Paper
6 October 2011 ESA-led ATHENA/IXO optics development status
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Abstract
The International X-ray Observatory (IXO) is a candidate mission in the ESA Space Science Programme Cosmic Vision 1525, and was studied as a joint mission with NASA and JAXA. Considering the programmatic evolution of the international context, the mission is being reformulated as an ESA-led mission, under the name of ATHENA (Advanced Telescope for High Energy Astrophysics), with possible participation of NASA and JAXA. The mission is building on the novel Silicon Pore Optics (SPO) technology to achieve the required performance for this demanding astrophysics observatory. This technology is being developed by an industrial consortium, and involves also several research institutes [1-12]. A second optics technology, slumped glass optics (SGO), which is being developed in Europe and the USA, was the backup technology for IXO, and additionally work is progressing on improved reflective coatings and X-ray test facilities [13-17].
© (2011) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Marcos Bavdaz, Nicola Rando, Eric Wille, Kotska Wallace, Brian Shortt, Maximilien Collon, Coen van Baren, Giovanni Pareschi, Finn Christensen, Michael Krumrey, and Michael Freyberg "ESA-led ATHENA/IXO optics development status", Proc. SPIE 8147, Optics for EUV, X-Ray, and Gamma-Ray Astronomy V, 81470C (6 October 2011); https://doi.org/10.1117/12.893567
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Cited by 7 scholarly publications.
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KEYWORDS
Mirrors

Space telescopes

Telescopes

X-rays

X-ray optics

Silicon

Observatories

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