IY UMa = TmzV85 campaign update Dear Colleagues, We have received several additional datasets on IY UMa = TmzV85, including an excellent run on Jan. 24 by the Nyrola team: Marko Moilanen, Arto Oksanen and Timo Kinnunen. The data sets from Brian Martin is under verification process now. We also had an additional excellent post-superoutburst run at Kyoto (Taichi Kato and Katsura Matsumoto). The double hump feature on Feb. 2 suggests that superhump-related variation still remains. The grand compiled light curve is posted on the VSNET TmzV85 = IY UMa page: http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/tmzv85.html 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