Università degli Studi di Roma 3 ArcA diA
Archivio Aperto di Ateneo

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

Please use this identifier to cite or link to this item: http://hdl.handle.net/2307/368

Title: ARGO-YBJ constraints on very high energy emission from GRBs
Authors: Aielli, G.
Bacci, Cesare
Bartoli, B.
Bernardini, P.
Bi, X. J.
Bleve, C.
Branchini, Paolo
Budano, Antonio
Bussino, Severino
Calabrese Melcarne, A. K.
Camarri, P.
Zhang, JianLi
Zhang, L.
Zhang, P.
Zhang, X. Y.
Zhang, Y.
Zhou, X. X.
Zhu, F. R.
Zhu, Q. Q.
Zizzi, G.
Cao, Z.
Cappa, A.
Cardarelli, R.
Catalanotti, S.
Cattaneo, C.
Celio, Paola
Chen, S. Z.
Chen, Y.
Cheng, N.
Creti, P.
Cui, S. W.
Dai, B. Z.
D'Ali Staiti, G.
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
Galeazzi, Fulvio
Galeotti, P.
Gargana, Riccardo
Gou, Q. B.
Guo, Y. Q.
He, H. H.
Hu, Haibing
Hu, Hongbo
Huang, Q.
Iacovacci, M.
Iuppa, R.
James, Irina
Jia, H. Y.
Li, H. J.
Li, J. Y.
Li, X. X.
Liberti, B.
Liguori, G.
Liu, C.
Liu, C. Q.
Liu, M. Y.
Liu, J.
Lu, H.
Ma, X. H.
Mancarella, G.
Mari, Stefano Maria
Marsella, G.
Martello, D.
Mastroianni, S.
Meng, X. R.
Montini, Paolo
Ning, C. C.
Pagliaro, A.
Panareo, M.
Perrone, L.
Pistilli, Pio
Qu, X. B.
Rossi, E.
Ruggieri, Federico
Saggese, L.
Salvini, P.
Santonico, R.
Shen, P. R.
Sheng, X. D.
Shi, F.
Stanescu, Cristian
Surdo, A.
Tan, Y. H.
Vallania, P.
Vernetto, S.
Vigorito, C.
Wang, B.
Wang, H.
Wu, C. Y.
Wu, H. R.
Xu, B.
Xue, L.
Yan, Y. X.
Yang, Q. Y.
Yang, X. C.
Yuan, A. F.
Zha, M.
Zhang, H. M.
Zhang, JiLong
Issue Date: Aug-2009
Publisher: Elsevier
Abstract: The ARGO-YBJ (Astrophysical Radiation Ground-based Observatory at YangBajing) experiment is designed for very high energy gamma-astronomy and cosmic ray researches. Due to the full coverage of a large area(5600 m(2)) with resistive plate chambers at a very high altitude (4300m a.s.l.), the ARGO-YBJ detector is used to search for transient phenomena, such as Gamma-ray bursts (GRBs). Because the ARGO-YBJ detector has a large field of view (similar to 2 sr) and is operated with a high duty cycle (>
URI: http://hdl.handle.net/2307/368
ISSN: 0927-6505
DOI: 10.1016/j.astropartphys.2009.05.005
URL: http://arxiv.org/abs/0903.0119
Appears in Collections:A - Articolo su rivista
X_Dipartimento di Fisica 'Edoardo Amaldi'

Files in This Item:

File Description SizeFormat
Argo_2009_4.pdfsolo archivio329.39 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