All names: SDSS J124140.02-073305.6, 2MASS J12414012-0733059, SDSS J124140.02-073305.7, SDSS J124140.03-073305.7, LAMOST J124140.02-073305.6, WD 1239-072, WDJ124140.10-073305.83, Gaia DR3 3676222491884053376, GALEX J124140.0-073305, SDSS J124140.03-073305.6, TIC 203250102, Gaia EDR3 3676222491884053376, Gaia DR2 3676222491884053376, J1241-0733
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Caron et al. 2023 | Kilic et al. 2020 | MWDD H | Gaia DR2 | Stilism | Guo et al. 2015 | Sayres et al. 2012 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | Kleinman et al. 2013 | Vincent et al. 2023 |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 12 41 39.92 (0.06) | 12 41 40.03 | 12 41 39.92 (0.1) | 12 41 40.12 | 12 41 39.92 | 12 41 40.10 (0.06) | 12 41 39.92 | 12 41 40.02 | ||||||||
Declination | -07 33 05.36 (0.04) | -07 33 05.70 | -07 33 05.38 (0.09) | -07 33 06.00 | -07 33 05.36 | -07 33 05.83 (0.04) | -07 33 05.38 | -07 33 05.67 | ||||||||
Spectral type | DA | DA | DA5.0 | DA | DA5.0 | DA | DA5 | DA | DA | |||||||
Effective temperature | [K] | 9930.0 (45) | 9800.0 (46) | 9828.0 | 10100.0 (50) | 9705.0 (90) | 9960.0 (20) | |||||||||
log(g) | [cgs] | 8.01 (0.01) | 7.98 (0.01) | 7.99 | 8.23 (0.05) | 7.97 (0.02) | 8.24 (0.02) | |||||||||
Mass | [M☉] | 0.605 (0.01) | 0.588 (0.01) | 0.591 | 0.58 (0.01) | 0.741 (0.01) | ||||||||||
log(Luminosity) | [L☉] | |||||||||||||||
Cooling age | [Gyr] | 0.6500 | 0.6185 | |||||||||||||
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] | 12.15 (0.08) | 12.08 (0.1) | 12.08 (0.2) | 12.15 | 12.15 (0.08) | 12.08 (0.2) | |||||||||
Distance | [pc] | 82.30 (0.5) | 82.78 (1) | 82.78 (1) | 82.90 | 82.30 | 82.30 (0.5) | 82.78 (1) | ||||||||
Composition | H | H | H | |||||||||||||
Proper motion (right ascension) | [mas/yr] | -172.0323539 (0.08) | -171.8379558 (0.2) | -172.032 (0.08) | -171.8379558 | |||||||||||
Proper motion (declination) | [mas/yr] | 29.20595366 (0.06) | 29.13186341 (0.1) | 29.206 (0.06) | 29.13186341 | |||||||||||
Variability | ||||||||||||||||
Magnetic | ||||||||||||||||
Bd | [MG] | |||||||||||||||
Infrared excess (disk) | ||||||||||||||||
Binarity | ||||||||||||||||
B magnitude | ||||||||||||||||
V magnitude | ||||||||||||||||
R magnitude | ||||||||||||||||
I magnitude | ||||||||||||||||
J magnitude | 16.67 (0.02) | 16.63 (0.1) | 16.63 (0.1) | |||||||||||||
H magnitude | 16.66 (0.03) | 17.66 | ||||||||||||||
K magnitude | 16.74 (0.06) | 16.28 | ||||||||||||||
u magnitude | 17.24 (0.01) | 17.24 (0.01) | 17.25 (0.01) | 17.24 (0.01) | 17.24 (0.01) | 17.26 (0.01) | ||||||||||
g magnitude | 16.79 (0.004) | 16.79 (0.004) | 16.79 (0.004) | 16.79 (0.004) | 16.83 (0.02) | |||||||||||
r magnitude | 16.86 (0.005) | (0.005) | 16.86 (0.005) | 16.86 (0.005) | 16.89 (0.01) | |||||||||||
i magnitude | 16.99 (0.006) | 16.99 (0.006) | 16.99 (0.006) | 16.99 (0.006) | 16.99 (0.01) | |||||||||||
z magnitude | 17.13 (0.01) | 17.14 (0.01) | 17.13 (0.01) | 17.13 (0.01) | 17.14 (0.02) | |||||||||||
G magnitude | 16.79 (0.004) | 16.81 | 16.79 | 16.79 (0.003) | 16.81 | |||||||||||
BP magnitude | 16.85 (0.004) | 16.85 | 16.85 | |||||||||||||
RP magnitude | 16.69 (0.006) | 16.69 | 16.69 | |||||||||||||
Pan g magnitude | 16.80 (0.003) | 16.80 (0.003) | ||||||||||||||
Pan r magnitude | 16.88 (0.004) | 16.88 (0.004) | ||||||||||||||
Pan i magnitude | 17.02 (0.008) | 17.02 (0.008) | ||||||||||||||
Pan z magnitude | 17.16 (0.005) | 17.16 (0.004) | ||||||||||||||
Pan y magnitude | 17.28 (0.007) | 17.28 (0.007) | ||||||||||||||
E(B-V) | 0.002 |
* 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.