The XXL Survey: LI. Pressure profile and YSZ-M scaling relation in three low-mass galaxy clusters at z∼1 observed with NIKA2

R. Adam; M. Ricci; D. Eckert; P. Ade; H. Ajeddig; B. Altieri; P. André; E. Artis; H. Aussel; A. Beelen; C. Benoist; A. Benoît; S. Berta; L. Bing; M. Birkinshaw; O. Bourrion; D. Boutigny; M. Bremer; M. Calvo; A. Cappi; A. Catalano; M. De Petris; F. X. Désert; S. Doyle; E. F.C. Driessen; L. Faccioli; C. Ferrari; F. Gastaldello; P. Giles; A. Gomez; J. Goupy; O. Hahn; C. Hanser; C. Horellou; F. Kéruzoré; E. Koulouridis; C. Kramer; B. Ladjelate; G. Lagache; S. Leclercq; J. F. Lestrade; J. F. Macías-Pérez; S. Madden; B. Maughan; S. Maurogordato; A. Maury; P. Mauskopf; A. Monfardini; M. Muñoz-Echeverría; F. Pacaud; L. Perotto; M. Pierre; G. Pisano; E. Pompei; N. Ponthieu; V. Revéret; A. Rigby; A. Ritacco; C. Romero; H. Roussel; F. Ruppin; M. Sereno; K. Schuster; A. Sievers; G. Tintoré Vidal; C. Tucker; R. Zylka

doi:10.1051/0004-6361/202348049

The XXL Survey: LI. Pressure profile and Y_SZ-M scaling relation in three low-mass galaxy clusters at z∼1 observed with NIKA2

R. Adam
, M. Ricci
, D. Eckert
, P. Ade
, H. Ajeddig
, B. Altieri
, P. André
, E. Artis
, H. Aussel
, A. Beelen
, C. Benoist
, A. Benoît
, S. Berta
, L. Bing
, M. Birkinshaw
, O. Bourrion
, D. Boutigny
, M. Bremer
, M. Calvo
, A. Cappi

A. Catalano, M. De Petris, F. X. Désert, S. Doyle, E. F.C. Driessen, L. Faccioli, C. Ferrari, F. Gastaldello, P. Giles, A. Gomez, J. Goupy, O. Hahn, C. Hanser, C. Horellou, F. Kéruzoré, E. Koulouridis, C. Kramer, B. Ladjelate, G. Lagache, S. Leclercq, J. F. Lestrade, J. F. Macías-Pérez, S. Madden, B. Maughan, S. Maurogordato, A. Maury, P. Mauskopf, A. Monfardini, M. Muñoz-Echeverría, F. Pacaud, L. Perotto, M. Pierre, G. Pisano, E. Pompei, N. Ponthieu, V. Revéret, A. Rigby, A. Ritacco, C. Romero, H. Roussel, F. Ruppin, M. Sereno, K. Schuster, A. Sievers, G. Tintoré Vidal, C. Tucker, R. Zylka

Earth and Space Exploration, School of (SESE)

Research output: Contribution to journal › Article › peer-review

5 Scopus citations

Abstract

Context. The thermodynamical properties of the intracluster medium (ICM) are driven by scale-free gravitational collapse, but they also reflect the rich astrophysical processes at play in galaxy clusters. At low masses (∼10¹⁴M) and high redshift (z≳1), these properties remain poorly constrained, observationally speaking, due to the difficulty in obtaining resolved and sensitive data. Aims. We aim to investigate the inner structure of the ICM as seen through the Sunyaev-Zel’dovich (SZ) effect in this regime of mass and redshift. We focused on the thermal pressure profile and the scaling relation between SZ flux and mass, namely the Y_SZ-M scaling relation. Methods. The three galaxy clusters XLSSC 072 (z=1.002), XLSSC 100 (z=0.915), and XLSSC 102 (z=0.969), with M₅₀₀∼2×10¹⁴M, were selected from the XXL X-ray survey and observed with the NIKA2 millimeter camera to image their SZ signal. XMM-Newton X-ray data were used as a complement to the NIKA2 data to derive masses based on the Y_X-M relation and the hydrostatic equilibrium. Results. The SZ images of the three clusters, along with the X-ray and optical data, indicate dynamical activity related to merging events. The pressure profile is consistent with that expected for morphologically disturbed systems, with a relatively flat core and a shallow outer slope. Despite significant disturbances in the ICM, the three high-redshift low-mass clusters follow the Y_SZ-M relation expected from standard evolution remarkably well. Conclusions. These results indicate that the dominant physics that drives cluster evolution is already in place by z∼1, at least for systems with masses above M₅₀₀∼10¹⁴M.

Original language	English (US)
Article number	A18
Journal	Astronomy and Astrophysics
Volume	684
DOIs	https://doi.org/10.1051/0004-6361/202348049
State	Published - Apr 1 2024

Keywords

galaxies: clusters: intracluster medium
techniques: high angular resolution

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.1051/0004-6361/202348049

Cite this

Adam, R., Ricci, M., Eckert, D., Ade, P., Ajeddig, H., Altieri, B., André, P., Artis, E., Aussel, H., Beelen, A., Benoist, C., Benoît, A., Berta, S., Bing, L., Birkinshaw, M., Bourrion, O., Boutigny, D., Bremer, M., Calvo, M., ... Zylka, R. (2024). The XXL Survey: LI. Pressure profile and Y_SZ-M scaling relation in three low-mass galaxy clusters at z∼1 observed with NIKA2. Astronomy and Astrophysics, 684, Article A18. https://doi.org/10.1051/0004-6361/202348049

Adam, R, Ricci, M, Eckert, D, Ade, P, Ajeddig, H, Altieri, B, André, P, Artis, E, Aussel, H, Beelen, A, Benoist, C, Benoît, A, Berta, S, Bing, L, Birkinshaw, M, Bourrion, O, Boutigny, D, Bremer, M, Calvo, M, Cappi, A, Catalano, A, De Petris, M, Désert, FX, Doyle, S, Driessen, EFC, Faccioli, L, Ferrari, C, Gastaldello, F, Giles, P, Gomez, A, Goupy, J, Hahn, O, Hanser, C, Horellou, C, Kéruzoré, F, Koulouridis, E, Kramer, C, Ladjelate, B, Lagache, G, Leclercq, S, Lestrade, JF, Macías-Pérez, JF, Madden, S, Maughan, B, Maurogordato, S, Maury, A, Mauskopf, P, Monfardini, A, Muñoz-Echeverría, M, Pacaud, F, Perotto, L, Pierre, M, Pisano, G, Pompei, E, Ponthieu, N, Revéret, V, Rigby, A, Ritacco, A, Romero, C, Roussel, H, Ruppin, F, Sereno, M, Schuster, K, Sievers, A, Tintoré Vidal, G, Tucker, C & Zylka, R 2024, 'The XXL Survey: LI. Pressure profile and Y_SZ-M scaling relation in three low-mass galaxy clusters at z∼1 observed with NIKA2', Astronomy and Astrophysics, vol. 684, A18. https://doi.org/10.1051/0004-6361/202348049

@article{44bbdbf2a39d455e8acec3f0aa235c94,

title = "The XXL Survey: LI. Pressure profile and YSZ-M scaling relation in three low-mass galaxy clusters at z∼1 observed with NIKA2",

abstract = "Context. The thermodynamical properties of the intracluster medium (ICM) are driven by scale-free gravitational collapse, but they also reflect the rich astrophysical processes at play in galaxy clusters. At low masses (∼1014M) and high redshift (z≳1), these properties remain poorly constrained, observationally speaking, due to the difficulty in obtaining resolved and sensitive data. Aims. We aim to investigate the inner structure of the ICM as seen through the Sunyaev-Zel{\textquoteright}dovich (SZ) effect in this regime of mass and redshift. We focused on the thermal pressure profile and the scaling relation between SZ flux and mass, namely the YSZ-M scaling relation. Methods. The three galaxy clusters XLSSC 072 (z=1.002), XLSSC 100 (z=0.915), and XLSSC 102 (z=0.969), with M500∼2×1014M, were selected from the XXL X-ray survey and observed with the NIKA2 millimeter camera to image their SZ signal. XMM-Newton X-ray data were used as a complement to the NIKA2 data to derive masses based on the YX-M relation and the hydrostatic equilibrium. Results. The SZ images of the three clusters, along with the X-ray and optical data, indicate dynamical activity related to merging events. The pressure profile is consistent with that expected for morphologically disturbed systems, with a relatively flat core and a shallow outer slope. Despite significant disturbances in the ICM, the three high-redshift low-mass clusters follow the YSZ-M relation expected from standard evolution remarkably well. Conclusions. These results indicate that the dominant physics that drives cluster evolution is already in place by z∼1, at least for systems with masses above M500∼1014M.",

keywords = "galaxies: clusters: intracluster medium, techniques: high angular resolution",

author = "R. Adam and M. Ricci and D. Eckert and P. Ade and H. Ajeddig and B. Altieri and P. Andr{\'e} and E. Artis and H. Aussel and A. Beelen and C. Benoist and A. Beno{\^i}t and S. Berta and L. Bing and M. Birkinshaw and O. Bourrion and D. Boutigny and M. Bremer and M. Calvo and A. Cappi and A. Catalano and \{De Petris\}, M. and D{\'e}sert, \{F. X.\} and S. Doyle and Driessen, \{E. F.C.\} and L. Faccioli and C. Ferrari and F. Gastaldello and P. Giles and A. Gomez and J. Goupy and O. Hahn and C. Hanser and C. Horellou and F. K{\'e}ruzor{\'e} and E. Koulouridis and C. Kramer and B. Ladjelate and G. Lagache and S. Leclercq and Lestrade, \{J. F.\} and Mac{\'i}as-P{\'e}rez, \{J. F.\} and S. Madden and B. Maughan and S. Maurogordato and A. Maury and P. Mauskopf and A. Monfardini and M. Mu{\~n}oz-Echeverr{\'i}a and F. Pacaud and L. Perotto and M. Pierre and G. Pisano and E. Pompei and N. Ponthieu and V. Rev{\'e}ret and A. Rigby and A. Ritacco and C. Romero and H. Roussel and F. Ruppin and M. Sereno and K. Schuster and A. Sievers and \{Tintor{\'e} Vidal\}, G. and C. Tucker and R. Zylka",

note = "Publisher Copyright: {\textcopyright} The Authors 2024.",

year = "2024",

month = apr,

day = "1",

doi = "10.1051/0004-6361/202348049",

language = "English (US)",

volume = "684",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

TY - JOUR

T1 - The XXL Survey

T2 - LI. Pressure profile and YSZ-M scaling relation in three low-mass galaxy clusters at z∼1 observed with NIKA2

AU - Adam, R.

AU - Ricci, M.

AU - Eckert, D.

AU - Ade, P.

AU - Ajeddig, H.

AU - Altieri, B.

AU - André, P.

AU - Artis, E.

AU - Aussel, H.

AU - Beelen, A.

AU - Benoist, C.

AU - Benoît, A.

AU - Berta, S.

AU - Bing, L.

AU - Birkinshaw, M.

AU - Bourrion, O.

AU - Boutigny, D.

AU - Bremer, M.

AU - Calvo, M.

AU - Cappi, A.

AU - Catalano, A.

AU - De Petris, M.

AU - Désert, F. X.

AU - Doyle, S.

AU - Driessen, E. F.C.

AU - Faccioli, L.

AU - Ferrari, C.

AU - Gastaldello, F.

AU - Giles, P.

AU - Gomez, A.

AU - Goupy, J.

AU - Hahn, O.

AU - Hanser, C.

AU - Horellou, C.

AU - Kéruzoré, F.

AU - Koulouridis, E.

AU - Kramer, C.

AU - Ladjelate, B.

AU - Lagache, G.

AU - Leclercq, S.

AU - Lestrade, J. F.

AU - Macías-Pérez, J. F.

AU - Madden, S.

AU - Maughan, B.

AU - Maurogordato, S.

AU - Maury, A.

AU - Mauskopf, P.

AU - Monfardini, A.

AU - Muñoz-Echeverría, M.

AU - Pacaud, F.

AU - Perotto, L.

AU - Pierre, M.

AU - Pisano, G.

AU - Pompei, E.

AU - Ponthieu, N.

AU - Revéret, V.

AU - Rigby, A.

AU - Ritacco, A.

AU - Romero, C.

AU - Roussel, H.

AU - Ruppin, F.

AU - Sereno, M.

AU - Schuster, K.

AU - Sievers, A.

AU - Tintoré Vidal, G.

AU - Tucker, C.

AU - Zylka, R.

PY - 2024/4/1

Y1 - 2024/4/1

N2 - Context. The thermodynamical properties of the intracluster medium (ICM) are driven by scale-free gravitational collapse, but they also reflect the rich astrophysical processes at play in galaxy clusters. At low masses (∼1014M) and high redshift (z≳1), these properties remain poorly constrained, observationally speaking, due to the difficulty in obtaining resolved and sensitive data. Aims. We aim to investigate the inner structure of the ICM as seen through the Sunyaev-Zel’dovich (SZ) effect in this regime of mass and redshift. We focused on the thermal pressure profile and the scaling relation between SZ flux and mass, namely the YSZ-M scaling relation. Methods. The three galaxy clusters XLSSC 072 (z=1.002), XLSSC 100 (z=0.915), and XLSSC 102 (z=0.969), with M500∼2×1014M, were selected from the XXL X-ray survey and observed with the NIKA2 millimeter camera to image their SZ signal. XMM-Newton X-ray data were used as a complement to the NIKA2 data to derive masses based on the YX-M relation and the hydrostatic equilibrium. Results. The SZ images of the three clusters, along with the X-ray and optical data, indicate dynamical activity related to merging events. The pressure profile is consistent with that expected for morphologically disturbed systems, with a relatively flat core and a shallow outer slope. Despite significant disturbances in the ICM, the three high-redshift low-mass clusters follow the YSZ-M relation expected from standard evolution remarkably well. Conclusions. These results indicate that the dominant physics that drives cluster evolution is already in place by z∼1, at least for systems with masses above M500∼1014M.

AB - Context. The thermodynamical properties of the intracluster medium (ICM) are driven by scale-free gravitational collapse, but they also reflect the rich astrophysical processes at play in galaxy clusters. At low masses (∼1014M) and high redshift (z≳1), these properties remain poorly constrained, observationally speaking, due to the difficulty in obtaining resolved and sensitive data. Aims. We aim to investigate the inner structure of the ICM as seen through the Sunyaev-Zel’dovich (SZ) effect in this regime of mass and redshift. We focused on the thermal pressure profile and the scaling relation between SZ flux and mass, namely the YSZ-M scaling relation. Methods. The three galaxy clusters XLSSC 072 (z=1.002), XLSSC 100 (z=0.915), and XLSSC 102 (z=0.969), with M500∼2×1014M, were selected from the XXL X-ray survey and observed with the NIKA2 millimeter camera to image their SZ signal. XMM-Newton X-ray data were used as a complement to the NIKA2 data to derive masses based on the YX-M relation and the hydrostatic equilibrium. Results. The SZ images of the three clusters, along with the X-ray and optical data, indicate dynamical activity related to merging events. The pressure profile is consistent with that expected for morphologically disturbed systems, with a relatively flat core and a shallow outer slope. Despite significant disturbances in the ICM, the three high-redshift low-mass clusters follow the YSZ-M relation expected from standard evolution remarkably well. Conclusions. These results indicate that the dominant physics that drives cluster evolution is already in place by z∼1, at least for systems with masses above M500∼1014M.

KW - galaxies: clusters: intracluster medium

KW - techniques: high angular resolution

UR - https://www.scopus.com/pages/publications/85189246917

UR - https://www.scopus.com/pages/publications/85189246917#tab=citedBy

U2 - 10.1051/0004-6361/202348049

DO - 10.1051/0004-6361/202348049

M3 - Article

AN - SCOPUS:85189246917

SN - 0004-6361

VL - 684

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - A18

ER -

The XXL Survey: LI. Pressure profile and Y_SZ-M scaling relation in three low-mass galaxy clusters at z∼1 observed with NIKA2

Abstract

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ASJC Scopus subject areas

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The XXL Survey: LI. Pressure profile and YSZ-M scaling relation in three low-mass galaxy clusters at z∼1 observed with NIKA2

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Keywords

ASJC Scopus subject areas

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XLSSC NIKA2 sample images

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The XXL Survey: LI. Pressure profile and Y_SZ-M scaling relation in three low-mass galaxy clusters at z∼1 observed with NIKA2