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This paper describes the 2018 Planck CMB likelihoods, following a hybrid approach similar to the 2015 one, with different approximations at low and high multipoles, and implementing several methodological and analysis refinements.
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Keskitalo, R., Ashdown, M. A. J., Cabella, P., et al., Residual noise covariance for Planck low-resolution data analysis. 2010, A&A, 522, A94, 0906.0175
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Hivon, E., Mottet, S., & Ponthieu, N., QuickPol: Fast calculation of effective beam matrices for CMB polarization. 2017, A&A, 598, A25, 1608.08833
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Valiviita, J., Power Spectra Based Planck Constraints on Compensated Isocurvature, and Forecasts for LiteBIRD and CORE Space Missions. 2017, JCAP, 1704, 014, 1701.07039
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Henning, J. W., Sayre, J. T., Reichardt, C. L., et al., Measurements of the Temperature and E-mode Polarization of the CMB from 500 Square Degrees of SPTpol Data. 2018, ApJ, 852, 97, 1707.09353
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