Contents

• A search for Low Surface Brightness galaxies in the near-infrared
• 1 Introduction
• 2 The 2MASS all-sky near-infrared survey
• 3 2MASS LSB galaxies selection
• 4 Basic properties of the sample
• 5 Discussion and further observations
• References
• 6 Online Material

A&A 405, 99-109 (2003)
DOI: 10.1051/0004-6361:20030585

A search for Low Surface Brightness galaxies in the near-infrared

I. Selection of the sample

D. Monnier Ragaigne¹ - W. van Driel¹ - S. E. Schneider² - T. H. Jarrett³ - C. Balkowski¹

1 - Observatoire de Paris, GEPI, CNRS UMR 8111 and Université Paris 7, 5 place Jules Janssen, 92195 Meudon Cedex, France
2 - University of Massachusetts, Astronomy Program, 536 LGRC, Amherst, MA 01003, USA
3 - IPAC, Caltech, MS 100-22, 770 South Wilson Ave., Pasadena, CA 91125, USA

Received 14 February 2003 / Accepted 16 April 2003

Abstract
A sample of about 3800 Low Surface Brightness (LSB) galaxies was selected using the all-sky near-infrared (J, H and $K_{\rm s}$-band) 2MASS survey. The selected objects have a mean central surface brightness within a 5'' radius around their centre fainter than 18 mag arcsec^-2 in the $K_{\rm s}$ band, making them the lowest surface brightness galaxies detected by 2MASS. A description is given of the relevant properties of the 2MASS survey and the LSB galaxy selection procedure, as well as of basic photometric properties of the selected objects. The latter properties are compared to those of other samples of galaxies, of both LSBs and "classical'' high surface brightness (HSB) objects, which were selected in the optical. The 2MASS LSBs have a $B_{\rm T_{c}}-K_{\rm T}$ colour which is on average 0.9 mag bluer than that of HSBs from the NGC. The 2MASS sample does not appear to contain a significant population of red objects.

Key words: galaxies: fundamental parameters - galaxies: general - galaxies: photometry - infrared: galaxies

1 Introduction

Observational bias in the selection of galaxies dates back to the visual searches by Messier and Herschel, as galaxies are diffuse objects selected in the presence of a contaminating signal: the brightness of the night sky. The night sky acts as a filter, which, when convolved with the true population of galaxies gives the population of galaxies we observe and which hampers the detection of low surface brightness objects. Based on this concern, the result of the study of Freeman (1970), which indicated a remarkably narrow range of central disc surface brightness values of spiral galaxies in the B-band ( $21.7\pm0.3$ mag arcsec^-2), was questioned by Disney (1976).

In the past few decades, observations of the local universe have shown the existence of galaxies well below the surface brightness of the average previously catalogued galaxies, and often even well below the surface brightness of the night sky, which are referred to as Low Surface Brightness (LSB) galaxies.

At present, the LSBs constitute the least well known fraction of galaxies: their number density and physical properties (like luminosity, colours, dynamics) are still quite uncertain. This is, per definition, mainly due to the fundamental difficulty in identifying them in imaging surveys and in measuring their properties. It is far from obvious that all existing classes and types of LSBs have been probed, given the limitations in sensitivity of the actual detectors and the biases in the selection criteria of the published samples.

In order to further investigate the often baffling properties of the LSB class of galaxies we selected a large sample of them from the 2MASS database, accessing the near-infrared, a wavelength domain that has been much less fully explored than the optical in the study of LSBs.

To date, the following studies were published on the near-infrared properties of LSB galaxies: Knezek & Wroten (1994) observed a small sample of mainly massive galaxies in JHK, Bergvall et al. (1999) observed 14 blue LSBs in JHK and compared their results to optical photometry, Bell et al. (2000) observed 26 LSBs in JHK and a subset of these in $BV\!R$, de Jong (1996) included a few LSBs among the spiral galaxies he observed in H and K, and Galaz et al. (2002) observed 88 LSBs in J and $K_{\rm s}$.

Although there is no unambiguous definition of LSB galaxy, those in common use are based on (1) the mean blue surface brightness within the 25 mag arcsec^-2 isophote, (2) the mean surface brightness within the half-light radius, or (3) the extrapolated central surface brightness of the disc component alone, after carrying out a disc-bulge decomposition.

For 2MASS galaxies, we used the mean $K_{\rm s}$-band magnitude within a fixed aperture to identify a sample of galaxies with relatively low infrared surface brightness. We selected galaxies in which the central surface brightness within a 5'' radius circular aperture was fainter than 18 mag arcsec^-2 in the $K_{\rm s}$-band. This criterion selects a relatively small fraction (<10%) of large angular diameter sources detected by 2MASS, increasing to about 40% for the small angular diameter sources detected in the survey.

If 2MASS detections have B-K=4.0 colors typical of early-type galaxies (Jarrett et al. 2003; also see Sect. 4.4), as might be anticipated for a sample of infrared-selected sources, this criterion would correspond roughly to the disc-component definition that LSB galaxies are objects with a blue central surface brightness $\mu_{B_0}>22.0$ mag arcsec^-2 (i.e., more than 1$\sigma$ fainter than the $21.7\pm0.3$ mag arcsec^-2 measured by Freeman 1970). Our sample galaxies can have an even lower disc surface brightness if the bulge component is significant, but since we average over a fixed angular aperture, on the other hand we may also include some higher central surface brightness sources that are more distant so that the aperture includes more of the disc. In this paper, we examine the properties of our sample based on 2MASS and LEDA data and compare it to optically-selected galaxy samples.

LSBs have remarkable properties which distinguish them from "classical'' High Surface Brightness (HSB) spirals, notably:

• LSBs seem to constitute at least 50% of the total galaxy population in number in the local Universe, which may have strong implications for the faint end slope of the galaxy luminosity function, on the baryonic matter density and especially on galaxy formation scenarios (O'Neil & Bothun 2000).
• LSBs discs are among the less evolved objects in the local universe since they have a very low star formation rate (van der Hulst et al. 1993; van Zee et al. 1997; van den Hoek et al. 2000).
• LSBs are embedded in dark matter halos which are of lower density and more extended than the haloes around HSB galaxies, and they appear to be strongly dominated by Dark Matter at all radii (e.g., de Blok et al. 1996, 2001; McGaugh et al. 2001)

The star formation history of LSBs has been the subject of recent debate. The LSBs best studied in the optical and in the near-infrared are blue (e.g., Bergvall et al. 1999), indicating a young mean stellar age and/or metallicity. Morphologically, most studied LSBs have discs, but little spiral structure. The current massive star formation rates in LSBs are an order of magnitude lower than those of HSBs (van Zee et al. 1997); H  I observations show that LSBs have high gas mass fractions, sometimes exceeding unity (Spitzak & Schneider 1998; McGaugh & de Blok 1997). All these observations are consistent with a scenario in which LSBs are relatively unevolved, low mass surface density, low metallicity systems with roughly constant star formation rate. However, this scenario has some difficulty accommodating giant LSBs like Malin 1 (Bothun et al. 1987), see, e.g., Boissier et al. (2003).

This study of infrared LSBs was also intended to investigate the possibility of there being a substantial population of red LSBs like those reported in the optical $UBV\!RI$-band study of O'Neil et al. (1997). Follow-up H  I line studies initially indicated that some of these red LSBs with rotational speeds exceeding 200 km s^-1 did not seem to follow the "standard'' Tully-Fisher relation established for HSB galaxies, in the sense that they appeared to be severely underluminous for their total mass (O'Neil et al. 2000). More recent H  I imaging observations by Chung et al. (2002) indicate that the rotational properties and total H  I mass of these red LSBs had been strongly overestimated due to confusion within the telescope beam with neighbouring galaxies. An infrared-selected sample should allow us to identify whether there is a significant population of very red LSBs.

In the present paper a description is given of the 2MASS LSB galaxy sample selection and its results, while 21-cm H  I line observations from Arecibo and Nançay will be presented in Papers II and III, respectively (Monnier Ragaigne et al. 2003b,c), optical $BV\!RI$-band CCD surface photometry of a sub-sample of 35 2MASS LSB galaxies will be presented in Paper IV (Monnier Ragaigne et al. 2003d) and an analysis of the full data set will be presented in Paper V. Models of the evolution of the 2MASS galaxies presented in Paper IV and of other samples of LSB galaxies are presented in Boissier et al. (2003).

The 2MASS survey is described in Sect. 2, and the 2MASS LSB galaxies sample selection in Sect. 3. Basic photometric properties of the sample are presented in Sect. 4 and compared with those of others samples of LSB and HSB galaxies. Subsets of the sample observed by us at other wavelengths are described in Sect. 5.

2 The 2MASS all-sky near-infrared survey

The Two Micron All Sky Survey, 2MASS, has imaged the entire celestial sphere in the near-infrared J (1.25 $\mu$m), H (1.65 $\mu$m) and $K_{\rm s}$ (2.16 $\mu$m) bands using two identical dedicated 1.3-meter telescopes, designed specifically for the survey. One goal of the survey was to probe the nearby Universe in detail out to redshifts of $z\sim 0.1$. Accordingly, it is highly uniform in both photometric and astrometric measurements. The 2MASS Extended Source Catalog (XSC) consists of more than 1.6 million galaxies brighter than 14th mag at $K_{\rm s}$ with angular diameters greater than $\sim$10''. The photometry includes accurate Point Spread Function (PSF)-derived measures and a variety of circular and elliptical aperture measures, fully characterizing both point-like and extended objects. The position centroids have an astrometric accuracy better than $\sim$ $0''~\hspace{-1.7mm}.\hspace{.1mm}5$. In addition to tabular information, 2MASS archives full-resolution images for each extended object, enabling detailed comparison with other imaging surveys.

Though 2MASS perforce needed to sacrifice depth for all-sky coverage, and is therefore less deep than some of the dedicated optical imaging surveys made of LSB galaxies over limited areas of the sky, it should still be sensitive to the bright end of the LSB spectrum, particularly if there is a class of very red LSB objects. It has a 95% completeness level in J, H and $K_{\rm s}$ of 15.1, 14.3 and 13.5 mag, respectively, for "normal'' galaxies (Jarrett et al. 2000); for LSB and blue objects the completeness limits are not yet known. In practice, 2MASS detects galaxies with central surface brightness values ranging from 14-20 mag arcsec^-2 of which the LSB fraction with $18<\mu_{K5}<20$ mag arcsec^-2 varies from $\sim$10% of the total 2MASS sample for large galaxies ( $r_{K_{20}} \geq20''$) to $\sim$40% for the smaller galaxies ( $20'' \geq r_{K_{20}} \geq 10''$). These near-infrared data will be less susceptible than optical surveys to the effects of extinction due to dust, both Galactic and internal to the galaxies. Also, the luminous mass distribution of galaxies is dominated by the older stellar populations, which emit most of their light in the near-infrared.

Initial results for galaxies detected by 2MASS, including LSB objects, are described in several publications (Schneider et al. 1997; Jarrett et al. 2000a,b; Hurt et al. 2000).

2.1 The extended source processor

The last major subsystem to run in the 2MASS quasi-linear data reduction "pipeline'' is the extended source processor, GALWORKS. The primary role of the processor is to characterize each detected source and decide which sources are extended or resolved with respect to the point spread function (PSF). Sources that are deemed extended are measured further and the information is written into a separate table. In addition to tabulated source information, a small "postage stamp'' image is extracted for each extended source from the corresponding J, H and $K_{\rm s}$ Atlas images. The source lists and image data are stored in the 2MASS extended source database. By the time GALWORKS is run in the 2MASS pipeline, point sources have been fully measured with refined positions and photometry, band-merged, coordinate positions calibrated, Atlas images constructed, and the time-dependent PSF characterized for every Atlas image. The high-level steps that encompass GALWORKS include: (1) bright star (and their associated features) masking, (2) Atlas image background subtraction, (3) measurement of the stellar number density and confusion noise, (4) source parameterisation and attribute measurements, (5) star-galaxy discrimination, (6) refined photometric measurements, and finally (7) source and image extraction (see Jarrett et al. 2000a for more details).

The sample selected for this study was extracted before the 2MASS data acquisition was completed, using an earlier version of the software extraction algorithms. However, comparisons between the final data and the earlier results show they are consistent. We also used the full 2MASS database, not just the high signal-to-noise sources that form the final catalog, so that our sample includes many fainter sources than are part of the publicly released catalogs.

2.2 Low Central Surface Brightness (LCSB) source processor

There are some galaxies whose central surface brightness is too low to be detected by the standard 2MASS procedure, but whose total integrated flux is significant. These may include low surface brightness galaxies and dwarf galaxies. We will refer to these sources with the generic moniker: Low Central Surface Brightness (LCSB) galaxies. LCSB galaxies present a different challenge to GALWORKS than the typical "normal'' galaxy 2MASS encounters. They are generally very faint (as measured in a standard aperture for "normal'' galaxies) and they do not have well defined cores; see Jarrett (1998) for examples. The LCSB processor was an experimental algorithm executed last in the chain of operations that comprise GALWORKS. Sources detected by this algorithm did not meet the stringent reliability criteria for inclusion in the public 2MASS catalogue, but it did occasionally identify interesting LSB galaxies, as confirmed with deep optical images. There are also some examples of galaxies observed to be low surface brightness in the near-infrared that have normal surface brightness in the optical, see, e.g., Galaz et al. (2002).

The input to the LCSB processor is a fully cleaned Atlas image in each band, where stars and previously found extended sources have been entirely masked. The image is then blocked up (using three independent kernel sizes: $2\times2$, $4\times4$ and $8\times8$ pixels) and "boxcar'' smoothed to increase the signal-to-noise ratio for large (but faint) objects normally hidden in the pixel noise. The detection step consists of 3-$\sigma$ threshold isolation of local peaks in cleaned, smoothed images. Source detections are then parameterised, with the primary measurements being: signal-to-noise ratio of the peak pixel, radial extent, integrated signal-to-noise ratio, surface brightness, integrated flux, and signal-to-noise ratio measurements using a J+H+$K_{\rm s}$ combined "super-coadd'' image. In principle, the "super-coadd'' provides the best medium from which to find faint LSB galaxies, given the effective increase in the signal-to-noise ratio.

The LCSB processor could be falsely triggered by faint stars and the wings of the PSF around bright stars. Meteor streaks (and other transient phenomena) that were not fully cleaned from the Atlas images could also generate numerous false LCSB sources. It is important to note that LCSB-detected sources were nearly always fainter than the catalogue limit of the 2MASS survey, so their exclusion from the released catalogue does not significantly compromise its completeness. Further information and some early science results with 2MASS LCSB galaxies can be found in Jarrett et al. (2000a).

3 2MASS LSB galaxies selection

After a period of testing with various combinations of photometric parameters, we defined a modus operandi for the sample selection based on as few 2MASS parameters as possible, which allowed the definition of a sample with low infrared surface brightness values. The 2MASS central surface brightness limit of $\sim$20 mag arcsec^-2 in $K_{\rm s}$ band is equivalent to a B surface brightness of $\sim$24 mag arcsec^-2 for a typical spiral galaxy colour. This corresponds to fairly "bright LSB'' galaxies, easily detected in deep photographic and CCD optical limited-coverage surveys. However, as we shall show later in this paper, our selection criteria yield a LSB sample with interesting complementary and contrasting properties compared to optically-selected samples.

3.1 Selection using the K_s-band central surface brightness

In order to select infrared LSB galaxies, our key photometric 2MASS parameter is $\mu _{K5}$, the mean $K_{\rm s}$-band central surface brightness within a circle of radius 5 arcsec. This aperture was selected because for the great majority of faint galaxies in the 2MASS catalogue, this small fixed circular aperture gives good signal-to-noise statistics while avoiding problems due to confusion and missing flux in the faint outer parts of galaxies. The circular 5'' radius aperture also appears more reliable than the peak central surface brightness measured in a single pixel of the original 1.8 s integration.

We selected sources with $\mu_{K5}>18.0~ \hbox{\mbox{mag~arcsec$^{-2}$ }}$. The usefulness of this criterion for the selection of LSB galaxies has been shown in Jarrett et al. (1998) for selecting LSB galaxies in the Coma cluster and SA57 region.

3.2 Selection using source size

The size of the sources is also important for the sample selection:

• A fixed-diameter aperture gives the surface brightness over different physical areas within the galaxy, depending on its distance. For angularly small galaxies, the fixed aperture gives a surface brightness closer to the mean over the whole galaxy.
• The reliability of the catalogue is related to the size of the objects. For very small sources, confusion with stars increases significantly
• We planned also to obtain observation in the 21 cm H  I radio line, and flux levels tend to be correlated with angular size.

For these reasons, we selected two samples of galaxies based on r_K20, the $K_{\rm s}$-band semi-major axis at an isophotal level of 20 mag arcsec^-2. Our primary sample is of sources with r_K20>20'' (hereafter referred to as the "Large'' 2MASS LSBs sample), and a secondary sample with 20''>r_K20>10'' (hereafter referred to as the "Small'' 2MASS LSBs sample).

3.3 Selection using colour range

Two effects make galaxies appear "redder'' in the 1 to 2 $\mu$m window (see Fig. 14, Sect. 5, in the Explanatory Supplement to the 2MASS Second Incremental Data):

• their light is dominated by older stellar populations
• their redshift tends to transfer additional stellar light into the 2 $\mu$m windows, boosting the $K_{\rm s}$ band flux relative to the J band flux (K-correction)

In general, the $(J-K_{\rm s})$ colour falls within a fairly narrow range for nearby galaxies, $0.8<(J-K_{\rm s})<1.3$, and GALWORKS uses this fact to help discriminate galaxies from other Galactic extended sources. Because we are exploring a potentially unusual class of galaxies, we examined a wider colour range of sources from the "Working Survey Database'' of 2MASS (including uncertain sources that do not meet the completeness and reliability criteria for the 2MASS catalogue). To exclude most artifacts and confusing sources, we select sources with $0.5<(J-K_{\rm s})<2.0$. This range also allows for larger photometric uncertainties that are more likely to be found for LSB galaxies.

Figure 1: The sky coverage of the selected sample of 2MASS LSB galaxies is illustrated by the distribution of the objects which were observed in H  I. The plot is in equatorial coordinates; the dotted line indicates the Galactic plane and the dashed lines the $-2^{\circ }$ to 38$^{\circ }$ declination range covered by the Arecibo radio telescope. All sources have declinations between $-39^{\circ }$ and +60$^{\circ }$. The upper panel is for the Large sources ( rK20>20''), the lower for the Small sources ( 20''>rK20>10''). Dots indicate galaxies detected in H  I, crosses undetected objects.

3.4 Sky coverage

The presently available 2MASS database covers all the sky. At the time when the sample was selected (end of 1999) the declination range of $\sim$0$^{\circ }$ to +12$^{\circ }$ had not yet been covered, however, as can been seen in Fig. 1, which shows the sky coverage of the objects from our sample observed in the H  I line.

To select our sample of LSB galaxies, we exclude the region inside the Zone of Avoidance ( $\vert b\vert<10^{\circ}$) where the confusion rate between multiple stars and galaxies is high, as well as the declinations not suited for observations with the Nançay and Arecibo radio telescopes.

Thus the area of the sky covered by our survey ranges from $-39^{\circ }$ to $\sim$0$^{\circ }$ and from $\sim$12$^{\circ }$ to +60$^{\circ }$ in declination, and the galactic latitude of our sources is $\vert b\vert>10^{\circ}$.

3.5 Final sample

Using the first and second algorithms described in Sects. 2.1 and 2.2, we selected, respectively, 34 000 and 318 LCSB sources with a mean central surface brightness $\mu _{K5}$ fainter than 18 mag arcsec^-2. All sources have a radius r_K20 larger than 10 arcsec.

In order to decide which of these faint sources really are galaxies, additional data on them were used that were listed in online databases such as NED (NASA Extragalactic Database) http://nedwww.ipac.caltech.edu, LEDA (Lyon-Meudon} Extragalactic Database) - recently incorporated in HyperLeda [http://www-obs.univ-lyon1/hypercat/] - and Aladin of the Centre de Données astronomiques de Strasbourg (CDS) [http://aladin.u-strasbg.fr], and by inspecting their Digital Sky Survey (DSS) optical images. As the acquisition and interpretation of these supplementary data for 34 000 sources was deemed to be too laborious, and as we intended, after a first inspection of the sample, to concentrate our multi-wavelength observations (see Sect. 5) on the larger-sized objects, we limited this phase of the selection procedure to all 2000 objects in the subset of "large'' sources ( r_K20 > 20'') and to 3000 randomly selected objects in the subset of "small'' sources ( 20''> r_K20 > 10''). Using this procedure, we selected a total of 3736 and 59 candidate 2MASS LSB galaxies from the sources extracted by the GALWORKS standard and LCSB algorithms, respectively. The total sample of 3796 objects constitutes our working database of 2MASS LSB galaxies.

As the selected LCSB sources are not part of the standard 2MASS data released for public use, unlike the other sources, we show their near-infrared images in Fig. 2.

4 Basic properties of the sample

Some basic parameters of our working database of 3795 2MASS LSB galaxies are listed in Tables 1-3. We have divided the subsets listed in the Tables according to two criteria: processor and size. Tables 1 and 2 list the objects extracted using the standard algorithm for, respectively, the Large and Small sources, while Table 3 lists the Faint objects extracted using the LCSB algorithm.

It should be noted that the selection of the infrared sources presented in this work, which are all derived from 2MASS J, H and $K_{\rm s}$-band imaging, was made in late 1999, when work on the 2MASS database was still in full progress. The five-year evolution of both detection and source characterization was driven by improvements in the pipeline reductions and the image calibration. These are realized through preliminary database holdings and public "sampler'' data releases, incremental data releases and finally the All Sky data release that achieved its milestone in March of 2003. Accordingly, the current sample is a mixture of these data releases, which are described in the 2MASS Explanatory Supplement, see URL http://www.ipac.caltech.edu/2mass/releases/allsky/doc/explsup.html.

The Large and Small sources put in parentheses in Tables 1 and 2, respectively, are those that are only found in the All Sky working databases, and not in the subsequent, more reliable, public data releases. Only 23 of the 836 Large sources we selected from the working databases do not occur in later data releases, as do 27 from the 2900 Small sources. Of these 50 non-confirmed sources, 41 have an entry in the PGC and 24 in other optical galaxy catalogues.

The situation is different for the 59 Faint sources, as these were selected for our survey using a dedicated LSB source detection routine (see Sect. 2.2), and none of them appeared in the working databases. Seventeen of them do appear in later public releases, however: see Table 3, where, for the sake of consistency, we have also put the names of the Faint sources that are not found in later public data releases in brackets.

The basic parameters listed in Tables 1-3 are as follows:

1.

No: the "work name'', used throughout the present series of papers, which consists of the type of the source (L: large; S: Small; F: LCSB (Faint source) processor) followed by its number and an indication of its inclusion in other catalogues (P: only in PGC (see Paturel et al. 1989, as updated continuously in LEDA), O: in other catalogue(s), N: not previously catalogued). Sources in parentheses did not appear in later public data releases (see above);

2.

2MASS: gives the J2000.0 right ascension and declination coordinates of the 2MASS source;

3.

PGC: the PGC catalogue entry, if available;

4.

Other: refers to entries in other galaxy catalogues;

5.

$\mu _{K5}$: the mean central surface brightness (in mag arcsec^-2) measured within a radius of 5 arcsec around the source's centre in the $K_{\rm s}$ band;

6.

$\mu_{B_{25}}$: the mean B-band surface brightness (in mag arcsec^-2) within the D₂₅ blue isophotal diameter, at a level of 25 mag arcsec^-2, as listed in LEDA;

7.

Obs: information on available observations: A for our Arecibo H  I detections and "a'' for the non-detections (see Paper II), N for our Nançay H  I detections and "n'' for the non-detections (see Paper III), O for other published H  I detections (from LEDA, see Paper V), and P for our $BV\!RI$ optical surface photometry data (see Paper IV).

4.1 2MASS and comparison samples

To study the basic properties of our galaxy sample, we compared various subsets to existing samples of optically selected High and Low Surface Brightness galaxies. We compared near-infrared and optical data from LEDA for the objects in the following samples which were detected in 2MASS:

1.

2MASS L: our "Large'' LSB galaxies from the 2MASS survey catalogue with a 20 mag arcsec^-2 $K_{\rm s}$-band isophotal radius $r_{K_{20}} \geq20''$ [836 objects];

2.

2MASS S: same for the "Small'' objects, with $20'' \geq r_{K_{20}} \geq 10''$ [2900 objects];

3.

2MASS F: 2MASS sources with lower central surface brightness, extracted using the LCSB algorithm (see Sect. 2.2) [59 objects];

4.

NGC L: "classical'' HSB galaxies from the NGC, with $r_{K_{20}} \geq20''$ [1973 objects];

5.

NGC S: same, with $r_{K_{20}} \leq 20''$ [252 objects];

6.

LSB opt.: optically selected LSB galaxies from Impey et al. (1996) [83 objects].

For the last sample of 693 optically selected LSB galaxies (derived from the inspection of UK Schmidt photographic plates) 83 objects were found in the 2MASS working survey database (i.e., 12%). These LSBs found in the 2MASS database have a central surface brightness in B (measured as described by Sprayberry et al. 1996) between 18.2 and 25.0 mag arcsec^-2 with a mean value around 21.6 mag arcsec^-2 (i.e., the Freeman value for HSB spiral discs) compared to the other objects in the Impey et al. sample, which have a median value around 22.8 mag arcsec^-2.

Figure 3: Comparison between the normalized distributions of several measures of infrared surface brightness in the $K_{\rm s}$-band for the three sub-samples of 2MASS LSB galaxies (Large/Small/Faint) with three other samples of galaxies, one of optically selected LSBs and two of HSB galaxies from the NGC, as described in Sect. 4.1. The plotted parameters, which are described and discussed further in Sect. 4.2, are: $\mu _{K5}$ is the mean surface brightness measured within a circle of 5'' radius at the centre of each galaxy, $\mu _0$ is the highest surface brightness measured at the centre of the galaxy, and $\mu _{K_{21}}$ and $\mu _{K_{21}} (i=0)$ are, respectively, the average surface brightness measured within the 21 mag arcsec-2 isophotal contour in the $K_{\rm s}$-band and this value corrected to face-on $(i=0^{\circ })$.

4.2 Infrared surface brightness in the K_s band

In Fig. 3 we compare several different measures of the $K_{\rm s}$-band surface brightness for the subsets of the 2MASS LSB sample and the optically selected samples:
$\bullet$ Central $K_{\rm s}$-band surface brightness: $\mu _{K5}$ is the primary selection criterion for inclusion in our 2MASS LSBs sample, the mean surface brightness measured within a circle of 5'' radius at the centre of each galaxy. Both the Large and Small 2MASS samples exhibit the highest counts at the 18 mag arcsec^-2 cut-off, while the sources detected with the LCSB algorithm peak about 1 mag arcsec^-2 lower. The 2MASS-selected sources span the lower surface brightness range of the optically selected LSBs detected by 2MASS. By contrast, the NGC sample objects are, on average, about 1.5 to 2 mag arcsec^-2 brighter than the Small and Large 2MASS samples, respectively. The difference between the two NGC samples appears to be due to the inclusion of more of the disc in the small galaxies within the 5'' radius aperture.
$\bullet$ Peak $K_{\rm s}$-band surface brightness: $\mu _0$ is the highest surface brightness measured in any of the 2'' camera pixels near the centre of the galaxy during the original observations. 2MASS made six observations in a dithered pattern so that one observation was likely to be well-centred on the galaxy nucleus and should normally have the highest surface brightness. The results for the various samples are approximately the same as for the central surface brightness, although the Large and Small 2MASS samples become better distinguished. The small galaxies have slightly higher peak surface brightness values on average because the ${\sim}1''$ radius aperture is more dominated by the bulge than the 5'' aperture, whereas the measurements of the larger galaxies were already more bulge dominated.
$\bullet$ Mean isophotal surface brightness and mean face-on isophotal surface brightness: $\mu _{K_{21}}$ and $\mu _{K_{21}} (i=0)$ are, respectively, the average surface brightness measured within the ellipse fit to the $K_{\rm s}$-band 21 mag arcsec^-2 isophotal contour and this value corrected to face-on $(i=0^{\circ })$. The latter value simply uses the major axis diameter as a measure of the face-on radius. These definitions corresponds to older, optical, definitions of surface brightness that used the B=25 mag arcsec^-2 isophotal size, D₂₅. Note again that our 2MASS samples exhibit some of the lowest infrared surface brightness values of any of the samples. As this figure shows, especially the Large sample is expected to contain a relatively many highly inclined, intrinsically quite LSB sources, due to selection effects (see Sect. 4.3). The optical LSB sample has relatively high surface brightness levels under this measurement scheme, because these galaxies may have a bright bulge even though their disc component has a low surface brightness, and a significant fraction may even have relatively bright discs, as the Impey et al. sample contains a significant number of non-LSB galaxies.

Figure 4: As in Fig. 3, for a number of other infrared photometric parameters: rK20 is the major-axis radius at the 20 mag arcsec-2 isophotal level in the $K_{\rm s}$ band, K20 is the total magnitude within the 20 mag arcsec-2 elliptical isophote in the $K_{\rm s}$ band, b/a is the minor-to-major axis ratio determined from an ellipse fit to the co-addition of the J-, H-, and $K_{\rm s}$-band images, and (J-K)20 is the difference between the J- and $K_{\rm s}$-band magnitudes measured within the $K_{\rm s}=20$ mag arcsec-2 elliptical isophote; note that the left half of the NGC S and NGC L curves overlap in the bottom panel. See Sect. 4.3 for further details on these parameters.

4.3 Other infrared properties

We compare a few other basic properties of the infrared emission in Fig. 4:

$\bullet$ $K_{\rm s}$-band isophotal radius: r_K20 is the major-axis radius at the $K_{\rm s}=20$ mag arcsec^-2 elliptical isophote. Our 2MASS samples tend to be dominated by sources near the minimum radius, while the NGC samples are weighted toward angularly larger objects. The optical LSB sample is also dominated by smaller sources.
$\bullet$ $K_{\rm s}$-band isophotal magnitude: K₂₀ is the total magnitude within the $K_{\rm s}=20$ mag arcsec^-2 elliptical isophote. Here again the 2MASS and optical LSB samples are weighted toward sources nearer the completeness limits of 2MASS, while the NGC samples include relatively bright objects.
$\bullet$ Infrared axis ratio:  b/a is determined from an ellipse fit to the co-addition of the J-, H-, and $K_{\rm s}$-band images. The fit is made at the 3-$\sigma$ isophotal level relative to the background noise in each image. (The Faint 2MASS LCSBs sample was not measured in this way because of the low S/N levels of the emission.) A sample of randomly oriented disc galaxies would exhibit a relatively flat distribution of b/a, while inclusion of elliptical galaxies and systems dominated by the bulge component tends to give a rising distribution toward larger values of b/a (e.g., Mihalas & Binney 1981). The NGC and optical LSB samples exhibit some tendency toward the distribution expected for bulge domination in the infrared, but the 2MASS samples show dominance by high-inclination systems, which is more pronounced for the Large sample than for the Small sources. This is due to the combined effects of the limits in observed central surface brightness and in apparent diameter, since, measured at a given isophotal level, highly inclined galaxies appear larger than more face-on objects with a similar intrinsic surface brightness profile. In particular the Large sample will contain an over-representation of highly inclined, intrinsically quite low surface brightness sources.
$\bullet$ Infrared colour: (J-K)₂₀ is the difference in J- and $K_{\rm s}$-band magnitudes measured within the $K_{\rm s}=20$ mag arcsec^-2 elliptical isophote. The samples peak near (J-K)=1, which is found quite generally for all galaxy types. The LCSB sample is bluer (0.9 mag), while the Small 2MASS sample is somewhat redder (1.2 mag) than the average. Although these colour differences may partly reflect differences in the K-correction due to galaxy redshift (bluer for nearer, redder for more distant), these are estimated to be of the order of 0.1 mag at most, however, and cannot explain the much larger observed differences.

Figure 5: As in Fig. 3 for a number of optical and optical-infrared colours, based on total corrected extrapolated magnitudes from 2MASS measured in the $K_{\rm s}$ band and from LEDA measured in the U, B, V and I bands. See Sect. 4.4 for a discussion of the plotted parameters.

4.4 Optical-infrared colours

In Fig. 5 we compare optical and optical-infrared colours of the 2MASS and optical samples. We show several combinations based on total corrected extrapolated magnitudes from 2MASS measured in the $K_{\rm s}$ band and from LEDA measured in the U, B, V and I bands.

The total corrected $K_{\rm s}$-band infrared magnitudes, $K_{\rm T}$, were derived by modelling the increase in flux with successively larger apertures and extrapolating to a total magnitude. No corrections were applied for inclination or extinction, as these are in practice negligible at this wavelength. The estimated uncertainty in the extrapolated $K_{\rm T}$ magnitudes is of the order of 0.15 mag for $K_{\rm T}\sim13$ mag, a typical value for the sample.

The total corrected optical magnitudes from LEDA are mostly derived from isophotal magnitudes, with corrections for galactic extinction, inclination and extinction effects (see Paturel et al. 1997). As the extinction correction depends on the morphological type, only galaxies with a $B_{\rm T_{c}}$ value and a morphological type listed in LEDA were considered. This limits the percentage of useable 2MASS LSB galaxies in the Large, Small and Faint categories to 63%, 15% and 5%, respectively, and the optically selected LSBs to 60%.

In comparisons between the U, B, V, and I bands, both the Large and Small 2MASS samples tend to be bluer than the optical samples: the optical LSB sample ("LSB opt'' in plot) is next bluest, and the NGC samples exhibit the reddest colours. (The LCSB Faint source sample had too few sources with LEDA optical magnitudes to show meaningful colour distributions in these plots.) It is well established that the average HSB galaxy tend to be redder than the average, non-dwarf LSB (e.g., O'Neil et al. 1997; Gerritsen & de Blok 1999; Burkholder et al. 2001). The presence in the Impey et al. "optical LSB'' sample of a significant fraction of galaxies with relatively high central surface brightness, which can in fact be considered as HSBs, may well explain the intermediairy colours found for this sample.

Regarding the $(B_{\rm T_{c}}-K_{\rm T})$ colour, the Large and Small NGC galaxies have an average of 3.6 and standard deviations of 1.3 and 0.3, respectively, while the optical LSBs are slightly bluer, $3.2\pm0.8$. Of the 2MASS samples, that of the Faint objects is the reddest on average, $3.2\pm0.6$, while the Small sources are also fairly red, $3.0\pm1.1$, but the mean of the Large 2MASS sample is $2.7\pm0.9$. Thus the infrared LSBs are not necessarily optical LSBs, according to our working definition of $\mu_{B_0,{\rm d}}>22$ mag arcsec^-2, as the adopted $K_{\rm s}$-band selection limit of 18 mag arcsec^-2 corresponds to a mean blue value of $\sim$20.8 mag arcsec^-2 for their mean colour, though this includes the (unknown) contribution from the bulges.

5 Discussion and further observations

Through a simple definition of infrared surface brightness based on the magnitude in a small fixed aperture, we have identified a sample of infrared LSB galaxies. This definition has been shown to work well at selecting LSB galaxies in the Coma cluster and SA57 region (Jarrett et al. 1998), and we find that our sample has low infrared surface brightness levels compared to optically-selected samples of HSBs and LSBs detected by 2MASS.

We had initially expected an infrared-selected sample of LSB galaxies to have redder colours than optical samples, but instead it appears that by requiring $\mu_{K5}>18$ mag arcsec^-2, we may have succeeded primarily in eliminating galaxies with significant bulge contributions. This already suggests that there is not a significant red population of LSB galaxies, although we note that the Large and Small 2MASS samples span a wide range of colours, particularly as measured in $B_{\rm T_{c}}-K_{\rm T}$.

To better understand the infrared LSB galaxies' properties we have carried out a multi-wavelength study of subsets of manageable size. These results will be described in subsequent papers (II-V). For observations in the 21-cm H  I line we selected two subsets: one of 367 Large, Small and Faint 2MASS LSBs for observations at Arecibo and another of 334 Large 2MASS LSBs for observations at Nançay, taking into account the difference in sensitivity and sky coverage of the two telescopes. The Arecibo and Nançay data will be presented in, respectively, Papers II and III of the present series. We have obtained CCD surface photometry of 35 objects in the B, V, R and I-bands using the 1.5-meter telescope at the San Pedro Martír Observatory in Mexico. These surface photometry data will be presented in Paper IV. Finally, in Paper V we will further analyse the infrared LSBs to better understand, e.g. their properties as a function of their colours, investigating whether there is a significant population of red LSB galaxies, and to see if these objects follow the "standard'' Tully-Fisher relation of HSB galaxies. In a related paper (Boissier et al. 2003), we present models of the evolution of samples of LSBs, including the 2MASS objects for which we obtained optical surface photometry.

Acknowledgements

We want to thank the referee, Dr. N. Bergvall, for his comments. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center, funded by the National Aeronautics and Space Administration and the National Science Foundation. This research also has made use of the Lyon-Meudon Extragalactic Database (LEDA), recently incorporated in HyperLeda, the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration and the Aladin database, operated at the CDS, Strasbourg, France. We acknowledge financial support from CNRS/NSF collaboration grant No. 10637.

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6 Online Material

 

 

Table 1a: Large objects.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
L1P	0006240+465851	2290356		18.02	24.77
L2P	0007208-280714	0571		18.22	24.32
L3O	0010167+305057	0726	UGC 93	18.54	25.65	O
L4P	0013146+404632	2170755		18.29	24.6	n
L5O	0014007+125749	0924	UGC 132	19.15	24.38
L6O	0014039-231054	0930	MCG -04-01-021	18.87	24.18	N,O
(L7O)	(0019092-243115)	1241	ESO 473-G11	18.47	22.95
L8O	0019256-040456	1261	MCG -01-01-077	18.36	22.94	N,P
L9O	0020006-062008	1288	MCG -01-02-001	18.75	23.37	N
L10O	0021312+293944	1387	UGC 207	18.01	23.61	O
L11O	0022570+161510	1478	UGC 219	18.38	23.6	O
L12O	0023481+144101	1511	UGC 226	18.04	23.53	A,P
L13O	0024028+162911	1525	NGC 100	18.06	24.49	O
L14O	0026463-334037	1651	NGC 115	18.13	23.21	O
L15O	0028281-072324	1751	MCG -01-02-021	18.55	23.68
L16O	0030298-084700	1862	MCG -02-02-033	18.02	23.04	O
L17O	0030459-292034	1879	ESO 410-G16	18.35	22.85	N
L18O	0031448-050908	1941	NGC 145	19.29	22.90	O
L19O	0032324+232342	1971	UGC 321	18.84	23.42	A,O
L20O	0033168-114120	170423	GSC 5271 01985	18.01	22.68	N,P
L21O	0034559+315655	2094	UGC 00346	18.02	23.39	O
L22O	0035274-104638	90484	FGC 63	18.56
L23O	0037092-175743	2219	ESO 540-G5	18.54	23.65	n
(L24O)	(0037574-091509)	2269	MCG -02-02-073	18.03	22.99	O
L25O	0038324-242023	2305	IC 1561	18.66	23.09	O
L26O	0038478+142858	1459324		18.48	24.64	a
L27O	0040562-015202	90490	FGC 75	18.44	23.70
L28O	0041449+362124	2493	NGC 218	19.69	24.12	O
L29O	0041576-325810	2510	ESO 351-G2	18.87	23.46	N
L30O	0044344-082048	2647	MCG -02-03-005	18.19	22.99
L31O	0046244+293726	2711	CGCG 500-083	18.81	24.59	O
L32O	0046342+294330	1875902	CGCG 500-085	18.67	23.75	O
L33O	0055215+314038	3274	UGC 565	18.40	23.67	O
L34O	0056269+503720	3363	UGC 576	18.05	23.77	O
L35O	0058084-061459	3472	MCG -01-03-050	19.09	23.85
L36O	0100136-304836	3595	ESO 412-G1	18.19	22.82	n
L37O	0101340-073517	3671	NGC 337A	19.33	25.29	O
L38O	0105048-061245	3853	MCG -01-03-085	18.07	24.28	O
L39O	0105188-052520	3861	MCG -01-03-089	18.13	23.74	N,P
L40N	0105335+353854			18.05
L41P	0106015-060925	1036120		18.16	24.13	n,P
L42O	0109560+204617	4148	UGC 723	18.58	23.76	O
L43O	0109575-014458	4151	UGC 726	18.75	23.95	O
L44O	0110192-354410	4173	ESO 352-G15	18.24	23.42	O
L45O	0110374-031324	4192	MCG -01-04-006	18.62	23.28	N
L46O	0111215-181646	4272	MCG -03-04-025	18.99	23.45	n
L47O	0111312+231256	4278	CGCG 480-048	18.11	23.55	O
L48O	0112390+383020	4355	UGC 755	18.27	23.81	O
L49O	0114254-072842	4471	MCG -01-04-016	18.08	23.36	n
L50O	0114443+502709	4481	UGC 786	18.42	23.89	n
L51O	0115495+310448	4561	NGC 444	18.29	23.70	O
L52O	0115539-322838	4566	ESO 352-G30	18.29	23.28	N
L53O	0117369+490042	4650	UGC 825	18.24	24.26	N,O
L54O	0117515-015721	4659	UGC 830	18.99	24.80	O
L55O	0117520-361847	4661	ESO 352-G36	18.83	22.98	n
L56O	0118402+310209	4698	UGC 835	18.65	23.66	O
L57O	0119042-000819	4734	UGC 847	19.04	23.92	N,O
L58O	0120050-335400	4799	NGC 491A	18.80	23.49	O
L59O	0122228-363630	4991	ESO 352-G58	18.09	23.85	N
L60O	0124299+154603	5181	UGC 955	18.54	23.68	O
L61O	0128568-163059	5532	MCG -03-04-075	18.79	23.06	N
L62O	0129399-221927	5571	ESO 476-G14	18.21	23.65	N
L63O	0131267+141637	5673	UGC 1087	18.03	23.99	O
L64O	0133176+131956	5792	UGC 1110	18.93	24.26	O
L65O	0139339-120438	6141	MCG -02-05-032	18.64	23.27	n
L66O	0141070-053405	6228	MCG -01-05-017	18.15	23.55	O
L67O	0141493-281450	6257	ESO 413-G23	18.01	23.42	O
L68O	0142271+135836	6292	UGC 1195	18.72	24.16	O
L69O	0142483+130918	6309	UGC 1200	18.72	23.82	O
L70O	0143029-341114	6319	IC 1722	18.41	23.33	N
L71O	0147306+271952	6574	IC 1727	19.21	24.08	O
L72O	0148562-234730	6655	NGC 686	18.76	23.63
L73O	0149098-100354	6667	UGCA 021	19.53	24.61	O
L74O	0149309+323510	6699	UGC 1281	19.30	23.09	O
L75O	0150124+271146	6756	IC 1731	18.03	23.77	O
L76O	0151084+215447	6833	IC 0167	18.20	23.99	O
L77O	0151519+170310	6893	UGC 1328	18.22	24.09	O
L78O	0154524-133915	7109	MCG -02-05-074	18.27	23.13	N,P
L79O	0155018+365511	7123	KUG 0152+366	18.26	24.01	O
L80O	0155289-310618	7176	ESO 414-G10	18.29	23.75	n

 

 

Table 1b: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
L81O	0155396+370219	7189	CGCG 522-068	18.05	23.27	a
L82O	0156210+372707	7254	UGC 1405	18.85	24.06	O
L83O	0157509+445503	7399	NGC 746	18.24	23.55	O
L84O	0158502-304004	7481	ESO 414-G19	18.03	23.12	N
L85O	0158518-080945	7485	KUG 0156-084	18.44	22.86	O
L86O	0159074-030859	7507	MCG -01-06-013	18.09	23.14	N
L87O	0159117-274838	7514	IC 1763	18.17	22.99	N
L88O	0200154-060530	7585	KUG 0157-063	18.16	22.86	N,P
L89O	0201122+194031	7663	UGC 1500	18.97	23.87	O
L90O	0201169+285025	7671	NGC 784	19.01	23.85	O
L91O	0201303-071731	7682	KUG 0159-075	18.15	22.88	N
L92O	0201351-311700	7690	ESO 414-G24	18.68	24.18	n
L93O	0201511-102803	7714	MCG -02-06-017	18.23	23.22	N
L94O	0203021-093919	7806	UGCA 023	18.02	23.46	O
L95O	0203201+183746	7826	UGC 1546	18.28	23.75	O
L96O	0203374+240432	7841	UGC 1551	18.77	24.44	O
L97O	0203412+261649	7843	CGCG 482-062	18.91	23.23	O
L98O	0206276+133952	1437074	FGC 243	18.78	25.57	n
L99O	0207082+425756	8078	UGC 1601	18.24	23.95	N,O
L100O	0207153+461519	90589	FGC 245	18.16	23.57	n
L101O	0208213+412846	8161	UGC 1626	18.07	24.11	O
L102O	0212026+462133	8424	UGC 1686	19.47	24.29	O
L103O	0212457+191107	8470	CGCG 461-061	18.31	23.83	O
L104O	0215387-100457	90602	FGC 269	18.92
L105O	0216096-115551	8673	IC217	18.09	23.46
(L106N)	(0217574+143306)	8775	NGC 877	18.52	22.93
L107N	0218006-025823			18.69		n
L108O	0218050+380436	8782	UGC 1767	18.26	23.60	O
L109O	0218512+334327	8829	UGC 1778	18.06	23.49	O
L110O	0220230+404731	8906	UGC 1796	18.66	24.56	O
L111O	0221227+163354		KPG 065A	19.16
L112O	0221252+252522	8954	UGC 1812	18.04	23.28	O
L113O	0223518-210138	9098	ESO 545-G12	18.32	23.42
L114O	0224247-020944	9126	UGC 1862	18.73	23.44	O
L115P	0227117+414120	2185194		18.04	24.29	n
L116O	0228124-012046	9394	UGC 1945	18.62	23.77	O
L117O	0228454-103047	9431	NGC 948	18.09	23.42	N,O,P
L118O	0228569-222104	9442	NGC 951	18.62	23.56	n
L119O	0230312-041300	9545	NGC 963	18.05	22.50
L120N	0232053-112516			18.08		N
L121O	0232180-350155	9658	ESO 355-G26	18.54	23.13	O
L122P	0233244+202330	1625902		18.04	24.73	A
L123O	0233281+220753	1664146	CGCG 484-009B	18.33	24.51	A
L124O	0234532-133938	9826	MCG -02-07-036	18.55	23.12	O
(L125O)	(0235204+405522)	9831	NGC980	18.55	24.11	N,O
L126O	0235327-070915	9846	NGC 991	18.16	23.88	O
L127N	0235567+322439			18.21		a
L128O	0236123+401210	9883	CGCG 539-059	18.10	25.53	n
L129O	0236321+313551	9902	UGC 2087	18.58	23.93	O
L130O	0238470+404155	10025	UGC 2126	18.30	24.06	O
L131O	0239425-211423	10085	ESO 545-G43	18.58	22.78	n
L132O	0240377+390326	10139	NGC 1023A	19.33	22.93	O
L133O	0241036-065558	10172	NGC1051	19.52	23.25
L134P	0241261-033936	1068434		18.27	24.88	n
L135O	0241550+320518	10218	UGC 2171	18.80	24.63	O
L136O	0242063-005335	10224	UGC 2177	18.28	23.67	N
L137O	0242460-212802	10271	ESO 546-G11	18.57	23.65	N
L138O	0243380-315641	10326	ESO 416-G12	18.12	23.49	N
L139O	0245142+351119	10421	UGC 2223	18.07	23.46	O
L140O	0245505+162521	10456	CGCG 463-008	18.14	23.33	O
L141O	0246534-223846	10526	ESO 479-G42	18.31	22.67	O
L142O	0248042-135935	10595	IC 1853	18.04	23.18	O
L143P	0249148-284019	132985		18.58	23.65
L144P	0251205-304655	10831		18.14	23.37	N
L145O	0255203+462016	11026	UGC 2383	18.01	24.55	O
L146N	0257297+195708			18.26		A
(L147N)	(0257331-090552)			18.21		n
L148O	0257535-022050	11202	IC 1870	18.33	24.08	O
L149O	0258215-020230	11245	UGC 2443	18.35	23.21	O
L150O	0258241-041743	11248	UGCA 47	18.36	24.01	O
L151P	0258245+443942	2249237		18.34	24.54	n
L152O	0300364+353745	11369	UGC 2466	18.12	24.38	O
L153O	0300373+401504	11371	UGC 2463	18.33	25.36	O
L154O	0302077+290623	11453	UGC 2497	18.32	24.40	O
L155O	0302385-185352	11480	NGC 1179	18.25	24.58	O
L156P	0303035-115056	145211		18.07	23.42	n
L157O	0303243-153725	11503	NGC 1189	18.35	23.59	N
L158P	0303285-095751	11510		18.15	24.39
L159O	0304555+212235	11592	UGC 2520	18.33	24.48	O
L160O	0305530+160701	11630	UGC 2532	19.04	24.57	A

 

 

Table 1c: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
L161O	0306290-094332	11656	IC 1880	18.79	24.45	N
L162O	0306403-325147	11665	IC 1885	18.23	23.38
L163O	0308272-230320	11750	IC 1892	18.83	23.33	O
L164N	0309131-141053			18.29		n
L165O	0309173+383857	11789	NGC 1213	18.81	24.73	O
L166P	0309401+365421	2089118		18.45	24.89	A
L167O	0310594+383932	11875	CGCG 524-060	18.35	24.39
L168O	0313292+440753	12005	UGC 2596	18.03	24.34	O
L169O	0313315-151526	12008	MCG -03-09-010	18.05	22.95	N
L170O	0314054-214627	12034	NGC 1258	18.24	23.00	N
L171P	0315264+410418	2175237		18.47	25.44	n
L172O	0316055-130203	12139	MCG -02-09-021	18.91	23.29	O
L173P	0316422+400344	213184		18.06	23.99	n
(L174O)	(0316451+400025)	12177	IC 311	18.63	24.51
L175O	0317246+363412	12216	UGC 2633	18.56	23.87
L176O	0318004+413106	12270	NGC 1264	19.09	23.56	n
L177O	0318185+385958	12282	UGC 2647	18.34	23.81
L178O	0318333-255004	12309	UGCA 064	18.32	23.57	O
L179O	0319344-322753	12404	IC 1913	18.31	23.66	O
L180O	0319538-033537	12439	FGC 410	18.09	23.83	n, O
L181O	0322416-041118	12650	NGC 1314	19.18	24.28	N
L182O	0322558-111207	12664	MCG -02-09-036	19.70	24.71	N,O
L183P	0323427+143037	1460054		18.32	24.58	A
L184O	0323483+403348	12702	UGC 2708	19.36	24.14	N
L185P	0324146+330920	2024928		18.10	25.53	A,P
L186O	0324484-212012	12754	NGC 1325A	18.21	23.61	O
L187O	0325247-161416	12798	UGCA 071	18.32	23.78	O
L188O	0327354-211341	12889	ESO 548-G21	18.66	23.43	O
(L189O)	(0329418-221644)	12989	NGC 1347	18.64	23.20	O
L190O	0329538+395020	12998	MCG +07-08-017	18.21	23.84
(L191O)	(0330358-175630)	13029	ESO 548-G28	18.22	23.28	N
(L192O)	(0332576-210521)	13150	ESO 548-G34	18.66	23.43	N
L193O	0333131+361103	13158	UGC 2780	18.31	25.32	O
L194O	0333297+402156	13180	UGC 2782	18.11		O
L195O	0333475-192931	13190	NGC 1359	18.02	22.97	O
L196O	0334381-172833	13235	ESO 548-G46	18.85	24.03	n
L197O	0334573-323823	13250	ESO 358-G20	18.88	23.24	O
L198O	0336173-253616	13304	ESO 482-G11	18.54	23.35	N
L199O	0337432-225436	13381	ESO 482-G17	18.76	23.63	n
L200O	0338512-094411	13432	MCG -02-10-003	18.13	23.41	n
L201O	0339283-130656	13464	IC 340	18.60	24.22
L202O	0339369+384123	13474	UGC 2808	18.36	23.61
L203O	0340415-223904	13532	ESO 482-G31	18.30	23.63	N
L204O	0340571-214249	13543	NGC 1414	18.41	23.17	N
L205O	0341296-043956	13568	IC 344	18.22	22.89
L206O	0342313-160005	13612	MCG -03-10-038	18.25	23.26	N
L207O	0343078-171106	13659	LSBG F549-029	18.37	23.53	n
L208P	0343516+414404	2185981		18.16	24.33
L209O	0345051+204542	13754	UGC 2850	18.76	24.43	O
L210P	0346291-111959	967071		18.20	23.97	n
L211O	0346556-114820	961488	FGC 452	18.39	24.55	N
L212O	0348141-212827	13871	ESO 549-G18	18.19	23.94	O
L213O	0348514-185845	13889	ESO 549-G22	18.52	23.44	O
L214O	0350397-251646	13952	ESO 482-G47	18.17	23.44	N
L215O	0350433-025141	13951	MCG -01-10-041	18.22	23.30	N,P
L216O	0350531+373637	13961	UGC 2876	18.73	25.05	A
L217N	0351556+385252			18.66
L218O	0352009-332803	13998	ESO 359-G3	18.43	23.51
L219O	0353180-102645	14037	MCG -02-10-018	18.66	23.56	N
L220O	0355047-061316	14100	MCG -01-10-047	18.44	23.73	N
L221P	0355478+164649	1516836		18.55	23.97	A,P
L222P	0358337-111759	967495		18.15	23.66	n
L223O	0400416-304951	14271	ESO 419-G13	18.41	24.00	N
L224O	0401376+244919	90699	FGC 464b	18.26	23.60	A,O
L225O	0409253-040927	14571	MCG -01-11-003	18.04	24.10	N
L226O	0410502-295535	14607	ESO 420-G8	18.12	23.34	N
L227O	0410505-295527	14607	ESO 420-G8	18.94	23.34	O
L228O	0411006-312426	14617	ESO 420-G9	18.33	23.38	O
(L229N)	(0412300-385436)			18.08
L230O	0413123+132519	14678	UGC 2984	19.03	24.77	O
L231O	0413589+365039	14709	UGC 2991	19.20
L232O	0414140+243943	14714	CGCG 487-028	18.42	23.13	O
L233O	0419044+261055	14853	UGC 3009	19.32	24.18
L234O	0419595-210502	14894	ESO 550-G22	18.14	23.48
L235O	0423105-071259	90710	FGC 481	18.29
L236O	0424492-010134	15057	UGC 3037	18.45	23.74
L237O	0429408-272430	15292	NGC 1592	18.29	23.20	N
(L238O)	(0430487-215452)	15344	ESO 551-G10	18.09	23.66
L239P	0430592-114510	177386		18.39	23.00
L240P	0431513-293708	133177		18.07	23.32	n

 

 

Table 1d: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
L241O	0435219-085619	997298	FGC 494	18.04	25.88
L242O	0436267-205043	15629	ESO 551-G18	18.06	22.77
L243O	0437498-122635	15688	MCG -02-12-048	18.49	23.17	N
L244O	0440148-241907	15780	ESO 485-G6	18.30	23.38	N
L245O	0440254-020127	15789	UGC 3127	18.58	23.81	O
L246O	0440388+170825	15799	UGC 3129	18.50	26.45	O
L247O	0441457-070516	15831	IC 387	18.94	23.28
L248O	0442290-214133	15858	ESO 551-G31	18.74	23.25	O
L249O	0443334-274006	15883	ESO 421-G13	18.06	24.34	N
L250N	0445255+182505			18.20		A
L251P	0446035-044309	1054464		18.02	23.57
L252O	0446072-020438	15958	NGC 1657	18.02	23.62	N,P
L253P	0447309+242207	1705745		18.76	24.27	A
L254P	0448017+282610	1835693		18.40	24.49	a
L255O	0451183-055738	16163	MCG -01-13-021	18.64	23.52	N,P
L256O	0455154-120927	16329	MCG -02-13-023	18.22	23.92	N
L257O	0455430-072005	16341	MCG -01-13-036	18.14	23.05
L258P	0458504-110500	178035		18.20	23.23	n
L259O	0459582-260137	16517	NGC 1744	18.78	24.36	O
L260O	0500455-295129	16543	ESO 422-G20	18.19	22.94	N
L261O	0501015-085726	16553	MCG -02-13-036	18.13	23.72	N,P
L262O	0501387-041533	16574	NGC 1741A	18.51	23.34	O
L263O	0502550-184609	16626	ESO 552-G56	18.48	23.28
L264P	0504455-092536	991209		18.16	24.49
L265O	0505070-314703	16702	ESO 422-G27	18.07	23.05	O
L266O	0507041-182521	16762	MCG -03-13-074	18.40		n
L267O	0507320-113905	16772	FGC 523	18.46	24.40	O
L268O	0508589-200044	16821	ESO 553-G11	18.76	23.42
L269O	0510046-145652	16850	MCG -02-14-002	18.40	22.77	O
(L270O)	(0510143-292359)	16854	ESO 422-G40	18.10	23.16	N
L271O	0511070-010441	16876	CGCG 395-013	18.97	24.24
L272O	0515387-224232	16990	ESO 486-G40	18.17	22.89	N
L273P	0517166+120504	1403526		18.45	25.72	A
L274O	0519270-324528	17098	ESO 362-G17	18.30	23.44
L275O	0528140-160728	17323	MCG -03-14-017	18.41	23.58	O
L276O	0531505-230843	17402	IC 2129	18.08	22.95	O
L277O	0534068-282754	17455	ESO 423-G2	18.02	23.13	O
L278N	0539281-004439			18.19		n
L279O	0541197-181642	17597	ESO 554-G24	18.08	23.39	O
L280N	0541365+513558			18.48		n
L281O	0543136-183820	17655	ESO 554-G28	18.73	23.21
L282O	0543282-302939	17662	IC 2147	18.29	22.99	O
L283O	0543523-191740	17668	UGCA 113	18.33	23.15	O
L284P	0545007+494013	2349901		18.76	24.17	n
L285O	0550539-144647	17978	UGCA 114	18.39	23.71	O
L286P	0551325-123801	949939		18.34	25.05
L287O	0555507-224824	18099	ESO 488-G44	18.70	23.65	O
L288O	0557284-295735	18138	ESO 424-G41	18.25	23.45	n
L289O	0558023-125546	148136	NPM1G -12.0210	18.24		N
L290O	0601082-214412	18259	ESO 555-G22	18.22	23.322	O
L291N	0602236-030330			18.47
L292O	0602426-122957	18315	IC 441	18.14	23.55	O
L293O	0603367-203915	18349	UGCA 118	18.46	23.76	O
L294O	0604429-260723	18377	UGCA 119	18.57	23.86	O
L295O	0608574-274806	18488	ESO 425-G10	18.02	22.73	O
L296P	0609212-140823	928447		18.83	24.13	N
L297O	0613188+530644	18651	UGC 3421	18.27		N
L298O	0613407+530619	18660	UGC 3424	18.01	24.75
L299O	0614368-302536	18693	ESO 425-G16	18.60	24.21	n
L300P	0617238-213956	825316		18.13	24.73
L301O	0623256-160943	18930	MCG -03-17-004	18.23	23.66	N
L302O	0624392-223549	18983	ESO 489-G50	18.53	25.05	N
L303O	0626230-314736	19047	ESO 426-G9	18.13	23.35	N
L304N	0627010-123153			18.24		N,P
L305O	0634277-274248	19269	ESO 426-G24	18.12	24.48	n
L306O	0640040-374548	19396	ESO 308-G24	18.43	23.35	n
L307O	0641352+501551	19440	CGCG 233-026	18.68	23.55	n
L308O	0643196-350925	19492	ESO 366-G11	18.12	23.27	N
L309O	0645516+452722	19561	CGCG 234-008	18.10	23.82
L310O	0649460+293133	19674	UGC 3551	18.11	23.92	O
L311O	0649573+253820	19682	MCG +04-16-003	18.12	22.69	O
L312P	0657029+424635	2205935		18.12	24.83	n
L313O	0711155+311014	20346	CGCG 146-033	18.03	23.52	A
L314O	0711574-352518	20373	ESO 367-G4	18.55	24.06	N
L315O	0720064+530036	20700	UGC 3799	18.49	23.78	O
L316O	0720334+490518	20719	CGCG 235-007	18.19	23.53	n
L317O	0721267+231059	20782	CGCG 117-017	18.96
L318O	0723447+332653	200234	UGC 3829	19.05	24.33
L319O	0727477+202347	21056	UGC 3862	18.40	24.03	O
L320O	0729174+275402	21120	UGC 3876	18.54	24.064	O

 

 

Table 1e: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
L321O	0740336+341348	21555	IC 2203	18.19	23.645	O
L322O	0740350+260805	21549	CGCG 117-064	18.28	23.813	O
L323O	0746187+390359	21754	CGCG 206-022	18.57	23.801
L324O	0748032+280141	21835	CGCG 148-026	18.16	24.324	A
L325O	0749057+283709	21881	CGCG 148-034	18.13	23.659	a
L326O	0753291+143641	22096	UGC 4077	18.61	24.24	O
L327O	0759220+180641	22389	UGC 4140	18.42	23.60	O
(L328O)	(0759559+472427)	22418	UGC 4136	18.50	23.80	n
L329O	0800062+130907	22433	UGC 4154	18.39	23.61	O
L330O	0801533+504415	22525	NGC 2500	18.06	23.30	O
L331O	0802121+321854	22545	KUG 0759+324	18.03	23.39	A
L332O	0804427+352357	22678	UGC 4201	18.50	23.70	O
L333O	0806112-031658	22748	CGCG 003-009	18.69	22.90	N
L334O	0813589+454434	23071	IC 2233	18.52	23.20	O
L335O	0815213+213330	23146	LSBC F561-02	18.03	23.28	O
L336O	0819021+211122	23319	UGC 4329	19.08	24.06	N,O
L337O	0819320+212339	23352	IC 2293	18.06	23.56	O
L338O	0820057-102913	23378	MCG -02-22-001	18.21	23.09	O
L339O	0820417-012455	23413	MCG +00-22-002	18.50	23.68
L340O	0822287-010243	23485	UGC 4370	18.26	23.44	O
L341O	0823519+144507	23559	UGC 4385	18.33	23.13	O
L342O	0825577-114645	23658	MCG -02-22-012	18.20	22.94	N
L343O	0827340-124524	23723	MCG -02-22-017	18.09	23.36	O
L344P	0832158-104420	152753		18.37	23.96
L345O	0832574-225403	23977	ESO 495-G17	18.49	23.53	N,O
L346O	0833230+293219	23998	NGC 2604	18.06	24.02	O
L347O	0833427-183153	24019	ESO 562-G16	18.56	22.18	n
L348O	0837450-191842	24246	ESO 563-G4	18.40	22.59	n
L349O	0839046-144423	24328	MCG -02-22-025	18.54	23	O
L350P	0839329-082901	1003139		18.48	23.86	N
L351O	0841204+535619	24421	CGCG 263-071	18.12	23.95
L352O	0843157-203945	24489	ESO 563-G16	18.85	23.42	N,O
L353N	0843512-185652			18.68
L354P	0843518-110808	969541		18.05	23.35	n
L355O	0844225-231255	24544	ESO 496-G5	18.35	23.93	n
L356O	0846355+190106	24656	UGC 4588	18.03	23.96	O
L357O	0851380-022159	24890	VV 041a	18.18	23.25
L358O	0856563-203138	25141	ESO 563-G34	18.04	23.142	N
L359N	0858094-152210			18.53		n
L360O	0900144+354352	25281	NGC 2719	19.29	21.71	N,O
L361O	0901017+354542	25331	NGC 2724	18.79	25.34	O
L362O	0902438+252516	25406	UGC 4746	18.07	23.65	O
L363O	0903081+173932	90887	FGC 828	18.29	23.42	A
L364O	0904337+451730	25472	UGC 4753	18.96	24.22	N,O
L365O	0907390+283810	1841518	FGC 842	18.69	25.68	n
L366N	0909504+205912			18.46		a
L367O	0911336+511516	25910	UGC 4824	18.59	23.93	O
L368O	0913163+312130	25984	CGCG 151-023	18.30	23.85	A
L369O	0915145+223845	26097	CGCG 121-044	18.10	23.73
L370P	0915558+175541	1545556		18.29	24.49	a
L371O	0917317+415932	26238	NGC 2799	18.43	22.95	N,O
L372O	0918125-182636	26276	ESO 564-G36	18.28	23.46	O
L373O	0918351+321611	26297	CGCG 151-053	18.01	23.17	O
L374O	0922337+501200	26541	UGC 4975	18.04	23.30	n
L375O	0923112+264900	26570	CGCG 151-073	19.55	23.58	O
L376O	0923370-102610	26609	NGC 2863	18.56	22.00	N
L377O	0926016+343911	26752	UGC 5020	18.76	24.58	O
L378O	0927073+423416	26802	CGCG 210-009	18.43	23.55	N
L379O	0927520+323912	26852	UGC 5041	18.14	23.60	O
L380O	0928590-144826	26905	MCG -02-24-027	18.09	23.03	O
L381O	0929175+302302	26915	CGCG 152-016	18.46	24.32	A
L382P	0929293-051228	1047805		18.28	24.02	n
L383O	0929352+243525	26944	CGCG 122-004	18.02	24.42	a,P
L384O	0935217+133255	27259	CGCG 63-015	18.33	23.61	A
L385O	0938552-045128	27515	MCG -01-25-011	18.04	23.42	n
L386O	0938557+354141	82492	KUG 0935+359	18.13	23.18	a
L387O	0940308-085636	27616	MCG -01-25-015	18.34	23.4	O
L388O	0940332+252921	27615	UGC 5156	18.17	23.22	A,O
L389O	0942232-061509	27747	MCG -01-25-024	18.77	23.13	O
L390O	0942492-160654	27774	MCG -03-25-016	18.60	23.24
L391O	0943550+144807	27857	CGCG 92-035	18.33	25.17
L392O	0945031-042947	90940	FGC 936	18.27		N
L393O	0949571-120548	28278	MCG -02-25-019	18.73		N
L394O	0951542-064916	28415	NGC 3035	18.50	22.70	O
L395O	0955464+322545	28645	UGC 5331	18.29	23.45
L396O	0957042-075301	28734	MCG -01-26-003	18.21	22.97
L397O	0958531+474411	28830	UGC 5354	18.81	24.51	O
L398O	1001090-192630	28995	ESO 567-G3	18.55	22.85
L399O	1004261-282638	29216	NGC 3113	18.27	23.56	O
L400O	1005255-174753	29281	ESO 567-G12	18.11	23.15	N

 

 

Table 1f: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
L401P	1010413-074003	1015078		18.82	23.48	N
L402O	1014216+220728	29865	UGC 5524	18.48	23.94	O
L403O	1014436-204836	29894	ESO 567-G28	18.32	23.45	N
L404O	1015038+211026	29924	UGC 5529	18.31	23.60	O
L405O	1015134-150534	29929	MCG -02-26-041	18.51		O
L406O	1017251+170532	30052	UGC 5552	18.57	23.68
L407O	1017478+215224	30068	NGC 3187	18.28	23.84	O
L408O	1020036+383656	30206	UGC 5577	18.10	23.33	O
L409O	1022407+461420	30386	UGC 5604	18.10	23.72	O
L410O	1023459+123349	30463	NGC 3230	18.56	24.23	N
L411O	1024175-054040	1041741	FGC 1062	19.17	25	n
L412O	1024241+280133	30508	NGC 3232	18.05	23.52
L413O	1024388-021935	30529	CGCG 009-022	18.12	22.74
L414O	1025056+170937	30560	NGC 3239	18.55	23.16	O
L415O	1027010+283824	30714	NGC 3245A	18.33	25.13	O
L416O	1028024-231522	30800	ESO 500-G44	18.03	22.84	N
L417O	1028208+223416	30818	UGC 5672	18.35	24.28	O
L418O	1031450+464018	31083	UGC 5714	18.47	23.68	N,P
L419O	1032167+274010	31122	NGC 3274	18.06	22.86	O
L420N	1032544+315657			18.13
L421O	1033024+223429	91024	FGC 1093	18.04	24.30
L422P	1033536+240119	31233		18.06	23.44	A,P
L423O	1036237+124226	31442	NGC 3299	19.31	23.94	O
L424O	1039469+475555	31720	UGC 5798	18.80	22.95	O
L425O	1042378-235608	31919	ESO 501-G80	18.39	23.12	O
L426N	1042485+132736			18.33
L427O	1043061+202513	31945	UGC 583	18.08	23.86	O
L428O	1043353-100923	31978	MCG -02-28-002	18.49	22.92	N
L429O	1046559+464235	32201	KUG 1043+469	18.94	23.47	N
L430O	1046572+595452	32204	UGC 5879	18.47	23.55	N,O
L431O	1048294-213805	32311	ESO 569-G9	18.53	23.60	O
L432O	1050134-011724	32463	UGC 5943	18.47	23	O
L433O	1051009+361135	32519	UGC 5951	18.73	23.40	O
L434O	1053125-072543	32681	MCG -01-28-004	18.09	23.35	O
L435O	1053238+164624	32694	NGC 3447a	18.94	25.04	O
L436O	1055232-073912	32817	MCG -01-28-006	18.02	23.30	N
L437O	1057389-253013	32946	ESO 502-IG 006	18.04	23.75
L438O	1059336-061646	156112	FGC 1176	18.01	23.58	N
L439O	1100237+164132	33163	UGC 6083	18.54	22.79	O
L440O	1100242-095842	33167	MCG -02-28-032	19.07	23.23
L441O	1101510+163626	33276	UGC 6104	18.32	22.96	O
L442O	1103216-050030	1050535	FGC 1189	18.05	25.07
L443O	1103433+285312	33408	NGC 3510	18.13	24.71	O
L444O	1109220-225232	33813	ESO 502-G20	18.40	23.26	O
L445O	1109530-234350	33860	IC 2627	18.11	23.23	N,O
L446O	1114298+222917	34247	UGC 6268	18.51
L447O	1117402+380309	34497	UGC 6307	18.01	23.02	N,O
L448O	1118175+185049	34556	UGC 6320	18.32	23.10	O
L449O	1120011+360556	34681	UGC 6338	18.25	23.31	O
L450O	1120398+311319	34733	UGC 6355	19.00	24.24
L451O	1125318+380337	35124	UGC 6433	19.15	23.71	O
L452O	1125453+240823	35138	CGCG 126-051	18.15	23.57	O
L453O	1127188+383951	35235	UGC 6454	18.16	23.82	O
L454P	1127189-053157	156602		18.22	23.20
L4550	1128100+165531	35292	NGC 3691	19.17	22.09	N,O
L456O	1133382-154617	35704	FGC 1272	18.35	23.45	O
L457O	1133438+172346	35701	UGC 6546	18.24	23.54	O
L458O	1136263+581130	35900	UGC 6575	18.35	23.55	O
L459O	1137500+475255	36008	NGC 3769A	19.00	22.89	N
L460O	1138215-162630	36049	MCG -03-30-004	18.33	23.07	N
L461O	1138440+334817	36079	UGC 6610	18.89	23.92	O
L462O	1140466+174746	36231	NGC 3806	18.40	23.62	O
L463O	1140544+561207	36238	NGC 3794	18.21	23.84	O
L464O	1141559+201911	36293	MCG +04-28-029	18.06	23.09
L465O	1142295+181955	36355	UGC 6670	18.05	23.55	O
L466O	1142394+244921	36363	UGC 6674	18.14	23.39	O
L467O	1143037+404935	36381	UGC 6679	18.34	23.22	n, O
L468O	1143297-122422	36422	MCG -02-30-025	18.74	23.47	N
L469O	1144148+550206	36506	NGC 3846A	18.52	24.2	O
L470O	1145261-100610	36643	UGCA 245	18.19	24.18	O
L471O	1145355+555312	36660	NGC 3850	18.70	23.83	O
L472O	1149238+163829	36929	UGC 6794	18.71	23.26	O
L473O	1150201+255742	36996	UGC 6806	18.27	23.55	O
L474O	1152308-035225	37196	IC 2969	18.42	22.28	N
L475O	1153508+332155	37308	IC 2973	18.27	23.61	O
L476O	1153544+204449	37311	UGC 6873	18.24	23.16
L477O	1154176+325143	37346	UGC 6878	18.27	23.44
L478O	1154547-271501	37377	ESO 504-G28	18.94	23.04	O
L479P	1155252-101703	170181		18.22		N
L480O	1155591+192652	91155	FGC 1335	18.18	23.51

 

 

Table 1g: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
L481O	1156249-121000	37518	MCG -02-31-002	18.54	23.46	N
L482O	1157489+251615	37629	CGCG 127-114E	18.01	23.34	O
L483O	1158339+424402	37692	IC 749	18.02	23.28	O
L484O	1158432+250238	37703	VV 216b	18.12	21.04
L485O	1158462-202001	37713	ESO 572-G33	18.34	22.80
L486O	1200190+503910	37832	UGC 6992	18.47	23.44	N
L487O	1201107-011750	37914	UGC 7000	18.66	22.89	N,O
L488O	1202257-041821	38008	MCG -01-31-002	18.17	23.00
L489O	1202463-290538	38037	ESO 440-G44	19.01	22.81	O
L490O	1203213+292510	38081	UGC 7031	18.27	23.91	O
L491O	1203348-252253	38114	ESO 505-G8	18.46	23.49	O
L492O	1204411-280658	38222	UGCA 267	19.23	23.73	O
L493O	1204495+321537	91167	FGC 1358	18.42	23.51	n
L494O	1206209+370050	38386	CGCG 187-007	18.24	23.67
L495O	1212045+324405	38874	KUG 1209+33	18.01	23.38
L496O	1212096+361014	38881	NGC 4163	19.06	24.09	O
L497O	1212205+291240	38897	NGC 4173	19.66	24.2	N,O
L498O	1212220+291218	38897	NGC 4173	19.27	24.2	O
L499O	1213447+363802	39023	NGC 4190	18.98	23.59	O
L500O	1215115-032628	39170	CGCG 013-112	18.68	23.39
L501O	1215127-273937	39175	ESO 505-G28	18.43	22.88	N
L502P	1216418-251505	781011		18.45	23.49	N
L503O	1217092+122714	39390	IC 3099	18.29	23.73	O
L504O	1217346+223226	39432	UGC 7321	18.61	24.29	O
L505O	1218309+053334	39537	NGC 4252	18.31	23.53	O
L506O	1219242+121805	39664	IC 3149	18.03	23.70
L507O	1219403+020446	39697	UGC 7370	18.50	23.28
L508O	1220237+391418	39807	CGCG 215-061	18.62	23.80
L509O	1220483+172914	39857	UGC 7399A	18.36	24.11
L510O	1221321+143648	39950	NGC 4298	18.07	22.64
L511O	1221387+154441	39965	IC 783	18.34	23.64
L512O	1222290-043904	40092	IC 784	18.10	23.26	N,O
L513O	1223016+155420	40171	NGC 4323	18.65	23.39
L514O	1225037+170055	40458	IC 3298	18.68	22.79	O
L515O	1227420+121855	40903	NGC 4436	18.08	23.47
L516O	1228359-222950	41041	ESO 574-G2	18.79	23.39	n
L517O	1229365-082614	41184	MCG -01-32-016	18.18	23.06
L518O	1230311+414200	41326	NGC 4485	18.09	22.78	O
L519O	1232032+164115	41531	NGC 4502	18.39	22.92	O
L520O	1232268+424217	41576	UGC 7690	18.47	23.02	O
L521O	1232418+140300	41608	IC 3476	18.21	23.38	O
L522O	1232480+373717	41620	UGC 7699	18.49	24.11	O
L523O	1233512+301639	41755	NGC 4525	18.04	23.65	O
L524O	1233567+152116	41763	IC 800	18.32	23.6	O
L525O	1234054+353108	41779	NGC 4534	18.57	23.89	O
L526O	1234492+174852	41853	IC 3530	18.41	23.76
L527O	1236224+400019	42045	UGC 7774	18.98	24.57	O
L528O	1240129-054758	42429	NGC 4597	18.85	23.77	O
L529O	1241203+144201	42558	IC 3658	18.87	23.53
L530O	1241229-030328	42559	CGCG 014-104	18.21	24.29
L531O	1242007-241750	42623	ESO 507-G1	18.02	23.95	n
L532O	1242373+142126	42699	NGC 4633	18.53	23.11	O
L533O	1243582+321010	42863	NGC 4656	18.32	24.25
L534O	1244035-054033	42868	DDO 142	18.86	24.03	O
L535P	1244398-052619	1044733		18.17	24.49	N
L536P	1244416-180312	873438		18.63	23.27	n
L537O	1244455+122105	42944	IC 3718	18.47	23.96	O
L538O	1244487-204706	42950	ESO 574-G28	18.39	24.05	O
L539O	1245319-003208	42999	NGC 4668	18.10	22.62	O
L540O	1245415-263802	43022	ESO 507-G8	18.23	23.22	O
L541O	1246148-132141	43071	MCG -02-33-006	18.63	23.26	N
L542O	1247545-215539	43199	ESO 574-G32	18.27	23.44	O
L543O	1248096-101111	43236	MCG -02-33-010	18.58	23.59
L544O	1249231-100711	43345	MCG -02-33-015	19.11	24.21	O
L545O	1249368+305043	43359	UGC 7978	18.04	23.36	O
L546O	1249423-043447	43385	NGC 4678	18.71	22.91	N
L547O	1250294-105120	43458	DDO 151	18.13	23.87	O
L548O	1250345-093111	43465	MCG -01-33-022	18.20	23.60	N
L549P	1251090-035539	158144		18.10	23.23	N
L550O	1251598-263716	43608	ESO 507-G29	18.16	23.53	O
L551O	1253002-240330	43742	ESO 507-G36	18.52	25.02
L552O	1253365-120104	43800	MCG -02-33-043	18.36	23.50	N
L553O	1254054-201102	43871	ESO 575-G21	18.08	23.18	O
L554O	1254191-034252	43894	CGCG 015-034	18.21	23.96
L555O	1255126+000659	44014	UGC 8041	18.11	23.71	O
L556O	1258173+143325	44432	UGC 8085	18.10	24.13	O
L557O	1301487-270728	44930	ESO 507-G67	18.22	24.12	O
L558N	1305102-045012			18.04
L559O	1307094-281340	45437	NGC 4965	18.08	23.09	O
L560O	1308377+540428	45561	UGC 8231	18.69	23.19	N

 

 

Table 1h: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
L561P	1309167-165311	892101		18.89	24.69	N
L562O	1309411-010253	45644	UGC 8238	18.27	23.49	O
L563O	1309507-241431	45666	ESO 508-G19	18.74	23.39
L564O	1310044+341050	45684	UGC 8246	19.16	24.93	O
L565O	1312520+403237	45889	CGCG 217-018	18.89	22.52	N
L566P	1313504-024216	117609		18.13	23.8	P
L567O	1313541+421235	45992	UGC 8313	19.12	23.54	O
L568O	1316132+360446	46189	UGC 8341	18.34	23.18	N
L569O	1316562-163534	46256	MCG -03-34-040	18.44	23.09	N
(L570O)	(1318100-011437)	46336	UGC 8360	18.05	23.84	O
L571O	1320527+573832	46589	NGC 5109	18.11	22.56	O
L572O	1321499-131230	46664	NGC 5105	19.37	22.84	N,O
L573P	1325301-073549	1016275		18.60	24.85	n,P
L574O	1327562-312910	98330	ESO 444-G46	18.57	24.5	n
L575O	1328100+464019	47231	NGC 5169	18.16	25.09	O
L576O	1328253-315129	47255	ESO 444-G47	18.29	23.43	O
L577O	1328335+465538	47270	IC 4263	18.78	24.51	O
L578O	1329362+582506	47368	NGC 5204	18.22	23.42	O
L579O	1329480-234059	47390	ESO 509-G30	18.77	23.50	N
L580N	1329480-225220			19.39		n
L581O	1331046-150605	47514	MCG -02-34-061	18.23	23.25
L582O	1332473+415155	47679	NGC 5214A	18.06	23.22	N
L583O	1334027+475455	47788	NGC 5229	18.77	24.55	O
L584O	1334394-234050	47844	ESO 509-IG 064	18.34	22.90
L585O	1335530-045536	47949	MCG -01-35-002	18.45	23.45
L586O	1337410-150615	48144	MCG -02-35-009	18.21	23.76	N
L587O	1340400+541958	48392	Holmberg V	18.04	23.49	O
L588O	1341173+334622	48441	UGC 8662	19.07	23.58	O
L589O	1343410+545707	91308	FGC 1661	18.17	24.22	n
L590P	1344086+292913	1867862		18.80	23.68
L591O	1344498+592525	48726	MCG +10-20-021	18.79	23.92	n
L592O	1345380-055904	48786	MCG -01-35-010	18.02	22.70	O
L593O	1347012+335336	48862	UGC 8713	18.24	23.46	O
L594O	1347069+335251	48869	UGC 8715	18.51	23.95	O
L595O	1348563+595008	49016	UGC 8741	18.31	23.44
L596O	1348567+595012	49016	UGC 8741	18.47	23.44	n
L597O	1349077-280016	49031	ESO 445-G48	19.30	23.67	N
L598O	1351472+505843	49215	IC 951	18.03	23.58	N
L599O	1352484+372926	49301	UGC 8795	18.66	23.43	O
L600O	1352545-010652	49308	NGC 5334	18.20	24.19	O
L601O	1353019+393449	49322	NGC 5346	18.21	24.53	O
L602P	1353346-270121	760834		18.26	24.51	N
L603O	1353376+360809	49370	NGC 5352	18.25	23.47
L604O	1355595-011541	49533	UGC 8844	18.04	23.96	O
L605O	1357472-345006	89801	CSRG 0754	18.43	23.24
L606P	1358022-341310	89802		18.22	23.63	N
L607O	1358550-263247		AM 1356-261	18.13		n
L608O	1359487+402248	49817	UGC 8917	18.63	23.86	O
L609O	1400288-343712	49855	ESO 384-G27	18.21	23.50	O
L610O	1401165+132448	49918	KUG 1358+136	18.87	23.76
L611O	1401213-330346	49923	NGC 5398	18.45	24.19	O
L612O	1401408+334945	49950	ARP 111	18.05	23.00
L613O	1405108-334539	50230	IC 4366	18.78	22.72	O
L614O	1406396-311249	50329	ESO 446-G9	18.16	22.87	N
L615O	1407054-311243	50360	ESO 446-G12	18.18	23.06	N
L616P	1407594-342215	89865		18.04		n
L617O	1409216+490215	50509	UGC 9056	18.04	23.04	O
L618O	1410030+541306	50581	UGC 9071	18.62	23.98	O
L619O	1411177+553043	50651	SBS 1409+557	18.38	23.62
L620O	1413300-293540	50799	ESO 446-G31	18.35	23.17	O
L621O	1413498+574610	50803	MCG +10-20-084	18.16	23.83	n
L622O	1414108+210116	50844	CGCG 133-016	18.01		n
L623O	1414140-185218	50852	ESO 579-G5	18.13	23.23	N
L624O	1416304+574843	50990	IC 995	18.63	23.09	O
L625P	1419445-165008	892797		18.96	23.39
L626O	1421293-331001	51304	ESO 385-G13	18.64	23.51
L627P	1422231-174025	51343		18.05	23.83	O
L628O	1422565+402501	51372	NGC 5603B	18.45	23.86	O
L629O	1424566+250129	51483	UGC 9236	18.07	23.07	O
L630O	1427322-311417	51628	ESO 447-G5	18.93	24.40	n, O
L631O	1428183+134649	51685	IC 1014	18.29	24.24	O
L632O	1428368+385957	51713	UGC 9291	18.26	23.85	O
L633O	1430313+404929	51839	UGC 9337	18.79	23.30	N
L634O	1433205+261229	52012	KUG 1431+264	18.95	23.25	N,O
L635O	1435333+125430	52159	UGC 9389	18.33	24.09	O
L636O	1439499-004306	52395	NGC 5705	18.58	24.37	O
L637O	1440261+335920	52424	NGC 5727	19.02	24.73	O
L638O	1442458-002105	52550	NGC 5733	18.18	22.71
L639O	1443558-182902	52612	ESO 580-G14	18.01	23.19	N,O
L640N	1445115-344405			18.34		N

 

 

Table 1i: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
L641O	1446510-315546	52775	ESO 447-G35	19.04	23.42	N
L642O	1447354-180414	52827	ESO 580-G30	18.27	23.57	O
L643O	1447561-141658	52853	MCG -02-38-015	18.63	24.10	N,O
L644O	1448271+314730	52874	IC 4509	18.11	22.32	N,P
L645O	1451123-202627	53035	UGCA 395	18.02	23.65	O
L646O	1453336+490807	53219	KUG 1451+493	18.14	23.30	n
L647O	1456333-243007	53412	ESO 513-G9	18.06	22.73	N
L648O	1502261-254847	53700	ESO 513-G14	18.46	23.47	N
(L649P)	(1502329-025150)	1081087		18.11		n
L650O	1505133+571907	53842	UGC 9704	18.35	23.67
L651O	1506463+125101	53961	CGCG 077-007	18.11	23.29	N
L652O	1510407-220137	54155	ESO 581-G21	18.32	23.33	O
L653P	1516129-115252	120860		18.74	24.2
L654P	1520526-285913	160462		18.28	23.61	N
L655O	1525169+532427	55047	UGC 9849	19.12	24.13	O
L656O	1526429+462639	55112	MCG +08-28-032	18.83	23.71	N
L657N	1527242-172215			18.32
L658O	1531574-244621	55328	ESO 514-G22	18.05	23.61	O
L659O	1532027-273750	55335	ESO 514-G23	18.34	23.18	O
L660O	1538313+214925	91463	FGC 1927	18.11	23.01
L661N	1540507-342101			19.26		N
L662O	1541121+153422	55793	IC 1133	18.17	23.32	O
L663O	1543242+142609	55867	UGC 9991	19.06	24.26	O
L664O	1543242+142609	55867	UGC 9991	19.06	24.26	O
L665O	1601211+161824	56700	UGC 10134	18.04	23.80
L666N	1601551-222731			18.21		n
L667O	1602162+491211	56778	UGC 10150	18.58	23.67
(L668O)	(1602345-254823)	56802	ESO 516-G2	18.01	23.36	N
L669O	1603106+492502	56846	MCG +08-29-040	18.11	23.60	n
L670O	1603469-224417	56889	ESO 516-G5	18.08	23.05	N
L671N	1604570-321710			18.64		n
L672O	1608396+120038	57275	CGCG 079-058	18.16	24.63
(L673O)	(1608463+164541)	57278	CGCG 108-158	19.20	23.30	n, O
L674O	1609297-290013	57312	ESO 451-G11	18.14	23.71
L675O	1610296+195715	57368	UGC 10243	18.10	23.29	O
L676O	1610443+572743	57384	NGC 6088	18.35	22.37
L677O	1610528+223732	57391	CGCG 137-051	18.50	24.25
L678O	1611002-322043	57399	ESO 451-G15	18.37		O
L679O	1615288+185427	57627	UGC 10297	18.39	23.66	O
L680O	1620008+333245	57852	KUGX 1618+336	18.03	23.05
L681P	1625543+435127	2230836		18.06	23.66	n
L682O	1628587+422511	91536	FGC 2039	18.49	24.00	n
L683O	1630074-303245	58369	ESO 452-G4	19.14	23.66	O
L684O	1631215+224149	58424	UGC 10435	18.05	23.94	O
L6850	1635100+461257	58544	IC 1222	18.42	23.77	O
L686O	1637275+465005	58624	MCG +08-30-036	18.22	24.44	n
L687O	1645574+395908	91553	FGC 2067	18.45	23.85	n
L688O	1650234+555018	59093	UGC 10589	18.42	24.19	N
L689O	1650561+594308	59109	UGC 10590	18.16	23.18	n
L690N	1651111-160153			18.22
L691O	1652580+533858	91565	FGC 2082	18.17	23.79	n
L692N	1653219-161713			18.48		N
L693O	1654470+363007	59244	NGC 6255	18.65	24.29	O
L694O	1656034+393844	59274	NGC 6257	18.03	24.37	O
L695O	1656105+345011	59276	UGC 10615	18.03	23.86
(L696O)	(1656166+550154)	59280	IC 1237	18.41	24.26
L697O	1702254+311308	84819	KUG 1700+312	18.26	23.27
L698O	1705335+382219	2125127	FGC 2107	18.34	25.57
L699O	1714474+522317	59921	CGCG 277-031	18.06	23.61	n
L700O	1716548+313139	59999	CGCG 170-010	18.69	23.99
L701N	1717133-125141			18.44
L702O	1718321+414006	91591	FGC 2126	18.05	23.80
L703O	1718514+495302	60052	UGC 10806	18.59	23.76	O
L704O	1718547+295122	60049	UGC 10799	18.03	22.77	O
L705O	1719223+490202	60073	VV 010b	18.96	23.89	N
L706P	1727232+121230	1405561		18.83	25.38	n
L707N	1727479+295117			19.07		n
L708N	1728392+152716			18.06		n
L709P	1729247-120739	957265		18.11	23.71	n
(L710O)	(1731392+321355)	60436	UGC 10890	18.58	23.20
L711O	1753367+582100	61058	UGC 11036	18.93	24.20	O
L712O	1803021+292225	61320	CGCG 171-049	18.01	23.85	N
L713O	1805048+171601	61377	UGC 11107	18.05	24.09	O
L714O	1807275+353348	61423	UGC 11124	18.71	24.41	O
L715O	1815469+252233	61657	UGC 11179	18.22	24.33
L716O	1817190+125646	61685	CGCG 084-032	18.22	23.62
L717O	1817566+303905	61699	UGC 11195	18.09	22.60
L718P	1818215+221224	1665576		18.08	25.23
L719O	1819580+143940	61746	MCG +02-47-001	18.02	23.80
L720O	1822530+122554	61802	UGC 11214	18.59		O

 

 

Table 1j: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
L721O	1831460+310523	61994	UGC 11264	18.05	23.43
L722O	1842201+460618	62282	CGCG 255-010	18.72	23.92	N
L723O	1846363+230247	2812817	CGMW 5-07537	18.74
L724O	1850074-342648	62474	ESO 396-G5	19.01
L725O	1853188+330359	62532	IC 1296	18.18	23.92
L726O	1900033+432620	62661	CGCG 229-012	18.17	23.63	N
L727O	1907080+414449	62784	CGCG 229-017	18.85	23.97	N
L728O	1908006+412547	62802	CGCG 229-020	18.25	23.74
L729O	1908189+430407	62807	UGC 11406	18.19	23.6	O
L730P	1909399+472538	2297982		18.69	23.79
L731P	1916324-384024	606434		18.49	24.01
L7320	1926373+494530	63212	IC 1301	18.12	23.56	O
L733O	1929177-205510	63275	ESO 594-G1	18.78	23.73	n
(L734O)	(1933188-330857)	63352	ESO 398-G8	18.37	23.13	N
L735O	1937276-172718	63425	ESO 594-G8	18.27	23.78	N,O
L736O	1940424-221613	63511	ESO 594-G11	18.44	22.60	N
L737O	1941463+503602	63534	CGCG 257-007	19.17	23.17	n
L738O	1948132-233029	63678	ESO 526-G6	18.53	23.60	N
L739O	1952561-250900	63776	ESO 526-G11	18.41	23.48	N,O
L740O	1957362-001406	63868	CGCG 372-002	18.25	23.92	N
L741O	2002039-273339	64007	ESO 461-G33	18.01	22.76	N
L742O	2005378-250842	64077	ESO 527-G8	18.04	23.02	n
L743O	2007377-210733	64140	ESO 595-G14	18.16	22.79	O
L744O	2015134-183910	92575	FGCE 1448	18.32	23.65	n
L745O	2017027-120651	64414	MCG -02-51-007	18.19	22.96	N
L746O	2018231-272726	64448	ESO 462-G7	18.73	23.31	N,O
L747O	2021261-220721	64521	ESO 596-G20	18.46	22.96	n
L748O	2021304-202516	64525	ESO 596-G21	18.74	22.97
L749O	2023389-281639	64605	ESO 462-G16	18.02	23.03	O
L750O	2027128-370947	64712	ESO 400-G23	18.76	24.44
L751N	2036015-335250			18.76		n
L752O	2042431-024601	91678	FGC 2286	18.69		N,O
L753O	2045178-351427	65312	ESO 401-G7	18.36	23.86	n
L754O	2047422-095712	65391	MCG -02-53-004	18.18	23.31
L755O	2048122-035221	65413	MCG -01-53-009	18.30		N,P
L756O	2052005+132950	65594	CGCG 425-015	18.13	23.78	A
L757O	2055062-310529	65707	ESO 463-IG 034	18.32	23.94
L758O	2055067-310530	65707	ESO 463-IG 034	18.18	23.94	N
L759P	2058016-354925	132331		18.12	23.18	n
L760O	2118531+154101	1490846	UGC 11719	18.23	25.24	n
(L761N)	(2123183+273431)			18.49		n
L762O	2132419-000724	66940	CGCG 376-008	18.80	23.90
L763O	2134186+331523	66980	CGCG 492-003	18.16	24.12	a
L764O	2136106+170341	67035	UGC 11774	18.61	24.06	O
L765O	2136162-224404	92680	FGCE 1622	18.32	23.65	N
L766O	2145578-344857	67310	ESO 403-G23	18.32	23.16	N
L767O	2158057-075042	140989	GSC 5802 00065	18.07		N,P
L768O	2203289-201901	67943	NGC 7188	18.14	23.12	O
L769O	2203532-165049	91725	FGC 2359	18.82		N
L770O	2208329-183728	68125	ESO 601-G23	18.25	23.99	n
L771O	2209116-202838	68158	ESO 601-G24	18.03	23.23	N
L772O	2209344-060651	68177	MCG -01-56-002	18.23	24.07	O
L773O	2209370-271447	68176	ESO 532-G23	18.49	23.22	N
L774O	2210507+411525	68221	UGC 11936	18.17	23.95	n
L775P	2212462+383404	2130585		18.08	23.93	n
L776P	2213271+371102	2094709		18.15	24.31	a
L777P	2216009-095612	984498		18.16	23.73	N
L778O	2218472-032946	68549	MCG -01-56-00	18.09	22.71	N
L779O	2219313+411422	68571	UGC 11986	18.43	24.19	O
L780O	2219384-251956	68576	ESO 533-G13	18.73	23.66	N
L781O	2221508+425704	68645	UGC 11999	18.57	23.70	N,O
L782O	2222356-040720	68691	NGC 7257	18.46	23.30
L783O	2223055-285716	68718	NGC 7259	18.04	22.57	N
L784P	2223348+344727	2054604		18.55	25.47	a
L785O	2225354-095658	68831	MCG -02-57-004	18.40	23.85
L786O	2228253+301736	68941	NGC 7292	18.74	23.14	O
L787O	2228469-150411	68958	MCG -03-57-008	18.09	23.98	O
L788O	2229599-050657	68996	IC 1447	18.68	22.68	N,O
L789O	2230420-283840	69027	ESO 468-G4	18.25	23.55
L790O	2230502+363348	69034	CGCG 514-048	18.15	23.22	A
(L791O)	( 2233495-285406)	69159	ESO 468-G14	18.36	23.85	n
L792O	2241023+192012	89517	FGC 2408	18.32	23.64	O
L793O	2241263+391732	69498	UGC 12156	18.32	23.57	O
L794O	2244347-225930	69635	ESO 534-G21	18.92	23.45	N
L795O	2245142-224344	69653	ESO 534-G24	18.61	23.26	O
L796O	2246055-192455	69678	ESO 603-G12	18.14	23.87	O
L797O	2249207-145013	91756	FGC 2421	18.29		n
L798O	2254252-202144	69969	IC 5261	18.15	23.32	O
L799N	2254424+435539			18.24
L800O	2257390+125458	70108	UGC 12264	18.85	23.91	O

   

Table 1k: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
L801O	2258011-034609	70127	MCG -01-58-009	18.95	22.65
L802P	2258027+322757	2800849		18.15		O, a
L803O	2258100+141832	70131	NGC 7437	18.65	23.76	O
L804O	2258283-103331	91765	FGC 2436	18.85
L805O	2258394+190407	1579500	FGC 2438	18.01	25.81
L806O	2259125+133620	70175	UGC 12281	18.21	24.27	O
L807O	2259414+240429	70197	UGC 12289	18.16	24.95	A,O
L808O	2300177+190733	70228	UGC 12296	18.01	23.82	O
L809O	2300483-352212	70253	IC 5269C	18.73	23.65
L810O	2302463+220545	70322	UGC 12326	18.12	24.52	O
L811O	2302489+215226	70323	IC 5282	18.20	24.04	O
L812O	2305201+165159	70433	UGC 12350	18.79	24.446	O
L813P	2312022+204721	1635906		18.47	23.91
L814O	2314126+133454	70761	NGC 7535	18.24	23.89	O
L815O	2314595+145919	70809	MCG +02-59-012	18.71		A
(L816O)	(2316000-015049)	70876	UGC 12466	18.58	23.16
L817O	2320116-015119	71118	UGC 12521	18.46	23.18	O
L818O	2320126+253547	71119	KUG 2317+253	18.04	23.28	O
L819P	2320521+432418	2219987		18.04	23.94	n
L820O	2321419+270414	71190	UGC 12545	18.57	23.99	O
L821O	2324336+235908	71354	UGC 12583	19.06	23.50	O
L822O	2325102+121820	71383	CGCG 431-060	18.21	23.19	a
L823O	2330015+270500	71597	UGC 12631	18.40	23.31
L824O	2333410+322303	71750	UGC 12666	18.04	23.15	O
L825O	2334383+231327	71785	UGC 12675	18.39	23.85	O
L826O	2341425-341212	72135	ESO 408-G16	18.08	23.54
L827O	2342309+280239	1824788	FGC 2526	18.41	24.83	O
L828P	2343174+444626	2251718		18.13	24.94
L829O	2347570+280747	91822	FGC 2536	18.42	23.86	A
L830O	2348568-163225	72499	NGC 7759A	18.12	22.25
L831O	2349195+475507	72523	UGC 12796	18.02	23.75	O
L832O	2355418+315358	72892	UGC 12845	18.50	24.96	O
L833O	2356097-272800	72933	ESO 471-G44	18.20	23.12	N
L834O	2356492-032058	72985	MCG -01-01-006	18.07	23.22
L835O	2359367+144824	73177	NGC 7800	18.08	23.48	O
L836P	2359437-290935	132729		18.55	23.36	n

Note: Obs: information on available observations: A for our Arecibo H  I detections and "a'' for the non-detections, N for our Nançay H  I detections and "n'' for the non-detections, O for other published H  I detections, and P for our $BV\!RI$ optical surface photometry data. No.: Source names in brackets are not found in later versions of the public 2MASS database (see Sect. 4).

 

 

Table 2a: Small objects.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
S1P	0000033-104315	974615		18.26	24.99
S2N	0000179+513620			18.73
S3O	0000222+343657	29	CGCG 517-010	18.47	23.22	O
S4P	0001187-351729	650806		18.79	26.09
S5O	0001539-301043	198768	DUKST 409-039	18.11	24
S6P	0002295+515310	2401995		18.20	24.29
S7P	0002452-250217	783321		18.14	23.5
S8O	0002495-315155	189	ESO 409-G8	19.38	23.61
S9O	0003379+202723	251	KUG 0001+201	18.19	24.16	a
S10O	0003512-275442	198774	DUKST 409-045	18.48	23.76
S11O	0004197-061138	90450	FGC 2	18.04	24.21
S12O	0005243-043015		NPM1G -04.00044	18.48
S13P	0005314-025329	1080508		18.45	25.53
S14P	0005315-302228	132721		18.33	22.95
S15O	0005483-073743	412	MCG -01-01-032	18.60	24.05
S16P	0006469-131829	939737		18.92	23.92
S17P	0007111-013549	1114975		18.48	25.16
S18P	0008072-004646	1134911		18.42	24.19
S19P	0008078-015802	1105227		18.14	23.91
S20O	0010423-320708	198794	DUKST 409-066	18.64	24.89
S21P	0010472-350542	653413		18.69	23.85
S22O	0011006-352508	199316	DUKST 349-062	18.07	24.21
S23P	0011013+212455	1649524		18.44	24.25	a
S24P	0011068-311705	706986		18.17	24.06
S25P	0011542+473115	2299686		18.61	24.52
S26O	0011559+230124	828	KUG 0009+227	18.81	23.23	O
S27O	0012089+221948	834	MCG +04-01-037	18.55	23.17
S28P	0012357-201907	134617		18.47	22.91
S29P	0014164-072333	1019747		18.44	23.99
S30N	0015169+143659			19.20
S31N	0015221+125906			18.24
S32P	0015248+174101	1538879		18.21	24.79
S33N	0015554-095011			18.85
S34P	0016288+173214	1535162		18.38	24.41
S35P	0016304-001602	1147615		18.30	23.21
S36O	0016316+161126	1088	CGCG 456-051	18.02	23.39	a
S37O	0016358-013619	1096	KUG 0014-018	18.99	23.74
S38P	0017140-102240	978948		18.73	24.34
S39P	0017345+165932	1521966		18.70	24.45	a
S40P	0017503-283454	143406		18.54	23.38
S41P	0017526+190918	1582373		18.19	24.93
S42P	0018424-264951	133680		18.03	23.7
S43O	0019429+295607	1266	MCG +05-01-073	18.42	23.37	a
S44O	0020308+383418	1312	CGCG 518-023	18.72	23.81	A
S45N	0020319-082301			18.86
S46O	0020326+152050	1316	CGCG 434-002	18.54		a
S47P	0020329-243551	788249		18.54	23.73
S48P	0021154-012612	1118692		18.92	24.28
S49P	0021196-343008	661370		18.34	24.56
S50P	0021351-311207	707944		18.02	24.07
S51P	0021410+000135	1155202		18.84	24.53
S52O	0021477+220136	1662109	CGCG 479-014B	18.58	24.16
S53O	0022014+234934	1694421	IRAS F00193+2332	18.26	24.57
S54P	0022107+231626	1684511		18.66	23.99
S55P	0022159-004524	143475		18.54	23.60
S56N	0022220-001726			18.70
S57P	0022280+221330	1665927		18.04	23.43
S58P	0022374+145628	1471031		18.60	24.4
S59P	0022507+144348	1465666		18.46	24.87	a
S60P	0023025-270211	760663		18.90	24.78
S61P	0023071-162523	898344		18.12	24.78
S62P	0023114-052550	1044813		19.12	24.21
S63P	0023118-014002	1113269		18.86	24.99
S64P	0023423-014523	1110936		18.17	23.37
S65P	0023464-012950	1117287		18.04	23.88
S66P	0023483-035120	1066013		18.16	23.34
S67O	0023507+160655	1501056	NPM1G +15.0013	18.02	23.63
S68P	0024052+154132	1490999		18.25	24.53
S69P	0024238+370225	2091822		18.08	24.08
S70P	0024490-334241	131857		18.23	23.07
S71P	0025279-010037	1129046		18.40	23.59
S72O	0025599+405822	1617	MCG +07-02-003	18.16	23.60
S73P	0026293+450157	2257486		18.33	24.89
S74P	0027372+520547	2406677		18.15	24.59
S75P	0027596+483216	2319724		18.44	24.51
S76O	0028023-145618	1728	MCG -03-02-014	18.25	22.92
S77P	0028117-172603	134657		18.20	23.45
S78O	0028229-305720	198821	DUKST 410-044	18.64
S79P	0028490+130510	1422600		19.19	24.6
S80P	0029184-270106	133676		18.80	23.28

 

 

Table 2b: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
S81O	0029264+172905	1803	MCG +03-02-014	19.30	24.19	a
S82O	0029331-150549	1812	MCG -03-02-017	19.16	23.26
S83O	0030294-164131	1856	MCG -03-02-018	18.16	23.33
S84P	0030392+360536	2074861		18.50	24.61
S85P	0030514-154504	906981		18.73	23.53
S86O	0031492-023153	1940	MCG -01-02-028	19.20	24.60
S87P	0031573-050807	1048844		18.19	24.01
S88P	0032015+213035	1651478		18.42	23.86
S89P	0032017+261515	1769117		18.64	24.49
S90P	0032436+130904	1424098		18.19	24.18
S91P	0032551+151522	1479643		19.08	24.8	a
S92P	0033142+120600	1403781		18.67	24.37
S93O	0034139-212811	2046	ESO 540-G2	18.29	23.17
S94O	0034160-071732	2049	MCG -01-02-033	18.35	23.20
S95O	0034199-073600	2059	IRAS 00318-0752	18.15	23.08
S96P	0035569-030552	143639		18.19
S97P	0036017-300858	720800		18.16	23.88
S98P	0036485-111619	967861		19.13	23.92
S99P	0036508-070838	1023784		18.87	24.24
S100P	0037177-022142	1094204		18.35	23.56
S101P	0037325-252439	198207		18.14	23.8
S102P	0037398-064226	1029742		18.40	24.63
S103P	0039008-075902	1010025		18.99	24.59
S104P	0039182-285252	736261		18.32	24.82
S105P	0040215+223301	1672036		18.36	24.92
S106P	0040367-111950	967100		19.40	24.35
S107P	0042334-275245			18.21
S108N	0043197+235920			18.51
S109O	0043208-121100	2576	MCG -02-02-096	18.87	23.55
S110P	0044372+215509	1659934		18.46	23.64
S111P	0044419+181155	1552854		18.62	24.83
S112O	0045065+254657	2655	CGCG 479-068	18.44	23.89	O
S113N	0046292-094848			18.16
S114P	0047112+430545	2212912		18.20	24.45
S115O	0048458-114553	2853	MCG -02-03-020	19.16	24.45
S116P	0048586-302050	718310		18.64	24.02
S117P	0049023-324122	172953		18.47	23.35
S118N	0049147+503647			18.82
S119P	0050234+300335	1888602		18.40	24.09
S120P	0050581-055057	1039689		18.21	23.62
S121O	0051299-125039	3014	IC 56	18.56	23.18	O
S122P	0051365-175136	876298		19.00	24.68
S123P	0051478+154022	1490543		18.45	24.79
S124O	0052068+342503	73446	KUG 0049+341	18.53	23.75
S125O	0052156-272058	3061	ESO 411-G24	18.13	22.93
S126P	0052221-263420	3068		18.14	23.43
S127P	0052560+154707	1493287		18.80	24.41	a
S128P	0053029-031406	173059		18.48	23.84
S129P	0053134-071506	173068		18.14	23.85
S130P	0053351-074534	1013464		18.45	24.91
S131O	0054049+302044	3184	CGCG 501-035	18.07	23.50	O
S132P	0054350+312706	1947795		18.34	24.28
S133O	0054467-325535	3223	ESO 351-G19	18.21	23.39
S134P	0055064-065310	1027407		18.29	25.13
S135P	0055079-115716	959641		18.20	23.84
S136O	0055182+314349	3269	UGC 566	18.42	24.50	O
S137P	0055337+294438	1876630		19.03	25.01	a
S138O	0055355-100524	3288	MCG -02-03-045	18.16	23.51
S139O	0056127-003548	1139461	GIN 023	18.21	24.48
S140P	0056468+300825	1891795		18.44	25.16	a
S141P	0057249+312836	1949020		18.92	24.58
(S142P)	(0057363-165350)	891955		19.04	24.16
S143P	0057395+461818	2278901		18.35	24.37
S144O	0057519-194434	851100	IRAS F00553-2000	18.64	23.78
S145P	0058049-323616	689119		19.06	24.53
S146N	0058089-214553			18.18
S147P	0058191+135450	1443996		18.15	23.99
S148P	0059147-163527	896189		18.29	23.69
S149P	0100013-302452	132845		18.77	23.12
S150O	0101339+495955	2359814	NPM1G +49.0010	18.09	23.86
S151P	0101437+270654	1798205		18.74	24.85	a
S152P	0101471-210845	832085		19.24	23.75
S153P	0101511-031718	1073389		18.60	23.57
S154P	0102130-353133	131901		18.65	22.96
S155P	0102205+325840	2019367		18.45	24.36	a
S156P	0102426+172514	1532359		18.48	24.73
S157N	0102471-115159			18.58
S158P	0103218-355251	73553		18.87	23.57
S159P	0103323-212622	828271		18.49	24.25
S160O	0103488+311152	3787	UGC 653	18.78	23.40	O

 

 

Table 2c: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
S161P	0104249+211110	1644665		18.46	24.39	a
S162P	0105186+333615	2035469		18.37	23.98
S163P	0105482-115855	959259		18.97	24.43
S164P	0105535-231852	133732		18.32	23.47
S165P	0106075-042525	1058390		18.32	25.02
S166P	0106310-181122	871475		18.17	23.76
S167O	0106380+365325	3935	KUG 0103+366	18.36	23.32
S168P	0107133-355737	173492		18.12	23.13
S169O	0107519+321521	197572	AGC 111070	18.70	24.05
S170P	0108172+320523	1979705		18.02	23.45	a
S171P	0108187+321335	1986786		18.90	24.3
S172O	0108469-123632	4076	MCG -02-04-003	18.56	23.69
S173P	0108470-150621	73655		18.78	23.60
S174P	0108537-153030	73662		18.08	23.90
S175P	0109025-160033	4100		18.38	23.40
S176O	0109028-173223	134713	APMBGC 541-045-121	18.22	23.18
S177P	0109032-064752	1028539		19.35	24.12
S178P	0109059+144521	1466339		18.29	24.28	a
S179O	0109114-013443	4107	MCG +00-04-012	18.18	23.70
S180P	0109362+211616	1646522		18.65	23.92
S181O	0110020+180629	1550388	IRAS F01073+1750	18.15	24.19
S182O	0110290+431716	4184	UGC 728	18.21	23.98	O
S183O	0111564+284742	4304	KUG 0109+285	18.21	23.78
S184P	0112094+214022	1654829		18.62	24.44
S185O	0112150-334648	173575	GSN 150	18.06	23.69
S186P	0113004-071010	1023413		18.23	23.82
S187P	0113408-054100	1041659		18.21	23.53
S188P	0114502-310128	710125		18.32	24.49
S189O	0115021-330115	4506	ESO 352-G29	18.21	23.56
S190O	0115097+334726	4516	KUG 0112+335	18.42	23.83	O
S191O	0116238+421144		NPM1G +41.0027	18.03
S192P	0117080-183227	866867		18.51	25.41
S193P	0117554-153002	910412		18.09	24.25
S194P	0118008+465350	2289010		18.50	24.53
(S195P)	(0118172-171816)	885445		18.46	25.1
S196P	0118316+143224	1460788		18.16	24.66
S197O	0118579+445839	4702	MCG +07-03-027	18.36	23.56
S198O	0119329+145218	4753	NGC 46	18.05	22.71
S199P	0119348+341238	2045594		18.45	24.75
S200O	0119375+182634	4766	CGCG 459-029	18.39	22.83	O
S201P	0119547+355606	2072274		18.31	24.96
S202O	0119564+435444	2232147	NPM1G +43.0035	18.05	23.82
S203O	0120146+174948	4807	CGCG 459-032	18.77	23.28	O
S204P	0120175+394043	2153933		18.46	24.58
S205O	0120320-364055	199441	DUKST 352-051	18.31	24.11
S206O	0120393-350437	653641	GSN 179	18.58	25.11
S207O	0120539-011949	4859	MCG +00-04-091	18.23
S208P	0121214-115801	959478		18.02	24.91
S209P	0121285-270533	133805		18.37	23.41
S210P	0121286+263201	1779780		18.02	23.83
S211P	0121386-261219	770327		18.85	23.21
S212O	0121476+390940	2144534	NPM1G +38.0030	19.14	24.19
S213O	0122015+372403	4971	UGC 909	18.21	24.14	O
S214P	0122032+500220	212729		18.11	24.29
S215P	0122195-081722	1005642		18.92	24.75
S216P	0122218-374454	618295		18.21	24.21
S217P	0122400+470648	2292575		19.04	24.08
S218O	0123163-104634	973895	NPM1G -11.0055	18.36	23.43
S219O	0123593-350738	5142	NGC 527B	18.23	24.60
S220P	0124426-192431	855652		18.39	24.55
S221P	0124587-031040	1075106		18.52	23.43
S222P	0125094-280928	745123		18.23	23.99
S223P	0125524-320335	697417		18.72	24.02
S224P	0125561+500858	2364336		18.68	24.89
S225P	0126077+503713	5327		18.48	24.11	O
S226P	0126162-205556	834955		18.25	24.6
S227O	0126491-170240	5378	MCG -03-04-066	18.18	23.19
S228P	0126499-172435	883743		19.04	24.47
S229P	0126581-373322	621317		18.10	23.25
S230P	0127040-071142	1022962		18.11	23.79
S231P	0127383+331015	2025379		18.30	24.86	a
S232N	0127498+335256			18.82		a
S233P	0127533-135700	931026		18.44	24.75
S234P	0128008+481106	2312147		19.27	24.18
S235O	0128131-354007	5483	ESO 353-G4	18.48	23.12
S236P	0128318-383626	109094		18.36	24.5
S237O	0128341-015333	166794	AGC 410583	19.15	23.38
S238O	0128557-014909	5534	UGC 1060	18.86	23.38
S239P	0128569-041339	144152		18.57	23.52
S240O	0129142-091307	5547	MCG -02-04-059	18.01	23.56

 

 

Table 2d: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
S241O	0130201-121433	5606	MCG -02-04-061	18.01	23.78
S242O	0131238-123727	5659	IC 128	18.58	23.33
S243O	0131243+313045	5668	KUG 0128+312	18.11	22.95	A
S244P	0131265+332122	2030200		18.12	23.92
S245P	0131364-215638	87856		18.34	24.19
S246O	0131483+303030	5694	KUG 0128+302	18.14	23.02
S247P	0131569-162125	899185		18.95	24.88
S248P	0132092-035837	1064545		18.66	23.71
S249N	0132395+353324			18.63
S250P	0132452-305910	710612		18.58	24.25
S251N	0132502-353622			18.68
S252N	0132574-325910			18.18
S253P	0133003+322559	1996634		18.11	24.54
S254P	0133341-094933	985942		18.95	23.08
S255P	0134529+265648	1793228		18.13	23.87	a
S256P	0136280-004152	1136936		18.94	24.17
S257O	0137135-133851	6000	MCG -02-05-021	18.27	23.42
S258O	0137512-175932	6037	ESO 543-G3	18.69	23.15
S259P	0138128-233929	133770		18.02	23.57
S260O	0138215-225824	133767	MBG 01360-2313	18.47	23.17
S261P	0138238-232716	133768		18.30	23.09
S262P	0138270-091133	994075		18.06	23.89
S263P	0138282-074201	1014474		18.18	24.04
S264P	0138302-141035	928026		18.32	23.82
S265P	0138385+184014	1566633		18.08	25.06	a
S266O	0140056-185440	6168	ESO 543-G10	18.11	23.73
S267P	0140173-274937	173941		18.30
S268P	0141012-082326	144233		18.22	23.62
S269O	0141021-092023	90557	FGC 186	19.28	23.57
S270P	0142093+345804	2057359		18.08	23.65
S271P	0142099-280642	745704		18.83	24.29
S272P	0143018-064631	1028865		18.60	24.18
S273N	0143117-103055			18.48
S274O	0143168+352804	6333	KUG 0140+352	18.81	23.88
S275P	0143537+312628	1947338		18.13	24.49
S276P	0144051-052832	1044255		18.22	24.64
S277P	0144058+251544	1730587		18.50	25.1	a
S278P	0144593+384845	2137189		18.45	23.73
S279P	0145141-225405	807346		18.60	24.38
S280P	0145223-221938	133812		18.66	23.27
S281P	0145233+173903	1538003		18.60	24.87	a
S282P	0145556+334650	2038677		18.32	24.29
S283P	0146209+301531	1896659		18.51	25.01
S284P	0146393+320629	1980643		18.53	25.26
S285P	0146569+323024	2000119		18.87	24.78	a
S286O	0147180-300903	132938	CSRG 0164	18.09	23.39
S287O	0147181-323418	131952	DUKST 353-016	18.38	23.13
S288P	0147250-334108	672906		18.28	25.18
S289P	0148296-152153	912193		18.05	24.5
S290P	0148304-150059	916840		18.21	24.87
S291P	0148396-181122	871479		18.15	24.47
S292O	0149234-082629	6680	MCG -02-05-054	18.22	23.39
S293O	0149450-214905	6713	MCG -04-05-009	18.62	23.32
S294P	0149500-284536	198965		18.06
S295O	0150072+340805	6745	KUG 0147+338	18.47	23.64
S296P	0150566-343320	95467		18.90	24.29
S297P	0151172+232530	1687132		18.75	24.56	a
S298P	0151249+223539	212849		18.50	24.19	A
S299P	0151528+123606	1412562		18.47	23.85	a
S300P	0153227+340703	2044135		18.65	24.2
S301O	0154576+372034	7124	UGC 1380	18.88	24.12	O, A
S302P	0154583+364544	2086489		18.39	24.25
S303P	0155035-330952	680035		18.22	24.59
S304P	0155058+350930	2060317		18.36	24.18	a
S305N	0155246+293208			18.39		a
S306P	0155299-081241	1006667		18.57	24.48
S307P	0155334-190810	859333		18.73	23.69
S308P	0155337-072126	1020355		18.46	24.5
S309O	0155488-103421	7205	KUG 0153-108	18.96	22.95
S310O	0156238+371256	7263	UGC 1404	18.70	24.69	O
S311P	0156522-075004	1012284		18.03	24.07
S312P	0157544-355751	642430		18.91	23.85
S313P	0157570-061048	1035869		18.37	24.16
S314P	0158011+405256	2172376		18.19	24.41
S315P	0158045-074331	1014020		18.05	23.78
S316P	0158191-105016	973138		18.56	24.45
S317P	0159422-024619	174599		18.11	23.14
S318P	0159429-105249	174602		18.18	23.12
S319P	0200008-192636	855168		18.26	24.55
S320O	0200470+174249	7637	UGC 1495	18.42	24.03	O

 

 

Table 2e: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
S321P	0202002+202546	1627043		18.47	24.33	a
S322O	0202320+445748	7767	UGC 1516	18.38	23.63
S323O	0202354-242752	7777	MCG -04-06-002	18.28	22.73
S324P	0203036-031111	1074951		18.35	23.59
S325P	0203387+460113	2274085		18.38	23.56
S326P	0203408-255155	133880		18.03	23.40
S327P	0203465-083326	1002196		18.17	24.38
(S328P)	(0203497-041049)	1061767		18.64	23.91
S329N	0204041+481832			18.78
S330P	0204355-135004	932618		18.28	23.97
S331P	0204422-115651	959754		18.58	25.22
S332P	0205242-105155	972785		18.04	23.36
S333P	0205529-093727	988597		18.36	23.64
S334P	0206477+153308	1487658		18.92	24.48	a
S335P	0206547+214910	1657954		18.61	23.59
S336O	0208012-102119	8142	KUG 0205-105	18.84	23.24
S337P	0208015-191703	857341		18.26	24.5
(S338P)	(0208099-245329)	198344		18.09
S339N	0209081+355129			18.57		a
S340P	0209178-121902	954598		18.24	23.86
S341O	0209596-085009	8274	KUG 0207-090	18.36	22.61
S342P	0210142-215918	820848		18.42	24.86
S343P	0211014+453808	2268147		18.45	24.24
S344P	0211135-063219	1031695		18.03	23.25
S345P	0211272-050201	1050210		18.48	23.85
S346N	0212509-043551			18.73
S347P	0212560-054620	1040585		19.02	24.71
S348P	0213180+410927	2176597		18.44	25.23
S349P	0213298-223231	133850		18.44	23.06
S350O	0213339+382521	8514	VI Zw 188	18.16	24.40
S351P	0213466-210751	174913		18.36	23.05
S352P	0213575-152903	910639		18.24	24.36
S353N	0214024+120347			19.00		a
S354P	0214504+440601	2236595		18.15	23.97
S355P	0215021-161910	174985		18.94	23.01
S356O	0215370-134310	8640	MCG -02-06-044	18.27	23.01
S357P	0215476-134754	933091		18.38	23.39
S358O	0217067-270931	91970	FGCE 0229	18.51	23.83
S359O	0217377+123032	8752	IC 1790	18.19	23.27	O
S360O	0217549-344811	8772	ESO 355-G4	18.16	23.04
S361O	0218025-274906	8781	ESO 415-G17	18.32	23.21
S362N	0218178+494822			18.02
S363N	0218220+243343			18.23		a
S364O	0218378-065345	8816	MCG -01-06-087	18.34
S365O	0218500-263236	91974	FGCE 0234	18.11	23.33
S366O	0219186-114757	8858	MCG -02-07-001	18.48	23.37
S367P	0219203+371329	2095670		18.99	23.52	a
S368P	0219264-105337	972456		18.22	24.17
S369P	0219270-112546	8861	KUG 0217-116	18.12	22.95
S370N	0219284+164731			18.86		a
S371P	0219285+344638	2054374		18.70	24	a
S372P	0221101-121757	954850		18.86	24.78
S373P	0221246+291221	1858979		18.73	23.39	a
S374O	0221511+172741		NPM1G +17.0095	18.51		a
S375P	0221555+370429	2092488		18.72	24.87	a
S376N	0223056+455845			18.27
S377P	0223454-190306	134921		19.06	23.60
(S378P)	(0224043-243951)	133857		18.18	23.40
S379P	0224095+431549	212968		19.15	25.06
S380N	0224134+374826			18.05
S381O	0224417-114632	9146	KUG 0222-120	18.15	23.09
S382O	0225042-194831	9175	ESO 545-G14	18.02	22.77
S383P	0225056-062805	1032505		18.77	23.44
S384P	0225148+270156	1795794		18.01	25.32	A
S385P	0225272+451538	2261877		18.23	24.28
S386P	0225381-134526	933698		19.16	23.68
S387O	0225395+271743	9220	CGCG 483-038	18.01	23.36	O
S388O	0225429+284034	9223	KUG 0222+284	18.18	24.01	a
S389P	0226467+244228	1714313		19.09	25.08	A
S390P	0226511-122252	953656		18.12	25.32
S391N	0227189+210523			18.30		a
S392P	0227455+152616	1484626		18.53	25.11	a
S393P	0228308-291920	730732		18.20	24.67
S394P	0229037-335219	670382		18.50	23.49
S395P	0229148-053609	1042634		18.25	24.66
S396N	0229235+280905			18.39		A
S397P	0230362-232214	133892		18.04	22.99
S398P	0230486-235042	796415		18.07	23.81
S399P	0230536-142532	924760		18.26	24.36
S400O	0231185+425236	9592	UGC 1989	18.57	24.92	O

 

 

Table 2f: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
S401P	0232496+230820	1682146		18.44	23.95	a
S402O	0232538+231938	9707	UGC 2020	18.53	23.56	O
S403P	0233273+425109	2207509		18.42	24.16
S404P	0234072-261601	133938		18.04	23.78
(S405P)	(0234244-084454)	999709		18.42	24.79
S406P	0234296+412032	2179618		18.48	24.48
S407P	0234361-002452	175238		18.39	23.44
S408P	0234434+373626	2104891		18.85	23.35	a
S409P	0236015-283201	175287		18.69	24.90
S410P	0236299-211602	830478		18.42	24.34
S411P	0237009+404103	2169424		18.43	24.45
S412P	0237043-140149	929902		18.57	24.22
S413P	0237323-340707	88008		18.29	24.17
S414O	0238141-271537	9990	MCG -05-07-010	18.60	23.19
S415P	0239475+410720	2176034		18.24	23.96
S416P	0239567-154319	175371		18.38	23.66
S417P	0239580+411911	2179231		19.23	24.6
S418P	0240025+174100	1538874		18.14	24.07	a
S419O	0240251+383347	10124	UGC 2157	19.00	23.89	O
S420N	0240466+201104			18.15		a
S421N	0241014-280601			18.79
S422P	0241214-142806	924251		18.21	23.4
S423P	0241548-275451	748156		18.39	24.73
S424P	0241575-030119	144981		18.02	24.72
S425O	0242013-150324	144985	NPM1G -15.0140	18.14	23.03
S426O	0242306-213504	10253	MCG -04-07-025	18.88	23.05
S427P	0243239+330042	2020570		18.43	24.57	a
S428P	0243255-080808	1007817		18.52	23.88
S429P	0243270-114829	961464		18.88	24.33
S430P	0243369-354514	145000		18.30	23.728
S431N	0243504-280514			18.73
S432O	0244200-344134	199586	DUKST 356-045	18.68	24.16
S433P	0244306-101204	981129		18.61	25.01
S434P	0245036-260624	771484		18.32	23.27
S435P	0246201-245830	784047		18.13	24.92
S436P	0246272-003930	1137865		18.07	24.17
S437P	0246541-003355	1140234		18.06	23.55
S438P	0247051-002652	1143065		18.07	24
S439O	0247222-144727	10564	MCG -03-08-026	18.72
S440P	0247269-314857	74204		18.69	23.58
S441P	0247354-310626	74210		18.10	23.21
S442P	0247409+353952	2068054		18.15	24.97	a
S443P	0247577-004503	145053		18.64	23.20
S444O	0247598-220004	10590	MCG -04-07-045	18.14	23.53
S445N	0248004-013753			18.83
S446P	0248590+151241	1478344		19.07	24.3	a
S447P	0249372+355358	2071747		18.75	25.15	A
S448P	0251239+415733	197724		18.22
S449P	0251314+125629	1419356		18.48	24.11	a
S450P	0251415-095748	984146		18.28	23.13
S451P	0252469-351149	652051		18.51	25.29
S452O	0253357+255645	10920	MCG +04-07-029	18.71	23.67	A
S453P	0253434-174942	876818		18.35	24.49
S454P	0253470-260310	91994		18.29	23.58
S455P	0253544+414026	197761		18.16	23.78
S456P	0254471+220418	1662967		18.72	24.99	a
S457O	0255592-120028	11078	IC 271	18.83	23.49
S458P	0256537-155511	904744		18.84	24.03
S459P	0256563+404816	197822		18.35	23.87
S460P	0257121+390900	2144325		18.66	24.27
S461P	0257418+425833	2210242		19.26	24.87
S462P	0257476-090807	994764		18.42	23.89
S463P	0257557-090103	996293		19.03	25.05
S464P	0257582-064153	1029847		18.41	23.91
S465O	0257591+252526	11212	CGCG 484-026	18.76	22.85	O
S466P	0258115+460457	2275064		18.22	25.2
S467P	0258283+250313	1724074		18.55	24.67	a
S468P	0259136+442215	2242768		18.06	24.4
S469P	0259324+445026	2253204		18.67	24.11
S470P	0259404+233100	1688741		18.13	24.88	a
S471P	0300104-011935	1121356		18.99	24.4
S472O	0300249-105338	145178	NPM1G -11.0111	18.32	23.06
S473O	0301389-265253	92001	FGCE 286	18.73	23.87
S474P	0302524+162718	1509176		18.06	24.86	A
S475P	0303350+354438	138596		18.13	24.6	a
S476P	0303350+355730	2072652		18.58	24.87	a
S477P	0304098-145825	917468		18.02	24.29
S478O	0304556-273028	11589	MCG -05-08-014	18.79	22.53
S479P	0305120-274127	133009		18.34	23.42
S480P	0305159-255519	773606		18.75	24.33

 

 

Table 2g: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
S481P	0305300-023502	11618		19.06	24.02	O
S482O	0305365+413408	213161	UGC 2528	18.57	25.25
S483P	0305414-014413	1111454		19.08	24.07
S484P	0306128-042000	1059697		18.14	24.47
S485P	0308121-225329	807492		18.18	24.4
S486P	0308123-244129	198434		18.75	24.49
S487O	0308157-244020	11738	ESO 480-G35	18.21	22.80
S488O	0308226-284820	199040	DUKST 417-031	18.10	24.99
S489P	0308455+424214	2204372		19.48	24.89
S490P	0308466+242048	1705247		18.06	23.89	A
S491P	0308586-115528	960038		18.18	24.44
S492P	0309045+440226	2235142		18.10	24.11
S493P	0309074+233902	1691142		18.79	24.41	a
S494N	0309078-083044			18.04
S495P	0309078-235510	133947		18.58	23.43
S496P	0309202-234459	797474		18.15	24.88
S497O	0309331-020046	11811	CGCG 390-011	19.10
S498P	0309406-262815	767439		18.07	24.53
S499P	0309426+412626	2181130		18.09	25.47
S500P	0309433-252254	779599		18.11	24.49
S501P	0310268-000045	1154156		19.00	25.34
S502P	0310312+191406	1585156		18.79	24.01	A
S503N	0310370+210938			18.40		A
S504P	0310591+423849	2203202		18.55	25.29
S505P	0310591-312446	705459		18.39	23.57
S506P	0311032-240350	794002		18.05	23.88
S507P	0311112+202114	1624788		18.61	24.71	a
S508P	0311147+210223	1641398		18.03	24.15	a
S509P	0311186-250631	11891	ESO 481-G5	18.49	23.25
S510P	0311300-191053	858770		18.42	23.98
S511P	0311462+244837	1717065		18.49	24.81	a
S512P	0311541-272331	755637		18.15	23.64
S513P	0311544-223836	810971		18.53	23.75
S514P	0311563-021648	1096537		18.46	25.08
S515P	0311568+201712	1622716		18.24	24.88	a
S516P	0312211-234649	797115		18.52	23.54
S517O	0312247-243246	11940	ESO 481-G11	18.11	23.56
S518P	0313176-134708	933261		18.73	24.5
S519O	0313190-122244	90664	FGC 398	18.41	23.99
S520N	0313382+293751			18.62		a
S521O	0314030-072349	175975	NPM1G -07.0121	18.69	24.56
S522O	0314079-061722	12037	KUG 0311-064	18.56	22.73
S523P	0314378-053033	1043831		18.86	24.37
S524N	0314466-290823			18.19
S525O	0314497-064215	170045	GSC 4714 01132	18.03
S526P	0314566-190102	860855		18.46	24.09
S527P	0315538-022549	1092239		19.20	24.75
S528P	0316152+364746	2087153		18.32	23.88	a
S529P	0316488+270654	1798183		18.77	24.99	A
S530P	0318208-224823	198450		18.30	24.49
S531P	0318494+404939	2171539		18.01	24.42
S532P	0318579+413805	12360		18.01	24.09
S533P	0319104+400132	2159426		18.30	24.14
S534P	0319161-101300	980956		18.27	23.51
S535P	0319182+395430	2157614		18.16	24.44
S536P	0320099-074304	1014161		19.34	24.61
S537P	0320099+425745	2209936		18.35	24.45
S538P	0320409+342131	2047947		18.48	24.71	a
S539O	0321124-252612	12573	ESO 481-IG 024	18.72	23.91
S540P	0321140+392755	2150261		18.38	23.8
S541P	0321214+410128	2174500		18.56	23.9
S542N	0321240+404615			18.66
S543N	0321357-163343			18.39
S544P	0321500-144955	919365		18.56	23.87
S545P	0322015-075258	1011541		18.07	25.15
S546N	0322247+294309			18.81		A
S547O	0322272-214144	824949	NPM1G -21.0116	18.06	23.48
S548P	0323095-202908	841076		18.51	23.79
S549O	0323372-354642	12691	ESO 357-G25	18.50	24.40
S550N	0323598+121455			19.05		A
S551O	0324039+150608	90673	FGC 418	18.52	23.70
S552O	0324073+174513	12719	UGC 2716	19.44	24.40	O
S553N	0325228+382538			18.31
S554O	0325255+404623	12796	UGC 2724	18.46	24.23
S555P	0325481+352504	2064213		18.03	23.92	a
S556O	0326029+411451	12830	UGC 2733	19.26	23.81
S557O	0326130-344838	132173	FCCB 0359	18.06	23.20
S558P	0326160-260832	771068		18.14	23.79
S559P	0326240-263027	176172		18.15	23.78
S560P	0326302+403207	213214		18.73	25.31

 

 

Table 2h: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
S561P	0326355-012207	176180		18.33	23.70
S562P	0326367-284021	738890		18.01	24.41
S563P	0327077-194926	135058		18.66	23.05
S564P	0327257-021304	1098383		18.34	24.39
S565P	0327261-033736	176219		18.33	24.12
S566P	0328112+355443	2071937		18.80	24.8	a
S567P	0328251-291842	730840		18.22	23.3
S568N	0328366+390550			18.65
S569O	0329088+412308	12967	CGCG 541-014	18.31	23.48
S570O	0330021-152058	912390	NPM1G -15.0189	18.55	23.55
S571O	0330496-343846	659447	FCCB 0676	18.40	24.21
S572N	0331139-284709			18.72
S573P	0331310-101701	980135		18.57	24.67
S574O	0331383-250030	13094	ESO 482-G2	18.03	23.28
S575O	0331455-334906	671105	FCCB 0739	18.33	23.62
S576N	0332265+415857			18.02
S577P	0333098+404615	2170678		18.33	24.3
S578N	0333114+372306			18.26		a
S579N	0333218+363754			18.08		a
S580N	0333315+383346			18.27
S581O	0333492-101502	13200	MCG -02-10-002	18.52	23.05
S582P	0334037-193203	135049		19.25	23.67
S583N	0334078-234336			18.65
S584P	0334189+133015	1432686		18.62	24.62	a
S585P	0334273-231137	176350		19.01	23.17
S586O	0334309-183944	13231	ESO 548-G45	18.09	23.92
S587P	0334448-024651	1083042		18.63	24.55
S588P	0334506-161502	900553		18.07	23.98
S589P	0335004-003931	1137854		18.64	24.07
S590O	0335467-300321	133048	APMBGC 418-077+005	18.47	23.30
S591O	0336353-215514	135065	APMBGC 548-055+107	18.54	23.29
S592P	0337054+262739	1777125		18.12	25.01	a
S593P	0337181-055515	1038883		18.63	25.08
S594O	0337452-301258	133046	APMBGC 418-100+014	18.30	23.47
S595N	0338017+352013			18.36		a
S596P	0338251-283145	740583		18.64	24.23
S597P	0338269+124840	1416658		18.14	24.32	A
S598O	0338276-241213	134070	APMBGC 482+045-039	18.35	24.13
S599O	0338330-052802	13421	MCG -01-10-014	18.44	24.03
S600O	0338562+301522	13438	UGC 2807	18.84	24.61	O
S601O	0339214-212456	13460	MCG -04-09-043	18.79	23.17
S602P	0339259-020133	1103619		18.22	23.59
S603O	0339313-330639		FCCB 1339	18.80
S604O	0339347+204231	1634156	NPM1G +20.0119	18.45	24.4	A
S605P	0339484+413210	2182626		18.80	24.58
S606N	0339586+370010			18.47		a
S607N	0340131+410247			18.58
S608O	0340343-011836	135683	KUG 0338-014	18.64	23.00
S609P	0341024+421955	2196795		18.84	24.53
S610P	0341049-152606	911276		18.49	23.73
S611P	0342200+300939	1892676		18.08	24.28	A
S612O	0342295-205413	135043	APMBGC 548-130+053	18.35	22.99
S613O	0342575-190111	13648	ESO 549-G2	19.15	23.78	O
S614P	0343306-195229	849334		18.27	23.63
S615P	0345017+402601	2165718		18.22	24.29
S616P	0345413-134418	933941		18.81	24.11
S617N	0346139+223529			18.21		a
S618O	0346241-280736	133073	APMBGC 419+067-098	18.73	23.29
S619P	0346273-035531	1065164		18.02	25.04
S620O	0346353-274041	133072	APMBGC 419+065-122	18.43	23.23
S621P	0348104-140456	929223		18.57	24.95
S622P	0348449+122942	1410586		18.56	24.56	A
S623P	0349149+160505	90695		18.38		O
S624P	0349467-095611	984515		18.09	24.62
S625P	0349496+143540	1462056		18.57	24.78	a
S626O	0350041-174513	13936	ESO 549-G27	18.56	23.72
S627N	0350107+345319			18.90		a
S628P	0352040-061801	1034463		18.91	24.66
S629P	0352275-062050	1033917		18.60	24.1
S630P	0352541+192745	1593172		18.05	24.27
S631N	0353196-315250			18.15
S632O	0353382-335214	14046	ESO 359-G4	18.92	23.45
S633P	0353405-164557	893853		18.44	23.89
S634O	0354051-235311	142604	APMBGC 483+123-055	18.15	23.82
S635O	0354154+363032	14068	UGC 2893	18.87	25.10	O
S636P	0354275-160333	902999		18.60	24.65
S637P	0354437-091613	993120		18.89	24.69
S638P	0355096+282040	1833185		18.08	24.32	A
S639N	0355523+395417			18.89
S640P	0356435-172434	883745		18.41	23.69

 

 

Table 2i: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
S641P	0357026-164640	893654		18.23	23.9
S642P	0357115-272958	754047		18.15	24.46
S643P	0357260-172604	883314		18.51	23.55
S644P	0357438-191414	857979		18.59	24.58
S645P	0358036+124505	1415508		18.66	24.44	a
S646N	0358047+384654			18.10
S647N	0358052+123215			18.74		a
S648P	0358066+143907	1463532		18.12	24.65	a
S649O	0358108-223400	14180	ESO 483-G3	19.27	23.18
S650N	0358386-020202			18.15
S651P	0358443+281647	1831323		18.48	24.31	a
S652O	0359552+323649	14246	UGC 2915	18.10		O
S653P	0400345-195830	847928		18.58	24.03
S654O	0401207+264925	14301	UGC 2924	18.35	23.87	O
S655P	0401554+230551	1681378		18.40	24.19	a
S656P	0402225+160138	1498974		18.58	24.44	a
S657P	0402296+163915	1513823		18.03	25.27	a
S658P	0402598+134515	1439552		18.15	25.63	a
S659P	0403121-282442	741998		18.71	24.36
S660O	0403122-252754	134102	LSBG F483-013	18.76	23.57
S661N	0403481-024459			18.38
S662P	0404018+195936	1612699		18.71	23.85	A
S663P	0404260-105316	972528		18.13	24.57
S664O	0404326-101802	14417	MCG -02-11-015	18.92	23.66
S665P	0405286-155046	146055		18.89	23.15
S666O	0405361-151137	146056	NPM1G -15.0204	18.12	23.32
S667O	0405559-150858	14456	MCG -03-11-010	18.23	22.84
S668N	0406181-032325			18.09
S669P	0406267+204843	1636442		18.29	24.52
S670N	0406535-013656			18.22
S671P	0407357-265733	761688		18.61	24.72
S672P	0407376-311718	176929		18.45	23.54
S673P	0407531-220920	818435		18.83	24.47
S674P	0408365-210352	135142	NPM1G -21.0135	18.05	24.05
S675N	0408494-035237			18.18
S676N	0409533+243427			18.78		a
S677N	0410098+251006			18.18
S678N	0412312+371943			18.66		a
S679N	0412357+254402			19.06		A
S680N	0412434-021255			18.67
S681O	0413129-122012	954325	NPM1G -12.0139	18.60	23.36
S682P	0413159+232625	1687428		18.13	24.52	a
S683N	0413211+361816			18.92		A
S684P	0413455-161736	899985		18.28	24.14
S685N	0413468+291419			19.03		a
S686O	0414013+264500	90703	FGC 470	18.99	23.41	A
S687P	0414170-290832	732831		18.13	23.5
S688P	0414481-350814	652836		18.54	24.45
S689P	0415596-072730	1018639		18.82	25.21
S690N	0417090+200810			18.13
S691P	0417277-065540	1026831		18.31	25.58
S692P	0417283-033230	1069873		18.77	24.76
S693P	0417297-134045	934702		18.50	23.45
S694N	0417350-010744			18.22
S695N	0418166+244733			18.43		a
S696N	0418169-155049			18.52
S697P	0418219-144833	919662		18.11	23.79
S698P	0419038-083040	1002779		18.06	25.06
S699P	0419256-043728	1055625		18.51	23.85
S700O	0419269-010124	14872	MCG +00-11-054	18.12	23.42
S701P	0419438-014917	1109135		18.05	24.83
S702N	0419465-003916			19.08
S703O	0420037-140528	929115	NPM1G -14.0202	18.03	23.55
S704P	0420342-120004	958996		18.56	23.32
S705P	0421151-152431	911598		18.34	25.1
S706P	0421290-024406	1084171		18.32	23.32
S707P	0421373+323323	2002312		18.36	24.57
S708N	0422078+351728			18.68		A
S709N	0422350-015812			18.41
S710P	0422371-032249	1072075		18.38	23.81
S711P	0423039-283821	739268		18.26	24.41
S712N	0423115+270553			18.06		a
S713N	0423419+270952			18.63		a
S714P	0423486-183055	867176		18.20	24.37
S715P	0423579-183235	866841		18.48	24.75
S716O	0424115-121618	15030	MCG -02-12-012	18.50	23.22
S717P	0424117-275613	146251		18.59	23.03
S718N	0424412+161626			18.07
S719N	0424437+170356			18.48		a
S720N	0424443+250341			18.08		a

 

 

Table 2j: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
(S721N)	(0424456+215937)			18.50		a
S722P	0425313-251205	781582		18.07	24.25
S723P	0425439-072349	146281		18.01	23.27
S724P	0425443-110928	969266		18.68	24.91
S725P	0425540-100324	982946		18.46	24.06
S726N	0426056-092627			18.58
S727P	0426153-123952	138728		18.46	24.06
S728P	0426586-184513	864155		19.02	24.13
S729P	0427047-053801	1042265		18.28	25.45
S730P	0427059-220911	818489		18.59	24.56
S731O	0427154-375444	92074	FGCE 400	18.18	23.60
S732P	0427394+125244	1418001		18.31	25.3	a
S733P	0428281-265147	762967		18.49	24.46
S734P	0428484-012407	1119498		18.11	24.93
S735O	0430120-125053	177353	AGC 440514	18.62	23.25
S736P	0430343-295954	146341		18.38	23.32
S737O	0430596-020012	15356	UGC 3070	18.44	23.66	O
S738O	0431375-321445	15400	ESO 421-G7	18.09	23.50
S739N	0432265-134523			18.70
(S740N)	(0432268-123902)			18.62
S741N	0432467+163006			18.64		a
S742O	0433016-104846	15500	VV 468	18.04	23.39
S743O	0433199-233923	798548	LSBG F484-005	18.29	24.44
S744P	0435122-350658	653129		18.74	24.44
S745P	0436174-334824	671292		18.07	23.99
S746P	0436347-310641	709050		18.21	24.78
S747N	0436386-140453			18.30
S748N	0437210+205834			18.42		a
S749P	0438154-125015	177603		18.31	23.91
S750P	0438350+294115	1874555		18.07	25.33
S751O	0439016-183906	135148	IRAS 04368-1844	18.04	23.24
S752N	0439319+193411			18.28		a
S753P	0439522-143529	922649		18.13	23.84
S754N	0440041-360609			18.07
S755N	0440089+251236			18.65		a
S756P	0440232-355559	642817		18.45	24.14
S757P	0440409-091548	993201		18.30	23.83
S758P	0440414-083931	1000846		18.46	24.43
S759P	0441100-091225	993896		18.19	24.18
S760P	0441329-370052	629621		18.16	24.57
S761P	0441402-373933	619665		18.34	23.19
S762P	0441444-014652	213291		19.07	24.47
S763P	0442008-383700	607039		18.05	24.36
S764O	0442189-261923	134212	APMBGC 485+069+072	18.24	23.21
S765P	0442524-220153	146494		18.57	22.89
S766N	0443104+290143			18.77		A
S767P	0443141-255044	134199		18.14	23.05
S768P	0443198-153028	910290		18.54	23.93
S769P	0443408-135421	177748		18.12	23.70
S770P	0444190-154518	906921		18.31	24.07
S771P	0444270-001315	1148837		18.69	24.21
S772P	0444432-160117	903469		18.38	23.9
S773N	0444445-150223			18.90
S774P	0444465-162929	897469		18.16	23.65
S775P	0444529-044639	1053623		18.04	24.94
S776N	0446027+284054			18.74		a
S777O	0446327-115545	15979	MCG -02-13-003	19.29	23.23
(S778P)	(0446362-255215)	774143		18.55	24.6
S779N	0447562+235010			18.48
S780P	0448356-235001	134178		19.08	23.10
S781N	0448386+265821			18.22		a
S782O	0448583-320732	16073	ESO 421-G18	18.22	23.27
S783P	0449007-331912	677941		18.82	24.12
S784P	0449046-371328	626586		18.74	24.76
S785N	0449068+171009			18.46		A
S786P	0449077-211955	146539		18.13	23.83
S787P	0449235-093444	146559		18.51	23.71
S788P	0450015-220442	819580		18.46	23.38
S789N	0451145-194946			18.21
S790O	0451172-300120	16161	ESO 422-G3	18.74	23.76
S791N	0451218+271254			18.17		A
S792P	0451312+173814	1537658		18.07	25.11	A
S793O	0452478-141135	927809	NPM1G -14.0221	18.35	23.21
S794P	0452566-064429	1029339		18.79	24.96
S795P	0453089-091508	993352		18.05	23.68
S796O	0453095-174222	16249	ESO 552-G18	18.81	23.7
S797N	0453276-024122			18.32
S798P	0453346-071910			18.26
S799N	0453465-154634			18.64
S800O	0454535-371915	16317	ESO 361-G19	18.60	24.10

 

 

Table 2k: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
S801P	0455166-195955	847586		18.85	23.64
S802O	0455167-224338	16334	ESO 485-G24	18.45	23.27
S803N	0455251-212015			18.06
S804P	0456398-364736	632556		18.34	24.64
S805P	0458179-141253	927507		18.71	24.81
S806P	0458394-004856	1134023		18.93	24.54
S807P	0459077-110532	970083		18.91	23.79
S808N	0459090-211457			19.02
S809N	0459137-065553			18.40
S810P	0459156-113041	964862		18.20	23.47
S811P	0459309-183931	865357		18.93	23.89
S812P	0500008-384824	605007		18.53	23.99
S813P	0500043-062024	1033995		18.61	24
S814N	0500071-075804			18.49
S815N	0500120-081159			18.30
S816N	0500139-094101			18.24
S817P	0500217-340845	146819		18.37	22.89
S818N	0500437-092745			18.11
S819O	0500484-363441	16546	ESO 361-G24	19.07	23.79
S820O	0501048-354742	132279	APMBGC 361-123+045	18.01	23.06
S821N	0501105-115036			18.36
S822P	0501106-113644	963738		18.09	24.91
S823O	0501414-200247	16577	MCG -03-13-056	18.03	21.87
S824P	0502554-212108	829395		18.27	23.59
S825P	0502598-183119	867094		18.09	24.21
S826O	0503207-202649		GIN 238	18.53
S827N	0503285-202711			18.19
S828P	0503350-003652	1138967		18.23	23.72
S829P	0503370-205119	836093		19.44	24.07
S830P	0503448-232316	801451		18.38	23.25
S831P	0503454-205850	834286		18.28	23.5
S832P	0503513-232910	800364		18.55	24.61
S833N	0503531+190758			18.19		a
S834P	0504190-010510	1127133		18.16	23.65
S835P	0504279-010506	1127160		18.31	24.72
S836N	0504398-045907			18.31
S837O	0505480-194854	16727	ESO 552-IG 070	18.94	22.89
S838N	0505489-075919			18.04
S839P	0505520-211051	831622		18.45	23.27
S840P	0505548-181415	870772		18.47	25.05
S841P	0505560-270406	760239		18.78	24
S842O	0506022-274804	16736	ESO 422-G29	18.08	22.66
S843P	0506080-351111	652208		18.63	23.93
S844O	0507352-162901		NPM1G -16.0208	18.11
S845P	0507364-063456	1031174		18.08	24.01
S846O	0507406-015848	92883	FGC 80A	18.34	24.55
S847O	0507417-110507		NPM1G -11.0179	18.61
S848O	0507448-193726	16782	ESO 553-G6	19.16	23.63
S849P	0508198-255213	774145		18.61	24.13
S850P	0508426-165745	16809	MCG -03-14-004	18.30
S851P	0508448-370916	627601		18.57	23.74
S852P	0509564+162522			19.15
S853P	0510046-352033	650140		18.16	24.66
S854P	0510065-005853	1129847		18.08	23.79
S855P	0510307-080701	147079		18.24	23.16
S856P	0510337-202336	842381		18.80	23.13
S857N	0511570+134808			18.50
S858N	0512141-211008			18.88
S859P	0514388-302027	718370		18.08	24.2
S860P	0514543-261946	769023		19.01	24.8
S861N	0514566+191925			18.67
S862P	0515110-192246	856050		18.85	24.09
S863P	0515328-183852	865508		18.14	23.52
S864P	0516215-225937	92123	FGCE 475	18.58	24.19
S865P	0518154-101435	980621		18.22	24.52
S866N	0520289+161402			18.32		a
S867N	0520534+145547			18.01
S868P	0522199+174913	1542586		18.27	25.03	A
S869P	0523068-262930	767248		18.67	24.43
S870P	0523425-224502	809420		18.13	24.34
S871P	0523467-121134	956376		18.39	23.23
S872P	0524076-084040	147433		18.14	22.88
S873N	0524511-291424			18.87
S874P	0525099-351254	651796		18.27	23.72
S875P	0525330-313051	704285		18.26	23.52
S876P	0525363-312419	705558		18.93	23.12
S877N	0526006-322829			18.41
S878N	0526165-312435			18.78
S879P	0526192-282726	741444		18.28	23.9
S880P	0526237-252547	147516		18.26	23.13

 

 

Table 2l: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
S881P	0526376-265141	762993		19.00	23.14
S882P	0527141-150430	178449		18.12	23.33
S883N	0527377-315755			18.04
S884P	0528288-340630	667027		18.66	24.42
S885P	0528384-223125	812892		18.44	24.39
S886O	0528539-205613	17337	ESO 554-G1	18.33	23.31
S887P	0528577-252541	779102		18.75	24.78
S888P	0529075-195601	17340	ESO 554-G2	18.53	23.41
S889P	0529123-344613	657788		18.35	24.37
S890N	0529128-341344			18.02
S891N	0529149-240714			18.17
S892N	0530038-083153			18.23
S893N	0530500-120358			18.19
S894O	0532147-213253	17406	ESO 554-G8	18.05	22.79
S895N	0533249-010624			18.22
S896N	0534309-105353			18.41
S897O	0536049-325452	17499	MCG -05-14-008	18.20
S898N	0536113+513705			18.50
S899N	0536472-003914			18.47
S900O	0537139-203358	17522	ESO 554-G21	19.06	23.65
S901P	0538224-261220	770321		18.62	24.63
S902P	0539069-113001	965017		18.20	24.43
S903O	0539215-292221	17559	ESO 424-G5	18.62	23.25
S904P	0541171-150658	915505		18.78	23.8
S905O	0543523-262758	17669	ESO 488-G2	18.02	22.88
S906N	0544052-035519			18.13
S907P	0544134-190613	147841		18.70	23.08
S908N	0544144-111627			18.59
S909N	0544308-064649			18.08
S910N	0545001-110929			18.46
S911P	0545043-255026	17719		18.28	23.65
S912N	0545569-091903			18.53
S913P	0546185-255036	75412		18.21	24.25
S914N	0546584-025352			18.20
S915P	0547041-222910	813492		18.40	24.48
S916P	0547262-193158	147979		18.25
S917P	0549411-341556	664796		18.40	23.82
S918P	0549416-045955	1050665		18.20	25.07
S919P	0549576-251729	17955		18.08	23.99
S920P	0550314-134344	934063		18.65	24.64
S921P	0550416-321159	695473		18.24	24.2
S922P	0550430+475826	2307986		18.42	24.67
S923P	0551346-045813	1051035		18.25	24.82
S924P	0551385-243102	2800796		18.01
S925P	0551448-252941	778316		18.41	24.45
S926P	0554544-003828	148100		18.14	24.23
S927N	0555151-064144			18.67
S928N	0556388-001531			18.21
S929P	0556522-052308	178737		18.38	23.41
S930P	0601223-204425	837594		18.26	23.73
S931P	0603368+465108	2288239		18.09	23.39
S932P	0603500-130001	944517		18.36	24.17
S933P	0604013-270525	759949		18.74	23.62
S934P	0605102-215550	821692		19.39	24.31
S935P	0606436-031705	1073450		18.21	24.7
S936N	0607466-035426			18.64
S937P	0608015-191725	857281		18.57	25.03
S938N	0608195-122406			18.03
S939P	0608550+432510	2220328		18.30	24.37
S940P	0609335-204052	838374		18.05	23.98
S941O	0612083-233217	18601	ESO 489-IG15	18.03	22.73
S942P	0612316+434435	2228094		18.17	23.89
S943N	0614258+453940			18.46
S944P	0614408+504356	2380781		18.36	25.32
S945P	0615572-155805	904095		18.94	25.12
S946P	0616048-131026	148592		18.23	23.31
S947P	0616224-132716	937774		18.04	23.26
S948P	0616307+465823	2290233		18.09	24.32
S949P	0617168+492346	2341755		18.16	24.37
S950P	0618494-242207	790691		18.26	23.97
S951O	0619597+512537	18825	UGC 3443	18.81	24.24
S952P	0620216+532424	2440232		18.18	24.88
S953P	0622381-230802	804390		18.01	23.96
S954P	0624563-354330	179432		18.26	23.23
S955P	0625254-325441	683988		18.45	23.56
S956P	0625505-223417	812170		18.69	23.8
S957P	0630168+391833	2147453		18.24	24.6
S958P	0632422+445932	2256653		18.89	25.28
S959P	0634169-333417	674568		18.42	24.97
S960P	0634273-240239	794243		18.41	23.46

 

 

Table 2m: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
S961P	0634292-342401	662842		18.35	23.91
S962P	0634533-221855	816078		18.63	24.23
S963P	0635066+531344	2435179		18.07	24.16
S964P	0635071+510910	2389278		18.59	24.76
S965P	0636367+512920	2394958		19.23	24.56
S966P	0640168-365545	630799		18.15	24.71
S967O	0640200-170224	75942	CGMW 1-0300	18.96	24.81
S968P	0640428+300108	1887003		18.01	25.59	a
S969P	0641189+533505	2445168		18.41	24.79
S970N	0642211+530411			18.46
S971P	0643019-361312	179758		18.89	22.93
S972P	0645081-301758	718916		18.01	23.58
S973P	0646153+434328	2227656		18.12	23.83
S974P	0647170+324132	2008383		18.09	24.44
S975P	0650548+470838	2293097		18.16	23.32
S976O	0651209-293533	19733	ESO 427-G14	18.76	23.48
S977N	0652072+325615			18.54		a
S978P	0652083+240320	1698831		18.38	24.98
S979P	0652101+420646	2192609		18.52	23.91
S980P	0653510-265952	76219		18.32	23.59
S981P	0654159+250610	1725530		18.39	24.19
S982P	0654443-344135	658790		18.38	25.21
S983P	0655127+472718	2298519		19.00	24.65
S984P	0655480-365427	631074		18.48	23.17
S985P	0656009-353349	647359		18.57	24.64
S986P	0656158+392645	2149910		18.81	24
S987P	0656329-384800	605083		18.66	25.15
S988P	0656368+214708	1657240		19.14	24.4
S989P	0656387+195403	1609491		18.29	24.28	a
S990P	0657589+425933	2210576		18.03	24.66
S991N	0658094+222151			18.27		a
S992P	0658098+220545	1663418		18.32	24.21	a
S993P	0658166+441216	2239051		18.36	24.13
S994P	0700514+473556	2301026		18.57	23.71
S995P	0702304-283218	740471		18.63	23.65
S996P	0702577-381154	611796		18.34	23.59
S997P	0704128+184613	1569747		18.71	23.95	a
S998P	0704239+205518	143088		18.42	25.12	O
S999P	0704252+245205	1718701		18.37	25.23	a
S1000P	0704335+475336	2306394		18.26	23.62
S1001P	0704363+261643	1770102		18.39	24.25	a
S1002N	0705213+223658			18.69		a
S1003P	0705392+403102	2166972		19.06	24.72
S1004P	0705430-312613	86012		18.30	23.57
S1005P	0706340+204200	1633959		18.14	23.96	a
S1006O	0706520+441627	86344	KUG 0703+443	18.82	24.18
S1007P	0706538+455536	2272589		18.88	24.09
S1008P	0707055+413904	2184556		18.76	24.19
S1009P	0708345+350120	2058199		18.44	24.21	a
S1010P	0709506-353024	648054		18.09	23.86
S1011P	0709531-381919	610296		18.39	25.26
S1012P	0710189+522120	2412889		19.11	24.87
S1013P	0710286-344558	657847		18.18	23.89
S1014N	0710351+504742			18.57
S1015P	0711116+233146	1688965		18.23	23.63	A
S1016P	0711168+453839	2268299		18.57	23.55
S1017O	0711278+311121	20355	CGCG 146-036	18.12	23.34	A
S1018P	0711352+435336	2231700		18.57	25.79
S1019O	0712255+234310	200233	UGC 3737	18.60	24.65
S1020P	0713033+232356	1686712		18.27	24.16	a
S1021P	0713075+445541	2255222		18.22	23.71
S1022P	0713331+455913	2273524		18.93	24.64
S1023P	0713355+340149	2042757		18.85	24.49
S1024P	0715280+235241	1695360		18.05	23.73	a
S1025P	0715472+193058	1595261		18.66	24.31	A
S1026P	0716199+372950	2102178		18.40	25.09
S1027N	0717407+462431			18.59
S1028P	0718097+431625	2216897		18.37	24.61
S1029N	0718419+380206			18.69
S1030P	0719128+401333	2162618		18.51	24.88
S1031P	0719193+225836	1679277		18.07	24.76
S1032P	0720051+504312	2380517		18.03	23.71
S1033P	0720185+234903	1694275		18.14	24.26	a
S1034N	0720375+481255			18.19
S1035O	0721585+292950	20814	CGCG 147-013	18.08	23.61	a
S1036P	0722426+200807	1617572		18.05	24.34	a
S1037P	0726545-385059	604523		18.34	24.36
S1038P	0727573+302753	1904896		18.15	24.52
S1039O	0729439+334124	21136	UGC 3879	18.57	24.48	O
S1040P	0730350+181644	1555098		19.01	23.69	a

 

 

Table 2n: continued.

No.	2MASS	PGC	Other	$\mu _{K5}$	$\mu_{B_{25}}$	Obs.
S1041P	0731059+474555	2304003		18.79	24.85
S1042P	0731070+412539	2180950		18.10	24.39
S1043O	0732327+361206	21241	KUG 0729+363	18.21	23.32	A
S1044O	0733006+392506	139027	B3 0729+395 ID	18.11	24.24
S1045O	0734342+212549	1649818	NPM1G +21.0165	18.02	23.7	a
S1046O	0734512+333218	21324	UGC 3913	18.59	24.23
S1047P	0735148+230634	1681613		19.16	24.31	A, P
S1048P	0736480+270247	1796259		18.81	24.46
S1049P	0739164-001041	1149933		18.57	24.22
S1050O	0739291+181044	21504	CGCG 087-025	18.33	23.87	A
S1051O	0740051+435403	2231876	NPM1G +44.0081	18.03	23.4
S1052P	0740139+440517	2236313		18.79	23.77
S1053O	0741001+125828	1420032	NPM1G +13.0153	18.03	23.48	a
S1054P	0742289+310556	1931577		18.84	24.6
S1055P	0742599-011132	1124570		18.19	23.6
S1056P	0743221+000441	1156518		18.87	24.38
S1057O	0744364+380240	21686	CGCG 177-045	18.37	23.30
S1058P	0745277+341023	2045032		18.12	24.37	A
S1059O	0746143+464455	21746	KUG 0742+468	18.41	23.77
S1060P	0747007+264315	1786279		18.96	25.38
S1061P	0747033+181120	1552617		18.47	24.81	A
S1062O	0747163+265703	21796	IC 0476	18.41	23.23	A
S1063P	0747231+222040	1668196		18.25	23.53	a
S1064O	0747553+340212	78450	KUG 0744+341	19.35	23.41
S1065O	0748160+183255	21842	CGCG 087-040	18.42	23.44	a
S1066O	0748516+362320		FGC 663	18.32
S1067P	0750442+302046	1900121		18.10	24.24
S1068O	0751037+175745	21978	UGC 4058	18.93	24.77	O
S1069O	0752015+440100	22038	CGCG 206-034	18.12	23.39