Imaging with the MART-LIME telescope on board the Spectrum X satellite

Details Imaging with the MART-LIME telescope on board the Spectrum X satellite Imaging with the MART-LIME telescope on board the Spectrum X satellite

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993spie.1948..109s&link_type=abstract

Proc. SPIE Vol. 1948, p. 109-118, Astroparticle Physics and Novel Gamma-Ray Telescopes, David B. Cline; Ed.

Physics

Scientific paper

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 in 1995. In particular, we discuss a 6 X 6 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.

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