  We report the first results from a new search for cataclysmic variables (CVs)
using a combined X-ray (ROSAT) / infrared (2MASS) target selection that
discriminates against background AGN. Identification spectra were obtained at
the Isaac Newton Telescope for a total of 174 targets, leading to the discovery
of 12 new CVs. Initially devised to find short-period low-mass-transfer CVs,
this selection scheme has been very successful in identifying new intermediate
polars. Photometric and spectroscopic follow-up observations identify four of
the new CVs as intermediate polars: 1RXSJ063631.9+353537 (Porb~201min,
Pspin=1008.3408s or 930.5829), 1RXSJ070407.9+262501 (Porb~250min,
Pspin=480.708s), 1RXSJ173021.5-055933 (Porb=925.27min, Pspin=128.0s), and
1RXSJ180340.0+401214 (Porb=160.21min, Pspin=1520.51s). RXJ1730, also a
moderately bright hard X-ray source in the INTEGRAL/IBIS Galactic plane survey,
resembles the enigmatic AE Aqr. It is likely that its white dwarf is not
rotating at the spin equilibrium period, and the system may represent a
short-lived phase in CV evolution.
