Search results for "004"

showing 10 items of 187 documents

Zvaigžņotā Debess: 2004/05, Ziema

2004

Contents: Ņ.Ozoliņa. Earthquakes in Latvia ; I.Daube. Space Craft “Ranger-7” ; M. Gailis. Moon Investigation in Riga ; J.Tambergs. Problems of Dialogue between Quantum Mechanics and Theology (concluded) ; Z Alksne, A.Alksnis. Ultra-Cool Dwarf Pair Weighed ; A.Balklavs. Successful Hunt of Protostars ; A.Balklavs. Silhouette of a Black Hole ; A.Balklavs. A Distant Giant Quasar ; A.Balklavs. Cosmic Objects in Captivating Photos – 3 ; J.Freimanis. Extragalactic Planetary Nebulae ; J.Jaunbergs. Cassini Enters the Saturnian System ; D.Krieviņš. Space Launchers of Early XXI Century. The Commonwealth of Independent States (CIS) ; J.Bārzdiņš. Professor Rusins-Martins Freivalds on the Path of Science…

Novembra kāvi Baltijas debesīsGalēji auksto punduru sistēma 2MASSW J0746425+2000321Herbiga-Haro objekti HH-30 HH-34 HH-47Krustvārdu mīklaLīgatnes meteorīts – hipotēzeProtozvaigznesPlanetārie miglāji – NGC 2392 (Eskimosa miglājs) NGC 6369 (Spociņa miglājs)Starptautiskā komandu olimpiāde “Baltijas ceļš – 2003” – uzdevumu atrisinājumiRisina lasītājsNASA Genesis – Saules vēja paraugiLU profesors Rūsiņš-Mārtiņš FreivaldsZemestrīces LatvijāBlumbaha spoguļteleskops BSTPirmās galaktikasCassini misija Saturna sistēmāJakobs Juliuss ZeibotsJupitera pavadoņa Jo putekļiRīgas topogrāfiskā uzmērīšanaSavādnieki eksaktajās zinātnēs – Dž.Maksvels O.Sevisaids H.Hercs V.Pauli V.Heizenbergs B.Mandelbrots A.Vītols J.Vītols G.Šipovs A.AkimovsMeteorītu panspermijaPlanetārie miglāji N52 N66 N192 SMP93 Lielajā Magelāna MākonīVenēras un Merkura aizklāšanāsKosmiskie transportlīdzekļi – NVSAstronomiskās parādības - 2005Melnais caurums – siluetsKalenaisa – “Hebridu Stounhendža”Planētu redzamības kompleksā diagramma 2005Zvaigžņu lietus novembrīESA Smart-1Astronomiskās parādības - 2004Kvantu mehānika un teoloģijaMilzu kvazārs J1432+158Londonas universitātes Berkbeka koledža
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Search for dark matter from the Galactic halo with the IceCube neutrino telescope

2011

Self-annihilating or decaying dark matter in the Galactic halo might produce high energy neutrinos detectable with neutrino telescopes. We have conducted a search for such a signal using 276 days of data from the IceCube 22-string configuration detector acquired during 2007 and 2008. The effect of halo model choice in the extracted limit is reduced by performing a search that considers the outer halo region and not the Galactic Center. We constrain any large-scale neutrino anisotropy and are able to set a limit on the dark matter self-annihilation cross section of ⟨σAv⟩≃10-22 cm3 s-1 for weakly interacting massive particle masses above 1 TeV, assuming a monochromatic neutrino line spectrum.

Nuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaDark matterAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesIceCubeGalactic halo0103 physical sciencesddc:530010306 general physicsAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsGamma-Ray EmissionHot dark matterAstronomyCosmic-Rays004Dark matter haloParticlesNeutrino detectorAnisotropyHigh Energy Physics::ExperimentHaloDwarf Spheroidal GalaxiesNeutrinoNeutrino astronomyinfo:eu-repo/classification/ddc/004
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Constraints on the extremely-high energy cosmic neutrino flux with the IceCube 2008-2009 data

2011

We report on a search for extremely-high energy neutrinos with energies greater than $10^6$ GeV using the data taken with the IceCube detector at the South Pole. The data was collected between April 2008 and May 2009 with the half completed IceCube array. The absence of signal candidate events in the sample of 333.5 days of livetime significantly improves model independent limit from previous searches and allows to place a limit on the diffuse flux of cosmic neutrinos with an $E^{-2}$ spectrum in the energy range $2.0 \times 10^{6}$ $-$ $6.3 \times 10^{9}$ GeV to a level of $E^2 \phi \leq 3.6 \times 10^{-8}$ ${\rm GeV cm^{-2} sec^{-1}sr^{-1}}$.

Nuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaFluxFOS: Physical sciencesCosmic rayRaysAstrophysicsParticle detectorHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Spectrumddc:530Instrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsSPECTRUMCOSMIC cancer databaseRAYS004Massless particleNeutrino detectorPhysics and AstronomyNeutrinoAstrophysics - Instrumentation and Methods for Astrophysicsinfo:eu-repo/classification/ddc/004Astrophysics - Cosmology and Nongalactic AstrophysicsLepton
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Direktīvas 2004/35/EK ieviešanas problēmas Latvijā: fizisko personu un operatora atbildības praktiskie aspekti un būtiskuma slieksnis

2019

Ņemot vērā vides atbildības korektas piemērošanas nozīmi mūsdienu situācijā, darba mērķis ir izvērtēt Direktīvas 2004/35/EK ieviešanas problemātiku Latvijā saistībā ar atbildības subjektu un būtiskuma slieksni. Tādējādi darba uzdevums ir sākotnēji izpētīt Direktīvas 2004/35/EK izpratni Latvijas tiesību sistēmā, analizējot tās materiāltiesisko, personu un laika tvēruma robežas. Tālākajā darba gaitā tiek aplūkoti ar direktīvu ieviestie jauninājumi Latvijas vides tiesību jomā salīdzinājumā ar iepriekš pastāvošo regulējumu. Darba praktiskajā daļā tiek turpmāk izvērsta operatora tiesiskā regulējuma attiecināšana uz fizisku personu, kā arī būtiskuma sliekšņa problemātika. Secināms, ka Latvija dir…

OperatorsBūtiskuma slieksnisDirektīva 2004/35/EKAtbildība par videi nodarīto kaitējumuJuridiskā zinātneFiziska persona kas neveic profesionālu darbību
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Ovide et les barbares tomitains

2016

Ovide 0043 av J-C-0017[SHS] Humanities and Social Sciencesbarbares
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Parallel and scalable short-read alignment on multi-core clusters using UPC++

2016

[Abstract]: The growth of next-generation sequencing (NGS) datasets poses a challenge to the alignment of reads to reference genomes in terms of alignment quality and execution speed. Some available aligners have been shown to obtain high quality mappings at the expense of long execution times. Finding fast yet accurate software solutions is of high importance to research, since availability and size of NGS datasets continue to increase. In this work we present an efficient parallelization approach for NGS short-read alignment on multi-core clusters. Our approach takes advantage of a distributed shared memory programming model based on the new UPC++ language. Experimental results using the …

Parallel computingInternetGenome HumanBioinformaticsPGASShort read alignmentlcsh:RComputational BiologyHigh-Throughput Nucleotide SequencingReproducibility of Resultslcsh:Medicine004 InformatikHumansProgramming Languageslcsh:QHigh performance computinglcsh:ScienceSequence AlignmentAlgorithms004 Data processingResearch Article
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Nuclear actin aggregation is a hallmark of anti-synthetase syndrome-induced dysimmune myopathy

2015

Objective: To analyze antisynthetase syndrome–associated myositis by modern myopathologic methods and to define its place in the spectrum of idiopathic inflammatory myopathies (IIMs). Methods: Skeletal muscle biopsies from antisynthetase syndrome–associated myositis and other IIMs from different institutions worldwide were analyzed by histopathology, quantitative PCR, and electron microscopy. Results: Myonuclear actin filament inclusions were identified as a unique morphologic hallmark of antisynthetase syndrome–associated myositis. Nuclear actin inclusions were never found in dermatomyositis, polymyositis, sporadic inclusion body myositis, autoimmune necrotizing myopathy associated with si…

Pathologymedicine.medical_specialtyBiopsyIntranuclear Inclusion Bodies10208 Institute of Neuropathology610 Medicine & healthAntisynthetase syndromeBiologyPolymyositisSensitivity and SpecificityNecrosisPerimysialmedicineHumansMyopathyMuscle SkeletalMyositisMyositisDermatomyositisActin cytoskeletonmedicine.diseaseAutoimmune necrotizing myopathyActins10040 Clinic for NeurologyActin Cytoskeleton2728 Neurology (clinical)Immunology570 Life sciences; biologyNeurology (clinical)medicine.symptom
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Filtered circular fingerprints improve either prediction or runtime performance while retaining interpretability

2016

Physical and Theoretical ChemistryLibrary and Information Sciences004 InformatikComputer Graphics and Computer-Aided Design004 Data processingComputer Science ApplicationsJournal of Cheminformatics
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FlexibleSUSY -- A spectrum generator generator for supersymmetric models

2014

We introduce FlexibleSUSY, a Mathematica and C++ package, which generates a fast, precise C++ spectrum generator for any SUSY model specified by the user. The generated code is designed with both speed and modularity in mind, making it easy to adapt and extend with new features. The model is specified by supplying the superpotential, gauge structure and particle content in a SARAH model file; specific boundary conditions e.g. at the GUT, weak or intermediate scales are defined in a separate FlexibleSUSY model file. From these model files, FlexibleSUSY generates C++ code for self-energies, tadpole corrections, renormalization group equations (RGEs) and electroweak symmetry breaking (EWSB) co…

PhysicsParticle physicsGenerator (computer programming)SuperpotentialElectroweak interactionHigh Energy Physics::PhenomenologyGeneral Physics and AstronomyFOS: Physical sciencesSupersymmetryTopologyHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Hardware and ArchitectureHiggs bosonSymmetry breakingBoundary value problemddc:004Minimal Supersymmetric Standard Model
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Recurrence of the blue wing enhancements in the high ionization lines of SDSS 1004+4112 A

2006

We present integral field spectroscopic observations of the quadruple-lensed QSO SDSS 1004+4112 taken with the fiber system INTEGRAL at the William Herschel Telescope on 2004 January 19. In 2003 May, a blueward enhancement in the high-ionization lines of SDSS 1004+4112A was detected, and then it faded. Our observations are the first to note a second event of similar characteristics less than 1 year after. Although initially attributed to microlensing, the resemblance among the spectra of both events and the absence of microlensing-induced changes in the continuum of component A are puzzling. The lack of a convincing explanation under the microlensing or intrinsic variability hypotheses make…

PhysicsQuasars: emission linesAstrophysics (astro-ph)Gravitational lensingFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsGravitational microlensingAstrophysicsSpectral lineemission lines [Quasars]Space and Planetary Scienceindividual (SDSS 1004-4112) [Quasars]IonizationQuasars: individual (SDSS 1004-4112)William Herschel Telescope
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