Multiwavelength view of SPT-CL J2106-5844. The radio galaxies and the thermal and relativistic plasmas in a massive galaxy cluster merger at z~1.13
arXiv:2101.02216 · doi:10.1051/0004-6361/202040260
Abstract
SPT-CL J2106-5844 is among the most massive galaxy clusters at z>1 yet discovered. While initially used in cosmological tests to assess the compatibility with CDM cosmology of such a massive virialized object at this redshift, more recent studies indicate SPT-CL J2106-5844 is undergoing a major merger, and is not an isolated system with a singular, well-defined halo. We use sensitive, high spatial resolution measurements from ALMA and ACA of the thermal SZ effect to reconstruct the pressure distribution of the intracluster medium in this system. These measurements are coupled with radio observations from the EMU pilot survey, using ASKAP and the ATCA to search for diffuse nonthermal emission. Further, to better constrain the thermodynamic structure of the cluster, we complement our analysis with reprocessed archival observations. We fit the ALMA+ACA SZ data in -space using a Bayesian forward modelling technique. The ASKAP and ATCA data are processed and imaged to specifically highlight any potential diffuse radio emission. In the ALMA+ACA SZ data, we reliably identify at high significance two main gas components associated with the mass clumps inferred from weak lensing. Our statistical test excludes at the ~9.9 level the possibility of describing the system with a single SZ component. While the components had been more difficult to identify in the X-ray data alone, we find that the bimodal gas distribution is supported by the X-ray hardness distribution. The EMU radio observations reveal a diffuse radio structure ~400 kpc in projected extent along the northwest-southeast direction, indicative of strong activity from the active galactic nucleus within the brightest cluster galaxy. Interestingly, a putative optical star-forming filamentary structure detected in the HST image is in an excellent alignment with the radio structure, albeit on a smaller scale.
18 pages, 14 figures, and 1 table; accepted for publication in A&A
References in corpus (40)
- Array Programming with NumPy
- Galaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ survey
- Diffuse Radio Emission from Galaxy Clusters
- The origin of cold fronts in the cores of relaxed galaxy clusters
- The Atacama Cosmology Telescope: A Catalog of > 4000 Sunyaev-Zel'dovich Galaxy Clusters
- Science With The Australian Square Kilometre Array Pathfinder
- X-ray cavities in a sample of 83 SPT-selected clusters of galaxies: Tracing the evolution of AGN feedback in clusters of galaxies out to z=1.2
- The impact of mergers on relaxed X-ray clusters - II. Effects on global X-ray and SZ properties and their scaling relations
- Redshifts, Sample Purity, and BCG Positions for the Galaxy Cluster Catalog from the first 720 Square Degrees of the South Pole Telescope Survey
- Constraining Gas Motions in the Intra-Cluster Medium
- The GOGREEN Survey: A deep stellar mass function of cluster galaxies at 1.0<z<1.4 and the complex nature of satellite quenching
- Radio halos in a mass-selected sample of 75 galaxy clusters. II. Statistical analysis
- The GOGREEN survey: The environmental dependence of the star-forming galaxy main sequence at
- The Three Hundred Project: correcting for the hydrostatic-equilibrium mass bias in X-ray and SZ surveys
- Fast magnetic field amplification in distant galaxyclusters
- Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey Description
- The Impact of Galaxy Cluster Mergers on Cosmological Parameter Estimation from Surveys of the Sunyaev-Zel'dovich Effect
- The GOGREEN and GCLASS Surveys: First Data Release
- Shocks and non-thermal particles in clusters of galaxies
- Radio Galaxy Zoo: The Distortion of Radio Galaxies by Galaxy Clusters
- Resolving galaxy cluster gas properties at z~1 with XMM-Newton and Chandra
- Wideband 67-116 GHz receiver development for ALMA Band 2
- How merger-driven gas motions in galaxy clusters can turn AGN bubbles into radio relics
- On the relation between mini-halos and AGN feedback in clusters of galaxies
- The formation of dusty cold gas filaments from galaxy cluster simulations
- ALMA-SZ Detection of a Galaxy Cluster Merger Shock at Half the Age of the Universe
- Understanding the radio relic emission in the galaxy cluster MACS J0717.5+3745: spectral analysis
- The Dust and Molecular Gas in the Brightest Cluster Galaxy in MACS 1931.8-2635
- A radio halo surrounding the Brightest Cluster Galaxy in RXCJ0232.2-4420: a mini-halo in transition ?
- A Study of High-redshift AGN Feedback in SZ Cluster Samples
- The Massive and Distant Clusters of WISE Survey X: Initial Results from a Sunyaev-Zeldovich Effect Study of Massive Galaxy Clusters at z>1 using MUSTANG2 on the GBT
- Reconstruction of Radio Relics and X-ray Tails in an Off-axis Cluster Merger: Hydrodynamical Simulations of A115
- The relation between the diffuse X-ray luminosity and the radio power of the central AGN in galaxy groups
- A Massive Cluster at z = 0.288 Caught in the Process of Formation: The Case of Abell 959
- The High-Redshift Clusters Occupied by Bent Radio AGN (COBRA) Survey: Follow-Up Optical Imaging
- Precise Mass Determination of SPT-CL J2106-5844, the Most Massive Cluster at z>1
- Line-of-sight gas sloshing in the cool core of Abell 907
- The Massive and Distant Clusters of WISE Survey IX: High Radio Activity in a Merging Cluster
- The Massive and Distant Clusters of WISE Survey: SZ effect Verification with the Atacama Compact Array -- Localization and Cluster Analysis
- Extended, Dusty Star Formation Fueled by a Residual Cooling Flow in the Cluster of Galaxies Sersic 159-03
Cited by in corpus (11)
- Forming intracluster gas in a galaxy protocluster at a redshift of 2.16
- Radio fossils, relics, and haloes in Abell 3266: cluster archaeology with ASKAP-EMU and the ATCA
- XLSSC 122 caught in the act of growing up: Spatially resolved SZ observations of a z=1.98 galaxy cluster
- Limits and challenges of the detection of cluster-scale diffuse radio emission at high redshift: The Massive and Distant Clusters of WISE Survey (MaDCoWS) in LoTSS-DR2
- Double radio relics and radio halo in the high redshift galaxy cluster El Gordo with the Upgraded GMRT
- Galaxy clusters at z~1 imaged by ALMA with the Sunyaev-Zel'dovich effect
- AGN feedback in an infant galaxy cluster: the LOFAR-Chandra view of the giant FRII radio galaxy J103025+052430 at z=1.7
- The MeerKAT Massive Distant Clusters Survey: detection of diffuse radio emission in galaxy clusters at
- The MeerKAT Massive Distant Clusters Survey: A Radio Halo in a Massive Galaxy Cluster at z = 1.23
- Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Resolving the Hot and Ionized Universe through the Sunyaev-Zeldovich effect
- A 600 kpc complex radio source at the center of Abell 3718 discovered by the EMU and POSSUM surveys