Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2333
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dc.contributor.authorBanerjee, D. P. K-
dc.contributor.authorBobra, A. D-
dc.contributor.authorSubhedar, D. V-
dc.date.accessioned2008-05-21T11:26:59Z-
dc.date.available2008-05-21T11:26:59Z-
dc.date.issued1997-
dc.identifier.citationBASI, Vol. 25, No. 4, pp. 555 - 562en
dc.identifier.urihttp://hdl.handle.net/2248/2333-
dc.description.abstractThe achromatic aberrations, which in general affect image quality in telescopes, have been studied in context of the 1.2 m Gurusikhar Infrared Telescope. The analysis gives the magnitudes of aberrations for different fields of view at the Cassegrain and prime focus thereby indicating the optimal field diameter that may be used for observations. The range of acceptable back – focal distances have also been worked out, thereby setting constraints on the location of the focal plane in back – end instruments to be used on the GRIT. This study should be especially useful while designing instruments for the 1.2 m telescope, in planning observations or in subsequent data analysisen
dc.format.extent548262 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1997BASI...25..555Ben
dc.subjectAberrationsen
dc.subjectCassegrain Focusen
dc.subjectPrime Focusen
dc.titleThe effect of aberrations on image quality - A study for the 1.2m Gurusikhar Infrared Telescopeen
dc.typeArticleen
Appears in Collections:BASI Publications

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