Dear colleagues, I just analyzed a run obtained yesterday by Petr Sobotka here at Brno. The light curve is very impressive - hump-like modulation which seems like the one observed by T. Kato (vsnet-superoutburst 364). The dataset will be sent to VSNET collaboration team for period analyzing. Light curve with some more information will be posted now to Amateru Data Archive (http://ada.astronomy.cz), in a few hours Sun will set and I will continue using 60cm reflector of masaryk University to get another run on this object. With best regards Rudolf Novak N. Copernicus Observatory Brno, CZ http://codel.astronomy.cz
vsnet-adm@kusastro.kyoto-u.ac.jp