Table C.1
GES parameters (see the exemplified Tables C.4 and C.5 for cluster NGC 2516).
| Column name | Description |
|---|---|
| CNAME | GES object name from coordinates |
| RA | Right ascension in J2000 (hrs) |
| DEC | Declination in J2000 (deg) |
| VRAD | Radial velocity (km s−1) |
| E_VRAD | Error in radial velocity (km s−1) |
| VSINI | υsini rotational velocity (km s−1) |
| E_VSINI | Error in υsini (km s−1) |
| TEFF | Effective temperature Teff (K) |
| E_TEFF | Error in Teff (K) |
| TEFF_IRFM | Infrared photometric temperature (K) (a) |
| E_TEFF_IRFM | Error in infrared photometric temperature (K) |
| LOGG | logg surface gravity (dex) (b) |
| E_LOGG | Error in logg (dex) |
| GAMMA | γ index (c) (dex) |
| E_GAMMA | Error in γ index (dex) |
| FEH | [Fe/H] metallicity (dex) |
| E_FEH | Error in [Fe/H] metallicity (dex) |
| EWC_LI | Blends-corrected values of EW(Li) (mǺ) |
| E_EWC_LI | Error in EW(Li) (mǺ) |
| LIM_EWC_LI | Flag for blends-corrected EW(Li) error (d) |
| EW_LI_UNVEIL | The primarily-used veiling-corrected values of EW(Li) (mǺ) |
| E_EW_LI_UNVEIL | Error in EW(Li) (mǺ) |
| LIM_EW_LI_UNVEIL | Flag for veiling-corrected EW(Li) errors (d) |
| LI1 | A(Li) neutral Li abundances in logϵ(X) (dex) |
| E_LI1 | Error in A(Li) (dex) |
| EW_HA_ACC | Hα EW: accretion (Ǻ) |
| E_EW_HA_ACC | Error in Hα EW: accretion (Ǻ) |
| HA10 | Hα 10%, width of the Hα emission line at 10% peak intensity (km s−1) |
| E_HA10 | Error in Hα 10% (km s−1) |
| EW_HA_CHR | Hα chromospheric activity (Ǻ) |
| E_EW_HA_CHR | Error in Hα chromospheric activity (Ǻ) |
Notes. (a)Not shown in Table C.4, primarily measured for young clusters. (b)Used in this work for intermediate-age and old clusters. (c)The empirical gravity indicator defined by Damiani et al. (2014) and used in the case of the young clusters. (d)0=no flag necessary; 1 = EW(Li) corrected by blends contribution using models; 2 = EW(Li) measured separately – Li line resolved, UVES only; and 3=Upper limit – no error for EW(Li) is given.
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