SDSS J170916.37+234111.3

All names: SDSS J170916.37+234111.3, Gaia DR3 4571743307909284992, Gaia EDR3 4571743307909284992, Gaia DR2 4571743307909284992, SDSS J170916.36+234111.3

Parameter Unit Gaia EDR3 Pan-STARRS DR1 SDSS DR12 Hardy et al. 2023a MWDD H Gaia DR2 Stilism Simbad Kleinman et al. 2013 Vincent et al. 2023
Right ascension 17 09 16.37 (0.3) 17 09 16.37 17 09 16.37 (0.4) 17 09 16.36 (0.3) 17 09 16.37
Declination 23 41 11.18 (0.3) 23 41 11.37 23 41 11.19 (0.5) 23 41 11.39 (0.3) 23 41 11.33
Spectral type DAH DAH DAH DAH DAH
Effective temperature [K] 13784.0 (817) 13453.0 17102.0 (998)
log(g) [cgs] 8.53 (0.2) 8.55 9.62 (0.2)
Mass [M] 0.9431738310881776 (0.3) 0.954
log(Luminosity) [L]
Cooling age [Gyr] 0.6453
log(H/He)
log(C/He)
log(Ca/He)
log(Ca/H)
log(C/H)
log(N/H)
log(O/H)
log(Na/H)
log(Mg/H)
log(Al/H)
log(Si/H)
log(P/H)
log(S/H)
log(Sc/H)
log(Ti/H)
log(Cr/H)
log(Mn/H)
log(Fe/H)
log(Ni/H)
Parallax [mas] 3.21 (0.5) 2.68 (0.7) 3.21 (0.5)
Distance [pc] 311.53 (47) 372.80 (94) 311.53 (47)
Composition H
Proper motion (right ascension) [mas/yr] 7.913902051 (0.4) 7.897906432 (0.9) 7.914 (0.4)
Proper motion (declination) [mas/yr] -12.98202716 (0.5) -12.59186006 (0.9) -12.982 (0.5)
Variability
Magnetic yes
Bd [MG] 12.066893221444351
Infrared excess (disk)
Binarity
B magnitude
V magnitude
R magnitude
I magnitude
J magnitude
H magnitude
K magnitude
u magnitude 20.61 (0.09) 20.61 (0.09) 20.55 (0.1)
g magnitude 20.28 (0.02) 20.28 (0.03) 20.29 (0.03)
r magnitude 20.35 (0.04) 20.35 (0.04) 20.34 (0.04)
i magnitude 20.64 (0.07) 20.64 (0.07) 20.62 (0.07)
z magnitude 20.87 (0.3) 20.87 (0.3) 20.86 (0.4)
G magnitude 20.29 (0.05) 20.35 20.29 (0.005)
BP magnitude 20.28 (0.05) 20.44
RP magnitude 20.17 (0.07) 20.05
Pan g magnitude 20.27 (0.009)
Pan r magnitude 20.34 (0.01)
Pan i magnitude 20.54 (0.03)
Pan z magnitude 20.81 (0.02)
Pan y magnitude
E(B-V) 0.027

* 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.