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Table 1

Be star candidates in the first exofields of CoRoT.

CoRoT ID Run V r Spec. type Photometry Spectroscopy
mag mag

101486436 LRC1 12.333 12.237 GIRAFFE
102595654 LRA1 13.819 13.522 GIRAFFE
102613778 LRA1 15.409 15.096 GIRAFFE
102617376 LRA1 12.597 12.226 T1.5−OAN R&J
102638133 LRA1 14.852 14.462 B3 INT
102640224 LRA1 15.324 15.125 B9 INT
102645018 LRA1 13.214 12.718 B0 INT R&J
102649238 LRA1 13.959 13.576 A0 INT
102656190 LRA1 13.885 13.706 B3 INT GIRAFFE
102667801 LRA1 13.167 13.012 B5 INT
102672979 LRA1 11.473 11.337 GIRAFFE
102675453 LRA1 14.887 14.727 B3 INT
102686433 LRA1 13.475 13.253 GIRAFFE
102690931 LRA1 14.041 13.853 B5 INT
102695055 LRA1 16.367 15.859 GIRAFFE
102695698 LRA1 13.914 13.758 GIRAFFE
102696078 LRA1 12.840 12.668 R&J
102710394 LRA1 14.459 14.128 B8 INT
102719279 LRA1* 14.074 13.809 B9 INT CAFOS, GIRAFFE
102721109 LRA1* 15.505 15.035 GIRAFFE
102725623 LRA1* 15.165 14.820 B6 INT CAFOS, GIRAFFE
102728404 LRA1 11.928 11.604 R&J, GIRAFFE
102736797 LRA1 12.873 12.678 B2 INT
102737893 LRA1 12.266 11.915 R&J
102749262 LRA1 15.864 15.599 GIRAFFE
102749390 LRA1 14.120 13.906 B3 INT
102761769 IR1 13.288 13.080 IDS
102762536 LRA1 13.902 13.513 B0 INT
102766835 LRA1* 13.197 12.817 B2 T1.5−OAN R&J, CAFOS, GIRAFFE
102777669 LRA1 14.640 14.391 GIRAFFE
102781703 LRA1 12.663 12.314 B3 INT
102785204 LRA1 12.058 11.756 B0 INT R&J, GIRAFFE, X-shooter
102785480 LRA1 12.899 12.591 B2 INT R&J, GIRAFFE
102791482 IR1 12.908 12.596 CAFOS
102798228 IR1 15.287 15.001 ALBIREO
102825808 IR1 14.424 14.165 ALBIREO, GIRAFFE
102829773 IR1 15.211 14.836 X-shooter
102847615 IR1 13.873 13.572 GIRAFFE
102875251 IR1 14.799 14.536 ALBIREO, GIRAFFE
102904910 IR1 14.019 13.773 CAFOS, X-shooter
102964342 IR1 14.550 14.256 CAFOS

Notes.(*) Observed by CoRoT in the LRA1 and IR1. Columns 3 & 4: magnitudes from the Exo-Dat database (Deleuil et al. 2009). Column 5: spectral types determined from Strömgren photometry. Column 6: telescopes used to identify photometrically the stars with the Be phenomenon. Column 7: instruments that helped identify the Be stars spectroscopically. GIRAFFE stands for the multifiber spectrograph at ESO; X-shooter for the single target spectrograph at ESO; INT for the Isaac Newton Telescope in la Palma (Spain); T1.5-OAN for telescope of 1.5 m in Observatorio Astronomico Nacional (OAN) in Calar Alto, Almeria (Spain); ALBIREO for the low resolution spectrograph at Observatorio de Sierra Nevada (OSN), Granada (Spain); CAFOS for the low resolution spectrograph at the Centro Astronómico Hispano Alemán (CAHA) in Calar Alto, Almeria (Spain); IDS for the Intermediate Dispersion Spectrograph attached on the Isaac Newton telescope (INT) at the Observatorio del Roque de los Muchachos in la Palma (Spain); R&J indicates stars in the emission-line catalog of Robertson & Jordan (1989).

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