All names: LSPM J2022+7811, SDSS J202201.80+781118.9, SDSS J202201.81+781118.9, USNO-B1.0 1681-00094121, Gaia EDR3 2291002488457478784, Gaia DR3 2291002488457478784, GALEX J202202.0+781119, Gaia DR2 2291002488457478784
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | MWDD H | Gaia DR2 | Stilism | Vincent et al. 2024 | Simbad | Kleinman et al. 2013 | Vincent et al. 2023 |
---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 20 22 02.07 (0.08) | 20 22 01.81 | 20 22 02.06 (0.09) | 20 22 02.07 | 20 22 01.73 (0.08) | 20 22 01.81 | |||||
Declination | 78 11 20.37 (0.08) | 78 11 18.95 | 78 11 20.32 (0.1) | 78 11 20.37 | 78 11 18.55 (0.08) | 78 11 18.92 | |||||
Spectral type | DA | DA | DA | DA | DA | ||||||
Effective temperature | [K] | 10063.0 | 10325.0 (212) | 10248.0 (56) | |||||||
log(g) | [cgs] | 7.98 | 8.02 (0.03) | 8.17 (0.07) | |||||||
Mass | [M☉] | 0.589 | 0.614 (0.03) | 0.699 (0.04) | |||||||
log(Luminosity) | [L☉] | ||||||||||
Cooling age | [Gyr] | 0.5781 | |||||||||
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] | 6.84 (0.08) | 6.84 (0.1) | 6.84 | 6.84 (0.08) | ||||||
Distance | [pc] | 146.16 (2) | 146.26 (2) | 146.16 | 146.16 (2) | ||||||
Composition | H | ||||||||||
Proper motion (right ascension) | [mas/yr] | 65.37273727 (0.1) | 65.45035858 (0.2) | 65.373 (0.1) | |||||||
Proper motion (declination) | [mas/yr] | 113.8627298 (0.1) | 113.7466749 (0.2) | 113.863 (0.1) | |||||||
Variability | |||||||||||
Magnetic | |||||||||||
Bd | [MG] | ||||||||||
Infrared excess (disk) | |||||||||||
Binarity | |||||||||||
B magnitude | 17.80 | ||||||||||
V magnitude | |||||||||||
R magnitude | 17.90 | ||||||||||
I magnitude | |||||||||||
J magnitude | |||||||||||
H magnitude | |||||||||||
K magnitude | |||||||||||
u magnitude | 18.35 (0.02) | 18.35 (0.02) | 18.36 (0.03) | ||||||||
g magnitude | 17.91 (0.006) | 17.91 (0.006) | 17.95 (0.02) | ||||||||
r magnitude | 18.00 (0.007) | 18.00 (0.007) | 18.00 (0.01) | ||||||||
i magnitude | 18.13 (0.009) | 18.13 (0.009) | 18.13 (0.01) | ||||||||
z magnitude | 18.30 (0.03) | 18.30 (0.03) | 18.30 (0.03) | ||||||||
G magnitude | 17.93 (0.01) | 17.95 | 17.93 | 17.93 (0.003) | |||||||
BP magnitude | 17.99 (0.01) | 17.97 | |||||||||
RP magnitude | 17.87 (0.02) | 17.86 | |||||||||
Pan g magnitude | 17.94 (0.009) | ||||||||||
Pan r magnitude | 18.03 (0.004) | ||||||||||
Pan i magnitude | 18.18 (0.005) | ||||||||||
Pan z magnitude | 18.35 (0.007) | ||||||||||
Pan y magnitude | 18.46 (0.03) | ||||||||||
E(B-V) | 0.009 |
* 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.