0000000000431075

AUTHOR

Angelo Francesco Gambino

showing 5 related works from this author

GrailQuest and HERMES: hunting for gravitational wave electromagnetic counterparts and probing space-time quantum foam

2021

GrailQuest (Gamma-ray Astronomy International Laboratory for Quantum Exploration of Space-Time) is an ambitious astrophysical mission concept that uses a fleet of small satellites whose main objective is to search for a dispersion law for light propagation in vacuo. Within Quantum Gravity theories, different models for space-time quantization predict relative discrepancies of the speed of photons w.r.t. the speed of light that depend on the ratio of the photon energy to the Planck energy. This ratio is as small as 10-23 for photons in the γ- ray band (100 keV). Therefore, to detect this effect, light must propagate over enormous distances and the experiment must have extraordinary sensitivi…

PhysicsCubeSatsGamma-Ray BurstsPhotonGravitational Wave counterparts010308 nuclear & particles physicsGravitational waveSpace timeQuantum gravityAstronomyTriangulation (social science)01 natural sciencesSettore FIS/05 - Astronomia E AstrofisicaAll-sky monitorObservatoryX-rays0103 physical sciencesQuantum gravityNano-satellitesTemporal triangulationGamma-ray burstQuantum foam010303 astronomy & astrophysics
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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
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Accretion in strong field gravity with eXTP

2019

In this paper we describe the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to accretion flows in the strong field gravity regime around both stellar-mass and supermassive black-holes. eXTP has the unique capability of using advanced 'spectral-timing-polarimetry' techniques to analyze the rapid variations with three orthogonal diagnostics of the flow and its geometry, yielding unprecedented insight into the inner accreting regions, the effects of strong field gravity on the material within them and the powerful outflows which are driven by the accretion process.

ACTIVE GALACTIC NUCLEIAccretionaccretion; black holes physics; X-ray; Physics and Astronomy (all)black holes physicAstronomyAstrophysics::High Energy Astrophysical PhenomenaBlack holes physicsPolarimetryFOS: Physical sciencesBLACK-HOLE SPINGeneral Physics and AstronomyStrong fieldAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesX-rayPhysics and Astronomy (all)ELECTROMAGNETIC EMISSIONSettore FIS/05 - Astronomia e Astrofisicablack holes physicsaccretion0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)XMM-NEWTONPhysicsLENS-THIRRING PRECESSION[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]QUASI-PERIODIC OSCILLATIONS[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]IRON KAccretion (astrophysics)X ray[SDU]Sciences of the Universe [physics]ULTRA-FAST OUTFLOWSAstrophysics::Earth and Planetary AstrophysicsSPECTRAL FEATURESAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]X-RAY BINARIESScience China Physics, Mechanics & Astronomy
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The scientific payload on-board the HERMES-TP and HERMES-SP CubeSat missions

2021

HERMES (High Energy Rapid Modular Ensemble of Satellites) Technological and Scientific pathfinder is a space borne mission based on a LEO constellation of nano-satellites. The 3U CubeSat buses host new miniaturized detectors to probe the temporal emission of bright high-energy transients such as Gamma-Ray Bursts (GRBs). Fast transient localization, in a field of view of several steradians and with arcmin-level accuracy, is gained by comparing time delays among the same event detection epochs occurred on at least 3 nano-satellites. With a launch date in 2022, HERMES transient monitoring represents a keystone capability to complement the next generation of gravitational wave experiments. In t…

Computer scienceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesField of viewAstrophysics01 natural sciencesAstrophysics - Instrumentation and MethodsSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesCubeSatTransient (computer programming)Aerospace engineeringInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsConstellationHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsbusiness.industryGravitational wavePayloadAstrophysics::Instrumentation and Methods for AstrophysicsSteradianSatelliteAstrophysics - Instrumentation and Methods for AstrophysicsbusinessAstrophysics - High Energy Astrophysical PhenomenaSpace Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray
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Broadband spectral analysis of MXB 1659-298 in its soft and hard state

2019

The X-ray transient eclipsing source MXB 1659-298 went in outburst in 1999 and 2015, respectively, during which it was observed by XMM-Newton, NuSTAR and Swift. Using these observations we studied the broadband spectrum of the source to constrain the continuum components and to verify the presence of a reflection component. We analysed the soft and hard state of the source, finding that the soft state can be modelled with a thermal component associated with the inner accretion disc plus a Comptonised component. A smeared reflection component and the presence of an ionised absorber are also requested in the best-fit model. On the other hand, the direct continuum emission in the hard state ca…

High Energy Astrophysical Phenomena (astro-ph.HE)X-rays: binariesstars: individual (MXB 1659-298)stars: neutronaccretionaccretion disksAstrophysics::High Energy Astrophysical PhenomenaAccretion Accretion disks Stars: individual (MXB 1659-298) Stars: neutron X-rays: binariesFOS: Physical sciences[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical Phenomena
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