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CHEX-MATE: Joint fit of the universal pressure profile and galaxy cluster masses
CHEX-MATE: Joint fit of the universal pressure profile and galaxy cluster masses
by Bourdin, H. , De Petris, M. , Melin, J.-B. , McBride, L. , Sereno, M. , Clerc, N. , Maughan, B. J. , Eckert, D. , Oppizzi, F. , Tristram, M. , Rossetti, M. , Salvati, L. , Pointecouteau, E. , Rasia, E. , Mazzotta, P. , Sayers, J. , Ilić, S. , Dupourqué, S. , Saxena, H. , Donahue, M. , Gitti, M. , Lovisari, L. , Douspis, M. , Kim, J. , Gaspari, M. , Gastaldello, F. , De Luca, F. , Bartalucci, I. , Muñoz-Echeverría, M. , Pratt, G. W. , Gorce, A. , Kay, S. T. , Macías-Pérez, J.-F. , Ettori, S.
2026
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CHEX-MATE: Joint fit of the universal pressure profile and galaxy cluster masses
by Bourdin, H. , De Petris, M. , Melin, J.-B. , McBride, L. , Sereno, M. , Clerc, N. , Maughan, B. J. , Eckert, D. , Oppizzi, F. , Tristram, M. , Rossetti, M. , Salvati, L. , Pointecouteau, E. , Rasia, E. , Mazzotta, P. , Sayers, J. , Ilić, S. , Dupourqué, S. , Saxena, H. , Donahue, M. , Gitti, M. , Lovisari, L. , Douspis, M. , Kim, J. , Gaspari, M. , Gastaldello, F. , De Luca, F. , Bartalucci, I. , Muñoz-Echeverría, M. , Pratt, G. W. , Gorce, A. , Kay, S. T. , Macías-Pérez, J.-F. , Ettori, S.
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2026
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CHEX-MATE: Joint fit of the universal pressure profile and galaxy cluster masses
CHEX-MATE: Joint fit of the universal pressure profile and galaxy cluster masses
by Bourdin, H. , De Petris, M. , Melin, J.-B. , McBride, L. , Sereno, M. , Clerc, N. , Maughan, B. J. , Eckert, D. , Oppizzi, F. , Tristram, M. , Rossetti, M. , Salvati, L. , Pointecouteau, E. , Rasia, E. , Mazzotta, P. , Sayers, J. , Ilić, S. , Dupourqué, S. , Saxena, H. , Donahue, M. , Gitti, M. , Lovisari, L. , Douspis, M. , Kim, J. , Gaspari, M. , Gastaldello, F. , De Luca, F. , Bartalucci, I. , Muñoz-Echeverría, M. , Pratt, G. W. , Gorce, A. , Kay, S. T. , Macías-Pérez, J.-F. , Ettori, S.
2026

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CHEX-MATE: Joint fit of the universal pressure profile and galaxy cluster masses
CHEX-MATE: Joint fit of the universal pressure profile and galaxy cluster masses
Journal Article

CHEX-MATE: Joint fit of the universal pressure profile and galaxy cluster masses

Bourdin, H.,
De Petris, M.,
Melin, J.-B.,
McBride, L.,
Sereno, M.,
Clerc, N.,
Maughan, B. J.,
Eckert, D.,
Oppizzi, F.,
Tristram, M.,
Rossetti, M.,
Salvati, L.,
Pointecouteau, E.,
Rasia, E.,
Mazzotta, P.,
Sayers, J.,
Ilić, S.,
Dupourqué, S.,
Saxena, H.,
Donahue, M.,
Gitti, M.,
Lovisari, L.,
Douspis, M.,
Kim, J.,
Gaspari, M.,
Gastaldello, F.,
De Luca, F.,
Bartalucci, I.,
Muñoz-Echeverría, M.,
Pratt, G. W.,
Gorce, A.,
Kay, S. T.,
Macías-Pérez, J.-F.,
Ettori, S.
2026
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Overview
Within the self-similar framework of structure formation, the thermal pressure of the hot intra-cluster medium follows a universal distribution that is independent of the cluster mass scale. Once normalised to the proper mass and redshift dependencies, this pressure distribution becomes common to all clusters. Reconstructing such a universal pressure profile requires individual estimates of each cluster’s mass. In this work, we present a methodology to simultaneously fit the universal pressure profile alongside the masses of individual clusters in a sample, while properly accounting for correlations between the profile’s shape, its amplitude, and cluster masses. We apply this method to a sub-sample of clusters from the CHEX-MATE project and demonstrate the strong impact that the assumed pressure profile has on the measured signal. This effect propagates into the thermal Sunyaev-Zel’dovich (tSZ) power spectrum and, in turn, influences the determination of cosmological parameters.
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