2MASS J11505233+6831161
All names: Gaia DR2 1058284412796260480, 2MASS J11505233+6831161, SDSS J115052.32+683115.9, TIC 142905656, SDSS J115052.32+683116.0, SDSS J115052.33+683116.0, WDJ115052.33+683115.97, SDSS J115052.31+683116.0, SDSS, WIRED J115052.31+683116.0, PM J11508+6831, Gaia DR3 1058284412796260480, CNS5 2904, 11508+6831, SDSS J115052.32+683116.1, WD 1148+687, GALEX J115052.3+683115, SDSS J115052.35+683115.7, Gaia EDR3 1058284412796260480, PSO J177.7182+68.5209, J1150+6831
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Kilic et al. 2025 | O'Brien et al. 2024 | Caron et al. 2023 | Kilic et al. 2020 | McCleery et al. 2020 | Blouin et al. 2019 | MWDD H | Gaia DR2 | Stilism | Holberg et al. 2016 | Limoges et al. 2015 | Sion et al. 2014 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) | Kleinman et al. 2013 | Kleinman et al. 2004 | Vincent et al. 2023 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 11 50 52.40 (0.02) | 11 50 52.33 | 11 50 52.40 (0.02) | 11 50 52.40 (0.02) | 11 50 52.08 | 11 50 52.40 | 11 50 52.33 (0.02) | 11 50 52.40 | 11 50 51.58 | 11 50 52.32 | 11 50 52.32 | ||||||||||||
| Declination | 68 31 15.31 (0.02) | 68 31 15.97 | 68 31 15.34 (0.02) | 68 31 15.34 (0.02) | 68 31 15.60 | 68 31 15.31 | 68 31 15.97 (0.02) | 68 31 15.34 | 68 31 13.08 | 68 31 16.05 | 68 31 16.07 | ||||||||||||
| Spectral type | DA | DA | DA | DA | DA | DA | DA | DA | DA | DA9.0 | DA | DA7 | DA | DA | DA | DA | |||||||
| Effective temperature | [K] | 6709.0 (14) | 6696.0 (41) | 6783.0 (11) | 6709.0 (14) | 6679.2 (23) | 6695.0 (40) | 6681.0 | 6620.0 (13) | 6650.0 (95) | 5640.0 | 6755.0 (19) | 6619.0 (13) | ||||||||||
| log(g) | [cgs] | 8.27 (0.003) | 8.26 (0.02) | 8.30 (0.003) | 8.27 (0.003) | 8.26 (0.009) | 8.28 (0.01) | 8.26 | 8.24 (0.02) | 8.17 (0.05) | 8.28 (0.005) | 8.27 (0.02) | |||||||||||
| Mass | [M☉] | 0.762 (0.003) | 0.754 (0.01) | 0.781 (0.003) | 0.762 (0.003) | 0.765 (0.009) | 0.756 | 0.75 (0.01) | 0.69 (0.04) | 0.767 (0.004) | 0.754 (0.01) | ||||||||||||
| log(Luminosity) | [L☉] | -3.64 | |||||||||||||||||||||
| Cooling age | [Gyr] | 3.2300 | 3.0510 (0.1) | 2.9720 | 2.9600 | ||||||||||||||||||
| 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] | 58.51 (0.02) | 58.51 (0.02) | 58.51 (0.03) | 58.51 (0.03) | 58.51 (0.03) | 58.51 (0.03) | 58.51 | 58.51 (0.02) | 58.51 (0.03) | |||||||||||||
| Distance | [pc] | 17.09 (0.006) | 17.09 (0.006) | 17.09 (0.009) | 17.09 (0.008) | 17.09 (0.008) | 17.09 (0.008) | 16.96 (0.1) | 18.00 (0.6) | 13.20 | 17.09 | 17.09 (0.006) | 17.09 (0.008) | ||||||||||
| Composition | H | H | H | H | H | H | H | ||||||||||||||||
| Proper motion (right ascension) | [mas/yr] | 23.39590669 (0.02) | 23.39154245 (0.05) | 23.396 (0.02) | 23.392 | 16.0 | |||||||||||||||||
| Proper motion (declination) | [mas/yr] | -41.04559835 (0.03) | -41.16561173 (0.05) | -41.046 (0.03) | -41.166 | -38.0 | |||||||||||||||||
| Variability | |||||||||||||||||||||||
| Magnetic | |||||||||||||||||||||||
| Bd | [MG] | ||||||||||||||||||||||
| Infrared excess (disk) | |||||||||||||||||||||||
| Binarity | |||||||||||||||||||||||
| B magnitude | |||||||||||||||||||||||
| V magnitude | 15.25 | ||||||||||||||||||||||
| R magnitude | |||||||||||||||||||||||
| I magnitude | |||||||||||||||||||||||
| J magnitude | 14.46 (0.03) | 14.46 (0.03) | 14.46 (0.03) | ||||||||||||||||||||
| H magnitude | 14.22 (0.04) | 14.22 (0.04) | 14.22 (0.04) | ||||||||||||||||||||
| K magnitude | 14.22 (0.06) | 14.22 (0.06) | 14.22 (0.06) | ||||||||||||||||||||
| u magnitude | 16.01 (0.005) | 15.98 (0.005) | 16.01 (0.005) | 15.98 (0.005) | 15.97 | 15.99 (0.02) | 15.97 (0.02) | ||||||||||||||||
| g magnitude | 15.37 (0.003) | 15.37 (0.002) | 15.36 (0.003) | 15.40 | 15.40 (0.02) | 15.40 (0.02) | |||||||||||||||||
| r magnitude | 15.16 (0.004) | 15.15 (0.006) | 15.15 (0.004) | 15.14 | 15.15 (0.02) | 15.14 (0.02) | |||||||||||||||||
| i magnitude | 15.07 (0.004) | 15.11 (0.004) | 15.08 (0.004) | 15.05 | 15.06 (0.02) | 15.05 (0.02) | |||||||||||||||||
| z magnitude | 15.10 (0.005) | 15.13 (0.002) | 15.11 (0.005) | 15.10 | 15.11 (0.01) | 15.10 (0.01) | |||||||||||||||||
| G magnitude | 15.13 (0.002) | 15.14 | 15.14 | 15.13 | 15.13 (0.003) | 15.14 | |||||||||||||||||
| BP magnitude | 15.34 (0.002) | 15.35 | 15.35 | ||||||||||||||||||||
| RP magnitude | 14.76 (0.002) | 14.77 | 14.77 | ||||||||||||||||||||
| Pan g magnitude | 15.37 (0.003) | 15.37 (0.002) | 15.37 (0.002) | ||||||||||||||||||||
| Pan r magnitude | 15.15 (0.008) | 15.15 (0.006) | 15.15 (0.006) | ||||||||||||||||||||
| Pan i magnitude | 15.11 (0.004) | 15.11 (0.004) | 15.11 (0.004) | ||||||||||||||||||||
| Pan z magnitude | 15.13 (0.002) | 15.13 (0.002) | 15.13 (0.002) | ||||||||||||||||||||
| Pan y magnitude | 15.15 (0.003) | 15.15 (0.003) | 15.15 (0.003) | ||||||||||||||||||||
| E(B-V) | 0.000 | ||||||||||||||||||||||
* 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
