All names: SDSS J152356.57+542256.8, WD 1522+545, USNO-B1.0 1443-00241905, PSO J152356.591+542257.022, Gaia DR2 1599573467458776704, SDSS J152356.57+542256.87
Parameter | Unit | MWDD H | Pan-STARRS DR1 | Gaia DR2 | Kepler et al. 2016 | SDSS DR12 | Simbad |
---|---|---|---|---|---|---|---|
Right ascension | 15 23 56.57 (0.1) | 15 23 56.59 | 15 23 56.59 | ||||
Declination | 54 22 57.00 (0.2) | 54 22 56.79 | 54 22 56.77 | ||||
Spectral type | DA | DA | DA | ||||
Effective temperature | [K] | 20610.0 | 21694.0 (136) | ||||
log(g) | [cgs] | 7.78 | 7.86 (0.02) | ||||
Mass | [M☉] | 0.51 | 0.5579999999999999 (0.009) | ||||
log(Luminosity) | [L☉] | ||||||
Cooling age | [Gyr] | 0.0372 | |||||
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] | 3.48 (0.1) | |||||
Distance | [pc] | 287.37 (10) | |||||
Composition | H | ||||||
Proper motion (right ascension) | [mas/yr] | -10.1507159354 (0.2) | -16.0 | ||||
Proper motion (declination) | [mas/yr] | 12.7182896703 (0.3) | 16.0 | ||||
Variability | |||||||
Magnetic | |||||||
Bd | [MG] | ||||||
Infrared excess (disk) | |||||||
Binarity | |||||||
B magnitude | 17.30 | ||||||
V magnitude | |||||||
R magnitude | 17.70 | ||||||
I magnitude | |||||||
J magnitude | |||||||
H magnitude | |||||||
K magnitude | |||||||
u magnitude | 17.45 (0.02) | 17.42 (0.009) | 17.43 | ||||
g magnitude | 17.47 (0.01) | 17.45 (0.005) | 17.47 | ||||
r magnitude | 17.89 (0.01) | 17.87 (0.006) | 17.89 | ||||
i magnitude | 18.18 (0.01) | 18.17 (0.009) | 18.17 | ||||
z magnitude | 18.50 (0.03) | 18.47 (0.03) | 18.50 | ||||
G magnitude | 17.71 | ||||||
BP magnitude | 17.55 | ||||||
RP magnitude | 17.90 | ||||||
Pan g magnitude | 17.54 (0.005) | ||||||
Pan r magnitude | 17.88 (0.004) | ||||||
Pan i magnitude | 18.20 (0.006) | ||||||
Pan z magnitude | 18.47 (0.008) | ||||||
Pan y magnitude | 18.68 (0.03) |
* Constant surface field
Spectra without link are available upon request
The Montreal White Dwarf Database is produced and maintained by Prof. Patrick Dufour at Université de Montréal. Please send database updates, corrections, suggestions or bug reports to dufourpa@astro.umontreal.ca.