Parameter . | Value . | Source . |
---|---|---|
Designations and coordinates | ||
EPIC ID | 211682544 | EPIC |
K2 ID | 263 | |
2-MASS ID | J08384378+1540503 | |
RA (J2000) | 08:38:43.78 | 2MASS |
Dec. (J2000) | 15:40:50.4 | 2MASS |
Magnitudes and parallax | ||
B | 12.35 ± 0.03 | APASS |
V | 11.61 ± 0.04 | APASS |
Kepler magnitude | 11.41 | EPIC |
J | 10.22 ± 0.02 | 2MASS |
H | 9.81 ± 0.02 | 2MASS |
K | 9.75 ± 0.02 | 2MASS |
Parallax π | 6.1262 ± 0.0514 | Gaia DR2 |
Distance d (pc) | 163.2 ± 1.4 | a |
Atmospheric parameters: effective temperature Teff, | ||
surface gravity log g, metallicity |$[\rm {Fe/H}]$|, projected | ||
rotational velocity vsin i, microturbulence ξt | ||
Teff (K) | 5372 ± 73 | b |
log g (cgs) | 4.58 ± 0.13 | b |
|$[\rm {Fe/H}]$| (dex) | −0.08 ± 0.05 | b |
ξt (km s−1) | 0.76 ± 0.08 | b |
Teff (K) | 5365 ± 50 | c |
log g [cgs] | 4.45 ± 0.10 | c |
|$[\rm {m/H}]$| (dex) | −0.07 ± 0.08 | c |
vsin i (km s−1) | <2.0 | c |
Adopted averaged parameters | ||
Teff (K) | 5368 ± 44 | |
log g (cgs) | 4.51 ± 0.08 | |
|$[\rm {m/H}]$| (dex) | −0.08 ± 0.05 | |
Mass, radius, age, luminosity | ||
M* (M⊙) | 0.86 ± 0.03 | d |
R* (R⊙) | 0.84 ± 0.02 | d |
Age t (Gyr) | 7 ± 4 | d |
L* (L⊙) | 0.55 ± 0.02 | e |
R* (R⊙) | 0.86 ± 0.02 | e |
M* (M⊙) | 0.87 − 0.89 | f |
Adopted averaged parameters | ||
M* (M⊙) | 0.88 ± 0.03 | |
R* (R⊙) | 0.85 ± 0.02 | |
ρ* (g cm−3) | 2.02 ± 0.16 |
Parameter . | Value . | Source . |
---|---|---|
Designations and coordinates | ||
EPIC ID | 211682544 | EPIC |
K2 ID | 263 | |
2-MASS ID | J08384378+1540503 | |
RA (J2000) | 08:38:43.78 | 2MASS |
Dec. (J2000) | 15:40:50.4 | 2MASS |
Magnitudes and parallax | ||
B | 12.35 ± 0.03 | APASS |
V | 11.61 ± 0.04 | APASS |
Kepler magnitude | 11.41 | EPIC |
J | 10.22 ± 0.02 | 2MASS |
H | 9.81 ± 0.02 | 2MASS |
K | 9.75 ± 0.02 | 2MASS |
Parallax π | 6.1262 ± 0.0514 | Gaia DR2 |
Distance d (pc) | 163.2 ± 1.4 | a |
Atmospheric parameters: effective temperature Teff, | ||
surface gravity log g, metallicity |$[\rm {Fe/H}]$|, projected | ||
rotational velocity vsin i, microturbulence ξt | ||
Teff (K) | 5372 ± 73 | b |
log g (cgs) | 4.58 ± 0.13 | b |
|$[\rm {Fe/H}]$| (dex) | −0.08 ± 0.05 | b |
ξt (km s−1) | 0.76 ± 0.08 | b |
Teff (K) | 5365 ± 50 | c |
log g [cgs] | 4.45 ± 0.10 | c |
|$[\rm {m/H}]$| (dex) | −0.07 ± 0.08 | c |
vsin i (km s−1) | <2.0 | c |
Adopted averaged parameters | ||
Teff (K) | 5368 ± 44 | |
log g (cgs) | 4.51 ± 0.08 | |
|$[\rm {m/H}]$| (dex) | −0.08 ± 0.05 | |
Mass, radius, age, luminosity | ||
M* (M⊙) | 0.86 ± 0.03 | d |
R* (R⊙) | 0.84 ± 0.02 | d |
Age t (Gyr) | 7 ± 4 | d |
L* (L⊙) | 0.55 ± 0.02 | e |
R* (R⊙) | 0.86 ± 0.02 | e |
M* (M⊙) | 0.87 − 0.89 | f |
Adopted averaged parameters | ||
M* (M⊙) | 0.88 ± 0.03 | |
R* (R⊙) | 0.85 ± 0.02 | |
ρ* (g cm−3) | 2.02 ± 0.16 |
aUsing the Gaia DR2 parallax.
bARES+MOOG (Sousa 2014), with the surface gravity corrected following (Mortier et al. 2014).
cSPC (Buchhave et al. 2012, 2014).
dUsing PARSEC isochrones (da Silva et al. 2006; Bressan et al. 2012).
eUsing distance, apparent magnitude, and bolometric correction.
fRelations of Moya et al. (2018).
Parameter . | Value . | Source . |
---|---|---|
Designations and coordinates | ||
EPIC ID | 211682544 | EPIC |
K2 ID | 263 | |
2-MASS ID | J08384378+1540503 | |
RA (J2000) | 08:38:43.78 | 2MASS |
Dec. (J2000) | 15:40:50.4 | 2MASS |
Magnitudes and parallax | ||
B | 12.35 ± 0.03 | APASS |
V | 11.61 ± 0.04 | APASS |
Kepler magnitude | 11.41 | EPIC |
J | 10.22 ± 0.02 | 2MASS |
H | 9.81 ± 0.02 | 2MASS |
K | 9.75 ± 0.02 | 2MASS |
Parallax π | 6.1262 ± 0.0514 | Gaia DR2 |
Distance d (pc) | 163.2 ± 1.4 | a |
Atmospheric parameters: effective temperature Teff, | ||
surface gravity log g, metallicity |$[\rm {Fe/H}]$|, projected | ||
rotational velocity vsin i, microturbulence ξt | ||
Teff (K) | 5372 ± 73 | b |
log g (cgs) | 4.58 ± 0.13 | b |
|$[\rm {Fe/H}]$| (dex) | −0.08 ± 0.05 | b |
ξt (km s−1) | 0.76 ± 0.08 | b |
Teff (K) | 5365 ± 50 | c |
log g [cgs] | 4.45 ± 0.10 | c |
|$[\rm {m/H}]$| (dex) | −0.07 ± 0.08 | c |
vsin i (km s−1) | <2.0 | c |
Adopted averaged parameters | ||
Teff (K) | 5368 ± 44 | |
log g (cgs) | 4.51 ± 0.08 | |
|$[\rm {m/H}]$| (dex) | −0.08 ± 0.05 | |
Mass, radius, age, luminosity | ||
M* (M⊙) | 0.86 ± 0.03 | d |
R* (R⊙) | 0.84 ± 0.02 | d |
Age t (Gyr) | 7 ± 4 | d |
L* (L⊙) | 0.55 ± 0.02 | e |
R* (R⊙) | 0.86 ± 0.02 | e |
M* (M⊙) | 0.87 − 0.89 | f |
Adopted averaged parameters | ||
M* (M⊙) | 0.88 ± 0.03 | |
R* (R⊙) | 0.85 ± 0.02 | |
ρ* (g cm−3) | 2.02 ± 0.16 |
Parameter . | Value . | Source . |
---|---|---|
Designations and coordinates | ||
EPIC ID | 211682544 | EPIC |
K2 ID | 263 | |
2-MASS ID | J08384378+1540503 | |
RA (J2000) | 08:38:43.78 | 2MASS |
Dec. (J2000) | 15:40:50.4 | 2MASS |
Magnitudes and parallax | ||
B | 12.35 ± 0.03 | APASS |
V | 11.61 ± 0.04 | APASS |
Kepler magnitude | 11.41 | EPIC |
J | 10.22 ± 0.02 | 2MASS |
H | 9.81 ± 0.02 | 2MASS |
K | 9.75 ± 0.02 | 2MASS |
Parallax π | 6.1262 ± 0.0514 | Gaia DR2 |
Distance d (pc) | 163.2 ± 1.4 | a |
Atmospheric parameters: effective temperature Teff, | ||
surface gravity log g, metallicity |$[\rm {Fe/H}]$|, projected | ||
rotational velocity vsin i, microturbulence ξt | ||
Teff (K) | 5372 ± 73 | b |
log g (cgs) | 4.58 ± 0.13 | b |
|$[\rm {Fe/H}]$| (dex) | −0.08 ± 0.05 | b |
ξt (km s−1) | 0.76 ± 0.08 | b |
Teff (K) | 5365 ± 50 | c |
log g [cgs] | 4.45 ± 0.10 | c |
|$[\rm {m/H}]$| (dex) | −0.07 ± 0.08 | c |
vsin i (km s−1) | <2.0 | c |
Adopted averaged parameters | ||
Teff (K) | 5368 ± 44 | |
log g (cgs) | 4.51 ± 0.08 | |
|$[\rm {m/H}]$| (dex) | −0.08 ± 0.05 | |
Mass, radius, age, luminosity | ||
M* (M⊙) | 0.86 ± 0.03 | d |
R* (R⊙) | 0.84 ± 0.02 | d |
Age t (Gyr) | 7 ± 4 | d |
L* (L⊙) | 0.55 ± 0.02 | e |
R* (R⊙) | 0.86 ± 0.02 | e |
M* (M⊙) | 0.87 − 0.89 | f |
Adopted averaged parameters | ||
M* (M⊙) | 0.88 ± 0.03 | |
R* (R⊙) | 0.85 ± 0.02 | |
ρ* (g cm−3) | 2.02 ± 0.16 |
aUsing the Gaia DR2 parallax.
bARES+MOOG (Sousa 2014), with the surface gravity corrected following (Mortier et al. 2014).
cSPC (Buchhave et al. 2012, 2014).
dUsing PARSEC isochrones (da Silva et al. 2006; Bressan et al. 2012).
eUsing distance, apparent magnitude, and bolometric correction.
fRelations of Moya et al. (2018).
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