0000000000431073

AUTHOR

Silvia Piranomonte

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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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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Time domain astronomy with the THESEUS satellite

2021

THESEUS is a medium size space mission of the European Space Agency, currently under evaluation for a possible launch in 2032. Its main objectives are to investigate the early Universe through the observation of gamma-ray bursts and to study the gravitational waves electromagnetic counterparts and neutrino events. On the other hand, its instruments, which include a wide field of view X-ray (0.3-5 keV) telescope based on lobster-eye focussing optics and a gamma-ray spectrometer with imaging capabilities in the 2-150 keV range, are also ideal for carrying out unprecedented studies in time domain astrophysics. In addition, the presence onboard of a 70 cm near infrared telescope will allow simu…

010504 meteorology & atmospheric sciencesmedia_common.quotation_subjectAstronomyAstrophysics::High Energy Astrophysical PhenomenaSocio-culturaleFOS: Physical sciencesX-ray sources01 natural scienceslaw.inventionTelescopeX-ray sourceSettore FIS/05 - Astronomia E Astrofisicalaw0103 physical sciencesTime domain[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Variability010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)0105 earth and related environmental sciencesmedia_commonTime domain astronomyPhysicsSpectrometerGravitational waveX-rays surveysAstronomyAstronomy and AstrophysicsUniverseSpace and Planetary ScienceSatelliteNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsExperimental Astronomy
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Pulsating in Unison at Optical and X-Ray Energies: Simultaneous High Time Resolution Observations of the Transitional Millisecond Pulsar PSR J1023+00…

2019

PSR J1023+0038 is the first millisecond pulsar discovered to pulsate in the visible band; such a detection took place when the pulsar was surrounded by an accretion disk and also showed X-ray pulsations. We report on the first high time resolution observational campaign of this transitional pulsar in the disk state, using simultaneous observations in the optical (TNG, NOT, TJO), X-ray (XMM-Newton, NuSTAR, NICER), infrared (GTC) and UV (Swift) bands. Optical and X-ray pulsations were detected simultaneously in the X-ray high intensity mode in which the source spends $\sim$ 70% of the time, and both disappeared in the low mode, indicating a common underlying physical mechanism. In addition, o…

AccretionAccretion disks-pulsars: Individual (psr j1023+0038)-stars: Neutron-X-rays: Binaries010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesSettore FIS/05 - Astronomia E AstrofisicaPulsarAccretion discMillisecond pulsar0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstrophysics::Instrumentation and Methods for AstrophysicsX-rayAstronomy and AstrophysicsTime resolutionAccretion (astrophysics)Space and Planetary ScienceVisible bandAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaThe Astrophysical Journal
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