SDSS J110142.82+122710.5
All names: Gaia DR2 3871670403232190080, GALEX J110142.8+122711, SDSS J110142.82+122710.58, Gaia EDR3 3871670403232190080, Gaia DR3 3871670403232190080, SDSS J110142.82+122710.5
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR10 | MWDD H | Gaia DR2 | Stilism | Kepler et al. 2015 | Simbad | Vincent et al. 2023 |
|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 11 01 42.81 (1) | 11 01 42.82 | 11 01 42.81 (1) | 11 01 42.82 (1) | ||||||
| Declination | 12 27 10.66 (0.7) | 12 27 10.59 | 12 27 10.66 (0.7) | 12 27 10.69 (0.7) | ||||||
| Spectral type | DA | DA | DA | DA+MS | ||||||
| Effective temperature | [K] | 7438.0 | 7546.0 (88) | |||||||
| log(g) | [cgs] | 6.96 | 7.69 (0.2) | |||||||
| Mass | [M☉] | 0.192 | 0.455 (0.07) | |||||||
| log(Luminosity) | [L☉] | |||||||||
| Cooling age | [Gyr] | |||||||||
| 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] | 3.88 (1) | 2.28 (1) | 3.88 (1) | ||||||
| Distance | [pc] | 257.97 (67) | 438.14 (217) | 257.97 (67) | ||||||
| Composition | H | |||||||||
| Proper motion (right ascension) | [mas/yr] | -5.567529759 (1) | -11.77055751 (2) | -5.568 (1) | ||||||
| Proper motion (declination) | [mas/yr] | -1.970616582 (1) | -4.568722447 (1) | -1.971 (1) | ||||||
| Variability | ||||||||||
| Magnetic | ||||||||||
| Bd | [MG] | |||||||||
| Infrared excess (disk) | ||||||||||
| Binarity | WDMS | |||||||||
| B magnitude | ||||||||||
| V magnitude | ||||||||||
| R magnitude | ||||||||||
| I magnitude | ||||||||||
| J magnitude | ||||||||||
| H magnitude | ||||||||||
| K magnitude | ||||||||||
| u magnitude | 20.62 (0.07) | 20.64 (0.07) | 20.64 (0.07) | |||||||
| g magnitude | 20.23 (0.02) | 20.26 (0.03) | 20.26 (0.03) | |||||||
| r magnitude | 20.04 (0.02) | 20.08 (0.03) | 20.08 (0.03) | |||||||
| i magnitude | 20.03 (0.04) | 20.07 (0.05) | 20.07 (0.05) | |||||||
| z magnitude | 19.94 (0.1) | 19.97 (0.1) | 19.97 (0.1) | |||||||
| G magnitude | 20.35 (0.07) | 20.38 | 20.35 (0.01) | |||||||
| BP magnitude | 20.26 (0.07) | 20.00 | ||||||||
| RP magnitude | 19.95 (0.08) | 19.44 | ||||||||
| Pan g magnitude | 20.20 (0.02) | |||||||||
| Pan r magnitude | 20.05 (0.02) | |||||||||
| Pan i magnitude | 20.13 (0.02) | |||||||||
| Pan z magnitude | 20.14 (0.03) | |||||||||
| Pan y magnitude | 19.96 (0.1) | |||||||||
| E(B-V) | 0.021 | |||||||||
* 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
