All Tables

Table 1: Sampled stars per spectral type.
Table 2: Absorption features selected to calculate radial velocities from wavelength shifts.
Table 3: Properties of high radial velocity stars.
Table 4: Summary of X-ray source counts predictions for each spectral type and range of age derived from XCOUNT (from Paper I).
Table 5: Summary of F6-F9, G and K observations derived in this work vs. scaled predictions derived from XCOUNT, for each range of age. For 8 stars of our sample of late-F to G and K stars we did not measure lithium EWs (upper limits) due to the low S/N ratio of their spectra and/or high rotation.
Table A.1: Observing Log for the NEP spectra. Scan numbers are from Gioia et al. (2003).
Table A.2: Results: $V_{\rm rad}$ , $V_{\rm rot}$ , Li equivalent width, Li abundance, Binarity.
Table A.3: Presence of H $\alpha$ and Na I(D₁,D₂) emission and presence of lithium feature (6707.8 Å).