Università degli Studi di Roma 3 ArcA diA
Archivio Aperto di Ateneo
DSpace@Roma3

ArcAdiA >
Tipologia di Documenti >
A - Articolo su rivista >

Please use this identifier to cite or link to this item: http://hdl.handle.net/2307/365

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 d
...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'

Files in This Item:

File Description SizeFormat
Argo_2009_2.pdfsolo archivio542.51 kBAdobe PDF
Restrict Access. You can Request a copy!


This item is protected by original copyright

Recommend this item

SFX Query

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.

 

Università degli Studi RomaTre SBA - Sistema Bibliotecario di Ateneo ICT support by CINECA