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The American Astronomical Society (AAS), established in 1899 and based in Washington, DC, is the major organization of professional astronomers in North America. Its membership of about 7,000 individuals also includes physicists, mathematicians, geologists, engineers, and others whose research and educational interests lie within the broad spectrum of subjects comprising contemporary astronomy. The mission of the AAS is to enhance and share humanity's scientific understanding of the universe.

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Groups of Galaxies in the Two Micron All Sky Redshift Survey

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© 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A.
,,Citation Aidan C. Crooket al 2007ApJ655 790DOI 10.1086/510201

This article is corrected by2008ApJ685 1320

Aidan C. Crook

AFFILIATIONS

Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA

John P. Huchra

AFFILIATIONS

Harvard-Smithsonian Center for Astrophysics, Cambridge, MA

Visiting Astronomer, Cerro Tololo Inter-American Observatory. CTIO is operated by AURA, Inc., under contract to the National Science Foundation

Nathalie Martimbeau

AFFILIATIONS

Harvard-Smithsonian Center for Astrophysics, Cambridge, MA

Karen L. Masters

AFFILIATIONS

Harvard-Smithsonian Center for Astrophysics, Cambridge, MA

Tom Jarrett

AFFILIATIONS

Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA

Lucas M. Macri

AFFILIATIONS

National Optical Astronomy Observatories, Tucson, AZ

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Dates

  1. Received2006 June 2
  2. Accepted2006 October 6
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0004-637X/655/2/790

Abstract

We present the results of applying a percolation algorithm to the initial release of the Two Micron All Sky Survey Extended Source Catalog, using subsequently measured redshifts for almost all of the galaxies withK < 11.25 mag. This group catalog is based on the first near-IR all-sky flux-limited survey that is complete to |b| = 5°. We explore the dependence of the clustering on the length and velocity scales involved. The paper describes a group catalog, complete to a limiting redshift of 104 km s-1, created by maximizing the number of groups containing three or more members. A second catalog is also presented, created by requiring a minimum density contrast of δρ/ρ ≥ 80 to identify groups. We identify known nearby clusters in the catalogs and contrast the groups identified in the two catalogs. We examine and compare the properties of the determined groups and verify that the results are consistent with the UZC-SSRS2 and northern CfA redshift survey group catalogs. The all-sky nature of the catalog will allow the development of a flow-field model based on the density field inferred from the estimated cluster masses.

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10.1086/510201

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