Search results for "TELESCOPE"

showing 10 items of 499 documents

Multiband variability studies and novel broadband SED modeling of Mrk 501 in 2009

2017

Astronomy and astrophysics 603, A31 (2017). doi:10.1051/0004-6361/201629540

extragalactic background lightmultiwavelength observationsAstrophysics::High Energy Astrophysical Phenomenabl-lacertae objectsGalaxies: BL Lacertae objects: individual: Markarian 501 ; Methods: data analysis ; observational ; Polarizationspectral energy-distributionFluxFOS: Physical sciencesAstrophysics01 natural scienceslaw.inventionindividual: Markarian 501 [BL Lacertae objects]lawCoincident0103 physical sciencesddc:530MAGIC (telescope)crab-nebulaBlazardata analysis [Methods]010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)tev blazars010308 nuclear & particles physicsstochastic accelerationtelescope observationsInstitut für Physik und AstronomieAstronomy and AstrophysicsAstronomy and Astrophysicgamma-ray emissionmethods: data analysis520BL Lacertae objects: individual: Markarian 501; Methods: data analysisSynchrotrondata analysi [Methods]BL Lacertae objects: individual: Markarian 501; Methods: data analysis; Astronomy and Astrophysics; Space and Planetary ScienceBL Lacertae objects: individual: Markarian 501x-raySpace and Planetary Scienceddc:520ElectrónicaFísica nuclearElectricidadDegeneracy (mathematics)Astrophysics - High Energy Astrophysical PhenomenaFlareBL Lac object
researchProduct

Flat bands and strongly correlated Fermi systems

2019

Many strongly correlated Fermi systems including heavy-fermion (HF) metals and high-Tc superconductors belong to that class of quantum many-body systems for which Landau Fermiliquid (LFL) theory fails. Instead, these systems exhibit non-Fermi-liquid properties that arise from violation of time-reversal (T) and particle-hole (C) invariance. Measurements of tunneling conductance provide a powerful experimental tool for detecting violations of these basic symmetries inherent to LFLs, which guarantee that the measured differential conductivity dI/dV, where I is the current and V the bias voltage, is a symmetric function of V. Thus, it has been predicted that the conductivity becomes asymmetric …

flat bandsPhysicstunneling conductanceTunneling conductancestrongly correlated Fermi systemsCondensed matter physicsCondensed Matter PhysicsMathematical PhysicsAtomic and Molecular Physics and OpticsFermi Gamma-ray Space TelescopePhysica Scripta
researchProduct

Unveiling the environment and faint features of the isolated galaxy CIG 96 with deep optical and HI observations

2018

Context. Asymmetries in atomic hydrogen (HI) in galaxies are often caused by the interaction with close companions, making isolated galaxies an ideal framework to study secular evolution. The AMIGA project has demonstrated that isolated galaxies show the lowest level of asymmetry in their HI integrated profiles compared to even field galaxies, yet some present significant asymmetries. CIG 96 (NGC 864) is a representative case reaching a 16% level. Aims. Our aim is to investigate the HI asymmetries of the spiral galaxy CIG 96 and what processes have triggered the star-forming regions observed in the XUV pseudo-ring. Methods. We performed deep optical observations at CAHA1.23m, CAHA2.2m and V…

galaxies: spiralHIERARCHICAL SATELLITE ACCRETIONmedia_common.quotation_subjectFOS: Physical sciencesAstrophysicsI.01 natural sciences7. Clean energyAsymmetryAMIGA SAMPLElaw.inventionTelescopelaw0103 physical scienceskinematics and dynamics [galaxies]DARK-MATTER SUBSTRUCTURESurface brightness010303 astronomy & astrophysicsStellar evolutionComputingMilieux_MISCELLANEOUSevolution [galaxies]galaxies: kinematics and dynamicsLOPSIDED SPIRAL GALAXIESmedia_commonindividual: NGC 864 [galaxies]Physicsradio lines: galaxiesSpiral galaxy010308 nuclear & particles physicsgalaxies: individual: NGC864Astronomy and AstrophysicsDISK GALAXIESAstrophysics - Astrophysics of GalaxiesAccretion (astrophysics)Galaxygalaxies [radio lines]RINGSTIDAL STREAMspiral [galaxies][SDU]Sciences of the Universe [physics]Space and Planetary ScienceGASAstrophysics of Galaxies (astro-ph.GA)structure [galaxies]galaxies: structureDIGITAL SKY SURVEYCirrusGalaxies: Individual: NGC 864galaxies: evolutionAstronomy & astrophysics
researchProduct

Faint γ-ray sources at low redshift: the radio galaxy IC 1531

2018

We present amultiwavelength study of IC 1531 (z=0.02564), an extragalactic radio source associated with the γ -ray object 3FGL J0009.9-3206 and classified as a blazar of uncertain type in the Third Fermi-Large Area Telescope AGN catalog (3LAC). A core-jet structure, visible in radio and X-rays, is enclosed within a ~220 kpc wide radio structure. The morphology and spectral characteristics of the kiloparsec jet in radio and X-rays are typical of Fanaroff-Riley type I galaxies. The analysis of the radio data and optical spectrum and different diagnostic methods based on the optical, infrared, and γ -ray luminosities also support a classification as a low-power RG seen at moderate angles (θ = …

gamma-rays: galaxiesRadio galaxyInfraredGamma-rays: galaxieAstrophysics::High Energy Astrophysical Phenomenagalaxies: activejets [galaxies]AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxies: jet01 natural sciencesRadio continuum: galaxielaw.inventionTelescopelaw0103 physical sciencesBlazargalaxies: individual: IC 1531010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsradio continuum: galaxies010308 nuclear & particles physicsAstronomy and AstrophysicsAstronomy and Astrophysicgalaxies: jetsGalaxyRedshiftgalaxies [radio continuum]galaxies [gamma-rays]Space and Planetary Scienceactive [galaxies]individual: ic 1531 [galaxies]Spectral energy distributionAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Fermi Gamma-ray Space Telescope
researchProduct

Design and performance of the prototype Schwarzschild-Couder telescope camera

2022

Journal of astronomical telescopes, instruments, and systems 8(01), 014007-1 (2022). doi:10.1117/1.JATIS.8.1.014007

imaging atmospheric Cherenkov telescopesinstrumentationPhysics - Instrumentation and Detectorsvery-high-energy gamma-ray astronomyPhysics::Instrumentation and DetectorsMechanical EngineeringSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)530Electronic Optical and Magnetic MaterialsCherenkov telescope arraySpace and Planetary ScienceControl and Systems Engineeringddc:530prototype Schwarzschild-Couder telescopeAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)silicon photomultipliers
researchProduct

The WEBT BL Lacertae Campaign 2001 and its extension : Optical light curves and colour analysis 1994–2002

2004

BL Lacertae has been the target of four observing campaigns by the Whole Earth Blazar Telescope (WEBT) collaboration. In this paper we present UBVRI light curves obtained by theWEBT from 1994 to 2002, including the last, extended BL Lac 2001 campaign. A total of about 7500 optical observations performed by 31 telescopes from Japan to Mexico have been collected, to be added to the ∼15 600 observations of the BL Lac Campaign 2000. All these data allow one to follow the source optical emission behaviour with unprecedented detail. The analysis of the colour indices reveals that the flux variability can be interpreted in terms of two components: longer-term variations occurring on a fewday time …

jetsAstrophysics::High Energy Astrophysical PhenomenaFluxScale (descriptive set theory)activeAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA01 natural sciencesPower lawlaw.inventionTelescopesymbols.namesakelawBL Lac objects0103 physical sciencesJetsBlazar010303 astronomy & astrophysicsQuasarsAstrophysics::Galaxy AstrophysicsPhysicsactive; galaxies: BL Lacertae objects: general; galaxies: jets; galaxies: quasars: general010308 nuclear & particles physicsActive galaxies ; BL Lacertae objects ; Jets ; Quasarsactive galaxiesAstronomy and AstrophysicsDecoupling (cosmology)galaxies: jetsLight curve:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]galaxies: quasars: generalSpace and Planetary Scienceactive galaxies; BL Lac objects; jetssymbolsgalaxies: BL Lacertae objects: generalActive galaxiesBL Lacertae objectsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaDoppler effect:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
researchProduct

BALDONE SCHMIDT (LATVIA) TELESCOPE ASTROPHOTOS ARCHIVE

2016

From 1967 to 2005, many astrophotos have been taken with the Baldone Schmidt telescope (80cmx120cmx240cm). These photos have being archived in theInstituteofAstronomyof theUniversityofLatvia(IAU code 069, longitude 24.4041 E, latitude 56.7734 N, altitude103 m). There are over 22000 direct and 2300 spectral photos of different regions of the sky in this archive. There are also information on the photo materials type as well as the types of color filters used for phographiing the sky fields and objects. The home page of theInstituteofAstronomy’s Baldone observatory (www.baldoneobservatory.lu.lv) has the archive’s description. Part of the description has also being published (Alksnis, et al., …

lcsh:Astronomymedia_common.quotation_subjectAstronomySchmidt cameralaw.inventionlcsh:QB1-991TelescopeSchmidt telescope; wide field plate archiveGeographylawObservatorySkyLongitudeRemote sensingmedia_commonOdessa Astronomical Publications
researchProduct

Design and development of safety and control systems in ATLAS

2021

El gran colisionador de hadrones, o LHC, es el acelerador de partículas más grande y potente del mundo. Ha sido construido por el CERN, la Organización Europea para la Investigación Nuclear, entre 1998 y 2008 en Ginebra, Suiza. Sucesivas mejoras en el LHC supondrán a partir de mediados del 2027 un incremento de la luminosidad, cuando pasará a llamarse High Luminosity LHC (HL-LHC). Esta tesis se divide en dos partes, por una parte la seguridad y operación de la infraestructura y por otra los sistemas de control y toma de datos. La primera parte de la tesis se dedica a la seguridad y operación de la infraestructura. Después de más de 10 años de funcionamiento, el riesgo de posibles fallos en …

leak detectionhadiation hardness:CIENCIAS TECNOLÓGICAS [UNESCO]CMOSexpert systemsLHCDetectors and Experimental TechniquesATLASUNESCO::CIENCIAS TECNOLÓGICASbeam telescopeSEU
researchProduct

SPI/INTEGRAL in-flight performance

2003

The SPI instrument has been launched on-board the INTEGRAL observatory on October 17, 2002. SPI is a spectrometer devoted to the sky observation in the 20 keV-8 MeV energy range using 19 germanium detectors. The performance of the cryogenic system is nominal and allows to cool the 19 kg of germanium down to 85 K with a comfortable margin. The energy resolution of the whole camera is 2.5 keV at 1.1 MeV. This resolution degrades with time due to particle irradiation in space. We show that the annealing process allows the recovery of the initial performance. The anticoincidence shield works as expected, with a low threshold at 75 keV, reducing the GeD background by a factor of 20. The digital …

media_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical scienceschemistry.chemical_elementGermaniumAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsGamma-rayObservatoryinstrument observations [gamma-ray]Observationsmedia_commonPhysicsSpectrometerINTEGRAL/SPIAstrophysics (astro-ph)DetectorAstronomy and AstrophysicsInstrumentDead timeGalactic planeINTEGRAL/SPI [space telescope]:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Gamma-ray ; Instrument ; Observations ; Space telescope ; INTEGRAL/SPIComputational physicsCrab NebulachemistrySpace and Planetary ScienceSkySpace telescopeUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
researchProduct

The ALHAMBRA survey: Bayesian photometric redshifts with 23 bands for 3 deg2

2014

A. Molino et al.

media_common.quotation_subjectPhotometric systemAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSurveyslaw.inventionPhotometry (optics)Telescopelawdistances and redshifts [Galaxies]Astrophysics::Solar and Stellar Astrophysicsdata analysis [Methods]Astrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSPhotometric redshiftmedia_commonPhysics[PHYS]Physics [physics]photometry [Galaxies]photometric [Techniques]Astrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstronomy and AstrophysicsCataloguesevolution [Galaxies]GalaxyRedshift13. Climate actionSpace and Planetary ScienceSkyMagnitude (astronomy)Astrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
researchProduct