[PDF] Top 20 High-energy interactions at the Pierre Auger Observatory
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High-energy interactions at the Pierre Auger Observatory
... (FAPESP), Minist´erio de Ciˆencia e Tecnologia (MCT), Brazil; AVCR AV0Z10100502 and AV0Z10100522, GAAV KJB100100904, MSMT-CR LA08016, LC527, 1M06002, MEB111003, and MSM0021620859, Czech Re- public; Centre de Calcul ... See full document
7
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
... in the detector configuration during data taking, due to the dead times of the SD stations, and to the increase of the array size during the construction phase, may introduce a ... 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 ...interact at any atmospheric depth through charged or neutral currents and induce a “downward-going” (DG) ... See full document
7
Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth
... within the Investissements d’Avenir Programme ANR- 11-IDEX-0004-02, French National Research Agency under grant ...2011-3-0062, the Minister of National Education, Programme for research - Space Technology ... See full document
15
Upper limit on the diffuse flux of ultrahigh energy tau neutrinos from the pierre auger observatory
... ultrahigh energy (UHE) cosmic neu- trinos at EeV (1 EeV 10 18 eV) energies and above is a long-standing experimental ...to the universe [ 4 ], and provide an unique opportunity to test fundamental ... See full document
7
Spectral Calibration of the Fluorescence Telescopes of the Pierre Auger Observatory
... The energy of the primary cosmic ray is a key measurable for the science of the observatory, and the FD measurement of the energy, with lower indepen- dent ... See full document
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Muons in air showers at the Pierre Auger Observatory: Mean number in highly inclined events
... PN-II-RU-PD-2011-3-0062, the Minister of National Education, Programme for research - Space Technology and Advanced Research - STAR, project number 83/2013, Romania; Slovenian Research Agency, Slovenia; Comunidad ... See full document
12
Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory
... The Auger Engineering Radio Array (AERA) is part of the Pierre Auger Observatory and is used to detect the radio emission of cosmic-ray air ...to the data of ... See full document
14
Techniques for Measuring Aerosol Attenuation using the Central Laser Facility at the Pierre Auger Observatory
... with the FD at Coihueco under various atmospheric conditions. The height is given above the ...FD. The number of photons at the aperture of the FD is normalized per ... See full document
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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
Depth of maximum of air-shower profiles at the Pierre Auger Observatory. II. Composition implications
... improves the fits for all hadronic interaction ...of the energy ...brings the models into remarkable agreement in their predictions of the protons and iron nuclei contributions despite ... See full document
13
Constraints and measurements of hadronic interactions in extensive air showers with the Pierre Auger Observatory
... of the Pierre Auger Observatory is to unveil the origin and nature of ...favoring the acceleration scenarios in astro- physical ...reach the fluxes of cosmological origin ... See full document
9
Measurement of the Proton-Air Cross Section at s√=57 TeV with the Pierre Auger Observatory
... MSM0021620859, Czech Republic; Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil Re´gional Ile-de-France, De´partement Physique Nucle´aire et Corpusculaire (PNC- IN2P3/CNRS), ... See full document
9
Depth of maximum of air-shower profiles at the Pierre Auger Observatory. I. Measurements at energies above 1017.8 eV
... II. THE PIERRE AUGER OBSERVATORY In this paper we present data from the Pierre Auger Observatory [35] ...in the province of Mendoza, Argentina, and consists ... See full document
25
Limit on the diffuse flux of ultrahigh energy tau neutrinos with the surface detector of the Pierre Auger Observatory
... as the electromagnetic component still develops, produce a ToT local trigger (see ...produce high amplitude signals extended in time or two independent muons can arrive inside the given time ...to ... See full document
15
A targeted search for point sources of EeV photons with the Pierre Auger Observatory
... adopts the Galac- tic point source target sets defined in Aab et ...adds the new H.E.S.S. unidentified sources reported in Deil et al. (2015). The Galactic source classes are millisecond pulsars ... See full document
9
Ultrahigh-Energy Neutrino Follow-Up of Gravitational Wave Events GW150914 and GW151226 with the Pierre Auger Observatory
... use the same identification criteria as in [21] to search for neutrinos in temporal and spa- tial coincidence with GW150914 and GW151226, as well as with the GW candidate event LVT151012 ...[4]. The ... See full document
10
Questions and Answers in Extreme Energy Cosmic Rays – a guide to explore the data set of the Pierre Auger Observatory
... The Pierre Auger Observatory is the largest extensive air shower detector, covering 3000 km 2 in ...Argentina. The Observatory makes available, for educational and ... See full document
5
Calibration of the logarithmic-periodic dipole antenna (LPDA) radio stations at the Pierre Auger Observatory using an octocopter
... in the MegaHertz (MHz) regime has become a complementary technique to exploit readout and calibration of the atmospheric calorimeter [ 2 – 7 ...this, the Pierre Auger Observatory ... 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 ...of the large data set (three times larger ... See full document
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