All names: USNO-B1.0 0965-00249504, LP 562-48, Gaia DR3 1162536355835288320, Gaia EDR3 1162536355835288320, LSPM J1530+0630, WDJ153033.10+063005.93, SDSS J153033.14+063005.5, NLTT 40405, J1530+0630, SDSS J153033.15+063005.5, SDSS J153033.14+063005.6, Gaia DR2 1162536355835288320, SDSS J153033.15+063005.6
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Kilic et al. 2025 | Caron et al. 2023 | Gaia DR2 | Stilism | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | Kleinman et al. 2013 | Vincent et al. 2023 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 15 30 33.32 (0.1) | 15 30 33.15 | 15 30 33.31 (0.2) | 15 30 33.32 | 15 30 33.10 (0.1) | 15 30 33.31 | 15 30 33.15 | ||||||
| Declination | 06 30 04.44 (0.1) | 06 30 05.59 | 06 30 04.49 (0.2) | 06 30 04.44 | 06 30 05.92 (0.1) | 06 30 04.49 | 06 30 05.59 | ||||||
| Spectral type | DC | DC | DC | DC | DC | DC: | |||||||
| Effective temperature | [K] | 7108.0 (56) | 7195.0 (53) | 7332.0 (213) | 10080.0 (6) | ||||||||
| log(g) | [cgs] | 8.41 (0.02) | 8.49 (0.02) | 8.53 (0.04) | 9.71 (0.4) | ||||||||
| Mass | [M☉] | 0.844 (0.01) | 0.897 (0.02) | 0.923 (0.03) | |||||||||
| log(Luminosity) | [L☉] | ||||||||||||
| Cooling age | [Gyr] | 3.5000 | |||||||||||
| log(H/He) | -3.4 | -3.4 | |||||||||||
| log(C/He) | |||||||||||||
| log(Ca/He) | |||||||||||||
| log(Ca/H) | |||||||||||||
| log(N/He) | |||||||||||||
| log(O/He) | |||||||||||||
| log(Na/He) | |||||||||||||
| log(Mg/He) | |||||||||||||
| log(Al/He) | |||||||||||||
| log(Si/He) | |||||||||||||
| log(P/He) | |||||||||||||
| log(S/He) | |||||||||||||
| log(Cl/He) | |||||||||||||
| log(Sc/He) | |||||||||||||
| log(Ti/He) | |||||||||||||
| log(V/He) | |||||||||||||
| log(Cr/He) | |||||||||||||
| log(Mn/He) | |||||||||||||
| log(Fe/He) | |||||||||||||
| log(Co/He) | |||||||||||||
| log(Ni/He) | |||||||||||||
| log(Cu/He) | |||||||||||||
| log(Zn/He) | |||||||||||||
| log(Ga/He) | |||||||||||||
| log(Ge/He) | |||||||||||||
| log(Sr/He) | |||||||||||||
| Parallax | [mas] | 14.21 (0.2) | 14.73 (0.3) | 14.73 (0.3) | 14.21 | 14.21 (0.2) | 14.73 (0.3) | ||||||
| Distance | [pc] | 70.38 (0.8) | 67.89 (1) | 67.90 (1) | 70.38 | 70.38 (0.8) | 67.90 (1) | ||||||
| Composition | He | ||||||||||||
| Proper motion (right ascension) | [mas/yr] | 200.239059 (0.2) | 199.9931674 (0.4) | 200.239 (0.2) | 199.9931674 | ||||||||
| Proper motion (declination) | [mas/yr] | -92.29474601 (0.1) | -92.84631628 (0.6) | -92.295 (0.1) | -92.84631628 | ||||||||
| Variability | |||||||||||||
| Magnetic | |||||||||||||
| Bd | [MG] | ||||||||||||
| Infrared excess (disk) | |||||||||||||
| Binarity | |||||||||||||
| B magnitude | 18.10 | ||||||||||||
| V magnitude | |||||||||||||
| R magnitude | 18.00 | ||||||||||||
| I magnitude | |||||||||||||
| J magnitude | 17.99 (0.04) | 17.99 (0.04) | |||||||||||
| H magnitude | 17.84 (0.06) | 17.84 (0.07) | |||||||||||
| K magnitude | 17.96 (0.1) | 18.00 (0.1) | |||||||||||
| u magnitude | 18.93 (0.02) | 18.94 (0.02) | 18.93 (0.02) | 18.93 (0.02) | 18.91 (0.02) | ||||||||
| g magnitude | 18.47 (0.007) | 18.48 (0.007) | 18.48 (0.007) | 18.49 (0.01) | |||||||||
| r magnitude | 18.37 (0.008) | 18.37 (0.008) | 18.37 (0.008) | 18.38 (0.01) | |||||||||
| i magnitude | 18.38 (0.01) | 18.38 (0.01) | 18.38 (0.01) | 18.39 (0.02) | |||||||||
| z magnitude | 18.44 (0.03) | 18.44 (0.03) | 18.44 (0.03) | 18.44 (0.03) | |||||||||
| G magnitude | 18.34 (0.02) | 18.37 | 18.34 | 18.34 (0.003) | 18.37 | ||||||||
| BP magnitude | 18.48 (0.02) | 18.51 | 18.51 | ||||||||||
| RP magnitude | 18.10 (0.02) | 18.08 | 18.08 | ||||||||||
| Pan g magnitude | 18.46 (0.006) | 18.46 (0.006) | |||||||||||
| Pan r magnitude | 18.38 (0.006) | 18.38 (0.007) | |||||||||||
| Pan i magnitude | 18.40 (0.005) | 18.40 (0.005) | |||||||||||
| Pan z magnitude | 18.46 (0.009) | 18.46 (0.008) | |||||||||||
| Pan y magnitude | 18.50 (0.01) | 18.50 (0.01) | |||||||||||
| E(B-V) | 0.005 | ||||||||||||
* Constant surface field
Spectra without link are available upon request
The Montreal White Dwarf Database is produced and maintained by Prof. Patrick Dufour (Université de Montréal) and Dr. Simon Blouin (University of Victoria). Please send database updates, corrections, suggestions or bug reports to patrick.dufour@umontreal.ca.