Planck 2015 results-III. LFI systematic uncertainties
We present the current accounting of systematic effect uncertainties for the Low Frequency
Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results …
Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results …
Exploring cosmic origins with CORE: Inflation
We forecast the scientific capabilities to improve our understanding of cosmic inflation of
CORE, a proposed CMB space satellite submitted in response to the ESA fifth call for a …
CORE, a proposed CMB space satellite submitted in response to the ESA fifth call for a …
The large scale polarization explorer (LSPE) for CMB measurements: performance forecast
The measurement of the polarization of the Cosmic Microwave Background (CMB) radiation
is one of the current frontiers in cosmology. In particular, the detection of the primordial …
is one of the current frontiers in cosmology. In particular, the detection of the primordial …
Robust forecasts on fundamental physics from the foreground-obscured, gravitationally-lensed CMB polarization
Recent results from the BICEP, Keck Array and Planck Collaborations demonstrate that
Galactic foregrounds are an unavoidable obstacle in the search for evidence of inflationary …
Galactic foregrounds are an unavoidable obstacle in the search for evidence of inflationary …
[HTML][HTML] Planck 2015 results-XXV. Diffuse low-frequency Galactic foregrounds
PAR Ade, N Aghanim, MIR Alves, M Arnaud… - Astronomy & …, 2016 - aanda.org
We discuss the Galactic foreground emission between 20 and 100 GHz based on
observations by Planck and WMAP. The total intensity in this part of the spectrum is …
observations by Planck and WMAP. The total intensity in this part of the spectrum is …
Revisiting the distance to radio Loops I and IV using Gaia and radio/optical polarization data
Galactic synchrotron emission exhibits large angular scale features known as radio spurs
and loops. Determining the physical size of these structures is important for understanding …
and loops. Determining the physical size of these structures is important for understanding …
Observations of the polarisation of the anomalous microwave emission: a review
The observational status of the polarisation of the anomalous microwave emission (AME) is
reviewed, both for individual compact Galactic regions as well as for the large‐scale Galactic …
reviewed, both for individual compact Galactic regions as well as for the large‐scale Galactic …
Characterization of the polarized synchrotron emission from Planck and WMAP data
FA Martire, RB Barreiro… - Journal of Cosmology …, 2022 - iopscience.iop.org
The purpose of this work is to characterize the diffuse Galactic polarized synchrotron, which
is the dominant CMB foreground emission at low frequency. We present EE, BB, and EB …
is the dominant CMB foreground emission at low frequency. We present EE, BB, and EB …
Polycyclic Aromatic Hydrocarbons, Anomalous Microwave Emission, and their Connection to the Cold Neutral Medium
BS Hensley, CE Murray, M Dodici - The Astrophysical Journal, 2022 - iopscience.iop.org
Using new large-area maps of the cold neutral medium (CNM) fraction, f CNM, we
investigate the relationship between the CNM, the abundance of polycyclic aromatic …
investigate the relationship between the CNM, the abundance of polycyclic aromatic …
The design of the Ali CMB Polarization Telescope receiver
Publisher's Note: This paper, originally published on 22 December 2020, was replaced with
a corrected/revised version on 12 March 2021. If you downloaded the original PDF but are …
a corrected/revised version on 12 March 2021. If you downloaded the original PDF but are …