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Home All issues Volume 520 (September-October 2010) A&A, 520 (2010) A74 Full HTML
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This article has an erratum: [https://doi.org/10.1051/0004-6361/200810284e]

 

 

Table 3:

Basic parameters of the observed eclipsing binaries: identifying number (Fig. 1), OGLE identifying code, coordinates, orbital period, epoch of primary minimum (see text), infrared and (B-V) and (V-I) color indices.

id 		OGLE $\alpha$ (J2000) $\delta $ (J2000) $P_{\rm orb}$ t0 (HJD $I_{\rm DIA}^{\rm q}$ $\Delta I^{\rm q}$ $(B-V)^{\rm q}$ $(V-I)^{\rm q}$
  object (h m s) ( $\hbox {$^\circ $ }$ $\hbox{$^\prime$ }$ $\hbox{$^{\prime\prime}$ }$) (d) -2 450 000) (mag) (mag) (mag) (mag)
1 4 110409 00:47:00.19 -73:18:43.1 2.973170(4) 619.49136 15.840 -0.002 $-0.036\pm0.007$ $ 0.006\pm0.004$
2 4 113853 00:47:03.76 -73:15:19.8 1.320757(4) 620.90811 17.340 -0.008 $-0.002\pm0.006$ $ 0.045\pm0.003$
3 4 117831 00:47:31.74 -73:12:02.2 1.164566(2) 621.36981 17.799 0.003 $-0.115\pm0.004$ $-0.102\pm0.003$
4 4 121084 00:47:32.05 -73:09:08.4 0.823722(1) 624.39596 16.959 -0.000 $-0.084\pm0.004$ $-0.052\pm0.004$
5 4 121110 00:47:04.60 -73:08:40.1 1.111991(1) 622.29034 17.003 0.009 $-0.090\pm0.005$ $-0.076\pm0.002$
6 4 121461 00:47:24.69 -73:09:35.5 1.94670 624.3954 17.926 0.003 $-0.060\pm0.005$ $-0.081\pm0.005$
7 4 159928 00:48:13.53 -73:19:30.8 1.150460(2) 621.13880 16.704 -0.000 $-0.079\pm0.002$ $-0.059\pm0.002$
8 4 160094 00:48:10.17 -73:19:37.1 1.699634(66) 620.04883 17.125 -0.000 $-0.163\pm0.002$ $-0.176\pm0.002$
9 4 163552 00:47:53.24 -73:15:56.5 1.545811(2) 620.73188 15.771 0.008 $-0.045\pm0.003$ $-0.030\pm0.002$
10 4 175149 00:48:34.80 -73:06:52.6 2.000375(3) 623.85898 14.970 -0.003 $-0.218\pm0.007$ $-0.238\pm0.004$
11 4 175333 00:48:15.38 -73:07:05.3 1.251126(9) 622.86576 17.732 -0.009 $-0.121\pm0.003$ $-0.122\pm0.003$
12 5 016658 00:49:02.93 -73:20:55.9 1.246158(2) 466.70225 17.446 -0.005 $-0.123\pm0.004$ $-0.133\pm0.002$
13 5 026631 00:48:59.84 -73:13:28.8 1.411680(1) 465.98392 16.242 -0.001 $-0.137\pm0.003$ $-0.168\pm0.001$
14 5 032412 00:48:56.86 -73:11:39.7 3.607857(1) 464.67202 16.318 0.005 $-0.033\pm0.006$ $-0.023\pm0.002$
15 5 038089 00:49:01.85 -73:06:06.9 2.389426(2) 468.55092 15.256 -0.002 ( $-0.216\pm0.011$) ( $-0.162\pm0.007$)
16 5 095337 00:49:15.34 -73:22:05.8 0.904590(1) 466.18186 17.090 0.004 $-0.118\pm0.052$ $-0.154\pm0.030$
17 5 095557 00:49:18.07 -73:21:55.3 2.421185(21) 466.80139 17.440 -0.012 $-0.100\pm0.003$ $-0.098\pm0.003$
18 5 100485 00:49:19.86 -73:17:55.6 1.519124(1) 467.15922 17.150 -0.008 $-0.138\pm0.008$ $-0.162\pm0.003$
19 5 100731 00:49:29.33 -73:17:57.9 1.133344(3) 467.82186 17.378 0.000 $-0.111\pm0.003$ $-0.140\pm0.002$
20 5 106039 00:49:20.00 -73:13:37.3 2.194069(5) 465.38253 16.695 -0.005 $-0.050\pm0.033$ $-0.016\pm0.019$
21 5 111649 00:49:17.19 -73:10:24.5 2.959578(3) 470.15054 16.726 0.007 $ 0.008\pm0.009$ $ 0.032\pm0.003$
22 5 123390 00:49:22.66 -73:03:42.8 2.172917(41) 464.12108 16.203 -0.001 $-0.162\pm0.015$ $-0.171\pm0.008$
23 5 180185 00:50:02.63 -73:17:34.4 5.491165(95) 469.37759 17.321 0.034 ( $-0.115\pm0.011$) ( $ 0.029\pm0.009$)
24 5 180576 00:50:13.44 -73:16:33.1 1.561124(2) 466.91033 17.607 0.006 $-0.071\pm0.009$ $-0.036\pm0.003$
25 5 185408 00:50:24.52 -73:14:56.0 1.454991(2) 466.28931 17.524 -0.006 $-0.122\pm0.003$ $-0.126\pm0.002$
26 5 196565 00:50:30.17 -73:07:38.2 3.942732(12) 468.26098 16.942 0.003 (no data) (no data)
27 5 261267 00:51:35.04 -73:17:11.5 1.276632(2) 464.97658 16.833 -0.005 ( $-0.129\pm0.006$) ( $-0.099\pm0.004$)
28 5 265970 00:51:28.13 -73:15:17.6 3.495685(54) 465.39125a 16.226 0.005 $-0.136\pm0.005$ $-0.164\pm0.002$
29 5 266015 00:51:16.82 -73:13:01.9 1.808925(2) 465.10449 15.964 0.002 $-0.086\pm0.004$ $-0.072\pm0.003$
30 5 266131 00:51:35.81 -73:12:44.8 1.302945(22) 465.50898 17.119 0.001 $-0.103\pm0.016$ $-0.104\pm0.004$
31 5 266513 00:50:57.49 -73:12:30.3 1.107510(2) 467.15823 18.066 0.005 $-0.035\pm0.005$ $ 0.009\pm0.003$
32 5 277080 00:51:11.68 -73:05:20.3 1.939346(4) 465.96082 16.070 0.002 ( $-0.019\pm0.013$) ( $-0.171\pm0.003$)
33 5 283079 00:50:58.67 -73:04:35.8 1.283583(1) 466.92376 17.422 -0.002 $-0.073\pm0.004$ $-0.013\pm0.002$

Notes. The difference $\Delta I^{\rm q}=I({\rm DIA})-I({\rm DoPhot})$ is also indicated. The ``q'' superscript denotes values at a quadrature (the brightest for the asymmetric light curves). $\alpha$, $\delta $are from Wyrzykowski et al. (2004), while $P_{\rm orb}$ and t0 are updated values based on both photometry and radial velocities (see text). The uncertainty of the period is given between parentheses as the value of the last digit or, in a few cases, of the last two digits. $I^{\rm q}$, $V^{\rm q}$, $(B-V)^{\rm q}$ and $(V-I)^{\rm q}$ were determined from the light-curve solutions. The color indices between parentheses are unreliable: they correspond to the outliers in Fig. 3.
(a) Incomplete observations for one of the eclipses.


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