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Table 1.
Parameters of CVSO 30 and hot-Jupiter candidate CVSO 30 b used in this study.
| Parameter | Value | Source (a) |
|---|---|---|
| Teff [K] | 3470 | B |
| Spectral type | M3 | B |
| Age [Myr] | 2.6 | B |
| vsin(i) [km s−1] | 80 ± 8.1 | E |
| Distance [pc] | 349 ± 9 | G |
| MS [M⊙] | 0.44 | Ba |
| RS [R⊙] | 1.03 | Ba |
| Planetary candidate CVSO 30 b | ||
| T0 [HJD] | 2455543.9402 ± 0.0008 | E |
| Porb [d] | 0.448413 ± 0.00004 | E |
| RP [RJ] | 1.68 ± 0.07 | Ba |
| MP [MJ] | 3.6 ± 0.3 | Ba |
Notes.
(a)
B: Briceño et al. (2005); E: van Eyken et al. (2012); G: Gaia DR2 (Gaia Collaboration 2016, 2018); Ba: Barnes et al. (2013) (solution for MS = 0.44 M⊙).
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