KK Tel bright outburst The suspected SU UMa-type dwarf nova KK Tel is undergoing a bright outburst. The last long outburst of KK Tel was observed in 1999 March )cf. vsnet-alert 2800, 2807). KK Tel has been suspected to be an SU UMa-type dwarf nova having a suspected orbital period of 2.02 hours (Howell et al. 1991, PASP 103, 300). A search for superhumps is strongly recommended. The present outburst will be put on the VSNET campaign object list. YYYYMMDD(UT) mag observer 20000326.851 <148 (A. Pearce) 20000328.851 <150 (A. Pearce) 20000329.841 <150 (A. Pearce) 20000402.854 <150 (A. Pearce) 20000405.847 <152 (A. Pearce) 20000407.849 <150 (A. Pearce) 20000409.849 <140 (A. Pearce) 20000510.601 <148 (R. Stubbings) 20000517.599 138 (R. Stubbings) 20000517.846 136 (A. Pearce) Regards, Taichi Kato