SDSS J145815.90+370017.4

All names: SDSS J145815.90+370017.4, SDSSJ145815.90+370017.4, SDSS J145815.90+370017.5, GALEX J145815.9+370016, LAMOST J145815.93+370016.9, Gaia EDR3 1295107633891682944, Gaia DR3 1295107633891682944, Gaia DR2 1295107633891682944, SDSS J145815.90+370017.50

Parameter Unit Gaia EDR3 Pan-STARRS DR1 SDSS DR10 Geier 2020 Gaia DR2 Stilism Kepler et al. 2015 Simbad
Right ascension 14 58 15.90 (0.05) 14 58 15.91 14 58 15.90 14 58 15.90 (0.05) 14 58 15.91 (0.05)
Declination 37 00 17.44 (0.06) 37 00 17.44 37 00 17.40 37 00 17.44 (0.06) 37 00 17.42 (0.06)
Spectral type He-sdO He-sdO sdOHe
Effective temperature [K] 49610.0 (600) 50000.0 (5000)
log(g) [cgs] 6.04 (0.1) 6.50 (0.5)
Mass [M]
log(Luminosity) [L]
Cooling age [Gyr]
log(H/He)
log(C/He)
log(Ca/He)
log(Ca/H)
Parallax [mas] 0.15 (0.07) 0.03 (0.08) 0.03 (0.08) 0.15 (0.07)
Distance [pc] 6765.79 (3288) 33557.05 (91437) 33553.79 (91387) 6765.90 (3287)
Composition
Proper motion (right ascension) [mas/yr] -12.02115161 (0.06) -11.952 (0.1) -11.95217478 (0.1) -12.021 (0.06)
Proper motion (declination) [mas/yr] 1.791943599 (0.08) 1.772 (0.1) 1.772282943 (0.1) 1.792 (0.08)
Variability
Magnetic
Bd [MG]
Infrared excess (disk)
Binarity
B magnitude
V magnitude
R magnitude
I magnitude
J magnitude
H magnitude
K magnitude
u magnitude 16.56 (0.006) 16.56 (0.006) 16.58 (0.02) 16.56 (0.006)
g magnitude 16.96 (0.004) 16.96 (0.004) 17.00 (0.01) 16.96 (0.004)
r magnitude 17.52 (0.005) 17.52 (0.005) 17.52 (0.01) 17.52 (0.005)
i magnitude 17.87 (0.007) 17.87 (0.007) 17.87 (0.02) 17.87 (0.007)
z magnitude 18.25 (0.02) 18.25 (0.02) 18.25 (0.03) 18.25 (0.02)
G magnitude 17.26 (0.005) 17.30 (0.002) 17.30 17.26 (0.003)
BP magnitude 17.11 (0.005) 17.01 (0.01) 17.01
RP magnitude 17.60 (0.01) 17.57 (0.009) 17.57
Pan g magnitude 17.10 (0.007) 17.10 (0.007)
Pan r magnitude 17.54 (0.003) 17.54 (0.003)
Pan i magnitude 17.91 (0.004) 17.91 (0.004)
Pan z magnitude 18.22 (0.01) 18.22 (0.01)
Pan y magnitude 18.41 (0.02) 18.41 (0.02)
E(B-V) 0.023

* 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.