All names: Gaia DR3 2792315366213367296, WDJ002128.60+150223.91, SDSS J002128.59+150223.8, SDSS J002128.59+150223.7, Gaia EDR3 2792315366213367296, SDSS J002128.60+150223.8, WIRED J002128.59+150223.7, J0021+1502, SDSS J002129.00+150223.7, Gaia DR2 2792315366213367296, WD 0018+147, SDSS J002128.60+150223.7
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Kilic et al. 2025 | Caron et al. 2023 | MWDD H | Gaia DR2 | Stilism | Ferrario et al. 2015 | Kulebi et al. 2009 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | Eisenstein et al. 2006 | White Dwarf Catalog (McCook & Sion 1999) | Kleinman et al. 2013 | Vincent et al. 2023 |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 00 21 28.62 (0.1) | 00 21 28.60 | 00 21 28.61 (0.2) | 00 21 29.00 | 00 21 28.62 | 00 21 28.60 (0.1) | 00 21 28.61 | 00 21 28.60 | 00 21 28.32 | 00 21 28.60 | ||||||||
Declination | 15 02 22.62 (0.09) | 15 02 23.80 | 15 02 22.66 (0.1) | 15 02 23.71 | 15 02 22.62 | 15 02 23.91 (0.09) | 15 02 22.66 | 15 02 23.81 | 15 02 20.40 | 15 02 23.75 | ||||||||
Spectral type | DAH | DAP | DA | DA | DAH | DC | DAP | DC | DC | DC | DCM | DC | ||||||
Effective temperature | [K] | 7119.0 (38) | 7352.0 (41) | 7093.0 | 7000.0 | 6499.0 (140) | 10080.0 (2) | 6301.0 (6) | ||||||||||
log(g) | [cgs] | 8.25 (0.01) | 8.34 (0.02) | 8.24 | 8.00 (0) | 8.03 (0.04) | 8.72 (0.2) | 10.00 (0.003) | ||||||||||
Mass | [M☉] | 0.747 (0.01) | 0.808 (0.02) | 0.742 | 0.59 (0.03) | |||||||||||||
log(Luminosity) | [L☉] | |||||||||||||||||
Cooling age | [Gyr] | 2.7400 | 2.2830 | |||||||||||||||
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] | 14.20 (0.1) | 14.20 (0.2) | 14.20 (0.2) | 14.20 | 14.20 (0.1) | 14.20 (0.2) | |||||||||||
Distance | [pc] | 70.42 (0.7) | 70.42 (1) | 70.42 (1) | 70.42 | 70.42 (0.7) | 70.42 (1) | |||||||||||
Composition | H | H | H | H | ||||||||||||||
Proper motion (right ascension) | [mas/yr] | 16.4647106 (0.2) | 16.37110147 (0.4) | 16.465 (0.2) | 16.371 | 15.4 | ||||||||||||
Proper motion (declination) | [mas/yr] | -80.24052107 (0.1) | -80.41859274 (0.2) | -80.241 (0.1) | -80.419 | -81.7 | ||||||||||||
Variability | ||||||||||||||||||
Magnetic | yes | yes | ||||||||||||||||
Bd | [MG] | 530.69 (64) | 530.69 (64) | |||||||||||||||
Infrared excess (disk) | ||||||||||||||||||
Binarity | ||||||||||||||||||
B magnitude | ||||||||||||||||||
V magnitude | ||||||||||||||||||
R magnitude | ||||||||||||||||||
I magnitude | ||||||||||||||||||
J magnitude | 17.50 (0.04) | 17.50 (0.04) | ||||||||||||||||
H magnitude | 17.56 (0.08) | 17.56 (0.08) | ||||||||||||||||
K magnitude | 17.28 (0.1) | 17.30 (0.1) | ||||||||||||||||
u magnitude | 18.71 (0.02) | 18.69 (0.02) | 18.67 (0.02) | 18.71 (0.02) | 18.69 (0.02) | 18.68 | 18.67 (0.02) | |||||||||||
g magnitude | 18.16 (0.007) | 18.17 (0.02) | 18.16 (0.007) | 18.18 (0.01) | 18.17 | 18.17 (0.01) | ||||||||||||
r magnitude | 17.95 (0.007) | 17.96 (0.02) | 17.95 (0.007) | 17.97 (0.01) | 17.97 | 17.96 (0.01) | ||||||||||||
i magnitude | 17.93 (0.008) | 17.93 (0.02) | 17.93 (0.008) | 17.93 (0.02) | 17.93 | 17.92 (0.02) | ||||||||||||
z magnitude | 17.97 (0.02) | 18.00 (0.03) | 17.97 (0.02) | 17.99 (0.03) | 17.99 | 17.98 (0.03) | ||||||||||||
G magnitude | 17.96 (0.01) | 17.99 | 17.96 | 17.96 (0.003) | 17.99 | |||||||||||||
BP magnitude | 18.20 (0.01) | 18.17 | 18.17 | |||||||||||||||
RP magnitude | 17.66 (0.01) | 17.65 | 17.65 | |||||||||||||||
Pan g magnitude | 18.15 (0.004) | 18.15 (0.004) | ||||||||||||||||
Pan r magnitude | 17.97 (0.005) | 17.97 (0.005) | ||||||||||||||||
Pan i magnitude | 17.98 (0.004) | 17.98 (0.003) | ||||||||||||||||
Pan z magnitude | 18.01 (0.009) | 18.01 (0.008) | ||||||||||||||||
Pan y magnitude | 18.06 (0.01) | 18.06 (0.01) | ||||||||||||||||
E(B-V) | 0.004 |
* 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.