The Simons Observatory 220 and 280 GHz Focal-Plane Module: Design and Initial Characterization

The Simons Observatory 220 and 280 GHz Focal-Plane Module: Design and Initial Characterization

Abstract The Simons Observatory (SO) will detect and map the temperature and polarization of the millimeter-wavelength sky from Cerro Toco, Chile, across a range of angular scales, providing rich data sets for cosmological and astrophysical analysis. The SO focal planes will be tiled...

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Bibliographic Details
Main Authors: Healy, Erin, Dutcher, Daniel, Atkins, Zachary, Austermann, Jason, Choi, Steve K., Duell, Cody J., Duff, Shannon, Galitzki, Nicholas, Huber, Zachary B., Hubmayr, Johannes, Johnson, Bradley R., McCarrick, Heather, Niemack, Michael D., Sonka, Rita, Staggs, Suzanne T., Vavagiakis, Eve, Wang, Yuhan
Other Authors: MIT Kavli Institute for Astrophysics and Space Research
Format: Article
Language:English
Published: Springer US 2022
Online Access:https://hdl.handle.net/1721.1/146732

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