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The fabrication of the Technology Mirror Assembly (TMA) is complete, and performance predictions were made based upon mechanical and visible light measurements of the surface properties. An X-ray calibration program has been executed, and a preliminary analysis of a portion of the data is presented. The X-ray image distribution results are in reasonable agreement with the performance predictions which were calculated prior the start of the X-ray tests. The measured X-ray imaging performance approaches that expected for the Advanced X-ray Astrophysics Facility (AXAF).
Leon Van Speybroeck,Paul Reid,Daniel Schwartz, andJames Bilbro
"Predicted And Preliminary Evaluation Of The X-Ray Performance Of The AXAF Technology Mirror Assembly", Proc. SPIE 1160, X-Ray/EUV Optics for Astronomy and Microscopy, (28 July 1989); https://doi.org/10.1117/12.962631
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Leon Van Speybroeck, Paul Reid, Daniel Schwartz, James Bilbro, "Predicted And Preliminary Evaluation Of The X-Ray Performance Of The AXAF Technology Mirror Assembly," Proc. SPIE 1160, X-Ray/EUV Optics for Astronomy and Microscopy, (28 July 1989); https://doi.org/10.1117/12.962631