Share Email Print

Proceedings Paper

Active x-ray optics for the next generation of x-ray telescopes
Author(s): Carolyn Atkins; Hongchang Wang; Peter Doel; David Brooks; Samantha Thompson; Charlotte Feldman; Richard Willingale; Tim Button; Daniel Rodriguez Sanmartin; Dou Zhang; Ady James; Craig Theobald; Graham Willis; Andrew D. Smith
Format Member Price Non-Member Price
PDF $17.00 $21.00

Paper Abstract

The immediate future for X-ray astronomy is the need for high sensitivity, requiring large apertures and collecting areas, the newly combined NASA, ESA and JAXA mission IXO (International X-ray Observatory) is specifically designed to meet this need. However, looking beyond the next decade, there have been calls for an X-ray space telescope that can not only achieve this high sensitivity, but could also boast an angular resolution of 0.1 arc-seconds, a factor of five improvement on the Chandra X-ray Observatory. NASA's proposed Generation-X mission is designed to meet this demand; it has been suggested that the X-ray optics must be active in nature in order to achieve this desired resolution. The Smart X-ray Optics (SXO) project is a UK based consortium looking at the application of active/adaptive optics to both large and small scale devices, intended for astronomical and medical purposes respectively. With Generation-X in mind, an active elliptical prototype has been designed by the SXO consortium to perform point-to-point X-ray focussing, while simultaneously manipulating its optical surface to improve its initial resolution. Following the completion of the large scale SXO prototype, presented is an overview of the production and operation of the prototype, with emphasis on the X-ray environment and preliminary results.

Paper Details

Date Published: 5 May 2009
PDF: 10 pages
Proc. SPIE 7360, EUV and X-Ray Optics: Synergy between Laboratory and Space, 736008 (5 May 2009); doi: 10.1117/12.820446
Show Author Affiliations
Carolyn Atkins, Univ. College London (United Kingdom)
Hongchang Wang, Univ. College London (United Kingdom)
Diamond Light Source, Ltd. (United Kingdom)
Peter Doel, Univ. College London (United Kingdom)
David Brooks, Univ. College London (United Kingdom)
Samantha Thompson, Univ. College London (United Kingdom)
Charlotte Feldman, Univ. of Leicester (United Kingdom)
Richard Willingale, Univ. of Leicester (United Kingdom)
Tim Button, Univ. of Birmingham (United Kingdom)
Daniel Rodriguez Sanmartin, Univ. of Birmingham (United Kingdom)
Dou Zhang, Univ. of Birmingham (United Kingdom)
Ady James, Univ. College London (United Kingdom)
Craig Theobald, Univ. College London (United Kingdom)
Graham Willis, Univ. College London (United Kingdom)
Andrew D. Smith, STFC Daresbury Lab. (United Kingdom)

Published in SPIE Proceedings Vol. 7360:
EUV and X-Ray Optics: Synergy between Laboratory and Space
René Hudec; Ladislav Pina, Editor(s)

© SPIE. Terms of Use
Back to Top
Sign in to read the full article
Create a free SPIE account to get access to
premium articles and original research
Forgot your username?