Absolute-energy-scale calibration of ARGO-YBJ for light primaries in multi-TeV region with the Moon shadow observation

• Published in: Astroparticle physics Vol. 90; pp. 20 - 27
• Main Authors: 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, De Mitri, I., D’Ettorre Piazzoli, B., Di Girolamo, T., Di Sciascio, G., Feng, C.F., Feng, Zhaoyang, Feng, Zhenyong, Gou, Q.B., Guo, Y.Q., He, H.H., Hu, Haibing, Hu, Hongbo, Iacovacci, M., Iuppa, R., Jia, H.Y., Labaciren, 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, Zhaxisangzhu, Zhou, X.X., Zhu, F.R., Zhu, Q.Q., collaboration), (The ARGO-YBJ
• Format: Journal Article
• Language: English
• Published: Elsevier B.V 01-04-2017
• Subjects: Cosmic ray; Energy calibration; Energy spectrum; Moon shadow; Energy spectrum; Cosmic ray; Moon shadow; Energy calibration
• ISSN: 0927-6505; 1873-2852
• DOI: 10.1016/j.astropartphys.2017.02.004

In 2011 ARGO-YBJ experiment has reported a work to study the absolute rigidity scale of the primary cosmic ray particles based on the Moon’s shadow observation. Given the progress in high energy hadronic interaction models with LHC data, in cosmic ray chemical composition measurement and in experimental data accumulation, more updates can be researched. This paper aims to further disentangle the composition dependence in absolute-energy-scale calibration by using specific moon-shadow data which mainly is comprised of light component cosmic rays. Results show that, 17% energy scale error is estimated from 3 TeV to 50 TeV. To validate the performance of this technique, the light component cosmic ray spectrum in the same energy region is shown.