Search results for "INOS"

showing 10 items of 2075 documents

Search for relativistic magnetic monopoles with the ANTARES neutrino telescope

2012

Magnetic monopoles are predicted in various unified gauge models and could be produced at intermediate mass scales. Their detection in a neutrino telescope is facilitated by the large amount of light emitted compared to that from muons. This paper reports on a search for upgoing relativistic magnetic monopoles with the ANTARES neutrino telescope using a data set of 116 days of live time taken from December 2007 to December 2008. The one observed event is consistent with the expected atmospheric neutrino and muon background, leading to a 90% C.L. upper limit on the monopole flux between 1.3 ¿ 10¿17 and 8.9 ¿ 10¿17 cm¿2 s¿1 sr¿1 for monopoles with velocity ß ¿ 0.625.

FLUXMuon backgroundParticle physicsGauge modelMagnetic monopolesAstrophysics::High Energy Astrophysical PhenomenaMagnetic monopoleneutrino telescopes; antares; magnetic monopoleFOS: Physical sciencesCosmic ray01 natural sciencesNuclear physics0103 physical sciencesNeutronFIELD010306 general physicsDETECTORCherenkov radiationZenithHigh Energy Astrophysical Phenomena (astro-ph.HE)NeutronsPhysicsSPECTRUMAtmospheric neutrinosMagnetic monopoleANTARES:Física::Acústica [Àrees temàtiques de la UPC]MuonCharged particles010308 nuclear & particles physicsAstronomy and AstrophysicsMonopols magnèticsUpper limitsNeutrino detectorMass scaleFISICA APLICADA[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Física nuclearData setsNeutrino telescopes[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical PhenomenaEvent (particle physics)TelescopesAstroparticle Physics
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Constraints on ultra-high-energy cosmic ray sources from a search for neutrinos above 10 PeV with IceCube

2016

We report constraints on the sources of ultra-high-energy cosmic ray (UHECR) above $10^{9}$ GeV, based on an analysis of seven years of IceCube data. This analysis efficiently selects very high energy neutrino-induced events which have deposited energies from $\sim 10^6$ GeV to above $10^{11}$ GeV. Two neutrino-induced events with an estimated deposited energy of $(2.6 \pm 0.3) \times 10^6$ GeV, the highest neutrino energies observed so far, and $(7.7 \pm 2.0) \times 10^5$ GeV were detected. The atmospheric background-only hypothesis of detecting these events is rejected at 3.6$\sigma$. The hypothesis that the observed events are of cosmogenic origin is also rejected at $>$99% CL because of…

FLUXSELECTIONFERMI-LATActive galactic nucleusCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciencesCosmic rayAstrophysicsParameter space7. Clean energy01 natural sciencesCOSMOGENIC NEUTRINOS; TRACK RECONSTRUCTION; FERMI-LAT; BURSTS; SPECTRUM; MODEL; FLUX; TELESCOPES; SELECTION; EMISSIONPulsar0103 physical sciencesTRACK RECONSTRUCTIONBURSTSddc:550Ultrahigh energy010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)SPECTRUM010308 nuclear & particles physicsStar formationCOSMOGENIC NEUTRINOSAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyMODELPhysics and Astronomy13. Climate actionTELESCOPESHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaEMISSIONEnergy (signal processing)Astrophysics - Cosmology and Nongalactic Astrophysics
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Probing the origin of cosmic-rays with extremely high energy neutrinos using the IceCube Observatory

2013

We have searched for extremely high energy neutrinos using data taken with the IceCube detector between May 2010 and May 2012. Two neutrino induced particle shower events with energies around 1 PeV were observed, as reported previously. In this work, we investigate whether these events could originate from cosmogenic neutrinos produced in the interactions of ultra-high energy cosmic-rays with ambient photons while propagating through intergalactic space. Exploiting IceCube's large exposure for extremely high energy neutrinos and the lack of observed events above 100 PeV, we can rule out the corresponding models at more than 90% confidence level. The model independent quasi-differential 90% …

FLUXSELECTIONFERMI-LATNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)PhotonRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayddc:500.2AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsLIMIT01 natural sciencesIceCubeHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Particle showerObservatory0103 physical sciencesddc:530010306 general physicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSPECTRUMRange (particle radiation)COSMOGENIC NEUTRINOS010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyPERFORMANCECOMPONENTMODELPhysics and Astronomy13. Climate actionIntergalactic travelHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaSYSTEMAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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First search for point sources of high-energy cosmic neutrinos with the ANTARES neutrino telescope

2011

Results are presented of a search for cosmic sources of high-energy neutrinos with the ANTARES neutrino telescope. The data were collected during 2007 and 2008 using detector configurations containing between 5 and 12 detection lines. The integrated live time of the analyzed data is 304 days. Muon tracks are reconstructed using a likelihood-based algorithm. Studies of the detector timing indicate a median angular resolution of 0.5 0.1deg. The neutrino flux sensitivity is 7.5 ¿ 10 -8(E ¿/ GeV) -2 GeV -1 s -1 cm -2 for the part of the sky that is always visible (¿ < -48deg), which is better than limits obtained by previous experiments. No cosmic neutrino sources have been observed.

FLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and Detectorsmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesDeclinationneutrinos; cosmic rays; astroparticle physicscosmic rays0103 physical sciencesAngular resolutionALGORITHMNeutrinosDETECTOR010303 astronomy & astrophysicsCosmic raysmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCOSMIC cancer databaseMuon010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorneutrinosASTRONOMYAstronomy and Astrophysicsastroparticle physics13. Climate actionSpace and Planetary ScienceSkyFISICA APLICADAddc:520Física nuclearHigh Energy Physics::ExperimentNeutrinoAstroparticle physicsAstrophysics - High Energy Astrophysical Phenomena
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MicroRNAs Associated With Biological Pathways of Left- and Right-sided Colorectal Cancer.

2020

BACKGROUND/AIM MicroRNAs (miRNAs) regulate the development of colorectal cancer (CRC). We aimed to investigate miRNAs and their relation to cancer-related signaling pathways in site-specific CRC. MATERIALS AND METHODS We used a total of 24 left- and right-sided Finnish CRC samples (discovery cohort) and The Cancer Genome Atlas public mature miRSeq dataset of 201 CRC samples (validation cohort). MiRNA differential expression and biological pathway analyses were performed using DESeq2 and the DIANA/mirPath tool, respectively. RESULTS We found 17 significantly differentially up-regulated [false discovery rate (FDR) <0.05] miRNAs in left-sided CRC ("left miRNAs"), and 15 in right-sided CRC ("ri…

False discovery rateOncologyMaleCancer Researchmedicine.medical_specialtyColorectal cancerDown-RegulationBiological pathwayCohort StudiesPhosphatidylinositol 3-KinasesTransforming Growth Factor betaInternal medicinemicroRNAMedicineHumansDifferential expressionPI3K/AKT/mTOR pathwayAgedbusiness.industryWnt signaling pathwayGeneral Medicinemedicine.diseasedigestive system diseasesUp-RegulationGene Expression Regulation NeoplasticOncologyCohortFemalebusinessColorectal NeoplasmsProto-Oncogene Proteins c-aktSignal TransductionAnticancer research
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Repaso a la evidencia isotópica sobre alimentación en la prehistoria valenciana durante el Mesolítico y el Neolítico

2016

Los análisis de isótopos estables son una herramienta fundamental a la hora de reconstruir la alimentación de poblaciones prehistóricas. Hasta hace poco este tipo de análisis no se había aplicado en nuestra tierra. Sin embargo, desde hace unos años el Este de la Península Ibérica se está convirtiendo en uno de los lugares del Mediterráneo donde se está realizando un mayor número de este tipo de estudios. Este artículo explica el potencial de los análisis isotópicos de carbono y nitrógeno sobre colágeno óseo para reconstruir las pautas alimentarias de poblaciones pasadas. También repasa todos los estudios publicados en tierras valencianas de cronología prehistórica publicados hasta la fecha,…

Farming developmentRecursos marinosMarine resourcesDietaIsótopos establesArqueologiaDesarrollo agrícolaDietStable isotopesArqueología
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Contribution to the knowledge of the Cynipidae (Hymenoptera) of Jordan

2006

10 paginas, 4 figuras y 1 table

FaunisticsQuercus calliprinosbiologyEcologyFaunaAndricusHedickianaHymenopteraInquilinesbiology.organism_classificationHedickiana levantinaQuercusGall waspsHedickianaBotanyAndricus miriamiGallAnimal Science and ZoologyTaxonomy (biology)
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Nutritional supplementation with myo-inositol-D-chiro-inositol: effect on reproductive system functionality in Long-term Survivors of Lymphoma

2022

Introduction/Background: The principal International scientific societies of oncology recommend that Long-term Survivors of Lymphoma join fertility programs. Therefore, we conducted a prospective observational controlled study, with the aim to assess the effects of oral supplementation with Myo-Inositol and D-Chiro-Inositol (MIC) on ovarian function parameters in Long-term Survivors of Lymphoma Methodology: Between January 2020 and January 2021, 90 female patients, long-term Survivors of Lymphoma with an average age of 34 years (range 25-44), were considered eligible and enrolled in the study (Figure 1). The study was registered on ClinicalTrials.gov (ID: NCT05410314). We conducted this stu…

FertilityLymphomaSettore MED/40 - Ginecologia E OstetriciaInositol
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Prenatal Ultrastructural Diagnosis in the Neuronal ceroid-lipofuscinoses

1994

Summary The neuronal ceroid-lipofuscinose (NCL) are autosomal-recessive disorders in childhood of unknown enzymatic origin. They can be recognized by the presence of abnormal lipopigments identified by electron microscopy. Based on the study of circulating lymphocytes, individual clinical subtypes of NCL can be correlated. Prenatal diagnosis of NCL with the electron microscope is now feasible for the infantile (Finnish) from (INCL) and late-infantile form (LINCL). INCL-specific granular lipopigments are present in endothelial cells of biopsied chorion stroma vessels of homozygously affected fetuses. In LINCL, disease-typical curvilinear bodies can be identified in uncultured amniotic fluid …

FetusPathologymedicine.medical_specialtyAmniotic fluid cellsCurvilinear bodiesPrenatal diagnosisChorionCell BiologyBiologyAmniotic FluidPathology and Forensic MedicineMicroscopy ElectronStromaNeuronal Ceroid-LipofuscinosesPregnancyPrenatal DiagnosisUltrastructuremedicineHumansFemaleElectron microscopicNeuronal Ceroid-LipofuscinosesPathology - Research and Practice
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Intervención nutricional en niños y adolescentes con fibrosis quística. Relación con la función pulmonar

2005

Cecilia.Martinez@uv.es; Francisco.Nunez@uv.es; Objetivo: Evaluar los efectos de la intervención nutricional precoz y continuada en pacientes pediátricos con fibrosis quística (FQ) y su posible implicación en la función pulmonar. Pacientes y métodos: Se incluyen el seguimiento de 19 pacientes con FQ (11 niñas, 8 niños) de 17 meses a 18 años de edad y promedio de 10 años de enfermedad. El genotipo de 16 pacientes es delta F 508 (10 homo, 6 heterocigotos). Cada 2-3 meses se les ha realizado: valoración clínica, dietética y antropométrica clasificando el estado de nutrición (EN) según Z pesto/talla, % peso para la talla, índice de masa corporal y Z talla/edad. Coincidentemente se obtuvo cultivo…

Fibrosis quísticaMalnutriciónValoración nutritionalUNESCO::CIENCIAS MÉDICAS ::Ciencias de la Nutrición ::Otras:CIENCIAS MÉDICAS ::Ciencias de la Nutrición ::Otras [UNESCO]Nutrición enteralPseudomonas aeruginosaFibrosis quística; Nutrición enteral; Malnutrición; Valoración nutritional; Pseudomonas aeruginosa; Función pulmonarFunción pulmonar
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