Planck 2018 results - IV. Diffuse component separation
A&A, 641 (2020) A4
Published online: 2020-09-11
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From BEYONDPLANCK to COSMOGLOBE: Preliminary WMAP Q-band analysis
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The Second Radio Synchrotron Background Workshop: Conference Summary and Report
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QUIJOTE Scientific Results – XVII. Studying the anomalous microwave emission in the Andromeda Galaxy with QUIJOTE-MFI
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Nonparametric maximum likelihood component separation for CMB polarization data
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Morphological analysis of the polarized synchrotron emission with WMAP and Planck
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Probing cosmic inflation with the LiteBIRD cosmic microwave background polarization survey
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Probing the Cold Neutral Medium through H I Emission Morphology with the Scattering Transform
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Constraining the Bispectrum from Bouncing Cosmologies with Planck
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Characterizing cosmic birefringence in the presence of Galactic foregrounds and instrumental systematic effects
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Generative Models of Multichannel Data from a Single Example—Application to Dust Emission
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Estimation of the Full-sky Power Spectrum between Intermediate and Large Angular Scales from Partial-sky CMB Anisotropies Using an Artificial Neural Network
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Testing Cosmic Microwave Background Anomalies in E-mode Polarization with Current and Future Data
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Magnetic Misalignment of Interstellar Dust Filaments
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Multi-scale Physical Properties of NGC 6334 as Revealed by Local Relative Orientations between Magnetic Fields, Density Gradients, Velocity Gradients, and Gravity
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Detection of Dipole Modulation in CMB Temperature Anisotropy Maps from WMAP and Planck using Artificial Intelligence
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A foreground model-independent Bayesian CMB temperature and polarization signal reconstruction and cosmological parameter estimation over large angular scales
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Galaxy cluster rotation revealed in the MACSIS simulations with the kinetic Sunyaev–Zeldovich effect
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A hybrid map-Cℓ component separation method for primordial CMB B-mode searches
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CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope
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Foreground separation and constraints on primordial gravitational waves with the PICO space mission
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A possible common explanation for several cosmic microwave background (CMB) anomalies: A strong impact of nearby galaxies on observed large-scale CMB fluctuations
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Simulating a full-sky high resolution Galactic synchrotron spectral index map using neural networks
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Optimizing foreground mitigation for CMB lensing with combined multifrequency and geometric methods
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Optimal method for reconstructing polychromatic maps from broadband observations with an asymmetric antenna pattern
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Unveiling polarized emission from interstellar dust of the Large Magellanic Cloud with Planck
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A measurement of the scale of homogeneity in the early Universe
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The mixing of dust and gas in the high latitude translucent cloud MBM 40
Marco Monaci, Loris Magnani and Steven N. ShoreAstronomy & Astrophysics 668 L9 (2022)
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Detailed study of HWP non-idealities and their impact on future measurements of CMB polarization anisotropies from space
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The Simons Observatory: Galactic Science Goals and Forecasts
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Improved galactic foreground removal for B-mode detection with clustering methods
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B-mode forecast of CMB-Bhārat
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