collaborators

10 papers

astro-ph.IM2026

Spectral performance of single-channel plastic and GAGG scintillator bars of the CUbesat Solar Polarimeter (CUSP)

Nicolas De Angelis, Abhay Kumar, Sergio Fabiani +45

Our Sun is the closest X-ray astrophysical source to Earth. As such, it makes a formidable case study to better understand astrophysical processes. Solar flares are in particular v…

physics.ins-det2025

Scalable Relay Switching Platform for Automated Multi-Point Resistance Measurements

Edoardo Boretti, Kostiantyn Torokhtii, Enrico Silva +1

In both research and industrial settings, it is often necessary to expand the input/output channels of measurement instruments using relay-based multiplexer boards. In research act…

physics.app-ph2025

Comparative Analysis of Thermal Models for Test Masses in Next-Generation Gravitational Wave Interferometers

Vincenzo Pierro, Vincenzo Fiumara, Guerino Avallone +8

Accurate thermal modeling of Terminal Test Masses (TTMs) is crucial for optimizing the sensitivity of gravitational wave interferometers like Virgo. In fact, in such gravitational…

astro-ph.SR2025

Solar Flare Hard X-ray Polarimetry with the CUbesat Solar Polarimeter (CUSP) mission

Nicolas De Angelis, Andrea Alimenti, Davide Albanesi +43

The CUbesat Solar Polarimeter (CUSP) project is a CubeSat mission planned for a launch in low-Earth orbit and aimed to measure the linear polarization of solar flares in the hard X…

astro-ph.IM2025

The multi-physics analysis, design and testing of CUSP, a CubeSat mission for space weather and solar flares x-ray polarimetry

Giovanni Lombardi, Sergio Fabiani, Ettore Del Monte +45

The space-based CUbesat Solar Polarimeter (CUSP) mission aims to measure the linear polarization of solar flares in the hard X-ray band by means of a Compton scattering polarimeter…

astro-ph.SR2025

CUbesat Solar Polarimeter (CUSP) Sensitivity Estimation and Performance Optimization using Geant4

Abhay Kumar, Giovanni Lombardi, Giovanni De Cesare +45

The CUbesat Solar Polarimeter (CUSP) aims to measure the linear polarization of solar flares in the 25-100 keV X-ray band using a Compton scattering polarimeter. CUSP will allow us…