SDSS J141303.59+325646.0
All names: SDSS J141303.59+325646.0, WIRED J141303.59+325646.0, J1413+3256, Gaia DR3 1478514389681253248, 2MASS J14130362+3256468, SDSS J141303.60+325646.0, SDSS J141303.58+325646.0, WDJ141303.62+325646.22, Gaia EDR3 1478514389681253248, TIC 105715029, Gaia DR2 1478514389681253248, GALEX J141303.5+325645, SDSS J141303.58+325645.9, LAMOST J141303.59+325646.0
| 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 | 14 13 03.50 (0.03) | 14 13 03.58 | 14 13 03.51 (0.04) | 14 13 03.50 | 14 13 03.62 (0.03) | 14 13 03.51 | 14 13 03.60 | ||||||||
| Declination | 32 56 45.26 (0.04) | 32 56 46.00 | 32 56 45.29 (0.06) | 32 56 45.26 | 32 56 46.22 (0.04) | 32 56 45.29 | 32 56 46.01 | ||||||||
| Spectral type | DA | DA | DA | DA | DA | DA | DA | DA | |||||||
| Effective temperature | [K] | 10097.0 (42) | 10135.0 (41) | 10096.0 (42) | 10152.0 | 10085.0 (79) | 10165.0 (33) | ||||||||
| log(g) | [cgs] | 7.96 (0.008) | 7.97 (0.01) | 7.97 (0.01) | 7.97 | 7.96 (0.01) | 8.16 (0.04) | ||||||||
| Mass | [M☉] | 0.575 (0.006) | 0.586 (0.008) | 0.581 (0.008) | 0.586 | 0.576 (0.01) | 0.692 (0.03) | ||||||||
| log(Luminosity) | [L☉] | ||||||||||||||
| Cooling age | [Gyr] | 0.5900 | 0.5614 | ||||||||||||
| 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] | 11.81 (0.06) | 11.89 (0.08) | 11.89 (0.08) | 11.81 | 11.81 (0.06) | 11.89 (0.08) | ||||||||
| Distance | [pc] | 84.65 (0.4) | 84.10 (0.6) | 84.12 (0.6) | 84.65 | 84.65 (0.4) | 84.12 (0.6) | ||||||||
| Composition | H | H | H | ||||||||||||
| Proper motion (right ascension) | [mas/yr] | -91.32047775 (0.03) | -91.24049936 (0.07) | -91.32 (0.03) | -91.24049936 | ||||||||||
| Proper motion (declination) | [mas/yr] | -60.13537632 (0.05) | -60.03389367 (0.1) | -60.135 (0.05) | -60.03389367 | ||||||||||
| Variability | |||||||||||||||
| Magnetic | |||||||||||||||
| Bd | [MG] | ||||||||||||||
| Infrared excess (disk) | |||||||||||||||
| Binarity | |||||||||||||||
| B magnitude | |||||||||||||||
| V magnitude | |||||||||||||||
| R magnitude | |||||||||||||||
| I magnitude | |||||||||||||||
| J magnitude | 16.84 (0.2) | 16.84 (0.2) | |||||||||||||
| H magnitude | 16.54 (0.2) | 16.54 (0.2) | |||||||||||||
| K magnitude | |||||||||||||||
| u magnitude | 17.14 (0.009) | 17.15 (0.009) | 17.14 (0.009) | 17.17 (0.009) | 17.15 (0.03) | ||||||||||
| g magnitude | 16.70 (0.004) | 16.70 (0.004) | 16.68 (0.004) | 16.79 (0.02) | |||||||||||
| r magnitude | 16.81 (0.004) | 16.81 (0.004) | 16.80 (0.004) | 16.80 (0.01) | |||||||||||
| i magnitude | 16.94 (0.005) | 16.94 (0.005) | 16.94 (0.005) | 16.91 (0.02) | |||||||||||
| z magnitude | 17.09 (0.01) | 17.09 (0.01) | 17.13 (0.01) | 17.13 (0.02) | |||||||||||
| G magnitude | 16.71 (0.004) | 16.73 | 16.71 | 16.71 (0.003) | 16.73 | ||||||||||
| BP magnitude | 16.77 (0.004) | 16.76 | 16.76 | ||||||||||||
| RP magnitude | 16.63 (0.004) | 16.64 | 16.64 | ||||||||||||
| Pan g magnitude | 16.70 (0.003) | 16.70 (0.003) | |||||||||||||
| Pan r magnitude | 16.80 (0.005) | 16.80 (0.005) | |||||||||||||
| Pan i magnitude | 16.94 (0.002) | 16.94 (0.003) | |||||||||||||
| Pan z magnitude | 17.13 (0.003) | 17.13 (0.004) | |||||||||||||
| Pan y magnitude | 17.23 (0.003) | 17.23 (0.003) | |||||||||||||
| E(B-V) | 0.006 | ||||||||||||||
* Constant surface field
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