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We quantify the calibration requirements for systematic uncertainties for next-generation ground-based observatories targeting the large-angle $B$-mode polarization of the Cosmic Microwave Background, with a focus on the Simons Observatory (SO).
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A. Suzuki, Multichroic Bolometric Detector Architecture for Cosmic Microwave Background Polarimetry Experiments , Ph.D. thesis, University of California, Berkeley, Jan., 2013
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C. Sheehy and A. Slosar, No evidence for dust B -mode decorrelation in Planck data , Phys. Rev. D 97
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S. M. Simon, J. A. Beall, N. F. Cothard, S. M. Duff, P. A. Gallardo, S. P. Ho et al., The Advanced ACTPol 27/39 GHz Array , Journal of Low Temperature Physics 193
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T. Matsumura, Y. Sakurai, N. Katayama, H. Sugai, H. Imada, H. Ishino et al., Prototype design and evaluation of the nine-layer achromatic half-wave plate for the LiteBIRD low frequency telescope , in Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX , J. Zmuidzinas and J.-R. Gao, eds., (Austin, United States), p. 142, SPIE, July, 2018, DOI
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P. Virtanen, R. Gommers, T. E. Oliphant, M. Haberland, T. Reddy, D. Cournapeau et al., SciPy 1.0: Fundamental Algorithms for Scientific Computing in Python , Nature Methods 17
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U. Seljak and M. Zaldarriaga, Signature of Gravity Waves in the Polarization of the Microwave Background , Phys. Rev. Lett. 78
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M. Kamionkowski, A. Kosowsky and A. Stebbins, A Probe of Primordial Gravity Waves and Vorticity , Phys. Rev. Lett. 78
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