All names: Gaia DR3 3808536101967194368, Gaia EDR3 3808536101967194368, J1102+0214, WDJ110234.22+021459.26, Gaia DR2 3808536101967194368, SDSS J110234.21+021459.2
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR14 | Kilic et al. 2025 | Caron et al. 2023 | Blouin 2020 | Coutu et al. 2019 | Gaia DR2 | Hollands et al. 2017 | Stilism | Simbad | Gentile Fusillo et al. 2018 | Vincent et al. 2023 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 11 02 34.13 (0.3) | 11 02 34.21 | 11 02 34.21 | 11 02 34.13 (0.4) | 11 02 34.22 (0.3) | 11 02 34.13 | ||||||||
| Declination | 02 14 59.54 (0.3) | 02 14 59.23 | 02 14 59.23 | 02 14 59.54 (0.4) | 02 14 59.26 (0.3) | 02 14 59.54 | ||||||||
| Spectral type | DZ | DZ | DZ | DZ | DZ | DZ | DZ | |||||||
| Effective temperature | [K] | 5729.0 (42) | 5675.0 (46) | 5699.0 (157) | 5699.0 (58) | 5730.0 (90) | ||||||||
| log(g) | [cgs] | 8.18 (0.05) | 8.14 (0.06) | 8.14 (0.08) | 8.14 | |||||||||
| Mass | [M☉] | 0.682 (0.04) | 0.656 (0.05) | 0.658 (0.05) | 0.661 | |||||||||
| log(Luminosity) | [L☉] | |||||||||||||
| Cooling age | [Gyr] | 4.7100 | 4.5100 | 3.9000 | ||||||||||
| log(H/He) | -4.0 | -4.0 | <-3.0 | |||||||||||
| log(C/He) | ||||||||||||||
| log(Ca/He) | -9.81 | -9.77 | -9.8 (0.1) | -9.7775 (0.1) | -9.75 | |||||||||
| log(Ca/H) | ||||||||||||||
| log(N/He) | ||||||||||||||
| log(O/He) | ||||||||||||||
| log(Na/He) | ||||||||||||||
| log(Mg/He) | -8.0 (0.5) | -8.84 | ||||||||||||
| log(Al/He) | ||||||||||||||
| log(Si/He) | ||||||||||||||
| log(P/He) | ||||||||||||||
| log(S/He) | ||||||||||||||
| log(Cl/He) | ||||||||||||||
| log(Sc/He) | ||||||||||||||
| log(Ti/He) | ||||||||||||||
| log(V/He) | ||||||||||||||
| log(Cr/He) | ||||||||||||||
| log(Mn/He) | ||||||||||||||
| log(Fe/He) | -8.6 (0.4) | -8.74 | ||||||||||||
| log(Co/He) | ||||||||||||||
| log(Ni/He) | ||||||||||||||
| log(Cu/He) | ||||||||||||||
| log(Zn/He) | ||||||||||||||
| log(Ga/He) | ||||||||||||||
| log(Ge/He) | ||||||||||||||
| log(Sr/He) | ||||||||||||||
| Parallax | [mas] | 10.46 (0.5) | 10.36 (0.5) | 10.36 | 10.36 (0.5) | 10.46 (0.5) | 10.36 (0.5) | |||||||
| Distance | [pc] | 95.57 (4) | 96.53 (5) | 96.69 (5) | 96.54 (5) | 96.54 (5) | 101.00 (13) | 95.57 (4) | 96.54 (5) | |||||
| Composition | He | He | He | He | ||||||||||
| Proper motion (right ascension) | [mas/yr] | -86.18544783 (0.4) | -85.90421423 (0.9) | -86.185 (0.4) | -85.90421423 | |||||||||
| Proper motion (declination) | [mas/yr] | 18.01578821 (0.3) | 17.4536269 (0.6) | 18.016 (0.3) | 17.4536269 | |||||||||
| Variability | ||||||||||||||
| Magnetic | ||||||||||||||
| Bd | [MG] | |||||||||||||
| Infrared excess (disk) | ||||||||||||||
| Binarity | ||||||||||||||
| B magnitude | ||||||||||||||
| V magnitude | ||||||||||||||
| R magnitude | ||||||||||||||
| I magnitude | ||||||||||||||
| J magnitude | 18.47 (0.07) | |||||||||||||
| H magnitude | 18.52 (0.07) | |||||||||||||
| K magnitude | 18.39 (0.1) | |||||||||||||
| u magnitude | 21.24 (0.09) | 21.38 (0.1) | 21.22 (0.08) | 21.22 (0.08) | 21.24 (0.09) | 21.24 (0.09) | ||||||||
| g magnitude | 19.51 (0.01) | 19.52 (0.02) | 19.52 (0.02) | 19.51 (0.01) | 19.51 (0.01) | |||||||||
| r magnitude | 19.18 (0.01) | 19.20 (0.02) | 19.20 (0.02) | 19.18 (0.01) | 19.18 (0.01) | |||||||||
| i magnitude | 19.17 (0.02) | 19.16 (0.02) | 19.16 (0.02) | 19.16 (0.02) | 19.16 (0.02) | |||||||||
| z magnitude | 19.29 (0.06) | 19.30 (0.06) | 19.30 (0.06) | 19.29 (0.06) | 19.29 (0.06) | |||||||||
| G magnitude | 19.23 (0.04) | 19.26 | 19.23 (0.005) | 19.26 | ||||||||||
| BP magnitude | 19.51 (0.04) | 19.42 | 19.42 | |||||||||||
| RP magnitude | 18.87 (0.06) | 18.76 | 18.76 | |||||||||||
| Pan g magnitude | 19.44 (0.01) | 19.44 (0.008) | ||||||||||||
| Pan r magnitude | 19.19 (0.01) | 19.19 (0.01) | ||||||||||||
| Pan i magnitude | 19.16 (0.009) | 19.16 (0.008) | ||||||||||||
| Pan z magnitude | 19.23 (0.02) | 19.23 (0.02) | ||||||||||||
| Pan y magnitude | 19.32 (0.06) | 19.32 (0.05) | ||||||||||||
| E(B-V) | 0.005 | |||||||||||||
* 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.