A5078458799- Astrophysics and Cosmic Phenomena
- Dark Matter and Cosmic Phenomena
- Neutrino Physics Research
- Particle physics theoretical and experimental studies
- Radio Astronomy Observations and Technology
- Particle Detector Development and Performance
- Gamma-ray bursts and supernovae
- Atmospheric Ozone and Climate
- Pulsars and Gravitational Waves Research
- Atmospheric aerosols and clouds
- Astronomical Observations and Instrumentation
- Ionosphere and magnetosphere dynamics
- Photocathodes and Microchannel Plates
- High-Energy Particle Collisions Research
- History and Developments in Astronomy
- Radiation Detection and Scintillator Technologies
- Radiation Therapy and Dosimetry
- Calibration and Measurement Techniques
- Solar and Space Plasma Dynamics
- Cosmology and Gravitation Theories
- Precipitation Measurement and Analysis
- Computational Physics and Python Applications
- Atmospheric and Environmental Gas Dynamics
- Lightning and Electromagnetic Phenomena
- Noncommutative and Quantum Gravity Theories
Osservatorio Astrofisico di Torino
2016-2025
Istituto Nazionale di Fisica Nucleare, Sezione di Torino
2016-2025
University of Buenos Aires
2009-2023
Consejo Nacional de Investigaciones Científicas y Técnicas
2009-2023
Instituto de Tecnologías en Detección y Astropartículas
2016-2023
National University of General San Martín
2016-2023
National Technological University
2010-2023
Pierre Auger Observatory
2007-2023
Institute of Scientific and Technical Research for Defense
2016-2023
Universidad Nacional de La Plata
2010-2023
In the framework of upgrade Pierre Auger Observatory, a new high voltage module is being employed for power supply 1-inch photomultiplier added to each water-Cherenkov detector surface array with aim increasing dynamic range measurements. This located in dedicated box near electronics and comprises low consumption DC-DC converter hosted inside an aluminum box. All modules have undergone specific tests verify their reliability extreme environmental conditions Argentinian pampa. this paper, we...
With the forthcoming of space borne observatories devoted to research Ultra High Energy Cosmic Rays (UHECR) in decade 1020eV, new challenges are posed experimental techniques. Mounted on International Space Station, Extreme Universe Observatory board Japanese Experimental Module (JEM-EUSO) will rely well established fluorescence technique observe Extensive Air Showers(EAS) propagating atmosphere from space. The EUSO Simulation and Analysis Framework (ESAF) has been developed this context...
The trigger system of the Surface Detector (SD) Pierre Auger Observatory is described, from identification candidate showers ($E>1$ EeV) at level a single station, among huge background (mainly muons), up to selection real events and rejection random coincidences higher central (including reconstruction accuracy). Efficiency station evaluated using data , high performance event hierarchy will be demonstrated.
Abstract The MERLINO project is developing a multi-detector setup with the goal of evaluating beam stopping power from Prompt-Gamma-Timing measurements in proton therapy. detectors are based on cerium-doped lanthanum bromide crystal, LaBr 3 :Ce, coupled to photo-multiplier tubes. system characterization ongoing and first calibration two showed 124 ps σ E / = 3% for timing energy resolution, respectively. measured experimental parameters were then used carry out preliminary estimation power....
The X-ray Calibration Facility (XCF) is a table-top, open-design irradiation setup for research, available at the Physics Department of University Turin. It offers beams photons different energies and with various spatial polarization configurations. These characteristics allow XCF to be suitable facility calibration test energy, position sensitive detectors.