IY UMa = TmzV85 campaign update Dear Colleagues, We have received several additional datasets on IY UMa = TmzV85. An excellent post-superoutburst run by Tonny Vanmunster, several runs from the Kyoto team, revised data sets from Brian Martin. The object now shows usual orbital humps and variations possibly related to late superhumps. The magnitudes reported suggest that the object has not returned to pre-outburst level. Detailed analysis is under way. The compiled light curve is posted on the VSNET TmzV85 = IY UMa page: http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/tmzv85.html The number of data points (some of them are averages of several exposures) to draw this light curve is now 9009. Regards, M. Uemura, T. Kato, K. Matsumoto, P. Schmeer, K. Takamizawa, R. Novak, L. T. Jensen, D. Buczynski, T. Vanmunster, T. Kinnunen, M. Moilanen, A. Oksanen, B. Martin, L. Cook, and J. Pietz --------- IY UMa (TmzV85) VSNET collaboration team