English

Characterization of a CdZnTe detector for a low-power CubeSat application

Instrumentation and Methods for Astrophysics 2022-08-10 v2 High Energy Astrophysical Phenomena

Abstract

We report spectral and imaging performance of a pixelated CdZnTe detector custom designed for the \emph{MeVCube} project: a small Compton telescope on a CubeSat platform. \emph{MeVCube} is expected to cover the energy range between 200  keV200\;\mathrm{keV} and 4  MeV4\;\mathrm{MeV}, with performance comparable to the last generation of larger satellites. In order to achieve this goal, an energy resolution of few percent in full width at half maximum (FWHM) and a 33-D spatial resolution of few millimeters for the individual detectors are needed. The severe power constraints present in small satellites require very low power read-out electronics for the detector. Our read-out is based on the VATA450.3 ASIC developed by \emph{Ideas}, with a power consumption of only 0.25  mW/channel0.25\;\mathrm{mW/channel}, which exhibits good performance in terms of dynamic range, noise and linearity. A 2.0  cm×2.0  cm×1.5  cm2.0\;\mathrm{cm} \times 2.0\;\mathrm{cm} \times 1.5\;\mathrm{cm} CdZnTe detector, with a custom 8×88 \times 8 pixel anode structure read-out by a VATA450.3 ASIC, has been tested. A preliminary read-out system for the cathode, based on a discrete \emph{Amptek} A250F charge sensitive pre-amplifier and a DRS4 ASIC, has been implemented. An energy resolution around 3%3\% FWHM has been measured at a gamma energy of 662  keV662\;\mathrm{keV}; at 200  keV200\;\mathrm{keV} the average energy resolution is 6.5%6.5\%, decreasing to 2%\lesssim 2\% at energies above 1  MeV1\;\mathrm{MeV}. A 33-D spatial resolution of 2mm\approx 2\,\mathrm{mm} is achieved.

Keywords

Cite

@article{arxiv.2204.00475,
  title  = {Characterization of a CdZnTe detector for a low-power CubeSat application},
  author = {Giulio Lucchetta and Markus Ackermann and David Berge and Ingo Bloch and Rolf Bühler and Hermann Kolanoski and Wolfgang Lange and Francesco Zappon},
  journal= {arXiv preprint arXiv:2204.00475},
  year   = {2022}
}

Comments

Accpted for publication in JINST

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