PHL 844

All names: SDSS J004840.88-011547.4, GALEX J004840.8-011547, Gaia EDR3 2530654516748362112, Gaia DR3 2530654516748362112, PHL 844, USNO-B1.0 0887-00008242, SDSSJ004840.88-011547.4, Gaia DR2 2530654516748362112, SDSS J004840.88-011547.5

Parameter Unit Gaia EDR3 Pan-STARRS DR1 Geier 2020 Gaia DR2 Stilism Simbad Eisenstein et al. 2006
Right ascension 00 48 40.89 (0.2) 00 48 40.88 00 48 40.89 (0.2) 00 48 40.88 (0.2) 00 48 40.89
Declination -01 15 47.51 (0.09) -01 15 47.40 -01 15 47.51 (0.2) -01 15 47.45 (0.09) -01 15 47.43
Spectral type sdB sdB SDB:
Effective temperature [K] 12233.0 (336)
log(g) [cgs] 8.72 (0.3)
Mass [M]
log(Luminosity) [L]
Cooling age [Gyr]
log(H/He)
log(C/He)
log(Ca/He)
log(Ca/H)
Parallax [mas] 0.23 (0.2) 0.10 (0.3) 0.10 (0.3) 0.23 (0.2)
Distance [pc] 4325.49 (3607) 10460.25 (29904) 10460.25 (29904) 4325.26 (3607)
Composition
Proper motion (right ascension) [mas/yr] 6.817692122 (0.3) 6.813 (0.5) 6.813 (0.5) 6.818 (0.3)
Proper motion (declination) [mas/yr] -3.447620735 (0.2) -3.398 (0.3) -3.398 (0.3) -3.448 (0.2)
Variability
Magnetic
Bd [MG]
Infrared excess (disk)
Binarity
B magnitude 18.10
V magnitude 18.80
R magnitude 18.80
I magnitude
J magnitude
H magnitude
K magnitude
u magnitude 18.31 (0.02) 18.31 (0.02) 18.31 (0.03)
g magnitude 18.33 (0.007) 18.33 (0.007) 18.39 (0.02)
r magnitude 18.53 (0.009) 18.53 (0.009) 18.55 (0.02)
i magnitude 18.62 (0.01) 18.62 (0.01) 18.66 (0.02)
z magnitude 18.68 (0.04) 18.68 (0.04) 18.78 (0.05)
G magnitude 18.39 (0.01) 18.42 (0.002) 18.42 18.39 (0.003)
BP magnitude 18.41 (0.01) 18.38 (0.01) 18.38
RP magnitude 18.34 (0.02) 18.30 (0.03) 18.30
Pan g magnitude 18.39 (0.009) 18.39 (0.009)
Pan r magnitude 18.53 (0.01) 18.53 (0.01)
Pan i magnitude 18.64 (0.006) 18.64 (0.006)
Pan z magnitude 18.74 (0.006) 18.74 (0.006)
Pan y magnitude 18.78 (0.02) 18.78 (0.02)
E(B-V) 0.025

* 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.