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Conference paper

XSPECT telescopes on the SRG: optical performance

From

National Space Institute, Technical University of Denmark1

Astrophysics, National Space Institute, Technical University of Denmark2

Mechanical Engineering, National Space Institute, Technical University of Denmark3

Sunclimate, National Space Institute, Technical University of Denmark4

The XSPECT, thin foil, multiply nested telescope on SRG has been designed to achieve a large effective area at energies between 6 and 15 keV. The design goal for the angular resolution is 2 arcmin (HPD). Results of foil figure error measurements are presented. A ray tracing analysis was performed including results of earlier scattering measurements and the foil determination.

The results of the analysis are compared with test measurements with X rays and show that there is a larger spread in the PSF than the model can account for. The decrease in effective area due to scattering is estimated to be 30% when the photons that scatter more than 6 arcmin are regarded as lost.

The vignetting at off-axis angles leads to an effective area at the edge of the FOV which is 15% of that of an on-axis source.

Language: English
Year: 1994
Pages: 526-531
Proceedings: Advances in Multilayer and Grazing Incidence X-Ray/EUV/FUV Optics
ISSN: 1996756x and 0277786x
Types: Conference paper
DOI: 10.1117/12.193167
ORCIDs: Westergaard, Niels Jørgen Stenfeldt , Christensen, Finn Erland and Nørgaard-Nielsen, Hans Ulrik

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