All names: GALEX J183517.8+642116, USNO-B1.0 1543-00212587, 2MASS J18351820+6421180, Gaia DR2 2256410856215182464, Gaia DR3 2256410856215182464, SDSS J183518.10+642118.4, LSPM J1835+6421, TIC 383647463, Gaia EDR3 2256410856215182464, SDSS J183518.11+642118.5, J1835+6421, WDJ183518.23+642117.68
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Kilic et al. 2025 | O'Brien et al. 2024 | Caron et al. 2023 | McCleery et al. 2020 | Tremblay et al. 2020 | MWDD H | MWDD HE | Gaia DR2 | Stilism | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 18 35 17.90 (0.06) | 18 35 17.91 (0.07) | 18 35 17.91 | 18 35 17.90 | 18 35 18.23 (0.06) | 18 35 17.91 | |||||||||
| Declination | 64 21 19.51 (0.06) | 64 21 19.45 (0.07) | 64 21 19.45 | 64 21 19.51 | 64 21 17.69 (0.06) | 64 21 19.45 | |||||||||
| Spectral type | DC | DC | DC | DC | DC | DC: | DC | ||||||||
| Effective temperature | [K] | 4833.0 (19) | 4908.0 (62) | 4841.0 (18) | 4857.5 (31) | 4860.0 (30) | 4869.0 | 4551.0 | 4948.0 (30) | ||||||
| log(g) | [cgs] | 7.97 (0.009) | 8.01 (0.05) | 7.97 (0.01) | 7.99 (0.03) | 7.99 (0.04) | 7.99 | 7.77 | 8.04 (0.01) | ||||||
| Mass | [M☉] | 0.559 (0.007) | 0.583 (0.03) | 0.562 (0.008) | 0.575 | 0.438 | 0.603 (0.01) | ||||||||
| log(Luminosity) | [L☉] | ||||||||||||||
| Cooling age | [Gyr] | 6.3800 | 6.2060 | 4.5910 | |||||||||||
| 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] | 33.09 (0.06) | 33.09 (0.06) | 33.12 (0.07) | 33.12 (0.07) | 33.12 (0.07) | 33.09 | 33.09 (0.06) | 33.12 (0.07) | ||||||
| Distance | [pc] | 30.22 (0.05) | 30.22 (0.05) | 30.19 (0.06) | 30.19 (0.06) | 30.19 (0.06) | 30.22 | 30.22 (0.05) | 30.19 (0.06) | ||||||
| Composition | H | H | |||||||||||||
| Proper motion (right ascension) | [mas/yr] | -134.0321892 (0.09) | -134.2720692 (0.2) | -134.032 (0.09) | -134.2720692 | ||||||||||
| Proper motion (declination) | [mas/yr] | 113.8913497 (0.08) | 114.0350867 (0.2) | 113.891 (0.08) | 114.0350867 | ||||||||||
| Variability | |||||||||||||||
| Magnetic | |||||||||||||||
| Bd | [MG] | ||||||||||||||
| Infrared excess (disk) | |||||||||||||||
| Binarity | |||||||||||||||
| B magnitude | 18.20 | ||||||||||||||
| V magnitude | |||||||||||||||
| R magnitude | 17.40 | ||||||||||||||
| I magnitude | |||||||||||||||
| J magnitude | 15.94 (0.09) | 15.94 (0.09) | |||||||||||||
| H magnitude | 15.59 (0.2) | 15.59 (0.2) | |||||||||||||
| K magnitude | |||||||||||||||
| u magnitude | 19.85 (0.04) | 19.88 (0.04) | 19.88 (0.04) | ||||||||||||
| g magnitude | 18.10 (0.006) | 18.10 (0.006) | |||||||||||||
| r magnitude | 17.33 (0.005) | 17.33 (0.005) | |||||||||||||
| i magnitude | 17.07 (0.006) | 17.07 (0.006) | |||||||||||||
| z magnitude | 16.95 (0.01) | 16.95 (0.01) | |||||||||||||
| G magnitude | 17.38 (0.01) | 17.39 | 17.39 | 17.38 | 17.38 (0.003) | 17.39 | |||||||||
| BP magnitude | 17.87 (0.01) | 17.89 | 17.89 | ||||||||||||
| RP magnitude | 16.73 (0.009) | 16.74 | 16.74 | ||||||||||||
| Pan g magnitude | 18.01 (0.008) | 18.01 (0.008) | |||||||||||||
| Pan r magnitude | 17.35 (0.003) | 17.35 (0.003) | |||||||||||||
| Pan i magnitude | 17.07 (0.003) | 17.07 (0.003) | |||||||||||||
| Pan z magnitude | 16.97 (0.004) | 16.97 (0.005) | |||||||||||||
| Pan y magnitude | 16.94 (0.01) | 16.94 (0.01) | |||||||||||||
| E(B-V) | 0.002 | ||||||||||||||
* 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.