SKA synergy with Microwave Background studies
Carlo Burigana, Paul Alexander, Carlo Baccigalupi, Domingos Barbosa,, Alain Blanchard, Adriano De Rosa, Gianfranco de Zotti, Fabio Finelli,, Alessandro Gruppuso, Michael Jones, Sabino Matarrese, Alessandro Melchiorri,, Diego Molinari, Mattia Negrello, Daniela Paoletti
TL;DR
This paper explores how the Square Kilometre Array (SKA) can enhance cosmological studies through synergy with cosmic microwave background (CMB) research, outlining scientific goals, technical needs, and observational strategies.
Contribution
It provides a comprehensive overview of SKA's potential contributions to cosmology in collaboration with CMB and other wavelength observations, highlighting new scientific opportunities.
Findings
SKA's high sensitivity and resolution will improve CMB-related cosmological measurements.
Synergies between SKA and CMB observations can address key questions in cosmology and astrophysics.
The paper identifies instrumental and data analysis requirements for effective collaboration.
Abstract
The extremely high sensitivity and resolution of the Square Kilometre Array (SKA) will be useful for addressing a wide set of themes relevant for cosmology, in synergy with current and future cosmic microwave background (CMB) projects. Many of these themes also have a link with future optical-IR and X-ray observations. We discuss the scientific perspectives for these goals, the instrumental requirements and the observational and data analysis approaches, and identify several topics that are important for cosmology and astrophysics at different cosmic epochs.
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