Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE · 1998 · 22 citations · 6 references
EngineeringAnalog DesignImage SensorNoise ReductionCircuit SystemMixed-signal Integrated CircuitNoiseCdznte Pixel DetectorsInstrumentationPixelated Cdznte DetectorsIndium BumpElectrical EngineeringComputer EngineeringCosmic RaySignal Processing ChainSynchrotron RadiationMicroelectronicsSignal ProcessingElectronic InstrumentationOptoelectronics
A custom analog VLSI chip is being developed for the readout of pixelated CdZnTe detectors in the focal plane of an astronomical hard x-ray telescope. The chip is intended for indium bump bonding to a pixel detector having pitch near 0.5 mm. A complete precision analog signal processing chain, including charge sensitive preamplifier, shaping amplifiers and peak detect and hold circuit, is provided for each pixel. Here we describe the circuitry and discus the performance of a functional prototype fabricated in a 1.2 micrometers CMOS process at Orbit Semiconductor. Dynamic performance is found to be close to SPICE model predictions over a self-triggering range extending from 1 to 50 keV. Integral non-linearity and noise while acceptable ar not as god as predicted. Power consumption is only 250 uW per pixel. Layout and design techniques are discussed which permit successful self-triggering operation at the low 1 keV threshold.
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The Apollo gamma-ray spectrometer
T. Harrington, James Marshall, J. R. Arnold et al. · Nuclear Instruments and Methods · 1974 · 48 citations
Apollo Gamma-ray Spectrometer, Radiation Detection, Instrumentation +1
Peter H. Mao, Fiona A. Harrison, Yuriy Y. Platonov et al. · Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE · 1997 · 18 citations
Keisuke Tamura, Koujun Yamashita, Hideyo Kunieda et al. · Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE · 1997 · 15 citations