Optimum deconvolution method for lunar occultations and cosmological studies using angular sizes of radio sources

Please use this identifier to cite or link to this item: http://localhost:8000/handle/2301/260

Full metadata record

DC Field	Value	Language
dc.contributor.author	Subrahmanya, C.R.	-
dc.date.accessioned	2016-05-19T07:12:03Z	-
dc.date.available	2016-05-19T07:12:03Z	-
dc.date.issued	1977-09	-
dc.identifier.citation	136 p.	en_US
dc.identifier.uri	http://hdl.handle.net/2301/260	-
dc.description	a thesis submitted for the PhD degree of the University of Bombay, 136 p.	en_US
dc.language.iso	en_US	en_US
dc.publisher	NCRA-TIFR	en_US
dc.subject	Lunar Occultations	en_US
dc.subject	Radio Sources	en_US
dc.title	Optimum deconvolution method for lunar occultations and cosmological studies using angular sizes of radio sources	en_US
dc.type	Thesis	en_US
Appears in Collections:	NCRA Thesis

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subrahmanya1.pdf	11.11 MB	Adobe PDF	View/Open
subrahmanya2.pdf	21.33 MB	Adobe PDF	View/Open
subrahmanya3.pdf	10.51 MB	Adobe PDF	View/Open
subrahmanya4.pdf	13.9 MB	Adobe PDF	View/Open

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