1988
DOI: 10.1117/12.948696
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Assembly Of The ROSAT Flight X-Ray Mirror System

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Cited by 4 publications
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“…Minor changes will also be made in the mirror system: in order to avoid spectral confusion by having more than one X-ray source in the direction of dispersion, the field of view is reduced from 2 degrees to 45 arcmin by a redesign of the optical stops. From the ROSAT experience it seems to be feasible to improve the on-axis angular resolution from 3" to 2" (half energy width) thereby increasing the spectral resolving power (Beckstette, 1988).…”
Section: The Spektrosat Conceptmentioning
confidence: 99%
“…Minor changes will also be made in the mirror system: in order to avoid spectral confusion by having more than one X-ray source in the direction of dispersion, the field of view is reduced from 2 degrees to 45 arcmin by a redesign of the optical stops. From the ROSAT experience it seems to be feasible to improve the on-axis angular resolution from 3" to 2" (half energy width) thereby increasing the spectral resolving power (Beckstette, 1988).…”
Section: The Spektrosat Conceptmentioning
confidence: 99%
“…From binary stars and black holes up to galaxy clusters and dark matter, high energetic events have been observed and analysed using powerful X-ray telescopes like e.g. Rosat, Chandra, and XMM-Newton [1,2,3], giving us detailed and unprecedented views of the high-energy universe.…”
Section: Introductionmentioning
confidence: 99%