AGNs in massive galaxy clusters: Role of galaxy merging, infalling groups, cluster mass, and dynamical state
Far-ultraviolet morphology of star-forming filaments in cool core brightest cluster galaxies
Galaxy Populations in Massive z = 0.2-0.9 Clusters. I. Analysis of Spectroscopy
Hubble Space Telescope Far-ultraviolet Observations of Brightest Cluster Galaxies: The Role of Star Formation in Cooling Flows and BCG Evolution
Kinematics, turbulence, and star formation of z ~ 1 strongly lensed galaxies seen with MUSE
LoCuSS: A Dynamical Analysis of X-Ray Active Galactic Nuclei in Local Clusters
LoCuSS: connecting the dominance and shape of brightest cluster galaxies with the assembly history of massive clusters
LoCuSS: first results from strong-lensing analysis of 20 massive galaxy clusters at z = 0.2
Occurrence of Radio Minihalos in a Mass-limited Sample of Galaxy Clusters
Radial profiles of lensed z ~ 1 galaxies on sub-kiloparsec scales
Resolved spectroscopy of gravitationally lensed galaxies: global dynamics and star-forming clumps on ~100 pc scales at 1 < z < 4
Separating the BL Lac and cluster X-ray emissions in Abell 689 with Chandra
Unveiling C II clumps in a lensed star-forming galaxy at z ~ 3.4
X-Ray Properties of AGN in Brightest Cluster Galaxies. I. A Systematic Study of the Chandra Archive in the 0.2 < z < 0.3 and 0.55 < z < 0.75 Redshift Range
Instrument
WFPC2, WFPC2/PC, WFPC2/WFC
Temporal Coverage
2007-08-10T22:08:16Z/2008-07-01T03:08:57Z
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, Smith comma Graham, 2008, 'The Local Cluster Substructure Survey {LoCuSS}: Deep Strong Lensing Observations with WFPC2', 1.0, European Space Agency, https://doi.org/10.5270/esa-ut5hw01
