Deconvolution and self-calibration in radio astronomy using MEM

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