Table 4
Parameters describing the MASCARA-1 system, derived from the best-fit models to the photometric and spectroscopic data.
Parameter | Symbol | Value | |
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Stellar parameters | |||
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Identifiers | HD 201585, HIP 104513 | ||
Right ascension | 21h10m12.37s | ||
Declination | + 10°44′19.9″ | ||
Spectral type | A8 | ||
V-band magnitude | m V | 8.3 | |
Agea | 1.0 ± 0.2 Gyr | ||
Effective temperatureb | T eff | 7554 ± 150 K | |
Projected rotation speed | vsini⋆ | 109 ± 4 km s-1 | |
Surface gravity | log g | 4 | |
Metallicity | [Fe/H] | 0 | |
Stellar massa | M ∗ | 1.72 ± 0.07 M⊙ | |
Stellar radius | R ∗ | 2.1 ± 0.2 R⊙ | |
Stellar density | ρ ∗ |
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Planet parameters | |||
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Planet radiusc | R p | 1.5 ± 0.3 RJup | |
Planet mass | M p | 3.7 ± 0.9 MJup | |
Planet density | ρ p | 1.5 ± 0.9 g cm-3 | |
Equilibrium temperatured | T eq |
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System parameters | |||
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Epoch | T p | 2 457 097.278 ± 0.002 BJD | |
Period | P | 2.148780 ± 0.000008 days | |
Semi-major axis | a | 0.043 ± 0.005 AU | |
Inclination | i |
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Eccentricity | e | 0 (fixed) | |
Projected obliquity | λ | 69.5° ± 3 |
Notes.
(a)
Computed using the BAGEMASS code from Maxted et al. (2015).
(b)
Taken from McDonald et al. (2012), assuming a typical uncertainty.
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