  The design and implementation of astronomical cameras based on the
large-format CCD and CMOS detectors is described in this paper. The Dinacon-5
controller is used for work with the CCDs and to achieve high performance and
low noise. A new controller is designed for CMOS sensors. The main
characteristics of the provided systems are estimated on the basis of
experimental data. The spatial autocorrelation analysis is applied for PSF
estimation. The obtained test results are presented.
