SDSS J225306.36+005102.0
All names: Gaia DR2 2654988253690446080, GALEX J225306.4+005103, SDSS J225306.36+005102.1, SDSS J225306.36+005102.05, Gaia EDR3 2654988253690446080, Gaia DR3 2654988253690446080, SDSS J225306.36+005102.0
| 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 | 22 53 06.35 (1) | 22 53 06.36 | 22 53 06.35 (2) | 22 53 06.36 (1) | ||||||
| Declination | 00 51 01.70 (0.7) | 00 51 02.02 | 00 51 01.72 (0.9) | 00 51 02.09 (0.7) | ||||||
| Spectral type | DA | DA | DA | DA | ||||||
| Effective temperature | [K] | 11247.0 | 10898.0 (62) | |||||||
| log(g) | [cgs] | 6.90 | 8.46 (0.08) | |||||||
| Mass | [M☉] | 0.209 | 0.8809999999999999 (0.05) | |||||||
| 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] | 1.15 (1) | 1.07 (2) | 1.15 (1) | ||||||
| Distance | [pc] | 870.35 (914) | 936.68 (1939) | 870.32 (914) | ||||||
| Composition | H | |||||||||
| Proper motion (right ascension) | [mas/yr] | -14.63698364 (1) | -15.43209906 (3) | -14.637 (1) | ||||||
| Proper motion (declination) | [mas/yr] | -24.41741504 (0.8) | -23.12938577 (2) | -24.417 (0.8) | ||||||
| Variability | ||||||||||
| Magnetic | ||||||||||
| Bd | [MG] | |||||||||
| Infrared excess (disk) | ||||||||||
| Binarity | ||||||||||
| B magnitude | ||||||||||
| V magnitude | ||||||||||
| R magnitude | ||||||||||
| I magnitude | ||||||||||
| J magnitude | ||||||||||
| H magnitude | ||||||||||
| K magnitude | ||||||||||
| u magnitude | 20.76 (0.07) | 20.75 (0.07) | 20.75 (0.07) | |||||||
| g magnitude | 20.29 (0.02) | 20.30 (0.03) | 20.30 (0.03) | |||||||
| r magnitude | 20.50 (0.03) | 20.55 (0.03) | 20.55 (0.03) | |||||||
| i magnitude | 20.69 (0.05) | 20.72 (0.05) | 20.72 (0.05) | |||||||
| z magnitude | 20.67 (0.2) | 20.64 (0.2) | 20.64 (0.2) | |||||||
| G magnitude | 20.39 (0.1) | 20.43 | 20.39 (0.01) | |||||||
| BP magnitude | 20.41 (0.1) | 20.61 | ||||||||
| RP magnitude | 20.30 (0.3) | 20.86 | ||||||||
| Pan g magnitude | 20.29 (0.02) | |||||||||
| Pan r magnitude | 20.42 (0.02) | |||||||||
| Pan i magnitude | 20.60 (0.04) | |||||||||
| Pan z magnitude | 20.81 (0.07) | |||||||||
| Pan y magnitude | ||||||||||
| E(B-V) | 0.054 | |||||||||
* 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
