Publication: Advanced functionality for radio analysis in the Offline software framework of the Pierre Auger Observatory.
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2011-04-11
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Elsevier Science BV
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Abstract
The advent of the Auger Engineering Radio Array (AERA) necessitates the development of a powerful framework for the analysis of radio measurements of cosmic ray air showers. As AERA performs "radio-hybrid" measurements of air shower radio emission in coincidence with the surface particle detectors and fluorescence telescopes of the Pierre Auger Observatory, the radio analysis functionality had to be incorporated in the existing hybrid analysis solutions for fluorescence and surface detector data. This goal has been achieved in a natural way by extending the existing Auger Offline software framework with radio functionality. In this article, we lay out the design, highlights and features of the radio extension implemented in the Auger Offline framework. Its functionality has achieved a high degree of sophistication and offers advanced features such as vectorial reconstruction of the electric field, advanced signal processing algorithms, a transparent and efficient handling of FFTs, a very detailed simulation of detector effects, and the read-in of multiple data formats including data from various radio simulation codes. The source code of this radio functionality can be made available to interested parties on request. (C) 2011 Elsevier B.V. All rights reserved.
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© 2011 Elsevier B.V. All rights reserved.
Artículo firmado por más de 10 autores (The Pierre Auger Collaboration).
We are grateful to the following agencies and organizations for financial support: Comision Nacional de Energia Atomica, Fundacion Antorchas, Gobierno De La Provincia de Mendoza, Municipalidad de Malargue, NDM Holdings and Valle Las Lenas, in gratitude for their continuing cooperation over land access, Argentina; the Australian Research Council; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundacao de Amparo a Pesquisa do Estado de Rio de Janeiro (FAPERJ), Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP), Ministerio de Ciencia e Tecnologia (MCT), Brazil; AVCR, AV0Z10100502 and AV0Z10100522, GAAV KJB300100801 and KJB100100904, MSMT-CR LA08016, LC527, 1M06002, and MSM0021620859, Czech Republic; Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil Regional Ile-de-France, Departement Physique Nucleaire et Corpusculaire (PNC-IN2P3/CNRS), Departement Sciences de l'Univers (SDU-INSU/CNRS), France; Bundesministerium fur Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Finanzministerium Baden-Wurttemberg, Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Ministerium fur Wissenschaft und Forschung, Nordrhein-Westfalen, Ministerium fur Wissenschaft, Forschung und Kunst, Baden-Wurttemberg, Germany; Istituto Nazionale di Fisica Nucleare (INFN), Istituto Nazionale di Astrofisica (INAF), Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR), Gran Sasso Center for Astroparticle Physics (CFA), Italy; Consejo Nacional de Ciencia y Tecnologia (CONACYT), Mexico; Ministerie van Onderwijs, Cultuur en Wetenschap, Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Stichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands; Ministry of Science and Higher Education, Grant nos. 1 P03 D 014 30 and N N202 207238, Poland; Fundacao para a Ciencia e a Tecnologia, Portugal; Ministry for Higher Education, Science, and Technology, Slovenian Research Agency, Slovenia; Comunidad de Madrid, Consejeria de Educacion de la Comunidad de Castilla La Mancha, FEDER funds, Ministerio de Ciencia e Innovacion and Consolider-Ingenio 2010 (CPAN), Generalitat Valenciana, Junta de Andalucia, Xunta de Galicia, Spain; Science and Technology Facilities Council, United Kingdom; Department of Energy, Contract nos. DE-AC02-07CH11359, DE-FR02-04ER41300; National Science Foundation, Grant no. 0969400, The Grainger Foundation USA; ALFA-EC/HELEN, European Union 6th Framework Program, Grant no. MEIF-CT-2005-025057, European Union 7th Framework Program, Grant no. PIEF-GA-2008-220240, and UNESCO.
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[1] J.V. Jelley, J.H. Fruin, N.A. Porter, et al., Nature 205 (1965) 327.
[2] D. Ardouin, A. Belle´toile, D. Charrier, et al., Nucl. Instr. and Meth. A 555 (2005) 148.
[3] H. Falcke, W.D. Apel, A.F. Badea, et al., Nature 435 (2005) 313.
[4] T. Huege, for the Pierre Auger Collaboration, Nucl. Instr. and Meth. A 617 (2009) 484.
[5] J. Abraham, M. Aglietta, I.C. Aguirre, et al., Nucl. Instr. and Meth. A 523 (2004) 50.
[6] S. Argiró , S.L.C. Barroso, J. Gonzalez, et al., Nucl. Instr. and Meth. A 580 (2007) 1485.
[7] S. Fliescher, the Pierre Auger Collaboration, Nucl. Instr. and Meth. A 604 (2009) S225.
[8] J. Coppens, the Pierre Auger Collaboration, Nucl. Instr. and Meth. A 604 (2009) S41.
[9] B. Revenu, the Pierre Auger and CODALEMA Collaborations, Nucl. Instr. And Meth. A 604 (2009) S37.
[10] O. Scholten, K. Werner, F. Rusydi, Astropart. Phys. 29 (2008) 94.
[11] T. Huege, R. Ulrich, R. Engel, Astropart. Phys. 27 (2007) 392.
[12] M. Ludwig, T. Huege, Astropart. Phys. 34 (2011) 438.
[13] M.A. DuVernois, B. Cai, D. Kleckner, Geosynchrotron radio pulse emission from extensive air showers: simulations with AIRES, in: Proceedings of the 29th ICRC, Pune, India, vol. 8, pp. 311–314.
[14] /http://www.fftw.orgS.
[15] /http://usg.lofar.org/svn/code/trunk/S