All names: Gaia DR3 3974868644764927744, AAVSO 1142+19, EUVE J1148+18.5, SDSS J114803.16+183046.8, J1148+1830, RE J1148+18, 1RXS J114804.5+183042, WDJ114803.16+183046.47, RX J1148.0+1830, TIC 87480677, [ZEH2003] RX J1148.0+1830 2, PG 1145+188, FAUST 2933, WD 1145+187, 1SWASP J114803.16+183046.6, Gaia EDR3 3974868644764927744, HS 1145+1847, 2MASS J11480316+1830464, GALEX J114803.1+183046, 2EUVE J1147+18.5, 2RE J114802+183059, USNO-B1.0 1085-00197676, Gaia DR2 3974868644764927744, RE J114802+183028, [BAE2000] 73, SDSS J114803.17+183046.9, EUVE J1147+18.5, RE J1148+183, 2RE J1148+183
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Kilic et al. 2025 | Kilic et al. 2020 | MWDD H | Gaia DR2 | Stilism | Gianninas et al. 2011 | Koester et al. 2009 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 11 48 03.18 (0.04) | 11 48 03.18 (0.05) | 11 48 03.18 | 11 48 03.16 (0.04) | 11 48 03.18 | 11 48 04.06 | ||||||||
| Declination | 18 30 47.56 (0.03) | 18 30 47.53 (0.05) | 18 30 47.56 | 18 30 46.47 (0.03) | 18 30 47.53 | 18 31 01.56 | ||||||||
| Spectral type | DA | DA | DA | DA | DA | DA1.8 | DA2 | |||||||
| Effective temperature | [K] | 27019.0 (381) | 27019.0 (380) | 25842.0 | 27390.0 (405) | 27167.0 (27) | 30226.0 (483) | |||||||
| log(g) | [cgs] | 7.92 (0.01) | 7.92 (0.01) | 7.86 | 7.87 (0.05) | 7.80 (0.004) | 8.06 (0.02) | |||||||
| Mass | [M☉] | 0.595 (0.01) | 0.595 (0.01) | 0.563 | 0.57 (0.02) | 0.681 (0.01) | ||||||||
| log(Luminosity) | [L☉] | |||||||||||||
| Cooling age | [Gyr] | 0.0153 | ||||||||||||
| 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] | 14.54 (0.04) | 14.55 (0.07) | 14.54 | 14.54 (0.04) | 14.55 (0.07) | ||||||||
| Distance | [pc] | 68.76 (0.2) | 68.73 (0.3) | 71.00 | 68.76 | 68.76 (0.2) | 68.73 (0.3) | |||||||
| Composition | H | H | H | |||||||||||
| Proper motion (right ascension) | [mas/yr] | 17.39125707 (0.05) | 17.45393059 (0.1) | 17.391 (0.04) | 17.45393059 | |||||||||
| Proper motion (declination) | [mas/yr] | 68.60883858 (0.03) | 68.65599061 (0.08) | 68.609 (0.03) | 68.65599061 | |||||||||
| Variability | ||||||||||||||
| Magnetic | ||||||||||||||
| Bd | [MG] | |||||||||||||
| Infrared excess (disk) | ||||||||||||||
| Binarity | ||||||||||||||
| B magnitude | 13.69 | |||||||||||||
| V magnitude | 14.22 | 14.38 | ||||||||||||
| R magnitude | 14.60 | |||||||||||||
| I magnitude | ||||||||||||||
| J magnitude | 14.88 (0.03) | |||||||||||||
| H magnitude | 14.94 (0.07) | |||||||||||||
| K magnitude | 15.11 (0.1) | |||||||||||||
| u magnitude | 13.85 (0.004) | 13.85 (0.004) | 13.89 | |||||||||||
| g magnitude | 15.80 (0.01) | 15.80 (0.01) | 14.01 | |||||||||||
| r magnitude | 14.46 (0.003) | 14.46 (0.003) | 14.46 | |||||||||||
| i magnitude | 14.79 (0.003) | 14.79 (0.003) | 14.79 | |||||||||||
| z magnitude | 15.11 (0.005) | 15.11 (0.005) | 15.08 | |||||||||||
| G magnitude | 14.25 (0.001) | 14.26 | 14.25 | 14.25 (0.003) | 14.26 | |||||||||
| BP magnitude | 14.12 (0.001) | 14.07 | 14.07 | |||||||||||
| RP magnitude | 14.50 (0.002) | 14.50 | 14.50 | |||||||||||
| Pan g magnitude | 14.08 (0.003) | |||||||||||||
| Pan r magnitude | 14.48 (0.002) | |||||||||||||
| Pan i magnitude | 14.84 (0.002) | |||||||||||||
| Pan z magnitude | 15.11 (0.003) | |||||||||||||
| Pan y magnitude | 15.30 (0.004) | |||||||||||||
| E(B-V) | 0.002 | |||||||||||||
* 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.