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Unveiling the complexity of radio foregrounds for the detectability of the CMB polarization B-mode

Project description

A closer look at polarised radio sky emissions

Detecting the primordial B-mode of CMB polarisation is a major challenge in cosmology. This faint signal would confirm the existence of an inflationary period in the early universe, but contaminant emissions hinder its detection. Therefore, the success of future experiments will depend on efficient emissions removal. The EU-funded RadioForegroundsPlus project aims to enhance understanding of polarised radio emissions from our galaxy, most notably synchrotron, and from other extra-galactic sources. The project will create high-level data products by integrating data from ESA’s Planck satellite with low-frequency experiments like QUIJOTE, C-BASS, and S-PASS. These will include improved component-separated maps and expanded radio catalogues. The project will forecast the impact of radio foregrounds on detecting B-mode polarisation in future CMB experiments.

Objective

One of the main challenges in Cosmology is the detection of the primordial B-mode of CMB polarization, which would constitute a confirmation of the inflationary period of the Universe. However, the presence of different contaminants, mainly coming from the emissions of our own Galaxy, constitutes one of the major limiting factors to constrain reliably the existence of the B-modes. Indeed, the success of future CMB polarization experiments lies in the improved understanding and removal capability of foreground emissions.
RadioForegrounds+ will provide a state-of-the art description of the highly complex properties of the polarised radio emission from our Galaxy, in particular the synchrotron and the anomalous microwave emissions, as well as of the population of radio sources. It will also provide an unprecedentedly thorough description of the intensity signal. This goal can only be achieved by combining the ESA’s Planck satellite maps (30-857GHz) with the unique low frequency experiments considered in this proposal: QUIJOTE (10-40 GHz), C-BASS (5 GHz) and S-PASS (2.3 GHz), by counting within the consortium with experts on the previous data sets (including the teams responsible for QUIJOTE and C-BASS) and by using the most advanced analysis techniques.
The combination of these datasets will provide high-level data products, that will range from more complete radio catalogues, including fainter sources and additional frequency coverage, to new component separated maps in wider regions of the sky. These new data products and models will be made available to the scientific community through widely-used platforms, increasing the scientific return and the impact of the project. We will also provide forecasts of the impact of radio foregrounds on the detectability of the B-mode of polarization for future CMB experiments. The resulting analyses will play a key role in preparing and supporting future international CMB missions as LiteBIRD or ground-based efforts as CMB-S4.

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HORIZON-RIA - HORIZON Research and Innovation Actions

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Call for proposal

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(opens in new window) HORIZON-CL4-2023-SPACE-01

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Coordinator

AGENCIA ESTATAL CONSEJO SUPERIOR DE INVESTIGACIONES CIENTIFICAS
Net EU contribution

Net EU financial contribution. The sum of money that the participant receives, deducted by the EU contribution to its linked third party. It considers the distribution of the EU financial contribution between direct beneficiaries of the project and other types of participants, like third-party participants.

€ 374 407,50
Address
CALLE SERRANO 117
28006 MADRID
Spain

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Region
Comunidad de Madrid Comunidad de Madrid Madrid
Activity type
Research Organisations
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Total cost

The total costs incurred by this organisation to participate in the project, including direct and indirect costs. This amount is a subset of the overall project budget.

€ 374 407,50

Participants (3)

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