a Northern Sky Survey for both Tev Cosmic-Ray Anisotropy and Tev Gamma-Ray Sources Using the Tibet Air Shower Array

Details a Northern Sky Survey for both Tev Cosmic-Ray Anisotropy and Tev Gamma-Ray Sources Using the Tibet Air Shower Array a Northern Sky Survey for both Tev Cosmic-Ray Anisotropy and Tev Gamma-Ray Sources Using the Tibet Air Shower Array

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005iche.conf..448z&link_type=abstract

HIGH ENERGY PHYSICS, ICHEP 2004. Proceedings of the 32nd International Conference. Held 16-22 August 2004 in Beijing, China. Edi

Physics

High Energy Physics

Scientific paper

Results on TeV γ-ray point source search using data taken from Tibet-HD (Feb.1997-Sep.1999) and Tibet-III (Nov.1999-0ct.2001) are presented. From 0° to 60° in declination, two sources, the well-known steady source Crab Nebula and the high state of the flare type source Markarian 421, are detected by all-sky survey. The large scale anisotropy of cosmic-ray intensity with a magnitude about 0.1% is observed simultaneously. For purpose of cross check, two techniques based on the equi-zenith method are independently developed.

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