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Table A.1

Fundamental parameters and rotational frequencies with their respective 1σ uncertainties.

CoRoT ID No SpT Teff log g v sin i log L R M ττMS frot i°
K dex km s−1 R M c d−1
CoRoT 101486436 1 B7 V 13000 ± 1500 4.1 ± 0.2 242 ± 30 2.24 ± 0.26 2.6 ± 0.5 3.5 ± 0.2 0.30 ± 0.23 2.12 ± 0.24 40 ± 15
CoRoT 102595654 2 B9 III 10500 ± 1500 3.4 ± 0.3 328 ± 30 2.75 ± 0.27 7.3 ± 1.5 3.9 ± 0.3 1.02 ± 0.01 1.28 ± 0.27 90 ± 10
CoRoT 102656190 4 B2 V 20500 ± 2000 4.1 ± 0.2 278 ± 30 3.31 ± 0.26 3.7 ± 0.7 7.0 ± 0.4 0.23 ± 0.21 1.83 ± 0.20 40 ± 15
CoRoT 102672979 5 B3 IV 16200 ± 2000 3.5 ± 0.4 222 ± 30 3.62 ± 0.28 8.4 ± 1.8 6.8 ± 0.5 1.00 ± 0.03 0.55 ± 0.07 50 ± 10
CoRoT 102686433 6 B3 IV 17600 ± 1500 3.7 ± 0.2 300 ± 30 3.69 ± 0.27 7.7 ± 1.6 7.4 ± 0.5 0.96 ± 0.05 0.73 ± 0.09 60 ± 20
CoRoT 102719279 9 B1 IV 22300 ± 1500 3.7 ± 0.2 287 ± 20 4.15 ± 0.28 8.1 ± 1.8 10.6 ± 0.8 0.88 ± 0.07 0.73 ± 0.09 50 ± 10
CoRoT 102725623 11 B7 III 13000 ± 1500 2.8 ± 0.3 296 ± 40 4.06 ± 0.30 21.8 ± 5.1 8.9 ± 1.0 1.02 ± 0.01 0.35 ± 0.08 90 ± 10
CoRoT 102728404 12 B1 V 23600 ± 2000 4.0 ± 0.3 200 ± 30 3.78 ± 0.27 4.7 ± 1.0 9.3 ± 0.5 0.45 ± 0.21 1.40 ± 0.15 40 ± 15
CoRoT 102766835 14 O9 IV 33400 ± 2000 3.8 ± 0.3 262 ± 50 5.01 ± 0.33 9.9 ± 2.5 23.1 ± 2.8 0.63 ± 0.12 0.83 ± 0.12 30 ± 10
CoRoT 102785480 17 B2 IV 21700 ± 2000 3.8 ± 0.2 331 ± 30 3.96 ± 0.27 6.9 ± 1.5 9.5 ± 0.7 0.83 ± 0.09 0.94 ± 0.12 60 ± 10
CoRoT 102825808 18 B2 V 20500 ± 2000 4.0 ± 0.3 369 ± 40 3.56 ± 0.26 4.9 ± 1.0 7.7 ± 0.4 0.63 ± 0.17 1.45 ± 0.19 60 ± 10
CoRoT 102829773 19 B1 V 23600 ± 2000 4.3 ± 0.3 409 ± 40 3.42 ± 0.25 3.1 ± 0.6 8.2 ± 0.4 0.02 ± 0.04 2.63 ± 0.30 60 ± 10
CoRoT 102847615 20 B3 V 17500 ± 2000 4.2 ± 0.3 220 ± 30 2.80 ± 0.26 2.8 ± 0.6 5.2 ± 0.3 0.11 ± 0.13 2.29 ± 0.25 30 ± 15
CoRoT 102904910 22 B2 V 18900 ± 2000 4.1 ± 0.2 296 ± 30 3.23 ± 0.26 4.0 ± 0.8 6.4 ± 0.3 0.50 ± 0.20 1.60 ± 0.18 40 ± 10

Notes. No = sequence number of stars attributed in Paper I. SpT = spectral type. Stellar luminosity L, mass M, and radius R are given in solar units. τ = stellar age; τMS = time that a rotating star spends in the main sequence phase. frot = rotational frequency. i° = estimated inclination angle of the rotation axis.

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