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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

Dreher, J.W., 1981, A.J.,86, 833.CrossRefGoogle Scholar
Eales, S.A., Duncan, W.D., and Alexander, P., 1990, Submillimeter Astronomy, eds. Watt, G.D. and Webster, A.S., Kluwer Academic Publishers.Google Scholar
Wright, M.C.H., and Birkinshaw, M., 1984, Ap.J. 281, 135.CrossRefGoogle Scholar