Gaia DR2 1563853976804546688
All names: SDSS J132002.69+553048.1, WDJ132002.68+553048.24, Gaia DR2 1563853976804546688, SDSS J132002.68+553048.0, Gaia EDR3 1563853976804546688, WDJ13202.68+553048.23, Gaia DR3 1563853976804546688, J1320+5530
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Kilic et al. 2025 | Caron et al. 2023 | Kilic et al. 2020 | MWDD H | MWDD HE | Gaia DR2 | Stilism | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 13 20 02.70 (0.2) | 13 20 02.70 | 13 20 02.70 | 13 20 02.68 (0.2) | 13 20 02.70 | ||||||||
| Declination | 55 30 47.30 (0.2) | 55 30 47.33 | 55 30 47.30 | 55 30 48.24 (0.2) | 55 30 47.33 | ||||||||
| Spectral type | DC | DC | DC | DA | DC | ||||||||
| Effective temperature | [K] | 5811.0 (74) | 5770.0 (74) | 5536.0 (71) | 6171.0 | 5928.0 | 6154.0 (169) | ||||||
| log(g) | [cgs] | 8.11 (0.04) | 8.08 (0.04) | 7.91 (0.04) | 8.27 | 8.14 | 8.29 (0.06) | ||||||
| Mass | [M☉] | 0.64 (0.03) | 0.618 (0.04) | 0.517 (0.04) | 0.761 | 0.658 | 0.772 (0.05) | ||||||
| log(Luminosity) | [L☉] | ||||||||||||
| Cooling age | [Gyr] | 3.8900 | 3.8430 | 3.7760 | |||||||||
| log(H/He) | -5 | ||||||||||||
| log(C/He) | |||||||||||||
| log(Ca/He) | |||||||||||||
| log(Ca/H) | |||||||||||||
| log(N/He) | |||||||||||||
| log(O/He) | |||||||||||||
| log(Na/He) | |||||||||||||
| log(Mg/He) | |||||||||||||
| log(Al/He) | |||||||||||||
| log(Si/He) | |||||||||||||
| log(P/He) | |||||||||||||
| log(S/He) | |||||||||||||
| log(Cl/He) | |||||||||||||
| log(Sc/He) | |||||||||||||
| log(Ti/He) | |||||||||||||
| log(V/He) | |||||||||||||
| log(Cr/He) | |||||||||||||
| log(Mn/He) | |||||||||||||
| log(Fe/He) | |||||||||||||
| log(Co/He) | |||||||||||||
| log(Ni/He) | |||||||||||||
| log(Cu/He) | |||||||||||||
| log(Zn/He) | |||||||||||||
| log(Ga/He) | |||||||||||||
| log(Ge/He) | |||||||||||||
| log(Sr/He) | |||||||||||||
| Parallax | [mas] | 10.52 (0.2) | 10.38 (0.3) | 10.38 (0.3) | 10.52 | 10.52 (0.2) | 10.38 (0.3) | ||||||
| Distance | [pc] | 95.03 (2) | 96.34 (3) | 96.36 (3) | 95.03 | 95.03 (2) | 96.36 (3) | ||||||
| Composition | He | He | |||||||||||
| Proper motion (right ascension) | [mas/yr] | 10.54530988 (0.2) | 10.50641241 (0.4) | 10.545 (0.2) | 10.50641241 | ||||||||
| Proper motion (declination) | [mas/yr] | -58.78517305 (0.2) | -58.69912509 (0.5) | -58.785 (0.2) | -58.69912509 | ||||||||
| Variability | |||||||||||||
| Magnetic | |||||||||||||
| Bd | [MG] | ||||||||||||
| Infrared excess (disk) | |||||||||||||
| Binarity | |||||||||||||
| B magnitude | |||||||||||||
| V magnitude | |||||||||||||
| R magnitude | |||||||||||||
| I magnitude | |||||||||||||
| J magnitude | 18.52 (0.09) | ||||||||||||
| H magnitude | |||||||||||||
| K magnitude | |||||||||||||
| u magnitude | 20.57 (0.05) | 20.51 (0.05) | 20.51 (0.05) | ||||||||||
| g magnitude | 19.55 (0.01) | 19.55 (0.01) | |||||||||||
| r magnitude | 19.23 (0.01) | 19.23 (0.01) | |||||||||||
| i magnitude | 19.13 (0.02) | 19.13 (0.02) | |||||||||||
| z magnitude | 19.04 (0.04) | 19.04 (0.04) | |||||||||||
| G magnitude | 19.22 (0.04) | 19.26 | 19.22 | 19.22 (0.004) | 19.26 | ||||||||
| BP magnitude | 19.59 (0.04) | 19.52 | 19.52 | ||||||||||
| RP magnitude | 18.80 (0.04) | 18.75 | 18.75 | ||||||||||
| Pan g magnitude | 19.52 (0.02) | 19.52 (0.02) | |||||||||||
| Pan r magnitude | 19.21 (0.009) | 19.21 (0.008) | |||||||||||
| Pan i magnitude | 19.13 (0.008) | 19.13 (0.01) | |||||||||||
| Pan z magnitude | 19.10 (0.01) | 19.10 (0.01) | |||||||||||
| Pan y magnitude | 19.13 (0.03) | 19.13 (0.03) | |||||||||||
| E(B-V) | 0.007 | ||||||||||||
* 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
