First measurements with the ARGO-YBJ detector

Autor: Bernardini P, Bleve C, Creti P, De Mitri I, DeVincenzi M, Mancarella G, Marsella G, Martello D, Panareo M, Pino C, Surdo A, Barone F, Bartoli B, Catalanotti S, Cavaliere S, D’Ettorre Piazzoli B, Di Girolamo T, Di Sciascio G, Iacovacci M, Mastroianni S, Milano L, Rossi E, Saggese L, Cusumano G, D’Ali’ Staiti G, Nicastro L, Sacco B, Liguori G, Salvini P, Aielli G, Camarri P, Cardarelli R, Cavaliere A, D’Elia V, Liberti B, Santonico R, Bacci C, Celio P, Cesaroni F, De Marinis E, Fratini K, MARI, Stefano Maria, Pieri L, Pistilli P, Stanescu C, Storini M, Vallania P, Vernetto S, Gou QB, He HH, Hu HB, Jing CL, Kuang HH, Lu H, Shen PR, Sheng XD, Tan YH, Wang H, Wang HY, Wu CY, Zhang HM, Zhang JL, Zhang Y, Zhu QQ, Feng CF, He M, Li JY, Wang YG, Xue L, Zhang NJ, Zhang XY, Feng ZY, Huang Q, Jia HY, Yu GC, Zhou XX, Danzengluobu, Ding XH, Guo HW, Hu Haibing, Labaciren, Meng XR, Ning CC, Yuan AF, Zhaxisangzhu, Gao XY, Geng QX, Liu CQ, Liu J, Mu J, Yangv HT, Yang QY, Yang XC, Zhang L, Zhang P, Bao KZ, Sun LR, Sun SC, Yue XD, Yao QK, Ma YM, Cheng KS, BUSSINO, Severino Angelo Maria

The detection of small size air showers at high altitude allows the search for γ-ray point sources at few hundreds GeV energy threshold. The ARGO-YBJ experiment, currently under construction at the Yangbajing Cosmic Ray Laboratory (4300 m a.s.l.), h

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______3668::4cfdd9150895d88fb5eb4b05d52a5f88
https://hdl.handle.net/11590/176997

BES upgrade

Autor: Bai, JZ, Bao, HC, Blum, I, Chai, ZW, Chen, GP, Chen, HF, Chen, J, Chen, JC, Chen, Y, Chen, YB, Chen, YQ, Cheng, BS, Chu, XM, Cui, XZ, Ding, HL, Ding, WY, Dong, LY, Du, YY, Du, ZZ, Dunwoodie, W, Fang, J, Fang, WZ, Gao, CS, Gao, ML, Gao, SQ, Gratton, P, Gu, JH, Gu, SD, Gu, WX, Guo, YN, Han, HG, Han, SW, Harris, FA, Han, Y, He, J, He, M, Heng, YK, Hitlin, DG, Hu, GY, Hu, HB, Hu, HM, Hu, JL, Hu, QH, Hu, T, Hu, XQ, Huang, GS, Huang, JD, Huang, YZ, Izen, JM, Jiang, CH, Jiang, YY, Jin, Y, Jones, BD, Ju, X, Ke, ZJ, Kelsey, MH, Kim, BK, Kong, D, Lai, YF, Lang, PF, Lankford, A, Li, CG, Li, F, Li, HB, Li, J, Li, PQ, Li, Q, Li, RB, Li, W, Li, WD, Li, WG, Li, WH, Li, XH, Li, XN, Liu, HM, Liu, J, Liu, JH, Liu, Q, Liu, QJ, Liu, RG, Liu, Y, Liu, ZX, Lou, JS, Lou, XC, Lowery, B, Lu, HY, Lu, JG, Luo, H, Luo, SQ, Luo, XL, Ma, EC, Ma, JM, Malchow, R, Mandelkern, M, Mao, HS, Mao, ZP, Meng, XC, Mo, XH

Publikováno v: Bai, JZ; Bao, HC; Blum, I; Chai, ZW; Chen, GP; Chen, HF; et al.(2001). BES upgrade. Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 458(3), 627-637. doi: 10.1016/S0168-9002(00)00934-7. UC Irvine: Retrieved from: http://www.escholarship.org/uc/item/0gc8d1bv

The Beijing Spectrometer (BES) detector is a general purpose solenoid detector at the Beijing Electron Positron Collider in Beijing, China. The recent upgrade of the initial BES detector to the improved BES II detector is described. A new drift chamb

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od_______325::6120e0e5b2f6675cf28cdbfc2c58e5fa
http://www.escholarship.org/uc/item/0gc8d1bv

Cosmic ray shower rate variations detected by the ARGO-YBJ experiment during thunderstorms

Autor: Axikegu, null, Bartoli, B., Bernardini, P., Bi, X. J., Cao, Z., Catalanotti, S., Chen, S. Z., Chen, T. L., Cui, S. W., Dai, B. Z., D’Amone, A., Danzengluobu, null, De Mitri, I., D’Ettorre Piazzoli, B. D., Di Girolamo, T., Di Sciascio, G., Feng, C. F., Feng, Zhenyong, Gao, W., Gou, Q. B., Guo, Y. Q., He, H. H., Hu, Haibing, Hu, Hongbo, Iacovacci, M., Iuppa, R., Jia, H. Y., Labaciren, null, Li, H. J., Liu, C., Liu, J., Liu, M. Y., Lu, H., Ma, L. L., Ma, X. H., Mancarella, G., Mari, S. M., Marsella, G., Mastroianni, S., Montini, P., Ning, C. C., Perrone, L., Pistilli, P., Salvini, P., Santonico, R., Shen, P. R., Sheng, X. D., Shi, F., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, C., Wang, H., Wu, C. Y., Wu, H. R., Xue, L., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M., Zhang, H. M., Zhang, L., Zhang, X. Y., Zhang, Y., Zhao, J., Zhaxiciren, null, Zhaxisangzhu, null, Zhou, X. X., Zhu, F. R., Zhu, Q. Q.

The ARGO-YBJ detector, located at the Yangbajing Cosmic Ray Laboratory (4300 m a. s. l., Tibet, China), was a "full coverage" air shower array. The high altitude location and the frequent occurrence of thunderstorms, made ARGO-YBJ suitable to study t

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::431a1a80a83afb68bf4a72493c479d5f
https://hdl.handle.net/11587/481724

Mean Interplanetary Magnetic Field Measurement Using the ARGO-YBJ Experiment

Autor: X. X. Li, Zhenyong Feng, L. Zhang, B. D'Ettorre Piazzoli, L. Xue, G. Mancarella, Q. B. Gou, A. Cappa, M. Zha, F. R. Zhu, M. Panareo, B. Z. Dai, M. Iacovacci, Piero Vallania, P. Creti, Danzengluobu, F. Ruggieri, A. K. Calabrese Melcarne, L. Perrone, P. Salvini, R. Cardarelli, G. Marsella, Q. Q. Zhu, Y. Q. Guo, P. Branchini, H. Y. Jia, G. Aielli, R. Santonico, H. H. He, C. Bacci, S. M. Mari, Zhengguo Cao, X. C. Yang, B. S. Wang, A. Pagliaro, Q. Y. Yang, Bingwei Xu, P. F. Zhang, E. Giroletti, Severino Angelo Maria Bussino, S. W. Cui, Hongbo Hu, A. Surdo, C. F. Feng, X. J. Bi, H. R. Wu, I. De Mitri, X. R. Meng, C. Stanescu, Irina James, A. F. Yuan, Chang-Chun Ning, Zhaoyang Feng, J. Y. Li, Jilong Zhang, T. Di Girolamo, F. Shi, Jianli Zhang, T. L. Chen, H. M. Zhang, G. Di Sciascio, Carlo Vigorito, P. Celio, C. Y. Wu, M. Y. Liu, M. De Vincenzi, Haibing Hu, R. Gargana, I. Bolognino, B. Bartoli, H. J. Li, X. D. Sheng, C. Bleve, Y. B. Chen, S. Z. Chen, L. Saggese, Y. Zhang, B. Liberti, Paolo Bernardini, D. Martello, X. B. Qu, X. H. Ding, Labaciren, J. K. K. Liu, P. Pistilli, X. X. Zhou, G. D'Alí Staiti, Y. H. Tan, P. Galeotti, Q. Huang, X. Y. Zhang, C. Liu, X. H. Ma, G. Liguori, C. X. Liu, Zhaxisangzhu, S. Catalanotti, Z. G. Yao, Y. X. Yan, E. Rossi, M. Dattoli, H. Lu, Paolo Montini, R. Iuppa, and G. Zizzi, P. Camarri, H. W. Wang, S. Vernetto, F. Galeazzi, A. Budano, S. Mastroianni, C. Cattaneo, P. R. Shen

The sun blocks cosmic ray particles from outside the solar system, forming a detectable shadow in the sky map of cosmic rays detected by the ARGO-YBJ experiment in Tibet. Because the cosmic ray particles are positive charged, the magnetic field betwe

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::368510a83f66a7cfa2674b4f9218b7a0

Gamma-Ray Flares from Mrk421 in 2008 observed with the ARGO-YBJ detector

Autor: Aielli, G., Bacci, C., Bartoli, B., Bernardini, P., Xj, B., Bleve, C., Branchini, P., Budano, A., Bussino, S., Calabrese Melcarne, A., Camarri, P., Cao, Z., Cappa, A., Cardarelli, R., Catalanotti, S., Cattaneo, C., Celio, P., Chen, S., Chen, Y., Cheng, N., Creti, P., Cui, S., Dai, B., D'Ali'Staiti, G., Danzengluobu, Dattoli, M., De Mitri, I., D’Ettorre Piazzoli, B., De Vincenzi, M., Di Girolamo, T., Ding, X., Di Sciascio, G., Feng, C., Feng, Z., Galeazzi, F., Galeotti, P., Gargana, R., Gou, Q., Guo, Y., Hh, H., Hbi, H., Hbo, H., Huang, Q., Iacovacci, M., Iuppa, R., James, I., Jia, H., Labaciren, Hj, L., Jy, L., Xx, L., Liberti, B., Liguori, G., Liu, C., Liu, J., Liu, M., Lu, H., Xh, M., Mancarella, G., Mari, S., Marsella, G., Martello, D., Mastroianni, S., Meng, X., Montini, P., Ning, C., Pagliaro, A., Panareo, M., Perrone, L., Pistilli, P., Xb, Q., Rossi, E., Ruggieri, F., Saggese, L., Salvini, P., Santonico, R., Shen, P., Sheng, X., Shi, F., Stanescu, C., Surdo, A., Tan, Y., Vallania, P., Vernetto, S., Vigorito, C., Wang, B., Wang, H., Cy, W., Hr, W., Xu, B., Xue, L., Yan, Y., Yang, Q., Yang, X., Yuan, A., Zha, M., Zhang, H., Zhang, J., Zhang, L., Zhang, P., Zhang, X., Zhang, Y., Zhaxisangzhu, Zhou, X., Zhu, F., Zhu, Q., Zizzi, G.

In 2008 the blazar Markarian 421 entered a very active phase and was one of the brightest sources in the sky at TeV energies, showing frequent flaring episodes. Using the data of ARGO-YBJ, a full coverage air shower detector located at Yangbajing (43

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b803fb8ebacf4ec34fa85dcb43287df8
http://hdl.handle.net/2108/37348