Preliminary results on the flux of TeV g-rays from crab system obtained with the PACT at Pachmarhi

dc.contributor.author	Sripathi Acharya, B
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.contributor.author	Vishwanath, P. R
dc.date.accessioned	2009-06-17T16:58:28Z
dc.date.available	2009-06-17T16:58:28Z
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. 2391 - 2394	en
dc.identifier.isbn	4-946443-80-0
dc.identifier.uri	http://hdl.handle.net/2248/4563
dc.description.abstract	We 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.iso	en	en
dc.publisher	International Union of Pure and Applied Physics	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2003ICRC....4.2381S	en
dc.relation.uri	http://www.uap.co.jp/uap/Publication/SERIES/DATA/00081/index.html	en
dc.subject	Crab system	en
dc.subject	Nebula	en
dc.subject	Pulsar	en
dc.subject	PACT	en
dc.subject	Crab Nebula	en
dc.subject	γ -rays	en
dc.title	Preliminary results on the flux of TeV g-rays from crab system obtained with the PACT at Pachmarhi	en
dc.type	Article	en