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Updated: Dec 16, 2025

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Published on: April 1, 2020
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Development of Flat Silicon-Based Mesh Lens Arrays for Millimeter and Sub-millimeter Wave Astronomy
Giampaolo Pisano1, Jason Austermann2, James Beall2
1School of Physics and Astronomy, Cardiff University, Cardiff, UK.
Summary
Future cosmic microwave background instruments require advanced detector coupling. This study introduces novel flat metal-mesh lenslet arrays on silicon, offering improved performance and manufacturability for sensitive telescope optics.
Area of Science:
- Astrophysics
- Optical Engineering
- Materials Science
Background:
- Future cosmic microwave background (CMB) instruments demand highly sensitive focal plane arrays with thousands of detectors.
- Coupling detectors to telescope optics presents significant challenges for current technologies.
- Existing solutions like phased-array antenna-coupled detectors and lenslet-coupled planar antennas face limitations in electromagnetic performance, manufacturing, and scalability.
Purpose of the Study:
- To present a novel approach for fabricating flat metal-mesh lenslet arrays.
- To adapt existing mesh-filter technology for silicon substrates, improving mechanical compatibility with detector arrays.
- To evaluate the performance of these novel lenslets for millimeter-wavelength applications.
Main Methods:
- Utilizing established mesh-filter technology to create flat metal-mesh lenslet arrays.
- Adapting a polypropylene-based mesh lens design to silicon substrates.
- Fabricating and testing prototype pixels operating at millimeter wavelengths.
Main Results:
- Demonstrated a novel method for producing flat metal-mesh lenslet arrays on silicon.
- Achieved good mechanical integration with silicon-based detector arrays.
- Presented measured performance data for prototype pixels at millimeter wavelengths.
Conclusions:
- The novel metal-mesh lenslet arrays offer a promising solution for detector-optic coupling in CMB instruments.
- The silicon-based design addresses mechanical compatibility and manufacturability challenges.
- The technology shows potential for meeting the stringent requirements of next-generation CMB observatories.

