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Naji, M. |
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Motta, Antonella |
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Aletan, Dirar |
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Mohamed, Tarek |
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Ertürk, Emre |
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Taccardi, Nicola |
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Kononenko, Denys |
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Petrov, R. H. | Madrid |
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Alshaaer, Mazen | Brussels |
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Bih, L. |
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Casati, R. |
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Muller, Hermance |
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Kočí, Jan | Prague |
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Šuljagić, Marija |
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Kalteremidou, Kalliopi-Artemi | Brussels |
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Azam, Siraj |
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Ospanova, Alyiya |
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Blanpain, Bart |
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Ali, M. A. |
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Popa, V. |
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Rančić, M. |
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Ollier, Nadège |
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Azevedo, Nuno Monteiro |
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Landes, Michael |
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Rignanese, Gian-Marco |
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Cotroneo, Vincenzo
in Cooperation with on an Cooperation-Score of 37%
Topics
Publications (10/10 displayed)
- 2017Design and fabrication of adjustable x-ray optics using piezoelectric thin filmscitations
- 2017Thermal forming of glass substrates for adjustable optics (Conference Presentation)citations
- 2016Thermal forming of substrates for the x-ray surveyor telescopecitations
- 2013Sputter deposition of PZT piezoelectric films on thin glass substrates for adjustable x-ray opticscitations
- 2012Improving yield of PZT piezoelectric devices on glass substratescitations
- 2010The optics system of the New Hard X-ray Mission: design and developmentcitations
- 2009Design and development of the optics system for the NHXM Hard X-ray and Polarimetric Missioncitations
- 2008Simbol-X mirror module design scientific optimization.
- 2008The relation between the weight and the quality image in a X-ray telescope, with a particular regard to Simbol-X
- 2003The HEXIT (High Energy X-ray Imaging Telescope) balloon-borne mission
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document
Thermal forming of substrates for the x-ray surveyor telescope
Abstract
In this paper we review the progress and current status of thermal forming activities at SAO, highlighting the most relevant technical problems and the way to solve them. These activities are devoted to the realization of mirror substrates for the X-ray surveyor mission concept, an observatory with Chandra-like angular resolution and 30 times more effective area or larger. The technology under development at SAO is based on the deposition of piezoelectric material on the back of the substrates. About 8000 mirror segments, with initial quality of 10 arcseconds or better are required for the telescope....