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SPT-3G: A Multichroic Receiver for the South Pole Telescope
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SPT-3G: A Multichroic Receiver for the South Pole Telescope
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SPT-3G: A Multichroic Receiver for the South Pole Telescope
SPT-3G: A Multichroic Receiver for the South Pole Telescope
Journal Article

SPT-3G: A Multichroic Receiver for the South Pole Telescope

Hu
2018
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Overview
A new receiver for the South Pole Telescope, SPT-3G, was deployed in early 2017 to map the cosmic microwave background at 95, 150, and 220 GHz with ∼ 16,000 detectors, 10 times more than its predecessor SPTpol. The increase in detector count is made possible by lenslet-coupled trichroic polarization-sensitive pixels fabricated at Argonne National Laboratory, new 68 × frequency-domain multiplexing readout electronics, and a higher-throughput optical design. The enhanced sensitivity of SPT-3G will enable a wide range of results including constraints on primordial B-mode polarization, measurements of gravitational lensing of the CMB, and a galaxy cluster survey. Here we present an overview of the instrument and its science objectives, highlighting its measured performance and plans for the upcoming 2018 observing season.