V877 Ara refined superhump period Dear Colleagues, We have received new data from Roland Santallo. The object still show vigorous superhumps. The best superhump period determined from the 2.2-d baseline is 0.08450(5) d. This period confirms that V877 Ara belongs to a member of long-period SU UMa-type dwarf novae. As in the case of V359 Cen, further obseravations (esp. superhump timing observations) are still highly wanted. Regards, Taichi Kato on behalf of the VSNET Collaboration team