All names: Gaia DR3 3859269561337846656, [SGR2010] J1043+0603, 2MASS J10435862+0603210, TIC 374351063, SDSS J104358.59+060320.9, WIRED J104358.59+060320.9, SDSS J104358.60+060321.0, SDSS J104358.59+060321.0, WD 1041+063, Gaia DR2 3859269561337846656, Gaia EDR3 3859269561337846656, SDSS J104358.60+060320.9
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Gaia DR2 | Stilism | sdss-wdms.org (29/04/2016) | Pyrzas et al. 2015 | Tremblay et al. 2011 | Simbad | Eisenstein et al. 2006 | White Dwarf Catalog (McCook & Sion 1999) | Kleinman et al. 2013 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 10 43 58.60 (0.4) | 10 43 58.59 | 10 43 58.60 (0.6) | 10 43 58.59 | 10 43 58.59 (0.4) | 10 43 58.59 | 10 43 58.15 | 10 43 58.60 | |||||
| Declination | 06 03 20.37 (0.4) | 06 03 20.95 | 06 03 20.40 (0.7) | 06 03 20.92 | 06 03 21.06 (0.4) | 06 03 20.97 | 06 03 14.40 | 06 03 20.96 | |||||
| Spectral type | DA+M | DA | DA+M | DA+M | DA d | DA+M | |||||||
| Effective temperature | [K] | 11173.0 (299) | 11170.0 | 12610.0 (630) | 9159.0 (87) | 8935.0 (84) | |||||||
| log(g) | [cgs] | 8.19 (0.2) | 8.19 | 8.42 (0.1) | 7.68 (0.2) | 7.38 (0.2) | |||||||
| Mass | [M☉] | 0.72 (0.1) | 0.87 (0.07) | ||||||||||
| log(Luminosity) | [L☉] | ||||||||||||
| Cooling age | [Gyr] | 0.7244 | |||||||||||
| 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] | 3.43 (0.4) | 3.43 (0.4) | ||||||||||
| Distance | [pc] | 291.70 (35) | 282.00 (12) | 291.70 (35) | |||||||||
| Composition | H | ||||||||||||
| Proper motion (right ascension) | [mas/yr] | 5.140184243 (0.5) | 5.14 (0.5) | 11.1 | |||||||||
| Proper motion (declination) | [mas/yr] | -42.83589815 (0.5) | -42.836 (0.5) | -46.6 | |||||||||
| Variability | VAR | ||||||||||||
| Magnetic | |||||||||||||
| Bd | [MG] | ||||||||||||
| Infrared excess (disk) | |||||||||||||
| Binarity | WDMS | WDMS | WDMS | ||||||||||
| B magnitude | |||||||||||||
| V magnitude | 18.70 | ||||||||||||
| R magnitude | |||||||||||||
| I magnitude | |||||||||||||
| J magnitude | 16.29 (0.1) | ||||||||||||
| H magnitude | 15.88 (0.2) | ||||||||||||
| K magnitude | 15.74 (0.1) | ||||||||||||
| u magnitude | 19.23 (0.02) | 19.25 | 19.25 (0.03) | 19.25 (0.03) | 19.25 | 19.24 (0.03) | |||||||
| g magnitude | 18.75 (0.008) | 18.75 | 18.75 (0.008) | 18.75 (0.02) | 18.75 | 18.76 (0.02) | |||||||
| r magnitude | 18.79 (0.01) | 18.79 | 18.78 (0.01) | 18.79 (0.02) | 18.79 | 18.80 (0.02) | |||||||
| i magnitude | 18.36 (0.009) | 18.36 | 18.36 (0.009) | 18.36 (0.02) | 18.36 | 18.37 (0.02) | |||||||
| z magnitude | 17.72 (0.01) | 17.71 | 17.70 (0.01) | 17.71 (0.02) | 17.71 | 17.73 (0.02) | |||||||
| G magnitude | 18.64 (0.02) | 18.60 | 18.64 (0.006) | ||||||||||
| BP magnitude | 18.87 (0.02) | 18.82 | |||||||||||
| RP magnitude | 17.86 (0.03) | 17.90 | |||||||||||
| Pan g magnitude | 18.76 (0.009) | ||||||||||||
| Pan r magnitude | 18.79 (0.008) | ||||||||||||
| Pan i magnitude | 18.38 (0.004) | ||||||||||||
| Pan z magnitude | 17.87 (0.006) | ||||||||||||
| Pan y magnitude | 17.56 (0.01) | ||||||||||||
| E(B-V) | 0.024 | ||||||||||||
| Period #1 | [s] | 164.9 | |||||||||||
| Amplitude #1 | [mma] | 6.6 | |||||||||||
| Period #2 | [s] | 292.5 | |||||||||||
| Amplitude #2 | [mma] | 5.3 | |||||||||||
| Period #3 | [s] | 324.7 | |||||||||||
| Amplitude #3 | [mma] | 28.8 | |||||||||||
| Period #4 | [s] | 634.4 | |||||||||||
| Amplitude #4 | [mma] | 8.5 | |||||||||||
* 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.