Dear colleagues, We made 120s second image of CI Gem with CCD ST-7 (I band) placed on Nicholas copernicus observatory in Brno. There is no new star on position given by Downes & Shara brighter than 17-18 mag. As mentioned by P. Schmeer the right position could be different. We placed CCD image on CBA Brno web page where is possible new star marked by arrows. Please have a look and send your comments if we are wrong. Now we are slowly finishing ~3hr. run of CT Hya. The star is bright and clearly visible on our CCD images. Observation made 16.02.1999 (my birth day! :) shows a superhumps with an amplitude close to 0.2 mag as reported by Taichi Kato. When todays run will be analyzed I'll send a results. With best regards Rudolf Novak CBA Brno web: http://i.am/cba