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Proceedings Article

Fabrication and performance of blazed transmission gratings for x-ray astronomy

[+] Author Affiliations
Ralf K. Heilmann, Minseung Ahn, Mark L. Schattenburg

Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology (USA)

Proc. SPIE 7011, Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray, 701106 (July 14, 2008); doi:10.1117/12.789176
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From Conference Volume 7011

  • Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray
  • Martin J. L. Turner; Kathryn A. Flanagan
  • Marseille, France | June 23, 2008

abstract

We have developed a new type of soft x-ray diffraction grating. This critical-angle transmission (CAT) grating combines the advantages of traditional transmission gratings (low mass, extremely relaxed alignment and flatness tolerances) with those of x-ray reflection gratings (high efficiency due to blazing in the direction of grazing-incidence reflection, increased resolution due to the use of higher diffraction orders). In addition, grating spectrometers based on CAT gratings are well-suited for co-existence with high-energy focal plane microcalorimeter detectors as planned for the Constellation-X mission, since most high-energy x rays are neither absorbed nor deflected, and arrive at the telescope focus. We describe the CAT grating principle and design, and fabrication and x-ray diffraction efficiency results for a CAT grating with 1742 lines/mm. We have observed up to 46% diffraction efficiency in a single order, and up to 55% at blaze at extreme ultraviolet wavelengths. We present our recent fabrication and soft x-ray diffraction results for 200 nm-period (5000 lines/mm) gratings.

© (2008) COPYRIGHT SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only.
Citation

Ralf K. Heilmann ; Minseung Ahn and Mark L. Schattenburg
"Fabrication and performance of blazed transmission gratings for x-ray astronomy", Proc. SPIE 7011, Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray, 701106 (July 14, 2008); doi:10.1117/12.789176; http://dx.doi.org/10.1117/12.789176


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