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Table 2

Astrometry, photometry, and spectroscopy stellar properties of TOI-2015.

Star information
Identifying information
TOI 2015
TIC 368287008
DR3 ID 1270814787767025408
2MASS J1523191+2721388
WISE J152831.86+272139.5

Parameter Value Source

Parallax and distance
RA (J2000) 15:28:31.84 (1)
Dec (J2000) +27:21:39.86 (1)
Parallax (mas) 21.13 ± 0.02 (1)
μRA (mas yr−1) −56.244 ± 0.010 (1)
μDec (mas yr−1) 63.807 ± 0.014 (1)
Distance (pc) 47.32 ± 0.05 (1)

Photometric properties
TESSmag 12.839 ± 0.007 (2)
Vmag (UCAC4) 16.11 ± 0.20 (3)
Bmag (UCAC4) 17.13 ± 0.10 (3)
Jmag (2MASS) 11.12 ± 0.02 (4)
Hmag (2MASS) 10.52 ± 0.02 (4)
Kmag (2MASS) 10.26 ± 0.02 (4)
Gmag (Gaia DR3) 14.176 ± 0.001 (1)
W1mag (WISE) 10.098 ± 0.022 (5)
W2mag (WISE) 9.93 ± 0.02 (5)
W3mag (WISE) 9.77 ± 0.04 (5)
W4mag (WISE) 9.32 (5)

Spectroscopic and derived parameters
Teff (K) 329728+14$\[\mathbf{3297_{-28}^{+14}}\]$ (BAM) this work
3211 ± 51 (MAROON-X) this work
3200 ± 75 (SED) this work
log g (dex) 5.04 ± 0.04 [MAROON-X] this work
5.01 ± 0.02 (SED) this work
(Fe/H) (dex) +0.29 ± 0.13 (optical) this work
0.31 ± 0.16 (MAROON-X) this work
M [M] 0.33 ± 0.02 (SED) this work
0.3043 ± 0.0067 athis work
0.30410.0312+0.0353$\[\mathbf{0.3041_{-0.0312}^{+0.0353}}\]$ (BMA) this work
R [R] 0.339 ± 0.016 (SED) this work
0.3240 ± 0.0094 athis work
0.32730.0051+0.0029$\[\mathbf{0.3273_{-0.0051}^{+0.0029}}\]$ (BMA) this work
Fbol [erg cm−2 s−1] 1.552 ± 0.018 × 10−11 (SED) this work
AV (mag) 0.02 ± 0.02 (SED) this work
L (L) 0.03220.0025+0.0028$\[0.0322_{-0.0025}^{+0.0028}\]$ (SED) this work
ρ (ρ) 8.370.98+1.03$\[8.37_{-0.98}^{+1.03}\]$ (BMA) this work
Age (Gyr) ≲ 5–6 (Hα) this work
v sin i (km s−1) ≲ 2 (MAROON-X) this work
Spectral type M4±0.5 (NIR) this work
M4.5±0.5 (optical) this work

Notes. (1) Gaia EDR3 Gaia Collaboration (2021); (2) TESS Input Catalog Stassun et al. (2018b); (3) UCAC4 Zacharias et al. (2012); (4) 2MASS Skrutskie et al. (2006); (5) WISE Cutri et al. (2021). (a)Stellar mass and radius values are computed from Mann et al. (2015); Mann et al. (2019). Parameters in bold are the stellar parameters used in priors for photodynamical modeling presented in Section 5.

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