WD 1515+668
All names: J1515+6642, Gaia DR2 1645204475617697536, WD 1515+668, GALEX J151552.9+664243, 2MASS J15155289+6642427, WDJ151552.91+664242.88, TIC 230059745, SDSS J151552.92+664243.4, Gaia EDR3 1645204475617697536, PG 1515+669, CHSS 2744, Gaia DR3 1645204475617697536
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Kilic et al. 2025 | O'Brien et al. 2024 | Caron et al. 2023 | Kilic et al. 2020 | McCleery et al. 2020 | MWDD H | Gaia DR2 | Stilism | Gianninas et al. 2011 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 15 15 52.96 (0.02) | 15 15 52.96 (0.03) | 15 15 52.96 (0.03) | 15 15 52.96 | 15 15 52.91 (0.02) | 15 15 52.96 | 15 15 52.32 | |||||||||
| Declination | 66 42 44.42 (0.02) | 66 42 44.37 (0.03) | 66 42 44.37 (0.03) | 66 42 44.42 | 66 42 42.88 (0.02) | 66 42 44.37 | 66 42 37.44 | |||||||||
| Spectral type | DA | DA | DA | DA | DA | DA | DA | DA | DA4.8 | DA5 | ||||||
| Effective temperature | [K] | 10099.0 (52) | 10298.0 (110) | 9983.0 (46) | 10099.0 (52) | 10220.6 (88) | 10041.0 | 10410.0 (157) | 9954.0 (58) | |||||||
| log(g) | [cgs] | 8.24 (0.006) | 8.27 (0.02) | 8.22 (0.006) | 8.25 (0.007) | 8.27 (0.02) | 8.24 | 8.48 (0.06) | 8.23 (0.009) | |||||||
| Mass | [M☉] | 0.753 (0.006) | 0.771 (0.01) | 0.74 (0.006) | 0.755 (0.006) | 0.749 | 0.91 (0.04) | 0.74 (0.008) | ||||||||
| log(Luminosity) | [L☉] | |||||||||||||||
| Cooling age | [Gyr] | 0.8800 | 0.8495 | |||||||||||||
| 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] | 26.16 (0.02) | 26.16 (0.02) | 26.23 (0.03) | 26.23 (0.03) | 26.23 (0.03) | 26.16 | 26.16 (0.02) | 26.23 (0.03) | |||||||
| Distance | [pc] | 38.22 (0.03) | 38.23 (0.03) | 38.12 (0.04) | 38.13 (0.04) | 38.13 (0.04) | 32.00 | 38.22 | 38.22 (0.03) | 38.13 (0.04) | ||||||
| Composition | H | H | H | H | H | |||||||||||
| Proper motion (right ascension) | [mas/yr] | 19.38712684 (0.03) | 19.32683352 (0.05) | 19.387 (0.03) | 19.32683352 | |||||||||||
| Proper motion (declination) | [mas/yr] | 96.31128011 (0.03) | 96.18579615 (0.05) | 96.311 (0.03) | 96.18579615 | |||||||||||
| Variability | ||||||||||||||||
| Magnetic | ||||||||||||||||
| Bd | [MG] | |||||||||||||||
| Infrared excess (disk) | ||||||||||||||||
| Binarity | ||||||||||||||||
| B magnitude | 15.59 | |||||||||||||||
| V magnitude | ||||||||||||||||
| R magnitude | ||||||||||||||||
| I magnitude | ||||||||||||||||
| J magnitude | 15.29 (0.05) | 15.29 (0.05) | ||||||||||||||
| H magnitude | 15.24 (0.1) | 15.24 (0.1) | ||||||||||||||
| K magnitude | 15.18 (0.2) | 15.18 (0.2) | ||||||||||||||
| u magnitude | 15.81 (0.005) | 15.80 (0.005) | 15.80 (0.005) | |||||||||||||
| g magnitude | 15.42 (0.003) | 15.42 (0.003) | ||||||||||||||
| r magnitude | 15.50 (0.004) | 15.50 (0.004) | ||||||||||||||
| i magnitude | 15.63 (0.004) | 15.63 (0.004) | ||||||||||||||
| z magnitude | 15.82 (0.007) | 15.82 (0.007) | ||||||||||||||
| G magnitude | 15.42 (0.002) | 15.44 | 15.44 | 15.42 | 15.42 (0.003) | 15.44 | ||||||||||
| BP magnitude | 15.47 (0.002) | 15.46 | 15.46 | |||||||||||||
| RP magnitude | 15.34 (0.002) | 15.35 | 15.35 | |||||||||||||
| Pan g magnitude | 15.43 (0.004) | 15.43 (0.004) | ||||||||||||||
| Pan r magnitude | 15.51 (0.002) | 15.51 (0.003) | ||||||||||||||
| Pan i magnitude | 15.65 (0.004) | 15.65 (0.004) | ||||||||||||||
| Pan z magnitude | 15.81 (0.003) | 15.81 (0.003) | ||||||||||||||
| Pan y magnitude | 15.94 (0.007) | 15.94 (0.007) | ||||||||||||||
| 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
