Optics for EUV, X-Ray, and Gamma-Ray Astronomy IX 2019
DOI: 10.1117/12.2528664
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Performance and time stability of Ir/SiC X-ray mirror coatings for ATHENA

Abstract: Excellent X-ray reflective mirror coatings are key in order to meet the performance requirements of the ATHENA telescope. The baseline coating design of ATHENA was initially formed by Ir/B 4 C but extensive studies have identified critical issues with the stability of the B 4 C top layer which shows strong evolution over time and appears incompatible with the industrialization processes required for the production of mirror modules. Motivated by the need for a compatible top layer material to improve the teles… Show more

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Cited by 16 publications
(16 citation statements)
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“…They are required to have high performance in the energy range from 0.3 to 12 keV which is obtained by utilizing mirror substrates coated with a combination of high and low-Z materials. The current baseline coating for ATHENA is an Ir/SiC bilayer design optimized for the energy band in question 3,4 . Previous studies performed at DTU Space have established that the requirement for effective area can be achieved at both 1 keV and at 6 keV using a combination of bilayer coatings and/or linear graded multilayers 5,6 .…”
Section: Introduction and Science Objectivementioning
confidence: 99%
“…They are required to have high performance in the energy range from 0.3 to 12 keV which is obtained by utilizing mirror substrates coated with a combination of high and low-Z materials. The current baseline coating for ATHENA is an Ir/SiC bilayer design optimized for the energy band in question 3,4 . Previous studies performed at DTU Space have established that the requirement for effective area can be achieved at both 1 keV and at 6 keV using a combination of bilayer coatings and/or linear graded multilayers 5,6 .…”
Section: Introduction and Science Objectivementioning
confidence: 99%
“…In 2018 we commissioned a fully automated plate coating machine [19,20], discussed elsewhere in these proceedings. It is already able to coat up to 100.000 plates per year.…”
Section: Mass Production Preparationsmentioning
confidence: 99%
“…After wedging, a final processing step is necessary to boost the reflectivity of the SPO mirror plates. Metal coatings such as iridium and low-Z overcoatings such as SiC or B4C are currently under investigation as materials for obtaining the required X-ray reflectivity for Athena [16,17]. Patterning of the metal layer is needed to ensure bondability of the silicon mirror plates during the stacking process.…”
Section: Wedging and Coatingmentioning
confidence: 99%
“…This report details the process steps utilized in the manufacture of silicon mirror plates for SPO [10,[12][13][14][15][16][17][18]. The plate manufacturing process begins with double-sided polished 300 mm wafers, and ends with diced, ribbed, wedged, and coated SPO plates which can be subsequently stacked to form an optical unit [1,2].…”
Section: Introductionmentioning
confidence: 99%