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arXiv:0910.3218 [astro-ph.SR]AbstractReferencesReviewsResources

Data Mining for Dwarf Novae in SDSS, GALEX and Astrometric Catalogues

Patrick Wils, Boris T. Gaensicke, Andrew J. Drake, John Southworth

Published 2009-10-19Version 1

By cross matching blue objects from SDSS with GALEX and the astrometric catalogues USNO-B1.0, GSC2.3 and CMC14, 64 new dwarf nova candidates with one or more observed outbursts have been identified. 14 of these systems are confirmed as cataclysmic variables through existing and follow-up spectroscopy. A study of the amplitude distribution and an estimate of the outburst frequency of these new dwarf novae and those discovered by the Catalina Real-time Transient Survey (CRTS) indicates that besides systems that are faint because they are farther away, there also exists a population of intrinsically faint dwarf novae with rare outbursts.

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