Search results for "lazar"

showing 10 items of 91 documents

L'Universitaire au pouvoir. Le discours juridique du professorat salazariste (1926-1974)

2023

In the shadow of the military, the Portugal of the Estado Novo (New State) was above all led by academics, especially those from the Faculty of Law in Coimbra. The generation of teachers born in 1880/1890, including all the deans (Beleza dos Santos, Cabral de Moncada, Fezas Vital, Figueiredo, etc.), gathered around Salazar, who held the chairs of public finance and political economy in Coimbra, and irrigated the state apparatus. It thus engendered an "Empire of the professor", a "dictatorship of the doctors" and even a cathedocracy. The present work studies their constitutional and legal thinking, explaining all their reforms (1933 Constitution, prison reform, codifications, especially in c…

Droit constitutionnel portugaisSalazarDroit corporatif[SHS.DROIT] Humanities and Social Sciences/LawProfesseurs de droitCorporative lawCorporativismoCorporatismeProfessores de direitoDroit administratifSalazarismeAdministration pénitentaireDroit pénal & procédure pénaleSalazarismoDireito constitucionalLaw professorsCorporatisme autoritaire
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Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data

2014

A search for high-energy neutrinos interacting within the IceCube detector between 2010 and 2012 provided the first evidence for a high-energy neutrino flux of extraterrestrial origin. Results from an analysis using the same methods with a third year (2012-2013) of data from the complete IceCube detector are consistent with the previously reported astrophysical flux in the 100 TeV - PeV range at the level of $10^{-8}\, \mathrm{GeV}\, \mathrm{cm}^{-2}\, \mathrm{s}^{-1}\, \mathrm{sr}^{-1}$ per flavor and reject a purely atmospheric explanation for the combined 3-year data at $5.7 \sigma$. The data are consistent with expectations for equal fluxes of all three neutrino flavors and with isotrop…

FLUXACTIVE GALACTIC NUCLEICosmology and Nongalactic Astrophysics (astro-ph.CO)TELESCOPESolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyIceCubeIceCube Neutrino ObservatoryHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)SEARCH0103 physical sciencesddc:550010303 astronomy & astrophysicsGAMMA-RAY BURSTSPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsGlashow resonanceHigh Energy Physics::PhenomenologyASTRONOMYAstronomySolar neutrino problemBLAZARSPhysics and AstronomyNeutrino detector13. Climate actionLEPTONSJETSMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyEMISSIONAstrophysics - High Energy Astrophysical PhenomenaphysicsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review Letters
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Nazioni senza frontiere. Daniel J. Elazar e l’etica del patto nella storia d’Europa

2020

Gli studi sul federalismo di Daniel J. Elazar sono noti soprattutto per la centralità lessicale ed ermeneutica attribuita al concetto di patto nei diversi ambiti culturali e istituzionali in cui prende forma il discorso politico. In questo saggio si mette a tema la sua ricostruzione dei passaggi ideologici che fanno da sottofondo all'evoluzione storica del federalismo nello scenario politico europeo. Daniel J. Elazar explores federalism by highlighting the lexical and hermeneutic centrality of the concept of the covenant in the various cultural and institutional spheres. This essay focuses on his reconstruction of the historical and ideological steps of federalism in the European political …

Federalism Daniel J. Elazar Covenantalism Covenant History of European unificationSettore SPS/02 - Storia Delle Dottrine PoliticheFederalismo Daniel J. Elazar Storia dell'unificazione europea
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Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation

2021

Full list of authors: Abdalla, H.; Abe, H.; Acero, F.; Acharyya, A.; Adam, R.; Agudo, I; Aguirre-Santaella, A.; Alfaro, R.; Alfaro, J.; Alispach, C.; Aloisio, R.; Batista, R. Alves; Amati, L.; Amato, E.; Ambrosi, G.; Anguner, E. O.; Araudo, A.; Armstrong, T.; Arqueros, F.; Arrabito, L.; Asano, K.; Ascasibar, Y.; Ashley, M.; Backes, M.; Balazs, C.; Balbo, M.; Balmaverde, B.; Baquero Larriva, A.; Martins, V. Barbosa; Barkov, M.; Baroncelli, L.; de Almeida, U. Barres; Barrio, J. A.; Batista, P-, I; Becerra Gonzalez, J.; Becherini, Y.; Beck, G.; Tjus, J. Becker; Belmont, R.; Benbow, W.; Bernardini, E.; Berti, A.; Berton, M.; Bertucci, B.; Beshley, V; Bi, B.; Biasuzzi, B.; Biland, A.; Bissaldi, …

Gamma ray AstronomyCherenkov Telescope ArrayaxionsMATÉRIA ESCURAredshift: dependenceAstronomyGamma ray experimentsgamma ray experimentsAstrophysics01 natural sciencesCosmologyObservatorycosmological model: parameter spacegamma ray experimentHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEPhysicsCherenkov telescopes ; IACT technique ; Gamma rays ; Cosmic raysnew physics4. EducationSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsGamma-ray astronomyviolation: Lorentz3. Good healthobservatoryExtragalactic background lightastro-ph.COaxion-like particlesFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic Astrophysicsgamma ray: propagationCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusAxionsAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsinvariance: Lorentzjet: relativisticdark matter: halo0103 physical sciencesactive galactic nuclei; gamma ray experiments; axions; extragalactic magnetic fieldsAGNBlazarbackground010308 nuclear & particles physicsFísicaAstronomy and AstrophysicssensitivityCherenkov Telescope Arrayaxionextragalactic magnetic fieldsactive galactic nuclei[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]absorptionstatisticalBlazarsTelescopes
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Atmospheric and astrophysical neutrinos above 1 TeV interacting in IceCube

2015

The IceCube Neutrino Observatory was designed primarily to search for high-energy (TeV--PeV) neutrinos produced in distant astrophysical objects. A search for $\gtrsim 100$~TeV neutrinos interacting inside the instrumented volume has recently provided evidence for an isotropic flux of such neutrinos. At lower energies, IceCube collects large numbers of neutrinos from the weak decays of mesons in cosmic-ray air showers. Here we present the results of a search for neutrino interactions inside IceCube's instrumented volume between 1~TeV and 1~PeV in 641 days of data taken from 2010--2012, lowering the energy threshold for neutrinos from the southern sky below 10 TeV for the first time, far bel…

HIGH-ENERGY NEUTRINOSNuclear and High Energy PhysicsParticle physicsAMANDAMesonSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaINDUCED CASCADESFOS: Physical sciencesCosmic rayAstrophysicsFLUX PREDICTIONS01 natural sciencesIceCube Neutrino ObservatoryIceCubeObservatorySEARCH0103 physical sciencesddc:530Blazar010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsASTRONOMYPERFORMANCEBLAZARSPROMPT LEPTONSGAMMA-RAYPhysics and AstronomyHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical PhenomenaphysicsPhysical Review D
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A Connection Between Apparent VLBA Jet Speeds and Initial Active Galactic Nucleus Detections Made by the Fermi Gamma-ray Observatory

2009

In its first three months of operations, the Fermi Gamma-Ray Observatory has detected approximately one quarter of the radio-flux-limited MOJAVE sample of bright flat-spectrum active galactic nuclei (AGNs) at energies above 100 MeV. We have investigated the apparent parsec-scale jet speeds of 26 MOJAVE AGNs measured by the Very Long Baseline Array (VLBA) that are in the LAT bright AGN sample (LBAS). We find that the gamma-ray bright quasars have faster jets on average than the non-LBAS quasars, with a median of 15 c, and values ranging up to 34 c. The LBAS AGNs in which the LAT has detected significant gamma-ray flux variability generally have faster jets than the nonvariable ones. These fi…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsActive galactic nucleus010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsQuasarAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAstrophysics - Astrophysics of GalaxiesGalaxyLuminositySpace and Planetary ScienceObservatoryAstrophysics of Galaxies (astro-ph.GA)0103 physical sciencesBlazarAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsVery Long Baseline ArrayAstrophysics::Galaxy AstrophysicsFermi Gamma-ray Space Telescope
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A survey of active galaxies at TeV photon energies with the HAWC gamma-ray observatory

2020

The High Altitude Water Cherenkov Gamma-Ray Observatory (HAWC) continuously detects TeV photons and particles within its large field-of-view, accumulating every day a deeper exposure of two thirds of the sky. We analyzed 1523~days of HAWC live data acquired over four and a half years, in a follow-up analysis of {138} nearby ($z<0.3$) active galactic nuclei from the {\em Fermi} 3FHL catalog culminating within $40^\circ$ of the zenith at Sierra Negra, the HAWC site. This search for persistent TeV emission used a maximum-likelihood analysis assuming intrinsic power-law spectra attenuated by pair production of gamma-ray photons with the extragalactic background light. HAWC clearly detects persi…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsActive galactic nucleusRadio galaxymedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaGamma rayFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsExtragalactic background lightSpace and Planetary ScienceObservatorySkyBlazarAstrophysics - High Energy Astrophysical PhenomenaCherenkov radiationmedia_common
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The unusual multiwavelength properties of the gamma-ray source PMN J1603-4904

2013

We investigate the nature and classification of PMNJ1603-4904, a bright radio source close to the Galactic plane, which is associated with one of the brightest hard-spectrum gamma-ray sources detected by Fermi/LAT. It has previously been classified as a low-peaked BL Lac object based on its broadband emission and the absence of optical emission lines. Optical measurements, however, suffer strongly from extinction and the absence of pronounced short-time gamma-ray variability over years of monitoring is unusual for a blazar. We are combining new and archival multiwavelength data in order to reconsider the classification and nature of this unusual gamma-ray source. For the first time, we stud…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstrofísicaActive galactic nucleusRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaExtinction (astronomy)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalactic planeAstrophysics - Astrophysics of GalaxiesSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Very-long-baseline interferometryAstronomiaSpectral energy distributionAstrophysics - High Energy Astrophysical PhenomenaBlazarAstrophysics::Galaxy AstrophysicsFermi Gamma-ray Space Telescope
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Numerical simulations of dynamics and emission from relativistic astrophysical jets

2013

Broadband emission from relativistic outflows (jets) of active galactic nuclei (AGN) and gamma-ray bursts (GRBs) contains valuable information about the nature of the jet itself, and about the central engine which launches it. Using special relativistic hydrodynamics and magnetohydronamics simulations we study the dynamics of the jet and its interaction with the surrounding medium. The observational signature of the simulated jets is computed using a radiative transfer code developed specifically for the purpose of computing multi-wavelength, time-dependent, non-thermal emission from astrophysical plasmas. We present results of a series of long-term projects devoted to understanding the dyn…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsHistoryJet (fluid)Active galactic nucleusAstrophysics::High Energy Astrophysical PhenomenaDynamics (mechanics)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsPlasmaAstrophysics01 natural sciences7. Clean energy010305 fluids & plasmasComputer Science ApplicationsEducationAfterglow13. Climate action0103 physical sciencesRadiative transferMagnetohydrodynamicsAstrophysics - High Energy Astrophysical PhenomenaBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsJournal of Physics: Conference Series
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Apparent superluminal core expansion and limb brightening in the candidate neutrino blazar TXS 0506+056

2019

IceCube has reported a very-high-energy neutrino (IceCube-170922A) in a region containing the blazar TXS 0506+056. Correlated {\gamma}-ray activity has led to the first high-probability association of a high-energy neutrino with an extragalactic source. This blazar has been found to be in a radio outburst during the neutrino event. We have performed target-of-opportunity VLBI imaging observations at 43 GHz frequency with the VLBA two and eight months, respectively, after the neutrino event. We produced two images of TXS 0506+056 with angular resolutions of (0.2x1.1) mas and (0.2x0.5) mas, respectively. The source shows a compact, high brightness temperature core (albeit not approaching the …

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)Superluminal motion010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAstrophysics - Astrophysics of GalaxiesGalaxyNeutrino detectorSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)0103 physical sciencesVery-long-baseline interferometryNeutrinoBlazarAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsVery Long Baseline Array
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