SDSS J133256.49+373004.5
All names: SDSS J133256.49+373004.5, SDSS J133256.49+373004.50, Gaia DR3 1475183586704726144, Gaia EDR3 1475183586704726144, Gaia DR2 1475183586704726144
| 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 | 13 32 56.50 (0.3) | 13 32 56.49 | 13 32 56.50 (0.5) | 13 32 56.49 (0.3) | ||||||
| Declination | 37 30 04.49 (0.3) | 37 30 04.52 | 37 30 04.49 (0.4) | 37 30 04.40 (0.3) | ||||||
| Spectral type | DA | DA | DA | DA | ||||||
| Effective temperature | [K] | 7907.0 | 7961.0 (89) | |||||||
| log(g) | [cgs] | 8.30 | 7.98 (0.1) | |||||||
| Mass | [M☉] | 0.787 | 0.584 (0.07) | |||||||
| log(Luminosity) | [L☉] | |||||||||
| Cooling age | [Gyr] | 1.9170 | ||||||||
| 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] | 4.28 (0.5) | 4.32 (0.6) | 4.28 (0.5) | ||||||
| Distance | [pc] | 233.64 (28) | 231.63 (33) | 233.64 (28) | ||||||
| Composition | H | |||||||||
| Proper motion (right ascension) | [mas/yr] | 7.390498235 (0.4) | 7.193698692 (0.9) | 7.39 (0.4) | ||||||
| Proper motion (declination) | [mas/yr] | 5.66462945 (0.4) | 5.842799526 (0.7) | 5.665 (0.4) | ||||||
| Variability | ||||||||||
| Magnetic | ||||||||||
| Bd | [MG] | |||||||||
| Infrared excess (disk) | ||||||||||
| Binarity | ||||||||||
| B magnitude | ||||||||||
| V magnitude | ||||||||||
| R magnitude | ||||||||||
| I magnitude | ||||||||||
| J magnitude | ||||||||||
| H magnitude | ||||||||||
| K magnitude | ||||||||||
| u magnitude | 20.86 (0.05) | 20.86 (0.05) | 20.86 (0.05) | |||||||
| g magnitude | 20.39 (0.02) | 20.40 (0.02) | 20.39 (0.02) | |||||||
| r magnitude | 20.30 (0.02) | 20.29 (0.03) | 20.30 (0.02) | |||||||
| i magnitude | 20.34 (0.03) | 20.33 (0.03) | 20.34 (0.03) | |||||||
| z magnitude | 20.27 (0.1) | 20.24 (0.1) | 20.27 (0.1) | |||||||
| G magnitude | 20.30 (0.06) | 20.35 | 20.30 (0.005) | |||||||
| BP magnitude | 20.52 (0.06) | 20.29 | ||||||||
| RP magnitude | 20.08 (0.06) | 19.92 | ||||||||
| Pan g magnitude | 20.39 (0.02) | |||||||||
| Pan r magnitude | 20.29 (0.02) | |||||||||
| Pan i magnitude | 20.34 (0.02) | |||||||||
| Pan z magnitude | 20.48 (0.05) | |||||||||
| Pan y magnitude | 20.37 (0.2) | |||||||||
| E(B-V) | 0.018 | |||||||||
* 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
