LAMOST J123001.23+025557.6

All names: SDSS J123001.22+025557.5, GALEX J123001.2+025558, Gaia DR2 3700737821613236352, LAMOST J123001.23+025557.6, SDSS J123001.23+025557.6, SDSS J123001.24+025557.6, SDSS J123001.24+025557.65, Gaia EDR3 3700737821613236352, Gaia DR3 3700737821613236352

Parameter Unit Gaia EDR3 Pan-STARRS DR1 SDSS DR10 MWDD H Gaia DR2 Stilism Guo et al. 2015 Kepler et al. 2015 Vincent et al. 2024 Simbad Vincent et al. 2023
Right ascension 12 30 01.24 (0.08) 12 30 01.22 12 30 01.24 (0.1) 12 30 01.24 12 30 01.23 (0.08)
Declination 02 55 57.76 (0.06) 02 55 57.54 02 55 57.76 (0.08) 02 55 57.76 02 55 57.57 (0.06)
Spectral type DA DA DA DA DA DA
Effective temperature [K] 17105.0 19983.0 (76) 17028.0 (467)
log(g) [cgs] 7.81 8.02 (0.01) 7.86 (0.03)
Mass [M] 0.517 0.633 (0.005) 0.538 (0.03)
log(Luminosity) [L]
Cooling age [Gyr] 0.0895
log(H/He)
log(C/He)
log(Ca/He)
log(Ca/H)
log(C/H)
log(N/H)
log(O/H)
log(Na/H)
log(Mg/H)
log(Al/H)
log(Si/H)
log(P/H)
log(S/H)
log(Sc/H)
log(Ti/H)
log(Cr/H)
log(Mn/H)
log(Fe/H)
log(Ni/H)
Parallax [mas] 5.20 (0.1) 5.01 (0.1) 5.20 5.20 (0.1)
Distance [pc] 192.36 (4) 199.73 (6) 192.36 192.36 (4)
Composition H
Proper motion (right ascension) [mas/yr] 14.52927825 (0.1) 15.01634652 (0.3) 14.529 (0.1)
Proper motion (declination) [mas/yr] 12.27794805 (0.08) 12.0201627 (0.2) 12.278 (0.08)
Variability
Magnetic
Bd [MG]
Infrared excess (disk)
Binarity
B magnitude
V magnitude
R magnitude
I magnitude
J magnitude
H magnitude 17.71 (0.07)
K magnitude 17.80 (0.1)
u magnitude 17.26 (0.009) 17.27 (0.02) 17.26 (0.009)
g magnitude 17.11 (0.004) 17.13 (0.02) 17.11 (0.004)
r magnitude 17.46 (0.005) 17.46 (0.02) 17.46 (0.005)
i magnitude 17.75 (0.008) 17.75 (0.02) 17.75 (0.008)
z magnitude 18.01 (0.02) 17.99 (0.03) 18.01 (0.03)
G magnitude 17.30 (0.005) 17.32 17.30 17.30 (0.003)
BP magnitude 17.23 (0.005) 17.20
RP magnitude 17.45 (0.009) 17.43
Pan g magnitude 17.15 (0.003)
Pan r magnitude 17.47 (0.003)
Pan i magnitude 17.77 (0.003)
Pan z magnitude 18.03 (0.006)
Pan y magnitude 18.18 (0.01)
E(B-V) 0.018

* Constant surface field

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The Montreal White Dwarf Database is produced and maintained by Prof. Patrick Dufour (Université de Montréal) and Dr. Simon Blouin (University of Victoria). Please send database updates, corrections, suggestions or bug reports to patrick.dufour@umontreal.ca.