Paper
11 November 1994 X-ray optics for the JET-X experiment aboard the Spectrum X satellite
Oberto Citterio, Paolo Conconi, Mauro Ghigo, Ralf Loi, Francesco Mazzoleni, Ennio Poretti, Giancarlo Conti, T. Mineo, Bruno Sacco, Heinrich W. Braeuninger, Wolfgang Burkert
Author Affiliations +
Abstract
The Joint European X-Ray Telescope, JET-X, is one of the core instruments of the scientific payload of the Russian SPECTRUM-X astrophysics mission. JET-X is designed to study the emission from x-ray sources in the band of 0.3 - 10 KeV, particularly to meet primary scientific goals is cosmology and extragalactic astronomy. JET-X consists of two identical, coaligned x-ray telescopes, each with a spatial resolution of 30 arcsecond Half Energy Width or better. Focal plane imaging is provided by cooled x-ray sensitive CCD detectors which will combine high spatial resolution with good spectral resolution, with particular emphasis on high sensitivity and spectral resolution around the 7 KeV Fe-line complex. Each telescope is composed of a nested array of 12 mirrors with an aperture of 0.3 m and focal length of 3.5 m; the total effective area is 360 cm2 at 1.5 KeV and 140 cm2 at 8 KeV. The mirror shells have a Wolter I geometry and are manufactured by an electroforming replica process. The paper presents a status report concerning the development of the X-ray optics.
© (1994) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Oberto Citterio, Paolo Conconi, Mauro Ghigo, Ralf Loi, Francesco Mazzoleni, Ennio Poretti, Giancarlo Conti, T. Mineo, Bruno Sacco, Heinrich W. Braeuninger, and Wolfgang Burkert "X-ray optics for the JET-X experiment aboard the Spectrum X satellite", Proc. SPIE 2279, Advances in Multilayer and Grazing Incidence X-Ray/EUV/FUV Optics, (11 November 1994); https://doi.org/10.1117/12.193159
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Cited by 9 scholarly publications.
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KEYWORDS
Mirrors

X-ray optics

Image quality

Telescopes

Spatial resolution

X-ray telescopes

X-rays

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