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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2872
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dc.contributor.authorDeep, A-
dc.contributor.authorRamaprakash, A. N-
dc.contributor.authorTandon, S. N-
dc.contributor.authorGupta, R-
dc.contributor.authorBurse, M. P-
dc.contributor.authorChordia, P. A-
dc.contributor.authorDas, H. K-
dc.contributor.authorEngineer, S-
dc.contributor.authorKohok, A. A-
dc.contributor.authorMestry, V. B-
dc.date.accessioned2008-07-24T06:23:41Z-
dc.date.available2008-07-24T06:23:41Z-
dc.date.issued2002-09-
dc.identifier.citationBASI, Vol. 30, No. 3, pp. 791 - 795en
dc.identifier.urihttp://hdl.handle.net/2248/2872-
dc.description.abstractIn this paper we present the current status of development of the Near Infrared PICNIC Imager (NIPI), which will be the first near-ffi instrument on IUCAA telescope. When used at one of the Cassegrain side ports of the telescope, it gives a plate scale of 0.8 arcsee per pixel at the PICNIC detector array with a field of view of 2.5 arc minutes. It offers imaging capabilities in J, H and K filter bands, with the reimager optimized in H-band for which almost 90encircled energy of a. point source is contained in a. pixel. Hardware and software for infrared readout are being developed at IUCAA.en
dc.format.extent157610 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectPICNICen
dc.subjectIUCAA Telescopeen
dc.subjectNear Infrared- Imageren
dc.titleNear Infrared PICNIC Imager (NIPI) for IUCAA Telescopeen
dc.typeArticleen
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