Search results for " Instrumentation."

showing 10 items of 712 documents

Euclid Preparation. XIV. The Complete Calibration of the Color–Redshift Relation (C3R2) Survey: Data Release 3

2021

Stanford, S. A., et al.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Calibration (statistics)FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsColor space217101 natural sciencesCosmologyLarge-scale structure010309 optics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]galaxy spectroscopySettore FIS/05 - Astronomia e AstrofisicaSpitzer Space Telescope0103 physical sciencesDISTRIBUTIONSAstrophysics::Solar and Stellar AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)PHOTOMETRIC REDSHIFTS010303 astronomy & astrophysicsWeak gravitational lensingAstrophysics::Galaxy AstrophysicsPhysicsHardware_MEMORYSTRUCTURESAstrophysics::Instrumentation and Methods for AstrophysicsEuclidAstronomy and AstrophysicsRedshiftGalaxyCosmologySpace and Planetary ScienceGalaxy spectroscopyDark energyAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Limits on spin-dependent WIMP-nucleon cross sections from 225 live days of XENON100 data

2013

We present new experimental constraints on the elastic, spin-dependent WIMP-nucleon cross section using recent data from the XENON100 experiment, operated in the Laboratori Nazionali del Gran Sasso in Italy. An analysis of 224.6 live days x 34 kg of exposure acquired during 2011 and 2012 revealed no excess signal due to axial-vector WIMP interactions with 129-Xe and 131-Xe nuclei. This leads to the most stringent upper limits on WIMP-neutron cross sections for WIMP masses above 6 GeV, with a minimum cross section of 3.5 x 10^{-40} cm^2 at a WIMP mass of 45 GeV, at 90% confidence level.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Dark matterGeneral Physics and AstronomyFOS: Physical sciences01 natural sciencesdark matterParticle detectorHigh Energy Physics - ExperimentNuclear physicsCross section (physics)High Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsPseudovectorInstrumentation and Methods for Astrophysics (astro-ph.IM)Spin-½Physics010308 nuclear & particles physics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]High Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Astrophysics - Instrumentation and Methods for AstrophysicsNucleonAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

The miniJPAS survey: a preview of the Universe in 56 colours

2021

Full list of authors: Bonoli, S.; Marín-Franch, A.; Varela, J.; Vázquez Ramió, H.; Abramo, L. R.; Cenarro, A. J.; Dupke, R. A.; Vílchez, J. M.; Cristóbal-Hornillos, D.; González Delgado, R. M.; Hernández-Monteagudo, C.; López-Sanjuan, C.; Muniesa, D. J.; Civera, T.; Ederoclite, A.; Hernán-Caballero, A.; Marra, V.; Baqui, P. O.; Cortesi, A.; Cypriano, E. S.; Daflon, S.; de Amorim, A. L.; Díaz-García, L. A.; Diego, J. M.; Martínez-Solaeche, G.; Pérez, E.; Placco, V. M.; Prada, F.; Queiroz, C.; Alcaniz, J.; Alvarez-Candal, A.; Cepa, J.; Maroto, A. L.; Roig, F.; Siffert, B. B.; Taylor, K.; Benitez, N.; Moles, M.; Sodré, L.; Carneiro, S.; Mendes de Oliveira, C.; Abdalla, E.; Angulo, R. E.; Apari…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectFOS: Physical sciencesAstrophysicsastronomical databases: miscellaneousSurveyslaw.inventionPhotometry (optics)Telescopetechniques: photometricExtended Groth StripsurveysObservatorylaw[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]observations [Cosmology]Instrumentation and Methods for Astrophysics (astro-ph.IM)stars: generalmedia_commonPhysicsgeneral [Stars]photometric [Techniques]Astronomy and AstrophysicsQuasargeneral [Galaxies]115 Astronomy Space sciencegalaxies: generalAstrophysics - Astrophysics of GalaxiesGalaxyRedshiftSpace and Planetary ScienceSkyAstrophysics of Galaxies (astro-ph.GA)cosmology: observationsmiscellaneous [Astronomical databases][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Removing krypton from xenon by cryogenic distillation to the ppq level

2017

The XENON1T experiment aims for the direct detection of dark matter in a detector filled with 3.3 tons of liquid xenon. In order to achieve the desired sensitivity, the background induced by radioactive decays inside the detector has to be sufficiently low. One major contributor is the β-emitter 85Kr which is present in the xenon. For XENON1T a concentration of natural krypton in xenon natKr/Xe<200ppq (parts per quadrillion, 1ppq=10-15mol/mol) is required. In this work, the design, construction and test of a novel cryogenic distillation column using the common McCabe–Thiele approach is described. The system demonstrated a krypton reduction factor of 6.4 · 10 5 with thermodynamic stability a…

CryostatPhysics - Instrumentation and DetectorsXenonPhysics and Astronomy (miscellaneous)WIMPDark matterAnalytical chemistryFOS: Physical scienceschemistry.chemical_elementlcsh:AstrophysicsWeakly Interact Massive ParticleSciences de l'ingénieur01 natural sciences7. Clean energyXenonlcsh:QB460-4660103 physical sciencesDark Matterlcsh:Nuclear and particle physics. Atomic energy. RadioactivitySensitivity (control systems)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsComputer science information & general worksEngineering (miscellaneous)Liquid XenonComputingMilieux_MISCELLANEOUSPhysicsAir separationPhysique010308 nuclear & particles physicsDistillation ColumnKryptonKryptonOrder (ring theory)Instrumentation and Detectors (physics.ins-det)AstronomiechemistryDirect Searchddc:000lcsh:QC770-798TPCOrder of magnitude
researchProduct

Timing techniques applied to distributed modular high-energy astronomy: the H.E.R.M.E.S. project

2021

The HERMES-TP/SP (High Energy Rapid Modular Ensemble of Satellites -- Technologic and Scientific Pathfinder) is an in-orbit demonstration of the so-called distributed astronomy concept. Conceived as a mini-constellation of six 3U nano-satellites hosting a new miniaturized detector, HERMES-TP/SP aims at the detection and accurate localisation of bright high-energy transients such as Gamma-Ray Bursts. The large energy band, the excellent temporal resolution and the wide field of view that characterize the detectors of the constellation represent the key features for the next generation high-energy all-sky monitor with good localisation capabilities that will play a pivotal role in the future …

CubeSatsHigh energyHigh-energy astronomyReal-time computingFOS: Physical sciences01 natural sciences7. Clean energy010309 opticsX-rays0103 physical sciencesNano-satellitesTemporal triangulationInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsConstellationHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsbusiness.industryDetectorAstrophysics::Instrumentation and Methods for AstrophysicsModular designPathfinderTemporal resolutionGamma Ray BurstsTransient (oscillation)Astrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsbusinessSpace Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray
researchProduct

The HERMES-Technologic and Scientific Pathfinder

2020

HERMES-TP/SP (High Energy Rapid Modular Ensemble of Satellites Technologic and Scientific Pathfinder) is a constellation of six 3U nano-satellites hosting simple but innovative X-ray detectors, characterized by a large energy band and excellent temporal resolution, and thus optimized for the monitoring of Cosmic High Energy transients such as Gamma Ray Bursts and the electromagnetic counterparts of Gravitational Wave Events, and for the determination of their positions. The projects are funded by the Italian Ministry of University and Research and by the Italian Space Agency, and by the European Union Horizon 2020 Research and Innovation Program under Grant Agreement No. 821896. HERMES-TP/S…

CubeSatsmedia_common.quotation_subjectCubeSats; Gamma Ray Bursts; Nano-satellites; X-raysFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyAstrophysics - Instrumentation and MethodsSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesX-raysmedia_common.cataloged_instanceEuropean unionAerospace engineeringNano-satellites010306 general physics010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)media_commonConstellationPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)COSMIC cancer databasebusiness.industryGravitational waveModular designPathfinderSkyTemporal resolutionGamma Ray BurstsbusinessAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysics
researchProduct

Gas cell studies of thorium using filament dispensers at IGISOL

2020

Abstract Filament-based dispensers of thorium have been investigated at the IGISOL facility, Jyvaskyla, for potential use as a thorium ion source for future collinear laser spectroscopy experiments. Several different filaments were manufactured in the Institute of Atomic and Subatomic Physics of TU Wien, with 232Th and 229Th prepared on tantalum substrates either by drying thorium nitrate solution or via molecular plating, while adding a layer of zirconium for oxide reduction. The filaments were characterized in a helium-filled gas cell by performing selective and efficient in-gas-cell resonance laser ionization and by analyzing the resulting ion beams by mass spectrometry. Additionally, th…

DECOMPOSITIONNuclear and High Energy PhysicsTechnologyEFFICIENCYAnalytical chemistrychemistry.chemical_elementOFF-LINEPhysics Atomic Molecular & ChemicalMass spectrometry01 natural sciencesIonlaw.inventionProtein filamentlawIonization0103 physical sciences010306 general physicsNuclear Science & TechnologyLANTHANIDEInstrumentationInstruments & InstrumentationRESONANCE IONIZATIONScience & TechnologySPECTROSCOPYResonance laser ionization010308 nuclear & particles physicsPhysicsThoriumThoriumLASER ION-SOURCEActinideLaserIon sourceIon sourceWORK-FUNCTIONSPhysics NuclearchemistryACTINIDE ELEMENTSPhysical SciencesGas cellTRANSITION
researchProduct

FRIPON: a worldwide network to track incoming meteoroids

2020

Context. Until recently, camera networks designed for monitoring fireballs worldwide were not fully automated, implying that in case of a meteorite fall, the recovery campaign was rarely immediate. This was an important limiting factor as the most fragile - hence precious - meteorites must be recovered rapidly to avoid their alteration. Aims. The Fireball Recovery and InterPlanetary Observation Network (FRIPON) scientific project was designed to overcome this limitation. This network comprises a fully automated camera and radio network deployed over a significant fraction of western Europe and a small fraction of Canada. As of today, it consists of 150 cameras and 25 European radio receiver…

DYNAMICS[INFO.INFO-AR]Computer Science [cs]/Hardware Architecture [cs.AR]MeteorsComputer scienceRadio receiver[INFO.INFO-DM]Computer Science [cs]/Discrete Mathematics [cs.DM]Surveys010502 geochemistry & geophysicsTrack (rail transport)01 natural sciencesMeteorites meteors meteoroidslaw.inventionPlanets and planetary system[INFO.INFO-TS]Computer Science [cs]/Signal and Image ProcessingMethods: observationallaw[INFO.INFO-RB]Computer Science [cs]/Robotics [cs.RO]meteoroids010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSObservational methodsEarth and Planetary Astrophysics (astro-ph.EP)meteoroids -surveys -methods: observational -interplanetary medium[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]ORIGIN[INFO.INFO-AO]Computer Science [cs]/Computer Arithmeticmeteorites meteors meteoroids – surveys – methods: observational – interplanetary mediumMeteoroidsRECOVERYORBITMeteoriteFully automatedInterplanetary medium; Meteorites meteors meteoroids; Methods: observational; Surveys[INFO.INFO-TI]Computer Science [cs]/Image Processing [eess.IV][INFO.INFO-DC]Computer Science [cs]/Distributed Parallel and Cluster Computing [cs.DC]Astrophysics - Instrumentation and Methods for Astrophysics[SPI.SIGNAL]Engineering Sciences [physics]/Signal and Image processingFLUXReal-time computingfripon[INFO.INFO-DS]Computer Science [cs]/Data Structures and Algorithms [cs.DS]FOS: Physical sciencesContext (language use)CAMERA[INFO.INFO-SE]Computer Science [cs]/Software Engineering [cs.SE][SPI.AUTO]Engineering Sciences [physics]/Automatic[SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology0103 physical sciencesFIREBALL NETWORKobservational [Methods]meteorsInstrumentation and Methods for Astrophysics (astro-ph.IM)0105 earth and related environmental sciencesMeteoroidINNISFREE METEORITE[INFO.INFO-CV]Computer Science [cs]/Computer Vision and Pattern Recognition [cs.CV]Astronomy and AstrophysicsMETEORITE FALLMeteorites meteors meteoroidCamera networkSpace and Planetary Science[SDU]Sciences of the Universe [physics]Interplanetary spaceflightmeteroids trackingmeteoroids - surveys - methods: observationalSYSTEMInterplanetary mediumAstrophysics - Earth and Planetary AstrophysicsMeteorites
researchProduct

Search for Event Rate Modulation in XENON100 Electronic Recoil Data

2015

We have searched for periodic variations of the electronic recoil event rate in the (2-6) keV energy range recorded between February 2011 and March 2012 with the XENON100 detector, adding up to 224.6 live days in total. Following a detailed study to establish the stability of the detector and its background contributions during this run, we performed an un-binned profile likelihood analysis to identify any periodicity up to 500 days. We find a global significance of less than 1 sigma for all periods suggesting no statistically significant modulation in the data. While the local significance for an annual modulation is 2.8 sigma, the analysis of a multiple-scatter control sample and the phas…

Dark Matter Wimps ModulationPhysicsPhysics - Instrumentation and DetectorsCosmology and Nongalactic Astrophysics (astro-ph.CO)530 PhysicsDetectorDark matterPhase (waves)FOS: Physical sciencesGeneral Physics and AstronomySigmaInstrumentation and Detectors (physics.ins-det)AstrophysicsParticle detectorHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)RecoilModulation[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Event (particle physics)Astrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review Letters
researchProduct

Design of New Resonant Haloscopes in the Search for the Dark Matter Axion: A Review of the First Steps in the RADES Collaboration

2022

This article belongs to the Special Issue Studying the Universe from Spain.

Dark matter detectorsResonant cavitiesaxionsdark matter detectorsPhysics - Instrumentation and Detectorshep-exAxionsGeneral Physics and AstronomyFOS: Physical sciencesElementary particle physicsInstrumentation and Detectors (physics.ins-det)QC793-793.5HaloscopesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)haloscopesDetectors and Experimental Techniquesphysics.ins-detParticle Physics - Experimentresonant cavities
researchProduct