Abstract
We study the effects of the Point Spread Function (PSF) on the performance of the Objective Crystal Spectrometer (OCS) of the SODART telescope. The advantage of OCS/SODART over XMM and AXAF instruments in studying of the diffuse sources is illustrated by modelling of the OCS/SODART observation of Tycho and Cas A Supernova Remnants (SNR).
Original language | English |
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Journal | Physica Scripta |
Volume | T77 |
Pages (from-to) | 139-141 |
ISSN | 0281-1847 |
Publication status | Published - 1998 |