SY Vol still bright The likely large-amplitude dwarf nova SY Vol is still bright according to observations by Rod Stubbings. If this star is an SU UMa-type dwarf nova, the present outburst should be a superoutburst. Time-resolved photometry is very strongly encouraged. Follow-up information will be provided in vsnet-campaign and vsnet-campaign-dn. YYYYMMDD(UT) mag observer 20000723.492 142 (R. Stubbings) 20000723.533 142 (R. Stubbings) 20000724.514 140 (R. Stubbings) 20000724.551 140 (R. Stubbings) 20000724.585 140 (R. Stubbings) 20000727.480 144 (R. Stubbings) Regards, Taichi Kato