Gaia DR2 1039163458912998272
All names: 2MASS J09254282+6120127, Gaia DR3 1039163458912998272, WDJ092542.84+612012.84, GALEX J092542.8+612013, TIC 86279816, SDSS J092542.83+612012.8, WDJ092542.84+612012.85, Gaia EDR3 1039163458912998272, J0925+6120, Gaia DR2 1039163458912998272, SDSS J092542.82+612012.9
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Kilic et al. 2025 | O'Brien et al. 2024 | Caron et al. 2023 | Kilic et al. 2020 | McCleery et al. 2020 | Tremblay et al. 2020 | MWDD H | MWDD HE | Gaia DR2 | Stilism | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 09 25 43.02 (0.02) | 09 25 43.02 (0.02) | 09 25 43.02 | 09 25 43.02 | 09 25 42.84 (0.02) | 09 25 43.02 | ||||||||||
| Declination | 61 20 13.63 (0.02) | 61 20 13.61 (0.02) | 61 20 13.61 | 61 20 13.63 | 61 20 12.85 (0.02) | 61 20 13.61 | ||||||||||
| Spectral type | DA | DA | DA | DA | DA | DA | DA | DA | ||||||||
| Effective temperature | [K] | 8160.0 (28) | 8009.0 (63) | 8031.0 (22) | 8160.0 (28) | 8008.8 (26) | 8010.0 (30) | 7945.0 | 7687.0 | 8179.0 (24) | ||||||
| log(g) | [cgs] | 7.89 (0.006) | 7.85 (0.02) | 7.86 (0.005) | 7.89 (0.006) | 7.85 (0.01) | 7.85 (0.01) | 7.84 | 7.74 | 7.89 (0.005) | ||||||
| Mass | [M☉] | 0.534 (0.005) | 0.508 (0.01) | 0.514 (0.004) | 0.534 (0.004) | 0.503 | 0.431 | 0.534 (0.004) | ||||||||
| log(Luminosity) | [L☉] | |||||||||||||||
| Cooling age | [Gyr] | 0.9200 | 0.8782 | 0.8814 | ||||||||||||
| 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] | 36.42 (0.02) | 36.42 (0.02) | 36.40 (0.03) | 36.40 (0.03) | 36.40 (0.03) | 36.42 | 36.42 (0.02) | 36.40 (0.03) | |||||||
| Distance | [pc] | 27.46 (0.02) | 27.46 (0.02) | 27.47 (0.02) | 27.47 (0.02) | 27.47 (0.02) | 27.46 | 27.46 (0.02) | 27.47 (0.02) | |||||||
| Composition | H | H | H | |||||||||||||
| Proper motion (right ascension) | [mas/yr] | 82.7338069 (0.02) | 82.66776332 (0.05) | 82.734 (0.02) | 82.66776332 | |||||||||||
| Proper motion (declination) | [mas/yr] | 49.02442682 (0.02) | 48.85881296 (0.05) | 49.024 (0.02) | 48.85881296 | |||||||||||
| Variability | ||||||||||||||||
| Magnetic | ||||||||||||||||
| Bd | [MG] | |||||||||||||||
| Infrared excess (disk) | ||||||||||||||||
| Binarity | ||||||||||||||||
| B magnitude | ||||||||||||||||
| V magnitude | ||||||||||||||||
| R magnitude | ||||||||||||||||
| I magnitude | ||||||||||||||||
| J magnitude | 14.50 (0.02) | 14.50 (0.02) | ||||||||||||||
| H magnitude | 14.36 (0.04) | 14.36 (0.04) | ||||||||||||||
| K magnitude | 14.26 (0.06) | 14.26 (0.06) | ||||||||||||||
| u magnitude | 15.46 (0.004) | 15.46 (0.004) | 15.46 (0.004) | |||||||||||||
| g magnitude | 15.04 (0.003) | 15.04 (0.003) | ||||||||||||||
| r magnitude | 14.97 (0.003) | 14.97 (0.003) | ||||||||||||||
| i magnitude | 14.99 (0.003) | 14.99 (0.003) | ||||||||||||||
| z magnitude | 15.08 (0.005) | 15.08 (0.005) | ||||||||||||||
| G magnitude | 14.92 (0.001) | 14.94 | 14.94 | 14.92 | 14.92 (0.003) | 14.94 | ||||||||||
| BP magnitude | 15.05 (0.001) | 15.04 | 15.04 | |||||||||||||
| RP magnitude | 14.69 (0.001) | 14.69 | 14.69 | |||||||||||||
| Pan g magnitude | 15.05 (0.003) | 15.05 (0.003) | ||||||||||||||
| Pan r magnitude | 14.98 (0.004) | 14.98 (0.004) | ||||||||||||||
| Pan i magnitude | 15.02 (0.003) | 15.02 (0.003) | ||||||||||||||
| Pan z magnitude | 15.11 (0.003) | 15.11 (0.003) | ||||||||||||||
| Pan y magnitude | 15.17 (0.003) | 15.17 (0.003) | ||||||||||||||
| E(B-V) | 0.001 | |||||||||||||||
* 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
