[PDF] Top 20 O Papel dos objectivos de trabalho no desempenho dos trabalhadores (Estudo de Caso)
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Average shape of longitudinal shower profiles measured at the Pierre Auger Observatory
... 1. Average longitudinal shower profile in data (top) and simulation (bottom) for events with energies between 10 ...The measured normalized energy deposit is shown in black, and the coloured ... See full document
11
Mass sensitive observables of the Pierre Auger Observatory
... air shower is more spread in time than its muonic ...be measured at different longitudinal depths by comparing signals in stations located up- and down-stream of the incoming shower ...the ... See full document
12
Depth of maximum of air-shower profiles: testing the compatibility of measurements performed at the Pierre Auger Observatory and the Telescope Array experiment
... the shower simulations with EPOS-LHC for the TA BR / LR will be ...the Auger and TA energy scales [19] and systematic errors on the fractions of nuclei in the AugerMix MC tem- plates used by Auger to ... See full document
10
Search for a correlation between the UHECRs measured by the Pierre Auger Observatory and the Telescope Array and the neutrino candidate events from IceCube and ANTARES
... their longitudinal development through telescopes that detect the fluorescence emission of the atmosphere particles or sampled at the ground with arrays of particle ...the Pierre Auger ... See full document
13
A measurement of the muon number in showers using inclined events detected at the Pierre Auger Observatory
... The Pierre Auger Observatory [1] is a hybrid cosmic ray air shower experiment that uses different techniques to detect extensive ...The longitudinal shower development is ... See full document
7
Latest results from the Pierre Auger Observatory
... the shower core between 1700 m and 4000 m were included, thus allowing a clear selection of the signal due to the muonic component, without any bias arising from the electromagnetic ... See full document
26
The Pierre Auger Observatory: Review of Latest Results and Perspectives
... the Pierre Auger Observatory for a diffuse flux of neutrinos in the period 1 Jan 2004 - 31 March ...in Auger using hybrid events, the blue dashed boxes mark the systematic uncertainties of ... See full document
6
Precision measurements of cosmic rays up to the highest energies with a large radio array at the Pierre Auger Observatory
... The renaissance of radio detection of cosmic rays be- gan in the early 2000s [6–8]. In parallel with the ex- perimental activities, strong efforts were devoted to the modeling of the radio emission physics. Two lines of ... See full document
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Correlation between the UHECRs measured by the Pierre Auger Observatory and Telescope Array and neutrino candidate events from IceCube
... The Pierre Auger Observatory, located in Malargüe, Argentina (35.2 ◦ S, 69.5 ◦ W, 1400 m a.s.l.) [5, 6], consists of surface detectors and air fluorescence telescopes designed to perform ... See full document
23
The Pierre Auger Observatory status and the AugerPrime upgrade program
... The Pierre Auger Observatory [1] with its 3000 km 2 of instrumented surface, brings unique capabilities to the UHECR ...The Observatory is located in the province of Mendoza (Argentina) near ... See full document
14
The Pierre Auger Observatory: latest results and future perspectives
... the shower. Furthermore, interactions of the secondary particles of a shower with the atmosphere can lead to the excitacion of nitrogen molecules, and then de-excitation via fluorescence light ...the ... See full document
18
Large scale anisotropy studies with the Pierre Auger Observatory
... The Pierre Auger Observatory in Argentina mea- sures air showers initiated by cosmic rays at EeV energy scales (1 EeV = 10 18 ...the Pierre Auger Observatory since 1 January ... See full document
6
Studies of Cosmic Rays at the Highest Energies with the Pierre Auger Observatory
... As mentioned above, the physical origin of the structure in the cosmic ray spectrum known as the “ankle" (at about 5 EeV) is not settled yet. There are two main candidate scenarios to explain it (see Ref. [1] for a ... See full document
15
Warped extra dimension and inclined events at Pierre Auger Observatory
... Recently, three neutrinos of energy 1-2 PeV, as well as tens of neutrinos above 10 TeV were de- tected with the IceCube experiment [1]. The cosmic neutrinos with energies near 1 EeV are detectable with the Surface ... See full document
30
Multi-messenger Astrophysics at Ultra-High Energy with the Pierre Auger Observatory
... that Auger is a highly sensitive neutrino detector with its sensitivity limited mainly by its lifetime but not by the background due to UHECR-induced showers since this can be very ef- ficiently reduced as shown ... See full document
17
Direct Measurement of the Muon Density in Air Showers with the Pierre Auger Observatory
... The largest systematic uncertainties result from the area-dependent e ffi ciency correction of the muon densi- ties recorded by individual detector modules (9.9%) and the lack of knowledge of the shape of the muon ... See full document
5
Measurement of the muon content in air showers at the Pierre Auger Observatory
... Nevertheless, an important effect can be expected from the hadronic-interaction models when they are tuned [10] to reproduce the rho-meson spectra from collider experiments [11] more accurately, especially in the extreme ... See full document
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Preliminary results of the AMIGA engineering array at the Pierre Auger Observatory
... air shower with reconstructed energy of ...air shower ar- rival geometry and energy were obtained from the surface WCD array, SD-750 ...The measured muon densities [9] at each position are shown in ... See full document
18
General overview of recent results from the Pierre Auger Observatory
... to one or both experiments could account for most differ- ences between them. The ankle seems to be somewhat more sharply defined in our data. This is possibly due to a system- atic energy offset between the two ... See full document
9
The importance of atmospheric monitoring at the Pierre Auger Observatory
... Complementary information is provided by scanning infra-red cameras, again one per FD site, which image the FD telescope fields of view (FOV) every 5 minutes and the entire sky every 15 minutes. In 2013 the cameras, ... See full document
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