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V803 Cen superhumps Dear Colleagues, We have received a nice data set from Neil D Butterworth. The light curve clearly indicate the presence of 0.06 mag superhumps. The period determined from this observation is 0.01860(8) d, which agrees with the "nominal superhump period" of this system within errors. The profile is placed at: http://vsnet.kusastro.kyoto-u.ac.jp/pub/vsnet/DNe/V803_Cen/sh0306.gif Although the light curve may look slightly noisy, mainly because of the low amplitude of the variations, the presence of the superhump-type variation is secure. Regards, Taichi Kato VSNET Collaboration team
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