Dear Colleagues, I've previously sent a preliminary description of the behaviour of WZ Sge as from my last night observation. Now, here is more complete one, based on the analysis of more than 1800 frames, grabbed under one of the best skies i've ever seen over Ceccano. The observing session lasted 8.5 hours and the resulting light curve shows that something of very importat is happening there. I've found 0.15 mag. superhumps, which shape is this time very simple! Sometimes peaks are sharper, sometimes broader, with very regular profile. After the peak, there is some flickering and the secondary hump is almost absent or weak (and located near the eclipse). Eclipses (and their expected times are marked with * on the light curve posted at the URL below) are very weak and 0.05 mag. deep; they are located close to previsions, but not exactly tuned with them: some of them are closer than others to times derived from ephemeris; it is interesting to note that the 6th ecplise occurred in coincidence of a small peak. I performed PDM analysis using "Period", getting an estimate of 0.05774d. The curve is sposted at. http://vsnet.eurolink.it/comets/wzsge.htm Regards, Gianluca -- *********************************************************************** * Gianluca Masi "Two things fill the soul * * Via Madonna de Loco, 47 with awe and reverence [...]: * * 03023 Ceccano (FR) the starry sky above me and * * ITALY the moral law within me" * * e-mail: gianmasi@fr.flashnet.it * * web: http://vsnet.eurolink.it/comets/ I. Kant * * Minor Planet Center Obs. Code: 470 - Ceccano * * Center for Backyard Astrophysics - Italy * * VSNET Collaboration Team member * * CCD-astrometry-photometry@yahoogroup.com mailing-list moderator * ***********************************************************************