Cosmology and source redshift distributions from combining radio weak lensing with CMB lensing Article Swipe
Alba Kalaja
,
I. Harrison
,
William R. Coulton
·
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.1088/1475-7516/2025/07/001
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.1088/1475-7516/2025/07/001
Measurements of weak gravitational lensing using the cosmic microwave background and the shapes of galaxies have refined our understanding of the late-time history of the Universe. While optical surveys have been the primary source for cosmic shear measurements, radio continuum surveys offer a promising avenue. Relevant radio sources, principally star-forming galaxies, have populations with higher mean redshifts and are less affected by dust extinction compared to optical sources. We focus on the future mid frequency SKA radio telescope and explore the cross-correlation between radio cosmic shear and CMB lensing convergence (γ R × κ CMB ). We investigate its potential in constraining the redshift distribution of radio galaxy samples and improving cosmological parameter constraints, including the neutrino sector. Using simulations of the first phase of the SKA and the Simons Observatory as a CMB experiment, we show how this γ R × κ CMB cross-correlation can provide ∼ 1 - 10% calibration of the overall radio source redshift distribution, which in turn can significantly tighten otherwise degenerate measurements of radio galaxy bias. For the case of the next-generation full SKA, we find that the full combination of auto- and cross-spectra between γ R and κ CMB becomes more powerful than the equivalent case using γ O from a Euclid -like survey, with constraints 30% tighter on ΛCDM parameters and narrower bounds on sum of neutrino masses at the level of ∼ 24%. These constraints are also driven by higher redshifts and larger scales than other galaxy-CMB cross-correlations, potentially shedding light on different physical models. Our findings demonstrate the potential of radio weak lensing in improving constraints, and establish the groundwork for future joint analyses of CMB experiments and radio continuum surveys.
Related Topics
Concepts
Physics
Cosmic microwave background
Cosmology
Redshift
Weak gravitational lensing
Astrophysics
Strong gravitational lensing
Gravitational lens
Observational cosmology
Astronomy
Dark energy
Galaxy
Anisotropy
Optics
Metadata
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All OpenAlex metadata
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https://doi.org/10.1088/1475-7516/2025/07/001Digital Object Identifier
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Cosmology and source redshift distributions from combining radio weak lensing with CMB lensingWork title
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articleOpenAlex work type
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2025Year of publication
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2025-07-01Full publication date if available
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Alba Kalaja, I. Harrison, William R. CoultonList of authors in order
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https://doi.org/10.1088/1475-7516/2025/07/001Publisher landing page
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hybridOpen access status per OpenAlex
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https://doi.org/10.1088/1475-7516/2025/07/001Direct OA link when available
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