SDSS J120508.16+640229.8
All names: Gaia EDR3 1584595752562122752, Gaia DR2 1584595752562122752, SDSS J120508.16+640229.8, SDSS J120508.16+640229.85, Gaia DR3 1584595752562122752
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | MWDD H | Gaia DR2 | Stilism | Kepler et al. 2016 | Simbad | Vincent et al. 2023 |
|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 12 05 08.17 (0.6) | 12 05 08.16 | 12 05 08.17 (1) | 12 05 08.17 (0.6) | ||||||
| Declination | 64 02 29.27 (0.7) | 64 02 29.59 | 64 02 29.28 (0.9) | 64 02 29.53 (0.7) | ||||||
| Spectral type | DA: | DA: | DA | DA | ||||||
| Effective temperature | [K] | 7371.0 | 8199.0 (368) | |||||||
| log(g) | [cgs] | 8.67 | 8.00 (1) | |||||||
| Mass | [M☉] | 1.024 | ||||||||
| log(Luminosity) | [L☉] | |||||||||
| Cooling age | [Gyr] | 3.8430 | ||||||||
| 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] | 4.94 (0.8) | 5.43 (1) | 4.94 (0.8) | ||||||
| Distance | [pc] | 202.46 (33) | 184.23 (36) | 202.46 (33) | ||||||
| Composition | H | |||||||||
| Proper motion (right ascension) | [mas/yr] | -0.122903349 (1) | -0.308723075 (2) | -0.123 (1) | ||||||
| Proper motion (declination) | [mas/yr] | -15.8226993 (1) | -14.28782202 (2) | -15.823 (1) | ||||||
| Variability | ||||||||||
| Magnetic | ||||||||||
| Bd | [MG] | |||||||||
| Infrared excess (disk) | ||||||||||
| Binarity | ||||||||||
| B magnitude | ||||||||||
| V magnitude | ||||||||||
| R magnitude | ||||||||||
| I magnitude | ||||||||||
| J magnitude | ||||||||||
| H magnitude | ||||||||||
| K magnitude | ||||||||||
| u magnitude | 21.32 (0.1) | 21.32 (0.1) | 21.32 (0.1) | |||||||
| g magnitude | 20.78 (0.03) | 20.80 (0.03) | 20.80 (0.03) | |||||||
| r magnitude | 20.79 (0.04) | 20.79 (0.04) | 20.79 (0.04) | |||||||
| i magnitude | 20.74 (0.06) | 20.72 (0.06) | 20.72 (0.06) | |||||||
| z magnitude | 20.57 (0.2) | 20.55 (0.2) | 20.55 (0.2) | |||||||
| G magnitude | 20.70 (0.1) | 20.75 | 20.70 (0.008) | |||||||
| BP magnitude | 20.93 (0.1) | 20.53 | ||||||||
| RP magnitude | 20.42 (0.1) | 20.01 | ||||||||
| Pan g magnitude | 20.79 (0.03) | |||||||||
| Pan r magnitude | 20.67 (0.03) | |||||||||
| Pan i magnitude | 20.71 (0.03) | |||||||||
| Pan z magnitude | 20.71 (0.05) | |||||||||
| Pan y magnitude | 20.23 (0.2) | |||||||||
| E(B-V) | 0.015 | |||||||||
* 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
