All names: Gaia DR3 623384098941292672, Gaia DR2 623384098941292672, SDSS J101053.50+181148.4, GALEX J101053.5+181149, TIC 27108889, SDSS J101053.51+181148.4, J1010+1811, WDJ101053.54+181148.24, SDSS J101053.51+181148.3, Gaia EDR3 623384098941292672, 2MASS J10105355+1811480
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Kilic et al. 2025 | Kilic et al. 2020 | Gaia DR2 | Stilism | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 |
|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 10 10 53.45 (0.05) | 10 10 53.45 | 10 10 53.45 | 10 10 53.54 (0.05) | 10 10 53.45 | |||||
| Declination | 18 11 48.81 (0.04) | 18 11 48.79 | 18 11 48.81 | 18 11 48.24 (0.04) | 18 11 48.79 | |||||
| Spectral type | DA | DA | DA | DA | ||||||
| Effective temperature | [K] | 12255.0 (87) | 12239.0 (88) | 12045.0 (167) | ||||||
| log(g) | [cgs] | 7.93 (0.007) | 7.95 (0.01) | 7.92 (0.01) | ||||||
| Mass | [M☉] | 0.566 (0.005) | 0.577 (0.01) | 0.56 (0.01) | ||||||
| log(Luminosity) | [L☉] | |||||||||
| Cooling age | [Gyr] | |||||||||
| 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] | 10.85 (0.06) | 10.99 (0.1) | 10.85 | 10.85 (0.06) | 10.99 (0.1) | ||||
| Distance | [pc] | 92.14 (0.5) | 91.01 (1) | 92.14 | 92.14 (0.5) | 91.01 (1) | ||||
| Composition | H | |||||||||
| Proper motion (right ascension) | [mas/yr] | -78.47899846 (0.05) | -78.35167042 (0.2) | -78.479 (0.05) | -78.35167042 | |||||
| Proper motion (declination) | [mas/yr] | 35.458746 (0.04) | 35.43455287 (0.2) | 35.459 (0.04) | 35.43455287 | |||||
| Variability | ||||||||||
| Magnetic | ||||||||||
| Bd | [MG] | |||||||||
| Infrared excess (disk) | ||||||||||
| Binarity | ||||||||||
| B magnitude | ||||||||||
| V magnitude | ||||||||||
| R magnitude | ||||||||||
| I magnitude | ||||||||||
| J magnitude | 16.62 (0.1) | |||||||||
| H magnitude | ||||||||||
| K magnitude | ||||||||||
| u magnitude | 16.72 (0.006) | 16.74 (0.008) | ||||||||
| g magnitude | 16.27 (0.004) | 16.29 (0.004) | ||||||||
| r magnitude | 16.49 (0.004) | 16.51 (0.004) | ||||||||
| i magnitude | 16.68 (0.005) | 16.71 (0.005) | ||||||||
| z magnitude | 16.96 (0.01) | 16.93 (0.01) | ||||||||
| G magnitude | 16.39 (0.003) | 16.41 | 16.39 | 16.39 (0.003) | 16.41 | |||||
| BP magnitude | 16.40 (0.003) | 16.39 | 16.39 | |||||||
| RP magnitude | 16.42 (0.005) | 16.43 | 16.43 | |||||||
| Pan g magnitude | 16.30 (0.003) | |||||||||
| Pan r magnitude | 16.50 (0.006) | |||||||||
| Pan i magnitude | 16.73 (0.006) | |||||||||
| Pan z magnitude | 16.95 (0.003) | |||||||||
| Pan y magnitude | 17.08 (0.007) | |||||||||
| 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.