Observation of Sub-TeV Gamma-Rays from RX J0852.04622 with the CANGAROO-II Telescope

Details Observation of Sub-TeV Gamma-Rays from RX J0852.04622 with the CANGAROO-II Telescope Observation of Sub-TeV Gamma-Rays from RX J0852.04622 with the CANGAROO-II Telescope

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.2409k&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

RX J0852.0-4622 (G266.2-1.2) is a type-I I supernova Remnant (SNR) located along the line of sight to the Vela SNR. We observed RX J0852.0-4622 with the CANGAROO-I I telescope from the middle of December, 2001, to the end of February, 2002, to search for sub-TeV gamma-rays. A preliminary analysis shows an apparent excess of gamma-ray-like events in alpha distribution from RX J0852.0-4622, which is to be examined in continued analyses and further observations.

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