Open Access

Table 1

Stellar properties of TOI-396.

Star names TOI-396
TIC 178155732
HR 858
HD 17926
HIP 13363
Gaia DR3 5064574724769475968

Parameter value Source

RA (h:min:s) 02:51:56.25 Gaia DR3
Dec (º:′:″) −30:48:52.26 Gaia DR3
B 6.862 ± 0.015 Perryman et al. (1997)
V 6.382 ± 0.010 Perryman et al. (1997)
BT 6.956 ± 0.015 Høg et al. (2000)
VT 6.438 ± 0.010 Høg et al. (2000)
J 5.473 ± 0.027 Cutri et al. (2003)
H 5.225 ± 0.034 Cutri et al. (2003)
K 5.149 ± 0.020 Cutri et al. (2003)
G 6.2650 ± 0.0028 Gaia DR3
GRP 6.5100 ± 0.0029 Gaia DR3
GBP 5.8555 ± 0.0038 Gaia DR3
π (mas) 31.564 ± 0.035 Gaia DR3 (a)

Teff (K) 6354 ± 70 Spectroscopy
[Fe/H] 0.025 ± 0.050 Spectroscopy
[Mg/H] −0.01 ± 0.07 Spectroscopy
[Si/H] −0.03 ± 0.05 Spectroscopy
log g (cgs) 4.30 ± 0.06 Spectroscopy
v sin i (km s−1) 7.5 ± 0.2 Spectroscopy
logRHK$\log {\rm{R}}_{{\rm{HK}}}^\prime $ -4.926 ± 0.014 Spectroscopy
Prot,⋆ (d) 6.7 ± 1.3 logRHK$\log {\rm{R}}_{{\rm{HK}}}^\prime $
R (R) 1.258 ± 0.019 π and photometry (b)
M (M) 1.204 ± 0.052 Isochrones
t (Gyr) 2.0 ± 0.6 Isochrones
L (L) 2.31 ± 0.12 From Teff and R
P (P) 0.605 ± 0.038 From M and R

Notes. RA and Dec are reported as in J2000 reference frame. Values in the bottom half of the table have been derived as part of this paper. (a) Zero-point correction from Lindegren et al. (2021) applied. (b)R is computed within the isochrone placement interpolation scheme as PARSEC isochrones convert stellar luminosity into absolute magnitudes via a series of bolometric correction tables built as explained in Marigo et al. (2017) and references therein.

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