PI: Joshua Wing, Boston University, email@example.com
Address: Astronomy Department, 725 Commonwealth Ave. Rm. 514, Boston, MA 02215, United States
CoI: Elizabeth Blanton, Boston University
Title: Radio Selected Clusters of Galaxies at High Redshift
Abstract: Previous studies have shown that three-component radio sources exhibiting some degree of bending between components are likely to be found in galaxy clusters. Often this radio emission is associated with a cD type galaxy at the center of a cluster. We have cross-correlated the Sloan Digital Sky Survey (SDSS) with samples selected from the Faint Images of the Radio Sky at Twenty Centimeters (FIRST) catalog and measured the richness of the cluster environments surrounding three- component sources exhibiting both bent and straight lobes. This has lead to the discovery and classification of a large number of galaxy clusters out to a redshift of z ~ 0.6. For both bent- and straight- lobed sources without an optical counterpart it is likely that the radio emission is associated with a galaxy fainter than m_r=22 (the limiting magnitude of the SDSS) and at a redshift higher than z~0.8. We propose to observe a small sub-sample of these sources with the NEWFIRM instrument on the Mayall 4-m telescope in an attempt to discover if these sources are located in high redshift (z\gtrsim0.8) galaxy clusters. In our visually-selected bent radio source sample, 69% of sources with counterparts in the SDSS are associated with clusters.
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