Free Access
Issue
Astron. Astrophys. Suppl. Ser.
Volume 120, Number 2, December_I 1996
Page(s) 375 - 384
DOI https://doi.org/10.1051/aas:1996287
Published online 15 December 1996
An approach to interferometric mosaicing DOI: 10.1051/aas:1996287

Astronomy and Astrophysics Supplement Series, Vol. 120, December I 1996, 375-384

An approach to interferometric mosaicing

R.J. Sault , L. Staveley-Smith and W.N. Brouw
Send offprint requests to: R.J. Sault

Australia Telescope National Facility, CSIRO, P.O. Box 76, Epping, N.S.W. 2121, Australia
Netherlands Foundation for Research in Astronomy, Postbus 2, 7990 AA Dwingeloo, The Netherlands

Received October 2, 1995; accepted April 19, 1996

Abstract:

In radio astronomy, mosaicing is the practice of combining multiple pointings of a telescope to produce an image significantly larger than the telescope's primary beam. We consider an approach to imaging and deconvolving interferometric mosaic observations. This approach directly deconvolves a linear mosaic of dirty images. We consider the advantages and limitations of this technique. Projection issues for mosaicing are also discussed. We present an example from a 320-pointing, spectral-line, mosaiced observation of the Small Magellanic Cloud.

Key words: techniques: interferometric --- methods: data analysis --- Magellanic Clouds --- radio lines: galaxies



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