RX J0558.3+6735: long-period SU UMa star? Dear Colleagus, We have finished analyzing the Kyoto data (observers: M. Uemura and R. Ishioka) taken on Apr. 1. Two apparent humps were detected during the 3-hour run. If this feature is genuine superhumps, this object can be a long period (~0.09 d) SU UMa-type dwarf nova. Since this period is near or within the famous period gap, further confirmatiry observations and long time-series observations are strongly encouraged. More detailed analysis will be later reported by Uemura-san or Ishioka-san. Please be sure to report observations to Uemura-san and Ishioka-san (uemura@kusastro.kyoto-u.ac.jp, ishioka@kusastro.kyoto-u.ac.jp) in order to minimize the delay of data analysis. Regards, Taichi Kato VSNET Collaboration team