SDSSp J173008.38+624754.7 brightened again Dear Colleagues, The observation last night (Nov. 6, M. Uemura and R. Ishioka) has shown that SDSSp J173008.38+624754.7, newly discovered SU UMa-type dwarf nova, brightened again. The object was found to be faint on Nov. 4. The present brightening may be a post-superoutburst rebrightening, or may represent the start of the phase of recurring normal outbursts. In the latter case, the recurrence time is expected to be short as inferred by the present observation. Observers are strongly urged to (also!) monitor this object closely, in order to clarify the nature of the rebrightening, and subsequent behavior. Regards, Taichi Kato VSNET Collaboration team