Three hot Jupiters transiting K-dwarfs with significant heavy element masses

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Table 5

Fitted and derived parameters for the companions presented in this paper.

Parameter			TOI-2969 b	TOI-2989 b	TOI-5300 b
Fitted parameters
Orbital period	P	[days]	1.8237146 ± 0.0000002	3.122832 ± 0.000001	2.262196 ± 0.000003
Time of transit	T₀	[rBJD]^(a)	9303.30015 $_{- 0.00008}^{+ 0.00009}$ $_{-0.00008}^{+0.00009}$	9302.2242 ± 0.0002	9470.4174 ± 0.0002
Radius ratio	R_pl/R_★		0.1613 ± 0.0008	0.152 $_{- 0.001}^{+ 0.002}$ $_{-0.001}^{+0.002}$	0.1389 $_{- 0.0010}^{+ 0.0011}$ $_{-0.0010}^{+0.0011}$
Impact parameter	b		0.713 ± 0.010	${0.36}_{- 0.07}^{+ 0.05}$ $0.36_{-0.07}^{+0.05}$	${0.13}_{- 0.09}^{+ 0.11}$ $0.13_{-0.09}^{+0.11}$
Stellar density	ρ_★	[ρ_⊙]	1.93 ± 0.07	1.8 ± 0.1	${2.13}_{- 0.12}^{+ 0.07}$ $2.13_{-0.12}^{+0.07}$
Eccentricity (fixed)	e		0	0	0
RV semi-amplitude	K	[m s⁻¹]	243 ± 8	$503_{- 37}^{+ 35}$ $503_{-37}^{+35}$	121 ± 22
Derived parameters
Planetary radius	R_pl	[R_Jup]	1.10 ± 0.08	1.12 ± 0.05	0.88 ± 0.08
Planetary mass	M_pl	[M_Jup]	1.16 ± 0.04	3.0 ± 0.2	0.6 ± 0.1
Planetary bulk density	ρ_pl	[g cm⁻³]	${1.1}_{- 0.2}^{+ 0.3}$ $1.1_{-0.2}^{+0.3}$	2.7 ± 0.4	${1.1}_{- 0.3}^{+ 0.4}$ $1.1_{-0.3}^{+0.4}$
Inclination	i	[°]	84.9 ± 0.4	${88.1}_{- 0.3}^{+ 0.4}$ $88.1_{-0.3}^{+0.4}$	${89.2}_{- 0.6}^{+ 0.5}$ $89.2_{-0.6}^{+0.5}$
Semi-major axis	a_pl	[mAU]	26.1 ± 0.2	38.4 ± 0.3	29.5 ± 0.3
Transit duration	T₁₄	[hours]	${1.846}_{- 0.011}^{+ 0.010}$ $1.846_{-0.011}^{+0.010}$	2.68 ± 0.02	2.36 ± 0.02
Equilibrium temperature^(b)	T_eq	[K]	1186 ± 52	$1001_{- 42}^{+ 43}$ $1001_{-42}^{+43}$	$1043_{- 66}^{+ 67}$ $1043_{-66}^{+67}$
Insolation	S_pl	[S_⊕]	$382_{- 11}^{+ 12}$ $382_{-11}^{+12}$	124 ± 4	198 ± 6
CORALIE parameters
Systemic RV	γ_CORALIE	[km s⁻¹]	52.043 ± 0.005	−9.68 ± 0.02	−66.61 ± 0.02
Jitter	σ_CORALIE	[m s⁻¹]	$8_{- 3}^{+ 5}$ $8_{-3}^{+5}$	$3_{- 3}^{+ 16}$ $3_{-3}^{+16}$	$2_{- 2}^{+ 10}$ $2_{-2}^{+10}$
Residual noise	RMS (O-C)	[m s⁻¹]	23	112	68

Notes. The limb darkening and photometric instrumental parameters can be found in Appendix F. The values assumed for the solar and planetary constants are the IAU 2015 Resolution B 3 values from Prša et al. (2016). ^(a)Reduced Barycentric Julian Date in Barycentric Dynamical Time (rBJD_TDB ), obtained by subtracting 2 450 000 from the BJD_TDB. ^(b)Assuming a Bond albedo A = 0.

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