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The given work is devoted to the modern developments in the field of radioastronomy instrumentation. In particular, the sensitivity of the multi-beamreflector radio telescope which is fed by phased array (PAF) is considered.Using PAF as reflector feed allows obtaining wide and continuous field of view(FOV) of the telescope. This has several advantages with compare tohorn-cluster feeds which are described in this work. The sensitivity insidewhole FOV was computed using three different beamforming schemes.

Multi-beaming propertieis of reflector antennas used in radio telescopes with wide field of view