Search results for "Instrumentation and Methods for Astrophysics"

showing 10 items of 706 documents

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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1.5Jy MOJAVE AGN sample and 3FGL data

2016

We use the complete MOJAVE 1.5Jy sample of active galactic nuclei (AGNs) to examine the gamma-ray detection statistics of the brightest radio-loud blazars in the northern sky. We find that 23% of these AGNs were not detected above 0.1GeV by the Fermi-LAT during the four-year 3FGL catalog period partly because of an instrumental selection effect and partly due to their lower Doppler boosting factors. Blazars with synchrotron peaks in their spectral energy distributions located below 10^13.4^Hz also tend to have high-energy peaks that lie below the 0.1GeV threshold of the LAT, and are thus less likely to be detected by Fermi. The non-detected AGNs in the 1.5Jy sample also have significantly l…

interstellar mediumActive galactic nucleigalactic and extragalactic astronomyAstrophysics and AstronomyGamma-ray astronomyhigh energy astrophysicsAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsRedshiftedComputer Science::Digital LibrariesCosmologyobservational astronomyRadio continuum emissionGamma ray astronomyRadio astronomyNatural SciencesAstrophysics::Galaxy Astrophysics
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YSOs in DROXO (Deep rho Oph XMM obs.)

2011

X-rays from very young stars are powerful probes to investigate the mechanisms at work in the very first stages of the star formation and the origin of X-ray emission in very young stars. We present results from a 500ks long observation of the rho Ophiuchi cloud with a XMM-Newton large program named DROXO, aiming at studying the X-ray emission of deeply embedded young stellar objects (YSOs). Cone search capability for table J/A+A/519/A34/tablea1 (List of sources detected in the DROXO EPIC images) Cone search capability for table J/A+A/519/A34/tablea3 (ISOCAM YSOs (Bontemps et al. 2001, J/A+A/372/173) undetected in the DROXO field of view)

interstellar mediumAstrophysics and AstronomyAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsX-ray sourcesstellar astronomyYoung stellar objectsCosmologyPhotometryobservational astronomyX ray sourcesAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsNatural SciencesAstrophysics::Galaxy AstrophysicsInfrared photometry
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XMM Optical Monitor Survey of TMC

2007

The Optical Monitor (OM) on-board XMM-Newton obtained optical/ultraviolet data for the XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST), simultaneously with the X-ray detectors. With the XEST OM data, we study the optical and ultraviolet properties of TMC members, and to perform correlative studies between the X-ray and OM light curves. In particular, we aim to determine whether accretion plays a significant role in the optical/ultraviolet and X-ray emissions. The Neupert effect in stellar flares is also investigated. Coordinates, average count rates and magnitudes were extracted from OM images, together with light curves with low time resolution (a few kiloseconds). For a fe…

interstellar mediumUltraviolet astronomyAstrophysics and AstronomyAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSurveysX-ray sourcesComputer Science::Digital LibrariesCosmologyPhotometryobservational astronomyX ray sourcesPhysics::Space PhysicsMolecular cloudsAstrophysics::Solar and Stellar AstrophysicsNatural SciencesAstrophysics::Galaxy Astrophysics
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Radio-optical scrutiny of compact AGN

2010

We study the correlations between the VLBA (Very Long Baseline Array) radio emission at 15GHz, extended emission at 151MHz, and optical nuclear emission at 5100{AA} for a complete sample of 135 compact jets. We use the partial Kendall's tau correlation analysis to check the link between radio properties of parsec-scale jets and optical nuclear luminosities of host active galactic nuclei (AGN). Cone search capability for table J/A+A/520/A62/table3 (Optical and radio parameters of 135 AGN)

interstellar mediumgalactic and extragalactic astronomyAstrophysics and Astronomyhigh energy astrophysicsAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxiesstellar astronomyOptical astronomyCosmologyobservational astronomyRadio continuum emissionRadio galaxiesRadio astronomyNatural SciencesQuasarsAstrophysics::Galaxy AstrophysicsSpectroscopyVery long baseline interferometry
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Seasonal Modulation of the $^7$Be Solar Neutrino Rate in Borexino

2017

We detected the seasonal modulation of the $^7$Be neutrino interaction rate with the Borexino detector at the Laboratori Nazionali del Gran Sasso in Italy. The period, amplitude, and phase of the observed time evolution of the signal are consistent with its solar origin, and the absence of an annual modulation is rejected at 99.99\% C.L. The data are analyzed using three methods: the sinusoidal fit, the Lomb-Scargle and the Empirical Mode Decomposition techniques, which all yield results in excellent agreement.

liquid scintillators detectorsPhysics - Instrumentation and Detectorsexperimental methodsneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinolow background detectorsSolar neutrinos01 natural sciencesflux: time dependenceneutrino: fluxHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Liquid scintillators detectors; Low background detectors; Neutrino oscillations; Solar neutrinos; Astronomy and Astrophysics[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Borexinoneutrino: interactionMSW effectPhysicsNeutrino oscillationsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)neutrino electron: elastic scatteringmodulationAmplitudeModulationsolar neutrinosBorexinoNeutrinoLiquid scintillators detectorFLUXLow background detectordata analysis methodNeutrino oscillationFOS: Physical sciencesSolar neutrinoNuclear physicsTIME-SERIES ANALYSIS[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]Low background detectorsLiquid scintillators detectorsSEARCH0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]SPACED DATA010306 general physicsNeutrino oscillationbackground: radioactivityneutrino oscillations010308 nuclear & particles physicsAstronomy and AstrophysicsEMPIRICAL MODE DECOMPOSITIONberylliumGran SassoHigh Energy Physics::Experimentneutrino: oscillationEvent (particle physics)experimental results
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Spurious source generation in mapping from noisy phase-self-calibrated data

2008

Phase self-calibration (or selfcal) is an algorithm often used in the calibration of interferometric observations in astronomy. Although a powerful tool, this algorithm presents strong limitations when applied to data with a low signal-to-noise ratio. We analyze the artifacts that the phase selfcal algorithm produces when applied to extremely noisy data. We show how the phase selfcal may generate a spurious source in the sky from a distribution of completely random visibilities. This spurious source is indistinguishable from a real one. We numerically and analytically compute the relationship between the maximum spurious flux density generated by selfcal from noise and the particulars of th…

media_common.quotation_subjectPhase (waves)FOS: Physical sciencesAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsNoise (electronics)Calibrationimage processing [Techniques]UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Otras especialidades astronómicasdata analysis [Methods]Spurious relationshipmedia_commonPhysicsArtifact (error)Techniques : interferometric; Methods : data analysis; Techniques : image processingAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsInterferometryDistribution (mathematics)Space and Planetary ScienceSkyinterferometric [Techniques]Algorithm:ASTRONOMÍA Y ASTROFÍSICA::Otras especialidades astronómicas [UNESCO]:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Astronomy & Astrophysics
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The ALHAMBRA survey: Bayesian photometric redshifts with 23 bands for 3 deg2

2014

A. Molino et al.

media_common.quotation_subjectPhotometric systemAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSurveyslaw.inventionPhotometry (optics)Telescopelawdistances and redshifts [Galaxies]Astrophysics::Solar and Stellar Astrophysicsdata analysis [Methods]Astrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSPhotometric redshiftmedia_commonPhysics[PHYS]Physics [physics]photometry [Galaxies]photometric [Techniques]Astrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstronomy and AstrophysicsCataloguesevolution [Galaxies]GalaxyRedshift13. Climate actionSpace and Planetary ScienceSkyMagnitude (astronomy)Astrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Imaging for Ballistic Trauma: Other Applications of Forensic Imaging in the Living

2019

Firearms are mechanical instruments that allow launching remote specific bodies with mass (bullets) exploiting burst gas energy. The role of imaging for ballistic trauma is crucial in order to define the main characteristics for both judiciary and nonjudiciary purpose, which are the intracorporeal trajectory, the entrance and exit wounds, and the general characteristics of gunshot injuries.

medicine.medical_specialtyForensic radiologyForensic imagingComputer scienceAstrophysics::High Energy Astrophysical PhenomenaGunshotPostmortem CTPostmortem ctAstrophysics::Instrumentation and Methods for AstrophysicsmedicineForensic radiologyMedical physicsBallistic trauma
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Design and implementation of the AMIGA embedded system for data acquisition

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 admin-istrative staff in Malargtie. We are very grateful to the following agencies and organizations for financial support: Comision Nacional de Energla Atomica, Agencia Nacional de Promocion Cientffica y Tec-nologica (ANPCyT) , Consejo Nacional de Investigaciones Cientfficas y Tecnicas (CONICET) , Gobierno de la Provincia de Mendoza, Municipalidad de Malargtie, NDM Holdings and Valle Las Leilas, in gratitude for their continuing cooperation over land access, Argentina; the Australian Research Council; Conselho…

muon: showersDetector control systems (detector and experiment monitoring and slow-control systems architecture hardware algorithms databases)Physics::Instrumentation and Detectorsdata acquisitionAstronomycosmic radiation: electromagnetic componentengineeringprimary [cosmic radiation]Particle detectors01 natural sciencesenergy: thresholdData acquisition concepthardwareInstrumentationMathematical Physicsshowers [muon]media_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEControl and monitor systems onlinePhysicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsthreshold [energy]16. Peace & justiceAugerelectromagnetic component [cosmic radiation]observatoryDetector control systems (detector andexperiment monitoring and slow-control systemslanguageupgradeAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomenadatabases)atmosphere [showers]Land accessarchitectureEuropean communityairAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesalgorithmsPolitical science0103 physical sciencesmedia_common.cataloged_instanceddc:530High Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]ddc:610Control and monitor systems online; Data acquisition concepts; Detector control systems (detector and experiment monitoring and slow-control systems architecture hardware algorithms databases); Particle detectorsEuropean union010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Ciencias Exactasscintillation countershowers: atmosphere010308 nuclear & particles physicsDetector control systems (detector and experiment monitoring and slow-control systemsData acquisition conceptsFísicastabilitylanguage.human_languagecosmic radiation: primarymonitoringResearch councilExperimental High Energy PhysicsHigh Energy Physics::ExperimentControl and monitor systems on-linePortuguese[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]HumanitiesRAIOS CÓSMICOSastro-ph.IM
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