GALAXY CLUSTERS DISCOVERED VIA THE SUNYAEV-ZEL'DOVICH EFFECT IN THE 2500-SQUARE-DEGREE SPT-SZ SURVEY

We present a catalog of galaxy clusters selected via their Sunyaev-Zel'dovich (SZ) effect signature from 2500 deg[superscript 2] of South Pole Telescope (SPT) data. This work represents the complete sample of clusters detected at high significance in the 2500 deg[superscript 2] SPT-SZ survey, w...

Full description

Bibliographic Details
Main Authors: Bautz, Marshall W. (Contributor), McDonald, Michael A. (Contributor)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2015-04-24T14:38:23Z.
Subjects:
Online Access:Get fulltext
LEADER 02325 am a22001933u 4500
001 96784
042 |a dc 
100 1 0 |a Bautz, Marshall W.  |e author 
100 1 0 |a MIT Kavli Institute for Astrophysics and Space Research  |e contributor 
100 1 0 |a Bautz, Marshall W.  |e contributor 
100 1 0 |a McDonald, Michael A.  |e contributor 
700 1 0 |a McDonald, Michael A.  |e author 
245 0 0 |a GALAXY CLUSTERS DISCOVERED VIA THE SUNYAEV-ZEL'DOVICH EFFECT IN THE 2500-SQUARE-DEGREE SPT-SZ SURVEY 
260 |b IOP Publishing,   |c 2015-04-24T14:38:23Z. 
856 |z Get fulltext  |u http://hdl.handle.net/1721.1/96784 
520 |a We present a catalog of galaxy clusters selected via their Sunyaev-Zel'dovich (SZ) effect signature from 2500 deg[superscript 2] of South Pole Telescope (SPT) data. This work represents the complete sample of clusters detected at high significance in the 2500 deg[superscript 2] SPT-SZ survey, which was completed in 2011. A total of 677 (409) cluster candidates are identified above a signal-to-noise threshold of ξ = 4.5 (5.0). Ground- and space-based optical and near-infrared (NIR) imaging confirms overdensities of similarly colored galaxies in the direction of 516 (or 76%) of the ξ > 4.5 candidates and 387 (or 95%) of the ξ > 5 candidates; the measured purity is consistent with expectations from simulations. Of these confirmed clusters, 415 were first identified in SPT data, including 251 new discoveries reported in this work. We estimate photometric redshifts for all candidates with identified optical and/or NIR counterparts; we additionally report redshifts derived from spectroscopic observations for 141 of these systems. The mass threshold of the catalog is roughly independent of redshift above z ~ 0.25 leading to a sample of massive clusters that extends to high redshift. The median mass of the sample is M [subscript 500c](ρ[subscript crit]) ~ 3.5 x 10[superscript 14] M[subscript ʘ] h[-1 over 70], the median redshift is z [subscript med] = 0.55, and the highest-redshift systems are at z > 1.4. The combination of large redshift extent, clean selection, and high typical mass makes this cluster sample of particular interest for cosmological analyses and studies of cluster formation and evolution. 
546 |a en_US 
655 7 |a Article 
773 |t The Astrophysical Journal. Supplement Series