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Table 2:

Determined atmospheric parameters for CoRoT-7, the Sun, and $\alpha $ Cen B.
  $\langle$Fe  I- II$\rangle$ $\langle$Mg 1b$\rangle$ $\langle$Ca6122$\rangle$ $\langle$Ca6162$\rangle$ $\langle$Ca6439$\rangle$ $\langle$Isol. lines$\rangle$
Spec. $T_{\rm eff}$ [K] $\log g$ [Fe/H] $v_{\rm micro}$ [km s-1] $\log g$ $\log g$ $\log g$ $\log g$ $v \sin i$ $v_{\rm macro}$
H1 $ 5180\pm67$ $ 4.30\pm0.08$ $+0.11\pm0.13$ $ 0.98\pm0.07$ $3.89\pm0.46 $ $4.44\pm0.08$ $4.43\pm0.10 $ $4.34\pm0.19 $ 1.3 1.2
H1 SME $ 5280\pm44$ $ 4.44\pm0.06$ $+0.13\pm0.06$ $ 0.80\pm0.07$ 4.62 4.66 4.53      
H2 $ 5300\pm41$ $ 4.46\pm0.08$ $+0.14\pm0.13$ $ 0.80\pm0.09$ $4.02\pm0.47 $ $4.43\pm0.05$ $4.56\pm0.06 $ $4.13\pm0.35 $ 1.1 1.2
H3 $ 5350\pm31$ $ 4.57\pm0.06$ $+0.15\pm0.09$ $ 0.76\pm0.07$ $4.14\pm0.44 $ $4.50\pm0.09$ $4.77\pm0.07 $ $4.72\pm0.26 $ 1.1 1.2
H1-7 $ 5280\pm35$ $ 4.48\pm0.06$ $+0.13\pm0.09$ $ 0.80\pm0.05$ $3.94\pm0.52 $ $4.47\pm0.06$ $4.60\pm0.08 $ $4.32\pm0.27 $ 0.9 1.4
H1-107 $ 5300\pm25$ $ 4.54\pm0.05$ $+0.13\pm0.08$ $ 0.77\pm0.05$ $3.91\pm0.55 $ $4.51\pm0.06$ $4.58\pm0.05 $ $4.45\pm0.18 $    
H1-107 SME $5290\pm44$ $ 4.49\pm0.06$ $+0.13\pm0.06$ $ 0.80\pm0.05$ 4.43 4.49 4.49      
U1 $ 5300\pm17$ $ 4.50\pm0.03$ $+0.11\pm0.06$ $ 0.70\pm0.08$ $3.94\pm0.49 $ $4.42\pm0.05$ $4.46\pm0.06 $ $4.41\pm0.19 $    
Ceres $ 5767\pm17$ $ 4.44\pm0.03$ $-0.01\pm0.03$ $ 1.01\pm0.03$ $4.50\pm0.08 $ $4.46\pm0.20$ $4.43\pm0.10 $ $4.43\pm0.42$ 1.4 2.1
Ganymede $ 5757\pm17$ $ 4.43\pm0.04$ $-0.00\pm0.04$ $ 0.93\pm0.03$ $4.51\pm0.10 $ $4.33\pm0.17$ $4.38\pm0.08 $ $4.47\pm0.37$ 1.1 2.3
Moon $ 5775\pm25$ $ 4.48\pm0.03$ $+0.02\pm0.04$ $ 0.91\pm0.04$ $4.41\pm0.08 $ $4.53\pm0.20$ $4.41\pm0.14 $ $4.50\pm0.33$ 2.1 2.2
$\alpha $ Cen B $ 5185\pm25$ $ 4.50\pm0.03$ $+0.31\pm0.05$ $ 0.83\pm0.04$ $4.01\pm0.50 $ $4.53\pm0.07$ $4.51\pm0.05 $ $4.65\pm0.16$ 1.0 0.8

Notes. Results are from VWA except H1 and H1-107, which are also given for the SME analysis. The 1-$\sigma $ uncertainties are internal errors.


Source LaTeX | All tables | In the text

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