All names: Gaia DR2 1682132737571666560, SDSS J124522.69+670036.0, Gaia DR3 1682132737571666560, J1245+6700, SDSS J124522.69+670036.21, SDSS J124522.69+670036.2, GALEX J124522.7+670036, Gaia EDR3 1682132737571666560
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Coutu et al. 2019 | Gaia DR2 | Stilism | Kepler et al. 2016 | Simbad | Vincent et al. 2023 |
---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 12 45 22.65 (0.4) | 12 45 22.70 | 12 45 22.70 | 12 45 22.65 (0.6) | 12 45 22.71 (0.4) | |||||
Declination | 67 00 36.04 (0.3) | 67 00 36.00 | 67 00 35.97 | 67 00 36.04 (0.5) | 67 00 35.97 (0.3) | |||||
Spectral type | DZ | DZ | DZ | DZ | ||||||
Effective temperature | [K] | 7842.0 (338) | 7978.0 (75) | |||||||
log(g) | [cgs] | 7.40 | 8.00 (0) | |||||||
Mass | [M☉] | 0.2931 | ||||||||
log(Luminosity) | [L☉] | |||||||||
Cooling age | [Gyr] | 0.6350 | ||||||||
log(H/He) | <-5.2505 | |||||||||
log(C/He) | ||||||||||
log(Ca/He) | -10.4861 (0.1) | -9.032 | ||||||||
log(Ca/H) | ||||||||||
log(N/He) | ||||||||||
log(O/He) | ||||||||||
log(Na/He) | ||||||||||
log(Mg/He) | ||||||||||
log(Al/He) | ||||||||||
log(Si/He) | ||||||||||
log(P/He) | ||||||||||
log(S/He) | ||||||||||
log(Cl/He) | ||||||||||
log(Sc/He) | ||||||||||
log(Ti/He) | ||||||||||
log(V/He) | ||||||||||
log(Cr/He) | ||||||||||
log(Mn/He) | ||||||||||
log(Fe/He) | ||||||||||
log(Co/He) | ||||||||||
log(Ni/He) | ||||||||||
log(Cu/He) | ||||||||||
log(Zn/He) | ||||||||||
log(Ga/He) | ||||||||||
log(Ge/He) | ||||||||||
log(Sr/He) | ||||||||||
Parallax | [mas] | 3.13 (0.4) | 2.75 | 2.75 (0.7) | 3.13 (0.4) | |||||
Distance | [pc] | 319.12 (43) | 363.64 (89) | 363.64 (89) | 319.11 (43) | |||||
Composition | He | He | ||||||||
Proper motion (right ascension) | [mas/yr] | -21.88483545 (0.4) | -19.87889037 (0.8) | -21.885 (0.4) | ||||||
Proper motion (declination) | [mas/yr] | 4.533646656 (0.4) | 4.394233011 (0.8) | 4.534 (0.4) | ||||||
Variability | ||||||||||
Magnetic | ||||||||||
Bd | [MG] | |||||||||
Infrared excess (disk) | ||||||||||
Binarity | ||||||||||
B magnitude | ||||||||||
V magnitude | ||||||||||
R magnitude | ||||||||||
I magnitude | ||||||||||
J magnitude | ||||||||||
H magnitude | ||||||||||
K magnitude | ||||||||||
u magnitude | 20.66 (0.07) | 20.65 (0.07) | 20.66 (0.07) | |||||||
g magnitude | 20.22 (0.02) | 20.21 (0.03) | 20.21 (0.02) | |||||||
r magnitude | 20.17 (0.03) | 20.14 (0.03) | 20.16 (0.03) | |||||||
i magnitude | 20.29 (0.04) | 20.28 (0.04) | 20.29 (0.04) | |||||||
z magnitude | 20.13 (0.1) | 20.13 (0.1) | 20.12 (0.1) | |||||||
G magnitude | 20.15 (0.05) | 20.19 | 20.15 (0.005) | |||||||
BP magnitude | 20.20 (0.05) | 20.30 | ||||||||
RP magnitude | 19.90 (0.09) | 19.86 | ||||||||
Pan g magnitude | 20.19 (0.01) | |||||||||
Pan r magnitude | 20.19 (0.01) | |||||||||
Pan i magnitude | 20.31 (0.03) | |||||||||
Pan z magnitude | 20.46 (0.08) | |||||||||
Pan y magnitude | 20.30 (0.2) | |||||||||
E(B-V) | 0.018 |
* 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.