PHL 411
All names: WD 2307+009, SDSS J230953.40+011213.2, SDSS J230953.44+011213.4, SDSS J230953.39+011213.2, SDSS J230953.43+011213.4, Gaia EDR3 2657498580470832384, GALEX J230953.4+011212, Gaia DR3 2657498580470832384, PHL 411, Gaia DR2 2657498576175242368, SDSS J230953.41+011213.2
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Bedard et al. 2020 | MWDD H | Gaia DR2 | Stilism | Tremblay et al. 2011 | Vincent et al. 2024 | Simbad | Eisenstein et al. 2006 | White Dwarf Catalog (McCook & Sion 1999) | Kleinman et al. 2013 | Kleinman et al. 2004 | Vincent et al. 2023 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 23 09 53.46 (0.08) | 23 09 53.44 | 23 09 53.46 (0.1) | 23 09 53.46 | 23 09 53.41 (0.08) | 23 09 53.42 | 23 09 52.49 | 23 09 53.40 | 23 09 53.40 | |||||||
| Declination | 01 12 13.52 (0.07) | 01 12 13.44 | 01 12 13.51 (0.09) | 01 12 13.52 | 01 12 13.26 (0.07) | 01 12 13.27 | 01 12 11.16 | 01 12 13.20 | 01 12 13.21 | |||||||
| Spectral type | DA | DA | DA | DA | DA | DA | DA1.6 | DA | DA | |||||||
| Effective temperature | [K] | 31364.0 (93) | 25226.0 | 31420.0 (140) | 28820.0 (1036) | 30882.0 (189) | 31054.0 (153) | 30958.0 (190) | ||||||||
| log(g) | [cgs] | 8.45 (0.02) | 8.36 | 8.48 (0.03) | 8.50 (0.04) | 8.59 (0.03) | 8.53 (0.03) | 8.60 (0.03) | ||||||||
| Mass | [M☉] | 0.92 (0.01) | 0.847 | 0.94 (0.02) | 0.94 (0.03) | 0.944 (0.01) | ||||||||||
| log(Luminosity) | [L☉] | -1.11 (0.02) | ||||||||||||||
| Cooling age | [Gyr] | 0.0275 (0.003) | 0.0650 | 0.0427 | ||||||||||||
| 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] | 6.65 (0.1) | 6.68 (0.1) | 6.65 | 6.65 (0.1) | |||||||||||
| Distance | [pc] | 150.29 (2) | 149.72 (3) | 150.29 | 150.29 (2) | |||||||||||
| Composition | H | H | H | |||||||||||||
| Proper motion (right ascension) | [mas/yr] | 48.38774791 (0.1) | 48.52079583 (0.2) | 48.388 (0.1) | 46.0 | 44.0 | ||||||||||
| Proper motion (declination) | [mas/yr] | 16.29338409 (0.09) | 16.27176698 (0.2) | 16.293 (0.09) | 19.9 | 21.0 | ||||||||||
| Variability | ||||||||||||||||
| Magnetic | ||||||||||||||||
| Bd | [MG] | |||||||||||||||
| Infrared excess (disk) | ||||||||||||||||
| Binarity | ||||||||||||||||
| B magnitude | 16.90 | |||||||||||||||
| V magnitude | 17.10 | |||||||||||||||
| R magnitude | ||||||||||||||||
| I magnitude | ||||||||||||||||
| J magnitude | 17.42 (0.02) | |||||||||||||||
| H magnitude | 17.48 (0.09) | |||||||||||||||
| K magnitude | 17.80 (0.2) | |||||||||||||||
| u magnitude | 16.27 (0.006) | 16.27 (0.006) | 16.34 (0.03) | 16.33 | 16.34 (0.03) | 16.33 (0.03) | ||||||||||
| g magnitude | 16.53 (0.004) | 16.53 (0.004) | 16.57 (0.02) | 16.57 | 16.59 (0.02) | 16.57 (0.03) | ||||||||||
| r magnitude | 16.98 (0.005) | 16.99 (0.005) | 16.98 (0.02) | 16.99 | 16.98 (0.02) | 16.99 (0.02) | ||||||||||
| i magnitude | 17.32 (0.006) | 17.33 (0.006) | 17.31 (0.01) | 17.31 | 17.31 (0.01) | 17.31 (0.01) | ||||||||||
| z magnitude | 17.60 (0.01) | 17.60 (0.01) | 17.61 (0.02) | 17.61 | 17.61 (0.02) | 17.61 (0.02) | ||||||||||
| G magnitude | 16.78 (0.004) | 16.79 | 16.78 | 16.78 (0.003) | ||||||||||||
| BP magnitude | 16.65 (0.004) | 16.63 | ||||||||||||||
| RP magnitude | 17.03 (0.01) | 17.04 | ||||||||||||||
| Pan g magnitude | 16.61 (0.003) | |||||||||||||||
| Pan r magnitude | 17.00 (0.003) | |||||||||||||||
| Pan i magnitude | 17.35 (0.006) | |||||||||||||||
| Pan z magnitude | 17.62 (0.008) | |||||||||||||||
| Pan y magnitude | 17.83 (0.009) | |||||||||||||||
| E(B-V) | 0.031 | |||||||||||||||
* 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
