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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2204
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dc.contributor.authorAnandarao, B. G-
dc.contributor.authorNanda Kumar, M. S-
dc.contributor.authorJog, N. S-
dc.contributor.authorPatel, R. T-
dc.date.accessioned2008-04-03T09:11:13Z-
dc.date.available2008-04-03T09:11:13Z-
dc.date.issued2000-
dc.identifier.citationBASI, Vol. 28, No. 4, pp. 687 - 695en
dc.identifier.urihttp://hdl.handle.net/2248/2204-
dc.description.abstractWe describe here a Near-Infrared Imaging Fabry-Perot Spectrometer (NIFS ) operating in the K band to provide a maximum spectral resolution of 2000-3000 over two optional fields of view of ~ 2? x 2? and 4? x 4? with plate scales of 0.5? and 1? / pixel respectively. N I F S is an add-on instrument to an existing infrared camera with a 256x256 HgCdTe array detector. The instrument is operational with a 1.2 m telescope to primarily work on star forming regions and starburst galaxies which strongly emit in several diagnostically important lines within the K band. The design, testing and operation of NIFS are discussed in the light of preliminary observations made on the Orion Molecular Cloud Complex.en
dc.format.extent841203 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28..687Aen
dc.subjectTechniques:spectroscopicen
dc.subjectInstrumentation:spectrographsen
dc.subjectInfrared:generalen
dc.titleNIFS : A Near Infrared Imaging Fabry-Perot Spectrometeren
dc.typeArticleen
Appears in Collections:BASI Publications

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