SDSS J234325.49+083725.2
All names: Gaia EDR3 2759588063311504768, USNO-B1.0 0986-00632542, SDSS J234325.48+083725.0, Gaia DR3 2759588063311504768, SDSS J234325.49+083725.2, SDSS J234325.48+083724.9, Gaia DR2 2759588063311504768, LP 583-36, J2343+0837, WDJ234325.54+083726.31, SDSS J234325.49+083725.0, LSPM J2343+0837, NLTT 57772
| 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 | 23 43 25.41 (0.08) | 23 43 25.49 | 23 43 25.42 (0.1) | 23 43 25.41 | 23 43 25.54 (0.08) | 23 43 25.42 | 23 43 25.49 | ||||||||
| Declination | 08 37 23.27 (0.06) | 08 37 24.97 | 08 37 23.36 (0.06) | 08 37 23.27 | 08 37 26.31 (0.06) | 08 37 23.36 | 08 37 25.02 | ||||||||
| Spectral type | DA | DA | DA | DA | DA | DA | DA | DA | |||||||
| Effective temperature | [K] | 6696.0 (52) | 6836.0 (39) | 6695.0 (52) | 6638.0 | 7035.0 (83) | 6696.0 (34) | ||||||||
| log(g) | [cgs] | 7.93 (0.01) | 7.98 (0.01) | 7.92 (0.01) | 7.90 | 8.05 (0.02) | 7.39 (0.1) | ||||||||
| Mass | [M☉] | 0.553 (0.01) | 0.579 (0.01) | 0.545 (0.01) | 0.534 | 0.621 (0.02) | 0.342 (0.03) | ||||||||
| log(Luminosity) | [L☉] | ||||||||||||||
| Cooling age | [Gyr] | 1.6100 | 1.5020 | ||||||||||||
| 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] | 17.61 (0.1) | 17.46 (0.1) | 17.46 (0.1) | 17.61 | 17.61 (0.1) | 17.46 (0.1) | ||||||||
| Distance | [pc] | 56.80 (0.3) | 57.27 (0.5) | 57.26 (0.5) | 56.80 | 56.80 (0.3) | 57.26 (0.5) | ||||||||
| Composition | H | H | H | ||||||||||||
| Proper motion (right ascension) | [mas/yr] | -118.461837 (0.1) | -118.7853856 (0.2) | -118.462 (0.1) | -118.7853856 | ||||||||||
| Proper motion (declination) | [mas/yr] | -190.4140201 (0.08) | -190.4260817 (0.1) | -190.414 (0.08) | -190.4260817 | ||||||||||
| Variability | |||||||||||||||
| Magnetic | |||||||||||||||
| Bd | [MG] | ||||||||||||||
| Infrared excess (disk) | |||||||||||||||
| Binarity | |||||||||||||||
| B magnitude | 17.80 | ||||||||||||||
| V magnitude | |||||||||||||||
| R magnitude | 17.40 | ||||||||||||||
| I magnitude | |||||||||||||||
| J magnitude | 16.55 (0.01) | 16.55 (0.01) | |||||||||||||
| H magnitude | 16.42 (0.03) | 16.42 (0.03) | |||||||||||||
| K magnitude | 16.33 (0.04) | 16.33 (0.04) | |||||||||||||
| u magnitude | 18.13 (0.01) | 18.10 (0.01) | 18.13 (0.01) | 18.10 (0.01) | 18.09 (0.02) | ||||||||||
| g magnitude | 17.50 (0.005) | 17.50 (0.005) | 17.50 (0.005) | 17.52 (0.02) | |||||||||||
| r magnitude | 17.30 (0.005) | 17.30 (0.005) | 17.28 (0.005) | 17.30 (0.01) | |||||||||||
| i magnitude | 17.24 (0.006) | 17.24 (0.006) | 17.22 (0.006) | 17.23 (0.01) | |||||||||||
| z magnitude | 17.22 (0.01) | 17.22 (0.01) | 17.23 (0.01) | 17.24 (0.02) | |||||||||||
| G magnitude | 17.27 (0.01) | 17.29 | 17.27 | 17.27 (0.003) | 17.29 | ||||||||||
| BP magnitude | 17.49 (0.01) | 17.48 | 17.48 | ||||||||||||
| RP magnitude | 16.92 (0.007) | 16.91 | 16.91 | ||||||||||||
| Pan g magnitude | 17.46 (0.2) | 17.46 (0.2) | |||||||||||||
| Pan r magnitude | 17.30 (0.004) | 17.30 (0.005) | |||||||||||||
| Pan i magnitude | 17.24 (0.004) | 17.24 (0.004) | |||||||||||||
| Pan z magnitude | 17.27 (0.005) | 17.27 (0.004) | |||||||||||||
| Pan y magnitude | 17.28 (0.009) | 17.28 (0.009) | |||||||||||||
| E(B-V) | 0.003 | ||||||||||||||
* 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
