1RXS J232953.9+062814 double humps! Dear Colleagues, We have received new data from Donn Starkey. The data have confirmed that the object retains the approximately same brightness for these two days. The most striking feature in Starkey's data is the presence of double-peaked humps. In contrast to a usual combination of superhumps and late superhumps, the profile shows a brighte maxima at later phases, similar to "early superhumps" as seen in WZ Sge. More detailed analysis is in progress. Further continous observations are strongly encouraged! Regards, Taichi Kato on behalf of the VSNET Collaboration team