AL Com observation May 18 at Kyoto Dear Colleagues, A quick look at the observation on May 18 (vsnet-alert 5891) shows a rapid brightening of the object at a rate of 3.0 mag/d! Although there was short-term variation, no very large superhump signal was present. Small (<0.1 mag) hump-like features are present, which may be the birth of "early superhumps" (if the present outburst evolves into a superoutburst). More detailed analyis will be presented later by Ishioka-san. Further observations, as long as possible, are strongly encouraged. Regards, VSNET Collaboration team