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2015ApJ...813...98A - Astrophys. J., 813, 98 (2015/November-2)

Search for gamma rays above 100 TeV from the Crab nebula with the tibet air shower array and the 100 m² muon detector.

AMENOMORI M., BI X.J., CHEN D., CHEN T.L., CHEN W.Y., CUI S.W., DANZENGLUOBU, DING L.K., FENG C.F., FENG Z., FENG Z.Y., GOU Q.B., GUO Y.Q., HE H.H., HE Z.T., HIBINO K., HOTTA N., HU H., HU H.B., HUANG J., JIA H.Y., JIANG L., KAJINO F., KASAHARA K., KATAYOSE Y., KATO C., KAWATA K., KOZAI M., LABACIREN, LE G.M., LI A.F., LI H.J., LI W.J., LIU C., LIU J.S., LIU M.Y., LU H., MENG X.R., MIYAZAKI T., MIZUTANI K., MUNAKATA K., NAKAJIMA T., NAKAMURA Y., NANJO H., NISHIZAWA M., NIWA T., OHNISHI M., OHTA I., OZAWA S., QIAN X.L., QU X.B., SAITO T., SAITO T.Y., SAKATA M., SAKO T.K., SHAO J., SHIBATA M., SHIOMI A., SHIRAI T., SUGIMOTO H., TAKITA M., TAN Y.H., TATEYAMA N., TORII S., TSUCHIYA H., UDO S., WANG H., WU H.R., XUE L., YAMAMOTO Y., YAMAUCHI K., YANG Z., YASUE S., YUAN A.F., YUDA T., ZHAI L.M., ZHANG H.M., ZHANG J.L., ZHANG X.Y., ZHANG Y., ZHANG Y., ZHANG Y., ZHAXISANGZHU, ZHOU X.X. (The Tibet AS{gamma} Collaboration)

Abstract (from CDS):

A 100 m² muon detector (MD) was successfully constructed under the existing Tibet air shower (AS) array in the late fall of 2007. The sensitivity of the Tibet AS array to cosmic gamma rays can be improved by selecting muon-poor events with the MD. Our MC simulation of the MD response reasonably agrees with the experimental data in terms of the charge distribution for one-muon events and the background rejection power. Using the data collected by the Tibet AS array and the 100 m² MD taken from 2008 March to 2010 February, we search for continuous gamma-ray emission from the Crab Nebula above ∼100 TeV. No significant excess is found, and the most stringent upper limit is obtained above 140 TeV.

Abstract Copyright: ∼

Journal keyword(s): cosmic rays - gamma rays: stars - ISM: supernova remnants

Simbad objects: 3

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