Search results for "methods [Gene Expression Profiling]"

showing 10 items of 838 documents

Evolution of Balmer jump selected galaxies in the ALHAMBRA survey

2016

Extragalactic astronomy.-- et al.

Galaxies: generalAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesevolution [Galaxy]high-redshift [Galaxies]Galactic haloBalmer jump0103 physical sciencesGalaxy formation and evolutionAstrophysics::Solar and Stellar Astrophysicshalo [Galaxy]010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy Astrophysics[PHYS]Physics [physics]PhysicsGalaxy: evolution010308 nuclear & particles physicsphotometry [Galaxies]Astrophysics::Instrumentation and Methods for AstrophysicsGalaxies: high-redshiftGalaxies: evolutiongeneral [Galaxies]Astronomy and AstrophysicsGalaxies: photometryevolution [Galaxies]Astrophysics - Astrophysics of GalaxiesGalaxyPhysics::History of PhysicsGalaxy: haloSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astronomy & Astrophysics
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VizieR Online Data Catalog: Gaia DR2 sources in GC and dSph (Gaia Collaboration+, 2018)

2018

The files contains lists of possible members of each of the objects (75 globular clusters, 9 dwarf spheroidal galaxies, the Bootes I UFD, the LMC and SMC). The stars in these lists have been selected and used to determine the astrometric parameters of the corresponding objects following either the procedures described in Sec. 2.1 (for the clusters and dwarfs) or in Sec. 2.2 (for the LMC and SMC). The first column is the "source_id" as given by Gaia, the ra and declination of the star in degrees, and its G-band magnitude (known as "photgmean_mag" in the Gaia archive). (2 data files).

Galaxies: nearbyPositional data[SDU.ASTR.IM] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]SurveysClusters: globular
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Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation

2021

Full list of authors: Abdalla, H.; Abe, H.; Acero, F.; Acharyya, A.; Adam, R.; Agudo, I; Aguirre-Santaella, A.; Alfaro, R.; Alfaro, J.; Alispach, C.; Aloisio, R.; Batista, R. Alves; Amati, L.; Amato, E.; Ambrosi, G.; Anguner, E. O.; Araudo, A.; Armstrong, T.; Arqueros, F.; Arrabito, L.; Asano, K.; Ascasibar, Y.; Ashley, M.; Backes, M.; Balazs, C.; Balbo, M.; Balmaverde, B.; Baquero Larriva, A.; Martins, V. Barbosa; Barkov, M.; Baroncelli, L.; de Almeida, U. Barres; Barrio, J. A.; Batista, P-, I; Becerra Gonzalez, J.; Becherini, Y.; Beck, G.; Tjus, J. Becker; Belmont, R.; Benbow, W.; Bernardini, E.; Berti, A.; Berton, M.; Bertucci, B.; Beshley, V; Bi, B.; Biasuzzi, B.; Biland, A.; Bissaldi, …

Gamma ray AstronomyCherenkov Telescope ArrayaxionsMATÉRIA ESCURAredshift: dependenceAstronomyGamma ray experimentsgamma ray experimentsAstrophysics01 natural sciencesCosmologyObservatorycosmological model: parameter spacegamma ray experimentHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEPhysicsCherenkov telescopes ; IACT technique ; Gamma rays ; Cosmic raysnew physics4. EducationSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsGamma-ray astronomyviolation: Lorentz3. Good healthobservatoryExtragalactic background lightastro-ph.COaxion-like particlesFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic Astrophysicsgamma ray: propagationCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusAxionsAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsinvariance: Lorentzjet: relativisticdark matter: halo0103 physical sciencesactive galactic nuclei; gamma ray experiments; axions; extragalactic magnetic fieldsAGNBlazarbackground010308 nuclear & particles physicsFísicaAstronomy and AstrophysicssensitivityCherenkov Telescope Arrayaxionextragalactic magnetic fieldsactive galactic nuclei[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]absorptionstatisticalBlazarsTelescopes
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Localisation of gamma-ray bursts from the combined SpIRIT+HERMES-TP/SP nano-satellite constellation

2023

Multi-messenger observations of the transient sky to detect cosmic explosions and counterparts of gravitational wave mergers critically rely on orbiting wide-FoV telescopes to cover the wide range of wavelengths where atmospheric absorption and emission limit the use of ground facilities. Thanks to continuing technological improvements, miniaturised space instruments operating as distributed-aperture constellations are offering new capabilities for the study of high energy transients to complement ageing existing satellites. In this paper we characterise the performance of the upcoming joint SpIRIT + HERMES-TP/SP nano-satellite constellation for the localisation of high-energy transients th…

Gamma ray transient sourceHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceX-ray transient sourceSpace telescopeTime domain astronomyFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)
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CARDIOVASCULAR DISEASE RISKS AND FACTORS INFLUENCING THEM AMONG MEDICAL COLLEGE STUDENTS

2016

The aim of the study is to identify the CVD risks among medical college students associating them to their lifestyle. It should be noted that cardiovascular diseases also affect young people, which students are also. Information obtained during research is necessary for prospective medical staff to acknowledge their cardiovascular health and its influencing factors, as well as for college lecturers to make changes in study programs. The theoretical part of the research discusses various CVD risk determination methods, as well as lifestyle`s impact on cardiovascular health. The empirical part of the research contains information about ten years CVD risk among students, using two Framingham m…

GerontologyFramingham Heart StudyFramingham Risk ScoreBlood pressureCVD risks; Framingham methods lifestyle`s impact on cardiovascular health; medical college studentsbusiness.industryMedicineDetermination methodsDiseaseRisk factorbusinessAffect (psychology)Body mass indexSOCIETY. INTEGRATION. EDUCATION. Proceedings of the International Scientific Conference
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A coordinated preventive care approach for healthy ageing in five European cities: A mixed methods study of process evaluation components

2019

To evaluate specific process components of the Urban Health Centres Europe (UHCE) approach; a coordinated preventive care approach aimed at healthy ageing by decreasing falls, polypharmacy, loneliness and frailty among older persons in community settings of five cities in the United Kingdom, Greece, Croatia, the Netherlands and Spain.Mixed methods evaluation of specific process components of the UHCE approach: reach of the target population, dose of the intervention actually delivered and received by participants and satisfaction and experience of main stakeholders involved in the approach.The UHCE approach intervention consisted of a preventive assessment, shared decision-making on a care …

GerontologyMaleFrail Elderlycoordinated careQualitative propertyfrailtycoordinated care ; frailty ; mixed methods study ; nurses ; older persons ; prevention ; primary care ; process evaluationnursesHealthy Agingprimary careprocess evaluation.03 medical and health sciences0302 clinical medicinepreventionBIOMEDICINA I ZDRAVSTVO. Javno zdravstvo i zdravstvena zaštita.Intervention (counseling)Surveys and QuestionnairesPreventive Health ServicesmedicineHumans030212 general & internal medicineGeriatric AssessmentGeneral NursingAgedPolypharmacyAged 80 and over030504 nursingDescriptive statisticsFrailtyLonelinessBIOMEDICINE AND HEALTHCARE. Public Health and Health Care.Urban HealthLonelinessmixed methods studyFocus groupEuropeCaregiversolder personsPolypharmacyAccidental FallsFemaleIndependent LivingThematic analysismedicine.symptom0305 other medical sciencePsychologyPsychosocialAttitude to HealthJournal of Advanced Nursing
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The puzzling case of the accreting millisecond X-ray pulsar IGR J00291+5934: flaring optical emission during quiescence

2017

We present an optical (gri) study during quiescence of the accreting millisecond X-ray pulsar IGR J00291+5934 performed with the 10.4m Gran Telescopio Canarias (GTC) in August 2014. Despite the source being in quiescence at the time of our observations, it showed a strong optical flaring activity, more pronounced at higher frequencies (i.e. the g band). Once the flares were subtracted, we tentatively recovered a sinusoidal modulation at the system orbital period in all bands, even if a significant phase shift with respect to an irradiated star, typical of accreting millisecond X-ray pulsars is detected. We conclude that the observed flaring could be a manifestation of the presence of an acc…

Gran Telescopio CanariasAstrophysics::High Energy Astrophysical Phenomenaneutron X-rays: binaries accretion accretion disks [stars]FOS: Physical sciencesAstrophysics01 natural sciencesSettore FIS/05 - Astronomia E AstrofisicaPulsarAccretion discstars: neutron X-rays: binaries accretion accretion disks0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMillisecond010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsLight curveOrbital period3. Good healthAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceOptical emission spectroscopyAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaX-ray pulsar
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Gravitational-wave Constraints on the Equatorial Ellipticity of Millisecond Pulsars

2020

We present a search for continuous gravitational waves from five radio pulsars, comprising three recycled pulsars (PSR J0437-4715, PSR J0711-6830, and PSR J0737-3039A) and two young pulsars: the Crab pulsar (J0534+2200) and the Vela pulsar (J0835-4510). We use data from the third observing run of Advanced LIGO and Virgo combined with data from their first and second observing runs. For the first time, we are able to match (for PSR J0437-4715) or surpass (for PSR J0711-6830) the indirect limits on gravitational-wave emission from recycled pulsars inferred from their observed spin-downs, and constrain their equatorial ellipticities to be less than 10-8. For each of the five pulsars, we perfor…

Gravitational waves; Neutron stars; Pulsars; Gravitational wave sources010504 meteorology & atmospheric sciencesAstronomyAstrophysicsVela01 natural sciencesGeneral Relativity and Quantum Cosmology[SPI]Engineering Sciences [physics]neutronMillisecond pulsaremission010303 astronomy & astrophysicsQCQBSettore FIS/01Physicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)[PHYS]Physics [physics]PhysicsAstrophysics::Instrumentation and Methods for Astrophysics[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenaGravitational-Waves Pulsars Neutron StarsGravitational wavePROPER MOTIONProper motiongr-qcAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesNeutron starGeneral Relativity and Quantum Cosmology (gr-qc)Gravitational-WavesGravitational wavesNeutron starsSEARCHESSettore FIS/05 - Astronomia e AstrofisicaPulsar0103 physical sciencesPulsar[CHIM]Chemical SciencesAstrophysiqueSTFCPulsarsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesGravitational wave sourcescrab pulsarGravitational waveCrab PulsarRCUKAstronomy and AstrophysicsNeutron StarsGravitational waves Neutron stars Pulsars Gravitational wave sourcesLIGONeutron starSpace and Planetary Science[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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The enhanced X-ray Timing and Polarimetry mission—eXTP

2019

In this paper we present the enhanced X-ray Timing and Polarimetry mission - eXTP. eXTP is a space science mission designed to study fundamental physics under extreme conditions of density, gravity and magnetism. The mission aims at determining the equation of state of matter at supra-nuclear density, measuring effects of QED, and understanding the dynamics of matter in strong-field gravity. In addition to investigating fundamental physics, eXTP will be a very powerful observatory for astrophysics that will provide observations of unprecedented quality on a variety of galactic and extragalactic objects. In particular, its wide field monitoring capabilities will be highly instrumental to det…

Gravity (chemistry)Computer sciencespace mission: eXTPX-ray timingPolarimetryGeneral Physics and AstronomyFOS: Physical sciences01 natural sciences7. Clean energyPhysics and Astronomy (all)Settore FIS/05 - Astronomia E AstrofisicaObservatoryX-ray instrumentation0103 physical sciencesX-ray polarimetryGround segmentAerospace engineering010306 general physics010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)High Energy Astrophysical Phenomena (astro-ph.HE)Spacecraftsezelebusiness.industryPayloadGravitational waveAstrophysics::Instrumentation and Methods for Astrophysicsspace mission: eXTP; X-ray instrumentation; X-ray polarimetry; X-ray timing; Physics and Astronomy (all)Space SciencebusinessAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Atmospheric and astrophysical neutrinos above 1 TeV interacting in IceCube

2015

The IceCube Neutrino Observatory was designed primarily to search for high-energy (TeV--PeV) neutrinos produced in distant astrophysical objects. A search for $\gtrsim 100$~TeV neutrinos interacting inside the instrumented volume has recently provided evidence for an isotropic flux of such neutrinos. At lower energies, IceCube collects large numbers of neutrinos from the weak decays of mesons in cosmic-ray air showers. Here we present the results of a search for neutrino interactions inside IceCube's instrumented volume between 1~TeV and 1~PeV in 641 days of data taken from 2010--2012, lowering the energy threshold for neutrinos from the southern sky below 10 TeV for the first time, far bel…

HIGH-ENERGY NEUTRINOSNuclear and High Energy PhysicsParticle physicsAMANDAMesonSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaINDUCED CASCADESFOS: Physical sciencesCosmic rayAstrophysicsFLUX PREDICTIONS01 natural sciencesIceCube Neutrino ObservatoryIceCubeObservatorySEARCH0103 physical sciencesddc:530Blazar010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsASTRONOMYPERFORMANCEBLAZARSPROMPT LEPTONSGAMMA-RAYPhysics and AstronomyHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical PhenomenaphysicsPhysical Review D
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