Sobrin, Joshua A., Ade, Peter ![]() ![]() ![]() |
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Official URL: http://dx.doi.org/10.1117/12.2314366
Abstract
The SPT-3G receiver was commissioned in early 2017 on the 10-meter South Pole Telescope (SPT) to map anisotropies in the cosmic microwave background (CMB). New optics, detector, and readout technologies have yielded a multichroic, high-resolution, low-noise camera with impressive throughput and sensitivity, offering the potential to improve our understanding of inflationary physics, astroparticle physics, and growth of structure. We highlight several key features and design principles of the new receiver, and summarize its performance to date.
Item Type: | Conference or Workshop Item (Paper) |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
ISSN: | 0277-786X |
Date of First Compliant Deposit: | 13 December 2019 |
Date of Acceptance: | 24 August 2018 |
Last Modified: | 26 Oct 2022 08:27 |
URI: | https://orca.cardiff.ac.uk/id/eprint/127519 |
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