IY UMa outburst (most likely superoutburst)! As reported by Pavol A. Dubovsky, the deeply eclipsing SU UMa-type dwarf nova IY UMa (TmzV85) is undergoing an outburst. The outburst has been expected by the VSNET Collaboration team, and we have already received and obtained most important pre-superoutburst observations. Please continue your observations to completely follow (first time in the history) of this very favorably situated (presumable) superoutburst! In addition to usual time-series photometry covering all phases and eclipses, we encourage time-resolved spectroscopy, since IY UMa is known to show prominent emission lines even during outbursts. Velocity mapping using eclipses, as well as an attempt to detect spiral patterns would be most vaulable. Please report your observations to vsnet-campaig-dn (when you send raw data, please send them to Uemura-san and Ishioka-san, uemura@kusastro.kyoto-u.ac.jp and ishioka@kusastro.kyoto-u.ac.jp) in order to avoid any delay. For a reference, the following VSNET page would be useful http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/tmzv85.html References: Uemura et al. (2000) PASJ 52, L9 : discovery of a deeply eclipsing SU UMa-type dwarf nova Uemura et al. (2000) IAUC 7349 Patterson et al. (2000) PASP 112, 1567 : binary parameters and superhumps Rolfe et al. (2001) MNRAS 324, 529 : late superhumps Rolfe et al. (2001) in "Astrotomography, Indirect Imaging Methods in Observational Astronomy" p.39 : Doppler tomography Wu et al. (2001) ApJ 549, L81 : prominent emission lines in outburst Kato et al. (2001) IBVS 5159 : supercycle Please enjoy the current event! Regards, Taichi Kato VSNET Collaboration team