SDSS J103619.86+472836.4
All names: GALEX J103619.8+472836, SDSS J103619.86+472836.4, Gaia EDR3 833792034216593920, SDSS J103619.86+472836.42, Gaia DR3 833792034216593920, Gaia DR2 833792034216593920, SDSS J103619.85+472836.3, SDSS J103619.85+472836.4
| 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 36 19.84 (0.3) | 10 36 19.86 | 10 36 19.84 (0.3) | 10 36 19.86 (0.3) | ||||||
| Declination | 47 28 35.65 (0.4) | 47 28 36.37 | 47 28 35.67 (0.6) | 47 28 36.49 (0.4) | ||||||
| Spectral type | DA | DA | DA | DA | ||||||
| Effective temperature | [K] | 7050.0 | 7188.0 (94) | |||||||
| log(g) | [cgs] | 8.21 | 7.66 (0.2) | |||||||
| Mass | [M☉] | 0.721 | 0.397 (0.07) | |||||||
| log(Luminosity) | [L☉] | |||||||||
| Cooling age | [Gyr] | 2.1350 | ||||||||
| 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] | 5.42 (0.5) | 5.85 (0.8) | 5.42 (0.5) | ||||||
| Distance | [pc] | 184.38 (17) | 170.85 (23) | 184.38 (17) | ||||||
| Composition | H | |||||||||
| Proper motion (right ascension) | [mas/yr] | -16.44450408 (0.3) | -16.02005025 (0.7) | -16.445 (0.3) | ||||||
| Proper motion (declination) | [mas/yr] | -52.38323342 (0.4) | -52.42121697 (1) | -52.383 (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 | 20.58 (0.07) | 20.55 (0.07) | 20.58 (0.07) | |||||||
| g magnitude | 20.08 (0.02) | 20.08 (0.03) | 20.08 (0.02) | |||||||
| r magnitude | 19.87 (0.02) | 19.86 (0.02) | 19.88 (0.02) | |||||||
| i magnitude | 19.90 (0.03) | 19.89 (0.05) | 19.90 (0.03) | |||||||
| z magnitude | 19.90 (0.09) | 19.89 (0.09) | 19.90 (0.09) | |||||||
| G magnitude | 19.86 (0.06) | 19.91 | 19.86 (0.005) | |||||||
| BP magnitude | 20.22 (0.06) | 20.15 | ||||||||
| RP magnitude | 19.56 (0.06) | 19.53 | ||||||||
| Pan g magnitude | 20.04 (0.01) | |||||||||
| Pan r magnitude | 19.89 (0.01) | |||||||||
| Pan i magnitude | 19.88 (0.01) | |||||||||
| Pan z magnitude | 19.92 (0.02) | |||||||||
| Pan y magnitude | 19.42 (0.08) | |||||||||
| E(B-V) | 0.012 | |||||||||
* 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
