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Search for first harmonic modulation in the right ascension distribution of cosmic rays detected at the Pierre Auger Observatory
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SYSNO ASEP 0364444 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title Search for first harmonic modulation in the right ascension distribution of cosmic rays detected at the Pierre Auger Observatory Author(s) Abreu, P. (AR)
Aglietta, M. (AR)
Ahn, E.J. (AR)
Boháčová, Martina (FZU-D) RID, ORCID
Chudoba, Jiří (FZU-D) RID, ORCID
Ebr, Jan (FZU-D) RID, ORCID
Kárová, Tatiana (FZU-D)
Mandát, Dušan (FZU-D) RID, ORCID
Nečesal, Petr (FZU-D)
Nožka, Libor (FZU-D) RID, ORCID
Nyklíček, Michal (FZU-D)
Palatka, Miroslav (FZU-D) RID, ORCID, SAI
Pech, Miroslav (FZU-D) RID, ORCID
Prouza, Michael (FZU-D) RID, ORCID
Řídký, Jan (FZU-D) RID, ORCID
Schovancová, Jaroslava (FZU-D)
Schovánek, Petr (FZU-D) RID, ORCID
Šmída, Radomír (FZU-D) RID
Trávníček, Petr (FZU-D) RID, ORCIDNumber of authors 470 Source Title Astroparticle Physics. - : Elsevier - ISSN 0927-6505
Roč. 34, č. 8 (2011), s. 627-639Number of pages 12 s. Language eng - English Country NL - Netherlands Keywords ultra-high energy cosmic rays ; large scale anisotropies ; Pierre Auger Observatory Subject RIV BF - Elementary Particles and High Energy Physics R&D Projects LC527 GA MŠMT - Ministry of Education, Youth and Sports (MEYS) 1M06002 GA MŠMT - Ministry of Education, Youth and Sports (MEYS) MEB111003 GA MŠMT - Ministry of Education, Youth and Sports (MEYS) LA08016 GA MŠMT - Ministry of Education, Youth and Sports (MEYS) CEZ AV0Z10100502 - FZU-D (2005-2011) AV0Z10100522 - FZU-D (2005-2011) UT WOS 000288930200007 DOI 10.1016/j.astropartphys.2010.12.007 Annotation We present the results of searches for dipolar-type anisotropies in different energy ranges above 2.5 × 1017 eV with the surface detector array of the Pierre Auger Observatory, reporting on both the phase and the amplitude measurements of the first harmonic modulation in the right-ascension distribution. Upper limits on the amplitudes are obtained, which provide the most stringent bounds at present, being below 2% at 99% C.L. for EeV energies. We also compare our results to those of previous experiments as well as with some theoretical expectations. Workplace Institute of Physics Contact Kristina Potocká, potocka@fzu.cz, Tel.: 220 318 579 Year of Publishing 2013
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