0000000001237305

AUTHOR

E. Amato

showing 6 related works from this author

Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants

2023

The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3~PeV. Sources which are capable of accelerating hadrons to such energies are called hadronic PeVatrons. However, hadronic PeVatrons have not yet been firmly identified within the Galaxy. Several source classes, including Galactic Supernova Remnants (SNRs), have been proposed as PeVatron candidates. The potential to search for hadronic PeVatrons with the Cherenkov Telescope Array (CTA) is assessed. The focus is on the usage of very high energy $\gamma$-ray spectral signatures for the identification of PeVatrons. Assuming that SNRs can accelerate CRs up to knee energies, the number of Galactic SNRs whi…

Cherenkov Telescope ArrayGamma rays: generalstatistical [methods]energy spectrumFOS: Physical sciencesVHESettore FIS/05 - Astronomia E Astrofisicacosmic raysMethods: data analysissupernovadata analysis [methods][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Cosmic raysInstrumentation and Methods for Astrophysics (astro-ph.IM)Cherenkov Telescope Arra ; alactic Supernova Remnants ; PeVatrons ;Methods: statisticalgalactic PeVatronsHigh Energy Astrophysical Phenomena (astro-ph.HE)emission spectrum) supernovae: general [(stars]Astronomy and AstrophysicssensitivityobservatoryGalactic PeVatronscosmic radiationspectralgalaxyhadron(Stars:) supernovae: generalAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]statisticalgeneral [gamma rays]signature
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XIPE: the x-ray imaging polarimetry explorer

2016

XIPE, the X-ray Imaging Polarimetry Explorer, is a mission dedicated to X-ray Astronomy. At the time of writing XIPE is in a competitive phase A as fourth medium size mission of ESA (M4). It promises to reopen the polarimetry window in high energy Astrophysics after more than 4 decades thanks to a detector that efficiently exploits the photoelectric effect and to X-ray optics with large effective area. XIPE uniqueness is time-spectrally-spatially- resolved X-ray polarimetry as a breakthrough in high energy astrophysics and fundamental physics. Indeed the payload consists of three Gas Pixel Detectors at the focus of three X-ray optics with a total effective area larger than one XMM mirror bu…

X-ray AstronomyHigh-energy astronomyPolarimetryX-ray opticsX-ray telescopeCondensed Matter Physic01 natural sciencesObservatory0103 physical sciencesPolarimetryElectronicOptical and Magnetic MaterialsSpectral resolutionElectrical and Electronic Engineering010303 astronomy & astrophysicsGas Pixel DetectorPhysicsX-ray astronomyta115X-ray optics010308 nuclear & particles physicsElectronic Optical and Magnetic MaterialApplied MathematicsVegaAstronomyComputer Science Applications1707 Computer Vision and Pattern RecognitionGas Pixel Detector; Polarimetry; X-ray Astronomy; X-ray opticsCondensed Matter PhysicsComputer Science ApplicationsApplied MathematicGas Pixel Detector; Polarimetry; X-ray Astronomy; X-ray optics; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringGas Pixel Detector; Polarimetry; X-ray Astronomy; X-ray optics; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications; Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringComputer Vision and Pattern RecognitionX-ray optic
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Accuracy evaluation of orthodontic movements with aligners: a prospective observational study.

2022

Abstract Background Since their introduction in orthodontics, clear aligners have been appreciated by patients, including adults, for their comfort and low aesthetic impact. Despite the enormous mobilization of financial resources all over the world aimed at producing new product lines, few clinical studies or high-quality evidence have been produced regarding the real effectiveness of such treatment. Given the few limited kinds of research on the subject, this study aims to produce and critically evaluate other data, to establish the concrete reliability of clear aligners in orthodontic therapy. Results Significant sample sizes were obtained for intrusion, vestibulo/lingual (V/L) crown tip…

IncisorCuspidTooth Movement TechniquesAccuracy Aligner treatment Orthodontic forces Orthodontic tooth movement Orthodontic predictability assessment InvisalignSettore MED/28 - Malattie OdontostomatologicheOrthodontic Appliances RemovableHumansOrthodontic Appliance DesignReproducibility of ResultsOrthodontics
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Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre

2021

Full list of authors: Acharyya, A.; Adam, R.; Adams, C.; Agudo, I.; Aguirre-Santaella, A.; Alfaro, R.; Alfaro, J.; Alispach, C.; Aloisio, R.; Alves Batista, R.; Amati, L.; Ambrosi, G.; Angüner, E. O.; Antonelli, L. A.; Aramo, C.; Araudo, A.; Armstrong, T.; Arqueros, F.; Asano, K.; Ascasíbar, Y. Ashley, M.; Balazs, C.; Ballester, O.; Baquero Larriva, A.; Barbosa Martins, V.; Barkov, M.; Barres de Almeida, U.; Barrio, J. A.; Bastieri, D.; Becerra, J.; Beck, G.; Becker Tjus, J.; Benbow, W.; Benito, M.; Berge, D.; Bernardini, E.; Bernlöhr, K.; Berti, A.; Bertucci, B.; Beshley, V.; Biasuzzi, B.; Biland, A.; Bissaldi, E.; Biteau, J.; Blanch, O.; Blazek, J.; Bocchino, F.; Boisson, C.; Bonneau Arbe…

Cherenkov Telescope ArrayMATÉRIA ESCURAscale: TeVAstronomyatmosphere [Cherenkov counter]dark matter experimentDark matter theoryenergy resolutionGamma ray experimentsParticleAstrophysicscosmic background radiation01 natural sciences7. Clean energyHigh Energy Physics - Phenomenology (hep-ph)benchmarkWIMPHESSenergy: fluxTeV [scale]relativistic [charged particle]gamma ray experimentMAGIC (telescope)Monte CarloEvent reconstructionPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Contractionspatial distributiontrack data analysisPhysicsdensity [dark matter]ClumpyAstrophysics::Instrumentation and Methods for AstrophysicsimagingHigh Energy Physics - Phenomenologydark matter experiments; dark matter theory; gamma ray experiments; galaxy morphologyDark matter experimentsFísica nuclearVERITASAstrophysics - High Energy Astrophysical PhenomenaSimulationsnoiseWIMPAstrophysics::High Energy Astrophysical PhenomenaDark mattersatelliteCosmic background radiationFOS: Physical sciencesAnnihilationdark matter: densityAstrophysics::Cosmology and Extragalactic AstrophysicsCherenkov counter: atmosphereheavy [dark matter]530annihilation [dark matter]GLASTDark matter experiments; Dark matter theory; Galaxy morphology; Gamma ray experimentscosmic radiation [p]0103 physical sciencesCherenkov [radiation]Candidatesddc:530AGNCherenkov radiationRadiative Processesthermal [cross section]010308 nuclear & particles physicsFísicadark matter: annihilationGamma-Ray SignalsCherenkov Telescope Array ; dark matter ; Galactic Center ; TeV gamma-ray astronomyAstronomy and AstrophysicsMassCherenkov Telescope Arrayradiation: CherenkovsensitivityMAGICGalaxyAstronomíadark matter: heavygamma rayp: cosmic radiation[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]correlationcharged particle: relativisticflux [energy]Galaxy morphology/dk/atira/pure/subjectarea/asjc/3100/3103galaxysupersymmetry[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cross section: thermal
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Sea urchin coelomocytes as a novel cellular biosensor of environmental stress: a field study in the Tremiti Island Marine Protected Area, Southern Ad…

2007

The aim of the present study was to investigate on the suitability of the sea urchin as a sentinel organism for the assessment of the macro-zoobenthos health state in bio-monitoring programmes. A field study was carried out during two oceanographic campaigns using immuno-competent cells, the coelomocytes, from sea urchins living in a marine protected area. In particular, coelomocytes subpopulations ratio and heat shock protein 70 (HSC70) levels were measured in specimens of Paracentrotus lividus (Lamark, 1816) collected in two sampling sites, namely Pianosa and Caprara Islands, both belonging to the Tremiti Island Marine Protected Area (MPA) in the Southern Adriatic Sea, Italy. By density g…

Health Toxicology and MutagenesisBiosensing TechniquesEnvironmentBiologyToxicologyEnvironmental stressParacentrotus lividusStress Physiologicalbiology.animalAnimalsSeawaterGonadsCoelomocyteSea urchinAtomic emission spectrometryGeographyHSC70 Heat-Shock ProteinsCell Biologybiology.organism_classificationTrace ElementsFisheryOn boardPhenotypeItalyMetalsSea UrchinsMarine protected areaProtected areaBiomarkersWater Pollutants ChemicalCell Biology and Toxicology
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XIPE: the X-ray imaging polarimetry explorer

2013

arXiv:1309.6995v1.-- et al.

AstronomyAstrophysics::High Energy Astrophysical PhenomenaPolarimetryFOS: Physical sciencesAstrophysics7. Clean energy01 natural scienceslaw.inventionX-raySettore FIS/05 - Astronomia E Astrofisicalaw0103 physical sciencesPolarimetry010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)Astronomy X-ray PolarimetryPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Solar flare[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]White dwarfAstronomy and AstrophysicsTorusMagnetic reconnectionPolarization (waves)Neutron starAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary Science[SDU]Sciences of the Universe [physics]Astrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsFlare
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