Dear readers, is anybody able to do precise CCD photometry of SW UMa? This should be very interesting to confirm results of OUDA and Brno observations from last year - increasing period during superoutburst and QSO's. And of course more covered first stages of superoutburst - we had just one night last year. I hope that dr. Kato will send article about SW UMa to vsnet soon - to inform you about results of our work. What about it dr. Kato? Have a nice day/night Rudolf