Mayet, F., Adam, R., Ade, P. ![]() ![]() ![]() ![]() ![]() ![]() |
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Abstract
he main limiting factor of cosmological analyses based on thermal Sunyaev-Zel’dovich (SZ) cluster statistics comes from the bias and systematic uncertainties that affect the estimates of the mass of galaxy clusters. High-angular resolution SZ observations at high redshift are needed to study a potential redshift or morphology dependence of both the mean pressure profile and of the mass-observable scaling relation used in SZ cosmological analyses. The NIKA2 camera is a new generation continuum instrument installed at the IRAM 30-m telescope. With a large field of view, a high angular resolution and a high-sensitivity, the NIKA2 camera has unique SZ mapping capabilities. In this paper, we present the NIKA2 SZ large program, aiming at observing a large sample of clusters at redshifts between 0.5 and 0.9, and the characterization of the first cluster oberved with NIKA2.
Item Type: | Article |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Publisher: | EDP Sciences |
ISSN: | 2100-014X |
Date of First Compliant Deposit: | 10 March 2020 |
Date of Acceptance: | 27 January 2020 |
Last Modified: | 05 May 2023 20:37 |
URI: | https://orca.cardiff.ac.uk/id/eprint/130290 |
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