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Table A.1

Irradiation of the planets, energy-limited mass-loss rates, and results from the simulations.

System d log 10( − ΦG) R XUV log 10(el) log 10(sim) log 10(ηeva)
(erg g-1) (Rpl) (g s-1) (g s-1)

WASP-12 b <4.26 13.14  1.20 12.52 11.60 − 0.92
GJ 3470 b  3.89 12.33  1.77 11.53 10.66 − 0.87
WASP-80 b  4.03 13.02  1.24 11.55 10.55 − 1.00
HD 149026 b  4.29 13.00  1.26 11.46 10.43 − 1.03
HAT-P-11 b  3.51 12.55  1.61 10.93 10.29 − 0.64
HD 209458 b <3.06 12.96  1.25 11.02 10.27 − 0.75
55 Cnc e  3.87 12.41  1.59 10.92 10.14 − 0.78
GJ 1214 b  2.93 12.19  1.51 10.25 9.68 − 0.57
GJ 436 b  2.80 12.54  1.48 10.21 9.65 − 0.56
HD 189733 b  4.32 13.26  1.15 11.69 9.61 − 2.08
HD 97658 b  2.98 12.33  1.75 10.01 9.47 − 0.54
WASP-77 b  4.51 13.42  1.10 11.76 8.79 − 2.97
WASP-43 b  4.82 13.54  1.08 11.73 8.04 − 3.69
Corot-2 b  5.19 13.61  1.06 12.33 7.63 − 4.70
WASP-8 b  3.66 13.57  1.07 10.77 5.0 5.77
WASP-10 b  4.08 13.73  1.07 10.86 2.7 8.16
HAT-P-2 b  4.12 14.14 <1.05 10.83 < 5.9 <− 5.4
HAT-P-20 b  4.08 14.18 <1.05 10.33 < 4.5 <− 6.3
Artificial planets
HD 209458 b (2.5)  3.06 13.36  1.10 10.45 7.15 − 3.31
HD 209458 b (5.0)  3.06 13.66  1.04 10.07 < 2.0 <− 8.1
WASP-10 b (0.1)  4.08 12.73  1.42 12.23 11.35 − 0.88
WASP-10 b (0.2)  4.08 13.03  1.25 11.77 10.76 − 1.01
WASP-10 b (0.33)  4.08 13.25  1.16 11.46 9.27 − 2.17
WASP-10 b (0.5)  4.08 13.43  1.10 11.21 7.44 − 3.77

Notes. Ranking according to simulated mass loss. Explanation of the columns: name of the system (mass scaling of artificial planets), XUV flux at planetary distance gravitational potential of the planet, bulk XUV absorption radius in the simulations, energy-limited mass-loss rate (Sanz-Forcada et al. 2011), mass-loss rate in the simulations (1/4 × 4πR2ρv), evaporation efficiency (see text). Mass-loss rates and evaporation efficiencies of hydrodynamically stable atmospheres are printed in italics.

(d)

(<912 Å, erg cm-2 s-1, see Salz et al. 2015b),

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