All names: Gaia DR2 3894780007343533184, 2MASS J12032867+0426532, USNO-B1.0 0944-00201067, SDSS J120328.64+042653.4, SDSS J120328.65+042653.4, WDJ120328.67+042653.27, Gaia DR3 3894780007343533184, LSPM J1203+0426, Gaia EDR3 3894780007343533184, J1203+0426, TIC 376813265, LP 554-23, NLTT 29432, WD 1200+047, SDSS J120328.64+042653.3
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Kilic et al. 2025 | Caron et al. 2023 | Bergeron et al. 2022 | MWDD H | MWDD HE | Gaia DR2 | Stilism | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 12 03 28.40 (0.09) | 12 03 28.40 (0.1) | 12 03 28.40 | 12 03 28.67 (0.09) | 12 03 28.40 | 12 03 28.70 | ||||||||
Declination | 04 26 55.70 (0.08) | 04 26 55.63 (0.09) | 04 26 55.70 | 04 26 53.26 (0.08) | 04 26 55.63 | 04 26 47.76 | ||||||||
Spectral type | DC-IRfaint | DC | DC | DC | DC | DC: | DC | DC10.4 | ||||||
Effective temperature | [K] | 4966.0 (21) | 4979.0 (20) | 4966.0 (21) | 4983.0 | 4690.0 | 5032.0 (43) | |||||||
log(g) | [cgs] | 7.48 (0.01) | 7.50 (0.02) | 7.33 | 7.10 | 7.36 (0.03) | ||||||||
Mass | [M☉] | 0.342 (0.004) | 0.349 (0.006) | 0.342 (0.004) | 0.265 | 0.186 | 0.273 (0.01) | |||||||
log(Luminosity) | [L☉] | |||||||||||||
Cooling age | [Gyr] | 4.1100 | 4.0210 | 1.8550 | 1.9290 | |||||||||
log(H/He) | -1.13 | -1.12 | -1.13 | |||||||||||
log(C/He) | ||||||||||||||
log(Ca/He) | ||||||||||||||
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] | 20.38 (0.1) | 20.45 (0.2) | 20.45 (0.2) | 20.38 | 20.38 (0.1) | 20.45 (0.2) | |||||||
Distance | [pc] | 49.07 (0.3) | 48.90 (0.4) | 48.90 (0.4) | 49.07 | 49.07 (0.3) | 48.90 (0.4) | |||||||
Composition | He | |||||||||||||
Proper motion (right ascension) | [mas/yr] | -253.6685527 (0.1) | -253.6079915 (0.3) | -253.669 (0.1) | -253.6079915 | |||||||||
Proper motion (declination) | [mas/yr] | 152.5099588 (0.08) | 152.3624383 (0.2) | 152.51 (0.08) | 152.3624383 | |||||||||
Variability | ||||||||||||||
Magnetic | ||||||||||||||
Bd | [MG] | |||||||||||||
Infrared excess (disk) | ||||||||||||||
Binarity | ||||||||||||||
B magnitude | 17.90 | |||||||||||||
V magnitude | ||||||||||||||
R magnitude | 17.60 | |||||||||||||
I magnitude | ||||||||||||||
J magnitude | 16.39 (0.01) | 16.39 (0.01) | ||||||||||||
H magnitude | 16.49 (0.02) | 16.49 (0.02) | ||||||||||||
K magnitude | 16.92 (0.06) | 16.92 (0.06) | ||||||||||||
u magnitude | 19.58 (0.03) | 19.58 (0.03) | 19.58 (0.03) | 19.47 | ||||||||||
g magnitude | 18.18 (0.006) | 18.18 (0.006) | 18.11 | |||||||||||
r magnitude | 17.47 (0.006) | 17.47 (0.006) | 17.45 | |||||||||||
i magnitude | 17.21 (0.006) | 17.21 (0.006) | 17.17 | |||||||||||
z magnitude | 17.12 (0.01) | 17.12 (0.01) | 17.09 | |||||||||||
G magnitude | 17.50 (0.01) | 17.52 | 17.50 | 17.50 (0.003) | 17.52 | |||||||||
BP magnitude | 17.99 (0.01) | 18.01 | 18.01 | |||||||||||
RP magnitude | 16.88 (0.007) | 16.89 | 16.89 | |||||||||||
Pan g magnitude | 18.11 (0.007) | 18.11 (0.006) | ||||||||||||
Pan r magnitude | 17.47 (0.008) | 17.47 (0.01) | ||||||||||||
Pan i magnitude | 17.23 (0.003) | 17.23 (0.003) | ||||||||||||
Pan z magnitude | 17.14 (0.004) | 17.14 (0.004) | ||||||||||||
Pan y magnitude | 17.12 (0.007) | 17.12 (0.007) | ||||||||||||
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.