Search results for " Identification"

showing 10 items of 707 documents

GRO J1744-28: an intermediate B-field pulsar in a low mass X-ray binary

2015

The bursting pulsar, GRO J1744-28, went again in outburst after $\sim$18 years of quiescence in mid-January 2014. We studied the broad-band, persistent, X-ray spectrum using X-ray data from a XMM-Newton observation, performed almost at the peak of the outburst, and from a close INTEGRAL observation, performed 3 days later, thus covering the 1.3-70.0 keV band. The spectrum shows a complex continuum shape that cannot be modelled with standard high-mass X-ray pulsar models, nor by two-components models. We observe broadband and peaked residuals from 4 to 15 keV, and we propose a self-consistent interpretation of these residuals, assuming they are produced by cyclotron absorption features and b…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Stars: individual: GRO J1744-28 -X-rays: binarieLine: identificationAstrophysics::High Energy Astrophysical PhenomenaCyclotronX-ray binaryFOS: Physical sciencesLine: formationAstronomy and AstrophysicsAstrophysicsX-rays: generalMagnetic fieldlaw.inventionSettore FIS/05 - Astronomia E AstrofisicaPulsarSpace and Planetary SciencelawIonizationHarmonicsThermalAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaLow Mass
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Development of an Endcap DIRC for PANDA

2014

Abstract The aim of this research is to develop a planar DIRC detector showing advantages and performance similar to a classical, barrel shaped DIRC, but at smaller polar angles which cannot be accessed using a cylindrical geometry. The device will complement the PANDA Barrel DIRC by covering polar angles from 5° to 22°. The envisaged π /K-separation is ≥ 3 σ up to 4 GeV/c. A major challenge is the adaption of the device to the PANDA environment including a magnetic field of ~1–2 T, high rates and radiation, limited space for optics and sensors as well as the lack of a common first-level trigger. This paper discusses a detector design which forms a compromise between these constraints and a…

PhysicsHigh rateNuclear and High Energy PhysicsPhysics::Instrumentation and Detectorsbusiness.industryDetectorBarrel (horology)Reconstruction methodParticle identificationOpticsPlanarHigh Energy Physics::ExperimentDevelopment (differential geometry)businessInstrumentationCherenkov radiationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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The backward end-cap for the PANDA electromagnetic calorimeter

2015

The PANDA experiment at the new FAIR facility will cover a broad experimental programme in hadron structure and spectroscopy. As a multipurpose detector, the PANDA spectrometer needs to ensure almost 4π coverage of the scattering solid angle, full and accurate multiple-particle event reconstruction and very good particle identification capabilities. The electromagnetic calorimeter (EMC) will be a key item for many of these aspects. Particle energies ranging from some MeVs to several GeVs have to be measured with a relative resolution of 1% ⊕ 2%/√E/GeV . It will be a homogeneous calorimeter made of PbWO4 crystals and will be operated at -25°C, in order to improve the scintillation light yiel…

PhysicsHistoryScintillationSpectrometerCalorimeter (particle physics)APDSPhysics::Instrumentation and Detectorsbusiness.industryDetectorAvalanche photodiodeParticle identificationComputer Science ApplicationsEducationlaw.inventionNuclear physicsOpticslawNuclear ExperimentbusinessEvent reconstructionJournal of Physics: Conference Series
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ChandraObservation of Cir X‐1 near the Periastron Passage: Evidence for an X‐Ray Jet?

2008

We present the results of a 25 ks long Chandra observation of the peculiar source Cir X-1 near the periastron passage. We report precise X-ray coordinates of the source, which were compatible with the optical and radio counterpart coordinates. We focus on the study of the detected emission features using the High Energy Transmission Grating Spectrometer on board the Chandra satellite. We detect emission lines associated with Mg XII, Si XIII, Si XIV, S XV, S XVI, Ar XVII, Ar XVIII, Ca XIX, Ca XX, Fe XXV, and Fe XXVI, showing an average redshift of 470 km s-1. The most intense emission features can be fitted with two lines; this is more evident for the 6.6 keV emission feature, which shows a …

PhysicsJet (fluid)Line-of-sightSpectrometerX-rayX-ray binaryAstronomyAstronomy and AstrophysicsAstrophysicsRedshiftLine: Formation Line: Identification Stars: Individual: Constellation Name: Circinus X-1 X-Rays: Binaries X-Rays: GeneralSettore FIS/05 - Astronomia E AstrofisicaJet velocitySpace and Planetary ScienceEmission spectrumThe Astrophysical Journal
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Tests and developments of the PANDA Endcap Disc DIRC

2016

The PANDA experiment at the future Facility for Antiproton and Ion Research (FAIR) requires excellent particle identification. Two different DIRC detectors will utilize internally reflected Cherenkov light of charged particles to enable the separation of pions and kaons up to momenta of 4 GeV/c. The Endcap Disc DIRC will be placed in the forward endcap of PANDA's central spectrometer covering polar angles between 5° and 22°. Its final design is based on MCP-PMTs for the photon detection and an optical system made of fused silica. A new prototype has been investigated during a test beam at CERN in May 2015 and first results will be presented. In addition a new synthetic fused silica material…

PhysicsLarge Hadron ColliderSpectrometerPhysics::Instrumentation and Detectors010308 nuclear & particles physicsDetectorRadiation01 natural sciencesCharged particleParticle identificationNuclear physics0103 physical sciencesFacility for Antiproton and Ion ResearchHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsInstrumentationMathematical PhysicsCherenkov radiationJournal of Instrumentation
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A re-analysis of the NuSTAR and XMM-Newton broad-band spectrum of Serpens X-1

2017

Context. High-resolution X-ray spectra of neutron star low-mass X-ray binaries (LMXBs) in the energy range 6.4-6.97 keV are often characterized by the presence of K alpha transition features of iron at different ionization stages. Since these lines are thought to originate by reflection of the primary Comptonization spectrum over the accretion disk, the study of these features allows us to investigate the structure of the accretion flow close to the central source. Thus, the study of these features gives us important physical information on the system parameters and geometry. Ser X-1 is a well studied LMXB that clearly shows a broad iron line. Several attempts to fit this feature as a smear…

PhysicsLine-of-sight010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaContinuum (design consultancy)Astronomy and AstrophysicsContext (language use)RadiusAstrophysicsX-rays: general01 natural sciencesX-rays: binarieSpectral linestars: neutronQuality (physics)Reflection (mathematics)Settore FIS/05 - Astronomia E AstrofisicaSpace and Planetary Science0103 physical sciencesstars: individual: Serpens X-1formation; line: identification; stars: individual: Serpens X-1; stars: neutron; X-rays: binaries; X-rays: general [line]line: formation010303 astronomy & astrophysicsline: identificationLine (formation)
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Search for the decay B0→a1±ρ∓

2006

We present a search for the rare B-meson decay B-0 -> a(1)(+/-)rho(-/+) with a(1)(+/-)->pi(+)pi(-)pi(+/-). We use (110 +/- 1.2)x10(6) Upsilon(4S)-> B (B) over bar decays collected with the BABAR detector at the PEP-II asymmetric-energy B Factory at SLAC. We obtain an upper limit of 30x10(-6) (90%C.L.) for the branching fraction product B(B-0 -> a(1)(+/-)rho(-/+))B(a(1)(+/-)->pi(+)pi(-)pi(+/-)), where we assume that the a(1)(+/-) decays exclusively to rho(0)pi(+/-).

PhysicsNuclear and High Energy Physics/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energy010308 nuclear & particles physicsBranching fractionAnalytical chemistryParticle physicsBABAR detector01 natural sciencesParticle identificationHEPB-factoryNuclear physicsParticle decay0103 physical sciencesBaBarPiSDG 7 - Affordable and Clean Energy010306 general physicsFísica de partículesExperiments
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Search for the decayB+→K¯*0(892)K+

2007

We report on a search for the process B+ -> (K) over bar*(0)(892)K+ using 232 X 10(6) Y(4S) -> B (B) over bar B decays collected with the BABAR detector at the PEP-II asymmetric-energy B factory at SLAC. From a signal yield of 25 +/- 13[stat] +/- 7[syst] B+ -> (K) over bar*(0)(892)(-> K-pi(+))K+ events, we place an upper limit on the branching fraction B(B+ -> (K) over bar*(0)(892)K+) of 1.1 X 10(-6), at the 90% confidence level.

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsBranching fractionElectron–positron annihilation0103 physical sciencesAnalytical chemistry010306 general physics01 natural sciencesEngineering physicsParticle identificationB-factoryBar (unit)Physical Review D
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Measurement of branching fractions in radiativeBdecays toηKγand search forBdecays toη′Kγ

2006

We present measurements of the B ->eta K gamma branching fractions and upper limits for the B ->eta K-'gamma branching fractions. For B+->eta K+gamma we also measure the time-integrated charge asymmetry. The data sample, collected with the BABAR detector at the Stanford Linear Accelerator Center, represents 232x10(6) produced B (B) over bar pairs. The results for branching fractions and upper limits at 90% confidence level in units of 10(-6) are: B(B-0 ->eta K-0 gamma)=11.3(-2.6)(+2.8)+/- 0.6, B(B+->eta K+gamma)=10.0 +/- 1.3 +/- 0.5, B(B-0 ->eta K-'(0)gamma) eta K-'(+)gamma) eta K+gamma is A(ch)=-0.09 +/- 0.12 +/- 0.01. The first errors are statistical and the second systematic.

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsBranching fractionElectron–positron annihilationAnalytical chemistryBranching (polymer chemistry)01 natural sciencesParticle identificationParticle decay0103 physical sciencesRadiative transferCP violationAtomic physics010306 general physicsPhysical Review D
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Measurements of the branching fractions of chargedBdecays toK±π∓π±final states

2004

We present results of searches for B-meson decays to K+ pi- pi+ with the BaBar detector. With a data sample of 61.6 million BBbar pairs, we measure the branching fractions and 90% confidence-level upper limits averaged over charge-conjugate states (the first error is statistical and the second is systematic): B+ --> K*0 pi+ = (15.5 +/- 1.8 +1.5 -4.0) x 10^-6, B+ --> f0 K+, f_0 --> pi+ pi- = (9.2 +/- 1.2 +2.1 -2.6) x 10^-6, B+ --> D0bar pi+, D0bar --> K+ pi- = (184.6 +/- 3.2 +/- 9.7) x 10^-6. B+ --> rho K+ K+ pi- pi+ non-resonant < 17 x 10^-6.

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsBranching fractionElectron–positron annihilationAnalytical chemistryDalitz plotBranching (polymer chemistry)Resonance (chemistry)01 natural sciencesParticle identificationNuclear physicsParticle decay0103 physical sciencesPi010306 general physicsPhysical Review D
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