X-ray characteristics of the Italian X-Ray Astronomy Satellite (SAX) flight mirror units

Details X-ray characteristics of the Italian X-Ray Astronomy Satellite (SAX) flight mirror units X-ray characteristics of the Italian X-Ray Astronomy Satellite (SAX) flight mirror units

Nov 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994spie.2279..101c&link_type=abstract

Proc. SPIE Vol. 2279, p. 101-109, Advances in Multilayer and Grazing Incidence X-Ray/EUV/FUV Optics, Richard B. Hoover; Arthur B

Physics

Optics

10

Scientific paper

The scientific instrumentation onboard the Italian X-ray Astronomy Satellite SAX foresees four X-ray Mirror Units operating in the energy range 0.1 - 10 KeV with spatial resolution of 1 arcmin Half Power Radius. The Mirror Units are composed of thirty nested confocal and coaxial very thin double cone mirrors made by a nickel electroforming replica technique. The paper presents the X-ray characterization data obtained at the PANTER facility on the Flight Mirror Units.

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