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Table A.4

Results obtained using our formalism for various telluric exoplanets.

Exoplanet Wind rM /RP α0 Prob. α0, periα0, apo
impact (°) (°)
Barnard’s b Super-Alf. 7.91 ± 0.16 20.84 ± 0.22 1.0 ± 0.0 2.4 ± 0.6
GJ 3323 b Super-Alf. 2.39 ± 0.05 40.3 ± 0.5 0.19 ± 0.02 3.6 ± 1.0
GJ 3323 c Super-Alf. 1.88 ± 0.04 46.8 ± 0.6 0.03 ± 0.01 4.5 ± 2.1
GJ 581 e Super-Alf. 2.69 ± 0.06 37.6 ± 0.5 0.32 ± 0.03 4.8 ± 0.9
K2-3 d Super-Alf. 1.83 ± 0.08 47.8 ± 1.4 0.03 ± 0.01 1.1 ± 0.6
Kepler-1185 b Super-Alf. 5.63 ± 0.15 24.9 ± 0.3 1.0 ± 0.0 0.0 ± 0.0
Kepler-1229 b Super-Alf. 4.98 ± 0.23 26.6 ± 0.7 0.98 ± 0.01 0.0 ± 0.0
Kepler-1649 b Super-Alf. 1.95 ± 0.05 45.8 ± 0.7 0.05 ± 0.01 0.0 ± 0.0
Kepler-186 f Super-Alf. 6.80 ± 0.15 22.6 ± 0.3 1.0 ± 0.0 0.0 ± 0.0
Kepler-22 b Super-Alf. 9.3 ± 0.3 19.1 ± 0.3 1.0 ± 0.0 0.0 ± 0.0
Kepler-442 b Super-Alf. 11.9 ± 0.3 16.83 ± 0.20 1.0 ± 0.0 0.24 ± 0.15
Kepler-62 e Super-Alf. 10.2 ± 0.3 18.3 ± 0.2 1.0 ± 0.0 0.0 ± 0.0
Kepler-62 f Super-Alf. 12.7 ± 0.3 16.32 ± 0.21 1.0 ± 0.0 0.0 ± 0.0
Proxima Cen b Super-Alf. 1.86 ± 0.04 47.3 ± 0.7 0.03 ± 0.01 3.7 ± 2.2
Ross 128 b Sub-Alf. 1.25 ± 0.03 63.6 ± 1.3 0.0 ± 0.0 7 ± 4
Teegarden’s b Super-Alf. 1.87 ± 0.04 47.1 ± 0.7 0.03 ± 0.01 1.6 ± 0.9
Teegarden’s c Super-Alf. 1.81 ± 0.04 48.1 ± 0.6 0.02 ± 0.0 1.7 ± 1.0
Trappist-1 c Sub-Alf. 1.26 ± 0.03 62.8 ± 1.3 0.0 ± 0.0 2.9 ± 1.7
Trappist-1 d Sub-Alf. 1.19 ± 0.03 66.4 ± 1.5 0.0 ± 0.0 2.7 ± 1.6
Trappist-1 e Sub-Alf. 1.27 ± 0.03 62.8 ± 1.3 0.0 ± 0.0 2.6 ± 1.5
Trappist-1 g Super-Alf. 1.38 ± 0.03 58.3 ± 1.1 0.0 ± 0.0 1.3 ± 0.7
Trappist-1 h Super-Alf. 1.35 ± 0.15 61 ± 7 0.0 ± 0.0 0.0 ± 0.0
Wolf 1061 b Super-Alf. 2.25 ± 0.05 41.9 ± 0.5 0.01 ± 0.02 2.9 ± 1.2
YZ Cet b Sub-Alf. 1.84 ± 0.05 47.6 ± 0.8 0.03 ± 0.01 1.7 ± 1.0
YZ Cet c Sub-Alf. 1.88 ± 0.04 46.9 ± 0.7 0.03 ± 0.01 1.8 ± 1.1
YZ Cet d Super-Alf. 1.89 ± 0.04 46.7 ± 0.7 0.03 ± 0.02 2.9 ± 1.3

Notes. α0, periα0, apo is the difference in aperture angles between the orbital periastron and apastron. The rest of the columns are described in the text.

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