کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
1828955 | 1027443 | 2008 | 5 صفحه PDF | دانلود رایگان |

Several successful development programs have been conducted on infra-red bolometer arrays at the “Commissariat à l’Energie Atomique” (CEA-LETI Grenoble) in collaboration with the CEA-SAp (Saclay); taking advantage of this background, we are now developing an X-ray spectro-imaging camera for next generation space astronomy missions, using silicon only technology. We have developed monolithic silicon micro-calorimeters based on implanted thermistors in an improved array that could be used for future space missions. The 8×8 array consists of a grid of 64 suspended pixels fabricated on a silicon on insulator (SOI) wafer. Each pixel of this detector array is made of a tantalum (Ta) absorber, which is bound by means of indium bump hybridization, to a silicon thermistor. The absorber array is bound to the thermistor array in a collective process. The fabrication process of our detector involves a combination of standard technologies and silicon bulk micro-machining techniques, based on deposition, photolithography and plasma etching steps. Finally, we present the results of measurements performed on these four primary building blocks that are required to create a detector array up to 32×32 pixels in size.
Journal: Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment - Volume 594, Issue 2, 1 September 2008, Pages 210–214