1RXS J232953.9+062814 Dear Colleagues, We have analyzed or have been analyzing our Kyoto run on Oct. 6, 7, 8, 9. Observations on earlier dates correspond to the fading phase, as Uemura-san already reported. Later observations suggests that the fading has become substantially slower. Since the object is near mag 15, continuing time-resolved photometry and spectroscopy are still very highly encouraged. Further astrometric analysis is also in progress by Yamaoka-san. Regards, Taichi Kato on behalf of the VSNET Collaboration team