Table 2
Coordinates, photometry and measurements of RV, EW(Li), vsini and estimated masses for 208 targets selected as Gamma Vel members.
| CNAME | RA | Dec | V | V − I | S/N | N | EW(Li) | ΔEW(Li) | RV | σRV | P A | vsini | M/M⊙ |
| (J2000) | (mÅ) | (km s-1) | (km s-1) | ||||||||||
|
|
|||||||||||||
| 08064077-4736441 | 08:06:41 | −47:36:44 | 13.48 | 1.31 | 135 | 1 | 425.8 | 1.7 | 61.14 | 0.25 | −1.0 | 1.2 | 1.23 |
| 08064390-4731532 | 08:06:44 | −47:31:53 | 17.65 | 2.67 | 21 | 1 | 178.2 | 14.3 | 16.54 | 0.31 | 0.85 | 13.7 | 0.45 |
| 08065007-4732221 | 08:06:50 | −47:32:22 | 18.22 | 2.72 | 13 | 1 | 452.7 | 22.0 | 20.89 | 0.37 | 0.05 | 1.0 | 0.43 |
Notes. The full table is available in electronic format at the CDS; a sample is shown here. N is the number of individual observations contributing to the mean values quoted. PA is the probability that the star belongs to kinematic population A, but is set to − 1 if the RV is outside the range 8 to 26 km s-1. Although values of vsini < 10 km s-1 are reported in the GESviDR1Final tables, we suspect that subsequent analysis will likely suggest these are unreliable and we treat them as upper limits at 10 km s-1 in Sect. 4.2.4. Masses are estimated from the V − I colour and models of Baraffe et al. (1998) for an assumed age of 10 Myr.
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