The recently discovered ultra-short orbital period SU UMa-type dwarf nova seems to be entering a stage of rapid decline following the superoutburst. Observers are strongly urged to monitor for possible rebrightening(s) expected a week (?) later. YYMMDD(UT) mag observer sequence(*) 970519.964 <149 (G. Poyner) 970520.340 <153 (R. J. Modic) 970521.319 131 (R. J. Modic) 970522.367 132 (R. J. Modic) 970522.910 125 (P. Schmeer) GSC 970522.930 135 (T. Kinnunen) 970523.137 131 (R. J. Modic) 970523.364 134 (R. J. Modic) 970523.901 126 (P. Schmeer) GSC 970523.910 135 (T. Kinnunen) 970523.924 12.91 (L. T. Jensen) CCD 970523.951 136 (G. Poyner) 970524.191 133 (R. J. Modic) 970524.912 127 (P. Schmeer) GSC 970524.953 140 (G. Poyner) 970524.964 12.92 (L. T. Jensen) CCD 970525.974 140 (G. Poyner) 970525.976 128 (P. Schmeer) GSC 970526.337 141 (R. J. Modic) 970526.997 129 (P. Schmeer) GSC 970527.326 141 (R. J. Modic) 970527.958 130 (P. Schmeer) GSC 970528.215 142 (R. J. Modic) 970528.985 144 (G. Poyner) 970528.998 131 (P. Schmeer) GSC 970529.966 144 (G. Poyner) 970529.980 132 (P. Schmeer) GSC 970530.958 13.60 (L. T. Jensen) 970530.965 133 (P. Schmeer) GSC 970530.969 145 (G. Poyner) 970531.011 13.55 (L. T. Jensen) 970531.960 134 (P. Schmeer) GSC 970531.962 13.59 (L. T. Jensen) 970601.012 13.59 (L. T. Jensen) 970601.957 144 (G. Poyner) 970603.963 147 (G. Poyner) 970604.035 137 (P. Schmeer) GSC 970604.101 151 (R. J. Modic) 970605.340 164 (R. J. Modic) (*) Most observers use photographic sequence by Antipin (unless otherwise indicated), which probably gives 0.5-1.0 mag fainter than the real V magnitude. Regards, Taichi Kato