All names: SDSS J162351.64+403211.3, Gaia DR2 1380934790002105088, SDSS J162351.60+403211.4, WIRED J162351.64+403211.3, SDSS J162351.63+403211.3, Gaia EDR3 1380934790002105088, SDSS J162351.64+403211.4, PTF1 J162351.64+403211.3, Gaia DR3 1380934790002105088, SDSS J162351.64+403211.2, GALEX J162351.6+403211, WD 1622+406
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Bedard et al. 2020 | MWDD H | Gaia DR2 | Stilism | sdss-wdms.org (29/04/2016) | Tremblay et al. 2011 | Vincent et al. 2024 | Simbad | Eisenstein et al. 2006 | White Dwarf Catalog (McCook & Sion 1999) | Kleinman et al. 2013 | Vincent et al. 2023 |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 16 23 51.63 (0.07) | 16 23 51.64 | 16 23 51.63 (0.1) | 16 23 51.64 | 16 23 51.63 | 16 23 51.64 (0.07) | 16 23 51.64 | 16 23 51.58 | 16 23 51.64 | |||||||
Declination | 40 32 11.26 (0.08) | 40 32 11.39 | 40 32 11.26 (0.1) | 40 32 11.29 | 40 32 11.26 | 40 32 11.40 (0.08) | 40 32 11.40 | 40 32 08.52 | 40 32 11.40 | |||||||
Spectral type | DA | DA+M | DA+M | DA | DA | DA+dM | DA+M | DA d | DA+M | DA+MS | ||||||
Effective temperature | [K] | 43739.0 (1523) | 14036.0 | 44479.0 (1567) | 45150.0 (1430) | 26234.0 (1219) | 46884.0 (1134) | 44327.0 (975) | ||||||||
log(g) | [cgs] | 7.71 (0.1) | 6.18 | 7.91 (0.1) | 7.84 (0.1) | 7.16 (0.07) | 7.97 (0.1) | 7.87 (0.09) | ||||||||
Mass | [M☉] | 0.54 (0.06) | 0.123 | 0.64 (0.07) | 0.61 (0.06) | 0.328 (0.02) | ||||||||||
log(Luminosity) | [L☉] | -0.02 (0.1) | ||||||||||||||
Cooling age | [Gyr] | 0.0028 (0.0006) | 0.0030 | |||||||||||||
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] | 1.67 (0.09) | 1.36 (0.1) | 1.67 | 1.67 (0.09) | |||||||||||
Distance | [pc] | 598.82 (33) | 734.21 (67) | 598.82 | 598.84 (33) | |||||||||||
Composition | H | H | H | |||||||||||||
Proper motion (right ascension) | [mas/yr] | -5.396314361 (0.09) | -5.748188719 (0.2) | -5.396 (0.09) | 2.0 | |||||||||||
Proper motion (declination) | [mas/yr] | -9.134461018 (0.1) | -8.971931998 (0.3) | -9.134 (0.1) | -10.3 | |||||||||||
Variability | ||||||||||||||||
Magnetic | ||||||||||||||||
Bd | [MG] | |||||||||||||||
Infrared excess (disk) | ||||||||||||||||
Binarity | WDMS | WDMS | WDMS | WDMS | ||||||||||||
B magnitude | ||||||||||||||||
V magnitude | ||||||||||||||||
R magnitude | ||||||||||||||||
I magnitude | ||||||||||||||||
J magnitude | ||||||||||||||||
H magnitude | ||||||||||||||||
K magnitude | ||||||||||||||||
u magnitude | 17.32 (0.01) | 17.30 | 17.32 (0.01) | 17.30 (0.02) | 17.30 | 17.33 (0.02) | ||||||||||
g magnitude | 17.72 (0.006) | 17.74 | 17.72 (0.006) | 17.74 (0.02) | 17.74 | 17.74 (0.02) | ||||||||||
r magnitude | 18.17 (0.007) | 18.18 | 18.17 (0.007) | 18.18 (0.02) | 18.18 | 18.18 (0.02) | ||||||||||
i magnitude | 18.33 (0.009) | 18.33 | 18.33 (0.009) | 18.33 (0.02) | 18.33 | 18.33 (0.02) | ||||||||||
z magnitude | 18.35 (0.03) | 18.31 | 18.34 (0.03) | 18.31 (0.03) | 18.31 | 18.32 (0.03) | ||||||||||
G magnitude | 17.92 (0.01) | 17.95 | 17.92 | 17.92 (0.003) | ||||||||||||
BP magnitude | 17.84 (0.01) | 17.75 | ||||||||||||||
RP magnitude | 18.01 (0.02) | 18.02 | ||||||||||||||
Pan g magnitude | 17.80 (0.008) | |||||||||||||||
Pan r magnitude | 18.21 (0.008) | |||||||||||||||
Pan i magnitude | 18.37 (0.01) | |||||||||||||||
Pan z magnitude | 18.39 (0.01) | |||||||||||||||
Pan y magnitude | 18.35 (0.02) | |||||||||||||||
E(B-V) | 0.018 |
* Constant surface field
Spectra without link are available upon request
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.