Dear Colleagues, desiote of the passing clouds, I managed to get 3 hours of very beautiful data. The light curve is amazing: eclipses are deep and the star enters eclipses arriving from its higher peak. Just after the beginning of recovery, the star experiences a secondary hump, of about 0.07 mag., with another minor fading, followed by another hump, another fading and, finally, it reaches the maximum. So, within the phases 0 -> 1, there are three ascending maxima, starting from the eclipse and ending with the higher one, going directly into the eclipse. As I have some other urgent observations under way, I will report my curve and my data with some delay. 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 * ***********************************************************************