  Photometric and spectroscopic observations of the candidate cataclysmic
variable KUV03580+0614, independently found from the Hamburg survey as
HS0357+0614, reveal this to be a cataclysmic variable with an orbital period of
3.4 hrs. CVs with periods in this range are usually novalikes belonging to the
SW Sex or Intermediate Polar categories. The variability, spectroscopic
characteristics and the lack of strong X-rays indicate a system similar to V795
Her, LS Peg and AH Men.
