UV Per superhump detection Dear Colleagues, From the 6.5-hour observation on Dec. 25 (vsnet-campaign 615), we have been able to detect growing superhumps! The amplitude grew from less than 0.1 mag to 0.15 mag. The other striking feature is the superimposed relatively rapid fading (0.3 mag/d). The superhump period determined from the run is 0.0678 d, which is substanstially longer than that obtained by other authros on earlier superoutbursts. This suggests that the superhump is still is in its unsteady phase. It is also striking to note such an early apperance of superhumps in such a short period system. The system warrants further urgent, detailed observations. More detailed analysis will be provided by Ishioka-san and Uemura-san. Regards, VSNET Collaboration team