Clusters of galaxies are the most recently assembled, massive, bound structures in the
Universe. As predicted by General Relativity, given their masses, clusters strongly deform …

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 …

ABSTRACT The Baryon Oscillation Spectroscopic Survey (BOSS) is designed to measure
the scale of baryon acoustic oscillations (BAO) in the clustering of matter over a larger …

We present a catalog of 68 galaxy clusters, of which 19 are new discoveries, detected via
the Sunyaev-Zel'dovich effect (SZ) at 148 GHz in the Atacama Cosmology Telescope (ACT) …

This biennial Review summarizes much of particle physics. Using data from previous
editions, plus 2158 new measurements from 551 papers, we list, evaluate, and average …

We present the most significant measurement of the cosmic microwave background (CMB)
lensing potential to date (at a level of 40σ), using temperature and polarization data from the …

We present the temperature power spectra of the cosmic microwave background (CMB)
derived from the three seasons of data from the Atacama Cosmology Telescope (ACT) at …

We present cosmological parameters derived from the angular power spectrum of the
cosmic microwave background (CMB) radiation observed at 148 GHz and 218 GHz over …

We present the Planck Sky Model (PSM), a parametric model for generating all-sky, few
arcminute resolution maps of sky emission at submillimetre to centimetre wavelengths, in …

Using high-resolution microwave sky maps made by the Atacama Cosmology Telescope,
we for the first time present strong evidence for motions of galaxy clusters and groups via …