SDSS J081531.20+245222.6

All names: Gaia DR3 682305655764689408, GALEX J081531.1+245223, SDSSJ081531.20+245222.6, SDSS J081531.20+245222.6, LAMOST J081531.20+245222.6, Gaia EDR3 682305655764689408, Gaia DR2 682305655764689408, SDSS J081531.20+245222.62

Parameter Unit Gaia EDR3 Pan-STARRS DR1 SDSS DR10 Geier 2020 Gaia DR2 Stilism Kepler et al. 2015 Simbad
Right ascension 08 15 31.21 (0.06) 08 15 31.21 08 15 31.20 08 15 31.21 (0.09) 08 15 31.21 (0.06)
Declination 24 52 22.62 (0.04) 24 52 22.64 24 52 22.60 24 52 22.62 (0.05) 24 52 22.63 (0.04)
Spectral type sdOB A/DAZ sdB
Effective temperature [K] 35360.0 (670) 33180.0 (109)
log(g) [cgs] 5.55 (0.1) 5.00 (0.01)
Mass [M]
log(Luminosity) [L]
Cooling age [Gyr]
log(H/He)
log(C/He)
log(Ca/He)
log(Ca/H)
Parallax [mas] 0.45 (0.07) 0.35 (0.1) 0.35 (0.1) 0.45 (0.07)
Distance [pc] 2240.08 (338) 2831.26 (875) 2831.57 (875) 2240.14 (338)
Composition
Proper motion (right ascension) [mas/yr] -0.610741496 (0.07) -0.915 (0.2) -0.914591978 (0.2) -0.611 (0.07)
Proper motion (declination) [mas/yr] -0.343237907 (0.04) -0.167 (0.1) -0.166536262 (0.1) -0.343 (0.04)
Variability
Magnetic
Bd [MG]
Infrared excess (disk)
Binarity
B magnitude
V magnitude
R magnitude
I magnitude
J magnitude 16.96 (0.2) 16.98 (0.01)
H magnitude 16.66 (0.2) 17.09 (0.05)
K magnitude 16.32 17.23 (0.09)
u magnitude 15.77 (0.004) 15.77 (0.004) 15.82 (0.02) 15.77 (0.004)
g magnitude 16.06 (0.003) 16.06 (0.003) 16.09 (0.02) 16.06 (0.003)
r magnitude 16.56 (0.004) 16.56 (0.004) 16.58 (0.02) 16.56 (0.004)
i magnitude 16.91 (0.005) 16.91 (0.005) 16.91 (0.02) 16.91 (0.005)
z magnitude 17.23 (0.01) 17.23 (0.01) 17.24 (0.02) 17.23 (0.01)
G magnitude 16.33 (0.003) 16.36 (0.002) 16.36 16.33 (0.003)
BP magnitude 16.18 (0.003) 16.11 (0.01) 16.11
RP magnitude 16.62 (0.007) 16.60 (0.007) 16.60
Pan g magnitude 16.13 (0.004) 16.13 (0.004)
Pan r magnitude 16.58 (0.003) 16.58 (0.003)
Pan i magnitude 16.95 (0.004) 16.95 (0.004)
Pan z magnitude 17.22 (0.005) 17.22 (0.005)
Pan y magnitude 17.40 (0.009) 17.40 (0.009)
E(B-V) 0.033

* Constant surface field

Special notes:

Spectra

Controls

Normalize at:
Normalize by mean flux

Range:

x: to
y: to

Spectra available:

Spectra without link are available upon request

Absorption lines

Photometric filters

BVRI
ugriz

Photometric fit





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.