Paper
1 January 1992 Calibration of the verification engineering test article-I for AXAF using the VETA-I x-ray detection system
Edwin M. Kellogg, Roger J. V. Brissenden, Kathryn A. Flanagan, Mark D. Freeman, John P. Hughes, Mark T. Jones, Malin Ljungberg, Phillip J. McKinnon, William A. Podgorski, Daniel A. Schwartz, Martin V. Zombeck
Author Affiliations +
Abstract
Advanced X-ray Astrophysics Facility (AXAF) X-ray optics testing is conducted by VETA-I, which consists of six nested Wolter type I grazing-incidence mirrors; VETA''s X-ray Detection System (VXDS) in turn measures the imaging properties of VETA-I, yielding FWHM and encircled energy of the X-ray image obtained, as well as its effective area. VXDS contains a high resolution microchannel plate imaging X-ray detector and a pinhole scanning system in front of proportional-counter detectors. VETA-I''s X-ray optics departs from the AXAF flight configuration in that it uses a temporary holding fixture; its mirror elements are not cut to final length, and are not coated with the metal film used to maximize high-energy reflection.
© (1992) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Edwin M. Kellogg, Roger J. V. Brissenden, Kathryn A. Flanagan, Mark D. Freeman, John P. Hughes, Mark T. Jones, Malin Ljungberg, Phillip J. McKinnon, William A. Podgorski, Daniel A. Schwartz, and Martin V. Zombeck "Calibration of the verification engineering test article-I for AXAF using the VETA-I x-ray detection system", Proc. SPIE 1546, Multilayer and Grazing Incidence X-Ray/EUV Optics, (1 January 1992); https://doi.org/10.1117/12.51221
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Cited by 4 scholarly publications.
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KEYWORDS
X-rays

X-ray optics

Sensors

X-ray detectors

Mirrors

Grazing incidence

Calibration

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