Gaia DR2 396963005168870528
All names: Gaia DR2 396963005168870528, WDJ013055.01+441423.28, J0130+4414, TIC 326914735, Gaia EDR3 396963005168870528, WDJ013055.01+441423.29, 2MASS J01305500+4414235, Gaia DR3 396963005168870528, SDSS J013055.07+441423.7
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Kilic et al. 2025 | O'Brien et al. 2024 | Caron et al. 2023 | Blouin & Xu 2022 | McCleery et al. 2020 | Tremblay et al. 2020 | MWDD H | MWDD HE | Gaia DR2 | Stilism | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 01 30 55.19 (0.09) | 01 30 55.18 (0.1) | 01 30 55.18 | 01 30 55.19 | 01 30 55.02 (0.09) | 01 30 55.18 | ||||||||||
| Declination | 44 14 24.67 (0.08) | 44 14 24.63 (0.1) | 44 14 24.63 | 44 14 24.67 | 44 14 23.29 (0.08) | 44 14 24.63 | ||||||||||
| Spectral type | DZA | DZA | DZA | DZA | DZA | DC: | DZA | |||||||||
| Effective temperature | [K] | 4985.0 (18) | 4964.0 (65) | 4998.0 (18) | 5005.0 (15) | 4987.8 (43) | 4990.0 (40) | 4999.0 | 4681.0 | 5045.0 (45) | ||||||
| log(g) | [cgs] | 7.98 (0.01) | 7.97 (0.05) | 7.98 (0.01) | 8.00 (0.01) | 7.99 (0.04) | 7.99 (0.04) | 7.99 | 7.77 | 8.04 (0.02) | ||||||
| Mass | [M☉] | 0.555 (0.008) | 0.56 (0.03) | 0.555 (0.009) | 0.578 (0.009) | 0.573 | 0.438 | 0.603 (0.02) | ||||||||
| log(Luminosity) | [L☉] | |||||||||||||||
| Cooling age | [Gyr] | 5.6700 | 5.8700 | 5.5590 | 4.2450 | |||||||||||
| log(H/He) | ||||||||||||||||
| log(C/He) | ||||||||||||||||
| log(Ca/He) | -9.72 | |||||||||||||||
| log(Ca/H) | -9.7 | -9.63 (0.07) | ||||||||||||||
| 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] | 26.20 (0.1) | 26.20 (0.1) | 26.02 (0.1) | 26.20 (0.1) | 26.02 (0.1) | 26.02 (0.1) | 26.20 | 26.20 (0.1) | 26.02 (0.1) | ||||||
| Distance | [pc] | 38.17 (0.2) | 38.17 (0.1) | 38.43 (0.2) | 38.17 (0.1) | 38.43 (0.2) | 38.43 (0.2) | 38.17 | 38.17 (0.2) | 38.43 (0.2) | ||||||
| Composition | H | H | H | |||||||||||||
| Proper motion (right ascension) | [mas/yr] | 115.5161983 (0.1) | 115.6003559 (0.3) | 115.516 (0.1) | 115.6003559 | |||||||||||
| Proper motion (declination) | [mas/yr] | 86.40458793 (0.1) | 86.64399195 (0.3) | 86.405 (0.1) | 86.64399195 | |||||||||||
| Variability | ||||||||||||||||
| Magnetic | ||||||||||||||||
| Bd | [MG] | |||||||||||||||
| Infrared excess (disk) | ||||||||||||||||
| Binarity | ||||||||||||||||
| B magnitude | ||||||||||||||||
| V magnitude | ||||||||||||||||
| R magnitude | ||||||||||||||||
| I magnitude | ||||||||||||||||
| J magnitude | 16.65 (0.1) | 16.65 (0.1) | ||||||||||||||
| H magnitude | 16.30 (0.2) | 16.30 (0.2) | ||||||||||||||
| K magnitude | ||||||||||||||||
| u magnitude | 20.06 (0.04) | 20.06 (0.04) | 20.06 (0.04) | |||||||||||||
| g magnitude | 18.46 (0.007) | 18.46 (0.007) | ||||||||||||||
| r magnitude | 17.75 (0.006) | 17.75 (0.006) | ||||||||||||||
| i magnitude | 17.47 (0.006) | 17.47 (0.006) | ||||||||||||||
| z magnitude | 17.33 (0.01) | 17.33 (0.01) | ||||||||||||||
| G magnitude | 17.77 (0.01) | 17.79 | 17.79 | 17.77 | 17.77 (0.003) | 17.79 | ||||||||||
| BP magnitude | 18.28 (0.01) | 18.26 | 18.26 | |||||||||||||
| RP magnitude | 17.15 (0.008) | 17.16 | 17.16 | |||||||||||||
| Pan g magnitude | 18.35 (0.007) | 18.35 (0.006) | 18.35 (0.007) | |||||||||||||
| Pan r magnitude | 17.74 (0.006) | 17.74 (0.006) | 17.74 (0.006) | |||||||||||||
| Pan i magnitude | 17.49 (0.004) | 17.49 (0.004) | 17.49 (0.004) | |||||||||||||
| Pan z magnitude | 17.39 (0.007) | 17.39 (0.008) | 17.39 (0.007) | |||||||||||||
| Pan y magnitude | 17.37 (0.007) | 17.37 (0.007) | 17.37 (0.007) | |||||||||||||
| E(B-V) | 0.001 | |||||||||||||||
* 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
