All names: LAMOST J161921.70+295506.0, SDSS J161921.70+295506.1, Gaia EDR3 1318236621192489216, SDSS J161921.70+295506.02, Gaia DR3 1318236621192489216, Gaia DR2 1318236621192489216, SDSS J161921.70+295506.0, SDSSJ161921.70+295506.1, LAMOST J161921.70+295506.1, GALEX J161921.7+295506
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | SDSS DR10 | Geier 2020 | Gaia DR2 | Stilism | Kepler et al. 2015 | Simbad | Eisenstein et al. 2006 |
|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 16 19 21.70 (0.04) | 16 19 21.70 | 16 19 21.70 | 16 19 21.70 | 16 19 21.70 (0.05) | 16 19 21.70 (0.04) | 16 19 21.70 | ||||
| Declination | 29 55 05.95 (0.05) | 29 55 06.13 | 29 55 06.13 | 29 55 06.10 | 29 55 05.96 (0.06) | 29 55 06.11 (0.05) | 29 55 06.11 | ||||
| Spectral type | sdB | DAO | sdO | SDO | |||||||
| Effective temperature | [K] | 34115.0 (933) | 34544.0 (118) | 33466.0 (267) | |||||||
| log(g) | [cgs] | 5.79 (0.1) | 5.69 (0.03) | 5.67 (0.05) | |||||||
| Mass | [M☉] | ||||||||||
| log(Luminosity) | [L☉] | ||||||||||
| Cooling age | [Gyr] | ||||||||||
| log(H/He) | |||||||||||
| log(C/He) | |||||||||||
| log(Ca/He) | |||||||||||
| log(Ca/H) | |||||||||||
| Parallax | [mas] | 0.37 (0.06) | 0.40 (0.07) | 0.40 (0.07) | 0.37 (0.06) | ||||||
| Distance | [pc] | 2683.34 (409) | 2485.71 (421) | 2485.42 (421) | 2683.12 (410) | ||||||
| Composition | |||||||||||
| Proper motion (right ascension) | [mas/yr] | 1.727989886 (0.06) | 1.61 (0.1) | 1.61042648 (0.1) | 1.728 (0.06) | -0.2 | |||||
| Proper motion (declination) | [mas/yr] | -9.518723632 (0.06) | -9.577 (0.1) | -9.577484311 (0.1) | -9.519 (0.06) | -8.5 | |||||
| Variability | |||||||||||
| Magnetic | |||||||||||
| Bd | [MG] | ||||||||||
| Infrared excess (disk) | |||||||||||
| Binarity | |||||||||||
| B magnitude | |||||||||||
| V magnitude | |||||||||||
| R magnitude | |||||||||||
| I magnitude | |||||||||||
| J magnitude | 17.52 (0.02) | ||||||||||
| H magnitude | 17.63 (0.06) | ||||||||||
| K magnitude | 17.80 (0.1) | ||||||||||
| u magnitude | 16.34 (0.006) | 16.34 (0.006) | 16.34 (0.006) | 16.36 (0.02) | 16.34 (0.006) | 16.35 (0.02) | |||||
| g magnitude | 16.59 (0.004) | 16.59 (0.004) | 16.59 (0.004) | 16.64 (0.02) | 16.59 (0.004) | 16.60 (0.02) | |||||
| r magnitude | 17.09 (0.005) | 17.09 (0.005) | 17.09 (0.005) | 17.10 (0.01) | 17.09 (0.005) | 17.11 (0.01) | |||||
| i magnitude | 17.43 (0.006) | 17.43 (0.006) | 17.43 (0.006) | 17.43 (0.01) | 17.43 (0.006) | 17.44 (0.02) | |||||
| z magnitude | 17.73 (0.02) | 17.73 (0.02) | 17.73 (0.02) | 17.74 (0.02) | 17.73 (0.02) | 17.73 (0.02) | |||||
| G magnitude | 16.84 (0.003) | 16.87 (0.001) | 16.87 | 16.84 (0.003) | |||||||
| BP magnitude | 16.71 (0.003) | 16.67 (0.009) | 16.67 | ||||||||
| RP magnitude | 17.13 (0.006) | 17.13 (0.007) | 17.13 | ||||||||
| Pan g magnitude | 16.67 (0.002) | 16.67 (0.002) | |||||||||
| Pan r magnitude | 17.10 (0.005) | 17.10 (0.005) | |||||||||
| Pan i magnitude | 17.45 (0.003) | 17.45 (0.003) | |||||||||
| Pan z magnitude | 17.71 (0.007) | 17.71 (0.007) | |||||||||
| Pan y magnitude | 17.90 (0.01) | 17.90 (0.01) | |||||||||
| E(B-V) | 0.025 | ||||||||||
* 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.