Table 3: Sample table of the HARPS GTO ``high precision'' spectroscopic catalogue. We provide the star name, effective temperature, surface gravity, micro turbulence, [Fe/H], the number of iron lines used in the spectroscopic analysis, a mass estimate, the surface gravity computed from the parallaxes, the luminosity of the star, and an indication of whether it hosts a planet. In the electronic table, we also indicate the error in the luminosity and the computed absolute magnitude of the stars.
Star ID $T_{{\rm eff}}$ $\log{g}_{\rm spec}$ $\xi_{{\rm t}}$ [Fe/H] N(Fe I, Fe II) Mass $\log{g}_{\rm hipp}$ Luminosity planet host?
  [K] [cm s-2] [km s-1]     [$M_{\odot }$] [cm s-2] [$L_{\odot}$]  
... ... ... ... ... ... ... ... ... ...
HD 63454 4840 $\pm$ 66 4.30 $\pm$ 0.16 0.81 $\pm$ 0.14 0.06 $\pm$ 0.03 227, 27 0.66 4.55 0.25 yes
HD 63765 5432 $\pm$ 19 4.42 $\pm$ 0.03 0.82 $\pm$ 0.03 -0.16 $\pm$ 0.01 249, 32 0.83 4.51 0.55 no
HD 65216 5612 $\pm$ 16 4.44 $\pm$ 0.02 0.78 $\pm$ 0.03 -0.17 $\pm$ 0.01 256, 34 0.87 4.48 0.71 yes
HD 65277 4802 $\pm$ 88 4.43 $\pm$ 0.18 0.55 $\pm$ 0.34 -0.31 $\pm$ 0.04 257, 32 0.49 4.49 0.21 no
HD 65562 5076 $\pm$ 47 4.39 $\pm$ 0.09 0.45 $\pm$ 0.18 -0.10 $\pm$ 0.03 252, 34 0.72 4.51 0.37 no
HD 65907A 5945 $\pm$ 16 4.52 $\pm$ 0.02 1.05 $\pm$ 0.02 -0.31 $\pm$ 0.01 256, 34 0.93 4.37 1.24 no
HD 66221 5635 $\pm$ 25 4.40 $\pm$ 0.04 0.92 $\pm$ 0.03 0.17 $\pm$ 0.02 260, 35 0.96 4.40 0.95 no
HD 66428 5705 $\pm$ 27 4.31 $\pm$ 0.06 0.96 $\pm$ 0.03 0.25 $\pm$ 0.02 258, 35 1.01 4.31 1.28 yes
HD 67458 5891 $\pm$ 12 4.53 $\pm$ 0.02 1.04 $\pm$ 0.01 -0.16 $\pm$ 0.01 256, 35 0.98 4.45 1.02 no
HD 68607 5215 $\pm$ 45 4.41 $\pm$ 0.08 0.82 $\pm$ 0.08 0.07 $\pm$ 0.03 251, 35 0.81 4.52 0.45 no
HD 68978A 5965 $\pm$ 22 4.48 $\pm$ 0.02 1.09 $\pm$ 0.02 0.05 $\pm$ 0.02 260, 34 1.08 4.43 1.24 no
HD 69655 5961 $\pm$ 12 4.44 $\pm$ 0.03 1.15 $\pm$ 0.01 -0.19 $\pm$ 0.01 249, 34 0.98 4.36 1.33 no
HD 69830 5402 $\pm$ 28 4.40 $\pm$ 0.04 0.80 $\pm$ 0.04 -0.06 $\pm$ 0.02 255, 36 0.82 4.46 0.60 yes
HD 70642 5668 $\pm$ 22 4.40 $\pm$ 0.04 0.82 $\pm$ 0.03 0.18 $\pm$ 0.02 253, 36 0.98 4.42 0.95 yes
... ... ... ... ... ... ... ... ... ...

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