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20192026
most citedLarge scale characterization and calibration strategy of a SiPM-based camera for gamma-ray astronomy

10 citations · 43 across the 20 of their papers we have counts for

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19 papers · 1 filter

astro-ph.IM2026

PolPy: A universal tool for X-ray/gamma-ray polarimetry using common data format standards

Sujay Mate, Hancheng Li, Utkarsh Pathak +4

X-ray/gamma-ray polarimetry has been a rapidly developing field in recent years. However, the lack of standardized analysis frameworks has hindered cross-instrument comparisons and…

astro-ph.IM2026

EXPO: a quantum leap in fast, wide-band X-ray polarimetry for astrophysics

Paolo Soffitta, Sebastien Guillot, Ian Hutchinson +137

The Enhanced X-ray Polarimetry Observatory (EXPO) is a mission concept proposed to ESA as an M8 candidate, with a prospective launch in 2041. Building on the scientific success of…

astro-ph.IM2026

In orbit background for hard X-ray CubeSat polarimeters: case study of the CUSP mission in low-earth orbit

Abhay Kumar, Giovanni Lombardi, Riccardo Campana +45

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

astro-ph.IM2026

The CUSP CubeSat mission for space weather multi-physics analysis, design, and testing

Giovanni Lombardi, Riccardo Di Spirito, Sergio Fabiani +48

The 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. CUSP is a…

astro-ph.IM2026

Compton Polarimeter Prototype for the CUbesat Solar Polarimeter (CUSP) mission

Nicolas De Angelis, Andrea Alimenti, Riccardo Campana +41

The space-based CUbesat Solar Polarimeter (CUSP) mission aims to measure the linear polarization of solar flares in the hard X-ray band (25-100 keV) by means of a dual-phase Compto…

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…

astro-ph.IM2025★ 5 cited

Design and Performance of a Universal SiPM Readout System for X- and Gamma-Ray Missions

Merlin Kole, Nicolas De Angelis, Nicolas Produit +15

The advent of both multi-messenger and time-domain astrophysics over the last decade has seen a large interest in the development of small-scale, cheap, and robust gamma-ray detect…

astro-ph.IM2024★ 3 cited

Optimizing the light output of a plastic scintillator and SiPM based detector through optical characterization and simulation: A case study for POLAR-2

Nicolas De Angelis, Franck Cadoux, Coralie Husi +2

The combination of plastic scintillators with Silicon Photo-Multipliers (SiPMs) is widely used for detecting radiation in high-energy astrophysics, particle physics, neutrino physi…

astro-ph.IM2024

The CUbesat Solar Polarimeter (CUSP) mission overview

Sergio Fabiani, Ettore Del Monte, Ilaria Baffo +35

The CUbesat Solar Polarimeter (CUSP) project is a future CubeSat mission orbiting the Earth aimed to measure the linear polarization of solar flares in the hard X-ray band, by mean…

astro-ph.IM2024

Characterization of avalanche photodiodes (APDs) for the CUbesat Solar Polarimeter (CUSP) mission

F. Cologgi, A. Alimenti, S. Fabiani +39

The CUbesat Solar Polarimeter (CUSP) project is a CubeSat mission orbiting the Earth aimed to measure the linear polarization of solar flares in the hard X-ray band by means of a C…

astro-ph.IM2024

The multiphysics analysis and design of CUSP, a two CubeSat constellation for Space Weather and Solar flares X-ray polarimetry

Giovanni Lombardi, Sergio Fabiani, Ettore Del Monte +38

The CUbesat Solar Polarimeter (CUSP) project aims to develop a constellation of two CubeSats orbiting the Earth to measure the linear polarization of solar flares in the hard X-ray…

astro-ph.IM2024

The evaluation of the CUSP scientific performance by a GEANT4 Monte Carlo simulation

Giovanni De Cesare, Sergio Fabiani, Riccardo Campana +35

The CUbesat Solar Polarimeter (CUSP) project is a CubeSat mission orbiting the Earth aimed to measure the linear polarization of solar flares in the hard X-ray band by means of a C…

astro-ph.IM2024★ 9 cited

Response of the first POLAR-2 Prototype to Polarized Beams

Merlin Kole, Nicolas de Angelis, Ana Bacelj +15

POLAR-2 is a dedicated gamma-ray polarimeter currently foreseen to be launched towards the China Space Station around 2027. The design of the detector is based on the legacy of its…

astro-ph.IM2024

Future Perspectives for Gamma-ray Burst Detection from Space

Enrico Bozzo, Lorenzo Amati, Wayne Baumgartner +35

Since their first discovery in the late 1960s, Gamma-ray bursts have attracted an exponentially growing interest from the international community due to their central role in the m…

astro-ph.IM2023★ 8 cited

POLAR-2, the next generation of GRB polarization detector

Nicolas Produit, Merlin Kole, Xin Wu +9

The POLAR-2 Gamma-Ray Burst (GRB) Polarimetry mission is a follow-up to the successful POLAR mission. POLAR collected six months of data in 2016-2017 on board the Tiangong-2 Chines…

astro-ph.IM2023★ 2 cited

Proton irradiation of plastic scintillator bars for POLAR-2

Slawomir Mianowski, Nicolas De Angelis, Kamil Brylew +8

POLAR-2, a plastic scintillator based Compton polarimeter, is currently under development and planned for a launch to the China Space Station in 2025. It is intended to shed a new…

astro-ph.IM2022★ 1 cited

Characterisation of the MUSIC ASIC for large-area silicon photomultipliers for gamma-ray astronomy

Nicolas De Angelis, David Gascón, Sergio Gómez +3

Large-area silicon photomultipliers (SiPMs) are desired in many applications where large surfaces have to be covered. For instance, a large area SiPM has been developed by Hamamats…

astro-ph.IM2020★ 10 cited

Large scale characterization and calibration strategy of a SiPM-based camera for gamma-ray astronomy

C. Alispach, J. Borkowski, F. R. Cadoux +18

The SST-1M is a 4-m diameter mirror Davies-Cotton gamma-ray telescope. It has been designed to cover the energy range above 500 GeV and to be part of an array of telescopes separat…

astro-ph.IM2019

Calibration and operation of SiPM-based cameras for gamma-ray astronomy in presence of high night-sky light

Imen Al Samarai, Cyril Martin Alispach, Matteo Balbo +56

The next generation of Cherenkov telescope cameras feature Silicon Photo Multipliers (SiPM), which can guarantee excellent performance and allow for observation also under moonligh…