OQ208, a non-ideal VLBI calibrator of flux density

Details OQ208, a non-ideal VLBI calibrator of flux density OQ208, a non-ideal VLBI calibrator of flux density

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993acasn..34...12z&link_type=abstract

Acta Astronomica Sinica (ISSN 0001-5245), vol. 34, no. 1, p. 12-16.

Astronomy and Astrophysics

Astronomy

3

Calibrating, Flux Density, Very Long Base Interferometry, Antennas, Image Analysis

Scientific paper

OQ208 is used more and more frequently as a VLBI calibrator of flux density. A 5-GHz VLBI image of OQ208 is provided. Its structure consists of a compact core and a component. The angular distance between the core and the component is about 7 milliarcsecs; the position angle is -125 degrees. In principle, OQ208 is not an ideal VLBI calibrator of flux density. This paper provides the structural information for correction of the structure effect when OQ208 is used as a calibrator.

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