WZ Sge: damping oscillation Dear Colleagues, 18 days have passed since the first post-superoutburst rebrightening. Up to now, ten distinct rebrightenings have been recongnized. As the time passes, it has been increasingly evident that these rebrightenings are a damping oscillation in nature, both in amplitude and period. The maxima of these rebrightenings have strictly followed the smooth extension of the decline of the main superoutburst. This general trend would suggest the continous shrinkage of the overall disk, through which the heating and cooling wave propagated. The damping nature of the oscillation may be naturally explained at a constant mass-transfer to the progressively shrinking accretion disk. The system now keeps relatively constant brighteness at about 11.5 mag. Further detailed, intensive observations are still strongly requested in order to follow the fate of the diminishing rebrightening oscillation. Regards, Taichi Kato VSNET Collaboration team