TL;DR
This paper introduces an extended baryonification model that efficiently predicts higher-order correlations in weak lensing and tSZ fields, enabling joint cosmological and baryonic parameter constraints from full-sky surveys.
Contribution
We develop a map-level baryonification method that models higher-order correlations in weak lensing and tSZ fields, fitting simulations and improving parameter constraints.
Findings
Model accurately fits higher-order moments in simulations.
Combining lensing and tSZ data improves constraints on cosmology and baryons.
Model is computationally efficient and publicly available.
Abstract
Semi-analytic methods can generate baryon-corrected fields from N-body simulations (``baryonification'') and are rapidly becoming a ubiquitous tool in modeling structure formation on non-linear scales. We extend this formalism to consistently model the weak lensing and thermal Sunyaev-Zeldovich (tSZ) fields directly on the full-sky, with an emphasis on higher-order correlations. We use the auto- and cross- th-order moments, with , as a summary statistic of the lensing and tSZ fields, and show that our model can jointly fit these statistics measured in IllustrisTNG to within measurement uncertainties, for scales above and across multiple redshifts. The model predictions change only minimally when including additional information from secondary halo properties, such as halo concentration and ellipticity. Each individual moment is dependent on…
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