The realization of a high angular resolution in astronomical observations

Details The realization of a high angular resolution in astronomical observations The realization of a high angular resolution in astronomical observations

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989azh....66..631d&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 66, May-June 1989, p. 631-640. In Russian.

Astronomy and Astrophysics

Astronomy

1

Angular Resolution, Astronomical Observatories, High Resolution, Image Processing, Globular Clusters, Halley'S Comet, Image Analysis, Optimization, Telescopes

Scientific paper

A complex approach to increasing the angular resolution of astronomical observations is proposed. It accounts for the optimization of the optical tract of the atmosphere, telescope, and receiver and the subsequent application of a posteriori processing. It was possible to increase the resolution of the reference material by 1.1-1.3 times for Comet Halley and by 1.3 times for M 13.

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