Authors

J. Abraham, Karlsruher Institut für Technologie, Campus Süd
M. Aglietta, Louisiana State University
C. Aguirre, National Technical University of Athens
D. Allard, Charles University
I. Allekotte, Consejo Nacional de Investigaciones Científicas y Técnicas
P. Allison, Universidade Estadual do Sudoeste da Bahia
C. Alvarez, The Ohio State University
J. Alvarez-Muñiz, Pierre Auger Observatory
M. Ambrosio, Colorado State University
L. Anchordoqui, Universidade Estadual de Feira de Santana
J. C. Anjos, Università degli Studi dell'Aquila
C. Aramo, Colorado State University
K. Arisaka, Universidade Federal Fluminense
E. Armengaud, Universidad Nacional Autónoma de México
F. Arneodo, Michigan Technological University
F. Arqueros, Consejo Nacional de Investigaciones Científicas y Técnicas
T. Asch, Instituto de Astronomía y Física del Espacio
H. Asorey, Consejo Nacional de Investigaciones Científicas y Técnicas
B. S. Atulugama, Universidade Federal da Bahia
J. Aublin, Universidad Michoacana de San Nicolás de Hidalgo
M. Ave, Charles University
G. Avila, Karlsruher Institut für Technologie, Campus Nord
J. Bacelar, University of Colorado Boulder
T. Bäcker, Universidad de Alcalá
D. Badagnani, Rheinisch-Westfälische Technische Hochschule Aachen
A. F. Barbosa, Università degli Studi dell'Aquila
H. M.J. Barbosa, Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
M. Barkhausen, Netherlands Foundation for Research in Astronomy
D. Barnhill, Universidade Federal Fluminense
S. L.C. Barroso, Università degli Studi dell'Aquila
P. Bauleo, Universidad Mayor de San Andres Bolivia
J. Beatty, Universidade Estadual do Sudoeste da Bahia
T. Beau, Universidad Nacional Autónoma de México

Document Type

Article

Publication Date

1-1-2007

Abstract

An upper limit of 16% (at 95% c.l.) is derived for the photon fraction in cosmic rays with energies greater than 1019 eV, based on observations of the depth of shower maximum performed with the hybrid detector of the Pierre Auger Observatory. This is the first such limit on photons obtained by observing the fluorescence light profile of air showers. This upper limit confirms and improves on previous results from the Haverah Park and AGASA surface arrays. Additional data recorded with the Auger surface detectors for a subset of the event sample support the conclusion that a photon origin of the observed events is not favored. © 2006 Elsevier B.V. All rights reserved.

Publication Source (Journal or Book title)

Astroparticle Physics

First Page

155

Last Page

168

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