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Deployment of Polarbear-2A

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Abstract

Polarbear-2A is the first of three receivers in the Simons array, a cosmic microwave background experiment located on the Atacama Plateau in Chile. Polarbear-2A was deployed and achieved the first light in January 2019 by mapping the microwave emission from planet observations. Commissioning work is underway to prepare the receiver for science observations.

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Notes

  1. The Nicholas Simons Telescope (North) and The Paul Simons Telescope (South).

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Acknowledgements

The Simons Array is supported by the Simons Foundation, the National Science Foundation grant (AST-0618398, AST-1212230, AST-1440338), NASA grant NNG06GJ08G, the Moore Foundation (GBMF4633), the Heising-Simons Foundation, Templeton Foundation grant number 58724, the Ax Center for Experimental Cosmology at UC San Diego, the U.S. Department of Energy, Office of Science, Office of High Energy Physics, JSPS KAKENHI Grant Number (JP26220709, JP15H03670, JP15H05891, JP18H01240), and JSPS Core-to-core Program, A. Advanced Research Networks.

Kavli IPMU authors are supported by World Premier International Research Center Initiative (WPI), MEXT, Japan.

The McGill authors acknowledge the Natural Sciences and Engineering Research Council and Canadian Institute for Advanced Research, National Commission for Scientific and Technological Research. The SISSA authors acknowledge support from the ASI-COSMOS network (cosmosnet.it) and the INDARK INFN Initiative.

The James Ax Observatory operates in the Parque Astronomico Atacama in Northern Chile under the auspices of the Comision Nacional de Investigacion Cientifica y Tecnologica de Chile (CONICYT).

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Correspondence to Daisuke Kaneko.

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Kaneko, D., Adachi, S., Ade, P.A.R. et al. Deployment of Polarbear-2A. J Low Temp Phys 199, 1137–1147 (2020). https://doi.org/10.1007/s10909-020-02366-w

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