Open Access

Table 1

Stellar parameters of HD 207496.

Parameter Value and uncertainty
RAGaia-CRF2(hh:mm:ss.ssss) 21:54:52.40
DecGaia-CRF2 (dd:mm:ss.ss) −77:20:19.78
G mag 7.9836 ± 0.0028
K mag(•) 5.967 ± 0.026
H mag (•) 6.085 ± 0.023
J mag(•) 6.570 ± 0.023
Effective temperature Teff (K)] 4819 ± 94
Surface gravity log g (g cm−2) 4.4 ± 0.21
Surface gravity log g(1) (g cm−2) 4.507 ± 0.04
Microturbulence (m s−1) 0.62 ± 0.19
Iron abundance [Fe/H] (dex) 0.095 ± 0.038
Magnesium abundance [Mg/H] (dex) 0.06 ± 0.09
Silicon abundance [Si/H] (dex) 0.11 ± 0.07
Carbon abundance [C/H](2) (dex) 0.01 ± 0.12
Oxygen abundance [O/H](2) (dex) 0.07 ± 0.11
log −4.457 ± 0.053
Spectral type K2.5V
Parallax(*) p (mas) 42.2929703 ± 0.018
Distance to Earth(*) d (pc) 23.63825230 ± 0.012
Stellar mass M (M) 0.80 ± 0.04
Stellar radius R (R) 0.769 ± 0.026
Stellar density ρ (p) 1.77 ± 0.20
Stellar age τ (Gyr) 0.52 ± 0.26
Stellar rotation PRot (days) 12.36 ± 0.12

Notes. (*)Parallax from Gaia EDR3 (Gaia Collaboration 2021) using the formulation of Lindegren et al. (2021). Distance from Bailer-Jones et al. (2021).(•) B and V magnitudes from Høg et al. (2000) and K, H, and J from Cutri et al. (2003).(1) Trigonometric surface gravity derived using the Gaia eDR3 parallaxes (Gaia Collaboration 2021).(2) The carbon and oxygen abundance have been estimated using a random forest machine learning method which uses Fe and Mg abundances as input.

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