Imaging and Spectral Performance of a 60 {\mu}m Pitch CdTe Double-Sided Strip Detector

TL;DR

This study evaluates a 60 μm pitch CdTe double-sided strip detector's imaging and spectral performance, introducing a new spectral reconstruction method and demonstrating high-resolution imaging capabilities for solar X-ray observations.

Contribution

The paper presents a novel spectral reconstruction technique using induced charge information and demonstrates improved energy resolution and imaging performance of a fine-pitch CdTe detector.

Findings

Achieved 0.76 keV and 1.0 keV FWHM energy resolutions at 14 keV and 60 keV.

Reduced spectral tail components and improved 60 keV peak resolution from 2.4 keV to 1.5 keV.

Obtained sub-strip pitch position resolution using charge sharing correction.

Abstract

We have evaluated the performance of a fine pitch CdTe Double-sided Strip Detector (CdTe-DSD), which was originally developed for the focal plane detector of a hard X-ray telescope to observe the Sun. The detector has a thickness of 750 um and has 128 strip electrodes with a 60 um strip pitch orthogonally placed on both sides of the detector and covers an energy range 4 keV to 80 keV. The study of the depth of photon interaction and charge sharing effects are of importance in order to provide good spectroscopic and imaging performance. We study the tail structure observed in the spectra caused by charge trapping and develop a new method to reconstruct the spectra based on induced charge information from both anode and cathode strips. By applying this method, energy resolutions (FWHM) of 0.76 keV and 1.0 keV can be obtained at photon energies of 14 keV and 60 keV, respectively, if the energy difference between the anode and cathode is within 1 keV. Furthermore, the tail component at 60 keV is reduced, and the energy resolution of the 60 keV peak is improved from 2.4 keV to 1.5 keV (FWHM) if the energy difference is greater than 1 keV. In order to study the imaging performance, we constructed a simple imaging system using a 5 mm thick tungsten plate that has a pinhole with a diameter of 100 um. We utilize a Ba-133 radioisotope of 1 mm in diameter as a target source in combination with a 100 um slit made from 0.5 mm thickness tungsten. We imaged the Ba-133 source behind the 100 um slit using a 30 keV peak, with a 100 um pinhole placed at the center of the source-detector distance. By applying a charge sharing correction between strips, we have succeeded in obtaining a position resolution better than the strip pitch of 60 um.