Cross-correlating radio continuum surveys and CMB lensing: constraining redshift distributions, galaxy bias and cosmology

TL;DR

This study cross-correlates radio galaxy surveys with CMB lensing to constrain redshift distributions, galaxy bias, and cosmological parameters, achieving significant detection and providing insights into high-redshift galaxy populations.

Contribution

It demonstrates the use of CMB lensing cross-correlation with radio surveys to constrain redshift distributions and galaxy bias, improving cosmological parameter estimates.

Findings

Detected a ~5σ cross-correlation signal.

Preferred broader redshift tail than photometric estimates.

Placed constraints on σ₈ and galaxy bias.

Abstract

We measure the harmonic-space auto-power spectrum of the galaxy overdensity in the LOFAR Two-metre Sky Survey (LoTSS) First Data Release and its cross correlation with the map of the lensing convergence of the cosmic microwave background (CMB) from the Planck collaboration. We report a $\sim5\sigma$ detection of the cross-correlation. We show that the combination of the clustering power spectrum and CMB lensing cross-correlation allows us to place constraints on the high-redshift tail of the redshift distribution, one of the largest sources of uncertainty in the use of continuum surveys for cosmology. Our analysis shows a preference for a broader redshift tail than that predicted by the photometric redshifts contained in the LoTSS value added catalog, as expected, and more compatible with predictions from simulations and spectroscopic data. Although the ability of CMB lensing to constrain the width and tail of the redshift distribution could also be valuable for the analysis of current and future photometric weak lensing surveys, we show that its performance relies strongly on the redshift evolution of the galaxy bias. Assuming the redshift distribution predicted by the Square Kilometre Array Design simulations, we use our measurements to place constraints on the linear bias of radio galaxies and the amplitude of matter inhomogeneities $\sigma_8$, finding $\sigma_8=0.69^{+0.14}_{-0.21}$ assuming the galaxy bias scales with the inverse of the linear growth factor, and $\sigma_8=0.79^{+0.17}_{-0.32}$ assuming a constant bias.