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Please use this identifier to cite or link to this item:
http://hdl.handle.net/2307/365
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| Title: | Software timing calibration of the ARGO-YBJ detector |
| Authors: | Aielli, G.
Bacci, Cesare
Bartoli, B.
Bernardini, P.
Bi, X. J.
Bleve, C.
Branchini, P.
Budano, A.
Bussino, Severino
Calabrese Melcarne, A. K.
Camarri, P.
Cao, Z.
Cappa, A.
Cardarelli, R.
Catalanotti, S.
Cattaneo, C.
Cavaliere, S.
Celio, Paola
Chen, S. Z.
Cheng, N.
Creti, P.
Cui, S. W.
Cusumano, G.
Dai, B. Z.
D'Ali Staiti, G.
Danzengluobu
Dattoli, M.
De Mitri, I.
D'Ettorre Piazzoli, B.
De Vincenzi, Mario
Di Girolamo, T.
Ding, X. H.
Di Sciascio, G.
Feng, C. F.
Feng, Zhaoyang
Feng, Zhenyong
Ferrigno, C.
Galeazzi, Fulvio
Galeotti, P.
Gao, X. Y.
Gargana, Riccardo
Gou, Q. B.
He, H. H.
Hu, Haibing
Hu, Hongbo
Huang, Q.
Iacovacci, M.
James, I.
Jia, H. Y.
Labaciren
Li, H. J.
Li, J. Y.
Liberti, B.
Liguori, G.
Liu, C. Q.
Liu, J.
Lu, H.
Mancarella, G.
Mari, Stefano Maria
Marsella, G.
Martello, D.
Mastroianni, Stefano
Meng, X. R.
Mu, J.
Nicastro, L.
Ning, C. C.
Palummo, L.
Panareo, M.
Perrone, L.
Pino, C.
Pistilli, Pio
Qu, X. B.
Rossi, E.
Ruggieri, Federico
Saggese, L.
Salvini, P.
Santonico, R.
Segreto, A.
Shen, P. R.
Sheng, X. D.
Shi, F.
Stanescu, Cristian
Surdo, A.
Tan, Y. H.
Vallania, P.
Vernetto, S.
Vigorito, C.
Wang, H.
Wang, Y. G.
Wu, C. Y.
Wu, H. R.
Xu, B.
Xue, L.
Yang, H. T.
Yang, Q. Y.
Yang, X. C.
Yu, G. C.
Yuan, A. F.
Zha, M.
Zhang, H. M.
Zhang, J. L.
Zhang, L.
Zhang, P.
Zhang, X. Y.
Zhang, Y.
Zhaxisangzhu
Zhou, X. X.
Zhu, F. R.
Zhu, Q. Q.
Zizzi, G. |
| Keywords: | Gamma astronomy
Extensive air showers
Timing calibration
Cosmic rays
Astroparticle physics |
| Issue Date: | Jan-2009 |
| Publisher: | Elsevier |
| Abstract: | The ARGO-YBJ experiment is mainly devoted to search for astronomical gamma sources. The arrival direction of air showers is reconstructed thanks to the times measured by the pixels of the detector. Therefore, the timing calibration of the detector pixels is crucial in order to get the best angular resolution and pointing accuracy. Because of the large number of pixels a hardware timing calibration is practically impossible. Therefore an off-line software calibration has been adopted. Here, the details of the procedure and the results are presented.
...more |
| URI: | http://hdl.handle.net/2307/365 |
| ISSN: | 0927-6505 |
| DOI: | 10.1016/j.astropartphys.2008.09.010 |
| Appears in Collections: | A - Articolo su rivista
Dipartimento di Fisica 'Edoardo Amaldi'
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| Argo_2009_2.pdf | solo archivio | 542.51 kB | Adobe PDF | |  |
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