All names: WD 0810+234, SDSS J081342.22+232024.0, LAMOST J081342.25+232023.3, GD 295, EGGR 347, LAMOST J081342.13+232023.9, Gaia DR2 677560232299128192, SDSS J081342.22+232023.9, Gaia EDR3 677560232299128192, TIC 82289574, GALEX J081342.2+232024, [BGK2006] J081342.22+232024.0, WDJ081342.20+232024.24, J0813+2320, WD 0810+23, 2MASS J08134220+2320242, Gaia DR3 677560232299128192, SDSS J081342.26+232023.4
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Kilic et al. 2025 | Kilic et al. 2020 | MWDD H | Gaia DR2 | Stilism | Guo et al. 2015 | Gianninas et al. 2011 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) | Vincent et al. 2023 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 08 13 42.30 (0.04) | 08 13 42.22 | 08 13 42.30 (0.07) | 08 13 42.30 | 08 13 42.20 (0.04) | 08 13 42.30 | 08 13 42.00 | |||||||||
| Declination | 23 20 23.02 (0.03) | 23 20 23.95 | 23 20 23.05 (0.05) | 23 20 23.02 | 23 20 24.24 (0.03) | 23 20 23.05 | 23 20 35.52 | |||||||||
| Spectral type | DA | DA | DA | DA | DA | DA | DA3.1 | DA3 | DA | |||||||
| Effective temperature | [K] | 15904.0 (174) | 15904.0 (174) | 15132.0 | 16360.0 (264) | 15828.0 (254) | ||||||||||
| log(g) | [cgs] | 8.01 (0.01) | 8.01 (0.01) | 7.95 | 8.03 (0.05) | 8.00 (0.01) | ||||||||||
| Mass | [M☉] | 0.618 (0.008) | 0.618 (0.01) | 0.586 | 0.63 (0.03) | 0.616 (0.01) | ||||||||||
| log(Luminosity) | [L☉] | |||||||||||||||
| Cooling age | [Gyr] | 0.1777 | ||||||||||||||
| 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] | 10.57 (0.05) | 10.57 (0.09) | 10.57 | 10.57 (0.05) | 10.57 (0.09) | ||||||||||
| Distance | [pc] | 94.59 (0.5) | 94.58 (0.8) | 94.00 | 94.59 | 94.59 (0.5) | 94.58 (0.8) | |||||||||
| Composition | H | H | H | |||||||||||||
| Proper motion (right ascension) | [mas/yr] | 82.43846846 (0.05) | 82.45391613 (0.1) | 82.438 (0.05) | 82.45391613 | |||||||||||
| Proper motion (declination) | [mas/yr] | -76.25121679 (0.04) | -76.24198149 (0.09) | -76.251 (0.04) | -76.24198149 | |||||||||||
| Variability | ||||||||||||||||
| Magnetic | ||||||||||||||||
| Bd | [MG] | |||||||||||||||
| Infrared excess (disk) | ||||||||||||||||
| Binarity | ||||||||||||||||
| B magnitude | 15.00 | |||||||||||||||
| V magnitude | ||||||||||||||||
| R magnitude | ||||||||||||||||
| I magnitude | ||||||||||||||||
| J magnitude | 16.46 (0.007) | |||||||||||||||
| H magnitude | 16.48 (0.02) | |||||||||||||||
| K magnitude | 16.46 (0.03) | |||||||||||||||
| u magnitude | 16.17 (0.005) | 16.17 (0.005) | 16.17 (0.005) | |||||||||||||
| g magnitude | 15.92 (0.003) | 15.92 (0.003) | 15.92 (0.003) | |||||||||||||
| r magnitude | 16.24 (0.004) | 16.24 (0.004) | 16.24 (0.004) | |||||||||||||
| i magnitude | 16.50 (0.004) | 16.50 (0.004) | 16.50 (0.004) | |||||||||||||
| z magnitude | 16.81 (0.01) | 16.81 (0.01) | 16.81 (0.01) | |||||||||||||
| G magnitude | 16.09 (0.004) | 16.11 | 16.09 | 16.09 (0.003) | 16.11 | |||||||||||
| BP magnitude | 16.05 (0.004) | 16.02 | 16.02 | |||||||||||||
| RP magnitude | 16.22 (0.005) | 16.22 | 16.22 | |||||||||||||
| Pan g magnitude | 15.97 (0.004) | |||||||||||||||
| Pan r magnitude | 16.26 (0.002) | |||||||||||||||
| Pan i magnitude | 16.53 (0.004) | |||||||||||||||
| Pan z magnitude | 16.77 (0.004) | |||||||||||||||
| Pan y magnitude | 16.93 (0.01) | |||||||||||||||
| E(B-V) | 0.003 | |||||||||||||||
* 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.