SBSS 1418+518

All names: Gaia EDR3 1604817278929750400, TIC 1001259992, SDSSJ142017.21+513904.1, Gaia DR3 1604817278929750400, SDSS J142017.21+513904.1, SBSS 1418+518, Gaia DR2 1604817278929750400

Parameter Unit Gaia EDR3 Pan-STARRS DR1 SDSS DR12 Geier 2020 Gaia DR2 Stilism Simbad Eisenstein et al. 2006
Right ascension 14 20 17.21 (0.1) 14 20 17.21 14 20 17.21 14 20 17.21 (0.2) 14 20 17.22 (0.1) 14 20 17.22
Declination 51 39 04.22 (0.1) 51 39 04.13 51 39 04.10 51 39 04.22 (0.2) 51 39 04.23 (0.1) 51 39 04.19
Spectral type sdO sdO SDO
Effective temperature [K] 82759.0 (8561)
log(g) [cgs] 5.12 (0.1)
Mass [M]
log(Luminosity) [L]
Cooling age [Gyr]
log(H/He)
log(C/He)
log(Ca/He)
log(Ca/H)
Parallax [mas] 0.20 (0.2) 0.08 (0.2) 0.08 (0.2) 0.20 (0.2)
Distance [pc] 5032.68 (4177) 13140.60 (39923) 13140.60 (39923) 5032.71 (4177)
Composition
Proper motion (right ascension) [mas/yr] -4.075789711 (0.2) -4.014 (0.3) -4.014 (0.3) -4.076 (0.2) -4.2
Proper motion (declination) [mas/yr] -0.483426282 (0.2) -0.712 (0.3) -0.712 (0.3) -0.483 (0.2) -2.3
Variability
Magnetic
Bd [MG]
Infrared excess (disk)
Binarity
B magnitude
V magnitude
R magnitude
I magnitude
J magnitude
H magnitude
K magnitude
u magnitude 18.24 (0.01) 18.24 (0.01) 18.24 (0.01) 18.23 (0.03)
g magnitude 18.64 (0.008) 18.64 (0.008) 18.64 (0.008) 18.63 (0.03)
r magnitude 19.14 (0.01) 19.14 (0.01) 19.14 (0.01) 19.16 (0.02)
i magnitude 19.51 (0.02) 19.51 (0.02) 19.51 (0.02) 19.54 (0.03)
z magnitude 19.95 (0.1) 19.95 (0.1) 20.00 (0.1) 19.98 (0.1)
G magnitude 18.92 (0.02) 18.99 (0.004) 18.99 18.92 (0.003)
BP magnitude 18.80 (0.02) 18.71 (0.02) 18.71
RP magnitude 19.25 (0.06) 19.28 (0.04) 19.28
Pan g magnitude 18.73 (0.0009) 18.73 (0.0009)
Pan r magnitude 19.17 (0.007) 19.17 (0.007)
Pan i magnitude 19.59 (0.02) 19.59 (0.02)
Pan z magnitude 19.84 (0.02) 19.84 (0.03)
Pan y magnitude 19.95 (0.09) 19.95 (0.09)
E(B-V) 0.019

* 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.