SDSS J110405.01+373711.9
All names: Gaia DR3 763234762449568896, Gaia EDR3 763234762449568896, GALEX J110405.0+373711, SDSS J110405.01+373711.9, Gaia DR2 763234762449568896, SDSS J110405.00+373711.8
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | MWDD H | Gaia DR2 | Stilism | Simbad | Kleinman et al. 2013 | Vincent et al. 2023 |
|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 11 04 05.01 (0.2) | 11 04 05.01 | 11 04 05.01 (0.3) | 11 04 05.01 (0.2) | 11 04 05.01 | |||||
| Declination | 37 37 11.85 (0.3) | 37 37 11.88 | 37 37 11.85 (0.5) | 37 37 11.88 (0.3) | 37 37 11.87 | |||||
| Spectral type | DA | DA | DA | DA | ||||||
| Effective temperature | [K] | 19554.0 | 22816.0 (692) | |||||||
| log(g) | [cgs] | 8.29 | 7.89 (0.1) | |||||||
| Mass | [M☉] | 0.801 | ||||||||
| log(Luminosity) | [L☉] | |||||||||
| Cooling age | [Gyr] | 0.1432 | ||||||||
| 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] | 1.72 (0.3) | 2.27 (0.4) | 1.72 (0.3) | ||||||
| Distance | [pc] | 582.20 (110) | 439.86 (82) | 582.21 (110) | ||||||
| Composition | H | |||||||||
| Proper motion (right ascension) | [mas/yr] | -0.760113759 (0.3) | -0.651980854 (0.6) | -0.76 (0.3) | ||||||
| Proper motion (declination) | [mas/yr] | -1.550188913 (0.4) | -0.9743151 (0.9) | -1.55 (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 | 19.26 (0.03) | 19.26 (0.03) | 19.29 (0.04) | |||||||
| g magnitude | 19.26 (0.01) | 19.26 (0.01) | 19.25 (0.02) | |||||||
| r magnitude | 19.66 (0.02) | 19.66 (0.02) | 19.69 (0.02) | |||||||
| i magnitude | 20.03 (0.03) | 20.03 (0.03) | 20.05 (0.04) | |||||||
| z magnitude | 20.17 (0.1) | 20.17 (0.1) | 20.17 (0.1) | |||||||
| G magnitude | 19.51 (0.03) | 19.56 | 19.51 (0.004) | |||||||
| BP magnitude | 19.45 (0.03) | 19.40 | ||||||||
| RP magnitude | 19.84 (0.07) | 19.71 | ||||||||
| Pan g magnitude | 19.33 (0.004) | |||||||||
| Pan r magnitude | 19.71 (0.02) | |||||||||
| Pan i magnitude | 20.00 (0.01) | |||||||||
| Pan z magnitude | 20.26 (0.03) | |||||||||
| Pan y magnitude | 20.16 (0.1) | |||||||||
| 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
