Search results for "Cosmology"

showing 10 items of 2905 documents

A K s -band-selected catalogue of objects in the ALHAMBRA survey

2016

The original ALHAMBRA catalogue contained over 400 000 galaxies selected using a synthetic F814W image, to the magnitude limit AB(F814W) ≈ 24.5. Given the photometric redshift depth of the ALHAMBRA multiband data (〈 z〉 = 0.86) and the approximately I-band selection, there is a noticeable bias against red objects at moderate redshift.We avoid this bias by creating a new catalogue selected in the Ks band. This newly obtained catalogue is certainly shallower in terms of apparent magnitude, but deeper in terms of redshift, with a significant population of red objects at z > 1. We select objects using the Ks band images, which reach an approximate AB magnitude limit Ks ≈ 22. We generate masks an…

PopulationFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsApproxSurveys01 natural sciencesPhotometry (optics)Apparent magnitude0103 physical sciencesobservations [Cosmology]education010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhotometric redshiftPhysicseducation.field_of_study010308 nuclear & particles physicsCosmology: observationsAstronomyGalaxies: evolutionAstronomy and AstrophysicsAB magnitudeevolution [Galaxies]Astrophysics - Astrophysics of GalaxiesGalaxyRedshiftSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Monthly Notices of the Royal Astronomical Society
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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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"Table 15" of "Measurements of Wgamma and Zgamma production in pp collisions at sqrt{s}= 7 TeV with the ATLAS detector at the LHC"

2014

Normalised fiducial cross section of Wgamma (l;nu;gamma) decay channel in bins of the jet multiplicity with leading photon pT > 15 GeV.

Proton-Proton ScatteringAstrophysics::High Energy Astrophysical Phenomena7000.0High Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic Astrophysics
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"Table 16" of "Measurements of Wgamma and Zgamma production in pp collisions at sqrt{s}= 7 TeV with the ATLAS detector at the LHC"

2014

Normalised fiducial cross section of Wgamma (l;nu;gamma) decay channel in bins of the jet multiplicity with leading photon pT > 60 GeV.

Proton-Proton ScatteringAstrophysics::High Energy Astrophysical Phenomena7000.0High Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic Astrophysics
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"Table 1" of "Measurements of Wgamma and Zgamma production in pp collisions at sqrt{s}= 7 TeV with the ATLAS detector at the LHC"

2014

The measured inclusive fiducial cross section of Wgamma (l;nu;gamma) decay channel. The first systematic (sys) error is the combined systematic uncertainty excluding that of the luminosity. The second (sys) error is the uncertainty on the luminosity.

Proton-Proton ScatteringAstrophysics::High Energy Astrophysical Phenomena7000.0High Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic AstrophysicsNuclear Experiment
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"Table 19" of "Measurements of Wgamma and Zgamma production in pp collisions at sqrt{s}= 7 TeV with the ATLAS detector at the LHC"

2014

Normalised fiducial cross section of Wgamma (l;nu;gamma) decay channel in bins of the transverse mass of Wgamma with leading photon pT > 40 GeV.

Proton-Proton ScatteringAstrophysics::High Energy Astrophysical Phenomena7000.0High Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic AstrophysicsNuclear Experiment
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"Table 2" of "Measurements of Wgamma and Zgamma production in pp collisions at sqrt{s}= 7 TeV with the ATLAS detector at the LHC"

2014

The measured exclusive fiducial cross section of Wgamma (l;nu;gamma) decay channel. The first systematic (sys) error is the combined systematic uncertainty excluding that of the luminosity. The second (sys) error is the uncertainty on the luminosity.

Proton-Proton ScatteringAstrophysics::High Energy Astrophysical Phenomena7000.0High Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic AstrophysicsNuclear Experiment
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"Table 2" of "Search for resonant top plus jet production in ttbar + jets events with the ATLAS detector in pp collisions at sqrt(s) = 7 TeV"

2013

Upper limits of the cross sections and couling (g_R) in the PHI colour triplet model.

Proton-Proton ScatteringHigh Energy Physics::PhenomenologyIntegrated Cross SectionExclusiveTop7000.0Astrophysics::Cosmology and Extragalactic AstrophysicsCross SectionMathematics::Representation TheorySIGAstrophysics::Galaxy AstrophysicsP P --> PHI TQBAR
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"Table 9" of "Measurements of Wgamma and Zgamma production in pp collisions at sqrt{s}= 7 TeV with the ATLAS detector at the LHC"

2014

Normalised fiducial cross section of Wgamma (l;nu;gamma) decay channel in bins of the leading photon PT. Leading Photon is the photon in the final state with highest PT.

Proton-Proton ScatteringPhysics::Optics7000.0Astrophysics::Cosmology and Extragalactic Astrophysics
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"Table 10" of "Measurements of Wgamma and Zgamma production in pp collisions at sqrt{s}= 7 TeV with the ATLAS detector at the LHC"

2014

Normalised fiducial cross section of Wgamma (l;nu;gamma) decay channel in bins of the leading photon PT. Leading Photon is the photon in the final state with highest PT.

Proton-Proton ScatteringPhysics::Optics7000.0Astrophysics::Cosmology and Extragalactic Astrophysics
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