This review covers the measurements related to the extragalactic background light intensity
from γ-rays to radio in the electromagnetic spectrum over 20 decades in wavelength. The …

Roughly half of the radiation from evolving galaxies in the early Universe reaches us in the
far-infrared and submillimeter wavelength ranges. Recent major advances in observing …

This paper presents the Planck 2013 likelihood, a complete statistical description of the two-
point correlation function of the CMB temperature fluctuations that accounts for all known …

An all sky map of the apparent temperature and optical depth of thermal dust emission is
constructed using the Planck-HFI (350μm to 2 mm) andIRAS (100μm) data. The optical …

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 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 …

We present measurements of secondary cosmic microwave background (CMB) anisotropies
and cosmic infrared background (CIB) fluctuations using data from the South Pole …

ABSTRACT We use South Pole Telescope data from 2008 and 2009 to detect the non-
Gaussian signature in the cosmic microwave background (CMB) produced by gravitational …

We present the first three-frequency South Pole Telescope (SPT) cosmic microwave
background (CMB) power spectra. The band powers presented here cover angular scales …

An Improved Measurement of the Secondary Cosmic Microwave Background Anisotropies
from the SPT-SZ + SPTpol Surveys - IOPscience This site uses cookies. By continuing to use …