Dear Colleagues, once again, I obtained time-series photometry for this star (it was my run n. 9). Plotting the resulting light curve from that 6.3-hours observing session it is interesting to see how the curve (of very nice quality) shows two series of maxima at the beginning of the run, turning to a complex modulation at the end. The oscillations are 0.2 mag. large. I performed PDM analysis, getting a period candidate of about 0.0576d. I look forward to see how these new observations will work with the previous dataset. The light curve and the PDM are posted, as usual, at: http://vsnet.eurolink.it/comets/wzsge.htm BTW: two night ago the star was about 0.3 mag brighter than now. Regards, Gianluca Masi -- *********************************************************************** * 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 * ***********************************************************************