PNVJ06245297+0208207: brightened further, Porb?

Itoh-san's new observations indicate that the object further brightened to 12 mag but superhumps have become weaker (amplitude typical for AM CVn stars). Crimean Astrophys. Obs. team also reported the rising part and superhumps were already present on Jan. 21 (good job!).

Preliminary analysis of the initial outburst yielded a possible period of 0.03433(4) d. Amplitude 0.02 mag and slower rise (similar to early superhumps).