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Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger Observatory

dc.contributor.authorPierre Auger collaboration (376 authors)
dc.contributor.authorAbreu, Pedro
dc.contributor.authorAndringa, Sofia
dc.contributor.authorAssis, Pedro
dc.contributor.authorBarreira Luz, Ricardo Jorge
dc.contributor.authorBlanco, Alberto
dc.contributor.authorCazon, Lorenzo
dc.contributor.authorConceição, Ruben
dc.contributor.authorDiogo, Francisco
dc.contributor.authorLopes, Luis
dc.contributor.authorPimenta, Mário
dc.contributor.authorRiehn, Felix
dc.contributor.authorSantos, Eva
dc.contributor.authorSarmento, Raul
dc.contributor.authorTomé, Bernardo
dc.date.accessioned2019-02-05T16:51:21Z
dc.date.available2019-02-05T16:51:21Z
dc.date.issued2018-11-13
dc.date.updated2019-02-05T16:51:21Z
dc.description.abstractWe present a detailed study of the large-scale anisotropies of cosmic rays with energies above 4 EeV measured using the Pierre Auger Observatory. For the energy bins [4,8] EeV and $E\geq 8$ EeV, the most significant signal is a dipolar modulation in right ascension at energies above 8 EeV, as previously reported. In this paper we further scrutinize the highest-energy bin by splitting it into three energy ranges. We find that the amplitude of the dipole increases with energy above 4 EeV. The growth can be fitted with a power law with index $\beta=0.79\pm 0.19$. The directions of the dipoles are consistent with an extragalactic origin of these anisotropies at all the energies considered. Additionally we have estimated the quadrupolar components of the anisotropy: they are not statistically significant. We discuss the results in the context of the predictions from different models for the distribution of ultrahigh-energy sources and cosmic magnetic fields.
dc.description.versionPeer Reviewed
dc.identifierAstrophys.J. 868 (2018) 4; DOI 10.3847/1538-4357/aae689
dc.identifier.urihttp://dx.doi.org/10.3847/1538-4357/aae689
dc.identifier.urihttp://hdl.handle.net/10400.26/27708
dc.language.isoeng
dc.titleLarge-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger Observatory
dc.typejournal article
dspace.entity.typePublication
rcaap.rightsopenAccesspt
rcaap.typearticle

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