AL Com early superhumps and decline Dear Colleagues, More analysis (still ongoing) of the May 19 data has revealed the rapid fading at a rate of 0.80 mag/d. Early superhumps are present, as already reported. The best period from the presently available data is very slightly shorter than the orbital period, but the difference is marginally within errors of respective measurements. This observation may be the first indication of "negative superhumps" in the earliest stage of WZ Sge-type superoutburst. The full amplitude of early superhumps is 0.04-0.05 mag, and humps are singly peaked. This makes striking contrast to early superhumps observed in the 1995 superoutburst. This may be an indicatation that we are witnessing the earlier stage of evolution of these humps than in 1995. More detailed analysis will be later presented by Ishioka-san et al. Intensive observations are very encouraged. Regards, Taichi Kato VSNET Collaboration team