TV Crv superhumps update The Kyoto team obtained another excellent run of TV Crv on Feb. 22 (Uemura, Ishioka et al.). The amplitude of superhumps has become slightly smaller, but are still prominent. The analysis of Feb. 20 - 22 observations has yielded a refined superhump period of 0.06489 d. More detailed analysis will be presented by Uemura-san et al. We are very looking forward to receiving any time-resolved photometry of this object, in order to investigate the fine structure of superhumps. Regards, VSNET Collaboration team

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