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Exploring the mass and redshift dependence of the cluster pressure profile with stacks on thermal SZ maps

We provide novel constraints on the parameters defining the universal pressure profile (UPP) within clusters of galaxies, and explore their dependence on the cluster mass and redshift, from measurements of Sunyaev-Zel'dovich Compton-\(y\) profiles. We employ both the \(\textit{Planck}\) 2015 MI...

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Published in:arXiv.org 2023-02
Main Authors: Tramonte, Denis, Yin-Zhe, Ma, Ziang Yan, Maturi, Matteo, Castignani, Gianluca, Sereno, Mauro, Bardelli, Sandro, Giocoli, Carlo, Marulli, Federico, Moscardini, Lauro, Puddu, Emanuella, Radovich, Mario, Ludovic Van Waerbeke, Wright, Angus H
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creator Tramonte, Denis
Yin-Zhe, Ma
Ziang Yan
Maturi, Matteo
Castignani, Gianluca
Sereno, Mauro
Bardelli, Sandro
Giocoli, Carlo
Marulli, Federico
Moscardini, Lauro
Puddu, Emanuella
Radovich, Mario
Ludovic Van Waerbeke
Wright, Angus H
description We provide novel constraints on the parameters defining the universal pressure profile (UPP) within clusters of galaxies, and explore their dependence on the cluster mass and redshift, from measurements of Sunyaev-Zel'dovich Compton-\(y\) profiles. We employ both the \(\textit{Planck}\) 2015 MILCA and the ACT-DR4 \(y\) maps over the common \(\sim 2,100\,\text{deg}^2\) footprint. We combine existing cluster catalogs based on KiDS, SDSS and DESI observations, for a total of 23,820 clusters spanning the mass range \(10^{14.0}\,\text{M}_{\odot}
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We employ both the \(\textit{Planck}\) 2015 MILCA and the ACT-DR4 \(y\) maps over the common \(\sim 2,100\,\text{deg}^2\) footprint. We combine existing cluster catalogs based on KiDS, SDSS and DESI observations, for a total of 23,820 clusters spanning the mass range \(10^{14.0}\,\text{M}_{\odot}&lt;M_{500}&lt;10^{15.1}\,\text{M}_{\odot}\) and the redshift range \(0.02&lt;z&lt;0.98\). We split the clusters into three independent bins in mass and redshift; for each combination we detect the stacked SZ cluster signal and extract the mean \(y\) angular profile. The latter is predicted theoretically adopting a halo model framework, and MCMCs are employed to estimate the UPP parameters, the hydrostatic mass bias \(b_{\rm h}\) and possible cluster miscentering effects. We constrain \([P_0,c_{500},\alpha,\beta]\) to \([5.9,2.0,1.8,4.9]\) with \(\textit{Planck}\) and to \([3.8,1.3,1.0,4.4]\) with ACT using the full cluster sample, in agreement with previous findings. 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subjects Bias
Galactic clusters
Galaxies
Mathematical models
Parameters
Pressure dependence
Red shift
title Exploring the mass and redshift dependence of the cluster pressure profile with stacks on thermal SZ maps
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