SDSS J232444.65+135815.9
All names: Gaia DR3 2813018860927054080, SDSS J232444.65+135815.8, SDSS J232444.65+135815.9, SDSS J232444.65+135815.90, SDSS J232444.64+135815.9, Gaia DR2 2813018860927054080, Gaia EDR3 2813018860927054080
| 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 24 44.66 (0.5) | 23 24 44.65 | 23 24 44.66 (0.6) | 23 24 44.65 (0.5) | ||||||
| Declination | 13 58 15.70 (0.4) | 13 58 15.90 | 13 58 15.70 (0.5) | 13 58 15.96 (0.4) | ||||||
| Spectral type | DA: | DA: | DA | DA | ||||||
| Effective temperature | [K] | 7330.0 | 7709.0 (99) | |||||||
| log(g) | [cgs] | 7.40 | 8.48 (0.1) | |||||||
| Mass | [M☉] | 0.308 | 0.8059999999999999 (0.1) | |||||||
| log(Luminosity) | [L☉] | |||||||||
| Cooling age | [Gyr] | 0.7183 | ||||||||
| 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] | 3.17 (0.6) | 2.99 (0.8) | 3.17 (0.6) | ||||||
| Distance | [pc] | 315.32 (59) | 334.06 (94) | 315.32 (59) | ||||||
| Composition | H | |||||||||
| Proper motion (right ascension) | [mas/yr] | 13.38189756 (0.5) | 13.66100844 (2) | 13.382 (0.5) | ||||||
| Proper motion (declination) | [mas/yr] | -16.3314627 (0.5) | -17.07635295 (1) | -16.331 (0.5) | ||||||
| Variability | ||||||||||
| Magnetic | ||||||||||
| Bd | [MG] | |||||||||
| Infrared excess (disk) | ||||||||||
| Binarity | ||||||||||
| B magnitude | ||||||||||
| V magnitude | ||||||||||
| R magnitude | ||||||||||
| I magnitude | ||||||||||
| J magnitude | ||||||||||
| H magnitude | ||||||||||
| K magnitude | ||||||||||
| u magnitude | 20.69 (0.06) | 20.67 (0.06) | 20.71 (0.06) | |||||||
| g magnitude | 20.27 (0.02) | 20.27 (0.03) | 20.27 (0.02) | |||||||
| r magnitude | 20.12 (0.02) | 20.11 (0.03) | 20.12 (0.02) | |||||||
| i magnitude | 20.23 (0.03) | 20.22 (0.04) | 20.22 (0.03) | |||||||
| z magnitude | 20.08 (0.09) | 20.09 (0.09) | 20.06 (0.09) | |||||||
| G magnitude | 20.11 (0.1) | 20.16 | 20.11 (0.007) | |||||||
| BP magnitude | 20.40 (0.1) | 20.32 | ||||||||
| RP magnitude | 20.03 (0.09) | 19.68 | ||||||||
| Pan g magnitude | 20.25 (0.03) | |||||||||
| Pan r magnitude | 20.14 (0.01) | |||||||||
| Pan i magnitude | 20.12 (0.02) | |||||||||
| Pan z magnitude | 20.18 (0.04) | |||||||||
| Pan y magnitude | 20.19 (0.1) | |||||||||
| E(B-V) | 0.055 | |||||||||
* 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
