TT Ind further brightens Further brightening has been observed, reaching the brightest level in the past. The object is at mag 18 in quiescence, so the present outburst has a chance of a superoutburst (or a large-amplitude SS Cyg star). Time-resolved photometry is strongly needed to clarify its nature. Follow-up information will be presented in vsnet-campaign-dn. YYYYMMDD(UT) mag observer 20000722.467 <146 (P. Williams) 20000722.635 <144 (R. Stubbings) 20000723.419 138 (R. Stubbings) 20000723.477 143 (P. Williams) 20000724.531 132 (A. Pearce) 20000724.541 127 (R. Stubbings) 20000724.819 128 (A. Pearce) Regards, Taichi Kato VSNET Collaboration team