[PDF] Top 20 A Targeted Search For Point Sources Of Eeev Photons With The Pierre Auger Observatory
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A Targeted Search For Point Sources Of Eeev Photons With The Pierre Auger Observatory
... operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in ...to ... See full document
7
A search for point sources of eev neutrons
... consists of events recorded by the surface detector (SD) from 2004 January 1 to 2011 September ...time, the size of the Observatory increased from 154 to 1660 SD ...neighbors ... See full document
11
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
... Details of the neutrino selection procedure, of the calculation of the detector exposure for ES showers, and of sources of systematic uncertainties are given ... See full document
7
A Search for Point Sources of EeV Neutrons
... is the upper limit on the number of events (as described above) divided by the directional exposure at the target ...center. The exposure depends on the trigger ... See full document
28
Multi-messenger physics with the Pierre Auger Observatory
... The Pierre Auger Observatory is the largest and most precise detector of ultra-high energy air showers, such as those regularly induced by cosmic ...correlation with light ... See full document
20
A Targeted Search for Point Sources of EeV Neutrons
... detection of neutron sources would have identified sources of EeV protons in the ...Galaxy. The null results here leave open the question of whether the ... See full document
17
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
... (2002). The observation of UHECRs makes an associated flux of ultra-high energy cosmic neutrinos (UHEνs) Becker (2008) very ...models of UHECR production predict neutrinos as a result of ... See full document
21
A search for anisotropy in the arrival directions of ultra high energy cosmic rays recorded at the Pierre Auger Observatory
... version of the classic 2pt-L test was devised: the 2pt+ method ...to the angular distance λ between event pairs, the 2pt+ test uses two extra variables related to the orientation ... See full document
22
Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory
... in the arrival direc- tions of cosmic rays are searched for using data of the Pierre Auger ...around the highest-energy cosmic rays with E ≥ 6×10 19 eV by analyz- ... See full document
16
Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory
... rays with energies above E = 5 × 10 18 eV arriving within an angular separation of approximately ...characterize the energy distributions inside these regions by two inde- pendent methods, one ... See full document
16
Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory
... 2017, the Advanced LIGO ( Aasi et ...from the merger, consistent with kilo- nova/macronova ...allowed the precise localization of the merger in the galaxy NGC 4993, at ... See full document
22
Ultrahigh Energy Neutrinos at the Pierre Auger Observatory
... detected with a variety of techniques [13, ...observed with arrays of detectors at ground level that are currently being used to measure extensive showers produced by cosmic rays ...[15]. ... See full document
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Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory
... prediction of the background. We observe that the tail of the background distribution of F is consistent with an exponential ...to the distribution of F for ... See full document
16
A targeted search for point sources of EeV photons with the Pierre Auger Observatory
... for photons and neutrons, any candi- date source of neutrons is also a candidate source of pho- ...adopts the Galac- tic point source target sets defined in Aab et ...adds the ... See full document
9
A search for point sources of EeV photons
... candidate sources and “stacks” of candidates having astrophysical characteristics in ...number of trials. Neutrons and photons arise from the same types of pion-producing ... See full document
28
Search for photons with energies above 10$^{18}$ eV using the hybrid detector of the Pierre Auger Observatory
... – the Australian Research Council; Brazil – Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq); Financiadora de Estudos e Projetos (FINEP); Fundação de Amparo à Pesquisa do Estado de Rio de ... See full document
23
Azimuthal Asymmetry in the Risetime of the Surface Detector Signals of the Pierre Auger Observatory
... appreciate the origin of the asymmetries, we have to un- derstand the behavior of the copious number of muons and electromagnetic particles that reach the ...shower ... See full document
16
Azimuthal asymmetry in the risetime of the surface detector signals of the Pierre Auger Observatory
... appreciate the origin of the asymmetries, we have to understand the behavior of the copious number of muons and electromagnetic particles that reach the ...shower ... See full document
17
Search for high-energy neutrinos from binary neutron star merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory
... within the Investissements d ’Avenir Programme grant ...Center of Excellence; Ministero degli Affari Esteri (MAE); Mexico—Consejo Nacional de Ciencia y Tecnología (CONACYT) ... See full document
19
Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory
... determination of the primary energy of extensive air showers using the fluorescence detection technique requires an estimation of the energy carried away by particles that do not ... See full document
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