Search results for "Interferometry"

showing 10 items of 343 documents

Monitoring the Morphology of M87* in 2009-2017 with the Event Horizon Telescope

2020

All authors: Wielgus, Maciek; Akiyama, Kazunori; Blackburn, Lindy; Chan, Chi-kwan; Dexter, Jason; Doeleman, Sheperd S.; Fish, Vincent L.; Issaoun, Sara; Johnson, Michael D.; Krichbaum, Thomas P.; Lu, Ru-Sen; Pesce, Dominic W.; Wong, George N.; Bower, Geoffrey C.; Broderick, Avery E.; Chael, Andrew; Chatterjee, Koushik; Gammie, Charles F.; Georgiev, Boris; Hada, Kazuhiro Loinard, Laurent; Markoff, Sera; Marrone, Daniel P.; Plambeck, Richard; Weintroub, Jonathan; Dexter, Matthew; MacMahon, David H. E.; Wright, Melvyn; Alberdi, Antxon; Alef, Walter; Asada, Keiichi; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David; Baloković, Mislav; Barausse, Enrico; Barrett, John; Bintley, Dan; Boland, Wilf…

Brightness1663Active galactic nucleus010504 meteorology & atmospheric sciences1346Event horizonAstronomyAstrophysics::High Energy Astrophysical PhenomenaGalaxy accretion disksFOS: Physical sciencesAstrophysicsF500Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences5752033Settore FIS/05 - Astronomia e AstrofisicaSupermassive black holes0103 physical sciencesVery-long-baseline interferometryAstronomy Astrophysics and Cosmology1769010303 astronomy & astrophysicsComputer Vision and Robotics (Autonomous Systems)Astronomy data modelingVery long baseline interferometry0105 earth and related environmental sciences162Black holes; Galaxy accretion disks; Galaxy accretion; Supermassive black holes; Active galactic nuclei; Low-luminosity active galactic nuclei; Very long baseline interferometry; Astronomy data modeling; Radio interferometryEvent Horizon TelescopePhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Active galactic nucleiSupermassive black holeBlack holesAstronomy and Astrophysics16Galaxy accretion562Position angleGalaxyLow-luminosity active galactic nucleiMedical Image ProcessingSpace and Planetary ScienceRadio interferometryAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]1859
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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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Detection of Intrinsic Source Structure at ~3 Schwarzschild Radii with Millimeter-VLBI Observations of SAGITTARIUS A*

2018

We report results from very long baseline interferometric (VLBI) observations of the supermassive black hole in the Galactic center, Sgr A*, at 1.3 mm (230 GHz). The observations were performed in 2013 March using six VLBI stations in Hawaii, California, Arizona, and Chile. Compared to earlier observations, the addition of the APEX telescope in Chile almost doubles the longest baseline length in the array, provides additional {\it uv} coverage in the N-S direction, and leads to a spatial resolution of $\sim$30 $\mu$as ($\sim$3 Schwarzschild radii) for Sgr A*. The source is detected even at the longest baselines with visibility amplitudes of $\sim$4-13% of the total flux density. We argue th…

BrightnessAstrophysics::High Energy Astrophysical PhenomenaAstronomyFOS: Physical sciencesContext (language use)General Relativity and Quantum Cosmology (gr-qc)Astrophysics01 natural sciencesGeneral Relativity and Quantum Cosmologylaw.inventionTelescopelaw0103 physical sciencesVery-long-baseline interferometry010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsSupermassive black hole010308 nuclear & particles physicsGalactic CenterAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesSagittarius A*Space and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Schwarzschild radius
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A Robust and Simple Measure for Quality-Guided 2D Phase Unwrapping Algorithms

2016

Quality-based 2D phase unwrapping algorithms provide one of the best tradeoffs between speed and quality of results. Their robustness depends on a quality map, which is used to build a path that visits the most reliable pixels first. Unwrapping then proceeds along this path, delaying unwrapping of noisy and inconsistent areas until the end, so that the unwrapping errors remain local. We propose a novel quality measure that is consistent, technically sound, effective, fast to compute, and immune to the presence of a carrier signal. The new measure combines the benefits of both the quality-guided and the residue-based phase unwrapping approaches. The quality map is justified from the two diff…

Carrier signalPixelbusiness.industryComputer science0211 other engineering and technologiesHolography02 engineering and technology01 natural sciencesComputer Graphics and Computer-Aided DesignPhase unwrappingGeneralLiterature_MISCELLANEOUSlaw.invention010309 opticsInterferometryRobustness (computer science)law0103 physical sciencesComputer visionArtificial intelligencebusinessAlgorithmSoftware021101 geological & geomatics engineeringIEEE Transactions on Image Processing
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Kinetics of rat CSD-C2 binding to H3.3 RNA

2017

Cold-shock domain containing protein C2 (CSD-C2; also known as PIPPin) is an RNA-binding protein conserved in the evolution that interacts with the 3’-untranslated region (3’-UTR) of rat H1.0 and H3.3 histone messengers. Biolayer interferometry (BLI) is a technique that measures changes in an interference pattern generated from visible light, reflected from an optical layer, and a biolayer which contains molecules of interest. In this study, we used the BLI methodology in order to analyze and describe the binding properties of CSD-C2 and the mRNA encoding the rat brain histone protein H3.3. Recombinant CSD-C2 was incubated with in vitro transcribed, and biotinylated H3.3 RNA fragments bound…

Chemistry0206 medical engineeringKineticsRNA02 engineering and technology021001 nanoscience & nanotechnology020601 biomedical engineeringSettore BIO/10 - BiochimicaAutomotive EngineeringBiophysicsRNA-protein interactions CSD-C2 Histone H3.3 RNA Biolayer interferometry.Settore BIO/06 - Anatomia Comparata E Citologia0210 nano-technology
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Detection of local specular gloss and surface roughness from black prints

2007

A combination of optical and tomographic imaging techniques for inspection of local surface roughness and specular gloss of black prints and coated paper are introduced. A diffractive optical-element-based glossmeter (DOG) and a low-coherence interferometer (LCI) were used to obtain local information about the print in terms of topographic and gloss maps. X-ray microcomputed tomography (μCT) was used to obtain 3D local structural information of the coated paper. Gloss and topographic maps were used to determine statistical gloss and roughness parameters. These parameters were useful when analysing the surface condition of prints and coated paper. We found an orientation-dependent gloss slop…

Coated paperInterferometryColloid and Surface ChemistryOpticsMaterials scienceTomographic reconstructionbusiness.industrySurface roughnessSurface finishSpecular reflectionTomographybusinessGloss (optics)Colloids and Surfaces A: Physicochemical and Engineering Aspects
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Automatic fringe pattern enhancement using truly adaptive period-guided bidimensional empirical mode decomposition.

2020

Fringe patterns encode the information about the result of a measurement performed via widely used optical full-field testing methods, e.g., interferometry, digital holographic microscopy, moiré techniques, structured illumination etc. Affected by the optical setup, changing environment and the sample itself fringe patterns are often corrupted with substantial noise, strong and uneven background illumination and exhibit low contrast. Fringe pattern enhancement, i.e., noise minimization and background term removal, at the pre-processing stage prior to the phase map calculation (for the measurement result decoding) is therefore essential to minimize the jeopardizing effect the mentioned error…

Computer sciencePhase contrast microscopyStructured illumination microscopy02 engineering and technology01 natural sciencesHilbert–Huang transformlaw.invention010309 opticsOpticslaw0103 physical sciencesbusiness.industrySignal reconstructionVDP::Technology: 500Moiré patternFilter (signal processing)021001 nanoscience & nanotechnologyAtomic and Molecular Physics and OpticsInterferometryVDP::Teknologi: 500Digital holographic microscopySpatial frequencySpeckle imaging0210 nano-technologybusinessAlgorithmOptics express
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Multi-beam capabilities for high precision astrometry at low frequencies using VLBI

2011

We are carrying out a simulation study to characterise the advantages of VLBI with multiple beams, which will be a feature of the next generation of instruments. We will focus on VLBI astrometric measurements at lower frequencies (1.4 GHz and below). For our simulations, we have selected a network consisting of ASKAP, the Australian SKA precursor, plus existing Australian antennas from the LBA (Long Baseline Array) and the new antenna in New Zealand (figure 1a). We have used different models to represent the ionospheric turbulences and frequencies. The preliminary results show an improvement of an order of magnitude in the astrometric precision achieved using multiple calibrators with angul…

Computer scienceVery-long-baseline interferometryAstrophysics::Instrumentation and Methods for AstrophysicsMulti beamPhase (waves)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrometryAntenna (radio)Focus (optics)GeodesyAstrophysics::Galaxy AstrophysicsRemote sensing
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Phase-shifting of correlation fringes created by image processing as an alternative to improve digital shearography

2016

Abstract The adoption of digital speckle pattern shearing interferometry, or speckle shearography, is well known in many areas when one needs to measure micro-displacements in-plane and out of the plane in biological and non-biological objects; it is based on the Michelson's Interferometer with the use of a piezoelectric transducer (PZT) in order to provide the phase-shift of the fringes and then to improve the quality of the final image. The creation of the shifting images using a PZT, despite its widespread use, has some drawbacks or limitations, such as the cost of the apparatus, the difficulties in applying the same displacement in the mirror repeated times, and when the phase-shift can…

Computer sciencebusiness.industryImage processingSpeckle noise02 engineering and technology021001 nanoscience & nanotechnology01 natural sciencesAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic Materials010309 opticsSpeckle patternInterferometryOpticsShearographyRobustness (computer science)Electronic speckle pattern interferometry0103 physical sciencesSpeckle imagingElectrical and Electronic EngineeringPhysical and Theoretical Chemistry0210 nano-technologybusinessOptics Communications
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Interferometric measurement of complex-field changes in transient detection imaging.

2020

We report an experimental method that combines nonlinear-crystal-based transient detection imaging (TDI) with interferometric complex-field retrieval. The system allows measuring both phase and amplitude of a dynamic scene while suppressing stationary background. Theoretical and experimental results prove the linear relation existing between input and output phases, as well as the benefits of phase analysis for both detection and measurement with high resolutions of λ/30, even under noisy conditions. Additionally, we present experimental evidence of the remarkable ability of the technique to detect phase sign changes in the scene —what we call differential-phase TDI— showing great detection…

Computer sciencebusiness.industryPhase (waves)02 engineering and technologyÒptica021001 nanoscience & nanotechnology01 natural sciencesAtomic and Molecular Physics and Optics010309 opticsInterferometryAmplitudeOptics0103 physical sciencesCalibrationSensitivity (control systems)Transient (oscillation)0210 nano-technologyPhase retrievalbusinessPhase modulationOptics express
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