All names: PSO J001.9769+39.7920, TIC 194300778, Gaia DR2 383108338321272448, WD 0005+395, Gaia DR3 383108338321272448, PM J00079+3947, 2MASS J00075407+3947322, NLTT 317, Gaia EDR3 383108338321272448, J0007+3947, LSPM J0007+3947, USNO-B1.0 1297-00003001, LP 240-30, WDJ000754.11+394732.18, 00079+3947
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | O'Brien et al. 2024 | Caron et al. 2023 | McCleery et al. 2020 | Blouin et al. 2019 | MWDD H | Gaia DR2 | Stilism | Holberg et al. 2016 | Limoges et al. 2015 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 00 07 54.61 (0.04) | 00 07 54.60 (0.05) | 00 07 54.60 (0.05) | 00 07 54.61 | 00 07 54.11 (0.04) | 00 07 54.60 | |||||||||
| Declination | 39 47 30.95 (0.03) | 39 47 30.99 (0.03) | 39 47 30.99 (0.03) | 39 47 30.95 | 39 47 32.18 (0.03) | 39 47 30.99 | |||||||||
| Spectral type | DC | DC | DC | DC | DC | DC | DC | DC: | DC | ||||||
| Effective temperature | [K] | 4679.0 (27) | 4759.0 (12) | 4626.7 (14) | 4680.0 (25) | 4690.0 | 4890.0 (435) | 4890.0 (453) | |||||||
| log(g) | [cgs] | 6.93 (0.04) | 7.05 (0.007) | 6.88 (0.02) | 6.77 (0.04) | 6.77 | 8.00 (0) | 8.00 (0) | |||||||
| Mass | [M☉] | 0.17 (0.009) | 0.201 (0.003) | 0.081 (0.02) | 0.114 | 0.58 (0) | 0.58 (0.1) | ||||||||
| log(Luminosity) | [L☉] | -4.09 | |||||||||||||
| Cooling age | [Gyr] | 2.4200 | 1.4020 (0.06) | 6.1400 | |||||||||||
| 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] | 29.10 (0.06) | 29.10 (0.06) | 29.04 (0.06) | 29.04 (0.06) | 29.04 (0.06) | 29.04 (0.06) | 29.10 | 29.10 (0.06) | 29.04 (0.06) | |||||
| Distance | [pc] | 34.36 (0.07) | 34.36 (0.07) | 34.44 (0.07) | 34.44 (0.08) | 34.44 (0.07) | 34.44 (0.08) | 20.21 (1) | 20.20 (3) | 34.36 | 34.36 (0.07) | 34.44 (0.08) | |||
| Composition | H | H | H | H | |||||||||||
| Proper motion (right ascension) | [mas/yr] | 359.0968889 (0.04) | 359.1601674 (0.1) | 359.097 (0.04) | 359.1601674 | ||||||||||
| Proper motion (declination) | [mas/yr] | -76.64011946 (0.04) | -76.62790112 (0.05) | -76.64 (0.04) | -76.62790112 | ||||||||||
| Variability | |||||||||||||||
| Magnetic | |||||||||||||||
| Bd | [MG] | ||||||||||||||
| Infrared excess (disk) | |||||||||||||||
| Binarity | |||||||||||||||
| B magnitude | 17.40 | ||||||||||||||
| V magnitude | 17.12 | ||||||||||||||
| R magnitude | 16.20 | ||||||||||||||
| I magnitude | |||||||||||||||
| J magnitude | 15.17 (0.01) | 15.18 (0.04) | 15.18 | 15.18 (0.04) | |||||||||||
| H magnitude | 14.85 (0.07) | 14.85 (0.07) | 14.85 | 14.85 (0.07) | |||||||||||
| K magnitude | 14.65 (0.08) | 14.65 (0.08) | 14.65 | 14.65 (0.08) | |||||||||||
| u magnitude | |||||||||||||||
| g magnitude | 17.25 (0.005) | ||||||||||||||
| r magnitude | 16.53 (0.003) | ||||||||||||||
| i magnitude | 16.23 (0.002) | ||||||||||||||
| z magnitude | 16.12 (0.003) | ||||||||||||||
| G magnitude | 16.57 (0.005) | 16.58 | 16.58 | 16.57 | 16.57 (0.003) | 16.58 | |||||||||
| BP magnitude | 17.11 (0.005) | 17.13 | 17.13 | ||||||||||||
| RP magnitude | 15.88 (0.002) | 15.88 | 15.88 | ||||||||||||
| Pan g magnitude | 17.26 (0.02) | 17.25 (0.005) | 17.25 (0.005) | ||||||||||||
| Pan r magnitude | 16.54 (0.009) | 16.53 (0.003) | 16.53 (0.003) | ||||||||||||
| Pan i magnitude | 16.23 (0.004) | 16.23 (0.002) | 16.23 (0.002) | ||||||||||||
| Pan z magnitude | 16.11 (0.0008) | 16.12 (0.003) | 16.12 (0.003) | ||||||||||||
| Pan y magnitude | 16.04 (0.005) | 16.06 (0.004) | 16.06 (0.004) | ||||||||||||
| 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.