Search results for "BAND"

showing 10 items of 2610 documents

The ‘grave of the Court Pit’, A rediscovered Bronze Age tomb from Carchemish

2014

This paper examines the British Museum unpublished records related to an Early Bronze (EB) Age pithos burial uncovered a century ago in the Inner Town at Carchemish. The grave, cursorily cited and variously dated (Chalcolithic, EB or even LBA) in the final reports, was described in some detail by Hogarth and Thompson; a precise dating is, however, possible today thanks to the information of paramount importance given by T. E. Lawrence who identified and took a picture of the associated finds, which was recently rediscovered in the Carchemish Archives. The pithos can be now ascribed to the third quarter of the third millennium BC and helps to confirm the recent theory according to which the …

ArcheologyHistoryHistoryVisual Arts and Performing ArtsMesopotamiaReligious studiesChalcolithicengineering.materialAncient historyArchaeologyCarchemish British Museum excavations T. E. Lawrence D. G. Hogarth EBA burial customs Euphrates Banded Ware Syrian BottlesBronze AgeengineeringBronzeSettore L-OR/05 - Archeologia E Storia Dell'Arte Del Vicino Oriente AnticoQuarter (Canadian coin)
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Photoluminescence Study of ZnSe Single Crystals Obtained by Solid Phase Recrystallization under Different Pressure Conditions. Effects of Thermal Tre…

2002

ZnSe single crystals, obtained by the Solid Phase Recrystallization (SPR) method under three different pressure conditions, 10 and 5 atm of Se, and 2 atm of argon, have been investigated by means of photoluminescence (PL) and optical microscopy. Special attention has been paid to the surface state of the samples. Samples recrystallized under 10 atm of Se present the best rate between the PL response for the excitonic zone and the deep level one that shows a clean PL emission without significant peaks and/or bands. The presence of slip bands has been detected and analysed by means of optical microscopy and photoluminescence. In order to study the changes introduced by post growth thermal tre…

ArgonPhotoluminescenceExcitonLüders bandAnalytical chemistrychemistry.chemical_elementRecrystallization (metallurgy)Thermal treatmentCondensed Matter PhysicsElectronic Optical and Magnetic Materialslaw.inventionCrystallographychemistryOptical microscopelawsense organsSurface statesphysica status solidi (a)
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Role of vitreous matrix on the optical activity of Ge-doped silica

2003

Abstract We report an experimental study on the relationship between the optical activity of Ge-oxygen deficient centers and dynamic properties and conformational heterogeneity of vitreous matrix in silica. We focus our attention on the absorption band at ∼5.2 eV (B 2β ) and on the two related emissions at ∼4.2 eV (α E ) and at ∼3.1 eV (β). From the temperature dependence of B 2β band we estimate a mean energy value of 26 meV for local vibrational modes coupled to the electronic transition, suggesting that the chromophore and its surrounding have access to low frequency dynamics. From the thermal behavior of the two emissions we distinguish the two competitive relaxation processes from the …

Arrhenius equationChemistryRelaxation (NMR)General ChemistryActivation energyChromophoreCondensed Matter PhysicsMolecular physicsMolecular electronic transitionsymbols.namesakeNuclear magnetic resonanceAbsorption bandExcited statesymbolsGeneral Materials ScienceTriplet stateJournal of Physics and Chemistry of Solids
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Broadband dielectric spectroscopy of 0.4PMN-0.3PSN-0.3PZN ceramics

2007

In this paper, results of the broadband dielectric spectroscopy of 0.4PbMg1/3Nb2/3O3-0.3PbZn1/3Nb2/3O3-0.3PbSc1/2Nb1/2O3(0.4PMN-0.3PZN-0.3PSN) are presented. Dielectric spectra of these solutions were investigated in a broad frequency range from 20 Hz to 100 GHz. Very strong and broad dielectric relaxation was analyzed in terms of distribution of relaxations times, using Tichonov regularization method. It revealed slowing down of the longest relaxation and the mean relaxation times in the agreement with the Vogel-Fulcher law and the Arrhenius law, respectively.

Arrhenius equationHistoryMaterials scienceCondensed matter physicsAnalytical chemistryDielectricComputer Science ApplicationsEducationDielectric spectroscopysymbols.namesakeDielectric spectrumvisual_artvisual_art.visual_art_mediumsymbolsCeramicSpectroscopyCole–Cole equationBroadband dielectric spectroscopyJournal of Physics: Conference Series
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Statistical modeling, simulation, and experimental verification of wideband indoor mobile radio channel

2018

This paper focuses on the modeling, simulation, and experimental verification of wideband single-input single-output (SISO) mobile fading channels for indoor propagation environments. The indoor reference channel model is derived from a geometrical rectangle scattering model, which consists of an infinite number of scatterers. It is assumed that the scatterers are exponentially distributed over the two-dimensional (2D) horizontal plane of a rectangular room. Analytical expressions are derived for the probability density function (PDF) of the angle of arrival (AOA), the PDF of the propagation path length, the power delay profile (PDP), and the frequency correlation function (FCF). An efficie…

Article SubjectComputer Networks and CommunicationsComputer sciencelcsh:T020206 networking & telecommunications020302 automobile design & engineeringStatistical model02 engineering and technologyCorrelation function (quantum field theory)lcsh:Technologylcsh:Telecommunication0203 mechanical engineeringAngle of arrivallcsh:TK5101-67200202 electrical engineering electronic engineering information engineeringElectronic engineeringFadingElectrical and Electronic EngineeringWidebandPower delay profileInformation SystemsCommunication channelComputer Science::Information Theory
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El virreinato del arzobispo de Valencia Fray Pedro de Urbina (1650-1652)

2010

El presente artículo analiza el virreinato del arzobispo de Valencia fray Pedro de Urbina, comprendido entre 1650 y 1652 y marcado por el bandolerismo endémico que asolaba el reino; las repercusiones de la guerra de Cataluña en el territorio regnícola; la crisis política del cap i casal; y el pulso sostenido por canónigos y pavordes en el seno de la catedral a resultas de las preeminencias reclamadas por unos y otros. (A)

ArzobisposBandolerismoGuerra de CataluñaUNESCO::HISTORIA::Historia por épocas::Historia antigua:HISTORIA::Historia por épocas::Historia antigua [UNESCO]VirreyesCrisis política
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Polarization calibration techniques for the new-generation VLBI

2020

The calibration and analysis of polarization observations in Very Long Baseline Interferometry (VLBI) requires the use of specific algorithms that suffer from several limitations, closely related to assumptions in the data properties that may not hold in observations taken with new-generation VLBI equipment. Nowadays, the instantaneous bandwidth achievable with VLBI backends can be as high as several GHz, covering several radio bands simultaneously. In addition, the sensitivity of VLBI observations with state-of-the-art equipment may reach dynamic ranges of tens of thousands, both in total intensity and in polarization. In this paper, we discuss the impact of the limitations of common VLBI …

AstrofísicaAstronomyAstrophysics::High Energy Astrophysical PhenomenaPolarimetryFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesRadio spectrumInstantaneous bandwidthSoftware0103 physical sciencesVery-long-baseline interferometry010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy AstrophysicsRemote sensingPhysicsEvent Horizon Telescope010308 nuclear & particles physicsbusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsPolarization (waves)Nonlinear systemSpace and Planetary ScienceAstronomiabusinessAstrophysics - Instrumentation and Methods for Astrophysics
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All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data

2019

We present results of an all-sky search for continuous gravitational waves (CWs), which can be produced by fast-spinning neutron stars with an asymmetry around their rotation axis, using data from the second observing run of the Advanced LIGO detectors. We employ three different semi-coherent methods ($\textit{FrequencyHough}$, $\textit{SkyHough}$, and $\textit{Time-Domain $\mathcal{F}$-statistic}$) to search in a gravitational-wave frequency band from 20 to 1922 Hz and a first frequency derivative from $-1\times10^{-8}$ to $2\times10^{-9}$ Hz/s. None of these searches has found clear evidence for a CW signal, so we present upper limits on the gravitational-wave strain amplitude $h_0$ (the …

AstronomyAstrophysicsRotation01 natural sciencesrotationGravitation Cosmology & AstrophysicsGeneral Relativity and Quantum CosmologyPhysics Particles & Fieldscontinuous gravitational waveLIGOneutron starGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)media_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01Physicsastro-ph.HEPhysicsPhysical SystemsAmplitudeGeneral relativitygravitational wavesPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave detectionAstrophysics - High Energy Astrophysical Phenomenacontinuous gravitational waves; Advanced LIGOcontinuous gravitational wavesasymmetryGravitationNeutron stars & pulsarsGeneral relativityFrequency bandmedia_common.quotation_subjectgr-qcFOS: Physical sciencesalternative theories of gravityGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & AstrophysicsGravitational waves0103 physical sciencesAdvanced LIGOddc:530Gravitation Cosmology & Astrophysics010306 general physicsgravitational radiation: frequencySTFCgravitational wavesneutron starsGravitational wave sourcesScience & TechnologyGravitational wave sources Gravitational waves Physical Systems Neutron stars and pulsars Gravitational wave detection010308 nuclear & particles physicsGravitational waveRCUKGravitational Wave PhysicsLIGONeutron stars & pulsarsNeutron starSkyNeutron stars and pulsarsDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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All-sky search for short gravitational-wave bursts in the second Advanced LIGO and Advanced Virgo run

2019

We present the results of a search for short-duration gravitational-wave transients in the data from the second observing run of Advanced LIGO and Advanced Virgo. We search for gravitational-wave transients with a duration of milliseconds to approximately one second in the 32-4096 Hz frequency band with minimal assumptions about the signal properties, thus targeting a wide variety of sources. We also perform a matched-filter search for gravitational-wave transients from cosmic string cusps for which the waveform is well-modeled. The unmodeled search detected gravitational waves from several binary black hole mergers which have been identified by previous analyses. No other significant event…

AstronomyGravitational waves detectionAstrophysicsdetector: network01 natural sciencesSignalGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsGravitational waves detection Stochastic gravitational-wavebinary [black hole]LIGOgravitational waveQCQBmedia_commonastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01Physicsgravitational waves neutron starsgravitational wavesGeneral relativityburst [gravitational radiation]network [detector]Physical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]direct detection [gravitational radiation]Advanced VirgoAstrophysics - High Energy Astrophysical PhenomenaFrequency bandsensitivity [detector]gr-qcmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesalternative theories of gravityGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & Astrophysicsgravitational radiation: direct detectionemission [gravitational radiation]Binary black holeSettore FIS/05 - Astronomia e Astrofisicabinary: coalescence0103 physical sciencesgravitational radiation: burstAdvanced LIGOWaveformddc:530010306 general physicscosmic stringSTFCScience & Technology010308 nuclear & particles physicsGravitational waveRCUKStochastic gravitational-waveGravitational Wave PhysicsLIGOgravitational radiation detectorgravitational waves; Advanced LIGO; Advanced VirgoCosmic stringdetector: sensitivityVIRGOPhysics and Astronomyblack hole: binarySkygravitational radiation: emissionDewey Decimal Classification::500 | Naturwissenschaften::530 | Physikcoalescence [binary][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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XMM observations of NGC 2516 stars

2007

We present the characteristics of the X-ray variability of stars in the cluster NGC 2516 as derived from XMM-Newton/EPIC/pn data. The X-ray variations on short (hours), medium (months), and long (years) time scales have been explored. We detected 303 distinct X-ray sources by analysing six EPIC/pn observations; 194 of them are members of the cluster. Stars of all spectral types, from the early-types to the late-M dwarfs, were detected. Cone search capability for table J/A+A/456/977/table2 (X-ray and optical properties of NGC 2516 members in the XMM-Newton/EPIC/pn observations having more than 25 counts.)

Astrophysics and AstronomyAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Cosmology and Extragalactic AstrophysicsLate type starsX-ray sourcesstellar astronomyOptical astronomyCosmologyOpen star clustersPhotometryobservational astronomyX ray sourcesAstrophysics::Solar and Stellar AstrophysicsWide-band photometryNatural SciencesLate-type starsAstrophysics::Galaxy AstrophysicsInfrared photometryWide band photometry
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