2007
DOI: 10.1117/12.733096
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Testing of the mirrors for the Constellation-X spectroscopy x-ray telescope with a refractive null

Abstract: We present an introduction to the use of a refractive null lens for testing grazing incidence x-ray mirrors for the Constellation-X mission. The singular role of mirror mounting in glass shell mirror metrology is also touched upon. We compare results achieved to date with mission requirements along with some of the unique properties of the null lens. Additionally, uses beyond mirror metrology are briefly discussed.

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Cited by 6 publications
(1 citation statement)
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“…In both cases, the OPD uncertainty introduced by the null optics can be estimated with a bottom up estimation of various error sources. For refractive null optics these errors include errors in alignment, index of refraction, and surface figure of the lens elements [19]. For CGH nulls, these errors include transmitted wavefront error of the CGH substrate and CGH pattern errors [17].…”
Section: Fizeau Interferometermentioning
confidence: 99%
“…In both cases, the OPD uncertainty introduced by the null optics can be estimated with a bottom up estimation of various error sources. For refractive null optics these errors include errors in alignment, index of refraction, and surface figure of the lens elements [19]. For CGH nulls, these errors include transmitted wavefront error of the CGH substrate and CGH pattern errors [17].…”
Section: Fizeau Interferometermentioning
confidence: 99%