All names: PM J15206+3903, Gaia EDR3 1388493176528426752, CSO 582, SDSS J152038.34+390349.7, WIRED J152038.34+390349.7, LSPM J1520+3903, Gaia DR3 1388493176528426752, USNO-B1.0 1290-00245814, TIC 138328116, SDSS J152038.34+390349.8, J1520+3903, WD 1518+392, 15206+3903, WDJ152038.37+390349.32, GALEX J152038.3+390350, Gaia DR2 1388493176528426752, PSO J230.1594+39.0643, 2MASS J15203838+3903492
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Caron et al. 2023 | Blouin et al. 2019 | MWDD H | Gaia DR2 | Stilism | Limoges et al. 2015 | 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 | 15 20 38.26 (0.03) | 15 20 38.26 (0.04) | 15 20 38.26 | 15 20 38.37 (0.04) | 15 20 38.26 | 15 20 38.16 | 15 20 38.34 | ||||||||
Declination | 39 03 51.73 (0.04) | 39 03 51.65 (0.06) | 39 03 51.73 | 39 03 49.31 (0.04) | 39 03 51.65 | 39 03 45.00 | 39 03 49.79 | ||||||||
Spectral type | DA | DA | DA | DA | DA | DA | DA | DA | DA | ||||||
Effective temperature | [K] | 8046.0 (35) | 7905.0 (80) | 7947.0 | 8710.0 (129) | 7979.0 (59) | 8627.0 (18) | ||||||||
log(g) | [cgs] | 7.32 (0.01) | 7.29 (0.03) | 7.29 | 8.05 (0.07) | 7.31 (0.01) | 8.03 (0.03) | ||||||||
Mass | [M☉] | 0.284 (0.004) | 0.277 (0.008) | 0.277 | 0.62 (0.04) | 0.281 (0.006) | 0.614 (0.02) | ||||||||
log(Luminosity) | [L☉] | -3.10 | |||||||||||||
Cooling age | [Gyr] | 0.5100 | 0.5540 (0.02) | 0.5475 | |||||||||||
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] | 10.58 (0.05) | 10.57 (0.06) | 10.57 (0.06) | 10.57 (0.06) | 10.58 | 10.58 (0.05) | 10.57 (0.06) | |||||||
Distance | [pc] | 94.50 (0.4) | 94.61 (0.5) | 94.60 (0.6) | 94.60 (0.6) | 68.00 (1) | 94.50 | 94.50 (0.4) | 94.60 (0.6) | ||||||
Composition | H | H | H | H | |||||||||||
Proper motion (right ascension) | [mas/yr] | -83.8810656 (0.04) | -83.95088716 (0.09) | -83.881 (0.04) | -83.95088716 | ||||||||||
Proper motion (declination) | [mas/yr] | 150.8930296 (0.06) | 150.5572866 (0.1) | 150.893 (0.06) | 150.5572866 | ||||||||||
Variability | |||||||||||||||
Magnetic | |||||||||||||||
Bd | [MG] | ||||||||||||||
Infrared excess (disk) | |||||||||||||||
Binarity | |||||||||||||||
B magnitude | 17.00 | ||||||||||||||
V magnitude | |||||||||||||||
R magnitude | 16.90 | ||||||||||||||
I magnitude | |||||||||||||||
J magnitude | 16.47 (0.02) | 16.35 (0.1) | 16.35 | 16.35 (0.1) | |||||||||||
H magnitude | 16.52 (0.03) | 16.52 | |||||||||||||
K magnitude | 15.83 (0.03) | 15.83 | |||||||||||||
u magnitude | 17.44 (0.03) | 17.44 | 17.68 (0.1) | 17.42 (0.01) | 17.68 (0.1) | ||||||||||
g magnitude | 16.95 | 17.02 (0.004) | 16.97 (0.004) | 17.00 (0.03) | |||||||||||
r magnitude | 17.00 | 16.96 (0.004) | 17.00 (0.004) | 17.36 (0.07) | |||||||||||
i magnitude | 16.82 | 17.00 (0.002) | 16.84 (0.005) | 16.97 (0.03) | |||||||||||
z magnitude | 16.79 | 17.08 (0.005) | 16.81 (0.01) | 17.07 (0.02) | |||||||||||
G magnitude | 16.91 (0.005) | 16.93 | 16.91 | 16.91 (0.003) | 16.93 | ||||||||||
BP magnitude | 17.04 (0.005) | 17.04 | 17.04 | ||||||||||||
RP magnitude | 16.67 (0.005) | 16.68 | 16.68 | ||||||||||||
Pan g magnitude | 17.02 (0.004) | 17.02 (0.004) | 17.02 (0.004) | ||||||||||||
Pan r magnitude | 16.96 (0.004) | 16.96 (0.004) | 16.96 (0.004) | ||||||||||||
Pan i magnitude | 17.00 (0.002) | 17.00 (0.002) | 17.00 (0.002) | ||||||||||||
Pan z magnitude | 17.08 (0.006) | 17.08 (0.005) | 17.08 (0.005) | ||||||||||||
Pan y magnitude | 17.15 (0.005) | 17.15 (0.005) | 17.15 (0.005) | ||||||||||||
E(B-V) | 0.014 |
* 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.