[PDF] Top 20 Large Scale Distribution of Ultra High Energy Cosmic Rays Detected at the Pierre Auger Observatory With Zenith Angles up to 80°
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Large Scale Distribution of Ultra High Energy Cosmic Rays Detected at the Pierre Auger Observatory With Zenith Angles up to 80°
... As the amplitudes of the large scale modulations to be measured are rather small, at the few percent level, it is very important to carefully account for ... See full document
26
A search for anisotropy in the arrival directions of ultra high energy cosmic rays recorded at the Pierre Auger Observatory
... Observations of cosmic ray arrival directions made with the Pierre Auger Obser- vatory have previously provided evidence of anisotropy at the 99% CL using ... See full document
22
Ultrahigh Energy Neutrinos at the Pierre Auger Observatory
... High energy neutrinos can be detected with a variety of techniques [13, ...observed with arrays of detectors at ground level that are currently being used to ... See full document
36
Searches for Anisotropies in the Arrival Directions of the Highest Energy Cosmic Rays Detected by the Pierre Auger Observatory
... measurements of the energy spectrum of ultra-high energy cosmic rays (UHE- CRs), their mass composition and the celestial distribution ... See full document
38
Searches for Large-Scale Anisotropy in the Arrival Directions of Cosmic Rays Detected above Energy of $10^{19}$ eV at the Pierre Auger Observatory and the Telescope Array
... evaluating the amplitude of the first harmonics for fictitious right ascension angles calculated by dilating the time of the events in a way that a solar day lasts about ... See full document
33
Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger Observatory
... ( The Pierre Auger Collaboration 2017b ), since, otherwise, systematic modulations of the rates as a function of the hour of the day or of the ... See full document
16
Measurement of the Cosmic Ray Spectrum above 4 $\times$ 10$^{18}$ eV Using Inclined Events Detected with the Pierre Auger Observatory
... choice of deep-water Cherenkov detectors for the Pierre Auger Observatory was made to give substantial solid angle coverage for zenith angles exceeding 60 ◦ thus ... See full document
25
Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory
... in the data can be used to establish a lower bound on the density of sources (the same happens also in the case of the 60 and 80 EeV energy ... See full document
25
Ultrahigh-Energy Neutrino Follow-Up of Gravitational Wave Events GW150914 and GW151226 with the Pierre Auger Observatory
... With the surface detector (SD) of the Pierre Auger Ob- servatory [20] we can identify neutrino-induced air show- ers in the energy range above 100 PeV ...neutrinos ... See full document
10
Multi-resolution anisotropy studies of ultrahigh-energy cosmic rays detected at the Pierre Auger Observatory
... scenarios of UHECR origin ...in the case of an excess along a plane such as the Galactic or super-galactic planes, which are plausible source regions at high ...Although ... See full document
27
Large-scale distribution of arrival directions of cosmic rays detected above 1018 ev at the pierre auger observatory
... amplitudes of anisotropy obviously depend on the rigidity E/Z of the cosmic rays, with Z the electric charge of the ...aim to illustrate ... See full document
20
Measurement of the average electromagnetic longitudinal shower profile at the Pierre Auger Observatory
... The Pierre Auger Observatory is a hybrid detector, consisting of a 3000 km 2 Surface Detector array (SD) overlooked by the Fluorescence Detector ...(FD). The FD consists ... See full document
8
Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory
... for the construction and operation of the LIGO Labo- ratory and Advanced LIGO as well as the Science and Tech- nology Facilities Council (STFC) of the United Kingdom, the ... See full document
22
Measurement of the Muon Content of EAS With the Pierre Auger Observatory
... The Pierre Auger Observatory is a hybrid detector with the aim of studying the characteristics of the longitudinal and lateral profiles of ... See full document
6
Measurement of the Proton-Air Cross Section at s√=57 TeV with the Pierre Auger Observatory
... patible with there being a substantial fraction of protons; also there are a large number of events recorded in this energy ...range. The corresponding average ... See full document
9
Particle physics measurements at the highest energies with the Pierre Auger Observatory
... on the average of the logarithm of the nuclear mass hln Ai, while its dispersion depends both on the hln Ai and σ 2 (ln ...between the moments of X max and ln A can ... See full document
7
Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory
... uses the standard thinning procedure [ 32 ] consisting in follow- ing only some branches in the tree of interactions in the ...attributed to the surviving branches, obtaining a ... See full document
16
Improved limit to the diffuse flux of ultrahigh energy neutrinos from the Pierre Auger Observatory
... Energ´ıa At´ omica, Fundaci´ on Antorchas, Gobierno de la Provincia de Mendoza, Mu- nicipalidad de Malarg¨ ue, NDM Holdings and Valle Las Le˜ nas, in gratitude for their continuing cooperation over land access, ... See full document
14
Highlights from the Pierre Auger Observatory
... isotropic distribution are indicated by the dotted ...similarly to the results from the analysis in [19], interesting hints for large scale anisotropies that will be ... See full document
9
Search for ultrarelativistic magnetic monopoles with the Pierre Auger Observatory
... max to be larger than X up , which is al- most always fulfilled by ultrarelativistic IMM ...6% of the UHECR proton showers of 10 ...cut, the fraction increasing to 32% for ... See full document
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