AL Com seems to have entered a new stage of outburst development. One manifestation is the appearance of large-amplitude superhumps with a definitely longer period (cf. preceding article by Nogami & Kato), the other is a "plateau"-like phase with a slower decline rate as indicated by the following nightly averaged magnitudes. In contrast to a rather rapid (~0.15 mag/day) rate of decline in the early stages (or even more at the brightness peak, as suggested from a compilation of visual estimates by T. Vanmunster), the present rate of decline is only 0.05-0.06 mag/day. We should watch closely what happens next in the present "the best monitored" WZ Sge-type superoutburst. mid-UT Al-comp S.D. N band V-mag -------------------------------- ------ 950407.643 -0.891 0.026 468 V 12.62 950408.571 -0.754 0.037 291 V 12.76 950409.589 -0.557 0.037 18 V 12.95 950410.627 -0.471 0.036 129 V 13.04 950412.635 -0.242 0.031 292 V 13.27 950413.465 -0.079 0.097 5 V 13.43 950417.562 0.143 0.078 157 V 13.65 Regards, Taichi Kato and Ouda team