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Abstract:

Data collected by the Pierre Auger Observatory through 31 August 2007 showed evidence for anisotropy in the arrival directions of cosmic rays above the Greisen-Zatsepin-Kuz'min energy threshold, 6 × 10 19 eV. The anisotropy was measured by the fraction of arrival directions that are less than 3.1° from the position of an active galactic nucleus within 75 Mpc (using the Véron-Cetty and Véron 12th catalog). An updated measurement of this fraction is reported here using the arrival directions of cosmic rays recorded above the same energy threshold through 31 December 2009. The number of arrival directions has increased from 27 to 69, allowing a more precise measurement. The correlating fraction is 38-6+7%, compared with 21% expected for isotropic cosmic rays. This is down from the early estimate of 69-13+11%. The enlarged set of arrival directions is examined also in relation to other populations of nearby extragalactic objects: galaxies in the 2 Microns All Sky Survey and active galactic nuclei detected in hard X-rays by the Swift Burst Alert Telescope. A celestial region around the position of the radiogalaxy Cen A has the largest excess of arrival directions relative to isotropic expectations. The 2-point autocorrelation function is shown for the enlarged set of arrival directions and compared to the isotropic expectation. © 2010 Elsevier B.V. All rights reserved.

Registro:

Documento: Artículo
Título:Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter
Autor:Multitudinario:480
Filiación:Centro Atómico Bariloche, Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
Centro Atómico Constituyentes, Buenos Aires, Argentina
Centro de Investigaciones en Láseres y Aplicaciones, CITEFA and CONICET, Argentina
Departamento de Física, FCEyN, Universidad de Buenos Aires y CONICET, Argentina
IFLP, Universidad Nacional de la Plata and CONICET, La Plata, Argentina
Instituto de Astronomía y Física Del Espacio (CONICET-UBA), Buenos Aires, Argentina
National Technological University, Faculty Mendoza (CONICET/CNEA), Mendoza, Argentina
Pierre Auger Southern Observatory, Malargüe, Argentina
Pierre Auger Southern Observatory, Comisión Nacional de Energía Atómica, Malargüe, Argentina
University of Adelaide, Adelaide, SA, Australia
Centro Brasileiro de Pesquisas Fisicas, Rio de Janeiro, RJ, Brazil
Pontifícia Universidade Católica, Rio de Janeiro, RJ, Brazil
Universidade de São Paulo, Instituto de Física, São Carlos, SP, Brazil
Universidade de São Paulo, Instituto de Física, São Paulo, SP, Brazil
Universidade Estadual de Campinas, IFGW, Campinas, SP, Brazil
Universidade Estadual de Feira de Santana, Brazil
Universidade Estadual Do Sudoeste da Bahia, Vitoria da Conquista, BA, Brazil
Universidade Federal da Bahia, Salvador, BA, Brazil
Universidade Federal Do ABC, Santo André, SP, Brazil
Universidade Federal Do Rio de Janeiro, Instituto de Física, Rio de Janeiro, RJ, Brazil
Rudjer Bošković Institute, 10000 Zagreb, Croatia, Croatia
Charles University, Faculty of Mathematics and Physics, Institute of Particle and Nuclear Physics, Prague, Czech Republic
Institute of Physics, Academy of Sciences of the Czech Republic, Prague, Czech Republic
Palacký University, Olomouc, Czech Republic
Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris 11, CNRS-IN2P3, Orsay, France
Laboratoire AstroParticule et Cosmologie (APC), Université Paris 7, CNRS-IN2P3, Paris, France
Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris 11, CNRS-IN2P3, Orsay, France
Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France
Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier, INPG, CNRS-IN2P3, Grenoble, France
SUBATECH, CNRS-IN2P3, Nantes, France
Bergische Universität Wuppertal, Wuppertal, Germany
Karlsruhe Institute of Technology, Campus North, Institut für Kernphysik, Karlsruhe, Germany
Karlsruhe Institute of Technology, Campus North, Institut für Prozessdatenverarbeitung und Elektronik, Karlsruhe, Germany
Karlsruhe Institute of Technology, Campus South, Institut für Experimentelle Kernphysik (IEKP), Karlsruhe, Germany
Max-Planck-Institut für Radioastronomie, Bonn, Germany
RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
Universität Hamburg, Hamburg, Germany
Universität Siegen, Siegen, Germany
Dipartimento di Fisica dell'Universit, INFN, Genova, Italy
Universit dell'Aquila, INFN, L'Aquila, Italy
Universit di Milano, Sezione INFN, Milan, Italy
Dipartimento di Fisica Dell, Universit Del Salento and Sezione INFN, Lecce, Italy
Universit di Napoli Federico, Sezione INFN, Napoli, Italy
Universit di Roma II Tor Vergata, Sezione INFN, Roma, Italy
Universit di Catania and Sezione INFN, Catania, Italy
Universit di Torino and Sezione INFN, Torino, Italy
Dipartimento di Ingegneria dell'Innovazione Dell', Universit Del Salento and Sezione INFN, Lecce, Italy
Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo (INAF), Palermo, Italy
Istituto di Fisica Dello Spazio Interplanetario (INAF), Universit di Torino and Sezione INFN, Torino, Italy
INFN, Laboratori Nazionali Del Gran Sasso, Assergi (L'Aquila), Italy
Universit di Palermo and Sezione INFN, Catania, Italy
Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
Centro de Investigación y de Estudios Avanzados Del IPN (CINVESTAV), México, Mexico
Universidad Michoacana de San Nicolas de Hidalgo, Morelia, Michoacan, Mexico
Universidad Nacional Autonoma de Mexico, Mexico, Mexico
IMAPP, Radboud University, Nijmegen, Netherlands
Kernfysisch Versneller Instituut, University of Groningen, Groningen, Netherlands
NIKHEF, Amsterdam, Netherlands
ASTRON, Dwingeloo, Netherlands
Institute of Nuclear Physics PAN, Krakow, Poland
University of Łódź, Łódź, Poland
LIP and Instituto Superior Técnico, Lisboa, Portugal
J. Stefan Institute, Ljubljana, Slovenia
Laboratory for Astroparticle Physics, University of Nova Gorica, Slovenia
Instituto de Física Corpuscular, CSIC-Universitat de Valncia, Valencia, Spain
Universidad Complutense de Madrid, Madrid, Spain
Universidad de Alcalá, Alcalá de Henares (Madrid), Spain
Universidad de Granada and C.A.F.P.E., Granada, Spain
Universidad de Santiago de Compostela, Spain
Rudolf Peierls Centre for Theoretical Physics, University of Oxford, Oxford, United Kingdom
School of Physics and Astronomy, University of Leeds, United Kingdom
Argonne National Laboratory, Argonne, IL, United States
Case Western Reserve University, Cleveland, OH, United States
Colorado School of Mines, Golden, CO, United States
Colorado State University, Fort Collins, CO, United States
Colorado State University, Pueblo, CO, United States
Fermilab, Batavia, IL, United States
Louisiana State University, Baton Rouge, LA, United States
Michigan Technological University, Houghton, MI, United States
New York University, New York, NY, United States
Northeastern University, Boston, MA, United States
Ohio State University, Columbus, OH, United States
Pennsylvania State University, University Park, PA, United States
Southern University, Baton Rouge, LA, United States
University of California, Los Angeles, CA, United States
University of Chicago, Enrico Fermi Institute, Chicago, IL, United States
University of Nebraska, Lincoln, NE, United States
University of New Mexico, Albuquerque, NM, United States
University of Wisconsin, Madison, WI, United States
University of Wisconsin, Milwaukee, WI, United States
Institute for Nuclear Science and Technology (INST), Hanoi, Viet Nam
Caltech, Pasadena, United States
Konan University, Kobe, Japan
Palabras clave:Anisotropy; Cosmic rays; Extra-galactic; GZK; Pierre Auger Observatory; UHECR; Anisotropy; Augers; Autocorrelation; Cosmic ray measurement; Cosmology; Galaxies; Observatories; X rays; Active galactic nuclei; Autocorrelation functions; Burst alert telescopes; Extra-galactic; Extragalactic objects; Pierre Auger observatory; Precise measurements; UHECR; Cosmic rays
Año:2010
Volumen:34
Número:5
Página de inicio:314
Página de fin:326
DOI: http://dx.doi.org/10.1016/j.astropartphys.2010.08.010
Título revista:Astroparticle Physics
Título revista abreviado:Astropart. Phys.
ISSN:09276505
CODEN:APHYE
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_09276505_v34_n5_p314_Multitudinario

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Citas:

---------- APA ----------
(2010) . Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter. Astroparticle Physics, 34(5), 314-326.
http://dx.doi.org/10.1016/j.astropartphys.2010.08.010
---------- CHICAGO ----------
Multitudinario:480. "Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter" . Astroparticle Physics 34, no. 5 (2010) : 314-326.
http://dx.doi.org/10.1016/j.astropartphys.2010.08.010
---------- MLA ----------
Multitudinario:480. "Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter" . Astroparticle Physics, vol. 34, no. 5, 2010, pp. 314-326.
http://dx.doi.org/10.1016/j.astropartphys.2010.08.010
---------- VANCOUVER ----------
Multitudinario:480. Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter. Astropart. Phys. 2010;34(5):314-326.
http://dx.doi.org/10.1016/j.astropartphys.2010.08.010