Three warm Jupiters orbiting TOI-6628, TOI-3837, and TOI-5027 and one sub-Saturn orbiting TOI-2328

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Table 4

Stellar parameters.

Parameter	TOI-6628	TOI-3837	TOI-5027	TOI-2328
TIC ID⁽¹⁾	75650448	308073360	361711730	394287035
RA (J2015.5)⁽²⁾	15h03m20.89s	10h10m39.91s	16h15m32.41s	02h06m45.78s
Dec (J2015.5)⁽²⁾	−35d13m50.08s	+24d16m23.24s	−69d13m01.55s	−81d14m50.55s
pmRA (mas/yr)⁽²⁾	−30.17±0.09	50.37±0.07	−22.02±0.03	31.80±0.03
pmDec (mas/yr)⁽²⁾	−15.94 ± 0.06	−37.02±0.07	−31.99±0.04	−1.67±0.03
π (mas)⁽²⁾	3.09±0.06	3.18±0.04	4.86±0.02	4.28±0.02

T (mag)⁽¹⁾	12.084 ± 0.006	11.366±0.007	10.910±0.006	11.584 ± 0.006
V (mag)⁽³⁾	12.771±0.068	11.960±0.028	11.512±0.101	12.297±0.008
B (mag)⁽³⁾	13.801±0.043	12.578±0.097	12.083±0.024	13.096±0.011
G (mag)⁽²⁾	12.640±0.002	11.804 ± 0.002	11.334 ± 0.002	12.108±0.002
J (mag)⁽⁴⁾	11.317±0.025	10.715±0.023	10.316±0.026	10.842±0.023
H (mag)⁽⁴⁾	10.943±0.026	10.401±0.021	10.042±0.023	10.458±0.021
K (mag)⁽⁴⁾	10.836±0.023	10.316±0.017	9.979±0.023	10.395±0.021

Distance (pc)⁽⁵⁾	315.2±8.3	306.7±5.8	202.2±1.5	228.9±1.5
Luminosity (L_⊙)⁽⁵⁾	${0.817}_{- 0.044}^{+ 0.046}$ $0.817_{ - 0.044}^{ + 0.046}$	${1.571}_{- 0.076}^{+ 0.085}$ $1.571_{ - 0.076}^{ + 0.085}$	${0.932}_{- 0.033}^{+ 0.034}$ $0.932_{ - 0.033}^{ + 0.034}$	${0.676}_{- 0.031}^{+ 0.032}$ $0.676_{ - 0.031}^{ + 0.032}$
Mass (M_⊙)⁽⁵⁾	0.97±0.06	0.89±0.05	1.02±0.05	0.95±0.06
Radius (R_⊙ )⁽⁵⁾	${1.01}_{- 0.05}^{+ 0.06}$ $1.01_{ - 0.05}^{ + 0.06}$	${1.20}_{- 0.05}^{+ 0.06}$ $1.20_{ - 0.05}^{ + 0.06}$	0.92±0.04	0.90±0.06
ρ_∗ (kg/cm³)⁽⁵⁾	$1323_{- 187}^{+ 225}$ $1323_{ - 187}^{ + 225}$	$725_{- 98}^{+ 118}$ $725_{ - 98}^{ + 118}$	$1831_{- 44}^{+ 38}$ $1831_{ - 44}^{ + 38}$	$1828_{- 245}^{+ 289}$ $1828_{ - 245}^{ + 289}$
T_eff (K)⁽⁵⁾	$5463_{- 142}^{+ 143}$ $5463_{ - 142}^{ + 143}$	$5905_{- 155}^{+ 157}$ $5905_{ - 155}^{ + 157}$	$5909_{- 144}^{+ 145}$ $5909_{ - 144}^{ + 145}$	$5525_{- 144}^{+ 147}$ $5525_{ - 144}^{ + 147}$
Age (Gyr)⁽⁵⁾	${7.5}_{- 2.5}^{+ 2.4}$ $7.5_{ - 2.5}^{ + 2.4}$	${11.2}_{- 2.6}^{+ 2.5}$ $11.2_{ - 2.6}^{ + 2.5}$	${0.4}_{- 0.3}^{+ 0.6}$ $0.4_{ - 0.3}^{ + 0.6}$	${4.0}_{- 2.7}^{+ 2.3}$ $4.0_{ - 2.7}^{ + 2.3}$
log g (cm s⁻²)⁽⁵⁾	${4.416}_{- 0.025}^{+ 0.024}$ $4.416_{ - 0.025}^{ + 0.024}$	${4.229}_{- 0.019}^{+ 0.018}$ $4.229_{ - 0.019}^{ + 0.018}$	${4.517}_{- 0.008}^{+ 0.006}$ $4.517_{ - 0.008}^{ + 0.006}$	${4.505}_{- 0.020}^{+ 0.021}$ $4.505_{ - 0.020}^{ + 0.021}$
A_v (mag)	${0.313}_{- 0.084}^{+ 0.083}$ $0.313_{ - 0.084}^{ + 0.083}$	${0.228}_{- 0.068}^{+ 0.072}$ $0.228_{ - 0.068}^{ + 0.072}$	${0.100}_{- 0.041}^{+ 0.042}$ $0.100_{ - 0.041}^{ + 0.042}$	${0.262}_{- 0.060}^{+ 0.063}$ $0.262_{ - 0.060}^{ + 0.063}$
[Fe/H] (dex)⁽⁵⁾	0.36±0.02	−0.26±0.05	−0.15±0.03	0.09±0.03
v sin i (km s⁻¹)⁽⁵⁾	3.13±0.20	3.47±0.26	4.52±0.13	2.61±0.25
log(R′_HK)	−4.998±0.013	−5.256±0.19	−4.805±0.066	−5.088±0.053
Rot. period (Upper limit) (days)	16.34±1.89	17.51±2.18	10.31±0.74	17.46±3.02

Notes.⁽¹⁾ TESS (Ricker et al. 2015);⁽²⁾ Gaia Collaboration (2018);⁽³⁾ APASS (Munari et al. 2014);⁽⁴⁾ 2MASS (Skrutskie et al. 2006);⁽⁵⁾ this work. Uncertainties refer to the 68% credibility interval.

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