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Table 1

Sellar parameters of the three planet-host stars.

Parameter TOI-1243 TOI-4529 TOI-5388 Reference (a)
Main identifiers and spectral type
Discovery name LSPM J0902+7138 G 2-21 Wolf 346 Lep05, Gic59, Wol19
Karmn J09029+716 J01078+128 J10087+355 AF15
TIC 219698776 384888319 407591297 Sta18/19
Spectral type M2.0: V M1.5 V M3.0 V This work, Lep13, Rei04
Astrometry
α (J2000) 09:02:55.82 01:07:52.53 10:08:42.37 Gaia DR3
δ (J2000) 71:38:11.3 12:52:51.4 35:32:51.2 Gaia DR3
μα cos δ (mas a−1) −100.482 ± 0.013 275.861 ± 0.036 192.380 ± 0.026 Gaia DR3
μδ(mas a−1) −142.980 ± 0.016 −22.973 ± 0.025 133.239 ± 0.021 Gaia DR3
d(pc) 43.126 ± 0.029 28.384 ± 0.023 18.5538 ± 0.0092 Gaia DR3
Photometry (b)
B (mag) 14.923 ± 0.100 13.601 ± 0.033 14.390 ± 0.011 APASS9, UCAC4, APASS9
V (mag) 13.427 ± 0.037 12.214 ± 0.146 12.728 ± 0.064 APASS9, UCAC4, APASS9
G (mag) 12.3452 ± 0.0028 11.2167 ± 0.0028 11.7206 ± 0.0028 Gaia DR3
T (mag) 11.1966 ± 0.0074 10.1406 ± 0.0073 10.5737 ± 0.0073 Sta18/19
J (mag) 9.731 ± 0.018 8.787 ± 0.020 9.167 ± 0.018 2MASS
H (mag) 9.093 ± 0.017 8.175 ± 0.017 8.618 ± 0.029 2MASS
Ks (mag) 8.878 ± 0.016 7.954 ± 0.024 8.319 ± 0.021 2MASS
Photospheric parameters
Teff(K) 3515 ± 79 3697 ± 71 3440 ± 85 This work
log g (cgs) 4.73 ± 0.12 4.61 ± 0.07 4.99 ± 0.21 This work
[Fe/H] (dex) −0.20 ± 0.16 −0.24 ± 0.07 −0.36 ± 0.20 This work
Physical parameters
Lbol(10−4 L) 358.5 ± 7.2 386.7 ± 7.0 113.40 ± 0.51 This work
R* (R) 0.511 ± 0.024 0.480 ± 0.019 0.300 ± 0.015 This work
M* (M) 0.515 ± 0.027 0.482 ± 0.023 0.292 ± 0.018 This work
ρ* (g cm−3) 5.4 ± 0.8 6.1 ± 0.8 17 ± 3 This work
Stellar activity
v sin i(km s−1) <2 <2 <2 This work
Prot (d) 20.7 ± 1.4(c) This work

Notes. (a) The references cited on this table are Lep05: Lépine & Shara 2005, Gic59: Giclas et al. 1959, Wol19: Wolf 1919, AF15: Alonso-Floriano et al. 2015, Sta18/19: Stassun et al. 2018, 2019, Lep13: Lépine et al. 2013, Rei04: Reid et al. 2004, Gaia DR3: Gaia Collaboration 2023, APASS9: Quirrenbach et al. 2014, UCAC4: Ahn et al. 2012, 2MASS: Skrutskie et al. 2006. (b) We also compiled photometry in the GALEX NUV, SDSS9 u g r i, UCAC4/APASS r i, and WISE W1 W2 W3 W4 bands (Cifuentes et al. 2020). (c) Rotational period derived from the weighted average of periodicities in the spectroscopic activity indicators, photometric data, and the GP hyperparameter Prot.

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