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Table 5

Derived planetary parameters obtained for GJ 357 b, c, and d using the posterior values from Table 4.

Parameter (a) GJ 357 b GJ 357 c GJ 357 d
Derived transit parameters
       
p = RpR
       
b = (aR)cos ip
       
aR
       
ip (deg)
       
u1 (b)
       
u2 (b)
       
tT (h)
       
Derived physical parameters
       
Mp (M) (c)
       
Rp (R)
       
ρp (g cm−3)
       
gp (m s−2)
       
ap (au)
       
Teq (K) (d)
       
S (S)
       

Notes. (a) Error bars denote the 68% posterior credibility intervals. (b) Derived only from the TESS light curve. (c) The masses for GJ 357 c and GJ 357 d are a lower limit (Mp sin i) since they are detected in the RV data only. (d)Equilibrium temperatures were calculated assuming zero Bond albedo.

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