Search for correlations between the arrival directions of IceCube neutrino events and ultrahigh-energy cosmic rays detected by the Pierre Auger Observatory and the Telescope Array

• Published in: Journal of Cosmology and Astroparticle Physics
• Main Authors: Arqueros Martínez, Fernando, García Pinto, Diego, Minaya Flores, Ignacio Andrés, Rosado Vélez, Jaime, Vázquez Peñas, José Ramón
• Format: Article in Journal/Newspaper
• Language: English
• Published: IOP Publishing LTD 2016
• Subjects: 539.1; Galactic magnetic-field; Surface detector; Spectrum; Deflections; Performance; Física nuclear; 2207 Física Atómica y Nuclear; Canada; Marsden; New Zealand; National Science Foundation Office of Polar Programs; Swedish Polar Research Secretariat
• Online Access: https://hdl.handle.net/20.500.14352/24426; https://doi.org/10.1088/1475-7516/2016/01/037

© 2016 IOP Publishing Ltd and Sissa Medialab srl. Artículo firmado por más de 10 autores. The IceCube Collaboration acknowledges the support from the following agencies: U.S. National Science Foundation-Office of Polar Programs, U.S. National Science Foundation Physics Division, University of Wisconsin Alumni Research Foundation, the Grid Laboratory Of Wisconsin (GLOW) grid infrastructure at the University of Wisconsin Madison, the Open Science Grid (OSG) grid infrastructure; U.S. Department of Energy, and National Energy Research Scientific Computing Center, the Louisiana Optical Network Initiative (LONI) grid computing resources; Natural Sciences and Engineering Research Council of Canada, WestGrid and Compute/Calcul Canada; Swedish Research Council, Swedish Polar Research Secretariat, Swedish National Infrastructure for Computing (SNIC), and Knut and Alice Wallenberg Foundation, Sweden; German Ministry for Education and Research (BMBF), Deutsche Forschungsgemeinschaft (DFG), Helmholtz Alliance for Astroparticle Physics (HAP), Research Department of Plasmas with Complex Interactions (Bochum), Germany; Fund for Scientific Research (FNRS-FWO), FWO Odysseus programme, Flanders Institute to encourage scientific and technological research in industry (IWT), Belgian Federal Science Policy Office (Belspo); University of Oxford, United Kingdom; Marsden Fund, New Zealand; Australian Research Council; Japan Society for Promotion of Science (JSPS); the Swiss National Science Foundation (SNSF), Switzerland; National Research Foundation of Korea (NRF); Danish National Research Foundation, Denmark (DNRF).; The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargue. We are very grateful to the following agencies and organizations for financial support: Comision Nacional de Energia Atomica, Agencia Nacional de Promocion Cientifica y Tecnologica (ANPCyT), Consejo Nacional ...