DocumentCode
909906
Title
An Imaging Proportional Counter for a 0.1 to 10 keV X-Ray Telescope
Author
Gorenstein, Paul ; Fabricant, Daniel
Author_Institution
Harvard/Smithsonian Center for Astrophysics 60 Garden Street Cambridge, MA 02138
Volume
33
Issue
1
fYear
1986
Firstpage
741
Lastpage
744
Abstract
A xenon multi-wire position sensitive proportional counter with a high degree of differential spatial linearity (better than 50¿m) and long-term stability has been constructed and tested in detail. It is suitable for a 0.1 to 10 keV X-ray telescope such as AXAF, which it would share with detectors having better spatial and spectral resolution. Compared to other detectors, the larger format, higher quantum efficiency, and lower background of the PSPC makes it generally the most useful instrument for observations of diffuse cosmic X-ray sources and associations of sources more extended than a few tenths of a degree in diameter. Given the good spatial linearity the systematic uncertainty for source locations is finer than an arcsecond. The spatial resolution varies as 0.3 mm/E0-5 (keV) over the range 0.2-4 keV in accordance with theoretical limits determined by the size and the number of electrons in the primary charge cloud.
Keywords
Counting circuits; Linearity; Optical imaging; Spatial resolution; Stability; Telescopes; X-ray detection; X-ray detectors; X-ray imaging; Xenon;
fLanguage
English
Journal_Title
Nuclear Science, IEEE Transactions on
Publisher
ieee
ISSN
0018-9499
Type
jour
DOI
10.1109/TNS.1986.4337205
Filename
4337205
Link To Document