KK Tel bright outburst As informed in [vsnet-alert 4860], The suspected SU UMa-type dwarf nova KK Tel is undergoing a bright outburst. The present season allows a relatively good perspective of time-resolved photoemtry. 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. Considering the relatively long (suggested) period, relatively long (more than 3 hours) runs are desirable. Please report the progress of observations and any finding to this list (and vsnet-alert when necessary). Regards, Taichi Kato VSNET Collaboration team