WD 0053-090
All names: Gaia EDR3 2474288985158936960, 2MASS J00554779-0845069, SDSS J005547.78-084507.3, SDSS J005547.77-084507.2, GALEX J005547.7-084507, SDSS J005547.78-084507.2, WD 0053-090, Gaia DR3 2474288985158936960, Gaia DR2 2474288985158936960, TIC 408015814
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Bedard et al. 2020 | MWDD H | Gaia DR2 | Stilism | Tremblay et al. 2011 | Vincent et al. 2024 | Simbad | Eisenstein et al. 2006 | White Dwarf Catalog (McCook & Sion 1999) | Kleinman et al. 2013 | Kleinman et al. 2004 | Vincent et al. 2023 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 00 55 47.79 (0.06) | 00 55 47.78 | 00 55 47.79 (0.07) | 00 55 47.79 | 00 55 47.78 (0.06) | 00 55 47.78 | 00 55 46.30 | 00 55 47.78 | 00 55 47.78 | |||||||
| Declination | -08 45 08.20 (0.03) | -08 45 07.24 | -08 45 08.17 (0.06) | -08 45 08.20 | -08 45 07.23 (0.03) | -08 45 07.24 | -08 45 03.96 | -08 45 07.29 | -08 45 07.27 | |||||||
| Spectral type | DA | DA | DA | DA | DA | DA | DA0.6 | DA | DA | |||||||
| Effective temperature | [K] | 76903.0 (2514) | 22372.0 | 84430.0 (3270) | 47037.0 (2740) | 80769.0 (2071) | 71388.0 (1618) | 81159.0 (2091) | ||||||||
| log(g) | [cgs] | 7.21 (0.08) | 6.15 | 7.14 (0.09) | 7.22 (0.3) | 7.37 (0.08) | 7.27 (0.07) | 7.39 (0.08) | ||||||||
| Mass | [M☉] | 0.48 (0.02) | 0.124 | 0.52 (0.02) | 0.423 (0.5) | 0.514 (0.02) | ||||||||||
| log(Luminosity) | [L☉] | 1.41 (0.09) | ||||||||||||||
| Cooling age | [Gyr] | 0.0001 | 0.0001 | |||||||||||||
| 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] | 2.41 (0.07) | 2.18 (0.09) | 2.41 | 2.41 (0.07) | |||||||||||
| Distance | [pc] | 415.43 (12) | 459.33 (19) | 415.43 | 415.42 (12) | |||||||||||
| Composition | H | H | H | |||||||||||||
| Proper motion (right ascension) | [mas/yr] | 7.258566151 (0.09) | 7.026012472 (0.2) | 7.259 (0.09) | 7.7 | 4.0 | ||||||||||
| Proper motion (declination) | [mas/yr] | -60.91948396 (0.07) | -60.96977199 (0.1) | -60.919 (0.07) | -58.3 | -61.0 | ||||||||||
| Variability | ||||||||||||||||
| Magnetic | ||||||||||||||||
| Bd | [MG] | |||||||||||||||
| Infrared excess (disk) | ||||||||||||||||
| Binarity | ||||||||||||||||
| B magnitude | ||||||||||||||||
| V magnitude | ||||||||||||||||
| R magnitude | ||||||||||||||||
| I magnitude | ||||||||||||||||
| J magnitude | 16.72 (0.1) | |||||||||||||||
| H magnitude | 16.90 (0.3) | |||||||||||||||
| K magnitude | ||||||||||||||||
| u magnitude | 15.54 (0.005) | 15.54 (0.005) | 15.49 (0.02) | 15.50 | 15.53 (0.02) | 15.50 (0.02) | ||||||||||
| g magnitude | 15.84 (0.004) | 15.84 (0.004) | 15.85 (0.03) | 15.85 | 15.88 (0.03) | 15.85 (0.03) | ||||||||||
| r magnitude | 16.26 (0.004) | 16.27 (0.004) | 16.25 (0.02) | 16.25 | 16.26 (0.02) | 16.25 (0.02) | ||||||||||
| i magnitude | 16.59 (0.005) | 16.59 (0.005) | 16.57 (0.02) | 16.57 | 16.58 (0.02) | 16.57 (0.02) | ||||||||||
| z magnitude | 16.87 (0.01) | 16.87 (0.01) | 16.86 (0.02) | 16.87 | 16.86 (0.02) | 16.87 (0.02) | ||||||||||
| G magnitude | 16.01 (0.003) | 16.03 | 16.01 | 16.01 (0.003) | ||||||||||||
| BP magnitude | 15.87 (0.003) | 15.81 | ||||||||||||||
| RP magnitude | 16.27 (0.006) | 16.25 | ||||||||||||||
| Pan g magnitude | 15.86 (0.002) | |||||||||||||||
| Pan r magnitude | 16.25 (0.005) | |||||||||||||||
| Pan i magnitude | 16.59 (0.002) | |||||||||||||||
| Pan z magnitude | 16.84 (0.006) | |||||||||||||||
| Pan y magnitude | 17.04 (0.009) | |||||||||||||||
| E(B-V) | 0.029 | |||||||||||||||
* 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
