Search results for "jet"

showing 10 items of 4711 documents

Multiband RadioAstron space VLBI imaging of the jet in quasar S5 0836+710

2019

Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.-- Open Access funding provided by Max Planck Society.

BrightnessActive galactic nucleusactive [Galaxies]010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)galaxies [Radio continuum]AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences7. Clean energyGalaxies: individual: S5 0836+710Radio continuum: galaxiesRadio telescopeAstrophysical jet0103 physical sciencesVery-long-baseline interferometry010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Jet (fluid)Computer Science::Information RetrievalAstronomy and AstrophysicsQuasarGalaxies: activeAstrophysics - Astrophysics of Galaxiesindividual: S5 0836+710 [Galaxies]Space and Planetary ScienceGalaxies: jetsAstrophysics of Galaxies (astro-ph.GA)jets [Galaxies]Astrophysics - High Energy Astrophysical Phenomena
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Relativistic beaming and gamma-ray brightness of blazars

2009

We investigate the dependence of gamma-ray brightness of blazars on intrinsic properties of their parsec-scale radio jets and the implication for relativistic beaming. By combining apparent jet speeds derived from high-resolution VLBA images from the MOJAVE program with millimetre-wavelength flux density monitoring data from Metsahovi Radio Observatory, we estimate the jet Doppler factors, Lorentz factors, and viewing angles for a sample of 62 blazars. We study the trends in these quantities between the sources which were detected in gamma-rays by the Fermi Large Area Telescope (LAT) during its first three months of science operations and those which were not detected. The LAT-detected blaz…

BrightnessCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical Phenomenajets [galaxies]FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural scienceslaw.inventionTelescopesymbols.namesakeRelativistic beaminglawquasars: general0103 physical sciencesBlazar010303 astronomy & astrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::GalaxiasHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsgeneral [quasars]general [BL Lacertae objects]010308 nuclear & particles physicsGamma rayAstronomy and Astrophysicsgalaxies: jetsViewing angle:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Galaxias [UNESCO]Lorentz factorSpace and Planetary Scienceactive [galaxies]BL Lacertae objectssymbolsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaAstrophysics - High Energy Astrophysical Phenomenagalaxies: active; ; ; BL Lacertae objects : generalFermi Gamma-ray Space TelescopeAstrophysics - Cosmology and Nongalactic Astrophysics
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Search for Gravitational-wave Signals Associated with Gamma-Ray Bursts during the Second Observing Run of Advanced LIGO and Advanced Virgo

2019

We present the results of targeted searches for gravitational-wave transients associated with gamma-ray bursts during the second observing run of Advanced LIGO and Advanced Virgo, which took place from 2016 November to 2017 August. We have analyzed 98 gamma-ray bursts using an unmodeled search method that searches for generic transient gravitational waves and 42 with a modeled search method that targets compact-binary mergers as progenitors of short gamma-ray bursts. Both methods clearly detect the previously reported binary merger signal GW170817, with p-values of <9.38 10-6 (modeled) and 3.1 10-4 (unmodeled). We do not find any significant evidence for gravitational-wave signals associate…

Burst astrophysicAstrofísicaneutron star: binary010504 meteorology & atmospheric sciencesBinary numberAstrophysics01 natural sciencesLIGOQCSUPERNOVArelativistic jetsQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01counterpartGRBGravitational waves (678)Physical SciencesRELATIVISTIC JETSAstrophysics - High Energy Astrophysical PhenomenaGravitational waveGravitationstarsblack-holeAstrophysics::High Energy Astrophysical PhenomenaGeneral Relativity and Quantum Cosmology (gr-qc)precursor activityGravitational wavesSettore FIS/05 - Astronomia e AstrofisicasupernovaCORE-COLLAPSEGamma-ray burstGravitational wave sourcesScience & TechnologyVirgoRCUKAstronomy and AstrophysicsHigh energy astrophysics (739)RedshiftDewey Decimal Classification::500 | Naturwissenschaften::520 | Astronomie Kartographiedetector: sensitivityVIRGOSpace and Planetary Sciencegravitational radiation: emissionBLACK-HOLEddc:520Gravitational wave astronomyGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]STARSGravitacióAstronomySignalGeneral Relativity and Quantum CosmologyBurst astrophysicslocalizationemission010303 astronomy & astrophysicsPhysicsDetectorGamma-ray bursts (629)[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave sourcePRECURSOR ACTIVITYGamma-ray burstsLIGO (920)High energy astrophysicsdata analysis methodBurst astrophysics (187)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstAstronomy & AstrophysicsMASSgravitational radiation: direct detectionGravitational wave astronomy Gravitational wave sources LIGO; Gravitational waves Gamma-ray bursts Burst astrophysics High energy astrophysicsGravitational wave astronomy (675)electromagnetic field: production0103 physical sciencesnumerical calculationsGRB; gravitational waves; LIGO; VirgoSTFC0105 earth and related environmental sciencesgravitational wavesneutron starsGravitational waveCOUNTERPARTgravitational radiationLIGOcore-collapsegravitational radiation detectorGravitational wave sources (677)radiationNeutron starPhysics and AstronomymassRADIATIONEMISSIONGravitational wave astronomy; Gravitational wave sources; LIGO; Gravitational waves; Gamma-ray bursts; Burst astrophysics; High energy astrophysics
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Los fueros del sujeto

1981

CIENCIAS SOCIALESPublicaciones: Obra periodística: Columnas y artículos de opiniónVidal-Beneyto JoséCOMUNICACIÓNSujetoObjetividadEdgar Morin
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Measurement of the lifetime of tau-lepton

1996

The tau lepton lifetime is measured with the L3 detector at LEP using the complete data taken at centre-of-mass energies around the Z pole resulting in tau_tau = 293.2 +/- 2.0 (stat) +/- 1.5 (syst) fs. The comparison of this result with the muon lifetime supports lepton universality of the weak charged current at the level of six per mille. Assuming lepton universality, the value of the strong coupling constant, alpha_s is found to be alpha_s(m_tau^2) = 0.319 +/- 0.015(exp.) +/- 0.014 (theory). The tau lepton lifetime is measured with the L3 detector at LEP using the complete data taken at centre-of-mass energies around the Z pole resulting in τ τ =293.2 ± 2.0 (stat) ± 1.5 (syst) fs . The c…

COLLISIONSNuclear and High Energy PhysicsParticle physicsLUND MONTE-CARLOPAIR PRODUCTIONElectron–positron annihilationFOS: Physical sciencesElementary particleddc:500.201 natural sciences7. Clean energyResonance (particle physics)JET FRAGMENTATIONDECAYSHigh Energy Physics - ExperimentNuclear physicsParticle decayHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]SILICON MICROVERTEX DETECTORPRECISE MEASUREMENTLimit (mathematics)QCD ANALYSIS010306 general physicsL3 EXPERIMENTCoupling constantPhysicsMuonAnnihilationTEST BEAME+E-PHYSICS010308 nuclear & particles physicsALPHA(S)High Energy Physics::PhenomenologyDetectorPair productionSPECTRAL FUNCTIONSComputingMethodologies_DOCUMENTANDTEXTPROCESSINGHigh Energy Physics::ExperimentParticle Physics - ExperimentLeptonNuclear and Particle Physics Proceedings
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Search for neutral heavy leptons produced in Z decays

1997

Weak isosinglet Neutral Heavy Leptons ($\nu_m$) have been searched for using data collected by the DELPHI detector corresponding to $3.3\times 10^{6}$ hadronic~Z$^{0}$ decays at LEP1. Four separate searches have been performed, for short-lived $\nu_m$ production giving monojet or acollinear jet topologies, and for long-lived $\nu_m$ giving detectable secondary vertices or calorimeter clusters. No indication of the existence of these particles has been found, leading to an upper limit for the branching ratio $BR($Z$^0\rightarrow \nu_m \overline{\nu})$ of about $1.3\times10^{-6}$ at 95\% confidence level for $\nu_m$ masses between 3.5 and 50 GeV/$c^2$. Outside this range the limit weakens rap…

COLLISIONSParticle physicsE+E ANNIHILATIONPhysics and Astronomy (miscellaneous)Electron–positron annihilationHadronMASSJet (particle physics)HIGH-ENERGY-PHYSICS; MONOJET PRODUCTION; E+E ANNIHILATION; MONTE-CARLO; BOSON; LIMITS; MASS; LEP; PERFORMANCE; COLLISIONSHIGH-ENERGY-PHYSICS01 natural sciences7. Clean energyMONOJET PRODUCTIONNuclear physicsLIMITSMONTE-CARLO0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsDELPHIBosonPhysics010308 nuclear & particles physicsBranching fractionHigh Energy Physics::PhenomenologyBOSONLEPPERFORMANCELARGE ELECTRON POSITRON COLLIDERPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHILarge Electron–Positron ColliderPARTICLE PHYSICSHigh Energy Physics::ExperimentNeutrinoParticle Physics - ExperimentLepton
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Charged particle multiplicity distributions in restricted rapidity intervals in Z0 hadronic decays.

1991

The multiplicity distributions of charged particles in restricted rapidity intervals in Z0 hadronic decays measured by the DELPHI detector are presented. The data reveal a shoulder structure, best visible for intervals of intermediate size, i.e. for rapidity limits around ±1.5. The whole set of distributions including the shoulder structure is reproduced by the Lund Parton Shower model. The structure is found to be due to important contributions from 3-and 4-jet events with a hard gluon jet. A different model, based on the concept of independently produced groups of particles, "clans", fluctuating both in number per event and particle content per clan, has also been used to analyse the pres…

COLLISIONSParticle physicsE+E ANNIHILATIONPhysics and Astronomy (miscellaneous)LUND MONTE-CARLOElectron–positron annihilationHadronElementary particlePETRA ENERGIES01 natural sciences250 GEV/CNuclear physicsDEPENDENCE0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]RapidityNuclear Experiment010306 general physicsParton showerEngineering (miscellaneous)LUND MONTE-CARLO; JET PRODUCTION-RATES; E+E ANNIHILATION; 250 GEV/C; PETRA ENERGIES; COLLISIONS; DEPENDENCE; FRAGMENTATION; QCD; RESONANCEPhysics010308 nuclear & particles physicsJET PRODUCTION-RATESMultiplicity (mathematics)RESONANCEQCDCharged particleGluonPhysique des particules élémentairesHigh Energy Physics::ExperimentFRAGMENTATIONParticle Physics - Experiment
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"Table 12" of "Measurement of the inclusive jet cross-section in p anti-p collisions at s**(1/2) =1.96-TeV"

1970

Correction factors for hadronization, underlying event and total non-perturbative effects for the absolute value of the jet rapidity in the range 0.4 to 0.8.

CORRECTIONInclusive20477612047761PBAR P --&gt; JET XHigh Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic AstrophysicsJet Production
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"Table 7" of "Measurement of the inclusive jet cross-section in p anti-p collisions at s**(1/2) =1.96-TeV"

1970

Correction factors for hadronization, underlying event and total non-perturbative effects for the absolute value of the jet rapidity in the range 0.0 to 0.4.

CORRECTIONInclusive20477612047761PBAR P --&gt; JET XHigh Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic AstrophysicsJet ProductionAstrophysics::Galaxy Astrophysics
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"Table 22" of "Measurement of the inclusive jet cross-section in p anti-p collisions at s**(1/2) =1.96-TeV"

1970

Correction factors for hadronization, underlying event and total non-perturbative effects for the absolute value of the jet rapidity in the range 1.2 to 1.6.

CORRECTIONInclusive20477612047761PBAR P --&gt; JET XHigh Energy Physics::ExperimentJet Production
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