Context
X-ray
telescopes use grazing incidence mirrors to produce a true image of the
X-ray sky. We know of only 3 basic geometries that can be used to focus
soft X-rays and produce an image: Wolter I, Kirkpatrick-Baez and
lobster eye, and the choice of geometry depends on the application and
the technology available to produce and assemble the mirrors. Because
they must conform to one of these 3 geometries the performance
characteristics of X-ray telescopes are somewhat different from
instruments used in other wavebands. |
Bibliography
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Wolter, H.,Annalen der Physik,1952,445,1-2,94-114
Wiley Online Library
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images by X-rays"
Kirkpatrick, P. and Baez, A.V.,J. Opt. Soc. Am.,38,9,766-773,1948
Optical Society of America
BibCode: kirkpatrick1948formation
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http://chandra.harvard.edu/about/telescope_system.html
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Telescope"
Burrows, D.N. et al., Space Science Reviews,2005,120,165-195
BibCode: 2005SSRv..120..165B
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Willingale, R., Pareschi, G., Christensen, F., den Herder, J-W., arXiv,
2013
BibCode: arXiv:1307.1709
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