SDSS J115936.09+052019.9
All names: SDSS J115936.09+052019.8, Gaia DR3 3897947150587650688, Gaia EDR3 3897947150587650688, SDSS J115936.09+052019.9, SDSS J115936.10+052020.0, Gaia DR2 3897947150587650688, SDSS J115936.09+052019.90, SDSS J115936.11+052020.1
| 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 | 11 59 36.07 (0.3) | 11 59 36.10 | 11 59 36.07 (0.5) | 11 59 36.12 (0.3) | ||||||
| Declination | 05 20 19.76 (0.2) | 05 20 20.07 | 05 20 19.78 (0.2) | 05 20 20.22 (0.2) | ||||||
| Spectral type | DA | DA | DA | DA | ||||||
| Effective temperature | [K] | 13420.0 | 17951.0 (283) | |||||||
| log(g) | [cgs] | 7.26 | 7.96 (0.05) | |||||||
| Mass | [M☉] | 0.293 | 0.597 (0.02) | |||||||
| log(Luminosity) | [L☉] | |||||||||
| Cooling age | [Gyr] | 0.1257 | ||||||||
| 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] | 1.50 (0.3) | 1.64 (0.8) | 1.50 (0.3) | ||||||
| Distance | [pc] | 668.20 (153) | 610.07 (280) | 668.18 (153) | ||||||
| Composition | H | |||||||||
| Proper motion (right ascension) | [mas/yr] | -51.46664751 (0.4) | -50.74300998 (1) | -51.467 (0.4) | ||||||
| Proper motion (declination) | [mas/yr] | -28.67009252 (0.2) | -29.20541431 (0.6) | -28.67 (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 | 19.45 (0.02) | 19.45 (0.03) | 19.45 (0.03) | |||||||
| g magnitude | 19.19 (0.01) | 19.22 (0.02) | 19.20 (0.01) | |||||||
| r magnitude | 19.52 (0.01) | 19.52 (0.02) | 19.52 (0.01) | |||||||
| i magnitude | 19.77 (0.02) | 19.74 (0.03) | 19.77 (0.02) | |||||||
| z magnitude | 20.15 (0.07) | 20.16 (0.07) | 20.15 (0.07) | |||||||
| G magnitude | 19.39 (0.04) | 19.43 | 19.39 (0.004) | |||||||
| BP magnitude | 19.37 (0.04) | 19.38 | ||||||||
| RP magnitude | 19.63 (0.07) | 19.53 | ||||||||
| Pan g magnitude | 19.25 (0.007) | |||||||||
| Pan r magnitude | 19.52 (0.01) | |||||||||
| Pan i magnitude | 19.84 (0.01) | |||||||||
| Pan z magnitude | 20.04 (0.03) | |||||||||
| Pan y magnitude | 20.00 (0.04) | |||||||||
| 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
