IY UMa likely superoutburst? If the current outburst of IY UMa is a genuine superoutburst (as inferred from possible superhump detections and recent visual estimates), the supercycle would becomd around 270 days. This may suggest two superoutbursts may have been missed between Takamiazawa's dicovery and the 2000 January one. It may have been the second missed one just fell in the seasonal gap of monitoring. Observations of the present outburst and a search for archival plates are very encouraged! In making CCD photometry, please make exposure times as short as reasonably achiebable. The 30s exposure would be adequate for small (20-30 cm) telescopes. Longer exposures will smear out the eclipse details, which need to be avoided. Regards, Taichi Kato VSNET Collaboration team