All Tables

Table 1: Log of the observations.
Table 2: List of the six line pairs used to derive the stellar temperature.
Table A.1: Object ID, coordinates (Equinox J2000, Epoch J2000.13), photometry, and proper motions of the targets (see Yadav et al. 2008, for details). In the last column the names of the stars according to Sanders (1977) or to Montgomery et al. (1993) are given. For a few stars, two names are given, because both stars are within 1 arc sec circle, according to SIMBAD database.
Table A.2: Radial velocities, effective temperatures, and lithium abundances of the 59 stars retained as possible single members. The values in Table are derived by adding the difference of $T_{\rm eff}$ between the stars and the Sun to the solar temperature (5777 K). The solar temperature derived from the GIRAFFE spectrum and our calibrations is 5792 and 5717 K for the LDR and H $\alpha$ methods, respectively. The 10 best solar twin candidates are indicated in bold face. The S/N /pixel of the co-added spectra varies between 80 and 110, depending on the magnitude of the stars.
Table A.3: Radial velocities of likely binaries or non members. For these stars, each of the three RV measurements is given. Fields with blanks indicate that problems were present with the cross-correlation profile of these objects.