Enhanced foreground mitigation in thermal SZ Compton-$y$ maps via polarization and deprojection
Jyothis Chandran, Mathieu Remazeilles, R. B. Barreiro

TL;DR
The paper introduces a hybrid NILC method that uses polarization data to better separate the thermal SZ signal from Galactic foregrounds in $y$-maps, reducing contamination and improving future survey analysis.
Contribution
It presents a novel hybrid NILC approach combining temperature and polarization maps, enhancing foreground removal in thermal SZ $y$-maps beyond previous methods.
Findings
$40\%$ reduction in Galactic dust correlation in $y$-maps.
Effective suppression of Galactic residuals in simulations for future surveys.
Improved CIB deprojection balancing noise and contamination.
Abstract
Residual foreground contamination in thermal Sunyaev-Zeldovich (SZ) Compton- parameter maps (-maps) arises mainly from Galactic emissions -- thermal dust and synchrotron radiation -- on large angular scales, and from cosmic infrared background (CIB) anisotropies on small scales. Unlike the thermal SZ effect, Galactic foregrounds are strongly polarized. Exploiting this distinction, we introduce a hybrid Needlet Internal Linear Combination (Hybrid NILC) method that combines Planck total-intensity and polarization frequency maps in the component-separation pipeline, thereby improving the suppression of residual Galactic emission while preserving the unpolarized SZ signal by leveraging the intrinsic and correlations of thermal dust and synchrotron. Using Planck PR4 data, we find that the Hybrid NILC -map exhibits about lower cross-correlation with the IRAS dust…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Radio Astronomy Observations and Technology · Astrophysics and Cosmic Phenomena
