0000000000104882

AUTHOR

H. Martinez

showing 96 related works from this author

Measurement of the cosmic-ray energy spectrum above 2.5×1018  eV using the Pierre Auger Observatory

2020

We report a measurement of the energy spectrum of cosmic rays for energies above 2.5×10^18 eV based on 215,030 events recorded with zenith angles below 60°. A key feature of the work is that the estimates of the energies are independent of assumptions about the unknown hadronic physics or of the primary mass composition. The measurement is the most precise made hitherto with the accumulated exposure being so large that the measurements of the flux are dominated by systematic uncertainties except at energies above 5×10^19 eV. The principal conclusions are(1) The flattening of the spectrum near 5×10^18 eV, the so-called "ankle,"is confirmed.(2) The steepening of the spectrum at around 5×10^19…

cosmic ray; astroparticle detectors; cosmic ray spectraEnergy SpectrumSettore FIS/01 - Fisica SperimentaleUltra-high energy cosmic rays energy spectrum Cherenkov detectorsUHE Cosmic Rays
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Measurement of the Higgs boson mass from theH→γγandH→ZZ*→4ℓchannels inppcollisions at center-of-mass energies of 7 and 8 TeV with the ATLAS detector

2014

An improved measurement of the mass of the Higgs boson is derived from a combined fit to the reconstructed invariant mass spectra of the decay channels H -> gamma gamma and H -> ZZ* -> 4l. The analysis uses the pp collision data sample recorded by the ATLAS experiment at the CERN Large Hadron Collider at center-of-mass energies of 7 TeV and 8 TeV, corresponding to an integrated luminosity of 25 fb(-1). The measured value of the Higgs boson mass is m(H) = 125.36 +/- 0.37(stat) +/- 0.18 (syst) GeV. This result is based on improved energy-scale calibrations for photons, electrons, and muons as well as other analysis improvements, and supersedes the previous result from ATLAS. Upper limits on t…

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderMuon010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyATLAS experiment7. Clean energy01 natural sciencesAtomic massNuclear physicsmedicine.anatomical_structureAtlas (anatomy)0103 physical sciencesmedicineHiggs bosonHigh Energy Physics::ExperimentInvariant massCenter of mass010306 general physicsPhysical Review D
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Measurement of the top pair production cross section in 8 TeV proton-proton collisions using kinematic information in thelepton+jetsfinal state with …

2015

A measurement is presented of the (tt) over bar inclusive production cross section in pp collisions at a center-ofmass energy of pffisffiffi root s = 8 TeV using data collected by the ATLAS detector at the CERN Large Hadron Collider. The measurement was performed in the lepton + jets final state using a data set corresponding to an integrated luminosity of 20.3 fb(-1). The cross section was obtained using a likelihood discriminant fit and b-jet identification was used to improve the signal-to-background ratio. The inclusive (tt) over bar production cross section was measured to be 260 +/- 1(stat)(-23)(+22)(stat) +/- 8(lumi) +/- 4(beam) pb assuming a top-quark mass of 172.5 GeV, in good agre…

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsAtlas (topology)Atlas detectorDetectorKinematics01 natural sciences7. Clean energyNuclear physicsPair production0103 physical sciencesHigh Energy Physics::Experiment010306 general physicsLeptonPhysical Review D
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Search for the Xb and other hidden-beauty states in the π+π−ϒ(1S) channel at ATLAS

2015

This Letter presents a search for a hidden-beauty counterpart of the X(3872) in the mass ranges 10.05--10.31 GeV and 10.40--11.00 GeV, in the channel Xb→π+π−Υ(1S)(→μ+μ−), using 16.2 fb−1 of s√=8 TeV pp collision data collected by the ATLAS detector at the LHC. No evidence for new narrow states is found, and upper limits are set on the product of the Xb cross section and branching fraction, relative to those of the Υ(2S), at the 95% confidence level using the CLS approach. These limits range from 0.8% to 4.0%, depending on mass. For masses above 10.1 GeV, the expected upper limits from this analysis are the most restrictive to date. Searches for production of the Υ(13DJ), Υ(10860), and Υ(110…

Nuclear physicsPhysicsNuclear and High Energy PhysicsPionLarge Hadron Collidermedicine.anatomical_structureChannel (digital image)MesonBranching fractionAtlas (anatomy)medicineQuarkoniumX(3872)Physics Letters B
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Deep-learning based reconstruction of the shower maximum X max using the water-Cherenkov detectors of the Pierre Auger Observatory

2021

The atmospheric depth of the air shower maximum $X_{\mathrm{max}}$ is an observable commonly used for the determination of the nuclear mass composition of ultra-high energy cosmic rays. Direct measurements of $X_{\mathrm{max}}$ are performed using observations of the longitudinal shower development with fluorescence telescopes. At the same time, several methods have been proposed for an indirect estimation of $X_{\mathrm{max}}$ from the characteristics of the shower particles registered with surface detector arrays. In this paper, we present a deep neural network (DNN) for the estimation of $X_{\mathrm{max}}$. The reconstruction relies on the signals induced by shower particles in the groun…

showers: energylongitudinal [showers]interaction: modelPhysics::Instrumentation and DetectorsAstronomyCalibration and fitting methods; Cluster finding; Data analysis; Large detector systems for particle and astroparticle physics; Particle identification methods; Pattern recognition01 natural sciencesHigh Energy Physics - ExperimentAugerHigh Energy Physics - Experiment (hep-ex)Particle identification methodscluster findingsurface [detector]ObservatoryLarge detector systemsInstrumentationMathematical PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEPhysicsPattern recognition cluster finding calibration and fitting methodsPhysicsSettore FIS/01 - Fisica Sperimentalemodel [interaction]DetectorAstrophysics::Instrumentation and Methods for AstrophysicsData analysicalibration and fitting methodsenergy [showers]AugerobservatoryPattern recognition cluster finding calibration and fitting methodastroparticle physicsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomenaatmosphere [showers]airneural networkAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]Data analysisFOS: Physical sciences610Cosmic raydetector: fluorescencePattern recognition0103 physical sciencesddc:530High Energy Physicsddc:610[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]cosmic radiation: UHEstructureparticle physicsnetwork: performance010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Ciencias ExactasCherenkov radiationfluorescence [detector]Pierre Auger ObservatoryCalibration and fitting methodsmass spectrum [nucleus]showers: atmospheredetector: surfacehep-ex010308 nuclear & particles physicsLarge detector systems for particle and astroparticle physicsCluster findingFísicaresolutioncalibrationComputational physicsperformance [network]Cherenkov counterAir showerLarge detector systems for particle and astroparticle physicExperimental High Energy PhysicsHigh Energy Physics::Experimentnucleus: mass spectrumshowers: longitudinalRAIOS CÓSMICOSEnergy (signal processing)astro-ph.IM
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Evidence ofWγγProduction inppCollisions ats=8  TeVand Limits on Anomalous Quartic Gauge Couplings with the ATLAS Detector

2015

This Letter reports evidence of triple gauge boson production pp -> W(l nu)gamma gamma + X, which is accessible for the first time with the 8 TeV LHC data set. The fiducial cross section for this process is measured in a data sample corresponding to an integrated luminosity of 20.3 fb(-1), collected by the ATLAS detector in 2012. Events are selected using the W boson decay to e nu or mu nu as well as requiring two isolated photons. The measured cross section is used to set limits on anomalous quartic gauge couplings in the high diphoton mass region.

Quantum chromodynamicsPhysicsParticle physicsGauge bosonMuonLuminosity (scattering theory)Large Hadron ColliderPhotonHigh Energy Physics::PhenomenologyElectroweak interactionGeneral Physics and AstronomyNuclear physicsmedicine.anatomical_structureAtlas (anatomy)medicinePhysical Review Letters
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Measurement of the cross section of high transverse momentumZ→bb¯production in proton–proton collisions ats=8 TeVwith the ATLAS detector

2014

This Letter reports the observation of a high transverse momentum Z -> b (b) over bar signal in proton-proton collisions at root s = 8TeVand the measurement of its production cross section. The data analysed were collected in 2012 with the ATLAS detector at the LHC and correspond to an integrated luminosity of 19.5 fb(-1). The Z -> b (b) over bar decay is reconstructed from a pair of b-tagged jets, clustered with the anti- k(t) jet algorithm with R = 0.4, that have low angular separation and form a dijet with p(T) > 200 GeV. The signal yield is extracted from a fit to the dijet invariant mass distribution, with the dominant, multi-jet background mass shape estimated by employing a fully dat…

PhysicsNuclear and High Energy PhysicsJet (fluid)Particle physicsLuminosity (scattering theory)Large Hadron ColliderProton010308 nuclear & particles physicsAngular distance01 natural sciencesNuclear physicsCross section (physics)0103 physical sciencesHigh Energy Physics::ExperimentInvariant mass010306 general physicsBar (unit)Physics Letters B
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Multi-resolution anisotropy studies of ultrahigh-energy cosmic rays detected at the Pierre Auger Observatory

2017

We report a multi-resolution search for anisotropies in the arrival directions of cosmic rays detected at the Pierre Auger Observatory with local zenith angles up to $80^\circ$ and energies in excess of 4 EeV ($4 \times 10^{18}$ eV). This search is conducted by measuring the angular power spectrum and performing a needlet wavelet analysis in two independent energy ranges. Both analyses are complementary since the angular power spectrum achieves a better performance in identifying large-scale patterns while the needlet wavelet analysis, considering the parameters used in this work, presents a higher efficiency in detecting smaller-scale anisotropies, potentially providing directional informa…

moment: dipoleAstronomy[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic ray experiments; ultra high energy cosmic rays; Astronomy and AstrophysicsCosmic rayanisotropyultra high energy cosmic raysSURFACE DETECTOR01 natural sciencesLARGE-SCALE DISTRIBUTIONwaveletSEARCH0103 physical sciencesARRIVAL DIRECTIONSHigh Energy Physicscosmic radiation: UHEAnisotropy010303 astronomy & astrophysicsZenithHigh Energy Astrophysical Phenomena (astro-ph.HE)Pierre Auger ObservatoryPhysicsSPECTRUM010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleSpectral densityAstronomy and AstrophysicsEEVASTROFÍSICAComputational physicsAugerCosmic ray experiments; ultra high energy cosmic raysobservatoryDipolecosmic ray experiments ultra high energy cosmic raysRESOLUTIONMoment (physics)Experimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGpower spectrum: angular dependenceARRAYcosmic ray experimentsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)
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Measurement of inclusive jet charged-particle fragmentation functions in Pb+Pb collisions at sNN=2.76 TeV with the ATLAS detector

2014

Measurements of charged-particle fragmentation functions of jets produced in ultra-relativistic nuclear collisions can provide insight into the modification of parton showers in the hot, dense medi ...

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderAtlas detectorAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryPartonCharged particleNuclear physicsFragmentation (mass spectrometry)High Energy Physics::ExperimentImpact parameterNuclear ExperimentPhysics Letters B
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A search for point sources of EeV neutrons

2012

A thorough search of the sky exposed at the Pierre Auger Cosmic Ray Observatory reveals no statistically significant excess of events in any small solid angle that would be indicative of a flux of neutral particles from a discrete source. The search covers from −90◦ to +15◦ in declination using four different energy ranges above 1 EeV (1018 eV). The method used in this search is more sensitive to neutrons than to photons. The upper limit on a neutron flux is derived for a dense grid of directions for each of the four energy ranges. These results constrain scenarios for the production of ultrahigh energy cosmic rays in the Galaxy.

AstronomyEnergy fluxAstrophysics01 natural sciences7. Clean energyNeutron fluxObservatorycosmic rays – Galaxy: disk – methods: data analysisNeutron detection010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Gamma rayAstrophysics::Instrumentation and Methods for AstrophysicsASTRONOMYPierre Auger ObservatoryCOSMIC-RAYSRadiación cósmicaUltra High Energy Cosmic RayComputingMethodologies_DOCUMENTANDTEXTPROCESSINGMASSIVE BLACK-HOLEFísica nuclearPierre Auger Observatory high-energy neutron sources neutron flux limitAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayGalaxiaGalaxy: diskcosmic rays0103 physical scienceshigh-energy neutron sourcesNeutronCosmic-ray observatoryCiencias ExactasANISOTROPY010308 nuclear & particles physicsGAMMA-RAYSAnálisis de datosAstronomyFísicaAstronomy and AstrophysicsASTROFÍSICAneutron flux limitmethods: data analysisNÊUTRONSSpace and Planetary ScienceUltra High Energy Cosmic RaysExperimental High Energy Physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]GALACTIC-CENTER
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Search for Dark Matter in Events with a Hadronically DecayingWorZBoson and Missing Transverse Momentum inppCollisions ats=8  TeVwith the ATLAS Detect…

2014

A search is presented for dark matter pair production in association with a W or Z boson in pp collisions representing 20.3 fb(-1) of integrated luminosity at root s = 8 TeV using data recorded with the ATLAS detector at the Large Hadron Collider. Events with a hadronic jet with the jet mass consistent with a W or Z boson, and with large missing transverse momentum are analyzed. The data are consistent with the standard model expectations. Limits are set on the mass scale in effective field theories that describe the interaction of dark matter and standard model particles, and on the cross section of Higgs production and decay to invisible particles. In addition, cross section limits on the…

PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsAtlas (topology)High Energy Physics::PhenomenologyHadronDark matterGeneral Physics and Astronomy01 natural sciencesNuclear physicsPair production0103 physical sciencesEffective field theoryHiggs bosonHigh Energy Physics::Experiment010306 general physicsBosonPhysical Review Letters
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Search for new phenomena in events with a photon and missing transverse momentum inppcollisions ats=8  TeVwith the ATLAS detector

2015

© 2015 CERN. © 2015 CERN, for the ATLAS Collaboration. Published by the American Physical Society under the terms of the »http://creativecommons.org/licenses/by/3.0/» Creative Commons Attribution 3.0 License. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. Results of a search for new phenomena in events with an energetic photon and large missing transverse momentum with the ATLAS experiment at the LHC are reported. Data were collected in proton-proton collisions at a center-of-mass energy of 8 TeV and correspond to an integrated luminosity of 20.3 fb-1. The observed data are well described by the expe…

PhysicsQuarkNuclear and High Energy PhysicsParticle physicsPhotonLarge Hadron Collider010308 nuclear & particles physicsAtlas (topology)ATLAS experimentDark matterSupersymmetry01 natural sciences7. Clean energyNuclear physicsPair production0103 physical sciencesHigh Energy Physics::Experiment010306 general physicsPhysical Review D
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Search for the neutral Higgs bosons of the Minimal Supersymmetric Standard Model in $pp$ collisions at $\sqrt{s}=7$ TeV with the ATLAS detector

2013

A search for neutral Higgs bosons of the Minimal Supersymmetric Standard Model (MSSM) is reported. The analysis is based on a sample of proton-proton collisions at a centre-of-mass energy of 7 TeV recorded with the ATLAS detector at the Large Hadron Collider. The data were recorded in 2011 and correspond to an integrated luminosity of 4.7 fb[superscript −1] to 4.8 fb[superscript −1]. Higgs boson decays into oppositely-charged muon or τ lepton pairs are considered for final states requiring either the presence or absence of b-jets. No statistically significant excess over the expected background is observed and exclusion limits at the 95% confidence level are derived. The exclusion limits ar…

7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Naturvetenskap[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]SUPERSYMMETRYQCBosonPhysicsLarge Hadron ColliderSettore FIS/01 - Fisica SperimentaleSupersymmetryATLASmedicine.anatomical_structureComputingMethodologies_DOCUMENTANDTEXTPROCESSINGHiggs bosonLHCNatural SciencesParticle Physics - ExperimentParticle physicsNuclear and High Energy PhysicsCiências Naturais::Ciências Físicas530 PhysicsHiggs boson:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesddc:500.2530Nuclear physicsAtlas (anatomy)0103 physical sciencesmedicineddc:530High Energy Physics010306 general physicsCiencias ExactasHadron-Hadron scattering; Nuclear and High Energy PhysicsMuonScience & TechnologyHadron-Hadron ScatteringATLAS detector010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaHadron-Hadron scatteringHADRON-HADRON COLLISIONSExperimental High Energy PhysicsHigh Energy Physics::ExperimentMinimal Supersymmetric Standard ModelLepton
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Constraints on the origin of cosmic rays above 10^18 eV from large-scale anisotropy searches in data of the Pierre Auger Observatory

2012

A thorough search for large-scale anisotropies in the distribution of arrival directions of cosmic rays detected above 10(18) eV at the Pierre Auger Observatory is reported. For the first time, these large-scale anisotropy searches are performed as a function of both the right ascension and the declination and expressed in terms of dipole and quadrupole moments. Within the systematic uncertainties, no significant deviation from isotropy is revealed. Upper limits on dipole and quadrupole amplitudes are derived under the hypothesis that any cosmic ray anisotropy is dominated by such moments in this energy range. These upper limits provide constraints on the production of cosmic rays above 10(…

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]AstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysics01 natural sciencesMAGNETIC-FIELDScosmic raysObservatory0103 physical sciencesUltra-high-energy cosmic rayAnisotropyastroparticle physics – cosmic rays010303 astronomy & astrophysicsCiencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)Pierre Auger ObservatoryAstroparticle physicsPhysicsCOSMIC cancer database010308 nuclear & particles physicsOBSERVATÓRIOS[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsAstronomyastroparticle physicFísicaAstronomy and AstrophysicsRadiación cósmica13. Climate actionSpace and Planetary Scienceastroparticle physicsExperimental High Energy PhysicsQuadrupoleComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica de partículasFísica nuclearAstroparticle physicsAstrophysics - High Energy Astrophysical Phenomena
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Search for a multi-Higgs-boson cascade inW+W−bb¯events with the ATLAS detector inppcollisions ats=8  TeV

2014

A search is presented for new particles in an extension to the Standard Model that includes a heavy Higgs boson (H-0), an intermediate charged Higgs-boson pair (H-+/-), and a light Higgs boson (h(0)). The analysis searches for events involving the production of a single heavy neutral Higgs boson which decays to the charged Higgs boson and a W boson, where the charged Higgs boson subsequently decays into a W boson and the lightest neutral Higgs boson decaying to a bottom-antibottom-quark pair. Such a cascade results in a W-boson pair and a bottom-antibottom-quark pair in the final state. Events with exactly one lepton, missing transverse momentum, and at least four jets are selected from a d…

Condensed Matter::Quantum GasesQuarkPhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderBranching fractionHigh Energy Physics::PhenomenologySupersymmetry7. Clean energyCharged particleNuclear physicsPair productionHiggs bosonHigh Energy Physics::ExperimentLeptonPhysical Review D
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Ultra-High Energy Neutrinos at the Pierre Auger Observatory

2013

The observation of ultrahigh energy neutrinos (UHE nu s) has become a priority in experimental astroparticle physics. UHE nu s can be detected with a variety of techniques. In particular, neutrinos can interact in the atmosphere (downward-going nu) or in the Earth crust (Earth-skimming nu), producing air showers that can be observed with arrays of detectors at the ground. With the surface detector array of the Pierre Auger Observatory we can detect these types of cascades. The distinguishing signature for neutrino events is the presence of very inclined showers produced close to the ground (i.e., after having traversed a large amount of atmosphere). In this work we review the procedure and …

ultra high energy neutrino[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and DetectorsCiencias FísicasAstronomyFluxAstrophysics7. Clean energy01 natural sciencesAltas energíasAuger//purl.org/becyt/ford/1 [https]surface [detector]ObservatoryneutriniCosmic-rayscosmic rayHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCascada atmosférica extensaOBSERVATÓRIOS[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsneutrino; Augerlcsh:QC1-999AugercascadeUHE [neutrino]observatoryPhysics::Space PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearultra high energy neutrinosNeutrinoAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTASsignatureTAU-NEUTRINOSatmosphere [showers]FLUXNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Article SubjectairAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayFísica de Partículas y CamposLIMITPartícules (Física nuclear)Ultra high energy cosmic rayAtmosphere[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Air-showersSEARCHNeutrino0103 physical sciencesddc:530010306 general physicsAstrophysiqueCiencias ExactasPierre Auger ObservatoryAstroparticle physicsSPECTRUM010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaUltra high energy cosmic raystelescopes//purl.org/becyt/ford/1.3 [https]Ultrahigh Energyflux13. Climate actionenergy [neutrino]Pierre AugerExperimental High Energy PhysicsARRAYHigh Energy Physics::ExperimentAstroparticle physicslcsh:Physics
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Measurement of the transverse polarization ofΛandΛ¯hyperons produced in proton-proton collisions ats=7  TeVusing the ATLAS detector

2015

The transverse polarization of Λ and Λ¯ hyperons produced in proton-proton collisions at a center-of-mass energy of 7 TeV is measured. The analysis uses 760  μb−1 of minimum bias data collected by the ATLAS detector at the LHC in the year 2010. The measured transverse polarization averaged over Feynman xF from 5×10−5 to 0.01 and transverse momentum pT from 0.8 to 15 GeV is −0.010±0.005(stat)±0.004(syst) for Λ and 0.002±0.006(stat)±0.004(syst) for Λ¯. It is also measured as a function of xF and pT, but no significant dependence on these variables is observed. Prior to this measurement, the polarization was measured at fixed-target experiments with center-of-mass energies up to about 40 GeV. …

PhysicsQuantum chromodynamicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderExtrapolationHyperonParticle acceleratorPolarization (waves)7. Clean energylaw.inventionNuclear physicssymbols.namesakeTransverse planelawsymbolsFeynman diagramHigh Energy Physics::ExperimentNuclear ExperimentPhysical Review D
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Search for Scalar Charm Quark Pair Production inppCollisions ats=8  TeVwith the ATLAS Detector

2015

The results of a dedicated search for pair production of scalar partners of charm quarks are reported. The search is based on an integrated luminosity of 20.3 fb(-1) of pp collisions at root s = 8 TeV recorded with the ATLAS detector at the LHC. The search is performed using events with large missing transverse momentum and at least two jets, where the two leading jets are each tagged as originating from c quarks. Events containing isolated electrons or muons are vetoed. In an R-parity-conserving minimal super-symmetric scenario in which a single scalar-charm state is kinematically accessible, and where it decays exclusively into a charm quark and a neutralino, 95% confidence-level upper li…

QuarkPhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyGeneral Physics and Astronomy7. Clean energy01 natural sciencesCharm quarkNuclear physicsmedicine.anatomical_structurePair productionPionAtlas (anatomy)0103 physical sciencesNeutralinomedicineHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsMinimal Supersymmetric Standard ModelPhysical Review Letters
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Interpretation of the depths of maximum of extensive air showers measured by the Pierre Auger Observatory

2013

To interpret the mean depth of cosmic ray air shower maximum and its dispersion, we parametrize those two observables as functions of the first two moments of the ln A distribution. We examine the goodness of this simple method through simulations of test mass distributions. The application of the parameterization to Pierre Auger Observatory data allows one to study the energy dependence of the mean ln A and of its variance under the assumption of selected hadronic interaction models. We discuss possible implications of these dependences in term of interaction models and astrophysical cosmic ray sources.

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Ciencias FísicasAstronomyAstrophysics::High Energy Astrophysical PhenomenaHadronFOS: Physical sciencesCosmic rayultra high energy cosmic rays01 natural sciencesultra high energy cosmic rayInterpretation (model theory)//purl.org/becyt/ford/1 [https]Nuclear physics0103 physical sciencesPARTICLES010306 general physicsDispersion (water waves)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatoryCOMPOSICIÓN DE MASAEXPERIMENTO AUGER010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsObservableASTROFÍSICA//purl.org/becyt/ford/1.3 [https]RAYOS COSMICOSAstronomíaENERGY COSMIC-RAYSMODELDistribution (mathematics)Air showerParticlesUltra High Energy Cosmic RaysExperimental High Energy PhysicsSIMULATIONComputingMethodologies_DOCUMENTANDTEXTPROCESSINGEnergy cosmic-raysFísica nuclearcosmic ray experimentsAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTASSimulationcosmic ray experiments; ultra high energy cosmic raysModel
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A neural network clustering algorithm for the ATLAS silicon pixel detector

2014

A novel technique to identify and split clusters created by multiple charged particles in the ATLAS pixel detector using a set of artificial neural networks is presented. Such merged clusters are a common feature of tracks originating from highly energetic objects, such as jets. Neural networks are trained using Monte Carlo samples produced with a detailed detector simulation. This technique replaces the former clustering approach based on a connected component analysis and charge interpolation. The performance of the neural network splitting technique is quantified using data from proton-proton collisions at the LHC collected by the ATLAS detector in 2011 and from Monte Carlo simulations. …

Physics::Instrumentation and DetectorsCiencias FísicasMonte Carlo methodHigh Energy Physics - Experiment//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)jetParticle tracking detectors[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]scattering [p p]Statistical physicscluster [track data analysis]Particle tracking detectors (solid-state detectors)InstrumentationQCMathematical PhysicsPhysicsArtificial neural networkAtlas (topology)Detectordetectors)Monte Carlo [numerical calculations]ATLASperformance [neural network]CERN LHC CollParticle tracking detectors (Solid-state detectors)Feature (computer vision)Physical SciencesParticle tracking detectors (Solid-stateParticle tracking detectors; Particle tracking detectors (Solid-state detectors)ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGLHCConnected-component labelingAlgorithmNeural networksCIENCIAS NATURALES Y EXACTASParticle Physics - ExperimentInterpolationCiências Naturais::Ciências Físicas530 Physicssplitting:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesParticle tracking detectors; Particle tracking detectors (solid-state detectors); Instrumentation; Mathematical Physics530FysikHigh Energy Physicsddc:610Cluster analysispixel [semiconductor detector]Science & TechnologyFísica//purl.org/becyt/ford/1.3 [https]High Energy Physics - Experiment; High Energy Physics - ExperimentParticle tracking detectorcluster [charged particle]AstronomíaParticle tracking detectors; Particle tracking detectors (Solid-state; detectors)Experimental High Energy Physicsimpact parameter [resolution]
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Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger Observatory

2021

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargue. We are very grateful to the following agencies and organizations for financial support: Argentina -Comision Nacional de Energia Atomica; Agencia Nacional de Promocion Cientifica y Tecnologica (ANPCyT); Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET); Gobierno de la Provincia de Mendoza; Municipalidad de Malargue; NDM Holdings and Valle Las Lenas; in gratitude for their continuing cooperation over land access; Australia -the Australian Research Council; Braz…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsAstronomyPerformance of High Energy Physics Detector01 natural sciences7. Clean energyEtc)030218 nuclear medicine & medical imaging0302 clinical medicineFront-end electronics for detector readoutAPDsInstrumentationphysics.ins-detPhoton detectors for UVMathematical PhysicsInstrumentation et méthodes en physiqueEBCCDsVisible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc)electronicsSettore FIS/01 - Fisica SperimentaleCalibration and fitting methods; Performance of High Energy Physics Detectors; Photon detectors for UVPhoton detectors for UV visible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc)Astrophysics::Instrumentation and Methods for AstrophysicsSi-PMTsInstrumentation and Detectors (physics.ins-det)charged particleAPDs; Calibration and fitting methods; Performance of High Energy Physics Detectors; Photon detectors for UV; CCDs; Cluster finding; CMOS imagers; EBCCDs; EMCCDs; Etc); Front-end electronics for detector readout; Pattern recognition; G-APDs; Si-PMTs; Visible and IR photons (solid-state) (PIN diodesAugerobservatorydensity [muon]Pattern recognition cluster finding calibration and fitting methodG-APDsChristian ministryupgradeddc:620Astrophysics - Instrumentation and Methods for Astrophysicsperformanceatmosphere [showers]Land accessCherenkov counter: waterairAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencesVisible and IR photons (solid-state) (PIN diodes03 medical and health sciencesPolitical sciencePattern recognition0103 physical sciencesmuon: densityFront-end electronics for detector readout; Pattern recognitionphotomultiplier: siliconHigh Energy Physicscosmic radiation: UHE[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]ddc:610CMOS imagersInstrumentation and Methods for Astrophysics (astro-ph.IM)Engineering & allied operationsscintillation counterCalibration and fitting methodsshowers: atmosphere010308 nuclear & particles physicswater [Cherenkov counter]Cluster findingAutres mathématiquesCCDsEMCCDsResearch councilefficiencyExperimental High Energy Physicssilicon [photomultiplier]Performance of High Energy Physics DetectorsHigh Energy Physics::ExperimentHumanitiesRAIOS CÓSMICOSastro-ph.IM
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A 3-Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic-Ray Observatory

2020

The time and location of the 1,598 verified and reconstructed elves, used for the analysis showcased in this paper, are publicly available on the website of the Pierre Auger Observatory (https://www.auger.org/ index.php/science/data). We wish to thank the World Wide Lightning Location Network (http://wwlln.net), a collaboration among over 50 universities and institutions, for providing the lightning location data used in this paper. We acknowledge Robert Marshall for providing one of the most advanced elve simulations to the public, a key tool in understanding the elves observed by the Pierre Auger Observatory. The successful installation, commissioning, and operation of the Pierre Auger Ob…

010504 meteorology & atmospheric sciencesAstronomyField of view010502 geochemistry & geophysics01 natural sciences7. Clean energyAugerlcsh:QB1-991ObservatoryultravioletStormddc:550UHE Cosmic Raystime resolutionCosmic-ray observatoryPhysicslcsh:QE1-996.5astro-ph.GeologyAugerwidth [beam]IonosphereField of viewGeologylcsh:AstronomyUHE [cosmic radiation]Environmental Science (miscellaneous)horizonLightningddc:530High Energy PhysicsIonosphereCosmic-ray observatory0105 earth and related environmental sciencesfluorescence [detector]backgroundFísicaAstronomyStormsensitivityLightningopticslcsh:GeologyElves UV fluorescence detectorsThunderstorm13. Climate actionExperimental High Energy PhysicsnetworkThunderstormGeneral Earth and Planetary SciencesElvesObservatory
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Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory

2019

Neutrinos with energies above 1017 eV are detectable with the Surface Detector Array of the Pierre Auger Observatory. The identification is efficiently performed for neutrinos of all flavors interacting in the atmosphere at large zenith angles, as well as for Earth-skimming τ neutrinos with nearly tangential trajectories relative to the Earth. No neutrino candidates were found in ∼ 14.7 years of data taken up to 31 August 2018. This leads to restrictive upper bounds on their flux. The 90% C.L. single-flavor limit to the diffuse flux of ultra-high-energy neutrinos with an Eν -2 spectrum in the energy range 1.0 × 1017 eV -2.5 × 1019 eV is E2 dNν/dEν < 4.4 × 10-9 GeV cm-2 s-1 sr-1, placing str…

cosmological neutrinosAstronomyFluxAstrophysics01 natural sciences7. Clean energycosmic ray experiments; cosmological neutrinos; neutrino astronomy; ultra high energy cosmic rayssurface [detector]Ultra-high-energy cosmic rayPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)cosmological neutrinoSettore FIS/01 - Fisica SperimentaleDETETORESneutrino: UHEUHE [neutrino]Augerobservatorytrajectoryneutrino: flavorProduction (computer science)NeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencescosmic ray experimentCosmic rayultra high energy cosmic raysneutrino: productionneutrino astronomyproduction [neutrino]TheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITY0103 physical sciencesddc:530model [neutrino]High Energy Physicscosmic radiation: UHEZenithAstrophysiqueneutrino: modelPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsdetector: surfaceHigh Energy Physics::Phenomenologyflavor [neutrino]Astronomy and AstrophysicsAstronomiefluxExperimental High Energy PhysicsatmosphereHigh Energy Physics::Experimentcosmic ray experiments[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)
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Large-scale Cosmic-Ray Anisotropies above 4 EeV Measured by the Pierre Auger Observatory

2018

We present a detailed study of the large-scale anisotropies of cosmic rays with energies above 4 EeV measured using the Pierre Auger Observatory. For the energy bins [4,8] EeV and $E\geq 8$ EeV, the most significant signal is a dipolar modulation in right ascension at energies above 8 EeV, as previously reported. In this paper we further scrutinize the highest-energy bin by splitting it into three energy ranges. We find that the amplitude of the dipole increases with energy above 4 EeV. The growth can be fitted with a power law with index $\beta=0.79\pm 0.19$. The directions of the dipoles are consistent with an extragalactic origin of these anisotropies at all the energies considered. Addi…

Astronomymagnetic fieldAstrophysicsAstrophysics01 natural sciencesAmplitudeastroparticle physics; cosmic raysAnisotropy010303 astronomy & astrophysicscosmic rayastroparticle physics cosmic raysRight ascensionHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HECOSMIC cancer databaseORIGINOBSERVATÓRIOSPhysicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsastroparticle physicAugerastroparticle physics; cosmic rays; Astronomy and Astrophysics; Space and Planetary ScienceobservatorymodulationAmplitudeastroparticle physicsCosmic cancer databaseAstrophysics - High Energy Astrophysical Phenomenalarge scale anysotropysplittingAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayContext (language use)cosmic radiation: anisotropycosmic rays0103 physical sciencesHigh Energy Physicscosmic radiation: UHEPierre auger observatoryPierre Auger Observatoryextragalactic origin010308 nuclear & particles physicsFísicaAstronomy and AstrophysicsContext (language use)Astronomy and AstrophysicCosmic rayDipoleSpace and Planetary ScienceExperimental High Energy PhysicsAnisotropyDipoleObservatoryAstroparticle physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Right ascensionlarge scale anysotropy extragalactic origindipole
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Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory

2016

Ultrahigh energy cosmic ray air showers probe particle physics at energies beyond the reach of accelerators. Here we introduce a new method to test hadronic interaction models without relying on the absolute energy calibration, and apply it to events with primary energy 6-16 EeV (ECM=110-170 TeV), whose longitudinal development and lateral distribution were simultaneously measured by the Pierre Auger Observatory. The average hadronic shower is 1.33±0.16 (1.61±0.21) times larger than predicted using the leading LHC-tuned models EPOS-LHC (QGSJetII-04), with a corresponding excess of muons.

Hadronic interaction[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Particle physicsCOLLISIONSAstronomyAstrophysics::High Energy Astrophysical PhenomenaHadronFOS: Physical sciencesGeneral Physics and AstronomyCosmic ray01 natural sciences7. Clean energyHigh Energy Physics - ExperimentAugerHigh Energy Physics - Experiment (hep-ex)Physics and Astronomy (all)High Energy Physics - Phenomenology (hep-ph)Observatory0103 physical sciencesCalibrationHigh Energy PhysicsUHE Cosmic Rays010306 general physicsParticle PhysicsCosmic raysGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatoryEnergyMuon010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsFísicaInteraction modelASTROFÍSICAHigh Energy Physics - Phenomenology13. Climate actionExperimental High Energy PhysicsHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical Phenomena
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The Lateral Trigger Probability function for the Ultra-High Energy Cosmic Ray Showers detected by the Pierre Auger Observatory

2011

In this paper we introduce the concept of Lateral Trigger Probability (LTP) function, i.e., the probability for an Extensive Air Shower (EAS) to trigger an individual detector of a ground based array as a function of distance to the shower axis, taking into account energy, mass and direction of the primary cosmic ray. We apply this concept to the surface array of the Pierre Auger Observatory consisting of a 1.5 km spaced grid of about 1600 water Cherenkov stations. Using Monte Carlo simulations of ultra-high energy showers the LTP functions are derived for energies in the range between 1017 and 1019 eV and zenith angles up to 65. A parametrization combining a step function with an exponenti…

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AstronomyAstrophysics::High Energy Astrophysical PhenomenaExtensive air showerUltra-high Energy Cosmic RayMonte Carlo methodFOS: Physical sciencesCosmic rayEXTENSIVE AIR-SHOWERSTrigger performance01 natural sciences7. Clean energyUltra-high Energy Cosmic Rays; Pierre Auger Observatory; Extensive air showers; Trigger performance; Surface detector; Hybrid detectorHigh Energy Physics - ExperimentAugerNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesUltra-high-energy cosmic ray010303 astronomy & astrophysicsCiencias ExactasZenithCherenkov radiationUltra-High Energy Cosmic RaysPhysicsPierre Auger ObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsPhysicsHybrid detector[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Surface detectorAstrophysics::Instrumentation and Methods for AstrophysicsFísicaAstronomy and AstrophysicsPierre Auger ObservatoryUltra-high Energy Cosmic Rays[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Air showerExperimental High Energy PhysicsSIMULATIONComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearExtensive Air ShowersAstrophysics - High Energy Astrophysical PhenomenaRAIOS CÓSMICOS
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Measurement of angular correlations in Drell–Yan lepton pairs to probe Z/γ⁎ boson transverse momentum at s=7 TeV with the ATLAS detector

2013

A measurement of angular correlations in Drell-Yan lepton pairs via the phi(eta)* observable is presented. This variable probes the same physics as the Z/gamma* boson transverse momentum with a better experimental resolution. The Z/gamma* -> e(+)e(-) and Z/gamma* -> mu(+)mu(-) decays produced in proton-proton collisions at a centre-of-mass energy of root s = 7 TeV are used. The data were collected with the ATLAS detector at the LHC and correspond to an integrated luminosity of 4.6 fb(-1). Normalised differential cross sections as a function of phi(eta)* are measured separately for electron and muon decay channels. These channels are then combined for improved accuracy. The cross section is …

PhysicsQuantum chromodynamicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderMuon010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyPerturbative QCDDrell–Yan process01 natural sciences7. Clean energyNuclear physics0103 physical sciencesHigh Energy Physics::ExperimentRapidity010306 general physicsLeptonBosonPhysics Letters B
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Limits on point-like sources of ultra-high-energy neutrinos with the Pierre Auger Observatory

2019

With the Surface Detector array (SD) of the Pierre Auger Observatory we can detect neutrinos with energy between 1017 eV and 1020 eV from point-like sources across the sky, from close to the Southern Celestial Pole up to 60 in declination, with peak sensitivities at declinations around ∼-53 and ∼+55, and an unmatched sensitivity for arrival directions in the Northern hemisphere. A search has been performed for highly-inclined air showers induced by neutrinos of all flavours with no candidate events found in data taken between 1 Jan 2004 and 31 Aug 2018. Upper limits on the neutrino flux from point-like steady sources have been derived as a function of source declination. An unrivaled sensit…

cosmological neutrinosAstronomypoleFluxAstrophysics01 natural sciencesneutrino: fluxcosmic ray experiments; cosmological neutrinos; neutrino astronomy; ultra high energy cosmic raysmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)AIR-SHOWERSastro-ph.HEcosmological neutrinoSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsCOSMIC-RAYSneutrino: UHEAugerobservatoryNEUTRINOSNeutrinoAstrophysics - High Energy Astrophysical Phenomenaairmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical Phenomenacosmic ray experimentFOS: Physical sciencesultra high energy cosmic raysDeclinationneutrino astronomyCelestial pole0103 physical sciencesflux: upper limitHigh Energy PhysicsDETECTORZenithAstrophysiquePierre Auger Observatoryflavorshowers: atmosphere010308 nuclear & particles physicsdetector: surfaceNorthern HemisphereAstronomy and AstrophysicsAstronomiesensitivitySkyExperimental High Energy PhysicsHigh Energy Physics::Experimentcosmic ray experiments[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Techniques for measuring aerosol attenuation using the Central Laser Facility at the Pierre Auger Observatory

2013

The Pierre Auger Observatory in Malargue, Argentina, is designed to study the properties of ultra-high energy cosmic rays with energies above 10(18) eV. It is a hybrid facility that employs a Fluorescence Detector to perform nearly calorimetric measurements of Extensive Air Shower energies. To obtain reliable calorimetric information from the FD, the atmospheric conditions at the observatory need to be continuously monitored during data acquisition. In particular, light attenuation due to aerosols is an important atmospheric correction. The aerosol concentration is highly variable, so that the aerosol attenuation needs to be evaluated hourly. We use light from the Central Laser Facility, lo…

AstronomyDetector alignment and calibration methods (lasers sources particle-beams)01 natural sciencesDetector alignment and calibration methods (laserObservatoryATMOSPHERIC CONDITIONSDetector alignment and calibration methodsInstrumentationcosmic rayMathematical PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsatmospheric monitoring[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsData analysiparticle-beams)ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGCentral Laser FacilityFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomenasources[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]sourceAuger Experimentaerosols * Authors are listed on the following pagesData analysisFOS: Physical sciencesCosmic rayAuger Experiment; cosmic rays; atmospheric monitoring; aerosolsOpticscosmic raysUltra-high energy cosmic rays. atmospheric monitoring. aerosols0103 physical sciences010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Pierre Auger Observatory010308 nuclear & particles physicsbusiness.industryLarge detector systems for particle and astroparticle physicsAttenuationAtmospheric correctionUltra-high energy cosmic rays[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AerosolDetector alignment and calibration methods (lasersAir showerdetector alignment and calibration methods (lasers; sources; particle-beams); large detector systems for particle and astroparticle physics; data analysisExperimental High Energy PhysicsLarge detector systems for particle and astroparticle physicbusinessRAIOS CÓSMICOSaerosolsSYSTEM
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Identifying clouds over the Pierre Auger Observatory using infrared satellite data

2013

We describe a new method of identifying night-time clouds over the Pierre Auger Observatory using infrared data from the Imager instruments on the GOES-12 and GOES-13 satellites. We compare cloud. identifications resulting from our method to those obtained by the Central Laser Facility of the Auger Observatory. Using our new method we can now develop cloud probability maps for the 3000 km(2) of the Pierre Auger Observatory twice per hour with a spatial resolution of similar to 2.4 km by similar to 5.5 km. Our method could also be applied to monitor cloud cover for other ground-based observatories and for space-based observatories. (C) 2013 Elsevier B.V. All rights reserved.

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Atmospheric MonitoringSatellitesInfraredAstronomyCloud coverFOS: Physical sciencesAtmospheric monitoring01 natural sciencesCiencias de la Tierra y relacionadas con el Medio AmbienteAuger//purl.org/becyt/ford/1 [https]//purl.org/becyt/ford/1.5 [https]ObservatoryClouds0103 physical sciencesExtensive air showers010306 general physicsDETECTORInstrumentation and Methods for Astrophysics (astro-ph.IM)Image resolutionCiencias ExactasPhysicsPierre Auger ObservatoryUHE Cosmic Rays atmosphere010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FísicaAstronomyPierre Auger ObservatoryAstronomy and AstrophysicsUltra-high energy cosmic rays[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]INFRAVERMELHOExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGPierre Auger observatoryultra-high energy cosmic rays; Pierre Auger Observatory; extensive air showers; atmospheric monitoring; clouds; satellitesFísica nuclearSatelliteCentral Laser FacilityExtensive Air ShowersAstrophysics - Instrumentation and Methods for AstrophysicsMeteorología y Ciencias AtmosféricasSYSTEMCIENCIAS NATURALES Y EXACTASAstroparticle Physics
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Search for WH production with a light Higgs boson decaying to prompt electron-jets in proton–proton collisions at \(\sqrt {s}=7\)  TeV with the ATLAS…

2013

A search is performed for WH production with a light Higgs boson decaying to hidden-sector particles resulting in clusters of collimated electrons, known as electron-jets. The search is performed with 2.04 fb[superscript −1] of data collected in 2011 with the ATLAS detector at the Large Hadron Collider in proton–proton collisions at √s=7 TeV . One event satisfying the signal selection criteria is observed, which is consistent with the expected background rate. Limits on the product of the WH production cross section and the branching ratio of a Higgs boson decaying to prompt electron-jets are calculated as a function of a Higgs boson mass in the range from 100 to 140 GeV.

Standard ModelAtlas detectorGeneral Physics and AstronomyElectron7. Clean energy01 natural sciencesSignal selectionHigh Energy Physics - ExperimentLepton-JetsHigh Energy Physics - Experiment (hep-ex)Naturvetenskap[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentQCPhysicsddc:539Large Hadron ColliderSettore FIS/01 - Fisica SperimentaleSignal selectionBranching ratioATLASLarge Hadron ColliderComputingMethodologies_DOCUMENTANDTEXTPROCESSINGHiggs bosonLHCNatural SciencesParticle Physics - ExperimentParticle physics530 PhysicsCiências Naturais::Ciências FísicasHiggs bosonAstrophysics::High Energy Astrophysical Phenomena:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesddc:500.2530Collimated lightNuclear physics0103 physical sciencesddc:530High Energy Physics010306 general physicsW BOSONScience & TechnologyProton proton collisions010308 nuclear & particles physicsBranching fractionATLAS detectorsHigh Energy Physics::PhenomenologyFísicaMassEnergiesHidden sectorProduction cross sectionHiggs boson; electron-jets; proton–proton collisions; ATLAS detectorHADRON-HADRON COLLISIONSExperimental High Energy PhysicsHigh Energy Physics::Experiment
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Measurements of Higgs boson production and couplings in the four-lepton channel inppcollisions at center-of-mass energies of 7 and 8 TeV with the ATL…

2015

The final ATLAS Run 1 measurements of Higgs boson production and couplings in the decay channel H -> ZZ* -> l(+)l(-)l(+)l'(-), where l, l' = e or mu, are presented. These measurements were performed using pp collision data corresponding to integrated luminosities of 4.5 and 20.3 fb(-1) at center-of-mass energies of 7 and 8 TeV, respectively, recorded with the ATLAS detector at the LHC. The H -> ZZ* -> 4l signal is observed with a significance of 8.1 standard deviations, with an expectation of 6.2 standard deviations, at m(H) = 125.36 GeV, the combined ATLAS measurement of the Higgs boson mass from the H -> gamma gamma and H -> ZZ* -> 4l channels. The production rate relative to the Standard…

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::Phenomenology7. Clean energy01 natural sciencesGluonStandard ModelNuclear physicsmedicine.anatomical_structureAtlas (anatomy)0103 physical sciencesmedicineHiggs bosonHigh Energy Physics::ExperimentCenter of mass010306 general physicsLeptonBar (unit)Physical Review D
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Measurement of Higgs boson production in the diphoton decay channel inppcollisions at center-of-mass energies of 7 and 8 TeV with the ATLAS detector

2014

A measurement of the production processes of the recently discovered Higgs boson is performed in the two-photon final state using 4.5 fb(-1) of proton-proton collisions data at root s = 7 TeV and 20.3 fb(-1) at root s = 8 TeV collected by the ATLAS detector at the Large Hadron Collider. The number of observed Higgs boson decays to diphotons divided by the corresponding Standard Model prediction, called the signal strength, is found to be mu = 1.17 +/- 0.27 at the value of the Higgs boson mass measured by ATLAS, m(H) = 125.4 GeV. The analysis is optimized to measure the signal strengths for individual Higgs boson production processes at this value of m(H). They are found to be mu(ggF) = 1.32…

PhysicsNuclear and High Energy PhysicsParticle physicsPhotonLarge Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::Phenomenology7. Clean energy01 natural sciencesStandard ModelVector bosonGluonNuclear physicsmedicine.anatomical_structure13. Climate actionAtlas (anatomy)0103 physical sciencesHiggs bosonmedicineHigh Energy Physics::ExperimentCenter of mass010306 general physicsPhysical Review D
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Measurement of the high-mass Drell–Yan differential cross-section in pp collisions at s=7 TeV with the ATLAS detector

2013

This Letter reports a measurement of the high-mass Drell–Yan differential cross-section in proton–proton collisions at a centre-of-mass energy of 7 TeV at the LHC. Based on an integrated luminosity ...

Quantum chromodynamicsPhysicsScattering cross-sectionNuclear and High Energy PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsAtlas detectorNuclear TheoryHigh Energy Physics::PhenomenologyDrell–Yan process01 natural sciencesNuclear physics0103 physical sciencesTransverse momentumHigh massPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentRapidityNuclear Experiment010306 general physicsPhysics Letters B
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Search for Higgs andZBoson Decays toJ/ψγandϒ(nS)γwith the ATLAS Detector

2015

A search for the decays of the Higgs and Z bosons to J/psi gamma and Upsilon(nS)gamma (n = 1,2,3) is performed with pp collision data samples corresponding to integrated luminosities of up to 20.3 fb(-1) collected at root s = 8 TeV with the ATLAS detector at the CERN Large Hadron Collider. No significant excess of events is observed above expected backgrounds and 95% C.L. upper limits are placed on the branching fractions. In the J/psi gamma final state the limits are 1.5 x 10(-3) and 2.6 x 10(-6) for the Higgs and Z boson decays, respectively, while in the Upsilon(1S, 2S, 3S)gamma. final states the limits are (1.3, 1.9, 1.3) x 10(-3) and (3.4, 6.5, 5.4) x 10(-6), respectively.

PhysicsParticle physicsLarge Hadron ColliderPhoton010308 nuclear & particles physicsBranching fractionAtlas detectorAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyQuarkonium7. Clean energy01 natural sciences0103 physical sciencesHiggs bosonHigh Energy Physics::Experiment010306 general physicsTellurium compoundsBosonPhysical Review Letters
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Measurement of Top Quark Polarization in Top-Antitop Events from Proton-Proton Collisions ats=7  TeVUsing the ATLAS Detector

2013

This Letter presents measurements of the polarization of the top quark in top-antitop quark pair events, using 4: 7 fb(-1) of proton-proton collision data recorded with the ATLAS detector at the La ...

PhysicsTop quarkParticle physicsMuon010308 nuclear & particles physicsAtlas (topology)High Energy Physics::PhenomenologyNuclear TheoryGeneral Physics and AstronomyElectronPolarization (waves)01 natural sciencesNuclear physicsPair production0103 physical sciencesPhysics::Atomic and Molecular ClustersCP violationHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsLeptonPhysical Review Letters
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Measurement of Spin Correlation in Top-Antitop Quark Events and Search for Top Squark Pair Production inppCollisions ats=8  TeVUsing the ATLAS Detect…

2015

A measurement of spin correlation in t (t) over bar production is presented using data collected with the ATLAS detector at the Large Hadron Collider in proton-proton collisions at a center-of-mass ...

PhysicsQuarkParticle physicsLarge Hadron ColliderPhysics::Instrumentation and Detectors010308 nuclear & particles physicsNuclear TheoryTevatronGeneral Physics and AstronomySuperpartnerSupersymmetry01 natural sciencesNuclear physicsPair production0103 physical sciencesNeutralinoPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsLeptonPhysical Review Letters
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Probing the radio emission from air showers with polarization measurements

2014

The emission of radio waves from air showers has been attributed to the so-called geomagnetic emission process. At frequencies around 50 MHz this process leads to coherent radiation which can be observed with rather simple setups. The direction of the electric field induced by this emission process depends only on the local magnetic field vector and on the incoming direction of the air shower. We report on measurements of the electric field vector where, in addition to this geomagnetic component, another component has been observed which cannot be described by the geomagnetic emission process. The data provide strong evidence that the other electric field component is polarized radially wit…

SignalsAstronomy01 natural sciencesElectric fieldComputational physicsCosmic-raysComposition energy spectra and interactionscosmic rayRadio wavePhysicsEarth's magnetic fieldHigh Energy Astrophysical Phenomena (astro-ph.HE)Radiation[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsAstrophysics::Instrumentation and Methods for AstrophysicsPolarization (waves)Polarization (waves)BolometersThunderstormsMagnetic fieldComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaCAMPO MAGNÉTICOradio emissionRadio waveNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Air showerComposition energy spectra and interactions; Solar electromagnetic emission; BolometersAstrophysics::High Energy Astrophysical Phenomenainfrared submillimeter wave microwave and radiowave receivers and detectorsFieldFOS: Physical sciencesPierre Auger Observatory ; air shower ; radio emissionRadiationMonte-carlo SimulationsOpticsElectric field0103 physical sciencesddc:530Pierre auger observatory010306 general physicsPulsesInstrumentation and Methods for Astrophysics (astro-ph.IM)Pierre Auger Observatory010308 nuclear & particles physicsbusiness.industrySolar electromagnetic emissionFísicaOpticsDetectorComputational physics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Air showerEarth's magnetic fieldMagnetic fieldExperimental High Energy PhysicsbusinessCodalema
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Measurement of hard double-parton interactions inW(???) + 2-jet events at $\sqrt{s}\,=7$ TeV with the ATLAS detector

2013

The production of W bosons in association with two jets in proton–proton collisions at a centre-of-mass energy of √s=7 TeV has been analysed for the presence of double-parton interactions using data corresponding to an integrated luminosity of 36 pb[superscript −1], collected with the ATLAS detector at the Large Hadron Collider. The fraction of events arising from double-parton interactions, f[superscript (D) over subscript DP], has been measured through the p[subscript T] balance between the two jets and amounts to f[superscript (D) over subscript DP] = 0.08 ± 0.01 (stat.) ± 0.02 (sys.) for jets with transverse momentum p[subscript T] > 20 GeV and rapidity |y| < 2.8. This corresponds to a …

Hard-partonCiencias FísicasGeneral Physics and AstronomyParton7. Clean energy01 natural sciencesHigh Energy Physics - Experimentlaw.inventionVector bosonScattering//purl.org/becyt/ford/1 [https]law[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]w bosonNuclear ExperimentQCBosonddc:539PhysicsLuminosity (scattering theory)Large Hadron ColliderSettore FIS/01 - Fisica SperimentaleATLAShard double-parton interactions; ATLAS detectorProbemedicine.anatomical_structureHadronic CollisionsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGLHCCIENCIAS NATURALES Y EXACTASParticle Physics - ExperimentParticle physicsMultiparton InteractionsCiências Naturais::Ciências Físicas530 PhysicsAstrophysics::High Energy Astrophysical Phenomena:Ciências Físicas [Ciências Naturais]ddc:500.25304-Jet EventsNuclear physicsAtlas (anatomy)0103 physical sciencesmedicineddc:530RapidityHigh Energy Physics010306 general physicsColliderCiencias ExactasCalorimeterScience & TechnologyATLAS detector010308 nuclear & particles physicsMeasurementsHigh Energy Physics::PhenomenologyFísica//purl.org/becyt/ford/1.3 [https]QCDAstronomíaHADRON-HADRON COLLISIONSExperimental High Energy Physicsproton-proton collisionsHigh Energy Physics::ExperimentCollider
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Measurement of the Proton-Air Cross Section ats=57  TeVwith the Pierre Auger Observatory

2012

We report a measurement of the proton-air cross section for particle production at the center-of-mass energy per nucleon of 57 TeV. This is derived from the distribution of the depths of shower maxima observed with the Pierre Auger Observatory: systematic uncertainties are studied in detail. Analyzing the tail of the distribution of the shower maxima, a proton-air cross section of [505 +/- 22(stat)(-36)(+28)(syst)] mb is found.

Pierre Auger ObservatoryPhysicsProton010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaHadronAstrophysics::Instrumentation and Methods for AstrophysicsGeneral Physics and Astronomy01 natural scienceslaw.inventionAugerNuclear physicsCross section (physics)law0103 physical sciencesHigh Energy Physics::ExperimentFermilabNuclear Experiment010306 general physicsNucleonColliderPhysical Review Letters
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Comprehensive measurements oft-channel single top-quark production cross sections ats=7  TeVwith the ATLAS detector

2014

This article presents measurements of the t-channel single top-quark ((t) over bart) and top-antiquark (_ t) total production cross sections sdtq_ and sd _ tq_, their ratio Rt sdtq_= sd _ tq_, and a measurement of the inclusive production cross section sdtq _ _ tq_ in proton-proton collisions at ffiffiffi ps = 7 TeV at the LHC. Differential cross sections for the tq and _ tq processes are measured as a function of the transverse momentum and the absolute value of the rapidity of t and _ t, respectively. The analyzed data set was recorded with the ATLAS detector and corresponds to an integrated luminosity of 4.59 fb-1. Selected events contain one charged lepton, large missing transverse mome…

Quantum chromodynamicsPhysicsNuclear and High Energy PhysicsTop quarkParticle physics010308 nuclear & particles physicsCabibbo–Kobayashi–Maskawa matrix01 natural sciencesStandard ModelNuclear physicsmedicine.anatomical_structurePair productionAtlas (anatomy)0103 physical sciencesmedicineRapidity010306 general physicsLeptonPhysical Review D
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The FRAM robotic telescope for atmospheric monitoring at the Pierre Auger Observatory

2021

FRAM (F/Photometric Robotic Atmospheric Monitor) is a robotic telescope operated at the Pierre Auger Observatory in Argentina for the purposes of atmospheric monitoring using stellar photometry. As a passive system which does not produce any light that could interfere with the observations of the fluorescence telescopes of the observatory, it complements the active monitoring systems that use lasers. We discuss the applications of stellar photometry for atmospheric monitoring at optical observatories in general and the particular modes of operation employed by the Auger FRAM. We describe in detail the technical aspects of FRAM, the hardware and software requirements for a successful operati…

AstronomyLarge detector systems for particle and astroparticle physics; Optics; Photon detectors for UV visible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc); Real-time monitoringReal-time monitoring01 natural sciencesAugerSuccessful operationObservatoryopticalAPDshardwareAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsInstrumentationPhoton detectors for UVMathematical PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEEBCCDsSettore FIS/01 - Fisica SperimentalePhoton detectors for UV visible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc)Astrophysics::Instrumentation and Methods for AstrophysicsSi-PMTsAugerobservatoryRobotic telescopeG-APDsAstrophysics::Earth and Planetary AstrophysicsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaSciences exactes et naturellesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesprogrammingdetector: fluorescencePhotometry (optics)0103 physical sciencesddc:610[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]High Energy Physicsvisible and IR photons (solid-state) (PIN diodesCMOS imagersInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy AstrophysicsRemote sensingetc)fluorescence [detector]Pierre Auger Observatory010308 nuclear & particles physicsLarge detector systems for particle and astroparticle physicsActive monitoringOpticsCCDslasermonitoringEMCCDsLarge detector systems for particle and astroparticle physicatmosphereExperimental High Energy PhysicsOpticEnvironmental science[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]RAIOS CÓSMICOSastro-ph.IM
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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

2012

The surface detector array of the Pierre Auger Observatory can detect neutrinos with energy Eν between 1017 eV and 1020 eV from point-like sources across the sky south of +55º and north of −65º declinations. A search has been performed for highly inclined extensive air showers produced by the interaction of neutrinos of all flavors in the atmosphere (downward-going neutrinos), and by the decay of tau leptons originating from tau neutrino interactions in Earth’s crust (Earth-skimming neutrinos). No candidate neutrinos have been found in data up to 2010 May 31. This corresponds to an equivalent exposure of ∼3.5 years of a full surface detector array for the Earth-skimming channel and ∼2 years…

Physics::Instrumentation and DetectorsSolar neutrinoAstronomyAstrophysics01 natural sciences7. Clean energyneutrinoTelescopiosTau neutrinoastroparticle physics; cosmic rays; neutrinos; telescopes010303 astronomy & astrophysicsGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)cosmic rayPhysics[PHYS]Physics [physics]High Energy Astrophysical Phenomena (astro-ph.HE)[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]neutrinosCOSMIC-RAYSCosmic neutrino backgroundastroparticle physicsMeasurements of neutrino speedFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Radiación CósmicaAstrophysics::High Energy Astrophysical PhenomenaTELESCÓPIOSFOS: Physical sciencesAstroparticle physiccosmic rays0103 physical sciencesDETECTORCiencias ExactasPierre Auger Observatory010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaAstronomy and AstrophysicstelescopesSolar neutrino problem13. Climate actionSpace and Planetary ScienceExperimental High Energy PhysicsHigh Energy Physics::ExperimentAstroparticle physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Lepton
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A Targeted Search for Point Sources of EeV Neutrons

2014

A flux of neutrons from an astrophysical source in the Galaxy can be detected in the Pierre Auger Observatory as an excess of cosmic-ray air showers arriving from the direction of the source. To avoid the statistical penalty for making many trials, classes of objects are tested in combinations as nine “target sets”, in addition to the search for a neutron flux from the Galactic Center or from the Galactic Plane. Within a target set, each candidate source is weighted in proportion to its electromagnetic flux, its exposure to the Auger Observatory, and its flux attenuation factor due to neutron decay. These searches do not find evidence for a neutron flux from any class of candidate sources. …

Astrofísica[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]AstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesGalaxy: diskcosmic raysNeutron fluxObservatory0103 physical sciencesdata analysis [methods]Neutron010306 general physics010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Pierre Auger ObservatoryPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Galactic CenterPierre Auger Observatory; cosmic ray; neutronsAstrophysics::Instrumentation and Methods for AstrophysicsFísicaAstronomy and AstrophysicsGalactic planemethods: data analysisMagnetic fluxGalaxyAstronomíaSpace and Planetary ScienceExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGddc:520Física nuclearAstrophysics - High Energy Astrophysical Phenomenadisk [Galaxy]
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Large-scale distribution of arrival directions of cosmic rays detected above 1018 eV at the Pierre Auger Observatory

2012

A thorough search for large-scale anisotropies in the distribution of arrival directions of cosmic rays detected above 1018 eV at the Pierre Auger Observatory is presented. This search is performed as a function of both declination and right ascension in several energy ranges above 1018 eV, and reported in terms of dipolar and quadrupolar coefficients. Within the systematic uncertainties, no significant deviation from isotropy is revealed. Assuming that any cosmic-ray anisotropy is dominated by dipole and quadrupole moments in this energy range, upper limits on their amplitudes are derived. These upper limits allow us to test the origin of cosmic rays above 1018 eV from stationary Galactic …

[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Radiación CósmicaAstronomyMilky WayAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysicsEXTENSIVE AIR-SHOWERSSURFACE DETECTOR01 natural sciencesGALACTIC MAGNETIC-FIELDSAuger[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]cosmic raysObservatory0103 physical sciencesastroparticle physics; cosmic raysAnisotropy010303 astronomy & astrophysicsGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)Ciencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)Astroparticle physicsPhysicsPierre Auger ObservatoryANISOTROPY010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyFísicaAstronomy and AstrophysicsENERGY-SPECTRUMUltra-High Energy Cosmic Rays Pierre Auger Observatory Large Scale AnisotropiesSpace and Planetary Scienceastroparticle physicsExperimental High Energy PhysicsROTATIONARRAYFísica nuclearAstroparticle physicsRight ascensionAstrophysics - High Energy Astrophysical Phenomena
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Calibration of the underground muon detector of the Pierre Auger Observatory

2021

To obtain direct measurements of the muon content of extensive air showers with energy above $10^{16.5}$ eV, the Pierre Auger Observatory is currently being equipped with an underground muon detector (UMD), consisting of 219 10 $\mathrm{m^2}$-modules, each segmented into 64 scintillators coupled to silicon photomultipliers (SiPMs). Direct access to the shower muon content allows for the study of both of the composition of primary cosmic rays and of high-energy hadronic interactions in the forward direction. As the muon density can vary between tens of muons per m$^2$ close to the intersection of the shower axis with the ground to much less than one per m$^2$ when far away, the necessary bro…

muon: showersdata acquisitionPhysics::Instrumentation and DetectorsAstronomyDetector alignment and calibration methods (lasers sources particle-beams)primary [cosmic radiation]Particle detectors7. Clean energy01 natural sciencesEtc)030218 nuclear medicine & medical imaging0302 clinical medicinecalibration [detector]ObservatoryAPDsdetector: calibrationatmosphere [muon]InstrumentationPhoton detectors for UVshowers [muon]Mathematical PhysicsPhoton detectors for UV visible and IR photons (solid-state) (PIN diodes APDsSi-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc)Particle-beams)Physicsenergy: highdetector [muon]EBCCDsPhysicselectronicsSettore FIS/01 - Fisica SperimentalePhoton detectors for UV visible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc)Astrophysics::Instrumentation and Methods for AstrophysicsSourcesSi-PMTsdetector: alignmentAugermuon: atmosphereobservatorydensity [muon]G-APDshigh [energy]Particle detectorAstrophysics - Instrumentation and Methods for Astrophysicsatmosphere [showers]Detector alignment and calibration methods (lasers sourcesparticle-beams)FOS: Physical sciencesCosmic rayScintillatorParticle detectorVisible and IR photons (solid-state) (PIN diodes03 medical and health sciencesOpticsSilicon photomultipliermuon: density0103 physical sciencesCalibrationddc:530photomultiplier: silicon[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]ddc:610High Energy PhysicsCMOS imagersInstrumentation and Methods for Astrophysics (astro-ph.IM)scintillation counterParticle detectors; Detector alignment and calibration methods (lasers sources particle-beams); Photon detectors for UV visible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc); Performance of High Energy Physics DetectorsPierre Auger ObservatoryMuonshowers: atmosphere010308 nuclear & particles physicsbusiness.industrymuon: detectorCCDscosmic radiation: primaryDetector alignment and calibration methods (lasersEMCCDsanalog-to-digital converterAPDs; CCDs; CMOS imagers; Detector alignment and calibration methods (lasers; EBCCDs; EMCCDs; Etc); G-APDs; Particle detectors; Particle-beams); Performance of High Energy Physics Detectors; Photon detectors for UV; Si-PMTs; Sources; Visible and IR photons (solid-state) (PIN diodesExperimental High Energy Physicssilicon [photomultiplier]Performance of High Energy Physics DetectorsHigh Energy Physics::Experimentphoton: detectorbusinessalignment [detector]RAIOS CÓSMICOSdetector [photon]astro-ph.IM
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Observation of inclined EeV air showers with the radio detector of the Pierre Auger Observatory

2018

With the Auger Engineering Radio Array (AERA) of the Pierre Auger Observatory, we have observed the radio emission from 561 extensive air showers with zenith angles between 60 and 84. In contrast to air showers with more vertical incidence, these inclined air showers illuminate large ground areas of several km2 with radio signals detectable in the 30 to 80 MHz band. A comparison of the measured radio-signal amplitudes with Monte Carlo simulations of a subset of 50 events for which we reconstruct the energy using the Auger surface detector shows agreement within the uncertainties of the current analysis. As expected for forward-beamed radio emission undergoing no significant absorption or sc…

Physics::Instrumentation and DetectorsAstronomyengineering01 natural sciencesultra high energy cosmic rayAugerHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)cosmic ray experiments; cosmic rays detectors; ultra high energy cosmic rays; Astronomy and Astrophysics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Cosmic ray experiments cosmic rays detectors ultra high energy cosmic rays Astronomy and Astrophysics.Absorption (electromagnetic radiation)Physicsradio waveSettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsDETETORESCOSMIC-RAYSAugerobservatoryAmplitudecosmic rays detectorsAstrophysics - Instrumentation and Methods for Astrophysicsnumerical calculations: Monte CarloairAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencescosmic ray experimentultra high energy cosmic rayscascade: electromagneticOptics0103 physical sciencesHigh Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]cosmic rays detector010306 general physicscosmic ray experiments cosmic rays detectors ultra high energy cosmic raysInstrumentation and Methods for Astrophysics (astro-ph.IM)ZenithAstrophysiquePierre Auger Observatoryshowers: atmosphere010308 nuclear & particles physicsbusiness.industryScatteringhep-exdetector: surfacescatteringAstronomy and AstrophysicsAstronomieAir showerExperimental High Energy PhysicsARRAYHigh Energy Physics::Experimentcosmic ray experimentscosmic ray experiments; cosmic rays detectors; ultra high energy cosmic raysEMISSIONbusinessabsorptionastro-ph.IM
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Reconstruction of events recorded with the surface detector of the Pierre Auger Observatory

2020

Cosmic rays arriving at Earth collide with the upper parts of the atmosphere, thereby inducing extensive air showers. When secondary particles from the cascade arrive at the ground, they are measured by surface detector arrays. We describe the methods applied to the measurements of the surface detector of the Pierre Auger Observatory to reconstruct events with zenith angles less than 60 using the timing and signal information recorded using the water-Cherenkov detector stations. In addition, we assess the accuracy of these methods in reconstructing the arrival directions of the primary cosmic ray particles and the sizes of the induced showers.

Physics::Instrumentation and DetectorsAstronomyprimary [cosmic radiation]01 natural sciences030218 nuclear medicine & medical imagingAugerHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)0302 clinical medicinesurface [detector]Observatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Data Processing; Large detector systems for particle and astroparticle physics; Large detector-systems performance; Performance of High Energy Physics DetectorsInstrumentationMathematical PhysicsData Processing; Large detector systems for particle and astroparticle physics; Largedetector-systems performance; Performance of High Energy Physics DetectorsLarge detector-systems performanceHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEInstrumentation et méthodes en physiqueData ProcessingDetectorAstrophysics::Instrumentation and Methods for AstrophysicsAugercascadeobservatoryCascadeLargedetector-systems performanceddc:620Astrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomenaatmosphere [showers]airAstrophysics::High Energy Astrophysical PhenomenawaterFOS: Physical sciencesCosmic rayAtmosphere03 medical and health sciencesOptics0103 physical sciencesHigh Energy Physics14. Life underwater[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]ddc:610Instrumentation and Methods for Astrophysics (astro-ph.IM)ZenithEngineering & allied operationsPierre Auger Observatoryshowers: atmosphere010308 nuclear & particles physicsbusiness.industryhep-exdetector: surfaceLarge detector systems for particle and astroparticle physicsAutres mathématiquescosmic radiation: primaryCherenkov counterExperimental High Energy PhysicsLarge detector systems for particle and astroparticle physicHigh Energy Physics::ExperimentPerformance of High Energy Physics Detectorsbusiness[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]RAIOS CÓSMICOSastro-ph.IM
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Antennas for the detection of radio emission pulses from cosmic-ray induced air showers at the Pierre Auger Observatory.

2012

The Pierre Auger Observatory is exploring the potential of the radio detection technique to study extensive air showers induced by ultra-high energy cosmic rays. The Auger Engineering Radio Array (AERA) addresses both technological and scientific aspects of the radio technique. A first phase of AERA has been operating since September 2010 with detector stations observing radio signals at frequencies between 30 and 80 MHz. In this paper we present comparative studies to identify and optimize the antenna design for the final configuration of AERA consisting of 160 individual radio detector stations. The transient nature of the air shower signal requires a detailed description of the antenna s…

Ciencias Astronómicas[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AstronomyAstrophysics::High Energy Astrophysical Phenomenashowers: atmosphere | cosmic radiation: UHE | polarization: effect | Auger | radio wave: emission | radio wave: detector | galaxy | background | reflection | noise | detector: networkFOS: Physical sciencesCosmic ray01 natural sciencesSignalKASCADEMHZOpticsSIGNALS0103 physical sciencesTransient responseTime domain010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)InstrumentationMathematical Physics[PHYS]Physics [physics]PhysicsPierre Auger ObservatorySPECTRUMLarge detector systems for particle and astroparticle physics010308 nuclear & particles physicsbusiness.industryPhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsFísica[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]ATMOSFERA (MONITORAMENTO)Air showerAntennaExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGRADIATIONAntennasFísica nuclearAntenna (radio)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Instrumentation and Methods for Astrophysicsbusiness
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Search for nonpointing photons in the diphoton andETmissfinal state ins=7  TeVproton-proton collisions using the ATLAS detector

2013

A search has been performed for photons originating in the decay of a neutral long-lived particle, exploiting the capabilities of the ATLAS electromagnetic calorimeter to make precise measurements of the flight direction of photons, as well as the calorimeter's excellent time resolution. The search has been made in the diphoton plus missing transverse energy final state, using the full data sample of 4.8 fb(-1) of 7 TeV proton-proton collisions collected in 2011 with the ATLAS detector at the LHC. No excess is observed above the background expected from Standard Model processes. The results are used to set exclusion limits in the context of gauge mediated supersymmetry breaking models, with…

PhysicsNuclear and High Energy PhysicsParticle physicsPhotonLarge Hadron ColliderPhysics::Instrumentation and Detectors010308 nuclear & particles physicsAtlas (topology)Atlas detectorHigh Energy Physics::Phenomenology01 natural sciencesSupersymmetry breakingNuclear physicsTransverse plane0103 physical sciencesNeutralinoHigh Energy Physics::ExperimentGravitino010306 general physicsPhysical Review D
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Measurements of the Nuclear Modification Factor for Jets inPb+PbCollisions atsNN=2.76  TeVwith the ATLAS Detector

2015

Measurements of inclusive jet production are performed in pp and Pb+Pb collisions at √sNN = 2.76 TeV with the ATLAS detector at the LHC, corresponding to integrated luminosities of 4.0 pb−1 and 0.14 nb−1, respectively. The jets are identified with the anti-kt algorithm with R = 0.4, and the spectra are measured over the kinematic range of jet transverse momentum 32 < pT < 500 GeV, and absolute rapidity |y| < 2.1 and as a function of collision centrality. The nuclear modification factor, RAA, is evaluated and jets are found to be suppressed by approximately a factor of two in central collisions compared to pp collisions. The RAA shows a slight increase with pT and no significant variation wi…

PhysicsParticle physicsJet (fluid)Large Hadron Collider010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and Astronomy01 natural sciencesSpectral lineNuclear physicsmedicine.anatomical_structureAtlas (anatomy)0103 physical sciencesQuark–gluon plasmamedicineHigh Energy Physics::ExperimentRapidityImpact parameterNuclear Experiment010306 general physicsJet quenchingPhysical Review Letters
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Measurements of normalized differential cross sections fortt¯production inppcollisions at(s)=7  TeVusing the ATLAS detector

2014

Measurements of normalized differential cross sections for top-quark pair production are presented as a function of the top-quark transverse momentum, and of the mass, transverse momentum, and rapidity of the t (t) over bar system, in proton proton collisions at a center-of-mass energy of root s = 7 TeV. The data set corresponds to an integrated luminosity of 4.6 fb(-1), recorded in 2011 with the ATLAS detector at the CERN Large Hadron Collider. Events are selected in the lepton jets channel, requiring exactly one lepton and at least four jets with at least one of the jets tagged as originating from a b-quark. The measured spectra are corrected for detector efficiency and resolution effects…

PhysicsNuclear and High Energy PhysicsParticle physicsLuminosity (scattering theory)Large Hadron ColliderProtonHigh Energy Physics::PhenomenologyParton7. Clean energyNuclear physicsPair productionmedicine.anatomical_structureAtlas (anatomy)medicineHigh Energy Physics::ExperimentRapidityNuclear ExperimentLeptonPhysical Review D
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Measurement of the cross-section for W boson production in association with b-jets in pp collisions at root s=7 TeV with the ATLAS detector

2013

This paper reports a measurement of the W +b-jets (W +b+ X and W + b[¯ over b] +X) production cross-section in proton-proton collisions at a centre-of-mass energy of 7 TeV at the LHC. These results are based on data corresponding to an integrated luminosity of 4.6 fb[superscript −1], collected with the ATLAS detector. Cross-sections are presented as a function of jet multiplicity and of the transverse momentum of the leading b-jet for both the muon and electron decay modes of the W boson. The W +b-jets cross-section, corrected for all known detector effects, is quoted in a limited kinematic range. Combining the muon and electron channels, the fiducial cross-section for W +b-jets is measured…

Particle physicsNuclear and High Energy PhysicsCiências Naturais::Ciências FísicasAtlas detectorlarge hadron collider530 PhysicsAstrophysics::High Energy Astrophysical Phenomena:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesElectronAstrophysics::Cosmology and Extragalactic Astrophysicsddc:500.201 natural sciences7. Clean energy530High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesNaturvetenskap[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]w bosonRapidityHigh Energy PhysicsMultiplicity (chemistry)010306 general physicsNuclear ExperimentCiencias ExactasQCQuantum chromodynamicsPhysicsLarge Hadron ColliderMuonScience & TechnologyHadron-Hadron ScatteringATLAS detector010308 nuclear & particles physicsDetectorSettore FIS/01 - Fisica SperimentaleFísicaATLASb-jetsExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGproton-proton collisionsHigh Energy Physics::ExperimentLHCNatural SciencesParticle Physics - Experiment
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Cosmic-Ray Anisotropies in Right Ascension Measured by the Pierre Auger Observatory

2020

We present measurements of the large-scale cosmic-ray anisotropies in right ascension, using data collected by the surface detector array of the Pierre Auger Observatory over more than 14 years. We determine the equatorial dipole component, ~d⊥, through a Fourier analysis in right ascension that includes weights for each event so as to account for the main detector-induced systematic effects. For the energies at which the trigger efficiency of the array is small, the “East-West” method is employed. Besides using the data from the array with detectors separated by 1500 m, we also include data from the smaller but denser sub-array of detectors with 750 m separation, which allows us to extend …

010504 meteorology & atmospheric sciencesAstronomyAstrophysicsAstrophysicsanisotropy [cosmic radiation]Amplitude01 natural sciencessurface [detector]010303 astronomy & astrophysicsRight ascensionastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsOBSERVATÓRIOSGalactic CenterAstrophysics::Instrumentation and Methods for AstrophysicsCosmic RaysAugerobservatoryAmplitudePhysics::Space PhysicsAstrophysics - High Energy Astrophysical PhenomenaExtragalactic cosmic rayAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic raycosmic radiation: anisotropyExtragalactic cosmic rayGalactic center0103 physical sciencesHigh Energy PhysicsPierre auger observatory0105 earth and related environmental sciencesPierre Auger Observatorydetector: surfaceFísicaAstronomy and AstrophysicsCosmic rayefficiency [trigger]GalaxyDipole* Automatic Keywords *Space and Planetary ScienceExperimental High Energy Physicstrigger: efficiencyddc:520galaxyDipoleObservatoryEnergy (signal processing)anisotropiesRight ascension[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)dipoleThe Astrophysical Journal
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Search for ultrarelativistic magnetic monopoles with the Pierre Auger Observatory

2016

We present a search for ultra-relativistic magnetic monopoles with the Pierre Auger Observatory. Such particles, possibly a relic of phase transitions in the early universe, would deposit a large amount of energy along their path through the atmosphere, comparable to that of ultrahigh-energy cosmic rays (UHECRs). The air shower profile of a magnetic monopole can be effectively distinguished by the fluorescence detector from that of standard UHECRs. No candidate was found in the data collected between 2004 and 2012, with an expected background of less than 0.1 event from UHECRs. The corresponding 90% confidence level (C.L.) upper limits on the flux of ultra-relativistic magnetic monopoles ra…

FLUORESCENCE YIELDAstronomymagnetic monopolemagnetic fieldAstrophysics7. Clean energy01 natural sciencesObservatoryUHE Cosmic Raysair-showerMonte Carlo010303 astronomy & astrophysicsMagnetic Monopolesmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicscritical phenomenaFLUORESCENCE YIELD; ENERGY LOSS; DETECTORAugerMagnetic fieldobservatoryLorentz factorComputingMethodologies_DOCUMENTANDTEXTPROCESSINGsymbolsFísica nuclearfluorescenceAstrophysics - High Energy Astrophysical Phenomenaspatial distribution [showers]LorentzENERGY LOSSatmosphere [showers]energyFLUXNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]airmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]Magnetic monopoleFOS: Physical sciencesCosmic rayNuclear physicssymbols.namesakecosmic rays0103 physical sciencesddc:530High Energy PhysicsDETECTORCiencias Exactasfluorescence [detector]Pierre Auger Observatorybackground010308 nuclear & particles physicsFísicaASTROFÍSICAUniversefluxultrarelativistic magnetic monopolesAir shower13. Climate actionExperimental High Energy PhysicsrelativisticgalaxyENERGY-LOSS
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Search for photons with energies above 1018 eV using the hybrid detector of the Pierre Auger Observatory

2017

A search for ultra-high energy photons with energies above 1 EeV is performed using nine years of data collected by the Pierre Auger Observatory in hybrid operation mode. An unprecedented separation power between photon and hadron primaries is achieved by combining measurements of the longitudinal air-shower development with the particle content at ground measured by the fluorescence and surface detectors, respectively. Only three photon candidates at energies 1-2 EeV are found, which is compatible with the expected hadron-induced background. Upper limits on the integral flux of ultra-high energy photons of 0.027, 0.009, 0.008, 0.008 and 0.007 km-2 sr-1 yr-1 are derived at 95% C.L. for ener…

ultra high energy cosmic rays cosmic ray experimentsPhoton[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]AstronomyHadronFluxultra high energy cosmic rays; cosmic ray experiments7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)energy: thresholdCosmic ray experiments[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsphoton: productionconstraint: energyCOSMIC-RAYSAugerobservatoryContent (measure theory)ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearfluorescenceAstrophysics - High Energy Astrophysical PhenomenalongitudinalAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesCosmic rayultra high energy cosmic raysdark matterUltra high energy cosmic rays Cosmic ray experiments Astronomy and Astrophysics.Nuclear physics[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesultra high energy cosmic rays; cosmic ray experiments; Astronomy and Astrophysicscosmic radiation: UHEHigh Energy PhysicsCiencias ExactasPierre Auger ObservatorySPECTRUMhybridbackgrounddetector: surface010308 nuclear & particles physicsFísicaUltra high energy cosmic raysAstronomy and AstrophysicsASTROFÍSICAULTRA-HIGH ENERGYfluxExperimental High Energy PhysicsHigh Energy Physics::Experimentcosmic ray experimentshadron[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)
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Search for a heavy narrow resonance decaying to eμ, eτ, or μτ with the ATLAS detector in s=7 TeV pp collisions at the LHC

2013

This Letter presents the results of a search for a heavy particle decaying into an e^±μ^∓e^±μ^∓, or μ^±τ^∓ final state in pp collisions at View the MathML sources=7 TeV. The data were recorded with the ATLAS detector at the LHC during 2011 and correspond to an integrated luminosity of 4.6 fb−14.6 fb^(−1). No significant excess above the Standard Model expectation is observed, and exclusions at 95% confidence level are placed on the cross section times branching ratio for the production of an R-parity-violating supersymmetric tau sneutrino. For a sneutrino mass of 500 (2000) GeV, the observed limits on the production cross section times branching ratio are 3.2 (1.4) fb, 42 (17) fb, and 40 (1…

PhysicsNuclear and High Energy PhysicsParticle physicsLuminosity (scattering theory)Large Hadron Collider010308 nuclear & particles physicsBranching fractionTevatronSupersymmetry01 natural sciencesStandard ModelNuclear physicsmedicine.anatomical_structureAtlas (anatomy)0103 physical sciencesmedicine010306 general physicsLeptonPhysics Letters B
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Measurement of the Fluctuations in the Number of Muons in Extensive Air Showers with the Pierre Auger Observatory

2021

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargue. We are very grateful to the following agencies and organizations for financial support: Argentina-Comision Nacional de Energia Atomica, Agencia Nacional de Promocion Cientifica y Tecnologica (ANPCyT), Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET), Gobierno de la Provincia de Mendoza, Municipalidad de Malargue, NDM Holdings and Valle Las Lenas; in gratitude for their continuing cooperation over land access; Australia-the Australian Research Council; Brazil…

interaction: modelPhysics::Instrumentation and DetectorsAstronomyHadronGeneral Physics and AstronomyUltra-high energy cosmic rays muons properties hadronic models01 natural sciencescosmic ray; particle interaction; astroparticle detectorsAugerHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ironsurface [detector]Observatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]cosmic rayPhysics4. EducationPhysicsSettore FIS/01 - Fisica Sperimentalemeasured [fluctuation]model [interaction]Astrophysics::Instrumentation and Methods for Astrophysicsmodel: hadronicfluctuation: measured3. Good healthAugerobservatoryparticle interactionSciences exactes et naturellesatmosphere [showers]model [particle]airCherenkov counter: waterAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencesCosmic raydetector: fluorescenceNuclear physicsastroparticle detectorscosmic raysmuon0103 physical sciencescalorimeterddc:53014. Life underwatercosmic radiation: UHEHigh Energy Physicsdistribution functionelectromagnetic component010306 general physicsAstrophysiquePierre Auger Observatoryfluorescence [detector]Muonshowers: atmospherehep-exdetector: surfacewater [Cherenkov counter]particle: modelSmall deviationsFísicaASTROFÍSICAAir showerExperimental High Energy PhysicsElementary Particles and Fieldshadronic [model]High Energy Physics::Experiment
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Muons in air showers at the Pierre Auger Observatory

2015

We present the first hybrid measurement of the average muon number in air showers at ultrahigh energies, initiated by cosmic rays with zenith angles between 62° and 80°. The measurement is based on 174 hybrid events recorded simultaneously with the surface detector array and the fluorescence detector of the Pierre Auger Observatory. The muon number for each shower is derived by scaling a simulated reference profile of the lateral muon density distribution at the ground until it fits the data. A 1019eV shower with a zenith angle of 67°, which arrives at the surface detector array at an altitude of 1450 m above sea level, contains on average (2.68±0.04±0.48(sys))×107 muons with energies large…

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Nuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsCosmic-ray interactionsAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayextensive atmospherical showers muon density muon number Pierre Auger Observatory cosmic radiation UHEHadronic interaction models7. Clean energyAugerSettore FIS/04 - Fisica Nucleare e SubnucleareNuclear physicsAltitudeSettore FIS/05 - Astronomia e AstrofisicaObservatoryNERGY COSMIC-RAYS DETECTOR MODEL.Extensive air showerscosmic radiation UHEDETECTORScalingCosmic raysZenithHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatoryMuonNERGY COSMIC-RAYSSettore FIS/01 - Fisica Sperimentaleenergy cosmic-rays; detector; modelAstrophysics::Instrumentation and Methods for AstrophysicsFísica[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Pierre Auger ObservatoryASTROFÍSICAextensive atmospherical showersmuon numberMODELmuon densityExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaPhysical Review D
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Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory

2015

Energy-dependent patterns in the arrival directions of cosmic rays are searched for using data of the Pierre Auger Observatory. We investigate local regions around the highest-energy cosmic rays with E ≥ 6×1019 eV by analyzing cosmic rays with energies above E ≥ 5×1018 eV arriving within an angular separation of approximately 15∘. We characterize the energy distributions inside these regions by two independent methods, one searching for angular dependence of energy-energy correlations and one searching for collimation of energy along the local system of principal axes of the energy distribution. No significant patterns are found with this analysis. The comparison of these measurements with …

AstrofísicaPhysics and Astronomy (miscellaneous)Raycosmic radiation anisotropy cosmic radiation propagation cosmic radiation deflectionAstronomymagnetic fieldpAstrophysicsanisotropy [cosmic radiation]01 natural sciencesSettore FIS/04 - Fisica Nucleare e SubnucleareAugerPierre//purl.org/becyt/ford/1 [https]ObservatoryJetsQuantum Chromodynamicscosmic radiation: VHEenergy: correlationPatternsMonte Carlo010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicscosmic radiation: propagationEnergyCOSMIC cancer databaseAngular distance[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsSettore FIS/01 - Fisica SperimentaleSearchAstrophysics::Instrumentation and Methods for Astrophysicscosmic radiation anisotropyPierre Auger Observatorycosmic radiation: deflectionRadiación cósmicaAugerSurface Detector ArrayCosmicArrivalComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaPrincipal axis theorem[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Regular Article - Experimental PhysicsAstrophysics::High Energy Astrophysical PhenomenaPhysics and Astronomy (miscellaneous) Engineering (miscellaneous).FOS: Physical sciencesCosmic ray530cosmic radiation: anisotropyParticle detectorSettore FIS/05 - Astronomia e AstrofisicaVHE [cosmic radiation]statistical analysisSpectrum0103 physical sciencesthrustddc:530Engineering (miscellaneous)AstrophysiqueCiencias ExactasPierre Auger Observatoryair: showerscosmic radiation propagationPhysics and Astronomy (miscellaneous); Engineering (miscellaneous)010308 nuclear & particles physicsturbulence[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FísicaAstroparticles//purl.org/becyt/ford/1.3 [https]ASTROFÍSICAGalactic Magnetic-fieldcorrelation [energy]DirectionExperimental High Energy Physicscosmic radiation deflectionpropagation [cosmic radiation]direct detectiongalaxyObservatory[ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]deflection [cosmic radiation]showers [air]Model
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Multi-channel search for squarks and gluinos in root s=7 TeV pp collisions with the ATLAS detector at the LHC

2013

A search for supersymmetric particles in final states with zero, one, and two leptons, with and without jets identified as originating from b-quarks, in 4.7 fb[superscript −1] of √s = 7 TeV pp collisions produced by the Large Hadron Collider and recorded by the ATLAS detector is presented. The search uses a set of variables carrying information on the event kinematics transverse and parallel to the beam line that are sensitive to several topologies expected in supersymmetry. Mutually exclusive final states are defined, allowing a combination of all channels to increase the search sensitivity. No deviation from the Standard Model expectation is observed. Upper limits at 95 % confidence level…

Brookhaven National LaboratoryParticle physicsPhysics and Astronomy (miscellaneous)Supergauge TransformationsContext (language use)ddc:500.253001 natural sciencesStandard ModelSet (abstract data type)CurrentsPions0103 physical sciencesddc:530Sensitivity (control systems)WeakHigh Energy Physics010306 general physicsEngineering (miscellaneous)QCCiencias ExactasPhysicsproton–proton collisionsHadron-Hadron ScatteringLarge Hadron ColliderATLAS detector010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleHigh Energy Physics::PhenomenologyFísicaSupersymmetryATLASgluinosHADRON-HADRON COLLISIONSExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGsquarksHigh Energy Physics::ExperimentSupersymmetryLHCEvent (particle physics)LeptonModel
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Study of heavy-flavor quarks produced in association with top-quark pairs at s=7  TeV using the ATLAS detector

2014

Using a sample of dilepton top-quark pair ((tt) over bar) candidate events, a study is performed of the production of top-quark pairs together with heavy-flavor (HF) quarks, the sum of (tt) over bar + b + X and (tt) over bar + c + X, collectively referred to as (tt) over bar + HF. The data set used corresponds to an integrated luminosity of 4.7 fb(-1) of proton-proton collisions at a center-of-mass energy of 7 TeV recorded by the ATLAS detector at the CERN Large Hadron Collider. The presence of additional HF (b or c) quarks in the (tt) over bar sample is inferred by looking for events with at least three b-tagged jets, where two are attributed to the b quarks from the (tt) over bar decays a…

QuarkQuantum chromodynamicsPhysicsNuclear and High Energy PhysicsParticle physicsTop quarkLarge Hadron ColliderMass distributionAtlas detectorHigh Energy Physics::Phenomenology7. Clean energyNuclear physicsMass spectrumHigh Energy Physics::ExperimentBoson
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A search for anisotropy in the arrival directions of ultra high energy cosmic rays recorded at the Pierre Auger Observatory

2012

Observations of cosmic ray arrival directions made with the Pierre Auger Observatory have previously provided evidence of anisotropy at the 99% CL using the correlation of ultra high energy cosmic rays (UHECRs) with objects drawn from the Véron-Cetty Véron catalog. In this paper we report on the use of three catalog independent methods to search for anisotropy. The 2pt–L, 2pt+ and 3pt methods, each giving a different measure of selfclustering in arrival directions, were tested on mock cosmic ray data sets to study the impacts of sample size and magnetic smearing on their results, accounting for both angular and energy resolutions. If the sources of UHECRs follow the same large scale structu…

HIRES STEREO[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]AstronomySMALL-SCALE ANISOTROPYAstrophysics01 natural sciencesAltas energíasCosmic Rays ShowerCosmologyUltra-high-energy cosmic rayAnisotropy010303 astronomy & astrophysicsmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[PHYS]Physics [physics]BL-LACERTAEAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryRadiación cósmicaFísica nuclearOBJECTSAstrophysics - High Energy Astrophysical Phenomenacosmic ray experiments; ultra high energy cosmic raysACTIVE GALACTIC NUCLEIActive galactic nucleusmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic raysearch for anisotropyultra high energy cosmic raysCosmic Ray[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciences010306 general physicsCiencias ExactasPierre Auger ObservatorySPECTRUMAstronomyFísicaAstronomy and AstrophysicsASTROFÍSICAUniverseGalaxyExperimental High Energy Physicsanisotrpycosmic ray experiments[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cosmologyJournal of Cosmology and Astroparticle Physics
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Searches for anisotropies in the arrival directions of the highest energy cosmic rays detected by the Pierre Auger Observatory

2015

We analyze the distribution of arrival directions of ultra-high energy cosmic rays recorded at the Pierre Auger Observatory in 10 years of operation. The data set, about three times larger than that used in earlier studies, includes arrival directions with zenith angles up to $80^\circ$, thus covering from $-90^\circ$ to $+45^\circ$ in declination. After updating the fraction of events correlating with the active galactic nuclei (AGNs) in the V��ron-Cetty and V��ron catalog, we subject the arrival directions of the data with energies in excess of 40 EeV to different tests for anisotropy. We search for localized excess fluxes and for self-clustering of event directions at angular scales up t…

acceleration of particles; astroparticle physicsNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Upper LimitAstronomyCiencias FísicasAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFieldCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsOtras Ciencias Físicas01 natural sciencesSettore FIS/04 - Fisica Nucleare e SubnucleareSettore FIS/05 - Astronomia e AstrofisicaObservatorySpectrum0103 physical sciencesacceleration of particles astroparticle physicsSurface Detector010303 astronomy & astrophysicsacceleration of particleAstrophysics::Galaxy Astrophysicsacceleration of particlesPhysicsPierre Auger ObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleArrayAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]astroparticle physicAstronomy and AstrophysicsASTROFÍSICANucleiSpace and Planetary Scienceastroparticle physicsExperimental High Energy Physicsacceleration of particles; astroparticle physics; Nuclear and High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearCatalogSkyAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTAS
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Measurement of differentialJ/ψproduction cross sections and forward-backward ratios inp + Pbcollisions with the ATLAS detector

2015

Measurements of differential cross sections for J/psi production in p + Pb collisions at root S-NN= 5.02 TeV at the CERN Large Hadron Collider with the ATLAS detector are presented. The data set us ...

Nuclear physicsPhysicsQuarkNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderPhysics::Instrumentation and DetectorsAtlas detectorAtlas (topology)Physics::Accelerator PhysicsHigh Energy Physics::ExperimentForward backwardNuclear ExperimentPhysical Review C
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The energy spectrum of cosmic rays beyond the turn-down around 1017 eV as measured with the surface detector of the Pierre Auger Observatory

2021

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargüe. We are very grateful to the following agencies and organizations for financial support: Argentina – Comisión Nacional de Energía Atómica; Agencia Nacional de Promoción Científica y Tecnológica (ANPCyT); Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET); Gobierno de la Provincia de Mendoza; Municipalidad de Malargüe; NDM Holdings and Valle Las Leñas; in gratitude for their continuing cooperation over land access; Australia – the Australian Research Council; Be…

Physics and Astronomy (miscellaneous)AstronomyAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencesFluxCosmic rayAstrophysics7. Clean energy01 natural sciencesdetector: fluorescenceAugercosmic rayssurface [detector]Observatory0103 physical sciencescalorimeterddc:530High Energy Physicscosmic radiation: UHEspectrum [cosmic radiation]010303 astronomy & astrophysicsEngineering (miscellaneous)Engineering & allied operationsHigh Energy Astrophysical Phenomena (astro-ph.HE)fluorescence [detector]Pierre Auger ObservatoryPhysicsastro-ph.HEcosmic radiation: energy spectrumcosmic radiation: spectrumdetector: surface010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsAugerCalorimeterfluxobservatoryspectralddc:620[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical Phenomenaenergy spectrum [cosmic radiation]Energy (signal processing)RAIOS CÓSMICOSultra-high energy cosmic rays energy spectrum features.
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Extraction of the Muon Signals Recorded with the Surface Detector of the Pierre Auger Observatory Using Recurrent Neural Networks

2021

The Pierre Auger Observatory, at present the largest cosmic-ray observatory ever built, is instrumented with a ground array of 1600 water-Cherenkov detectors, known as the Surface Detector (SD). The SD samples the secondary particle content (mostly photons, electrons, positrons and muons) of extensive air showers initiated by cosmic rays with energies ranging from $10^{17}~$eV up to more than $10^{20}~$eV. Measuring the independent contribution of the muon component to the total registered signal is crucial to enhance the capability of the Observatory to estimate the mass of the cosmic rays on an event-by-event basis. However, with the current design of the SD, it is difficult to straightfo…

PhotonPhysics::Instrumentation and DetectorsAstronomyElectron01 natural sciencesHigh Energy Physics - ExperimentAugerHigh Energy Physics - Experiment (hep-ex)mass [cosmic radiation]surface [detector]Observatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]photon: cosmic radiationInstrumentationMathematical PhysicsPhysicsAGASAPhysicsSettore FIS/01 - Fisica SperimentaleDetectorcosmic radiation [photon]Astrophysics::Instrumentation and Methods for AstrophysicsMonte Carlo [numerical calculations]electromagnetic [showers]Augerobservatorycosmic radiation [electron]Analysis and statistical methodsnumerical calculations: Monte CarloAnalysis and statistical methodperformancepositron: cosmic radiationatmosphere [showers]Cherenkov detectordata analysis methodAnalysis and statistical methods; Calibration and fitting methods; Cherenkov detectors; Cluster finding; Large detector systems for particle and astroparticle physics; Pattern recognitionCherenkov counter: waterairneural networkAstrophysics::High Energy Astrophysical Phenomena610FOS: Physical sciencesCosmic raycosmic radiation [positron]cosmic radiation: massCalibration and fitting methodNuclear physicsstatistical analysisPattern recognition0103 physical sciencesshowers: electromagneticddc:530ddc:610High Energy Physics010306 general physicsZenithPierre Auger ObservatoryCalibration and fitting methodscosmic radiation [muon]Muonshowers: atmosphere010308 nuclear & particles physicsdetector: surfacehep-exLarge detector systems for particle and astroparticle physicswater [Cherenkov counter]Cherenkov detectorsCluster findingelectron: cosmic radiationRecurrent neural networkmuon: cosmic radiationLarge detector systems for particle and astroparticle physicExperimental High Energy PhysicsHigh Energy Physics::ExperimentRAIOS CÓSMICOSexperimental results
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Measurement of the cosmic ray energy spectrum using hybrid events of the Pierre Auger Observatory

2012

The energy spectrum of ultra-high energy cosmic rays above 10$^{18}$ eV is measured using the hybrid events collected by the Pierre Auger Observatory between November 2005 and September 2010. The large exposure of the Observatory allows the measurement of the main features of the energy spectrum with high statistics. Full Monte Carlo simulations of the extensive air showers (based on the CORSIKA code) and of the hybrid detector response are adopted here as an independent cross check of the standard analysis (Phys. Lett. B 685, 239 (2010)). The dependence on mass composition and other systematic uncertainties are discussed in detail and, in the full Monte Carlo approach, a region of confiden…

FLUORESCENCE DETECTORAstronomyAstrophysics::High Energy Astrophysical PhenomenaMonte Carlo methodenergy spectrumFOS: Physical sciencesGeneral Physics and AstronomyFluxCosmic rayEXTENSIVE AIR-SHOWERSSURFACE DETECTOR01 natural sciencesCosmic RayAugerPierre Auger Observatory ; Monte Carlo simulations ; ultra-high energy cosmic raysHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Observatory0103 physical sciencesRECONSTRUCTIONFermilab010306 general physicsUHE Cosmic Rays Monte Carlo Energy SpectrumTRIGGERNuclear PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatoryPACS: 96.50.S 96.50.sb 96.50.sd 98.70.Sa010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Pierre Auger Observatory; Monte Carlo simulations; ultra-high energy cosmic raysPhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryPROFILES[PHYS.PHYS.PHYS-SPACE-PH]Physics [physics]/Physics [physics]/Space Physics [physics.space-ph]Experimental High Energy PhysicsSIMULATIONComputingMethodologies_DOCUMENTANDTEXTPROCESSINGARRAYFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaRAIOS CÓSMICOS
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Monitoring and data quality assessment of the ATLAS liquid argon calorimeter

2014

The liquid argon calorimeter is a key component of the ATLAS detector installed at the CERN Large Hadron Collider. The primary purpose of this calorimeter is the measurement of electron and photon kinematic properties. It also provides a crucial input for measuring jets and missing transverse momentum. An advanced data monitoring procedure was designed to quickly identify issues that would affect detector performance and ensure that only the best quality data are used for physics analysis. This article presents the validation procedure developed during the 2011 and 2012 LHC data-taking periods, in which more than 98% of the proton-proton luminosity recorded by ATLAS at a centre-of-mass ener…

interaction [p nucleus]data acquisitionPhysics::Instrumentation and DetectorsCiencias FísicasNuclear engineeringinteraction [p p]7. Clean energy01 natural sciencesHigh Energy Physics - Experiment//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)Particle identification methodsData acquisitionParticle Identification Methodsperformance [monitoring]Naturvetenskap[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]InstrumentationQCMathematical PhysicsPhysicsLarge Hadron ColliderLuminosity (scattering theory)Settore FIS/01 - Fisica SperimentaleDetectorATLASCalorimeterCERN LHC Collmedicine.anatomical_structurePhysical SciencesComputingMethodologies_DOCUMENTANDTEXTPROCESSINGLHCNatural SciencesCIENCIAS NATURALES Y EXACTASParticle Physics - ExperimentnoiseCiências Naturais::Ciências Físicas530 Physics:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesCalorimeters; Large detector systems for particle and astroparticle physics; Particle identification methods; Instrumentation; Mathematical Physics530Nuclear physicsParticle identification methodCalorimetersParticle identification methods; Calorimeters; Large detector systems for particle and astroparticle physicsscattering [heavy ion]Atlas (anatomy)0103 physical sciencesCalibrationmedicineFysikHigh Energy Physicsddc:610010306 general physicsCalorimeters; Large detector systems for particle and astroparticle physics; Particle identification methodsCiencias ExactasCalorimeterleadScience & TechnologyLarge detector systems for particle and astroparticle physics010308 nuclear & particles physicsFísica//purl.org/becyt/ford/1.3 [https]calibrationAstronomíamissing-energy [transverse momentum]Data qualityExperimental High Energy PhysicsLarge detector systems for particle and astroparticle physicPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentLarge Detector Systems for Particle and Astroparticle Physicsliquid argon [calorimeter]
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Search for dark matter in events with heavy quarks and missing transverse momentum in [Formula: see text] collisions with the ATLAS detector.

2014

This article reports on a search for dark matter pair production in association with bottom or top quarks in \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$20.3 \mathrm {~fb}^{-1}$$\end{document}20.3fb-1 of \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$pp$$\end{document}pp collisions collected at \documentclass[12pt]{minimal} \use…

Regular Article - Experimental PhysicsThe European physical journal. C, Particles and fields
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Simultaneous measurements of thett¯,W+W−, andZ/γ*→ττproduction cross-sections inppcollisions ats=7  TeVwith the ATLAS detector

2015

Simultaneous measurements of the t (t) over bar, W+W-, and Z/gamma* -> tau tau production cross-sections using an integrated luminosity of 4.6 fb(-1) of pp collisions at root s = 7 TeV collected ...

Quantum chromodynamicsPhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderLuminosity (scattering theory)010308 nuclear & particles physicsAtlas detectorAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::Phenomenology01 natural sciencesNuclear physicsmedicine.anatomical_structureAtlas (anatomy)0103 physical sciencesmedicineHigh Energy Physics::ExperimentProduction (computer science)010306 general physicsAstrophysics::Galaxy AstrophysicsBar (unit)Physical Review D
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Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory

2019

The 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 deposit all their energy in the atmosphere. This estimation is typically made using Monte Carlo simulations and thus depends on the assumed primary particle mass and on model predictions for neutrino and muon production. In this work we present a new method to obtain the invisible energy from events detected by the Pierre Auger Observatory. The method uses measurements of the muon number at ground level, and it allows us to significantly reduce the systematic uncertainties related to the mass composition and th…

Primary energyAstronomyAstrophysics::High Energy Astrophysical PhenomenaMonte Carlo methodHadronFOS: Physical sciencesCosmic rayultra high energy cosmic rays01 natural sciencesNuclear physicscosmic rays0103 physical sciencesExperiments in gravityddc:530High Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)DETECTORPierre Auger ObservatoryPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Muon010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsGénéralitésDETETORESMODEL13. Climate actioncosmic rays detectors ultra high energy cosmic raysExperimental High Energy Physicscosmic rays detectorsNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cosmologyEnergy (signal processing)Physical Review D
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Search for high-mass diphoton resonances inppcollisions ats=8  TeVwith the ATLAS detector

2015

Search for high-mass diphoton resonances in pp collisions at pffisffi root s=8 TeV with the ATLAS detector

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderPhotonPhysics::Instrumentation and DetectorsAtlas detectorAtlas (topology)Astrophysics::High Energy Astrophysical PhenomenaGraviton750 GeV diphoton excessNuclear physicsRandall–Sundrum modelHigh massHigh Energy Physics::ExperimentPhysical Review D
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Measurement of the radiation energy in the radio signal of extensive air showers as a universal estimator of cosmic-ray energy

2016

We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8±0.7(stat)±6.7(syst) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principles calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the d…

Ciencias FísicasAstronomyGeneral Physics and Astronomyultra-high energy cosmic raysAstrophysics01 natural sciencesHigh Energy Physics - Experiment//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)CODALEMAObservatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]GeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsRange (particle radiation)Radio detectorTUNKA-REXSettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsRadio TechniqueFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysicsradio emissionCIENCIAS NATURALES Y EXACTASRadio wave[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsPhysics and Astronomy (all)0103 physical sciencesextensive air showersHigh Energy Physicsultra-high energy cosmic rays extensive air showers radio emission010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysPierre Auger Observatory010308 nuclear & particles physicsRadiant energyFísicaLOFAR//purl.org/becyt/ford/1.3 [https]LOFARASTROFÍSICASIMULATIONSComputational physicsAstronomíaCOREASExperimental High Energy PhysicsARRAYEMISSION SIMULATIONS LOFAR.EMISSION
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An Indication of Anisotropy in Arrival Directions of Ultra-high-energy Cosmic Rays through Comparison to the Flux Pattern of Extragalactic Gamma-Ray …

2018

A new analysis of the dataset from the Pierre Auger Observatory provides evidence for anisotropy in the arrival directions of ultra-high-energy cosmic rays on an intermediate angular scale, which is indicative of excess arrivals from strong, nearby sources. The data consist of 5514 events above 20 EeV with zenith angles up to 80 deg recorded before 2017 April 30. Sky models have been created for two distinct populations of extragalactic gamma-ray emitters: active galactic nuclei from the second catalog of hard Fermi-LAT sources (2FHL) and starburst galaxies from a sample that was examined with Fermi-LAT. Flux-limited samples, which include all types of galaxies from the Swift-BAT and 2MASS …

Astronomy[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Ciencias Físicascosmic radiation: densitygalaxies: starburstAstrophysics01 natural sciences//purl.org/becyt/ford/1 [https]methods: data analysis Supporting material: FITS fileUltra-high-energy cosmic raydata analysis [Methods]Anisotropycosmic radiation: model010303 astronomy & astrophysicscosmic rayHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsOBSERVATÓRIOSSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsastroparticle physicastroparticle physics; cosmic rays; galaxies: active; galaxies: starburst; methods: data analysis Supporting material: FITS files; Astronomy and Astrophysics; Space and Planetary ScienceAugerobservatorygamma ray: emissiondata analysis Supporting material: FITS file [methods]astroparticle physicsAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTASAstrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusactive [Galaxies]Astrophysics::High Energy Astrophysical Phenomenagalaxies: activeData analysisFOS: Physical sciencesStarburstCosmic rayanisotropyAstrophysics::Cosmology and Extragalactic AstrophysicsOtras Ciencias FísicasGLASTcosmic raysastroparticle physics; cosmic rays; galaxies: active; galaxies: starburst; methods: data analysis Supporting material: FITS files0103 physical sciencesHigh Energy Physicscosmic radiation: UHEAGNCosmic raysAstrophysics::Galaxy AstrophysicsZenithmethods: data analysis Supporting material: FITS filesPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsIsotropyFísicaAstronomy and Astrophysics//purl.org/becyt/ford/1.3 [https]Astronomy and Astrophysicmethods: data analysisGalaxyfluxstarburst [Galaxies]Space and Planetary ScienceExperimental High Energy PhysicsActive galaxiesgalaxyAstroparticle physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]statistical
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Search for Quantum Black Hole Production in High-Invariant-MassLepton+JetFinal States UsingppCollisions ats=8  TeVand the ATLAS Detector

2014

This Letter presents a search for quantum black-hole production using 20.3 fb(-1) of data collected with the ATLAS detector in pp collisions at the LHC at root s = 8 TeV. The quantum black holes are assumed to decay into a final state characterized by a lepton (electron or muon) and a jet. In either channel, no event with a lepton-jet invariant mass of 3.5 TeV or more is observed, consistent with the expected background. Limits are set on the product of cross sections and branching fractions for the lepton + jet final states of quantum black holes produced in a search region for invariant masses above 1 TeV. The combined 95% confidence level upper limit on this product for quantum black hol…

PhysicsParticle physicsMuonLarge Hadron ColliderMesonAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyGeneral Physics and AstronomyElementary particleElectronNuclear physicsBlack holeGeneral Relativity and Quantum CosmologyHigh Energy Physics::ExperimentInvariant massLeptonPhysical Review Letters
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Dynamics of isolated-photon plus jet production in pp collisions at s=7 TeV with the ATLAS detector

2013

The dynamics of isolated-photon plus jet production in pp collisions at a centre-of-mass energy of 7 TeV has been studied with the ATLAS detector at the LHC using an integrated luminosity of 37 pb( ...

Quantum chromodynamicsPhysicsNuclear and High Energy PhysicsLarge Hadron ColliderPhotonPhysics::Instrumentation and Detectors010308 nuclear & particles physicsAtlas (topology)Atlas detectorAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::Phenomenology01 natural sciences7. Clean energyNuclear physics0103 physical sciencesHigh Energy Physics::ExperimentAngular dependence010306 general physicsBosonNuclear Physics B
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Search for long-lived, multi-charged particles in pp collisions at s=7 TeV using the ATLAS detector

2013

A search for highly ionising, penetrating particles with electric charges from |q| = 2e to 6e is performed using the ATLAS detector at the CERN Large Hadron Collider. Proton-proton collision data taken at sqrt(s)=7 TeV during the 2011 running period, corresponding to an integrated luminosity of 4.4 fb^-1, are analysed. No signal candidates are observed, and 95% confidence level cross-section upper limits are interpreted as mass-exclusion lower limits for a simplified Drell--Yan production model. In this model, masses are excluded from 50 GeV up to 430, 480, 490, 470 and 420 GeV for charges 2e, 3e, 4e, 5e and 6e, respectively.

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderLuminosity (scattering theory)010308 nuclear & particles physicsPhysics beyond the Standard ModelDrell–Yan processCharge (physics)7. Clean energy01 natural sciencesElectric chargeCharged particleNuclear physicsmedicine.anatomical_structureAtlas (anatomy)0103 physical sciencesmedicineHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsPhysics Letters B
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Search for charged Higgs bosons through the violation of lepton universality in t(t)over-bar events using pp collision data at root s=7 TeV with the …

2013

In several extensions of the Standard Model, the top quark can decay into a bottom quark and a light charged Higgs boson H [superscript +], t → bH [superscript +], in addition to the Standard Model decay t → bW. Since W bosons decay to the three lepton generations equally, while H [superscript +] may predominantly decay into τν, charged Higgs bosons can be searched for using the violation of lepton universality in top quark decays. The analysis in this paper is based on 4.6 fb[superscript −1] of proton-proton collision data at √s = 7 TeV collected by the ATLAS experiment at the Large Hadron Collider. Signatures containing leptons (e or μ) and/or a hadronically decaying τ (τ [subscript had])…

Nuclear and High Energy PhysicsTop quarkParticle physicsleptonsHiggs boson530 PhysicsCiências Naturais::Ciências Físicas:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesddc:500.201 natural sciences7. Clean energyBottom quark530High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Naturvetenskap0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530High Energy Physics010306 general physicsQCBosonPhysicsHIGGS BOSONLarge Hadron ColliderScience & TechnologyHadron-Hadron Scattering010308 nuclear & particles physicsBranching fractionSettore FIS/01 - Fisica SperimentaleATLAS experimentHigh Energy Physics::PhenomenologyFísicaNEW PHYSICSATLASHADRON-HADRON COLLISIONSExperimental High Energy PhysicsHiggs bosonComputingMethodologies_DOCUMENTANDTEXTPROCESSINGproton-proton collisionsHigh Energy Physics::ExperimentLHCNatural SciencesParticle Physics - ExperimentLepton
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Direct measurement of the muonic content of extensive air showers between 2× 1017 and 2×1018 eV at the Pierre Auger Observatory

2020

The hybrid design of the Pierre Auger Observatory allows for the measurement of the properties of extensive air showers initiated by ultra-high energy cosmic rays with unprecedented precision. By using an array of prototype underground muon detectors, we have performed the first direct measurement, by the Auger Collaboration, of the muon content of air showers between 2 × 10 17 and 2 × 10 18 eV. We have studied the energy evolution of the attenuation-corrected muon density, and compared it to predictions from air shower simulations. The observed densities are found to be larger than those predicted by models. We quantify this discrepancy by combining the measurements from the muon detector …

Muon detector ultra-high energy cosmic raysmuonsUHE Cosmic Rays
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Measurement of the production of neighbouring jets in lead–lead collisions at sNN=2.76 TeV with the ATLAS detector

2015

This Letter presents measurements of correlated production of nearby jets in Pb+Pb collisions at root s(NN) = 2.76 TeV using the ATLAS detector at the Large Hadron Collider. The measurement was performed using 0.14 nb(-1)of data recorded in 2011. The production of correlated jet pairs was quantified using the rate, R-Delta R, of "neighbouring" jets that accompany "test" jets within a given range of angular distance, Delta R, in the pseudorapidity-azimuthal angle plane. The jets were measured in the ATLAS calorimeter and were reconstructed using the anti-ktalgorithm with radius parameters d = 0.2, 0.3, and 0.4. R-Delta R was measured in different Pb+Pbcollision centrality bins, characterized…

PhysicsNuclear and High Energy PhysicsParticle physicsJet (fluid)Large Hadron ColliderAngular distanceHadronRadiusCalorimeterNuclear physicsTransverse planemedicine.anatomical_structureAtlas (anatomy)medicineHigh Energy Physics::ExperimentPhysics Letters B
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Search for long-lived stoppedR-hadrons decaying out of time withppcollisions using the ATLAS detector

2013

An updated search is performed for gluino, top squark, or bottom squark R-hadrons that have come to rest within the ATLAS calorimeter, and decay at some later time to hadronic jets and a neutralino, using 5.0 and 22.9 fb(-1) of pp collisions at 7 and 8 TeV, respectively. Candidate decay events are triggered in selected empty bunch crossings of the LHC in order to remove pp collision backgrounds. Selections based on jet shape and muon system activity are applied to discriminate signal events from cosmic ray and beam-halo muon backgrounds. In the absence of an excess of events, improved limits are set on gluino, stop, and sbottom masses for different decays, lifetimes, and neutralino masses. …

PhysicsNuclear and High Energy PhysicsParticle physicsGluinoLarge Hadron ColliderMuon010308 nuclear & particles physicsBranching fractionHigh Energy Physics::PhenomenologyHadronSupersymmetry01 natural sciences7. Clean energyNuclear physicsR-hadron0103 physical sciencesNeutralinoHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsPhysical Review D
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Performance of $b$-Jet Identification in the ATLAS Experiment

2016

We thank CERN for the very successful operation of the LHC, as well as the support staff from our institutions without whom ATLAS could not be operated efficiently. We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWFW and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile; CAS, MOST and NSFC, China; COLCIENCIAS, Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF, DNSRC and Lundbeck Foundation, Denmark; IN2P3-CNRS, CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, HGF, and MPG, Germany; GSRT, Greece; RGC, Hong Kong SAR, China; ISF, I-CORE and Benoziyo Center, Israel; INFN, Italy; MEXT an…

detector-systems performancePerformance of High Energy Physics Detectorsecondary [vertex]Elementary particle01 natural sciencesPARTONlaw.inventionSubatomär fysikCHANNELcluster findingscattering [p p]impact parameterGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)протон-протонные столкновенияQBLarge detector-systems performanceHigh energy physics detectorLarge Hadron ColliderLarge detector systems for particle and astroparticle physics; Large detector-systems performance; Pattern recognition cluster finding calibration and fitting methods; Performance of High Energy Physics Detectors; Instrumentation; Mathematical Physicstrack data analysisQUARK PAIR PRODUCTIONbottom [jet]CERN LHC CollPattern recognition cluster finding calibration and fitting method7000 GeV-cmscolliding beams [p p]performanceHADRONIC COLLISIONSCiências Naturais::Ciências FísicasLarge detectorFitting methodHigh energy physicATLAS LHC High Energy Physics510 MathematicsmuonDISTRIBUTIONSUncertainty analysis Astroparticle physicHigh Energy Physics010306 general physicsSystematic uncertainties AlgorithmsAstroparticle physicsCalibration and fitting methodsScience & Technology010308 nuclear & particles physicsLarge detector systems for particle and astroparticle physicsParticle acceleratorRangingPerformance of High Energy PhysicsCOLLIDERScorrelationExperimental High Energy PhysicsPerformance of High Energy Physics DetectorshadronATLAS детекторБольшой адронный коллайдерcharm [jet]Elementary particleHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)lawSubatomic Physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Detectors and Experimental TechniquesInstrumentationUncertainty analysisMathematical PhysicsPhysicsPattern recognition cluster finding calibration and fitting methods4. EducationATLAS experimentSettore FIS/01 - Fisica SperimentaleDetectorsflavor [jet]calibration and fitting methodsATLASLarge Hadron ColliderLarge detector systems for particle and astroparticle physics; Large; detector-systems performance; Pattern recognition cluster finding; calibration and fitting methods; Performance of High Energy Physics; Detectors; PRODUCTION CROSS-SECTION; QUARK PAIR PRODUCTION; ROOT-S=7 TEV; PARTON; DISTRIBUTIONS; HADRONIC COLLISIONS; MATRIX-ELEMENTS; LHC; COLLIDERS; DETECTOR; CHANNEL8. Economic growthCalibrationparticle identification [bottom]LHCImpact parameterParticle Physics - ExperimentParticle physicsdata analysis method530 Physics:Ciências Físicas [Ciências Naturais]FOS: Physical sciences530MATRIX-ELEMENTSparticle identification [charm]on-line [trigger]Pattern recognition0103 physical sciencesComplementary methodddc:610DETECTORROOT-S=7 TEVCluster findingFísicaLarge detector systems for particle and astroparticle physics; Large detector-systems performance; Pattern recognition cluster finding calibration and fitting methods; Performance of High Energy Physics DetectorsPattern recognition systemcalibrationtracksPRODUCTION CROSS-SECTIONefficiencyHadronLarge detector systems for particle and astroparticle physicLargeHigh Energy Physics::ExperimentStatistical correlationstatisticalexperimental results
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Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth

2014

The surface detector array of the Pierre Auger Observatory provides information about the longitudinal development of the muonic component of extensive air showers. Using the timing information from the flash analog-to-digital converter traces of surface detectors far from the shower core, it is possible to reconstruct a muon production depth distribution. We characterize the goodness of this reconstruction for zenith angles around 60° and different energies of the primary particle. From these distributions, we define Xμmax as the depth along the shower axis where the production of muons reaches maximum. We explore the potentiality of Xμmax as a useful observable to infer the mass compositi…

AstrofísicaPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsAstronomyCiencias Físicasmuonshadronic interaction modelsAstrophysics01 natural sciencesHigh Energy Physics - ExperimentAuger//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)Air showersProduction depthSURFACE DETECTOR ARRAY[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsHigh-Energy Cosmic Rays[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsDetectorAstrophysics::Instrumentation and Methods for Astrophysics[ SDU.ASTR.IM ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Pierre Auger ObservatoryObservableInstrumentation and Detectors (physics.ins-det)COSMIC-RAYSlongitudinal developmentCore (optical fiber)ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTAS[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Nuclear and High Energy Physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayNuclear physicscosmic rays[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesextensive air showers[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)ZenithCiencias ExactasPierre Auger ObservatoryMuon010308 nuclear & particles physics[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Física//purl.org/becyt/ford/1.3 [https]ASTROFÍSICA[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AstronomíaMODELExperimental High Energy PhysicsHigh Energy Physics::Experiment[ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][ PHYS.ASTR.IM ] Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]muonic componentSYSTEM
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A search for point sources of EeV photons

2014

Measurements of air showersmade using the hybrid technique developed with the fluorescence and surface detectors of the Pierre Auger Observatory allow a sensitive search for point sources of EeV photons anywhere in the exposed sky. A multivariate analysis reduces the background of hadronic cosmic rays. The search is sensitive to a declination band from −85º to +20º, in an energy range from 1017.3 eV to 1018.5 eV. No photon point source has been detected. An upper limit on the photon flux has been derived for every direction. The mean value of the energy flux limit that results from this, assuming a photon spectral index of −2, is 0.06 eV cm−2 s−1, and no celestial direction exceeds 0.25 eV …

Astrofísica[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhotonPoint sourcemedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaAstronomyEnergy fluxFOS: Physical sciencesCosmic rayAstrophysics7. Clean energycosmic raysCiencias Exactasmedia_commonPhysicsPierre Auger ObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)Spectral index[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsFísicaAstronomy and AstrophysicsRadiación cósmicamethods: data analysisGalaxy13. Climate actionSpace and Planetary ScienceSkyastroparticle physicsExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstroparticle physicsAstrophysics - High Energy Astrophysical Phenomena
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Centrality, rapidity, and transverse momentum dependence of isolated prompt photon production in lead-lead collisions atsNN=2.76TeV measured with the…

2016

Prompt photon production in root S-NN = 2.76-TeV Pb + Pb collisions has been measured by the ATLAS experiment at the Large Hadron Collider using data collected in 2011 with an integrated luminosity ...

PhysicsParticle physicsPhotonLarge Hadron ColliderLuminosity (scattering theory)Physics::Instrumentation and Detectors010308 nuclear & particles physicsAtlas detectorAstrophysics::High Energy Astrophysical PhenomenaATLAS experiment01 natural sciences7. Clean energyNuclear physics0103 physical sciencesTransverse momentumHigh Energy Physics::ExperimentRapidityNuclear Experiment010306 general physicsPhysical Review C
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Studies on the response of a water-Cherenkov detector of the Pierre Auger Observatory to atmospheric muons using an RPC hodoscope

2020

Extensive air showers, originating from ultra-high energy cosmic rays, have been successfully measured through the use of arrays of water-Cherenkov detectors (WCDs). Sophisticated analyses exploiting WCD data have made it possible to demonstrate that shower simulations, based on different hadronic-interaction models, cannot reproduce the observed number of muons at the ground. The accurate knowledge of the WCD response to muons is paramount in establishing the exact level of this discrepancy. In this work, we report on a study of the response of a WCD of the Pierre Auger Observatory to atmospheric muons performed with a hodoscope made of resistive plate chambers (RPCs), enabling us to selec…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsAstronomy01 natural sciences030218 nuclear medicine & medical imaginglaw.invention0302 clinical medicinelawObservatoryatmosphere [muon]Instrumentationphysics.ins-detMathematical PhysicsLarge detector-systems performancePhysicsInstrumentation et méthodes en physiquePerformance of high energy physics detectorsData reduction methods; Large detector systems for particle and astroparticle physics; Large detector-systems performance; Performance of high energy physics detectorsDetectorSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsresistive plate chamberInstrumentation and Detectors (physics.ins-det)trajectory [muon]Augerobservatorymuon: atmosphereAstrophysics - Instrumentation and Methods for AstrophysicsData reduction methodsatmosphere [showers]Cherenkov detectorairCherenkov counter: waterAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencesCosmic raymuon: trajectoryNuclear physics03 medical and health sciencesHodoscopeData reduction method0103 physical sciencesCalibrationHigh Energy Physicsddc:610cosmic radiation: UHE[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Instrumentation and Methods for Astrophysics (astro-ph.IM)ZenithCiencias ExactasPierre Auger Observatoryshowers: atmosphere010308 nuclear & particles physicsLarge detector systems for particle and astroparticle physicswater [Cherenkov counter]hodoscopeFísicaAutres mathématiquesstabilitycalibrationData reduction methods Large detector systems for particle and astroparticle physics Large detector-systems performance Performance of High Energy Physics DetectorsExperimental High Energy PhysicsLarge detector systems for particle and astroparticle physicHigh Energy Physics::ExperimentRAIOS CÓSMICOSastro-ph.IM
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Measurement of the average shape of longitudinal profiles of cosmic-ray air showers at the Pierre Auger Observatory

2019

The profile of the longitudinal development of showers produced by ultra-high energy cosmic rays carries information related to the interaction properties of the primary particles with atmospheric nuclei. In this work, we present the first measurement of the average shower profile in traversed atmospheric depth at the Pierre Auger Observatory. The shapes of profiles are well reproduced by the Gaisser-Hillas parametrization within the range studied, for E>10 17.8 eV .A detailed analysis of the systematic uncertainties is performed using ten years of data and a full detector simulation. The average shape is quantified using two variables related to the width and asymmetry of the profile, and …

p: showersphoton: Cherenkovinteraction: modelAstronomyHadronpiastro-ph.HE; astro-ph.HE01 natural sciencesnitrogenironParametrization (atmospheric modeling)Monte Carlomedia_commonPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Range (particle radiation)photomultiplierSettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsDETETOREScosmic rays detectors; ultra high energy cosmic rays; Astronomy and AstrophysicsAugerobservatorycosmic rays detectorscosmic rays detectors; ultra high energy cosmic raysgeometricalAstrophysics - High Energy Astrophysical PhenomenaasymmetrylongitudinalCherenkov counter: waterairmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayheliumultra high energy cosmic raysnucleus: atmosphereAsymmetry0103 physical sciencesHigh Energy Physicscosmic radiation: UHEcosmic rays detectorFLUORESCENCEAstrophysiquePierre Auger Observatoryelectron positronshowers: atmosphere010308 nuclear & particles physicsbackgrounddetector: surfaceshowers: spatial distributionparametrizationAstronomy and AstrophysicsAstronomieComputational physics13. Climate actiongamma rayExperimental High Energy Physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)Journal of Cosmology and Astroparticle Physics
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Search for single b⁎-quark production with the ATLAS detector at s=7 TeV

2013

The results of a search for an excited bottom-quark b* in pp collisions at root s = 7 TeV, using 4.7 fb(-1) of data collected by the ATLAS detector at the LHC are presented. In the model studied, a ...

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderPhysics::Instrumentation and Detectors010308 nuclear & particles physicsAtlas (topology)Atlas detectorHigh Energy Physics::PhenomenologyElectroweak interaction01 natural sciencesBottom quarkNuclear physicsPair production0103 physical sciencesHigh Energy Physics::ExperimentStatistical analysis010306 general physicsLeptonPhysics Letters B
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Origin of atmospheric aerosols at the Pierre Auger Observatory using studies of air mass trajectories in South America

2014

The Pierre Auger Observatory is making significant contributions towards understanding the nature and origin of ultra-high energy cosmic rays. One of its main challenges is the monitoring of the atmosphere, both in terms of its state variables and its optical properties. The aim of this work is to analyze aerosol optical depth $\tau_{\rm a}(z)$ values measured from 2004 to 2012 at the observatory, which is located in a remote and relatively unstudied area of the Pampa Amarilla, Argentina. The aerosol optical depth is in average quite low - annual mean $\tau_{\rm a}(3.5~{\rm km})\sim 0.04$ - and shows a seasonal trend with a winter minimum - $\tau_{\rm a}(3.5~{\rm km})\sim 0.03$ -, and a sum…

Atmospheric Science010504 meteorology & atmospheric sciencesaerosolAstronomyObservatoriesAerosol concentrationAir pollution010501 environmental sciencesAtmospheric sciencesmedicine.disease_causeAerosols Atmospheric aerosols Augers Cosmic rays Observatories; Aerosol concentration Aerosol optical depths Air mass Atmospheric effects GDAS HYSPLIT Pierre Auger observatory Ultra high-energy cosmic rays; Meteorology; aerosol property air mass concentration (composition) optical depth trajectory urban area urban atmosphere; Argentina01 natural sciencesoptical depthObservatory11. Sustainabilityddc:550MeteorologiaAugersmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsconcentration (composition)Physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]urban atmosphereAtmospheric effectsGDASAtmospheric aerosolscosmic ray; aerosol; air masses; atmospheric effectPhysics - Atmospheric and Oceanic PhysicstrajectoryClimatologyComputingMethodologies_DOCUMENTANDTEXTPROCESSINGHYSPLITAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaPollutionaerosol property[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]media_common.quotation_subjectatmospheric effectArgentinaFOS: Physical sciencesHYSPLITAtmósferaAtmosphereMeteorologycosmic raysmedicineAerosol optical depthsInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysCiencias ExactasAir mass0105 earth and related environmental sciencesAerosols[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Pierre Auger ObservatoryFísicaASTROFÍSICA[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Aerosol13. Climate actionExperimental High Energy PhysicsAtmospheric and Oceanic Physics (physics.ao-ph)Pierre Auger observatoryAir massair massesUltra high-energy cosmic raysurban area
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Measurement with the ATLAS detector of multi-particle azimuthal correlations in p+Pb collisions at sNN=5.02 TeV

2013

In order to study further the long-range correlations ("ridge") observed recently in p + Pb collisions at root s(NN) = 5.02 TeV, the second-order azimuthal anisotropy parameter ofcharged particles, ...

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsAtlas detectorElliptic flowRidge (differential geometry)01 natural sciencesAzimuthNuclear physicsmedicine.anatomical_structureAtlas (anatomy)0103 physical sciencesmedicineParticleNuclear Experiment010306 general physicsPhysics Letters B
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Reconstruction of inclined air showers detected with the Pierre Auger Observatory

2014

We describe the method devised to reconstruct inclined cosmic-ray air showers with zenith angles greater than $60^\circ$ detected with the surface array of the Pierre Auger Observatory. The measured signals at the ground level are fitted to muon density distributions predicted with atmospheric cascade models to obtain the relative shower size as an overall normalization parameter. The method is evaluated using simulated showers to test its performance. The energy of the cosmic rays is calibrated using a sub-sample of events reconstructed with both the fluorescence and surface array techniques. The reconstruction method described here provides the basis of complementary analyses including an…

AstrofísicaAstronomyCiencias Físicas01 natural sciencesultra high energy cosmic rayHigh Energy Physics - Experiment//purl.org/becyt/ford/1 [https]ENERGYHigh Energy Physics - Experiment (hep-ex)EXPERIMENTS[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]HIGHPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryCascadeComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTASNormalization (statistics)[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]COSMICAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic ray[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesEnergy spectrum010306 general physicsULTRAZenithShower reconstructionPierre Auger ObservatoryMuon010308 nuclear & particles physics[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FísicaAstronomy and Astrophysics//purl.org/becyt/ford/1.3 [https]Ultra-high energy cosmic raysRAYSComputational physicsAstronomíaInclined extensive air showersExperimental High Energy Physicscosmic ray experiments[ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Energy (signal processing)Journal of Cosmology and Astroparticle Physics
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Description of atmospheric conditions at the Pierre Auger Observatory using the Global Data Assimilation System (GDAS)

2012

Atmospheric conditions at the site of a cosmic ray observatory must be known for reconstructing observed extensive air showers. The Global Data Assimilation System (GDAS) is a global atmospheric model predicated on meteorological measurements and numerical weather predictions. GDAS provides altitude-dependent profiles of the main state variables of the atmosphere like temperature, pressure, and humidity. The original data and their application to the air shower reconstruction of the Pierre Auger Observatory are described. By comparisons with radiosonde and weather station measurements obtained on-site in Malargüe and averaged monthly models, the utility of the GDAS data is shown.

AstronomyAtmospheric modelAtmospheric monitoringAtmospheric sciencesCosmic Rays Shower01 natural scienceslaw.inventionData assimilationlawcosmic rays; extensive air showers; atmospheric monitoring; atmospheric modelsDEPENDENCEATMOSFERA (OBSERVAÇÃO)TEMPERATUREPhysics::Atmospheric and Oceanic PhysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[PHYS]Physics [physics]Cascada atmosférica extensaOPTICAL DEPTH[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryAtmospheric temperatureRadiación cósmicaAtmosphere of EarthComputingMethodologies_DOCUMENTANDTEXTPROCESSINGRadiosondeFísica nuclearREFRACTIVE-INDEXAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]MeteorologyAtmospheric MonitoringAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic Rays ShowersEXTENSIVE AIR-SHOWERSCosmic RayAtmósferaWeather stationAtmospheric models0103 physical sciencesExtensive air showers010306 general physicsCosmic raysDETECTORCiencias ExactasPierre Auger ObservatoryAtmospheric models010308 nuclear & particles physicsFísicaAstronomy and Astrophysics13. Climate actionExperimental High Energy PhysicsEMISSION[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Observation of top-quark pair production in association with a photon and measurement of thett¯γproduction cross section inppcollisions ats=7TeV usin…

2015

A search is performed for top-quark pairs (t (t) over bar) produced together with a photon (gamma) with transverse energy greater than 20 GeV using a sample of t (t) over bar candidate events in final states with jets, missing transverse momentum, and one isolated electron or muon. The data set used corresponds to an integrated luminosity of 4.59 fb(-1) of proton-proton collisions at a center-of-mass energy of 7 TeV recorded by the ATLAS detector at the CERN Large Hadron Collider. In total, 140 and 222 t (t) over bar gamma candidate events are observed in the electron and muon channels, to be compared to the expectation of 79 +/- 26 and 120 +/- 39 non-t (t) over bar gamma background events,…

QuarkPhysicsNuclear and High Energy PhysicsTop quarkParticle physicsMuonLarge Hadron ColliderBranching fractionHigh Energy Physics::PhenomenologyParton7. Clean energyNuclear physicsPair productionHigh Energy Physics::ExperimentLeptonPhysical Review D
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Nanosecond-level time synchronization of autonomous radio detector stations for extensive air showers

2016

To exploit the full potential of radio measurements of cosmic-ray air showers at MHz frequencies, a detector timing synchronization within 1 ns is needed. Large distributed radio detector arrays such as the Auger Engineering Radio Array (AERA) rely on timing via the Global Positioning System (GPS) for the synchronization of individual detector station clocks. Unfortunately, GPS timing is expected to have an accuracy no better than about 5 ns. In practice, in particular in AERA, the GPS clocks exhibit drifts on the order of tens of ns. We developed a technique to correct for the GPS drifts, and an independent method is used to cross-check that indeed we reach a nanosecond-scale timing accura…

Physics - Instrumentation and DetectorsAutomatic dependent surveillance-broadcastComputer scienceCiencias FísicasAstronomyDetector alignment and calibration methods (lasers sources particle-beams)Calibration and fitting methods; Cluster finding; Detector alignment and calibration methods (lasers sources particle-beams); Pattern recognition; Timing detectors01 natural sciencesTiming detectorsSynchronizationHigh Energy Physics - Experiment//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)Sine wave[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]InstrumentationMathematical PhysicsTransmitterDetectorSettore FIS/01 - Fisica Sperimentaleparticle-beams)Instrumentation and Detectors (physics.ins-det)Pattern recognition cluster finding calibration and fitting methodGlobal Positioning SystemComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearCIENCIAS NATURALES Y EXACTASsourcesReal-time computingFOS: Physical sciencesCalibration and fitting methodClustersPattern recognition0103 physical sciencesCalibrationHigh Energy Physics010306 general physicsCiencias ExactasCalibration and fitting methods010308 nuclear & particles physicsbusiness.industryCluster findingFísicaAstroparticles//purl.org/becyt/ford/1.3 [https]PhaserAstronomíaDetector alignment and calibration methods (lasersTiming detectorPierre AugerExperimental High Energy PhysicsRECONHECIMENTO DE PADRÕESCalibration and fitting methods; Cluster finding; Detector alignment and calibration methods (lasers sources particle-beams); Pattern recognition; Timing detectors; Instrumentation; Mathematical PhysicsbusinessJournal of Instrumentation
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Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory

2013

We derive lower bounds on the density of sources of ultra-high energy cosmic rays from the lack of significant clustering in the arrival directions of the highest energy events detected at the Pierre Auger Observatory. The density of uniformly distributed sources of equal intrinsic intensity was found to be larger than similar to (0.06 – 5) x 10(-4) Mpc(-3) at 95% CL, depending on the magnitude of the magnetic defections. Similar bounds, in the range (0.2 – 7) x 10(-4) Mpc(-3), were obtained for sources following the local matter distribution.

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Ciencias FísicasAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesultra-high energy cosmic raysCosmic rayAstrophysicsultra high energy cosmic raysAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAugerNUMBERObservatoryCosmic ray experiments0103 physical sciencesultra-high energy cosmic rayUltra-high-energy cosmic ray010303 astronomy & astrophysicsDETECTORLuminosity functionPierre Auger ObservatoryPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)FÍSICA DE PARTÍCULASRange (particle radiation)SPECTRUMCosmologia010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astronomy and AstrophysicsUltra high energy cosmic raysAstronomíaLUMINOSITY FUNCTIONMagnitude (astronomy)Experimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGAstronomiaFísica nuclearcosmic ray experimentsAstrophysics - High Energy Astrophysical Phenomenacosmic ray experiments; ultra high energy cosmic raysCIENCIAS NATURALES Y EXACTAS
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