Table 3
Basic host star properties for the analyzed CoRoT planets.
| Star | Spectral type | V | T ⋆ [K] | M ⋆ [M⊙] | R ⋆ [R⊙] | log g | [Fe/H] | Contamination [%] | Ref. |
| Systems with significant eclipse events | |||||||||
| CoRoT-1 | G0V | 13.6 | 5950 ± 150 | 0.95 ± 0.15 | 1.11 ± 0.05 | 4.25 ± 0.30 | −0.30 ± 0.25 | ~0 | 1 |
| CoRoT-2 | G7V | 12.6 | 5625 ± 120 | 0.97 ± 0.06 | 0.90 ± 0.02 | 4.30 ± 0.20 | 0.00 ± 0.10 | 5.6 | 2, 3 |
| CoRoT-6 | F9V | 13.9 | 6090 ± 50 | 1.05 ± 0.05 | 1.03 ± 0.03 | 4.44 ± 0.23 | −0.20 ± 0.10 | 2.8 | 5 |
| CoRoT-11 | F6V | 12.9 | 6440 ± 120 | 1.27 ± 0.05 | 1.37 ± 0.03 | 4.22 ± 0.23 | −0.03 ± 0.08 | 13.0 | 6 |
| CoRoT-15 | F7V | 6350 ± 200 | 1.32 ± 0.12 |
|
4.30 ± 0.20 | 0.10 ± 0.20 | 1.9 | 8 | |
| Systems with marginal eclipse events | |||||||||
| CoRoT-3 | F3V | 13.3 | 6740 ± 140 | 1.37 ± 0.09 | 1.56 ± 0.09 | 4.22 ± 0.07 | −0.02 ± 0.06 | 8.2 | 4 |
| CoRoT-13 | G0V | 15.0 | 5945 ± 90 | 1.09 ± 0.02 | 1.01 ± 0.03 | 4.30 ± 0.10 | 0.01 ± 0.07 | 11.0 | 7 |
| CoRoT-18 | G9V | 15.0 | 5440 ± 100 | 0.95 ± 0.15 | 1.00 ± 0.13 | 4.40 ± 0.10 | −0.10 ± 0.10 | 2.0 | 9 |
| CoRoT-21 | F8IV | 16.1 | 6200 ± 100 | 1.29 ± 0.09 | 1.95 ± 0.21 | 3.70 ± 0.10 | 0.00 ± 0.10 | 8.5 | 10 |
| Systems without identified eclipse events | |||||||||
| CoRoT-4 | F8V | 13.7 | 6190 ± 60 | 1.16 ± 0.03 | 1.17 ± 0.03 | 4.41 ± 0.05 | 0.05 ± 0.07 | 0.3 | 11, 12 |
| CoRoT-5 | F9V | 14.0 | 6100 ± 65 | 1.00 ± 0.02 | 1.19 ± 0.04 | 4.19 ± 0.03 | −0.25 ± 0.06 | 8.4 | 13 |
| CoRoT-7 | K0V | 11.7 | 5250 ± 60 | 0.91 ± 0.03 | 0.82 ± 0.04 | 4.57 ± 0.05 | 0.12 ± 0.06 | 0.5 | 14, 15 |
| CoRoT-8 | K1V | 14.8 | 5080 ± 80 | 0.88 ± 0.04 | 0.77 ± 0.02 | 4.58 ± 0.08 | 0.30 ± 0.10 | 0.7 | 16 |
| CoRoT-9 | G3V | 13.7 | 5625 ± 80 | 0.99 ± 0.04 | 0.94 ± 0.04 | 4.54 ± 0.09 | −0.01 ± 0.06 | 2.5 | 17 |
| CoRoT-10 | K1V | 15.2 | 5075 ± 75 | 0.89 ± 0.05 | 0.79 ± 0.05 | 4.65 ± 0.10 | 0.26 ± 0.07 | 5.5 | 18 |
| CoRoT-12 | G2V | 15.5 | 5675 ± 80 | 1.08 ± 0.08 | 1.10 ± 0.10 | 4.52 ± 0.08 | 0.16 ± 0.10 | 3.3 | 19 |
| CoRoT-14 | F9V | 16.0 | 6035 ± 100 | 1.13 ± 0.09 | 1.21 ± 0.08 | 4.35 ± 0.15 | 0.05 ± 0.15 | 7.0 | 20 |
| CoRoT-16 | G5V | 15.6 | 5650 ± 100 | 1.10 ± 0.08 | 1.19 ± 0.14 | 4.36 ± 0.10 | 0.19 ± 0.06 | 2.3 | 21 |
| CoRoT-17 | G2V | 15.5 | 5740 ± 80 | 1.04 ± 0.10 | 1.59 ± 0.07 | 4.40 ± 0.10 | 0.00 ± 0.10 | 8.0 | 22 |
| CoRoT-19 | F9V | 14.8 | 6090 ± 70 | 1.21 ± 0.05 | 1.65 ± 0.04 | 4.07 ± 0.03 | −0.02 ± 0.10 | 0.3 | 23 |
| CoRoT-20 | G2V | 14.7 | 5880 ± 90 | 1.14 ± 0.08 | 1.02 ± 0.05 | 4.20 ± 0.15 | 0.14 ± 0.12 | <0.6 | 24 |
| CoRoT-23 | G0V | 15.6 | 5900 ± 100 | 1.14 ± 0.08 | 1.61 ± 0.18 | 4.30 ± 0.20 | 0.05 ± 0.10 | 7.2 | 25 |
References. (1) Barge et al. (2008); (2) Alonso et al. (2008); (3) Bouchy et al. (2008); (4) Deleuil et al. (2008); (5) Fridlund et al. (2010); (6) Gandolfi et al. (2010); (7) Cabrera et al. (2010); (8) Bouchy et al. (2010); (9) Hébrard et al. (2011); (10) Pätzold et al. (2012); (11) Aigrain et al. (2008); (12) Moutou et al. (2008); (13) Rauer et al. (2009); (14) Léger et al. (2009); (15) Bruntt et al. (2010); (16) Bordé et al. (2010); (17) Deeg et al. (2010); (18) Bonomo et al. (2010); (19) Gillon et al. (2010); (20) Tingley et al. (2011b); (21) Ollivier et al. (2012); (22) Csizmadia et al. (2011); (23) Guenther et al. (2012); (24) Deleuil et al. (2012); (25) Rouan et al. (2012).
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