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Precision of the calibration of the AXAF Engineering Test Article (VETA) mirrorsMeasurements of the VETA encircled energies have been performed at 5 energies within 16 radii ranging from 0.05 to 200 arcseconds. We report here on the analysis of the accuracy of those measurements. A common 'error tree' structure applies, and we present representative numbers for the larger terms. At 0.277, 1.5, and 2.07 keV, and for radii of 3 arcsec and larger, our measurements have estimated 1 sigma errors of 0.6 to 1.5 percent. Effects of measurement statistics and of the VETA test mount limit the accuracy at smaller angles, and modulation by the counter window support structure together with the imperfect position repeatability limit the accuracy for the 0.93 and 2.3 keV energies. We expect to mitigate these limitations when calibrating the complete AXAF flight mirror assembly.
Document ID
19930055615
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Schwartz, D. A.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Chartas, G.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Hughes, J. P.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Kellogg, E. M.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Zhao, Ping
(Smithsonian Astrophysical Observatory Cambridge, MA, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1993
Publication Information
Publication: In: Multilayer and grazing incidence X-ray(EUV optics for astronomy and projection lithography; Proceedings of the Meeting, San Diego, CA, July 19-22, 1992 (A93-39601 15-74)
Publisher: Society of Photo-Optical Instrumentation Engineers
Subject Category
Optics
Accession Number
93A39612
Funding Number(s)
CONTRACT_GRANT: NAS8-36123
Distribution Limits
Public
Copyright
Other

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