Creating a database of pulse waveforms for scintillator-based gamma-ray detectors
Pre-published on:
August 18, 2023
Published on:
September 27, 2024
Abstract
The first Gamma-ray Burst (GRB) counterpart to a gravitational wave event, GRB 170817A, proved that monitoring for gamma-ray transients is an essential part of multi-messenger astronomy. As a result, research teams, globally, are now working towards the next generation of GRB instruments. To aid this work, we are creating a database of pulse waveforms for scintillation detectors over gamma-ray energies from 30-1000 keV. This database will inform performance estimates, such as the minimum energy threshold and pulse shape discrimination ability in phoswich-style detectors. We will present initial results from the database using a Hamamatsu R12699 flat panel photomultiplier tube (PMT) coupled to NaI(Tl) and CsI(Na) scintillators.
DOI: https://doi.org/10.22323/1.444.0704
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