SDSS J005229.94+354211.8
All names: Gaia EDR3 363891001075403648, SDSS J005229.94+354211.8, SDSS J005229.94+354211.89, Gaia DR3 363891001075403648, Gaia DR2 363891001075403648, SDSS J005229.93+354211.8
| 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 | 00 52 29.95 (0.7) | 00 52 29.94 | 00 52 29.95 (0.9) | 00 52 29.93 (0.7) | ||||||
| Declination | 35 42 11.91 (0.3) | 35 42 11.86 | 35 42 11.91 (1) | 35 42 11.91 (0.3) | ||||||
| Spectral type | DA | DA | DA | DA | ||||||
| Effective temperature | [K] | 8477.0 | 8508.0 (100) | |||||||
| log(g) | [cgs] | 9.01 | 7.92 (0.2) | |||||||
| Mass | [M☉] | 1.201 | 0.455 (0.07) | |||||||
| log(Luminosity) | [L☉] | |||||||||
| Cooling age | [Gyr] | 3.1140 | ||||||||
| 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] | 4.39 (1) | 6.12 (1) | 4.39 (1) | ||||||
| Distance | [pc] | 227.69 (51) | 163.42 (36) | 227.69 (51) | ||||||
| Composition | H | |||||||||
| Proper motion (right ascension) | [mas/yr] | 16.35389361 (0.8) | 17.30290185 (2) | 16.354 (0.8) | ||||||
| Proper motion (declination) | [mas/yr] | 0.198575627 (0.6) | 1.909257793 (3) | 0.199 (0.6) | ||||||
| Variability | ||||||||||
| Magnetic | ||||||||||
| Bd | [MG] | |||||||||
| Infrared excess (disk) | ||||||||||
| Binarity | ||||||||||
| B magnitude | ||||||||||
| V magnitude | ||||||||||
| R magnitude | ||||||||||
| I magnitude | ||||||||||
| J magnitude | ||||||||||
| H magnitude | ||||||||||
| K magnitude | ||||||||||
| u magnitude | 21.22 (0.1) | 21.23 (0.1) | 21.23 (0.1) | |||||||
| g magnitude | 20.75 (0.03) | 20.75 (0.03) | 20.75 (0.03) | |||||||
| r magnitude | 20.61 (0.04) | 20.62 (0.04) | 20.62 (0.04) | |||||||
| i magnitude | 20.65 (0.06) | 20.64 (0.06) | 20.64 (0.06) | |||||||
| z magnitude | 20.87 (0.2) | 20.77 (0.2) | 20.77 (0.2) | |||||||
| G magnitude | 20.59 (0.09) | 20.65 | 20.59 (0.006) | |||||||
| BP magnitude | 20.77 (0.09) | 20.67 | ||||||||
| RP magnitude | 20.25 (0.08) | 20.39 | ||||||||
| Pan g magnitude | 20.68 (0.03) | |||||||||
| Pan r magnitude | 20.61 (0.02) | |||||||||
| Pan i magnitude | 20.66 (0.02) | |||||||||
| Pan z magnitude | 20.83 (0.02) | |||||||||
| Pan y magnitude | 20.86 (0.2) | |||||||||
| E(B-V) | 0.027 | |||||||||
* 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
