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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 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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