The Status of the ARGO Experiment at YBJ
- G. Aiellia
- C. Baccib
- B. Bartolic
- P. Bernardinid
- X. J. Bie
- C. Bleved
- S. Bussinob
- A. K. Calabrese Melcarned
- P. Camarria
- D. Campanac
- Z. Caoe
- R. Cardarellia
- S. Catalanottic S. Cavalierec
- P. Celiob
- S. Z. Chene
- N. Chenge
- P. Cretid
- S. W. Cuif
- G. Cusumanog
- B. Z. Daih
- Danzengluobui
- X. H. Dingi
- G. D’Ali Staitij
- B. D’Ettorre Piazzolic
- E. De Marinisb
- I. De Mitrid
- M. De Vincenzib
- T. Di Girolamoc
- G. Di Sciascioc
- C. F. Fengk
- Zhaoyang Fenge
- Zhenyong Fengl
- C. Ferrignoj
- X. Y. Gaoh
- Q. B. Goue
- H. H. Hee ∗
- Hongbo Hue
- Haibing Hui
- Q. Huangl
- M. Iacovaccic
- I. Jamesm
- H. Y. Jial
- Labacireni
- J. Y. Lik
- H. J. Lii
- B. Libertia
- G. Liguorim
- C. Q. Liuh
- J. Liuh
- H. Lue
- G. Mancarellad
- b
- G. Marsellad
- D. Martellod
- S. Mastroiannic
- X. R. Mengi
- J. Muh
- L. Nicastrog
- C. C. Ningi
- L. Palummoa
- M. Panareod
- L. Perroned
- P. Pistillib
- X. B. Quk
- E. Realia
- E. Rossic
- B. Saccoj
- L. Saggesec
- P. Salvinim
- A. Segretog
- R. Santonicoa
- P. R. Shene
- X. D. Shenge
- F. Shie
- C. Stanescub
- A. Surdod
- Y. H. Tane
- P. Vallanian
- S. Vernetton
- H. Wange
- Y. G. Wange
- C. Y. Wue
- B. Xul
- L. Xuek
- H. T. Yangh
- Q. Y. Yangh
- X. C. Yangh
- G. C. Yul
- A. F. Yuani
- M. Zhae
- H. M. Zhange
- L. Zhangh
- P. Zhangh
- X. Y. Zhangk
- Y. Zhange
- Zhaxisangzhui
- X. X. Zhoul
- F. R. Zhue
- Q. Q. Zhue
- MARI, Stefano Maria
DOIAbstract
The ARGO-YBJ experiment, located at Yangbajing, Tibet, China, performed by a wide Sino-Italian collaboration, is designed to study cosmic rays, sub-TeV gamma ray sources and GeV Gamma Ray Burst (GRB) emission in the northern hemisphere, by means of detecting small size EAS (Extensive Air Shower) using a full coverage RPC (Resistive Plate Chamber) carpet. The central carpet of the detector is installed and put into operation to date, with 1900m2 of the carpet already operating since December 2004. With a trigger multiplicity of ≥60 hits, corresponding to a primary mode energy of 2 TeV, the angular resolution of EAS measurements is < 1o for showers with more than 500 recorded hits. We report the preliminary results of data taking perfo...
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