We report the discovery of 8 991 new spectroscopically confirmed white dwarfs and subdwarfs in the Sloan Digital Sky Survey Data Release 10. We obtain T-eff,, log g and mass for hydrogen atmosphere white dwarf stars (DAs) and helium atmosphere white dwarf stars (DBs), and estimate the calcium/helium abundances for the white dwarf stars with metallic lines (DZs) and carbon/helium for cool carbon dominated spectra DQs. We found 2 new oxygen dominated spectra white dwarfs, 69 DQs, 42 hot DO/PG1159s, 175 white dwarf+main sequence star binaries, 206 magnetic DAHs, 325 continuum dominated DCs, 397 metal polluted white dwarfs, 450 helium dominated white dwarfs, 636 subdwarfs and 6796 new hydrogen dominated white dwarf stars.CPCI-S(ISTP)kepler@if.u...
We have detected 21 new, very hot hydrogen-deficient (pre-) white dwarfs (spectral types O(He), hot ...
We have detected 21 new, very hot hydrogen-deficient (pre-) white dwarfs (spectral types O(He), hot ...
We have detected 21 new, very hot hydrogen-deficient (pre-) white dwarfs (spectral types O(He), hot ...
We report the discovery of 9088 new spectroscopically confirmed white dwarfs and subdwarfs in the Sl...
We report the discovery of 9088 new spectroscopically confirmed white dwarfs and subdwarfs in the Sl...
We report the discovery of 9088 new spectroscopically confirmed white dwarfs and subdwarfs in the Sl...
We report the discovery of 6576 new spectroscopically confirmed white dwarf and subdwarf stars in th...
We report the discovery of 6576 new spectroscopically confirmed white dwarf and subdwarf stars in th...
An initial assessment is made of white dwarf and hot subdwarf stars observed in the Sloan Digital Sk...
White dwarfs carry information on the structure and evolution of the Galaxy, especially through thei...
White dwarfs are the end state of the evolution of more than 97 per cent of all stars, and therefore...
White dwarfs are the end state of the evolution of more than 97 per cent of all stars, and therefore...
We present a new catalog of spectroscopically confirmed white dwarf stars from the Sloan Digital Sky...
We identify seven new ultracool white dwarfs discovered in the Sloan Digital Sky Survey (SDSS). The ...
We present a new catalog of spectroscopically confirmed white dwarf stars from the Sloan Digital Sky...
We have detected 21 new, very hot hydrogen-deficient (pre-) white dwarfs (spectral types O(He), hot ...
We have detected 21 new, very hot hydrogen-deficient (pre-) white dwarfs (spectral types O(He), hot ...
We have detected 21 new, very hot hydrogen-deficient (pre-) white dwarfs (spectral types O(He), hot ...
We report the discovery of 9088 new spectroscopically confirmed white dwarfs and subdwarfs in the Sl...
We report the discovery of 9088 new spectroscopically confirmed white dwarfs and subdwarfs in the Sl...
We report the discovery of 9088 new spectroscopically confirmed white dwarfs and subdwarfs in the Sl...
We report the discovery of 6576 new spectroscopically confirmed white dwarf and subdwarf stars in th...
We report the discovery of 6576 new spectroscopically confirmed white dwarf and subdwarf stars in th...
An initial assessment is made of white dwarf and hot subdwarf stars observed in the Sloan Digital Sk...
White dwarfs carry information on the structure and evolution of the Galaxy, especially through thei...
White dwarfs are the end state of the evolution of more than 97 per cent of all stars, and therefore...
White dwarfs are the end state of the evolution of more than 97 per cent of all stars, and therefore...
We present a new catalog of spectroscopically confirmed white dwarf stars from the Sloan Digital Sky...
We identify seven new ultracool white dwarfs discovered in the Sloan Digital Sky Survey (SDSS). The ...
We present a new catalog of spectroscopically confirmed white dwarf stars from the Sloan Digital Sky...
We have detected 21 new, very hot hydrogen-deficient (pre-) white dwarfs (spectral types O(He), hot ...
We have detected 21 new, very hot hydrogen-deficient (pre-) white dwarfs (spectral types O(He), hot ...
We have detected 21 new, very hot hydrogen-deficient (pre-) white dwarfs (spectral types O(He), hot ...