V893 Sco outburst fading Maybe we had better wait for the next outburst. S. Kiyota (Tsukuba, Japan) has provided very important photometry immediately preceding the outburst. YYYYMMDD(UT) mag observer 20000523.790 <140 (B. Monard) 20000524.419 <139 (P. Williams) 20000525.826 <146 (B. Monard) 20000525.830 <146 (B. Monard) 20000526.819 144 (B. Monard) 20000527.819 147 (B. Monard) 20000528.719 <140 (B. Monard) 20000529.542 147:V (S. Kiyota) 20000529.753 127 (B. Monard) 20000530.460 127 (R. Stubbings) 20000530.497 127 (R. Stubbings) 20000530.714 127 (B. Monard) 20000531.057 132 (B. Monard) 20000531.501 131 (R. Stubbings) 20000601.513 137 (A. Pearce) Regards, Taichi Kato VSNET Collaboration team