Laue Gamma-Ray Lenses for Space Astrophysics: Status and Prospects

<table>3<svg height="6.2750001" id="M233" style="vertical-align:-0.12375pt" version="1.1" viewbox="0 0 8.3500004 6.2750001" width="8.3500004" xmlns="http://www.w3.org/2000/svg">
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<g transform="translate(72,-66.98)">
<text transform="matrix(1,0,0,-1,-71.95,67.15)">
<tspan style="font-size: 11.21px; " x="0" y="0">𝜎</tspan>
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</svg> continuum sensitivity (<svg height="9.7875004" id="M234" style="vertical-align:-0.1575pt" version="1.1" viewbox="0 0 58.525002 9.7875004" width="58.525002" xmlns="http://www.w3.org/2000/svg">
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<tspan style="font-size: 11.21px; " x="0" y="0">Δ</tspan>
<tspan style="font-size: 11.21px; " x="8.0921764" y="0">𝐸</tspan>
<tspan style="font-size: 11.21px; " x="19.199305" y="0">=</tspan>
<tspan style="font-size: 11.21px; " x="29.992607" y="0">𝐸</tspan>
<tspan style="font-size: 11.21px; " x="37.995121" y="0">/</tspan>
<tspan style="font-size: 11.21px; " x="41.110943" y="0">2</tspan>
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</svg>) of the lens discussed in Section <a href="https://static.hindawi.com/articles/xroi/volume-2010/215375/figures/#sec4.5.2">4.5.2</a> for 100 ks observation time. Reprinted from [<a href="/journals/xroi/2010/215375/#B28">28</a>].</table>

X-Ray Optics and Instrumentation

Laue Gamma-Ray Lenses for Space Astrophysics: Status and Prospects

Figure 23