SDSS J094459.18+065102.1
All names: SDSS J094459.16+065102.4, SDSS J094459.18+065102.19, Gaia DR2 3853365905451141120, GALEX J094459.1+065102, Gaia EDR3 3853365905451141120, SDSS J094459.17+065102.1, SDSS J094459.18+065102.1, Gaia DR3 3853365905451141120
| 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 | 09 44 59.18 (0.3) | 09 44 59.16 | 09 44 59.18 (0.5) | 09 44 59.16 (0.3) | ||||||
| Declination | 06 51 02.00 (0.3) | 06 51 02.42 | 06 51 02.01 (0.4) | 06 51 02.49 (0.3) | ||||||
| Spectral type | DA | DA | DA | DA | ||||||
| Effective temperature | [K] | 13548.0 | 16076.0 (140) | |||||||
| log(g) | [cgs] | 7.40 | 8.10 (0) | |||||||
| Mass | [M☉] | 0.335 | 0.6679999999999999 (0) | |||||||
| log(Luminosity) | [L☉] | |||||||||
| Cooling age | [Gyr] | 0.1339 | ||||||||
| 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] | 2.01 (0.4) | 1.82 (0.6) | 2.01 (0.4) | ||||||
| Distance | [pc] | 497.44 (90) | 549.30 (188) | 497.44 (90) | ||||||
| Composition | H | |||||||||
| Proper motion (right ascension) | [mas/yr] | 20.41923359 (0.4) | 19.97937507 (0.8) | 20.419 (0.4) | ||||||
| Proper motion (declination) | [mas/yr] | -30.49477137 (0.3) | -30.13222121 (0.8) | -30.495 (0.3) | ||||||
| Variability | ||||||||||
| Magnetic | ||||||||||
| Bd | [MG] | |||||||||
| Infrared excess (disk) | ||||||||||
| Binarity | ||||||||||
| B magnitude | ||||||||||
| V magnitude | ||||||||||
| R magnitude | ||||||||||
| I magnitude | ||||||||||
| J magnitude | ||||||||||
| H magnitude | ||||||||||
| K magnitude | ||||||||||
| u magnitude | 19.56 (0.03) | 19.56 (0.03) | 19.56 (0.03) | |||||||
| g magnitude | 19.21 (0.01) | 19.21 (0.01) | 19.21 (0.01) | |||||||
| r magnitude | 19.50 (0.01) | 19.50 (0.01) | 19.50 (0.01) | |||||||
| i magnitude | 19.75 (0.03) | 19.75 (0.03) | 19.75 (0.03) | |||||||
| z magnitude | 20.26 (0.1) | 20.26 (0.1) | 20.26 (0.1) | |||||||
| G magnitude | 19.37 (0.04) | 19.41 | 19.37 (0.004) | |||||||
| BP magnitude | 19.40 (0.04) | 19.27 | ||||||||
| RP magnitude | 19.49 (0.05) | 19.46 | ||||||||
| Pan g magnitude | 19.22 (0.01) | |||||||||
| Pan r magnitude | 19.50 (0.007) | |||||||||
| Pan i magnitude | 19.77 (0.02) | |||||||||
| Pan z magnitude | 19.96 (0.04) | |||||||||
| Pan y magnitude | 19.92 (0.1) | |||||||||
| E(B-V) | 0.025 | |||||||||
* 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
