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A search for 100 TeV celestial gamma rays with the Tibet air shower array and a future prospect
OtherAbstract:Palabras claves:Autores:TK SakoFuentes:googleFuture plan for observation of cosmic gamma rays in the 100 TeV energy region with the Tibet air shower array: simulation and sensitivity
OtherAbstract: The Tibet air shower array, which has an effective area of 37,000 square meters and is located at 43Palabras claves:Autores:TK SakoFuentes:googleMoon shadow by cosmic rays under the influence of geomagnetic field and search for antiprotons at multi-TeV energies
ArticleAbstract: We have observed the shadowing of galactic cosmic ray flux in the direction of the moon, the so-callPalabras claves:Air shower, Anti-matter, cosmic rays, Observation and data analysis, SimulationsAutores:Amenomori M., Ayabe S., Bi X.J., Chen D., Cui S.W., Danzengluobu , Ding L.K., Ding X.H., Feng C.F., Feng Z.Y., Gao X.Y., Geng Q.X., Guo H.W., He H.H., He M., Hibino K., Hotta N., Hu H.B., Huang J., Huang Q., Jia H.Y., Kajino F., Kasahara K., Katayose Y., Kato C., Kawata K., Labaciren , Le G.M., Li A.F., Li J.Y., Lou Y.Q., Lu H., Lu S.L., Meng X.R., Mizutani K., Mu J., Munakata K., Nagai A., Nanjo H., Nishizawa M., Ohnishi M., Ohta I., Onuma H., Ouchi T., Ozawa S., Ren J.R., Saito T., Saito T.Y., Sakata M., Sasaki T., Shibata M., Shiomi A., Shirai T., Sugimoto H., T. K. Sako, Takita M., Tan Y.H., Tateyama N., TK Sako, Torii S., Tsuchiya H., Udo S., Wang B.S., Wang H., Wang X., Wang Y.G., Wu H.R., Xue L., Yamamoto Y., Yan C.T., Yang X.C., Yasue S., Ye Z.H., Yu G.C., Yuan A.F., Yuda T., Zhang H.M., Zhang J.L., Zhang N.J., Zhang X.Y., Zhang Y., Zhaxisangzhu , Zhou X.X.Fuentes:googlescopusNew estimation of the spectral index of high-energy cosmic rays as determined by the Compton-Getting anisotropy
OtherAbstract: The amplitude of the Compton-Getting (CG) anisotropy contains the power-law index of the cosmic-rayPalabras claves:Autores:TK SakoFuentes:googleImplication of the sidereal anisotropy of∼ 5 TeV cosmic ray intensity observed with the Tibet III air shower array
OtherAbstract: We show that the large-scale anisotropy of~ 5 TeV galactic cosmic ray (GCR) intensity observed by TiPalabras claves:Autores:TK SakoFuentes:googleTwo-dimensional observation on TeV Cosmic-ray solar diurnal variation using the Tibet Air Shower Array
OtherAbstract:Palabras claves:Autores:TK SakoFuentes:googleUnderground water Cherenkov muon detector array with the Tibet air shower array for gamma-ray astronomy in the 100 TeV region
OtherAbstract: We propose to build a large water-Cherenkov-type muon-detector array (Tibet MD array) around the 37Palabras claves:Autores:TK SakoFuentes:googleSearch for pulsed multi-TeV gamma rays from the Crab pulsar u sing the Tibet-III air shower array
OtherAbstract:Palabras claves:Autores:TK SakoFuentes:google