The XXL Survey: LI. Pressure profile and YSZ -M scaling relation in three low-mass galaxy clusters at z∼1 observed with NIKA2
Artikel i vetenskaplig tidskrift, 2024
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.
techniques: high angular resolution
galaxies: clusters: intracluster medium
Författare
R. M. Adam
École polytechnique
Laboratoire Joseph-Louis Lagrange
M. Ricci
Université Savoie Mont Blanc
APC - AstroParticule et Cosmologie
Laboratoire Joseph-Louis Lagrange
D. Eckert
Université de Genève
P., Ade
Cardiff University
H. Ajeddig
Université Paris-Saclay
B. Altiéri
European Space Astronomy Centre (ESAC)
P. André
Université Paris-Saclay
E. Artis
Université Grenoble Alpes
H. Aussel
Université Paris-Saclay
A. Beelen
Laboratoire d'Astrophysique de Marseille
C. Benoist
Laboratoire Joseph-Louis Lagrange
A. Benoît
Université Grenoble Alpes
S. Berta
Institut de Radioastronomie Millimétrique (IRAM)
L. Bing
Laboratoire d'Astrophysique de Marseille
M. Birkinshaw
University of Bristol
O. Bourrion
Université Grenoble Alpes
D. Boutigny
Université Savoie Mont Blanc
M. Bremer
University of Bristol
M. Calvo
Université Grenoble Alpes
A. Cappi
Laboratoire Joseph-Louis Lagrange
Istituto nazionale di astrofisica (INAF)
A. Catalano
Université Grenoble Alpes
M. De Petris
Sapienza, Università di Roma
F. X. Désert
Institut de Planétologie et d’Astrophysique de Grenoble (IPAG)
S. Doyle
Cardiff University
E. F.C. Driessen
Institut de Radioastronomie Millimétrique (IRAM)
L. Faccioli
Université Paris-Saclay
C. Ferrari
Laboratoire Joseph-Louis Lagrange
F. Gastaldello
Istituto nazionale di astrofisica (INAF)
P. Giles
University of Sussex
A. Gomez
Centro de Astrobiologia (CAB)
J. Goupy
Université Grenoble Alpes
O. Hahn
Laboratoire Joseph-Louis Lagrange
C. Hanser
Université Grenoble Alpes
Cathy Horellou
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
F. Kéruzoré
Argonne National Laboratory
E. Koulouridis
Université Paris-Saclay
National Observatory of Athens
Jae-Young Kim
Institut de Radioastronomie Millimétrique (IRAM)
B. Ladjelate
Institut de Radioastronomie Millimétrique (IRAM)
Guilaine Lagache
Laboratoire d'Astrophysique de Marseille
S. Leclercq
Institut de Radioastronomie Millimétrique (IRAM)
J.F. Lestrade
Observatoire de Paris
J. F. Maciás-Pérez
Université Grenoble Alpes
S. C. Madden
Université Paris-Saclay
B. Maughan
University of Bristol
S. Maurogordato
Laboratoire Joseph-Louis Lagrange
A. Maury
Université Paris-Saclay
P. Mauskopf
Cardiff University
Arizona State University
A. Monfardini
Université Grenoble Alpes
M. Muñoz-Echeverría
Université Grenoble Alpes
F. Pacaud
Universität Bonn
L. Perotto
Université Grenoble Alpes
M. Pierre
Université Paris-Saclay
G. Pisano
Sapienza, Università di Roma
E. Pompei
European Southern Observatory Santiago
N. Ponthieu
Institut de Planétologie et d’Astrophysique de Grenoble (IPAG)
V. Revéret
Université Paris-Saclay
Andrew Rigby
Cardiff University
A. Ritacco
Laboratoire de Physique de l’Ecole Normale Supérieure
Istituto nazionale di astrofisica (INAF)
C. Romero
University of Pennsylvania
H. Roussel
Institut d 'Astrophysique de Paris
F. Ruppin
Université de Lyon
M. Sereno
Istituto Nazionale di Fisica Nucleare
Istituto nazionale di astrofisica (INAF)
K. Schuster
Institut de Radioastronomie Millimétrique (IRAM)
A. Sievers
Institut de Radioastronomie Millimétrique (IRAM)
G. Tintoré Vidal
École polytechnique
C. Tucker
Cardiff University
R. Zylka
Institut de Radioastronomie Millimétrique (IRAM)
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 684 A18Ämneskategorier
Astronomi, astrofysik och kosmologi
Geofysik
DOI
10.1051/0004-6361/202348049