Dear Colleagues, we reduced the images collected last night, with the 0.8m-f/8 telescope (Campocatino Astronomical Observatory) when we followed this star for about 3 hours. As we have already reported early this morning to Dr. Kato, our light-curve shows an evident modulation (probable superhumps), with a full amplitude of less than 0.1 mag. (unfiltered CCD photometry). The signal is clearly modulated by a period around 25 minutes (as reported by Matt Wood). During the run the star showed a constant fading, loosing 0.05 mag during the 3+ hours. Regards, Gianluca Masi, Ugo Tagliaferri PS: as reported, a reference image from the current outburst can be faound at: http://vsnet.bellatrixobservatory.org/kldra.jpg -- *********************************************************************** * 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.bellatrixobservatory.org 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 * ***********************************************************************