The world-wide VSNET campaign for this new object is now more extensive. J. Pietz has kindly sent us time-series observations which shows clear humps with amplitudes of about 0.25mag. Including this new data, we obtained revised superhump period of 0.046311 (12) d. Just now we have started tonight run on this object at Kyoto. The object is about 13mag. Regards, Makoto Uemura, Ryoko Ishioka, and Taichi Kato