All names: Gaia DR2 1391723889583920512, SDSS J151053.70+393932.1, SDSS J151053.71+393932.1, Gaia EDR3 1391723889583920512, SDSS J151053.71+393932.11, SDSS J151053.72+393932.0, Gaia DR3 1391723889583920512, [BGK2006] J151053.72+393932.0, SDSS J151053.72+393931.9, GALEX J151053.7+393932
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR10 | MWDD H | Gaia DR2 | Stilism | Kepler et al. 2015 | Vincent et al. 2024 | Simbad | Vincent et al. 2023 |
---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 15 10 53.70 (0.04) | 15 10 53.72 | 15 10 53.70 (0.06) | 15 10 53.70 | 15 10 53.73 (0.04) | ||||||
Declination | 39 39 32.20 (0.06) | 39 39 31.96 | 39 39 32.19 (0.08) | 39 39 32.20 | 39 39 31.92 (0.06) | ||||||
Spectral type | DA | DA | DA | DA | DA | ||||||
Effective temperature | [K] | 15839.0 | 18791.0 (81) | 17594.0 (435) | |||||||
log(g) | [cgs] | 7.92 | 8.10 (0.01) | 8.00 (0.03) | |||||||
Mass | [M☉] | 0.57 | 0.6729999999999999 (0.005) | 0.619 (0.02) | |||||||
log(Luminosity) | [L☉] | ||||||||||
Cooling age | [Gyr] | 0.1445 | |||||||||
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] | 5.82 (0.07) | 5.95 (0.09) | 5.82 | 5.82 (0.07) | ||||||
Distance | [pc] | 171.74 (2) | 168.11 (2) | 171.74 | 171.74 (2) | ||||||
Composition | H | ||||||||||
Proper motion (right ascension) | [mas/yr] | -22.35468352 (0.06) | -22.40721266 (0.1) | -22.355 (0.06) | |||||||
Proper motion (declination) | [mas/yr] | 17.39275989 (0.08) | 17.47753594 (0.2) | 17.393 (0.08) | |||||||
Variability | |||||||||||
Magnetic | |||||||||||
Bd | [MG] | ||||||||||
Infrared excess (disk) | |||||||||||
Binarity | |||||||||||
B magnitude | |||||||||||
V magnitude | |||||||||||
R magnitude | |||||||||||
I magnitude | |||||||||||
J magnitude | |||||||||||
H magnitude | |||||||||||
K magnitude | |||||||||||
u magnitude | 17.22 (0.008) | 17.21 (0.2) | 17.22 (0.008) | ||||||||
g magnitude | 17.04 (0.005) | 17.06 (0.05) | 17.04 (0.005) | ||||||||
r magnitude | 17.38 (0.006) | 17.39 (0.05) | 17.38 (0.006) | ||||||||
i magnitude | 17.63 (0.007) | 17.67 (0.3) | 17.63 (0.007) | ||||||||
z magnitude | 17.82 (0.02) | 17.85 (0.7) | 17.82 (0.02) | ||||||||
G magnitude | 17.22 (0.005) | 17.24 | 17.22 | 17.22 (0.003) | |||||||
BP magnitude | 17.17 (0.005) | 17.13 | |||||||||
RP magnitude | 17.36 (0.02) | 17.36 | |||||||||
Pan g magnitude | 17.08 (0.003) | ||||||||||
Pan r magnitude | 17.38 (0.007) | ||||||||||
Pan i magnitude | 17.67 (0.007) | ||||||||||
Pan z magnitude | 17.92 (0.01) | ||||||||||
Pan y magnitude | 18.05 (0.01) | ||||||||||
E(B-V) | 0.020 |
* Constant surface field
Spectra without link are available upon request
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.