Rapid fading of T Leo The SU UMa-type dwarf nova T Leo is rapidly fading from the recent anomalous superoutburst (preceded by a well-separated precursor etc.). Intensive observations are encouraged to follow the post-superoutburst state. YYMMDD(UT) mag observer 980417.401 106 (R. Stubbings) 980417.520 108 (P. Nelson) 980417.883 115 (G. Poyner) 980418.414 110 (R. Stubbings) 980418.569 116 (P. Nelson) 980418.662 113 (T. Watanabe) 980418.887 117 (R. J. Bouma) 980418.962 125 (G. Poyner) 980419.246 128 (G. Hanson) 980419.465 130 (S. Takahashi) 980419.476 128 (T. Watanabe) 980419.531 <110 (H. Maehara)