Abstract
Advanced ACTPol is the second-generation polarization-sensitive upgrade to the \(6\, {\mathrm{m}}\) aperture Atacama Cosmology Telescope (ACT), which increased detector count and frequency coverage compared to the previous ACTPol receiver. Advanced ACTPol utilizes a new two-stage time-division multiplexing readout architecture based on superconducting quantum interference devices to achieve a multiplexing factor as high as 64 (rows), fielding a 2012 detector camera at 150/220 GHz and two 90/150 GHz cameras containing 1716 detectors each. In a time-domain system, aliasing introduces noise to the readout. In this work we present a figure of merit to measure this noise contribution and present measurements of the aliased noise fraction of the Advanced ACTPol receiver as deployed.
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Acknowledgements
The authors thank Max Fankhanel and Rodrigo Quiroga for helping with the site operations during the measurements presented here. Comments on this draft were received from two anonymous reviewers.
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Gallardo, P.A., Niemack, M.D., Austermann, J.E. et al. Characterization of Aliased Noise in the Advanced ACTPol Receiver. J Low Temp Phys 199, 762–770 (2020). https://doi.org/10.1007/s10909-020-02344-2
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DOI: https://doi.org/10.1007/s10909-020-02344-2