Aspects of Design and Development of a Near Infrared Photometer for Low Altitude Astronomical Sites

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/8047

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DC Field	Value	Language
dc.contributor.author	Anwesh Kumar, M	-
dc.date.accessioned	2022-09-07T05:09:45Z	-
dc.date.available	2022-09-07T05:09:45Z	-
dc.date.issued	2021-01	-
dc.identifier.citation	Ph.D. Thesis, University of Calcutta, Calcutta	en_US
dc.identifier.uri	http://hdl.handle.net/2248/8047	-
dc.description	Thesis Supervisor Prof. U. S. Kamath	en_US
dc.description.abstract	In order to fill the void of observation of bright near infrared astronomical sources, we propose a Near Infrared photometer operating from a low latitude astronomical site. As part of this thesis work, design decisions defining the specifications of such a photometer is presented. InGaAs single pixel detectors and IRWG (Infrared Working Group) recommended filters are identified to be capable of achieving high signal to ratio while observing bright sources with short integration duration. Design, development and tests of various components of this photometer are discussed.	en_US
dc.language.iso	en	en_US
dc.publisher	Indian Institute of Astrophysics	en_US
dc.relation.uri	© Indian Institute of Astrophysics	-
dc.title	Aspects of Design and Development of a Near Infrared Photometer for Low Altitude Astronomical Sites	en_US
dc.type	Thesis	en_US
Appears in Collections:	IIAP Ph.D.Theses

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