SDSS J150005.09+314405.4
All names: SDSS J150005.09+314405.42, SDSS J150005.08+314405.4, SDSS J150005.08+314405.3, Gaia DR3 1288466274422424960, SDSS J150005.09+314405.4, Gaia DR2 1288466274422424960, Gaia EDR3 1288466274422424960
| 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 00 05.09 (0.3) | 15 00 05.08 | 15 00 05.09 (0.3) | 15 00 05.08 (0.3) | ||||||
| Declination | 31 44 05.06 (0.3) | 31 44 05.42 | 31 44 05.08 (0.4) | 31 44 05.48 (0.3) | ||||||
| Spectral type | DA: | DA: | DA | DA | ||||||
| Effective temperature | [K] | 6772.0 | 6946.0 (137) | |||||||
| log(g) | [cgs] | 7.97 | 7.92 (0.2) | |||||||
| Mass | [M☉] | 0.574 | 0.5489999999999999 (0.1) | |||||||
| log(Luminosity) | [L☉] | |||||||||
| Cooling age | [Gyr] | 1.5790 | ||||||||
| 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] | 4.25 (0.5) | 4.46 (0.6) | 4.25 (0.5) | ||||||
| Distance | [pc] | 235.35 (26) | 224.22 (31) | 235.36 (26) | ||||||
| Composition | H | |||||||||
| Proper motion (right ascension) | [mas/yr] | 4.101771035 (0.3) | 4.314412759 (0.7) | 4.102 (0.3) | ||||||
| Proper motion (declination) | [mas/yr] | -25.71755589 (0.4) | -25.50516676 (1) | -25.718 (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 | 21.15 (0.08) | 21.16 (0.08) | 21.15 (0.08) | |||||||
| g magnitude | 20.53 (0.02) | 20.56 (0.03) | 20.53 (0.02) | |||||||
| r magnitude | 20.36 (0.02) | 20.39 (0.03) | 20.36 (0.03) | |||||||
| i magnitude | 20.24 (0.03) | 20.26 (0.04) | 20.24 (0.03) | |||||||
| z magnitude | 20.21 (0.1) | 20.22 (0.1) | 20.21 (0.1) | |||||||
| G magnitude | 20.30 (0.06) | 20.35 | 20.30 (0.005) | |||||||
| BP magnitude | 20.55 (0.06) | 20.54 | ||||||||
| RP magnitude | 19.93 (0.06) | 19.99 | ||||||||
| Pan g magnitude | 20.48 (0.02) | |||||||||
| Pan r magnitude | 20.26 (0.02) | |||||||||
| Pan i magnitude | 20.26 (0.01) | |||||||||
| Pan z magnitude | 20.29 (0.03) | |||||||||
| Pan y magnitude | 19.97 (0.1) | |||||||||
| E(B-V) | 0.024 | |||||||||
* 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
