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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2485
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dc.contributor.authorBaliyan, K. S-
dc.contributor.authorGanesh, S-
dc.contributor.authorJoshi, U. C-
dc.contributor.authorGlass, I. S-
dc.date.accessioned2008-06-23T07:30:39Z-
dc.date.available2008-06-23T07:30:39Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 3&4, pp. 403 - 405en
dc.identifier.urihttp://hdl.handle.net/2248/2485-
dc.description.abstractInner 300 pc of the Galactic Center region is surveyed with the SIR-IUS camera mounted on the InfraRed Survey Facility (IRSF) telescope of the SAAO, during June-July 2002, resulting in the deepest near infrared view of the Milky Way Nuclear Bulge Region. Here we present first results from this survey underlining the capabilities of the SIRIUS camera and the photometric procedures adopted in this work involving highly crowded star fields.en
dc.format.extent94623 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31..403Ben
dc.subjectGalaxyen
dc.subjectMilky way: nuclear bulgeen
dc.subjectSurveys: near infrareden
dc.titleNear Infrared Survey of the Galactic Nuclear Bulge Regionen
dc.typeArticleen
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