Why z > 1 radio-loud galaxies are commonly located in protoclusters
Main Authors: | 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 |
---|---|
Format: | Journal article |
Published: |
2014
|
Similar Items
-
GALAXY CLUSTERS AROUND RADIO-LOUD ACTIVE GALACTIC NUCLEI AT 1.3 < z < 3.2 AS SEEN BY SPITZER
by: Wylezalek, D, et al.
Published: (2013) -
A mature galaxy cluster at z = 1.58 around the radio galaxy 7C 1753+6311
by: Cooke, E, et al.
Published: (2016) -
THE GALAXY CLUSTER MID-INFRARED LUMINOSITY FUNCTION AT 1.3 < z < 3.2
by: Wylezalek, D, et al.
Published: (2014) -
HST grism confirmation of 16 structures at 1.4 < z < 2.8 from the Clusters Around Radio-Loud AGN (CARLA) survey
by: Noirot, G, et al.
Published: (2018) -
Brightest Cluster Galaxy Formation in the z = 4.3 Protocluster SPT 2349-56: Discovery of a Radio-loud Active Galactic Nucleus
by: Scott C. Chapman, et al.
Published: (2024-01-01)