Why z > 1 radio-loud galaxies are commonly located in protoclusters

Why z > 1 radio-loud galaxies are commonly located in protoclusters

Manylion Llyfryddiaeth
Prif Awduron:	Hatch, N, Wylezalek, D, Kurk, J, Stern, D, De Breuck, C, Jarvis, M, Galametz, A, Gonzalez, A, Hartley, W, Mortlock, A, Seymour, N, Stevens, J
Fformat:	Journal article
Cyhoeddwyd:	2014

Eitemau Tebyg

GALAXY CLUSTERS AROUND RADIO-LOUD ACTIVE GALACTIC NUCLEI AT 1.3 < z < 3.2 AS SEEN BY SPITZER
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A mature galaxy cluster at z = 1.58 around the radio galaxy 7C 1753+6311
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HST grism confirmation of 16 structures at 1.4 < z < 2.8 from the Clusters Around Radio-Loud AGN (CARLA) survey
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Brightest Cluster Galaxy Formation in the z = 4.3 Protocluster SPT 2349-56: Discovery of a Radio-loud Active Galactic Nucleus
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The formation history of massive cluster galaxies as revealed by CARLA
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HI in the protocluster environment at z > 2: absorbing haloes and the Ly alpha forest
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A Protocluster of Massive Quiescent Galaxies at z = 4
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Identification of Galaxy Protoclusters Based on the Spherical Top-hat Collapse Theory
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The Obelisk simulation: galaxies contribute more than AGN to HI reionization of protoclusters
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Spectral age distribution for radio-loud active galaxies in the XMM-LSS field
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ODIN: Identifying Protoclusters and Cosmic Filaments Traced by Lyα-emitting Galaxies
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The Stability of Dense Cores near the Serpens South Protocluster
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Kinematic Analysis of z = 4.3 Galaxies in the SPT2349–56 Protocluster Core
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$\textit{Herschel}$-ATLAS:The connection between star formation and AGN activity in radio-loud and radio-quiet active galaxies
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Spectroscopic Confirmation of an Ultra-Massive Galaxy in a Protocluster at $z \sim 4.9$
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The Emergence of a Brightest Cluster Galaxy in a Protocluster Core at z = 2.24
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COSMOS2020: Discovery of a Protocluster of Massive Quiescent Galaxies at z = 2.77
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RAPID COEVAL BLACK HOLE AND HOST GALAXY GROWTH IN MRC 1138-262: THE HUNGRY SPIDER
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Observational Evidence for Large-scale Gas Heating in a Galaxy Protocluster at z = 2.30
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Gas-rich mergers and feedback are ubiquitous amongst starbursting radio galaxies, as revealed by the VLA, IRAM PdBI and Herschel
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Powerful Radio-loud Quasars Are Triggered by Galaxy Mergers in the Cosmic Bright Ages
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COALAS: I. ATCA CO(1-0) survey and luminosity function in the Spiderweb protocluster at z=2.16
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A Search for Blazar-Like Radio-Loud Narrow-Line Seyfert 1 Galaxies
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Is there enough star formation in simulated protoclusters?
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Revealing the Quiescent Galaxy Population in the Spiderweb Protocluster at z = 2.16 with Deep HST/WFC3 Slitless Spectroscopy
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A Quasar-anchored Protocluster at z = 6.6 in the ASPIRE Survey. II. An Environmental Analysis of Galaxy Properties in an Overdense Structure
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Formation of Protoclusters in the Tank Industry of the Urals in 1941–1945
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