Technique for conducting a fast sky survey at 8550 MHz and computer processing of radio astronomical data

Details Technique for conducting a fast sky survey at 8550 MHz and computer processing of radio astronomical data Technique for conducting a fast sky survey at 8550 MHz and computer processing of radio astronomical data

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976azh....53..241l&link_type=abstract

Astronomicheskii Zhurnal, vol. 53, Mar.-Apr. 1976, p. 241-250. In Russian.

Astronomy and Astrophysics

Astronomy

Computer Techniques, Data Processing, Radio Astronomy, Radio Sources (Astronomy), Signal To Noise Ratios, Sky Surveys (Astronomy), Angular Velocity, Digital Computers, Error Analysis, Flux Density, Magnetic Recording, Microwave Equipment, Monte Carlo Method, Position Errors

Scientific paper

A fast survey of the sky region between declinations 0 and +30 deg was carried out with a 22-m reflector at 8550 MHz over an area of 2 sr. The survey technique is described. A magnetic tape-recorder was used for recording the receiver output. The principal receiver parameters are reported. Davis' (1967) method of searching for sources was used. Completeness, reliability, flux density and position errors are analyzed. The same parameters are reported for reobservations of the surveyed sources in the selected areas.

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