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We reconstruct the Cosmic Microwave Background (CMB) lensing potential on the latest Planck CMB PR4 (NPIPE) maps, which include slightly more data than the 2018 PR3 release, and implement quadratic estimators using more optimal filtering.
1902
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1911
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T. Okamoto and W. Hu, CMB lensing reconstruction on the full sky, Phys. Rev. D67
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M. Kesden, A. Cooray, and M. Kamionkowski, Lensing reconstruction with CMB temperature and polarization, Phys. Rev. D 67
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J. Torrado and A. Lewis, Cobaya: Code for Bayesian Analysis of hierarchical physical models, JCAP 05
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2007
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2007
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2008
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2016
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2016
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G. Pratten and A. Lewis, Impact of post-Born lensing on the CMB, JCAP 1608
2016
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2011
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A. Lewis, A. Challinor, and D. Hanson, The shape of the CMB lensing bispectrum, JCAP 03
2011
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2011
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P. A. R. Ade et al. (Planck), Planck 2013 results. XIV. Zodiacal emission, Astron. Astrophys. 571
2013
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2013
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T. Namikawa, D. Hanson, and R. Takahashi, Bias-hardened CMB lensing, MNRAS 431
2013
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2014
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P. A. R. Ade et al. (Planck), Planck 2015 results. XV. Gravitational lensing, Astron. Astrophys. 594
2015
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2017
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N. Aghanim et al. (Planck), Planck 2018 results. VIII. Gravitational lensing, Astron. Astrophys. 641
2018
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2018
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2018
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A. Zonca, L. Singer, D. Lenz, M. Reinecke, C. Rosset, E. Hivon, and K. Gorski, healpy: equal area pixelization and spherical harmonics transforms for data on the sphere in python, Journal of Open Source Software 4
2019
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V. Mossa et al. , The baryon density of the Universe from an improved rate of deuterium burning, Nature 587
2020
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2021
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N. Aghanim et al. (Planck), Planck 2018 results. VI. Cosmological parameters, Astron. Astrophys. 641
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2022
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