Search results for "methods [Gene Expression Profiling]"

showing 10 items of 838 documents

Nonlinear dynamics of a two-photon Fabry–Pérot laser

2000

Abstract The steady-state emission, stability and temporal dynamics of a single-mode two-photon laser with a Fabry–Perot cavity is investigated and compared with that of a ring-cavity laser. It is found that the Fabry–Perot cavity makes the laser less efficient than the ring cavity because of spatial hole burning, but the domain of stability is larger for the Fabry–Perot laser. The intensity and phase dynamics are numerically investigated and distinctive features are found in the phase dynamics as compared with one-photon lasers.

Distributed feedback laserMaterials sciencePhysics::Instrumentation and Detectorsbusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsPhysics::OpticsInjection seederLaserAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsIntensity (physics)law.inventionNonlinear systemOpticsTwo-photon excitation microscopylawPhysics::Atomic PhysicsLaser power scalingElectrical and Electronic EngineeringPhysical and Theoretical ChemistrybusinessFabry–Pérot interferometerOptics Communications
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Observational Approach and Perspective

1983

Well you did not cover more than half of my planned talk! (laughter). Let me comment on interferometric techniques, in particular speckle imaging which you mentioned. Doing speckle imaging with the largest telescopes now available will not give you better than the theoretical resolving power of the telescope. With a 4m telescope that is about 30 marc sec in the visible. That happens to be the radius of the supergiant Betelguese. So you are not going to achieve much with speckle imaging on these stars. One technique which has not been adequately exploited is that of lunar occultation which can give much better angular resolution than speckle, of the order of 2-3 marc sec. By using suitably c…

Dwarf starComputer scienceAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyOccultationlaw.inventionTelescopeSpeckle patternInterferometryStarslawAstrophysics::Solar and Stellar AstrophysicsAngular resolutionAstrophysics::Earth and Planetary AstrophysicsSpeckle imagingAstrophysics::Galaxy Astrophysics
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Massive evaluation and analysis of Poincar�� recurrences on grids of initial data: a tool to map chaotic diffusion

2020

We present a novel numerical method aimed to characterize global behaviour, in particular chaotic diffusion, in dynamical systems. It is based on an analysis of the Poincar\'e recurrence statistics on massive grids of initial data or values of parameters. We concentrate on Hamiltonian systems, featuring the method separately for the cases of bounded and non-bounded phase spaces. The embodiments of the method in each of the cases are specific. We compare the performances of the proposed Poincar\'e recurrence method (PRM) and the custom Lyapunov exponent (LE) methods and show that they expose the global dynamics almost identically. However, a major advantage of the new method over the known g…

Dynamical systems theoryComputer scienceChaoticGeneral Physics and AstronomyFOS: Physical sciencesLyapunov exponent01 natural sciences010305 fluids & plasmasHamiltonian systemsymbols.namesakeSimple (abstract algebra)0103 physical sciencesApplied mathematicsDiffusion (business)010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)ComputingMilieux_MISCELLANEOUSEarth and Planetary Astrophysics (astro-ph.EP)Numerical analysisNonlinear Sciences - Chaotic DynamicsHardware and ArchitectureBounded functionsymbolsChaotic Dynamics (nlin.CD)Astrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Earth and Planetary Astrophysics
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IPHAS-selected classical Be stars

2016

We present a semi-automatic procedure to obtain fundamental physical parameters and distances of classical Be (CBe) stars, based on the Barbier-Chalonge-Divan (BCD) spectrophotometric system. Our aim is to apply this procedure to a large sample of CBe stars detected by the IPHAS photometric survey, to determine their fundamental physical parameters and to explore their suitability as galactic structure tracers. In this paper we describe the methodology used and the validation of the procedure by comparing our results with those obtained from different independent astrophysical techniques for subsamples of stars in common with other studies. We also present a test case study of the galactic …

Early type starsAstrophysics and AstronomyPhysicsAstrophysics::Instrumentation and Methods for AstrophysicsStellar distanceAstrophysics::Cosmology and Extragalactic AstrophysicsComputer Science::Digital Librariesobservational astronomyStellar AstronomyEarly-type starsBe starsAstrophysics::Solar and Stellar AstrophysicsNatural SciencesAstrophysics::Galaxy Astrophysics
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Be stars in the exofield of CoRoT. II.

2018

The class of Be stars are the epitome of rapid rotators in the main sequence. These stars are privileged candidates for studying the incidence of rotation on the stellar internal structure and on non-radial pulsations. Pulsations are considered possible mechanisms to trigger mass-ejection phenomena required to build up the circumstellar disks of Be stars. Time series analyses of the light curves of 15 faint Be stars observed with the CoRoT satellite were performed to obtain the distribution of non-radial pulsation (NRP) frequencies in their power spectra at epochs with and without light outbursts and to discriminate pulsations from rotation-related photometric variations. Standard Fourier t…

Early type starsAstrophysics and AstronomyStellar AstronomyEarly-type starsBe starsPhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsNatural SciencesAstrophysics::Galaxy Astrophysics
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Walking on exoplanets: Is Star Wars right?

2016

As the number of detected extrasolar planets increases, exoplanet databases become a valuable resource, confirming some details about planetary formation, but also challenging our theories with new unexpected properties.

Earth and Planetary Astrophysics (astro-ph.EP)010504 meteorology & atmospheric sciencesExtraterrestrial EnvironmentComputer scienceMotion PicturesAstrophysics::Instrumentation and Methods for AstrophysicsPlanetsFOS: Physical sciencesWalkingStar (graph theory)01 natural sciencesAgricultural and Biological Sciences (miscellaneous)ExoplanetAstrobiologySpace and Planetary Science0103 physical sciencesExobiologyAstrophysics::Earth and Planetary Astrophysics010303 astronomy & astrophysics0105 earth and related environmental sciencesGravitationAstrophysics - Earth and Planetary Astrophysics
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Hiding in plain sight: observing planet-starspot crossings with the James Webb Space Telescope

2021

Transiting exoplanets orbiting active stars frequently occult starspots and faculae on the visible stellar disc. Such occultations are often rejected from spectrophotometric transits, as it is assumed they do not contain relevant information for the study of exoplanet atmopsheres. However, they can provide useful constraints to retrieve the temperature of active features and their effect on transmission spectra. We analyse the capabilities of the James Webb Space Telescope in the determination of the spectra of occulted starspots, despite its lack of optical wavelength instruments on board. Focusing on K and M spectral types, we simulate starspots with different temperatures and in differen…

Earth and Planetary Astrophysics (astro-ph.EP)PhysicsJames Webb Space TelescopeStarspotAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomyAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsStellar classificationExoplanetStarsWavelengthAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePlanetAstrophysics::Solar and Stellar AstrophysicsPrismAstrophysics::Earth and Planetary AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsAstrophysics - Earth and Planetary Astrophysics
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A network of precision gravimeters as a detector of matter with feeble nongravitational coupling

2019

Hidden matter that interacts only gravitationally would oscillate at characteristic frequencies when trapped inside of Earth. For small oscillations near the center of the Earth, these frequencies are around 300 $\mu$Hz. Additionally, signatures at higher harmonics would appear because of the non-uniformity of Earth's density. In this work, we use data from a global network of gravimeters of the International Geodynamics and Earth Tide Service (IGETS) to look for these hypothetical trapped objects. We find no evidence for such objects with masses on the order of 10$^{14}$ kg or greater with an oscillation amplitude of 0.1 $r_e$. It may be possible to improve the sensitivity of the search by…

Earth and Planetary Astrophysics (astro-ph.EP)Physics::Space PhysicsFOS: Physical sciencesAstrophysics::Earth and Planetary AstrophysicsAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics - Earth and Planetary AstrophysicsPhysics::Geophysics
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Model Based Monte Carlo Pricing of Energy and Temperature Quanto Options

2010

Weather derivatives have become very popular tools in weather risk management in recent years. One of the elements supporting their diffusion has been the increase in volatility observed on many energy markets. Among the several available contracts, Quanto options are now becoming very popular for a simple reason: they take into account the strong correlation between energy consumption and certain weather conditions, so enabling price and weather risk to be controlled at the same time. These products are more efficient and, in many cases, significantly cheaper than simpler plain vanilla options. Unfortunately, the specific features of energy and weather time series do not enable the use of …

Economics and EconometricsComputer scienceMonte Carlo methodTemperature levelBivariate analysisEnergy priceDynamic modelMicroeconomicsEconomicsEconometricsweather derivatives Quanto options pricing derivative pricing model simulation and forecast.Time seriesQuanto options; Temperature level; Energy price; Dynamic modelMonte Carlo methods for option pricingjel:C53Quanto optionsjel:C51Energy consumptionVariance (accounting)jel:C32Quantojel:G13weather derivatives; Quanto options pricing; derivative pricing; model simulation; forecastjel:L94jel:G17General Energyjel:Q54Binomial options pricing modelVolatility (finance)Futures contract
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Externalities and article citations: experience of a national public health journal (Gaceta Sanitaria)

2016

Purpose: The purpose of the study was to analyze the determinants of citations such as publication year, article type, article topic, article selected for a press release, number of articles previously published by the corresponding author, and publication language in a Spanish journal of public health. Methods: Observational study including all articles published in Gaceta Sanitaria during 2007-2011. We retrieved the number of citations from the ISI Web of Knowledge database in June 2013 and also information on other variables such as number of articles published by the corresponding author in the previous 5 years (searched through PubMed), selection for a press release, publication langua…

Editorial policiesmedicine.medical_specialtyOperations researchEpidemiologybusiness.industryPublic healthLibrary science030204 cardiovascular system & hematologyBibliometricsMethods observational03 medical and health sciences0302 clinical medicineWeb of knowledgeBibliometricsPress releaseMedicina Preventiva y Salud PúblicaMedicine030212 general & internal medicineJournal of Public HealthJournal Impact FactorbusinessExternalityAnnals of Epidemiology
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