Conveners
Workshop on Astro-Cosmo-Gravity
- Larisa Bravina
- Sonia Kabana (Instituto De Alta Investigación, Universidad de Tarapacá (CL))
Workshop on Astro-Cosmo-Gravity
- Francesco Loparco (Universita e INFN, Bari (IT))
Workshop on Astro-Cosmo-Gravity
- Andrea Pareti (Pavia University and INFN (IT))
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Dariusz Gora (Institute of Nuclear Physics PAN)17/07/2025, 10:00Workshop on Astro-Cosmo-GravityTalk
The Pierre Auger Observatory, with two decades of data, has significantly advanced our understanding of ultra-high-energy cosmic rays (UHECRs) with energies exceeding 10^18 eV. Key results of the Observatory include: precise measurement of the cosmic-ray spectrum at the highest energies, observation of anisotropies in UHECR arrival directions, pointing to possible sources and mass composition...
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Fabio Gargano (INFN, Bari (IT))23/07/2025, 18:50Workshop on Astro-Cosmo-GravityTalk
The Antarctic Demonstrator for the Advanced Particle-astrophysics Telescope (ADAPT) is a NASA-funded balloon-borne mission designed to validate key technologies for the forthcoming Advanced Particle-astrophysics Telescope (APT). APT is envisioned as a next-generation gamma-ray observatory, operating both as a pair-conversion telescope for 50 MeV to ~50 GeV γ-rays and as a Compton telescope...
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Léonard Georges Théodore Lebrun23/07/2025, 19:10Workshop on Astro-Cosmo-GravityTalk
The DArk Matter Particle Explorer (DAMPE) is a satellite-based experiment designed to detect charged cosmic rays and gamma rays. It surveys the gamma-ray sky in the energy range from approximately 2 GeV to 10 TeV. Using a new gamma-ray selection algorithm and taking advantage of DAMPE’s excellent energy resolution, we obtain high-precision energy spectra for bright pulsars. In this work, we...
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Andrea Simongini24/07/2025, 11:00Cosmology, Astrophysics, Gravity, Mathematical PhysicsTalk
The Vera Rubin Observatory’s Legacy Survey of Space and Time (LSST) will revolutionize time-domain optical astronomy, detecting faint sources down to r~27.5 mag and generating nearly 32 trillion observations over 10 years. Among these, ~10 million will be supernovae (SNe), covering a wide range of redshifts. This unprecedented dataset will allow comprehensive characterization of every phase of...
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Zacharias Roupas (Physics department, University of Milano-Bicocca, Italy)24/07/2025, 11:25Workshop on Astro-Cosmo-GravityTalk
The existence of gaseous proto-stellar clusters with initial gas mass from one to one hundred million solar masses, and high temperature, primarily composed of atomic hydrogen at the epoch of reionization is strongly supported by cosmological, astrophysical, and recent direct observational evidence. Such systems form from the collapse of a respective compact massive cloud. We consider the...
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