CSO 1001
All names: Gaia DR3 1471998511973713152, 2MASS J13350114+3609591, SDSS J133501.10+360959.5, WISE J133501.00+360959.8, J1335+3610, TIC 22817483, SDSS J133501.10+360959.4, WISEA J133501.01+360959.7, SDSS J133501.09+360959.4, WIRED J133501.09+360959.4, Gaia DR2 1471998511973713152, CSO 1001, Gaia EDR3 1471998511973713152, WDJ133501.14+360959.22
| 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 | 13 35 00.98 (0.03) | 13 35 01.10 | 13 35 00.99 (0.05) | 13 35 00.98 | 13 35 01.14 (0.03) | 13 35 00.99 | 13 35 01.10 | ||||||||
| Declination | 36 10 00.25 (0.03) | 36 09 59.47 | 36 10 00.22 (0.05) | 36 10 00.25 | 36 09 59.22 (0.03) | 36 10 00.22 | 36 09 59.46 | ||||||||
| Spectral type | DA | DA | DA | DA | DA | DA | DA | DA | |||||||
| Effective temperature | [K] | 10040.0 (64) | 10050.0 (57) | 10040.0 (64) | 9884.0 | 10043.0 (67) | 10056.0 (22) | ||||||||
| log(g) | [cgs] | 7.98 (0.01) | 7.99 (0.01) | 7.99 (0.01) | 7.96 | 7.99 (0.01) | 8.29 (0.02) | ||||||||
| Mass | [M☉] | 0.59 (0.009) | 0.593 (0.009) | 0.593 (0.009) | 0.577 | 0.594 (0.01) | 0.772 (0.01) | ||||||||
| log(Luminosity) | [L☉] | ||||||||||||||
| Cooling age | [Gyr] | 0.6200 | 0.5902 | ||||||||||||
| 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] | 12.59 (0.06) | 12.62 (0.08) | 12.62 (0.08) | 12.59 | 12.59 (0.06) | 12.62 (0.08) | ||||||||
| Distance | [pc] | 79.42 (0.4) | 79.24 (0.5) | 79.25 (0.5) | 79.42 | 79.42 (0.4) | 79.25 (0.5) | ||||||||
| Composition | H | H | H | ||||||||||||
| Proper motion (right ascension) | [mas/yr] | -118.3275053 (0.03) | -118.5551879 (0.1) | -118.328 (0.03) | -118.5551879 | ||||||||||
| Proper motion (declination) | [mas/yr] | 64.69693755 (0.04) | 64.63725703 (0.1) | 64.697 (0.04) | 64.63725703 | ||||||||||
| Variability | |||||||||||||||
| Magnetic | |||||||||||||||
| Bd | [MG] | ||||||||||||||
| Infrared excess (disk) | |||||||||||||||
| Binarity | |||||||||||||||
| B magnitude | |||||||||||||||
| V magnitude | |||||||||||||||
| R magnitude | |||||||||||||||
| I magnitude | |||||||||||||||
| J magnitude | 16.60 (0.02) | 16.43 (0.09) | |||||||||||||
| H magnitude | 16.49 (0.02) | 16.37 (0.2) | |||||||||||||
| K magnitude | 16.56 (0.06) | 15.77 (0.2) | |||||||||||||
| u magnitude | 17.03 (0.008) | 17.02 (0.008) | 17.02 (0.008) | 17.02 (0.008) | 17.04 (0.03) | ||||||||||
| g magnitude | 16.61 (0.004) | 16.61 (0.004) | 16.61 (0.004) | 16.62 (0.02) | |||||||||||
| r magnitude | 16.71 (0.004) | 16.71 (0.004) | 16.71 (0.004) | 16.70 (0.02) | |||||||||||
| i magnitude | 16.84 (0.005) | 16.84 (0.005) | 16.84 (0.005) | 16.83 (0.03) | |||||||||||
| z magnitude | 17.03 (0.01) | 17.03 (0.01) | 17.03 (0.01) | 17.05 (0.02) | |||||||||||
| G magnitude | 16.64 (0.003) | 16.66 | 16.64 | 16.64 (0.003) | 16.66 | ||||||||||
| BP magnitude | 16.69 (0.003) | 16.68 | 16.68 | ||||||||||||
| RP magnitude | 16.56 (0.004) | 16.57 | 16.57 | ||||||||||||
| Pan g magnitude | 16.65 (0.007) | 16.65 (0.008) | |||||||||||||
| Pan r magnitude | 16.73 (0.003) | 16.73 (0.003) | |||||||||||||
| Pan i magnitude | 16.87 (0.004) | 16.87 (0.003) | |||||||||||||
| Pan z magnitude | 17.03 (0.003) | 17.03 (0.003) | |||||||||||||
| Pan y magnitude | 17.13 (0.01) | 17.13 (0.01) | |||||||||||||
| E(B-V) | 0.005 | ||||||||||||||
* 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
