0000000000104798

AUTHOR

A. Filipčič

showing 102 related works from this author

Measurement of the W→τντ cross section in pp collisions at s=7 TeV with the ATLAS experiment

2012

The cross section for the production of W bosons with subsequent decay W to tau nu is measured with the ATLAS detector at the LHC. The analysis is based on a data sample that was recorded in 2010 at a proton-proton center-of-mass energy of sqrt(s) = 7 TeV and corresponds to an integrated luminosity of 34 pb^-1. The cross section is measured in a region of high detector acceptance and then extrapolated to the full phase space. The product of the total W production cross section and the W to tau nu branching ratio is measured to be 11.1 +/- 0.3 (stat) +/- 1.7 (syst) +/- 0.4 (lumi) nb.

PhysicsNuclear and High Energy PhysicsParticle physicsLuminosity (scattering theory)Large Hadron Collider010308 nuclear & particles physicsBranching fractionATLAS experiment7. Clean energy01 natural sciencesStandard ModelNuclear physicsCross section (physics)medicine.anatomical_structureAtlas (anatomy)0103 physical sciencesmedicineHigh Energy Physics::Experiment010306 general physicsBosonPhysics Letters B
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Search for light top squark pair production in final states with leptons and b-jets with the ATLAS detector in s=7 TeV proton–proton collisions

2013

The results of a search for pair production of light top squarks are presented, using 4.7 fb(-1) of root s = 7 TeV proton-proton collisions collected with the ATLAS detector at the Large Hadron Collider. This search targets top squarks with masses similar to, or lighter than, the top quark mass. Final states containing exclusively one or two leptons (e, mu), large missing transverse momentum, light-flavour jets and b-jets are used to reconstruct the top squark pair system. Event-based mass scale variables are used to separate the signal from a large t (t) over bar background. No excess over the Standard Model expectations is found. The results are interpreted in the framework of the Minimal…

PhysicsNuclear and High Energy PhysicsTop quarkParticle physicsStop squarkLarge Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySupersymmetry01 natural sciencesNuclear physicsPair production0103 physical sciencesNeutralinoHigh Energy Physics::Experiment010306 general physicsLeptonMinimal Supersymmetric Standard ModelPhysics Letters B
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Measurement of the differential cross-sections of inclusive, prompt and non-prompt J/ψ production in proton–proton collisions at s=7 TeV

2011

The inclusive J/psi production cross-section and fraction of J/psi mesons produced in B-hadron decays are measured in proton proton collisions at root s = 7 TeV with the ATLAS detector at the LHC, as a function of the transverse momentum and rapidity of the J/psi, using 2.3 pb(-1) of integrated luminosity. The cross-section is measured from a minimum P-T of 1 GeV to a maximum of 70 GeV and for rapidities within vertical bar y vertical bar < 2.4 giving the widest reach of any measurement of J/psi production to date. The differential production cross-sections of prompt and non-prompt J/psi are separately determined and are compared to Colour Singlet NNLO*, Colour Evaporation Model, and FONLL …

Quantum chromodynamicsPhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderLuminosity (scattering theory)ProtonMeson010308 nuclear & particles physicsAtlas detector01 natural sciencesNuclear physicsmedicine.anatomical_structureAtlas (anatomy)0103 physical sciencesmedicineHigh Energy Physics::ExperimentRapidityNuclear Experiment010306 general physicsNuclear Physics B
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Search for a Standard Model Higgs boson in the mass range 200–600 GeV in the H→ZZ→ℓ+ℓ−qq¯ decay channel with the ATLAS detector

2012

A search for a heavy Standard Model Higgs boson decaying via H -> ZZ -> l(+)l(-)q (q) over bar, where l = e or mu, is presented. The search uses a data set of pp collisions at root s = 7 TeV, ...

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsAtlas detectorHigh Energy Physics::Phenomenology01 natural sciencesNuclear physics0103 physical sciencesLarge Electron–Positron ColliderBibliographyHiggs bosonHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsPhysics Letters B
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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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Measurement of exclusive γγ→ℓ+ℓ− production in proton–proton collisions at s=7 TeV with the ATLAS detector

2015

This Letter reports a measurement of the exclusive gamma gamma -> l(+)l(-) (l = e, mu) cross-section in proton-proton collisions at a centre-of-mass energy of 7 TeV by the ATLAS experiment at the LHC, based on an integrated luminosity of 4.6 fb(-1). For the electron or muon pairs satisfying exclusive selection criteria, a fit to the dilepton acoplanarity distribution is used to extract the fiducial cross-sections. The cross-section in the electron channel is determined to be sigma(excl)(gamma gamma -> e+e-) = 0.428 +/- 0.035 (stat.) +/- 0.018 (syst.) pbfor a phase-space region with invariant mass of the electron pairs greater than 24GeV, in which both electrons have transverse momentum p(T)…

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderMuonProtonATLAS experimentAcoplanarityNuclear physicsmedicine.anatomical_structureAtlas (anatomy)PseudorapiditymedicineHigh Energy Physics::ExperimentInvariant massNuclear ExperimentPhysics Letters B
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Measurement of the energy spectrum of cosmic rays above 10^18 eV using the Pierre Auger Observatory

2010

We report a measurement of the flux of cosmic rays with unprecedented precision and Statistics using the Pierre Auger Observatory Based on fluorescence observations in coincidence with at least one Surface detector we derive a spectrum for energies above 10(18) eV We also update the previously published energy spectrum obtained with the surface detector array The two spectra are combined addressing the systematic uncertainties and, in particular. the influence of the energy resolution on the spectral shape The spectrum can be described by a broken power law E-gamma with index gamma = 3 3 below the ankle which is measured at log(10)(E-ankle/eV) = 18 6 Above the ankle the spectrum is describe…

Nuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Radiación CósmicaAstronomyAstrophysics::High Energy Astrophysical Phenomenaenergy spectrumFluxFOS: Physical sciencesCosmic rayAstrophysicsElectronSURFACE DETECTORUPPER LIMITENERGIAPHOTON FRACTION01 natural sciencesSpectral lineAugerNuclear physicscosmic raysObservatorySHOWERS0103 physical sciencesHigh-Energy Cosmic Ray010306 general physicsCosmic raysCiencias ExactasPhysicsPierre Auger ObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Spectral densityFísicaPierre Auger ObservatoryCosmic rayELECTRONS3. Good healthPierre Auger Observatory; Cosmic rays; Energy spectrumSIMULATIONExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFluorescenciaARRAYFísica nuclearEnergy spectrumAstrophysics - High Energy Astrophysical PhenomenaSYSTEM
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Measurement of the cross-section for b-jets produced in association with a Z boson at s=7 TeV with the ATLAS detector

2012

A measurement is presented of the inclusive cross-section for b-jet production in association with a Z boson in pp collisions at a centre-of-mass energy of root s = 7 TeV. The analysis uses the data sample collected by the ATLAS experiment in 2010, corresponding to an integrated luminosity of approximately 36 pb(-1). The event selection requires a Z boson decaying into high P-T electrons or muons, and at least one b-jet, identified by its displaced vertex, with transverse momentum p(T) > 25 GeV and rapidity vertical bar y vertical bar < 2.1. After subtraction of background processes, the yield is extracted from the vertex mass distribution of the candidate b-jets. The ratio of this cross-se…

PhysicsQuantum chromodynamicsNuclear and High Energy PhysicsParticle physicsMuonLarge Hadron ColliderMass distribution010308 nuclear & particles physicsATLAS experimentPerturbative QCD01 natural sciencesNuclear physics0103 physical sciencesHigh Energy Physics::ExperimentRapidity010306 general physicsBosonPhysics 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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Measurement of the transverse momentum distribution of Z/γ⁎ bosons in proton–proton collisions at s=7 TeV with the ATLAS detector

2011

A measurement of the Z/gamma* transverse momentum (p(T)(Z)) distribution in proton-proton collisions at root s = 7 TeV is presented using Z/gamma* -> e(+)e(-) and Z/gamma* -> mu(+)mu(-) decay ...

Quantum chromodynamicsPhysicsNuclear and High Energy PhysicsParticle physicsMuonProton010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryMonte Carlo methodPerturbative QCDElectron01 natural sciencesNuclear physicsmedicine.anatomical_structureAtlas (anatomy)0103 physical sciencesmedicinePhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsBosonPhysics Letters B
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Measurement of the transverse momentum distribution ofWbosons inppcollisions ats=7  TeVwith the ATLAS detector

2012

This paper describes a measurement of the W boson transverse momentum distribution using ATLAS pp collision data from the 2010 run of the LHC at root s = 7 TeV, corresponding to an integrated lumin ...

PhysicsNuclear and High Energy PhysicsParticle physicsMuonLuminosity (scattering theory)Large Hadron ColliderPhysics::Instrumentation and Detectors010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyElementary particleFermion01 natural sciencesNuclear physicsmedicine.anatomical_structureAtlas (anatomy)0103 physical sciencesmedicineNuclear Experiment010306 general physicsBosonLeptonPhysical Review D
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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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Measurements ofWγandZγproduction inppcollisions ats=7  TeVwith the ATLAS detector at the LHC

2013

The integrated and differential fiducial cross sections for the production of a W or Z boson in association with a high-energy photon are measured using pp collisions at root s = 7 TeV. The analyse ...

QuarkPhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderPhoton010308 nuclear & particles physicsAtlas detectorHigh Energy Physics::PhenomenologyTevatronTechnicolor01 natural sciences7. Clean energyNuclear physicsmedicine.anatomical_structureAtlas (anatomy)0103 physical sciencesmedicine010306 general physicsBosonPhysical Review D
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Search for new physics in the dijet mass distribution using 1 fb−1 of pp collision data at s=7 TeV collected by the ATLAS detector

2012

Invariant mass distributions of jet pairs (dijets) produced in LHC proton-proton collisions at a centre-of-mass energy root s = 7 TeV have been studied using a data set corresponding to an integrat ...

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderMass distribution010308 nuclear & particles physicsAtlas detectorAstrophysics::High Energy Astrophysical PhenomenaPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologyCollision01 natural sciencesNuclear physicsChiral color0103 physical sciencesPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentInvariant massNuclear Experiment010306 general physicsPhysics Letters B
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Measurement of the cross section for the production of a W boson in association with b-jets in pp collisions at s=7 TeV with the ATLAS detector

2012

A measurement is presented of the cross section for the production of a W boson with one or two jets, of which at least one must be a b-jet, in pp collisions at root s = 7 TeV. Production via top d ...

PhysicsQuantum chromodynamicsNuclear and High Energy PhysicsParticle physicsMuonLarge Hadron Collider010308 nuclear & particles physicsAtlas detectorAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyElectron01 natural sciencesNuclear physics0103 physical sciencesTransverse momentumHigh Energy Physics::ExperimentRapidity010306 general physicsLeptonPhysics Letters B
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Measurement of the top quark pair production cross section in pp collisions at s=7 TeV in dilepton final states with ATLAS

2012

A measurement of the production cross section of top quark pairs (ttbar) in proton-proton collisions at a center-of-mass energy of 7 TeV recorded with the ATLAS detector at the Large Hadron Collider is reported. Candidate events are selected in the dilepton topology with large missing transverse energy and at least two jets. Using a data sample corresponding to an integrated luminosity of 35 pb^-1, a ttbar production cross section of 171 +/- 20(stat.) +/- 14(syst.) +8-6(lum.) pb is measured for an assumed top quark mass of 172.5 GeV. A second measurement requiring at least one jet identified as coming from a b quark yields a comparable result, demonstrating that the dilepton final states ar…

QuarkPhysicsNuclear and High Energy PhysicsParticle physicsTop quarkLarge Hadron Collider010308 nuclear & particles physicsAtlas (topology)Nuclear TheoryHigh Energy Physics::PhenomenologyHadron01 natural sciences7. Clean energyBottom quarkNuclear physicsTransverse planePair production0103 physical sciencesHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsPhysics Letters B
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Search for the Standard Model Higgs boson in the decay channel H→ZZ(⁎)→4ℓ with the ATLAS detector

2011

A search for the Standard Model Higgs boson in the decay channel H -> ZZ(()*()) l(+)l(-)l'l'(-), where l = e, mu, is presented. Proton-proton collision data at root s = 7 TeV recorded with the A ...

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsBranching fractionNuclear TheoryHigh Energy Physics::PhenomenologyElementary particle01 natural sciencesNuclear physics0103 physical sciencesHiggs bosonPhysics::Accelerator PhysicsGrand Unified TheoryHigh Energy Physics::ExperimentQuantum field theoryNuclear Experiment010306 general physicsLeptonBosonPhysics Letters B
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Measurement of the t-channel single top-quark production cross section in pp collisions at s=7 TeV with the ATLAS detector

2012

We report a measurement of the cross section of single top-quark production in the t-channel using 1.04 fb -1 of pp collision data at s=7 TeV recorded with the ATLAS detector at the LHC. Selected e ...

PhysicsNuclear and High Energy PhysicsTop quarkParticle physicsLarge Hadron ColliderChannel (digital image)Physics::Instrumentation and Detectors010308 nuclear & particles physicsCabibbo–Kobayashi–Maskawa matrixAtlas detectorHigh Energy Physics::Phenomenology01 natural sciencesCross section (physics)medicine.anatomical_structureAtlas (anatomy)0103 physical sciencesmedicineHigh Energy Physics::ExperimentProduction (computer science)010306 general physicsPhysics Letters B
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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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Search for diphoton events with large missing transverse momentum in 1 fb−1 of 7 TeV proton–proton collision data with the ATLAS detector

2012

A search for diphoton events with large missing transverse momentum has been performed using 1.07 fb(-1) of proton-proton collision data at root s = 7 TeV recorded with the ATLAS detector. No excess of events was observed above the Standard Model prediction and 95% Confidence Level (CL) upper limits are set on the production cross section for new physics. The limits depend on each model parameter space and vary as follows: sigma < (22-129) fb in the context of a generalised model of gauge-mediated supersymmetry breaking (GGM) with a bino-like lightest neutralino, sigma < (27-91) fb in the context of a minimal model of gauge-mediated supersymmetry breaking (SPS8), and sigma < (15-27) fb in t…

PhysicsNuclear and High Energy PhysicsGluinoParticle physics010308 nuclear & particles physicsPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologySupersymmetryLambda01 natural sciencesSupersymmetry breakingUniversal extra dimensionNuclear physics0103 physical sciencesNeutralinoHigh Energy Physics::Experiment010306 general physicsPhenomenology (particle physics)Physics Letters B
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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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Search for first generation scalar leptoquarks in pp collisions at s=7 TeV with the ATLAS detector

2012

We report a search for first generation scalar leptoquarks using 1.03 fb(-1) of proton-proton collisions data produced by the Large Hadron Collider at root s = 7 TeV and recorded by the ATLAS experiment. Leptoquarks are sought via their decay into an electron or neutrino and a quark, producing events with two oppositely charged electrons and at least two jets, or events with an electron, missing transverse momentum and at least two jets. Control data samples are used to validate background predictions from Monte Carlo simulation. In the signal region, the observed event yields are consistent with the background expectations. We exclude at 95% confidence level the production of first generat…

QuarkPhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsBranching fractionHigh Energy Physics::PhenomenologyATLAS experimentHERA01 natural sciencesNuclear physics0103 physical sciencesHigh Energy Physics::ExperimentLeptoquarkNeutrino010306 general physicsLeptonPhysics Letters B
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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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Searches for heavy long-lived sleptons and R-hadrons with the ATLAS detector in pp collisions at

2013

A search for long-lived particles is performed using a data sample of 4.7 fb(-1) from proton-proton collisions at a centre-of-mass energy. root s = 7 TeV collected by the ATLAS detector at the LHC. No excess is observed above the estimated background and lower limits, at 95% confidence level, are set on the mass of the long-lived particles in different scenarios, based on their possible interactions in the inner detector, the calorimeters and the muon spectrometer. Long-lived staus in gauge-mediated SUSY-breaking models are excluded up to a mass of 300 GeV for tan beta = 5-20. Directly produced long-lived sleptons are excluded up to a mass of 278 GeV. R-hadrons, composites of gluino (stop, …

PhysicsQuarkNuclear and High Energy PhysicsParticle physicsGluinoLarge Hadron Collider010308 nuclear & particles physicsPhysics::Instrumentation and Detectors530 PhysicsHadronDetectorHigh Energy Physics::Phenomenology7. Clean energy01 natural sciencesNuclear physicsPionR-hadronHADRON-HADRON COLLISIONS0103 physical sciencesHigh Energy Physics::Experiment010306 general physicsNuclear ExperimentSUPERSYMMETRYLepton
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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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Measurement of the top quark pair cross section with ATLAS in pp collisions at s=7 TeV using final states with an electron or a muon and a hadronical…

2012

Measurement of the top quark pair cross section with ATLAS in pp collisions at root s=7 TeV using final states with an electron or a muon and a hadronically decaying tau lepton

PhysicsNuclear and High Energy PhysicsTop quarkParticle physicsMuonPhysics::Instrumentation and Detectors010308 nuclear & particles physicsAtlas detectorAtlas (topology)High Energy Physics::PhenomenologyElectron01 natural sciencesNuclear physics0103 physical sciencesPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsLeptonPhysics Letters B
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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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Search for Supersymmetry Using Final States with One Lepton, Jets, and Missing Transverse Momentum with the ATLAS Detector ins=7  TeVppCollisions

2011

This Letter presents the first search for supersymmetry in final states containing one isolated electron or muon, jets, and missing transverse momentum from sqrt{s} = 7 TeV proton-proton collisions at the LHC. The data were recorded by the ATLAS experiment during 2010 and correspond to a total integrated luminosity of 35 pb-1. No excess above the standard model background expectation is observed. Limits are set on the parameters of the minimal supergravity framework, extending previous limits. For A_0 = 0 GeV, tan beta = 3, mu > 0 and for equal squark and gluino masses, gluino masses below 700 GeV are excluded at 95% confidence level.

PhysicsGluinoParticle physicsMuonLarge Hadron Collider010308 nuclear & particles physicsSupergravityHigh Energy Physics::PhenomenologyATLAS experimentGeneral Physics and AstronomySupersymmetry01 natural sciencesNuclear physics0103 physical sciencesGrand Unified TheoryHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsLeptonPhysical Review Letters
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Search for new phenomena with the monojet and missing transverse momentum signature using the ATLAS detector in s=7TeV proton–proton collisions

2011

A search for new phenomena in events featuring a high energy jet and large missing transverse momentum in proton-proton collisions at root s = 7 TeV is presented using a dataset corresponding to an integrated luminosity of 33 pb(-1) recorded with the ATLAS detector at the Large Hadron Collider. The number of observed events is consistent with the Standard Model prediction. This result is interpreted in terms of limits on a model of Large Extra Dimensions. (C) 2011 CERN. Published by Elsevier B.V. All rights reserved.

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderLuminosity (scattering theory)Proton010308 nuclear & particles physicsHadronJet (particle physics)01 natural sciencesStandard ModelNuclear physicsmedicine.anatomical_structureAtlas (anatomy)0103 physical sciencesmedicinePhysics::Accelerator PhysicsLarge extra dimensionHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsPhysics Letters B
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Limit on the diffuse flux of ultrahigh energy tau neutrinos with the surface detector of the Pierre Auger Observatory

2009

Data collected at the Pierre Auger Observatory are used to establish an upper limit on the diffuse flux of tau neutrinos in the cosmic radiation. Earth-skimming ντ may interact in the Earth's crust and produce a τ lepton by means of charged-current interactions. The τ lepton may emerge from the Earth and decay in the atmosphere to produce a nearly horizontal shower with a typical signature, a persistent electromagnetic component even at very large atmospheric depths. The search procedure to select events induced by τ decays against the background of normal showers induced by cosmic rays is described. The method used to compute the exposure for a detector continuously growing with time is de…

ACTIVE GALACTIC NUCLEIASTROPHYSICS[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Nuclear and High Energy PhysicsActive galactic nucleusPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayPROPAGATIONAstrophysics7. Clean energy01 natural sciencesLeptonSpectral lineSettore FIS/04 - Fisica Nucleare e SubnucleareAugerSEARCHTau neutrino0103 physical sciencesTau neutrinoOSCILLATIONS010306 general physicsCiencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)AIR-SHOWERSPierre Auger ObservatoryPhysicsSPECTRUM010308 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 AstrophysicsFísicaultrahigh energy cosmic rays ; tau neutrinos ; Pierre Auger ObservatoryDiffuse fluxPierre Auger ObservatoryPERFORMANCECOSMIC-RAYScosmic radiation13. Climate actionTELESCOPESHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaLeptonPhysical Review D
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High-ET isolated-photon plus jets production in pp collisions at s=8 TeV with the ATLAS detector

2017

The dynamics of isolated-photon plus one-, two- and three-jet production in pp collisions at a centre-of-mass energy of 8 TeV are studied with the ATLAS detector at the LHC using a data set with an ...

Quantum chromodynamicsPhysicsNuclear and High Energy PhysicsParticle physicsPhotonLarge Hadron ColliderPhysics::Instrumentation and Detectors010308 nuclear & particles physicsAtlas detectorAstrophysics::High Energy Astrophysical Phenomena01 natural sciences7. Clean energyNuclear physics0103 physical sciencesTransverse momentumHigh Energy Physics::Experiment010306 general physicsNuclear Physics B
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Search for the Higgs boson in the H→WW→ℓνjj decay channel at s=7 TeV with the ATLAS detector

2012

A search for the Standard Model Higgs boson has been performed in the H→WW→lνjj channel using 4.7 fb^(−1) of pp collision data recorded at a centre-of-mass energy of √s = 7 TeV with the ATLAS detector at the Large Hadron Collider. Higgs boson candidates produced in association with zero, one or two jets are included in the analysis to maximize the acceptance for both gluon fusion and weak boson fusion Higgs boson production processes. No significant excess of events is observed over the expected background and limits on the Higgs boson production cross section are derived for a Higgs boson mass in the range 300 GeV<m_H<600 GeV. The best sensitivity is reached for m_H=400 GeV, where the obse…

PhysicsNuclear and High Energy PhysicsLarge Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::Phenomenology7. Clean energy01 natural sciencesUpper and lower boundsSearch for the Higgs bosonStandard ModelGluonNuclear physicsmedicine.anatomical_structureAtlas (anatomy)0103 physical sciencesHiggs bosonmedicineHigh Energy Physics::Experiment010306 general physicsBosonPhysics Letters B
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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 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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Measurements of spin correlation in top-antitop quark events from proton-proton collisions ats=7  TeVusing the ATLAS detector

2014

Measurements of spin correlation in top quark pair production are presented using data collected with the ATLAS detector at the LHC with proton-proton collisions at a center-of-mass energy of 7 TeV, corresponding to an integrated luminosity of 4.6 fb(-1). Events are selected in final states with two charged leptons and at least two jets and in final states with one charged lepton and at least four jets. Four different observables sensitive to different properties of the top quark pair production mechanism are used to extract the correlation between the top and antitop quark spins. Some of these observables are measured for the first time. The measurements are in good agreement with the Stan…

QuarkPhysicsNuclear and High Energy PhysicsParticle physicsTop quarkLarge Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyTevatron01 natural sciences7. Clean energyBottom quarkNuclear physicsPair production0103 physical sciencesHigh Energy Physics::Experiment010306 general physicsLeptonBosonPhysical 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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Measurement of the pseudorapidity and transverse momentum dependence of the elliptic flow of charged particles in lead–lead collisions at sNN=2.76 Te…

2012

This Letter describes the measurement of elliptic flow of charged particles in lead-lead collisions at root s(NN) = 2.76 TeV using the ATLAS detector at the Large Hadron Collider (LHC). The results ...

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderPhysics::Instrumentation and Detectors010308 nuclear & particles physicsAtlas detectorAtlas (topology)High Energy Physics::PhenomenologyHadronElliptic flow01 natural sciencesCharged particleNuclear physicsPseudorapidity0103 physical sciencesTransverse momentumHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsPhysics Letters B
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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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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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Search for displaced muonic lepton jets from light Higgs boson decay in proton–proton collisions at s=7 TeV with the ATLAS detector

2013

A search is performed for collimated muon pairs displaced from the primary vertex produced in the decay of long-lived neutral particles in proton-proton collisions at root s = 7 TeV centre-of-mass ...

PhysicsNuclear and High Energy PhysicsParticle physicsMuonLarge Hadron Collider010308 nuclear & particles physicsAtlas detectorAstrophysics::High Energy Astrophysical Phenomena01 natural sciencesCollimated lightNuclear physicsMassless particleHidden sector0103 physical sciencesHiggs bosonPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsLeptonPhysics Letters B
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Search for direct slepton and gaugino production in final states with two leptons and missing transverse momentum with the ATLAS detector in pp colli…

2013

A search for the electroweak pair production of charged sleptons and weak gauginos decaying into final states with two leptons is performed using 4.7 fb(-1) of proton-proton collision data at root s = 7 TeV recorded with the ATLAS experiment at the Large Hadron Collider. No significant excesses are observed with respect to the prediction from Standard Model processes. In the scenario of direct slepton production, if the sleptons decay directly into the lightest neutralino, left-handed slepton masses between 85 and 195 GeV are excluded at 95% confidence level for a 20 GeV neutralino. Chargino masses between 110 and 340 GeV are excluded in the scenario of direct production of wino-like chargi…

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::PhenomenologyGaugino7. Clean energy01 natural sciencesNuclear physicsCharginoPair productionHADRON-HADRON COLLISIONS0103 physical sciencesNeutralinoHigh Energy Physics::Experiment010306 general physicsNuclear ExperimentSUPERSYMMETRYMinimal Supersymmetric Standard ModelLepton
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Charged-particle multiplicities in pp interactions at s=900 GeV measured with the ATLAS detector at the LHC

2010

The first measurements from proton-proton collisions recorded with the ATLAS detector at the LHC are presented. Data were collected in December 2009 using a minimum-bias trigger during collisions at a centre-of-mass energy of 900 GeV. The charged-particle multiplicity, its dependence on transverse momentum and pseudorapidity, and the relationship between mean transverse momentum and charged-particle multiplicity are measured for events with at least one charged particle in the kinematic range vertical bar eta vertical bar 500 MeV. The measurements are compared to Monte Carlo models of proton-proton collisions and to results from other experiments at the same centre-of-mass energy. The charg…

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsAtlas detectorMonte Carlo methodMultiplicity (mathematics)01 natural sciences7. Clean energyCharged particleNuclear physicsMinimum biasPseudorapidity0103 physical sciencesTransverse momentumHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsPhysics Letters B
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Search for the Standard Model Higgs boson in the H→WW(⋆)→ℓνℓν decay mode with 4.7 fb−1 of ATLAS data at s=7 TeV

2012

A search for the Standard Model Higgs boson in the H -> WW(*()) -> lvlv (l = e.mu) decay mode is presented. The search is performed using proton-proton collision data corresponding to an inte ...

PhysicsNuclear and High Energy PhysicsLarge Hadron Collider010308 nuclear & particles physicsAtlas detectorNuclear TheoryHigh Energy Physics::Phenomenology7. Clean energy01 natural sciencesNuclear physics0103 physical sciencesAtlas dataHiggs bosonPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsPhysics Letters B
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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 a standard model Higgs boson in the H→ZZ→ℓ+ℓ−νν¯ decay channel using 4.7 fb−1 of s=7 TeV data with the ATLAS detector

2012

A search for a Standard Model Higgs boson decaying via H -> ZZ -> l(+)l(-) nu(nu) over bar, where l represents electrons or muons, is presented. It is based on proton-proton collision data at ...

Quantum chromodynamicsPhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderMuonPhysics::Instrumentation and Detectors010308 nuclear & particles physicsAtlas detectorHigh Energy Physics::PhenomenologyElectron01 natural sciencesNuclear physics0103 physical sciencesHiggs bosonPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsPhysics Letters B
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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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Search for long-lived, heavy particles in final states with a muon and multi-track displaced vertex in proton–proton collisions at s=7 TeV with the A…

2013

Many extensions of the Standard Model posit the existence of heavy particles with long lifetimes. In this Letter, results are presented of a search for events containing one or more such particles, which decay at a significant distance from their production point, using a final state containing charged hadrons and an associated muon. This analysis uses a data sample of proton-proton collisions at root s = 7 TeV corresponding to an integrated luminosity of 4.4 fb(-1) collected in 2011 by the ATLAS detector operating at the Large Hadron Collider. Results are interpreted in the context of R-parity violating supersymmetric scenarios. No events in the signal region are observed and limits are se…

PhysicsNuclear and High Energy PhysicsParticle physicsMuonLarge Hadron Collider010308 nuclear & particles physicsBranching fractionHigh Energy Physics::PhenomenologySuperpartnerSupersymmetry01 natural sciencesNuclear physicsPair production0103 physical sciencesNeutralinoHiggs bosonHigh Energy Physics::Experiment010306 general physicsPhysics Letters B
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Search for FCNC single top-quark production at s=7 TeV with the ATLAS detector

2012

A search for the production of single top-quarks via flavour-changing neutral-currents is presented. Data collected with the ATLAS detector at a centre-of-mass energy of root s = 7 TeV, correspondi ...

PhysicsNuclear and High Energy PhysicsTop quarkParticle physicsPhysics::Instrumentation and Detectors010308 nuclear & particles physicsAtlas (topology)Atlas detectorHigh Energy Physics::LatticeHigh Energy Physics::Phenomenology01 natural sciencesNuclear physics0103 physical sciencesHigh Energy Physics::Experiment010306 general physicsPhysics Letters B
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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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Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter

2010

Data collected by the Pierre Auger Observatory through 31 August 2007 showed evidence for anisotropy in the arrival directions of cosmic rays above the Greisen-Zatsepin-Kuz'min energy threshold, 6 x 10(19) eV. The anisotropy was measured by the fraction of arrival directions that are less than 3.1 degrees from the position of an active galactic nucleus within 75 Mpc (using the Veron-Cetty and Veron 12th catalog). An updated measurement of this fraction is reported here using the arrival directions of cosmic rays recorded above the same energy threshold through 31 December 2009. The number of arrival directions has increased from 27 to 69, allowing a more precise measurement. The correlating…

AstronomyAstrophysicsUltra High Energy Cosmic ray01 natural scienceslaw.inventionObservatorylawAnisotropy010303 astronomy & astrophysicsmedia_commonHigh 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]UHECRAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryGZKAnisotropíaGALAXIESNEUTRINOSGreisen–Zatsepin–Kuz’minComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaACTIVE GALACTIC NUCLEIHIPASS CATALOG[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Active galactic nucleusRadiación Cósmicamedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsTelescope0103 physical sciencesCosmic raysCiencias ExactasAstrophysics::Galaxy AstrophysicsPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsAstronomyFísicaAstronomy and AstrophysicsCosmic rayGalaxyCorrelation with astrophysical sourcesCosmic rays; UHECR; Anisotropy; Pierre Auger Observatory; Extra-galactic; GZKSkyExperimental High Energy PhysicsAnisotropyExtra-galactic
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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 centrality dependence of J/ψ yields and observation of Z production in lead–lead collisions with the ATLAS detector at the LHC

2011

Using the ATLAS detector, a centrality-dependent suppression has been observed in the yield of J/psi mesons produced in the collisions of lead ions at the Large Hadron Collider. In a sample of minimum-bias lead-lead collisions at a nucleon-nucleon centre of mass energy root s(NN) = 2.76 TeV, corresponding to an integrated luminosity of about 6.7 mu b(-1), J/psi mesons are reconstructed via their decays to mu(+)mu(-) pairs. The measured J/psi yield, normalized to the number of binary nucleon-nucleon collisions, is found to significantly decrease from peripheral to central collisions. The centrality dependence is found to be qualitatively similar to the trends observed at previous, lower ener…

PhysicsNuclear and High Energy PhysicsParticle physicsLuminosity (scattering theory)Large Hadron ColliderMeson010308 nuclear & particles physicsBinary number01 natural sciencesIonNuclear physicsmedicine.anatomical_structureAtlas (anatomy)0103 physical sciencesmedicineHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsScalingBosonPhysics Letters B
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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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Measurement of D⁎±, D± and Ds± meson production cross sections in pp collisions at s=7 TeV with the ATLAS detector

2016

The production of D*(+/-), D-+/- and D-S(+/-) charmed mesons has been measured with the ATLAS detector in pp collisions at,/7s = 7 TeV at the LHC, using data corresponding to an integrated luminosi ...

Quantum chromodynamicsPhysicsNuclear and High Energy PhysicsParticle physicsMeson productionLarge Hadron ColliderMesonPhysics::Instrumentation and Detectors010308 nuclear & particles physicsAtlas detectorHigh Energy Physics::PhenomenologyDeep inelastic scattering01 natural sciences7. Clean energymedicine.anatomical_structureAtlas (anatomy)0103 physical sciencesTransverse momentummedicineHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsNuclear Physics B
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Measurement of the production cross section for W-bosons in association with jets in pp collisions at s=7 TeV with the ATLAS detector

2011

This Letter reports on a first measurement of the inclusive W + jets cross section in proton-proton collisions at a centre-of-mass energy of 7 TeV at the LHC, with the ATLAS detector. Cross section ...

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderPhysics::Instrumentation and Detectors010308 nuclear & particles physicsAtlas (topology)Atlas detectorAstrophysics::High Energy Astrophysical Phenomena01 natural sciencesNuclear physics0103 physical sciencesPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsBosonPhysics Letters B
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Atmospheric effects on extensive air showers observed with the Surface Detector of the Pierre Auger Observatory

2009

Atmospheric parameters, such as pressure (P), temperature (T) and density (ρ ∝ P/T), affect the development of extensive air showers initiated by energetic cosmic rays. We have studied the impact of atmospheric variations on extensive air showers by means of the surface detector of the Pierre Auger Observatory. The rate of events shows a ∼ 10% seasonal modulation and ∼ 2% diurnal one. We find that the observed behaviour is explained by a model including the effects associated with the variations of P and ρ. The former affects the longitudinal development of air showers while the latter influences the Molière radius and hence the lateral distribution of the shower particles. The model is val…

[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]: 96.50.sdRadiación CósmicaIMPACTAstronomyExtensive air showerFOS: Physical sciencesCosmic rayAstrophysicsExtensive air showers; UHECR; Atmosphere; Weather01 natural sciencesCOSMIC-RAY CASCADESAugerAtmosphereENERGYObservatory0103 physical sciencesExtensive air showersRECONSTRUCTION96.50.sf010303 astronomy & astrophysicsMolière radiusWeatherInstrumentation and Methods for Astrophysics (astro-ph.IM)96.50.sbPierre Auger ObservatoryPhysics010308 nuclear & particles physicsAtmosphereUHECRDetectorFísicaAstronomy and AstrophysicsPresión AtmosféricaPROFILES[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Longitudinal developmentATMOSFERA (ESTUDO)13. Climate actionExperimental High Energy PhysicsSIMULATIONComputingMethodologies_DOCUMENTANDTEXTPROCESSINGClimaAstrophysics - Instrumentation and Methods for Astrophysics
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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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Search for squarks and gluinos using final states with jets and missing transverse momentum with the ATLAS detector in s=7 TeV proton–proton collisio…

2011

A search for squarks and gluinos in events containing jets, missing transverse momentum and no electrons or muons is presented. The data were recorded in 2011 by the ATLAS experiment in root s = 7 TeV proton-proton collisions at the Large Hadron Collider. No excess above the Standard Model background expectation is observed in 1.04 fb(-1) of data. Gluino and squark masses below 700 GeV and 875 GeV respectively are excluded at the 95% confidence level in simplified models containing only squarks of the first two generations, a gluino octet and a massless neutralino. The exclusion limit increases to 1075 GeV for squarks and gluinos of equal mass. In MSUGRA/CMSSM models with tan beta = 10, A(0…

PhysicsNuclear and High Energy PhysicsParticle physicsGluinoLarge Hadron ColliderMuon010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyATLAS experimentSupersymmetry01 natural sciencesStandard ModelNuclear physicsMassless particlemedicine.anatomical_structureAtlas (anatomy)0103 physical sciencesNeutralinomedicineHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsMinimal Supersymmetric Standard ModelPhysics Letters B
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Erratum to "Atmospheric effects on extensive air showers observed with the surface detector of the Pierre Auger observatory"[Astroparticle Physics 32…

2010

The Pierre Auger Collaboration... K.B. Barber... J.A. Bellido... R.W. Clay... B.R. Dawson... V.C. Holmes... J. Sorokin... P. Wahrlich... B.J. Whelan... M.G. Winnick... et al.

Astroparticle physicsPhysicsPierre Auger Observatory[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]010308 nuclear & particles physicsAstronomyDetectorAstronomyAstronomy and AstrophysicsAstrophysics01 natural sciencesAuger[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Experimental High Energy Physics0103 physical sciences010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSAstroparticle Physics
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Measurement of the inclusive isolated prompt photon cross-section in pp collisions at s=7 TeV using 35 pb−1 of ATLAS data

2011

A measurement of the differential cross-section for the inclusive production of isolated prompt photons in pp collisions at a center-of-mass energy root s = 7 TeV is presented. The measurement cove ...

PhysicsQuantum chromodynamicsNuclear and High Energy PhysicsParticle physicsPhotonLarge Hadron Collider010308 nuclear & particles physicsAtlas detectorAstrophysics::High Energy Astrophysical Phenomena01 natural sciencesNuclear physics0103 physical sciencesAtlas data010306 general physicsPhysics Letters B
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Measurement of the Depth of Maximum of Extensive Air Showers above 10(18) eV

2010

We describe the measurement of the depth of maximum, Xmax, of the longitudinal development of air showers induced by cosmic rays. Almost four thousand events above 10¹⁸ eV observed by the fluorescence detector of the Pierre Auger Observatory in coincidence with at least one surface detector station are selected for the analysis. The average shower maximum was found to evolve with energy at a rate of (106⁺³⁵₋₂₁) g/cm²/decade below 1018.24 ± 0.05 eV and (24 ± 3) g/cm²/decade above this energy. The measured shower-to-shower fluctuations decrease from about 55 to 26 g/cm². The interpretation of these results in terms of the cosmic ray mass composition is briefly discussed.

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FLUORESCENCE LIGHTGeneral Physics and AstronomyPierre Auger Observatory; depth of maximum; fluorescence detector; cosmic raysFOS: Physical sciencesCosmic rayChemical CompositionAstrophysicsMass compositionENERGIA01 natural sciencesCoincidenceAugerNuclear physicsPhysics and Astronomy (all)cosmic rays0103 physical sciencesRECONSTRUCTIONHigh-Energy Cosmic Ray010303 astronomy & astrophysicsDETECTORCiencias ExactasPierre Auger ObservatoryPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MeasurementSPECTRUM010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Pierre Auger ExperimentDetectorPrimary compositionFísicaPierre Auger ObservatoryCOSMIC-RAYSCosmic raylongitudinal developmentLongitudinal developmentRESOLUTIONFísica nuclearfluorescenceAstrophysics - High Energy Astrophysical PhenomenaenergyPhysical Review Letters
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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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Measurement of Wγ and Zγ production cross sections in pp collisions at s=7 TeV and limits on anomalous triple gauge couplings with the ATLAS detector

2012

This Letter presents measurements of l(+/-) nu gamma and l(+)l(-)gamma (l = e.mu) production in 1.02 fb(-1) of pp collision data recorded at root s = 7 TeV with the ATLAS detector at the LHC in the ...

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderPhysics::Instrumentation and Detectors010308 nuclear & particles physicsAtlas detectorAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyGauge (firearms)01 natural sciencesNuclear physicsmedicine.anatomical_structureAtlas (anatomy)0103 physical sciencesmedicinePhysics::Accelerator PhysicsHigh Energy Physics::ExperimentProduction (computer science)010306 general physicsBosonPhysics 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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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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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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Search for a heavy Standard Model Higgs boson in the channel H→ZZ→ℓ+ℓ−qq¯ using the ATLAS detector

2012

A search for a heavy Standard Model Higgs boson decaying via H -> ZZ -> l(+)l(-)q (q) over bar, where l = e, mu, is presented. The search is performed using a data set of pp collisions at root s = 7 TeV, corresponding to an integrated luminosity of 1.04 fb(-1) collected in 2011 by the ATLAS detector at the CERN LHC collider. No significant excess of events above the estimated background is found. Upper limits at 95% confidence level on the production cross section (relative to that expected from the Standard Model) of a Higgs boson with a mass in the range between 200 and 600 GeV are derived. Within this mass range, there is at present insufficient sensitivity to exclude a Standard Model Hi…

PhysicsNuclear physicsNuclear and High Energy PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsAtlas detectorHigh Energy Physics::Phenomenology0103 physical sciencesHiggs bosonHigh Energy Physics::Experiment010306 general physics01 natural sciencesPhysics Letters B
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Measurements of the electron and muon inclusive cross-sections in proton–proton collisions at s=7 TeV with the ATLAS detector

2012

This Letter presents measurements of the differential cross-sections for inclusive electron and muon production in proton-proton collisions at a centre-of-mass energy of root s = 7 TeV, using data collected by the ATLAS detector at the LHC. The muon cross-section is measured as a function of p(T) in the range 4 < p(T) < 100 GeV and within pseudorapidity vertical bar eta vertical bar < 2.5. In addition the electron and muon cross-sections are measured in the range 7 < p(T) < 26 GeV and within vertical bar eta vertical bar < 2.0, excluding 1.37 < vertical bar eta vertical bar < 1.52. Integrated luminosities of 1.3 pb(-1) and 1.4 pb(-1) are used for the electron and muon measurements, respecti…

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderMuon010308 nuclear & particles physicsAtlas detectorHigh Energy Physics::PhenomenologyElectron01 natural sciencesNuclear physicsPseudorapidity0103 physical sciencesHigh Energy Physics::ExperimentResummationNuclear Experiment010306 general physicsPhysics Letters B
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Search for supersymmetry in pp collisions at s=7 TeV in final states with missing transverse momentum and b-jets

2011

Results are presented of a search for supersymmetric particles in events with large missing transverse momentum and at least one heavy flavour jet candidate in sqrt{s} = 7 TeV proton-proton collisions. In a data sample corresponding to an integrated luminosity of 35 pb-1 recorded by the ATLAS experiment at the Large Hadron Collider, no significant excess is observed with respect to the prediction for Standard Model processes. For R-parity conserving models in which sbottoms (stops) are the only squarks to appear in the gluino decay cascade, gluino masses below 590 GeV (520 GeV) are excluded at the 95% C.L. The results are also interpreted in an MSUGRA/CMSSM supersymmetry breaking scenario w…

PhysicsNuclear and High Energy PhysicsParticle physicsGluinoLarge Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyATLAS experimentSupersymmetry01 natural sciencesSupersymmetry breakingStandard ModelNuclear physicsR-parity0103 physical sciencesHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsMinimal Supersymmetric Standard ModelPhysics Letters B
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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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Transverse momentum, rapidity, and centrality dependence of inclusive charged-particle production in sNN=5.02 TeV p+ Pb collisions measured by the AT…

2016

Measurements of the per-event charged-particle yield as a function of the charged-particle transverse momentum and rapidity are performed using p+Pbp+Pb collision data collected by the ATLAS experiment at the LHC at a centre-of-mass energy of sqrt (SNN) = 5.01 TeV. Charged particles are reconstructed over pseudorapidity |η|<2.3|η|<2.3 and transverse momentum between 0.1 GeV0.1 GeV and 22 GeV22 GeV in a dataset corresponding to an integrated luminosity of 1 μb−11 μb−1. The results are presented in the form of charged-particle nuclear modification factors, where the p+Pbp+Pb charged-particle multiplicities are compared between central and peripheral p+Pbp+Pb collisions as well as to charged-p…

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderLuminosity (scattering theory)Proton010308 nuclear & particles physics01 natural sciencesCharged particleNuclear physicsPseudorapidity0103 physical sciencesRapidityNuclear Experiment010306 general physicsNucleonGlauberPhysics Letters B
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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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A measurement of the ratio of the W and Z cross sections with exactly one associated jet in pp collisions at with ATLAS

2012

The ratio of production cross sections of the W and Z bosons with exactly one associated jet is presented as a function of jet transverse momentum threshold. The measurement has been designed to ma ...

PhysicsNuclear and High Energy PhysicsJet (fluid)Particle physics010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaPerturbative QCDFunction (mathematics)01 natural sciencesStandard ModelNuclear physicsmedicine.anatomical_structureAtlas (anatomy)W and Z bosons0103 physical sciencesTransverse momentummedicineHigh Energy Physics::Experiment010306 general physics
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Search for pair production of heavy top-like quarks decaying to a high-pT W boson and a b quark in the lepton plus jets final state at s=7 TeV with t…

2013

A search is presented for production of a heavy up-type quark (t') together with its antiparticle, assuming a significant branching ratio for subsequent decay into a W boson and a b quark. The search is based on 4.7 fb(-1) of pp collisions root s = 7 TeV recorded in 2011 with the ATLAS detector at the CERN Large Hadron Collider. Data are analyzed in the lepton + jets final state, characterized by a high-transverse-momentum isolated electron or muon, large missing transverse momentum and at least three jets. The analysis strategy relies on the substantial boost of the W bosons in the t'(t') over bar signal when m(t') greater than or similar to 400 GeV. No significant excess of events above t…

PhysicsQuarkNuclear and High Energy PhysicsTop quarkParticle physicsLarge Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::Phenomenology01 natural sciences7. Clean energyBottom quarkStandard ModelNuclear physicsW and Z bosons0103 physical sciencesHiggs bosonHigh Energy Physics::Experiment010306 general physicsBosonPhysics Letters B
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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 flavour composition of dijet events in pp collisions at √s = 7 TeV with the ATLAS detector

2013

This paper describes a measurement of the flavour composition of dijet events produced in pp collisions at s√=7~TeVs=7~TeV using the ATLAS detector. The measurement uses the full 2010 data sample, corresponding to an integrated luminosity of 39 pb−1. Six possible combinations of light, charm and bottom jets are identified in the dijet events, where the jet flavour is defined by the presence of bottom, charm or solely light flavour hadrons in the jet. Kinematic variables, based on the properties of displaced decay vertices and optimised for jet flavour identification, are used in a multidimensional template fit to measure the fractions of these dijet flavour states as functions of the leadin…

Physics and Astronomy (miscellaneous)Ciencias FísicasHadronFlavourNuclear physics01 natural sciencesHigh Energy Physics - ExperimentLuminosity (scattering theory)//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)Ciencias Naturales y ExactasNaturvetenskap[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Charm (quantum number)Nuclear ExperimentQCPhysicsJet (fluid)Luminosity (scattering theory)PhysicsSettore FIS/01 - Fisica SperimentaleParticle physicsCross-SectionATLASmedicine.anatomical_structureComputingMethodologies_DOCUMENTANDTEXTPROCESSINGLHCNatural SciencesParticle Physics - ExperimentParticle physics530 PhysicsCiências Naturais::Ciências FísicasAstrophysics::High Energy Astrophysical Phenomena:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesddc:500.2Física de Partículas y Campos530GluonNuclear physicsAtlas (anatomy)Jet (fluid)0103 physical sciencesmedicineCharm (quantum number)Rapidityddc:530High Energy Physics010306 general physicsEngineering (miscellaneous)Hadron-Hadron ScatteringScience & Technology010308 nuclear & particles physicsParton DistributionsHigh Energy Physics::PhenomenologyFísica//purl.org/becyt/ford/1.3 [https]GluonJETHADRON-HADRON COLLISIONSHadronExperimental High Energy PhysicsFlavourRapidityHigh Energy Physics::ExperimentFLAVORColliderEuropean Physical Journal C
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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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The ATLAS Data Acquisition and High Level Trigger system

2016

Journal of Instrumentation 11(06), P06008 (2016). doi:10.1088/1748-0221/11/06/P06008

High level triggerComputer sciencedata acquisitionPhysics::Instrumentation and DetectorsLarge hadron collideronline filteringTrigger Concepts and Systems (Hardware and Software)Control and Monitor Systems Online01 natural sciencesOnline farms and online filteringData acquisitionRecopilación de datos[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Detectors and Experimental TechniquesInstrumentationMathematical PhysicsSettore FIS/01Online Farms and Online FilteringLarge Hadron ColliderControl and monitor systems onlineATLAS experimentATLASmedicine.anatomical_structureTrigger concepts and systems (hardware and software)Triggers and rulesComputer hardwareperformanceOnline farms andControl and monitor systems online; Data acquisition concepts; Online farms and online filtering; Trigger concepts and systems (hardware and software)Ciências Naturais::Ciências Físicas:Ciências Físicas [Ciências Naturais]Data Acquisition ConceptsATLAS detector; ATLAS experiment; CERN; Large Hadron ColliderATLAS experiment610Accelerator Physics and Instrumentation530LHC ATLAS High Energy Physics TriggerAtlas (anatomy)0103 physical sciencesmedicineddc:610ElectronicsInstrumentation (computer programming)Control and monitor systems online; Data acquisition concepts; Online farms and; online filtering; Trigger concepts and systems (hardware and software)010306 general physicsCiencias ExactasScience & Technology010308 nuclear & particles physicsbusiness.industryData acquisition conceptsFísicaAcceleratorfysik och instrumenteringtriggerSistema en líneaData flow diagrammonitoringHigh Energy Physics::Experimentbusiness
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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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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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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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Search for Gluinos in Events with Two Same-Sign Leptons, Jets, and Missing Transverse Momentum with the ATLAS Detector in Collisions at

2012

A search is presented for gluinos decaying via the supersymmetric partner of the top quark using events with two same-sign leptons, jets, and missing transverse momentum. The analysis is performed ...

PhysicsQuantum chromodynamicsParticle physicsTop quark010308 nuclear & particles physicsAtlas (topology)High Energy Physics::LatticeSupergravityHigh Energy Physics::PhenomenologyGeneral Physics and Astronomy01 natural sciencesNuclear physicsPion0103 physical sciencesTransverse momentumGrand Unified TheoryHigh Energy Physics::Experiment010306 general physicsLepton
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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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Single hadron response measurement and calorimeter jet energy scale uncertainty with the ATLAS detector at the LHC

2013

The uncertainty on the calorimeter energy response to jets of particles is derived for the ATLAS experiment at the Large Hadron Collider (LHC). First, the calorimeter response to single isolated charged hadrons is measured and compared to the Monte Carlo simulation using proton-proton collisions at centre-of-mass energies of √s = 900 GeV and 7 TeV collected during 2009 and 2010. Then, using the decay of Ks and Λ particles, the calorimeter response to specific types of particles (positively and negatively charged pions, protons, and anti-protons) is measured and compared to the Monte Carlo predictions. Finally, the jet energy scale uncertainty is determined by propagating the response uncert…

Physics and Astronomy (miscellaneous)large hadron colliderPhysics::Instrumentation and DetectorsHadronMonte Carlo methodNuclear Theory01 natural sciences7. Clean energyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Naturvetenskap[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentPhysicsJet (fluid)End-Cap CalorimeterLarge Hadron ColliderATLAS experimentSettore FIS/01 - Fisica Sperimentalemedicine.anatomical_structurePhysical SciencesComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearLHC ATLAS High Energy PhysicsNatural SciencesParticle Physics - ExperimentParticle physics530 PhysicsCiências Naturais::Ciências Físicas:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesddc:500.2530Nuclear physicsPionAtlas (anatomy)0103 physical sciencesBeam TestsmedicineFysikddc:530010306 general physicsEngineering (miscellaneous)Ciencias ExactasScience & TechnologyHadron-Hadron ScatteringATLAS detectorCalorimeter (particle physics)010308 nuclear & particles physicsFísicaBarrel Calorimeterjet energyExperimental High Energy Physicsproton-proton collisionsHigh Energy Physics::Experiment
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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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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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Measurement of W ± Z production in proton-proton collisions at √s =7 TeV with the ATLAS detector

2012

A study of W±Z production in proton-proton collisions at √s=7 TeV is presented using data corresponding to an integrated luminosity of 4.6 fb−1 collected with the ATLAS detector at the Large Hadron Collider in 2011. In total, 317 candidates, with a background expectation of 68±10 events, are observed in double-leptonic decay final states with electrons, muons and missing transverse momentum. The total cross-section is determined to be σtotWZ=19.0+1.4−1.3(stat.)±0.9(syst.)±0.4(lumi.) pb, consistent with the Standard Model expectation of 17.6+1.1−1.0 pb. Limits on anomalous triple gauge boson couplings are derived using the transverse momentum spectrum of Z bosons in the selected events. The …

Physics and Astronomy (miscellaneous)Proton7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Naturvetenskap[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Invariant massNuclear ExperimentQCDetectors de radiacióBosonPhysicsddc:539Large Hadron ColliderSettore FIS/01 - Fisica Sperimentalez bosonATLASmedicine.anatomical_structureComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearLHCNatural SciencesParticle Physics - ExperimentParticle physicsATLAS; detectorCiências Naturais::Ciências Físicas:Ciências Físicas [Ciências Naturais]FOS: Physical sciences530Partícules (Física nuclear)Standard ModelNuclear physicsAtlas (anatomy)0103 physical sciencesmedicineddc:530High Energy Physics010306 general physicsEngineering (miscellaneous)Ciencias ExactasGauge bosonMuonScience & TechnologyATLAS detector010308 nuclear & particles physicsFísicaCol·lisions (Física nuclear)Experimental High Energy Physicsproton-proton collisionsHigh Energy Physics::ExperimentEuropean Physical Journal C
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Search for diphoton events with large missing transverse momentum in 7 TeV proton-proton collision data with the ATLAS detector

2012

A search for diphoton events with large missing transverse momentum has been performed using proton–proton collision data at √s = 7 TeV recorded with the ATLAS detector, corresponding to an integrated luminosity of 4.8 fb[superscript −1]. No excess of events was observed above the Standard Model prediction and model-dependent 95% confidence level exclusion limits are set. In the context of a generalised model of gauge-mediated supersymmetry breaking with a bino-like lightest neutralino of mass above 50 GeV, gluinos (squarks) below 1.07 TeV (0.87 TeV) are excluded, while a breaking scale Λ below 196 TeV is excluded for a minimal model of gauge-mediated supersymmetry breaking. For a specific …

ParticleLambda01 natural sciencesHigh Energy Physics - ExperimentUniversal extra dimensionHigh Energy Physics - Experiment (hep-ex)proton-proton collisionExtensionBibliography[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]QCPhysicsLarge Hadron ColliderSettore FIS/01 - Fisica SperimentaleSupersymmetry breakingDynamical Supersymmetry BreakingComputingMethodologies_DOCUMENTANDTEXTPROCESSINGdiphoton events; ATLAS detectorUniversal Extra DimensionsPhenomenologyFísica nuclearPhenomenology (particle physics)Particle Physics - ExperimentParticle physicsNuclear and High Energy PhysicsFortran CodeCiências Naturais::Ciências FísicasAstrophysics::High Energy Astrophysical PhenomenaSupergauge Transformations:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesddc:500.2530Partícules (Física nuclear)Nuclear physicsMinimal model0103 physical sciencesddc:530010306 general physicsCiencias ExactasScience & TechnologyATLAS detector010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicadiphotonHadron CollidersGeneratorsHADRON-HADRON COLLISIONSNeutralinoExperimental High Energy PhysicsHigh Energy Physics::ExperimentModel
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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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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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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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Measurement of the inelastic proton-proton cross-section at √s = 7 TeV with the ATLAS detector

2011

The dependence of the rate of proton–proton interactions on the centre-of-mass collision energy, √s, is of fundamental importance for both hadron collider physics and particle astrophysics. The dependence cannot yet be calculated from first principles; therefore, experimental measurements are needed. Here we present the first measurement of the inelastic proton–proton interaction cross-section at a centre-of-mass energy, √s, of 7 TeV using the ATLAS detector at the Large Hadron Collider. Events are selected by requiring hits on scintillation counters mounted in the forward region of the detector. An inelastic cross-section of 60.3±2.1 mb is measured for ξ>5×10[superscript −6], where ξ is ca…

DiffractionAtlas detectorNuclear TheoryGeneral Physics and AstronomyPP01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Detectors and Experimental TechniquesNuclear ExperimentGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)ComputingMilieux_MISCELLANEOUSddc:539PhysicsMultidisciplinaryLarge Hadron Colliderphysical sciences; particle physicsSettore FIS/01 - Fisica SperimentaleSoftATLASDiffraction DissociationPhotoproductionElastic-ScatteringScintillation counterComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearLHCddc:500Particle Physics - ExperimentParticle physicsCiências Naturais::Ciências Físicas:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesddc:500.2High-Energies530General Biochemistry Genetics and Molecular BiologyArticleNuclear physicsphysical sciencesinelastic; proton–proton cross-section;ATLAS detector0103 physical sciencesAmplitudesHigh Energy Physicsparticle physics010306 general physicsAstroparticle physicsHardScience & Technology010308 nuclear & particles physicsGeneral ChemistryCollisionExperimental High Energy PhysicsPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentModel
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