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Table 4:

Stellar properties.
Star Spect. MK Teff Ref. Mass [Fe/H] Ref. Derived $T_{\rm eff}$ $v\sin i$ $\log R'_{HK}$ Instr. Radius
  Type   K   [$M_{\odot}$]     K km s-1     [$R_{\odot}$]

GJ 663 A
K0V - -   - -0.20 (3) 4843 $\pm$ 134 - - VINCI 0.817 $\pm$ 0.016
GJ 166 A K0.5V 3.90 $\pm$ 0.02 5201 (3) 0.877 $\pm$ 0.044 -0.25 (3) 5269 $\pm$ 35 0.78 -4.87 AMBER 0.770 $\pm$ 0.021
GJ 570 A K4V 4.20 $\pm$ 0.03 4758 (3) 0.802 $\pm$ 0.040 0.06 (3) 4597 $\pm$ 101 1.50 -4.48 VINCI 0.739 $\pm$ 0.019
GJ 845 K5V 4.38 $\pm$ 0.03 4630 (3) 0.762 $\pm$ 0.038 -0.06 (3) 4568 $\pm$ 59 1.46 -4.56 VINCI 0.732 $\pm$ 0.006
GJ 879 K5Vp 4.54 $\pm$ 0.08 4574 (3) 0.725 $\pm$ 0.036 0.02 (3) 4711  $\pm$ 134 2.93 -4.27 AMBER 0.629 $\pm$ 0.051
GJ 887 M0.5V 5.78 $\pm$ 0.03 3626 (1) 0.503 $\pm$ 0.025 -0.22 (4) 3797  $\pm$ 45 - - AMBER 0.459 $\pm$ 0.011
GJ 551 M5.5V 8.80 $\pm$ 0.04 3042 (1) 0.123 $\pm$ 0.006 0.19 (2) 3098 $\pm$ 56 - - AMBER 0.141 $\pm$ 0.007
References: For $T_{\rm eff}$ and [Fe/H]:
(1) Ségransan et al. (2003); (2) Edvardsson et al. (1993); (3) CORALIE and (4) Woolf & Wallerstein (2005).
For $v\sin i$ and $\log R'_{HK}$: CORALIE.
Masses for M-dwarfs are derived from Delfosse et al. (2000) while empirical relation from Xia et al. (2008) is used for K-dwarfs.
Metallicity values provided are all directly determined by spectroscopy.

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