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Title: The Massive and Distant Clusters of WISE Survey. I. Survey Overview and a Catalog of >2000 Galaxy Clusters at z ≃ 1

Journal Article · · The Astrophysical Journal. Supplement Series (Online)
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  1. Univ. of Florida, Gainesville, FL (United States)
  2. Univ. of Missouri, Kansas City, MO (United States)
  3. California Inst. of Technology (CalTech), Pasadena, CA (United States)
  4. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States); Univ. of California, Davis, CA (United States)
  5. European Southern Observatory, Garching bei München (Germany)
  6. Univ. of Arizona, Tucson, AZ (United States)
  7. LSST, Tucson, AZ (United States)
  8. Univ. of Chicago, IL (United States)
  9. Univ. of Missouri, Kansas City, MO (United States); Univ. of Michigan, Ann Arbor, MI (United States)
  10. Univ. of Hawaii, Honolulu, HI (United States)
  11. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
  12. Academia Sinica, Taipei (Taiwan)
  13. Stanford Univ., CA (United States)
  14. Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States)
  15. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States)
  16. Univ. of California, Los Angeles, CA (United States)
  17. Univ. of Texas, Austin, TX (United States)
+ Show Author Affiliations

We introduce the Massive and Distant Clusters of WISE Survey (MaDCoWS), a search for galaxy clusters at 0.7 ≲ z ≲ 1.5 based upon data from the Wide-field Infrared Survey Explorer (WISE) mission. MaDCoWS is the first cluster survey capable of discovering massive clusters at these redshifts over the full extragalactic sky. The search is divided into two regions—the region of the extragalactic sky covered by Pan-STARRS (δ > –30°) and the remainder of the southern extragalactic sky at δ < –30° for which shallower optical data from the SuperCOSMOS Sky Survey is available. Here, we describe the search algorithm, characterize the sample, and present the first MaDCoWS data release—catalogs of the 2433 highest amplitude detections in the WISE–Pan-STARRS region and the 250 highest amplitude detections in the WISE–SuperCOSMOS region. A total of 1723 of the detections from the WISE–Pan-STARRS sample have also been observed with the Spitzer Space Telescope, providing photometric redshifts and richnesses, and an additional 64 detections within the WISE–SuperCOSMOS region also have photometric redshifts and richnesses. Spectroscopic redshifts for 38 MaDCoWS clusters with IRAC photometry demonstrate that the photometric redshifts have an uncertainty of σ z/(1 + z) ≃ 0.036. Combining the richness measurements with Sunyaev–Zel'dovich observations of MaDCoWS clusters, we also present a preliminary mass–richness relation that can be used to infer the approximate mass distribution of the full sample. The estimated median mass for the WISE–Pan-STARRS catalog is $${M}_{500}={1.6}_{-0.8}^{+0.7}\times {10}^{14}\,{M}_{\odot }$$, with the Sunyaev–Zel'dovich data confirming that we detect clusters with masses up to M 500 ~ 5 × 1014 M ⊙ (M 200 ~ 1015 M ⊙).

Research Organization:
Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)
Sponsoring Organization:
USDOE Office of Science (SC)
Grant/Contract Number:
AC52-07NA27344
OSTI ID:
1545293
Journal Information:
The Astrophysical Journal. Supplement Series (Online), Vol. 240, Issue 2; ISSN 1538-4365
Publisher:
American Astronomical Society/IOPCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 49 works
Citation information provided by
Web of Science

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Galaxy clusters discovered via the Sunyaev-Zel'dovich effect in the first 720 square degrees of the South Pole Telescope survey text January 2012
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The Atacama Cosmology Telescope: Sunyaev-Zel'dovich Selected Galaxy Clusters at 148 GHz from Three Seasons of Data text January 2013
Discovery of a Rich Cluster at z = 1.63 using the Rest-Frame 1.6um "Stellar Bump Sequence" Method text January 2013
HMFcalc: An Online Tool for Calculating Dark Matter Halo Mass Functions preprint January 2013
Cluster Magnification & the Mass-Richness Relation in CFHTLenS text January 2013
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Richness-based masses of rich and famous galaxy clusters text January 2016
Galaxy evolution in protoclusters text January 2017
Optical identifications of high-redshift galaxy clusters from Planck Sunyaev-Zeldovich survey text January 2018
The Massive and Distant Clusters of WISE Survey IV: The Distribution of Active Galactic Nuclei in Galaxy Clusters at $z\sim1$ text January 2018
Bright Type IIP Supernovae in Low-Metallicity Galaxies text January 2018
2MASS Extended Source Catalog: Overview and Algorithms text January 2000
Chandra Observations of the Lensing Cluster EMSS 1358+6245: Implications for Self-Interacting Dark Matter text January 2001
Stellar population synthesis at the resolution of 2003 text January 2003
Weak lensing mass reconstruction of the interacting cluster 1E0657-558: Direct evidence for the existence of dark matter text January 2003
Batch discovery of nine z~1 clusters using x-ray and K or R,z' images text January 2005
A MaxBCG Catalog of 13,823 Galaxy Clusters from the Sloan Digital Sky Survey text January 2007
Redshift Evolution of Galaxy Cluster Densities text January 1996
The ROSAT Brightest Cluster Sample (BCS) - I. The compilation of the sample and the cluster log N-log S distribution text January 1998
Reversal of Fortune: Confirmation of an Increasing Star Formation-Density Relation in a Cluster at z = 1.62 text January 2010

Cited By (4)

ComPRASS: a Combined Planck -RASS catalogue of X-ray-SZ clusters journal May 2019
The High-redshift Clusters Occupied by Bent Radio AGN (COBRA) Survey: Follow-up Optical Imaging journal December 2019
The Massive and Distant Clusters of WISE Survey. VII. The Environments and Properties of Radio Galaxies in Clusters at z ∼ 1 journal January 2020
The Massive and Distant Clusters of WISE Survey VII: The Environments and Properties of Radio Galaxies in Clusters at z~1 text January 2019

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