3-11 July 2007
Merida, Mexico
Mexico/General timezone
- icrc2007@icrc2007.unam.mx
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Contribution Oral
Merida, Mexico
-
Yucatan II+III+IV (Fiesta Americana)
HE.1.2.A
Preliminary results of the Moon shadow using the ARGO-YBJ experiment
Speakers
- Dr. Bo WANG
Primary authors
- Dr. Bo WANG (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China)
Co-authors
- Silvia VERNETTO (IFSI-Istituto Nazionale di Astrofisica and INFN, Torino, Italy)
- Tianlu CHEN (Department of Mathematics and Physics, Tibet University, Lhasa 85000, China.)
- Jianli ZHANG (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China)
- Jun LIU (Department of Physics, Yunnan University, Kunming 650091, China)
- Yi ZHANG (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China)
- Yiqing GUO (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China)
- Hongbo HU (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China)
- Huihai HE (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China)
- A.K. CALABRESE MELCARNE (Dipartimento di Fisica dell’Universita di Lecce, Italy)
- Songzhan CHEN (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China)
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Abstract content
ARGO-YBJ is a "full coverage" air shower detector consisting of a carpet of Resistive Plate Chambers, located at Yangbajing (4300m a.s.l.). Using the data collected by the central detector (5800m^2 area) the cosmic ray shadowing effect due to the Moon is studied. The comparison of experimental results with Montecarlo simulations is also discussed.
If this papers is presented for a collaboration, please specify the collaboration
for the ARGO-YBJ collaboration
Reference
Proceedings of the 30th International Cosmic Ray Conference; Rogelio Caballero, Juan Carlos D'Olivo, Gustavo Medina-Tanco, Lukas Nellen, Federico A. Sánchez, José F. Valdés-Galicia (eds.); Universidad Nacional Autónoma de México, Mexico City, Mexico, 2008; Vol. 4 (HE part 1), pages 107-110