Table 5
Estimates of the distance to CoRoT 223992193 using V and K-band magnitudes, bolometric corrections (BCs; Bessell et al. 1998) for different effective temperature estimates, and a range of extinction estimates (from both the literature and as indicated from the CAHA spectrum, Fig. 4).
| Extinction | Teff (K) | Distance | |
| (mag) | (pri) | (sec) | (pc) |
|
|
|||
| AV = 0.71 | 3500 | 3500 | 561 ± 61 |
| (Dahm & Simon 2005) | 3750 | 3500 | 627 ± 71 |
| 3750 | 3750 | 668 ± 73 | |
| AV = 0.45 | 3500 | 3500 | 633 ± 69 |
| (Rebull et al. 2002) | 3750 | 3500 | 707 ± 80 |
| 3750 | 3750 | 754 ± 83 | |
| AV = 0.25 | 3500 | 3500 | 694 ± 76 |
| (Sung et al. 1997) | 3750 | 3500 | 775 ± 88 |
| 3750 | 3750 | 826 ± 91 | |
| AV = 0.0 | 3500 | 3500 | 776 ± 85 |
| (CAHA spectrum) | 3750 | 3500 | 868 ± 98 |
| 3750 | 3750 | 924 ± 101 | |
| AK = 0.073 | 3500 | 3500 | 766 ± 85 |
| (Rebull et al. 2002) | 3750 | 3500 | 743 ± 82 |
| 3750 | 3750 | 728 ± 81 | |
| AK = 0.0 | 3500 | 3500 | 791 ± 87 |
| (CAHA spectrum) | 3750 | 3500 | 768 ± 84 |
| 3750 | 3750 | 751 ± 83 | |
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