TeV Gamma Ray Observations of PSR J1420-6048 with the CANGAROO-II Telescope

Details TeV Gamma Ray Observations of PSR J1420-6048 with the CANGAROO-II Telescope TeV Gamma Ray Observations of PSR J1420-6048 with the CANGAROO-II Telescope

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.2489n&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

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PSR J1420-6048 is a young radio pulsar recently discovered within the error box of the EGRET source 3EG 1420-6038. The pulse period is 68 ms, and both the spin-down energy and flux are as large as those of the pulsars in the TeV gamma ray detected nebulae, Crab and PSR B1706-44. Thus PSR J1420-6048 is a good candidate TeV gamma ray source, and so we observed it with the CANGAROO-I I telescope in March and June 2002. No significant excess of gamma ray events was detected, and we have placed an upper limit on

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