Table A.1
Jump parameters used as starting points for the MCMC analysis.
| Planet | a∕Rs | inc | Rp ∕Rs | Period | Eccentricity | Teff | log(g*) | [Fe/H] | Ref. |
|---|---|---|---|---|---|---|---|---|---|
| ° | days | Kelvin | log10(cm s−2) | dex | |||||
| HAT-P-32 b | 6.05(4) | 88.9(4) | 0.1508(4) | 2.150008(1) | 0.16(6) | 6207(88) | 4.33(1) | −0.04(8) | 13 |
| XO-1 b | 11.24(9) | 88.8(2) | 0.1320(5) | 3.94150685(91) | 0 | 5750(75) | 4.50(1) | 0.02(8) | 6 |
| HAT-P-1 b | 9.85(7) | 85.63(06) | 0.1180(2) | 4.46529976(55) | 0 | 5980(49) | 4.36(1) | 0.13(1) | 19 |
| WASP-17 b | 7.05(7) | 86.83(68) | 0.13 | 3.7354380(68) | 0.03(2) | 6650(80) | 4.16(3) | −0.19(9) | 1 |
| WASP-39 b | 11.37(24) | 87.75(27) | 0.1457(16) | 4.0552765(35) | 0 | 5400(150) | 4.4(2) | −0.12(10) | 18,10 |
| HAT-P-12 b | 11.77(21) | 89.0(4) | 0.1406(13) | 3.2130598(21) | 0.03(3) | 4650(60) | 4.61(1) | −0.29(5) | 11 |
| HAT-P-18 b | 16.04(75) | 88.8(3) | 0.1365(15) | 5.508023(6) | 0.08(5) | 4803(80) | 4.57(4) | 0.10(08) | 14 |
| TrES2 b | 7.90(2) | 83.87(02) | 0.1254(5) | 2.47061317(9) | 0.02(2) | 5850(50) | 4.43(2) | −0.15(10) | 9, 22 |
| WASP-4 b | 5.46(2) | 88.52(39) | 0.1544(2) | 1.33823204(16) | 0.003(7) | 5436(34) | 4.46(5) | −0.05(4) | 15,20 |
| XO-2 b | 8.18(3) | 88.9(7) | 0.1 | 2.615857(50) | 0 | 5340(32) | 4.48(5) | 0.45(2) | 5 |
| GJ3470 b | 13.94(49) | 88.88(72) | 0.0764(4) | 3.3366487(43) | 0.02(2) | 3652(50) | 4.78(12) | 0.17(6) | 3 |
| WASP-21 b | 9.62(17) | 87.12(24) | 0.1030(8) | 4.3225126(22) | 0 | 5800(100) | 4.2(1) | −0.46(11) | 21,4 |
| WASP-31 b | 8.00(19) | 84.41(22) | 0.127 | 3.4059096(50) | 0 | 6302(102) | 4.31(2) | −0.20(09) | 2 |
| WASP-1 b | 5.69(6) | 90.0(1.3) | 0.1036(8) | 2.5199454(5) | 0.01(3) | 6200(200) | 4.3(3) | 0.1(2) | 17,7 |
| HAT-P-26 b | 13.44(83) | 88.6(9) | 0.0737(12) | 4.234516(15) | 0.12(6) | 5079(88) | 4.56(6) | −0.04(8) | 12 |
| WASP-107 b | 18.2(1) | 89.56(08) | 0.1446(2) | 5.72149242(46) | 0 | 4430(120) | 4.5(1) | 0.02(10) | 23 |
| WASP-13 b | 7.58(15) | 85.64(24) | 0.0922(8) | 4.353011(13) | 0 | 5826(100) | 4.04(20) | 0.0(2) | 24,25 |
| WASP-121 b | 3.75(3) | 87.6(6) | 0.1245(5) | 1.27492550(25) | 0 | 6459(140) | 4.24(1) | 0.13(9) | 26 |
| WASP-69 b | 11.96(17) | 86.71(20) | 0.1336(16) | 3.8681382(17) | 0 | 4700(50) | 4.54(2) | 0.15(8) | 35 |
| WASP-67 b | 13.42(13) | 85.8(3) | 0.1345(48) | 4.61442(1) | 0 | 5417(85) | 4.53(2) | 0.18(6) | 36 |
| HATS7 b | 10.59(51) | 87.92(75) | 0.0711(19) | 3.185315(5) | 0 | 4985(50) | 4.54(5) | 0.25(8) | 37 |
| WASP-29 b | 12.15(44) | 88.8(7) | 0.101(2) | 3.922719(7) | 0.03(5) | 4875(65) | 4.54(4) | 0.11(14) | 38 |
| HAT-P-41 b | 5.45(18) | 87.7(1.0) | 0.1028(16) | 2.694050(4) | 0 | 6390(100) | 4.14(2) | 0.21(10) | 32 |
| WASP-101 b | 8.45(30) | 85.0(2) | 0.1140(9) | 3.585720(4) | 0 | 6380(120) | 4.31(8) | 0.20(12) | 32 |
| WASP-131 b | 8.53(9) | 85.0(3) | 0.0815(7) | 5.322023(5) | 0 | 6030(90) | 4.09(3) | −0.18(8) | 39 |
| WASP-36 b | 5.85(6) | 83.15(13) | 0.1368(6) | 1.53736596(24) | 0 | 5959(134) | 4.49(1) | −0.26(10) | 40 |
| WASP-63 b | 6.59(30) | 87.8(1.3) | 0.0781(11) | 4.378080(6) | 0 | 5550(100) | 4.01(3) | 0.08(7) | 32 |
| WASP-79 b | 7.03(36) | 85.4(6) | 0.1049(24) | 3.662380(5) | 0 | 6600(100) | 4.20(15) | 0.03(1) | 32 |
| WASP-94 Ab | 7.3(7) | 88.7(7) | 0.1094(8) | 3.9501907(44) | 0 | 6153(75) | 4.18(1) | 0.26(15) | 41 |
| WASP-74 b | 4.86(20) | 79.81(24) | 0.0964(7) | 2.137750(1) | 0 | 5990(110) | 4.39(7) | 0.03(10) | 33 |
| WASP-62 b | 9.55(41) | 88.30(75) | 0.1095(9) | 4.411950(3) | 0 | 6230(80) | 4.45(10) | 0.04(6) | 34 |
| Kepler-45 b | 10.6(1.0) | 87.0(7) | 0.179(2) | 2.455239(4) | 0.11(10) | 3820(90) | 3.1(1) | 0.13(13) | 16 |
Notes. Eccentricity was fixed to zero for all planets because it did not affect the resulting transit depths. Stellar parameters (Teff, log g and [Fe/H]) are used to calculate linear limb-darkening parameters.
References. (1) Anderson et al. (2011b); (2) Anderson et al. (2011a); (3) Biddle et al. (2014); (4) Bouchy et al. (2010); (5) Burke et al. (2007); (6) Burke et al. (2010); (7) Collier Cameron et al. (2007); (8) Doyle et al. (2011); (9) Esteves et al. (2015); (10) Faedi et al. (2011); (11) Hartman et al. (2009); (12) Hartman et al. (2011a); (13) Hartman et al. (2011c); (14) Hartman et al. (2011b); (15) Hoyer et al. (2013); (16) Johnson et al. (2012); (17) Maciejewski et al. (2014); (18) Maciejewski et al. (2016); (19) Nikolov et al. (2014); (20) Petrucci et al. (2013); (21) Seeliger et al. (2015); (22) Sozzetti et al. (2007); (23) Močnik et al. (2017); (24) Barros et al. (2012); (25) Skillen et al. (2009); (26) Delrez et al. (2016); (27) Holman et al. (2010); (28) Torres et al. (2011); (32) Stassun et al. (2017); (33) Stassun et al. (2018); (34) Stassun et al. (2019); (35) Anderson et al. (2014); (36) Hellier et al. (2012); (37) Bakos et al. (2015); (38) Hellier et al. (2010); (39) Hellier et al. (2017); (40) Mancini et al. (2016) and (41) Neveu-VanMalle et al. (2014).
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