SDSS J121135.18+205340.8
All names: 2MASS J12113516+2053407, Gaia DR3 3951770649948609920, PSO J182.8964+20.8945, Gaia DR2 3951770649948609920, TIC 357290255, SDSS J121135.18+205340.8, J1211+2053, SDSS J121135.18+205340.7, WDJ121135.20+205340.93, Gaia EDR3 3951770649948609920, GALEX J121135.3+205341
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Caron et al. 2023 | Kilic et al. 2020 | Blouin et al. 2019 | 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 | 12 11 35.16 (0.09) | 12 11 35.18 | 12 11 35.16 (0.1) | 12 11 35.16 | 12 11 35.20 (0.09) | 12 11 35.16 | 12 11 35.18 | ||||||||
| Declination | 20 53 40.32 (0.08) | 20 53 40.76 | 20 53 40.34 (0.1) | 20 53 40.32 | 20 53 40.93 (0.08) | 20 53 40.34 | 20 53 40.78 | ||||||||
| Spectral type | DA | DA | DA | DA | DA | DA | DA | DA | |||||||
| Effective temperature | [K] | 6733.0 (29) | 6687.0 (30) | 6660.0 (60) | 6676.0 | 6799.0 (93) | 6539.0 (29) | ||||||||
| log(g) | [cgs] | 7.19 (0.02) | 7.17 (0.02) | 7.16 (0.04) | 7.16 | 7.17 (0.03) | 7.53 (0.07) | ||||||||
| Mass | [M☉] | 0.239 (0.007) | 0.235 (0.008) | 0.235 (0.009) | 0.234 | 0.237 (0.01) | |||||||||
| log(Luminosity) | [L☉] | ||||||||||||||
| Cooling age | [Gyr] | 0.6800 | 0.7710 (0.02) | 0.7649 | |||||||||||
| 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] | 9.80 (0.1) | 10.04 (0.2) | 10.04 (0.2) | 10.04 (0.2) | 9.80 | 9.80 (0.1) | 10.04 (0.2) | |||||||
| Distance | [pc] | 102.02 (1) | 99.60 (2) | 99.62 (2) | 99.62 (2) | 102.02 | 102.02 (1) | 99.62 (2) | |||||||
| Composition | H | H | H | ||||||||||||
| Proper motion (right ascension) | [mas/yr] | -36.9383302 (0.1) | -37.15491646 (0.2) | -36.938 (0.1) | -37.15491646 | ||||||||||
| Proper motion (declination) | [mas/yr] | -38.31619921 (0.09) | -38.21324962 (0.3) | -38.316 (0.09) | -38.21324962 | ||||||||||
| Variability | |||||||||||||||
| Magnetic | |||||||||||||||
| Bd | [MG] | ||||||||||||||
| Infrared excess (disk) | |||||||||||||||
| Binarity | |||||||||||||||
| B magnitude | |||||||||||||||
| V magnitude | |||||||||||||||
| R magnitude | |||||||||||||||
| I magnitude | |||||||||||||||
| J magnitude | 16.81 (0.02) | 16.74 (0.1) | 16.74 (0.1) | ||||||||||||
| H magnitude | |||||||||||||||
| K magnitude | 15.88 (0.2) | 15.88 (0.2) | |||||||||||||
| u magnitude | 18.38 (0.02) | 18.38 (0.02) | 18.38 (0.02) | 18.38 (0.02) | 18.39 (0.02) | ||||||||||
| g magnitude | 17.77 (0.006) | 17.75 (0.005) | 17.77 (0.006) | 17.79 (0.04) | |||||||||||
| r magnitude | 17.53 (0.006) | 17.55 (0.004) | 17.53 (0.006) | 17.52 (0.01) | |||||||||||
| i magnitude | 17.46 (0.006) | 17.48 (0.005) | 17.46 (0.006) | 17.44 (0.02) | |||||||||||
| z magnitude | 17.48 (0.01) | 17.53 (0.004) | 17.48 (0.01) | 17.50 (0.02) | |||||||||||
| G magnitude | 17.52 (0.007) | 17.53 | 17.52 | 17.52 (0.003) | 17.53 | ||||||||||
| BP magnitude | 17.75 (0.007) | 17.73 | 17.73 | ||||||||||||
| RP magnitude | 17.16 (0.009) | 17.16 | 17.16 | ||||||||||||
| Pan g magnitude | 17.75 (0.005) | 17.75 (0.005) | 17.75 (0.005) | ||||||||||||
| Pan r magnitude | 17.55 (0.003) | 17.55 (0.004) | 17.55 (0.004) | ||||||||||||
| Pan i magnitude | 17.48 (0.004) | 17.48 (0.005) | 17.48 (0.005) | ||||||||||||
| Pan z magnitude | 17.53 (0.004) | 17.53 (0.003) | 17.53 (0.003) | ||||||||||||
| Pan y magnitude | 17.53 (0.008) | 17.53 (0.008) | 17.53 (0.008) | ||||||||||||
| E(B-V) | 0.004 | ||||||||||||||
* Constant surface field
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