Systematic effects on the upcoming NIKA2 LPSZ scaling relation

Authors :: Moyer-Anin A.
Adam R.
Ade P.
Ajeddig H.
André P.
Artis E.
Aussel H.
Bartalucci I.
Beelen A.
Benoît A.
Berta S.
Bing L.
Bourrion O.
Calvo M.
Catalano A.
De Petris M.
Désert F.-X.
Doyle S.
Driessen E.F.C.
Ejlali G.
Gomez A.
Goupy J.
Hanser C.
Katsioli S.
Kéruzoré F.
Kramer C.
Ladjelate B.
Lagache G.
Leclercq S.
Lestrade J.-F.
Macías-Pérez J.F.
Madden S.C.
Maury A.
Mauskopf P.
Mayet F.
Monfardini A.
Muñoz-Echeverría M.
Paliwal A.
Perotto L.
Pisano G.
Pointecouteau E.
Ponthieu N.
Pratt G.W.
Revéret V.
Rigby A.J.
Ritacco A.
Romero C.
Roussel H.
Ruppin F.
Schuster K.
Sievers A.
Tucker C.
Source :: EPJ Web of Conferences, Vol 293, p 00032 (2024)
Publication Year :: 2024
Publisher :: EDP Sciences, 2024.
Abstract: In cluster cosmology, cluster masses are the main parameter of interest. They are needed to constrain cosmological parameters through the cluster number count. As the mass is not an observable, a scaling relation is needed to link cluster masses to the integrated Compton parameters Y, i.e. the Sunyaev-Zeldovich observable (SZ). Planck cosmological results obtained with cluster number counts are based on a scaling relation measured with clusters at low redshift (z

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