V485 Cen superhumps The analysis of the early part of the Kyoto data (March. 31 - Apr. 5, 2466 points) obtained by Ishioka-san et al. clearly shows the presence of superhumps. The object has shown monotonous fading during this period. The average superhump period is 0.04209 d, which is slightly shorter than the previous report by Olech (Acta Astrion. 47, 281). More detailed analysis, together with newly available and newly coming data, and further information will be presented by Ishioka-san. Further observations are strongly encouraged. Regards, VSNET Collaboration team