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The Q/U imaging experiment instrument
(The American Astronomical Society, 2013)
The Q/U Imaging ExperimenT (QUIET) is designed to measure polarization in the cosmic microwave background,
targeting the imprint of inflationary gravitational waves at large angular scales(∼1◦). Between 2008 October
and ...
Planck 2018 results VII. Isotropy and statistics of the CMB
(EDP Sciences, 2020)
Analysis of the Planck 2018 data set indicates that the statistical properties of the cosmic microwave background (CMB) temperature anisotropies are in excellent agreement with previous studies using the 2013 and 2015 data ...
Planck 2018 results. XI. Polarized dust foregrounds
(EDP Sciences, 2020)
The study of polarized dust emission has become entwined with the analysis of the cosmic microwave background (CMB) polarization in the quest for the curl-like B-mode polarization from primordial gravitational waves and ...
Planck 2018 results VIII. Gravitational lensing
(EDP Sciences, 2020)
We present measurements of the cosmic microwave background (CMB) lensing potential using the final Planck 2018 temperature and polarization data. Using polarization maps filtered to account for the noise anisotropy, we ...
Planck 2018 results IX. Constraints on primordial non-Gaussianity
(EDP Sciences, 2020)
We analyse the Planck full-mission cosmic microwave background (CMB) temperature and E-mode polarization maps to obtain constraints on primordial non-Gaussianity (NG). We compare estimates obtained from separable ...
The contribution of discrete sources to the sky temperature at 144 MHz
(EDP Sciences, 2021)
In recent years, the level of the extragalactic radio background has become a point of considerable interest, with some lines of argument pointing to an entirely new cosmological synchrotron background. The contribution ...
Cosmic microwave background constraints on a physical model of reionization
(Oxford University Press, 2021)
We study constraints on allowed reionization histories by comparing predictions of a physical seminumerical model with secondary temperature and polarization anisotropies of the cosmic microwave background (CMB). Our model ...
Characterizing line-of-sight variability of polarized dust emission with future cmb experiments
(Oxford University Press, 2023)
While Galactic dust emission is often accounted for in cosmic microwave background (CMB) analyses by fitting a two-parameter modified blackbody (MBB) model in each pixel, typically a number of such clouds are found along ...