IY UMa = TmzV85 (UGSU+E) UMAIY 20000418.194 169C Scp UMAIY 20000420.175 141C Scp Sequence: Henden, R = V - 0.508*(B-V) - 0.040 Instrument: IRO (0.5-m RCT + AP-8) This eclipsing SU UMa-type dwarf nova is undergoing its third ever recorded outburst. The most recently observed one (a supermaximum) started between 2000 Jan. 9 and 13 (cf. vsnet-alert 4027). The interval between the two brightenings was only 96-103 days. Time-resolved photometry during the current (normal?) outburst is strongly recommended. Clear skies, Patrick