All names: SDSS J103103.55+323452.6, LAMOST J103103.54+323452.9, 2MASS J10310356+3234529, Ton S 523, TIC 407612980, J1031+3234, Gaia DR3 748517142181920768, Gaia DR2 748517142181920768, CBS 21, SDSS J103103.55+323452.9, WD 1028+328, WDJ103103.54+323453.09, Gaia EDR3 748517142181920768, SDSS J103103.54+323452.9, SDSS J103103.54+323452.6, Ton 523
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Kilic et al. 2025 | Kilic et al. 2020 | MWDD H | Gaia DR2 | Stilism | Guo et al. 2015 | Gianninas et al. 2011 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) | Kleinman et al. 2013 | Vincent et al. 2023 |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 10 31 03.55 (0.04) | 10 31 03.55 | 10 31 03.55 (0.07) | 10 31 03.55 | 10 31 03.54 (0.04) | 10 31 03.55 | 10 31 03.24 | 10 31 03.54 | |||||||||
Declination | 32 34 52.51 (0.04) | 32 34 52.92 | 32 34 52.53 (0.1) | 32 34 52.51 | 32 34 53.09 (0.04) | 32 34 52.53 | 32 35 04.92 | 32 34 52.94 | |||||||||
Spectral type | DA | DA | DA | DA | DA | DA | DA3.3 | DA | DA5 | DA | DA | ||||||
Effective temperature | [K] | 15437.0 (203) | 15439.0 (204) | 15107.0 | 16967.0 (371) | 15260.0 (288) | 15207.0 (217) | 15949.0 (76) | |||||||||
log(g) | [cgs] | 8.11 (0.01) | 8.11 (0.01) | 8.09 | 8.06 (0.08) | 8.16 (0.05) | 8.10 (0.01) | 8.07 (0.01) | |||||||||
Mass | [M☉] | 0.682 (0.009) | 0.678 (0.01) | 0.664 | 0.65 (0.05) | 0.71 (0.03) | 0.671 (0.01) | 0.651 (0.006) | |||||||||
log(Luminosity) | [L☉] | ||||||||||||||||
Cooling age | [Gyr] | 0.2215 | |||||||||||||||
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] | 10.74 (0.06) | 10.70 (0.1) | 10.74 | 10.74 (0.06) | 10.70 (0.1) | |||||||||||
Distance | [pc] | 93.08 (0.5) | 93.41 (1) | 80.00 | 93.08 | 93.08 (0.5) | 93.42 (1) | ||||||||||
Composition | H | H | H | ||||||||||||||
Proper motion (right ascension) | [mas/yr] | 7.766183655 (0.05) | 7.63483051 (0.2) | 7.766 (0.05) | 7.635 | ||||||||||||
Proper motion (declination) | [mas/yr] | -36.01253611 (0.05) | -35.83762922 (0.3) | -36.013 (0.05) | -35.838 | ||||||||||||
Variability | |||||||||||||||||
Magnetic | |||||||||||||||||
Bd | [MG] | ||||||||||||||||
Infrared excess (disk) | |||||||||||||||||
Binarity | |||||||||||||||||
B magnitude | 15.40 | ||||||||||||||||
V magnitude | |||||||||||||||||
R magnitude | |||||||||||||||||
I magnitude | |||||||||||||||||
J magnitude | 16.20 (0.1) | ||||||||||||||||
H magnitude | |||||||||||||||||
K magnitude | |||||||||||||||||
u magnitude | 16.38 (0.006) | 16.38 (0.006) | 16.38 (0.006) | 16.35 (0.02) | |||||||||||||
g magnitude | 16.11 (0.004) | 16.11 (0.004) | 16.11 (0.004) | 16.17 (0.04) | |||||||||||||
r magnitude | 16.40 (0.004) | 16.40 (0.004) | 16.41 (0.004) | 16.44 (0.02) | |||||||||||||
i magnitude | 16.69 (0.005) | 16.69 (0.005) | 16.67 (0.005) | 16.68 (0.01) | |||||||||||||
z magnitude | 16.94 (0.01) | 16.94 (0.01) | 16.93 (0.01) | 16.93 (0.02) | |||||||||||||
G magnitude | 16.28 (0.003) | 16.29 | 16.28 | 16.28 (0.003) | 16.29 | ||||||||||||
BP magnitude | 16.24 (0.003) | 16.22 | 16.22 | ||||||||||||||
RP magnitude | 16.39 (0.004) | 16.39 | 16.39 | ||||||||||||||
Pan g magnitude | 16.15 (0.006) | ||||||||||||||||
Pan r magnitude | 16.42 (0.004) | ||||||||||||||||
Pan i magnitude | 16.70 (0.002) | ||||||||||||||||
Pan z magnitude | 16.94 (0.004) | ||||||||||||||||
Pan y magnitude | 17.11 (0.01) | ||||||||||||||||
E(B-V) | 0.005 |
* 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.