Authors

B. Revenu, Université de Nantes
A. Aab, Universität SiegenFollow
P. Abreu, Instituto Superior TécnicoFollow
M. Aglietta, Istituto Nazionale di Fisica Nucleare, Sezione di TorinoFollow
E. J. Ahn, Fermi National Accelerator LaboratoryFollow
I. Al Samarai, Laboratoire de Physique Nucléaire et de Hautes EnergiesFollow
I. F.M. Albuquerque, Universidade de São PauloFollow
I. Allekotte, Instituto BalseiroFollow
P. Allison, The Ohio State UniversityFollow
A. Almela, Consejo Nacional de Investigaciones Científicas y Técnicas
J. Alvarez Castillo, Universidad Nacional Autónoma de MéxicoFollow
J. Alvarez-Muñiz, Universidad de Santiago de CompostelaFollow
M. Ambrosio, Istituto Nazionale di Fisica Nucleare, Sezione di NapoliFollow
G. A. Anastasi, Gran Sasso Science InstituteFollow
L. Anchordoqui, Lehman CollegeFollow
B. Andrada, Consejo Nacional de Investigaciones Científicas y TécnicasFollow
S. Andringa, Instituto Superior TécnicoFollow
C. Aramo, Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
F. Arqueros, Universidad Complutense de Madrid
N. Arsene, Universitatea din Bucuresti
H. Asorey, Instituto Balseiro
P. Assis, Instituto Superior Técnico
J. Aublin, Laboratoire de Physique Nucléaire et de Hautes Energies
G. Avila, Pierre Auger Observatory
A. M. Badescu, University Politehnica of Bucharest
A. Balaceanu, Horia Hulubei National Institute of Physics and Nuclear Engineering
C. Baus, Karlsruher Institut für Technologie
J. J. Beatty, The Ohio State University
K. H. Becker, Bergische Universität Wuppertal
J. A. Bellido, The University of Adelaide
C. Berat, Universite Grenoble Alpes
M. E. Bertaina, Istituto Nazionale di Fisica Nucleare, Sezione di Torino
X. Bertou, Instituto Balseiro

Document Type

Conference Proceeding

Publication Date

3-23-2017

Abstract

We present the lastest results and status of the Auger Engineering Radio Array (AERA), located within the Pierre Auger Observatory. AERA, with more than 150 radio stations spread over 17 km2, is the largest radio detector in the world for extensive air showers above 1017 eV. The electric field emitted by secondary electrons and positrons allows us to estimate all characteristics of the primary cosmic ray: arrival direction, energy and mass composition. The performance of AERA together with the analysis methods are described. The final aim of AERA is mainly to improve the composition estimation of ultra-high energy cosmic rays as a standalone detector or in association with other instruments such as a ground particle detector or a fluorescence telescope.

Publication Source (Journal or Book title)

EPJ Web of Conferences

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