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Table 2

Stellar parameters of Gl 486.

Parameter Value Reference
Basic identifiers and data
Wolf 437 Wol19
Gl 486 Gli69
Karmn J12479+097 AF15, Cab16a
Sp. type M3.5 V PMSU
T (mag) 8.8223 ± 0.0073 ExoFOP-TESS(a)
Astrometry and kinematics
α (J2016.0) 12:47:55.53 Gaia EDR3
δ (J2016.0) +09:44:57.7 Gaia EDR3
µα cos δ (mas a−1) −1008.267 ± 0.040 Gaia EDR3
µδ (mas a−1) −460.034 ± 0.033 Gaia EDR3
ϖ (mas) 123. 722 ± 0.033 Gaia EDR3, Lin21
d (pc) 8.0827 ± 0.0021 Gaia EDR3, Lin21
γ (km s−1) + 19.106 ± 0.013 Sou18
(m s−1 a −1) +0.2274 ± 0.0011 This work
U (km s−1) −20.6015 ± 0.0093 This work
V (km s−1) −39.8626 ± 0.0076 This work
W (km s−1) + 12.440 ± 0.012 This work
Galactic population Thin disc This work
Fundamental parameters
θLDD (mas) 0.390 ± 0.018 This work
R* (R) 0.339 ± 0.015 This work
M* (M) 0.333 ± 0.019 This work
L* (10−6 L) 12120± 82 This work
Teff (K) 3291 ± 75 This work
log gspec 4.82 ± 0.12 Mar21
[Fe/H] 0.15 0.13 Mar21 (b)
Activity and age
v sin i* (km s−1) <2.0 Rei18
Prot,phot (days) 49.9 ± 5.5 This work(c)
pEW(He i D3) (Å) +0.098 ± 0.007 Fuh20
pEW(Hα) (Å) +0.163 ± 0.016 Fuh20
pEW(Ca ii IRT1)(Å) +0.609 ± 0.003 Fuh20
pEW(He i IR) (Å) +0.046 ± 0.013 Fuh20
log RHK This work (d)
〈B〉 (G) <240 Rei22
log Lx (erg s−1) <26.62 Ste13
Age (Ga) 1–8 This work(e)

Notes. Throughout the paper, we use the symbol ‘a’ for annus (year in Latin), the unit of time that is exactly 365.25 days (86 400 s): http://exoterrae.eu/annus.html. (a)See Table A.2 for multi-band photometry different from TESS T. (b)See Sect. 4.3 for an element abundance analysis. (c)See Sect. 4.2 for the Prot determination from ground photometry. (d)From data compiled by Perdelwitz et al. (2021).(e)Passegger et al. (2019) assumed a mean age of 5 Ga.

References. AF15: Alonso-Floriano et al. (2015); Cab16a: Caballero et al. (2016a); ExoFOP-TESS: https://exofop.ipac.caltech.edu/tess/; Fuh20: Fuhrmeister et al. (2020); Gaia EDR3: Gaia Collaboration (2021a); Gli69: Gliese (1969); Lin21: Lindegren et al. (2021); Mar21: Marfil et al. (2021); PMSU: Reid et al. (1995); Rei18: Reiners et al. (2018); Rei22: Reiners et al. (2022); Ste13: Stelzer et al. (2013); Sou18: Soubiran et al. (2018); Wol19: Wolf (1919).

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