Dear colleagues, we finished time-resolved photometry of SU UMa type variable CT Hya. Superhumps are apparent on light curve as suspected. Preliminary period determination (using PDM) shows a signal at 0.067+-0.001 aproximately. Further analyzis are planned. The light curves with superhumps observed at Nicholas Copernicus Observatory and Planetarium in Brno using I band on ST-7 CCD (0.4m Newton) are placed at CBA Brno page. Don't forget to visit also official variable stars web server at http://astro.sci.muni.cz/variables! :) With best regards Rudolf Novak CBA Brno, http://i.am/cba