Collaboration, Planck, Y. Akrami, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, A. J. Banday, et al. (2020) 2020. “Planck 2018 Results. XI. Polarized Dust Foregrounds”. \aap 641: A11. doi:10.1051/0004-6361/201832618.

Collaboration, Planck, Y. Akrami, F. Arroja, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, et al. (2020) 2020. “Planck 2018 Results. X. Constraints on Inflation”. \aap 641: A10. doi:10.1051/0004-6361/201833887.

Collaboration, Planck, N. Aghanim, Y. Akrami, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, et al. (2020) 2020. “Planck 2018 Results. VI. Cosmological Parameters”. \aap 641: A6. doi:10.1051/0004-6361/201833910.

Collaboration, Planck, N. Aghanim, Y. Akrami, F. Arroja, M. Ashdown, J. Aumont, C. Baccigalupi, et al. (2020) 2020. “Planck 2018 Results. I. Overview and the Cosmological Legacy of Planck”. \aap 641: A1. doi:10.1051/0004-6361/201833880.

Collaboration, Planck, N. Aghanim, Y. Akrami, M. I. R. Alves, M. Ashdown, J. Aumont, C. Baccigalupi, et al. 2020. “Planck 2018 Results. XII. Galactic Astrophysics Using Polarized Dust Emission”. \aap 641: A12. doi:10.1051/0004-6361/201833885.

Collaboration, Planck, N. Aghanim, Y. Akrami, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, et al. (2019) 2019. “Planck 2018 Results. V. CMB Power Spectra and Likelihoods”. ArXiv E-Prints, arXiv:1907.12875.

Collaboration, Planck, Y. Akrami, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, A. J. Banday, et al. (2019) 2019. “Planck 2018 Results. VII. Isotropy and Statistics of the CMB”. ArXiv E-Prints, arXiv:1906.02552.

Collaboration, Planck, Y. Akrami, F. Arroja, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, et al. (2019) 2019. “Planck 2018 Results. IX. Constraints on Primordial Non-Gaussianity”. ArXiv E-Prints, arXiv:1905.05697.

Collaboration, Planck, Y. Akrami, F. Argüeso, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, et al. (2018) 2018. “Planck Intermediate Results. LIV. The Planck Multi-Frequency Catalogue of Non-Thermal Sources”. \aap 619: A94. doi:10.1051/0004-6361/201832888.

Collaboration, Planck, N. Aghanim, Y. Akrami, M. I. R. Alves, M. Ashdown, J. Aumont, C. Baccigalupi, et al. (2018) 2018. “Planck 2018 Results. XII. Galactic Astrophysics Using Polarized Dust Emission”. ArXiv E-Prints, arXiv:1807.06212.

Collaboration, Planck, Y. Akrami, F. Arroja, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, et al. (2018) 2018. “Planck 2018 Results. X. Constraints on Inflation”. ArXiv E-Prints, arXiv:1807.06211.

Collaboration, Planck, N. Aghanim, Y. Akrami, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, et al. (2018) 2018. “Planck 2018 Results. VIII. Gravitational Lensing”. ArXiv E-Prints, arXiv:1807.06210.

Collaboration, Planck, N. Aghanim, Y. Akrami, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, et al. (2018) 2018. “Planck 2018 Results. VI. Cosmological Parameters”. ArXiv E-Prints, arXiv:1807.06209.

Collaboration, Planck, N. Aghanim, Y. Akrami, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, et al. (2018) 2018. “Planck 2018 Results. III. High Frequency Instrument Data Processing and Frequency Maps”. ArXiv E-Prints, arXiv:1807.06207.

Collaboration, Planck, Y. Akrami, F. Argüeso, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, et al. (2018) 2018. “Planck 2018 Results. II. Low Frequency Instrument Data Processing”. ArXiv E-Prints, arXiv:1807.06206.

Collaboration, Planck, Y. Akrami, F. Arroja, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, et al. (2018) 2018. “Planck 2018 Results. I. Overview and the Cosmological Legacy of Planck”. ArXiv E-Prints, arXiv:1807.06205.

Collaboration, Planck, Y. Akrami, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, A. J. Banday, et al. (2018) 2018. “Planck 2018 Results. XI. Polarized Dust Foregrounds”. ArXiv E-Prints, arXiv:1801.04945.

Collaboration, Planck, N. Aghanim, M. I. R. Alves, D. Arzoumanian, J. Aumont, C. Baccigalupi, M. Ballardini, et al. (2016) 2016. “Planck Intermediate Results. XLIV. Structure of the Galactic Magnetic Field from Dust Polarization Maps of the Southern Galactic Cap”. \aap 596: A105. doi:10.1051/0004-6361/201628636.

Collaboration, Planck, N. Aghanim, Y. Akrami, M. Ashdown, J. Aumont, M. Ballardini, A. J. Banday, et al. (2016) 2016. “Planck Intermediate Results. LI. Features in the Cosmic Microwave Background Temperature Power Spectrum and Shifts in Cosmological Parameters”. ArXiv E-Prints.

Collaboration, Planck, P. A. R. Ade, N. Aghanim, M. Arnaud, M. Ashdown, J. Aumont, C. Baccigalupi, et al. 2016. “Planck Intermediate Results. XXXVIII. E- and B-Modes of Dust Polarization from the Magnetized Filamentary Structure of the Interstellar Medium”. \aap 586: A141. doi:10.1051/0004-6361/201526506.

Collaboration, Planck, N. Aghanim, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, A. J. Banday, et al. 2017. “Planck Intermediate Results. L. Evidence of Spatial Variation of the Polarized Thermal Dust Spectral Energy Distribution and Implications for CMB B-Mode Analysis”. \aap 599: A51. doi:10.1051/0004-6361/201629164.

Collaboration, Planck, Y. Akrami, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, A. J. Banday, et al. 2016. “Planck Intermediate Results. LII. Planet Flux Densities”. ArXiv E-Prints.

Collaboration, Planck, N. Aghanim, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, A. J. Banday, et al. (2016) 2016. “Planck Intermediate Results. XLIX. Parity-Violation Constraints from Polarization Data”. \aap 596: A110. doi:10.1051/0004-6361/201629018.

Collaboration, Planck, N. Aghanim, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, A. J. Banday, et al. (2016) 2016. “Planck Intermediate Results. XLVIII. Disentangling Galactic Dust Emission and Cosmic Infrared Background Anisotropies”. \aap 596: A109. doi:10.1051/0004-6361/201629022.

Collaboration, Planck, N. Aghanim, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, A. J. Banday, et al. (2016) 2016. “Planck Intermediate Results. XLVI. Reduction of Large-Scale Systematic Effects in HFI Polarization Maps and Estimation of the Reionization Optical Depth”. \aap 596: A107. doi:10.1051/0004-6361/201628890.