Dear Colleagues, I performed a run on the variable in the subject, getting the following results. While the dataset is still noisy, mainly dued to the very brigh moon, there is clear evidence of a superhump. I will be sending an url with the light curve soon, as I have to do the plot. Also, it very difficult to estimate, at least with the eyes, the superhump period, because the run icluded only an hump. More details will be available later. 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 * ***********************************************************************