Cluster galaxies at redshift about 1.1 to 1.4 show lower IR-to-radio ratios than field galaxies at roughly 2 to 3 sigma, suggesting a possible environment-linked radio excess.
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Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon
Cluster galaxies at redshift about 1.1 to 1.4 show lower IR-to-radio ratios than field galaxies at roughly 2 to 3 sigma, suggesting a possible environment-linked radio excess.