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Johnson, B. R.; Flanigan, D.; Abitbol, M. H.; Ade, P. A. R.; Bryan, S.; Cho, H.-M.; Datta, R.; Day, P.; Doyle, S.; Irwin, K.; Jones, G.; Li, D.; Mauskopf, P.; McCarrick, H.; McMahon, J.; Miller, A.; Pisano, G.; Song, Y.; Surdi, H.; Tucker, C.
Journal of low temperature physics, 11/2018, Letnik: 193, Številka: 3-4Journal Article
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.
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JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
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in: SICRIS
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