Kirkpatrick-Baez (KB) and Lobster Eye (LE) Optics for Astronomical and Laboratory Applications

<table>Measurements of MFO LE optics with <svg height="12.3875" id="M120" style="vertical-align:-2.10374pt" version="1.1" viewbox="0 0 39.287498 12.3875" width="39.287498" xmlns="http://www.w3.org/2000/svg">
<g transform="matrix(1.25,0,0,-1.25,0,12.3875)">
<g transform="translate(72,-62.09)">
<text transform="matrix(1,0,0,-1,-71.95,64.24)">
<tspan style="font-size: 11.21px; " x="0" y="0">𝑓</tspan>
<tspan style="font-size: 11.21px; " x="9.3250561" y="0">=</tspan>
<tspan style="font-size: 11.21px; " x="20.118361" y="0">2</tspan>
<tspan style="font-size: 11.21px; " x="25.722361" y="0">5</tspan>
</text>
</g>
</g>
</svg> cm in the Palermo X-ray facility (measured FWHM of about 10 arcmin between 0.28 and 8 keV (Tichy et al., 2010b [<a href="/journals/xroi/2010/139148/#B117">74</a>]).</table>

X-Ray Optics and Instrumentation

fig56

Figure 56

Figure 56: Kirkpatrick-Baez (KB) and Lobster Eye (LE) Optics for Astronomical and Laboratory Applications 