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The Method ‘Clean’ — Use, Misuse and Variations

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Image Formation from Coherence Functions in Astronomy

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 76))

Summary

The mathematical background of the method CLEAN, as given by Schwarz (1978) is summarized. A method to derive source parameters (flux, position, extent) as a direct application of the theory is described. The ambiguity of the CLEAN method is discussed from a theoretical and practical point of view. Empirical results on the influence of the loop-gain are given. A new approach for the processing of maps with limited phase information is presented and a novel application of CLEAN for beam-switching observations (as an example for the case of a non-symmetric beam) is given.

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© 1979 D. Reidel Publishing Company

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Schwarz, U.J. (1979). The Method ‘Clean’ — Use, Misuse and Variations. In: Van Schooneveld, C. (eds) Image Formation from Coherence Functions in Astronomy. Astrophysics and Space Science Library, vol 76. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-9449-2_30

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  • DOI: https://doi.org/10.1007/978-94-009-9449-2_30

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-009-9451-5

  • Online ISBN: 978-94-009-9449-2

  • eBook Packages: Springer Book Archive

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