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Table C.1

Physical and orbital parameters of potentially favourable exoplanet targets for a UV mission. The density, surface gravity and log10(g) were calculated (alongside their respective errors) for each planet based on the mass and radius. All planets marked with* have Msin(i) instead of M. Planets marked with** had their Teff,P calculated from Equ. 12 from Baeyens et al. (2022), with AB=0 and ƒ=2. Table C.2 list the corresponding host star parameters.

Planet a [AU] P [days] Teff,P [K] MP [MJup] RP [RJup] ρP,bulk [g cm−3] log10(g) [cm s−2]
ups And b 0.05922166±0.00000020 4.617033±0.000023 0.6876±0.0044*
tau Boo A b 0.049±0.003 3 3124568±0 0000069 4.32±0.04*
61 Vir b 0.050201±0.000005 4.2150±0.0006 1397±44** 0.016±0.002*
51 Peg b 0.0527±0.0030 4.230785±0.000036 0.472±0.039*
HD 179949 b 0.0443±0.0026 3.092514±0.000032 0.916±0.076*
HD 75289 b 0.050±0.000* 3.509270±0.000064 1260 0.49±0.03*
KELT-20 b 0.057±0.006 2260±50 17 1.83±0.07
HD 209458 b 3 52474859±0 00000038 1484±18
HD 212301 A b 0 030±0 000 2.24571±0.00028 0.51±0.04* 1.07
HD 149143 b 0 0530±0 0029 4.07182±0.00001 1756±285 ** 1.33±0.15*
HAT-P-7b 0.03813±0.00036 2 204737±0 000017 2733±21 1.806±0.036 1 510±0 020 0 6956±0 0211 3.3121±0.0274
WASP-18b 0 02087±0 00068 2413±44 10.4 1.191±0.038 8 163 4.279
WASP-103b 0.01985±0.00021 0.9255456±0.0000013
WASP-121b 2720±8 1.865±0.044

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