USNO 1425.09823278 (rebrightening) The most recent reports indicate the system has not significantly faded after it reached the second (rebrightening) maximum. This may be an evidence of the "double superoutburst" nature of the present rebrightening. Observations, espcially time-resolved photometry, is urgently requested to follow the possible development of superhumps during the second outburst. (see. cf. AL Com, D. Nogami et al., ApJ in press, available at the VSNET anonymous ftp). YYMMDD(UT) mag observer 970910.610 14.64V (Ouda team) 970910.824 14.68 (L. T. Jensen, CCD unfiltered) 970910.836 14.68 (L. T. Jensen, CCD unfiltered) 970910.838 14.71 (L. T. Jensen, CCD unfiltered) 970910.880 142 (J. Pietz) 970912.244 147 (R. J. Modic) 970912.901 143 (G. Poyner) 970913.015 141 (G. Poyner) Best regards, Taichi Kato