RZ Leo: beat phenomenon? Dear Colleagues, We have finished analyzing the data on Dec. 27, both by the Kyoto team and Kiyota-san (total of 722 points). The data show rather steep fading in contrast to observations in Dec. 26. There seem to be a wavy pattern with a period of 2-3 d in the averaged light curve. The amplitude of superhumps seems to vary with this period. This is likely caused by the beat phenomenon between the superhump period and the orbital period, a natural consequence of a high-inclination system as suggested by earlier quiescent observations. The observed period is totally consistent with ther previously suggested superhump and orbital periods. More detailed analysis of superhump timing and profile analysis is keenly in progress by Ishioka-san et al. The VSNET Collaboration team is eager to receive any data on this superoutburst, in order to reveal this intriguing behavior! Regards, VSNET Collaboration team