Dear Colleagues, a look to the data from my last night run, shows that no particular modulation is present in the resulting light curve. So, no superhumps here. I performed astrometry of the source with the following result: V589 HER R.A:16 22 07.15, Decl.: +19 22 37.2 (J2000.0) 8 reference stars from USNO A2.0; mean residuals: 0.25" Dr. Yamaoka will be performing independent astrometry of some images of mine and will be informing us about his results. Sincerely, Gianluca Masi Bellatrix Observatory -- *********************************************************************** * 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 * ***********************************************************************