A self-calibration procedure for a large field of view and low resolution synthesis telescope.

Details A self-calibration procedure for a large field of view and low resolution synthesis telescope. A self-calibration procedure for a large field of view and low resolution synthesis telescope.

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pbeio..20...47z&link_type=abstract

Publications of the Beijing Astronomical Observatory, No. 20, p. 47 - 50

Astronomy and Astrophysics

Astronomy

Scientific paper

A modified method of self-calibration is presented. The main feature of
the method is that the input model for self-calibration is a new kind of
CC-table which is obtained according to the sidelobe variation of
sources. By using the model, one can represent the visibility function
well. So the self-calibration can be improved.

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