Likely superoutburst of SBS1017+533 H. Maehara (vsnet-alert 2903) reports the detection of a bright outburst of the recently identified SU UMa-star, SBS1017+533. The object was independently discovered by the SBS survey and by the RASS optical identification of ROSAT sources. The suggested ROSAT association based on the former information, relayed via VSNET, Garanavich discovered the object in outburst in late January, 1998 (vsnet-alert 1441). Time-resolved CCD photometry by T. Vanmunster revelaed the presence of superhumps (CVC 161, vsnet-alert 1448; CVC 162, vsnet-alert 1450) with a period of 0.0697 d. D. Nogami (vsnet-alert 1452) also detected superhumps with a period of 0.069 d. The present presumable superoutburst is the first known since 1998 Jannuary, though several fainter outbursts have been detected (T. Watanabe, VSOLJ Variable Star Bulletin). Time-resolved photometry at this early stage of superoutburst is very strongly encouraged. YYMMDD(UT) mag observer 990421.030 <143 (T. Kinnunen) 990424.915 <143 (G. Poyner) 990427.917 <146 (G. Poyner) 990429.508 127 (H. Maehara) 990429.519 126 (H. Maehara) 990429.665 129 (T. Watanabe) Regards, Taichi Kato