Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5097
Title: Profile fitting for the stellar photometry
Authors: Sagar, R
Keywords: Stellar Photometry;Stellar Images;Modified Lorentzian;Stellar Profile;Stellar Region;Photometry
Issue Date: 1988
Publisher: Tata Institute of Fundamental Research
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
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.
Description: Open Access
URI: http://hdl.handle.net/2248/5097
???metadata.dc.rights???: © Tata Institute of Fundamental Research
Appears in Collections:IIAP Publications

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