We present a method which uses colour-colour cuts on the Sloan Digital Sky Survey (SDSS) photometry to select white dwarfs with hydrogen-rich (DA) atmospheres without the recourse to spectroscopy. This method results in a sample of DA white dwarfs that is 95 per cent complete at an efficiency of returning a true DA white dwarf of 62 per cent. The approach was applied to SDSS Data Release 7 for objects with and without SDSS spectroscopy.
Cone search capability for table J/MNRAS/417/1210/spec (SDSS DR7 spectroscopic white dwarfs)
Cone search capability for table J/MNRAS/417/1210/phot (SDSS DR7 photometric white dwarfs)
Cone search capability for table J/MNRAS/417/1210/ire (SDSS DR7 & UKIDSS DR8 IR excess candidates)
Cone search capability for table J/MNRAS/417/1210/posqso (SDSS DR7 & UKIDSS DR8 possible QSOs)