2MASS J08034287+4256525

All names: WISE J080342.85+425652.6, SDSS J080342.86+425652.6, SDSS J080342.85+425652.7, NPM1G +43.0108, SDSS J080342.87+425652.7, SDSS J080342.86+425652.7, 2MASS J08034287+4256525, 2MASX J08034286+4256530, TIC 39697596, WD 0800+430, Gaia DR2 922744762581250688, LEDA 2209603, WIRED J080342.86+425652.7, WISEA J080342.86+425652.3

Parameter Unit SDSS DR12 Gaia DR2 Simbad Eisenstein et al. 2006 White Dwarf Catalog (McCook & Sion 1999)
Right ascension 08 03 42.86 08 03 42.85 (17) 08 03 42.86 08 03 42.86 08 03 42.46
Declination 42 56 52.68 42 56 52.96 (11) 42 56 52.68 42 56 52.75 42 56 49.56
Spectral type D WD:+M WD: d
Effective temperature [K] 6300.0 (2)
log(g) [cgs] 8.97 (0.04)
Mass [M]
log(Luminosity) [L]
Cooling age [Gyr]
log(H/He)
log(C/He)
log(Ca/He)
log(Ca/H)
Parallax [mas]
Distance [pc]
Composition
Proper motion (right ascension) [mas/yr]
Proper motion (declination) [mas/yr]
Variability
Magnetic
Bd [MG]
Infrared excess (disk)
Binarity WDMS
B magnitude
V magnitude
R magnitude
I magnitude
J magnitude 13.82 (0.03)
H magnitude 13.14 (0.03)
K magnitude 12.83 (0.04)
u magnitude 18.58 (0.03) 18.57 (0.03) 20.17 (0.04) 20.17
g magnitude 16.89 (0.004) 16.89 (0.004) 18.25 (0.02) 18.25
r magnitude 15.97 (0.003) 15.97 (0.003) 17.25 (0.03) 17.25
i magnitude 15.30 (0.004) 15.30 (0.004) 16.29 (0.03) 16.29
z magnitude 14.72 (0.005) 14.72 (0.005) 15.54 (0.03) 15.54
G magnitude 18.71
BP magnitude
RP magnitude
Pan g magnitude
Pan r magnitude
Pan i magnitude
Pan z magnitude
Pan y magnitude
E(B-V)

* 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.