Environment is one of the primary drivers of galaxy evolution; via multiple mechanisms, it
can control the critical process of transforming galaxies from star forming to quiescent …

We present a catalog of 4195 optically confirmed Sunyaev–Zel'dovich (SZ) selected galaxy
clusters detected with signal-to-noise ratio> 4 in 13,211 deg 2 of sky surveyed by the …

We present the first cosmological study of a sample of eROSITA clusters, which were
identified in the eROSITA Final Equatorial Depth Survey (eFEDS). In a joint selection on X …

Galaxy clusters are the most massive gravitationally bound structures in the Universe,
comprising thousands of galaxies and pervaded by a diffuse, hot intracluster medium (ICM) …

We present a detailed overview of the science goals and predictions for the Prime-Cam
direct-detection camera–spectrometer being constructed by the CCAT-prime collaboration …

Context. Inferences about dark matter, dark energy, and the missing baryons all depend on
the accuracy of our model of large-scale structure evolution. In particular, with cosmological …

We present a new pipeline for the efficient generation of synthetic observations of the
extragalactic microwave sky, tailored to large ground-based CMB experiments such as the …

We forecast the number of galaxy clusters that can be detected via the thermal Sunyaev–
Zel'dovich (tSZ) signals by future cosmic microwave background (CMB) experiments …

Clusters of galaxies can be used as powerful probes to study astrophysical processes on
large scales, test theories of the growth of structure, and constrain cosmological models. The …

We present an extensive ALMA spectroscopic follow-up programme of the structure
SPT2349–56, one of the most actively star-forming protocluster cores known, to identify …