Profile fitting for the stellar photometry

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5097

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DC Field	Value	Language
dc.contributor.author	Sagar, R	-
dc.date.accessioned	2010-04-09T14:31:02Z	-
dc.date.available	2010-04-09T14:31:02Z	-
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. 79 – 85	en
dc.identifier.uri	http://hdl.handle.net/2248/5097	-
dc.description	Open Access	en
dc.description.abstract	The point spread functions used for doing photometry on two-dimensional stellar images are described. Analytical functions used for this purpose are discussed and it is indicated that amongst them modified Lorentzian fits the best to the observed stellar profile. The computer programs presently used in crowded stellar region for accurate photometry are also described.	en
dc.language.iso	en	en
dc.publisher	Tata Institute of Fundamental Research	en
dc.rights	© Tata Institute of Fundamental Research	en
dc.subject	Stellar Photometry	en
dc.subject	Stellar Images	en
dc.subject	Modified Lorentzian	en
dc.subject	Stellar Profile	en
dc.subject	Stellar Region	en
dc.subject	Photometry	en
dc.title	Profile fitting for the stellar photometry	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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