The Massive Distant Clusters of WISE Survey: The First Distant Galaxy Cluster Discovered by WISE
arXiv:1205.7092 · doi:10.1088/2041-8205/759/1/L23
Abstract
We present spectroscopic confirmation of a z=0.99 galaxy cluster discovered using data from the Wide-field Infrared Survey Explorer (WISE). This is the first z~1 cluster candidate from the Massive Distant Clusters of WISE Survey (MaDCoWS) to be confirmed. It was selected as an overdensity of probable z>~1 sources using a combination of WISE and SDSS-DR8 photometric catalogs. Deeper follow-up imaging data from Subaru and WIYN reveal the cluster to be a rich system of galaxies, and multi-object spectroscopic observations from Keck confirm five cluster members at z=0.99. The detection and confirmation of this cluster represents a first step towards constructing a uniformly-selected sample of distant, high-mass galaxy clusters over the full extragalactic sky using WISE data.
6 pages, 5 figures, ApJL Accepted
References in corpus (11)
- A direct empirical proof of the existence of dark matter
- The XMM-Newton wide-field survey in the COSMOS field: VI. Statistical properties of clusters of galaxies
- Strong and weak lensing united III: Measuring the mass distribution of the merging galaxy cluster 1E0657-56
- Symmetries for Galileons and DBI scalars on curved space
- IDCS J1426+3508: Discovery of a Massive, IR-Selected Galaxy Cluster at z = 1.75
- EzGal: A Flexible Interface for Stellar Population Synthesis Models
- The Angular Clustering of Distant Galaxy Clusters
- IDCS J1433.2+3306: An IR-Selected Galaxy Cluster at z = 1.89
- IDCS J1426.5+3508: Sunyaev-Zel'dovich Measurement of a Massive IR-selected Cluster at z=1.75
- Implications of multiple high-redshift galaxy clusters
- IDCS J1426.5+3508: Cosmological implications of a massive, strong lensing cluster at Z = 1.75
Cited by in corpus (28)
- Galaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ survey
- Galaxy Clusters around radio-loud AGN at 1.3 < z < 3.2 as seen by Spitzer
- Characterizing the Mid-IR Extragalactic Sky with WISE and SDSS
- An optically-selected cluster catalog at redshift 0.1<z<1.1 from the Hyper Suprime-Cam Subaru Strategic Program S16A data
- The Massive and Distant Clusters of WISE Survey. I: Survey Overview and a Catalog of >2000 Galaxy Clusters at z~1
- SPT-CLJ2040-4451: An SZ-Selected Galaxy Cluster at z = 1.478 With Significant Ongoing Star Formation
- The GEEC2 spectroscopic survey of Galaxy Groups at
- The Massive and Distant Clusters of WISE Survey II: Initial Spectroscopic Confirmation of z ~ 1 Galaxy Clusters Selected from 10,000 Square Degrees
- The Massive and Distant Clusters of WISE Survey. III. Sunyaev-Zel'dovich Masses of Galaxy Clusters at
- KAT-7 Science Verification: Cold Gas, Star Formation, and Substructure in the Nearby Antlia Cluster
- Evidence for the existence of abundant intracluster light at z= 1.24
- The Massive and Distant Clusters of WISE Survey IV: The Distribution of Active Galactic Nuclei in Galaxy Clusters at
- The X-CLASS - redMaPPer galaxy cluster comparison: I. Identification procedures
- 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
- Candidate Clusters of Galaxies at Identified in the Spitzer SPT Deep Field Survey
- Spectroscopic Confirmation of Five Galaxy Clusters at z > 1.25 in the 2500 sq. deg. SPT-SZ Survey
- Prospects for high-z cluster detections with Planck, based on a follow-up of 28 candidates using MegaCam@CFHT
- A Multi-Wavelength Mass Analysis of RCS2 J232727.6-020437, a ~3x10M Galaxy Cluster at z=0.7
- The 2XMMi/SDSS Galaxy Cluster Survey. III. Clusters associated with spectroscopically targeted luminous red galaxies in SDSS-DR10
- Serendipitous detection of an overdensity of Herschel-SPIRE 250 micron sources south of MRC1138-26
- The Massive and Distant Clusters of WISE Survey VI: Stellar Mass Fractions of a Sample of High-Redshift Infrared-selected Clusters
- Synthesizing Stellar Populations in South Pole Telescope Galaxy Clusters: I. Ages of Quiescent Member Galaxies at 0.3 < z < 1.4
- The Spitzer-IRAC/MIPS Extragalactic survey (SIMES) in the South Ecliptic Pole field
- CARMA observations of massive Planck-discovered cluster candidates at z>0.5 associated with WISE overdensities: Breaking the size-flux degeneracy
- CARMA observations of massive Planck-discovered cluster candidates at z>0.5 associated with WISE overdensities: strategy, observations and validation
- Distant clusters of galaxies in the 2XMM/SDSS footprint: follow-up observations with the LBT