SDSS J150147.38+140150.9
All names: Gaia EDR3 1182119619998752896, SDSS J150147.38+140150.95, Gaia DR2 1182119619998752896, SDSS J150147.38+140150.9, SDSS J150147.38+140151.0, Gaia DR3 1182119619998752896, GALEX J150147.4+140150
| 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 01 47.38 (0.2) | 15 01 47.38 | 15 01 47.38 (0.2) | 15 01 47.38 (0.2) | ||||||
| Declination | 14 01 50.94 (0.2) | 14 01 50.90 | 14 01 50.94 (0.2) | 14 01 50.79 (0.2) | ||||||
| Spectral type | DA | DA | DA | DA | ||||||
| Effective temperature | [K] | 15111.0 | 17730.0 (201) | |||||||
| log(g) | [cgs] | 7.74 | 7.91 (0.04) | |||||||
| Mass | [M☉] | 0.473 | 0.5720000000000001 (0.02) | |||||||
| log(Luminosity) | [L☉] | |||||||||
| Cooling age | [Gyr] | 0.1258 | ||||||||
| 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] | 2.38 (0.2) | 2.46 (0.3) | 2.38 (0.2) | ||||||
| Distance | [pc] | 420.05 (37) | 406.74 (43) | 420.04 (37) | ||||||
| Composition | H | |||||||||
| Proper motion (right ascension) | [mas/yr] | -2.704602708 (0.3) | -2.525354211 (0.5) | -2.705 (0.3) | ||||||
| Proper motion (declination) | [mas/yr] | 9.145214736 (0.2) | 9.227755243 (0.5) | 9.145 (0.2) | ||||||
| Variability | ||||||||||
| Magnetic | ||||||||||
| Bd | [MG] | |||||||||
| Infrared excess (disk) | ||||||||||
| Binarity | ||||||||||
| B magnitude | ||||||||||
| V magnitude | ||||||||||
| R magnitude | ||||||||||
| I magnitude | ||||||||||
| J magnitude | ||||||||||
| H magnitude | ||||||||||
| K magnitude | ||||||||||
| u magnitude | 19.04 (0.02) | 19.04 (0.03) | 19.04 (0.02) | |||||||
| g magnitude | 18.80 (0.008) | 18.82 (0.02) | 18.80 (0.008) | |||||||
| r magnitude | 19.12 (0.01) | 19.14 (0.02) | 19.12 (0.01) | |||||||
| i magnitude | 19.40 (0.02) | 19.40 (0.02) | 19.40 (0.02) | |||||||
| z magnitude | 19.85 (0.07) | 19.86 (0.07) | 19.85 (0.07) | |||||||
| G magnitude | 18.98 (0.03) | 19.01 | 18.98 (0.004) | |||||||
| BP magnitude | 19.03 (0.03) | 19.00 | ||||||||
| RP magnitude | 19.20 (0.06) | 19.11 | ||||||||
| Pan g magnitude | 18.83 (0.01) | |||||||||
| Pan r magnitude | 19.11 (0.005) | |||||||||
| Pan i magnitude | 19.43 (0.01) | |||||||||
| Pan z magnitude | 19.61 (0.02) | |||||||||
| Pan y magnitude | 19.80 (0.01) | |||||||||
| E(B-V) | 0.029 | |||||||||
* 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
