Details

Autor(en) / Beteiligte

• Aielli, G.
• Bacci, C.
• Bartoli, B.
• Bernardini, P.
• Bi, X.J.
• Bleve, C.
• Branchini, P.
• Budano, A.
• Bussino, S.
• Calabrese Melcarne, A.K.
• Camarri, P.
• Cao, Z.
• Cappa, A.
• Cardarelli, R.
• Cattaneo, C.
• Cavaliere, S.
• Celio, P.
• Chen, S.Z.
• Cheng, N.
• Creti, P.
• Cui, S.W.
• Dai, B.Z.
• D’Alí Staiti, G.
• Danzengluobu
• Dattoli, M.
• D’Ettorre Piazzoli, B.
• De Vincenzi, M.
• Di Girolamo, T.
• Ding, X.H.
• Di Sciascio, G.
• Feng, C.F.
• Feng, Zhaoyang
• Feng, Zhenyong
• Ferrigno, C.
• Galeazzi, F.
• Galeotti, P.
• Gao, X.Y.
• Gargana, R.
• Gou, Q.B.
• He, H.H.
• Hu, Haibing
• Hu, Hongbo
• Huang, Q.
• Jia, H.Y.
• Labaciren
• Li, H.J.
• Li, J.Y.
• Liberti, B.
• Liguori, G.
• Liu, C.Q.
• Liu, J.
• Lu, H.
• Mancarella, G.
• Mari, S.M.
• Marsella, G.
• Martello, D.
• Mastroianni, S.
• Meng, X.R.
• Mu, J.
• Ning, C.C.
• Palummo, L.
• Panareo, M.
• Perrone, L.
• Pistilli, P.
• Qu, X.B.
• Rossi, E.
• Ruggieri, F.
• Saggese, L.
• Salvini, P.
• Santonico, R.
• Segreto, A.
• Sheng, X.D.
• Shi, F.
• Stanescu, C.
• 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, P.
• Zhang, X.Y.
• Zhang, Y.
• Zhaxisangzhu
• Zhou, X.X.
• Zhu, F.R.
• Zhu, Q.Q.
• Zizzi, G.

Titel

Software timing calibration of the ARGO-YBJ detector

Ist Teil von

• Astroparticle physics, 2009, Vol.30 (6), p.287-292

Ort / Verlag

Elsevier B.V

Erscheinungsjahr

2009

Quelle

Alma/SFX Local Collection

Beschreibungen/Notizen

• 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.