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Table 3

Properties of known transiting planets and their host stars.

Planet Host star
Name M p R p P a p Sp.T. M ⋆ R ⋆ V vrotsini⋆ T eff Ref. F X/EUV log ṁ γ
() () (d) (AU) (M⊙) (R⊙) (mag) (km s-1) (K) (1) (g s-1)
CoRoT-1 b 1.03 1.49 1.50 0.025 G0V 0.95 1.11 13.6 5.20 5950 2 11.4 42.6
CoRoT-10 b 2.75 0.97 13.2 0.105 K1V 0.89 0.79 15.2 2.00 5075 3 8.30 31.7
CoRoT-11 b 2.33 1.43 2.99 0.043 F6V 1.27 1.37 12.9 40.0 6440 4 11.5 41.8
CoRoT-12 b 0.91 1.44 2.82 0.040 G2V 1.07 1.11 15.5 1.00 5675 5 9.90 39.9
CoRoT-13 b 1.30 0.88 4.03 0.051 G0V 1.09 1.01 15.0 4.00 5945 6 9.60 39.7
CoRoT-2 b 3.31 1.46 1.74 0.028 G7V 0.97 0.90 12.5 11.5 5625 7 11.1 33.6
CoRoT-3 b 21.6 1.01 4.25 0.057 F3V 1.37 1.56 13.3 17.0 6740 8 9.29 49.2
CoRoT-4 b 0.72 1.19 9.20 0.090 F0V 1.10 1.15 13.7 6.40 6190 9 10.0 34.6
CoRoT-5 b 0.46 1.38 4.03 0.049 F9V 1.00 1.18 14.0 1.00 6100 10 9.95 34.6
CoRoT-6 b 2.96 1.16 8.88 0.085 F5V 1.05 1.02 13.9 7.50 6090 11 9.51 30.9
CoRoT-7 b 0.01 0.15 0.85 0.017 K0V 0.93 0.87 11.7  <3.50 5275 12 9.84 36.1
CoRoT-8 b 0.22 0.57 6.21 0.063 K1V 0.88 0.77 14.8 2.00 5080 13 9.19 31.1
CoRoT-9 b 0.84 1.05 95.2 0.407 G3V 0.99 0.94 13.7  <3.50 5625 14 8.06 34.6
GJ 1214 b 0.01 0.24 1.58 0.014 M4.5 0.15 0.21 14.6  <2.00 3026 15 9.36 5.82
GJ 436 b 0.07 0.43 2.64 0.028 M2.5 0.45 0.46 10.6  <3.00 3585 16, 17 1.17 ± 0.52 9.20 15.2
HAT-P-1 b 0.52 1.22 4.46 0.055 G0V 1.13 1.11 10.4 2.20 6047 18  <0.64 10.0 43.8
HAT-P-11 b 0.08 0.45 4.88 0.053 K4 0.81 0.75 9.59 1.50 4780 19  <0.64 9.23 27.8
HAT-P-12 b 0.21 0.95 3.21 0.038 K5 0.73 0.70 12.8 0.50 4650 20 9.62 25.3
HAT-P-13 b 0.85 1.28 2.91 0.042 G4 1.22 1.56 10.6 1.76 5653 21 10.0 50.8
HAT-P-14 b 2.23 1.15 4.62 0.060 F 1.38 1.46 9.98 8.40 6600 22 10.0 45.6
HAT-P-15 b 1.94 1.07 10.8 0.096 G5 1.01 1.08 12.1 2.00 5568 23 8.67 37.8
HAT-P-16 b 4.19 1.28 2.77 0.041 F8 1.21 1.23 10.8 3.50 6158 24 9.71 36.2
HAT-P-17 b 0.53 1.01 10.3 0.088 K 0.85 0.83 10.5 0.30 5246 25 8.10 34.7
HAT-P-18 b 0.19 0.99 5.50 0.055 K 0.77 0.74 12.7 1.50 4750 26 9.97 27.5
HAT-P-19 b 0.29 1.13 4.00 0.046 K 0.84 0.82 12.9 2.10 4875 26 10.3 30.6
HD 147506 b 9.09 1.15 5.63 0.068 F8 1.36 1.64 8.71 19.8 6290 27 9.78 46.1
HAT-P-20 b 7.24 0.86 2.87 0.036 K3 0.75 0.69 11.3 2.10 4595 28 8.71 24.7
HAT-P-21 b 4.06 1.02 4.12 0.049 G3 0.94 1.10 11.6 3.50 5588 28 9.23 38.7
HAT-P-22 b 2.14 1.08 3.21 0.041 G5 0.91 1.04 9.73 0.50 5302 28 8.58 34.2
HAT-P-23 b 2.09 1.36 1.21 0.023 G0 1.13 1.20 12.4 8.10 5905 28 11.3 44.7
HAT-P-24 b 0.68 1.24 3.35 0.046 F8 1.19 1.31 11.8 10.0 6373 29 11.0 40.0
HAT-P-25 b 0.56 1.19 3.65 0.046 G5 1.01 0.95 13.1 0.50 5500 30 9.26 34.0
HAT-P-26 b 0.05 0.56 4.23 0.047 K1 0.81 0.78 11.7 1.80 5079 31 10.0 31.6
HAT-P-3 b 0.59 0.89 2.89 0.038 K 0.93 0.82 11.8 0.50 5185 32  <0.64 8.98 33.7
HAT-P-4 b 0.68 1.33 3.05 0.044 F 1.26 1.60 11.2 5.50 5860 33  <0.64 10.8 40.8
HAT-P-5 b 1.06 1.26 2.78 0.040 G 1.16 1.16 12.0 2.60 5960 34  <0.64 10.1 44.4
HAT-P-6 b 1.05 1.33 3.85 0.052 F 1.29 1.46 10.5 8.70 6570 35  <0.64 10.7 45.2
HAT-P-7 b 1.80 1.42 2.20 0.037 F6 1.47 1.84 10.5 3.80 6350 36  <0.64 10.4 50.9
HAT-P-8 b 1.52 1.50 3.07 0.048 F 1.28 1.58 10.1 11.5 6200 37 10.9 43.9
HAT-P-9 b 0.78 1.40 3.92 0.053 F 1.28 1.32 11.9 6350 38 11.1 39.8
HD 149026 b 0.35 0.65 2.87 0.043 G0 IV 1.30 1.49 8.15 6.00 6147 39  <1.15 10.2 55.8
HD 17156 b 3.21 1.02 21.2 0.162 G0 1.24 1.44 8.17 2.60 6079 40  <2.06 8.07 53.5
HD 189733 b 1.13 1.13 2.21 0.030 K1-K2 0.80 0.75 7.67 2.97 5050 41, 42 6.08 ± 0.18 10.3 30.3
HD 209458 b 0.68 1.32 3.52 0.047 G0 V 1.01 1.14 7.65 3.75 5942 43, 44 0.03 ± 0.01 10.5 43.6
HD 80606 b 3.94 0.92 111. 0.449 G5 0.90 0.98 8.93 2.20 5574 45  <1.80 6.85 35.2
Kepler-4 b 0.07 0.35 3.21 0.045 G0 1.22 1.48 12.7 2.20 5857 46 9.40 51.7
Kepler-5 b 2.11 1.43 3.54 0.050 1.37 1.79 4.80 6297 47 10.1
Kepler-6 b 0.66 1.32 3.23 0.045 1.20 1.39 3.00 5647 48 10.4
Kepler-7 b 0.43 1.47 4.88 0.062 G0 1.34 1.84 4.20 5933 49 10.7 61.7
Kepler-8 b 0.60 1.41 3.52 0.048 1.21 1.48 13.9 10.5 6213 50 11.3
Kepler-9 b 0.25 0.84 19.2 0.140 G2 1.00 1.10 13.9 1.90 5777 51 8.89 40.5
Kepler-9 c 0.17 0.82 38.9 0.225 G2 1.00 1.10 13.9 1.90 5777 51 8.60 40.5
Kepler-9 d 0.02 0.14 1.59 0.027 G2 1.00 1.10 13.9 1.90 5777 90 9.15 40.5
Kepler-10 b 0.01 0.12 0.83 0.016 G 0.89 1.05 10.9 0.50 5627 91 8.82 37.8
Lupus-TR-3 b 0.81 0.89 3.91 0.046 K1V 0.87 0.82 17.4 0.00  <0.64
OGLE-TR-10 b 0.63 1.26 3.10 0.041 G or K 1.18 1.16 7.70 6220 52 0.08 ± 0.04 11.0 47.0
OGLE-TR-111 b 0.53 1.06 4.01 0.047 G or K 0.82 0.85  <5.00 5070 53  <0.64 10.5 27.4
OGLE-TR-113 b 1.32 1.09 1.43 0.022 K 0.78 0.77  <5.00 4752 52  <1.80 10.8 28.1
OGLE-TR-132 b 1.14 1.18 1.68 0.030 F 1.26 1.34  <5.00 6411 52  <1.78 10.7 40.9
OGLE-TR-182 b 1.01 1.13 3.97 0.051 1.14 1.14 16.8 0.00  <1.76
OGLE-TR-211 b 1.03 1.36 3.67 0.051 1.33 1.64 0.00  <1.83
OGLE-TR-56 b 1.29 1.30 1.21 0.022 G 1.17 1.32 16.6 5.00 5970 52  <1.79 11.2 48.7
OGLE2-TR-L9 b 4.50 1.61 2.48 0.030 F3 1.52 1.53 39.3 6933 54 11.8 50.6
SWEEPS-04 3.80 0.81 4.20 0.055 1.24 1.18 18.8 0.00  <0.64
SWEEPS-11 9.70 1.13 1.79 0.030 1.10 1.45 19.8 0.00 64.9 ± 4.55
TrES-1 0.61 1.08 3.03 0.039 K0V 0.87 0.83 11.7 1.08 5214 55  <1.14 9.71 34.2
TrES-2 1.20 1.17 2.47 0.035 G0V 0.98 0.94 11.4 2.00 5850 33  <1.46 9.98 36.7
TrES-3 1.91 1.32 1.30 0.022 G 0.92 0.81 12.4 1.50 5650 33  <0.64 10.2 31.4
TrES-4 0.91 1.79 3.55 0.050 F 1.38 1.84 11.5 8.50 6200 57  <1.50 11.3 49.3
WASP-1 b 0.89 1.35 2.51 0.038 F7V 1.24 1.24 11.7  <5.00 6200 58  <0.64 10.8 36.7
WASP-10 b 3.06 1.08 3.09 0.037 K5 0.71 0.78 12.7  <6.00 4675 59 10.0 27.8
WASP-11 b 0.46 1.04 3.72 0.043 K3V 0.82 0.81 11.8 0.50 4980 60 9.22 31.4
WASP-12 b 1.41 1.79 1.09 0.022 G0 1.35 1.57 11.6  <2.20 6300 61 11.4 59.9
WASP-13 b 0.46 1.21 4.35 0.052 G1V 0.00 1.34 10.4  <4.90 5826 62 10.4 47.5
WASP-14 b 7.72 1.25 2.24 0.037 F5V 1.31 1.29 9.75 4.90 6475 63 9.71 40.5
WASP-15 b 0.54 1.42 3.75 0.049 F5 1.18 1.47 10.9 4.00 6300 64 10.7 42.8
WASP-16 b 0.85 1.00 3.11 0.042 G3V 1.02 0.94 11.3 3.00 5700 65 10.0 35.5
WASP-17 b 0.49 1.74 3.73 0.051 F6 1.20 1.38 11.6 9.00 6550 66 11.6 43.1
WASP-18 b 10.4 1.16 0.94 0.020 F6 1.28 1.21 9.30 11.0 6400 67 10.5 37.9
WASP-19 b 1.15 1.31 0.78 0.016 G8V 0.95 0.93 12.3 4.00 5500 68 11.7 33.2
WASP-2 b 0.91 1.01 2.15 0.031 K1V 0.84 0.78 11.9  <5.00 5200 58  <0.64 10.5 32.5
WASP-21 b 0.30 1.07 4.32 0.052 G3V 1.01 1.06 11.6 1.50 5800 69 9.97 39.7
WASP-22 b 0.56 1.12 3.53 0.046 G 1.10 1.13 12.0 3.50 6000 70 10.3 43.7
WASP-24 b 1.03 1.10 2.34 0.035 F8-9 1.12 1.14 11.3 6.96 6075 71 10.7 33.6
WASP-25 b 0.58 1.26 3.76 0.047 G4 1.00 0.95 11.9 3.00 5750 72 10.4 36.1
WASP-26 b 1.02 1.32 2.75 0.040 G0 1.12 1.34 11.3 2.40 5950 73 10.2 49.0
WASP-28 b 0.91 1.12 3.40 0.045 F8-G0 1.08 1.05 12.0 2.20 6100 64 9.86 31.6
WASP-29 b 0.24 0.74 3.92 0.045 K4V 0.82 0.84 11.3 1.50 4800 74 9.64 30.6
WASP-3 b 1.76 1.39 1.84 0.031 F7V 1.24 1.35 10.6 13.4 6400 33  <0.64 11.3 41.0
WASP-33 b 4.10 1.49 1.21 0.025 A5 1.49 1.44 8.30 90.0 7430 76 12.4 28.5
WASP-37 b 1.69 1.13 3.57 0.043 G2 0.84 0.97 12.7 2.40 5800 77 9.67 37.3
WASP-38 b 2.71 1.07 6.87 0.075 F8 1.21 1.36 9.42 8.60 6150 78 9.64 38.9
WASP-4 b 1.12 1.41 1.33 0.023 G7V 0.90 1.15 12.6 2.20 5500 79  <0.64 10.9 38.9
WASP-5 b 1.63 1.17 1.62 0.027 G4V 1.02 1.08 12.2 3.40 5700 80  <0.64 10.4 39.3
WASP-6 b 0.50 1.22 3.36 0.042 G8 0.00 0.87 12.4 1.40 5450 81 9.89 31.2
WASP-7 b 0.96 0.91 4.95 0.061 F5V 1.28 1.23 9.51 17.2 6400 82 10.5 38.4
WASP-8 b 2.23 1.17 8.15 0.079 G6 1.03 0.95 9.90 2.00 5600 83 8.90 34.8
XO-1 b 0.90 1.18 3.94 0.048 G1V 1.00 0.92 11.3  <3.00 5750 84  <0.64 10.0 35.4
XO-2 b 0.57 0.97 2.61 0.036 K0V 0.98 0.96 11.1  <2.30 5340 85  <0.64 10.1 39.7
XO-3 b 11.7 1.21 3.19 0.045 F5V 1.21 1.37 9.80 18.5 6429 86, 87  <0.64 10.0 41.9
XO-4 b 1.72 1.34 4.12 0.055 F5V 1.32 1.55 10.7 8.80 6397 88 10.4 45.4
XO-5 b 1.07 1.08 4.18 0.048 G8V 0.88 1.06 12.1 0.70 5370 89 8.96 35.3

References. (1) Flux from Kashyap et al. (2008) in units of 10-13 erg s-1 cm-2; (2) Barge et al. (2008); (3) Bonomo et al. (2010); (4) Gandolfi et al. (2010); (5) Gillon et al. (2010); (6) Cabrera et al. (2010); (7) Bouchy et al. (2008); (8) Deleuil et al. (2008); (9) Moutou et al. (2008); (10) Rauer et al. (2009); (11) Fridlund et al. (2010); (12) Léger et al. (2009); (13) Bordé et al. (2010); (14) Deeg et al. (2010); (15) Charbonneau et al. (2009); (16) Butler et al. (2004); (17) Torres (2007); (18) Bakos et al. (2007a); (19) Bakos et al. (2010a); (20) Hartman et al. (2009); (21) Bakos et al. (2009b); (22) Torres et al. (2010); (23) Kovács et al. (2010); (24) Buchhave et al. (2010); (25) Howard et al. (2010); (26) Hartman et al. (2011a); (27) Bakos et al. (2007b); (28) Bakos et al. (2010b); (29) Kipping et al. (2010); (30) Quinn et al. (2010); (31) Hartman et al. (2011b); (32) Torres et al. (2007); (33) Christiansen et al. (2011); (34) Bakos et al. (2007c); (35) Noyes et al. (2008); (36) Pál et al. (2008); (37) Latham et al. (2009); (38) Shporer et al. (2009); (39) Sato et al. (2005); (40) Winn et al. (2009); (41) Bouchy et al. (2005); (42) Winn et al. (2007); (43) Queloz et al. (2000); (44) Brown et al. (2001); (45) Moutou et al. (2009); (46) Borucki et al. (2010); (47) Koch et al. (2010); (48) Dunham et al. (2010); (49) Latham et al. (2010); (50) Jenkins et al. (2010); (51) Holman et al. (2010); (52) Bouchy et al. (2004); (53) Pont et al. (2004); (54) Snellen et al. (2009); (55) Laughlin et al. (2005); (57) Sozzetti et al. (2009); (58) Collier-Cameron et al. (2007); (59) Christian et al. (2009); (60) Bakos et al. (2009a); (61) Hebb et al. (2009); (62) Skillen et al. (2009); (63) Joshi et al. (2008); (64) West et al. (2009); (65) Lister et al. (2009); (66) Anderson et al. (2010); (67) Hellier et al. (2009a); (68) Hebb et al. (2010); (69) Bouchy et al. (2010); (70) Maxted et al. (2010); (71) Street et al. (2010); (72) Enoch et al. (2011); (73) Smalley et al. (2011); (74) Hellier et al. (2010); (76) Collier-Cameron et al. (2010); (77) Simpson et al. (2011); (78) Barros et al. (2011); (79) Wilson et al. (2008); (80) Anderson et al. (2008); (81) Gillon et al. (2009); (82) Hellier et al. (2009b); (83) Queloz et al. (2010); (84) McCullough et al. (2006); (85) Burke et al. (2007); (86) Johns-Krull et al. (2008); (87) Hébrard et al. (2008); (88) McCullough et al. (2008); (89)Pál et al. (2009); (90) Torres et al. (2011); (91) Batalha et al. (2011).

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