Future plan for observation of cosmic gamma rays in the 100 TeV energy region with the Tibet air shower array : simulation and sensitivity

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dc.creatorAmenomori, M.
dc.creatorBi, X. J.
dc.creatorChen, D.
dc.creatorCui, S. W.
dc.creatorDanzengluobu
dc.creatorDing, L. K.
dc.creatorDing, X. H.
dc.creatorFan, C.
dc.creatorFeng, C. F.
dc.creatorFeng, Zhaoyang
dc.creatorFeng, Z. Y.
dc.creatorGao, X. Y.
dc.creatorGeng, Q. X.
dc.creatorGuo, H. W.
dc.creatorHe, H. H.
dc.creatorHe, M.
dc.creatorHibino, K.
dc.creatorHotta, N.
dc.creatorHu, Haibing
dc.creatorHu, H. B.
dc.creatorHuang, J.
dc.creatorHuang, Q.
dc.creatorJia, H. Y.
dc.creatorKajino, F.
dc.creatorKasahara, K.
dc.creatorKatayose, Y.
dc.creatorKato, C.
dc.creatorKawata, K.
dc.creatorLabaciren
dc.creatorLe, G. M.
dc.creatorLi, A. F.
dc.creatorLi, J. Y.
dc.creatorLou, Y. -Q.
dc.creatorLu, H.
dc.creatorLu, S. L.
dc.creatorMeng, X. R.
dc.creatorMizutani, K.
dc.creatorMu, J.
dc.creatorMunakata, K.
dc.creatorNagai, A.
dc.creatorNanjo, H.
dc.creatorNishizawa, M.
dc.creatorOhnishi, M.
dc.creatorOhta, I.
dc.creatorOnuma, H.
dc.creatorOuchi, T.
dc.creatorOzawa, S.
dc.creatorRen, J. R.
dc.creatorSaito, T.
dc.creatorSaito, T. Y.
dc.creatorSakata, M.
dc.creatorSako, T. K.
dc.creatorShibata, M.
dc.creatorShiomi, A.
dc.creatorShirai, T.
dc.creatorSugimoto, H.
dc.creatorTakita, M.
dc.creatorTan, Y. H.
dc.creatorTateyama, N.
dc.creatorTorii, S.
dc.creatorTsuchiya, H.
dc.creatorUdo, S.
dc.creatorWang, B.
dc.creatorWang, H.
dc.creatorWang, X.
dc.creatorWang, Y.
dc.creatorWang, Y. G.
dc.creatorWu, H. R.
dc.creatorXue, L.
dc.creatorYamamoto, Y.
dc.creatorYan, C. T.
dc.creatorYang, X. C.
dc.creatorYasue, S.
dc.creatorYe, Z. H.
dc.creatorYu, G. C.
dc.creatorYuan, A. F.
dc.creatorYuda, T.
dc.creatorZhang, H. M.
dc.creatorZhang, J. L.
dc.creatorZhang, N. J.
dc.creatorZhang, X. Y.
dc.creatorZhang, Y.
dc.creatorZhang, Yi
dc.creatorZhaxisangzhu
dc.creatorZhou, X. X.
dc.date2007-10-15
dc.date.accessioned2026-07-07T08:36:20Z
dc.date.available2026-07-07T08:36:20Z
dc.descriptionThe Tibet air shower array, which has an effective area of 37,000 square meters and is located at 4300 m in altitude, has been observing air showers induced by cosmic rays with energies above a few TeV. We have a plan to add a large muon detector array to it for the purpose of increasing its sensitivity to cosmic gamma rays in the 100 TeV energy region by discriminating them from cosmic-ray hadrons. We have deduced the attainable sensitivity of the muon detector array using our Monte Carlo simulation. We report here on the detailed procedure of our Monte Carlo simulation.
dc.description4 pages, 5 figures, 30th International Cosmic Ray Conference
dc.identifierhttps://arxiv.org/abs/0710.2752
dc.identifierhttp://arxiv.org/abs/0710.2752
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/140030
dc.subjectAstrophysics
dc.titleFuture plan for observation of cosmic gamma rays in the 100 TeV energy region with the Tibet air shower array : simulation and sensitivity
dc.typetext

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