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Proceedings ArticleDOI

Fabrication of single crystal silicon mirror substrates for X-ray astronomical missions

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TLDR
In this article, the authors describe the early pursuit of suitable fabrication technologies for the mass production of sub-arcsecond angular resolution single-crystal silicon mirror substrates for X-ray telescopes.
Abstract
The advancement of X-ray astronomy largely depends on technological advances in the manufacturing of X-ray optics. Future X-ray astronomy missions will require thousands of nearly perfect mirror segments to produce an X-ray optical assembly with < 5 arcsecond resolving capability. Present-day optical manufacturing technologies are not capable of producing thousands of such mirrors within typical mission time and budget allotments. Therefore, efforts towards the establishment of a process capable of producing sufficiently precise X-ray mirrors in a time-efficient and cost-effective manner are needed. Single-crystal silicon is preferred as a mirror substrate material over glass since it is stronger and free of internal stress, allowing it to retain its precision when cut into very thin mirror substrates. This paper details our early pursuits of suitable fabrication technologies for the mass production of sub-arcsecond angular resolution single-crystal silicon mirror substrates for X-ray telescopes.

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Citations
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Journal ArticleDOI

Material removal characteristics of full aperture optical polishing process

TL;DR: In this paper, a good control and systematic understanding of polishing process and its parameters are required to achieve the required optical surface parameters, to exploit the process to the extent, it is must to have a scientific understanding of material removal behavior.
Proceedings ArticleDOI

Progress on the fabrication of lightweight single-crystal silicon x-ray mirrors

TL;DR: In this article, a process for producing high resolution and lightweight X-ray mirror segments at low cost and with high throughput was developed at NASA Goddard Space Flight Center (GSFC).
Proceedings ArticleDOI

Fabrication of lightweight silicon x-ray mirrors for high-resolution x-ray optics

TL;DR: In this article, the authors report an overview of the X-ray mirror manufacturing process and the most recent results, including traditional grinding, lapping, and polishing methods adapted to Xray mirror geometry.
Proceedings ArticleDOI

Preserving accurate figures in coating and bonding mirrors for lightweight x-ray telescopes

TL;DR: In this paper, the most recent two test modules achieving the intermediate goal of 10 arc-second resolution were presented, and the results from tests of bonding mirrors onto experimental strongbacks, as well as the sensitivity on bonding procedure, bond parameters and environment were presented.
References
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Proceedings ArticleDOI

Imaging performance of the XMM-Newton x-ray telescopes

TL;DR: In this paper, the in-orbit imaging performance of the three X-ray telescopes on board of the Xray astronomy observatory XMM-Newton is compared with the performance measured on ground at the MPE PANTER test facility.
Journal ArticleDOI

Chandra x-ray optics

TL;DR: The Chandra X-ray Observatory as mentioned in this paper is an observatory designed to study the x-ray emission from all categories of astronomical objects-from comets, planets, and normal stars to quasars, galaxies, and clusters of galaxies.
Proceedings ArticleDOI

The International X-ray Observatory

TL;DR: The International X-ray Observatory (IXO) as discussed by the authors is a joint ESA-JAXA-NASA effort to address fundamental and timely questions in astrophysics: What happens close to a black hole? How did supermassive black holes grow? What is the connection between these processes?
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