Gaia DR2 2393834386459511680
All names: Gaia DR3 2393834386459511680, GD 1222, PSO J355.1832-18.3297, Gaia DR2 2393834386459511680, USNO-B1.0 0716-00902976, Gaia EDR3 2393834386459511680, J2340-1819, DENIS J234043.9-181945, WDJ234043.98-181945.62
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Jewett et al. 2024 | Kilic et al. 2024 | MWDD H | MWDD HE | Gaia DR2 | Stilism | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 23 40 43.98 (0.1) | 23 40 43.98 | 23 40 43.98 | 23 40 43.98 (0.1) | 23 40 43.98 | |||||||
| Declination | -18 19 47.45 (0.1) | -18 19 47.40 | -18 19 47.45 | -18 19 45.63 (0.1) | -18 19 47.40 | |||||||
| Spectral type | DAQ | DAQ | DA | DAQ | ||||||||
| Effective temperature | [K] | 15836.0 (291) | 15836.0 (291) | 15819.0 | 15705.0 | 20342.0 (836) | ||||||
| log(g) | [cgs] | 8.95 | 8.95 (0.02) | 8.87 | 8.89 | 9.08 (0.03) | ||||||
| Mass | [M☉] | 1.167 (0.01) | 1.167 (0.01) | 1.142 | 1.138 | 1.232 (0.01) | ||||||
| log(Luminosity) | [L☉] | |||||||||||
| Cooling age | [Gyr] | 0.9700 (0.05) | 0.9700 (0.05) | 0.8139 | 0.8598 | |||||||
| log(H/He) | ||||||||||||
| log(C/He) | ||||||||||||
| log(Ca/He) | ||||||||||||
| log(Ca/H) | ||||||||||||
| Parallax | [mas] | 10.58 (0.2) | 10.38 (0.2) | 10.58 | 10.58 (0.2) | 10.38 (0.2) | ||||||
| Distance | [pc] | 94.50 (1) | 96.30 (2) | 94.50 | 94.50 (1) | 96.30 (2) | ||||||
| Composition | C | |||||||||||
| Proper motion (right ascension) | [mas/yr] | -0.583771862 (0.1) | -0.545047624 (0.3) | -0.584 (0.1) | -0.545047624 | |||||||
| Proper motion (declination) | [mas/yr] | -114.1842465 (0.1) | -114.4156672 (0.3) | -114.184 (0.1) | -114.4156672 | |||||||
| Variability | ||||||||||||
| Magnetic | ||||||||||||
| Bd | [MG] | |||||||||||
| Infrared excess (disk) | ||||||||||||
| Binarity | ||||||||||||
| B magnitude | 18.30 | |||||||||||
| V magnitude | ||||||||||||
| R magnitude | 17.90 | |||||||||||
| I magnitude | 17.88 (0.2) | |||||||||||
| J magnitude | ||||||||||||
| H magnitude | ||||||||||||
| K magnitude | ||||||||||||
| u magnitude | ||||||||||||
| g magnitude | 17.52 (0.009) | |||||||||||
| r magnitude | 17.78 (0.006) | |||||||||||
| i magnitude | 18.04 (0.003) | |||||||||||
| z magnitude | 18.29 (0.004) | |||||||||||
| G magnitude | 17.60 (0.008) | 17.63 | 17.60 | 17.60 (0.003) | 17.63 | |||||||
| BP magnitude | 17.54 (0.008) | 17.51 | 17.51 | |||||||||
| RP magnitude | 17.75 (0.01) | 17.75 | 17.75 | |||||||||
| Pan g magnitude | 17.52 (0.009) | |||||||||||
| Pan r magnitude | 17.78 (0.006) | |||||||||||
| Pan i magnitude | 18.04 (0.003) | |||||||||||
| Pan z magnitude | 18.29 (0.004) | |||||||||||
| Pan y magnitude | 18.45 (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
