SDSS J100528.58+565049.5
All names: Gaia DR2 1045371709584368896, SDSS J100528.58+565049.51, Gaia DR3 1045371709584368896, SDSS J100528.58+565049.5, SDSS J100528.59+565049.2, GALEX J100528.7+565048, Gaia EDR3 1045371709584368896
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | MWDD H | Gaia DR2 | Stilism | Kepler et al. 2016 | Simbad | Vincent et al. 2023 |
|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 10 05 28.57 (0.3) | 10 05 28.59 | 10 05 28.57 (0.5) | 10 05 28.61 (0.3) | ||||||
| Declination | 56 50 48.93 (0.3) | 56 50 49.22 | 56 50 48.94 (0.5) | 56 50 49.22 (0.3) | ||||||
| Spectral type | DA: | DA: | DA | DA | ||||||
| Effective temperature | [K] | 7030.0 | 6921.0 (129) | |||||||
| log(g) | [cgs] | 7.60 | 7.98 (0.2) | |||||||
| Mass | [M☉] | 0.383 | 0.5489999999999999 (0.1) | |||||||
| log(Luminosity) | [L☉] | |||||||||
| Cooling age | [Gyr] | 0.9219 | ||||||||
| 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] | 3.81 (0.4) | 3.36 (0.6) | 3.81 (0.4) | ||||||
| Distance | [pc] | 262.32 (31) | 297.57 (57) | 262.32 (31) | ||||||
| Composition | H | |||||||||
| Proper motion (right ascension) | [mas/yr] | -19.52151945 (0.5) | -19.728908 (1) | -19.522 (0.5) | ||||||
| Proper motion (declination) | [mas/yr] | -17.70156552 (0.4) | -18.13267915 (1) | -17.702 (0.4) | ||||||
| Variability | ||||||||||
| Magnetic | ||||||||||
| Bd | [MG] | |||||||||
| Infrared excess (disk) | ||||||||||
| Binarity | ||||||||||
| B magnitude | ||||||||||
| V magnitude | ||||||||||
| R magnitude | ||||||||||
| I magnitude | ||||||||||
| J magnitude | ||||||||||
| H magnitude | ||||||||||
| K magnitude | ||||||||||
| u magnitude | 20.98 (0.07) | 21.02 (0.1) | 20.98 (0.07) | |||||||
| g magnitude | 20.44 (0.02) | 20.47 (0.04) | 20.45 (0.03) | |||||||
| r magnitude | 20.28 (0.03) | 20.31 (0.04) | 20.29 (0.03) | |||||||
| i magnitude | 20.29 (0.04) | 20.30 (0.04) | 20.30 (0.04) | |||||||
| z magnitude | 20.04 (0.1) | 20.07 (0.1) | 20.05 (0.1) | |||||||
| G magnitude | 20.25 (0.05) | 20.30 | 20.25 (0.006) | |||||||
| BP magnitude | 20.47 (0.05) | 20.18 | ||||||||
| RP magnitude | 20.14 (0.09) | 19.96 | ||||||||
| Pan g magnitude | 20.42 (0.01) | |||||||||
| Pan r magnitude | 20.27 (0.02) | |||||||||
| Pan i magnitude | 20.30 (0.01) | |||||||||
| Pan z magnitude | 20.35 (0.04) | |||||||||
| Pan y magnitude | 20.03 (0.05) | |||||||||
| E(B-V) | 0.017 | |||||||||
* 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
