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Table 4

WASP-12b orbital parameters derived from PyORBIT Markov chain Monte Carlo analysis.

Parameter Units Prior Posterior value
Fitted parameters
Orbital period (P) [days] 𝒰 [1.09142090, 0.00000020] 1.09142100.00000020+0.00000019${1.0914210_{ - 0.00000020}^{ + 0.00000019}}$
Impact parameter (b) 𝒰 [0,1 + (R/Rp)/2] 0.4240.013+0.012${0.424_{ - 0.013}^{ + 0.012}}$
Quadratic limb darkening term c1 (RC filter) 𝒰 [0.412, 0.10] 0.3490.029+0.029${0.349_{ - 0.029}^{ + 0.029}}$
Quadratic limb darkening term c2 (RC filter) 𝒰 [0.148, 0.10] 0.1670.049+0.049${0.167_{ - 0.049}^{ + 0.049}}$
Quadratic limb darkening term c1 (SDSS.r filter) 𝒰 [0.428, 0.10] 0.3690.031+0.030${0.369_{ - 0.031}^{ + 0.030}}$
Quadratic limb darkening term c2 (SDSS.r filter) 𝒰 [0.15, 0.10] 0.1090.051+0.053${0.109_{ - 0.051}^{ + 0.053}}$
Derived parameters
Semimajor axis (a) [au] 0.02340.0010+0.0010${0.0234_{ - 0.0010}^{ + 0.0010}}$
Inclination (i) [deg] 81.800.27+0.29${81.80_{ - 0.27}^{ + 0.29}}$
Planet radius (Rp) [RJ] 1.9650.087+0.088${1.965_{ - 0.087}^{ + 0.088}}$
Transit duration (T14) [days] 0.12504 ± 0.00018

Notes. The listed best-fit values and uncertainties are the medians and 15.865th-84.135th percentiles of the posterior distributions, respectively.

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