SBSS 1610+558

All names: Gaia DR2 1429687032498740992, Gaia EDR3 1429687032498740992, Gaia DR3 1429687032498740992, SDSSJ161143.29+554044.39, SDSS J161143.29+554044.39, SDSS J161143.29+554044.3, SBSS 1610+558, SDSS J161143.29+554044.4

Parameter Unit Gaia EDR3 Pan-STARRS DR1 SDSS DR12 Geier 2020 Gaia DR2 Stilism Kepler et al. 2016 Simbad
Right ascension 16 11 43.30 (0.09) 16 11 43.29 16 11 43.29 16 11 43.30 (0.1) 16 11 43.30 (0.09)
Declination 55 40 44.37 (0.09) 55 40 44.40 55 40 44.39 55 40 44.37 (0.1) 55 40 44.39 (0.09)
Spectral type He-sdO sdO sdO
Effective temperature [K] 58588.0 (1940)
log(g) [cgs] 5.71 (0.1)
Mass [M]
log(Luminosity) [L]
Cooling age [Gyr]
log(H/He)
log(C/He)
log(Ca/He)
log(Ca/H)
Parallax [mas] 0.13 (0.09) 0.07 (0.1) 0.07 (0.1) 0.13 (0.09)
Distance [pc] 7694.27 (5514) 13755.16 (23026) 13747.17 (23002) 7692.31 (5509)
Composition
Proper motion (right ascension) [mas/yr] -0.064561332 (0.1) 0.176 (0.2) 0.17626276 (0.2) -0.065 (0.1)
Proper motion (declination) [mas/yr] -0.893432683 (0.1) -0.68 (0.2) -0.680463675 (0.2) -0.893 (0.1)
Variability
Magnetic
Bd [MG]
Infrared excess (disk)
Binarity
B magnitude 18.00
V magnitude
R magnitude
I magnitude
J magnitude
H magnitude
K magnitude
u magnitude 17.49 (0.01) 17.49 (0.01) 17.50 (0.02) 17.50 (0.02)
g magnitude 17.93 (0.006) 17.93 (0.006) 17.95 (0.02) 17.95 (0.02)
r magnitude 18.47 (0.009) 18.48 (0.009) 18.49 (0.02) 18.49 (0.02)
i magnitude 18.85 (0.01) 18.86 (0.01) 18.87 (0.02) 18.87 (0.02)
z magnitude 19.21 (0.08) 19.23 (0.08) 19.22 (0.08) 19.22 (0.08)
G magnitude 18.21 (0.009) 18.25 (0.002) 18.25 18.21 (0.003)
BP magnitude 18.07 (0.009) 17.97 (0.01) 17.97
RP magnitude 18.62 (0.03) 18.56 (0.03) 18.56
Pan g magnitude 18.03 (0.01) 18.03 (0.01)
Pan r magnitude 18.48 (0.009) 18.48 (0.009)
Pan i magnitude 18.88 (0.005) 18.88 (0.005)
Pan z magnitude 19.18 (0.009) 19.18 (0.009)
Pan y magnitude 19.34 (0.05) 19.34 (0.05)
E(B-V) 0.021

* 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.