Bolognino, Irene (2011) Gamma astronomy with ARGO-YBJ. Il nuovo cimento C, 34 (6). pp. 348-349. ISSN 1826-9885
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Abstract
ARGO-YBJ, an extensive air shower detector located at Yangbajing (Tibet, China) at 4300m a.s.l., is made by a full coverage carpet plus a guard ring (∼ 6700m2) of resistive plate chambers. Its structure, and the high altitude allow exhaustive studies of γ astronomy with energy range in the TeV region. In this paper some of the ARGO-YBJ results in γ astronomy are discussed. In particular the TeV emissions of the blazar Mrk 421, the analysis of its last two flares and the comparison with Cherenkov telescopes results are presented.
| Item Type: | Article |
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| Uncontrolled Keywords: | X- and γ-ray telescopes and instrumentation ; γ-ray sources; γ-ray bursts |
| Subjects: | 500 Scienze naturali e Matematica > 530 Fisica |
| Depositing User: | Marina Spanti |
| Date Deposited: | 14 Apr 2020 13:35 |
| Last Modified: | 14 Apr 2020 13:35 |
| URI: | http://eprints.bice.rm.cnr.it/id/eprint/17611 |
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