V877 Ara superhump light curve Dear Colleagues, We have updated the VSNET page on V877 Ara http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/v877ara.html The page now presents the light curve newly analyzed from Roland Santallo. The superhump profile is quite characteristic of fully grown SU UMa-type superhumps during the early stage of a superoutburst. We expect that Yamaoka-san will soon resume astrometry works, with which the correct quiescent counterpart is finally identified! Please keep a close watch on this object. Regards, Taichi Kato VSNET Collaboration team