The Simons Observatory microwave SQUID multiplexing detector module design
Heather McCarrick, Erin Healy, Zeeshan Ahmed, Kam Arnold, Zachary, Atkins, Jason E. Austermann, Tanay Bhandarkar, Jim A. Beall, Sarah Marie, Bruno, Steve K. Choi, Jake Connors, Nicholas F. Cothard, Kevin D. Crowley,, Simon Dicker, Bradley Dober, Cody J. Duell, Shannon M. Duff

TL;DR
This paper introduces a novel microwave SQUID multiplexing detector module for the Simons Observatory, enabling higher multiplexing factors and validated performance that exceeds science requirements for cosmic microwave background observations.
Contribution
The paper presents a new focal-plane module design with significantly higher multiplexing factors using microwave SQUID multiplexing, validated through measurements with prototype bolometer arrays.
Findings
Achieved a 910 multiplexing factor with 95% yield.
Median white noise per channel is 65 pA/√Hz.
Projected impact on SO mapping speed is less than 8%.
Abstract
Advances in cosmic microwave background (CMB) science depend on increasing the number of sensitive detectors observing the sky. New instruments deploy large arrays of superconducting transition-edge sensor (TES) bolometers tiled densely into ever larger focal planes. High multiplexing factors reduce the thermal loading on the cryogenic receivers and simplify their design. We present the design of focal-plane modules with an order of magnitude higher multiplexing factor than has previously been achieved with TES bolometers. We focus on the novel cold readout component, which employs microwave SQUID multiplexing (mux). Simons Observatory will use 49 modules containing 60,000 bolometers to make exquisitely sensitive measurements of the CMB. We validate the focal-plane module design, presenting measurements of the readout component with and without a prototype detector array of 1728…
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