GD 64
All names: 04573+4155, Gaia EDR3 201881364339401728, 2MASS J04572254+4155567, GCRV 21688, LP 202-4, UCAC2 46253351, TIC 65828507, GEN# +6.10060064, EGGR 209, LSPM J0457+4155, NLTT 14208, WD 0453+418, WD 0453+41, PM J04573+4155, WDJ045722.54+415556.48, uvby98 610060064, USNO-B1.0 1319-00119098, USNO 501, PLX 1099.02, GD 64, UCAC4 660-028908, Gaia DR2 201881364339401728, Gaia DR3 201881364339401728, 1SWASP J045722.55+415556.6
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | O'Brien et al. 2024 | McCleery et al. 2020 | MWDD H | Gaia DR2 | Bedard et al. 2017 | Stilism | Limoges et al. 2015 | Gianninas et al. 2011 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 04 57 22.57 (0.02) | 04 57 22.57 (0.05) | 04 57 22.57 (0.05) | 04 57 22.57 | 04 57 22.54 (0.02) | 04 57 22.57 | 04 57 21.34 | ||||||||
| Declination | 41 55 53.06 (0.02) | 41 55 53.17 (0.04) | 41 55 53.17 (0.04) | 41 55 53.06 | 41 55 56.48 (0.02) | 41 55 53.17 | 41 56 07.80 | ||||||||
| Spectral type | DA | DA | DA | DA | DA | DA | DA | DA3.5 | DA3.5 | ||||||
| Effective temperature | [K] | 14268.0 (212) | 14150.3 (106) | 13837.0 | 14523.0 (248) | 14290.0 (255) | 14320.0 (256) | 14836.0 (87) | |||||||
| log(g) | [cgs] | 7.79 (0.02) | 7.79 (0.01) | 7.77 | 7.85 (0.05) | 7.82 (0.05) | 7.81 (0.05) | 7.84 (0.006) | |||||||
| Mass | [M☉] | 0.496 (0.01) | 0.487 | 0.51 (0.03) | 0.51 (0.03) | 0.527 (0.004) | |||||||||
| log(Luminosity) | [L☉] | -2.10 | |||||||||||||
| Cooling age | [Gyr] | 0.1798 | |||||||||||||
| 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] | 26.24 (0.03) | 26.24 (0.03) | 26.20 (0.07) | 26.20 (0.07) | 23.00 (3) | 26.24 | 26.24 (0.03) | 26.20 (0.07) | 22.80 (26) | |||||
| Distance | [pc] | 38.11 (0.04) | 38.11 (0.04) | 38.16 (0.1) | 38.16 (0.1) | 43.90 (5) | 43.50 (5) | 38.00 | 38.11 | 38.11 (0.04) | 38.16 (0.1) | 43.86 (50) | |||
| Composition | H | H | H | H | |||||||||||
| Proper motion (right ascension) | [mas/yr] | 18.14442549 (0.03) | 18.29337454 (0.08) | 18.144 (0.03) | 18.29337454 | ||||||||||
| Proper motion (declination) | [mas/yr] | -213.4432463 (0.03) | -213.2599978 (0.08) | -213.443 (0.03) | -213.2599978 | ||||||||||
| Variability | NOV | ||||||||||||||
| Magnetic | |||||||||||||||
| Bd | [MG] | ||||||||||||||
| Infrared excess (disk) | |||||||||||||||
| Binarity | |||||||||||||||
| B magnitude | 14.04 (0.008) | ||||||||||||||
| V magnitude | 13.98 (0.002) | ||||||||||||||
| R magnitude | 14.05 (0.005) | ||||||||||||||
| I magnitude | 14.12 (0.005) | ||||||||||||||
| J magnitude | 14.40 (0.04) | ||||||||||||||
| H magnitude | 14.36 (0.06) | ||||||||||||||
| K magnitude | 14.55 (0.1) | ||||||||||||||
| u magnitude | |||||||||||||||
| g magnitude | 13.91 (0.04) | ||||||||||||||
| r magnitude | 14.14 (0.05) | ||||||||||||||
| i magnitude | 14.39 (0.08) | ||||||||||||||
| z magnitude | |||||||||||||||
| G magnitude | 14.02 (0.001) | 14.04 | 14.04 | 14.02 | 14.02 (0.003) | 14.04 | |||||||||
| BP magnitude | 13.99 (0.001) | 13.99 | 13.99 | ||||||||||||
| RP magnitude | 14.11 (0.0009) | 14.12 | 14.12 | ||||||||||||
| Pan g magnitude | 13.92 (0.003) | ||||||||||||||
| Pan r magnitude | 14.19 (0.002) | ||||||||||||||
| Pan i magnitude | 14.44 (3e-05) | ||||||||||||||
| Pan z magnitude | 14.67 (0.002) | ||||||||||||||
| Pan y magnitude | 14.83 (0.002) | ||||||||||||||
| 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
