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 |
|---|---|
| Journal | Physica Scripta |
| Volume | T77 |
| Pages (from-to) | 139-141 |
| ISSN | 0281-1847 |
| Publication status | Published - 1998 |