Table B.1
NGC 2264 WTTS considered in this study.
CSI-Mon | GES-NAME | RA(2000) | Dec(2000) | T eff | σ T eff | EW(Li) | σ EW(Li) | Flag† | Period | Ref‡ | V rad | σ V rad | vsini | σ vsini | Notes |
deg. | deg. | K | K | mÅ | mÅ | days | km s-1 | km s-1 | km s-1 | km s-1 | |||||
|
|||||||||||||||
000018 | 06411322+0955087 | 100.3052 | 9.91909 | 4326 | 114 | 515.1 | 30.4 | 1 | 4.26 | V+16 | 17.7 | 0.9 | 30.0 | 0.5 | |
000020 | 06420924+0944034 | 100.53849 | 9.73427 | 4085 | 221 | 550.2 | 8.4 | 1 | 5.179 | V+16 | 16.6 | 0.7 | 15.9 | 1.6 | |
000029 | 06410328+0957549 | 100.26367 | 9.96528 | 4396 | 307 | 550.8 | 6.1 | 1 | 8.012 | V+16 | 19.1 | 0.7 | 15.0 | 0.5 | |
000033 | 06410726+0958311 | 100.28026 | 9.97533 | 4376 | 224 | 552.4 | 16.0 | 1 | 2.586 | V+16 | 21.5 | 1.6 | 34.7 | 1.7 | |
000038 | 06411088+1000409 | 100.29532 | 10.01136 | 6289 | 7 | 34.8 | 4.3 | 1 | 3.615 | V+16 | 13.6 | 0.7 | 24.0 | 0.5 | (1) |
Notes. Only the first five lines of Table 1 are shown here. The full table is only available in electronic form at the CDS.
1: EW(Li) is corrected from line blends contribution using stellar models (see text); 2: EW(Li) is measured separately from line blends (UVES spectra only); 3: Only an EW(Li) upper limit could be derived.
V+16: Venuti et al. (in prep.); L+04: Lamm et al. (2004); M+04: Makidon et al. (2004); A+13: Affer et al. (2013); LRpv: L. Rebull, priv. comm. (1) This source has low EW(Li) for its Teff and a discrepant Vrad (see text); (2) This source has low EW(Li) for its Teff (see text); (3) This source has multiple periods detected in its light curve (see text).
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