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Proceedings Paper

Polarization sensitive Multi-Chroic MKIDs
Author(s): Bradley R. Johnson; Daniel Flanigan; Maximilian H. Abitbol; Peter A. R. Ade; Sean Bryan; Hsiao-Mei Cho; Rahul Datta; Peter Day; Simon Doyle; Kent Irwin; Glenn Jones; Sarah Kernasovskiy; Dale Li; Philip Mauskopf; Heather McCarrick; Jeff McMahon; Amber Miller; Giampaolo Pisano; Yanru Song; Harshad Surdi; Carole Tucker
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Paper Abstract

We report on the development of scalable prototype microwave kinetic inductance detector (MKID) arrays tai- lored for future multi-kilo-pixel experiments that are designed to simultaneously characterize the polarization properties of both the cosmic microwave background (CMB) and Galactic dust emission. These modular arrays are composed of horn-coupled, polarization-sensitive MKIDs, and each pixel has four detectors: two polariza- tions in two spectral bands between 125 and 280 GHz. A horn is used to feed each array element, and a planar orthomode transducer, composed of two waveguide probe pairs, separates the incoming light into two linear po- larizations. Diplexers composed of resonant-stub band-pass filters separate the radiation into 125 to 170 GHz and 190 to 280 GHz pass bands. The millimeter-wave power is ultimately coupled to a hybrid co-planar waveguide microwave kinetic inductance detector using a novel, broadband circuit developed by our collaboration. Elec- tromagnetic simulations show the expected absorption efficiency of the detector is approximately 90%. Array fabrication will begin in the summer of 2016.

Paper Details

Date Published: 19 July 2016
PDF: 12 pages
Proc. SPIE 9914, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII, 99140X (19 July 2016); doi: 10.1117/12.2233243
Show Author Affiliations
Bradley R. Johnson, Columbia Univ. (United States)
Daniel Flanigan, Columbia Univ. (United States)
Maximilian H. Abitbol, Columbia Univ. (United States)
Peter A. R. Ade, Cardiff Univ. (United Kingdom)
Sean Bryan, Arizona State Univ. (United States)
Hsiao-Mei Cho, SLAC National Accelerator Lab. (United States)
Rahul Datta, Univ. of Michigan (United States)
Peter Day, Jet Propulsion Lab. (United States)
Simon Doyle, Cardiff Univ. (United Kingdom)
Kent Irwin, Stanford Univ. (United States)
SLAC National Accelerator Lab. (United States)
Glenn Jones, Columbia Univ. (United States)
Sarah Kernasovskiy, Stanford Univ. (United States)
Dale Li, SLAC National Accelerator Lab. (United States)
Philip Mauskopf, Arizona State Univ. (United States)
Heather McCarrick, Columbia Univ. (United States)
Jeff McMahon, Univ. of Michigan (United States)
Amber Miller, Columbia Univ. (United States)
Giampaolo Pisano, Cardiff Univ. (United Kingdom)
Yanru Song, Stanford Univ. (United States)
Harshad Surdi, Arizona State Univ. (United States)
Carole Tucker, Cardiff Univ. (United Kingdom)


Published in SPIE Proceedings Vol. 9914:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII
Wayne S. Holland; Jonas Zmuidzinas, Editor(s)

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