The remarkable similarity of massive galaxy clusters from z~0 to z~1.9

McDonald, M.; Allen, S. W.; Bayliss, M.; Benson, B. A.; Bleem, L. E.; Brodwin, M.; Bulbul, E.; Carlstrom, J. E.; Forman, W. R.; Hlavacek-Larrondo, J.; Garmire, G. P.; Gaspari, M.; Gladders, M. D.; Mantz, A. B.; Murray, S. S.

doi:10.3847/1538-4357/aa7740

Title: The remarkable similarity of massive galaxy clusters from z~0 to z~1.9

Journal Article · Wed Jun 28 00:00:00 EDT 2017 · The Astrophysical Journal (Online)

DOI:https://doi.org/10.3847/1538-4357/aa7740· OSTI ID:1369250

^[1]; Allen, S. W. ^[2];

^[1]; Benson, B. A. ^[3]; Bleem, L. E. ^[4];

^[5]; Bulbul, E. ^[1]; Carlstrom, J. E. ^[4];

^[6];

^[7];

^[8];

^[9]; Gladders, M. D. ^[10]; Mantz, A. B. ^[2]; Murray, S. S. ^[6]

Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States)
Stanford Univ., Stanford, CA (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States)
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Chicago, Chicago, IL (United States)
Univ. of Chicago, Chicago, IL (United States); Argonne National Lab. (ANL), Argonne, IL (United States)
Univ. of Missouri, Columbia, MO (United States)
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
Univ. de Montreal, Montreal, QC (Canada)
Huntingdon Institute for X-ray Astronomy, Huntingdon, PA (United States)
Princeton Univ., Princeton, NJ (United States)
Univ. of Chicago, Chicago, IL (United States)

We present the results of a Chandra X-ray survey of the 8 most massive galaxy clusters at z > 1.2 in the South Pole Telescope 2500 deg2 survey. We combine this sample with previously-published Chandra observations of 49 massive X-ray-selected clusters at 0 < z < 0.1 and 90 SZ-selected clusters at 0.25 < z < 1.2 to constrain the evolution of the intracluster medium (ICM) over the past ~10 Gyr. We find that the bulk of the ICM has evolved self similarly over the full redshift range probed here, with the ICM density at r > 0.2R500 scaling like E(z) 2 . In the centers of clusters (r . 0.01R500), we find significant deviations from self similarity (ne ∝ E(z) 0.1±0.5 ), consistent with no redshift dependence. When we isolate clusters with over-dense cores (i.e., cool cores), we find that the average over-density profile has not evolved with redshift – that is, cool cores have not changed in size, density, or total mass over the past ~9–10 Gyr. We show that the evolving “cuspiness” of clusters in the Xray, reported by several previous studies, can be understood in the context of a cool core with fixed properties embedded in a self similarly-evolving cluster. We find no measurable evolution in the X-ray morphology of massive clusters, seemingly in tension with the rapidly-rising (with redshift) rate of major mergers predicted by cosmological simulations. We show that these two results can be brought into agreement if we assume that the relaxation time after a merger is proportional to the crossing time, since the latter is proportional to H(z) -1.

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Research Organization:: SLAC National Accelerator Lab., Menlo Park, CA (United States); Argonne National Lab. (ANL), Argonne, IL (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF); National Aeronautics and Space Administration (NASA); USDOE Office of Science (SC), Basic Energy Sciences (BES); Gordon and Betty Moore Foundation

Contributing Organization:: SPT

Grant/Contract Number:: AC02-76SF00515; AC02-07CH11359; AC02-06CH11357

OSTI ID:: 1369250

Alternate ID(s):: OSTI ID: 1352199; OSTI ID: 1373896

Report Number(s):: FERMILAB-PUB-17-072-AE; arXiv:1702.05094

Journal Information:: The Astrophysical Journal (Online), Vol. 843, Issue 1; ISSN 1538-4357

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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The Three Hundred Project: The evolution of galaxy cluster density profiles Mostoghiu, Robert; Knebe, Alexander; Cui, Weiguang Monthly Notices of the Royal Astronomical Society, Vol. 483, Issue 3 https://doi.org/10.1093/mnras/sty3306	journal	December 2018
Introducing romulusc : a cosmological simulation of a galaxy cluster with an unprecedented resolution Tremmel, M.; Quinn, T. R.; Ricarte, A. Monthly Notices of the Royal Astronomical Society, Vol. 483, Issue 3 https://doi.org/10.1093/mnras/sty3336	journal	December 2018
Inquiring into the nature of the Abell 2667 brightest cluster galaxy: physical properties from MUSE Iani, E.; Rodighiero, G.; Fritz, J. Monthly Notices of the Royal Astronomical Society, Vol. 487, Issue 4 https://doi.org/10.1093/mnras/stz1631	journal	June 2019
Enhancing AGN efficiency and cool-core formation with anisotropic thermal conduction Barnes, David J.; Kannan, Rahul; Vogelsberger, Mark Monthly Notices of the Royal Astronomical Society, Vol. 488, Issue 3 https://doi.org/10.1093/mnras/stz1814	journal	July 2019
A one-dimensional hydrodynamic model for accretion, cooling, and heating of gas in dark matter haloes from z = 6 to z = 0 Choudhury, Prakriti Pal; Kauffmann, Guinevere; Sharma, Prateek Monthly Notices of the Royal Astronomical Society, Vol. 485, Issue 3 https://doi.org/10.1093/mnras/stz567	journal	February 2019
X-ray properties of high-richness CAMIRA clusters in the Hyper Suprime-Cam Subaru Strategic Program field Ota, Naomi; Mitsuishi, Ikuyuki; Babazaki, Yasunori Publications of the Astronomical Society of Japan https://doi.org/10.1093/pasj/psz118	journal	November 2019
JVLA 1.5 GHz Continuum Observation of CLASH Clusters. I. Radio Properties of the BCGs Yu, Heng; Tozzi, Paolo; van Weeren, Reinout The Astrophysical Journal, Vol. 853, Issue 2 https://doi.org/10.3847/1538-4357/aaa421	journal	January 2018
Revisiting the Cooling Flow Problem in Galaxies, Groups, and Clusters of Galaxies McDonald, M.; Gaspari, M.; McNamara, B. R. The Astrophysical Journal, Vol. 858, Issue 1 https://doi.org/10.3847/1538-4357/aabace	journal	May 2018
X-Ray Properties of AGN in Brightest Cluster Galaxies. I. A Systematic Study of the Chandra Archive in the 0.2 < z < 0.3 and 0.55 < z < 0.75 Redshift Range Yang, Lilan; Tozzi, Paolo; Yu, Heng The Astrophysical Journal, Vol. 859, Issue 1 https://doi.org/10.3847/1538-4357/aabfd7	journal	May 2018
A Galaxy-scale Fountain of Cold Molecular Gas Pumped by a Black Hole Tremblay, G. R.; Combes, F.; Oonk, J. B. R. The Astrophysical Journal, Vol. 865, Issue 1 https://doi.org/10.3847/1538-4357/aad6dd	journal	September 2018
Spectroscopic Confirmation of Five Galaxy Clusters at z > 1.25 in the 2500 deg ² SPT-SZ Survey Khullar, G.; Bleem, L. E.; Bayliss, M. B. The Astrophysical Journal, Vol. 870, Issue 1 https://doi.org/10.3847/1538-4357/aaeed0	journal	December 2018
A Detailed Study of the Most Relaxed SPT-selected Galaxy Clusters: Properties of the Cool Core and Central Galaxy McDonald, M.; Allen, S. W.; Hlavacek-Larrondo, J. The Astrophysical Journal, Vol. 870, Issue 2 https://doi.org/10.3847/1538-4357/aaf394	journal	January 2019
The Impact of Radio AGN Bubble Composition on the Dynamics and Thermal Balance of the Intracluster Medium Yang, H. -Y. Karen; Gaspari, Massimo; Marlow, Carl The Astrophysical Journal, Vol. 871, Issue 1 https://doi.org/10.3847/1538-4357/aaf4bd	journal	January 2019
Cluster Cosmology Constraints from the 2500 deg ² SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope Bocquet, S.; Dietrich, J. P.; Schrabback, T. The Astrophysical Journal, Vol. 878, Issue 1 https://doi.org/10.3847/1538-4357/ab1f10	journal	June 2019
Expanding the Sample of Radio Minihalos in Galaxy Clusters Giacintucci, Simona; Markevitch, Maxim; Cassano, Rossella The Astrophysical Journal, Vol. 880, Issue 2 https://doi.org/10.3847/1538-4357/ab29f1	journal	July 2019
On the Assembly Bias of Cool Core Clusters Traced by H α Nebulae Medezinski, Elinor; McDonald, Michael; More, Surhud The Astrophysical Journal, Vol. 882, Issue 2 https://doi.org/10.3847/1538-4357/ab2da2	journal	September 2019
The X-Ray Halo Scaling Relations of Supermassive Black Holes Gaspari, M.; Eckert, D.; Ettori, S. The Astrophysical Journal, Vol. 884, Issue 2 https://doi.org/10.3847/1538-4357/ab3c5d	journal	October 2019
Probing the Origin of Diffuse Radio Emission in the Cool Core of the Phoenix Galaxy Cluster Raja, Ramij; Rahaman, Majidul; Datta, Abhirup The Astrophysical Journal, Vol. 889, Issue 2 https://doi.org/10.3847/1538-4357/ab620d	journal	January 2020
Discovery of a Powerful >10 ⁶¹ erg AGN Outburst in the Distant Galaxy Cluster SPT-CLJ0528-5300 Calzadilla, Michael S.; McDonald, Michael; Bayliss, Matthew The Astrophysical Journal, Vol. 887, Issue 1 https://doi.org/10.3847/2041-8213/ab5b07	journal	December 2019
Enhancing AGN efficiency and cool-core formation with anisotropic thermal conduction Barnes, David J.; Kannan, Rahul; Vogelsberger, Mark arXiv https://doi.org/10.48550/arxiv.1805.04109	text	January 2018
Cluster Cosmology Constraints from the 2500 deg$^2$ SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope Bocquet, S.; Dietrich, J. P.; Schrabback, T. arXiv https://doi.org/10.48550/arxiv.1812.01679	text	January 2018
The Three Hundred Project: The evolution of galaxy cluster density profiles Mostoghiu, Robert; Knebe, Alexander; Cui, Weiguang arXiv https://doi.org/10.48550/arxiv.1812.04009	text	January 2018
Constraining Gas Motions in the Intra-Cluster Medium Simionescu, A.; ZuHone, J.; Zhuravleva, I. arXiv https://doi.org/10.48550/arxiv.1902.00024	text	January 2019
Expanding the sample of radio minihalos in galaxy clusters Giacintucci, Simona; Markevitch, Maxim; Cassano, Rossella arXiv https://doi.org/10.48550/arxiv.1906.07087	text	January 2019
Evidence for ram pressure stripping in a cluster of galaxies at z=0.7 arXiv https://doi.org/10.48550/arxiv.1909.05491	text	January 2019
Probing the origin of diffuse radio emission in the cool-core of the Phoenix galaxy cluster Raja, Ramij; Rahaman, Majidul; Datta, Abhirup arXiv https://doi.org/10.48550/arxiv.1912.07853	text	January 2019

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