arXiv · 2003.08949
Simons Observatory Microwave SQUID Multiplexing Readout -- Cryogenic RF Amplifier and Coaxial Chain Design
Abstract
The Simons Observatory (SO) is an upcoming polarization-sensitive Cosmic Microwave Background (CMB) experiment on the Cerro Toco Plateau (Chile) with large overlap with other optical and infrared surveys (e.g., DESI, LSST, HSC). To enable the readout of \bigO(10,000) detectors in each of the four telescopes of SO, we will employ the microwave SQUID multiplexing technology. With a targeted multiplexing factor of \bigO{(1,000)}, microwave SQUID multiplexing has never been deployed on the scale needed for SO. Here we present the design of the cryogenic coaxial cable and RF component chain that connects room temperature readout electronics to superconducting resonators that are coupled to Transition Edge Sensor bolometers operating at sub-Kelvin temperatures. We describe design considerations including cryogenic RF component selection, system linearity, noise, and thermal power dissipation.
Explore related subjects
Keep this discovery
Mayuri Sathyanarayana Rao, Maximiliano Silva-Feaver, Aamir Ali, Kam Arnold, Peter Ashton, Bradley J. Dober, Cody J. Duell, Shannon M. Duff, Nicholas Galitzki, Erin Healy, Shawn Henderson, Shuay-Pwu Patty Ho, Jonathan Hoh, Anna M. Kofman, Akito Kusaka, Adrian T. Lee, Aashrita Mangu, Justin Mathewson, Philip Mauskopf, Heather McCarrick, Jenna Moore, Michael D. Niemack, Christopher Raum, Maria Salatino, Trevor Sasse, Joseph Seibert, Sara M. Simon, Suzanne Staggs, Jason R. Stevens, Grant Teply, Robert Thornton, Joel Ullom, Eve M. Vavagiakis, Benjamin Westbrook, Zhilei Xu, Ningfeng Zhu. 2020-03-19. Simons Observatory Microwave SQUID Multiplexing Readout -- Cryogenic RF Amplifier and Coaxial Chain Design. https://doi.org/10.1007/s10909-020-02429-y
Cite the original work for its findings. Save a collection to share your selection of sources.