.27	3	2	2.02	0.17	0.22	-0.64	0.16	0.23	5	3	4.77	0.13	0.19	0.00	0.14	0.22	55	50	2.41	0.16	0.22	0.22	0.15	0.24	6	6	3.86	0.18	0.29	0.34	0.18	0.27	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.23	0.21	0.30	-0.01	0.19	0.28	3	2	-0.52	0.19	0.24	-0.03	0.16	0.25	6	3	0.31	0.19	0.24	0.44	0.17	0.26	3	1	-0.25	0.19	0.26	0.34	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.57	0.19	0.23	0.65	0.16	0.25	4	3
HE 0316+0214	35	4639	100	1.39	0.27	0.37	-3.13	0.11	0.17	1.98	0.14	0.24	4.54	0.23	0.29	-0.71	0.22	0.30	1	1	5.11	0.12	0.19	0.67	0.15	0.23	7	7	2.84	0.26	0.33	-0.49	0.27	0.34	1	1	3.45	0.12	0.20	0.22	0.15	0.25	9	6	0.44	0.18	0.23	0.40	0.17	0.26	5	5	2.07	0.14	0.20	0.19	0.15	0.23	17	13	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.13	0.17	0.26	-0.40	0.18	0.26	3	3	1.52	0.17	0.32	-0.73	0.21	0.33	5	3	4.36	0.11	0.17	0.00	0.14	0.22	55	45	1.87	0.16	0.22	0.09	0.16	0.25	6	5	3.42	0.23	0.32	0.31	0.22	0.31	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-1.65	0.21	0.28	-1.48	0.21	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-2.39	0.19	0.23	-1.38	0.19	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0317-4640	54	5872	100	4.10	0.24	0.34	-2.33	0.11	0.17	1.49	0.13	0.23	6.29	0.17	0.23	0.22	0.17	0.26	1	1	5.57	0.11	0.17	0.31	0.14	0.23	7	4	3.24	0.13	0.22	-0.91	0.16	0.25	1	1	4.33	0.11	0.20	0.30	0.14	0.25	9	8	0.85	0.17	0.23	0.01	0.17	0.27	5	2	2.94	0.14	0.20	0.24	0.15	0.24	17	8	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.07	0.15	0.21	-0.28	0.16	0.23	3	3	2.38	0.16	0.20	-0.69	0.16	0.24	5	2	5.18	0.11	0.17	0.00	0.14	0.22	55	42	2.74	0.15	0.21	0.14	0.16	0.25	6	4	3.84	0.16	0.22	-0.09	0.16	0.24	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.56	0.18	0.27	-0.09	0.18	0.28	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.38	0.19	0.23	-0.19	0.18	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0323-4529	41	5127	100	2.51	0.27	0.37	-3.15	0.13	0.18	1.62	0.14	0.24	5.63	0.19	0.26	0.38	0.18	0.28	1	1	4.82	0.12	0.19	0.38	0.16	0.24	7	4	2.52	0.17	0.24	-0.81	0.18	0.26	1	1	3.52	0.12	0.20	0.30	0.15	0.25	9	5	0.16	0.18	0.23	0.13	0.16	0.25	5	4	2.20	0.16	0.21	0.32	0.15	0.24	17	9	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.16	0.17	0.22	-0.37	0.16	0.23	3	3	1.47	0.17	0.21	-0.78	0.16	0.24	5	3	4.36	0.13	0.18	0.00	0.14	0.22	55	36	2.01	0.16	0.22	0.23	0.15	0.25	6	5	3.17	0.18	0.24	0.07	0.16	0.24	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.11	0.21	0.31	0.28	0.20	0.30	3	2	-0.72	0.19	0.24	0.18	0.17	0.26	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.71	0.23	0.28	0.30	0.20	0.28	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0328-1047	52	5301	100	3.03	0.24	0.34	-2.25	0.11	0.18	1.21	0.13	0.23	6.29	0.20	0.25	0.15	0.18	0.27	1	1	5.55	0.11	0.18	0.21	0.14	0.23	7	6	3.47	0.13	0.24	-0.76	0.17	0.26	1	1	4.34	0.12	0.20	0.23	0.14	0.24	9	8	1.02	0.19	0.24	0.09	0.17	0.27	5	4	3.03	0.16	0.21	0.26	0.16	0.25	17	15	1.79	0.16	0.20	0.03	0.16	0.25	3	1	3.28	0.16	0.26	-0.14	0.17	0.26	3	3	2.70	0.16	0.21	-0.45	0.16	0.24	5	3	5.26	0.11	0.18	0.00	0.14	0.22	55	52	2.88	0.16	0.23	0.21	0.16	0.25	6	6	4.03	0.14	0.27	0.02	0.17	0.27	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.74	0.14	0.23	0.01	0.16	0.25	3	2	-0.10	0.18	0.23	-0.09	0.17	0.27	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.18	0.23	0.29	-0.07	0.22	0.30	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.31	0.18	0.23	0.42	0.17	0.28	4	1
HE 0330-4004	42	5946	100	3.78	0.27	0.37	-2.20	0.12	0.17	1.53	0.14	0.24	6.28	0.18	0.24	0.08	0.19	0.28	1	1	5.63	0.12	0.18	0.25	0.15	0.23	7	4	3.29	0.16	0.23	-0.99	0.17	0.26	1	1	4.54	0.11	0.20	0.38	0.15	0.25	9	8	1.18	0.18	0.23	0.20	0.17	0.26	5	4	3.19	0.16	0.21	0.36	0.16	0.24	17	10	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.34	0.16	0.23	-0.14	0.16	0.24	3	3	2.47	0.15	0.20	-0.72	0.16	0.24	5	3	5.31	0.12	0.17	0.00	0.14	0.22	55	43	2.82	0.15	0.21	0.09	0.16	0.25	6	3	4.02	0.16	0.22	-0.03	0.17	0.24	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.72	0.21	0.30	-0.06	0.20	0.29	3	2	0.15	0.31	0.34	0.11	0.28	0.34	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.09	0.22	0.26	-0.03	0.20	0.28	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0330-4144	46	5961	100	4.20	0.24	0.34	-1.90	0.10	0.17	1.52	0.14	0.24	6.69	0.16	0.23	0.19	0.17	0.26	1	1	5.96	0.11	0.17	0.28	0.14	0.23	7	5	3.71	0.13	0.23	-0.87	0.17	0.26	1	1	4.68	0.11	0.20	0.22	0.14	0.24	9	7	1.44	0.15	0.21	0.16	0.16	0.27	5	3	3.42	0.15	0.20	0.30	0.16	0.25	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.61	0.15	0.22	-0.16	0.17	0.24	3	3	3.11	0.15	0.20	-0.39	0.16	0.24	5	3	5.61	0.10	0.17	0.00	0.14	0.22	55	50	3.09	0.16	0.22	0.06	0.17	0.26	6	4	4.20	0.14	0.22	-0.15	0.17	0.25	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	1.18	0.15	0.24	0.10	0.17	0.26	3	2	0.38	0.18	0.23	0.03	0.18	0.28	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	0.21	0.20	0.24	-0.03	0.20	0.28	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0331-4939	40	5206	100	2.60	0.28	0.38	-2.90	0.12	0.18	1.55	0.14	0.24	5.86	0.19	0.26	0.34	0.20	0.30	1	1	5.04	0.12	0.19	0.33	0.16	0.25	7	5	2.60	0.18	0.25	-1.00	0.19	0.27	1	1	3.66	0.12	0.20	0.18	0.15	0.25	9	6	0.43	0.18	0.23	0.14	0.17	0.26	5	4	2.38	0.16	0.21	0.24	0.16	0.24	17	11	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.33	0.17	0.23	-0.47	0.17	0.24	3	3	1.84	0.16	0.21	-0.68	0.16	0.24	5	3	4.63	0.12	0.18	0.00	0.14	0.22	55	41	2.31	0.16	0.22	0.27	0.17	0.26	6	5	3.36	0.19	0.25	-0.02	0.18	0.25	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.03	0.23	0.33	-0.07	0.21	0.30	3	2	-0.67	0.19	0.24	-0.04	0.18	0.26	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.67	0.20	0.24	-0.93	0.19	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0333-4001	46	5892	100	4.31	0.26	0.36	-2.64	0.12	0.17	1.30	0.14	0.24	6.06	0.17	0.24	0.32	0.17	0.26	1	1	5.31	0.11	0.17	0.37	0.15	0.23	7	3	2.94	0.11	0.20	-0.89	0.15	0.24	1	1	4.00	0.11	0.20	0.28	0.15	0.24	9	5	0.66	0.18	0.23	0.13	0.17	0.27	5	2	2.63	0.16	0.21	0.26	0.16	0.25	17	5	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.77	0.15	0.20	-0.26	0.15	0.23	3	3	2.07	0.16	0.20	-0.68	0.16	0.24	5	3	4.86	0.12	0.17	0.00	0.14	0.22	55	36	2.50	0.15	0.21	0.23	0.15	0.25	6	2	3.64	0.16	0.21	0.03	0.16	0.24	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.18	0.18	0.26	-0.14	0.18	0.28	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.67	0.19	0.23	-0.16	0.17	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0336-3829	41	5740	100	3.22	0.25	0.35	-2.75	0.13	0.18	1.48	0.15	0.25	5.87	0.16	0.27	0.23	0.22	0.32	1	1	5.17	0.12	0.18	0.35	0.15	0.24	7	3	2.60	0.15	0.22	-1.12	0.16	0.25	1	1	4.06	0.12	0.20	0.45	0.15	0.25	9	6	0.48	0.18	0.23	0.06	0.16	0.24	5	2	2.67	0.16	0.21	0.40	0.15	0.23	17	6	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.67	0.15	0.20	-0.25	0.15	0.23	3	3	2.03	0.16	0.20	-0.61	0.15	0.23	5	3	4.75	0.13	0.18	0.00	0.14	0.22	55	34	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	3.37	0.17	0.21	-0.13	0.16	0.23	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.07	0.25	0.33	-0.29	0.22	0.31	3	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.70	0.20	0.24	-0.08	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0337-5127	46	5247	100	2.86	0.25	0.35	-2.62	0.13	0.18	1.55	0.14	0.24	5.94	0.19	0.25	0.16	0.18	0.27	1	1	5.30	0.11	0.19	0.33	0.16	0.25	7	5	3.63	0.14	0.25	-0.23	0.17	0.27	1	1	4.08	0.13	0.21	0.33	0.14	0.25	9	8	0.67	0.18	0.23	0.11	0.16	0.26	5	4	2.67	0.17	0.22	0.26	0.15	0.24	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.83	0.17	0.25	-0.23	0.17	0.25	3	3	2.13	0.17	0.22	-0.65	0.16	0.24	5	3	4.89	0.13	0.18	0.00	0.14	0.22	55	46	2.54	0.17	0.23	0.23	0.16	0.25	6	6	3.55	0.18	0.26	-0.09	0.18	0.26	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.35	0.20	0.29	-0.01	0.19	0.29	3	2	-0.51	0.19	0.23	-0.14	0.17	0.26	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.50	0.21	0.27	-0.02	0.19	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.50	0.19	0.24	0.60	0.17	0.27	4	1
HE 0338-3945	47	6162	100	4.09	0.25	0.35	-2.41	0.13	0.18	1.33	0.14	0.24	8.05	0.15	0.23	2.07	0.16	0.27	1	1	5.56	0.11	0.17	0.39	0.15	0.24	5	1	3.37	0.15	0.22	-0.69	0.16	0.26	1	1	4.32	0.11	0.20	0.37	0.15	0.25	5	3	1.24	0.18	0.23	0.48	0.16	0.25	3	2	3.02	0.13	0.19	0.41	0.15	0.23	11	7	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	3.22	0.16	0.22	-0.04	0.16	0.24	1	1	2.50	0.15	0.20	-0.48	0.15	0.23	4	2	5.09	0.13	0.18	0.00	0.14	0.22	35	23	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0	3.76	0.16	0.21	-0.08	0.16	0.23	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	1	0	1.29	0.16	0.24	0.73	0.16	0.26	2	2	0.56	0.19	0.24	0.73	0.17	0.25	4	1	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	2.13	0.12	0.18	2.41	0.15	0.22	2	2	1.01	0.18	0.22	2.26	0.16	0.24	3	3	1.38	0.18	0.24	2.21	0.16	0.26	7	4	1.18	0.18	0.23	2.09	0.16	0.24	5	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-0.01	0.18	0.23	1.89	0.16	0.25	3	2
HE 0339-4027	55	5896	100	4.11	0.24	0.34	-1.81	0.11	0.18	1.48	0.14	0.24	6.76	0.17	0.23	0.18	0.16	0.25	1	1	6.07	0.11	0.17	0.31	0.14	0.23	7	4	3.97	0.11	0.22	-0.69	0.16	0.26	1	1	4.90	0.11	0.20	0.35	0.14	0.24	9	9	1.45	0.17	0.22	0.09	0.16	0.27	5	4	3.46	0.15	0.20	0.25	0.15	0.24	17	13	2.27	0.15	0.19	0.08	0.15	0.24	3	1	3.79	0.14	0.23	-0.06	0.16	0.24	3	3	3.24	0.15	0.20	-0.34	0.15	0.24	5	3	5.69	0.11	0.18	0.00	0.14	0.22	55	52	3.19	0.15	0.22	0.08	0.15	0.25	6	4	4.35	0.15	0.24	-0.08	0.17	0.26	4	3	2.92	0.14	0.21	0.13	0.15	0.26	2	1	1.33	0.13	0.22	0.18	0.15	0.25	3	2	0.44	0.18	0.22	0.01	0.16	0.27	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	0.22	0.20	0.25	-0.09	0.19	0.28	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0340-3430	49	5914	100	3.81	0.25	0.35	-1.95	0.12	0.18	1.59	0.14	0.24	6.50	0.17	0.23	0.06	0.17	0.26	1	1	5.82	0.11	0.18	0.19	0.15	0.23	7	4	3.52	0.15	0.24	-1.00	0.17	0.26	1	1	4.77	0.11	0.20	0.36	0.15	0.25	9	8	1.32	0.17	0.23	0.10	0.16	0.25	5	3	3.32	0.16	0.21	0.25	0.15	0.24	17	13	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.56	0.16	0.23	-0.16	0.16	0.24	3	3	2.94	0.16	0.21	-0.50	0.15	0.23	5	3	5.55	0.12	0.18	0.00	0.14	0.22	55	48	2.92	0.14	0.20	-0.05	0.15	0.24	6	4	4.04	0.25	0.29	-0.26	0.22	0.28	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.89	0.17	0.28	-0.13	0.17	0.28	3	2	-0.02	0.25	0.28	-0.31	0.21	0.29	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.04	0.20	0.25	-0.22	0.18	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0340-5355	59	4862	100	1.81	0.25	0.35	-2.89	0.13	0.18	1.87	0.12	0.22	5.40	0.20	0.26	-0.11	0.18	0.28	1	1	4.66	0.10	0.18	-0.04	0.15	0.24	7	4	2.33	0.15	0.23	-1.26	0.16	0.25	1	1	3.58	0.12	0.20	0.10	0.15	0.25	9	8	0.21	0.18	0.23	-0.08	0.16	0.25	5	4	2.07	0.16	0.21	-0.07	0.15	0.23	17	13	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.28	0.16	0.24	-0.51	0.15	0.24	3	3	1.63	0.16	0.22	-0.88	0.15	0.23	5	3	4.62	0.13	0.18	0.00	0.14	0.22	55	53	1.88	0.16	0.22	-0.16	0.15	0.24	6	6	2.55	0.18	0.22	-0.82	0.16	0.23	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.44	0.23	0.33	-0.53	0.20	0.31	3	2	-1.20	0.18	0.23	-0.56	0.16	0.25	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-2.16	0.19	0.23	-1.41	0.16	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0341-4024	79	6108	100	4.20	0.24	0.34	-1.82	0.12	0.17	1.41	0.13	0.23	6.83	0.15	0.22	0.27	0.16	0.25	1	1	5.95	0.11	0.17	0.19	0.14	0.23	7	4	-9.99	0.00	0.00	-9.99	0.00	0.00	1	1	4.79	0.11	0.20	0.26	0.14	0.24	9	9	1.41	0.17	0.22	0.07	0.16	0.25	5	4	3.45	0.15	0.20	0.26	0.15	0.24	17	14	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.80	0.14	0.22	-0.05	0.15	0.24	3	3	3.10	0.14	0.20	-0.47	0.15	0.23	5	3	5.68	0.12	0.17	0.00	0.14	0.22	55	53	3.11	0.14	0.21	0.02	0.15	0.24	6	4	4.24	0.15	0.22	-0.18	0.16	0.24	4	2	2.88	0.14	0.21	0.10	0.15	0.25	2	1	1.05	0.16	0.25	-0.09	0.16	0.26	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	0.23	0.19	0.24	-0.08	0.17	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-0.62	0.18	0.23	0.69	0.16	0.26	4	1
HE 0344+0139	42	6291	100	4.18	0.26	0.36	-1.81	0.12	0.18	1.45	0.15	0.25	7.00	0.16	0.23	0.41	0.17	0.26	1	1	5.90	0.11	0.17	0.12	0.15	0.23	7	3	3.41	0.15	0.22	-1.26	0.16	0.26	1	1	4.85	0.10	0.19	0.29	0.15	0.25	9	8	1.48	0.16	0.22	0.11	0.16	0.26	5	3	3.48	0.15	0.21	0.26	0.15	0.24	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.86	0.16	0.23	-0.01	0.16	0.24	3	3	3.20	0.14	0.20	-0.39	0.15	0.23	5	3	5.70	0.12	0.18	0.00	0.14	0.22	55	47	3.12	0.15	0.21	-0.00	0.15	0.25	6	2	4.41	0.19	0.25	-0.04	0.18	0.26	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	1.03	0.20	0.29	-0.14	0.19	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	0.19	0.19	0.24	-0.14	0.17	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0347-1819	59	5198	100	4.23	0.24	0.34	-2.78	0.14	0.19	1.61	0.15	0.25	5.65	0.23	0.28	0.03	0.18	0.26	1	1	5.23	0.14	0.19	0.42	0.14	0.24	7	3	3.26	0.12	0.22	-0.44	0.15	0.25	1	1	3.94	0.13	0.20	0.35	0.14	0.24	9	8	0.46	0.18	0.24	0.07	0.16	0.26	5	2	2.41	0.17	0.22	0.16	0.15	0.24	17	11	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.84	0.15	0.21	-0.06	0.15	0.23	3	3	2.10	0.18	0.22	-0.52	0.15	0.23	5	2	4.73	0.14	0.19	0.00	0.14	0.22	55	43	2.20	0.18	0.23	0.06	0.15	0.25	6	5	3.27	0.16	0.21	-0.21	0.15	0.23	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.02	0.19	0.25	-0.18	0.17	0.26	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.15	0.20	0.25	-0.51	0.16	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0353-6024	53	5320	100	3.15	0.27	0.37	-3.17	0.13	0.18	1.49	0.14	0.24	5.51	0.19	0.25	0.29	0.17	0.27	1	1	4.62	0.12	0.21	0.21	0.17	0.26	7	4	2.49	0.12	0.21	-0.81	0.16	0.26	1	1	3.30	0.12	0.20	0.11	0.15	0.25	9	3	0.28	0.18	0.23	0.27	0.16	0.25	5	2	2.11	0.16	0.22	0.25	0.15	0.24	17	9	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.07	0.16	0.21	-0.43	0.15	0.23	3	2	1.46	0.16	0.21	-0.76	0.15	0.23	5	3	4.33	0.13	0.18	0.00	0.14	0.22	55	37	2.24	0.15	0.21	0.49	0.15	0.24	6	5	3.25	0.17	0.23	0.17	0.16	0.24	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-1.48	0.19	0.26	-1.28	0.17	0.27	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0400-2917	61	5065	100	2.39	0.25	0.35	-2.88	0.12	0.18	1.67	0.13	0.23	5.66	0.19	0.26	0.15	0.18	0.27	1	1	4.68	0.11	0.18	-0.02	0.15	0.24	7	5	2.21	0.15	0.22	-1.38	0.16	0.25	1	1	3.50	0.12	0.20	0.02	0.14	0.25	9	7	0.18	0.18	0.23	-0.11	0.16	0.25	5	4	2.12	0.16	0.21	-0.02	0.15	0.24	17	11	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.34	0.16	0.23	-0.45	0.16	0.23	3	3	1.83	0.17	0.22	-0.68	0.15	0.23	5	3	4.62	0.12	0.18	0.00	0.14	0.22	55	49	2.03	0.16	0.22	-0.01	0.15	0.25	6	5	3.23	0.18	0.26	-0.14	0.17	0.25	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.78	0.22	0.30	-0.87	0.19	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.84	0.19	0.23	-1.10	0.16	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0401-0138	56	4866	100	1.76	0.27	0.37	-3.34	0.13	0.18	1.45	0.13	0.23	5.30	0.20	0.27	0.24	0.18	0.28	1	1	4.67	0.12	0.19	0.42	0.15	0.23	7	5	2.07	0.11	0.21	-1.06	0.15	0.25	1	1	3.37	0.12	0.20	0.35	0.15	0.25	9	6	-0.06	0.18	0.23	0.11	0.16	0.25	5	4	1.97	0.16	0.21	0.28	0.15	0.23	17	10	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.87	0.16	0.22	-0.46	0.15	0.23	3	3	1.25	0.15	0.20	-0.80	0.15	0.23	5	3	4.16	0.13	0.18	0.00	0.14	0.22	55	41	1.82	0.16	0.22	0.24	0.15	0.24	6	5	2.94	0.18	0.26	0.02	0.17	0.26	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.26	0.23	0.35	0.11	0.21	0.33	3	2	-1.05	0.19	0.23	0.05	0.17	0.25	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.41	0.20	0.25	-0.21	0.18	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0417-0821	62	5811	100	4.83	0.24	0.34	-2.33	0.12	0.17	1.40	0.14	0.24	6.31	0.18	0.23	0.25	0.16	0.25	1	1	5.49	0.12	0.18	0.24	0.14	0.24	7	3	3.39	0.11	0.21	-0.75	0.15	0.25	1	1	4.26	0.12	0.20	0.23	0.14	0.24	9	8	0.97	0.17	0.22	0.13	0.16	0.26	5	2	2.95	0.15	0.21	0.26	0.15	0.25	17	10	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.24	0.13	0.20	-0.10	0.15	0.23	3	3	2.69	0.16	0.20	-0.37	0.15	0.24	5	3	5.17	0.12	0.17	0.00	0.14	0.22	55	41	2.78	0.16	0.22	0.19	0.15	0.25	6	4	3.92	0.15	0.21	0.00	0.16	0.23	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.48	0.16	0.24	-0.16	0.17	0.27	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.56	0.18	0.23	-0.36	0.17	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0430-4404	49	6214	100	4.27	0.25	0.35	-2.07	0.11	0.17	1.41	0.14	0.24	7.75	0.15	0.22	1.44	0.16	0.26	1	1	5.79	0.11	0.17	0.29	0.15	0.23	7	3	3.42	0.14	0.22	-0.97	0.16	0.25	1	1	4.61	0.11	0.20	0.33	0.15	0.25	9	7	1.28	0.17	0.23	0.19	0.17	0.26	5	3	3.26	0.16	0.21	0.32	0.16	0.25	17	9	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.57	0.15	0.21	-0.02	0.16	0.23	3	3	2.84	0.15	0.20	-0.47	0.15	0.24	5	3	5.42	0.11	0.17	0.00	0.14	0.22	55	41	2.94	0.15	0.21	0.10	0.15	0.25	6	3	4.18	0.15	0.21	0.01	0.16	0.23	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	1.45	0.14	0.23	0.56	0.16	0.25	3	2	0.76	0.18	0.23	0.60	0.17	0.26	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.67	0.14	0.18	1.62	0.15	0.23	2	2	0.50	0.17	0.22	1.41	0.17	0.26	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0430-4901	50	5296	100	3.12	0.25	0.35	-2.72	0.12	0.18	1.32	0.13	0.23	5.76	0.19	0.25	0.09	0.18	0.27	1	1	5.03	0.11	0.19	0.17	0.16	0.24	7	5	2.57	0.15	0.22	-1.18	0.16	0.25	1	1	3.76	0.12	0.20	0.12	0.14	0.25	9	7	0.42	0.18	0.23	-0.03	0.16	0.26	5	4	2.43	0.16	0.21	0.13	0.16	0.25	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.62	0.17	0.24	-0.33	0.16	0.24	3	3	1.96	0.17	0.21	-0.71	0.16	0.24	5	3	4.78	0.12	0.18	0.00	0.14	0.22	55	46	2.25	0.16	0.22	0.04	0.15	0.25	6	5	3.50	0.17	0.22	-0.03	0.17	0.24	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.25	0.18	0.27	-0.01	0.18	0.28	3	2	-0.45	0.19	0.24	0.02	0.17	0.27	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.08	0.22	0.27	0.50	0.20	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.05	0.18	0.23	1.16	0.17	0.27	4	3
HE 0432-0923	74	5131	100	2.64	0.23	0.33	-3.19	0.13	0.18	1.54	0.12	0.22	5.44	0.18	0.25	0.24	0.17	0.27	1	1	4.73	0.11	0.18	0.34	0.16	0.24	7	5	2.32	0.14	0.22	-0.96	0.15	0.25	1	1	3.49	0.11	0.20	0.32	0.15	0.25	9	6	0.07	0.17	0.22	0.09	0.15	0.24	5	4	2.16	0.15	0.21	0.33	0.14	0.23	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.97	0.16	0.21	-0.51	0.15	0.23	3	3	1.47	0.21	0.24	-0.73	0.17	0.25	5	3	4.31	0.13	0.18	0.00	0.14	0.22	55	41	2.03	0.16	0.22	0.29	0.15	0.24	6	5	3.17	0.18	0.24	0.11	0.16	0.24	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.26	0.17	0.26	0.47	0.16	0.27	3	2	-0.44	0.18	0.22	0.51	0.15	0.24	6	3	0.29	0.18	0.22	0.88	0.15	0.25	3	1	-0.34	0.20	0.26	0.72	0.18	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.43	0.18	0.23	1.25	0.15	0.24	4	2
HE 0436-4008	40	5431	100	3.34	0.24	0.34	-2.35	0.12	0.18	1.30	0.14	0.24	6.53	0.19	0.25	0.49	0.17	0.26	1	1	5.45	0.15	0.20	0.22	0.15	0.24	7	5	2.94	0.18	0.25	-1.18	0.19	0.28	1	1	4.26	0.12	0.20	0.25	0.14	0.24	9	8	0.86	0.18	0.23	0.05	0.16	0.26	5	4	2.97	0.16	0.21	0.30	0.15	0.24	17	14	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.17	0.17	0.25	-0.15	0.17	0.25	3	3	2.63	0.16	0.21	-0.41	0.16	0.24	5	3	5.15	0.12	0.18	0.00	0.14	0.22	55	49	2.75	0.15	0.22	0.18	0.15	0.25	6	5	3.97	0.19	0.27	0.07	0.18	0.26	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.95	0.14	0.22	0.33	0.15	0.24	3	2	0.01	0.18	0.23	0.12	0.17	0.26	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.48	0.22	0.27	-0.26	0.20	0.28	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0441-4343	44	5629	100	3.59	0.25	0.35	-2.52	0.12	0.18	1.29	0.15	0.25	6.20	0.18	0.24	0.33	0.17	0.26	1	1	5.37	0.12	0.18	0.32	0.15	0.23	7	4	2.86	0.15	0.23	-1.09	0.17	0.26	1	1	4.02	0.11	0.20	0.18	0.15	0.24	9	7	0.78	0.18	0.24	0.13	0.17	0.26	5	4	2.77	0.16	0.21	0.27	0.15	0.24	17	9	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.78	0.16	0.22	-0.36	0.15	0.23	3	3	2.23	0.16	0.21	-0.63	0.16	0.24	5	3	4.98	0.12	0.18	0.00	0.14	0.22	55	40	2.74	0.16	0.22	0.34	0.15	0.25	6	3	3.79	0.18	0.25	0.07	0.17	0.25	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.34	0.21	0.30	-0.10	0.20	0.30	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.99	0.19	0.24	-0.59	0.17	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0442-1234	77	4604	100	1.34	0.24	0.34	-2.41	0.14	0.20	2.21	0.12	0.22	5.37	0.22	0.27	-0.61	0.18	0.27	1	1	5.48	0.11	0.18	0.32	0.15	0.24	7	5	3.72	0.14	0.24	-0.34	0.15	0.25	1	1	4.14	0.12	0.20	0.20	0.15	0.25	9	9	0.91	0.18	0.23	0.16	0.15	0.24	5	5	2.76	0.16	0.21	0.15	0.14	0.23	17	17	1.49	0.17	0.21	-0.09	0.15	0.23	3	3	2.74	0.21	0.30	-0.52	0.17	0.26	3	3	2.59	0.15	0.20	-0.39	0.14	0.23	5	5	5.09	0.14	0.20	0.00	0.14	0.22	55	54	2.54	0.17	0.24	0.03	0.15	0.24	6	6	3.82	0.25	0.34	-0.02	0.20	0.29	4	4	2.26	0.13	0.20	0.07	0.14	0.25	2	2	0.24	0.19	0.26	-0.32	0.16	0.25	3	1	-0.42	0.18	0.22	-0.24	0.14	0.24	6	6	0.27	0.17	0.22	0.08	0.14	0.24	3	2	-0.42	0.23	0.34	-0.13	0.20	0.30	2	1	-1.21	0.18	0.22	0.03	0.14	0.25	6	5	-0.85	0.18	0.24	-0.01	0.14	0.27	10	3	-0.80	0.18	0.23	0.11	0.14	0.25	9	6	-1.00	0.18	0.23	0.40	0.14	0.25	8	2	-1.38	0.17	0.22	0.52	0.14	0.25	4	4
HE 0447-4858	18	5995	100	3.86	0.27	0.37	-1.69	0.12	0.18	1.35	0.19	0.29	6.74	0.17	0.24	0.04	0.18	0.27	1	1	6.14	0.12	0.18	0.24	0.15	0.24	7	2	3.97	0.24	0.31	-0.81	0.25	0.32	1	1	4.91	0.12	0.20	0.24	0.15	0.25	9	2	1.67	0.18	0.23	0.19	0.18	0.28	5	2	3.62	0.17	0.22	0.28	0.17	0.26	17	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	4.07	0.21	0.28	0.09	0.22	0.28	3	2	3.39	0.14	0.20	-0.31	0.16	0.24	5	1	5.81	0.12	0.18	0.00	0.14	0.22	55	18	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	4.90	0.37	0.43	0.33	0.41	0.45	4	1	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	1.95	0.14	0.22	0.67	0.16	0.25	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	0.89	0.22	0.28	0.45	0.23	0.29	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0450-4705	48	5429	100	3.34	0.28	0.38	-3.10	0.13	0.18	1.49	0.15	0.25	6.14	0.18	0.25	0.84	0.17	0.27	1	1	4.70	0.12	0.21	0.22	0.17	0.26	7	4	2.51	0.14	0.26	-0.86	0.21	0.30	1	1	3.48	0.12	0.20	0.21	0.15	0.25	9	3	0.06	0.18	0.23	-0.01	0.17	0.26	5	1	2.16	0.15	0.20	0.24	0.15	0.24	17	7	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.34	0.16	0.21	-0.24	0.15	0.23	3	3	2.04	0.17	0.21	-0.25	0.16	0.23	5	2	4.40	0.13	0.18	0.00	0.14	0.22	55	34	2.13	0.16	0.22	0.31	0.15	0.25	6	4	3.52	0.16	0.23	0.36	0.16	0.24	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.61	0.21	0.29	-0.48	0.19	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0
HE 0454-4758	77	5388	100	3.33	0.25	0.35	-3.10	0.13	0.18	1.49	0.13	0.23	5.72	0.18	0.25	0.44	0.17	0.27	1	1	4.77	0.11	0.20	0.29	0.17	0.26	7	4	2.43	0.18	0.24	-0.94	0.16	0.26	1	1	3.54	0.11	0.20	0.28	0.15	0.25	9	6	0.18	0.18	0.23	0.11	0.16	0.25	5	2	2.24	0.16	0.21	0.32	0.15	0.24	17	10	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.22	0.17	0.21	-0.35	0.16	0.23	3	2	1.59	0.16	0.21	-0.70	0.15	0.23	5	3	4.40	0.13	0.18	0.00	0.14	0.22	55	39	2.15	0.15	0.21	0.33	0.15	0.24	6	5	3.22	0.16	0.21	0.07	0.15	0.23	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.49	0.20	0.28	-0.36	0.18	0.28	3	2	-0.97	0.19	0.24	-0.11	0.17	0.26	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.66	0.19	0.23	-0.69	0.16	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0501-5139	21	5861	100	3.54	0.26	0.36	-2.38	0.14	0.19	1.49	0.16	0.26	6.41	0.18	0.24	0.40	0.18	0.28	1	1	5.39	0.12	0.18	0.19	0.16	0.24	7	1	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	4.32	0.12	0.20	0.34	0.15	0.25	9	1	0.88	0.18	0.23	0.09	0.15	0.24	5	1	3.03	0.16	0.21	0.39	0.15	0.23	17	5	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.05	0.17	0.23	-0.24	0.16	0.24	3	2	2.44	0.16	0.21	-0.57	0.15	0.23	5	1	5.12	0.14	0.19	0.00	0.14	0.22	55	18	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	3.74	0.20	0.25	-0.13	0.19	0.26	4	1	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.46	0.26	0.35	-0.13	0.23	0.33	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0501-5644	41	5033	100	2.30	0.25	0.35	-2.41	0.12	0.19	1.76	0.13	0.23	6.26	0.20	0.26	0.27	0.19	0.27	1	1	5.47	0.12	0.18	0.29	0.15	0.23	7	6	3.33	0.18	0.27	-0.74	0.20	0.28	1	1	4.24	0.13	0.21	0.28	0.14	0.25	9	8	0.91	0.17	0.23	0.15	0.16	0.25	5	5	2.78	0.16	0.21	0.16	0.15	0.24	17	16	1.54	0.16	0.20	-0.06	0.16	0.24	3	1	3.06	0.19	0.29	-0.20	0.18	0.27	3	3	2.63	0.15	0.20	-0.36	0.15	0.23	5	3	5.10	0.12	0.19	0.00	0.14	0.22	55	52	2.60	0.16	0.23	0.08	0.16	0.25	6	6	3.59	0.21	0.30	-0.25	0.20	0.28	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.41	0.20	0.29	-0.16	0.20	0.29	3	1	-0.34	0.19	0.23	-0.17	0.17	0.26	6	3	0.64	0.18	0.23	0.44	0.16	0.26	3	1	-0.72	0.23	0.29	-0.45	0.21	0.29	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.59	0.18	0.23	0.30	0.16	0.26	4	3
HE 0512-3835	41	4948	100	2.01	0.25	0.35	-2.40	0.12	0.19	1.90	0.14	0.24	5.77	0.21	0.26	-0.22	0.21	0.29	1	1	5.52	0.12	0.19	0.33	0.15	0.24	7	5	3.63	0.18	0.27	-0.44	0.19	0.27	1	1	4.28	0.12	0.21	0.31	0.15	0.25	9	8	0.96	0.18	0.23	0.19	0.17	0.26	5	5	2.94	0.17	0.22	0.31	0.16	0.24	17	17	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.03	0.18	0.29	-0.25	0.18	0.26	3	3	2.65	0.14	0.20	-0.35	0.15	0.23	5	3	5.11	0.12	0.19	0.00	0.14	0.22	55	53	2.53	0.16	0.23	-0.00	0.16	0.25	6	6	3.52	0.21	0.30	-0.34	0.20	0.28	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.61	0.18	0.25	0.03	0.17	0.26	3	2	-0.40	0.19	0.23	-0.25	0.17	0.27	6	3	0.45	0.18	0.23	0.24	0.17	0.27	3	1	-0.37	0.23	0.30	-0.11	0.21	0.29	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.51	0.18	0.23	0.37	0.17	0.28	4	3
HE 0513-4557	19	5629	100	3.62	0.28	0.38	-2.79	0.13	0.18	1.44	0.20	0.30	5.99	0.18	0.25	0.39	0.18	0.27	1	1	5.13	0.12	0.18	0.34	0.15	0.24	7	1	-9.99	0.00	0.00	-9.99	0.00	0.00	1	0	3.78	0.12	0.20	0.21	0.15	0.25	9	1	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	-9.99	0.00	0.00	-9.99	0.00	0.00	17	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	4.71	0.13	0.18	0.00	0.14	0.22	55	10	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.19	0.23	0.32	0.01	0.21	0.30	3	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0516-3820	51	5342	100	3.05	0.24	0.34	-2.33	0.12	0.18	1.48	0.13	0.23	6.46	0.19	0.25	0.39	0.18	0.26	1	1	5.48	0.11	0.18	0.22	0.15	0.23	7	5	3.03	0.18	0.26	-1.12	0.20	0.28	1	1	4.28	0.11	0.20	0.24	0.14	0.24	9	8	0.92	0.18	0.23	0.07	0.16	0.26	5	4	2.92	0.15	0.20	0.22	0.15	0.24	17	15	1.70	0.16	0.20	0.03	0.16	0.24	3	1	3.26	0.16	0.26	-0.08	0.17	0.26	3	3	2.82	0.15	0.20	-0.25	0.15	0.23	5	4	5.18	0.12	0.18	0.00	0.14	0.22	55	54	2.70	0.17	0.23	0.10	0.16	0.25	6	6	3.80	0.19	0.27	-0.12	0.18	0.26	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.69	0.16	0.24	0.05	0.16	0.25	3	2	-0.08	0.19	0.23	0.00	0.17	0.26	6	3	0.69	0.19	0.23	0.41	0.17	0.27	3	1	-0.30	0.23	0.29	-0.11	0.21	0.29	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-0.22	0.19	0.24	0.60	0.17	0.27	9	1	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.15	0.18	0.23	0.67	0.16	0.27	4	3
HE 0517-1952	69	5254	100	1.99	0.25	0.35	-2.61	0.14	0.19	2.09	0.12	0.22	5.26	0.20	0.26	-0.52	0.19	0.29	1	1	5.17	0.12	0.18	0.20	0.15	0.24	7	7	3.01	0.16	0.24	-0.84	0.16	0.26	1	1	4.01	0.11	0.19	0.27	0.15	0.25	9	8	0.66	0.18	0.23	0.10	0.15	0.23	5	5	2.65	0.17	0.22	0.24	0.15	0.23	17	15	1.39	0.15	0.20	0.00	0.15	0.23	3	1	2.66	0.18	0.23	-0.40	0.15	0.23	3	3	2.14	0.16	0.21	-0.64	0.15	0.23	5	3	4.89	0.14	0.19	0.00	0.14	0.22	55	52	2.44	0.15	0.22	0.13	0.15	0.24	6	6	3.59	0.15	0.23	-0.05	0.15	0.24	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.33	0.22	0.33	-0.03	0.19	0.30	3	2	-0.64	0.18	0.23	-0.27	0.15	0.23	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.86	0.21	0.25	-0.38	0.17	0.24	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0519-5525	26	5580	100	3.48	0.27	0.37	-2.52	0.12	0.18	1.45	0.16	0.26	6.16	0.18	0.25	0.29	0.17	0.26	1	1	5.47	0.12	0.18	0.41	0.15	0.23	7	1	3.20	0.18	0.26	-0.76	0.20	0.28	1	1	4.21	0.12	0.20	0.37	0.15	0.24	9	3	0.74	0.19	0.24	0.08	0.17	0.26	5	1	2.87	0.17	0.22	0.37	0.16	0.24	17	5	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.96	0.18	0.24	-0.19	0.17	0.25	3	3	2.34	0.17	0.22	-0.53	0.16	0.24	5	2	4.98	0.12	0.18	0.00	0.14	0.22	55	29	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	3.86	0.23	0.30	0.13	0.22	0.30	4	1	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.64	0.20	0.29	0.18	0.19	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.58	0.20	0.25	-0.20	0.19	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0520-1748	72	5272	100	3.06	0.24	0.34	-2.52	0.12	0.18	1.46	0.12	0.22	6.32	0.19	0.25	0.45	0.17	0.26	1	1	5.30	0.11	0.18	0.24	0.15	0.23	7	6	2.88	0.14	0.23	-1.07	0.16	0.25	1	1	4.10	0.12	0.20	0.26	0.14	0.24	9	8	0.70	0.18	0.23	0.05	0.16	0.26	5	4	2.75	0.16	0.21	0.26	0.15	0.24	17	16	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.06	0.15	0.24	-0.09	0.16	0.25	3	3	2.66	0.12	0.20	-0.21	0.15	0.23	5	4	4.98	0.12	0.18	0.00	0.14	0.22	55	52	2.53	0.16	0.22	0.13	0.15	0.25	6	5	3.66	0.16	0.25	-0.07	0.17	0.25	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.09	0.23	0.33	-0.54	0.22	0.33	3	2	-0.61	0.19	0.23	-0.33	0.16	0.26	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.98	0.19	0.24	-0.58	0.17	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0524-2055	66	4739	100	1.57	0.24	0.34	-2.58	0.12	0.19	1.95	0.12	0.22	5.56	0.21	0.26	-0.25	0.19	0.28	1	1	5.32	0.11	0.18	0.32	0.15	0.24	7	6	3.59	0.14	0.24	-0.29	0.16	0.25	1	1	4.01	0.12	0.20	0.24	0.15	0.25	9	8	0.63	0.18	0.23	0.05	0.15	0.25	5	5	2.64	0.16	0.21	0.21	0.15	0.23	17	17	1.30	0.16	0.20	-0.11	0.15	0.24	3	3	2.77	0.17	0.28	-0.32	0.16	0.26	3	3	2.36	0.15	0.20	-0.45	0.15	0.23	5	5	4.91	0.12	0.19	0.00	0.14	0.22	55	54	2.43	0.16	0.23	0.10	0.15	0.24	6	6	3.66	0.19	0.29	-0.01	0.18	0.26	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.51	0.16	0.23	0.13	0.15	0.25	3	1	-0.56	0.18	0.22	-0.21	0.15	0.25	6	6	0.28	0.17	0.22	0.27	0.15	0.25	3	2	-0.39	0.21	0.31	0.07	0.20	0.29	2	1	-1.33	0.18	0.22	0.08	0.15	0.25	6	4	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-0.89	0.18	0.23	0.20	0.15	0.25	9	2	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.59	0.18	0.22	0.49	0.15	0.25	4	4
HE 0534-4615	53	5506	100	3.40	0.24	0.34	-2.01	0.12	0.18	1.43	0.13	0.23	6.51	0.19	0.25	0.13	0.17	0.26	1	1	5.80	0.12	0.18	0.22	0.14	0.23	7	4	3.59	0.13	0.23	-0.87	0.16	0.25	1	1	4.64	0.11	0.20	0.28	0.14	0.24	9	8	1.21	0.18	0.23	0.05	0.16	0.27	5	4	3.20	0.16	0.21	0.19	0.15	0.25	17	15	2.04	0.16	0.20	0.04	0.15	0.24	3	2	3.48	0.15	0.24	-0.18	0.16	0.25	3	3	3.03	0.15	0.20	-0.35	0.15	0.24	5	4	5.49	0.12	0.18	0.00	0.14	0.22	55	53	2.93	0.15	0.22	0.02	0.15	0.25	6	5	4.04	0.18	0.27	-0.20	0.19	0.27	4	3	2.77	0.14	0.21	0.18	0.15	0.26	2	1	1.01	0.14	0.22	0.04	0.15	0.25	3	2	0.06	0.18	0.23	-0.17	0.16	0.27	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	0.11	0.22	0.27	-0.01	0.20	0.30	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.00	0.18	0.23	0.49	0.16	0.27	4	3
HE 0538-4515	41	5896	100	3.97	0.25	0.35	-1.52	0.10	0.18	1.52	0.14	0.24	7.02	0.16	0.23	0.15	0.18	0.26	1	1	6.27	0.11	0.17	0.21	0.14	0.23	7	4	4.26	0.12	0.24	-0.69	0.17	0.26	1	1	5.12	0.10	0.20	0.28	0.14	0.24	9	9	1.82	0.17	0.22	0.17	0.18	0.28	5	5	3.73	0.15	0.20	0.23	0.17	0.26	17	14	2.62	0.15	0.19	0.14	0.16	0.26	3	2	4.14	0.13	0.23	-0.01	0.17	0.25	3	3	3.72	0.13	0.18	-0.15	0.15	0.24	5	5	5.98	0.10	0.18	0.00	0.14	0.22	55	53	3.50	0.14	0.21	0.10	0.16	0.26	6	5	4.54	0.17	0.26	-0.19	0.19	0.27	4	3	3.24	0.14	0.21	0.16	0.16	0.27	2	1	1.61	0.14	0.21	0.16	0.16	0.25	3	1	0.71	0.18	0.23	-0.01	0.19	0.28	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	0.51	0.23	0.28	-0.10	0.24	0.31	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-0.50	0.18	0.23	0.51	0.18	0.29	4	1
HE 0547-4539	94	5152	100	2.59	0.24	0.34	-3.01	0.13	0.18	1.57	0.12	0.22	5.88	0.19	0.26	0.50	0.17	0.27	1	1	4.70	0.11	0.18	0.13	0.15	0.24	7	5	2.38	0.14	0.22	-1.07	0.15	0.24	1	1	3.48	0.12	0.20	0.13	0.14	0.24	9	7	0.23	0.17	0.22	0.07	0.15	0.24	5	4	2.20	0.16	0.21	0.19	0.15	0.23	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.38	0.16	0.22	-0.27	0.15	0.23	3	3	1.83	0.16	0.21	-0.55	0.15	0.23	5	3	4.49	0.13	0.18	0.00	0.14	0.22	55	49	2.10	0.16	0.22	0.19	0.15	0.24	6	6	3.27	0.16	0.23	0.03	0.16	0.24	4	4	2.22	0.14	0.21	0.63	0.14	0.25	2	1	0.14	0.19	0.29	0.18	0.18	0.29	3	2	-1.10	0.18	0.23	-0.33	0.16	0.25	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.91	0.18	0.23	-1.03	0.16	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0858-0016	39	4447	100	0.75	0.26	0.36	-2.73	0.12	0.19	2.35	0.14	0.24	4.84	0.21	0.27	-0.80	0.20	0.28	1	1	5.09	0.11	0.19	0.26	0.15	0.23	7	4	3.31	0.17	0.26	-0.41	0.18	0.27	1	1	3.80	0.12	0.20	0.19	0.15	0.25	9	7	0.38	0.15	0.21	-0.04	0.15	0.24	5	5	2.45	0.12	0.18	0.18	0.15	0.23	17	17	1.05	0.16	0.20	-0.21	0.16	0.24	3	1	2.49	0.22	0.30	-0.43	0.20	0.28	3	3	2.31	0.16	0.21	-0.33	0.16	0.23	5	4	4.75	0.12	0.19	0.00	0.14	0.22	55	47	2.13	0.16	0.24	-0.04	0.16	0.25	6	6	3.99	0.23	0.32	0.49	0.21	0.29	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.48	0.25	0.35	-0.70	0.24	0.33	3	1	-1.12	0.18	0.23	-0.61	0.16	0.26	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.16	0.24	0.30	-0.54	0.22	0.29	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-2.25	0.19	0.23	-0.01	0.17	0.26	4	3
HE 0926-0508	124	6249	100	4.24	0.25	0.35	-2.78	0.12	0.17	1.60	0.12	0.22	6.23	0.14	0.23	0.62	0.16	0.27	1	1	5.08	0.12	0.18	0.28	0.14	0.23	7	1	2.79	0.13	0.20	-0.90	0.14	0.24	1	1	3.96	0.11	0.19	0.37	0.14	0.24	9	3	0.67	0.17	0.22	0.28	0.15	0.25	5	1	2.73	0.15	0.21	0.49	0.15	0.24	17	6	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.75	0.14	0.19	-0.14	0.15	0.22	3	3	2.07	0.14	0.19	-0.54	0.15	0.23	5	2	4.72	0.12	0.17	0.00	0.14	0.22	55	33	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	3.42	0.14	0.19	-0.06	0.15	0.22	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.17	0.18	0.26	-0.02	0.17	0.27	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.92	0.18	0.22	-0.28	0.16	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0938+0114	307	6777	100	4.89	0.23	0.33	-2.51	0.12	0.17	1.76	0.11	0.21	6.54	0.14	0.22	0.65	0.16	0.27	1	1	5.29	0.11	0.17	0.22	0.14	0.23	7	1	3.18	0.12	0.20	-0.79	0.14	0.24	1	1	4.22	0.11	0.19	0.37	0.15	0.24	9	3	1.12	0.16	0.22	0.46	0.15	0.24	5	1	3.05	0.15	0.21	0.53	0.14	0.23	17	5	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.13	0.13	0.18	-0.03	0.14	0.22	3	3	2.45	0.12	0.17	-0.43	0.14	0.22	5	1	4.99	0.12	0.17	0.00	0.14	0.22	55	30	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	3.78	0.14	0.18	0.04	0.14	0.22	4	1	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.38	0.17	0.24	-0.08	0.16	0.26	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.48	0.17	0.21	-0.10	0.15	0.24	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 0951-1152	41	5349	100	4.75	0.25	0.35	-2.62	0.14	0.18	1.42	0.17	0.27	5.88	0.24	0.28	0.10	0.19	0.27	1	1	5.50	0.14	0.20	0.54	0.14	0.24	7	3	3.80	0.13	0.22	-0.05	0.16	0.26	1	1	3.99	0.13	0.21	0.25	0.14	0.24	9	7	0.82	0.19	0.24	0.27	0.16	0.26	5	2	2.66	0.17	0.22	0.25	0.16	0.25	17	9	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.07	0.14	0.20	0.02	0.15	0.23	3	3	2.58	0.15	0.20	-0.19	0.15	0.23	5	3	4.88	0.14	0.18	0.00	0.14	0.22	55	37	2.47	0.17	0.23	0.17	0.15	0.25	6	5	3.53	0.15	0.20	-0.10	0.15	0.23	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.15	0.19	0.25	-0.51	0.17	0.27	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.40	0.20	0.26	0.09	0.17	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1006-2218	65	6638	100	4.62	0.30	0.40	-2.69	0.13	0.18	1.79	0.16	0.26	-9.99	0.00	0.00	-9.99	0.00	0.00	1	0	-9.99	0.00	0.00	-9.99	0.00	0.00	7	0	2.99	0.13	0.20	-0.79	0.15	0.25	1	1	3.99	0.12	0.20	0.32	0.15	0.25	9	2	0.83	0.18	0.23	0.35	0.16	0.25	5	1	2.81	0.17	0.22	0.48	0.16	0.25	17	5	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.87	0.13	0.18	-0.11	0.15	0.23	3	3	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	4.81	0.13	0.18	0.00	0.14	0.22	55	22	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.13	0.19	0.26	-0.15	0.17	0.26	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1015-0027	47	6315	100	4.40	0.27	0.37	-2.66	0.12	0.17	1.43	0.15	0.25	-9.99	0.00	0.00	-9.99	0.00	0.00	1	0	5.27	0.12	0.18	0.35	0.15	0.24	7	1	2.81	0.14	0.21	-1.00	0.16	0.25	1	1	4.11	0.11	0.19	0.41	0.15	0.25	9	3	0.79	0.18	0.23	0.28	0.17	0.26	5	1	2.91	0.16	0.21	0.55	0.16	0.25	17	6	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.78	0.14	0.19	-0.24	0.15	0.23	3	3	2.29	0.15	0.20	-0.45	0.16	0.24	5	1	4.85	0.12	0.17	0.00	0.14	0.22	55	27	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	3.50	0.15	0.19	-0.10	0.16	0.23	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.75	0.20	0.28	0.44	0.19	0.28	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1044-2509	51	5227	100	2.78	0.26	0.36	-2.89	0.12	0.18	1.84	0.14	0.24	6.03	0.19	0.26	0.52	0.18	0.28	1	1	4.99	0.11	0.19	0.29	0.16	0.25	7	6	3.00	0.13	0.24	-0.59	0.16	0.26	1	1	3.85	0.12	0.20	0.37	0.15	0.25	9	7	0.54	0.18	0.23	0.25	0.16	0.26	5	4	2.37	0.16	0.22	0.24	0.15	0.24	17	10	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.63	0.17	0.24	-0.16	0.16	0.24	3	3	1.99	0.17	0.22	-0.52	0.16	0.24	5	3	4.62	0.12	0.18	0.00	0.14	0.22	55	40	2.28	0.16	0.22	0.25	0.15	0.25	6	5	3.42	0.18	0.25	0.05	0.17	0.24	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.32	0.20	0.29	0.23	0.18	0.28	3	2	-0.46	0.19	0.24	0.18	0.17	0.26	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.52	0.21	0.26	0.24	0.19	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.44	0.18	0.23	0.94	0.17	0.26	4	1
HE 1052-2548	93	6534	100	4.52	0.25	0.35	-2.29	0.12	0.17	1.57	0.13	0.23	6.61	0.14	0.22	0.51	0.17	0.26	1	1	5.45	0.11	0.17	0.16	0.14	0.23	7	1	3.70	0.12	0.21	-0.48	0.15	0.25	1	1	4.34	0.11	0.19	0.27	0.14	0.24	9	7	1.14	0.17	0.22	0.27	0.16	0.25	5	2	3.17	0.15	0.20	0.45	0.15	0.24	17	9	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.26	0.13	0.18	-0.12	0.15	0.22	3	3	2.62	0.14	0.19	-0.48	0.15	0.23	5	3	5.21	0.12	0.17	0.00	0.14	0.22	55	35	2.88	0.14	0.21	0.25	0.16	0.25	6	1	3.99	0.15	0.19	0.03	0.15	0.22	4	1	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.93	0.18	0.27	0.26	0.18	0.28	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	0.71	0.18	0.23	0.88	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1054-0059	38	4601	100	1.19	0.27	0.37	-3.34	0.13	0.18	2.21	0.14	0.24	4.32	0.22	0.29	-0.73	0.20	0.29	1	1	4.51	0.13	0.19	0.27	0.15	0.23	7	4	2.36	0.21	0.29	-0.77	0.23	0.31	1	1	3.26	0.12	0.20	0.24	0.15	0.24	9	3	-0.04	0.17	0.22	0.12	0.16	0.25	5	3	1.88	0.16	0.21	0.20	0.15	0.23	17	11	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.69	0.16	0.22	-0.64	0.16	0.24	3	3	1.43	0.16	0.22	-0.62	0.16	0.24	5	3	4.16	0.13	0.18	0.00	0.14	0.22	55	40	1.80	0.16	0.22	0.22	0.15	0.24	6	5	2.93	0.19	0.27	0.01	0.19	0.28	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-1.08	0.23	0.32	-0.71	0.22	0.32	3	2	-1.43	0.20	0.24	-0.33	0.18	0.26	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-2.42	0.19	0.23	-1.21	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1059-0118	49	5560	100	4.30	0.25	0.35	-2.81	0.12	0.18	1.28	0.18	0.28	5.95	0.19	0.25	0.37	0.17	0.26	1	1	5.24	0.12	0.18	0.46	0.15	0.24	7	3	2.93	0.14	0.22	-0.73	0.16	0.25	1	1	3.86	0.12	0.20	0.31	0.14	0.24	9	7	0.50	0.18	0.23	0.14	0.18	0.28	5	2	2.42	0.16	0.21	0.21	0.16	0.27	17	8	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.51	0.14	0.20	-0.36	0.15	0.23	3	3	2.14	0.17	0.22	-0.45	0.17	0.25	5	2	4.70	0.12	0.18	0.00	0.14	0.22	55	35	2.44	0.15	0.22	0.32	0.16	0.25	6	3	3.55	0.15	0.21	0.11	0.16	0.24	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.34	0.19	0.26	-0.50	0.19	0.30	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1100-0137	50	6101	100	4.25	0.32	0.42	-2.92	0.13	0.18	1.29	0.17	0.27	5.96	0.21	0.28	0.47	0.22	0.30	1	1	-9.99	0.00	0.00	-9.99	0.00	0.00	7	0	2.39	0.14	0.21	-1.17	0.16	0.26	1	1	3.67	0.12	0.20	0.22	0.15	0.25	9	2	0.49	0.18	0.23	0.22	0.18	0.27	5	1	2.37	0.17	0.23	0.25	0.17	0.27	17	5	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.38	0.15	0.19	-0.39	0.15	0.23	3	3	2.19	0.15	0.20	-0.30	0.16	0.24	5	2	4.60	0.13	0.18	0.00	0.14	0.22	55	23	2.57	0.15	0.21	0.55	0.16	0.25	6	1	3.27	0.16	0.20	-0.07	0.16	0.23	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	0.65	0.20	0.25	2.05	0.19	0.28	9	1	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1105+0027	43	6132	100	3.45	0.25	0.35	-2.42	0.13	0.19	1.52	0.14	0.24	7.97	0.15	0.23	2.00	0.17	0.28	1	1	5.63	0.11	0.17	0.47	0.16	0.24	7	2	3.16	0.15	0.22	-0.89	0.17	0.26	1	1	4.41	0.12	0.20	0.47	0.15	0.25	9	6	1.03	0.17	0.22	0.28	0.15	0.23	5	2	2.92	0.15	0.21	0.32	0.15	0.23	17	6	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.30	0.16	0.22	0.05	0.15	0.23	3	3	2.46	0.15	0.20	-0.51	0.15	0.24	5	3	5.08	0.13	0.19	0.00	0.14	0.22	55	34	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	3.54	0.16	0.20	-0.29	0.16	0.23	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	1.28	0.20	0.29	0.73	0.18	0.28	3	2	0.57	0.18	0.23	0.75	0.16	0.24	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.16	0.11	0.18	2.45	0.16	0.23	2	2	0.85	0.17	0.22	2.10	0.15	0.24	6	4	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	1.14	0.18	0.23	2.06	0.16	0.24	9	4	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-0.10	0.18	0.23	1.81	0.16	0.24	4	4
HE 1120-0153	194	6191	100	4.09	0.24	0.34	-2.77	0.11	0.17	0.68	0.12	0.22	6.26	0.16	0.23	0.63	0.17	0.26	1	1	4.86	0.11	0.17	0.04	0.14	0.23	7	1	2.64	0.13	0.20	-1.07	0.14	0.25	1	1	3.80	0.11	0.19	0.20	0.15	0.24	9	2	0.61	0.16	0.22	0.20	0.15	0.25	5	1	2.56	0.15	0.21	0.30	0.15	0.25	17	5	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.69	0.14	0.19	-0.22	0.15	0.22	3	3	1.94	0.14	0.19	-0.69	0.15	0.23	5	1	4.74	0.11	0.17	0.00	0.14	0.22	55	34	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	3.30	0.14	0.19	-0.19	0.15	0.22	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.03	0.18	0.25	-0.18	0.17	0.27	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.76	0.15	0.20	-0.13	0.15	0.24	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1122-1429	44	5787	100	3.29	0.27	0.37	-2.65	0.13	0.18	1.54	0.15	0.25	6.18	0.18	0.25	0.44	0.18	0.28	1	1	5.26	0.11	0.17	0.34	0.16	0.24	7	2	2.89	0.15	0.22	-0.92	0.16	0.26	1	1	4.21	0.11	0.20	0.50	0.15	0.25	9	7	0.55	0.18	0.23	0.04	0.16	0.25	5	2	2.67	0.17	0.23	0.30	0.16	0.24	17	6	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.74	0.15	0.20	-0.27	0.15	0.23	3	3	2.00	0.15	0.20	-0.74	0.15	0.23	5	2	4.85	0.13	0.18	0.00	0.14	0.22	55	32	2.41	0.16	0.22	0.14	0.15	0.25	6	1	3.27	0.19	0.22	-0.32	0.17	0.24	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.26	0.23	0.33	-0.05	0.21	0.31	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.87	0.19	0.23	-0.34	0.16	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1124-2335	48	5226	100	2.68	0.26	0.36	-2.95	0.14	0.19	1.65	0.13	0.23	6.31	0.19	0.26	0.86	0.18	0.28	1	1	5.00	0.11	0.19	0.35	0.19	0.27	7	6	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	3.62	0.12	0.20	0.19	0.15	0.25	9	7	0.41	0.16	0.21	0.18	0.15	0.23	5	4	2.43	0.16	0.21	0.34	0.15	0.23	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.69	0.17	0.24	-0.05	0.16	0.24	3	3	2.18	0.16	0.21	-0.28	0.15	0.23	5	3	4.57	0.14	0.19	0.00	0.14	0.22	55	42	2.34	0.16	0.22	0.35	0.15	0.24	6	6	3.56	0.18	0.27	0.25	0.17	0.26	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.12	0.22	0.32	0.09	0.19	0.30	3	2	-0.68	0.19	0.23	0.01	0.16	0.25	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.86	0.19	0.23	-1.06	0.16	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1126-1735	46	5689	100	3.31	0.28	0.38	-2.69	0.13	0.18	1.55	0.15	0.25	5.93	0.18	0.25	0.23	0.18	0.28	1	1	5.20	0.11	0.17	0.31	0.16	0.24	7	3	2.72	0.13	0.21	-1.06	0.15	0.24	1	1	4.00	0.12	0.20	0.32	0.15	0.25	9	5	0.55	0.18	0.23	0.07	0.16	0.25	5	2	2.66	0.16	0.22	0.33	0.15	0.24	17	6	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.69	0.18	0.22	-0.29	0.16	0.23	3	3	1.99	0.16	0.20	-0.71	0.15	0.23	5	3	4.81	0.13	0.18	0.00	0.14	0.22	55	34	2.35	0.15	0.22	0.12	0.15	0.25	6	2	3.53	0.13	0.24	-0.04	0.17	0.26	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.11	0.22	0.32	-0.17	0.20	0.31	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.02	0.19	0.24	-0.46	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1127-1143	49	5224	100	2.64	0.25	0.35	-2.73	0.14	0.19	1.59	0.14	0.24	6.21	0.19	0.25	0.54	0.17	0.27	1	1	5.08	0.11	0.18	0.22	0.16	0.25	7	6	2.87	0.16	0.25	-0.87	0.17	0.26	1	1	3.89	0.12	0.20	0.26	0.15	0.25	9	8	0.57	0.18	0.23	0.13	0.15	0.24	5	4	2.48	0.16	0.21	0.19	0.14	0.23	17	13	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.65	0.17	0.24	-0.29	0.15	0.24	3	3	1.92	0.17	0.22	-0.75	0.15	0.23	5	2	4.78	0.14	0.19	0.00	0.14	0.22	55	46	2.48	0.16	0.22	0.28	0.15	0.24	6	6	3.71	0.20	0.28	0.19	0.17	0.26	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.49	0.22	0.30	0.24	0.19	0.28	3	1	-0.27	0.19	0.24	0.22	0.16	0.24	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	0.03	0.22	0.29	0.63	0.19	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-0.37	0.19	0.23	0.86	0.16	0.24	9	2	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.14	0.18	0.23	1.08	0.15	0.24	4	3
HE 1128-0823	65	5909	100	3.71	0.25	0.35	-2.71	0.13	0.18	1.49	0.13	0.23	6.15	0.17	0.24	0.47	0.17	0.27	1	1	5.10	0.12	0.18	0.23	0.15	0.23	7	2	2.79	0.14	0.21	-0.97	0.15	0.25	1	1	3.99	0.11	0.20	0.34	0.15	0.25	9	7	0.71	0.17	0.23	0.25	0.16	0.24	5	2	2.73	0.15	0.20	0.42	0.15	0.23	17	7	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.66	0.15	0.19	-0.30	0.15	0.22	3	3	1.96	0.15	0.20	-0.72	0.15	0.23	5	3	4.79	0.13	0.18	0.00	0.14	0.22	55	37	2.40	0.14	0.21	0.20	0.15	0.24	6	2	3.55	0.22	0.26	0.01	0.19	0.25	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.28	0.17	0.28	0.02	0.17	0.28	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.74	0.18	0.23	-0.16	0.16	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1131+0141	45	5236	100	2.98	0.25	0.35	-2.48	0.13	0.18	1.63	0.14	0.24	6.02	0.20	0.25	0.12	0.17	0.26	1	1	5.33	0.12	0.18	0.23	0.15	0.23	7	5	3.15	0.18	0.26	-0.84	0.21	0.29	1	1	4.15	0.12	0.20	0.28	0.15	0.24	9	8	0.67	0.18	0.24	-0.01	0.16	0.26	5	3	2.71	0.17	0.22	0.18	0.16	0.25	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.94	0.16	0.25	-0.25	0.16	0.25	3	3	2.44	0.17	0.22	-0.47	0.16	0.24	5	3	5.01	0.13	0.18	0.00	0.14	0.22	55	49	2.38	0.16	0.22	-0.05	0.15	0.25	6	5	3.72	0.18	0.27	-0.04	0.18	0.26	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.63	0.17	0.25	0.15	0.17	0.26	3	2	-0.18	0.18	0.23	0.07	0.16	0.26	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	0.17	0.19	0.25	0.52	0.18	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.10	0.18	0.23	0.87	0.16	0.26	4	3
HE 1132+0125	50	5732	100	3.54	0.26	0.36	-2.42	0.11	0.18	1.41	0.13	0.23	6.25	0.18	0.24	0.24	0.20	0.28	1	1	5.58	0.11	0.18	0.38	0.15	0.24	7	5	3.09	0.15	0.23	-1.00	0.17	0.26	1	1	4.29	0.11	0.20	0.31	0.15	0.25	9	7	0.83	0.18	0.23	0.04	0.18	0.28	5	3	2.83	0.16	0.21	0.19	0.17	0.26	17	10	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.07	0.17	0.23	-0.22	0.17	0.25	3	3	2.15	0.16	0.21	-0.86	0.18	0.26	5	2	5.12	0.11	0.18	0.00	0.14	0.22	55	44	2.58	0.15	0.21	0.04	0.17	0.26	6	3	3.62	0.18	0.23	-0.25	0.18	0.25	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.56	0.19	0.29	-0.03	0.19	0.29	3	2	-0.19	0.18	0.23	-0.05	0.19	0.28	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.41	0.19	0.24	-0.16	0.19	0.28	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1132+0204	42	5046	100	2.25	0.25	0.35	-2.55	0.11	0.18	1.68	0.13	0.23	5.99	0.20	0.26	0.13	0.20	0.29	1	1	5.25	0.12	0.18	0.20	0.15	0.24	7	6	2.90	0.19	0.27	-1.04	0.20	0.28	1	1	4.01	0.11	0.20	0.18	0.14	0.25	9	8	0.59	0.15	0.21	-0.05	0.15	0.25	5	4	2.56	0.16	0.21	0.07	0.16	0.25	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.93	0.19	0.28	-0.21	0.19	0.27	3	3	2.32	0.17	0.23	-0.54	0.17	0.25	5	3	4.97	0.11	0.18	0.00	0.14	0.22	54	52	2.54	0.16	0.22	0.15	0.16	0.26	6	6	3.73	0.19	0.30	0.01	0.19	0.28	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.22	0.21	0.32	-0.22	0.21	0.31	3	2	-0.70	0.19	0.24	-0.41	0.18	0.27	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.09	0.21	0.26	-0.69	0.20	0.28	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.77	0.19	0.23	0.25	0.18	0.28	4	1
HE 1135+0139	47	5487	100	1.80	0.26	0.36	-2.33	0.13	0.18	2.66	0.12	0.22	7.28	0.17	0.25	1.19	0.19	0.29	1	1	5.60	0.11	0.17	0.33	0.15	0.24	7	7	3.28	0.17	0.24	-0.89	0.17	0.26	1	1	4.44	0.12	0.20	0.38	0.15	0.25	9	8	1.02	0.18	0.23	0.15	0.16	0.24	5	5	2.86	0.18	0.23	0.14	0.16	0.25	17	15	1.72	0.16	0.21	0.03	0.16	0.24	3	1	3.13	0.14	0.21	-0.24	0.14	0.22	3	3	2.64	0.16	0.21	-0.44	0.16	0.23	5	2	5.19	0.13	0.18	0.00	0.14	0.22	55	47	2.76	0.17	0.23	0.14	0.17	0.26	6	5	3.95	0.14	0.21	0.01	0.15	0.23	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	1.32	0.18	0.25	0.66	0.17	0.26	3	1	0.29	0.18	0.23	0.36	0.16	0.24	6	6	0.75	0.16	0.21	0.46	0.15	0.24	3	1	0.95	0.18	0.23	1.13	0.16	0.24	2	2	-0.21	0.18	0.23	0.93	0.16	0.25	6	4	0.45	0.18	0.25	1.17	0.16	0.27	10	6	-0.03	0.18	0.23	0.77	0.16	0.25	9	2	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.46	0.18	0.23	0.33	0.16	0.25	4	1
HE 1135-0344	45	6154	100	4.03	0.31	0.41	-2.63	0.12	0.18	1.17	0.17	0.27	6.80	0.16	0.24	1.03	0.17	0.27	1	1	-9.99	0.00	0.00	-9.99	0.00	0.00	7	0	2.58	0.15	0.22	-1.26	0.17	0.26	1	1	4.00	0.12	0.20	0.27	0.15	0.25	9	3	0.72	0.18	0.24	0.18	0.18	0.26	5	1	2.84	0.16	0.21	0.45	0.16	0.25	17	6	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.82	0.15	0.20	-0.22	0.15	0.23	3	3	2.09	0.15	0.20	-0.67	0.16	0.24	5	1	4.87	0.12	0.18	0.00	0.14	0.22	55	29	2.60	0.16	0.22	0.30	0.16	0.26	6	1	3.48	0.16	0.20	-0.14	0.16	0.23	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.72	0.22	0.31	0.38	0.21	0.31	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1148-0037	76	5964	100	4.16	0.35	0.45	-3.47	0.13	0.18	0.81	0.20	0.30	5.76	0.20	0.27	0.84	0.19	0.29	1	1	4.03	0.41	0.44	-0.09	0.35	0.40	7	1	1.98	0.14	0.21	-1.02	0.16	0.26	1	1	2.95	0.17	0.23	0.06	0.16	0.26	9	1	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	1.97	0.18	0.23	0.41	0.18	0.27	17	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	4.03	0.13	0.18	0.00	0.14	0.22	55	18	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	2.52	0.20	0.23	-0.26	0.18	0.25	4	1	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.92	0.19	0.26	-0.42	0.19	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1207-2031	50	6281	100	4.40	0.30	0.40	-2.82	0.12	0.17	1.42	0.16	0.26	6.21	0.19	0.26	0.64	0.19	0.28	1	1	-9.99	0.00	0.00	-9.99	0.00	0.00	7	0	2.70	0.14	0.21	-0.96	0.15	0.25	1	1	4.05	0.11	0.20	0.50	0.15	0.25	9	3	0.78	0.18	0.23	0.43	0.17	0.26	5	1	2.75	0.16	0.22	0.54	0.16	0.25	17	5	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.65	0.14	0.19	-0.20	0.15	0.23	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	4.68	0.12	0.17	0.00	0.14	0.22	55	24	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	3.29	0.15	0.19	-0.14	0.15	0.23	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.01	0.19	0.26	-0.16	0.18	0.28	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1210+0048	49	6028	100	3.73	0.27	0.37	-2.28	0.11	0.18	1.56	0.14	0.24	6.70	0.16	0.23	0.57	0.18	0.28	1	1	5.57	0.12	0.18	0.25	0.15	0.25	7	3	3.06	0.15	0.22	-1.15	0.17	0.26	1	1	4.42	0.11	0.20	0.32	0.15	0.25	9	7	0.98	0.18	0.23	0.07	0.18	0.27	5	1	3.08	0.16	0.21	0.32	0.16	0.25	17	10	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.27	0.16	0.22	-0.14	0.16	0.24	3	3	2.46	0.15	0.20	-0.67	0.17	0.25	5	2	5.24	0.11	0.18	0.00	0.14	0.22	55	41	2.80	0.15	0.21	0.14	0.16	0.26	6	2	3.75	0.17	0.21	-0.24	0.17	0.24	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.64	0.22	0.32	-0.07	0.21	0.30	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.18	0.19	0.24	-0.05	0.19	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	0.61	0.18	0.23	1.37	0.18	0.28	9	1	1.06	0.19	0.24	2.31	0.19	0.28	8	1	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1210-1956	50	5790	100	3.30	0.27	0.37	-2.57	0.13	0.18	1.52	0.14	0.24	6.04	0.21	0.26	0.22	0.19	0.28	1	1	5.42	0.12	0.18	0.41	0.15	0.23	7	4	2.94	0.14	0.22	-0.96	0.16	0.25	1	1	4.32	0.11	0.20	0.53	0.15	0.25	9	7	0.56	0.18	0.23	-0.04	0.16	0.24	5	2	2.78	0.16	0.22	0.33	0.15	0.23	17	9	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.92	0.16	0.21	-0.18	0.15	0.23	3	3	2.15	0.16	0.20	-0.68	0.15	0.23	5	2	4.93	0.13	0.18	0.00	0.14	0.22	55	41	2.40	0.15	0.21	0.05	0.15	0.25	6	3	3.43	0.16	0.21	-0.25	0.15	0.22	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.44	0.23	0.32	0.04	0.20	0.31	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.86	0.19	0.23	-0.43	0.16	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1212-0127	30	4915	100	1.85	0.26	0.36	-2.15	0.13	0.19	1.87	0.14	0.24	5.85	0.20	0.26	-0.39	0.18	0.27	1	1	5.55	0.12	0.19	0.13	0.15	0.24	7	5	3.77	0.23	0.30	-0.54	0.24	0.31	1	1	4.35	0.12	0.21	0.15	0.15	0.25	9	8	0.95	0.15	0.22	-0.07	0.16	0.24	5	5	2.91	0.18	0.24	0.05	0.16	0.25	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.19	0.20	0.33	-0.33	0.21	0.31	3	3	2.82	0.15	0.20	-0.42	0.15	0.24	5	3	5.34	0.13	0.19	0.00	0.14	0.22	55	54	2.65	0.17	0.24	-0.11	0.16	0.25	6	6	3.53	0.26	0.34	-0.56	0.24	0.32	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.62	0.19	0.26	-0.20	0.18	0.26	3	2	-0.23	0.17	0.22	-0.31	0.16	0.26	6	3	0.56	0.19	0.23	0.11	0.17	0.27	3	1	-0.34	0.27	0.35	-0.32	0.27	0.34	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.30	0.18	0.23	0.35	0.16	0.27	4	3
HE 1214-1819	53	4916	100	1.88	0.26	0.36	-3.01	0.12	0.18	1.74	0.13	0.23	5.74	0.20	0.26	0.35	0.19	0.28	1	1	4.96	0.12	0.19	0.39	0.15	0.24	7	5	2.73	0.19	0.27	-0.74	0.20	0.29	1	1	3.70	0.12	0.20	0.34	0.15	0.25	9	8	0.33	0.18	0.23	0.16	0.16	0.25	5	4	2.30	0.16	0.21	0.28	0.15	0.23	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.35	0.17	0.24	-0.32	0.16	0.24	3	3	1.71	0.17	0.21	-0.68	0.16	0.23	5	3	4.50	0.12	0.18	0.00	0.14	0.22	55	47	2.13	0.16	0.22	0.22	0.15	0.24	6	5	3.46	0.19	0.28	0.21	0.18	0.27	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.23	0.17	0.29	0.27	0.18	0.29	3	2	-0.65	0.19	0.23	0.11	0.16	0.25	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.92	0.22	0.28	-0.04	0.19	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-2.00	0.19	0.23	0.49	0.16	0.26	4	1
HE 1215+0149	35	5098	100	2.37	0.27	0.37	-2.90	0.13	0.19	1.48	0.14	0.24	5.65	0.20	0.26	0.15	0.19	0.28	1	1	5.03	0.12	0.19	0.35	0.16	0.24	7	6	3.10	0.20	0.28	-0.47	0.21	0.29	1	1	3.74	0.12	0.20	0.27	0.15	0.25	9	5	0.33	0.18	0.23	0.06	0.16	0.26	5	4	2.48	0.17	0.22	0.36	0.16	0.24	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.27	0.18	0.24	-0.51	0.17	0.24	3	2	1.77	0.17	0.22	-0.72	0.16	0.24	5	3	4.60	0.13	0.19	0.00	0.14	0.22	55	42	2.25	0.16	0.22	0.23	0.16	0.25	6	5	3.50	0.22	0.30	0.15	0.20	0.27	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.36	0.20	0.30	0.29	0.19	0.29	3	2	-0.71	0.20	0.24	-0.05	0.18	0.26	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.53	0.20	0.24	-0.76	0.18	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1217-0540	45	5700	100	4.20	0.27	0.37	-2.95	0.12	0.18	1.41	0.17	0.27	6.26	0.17	0.24	0.81	0.17	0.26	1	1	5.06	0.12	0.18	0.42	0.15	0.24	7	1	2.82	0.14	0.22	-0.71	0.16	0.25	1	1	3.67	0.12	0.20	0.25	0.15	0.25	9	3	0.24	0.18	0.23	0.01	0.18	0.28	5	1	2.34	0.16	0.22	0.27	0.17	0.27	17	5	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.55	0.16	0.20	-0.18	0.16	0.23	3	3	1.82	0.16	0.21	-0.62	0.16	0.25	5	3	4.56	0.12	0.18	0.00	0.14	0.22	54	30	2.27	0.16	0.22	0.30	0.16	0.26	6	2	3.21	0.16	0.20	-0.09	0.16	0.23	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.16	0.20	0.28	0.13	0.20	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1219-0312	46	5140	100	2.40	0.26	0.36	-2.81	0.12	0.18	1.54	0.13	0.23	5.51	0.19	0.26	-0.08	0.19	0.28	1	1	4.82	0.11	0.19	0.04	0.16	0.24	7	4	2.56	0.17	0.24	-1.11	0.17	0.26	1	1	3.53	0.11	0.20	-0.03	0.15	0.25	9	6	0.31	0.18	0.23	-0.07	0.17	0.25	5	4	2.21	0.16	0.21	-0.01	0.15	0.24	17	9	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.35	0.16	0.23	-0.52	0.16	0.24	3	3	2.10	0.25	0.42	-0.49	0.32	0.44	5	3	4.70	0.12	0.18	0.00	0.14	0.22	55	44	2.14	0.16	0.22	0.02	0.16	0.25	6	4	3.41	0.19	0.26	-0.05	0.18	0.26	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.38	0.18	0.27	0.20	0.18	0.27	3	2	-0.27	0.19	0.24	0.29	0.17	0.26	6	4	0.45	0.19	0.23	0.65	0.17	0.26	3	1	-0.16	0.29	0.35	0.51	0.25	0.33	2	1	-0.72	0.18	0.23	0.91	0.17	0.26	6	4	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-0.31	0.19	0.23	0.98	0.17	0.26	9	2	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-0.87	0.19	0.23	1.41	0.17	0.26	4	3
HE 1221-0522	44	5789	100	4.04	0.28	0.38	-2.84	0.12	0.17	1.29	0.17	0.27	6.08	0.18	0.24	0.53	0.17	0.26	1	1	5.19	0.11	0.18	0.45	0.15	0.23	7	2	2.96	0.15	0.23	-0.67	0.16	0.26	1	1	3.99	0.11	0.20	0.47	0.15	0.25	9	5	0.47	0.18	0.24	0.14	0.18	0.27	5	1	2.49	0.16	0.21	0.31	0.16	0.25	17	4	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.61	0.15	0.20	-0.22	0.15	0.23	3	3	1.98	0.16	0.20	-0.57	0.16	0.24	5	3	4.66	0.12	0.17	0.00	0.14	0.22	55	32	2.41	0.16	0.22	0.32	0.16	0.25	6	2	3.45	0.16	0.21	0.04	0.16	0.24	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.32	0.20	0.27	-0.46	0.19	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1221-1948	57	6083	100	3.81	0.28	0.38	-3.36	0.13	0.18	1.65	0.15	0.25	6.46	0.22	0.28	1.42	0.22	0.31	1	1	5.02	0.13	0.19	0.80	0.15	0.24	7	1	2.39	0.14	0.21	-0.72	0.16	0.25	1	1	3.81	0.12	0.20	0.81	0.15	0.25	9	3	0.10	0.18	0.23	0.29	0.17	0.26	5	1	2.19	0.16	0.22	0.52	0.16	0.25	17	5	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.12	0.14	0.19	-0.19	0.15	0.23	3	1	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	4.14	0.13	0.18	0.00	0.14	0.22	55	18	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	2.79	0.15	0.19	-0.10	0.16	0.23	4	1	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1222-0200	45	5288	100	2.72	0.26	0.36	-2.45	0.13	0.19	1.50	0.14	0.24	6.18	0.19	0.25	0.23	0.18	0.27	1	1	5.31	0.12	0.18	0.17	0.15	0.24	7	5	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	4.20	0.12	0.20	0.29	0.14	0.24	9	8	0.68	0.18	0.24	-0.04	0.16	0.26	5	4	2.71	0.17	0.22	0.14	0.15	0.24	17	14	1.99	0.16	0.20	0.43	0.15	0.24	3	3	3.36	0.18	0.28	0.13	0.17	0.26	3	3	2.54	0.14	0.26	-0.41	0.19	0.28	5	3	5.06	0.13	0.19	0.00	0.14	0.22	55	47	2.78	0.16	0.22	0.31	0.15	0.24	6	6	3.92	0.19	0.29	0.12	0.18	0.27	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.40	0.20	0.31	-0.13	0.19	0.30	3	2	-0.42	0.19	0.24	-0.22	0.17	0.26	6	2	0.79	0.18	0.23	0.64	0.17	0.26	3	1	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.34	0.19	0.23	0.60	0.16	0.26	4	1
HE 1222-0336	46	6052	100	3.96	0.25	0.35	-2.04	0.11	0.17	1.30	0.14	0.24	6.57	0.15	0.23	0.22	0.16	0.26	1	1	5.63	0.11	0.17	0.09	0.15	0.23	7	3	3.14	0.15	0.22	-1.28	0.16	0.25	1	1	4.58	0.11	0.20	0.26	0.15	0.25	9	8	1.15	0.17	0.23	0.02	0.17	0.26	5	2	3.27	0.16	0.21	0.29	0.16	0.24	17	10	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.48	0.16	0.23	-0.14	0.16	0.24	3	3	2.84	0.16	0.20	-0.51	0.16	0.24	5	3	5.46	0.11	0.17	0.00	0.14	0.22	55	45	2.79	0.15	0.21	-0.09	0.16	0.25	6	2	4.11	0.18	0.25	-0.10	0.19	0.26	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.60	0.20	0.29	-0.33	0.20	0.30	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.11	0.19	0.24	-0.20	0.18	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1225+0155	100	4842	100	1.80	0.23	0.33	-2.75	0.12	0.18	1.85	0.11	0.21	5.90	0.20	0.26	0.26	0.19	0.28	1	1	5.30	0.12	0.18	0.46	0.15	0.23	7	6	3.18	0.12	0.24	-0.54	0.15	0.25	1	1	3.98	0.13	0.21	0.37	0.14	0.25	9	9	0.56	0.17	0.22	0.14	0.15	0.24	5	5	2.58	0.16	0.21	0.30	0.15	0.23	17	17	1.26	0.15	0.19	0.00	0.15	0.23	3	2	2.67	0.15	0.26	-0.25	0.15	0.25	3	3	2.17	0.14	0.21	-0.48	0.15	0.23	5	4	4.75	0.12	0.18	0.00	0.14	0.22	55	54	2.32	0.16	0.23	0.15	0.15	0.24	6	6	3.33	0.14	0.26	-0.18	0.15	0.26	4	4	2.11	0.13	0.20	0.26	0.14	0.25	2	2	0.30	0.17	0.26	0.07	0.16	0.26	3	2	-0.67	0.17	0.22	-0.17	0.15	0.24	6	6	0.16	0.17	0.22	0.30	0.15	0.24	3	2	-1.07	0.20	0.26	-0.45	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.99	0.18	0.23	0.25	0.15	0.25	4	3
HE 1225-0515	41	6210	100	3.81	0.27	0.37	-1.96	0.13	0.18	1.35	0.15	0.25	6.94	0.16	0.23	0.52	0.17	0.27	1	1	5.80	0.12	0.18	0.18	0.15	0.24	7	3	3.51	0.16	0.24	-1.00	0.18	0.26	1	1	4.67	0.11	0.20	0.27	0.15	0.25	9	8	1.22	0.17	0.23	0.02	0.16	0.25	5	3	3.40	0.15	0.21	0.34	0.15	0.23	17	10	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.62	0.17	0.23	-0.08	0.16	0.24	3	3	2.93	0.15	0.20	-0.50	0.15	0.23	5	3	5.54	0.13	0.18	0.00	0.14	0.22	55	44	3.01	0.15	0.21	0.05	0.15	0.25	6	3	4.12	0.18	0.24	-0.16	0.17	0.24	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.82	0.23	0.32	-0.18	0.21	0.31	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.12	0.19	0.24	-0.29	0.17	0.25	2	1	0.44	0.18	0.23	1.24	0.17	0.25	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1230-1724	54	5952	100	3.98	0.24	0.34	-2.30	0.12	0.17	1.39	0.15	0.25	6.22	0.17	0.23	0.13	0.17	0.26	1	1	5.50	0.12	0.18	0.22	0.15	0.23	7	4	3.17	0.14	0.22	-1.00	0.16	0.25	1	1	4.36	0.11	0.20	0.30	0.14	0.24	9	8	0.86	0.18	0.23	-0.01	0.16	0.26	5	2	2.91	0.16	0.21	0.18	0.15	0.24	17	8	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.19	0.15	0.21	-0.19	0.16	0.23	3	3	2.42	0.16	0.20	-0.67	0.15	0.23	5	3	5.20	0.12	0.17	0.00	0.14	0.22	55	44	2.57	0.15	0.21	-0.05	0.15	0.25	6	2	3.72	0.20	0.24	-0.23	0.18	0.25	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	0.61	0.20	0.29	-0.07	0.19	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.34	0.18	0.23	-0.18	0.17	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1237-3103	48	4851	100	1.72	0.26	0.36	-2.91	0.13	0.18	2.04	0.13	0.23	5.42	0.20	0.27	-0.06	0.18	0.28	1	1	4.88	0.12	0.18	0.21	0.15	0.23	7	6	2.72	0.16	0.26	-0.84	0.18	0.28	1	1	3.69	0.12	0.20	0.24	0.15	0.25	9	8	0.31	0.18	0.23	0.05	0.16	0.24	5	4	2.30	0.15	0.20	0.19	0.15	0.23	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.22	0.17	0.23	-0.54	0.16	0.24	3	3	2.13	0.19	0.26	-0.35	0.17	0.25	5	3	4.59	0.13	0.18	0.00	0.14	0.22	55	50	2.25	0.16	0.22	0.24	0.15	0.24	6	6	3.29	0.17	0.26	-0.05	0.17	0.26	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.13	0.23	0.33	-0.19	0.21	0.32	3	2	-1.01	0.18	0.23	-0.34	0.16	0.24	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.38	0.22	0.27	-0.60	0.19	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1243-1425	50	5507	100	3.19	0.26	0.36	-2.67	0.12	0.18	1.11	0.15	0.25	6.23	0.18	0.25	0.51	0.18	0.27	1	1	5.13	0.12	0.18	0.22	0.15	0.24	7	2	2.74	0.16	0.23	-1.06	0.17	0.26	1	1	3.89	0.11	0.20	0.20	0.15	0.25	9	7	0.76	0.18	0.23	0.26	0.17	0.26	5	4	2.60	0.16	0.21	0.25	0.15	0.24	17	9	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.76	0.16	0.23	-0.25	0.16	0.24	3	3	1.83	0.16	0.20	-0.89	0.16	0.24	5	3	4.83	0.12	0.18	0.00	0.14	0.22	55	38	2.58	0.16	0.22	0.33	0.16	0.25	6	4	4.01	0.17	0.27	0.43	0.17	0.25	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.54	0.18	0.28	0.23	0.18	0.27	3	1	-0.14	0.19	0.24	0.28	0.18	0.27	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.94	0.20	0.24	-0.41	0.18	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1245-1616	47	6191	100	4.04	0.32	0.42	-2.98	0.13	0.18	1.53	0.17	0.27	6.19	0.21	0.28	0.77	0.26	0.34	1	1	-9.99	0.00	0.00	-9.99	0.00	0.00	7	0	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	3.88	0.12	0.20	0.50	0.15	0.25	9	3	0.39	0.19	0.24	0.19	0.17	0.26	5	1	2.61	0.17	0.23	0.57	0.16	0.25	17	5	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.56	0.15	0.19	-0.13	0.15	0.23	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	4.53	0.13	0.18	0.00	0.14	0.22	55	20	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	3.12	0.15	0.19	-0.15	0.16	0.23	4	1	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.26	0.22	0.30	0.26	0.20	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.56	0.19	0.24	0.28	0.17	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1246-1344	49	4853	100	1.65	0.27	0.37	-3.40	0.14	0.19	1.84	0.13	0.23	4.93	0.20	0.27	-0.06	0.19	0.29	1	1	4.68	0.12	0.19	0.50	0.15	0.24	7	5	2.33	0.17	0.25	-0.74	0.18	0.27	1	1	3.35	0.12	0.20	0.39	0.15	0.25	9	6	0.12	0.18	0.22	0.35	0.15	0.23	5	4	1.87	0.16	0.21	0.25	0.15	0.23	17	11	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.82	0.16	0.21	-0.45	0.15	0.23	3	3	1.08	0.17	0.21	-0.91	0.16	0.23	5	3	4.10	0.14	0.19	0.00	0.14	0.22	55	39	1.64	0.15	0.22	0.12	0.15	0.24	6	3	2.84	0.17	0.23	-0.01	0.16	0.24	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-1.68	0.19	0.26	-1.25	0.17	0.26	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1247-2114	54	5012	100	2.08	0.25	0.35	-2.61	0.12	0.18	1.67	0.12	0.22	6.10	0.19	0.26	0.32	0.18	0.28	1	1	5.21	0.11	0.19	0.25	0.15	0.24	7	7	2.89	0.16	0.25	-0.96	0.18	0.27	1	1	3.94	0.11	0.20	0.20	0.15	0.24	9	8	0.56	0.19	0.24	0.00	0.16	0.25	5	4	2.57	0.16	0.21	0.17	0.15	0.23	17	15	1.41	0.15	0.20	0.02	0.15	0.23	3	1	2.74	0.17	0.27	-0.32	0.17	0.26	3	3	2.36	0.15	0.21	-0.42	0.15	0.23	5	3	4.89	0.12	0.18	0.00	0.14	0.22	55	53	2.39	0.16	0.22	0.08	0.15	0.24	6	6	3.60	0.18	0.29	-0.04	0.18	0.29	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.72	0.14	0.22	0.37	0.15	0.24	3	2	-0.34	0.18	0.23	0.04	0.16	0.25	6	6	0.41	0.18	0.22	0.42	0.16	0.25	3	1	-0.91	0.22	0.28	-0.43	0.20	0.28	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.88	0.18	0.23	0.22	0.16	0.25	4	1
HE 1248-1800	43	5288	100	2.92	0.27	0.37	-2.89	0.14	0.19	1.47	0.14	0.24	6.02	0.19	0.25	0.53	0.17	0.27	1	1	4.95	0.11	0.20	0.27	0.16	0.25	7	4	2.87	0.18	0.26	-0.71	0.19	0.27	1	1	3.71	0.12	0.20	0.24	0.15	0.25	9	6	0.33	0.18	0.23	0.05	0.16	0.25	5	3	2.45	0.16	0.21	0.32	0.15	0.23	17	10	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.28	0.16	0.21	-0.50	0.15	0.22	3	3	1.83	0.17	0.21	-0.67	0.15	0.23	5	3	4.61	0.14	0.19	0.00	0.14	0.22	55	39	2.22	0.16	0.22	0.20	0.15	0.24	6	5	3.27	0.18	0.24	-0.09	0.16	0.23	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.18	0.23	0.33	-0.25	0.21	0.32	3	2	-0.85	0.19	0.24	-0.20	0.17	0.25	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.89	0.20	0.25	-0.12	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1249-2932	56	4718	100	1.52	0.24	0.34	-2.65	0.13	0.18	2.09	0.12	0.22	5.32	0.20	0.26	-0.41	0.18	0.27	1	1	5.03	0.12	0.18	0.11	0.15	0.23	7	6	3.07	0.17	0.26	-0.75	0.18	0.27	1	1	3.73	0.12	0.20	0.03	0.15	0.25	9	8	0.48	0.18	0.23	-0.03	0.16	0.24	5	5	2.44	0.16	0.21	0.07	0.15	0.23	17	16	1.31	0.15	0.19	-0.04	0.15	0.23	3	3	2.76	0.13	0.28	-0.26	0.15	0.27	3	3	2.57	0.14	0.19	-0.17	0.15	0.23	5	5	4.85	0.13	0.18	0.00	0.14	0.22	55	55	2.26	0.15	0.22	-0.00	0.15	0.24	6	6	3.93	0.16	0.28	0.33	0.16	0.27	4	4	2.42	0.13	0.20	0.47	0.14	0.25	2	2	-0.56	0.23	0.33	-0.88	0.21	0.31	3	1	-1.52	0.19	0.23	-1.11	0.16	0.25	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.73	0.18	0.23	-1.20	0.16	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1249-3121	47	5373	100	3.40	0.30	0.40	-3.23	0.14	0.19	1.58	0.18	0.28	7.01	0.18	0.26	1.86	0.17	0.27	1	1	4.61	0.14	0.23	0.26	0.20	0.29	5	3	2.43	0.31	0.36	-0.81	0.25	0.35	1	1	3.51	0.14	0.26	0.38	0.22	0.32	5	2	0.53	0.21	0.26	0.59	0.18	0.26	3	1	2.22	0.17	0.22	0.43	0.15	0.24	11	5	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	2.16	0.17	0.22	-0.28	0.16	0.23	1	1	1.67	0.19	0.23	-0.49	0.17	0.25	4	2	4.27	0.14	0.19	0.00	0.14	0.22	35	17	2.03	0.16	0.22	0.34	0.15	0.25	4	3	2.98	0.17	0.21	-0.03	0.15	0.22	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	1	0	-1.24	0.20	0.26	-0.98	0.17	0.27	2	2	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	7	0	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0
HE 1251-0104	53	5084	100	2.32	0.24	0.34	-2.73	0.13	0.18	1.58	0.13	0.23	5.91	0.19	0.25	0.25	0.18	0.27	1	1	4.91	0.11	0.18	0.06	0.15	0.24	7	6	2.62	0.16	0.24	-1.12	0.17	0.26	1	1	3.79	0.12	0.20	0.16	0.15	0.25	9	7	0.35	0.17	0.22	-0.09	0.15	0.24	5	4	2.46	0.16	0.21	0.17	0.15	0.23	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.55	0.17	0.25	-0.39	0.16	0.24	3	3	2.05	0.17	0.22	-0.61	0.15	0.23	5	3	4.77	0.13	0.18	0.00	0.14	0.22	55	50	2.28	0.16	0.22	0.09	0.15	0.24	6	5	3.55	0.18	0.28	0.03	0.17	0.27	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.02	0.21	0.31	-0.22	0.20	0.30	3	2	-0.85	0.19	0.24	-0.36	0.16	0.25	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.97	0.20	0.25	-0.37	0.18	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1252+0044	44	5296	100	2.98	0.29	0.39	-3.28	0.14	0.19	1.57	0.15	0.25	5.70	0.19	0.26	0.60	0.18	0.28	1	1	4.81	0.12	0.20	0.51	0.18	0.26	7	4	2.51	0.15	0.23	-0.68	0.16	0.25	1	1	3.56	0.12	0.20	0.48	0.15	0.25	9	3	-0.05	0.19	0.24	0.06	0.17	0.25	5	1	2.10	0.17	0.22	0.36	0.15	0.24	17	7	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.11	0.15	0.20	-0.28	0.15	0.23	3	3	1.36	0.17	0.21	-0.75	0.16	0.24	5	3	4.22	0.14	0.19	0.00	0.14	0.22	55	31	1.88	0.16	0.22	0.24	0.15	0.25	6	2	3.08	0.16	0.21	0.11	0.15	0.22	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.39	0.19	0.28	0.70	0.18	0.28	3	2	-0.41	0.19	0.24	0.64	0.17	0.25	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.68	0.20	0.24	-0.53	0.17	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1252-0117	53	4847	100	1.67	0.26	0.36	-2.89	0.11	0.18	1.88	0.13	0.23	5.38	0.20	0.27	-0.16	0.22	0.31	1	1	4.86	0.12	0.18	0.14	0.16	0.25	7	6	2.79	0.20	0.29	-0.82	0.22	0.29	1	1	3.44	0.12	0.20	-0.06	0.15	0.26	9	7	0.05	0.18	0.23	-0.26	0.18	0.28	5	4	2.17	0.16	0.21	0.01	0.17	0.25	17	14	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.22	0.16	0.23	-0.59	0.17	0.24	3	3	2.56	0.14	0.19	0.03	0.16	0.24	5	4	4.64	0.11	0.18	0.00	0.14	0.22	55	52	2.66	0.15	0.22	0.59	0.17	0.25	6	6	4.10	0.17	0.30	0.71	0.18	0.27	4	4	2.30	0.14	0.21	0.55	0.16	0.27	2	1	-0.88	0.22	0.32	-0.99	0.22	0.31	3	2	-1.51	0.19	0.23	-0.89	0.19	0.29	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-2.38	0.19	0.23	-1.65	0.19	0.29	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1254+0009	54	4865	100	1.86	0.25	0.35	-2.94	0.14	0.19	1.78	0.13	0.23	5.34	0.20	0.26	-0.11	0.18	0.28	1	1	4.89	0.12	0.19	0.26	0.15	0.24	7	5	2.78	0.19	0.28	-0.74	0.20	0.29	1	1	3.63	0.12	0.20	0.21	0.15	0.25	9	8	0.33	0.17	0.22	0.11	0.15	0.23	5	4	2.32	0.16	0.21	0.25	0.15	0.23	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.23	0.16	0.23	-0.49	0.15	0.24	3	3	1.62	0.16	0.21	-0.82	0.15	0.23	5	3	4.55	0.14	0.19	0.00	0.14	0.22	55	51	2.09	0.16	0.22	0.11	0.15	0.24	6	6	3.32	0.18	0.28	0.02	0.17	0.27	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.32	0.23	0.34	-0.35	0.21	0.32	3	2	-1.30	0.19	0.24	-0.59	0.16	0.24	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.67	0.19	0.23	-0.86	0.16	0.24	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1256-0228	48	4860	100	1.83	0.25	0.35	-2.07	0.12	0.20	1.69	0.13	0.23	6.27	0.21	0.26	-0.04	0.19	0.28	1	1	5.77	0.11	0.19	0.27	0.15	0.24	7	6	3.61	0.16	0.24	-0.77	0.18	0.27	1	1	4.57	0.12	0.21	0.29	0.15	0.25	9	8	1.38	0.17	0.24	0.30	0.16	0.25	5	5	3.10	0.17	0.23	0.16	0.16	0.25	17	16	1.77	0.16	0.20	-0.15	0.15	0.24	3	3	3.33	0.17	0.30	-0.26	0.17	0.27	3	3	2.93	0.14	0.19	-0.38	0.15	0.24	5	5	5.42	0.12	0.20	0.00	0.14	0.22	55	51	2.81	0.21	0.27	-0.02	0.18	0.26	6	6	4.59	0.15	0.25	0.42	0.16	0.23	4	3	2.83	0.14	0.21	0.31	0.15	0.26	2	2	0.89	0.14	0.21	0.00	0.15	0.25	3	1	0.11	0.19	0.25	-0.05	0.17	0.27	6	5	0.79	0.18	0.23	0.27	0.16	0.27	3	2	0.17	0.22	0.28	0.12	0.20	0.28	2	1	-0.64	0.18	0.23	0.28	0.16	0.27	6	4	-0.15	0.18	0.25	0.35	0.16	0.28	10	5	-0.15	0.18	0.23	0.43	0.16	0.27	9	8	-0.25	0.18	0.23	0.82	0.16	0.27	8	2	-1.07	0.18	0.23	0.51	0.16	0.27	4	3
HE 1256-0651	44	6137	100	4.05	0.28	0.38	-2.36	0.13	0.18	1.50	0.16	0.26	6.65	0.20	0.26	0.62	0.23	0.31	1	1	5.44	0.12	0.18	0.22	0.15	0.24	7	2	3.06	0.15	0.22	-1.06	0.16	0.25	1	1	4.33	0.11	0.20	0.32	0.15	0.25	9	7	0.88	0.18	0.23	0.06	0.17	0.26	5	2	2.96	0.16	0.21	0.30	0.15	0.24	17	6	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.15	0.15	0.20	-0.17	0.15	0.23	3	3	2.48	0.15	0.20	-0.56	0.15	0.23	5	3	5.15	0.13	0.18	0.00	0.14	0.22	55	34	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	3.95	0.17	0.22	0.06	0.16	0.23	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.27	0.20	0.28	-0.35	0.18	0.28	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.49	0.19	0.23	-0.26	0.17	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1259-0621	44	5787	100	3.68	0.25	0.35	-2.64	0.13	0.18	1.60	0.14	0.24	6.16	0.17	0.24	0.41	0.17	0.27	1	1	5.26	0.10	0.17	0.32	0.16	0.24	7	2	2.92	0.15	0.22	-0.91	0.16	0.25	1	1	3.99	0.12	0.20	0.28	0.15	0.25	9	7	0.61	0.18	0.23	0.08	0.16	0.25	5	2	2.77	0.15	0.21	0.40	0.15	0.23	17	9	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.71	0.15	0.20	-0.31	0.15	0.22	3	3	2.16	0.16	0.20	-0.59	0.15	0.23	5	3	4.86	0.13	0.18	0.00	0.14	0.22	55	36	2.62	0.15	0.21	0.35	0.15	0.25	6	3	3.52	0.17	0.21	-0.09	0.16	0.23	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.40	0.21	0.30	0.08	0.20	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.48	0.19	0.24	0.04	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1300+0157	56	5411	100	3.38	0.34	0.44	-3.76	0.13	0.19	1.43	0.17	0.27	5.82	0.20	0.27	1.17	0.20	0.29	1	1	4.25	0.15	0.24	0.40	0.19	0.27	7	3	1.90	0.15	0.22	-0.83	0.17	0.27	1	1	3.10	0.13	0.22	0.47	0.15	0.25	9	1	-0.30	0.19	0.24	0.26	0.20	0.29	5	1	1.62	0.16	0.22	0.34	0.18	0.28	17	5	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.56	0.16	0.20	-0.37	0.17	0.25	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	3.76	0.13	0.19	0.00	0.14	0.22	55	18	1.69	0.19	0.25	0.50	0.20	0.30	6	1	2.48	0.12	0.17	-0.04	0.15	0.23	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.94	0.16	0.22	0.56	0.22	0.31	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1300-0641	44	5308	100	2.96	0.29	0.39	-3.14	0.13	0.18	1.59	0.15	0.25	6.54	0.18	0.26	1.29	0.17	0.27	1	1	4.48	0.12	0.21	0.04	0.17	0.26	7	3	2.12	0.15	0.22	-1.21	0.16	0.25	1	1	3.23	0.11	0.20	0.01	0.17	0.26	9	2	-0.01	0.19	0.24	-0.04	0.17	0.25	5	2	1.87	0.17	0.22	-0.01	0.15	0.25	17	6	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.36	0.16	0.22	-0.17	0.15	0.23	3	3	1.80	0.17	0.22	-0.44	0.16	0.23	5	2	4.36	0.13	0.18	0.00	0.14	0.22	55	34	1.90	0.16	0.22	0.12	0.15	0.25	6	3	3.41	0.18	0.25	0.30	0.17	0.25	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.77	0.22	0.29	-0.59	0.20	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	-1.78	0.20	0.24	-0.77	0.17	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1300-0642	43	5173	100	2.68	0.27	0.37	-3.03	0.12	0.18	1.57	0.14	0.24	5.71	0.19	0.26	0.34	0.19	0.28	1	1	4.82	0.11	0.19	0.26	0.16	0.25	7	3	2.31	0.16	0.23	-1.14	0.17	0.26	1	1	3.65	0.12	0.20	0.31	0.15	0.25	9	4	0.32	0.18	0.23	0.17	0.17	0.26	5	4	2.30	0.16	0.21	0.30	0.16	0.24	17	10	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.25	0.17	0.22	-0.40	0.16	0.23	3	3	1.63	0.17	0.21	-0.74	0.16	0.24	5	3	4.48	0.12	0.18	0.00	0.14	0.22	55	40	2.12	0.16	0.22	0.22	0.16	0.25	6	4	3.25	0.17	0.24	0.02	0.17	0.24	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.27	0.25	0.34	-0.22	0.22	0.33	3	2	-0.80	0.19	0.24	-0.02	0.18	0.26	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.27	0.19	0.24	-0.38	0.18	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1300-2201	52	6332	100	4.64	0.28	0.38	-2.61	0.11	0.17	1.34	0.15	0.25	6.80	0.16	0.23	1.01	0.17	0.27	1	1	5.27	0.12	0.18	0.29	0.15	0.24	7	1	2.95	0.13	0.21	-0.92	0.15	0.25	1	1	4.05	0.11	0.20	0.29	0.15	0.25	9	3	0.76	0.18	0.23	0.19	0.18	0.27	5	1	2.80	0.16	0.22	0.38	0.17	0.26	17	5	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.97	0.14	0.19	-0.11	0.16	0.23	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	4.90	0.11	0.17	0.00	0.14	0.22	55	30	2.72	0.14	0.21	0.39	0.16	0.25	6	1	3.58	0.15	0.19	-0.07	0.16	0.23	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.65	0.19	0.27	0.28	0.19	0.28	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.51	0.18	0.23	-0.04	0.18	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0
HE 1300-2431	47	5029	100	1.96	0.27	0.37	-3.25	0.14	0.19	1.92	0.13	0.23	4.98	0.24	0.30	-0.16	0.21	0.31	1	1	4.73	0.12	0.18	0.40	0.16	0.24	7	5	2.49	0.17	0.25	-0.73	0.18	0.27	1	1	3.39	0.12	0.20	0.28	0.15	0.25	9	3	0.15	0.18	0.23	0.23	0.15	0.23	5	4	2.44	0.15	0.20	0.67	0.14	0.22	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.09	0.16	0.21	-0.33	0.15	0.23	3	3	1.29	0.16	0.21	-0.84	0.15	0.23	5	3	4.25	0.14	0.19	0.00	0.14	0.22	55	41	2.11	0.15	0.22	0.44	0.15	0.24	6	5	3.22	0.19	0.25	0.22	0.16	0.24	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.67	0.24	0.33	-0.39	0.21	0.31	3	2	-1.05	0.19	0.23	-0.04	0.16	0.24	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.57	0.18	0.23	-0.45	0.15	0.24	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1305-0331	46	6081	100	4.22	0.38	0.48	-3.26	0.13	0.18	1.58	0.19	0.29	6.26	0.19	0.26	1.13	0.20	0.29	1	1	-9.99	0.00	0.00	-9.99	0.00	0.00	7	0	2.49	0.14	0.21	-0.72	0.16	0.25	1	1	3.50	0.13	0.21	0.40	0.15	0.25	9	1	0.32	0.20	0.25	0.41	0.20	0.28	5	1	2.29	0.19	0.25	0.53	0.19	0.28	17	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.24	0.15	0.19	-0.17	0.15	0.23	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	4.24	0.13	0.18	0.00	0.14	0.22	55	17	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	2.99	0.16	0.20	-0.01	0.16	0.23	4	1	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.46	0.20	0.26	-0.17	0.19	0.28	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1311-1412	56	4796	100	1.50	0.25	0.35	-2.91	0.13	0.18	1.92	0.12	0.22	5.35	0.20	0.27	-0.15	0.18	0.28	1	1	4.96	0.12	0.18	0.26	0.15	0.23	7	7	2.97	0.18	0.27	-0.62	0.18	0.28	1	1	3.62	0.13	0.20	0.14	0.14	0.25	9	8	0.22	0.17	0.22	-0.07	0.15	0.24	5	4	2.26	0.15	0.20	0.13	0.14	0.23	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.42	0.16	0.25	-0.37	0.15	0.25	3	3	1.91	0.16	0.22	-0.60	0.15	0.23	5	3	4.62	0.13	0.18	0.00	0.14	0.22	55	52	2.10	0.16	0.22	0.06	0.15	0.24	6	5	3.26	0.18	0.28	-0.10	0.18	0.27	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.03	0.22	0.33	-0.06	0.20	0.32	3	1	-0.96	0.18	0.22	-0.32	0.15	0.24	6	3	-0.01	0.18	0.22	0.27	0.15	0.24	3	1	-0.81	0.24	0.31	-0.06	0.21	0.29	2	1	-1.48	0.18	0.23	0.23	0.16	0.24	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-1.13	0.18	0.23	0.25	0.16	0.24	9	1	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.84	0.18	0.23	0.53	0.15	0.24	4	4
HE 1314-3036	82	4757	100	1.54	0.23	0.33	-2.99	0.12	0.18	1.88	0.11	0.21	5.27	0.20	0.27	-0.13	0.19	0.28	1	1	4.92	0.11	0.18	0.32	0.15	0.23	7	7	2.61	0.14	0.24	-0.87	0.15	0.26	1	1	3.60	0.12	0.20	0.23	0.14	0.25	9	8	0.23	0.17	0.22	0.04	0.15	0.24	5	5	2.24	0.14	0.19	0.21	0.14	0.22	17	16	0.99	0.15	0.20	-0.02	0.15	0.23	3	2	2.34	0.15	0.24	-0.35	0.15	0.24	3	3	1.77	0.14	0.21	-0.64	0.15	0.23	5	3	4.52	0.12	0.18	0.00	0.14	0.22	55	53	2.09	0.15	0.22	0.16	0.15	0.24	6	6	3.03	0.16	0.25	-0.23	0.16	0.24	4	4	2.01	0.13	0.20	0.39	0.14	0.25	2	1	-0.13	0.20	0.31	-0.12	0.19	0.29	3	2	-1.02	0.18	0.22	-0.27	0.16	0.24	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.90	0.19	0.27	-0.05	0.18	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-2.30	0.18	0.22	0.17	0.16	0.25	4	1
HE 1320-1339	291	4935	100	1.69	0.22	0.32	-2.78	0.13	0.18	1.97	0.10	0.20	5.10	0.19	0.26	-0.51	0.18	0.28	1	1	5.05	0.11	0.18	0.25	0.15	0.23	7	7	2.89	0.12	0.23	-0.80	0.14	0.25	1	1	3.84	0.11	0.20	0.26	0.15	0.25	9	8	0.66	0.16	0.22	0.27	0.15	0.23	5	5	2.49	0.15	0.21	0.25	0.14	0.23	17	17	1.23	0.15	0.19	0.01	0.15	0.23	3	2	2.56	0.15	0.23	-0.33	0.14	0.24	3	3	2.04	0.15	0.22	-0.56	0.14	0.23	5	3	4.72	0.13	0.18	0.00	0.14	0.22	55	54	2.29	0.16	0.22	0.16	0.15	0.24	6	6	3.89	0.16	0.28	0.43	0.15	0.27	4	4	2.25	0.13	0.20	0.43	0.14	0.24	2	2	0.42	0.17	0.27	0.23	0.16	0.26	3	2	-0.67	0.18	0.22	-0.13	0.15	0.23	6	6	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.08	0.19	0.24	-0.42	0.16	0.24	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-2.11	0.18	0.22	0.16	0.15	0.24	4	1
HE 1330-0354	47	6257	100	4.13	0.27	0.37	-2.29	0.12	0.18	1.49	0.15	0.25	7.15	0.16	0.24	1.05	0.18	0.27	1	1	5.61	0.11	0.17	0.32	0.15	0.23	7	2	3.25	0.14	0.22	-0.93	0.16	0.25	1	1	4.47	0.11	0.19	0.40	0.15	0.25	9	8	1.24	0.18	0.23	0.36	0.17	0.25	5	2	3.27	0.16	0.21	0.54	0.15	0.24	17	8	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.33	0.15	0.20	-0.05	0.15	0.23	3	3	2.55	0.15	0.19	-0.55	0.15	0.23	5	3	5.21	0.12	0.18	0.00	0.14	0.22	55	36	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	3.88	0.16	0.20	-0.08	0.16	0.23	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.69	0.21	0.30	0.01	0.19	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.63	0.18	0.23	-0.47	0.17	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1330-0607	41	5094	100	2.30	0.24	0.34	-2.33	0.13	0.19	1.90	0.14	0.24	6.27	0.19	0.25	0.21	0.17	0.26	1	1	5.35	0.12	0.18	0.10	0.15	0.23	7	5	3.31	0.18	0.26	-0.83	0.19	0.28	1	1	4.26	0.12	0.20	0.23	0.15	0.25	9	7	0.82	0.18	0.23	-0.02	0.16	0.25	5	4	2.87	0.17	0.23	0.18	0.15	0.24	17	14	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.35	0.20	0.29	0.01	0.19	0.27	3	2	2.84	0.15	0.20	-0.22	0.15	0.23	5	4	5.17	0.13	0.19	0.00	0.14	0.22	55	52	2.78	0.16	0.23	0.19	0.15	0.24	6	6	3.74	0.20	0.27	-0.18	0.19	0.26	4	4	2.64	0.14	0.21	0.37	0.15	0.25	2	1	0.19	0.23	0.34	-0.45	0.22	0.32	3	2	-0.40	0.19	0.24	-0.31	0.16	0.25	6	3	0.51	0.18	0.23	0.24	0.16	0.25	3	1	-0.96	0.23	0.27	-0.76	0.20	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.57	0.19	0.23	0.25	0.16	0.25	4	1
HE 1332-0309	38	5125	100	2.40	0.26	0.36	-2.46	0.13	0.18	1.64	0.14	0.24	6.14	0.19	0.26	0.21	0.18	0.27	1	1	5.25	0.12	0.19	0.13	0.15	0.24	7	5	3.05	0.16	0.25	-0.96	0.19	0.28	1	1	4.11	0.12	0.20	0.21	0.14	0.24	9	8	0.82	0.18	0.23	0.11	0.16	0.25	5	4	2.88	0.16	0.22	0.32	0.15	0.24	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.17	0.19	0.29	-0.03	0.18	0.27	3	3	2.49	0.16	0.22	-0.44	0.16	0.24	5	3	5.04	0.13	0.18	0.00	0.14	0.22	55	51	2.60	0.17	0.23	0.14	0.15	0.25	6	6	3.78	0.21	0.31	-0.01	0.20	0.29	4	4	2.71	0.14	0.21	0.57	0.15	0.26	2	1	0.81	0.15	0.24	0.30	0.16	0.25	3	2	-0.19	0.19	0.24	0.03	0.17	0.26	6	3	0.69	0.18	0.23	0.55	0.17	0.26	3	1	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-0.30	0.19	0.24	0.66	0.17	0.26	9	1	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.47	0.19	0.23	0.48	0.16	0.26	4	1
HE 1333-0340	41	6053	100	4.18	0.31	0.41	-2.64	0.12	0.18	1.37	0.19	0.29	-9.99	0.00	0.00	-9.99	0.00	0.00	1	0	5.18	0.12	0.18	0.24	0.16	0.25	7	1	3.01	0.17	0.24	-0.82	0.17	0.27	1	1	4.02	0.11	0.20	0.30	0.15	0.25	9	3	0.76	0.19	0.24	0.23	0.18	0.27	5	1	2.64	0.17	0.23	0.27	0.17	0.26	17	5	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.76	0.15	0.20	-0.27	0.15	0.23	3	3	2.19	0.15	0.19	-0.55	0.16	0.24	5	2	4.86	0.12	0.18	0.00	0.14	0.22	55	31	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	3.62	0.16	0.21	0.01	0.17	0.23	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.60	0.22	0.31	0.27	0.21	0.31	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1335+0135	50	5246	100	2.94	0.25	0.35	-2.47	0.12	0.18	1.34	0.13	0.23	6.06	0.20	0.26	0.13	0.18	0.26	1	1	5.39	0.12	0.18	0.28	0.14	0.23	7	5	3.07	0.16	0.24	-0.93	0.18	0.26	1	1	4.13	0.11	0.20	0.24	0.14	0.24	9	8	0.72	0.18	0.23	0.01	0.16	0.26	5	4	2.74	0.15	0.20	0.18	0.15	0.24	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.21	0.17	0.27	0.01	0.17	0.26	3	3	2.63	0.15	0.21	-0.29	0.16	0.24	5	3	5.03	0.12	0.18	0.00	0.14	0.22	55	49	2.56	0.17	0.23	0.11	0.16	0.25	6	6	3.95	0.17	0.27	0.17	0.17	0.26	4	4	2.68	0.14	0.21	0.55	0.15	0.26	2	1	0.54	0.16	0.25	0.04	0.17	0.26	3	2	-0.38	0.19	0.24	-0.15	0.17	0.27	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.11	0.19	0.24	-0.78	0.17	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1337+0012	229	6141	100	4.25	0.27	0.37	-3.44	0.13	0.18	1.49	0.12	0.22	5.66	0.19	0.25	0.71	0.18	0.27	1	1	4.69	0.12	0.18	0.55	0.15	0.23	7	1	2.38	0.13	0.20	-0.65	0.14	0.24	1	1	3.40	0.11	0.20	0.48	0.14	0.25	9	1	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	2.09	0.15	0.21	0.51	0.15	0.24	17	4	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	4.06	0.13	0.18	0.00	0.14	0.22	55	20	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	2.98	0.14	0.19	0.17	0.14	0.22	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.42	0.18	0.25	0.06	0.16	0.26	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.24	0.18	0.23	0.07	0.16	0.24	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1337-0453	50	5938	100	3.56	0.27	0.37	-2.34	0.13	0.18	1.62	0.13	0.23	6.17	0.19	0.26	0.12	0.19	0.28	1	1	5.62	0.12	0.18	0.38	0.15	0.24	7	3	3.06	0.14	0.22	-1.07	0.16	0.25	1	1	4.46	0.11	0.20	0.44	0.15	0.25	9	8	0.98	0.18	0.23	0.15	0.16	0.25	5	3	3.07	0.16	0.21	0.39	0.15	0.23	17	11	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.19	0.16	0.22	-0.14	0.15	0.23	3	3	2.50	0.15	0.20	-0.56	0.15	0.23	5	3	5.16	0.13	0.18	0.00	0.14	0.22	55	42	2.65	0.14	0.21	0.06	0.15	0.25	6	3	3.78	0.12	0.18	-0.14	0.17	0.24	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.78	0.18	0.29	0.15	0.17	0.28	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.45	0.19	0.24	-0.24	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1343-0640	43	5942	100	3.97	0.25	0.35	-1.90	0.11	0.17	1.48	0.14	0.24	7.26	0.17	0.23	0.77	0.17	0.26	1	1	6.05	0.11	0.18	0.37	0.14	0.23	7	5	3.72	0.15	0.24	-0.85	0.18	0.26	1	1	4.87	0.10	0.20	0.41	0.15	0.25	9	8	1.34	0.16	0.21	0.06	0.16	0.26	5	4	3.44	0.15	0.21	0.32	0.16	0.25	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.74	0.16	0.24	-0.04	0.17	0.25	3	3	3.06	0.16	0.21	-0.43	0.16	0.24	5	3	5.60	0.11	0.17	0.00	0.14	0.22	55	50	2.94	0.16	0.22	-0.08	0.16	0.26	6	2	4.14	0.26	0.31	-0.21	0.24	0.30	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	1.75	0.13	0.21	0.68	0.15	0.24	3	1	0.85	0.20	0.24	0.51	0.18	0.27	6	2	1.68	0.18	0.23	0.98	0.18	0.27	3	1	0.94	0.19	0.25	0.70	0.19	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1345-0206	34	5006	100	2.22	0.27	0.37	-2.82	0.14	0.19	1.65	0.14	0.24	5.91	0.20	0.26	0.34	0.18	0.28	1	1	4.87	0.13	0.19	0.11	0.16	0.24	7	4	2.53	0.17	0.24	-1.12	0.18	0.27	1	1	3.59	0.12	0.20	0.05	0.15	0.25	9	4	0.19	0.18	0.23	-0.16	0.16	0.24	5	3	2.16	0.17	0.22	-0.04	0.15	0.23	17	9	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.55	0.18	0.28	-0.30	0.18	0.28	3	3	1.79	0.17	0.23	-0.78	0.16	0.23	5	3	4.68	0.14	0.19	0.00	0.14	0.22	55	44	2.07	0.15	0.22	-0.03	0.15	0.24	6	4	3.03	0.21	0.26	-0.40	0.18	0.25	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.28	0.20	0.31	-0.43	0.18	0.30	3	2	-1.08	0.20	0.24	-0.50	0.17	0.25	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.79	0.20	0.24	-1.10	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1351-1049	45	5204	100	2.85	0.26	0.36	-3.46	0.13	0.18	1.48	0.16	0.26	6.49	0.18	0.26	1.55	0.18	0.28	1	1	4.43	0.12	0.21	0.30	0.17	0.27	5	3	2.25	0.15	0.22	-0.77	0.16	0.25	1	1	3.23	0.12	0.21	0.32	0.16	0.25	5	2	0.00	0.19	0.24	0.28	0.17	0.25	3	1	1.87	0.17	0.22	0.30	0.16	0.25	11	4	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	1.94	0.17	0.22	-0.28	0.16	0.24	1	1	1.32	0.17	0.21	-0.63	0.16	0.24	4	2	4.05	0.13	0.18	0.00	0.14	0.22	35	17	1.95	0.16	0.22	0.48	0.16	0.25	4	3	3.10	0.18	0.23	0.30	0.16	0.23	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	1	0	-0.45	0.23	0.32	0.03	0.21	0.30	2	2	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-1.18	0.20	0.24	0.13	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	7	0	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0
HE 1413-1954	48	6533	100	4.59	0.43	0.53	-3.22	0.12	0.17	1.40	0.16	0.26	6.65	0.22	0.30	1.45	0.24	0.32	1	1	-9.99	0.00	0.00	-9.99	0.00	0.00	7	0	-9.99	0.00	0.00	-9.99	0.00	0.00	1	0	3.50	0.13	0.22	0.33	0.15	0.25	9	1	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	-9.99	0.00	0.00	-9.99	0.00	0.00	17	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	4.31	0.12	0.17	0.00	0.14	0.22	54	14	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.69	0.21	0.28	-0.47	0.21	0.31	3	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1419-1759	45	4809	100	1.63	0.25	0.35	-3.18	0.13	0.18	1.83	0.13	0.23	5.02	0.20	0.27	-0.20	0.19	0.29	1	1	4.68	0.11	0.18	0.27	0.15	0.23	7	5	2.34	0.18	0.26	-0.95	0.19	0.28	1	1	3.47	0.12	0.20	0.29	0.15	0.25	9	7	0.07	0.17	0.22	0.07	0.16	0.24	5	4	1.98	0.16	0.21	0.13	0.15	0.23	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.02	0.16	0.23	-0.48	0.16	0.23	3	3	1.30	0.16	0.21	-0.92	0.15	0.23	5	3	4.33	0.13	0.18	0.00	0.14	0.22	55	46	1.89	0.16	0.22	0.15	0.15	0.25	6	6	3.07	0.18	0.27	-0.00	0.17	0.26	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.47	0.25	0.36	-0.26	0.23	0.34	3	2	-1.48	0.19	0.24	-0.54	0.17	0.25	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.85	0.19	0.23	-0.81	0.16	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1421-2006	49	5687	100	3.73	0.25	0.35	-2.65	0.12	0.18	1.33	0.14	0.24	6.04	0.17	0.24	0.30	0.17	0.26	1	1	5.31	0.10	0.17	0.37	0.15	0.23	7	3	2.86	0.15	0.22	-0.97	0.16	0.25	1	1	4.09	0.11	0.20	0.37	0.15	0.24	9	7	0.52	0.18	0.23	-0.01	0.17	0.26	5	2	2.62	0.15	0.20	0.25	0.15	0.24	17	6	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.74	0.14	0.20	-0.29	0.15	0.23	3	3	2.03	0.16	0.21	-0.72	0.16	0.24	5	3	4.85	0.12	0.18	0.00	0.14	0.22	55	37	2.29	0.16	0.22	0.02	0.16	0.25	6	2	3.37	0.16	0.21	-0.24	0.16	0.23	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.22	0.20	0.29	-0.10	0.20	0.30	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.65	0.19	0.23	-0.14	0.17	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1430+0053	71	5201	100	2.74	0.24	0.34	-3.03	0.13	0.18	1.55	0.13	0.23	5.65	0.18	0.25	0.29	0.17	0.27	1	1	4.77	0.11	0.19	0.21	0.16	0.25	7	6	2.47	0.14	0.22	-0.98	0.15	0.25	1	1	3.56	0.11	0.19	0.23	0.15	0.25	9	7	0.19	0.18	0.23	0.04	0.15	0.24	5	4	2.25	0.16	0.21	0.26	0.15	0.23	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.21	0.16	0.21	-0.43	0.15	0.23	3	3	1.59	0.16	0.21	-0.77	0.15	0.23	5	3	4.47	0.13	0.18	0.00	0.14	0.22	55	45	2.17	0.16	0.22	0.27	0.15	0.24	6	6	3.23	0.17	0.23	0.01	0.16	0.24	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.84	0.21	0.28	-0.78	0.18	0.28	3	2	-1.35	0.19	0.23	-0.57	0.16	0.25	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.99	0.21	0.25	-0.10	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.80	0.18	0.23	0.72	0.15	0.24	4	1
HE 1430-0026	53	5855	100	4.12	0.26	0.36	-2.79	0.11	0.17	1.38	0.14	0.24	6.13	0.17	0.24	0.52	0.17	0.26	1	1	5.09	0.11	0.17	0.29	0.15	0.23	7	2	2.79	0.14	0.21	-0.89	0.15	0.25	1	1	3.89	0.11	0.20	0.31	0.14	0.24	9	6	0.49	0.18	0.23	0.10	0.17	0.27	5	1	2.52	0.16	0.22	0.28	0.16	0.26	17	6	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.60	0.15	0.20	-0.29	0.15	0.23	3	3	2.02	0.16	0.20	-0.59	0.16	0.24	5	3	4.72	0.11	0.17	0.00	0.14	0.22	55	37	2.49	0.15	0.21	0.35	0.16	0.25	6	3	3.38	0.16	0.20	-0.09	0.16	0.23	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.03	0.19	0.27	-0.22	0.19	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.91	0.18	0.23	-0.26	0.17	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1430-1123	43	5915	100	3.75	0.29	0.39	-2.71	0.13	0.18	1.40	0.16	0.26	7.53	0.16	0.24	1.84	0.18	0.28	1	1	5.23	0.13	0.19	0.35	0.16	0.24	7	2	2.86	0.15	0.22	-0.91	0.16	0.26	1	1	4.13	0.11	0.20	0.47	0.15	0.25	9	5	0.84	0.18	0.23	0.37	0.17	0.26	5	2	2.57	0.17	0.22	0.25	0.16	0.25	17	5	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.97	0.16	0.21	-0.00	0.16	0.23	3	2	2.12	0.16	0.20	-0.57	0.16	0.24	5	3	4.80	0.13	0.18	0.00	0.14	0.22	55	31	2.61	0.14	0.20	0.39	0.15	0.25	6	2	3.34	0.17	0.21	-0.21	0.17	0.23	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.51	0.21	0.30	0.24	0.19	0.29	3	2	0.05	0.30	0.33	0.50	0.26	0.32	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.25	0.14	0.21	1.82	0.16	0.23	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	0.53	0.23	0.27	1.72	0.20	0.28	9	1	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1431-2142	53	6137	100	4.10	0.25	0.35	-2.60	0.13	0.18	1.55	0.14	0.24	6.28	0.17	0.24	0.48	0.18	0.28	1	1	5.34	0.12	0.18	0.35	0.15	0.23	7	2	2.85	0.14	0.21	-1.02	0.15	0.25	1	1	4.13	0.10	0.20	0.37	0.16	0.26	9	7	0.82	0.17	0.23	0.24	0.16	0.25	5	2	2.79	0.15	0.21	0.36	0.15	0.23	17	6	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.95	0.14	0.19	-0.13	0.15	0.22	3	3	2.30	0.15	0.19	-0.50	0.15	0.23	5	3	4.90	0.13	0.18	0.00	0.14	0.22	55	33	2.56	0.15	0.21	0.23	0.15	0.25	6	1	3.69	0.15	0.20	0.04	0.15	0.22	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.34	0.20	0.28	-0.03	0.18	0.28	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.34	0.18	0.23	0.13	0.16	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 1500-1628	45	4994	100	2.10	0.25	0.35	-2.31	0.12	0.18	1.85	0.13	0.23	6.21	0.20	0.26	0.13	0.18	0.27	1	1	5.45	0.11	0.18	0.18	0.15	0.23	7	6	3.15	0.20	0.28	-1.01	0.21	0.29	1	1	3.87	0.12	0.20	-0.18	0.14	0.24	9	7	0.90	0.18	0.23	0.04	0.17	0.26	5	5	2.48	0.16	0.21	-0.23	0.15	0.24	17	15	1.52	0.16	0.20	-0.18	0.16	0.24	3	2	3.05	0.18	0.28	-0.31	0.18	0.27	3	3	2.80	0.15	0.20	-0.29	0.15	0.23	5	5	5.19	0.12	0.18	0.00	0.14	0.22	55	54	2.77	0.17	0.24	0.15	0.16	0.25	6	5	3.95	0.18	0.32	0.01	0.19	0.31	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-1.10	0.24	0.30	-1.76	0.20	0.30	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.85	0.19	0.23	-1.68	0.17	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2133-1432	46	5716	100	3.46	0.24	0.34	-2.02	0.12	0.18	1.46	0.13	0.23	6.49	0.17	0.24	0.12	0.17	0.26	1	1	5.90	0.12	0.18	0.33	0.15	0.23	7	4	3.67	0.12	0.23	-0.78	0.17	0.26	1	1	4.72	0.11	0.20	0.38	0.15	0.25	9	8	1.21	0.18	0.23	0.06	0.16	0.25	5	4	3.27	0.15	0.21	0.27	0.15	0.24	17	14	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.59	0.16	0.24	-0.06	0.16	0.24	3	3	2.89	0.16	0.22	-0.49	0.16	0.23	5	3	5.48	0.12	0.18	0.00	0.14	0.22	55	50	2.89	0.15	0.22	-0.01	0.15	0.25	6	4	4.03	0.15	0.24	-0.20	0.16	0.24	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	1.06	0.17	0.25	0.10	0.16	0.26	3	2	0.12	0.18	0.23	-0.10	0.16	0.26	6	2	1.10	0.18	0.23	0.52	0.17	0.26	3	1	0.06	0.22	0.27	-0.05	0.20	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2134+0001	37	5257	100	3.00	0.25	0.35	-2.22	0.12	0.19	1.55	0.14	0.24	6.38	0.21	0.26	0.20	0.18	0.27	1	1	5.75	0.12	0.18	0.38	0.14	0.23	7	4	3.42	0.16	0.25	-0.83	0.18	0.27	1	1	4.54	0.12	0.21	0.40	0.14	0.24	9	8	1.00	0.18	0.23	0.05	0.16	0.26	5	3	3.04	0.17	0.22	0.24	0.16	0.25	17	14	1.78	0.16	0.20	0.00	0.15	0.24	3	1	3.48	0.16	0.26	0.03	0.17	0.26	3	3	2.89	0.11	0.22	-0.28	0.19	0.26	5	3	5.28	0.12	0.19	0.00	0.14	0.22	55	52	2.85	0.17	0.23	0.14	0.16	0.25	6	5	3.87	0.20	0.29	-0.16	0.20	0.28	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.67	0.17	0.25	-0.08	0.17	0.27	3	2	-0.22	0.19	0.24	-0.24	0.17	0.27	6	2	0.76	0.18	0.23	0.38	0.16	0.27	3	1	-0.51	0.25	0.29	-0.42	0.23	0.31	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	-1.24	0.19	0.24	0.47	0.16	0.27	4	1
HE 2139-1851	83	4925	100	1.86	0.25	0.35	-3.25	0.13	0.18	1.78	0.12	0.22	5.64	0.19	0.26	0.49	0.18	0.28	1	1	4.70	0.11	0.18	0.36	0.15	0.24	7	6	2.31	0.14	0.22	-0.92	0.15	0.25	1	1	3.44	0.12	0.20	0.33	0.15	0.25	9	7	-0.02	0.17	0.22	0.06	0.15	0.24	5	4	2.04	0.16	0.21	0.26	0.15	0.23	17	13	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.01	0.15	0.21	-0.41	0.15	0.23	3	3	1.23	0.16	0.21	-0.91	0.15	0.23	5	3	4.26	0.13	0.18	0.00	0.14	0.22	55	47	1.92	0.15	0.22	0.25	0.15	0.24	6	6	2.95	0.16	0.23	-0.05	0.15	0.23	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.02	0.20	0.32	0.29	0.19	0.31	3	2	-1.06	0.18	0.23	-0.05	0.16	0.24	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-2.01	0.18	0.23	-0.90	0.16	0.24	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2143+0030	43	4688	100	1.50	0.25	0.35	-2.43	0.12	0.19	1.91	0.12	0.22	5.60	0.21	0.26	-0.36	0.18	0.27	1	1	5.37	0.11	0.19	0.22	0.15	0.23	7	7	3.33	0.17	0.26	-0.71	0.19	0.27	1	1	4.04	0.12	0.20	0.11	0.14	0.25	9	8	0.66	0.16	0.21	-0.08	0.15	0.25	5	5	2.70	0.16	0.21	0.11	0.15	0.24	17	17	1.38	0.15	0.20	-0.19	0.15	0.23	3	3	2.99	0.17	0.30	-0.24	0.16	0.26	3	3	2.62	0.14	0.19	-0.34	0.15	0.23	5	4	5.07	0.12	0.19	0.00	0.14	0.22	55	52	2.41	0.17	0.24	-0.08	0.16	0.25	6	6	3.98	0.19	0.30	0.17	0.19	0.27	4	4	2.45	0.14	0.21	0.28	0.15	0.27	2	1	0.45	0.18	0.25	-0.09	0.17	0.26	3	2	-0.57	0.18	0.23	-0.37	0.15	0.26	6	5	0.21	0.17	0.22	0.04	0.15	0.26	3	2	-0.68	0.28	0.35	-0.38	0.25	0.33	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.93	0.18	0.23	-0.01	0.15	0.27	4	3
HE 2145-3025	26	5608	100	2.22	0.29	0.39	-2.69	0.14	0.19	2.47	0.15	0.25	-9.99	0.00	0.00	-9.99	0.00	0.00	1	0	5.25	0.12	0.18	0.36	0.16	0.24	7	1	3.04	0.17	0.23	-0.73	0.17	0.26	1	1	4.02	0.12	0.20	0.35	0.15	0.25	9	1	0.65	0.18	0.23	0.17	0.16	0.24	5	2	2.67	0.17	0.22	0.35	0.15	0.23	17	5	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.80	0.16	0.21	-0.18	0.15	0.23	3	3	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	4.81	0.14	0.19	0.00	0.14	0.22	55	25	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	3.49	0.17	0.22	-0.07	0.16	0.23	4	1	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.74	0.27	0.37	0.46	0.25	0.36	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.87	0.20	0.25	-0.31	0.17	0.24	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2150-0825	39	5960	100	3.67	0.26	0.36	-1.98	0.12	0.18	1.57	0.15	0.25	7.76	0.16	0.23	1.35	0.17	0.27	1	1	5.95	0.12	0.18	0.36	0.15	0.24	7	5	3.40	0.17	0.24	-1.09	0.18	0.26	1	1	4.83	0.11	0.20	0.46	0.15	0.25	9	8	1.41	0.18	0.23	0.22	0.16	0.26	5	4	3.35	0.16	0.21	0.31	0.15	0.24	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.76	0.17	0.25	0.07	0.17	0.25	3	3	3.03	0.15	0.20	-0.37	0.15	0.23	5	3	5.52	0.12	0.18	0.00	0.14	0.22	55	47	2.95	0.15	0.22	0.02	0.16	0.25	6	3	3.99	0.17	0.23	-0.27	0.17	0.24	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	1.64	0.15	0.23	0.66	0.16	0.25	3	1	1.10	0.18	0.23	0.85	0.17	0.25	6	5	1.59	0.18	0.23	0.97	0.17	0.26	3	1	1.85	0.14	0.19	1.70	0.15	0.22	2	2	0.60	0.16	0.22	1.41	0.16	0.25	6	5	1.08	0.18	0.25	1.48	0.17	0.28	10	1	0.93	0.18	0.23	1.42	0.17	0.26	9	2	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2151-2858	42	5598	100	4.14	0.25	0.35	-2.38	0.11	0.18	1.39	0.15	0.25	6.11	0.19	0.24	0.10	0.18	0.26	1	1	5.57	0.12	0.18	0.37	0.14	0.24	7	4	3.48	0.12	0.25	-0.61	0.17	0.27	1	1	4.28	0.12	0.20	0.30	0.14	0.24	9	8	0.85	0.18	0.23	0.06	0.18	0.28	5	3	2.91	0.13	0.19	0.27	0.15	0.24	17	10	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.17	0.15	0.22	-0.12	0.16	0.24	3	3	2.48	0.16	0.21	-0.53	0.17	0.25	5	2	5.12	0.11	0.18	0.00	0.14	0.22	55	41	2.64	0.16	0.22	0.10	0.16	0.26	6	4	3.75	0.16	0.24	-0.12	0.18	0.25	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.31	0.18	0.26	-0.29	0.19	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	-0.50	0.20	0.24	-0.26	0.19	0.29	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2153-2719	73	4898	100	2.01	0.23	0.33	-2.49	0.12	0.18	1.80	0.12	0.22	6.02	0.21	0.27	0.12	0.19	0.27	1	1	5.46	0.11	0.18	0.36	0.15	0.23	7	6	3.47	0.13	0.24	-0.51	0.15	0.25	1	1	4.20	0.12	0.20	0.33	0.14	0.24	9	9	0.82	0.18	0.23	0.14	0.15	0.25	5	4	2.77	0.16	0.21	0.24	0.15	0.23	17	17	1.52	0.16	0.20	0.01	0.15	0.23	3	3	3.10	0.15	0.28	-0.08	0.16	0.27	3	3	2.50	0.14	0.20	-0.41	0.15	0.23	5	5	5.01	0.12	0.18	0.00	0.14	0.22	55	54	2.44	0.16	0.23	0.01	0.15	0.24	6	6	3.62	0.16	0.28	-0.15	0.17	0.27	4	4	2.31	0.13	0.20	0.19	0.14	0.25	2	2	0.48	0.15	0.24	-0.00	0.15	0.25	3	2	-0.46	0.19	0.24	-0.22	0.16	0.26	6	6	0.30	0.17	0.22	0.19	0.15	0.25	3	2	-1.05	0.19	0.25	-0.69	0.18	0.26	2	1	-1.42	0.18	0.23	-0.11	0.15	0.26	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-1.01	0.19	0.23	-0.03	0.16	0.26	9	2	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.77	0.18	0.22	0.21	0.15	0.25	4	3
HE 2154-2838	44	5303	100	3.18	0.25	0.35	-1.85	0.12	0.19	1.46	0.14	0.24	6.58	0.20	0.25	0.05	0.17	0.27	1	1	5.91	0.11	0.18	0.18	0.14	0.23	7	5	3.96	0.14	0.23	-0.66	0.17	0.26	1	1	4.78	0.12	0.21	0.28	0.14	0.24	9	9	1.51	0.17	0.22	0.20	0.16	0.27	5	5	3.39	0.16	0.21	0.23	0.16	0.25	17	17	2.13	0.16	0.20	-0.01	0.15	0.25	3	3	3.83	0.14	0.24	0.02	0.16	0.24	3	3	3.26	0.15	0.20	-0.28	0.15	0.24	5	5	5.65	0.12	0.19	0.00	0.14	0.22	55	53	3.18	0.18	0.24	0.11	0.17	0.26	6	5	4.19	0.17	0.27	-0.20	0.18	0.26	4	4	2.78	0.14	0.21	0.03	0.15	0.27	2	1	1.15	0.14	0.22	0.03	0.15	0.25	3	2	0.30	0.18	0.23	-0.08	0.17	0.28	6	5	1.15	0.18	0.23	0.40	0.17	0.28	3	2	0.24	0.21	0.29	-0.03	0.22	0.30	2	1	-0.55	0.19	0.23	0.14	0.16	0.29	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-0.89	0.19	0.24	0.45	0.16	0.29	4	3
HE 2155+0136	37	5331	100	3.22	0.25	0.35	-2.07	0.12	0.19	1.23	0.15	0.25	6.32	0.20	0.25	-0.00	0.18	0.27	1	1	5.73	0.11	0.18	0.22	0.15	0.23	7	5	3.44	0.17	0.25	-0.96	0.18	0.27	1	1	4.66	0.12	0.21	0.37	0.14	0.24	9	8	1.07	0.18	0.23	-0.03	0.17	0.28	5	4	3.16	0.15	0.21	0.21	0.16	0.26	17	13	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.52	0.15	0.26	-0.08	0.17	0.25	3	3	3.01	0.15	0.20	-0.32	0.16	0.24	5	3	5.43	0.12	0.19	0.00	0.14	0.22	55	52	3.00	0.16	0.24	0.15	0.16	0.26	6	6	4.22	0.19	0.28	0.04	0.19	0.28	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.78	0.16	0.24	-0.13	0.17	0.26	3	2	-0.05	0.19	0.24	-0.22	0.18	0.29	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	0.20	0.21	0.28	0.13	0.21	0.29	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-0.87	0.18	0.23	0.68	0.17	0.29	4	3
HE 2156-3130	60	4692	100	1.28	0.26	0.36	-3.13	0.13	0.18	1.93	0.13	0.23	6.00	0.20	0.27	0.74	0.19	0.29	1	1	5.22	0.11	0.19	0.77	0.15	0.24	5	5	3.27	0.15	0.25	-0.07	0.17	0.27	1	1	3.53	0.11	0.20	0.31	0.15	0.25	5	4	0.42	0.19	0.24	0.39	0.16	0.25	3	3	2.05	0.15	0.20	0.16	0.15	0.22	11	10	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	2.17	0.17	0.26	-0.37	0.17	0.26	1	1	1.71	0.11	0.23	-0.55	0.16	0.26	4	2	4.37	0.13	0.18	0.00	0.14	0.22	35	34	2.04	0.15	0.22	0.26	0.15	0.24	4	3	2.91	0.17	0.26	-0.21	0.16	0.26	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	1	0	-1.06	0.20	0.30	-0.89	0.19	0.29	2	2	-1.79	0.19	0.24	-0.90	0.17	0.25	4	1	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.48	0.22	0.31	0.52	0.20	0.29	2	1	-1.64	0.18	0.22	0.32	0.16	0.24	3	1	-9.99	0.00	0.00	-9.99	0.00	0.00	7	0	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0
HE 2158-3112	85	4843	100	1.85	0.23	0.33	-2.75	0.12	0.18	1.85	0.11	0.21	5.61	0.20	0.26	-0.04	0.18	0.27	1	1	5.13	0.11	0.18	0.29	0.15	0.23	7	6	3.02	0.14	0.24	-0.71	0.16	0.26	1	1	3.80	0.11	0.20	0.18	0.15	0.24	9	8	0.57	0.17	0.22	0.14	0.15	0.24	5	5	2.44	0.16	0.21	0.16	0.15	0.23	17	17	1.21	0.15	0.20	-0.05	0.15	0.23	3	2	2.59	0.16	0.25	-0.34	0.16	0.25	3	3	2.28	0.14	0.21	-0.37	0.15	0.23	5	4	4.76	0.12	0.18	0.00	0.14	0.22	55	53	2.33	0.15	0.22	0.14	0.15	0.24	6	6	3.46	0.17	0.27	-0.05	0.17	0.26	4	4	2.07	0.13	0.20	0.21	0.14	0.25	2	1	0.03	0.18	0.29	-0.20	0.18	0.28	3	2	-0.79	0.18	0.23	-0.29	0.16	0.25	6	4	-0.10	0.18	0.22	0.04	0.15	0.25	3	1	-1.45	0.19	0.23	-0.84	0.16	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-2.21	0.18	0.23	0.02	0.16	0.25	4	1
HE 2200-2030	40	5870	100	3.42	0.27	0.37	-2.00	0.12	0.18	1.64	0.15	0.25	6.49	0.17	0.24	0.10	0.18	0.28	1	1	5.82	0.12	0.18	0.24	0.15	0.24	7	4	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	4.67	0.11	0.20	0.32	0.15	0.25	9	8	1.20	0.18	0.23	0.03	0.17	0.26	5	3	3.26	0.16	0.22	0.25	0.16	0.24	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.58	0.18	0.25	-0.09	0.17	0.25	3	3	2.96	0.18	0.23	-0.43	0.17	0.24	5	3	5.50	0.12	0.18	0.00	0.14	0.22	55	48	2.89	0.15	0.21	-0.03	0.16	0.25	6	3	4.08	0.19	0.26	-0.16	0.18	0.25	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.90	0.21	0.31	-0.07	0.19	0.29	3	2	-0.06	0.19	0.24	-0.30	0.18	0.27	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	0.09	0.23	0.28	-0.03	0.20	0.28	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2201-0637	43	4976	100	2.21	0.25	0.35	-2.61	0.11	0.18	1.69	0.13	0.23	5.93	0.20	0.26	0.14	0.21	0.29	1	1	5.18	0.12	0.19	0.19	0.15	0.24	7	5	2.91	0.21	0.28	-0.96	0.22	0.29	1	1	4.00	0.12	0.20	0.24	0.15	0.25	9	8	0.56	0.18	0.23	-0.01	0.18	0.27	5	4	2.57	0.15	0.21	0.15	0.16	0.24	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.82	0.18	0.28	-0.26	0.18	0.26	3	3	2.11	0.18	0.25	-0.69	0.18	0.25	5	3	4.91	0.11	0.18	0.00	0.14	0.22	55	52	2.35	0.23	0.29	0.02	0.22	0.31	6	5	3.64	0.21	0.31	-0.02	0.20	0.29	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.28	0.20	0.28	-0.10	0.19	0.28	3	2	-0.64	0.19	0.23	-0.28	0.18	0.28	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.13	0.20	0.24	-0.66	0.20	0.29	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2204-1703	36	4932	100	1.87	0.27	0.37	-2.79	0.12	0.18	1.84	0.13	0.23	5.81	0.20	0.26	0.21	0.20	0.29	1	1	5.16	0.12	0.19	0.36	0.15	0.24	7	6	3.27	0.20	0.29	-0.41	0.21	0.30	1	1	3.77	0.12	0.20	0.20	0.15	0.25	9	6	0.61	0.18	0.23	0.23	0.17	0.25	5	4	2.44	0.17	0.22	0.21	0.16	0.24	17	14	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.59	0.18	0.27	-0.29	0.18	0.26	3	3	1.87	0.17	0.23	-0.73	0.17	0.24	5	3	4.71	0.12	0.18	0.00	0.14	0.22	55	45	2.41	0.15	0.22	0.27	0.16	0.25	6	4	3.49	0.21	0.30	0.03	0.20	0.28	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.35	0.26	0.36	-0.53	0.24	0.34	3	2	-0.95	0.19	0.24	-0.40	0.18	0.26	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.41	0.22	0.26	-0.75	0.20	0.28	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2206-2245	45	5100	100	2.45	0.25	0.35	-2.73	0.12	0.18	1.70	0.13	0.23	5.87	0.19	0.26	0.21	0.18	0.27	1	1	5.17	0.11	0.19	0.32	0.15	0.24	7	6	2.82	0.17	0.25	-0.92	0.18	0.27	1	1	3.99	0.12	0.20	0.36	0.15	0.25	9	8	0.58	0.18	0.23	0.14	0.16	0.25	5	3	2.55	0.16	0.21	0.26	0.15	0.24	17	13	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.67	0.18	0.25	-0.27	0.17	0.25	3	3	2.11	0.18	0.24	-0.55	0.17	0.24	5	2	4.77	0.12	0.18	0.00	0.14	0.22	55	48	2.38	0.16	0.23	0.20	0.15	0.25	6	6	3.52	0.19	0.28	0.00	0.18	0.26	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.19	0.19	0.30	-0.05	0.19	0.29	3	2	-0.70	0.19	0.24	-0.21	0.17	0.26	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.71	0.23	0.28	-0.11	0.20	0.28	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.61	0.19	0.23	0.62	0.16	0.26	4	1
HE 2216-0621	42	4671	100	1.27	0.27	0.37	-3.23	0.13	0.18	2.02	0.12	0.22	4.50	0.21	0.28	-0.66	0.20	0.30	1	1	4.57	0.12	0.19	0.22	0.15	0.23	7	5	2.40	0.18	0.27	-0.84	0.21	0.30	1	1	3.27	0.12	0.20	0.14	0.15	0.25	9	5	0.05	0.16	0.21	0.11	0.15	0.24	5	4	1.87	0.15	0.20	0.08	0.15	0.23	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.93	0.15	0.22	-0.51	0.15	0.23	3	3	1.61	0.13	0.21	-0.55	0.15	0.24	5	3	4.27	0.13	0.18	0.00	0.14	0.22	55	43	1.94	0.14	0.21	0.24	0.15	0.24	6	5	3.37	0.19	0.30	0.35	0.19	0.30	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.75	0.24	0.34	-0.49	0.22	0.33	3	2	-1.48	0.19	0.24	-0.49	0.17	0.25	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-2.36	0.19	0.23	-1.27	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2216-1548	75	5154	100	1.73	0.24	0.34	-1.70	0.14	0.20	2.69	0.12	0.22	6.31	0.19	0.25	-0.38	0.18	0.27	1	1	6.05	0.11	0.18	0.17	0.15	0.24	7	5	3.88	0.15	0.26	-0.89	0.17	0.26	1	1	4.85	0.13	0.21	0.19	0.15	0.25	9	9	1.41	0.16	0.22	-0.06	0.14	0.23	5	5	3.44	0.16	0.22	0.11	0.14	0.23	17	17	2.17	0.15	0.20	-0.13	0.15	0.23	3	3	3.56	0.18	0.27	-0.41	0.16	0.25	3	2	3.39	0.14	0.19	-0.30	0.15	0.23	5	5	5.80	0.14	0.20	0.00	0.14	0.22	55	52	3.30	0.16	0.23	0.08	0.15	0.24	6	6	4.53	0.20	0.29	-0.02	0.17	0.25	4	4	2.96	0.13	0.20	0.06	0.14	0.25	2	2	1.32	0.16	0.22	0.05	0.15	0.24	3	2	0.40	0.18	0.23	-0.14	0.15	0.24	6	6	1.20	0.18	0.23	0.30	0.14	0.24	3	3	0.72	0.16	0.22	0.29	0.14	0.23	2	2	-0.34	0.18	0.22	0.19	0.14	0.24	6	5	0.03	0.18	0.25	0.15	0.15	0.27	10	5	0.00	0.18	0.23	0.20	0.15	0.24	9	8	-0.29	0.18	0.23	0.40	0.15	0.25	8	3	-0.61	0.18	0.23	0.58	0.15	0.25	4	4
HE 2217-0706	45	4497	100	1.01	0.24	0.34	-2.56	0.12	0.19	2.13	0.12	0.22	5.27	0.21	0.27	-0.55	0.19	0.28	1	1	5.34	0.11	0.18	0.33	0.15	0.24	7	5	3.37	0.17	0.27	-0.52	0.18	0.27	1	1	4.02	0.11	0.20	0.23	0.15	0.25	9	8	0.65	0.17	0.22	0.05	0.15	0.24	5	5	2.54	0.15	0.20	0.09	0.15	0.23	17	17	1.31	0.16	0.20	-0.11	0.16	0.24	3	3	2.53	0.18	0.28	-0.56	0.17	0.25	3	3	2.42	0.15	0.20	-0.39	0.16	0.24	5	5	4.92	0.12	0.19	0.00	0.14	0.22	55	52	2.39	0.16	0.23	0.05	0.15	0.24	6	6	3.71	0.22	0.33	0.03	0.21	0.29	4	4	2.20	0.13	0.20	0.17	0.14	0.26	2	2	0.20	0.18	0.27	-0.20	0.18	0.27	3	1	-0.68	0.18	0.22	-0.34	0.15	0.25	6	6	0.03	0.17	0.22	0.01	0.15	0.25	3	2	-1.01	0.24	0.30	-0.57	0.21	0.28	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-1.34	0.19	0.23	-0.26	0.16	0.26	9	2	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-2.21	0.18	0.23	-0.15	0.16	0.26	4	3
HE 2217-1523	48	4847	100	1.82	0.25	0.35	-2.62	0.13	0.19	1.81	0.13	0.23	5.80	0.20	0.26	0.04	0.18	0.27	1	1	5.28	0.10	0.18	0.32	0.16	0.24	7	6	3.19	0.18	0.28	-0.66	0.20	0.29	1	1	4.05	0.11	0.20	0.31	0.15	0.25	9	8	0.65	0.19	0.24	0.11	0.16	0.25	5	5	2.62	0.16	0.22	0.23	0.15	0.23	17	17	1.31	0.16	0.20	-0.07	0.16	0.24	3	1	2.64	0.17	0.27	-0.41	0.17	0.26	3	3	2.33	0.14	0.21	-0.44	0.15	0.23	5	3	4.88	0.13	0.19	0.00	0.14	0.22	55	53	2.40	0.16	0.23	0.10	0.15	0.24	6	6	3.57	0.20	0.31	-0.06	0.19	0.29	4	4	2.26	0.14	0.21	0.29	0.15	0.25	2	1	0.20	0.18	0.28	-0.14	0.18	0.27	3	2	-0.67	0.20	0.24	-0.29	0.16	0.26	6	4	0.06	0.18	0.23	0.09	0.16	0.25	3	1	-1.01	0.23	0.29	-0.52	0.20	0.28	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2219-0713	55	4789	100	1.68	0.25	0.35	-2.91	0.12	0.18	1.64	0.13	0.23	5.30	0.20	0.27	-0.17	0.19	0.28	1	1	4.91	0.12	0.18	0.25	0.15	0.23	7	7	2.52	0.16	0.25	-1.03	0.17	0.27	1	1	3.62	0.12	0.20	0.17	0.14	0.25	9	8	0.15	0.17	0.22	-0.10	0.16	0.25	5	4	2.15	0.15	0.21	0.05	0.15	0.23	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.43	0.17	0.27	-0.32	0.16	0.26	3	3	1.91	0.14	0.22	-0.56	0.15	0.23	5	3	4.58	0.12	0.18	0.00	0.14	0.22	55	52	2.00	0.16	0.22	0.00	0.15	0.25	6	5	3.23	0.18	0.29	-0.10	0.18	0.27	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.27	0.22	0.34	-0.32	0.21	0.32	3	2	-1.30	0.19	0.23	-0.62	0.17	0.26	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-2.15	0.19	0.23	-1.36	0.17	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2221-4150	53	5887	100	4.06	0.24	0.34	-2.03	0.11	0.17	1.41	0.14	0.24	6.59	0.16	0.23	0.23	0.17	0.25	1	1	5.87	0.11	0.17	0.32	0.14	0.23	7	4	3.43	0.14	0.22	-1.01	0.16	0.26	1	1	4.64	0.11	0.20	0.31	0.14	0.24	9	8	1.19	0.17	0.22	0.05	0.17	0.27	5	4	3.24	0.16	0.21	0.25	0.16	0.25	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.48	0.15	0.23	-0.16	0.16	0.25	3	3	2.91	0.15	0.21	-0.45	0.16	0.24	5	3	5.47	0.11	0.17	0.00	0.14	0.22	55	47	2.95	0.15	0.21	0.06	0.15	0.25	6	4	4.06	0.17	0.23	-0.16	0.17	0.25	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.96	0.16	0.25	0.02	0.17	0.27	3	2	0.13	0.18	0.23	-0.08	0.17	0.27	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	0.19	0.20	0.24	0.09	0.19	0.28	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2222-4156	51	5537	100	3.27	0.24	0.34	-2.73	0.12	0.18	1.44	0.14	0.24	6.08	0.17	0.24	0.42	0.17	0.27	1	1	5.28	0.12	0.21	0.42	0.20	0.27	7	2	2.82	0.15	0.23	-0.93	0.16	0.25	1	1	3.99	0.11	0.20	0.35	0.15	0.25	9	7	0.47	0.17	0.23	0.03	0.16	0.25	5	2	2.62	0.16	0.21	0.33	0.15	0.24	17	9	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.73	0.16	0.22	-0.21	0.16	0.23	3	3	1.95	0.16	0.21	-0.71	0.16	0.24	5	3	4.77	0.12	0.18	0.00	0.14	0.22	55	38	2.26	0.16	0.22	0.07	0.15	0.25	6	3	3.51	0.18	0.24	-0.02	0.17	0.24	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.30	0.21	0.31	0.06	0.19	0.30	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.76	0.19	0.23	-0.16	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2224+0143	88	5198	100	2.66	0.24	0.34	-2.58	0.12	0.18	1.67	0.12	0.22	6.16	0.19	0.25	0.35	0.17	0.26	1	1	5.32	0.11	0.18	0.32	0.15	0.23	7	6	2.90	0.14	0.23	-0.98	0.15	0.25	1	1	4.07	0.13	0.20	0.29	0.14	0.24	9	8	0.72	0.17	0.22	0.13	0.15	0.25	5	5	2.74	0.16	0.21	0.31	0.15	0.23	17	16	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.88	0.16	0.24	-0.21	0.16	0.24	3	3	2.34	0.16	0.22	-0.47	0.15	0.23	5	3	4.92	0.12	0.18	0.00	0.14	0.22	55	54	2.57	0.16	0.22	0.24	0.15	0.24	6	6	3.63	0.17	0.25	-0.04	0.16	0.25	4	4	2.29	0.14	0.21	0.27	0.14	0.25	2	1	0.62	0.15	0.24	0.23	0.15	0.25	3	2	-0.22	0.18	0.23	0.13	0.16	0.25	6	5	0.60	0.18	0.22	0.58	0.15	0.25	3	1	0.13	0.20	0.27	0.59	0.18	0.27	2	1	-0.77	0.18	0.23	0.65	0.15	0.25	6	4	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-0.47	0.18	0.23	0.61	0.16	0.25	9	2	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.02	0.18	0.23	1.05	0.15	0.25	4	4
HE 2224-4103	49	5074	100	2.32	0.25	0.35	-2.64	0.12	0.17	1.75	0.12	0.22	6.02	0.20	0.26	0.23	0.19	0.28	1	1	5.34	0.11	0.19	0.36	0.15	0.24	7	6	3.10	0.16	0.25	-0.77	0.17	0.26	1	1	4.12	0.12	0.20	0.36	0.15	0.25	9	8	0.74	0.18	0.23	0.18	0.17	0.25	5	4	2.68	0.16	0.21	0.27	0.15	0.24	17	15	1.47	0.16	0.20	0.07	0.16	0.24	3	1	2.78	0.17	0.26	-0.29	0.17	0.26	3	3	2.26	0.14	0.22	-0.53	0.15	0.24	5	3	4.90	0.12	0.17	0.00	0.14	0.22	55	52	2.46	0.16	0.22	0.15	0.16	0.25	6	5	3.51	0.19	0.27	-0.13	0.18	0.26	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.27	0.18	0.29	-0.10	0.18	0.29	3	2	-0.66	0.19	0.24	-0.29	0.18	0.26	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.04	0.20	0.25	-0.57	0.18	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2226-4102	49	5140	100	2.43	0.26	0.36	-2.87	0.13	0.19	1.73	0.13	0.23	5.98	0.19	0.26	0.46	0.18	0.27	1	1	4.95	0.12	0.18	0.23	0.15	0.24	7	6	2.60	0.16	0.24	-1.01	0.16	0.26	1	1	3.75	0.12	0.20	0.26	0.15	0.25	9	7	0.40	0.18	0.23	0.10	0.16	0.25	5	4	2.33	0.16	0.21	0.17	0.15	0.24	17	11	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.48	0.17	0.24	-0.32	0.16	0.24	3	3	1.98	0.17	0.22	-0.55	0.15	0.23	5	3	4.63	0.13	0.19	0.00	0.14	0.22	55	45	2.30	0.16	0.22	0.25	0.15	0.24	6	6	3.27	0.18	0.24	-0.11	0.16	0.24	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.05	0.22	0.33	-0.06	0.20	0.31	3	2	-0.77	0.19	0.23	-0.15	0.16	0.25	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.74	0.19	0.23	-1.00	0.16	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2227-4044	49	5811	100	3.85	0.25	0.35	-2.32	0.11	0.17	1.40	0.14	0.24	7.75	0.16	0.23	1.67	0.17	0.26	1	1	5.56	0.11	0.18	0.30	0.15	0.23	5	2	3.42	0.14	0.23	-0.73	0.16	0.25	1	1	4.43	0.11	0.21	0.39	0.15	0.25	5	4	1.17	0.18	0.23	0.32	0.17	0.26	3	2	2.94	0.15	0.20	0.24	0.15	0.24	11	8	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	3.33	0.17	0.24	-0.03	0.17	0.25	1	1	2.54	0.16	0.21	-0.54	0.16	0.24	4	2	5.18	0.11	0.17	0.00	0.14	0.22	35	26	2.65	0.16	0.22	0.05	0.16	0.25	4	2	3.79	0.16	0.22	-0.14	0.16	0.23	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	1	0	1.06	0.14	0.24	0.41	0.15	0.25	2	2	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	1.19	0.17	0.21	1.38	0.17	0.24	2	1	0.13	0.18	0.23	1.28	0.17	0.26	3	1	-9.99	0.00	0.00	-9.99	0.00	0.00	7	0	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0
HE 2228-3806	50	5175	100	2.62	0.27	0.37	-3.07	0.13	0.18	1.65	0.14	0.24	5.74	0.19	0.26	0.42	0.18	0.27	1	1	4.84	0.11	0.19	0.33	0.15	0.24	7	4	2.43	0.15	0.22	-0.97	0.16	0.25	1	1	3.64	0.12	0.20	0.35	0.15	0.25	9	7	0.23	0.18	0.23	0.12	0.16	0.25	5	4	2.25	0.16	0.22	0.30	0.15	0.24	17	10	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.17	0.16	0.21	-0.43	0.15	0.23	3	3	1.58	0.16	0.21	-0.74	0.15	0.23	5	3	4.43	0.13	0.18	0.00	0.14	0.22	55	40	2.15	0.16	0.22	0.30	0.15	0.24	6	5	3.11	0.18	0.24	-0.07	0.16	0.24	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.29	0.23	0.32	-0.19	0.21	0.31	3	2	-1.03	0.19	0.24	-0.20	0.17	0.26	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.51	0.19	0.24	-0.57	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2229-4153	74	5138	100	2.47	0.24	0.34	-2.62	0.12	0.18	1.79	0.12	0.22	6.17	0.19	0.26	0.37	0.19	0.28	1	1	5.29	0.12	0.18	0.29	0.15	0.23	7	5	3.09	0.14	0.24	-0.79	0.16	0.26	1	1	4.11	0.11	0.20	0.34	0.14	0.25	9	8	0.71	0.18	0.23	0.13	0.16	0.25	5	5	2.65	0.16	0.21	0.22	0.15	0.23	17	14	1.46	0.15	0.20	0.05	0.15	0.24	3	1	2.84	0.16	0.24	-0.25	0.16	0.24	3	3	2.33	0.16	0.22	-0.47	0.16	0.23	5	3	4.91	0.12	0.18	0.00	0.14	0.22	55	53	2.51	0.16	0.22	0.18	0.15	0.25	6	6	3.48	0.17	0.26	-0.19	0.17	0.25	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.47	0.17	0.26	0.09	0.16	0.26	3	2	-0.46	0.18	0.23	-0.12	0.16	0.26	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.74	0.21	0.26	-0.28	0.18	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.63	0.18	0.23	0.45	0.16	0.26	4	1
HE 2231-0622	22	5211	100	2.90	0.27	0.37	-2.12	0.13	0.19	1.50	0.15	0.25	6.19	0.20	0.26	-0.08	0.18	0.26	1	1	5.62	0.12	0.18	0.15	0.15	0.23	7	5	2.96	0.31	0.37	-1.39	0.33	0.39	1	1	4.43	0.11	0.21	0.19	0.15	0.25	9	8	0.91	0.19	0.24	-0.14	0.18	0.28	5	4	3.02	0.15	0.21	0.11	0.17	0.25	17	13	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.43	0.20	0.29	-0.12	0.20	0.29	3	3	2.91	0.17	0.21	-0.36	0.17	0.25	5	3	5.38	0.13	0.19	0.00	0.14	0.22	55	43	2.78	0.17	0.23	-0.03	0.17	0.26	6	5	3.53	0.29	0.35	-0.61	0.29	0.35	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.35	0.25	0.33	-0.50	0.25	0.34	3	2	-0.17	0.21	0.26	-0.29	0.20	0.30	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.45	0.30	0.35	-0.46	0.31	0.37	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2234-0521	34	5332	100	3.15	0.25	0.35	-2.78	0.13	0.18	1.39	0.15	0.25	5.97	0.19	0.25	0.36	0.17	0.26	1	1	5.13	0.11	0.19	0.32	0.16	0.25	7	5	2.60	0.17	0.24	-1.09	0.17	0.26	1	1	3.88	0.12	0.20	0.30	0.15	0.25	9	6	0.58	0.18	0.23	0.19	0.16	0.25	5	3	2.54	0.17	0.22	0.30	0.15	0.24	17	9	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.50	0.17	0.23	-0.39	0.16	0.24	3	3	1.92	0.17	0.21	-0.69	0.16	0.23	5	3	4.72	0.13	0.18	0.00	0.14	0.22	55	39	2.44	0.16	0.22	0.29	0.15	0.25	6	5	3.56	0.15	0.21	0.09	0.15	0.22	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.11	0.23	0.32	-0.30	0.22	0.31	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.49	0.20	0.24	-0.84	0.17	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2238-2152	48	5427	100	3.28	0.25	0.35	-2.40	0.12	0.18	1.46	0.13	0.23	6.12	0.19	0.25	0.13	0.17	0.26	1	1	5.37	0.11	0.18	0.19	0.15	0.23	7	6	2.89	0.16	0.24	-1.18	0.17	0.26	1	1	4.19	0.12	0.20	0.23	0.14	0.25	9	7	0.70	0.18	0.23	-0.07	0.16	0.26	5	4	2.82	0.15	0.20	0.21	0.15	0.24	17	13	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.95	0.17	0.24	-0.32	0.16	0.24	3	3	2.41	0.17	0.22	-0.58	0.16	0.24	5	3	5.10	0.12	0.18	0.00	0.14	0.22	55	48	2.60	0.17	0.23	0.08	0.15	0.25	6	5	3.68	0.18	0.25	-0.17	0.17	0.25	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.28	0.20	0.29	-0.29	0.19	0.29	3	2	-0.50	0.17	0.22	-0.34	0.16	0.26	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.64	0.21	0.25	-0.37	0.18	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2240-0412	30	5852	100	4.33	0.29	0.39	-2.20	0.12	0.18	1.30	0.18	0.28	7.54	0.17	0.24	1.35	0.16	0.26	1	1	5.66	0.12	0.18	0.28	0.15	0.24	5	1	3.51	0.19	0.27	-0.76	0.21	0.29	1	1	4.39	0.12	0.21	0.23	0.15	0.25	5	3	1.09	0.19	0.24	0.12	0.19	0.27	3	1	3.06	0.14	0.19	0.25	0.15	0.24	11	8	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	3.31	0.19	0.26	-0.16	0.20	0.27	1	1	2.59	0.17	0.21	-0.60	0.17	0.24	4	2	5.30	0.12	0.18	0.00	0.14	0.22	35	24	2.91	0.16	0.22	0.19	0.16	0.25	4	2	4.04	0.18	0.25	-0.01	0.20	0.27	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	1	0	1.01	0.17	0.24	0.24	0.17	0.26	2	2	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	1.30	0.13	0.19	1.37	0.16	0.23	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	7	0	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0
HE 2242-1930	33	5281	100	2.99	0.26	0.36	-2.21	0.13	0.19	1.81	0.15	0.25	6.27	0.20	0.25	0.09	0.17	0.26	1	1	5.59	0.13	0.19	0.22	0.15	0.23	7	6	3.19	0.22	0.29	-1.07	0.23	0.30	1	1	4.49	0.12	0.20	0.34	0.15	0.25	9	8	0.99	0.18	0.23	0.03	0.17	0.26	5	4	3.05	0.17	0.22	0.24	0.16	0.24	17	14	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.18	0.19	0.27	-0.28	0.18	0.26	3	3	2.89	0.16	0.21	-0.29	0.16	0.24	5	3	5.29	0.13	0.19	0.00	0.14	0.22	55	49	2.95	0.18	0.24	0.24	0.16	0.25	6	5	4.10	0.21	0.30	0.06	0.21	0.29	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.72	0.20	0.28	-0.04	0.20	0.29	3	2	-0.01	0.19	0.24	-0.04	0.17	0.26	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.18	0.24	0.29	-0.10	0.22	0.30	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.15	0.19	0.24	0.56	0.17	0.27	4	1
HE 2243-0151	41	6113	100	3.88	0.25	0.35	-1.61	0.11	0.18	1.65	0.14	0.24	7.04	0.16	0.23	0.26	0.17	0.27	1	1	6.15	0.11	0.17	0.18	0.15	0.24	7	4	3.97	0.16	0.24	-0.89	0.19	0.27	1	1	5.11	0.11	0.20	0.36	0.15	0.24	9	8	1.59	0.18	0.23	0.03	0.17	0.27	5	4	3.79	0.15	0.21	0.38	0.16	0.24	17	14	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.99	0.16	0.24	-0.07	0.17	0.25	3	3	3.37	0.14	0.20	-0.41	0.16	0.23	5	3	5.89	0.11	0.18	0.00	0.14	0.22	55	48	3.42	0.15	0.21	0.11	0.16	0.25	6	4	4.82	0.18	0.26	0.18	0.19	0.26	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	1.50	0.17	0.25	0.14	0.17	0.26	3	2	0.82	0.18	0.23	0.19	0.17	0.27	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	0.51	0.23	0.28	-0.01	0.22	0.29	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	0.68	0.18	0.23	0.79	0.18	0.27	9	1	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2244-1503	46	5122	100	2.57	0.25	0.35	-2.88	0.12	0.18	1.52	0.13	0.23	5.67	0.19	0.26	0.15	0.19	0.28	1	1	5.01	0.12	0.18	0.30	0.15	0.23	7	5	2.65	0.18	0.26	-0.95	0.19	0.27	1	1	3.81	0.12	0.20	0.32	0.15	0.25	9	7	0.29	0.18	0.23	-0.01	0.16	0.26	5	3	2.47	0.16	0.21	0.32	0.15	0.24	17	14	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.58	0.17	0.25	-0.23	0.17	0.25	3	3	2.01	0.17	0.22	-0.51	0.16	0.24	5	3	4.63	0.12	0.18	0.00	0.14	0.22	55	43	2.24	0.16	0.22	0.19	0.16	0.25	6	5	3.50	0.19	0.28	0.12	0.19	0.27	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.10	0.22	0.32	-0.20	0.21	0.31	3	2	-0.78	0.19	0.23	-0.15	0.17	0.26	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.29	0.23	0.29	0.45	0.21	0.29	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.41	0.18	0.23	0.95	0.17	0.27	4	3
HE 2247-3705	57	5366	100	3.04	0.24	0.34	-2.27	0.12	0.18	1.48	0.12	0.22	6.48	0.19	0.25	0.36	0.18	0.26	1	1	5.46	0.11	0.18	0.14	0.15	0.23	7	4	3.19	0.15	0.24	-1.02	0.17	0.26	1	1	4.28	0.11	0.20	0.18	0.14	0.24	9	8	1.03	0.18	0.23	0.12	0.16	0.26	5	3	2.99	0.16	0.21	0.24	0.15	0.24	17	14	1.74	0.15	0.20	0.01	0.15	0.24	3	1	3.25	0.16	0.25	-0.15	0.17	0.25	3	3	2.88	0.15	0.20	-0.25	0.15	0.23	5	4	5.24	0.12	0.18	0.00	0.14	0.22	55	53	2.97	0.16	0.23	0.32	0.16	0.25	6	6	3.87	0.20	0.28	-0.11	0.20	0.27	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.38	0.19	0.28	-0.33	0.19	0.28	3	2	-0.48	0.19	0.23	-0.46	0.17	0.27	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.96	0.19	0.24	-0.83	0.17	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2248-3345	53	5011	100	2.11	0.25	0.35	-2.74	0.12	0.18	1.71	0.13	0.23	5.88	0.19	0.26	0.21	0.18	0.28	1	1	4.78	0.12	0.18	-0.08	0.15	0.24	7	5	2.49	0.16	0.24	-1.25	0.17	0.26	1	1	3.61	0.12	0.20	-0.02	0.15	0.25	9	7	-0.03	0.18	0.23	-0.47	0.16	0.25	5	4	2.11	0.16	0.21	-0.18	0.15	0.24	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.73	0.17	0.26	-0.22	0.16	0.25	3	3	2.39	0.15	0.20	-0.27	0.15	0.23	5	3	4.77	0.12	0.18	0.00	0.14	0.22	55	53	1.99	0.16	0.22	-0.21	0.16	0.25	6	5	3.45	0.19	0.28	-0.07	0.18	0.26	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-1.75	0.19	0.25	-1.99	0.17	0.27	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.97	0.19	0.23	-1.37	0.17	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2250-2132	54	5705	100	3.69	0.25	0.35	-2.22	0.12	0.18	1.43	0.13	0.23	6.58	0.17	0.24	0.41	0.17	0.26	1	1	5.68	0.11	0.17	0.31	0.14	0.23	7	5	3.19	0.15	0.23	-1.07	0.16	0.26	1	1	4.43	0.11	0.19	0.29	0.14	0.24	9	8	1.44	0.17	0.23	0.49	0.16	0.26	5	5	3.15	0.16	0.21	0.35	0.15	0.24	17	13	2.17	0.15	0.20	0.39	0.15	0.24	3	1	3.34	0.16	0.23	-0.12	0.16	0.24	3	3	2.83	0.16	0.20	-0.35	0.16	0.24	5	2	5.28	0.12	0.18	0.00	0.14	0.22	55	50	2.90	0.15	0.22	0.20	0.15	0.25	6	5	4.08	0.17	0.25	0.05	0.17	0.26	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.75	0.17	0.26	-0.00	0.17	0.27	3	2	-0.02	0.19	0.24	-0.04	0.17	0.27	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.40	0.19	0.24	-0.31	0.18	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2252-4157	70	5090	100	2.87	0.24	0.34	-1.93	0.12	0.18	1.55	0.12	0.22	6.31	0.22	0.27	-0.15	0.18	0.27	1	1	5.91	0.11	0.18	0.25	0.15	0.23	7	4	3.84	0.12	0.22	-0.70	0.15	0.25	1	1	4.71	0.12	0.21	0.28	0.14	0.24	9	9	1.35	0.14	0.20	0.11	0.16	0.25	5	5	3.28	0.17	0.22	0.19	0.16	0.25	17	17	2.07	0.16	0.21	-0.00	0.15	0.24	3	3	3.65	0.14	0.23	-0.10	0.15	0.24	3	3	3.27	0.16	0.24	-0.19	0.16	0.25	5	3	5.57	0.12	0.18	0.00	0.14	0.22	55	51	3.14	0.19	0.26	0.15	0.17	0.27	6	6	3.96	0.15	0.26	-0.37	0.17	0.27	4	4	2.79	0.13	0.21	0.12	0.14	0.26	2	2	1.05	0.14	0.21	0.01	0.15	0.24	3	2	0.22	0.18	0.23	-0.09	0.16	0.27	6	6	0.96	0.18	0.23	0.29	0.16	0.27	3	2	0.49	0.15	0.20	0.29	0.16	0.24	2	1	-0.65	0.18	0.23	0.11	0.16	0.27	6	5	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-0.25	0.18	0.23	0.18	0.16	0.27	9	2	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-0.89	0.18	0.23	0.53	0.15	0.27	4	4
HE 2252-4225	68	4708	100	1.53	0.24	0.34	-2.83	0.12	0.18	1.92	0.12	0.22	5.18	0.20	0.27	-0.39	0.19	0.28	1	1	4.94	0.11	0.18	0.17	0.15	0.23	7	6	2.87	0.14	0.26	-0.78	0.17	0.27	1	1	3.68	0.12	0.20	0.14	0.14	0.25	9	8	0.31	0.17	0.22	-0.04	0.16	0.24	5	5	2.49	0.15	0.20	0.29	0.15	0.23	17	16	1.12	0.16	0.20	-0.06	0.15	0.24	3	2	2.73	0.16	0.28	-0.12	0.16	0.26	3	3	2.49	0.13	0.19	-0.08	0.15	0.23	5	5	4.68	0.12	0.18	0.00	0.14	0.22	55	51	2.22	0.15	0.22	0.12	0.15	0.24	6	6	3.70	0.17	0.28	0.26	0.16	0.26	4	4	2.39	0.13	0.20	0.61	0.14	0.25	2	2	0.21	0.17	0.27	0.06	0.17	0.27	3	2	-0.54	0.18	0.22	0.04	0.16	0.25	6	6	0.16	0.18	0.22	0.38	0.16	0.25	3	2	-0.24	0.19	0.27	0.45	0.19	0.27	2	1	-1.08	0.18	0.22	0.57	0.16	0.25	6	5	-0.70	0.18	0.24	0.54	0.16	0.27	10	4	-0.71	0.18	0.23	0.60	0.16	0.25	9	5	-0.82	0.18	0.23	0.98	0.16	0.26	8	1	-1.32	0.18	0.22	0.99	0.16	0.25	4	4
HE 2258-3456	51	4988	100	1.55	0.26	0.36	-2.97	0.12	0.18	2.00	0.13	0.23	5.22	0.19	0.26	-0.20	0.19	0.30	1	1	4.85	0.12	0.18	0.24	0.15	0.23	7	5	2.53	0.17	0.24	-0.98	0.18	0.27	1	1	3.58	0.12	0.20	0.19	0.15	0.25	9	7	0.11	0.18	0.23	-0.09	0.16	0.24	5	4	2.11	0.16	0.21	0.06	0.15	0.23	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.27	0.16	0.22	-0.43	0.15	0.23	3	3	1.48	0.17	0.21	-0.94	0.16	0.24	5	3	4.53	0.12	0.18	0.00	0.14	0.22	55	46	1.97	0.15	0.22	0.02	0.16	0.25	6	5	2.95	0.16	0.22	-0.34	0.16	0.23	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-1.03	0.22	0.31	-1.03	0.20	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.99	0.19	0.23	-1.15	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2259-3407	54	6266	100	4.32	0.26	0.36	-2.29	0.11	0.17	1.37	0.15	0.25	6.51	0.15	0.23	0.41	0.18	0.27	1	1	5.52	0.11	0.17	0.22	0.15	0.23	7	2	3.20	0.16	0.23	-0.98	0.17	0.26	1	1	4.36	0.11	0.19	0.29	0.15	0.25	9	6	1.01	0.18	0.23	0.13	0.18	0.27	5	2	3.13	0.15	0.21	0.40	0.16	0.24	17	8	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.23	0.13	0.19	-0.15	0.15	0.23	3	3	2.60	0.15	0.19	-0.50	0.16	0.24	5	3	5.21	0.11	0.17	0.00	0.14	0.22	55	37	2.87	0.14	0.21	0.24	0.16	0.25	6	3	3.92	0.16	0.21	-0.04	0.17	0.23	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.50	0.21	0.29	-0.18	0.20	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.68	0.19	0.24	-0.52	0.19	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2301-4024	55	5743	100	3.76	0.25	0.35	-2.11	0.11	0.17	1.60	0.13	0.23	6.59	0.17	0.24	0.30	0.17	0.26	1	1	5.68	0.11	0.18	0.20	0.14	0.23	7	5	3.39	0.14	0.23	-0.98	0.16	0.26	1	1	4.52	0.11	0.20	0.26	0.14	0.24	9	8	1.18	0.18	0.23	0.10	0.17	0.26	5	4	3.17	0.16	0.21	0.24	0.16	0.25	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.41	0.16	0.23	-0.16	0.16	0.24	3	3	2.97	0.14	0.20	-0.32	0.15	0.23	5	3	5.40	0.11	0.17	0.00	0.14	0.22	55	52	2.96	0.15	0.21	0.14	0.15	0.25	6	4	4.13	0.16	0.24	-0.03	0.17	0.25	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.87	0.16	0.26	-0.00	0.17	0.27	3	2	0.27	0.18	0.23	0.13	0.17	0.27	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	0.52	0.19	0.24	0.49	0.18	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-0.61	0.18	0.23	0.98	0.17	0.27	4	3
HE 2301-4126	55	5841	100	3.66	0.26	0.36	-2.37	0.13	0.19	1.53	0.14	0.24	6.41	0.17	0.24	0.39	0.17	0.27	1	1	5.43	0.11	0.17	0.22	0.15	0.24	7	4	3.18	0.14	0.22	-0.92	0.16	0.25	1	1	4.19	0.11	0.20	0.20	0.15	0.25	9	7	0.97	0.18	0.23	0.16	0.16	0.25	5	4	2.94	0.16	0.21	0.28	0.15	0.23	17	8	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.15	0.16	0.22	-0.15	0.15	0.23	3	3	2.51	0.15	0.20	-0.51	0.15	0.23	5	2	5.13	0.13	0.19	0.00	0.14	0.22	55	42	2.66	0.15	0.21	0.10	0.15	0.25	6	2	3.81	0.17	0.23	-0.07	0.16	0.23	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.53	0.21	0.30	-0.08	0.18	0.28	3	2	-0.15	0.19	0.24	-0.02	0.17	0.26	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.13	0.20	0.25	0.11	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2304-4153	58	4663	100	1.01	0.26	0.36	-3.02	0.12	0.18	2.12	0.12	0.22	4.72	0.21	0.28	-0.65	0.20	0.29	1	1	4.66	0.12	0.18	0.10	0.15	0.23	7	6	2.91	0.15	0.26	-0.54	0.18	0.28	1	1	3.50	0.12	0.20	0.16	0.14	0.24	9	7	0.19	0.16	0.22	0.04	0.15	0.24	5	5	2.13	0.15	0.20	0.14	0.15	0.23	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.33	0.15	0.24	-0.32	0.15	0.24	3	3	2.13	0.14	0.20	-0.24	0.15	0.23	5	2	4.48	0.12	0.18	0.00	0.14	0.22	55	49	1.85	0.15	0.22	-0.04	0.15	0.24	6	5	3.22	0.15	0.27	-0.00	0.17	0.27	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-1.68	0.19	0.26	-1.62	0.18	0.27	3	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-2.50	0.19	0.23	-1.61	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2311+0129	58	5188	100	2.65	0.25	0.35	-2.78	0.12	0.18	1.54	0.12	0.22	5.94	0.19	0.26	0.33	0.18	0.27	1	1	5.12	0.11	0.18	0.31	0.15	0.24	7	6	2.82	0.15	0.24	-0.87	0.17	0.26	1	1	3.90	0.12	0.20	0.32	0.14	0.25	9	8	0.56	0.18	0.23	0.16	0.16	0.25	5	4	2.53	0.16	0.21	0.28	0.15	0.24	17	15	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.63	0.17	0.24	-0.26	0.16	0.24	3	3	2.00	0.17	0.22	-0.61	0.16	0.23	5	3	4.72	0.12	0.18	0.00	0.14	0.22	55	49	2.35	0.16	0.22	0.21	0.15	0.25	6	6	3.50	0.18	0.26	0.03	0.17	0.25	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.29	0.18	0.28	0.09	0.18	0.28	3	2	-0.64	0.18	0.23	-0.10	0.16	0.25	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.84	0.21	0.25	-0.19	0.18	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2314-1554	52	5139	100	2.62	0.27	0.37	-3.27	0.13	0.18	1.73	0.14	0.24	5.71	0.19	0.26	0.60	0.18	0.27	1	1	4.81	0.12	0.19	0.50	0.16	0.25	7	5	2.79	0.15	0.24	-0.41	0.17	0.26	1	1	3.52	0.12	0.20	0.43	0.15	0.25	9	5	0.28	0.18	0.23	0.38	0.16	0.25	5	4	2.14	0.16	0.21	0.39	0.15	0.24	17	10	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.97	0.16	0.20	-0.42	0.15	0.22	3	3	1.11	0.17	0.21	-1.00	0.15	0.23	5	3	4.23	0.13	0.18	0.00	0.14	0.22	55	37	2.02	0.15	0.22	0.38	0.15	0.24	6	5	3.05	0.18	0.23	0.08	0.16	0.24	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.24	0.23	0.32	0.06	0.21	0.31	3	2	-0.82	0.19	0.24	0.21	0.17	0.25	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.45	0.20	0.24	-0.31	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2319-0852	36	4724	100	1.36	0.27	0.37	-3.38	0.13	0.18	1.97	0.14	0.24	4.69	0.21	0.28	-0.32	0.20	0.30	1	1	4.33	0.13	0.20	0.13	0.15	0.24	7	3	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	3.34	0.12	0.20	0.36	0.15	0.25	9	3	-0.06	0.18	0.22	0.14	0.16	0.24	5	3	1.88	0.16	0.21	0.24	0.15	0.23	17	9	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.74	0.16	0.22	-0.55	0.16	0.23	3	3	1.06	0.16	0.21	-0.95	0.16	0.23	5	3	4.12	0.13	0.18	0.00	0.14	0.22	55	38	1.78	0.16	0.22	0.23	0.15	0.25	6	5	3.18	0.19	0.28	0.31	0.18	0.28	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.94	0.25	0.34	-0.54	0.24	0.33	3	2	-1.30	0.20	0.24	-0.17	0.18	0.25	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-2.24	0.19	0.23	-1.00	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2325-0755	57	5665	100	3.17	0.27	0.37	-2.85	0.13	0.18	1.48	0.13	0.23	5.76	0.19	0.25	0.21	0.19	0.28	1	1	5.05	0.11	0.18	0.31	0.15	0.24	7	2	2.61	0.14	0.22	-1.02	0.15	0.25	1	1	3.97	0.12	0.20	0.46	0.15	0.25	9	7	0.47	0.18	0.23	0.14	0.16	0.25	5	2	2.53	0.16	0.21	0.35	0.15	0.23	17	8	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.54	0.15	0.20	-0.29	0.15	0.22	3	3	1.84	0.16	0.20	-0.71	0.15	0.23	5	3	4.65	0.13	0.18	0.00	0.14	0.22	55	37	2.18	0.15	0.22	0.10	0.15	0.25	6	2	3.23	0.16	0.21	-0.18	0.15	0.22	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.12	0.21	0.30	-0.24	0.19	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.29	0.19	0.23	-0.57	0.16	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2326+0038	54	5145	100	2.51	0.24	0.34	-2.77	0.13	0.19	1.62	0.13	0.23	5.84	0.19	0.25	0.23	0.18	0.27	1	1	5.05	0.11	0.18	0.24	0.15	0.24	7	7	2.76	0.16	0.24	-0.93	0.17	0.26	1	1	3.81	0.12	0.20	0.23	0.15	0.25	9	8	0.53	0.18	0.23	0.13	0.15	0.24	5	4	2.45	0.16	0.21	0.21	0.15	0.23	17	13	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.60	0.17	0.24	-0.30	0.16	0.24	3	3	1.91	0.17	0.21	-0.71	0.15	0.23	5	3	4.72	0.13	0.19	0.00	0.14	0.22	55	47	2.38	0.16	0.22	0.23	0.15	0.24	6	6	3.37	0.19	0.27	-0.10	0.17	0.25	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-0.26	0.23	0.33	-0.46	0.20	0.30	3	2	-1.03	0.19	0.23	-0.49	0.16	0.25	6	2	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-1.31	0.19	0.24	-0.66	0.16	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2327-5642	69	5048	100	2.22	0.25	0.35	-2.95	0.12	0.18	1.69	0.12	0.22	5.88	0.19	0.26	0.43	0.19	0.29	1	1	4.79	0.11	0.18	0.14	0.15	0.24	7	6	2.63	0.14	0.23	-0.90	0.16	0.25	1	1	3.60	0.12	0.20	0.18	0.15	0.25	9	7	0.17	0.18	0.23	-0.06	0.16	0.25	5	4	2.14	0.16	0.21	0.06	0.15	0.24	17	12	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.32	0.16	0.23	-0.42	0.16	0.23	3	3	1.78	0.17	0.22	-0.68	0.16	0.24	5	3	4.57	0.12	0.18	0.00	0.14	0.22	55	50	2.14	0.16	0.22	0.15	0.16	0.25	6	5	3.32	0.16	0.25	0.01	0.16	0.25	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.34	0.18	0.28	0.31	0.18	0.27	3	2	-0.57	0.18	0.23	0.12	0.17	0.26	6	3	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.14	0.21	0.28	0.66	0.19	0.27	2	1	-1.10	0.18	0.23	0.67	0.17	0.26	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-0.69	0.18	0.23	0.74	0.17	0.26	9	2	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-1.20	0.18	0.23	1.22	0.17	0.26	4	4
HE 2329-3702	38	6060	100	3.72	0.28	0.38	-2.16	0.12	0.18	1.65	0.15	0.25	6.39	0.20	0.26	0.15	0.21	0.30	1	1	5.74	0.11	0.17	0.31	0.15	0.24	7	3	3.26	0.15	0.23	-1.06	0.17	0.26	1	1	4.65	0.11	0.20	0.44	0.15	0.25	9	8	1.23	0.18	0.24	0.21	0.17	0.26	5	3	3.29	0.16	0.21	0.42	0.15	0.24	17	9	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.35	0.16	0.22	-0.17	0.16	0.23	3	3	2.66	0.15	0.20	-0.58	0.16	0.24	5	3	5.35	0.12	0.18	0.00	0.14	0.22	55	40	2.81	0.15	0.21	0.04	0.16	0.25	6	1	3.88	0.16	0.21	-0.22	0.16	0.23	4	1	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.96	0.21	0.30	0.14	0.20	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.16	0.20	0.24	-0.14	0.18	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2333-1358	40	5020	100	2.15	0.29	0.39	-3.34	0.13	0.18	1.57	0.15	0.25	5.38	0.20	0.27	0.33	0.19	0.29	1	1	4.70	0.12	0.19	0.46	0.16	0.24	7	4	2.20	0.17	0.24	-0.93	0.17	0.26	1	1	3.28	0.12	0.20	0.26	0.15	0.25	9	3	0.16	0.18	0.23	0.33	0.17	0.25	5	4	1.80	0.18	0.23	0.12	0.16	0.25	17	8	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.80	0.23	0.28	-0.53	0.19	0.27	3	3	1.26	0.17	0.21	-0.79	0.16	0.24	5	3	4.16	0.13	0.18	0.00	0.14	0.22	55	32	1.98	0.16	0.22	0.40	0.15	0.25	6	5	3.21	0.19	0.27	0.31	0.18	0.27	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-2.24	0.20	0.26	-1.87	0.18	0.28	3	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2334-0604	72	4820	100	1.51	0.25	0.35	-3.41	0.13	0.18	2.15	0.11	0.21	4.32	0.22	0.28	-0.67	0.20	0.30	1	1	4.23	0.12	0.19	0.06	0.15	0.23	7	4	2.71	0.14	0.24	-0.36	0.16	0.26	1	1	3.05	0.12	0.20	0.10	0.15	0.25	9	3	-0.25	0.17	0.22	-0.02	0.15	0.24	5	4	1.61	0.16	0.21	-0.00	0.15	0.23	17	10	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	1.68	0.15	0.20	-0.59	0.15	0.22	3	3	1.26	0.16	0.21	-0.72	0.15	0.23	5	3	4.09	0.13	0.18	0.00	0.14	0.22	55	44	1.73	0.15	0.22	0.22	0.15	0.24	6	5	2.82	0.16	0.22	-0.03	0.15	0.23	4	4	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-1.28	0.19	0.27	-0.84	0.17	0.27	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-2.58	0.19	0.23	-1.30	0.16	0.24	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2335-5958B	37	5765	100	3.24	0.28	0.38	-2.33	0.13	0.18	1.63	0.14	0.24	6.15	0.19	0.26	0.08	0.20	0.29	1	1	5.47	0.12	0.18	0.21	0.15	0.24	7	3	3.10	0.18	0.24	-1.05	0.18	0.27	1	1	4.45	0.12	0.20	0.41	0.15	0.25	9	8	0.93	0.17	0.23	0.08	0.16	0.25	5	3	3.01	0.16	0.21	0.31	0.15	0.23	17	10	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.25	0.17	0.24	-0.10	0.16	0.24	3	3	2.57	0.16	0.21	-0.50	0.16	0.23	5	3	5.18	0.13	0.18	0.00	0.14	0.22	55	42	2.73	0.15	0.22	0.13	0.16	0.25	6	3	4.03	0.20	0.27	0.10	0.18	0.26	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.60	0.23	0.33	-0.05	0.21	0.31	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.51	0.21	0.25	-0.32	0.18	0.26	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2338-1311	20	5582	100	3.50	0.28	0.38	-2.86	0.13	0.18	1.27	0.18	0.28	5.87	0.19	0.25	0.34	0.18	0.27	1	1	5.10	0.12	0.18	0.38	0.16	0.25	7	1	-9.99	0.00	0.00	-9.99	0.00	0.00	0	0	3.82	0.12	0.20	0.32	0.15	0.25	9	1	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	2.52	0.16	0.21	0.36	0.16	0.24	17	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.57	0.15	0.21	-0.24	0.15	0.23	3	1	-9.99	0.00	0.00	-9.99	0.00	0.00	5	0	4.64	0.13	0.18	0.00	0.14	0.22	55	16	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2338-1618	40	5515	100	3.38	0.27	0.37	-2.65	0.12	0.18	1.43	0.16	0.26	6.22	0.18	0.25	0.47	0.18	0.27	1	1	5.10	0.12	0.18	0.16	0.15	0.24	7	2	2.86	0.16	0.24	-0.97	0.17	0.26	1	1	3.94	0.12	0.20	0.23	0.15	0.25	9	6	0.61	0.18	0.23	0.08	0.18	0.27	5	2	2.55	0.16	0.21	0.17	0.16	0.25	17	7	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	2.87	0.18	0.24	-0.16	0.18	0.25	3	3	2.12	0.16	0.21	-0.62	0.16	0.24	5	3	4.86	0.12	0.18	0.00	0.14	0.22	55	38	2.61	0.16	0.22	0.34	0.16	0.25	6	3	3.82	0.21	0.27	0.21	0.19	0.26	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.11	0.23	0.32	-0.22	0.22	0.32	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2345-1919	44	5617	100	4.46	0.25	0.35	-2.46	0.12	0.18	1.47	0.16	0.26	6.17	0.19	0.24	0.24	0.17	0.26	1	1	5.45	0.12	0.18	0.33	0.14	0.24	7	3	3.42	0.13	0.23	-0.59	0.16	0.25	1	1	4.15	0.12	0.20	0.25	0.14	0.25	9	8	0.68	0.18	0.23	-0.03	0.17	0.28	5	2	2.78	0.16	0.21	0.22	0.16	0.26	17	9	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.13	0.15	0.22	-0.08	0.16	0.24	3	3	2.51	0.15	0.21	-0.41	0.16	0.24	5	3	5.04	0.12	0.18	0.00	0.14	0.22	55	39	2.63	0.16	0.22	0.17	0.16	0.26	6	3	3.78	0.16	0.22	-0.01	0.17	0.24	4	3	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.23	0.18	0.25	-0.28	0.19	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.79	0.19	0.24	-0.45	0.18	0.29	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2347-1254	80	6132	100	3.95	0.24	0.34	-1.83	0.13	0.18	1.67	0.12	0.22	6.83	0.15	0.22	0.27	0.16	0.26	1	1	6.04	0.11	0.17	0.29	0.15	0.23	7	4	3.90	0.12	0.22	-0.74	0.15	0.25	1	1	4.90	0.11	0.20	0.37	0.15	0.25	9	9	1.60	0.17	0.22	0.26	0.15	0.24	5	4	3.58	0.15	0.20	0.39	0.14	0.23	17	14	2.39	0.14	0.19	0.22	0.15	0.23	3	1	3.72	0.15	0.22	-0.13	0.15	0.23	3	3	3.17	0.15	0.20	-0.39	0.15	0.23	5	3	5.67	0.13	0.18	0.00	0.14	0.22	55	53	3.23	0.14	0.21	0.14	0.15	0.24	6	4	4.26	0.16	0.22	-0.16	0.16	0.23	4	2	2.90	0.13	0.20	0.13	0.15	0.25	2	1	1.36	0.16	0.25	0.21	0.16	0.26	3	2	0.57	0.17	0.22	0.16	0.15	0.25	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	0.31	0.20	0.25	0.01	0.17	0.25	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0
HE 2347-1334	81	4453	100	0.95	0.24	0.34	-2.55	0.12	0.19	2.38	0.11	0.21	5.33	0.21	0.26	-0.50	0.18	0.27	1	1	5.31	0.12	0.19	0.28	0.15	0.23	7	5	3.32	0.15	0.25	-0.59	0.16	0.26	1	1	3.97	0.11	0.20	0.17	0.14	0.24	9	9	0.59	0.15	0.20	-0.02	0.14	0.23	5	5	2.51	0.15	0.20	0.05	0.15	0.23	17	17	1.23	0.16	0.20	-0.22	0.15	0.23	3	3	2.61	0.19	0.29	-0.50	0.17	0.26	3	3	2.38	0.14	0.20	-0.45	0.15	0.23	5	5	4.94	0.12	0.19	0.00	0.14	0.22	55	54	2.26	0.17	0.24	-0.10	0.16	0.25	6	6	3.62	0.31	0.38	-0.07	0.26	0.34	4	4	2.16	0.12	0.20	0.12	0.14	0.25	2	2	0.20	0.16	0.23	-0.21	0.15	0.25	3	1	-0.61	0.17	0.22	-0.30	0.14	0.24	6	6	0.15	0.17	0.21	0.11	0.14	0.25	3	2	-1.21	0.19	0.25	-0.78	0.17	0.26	2	1	-1.88	0.17	0.21	-0.49	0.14	0.25	6	1	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-1.49	0.18	0.23	-0.43	0.15	0.26	9	2	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-2.30	0.18	0.22	-0.25	0.15	0.26	4	3
HE 2347-1448	43	6162	100	3.98	0.27	0.37	-2.31	0.12	0.18	0.84	0.17	0.27	6.58	0.18	0.24	0.50	0.19	0.27	1	1	5.40	0.12	0.18	0.13	0.15	0.24	7	1	3.05	0.16	0.22	-1.11	0.17	0.26	1	1	4.25	0.11	0.20	0.21	0.15	0.25	9	3	0.93	0.18	0.23	0.07	0.18	0.27	5	2	3.01	0.16	0.21	0.31	0.16	0.25	17	5	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	3.31	0.16	0.22	-0.05	0.17	0.24	3	3	2.40	0.16	0.20	-0.68	0.16	0.25	5	1	5.19	0.12	0.18	0.00	0.14	0.22	55	32	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	4.21	0.21	0.27	0.27	0.21	0.27	4	2	-9.99	0.00	0.00	-9.99	0.00	0.00	2	0	0.74	0.20	0.29	0.08	0.20	0.29	3	2	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	3	0	-0.34	0.19	0.24	-0.16	0.19	0.27	2	1	-9.99	0.00	0.00	-9.99	0.00	0.00	6	0	-9.99	0.00	0.00	-9.99	0.00	0.00	10	0	-9.99	0.00	0.00	-9.99	0.00	0.00	9	0	-9.99	0.00	0.00	-9.99	0.00	0.00	8	0	-9.99	0.00	0.00	-9.99	0.00	0.00	4	0

$\displaystyle \sigma_{\varepsilon}^2$	=	$\displaystyle \left(\frac{\partial\varepsilon}{\partial T}\right)^2 \sigma_T^2 ... ...g g}^2 + \left(\frac{\partial\varepsilon}{\partial \xi}\right)^2 \sigma_{\xi}^2$
		$\displaystyle + \sigma_{\log gf}^2 + \sigma_{\varepsilon}^2({\rm obs}) + \sigma_{\varepsilon}^2 ({\rm cont}) + \sigma_{\varepsilon}^2 ({\rm model})$
		$\displaystyle + 2 \left\{ \frac{\partial\varepsilon}{\partial T} \frac{\partial... ...on}{\partial T} \frac{\partial\varepsilon}{\partial \xi} \sigma_{T,\xi} \right.$
		$\displaystyle \left. + \frac{\partial\varepsilon}{\partial \log g} \frac{\partial\varepsilon}{\partial \xi} \sigma_{\log g, \xi} \right\} ,$	(B.1)

$\displaystyle \sigma_{\varepsilon}^2$	=	$\displaystyle \left(\frac{\partial\varepsilon}{\partial T}\right)^2 \sigma_T^2 ... ...g g}^2 + \left(\frac{\partial\varepsilon}{\partial \xi}\right)^2 \sigma_{\xi}^2$
		$\displaystyle + \sigma_{\log gf}^2 + \sigma_{\varepsilon}^2({\rm obs}) + \sigma_{\varepsilon}^2 ({\rm cont}) + \sigma_{\varepsilon}^2 ({\rm model})$	(B.2)
		$\displaystyle + 2 \left\{ \frac{\partial\varepsilon}{\partial T} \frac{\partial... ...\log g} \frac{\partial\varepsilon}{\partial \xi} \sigma_{\log g,\xi} \right\} .$

$\displaystyle \sigma_{A,B}$	=	$\displaystyle \frac{\partial\varepsilon_A}{\partial T} \frac{\partial\varepsilo... ...silon_A}{\partial \xi}\frac{\partial\varepsilon_B}{\partial \xi} \sigma_{\xi}^2$
		$\displaystyle + \left\{ \frac{\partial\varepsilon_A}{\partial T}\frac{\partial\... ...tial \log g}\frac{\partial\varepsilon_B}{\partial T}\right\} \sigma_{T, \log g}$
		$\displaystyle + \left\{ \frac{\partial\varepsilon_A}{\partial \xi}\frac{\partia... ...\log g}\frac{\partial\varepsilon_B}{\partial \xi}\right\} \sigma_{\log g, \xi}.$	(B.4)

Star	$S/N_{\rm av}$	$T_{\rm eff}$	$\sigma_{T_{\rm eff}}$	$\log g$	$\sigma_{\log g}^{\rm rel}$	$\sigma_{\log g}^{\rm abs}$	[Fe/H]	$\sigma_{\rm [Fe/H]}^{\rm rel}$	$\sigma_{\rm [Fe/H]}^{\rm abs}$	$\xi$	$\sigma_\xi^{\rm rel}$	$\sigma_\xi^{\rm abs}$	$\log\epsilon_{\rm C}$	$\sigma_{\log\epsilon_{\rm C}}^{\rm rel}$	$\sigma_{\log\epsilon_{\rm C}}^{\rm abs}$	[C/Fe]	$\sigma_{\rm [C/Fe]}^{\rm rel}$	$\sigma_{\rm [C/Fe]}^{\rm abs}$	N	N3	...
		[K]		[cm s^-2]						[km s^-1]											...
CS 22175-007	31	5108	100	2.46	0.26	0.36	-2.81	0.13	0.18	1.67	0.14	0.24	5.77	0.19	0.26	0.19	0.18	0.27	1	1	$\ldots$
CS 22186-023	55	5066	100	2.19	0.24	0.34	-2.72	0.13	0.18	1.58	0.11	0.21	5.97	0.19	0.25	0.30	0.18	0.27	1	1	$\ldots$
CS 22186-025	32	4985	100	1.70	0.26	0.36	-2.87	0.14	0.19	2.14	0.13	0.23	4.83	0.20	0.27	-0.68	0.19	0.29	1	1	$\ldots$
CS 22886-042	39	4881	100	1.85	0.25	0.35	-2.68	0.12	0.18	1.84	0.12	0.22	5.72	0.19	0.26	0.01	0.19	0.28	1	1	$\ldots$
CS 22892-052	46	4884	100	1.81	0.26	0.36	-2.95	0.14	0.19	1.67	0.12	0.22	6.44	0.19	0.26	1.00	0.18	0.28	1	1	$\ldots$
CS 22945-028	31	5126	100	2.55	0.26	0.36	-2.66	0.13	0.18	1.53	0.14	0.24	5.93	0.19	0.26	0.21	0.18	0.27	1	1	$\ldots$
CS 22957-013	35	4904	100	1.96	0.25	0.35	-2.64	0.14	0.19	1.79	0.12	0.22	5.85	0.19	0.26	0.10	0.17	0.27	1	1	$\ldots$
CS 22958-083	32	5101	100	2.40	0.26	0.36	-2.79	0.12	0.18	1.50	0.13	0.23	6.24	0.20	0.26	0.64	0.18	0.27	1	1	$\ldots$
CS 22960-010	35	5737	100	4.85	0.25	0.35	-2.65	0.12	0.17	1.53	0.17	0.27	6.56	0.17	0.24	0.82	0.16	0.25	1	1	$\ldots$
CS 29491-069	57	5103	100	2.45	0.24	0.34	-2.81	0.13	0.18	1.54	0.12	0.22	5.76	0.19	0.25	0.18	0.17	0.27	1	1	$\ldots$
$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\ldots$
HE 2338-1618	40	5515	100	3.38	0.27	0.37	-2.65	0.12	0.18	1.43	0.16	0.26	6.22	0.18	0.25	0.47	0.18	0.27	1	1	$\ldots$
HE 2345-1919	44	5617	100	4.46	0.25	0.35	-2.46	0.12	0.18	1.47	0.16	0.26	6.17	0.19	0.24	0.24	0.17	0.26	1	1	$\ldots$
HE 2347-1254	80	6132	100	3.95	0.24	0.34	-1.83	0.13	0.18	1.67	0.12	0.22	6.83	0.15	0.22	0.27	0.16	0.26	1	1	$\ldots$
HE 2347-1334	81	4453	100	0.95	0.24	0.34	-2.55	0.12	0.19	2.38	0.11	0.21	5.33	0.21	0.26	-0.50	0.18	0.27	1	1	$\ldots$
HE 2347-1448	43	6162	100	3.98	0.27	0.37	-2.31	0.12	0.18	0.84	0.17	0.27	6.58	0.18	0.24	0.50	0.19	0.27	1	1	$\ldots$

The Hamburg/ESO R-process enhanced star survey (HERES),

II. Spectroscopic analysis of the survey sample