Kavli Affiliate: Adam Mantz | Summary:Galaxy cluster abundance provides a powerful probe of the $Λ$CDM model and enables precise constraints on cosmological parameters. Millimeter-wavelength surveys detect clusters through the Sunyaev-Zeldovich (SZ) effect, and are particularly effective at high redshifts. However, the SZ signal can be significantly contaminated by emission from Active Galactic Nuclei (AGN), particularly […]
Continue.. Clusters Hiding Under Millimeter Sources (CHUMS) I: Extreme CHUMS