Search results for "lazar"

showing 10 items of 91 documents

ANTARES constrains a blazar origin of two IceCube PeV neutrino events

2015

Abstract Context. The source(s) of the neutrino excess reported by the IceCube Collaboration is unknown. The TANAMI Collaboration recently reported on the multiwavelength emission of six bright, variable blazars which are positionally coincident with two of the most energetic IceCube events. Objects like these are prime candidates to be the source of the highest-energy cosmic rays, and thus of associated neutrino emission. Aims. We present an analysis of neutrino emission from the six blazars using observations with the ANTARES neutrino telescope. Methods. The standard methods of the ANTARES candidate list search are applied to six years of data to search for an excess of muons and hence th…

Astrofísicaactive [Galaxies]Astrophysics::High Energy Astrophysical PhenomenaMonte Carlo methodFluxFOS: Physical sciencesCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics7. Clean energy01 natural sciencesSpectral line0103 physical sciencesNeutrinoGalaxies: active; Neutrinos; Quasars: generalNeutrinsNeutrinosBlazar010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MuonCosmologia010308 nuclear & particles physicsFísicaAstronomy and Astrophysicsgeneral [Quasars]Galaxies: activeAstronomy and AstrophysicNeutrino astrophysicsQuasars generalCosmologyneutrinos – galaxies: active – quasars: generalQuasars: generalSpace and Planetary ScienceGalaxies activeCol·lisions (Física nuclear)Galaxies: active; Neutrinos; Quasars: general; Astronomy and Astrophysics; Space and Planetary Science:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]FISICA APLICADAFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaMATEMATICA APLICADA[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Event (particle physics)Astronomy & astrophysics
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Gamma-Ray Flares from Mrk421 in 2008 observed with the ARGO-YBJ detector

2010

In 2008 the blazar Markarian 421 entered a very active phase and was one of the brightest sources in the sky at TeV energies, showing frequent flaring episodes. Using the data of ARGO-YBJ, a full coverage air shower detector located at Yangbajing (4300 m a.s.l., Tibet, China), we monitored the source at gamma ray energies E > 0.3 TeV during the whole year. The observed flux was variable, with the strongest flares in March and June, in correlation with X-ray enhanced activity. While during specific episodes the TeV flux could be several times larger than the Crab Nebula one, the average emission from day 41 to 180 was almost twice the Crab level, with an integral flux of (3.6 +-0.6) 10^-1…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysicsBL Lacertae objectSettore FIS/05 - Astronomia E AstrofisicaExtended Air showersSettore FIS/05 - Astronomia e Astrofisicageneral" ["gamma rays]BlazarBL Lacertae objects; Markarian 421; gamma rays; Extended Air showersCherenkov radiationHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSpectral indexindividual (Markarian 421)" ["BL Lacertae objects]Markarian 421Settore FIS/01 - Fisica SperimentaleGamma rayindividual (Markarian 421) - gamma rays: observations [BL Lacertae objects]Astronomy and AstrophysicsAir showerCrab NebulaSpace and Planetary Sciencegamma rayIntergalactic travelAstrophysics - High Energy Astrophysical Phenomena
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ALMA full polarization observations of PKS1830-211 during its record-breaking flare of 2019

2020

We report Atacama Large Millimeter Array (ALMA) Band 6 full-polarization observations of the lensed blazar PKS 1830-211 during its record-breaking radio and gamma-ray flare in the spring of 2019. The observations were taken close to the peak of the gamma activity and show a clear difference in polarization state between the two time-delayed images. The leading image has a fractional polarization about three times lower than the trailing image, implying that significant depolarization occurred during the flare. In addition, we observe clear intra-hour variability of the polarization properties between the two lensed images, with a quasi-linear increase in the differential electric-vector pos…

Astrophysics::High Energy Astrophysical PhenomenaGamma rays: generalgeneral [Gamma rays]FOS: Physical sciencesQuasars: individual: PKS1830-211AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural scienceslaw.inventionlawPolarization0103 physical sciencesindividual: PKS1830-211 [Quasars]Blazar010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomy and AstrophysicsQuasarAtacama Large Millimeter ArrayPolarization (waves)Position angleFractional polarizationSpace and Planetary ScienceAstrophysics - High Energy Astrophysical PhenomenaFlare
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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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High-Frequency Polarization Variability from Active Galactic Nuclei

2021

The linear polarization of non-thermal emission encodes information about the structure of the magnetic fields, either from the region where the emission is produced (i.e., the intrinsic polarization angle) and/or from the screens of magnetized plasma that may be located on its way towards Earth (i.e., the effect of Faraday rotation). In addition, the variability timescale of the polarized emission, or its Faraday rotation, can be used to estimate the size of the region where the emission (or the Faraday rotation) originates. The observation of polarized emission from active galactic nuclei (AGN) and, in particular, its time evolution, also provides information about the critical role that …

Camps magnèticsActive galactic nucleusAstrophysics::High Energy Astrophysical PhenomenaAstronomyquasarsblazarsQB1-991AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencessymbols.namesake0103 physical sciencesFaraday effectBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicspolarization010308 nuclear & particles physicsLinear polarizationAstronomy and AstrophysicsQuasarPlasmaPolarization (waves)Magnetic fieldgamma raysgeneralsymbolsAstronomia
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Integrismo político en EEUU / 2. Integrismo y tortura

2004

Corte PenalVidal-Beneyto JoséAbu GhraibIrakPolíticaPublicaciones: Obra periodística: Columnas y artículos de opiniónPaz comúnPatriaIdeología nacional-religiosaIntegrismoSalazarismoIntegrismo políticoBushDemocraciaCruzadasDiosESTADOS UNIDOSBienTORTURAMalPresosFranquismoFeGuantánamoDerechos HumanosInquisiciónGuerra permanenteIdeologíaInformaciónAmerican way of life
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MOJAVE: Monitoring of Jets in Active Galactic Nuclei with VLBA Experiments. VI. Kinematics Analysis of a Complete Sample of Blazar Jets

2009

We discuss the jet kinematics of a complete flux-density-limited sample of 135 radio-loud active galactic nuclei (AGN) resulting from a 13 year program to investigate the structure and evolution of parsec-scale jet phenomena. Our analysis is based on new 2 cm Very Long Baseline Array (VLBA) images obtained between 2002 and 2007, but includes our previously published observations made at the same wavelength, and is supplemented by VLBA archive data. In all, we have used 2424 images spanning the years 1994-2007 to study and determine the motions of 526 separate jet features in 127 jets. The data quality and temporal coverage (a median of 15 epochs per source) of this complete AGN jet sample r…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusLorentz transformationAstrophysics::High Energy Astrophysical PhenomenaPopulationFOS: Physical sciencesAstrophysicsKinematicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencessymbols.namesake0103 physical scienceseducationBlazar010303 astronomy & astrophysicsVery Long Baseline ArrayPhysicseducation.field_of_study010308 nuclear & particles physicsAstronomy and AstrophysicsWavelength13. Climate actionSpace and Planetary SciencesymbolsDoppler effectAstrophysics - Cosmology and Nongalactic Astrophysics
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El ejército portugués dio paso a la democracia 25 de Abril en Portugal

1999

DemocraciaFuerzas ArmadasSalazarPortugalVidal-Beneyto JoséClavelesTransiciónCapitanesPolíticaMemoria democráticaPublicaciones: Obra periodística: Columnas y artículos de opiniónCaetanoResistenciaRevoluciónEjércitoCaetanismoDictadura
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Soportes de la lucha para la democracia

1996

Notas de José Vidal-Beneyto para un discurso dado en el Centro Nacional de Cultura de Lisboa en octubre 1996.

DemocraciaSalazarCulturaPortugalCooperaciónVidal-Beneyto JoséPactos ibéricosColoquiosIntervenciones públicasDemocracia españolaLibertadMEMORIA DEMOCRÁTICAAcciones: Acciones de una vida: Democracia (II)Lucha democráticaTierra de descubrimientoSeminariosDebates
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De la dictadura a la democracia pasando por la revolución

1999

Se trata del texto de una conferencia de José Vidal-Beneyto. Se desconoce en qué espacio y contexto fue pronunciada y aqunque aquí se recoge la versión mecanografiada por el propio autor, existe una versión publicada en: Vidal-Beneyto, José (2007). Memoria democrática (pp. 149-154). Madrid: Foca.

DemocraciaSociedad civilFuerzas ArmadasSalazarPortugalPluralismo políticoVidal-Beneyto JoséPublicaciones: Obra académico-científica: LibrosTransiciónPolíticaIntervenciones públicasMemoria democráticaCaetanoRuptura políticaResistenciaMovimiento de los CapitanesRevoluciónRuptura socialCaetanismoDictadura
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