SDSS J094629.78+673854.3
All names: SDSS J094629.78+673854.3, J0946+6738, WDJ094629.78+673854.11, SDSS J094629.78+673854.2, Gaia DR2 1069735341067492224, Gaia DR3 1069735341067492224, SDSS J094629.77+673854.2, GALEX J094629.8+673854, Gaia EDR3 1069735341067492224
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Kilic et al. 2025 | Caron et al. 2023 | Kilic et al. 2020 | MWDD H | Gaia DR2 | Stilism | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | Kleinman et al. 2013 | Vincent et al. 2023 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 09 46 29.74 (0.08) | 09 46 29.78 | 09 46 29.74 (0.1) | 09 46 29.74 | 09 46 29.78 (0.08) | 09 46 29.74 | 09 46 29.78 | ||||||||
| Declination | 67 38 54.88 (0.1) | 67 38 54.27 | 67 38 54.86 (0.2) | 67 38 54.88 | 67 38 54.10 (0.1) | 67 38 54.86 | 67 38 54.28 | ||||||||
| Spectral type | DA | DA | DA | DA | DA | DA | DA | DA | |||||||
| Effective temperature | [K] | 6686.0 (46) | 6713.0 (44) | 6685.0 (46) | 6696.0 | 6831.0 (98) | 6766.0 (49) | ||||||||
| log(g) | [cgs] | 8.05 (0.02) | 8.04 (0.02) | 8.03 (0.02) | 8.04 | 8.12 (0.03) | 7.87 (0.1) | ||||||||
| Mass | [M☉] | 0.623 (0.01) | 0.614 (0.02) | 0.608 (0.02) | 0.612 | 0.662 (0.03) | 0.523 (0.06) | ||||||||
| log(Luminosity) | [L☉] | ||||||||||||||
| Cooling age | [Gyr] | 1.8500 | 1.8000 | ||||||||||||
| 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] | 12.52 (0.1) | 12.33 (0.2) | 12.33 (0.2) | 12.52 | 12.52 (0.1) | 12.33 (0.2) | ||||||||
| Distance | [pc] | 79.87 (0.7) | 81.10 (1) | 81.07 (1) | 79.87 | 79.87 (0.7) | 81.07 (1) | ||||||||
| Composition | H | H | H | ||||||||||||
| Proper motion (right ascension) | [mas/yr] | -16.56511059 (0.1) | -16.57650412 (0.2) | -16.565 (0.1) | -16.57650412 | ||||||||||
| Proper motion (declination) | [mas/yr] | 48.66799122 (0.1) | 48.39076674 (0.3) | 48.668 (0.1) | 48.39076674 | ||||||||||
| 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) | 19.03 (0.02) | 19.04 (0.02) | 19.04 (0.02) | 19.04 (0.03) | ||||||||||
| g magnitude | 18.38 (0.007) | 18.38 (0.007) | 18.38 (0.007) | 18.37 (0.02) | |||||||||||
| r magnitude | 18.19 (0.007) | 18.19 (0.007) | 18.19 (0.007) | 18.18 (0.02) | |||||||||||
| i magnitude | 18.12 (0.009) | 18.12 (0.009) | 18.12 (0.009) | 18.12 (0.04) | |||||||||||
| z magnitude | 18.17 (0.03) | 18.17 (0.03) | 18.17 (0.03) | 18.17 (0.03) | |||||||||||
| G magnitude | 18.19 (0.02) | 18.21 | 18.19 | 18.19 (0.003) | 18.21 | ||||||||||
| BP magnitude | 18.40 (0.02) | 18.35 | 18.35 | ||||||||||||
| RP magnitude | 17.83 (0.02) | 17.81 | 17.81 | ||||||||||||
| Pan g magnitude | 18.41 (0.006) | 18.41 (0.006) | |||||||||||||
| Pan r magnitude | 18.20 (0.01) | 18.20 (0.01) | |||||||||||||
| Pan i magnitude | 18.15 (0.005) | 18.15 (0.007) | |||||||||||||
| Pan z magnitude | 18.20 (0.01) | 18.20 (0.009) | |||||||||||||
| Pan y magnitude | 18.17 (0.03) | 18.17 (0.02) | |||||||||||||
| E(B-V) | 0.004 | ||||||||||||||
* 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
