1RXS J232953.9+062814 humps Dear Colleagues, We have received new data from D. Starkey. We have analyzed or have been analyzing newly available data at Kyoto and Okayama. A period analysis of the data between Nov. 13 and 14 has yielded a period of 0.04591(8) d, which is 0.8% shorter than the superhump period. Although more analysis and longer coverage are necessary to resolve persisting superhump signal and likely orbital one, the emergence of a significantly different period is highly suggestive of the (co-)existence of orbital modulations. More detailed analysis is being undertaken by Uemura-san. The hump profile is very complex, with two distinct maxima within one period, as best exemplified in the latest Starkey's data. Regards, Taichi Kato VSNET Collaboration team