DV UMa: eclipses on April 9 The Kyoto team has succeeded in obtaining the light curves of three eclipses of DV UMa on April 9. There is no superhump in this light curve. The eclipses apparently have two components, one is presumably of a disk and the other is probably of a white dwarf or a very bright region in an inner accretion disk: the object must have been in a very early phase of superoutburst at that time. The superoutburst is still ongoing. More time-series observations are encouraged. The weather was bad for these days in Kyoto, but we will be able to restart observations tonight. Regards, Makoto Uemura