PB 5070
All names: Gaia DR3 2677321641247692032, SDSS J220602.41-004632.9, Gaia DR2 2677321641247692032, 2MASS J22060239-0046328, WD 2203-010, TIC 404722884, SDSS J220602.42-004632.8, WDJ220602.42-004632.71, GALEX J220602.4-004633, Gaia EDR3 2677321641247692032, USNO-B1.0 0892-00618661, SDSS J220602.41-004632.7, SDSS J220602.42-004632.92, SDSS J220602.42-004632.9, PB 5070, HE 2203-0101, J2206-0046, SDSS J220602.42-004632.7
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | SDSS DR10 | Kilic et al. 2025 | Kilic et al. 2020 | MWDD H | Gaia DR2 | Stilism | Kepler et al. 2015 | Koester et al. 2009 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) | Vincent et al. 2023 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 22 06 02.41 (0.04) | 22 06 02.42 | 22 06 02.42 | 22 06 02.41 (0.08) | 22 06 02.41 | 22 06 02.42 (0.04) | 22 06 02.41 | 22 06 02.28 | |||||||||
| Declination | -00 46 33.01 (0.04) | -00 46 32.77 | -00 46 32.77 | -00 46 33.00 (0.08) | -00 46 33.01 | -00 46 32.71 (0.04) | -00 46 33.00 | -00 46 27.84 | |||||||||
| Spectral type | DA | DA | DA | DA | DA | DA | DA | DA | DA | ||||||||
| Effective temperature | [K] | 18091.0 (273) | 18085.0 (274) | 17618.0 | 19001.0 (48) | 18047.0 (33) | 17369.0 (320) | ||||||||||
| log(g) | [cgs] | 8.04 (0.01) | 8.04 (0.01) | 8.01 | 8.10 (0.01) | 7.87 (0.007) | 7.99 (0.02) | ||||||||||
| Mass | [M☉] | 0.642 (0.01) | 0.643 (0.01) | 0.626 | 0.6729999999999999 (0.005) | 0.612 (0.01) | |||||||||||
| log(Luminosity) | [L☉] | ||||||||||||||||
| Cooling age | [Gyr] | 0.1176 | |||||||||||||||
| 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] | 10.17 (0.05) | 10.19 (0.09) | 10.17 | 10.16 (0.05) | 10.19 (0.09) | |||||||||||
| Distance | [pc] | 98.38 (0.5) | 98.18 (0.9) | 98.38 | 98.38 (0.5) | 98.18 (0.9) | |||||||||||
| Composition | H | H | |||||||||||||||
| Proper motion (right ascension) | [mas/yr] | -3.796695291 (0.05) | -3.75510554 (0.1) | -3.797 (0.05) | -3.755 | ||||||||||||
| Proper motion (declination) | [mas/yr] | -18.53799652 (0.05) | -18.41090931 (0.1) | -18.538 (0.05) | -18.411 | ||||||||||||
| Variability | |||||||||||||||||
| Magnetic | |||||||||||||||||
| Bd | [MG] | ||||||||||||||||
| Infrared excess (disk) | |||||||||||||||||
| Binarity | |||||||||||||||||
| B magnitude | 15.82 | 15.50 | |||||||||||||||
| V magnitude | |||||||||||||||||
| R magnitude | 16.40 | ||||||||||||||||
| I magnitude | |||||||||||||||||
| J magnitude | 16.43 (0.01) | ||||||||||||||||
| H magnitude | 16.44 (0.03) | ||||||||||||||||
| K magnitude | 16.46 (0.05) | ||||||||||||||||
| u magnitude | 15.95 (0.006) | 15.95 (0.006) | 15.95 (0.02) | 15.95 (0.006) | 15.93 (0.005) | ||||||||||||
| g magnitude | 15.81 (0.004) | 15.81 (0.004) | 15.85 (0.02) | 15.81 (0.004) | 15.80 (0.004) | ||||||||||||
| r magnitude | 16.17 (0.005) | 16.17 (0.005) | 16.16 (0.01) | 16.17 (0.005) | 16.16 (0.005) | ||||||||||||
| i magnitude | 16.43 (0.006) | 16.43 (0.006) | 16.42 (0.02) | 16.43 (0.006) | 16.42 (0.005) | ||||||||||||
| z magnitude | 16.70 (0.01) | 16.70 (0.01) | 16.69 (0.02) | 16.70 (0.01) | 16.74 (0.01) | ||||||||||||
| G magnitude | 16.00 (0.003) | 16.01 | 16.00 | 16.00 (0.003) | 16.01 | ||||||||||||
| BP magnitude | 15.93 (0.003) | 15.93 | 15.93 | ||||||||||||||
| RP magnitude | 16.15 (0.004) | 16.15 | 16.15 | ||||||||||||||
| Pan g magnitude | 15.85 (0.006) | ||||||||||||||||
| Pan r magnitude | 16.17 (0.002) | ||||||||||||||||
| Pan i magnitude | 16.48 (0.002) | ||||||||||||||||
| Pan z magnitude | 16.70 (0.004) | ||||||||||||||||
| Pan y magnitude | 16.90 (0.02) | ||||||||||||||||
| E(B-V) | 0.007 | ||||||||||||||||
* 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
