All names: Gaia EDR3 4463681655863346816, PM J16265+1355, LSPM J1626+1355, J1626+1355, WDJ162632.04+135554.52, TIC 149795667, 2MASS J16263203+1355547, USNO-B1.0 1039-00252184, WIRED J162632.08+135554.9, 16265+1355, PSO J246.6340+13.9322, Gaia DR2 4463681655863346816, SDSS J162632.08+135554.9, Gaia DR3 4463681655863346816, SDSS J162632.09+135554.9
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Kilic et al. 2025 | Caron et al. 2023 | Kilic et al. 2020 | Blouin et al. 2019 | MWDD H | Gaia DR2 | Stilism | Limoges et al. 2015 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | Kleinman et al. 2013 | Vincent et al. 2023 |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 16 26 32.19 (0.05) | 16 26 32.09 | 16 26 32.19 (0.06) | 16 26 32.19 | 16 26 32.04 (0.05) | 16 26 32.19 | 16 26 32.09 | ||||||||||
Declination | 13 55 56.05 (0.04) | 13 55 54.91 | 13 55 56.00 (0.04) | 13 55 56.05 | 13 55 54.51 (0.04) | 13 55 56.00 | 13 55 54.93 | ||||||||||
Spectral type | DA | DA | DA | DA | DA | DA | DA | DA | DA | DA | DA | ||||||
Effective temperature | [K] | 6808.0 (41) | 6576.0 (30) | 6808.0 (41) | 6785.0 (65) | 6815.0 | 6820.0 (101) | 6744.0 (39) | 6614.0 (29) | ||||||||
log(g) | [cgs] | 7.97 (0.01) | 7.86 (0.01) | 7.96 (0.01) | 7.97 (0.03) | 7.97 | 7.97 (0.09) | 7.94 (0.01) | 7.75 (0.06) | ||||||||
Mass | [M☉] | 0.573 (0.009) | 0.508 (0.008) | 0.57 (0.009) | 0.571 (0.01) | 0.572 | 0.57 (0.05) | 0.557 (0.01) | 0.473 (0.03) | ||||||||
log(Luminosity) | [L☉] | -3.48 | |||||||||||||||
Cooling age | [Gyr] | 1.5000 | 1.5600 (0.07) | 1.5460 | |||||||||||||
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] | 17.70 (0.07) | 17.66 (0.09) | 17.66 (0.09) | 17.66 (0.09) | 17.70 | 17.70 (0.07) | 17.66 (0.09) | |||||||||
Distance | [pc] | 56.48 (0.2) | 56.63 (0.3) | 56.62 (0.3) | 56.62 (0.3) | 56.90 (1) | 56.48 | 56.48 (0.2) | 56.62 (0.3) | ||||||||
Composition | H | H | H | H | H | ||||||||||||
Proper motion (right ascension) | [mas/yr] | 133.8757814 (0.06) | 133.7711394 (0.1) | 132.0 | 133.876 (0.06) | 133.771 | |||||||||||
Proper motion (declination) | [mas/yr] | 95.94234846 (0.05) | 95.77641178 (0.1) | 103.0 | 95.942 (0.05) | 95.776 | |||||||||||
Variability | |||||||||||||||||
Magnetic | |||||||||||||||||
Bd | [MG] | ||||||||||||||||
Infrared excess (disk) | |||||||||||||||||
Binarity | |||||||||||||||||
B magnitude | 18.40 | ||||||||||||||||
V magnitude | |||||||||||||||||
R magnitude | 17.10 | ||||||||||||||||
I magnitude | |||||||||||||||||
J magnitude | 16.54 (0.01) | 16.49 (0.1) | 16.49 | 16.49 (0.1) | |||||||||||||
H magnitude | 16.16 (0.2) | 16.16 (0.2) | 16.16 | 16.16 (0.2) | |||||||||||||
K magnitude | 15.85 (0.03) | 15.85 | 15.85 (0.1) | ||||||||||||||
u magnitude | 18.08 (0.01) | 18.08 (0.01) | 18.08 | 18.08 (0.01) | 18.08 (0.01) | 18.07 (0.02) | |||||||||||
g magnitude | 17.48 (0.005) | 17.48 | 17.45 (0.008) | 17.48 (0.005) | 17.51 (0.02) | ||||||||||||
r magnitude | 17.26 (0.005) | 17.26 | 17.28 (0.003) | 17.26 (0.005) | 17.27 (0.01) | ||||||||||||
i magnitude | 17.21 (0.006) | 17.21 | 17.23 (0.005) | 17.21 (0.006) | 17.20 (0.01) | ||||||||||||
z magnitude | 17.23 (0.01) | 17.24 | 17.25 (0.004) | 17.23 (0.01) | 17.25 (0.02) | ||||||||||||
G magnitude | 17.25 (0.005) | 17.27 | 17.25 | 17.25 (0.003) | 17.27 | ||||||||||||
BP magnitude | 17.47 (0.005) | 17.46 | 17.46 | ||||||||||||||
RP magnitude | 16.89 (0.005) | 16.89 | 16.89 | ||||||||||||||
Pan g magnitude | 17.45 (0.008) | 17.45 (0.008) | 17.45 (0.008) | ||||||||||||||
Pan r magnitude | 17.28 (0.004) | 17.28 (0.003) | 17.28 (0.003) | ||||||||||||||
Pan i magnitude | 17.23 (0.004) | 17.23 (0.005) | 17.23 (0.005) | ||||||||||||||
Pan z magnitude | 17.25 (0.006) | 17.25 (0.004) | 17.25 (0.004) | ||||||||||||||
Pan y magnitude | 17.28 (0.01) | 17.28 (0.01) | 17.28 (0.01) | ||||||||||||||
E(B-V) | 0.003 |
* 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.