GZ Cnc outburst YYYYMMDD(UT) mag observer 20021203.319 <145 (Mike Simonsen) 20021208.149 <147 (Pavol A. Dubovsky) 20021209.289 <150 (Mike Simonsen) 20021210.058 <147 (Pavol A. Dubovsky) 20021210.374 <150 (Mike Simonsen) 20021212.141 <147 (Pavol A. Dubovsky) 20021212.415 <150 (Mike Simonsen) 20021226.656 135 (Rod Stubbings) 20021226.662 135 (Rod Stubbings) The object is currently known as a short Porb (~2 hr) object, which is a good candidate for an SU UMa-type star. However, see * Kato et al. (2001) IBVS 5123 absence of superhumps during a long outburst * Kato et al. (2002) A&A 396, 929 unusual clustering of short outbursts (Click [2001] and [2002] on the VSNET top page to find more detailed information for these works.) Both suggest that GZ Cnc may be an unusual object. Further detailed observations during the present outburst are strongly encouraged! Regards, Taichi Kato VSNET Collaboration team