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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
Places of action
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article
The HEXIT (High Energy X-ray Imaging Telescope) balloon-borne mission
Abstract
The HEXIT balloon-borne experiment is devoted to the validation of new-generation hard X-ray (20-70 keV) telescopes based on focusing multilayer optics and high Z solid-state detectors. Moreover, the gain achieved by means of concentration techniques will allow us the observation with unprecedented flux sensitivity and angular resolution of hard X-ray sources. The production of the multilayer mirrors is the Ni electroforming replication, while the detectors will be formed by arrays of CdZnTe pixels. It is also envisaged the possibility of hosting aboard a prototype of mosaic crystals Bragg concentrator prototype to increase the energy working range up to 140 keV. The attitude control, which is a particularly important subsystem since it has to match the high imaging capabilities of the telescope (30 arcsec), is based on a GPS antenna array working in parallel to a star/Sun-sensor system. The first HEXIT flight is scheduled in the 2005 year from the Trapani/Milo (Sicily) base operated by ASI....