PACT results on very high energy g-ray emission from CRAB pulsar

Sripathi Acharya, B; Vishwanath, P. R; Bhat, P. N; Chitnis, V. R; Majumdar, P; Rahman, M. A; Singh, B. B

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dc.contributor.author	Sripathi Acharya, B
dc.contributor.author	Vishwanath, P. R
dc.contributor.author	Bhat, P. N
dc.contributor.author	Chitnis, V. R
dc.contributor.author	Majumdar, P
dc.contributor.author	Rahman, M. A
dc.contributor.author	Singh, B. B
dc.date.accessioned	2009-06-17T16:57:15Z
dc.date.available	2009-06-17T16:57:15Z
dc.date.issued	2003-07
dc.identifier.citation	Kajita, 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. 2501 - 2504	en
dc.identifier.isbn	4-946443-80-0
dc.identifier.uri	http://hdl.handle.net/2248/4562
dc.description.abstract	The data taken on the Crab pulsar by the recently commissioned array of ˇ Cerenkov telescopes at Pachmarhi using the wave front sampling technique have been analyzed. The phasograms show significant excess of events at the Radio Main Pulse phase. This excess corresp onds to a 5.7σ signal and is confined to a narrow angular region around the source. It is present in most runs indicating constancy of emission. The energy estimate of the events indicate that the signal is due to higher energy events. This excess could corresp ond to the possible second component of Outer Gap models.	en
dc.language.iso	en	en
dc.publisher	International Union of Pure and Applied Physics	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2003ICRC....4.2501S	en
dc.subject	PACT Results	en
dc.subject	Very High Energy g-Ray Emission	en
dc.subject	CRAB Pulsar	en
dc.subject	Radio Main Pulse Phase	en
dc.title	PACT results on very high energy g-ray emission from CRAB pulsar	en
dc.type	Article	en