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Proceedings Paper

High-angular-resolution hard x-ray imager for the high-energy detector on board the Spectrum X-GAMMA satellite
Author(s): Pietro Ubertini; Angela Bazzano; L. Boccaccini; M. Federici; Massimo Frutti; G. Gianni; M. Manzan; R. Patriarca; Marie Eleanore Soggiu; S. Ugazio
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Paper Abstract

Consideration is given to a new type of position-sensitive MultiWire Proportional Counter proposed as the high-energy instrument for the Spectrum X-Gamma Satellite. Two of them are based on high-throughput X-ray optics, sensitive up to about 20 keV. The third one, MART-LIME, is the high-energy instrument to cover the band 5-150 keV. This X-ray observatory-class orbiter comprises three major coaligned instruments. The scientific objective of this hard X-ray telescope is to produce sky images with arcmin angular resolution and good spectral resolution and submilliCrab sensitivity, during a typical observation time of 100,000 sec. The MART-LIME experiment is expected to produce a breakthrough in high-energy astrophysics by means of deep observations over a wide field of view. The missions are to produce a complete hard X-ray catalog, which is still nonexistent at the milliCrab sensitivity level.

Paper Details

Date Published: 1 November 1990
PDF: 13 pages
Proc. SPIE 1344, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy, (1 November 1990); doi: 10.1117/12.23273
Show Author Affiliations
Pietro Ubertini, Istituto di Astrofisica Spaziale (Italy)
Angela Bazzano, Istituto di Astrofisica Spaziale (Italy)
L. Boccaccini, Istituto di Astrofisica Spaziale (Italy)
M. Federici, Istituto di Astrofisica Spaziale (Italy)
Massimo Frutti, Istituto di Astrofisica Spaziale (Italy)
G. Gianni, Istituto di Astrofisica Spaziale (Italy)
M. Manzan, Istituto di Astrofisica Spaziale (Italy)
R. Patriarca, Istituto di Astrofisica Spaziale (Italy)
Marie Eleanore Soggiu, Istituto di Astrofisica Spaziale (Italy)
S. Ugazio, Istituto di Astrofisica Spaziale (Italy)

Published in SPIE Proceedings Vol. 1344:
EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy
Oswald H. W. Siegmund; Hugh S. Hudson, Editor(s)

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