A&A 393, 887-896 (2002)
DOI: 10.1051/0004-6361:20020916

On Be star candidates and possible blue pre-main sequence objects in the Small Magellanic Cloud

R. E. Mennickent¹ - G. Pietrzynski ^1,2 - W. Gieren¹ - O. Szewczyk²

1 - Universidad de Concepción, Departamento de Física, Casilla 160-C, Concepción, Chile
2 - Warsaw University Observatory, Al. Ujazdowskie 4,00-478, Warsaw, Poland

Received 24 April 2002 / Accepted 17 June 2002

Abstract
Recently the OGLE experiment has provided accurate light curves and colours for about 2 millions stars in the Small Magellanic Cloud. We have examined this database for its content of Be stars, applying some selection criteria, and we have found a sample of $\sim$1000 candidates. Some of these stars show beautiful light curves with amazing variations never observed in any Galactic variable. We find outbursts in 13% of the sample (type-1 stars), high and low states in 15%, periodic variations in 7%, and the usual variations seen in Galactic Be stars in 65% of the cases. The Galactic counterparts of type-1 objects could be the outbursting Be stars found by Hubert & Floquet (1998) after the analysis of Hipparcos photometry. We discuss the possibility that type-1 stars could correspond to Be stars with accreting white dwarf companions or alternatively, blue pre-main sequence stars surrounded by thermally unstable accretion disks. We provide coordinates and basic photometric information for these stars and some examples of light curves.

Key words: stars: pre-main sequence - stars: emission-line, Be - stars: variable: general - X-rays: binaries - galaxies: individual: SMC

Note to the reader concerning this PDF file: legends and scales of the figures were added on July 5, 2013.

1 Introduction

About 1/6-1/3 of all Galactic B-type stars with luminosity class III-V once showed H$\alpha$ in emission and have therefore been classified as Be stars (e.g. Zorec & Briot 1997). The optical and near-infrared spectra of Galactic Be stars usually display hydrogen, He I and singly ionized metallic emission lines, whose double-peaked shape indicate their origin in a circumstellar gaseous quasi-Keplerian disk. Detailed studies of Be stars in the Small Magellanic Cloud (SMC) have been performed only in recent years, being especially confined to open clusters like NGC 330 (e.g. Keller et al. 1999). These studies show the importance of studying Be stars in the low metallicity environment of the SMC since they serve as probes to test for the mechanisms of disk formation and of global disk oscillations (Baade et al. 2002; Hummel et al. 2001).

Over the past years, the microlensing projects (OGLE, MACHO, EROS) have monitored millions of stars in the Magellanic Clouds and Galactic bulge for variability. The huge resulting photometric databases are very well suited not only for microlensing studies but also for many other issues of modern astrophysics, including the distance scale, variable stars, star clusters etc. In particular, the OGLE II project (Udalski et al. 1997), has provided accurate BVI measurements for about 6.5 million stars from the central parts of the Magellanic Clouds (Udalski et al. 1998, 2000). Based on this same material, a unique catalog containing about 68 000 variable stars has just been released (Zebrun et al. 2001b).

The aim of this paper is to search the OGLE II database for Be star candidates and provide a much larger sample of these stars in the SMC than previously known. This will provide the basis for posterior follow-up spectroscopic studies of these objects, necessary to fully understand their nature. We will also call attention to several apparently new classes of light curves which appeared during our search for Be stars in the SMC.

The paper has the following structure. Observational data and the applied selection criteria are described in Sect. 2. Results are presented in Sect. 3, and discussed in Sect. 4. In Sect. 5, we present our current conclusions on the underlying nature of the observed types of variability.

2 The data

During four years (1997-2000), about 4.5 and 2 million stars were monitored in the LMC and SMC, respectively, in the course of the OGLE II project (Udalski et al. 1997). Typically, about 400 I and 30 B and V observations were secured for each star. An application of a newly developed photometric pipeline (Wozniak 2000; Zebrun et al. 2001a) to the data, based on the DIA method introduced by Alard & Lupton (1998), resulted in the detection of about 68 000 variable stars (Zebrun et al. 2001b). This catalog, apart from presenting positions and light curves for all its objects, provides in addition cross identifications with objects detected during earlier reductions carried out with Dophot. It should be stressed that the positions of the variable stars obtained with the DIA package were obtained from the variable signal only, and may be in principle quite different, especially in the very crowded regions, from the positions obtained from the Dophot photometry. However, the great majority of variable sources detected with DIA were unambiguously cross-correlated with objects detected with Dophot (Zebrun et al. 2001a).

To carry out our search, we inspected the OGLE II SMC BVI maps, and looked for stars matching the usual luminosities and colours observed in Galactic Be stars. Absolute magnitudes of Be stars based on Hipparcos parallaxes (Wegner 2000) indicate that Be stars of luminosity classes IV-V and III have absolute V-band magnitudes between -4 and 0. However, Garmany & Humphreys (1985) report on a population of extremely luminous non-supergiant Be stars in the Magellanic Clouds with absolute V-band magnitudes up to -6. Therefore, we searched for stars having absolute V-band magnitudes between -6 and 0. Assuming a distance modulus for the SMC of  $19.0 \pm 0.2$ mag, a visual extinction of 0.3 mag and a typical amplitude of the photometric variations of Be stars of 0.2 mag, the above absolute magnitudes imply apparent V-band magnitudes between 13.1 and 19.7. In addition to this magnitude constraint, we required that the selected stars should have colours in the range in which Galactic Be stars are usually found, viz.  -0.4 < B-V < 0.6 and -0.35 <V-I < 0.8. Using these criteria, we obtained a first sample of 5168 Be star candidates in our database. As a next step, we extracted the I-band light curves for each of these objects from the OGLE II catalog of variable stars (Zebrun et al. 2001b). The light curves were visually inspected and spurious variables, Cepheids and eclipsing binaries rejected. We then proceeded in classifying the remaining 1056 stars according to the appearance of their light curves. Our set of Be star candidates is likely to be complete for stars showing a rms larger than 0.02 mag in the I band. However, we could have missed Be stars either not showing long-term variations, or with I-band amplitudes less than 0.02 mag.

3 Results

Surprisingly, we found not only a large sample of 685 objects showing light curves similar to those observed for Galactic Be stars (we call them type-4 stars, with stochastic or sometimes quasi-periodic variations), but also 139 objects showing outbursts (called type-1 stars), 154 showing high and low states (called type-2 stars), and 78 stars showing periodic or near-periodic long-term oscillations (type-3 stars). 18 type-1 stars also showed sudden luminosity jumps like those observed in type-2 stars. We called them type-1/type-2 stars. In Figs. 1-6, we show examples of light curves for objects of the type-1 to type-4 subclasses. Basic information (OGLE name, distance (in arcsec) to the nearest star detected with Dophot, V magnitude, B-V and V-I colours, scatter of I-band magnitudes, and optional comments) on these stars is given in Tables 1-6. It is striking that type-2 and type-3 light curves have not been observed in any Galactic variable, to the best of our knowledge, and very few cases of Galactic type-1 stars seems to have been detected (see Sect. 3.1). Therefore all these stars clearly deserve further study. In Figs. 7 and 8 we show the V versus B-V, and V-Iversus B-V diagrams for the entire sample of stars. It is observed that the number of Be star candidates declines towards the extremes in both diagrams, indicating that the ranges of magnitude and colour we chose for our search were probably near-optimum to include all the Be stars in the database. Regarding the main sequence, most stars are displaced to the red in the V versus B-V diagram; this is in principle consistent with hydrogen recombination (free-bound and free-free) emission from circumstellar envelopes around Be stars (Dachs et al. 1988). Keeping in mind that our data have not been corrected for interstellar or circumstellar reddening, the sharp blue cut-off in the B-V colour is notable. This observational fact is consistent with the vanishing of the Be phenomenon in spectral types earlier than B0, partly due to the efficiency of radiation pressure to remove circumstellar gas in hotter stars.

3.1 Type-1 stars

 

 

Table 1: Type-1 stars. $\Delta \Phi$ is the distance (in arcsec) to the nearest star detected with Dophot.

Star	$\Delta \Phi$	V	B-V	V-I	rms
003623.36-733922.3	0.601	16.158	-0.233	-0.212	0.012
003832.64-732234.9	0.076	15.264	-0.139	-0.117	0.01
003918.20-733656.6	0.245	14.548	0.484	0.714	0.017
003922.09-732531.6	0.031	16.931	-0.041	-0.146	0.019
004036.15-732921.6	0.04	16.548	0.13	-0.03	0.062
004207.86-734501.9	0.136	16.804	-0.055	0.049	0.02
004215.08-731710.4	0.097	15.966	-0.157	-0.055	0.019
004231.84-732200.9	0.024	15.376	-0.106	-0.019	0.077
004326.72-725910.3	0.439	16.858	-0.128	-0.127	0.018
004502.43-732318.6	0.137	16.777	-0.048	0.039	0.012
004624.69-724657.3	0.609	19.333	0.203	0.463	0.045
004624.74-731941.7	0.102	15.851	0.069	0.169	0.09
004631.41-730335.6	0.085	17.113	-0.118	-0.002	0.04
004646.81-731849.2	0.054	16.701	-0.013	0.207	0.015
004650.39-731017.7	0.092	15.513	-0.105	-0.022	0.014
004653.17-732330.2	0.327	15.252	-0.033	0.012	0.014
004717.43-725227.6	0.119	17.071	0.353	0.403	0.136
004757.42-731050.8	0.122	15.714	-0.036	0.041	0.02
004800.14-730728.6	0.055	16.354	-0.226	0.046	0.101
004803.08-725404.2	0.347	16.704	-0.127	-0.126	0.015

 

 

Table 2: Type-1 stars showing transient quasi-periodic outbursts. ART means "after removing trend", BHS "before high state" and BF "before fading".

Star	$\Delta \Phi$	V	B-V	V-I	rms	Time-scale (days)
004957.09-730204.5	1.776	17.129	-0.133	0.122	0.049	332, ART
005039.05-725751.4	0.028	17.211	0.15	0.301	0.078	136
005118.72-732846.3	0.158	15.765	0.039	0.248	0.013	216, ART
005149.34-724134.3	0.069	16.026	-0.013	0.163	0.02	38, BF
005157.18-730811.8	0.183	16.544	-0.058	0.092	0.025	22, ART
005235.60-723751.7	0.03	14.573	-0.145	-0.114	0.045	94
005312.58-725533.6	0.039	16.024	-0.121	-0.029	0.037	58
005321.08-724548.3	0.095	15.526	-0.201	-0.067	0.049	231
005355.66-724359.2	0.151	15.56	-0.092	-0.057	0.114	85 or 42, ART, BHS
005623.53-723926.3	0.071	16.225	0.065	0.309	0.022	215, ART
005758.52-722228.7	0.084	15.794	-0.088	0.002	0.03	40, ART, BF
005802.33-724137.5	0.031	17.092	-0.167	-0.154	0.057	16, ART
005950.21-722817.4	0.123	17.342	-0.112	0.03	0.017	173, ART
010001.47-724046.9	0.062	15.876	-0.187	-0.039	0.154	133 or 101, ART
010023.52-723302.7	0.025	15.6	-0.194	-0.079	0.022	168, ART
010120.64-721118.7	0.097	15.489	-0.065	0.078	0.019	75, ART
010332.59-720326.5	0.086	14.91	-0.207	-0.129	0.146	127, ART
010409.79-723835.6	0.086	15.325	-0.097	0.046	0.026	112, BHS
010838.56-723633.5	0.036	16.115	-0.075	0.092	0.035	136

	Figure 1: Examples of type-1 Be star candidates showing sharp outbursts.
Open with DEXTER

	Figure 2: Examples of type-1 Be star candidates showing hump-like outbursts.
Open with DEXTER

The outbursts shown by type-1 stars were basically of two types: those characterized by a sudden rise of luminosity followed by a gradual decline, generally lasting tens of days with amplitudes $\mathrel{\copy\laxbox}$0.2 mag, and those with usually slower declines, lasting hundreds of days with amplitudes >0.2 mag, and characterized by more symmetric rising and fading timescales. In general, in both kinds of outbursts, the stars were redder when brighter and we could not find any evidence of a correlation of outburst rising delay with wavelength. Some stars showed both kinds of outbursts, and sometimes it was difficult to classify them when the outburst was faint and not well resolved, or in the cases of noisy light curves. For this reason we do not provide a sub-classification for type-1 stars. Not always these stars are showing a constant quiescence brightness level. For 16% of type-1 stars (22 objects) it was possible to identify an outburst time-scale, i.e.  a typical time for outburst recurrence, although this recursion sometimes was observed only as a transient phenomenon and not during the whole observing period. Basic information for type-1 stars is given in Tables 1 and 2. Exemplary light curves of this type of variable stars are shown in Figs. 1 and 2. The outburst time-scales, given in Table 2, run from 16 to 332 days, with a mean of 126 days. The time-scale histogram shows a decrease of cases toward longer periods; 68% of the objects show time-scales shorter than 150 days. There is no clear correlation between outburst time-scale, and stellar colour or apparent magnitude.

Our type-1 objects probably correspond to the bumpers found in the Large Magellanic Cloud by Cook et al. (1995) after analysing the MACHO collaboration database. These authors report on the discovery of a group of bright main sequence stars with $V \sim 15{-}17$ which have a constant luminosity for extended periods of time, but show occasional outbursts at 10-30% amplitude level. They found that the episodes in more than 50% of the cases are asymmetric and shorter than about 50 days with a more rapid brightening than dimming. The fact that H$\alpha$ and H$\beta$ emission was observed in the spectra of 7 of these stars led Cook et al. (1995) to suggest that these stars could be related to, or maybe identical to, Galactic Be stars.

The Galactic counterparts of type-1 objects could be the outbursting Be stars found by Hubert & Floquet (1998) analyzing Hipparcos photometry. They find short-lived outbursts in $\omega$ CMa and other 13 Be stars, and also a long-lived outburst in $\upsilon$ Cyg and another 7 Be stars. The outbursts were preferentially detected in early Be stars with rather low to moderate projected rotational velocities. The average time scale for the recurrence of short-lived outburst is, however, slightly larger than that observed for our SMC sample. Hubert & Floquet (1998) argue that both kinds of outbursts probably have the same origin and can be explained by discrete high density emitting plasma events seen under low inclination angles with respect to the rotational axis. The number of cases presented by these authors is too small and the photometry too scarce to make a detailed comparison with our type-1 stars, however.

Although at present we cannot exclude the Be star nature of type-1 objects, we will present, in the next section, two possible alternative explanations for these objects.

3.2 Type-2 stars and type-1/type-2 stars

Type-2 stars show sudden brightness jumps of an amplitude of a few tenths of magnitude, with the star remaining at a rather constant brightness level for hundreds of days. Type-2 stars usually don't show additional variability, like the irregular variations observed in type-4 stars, except for rather smooth long-term changes. Type-2 stars can be found in basically the same colour range as type-1 stars, but type-2 stars are statistically bluer than type-1 stars. Eighteen type-1 stars in our database also showed high-low states like those observed in type-2 stars. These type-1/type-2 stars were only found in the range of 15.5<V<17 and in a narrow colour box characterized by  -0.2<B-V<0.2 and -0.2<V-I<0.25. The existence of these "transition" stars supports the conjecture that type-1 and type-2 stars could correspond to the same kind of object. Basic information for type-2 and type-1/type-2 stars is given in Tables 3 and 4.

 

 

Table 3: Type-2 stars.

Star	$\Delta \Phi$	V	B-V	V-I	rms
004234.39-733058.2	0.043	15.989	-0.148	0.002	0.021
004258.05-730230.7	0.036	16.059	0.028	0.176	0.019
004319.46-731705.7	0.099	16.403	-0.056	0.132	0.032
004330.69-732034.2	0.028	16.428	-0.194	-0.177	0.009
004414.25-731215.5	0.086	17.297	-0.107	-0.028	0.023
004443.05-731316.5	0.068	16.217	-0.072	0.028	0.017
004504.35-724449.9	0.076	17.906	0.336	0.549	0.051
004510.40-731648.1	0.104	15.855	-0.105	-0.022	0.009
004539.31-731040.1	0.433	17.849	-0.104	0.702	0.088
004546.74-733233.1	0.008	16.284	-0.032	0.158	0.032
004556.84-730919.8	0.068	17.128	-0.057	0.031	0.013
004601.22-731821.9	0.11	16.374	0.033	0.255	0.018
004610.97-732535.2	0.037	15.439	0.009	0.032	0.146
004633.48-730352.1	0.026	15.489	-0.066	0.063	0.04
004639.77-725241.0	0.047	15.614	-0.179	-0.173	0.011
004651.07-730215.3	0.048	15.801	-0.026	0.176	0.026
004655.32-731207.6	0.094	16.164	-0.113	0.103	0.03
004714.29-731044.0	0.09	17.635	-0.022	0.043	0.022
004714.53-731349.7	0.131	15.068	-0.196	-0.172	0.009
004719.31-732533.6	0.11	16.449	-0.074	0.145	0.073

 

 

Table 4: Type-1/type-2 stars. The nomenclature is as in Table 2.

Star	$\Delta \Phi$	V	B-V	V-I	rms	Time-scale (days)
004402.00-733129.4	0.221	15.456	-0.003	0.232	0.016	284
004406.65-732938.2	0.034	16.285	-0.029	0.114	0.02
004650.21-732807.3	0.042	15.442	-0.192	-0.191	0.017
004738.11-731126.1	0.12	15.484	-0.114	0.022	0.008
004800.73-732253.0	0.137	15.842	-0.048	0.144	0.018
004817.58-725028.8	0.133	16.329	-0.109	-0.048	0.016
004848.27-732611.3	0.062	15.462	-0.098	0.016	0.067	39, BF
004858.25-724119.4	0.054	16.157	-0.074	0.076	0.015
005045.50-730112.9	0.071	16.398	-0.057	0.038	0.019
005053.20-731030.8	0.046	15.925	-0.054	0.157	0.096
005105.65-731311.5	0.044	15.911	-0.032	0.208	0.047
005112.13-725656.2	0.08	16.196	-0.082	0.09	0.034	52, ART
005141.43-731129.9	0.051	16	-0.123	0.024	0.091
005147.58-730924.7	0.066	15.629	-0.073	0.077	0.045
005456.92-731200.4	0.056	16.344	-0.156	-0.143	0.01
005651.99-724027.1	0.059	15.735	-0.065	-0.015	0.067
005854.06-722841.9	0.114	17.014	-0.04	0.134	0.042
010701.71-724754.9	0.036	15.601	-0.152	-0.053	0.021

3.3 Type-3 stars

In these periodic objects, we searched for periods longer than 0.2 days using a variety of period searching algorithms implemented in graphic C-routines written by us, and also in IRAF. We found periodicities in the range of 17 to 720 days. The accuracy for periods longer than 200 days is low, and these variations can easily be quasi-periodic rather than strictly periodic. 51% of the periods were found in the range of 17-100 days. The mean period was 135 days. Many of the stars showed significant aliases in the periodogram in addition to the main period, and 2 showed evidence of a variable period. Five stars turned out to be eclipsing binaries, with evidence of additional variability not related to changing aspects of the binary system. In general, type-3 stars were redder when brighter. All the relevant information is given in Table 5. The 9 type-3 stars in our sample with periods longer than 200 days have V-I colours in the range of 0.0-0.2 mag, and B-V colours in the range of -0.1-0.0 mag. They correspond to stars with visual magnitudes between 15.5 and 18.0 mag. In general, type-3 stars show similar colours than the other types of stars we are discussing, but they appear more homogeneously distributed in Figs. 7 and 8, with a tendency to concentrate in the red part of the colour-colour diagram.

 

 

Table 5: Type-3 stars. ART means "after-removing-trend", ChP changing period, LA low amplitude, MA multiple aliases, and VA variable amplitude.

Star	$\Delta \Phi$	V	B-V	V-I	rms	Period (days)
003813.22-734144.7	0.291	16.607	-0.045	0.022	0.058	$187\pm19$
003832.82-734404.2	0.385	17.447	0.448	0.609	0.106	$79\pm3$, MA
003833.35-731510.1	0.177	16.467	0.019	0.084	0.064	$164\pm3$
003927.34-733309.6	0.322	15.855	-0.158	0.057	0.055	$\sim$27, ART, MA
003952.15-730057.7	0.53	18.815	-0.042	0.022	0.077	$107\pm6$, double eclipse?
004019.36-730402.9	2.172	16.207	-0.033	0.146	0.059	$200\pm22$, VA
004024.94-734416.1	1.58	16.531	-0.018	0.04	0.01	$\sim$448
004211.38-732437.7	0.345	17.916	-0.089	0.01	0.058	$74\pm3$
004212.21-734120.0	0.017	15.921	-0.197	-0.138	0.039	$46\pm1$, alias 1.01932
004323.84-733930.1	0.636	16.341	-0.19	-0.145	0.016	$62\pm2$, alias 0.98134
004336.91-732637.7	0.097	14.178	0.181	0.331	0.031	$118\pm7$, MA
004357.18-732019.9	0.139	16.51	0.386	0.668	0.065	$29\pm1$
004454.66-732802.9	0.183	14.817	0.286	0.576	0.03	$17.37\pm0.15$, VA
004517.55-732343.6	0.044	17.513	0.306	0.222	0.094	$171\pm15$
004541.10-731219.2	0.082	17.149	0.089	0.24	0.032	$182\pm18$
004541.80-724932.3	0.046	17.252	0.308	0.48	0.206	$85\pm3$
004554.14-731404.3	0.781	15.483	0.517	0.709	0.01	$99\pm4$, LA
004633.06-731919.1	0.129	17.15	-0.012	0.181	0.021	$38\pm1$, ART
004633.76-731204.3	0.092	14.058	0.206	0.385	0.057	$184\pm18$, eclipsing
004652.03-731423.7	0.084	15.995	-0.069	0.087	0.021	$\sim$567, other 67?
004653.24-724300.0	0.495	19.469	0.03	0.12	0.166	$66\pm3$
004702.75-730618.3	0.126	16.57	0.122	0.243	0.016	$17.3\pm0.15$, ART, eclipsing
004723.53-730347.0	0.11	16.328	-0.043	0.162	0.016	$101\pm2$, ART, eclipsing
004748.20-731906.1	0.073	18.355	0.194	0.392	0.079	$177\pm10$
004750.14-731316.4	0.222	15.475	0.269	0.471	0.009	$30.0\pm0.3$, LA
004816.01-730635.7	0.212	15.917	0.123	0.338	0.04	$26.45\pm0.20$, strange phase curve, also type-1?
004833.67-732955.6	0.221	19.403	0.129	0.417	0.14	$161\pm12$
004843.23-731415.8	0.111	16.736	-0.081	0.066	0.062	$\sim$357, VA
004849.06-724309.2	0.088	17.588	0.446	0.639	0.108	$150\pm15$, rather time-scale

 

 

Table 6: Type-4 stars.

Star	$\Delta \Phi$	V	B-V	V-I	rms
003618.14-734624.6	0.086	14.929	0.353	0.779	0.279
003618.15-734247.4	1.419	16.177	-0.131	-1E-3	0.036
003619.44-732553.1	0.132	19.519	0.258	0.516	0.182
003621.53-732610.6	0.05	14.741	0.067	0.214	0.124
003623.02-734651.0	0.016	19.551	0.484	0.531	0.304
003645.28-733259.7	1.863	15.59	-0.024	0.2	0.015
003652.74-732857.9	3.222	14.397	0.081	0.177	0.016
003715.60-734546.0	1.804	16.09	0.453	0.647	0.013
003726.27-731420.0	0.511	19.63	0.318	0.559	0.25
003730.99-731112.4	1.965	15.846	0.109	0.209	0.01
003744.41-730447.6	0.109	16.996	-0.087	-0.051	0.028
003804.71-735150.5	0.329	19.434	0.009	0.092	0.065
003810.16-730138.4	1.22	17.296	0.59	0.767	0.02
003813.77-731340.0	0.208	17.335	-0.081	0.116	0.016
003817.01-734852.6	0.025	15.199	0.462	0.709	0.28
003827.69-733314.5	1.499	16.126	-0.156	0.124	0.021
003833.29-732629.4	1.317	16.725	0.414	0.619	0.011
003836.25-734813.4	0.303	15.383	-0.14	-0.082	0.022
003837.66-731158.3	0.093	14.894	-0.085	0.057	0.028

3.4 Type-4 stars

	Figure 3: Examples of type-1/type-2 Be star candidates showing outbursts and high-low states.
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	Figure 4: Examples of type-2 Be star candidates showing high and low states.
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	Figure 5: Examples of type-3 Be star candidates showing periodic oscillations.
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	Figure 6: Examples of type-4 Be star candidates showing random variability.
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They are the most numerous in our sample, sharing colour ranges with the other types of variables. They usually show stochastic variability in time scales running from days to years (Fig. 6). In some occasions we observed quasi-periodic oscillations on time scales of weeks, and in others short-duration, eclipse-like events. Information on type-4 stars is given in Table 6.

4 Discussion

We have reviewed the literature in order to find out if our stars have already been detected as variable stars by other surveys. In the original sample of 5168 objects, we found 8 stars classified as Be stars by Keller et al. (1999). We classified four of them as type-4 (ngc 330/219, ngc 330/235, ngc 346/259 and ngc 346/377), and the others were missed by our visual inspection search method since they show I-band rms lower than 0.02 mag (ngc 330/238, ngc 330/1054, ngc 330/1064 and ngc 330/1239). We also found one type-4 star listed as extreme Be-star by Garmany & Humphreys (1985, their star AV433). Another two type-4 stars are listed as Be/X-ray binaries and one as possible Be/X-ray binary in the compilation by Haberl & Sasaki (2000, their stars 20, 23 and 6, respectively). The fact that eight type-4 stars have been previously classified as Be stars or Be/X-ray binaries suggests that all type-4 stars might be related with Be stars in some way. Their light curve morphology, quite similar to Galactic Be stars, supports this conjecture.

Type-1 light curves are reminiscent of those observed in FU Orionis stars, thought to be caused by accretion events in protostellar disks around young solar-type stars. There is a notable similarity between the shape of the sharp type-1 outbursts with those observed in the extreme classical T Tauri star EX Lupi (Herbig et al. 2001) and the FU Ori star V 1057 Cyg (Bell et al. 1995). However, the amplitude and duration of the outbursts are respectively factors 20 and 1000 smaller in type-1 stars. On the other hand, the general appearance of type-2 light curves, i.e., a rapid rise of luminosity followed by a "plateau'' of rather constant brightness resemble (except for a scale factor) the initial stages of the outbursts observed in V1515 Cyg and FU Ori (Bell et al. 1995). Type-1 light curves are also quite similar in shape to those observed in cataclysmic variables (CVs) of the dwarf novae type. However, these objects experience in general much larger amplitude outbursts ($\sim$2-7 mags), have a rather constant luminosity at maximum and usually return to the same quiescence level after outburst.

The outbursts observed in CVs and FU Ori stars have been modeled by mass transfer instabilities in accretion disks (Meyer & Meyer-Hofmeister 1981; Bell et al. 1995). A heating front propagates across the disk after a certain critical density is reached, pushing the disk into a hot state with high mass transfer rate and consequently high accretion luminosity. Rapid outburst rising times can be produced by outbursts starting in the outer disk and propagating inwards, and slower rising times can be produced by outbursts triggered in the inner disk and propagating outwards. We can speculate that the same phenomenon responsible for FU Ori outbursts is also present in more massive young stars, producing light curve patterns like the ones observed in type-1 and type-2 stars. In this view, the smaller outburst amplitude and shorter duration of type-1 outburst when compared with those observed in FU Ori stars should correspond to accretion of matter with lower mass transfer rates. Sharp and hump-like outbursts should correspond to outside-in and inside-out outbursts, respectively. Type-2 stars could be explained by outside-in outbursts followed by a sustained period of a high mass-transfer rate. A characteristic of the FU Ori outbursts is their larger amplitude at shorter wavelengths, contrary to what is observed in type-1 stars. However, dwarf novae are redder at maximum.

In connection with the above ideas, it is interesting that one of our objects classified as type-1 was identified by Beaulieu et al. (2001) as a possible pre-main sequence star (ESHC2). In principle, this is in contradiction with the Cook et al. (1995) classification of some of these objects as Be stars. It is possible that the presence of Balmer emission not necessarily implies a Be star classification for the "bumpers" detected in the LMC by Cook and collaborators. In fact, the low ionization metal absorption lines usually found in optical spectra of Herbig Ae/Be stars could be hard to detect in low metallicity stellar photospheres like those found in the SMC and LMC. Therefore, it is reasonable to ask if perhaps all of type-1 and type-2 objects are actually pre-main sequence stars with FU Ori-like accretion disk activity. In this case, the mass accretion rates need to be much higher than those observed in normal Be star discs, or even in Be/X-ray binaries, to yield luminosities comparable or larger than the luminosity of the accreting B-type star. Since the nebulosities defining Herbig Ae/Be objects cannot be resolved at the distance of the Magellanic Clouds, the answer to the above question needs to await future spectroscopic studies, especially in the infrared, and possibly very high-resolution imaging studies which could reveal the surrounding nebulosities. We must keep in mind, however, that Hipparcos photometry of Galactic Herbig Ae/Be stars apparently does not reveal type-1 like activity (van den Ancker et al. 1998). Also, the optical light of some Galactic Be stars showing outbursts, like $\lambda$ Eri and $\mu$ Cen, is apparently dominated by the stellar continuum during quiescence, and the spectrum does not reveal the strong emission lines typical of massive Herbig Ae/Be envelopes. Although it is not clear if these Galactic Be stars are the same kind of object that type-1/type-2 stars, we recognize that these two facts are the weak points in the pre-main sequence scenario. We therefore offer an alternative explanation in the next paragraph.

Type-1 star outbursts resemble also in shape the optical outbursts observed in some Be/X-ray binaries (e.g. A 0538-66, Densham et al.  1983), except for their much smaller amplitudes and redder colours. It is currently assumed that in these objects a neutron star companion undergoes episodes of mass accretion when passing through the envelope of a Be star primary (e.g., Okazaki & Negueruela 2001). These high-energy phenomena are no doubt relevant in the X-ray domain, but should not show up at optical and near infrared wavelengths. In addition, the optical counterparts of Galactic and Magellanic Cloud Be/X-ray binaries have spectral types earlier than B2 (Negueruela 1998). This is in principle contrary to the distribution of B-V colours in Fig. 7. However, the similarity between the X-ray type-I and type-II outbursts observed in Be/X-ray binaries and the narrow and hump-like outburst observed in type-1 stars suggest that they could be due to accretion by a white dwarf, not a neutron star. The Be+WD system should produce less energetic outburst, eventually much prominent in the optical and infrared. Favouring this hypothesis is the fact that many Be+WD binaries, even with late-type B stars, are expected from evolutionary calculations (Raguzova 2000; Waters et al. 1989). Only few candidates for these systems have been found up to now, likely due that the white dwarfs, if present, should be hard to detect (Apparao 1991). The hypothesis of accreting white dwarf companions would naturally explain some of the type-1 light curves. The same model for periodic X-ray outbursts in Be/X-ray binaries by Okazaki & Negueruela (2001) could eventually be applied to Be+WD systems. In this model, periodic narrow outbursts occur in systems with high orbital eccentricity, every time that the compact object captures gas from the disc at every periastron passage. Hump-like outbursts occurs in systems with low eccentricity, when the outer disc eventually passes beyond the orbit of the companion. Accordingly to Apparao (1991), observations of time delays between enhancements of optical line and continuum emission could identify Be stars with white dwarf companions. We must keep in mind, that only a small fraction of type-1 objects shows periodic or quasiperiodic outbursts, however.

Concerning type-3 stars, they can be ruled out to be Cepheids, since their large periods (sometimes hundreds of days) are incompatible with their inferred luminosities. On the other hand, the periods are one or two orders of magnitude longer than those observed in Galactic pulsating B stars. This hints at the possibility that type-3 variability is linked to the envelope rather than to the star itself. There is evidence for global one-armed oscillations in the envelopes of Galactic Be stars (Okazaki 1997), but the associated photometric variations are not so strictly periodic as those observed in type-3 stars, the time-scales are longer, about 7 years in average, and, from a theoretical point of view, the oscillations are expected to disappear in the low metallicity environment of the SMC or, alternatively, to slow down, yielding periods in excess of several years (Hummel et al. 2001), in disagreement with the observed type-3 oscillations. The distribution of type-3 stars in the colour-colour diagram of Fig. 8 suggests that these stars are perhaps not be linked to the Be star phenomenon at all. Preliminary spectroscopy of one type-3 object seems to corroborate this view. It shows double H$\alpha$ emission with a deep central absorption and total equivalent width $\sim$100 Å, too large for an isolated Be star (Mennickent et al.  in preparation). We speculate that type-3 stars could be young objects with massive envelopes ongoing some kind of oscillation.

5 Conclusions

We have presented a sample of $\sim$1000 Be star candidates in the Small Magellanic Cloud, giving positions and basic photometric information along with periodicities when present. Many of these objects show apparently new kinds of photometric variability never seen before, and this feature enabled us to carry out an empirical classification based on the light curve appearance. There is evidence that some of these objects are truly Be stars, but spectroscopy is needed to confirm this suspicion. On the other hand, the hypothesis that at least part of the type-1 and type-2 stars are Be-stars with accreting white dwarfs, or alternatively, pre-main sequence stars showing accretion disk instabilities, should be studied more thoroughly.

	Figure 7: The V vs. B-V diagram for the sample stars. Blue dots correspond to type-1 stars, red dots to type-2 stars, green dots to type-3 stars, circles to type-4 stars and black dots to type-1 stars showing high and low states, as type-2 stars. The track of the main sequence (Allen 2000) is shown for reference. Note the sharp cut-off at the blue edge.
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	Figure 8: The V-I vs. B-V diagram for the sample stars. The track of the main sequence (Allen 2000) is shown as a reference. Meaning of the symbols are as in Fig. 7.
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The understanding of the phenomena causing the photometric variability of the stars discussed in this paper requires knowledge of the spectral energy distributions of these stars. We plan to discuss, in a forthcoming paper, the detailed photometric properties of these objects along with spectroscopic data. It should be interesting to test the accretion scenario for type-1 stars. Since the theory of accretion is rather well developed, it could be a source of physical information about the environments surrounding these objects. We also plan to search the OGLE-II database for Be stars in the Large Magellanic Cloud. It should be interesting to investigate if the same types of light curves are observed in the LMC, whose metallicity is intermediate between the SMC and our Galaxy, and how the light curve properties are modified by the change in metallicity.

Acknowledgements

This work was supported by Grant Fondecyt 1000324 and DI UdeC 202.011.030-1.0. The authors are very grateful to Professor Bohdan Paczynski for many interesting suggestions on this paper. We would also like to thank the OGLE collaboration for making their data public domain, thus enabling us to carry out this research. We also acknowledge the anonymous referee who made valuable comments to improve a first version of this manuscript.

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Online Material

 

Table 1: Type-1 stars.

Star	$\Delta\Phi$	V	B-V	V-I	rms
OGLE003623.36-733922.3	0.601	16.158	-0.233	-0.212	0.012
OGLE003832.64-732234.9	0.076	15.264	-0.139	-0.117	0.01
OGLE003918.20-733656.6	0.245	14.548	0.484	0.714	0.017
OGLE003922.09-732531.6	0.031	16.931	-0.041	-0.146	0.019
OGLE004036.15-732921.6	0.04	16.548	0.13	-0.03	0.062
OGLE004207.86-734501.9	0.136	16.804	-0.055	0.049	0.02
OGLE004215.08-731710.4	0.097	15.966	-0.157	-0.055	0.019
OGLE004231.84-732200.9	0.024	15.376	-0.106	-0.019	0.077
OGLE004326.72-725910.3	0.439	16.858	-0.128	-0.127	0.018
OGLE004502.43-732318.6	0.137	16.777	-0.048	0.039	0.012
OGLE004624.69-724657.3	0.609	19.333	0.203	0.463	0.045
OGLE004624.74-731941.7	0.102	15.851	0.069	0.169	0.09
OGLE004631.41-730335.6	0.085	17.113	-0.118	-0.002	0.04
OGLE004646.81-731849.2	0.054	16.701	-0.013	0.207	0.015
OGLE004650.39-731017.7	0.092	15.513	-0.105	-0.022	0.014
OGLE004653.17-732330.2	0.327	15.252	-0.033	0.012	0.014
OGLE004717.43-725227.6	0.119	17.071	0.353	0.403	0.136
OGLE004757.42-731050.8	0.122	15.714	-0.036	0.041	0.02
OGLE004800.14-730728.6	0.055	16.354	-0.226	0.046	0.101
OGLE004803.08-725404.2	0.347	16.704	-0.127	-0.126	0.015
OGLE004809.31-732028.9	0.298	15.594	-0.165	-0.134	0.019
OGLE004814.06-732203.5	0.098	14.906	-0.17	-0.124	0.175
OGLE004815.63-731022.8	0.113	16.352	0.482	0.745	0.026
OGLE004833.67-732955.6	0.221	19.403	0.129	0.417	0.14
OGLE004847.74-732026.3	0.031	16.575	0.032	0.156	0.014
OGLE004857.01-730856.4	0.088	16.989	0.212	0.366	0.053
OGLE004903.51-730441.3	0.045	17.208	-0.039	-0.01	0.018
OGLE004911.46-724937.0	0.079	15.721	0.071	0.196	0.204
OGLE004911.88-730854.8	0.096	16.121	-0.018	0.006	0.017
OGLE004912.79-725948.5	0.245	16.95	-0.081	-0.028	0.026
OGLE004914.12-731652.0	0.092	15.329	-0.05	0.106	0.033
OGLE004924.46-731226.8	0.054	15.769	-0.04	0.033	0.036
OGLE004925.37-730058.8	0.121	16.811	-0.061	0.119	0.036
OGLE004942.00-732314.2	0.251	14.975	0.046	0.248	0.02
OGLE004951.50-725730.6	0.072	15.874	0.046	0.167	0.129
OGLE005011.58-725459.5	0.055	16.006	0.126	0.48	0.025
OGLE005025.61-725136.0	0.462	16.665	-0.219	-0.05	0.075
OGLE005026.02-725131.2	0.438	16.837	-0.211	-0.006	0.103
OGLE005039.13-724154.3	0.063	18.871	0.265	0.566	0.027
OGLE005042.39-730930.5	0.021	15.899	-0.045	0.182	0.049
OGLE005045.58-730253.9	0.395	16.313	0.05	0.154	0.017
OGLE005057.76-731958.5	0.069	16.199	-0.069	0.062	0.029
OGLE005059.21-724357.3	0.172	14.805	-0.02	0.352	0.034
OGLE005120.56-724325.0	0.01	15.774	-0.091	0.227	0.052
OGLE005130.91-725549.8	2.081	18.66	-0.056	0.359	0.123
OGLE005153.47-724009.2	0.132	15.421	-0.129	-0.159	0.012
OGLE005154.82-731616.1	0.03	15.479	-0.131	-0.128	0.011
OGLE005215.39-731915.0	0.014	15.916	-0.099	-0.035	0.053
OGLE005217.38-731926.0	0.059	15.981	-0.12	-0.071	0.025
OGLE005224.40-724038.6	0.042	14.032	0.003	0.021	0.26
OGLE005227.51-732001.2	0.123	13.186	1E-3	0.048	0.018
OGLE005228.02-731539.5	0.026	16.592	-0.138	-0.092	0.031
OGLE005232.63-731707.2	0.056	17.012	-0.055	0.066	0.024
OGLE005246.43-732424.2	0.087	17.852	-0.042	0.123	0.033
OGLE005252.49-731833.5	0.05	15.254	0.163	0.57	0.178
OGLE005256.10-725326.6	0.165	16.524	-0.118	-0.021	0.021
OGLE005258.18-724410.5	0.151	15.475	-0.075	0.235	0.028
OGLE005302.77-731759.1	0.018	15.079	-0.007	0.132	0.053
OGLE005307.87-724727.7	0.04	16.668	-0.238	0.034	0.081
OGLE005347.05-730608.6	0.225	15.443	-0.174	-0.144	0.019
OGLE005356.76-731029.2	0.032	15.049	-0.148	0.184	0.067
OGLE005358.65-731018.0	0.126	17.73	-0.047	0.024	0.019
OGLE005451.66-723910.8	0.157	16.004	-0.012	-0.058	0.039
OGLE005504.55-724637.3	0.253	14.156	-0.111	-0.178	0.02
OGLE005516.89-724607.1	0.443	15.837	-0.166	-0.18	0.02
OGLE005523.54-725528.8	0.089	16.318	0.014	-0.336	0.084
OGLE005531.38-730439.3	0.083	16.052	-0.138	-0.099	0.014
OGLE005614.63-723755.1	0.045	14.568	0.05	0.349	0.008
OGLE005626.60-722622.9	0.122	16.167	-0.107	-0.099	0.029
OGLE005641.86-724425.4	0.137	14.717	-0.113	-0.137	0.007
OGLE005837.83-721628.8	0.109	16.086	-0.091	0.095	0.017
OGLE005854.41-724352.3	0.116	15.048	-0.182	-0.153	0.027
OGLE005904.99-722252.3	0.048	15.788	-0.061	0.083	0.018
OGLE005916.06-722100.3	0.024	14.512	-0.034	0.16	0.072
OGLE005929.29-723103.7	0.141	16.124	-0.116	-0.083	0.009
OGLE005939.44-725241.5	0.022	15.352	0.102	0.113	0.309
OGLE010041.93-723028.6	0.149	14.73	-0.178	-0.19	0.031
OGLE010043.94-722604.8	0.157	14.508	-0.194	-0.164	0.026
OGLE010056.79-721635.2	0.221	15.195	-0.161	-0.038	0.022
OGLE010058.69-723049.9	0.112	13.957	-0.089	0.015	0.026
OGLE010104.52-722023.4	0.024	15.251	-0.028	0.138	0.012
OGLE010137.82-721844.4	0.041	15.562	-0.147	0.007	0.072
OGLE010144.76-723405.3	0.795	16.976	-0.148	-0.015	0.012
OGLE010150.83-721102.4	0.01	16.243	-0.207	-0.043	0.034
OGLE010201.88-721512.1	0.067	17.666	-0.265	-0.156	0.039
OGLE010213.80-722213.0	0.015	14.376	0.035	0.229	0.01
OGLE010237.04-725943.8	0.044	17.672	0.369	0.57	0.202
OGLE010244.01-722954.7	0.121	15.103	-0.078	0.134	0.022
OGLE010350.50-724853.2	0.128	14.989	-0.159	-0.094	0.039
OGLE010353.59-724908.0	0.05	16.012	-0.01	0.3	0.021
OGLE010422.27-723534.5	0.075	17.701	-0.14	-0.101	0.019
OGLE010542.57-722747.3	0.037	14.794	0.052	0.279	0.029
OGLE010603.21-724931.1	0.068	14.801	-0.086	0.028	0.057
OGLE010615.06-725741.9	0.312	16.008	0.041	0.174	0.068
OGLE010621.11-721603.7	0.071	15.292	-0.147	-0.106	0.033
OGLE010710.78-722216.2	0.462	17.191	0.588	0.722	0.013
OGLE010712.24-722218.9	0.331	15.09	0.022	0.147	0.021
OGLE010740.60-722237.3	1.705	18.274	0.325	0.607	0.024
OGLE010744.20-722740.9	0.165	15.482	-0.08	0.227	0.045
OGLE010807.38-721932.6	0.071	14.189	-0.181	-0.12	0.034
OGLE010809.52-721556.8	0.116	14.484	-0.183	-0.097	0.03
OGLE010825.82-722327.2	0.092	13.969	-0.031	0.206	0.034

 

Table 3: Type-2 stars.

Star	$\Delta\Phi$	V	B-V	V-I	rms
OGLE004234.39-733058.2	0.043	15.989	-0.148	0.002	0.021
OGLE004258.05-730230.7	0.036	16.059	0.028	0.176	0.019
OGLE004319.46-731705.7	0.099	16.403	-0.056	0.132	0.032
OGLE004330.69-732034.2	0.028	16.428	-0.194	-0.177	0.009
OGLE004414.25-731215.5	0.086	17.297	-0.107	-0.028	0.023
OGLE004443.05-731316.5	0.068	16.217	-0.072	0.028	0.017
OGLE004504.35-724449.9	0.076	17.906	0.336	0.549	0.051
OGLE004510.40-731648.1	0.104	15.855	-0.105	-0.022	0.009
OGLE004539.31-731040.1	0.433	17.849	-0.104	0.702	0.088
OGLE004546.74-733233.1	0.008	16.284	-0.032	0.158	0.032
OGLE004556.84-730919.8	0.068	17.128	-0.057	0.031	0.013
OGLE004601.22-731821.9	0.11	16.374	0.033	0.255	0.018
OGLE004610.97-732535.2	0.037	15.439	0.009	0.032	0.146
OGLE004633.48-730352.1	0.026	15.489	-0.066	0.063	0.04
OGLE004639.77-725241.0	0.047	15.614	-0.179	-0.173	0.011
OGLE004651.07-730215.3	0.048	15.801	-0.026	0.176	0.026
OGLE004655.32-731207.6	0.094	16.164	-0.113	0.103	0.03
OGLE004714.29-731044.0	0.09	17.635	-0.022	0.043	0.022
OGLE004714.53-731349.7	0.131	15.068	-0.196	-0.172	0.009
OGLE004719.31-732533.6	0.11	16.449	-0.074	0.145	0.073
OGLE004721.86-730650.1	0.074	14.026	-0.029	0.186	0.007
OGLE004732.99-731531.6	0.103	15.23	0.089	0.255	0.037
OGLE004735.47-732248.2	0.03	16.926	0.039	0.289	0.036
OGLE004748.07-730140.3	0.022	16.338	-0.031	0.185	0.012
OGLE004748.70-731752.4	0.356	18.438	-0.002	0.024	0.022
OGLE004748.79-730519.4	0.2	16.503	0.028	0.278	0.016
OGLE004756.74-730308.4	0.157	15.807	-0.054	0.172	0.014
OGLE004801.18-731523.5	0.099	17.095	0.04	0.264	0.085
OGLE004812.73-731201.0	0.139	17.265	-0.004	0.097	0.017
OGLE004817.65-730933.6	0.189	17.123	0.05	0.276	0.025
OGLE004822.43-725856.8	0.061	17.324	-0.093	-0.065	0.014
OGLE004832.21-724558.5	0.093	17.593	-0.15	-0.043	0.029
OGLE004839.28-730828.6	0.066	16.617	-0.184	-0.106	0.045
OGLE004847.09-732004.4	0.68	16.714	0.245	0.436	0.107
OGLE004848.83-730620.1	0.026	14.382	-0.04	0.114	0.056
OGLE004849.49-724800.0	0.126	15.138	0.207	0.388	0.044
OGLE004853.10-731409.8	0.098	14.919	-0.106	0.026	0.013
OGLE004853.63-730822.9	0.178	17.377	0.382	0.668	0.018
OGLE004854.10-725526.1	0.089	16.316	-0.052	1E-3	0.024
OGLE004905.07-731832.0	0.081	15.87	-0.07	-0.017	0.085
OGLE004909.39-731831.9	0.378	16.625	0.029	0.209	0.02
OGLE004909.67-724839.2	0.045	16.928	0.159	0.127	0.063
OGLE004918.21-732039.3	0.129	16.416	-0.102	-0.011	0.016
OGLE004926.12-731632.5	0.092	15.966	-0.088	0.139	0.114
OGLE004926.81-730601.4	0.067	16.283	-0.047	0.058	0.036
OGLE004935.11-732320.4	0.041	15.91	-0.036	0.06	0.045
OGLE004938.01-730610.0	0.029	14.435	-0.123	0.105	0.082
OGLE004954.54-732114.6	0.101	15.865	-0.053	0.167	0.027
OGLE004954.93-730751.4	0.042	16.667	0.017	0.026	0.031
OGLE005007.91-732910.0	0.055	17.204	-0.049	0.056	0.015
OGLE005010.70-730654.6	0.063	16.451	0.031	0.244	0.056
OGLE005011.50-730652.1	0.164	15.583	-0.131	0.056	0.055
OGLE005014.55-725941.8	0.035	17.038	-0.222	-0.15	0.076
OGLE005038.60-725344.1	0.034	16.681	-0.131	0.004	0.026
OGLE005041.48-724537.7	0.046	15.677	-0.099	0.13	0.063
OGLE005043.72-730147.0	0.157	16.484	0.064	0.303	0.015
OGLE005053.87-724716.6	0.056	16.708	-0.131	-0.047	0.028
OGLE005104.25-730821.9	0.13	17.343	-0.2	0.032	0.123
OGLE005108.72-725623.6	0.058	15.49	-0.087	0.041	0.094
OGLE005108.86-724051.8	0.09	15.475	-0.094	0.034	0.021
OGLE005112.72-731151.1	0.075	18.187	-0.037	0.184	0.023
OGLE005115.43-730803.1	0.057	15.747	0.076	0.299	0.025
OGLE005117.02-730446.8	0.043	15.572	-0.157	0.002	0.024
OGLE005117.54-730254.4	0.06	15.618	-0.204	-0.052	0.049
OGLE005123.29-725756.0	0.155	16.553	-0.014	0.244	0.028
OGLE005130.68-731355.2	0.048	17.308	-0.101	-0.029	0.018
OGLE005131.35-725054.2	0.147	17.983	0.023	0.146	0.106
OGLE005131.37-725054.2	0.092	18.039	0.098	0.177	0.102
OGLE005132.33-725218.2	0.024	16.741	-0.046	0.205	0.027
OGLE005134.85-731843.2	0.135	16.018	-0.149	-0.089	0.017
OGLE005134.86-731843.2	0.012	16.065	-0.197	-0.048	0.021
OGLE005135.29-723237.6	0.108	16.451	-0.241	-0.104	0.035
OGLE005137.19-731429.2	0.068	17.244	0.027	0.275	0.04
OGLE005145.65-724358.3	0.123	16.271	-0.07	0.229	0.111
OGLE005152.30-730904.2	0.682	16.658	-0.104	0.056	0.019
OGLE005156.68-724116.8	0.12	15.866	-0.155	-0.037	0.026
OGLE005206.05-725208.7	0.027	15.961	-0.148	0.054	0.063
OGLE005209.29-731711.6	0.09	15.857	-0.078	-0.024	0.023
OGLE005209.92-731820.4	0.015	15.672	-0.15	-0.156	0.013
OGLE005211.60-730049.1	0.018	17.013	-0.144	-0.139	0.036
OGLE005212.06-723723.4	0.095	15.658	-0.027	0.165	0.056
OGLE005212.34-731008.3	0.128	15.535	-0.09	0.042	0.068
OGLE005212.69-730037.5	0.09	16.02	-0.164	-0.071	0.019
OGLE005222.36-730239.2	0.013	16.423	-0.064	0.155	0.022
OGLE005222.51-731842.7	0.03	15.867	0.042	0.146	0.03
OGLE005224.40-724038.6	0.042	14.032	0.003	0.021	0.26
OGLE005235.39-725050.1	0.251	15.065	-0.052	0.199	0.016
OGLE005237.21-730901.2	0.043	16.955	-0.181	-0.136	0.026
OGLE005241.79-732404.1	0.05	16.262	-0.078	-0.017	0.029
OGLE005243.27-731812.2	0.1	17.522	-0.18	0.041	0.035
OGLE005251.97-723508.5	0.076	14.637	-0.158	0.257	0.073
OGLE005254.57-730648.7	1.213	18.374	-0.088	-0.203	0.05
OGLE005300.82-731638.7	0.169	16.151	-0.071	0.215	0.037
OGLE005310.28-730325.4	0.023	16.041	-0.03	0.106	0.041
OGLE005312.20-724842.9	0.049	16.523	-0.137	0.097	0.047
OGLE005338.91-724026.9	0.182	15.926	-0.045	0.219	0.016
OGLE005339.70-724042.1	0.271	15.091	0.026	0.271	0.027
OGLE005341.39-725253.4	0.042	16.006	-0.033	0.174	0.043
OGLE005341.70-730130.7	0.128	15.254	-0.213	-0.155	0.044
OGLE005342.40-725116.7	0.229	16.947	-0.174	-0.156	0.02
OGLE005348.08-730348.2	0.069	16.557	-0.143	-0.107	0.022
OGLE005352.47-724624.4	0.238	16.399	0.075	0.13	0.027
OGLE005416.84-731147.8	1.114	17.984	-0.2	0.027	0.029
OGLE005427.52-731359.0	0.193	16.633	0.016	0.057	0.014
OGLE005433.24-723211.5	0.181	16.446	-0.101	0.281	0.064
OGLE005440.67-723028.4	0.018	15.312	-0.169	-0.171	0.007
OGLE005453.63-723529.2	0.136	15.377	-0.178	-0.156	0.019
OGLE005506.26-731347.5	0.067	15.739	-0.153	0.047	0.011
OGLE005548.22-731828.4	2.842	18.72	-0.112	-0.144	0.028
OGLE005614.45-724053.2	0.216	14.348	0.295	0.476	0.017
OGLE005618.51-722645.2	0.553	13.912	0.046	0.146	0.005
OGLE005642.51-723508.6	0.05	15.326	-0.152	0.003	0.037
OGLE005705.71-723341.8	0.106	16.14	-0.178	-0.124	0.035
OGLE005727.09-723721.8	0.207	18.007	-0.124	-0.068	0.022
OGLE005729.42-721550.4	0.106	15.439	-0.132	0.143	0.069
OGLE005735.61-721754.9	0.117	16.153	-0.07	0.114	0.05
OGLE005744.30-721610.6	0.053	15.582	-0.161	-0.133	0.011
OGLE005806.05-723544.5	0.099	14.838	-0.007	0.071	0.016
OGLE005844.81-724435.6	0.039	15.919	-0.009	0.246	0.021
OGLE005845.21-723651.9	0.079	15.123	-0.033	0.278	0.016
OGLE005853.13-722023.4	0.065	15.642	0.002	0.199	0.018
OGLE005858.73-725220.9	0.074	14.827	-0.1	0.04	0.035
OGLE005901.96-723911.0	0.154	15.444	0	0.284	0.012
OGLE005912.13-721211.4	0.051	15.824	0.073	0.274	0.017
OGLE005932.85-724358.7	0.061	16.952	-0.12	-0.032	0.022
OGLE005938.00-722734.5	0.162	17.459	-0.217	-0.089	0.047
OGLE010009.17-722159.3	0.08	16.29	-0.005	0.215	0.009
OGLE010025.10-724632.2	0.109	14.704	-0.106	-0.029	0.07
OGLE010027.11-722657.5	0.053	17.743	-0.113	-0.089	0.037
OGLE010055.96-722321.3	0.108	15.787	-0.128	-0.012	0.02
OGLE010149.74-722818.7	0.079	15.849	-0.206	-0.076	0.094
OGLE010156.61-721526.4	0.053	16.265	-0.119	-1E-3	0.021
OGLE010210.38-724422.6	0.031	16.252	-0.101	-0.144	0.007
OGLE010215.48-723557.2	0.056	16.164	-0.051	-0.076	0.031
OGLE010309.31-724553.2	0.274	16.655	-0.059	-0.076	0.019
OGLE010322.56-724950.6	0.427	16.977	-0.099	0.122	0.027
OGLE010337.46-720416.9	0.033	15.179	-0.135	0.074	0.041
OGLE010401.11-723311.1	0.079	13.12	-0.019	0.124	0.013
OGLE010405.20-724334.2	0.128	14.923	-0.021	0.181	0.012
OGLE010415.39-724829.3	0.042	16.422	-0.111	0.145	0.012
OGLE010415.81-722618.8	0.135	14.971	-0.02	0.239	0.013
OGLE010447.25-722559.4	0.222	14.781	-0.084	0.14	0.017
OGLE010450.00-720225.2	0.072	15.42	-0.128	0.064	0.023
OGLE010507.19-722644.3	0.093	15.305	-0.109	0.018	0.012
OGLE010544.48-722807.5	0.082	16.069	-0.186	-0.191	0.019
OGLE010554.27-722841.9	0.084	15.965	-0.077	0.101	0.01
OGLE010642.82-721527.3	0.102	15.736	-0.213	-0.234	0.01
OGLE010649.98-721621.0	0.023	15.034	-0.137	-0.015	0.057
OGLE010720.35-723929.1	0.107	17.247	-0.152	-0.097	0.02
OGLE010743.07-722148.1	0.026	15.199	-0.076	0.204	0.039
OGLE010744.48-722747.1	0.144	16.199	-0.199	-0.101	0.012
OGLE010755.71-723506.9	0.009	15.524	-0.068	0.073	0.077
OGLE010822.18-723716.8	0.035	15.367	-0.164	-0.107	0.04
OGLE010837.86-723021.6	0.089	16.658	-0.113	0.033	0.054

 

Table 5: Type-3 stars.

Star	$\Delta\Phi$	V	B-V	V-I	rms	Time-scale (days)
OGLE003813.22-734144.7	0.291	16.607	-0.045	0.022	0.058	187$\pm$19
OGLE003832.82-734404.2	0.385	17.447	0.448	0.609	0.106	79$\pm$3,MA
OGLE003833.35-731510.1	0.177	16.467	0.019	0.084	0.064	164$\pm$3
OGLE003927.34-733309.6	0.322	15.855	-0.158	0.057	0.055	$\sim$27,ART,MA
OGLE003952.15-730057.7	0.530	18.815	-0.042	0.022	0.077	107$\pm$6,double eclipse?
OGLE004019.36-730402.9	2.172	16.207	-0.033	0.146	0.059	200$\pm$22,VA
OGLE004024.94-734416.1	1.580	16.531	-0.018	0.040	0.010	$\sim$448
OGLE004211.38-732437.7	0.345	17.916	-0.089	0.010	0.058	74$\pm$3
OGLE004212.21-734120.0	0.017	15.921	-0.197	-0.138	0.039	46$\pm$1,alias 1.01932
OGLE004323.84-733930.1	0.636	16.341	-0.190	-0.145	0.016	62$\pm$2,alias 0.98134
OGLE004336.91-732637.7	0.097	14.178	0.181	0.331	0.031	118$\pm$7,MA
OGLE004357.18-732019.9	0.139	16.510	0.386	0.668	0.065	29$\pm$1
OGLE004454.66-732802.9	0.183	14.817	0.286	0.576	0.030	17.37$\pm$0.15,VA
OGLE004517.55-732343.6	0.044	17.513	0.306	0.222	0.094	171$\pm$15
OGLE004541.10-731219.2	0.082	17.149	0.089	0.240	0.032	182$\pm$18
OGLE004541.80-724932.3	0.046	17.252	0.308	0.480	0.206	85$\pm$3
OGLE004554.14-731404.3	0.781	15.483	0.517	0.709	0.010	99$\pm$4,LA
OGLE004633.06-731919.1	0.129	17.150	-0.012	0.181	0.021	38$\pm$1,ART
OGLE004633.76-731204.3	0.092	14.058	0.206	0.385	0.057	184$\pm$18,eclipsing
OGLE004652.03-731423.7	0.084	15.995	-0.069	0.087	0.021	$\sim$567,other 67?
OGLE004653.24-724300.0	0.495	19.469	0.030	0.120	0.166	66$\pm$3
OGLE004702.75-730618.3	0.126	16.570	0.122	0.243	0.016	17.3$\pm$0.15,ART,eclipsing
OGLE004723.53-730347.0	0.110	16.328	-0.043	0.162	0.016	101$\pm$2,ART,eclipsing
OGLE004748.20-731906.1	0.073	18.355	0.194	0.392	0.079	177$\pm$10
OGLE004750.14-731316.4	0.222	15.475	0.269	0.471	0.009	30.0$\pm$0.3,LA
OGLE004816.01-730635.7	0.212	15.917	0.123	0.338	0.040	26.45$\pm$0.20,strange phase curve, also Type-1?
OGLE004833.67-732955.6	0.221	19.403	0.129	0.417	0.140	161$\pm$12
OGLE004843.23-731415.8	0.111	16.736	-0.081	0.066	0.062	$\sim$357,VA
OGLE004849.06-724309.2	0.088	17.588	0.446	0.639	0.108	150$\pm$15,rather time scale
OGLE004921.41-725844.9	3.839	14.614	0.320	0.504	0.020	197$\pm$20
OGLE004940.01-732128.8	0.078	15.891	-0.008	0.110	0.032	58$\pm$2,alias 0.98312
OGLE004942.46-730649.5	0.241	17.396	0.001	0.042	0.027	66$\pm$2,MA,including 0.98236
OGLE005011.61-730504.3	0.060	16.844	-0.032	0.180	0.091	242$\pm$30
OGLE005014.47-724428.6	0.480	16.438	-0.076	0.126	0.023	70$\pm$3,alias,0.98313
OGLE005019.83-730737.1	0.249	17.967	0.169	0.373	0.033	180$\pm$15
OGLE005020.11-724313.3	0.113	17.812	0.026	0.178	0.097	124$\pm$8
OGLE005025.64-725807.1	0.403	14.011	0.291	0.451	0.014	27.32$\pm$0.40
OGLE005043.44-732705.3	0.096	13.650	-0.192	0.013	0.039	62$\pm$2
OGLE005049.20-731356.1	0.070	16.122	-0.041	0.067	0.025	117$\pm$7,ART,alias 1.00574
OGLE005058.52-725656.6	0.041	15.604	-0.007	0.180	0.056	$\sim$617,VA
OGLE005100.18-725303.9	0.131	13.609	-0.028	0.194	0.026	63$\pm$3,ART,VA,MA
OGLE005107.59-732636.6	0.782	15.046	0.015	-0.027	0.016	185$\pm$17,LA
OGLE005117.44-725920.8	0.018	16.315	-0.028	0.159	0.062	264$\pm$40
OGLE005150.78-724521.9	0.148	15.501	-0.001	0.200	0.024	54$\pm$1,MA,including 1.015995
OGLE005201.48-732024.9	0.026	17.821	0.324	0.670	0.129	146$\pm$15,MA
OGLE005206.92-723400.4	0.163	17.130	-0.232	0.118	0.081	40$\pm$1,alias 0.97269
OGLE005214.98-730858.1	1.022	17.763	-0.068	0.030	0.036	$\sim$720,alias 1.00146
OGLE005215.23-725629.4	0.197	16.286	-0.063	0.083	0.031	$\sim$529,alias 1.01997,additionallong-term trend
OGLE005222.57-730326.6	0.512	18.967	0.506	0.699	0.060	69$\pm$2,ART
OGLE005259.82-730154.1	0.087	16.381	-0.023	0.100	0.045	171$\pm$6
OGLE005348.44-730755.2	0.081	17.996	0.108	0.229	0.084	149$\pm$5
OGLE005352.68-731839.3	0.002	16.287	0.420	0.775	0.016	112$\pm$3,strange phase curve
OGLE005356.05-731252.7	0.027	15.916	-0.083	0.179	0.026	72$\pm$3,ART,alias 1.01142
OGLE005359.22-723508.9	0.124	14.400	0.115	0.326	0.023	73$\pm$3
OGLE005411.38-731039.6	0.237	16.165	-0.065	0.109	0.019	89$\pm$2,ART,alias 1.01142
OGLE005419.85-723952.1	0.055	16.372	-0.153	0.008	0.040	124$\pm$8,ART,VA
OGLE005442.38-723521.0	0.020	16.626	-0.132	-0.107	0.076	182$\pm$7,alias 61 or 1.00692
OGLE005513.72-731245.9	0.190	15.434	-0.092	0.079	0.036	67$\pm$2 or 1.012355
OGLE005520.27-723710.1	0.035	14.876	0.190	0.295	0.041	107$\pm$3
OGLE005536.43-731301.9	0.241	17.745	0.079	0.268	0.043	176$\pm$17
OGLE005553.95-730516.3	0.159	17.788	0.011	0.179	0.069	119$\pm$8
OGLE005606.93-730002.5	0.231	16.065	-0.026	0.122	0.063	191$\pm$20
OGLE005702.18-722555.1	0.048	15.838	-0.051	0.134	0.021	$\sim$290,VA,alias 0.99667
OGLE005733.81-731706.5	0.016	17.461	0.356	0.542	0.197	$\sim$50,ChP?
OGLE005745.18-723652.1	0.041	17.518	0.474	0.551	0.173	96$\pm$10,MA,ChP?
OGLE005745.25-723532.1	0.337	13.823	-0.146	-0.148	0.011	26.20$\pm$1,or 13.12$\pm$0.3,ART
OGLE005812.58-723048.5	0.054	14.897	0.061	0.263	0.017	60$\pm$2,ART,periodic outbursts?
OGLE005822.04-722426.5	0.052	15.105	0.038	0.254	0.021	31$\pm$1,ART
OGLE010000.78-725522.9	0.023	14.435	0.045	0.243	0.033	35$\pm$3,ART
OGLE010114.84-724755.9	0.111	15.226	-0.098	0.050	0.036	31$\pm$1,ART,MA
OGLE010325.11-723915.1	0.032	16.672	0.272	0.429	0.078	83$\pm$3,alias,68
OGLE010451.21-724646.9	0.324	13.419	-0.042	0.132	0.016	44$\pm$3
OGLE010452.99-715918.8	0.128	14.224	-0.165	-0.072	0.026	44$\pm$3
OGLE010528.60-722547.0	0.257	15.610	0.217	0.418	0.063	64$\pm$3,eclipsing
OGLE010535.01-724727.5	0.153	17.112	-0.035	0.041	0.046	126$\pm$8
OGLE010619.77-721338.9	0.040	17.484	0.265	0.587	0.177	84$\pm$5,MA
OGLE010844.31-723704.1	0.061	16.948	0.401	0.516	0.235	90$\pm$5,alias 72
OGLE010902.25-723710.1	0.086	16.224	-0.028	-0.067	0.030	60$\pm$1,ART,eclipse-like events

   

Table 6: Type-4 stars.

Star	$\Delta\Phi$	V	B-V	V-I	rms
OGLE003618.14-734624.6	0.086	14.929	0.353	0.779	0.279
OGLE003618.15-734247.4	1.419	16.177	-0.131	-0.001	0.036
OGLE003619.44-732553.1	0.132	19.519	0.258	0.516	0.182
OGLE003621.53-732610.6	0.050	14.741	0.067	0.214	0.124
OGLE003623.02-734651.0	0.016	19.551	0.484	0.531	0.304
OGLE003645.28-733259.7	1.863	15.590	-0.024	0.200	0.015
OGLE003652.74-732857.9	3.222	14.397	0.081	0.177	0.016
OGLE003715.60-734546.0	1.804	16.090	0.453	0.647	0.013
OGLE003726.27-731420.0	0.511	19.630	0.318	0.559	0.250
OGLE003730.99-731112.4	1.965	15.846	0.109	0.209	0.010
OGLE003744.41-730447.6	0.109	16.996	-0.087	-0.051	0.028
OGLE003804.71-735150.5	0.329	19.434	0.009	0.092	0.065
OGLE003810.16-730138.4	1.220	17.296	0.590	0.767	0.020
OGLE003813.77-731340.0	0.208	17.335	-0.081	0.116	0.016
OGLE003817.01-734852.6	0.025	15.199	0.462	0.709	0.280
OGLE003827.69-733314.5	1.499	16.126	-0.156	0.124	0.021
OGLE003833.29-732629.4	1.317	16.725	0.414	0.619	0.011
OGLE003836.25-734813.4	0.303	15.383	-0.140	-0.082	0.022
OGLE003837.66-731158.3	0.093	14.894	-0.085	0.057	0.028
OGLE003859.60-732525.2	0.385	15.405	-0.121	0.090	0.023
OGLE003904.81-735021.5	0.108	15.891	-0.151	-0.088	0.015
OGLE003907.18-732059.3	0.232	15.567	0.365	0.549	0.006
OGLE003915.99-734111.2	0.701	14.126	0.016	0.164	0.010
OGLE003917.62-733806.6	0.948	16.748	-0.083	0.023	0.036
OGLE003922.07-732531.6	0.170	16.942	0.106	-0.234	0.026
OGLE003940.84-732601.1	0.199	15.268	-0.056	0.111	0.035
OGLE004001.52-734112.6	0.296	17.708	-0.163	-0.139	0.064
OGLE004003.31-733722.5	0.379	16.013	-0.118	-0.147	0.022
OGLE004005.89-730410.7	1.746	15.755	0.110	0.304	0.021
OGLE004008.41-733710.1	0.675	17.375	-0.124	-0.103	0.028
OGLE004028.10-733233.0	0.055	14.992	0.027	0.230	0.013
OGLE004043.55-732059.1	1.568	18.542	0.530	0.761	0.027
OGLE004043.88-732422.9	0.069	15.275	-0.046	0.138	0.019
OGLE004044.77-732307.5	0.110	16.925	-0.158	-0.017	0.031
OGLE004049.32-732522.9	0.238	17.696	-0.151	-0.082	0.062
OGLE004101.34-734006.9	0.102	16.453	-0.018	0.203	0.014
OGLE004109.12-730646.7	0.126	17.769	-0.063	0.044	0.030
OGLE004111.34-734118.3	0.515	16.708	-0.056	0.112	0.009
OGLE004140.28-734424.6	1.224	17.818	-0.118	-0.090	0.015
OGLE004141.80-734129.3	0.886	16.294	-0.034	-0.182	0.012
OGLE004144.34-733957.1	0.711	17.609	0.584	0.769	0.015
OGLE004154.09-730916.3	0.177	17.784	-0.094	0.080	0.019
OGLE004157.28-734133.3	0.486	17.430	-0.116	0.013	0.017
OGLE004207.95-733653.7	1.128	16.162	-0.133	-0.158	0.014
OGLE004209.92-731356.2	0.234	14.732	-0.185	-0.226	0.016
OGLE004212.32-732312.1	0.010	15.272	-0.072	0.102	0.025
OGLE004214.49-731644.4	0.724	19.401	0.249	0.418	0.152
OGLE004218.06-731809.5	0.259	16.616	-0.004	0.229	0.012
OGLE004218.81-732708.4	0.033	16.045	-0.143	-0.024	0.094
OGLE004221.87-732417.1	0.038	16.158	0.402	0.669	0.056
OGLE004222.70-732335.8	2.067	19.548	0.355	0.607	0.034
OGLE004222.72-732627.9	0.212	18.761	-0.123	-0.097	0.052
OGLE004224.08-730543.4	0.437	16.546	0.555	0.723	0.017
OGLE004224.64-731658.7	0.166	15.880	-0.078	0.127	0.021
OGLE004237.76-725918.3	0.120	16.465	0.034	-0.039	0.054
OGLE004241.20-732910.9	0.030	16.228	-0.038	0.174	0.025
OGLE004244.55-732610.1	0.669	15.759	-0.175	-0.141	0.017
OGLE004245.62-724628.0	0.589	19.663	-0.097	0.026	0.177
OGLE004245.90-733026.6	0.232	17.794	-0.085	0.042	0.022
OGLE004310.22-733430.7	0.032	15.650	-0.090	0.159	0.035
OGLE004323.41-732731.8	0.116	16.231	-0.038	0.140	0.015
OGLE004326.75-730709.8	1.043	19.566	0.127	0.201	0.052
OGLE004327.84-732432.4	0.053	15.807	-0.064	0.087	0.020
OGLE004329.13-732216.4	3.723	19.081	-0.055	-0.024	0.036
OGLE004335.78-732737.3	0.034	15.586	-0.044	0.190	0.015
OGLE004336.13-731032.0	0.088	16.037	0.045	0.348	0.019
OGLE004339.05-732217.8	0.070	14.981	0.026	0.239	0.010
OGLE004349.56-733906.3	0.076	16.431	-0.128	0.048	0.038
OGLE004350.54-733141.2	0.390	19.690	0.508	0.604	0.259
OGLE004354.74-725803.3	1.156	19.615	0.153	0.163	0.084
OGLE004355.02-732725.6	0.230	16.007	-0.079	0.086	0.058
OGLE004357.34-732419.1	0.257	15.796	-0.115	-0.101	0.017
OGLE004404.12-731105.7	0.024	16.961	0.048	-0.225	0.034
OGLE004417.11-733225.0	1.462	16.540	0.449	0.661	0.010
OGLE004419.56-731659.3	0.449	16.813	0.057	0.239	0.014
OGLE004420.14-732913.8	1.467	16.474	-0.007	0.232	0.012
OGLE004433.70-732215.9	0.080	16.465	0.039	0.290	0.015
OGLE004441.11-731256.1	0.076	16.553	-0.037	0.168	0.022
OGLE004443.16-733128.8	0.438	17.637	0.013	0.004	0.050
OGLE004454.05-732323.1	0.099	17.572	0.026	0.246	0.030
OGLE004456.28-732256.2	0.183	14.660	0.036	0.305	0.027
OGLE004456.96-731938.0	0.059	16.318	0.096	0.357	0.025
OGLE004457.11-730046.6	0.075	14.379	-0.041	0.250	0.037
OGLE004502.90-732225.8	1.938	19.444	-0.011	0.098	0.038
OGLE004503.33-733831.7	0.066	14.808	0.067	0.246	0.027
OGLE004505.83-732311.7	0.125	13.860	-0.036	0.034	0.012
OGLE004509.37-730926.7	0.284	16.303	-0.060	0.090	0.012
OGLE004515.21-731734.3	0.649	16.501	-0.027	0.234	0.012
OGLE004518.91-731707.2	0.096	15.390	-0.049	0.142	0.013
OGLE004521.22-732147.0	1.010	16.092	-0.057	0.020	0.008
OGLE004522.49-732811.1	0.196	15.443	0.003	0.304	0.020
OGLE004522.52-732811.1	0.212	15.492	0.079	0.324	0.050
OGLE004524.92-733159.3	1.674	16.001	-0.182	-0.046	0.043
OGLE004525.64-731629.5	0.158	17.395	0.260	0.138	0.021
OGLE004526.51-733014.2	1.331	16.883	0.907	1.092	0.034
OGLE004530.65-730512.4	1.788	16.161	0.570	0.784	0.034
OGLE004532.16-731601.8	0.499	15.971	0.029	0.306	0.015
OGLE004533.00-732909.2	0.612	16.485	-0.154	-0.186	0.016
OGLE004535.82-731412.2	0.445	13.044	-0.066	0.019	0.021
OGLE004543.60-731202.1	0.254	19.524	0.089	0.071	0.071
OGLE004545.92-731412.7	0.130	17.163	-0.062	0.058	0.024
OGLE004551.19-731157.0	0.071	17.130	0.179	0.439	0.015
OGLE004551.65-730733.1	0.293	16.968	-0.039	0.230	0.046
OGLE004553.80-730754.7	0.222	14.970	-0.012	0.043	0.023
OGLE004555.11-731134.4	0.091	17.549	0.283	0.396	0.038
OGLE004555.92-733336.5	0.271	18.253	-0.124	-0.144	0.017
OGLE004604.42-732640.7	0.213	16.403	-0.067	0.006	0.015
OGLE004614.24-724305.8	0.643	15.455	0.122	0.262	0.019
OGLE004617.21-725439.7	0.423	16.758	-0.090	0.069	0.015
OGLE004618.42-731650.8	1.163	19.600	0.003	0.451	0.226
OGLE004619.23-731945.7	0.246	17.923	-0.008	0.097	0.024
OGLE004628.33-732742.8	0.053	15.043	0.068	0.284	0.017
OGLE004631.22-730055.8	0.432	16.848	-0.031	0.164	0.024
OGLE004638.24-731109.0	0.228	16.723	0.056	0.330	0.017
OGLE004651.14-732300.3	0.101	16.229	0.078	0.362	0.016
OGLE004653.27-733325.3	0.129	17.109	0.096	0.355	0.015
OGLE004700.00-731705.6	1.049	15.834	0.138	0.415	0.019
OGLE004701.81-731650.6	0.111	17.852	0.118	0.210	0.023
OGLE004702.72-732821.0	0.873	17.164	0.394	0.687	0.036
OGLE004702.90-730800.9	0.469	18.036	0.469	0.689	0.089
OGLE004704.02-731917.1	0.078	16.250	0.160	0.421	0.012
OGLE004705.03-730611.6	0.319	17.285	0.047	0.312	0.025
OGLE004708.64-731711.0	0.112	16.581	-0.002	0.123	0.011
OGLE004710.45-732817.5	0.018	14.990	0.222	0.534	0.020
OGLE004711.52-730756.4	0.135	14.316	-0.108	-0.031	0.013
OGLE004712.08-730731.4	0.165	17.149	0.064	0.309	0.019
OGLE004712.59-730754.4	3.545	19.217	0.065	0.085	0.072
OGLE004714.28-731717.2	0.488	16.198	0.033	0.224	0.016
OGLE004714.57-731122.7	0.401	16.672	0.007	0.205	0.011
OGLE004718.13-731907.5	0.086	17.602	0.086	0.355	0.026
OGLE004719.44-730454.1	0.028	17.073	0.161	0.419	0.015
OGLE004719.95-724111.3	0.012	16.935	-0.106	-0.077	0.011
OGLE004721.29-731818.3	0.071	16.225	-0.019	0.170	0.013
OGLE004721.78-730214.5	0.071	15.965	-0.001	0.233	0.006
OGLE004722.13-730844.4	0.199	17.680	0.052	0.216	0.019
OGLE004723.21-732854.2	0.032	16.426	-0.080	0.038	0.016
OGLE004723.37-731226.9	0.329	16.139	-0.038	0.135	0.010
OGLE004736.84-733428.3	0.056	16.034	-0.089	0.025	0.010
OGLE004737.20-730804.4	0.119	15.228	-0.119	-0.015	0.027
OGLE004738.42-725751.5	0.258	16.489	-0.078	-0.029	0.014
OGLE004738.73-731911.7	0.440	16.927	-0.051	0.042	0.021
OGLE004741.62-730208.1	1.478	14.866	-0.176	-0.157	0.008
OGLE004743.68-731630.1	0.271	17.532	0.133	0.321	0.012
OGLE004746.42-732547.1	0.419	16.293	-0.039	0.157	0.013
OGLE004748.98-731633.1	0.036	14.776	0.000	0.147	0.018
OGLE004750.12-731329.6	0.168	17.769	0.040	0.238	0.027
OGLE004750.78-730851.8	0.001	14.054	-0.019	0.186	0.010
OGLE004754.90-731312.1	0.153	15.847	-0.026	0.097	0.021
OGLE004756.19-725648.2	0.105	17.257	-0.052	0.001	0.026
OGLE004758.43-724949.7	2.498	19.428	0.034	0.135	0.053
OGLE004758.57-732109.3	0.093	15.286	-0.008	0.208	0.009
OGLE004759.69-730734.9	0.206	15.213	0.165	0.476	0.030
OGLE004805.16-731203.1	0.131	14.406	-0.055	0.131	0.031
OGLE004808.84-732209.7	0.168	15.961	-0.055	0.131	0.010
OGLE004812.18-730230.5	0.279	17.249	-0.081	0.006	0.016
OGLE004813.94-730303.1	0.084	17.365	0.024	0.251	0.020
OGLE004814.13-731003.5	0.021	15.743	0.001	0.070	0.040
OGLE004815.41-731112.2	0.045	16.569	-0.051	0.103	0.010
OGLE004818.25-731242.8	0.102	17.446	0.047	0.252	0.013
OGLE004818.96-731458.7	0.268	13.147	-0.011	0.042	0.024
OGLE004820.54-725107.9	0.036	14.244	0.137	0.337	0.045
OGLE004820.99-732110.0	0.229	15.611	0.084	0.359	0.011
OGLE004823.33-724348.7	0.159	13.963	-0.056	0.206	0.014
OGLE004827.42-731456.9	0.228	16.422	-0.098	0.070	0.036
OGLE004827.80-731140.8	4.868	19.687	0.061	0.086	0.052
OGLE004828.13-732022.7	0.216	16.613	-0.119	-0.080	0.025
OGLE004830.29-730629.1	0.196	15.984	-0.008	0.155	0.020
OGLE004830.55-725547.1	0.193	14.541	-0.301	0.161	0.147
OGLE004830.58-725547.1	0.113	14.306	-0.149	-0.036	0.036
OGLE004830.85-731545.5	0.153	14.421	-0.205	-0.088	0.041
OGLE004830.86-731545.3	0.121	14.418	-0.188	-0.061	0.026
OGLE004832.20-724558.6	0.075	17.564	-0.084	-0.024	0.030
OGLE004832.56-731412.6	0.279	17.878	0.071	0.528	0.105
OGLE004833.39-731623.7	0.107	17.147	-0.052	0.124	0.045
OGLE004833.42-731623.6	0.317	17.126	-0.023	0.195	0.032
OGLE004833.68-732955.6	0.202	19.409	0.151	0.419	0.138
OGLE004834.01-725009.2	1.220	16.796	0.464	0.640	0.029
OGLE004834.12-730230.9	0.074	15.108	-0.229	0.275	0.120
OGLE004834.13-730230.8	0.200	14.947	-0.089	0.138	0.037
OGLE004834.79-730652.7	0.082	14.989	-0.186	-0.150	0.163
OGLE004834.85-731753.4	0.066	15.030	0.049	0.326	0.027
OGLE004836.66-730000.8	0.080	16.309	-0.064	0.074	0.020
OGLE004838.16-731447.1	0.051	13.565	0.138	0.196	0.037
OGLE004848.91-732021.9	0.209	16.423	-0.088	-0.032	0.026
OGLE004849.34-731624.0	0.116	14.530	-0.015	0.178	0.025
OGLE004853.15-732019.8	0.079	16.127	-0.140	-0.045	0.015
OGLE004855.30-731807.5	0.254	16.020	-0.021	-0.021	0.006
OGLE004855.44-730301.6	0.035	16.514	0.063	0.232	0.011
OGLE004857.01-725729.5	0.118	17.210	-0.024	0.057	0.032
OGLE004857.42-725350.8	0.239	17.031	0.010	0.173	0.025
OGLE004857.93-725342.8	1.110	16.383	0.049	0.317	0.037
OGLE004858.20-730126.1	0.156	17.009	-0.020	0.113	0.044
OGLE004859.50-732325.1	0.247	15.443	-0.030	0.149	0.019
OGLE004900.05-730605.2	0.099	16.433	-0.102	0.444	0.184
OGLE004900.93-731330.0	0.149	17.192	-0.103	-0.110	0.014
OGLE004901.85-732202.4	0.126	15.920	-0.143	0.000	0.024
OGLE004901.99-730617.4	0.013	15.079	0.104	0.245	0.020
OGLE004902.43-731741.5	0.274	17.039	-0.048	0.055	0.010
OGLE004903.35-725052.1	0.150	16.936	0.085	0.223	0.059
OGLE004904.76-732114.2	0.044	16.037	-0.084	0.013	0.016
OGLE004905.46-731059.7	0.065	15.655	-0.002	0.161	0.034
OGLE004905.88-730257.5	0.155	17.973	0.028	0.139	0.061
OGLE004907.62-725220.8	1.090	16.979	0.551	0.670	0.016
OGLE004909.38-730352.3	0.103	16.653	-0.043	-0.045	0.018
OGLE004913.03-725917.4	0.478	15.535	0.038	0.274	0.024
OGLE004913.65-731137.4	0.133	16.517	0.097	0.292	0.019
OGLE004914.30-733007.9	0.535	15.737	-0.072	-0.080	0.020
OGLE004915.62-731210.4	0.632	13.321	0.173	0.328	0.023
OGLE004917.94-731736.2	0.286	15.719	-0.141	-0.148	0.015
OGLE004918.90-725202.5	1.405	16.658	-0.086	-0.047	0.022
OGLE004921.94-730710.1	0.100	17.321	0.143	0.316	0.022
OGLE004922.76-731805.8	0.167	16.565	-0.073	-0.027	0.031
OGLE004925.12-730610.0	2.623	18.249	-0.016	0.020	0.026
OGLE004930.26-732427.3	0.351	16.666	-0.026	0.132	0.015
OGLE004930.32-730831.4	0.165	16.411	0.090	0.334	0.022
OGLE004930.40-731857.8	0.129	16.421	0.053	0.226	0.027
OGLE004930.52-733108.8	0.127	14.655	-0.055	0.155	0.019
OGLE004931.88-731133.1	0.358	17.358	-0.064	-0.014	0.045
OGLE004932.55-731621.1	0.299	16.144	-0.173	-0.143	0.027
OGLE004932.61-731340.2	0.102	15.850	0.028	0.256	0.012
OGLE004940.71-732727.0	0.007	16.604	0.196	0.387	0.100
OGLE004942.47-730350.5	0.131	17.005	-0.069	-0.005	0.038
OGLE004942.68-725843.0	0.081	19.447	-0.288	0.649	0.299
OGLE004942.75-731717.7	0.056	14.453	-0.115	0.049	0.040
OGLE004947.32-730130.1	0.121	17.196	-0.104	-0.014	0.031
OGLE004947.99-732053.7	0.174	16.161	-0.083	0.102	0.118
OGLE004948.59-724835.0	0.977	15.606	-0.201	-0.120	0.031
OGLE004948.98-732636.1	0.302	16.984	-0.012	0.223	0.022
OGLE004955.63-730734.9	0.053	14.648	-0.080	0.097	0.093
OGLE004957.03-725007.7	0.173	16.630	-0.066	0.069	0.216
OGLE005002.60-731515.2	0.098	15.158	-0.087	0.121	0.048
OGLE005003.91-732413.2	0.088	14.050	-0.134	-0.037	0.029
OGLE005009.08-731905.6	0.246	16.386	-0.100	0.098	0.013
OGLE005009.11-731559.5	0.122	15.676	-0.130	-0.067	0.024
OGLE005009.75-731759.7	0.130	17.313	-0.040	0.080	0.012
OGLE005011.93-730931.1	0.356	17.088	-0.059	0.058	0.016
OGLE005012.43-731156.0	0.184	15.447	0.075	0.348	0.028
OGLE005014.51-732038.2	0.046	14.813	0.051	0.257	0.019
OGLE005015.42-730431.4	0.017	16.820	-0.040	0.331	0.054
OGLE005016.15-731707.8	0.929	16.838	-0.155	-0.076	0.024
OGLE005016.39-730707.2	0.314	14.459	0.248	0.045	0.022
OGLE005017.10-730036.7	0.061	17.192	-0.163	-0.120	0.048
OGLE005017.35-731356.0	0.133	17.135	0.066	0.375	0.039
OGLE005019.78-731552.5	0.463	17.521	-0.065	0.137	0.029
OGLE005021.17-730443.4	2.716	14.808	0.433	0.735	0.033
OGLE005022.74-732246.1	2.783	19.692	0.131	0.351	0.069
OGLE005024.32-732546.8	0.101	15.177	-0.024	0.114	0.025
OGLE005026.09-733219.7	1.181	16.518	0.499	0.703	0.010
OGLE005026.27-731934.9	0.101	15.087	-0.017	0.061	0.032
OGLE005026.82-731709.3	0.207	16.649	0.027	0.283	0.011
OGLE005027.22-733021.2	0.116	14.119	0.027	0.251	0.021
OGLE005027.44-731842.3	0.220	18.035	-0.111	-0.051	0.138
OGLE005031.87-731021.4	1.569	15.835	-0.177	-0.128	0.013
OGLE005033.63-725159.8	0.059	17.116	-0.270	0.376	0.155
OGLE005034.47-730729.9	0.197	13.259	-0.050	0.148	0.053
OGLE005034.81-731959.4	0.170	16.038	-0.155	-0.106	0.023
OGLE005042.16-724141.3	0.248	16.197	-0.037	0.173	0.014
OGLE005043.41-731646.8	0.118	16.513	-0.094	0.051	0.017
OGLE005045.99-724200.9	0.531	17.272	-0.122	-0.040	0.010
OGLE005045.99-730143.9	0.468	16.700	-0.055	0.037	0.021
OGLE005046.48-730807.3	0.117	13.807	0.097	0.291	0.044
OGLE005047.63-733238.4	0.090	15.644	0.001	0.180	0.026
OGLE005047.75-731812.6	0.078	15.769	0.018	0.242	0.029
OGLE005047.96-724119.0	0.131	15.915	0.052	0.141	0.017
OGLE005048.00-731817.6	0.173	15.303	0.049	0.216	0.070
OGLE005049.01-732332.8	0.300	17.372	0.129	0.107	0.082
OGLE005049.43-730445.2	0.085	15.769	-0.165	0.039	0.052
OGLE005049.77-730504.7	0.304	18.075	-0.118	0.095	0.069
OGLE005052.39-730822.4	0.163	15.780	-0.169	0.032	0.048
OGLE005053.26-724533.3	0.376	16.938	-0.080	0.026	0.014
OGLE005055.20-724853.3	0.094	15.609	0.174	0.391	0.042
OGLE005055.43-724851.5	0.056	16.273	0.030	0.223	0.056
OGLE005055.48-724655.3	0.053	16.184	-0.081	0.200	0.050
OGLE005055.72-731500.6	0.064	15.691	0.063	0.254	0.013
OGLE005056.48-730919.0	0.096	16.170	-0.036	0.244	0.012
OGLE005058.00-731357.0	0.072	19.410	0.256	0.588	0.102
OGLE005058.72-724545.2	0.223	14.397	-0.047	0.164	0.022
OGLE005059.66-731719.9	0.169	15.169	0.019	0.309	0.014
OGLE005104.25-725745.2	0.046	15.963	-0.009	0.268	0.018
OGLE005105.11-724809.6	1.470	15.716	-0.216	-0.170	0.013
OGLE005106.33-724500.3	0.121	17.686	-0.203	-0.017	0.041
OGLE005107.55-724406.5	0.052	14.650	0.012	0.241	0.042
OGLE005107.60-725845.5	1.316	16.315	-0.012	0.257	0.020
OGLE005109.18-731809.3	0.187	14.878	-0.027	0.186	0.013
OGLE005109.37-725448.5	0.065	15.563	-0.018	0.338	0.061
OGLE005109.63-731750.1	0.036	16.829	-0.117	-0.006	0.035
OGLE005110.02-731645.0	1.213	16.137	-0.147	-0.111	0.012
OGLE005110.73-724221.4	0.095	16.495	-0.142	0.063	0.024
OGLE005111.66-725619.4	0.563	16.747	-0.307	0.292	0.168
OGLE005113.04-730455.4	0.057	17.072	-0.047	0.178	0.037
OGLE005113.73-731937.9	0.313	16.039	-0.197	-0.136	0.020
OGLE005115.37-725740.9	1.248	19.108	-0.368	0.088	0.175
OGLE005117.09-731606.4	0.109	15.226	-0.008	0.285	0.017
OGLE005118.81-730547.8	0.037	14.728	-0.021	0.213	0.027
OGLE005119.57-731327.7	1.405	18.826	0.388	0.134	0.321
OGLE005119.96-724533.1	1.031	16.866	0.015	0.226	0.031
OGLE005122.47-733041.2	0.736	18.707	-0.117	-0.157	0.026
OGLE005126.81-725655.9	0.103	15.027	-0.058	0.207	0.043
OGLE005126.83-725907.7	0.810	19.614	0.038	-0.005	0.056
OGLE005127.13-725740.9	0.077	17.028	-0.034	0.212	0.028
OGLE005127.14-725741.0	0.033	16.995	-0.051	0.134	0.019
OGLE005129.21-725146.5	0.126	16.675	0.267	0.729	0.108
OGLE005132.13-733437.3	0.485	17.966	-0.045	-0.018	0.033
OGLE005133.43-730122.6	1.456	17.393	-0.101	0.037	0.029
OGLE005135.55-725646.9	0.137	15.759	-0.036	0.180	0.035
OGLE005135.82-731430.3	0.616	16.375	0.039	0.279	0.011
OGLE005136.59-732016.4	0.064	18.036	0.311	0.794	0.120
OGLE005136.90-725445.9	3.085	14.697	0.167	0.358	0.026
OGLE005137.18-731429.2	0.113	17.221	0.018	0.248	0.039
OGLE005138.11-733229.3	0.280	17.228	-0.139	0.243	0.065
OGLE005138.94-732003.5	1.662	15.327	-0.162	-0.123	0.033
OGLE005139.07-725252.0	0.395	16.690	-0.016	0.173	0.012
OGLE005139.29-724430.8	0.314	15.163	-0.004	-0.007	0.031
OGLE005142.24-725548.1	0.060	15.764	0.037	0.214	0.037
OGLE005142.87-732007.3	0.187	15.960	0.025	0.228	0.031
OGLE005144.12-731428.5	0.123	17.019	-0.031	0.091	0.018
OGLE005146.57-730621.5	0.053	16.425	-0.072	0.071	0.023
OGLE005149.97-731708.7	0.767	15.920	-0.117	-0.013	0.026
OGLE005150.13-724136.3	0.269	16.714	-0.189	-0.075	0.077
OGLE005152.02-731033.7	0.089	14.476	-0.076	0.069	0.018
OGLE005153.12-723148.3	0.050	14.898	-0.270	-0.059	0.119
OGLE005154.02-732010.8	0.695	15.971	-0.023	0.167	0.019
OGLE005155.59-725932.1	1.394	18.222	-0.104	-0.080	0.069
OGLE005155.80-725657.9	0.951	15.703	-0.030	0.272	0.026
OGLE005155.87-723203.2	0.075	13.933	-0.133	-0.030	0.016
OGLE005156.53-730457.3	0.079	16.739	-0.008	0.175	0.018
OGLE005157.74-731421.5	0.111	17.331	0.162	0.535	0.046
OGLE005158.21-731749.9	0.073	15.187	-0.117	-0.114	0.025
OGLE005159.19-730956.3	0.105	15.920	-0.029	0.152	0.024
OGLE005159.89-723510.7	0.094	16.535	0.049	0.220	0.034
OGLE005203.69-730821.1	0.126	16.550	-0.185	-0.064	0.040
OGLE005203.76-731411.5	0.460	16.393	-0.055	0.493	0.196
OGLE005204.57-731234.1	0.165	15.561	0.054	0.251	0.013
OGLE005205.23-732318.4	0.322	16.478	0.061	-0.011	0.022
OGLE005205.91-730424.9	0.118	13.904	0.065	0.280	0.022
OGLE005206.43-730629.0	0.061	13.983	0.217	0.263	0.065
OGLE005206.56-724946.6	0.085	14.868	-0.156	-0.113	0.029
OGLE005207.23-723537.2	0.858	15.816	-0.223	-0.195	0.015
OGLE005208.17-724150.1	0.087	16.253	-0.046	0.081	0.016
OGLE005208.86-731622.3	0.891	16.934	0.588	0.702	0.015
OGLE005208.95-723802.9	0.082	15.033	0.137	0.290	0.020
OGLE005213.99-731918.3	0.054	14.671	-0.005	0.137	0.043
OGLE005214.15-731638.1	0.079	16.153	-0.128	0.035	0.040
OGLE005215.50-724551.6	0.099	14.683	-0.024	-0.057	0.047
OGLE005216.56-731133.4	0.295	17.001	-0.198	-0.134	0.019
OGLE005216.98-731037.4	0.746	16.975	-0.057	0.089	0.014
OGLE005220.55-732534.6	0.403	17.471	-0.125	-0.074	0.016
OGLE005222.68-731219.3	0.106	16.206	-0.067	0.009	0.036
OGLE005222.89-730252.5	0.135	17.091	-0.075	0.028	0.025
OGLE005223.24-724709.0	0.038	15.012	0.028	0.113	0.229
OGLE005223.57-731917.4	0.075	15.850	0.023	0.318	0.022
OGLE005228.37-724753.4	0.128	16.262	-0.036	0.168	0.024
OGLE005228.58-723926.2	0.181	16.031	-0.038	0.078	0.016
OGLE005228.85-725159.2	0.851	16.309	-0.027	0.219	0.023
OGLE005229.34-730434.1	0.489	16.951	-0.093	0.174	0.084
OGLE005232.40-732424.4	0.646	15.515	-0.123	-0.084	0.020
OGLE005232.84-731941.6	0.306	15.346	-0.094	0.188	0.065
OGLE005234.68-724548.5	0.086	14.306	-0.055	0.145	0.038
OGLE005237.00-730420.8	0.106	16.209	-0.081	0.096	0.016
OGLE005238.44-731037.3	0.110	16.129	-0.117	-0.073	0.102
OGLE005238.71-725635.1	0.249	15.574	-0.044	0.185	0.021
OGLE005245.80-731836.3	0.034	15.130	-0.098	0.234	0.102
OGLE005246.38-724244.2	0.164	14.130	-0.082	0.207	0.048
OGLE005252.28-724829.8	0.037	14.416	-0.105	0.166	0.048
OGLE005253.15-725614.6	0.237	16.770	-0.204	0.106	0.055
OGLE005253.18-724955.5	0.006	17.616	-0.144	0.027	0.031
OGLE005254.68-730315.3	0.056	15.894	-0.014	0.205	0.051
OGLE005255.05-731505.3	0.015	15.777	-0.073	0.040	0.013
OGLE005256.87-731358.3	2.936	16.915	0.396	0.691	0.030
OGLE005257.65-725708.9	0.106	15.964	-0.039	0.165	0.040
OGLE005258.65-730218.4	0.140	15.119	-0.036	0.132	0.016
OGLE005259.91-731436.0	0.053	16.692	0.125	0.467	0.024
OGLE005300.73-724305.2	1.533	15.647	-0.183	-0.102	0.016
OGLE005301.29-725132.9	0.055	15.920	-0.108	0.008	0.041
OGLE005301.95-730053.0	0.056	16.157	-0.133	0.092	0.019
OGLE005306.41-723108.9	1.032	16.983	-0.215	-0.068	0.056
OGLE005307.38-723730.3	0.099	15.708	-0.214	0.093	0.085
OGLE005310.17-725248.0	1.958	19.556	-0.385	0.549	0.289
OGLE005311.24-723933.9	0.275	15.357	-0.093	0.246	0.045
OGLE005314.03-725958.6	0.123	16.779	-0.094	0.133	0.015
OGLE005316.80-724219.9	0.221	19.263	0.168	0.402	0.083
OGLE005317.30-724546.5	1.915	19.694	0.012	0.169	0.104
OGLE005318.29-724834.0	0.352	19.173	0.108	0.685	0.222
OGLE005318.32-730222.1	1.392	16.748	-0.105	0.064	0.025
OGLE005329.27-731847.7	1.314	16.655	-0.241	0.007	0.076
OGLE005334.72-724334.2	0.398	15.339	-0.017	0.262	0.022
OGLE005334.81-723923.1	0.110	16.869	0.314	0.503	0.076
OGLE005334.97-723245.5	0.626	14.982	0.224	0.524	0.036
OGLE005335.95-724122.2	2.008	15.344	-0.238	-0.188	0.018
OGLE005339.54-724549.2	0.052	16.441	-0.085	0.065	0.016
OGLE005341.12-724142.4	0.084	16.213	-0.085	0.188	0.065
OGLE005342.13-731642.7	0.123	19.608	0.396	0.452	0.368
OGLE005342.19-725309.4	0.112	14.737	-0.042	0.277	0.059
OGLE005343.83-724521.7	0.120	15.213	-0.138	0.058	0.047
OGLE005344.05-730802.5	0.369	16.615	-0.115	0.104	0.034
OGLE005344.55-731236.9	0.120	14.496	-0.044	0.154	0.019
OGLE005347.99-723341.1	0.078	15.076	-0.071	0.128	0.026
OGLE005349.66-723859.7	0.400	14.707	0.031	0.224	0.027
OGLE005356.02-724557.0	0.069	16.004	-0.171	0.028	0.035
OGLE005357.76-731606.3	1.103	17.232	-0.147	0.658	0.133
OGLE005401.58-730003.5	0.314	16.950	-0.049	0.150	0.019
OGLE005402.30-725443.5	0.055	16.417	-0.147	-0.038	0.023
OGLE005402.41-724446.5	0.079	17.771	-0.203	0.161	0.102
OGLE005405.24-723638.9	0.105	16.231	-0.141	0.049	0.025
OGLE005414.02-731809.2	1.845	17.236	0.522	0.726	0.014
OGLE005415.70-731739.2	0.039	16.036	0.159	0.514	0.029
OGLE005418.94-723737.7	0.291	18.137	0.056	0.243	0.034
OGLE005424.42-723904.2	0.143	19.494	0.131	0.226	0.132
OGLE005425.25-731257.2	0.051	16.420	-0.131	0.080	0.028
OGLE005426.26-731822.7	2.314	19.594	-0.022	0.060	0.055
OGLE005432.80-724239.3	0.058	15.560	-0.099	0.203	0.019
OGLE005433.66-725115.9	2.650	19.659	0.093	0.114	0.088
OGLE005436.27-724655.0	0.085	16.084	0.043	0.327	0.023
OGLE005437.52-724710.5	0.141	17.105	-0.012	0.134	0.017
OGLE005437.57-730456.6	0.019	15.177	-0.049	0.111	0.035
OGLE005438.09-722554.2	2.634	19.621	0.073	0.112	0.074
OGLE005439.15-722923.0	0.039	14.398	-0.012	0.209	0.023
OGLE005439.20-725917.3	0.260	16.656	-0.089	-0.027	0.024
OGLE005440.37-724849.5	0.087	16.149	-0.129	-0.113	0.022
OGLE005442.28-723919.8	0.326	19.602	0.071	0.456	0.059
OGLE005444.01-722748.9	0.148	14.891	-0.149	-0.081	0.023
OGLE005447.39-722758.5	0.040	16.707	-0.098	-0.056	0.021
OGLE005448.97-722544.5	0.300	19.001	0.177	0.737	0.095
OGLE005450.12-724528.4	0.057	16.265	0.004	0.229	0.027
OGLE005451.22-730844.4	0.049	17.064	-0.145	-0.102	0.030
OGLE005456.17-722647.6	0.038	15.301	-0.044	0.129	0.014
OGLE005457.54-731458.6	0.178	16.784	-0.071	0.057	0.017
OGLE005457.89-731146.6	0.210	16.036	-0.090	0.052	0.010
OGLE005505.12-732011.8	0.158	14.957	0.071	0.188	0.018
OGLE005511.90-731329.4	0.716	17.209	-0.059	-0.102	0.031
OGLE005512.69-723626.1	0.278	17.504	-0.114	-0.043	0.019
OGLE005514.22-722628.2	0.186	15.902	-0.069	0.188	0.053
OGLE005516.02-731100.1	1.593	13.979	0.536	0.714	0.014
OGLE005517.86-730435.3	0.084	15.507	-0.039	0.112	0.013
OGLE005520.93-730748.0	0.091	16.069	-0.130	0.012	0.028
OGLE005520.95-723342.6	0.042	15.257	-0.087	0.003	0.018
OGLE005521.02-731509.6	1.671	16.588	-0.094	0.098	0.018
OGLE005523.34-723009.8	0.797	15.701	-0.164	-0.148	0.010
OGLE005524.33-725336.8	0.180	19.477	0.140	0.342	0.285
OGLE005525.38-722957.0	1.389	16.228	-0.084	0.070	0.008
OGLE005525.99-731847.4	0.551	14.505	0.593	0.733	0.007
OGLE005531.74-723023.7	0.031	15.029	-0.056	0.103	0.009
OGLE005533.66-723839.7	0.122	16.178	-0.047	0.118	0.017
OGLE005535.14-722906.4	0.130	14.689	-0.046	0.106	0.012
OGLE005535.78-731747.3	0.211	15.996	-0.147	-0.123	0.011
OGLE005537.35-723603.3	0.104	15.797	-0.045	0.130	0.013
OGLE005539.39-731748.4	0.475	16.121	-0.123	-0.097	0.019
OGLE005540.16-722641.6	0.339	16.501	-0.035	0.181	0.009
OGLE005542.42-731730.2	0.146	14.048	-0.208	-0.195	0.010
OGLE005545.39-725555.5	0.184	15.295	-0.024	0.168	0.015
OGLE005546.37-730307.8	0.082	16.652	-0.059	0.021	0.030
OGLE005546.44-731754.0	0.413	16.329	-0.089	0.105	0.024
OGLE005548.59-725207.2	0.119	14.777	-0.060	0.142	0.024
OGLE005549.19-730023.0	0.059	17.593	-0.072	0.112	0.025
OGLE005552.03-730822.6	0.114	16.240	-0.070	0.150	0.006
OGLE005553.00-723509.8	1.368	16.026	-0.176	-0.186	0.014
OGLE005554.24-724955.1	0.018	16.896	-0.125	-0.031	0.101
OGLE005554.52-724008.5	0.065	16.187	-0.024	0.202	0.016
OGLE005555.26-724056.4	0.331	16.900	-0.051	0.045	0.047
OGLE005555.41-723917.3	1.251	17.530	0.408	0.676	0.027
OGLE005559.08-731822.3	1.859	19.426	0.489	0.582	0.031
OGLE005602.12-730539.4	0.322	16.978	-0.096	-0.060	0.036
OGLE005604.66-723341.0	1.268	16.184	0.013	0.258	0.015
OGLE005605.99-731133.4	0.181	16.872	-0.158	0.065	0.073
OGLE005607.66-724230.9	0.222	17.312	-0.157	-0.102	0.025
OGLE005613.07-730813.7	0.216	16.458	-0.075	0.047	0.011
OGLE005614.68-722929.5	0.056	16.324	-0.120	-0.285	0.079
OGLE005616.05-722758.9	0.103	15.946	0.123	0.238	0.070
OGLE005620.79-722758.3	0.893	17.282	0.139	0.113	0.049
OGLE005620.81-722833.9	0.207	13.263	-0.073	-0.041	0.016
OGLE005622.02-731117.3	0.046	14.918	-0.025	0.181	0.024
OGLE005624.37-722756.9	0.179	16.884	-0.194	0.015	0.020
OGLE005628.94-725411.5	0.222	17.069	-0.086	0.062	0.021
OGLE005630.42-723628.3	0.088	15.837	-0.044	0.152	0.025
OGLE005634.36-730431.8	0.343	16.085	-0.117	-0.091	0.020
OGLE005636.36-730211.0	0.116	13.694	0.007	0.116	0.027
OGLE005639.14-730101.2	0.667	17.535	-0.037	0.071	0.054
OGLE005639.94-724523.9	0.084	14.391	0.149	0.373	0.033
OGLE005640.51-725247.5	0.106	16.138	-0.081	0.047	0.120
OGLE005643.19-723118.0	0.038	15.920	-0.055	0.082	0.022
OGLE005643.60-723448.4	0.354	16.674	-0.067	0.123	0.011
OGLE005644.33-722906.2	0.069	14.565	-0.047	0.062	0.036
OGLE005647.94-722846.3	1.031	14.304	-0.153	-0.102	0.012
OGLE005718.54-723317.5	0.934	16.286	0.001	0.231	0.016
OGLE005718.95-724317.2	0.118	15.226	-0.021	0.170	0.016
OGLE005724.22-722701.8	1.990	16.324	-0.095	0.078	0.014
OGLE005725.10-725841.3	0.108	17.730	-0.115	-0.093	0.019
OGLE005725.29-723106.9	0.043	16.858	-0.063	0.000	0.014
OGLE005726.03-724328.9	1.423	15.403	0.550	0.751	0.013
OGLE005726.39-724359.2	0.114	16.365	-0.075	0.111	0.020
OGLE005730.36-721340.2	1.497	15.957	-0.135	-0.015	0.018
OGLE005731.28-725124.9	1.044	16.762	0.461	0.663	0.020
OGLE005731.31-724712.6	0.406	16.885	-0.045	0.076	0.047
OGLE005736.01-721933.9	0.171	16.015	-0.023	0.224	0.023
OGLE005737.23-721309.0	0.076	13.558	-0.096	0.024	0.016
OGLE005738.07-723251.7	0.308	15.704	-0.084	-0.054	0.013
OGLE005738.39-723038.3	1.514	15.086	-0.202	-0.089	0.035
OGLE005741.28-722108.6	0.128	16.599	-0.132	0.043	0.017
OGLE005745.53-721936.3	0.351	15.959	-0.042	0.036	0.012
OGLE005747.15-725432.5	0.129	16.247	-0.137	-0.016	0.023
OGLE005747.19-721803.5	0.079	17.395	0.407	0.540	0.113
OGLE005749.05-722245.3	0.035	14.788	-0.003	0.168	0.017
OGLE005750.13-722623.4	0.425	15.027	-0.099	-0.040	0.018
OGLE005757.62-723808.3	0.023	18.127	0.590	0.588	0.156
OGLE005802.04-722603.4	0.094	16.090	-0.006	0.034	0.013
OGLE005804.95-725258.3	0.099	17.408	-0.125	-0.127	0.017
OGLE005813.14-725529.7	0.813	19.317	0.385	0.454	0.307
OGLE005813.19-724635.7	0.130	14.394	-0.096	-0.014	0.025
OGLE005822.05-722203.5	0.947	15.911	0.001	0.201	0.019
OGLE005823.26-723418.2	1.278	18.583	-0.074	0.047	0.038
OGLE005824.17-721246.6	0.030	14.983	-0.010	0.267	0.024
OGLE005824.36-723716.4	1.131	16.755	-0.081	-0.004	0.016
OGLE005825.30-723328.8	0.173	17.454	-0.065	0.018	0.012
OGLE005829.12-724738.5	0.285	15.822	0.027	0.181	0.013
OGLE005830.29-722215.6	0.012	15.066	-0.135	-0.075	0.030
OGLE005831.58-721821.1	0.132	15.076	-0.151	-0.150	0.013
OGLE005833.34-723931.8	0.160	14.120	-0.012	0.227	0.014
OGLE005837.36-722204.8	0.591	17.180	-0.046	0.065	0.016
OGLE005839.66-722022.8	0.079	14.738	0.014	0.175	0.013
OGLE005840.81-723905.5	1.317	16.702	-0.060	0.068	0.010
OGLE005844.56-722130.7	0.311	15.360	-0.015	0.190	0.012
OGLE005846.40-725330.9	0.126	16.171	-0.033	0.198	0.011
OGLE005847.07-721301.5	0.082	14.668	-0.086	0.048	0.019
OGLE005847.47-721236.4	0.057	15.441	-0.178	-0.040	0.034
OGLE005852.18-723853.8	0.385	15.613	-0.134	-0.094	0.014
OGLE005853.17-723751.8	0.090	17.041	-0.090	0.054	0.021
OGLE005855.40-724300.8	0.651	14.626	-0.142	-0.111	0.017
OGLE005856.54-723044.6	1.750	15.835	-0.062	0.095	0.012
OGLE005857.06-723313.6	1.282	19.469	-0.232	0.720	0.185
OGLE005857.56-721934.7	2.576	19.404	-0.104	-0.084	0.043
OGLE005859.91-721737.6	0.161	17.245	-0.058	0.162	0.018
OGLE005912.40-721617.4	0.036	16.215	-0.140	-0.129	0.010
OGLE005921.03-722317.1	0.128	14.829	-0.070	0.033	0.023
OGLE005935.19-721633.7	0.538	17.350	0.149	-0.023	0.020
OGLE005942.73-721421.6	0.027	15.246	-0.039	0.134	0.011
OGLE005944.09-722902.9	0.032	16.112	-0.058	0.153	0.023
OGLE005946.45-722250.0	0.150	15.975	-0.052	0.102	0.014
OGLE005951.98-722525.9	0.047	16.072	-0.053	0.131	0.019
OGLE010002.38-730104.2	0.099	16.506	-0.038	0.241	0.013
OGLE010002.49-722214.7	1.397	15.995	-0.078	0.006	0.009
OGLE010002.77-722151.4	1.013	15.492	-0.161	-0.112	0.016
OGLE010003.10-721937.3	0.411	18.418	-0.050	0.034	0.028
OGLE010016.18-722930.6	0.238	15.769	0.005	0.182	0.033
OGLE010022.15-723048.5	0.130	14.696	-0.167	-0.202	0.043
OGLE010024.71-724632.1	4.325	14.691	-0.136	-0.046	0.068
OGLE010026.96-722258.4	0.090	15.291	-0.009	0.258	0.018
OGLE010027.93-723650.2	1.026	16.841	-0.124	-0.104	0.050
OGLE010028.65-724909.4	2.314	16.965	0.027	0.184	0.031
OGLE010028.97-725918.5	0.105	17.603	-0.072	0.160	0.079
OGLE010030.75-724716.3	1.680	16.407	-0.201	-0.162	0.027
OGLE010035.00-723238.1	0.095	15.913	0.019	-0.047	0.047
OGLE010043.30-720742.6	0.329	16.393	-0.094	0.018	0.015
OGLE010043.35-720754.4	0.443	19.668	0.025	0.092	0.029
OGLE010058.06-721216.5	0.036	15.275	-0.083	0.074	0.048
OGLE010100.62-724938.9	0.143	16.717	-0.105	-0.036	0.032
OGLE010102.24-725658.5	0.053	16.091	-0.177	-0.166	0.016
OGLE010102.58-722207.7	0.140	17.133	-0.144	-0.140	0.016
OGLE010103.75-721544.4	0.053	14.579	-0.107	0.084	0.017
OGLE010108.13-724509.3	0.056	15.979	-0.019	0.070	0.020
OGLE010108.82-724009.5	0.198	17.256	-0.104	-0.009	0.019
OGLE010110.19-721203.2	0.059	15.598	-0.194	-0.165	0.034
OGLE010112.17-721045.4	0.125	17.037	-0.076	0.067	0.016
OGLE010118.10-723829.1	0.435	15.437	-0.052	0.155	0.018
OGLE010118.78-723632.5	0.631	15.467	-0.152	-0.031	0.021
OGLE010124.23-721946.7	0.133	16.031	-0.104	0.039	0.024
OGLE010124.28-724543.6	0.117	16.662	-0.039	0.011	0.020
OGLE010125.94-723404.4	0.145	15.125	-0.038	0.215	0.010
OGLE010127.63-722422.5	0.154	19.058	0.132	0.384	0.029
OGLE010129.50-722319.7	0.048	13.794	-0.077	0.128	0.027
OGLE010139.87-720615.0	0.066	14.985	-0.193	-0.158	0.015
OGLE010144.10-723534.7	0.342	16.781	-0.153	-0.105	0.022
OGLE010144.44-723353.0	0.135	15.566	0.114	-0.002	0.166
OGLE010146.69-723003.4	0.146	14.736	-0.080	0.013	0.025
OGLE010151.74-723041.3	0.031	17.498	-0.087	-0.057	0.016
OGLE010153.18-720708.3	0.156	16.180	-0.203	-0.175	0.039
OGLE010154.13-721854.6	0.021	16.739	-0.126	0.017	0.027
OGLE010155.00-724157.2	0.086	17.566	-0.013	-0.115	0.022
OGLE010155.77-723236.1	0.031	13.907	-0.076	0.057	0.043
OGLE010201.63-722505.6	0.076	16.095	-0.039	0.158	0.012
OGLE010202.54-723710.1	0.477	15.316	-0.175	-0.146	0.014
OGLE010205.77-721920.7	0.115	15.626	-0.117	0.015	0.009
OGLE010218.40-724853.9	1.833	15.522	0.160	0.331	0.009
OGLE010227.30-720514.3	0.123	15.827	-0.132	0.072	0.013
OGLE010232.69-724900.3	1.485	16.145	0.505	0.690	0.008
OGLE010232.98-723534.4	0.125	19.697	0.374	0.565	0.282
OGLE010234.69-725424.1	0.275	18.346	0.342	0.705	0.018
OGLE010235.08-723655.4	0.078	16.863	-0.042	0.138	0.013
OGLE010236.25-720806.2	0.048	16.895	-0.130	-0.070	0.012
OGLE010238.96-721454.2	0.134	16.130	-0.192	-0.106	0.018
OGLE010240.50-724749.7	0.053	16.195	0.063	0.041	0.029
OGLE010244.86-721521.7	0.361	18.892	0.491	0.480	0.043
OGLE010246.44-721608.4	0.077	16.912	-0.108	0.148	0.019
OGLE010251.96-720514.0	0.118	13.585	-0.042	0.053	0.009
OGLE010256.82-724351.2	0.157	15.698	-0.144	-0.121	0.011
OGLE010258.79-723033.7	0.069	14.391	-0.013	0.215	0.008
OGLE010302.31-720836.1	0.114	14.399	-0.162	-0.069	0.044
OGLE010302.72-720451.7	0.055	13.929	-0.180	-0.087	0.013
OGLE010307.50-721920.7	0.100	15.734	-0.212	-0.151	0.022
OGLE010307.88-721404.2	0.252	14.825	-0.063	0.179	0.012
OGLE010310.37-724220.2	0.784	15.400	-0.149	-0.132	0.012
OGLE010310.48-721418.5	0.425	15.740	-0.209	-0.175	0.018
OGLE010311.24-720844.8	4.234	15.780	-0.204	-0.166	0.011
OGLE010311.85-721736.6	0.056	15.584	-0.102	-0.109	0.047
OGLE010313.40-720557.1	0.198	14.297	-0.218	-0.159	0.018
OGLE010314.06-722102.0	0.197	16.946	-0.162	-0.025	0.020
OGLE010320.83-725435.2	1.976	19.687	-0.048	-0.010	0.039
OGLE010322.77-725411.2	0.221	15.023	-0.027	0.206	0.015
OGLE010323.85-723010.8	0.118	17.542	0.023	-0.029	0.065
OGLE010325.34-725351.3	0.384	13.512	-0.116	-0.028	0.018
OGLE010325.86-723900.1	0.280	15.192	-0.146	-0.016	0.024
OGLE010326.21-723418.4	0.352	16.581	-0.112	0.042	0.016
OGLE010326.30-720554.3	0.233	15.425	-0.136	-0.165	0.017
OGLE010327.52-723641.0	1.236	19.003	-0.143	-0.052	0.035
OGLE010327.52-725128.6	0.021	16.336	-0.056	-0.022	0.027
OGLE010328.03-720611.7	0.134	14.478	-0.069	0.042	0.021
OGLE010338.29-723734.2	0.056	16.122	-0.041	0.170	0.013
OGLE010338.67-722246.4	0.513	16.376	-0.022	0.148	0.009
OGLE010340.50-720343.1	0.046	15.939	-0.112	0.112	0.013
OGLE010341.75-722219.5	0.257	16.227	-0.092	-0.067	0.017
OGLE010342.34-721342.4	0.047	13.861	0.113	0.317	0.015
OGLE010342.92-723243.6	0.157	15.509	-0.099	0.006	0.011
OGLE010345.55-720947.9	0.165	16.573	-0.054	0.160	0.031
OGLE010349.33-724013.0	0.034	16.616	-0.080	0.132	0.011
OGLE010353.06-724939.2	0.083	15.092	-0.111	0.039	0.034
OGLE010353.36-725007.0	0.072	16.186	-0.109	0.141	0.012
OGLE010354.84-721516.5	0.124	16.079	-0.066	0.153	0.017
OGLE010356.74-724926.2	0.133	15.366	-0.128	0.045	0.020
OGLE010400.15-720412.0	0.380	16.132	-0.106	0.041	0.011
OGLE010412.69-724701.8	0.068	15.921	-0.138	-0.087	0.048
OGLE010413.67-723331.1	0.022	16.319	-0.083	0.042	0.031
OGLE010415.69-724456.6	0.183	15.466	-0.113	0.054	0.044
OGLE010415.96-724619.1	0.272	16.842	-0.144	-0.054	0.018
OGLE010417.80-720605.4	0.299	15.628	-0.165	-0.168	0.022
OGLE010421.15-720915.6	3.490	13.507	-0.123	0.092	0.013
OGLE010422.88-723256.5	3.264	16.569	0.497	0.522	0.023
OGLE010429.74-720150.5	0.283	15.788	-0.224	-0.204	0.009
OGLE010436.27-720941.2	0.121	15.766	-0.134	0.011	0.019
OGLE010437.61-720938.4	0.217	15.879	-0.153	0.138	0.076
OGLE010437.78-721352.7	0.740	15.440	-0.276	-0.232	0.016
OGLE010438.44-722756.0	0.013	15.880	-0.026	0.261	0.012
OGLE010448.12-724237.6	0.749	16.693	-0.169	-0.136	0.014
OGLE010456.35-720157.9	1.366	17.828	0.562	0.774	0.015
OGLE010457.92-725003.1	0.087	15.109	-0.130	0.125	0.020
OGLE010504.42-725129.1	0.048	15.032	-0.133	0.011	0.009
OGLE010505.32-722358.5	0.028	14.474	-0.106	-0.024	0.035
OGLE010553.61-724600.2	0.764	15.652	-0.174	-0.162	0.014
OGLE010556.93-723244.0	0.961	16.182	-0.114	-0.066	0.010
OGLE010558.23-721836.9	0.312	16.145	-0.233	-0.210	0.008
OGLE010601.14-724631.2	1.828	15.819	-0.209	-0.145	0.017
OGLE010605.04-724220.0	0.098	16.657	-0.101	0.150	0.016
OGLE010605.07-724643.6	0.330	17.472	-0.154	-0.095	0.017
OGLE010616.25-722058.9	0.104	17.568	0.494	0.663	0.019
OGLE010617.18-722746.4	0.044	13.372	-0.120	-0.028	0.041
OGLE010617.23-722648.7	0.393	15.435	0.129	0.412	0.014
OGLE010621.19-722059.6	0.723	15.582	-0.144	-0.209	0.012
OGLE010621.90-724640.4	0.180	15.752	-0.127	0.095	0.020
OGLE010625.05-723843.2	0.564	19.685	-0.064	0.124	0.221
OGLE010634.51-721504.7	0.112	16.682	0.131	0.398	0.035
OGLE010646.38-721629.6	0.019	15.320	-0.142	-0.031	0.019
OGLE010648.54-721213.4	0.051	19.436	0.094	-0.174	0.089
OGLE010656.24-724125.9	3.170	17.252	-0.135	-0.155	0.012
OGLE010700.96-722318.1	0.118	15.582	-0.043	0.202	0.032
OGLE010705.79-722707.5	0.144	14.149	-0.143	0.086	0.047
OGLE010706.20-721603.0	0.149	14.873	-0.039	0.177	0.010
OGLE010710.69-722034.5	0.103	15.370	-0.208	-0.145	0.019
OGLE010714.44-722235.3	0.079	15.920	-0.125	0.046	0.022
OGLE010716.19-723251.6	0.039	16.705	-0.044	0.225	0.030
OGLE010721.61-724845.5	0.612	18.970	0.246	0.690	0.054
OGLE010729.13-721519.4	0.022	13.702	-0.064	0.092	0.033
OGLE010733.16-723334.1	0.174	17.049	-0.088	0.139	0.013
OGLE010736.82-722004.0	0.024	14.931	0.028	0.254	0.012
OGLE010738.79-730015.2	0.189	16.696	-0.036	-0.065	0.031
OGLE010742.34-722353.0	0.761	19.451	0.195	0.494	0.284
OGLE010749.63-722639.3	0.253	13.900	-0.128	-0.009	0.050
OGLE010749.94-725059.2	0.955	16.153	-0.191	-0.136	0.015
OGLE010807.28-724136.1	0.104	15.183	-0.030	0.221	0.022
OGLE010818.03-723624.6	0.294	15.109	0.014	0.275	0.026
OGLE010819.29-723102.0	1.532	15.043	0.264	0.484	0.022
OGLE010830.47-722708.4	2.048	14.805	-0.237	-0.198	0.034
OGLE010849.29-722355.8	0.145	15.309	-0.087	0.113	0.028
OGLE010851.41-724542.8	1.187	18.724	0.498	0.586	0.235
OGLE010851.50-722708.3	0.147	15.137	-0.195	-0.194	0.037
OGLE010902.76-723016.4	0.643	17.494	-0.126	0.001	0.048
OGLE010905.89-722139.9	0.164	14.572	-0.288	0.226	0.144
OGLE010910.42-722408.4	0.192	14.832	-0.078	0.134	0.042