The Massive and Distant Clusters of WISE Survey. III. Sunyaev-Zel'dovich Masses of Galaxy Clusters at
arXiv:1410.2355 · doi:10.1088/0004-637X/806/1/26
Abstract
We present CARMA 30 GHz Sunyaev-Zel'dovich (SZ) observations of five high-redshift (), infrared-selected galaxy clusters discovered as part of the all-sky Massive and Distant Clusters of WISE Survey (MaDCoWS). The SZ decrements measured toward these clusters demonstrate that the MaDCoWS selection is discovering evolved, massive galaxy clusters with hot intracluster gas. Using the SZ scaling relation calibrated with South Pole Telescope clusters at similar masses and redshifts, we find these MaDCoWS clusters have masses in the range . Three of these are among the most massive clusters found to date at , demonstrating that MaDCoWS is sensitive to the most massive clusters to at least . The added depth of the AllWISE data release will allow all-sky infrared cluster detection to and beyond.
arXiv comment8 pages, 4 figures, 3 tables; Accepted to ApJ after minor revisions; results unchanged
References in corpus (46)
- The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance
- The Eighth Data Release of the Sloan Digital Sky Survey: First Data from SDSS-III
- The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the Y_SZ-M_500 relation
- Dark matter halo concentrations in the Wilkinson Microwave Anisotropy Probe year 5 cosmology
- Galaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ survey
- Effects of Galaxy Formation on Thermodynamics of the Intracluster Medium
- The ROSAT-ESO Flux Limited X-ray (REFLEX) Galaxy Cluster Survey. V. The cluster catalogue
- The MCXC: a Meta-Catalogue of X-ray detected Clusters of galaxies
- The Northern ROSAT All-Sky (NORAS) Galaxy Cluster Survey I: X-ray Properties of Clusters Detected as Extended X-ray Sources
- Planck 2013 results. XXIX. Planck catalogue of Sunyaev-Zeldovich sources
- MACS: A quest for the most massive galaxy clusters in the universe
- The Atacama Cosmology Telescope: Sunyaev-Zel'dovich Selected Galaxy Clusters at 148 GHz from Three Seasons of Data
- A complete sample of twelve very X-ray luminous galaxy clusters at z>0.5
- The Atacama Cosmology Telescope: Sunyaev Zel'dovich Selected Galaxy Clusters at 148 GHz in the 2008 Survey
- Galaxy clusters discovered via the Sunyaev-Zel'dovich effect in the first 720 square degrees of the South Pole Telescope survey
- A Spitzer-Selected Galaxy Cluster at z=1.62
- Clusters of Galaxies in the First Half of the Universe from the IRAC Shallow Survey
- Discovery of an X-ray-Luminous Galaxy Cluster at z=1.4
- The X-ray brightest clusters of galaxies from the Massive Cluster Survey
- The Era of Star Formation in Galaxy Clusters
- Spectroscopic Confirmation of the Rich z=1.80 Galaxy Cluster JKCS 041 Using the WFC3 Grism: Environmental Trends in the Ages and Structure of Quiescent Galaxies
- The XMM Cluster Survey: A Massive Galaxy Cluster at z=1.45
- The XMM Cluster Survey: Optical analysis methodology and the first data release
- X-ray Properties of the First SZE-selected Galaxy Cluster Sample from the South Pole Telescope
- Spectroscopic Confirmation of Two Massive Red-Sequence-Selected Galaxy Clusters at z ~ 1.2 in the SpARCS-North Cluster Survey
- IDCS J1426+3508: Discovery of a Massive, IR-Selected Galaxy Cluster at z = 1.75
- Chandra and XMM-Newton Observations of RDCS1252.9-2927, A Massive Cluster at z=1.24
- Discovery of a Rich Cluster at z = 1.63 using the Rest-Frame 1.6um "Stellar Bump Sequence" Method
- Redshifts, Sample Purity, and BCG Positions for the Galaxy Cluster Catalog from the first 720 Square Degrees of the South Pole Telescope Survey
- SPT-CL J0546-5345: A Massive z > 1 Galaxy Cluster Selected Via the Sunyaev-Zel'dovich Effect with the South Pole Telescope
- The X-ray luminous galaxy cluster population at 0.9<z<~1.6 as revealed by the XMM-Newton Distant Cluster Project
- Observations of High-Redshift X-Ray Selected Clusters with the Sunyaev-Zel'dovich Array
- The X-ray luminous galaxy cluster XMMU J1007.4+1237 at z=1.56 - The dawn of starburst activity in cluster cores
- IDCS J1433.2+3306: An IR-Selected Galaxy Cluster at z = 1.89
- Discovery of a massive X-ray luminous galaxy cluster at z=1.579
- IDCS J1426.5+3508: Sunyaev-Zel'dovich Measurement of a Massive IR-selected Cluster at z=1.75
- Distant galaxy clusters in the XMM Large Scale Structure survey
- H Star Formation Rates of > 1 Galaxy Clusters in the IRAC Shallow Cluster Survey
- SPT-CLJ2040-4451: An SZ-Selected Galaxy Cluster at z = 1.478 With Significant Ongoing Star Formation
- The Massive and Distant Clusters of WISE Survey II: Initial Spectroscopic Confirmation of z ~ 1 Galaxy Clusters Selected from 10,000 Square Degrees
- IDCS J1426.5+3508: Cosmological implications of a massive, strong lensing cluster at Z = 1.75
- The Massive Distant Clusters of WISE Survey: The First Distant Galaxy Cluster Discovered by WISE
- CARMA Measurements of the Sunyaev-Zel'dovich Effect in RXJ1347.5-1145
- Offsets between the X-ray and the Sunyaev-Zel'dovich-effect peaks in merging galaxy clusters and their cosmological implications
- Candidate Clusters of Galaxies at Identified in the Spitzer SPT Deep Field Survey
- Spectroscopic confirmation of a galaxy cluster associated with 7C1756+6520 at z=1.416
Cited by in corpus (31)
- Planck 2013 results. XXIX. The Planck catalogue of Sunyaev-Zeldovich sources: Addendum
- The Massive and Distant Clusters of WISE Survey. I: Survey Overview and a Catalog of >2000 Galaxy Clusters at z~1
- Grism Confirmation of Structures at from the Clusters Around Radio-Loud AGN (CARLA) Survey
- Characterising filaments in the SDSS volume from the galaxy distribution
- The XXL Survey: XVII. X-ray and Sunyaev-Zel'dovich Properties of the Redshift 2.0 Galaxy Cluster XLSSC 122
- The Growth of Brightest Cluster Galaxies and Intracluster Light Over the Past Ten Billion Years
- Like a spider in its web: a study of the Large Scale Structure around the Coma cluster
- The rate of Type-Ia supernovae in galaxy clusters and the delay-time distribution out to redshift 1.75
- Constraints on the Thermal Contents of the X-ray Cavities of Cluster MS 0735.6+7421 with Sunyaev-Zel'dovich Effect Observations
- Evidence for the existence of abundant intracluster light at z= 1.24
- The High-Redshift Clusters Occupied by Bent Radio AGN (COBRA) Survey: The \spitzer Catalog
- The Massive and Distant Clusters of WISE Survey IV: The Distribution of Active Galactic Nuclei in Galaxy Clusters at
- A sample of 1959 massive galaxy clusters at high redshifts
- The Discovery of a Gravitationally Lensed Supernova Ia at Redshift 2.22
- The Massive and Distant Clusters of WISE Survey: MOO J1142+1527, A 10 M Galaxy Cluster at z=1.19
- 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
- Spectroscopic Confirmation of Five Galaxy Clusters at z > 1.25 in the 2500 sq. deg. SPT-SZ Survey
- Physical properties of Brightest Cluster Galaxies up to redshift 1.80 based on HST data
- Thermodynamic evolution of the galaxy cluster IDCS J1426.5+3508
- The High-Redshift Clusters Occupied by Bent Radio AGN (COBRA) Survey: Follow-Up Optical Imaging
- The HST See Change Program: I. Survey Design, Pipeline, and Supernova Discoveries
- The High-Redshift Clusters Occupied by Bent Radio AGN (COBRA) Survey: Radio Source Properties
- The Massive and Distant Clusters of WISE Survey V: Extended Radio Sources in Massive Galaxy Clusters at z~1
- The Massive and Distant Clusters of WISE Survey VI: Stellar Mass Fractions of a Sample of High-Redshift Infrared-selected Clusters
- 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
- The Massive and Distant Clusters of WISE Survey: SZ effect Verification with the Atacama Compact Array -- Localization and Cluster Analysis
- Mass-Richness relations for X-ray and SZE-selected clusters at as seen by at 4.5m
- See Change: VLT spectroscopy of a sample of high-redshift Type Ia supernova host galaxies
- Low Surface Brightness Galaxies in z > 1 Galaxy Clusters: HST approaches the Progenitors of Local Ultra Diffuse Galaxies
- The Massive and Distant Clusters of WISE Survey XI: Stellar Mass Fractions and Luminosity Functions of MaDCoWS Clusters at
- Hosts and environments: a (large-scale) radio history of AGN and star-forming galaxies