SDSS J084825.62+015013.9
All names: Gaia DR3 3075901233451525888, Gaia EDR3 3075901233451525888, SDSS J084825.62+015013.9, Gaia DR2 3075901233451525888, SDSS J084825.62+015014.0, SDSS J084825.62+015013.99
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | SDSS DR10 | MWDD H | MWDD HE | Gaia DR2 | Stilism | sdss-wdms.org (29/04/2016) | Kepler et al. 2015 | Simbad | Vincent et al. 2023 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 08 48 25.61 (0.3) | 08 48 25.62 | 08 48 25.62 | 08 48 25.62 (0.5) | 08 48 25.62 | 08 48 25.62 (0.3) | |||||||
| Declination | 01 50 13.74 (0.2) | 01 50 13.97 | 01 50 13.97 | 01 50 13.75 (0.4) | 01 50 13.98 | 01 50 14.00 (0.2) | |||||||
| Spectral type | WD+MS | WD+MS | WD+MS | DA | DA+dM | DA+MS | |||||||
| Effective temperature | [K] | 5782.0 | 5565.0 | 16994.0 (794) | 8394.0 (94) | ||||||||
| log(g) | [cgs] | 6.97 | 6.66 | 7.52 (0.2) | 7.53 (0.1) | ||||||||
| Mass | [M☉] | 0.178 | 0.095 | 0.475 (0.1) | 0.391 (0.05) | ||||||||
| log(Luminosity) | [L☉] | ||||||||||||
| Cooling age | [Gyr] | ||||||||||||
| log(H/He) | |||||||||||||
| log(C/He) | |||||||||||||
| log(Ca/He) | |||||||||||||
| log(Ca/H) | |||||||||||||
| Parallax | [mas] | 3.83 (0.4) | 4.20 (0.6) | 3.83 (0.4) | |||||||||
| Distance | [pc] | 261.20 (28) | 238.00 (34) | 1335.00 (196) | 261.20 (28) | ||||||||
| Composition | |||||||||||||
| Proper motion (right ascension) | [mas/yr] | -9.585416809 (0.4) | -10.86711159 (1) | -9.585 (0.4) | |||||||||
| Proper motion (declination) | [mas/yr] | -16.23595663 (0.3) | -16.27220857 (0.7) | -16.236 (0.3) | |||||||||
| Variability | |||||||||||||
| Magnetic | |||||||||||||
| Bd | [MG] | ||||||||||||
| Infrared excess (disk) | |||||||||||||
| Binarity | WDMS | WDMS | |||||||||||
| B magnitude | |||||||||||||
| V magnitude | |||||||||||||
| R magnitude | |||||||||||||
| I magnitude | |||||||||||||
| J magnitude | |||||||||||||
| H magnitude | |||||||||||||
| K magnitude | |||||||||||||
| u magnitude | 20.51 (0.05) | 20.51 (0.05) | 20.50 | 20.50 (0.05) | 20.51 (0.05) | ||||||||
| g magnitude | 19.99 (0.02) | 19.99 (0.02) | 19.99 | 19.99 (0.02) | 19.99 (0.02) | ||||||||
| r magnitude | 19.95 (0.02) | 19.95 (0.02) | 19.96 | 19.96 (0.03) | 19.95 (0.02) | ||||||||
| i magnitude | 19.83 (0.03) | 19.83 (0.03) | 19.83 | 19.83 (0.03) | 19.83 (0.03) | ||||||||
| z magnitude | 19.18 (0.06) | 19.18 (0.06) | 19.17 | 19.17 (0.06) | 19.18 (0.06) | ||||||||
| G magnitude | 19.80 (0.04) | 19.84 | 19.80 (0.004) | ||||||||||
| BP magnitude | 20.02 (0.04) | 20.01 | |||||||||||
| RP magnitude | 19.37 (0.04) | 19.27 | |||||||||||
| Pan g magnitude | 20.01 (0.02) | ||||||||||||
| Pan r magnitude | 19.97 (0.02) | ||||||||||||
| Pan i magnitude | 19.78 (0.01) | ||||||||||||
| Pan z magnitude | 19.38 (0.02) | ||||||||||||
| Pan y magnitude | 18.98 (0.05) | ||||||||||||
| E(B-V) | 0.020 | ||||||||||||
* Constant surface field
Special notes:
Spectra
Controls
Normalize at:
Normalize by mean flux
Range:
x:
to
y:
to
Spectra available:
Spectra without link are available upon request
Absorption lines
Photometric filters
BVRI
ugriz
Photometric fit
