Search results for "FOS"

showing 10 items of 15075 documents

Breather Molecular Complexes in a Passively Mode‐Locked Fiber Laser

2021

International audience; Breathing solitons are nonlinear waves in which the energy concentrates in a localized and oscillatory fashion. Similarly to stationary solitons, breathers in dissipative systems can form stable bound states displaying molecule-like dynamics, which are frequently called breather molecules. So far, the experimental observation of optical breather molecules and the real-time detection of their dynamics are limited to diatomic molecules, that is, bound states of only two breathers. In this work, the observation of different types of breather complexes in a mode-locked fiber laser: multibreather molecules, and molecular complexes originating from the binding of two breat…

BreatherFOS: Physical sciences02 engineering and technology01 natural sciencesMolecular physics010309 opticsFiber laser0103 physical sciencesBound statePhysics::Chemical PhysicsNonlinear Sciences::Pattern Formation and SolitonsPhysics[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]Intermolecular force021001 nanoscience & nanotechnologyCondensed Matter PhysicsDiatomic moleculeAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsNonlinear Sciences::Exactly Solvable and Integrable SystemsMode-lockingDissipative systemSoliton0210 nano-technologyPhysics - OpticsOptics (physics.optics)
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Extropy: Complementary Dual of Entropy

2015

This article provides a completion to theories of information based on entropy, resolving a longstanding question in its axiomatization as proposed by Shannon and pursued by Jaynes. We show that Shannon's entropy function has a complementary dual function which we call "extropy." The entropy and the extropy of a binary distribution are identical. However, the measure bifurcates into a pair of distinct measures for any quantity that is not merely an event indicator. As with entropy, the maximum extropy distribution is also the uniform distribution, and both measures are invariant with respect to permutations of their mass functions. However, they behave quite differently in their assessments…

Bregman divergenceFOS: Computer and information sciencesStatistics and ProbabilitySettore MAT/06 - Probabilita' E Statistica MatematicaKullback–Leibler divergenceComputer Science - Information TheoryGeneral MathematicsFOS: Physical sciencesBinary numberMathematics - Statistics TheoryStatistics Theory (math.ST)Kullback–Leibler divergenceBregman divergenceproper scoring rulesGini index of heterogeneityDifferential entropyBinary entropy functionFOS: MathematicsEntropy (information theory)Statistical physicsDual functionAxiomMathematicsdifferential and relative entropy/extropy Kullback- Leibler divergence Bregman divergence duality proper scoring rules Gini index of heterogeneity repeat rate.Settore ING-INF/05 - Sistemi Di Elaborazione Delle InformazioniDifferential and relative entropy/extropyInformation Theory (cs.IT)Probability (math.PR)repeat ratePhysics - Data Analysis Statistics and ProbabilitydualityStatistics Probability and UncertaintySettore SECS-S/01 - StatisticaMathematics - ProbabilityData Analysis Statistics and Probability (physics.data-an)Statistical Science
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Growth of immobilized DNA by polymerase: bridging nanoelectrodes with individual dsDNA molecules.

2011

We present a method for controlled connection of gold electrodes with dsDNA molecules (locally on a chip) by utilizing polymerase to elongate single-stranded DNA primers attached to the electrodes. Thiol-modified oligonucleotides are directed and immobilized to nanoscale electrodes by means of dielectrophoretic trapping, and extended in a procedure mimicking PCR, finally forming a complete dsDNA molecule bridging the gap between the electrodes. The technique opens up opportunities for building from the bottom-up, for detection and sensing applications, and also for molecular electronics.

Bridging (networking)Sensing applicationsFOS: Physical sciencesNanotechnology02 engineering and technologyDNA-Directed DNA PolymeraseCondensed Matter - Soft Condensed Matter03 medical and health sciencesMoleculeNanotechnologyGeneral Materials SciencePhysics - Biological PhysicsElectrodesPolymerase030304 developmental biologyDNA PrimersFluorescent Dyes0303 health sciencesbiologyImmobilized DNAta114OligonucleotideChemistryta1182Molecular electronicsDNA021001 nanoscience & nanotechnologyCondensed Matter - Other Condensed MatterBiological Physics (physics.bio-ph)Electrodebiology.proteinSoft Condensed Matter (cond-mat.soft)Gold0210 nano-technologyNucleic Acid Amplification TechniquesOther Condensed Matter (cond-mat.other)Nanoscale
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Spectroscopic Observations of the Delta Scorpii Binary during Its Recent Periastron Passage

2001

The bright star delta Sco has been considered a typical B0-type object for many years. Spectra of the star published prior to 1990 showed no evidence of emission, but only of short-term line profile variations attributed to nonradial pulsations. Speckle interferometric observations show that delta Sco is a binary system with a highly-eccentric orbit and a period of 10.6 years. Weak emission in the H-alpha line was detected in its spectrum for the first time during a periastron passage in 1990. Shortly before the next periastron passage in the summer of 2000, the binary entered a strong H-alpha emission and enhanced mass loss phase. We monitored the spectroscopic development of the Be outbur…

Bright starAstrophysics::High Energy Astrophysical PhenomenaBinary numberFOS: Physical sciencesOrbital eccentricityAstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA01 natural sciencesSpectral lineSpectroscopic Technich0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsBinary systemSpectroscopy010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsLine (formation)Physics010308 nuclear & particles physicsBinariesAstrophysics (astro-ph)Astronomy and Astrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Emission-line ; Binaries ; Sco ; Spectroscopic TechnichOrbitScoSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaEmission-line:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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ARES I: WASP-76 b, A Tale of Two HST Spectra

2020

We analyse the transmission and emission spectra of the ultra-hot Jupiter WASP-76b, observed with the G141 grism of the Hubble Space Telescope's Wide Field Camera 3 (WFC3). We reduce and fit the raw data for each observation using the open-source software Iraclis before performing a fully Bayesian retrieval using the publicly available analysis suite TauRex 3. Previous studies of the WFC3 transmission spectra of WASP-76 b found hints of titanium oxide (TiO) and vanadium oxide (VO) or non-grey clouds. Accounting for a fainter stellar companion to WASP-76, we reanalyse this data and show that removing the effects of this background star changes the slope of the spectrum, resulting in these vi…

Brightness010504 meteorology & atmospheric sciencesExoplanet atmospheres; Exoplanet atmospheric composition; Hubble Space Telescope; Astrophysics - Earth and Planetary AstrophysicsFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAstronomy & AstrophysicsExoplanet atmospheres; Exoplanet atmospheric composition; Hubble Space Telescope01 natural sciencesSpectral lineAtmosphereJupiterHAT-P-7B0103 physical sciencesHubble Space TelescopeAstrophysics::Solar and Stellar AstrophysicsEmission spectrumMOLECULAR LINE LISTS010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesHOTPhysicsEarth and Planetary Astrophysics (astro-ph.EP)Science & TechnologyAstronomy and AstrophysicsATMOSPHEREGIANT EXOPLANETGrismRESOLUTIONTransmission (telecommunications)Exoplanet atmospheric composition13. Climate actionSpace and Planetary Science[SDU]Sciences of the Universe [physics]Physical SciencesINFERENCEAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Wide Field Camera 3STARSExoplanet atmospheresAstrophysics - Earth and Planetary Astrophysics
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First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole

2019

We present the first Event Horizon Telescope (EHT) images of M87, using observations from April 2017 at 1.3 mm wavelength. These images show a prominent ring with a diameter of ~40 μas, consistent with the size and shape of the lensed photon orbit encircling the "shadow" of a supermassive black hole. The ring is persistent across four observing nights and shows enhanced brightness in the south. To assess the reliability of these results, we implemented a two-stage imaging procedure. In the first stage, four teams, each blind to the others' work, produced images of M87 using both an established method (CLEAN) and a newer technique (regularized maximum likelihood). This stage allowed us to av…

Brightness010504 meteorology & atmospheric sciencesgalaxies: jetAstronomyblack hole physicsFOS: Physical sciencesgalaxies: individualtechniques: image processingAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)galaxies: individual: M8701 natural sciencesSynthetic dataGeneral Relativity and Quantum Cosmologygalaxies: individual (M87)0103 physical sciencesimage processing [Techniques]010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)0105 earth and related environmental sciencesEvent Horizon TelescopePhysicsGround truthSupermassive black holetechniques: high angular resolutionAstronomy and AstrophysicsBlack hole physicsgalaxies: jetsindividual (M87) [Galaxies]Astrophysics - Astrophysics of Galaxiesblack hole physic3. Good healthOrbitInterferometryhigh angular resolution [Techniques]Space and Planetary Sciencetechniques: interferometricAstrophysics of Galaxies (astro-ph.GA)interferometric [Techniques]jets [Galaxies]Deconvolution[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Instrumentation and Methods for Astrophysics
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The Second Flight of the Sunrise Balloon-borne Solar Observatory: Overview of Instrument Updates, the Flight, the Data, and First Results

2017

S. K. Solanki et. al.

Brightness010504 meteorology & atmospheric sciencesphotosphere [Sun]PolarimetryFOS: Physical scienceschromosphere [Sun]Sun: faculae plagesAstrophysicspolarimetric [Techniques]01 natural scienceslaw.inventionTelescopelaw0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsSunrisefaculae plages [Sun]Sun: magnetic fields010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysicsPhotosphereSolar observatorySunspotsSun: chromosphereTechniques: polarimetricSun: photosphereAstronomy and AstrophysicsPolarimeterAstrophysics - Solar and Stellar Astrophysicsmagnetic fields [Sun]Space and Planetary ScienceData reductionThe Astrophysical Journal Supplement Series
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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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