SDSS J150342.55+073819.9
All names: Gaia EDR3 1160738345086471168, SDSS J150342.55+073819.90, Gaia DR2 1160738345086471168, SDSS J150342.55+073819.8, SDSS J150342.55+073819.9, Gaia DR3 1160738345086471168
| 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 | 15 03 42.54 (0.6) | 15 03 42.55 | 15 03 42.54 (0.7) | 15 03 42.56 (0.6) | ||||||
| Declination | 07 38 19.86 (0.4) | 07 38 19.90 | 07 38 19.86 (0.5) | 07 38 19.91 (0.4) | ||||||
| Spectral type | DA: | DA: | DA | DA | ||||||
| Effective temperature | [K] | 7268.0 | 7012.0 (106) | |||||||
| log(g) | [cgs] | 8.21 | 7.77 (0.2) | |||||||
| Mass | [M☉] | 0.724 | 0.488 (0.08) | |||||||
| log(Luminosity) | [L☉] | |||||||||
| Cooling age | [Gyr] | 1.9580 | ||||||||
| 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] | 5.47 (0.6) | 4.98 (0.7) | 5.47 (0.6) | ||||||
| Distance | [pc] | 182.88 (18) | 200.75 (29) | 182.88 (19) | ||||||
| Composition | H | |||||||||
| Proper motion (right ascension) | [mas/yr] | -15.06836963 (0.7) | -12.4587099 (1) | -15.068 (0.7) | ||||||
| Proper motion (declination) | [mas/yr] | -3.075514784 (0.6) | -3.365192683 (1) | -3.076 (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 | 20.86 (0.07) | 20.85 (0.06) | 20.86 (0.07) | |||||||
| g magnitude | 20.26 (0.02) | 20.27 (0.02) | 20.26 (0.02) | |||||||
| r magnitude | 20.15 (0.02) | 20.18 (0.03) | 20.14 (0.02) | |||||||
| i magnitude | 20.09 (0.03) | 20.11 (0.03) | 20.09 (0.03) | |||||||
| z magnitude | 20.13 (0.1) | 20.14 (0.1) | 20.13 (0.1) | |||||||
| G magnitude | 20.12 (0.1) | 20.18 | 20.12 (0.008) | |||||||
| BP magnitude | 20.05 (0.1) | 20.46 | ||||||||
| RP magnitude | 19.78 (0.1) | 19.71 | ||||||||
| Pan g magnitude | 20.26 (0.02) | |||||||||
| Pan r magnitude | 20.13 (0.02) | |||||||||
| Pan i magnitude | 20.16 (0.02) | |||||||||
| Pan z magnitude | 20.20 (0.02) | |||||||||
| Pan y magnitude | 20.06 (0.05) | |||||||||
| E(B-V) | 0.023 | |||||||||
* 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
