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Design and Assembly of SPT-3G Cold Readout Hardware
Design and Assembly of SPT-3G Cold Readout Hardware
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Design and Assembly of SPT-3G Cold Readout Hardware
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Design and Assembly of SPT-3G Cold Readout Hardware
Design and Assembly of SPT-3G Cold Readout Hardware

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Design and Assembly of SPT-3G Cold Readout Hardware
Design and Assembly of SPT-3G Cold Readout Hardware
Journal Article

Design and Assembly of SPT-3G Cold Readout Hardware

2018
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Overview
The third-generation upgrade to the receiver on the South Pole Telescope, SPT-3G, was installed at the South Pole during the 2016–2017 austral summer to measure the polarization of the cosmic microwave background. Increasing the number of detectors by a factor of 10 to ∼ 16 , 000 required the multiplexing factor to increase to 68 and the bandwidth of the frequency-division readout electronics to span 1.6–5.2 MHz. This increase necessitates low-thermal conductance, low-inductance cryogenic wiring. Our cold readout system consists of planar thin-film aluminum inductive–capacitive resonators, wired in series with the detectors, summed together, and connected to 4K SQUIDs by 10 - μ m -thick niobium–titanium (NbTi) broadside-coupled striplines. Here, we present an overview of the cold readout electronics for SPT-3G, including assembly details and characterization of electrical and thermal properties of the system. We report, for the NbTi striplines, values of R ≤ 10 - 4 Ω , L = 21 ± 1 nH , and C = 1.47 ± . 02 nF . Additionally, the striplines’ thermal conductivity is described by k A = 6.0 ± 0.3 T 0.92 ± 0.04 μ W mm K - 1 . Finally, we provide projections for cross talk induced by parasitic impedances from the stripline and find that the median value of percentage cross talk from leakage current is 0.22 and 0.09 % from wiring impedance.