Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Y. Q. Guo9"'
Autor:
THE ARGO YBJ C.O.L.L.A.B.O.R.A.T.I.O.N.G. Aielli1, 2, C. Bacci3, 4, B. Bartoli5, 6, P. Bernardini7, 8, X. J. Bi9, C. Bleve7, P. Branchini4, A. Budano4, BUSSINO, Severino Angelo Maria, A. K. Calabrese Melcarne10, P. Camarri1, Z. Cao9, A. Cappa11, R. Cardarelli2, S. Catalanotti5, C. Cattaneo13, P. Celio3, S. Z. Chen9, Y. Chen9, N. Cheng9, P. Creti8, S. W. Cui14, B. Z. Dai15, G. D’Al´ı Staiti16, 17, Danzengluobu18, M. Dattoli11, 12, 19, DE VINCENZI, Mario, B. D’Ettorre Piazzoli5, M. De Vincenzi3, T. Di Girolamo5, X. H. Ding18, G. Di Sciascio2, C. F. Feng20, Zhaoyang Feng9, Zhenyong Feng21, F. Galeazzi4, P. Galeotti11, R. Gargana4, Q. B. Gou9, Y. Q. Guo9, H. H. He9, Haibing Hu18, Hongbo Hu9, Q. Huang21, M. Iacovacci5, R. Iuppa1, I. James3, H. Y. Jia21, Labaciren18, H. J. Li18, J. Y. Li20, X. X. Li9, B. Liberti2, G. Liguori13, C. Liu9, C. Q. Liu15, M. Y. Liu14, J. Liu15, H. Lu9, X. H. Ma9, G. Mancarella7, MARI, Stefano Maria, 3, 4, G. Marsella8, D. Martello7, S. Mastroianni6, X. R. Meng18, P. Montini3, C. C. Ning18, A. Pagliaro24, M. Panareo8, L. Perrone8, P. Pistilli3, 4.X. B. Qu20, E. Rossi5, F. Ruggieri4, L. Saggese5, P. Salvini13, R. Santonico1, P. R. Shen9, X. D. Sheng9, F. Shi9, C. Stanescu4, A. Surdo8, Y. H. Tan9, P. Vallania11, S. Vernetto11, C. Vigorito11, B. Wang9, H. Wang9, C. Y. Wu9, H. R. Wu9, B. Xu21, L. Xue20, Y. X. Yan14, Q. Y. Yang15, X. C. Yang15, A. F. Yuan18, M. Zha9, H. M. Zhang9, Jilong Zhang9, Jianli Zhang9, L. Zhang15, P. Zhang15, X. Y. Zhang20, Y. Zhang9, Zhaxisangzhu18, X. X. Zhou21, F. R. Zhu9, Q. Q. Zhu9, G. Zizzi7
The ARGO-YBJ experiment at YangBaJing in Tibet (4300 m a.s.l.) has been taking data with its full layout since October 2007. Here we present the first significant results obtained in gamma-ray astronomy and cosmic-ray physics. Emphasis is placed on t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1c710d066fe02b009594a8bdaec96ce8
https://hdl.handle.net/11590/122475
https://hdl.handle.net/11590/122475
Autor:
THE ARGO YBJ C.O.L.L.A.B.O.R.A.T.I.O.N.G. Aielli1, 2, C. Bacci3, 4, B. Bartoli5, 6, P. Bernardini7, 8, X. J. Bi9, C. Bleve7, P. Branchini4, A. Budano4, BUSSINO, Severino Angelo Maria, A. K. Calabrese Melcarne10, P. Camarri1, Z. Cao9, A. Cappa11, R. Cardarelli2, S. Catalanotti5, C. Cattaneo13, P. Celio3, S. Z. Chen9, Y. Chen9, N. Cheng9, P. Creti8, S. W. Cui14, B. Z. Dai15, G. D’Al´ı Staiti16, 17, Danzengluobu18, M. Dattoli11, 12, 19, DE VINCENZI, Mario, B. D’Ettorre Piazzoli5, M. De Vincenzi3, T. Di Girolamo5, X. H. Ding18, G. Di Sciascio2, C. F. Feng20, Zhaoyang Feng9, Zhenyong Feng21, F. Galeazzi4, P. Galeotti11, R. Gargana4, Q. B. Gou9, Y. Q. Guo9, H. H. He9, Haibing Hu18, Hongbo Hu9, Q. Huang21, M. Iacovacci5, R. Iuppa1, I. James3, H. Y. Jia21, Labaciren18, H. J. Li18, J. Y. Li20, X. X. Li9, B. Liberti2, G. Liguori13, C. Liu9, C. Q. Liu15, M. Y. Liu14, J. Liu15, H. Lu9, X. H. Ma9, G. Mancarella7, 3, 4, G. Marsella8, D. Martello7, S. Mastroianni6, X. R. Meng18, P. Montini3, C. C. Ning18, A. Pagliaro24, M. Panareo8, L. Perrone8, P. Pistilli3, 4.X. B. Qu20, E. Rossi5, F. Ruggieri4, L. Saggese5, P. Salvini13, R. Santonico1, P. R. Shen9, X. D. Sheng9, F. Shi9, C. Stanescu4, A. Surdo8, Y. H. Tan9, P. Vallania11, S. Vernetto11, C. Vigorito11, B. Wang9, H. Wang9, C. Y. Wu9, H. R. Wu9, B. Xu21, L. Xue20, Y. X. Yan14, Q. Y. Yang15, X. C. Yang15, A. F. Yuan18, M. Zha9, H. M. Zhang9, Jilong Zhang9, Jianli Zhang9, L. Zhang15, P. Zhang15, X. Y. Zhang20, Y. Zhang9, Zhaxisangzhu18, X. X. Zhou21, F. R. Zhu9, Q. Q. Zhu9, G. Zizzi7, MARI, Stefano Maria
The ARGO-YBJ experiment, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300 m a.s.l., is a detector 100x110m2 large, made by a layer of Resistive Plate Counters (RPCs) consisting of a central carpet with almost full coverage ex
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3668::c8dd90a56c46bbdba26f2a4d5250f0cb
https://hdl.handle.net/11590/122986
https://hdl.handle.net/11590/122986
Autor:
THE ARGO YBJ COLLABORATION G. Aielli1, 2, C. Bacci3, 4, B. Bartoli5, 6, P. Bernardini7, 8, X. J. Bi9, C. Bleve7, P. Branchini4, A. Budano4, BUSSINO, Severino Angelo Maria, A. K. Calabrese Melcarne10, P. Camarri1, Z. Cao9, A. Cappa11, R. Cardarelli2, S. Catalanotti5, C. Cattaneo13, P. Celio3, S. Z. Chen9, Y. Chen9, N. Cheng9, P. Creti8, S. W. Cui14, B. Z. Dai15, G. D’Al´ı Staiti16, 17, Danzengluobu18, M. Dattoli11, 12, 19, DE VINCENZI, Mario, B. D’Ettorre Piazzoli5, M. De Vincenzi3, T. Di Girolamo5, X. H. Ding18, G. Di Sciascio2, C. F. Feng20, Zhaoyang Feng9, Zhenyong Feng21, F. Galeazzi4, P. Galeotti11, R. Gargana4, Q. B. Gou9, Y. Q. Guo9, H. H. He9, Haibing Hu18, Hongbo Hu9, Q. Huang21, M. Iacovacci5, R. Iuppa1, I. James3, H. Y. Jia21, Labaciren18, H. J. Li18, J. Y. Li20, X. X. Li9, B. Liberti2, G. Liguori13, C. Liu9, C. Q. Liu15, M. Y. Liu14, J. Liu15, H. Lu9, X. H. Ma9, G. Mancarella7, 3, 4, G. Marsella8, D. Martello7, S. Mastroianni6, X. R. Meng18, P. Montini3, C. C. Ning18, A. Pagliaro24, M. Panareo8, L. Perrone8, P. Pistilli3, 4 X. B. Qu20, E. Rossi5, F. Ruggieri4, L. Saggese5, P. Salvini13, R. Santonico1, P. R. Shen9, X. D. Sheng9, F. Shi9, C. Stanescu4, A. Surdo8, Y. H. Tan9, P. Vallania11, S. Vernetto11, C. Vigorito11, B. Wang9, H. Wang9, C. Y. Wu9, H. R. Wu9, B. Xu21, L. Xue20, Y. X. Yan14, Q. Y. Yang15, X. C. Yang15, A. F. Yuan18, M. Zha9, H. M. Zhang9, Jilong Zhang9, Jianli Zhang9, L. Zhang15, P. Zhang15, X. Y. Zhang20, Y. Zhang9, Zhaxisangzhu18, X. X. Zhou21, F. R. Zhu9, Q. Q. Zhu9, G. Zizzi7, MARI, Stefano Maria
Very High Energy (VHE) g -astronomy and cosmic ray physics are the main goals of the ARGOYBJ experiment. The detector is located in Tibet (People's Republic of China) and is a full coverage Extensive Air Shower array consisting of a carpet of Resisti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3668::63a10c2aeeb984f97ec66c6d648a132a
https://hdl.handle.net/11590/119455
https://hdl.handle.net/11590/119455