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Proceedings Paper

Imaging with the MART-LIME telescope on board the Spectrum X satellite
Author(s): Marie Eleanore Soggiu; Angela Bazzano; Pietro Ubertini; L. Waldron
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Paper Abstract

Recent results obtained by balloon and satellite borne coded-mask instruments have been used to simulate the imaging performance of MART-LIME, a coded mask telescope to be flown on board the international observatory SPECTRUM-X-GAMMA on 1995. In particular, we discuss a 6x6 square degree field-of-view centered on the hard X-Ray source responsible for the high energy emission from Galactic Center, at energies above 30 keV. The contributions of GX1+4, GRS1758-25, Terzan 2, Tr 1741-322 and GX354-0 to this field-of-view are also considered. Deconvolved images obtained via the cross-correlation technique are presented. From these images, the limiting sensitivity of the telescope in a crowded sky field is correctly determined.

Paper Details

Date Published: 19 October 1993
PDF: 10 pages
Proc. SPIE 1948, Astroparticle Physics and Novel Gamma-Ray Telescopes, (19 October 1993); doi: 10.1117/12.161380
Show Author Affiliations
Marie Eleanore Soggiu, Istituto di Astrofisica Spaziale (Italy)
Angela Bazzano, Istituto di Astrofisica Spaziale (Italy)
Pietro Ubertini, Istituto di Astrofisica Spaziale (Italy)
L. Waldron, Istituto di Astrofisica Spaziale (Italy)


Published in SPIE Proceedings Vol. 1948:
Astroparticle Physics and Novel Gamma-Ray Telescopes
David B. Cline, Editor(s)

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