0000000000980384

AUTHOR

Stelzer B.

showing 3 related works from this author

Search for Magnetic Monopoles and Stable High-Electric-Charge Objects in 13 Tev Proton-Proton Collisions with the ATLAS Detector

2020

We thank CERN for the very successful operation of the LHC, aswell as the support staff fromour institutionswithout whom ATLAS could not be operated efficiently. We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; FWF, BMWFW, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq, FAPESP, Brazil; NSERC, CFI, NRC, Canada; CERN; CONICYT, Chile; CAS, NSFC, MOST, China; COLCIENCIAS, Colombia; VSC CR, MSMT CR, MPO CR, Czech Republic; DNSRC, DNRF, Denmark; IN2P3-CNRS, CEA-DRF/IRFU, France; SRNSFG, Georgia; MPG, HGF, BMBF, Germany; GSRT, Greece; RGC, Hong Kong SAR, Hong Kong China; Benoziyo Center, ISF, Israel; INFN, Italy; JSPS, MEXT, Japan; JINR; CNRST, Morocco; NWO, Nether…

electric [charge]Drell-Yan process:Kjerne- og elementærpartikkelfysikk: 431 [VDP]Magnetic monopolesProton13000 GeV-cmsPhysics::Instrumentation and Detectorselectromagnetic [calorimeter]magnetic [charge]General Physics and Astronomy7. Clean energy01 natural scienceschannel cross section: upper limitHigh Energy Physics - Experimentmagnetic monopole: massSubatomär fysikparticle: stabilityHigh Energy Physics - Experiment (hep-ex)magnetic monopole: pair productionSubatomic Physicsscattering [p p][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]tracking detectorstability [particle]0 [spin]1/2 [spin]Particle productionHadron collidersPhysicsRange (particle radiation)Large Hadron Colliderupper limit [channel cross section]DetectorSettore FIS/01 - Fisica Sperimentalemass [magnetic monopole]ATLAS3. Good health:Nuclear and elementary particle physics: 431 [VDP]CERN LHC Collhigh [ionization]ATLAS Detectorslower limit [mass]atlas; lhc; higgs;colliding beams [p p]pair production [magnetic monopole]Particle Physics - ExperimentsignatureDirect Productionp p: scatteringHigh-Ionizationdirect production [magnetic monopole]530 PhysicsCiências Naturais::Ciências Físicasmass: lower limit:Ciências Físicas [Ciências Naturais]Magnetic monopolespin: 0FOS: Physical sciencesLHC ATLAS High Energy Physicsddc:500.2Electromagnetic CalorimeterElectric chargeComputer Science::Digital LibrariesChargeNuclear physicsionization: high0103 physical sciencesTransition Radiation Trackersddc:530High Energy Physicsspin: 1/2010306 general physicsCiencias ExactasATLAS Collaborationcharge: magneticmagnetic monopolesS028CScience & Technologyhep-excharge: electricFísicaCharge (physics)triggerPair productioncalorimeter: electromagneticProton Proton CollisionsExperimental High Energy PhysicsMagnetic ChargesElementary Particles and FieldsHigh Energy Physics::Experimenttransition radiationHadron-hadron collisionsp p: colliding beamsmagnetic monopole: direct productionexperimental resultsPhysical Review Letters
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XMM-Newton Extended Survey of Taurus

2007

The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST) surveys the most populated ~5 square degrees of the Taurus Molecular Cloud, using the XMM-Newton X-ray observatory to study the thermal structure, variability, and long-term evolution of hot plasma, to investigate the magnetic dynamo, and to search for new potential members of the association. We present overall correlations with fundamental stellar parameters that were derived from the previous literature. The present overview paper introduces the project and provides the basic results from the X-ray analysis of all sources detected in the XEST survey. Comprehensive tables summarize the stellar properties of all targets su…

Astrophysics and AstronomyStellar associationsPhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSurveysX-ray sourcesComputer Science::Digital Librariesobservational astronomyPre main sequence starsX ray sourcesStellar AstronomyAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsNatural SciencesPre-main sequence starscosmologyAstrophysics::Galaxy Astrophysics
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Activity and accretion in {gamma} Vel and Cha I

2015

We use the fundamental parameters (effective temperature, surface gravity, lithium abundance, and radial velocity) delivered by the GES consortium in the first internal data release to select the members of Gamma Vel and Cha I among the UVES and GIRAFFE spectroscopic observations. A total of 140 Gamma Vel members and 74 Cha I members were studied. The procedure adopted by the GES to derive stellar fundamental parameters provided also measures of the projected rotational velocity (vsini). We calculated stellar luminosities through spectral energy distributions, while stellar masses were derived by comparison with evolutionary tracks. The spectral subtraction of low-activity and slowly rotati…

Astrophysics and AstronomyRadial velocityAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsobservational astronomyOpen star clustersPre main sequence starsExoplanet AstronomyStellar AstronomyAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsNatural SciencesPre-main sequence starsLine intensitiesAstrophysics::Galaxy Astrophysics
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