Dear Colleagues, I reported to you a light curve, obtained from my observations presented in [vsnet-obs 19970]. To draw this curve I reported the difference V-C2, where C2 is GSC 1375:804 07h55m07.1s +22d05'14" J2000.0 V= 11.408, B-V= 0.491 The data file attached to my previous note reported the difference V-C1, but now I preferred to draw V-C2, because C1 is perhaps to red and sensitive to differential atmospheric extintion. Th elight curve is posted at http://vsnet.eurolink.it/comets/ugem.gif And it shows clearly the presence of an eclipse just after the beginning of the run. Regards, Gianluca Masi CBA - Italy -- *********************************************************************** * 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" * * email: gianmasi@fr.flashnet.it * * http://vsnet.eurolink.it/comets/ I. Kant * ***********************************************************************