Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/726
Full metadata record
DC FieldValueLanguage
dc.contributor.authorDas, H. K-
dc.contributor.authorKohok, A-
dc.contributor.authorTandon, S. N-
dc.date.accessioned2006-03-13T06:24:49Z-
dc.date.available2006-03-13T06:24:49Z-
dc.date.issued2004-06-
dc.identifier.citationBASI, Vol. 32, No. 2, pp. 121-131en
dc.identifier.urihttp://hdl.handle.net/2248 /726-
dc.description.abstractBased on the transfer pupil technique we develop a method to measure the lower order aberration coeffcients for optical telescopes; the method makes use of a Hartmann mask in a spectrograph for sampling the wavefront at different locationsen
dc.format.extent115068 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectOptical telescopesen
dc.titleAn implementation of transfer-pupil in a spectrograph on optical telescopesen
dc.typeArticleen
Appears in Collections:BASI Publications

Files in This Item:
File Description SizeFormat 
HK_DAS.PDF112.37 kBAdobe PDFThumbnail
View/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.