The Simons Observatory: Large-Scale Characterization of 90/150 GHz TES Detector Modules

• Published in: arXiv.org
• Main Authors: Dutcher, Daniel, Duff, Shannon M, Groh, John C, Healy, Erin, Hubmayr, Johannes, Johnson, Bradley R, Jones, Dante, Keller, Ben, Lin, Lawrence T, Link, Michael J, Lucas, Tammy J, Morgan, Samuel, Seino, Yudai, Sonka, Rita F, Staggs, Suzanne T, Wang, Yuhan, Zheng, Kaiwen
• Format: Paper Journal Article
• Language: English
• Published: Ithaca Cornell University Library, arXiv.org 29.01.2024
• Subjects: Cosmic microwave background; Cryostats; Modules; Observatories; Physics - Instrumentation and Methods for Astrophysics; Sensor arrays; Sensors; Telescopes
• ISSN: 2331-8422
• DOI: 10.48550/arxiv.2311.05583

The Simons Observatory (SO) is a cosmic microwave background instrumentation suite being deployed in the Atacama Desert in northern Chile. The telescopes within SO use three types of dichroic transition-edge sensor (TES) detector arrays, with the 90 and 150 GHz Mid-Frequency (MF) arrays containing 65% of the approximately 68,000 detectors in the first phase of SO. All of the 26 required MF detector arrays have now been fabricated, packaged into detector modules, and tested in laboratory cryostats. Across all modules, we find an average operable detector yield of 84% and median saturation powers of (2.8, 8.0) pW with interquartile ranges of (1, 2) pW at (90, 150) GHz, respectively, falling within their targeted ranges. We measure TES normal resistances and superconducting transition temperatures on each detector wafer to be uniform within 3%, with overall central values of 7.5 mohm and 165 mK, respectively. Results on time constants, optical efficiency, and noise performance are also presented and are consistent with achieving instrument sensitivity forecasts.