From Event: SPIE Astronomical Telescopes + Instrumentation, 2018
To enable the next-generation of bolometric cameras, we are developing the microwave SQUID multiplexer (μMUX). Upcoming receivers such as Simons Observatory, CCAT-prime, BICEP array, Ali-CPT, and CMB-S4 plan to instrument focal planes with 50,000-500,000 sensors. Sensor count is achieved by tiling many 150 mm-diameter densely packed detector arrays into these focal planes. The fabrication and quality of large-format bolometer arrays has been demonstrated and is now mature. In contrast, the readout technology required for next-generation receivers needs development. The sensitivity, low cross-talk, high multiplexing density, and small component size make the μMUX well-suited for this goal. In this approach, the TES signal modulates the inductance of an rf-SQUID that loads a high-Q microwave resonator. The coupled signal therefore modulates the microwave resonance frequency, which may be read out using homodyne techniques. By coupling each resonator to the same microwave feedline, many detectors can be read out on a single coaxial cable pair. The multiplexing density is in practice limited by signal bandwidth, allowable cross-talk, and the digitization bandwidth of room-temperature readout electronics.
We present the design and performance of a scalable 64-channel multiplexer chip optimized for bolometric applications. We utilize a new quarter wave resonator design that increases the physical linear density by a factor of two, therefore achieving a smaller footprint for simplified detector packaging. Measurements of this design show 100 kHz resonator bandwidth, uniform 1.8 MHz frequency spacing, and an input referred current noise of 35 pA/√Hz that is well below the level of an optimized, background-limited TES bolometer. Using 8 daisy-chained and frequency scaled chips, we create a 512-channel multiplexer and use it to readout a 512 TES-bolometer array. We present the results of this large-scale μMUX demonstration including system yield, signal cross-talk, and an analysis of noise in various TES bias configurations. The result demonstrates the multiplexing density required to read out 2,000 sensors between 4-8 GHz.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Bradley Dober, Zeeshan Ahmed, Jason Austermann, Daniel Becker, Douglas A. Bennett, David Brown, Saptarshi Chaudhuri, Hsiao-Mei Sherry Cho, John M. D'Ewart, Shannon Duff, John E. Dusatko, Sofia Fatigoni, Josef C. Frisch, Johnathon D. Gard, Mark Halpern, Shawn W. Henderson, Gene C. Hilton, Johannes Hubmayr, Kent D. Irwin, Ethan D. Karpel, Sarah S. Kernasovskiy, John A. B. Mates, Carl D. Reintsema, Michael Vissers, Leila R. Vale, Joel Ullom, Stephen E. Kuenstner, Chao-Lin Kuo, Dale Li, Stephen R. Smith, Daniel D. Van Winkle, Betty A. Young, and Cyndia Yu, "Readout demonstration of 512 TES bolometers using a single microwave SQUID multiplexer (Conference Presentation)," Proc. SPIE 10708, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX, 1070818 (Presented at SPIE Astronomical Telescopes + Instrumentation: June 14, 2018; Published: 10 July 2018); https://doi.org/10.1117/12.2314231.5807231875001.