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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2534
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dc.contributor.authorChandrasekhar, T-
dc.contributor.authorShah, R-
dc.contributor.authorMondal, S-
dc.date.accessioned2008-06-27T11:05:15Z-
dc.date.available2008-06-27T11:05:15Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 3&4, pp. 471 - 474en
dc.identifier.urihttp://hdl.handle.net/2248/2534-
dc.description.abstractRecently we have successfully observed the lunar occulation of a carbon star IRC+20120 and a M5 star IRC+10241 with the NICMOS sub array at the 1.2m Gurushikhar telescope. The integration times were respectively 5 millisec and 3 millisec per sample in the broad K band. The interval between two integrations was ~ 16 millisec. FOV of the sub array was 10 arcsec x 10 arcsec. Details of the experiment and results are discussed.en
dc.format.extent115163 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31..471Cen
dc.subjectInfrared arraysen
dc.subjectLunar occultaionen
dc.subjectHigh angular resolutionen
dc.titleLunar Occulations with Infrared Arraysen
dc.typeArticleen
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