English

The 90 and 150 GHz universal focal-plane modules for the Simons Observatory

Instrumentation and Methods for Astrophysics 2021-12-03 v1

Abstract

The Simons Observatory (SO) is a suite of telescopes located in the Atacama Desert in Chile that will make sensitive measurements of the cosmic microwave background. There are a host of cosmological and astrophysical questions that SO is forecasted to address. The universal focal-plane modules (UFMs) populate the four SO telescope receiver focal planes. There are three varieties of UFMs, each of which contains transition-edge-sensor bolometers observing in two spectral bands between 30 and 290~GHz. We describe the novel mid-frequency UFMs, which target two of the six spectral bands at 90 and 150~GHz and are central to the cosmological goals of SO.

Keywords

Cite

@article{arxiv.2112.01458,
  title  = {The 90 and 150 GHz universal focal-plane modules for the Simons Observatory},
  author = {Heather McCarrick and Kam Arnold and Zachary Atkins and Jason Austermann and Tanay Bhandarkar and Steve K. Choi and Cody J. Duell and Shannon M. Duff and Daniel Dutcher and Nicholas Galitzk and Erin Healy and Zachary B. Huber and Johannes Hubmayr and Bradley R. Johnson and Michael D. Niemack and Joseph Seibert and Maximiliano Silva-Feaver and Rita F. Sonka and Suzanne T. Staggs and Eve M. Vavagiakis and Yuhan Wang and Zhilei Xu and Kaiwen Zheng and Ningfeng Zhu},
  journal= {arXiv preprint arXiv:2112.01458},
  year   = {2021}
}

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