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Table A.1:

Spectral-type reference stars and radial velocity standards (marked with *).
HD/GJ SpT $V_{\rm r} \pm \sigma_{V_{\rm r}}$ Ref$_{\rm v}$ $v \sin i$ Ref$_{\rm r}$ $S \pm \sigma_{\rm S}$ Observing run
    (km s-1)   (km s-1)      
212754 F7 V -17.8 $\pm$ 1.2 a 7.9 $\pm$ 0.7 j 0.142 $\pm$ 0.001 4, 5
43587 * F9 V   4.6 $\pm$ 0.1 b ...   0.158 $\pm$ 0.001 5, 6
84737 * G0.5 V   6.0 $\pm$ 1.1 b 2.8 $\pm$ 0.8 j 0.144 $\pm$ 0.000 10
10307 G2 V ...   2.1 $\pm$ 0.5 k 0.152 $\pm$ 0.003 7
193664 G3 V  -4.7 $\pm$ 1.2 a ...   0.161 $\pm$ 0.004 7
25680 G5 V  24.0 $\pm$ 0.1 c 7.0 $\pm$ 0.7 j 0.281 $\pm$ 0.000 5, 7
31966 G5 V -18.1 $\pm$ 0.1 c ...   ... 5
71148 * G5 V -31.0 $\pm$ 0.7 b ...   1.570 $\pm$ 0.000 10
159222 * G5 V -50.5 $\pm$ 1.2 b ...   0.164 $\pm$ 0.002 1, 4, 11
182488 * G8 V -21.5 d 0.6 $\pm$ 0.5 k 0.155 $\pm$ 0.008 1, 4, 11
48432 K0 III  17.9 $\pm$ 0.2 e <1.0 e 0.120 $\pm$ 0.000 5, 6
62509 * K0 III   3.2 $\pm$ 0.3 b 1.7 $\pm$ 0.5 k 0.140 $\pm$ 0.019 3
100696 * K0 III   0.2 $\pm$ 0.5 b 1.2 $\pm$ 1.0 l ... 10
197989 K0 III -10.6 $\pm$ 0.5 a 2.0 $\pm$ 0.5 k 0.104 $\pm$ 0.001 1, 2, 4, 7, 8, 11
3651 * K0 V -32.8 $\pm$ 0.8 b 2.2 $\pm$ 0.5 k 0.191 $\pm$ 0.001 2, 3, 4, 5, 7
97004 K0 V   5.4 $\pm$ 0.1 c ...   ... 10
112758 K0 V  -4.1 $\pm$ 1.2 a ...   0.206 $\pm$ 0.000 10
136442 * K0 V -45.6 $\pm$ 0.8 b ...   ... 10
185144 K0 V  26.7 $\pm$ 0.1 c 0.6 $\pm$ 0.5 k 0.195 $\pm$ 0.003 11
201651 K0 V -13.7 $\pm$ 1.2 a ...   ... 4, 7, 8
92588 * K1 IV  43.5 $\pm$ 0.3 f <1.0 e ... 9, 10
10476 * K1 V -33.9 $\pm$ 0.9 b 0.6 $\pm$ 0.5 k 0.192 $\pm$ 0.001 1, 5
12929 * K2 III -14.6 $\pm$ 0.2 g 1.8 $\pm$ 0.5 k 0.118 $\pm$ 0.002 5
124897 * K2 III  -5.3 $\pm$ 0.3 g 3.3 $\pm$ 0.5 k 0.144 $\pm$ 0.012 6, 10
161096 * K2 III -12.5 $\pm$ 0.3 g 2.5 $\pm$ 0.5 k 0.103 $\pm$ 0.002 1, 4, 11
201196 K2 IV -34.8 $\pm$ 0.2 e <1.0 e ... 1, 5
4628 * K2 V -10.1 $\pm$ 0.4 f 0.0 $\pm$ 0.5 h 0.223 $\pm$ 0.001 2, 5, 8, 12
136713 K2 V  -6.0 $\pm$ 0.1 c 3.8 $\pm$ 5.7 m ... 6
166620 K2 V   6.9 $\pm$ 0.1 h 0.0 $\pm$ 0.4 h 0.193 $\pm$ 0.001 1, 2, 4, 6, 7, 9, 10, 11
16160 K3 V  25.8 $\pm$ 0.1 c 1.0 $\pm$ 1.0 h 0.221 $\pm$ 0.002 8
219134 K3/4 V -18.6 $\pm$ 0.1 c 2.1 $\pm$ 0.5 k 0.229 $\pm$ 0.003 1, 2, 4, 5, 11
29139 * K5 III  54.2 $\pm$ 0.2 g 2.0 $\pm$ 1.0 e ... 4, 6, 7
154363 K5 V  34.1 $\pm$ 0.1 c 3.7 $\pm$ 5.9   0.197 $\pm$ 0.001 1, 6, 10
201091 K5 V   7.0 $\pm$ 0.1 h 0.0 $\pm$ 0.8 h 0.613 $\pm$ 0.006 1, 4, 5, 6, 7, 8, 10, 11
GJ 910 K5 V   2.0 i 0.0 $\pm$ 0.0 m ... 7
151877 K7 V   2.0 $\pm$ 0.1 c 0.0 $\pm$ 0.0 m ... 1
201092 K7 V   7.2 $\pm$ 0.1 h 1.7 $\pm$ 0.6 h 0.922 $\pm$ 0.011 1, 4, 5, 6, 7, 8, 10, 11
GJ 466 M0 V  -5.0 $\pm$ 5.0 a ...   ... 10
147379 M0 V -18.8 $\pm$ 0.1 c 4.2 $\pm$ 6.2 m 1.761 $\pm$ 0.160 11
GJ 720A M0 V -25.0 $\pm$ 2.5 a 6.3 $\pm$ 1.7 m ... 7
GJ 16 M0/1 V ...   ...   ... 8
GJ 806 M1.5 V -24.7 $\pm$ 0.1 c 1.9 $\pm$ 0.7 n ... 11
18884 * M2 III -26.1 $\pm$ 0.3 g ...   0.331 $\pm$ 0.004 8
115521 * M2 III -28.6 $\pm$ 2.3 g ...   ... 6, 10
95735 M2 V -84.7 $\pm$ 0.1 c 0.0 $\pm$ 0.0 n 0.392 $\pm$ 0.009 6, 10
GJ 687B$^{\dag }$ M3.5 V -28.8 $\pm$ 0.1 c ...   ... 6, 10

Notes.  $^{(\dag )}$ The radial velocity given for GJ 687B is that of GJ 687A.

References. a Dufflot et al. (1995), WEB (Wilson Evans Batten Catalogue); b Barnes et al. (1986); c Nidever et al. (2002); d ELODIE;  e De Medeiros & Major (1999); f Beavers et al. (1979); g Udry et al. (1999); h Benz & Major (1984); i Dyer (1954); j Soderblom (1982), Soderblom et al. (1989); k Fekel (1997); l De Medeiros et al. (2000); m Tokovinin (1992); n Marcy & Chen (1992).


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