论文信息 - Imaging characteristics of the development model of the JET-X x-ray telescope

Imaging characteristics of the development model of the JET-X x-ray telescope

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.

[1] Oberto Citterio,et al. Optical monitor for x-ray satellites , 1990, Astronomical Telescopes and Instrumentation.

[2] Oberto Citterio,et al. Optics for X-ray concentrators on board of the Astronomy Satellite SAX , 1986, Other Conferences.

[3] Bernd Aschenbach,et al. X-Ray Test Facilities At Max-Planck-Institut Garching , 1979, Other Conferences.

[4] Wolfgang Burkert,et al. Optics for the x-ray imaging concentrators aboard the x-ray astronomy satellite SAX. , 1988, Applied optics.