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H. McCarrick, G. Jones, Bradley Johnson, M. Abitbol, P. Ade, S. Bryan, P. Day, T. Essinger-Hileman, D. Flanigan, H. Leduc, M. Limon, P. Mauskopf, A.J. Miller, C. Tucker (2017)
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We report on the status of an ongoing effort to develop arrays of horn-coupled, polarization-sensitive microwave kinetic inductance detectors (MKIDs) that are each sensitive to two spectral bands between 125 and 280 GHz. These multi-chroic MKID arrays are tailored for next-generation, large-detector-count experiments that are being designed to simultaneously characterize the polarization properties of both the cosmic microwave background and Galactic dust emission. We present our device design and describe laboratory-based measurement results from two 23-element prototype arrays. From dark measurements of our first engineering array, we demonstrated a multiplexing factor of 92, showed the resonators respond to bath temperature changes as expected, and found that the fabrication yield was 100%. From our first optically loaded array, we found the MKIDs respond to millimeter-wave pulses; additional optical characterization measurements are ongoing. We end by discussing our plans for scaling up this technology to kilo-pixel arrays over the next 2 years.
Journal of Low Temperature Physics – Springer Journals
Published: Jul 30, 2018
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