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) | ![]() |
(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 | |
![]() |
(BMA) this work | |
R⋆ [R⊙] | 0.339 ± 0.016 | (SED) this work |
0.3240 ± 0.0094 | athis work | |
![]() |
(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⊙) | ![]() |
(SED) this work |
ρ⋆ (ρ⊙) | ![]() |
(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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