A Mature Galaxy Cluster at z=1.58 around the Radio Galaxy 7C1753+6311
HST Grism Confirmation of 16 Structures at 1.4 < z < 2.8 from the Clusters Around Radio-Loud AGN (CARLA) Survey
HST Grism Confirmation of Two z ~ 2 Structures from the Clusters around Radio-loud AGN (CARLA) Survey
Massive molecular gas reservoir around the central AGN in the CARLA J1103 + 3449 cluster at z = 1.44
Morphology-density relation, quenching, and mergers in CARLA clusters and protoclusters at 1.4 < z < 2.8
The galaxy mass-size relation in CARLA clusters and proto-clusters at 1.4 < z < 2.8: Larger cluster galaxy sizes
Instrument
WFC3, WFC3/IR
Temporal Coverage
2014-10-14T18:07:04Z/2016-03-03T20:52:38Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Stern comma Daniel K, 2017, 'Clusters Around Radio-Loud AGN: Spectroscopy of Infrared-Selected Galaxy Clusters at z>1.4', 1.0, European Space Agency, https://doi.org/10.5270/esa-kz46jsb