SDSS J131730.85+483332.8
All names: Gaia DR2 1556005701461744640, Gaia EDR3 1556005701461744640, GALEX J131730.9+483334, SDSS J131730.85+483332.7, WDJ131730.86+483333.05, SDSS J131730.85+483332.80, SDSS J131730.85+483332.8, SDSS J131730.84+483332.7, Gaia DR3 1556005701461744640, J1317+4833
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Kilic et al. 2025 | O'Brien et al. 2024 | Caron et al. 2023 | McCleery et al. 2020 | Kilic et al. 2020 | MWDD H | Gaia DR2 | Stilism | Kepler et al. 2016 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | Vincent et al. 2023 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 13 17 30.75 (0.04) | 13 17 30.85 | 13 17 30.75 (0.05) | 13 17 30.75 (0.05) | 13 17 30.75 | 13 17 30.86 (0.04) | 13 17 30.75 | ||||||||||
| Declination | 48 33 31.24 (0.05) | 48 33 32.78 | 48 33 31.30 (0.05) | 48 33 31.30 (0.05) | 48 33 31.24 | 48 33 33.05 (0.05) | 48 33 31.30 | ||||||||||
| Spectral type | DA | DA | DA | DA | DA | DA | DA | DA | DA | DA | DA | ||||||
| Effective temperature | [K] | 5904.0 (22) | 5798.0 (54) | 5885.0 (19) | 5786.7 (47) | 5903.0 (22) | 5788.0 | 6000.0 (1000) | 6034.0 (32) | ||||||||
| log(g) | [cgs] | 8.05 (0.008) | 8.00 (0.03) | 8.03 (0.008) | 8.00 (0.03) | 8.04 (0.008) | 7.99 | 7.95 (0.5) | 8.11 (0.01) | ||||||||
| Mass | [M☉] | 0.618 (0.007) | 0.585 (0.02) | 0.608 (0.007) | 0.613 (0.007) | 0.581 | 0.658 (0.009) | ||||||||||
| log(Luminosity) | [L☉] | ||||||||||||||||
| Cooling age | [Gyr] | 2.6300 | 2.4520 | ||||||||||||||
| 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] | 25.63 (0.06) | 25.63 (0.06) | 25.53 (0.07) | 25.53 (0.07) | 25.53 (0.07) | 25.63 | 25.63 (0.06) | 25.53 (0.07) | ||||||||
| Distance | [pc] | 39.01 (0.08) | 39.02 (0.09) | 39.17 (0.1) | 39.18 (0.1) | 39.18 (0.1) | 39.01 | 39.01 (0.08) | 39.18 (0.1) | ||||||||
| Composition | H | H | H | H | |||||||||||||
| Proper motion (right ascension) | [mas/yr] | -68.77859863 (0.05) | -68.86903253 (0.08) | -68.779 (0.04) | -68.869 | ||||||||||||
| Proper motion (declination) | [mas/yr] | -113.211447 (0.06) | -113.2502567 (0.09) | -113.211 (0.07) | -113.25 | ||||||||||||
| Variability | |||||||||||||||||
| Magnetic | |||||||||||||||||
| Bd | [MG] | ||||||||||||||||
| Infrared excess (disk) | |||||||||||||||||
| Binarity | |||||||||||||||||
| B magnitude | |||||||||||||||||
| V magnitude | |||||||||||||||||
| R magnitude | |||||||||||||||||
| I magnitude | |||||||||||||||||
| J magnitude | |||||||||||||||||
| H magnitude | |||||||||||||||||
| K magnitude | |||||||||||||||||
| u magnitude | 18.44 (0.01) | 18.44 (0.01) | 18.42 (0.02) | 18.44 (0.01) | 18.44 (0.01) | ||||||||||||
| g magnitude | 17.52 (0.005) | 17.52 (0.02) | 17.52 (0.005) | 17.52 (0.005) | |||||||||||||
| r magnitude | 17.13 (0.005) | 17.16 (0.02) | 17.13 (0.005) | 17.13 (0.005) | |||||||||||||
| i magnitude | 16.99 (0.005) | 16.99 (0.02) | 16.99 (0.005) | 16.99 (0.005) | |||||||||||||
| z magnitude | 17.08 (0.01) | 17.07 (0.1) | 17.08 (0.01) | 17.08 (0.01) | |||||||||||||
| G magnitude | 17.13 (0.005) | 17.15 | 17.15 | 17.13 | 17.13 (0.003) | 17.15 | |||||||||||
| BP magnitude | 17.44 (0.005) | 17.45 | 17.45 | ||||||||||||||
| RP magnitude | 16.62 (0.007) | 16.63 | 16.63 | ||||||||||||||
| Pan g magnitude | 17.49 (0.005) | 17.49 (0.005) | |||||||||||||||
| Pan r magnitude | 17.12 (0.004) | 17.12 (0.005) | |||||||||||||||
| Pan i magnitude | 16.97 (0.005) | 16.97 (0.003) | |||||||||||||||
| Pan z magnitude | 16.97 (0.01) | 16.97 (0.01) | |||||||||||||||
| Pan y magnitude | 16.92 (0.01) | 16.92 (0.01) | |||||||||||||||
| E(B-V) | 0.002 | ||||||||||||||||
* 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
