Microwave SQUID multiplexer

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Transition-Edge Sensors (2005, background): “5 μΦ0/ √ Hz at 4K) and high bandwidth (∼ 100MHz) [158].”
PICO: Probe of Inflation and Cosmic Origins (2019, background): “dout focal planes comparable in size to PICO. Microwave frequency SQUID multiplexing can increase the multiplexing density and reduce the number of lines between the 4K and ambient temperature stages [308, 309]. Kinetic Inductance Detectors (KIDs) and Thermal KIDs (TKIDs) can further reduce the wire”
Neutrino Physics from the Cosmic Microwave Background and Large-Scale Structure (2013, unknown): “duction of the 500,000 detectors required by CMB-S4. Second TES devices are low-impedance (1 ) and can be multiplexed with modern-day Superconducting QUantum Interference Device (SQUID) multiplexers [96, 97, 98]. Multiplexed readouts are important for operating large detector arrays at sub-Kelvin te”
NIKA: A millimeter-wave kinetic inductance camera (2010, methodology): “This technique has been previously demonstrated by integrating superconducing quantum interference devices (SQUIDs) with a type of bolometer known as the transition edge sensor (TES) (Yoon et al. 2001; Irwin & Lehnert 2004; Irwin & Hilton 2005).”
Radio for hidden-photon dark matter detection (2014, background): “The salient ideas for the microwave SQUID readout technique are presented in [51].”