| Foreword |
| O. Straniero | Stars and physics beyond the Standard Model |
| E. Orlando | The high-energy emission from the quiet Sun |
| T. Belloni et al. | High-Energy observations of Stellar-mass Compact Objects: from CVs to the most luminous X-Ray Binaries |
| G. Israel et al. | The Extragalactic Population of Accreting Neutron Stars and the Ultraluminous
X-ray Sources Paradigm: from ULTraS to PULSULTraS |
| M. Orio | X-ray observations of accreting and burning white dwarfs |
| M. Brusa et al. | Supermassive Black Hole Winds in X–rays |
| M. Dadina et al. | Probing AGN feedback in the most luminous QSO at cosmic noon |
| G. Risaliti et al. | Quasars at High-Redshift: Physics and Cosmology |
| P. Severgnini et al. | Supermassive Black Hole Binaries and dual AGN |
| E. Torresi et al. | Exploring the radio morphology-accretion mode link in radio galaxies at high energies |
| E. Pian et al. | Probing the physics of compact extragalactic sources over multiple scales |
| S. Andreon & F. Castagna | Our approach to the thermodynamic evolution of galaxy clusters |
| S. Ettori et al. | Galaxy clusters in X-rays: the buildup of massive structures in the last 10 Gyrs,
and CHEX-MATE |
| A. Moretti et al. | Environmental processes at work in galaxy clusters: triggering of the AGN activity
and development of X–ray tails |
| P. Tozzi et al. | Mapping Feedback Processes in the Intracluster Medium at low and high redshift |
| A. De Luca et al. | The ULTraS project: Understanding the X-ray variable and transient sky |
| G. Stratta et al. | On the origin of afterglow ”plateaus” in gamma-ray bursts |
| G. Ghisellini et al. | The new age of Gamma Ray Bursts: physics and multi-messengers |
| C. Guidorzi et al. | A search for high-energy counterparts to extragalactic fast radio burst sources with Insight–HXMT |
| M. Bertaina et al | A search for Extreme Energy Cosmic Rays and nuclearites in TUS observations
and a study of the relative exposure |
| E. Amato et al. | On the escape of cosmic ray leptons and their impact on the background plasma |
| P. Blasi et al. | A Modern Approach to Cosmic Ray Transport in the Galaxy |
| F. Donato & S. Recchia | nverse Compton halos around Pulsar Wind Nebulae |
| S. Orlando et al. | Connecting supernova remnants to their parent supernovae |
| M. Regis et al. | Deciphering the high-energy sky via angular cross correlations |
| E. Caroli et al. | 3DCaTM: a 3D Cadmium Zinc Telluride spectroscopic module for hard X- and
γ-ray astronomy |
| O. Catalano et al. | FluChe: Fluorescence and Cherenkov light detection with SiPM for space and
ground applications |
| E. Virgilli et al. | Increase of the Technological Readiness Level for the realization of hard X-/soft gamma-ray Laue optics |
| R. Gilli et al. | Next Generation X-ray Imaging Surveys |
| A. De Rosa et al. | Science case study and scientific simulations for the enhanced X-ray Timing Polarimetry mission, eXTP |
| D. D’Urso, et al. | POX – PANGU Optimization and eXperimental verification: design and perfor-
mance |
Memorie della SAIT - Osservatorio
Astronomico di Roma, via Frascati 33, 00078, Monte Porzio Catone, Roma
