WD 1124+017
All names: SDSS J112649.47+012758.46, SDSS J112649.47+012758.4, WD 1124+017, Gaia DR3 3798659326454564224, NLTT 27402, LAMOST J112649.62+012758.3, 2MASS J11264960+0127581, TIC 363550034, GALEX J112649.6+012758, Gaia EDR3 3798659326454564224, Gaia DR2 3798659326454564224, SDSS J112649.58+012758.0, USNO-B1.0 0914-00200068, HE1124+0144, [BGK2006] J112649.58+012758.0, LP 612-69, HE 1124+0144
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR10 | SDSS DR12 | MWDD H | Gaia DR2 | Stilism | Guo et al. 2015 | Kepler et al. 2015 | Koester et al. 2009 | Koester et al. 2001 | Vincent et al. 2024 | Simbad | White Dwarf Catalog (McCook & Sion 1999) | Vincent et al. 2023 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 11 26 49.41 (0.05) | 11 26 49.58 | 11 26 49.58 | 11 26 49.42 (0.07) | 11 26 49.70 | 11 26 49.41 | 11 26 49.60 (0.05) | 11 26 49.03 | ||||||||
| Declination | 01 27 58.67 (0.04) | 01 27 58.01 | 01 27 58.01 | 01 27 58.65 (0.05) | 01 27 56.00 | 01 27 58.67 | 01 27 57.97 (0.04) | 01 27 52.92 | ||||||||
| Spectral type | DA | DA | DA | DA | DA | DA3.2 | DA3.2 | DA | ||||||||
| Effective temperature | [K] | 14851.0 | 16755.0 (43) | 16246.0 (35) | 15885.0 (63) | 15633.0 (314) | ||||||||||
| log(g) | [cgs] | 7.73 | 7.86 (0.01) | 7.74 (0.007) | 7.68 (0.01) | 7.80 (0.02) | ||||||||||
| Mass | [M☉] | 0.47 | 0.545 (0.005) | 0.45 | 0.505 (0.01) | |||||||||||
| log(Luminosity) | [L☉] | |||||||||||||||
| Cooling age | [Gyr] | 0.1326 | ||||||||||||||
| 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] | 8.54 (0.06) | 8.50 (0.08) | 8.54 | 8.54 (0.06) | |||||||||||
| Distance | [pc] | 117.16 (0.9) | 117.58 (1) | 117.16 | 117.16 (0.9) | |||||||||||
| Composition | H | |||||||||||||||
| Proper motion (right ascension) | [mas/yr] | -172.1525486 (0.06) | -171.9162141 (0.1) | -172.153 (0.06) | ||||||||||||
| Proper motion (declination) | [mas/yr] | 43.74259964 (0.05) | 43.75128485 (0.09) | 43.743 (0.05) | ||||||||||||
| Variability | ||||||||||||||||
| Magnetic | ||||||||||||||||
| Bd | [MG] | |||||||||||||||
| Infrared excess (disk) | ||||||||||||||||
| Binarity | ||||||||||||||||
| B magnitude | 16.50 | |||||||||||||||
| V magnitude | 16.30 | 16.30 | 16.30 | |||||||||||||
| R magnitude | 16.60 | |||||||||||||||
| I magnitude | ||||||||||||||||
| J magnitude | 16.68 (0.02) | |||||||||||||||
| H magnitude | 16.70 (0.04) | |||||||||||||||
| K magnitude | 16.75 (0.06) | |||||||||||||||
| u magnitude | 16.36 (0.005) | 16.36 (0.005) | 16.37 (0.01) | 16.36 (0.005) | ||||||||||||
| g magnitude | 16.10 (0.004) | 16.10 (0.004) | 16.12 (0.01) | 16.11 (0.004) | ||||||||||||
| r magnitude | 16.42 (0.004) | 16.42 (0.004) | 16.42 (0.01) | 16.42 (0.004) | ||||||||||||
| i magnitude | 16.69 (0.005) | 16.69 (0.005) | 16.69 (0.02) | 16.69 (0.005) | ||||||||||||
| z magnitude | 16.98 (0.01) | 16.98 (0.01) | 16.98 (0.02) | 16.98 (0.01) | ||||||||||||
| G magnitude | 16.29 (0.004) | 16.31 | 16.29 | 16.29 (0.003) | ||||||||||||
| BP magnitude | 16.25 (0.004) | 16.23 | ||||||||||||||
| RP magnitude | 16.41 (0.005) | 16.41 | ||||||||||||||
| Pan g magnitude | 16.16 (0.003) | |||||||||||||||
| Pan r magnitude | 16.44 (0.006) | |||||||||||||||
| Pan i magnitude | 16.71 (0.003) | |||||||||||||||
| Pan z magnitude | 16.97 (0.003) | |||||||||||||||
| Pan y magnitude | 17.12 (0.009) | |||||||||||||||
| E(B-V) | 0.009 | |||||||||||||||
* 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
