All names: SDSS J114732.09+235708.5, SDSS J114732.09+235708.54, Gaia DR2 4004206977952873344, Gaia DR3 4004206977952873344, Gaia EDR3 4004206977952873344
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Stilism | Kepler et al. 2016 | Simbad |
|---|---|---|---|---|---|---|---|
| Right ascension | 11 47 32.05 (0.8) | 11 47 32.09 | 11 47 32.10 (0.8) | ||||
| Declination | 23 57 08.18 (0.8) | 23 57 08.53 | 23 57 08.76 (0.8) | ||||
| Spectral type | sdA | sdA | |||||
| Effective temperature | [K] | 20873.0 (1455) | |||||
| log(g) | [cgs] | 5.58 (0.2) | |||||
| Mass | [M☉] | 0.177 (0.05) | |||||
| log(Luminosity) | [L☉] | ||||||
| Cooling age | [Gyr] | ||||||
| log(H/He) | |||||||
| log(C/He) | |||||||
| log(Ca/He) | |||||||
| log(Ca/H) | |||||||
| Parallax | [mas] | 1.59 (1) | 1.59 (1) | ||||
| Distance | [pc] | 630.87 (443) | 630.88 (443) | ||||
| Composition | |||||||
| Proper motion (right ascension) | [mas/yr] | -42.63719375 (0.9) | -42.637 (0.9) | ||||
| Proper motion (declination) | [mas/yr] | -36.33107541 (0.9) | -36.331 (0.9) | ||||
| Variability | |||||||
| Magnetic | |||||||
| Bd | [MG] | ||||||
| Infrared excess (disk) | |||||||
| Binarity | |||||||
| B magnitude | |||||||
| V magnitude | |||||||
| R magnitude | |||||||
| I magnitude | |||||||
| J magnitude | |||||||
| H magnitude | |||||||
| K magnitude | |||||||
| u magnitude | 21.28 (0.1) | 21.25 (0.09) | 21.25 (0.09) | ||||
| g magnitude | 20.49 (0.02) | 20.50 (0.03) | 20.50 (0.03) | ||||
| r magnitude | 20.48 (0.03) | 20.51 (0.03) | 20.51 (0.03) | ||||
| i magnitude | 20.53 (0.04) | 20.55 (0.04) | 20.55 (0.04) | ||||
| z magnitude | 20.39 (0.1) | 20.41 (0.1) | 20.41 (0.1) | ||||
| G magnitude | 20.46 (0.1) | 20.46 (0.01) | |||||
| BP magnitude | 20.40 (0.1) | ||||||
| RP magnitude | 20.55 (0.2) | ||||||
| Pan g magnitude | 20.55 (0.04) | ||||||
| Pan r magnitude | 20.49 (0.03) | ||||||
| Pan i magnitude | 20.54 (0.02) | ||||||
| Pan z magnitude | 20.63 (0.02) | ||||||
| Pan y magnitude | 20.39 (0.2) | ||||||
| E(B-V) | 0.019 | ||||||
* 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.