Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998spie.3445..347c&link_type=abstract
Proc. SPIE Vol. 3445, p. 347-354, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy IX, Oswald H. Siegmund; Mark A. Gummin
Astronomy and Astrophysics
Astronomy
6
Scientific paper
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.
Burnham Jill A.
Cook Walter R.
Harrison Fiona A.
No associations
LandOfFree
Low-noise custom VLSI for CdZnTe pixel detectors does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Low-noise custom VLSI for CdZnTe pixel detectors, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Low-noise custom VLSI for CdZnTe pixel detectors will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-805544