Table 6: Visual magnitude, VT, parallax, absolute magnitude MVT, bolometric correction BC, bolometric magnitudes and luminosities of the sample stars. The last column refers to the luminosity uncertainty due to error propagation of the involved quantities.
Star VT $\pi$ (mas) MVT BC $M_{\rm BOL}$ $\sigma_{M_{\rm BOL}}$ $\log (L_{\star} / L_{\odot}$) $\sigma_{\log (L_{\star} / L_{\odot})}$

HR 440		 4.05 22.15 +0.78 -0.34 +0.44 0.04 1.75 0.02
HR 649 4.47 9.01 -0.76 -0.22 -0.98 0.21 2.32 0.09
HR 1016 5.60 7.75 +0.04 -0.23 -0.19 0.14 2.00 0.05
HR 1326 3.98 27.85 +1.21 -0.39 -0.81 0.03 1.60 0.01
HR 2392 6.39 8.25 +0.97 -0.28 +0.68 0.16 1.65 0.07
HR 4608 4.22 19.08 +0.63 -0.29 +0.34 0.06 1.79 0.03
$\epsilon $ Vir 2.95 31.90 +0.47 -0.23 +0.24 0.04 1.83 0.02
HR 5058 5.24 15.73 +1.23 -0.34 +0.89 0.08 1.57 0.03
HR 5802 5.36 13.89 +1.07 -0.26 +0.82 0.09 1.60 0.04
HR 7321 6.52 6.68 +0.64 -0.33 +0.31 0.21 1.80 0.08
HR 8115 3.31 21.62 -0.01 -0.29 -0.31 0.03 2.05 0.01
HR 8204 3.86 8.19 -1.57 -0.18 -1.76 0.18 2.63 0.07
HD 205011 6.54 6.31 +0.54 -0.34 +0.20 0.15 1.85 0.06
HR 8878 5.21 9.56 +0.11 -0.52 -0.41 0.13 2.09 0.05


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