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The high throughput of the ROSAT X-ray telescope is largely dependent on the reflectance of the gold coating of the mirrors in the wavelength region 6 - 100 Å. In this context measurements of the reflectivity and scattering of soft X-rays at various wavelengths and reflection angles have been performed on a large variety of flat mirror samples. The effects related to coating technique and surface contamination are discussed.
W. Burkert,B. Aschenbach, andH. Brauninger
"Effects Of Mirror Contamination Observed In The ROSAT Programme", Proc. SPIE 0733, Soft X-Ray Optics and Technology, (1 January 1986); https://doi.org/10.1117/12.964913
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W. Burkert, B. Aschenbach, H. Brauninger, "Effects Of Mirror Contamination Observed In The ROSAT Programme," Proc. SPIE 0733, Soft X-Ray Optics and Technology, (1 January 1986); https://doi.org/10.1117/12.964913