Table 9
Derived physical parameters for the stars observed in the LRa01, LRc01, and SRc01 CoRoT fields.
| CoRoT ID | V sin i | Vrad | σVrad | Teff | σTeff | log g | σlog g | [M/H] | σ[M/H] | [α/Fe] | σ[α/Fe] | SNR |
| (km s-1) | (km s-1) | (km s-1) | (K) | (K) | (dex) | (dex) | (dex) | (dex) | (dex) | (dex) | ||
|
|
||||||||||||
| 100603128 | 3.81 | −7.83 | 0.187 | 5350 | 79 | 4.01 | 0.13 | −0.24 | 0.08 | 0.06 | 0.04 | 9 |
| 100583300 | 17.81 | −61.10 | 0.163 | − | − | − | − | − | − | − | − | 23 |
| 100567221 | 1.41 | −25.66 | 0.075 | 5889 | 48 | 4.29 | 0.08 | −0.04 | 0.05 | 0.02 | 0.02 | 23 |
| 100565715 | 5.81 | 92.85 | 0.246 | 6445 | 71 | 4.64 | 0.12 | −0.25 | 0.07 | 0.16 | 0.03 | 12 |
| 100577769 | 8.21 | −27.26 | 0.272 | 5117 | 76 | 3.02 | 0.13 | −1.02 | 0.08 | 0.24 | 0.04 | 10 |
| 100588558 | 11.31 | 39.90 | 0.299 | − | − | − | − | − | − | − | − | 13 |
| 100576988 | 4.81 | −26.10 | 0.118 | 5963 | 60 | 4.41 | 0.1 | 0.0 | 0.06 | −0.02 | 0.03 | 16 |
| 100636016 | 2.71 | 22.55 | 0.322 | 5673 | 80 | 4.29 | 0.13 | −0.88 | 0.08 | 0.24 | 0.04 | 8 |
| 100637229 | 19.41 | −12.39 | 0.224 | − | − | − | − | − | − | − | 28 | |
| 100604545 | 10.71 | 0.37 | 0.231 | − | − | − | − | − | − | − | − | 10 |
| 100634976 | 3.91 | −37.27 | 0.221 | 6100 | 73 | 4.07 | 0.12 | −0.35 | 0.08 | 0.07 | 0.04 | 11 |
| ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... |
Notes. The error bars for the atmospheric parameters are only internal errors coming from Fig. 3. The V sin i error is of the order of 10% of its value. The quality flag (exponent of the value) was set to 1 if the V sin i estimate is not affected by noise or a second component in the CCF; 2 the target is a SB2 and the V sin i is related to the main component of the CCF; 3 the contrast and shape of the CCF are insufficient to assure a proper estimate of its parameters. The SNR of the FLAMES/GIRAFFE spectrum is listed in the last column of the table. We remind the reader that the coordinates, observing dates and magnitudes are publicly available through Exo-Dat.
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