L. A. Page

TL;DR: In this article, a simple cosmological model with only six parameters (matter density, Omega_m h^2, baryon density, BH 2, Hubble Constant, H_0, amplitude of fluctuations, sigma_8, optical depth, tau, and a slope for the scalar perturbation spectrum, n_s) was proposed to fit the three-year WMAP temperature and polarization data.

TL;DR: In this paper, the first five years of the WMAP sky survey were used for full-sky temperature and polarization maps in five frequency bands from 23 to 94 GHz, and several new tests for systematic errors in the polarization data and conclude that Ka band data (33 GHz) is suitable for use in cosmological analysis, after foreground cleaning.

TL;DR: In this article, the angular power spectrum derived from the first-year Wilkinson Microwave Anisotropy Probe (WMAP) sky maps is presented, where the data are modestly contaminated by diffuse Galactic foreground emission.

TL;DR: The Atacama Cosmology Telescope (ACT) has been used to measure the angular power spectrum of the cosmic microwave background (CMB) radiation observed at 148 GHz and 218 GHz over 296 deg^2 with the ACT during its 2008 season as discussed by the authors.

TL;DR: In this article, the angular spectrum of the CMB was measured at 144 GHz from Cerro Toco in the Chilean altiplano, where the angular anisotropy of the spectrum was found to have the same properties as the spectrum at 30 and 40 GHz.