Planck 2018 results

@article{Aghanim2020Planck2R,
  title={Planck 2018 results},
  author={Planck Collaboration N. Aghanim and Yashar Akrami and Mark Ashdown and J. Aumont and Carlo Baccigalupi and Mario Ballardini and Anthony J. Banday and Rita Bel{\'e}n Barreiro and Nicola Bartolo and Soumen Basak and Karim Benabed and J-Ph. Bernard and M. Bersanelli and Pawel Bielewicz and J. Richard Bond and Julian Borrill and Francois R. Bouchet and Francois Boulanger and Manfred Bucher and Carlo Burigana and Erminia Calabrese and Jean-François Cardoso and Julien Carron and Anthony Challinor and H. C. Chiang and Loris P. L. Colombo and C{\'e}line Combet and François Couchot and Brendan P. Crill and F. Cuttaia and Paolo Bernardis and Adriano de Rosa and Gianfranco de Zotti and Jacques Delabrouille and J. M. Delouis and Eleonora Di Valentino and Jose M. Diego and Olivier Dor'e and Marian Douspis and Anne Ducout and Xavier Dupac and George P. Efstathiou and Franz Elsner and Torsten A. Ensslin and Hans Kristian Eriksen and Edith Falgarone and Yabebal T. Fantaye and Fabio Finelli and Marco Frailis and Aur'elien A. Fraisse and Enrico Franceschi and Andrei V. Frolov and S. Galeotta and Silvia Galli and Ken Ganga and Ricardo T. G'enova-Santos and Martina Gerbino and Tuhin Ghosh and Joaquin Gonz'alez-Nuevo and Krzysztof M. G'orski and Steven Gratton and Alessandro Gruppuso and Jon E. Gudmundsson and Will Handley and Frode K. Hansen and Sophie Henrot-Versill'e and Diego Herranz and Eric Hivon and Z. Huang and Andrew H. Jaffe and William C Jones and Ata Karakci and Elina Keihanen and Reijo Keskitalo and Kimmo Kiiveri and J. Kim and Theodore Kisner and Nicoletta Krachmalnicoff and Martin Kunz and Hannu Kurki-Suonio and Guilaine Lagache and J-M. Lamarre and Anthony N. Lasenby and Massimiliano Lattanzi and Charles R. Lawrence and F. Levrier and Michele Liguori and Per B. Lilje and V. Lindholm and Marcos L'opez-Caniego and Y.-Z. Ma and Juan-Fancisco Mac'ias-P'erez and Gianmarco Maggio and Davide Maino and Nazzareno Mandolesi and Anna Mangilli and P. G. Martin and E. Mart'inez-Gonz'alez and S. Matarrese and Nicoletta Mauri and Jason D. McEwen and Alessandro Melchiorri and Aniello Mennella and Marina Migliaccio and Marc-Antoine Miville-Desch{\^e}nes and Diego Molinari and Andrea Moneti and Ludovic Montier and G. Morgante and Adam Moss and Sylvain Mottet and Paolo Natoli and Luca Pagano and Daniela Paoletti and Bruce Partridge and Guillaume Patanchon and Laura Patrizii and Olivier Perdereau and F. Perrotta and Valeria Pettorino and Francesco Piacentini and J-L. Puget and Jorg P. Rachen and Martin Reinecke and Mathieu Remazeilles and Alessandro Renzi and Graca M. Rocha and Gael M. Roudier and Laura Salvati and M. Sandri and Matti Savelainen and Douglas Scott and C. Sirignano and G. Sirri and Locke D Spencer and Rashid Sunyaev and A.-S. Suur-Uski and Jan Tauber and Daniele Tavagnacco and M. Tenti and Luigi Toffolatti and Maurizio Tomasi and M. Tristram and Tiziana Trombetti and Jussi Valiviita and F Vansyngel and Bartjan van Tent and L. Vibert and Patricio Vielva and Fabrizio Villa and Nicola Vittorio and Benjamin D. Wandelt and Ingunn Kathrine Wehus and Andrea Zonca},
  journal={Astronomy \& Astrophysics},
  year={2020}
}
The study of polarized dust emission has become entwined with the analysis of the cosmic microwave background (CMB) polarization in the quest for the curl-like B-mode polarization from primordial gravitational waves and the low-multipole E-mode polarization associated with the reionization of the Universe. We used the new Planck PR3 maps to characterize Galactic dust emission at high latitudes as a foreground to the CMB polarization and use end-to-end simulations to compute uncertainties and… 
Planck intermediate results. LIV. Polarized dust foregrounds
The study of polarized dust emission has become entwined with the analysis of the cosmic microwave background (CMB) polarization. We use new Planck maps to characterize Galactic dust emission as a
Dust polarization modelling at large scale over the northern Galactic cap using EBHIS and Planck data
The primary source of systematic uncertainty in the quest for the B-mode polarization of the Cosmic Microwave Background (CMB) introduced by primordial gravitational waves is polarized thermal
Characterization of the polarized synchrotron emission from Planck and WMAP data
The purpose of this work is to characterize the diffuse Galactic polarized synchrotron, which is the dominant CMB foreground emission at low frequency. We present EE, BB, and EB power spectra
Planck 2018 results. XII. Galactic astrophysics using polarized dust emission
We present 353 GHz full-sky maps of the polarization fraction p, angle ψ, and dispersion of angles S of Galactic dust thermal emission produced from the 2018 release of Planck data. We confirm that
Predictions of Cosmic Microwave Background Foreground Dust Polarization Using Velocity Gradients
The observations of fluctuations in the cosmic microwave background provide information about primordial inhomogeneities in the universe. However, the B-mode polarization of the inflationary
A Constraint on Primordial B-modes from the First Flight of the Spider Balloon-borne Telescope
We present the first linear polarization measurements from the 2015 long-duration balloon flight of Spider, which is an experiment that is designed to map the polarization of the cosmic microwave
Link between E–B polarization modes and gas column density from interstellar dust emission
Context. The analysis of the Planck polarization E and B mode power spectra of interstellar dust emission at 353 GHz recently raised new questions concerning the impact of Galactic foregrounds on the
Limits on Polarized Dust Spectral Index Variations for CMB Foreground Analysis
Using Planck polarization data, we search for and constrain spatial variations of the polarized dust foreground for cosmic microwave background (CMB) observations, specifically in its spectral index,
Full-sky, Arcminute-scale, 3D Models of Galactic Microwave Foreground Dust Emission Based on Filaments
We present the DustFilaments code, a full-sky model for the millimeter Galactic emission of thermal dust. Our model, composed of millions of filaments that are imperfectly aligned with the magnetic
Large-scale CIB maps from Planck
The cosmic infrared background (CIB) is a powerful probe of large-scale structure across a very large redshift range, consisting of unresolved redshifted infrared emission from dusty galaxies. It can
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References

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Planck 2018 results-XI. Polarized dust foregrounds
The study of polarized dust emission has become entwined with the analysis of the cosmic microwave background (CMB) polarization in the quest for the curl-like B-mode polarization from primordial
Planck intermediate results. LIV. Polarized dust foregrounds
The study of polarized dust emission has become entwined with the analysis of the cosmic microwave background (CMB) polarization. We use new Planck maps to characterize Galactic dust emission as a
Planck intermediate results L. Evidence of spatial variation of the polarized thermal dust spectral energy distribution and implications for CMB B-mode analysis
The characterization of the Galactic foregrounds has been shown to be the main obstacle in thechallenging quest to detect primordial B -modes in the polarized microwave sky. We make use of the Planck
Planck intermediate results - XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes
The polarized thermal emission from diffuse Galactic dust is the main foreground present in measurements of the polarization of the cosmic microwave background (CMB) at frequencies above 100 GHz. In
Statistical simulations of the dust foreground to cosmic microwave background polarization
The characterization of the dust polarization foreground to the cosmic microwave background (CMB) is a necessary step toward the detection of the B-mode signal associated with primordial
Planck 2018 results. XII. Galactic astrophysics using polarized dust emission
We present 353 GHz full-sky maps of the polarization fraction p, angle ψ, and dispersion of angles S of Galactic dust thermal emission produced from the 2018 release of Planck data. We confirm that
Planck intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarization
Planck has mapped the intensity and polarization of the sky at microwave frequencies with unprecedented sensitivity. We use these data to characterize the frequency dependence of dust emission. We
Planck 2015 results - XXV. Diffuse low-frequency Galactic foregrounds
We discuss the Galactic foreground emission between 20 and 100 GHz based on observations by Planck and WMAP. The total intensity in this part of the spectrum is dominated by free-free and spinning
Modelling and simulation of large-scale polarized dust emission over the southern Galactic cap using the GASS HI data
The Planck survey has quantified polarized Galactic foregrounds and established that they are a main limiting factor in the quest for the cosmic microwave background (CMB) B-mode signal induced by
S–PASS view of polarized Galactic synchrotron at 2.3 GHz as a contaminant to CMB observations
We have analyzed the southern sky emission in linear polarization at 2.3 GHz as observed by the S -band Polarization All Sky Survey (S-PASS). Our purpose is to study the properties of the diffuse
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