This is, to the best of my knowledge, a list of all credible planets
orbiting giant stars. Typically, only refereed publications are considered.
Planets orbiting subgiant stars are not included.
The table is now sortable (click on the column headers) and downloadable in csv format!
# | name | hip | V | - | + | K | - | + | sptype | feh | - | + | mstar | - | + | m2sini | - | + | period | - | + | tzero | - | + | ecc | - | + | omega | - | + | mf | - | + | a2 | - | + | Krv | - | + | reference | telescope | remarks |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
[mag] | [mag] | [M_Sun] | [M_Jup] | [days] | [JD] | [deg] | [M_Sun] | [AU] | [m/s] | |||||||||||||||||||||||||||||||||
1 | iota Dra b | 75458 | 3.29 | 0.671 | K2 III | 0.11 | 1.05 | 0.36 | 0.36 | 8.7 | 510.72 | 0.07 | 0.07 | 2452015.36 | 0.16 | 0.16 | 0.713 | 0.008 | 0.008 | 92.5 | 0.7 | 0.7 | 5.227e-7 | 1.27 | 306.0 | 3.8 | 3.8 | Frink et al. 2002; Kane et al. 2010 | Hamilton (Lick) | Additional linear trend. Updated elements here | ||||||||||||
2 | Pollux b | 37826 | 1.16 | -0.936 | K0 IIIb | 0.07 | 1.86 | 2.9 | 0.3 | 0.3 | 589.7 | 3.5 | 3.5 | 2452337.9 | 52 | 70 | 0.06 | 0.04 | 0.04 | 277 | 8 | 8 | 6.2e-9 | 0.6e-9 | 0.6e-9 | 1.69 | 0.03 | 0.03 | 46.9 | 1.5 | 1.5 | Reffert et al. 2006 | Hamilton (Lick) | similar elements by Hatzes et al. 2006 | ||||||||
3 | HD 11977 b | 8928 | 4.68 | 2.590 | G5 III | -0.16 | 2.31 | 6.54 | 621.6 | 2.4 | 2.4 | 2452906.6 | 10 | 10 | 0.3 | 0.03 | 0.03 | 35.5 | 5.8 | 5.8 | 1.89 | 0.005 | 0.005 | Setiawan et al. 2005;Soto et al. 2015 | FEROS; later HARPS and CHIRON | updated elements | ||||||||||||||||
4 | HD 47536 b | 31688 | 5.25 | 2.383 | K1 III | -0.65 | 0.04 | 0.04 | 0.98 | 0.08 | 0.08 | 4.0 | 0.4 | 0.4 | 434.9 | 2.6 | 2.6 | 2453040.8 | 30 | 30 | 0.3 | 0.1 | 0.1 | 268.6 | 17.3 | 17.3 | 1.12 | 0.005 | 0.005 | Setiawan et al. 2003; Soto et al. 2015 | FEROS; Coralie; HARPS; CHIRON | second planet most likely not real | ||||||||||
5 | HD 13189 b | 10085 | 7.57 | 3.997 | K2 II | 4.5 | 2.5 | 2.5 | 14 | 6 | 6 | 471.6 | 6.0 | 6.0 | 2452327.9 | 20.2 | 20.2 | 0.27 | 0.06 | 0.06 | 160.7 | 12.0 | 12.0 | 2.26e-7 | 0.37e-7 | 0.37e-7 | 1.5-2.2 | 173.3 | 9.8 | 9.8 | Hatzes et al. 2005 | Tautenburg; McDonald; HET | ||||||||||
6 | epsilon Tau b | 20889 | 3.53 | 1.422 | K0 III | 0.17 | 0.04 | 0.04 | 2.7 | 0.1 | 0.1 | 7.6 | 0.2 | 0.2 | 594.9 | 5.3 | 5.3 | 0.151 | 0.023 | 0.023 | 1.93 | 0.03 | 0.03 | 95.9 | 1.8 | 1.8 | Sato et al. 2007 | HIDES (Okayama) | ||||||||||||||
7 | HD 104985 b | 58952 | 5.78 | 3.274 | G9 III | -0.35 | 2.3 | 8.3 | 199.505 | 0.085 | 0.085 | 2451927.5 | 3.3 | 3.3 | 0.090 | 0.009 | 0.009 | 203.5 | 5.7 | 5.7 | 0.953e-7 | 0.022e-7 | 0.022e-7 | 0.95 | 166.8 | 1.3 | 1.3 | Sato et al. 2003; Sato et al. 2008a | HIDES (Okayama) | |||||||||||||
8 | NGC2423 No.3 b | 9.45 | 0.14 | 0.09 | 0.09 | 2.4 | 0.2 | 0.2 | 10.6 | 714 | 2453213 | 21 | 21 | 0.21 | 0.07 | 0.07 | 18 | 10 | 10 | 0.180e-6 | 2.10 | 137.6 | 9.1 | 9.1 | Lovis & Mayor 2007 | Coralie; HARPS | ||||||||||||||||
9 | NGC4349 No.127 b | 10.88 | -0.12 | 0.04 | 0.04 | 3.9 | 0.3 | 0.3 | 19.8 | 678 | 2454114 | 34 | 34 | 0.19 | 0.07 | 0.07 | 61 | 19 | 19 | 0.442e-6 | 2.38 | 188 | 13 | 13 | Lovis & Mayor 2007 | Coralie; HARPS | ||||||||||||||||
10 | 4 UMa b | 42527 | 4.59 | 1.734 | K1 III | -0.25 | 0.04 | 0.04 | 1.23 | 0.15 | 0.15 | 7.1 | 1.6 | 1.6 | 269.3 | 0.43 | 0.02 | 0.02 | 2.05e-7 | 0.24e-7 | 0.24e-7 | 216.8 | Döllinger et al. 2007 | Tautenburg | ||||||||||||||||||
11 | HD 17092 b | 7.74 | 4.807 | K0 III | 0.22 | 2.3 | 0.3 | 0.3 | 4.6 | 0.3 | 0.3 | 359.9 | 2.4 | 2.4 | 2452970.0 | 12.3 | 12.3 | 0.166 | 0.062 | 0.062 | 347.4 | 13.4 | 13.4 | 2.001e-8 | 0.11e-8 | 0.11e-8 | 1.29 | 0.05 | 0.05 | 82.4 | 3.2 | 3.2 | Niedzielski et al. 2007 | HET | ||||||||
12 | 11 Com b | 60202 | 4.72 | 2.282 | G8 III | -0.35 | 0.09 | 0.09 | 2.7 | 0.3 | 0.3 | 19.4 | 1.5 | 1.5 | 326.03 | 0.32 | 0.32 | 2452899.6 | 1.6 | 1.6 | 0.231 | 0.005 | 0.005 | 94.8 | 1.5 | 1.5 | 8.68e-7 | 0.21e-7 | 0.21e-7 | 1.29 | 0.05 | 0.05 | 302.8 | 2.6 | 2.6 | Liu et al. 2008 | Xinglong; OAO | |||||
13 | 18 Del b | 103527 | 5.51 | 3.366 | G6 III | -0.052 | 0.023 | 0.023 | 2.3 | 10.3 | 993.3 | 3.2 | 3.2 | 2451672 | 18 | 18 | 0.08 | 0.01 | 0.01 | 166.1 | 6.5 | 6.5 | 1.743e-7 | 0.054e-7 | 0.054e-7 | 2.6 | 119.4 | 1.3 | 1.3 | Sato et al. 2008a | HIDES (Okayama) | |||||||||||
14 | xi Aql b | 97938 | 4.71 | 2.171 | K0 III | -0.205 | 0.039 | 0.039 | 2.2 | 2.8 | 136.75 | 0.25 | 0.25 | 2453001.7 | 1.4 | 1.4 | 0 | 0 | 0.0399e-7 | 0.0031e-7 | 0.0031e-7 | 0.68 | 65.4 | 1.7 | 1.7 | Sato et al. 2008a | HIDES (Okayama) | circular orbit fixed | ||||||||||||||
15 | HD 81688 b | 46471 | 5.40 | 3.056 | K0 III-IV | -0.359 | 0.020 | 0.020 | 2.1 | 2.7 | 184.02 | 0.18 | 0.18 | 2452335.4 | 1.1 | 1.1 | 0 | 0 | 0.0385e-7 | 0.0019e-7 | 0.0019e-7 | 0.81 | 58.58 | 0.97 | 0.97 | Sato et al. 2008a | HIDES (Okayama) | circular orbit fixed | ||||||||||||||
16 | 14 And b | 116076 | 5.22 | 2.331 | K0 III | -0.24 | 0.03 | 0.03 | 2.2 | 0.2 | 0.1 | 4.8 | 185.84 | 0.23 | 0.23 | 2452861.4 | 1.5 | 1.5 | 0 | 0 | 1.936e-6 | 0.0079e-6 | 0.0079e-6 | 0.83 | 100.0 | 1.3 | 1.3 | Sato et al. 2008b | HIDES (Okayama) | circular orbit fixed | ||||||||||||
17 | 81 Cet b | 12247 | 5.65 | 3.266 | G5 III | -0.06 | 0.03 | 0.03 | 2.4 | 0.4 | 0.1 | 5.3 | 952.7 | 8.8 | 8.8 | 2452486. | 26. | 26. | 0.206 | 0.029 | 0.029 | 175.0 | 6.9 | 6.9 | 2.30e-6 | 0.15e-6 | 0.15e-6 | 2.5 | 62.8 | 1.5 | 1.5 | Sato et al. 2008b | HIDES (Okayama) | |||||||||
18 | HD 102272 b | 57428 | 8.69 | 6.259 | K0 III | -0.26 | 0.08 | 0.08 | 1.9 | 5.9 | 0.2 | 0.2 | 127.58 | 0.30 | 0.30 | 2452146.5 | 64 | 64 | 0.05 | 0.04 | 0.04 | 118 | 58 | 58 | 0.614 | 0.001 | 0.001 | 155.5 | 5.6 | 5.6 | Niedzielski et al. 2009a | HET | ||||||||||
19 | HD 102272 c | 57428 | 8.69 | 6.259 | K0 III | -0.26 | 0.08 | 0.08 | 1.9 | 2.6 | 0.4 | 0.4 | 520. | 26 | 26 | 2454135.5 | 260 | 260 | 0.68 | 0.06 | 0.06 | 320 | 10 | 10 | 1.57 | 0.05 | 0.05 | 59 | 11 | 11 | Niedzielski et al. 2009a | HET | ||||||||||
20 | HD 240210 b | 8.33 | K3 III | -0.18 | 0.12 | 0.12 | 0.82 | 0.15 | 0.15 | 5.21 | 501.75 | 2.33 | 2.33 | 2454486.88 | 10.93 | 10.93 | 0.15 | 0.02 | 0.02 | 277.59 | 7.77 | 7.77 | 1.16 | 161.89 | 3.49 | 3.49 | Niedzielski et al. 2009b | HET | ||||||||||||||
21 | BD +20 2457 b | 9.75 | K2 III | -1.00 | 0.07 | 0.07 | 2.8 | 1.5 | 1.5 | 21.42 | 379.63 | 2.01 | 2.01 | 2454677.03 | 28.19 | 28.19 | 0.15 | 0.03 | 0.03 | 207.64 | 21.99 | 21.99 | 1.45 | 322.35 | 9.57 | 9.57 | Niedzielski et al. 2009b | HET | dynamical stability unclear | |||||||||||||
22 | BD +20 2457 c | 9.75 | K2 III | -1.00 | 0.07 | 0.07 | 2.8 | 1.5 | 1.5 | 12.47 | 621.99 | 10.20 | 10.20 | 2453866.95 | 27.99 | 27.99 | 0.18 | 0.06 | 0.06 | 126.02 | 16.54 | 16.54 | 2.01 | 160.03 | 7.21 | 7.21 | Niedzielski et al. 2009b | HET | dynamical stability unclear | |||||||||||||
23 | HD 173416 b | 91852 | 6.057 | G8 III | 2.0 | 0.3 | 0.3 | 2.7 | 0.3 | 0.3 | 323.6 | 2.2 | 2.2 | 2453465.8 | 8.3 | 8.3 | 0.21 | 0.04 | 0.04 | 254 | 11 | 11 | 4.38e-5 | 0.51e-5 | 0.51e-5 | 1.16 | 0.06 | 0.06 | 51.8 | 2.0 | 2.0 | Liu et al. 2009 | CES (Xinglong); HIDES (Okayama) | |||||||||
24 | 42 Dra b | 90344 | 4.833 | K1.5 III | -0.46 | 0.05 | 0.05 | 0.98 | 0.05 | 0.05 | 3.88 | 0.85 | 0.85 | 479.1 | 6.2 | 6.2 | 2452757.4 | 3.7 | 3.7 | 0.38 | 0.06 | 0.06 | 218.7 | 10.6 | 10.6 | 5.29e-8 | 0.62e-8 | 0.62e-8 | 1.19 | 0.01 | 0.01 | 110.5 | 7.0 | 7.0 | Döllinger et al. 2009a | Tautenburg | RV amplitude has changed considerably; see comment in Hrudková et al. 2017 | |||||
25 | HD 139357 b | 76311 | 5.977 | K4 III | -0.13 | 0.05 | 0.05 | 1.35 | 0.24 | 0.24 | 9.76 | 2.15 | 2.15 | 1125.7 | 9.0 | 9.0 | 2452466.7 | 3.2 | 3.2 | 0.10 | 0.02 | 0.02 | 235.4 | 10.6 | 10.6 | 4.79e-7 | 0.57e-7 | 0.57e-7 | 2.36 | 0.02 | 0.02 | 161.2 | 3.2 | 3.2 | Döllinger et al. 2009a | Tautenburg | ||||||
26 | 11 UMi b | 74793 | 5.024 | 0.005 | 0.005 | K4 III | 0.04 | 0.04 | 0.04 | 1.80 | 0.25 | 0.25 | 11.20 | 2.47 | 2.47 | 516.22 | 3.25 | 3.25 | 2452861.04 | 2.06 | 2.06 | 0.08 | 0.03 | 0.03 | 117.63 | 21.06 | 21.06 | 3.61e-7 | 0.44e-7 | 0.44e-7 | 1.54 | 0.07 | 0.07 | 189.70 | 7.15 | 7.15 | Döllinger et al. 2009b | Tautenburg | ||||
27 | HD 32518 b | 24003 | 6.436 | 0.005 | 0.005 | K1 III | -0.15 | 0.04 | 0.04 | 1.13 | 0.18 | 0.18 | 3.04 | 0.68 | 0.68 | 157.54 | 0.38 | 0.38 | 2452950.29 | 13.66 | 13.66 | 0.01 | 0.03 | 0.03 | 306.11 | 126.71 | 126.71 | 2.20e-8 | 0.24e-8 | 0.24e-8 | 0.59 | 0.03 | 0.03 | 115.83 | 4.67 | 4.67 | Döllinger et al. 2009b | Tautenburg | ||||
28 | HD 110014 b | 61740 | 4.657 | K2 III | 0.14 | 2.09 | 13.67 | 2.3 | 2.3 | 936.4 | 44.5 | 44.5 | 2453842.0 | 206.6 | 206.6 | 0.06 | 0.09 | 0.09 | 119.55 | 84.2 | 84.2 | 2.5 | 0.08 | 0.08 | de Medeiros et al. 2009; Soto et al. 2015 | FEROS; HARPS; Coralie | second planet signal could be real | |||||||||||||||
29 | HD 119445 b | 66892 | 6.30 | G6 III | 0.04 | 0.18 | 0.18 | 3.9 | 0.4 | 0.4 | 37.6 | 2.6 | 2.6 | 410.2 | 0.6 | 0.6 | 2452873.9 | 5.6 | 5.6 | 0.082 | 0.007 | 0.007 | 160.5 | 4.3 | 4.3 | 2.975e-6 | 0.058e-6 | 0.058e-6 | 1.71 | 0.06 | 0.06 | 413.5 | 2.6 | 2.6 | Omiya et al. 2009 | BOES (BOAO) + HIDES (OAO) | ||||||
30 | TYC 0434-04538-1 b | 10.25 | 0.06 | 0.06 | 7.413 | 0.027 | 0.027 | -0.38 | 0.06 | 0.06 | 1.04 | 0.15 | 0.15 | 6.1 | 0.7 | 0.7 | 193.2 | 0.4 | 0.4 | 2454829. | 15. | 18. | 0.08 | 0.05 | 0.03 | 196. | 30. | 34. | 0.66 | 0.04 | 0.04 | 209. | 2. | 2. | Niedzielski et al. 2009 | HET, HARPS-N | ||||||
31 | HD 206610 b | 107251 | 8.35 | 0.01 | 0.01 | 5.952 | 0.026 | 0.026 | K0 III | 0.014 | 0.03 | 0.03 | 1.56 | 0.11 | 0.11 | 2.2 | 0.1 | 0.1 | 610. | 13. | 13. | 2454677. | 20. | 20. | 0.229 | 0.058 | 0.058 | 296. | 10. | 10. | 1.68 | 0.05 | 0.05 | 40.7 | 1.9 | 1.9 | Johnson et al. 2010 | Keck | ||||
32 | HD 145457 b | 79219 | 6.57 | 4.122 | K0 III | -0.14 | 0.09 | 0.09 | 1.9 | 0.3 | 0.3 | 2.9 | 176.30 | 0.39 | 0.39 | 2453518 | 13 | 13 | 0.112 | 0.035 | 0.035 | 300 | 26 | 26 | 6.3e-9 | 0.86e-9 | 0.86e-9 | 0.76 | 70.6 | 3.1 | 3.1 | Sato et al. 2010 | HDS (Subaru) + HIDES (OAO) | |||||||||
33 | HD 180314 b | 94576 | 6.61 | 4.312 | K0 III | 0.20 | 0.09 | 0.09 | 2.6 | 0.3 | 0.3 | 22 | 396.03 | 0.62 | 0.62 | 2453565.0 | 3.1 | 3.1 | 0.257 | 0.010 | 0.010 | 303.1 | 2.3 | 2.3 | 1.465e-6 | 0.046e-6 | 0.046e-6 | 1.4 | 340.8 | 3.3 | 3.3 | Sato et al. 2010 | HDS (Subaru) + HIDES (OAO) | |||||||||
34 | gamma1 Leo b | 50583 | 2.01 | K0 - K4 III | -0.51 | 0.05 | 0.05 | 1.23 | 0.21 | 0.21 | 8.78 | 1.0 | 1.0 | 428.5 | 1.25 | 1.25 | 2451236 | 13.5 | 13.5 | 0.144 | 0.046 | 0.046 | 206.7 | 9.2 | 9.2 | 1.19 | 0.02 | 0.02 | 208.3 | 4.3 | 4.3 | Han et al. 2010 | BOES (Bohyunsan) | |||||||||
35 | HD 1690 b | 1692 | 9.17 | 6.018 | K1 III | -0.32 | 0.06 | 0.06 | 1.09 | 0.15 | 0.15 | 6.1 | 0.9 | 0.9 | 533 | 1.7 | 1.7 | 2454449 | 5 | 5 | 0.64 | 0.04 | 0.04 | 122 | 8 | 8 | 1.81e-7 | 0.84e-7 | 0.84e-7 | 1.3 | 0.02 | 0.02 | 190 | 29 | 29 | Moutou et al. 2011 | HARPS | linear trend -7.2+/- 0.4 m/s | ||||
36 | HD 28678 b | 21109 | 8.54 | 5.775 | 0.023 | 0.023 | K0 | -0.11 | 0.03 | 0.03 | 1.74 | 0.12 | 0.12 | 1.7 | 0.1 | 0.1 | 387.1 | 4.2 | 4.2 | 2455517. | 30. | 30. | 0.168 | 0.068 | 0.068 | 131. | 30. | 30. | 1.24 | 0.03 | 0.03 | 33.5 | 2.3 | 2.3 | Johnson et al. 2011 | Keck | ||||||
37 | HD 5891 b | 4715 | 8.25 | 5.621 | 0.016 | 0.016 | G5 | -0.02 | 0.03 | 0.03 | 1.91 | 0.13 | 0.13 | 7.6 | 0.02 | 0.02 | 177.11 | 0.31 | 0.31 | 2455432. | 10. | 10. | 0.066 | 0.020 | 0.020 | 360. | 30. | 30. | 0.76 | 0.02 | 0.02 | 178.5 | 4.1 | 4.1 | Johnson et al. 2011 | Keck | ||||||
38 | HD 99706 b | 55994 | 7.81 | 5.335 | 0.016 | 0.016 | K0 | 0.14 | 0.03 | 0.03 | 1.72 | 0.12 | 0.12 | 1.4 | 0.1 | 0.1 | 868. | 31. | 31. | 2455219. | 30. | 30. | 0.365 | 0.10 | 0.10 | 359. | 20. | 20. | 2.14 | 0.08 | 0.08 | 22.4 | 2.2 | 2.2 | Johnson et al. 2011 | Keck | linear trend -7.4 +/- 2.0 m/s/yr | |||||
39 | HD 99706 c | 55994 | 7.81 | 5.335 | 0.016 | 0.016 | K0 | 0.14 | 0.03 | 0.03 | 1.72 | 0.12 | 0.12 | 5.69 | 1.43 | 0.96 | 1278. | 151. | 198. | 2455383. | 249. | 140. | 0.411 | 0.231 | 0.178 | 136. | 64. | 64. | 13.8 | 2.9 | 2.5 | Bryan et al. 2016 | Keck | no updated solution for HD 99706 b after second planet | ||||||||
40 | nu Oph b | 88048 | 3.32 | 1.225 | 0.306 | 0.306 | K0 III | +0.06 | 0.1 | 0.1 | 2.72 | 0.15 | 0.15 | 22.3 | 529.9 | 0.1 | 0.1 | 2452035.0 | 2.4 | 2.4 | 0.127 | 0.004 | 0.004 | 8.90 | 0.03 | 0.03 | 1.286e-6 | 1.78 | 288.4 | Quirrenbach et al. 2011 | Hamilton (Lick) | similar elements by Sato et al. 2012 | ||||||||||
41 | nu Oph c | 88048 | 3.32 | 1.225 | 0.306 | 0.306 | K0 III | +0.06 | 0.1 | 0.1 | 2.72 | 0.15 | 0.15 | 24.5 | 3184 | 7 | 7 | 2453076 | 17 | 17 | 0.190 | 0.007 | 0.007 | 9.66 | 0.04 | 0.04 | 1.684e-6 | 5.89 | 175.4 | Quirrenbach et al. 2011 | Hamilton (Lick) | similar elements by Sato et al. 2012 | ||||||||||
42 | HD 175679 b | 92968 | 6.14 | G8 III | -0.14 | 2.7 | 0.3 | 0.3 | 37.3 | 1366.8 | 5.7 | 5.7 | 2453263.9 | 7.6 | 7.6 | 0.378 | 0.008 | 0.008 | 346.4 | 1.3 | 1.3 | 6.18e-6 | 1.7e-6 | 1.7e-6 | 3.36 | 0.12 | 0.12 | 380.2 | 3.2 | 3.2 | Wang et al. 2012 | Xinglong; OAO | ||||||||||
43 | HD 240237 b | 114840 | 8.19 | K2 III | -0.26 | 0.07 | 0.07 | 1.69 | 0.42 | 0.42 | 5.3 | 745.7 | 13.8 | 13.8 | 2454292.5 | 28.3 | 28.3 | 0.4 | 0.1 | 0.1 | 108.1 | 21.8 | 21.8 | 1.9 | 91.5 | 12.8 | 12.8 | Gettel et al. 2012a | HET | |||||||||||||
44 | BD +48 738 b | 9.14 | K0 III | -0.20 | 0.07 | 0.07 | 0.74 | 0.39 | 0.39 | 0.91 | 392.6 | 5.5 | 5.5 | 2454457.7 | 28.5 | 28.5 | 0.2 | 0.1 | 0.1 | 358.9 | 31.1 | 31.1 | 1.0 | 31.9 | 2.6 | 2.6 | Gettel et al. 2012a | HET | ||||||||||||||
45 | HD 96127 b | 54232 | 7.43 | K2 III | -0.24 | 0.10 | 0.10 | 0.91 | 0.25 | 0.25 | 4.0 | 647.3 | 16.8 | 16.8 | 2453969.9 | 31.0 | 31.0 | 0.3 | 0.1 | 0.1 | 162.0 | 18.2 | 18.2 | 1.4 | 104.8 | 10.6 | 10.6 | Gettel et al. 2012a | HET | |||||||||||||
46 | BD +20 274 b | 9.36 | 6.169 | K5 III | -0.46 | 0.07 | 0.07 | 0.8 | 0.2 | 0.2 | 4.2 | 578.2 | 5.4 | 5.4 | 2453921.0 | 33.2 | 33.2 | 0.21 | 0.06 | 0.06 | 108.5 | 38.1 | 38.1 | 1.3 | 121.4 | 6.4 | 6.4 | Gettel et al. 2012b | HET | |||||||||||||
47 | HD 219415 b | 8.94 | 6.421 | K0 III | -0.04 | 0.09 | 0.09 | 1.0 | 0.1 | 0.1 | 1.0 | 2093.3 | 32.7 | 32.7 | 2453461.4 | 57.7 | 57.7 | 0.40 | 0.09 | 0.09 | 207.0 | 12.3 | 12.3 | 3.2 | 18.2 | 2.2 | 2.2 | Gettel et al. 2012b | HET | |||||||||||||
48 | epsilon CrB b | 78159 | 4.14 | 1.349 | K2 III | -0.094 | 0.001 | 0.001 | 1.7 | 0.1 | 0.1 | 6.7 | 0.3 | 0.3 | 417.9 | 0.5 | 0.5 | 2451235.3 | 39.7 | 39.7 | 0.11 | 0.33 | 0.33 | 133.1 | 33.3 | 33.3 | 9.227e-8 | 1.3 | 129.4 | 2.0 | 2.0 | Lee et al. 2012a | BOES (BOAO) | |||||||||
49 | HD 66141 b | 39311 | 4.39 | 1.4 | 0.3 | 0.3 | K2 III | -0.323 | 0.034 | 0.034 | 1.1 | 0.1 | 0.1 | 6.0 | 0.3 | 0.3 | 480.5 | 0.5 | 0.5 | 2451320.8 | 4.8 | 4.8 | 0.07 | 0.03 | 0.03 | 22.1 | 3.5 | 3.5 | 1.545e-7 | 1.2 | 0.1 | 0.1 | 146.2 | 2.7 | 2.7 | Lee et al. 2012b | BOES (BOAO) | |||||
50 | Kepler-56 b | 10.227 | 0.018 | 0.018 | K III | 0.20 | 0.16 | 0.16 | 1.32 | 0.13 | 0.13 | 0.047 | 0.047 | 0.047 | 10.5034294 | 0.00025 | 0.00025 | 0.1042 | 0.00174 | 0.00174 | Steffen et al. 2013 | Kepler | ||||||||||||||||||||
51 | Kepler-56 c | 10.227 | 0.018 | 0.018 | K III | 0.20 | 0.16 | 0.16 | 1.32 | 0.13 | 0.13 | 0.20 | 0.197 | 0.197 | 21.40505 | 0.00036 | 0.00036 | 0.1676 | 0.0028 | 0.0028 | Steffen et al. 2013 | Kepler | ||||||||||||||||||||
52 | 75 Cet b | 11791 | 5.36 | 3.207 | 0.272 | 0.272 | G3 III: | 0.00 | 0.04 | 0.04 | 2.49 | 0.27 | 0.02 | 3.0 | 691.9 | 3.6 | 3.6 | 2452213 | 54 | 54 | 0.117 | 0.048 | 0.048 | 165 | 28 | 28 | 3.95e-5 | 0.62e-5 | 0.62e-5 | 2.1 | 38.3 | 2.0 | 2.0 | Sato et al. 2012 | HIDES (Okayama) | |||||||
53 | omicron UMa b | 41704 | 3.35 | 1.339 | 0.202 | 0.202 | G4 II-III | -0.09 | 0.02 | 0.02 | 3.09 | 0.07 | 0.07 | 4.1 | 1630 | 35 | 35 | 2453400 | 170 | 170 | 0.130 | 0.065 | 0.065 | 58 | 42 | 42 | 6.3e-5 | 1.2e-5 | 1.2e-5 | 3.9 | 33.6 | 2.1 | 2.1 | Sato et al. 2012 | HIDES (Okayama) | |||||||
54 | omicron CrB b | 75049 | 5.51 | 2.934 | 0.322 | 0.322 | K0 III | -0.29 | 0.03 | 0.03 | 2.13 | 0.23 | 0.01 | 1.5 | 187.83 | 0.54 | 0.54 | 2452211 | 17 | 17 | 0.191 | 0.085 | 0.085 | 79 | 36 | 36 | 6.2e-4 | 1.6e-4 | 1.6e-4 | 0.83 | 32.25 | 2.8 | 2.8 | Sato et al. 2012 | HIDES (Okayama) | |||||||
55 | kappa CrB b | 77655 | 4.79 | 2.423 | 0.242 | 0.242 | K0 III-IV | +0.10 | 0.04 | 0.04 | 1.51 | 0.19 | 0.19 | 1.6 | 1251 | 15 | 15 | 2451860 | 180 | 180 | 0.073 | 0.049 | 0.049 | 210 | 51 | 51 | 1.69e-5 | 0.25e-5 | 0.25e-5 | 2.6 | 23.6 | 1.1 | 1.1 | Sato et al. 2012 | HIDES (Okayama) | |||||||
56 | HD 208527 b | 108296 | 6.4 | 2.2 | M1 III | -0.09 | 0.16 | 0.16 | 1.6 | 0.4 | 0.4 | 9.9 | 1.7 | 1.7 | 875.5 | 5.8 | 5.8 | 2450745.3 | 45.7 | 45.7 | 0.08 | 0.04 | 0.04 | 278.0 | 19.5 | 19.5 | 3.375e-7 | 2.1 | 0.2 | 0.2 | 155.4 | 3.2 | 3.2 | Lee et al. 2013 | BOES (BOAO) | |||||||
57 | HD 220074 b | 115218 | 6.4 | 2.0 | M2 III | -0.25 | 0.25 | 0.25 | 1.2 | 0.3 | 0.3 | 11.1 | 1.8 | 1.8 | 672.1 | 3.7 | 3.7 | 2451158.2 | 31.7 | 31.7 | 0.14 | 0.05 | 0.05 | 323.0 | 8.5 | 8.5 | 8.314e-7 | 1.6 | 0.1 | 0.1 | 230.8 | 5.0 | 5.0 | Lee et al. 2013 | BOES (BOAO) | |||||||
58 | BD +15 2940 b | 78407 | 9.05 | 6.525 | K0 | 0.28 | 0.07 | 0.07 | 1.1 | 0.2 | 0.2 | 1.1 | 137.48 | 0.34 | 0.34 | 2453464.5 | 16 | 16 | 0.26 | 0.10 | 0.10 | 302 | 33 | 33 | 0.539 | 42.7 | 4.4 | 4.4 | Nowak et al. 2013 | HET | ||||||||||||
59 | HD 233604 b | 10.29 | 7.979 | K5 | -0.36 | 0.04 | 0.04 | 1.5 | 0.3 | 0.3 | 6.6 | 192.00 | 0.22 | 0.22 | 2453022 | 77 | 77 | 0.05 | 0.03 | 0.03 | 281 | 43 | 43 | 0.747 | 177.8 | 4.3 | 4.3 | Nowak et al. 2013 | HET | K5 questionable | ||||||||||||
60 | tau Gem b | 34693 | 4.41 | 1.681 | 0.254 | 0.254 | K2 III | 0.14 | 0.1 | 0.1 | 2.3 | 0.3 | 0.3 | 20.6 | 305.5 | 0.1 | 0.1 | 2453270.7 | 14.8 | 14.8 | 0.031 | 0.0009 | 0.0009 | 137.4 | 0.3 | 0.3 | 1.36e-6 | 1.17 | 350.2 | Mitchell et al. 2013 | Hamilton (Lick) | |||||||||||
61 | 91 Aqr b | 114855 | 4.24 | 1.597 | 0.236 | 0.236 | K0 III | -0.03 | 0.1 | 0.1 | 1.4 | 0.1 | 0.1 | 3.2 | 181.4 | 0.1 | 0.1 | 2453472.1 | 24.5 | 24.5 | 0.0027 | 0.026 | 0.026 | 177.3 | 0.8 | 0.8 | 1.44e-8 | 0.70 | 91.5 | Mitchell et al. 2013 | Hamilton (Lick) | |||||||||||
62 | HD 112410 b | 63242 | 6.86 | 0.01 | 0.01 | 4.406 | 0.016 | 0.016 | G8 III | -0.31 | 0.09 | 0.09 | 1.54 | 0.05 | 0.05 | 9.18 | 124.6 | 2455376.2 | 0.23 | 118.2 | 0.565 | 287.5 | Jones et al. 2013 | FEROS | ||||||||||||||||||
63 | HD 2952 b | 2611 | 5.93 | 3.629 | K0 III | 0.00 | 0.04 | 0.04 | 2.54 | 0.09 | 0.12 | 1.6 | 311.6 | 1.9 | 1.7 | 2450112 | 54 | 64 | 0.129 | 0.085 | 0.099 | 64 | 48 | 56 | 5.7e-10 | 1.9e-10 | 2.7e-10 | 1.2 | 26.3 | 3.4 | 3.8 | Sato et al. 2013 | HIDES (Okayama) | |||||||||
64 | HD 120084 b | 66903 | 5.91 | 3.572 | G7 III | +0.09 | 0.05 | 0.05 | 2.39 | 0.3 | 0.06 | 4.5 | 2082 | 35 | 24 | 2450774 | 61 | 80 | 0.66 | 0.10 | 0.14 | 117 | 9 | 12 | 1.4e-8 | 0.5e-8 | 1.8e-8 | 4.3 | 53 | 11 | 33 | Sato et al. 2013 | HIDES (Okayama) | |||||||||
65 | omega Ser b | 77578 | 5.21 | 4.107 | G8 III | -0.24 | 0.02 | 0.02 | 2.17 | 0.29 | 0.21 | 1.7 | 277.02 | 0.51 | 0.52 | 2450022 | 38 | 27 | 0.106 | 0.069 | 0.079 | 132 | 52 | 34 | 9.0e-10 | 1.8e-10 | 2.1e-10 | 1.1 | 31.8 | 2.3 | 2.3 | Sato et al. 2013 | HIDES (Okayama) | |||||||||
66 | Kepler-91 b | 12.884 | 10.136 | 0.021 | 0.021 | K3 III | 0.11 | 0.07 | 0.07 | 1.31 | 0.10 | 0.10 | 1.09 | 0.20 | 0.20 | 6.246580 | 0.000082 | 0.000082 | 0.066 | 0.017 | 0.013 | 250 | 100 | 100 | 0.0726 | 0.0019 | 0.0019 | 93 | 17 | 17 | Lillo-Box et al. 2014 | Kepler | lum. class might be III-IV (R = 6.30 R_Sun) | |||||||||
67 | Sand 364 b | 9.8 | 6.7 | K3 III | -0.02 | 0.04 | 0.04 | 1.35 | 0.05 | 0.05 | 1.54 | 0.24 | 0.24 | 121.710 | 0.305 | 0.305 | 2456240.9 | 3.7 | 3.7 | 0.35 | 0.08 | 0.08 | 273.51 | 12.81 | 12.81 | 67.42 | 5.85 | 5.85 | Brucalassi et al. 2014 | HARPS; Coralie; Sophie; HET | member of M67 | |||||||||||
68 | HIP 105854 b | 105854 | 5.64 | 2.994 | 0.232 | 0.232 | K2 III | 0.31 | 0.18 | 0.18 | 2.1 | 0.1 | 0.1 | 8.2 | 0.2 | 0.2 | 184.2 | 0.5 | 0.5 | 2455262.4 | 2.4 | 2.4 | 0.02 | 0.03 | 0.03 | 343.2 | 4.9 | 4.9 | 0.81 | 0.03 | 0.03 | 178.1 | 10.0 | 10.0 | Jones et al. 2014 | FEROS; CHIRON | ||||||
69 | eta Cet b | 5364 | 3.46 | 0.922 | 0.250 | 0.250 | K1 III | 0.07 | 0.1 | 0.1 | 1.7 | 0.1 | 0.1 | 2.55 | 0.16 | 0.16 | 407.5 | 2.7 | 2.7 | 2454025.03 | 0.12 | 0.05 | 0.05 | 245.4 | 9.5 | 9.5 | 1.28 | 49.4 | Trifonov et al. 2014 | Lick | dynamically stable 2 planet system; possibly in 2:1 MMR | |||||||||||
70 | eta Cet c | 5364 | 3.46 | 0.922 | 0.250 | 0.250 | K1 III | 0.07 | 0.1 | 0.1 | 1.7 | 0.1 | 0.1 | 3.26 | 0.17 | 0.17 | 739.9 | 4.8 | 4.8 | 2454124.91 | 0.08 | 0.04 | 0.04 | 68.2 | 22.3 | 22.3 | 1.91 | 51.6 | Trifonov et al. 2014 | Lick | dynamically stable 2 planet system; possibly in 2:1 MMR | |||||||||||
71 | HD 14067 b | 10657 | 6.41 | 4.097 | 0.036 | 0.036 | G9 III | -0.10 | 0.08 | 0.08 | 2.4 | 0.2 | 0.2 | 9.0 | 0.9 | 0.9 | 2850 | 290 | 430 | 2450092 | 862 | 586 | 0.697 | 0.051 | 0.045 | 102.1 | 5.3 | 5.1 | 1.10e-7 | 0.15e-7 | 0.16e-7 | 5.3 | 0.4 | 0.6 | 100.1 | 4.8 | 4.9 | Wang et al. 2014 | Xinglong; OAO | |||
72 | Kepler-432 b | 12.464 | 0.058 | 0.058 | 10.121 | 0.017 | 0.017 | K2 III | -0.02 | 0.06 | 0.06 | 1.35 | 0.10 | 0.10 | 5.84 | 0.05 | 0.05 | 52.501134 | 0.00007 | 0.000107 | 2456841.06 | 0.03 | 0.03 | 0.478 | 0.004 | 0.004 | 68.4 | 0.7 | 0.7 | 0.303 | 0.007 | 0.007 | 294.6 | 2.1 | 2.1 | Ortiz et al. 2015; Ciceri et al. 2015; Quinn et al. 2015 | Kepler; RV | second planet present | ||||
73 | HIP 67851 b | 67851 | 6.17 | 3.751 | 0.236 | 0.236 | K0 III | 0.00 | 0.10 | 0.10 | 1.63 | 0.22 | 0.22 | 1.38 | 0.15 | 0.15 | 88.9 | 0.1 | 0.1 | 2452997.8 | 16.7 | 16.7 | 0.05 | 0.04 | 0.04 | 138.1 | 60.0 | 60.0 | 0.46 | 0.02 | 0.02 | 45.5 | 1.6 | 1.6 | Jones et al. 2015a; Jones et al. 2015b | FEROS; CHIRON | updated orbital parameters after announcement of second planet | |||||
74 | HIP 67851 c | 67851 | 6.17 | 3.751 | 0.236 | 0.236 | K0 III | 0.00 | 0.10 | 0.10 | 1.63 | 0.22 | 0.22 | 5.98 | 0.76 | 0.76 | 2131.8 | 88.3 | 88.3 | 2452684.1 | 235.7 | 235.7 | 0.17 | 0.06 | 0.06 | 166.5 | 20.5 | 20.5 | 3.82 | 0.23 | 0.23 | 69.0 | 3.3 | 3.3 | Jones et al. 2015b | FEROS; CHIRON | ||||||
75 | TYC 1422-614-1 b | 10.21 | 7.728 | 0.031 | 0.031 | K0 III | -0.20 | 0.08 | 0.08 | 1.15 | 0.18 | 0.18 | 2.51 | 0.12 | 0.12 | 198.44 | 0.64 | 0.64 | 2452843 | 40 | 40 | 0.07 | 0.04 | 0.04 | 62 | 46 | 46 | 0.6879 | 0.0015 | 0.0015 | 82.2 | 3.7 | 3.7 | Niedzielski et al. 2015a | HRS; HARPS-N | two planet system | ||||||
76 | TYC 1422-614-1 c | 10.21 | 7.728 | 0.031 | 0.031 | K0 III | -0.20 | 0.08 | 0.08 | 1.15 | 0.18 | 0.18 | 10.10 | 0.14 | 0.14 | 569.2 | 2.1 | 2.1 | 2452617 | 30 | 30 | 0.049 | 0.014 | 0.014 | 124 | 20 | 20 | 1.3916 | 0.0033 | 0.0033 | 232.8 | 3.3 | 3.3 | Niedzielski et al. 2015a | HRS; HARPS-N | two planet system | ||||||
77 | HD 145934 b | 8.5 | 6.145 | 0.015 | 0.015 | K0 III | 1.748 | 0.105 | 0.105 | 2.28 | 2.26 | 2.26 | 2730 | 100 | 100 | 2451430 | 370 | 370 | 0.053 | 0.053 | 0.053 | 215 | 62 | 62 | 4.60 | 0.14 | 0.14 | 22.9 | 2.6 | 2.6 | Feng et al. 2015 | HIRES (Keck) | ||||||||||
78 | HIP 65891 b | 65891 | 6.75 | 4.453 | 0.023 | 0.023 | K0 III | 0.16 | 0.10 | 0.10 | 2.50 | 0.21 | 0.21 | 6.00 | 0.49 | 0.49 | 1084.5 | 23.2 | 23.2 | 2456014.8 | 49.3 | 49.3 | 0.13 | 0.05 | 0.05 | 355.5 | 15.5 | 15.5 | 2.81 | 0.09 | 0.09 | 64.9 | 2.4 | 2.4 | Jones et al. 2015b | FEROS; CHIRON | ||||||
79 | HIP 107773 b | 107773 | 5.62 | 3.292 | 0.250 | 0.250 | K1 III | 0.03 | 0.10 | 0.10 | 2.42 | 0.27 | 0.27 | 1.98 | 0.21 | 0.21 | 144.3 | 0.5 | 0.5 | 2456202.3 | 12.8 | 12.8 | 0.09 | 0.06 | 0.06 | 166.0 | 32.6 | 32.6 | 0.72 | 0.03 | 0.03 | 42.7 | 2.7 | 2.7 | Jones et al. 2015b | FEROS; CHIRON | ||||||
80 | BD +49 828 b | 9.38 | 0.02 | 0.02 | 6.571 | 0.021 | 0.021 | K0 III | -0.19 | 0.06 | 0.06 | 1.52 | 0.22 | 0.22 | 1.6 | 0.2 | 0.4 | 2590 | 180 | 300 | 2455479.5 | 170 | 200 | 0.35 | 0.10 | 0.24 | 170 | 30 | 32 | 4.2 | 0.20 | 0.32 | 18.8 | 2.0 | 6.2 | Niedzielski et al. 2015b | HET | |||||
81 | HD 95127 b | 53733 | 8.15 | 0.01 | 0.01 | 5.022 | 0.018 | 0.018 | K0 III | -0.18 | 0.05 | 0.05 | 1.20 | 0.22 | 0.22 | 5.01 | 0.44 | 0.61 | 482 | 5 | 5 | 2453200.5 | 50 | 50 | 0.11 | 0.06 | 0.15 | 40 | 40 | 37 | 1.28 | 0.01 | 0.01 | 116 | 9 | 16 | Niedzielski et al. 2015b | HET | ||||
82 | HD 216536 b | 9.23 | 0.02 | 0.02 | 6.496 | 0.018 | 0.018 | K0 III | -0.17 | 0.09 | 0.09 | 1.36 | 0.38 | 0.38 | 1.47 | 0.12 | 0.20 | 148.6 | 0.7 | 0.7 | 2453587.5 | 11 | 11 | 0.38 | 0.10 | 0.12 | 270 | 20 | 21 | 0.609 | 0.002 | 0.002 | 50 | 4 | 8 | Niedzielski et al. 2015b | HET | |||||
83 | HD 155233 b | 84056 | 6.813 | 4.493 | 0.036 | 0.036 | K1 III | +0.10 | 0.07 | 0.07 | 1.50 | 0.20 | 0.20 | 2.0 | 0.5 | 0.5 | 885 | 63 | 63 | 2455112 | 412 | 412 | 0.03 | 0.20 | 0.20 | 95 | 90 | 90 | 2.07 | 0.10 | 0.10 | 32.2 | 8.7 | 8.7 | Wittenmyer et al. 2016a | UCLES | linear trend 15.4+/-6.5 m/s/yr | |||||
84 | HD 11755 b | 9242 | 6.87 | 3.760 | 0.280 | 0.280 | G5 III | -0.74 | 0.02 | 0.02 | 0.9 | 0.1 | 0.1 | 6.5 | 1.0 | 1.0 | 433.7 | 3.2 | 3.2 | 2457018.2 | 14.0 | 14.0 | 0.19 | 0.10 | 0.10 | 155.3 | 12.6 | 12.6 | 1.08 | 0.04 | 0.04 | 191.3 | 10.2 | 10.2 | Lee et al. 2015 | BOES (BOAO) | ||||||
85 | HD 12648 b | 10800 | 6.98 | 4.743 | 0.031 | 0.031 | G5 III | -0.57 | 0.02 | 0.02 | 1.2 | 0.1 | 0.1 | 2.9 | 0.4 | 0.4 | 133.6 | 0.5 | 0.5 | 2452324.7 | 57.6 | 57.6 | 0.04 | 0.16 | 0.16 | 99.3 | 140.7 | 140.7 | 0.54 | 0.02 | 0.02 | 102.0 | 8.4 | 8.4 | Lee et al. 2015 | BOES (BOAO) | ||||||
86 | HD 24064 b | 18451 | 6.75 | 3.130 | 0.394 | 0.394 | K0 III | -0.49 | 0.06 | 0.06 | 1.0 | 0.1 | 0.1 | 9.4 | 1.3 | 1.3 | 535.6 | 3.0 | 3.0 | 2455278.3 | 11.8 | 11.8 | 0.35 | 0.08 | 0.08 | 250.8 | 6.3 | 6.3 | 1.29 | 0.05 | 0.05 | 251.0 | 9.3 | 9.3 | Lee et al. 2015 | BOES (BOAO) | ||||||
87 | 8 UMi b | 73136 | 6.83 | 4.515 | 0.020 | 0.020 | K0 III | -0.03 | 0.02 | 0.02 | 1.8 | 0.1 | 0.1 | 1.5 | 0.2 | 0.2 | 93.4 | 4.5 | 4.5 | 2454108.5 | 22.8 | 22.8 | 0.06 | 0.18 | 0.18 | 91.0 | 84.6 | 84.6 | 0.49 | 0.03 | 0.03 | 46.1 | 4.0 | 4.0 | Lee et al. 2015 | BOES (BOAO) | ||||||
88 | HD 33844 b | 24275 | 7.29 | 4.945 | 0.018 | 0.018 | K0 III | 0.27 | 0.09 | 0.09 | 1.78 | 0.18 | 0.18 | 1.92 | 0.11 | 0.11 | 547.9 | 6.4 | 6.4 | 2454578. | 50 | 50 | 0.16 | 0.07 | 0.07 | 190 | 62 | 62 | 1.59 | 0.01 | 0.01 | 32.9 | 2.2 | 2.2 | Wittenmyer et al. 2016b | AAT; Keck; FEROS | 2 planet system in 5:3 MMR | |||||
89 | HD 33844 c | 24275 | 7.29 | 4.945 | 0.018 | 0.018 | K0 III | 0.27 | 0.09 | 0.09 | 1.78 | 0.18 | 0.18 | 1.68 | 0.16 | 0.16 | 924.3 | 32.5 | 32.5 | 2454356. | 281 | 281 | 0.09 | 0.08 | 0.08 | 5 | 30 | 30 | 2.25 | 0.03 | 0.03 | 24.0 | 2.2 | 2.2 | Wittenmyer et al. 2016b | AAT; Keck; FEROS | 2 planet system in 5:3 MMR | |||||
90 | HD 11343 b | 8541 | 7.88 | 5.290 | 0.029 | 0.029 | K2 III/IV | -0.15 | 0.08 | 0.08 | 1.17 | 0.28 | 0.28 | 5.5 | 1.0 | 1.0 | 1560.2 | 53.9 | 53.9 | 2459346.9 | 93.4 | 93.4 | 0.16 | 0.06 | 0.06 | 293.9 | 15.2 | 15.2 | 2.8 | 0.25 | 0.25 | 87.4 | 6.4 | 6.4 | Jones et al. 2016 | CHIRON; FEROS; UCLES | ||||||
91 | HD 135760 b | 74890 | 7.05 | 4.639 | 0.016 | 0.016 | K1 III | +0.20 | 0.13 | 0.13 | 1.74 | 0.21 | 0.21 | 2.4 | 0.3 | 0.3 | 822.3 | 16.8 | 16.8 | 2459820.4 | 379.8 | 379.8 | 0.07 | 0.07 | 0.07 | 181.9 | 93.9 | 93.9 | 2.1 | 0.09 | 0.09 | 36.5 | 2.7 | 2.7 | Jones et al. 2016 | FEROS; UCLES | ||||||
92 | HD 155233 b | 84056 | 6.81 | 4.493 | 0.036 | 0.036 | K1 III | +0.08 | 0.07 | 0.07 | 1.69 | 0.14 | 0.14 | 2.6 | 0.3 | 0.3 | 818.8 | 12.1 | 12.1 | 2460282.0 | 192.1 | 192.1 | 0.04 | 0.04 | 0.04 | 120.0 | 71.9 | 71.9 | 2.0 | 0.06 | 0.06 | 40.5 | 3.1 | 3.1 | Jones et al. 2016 | CHIRON; FEROS | ||||||
93 | HD 181342 b | 95124 | 7.55 | 5.251 | 0.020 | 0.020 | K0 III | +0.20 | 0.08 | 0.08 | 1.89 | 0.11 | 0.11 | 2.9 | 0.2 | 0.2 | 562.1 | 6.0 | 6.0 | 2459915.5 | 54.3 | 54.3 | 0.10 | 0.07 | 0.07 | 311.8 | 35.8 | 35.8 | 1.65 | 0.04 | 0.04 | 46.5 | 1.8 | 1.8 | Jones et al. 2016 | CHIRON; FEROS; UCLES | ||||||
94 | HD 5583 b | 7.6 | 5.221 | 0.020 | 0.020 | K0 III | -0.50 | 0.18 | 0.18 | 1.01 | 0.1 | 0.1 | 5.78 | 0.53 | 0.53 | 139.35 | 0.22 | 0.21 | 2456021.5 | 17 | 18 | 0.076 | 0.023 | 0.070 | 12 | 6 | 330 | 0.53 | 0.02 | 0.02 | 225.8 | 4.0 | 4.5 | Niedzielski et al. 2016a | HET; HARPS-N (Tapas) | |||||||
95 | BD +15 2375 b | 10.31 | 7.718 | 0.017 | 0.017 | -0.22 | 0.08 | 0.08 | 1.08 | 0.14 | 0.14 | 1.061 | 0.27 | 0.27 | 153.22 | 0.44 | 0.44 | 2457680.5 | 630 | 700 | 0.001 | 0.001 | 0.25 | 55 | 17 | 240 | 0.576 | 0.027 | 0.027 | 38.3 | 1.0 | 2.3 | Niedzielski et al. 2016a | HET; HARPS-N (Tapas) | ||||||||
96 | TYC 3667-1280 b | 9.86 | 7.100 | 0.017 | 0.017 | -0.08 | 0.05 | 0.05 | 1.87 | 0.17 | 0.17 | 5.4 | 0.4 | 0.4 | 26.468 | 0.005 | 0.005 | 2456320.1 | 3.3 | 3.7 | 0.036 | 0.014 | 0.043 | 240 | 50 | 50 | 0.21 | 0.01 | 0.01 | 242.4 | 1.2 | 1.0 | Niedzielski et al. 2016b | HET; HARPS-N (Tapas) | ||||||||
97 | HD 47366 b | 31674 | 6.11 | 4.055 | 0.290 | 0.290 | K1 III | -0.02 | 0.09 | 0.09 | 1.81 | 0.13 | 0.13 | 1.75 | 0.17 | 0.20 | 363.3 | 2.4 | 2.5 | 2450122. | 55 | 71 | 0.089 | 0.060 | 0.079 | 100. | 71. | 100. | 1.214 | 0.029 | 0.030 | 33.6 | 2.8 | 3.6 | Sato et al. 2016 | HIDES (Okayama); Xinglong; AAT | multiple system; possibly retrograde | |||||
98 | HD 47366 c | 31674 | 6.11 | 4.055 | 0.290 | 0.290 | K1 III | -0.02 | 0.09 | 0.09 | 1.81 | 0.13 | 0.13 | 1.86 | 0.15 | 0.16 | 684.7 | 4.9 | 5.0 | 2450445. | 62. | 55. | 0.278 | 0.094 | 0.067 | 132. | 20. | 17. | 1.853 | 0.045 | 0.045 | 30.1 | 2.0 | 2.1 | Sato et al. 2016 | HIDES (Okayama); Xinglong; AAT | multiple system; possibly retrograde | |||||
99 | K2-97 b | 12.611 | 0.031 | 0.031 | 10.035 | 0.021 | 0.021 | K III | +0.38 | 0.08 | 0.08 | 1.16 | 0.12 | 0.12 | 1.10 | 0.11 | 0.11 | 8.4080 | 0.0002 | 0.0002 | 2457416.808 | 0.007 | 0.007 | 103 | 8 | 8 | Grunblatt et al. 2016 | K2, Keck, APF | inflated hot Jupiter | |||||||||||||
100 | nu Oct b | 107089 | 3.743 | 0.015 | 0.015 | 1.458 | 0.306 | 0.306 | K1 III/IV | +0.18 | 0.04 | 0.04 | 1.61 | 2.11 | 0.02 | 0.02 | 414.8 | 2.6 | 3.6 | 2452136. | 0.086 | 0.036 | 0.043 | 350. | 25. | 8. | 1.276 | 0.005 | 0.007 | 38.74 | 1.2 | 0.9 | Ramm et al. 2009; Ramm et al. 2016 | HERCULES, Mt. John Observatory | planet in 2.6 AU spectroscopic binary; dynamical fit | |||||||
101 | HD 59686 Ab | 36616 | 5.45 | 2.922 | 0.300 | 0.300 | K2 III | 0.15 | 0.1 | 0.1 | 1.9 | 0.2 | 0.2 | 6.92 | 0.24 | 0.18 | 299.36 | 0.31 | 0.26 | 2451531.06 | 0.05 | 0.02 | 0.03 | 121. | 24 | 28 | 1.0860 | 0.0007 | 0.0006 | 136.9 | 4.6 | 3.8 | Ortiz et al. 2016 | Hamilton (Lick) | planet in 13.6 AU spectroscopic binary; dynamical fit | |||||||
102 | HD 102329 b | 57467 | 8.04 | 5.402 | 0.018 | 0.018 | K0 III | 0.3 | 0.03 | 0.03 | 1.95 | 0.14 | 0.14 | 5.9 | 0.3 | 0.3 | 778.1 | 7.1 | 7.1 | 2455096. | 20. | 20. | 0.211 | 0.044 | 0.044 | 182. | 10. | 10. | 2.01 | 0.05 | 0.05 | 84.8 | 3.4 | 3.4 | Johnson et al. 2011 | Keck | b and c solutions are not consistent, and also the stellar parameters differ | |||||
103 | HD 102329 c | 57467 | 8.04 | 5.402 | 0.018 | 0.018 | K0 III | 0.05 | 1.3 | 0.15 | 0.15 | 1.52 | 0.3 | 0.25 | 1123. | 79. | 53. | 2454736. | 569. | 200. | 0.209 | 0.231 | 0.202 | 21. | 165. | 74. | 27.4 | 6.8 | 4.5 | Bryan et al. 2016 | Keck | |||||||||||
104 | HD 175370 b | 92668 | 7.19 | 0.01 | 0.01 | 4.224 | 0.017 | 0.017 | K2 III | -0.52 | 0.07 | 0.07 | 1.02 | 0.16 | 0.16 | 4.2 | 0.7 | 0.7 | 347.7 | 3.1 | 3.1 | 2456276. | 38 | 38 | 0.15 | 0.10 | 0.10 | 171. | 37. | 37. | 0.98 | 0.05 | 0.05 | 122. | 13. | 13. | Hrudková et al. 2017 | Tautenburg and HERMES/Mercator | Kepler; masses are for the RGB phase; 22 AU spectroscopic binary | |||
105 | HD 86950 b | 49129 | 7.46 | 0.01 | 0.01 | 5.038 | 0.018 | 0.018 | K1 III | 0.04 | 0.10 | 0.10 | 1.66 | 0.25 | 0.25 | 3.6 | 0.7 | 0.7 | 1270. | 57. | 57. | 2454245. | 161. | 161. | 0.17 | 0.16 | 0.16 | 243. | 70. | 70. | 2.72 | 0.08 | 0.08 | 49. | 12. | 12. | Wittenmyer et al. 2017 | AAT; FEROS; CHIRON | ||||
106 | HD 222076 b | 116630 | 7.47 | 5.127 | 0.027 | 0.027 | K0 III | 0.05 | 0.10 | 0.10 | 1.07 | 0.25 | 0.25 | 1.56 | 0.11 | 0.11 | 871. | 19. | 19. | 2454264. | 189. | 189. | 0.08 | 0.05 | 0.05 | 241. | 60. | 60. | 1.83 | 0.03 | 0.03 | 31.9 | 2.3 | 2.3 | Wittenmyer et al. 2017 | AAT; FEROS; CHIRON | ||||||
107 | HD 120457 b | 67537 | 6.44 | 0.005 | 0.005 | 4.196 | 0.036 | 0.036 | K1 III | 0.15 | 0.08 | 0.08 | 2.41 | 0.16 | 0.16 | 11.1 | 0.6 | 0.6 | 2592.5 | 116.1 | 116.1 | 2456293.3 | 29.9 | 29.9 | 0.59 | 0.04 | 0.04 | 120.7 | 5.3 | 5.3 | 2.2e-7 | 4.96 | 0.24 | 0.24 | 113.2 | 4.0 | 4.0 | Jones et al. 2017 | FEROS; CHIRON | upper mass limit 0.22 M_Sun from astrometry | ||
108 | HD 208897 b | 108513 | 6.510 | 0.009 | 0.009 | 4.198 | 0.036 | 0.036 | K0 | 0.21 | 0.15 | 0.15 | 1.25 | 0.11 | 0.11 | 1.40 | 372.5 | 1.7 | 1.7 | 2455036. | 82. | 82. | 0.07 | 0.06 | 0.06 | 167. | 83. | 83. | 1.5e-9 | 0.3e-9 | 0.3e-9 | 1.05 | 34.7 | 2.2 | 2.2 | Yilmaz et al. 2017 | TUG; OAO | |||||
109 | TYC 4282 0605 b | 10.58 | 0.01 | 0.01 | 6.778 | 0.021 | 0.021 | -0.07 | 0.16 | 0.16 | 0.97 | 0.03 | 0.03 | 10.78 | 0.12 | 0.12 | 101.54 | 0.05 | 0.05 | 2456479.28 | 0.57 | 0.57 | 0.28 | 0.01 | 0.01 | 288.94 | 2.38 | 2.38 | 0.422 | 0.009 | 0.009 | 495.2 | 5.1 | 5.1 | González-Álvarez et al. 2017 | HARPS-N; Giano | NIR RV amplitude identical to the optical one | |||||
110 | HD 76920 b | 43803 | 7.82 | 0.01 | 0.01 | 5.253 | 0.026 | 0.026 | K1 III | -0.19 | 0.06 | 0.06 | 1.0 | 0.2 | 0.2 | 3.71 | 0.33 | 0.32 | 415.891 | 0.039 | 0.043 | 2454812.47 | 0.33 | 0.30 | 0.87826 | 0.0025 | 0.0025 | 1.2 | 1.0 | 1.0 | 1.091 | 0.077 | 0.068 | 178.1 | 2.6 | 2.7 | Wittenmyer et al. 2017, Bergmann et al. 2021 | AAT; FEROS; CHIRON, Hercules | most eccentric planet around a giant star | |||
111 | K2-132 b | 11.897 | 0.030 | 0.030 | 9.540 | 0.023 | 0.023 | -0.11 | 0.05 | 0.05 | 1.19 | 0.04 | 0.04 | 0.495 | 0.0068 | 0.0063 | 9.1708 | 0.0025 | 0.0025 | 2457608.5289 | 0.0087 | 0.0087 | 0.290 | 0.049 | 0.049 | 82.6 | 4.0 | 4.2 | 0.0916 | 0.0006 | 0.0006 | 43.0 | 1.8 | 1.8 | Grunblatt et al. 2017; Jones et al. 2018 | K2; Keck; HARPS; FEROS | inflated hot Jupiter; update by Jones et al. 2018 | |||||
112 | HD 40956 b | 28951 | 6.584 | 0.001 | 0.001 | 4.143 | 0.324 | 0.324 | K0 | 0.14 | 0.05 | 0.05 | 2.00 | 0.08 | 0.08 | 2.7 | 0.6 | 0.6 | 578.6 | 3.3 | 3.3 | 2455341.88 | 11.07 | 11.07 | 0.24 | 0.05 | 0.05 | 338.62 | 7.74 | 7.74 | 1.4 | 0.1 | 0.1 | 68. | 2. | 2. | Jeong et al. 2018 | BOES (BOAO) + HIDES (OAO) | ||||
113 | HD 111591 b | 62653 | 6.594 | 0.001 | 0.001 | 2.980 | 0.252 | 0.252 | K0 III | 0.07 | 0.04 | 0.04 | 1.94 | 0.07 | 0.07 | 4.4 | 0.4 | 0.4 | 1056.4 | 14.3 | 14.3 | 2455602.40 | 30.85 | 30.85 | 0.26 | 0.10 | 0.10 | 78.72 | 11.94 | 11.94 | 2.5 | 0.1 | 0.1 | 59. | 3. | 3. | Jeong et al. 2018 | BOES (BOAO) + HIDES (OAO) | ||||
114 | HD 113996 b | 64022 | 4.69 | 0.02 | 0.02 | 1.493 | 0.178 | 0.178 | K5 III | 0.13 | 0.08 | 0.08 | 1.49 | 0.18 | 0.18 | 6.3 | 1.0 | 1.0 | 610.2 | 3.8 | 3.8 | 2453309.94 | 23.67 | 23.67 | 0.28 | 0.12 | 0.12 | 92.06 | 17.25 | 17.25 | 1.6 | 0.1 | 0.1 | 120. | 9. | 9. | Jeong et al. 2018 | BOES (BOAO) + HIDES (OAO) | ||||
115 | HD 238914 b | 91388 | 8.79 | 0.01 | 0.01 | 6.325 | 0.034 | 0.034 | K III | -0.25 | 0.09 | 0.09 | 1.47 | 0.47 | 0.47 | 6.0 | 2.7 | 2.7 | 4100. | 240. | 210. | 2460540.5 | 250. | 230. | 0.56 | 0.05 | 0.07 | 318. | 7. | 8. | 5.7 | 0.9 | 0.9 | 71. | 11. | 7. | Adamów et al. 2018 | HET; HARPS-N | Li-rich; sp.typ. and mass uncertain | |||
116 | TYC 3318-01333-1 b | 9.90 | 0.03 | 0.03 | 6.869 | 0.021 | 0.021 | -0.06 | 0.06 | 0.06 | 1.19 | 0.14 | 0.14 | 3.42 | 0.35 | 0.35 | 562. | 4.0 | 4.1 | 2454340.5 | 60. | 60. | 0.098 | 0.032 | 0.082 | 129. | 36. | 40. | 1.414 | 0.063 | 0.063 | 75.42 | 0.7 | 0.9 | Adamów et al. 2018 | HET; HARPS-N | Li-rich; linear trend indicating a stellar binary | |||||
117 | BD +48 740 b | 12684 | 8.70 | 0.01 | 0.01 | 5.645 | 0.017 | 0.017 | K3 III | -0.13 | 0.06 | 0.06 | 1.09 | 0.16 | 0.16 | 1.7 | 0.7 | 0.7 | 733. | 8. | 5. | 2454774.5 | 15. | 21. | 0.76 | 0.09 | 0.05 | 100. | 15. | 12. | 1.7 | 0.1 | 0.1 | 54. | 8. | 5.2 | Adamów et al. 2012; 2018 | HET; HARPS-N | Li-rich | |||
118 | 24 Boo b | 70791 | 5.58 | 3.159 | 0.280 | 0.280 | G3 IV | -0.77 | 0.03 | 0.03 | 0.99 | 0.13 | 0.19 | 0.91 | 0.10 | 0.13 | 30.3506 | 0.0077 | 0.0078 | 2450008.6 | 7.9 | 10.1 | 0.042 | 0.029 | 0.048 | 210 | 130 | 100 | 0.190 | 0.009 | 0.012 | 59.9 | 3.2 | 3.3 | Takarada et al. 2018 | HIDES (Okayama) | radius and log(g) indicate a giant rather than a subgiant | |||||
119 | gamma Lib b | 76333 | 3.91 | 1.506 | 0.01 | 0.01 | K0 III | -0.30 | 0.03 | 0.03 | 1.47 | 0.20 | 0.20 | 1.02 | 0.14 | 0.14 | 415.2 | 1.9 | 1.8 | 2450041. | 33 | 36 | 0.21 | 0.10 | 0.10 | 187. | -38 | 30 | 1.24 | 0.10 | 0.10 | 22.0 | 2.2 | 2.2 | Takarada et al. 2018 | HIDES (Okayama) | Keplerian solution; 7:3 MMR | |||||
120 | gamma Lib c | 76333 | 3.91 | 1.506 | 0.01 | 0.01 | K0 III | -0.30 | 0.03 | 0.03 | 1.47 | 0.20 | 0.20 | 4.58 | 0.43 | 0.45 | 964.6 | 3.1 | 3.1 | 2450725. | 110 | 87 | 0.057 | 0.032 | 0.034 | 146. | -43. | 32. | 2.17 | 0.10 | 0.10 | 73.0 | 2.1 | 2.1 | Takarada et al. 2018 | HIDES (Okayama) | Keplerian solution; 7:3 MMR | |||||
121 | 7 CMa b | 31592 | 3.91 | 1.60 | K1 III | 0.21 | 0.1 | 0.1 | 1.34 | 0.11 | 0.12 | 1.85 | 0.06 | 0.04 | 735.1 | 14.8 | 1.0 | 2451492.34 | 560. | 1.75 | 0.06 | 0.03 | 0.03 | 165.3 | 5.1 | 70.8 | 1.758 | 0.024 | 0.001 | 34.3 | 1.2 | 0.9 | Luque et al. 2019 | Lick, UCLES, HARPS, SONG | 4:3 resonance | |||||||
122 | 7 CMa c | 31592 | 3.91 | 1.60 | K1 III | 0.21 | 0.1 | 0.1 | 1.34 | 0.11 | 0.12 | 0.87 | 0.06 | 0.06 | 996.0 | 1.5 | 52.4 | 2451957.42 | 53.00 | 58.25 | 0.08 | 0.05 | 0.04 | 233.5 | 7.7 | -40.2 | 2.153 | 0.003 | 0.08 | 14.9 | 0.9 | 1.1 | Luque et al. 2019 | Lick, UCLES, HARPS, SONG | 4:3 resonance | |||||||
123 | HD 125390 b | 69888 | 8.59 | 0.01 | 0.01 | 5.875 | 0.018 | 0.018 | G7 III | 1.36 | 22.2 | 1.2 | 1.2 | 1756.2 | 3.9 | 3.9 | 2455914.0 | 6.7 | 6.7 | 0.591 | 0.014 | 0.014 | 342.4 | 1.2 | 1.2 | 3.16 | 0.54 | 0.54 | 373. | 16. | 16. | Luhn et al. 2019 | Keck | mass in text and table of paper differ; yet another mass in Brewer et al. (2016) which is reference | ||||||||
124 | HD 202696 b | 105056 | 8.22 | 0.01 | 0.01 | 5.877 | 0.020 | 0.020 | K0 III-IV | 0.02 | 0.04 | 0.04 | 1.91 | 0.09 | 0.14 | 1.996 | 0.220 | 0.100 | 517.8 | 8.9 | 3.9 | 2450088.03 | 100.75 | 21.00 | 0.011 | 0.078 | 0.011 | 201.6 | 97.8 | 98.5 | 1.5666 | 0.016 | 0.017 | 34.1 | 2.3 | 2.9 | Trifonov et al. 2019 | Keck | possibly in 11:6 mean motion resonance | |||
125 | HD 202696 c | 105056 | 8.22 | 0.01 | 0.01 | 5.877 | 0.020 | 0.020 | K0 III-IV | 0.02 | 0.04 | 0.04 | 1.91 | 0.09 | 0.14 | 1.864 | 0.177 | 0.227 | 946.6 | 20.7 | 20.9 | 2449526.70 | 260.10 | 286.25 | 0.028 | 0.065 | 0.012 | 136.8 | 143.0 | 62.7 | 2.342 | 0.034 | 0.035 | 25.3 | 2.1 | 3.3 | Trifonov et al. 2019 | Keck | possibly in 11:6 mean motion resonance | |||
126 | HD 25723 b | 19011 | 5.611 | 0.010 | 0.010 | 3.044 | 0.272 | 0.272 | K1 III | -0.03 | 0.10 | 0.10 | 2.12 | 0.41 | 0.55 | 2.50 | 0.14 | 0.17 | 457.01 | 1.29 | 1.31 | 2451455.13 | 44.57 | 70.82 | 0.04 | 0.05 | 0.03 | 112.97 | 55.83 | 44.06 | 3.03e-9 | 0.06e-9 | 0.06e-9 | 1.49 | 0.04 | 0.05 | 40.03 | 2.40 | 2.42 | Tala Pinto et al. 2020 | Hamilton (Lick) | possible second planet |
127 | 17 Sco b | 79540 | 5.239 | 0.009 | 0.009 | 2.094 | 0.244 | 0.244 | K3 III | -0.01 | 0.10 | 0.10 | 1.22 | 0.13 | 0.14 | 4.32 | 0.15 | 0.12 | 578.38 | 2.01 | 2.09 | 2453294.41 | 174.23 | 182.91 | 0.06 | 0.03 | 0.02 | 57.03 | 113.18 | 106.77 | 4.70e-8 | 0.09e-8 | 0.10e-8 | 1.45 | 0.02 | 0.02 | 92.40 | 3.90 | 3.84 | Tala Pinto et al. 2020 | Hamilton (Lick) | |
128 | HD 4760 b | 3869 | 7.49 | 0.01 | 0.01 | 3.993 | 0.027 | 0.027 | K2 | -0.91 | 0.09 | 0.09 | 1.05 | 0.19 | 0.19 | 13.9 | 2.4 | 2.4 | 434. | 3. | 3. | 2453955.5 | 23. | 27. | 0.23 | 0.09 | 0.06 | 265. | 13. | 16. | 1.14 | 0.08 | 0.08 | 370. | 12. | 9. | Niedzielski et al. 2021 | HET, HARPS-N | ||||
129 | HD 96992 b | 54595 | 8.56 | 0.01 | 0.01 | 6.015 | 0.020 | 0.020 | K0 | -0.45 | 0.08 | 0.08 | 0.96 | 0.09 | 0.09 | 1.14 | 0.31 | 0.31 | 514. | 4. | 4. | 2453620.5 | 30. | 40. | 0.41 | 0.24 | 0.12 | 149. | 24. | 31. | 1.24 | 0.05 | 0.05 | 33. | 3. | 3. | Niedzielski et al. 2021 | HET, HARPS-N | ||||
130 | HD 360 b | 671 | 5.980 | 0.01 | 0.01 | 3.653 | 0.01 | 0.01 | G8 III | -0.08 | 1.69 | 0.15 | 0.53 | 0.75 | 0.12 | 0.15 | 273.1 | 1.6 | 0.8 | 2455184.5 | 44.9 | 92.8 | 0.139 | 0.108 | 0.104 | 133 | 119 | 63 | 0.98 | 0.11 | 0.03 | 16.8 | 1.8 | 2.6 | Teng et al. 2022 | HIDES (Okayama) | ||||||
131 | HD 10975 b | 8423 | 5.929 | 0.009 | 0.009 | 3.875 | 0.308 | 0.308 | K0 III | -0.17 | 1.41 | 0.34 | 0.35 | 0.45 | 0.06 | 0.15 | 283.8 | 12.7 | 0.1 | 2455450.7 | 29.1 | -182.9 | 0.442 | 0.040 | 0.389 | 135. | 153. | 35. | 0.95 | 0.06 | 0.08 | 12.3 | 0.2 | 3.5 | Teng et al. 2022 | HIDES (Okayama) | ||||||
132 | HD 79181 b | 45158 | 9.687 | 0.009 | 0.009 | 3.540 | 0.242 | 0.242 | G8 III | -0.29 | 1.28 | 0.32 | 0.28 | 0.64 | 0.06 | 0.16 | 273.1 | 1.3 | 0.4 | 2455123.0 | 103.8 | 11.6 | 0.259 | 0.067 | 0.206 | 318. | 48. | 32. | 0.64 | 0.06 | 0.16 | 17.7 | 1.6 | -2.2 | Teng et al. 2022 | HIDES (Okayama) | ||||||
133 | HD 99283 b | 55797 | 5.700 | 0.009 | 0.009 | 3.568 | 0.322 | 0.322 | K0 III | -0.17 | 1.76 | 0.31 | 0.30 | 0.97 | 0.06 | 0.25 | 310.4 | 5.2 | 1.7 | 2455291.1 | 256.1 | -25.6 | 0.200 | 0.102 | 0.146 | 291. | 62. | 41. | 1.08 | 0.05 | 0.07 | 20.4 | 1.9 | 3.5 | Teng et al. 2022 | HIDES (Okayama) | ||||||
134 | upsilon Leo b | 56647 | 4.30 | 2.01 | G9 III | -0.19 | 1.48 | 0.90 | 0.38 | 0.51 | 0.06 | 0.26 | 385.2 | 2.8 | 1.3 | 2455279.6 | 27.9 | 34.2 | 0.320 | 0.134 | 0.218 | 131. | 36. | 31. | 1.18 | 0.11 | 0.32 | 11.7 | 1.7 | 1.6 | Teng et al. 2022 | HIDES (Okayama) | ||||||||||
135 | HD 161178 b | 86219 | 5.869 | 0.009 | 0.009 | 3.657 | 0.236 | 0.236 | G9 III | -0.20 | 1.06 | 0.25 | 0.17 | 0.57 | 0.02 | 0.16 | 279.3 | 1.0 | 0.8 | 2455296.6 | 218.4 | 12.0 | 0.044 | 0.132 | 0.019 | 300. | 180. | 70. | 0.85 | 0.05 | 0.07 | 17.0 | 1.6 | 2.3 | Teng et al. 2022 | HIDES (Okayama) | ||||||
136 | HD 219139 b | 114641 | 5.852 | 0.010 | 0.010 | 3.392 | 0.230 | 0.230 | G5 III | -0.19 | 1.46 | 0.31 | -0.29 | 0.78 | 0.05 | 0.20 | 275.5 | 2.3 | 1.0 | 2455240.1 | 198.9 | 12.2 | 0.110 | 0.087 | 0.081 | 318. | 113. | 67. | 0.94 | 0.06 | 0.07 | 19.2 | 1.8 | 2.6 | Teng et al. 2022 | HIDES (Okayama) | ||||||
137 | gamma Psc b | 114971 | 3.70 | 1.441 | 0.01 | 0.01 | G7 III | -0.62 | 0.99 | 0.17 | 0.13 | 1.34 | 0.02 | 0.31 | 555.1 | 6.0 | 2.5 | 2455394.6 | 60.6 | 63.5 | 0.204 | 0.114 | 0.141 | 44. | 34. | 56. | 1.32 | 0.05 | 0.08 | 34.0 | 3.9 | 5.0 | Teng et al. 2022 | HIDES (Okayama) | ||||||||
138 | HD 22532 b | 16732 | 7.84 | 0.01 | 0.01 | 5.671 | 0.017 | 0.017 | G8 III/IV | -0.19 | 0.02 | 0.02 | 1.20 | 0.05 | 0.05 | 2.12 | 0.09 | 0.09 | 872.6 | 2.8 | 2.8 | 2455575.0 | 221.0 | 221.0 | 0.03 | 0.03 | 0.03 | 169.1 | 88.7 | 88.7 | 1.900 | 0.004 | 0.004 | 40.0 | 1.6 | 1.6 | Ottoni et al. 2022 | Coralie (La Silla) | ||||
139 | HD 64121 b | 38181 | 7.43 | 0.01 | 0.01 | 5.244 | 0.021 | 0.021 | G8/K0 III | -0.21 | 0.02 | 0.02 | 1.18 | 0.05 | 0.05 | 2.56 | 0.19 | 0.19 | 623.0 | 3.4 | 3.4 | 2455653.0 | 130.0 | 130.0 | 0.11 | 0.07 | 0.07 | 2.7 | 56.0 | 56.0 | 1.510 | 0.006 | 0.006 | 55.2 | 4.1 | 4.1 | Ottoni et al. 2022 | Coralie (La Silla) | ||||
140 | HD 69123 b | 40344 | 5.765 | 0.009 | 0.009 | 3.586 | 0.242 | 0.242 | K1 III | 0.05 | 0.03 | 0.03 | 1.43 | 0.07 | 0.07 | 3.04 | 0.16 | 0.16 | 1193.3 | 7.0 | 7.0 | 2455715.7 | 64.6 | 64.6 | 0.19 | 0.06 | 0.06 | 292.7 | 21.7 | 21.7 | 2.482 | 0.010 | 0.010 | 46.8 | 2.4 | 2.4 | Ottoni et al. 2022 | Coralie (La Silla) | ||||
141 | HD 29399 b | 21253 | 5.780 | 0.009 | 0.009 | 3.78 | 0.24 | 0.24 | K1 III | 0.14 | 0.03 | 0.03 | 1.17 | 0.10 | 0.10 | 1.57 | 0.11 | 0.11 | 892.7 | 5.9 | 5.9 | 2455965.0 | 210.0 | 210.0 | 0.05 | 0.05 | 0.05 | 346.9 | 85.1 | 85.1 | 1.913 | 0.008 | 0.008 | 29.9 | 2.2 | 2.2 | Pezzotti et al. 2022 | Coralie (La Silla) | ||||
142 | KIC 3526061 b | 10.37 | 0.04 | 0.04 | 7.776 | 0.029 | 0.029 | 0.12 | 0.10 | 0.11 | 1.42 | 0.041 | 0.041 | 18.15 | 0.44 | 0.44 | 3552. | 158. | 135. | 2458708.1 | 2.0 | 1.9 | 0.85 | 0.01 | 0.01 | 75.7 | 1.3 | 1.3 | 5.14 | 0.16 | 0.16 | 355.7 | 5.1 | 5.0 | Karjalainen et al. 2022 | TS2 (McDonald), HERMES (La Palma) |