V893 Sco outburst: (eclipse) observations encouraged The object stays above minimum since Mar. 9, the duration of the bright state may be longer than usual short outbursts (or separate outbursts?). More intensirve coverage of the present outburst is recommended. Despite that V893 Sco, the eclipsing dwarf nova below the period gap, is a very good candidate for an SU UMa star, no apparent superoutbursts have been observed in modern times. Please keep a close watch on this and others outburst to see whether any of them actually turns out to be a superoutburst. YYYYMMDD(UT) mag observer 20010227.805 145 (A. Pearce) 20010228.964 <146 (B. Monard) 20010302.049 <146 (B. Monard) 20010302.692 148 (R. Stubbings) 20010302.797 15.32:V (S. Kiyota) 20010302.819 145 (A. Pearce) 20010303.801 145 (A. Pearce) 20010304.035 147 (B. Monard) 20010304.826 146 (A. Pearce) 20010305.072 150 (B. Monard) 20010305.837 142 (A. Pearce) 20010306.090 148 (B. Monard) 20010306.726 144 (R. Stubbings) 20010308.085 <146 (B. Monard) 20010309.748 12.95V (S. Kiyota) 20010310.774 13.86V (S. Kiyota) 20010315.842 136 (A. Pearce) Regards, VSNET Collaboration team