Search results for "Curve"

showing 10 items of 1693 documents

Search for neutrino emission from gamma-ray flaring blazars with the ANTARES telescope

2012

The ANTARES telescope observes a full hemisphere of the sky all the time with a duty cycle close to 100%. This makes it well suited for an extensive observation of neutrinos produced in astrophysical transient sources. In the surrounding medium of blazars, i.e. active galactic nuclei with their jets pointing almost directly towards the observer, neutrinos may be produced together with gamma-rays by hadronic interactions, so a strong correlation between neutrinos and gamma-rays emissions is expected. The time variability information of the studied source can be obtained by the gamma-ray light curves measured by the LAT instrument on-board the Fermi satellite. If the expected neutrino flux ob…

ASTROPHYSICSAstrofísicaAstrophysicsNeutrino Astronomy01 natural sciences7. Clean energyLARGE-AREA TELESCOPElaw.inventionlawWATERInstrumentation010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Time-dependent searchCATALOGLIGHTNeutrino astronomyFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaACTIVE GALACTIC NUCLEINuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Active galactic nucleus[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Point sourceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsfermi lat transient sources; neutrino astronomy; time-dependent search; antares; blazarsTelescopeMUONS0103 physical sciencesANTARES; Neutrino Astronomy; Fermi LAT transient sourcesBlazarANTARES010308 nuclear & particles physicsAstronomyAstronomy and AstrophysicsFermi LAT transient sourcesLight curveNeutrino astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]MODEL13. Climate actionFISICA APLICADA:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]Neutrino astronomy[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]BlazarsFermi Gamma-ray Space Telescope
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H-He collision-induced satellite in the Lyman alpha profile of DBA white dwarf stars

2020

The spectra of helium-dominated white dwarf stars with hydrogen in their atmosphere present a distinctive broad feature centered around 1160~\AA\/ in the blue wing of the Lyman-$\alpha$ line. It is extremely apparent in WD 1425+540 recently observed with HST COS. With new theoretical line profiles based on ab initio atomic interaction potentials we show that this feature is a signature of a collision-induced satellite due to an asymptotically forbidden transition. This quasi-molecular spectral satellite is crucial to understanding the asymmetrical shape of Lyman-$\alpha$ seen in this and other white dwarf spectra. Our previous work predicting this absorption feature was limited by molecular…

ATOMIC DATALINE: PROFILEAb initiochemistry.chemical_elementBASIS-SETLINEEXCITED-STATEAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSpectral linePhysics - Atomic PhysicsWHITE DWARF0103 physical sciencesRadiative transferABSORPTIONAstrophysics::Solar and Stellar AstrophysicsAB-INITIO CALCULATIONPhysics::Atomic PhysicsELECTRONIC-TRANSITION MOMENT010306 general physicsSTARS: ATMOSPHERE010303 astronomy & astrophysicsHeliumLine (formation)POTENTIAL-ENERGY CURVEPhysics[PHYS]Physics [physics]BALMER-ALPHAWhite dwarfAstronomy and AstrophysicsMOLECULAR DATAPotential energyDipolechemistryAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceATOMIC PROCESSSHAPE[PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]Atomic physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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An Arakelov inequality in characteristic p and upper bound of p-rank zero locus

2008

In this paper we show an Arakelov inequality for semi-stable families of algebraic curves of genus $g\geq 1$ over characteristic $p$ with nontrivial Kodaira-Spencer maps. We apply this inequality to obtain an upper bound of the number of algebraic curves of $p-$rank zero in a semi-stable family over characteristic $p$ with nontrivial Kodaira-Spencer map in terms of the genus of a general closed fiber, the genus of the base curve and the number of singular fibres. An extension of the above results to smooth families of Abelian varieties over $k$ with $W_2$-lifting assumption is also included.

Abelian varietyAlgebra and Number TheoryStable curveCombinatoricsAlgebraic cycleMathematics - Algebraic GeometryMathematics::Algebraic Geometry14D05 (Primary) 14G25 14H10 (Secondary)Algebraic surfaceFOS: MathematicsGenus fieldAlgebraic curveAbelian groupAlgebraic Geometry (math.AG)Singular point of an algebraic varietyMathematicsJournal of Number Theory
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Automorphisms of hyperelliptic GAG-codes

2009

Abstract We determine the n –automorphism group of generalized algebraic-geometry codes associated with rational, elliptic and hyperelliptic function fields. Such group is, up to isomorphism, a subgroup of the automorphism group of the underlying function field.

Abelian varietyDiscrete mathematicsautomorphismsGroup (mathematics)Applied Mathematicsgeneralized algebraic geometry codes.Outer automorphism groupReductive groupAutomorphismTheoretical Computer ScienceCombinatoricsMathematics::Group Theorygeometric Goppa codeAlgebraic groupDiscrete Mathematics and Combinatoricsalgebraic function fieldsSettore MAT/03 - GeometriaIsomorphismfinite fieldsGeometric Goppa codesfinite fieldalgebraic function fieldHyperelliptic curvegeneralized algebraic-geometry codesMathematicsDiscrete Mathematics
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Chapter 3 patterns and thresholds of runoff generation and sediment transport on some Mediterranean hillslopes

2005

Abstract Runoff and sediment transport data obtained from hillslopes in two limestone areas in southeast Spain are analysed in order to define spatial and temporal thresholds for sediment movement at the patch scale under Mediterranean semiarid and subhumid climatological conditions. The data discussed in this paper include a 7-year series of runoff and sediment collection in open Gerlach plots. The 136 events are analysed in relation to characteristics of rainfall, soil and soil surface components. In both cases slopes behave as a patchwork of runoff and runon areas and the size of the runoff or runon patches being dependent on the climatological conditions. These control the hydrological …

Abiotic componentMediterranean climateHydrologyStreamflowEnvironmental scienceWEPPRunoff curve numberSaturation (chemistry)Surface runoffSediment transport
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The large trans-Neptunian object 2002 TC 302 from combined stellar occultation, photometry, and astrometry data

2020

All authors: Ortiz, J. L.; Santos-Sanz, P.; Sicardy, B.; Benedetti-Rossi, G.; Duffard, R.; Morales, N.; Braga-Ribas, F.; Fernández-Valenzuela, E.; Nascimbeni, V.; Nardiello, D.; Carbognani, A.; Buzzi, L.; Aletti, A.; Bacci, P.; Maestripieri, M.; Mazzei, L.; Mikuz, H.; Skvarc, J.; Ciabattari, F.; Lavalade, F. Scarfi, G.; Mari, J. M.; Conjat, M.; Sposetti, S.; Bachini, M.; Succi, G.; Mancini, F.; Alighieri, M.; Dal Canto, E.; Masucci, M.; Vara-Lubiano, M.; Gutiérrez, P. J.; Desmars, J.; Lecacheux, J.; Vieira-Martins, R.; Camargo, J. I. B.; Assafin, M.; Colas, F.; Beisker, W.; Behrend, R.; Mueller, T. G.; Meza, E.; Gomes-Junior, A. R.; Roques, F.; Vachier, F.; Mottola, S.; Hellmich, S.; Campo …

Absolute magnitude010504 meteorology & atmospheric sciencesFOS: Physical sciencesAstrophysicsKuiper belt objects: individual: 2002 TC30201 natural sciencesOccultationlaw.inventionTelescopePhotometry (optics)lawGeometric albedoFísica Aplicada0103 physical sciencesTrans-Neptunian object010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciencesPhysics[PHYS]Physics [physics]Earth and Planetary Astrophysics (astro-ph.EP)photometric [Techniques]Astronomy and Astrophysicsgeneral [Kuiper belt]Astrometryindividual: 2002 TC302 [Kuiper belt objects]AstrometryAstrometry; Kuiper belt objects: individual: 2002 TC302; Kuiper belt: general; Occultations; Techniques: photometricLight curveSpace and Planetary Science[SDU]Sciences of the Universe [physics]Kuiper belt: generalOccultations[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Techniques: photometricAstrophysics - Earth and Planetary AstrophysicsAstronomy & Astrophysics
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Creatinine determination in urine samples by batchwise kinetic procedure and flow injection analysis using the Jaffé reaction: chemometric study

2001

The classical Jaffé reaction for the determination of creatinine in urine samples is tested. A comparative study of the main analytical characteristics focussed to minimize the bias error and improve the precision, for the batchwise and flow injection (FI) methods is realized. Also, the effect of the albumin concentration in the determination of creatinine has been studied. Different analytical signals were studied. Absorbance increments at different times permit to estimate the creatinine concentration free from bias error in urine by the batchwise method using the calibration graph obtained with creatinine standards and no measurement of the blank solution is needed. The lineal interval w…

AbsorbanceFlow injection analysisCreatininechemistry.chemical_compoundChromatographychemistryCalibration curveStandard additionCalibrationAnalytical chemistryUrineQuantitative analysis (chemistry)Analytical ChemistryTalanta
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Estimation of ADME Properties in Drug Discovery: Predicting Caco-2 Cell Permeability Using Atom-Based Stochastic and Non-stochastic Linear Indices

2007

The in vitro determination of the permeability through cultured Caco-2 cells is the most often-used in vitro model for drug absorption. In this report, we use the largest data set of measured P(Caco-2), consisting of 157 structurally diverse compounds. Linear discriminant analysis (LDA) was used to obtain quantitative models that discriminate higher absorption compounds from those with moderate-poorer absorption. The best LDA model has an accuracy of 90.58% and 84.21% for training and test set. The percentage of good correlation, in the virtual screening of 241 drugs with the reported values of the percentage of human intestinal absorption (HIA), was greater than 81%. In addition, multiple …

Absorption (pharmacology)Stochastic ProcessesVirtual screeningQuantitative structure–activity relationshipDrug discoveryStereochemistryLinear modelQuantitative Structure-Activity RelationshipPharmaceutical ScienceLinear discriminant analysisPermeabilityData setROC CurveDrug DesignTest setLinear regressionLinear ModelsHumansPharmacokineticsCaco-2 CellsBiological systemADMEMathematicsJournal of Pharmaceutical Sciences
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NuSTAR and NICER reveal IGR J17591-2342 as a new accreting millisecond X-ray pulsar

2018

We report the discovery by the Nuclear Spectroscopic Telescope Array (NuSTAR) and the Neutron Star Interior Composition Explorer (NICER) of the accreting millisecond X-ray pulsar IGR J17591-2342. Coherent X-ray pulsations around 527.4 Hz (1.9 ms) with a clear Doppler modulation were detected. This implies an orbital period of ∼8.8 h and a projected semi-major axis of ∼1.23 lt-s. With the binary mass function, we estimate a minimum companion mass of 0.42 M, obtained assuming a neutron star mass of 1.4[subscript ⊙] and an inclination angle lower than 60°, as suggested by the absence of eclipses or dips in the light curve of the source. The broad-band energy spectrum, obtained by combining NuS…

AccretionAstrophysics::High Energy Astrophysical Phenomenageneral [Pulsars]FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSpectral linelaw.inventionTelescopeX-rays: binariesSettore FIS/05 - Astronomia E AstrofisicaPulsarlow-mass [Stars]lawstars: low-mass0103 physical sciencesStars: low-maAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Neutron Star Interior Composition Explorer010308 nuclear & particles physicsComputer Science::Information Retrievalaccretion disksneutron [Stars]Astronomy and AstrophysicsAstronomy and AstrophysicOrbital periodLight curveX-rays: binarieStars: neutronNeutron starPulsars: generalAccretion diskSpace and Planetary ScienceAccretion disksbinaries [X-rays]Astrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]X-ray pulsar
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A Hard X-Ray View of Scorpius X-1 with INTEGRAL : Nonthermal Emission?

2006

We present here simultaneous INTEGRAL/RXTE observations of Sco X-1, and in particular a study of the hard X-ray emission of the source and its correlation with the position in the Z-track of the X-ray color-color diagram. We find that the hard X-ray (above about 30 keV) emission of Sco X-1 is dominated by a power-law component with a photon index of ~3. The flux in the power-law component slightly decreases when the source moves in the color-color diagram in the sense of increasing inferred mass accretion rate from the horizontal branch to the normal branch/flaring branch vertex. It becomes not significantly detectable in the flaring branch, where its flux has decreased by about an order of…

AccretionPhotonAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysicsAstrophysics01 natural sciencesneutron starsX-ray[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Position (vector)Accretion DisksStars: Neutron0103 physical sciencesX-Rays: StarsAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)DiagramAstronomy and AstrophysicsSense (electronics)Horizontal branchX-Rays: BinariesX-Rays: GeneralSpace and Planetary ScienceVertex (curve)accreting millisecondStars: Individual: Constellation Name: Scorpius X-1Order of magnitudeThe Astrophysical Journal
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