Gas filled prototype of a CdZnTe pixel detector

CdZnTe pixel structures are currently the most promising detectors for the focal planes of hard X-ray telescopes, for astronomical observation in the range 5-100keV. In Sharma et al. (Proc. SPIE 3765 (1999) 822) and Ramsey et al. (Nucl. Instrum. Methods A 458 (2001) 55) we presented preliminary resu lts on the development of prototype 4 x 4 CdZnTe imaging detectors operated under vacuum. These pixel detectors were installed inside vacuum chambers on three-stage Peltier coolers providing detector temperatures down to -40 degreesC. A miniature sputter ion pump inside each chamber maintained the n ecessary vacuum of 10(-5)Torr. At a temperature of -20 degreesC we achieved an FWHM energy resolution of between 2% and 3% at 60 keV and approximate t o 15% at 5.9 keV; however, the dependency on temperature was weak and at +2 0 degreesC the respective resolutions were 3% and 20%. As the detectors cou ld be operated at room temperature without loss of their good characteristi cs it was possible to exclude the sputter ion pump and fill the chamber wit h dry nitrogen instead. We have tested a nitrogen-filled CdZnTe (5 x 5 x 1 mm(3)) prototype having 0.65 x 0.65 mm(2) readout pads on a 0.75 mm. pitch. The interpixel resistance at an applied voltage of 10 V was higher than 50 G Omega and the pixel leakage currents at room temperature with a bias of 200 V between each pad and the common electrode did not exceed 0.8 nA. The pixel detector inside the microassembly, which also contained the input sta ges of the preamplifiers, was installed on a Peltier cooler to maintain the detector temperature at +20 degreesC. To define real leakage currents of t he pixels in their switched-on state we have checked the voltage on the pre amplifiers feedback resistors. The resulting currents were 10-50 pA at a de tector bias of 500 V. Under test, the typical energy resolution per pixel a t +20 degreesC was approximate to3% at energy 59.6 keV and approximate to 2 0% at energy 5.9 keV, which are similar to the values obtained in the vacuu m prototype at room temperature (Nucl. Instrum. Methods A 458 (2001) 55). U sing the three stage Peltier cooler it is possible to cool the pixel detect or in the nitrogen atmosphere to 0 degreesC which would slightly improve th ese spectrometrical characteristics. Thus the conclusion here is that the u se of a nitrogen environment instead of a vacuum one did not cause any dete rioration of the characteristics of the CdZnTe imaging detector. (C) 2001 E lsevier Science Ltd. All rights reserved.