Search results for "actin"

showing 10 items of 1375 documents

Identification of Novel Molecular Components of the Photoreceptor Connecting Cilium by Immunoscreens

2002

Abstract The connecting cilium of photoreceptor cells is the only intracellular link between the morphologically, functionally and biochemically different compartments of the inner and outer segments. The non-motile modified cilium plays an important role in the organization and the function of photoreceptor cells, namely in delivery and turnover of enzymes and substrates of the visual transduction cascade, and the photosensitive membranes of the outer segment. The protein components of the cilium participate in the intracellular transport through the cilium, in the outer segment disk morphogenesis and in the maintenance of discrete membrane domains. In order to identify yet unknown cytoske…

Photoreceptor Connecting CiliumAdenomatous Polyposis Coli ProteinXenopus ProteinsBiologyPhotoreceptor cellRats Sprague-DawleyMiceCellular and Molecular NeurosciencemedicineAnimalsDrosophila ProteinsCiliaCloning MolecularCytoskeletonMicrotubule-Associated Protein 4CytoskeletonGene LibraryRetinaCiliumCalcium-Binding ProteinsDynactin ComplexSensory SystemsRatsCell biologyMice Inbred C57BLOphthalmologymedicine.anatomical_structureCentrinsense organsMicrotubule-Associated ProteinsPhotoreceptor Cells VertebrateVisual phototransductionExperimental Eye Research
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Molecular analysis of lichen-associated bacterial communities

2006

The bacterial communities associated with 11 different lichen samples (belonging to eight different species) from different habitats were investigated. The culturable aerobic-heterotrophic fraction of the bacterial communities was isolated from nine lichen samples on protein-rich and sugar-rich/N-free media. Thirty-four bacterial isolates were purified and pooled into groups (phylotypes) by analysis of the ribosomal internal transcribed spacer polymorphism. Twenty five phylotypes were identified, each comprising between one and three isolates. One isolate of each phylotype was partially sequenced and the resulting 16S rRNA gene sequences were compared in a phylogenetic analysis. Three gener…

PhylotypeEcologybiologyFirmicutesbiology.organism_classificationApplied Microbiology and BiotechnologyMicrobiologyActinobacteriaBurkholderiaBotanyInternal transcribed spacerProteobacteriaLichenRibosomal DNAFEMS Microbiology Ecology
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Material radioassay and selection for the XENON1T dark matter experiment

2017

The XENON1T dark matter experiment aims to detect weakly interacting massive particles (WIMPs) through low-energy interactions with xenon atoms. To detect such a rare event necessitates the use of radiopure materials to minimize the number of background events within the expected WIMP signal region. In this paper we report the results of an extensive material radioassay campaign for the XENON1T experiment. Using gamma-ray spectroscopy and mass spectrometry techniques, systematic measurements of trace radioactive impurities in over one hundred samples within a wide range of materials were performed. The measured activities allowed for stringent selection and placement of materials during the…

Physics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsDark matterMonte Carlo methodmeasurement methodsFOS: Physical scienceschemistry.chemical_elementRadiopuritylcsh:AstrophysicsWIMP: detectorSciences de l'ingénieur01 natural sciencesgamma ray: energy spectrumNuclear physicsmass spectrumXENONXenonWIMPlcsh:QB460-4660103 physical sciencesDark Matterlcsh:Nuclear and particle physics. Atomic energy. Radioactivity[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsSpectroscopy[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Engineering (miscellaneous)background: radioactivityPhysicsRange (particle radiation)Physique010308 nuclear & particles physicsDetectorInstrumentation and Detectors (physics.ins-det)AstronomiesensitivitychemistryWeakly interacting massive particleslcsh:QC770-798TPCnumerical calculations: Monte Carlo
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Search for WIMP Inelastic Scattering off Xenon Nuclei with XENON100

2017

We present the first constraints on the spin-dependent, inelastic scattering cross section of weakly interacting massive particles (WIMPs) on nucleons from XENON100 data with an exposure of 7.64 ×103 kg .days . XENON100 is a dual-phase xenon time projection chamber with 62 kg of active mass, operated at the Laboratori Nazionali del Gran Sasso (LNGS) in Italy and designed to search for nuclear recoils from WIMP-nucleus interactions. Here we explore inelastic scattering, where a transition to a low-lying excited nuclear state of Xe 129 is induced. The experimental signature is a nuclear recoil observed together with the prompt deexcitation photon. We see no evidence for such inelastic WIMP-Xe…

Physics - Instrumentation and DetectorsXenonPhysics and Astronomy (miscellaneous)Physics::Instrumentation and Detectors[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)XenonRecoilWIMP[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Dark MatterNuclear Experiment[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]nucleus: recoilPhysicsTime projection chamberAstrophysics::Instrumentation and Methods for AstrophysicsWIMP nucleon: cross sectionInstrumentation and Detectors (physics.ins-det)Excited stateWeakly interacting massive particlesTPCNucleonchannel cross section: measuredsignatureAstrophysics - Cosmology and Nongalactic AstrophysicsParticle physicsdata analysis methodCosmology and Nongalactic Astrophysics (astro-ph.CO)WIMPchemistry.chemical_elementFOS: Physical sciencesInelastic scatteringspin: dependenceNuclear physicsstatistical analysis[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]photon: emission0103 physical sciencescross section: inelastic scattering[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsWIMP nucleon: inelastic scattering010308 nuclear & particles physicsS030DP2WIMP nucleus: interactionGran SassochemistryDirect Searchtime projection chamber: xenonHigh Energy Physics::Experiment[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]experimental results
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Growth Aspects of Scad Decapterus macrosoma on Fish Point Sanggeng-Manokwari Regency

2018

Tujuan dari penelitian ini adalah untuk mengetahui aspek pertumbuhan ikan meliputi: distribusi ukuran, hubungan panjang-berat, faktor kondisi dan model pertumbuhan. Penelitian ini dilaksanakan pada bulan Maret sampai dengan bulan Juni 2015. Metode yang digunakan adalah metode deskriptif dengan teknik observasi. Jumlah ikan layang yang didapatkan sebanyak 500 ekor. Sebaran ukuran panjang yang diperoleh untuk individu jantan 109-303 mm dan 125-299 mm untuk individu betina. Berdasarkan hasil analisis korelasi antara panjang dan berat ikan layang seluruhnya positif dan sangat kuat, ikan betina memiliki nilai koefisien korelasin 0,6184 dengan koefisien determinasi (R2) 0,3824 dan ikan jantan 0,5…

PhysicsAnimal scienceFish <Actinopterygii>Decapterus macrosomaGrowth aspectsJURNAL SUMBERDAYA AKUATIK INDOPASIFIK
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Reconstructing WIMP properties with neutrino detectors

2008

If the dark matter of the Universe is constituted by weakly interacting massive particles (WIMP), they would accumulate in the core of astrophysical objects as the Sun and annihilate into particles of the Standard Model. High-energy neutrinos would be produced in the annihilations, both directly and via the subsequent decay of leptons, quarks and bosons. While Cherenkov neutrino detectors/telescopes can only count the number of neutrinos above some threshold energy, we study how, by exploiting their energy resolution, large magnetized iron calorimeter and, possibly, liquid argon and totally active scintillator detectors, planned for future long baseline neutrino experiments, have the capabi…

PhysicsAstrofísicaParticle physicsNuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Dark matterHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical scienceshep-phSolar neutrino problemAstrophysicsNuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino detectorWIMPastro-phWeakly interacting massive particlesHigh Energy Physics::ExperimentNeutrinoLight dark matterPhysics Letters B
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Luminosity function for galaxy clusters

2014

AbstractWe constructed and studied the luminosity function of 6188 galaxy clusters. This was performed by counting brightness of galaxies belonging to clusters in the PF catalogue, taking galaxy data from MRSS. Our result shows that the investigated structures are characterized by a luminosity function different from that of optical galaxies and radiogalaxies (Machalski &amp; Godłowski 2000). The implications of this result for theories of galaxy formation are briefly discussed.

PhysicsAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGalaxy mergerLuminosityBarred spiral galaxyGalaxy groups and clustersSpace and Planetary ScienceGalaxy groupInteracting galaxyLenticular galaxyAstrophysics::Galaxy AstrophysicsLuminosity function (astronomy)Proceedings of the International Astronomical Union
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Spin and rotational symmetries in unrestricted Hartree–Fock states of quantum dots

2007

Ground state energies are obtained using the unrestricted Hartree Fock method for up to four interacting electrons parabolically confined in a quantum dot subject to a magnetic field. Restoring spin and rotational symmetries we recover Hund first rule. With increasing magnetic field, crossovers between ground states with different quantum numbers are found for fixed electron number that are not reproduced by the unrestricted Hartree Fock approximation. These are consistent with the ones obtained with more refined techniques. We confirm the presence of a spin blockade due to a spin mismatch in the ground states of three and four electrons.

PhysicsCondensed Matter - Mesoscale and Nanoscale PhysicsMAGNETIC-FIELDARTIFICIAL ATOMSFOS: Physical sciencesGeneral Physics and AstronomyUnrestricted Hartree–Fockquantum dotsElectronINTERACTING ELECTRONSQuantum numberSettore FIS/03 - Fisica Della MateriaMagnetic fieldDIFFUSION MONTE-CARLOQuantum dotQuantum mechanicsMesoscale and Nanoscale Physics (cond-mat.mes-hall)Homogeneous spaceMANY-PARTICLE SYSTEMSGround stateSpin-½New Journal of Physics
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Ionization of atoms by slow heavy particles, including dark matter

2016

Atoms and molecules can become ionized during the scattering of a slow, heavy particle off a bound electron. Such an interaction involving leptophilic weakly interacting massive particles (WIMPs) is a promising possible explanation for the anomalous 9 sigma annual modulation in the DAMA dark matter direct detection experiment [R. Bernabei et al., Eur. Phys. J. C 73, 2648 (2013)]. We demonstrate the applicability of the Born approximation for such an interaction by showing its equivalence to the semiclassical adiabatic treatment of atomic ionization by slow-moving WIMPs. Conventional wisdom has it that the ionization probability for such a process should be exponentially small. We show, howe…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Atomic Physics (physics.atom-ph)010308 nuclear & particles physicsScatteringDark matterAtoms in moleculesFOS: Physical sciencesGeneral Physics and AstronomyElectron01 natural sciencesAstrophysics - Astrophysics of GalaxiesPhysics - Atomic PhysicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Astrophysics of Galaxies (astro-ph.GA)IonizationWeakly interacting massive particles0103 physical sciencesBorn approximationAtomic physics010306 general physicsRelativistic quantum chemistryAstrophysics - Cosmology and Nongalactic Astrophysics
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Study and implementation of a soft X-ray 100 eV -20 keV fixed exit monochromator system

2006

We describe a “built in house” X-ray monochromator which produces a fixed exit X-ray beam tunable in the full energy range 0.1 - 20 keV. The system is based on a double diffraction on two large size parallel crystals positioned using a remotely controlled micropositioning system in order to keep the position of the monochromatic beam for any chosen energy. Up to six different diffracting elements can be selected without breaking the vacuum. This allows to cover the full energy range of interest. The system is part of an upgrading project of the XACT facility at the Istituto Nazionale di Astrofisica - Osservatorio Astronomico di Palermo G.S. Vaiana, and will be employed for the testing and c…

PhysicsDiffractionRange (particle radiation)business.industryDetectorlaw.inventionWavelengthOpticslawCalibrationbusinessEnergy (signal processing)Beam (structure)MonochromatorX-ray monochromator crystals multilayer diffracting elements soft x-ray
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