Table 1
Parameters of the planets considered for the comparison with the results of Salz et al. (2016a).
| Planet | Mpl [M⊕] | Rpl [R⊕] | Teq [K] | a [AU] | M* [M⊙] | FX [erg s−1 cm−2] | FEUV [erg s−1 cm−2] | Ṁsalz2016 [g s−1] | Ṁwind [g s−1] | Ṁdef [g s−1] |
|---|---|---|---|---|---|---|---|---|---|---|
| GJ 3470 b | 14.0 | 4.14 | 650 | 0.036 | 0.539 | 1170.4 | 6431.6 | 1.86 × 1011 | 1.51 × 1011 | 2.10 × 1011 |
| HAT-P-11 b | 26.4 | 4.70 | 850 | 0.053 | 0.8 | 449.1 | 2706.3 | 8.08 × 1010 | 8.01 × 1010 | 8.69 × 1010 |
| GJ 1214 b | 6.36 | 2.69 | 550 | 0.014 | 0.18 | 147.5 | 739.0 | 1.98 × 1010 | 2.05 × 1010 | 2.54 × 1010 |
| GJ436b | 23.2 | 4.25 | 650 | 0.029 | 0.45 | 38.6 | 583.6 | 1.88 × 1010 | 1.53 × 1010 | 1.56 × 1010 |
| HD 97658 b | 7.95 | 2.35 | 750 | 0.08 | 0.85 | 92.2 | 860.5 | 1.23 × 1010 | 1.12 × 1010 | 1.50 × 1010 |
| HD 149026 b | 114.4 | 7.28 | 1440 | 0.043 | 1.3 | 7655.8 | 12134 | 1.10 × 1011 | 1.11 × 1011 | 1.50 × 1011 |
| HD 189733 b | 349.8 | 12.31 | 1200 | 0.031 | 0.81 | 5600.2 | 15073 | 1.59 × 1010 | 1.39 × 1010 | 2.05 × 1010 |
| HD 209458 b | 219.4 | 15.67 | 1320 | 0.047 | 1.12 | 40.4 | 1113.6 | 8.16 × 1010 | 1.67 × 1011 | 2.62 × 1011 |
| WASP-80b | 174.88 | 10.64 | 800 | 0.034 | 0.57 | 2177.6 | 8870.9 | 1.46 × 1011 | 1.92 × 1011 | 2.18 × 1011 |
Notes. The last three columns correspond to the atmospheric mass-loss rate obtained by Salz et al. (2016a, ṀSalz2016) and obtained with our model including (Ṁwind) and excluding (Ṁdef) wind advection in the Cloudy computation. According to Salz et al. (2016a), the planetary and stellar parameters were adopted from the following studies. GJ 3470 b: Bonfils et al. (2012); Biddle et al. (2014) ; HAT-P-11 b: Bakos et al. (2010); GJ 1214b: Charbonneau et al. (2009); Berta et al. (2011); GJ 436 b: Butler et al. (2004); Knutson et al. (2011); HD 97658 b: Howard et al. (2011); HD 149026 b: Sato et al. (2005); Knutson et al. (2009); HD 189733 b: Bouchy et al. (2005); Henry & Winn (2008); Southworth (2010); Knutson et al. (2009); HD 209458 b: Charbonneau et al. (2000); Henry et al. (2000); Torres et al. (2008); Silva-Valio (2008); Crossfield et al. (2012); and WASP-80 b: Triaud et al. (2013). The values of the atmospheric mass-loss rates given here are a factor of four higher compared to those given in Table 3 of Salz et al. (2016a), as we do not apply surface averaging.
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