QY Per superoutburst update Dear Colleagues, Congratulations to all who detected the outburst, and succeeded in observation! Special thanks to all who quickly responded to the alert and recorded superhumps. Please continue your nice observations as long as possible on this rare occasion! As for the Kyoto observation, we (T. Kato and M. Uemura) observed QY Per for 8 hour's nearly continuously last night. A very preliminary analysis of the (partly reduced) data has yielded a superhump period of ~0.082 d, close to the one reported by Gianluca Masi. The relatively long superhump period and the rare outburst occurence seem to strengthen the relationship with DV UMa, whose spectacular superoutburst is still fresh in our memory. We would like to inform more detailed information after finishing the present reduction and collating incoming information. We would like to set up a special page on QY Per, as we have had on DV UMa. We would be extremely happy to receive the data to be reflected to the Web page (Y2K and time permitting...). The data should be sent to tkato@kusastro.kyoto-u.ac.jp. Congratulations and thanks again to all! We will be having the second- night run soon after this. Regards, Taichi Kato and Makoto Uemura