SDSS J171315.76+405346.2
All names: Gaia DR3 1342008814203085440, WDJ171315.83+405345.85, J1713+4053, SDSS J171315.76+405346.2, SDSS J171315.74+405347.0, WIRED J171315.73+405347.0, SDSS J171315.73+405347.0, SDSS J171315.78+405346.1, LAMOST J171315.73+405347.0, Gaia EDR3 1342008814203085440, SDSS J171315.74+405347.1, Gaia DR2 1342008814203085440, GALEX J171315.8+405346
| 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 | Guo et al. 2015 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | Kleinman et al. 2013 | Vincent et al. 2023 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 17 13 15.65 (0.05) | 17 13 15.78 | 17 13 15.66 (0.07) | 17 13 15.65 | 17 13 15.83 (0.05) | 17 13 15.66 | 17 13 15.74 | |||||||||
| Declination | 40 53 46.88 (0.06) | 40 53 46.14 | 40 53 46.85 (0.08) | 40 53 46.88 | 40 53 45.84 (0.06) | 40 53 46.85 | 40 53 47.08 | |||||||||
| Spectral type | DA | DA | DA | DA | DA | DA | DA | DA | DA | |||||||
| Effective temperature | [K] | 8688.0 (64) | 8958.0 (61) | 8690.0 (64) | 8915.0 | 9067.0 (130) | 8946.0 (40) | |||||||||
| log(g) | [cgs] | 8.53 (0.01) | 8.57 (0.01) | 8.52 (0.01) | 8.56 | 8.60 (0.02) | 8.75 (0.05) | |||||||||
| Mass | [M☉] | 0.935 (0.008) | 0.963 (0.008) | 0.932 (0.009) | 0.957 | 0.982 (0.02) | 1.042 (0.03) | |||||||||
| log(Luminosity) | [L☉] | |||||||||||||||
| Cooling age | [Gyr] | 2.4600 | 2.3030 | |||||||||||||
| 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] | 16.00 (0.06) | 15.93 (0.09) | 15.93 (0.09) | 16.00 | 16.00 (0.06) | 15.93 (0.09) | |||||||||
| Distance | [pc] | 62.49 (0.2) | 62.77 (0.4) | 62.79 (0.3) | 62.49 | 62.49 (0.2) | 62.79 (0.3) | |||||||||
| Composition | H | H | H | |||||||||||||
| Proper motion (right ascension) | [mas/yr] | -126.577344 (0.07) | -126.6472335 (0.2) | -126.577 (0.07) | -126.6472335 | |||||||||||
| Proper motion (declination) | [mas/yr] | 64.78699997 (0.08) | 64.55257681 (0.2) | 64.787 (0.08) | 64.55257681 | |||||||||||
| Variability | ||||||||||||||||
| Magnetic | ||||||||||||||||
| Bd | [MG] | |||||||||||||||
| Infrared excess (disk) | ||||||||||||||||
| Binarity | ||||||||||||||||
| B magnitude | ||||||||||||||||
| V magnitude | ||||||||||||||||
| R magnitude | ||||||||||||||||
| I magnitude | ||||||||||||||||
| J magnitude | 17.20 (0.02) | |||||||||||||||
| H magnitude | ||||||||||||||||
| K magnitude | ||||||||||||||||
| u magnitude | 17.92 (0.01) | 17.87 (0.01) | 17.92 (0.01) | 17.92 (0.01) | 17.88 (0.02) | |||||||||||
| g magnitude | 17.54 (0.005) | 17.54 (0.005) | 17.54 (0.005) | 17.53 (0.02) | ||||||||||||
| r magnitude | 17.55 (0.005) | 17.55 (0.005) | 17.55 (0.005) | 17.52 (0.01) | ||||||||||||
| i magnitude | 17.60 (0.007) | 17.60 (0.007) | 17.60 (0.007) | 17.59 (0.01) | ||||||||||||
| z magnitude | 17.70 (0.02) | 17.70 (0.02) | 17.70 (0.02) | 17.70 (0.02) | ||||||||||||
| G magnitude | 17.45 (0.007) | 17.47 | 17.45 | 17.45 (0.003) | 17.47 | |||||||||||
| BP magnitude | 17.56 (0.007) | 17.54 | 17.54 | |||||||||||||
| RP magnitude | 17.32 (0.01) | 17.31 | 17.31 | |||||||||||||
| Pan g magnitude | 17.49 (0.005) | 17.49 (0.005) | ||||||||||||||
| Pan r magnitude | 17.53 (0.004) | 17.53 (0.005) | ||||||||||||||
| Pan i magnitude | 17.61 (0.002) | 17.61 (0.002) | ||||||||||||||
| Pan z magnitude | 17.73 (0.006) | 17.73 (0.008) | ||||||||||||||
| Pan y magnitude | 17.79 (0.007) | 17.79 (0.007) | ||||||||||||||
| E(B-V) | 0.009 | |||||||||||||||
* Constant surface field
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