most citedMeasurement of the non-linearity in the gamma-ray response of the GAGG:Ce inorganic scintillator

6 citations · 9 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.IM2023

Imaging performance above 150 keV of the wide field monitor on board the ASTENA concept mission

Lisa Ferro, Leo Cavazzini, Miguel Moita +10

A new detection system for X-/Gamma-ray broad energy passband detectors for astronomy has been developed. This system is based on Silicon Drift Detectors (SDDs) coupled with scinti…

astro-ph.IM20233 cited

The TRILL project: increasing the technological readiness of Laue lenses

Lisa Ferro, Enrico Virgilli, Miguel Moita +16

Hard X-/soft Gamma-ray astronomy (> 100 keV) is a crucial field for the study of important astrophysical phenomena such as the 511 keV positron annihilation line in the Galactic ce…

physics.ins-det20236 cited

Measurement of the non-linearity in the gamma-ray response of the GAGG:Ce inorganic scintillator

R. Campana, C. Evola, C. Labanti +6

A characteristic of every inorganic scintillator crystal is its light yield, i.e., the amount of emitted scintillation photons per unit of energy deposited in the crystal. Light yi…

astro-ph.IM2023

Opening the path to hard X-/soft gamma-ray focussing: the ASTENA-pathfinder mission

Enrico Virgilli, Lorenzo Amati, Natalia Auricchio +10

Hard X-/soft gamma-ray astronomy is a crucial field for transient, nuclear and multimessenger astrophysics. However, the spatial localization, imaging capabilities and sensitivity…

astro-ph.IM2023

CdTe Spectroscopic-Imager Measurements with Bent Crystals for Broad Band Laue Lenses

N. Auricchio, L. Ferro, J. B. Stephen +15

In astrophysics, several key questions in the hard X soft Gamma-ray range (above 100 keV) require sensitivity and angular resolution that are hardly achievable with current technol…