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A Multi-chroic Kinetic Inductance Detectors Array Using Hierarchical Phased Array Antenna

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Abstract

We present a multi-chroic kinetic inductance detector (KID) pixel design integrated with a broadband hierarchical phased-array antenna. Each low-frequency pixel consists of four high-frequency pixels. Four passbands are designed from 125 to 365 GHz according to the atmospheric windows. The lumped element KIDs consist of 100-nm thick AlMn inductors and Nb parallel plate capacitors with hydrogenated amorphous Si dielectric. Two different coupling structures are designed to couple millimeter-wave from microstrip lines to KIDs. The KID designs are optimized for a 10-m-class telescope at a high, dry site, for example, the Leighton Chajnantor Telescope. Preliminary measurement results using Al KIDs are discussed.

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Data Availability Statement

The datasets generated during and analysed during the current study are available from the corresponding author on reasonable request.

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Acknowledgements

This work has been partially funded by Department of Energy DE-SC0018126 and NASA 80NSSC18K0385.

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Correspondence to Shibo Shu.

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Shu, S., Beyer, A., Day, P. et al. A Multi-chroic Kinetic Inductance Detectors Array Using Hierarchical Phased Array Antenna. J Low Temp Phys 209, 330–336 (2022). https://doi.org/10.1007/s10909-022-02890-x

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