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Conference Paper

Silicon Pore Optics X-ray mirror development for the ATHENA telescope

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Bradshaw,  Miranda
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Burwitz,  Vadim
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Citation

Collon, M. J., Babic, L., Barrière, N. M., Bayerle, A., Castiglione, L., Eenkhoorn, N., et al. (2021). Silicon Pore Optics X-ray mirror development for the ATHENA telescope. In Optics for EUV, X-Ray, and Gamma-Ray Astronomy X. doi:10.1117/12.2593505.


Cite as: https://hdl.handle.net/21.11116/0000-000A-AD16-B
Abstract
Athena, the largest space-based x-ray telescope to be flown by the European Space Agency, uses a new modular technology to assemble its 2.5 m diameter lens. The lens will consist of several hundreds of smaller x-ray lenslets, called mirror modules, which each consist of up to 76 stacked mirror pairs. Those mirror modules are arranged in circles in a large optics structure and will focus x-ray photons with an energy of 0.5 to 10 keV at a distance of 12 m onto the detectors of Athena. The point-spread function (PSF) of the optic shall achieve a half-energy width (HEW) of 5” at an energy of 1 keV, with an effective area of about 1.4 m2, corresponding to several hundred m2 of super-polished mirrors with a roughness of about 0.3 nm and a thickness of down to 110 µm. This paper will present the status of the technology and of the mass production capabilities, show latest performance results and discuss the next steps in the development.