Search results for " nuclei"

showing 10 items of 602 documents

Real-life evaluation of a rapid extraction-free SARS-CoV-2 RT-PCR assay (COVID-19 PCR Fast-L) for the diagnosis of COVID-19.

2021

2019-20 coronavirus outbreakCoronavirus disease 2019 (COVID-19)SARS-CoV-2Severe acute respiratory syndrome coronavirus 2 (SARS-CoV-2)Extraction (chemistry)COVID-19BiologyVirologyPolymerase Chain ReactionSensitivity and SpecificityInfectious DiseasesReal-time polymerase chain reactionLife evaluationVirologyCOVID-19 Nucleic Acid TestingHumansRNA ViralProspective StudiesLetter to the EditorJournal of medical virology
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Non-symmetrized Hyperspherical Harmonics Method for Non-equal Mass Three-Body Systems

2018

The non-symmetrized hyperspherical harmonics method for a three-body system, composed by two particles having equal masses, but different from the mass of the third particle, is reviewed and applied to the $^3$H, $^3$He nuclei and $^3_{\Lambda}$H hyper-nucleus, seen respectively as $nnp$, $ppn$ and $NN\Lambda$ three-body systems. The convergence of the method is first tested in order to estimate its accuracy. Then, the difference of binding energy between $^3$H and $^3$He due to the difference of the proton and the neutron masses is studied using several central spin-independent and spin-dependent potentials. Finally, the $^3_{\Lambda}$H hypernucleus binding energy is calculated using diffe…

3HeProtonMaterials Science (miscellaneous)hypertritonBinding energyBiophysicsGeneral Physics and AstronomyLambda01 natural sciencesthree-body systemstriton0103 physical sciencesNeutronhypersperical harmonics methodPhysical and Theoretical Chemistry010306 general physicsMathematical PhysicsMathematical physicsPhysics010308 nuclear & particles physicslight nucleiOrder (ring theory)Hypernucleuslcsh:QC1-999Harmonicslcsh:PhysicsHypertritonFrontiers in Physics
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Genomic organization and promoter characterization of the gene encoding a putative endoplasmic reticulum chaperone, ERp29

2002

Abstract ERp29 is a soluble protein localized in the endoplasmic reticulum (ER) of eukaryotic cells, which is conserved in all mammalian species. The N-terminal domain of ERp29 displays sequence and structural similarity to the protein disulfide isomerase despite the lack of the characteristic double cysteine motif. Although the exact function of ERp29 is not yet known, it was hypothesized that it may facilitate folding and/or export of secretory proteins in/from the ER. ERp29 is induced by ER stress, i.e. accumulation of unfolded proteins in the ER. To gain an insight into the mechanisms regulating ERp29 expression we have cloned and characterized the rat ERp29 gene and studied in details …

5' Flanking RegionRecombinant Fusion ProteinsMolecular Sequence DataCHO CellsBiologyCell LineMiceCricetinaeSequence Homology Nucleic AcidGene expressionTumor Cells CulturedGeneticsAnimalsHumansRNA MessengerLuciferasesPromoter Regions GeneticProtein disulfide-isomeraseGeneHeat-Shock ProteinsPhylogenyBase SequenceGene Expression ProfilingEndoplasmic reticulumPromoter3T3 CellsDNAExonsSequence Analysis DNAGeneral MedicineMolecular biologyIntronsRatsHousekeeping geneSecretory proteinGenesUnfolded protein responseFemaleTranscription Initiation SiteSequence AlignmentHeLa CellsGene
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Sequence of a sea urchin hsp70 gene and its 5' flanking region.

1990

We report the nucleotide sequence of a 4470-bp fragment derived from a sea urchin genomic clone containing part of a heat-shock protein 70 (Hsp70)-encoding gene. This fragment, named hsp70 gene II, contains 1271 bp of the flanking region and 3299 bp of structural gene sequence interrupted by five introns and encoding the N-terminal 371 amino acids (aa) of the protein. The 5' flanking region contains a putative TATA element, two CCAAT boxes, four heat-shock consensus sequence elements (hse) and one consensus sequence for binding of Sp1. Remarkable homologies were observed for deduced aa sequence and intron-exon organization between hsp70 gene II and rat hsc73 gene.

5' flanking regionMolecular Sequence DataRestriction MappingBiologyExonSequence Homology Nucleic AcidConsensus SequenceGeneticsConsensus sequenceAnimalsAmino Acid SequencePromoter Regions GeneticGenePeptide sequenceHeat-Shock ProteinsGeneticsBase SequenceStructural geneNucleic acid sequenceGeneral MedicineExonsMolecular biologyIntronsGenesRegulatory sequenceSea UrchinsGene
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Isomeric state of $^{80}$Y and its role in the astrophysical rp-process

2001

5 pages, 7 figures.-- PACS nrs: 21.10.Tg; 23.20.Nx; 27.50.+e.

59 ≤ A ≤ 89 [[PACS] Properties of specific nuclei listed by mass ranges]PhysicsNuclear and High Energy Physics[PACS] Properties of specific nuclei listed by mass ranges: 59 ≤ A ≤ 89Proton[PHYS.NEXP] Physics [physics]/Nuclear Experiment [nucl-ex]010308 nuclear & particles physicsHadronElectron[PACS] Internal conversion and extranuclear effects (including Auger electrons and internal bremsstrahlung)rp-processNuclear isomer[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyNuclear physicsExcited state0103 physical sciences[PACS] Lifetimes widthsAtomic physics010306 general physicsInternal conversion coefficientExcitation
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[1,2,3]Triazolo[1,5-a]piridinas y compuestos relacionados : aplicaciones en química supramolecular : actividad biológica

2013

Los heterociclos nitrogenados son moléculas clave dentro de numerosos campos científicos. En concreto, los triazoles han encontrado numerosas aplicaciones en química médica como antifúngicos (fluconazol, posaconazol), antidepresivos (trazodona) o anticancerígenos (triazoloacridonas). En este contexto se decidió sintetizar nuevos derivados de [1,2,3]triazolo[1,5-a]piridinas con el fin de explorar su capacidad de interaccionar con ADN y su actividad leishmanicida y antichagásica. Con este objetivo se ha utilizado la química clásica de las triazolopiridinas (reacción de litiación regioselectiva de este heterociclo, seguida de adición de un electrófilo), para obtener nuevos derivados con estruc…

:QUÍMICA::Química orgánica::Mecanismos de reacción [UNESCO]:QUÍMICA::Química Farmacéutica::Diseño.Síntesis y estudio nuevos fármacos [UNESCO]heterociclos nitrogenadosleishmanicidal agentUNESCO::QUÍMICA::Química Farmacéutica::Diseño.Síntesis y estudio nuevos fármacosquinolinasUNESCO::QUÍMICA::Química orgánica::Mecanismos de reacciónUNESCO::QUÍMICA:QUÍMICA::Química orgánica [UNESCO]antichagasic agentcicloadición 13-dipolarDNA:QUÍMICA [UNESCO]oligocarbonilpiridinaUNESCO::QUÍMICA::Bioquímica::Acidos nucleicosazahelicenos:QUÍMICA::Química orgánica::Compuestos heterocíclicos [UNESCO]:QUÍMICA::Bioquímica::Acidos nucleicos [UNESCO]triazolopiridinasUNESCO::QUÍMICA::Química orgánica::Compuestos heterocíclicostransferencia de hidrógenoUNESCO::QUÍMICA::Química orgánica
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Limit on the diffuse flux of ultrahigh energy tau neutrinos with the surface detector of the Pierre Auger Observatory

2009

Data collected at the Pierre Auger Observatory are used to establish an upper limit on the diffuse flux of tau neutrinos in the cosmic radiation. Earth-skimming ντ may interact in the Earth's crust and produce a τ lepton by means of charged-current interactions. The τ lepton may emerge from the Earth and decay in the atmosphere to produce a nearly horizontal shower with a typical signature, a persistent electromagnetic component even at very large atmospheric depths. The search procedure to select events induced by τ decays against the background of normal showers induced by cosmic rays is described. The method used to compute the exposure for a detector continuously growing with time is de…

ACTIVE GALACTIC NUCLEIASTROPHYSICS[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Nuclear and High Energy PhysicsActive galactic nucleusPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayPROPAGATIONAstrophysics7. Clean energy01 natural sciencesLeptonSpectral lineSettore FIS/04 - Fisica Nucleare e SubnucleareAugerSEARCHTau neutrino0103 physical sciencesTau neutrinoOSCILLATIONS010306 general physicsCiencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)AIR-SHOWERSPierre Auger ObservatoryPhysicsSPECTRUM010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsFísicaultrahigh energy cosmic rays ; tau neutrinos ; Pierre Auger ObservatoryDiffuse fluxPierre Auger ObservatoryPERFORMANCECOSMIC-RAYScosmic radiation13. Climate actionTELESCOPESHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaLeptonPhysical Review D
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Accretion in strong field gravity with eXTP

2019

In this paper we describe the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to accretion flows in the strong field gravity regime around both stellar-mass and supermassive black-holes. eXTP has the unique capability of using advanced 'spectral-timing-polarimetry' techniques to analyze the rapid variations with three orthogonal diagnostics of the flow and its geometry, yielding unprecedented insight into the inner accreting regions, the effects of strong field gravity on the material within them and the powerful outflows which are driven by the accretion process.

ACTIVE GALACTIC NUCLEIAccretionaccretion; black holes physics; X-ray; Physics and Astronomy (all)black holes physicAstronomyAstrophysics::High Energy Astrophysical PhenomenaBlack holes physicsPolarimetryFOS: Physical sciencesBLACK-HOLE SPINGeneral Physics and AstronomyStrong fieldAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesX-rayPhysics and Astronomy (all)ELECTROMAGNETIC EMISSIONSettore FIS/05 - Astronomia e Astrofisicablack holes physicsaccretion0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)XMM-NEWTONPhysicsLENS-THIRRING PRECESSION[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]QUASI-PERIODIC OSCILLATIONS[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]IRON KAccretion (astrophysics)X ray[SDU]Sciences of the Universe [physics]ULTRA-FAST OUTFLOWSAstrophysics::Earth and Planetary AstrophysicsSPECTRAL FEATURESAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]X-RAY BINARIESScience China Physics, Mechanics & Astronomy
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Event Horizon Telescope imaging of the archetypal blazar 3C 279 at an extreme 20 microarcsecond resolution

2020

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.--All authors: Kim, Jae-Young; Krichbaum, Thomas P.; Broderick, Avery E.; Wielgus, Maciek; Blackburn, Lindy; Gómez, José L.; Johnson, Michael D.; Bouman, Katherine L.; Chael, Andrew; Akiyama, Kazunori; Jorstad, Svetlana; Marscher, Alan P.; Issaoun, Sara; Janssen, Michael; Chan, Chi-kwan; Savolainen, Tuomas; Pesce, Dominic W.; Özel, Feryal; Alberdi, Antxon; Alef, Walt…

ACTIVE GALACTIC NUCLEIBrightnessActive galactic nucleusactive [Galaxies]Astrophysics::High Energy Astrophysical PhenomenaAstronomygalaxies: activeAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSubmillimeter ArrayFLOWSSCALE CIRCULAR-POLARIZATION0103 physical sciencesVery-long-baseline interferometryBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsEvent Horizon Telescope[PHYS]Physics [physics]Jet (fluid)010308 nuclear & particles physicsAstronomy and AstrophysicsFLAREgalaxies: jetsindividual: 3C 279 [Galaxies]LONGVARIABILITYgalaxies: individual: 3C 279GAMMA-RAYQUASARS13. Climate actionSpace and Planetary Sciencetechniques: interferometricBrightness temperatureACCRETION DISKSinterferometric [Techniques]jets [Galaxies]RELATIVISTIC JETS[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astronomy & astrophysics
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Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory

2011

The Pierre Auger Collaboration has reported evidence for anisotropy in the distribution of arrival directions of the cosmic rays with energies $E>E_{th}=5.5\times 10^{19}$ eV. These show a correlation with the distribution of nearby extragalactic objects, including an apparent excess around the direction of Centaurus A. If the particles responsible for these excesses at $E>E_{th}$ are heavy nuclei with charge $Z$, the proton component of the sources should lead to excesses in the same regions at energies $E/Z$. We here report the lack of anisotropies in these directions at energies above $E_{th}/Z$ (for illustrative values of $Z=6,\ 13,\ 26$). If the anisotropies above $E_{th}$ are du…

ACTIVE GALACTIC NUCLEI[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]ProtonAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencescosmic ray experimentAcceleration (differential geometry)Cosmic rayultra high energy cosmic rays; cosmic ray experimentsultra high energy cosmic rays7. Clean energy01 natural sciencesultra high energy cosmic rayAugerNuclear physics0103 physical sciencesUltra-high-energy cosmic ray010306 general physicsAnisotropyNuclear ExperimentDETECTORHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FísicaCharge (physics)Astronomy and Astrophysics13. Climate actionExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearcosmic ray experimentsAstrophysics - High Energy Astrophysical PhenomenaJournal of Cosmology and Astroparticle Physics
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