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Table 1

System parameters of the complete sample (see Sect. 2.1).

Host star Planet


System Sp. type Teff V BV JK d Prot Age Rpl Mpl ρpl Teq Porb a e TD
(K) (mag) (mag) (mag) (pc) (d) (Ga) (Rjup) (Mjup) (g cm-3) (K) (d) (au) (%)

WASP-12 G0V 6300 11.6 0.57 0.29 380 37.5  13.2 1.8 1.4 0.32 2900 1.1 0.023 0.05 1.4
GJ 3470 M1.5 3600 12.3 1.17 0.81 29 20.7  ± 0.2 1.2 0.37 0.044 1.1 650 3.3 0.036 0 0.57
WASP-80 K7-M0V 4150 11.9 0.94 0.87 60 8.1  ± 0.8 0.2 0.95 0.55 0.73 800 3.1 0.034 0 2.9
HD 149026 G0IV 6150 8.1 0.61 79 11.5  1.2 0.65 0.36 1.6 1440 2.9 0.043 0 0.29
HAT-P-11 K4V 4750 9.5 1.19 0.60 37 29.2  2.9 0.42 0.083 1.3 850 4.9 0.053 0.2 0.33
HD 209458 G0V 6065 7.6 0.58 0.28 50 11.4  1.5 1.4 0.69 0.34 1320 3.5 0.047 0 1.5
55 Cnc (e) K0IV-V 5200 6.0 0.87 0.58 12 42.7  ± 2.5 6.7 0.19 0.026 4.2 1950 0.7 0.015 0 0.045
GJ 1214 M4.5 3050 14.7 1.73 0.97 13 44.3  ± 1.2 3.4 0.24 0.020 1.9 550 1.6 0.014 0 1.3
GJ 436 M2.5V 3350 10.6 1.47 0.83 10 56.5  6.5 0.38 0.073 1.7 650 2.6 0.029 0.2 0.70
HD 189733 K0-2V 5040 7.6 0.93 0.53 19 12.0  ± 0.1 0.7 1.1 1.1 0.96 1200 2.2 0.031 0 2.4
HD 97658 K1V 5100 7.7 0.86 0.47 21 38.5  ± 1.0 6.6 0.21 0.025 3.4 750 9.5 0.080 0.06 0.085
WASP-77 G8V 5500 10.3 0.75 0.37 93 15.4  ± 0.4 1.7 1.2 1.8 1.3 1650 1.4 0.024 0 1.7
WASP-43 K7V 4400 12.4 1.00 0.73 80 15.6  ± 0.4 0.8 0.93 1.8 2.9 1350 0.8 0.014 0 2.6
CoRoT-2 G7V 5650 12.6 0.85 0.47 270 4.5  ± 0.1 0.1 1.5 3.3 1.5 1550 1.7 0.028 0.01 2.8
WASP-8 G8V 5600 9.9 0.82 0.41 87 16.4  ± 1.0 1.6 1.0 2.2 2.6 950 8.2 0.080 0.3 1.3
WASP-10 K5V 4700 12.7 1.15 0.62 90 11.9  ± 0.9 0.6 1.1 3.2 3.1 950 3.1 0.038 0.05 2.5
HAT-P-2 F8V 6300 8.7 0.46 0.19 114 3.7  ± 0.4 0.4 1.2 8.9 7.3 1700 5.6 0.068 0.5 0.52
HAT-P-20 K3V 4600 11.3 0.99 0.67 70 14.6  ± 0.9 0.8 0.87 7.3 13.8 950 2.9 0.036 0.01 1.6
WASP-38 F8V 6200 9.4 0.48 0.29 110 7.5  ± 1.0 1.0 1.1 2.7 2.1 1250 6.9 0.076 0.03 0.69
WASP-18 F6IV-V 6400 9.3 0.44 0.28 99 5.0  ± 1.0 0.7 1.3 10.2 10.3 2400 0.9 0.020 0.01 0.92
55 Cnc (b) K0IV-V 5200 6.0 0.87 0.58 12 42.7  ± 2.5 6.7 0.80 700 14.6 0.113 0

Notes. Sorted according to the strength of the simulated mass loss. Explanation of the columns: name of the system, spectral type, effective temperature, visual magnitude, colors (SIMBAD), distance, stellar rotation period, gyrochronological age according to Brown (2014) or mean of the three color based age estimates from the same author, planetary radius, mass, density, equilibrium temperature or where cited average dayside brightness temperature, orbital period, semimajor axis, orbit eccentricity, and transit depth.

Reference. The data were compiled using exoplanets.org (Wright et al. 2011) and the following publications: HAT-P-2: Bakos et al. (2007), van Leeuwen (2007), Pál et al. (2010), Prot from v sini, Teq varies due to eccentricity (1250 to 2150 K); WASP-38: Barros et al. (2011), Brown et al. (2012); WASP-77: Maxted et al. (2013); WASP-10: Christian et al. (2009), Johnson et al. (2009), Smith et al. (2009), Prot from (Salz et al. 2015b); HAT-P-20: Bakos et al. (2011), Prot from (Salz et al. 2015b); WASP-8: Queloz et al. (2010), Cubillos et al. (2012), Prot from (Salz et al. 2015b); WASP-80: Triaud et al. (2013), Prot from v sini; WASP-43: Hellier et al. (2011); WASP-18: Hellier et al. (2009), Pillitteri et al. (2014), Prot from v sini; HD 209458: Charbonneau et al. (2000), Henry et al. (2000), Torres et al. (2008), Silva-Valio (2008), dayside brightness temperature from Spitzer observation (Crossfield et al. 2012); HD 189733: Bouchy et al. (2005), Henry & Winn (2008), Southworth (2010), dayside brightness temperature from Spitzer observation (Knutson et al. 2007); GJ 1214: Charbonneau et al. (2009), Berta et al. (2011), Narita et al. (2013); GJ 3470: Bonfils et al. (2012), Biddle et al. (2014); GJ 436: Butler et al. (2004), Knutson et al. (2011); 55 Cnc: Butler et al. (1997), McArthur et al. (2004), Gray et al. (2003), Fischer et al. (2008); HAT-P-11: Bakos et al. (2010); HD 149026: Sato et al. (2005), Prot from v sini, dayside brightness temperature from Spitzer observation (Knutson et al. 2009); HD 97658: Howard et al. (2011), Henry et al. (2011); WASP-12: Hebb et al. (2009), Prot upper limit from v sini, dayside brightness temperature from HST WFC3 observation (Swain et al. 2013); CoRoT-2: Alonso et al. (2008), Lanza et al. (2009), Schröter et al. (2011).

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