Observations of Markarian 421 by the CAT imaging telescope

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DC Field	Value	Language
dc.contributor.author	Fleury, P	-
dc.date.accessioned	2008-06-13T06:22:28Z	-
dc.date.available	2008-06-13T06:22:28Z	-
dc.date.issued	2002	-
dc.identifier.citation	BASI, Vol. 30, No. 1, pp. 291 - 296	en
dc.identifier.uri	http://hdl.handle.net/2248/2425	-
dc.description.abstract	The CAT imaging telescope has been exploited since 1997 for the observation of Mrk-421 among other sources. After a brief review of the characteristics of the CAT telescope, the event reconstruction method will be described. We then present recent analysis results, with emphasis on the determination of the energy spectrum, its shape and its dependence upon the level of activity of the blazar.	en
dc.format.extent	546877 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2002BASI...30..291F	en
dc.subject	Gamma Astronomy	en
dc.subject	Space Astronomy	en
dc.subject	Atmospheric Cherenkov Detectors	en
dc.title	Observations of Markarian 421 by the CAT imaging telescope	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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