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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2796
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dc.contributor.authorRannot, R. C-
dc.contributor.authorYadav, K. K-
dc.contributor.authorDhar, V. K-
dc.contributor.authorTickoo, A. K-
dc.contributor.authorBhatt, N-
dc.contributor.authorBhattacharyya, S-
dc.contributor.authorChandra, P-
dc.contributor.authorGoyal, H. C-
dc.contributor.authorKaul, C. L-
dc.contributor.authorKaul, R. K-
dc.contributor.authorKothari, M-
dc.contributor.authorKotwal, S-
dc.contributor.authorKoul, R-
dc.contributor.authorSahayanathan, S-
dc.contributor.authorSapru, M. L-
dc.contributor.authorSharma, M-
dc.contributor.authorVenugopal, K-
dc.contributor.authorBhat, C. L-
dc.date.accessioned2008-07-22T09:09:52Z-
dc.date.available2008-07-22T09:09:52Z-
dc.date.issued2002-09-
dc.identifier.citationBASI, Vol. 30, No. 3, pp. 699 - 700en
dc.identifier.urihttp://hdl.handle.net/2248/2796-
dc.description.abstractThe TACTIC Imaging Element has observed Crab Nebula/pulsar for a total. of about 40 hours during Jan.- Mar. 2001. Preliminary results do not show any evidence of the 33 ms pulsations from the pulsar direction at an energy threshold of 1 TeV. The 99.9% confidence level upper limit for pulsed emission has been derived to be ~ 22% of the steady flux from the Crab Nebula.en
dc.format.extent73748 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectTeV Gamma Raysen
dc.subjectThe Crab Nebulaen
dc.titleSearch for pulsed Te V gamma- rays from Crab pulsar with the TACTIC Imaging gamma-ray Telescopeen
dc.typeArticleen
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