We present new arcminute-resolution maps of the Cosmic Microwave Background
temperature and polarization anisotropy from the Atacama Cosmology Telescope, using …

The Simons Observatory (SO) is a new cosmic microwave background experiment being
built on Cerro Toco in Chile, due to begin observations in the early 2020s. We describe the …

We present constraints on extensions to the Λ CDM cosmological model from
measurements of the E-mode polarization autopower spectrum and the temperature-E …

Optimal analyses of many signals in the cosmic microwave background (CMB) require map-
level extraction of individual components in the microwave sky, rather than measurements at …

We present measurements of the E-mode (EE) polarization power spectrum and
temperature-E-mode (TE) cross-power spectrum of the cosmic microwave background using …

We present a measurement of the B-mode polarization power spectrum of the cosmic
microwave background (CMB) using data taken from 2014 July to 2016 December with 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 …

Observations of the millimeter sky contain valuable information on a number of signals,
including the blackbody cosmic microwave background (CMB), Galactic emissions, and the …

Extragalactic foregrounds are known to generate significant biases in temperature-based
cosmic microwave background (CMB) lensing reconstruction. Several techniques, which …

The combination and cross-correlation of the upcoming Euclid data with cosmic microwave
background (CMB) measurements is a source of great expectation since it will provide the …