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Table 5

Median and 1-σ limits of the marginalized posterior distributions obtained for the WASP-64 system parameters as derived from our MCMC analysis.

WASP-64

Free parameters e ≥ 0 e = 0 (adopted)

Planet/star area ratio (Rp/R)2 [%] 1.524 ± 0.025 1.522 ± 0.025
b′ = acosip/R [R]
Transit width W [d] 0.10005 ± 0.00047 0.09999 ± 0.00046
T0 − 2 450 000 [HJDTDB] 5582.60171 ± 0.00026 5582.60169 ± 0.00027
Orbital period P [d] 1.5732918 ± 0.0000015 1.5732918 ± 0.0000015
RV K2 [m s-1 d1/3] 248 ± 14 257 ± 11
RV γ [km s-1] 33.191 ± 0.010 33.1854 ± 0.0057
0 (fixed)
 −0.10 ± 0.15 0 (fixed)
c1V 1.167 ± 0.058 1.168 ± 0.058
c2V 0.017 ± 0.056 0.016 ± 0.061
c1Gunn − r 0.983 ± 0.050 0.985 ± 0.050
c2Gunn − r −0.121 ± 0.044 −0.122 ± 0.045
c1BB 1.040 ± 0.045 1.041 ± 0.045
c2BB −0.129 ± 0.053 −0.125 ± 0.051
c1I + z 0.859 ± 0.053 0.856 ± 0.053
c2I + z −0.206 ± 0.041 −0.208 ± 0.0241
Teff [K]a 5400 ± 100 5400 ± 100
[Fe/H]a −0.08 ±  0.11 −0.08 ±  0.11

Deduced stellar parameters

Density ρ [ρ]
Surface gravity log g [cgs] 4.392 ± 0.016
Mass M [M] 1.004 ± 0.028
Radius R [R] 1.058 ± 0.025
Luminosity L [L] 0.90 ± 0.15 0.95 ± 0.13
u1V 0.470 ± 0.033 0.470 ± 0.035
u2V 0.226 ± 0.027 0.227 ± 0.028
u1Gunn − r 0.369 ± 0.027 0.370 ± 0.027
u2Gunn − r 0.245 ± 0.020 0.246 ± 0.020
u1BB 0.391 ± 0.025 0.392 ± 0.025
u2BB 0.259 ± 0.023 0.259 ± 0.022
u1I + z 0.302 ± 0.028 0.301 ± 0.028
u2I + z 0.255 ± 0.017 0.255 ± 0.018

Deduced planet parameters

RV K [m s-1] 214 ± 13 221 ± 11
Rp/R 0.1234 ± 0.0011 0.1234 ± 0.0011
btr [R]
boc [R]
Toc − 2 450 000 [HJDTDB] 5583.38834 ± 0.00029
Orbital semi-major axisa [AU] 0.02648 ± 0.00024
a/R
Orbital inclination ip [deg]
Orbital eccentricitye , < 0.132 (95%) 0 (fixed)
Argument of periastron ω [deg]
Equilibrium temperature Teq [K]b 1689 ± 49
Density ρp [ρJup]
Surface gravity log gp [cgs] 3.292 ± 0.030
Mass Mp [MJup] 1.217 ± 0.083 1.271 ± 0.068
Radius Rp [RJup] 1.271 ± 0.039

Notes. 

(a)

Using as priors the spectroscopic values given in Table 3.

(b)

Assuming a null Bond albedo (AB = 0) and isotropic reradiation (f = 1/4).

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