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Dear Colleagues, I've analyzed a fraction of my latest run, from Aug 3.88 to Aug 4.06. The lightcurve is broader, as reported by Dr. Kato in vsnet-alert 6187. But sometimes peaks are closer and sharper than in other occasions, during the same run. If I combine these (partial: 2-hours of observations are still under reduction) data with the ones I've got yesterday I have, with PDM analysis via AVE, a period candidate of 0.05659d, this confirming the tendency to have a shorter period than the orbital one. When the whole dataset will be reduced I'll perform a definitive analysis, posting data on my website and sending them to Kyoto. 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@egroup.com mailing-list moderator * ***********************************************************************
Return to the Powerful Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
