SDSS J232723.11+111704.3
All names: GALEX J232723.0+111704, Gaia DR2 2762859003029046784, SDSS J232723.11+111704.33, SDSS J232723.11+111704.3, SDSS J232723.11+111704.2, Gaia DR3 2762859003029046784, Gaia EDR3 2762859003029046784
| 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 | 23 27 23.13 (0.2) | 23 27 23.12 | 23 27 23.13 (0.3) | 23 27 23.12 (0.2) | ||||||
| Declination | 11 17 04.36 (0.2) | 11 17 04.27 | 11 17 04.36 (0.2) | 11 17 04.27 (0.2) | ||||||
| Spectral type | DA | DA | DA | DA | ||||||
| Effective temperature | [K] | 13736.0 | 19476.0 (165) | |||||||
| log(g) | [cgs] | 7.79 | 8.00 (0.03) | |||||||
| Mass | [M☉] | 0.495 | 0.621 (0.01) | |||||||
| log(Luminosity) | [L☉] | |||||||||
| Cooling age | [Gyr] | 0.1887 | ||||||||
| 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] | 2.30 (0.3) | 2.59 (0.4) | 2.30 (0.3) | ||||||
| Distance | [pc] | 435.14 (51) | 386.49 (57) | 435.14 (51) | ||||||
| Composition | H | |||||||||
| Proper motion (right ascension) | [mas/yr] | 10.17825508 (0.3) | 9.397799126 (0.7) | 10.178 (0.3) | ||||||
| Proper motion (declination) | [mas/yr] | 5.722429421 (0.2) | 5.348094158 (0.4) | 5.722 (0.2) | ||||||
| Variability | ||||||||||
| Magnetic | ||||||||||
| Bd | [MG] | |||||||||
| Infrared excess (disk) | ||||||||||
| Binarity | ||||||||||
| B magnitude | ||||||||||
| V magnitude | ||||||||||
| R magnitude | ||||||||||
| I magnitude | ||||||||||
| J magnitude | 19.60 (0.2) | |||||||||
| H magnitude | 19.60 (0.3) | |||||||||
| K magnitude | ||||||||||
| u magnitude | 19.09 (0.02) | 19.09 (0.02) | 19.10 (0.02) | |||||||
| g magnitude | 18.93 (0.009) | 18.94 (0.02) | 18.93 (0.009) | |||||||
| r magnitude | 19.20 (0.01) | 19.19 (0.03) | 19.20 (0.01) | |||||||
| i magnitude | 19.49 (0.02) | 19.48 (0.03) | 19.48 (0.02) | |||||||
| z magnitude | 19.74 (0.09) | 19.72 (0.09) | 19.73 (0.09) | |||||||
| G magnitude | 19.10 (0.02) | 19.15 | 19.10 (0.004) | |||||||
| BP magnitude | 19.05 (0.02) | 19.04 | ||||||||
| RP magnitude | 19.21 (0.04) | 19.12 | ||||||||
| Pan g magnitude | 18.99 (0.01) | |||||||||
| Pan r magnitude | 19.24 (0.008) | |||||||||
| Pan i magnitude | 19.53 (0.02) | |||||||||
| Pan z magnitude | 19.71 (0.02) | |||||||||
| Pan y magnitude | 19.88 (0.1) | |||||||||
| E(B-V) | 0.061 | |||||||||
* 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
