Planck 2013 results. XV. CMB power spectra and likelihood
PAR Ade, N Aghanim, C Armitage-Caplan… - Astronomy & …, 2014 - aanda.org
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 …
point correlation function of the CMB temperature fluctuations that accounts for all known …
Neutrino physics from the cosmic microwave background and large scale structure
This is a report on the status and prospects of the quantification of neutrino properties
through the cosmological neutrino background for the Cosmic Frontier of the Division of …
through the cosmological neutrino background for the Cosmic Frontier of the Division of …
The Atacama Cosmology Telescope: Cosmological parameters from three seasons of data
JL Sievers, RA Hlozek, MR Nolta… - … of Cosmology and …, 2013 - iopscience.iop.org
We present constraints on cosmological and astrophysical parameters from high-resolution
microwave background maps at 148 GHz and 218 GHz made by the Atacama Cosmology …
microwave background maps at 148 GHz and 218 GHz made by the Atacama Cosmology …
A measurement of the damping tail of the cosmic microwave background power spectrum with the South Pole Telescope
R Keisler, CL Reichardt, KA Aird… - The Astrophysical …, 2011 - iopscience.iop.org
We present a measurement of the angular power spectrum of the cosmic microwave
background (CMB) using data from the South Pole Telescope (SPT). The data consist of 790 …
background (CMB) using data from the South Pole Telescope (SPT). The data consist of 790 …
A Measurement of the Cosmic Microwave Background Damping Tail from the 2500-square-degree SPT-SZ survey
We present a measurement of the cosmic microwave background (CMB) temperature power
spectrum using data from the recently completed South Pole Telescope Sunyaev–Zel'dovich …
spectrum using data from the recently completed South Pole Telescope Sunyaev–Zel'dovich …
The Atacama Cosmology Telescope: temperature and gravitational lensing power spectrum measurements from three seasons of data
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 …
derived from the three seasons of data from the Atacama Cosmology Telescope (ACT) at …
The atacama cosmology telescope: cosmological parameters from the 2008 power spectrum
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 …
cosmic microwave background (CMB) radiation observed at 148 GHz and 218 GHz over …
The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths
J Delabrouille, M Betoule, JB Melin… - Astronomy & …, 2013 - aanda.org
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 …
arcminute resolution maps of sky emission at submillimetre to centimetre wavelengths, in …
A measurement of secondary cosmic microwave background anisotropies from the 2500 square-degree SPT-SZ survey
EM George, CL Reichardt, KA Aird… - The Astrophysical …, 2015 - iopscience.iop.org
We present measurements of secondary cosmic microwave background (CMB) anisotropies
and cosmic infrared background (CIB) fluctuations using data from the South Pole …
and cosmic infrared background (CIB) fluctuations using data from the South Pole …
A measurement of gravitational lensing of the microwave background using South Pole Telescope data
A Van Engelen, R Keisler, O Zahn, KA Aird… - The Astrophysical …, 2012 - iopscience.iop.org
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 …
Gaussian signature in the cosmic microwave background (CMB) produced by gravitational …