All names: SDSS J143358.20+190737.4, Gaia EDR3 1239213243034520192, LSPM J1433+1907, 14339+1907, WD 1431+193, J1433+1907, LP 440-41, SDSS J143358.19+190737.3, WDJ143358.25+190738.16, Gaia DR2 1239213243034520192, 2MASS J14335820+1907382, NLTT 37753, PSO J218.4921+19.1266, USNO-B1.0 1091-00226688, Gaia DR3 1239213243034520192, TIC 257959972, PM J14339+1907
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Kilic et al. 2025 | Caron et al. 2023 | Kilic et al. 2020 | Blouin et al. 2019 | MWDD H | Gaia DR2 | Stilism | Limoges et al. 2015 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 14 33 58.09 (0.09) | 14 33 58.10 (0.2) | 14 33 58.09 | 14 33 58.25 (0.09) | 14 33 58.10 | 14 33 58.34 | |||||||||
| Declination | 19 07 35.56 (0.1) | 19 07 35.64 (0.2) | 19 07 35.56 | 19 07 38.15 (0.1) | 19 07 35.64 | 19 07 34.68 | |||||||||
| Spectral type | DA | DA | DA | DA | DA | DA | DC: | DA | DC | ||||||
| Effective temperature | [K] | 5025.0 (30) | 5049.0 (29) | 5023.0 (30) | 5080.0 (35) | 5125.0 | 5020.0 (62) | 5136.0 (49) | |||||||
| log(g) | [cgs] | 7.90 (0.02) | 7.90 (0.02) | 7.87 (0.02) | 7.91 (0.03) | 7.94 | 8.00 (0) | 7.96 (0.03) | |||||||
| Mass | [M☉] | 0.519 (0.01) | 0.521 (0.02) | 0.504 (0.02) | 0.525 (0.02) | 0.543 | 0.58 (0.1) | 0.556 (0.02) | |||||||
| log(Luminosity) | [L☉] | -4.04 | |||||||||||||
| Cooling age | [Gyr] | 4.2100 | 4.1160 (0.4) | 4.2300 | |||||||||||
| 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] | 20.52 (0.1) | 20.24 (0.2) | 20.24 (0.2) | 20.24 (0.2) | 20.52 | 20.52 (0.1) | 20.24 (0.2) | |||||||
| Distance | [pc] | 48.73 (0.3) | 49.41 (0.5) | 49.42 (0.5) | 49.42 (0.5) | 45.80 (5) | 48.73 | 48.73 (0.3) | 49.42 (0.5) | ||||||
| Composition | H | H | H | H | H | ||||||||||
| Proper motion (right ascension) | [mas/yr] | -140.5185467 (0.1) | -139.963265 (0.3) | -140.519 (0.1) | -139.963265 | ||||||||||
| Proper motion (declination) | [mas/yr] | -162.0391886 (0.1) | -162.4221649 (0.4) | -162.039 (0.1) | -162.4221649 | ||||||||||
| Variability | |||||||||||||||
| Magnetic | |||||||||||||||
| Bd | [MG] | ||||||||||||||
| Infrared excess (disk) | |||||||||||||||
| Binarity | |||||||||||||||
| B magnitude | 19.10 | ||||||||||||||
| V magnitude | |||||||||||||||
| R magnitude | 18.10 | ||||||||||||||
| I magnitude | |||||||||||||||
| J magnitude | 16.90 (0.03) | 16.88 (0.2) | 16.88 | 16.88 (0.2) | |||||||||||
| H magnitude | 16.07 (0.03) | 16.07 | |||||||||||||
| K magnitude | 15.33 (0.03) | 15.33 | |||||||||||||
| u magnitude | 20.42 (0.05) | 20.43 | 20.42 (0.05) | 20.42 (0.05) | |||||||||||
| g magnitude | 18.76 | 18.67 (0.008) | 18.76 (0.008) | ||||||||||||
| r magnitude | 18.10 | 18.09 (0.006) | 18.10 (0.007) | ||||||||||||
| i magnitude | 17.82 | 17.85 (0.009) | 17.82 (0.007) | ||||||||||||
| z magnitude | 17.75 | 17.75 (0.02) | 17.75 (0.02) | ||||||||||||
| G magnitude | 18.13 (0.02) | 18.15 | 18.13 | 18.13 (0.003) | 18.15 | ||||||||||
| BP magnitude | 18.60 (0.02) | 18.66 | 18.66 | ||||||||||||
| RP magnitude | 17.52 (0.01) | 17.52 | 17.52 | ||||||||||||
| Pan g magnitude | 18.67 (0.007) | 18.67 (0.008) | 18.67 (0.008) | ||||||||||||
| Pan r magnitude | 18.09 (0.005) | 18.09 (0.006) | 18.09 (0.006) | ||||||||||||
| Pan i magnitude | 17.85 (0.009) | 17.85 (0.009) | 17.85 (0.009) | ||||||||||||
| Pan z magnitude | 17.79 (0.02) | 17.79 (0.02) | 17.79 (0.02) | ||||||||||||
| Pan y magnitude | 17.77 (0.02) | 17.77 (0.02) | 17.77 (0.02) | ||||||||||||
| 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.