Abstract
A state-of-the-art compact Low-Energy X-ray Reflectometer is in
operation at DTU Space and is used to characterize x-ray coatings for
the optics of future spaceborne and ground-based telescopes. The
reflectometer is housed in a vacuum chamber and operates at 1.487 keV,
complimenting an existing 8.048 keV reflectometer. With a microfocus
source and plane-parabolic Kirkpatrick–Baez mirrors, the 0.5-mm wide
beam is collimated to <0.75 arcmin. An actively cooled 2D CCD yields
sample alignment precision of 26 μm in linear position and 0.18 arcmin
in angle. A multilayer monochromator provides a peak reflectance of
43.5% and beam purity > 99 % . The reflectometer has a 2θ range of
0 deg to 35 deg and dynamic range up to eight orders of magnitude.
Techniques are demonstrated to investigate the sample surface morphology
and we show the system’s capability to detect the presence of
atmospheric contaminants on coated mirrors.
Original language | English |
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Article number | 048004 |
Journal | Journal of Astronomical Telescopes, Instruments, and Systems |
Volume | 7 |
Issue number | 4 |
Number of pages | 19 |
ISSN | 2329-4124 |
DOIs | |
Publication status | Published - 2021 |
Keywords
- Grazing incidence
- LEXR
- Reflectometer validation
- Thin-film characterization
- X-ray optics
- X-ray reflectometry