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Hot spots in Cygnus A; A mosaiced map at 86 GHz

Published online by Cambridge University Press:  12 April 2016

M.C.H. Wright  and
R.J. Sault
M.C.H. Wright
Affiliation:
Radio Astronomy Laboratory, University of California, Berkeley
R.J. Sault
Affiliation:
National Center for Supercomputing Applications, University of Illinois, Urbana-Champaign

Abstract

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We describe a new software package, MIRIAD, for making multichannel images of multiple-field aperture synthesis observations. As an example of the use of the new software we present a map of the radio galaxy Cygnus A. We used the BIMA array to map Cygnus A at 86 GHz with 2.28 × 3.06 arcsec resolution in 3 fields centered on the central radio source and the radio hot spots in each radio lobe. The 3 fields were combined and deconvolved to find the positions and flux densities of the radio source components.

Type
Imaging
Information
International Astronomical Union Colloquium , Volume 131: Radio Interferometry: Theory, Techniques, and Applications , 1991 , pp. 276 - 280
Copyright
Copyright © Astronomical Society of the Pacific 1991

References

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