1 January 1992 Imaging characteristics of the development model of the JET-X x-ray telescope
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The Joint European X-ray Telescope, ''JET-X'', which is to be the core instrument of the Russian Spectrum-X astrophysics mission in 1994, will study the 3-10 keV-band emission from X-ray sources. The instrument is configured as two identical coaligned X-ray imaging telescopes; focal plane imaging is furnished by a cooled CCD detector which yields both good spectral resolution and high spatial resolution. The mirror shells have Wolter I geometry, and are manufactured by means of an electroforming replication process.
© (1992) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Oberto Citterio, Oberto Citterio, Paolo Conconi, Paolo Conconi, Francesco Mazzoleni, Francesco Mazzoleni, Giancarlo Conti, Giancarlo Conti, Giancarlo Cusumano, Giancarlo Cusumano, Bruno Sacco, Bruno Sacco, Heinrich W. Braeuninger, Heinrich W. Braeuninger, Wolfgang Burkert, Wolfgang Burkert, } "Imaging characteristics of the development model of the JET-X x-ray telescope", Proc. SPIE 1546, Multilayer and Grazing Incidence X-Ray/EUV Optics, (1 January 1992); doi: 10.1117/12.51231; https://doi.org/10.1117/12.51231


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