Instituto de Astronomía. Universidad Nacional Autónoma de México
Abstract
As a part of our collaboration in the COSMOS Project, devoted to the characterization of galaxies during the ep o c h of maximum star formation in the history of the Universe, we have carried out a deep photometric survey covering about 380 arcmin^(2) in the so-called Groth Strip Flanking Fields. The observations were obtained in the K´ band with the OMEGA-PRIME infrared camera at the 3.5 m telescope at the Hispano–German Calar Alto Observatory . Galaxy counts and photometric redshifts will be computed in order to prepare future observations with EMIR
