GALAXY CLUSTERS AROUND RADIO-LOUD ACTIVE GALACTIC NUCLEI AT 1.3 < z < 3.2 AS SEEN BY SPITZER

We report the first results from the Clusters Around Radio-Loud AGN program, a Cycle 7 and 8 Spitzer Space Telescope snapshot program to investigate the environments of a large sample of obscured and unobscured luminous radio-loud active galactic nuclei (AGNs) at 1.2 < z < 3.2. We investigate...

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Published inThe Astrophysical journal Vol. 769; no. 1; pp. 1 - 10
Main Authors WYLEZALEK, DOMINIKA, GALAMETZ, AUDREY, Stern, Daniel, Vernet, Joel, De Breuck, Carlos, Seymour, Nick, Brodwin, Mark, Eisenhardt, Peter R M, Gonzalez, Anthony H, Hatch, Nina
Format Journal Article
LanguageEnglish
Published United States 20.05.2013
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Summary:We report the first results from the Clusters Around Radio-Loud AGN program, a Cycle 7 and 8 Spitzer Space Telescope snapshot program to investigate the environments of a large sample of obscured and unobscured luminous radio-loud active galactic nuclei (AGNs) at 1.2 < z < 3.2. We investigate how environment depends on AGN type (unobscured radio-loud quasars versus obscured radio galaxies), radio luminosity and redshift, finding no correlation with either AGN type or radio luminosity. We find a decrease in density with redshift, consistent with galaxy evolution for this uniform, flux-limited survey. These results are consistent with expectations from the orientation-driven AGN unification model, at least for the high radio luminosity regimes considered in this sample.
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ISSN:0004-637X
1538-4357
DOI:10.1088/0004-637X/769/1/79