Table C.2
Physical parameters of the exoplanet host stars of potentially favourable targets for a UV mission.
| Star | Teff [K] | M, [M0] | R, [Rø] | Spectral Type | [Fe/H] | Planet |
|---|---|---|---|---|---|---|
| HD 9826 |  |
 |
 |
F8 V | 0 09±0 06 | ups And b |
| HD 120136 |  |
 |
 |
F7 V | 0 2642300±0 0199902 | tau Boo A b |
| HD 115617 | 5577±33 | 0.942 +0.034-0.029 | 0.963±0.011 | G5 V | −0 01 | 61 Vir b |
| HD 217014 |  |
 |
 |
G2 IV | 0 2057±0 0598 | 51 Peg b |
| HD 179949 | 6168 | 1.21 | 1 2202±0 0375 | F8 V | 0 137 | HD 179949 b |
| HD 75289 | 6117±16 | 1.29±0.10 | 1 23±0 02 | G0 | 0 26 | HD 75289 b |
| HD 185603 |  |
 |
1 60±0 06 | A2 V | −0 02±0 07 | KELT-20 b |
| HD 209458 | 6065±50 | 1.119±0.033 |  |
G0 V | 0 01 | HD 209458 b |
| HD 212301 A | 6239±24 | 1 55±0 16 | 1 16±0 02 | F8 V | 0 18 | HD 212301 Ab |
| HD 149143 | 5856 | 1.20±0.20 | 1 44±0 08 | G0 | 0 29 | HD 149143 b |
| HAT-P-7 | 6449±129 |  |
 |
F8 | 0 260±0 080 | HAT-P-7b |
| WASP-18 | 6431±48 | 1 46±0 29 | 1 26±0 04 | F6 IV-V | 0 11±0 08 | WASP-18b |
| WASP-103 | 6110±160 |  |
 |
F8 V |  |
WASP-103b |
| WASP-121 | 6459±140 |  |
1 458±0 030 | F6 V | 0 13±0 09 | WASP-121b |
References: ups And b: Curiel et al. (2011), Stassun et al. (2019), Fuhrmann et al. (1998); tau Boo A b: Butler et al. (1997), Stassun et al. (2019), Borsa et al. (2015); 61 Vir b: Vogt et al. (2010); 51 Peg b: Butler et al. (2006), Keenan & McNeil (1989), Rosenthal et al. (2021), Stassun et al. (2019); HD 179949 b: Butler et al. (2006), Rosenthal et al. (2021); HD 75289 b: Stassun et al. (2017), Udry et al. (2000); KELT-20 b: Talens et al. (2018), Lund et al. (2017); HD 209458 b: Bonomo et al. (2017), Evans et al. (2015), Stassun et al. (2017), Stassun et al. (2019); HD 212301 A b: Stassun et al. (2017), Lo Curto et al. (2006); HD 149143 b: Ment et al. (2018); HAT-P-7 b: Bonomo et al. (2017), Stassun et al. (2017), Berger et al. (2018), Morris et al. (2013), Stassun et al. (2019); WASP-18b: Shporer et al. (2019), Salz et al. (2015), Southworth (2012), Stassun et al. (2019); WASP-103b: Gillon et al. (2014), Bonomo et al. (2017), Southworth & Evans (2016); WASP-121b: Delrez et al. (2016), Mikal-Evans et al. (2019), Stassun et al. (2019).
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