[PDF] Top 20 Large scale distribution of ultra high energy cosmic rays detected at the Pierre Auger Observatory with zenith angles up to 80 degrees
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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 degrees
... operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in ...grateful ... See full document
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Searches for Anisotropies in the Arrival Directions of the Highest Energy Cosmic Rays Detected by the Pierre Auger Observatory
... In the later sections we analyze the distribution of the arrival ...update the fraction of events correlating with AGNs in the VCV ...spite of ... See full document
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A search for anisotropy in the arrival directions of ultra high energy cosmic rays recorded at the Pierre Auger Observatory
... use of mock data sets built from the large scale structure of the Universe provides a useful tool to study the sensitivity of the three ...methods. ... See full document
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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
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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
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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
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Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger Observatory
... examples of the large-scale anisotropies expected from a Galactic CR component, we show in ...5 the direction of the dipole that would result for cosmic rays ... See full document
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Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger observatory
... is the same as that considered in The Pierre Auger Collaboration ( 2017a ), including events from the SD array with 1500 m separation detected from 2004 January 1 ... See full document
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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
... aim at characterizing the arrival directions in both right ascension and declination angles, it is also important to control the event rate in terms of local ...angles. ... See full document
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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 such a way that a solar day lasts ... See full document
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Searches for anisotropies in the arrival directions of the highest energy cosmic rays detected by the Pierre Auger observatory
... evidence of anisotropy at energies larger than 53 ...in the later sections we explore the set of arrival directions for cosmic rays observed with energies above 40 ... See full document
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Large-scale distribution of arrival directions of cosmic rays detected above 1018 ev at the pierre auger observatory
... The large-scale distribution of arrival directions of UHECRs as a function of the energy is thus one important observable to provide key elements for ... See full document
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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
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Multi-resolution anisotropy studies of ultrahigh-energy cosmic rays detected at the Pierre Auger Observatory
... whereas the needlet method with the same parameters used in this work achieves a detection power around ...On the other hand, for a point source with a given width, the angular ... See full document
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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
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Search for point-like sources of ultra-high energy neutrinos at the Pierre Auger Observatory and improved limit on the diffuse flux of tau neutrinos
... Although the primary goal of the SD is to detect UHECRs, it can also identify ultra-high energy ...Neutrinos of all flavours can interact at any atmospheric ... See full document
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Search for point-like sources of ultra-high energy neutrinos at the Pierre auger observatory and improved limit on the diffuse flux of tau neutrinos
... Although the primary goal of the SD is to detect UHECRs, it can also identify UHE ...Neutrinos of all flavors can interact at any atmospheric depth through charged or neutral ... See full document
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Ultrahigh-energy Neutrino Follow-up Of Gravitational Wave Events Gw150914 And Gw151226 With The Pierre Auger Observatory
... 2015 the Advanced LIGO detectors observed their first gravitational wave (GW) transient ...inferred to have arisen from the merger of black holes in binary ...from the formation ... See full document
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Hadronic physics with the Pierre Auger Observatory
... is the composition-averaged shower-to-shower ...on the details of hadronic interactions, and in practice is parametrized from the interaction models ...and the latest update ... See full document
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Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory
... value of the measurements lies in their ability to constrain UHECR propagation ...outline the pro- cedure to derive limits on scenario parameters using a sim- ple model for ... See full document
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