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Cited article:

Using Two-frequency Dust Spectral Matching to Separate Galactic Synchrotron and Free–Free Temperature Foregrounds from the Cosmic Microwave Background

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CLASS Angular Power Spectra and Map-component Analysis for 40 GHz Observations through 2022

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The Astrophysical Journal 963 (2) 92 (2024)
https://doi.org/10.3847/1538-4357/ad1abf

COSMOGLOBE DR1 results

D. J. Watts, U. Fuskeland, R. Aurlien, A. Basyrov, L. A. Bianchi, M. Brilenkov, H. K. Eriksen, K. S. F. Fornazier, M. Galloway, E. Gjerløw, B. Hensley, L. T. Hergt, D. Herman, H. Ihle, K. Lee, J. G. S. Lunde, S. K. Nerval, M. San, N. O. Stutzer, H. Thommesen and I. K. Wehus
Astronomy & Astrophysics 686 A297 (2024)
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Statistical properties of galactic synchrotron temperature and polarization maps — a multi-frequency comparison

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Journal of Cosmology and Astroparticle Physics 2024 (01) 036 (2024)
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Sensitivity-improved Polarization Maps at 40 GHz with CLASS and WMAP Data

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The Simons Observatory: Combining cross-spectral foreground cleaning with multitracer B -mode delensing for improved constraints on inflation

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Tensor-to-scalar ratio forecasts for extended LiteBIRD frequency configurations

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Improved Constraints on Primordial Gravitational Waves using Planck , WMAP, and BICEP/ Keck Observations through the 2018 Observing Season

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Revisiting the Distance to Radio Loops I and IV Using Gaia and Radio/Optical Polarization Data

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Limits on Polarized Dust Spectral Index Variations for CMB Foreground Analysis

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