Table 1
Planets used for occurrence rate calculation.
Karmn | P | Mpl sin i | RV FAP | Ref. | |
---|---|---|---|---|---|
(d) | (M⊕) | (%) | |||
J01125–169 | c | 3.060 | ![]() |
0.0047 | Sto20a |
J01125–169 | d | 4.656 | ![]() |
0.0349 | Sto20a |
J02530+168 | b | 4.910 | ![]() |
<10−6 | Zec19 |
J02530+168 | c | 11.41 | ![]() |
<10−6 | Zec19 |
J03133+047 | b | 2.291 | ![]() |
<10−6 | Bau20 |
J06548+332 | b | 14.24 | ![]() |
<10−6 | Sto20b |
J08413+594 | b | 203.6 | ![]() |
<10−6 | Mor19 |
J09144+526 | b | 24.45 | ![]() |
0.0012 | Gon20 |
J11033+359 | b | 12.95 | ![]() |
<10−6 | Sto20b |
J11417+427 | b | 41.38 | ![]() |
<10−6 | Tri18 |
J11417+427 | c | 532.5 | ![]() |
<10−6 | Tri18 |
J11421+267 | b | 2.644 | ![]() |
<10−6 | Tri18 |
J12123+544S | b | 13.67 | ![]() |
<10−6 | Sto20b |
J12479+097 (a) | b | 1.467 | ![]() |
0.0012 | Tri21 |
J13229+244 | b | 3.023 | ![]() |
<10−6 | Luq18 |
J16167+672S | b | 86.54 | ![]() |
<10−6 | Rei18 |
J16303–126 (b) | b | 1.26 | ![]() |
0.453 | Wri16 |
J16303–126 | c | 17.87 | ![]() |
0.0011 | Wri16 |
J17378+185 | b | 15.53 | ![]() |
0.0007 | Lal19 |
J19169+051N | b | 105.9 | ![]() |
<10−6 | Kam18 |
J21164+025 | b | 14.44 | ![]() |
<10−6 | Lal19 |
J21466+668 | b | 2.305 | ![]() |
<10−6 | Ama21 |
J21466+668 | c | 8.052 | ![]() |
<10−6 | Ama21 |
J22137–176 | b | 3.651 | ![]() |
<10−6 | Luq18 |
J22252+594 | b | 13.35 | ![]() |
<10−6 | Nag19 |
J22532–142 | b | 61.08 | ![]() |
<10−6 | Tri18 |
J22532–142 | c | 30.13 | ![]() |
<10−6 | Tri18 |
Notes. (a) We tabulate the actual mass of the transiting planet GJ 486 (J12479+097). (b) The orbital period of GJ 628 b (J16303–126) reported by Wri16 was 4.89 d.
References. Ama21: Amado et al. (2021); Bau20: Bauer et al. (2020); Gon20: González-Álvarez et al. (2020); Kam18: Kaminski et al. (2018); Lal19: Lalitha et al. (2019); Luq18: Luque et al. (2018); Mor19: Morales et al. (2019); Nag19: Nagel et al. (2019); Rei18: Reiners et al. (2018a); Sto20a: Stock et al. (2020a); Sto20b: Stock et al. (2020b); Tri18: Trifonov et al. (2018); Tri21: Trifonov et al. (2021); Wri16: Wright et al. (2016); Zec19: Zechmeister et al. (2019).
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