All names: WD 1018+410, LAMOST J102155.49+405014.7, Gaia EDR3 804169064957527552, LAMOST J102155.50+405015.9, 2MASS J10215550+4050138, SDSS J102155.49+405014.7, SDSS J102155.50+405014.75, UCAC3 262-117114, PG 1018+411, CMC14 J102155.5+405014, LAMOST J102155.50+405014.8, TIC 8152776, LAMOST J102155.50+405014.85, GALEX J102155.4+405015, Gaia DR3 804169064957527552, UCAC4 655-053125, FBS 1018+411, GSC2.3 N9A2003465, SDSS J102155.50+405014.7, FBS B 71, Gaia DR2 804169064957527552, SDSS J102155.50+405014.8, USNO-B1.0 1308-00212469
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR10 | SDSS DR12 | MWDD H | Gaia DR2 | Stilism | Guo et al. 2015 | Kepler et al. 2015 | Zhao et al. 2013 | Gianninas et al. 2011 | Vincent et al. 2024 | Simbad | White Dwarf Catalog (McCook & Sion 1999) | Vincent et al. 2023 |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 10 21 55.50 (0.04) | 10 21 55.51 | 10 21 55.51 | 10 21 55.50 (0.07) | 10 21 55.50 | 10 21 55.50 | 10 21 55.51 (0.04) | 10 21 54.17 | ||||||||
Declination | 40 50 14.70 (0.04) | 40 50 14.83 | 40 50 14.83 | 40 50 14.71 (0.07) | 40 50 14.85 | 40 50 14.70 | 40 50 14.89 (0.04) | 40 50 09.24 | ||||||||
Spectral type | DA | DA;debris_disk | DA | DA | DA | DA3 | DA3 | DA | ||||||||
Effective temperature | [K] | 19052.0 | 25498.0 (314) | 25330.0 (69) | 23364.0 (999) | 24440.0 (405) | 21520.0 (395) | |||||||||
log(g) | [cgs] | 7.91 | 8.03 (0.04) | 8.23 (0.01) | 7.96 (0.1) | 8.11 (0.05) | 8.07 (0.02) | |||||||||
Mass | [M☉] | 0.574 | 0.65 (0.02) | 0.759 (0.008) | 0.61 (0.09) | 0.69 (0.03) | 0.665 (0.01) | |||||||||
log(Luminosity) | [L☉] | |||||||||||||||
Cooling age | [Gyr] | 0.0686 | 0.0280 (0.02) | |||||||||||||
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] | 7.36 (0.06) | 7.26 (0.1) | 7.36 | 7.36 (0.06) | |||||||||||
Distance | [pc] | 135.96 (1) | 137.72 (2) | 153.00 | 100.00 | 135.96 | 135.95 (1) | |||||||||
Composition | H | H | ||||||||||||||
Proper motion (right ascension) | [mas/yr] | -8.316059186 (0.05) | -8.662896733 (0.1) | -8.316 (0.05) | ||||||||||||
Proper motion (declination) | [mas/yr] | -11.46920342 (0.05) | -11.36888088 (0.2) | -11.469 (0.05) | ||||||||||||
Variability | ||||||||||||||||
Magnetic | ||||||||||||||||
Bd | [MG] | |||||||||||||||
Infrared excess (disk) | ||||||||||||||||
Binarity | ||||||||||||||||
B magnitude | 16.34 (0.06) | |||||||||||||||
V magnitude | 16.37 (0.03) | |||||||||||||||
R magnitude | 16.46 (0.4) | |||||||||||||||
I magnitude | 16.66 (0.4) | |||||||||||||||
J magnitude | 16.67 (0.1) | |||||||||||||||
H magnitude | ||||||||||||||||
K magnitude | ||||||||||||||||
u magnitude | 16.20 (0.006) | 16.20 (0.006) | 16.19 (0.01) | 16.19 | 16.20 (0.006) | |||||||||||
g magnitude | 16.22 (0.004) | 16.22 (0.004) | 16.25 (0.02) | 16.25 | 16.22 (0.004) | |||||||||||
r magnitude | 16.60 (0.005) | 16.60 (0.005) | 16.61 (0.03) | 16.61 | 16.60 (0.005) | |||||||||||
i magnitude | 16.91 (0.005) | 16.91 (0.005) | 16.91 (0.02) | 16.91 | 16.91 (0.005) | |||||||||||
z magnitude | 17.22 (0.01) | 17.22 (0.01) | 17.23 (0.03) | 17.23 | 17.22 (0.01) | |||||||||||
G magnitude | 16.44 (0.004) | 16.45 | 16.44 | 16.44 (0.003) | ||||||||||||
BP magnitude | 16.34 (0.004) | 16.31 | ||||||||||||||
RP magnitude | 16.62 (0.005) | 16.63 | ||||||||||||||
Pan g magnitude | 16.29 (0.005) | |||||||||||||||
Pan r magnitude | 16.61 (0.006) | |||||||||||||||
Pan i magnitude | 16.94 (0.002) | |||||||||||||||
Pan z magnitude | 17.22 (0.006) | |||||||||||||||
Pan y magnitude | 17.36 (0.02) | |||||||||||||||
E(B-V) | 0.008 |
* 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.