Search results for "Swift"

showing 10 items of 39 documents

Generalized complex Swift-Hohenberg equation for optical parametric oscillators

1997

A generalized complex Swift-Hohenberg equation including diffraction and nonlinear resonance terms is derived for spatially extended nondegenerate optical parametric oscillators (OPOs) with flat end mirrors. For vanishing pump detuning this equation becomes the complex Swift-Hohenberg (SH) equation valid also for lasers. Nevertheless the similarities between OPOs and lasers are limited, since the diffractive character of OPOs is lost when the diffraction coefficients of signal and idler fields are equal. This manifests, e.g., in the absence of advection by traveling waves (TWs), a clear difference with lasers. When pump detuning is nonzero a nonlinear resonance develops, as it occurs in deg…

PhysicsDiffractionOPOSBistabilityDegenerate energy levelsPhysics::OpticsLaserAtomic and Molecular Physics and Opticslaw.inventionSwift–Hohenberg equationlawQuantum mechanicsNonlinear resonanceParametric statisticsPhysical Review A
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Swift Observations of GRB 070110: An Extraordinary X-Ray Afterglow Powered by the Central Engine

2007

We present a detailed analysis of Swift multi-wavelength observations of GRB 070110 and its remarkable afterglow. The early X-ray light curve, interpreted as the tail of the prompt emission, displays a spectral evolution already seen in other gamma-ray bursts. The optical afterglow shows a shallow decay up to ~2 d after the burst, which is not consistent with standard afterglow models. The most intriguing feature is a very steep decay in the X-ray flux at ~20 ks after the burst, ending an apparent plateau. The abrupt drop of the X-ray light curve rules out an external shock as the origin of the plateau in this burst and implies long-lasting activity of the central engine. The temporal and s…

PhysicsSwiftAstrophysics::High Energy Astrophysical PhenomenaSpectral propertiesAstrophysics (astro-ph)X-rayPhase pointFOS: Physical sciencesGamma Rays: Bursts; X-rays: individual (GRB 070110)Astronomy and AstrophysicsAstrophysicsAstrophysicsLight curveAfterglowGamma Rays: BurstsSpace and Planetary ScienceMillisecond pulsarGamma-ray burstcomputerX-rays: individual (GRB 070110)computer.programming_language
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Swift follow-up of IceCube triggers, and implications for the Advanced-LIGO era

2015

Between 2011 March and 2014 August Swift responded to 20 triggers from the IceCube neutrino observatory, observing the IceCube 50% confidence error circle in X-rays, typically within 5 hours of the trigger. No confirmed counterpart has been detected. We describe the Swift follow up strategy and data analysis and present the results of the campaign. We discuss the challenges of distinguishing the X-ray counterpart to a neutrino trigger from serendipitous uncatalogued X-ray sources in the error circle, and consider the implications of our results for future strategies for multi-messenger astronomy, with particular reference to the follow up of gravitational wave triggers from the advanced-era…

PhysicsSwiftHigh Energy Astrophysical Phenomena (astro-ph.HE)Astrophysics::High Energy Astrophysical PhenomenaAstronomyLibrary scienceFOS: Physical sciencesAstronomy and AstrophysicsMethods observationalLIGOSpace and Planetary Scienceddc:520Astrophysics - High Energy Astrophysical Phenomenacomputercomputer.programming_language
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The Status of the Ultra Fast Flash Observatory - Pathfinder

2012

On behalf of the UFFO Collaboration; International audience; The Ultra Fast Flash Observatory (UFFO) is a project to study early optical emissions from Gamma Ray Bursts (GRBs). The primary scientific goal of UFFO is to see if GRBs can be calibrated with their rising times, so that they could be used as new standard candles. In order to minimize delay in optical follow-up measurements, which is now about 100 sec after trigger from the Swift experiment, we rotate a mirror to redirect light path so that optical measurement can be performed within a second after the trigger. We have developed a pathfinder mission, UFFO-pathfinder to launch on board the Lomonosov satellite in 2012. In this talk,…

PhysicsSwiftNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]AstronomyCosmic ray01 natural sciencesAtomic and Molecular Physics and OpticsEarly Light Emissions[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Flash (photography)PathfinderObservatory0103 physical sciencesGamma Ray BurstsUltra fastSatelliteGamma-ray burst010303 astronomy & astrophysicscomputerUltra Fast Flash Observatorycomputer.programming_language
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Stability of localized structures in the Swift-Hohenberg equation.

1999

We show that nonmonotonic (oscillatory) decay of the boundaries of phase domains is crucial for the stability of localized structures in systems described by Swift-Hohenberg equation. The less damped (more oscillatory) are the boundaries, the larger are the existence ranges of the localized structures. For very weakly damped spatial oscillations, higher-order localized structures are possible.

PhysicsSwift–Hohenberg equationPhase (matter)Quantum mechanicsStability (probability)Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics
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OpenTIMS, TimsPy, and TimsR: Open and Easy Access to timsTOF Raw Data

2021

The Bruker timsTOF Pro is an instrument that couples trapped ion mobility spectrometry (TIMS) to high-resolution time-of-flight (TOF) mass spectrometry (MS). For proteomics, lipidomics, and metabolomics applications, the instrument is typically interfaced with a liquid chromatography (LC) system. The resulting LC-TIMS-MS data sets are, in general, several gigabytes in size and are stored in the proprietary Bruker Tims data format (TDF). The raw data can be accessed using proprietary binaries in C, C++, and Python on Windows and Linux operating systems. Here we introduce a suite of computer programs for data accession, including OpenTIMS, TimsR, and TimsPy. OpenTIMS is a C++ library capable …

Proteomics0301 basic medicineSwift030102 biochemistry & molecular biologyComputer scienceReading (computer)SuiteGeneral Chemistrycomputer.file_formatPython (programming language)Hierarchical Data Formatcomputer.software_genreBiochemistryMass Spectrometry03 medical and health sciences030104 developmental biologyData accessIon Mobility SpectrometryOperating systemRaw datacomputerSoftwareChromatography Liquidcomputer.programming_languageCodebaseJournal of Proteome Research
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Piezospectroscopic study of mechanical stress in Al2O3:Cr under swift heavy ion irradiation

2009

Abstract The spatial distribution of mechanical stresses in Al2O3:Cr single crystal irradiated with (1 ÷ 3) MeV/amu Kr, Xe and Bi ions has been studied by using laser confocal scanning microscopy technique. The stress level as a function of the ion penetration depth has been evaluated from depth-resolved photostimulated R-line luminescence spectra exploiting the piezospectroscopic method. As it was found, the stress field generated by swift heavy ion irradiation is composed of stresses with maximal magnitude comparable with the ultimate stress limit of ruby crystals. Experimental data are discussed in the framework of a model considering the Cr3+ atoms as individual piezosensors.

Stress fieldSwift heavy ionMaterials scienceRadiation damageIrradiationAtomic physicsConfocal scanning microscopyCondensed Matter PhysicsPenetration depthInstrumentationSingle crystalSurfaces Coatings and FilmsIonVacuum
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Phase-bistable patterns and cavity solitons induced by spatially periodic injection into vertical-cavity surface-emitting lasers

2014

Spatial rocking is a kind of resonant forcing able to convert a self-oscillatory system into a phase-bistable, pattern forming system, whereby the phase of the spatially averaged oscillation field locks to one of two values differing by $\ensuremath{\pi}$. We propose the spatial rocking in an experimentally relevant system---the vertical-cavity surface-emitting laser (VCSEL)---and demonstrate its feasibility through analytical and numerical tools applied to a VCSEL model. We show phase bistability, spatial patterns, such as roll patterns, domain walls, and phase (dark-ring) solitons, which could be useful for optical information storage and processing purposes.

Surface (mathematics)PhysicsField (physics)Bistabilitybusiness.industryOscillationPhase (waves)Physics::OpticsÒpticaLaserSEMICONDUCTOR-LASERS; OPTICAL-SYSTEMSAtomic and Molecular Physics and OpticsVertical-cavity surface-emitting laserlaw.inventionOpticslawDYNAMICS; OSCILLATORS; PIXELSSpatial ecologySWIFT-HOHENBERG EQUATION; LOCALIZED STRUCTURES;businessPhysical Review A
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Optical counterpart to Swift J0243.6+6124

2020

Context. Swift J0243.6+6124 is a unique system. It is the first and only ultra-luminous X-ray source in our Galaxy. It is the first and only high-mass Be X-ray pulsar showing radio jet emission. It was discovered during a giant X-ray outburst in October 2017. While there are numerous studies in the X-ray band, very little is known about the optical counterpart. Aims. Our aim is to characterize the variability timescales in the optical and infrared bands in order to understand the nature of this intriguing system. Methods. We performed optical spectroscopic observations to determine the spectral type. Long-term photometric light curves together with the equivalent width of the Hα line were u…

Swift010504 meteorology & atmospheric sciencesBe starAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAngular velocityAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsindividual: swift J0243.6+6124 [Stars]Star (graph theory)01 natural sciencesLuminosity0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencescomputer.programming_languageHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPhotosphereAstronomy and AstrophysicsBeneutron [Stars]DissipationCircumstellar diskSpace and Planetary ScienceAstrophysics::Earth and Planetary Astrophysicsemission line [Stars]Astrophysics - High Energy Astrophysical Phenomenacomputerclose [Binaries]binaries [X rays]
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“The drops which fell from Shakespear’s Pen”: Hamlet in Contemporary Fiction

2012

Questions of gender, ethnicity and sexuality have all been raised by novelists intent on rewriting Shakespeare from the position of what have been seen as cultural margins. While discussions of such rewritings are ongoing, few concerted efforts have been made to trace a pattern in the treatment of Shakespearean allusion and adaptation at the hands of British and American writers of the literary mainstream. The present essay sets out to investigate the way in which three such writers —Ian McEwan, Graham Swift, and John Updike— employ allusion to/adaptations of Hamlet in their novels and what their respective stances reveal about their understanding of their role as canonical writers.

SwiftEmbryologymedia_common.quotation_subjectEthnic groupHuman sexualitylcsh:PR1-9680HamletAllusionMainstreamAdaptationHamlet (place)media_commoncomputer.programming_languageLiteraturegeographylcsh:English languagegeography.geographical_feature_categoryAllusionbusiness.industryShakespeare WilliamFellCell BiologyArtlcsh:English literatureTrace (semiology)lcsh:PE1-3729AnatomyContemporary fictionbusinessFilología InglesacomputerDevelopmental Biology
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