
After the long interruption of the Frascati Workshops series due to the Covid-19 Pandemic, we are finally able to restart this historic series in complete safety. This is the fourteenth edition of the series of Frascati Workshops on "Multifrequency Behaviour of High Energy Cosmic Sources" which is undoubtedly a largely accepted biennial meeting in which an updated experimental and theoretical panorama will be depicted. This edition comes at the 39th anniversary of the first historical "multifrequency" workshop about "Multifrequency Behaviour of Galactic Accreting Sources", held in Vulcano (Archipelago of the Eolian Islands) in September 1984.
This surely renders the Frascati Workshop Series the oldest among the many devoted to "Multifrequency Studies of Cosmic Sources".
The study of the physics governing the cosmic sources will be the main goal of the workshop considering also the recent detection of gravitational waves from the merging of collapsed objects. A session devoted to the ongoing and next generation ground- and space-based experiments will give the actual prospects for the first decades of this millennium.
We deliberately do not want to change the workshop name from "Multifrequency Behavior of High Energy Cosmic Sources" to "Multimessenger Behavior of High Energy Cosmic Sources" in order to preserve the name of our historical workshop series.
• The following items will be reviewed:Cosmology: Cosmic Background, Clusters of Galaxies
• Extragalactic Sources: Active Galaxies, Normal Galaxies
• Gamma-Rays Burst: Experiments versus Theories
• Galactic Sources: Pre-Main-Sequence and Main-Sequence Stars, Cataclysmic Variables and Novae, Supernovae and SNRs, X-Ray Binary Systems, Pulsars, Black Holes, Gamma-Ray Sources,Nucleosynthesis.
• Gravitationl waves: Theory Vs Experiments.
• Science from large area multiwavelength surveys and deep-exposure pointings.
• The Astrophysics with the Ongoing and Future Experiments: Space-Based Experiments,Ground-Based Experiments.
Participation in the workshop is by invitation only.
All participants are kindly invited to attend the whole workshop.
The workshop will include several 30-min talks to introduce the current problems, and typically 20-min talks giving new experimental and theoretical results.
A series of 15-min talks will be devoted to ongoing and next generation experiments.
Opening Remarks |
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A Journey to Understand Our Universe
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Neutrino Astronomy in the IceCube Era
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Search for Gamma-Ray Counterparts of IceCube Neutrino Events in the AGILE Public Archive
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Blazars as neutrino sources
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The two-dimensional and three-dimensional relations in the plateau emission in multi-wavelengths
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Search for neutral particles with the Pierre Auger Observatory
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On the origin of UHE Cosmic Rays
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The Birth of a Relativistic Jet Following the Disruption of a Star by a Cosmological Black Hole
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JWST data and possible interpretation
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Results of the Heavy Cosmic-Ray Analysis with CALET on the International Space Station
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Latest results on cosmic rays light elements with the CALorimetric Electron Telescope (CALET) on the International Space Station
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The dynamics of Globular Clusters with the GAIA Data
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Cosmology |
Superheavy SUSY-kind dark matter and high energy cosmic rays
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Multi-messenger cosmology and astrophysics with Gamma-Ray Bursts
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Testing General Relativity with Black Hole X-Ray Data and ABHModels
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High-z GRBs as witness of infant Universe
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Limits on the Primordial Black Holes Dark Matter with current and future missions
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Cosmic Microwave Background Observations: looking for the Cosmic Web through the Sunyaev Zeldovich effect
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Gravitational Waves |
Gravitational Waves Astronomy: present and future
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The new world discovered with the detection of Gravitational Waves
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Multimessenger detection of binary neutron star mergers
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Multimessenger Era: Integral observations of GW and transient phenomena
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Star Formation |
JWST spectroscopy of accreting pre-main sequence stars in the Milky Way and Magellanic Clouds
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Jets, Outflows, and Explosions in Massive Star Formation
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Multi-band observations of the extended green objects (EGO) G45.47+0.13
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Astrophysics of High Energy Cosmic Sources |
Evolution of accreting white dwarfs from HST and Gaia
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Supersoft X-ray emission from the classical nova AT 2018bej
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TESS and ground based photometry of magnetic CVs
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THESEUS Science on Time-domain Studies of Compact Object Binaries
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X-Ray Polarimetry and IXPE mission
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Observations of Blazars, AGN, and Magnetars with the Imaging X-ray Polarimetry Explorer (IXPE)
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Magnetars - An updated review
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Polarized X-rays from the magnetar sources
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X-ray polarization of Blazars
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The look and nature of massive blazars in the early Universe
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A shared accretion instability for black holes and neutron stars
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Black Holes studies with Insight-HXMT
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First Year of Stellar-Mass Black Hole Observations with the Imaging X-ray Polarimetry Explorer
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eROSITA AGN Science Highlights
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An explosive year: first X-ray polarization detection of supernova remnants
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Fermi-LAT Gamma-ray Emission Discovered From the Composite Supernova Remnant B0453-685 in the Large Magellanic Cloud
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Modeling the Evolution from Massive Stars to Supernovae and Supernova Remnants
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Progenitor constraint using line ratios of the CNO elements in supernova remnants
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Suzaku observations of Fe K-shell lines in the supernova remnant W51C and hard X-ray sources in the proximity
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Modelling the optical/UV emission of Swift J0243.6+6124 during its 2017–2018 giant outburst
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The role of stellar winds in the formation of massive stellar black holes
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Broadband X-ray Spectroscopy of the Pulsar Wind Nebula in HESS J1640-465
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Uncovering X-ray binary population in eROSITA using machine learning methods
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X-ray study on the nature of the colliding stellar winds in the massive star binary WR140
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Binary systems at gamma-rays: status and prospects
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The Be/X-ray binary A0538-66 - A Short Review
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Timing (Pulsating) ULX-ray sources – lessons learned from M82
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Supergiant Fast X-ray Transients (SFXT) – A Review
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X-ray observations of isolated neutron stars
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Intermediate Mass Black Holes - A Review
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Accretion and ejection connection in AGN
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The relation between X-ray and UV emission in quasars
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The Peculiar Properties of Cold Quasars
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Blazars from the new window of X-ray polarimetry: IXPE observations of Mrk 421
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Dual and binary supermassive black holes
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X-ray vs H_alpha emissions among Stars and XRISM Plan
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SGR1806-20 activity spanning 20 years of INTEGRAL
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Jet Sources & Gamma-Ray Bursts |
The contribution of AGILE to the knowledge of GRBs and other transients
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Global MASTER-Net Highlights
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Jet variability in Stellar-mass Compact
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Jets in accreting black-hole binaries Objects
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Shedding new light on the Hubble constant tension through Supernovae Ia
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On the origin of afterglow "plateaus" in gamma-ray bursts
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GRB 210905A at 𝒛 = 6.3: a powerful blast from the past.
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The role of the magnetic fields in GRB outflows
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GRBAlpha and VZLUSAT-2 CubeSats Observing Gamma-Ray Transients
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Multifrequency and multimessenger observations of short GRBs and kilonovae
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Ongoimg Experiments |
Einstein Probe Mission
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Novel space experiments for X-ray astrophysics: LOBSTER EYE
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The Rocket Experiment Demonstration of a Soft X-ray Polarimeter (REDSoX)
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The SVOM mission in the multimessenger era
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QUVIK (Ultra-VIolet Kilonova surveyor Experiment)
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Localisation of GRBs from the combined SpIRIT+HERMES-TP/SP nano-satellite constellation
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The Quick Look subsystem of the GRASS-2 Experiment
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Special Night Session |
Stellar, Galactic, and Super-Galactic Habitable Zones
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Concluding Remarks |
Concluding Remarks - I
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From the gravitational waves to the exoplanets: the Research Highlights
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Concluding Remarks - III
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Concluding Remarks - IV
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Concluding Address |
Frascati Workshop 2023: Concluding Address
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