Table 7
Adopted orbital and planetary parameters for HAT-P-42b and HAT-P-43b assuming circular orbits.
HAT-P-42 | HAT-P-43 | |
Parameter | Value | Value |
|
||
Light curve parameters | ||
P (days) | 4.641878 ± 0.000032 | 3.332687 ± 0.000015 |
Tc (BJD)a | 2 455 952.52603 ± 0.00075 | 2 455 997.37106 ± 0.00032 |
T14 (days)a | 0.1681 ± 0.0039 | 0.1354 ± 0.0011 |
T12 = T34 (days)a | 0.0193 ± 0.0037 | 0.0149 ± 0.0009 |
a/R⋆ |
![]() |
![]() |
ζ/R⋆b | 13.40 ± 0.14 | 16.60 ± 0.08 |
Rp/R⋆ | 0.0860 ± 0.0033 | 0.1193 ± 0.0018 |
b 2 |
![]() |
![]() |
b ≡ acosi/R⋆ |
![]() |
![]() |
i (deg) |
![]() |
88.7 ± 0.7 |
Limb-darkening coefficients c | ||
c1,i (linear term) | 0.2863 | 0.3003 |
c2,i (quadratic term) | 0.3274 | 0.3180 |
RV parameters | ||
K (m s-1) | 113.5 ± 7.9 | 87.7 ± 7.7 |
e | 0 (fixed) | 0 (fixed) |
Planetary parameters | ||
Mp (MJ) | 1.044 ± 0.083 | 0.662 ± 0.060 |
Rp (RJ) | 1.280 ± 0.153 |
![]() |
C(Mp,Rp)d | 0.23 | 0.09 |
ρp (g cm-3) |
![]() |
0.39 ± 0.05 |
log gp (cgs) | 3.20 ± 0.10 | 3.00 ± 0.05 |
a (AU) | 0.0575 ± 0.0011 |
![]() |
Teq (K)e | 1428 ± 60 | 1361 ± 25 |
Θf |
![]() |
0.044 ± 0.004 |
⟨ F ⟩ (108 erg s-1 cm-2)g | 9.38 ± 1.56 |
![]() |
Notes.
Reported times are in Barycentric Julian Date calculated directly from UTC, without correction for leap seconds. Tc: reference epoch of mid transit that minimizes the correlation with the orbital period. T14: total transit duration, time between first to last contact; T12 = T34: ingress/egress time, time between first and second, or third and fourth contact.
Reciprocal of the half duration of the transit used as a jump parameter in our MCMC
analysis in place of
a/R⋆. It is related
to a/R⋆ by the
expression (Bakos et al. 2010).
Values for a quadratic law, adopted from the tabulations by Claret (2004) according to the spectroscopic (SPC) parameters listed in Table 5.
Planet equilibrium temperature averaged over the orbit, calculated assuming a Bond albedo of zero, and that flux is re-radiated from the full planet surface.
The Safronov number is given by (see Hansen & Barman 2007).
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