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We present a new pipeline for the efficient generation of synthetic observations of the extragalactic microwave sky, tailored to large ground-based CMB experiments such as the Simons Observatory, Advanced ACTPol, SPT-3G, and CMB-S4.
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L. D. Shaw, D. H. Rudd and D. Nagai, Deconstructing the Kinetic SZ Power Spectrum , ApJ 756
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N. Battaglia, The tau of galaxy clusters , JCAP 8
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