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Home All issues Volume 506 / No 1 (October IV 2009) A&A, 506 1 (2009) 321-336 Full HTML
 

 

Table 2:

Pre-launch information on IRa01 transit candidates derived from multi-colour photometry.
WinID CoRoT ID RA Dec Ba V r Jb K SpT Teffc Instr. Contad
E1-2046 102723949 06:44:10.95 -01:11:13.24 14.885 13.958 13.598 12.355 11.683 K0III 5000 PH 0.0101
E2-3010 102800106 06:45:57.58 -02:28:00.73 16.82 15.883 15.489 13.896 13.363 K2V 4800 PH 0.046
E2-3854 102841669 06:47:09.41 -02:46:39.11 16.419 15.333 14.906 12.919 12.383 K5III 4500 PH 0.038
E2-3856 102954464 06:49:37.33 -02:30:49.14 17.548 16.478 15.966 14.304 13.540 K5V 4500 PH 0.010
E1-1158 102763847 06:45:05.23 -01:21:25.24 13.604 13.199 13.112 12.530 12.374 F0V 7250 PH 0.004
E2-0203 102825481 06:46:43.20 -02:35:58.31 14.025 13.308 13.068 12.058 11.681 G1V 5800 PH 0.000
E2-2430 102815260 06:46:25.78 -03:09:13.28 15.74 14.893 14.569 13.122 12.648 F2V 7000 SO 0.019
E1-0399 102829121 06:46:49.37 -01:23:11.62 14.708 13.933 13.663 12.543 12.126 G4V 5550 PH 0.003
E2-1736 102855534 06:47:30.58 -02:55:04.12 14.681 14.062 13.845 12.762 12.412 G0V 5900 PH 0.086
E2-2604 102805893 06:46:08.99 -02:02:00.35 16.513 15.703 15.416 14.110 13.635 G8V 5200 PH 0.0194
E2-1136 102809071 06:46:15.36 -03:05:19.61 13.497 13.228 13.204 12.611 12.496 A9V 7400 PH 0.08
E2-4300 102802430 06:46:02.21 -02:00:13.43 15.234 14.552 14.327 13.135 12.817 G3V 5600 PH 0.212
E1-0288 102787048 06:45:36.24 -00:43:17.40 14.149 13.452 13.174 12.269 11.928 F9V 6000 PH 0.17
E2-1857 102798247 06:45:53.90 -02:47:15.90 14.857 14.259 14.062 13.050 12.674 F9V 5950 PH 0.006
E2-2009 102788073 06:45:37.69 -01:58:09.30 16.48 14.865 14.184 11.542 10.614 M0II 3800 PH 0.039
E1-2329 102869286 06:47:49.45 -00:36:29.05 16.895 15.957 15.520 14.327 13.715 G9IV 5100 PH 0.062
E1-3336 102876631 06:48:00.16 -01:05:05.96 16.417 15.099 14.557 12.479 11.651 K8V 4050 PH 0.016
E1-4617 102753331 06:44:50.87 -00:42:53.28 16.855 16.158 15.868 14.563 14.087 G7V 5300 PH 0.002
E1-0783 102895957 06:48:26.40 -01:14:31.34 13.246 12.852 12.720 11.951 11.760 F2IV 6800 PH 0.028
E2-4467 102940315 06:49:20.63 -02:05:37.72 17.079 16.177 15.814 14.033 13.570 K2III 4800 PH 0.000
E1-4591 102806520 06:46:10.25 -01:42:23.70 14.452 13.863 13.697 12.705 12.418 F9V 6000 PH 0.315
E2-1712 102826302 06:46:44.59 -03:02:32.21 14.868 14.197 13.976 12.843 12.530 F5IV 6700 HA 0.04
E2-3425 102835817 06:47:00.12 -02:34:07.14 16.671 15.903 15.598 14.320 13.862 G7III 5800 HA 0.26
E1-4998 102821773 06:46:36.92 -01:06:15.77 16.41 15.71 15.475 14.354 13.909 G2V 5700 PH 0.258
E2-0704 102855472 06:47:30.49 -02:36:40.14 15.085 14.215 13.865 12.514 12.028 G7III 5400 HA 0.102
E2-1677 102874481 06:47:57.12 -02:56:10.89 14.403 13.941 13.839 12.989 12.707 F4V 6500 PH 0.015
E1-4108 102779966 06:45:26.87 -01:14:09.46 16.512 15.412 14.936 13.571 12.880 K2V 5100 HA 0.0437
E2-1126 102890318 06:48:19.20 -03:06:07.77 14.197 13.624 13.431 12.462 12.149 G0V 5950 UV 0.0383
E1-0330 102912369 06:48:46.70 -00:40:21.97 14.312 13.694 13.450 12.619 12.288 F0V 6190 UV 0.003
a Optical magnitudes were measured at the Isaac Newton Telescope with the Wide Field Camera; B and V filters are from the Harris system, and r from the Sloan system. b J and K magnitudes are 2MASS measurements. c The origin of the estimate for effective temperature (Teff), spectral type and luminosity class (SpT) may be from spectral analysis (HA for HARPS, UV for UVES, SO for SOPHIE) or by default, from multicolour photometry. d ``conta'' is the ratio between the background flux and the total flux.

Source LaTeX | All tables | In the text

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