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Table A.3

Same as Table A.1 for targets 10–14.

Star HD 47186 HD 51608 HD 93385 HD 96700 HD 115617
d [parsec] 39.6 ± 1.01 34.8 ± 0.71 42.2 ± 1.31 25.7 ± 0.41 8.56 ± 0.021
V [mag] 7.63 ± 0.012 8.17 ± 0.012 7.49 ± 0.012 6.50 ± 0.012 4.73 ± 0.014
K [mag] 6.01 ± 0.033 6.33 ± 0.023 6.07 ± 0.023 5.00 ± 0.023 2.96 ± 0.243
Spectral type G5V4 G7V4 G2/G3V4 G1/G2V4 G5V4
Teff [K]a 5675 ± 505 5360 ± 505 5975 ± 505 5845 ± 505 5575 ± 505
[Fe/H] [dex] 0.23 ± 0.025 -0.07 ± 0.015 0.02 ± 0.015 −0.18 ± 0.015 0.01 ± 0.055
M∗ [M⊙] 1.03 ± 0.075 0.86 ± 0.065 1.04 ± 0.075 0.96 ± 0.075 0.94 ± 0.085
Bolometric correction −0.100 ± 0.0106 −0.176 ± 0.0166 −0.049 ± 0.0076 −0.069 ± 0.0086 −0.120 ± 0.0126
R∗ [R⊙]a 1.10 ± 0.02 0.91 ± 0.02 1.15 ± 0.02 1.16 ± 0.02 0.98 ± 0.02
log g [cgs] 4.37 ± 0.04 4.45 ± 0.04 4.33 ± 0.04 4.29 ± 0.04 4.43 ± 0.05
RV
Data HARPS: 667+67 HARPS: 1188+92 HARPS: 1278+106 HARPS: 1468+98 AAT: 12610
+ Keck: 8010
Model 2 Keplerians 2 Keplerians 3 Keplerians 2 Keplerians 3 Keplerians
+ quadratic trend + quadratic trend
+ CCF function + CCF function
Jitter noise [m s-1] 0.9 1.2 1.3 1.6 Keck: 2.3
AAT: 2.2
Planet HD 47186 b7 HD 51608 b8,9 HD 93385 d10 HD 96700 b7,10 HD  115617 b11
Mpsini [M⊕] 23.2 ± 1.1 13.12 ± 0.77 3.97 ± 0.48 9.05 ± 0.64 5.86 ± 0.66
Min. Rp [R⊕]c 1.77 ± 0.02 1.54 ± 0.02 1.11 ± 0.03 1.40 ± 0.02 1.24 ± 0.04
Min. (Rp/R∗)2 [ppm]c 217 ± 9 239 ± 13 79 ± 7 121 ± 6 135 ± 9
Teq [K]d 1277 ± 22 749 ± 14 1129 ± 19 1087 ± 19 1190 ± 24
T0-2 450 000 [BJDTDB] 5179.972 ± 0.021 6364.17 ± 0.27 6521.26 ± 0.16 5280.71 ± 0.17
P [d] 4.084575 ± 0.000043 14.0702 ± 0.0015 7.3422 ± 0.0014 8.12541 ± 0.00068 4.21504 ± 0.00061
Wb = 0 [min] 190 ± 6 255 ± 11 174 ± 9
K [m s-1] 9.1 ± 1.3 3.85 ± 0.14 4.51 ± 0.15 2.97 ± 0.15 2.44 ± 0.24
a [AU] 0.0505 ± 0.0012 0.1084 ± 0.0025 0.0749 ± 0.0017 0.0780 ± 0.0019 0.0500 ± 0.0014
e 0.039 ± 0.014
ω [deg] 57 ± 23 87 ± 60 293 ± 74
Prior Ptransit [%] 10.45 ± 0.34
Prior Poccultation [%] 9.84 ± 0.31 3.84 ± 0.17

Reference. (1) Van Leeuwen (2007); (2) Hog et al. (2000); (3) Skrutskie et al. (2006); (4) Kharchenko (2001); (5) Santos et al. (2013); (6) Flower (1996); (7) Bouchy et al. (2009); (8) Mayor et al. (2011); (9) Udry et al. (in prep.); (10) Queloz et al. (in prep.); (11) Vogt et al. (2010).

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