Si/CdTe semiconductor compton camera

TL;DR: The Soft Gamma-ray Detector (SGD) on board the NeXT (Japanese future high energy astrophysics mission) is a Compton telescope with narrow field of view (FOV), which utilizes Compton kinematics to enhance its background rejection capabilities as mentioned in this paper.

TL;DR: The simulation results demonstrated the feasibility of the in vivo monitoring of the position and distribution of 225Ac radionuclide using the γ-rays in TAT.

TL;DR: The soft gamma-ray detector (SGD) on board NeXT (Japanese future high energy astrophysics mission) is a Compton telescope with narrow field of view (FOV), which utilizes Compton kinematics to enhance its background rejection capabilities.

TL;DR: In this paper, the authors developed analog ASICs for Cadmium Telluride (CdTe) pixel and line sensors for high energy astrophysics and other applications, which achieved an energy resolution of 4.9 keV (FWHM) for 59.5 keV gamma-rays combined with a Schottky CdTe diode detector.

TL;DR: The VA32TA as discussed by the authors achieves an energy resolution of 1.3 keV (FWHM) for 60 keV and 122 keV at 0 degree C with a DSSD and 1.7 keV with a CdTe detector.

TL;DR: In this paper, the Schottky CdTe diode detectors employing a guard-ring (GR) electrode are reported, and a detailed study of the characteristics of these devices working as a gamma-ray detector is presented.

TL;DR: The VA32TA as mentioned in this paper achieves an energy resolution of 1.3 keV for 60 and 122 keV at 0/spl deg/C with a DSSD and 1.7 keV with a CdTe detector.

TL;DR: In this article, the authors developed prototype modules for a low noise Double-sided Silicon Strip Detector (DSSD) system which is an essential element of the Semiconductor Multiple-Compton Telescope (SMCT).