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Table 4

Stellar and planetary parameters derived from the multi-colour joint transit analysis of WASP-74 b.

Parameter Unit Value(a)
Ephemeris
T0 [BJD] 2457173.871756 ± 9 × 10−5
     
P [d] 2.13775138 ± 2.4 × 10−7
     
T14 [h] 2.38 ± 0.02
Fitted parameters
kg 0.09943 ± 0.00081
     
kr 0.09762 ± 0.00072
     
ki 0.09627 ± 0.00063
     
ks 0.09376 ± 0.00064
     
kCI 0.09844 ± 0.00119
     
kBI 0.09128 ± 0.00040
     
kz 0.09376 ± 0.00064
     
kJ 0.08976 ± 0.00158
     
kH 0.09544 ± 0.00154
     
kK 0.09477 ± 0.00246
     
k3.6μm 0.09406 ± 0.00070
     
k4.5μm 0.09509 ± 0.00073
     
as [R] 4.97 ± 0.03
     
b 0.84 ± 0.01
     
ρ [g cm−3] 0.509 ± 0.01
Derived parameters(b)
Rp,g [RJ] 1.429 ± 0.045
     
Rp,r [RJ] 1.403 ± 0.044
     
Rp,i [RJ] 1.383 ± 0.043
     
Rp,z [RJ] 1.348 ± 0.042
     
Rp,CI [RJ] 1.415 ± 0.046
     
Rp,BI [RJ] 1.312 ± 0.040
     
Rp,J [RJ] 1.290 ± 0.045
     
Rp,H [RJ] 1.372 ± 0.047
     
Rp,K [RJ] 1.362 ± 0.055
     
Rp,3.6μm [RJ] 1.352 ± 0.042
     
Rp,4.5μm [RJ ] 1.367 ± 0.043
     
a [AU] 0.0334 ± 0.001
     
i [deg] 80.32 ± 0.09
Teq [K] 1865 ± 20

Notes. (a) The estimates correspond to the posterior median (P50) with 1σ uncertainty estimate based on the 16th and 84th posterior percentiles (P16 and P84, respectively) for symmetric, approximately normal posteriors. For asymmetric, unimodal, posteriors, the estimates are . (b) The derived planetary parameters are based on the stellar parameters shown in Table 2.

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