All names: SDSS J110751.03+524653.3, SDSS J110751.04+524653.0, SDSS J110751.05+524653.2, Gaia EDR3 842504358196167680, Gaia DR2 842504358196167680, J1107+5246, Gaia DR3 842504358196167680, WD 1104+530.1, SDSS J110751.04+524653.3, SDSS J110751.05+524653.1, WDJ110751.05+524653.09, GALEX J110751.1+524653, SDSS J110751.04+524653.1
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Kilic et al. 2025 | Caron et al. 2023 | Kilic et al. 2020 | MWDD H | Gaia DR2 | Stilism | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | Eisenstein et al. 2006 | White Dwarf Catalog (McCook & Sion 1999) | Kleinman et al. 2013 | Vincent et al. 2023 |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 11 07 51.02 (0.08) | 11 07 51.05 | 11 07 51.02 (0.09) | 11 07 51.02 | 11 07 51.05 (0.08) | 11 07 51.02 | 11 07 51.05 | 11 07 51.24 | 11 07 51.05 | ||||||||
Declination | 52 46 53.25 (0.1) | 52 46 53.09 | 52 46 53.24 (0.1) | 52 46 53.25 | 52 46 53.10 (0.1) | 52 46 53.24 | 52 46 53.12 | 52 46 51.24 | 52 46 53.16 | ||||||||
Spectral type | DA | DA | DA | DA: | DA | DA | DA | DA: | DA: | DA | DA | ||||||
Effective temperature | [K] | 6719.0 (48) | 6753.0 (48) | 6720.0 (48) | 6594.0 | 6688.0 (107) | 7117.0 (58) | 6693.0 (60) | |||||||||
log(g) | [cgs] | 8.01 (0.02) | 8.04 (0.02) | 8.02 (0.02) | 7.98 | 7.98 (0.03) | 8.74 (0.2) | 8.04 (0.2) | |||||||||
Mass | [M☉] | 0.595 (0.02) | 0.612 (0.02) | 0.603 (0.02) | 0.576 | 0.581 (0.03) | 0.615 (0.1) | ||||||||||
log(Luminosity) | [L☉] | ||||||||||||||||
Cooling age | [Gyr] | 1.8100 | 1.6970 | ||||||||||||||
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] | 10.24 (0.1) | 10.33 (0.2) | 10.33 (0.2) | 10.24 | 10.24 (0.1) | 10.33 (0.2) | ||||||||||
Distance | [pc] | 97.65 (1) | 96.81 (2) | 96.81 (2) | 97.65 | 97.65 (1) | 96.81 (2) | ||||||||||
Composition | H | H | H | ||||||||||||||
Proper motion (right ascension) | [mas/yr] | -18.99465301 (0.1) | -19.06702314 (0.2) | -18.995 (0.1) | -19.067 | -14.8 | |||||||||||
Proper motion (declination) | [mas/yr] | 9.09656591 (0.1) | 9.502046769 (0.3) | 9.097 (0.1) | 9.502 | 7.7 | |||||||||||
Variability | |||||||||||||||||
Magnetic | |||||||||||||||||
Bd | [MG] | ||||||||||||||||
Infrared excess (disk) | |||||||||||||||||
Binarity | |||||||||||||||||
B magnitude | |||||||||||||||||
V magnitude | |||||||||||||||||
R magnitude | |||||||||||||||||
I magnitude | |||||||||||||||||
J magnitude | 17.85 (0.05) | ||||||||||||||||
H magnitude | |||||||||||||||||
K magnitude | |||||||||||||||||
u magnitude | 19.36 (0.03) | 19.37 (0.03) | 19.36 (0.03) | 19.36 (0.03) | 19.40 (0.04) | 19.39 | 19.39 (0.04) | ||||||||||
g magnitude | 18.75 (0.009) | 18.75 (0.009) | 18.75 (0.009) | 18.80 (0.01) | 18.79 | 18.80 (0.01) | |||||||||||
r magnitude | 18.54 (0.009) | 18.54 (0.009) | 18.54 (0.009) | 18.56 (0.03) | 18.56 (0.03) | ||||||||||||
i magnitude | 18.47 (0.01) | 18.47 (0.01) | 18.47 (0.01) | 18.47 (0.01) | 18.47 (0.01) | ||||||||||||
z magnitude | 18.51 (0.03) | 18.51 (0.03) | 18.51 (0.03) | 18.48 (0.04) | 18.48 (0.04) | ||||||||||||
G magnitude | 18.53 (0.02) | 18.55 | 18.53 | 18.53 (0.003) | 18.55 | ||||||||||||
BP magnitude | 18.80 (0.02) | 18.77 | 18.77 | ||||||||||||||
RP magnitude | 18.15 (0.01) | 18.17 | 18.17 | ||||||||||||||
Pan g magnitude | 18.79 (0.009) | 18.79 (0.007) | |||||||||||||||
Pan r magnitude | 18.57 (0.01) | 18.57 (0.01) | |||||||||||||||
Pan i magnitude | 18.49 (0.004) | 18.49 (0.003) | |||||||||||||||
Pan z magnitude | 18.51 (0.01) | 18.51 (0.01) | |||||||||||||||
Pan y magnitude | 18.57 (0.03) | 18.57 (0.03) | |||||||||||||||
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.