The object is declining rapidly from its 'outburst', so we strongly encourage follow-up observations. Dear colleagues, I'v just finished ccd images of new var. It seems to be a new SU UMa type dwarf nova. I'll prepare light curve to GAMA's page when I'll back at observatory. USNO 1425.09823278 Recent reports suggest that the variable has entered a stage of rapid decline.
Several observers report by CCD photometry the possible existence of superhumps.
Observers should note in some SU UMa stars, superhumps may once decay during the plateau stage and may become prominent again even during the rapid decline, often showing double waves probably consisting of usual superhumps and late superhumps. A good such example was observed during the 1991 December - 1992 January superoutbrust of UV Per. Rudolf Novak's report suggests the superhump signal still persists. Follow-up observations are still highly encouraged until the object finally fades away. Tonny Vanmunster, CBA Belgium Observatory reports a rebrightening of this newly discovered variable.