Table B.1
Excerpt from the available electronic data table.
| Planet | Distance | Semi-major Axis | Mpl | Rpl | X-ray | FX | LX | >LXUV | FX, pl | FXUV, pl | Mass-loss |
|---|---|---|---|---|---|---|---|---|---|---|---|
| (pc) | (AU) | (M⊕) | (R⊕) | provenance | (erg s1 cm−2) | (erg s−1) | (erg s−1) | (erg s−1 cm−2) | (erg s−1 cm−2) | (g s−1) | |
| 11 Comb | 93.2 | 1.29 | 6165.6 | 12.4A | E | 2.8e 14 | 2.9e+28 | 2.5e+29 | 6.3e+00 | 5.3e+01 | 6.1e+06 |
| 14 Her b | 17.9 | 2.93 | 1481.1 | 13.1A | X | 2.4e 14 | 9.4e+26 | 1.2e+28 | 3.9e 02 | 5.1e-01 | 2.9e+05 |
| 18 Del b | 76.2 | 2.60 | 3273.5 | 12.7A | R | 2.5e-13C | 1.7e+29 | 1.2e+30 | 9.2e+00 | 6.3e+01 | 1.5e+07 |
| 1RXS J160929.1-210524b | 139 1 | 330.00 | 3000.0 | 12.8A | E | 2.3e 13 | 5.4e+29 | 3.3e+30 | 1.8e 03 | 1.1e 02 | 2.7e+03 |
| 2MASS J01033563-5515561 AB b | 84.00 | E | 7.8e-14C | ||||||||
| 2MASS J01225093-2439505 b | 33.8 | 52.00 | 7786.5 | 12.3A | E | 4.8e 13 | 6.5e+28 | 5.1e+29 | 8.6e 03 | 6.6e 02 | 5.9e+03 |
| 2MASS J02192210-3925225 b | 156.00 | E | 5.3e 14 | ||||||||
| 30 Ari B b | 44.7 | 0.99 | 4392.4 | 12.6A | R | 2.9e 12 | 6.9e+29 | 4.0e+30 | 2.5e+02 | 1.5e+03 | 2.5e+08 |
| 51 Eri b | 29.8 | 12.00 | E | 2.4e 13 | 2.5e+28 | 2.2e+29 | 6.2e 02 | 5.4e-01 | |||
| 55 Cnc b | 12.6 | 0.11 | 255.4 | 14.1A | E | 4.6e 14 | 8.7e+26 | 1.1e+28 | 2.4e+01 | 3.2e+02 | 1.3e+09 |
| 55 Cnc c | 12.6 | 0.24 | 51.2 | 8.4A | E | 4.6e 14 | 8.7e+26 | 1.1e+28 | 5.5e+00 | 7.2e+01 | 3.1e+08 |
| 55 Cnc d | 12.6 | 5.96 | 991.6 | 13.3A | E | 4.6e 14 | 8.7e+26 | 1.1e+28 | 8.7e 03 | 1.1e-01 | 1.0e+05 |
| 55 Cnc e | 12.6 | 0.02 | 8.0 | 1.9 | E | 4.6e 14 | 8.7e+26 | 1.1e+28 | 1.3e+03 | 1.7e+04 | 5.2e+09 |
| 55 Cnc f | 12.6 | 0.77 | 47.8 | 8.0a | E | 4.6e 14 | 8.7e+26 | 1.1e+28 | 5.2e 01 | 6.9e+00 | 2.7e+07 |
| 61 Vir b | 8.5 | 0.05 | 5.1 | 2.1a | E | 7.2e 14 | 6.2e+26 | 8.6e+27 | 8.8e+01 | 1.2e+03 | 8.6e+08 |
| 61 Vir c | 8.5 | 0.22 | 18.2 | 4.5a | E | 7.2e 14 | 6.2e+26 | 8.6e+27 | 4.7e+00 | 6.4e+01 | 1.2e+08 |
| 61 Vir d | 8.5 | 0.48 | 22.9 | 5.2a | E | 7.2e 14 | 6.2e+26 | 8.6e+27 | 9.8e 01 | 1.3e+01 | 3.1e+07 |
| AB Pic b | 50.0 | 260.00 | 4290.5 | 12.6a | E | 2.4e 12 | 7.2e+29 | 4.2e+30 | 3.8e 03 | 2.2e-02 | 3.8e+03 |
| … | … | … | … | … | … | … | … | … | … | … |
Notes. The full table has additional columns and 343 rows. Radius superscript A denotes planets without measured radius values whose radii were estimated according to the mass-radius relationship by Chen & Kipping (2017). The same method was used to estimate planet masses with no measured value, which are denoted with superscript B in the electronic table. Superscript C for the X-ray flux denotes that the host star adopted X-ray flux and all entries derived from it were adjusted for unresolved bound stellar companions. The provenance of the used X-ray flux is given as E, R, X, and C for eROSITA, ROSAT, XMM-Newton, and Chandra, respectively.
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