Characterization of Transition Edge Sensors for the Simons Observatory
Jason R. Stevens, Nicholas F. Cothard, Eve M. Vavagiakis, Aamir Ali,, Kam Arnold, Jason E. Austermann, Steve K. Choi, Bradley J. Dober, Cody Duell,, Shannon M. Duff, Gene C. Hilton, Shuay-Pwu Patty Ho, Thuong D. Hoang,, Johannes Hubmayr, Adrian T. Lee, Aashrita Mangu

TL;DR
This paper details the characterization and testing of transition edge sensors (TES) for the Simons Observatory, focusing on their cryogenic performance, electrical properties, and suitability for CMB observations.
Contribution
It provides detailed test results and analysis of prototype TES devices, informing the fabrication process for the observatory's detectors.
Findings
TES devices achieved required cryogenic temperatures
Electrical and thermal properties characterized successfully
Prototype performance meets design specifications
Abstract
The Simons Observatory is building both large (6 m) and small (0.5 m) aperture telescopes in the Atacama desert in Chile to observe the cosmic microwave background (CMB) radiation with unprecedented sensitivity. Simons Observatory telescopes in total will use over 60,000 transition edge sensor (TES) detectors spanning center frequencies between 27 and 285 GHz and operating near 100 mK. TES devices have been fabricated for the Simons Observatory by NIST, Berkeley, and HYPRES/SeeQC corporation. Iterations of these devices have been tested cryogenically in order to inform the fabrication of further devices, which will culminate in the final TES designs to be deployed in the field. The detailed design specifications have been independently iterated at each fabrication facility for particular detector frequencies. We present test results for prototype devices, with emphasis on NIST high…
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