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Table 1

TOI-1453 stellar parameters.

Parameter (unit) Value Source(†)
Designations and coordinates
TOI ID 1453
TIC ID 198390247
2MASS ID J17125372+5711520
Gaia DR3 ID 1433062331332673792
RA (J2000) (h m s) 17:12:53.72 1
Dec (J2000) (d m s) +57:11:52.00 1
Magnitudes and astrometric solution
B 12.03±0.15 2
V 11.11±0.08 2
G 10.7279±0.0028 1
J 9.275±0.023 3
H 8.766±0.029 3
K 8.686±0.019 3
W1 8.635±0.023 4
W2 8.678±0.02 4
W3 8.604±0.021 4
µα (mas/yr) –70.974±0.013 1
µδ (mas/yr) –0.085±0.015 1
Parallax π (mas) 12.676±0.010 1
Distance d (pc) 78.885±0.064 5
ULSR (km/s)(1) –58.99±0.36 5
VLSR (km/s)(1) –5.33±0.62 5
WLSR (km/s)(1) –10.61±0.59 5
Physical parameters
Teff(K) 4975±68 5
[Fe/H] (dex) –0.31±0.06 5
log giso (cgs) 4.576±0.015 5
υ sin i (km/s) <2 5
log  (RHK)$\log \,\,\left( {{{R'}_{HK}}} \right)$ –4.91±0.06 5
Mass (M)(2) 0.715±0.035 5
Radius (R)(2) 0.720±0.029 5
ρ (ρ) 1.9180.034+0.076${1.918_{ - 0.034}^{ + 0.076}}$ 5
Age (Gyr) 12.03.8+1.1${12.0_{ - 3.8}^{ + 1.1}}$ 5

Notes.(1) The uncertainties reported on ULSR, VLSR, WLSR account for the uncertainties on the motion of the Sun in the LSR reported by Dehnen & Binney (1998).(2) The uncertainties on the stellar mass and radius account for the systematic differences between various stellar evolution models.(†) 1. Gaia DR3 (Gaia Collaboration 2023). 2. Tycho-2 (Høg et al. 2000). 3. 2MASS (Cutri et al. 2003). 4. WISE (Cutri & et al. 2012). 5. This work.

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