Deconvolution and self-calibration in radio astronomy using MEM

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5945

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DC Field	Value	Language
dc.contributor.author	Shevgaonkar, R. K	-
dc.date.accessioned	2012-12-12T10:49:54Z	-
dc.date.available	2012-12-12T10:49:54Z	-
dc.date.issued	1988	-
dc.identifier.citation	Velusamy, T and Venugopal, V. R eds., Image processing in astronomy: Proceedings of the workshop in imaging processing in astronomy held in Ooty 23 - 27 March 1987, pp. 119 - 131	en
dc.identifier.uri	http://hdl.handle.net/2248/5945	-
dc.description.abstract	Aperture synthesis technique is the most powerful indirect imaging technique used in radio astronomy for obtainIng high resolution images. The technique, instead of measuring the image directly, measures its Fourier components which form the required image after Fourier inversion.	en
dc.language.iso	en	en
dc.publisher	Tata Institute of Fundamental Reserach	en
dc.title	Deconvolution and self-calibration in radio astronomy using MEM	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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