1RXS J232953.9+062814 orbital humps? Dear Colleagues, D. Starkey has sent additional most recent data. The data show further fading, but the decline has become slower. The data also show emergence of another type of periodic signal. Provisional period analysis of the data between Nov. 11.11 and 12.10 has yielded a period of 0.04608(4) d. Although a longer baseline is required to confirm the periodicity and to firmly separate the signal from the persistent superhumps, this period may reflect (the upper limit of) the orbital period. This in turn suggests the lower limit of fractional superhump excess of 0.5 %. More analysis will be later presented by Uemura-san. Regards, Taichi Kato on behalf of the VSNET Collaboration team