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V585 Lyr: Brno observation Dear Colleagues, We have also received the following report from Rudolf Novak: === Dear colleagues I just made more precise analyses of the dataset obtained here in Brno at 14.9.2003. I use 40cm reflector with ST-7 CCD and R filter (from Kron-Cousins). The star was quite bright, since I have no R magnitudes for the field I can't say exact value. Using comparison star and check stars I got linear profile of variable. Uncertainty of the run was computed as error of linear fit and was equall to 0.04 mag. Comparison star was measured with 0.01 mag uncertainty. Error of variable is same as error computed for another constant star with quite exact same brightness so I suspect that there was no variability at all (more than 0.04mag) in V585 Lyr system. During the run the star was very little brightening. I include the whole dataset here altogether with deep-field image of the field (combine 490 images, each 30s exposure). With best regards Rudolf Novak Copernicus Observatory Brno, Czech Republic === Regards, Taichi Kato VSNET Collaboration team
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