An approach to interferometric mosaicing.

Details An approach to interferometric mosaicing. An approach to interferometric mosaicing.

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26as..120..375s&link_type=abstract

Astronomy and Astrophysics Supplement, v.120, p.375-384

Astronomy and Astrophysics

Astrophysics

79

Techniques: Interferometric, Methods: Data Analysis, Magellanic Clouds, Radio Lines: Galaxies

Scientific paper

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.

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