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(2022)
QUBIC I: Overview and science program.
Journal of Cosmology and Astroparticle Physics, 034.
pp. 1-39.
ISSN 1475-7516
Abstract
The Q & U Bolometric Interferometer for Cosmology (QUBIC) is a novel kind
of polarimeter optimized for the measurement of the B-mode polarization of the Cosmic Microwave Background (CMB), which is one of the major challenges of observational cosmology.
The signal is expected to be of the order of a few tens of nK, prone to instrumental systematic effects and polluted by various astrophysical foregrounds which can only be controlled
through multichroic observations. QUBIC is designed to address these observational issues
with a novel approach that combines the advantages of interferometry in terms of control
of instrumental systematic effects with those of bolometric detectors in terms of wide-band,
background-limited sensitivity. The QUBIC synthesized beam has a frequency-dependent
shape that results in the ability to produce maps of the CMB polarization in multiple subbands within the two physical bands of the instrument (150 and 220 GHz). These features
make QUBIC complementary to other instruments and makes it particularly well suited to
characterize and remove Galactic foreground contamination. In this article, first of a series of
eight, we give an overview of the QUBIC instrument design, the main results of the calibration
campaign, and present the scientific program of QUBIC including not only the measurement
of primordial B-modes, but also the measurement of Galactic foregrounds. We give forecasts for typical observations and measurements: with three years of integration on the sky and
assuming perfect foreground removal as well as stable atmospheric conditions from our site in
Argentina, our simulations show that we can achieve a statistical sensitivity to the effective
tensor-to-scalar ratio (including primordial and foreground B-modes) σ(r) = 0.015.
Item Type: |
Article
|
Keywords: |
CMBR experiments; CMBR theory; cosmological parameters from CMBR; gravitational waves; CMBR polarization; |
Academic Unit: |
Faculty of Science and Engineering > Experimental Physics |
Item ID: |
17821 |
Identification Number: |
https://doi.org/10.1088/1475-7516/2022/04/034 |
Depositing User: |
Dr. Créidhe O'Sullivan
|
Date Deposited: |
14 Nov 2023 10:59 |
Journal or Publication Title: |
Journal of Cosmology and Astroparticle Physics |
Publisher: |
IOP Publishing |
Refereed: |
Yes |
URI: |
|
Use Licence: |
This item is available under a Creative Commons Attribution Non Commercial Share Alike Licence (CC BY-NC-SA). Details of this licence are available
here |
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