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Design and characterization of the SPT-3G receiver

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arxiv 1809.00032 v1 pith:ZQCAPDLB submitted 2018-08-31 astro-ph.IM astro-ph.COphysics.ins-det

Design and characterization of the SPT-3G receiver

classification astro-ph.IM astro-ph.COphysics.ins-det
keywords receiverdesignphysicsspt-3ganisotropiesastroparticlebackgroundcamera
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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.

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Cited by 1 Pith paper

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  1. CMB Lensing Reconstruction Using Two Years of Temperature Data from the SPT-3G Summer Survey

    astro-ph.CO 2026-07 conditional novelty 5.0

    First CMB lensing reconstruction from two years of SPT-3G Summer temperature data yields A_comb = 1.015 ± 0.053 over 50 < L < 2000, consistent with Planck 2018 ΛCDM.