CP Dra photometry preliminary result Preliminary analysis of a part of the Kyoto CP Dra run (0.06 d long) shows no apparent variations greater than 0.1 mag. There are natural possibilities that superhumps have not developed yet, or the object may be an another large-amplitude V344 Ori-like star, or something else (?) Only further observations can discriminate the possibilities! Please go as long as possible! Regards, VSNET Collaboration team