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Monte Carlo simulations for the Cherenkov Telescope Array Observatory using PL-Grid e-infrastructure

Treść / Zawartość
Identyfikatory
Warianty tytułu
Języki publikacji
EN
Abstrakty
EN
The paper presents Monte Carlo simulations carried out during the preparatory phase of the Cherenkov Telescope Array project. The aim of the project is to build the next generation observatory of very high energy gamma rays. During the preparatory phase there is a need to optimize and verify design concepts for various elements of the array. In this paper we describe the main components of the software being used for that purpose, their functions and requirements. Preliminary results of the optimization of the small telescope – one of the several kinds intended for the array, are presented.
Wydawca
Czasopismo
Rocznik
Strony
113--122
Opis fizyczny
Bibliogr. 10 poz., rys., wykr.
Twórcy
autor
  • Nicolaus Copernicus Astronomical Center, Warsaw, Poland
  • DSM/IRFU/SPP, CEA/Saclay, Gif-sur-Yvette, France
autor
  • Department of Information Technologies, Faculty of Physics, Astronomy and Applied Computer Science, Jagellonian University, Warsaw, Poland
  • Astronomical Observatory, Warsaw, Poland
autor
  • Nicolaus Copernicus Astronomical Center, Warsaw, Poland
autor
  • LAPP, Universitas de Savoie et IN2P3/CNRS, Annecy, France
autor
  • LAPP, Universitas de Savoie et IN2P3/CNRS, Annecy, France
autor
  • Nicolaus Copernicus Astronomical Center, Warsaw, Poland
Bibliografia
  • [1] Vasileiadis, G.: The H.E.S.S experimental project. [in:] Proceedings of the Fifth International Workshop on Ring Imaging Detectors, Nucl. Instr. and Methods in Phys. Research A, 553 (2005) 268–273
  • [2] Ferenc, D. and MAGIC Collaboration: The MAGIC gamma-ray observatory. Nucl. Instr. and Methods in Phys. Research A, 553 (2005) 274–281
  • [3] LeBohec, S. et al. Deployment of the VERITAS observatory. J. Phys.: Conf. Ser. 47 (2006) 232–237
  • [4] Glicenstein, J.-F. for the CTA Consortium: The Cherenkov telescope array, an advanced facility for ground based gamma-ray astronomy. [in:] Proceedings of the Seventh International Workshop on Ring Imaging Cherenkov Detectors, Nucl. Instr. and Methods in Phys. Research A, 639 (2011) 46–49
  • [5] Ghiselli, A., and Mazzucato, M.: Grid: From EGEE to EGI and from INFN-GRID to IGI. Il Nuovo Cimento C 32 (2009) 233–241
  • [6] Barnacka, A. et al.: PL-Grid e-Infrastructure for the Cherenkov Telescope Array Observatory. [in:] Bubak, M., Szepieniec, T., and Wiatr, K., eds, Building a National Distributed e-Infrastructure – PL-Grid, Lecture Notes [in:] Computer Science vol. 7136, Springer 2012
  • [7] Capdevielee, J. N. et al.: Extensive air shower simulations with the CORSIKA program. [in:] L. Jones, ed., Very High Energy Cosmic-Ray Interactions, AIP Conference Series, 276 (1993) 545–553
  • [8] Heck, D., & The KASCADE Collaboration: Hadronic Interaction Models and the Air Shower Simulation Program CORSIKA. [in:] Proceedings of the 27th International Cosmic Ray Conference, International Cosmic Ray Conference, 1 (2001) 233
  • [9] Actis, M. et al.: Design Concepts for the Cherenkov Telescope Array: an advanced facility for ground-based high-energy gamma-ray astronomy. Experimantal Astronomy, 32 (2010) 193–316
  • [10] Bernloehr, K.: CTA simulations with CORSIKA/sim telarray, [in:] F. A. Aharonian, W. Hofmann, & F. Rieger, eds, HIGH ENERGY GAMMA-RAY ASTRONOMY: Proceedings of the 4th International Meeting on High Energy Gamma- Ray Astronomy. AIP Conference Series, 1085 (2008) 874–877
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-article-AGH1-0028-0207
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