Table 1: Linear relations between the $\gamma $-velocities and the $\gamma $-asymmetries $ V_{\gamma } = a_{{\rm0}} A_{\gamma } + b_{{\rm0}}$ for all stars. The last column corresponds to the final physically calibrated $\gamma $-velocities for each star (see Sect. 3.1 for details). The subscripts give the $1\sigma $ uncertainty.

Name		 HD Pa $a_{{\rm0}}$ $\chi_{{\rm red}}^2$ $V_{\gamma {\rm GCD}}$ Correction $b_{{\rm0}}$ $V_{\gamma \star}$
    [days] [km s-1/%]   [km s-1] [km s-1] [km s-1]
R TrA 135592 3.38925 $ -0.13 _{\pm 0.05 }$ 3 -13.2 $ 1.9 _{\pm 0.3 }$ $ -11.3 _{\pm 0.3 }$
S Cru 112044 4.68976 $ -0.16 _{\pm 0.07 }$ 2 -7.1 $ 3.6 _{\pm 0.4 }$ $ -3.5 _{\pm 0.4 }$
Y Sgr 168608 5.77338 $ -0.19 _{\pm 0.04 }$ 14 -2.5 $ 1.0 _{\pm 0.2 }$ $ -1.5 _{\pm 0.2 }$
$\beta $ Dor 37350 9.84262 $ -0.16 _{\pm 0.02 }$ 30 7.4 $ 2.4 _{\pm 0.1 }$ $ 9.8 _{\pm 0.1 }$
$\zeta$ Gem 52973 10.14960 $ -0.11 _{\pm 0.02 }$ 22 6.9 $ 0.2 _{\pm 0.1 }$ $ 7.1 _{\pm 0.1 }$
RZ Vel 73502 20.40020 $ -0.14 _{\pm 0.09 }$ 1 24.1 $ 0.5 _{\pm 0.4 }$ $ 24.6 _{\pm 0.4 }$
$\ell$ Car 84810 35.55134 $ -0.15 _{\pm 0.03 }$ 15 3.6 $ 0.8 _{\pm 0.1 }$ $ 4.4 _{\pm 0.1 }$
RS Pup 68860 41.51500 $ -0.13 _{\pm 0.05 }$ 4 22.1 $ 3.6 _{\pm 0.2 }$ $ 25.7 _{\pm 0.2 }$
$\textstyle \parbox{12cm}{ $^{a}$\space The corresponding Julian dates ($T_{{\rm o}}$ ) can be found in Paper~II.}$


Source LaTeX | All tables | In the text