All names: PHL 3104, USNO-B1.0 0652-00010142, GD 661, TIC 63794724, WD 0052-250, Gaia DR3 2345431719942784768, WDJ005435.53-244353.05, 2MASS J00543551-2443531, Gaia DR2 2345431719942784768, Gaia EDR3 2345431719942784768
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Gaia DR2 | Stilism | Gianninas et al. 2011 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) |
|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 00 54 35.51 (0.05) | 00 54 35.51 (0.07) | 00 54 35.51 | 00 54 35.53 (0.05) | 00 54 35.51 | 00 54 35.62 | ||||
| Declination | -24 43 54.52 (0.04) | -24 43 54.47 (0.05) | -24 43 54.52 | -24 43 53.05 (0.04) | -24 43 54.47 | -24 43 50.52 | ||||
| Spectral type | DA | DA | DA3.7 | DA5 | ||||||
| Effective temperature | [K] | 13760.0 (413) | 13783.0 (190) | |||||||
| log(g) | [cgs] | 8.00 (0.06) | 8.10 (0.01) | |||||||
| Mass | [M☉] | 0.61 (0.03) | 0.667 (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] | 10.41 (0.06) | 10.39 (0.08) | 10.41 | 10.41 (0.06) | 10.39 (0.08) | ||||
| Distance | [pc] | 96.10 (0.6) | 96.22 (0.7) | 105.00 | 96.10 | 96.10 (0.6) | 96.22 (0.7) | |||
| Composition | H | |||||||||
| Proper motion (right ascension) | [mas/yr] | -12.5248807 (0.06) | -12.58226727 (0.1) | -12.525 (0.06) | -12.58226727 | |||||
| Proper motion (declination) | [mas/yr] | -91.44402889 (0.06) | -91.34503843 (0.09) | -91.444 (0.06) | -91.34503843 | |||||
| Variability | ||||||||||
| Magnetic | ||||||||||
| Bd | [MG] | |||||||||
| Infrared excess (disk) | ||||||||||
| Binarity | ||||||||||
| B magnitude | 16.00 | |||||||||
| V magnitude | ||||||||||
| R magnitude | 16.30 | |||||||||
| I magnitude | ||||||||||
| J magnitude | 16.51 (0.1) | |||||||||
| H magnitude | ||||||||||
| K magnitude | ||||||||||
| u magnitude | ||||||||||
| g magnitude | ||||||||||
| r magnitude | ||||||||||
| i magnitude | ||||||||||
| z magnitude | ||||||||||
| G magnitude | 16.53 (0.003) | 16.56 | 16.53 | 16.53 (0.003) | 16.56 | |||||
| BP magnitude | 16.53 (0.003) | 16.53 | 16.53 | |||||||
| RP magnitude | 16.59 (0.005) | 16.60 | 16.60 | |||||||
| Pan g magnitude | 16.46 (0.02) | |||||||||
| Pan r magnitude | 16.67 (0.005) | |||||||||
| Pan i magnitude | 16.90 (0.004) | |||||||||
| Pan z magnitude | 17.12 (0.007) | |||||||||
| Pan y magnitude | 17.28 (0.01) | |||||||||
| E(B-V) | 0.001 | |||||||||
* 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.