Search results for " observations"

showing 10 items of 100 documents

A White Paper on keV sterile neutrino Dark Matter

2017

We present a comprehensive review of keV-scale sterile neutrino Dark Matter, collecting views and insights from all disciplines involved - cosmology, astrophysics, nuclear, and particle physics - in each case viewed from both theoretical and experimental/observational perspectives. After reviewing the role of active neutrinos in particle physics, astrophysics, and cosmology, we focus on sterile neutrinos in the context of the Dark Matter puzzle. Here, we first review the physics motivation for sterile neutrino Dark Matter, based on challenges and tensions in purely cold Dark Matter scenarios. We then round out the discussion by critically summarizing all known constraints on sterile neutrin…

AstrofísicaSterile neutrinocosmological modelCold dark mattercosmological neutrinosPhysics beyond the Standard Model[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Dark matter theory01 natural sciencesCosmologyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)White paperHigh Energy Physics - Phenomenology (hep-ph)X-RAY-EMISSIONMETALLIC MAGNETIC CALORIMETERSQUANTUM-FIELD THEORY[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]neutrino: dark matterCosmological neutrinos; Dark matter experiments; Dark matter theory; Particle physics - cosmology connection010303 astronomy & astrophysicsPhysicsdark matter theorynew physicsDOUBLE-BETA-DECAYhep-phneutrino: sterileCosmological neutrinos; Dark matter experiments; Dark matter theory; Particle physics - cosmology connection; Astronomy and AstrophysicsNuclear & Particles PhysicsHigh Energy Physics - Phenomenologyneutrino: detectorDark matter experimentsparticle physics - cosmology connectionastro-ph.COMILKY-WAY SATELLITESCosmological neutrinos3.5 KEV LINENeutrinoParticle Physics - ExperimentAstrophysics - Cosmology and Nongalactic AstrophysicsParticle physicsAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)astro-ph.GADark matterLY-ALPHA FORESTreviewFOS: Physical sciencesContext (language use)neutrino: productionX-raySettore FIS/05 - Astronomia e Astrofisica[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]RIGHT-HANDED NEUTRINOS0103 physical sciencesAstronomical And Space Sciencesnumerical calculationsDark matter experimentXMM-NEWTON OBSERVATIONSneutrino: modelParticle Physics - PhenomenologyDWARF SPHEROIDAL GALAXYCosmologia010308 nuclear & particles physicshep-exdark matter experimentsHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsAtomic Molecular Nuclear Particle And Plasma PhysicsCosmological neutrinoAstrophysics - Astrophysics of Galaxies13. Climate actionAstrophysics of Galaxies (astro-ph.GA)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Particle physics - cosmology connection[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experimentneutrino: oscillation[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Journal of Cosmology and Astroparticle Physics
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Multifrequency Studies of the Peculiar Quasar 4C +21.35 during the 2010 Flaring Activity

2014

著者人数: 290名

AstrofísicaelectronPhotontorusAstrophysics01 natural scienceslaw.inventiongalaxies: active – gamma rays: general – quasars: general – quasars: individual (4C +21.35) – radiation mechanisms: non-thermalactive gamma rays: general quasars: general quasars: individual: 4C +21.35 radiation mechanisms: non-thermal [galaxies]lawblack hole: Kerrgalaxies: active; gamma rays: general; quasars: general; quasars: individual: 4C +21.35; radiation mechanisms: non-thermalopticalGalaxies: active; Gamma rays: general; Quasars: general; Quasars: individual (4C +21.35); Radiation mechanisms: non-thermal010303 astronomy & astrophysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsenergy: highPhysicsphotonRadiusnon-thermal [radiation mechanisms]Synchrotrongamma ray: emissionactive [galaxies]astro-ph.COElectrónicaFísica nuclearElectricidadGalaxies: active; Gamma rays: general; Quasars: general; Quasars: individual (4C +21.35); Radiation mechanisms: non-thermal; Nuclear and High Energy PhysicsAstrophysics - High Energy Astrophysical Phenomenaquasars: individual (4C +21.35)Astrophysics - Cosmology and Nongalactic AstrophysicsFlareradiation mechanisms: non-thermal; galaxies: active; quasars: general; quasars: individual (4C +21.35); gamma rays: observationsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)astro-ph.GAAstrophysics::High Energy Astrophysical Phenomenaeducationgalaxies: activeFOS: Physical sciencesquasars: individual: 4C +21.35Astrophysics::Cosmology and Extragalactic AstrophysicsVHEGLASTemission: modelTelescopeX-rayquasars: general0103 physical sciencessynchrotrongalaxies: active gamma rays: general quasars: general quasars: individual: 4C +21.35 radiation mechanisms: non-thermalquasarflux: densityindividual: 4C +21.35 [quasars]Astrophysics::Galaxy AstrophysicsAstronomia Observacionsgeneral [quasars]010308 nuclear & particles physicsAstronomy and AstrophysicsQuasargamma rays: generalradiation mechanisms: non-thermalAstrophysics - Astrophysics of GalaxiesMAGICRotating black holeSpace and Planetary SciencegravitationAstrophysics of Galaxies (astro-ph.GA)ddc:520spectral[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]general [gamma rays]Fermi Gamma-ray Space Telescope
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SDSS-III: Massive Spectroscopic Surveys of the Distant Universe, the Milky Way Galaxy, and Extra-Solar Planetary Systems

2011

Building on the legacy of the Sloan Digital Sky Survey (SDSS-I and II), SDSS-III is a program of four spectroscopic surveys on three scientific themes: dark energy and cosmological parameters, the history and structure of the Milky Way, and the population of giant planets around other stars. In keeping with SDSS tradition, SDSS-III will provide regular public releases of all its data, beginning with SDSS DR8 (which occurred in Jan 2011). This paper presents an overview of the four SDSS-III surveys. BOSS will measure redshifts of 1.5 million massive galaxies and Lya forest spectra of 150,000 quasars, using the BAO feature of large scale structure to obtain percent-level determinations of the…

Astrofísicaplanets and satellites: detection[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Milky WayFOS: Physical sciencesEspectros astronômicosAstrophysics::Cosmology and Extragalactic AstrophysicsSurveys01 natural sciencesevolution [Galaxy]Movimento estelarsurveysPlanetBulge0103 physical sciencesPhysical Sciences and MathematicsAstrophysics::Solar and Stellar AstrophysicsMatéria escuraobservations [Cosmology]Instrumentation and Methods for Astrophysics (astro-ph.IM)Tecnicas astronomicas010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsMapeamentos astronômicosAglomerados de galaxiasPlanetas extrasolaresPhysicsGalaxy: evolutionCosmologia010308 nuclear & particles physicsGiant planetAstrophysics::Instrumentation and Methods for AstrophysicsFísicaAstronomyAstronomy and AstrophysicsQuasarComposicao estelarPlanetary systemEspectros estelaresRedshiftGalaxy[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]detection [Planets and satellites]Space and Planetary Sciencecosmology: observationsAstrophysics::Earth and Planetary AstrophysicsAstrophysics - Instrumentation and Methods for Astrophysics
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Detection of GRB 060927 at z = 5.47: Implications for the Use of Gamma-Ray Bursts as Probes of the End of the Dark Ages

2007

We report on follow-up observations of the GRB 060927 using the ROTSE-IIIa telescope and a suite of larger aperture ground-based telescopes. An optical afterglow was detected 20 s after the burst, the earliest rest-frame detection of optical emission from any GRB. Spectroscopy performed with the VLT about 13 hours after the trigger shows a continuum break at lambda ~ 8070 A produced by neutral hydrogen absorption at z~5.6. We also detect an absorption line at 8158 A which we interpret as SiII at z=5.467. Hence, GRB 060927 is the second most distant GRB with a spectroscopically measured redshift. The shape of the red wing of the spectral break can be fitted by a damped Lyalpha profile with a…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesCosmology: ObservationsSpectral linelaw.inventionTelescopeCosmology: Observations; gamma rays: bursts (GRB 060927)law0103 physical sciences010303 astronomy & astrophysicsReionizationAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsAstrophysics (astro-ph)Astronomy and AstrophysicsGalaxyRedshiftAfterglowQC Physics13. Climate actionSpace and Planetary ScienceDark Agesgamma rays: bursts(GRB 060927)Gamma-ray burstgamma rays: bursts (GRB 060927)Astrophysical Journal
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Gamma-Ray Flares from Mrk421 in 2008 observed with the ARGO-YBJ detector

2010

In 2008 the blazar Markarian 421 entered a very active phase and was one of the brightest sources in the sky at TeV energies, showing frequent flaring episodes. Using the data of ARGO-YBJ, a full coverage air shower detector located at Yangbajing (4300 m a.s.l., Tibet, China), we monitored the source at gamma ray energies E > 0.3 TeV during the whole year. The observed flux was variable, with the strongest flares in March and June, in correlation with X-ray enhanced activity. While during specific episodes the TeV flux could be several times larger than the Crab Nebula one, the average emission from day 41 to 180 was almost twice the Crab level, with an integral flux of (3.6 +-0.6) 10^-1…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysicsBL Lacertae objectSettore FIS/05 - Astronomia E AstrofisicaExtended Air showersSettore FIS/05 - Astronomia e Astrofisicageneral" ["gamma rays]BlazarBL Lacertae objects; Markarian 421; gamma rays; Extended Air showersCherenkov radiationHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSpectral indexindividual (Markarian 421)" ["BL Lacertae objects]Markarian 421Settore FIS/01 - Fisica SperimentaleGamma rayindividual (Markarian 421) - gamma rays: observations [BL Lacertae objects]Astronomy and AstrophysicsAir showerCrab NebulaSpace and Planetary Sciencegamma rayIntergalactic travelAstrophysics - High Energy Astrophysical Phenomena
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SOUTHTRAC-GW: An airborne field campaign to explore gravity wave dynamics at the world’s strongest hotspot

2021

The southern part of South America and the Antarctic peninsula are known as the world’s strongest hotspot region of stratospheric gravity wave (GW) activity. Large tropospheric winds are deflected by the Andes and the Antarctic Peninsula and excite GWs that might propagate into the upper mesosphere. Satellite observations show large stratospheric GW activity above the mountains, the Drake Passage, and in a belt centered along 60°S. This scientifically highly interesting region for studying GW dynamics was the focus of the Southern Hemisphere Transport, Dynamics, and Chemistry–Gravity Waves (SOUTHTRAC-GW) mission. The German High Altitude and Long Range Research Aircraft (HALO) was deployed …

Atmospheric Science010504 meteorology & atmospheric sciences0207 environmental engineering02 engineering and technologySudden stratospheric warmingGravity waves01 natural sciencesTroposphereMountain wavesHotspot (geology)ddc:550Gravity wave020701 environmental engineeringSouthern Hemisphere0105 earth and related environmental sciencesStratospheric circulationInstitut für Physik der AtmosphäreLidarVerkehrsmeteorologieAircraft observationsEffects of high altitude on humansGeofísicaTrace gasDynamicsEarth sciencesLidarClimatologyGeology
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Assessment of the SMAP Level-4 Surface and Root-Zone Soil Moisture Product Using In Situ Measurements

2017

International audience; The Soil Moisture Active Passive (SMAP) mission Level-4 Surface and Root-Zone Soil Moisture (L4_SM) data product is generated by assimilating SMAP L-band brightness temperature observations into the NASA Catchment land surface model. The L4_SM product is available from 31 March 2015 to present (within 3 days from real time) and provides 3-hourly, global, 9-km resolution estimates of surface (0-5 cm) and root-zone (0-100 cm) soil moisture and land surface conditions. This study presents an overview of the L4_SM algorithm, validation approach, and product assessment versus in situ measurements. Core validation sites provide spatially averaged surface (root zone) soil m…

Atmospheric Science010504 meteorology & atmospheric sciences0208 environmental biotechnologyDrainage basin[SDU.STU]Sciences of the Universe [physics]/Earth SciencesSoil science02 engineering and technologyLand cover01 natural sciencesStandard deviationITC-HYBRIDData assimilationSoil temperatureWater content0105 earth and related environmental sciencesgeographygeography.geographical_feature_category020801 environmental engineeringSatellite observations[SDU]Sciences of the Universe [physics]Brightness temperatureITC-ISI-JOURNAL-ARTICLEData assimilationDNS root zoneEnvironmental scienceSoil moistureLand surface modelScale (map)Kalman filtersJournal of hydrometeorology
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Microphysical Properties of Ice Crystal Precipitation and Surface-Generated Ice Crystals in a High Alpine Environment in Switzerland

2017

AbstractDuring the Cloud and Aerosol Characterization Experiment (CLACE) 2013 field campaign at the High Altitude Research Station Jungfraujoch, Switzerland, optically thin pure ice clouds and ice crystal precipitation were measured using holographic and other in situ particle instruments. For cloud particles, particle images, positions in space, concentrations, and size distributions were obtained, allowing one to extract size distributions classified by ice crystal habit. Small ice crystals occurring under conditions with a vertically thin cloud layer above and a stratocumulus layer approximately 1 km below exhibit similar properties in size and crystal habits as Antarctic/Arctic diamond …

Atmospheric Science010504 meteorology & atmospheric sciencesAtmospheric sciences01 natural sciencesPhysics::Geophysics010309 opticsDiamond dustSea ice growth processesCloud microphysics0103 physical sciencesIce fogPrecipitationCrystal habitComplex terrainPhysics::Atmospheric and Oceanic Physics0105 earth and related environmental sciencesIce crystalsIce particlesSurface observations13. Climate actionIn situ atmospheric observationsIce nucleusParticleAstrophysics::Earth and Planetary Astrophysics/dk/atira/pure/subjectarea/asjc/1900/1902GeologyJournal of Applied Meteorology and Climatology
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Advances in understanding mineral dust and boundary layer processes over the Sahara from Fennec aircraft observations

2015

Abstract. The Fennec climate programme aims to improve understanding of the Saharan climate system through a synergy of observations and modelling. We present a description of the Fennec airborne observations during 2011 and 2012 over the remote Sahara (Mauritania and Mali) and the advances in the understanding of mineral dust and boundary layer processes they have provided. Aircraft instrumentation aboard the UK FAAM BAe146 and French SAFIRE (Service des Avions Français Instrumentés pour la Recherche en Environnement) Falcon 20 is described, with specific focus on instrumentation specially developed for and relevant to Saharan meteorology and dust. Flight locations, aims and associated met…

Atmospheric Science010504 meteorology & atmospheric sciencesMeteorologyPlanetary boundary layerCONVECTIVE SYSTEMEnvironmental Sciences & EcologyAEROSOL OPTICAL-PROPERTIESMineral dust010502 geochemistry & geophysicsAtmospheric sciences01 natural sciencesCOARSE MODElcsh:ChemistryHaboobDust storm0201 Astronomical and Space SciencesMeteorology & Atmospheric SciencesSatellite imagerySOUTHERN MOROCCO0105 earth and related environmental sciences[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]GBScience & TechnologyHEAT LOWAIRBORNE OBSERVATIONSRETRIEVAL PRODUCTSOzone depletionlcsh:QC1-999PARTICLE-SIZEAERONETBoundary layerlcsh:QD1-99913. Climate action[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/ClimatologyPhysical SciencesWEST-AFRICAN MONSOONEnvironmental science0401 Atmospheric SciencesNORTH-ATLANTIC OCEANLife Sciences & Biomedicinelcsh:PhysicsEnvironmental SciencesAtmospheric Chemistry and Physics
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Mixed-Phase Clouds: Progress and Challenges

2017

Mixed-phase clouds represent a three-phase colloidal system consisting of water vapor, ice particles, and coexisting supercooled liquid droplets. Mixed-phase clouds are ubiquitous in the troposphere, occurring at all latitudes from the polar regions to the tropics. Because of their widespread nature, mixed-phase processes play critical roles in the life cycle of clouds, precipitation formation, cloud electrification, and the radiative energy balance on both regional and global scales. Yet, in spite of many decades of observations and theoretical studies, our knowledge and understanding of mixed-phase cloud processes remains incomplete. Mixed-phase clouds are notoriously difficult to represe…

Atmospheric Science010504 meteorology & atmospheric sciencesMeteorologybusiness.industryEarth scienceCloud physicsCloud computing010502 geochemistry & geophysicsOceanographyNumerical weather prediction01 natural sciencesTroposphere13. Climate actionInternational Satellite Cloud Climatology Projectddc:550Clouds; Aircraft observations; Lidars/Lidar observations; Microwave observations; Radars/Radar observations; Climate modelsEnvironmental scienceClimate modelPrecipitationbusinessWater vaporAstrophysics::Galaxy AstrophysicsPhysics::Atmospheric and Oceanic Physics0105 earth and related environmental sciences
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