Search results for "Extra-galactic"

showing 10 items of 83 documents

The data acquisition system for the ANTARES neutrino telescope

2006

The ANTARES neutrino telescope is being constructed in the Mediterranean Sea. It consists of a large three-dimensional array of photo-multiplier tubes. The data acquisition system of the detector takes care of the digitisation of the photo-multiplier tube signals, data transport, data filtering, and data storage. The detector is operated using a control program interfaced with all elements. The design and the implementation of the data acquisition system are described.

Nuclear and High Energy Physics[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and DetectorsData managementAstrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONFOS: Physical sciencesAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Data filteringData acquisition0103 physical sciences14. Life underwaterElectronics010306 general physicsInstrumentationdata acquisition system; neutrino telescopeRemote sensingAstroparticle physicsPhysicsneutrino telescope data acquisition system[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsbusiness.industryDetectorAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsAstronomyneutrino telescopedata acquisition systemComputer data storageFísica nuclearbusiness
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New Pre-Main Sequence Candidates in the Taurus-Auriga Star Forming Region

2007

Aims. We have studied the X-ray source population of the Taurus Molecular Cloud (TMC) to search for new members of the Taurus-Auriga star forming region. Methods. Candidate members have been selected among the X-ray sources detected in 24 fields of the XMM-Newton Extended Survey of the Taurus Molecular Cloud, having an IR counterpart in the 2MASS catalog, based on color-magnitude and color-color diagrams. Their X-ray spectral properties have been compared with those of known members and other X-ray sources in the same fields but without a NIR counterpart. A search for flare-like variability in the time series of all new candidates and the analysis of the X-ray spectra of the brightest candi…

010504 meteorology & atmospheric sciencesStellar massAstrophysics::High Energy Astrophysical PhenomenaAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxy : open clusters and associations : individual : Taurus Molecular Cloud01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]stars : activitystars : pre-main-sequence0103 physical sciencesstars : luminosity function mass functionAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsLuminosity functionAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsAURIGAMolecular cloudAstronomyAstronomy and AstrophysicsLight curveStarsStar clusterSpace and Planetary Science[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]X-rays : starAstrophysics::Earth and Planetary Astrophysicsstars : coronaeOpen cluster
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Cosmologie des théories de gravite modifiées

2017

The study of physical cosmology has reached an exciting era. For the first time in human history, a quantitative model for the formation and the evolution of the Universe exists, which explains a wide range of phenomena and has been tested with incredible accuracy during the last century. Moreover, weare approaching a time when a bounty of high quality cosmological data will be available,allowing us to use cosmology as a tool to test fundamental physics.In particular, as the large-scale structures of the Universe are governed by gravity, cosmology can help us to asses the correctness of Albert Einstein’s general relativity. This idea fueledmost of the work described in this manuscript,in wh…

[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Modified gravity[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Gravite modifiéeLarge scale structureCosmologieCosmologyStructure grand echelle
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Fracture Processes Observed with A Cryogenic Detector

2006

In the early stages of running of the CRESST dark matter search using sapphire detectors at very low temperature, an unexpectedly high rate of signal pulses appeared. Their origin was finally traced to fracture events in the sapphire due to the very tight clamping of the detectors. During extensive runs the energy and time of each event was recorded, providing large data sets for such phenomena. We believe this is the first time the energy release in fracture has been directly and accurately measured on a microscopic event-by-event basis. The energy threshold corresponds to the breaking of only a few hundred covalent bonds, a sensitivity some orders of magnitude greater than that of previou…

Physics - Instrumentation and Detectorsmedia_common.quotation_subjectDark matterGeneral Physics and AstronomyFOS: Physical sciencesAstrophysics01 natural sciencesAsymmetryPower law010305 fluids & plasmasHigh Energy Physics - Experiment[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Time domain[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsmedia_commonPhysicsHurst exponent[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]AutocorrelationAstrophysics (astro-ph)Instrumentation and Detectors (physics.ins-det)Computational physicsExponential functionOrders of magnitude (time)
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The Baryon Oscillation Spectroscopic Survey of SDSS-III

2012

The Baryon Oscillation Spectroscopic Survey (BOSS) is designed to measure the scale of baryon acoustic oscillations (BAO) in the clustering of matter over a larger volume than the combined efforts of all previous spectroscopic surveys of large-scale structure. BOSS uses 1.5 million luminous galaxies as faint as i = 19.9 over 10,000 deg(2) to measure BAO to redshifts z < 0.7. Observations of neutral hydrogen in the Ly alpha forest in more than 150,000 quasar spectra (g < 22) will constrain BAO over the redshift range 2.15 < z < 3.5. Early results from BOSS include the first detection of the large-scale three-dimensional clustering of the Ly alpha forest and a strong detection from the Data R…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSurveysAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Settore FIS/05 - Astronomia e AstrofisicaObservacions astronòmiques0103 physical sciencesPhysical Sciences and Mathematicsobservations [Cosmology]010303 astronomy & astrophysicsObservationsAstrophysics::Galaxy AstrophysicsPhysicsCosmologia010308 nuclear & particles physicsAngular diameter distanceAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsQuasarCosmology and Extragalactic AstrophysicsLyman-alpha forestRedshiftGalaxyCosmologyBaryonBossSpace and Planetary ScienceAstronomiaBaryon acoustic oscillationsAstronomical observationsAstrophysics - Cosmology and Nongalactic Astrophysics
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 9 Spectroscopic …

2012

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2012 RAS © 2012 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

AstrofísicaCosmology and GravitationCosmology and Nongalactic Astrophysics (astro-ph.CO)Large-scale structure of Universe[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Cosmological parametersFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsEnergia fosca (Astronomia)Astrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Measurement of distancesObservacions astronòmiquesDark energy0103 physical sciencesobservations [Cosmology]Dark energy (Astronomy)010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics/dk/atira/pure/core/subjects/cosmologyDistance scaleCosmologia010308 nuclear & particles physicsCosmology: observationsFísicaAstronomy and AstrophysicsCosmology and Extragalactic AstrophysicsCosmologyMesurament de les distànciesSpace and Planetary Science[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic AstrophysicsAstronomical observations
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Euclid preparation XV. Forecasting cosmological constraints for the Euclid and CMB joint analysis

2022

The combination and cross-correlation of the upcoming $Euclid$ data with cosmic microwave background (CMB) measurements is a source of great expectation since it will provide the largest lever arm of epochs, ranging from recombination to structure formation across the entire past light cone. In this work, we present forecasts for the joint analysis of $Euclid$ and CMB data on the cosmological parameters of the standard cosmological model and some of its extensions. This work expands and complements the recently published forecasts based on $Euclid$-specific probes, namely galaxy clustering, weak lensing, and their cross-correlation. With some assumptions on the specifications of current and…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmic microwave backgroundstatistical [methods]FOS: Physical sciencesAstrophysicscosmic background radiationAstrophysics::Cosmology and Extragalactic AstrophysicsJoint analysiskosmologia01 natural sciencesmethodsNOpimeä aine[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]mikroaallotSettore FIS/05 - Astronomia e Astrofisicasurveys0103 physical sciencestszsurvey010303 astronomy & astrophysicsPhysicsmethods: statistical010308 nuclear & particles physicsComputer Science::Information RetrievalmaailmankaikkeusAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicscross-correlation115 Astronomy Space scienceCosmic background radiation; Large-scale structure of Universe; Methods: statistical; Surveyskosminen taustasäteilySpace and Planetary Sciencemethodlarge-scale structure of Universepimeä energia[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]statisticalAstrophysics - Cosmology and Nongalactic Astrophysics
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Assessing the potential long-term increase of oceanic fossil fuel CO2 uptake due to CO2-calcification feedback

2007

International audience; Plankton manipulation experiments exhibit a wide range of sensitivities of biogenic calcification to simulated anthropogenic acidification of the ocean, with the "lab rat" of planktic calcifiers, Emiliania huxleyi apparently not representative of calcification generally. We assess the implications of this observational uncertainty by creating an ensemble of realizations of an Earth system model that encapsulates a comparable range of uncertainty in calcification response to ocean acidification. We predict that a substantial reduction in marine carbonate production is possible in the future, with enhanced ocean CO2 sequestration across the model ensemble driving a 4?1…

[ SDU.OCEAN ] Sciences of the Universe [physics]/Ocean Atmosphere[SDU.OCEAN] Sciences of the Universe [physics]/Ocean Atmospherelcsh:QE1-996.5fungilcsh:Life[ SDU.STU ] Sciences of the Universe [physics]/Earth Sciences[SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph][ PHYS.ASTR.CO ] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO][SDU.ENVI] Sciences of the Universe [physics]/Continental interfaces environmentlcsh:Geologylcsh:QH501-531[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]lcsh:QH540-549.5[SDU.STU] Sciences of the Universe [physics]/Earth Sciences[ SDU.ENVI ] Sciences of the Universe [physics]/Continental interfaces environmentlcsh:Ecology[ SDU.ASTR ] Sciences of the Universe [physics]/Astrophysics [astro-ph]
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Decoherence in supernova neutrino transformations suppressed by deleptonization

2007

16 pages, 12 figures.-- PACS nrs.: 14.60.Pq; 97.60.Bw.-- ISI Article Identifier: 000251987300100.-- ArXiv pre-print available at: http://arxiv.org/abs/0706.2498

HistoryParticle physicsNuclear and High Energy PhysicsQuantum decoherence[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and Detectorsmedia_common.quotation_subjectHigh Energy Physics::LatticeAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences[PACS] Supernovae[PACS] Neutrino mass and mixingAstrophysicsAsymmetryMeasure (mathematics)01 natural sciences7. Clean energyEarly UniverseStandard ModelEducationLuminosity[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesInvariant massddc:530High Energy Physics010306 general physicsMixing (physics)media_commonPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)High Energy Physics::PhenomenologyFísicaWeinberg angleFunction (mathematics)Atomic and Molecular Physics and OpticsComputer Science Applications3. Good healthSupernovaHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]PhenomenologyHigh Energy Physics::ExperimentNeutrino
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Microbiology and atmospheric processes: biological, physical and chemical characterization of aerosol particles

2008

Abstract. The interest in bioaerosols has traditionally been linked to health hazards for humans, animals and plants. However, several components of bioaerosols exhibit physical properties of great significance for cloud processes, such as ice nucleation and cloud condensation. To gain a better understanding of their influence on climate, it is therefore important to determine the composition, concentration, seasonal fluctuation, regional diversity and evolution of bioaerosols. In this paper, we will review briefly the existing techniques for detection, quantification, physical and chemical analysis of biological particles, attempting to bridge physical, chemical and biological methods for …

010504 meteorology & atmospheric sciencesIndoor bioaerosollcsh:LifeBiological particles[SDU.STU]Sciences of the Universe [physics]/Earth SciencesNanotechnology[SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph]01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]03 medical and health scienceslcsh:QH540-549.5[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces environmentEcology Evolution Behavior and Systematics0105 earth and related environmental sciencesEarth-Surface Processes[SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmosphere0303 health sciences[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.OCEAN] Sciences of the Universe [physics]/Ocean Atmosphere030306 microbiologyChemistrylcsh:QE1-996.5[SDU.ENVI] Sciences of the Universe [physics]/Continental interfaces environmentAerosolCharacterization (materials science)lcsh:Geologylcsh:QH501-531[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]13. Climate action[SDU.STU] Sciences of the Universe [physics]/Earth SciencesIce nucleuslcsh:EcologyBiochemical engineeringAerosol sampling
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