WZ Sge rebrightening! Dear Colleagues, We have receievd new data from G. Masi, A. Oksanen, T. Vanumunster, M. Moriyama, and revised from by B. Martin. We are also intensively analyzing the Kyoto data. The latest data have confirmed the brightening trend, as well as the further growth of superhumps! This indication of the brightening was also detected visually (vsnet-obs 35257, H-.G. Lindberg). The short duration of the fading suggests that the present fading is "dip"-type, as observed in AL Com (1995, 2001) and V2176 Cyg. The object may enter its second superoutburst (the nomenclature proposed by Nogami et al. in AL Com), as inferred from the strong reappearance of superhumps. Observations are most urgently requested! Since the system will be back to its "outburst" magnitude, please use short exposure times, and a brighter comparison star, as you have used during the main superoutburst. More detailed analysis and Web presentation will be announced by Uemura-san and Ishioka-san. Regards, Taichi Kato VSNET Collaboration team