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Table 3

Stellar and planetary parameters of the exoplanet host star sample.

Name Spectral Distance L ⋆ T ⋆ [Fe/H] Ca ii Age X-ray Age N Planet a M sini b a c e Planet d Ref.
Type [pc] [L⊙] [K] [Gyr] [Gyr] [MJup] [AU]
HD 1237 G8 V 17.49 ± 0.09 0.643 5514 0.07 0.3 0.4 1 3.37 ± 0.09 0.4947 ± 0.0083 0.511 ± 0.017 1
HD 3651 K0 V 11.06 ± 0.04 0.529 5204 0.16 6.4 4.5 1 0.229 ± 0.015 0.2947 ± 0.0049 0.63 ± 0.04 2
HD 4308 G3 V 22.06 ± 0.16 1.012 5670 −0.24 4.0 4.5 1 0.0405 ± 0.005 0.118 ± 0.0009 0.27 ± 0.12 3
υ And F8 V 13.49 ± 0.03 3.363 6155 0.10 7.3 2.9 3 4.12 ± 0.165 2.525 ± 0.042 0.013 ± 0.016 4
q1 Eri F8 V 17.43 ± 0.08 1.523 6155 −0.04 1.2 0.8 1 0.93 ± 0.18 2.03 ± 0.15 0.1 ± 0.01 5
τ Ceti G8 V 3.65 ± 0.01 0.526 5312 −0.43 8.5 ... 5 0.02 ± 0.01 1.35 ± 0.09 0.16 6
GJ 86 K0 V 10.78 ± 0.04 0.406 5165 −0.22 1.5 3.6 1 4.00 ± 0.137 0.1142 ± 0.0019 0.0416 ± 0.0072 7
ι Hor F8 V 17.17 ± 0.06 1.520 6227 0.19 1.6 0.5 1 2.05 ± 0.20 0.924 ± 0.016 0.14 ± 0.13 8
HD 19994 F8 V 22.58 ± 0.14 3.848 6187 0.21 5.67 1.2 1 1.33 ± 0.11 1.306 ± 0.022 0.266 ± 0.014 9
HD 20794 G8 V 6.04 ± 0.01 0.663 5413 −0.34 6.22 10.4 3 0.0148 ± 0.0018 0.3498 ± 0.0058 0 10
ϵ Eri K2 V 3.22 ± 0.01 0.425 5061 −0.08 0.8 ... 1 1.05 ± 0.19 3.38 ± 0.32 0.25 ± 0.23 11
HD 33564 F6 V 20.88 ± 0.09 3.224 6307 0.10 5.7 1.2 1 9.13 ± 0.37 1.124 ± 0.020 0.34 ± 0.02 12
HD 39091 G1 IV 18.32 ± 0.07 1.535 6003 0.09 5.1 3.2 1 10.09 ± 0.38 3.35 ± 0.10 0.6405 ± 0.0072 13
HD 40307 K3 V 13.00 ± 0.06 0.245 4979 −0.31 7.3 6.7 3 0.0281 ± 0.0002 0.1324 ± 0.0022 0 14
HD 69830 K0 V 12.49 ± 0.05 0.595 5405 −0.04 6.4 3.3 3 0.0563 ± 0.0052 0.627 ± 0.012 0.10 ± 0.04 15
55 Cnc G8 V 12.34 ± 0.11 0.602 5295 0.36 8.4 11.2 5 3.835 ± 0.08 5.475 ± 0.094 0.004 ± 0.003 4
47 UMa G0 V 14.06 ± 0.05 1.600 5908 0.03 4.9 ... 3 2.546 ± 0.096 3.570 ± 0.111 0.032 ± 0.014 16
HD 99492 K2 V 17.96 ± 0.46 0.327 4810 0.26 4.0 13.0 2 0.36 ± 0.02 5.4 ± 0.1 0.254 ± 0.092 17
HD 102365 G3/G5 V 9.22 ± 0.02 0.839 5630 −0.28 5.7 8.83 1 0.051 ± 0.008 0.4633 ± 0.0078 0.34 ± 0.14 18
61 Vir G5 V 8.56 ± 0.02 0.835 5646 −0.02 6.6 8.0 3 0.0716 ± 0.0093 0.475 ± 0.008 0.12 ± 0.11 19
70 Vir G5 V 17.98 ± 0.08 2.989 5513 −0.07 7.9 5.6 1 7.46 ± 0.25 0.4836 ± 0.0081 0.4007 ± 0.0035 20
τ Boo F7 V 15.62 ± 0.05 3.062 6376 0.26 4.8 0.4 1 5.95 ± 0.28 0.046 0.023 ± 0.015 4
α Cen B K1 V 1.25 ± 0.04 0.444 5178 0.15 5.2 4.27 1 0.00356 ± 0.00028 0.0419 ± 0.0007 0 21
GJ 581 M5 V 6.27 ± 0.09 0.012 3315 −0.02 2.00 7.0 4e 0.0499 ± 0.0023 0.2177 ± 0.0047 0.32 ± 0.09 22
ρ CrB G2 V 17.24 ± 0.08 1.742 5834 −0.19 4.3 <1.09 1 1.064 ± 0.053 0.2257 ± 0.0038 0.057 ± 0.028 23
14 Her K0 V 17.57 ± 0.10 0.653 5336 0.43 6.9 7.5 1 5.21 ± 0.30 2.934 ± 0.084 0.369 ± 0.005 24
HD 154345 G8 V 18.58 ± 0.11 0.617 5488 −0.07 3.8 5.6 1 0.957 ± 0.061 4.21 ± 0.11 0.044 25
μ Ara G5 V 15.51 ± 0.07 1.821 5787 0.29 7.5 ... 4 1.89 ± 0.22 5.34 ± 0.40 0.172 ± 0.040 26
HD 176051 G0 V 14.87 ± 0.08 1.603 5840 −0.11 8.1 1.1 1 1.50 ± 0.30 1.76 ± 0.07 0 27
16 Cyg B G5 V 21.21 ± 0.12 1.271 5772 0.08 7.4 <10.3 1 1.640 ± 0.083 1.660 ± 0.028 0.681 ± 0.017 28
HD 189567 G2 V 17.73 ± 0.14 1.027 5735 −0.22 4.1 ... 1 0.0316 ± 0.0034 0.1099 ± 0.0018 0.23 ± 0.14 29
HD 192310 K3 V 8.91 ± 0.02 0.407 5105 −0.03 7.5 2.9 2 0.0736 ± 0.0098 1.184 ± 0.024 0.13 ± 0.04 30
GJ 832 M1 V 7.86 ± 0.12 0.031 3695 −0.31 ... 9.2 1 0.644 ± 0.075 3.40 ± 0.15 0.12 ± 0.11 31
HD 210277 G0 V 21.56 ± 0.22 1.002 5540 0.22 6.8 ... 1 1.273 ± 0.005 1.131 ± 0.019 0.476 ± 0.017 32
GJ 876 M5 V 4.69 ± 0.05 0.013 3473 0.19 6.5 ... 4 2.2756 ± 0.0045 0.3343 ± 0.0013 0.207 ± 0.055 33
51 Peg G5 V 15.61 ± 0.09 1.368 5791 0.20 8.0 13.6 1 0.461 ± 0.016 0.05211 ± 0.00087 0.013 ± 0.012 34
HD 217107 G8 IV 19.86 ± 0.15 1.162 5646 0.4 8.1 ... 2 2.62 ± 0.15 5.33 ± 0.02 0.1276 ± 0.0052 35

Notes.

(a)

Number of known exoplanets.

(b)

Projected (minimum) mass of the most massive exoplanet.

(c)

Semi-major axis of the outermost exoplanet in the system.

(d)

Eccentricity of innermost exoplanet in the system.

(e)

Vogt et al. (2012) reported strong evidence for a five-planet system. A summary of all reported exoplanets in each system is given in Table 4. Planets for which no eccentricity could be found are assumed to have e = 0.00.

Reference. Discovery references: (1) Naef et al. (2001); (2) Fischer et al. (2003); (3) Udry et al. (2006); (4) Butler et al. (1997); (5) Butler et al. (2006); (6) Tuomi et al. (2013); (7) Queloz et al. (2000); (8) Kürster et al. (2000); (9) Mayor et al. (2004); (10) Pepe et al. (2011); (11) Hatzes et al. (2000); (12) Galland et al. (2005); (13) Jones et al. (2002); (14) Mayor et al. (2009); (15) Lovis et al. (2006); (16) Butler & Marcy (1996); (17) Marcy et al. (2005); (18) Tinney et al. (2011); (19) Vogt et al. (2010); (20) Marcy & Butler (1996); (21) Dumusque et al. (2012); (22) Bonfils et al. (2005); (23) Noyes et al. (1997); (24) Butler et al. (2003); (25) Wright et al. (2007); (26) Butler et al. (2001); (27) Muterspaugh et al. (2010); (28) Cochran et al. (1997); (29) Mayor et al. (2011); (30) Howard et al. (2011); (31) Bailey et al. (2009); (32) Marcy et al. (1999); (33) Delfosse et al. (1998); (34) Mayor & Queloz (1995); (35) Fischer et al. (1999).

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