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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4563
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dc.contributor.authorSripathi Acharya, B-
dc.contributor.authorBhat, P. N-
dc.contributor.authorChitnis, V. R-
dc.contributor.authorMajumdar, P-
dc.contributor.authorRahman, M. A-
dc.contributor.authorSingh, B. B-
dc.contributor.authorVishwanath, P. R-
dc.date.accessioned2009-06-17T16:58:28Z-
dc.date.available2009-06-17T16:58:28Z-
dc.date.issued2003-07-
dc.identifier.citationKajita, Y. Asaoka, A. Kawachi, Y. Matsubara and M. Sasaki., eds., Proceedings of the 28th International Cosmic Ray Conference. July 31 - August 7, Trukuba, Japan, 2003. pp. 2391 - 2394en
dc.identifier.isbn4-946443-80-0-
dc.identifier.urihttp://hdl.handle.net/2248/4563-
dc.description.abstractWe have observed the Crab system (Nebula and Pulsar) and the corresponding background regions during many clear nights in the years 1999-2002 ˇ using the atmospheric Cerenkov array at Pachmarhi, PACT. Preliminary results indicate a steady emission of TeV γ -rays from the Crab Nebula.en
dc.language.isoenen
dc.publisherInternational Union of Pure and Applied Physicsen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003ICRC....4.2381Sen
dc.relation.urihttp://www.uap.co.jp/uap/Publication/SERIES/DATA/00081/index.htmlen
dc.subjectCrab systemen
dc.subjectNebulaen
dc.subjectPulsaren
dc.subjectPACTen
dc.subjectCrab Nebulaen
dc.subjectγ -raysen
dc.titlePreliminary results on the flux of TeV g-rays from crab system obtained with the PACT at Pachmarhien
dc.typeArticleen
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