All names: TIC 386839208, PM J08082+1854, GALEX J080812.6+185420, NLTT 18981, USNO-B1.0 1089-00160390, SDSS J080812.74+185421.04, LP 424-13, SDSS J080812.74+185421.0, J0808+1854, Gaia DR2 669444943132791424, PSO J122.0526+18.9054, 2MASS J08081279+1854213, Gaia DR3 669444943132791424, Gaia EDR3 669444943132791424, SDSS J080812.73+185421.0, 08082+1854, WDJ080812.78+185421.63, LSPM J0808+1854, SDSS J080812.70+185420.6
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR10 | 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 | Kepler et al. 2015 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | Vincent et al. 2023 |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 08 08 12.62 (0.09) | 08 08 12.74 | 08 08 12.62 (0.1) | 08 08 12.62 | 08 08 12.78 (0.09) | 08 08 12.62 | |||||||||||
Declination | 18 54 19.39 (0.07) | 18 54 21.02 | 18 54 19.46 (0.07) | 18 54 19.39 | 18 54 21.63 (0.07) | 18 54 19.46 | |||||||||||
Spectral type | DA | DA | DA | DA | DA | DA | DA | DA | DA | DA | DA | ||||||
Effective temperature | [K] | 5676.0 (26) | 5687.0 (25) | 5674.0 (26) | 5630.0 (45) | 5644.0 | 5690.0 (126) | 6166.0 (154) | 5745.0 (63) | ||||||||
log(g) | [cgs] | 7.97 (0.01) | 7.95 (0.01) | 7.95 (0.01) | 7.93 (0.03) | 7.94 | 8.21 (0.3) | 8.13 (0.05) | 8.00 (0.02) | ||||||||
Mass | [M☉] | 0.566 (0.009) | 0.556 (0.01) | 0.557 (0.01) | 0.546 (0.01) | 0.548 | 0.72 (0.2) | 0.665 (0.03) | 0.585 (0.02) | ||||||||
log(Luminosity) | [L☉] | -3.94 | |||||||||||||||
Cooling age | [Gyr] | 2.4900 | 2.4660 (0.1) | 2.4490 | |||||||||||||
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] | 19.45 (0.1) | 19.28 (0.1) | 19.28 (0.1) | 19.28 (0.1) | 19.45 | 19.45 (0.1) | 19.28 (0.1) | |||||||||
Distance | [pc] | 51.41 (0.3) | 51.87 (0.4) | 51.87 (0.4) | 51.87 (0.4) | 43.80 (1) | 51.41 | 51.41 (0.3) | 51.87 (0.4) | ||||||||
Composition | H | H | H | H | H | ||||||||||||
Proper motion (right ascension) | [mas/yr] | -146.0422468 (0.1) | -146.2087881 (0.2) | -143.0 | -146.042 (0.1) | -146.209 | |||||||||||
Proper motion (declination) | [mas/yr] | -140.0773929 (0.08) | -139.9570025 (0.1) | -143.0 | -140.077 (0.08) | -139.957 | |||||||||||
Variability | |||||||||||||||||
Magnetic | |||||||||||||||||
Bd | [MG] | ||||||||||||||||
Infrared excess (disk) | |||||||||||||||||
Binarity | |||||||||||||||||
B magnitude | 18.30 | ||||||||||||||||
V magnitude | |||||||||||||||||
R magnitude | 17.30 | ||||||||||||||||
I magnitude | |||||||||||||||||
J magnitude | 16.77 (0.02) | 16.82 (0.1) | 16.82 | 16.82 (0.1) | |||||||||||||
H magnitude | 16.36 (0.2) | 16.36 (0.2) | 16.36 | 16.36 (0.2) | |||||||||||||
K magnitude | 16.24 (0.03) | 16.24 | |||||||||||||||
u magnitude | 19.28 (0.02) | 19.23 (0.03) | 19.28 | 19.28 (0.02) | 19.28 (0.03) | 19.28 (0.03) | |||||||||||
g magnitude | 18.23 (0.007) | 18.22 | 18.23 (0.01) | 18.17 (0.009) | 18.22 (0.007) | ||||||||||||
r magnitude | 17.76 (0.006) | 17.76 | 17.76 (0.01) | 17.76 (0.005) | 17.76 (0.006) | ||||||||||||
i magnitude | 17.57 (0.007) | 17.57 | 17.57 (0.01) | 17.60 (0.005) | 17.60 (0.006) | ||||||||||||
z magnitude | 17.49 (0.01) | 17.50 | 17.49 (0.01) | 17.56 (0.004) | 17.50 (0.01) | ||||||||||||
G magnitude | 17.78 (0.02) | 17.80 | 17.78 | 17.78 (0.003) | 17.80 | ||||||||||||
BP magnitude | 18.08 (0.02) | 18.11 | 18.11 | ||||||||||||||
RP magnitude | 17.26 (0.01) | 17.26 | 17.26 | ||||||||||||||
Pan g magnitude | 18.17 (0.01) | 18.17 (0.009) | 18.17 (0.009) | ||||||||||||||
Pan r magnitude | 17.76 (0.007) | 17.76 (0.006) | 17.76 (0.006) | ||||||||||||||
Pan i magnitude | 17.60 (0.005) | 17.60 (0.005) | 17.60 (0.005) | ||||||||||||||
Pan z magnitude | 17.56 (0.004) | 17.56 (0.004) | 17.56 (0.004) | ||||||||||||||
Pan y magnitude | 17.55 (0.02) | 17.55 (0.02) | 17.55 (0.02) | ||||||||||||||
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.