A Comparison of Direct and Indirect Mass Estimates for Distant Clusters of Galaxies
A Hubble Space Telescope lensing survey of X-ray-luminous galaxy clusters - II. A search for gravitationally lensed EROs *
A Hubble Space Telescope lensing survey of X-ray luminous galaxy clusters - IV. Mass, structure and thermodynamics of cluster cores at z= 0.2
A New Survey for Giant Arcs
Arcfinder: an algorithm for the automatic detection of gravitational arcs
A simple prescription for simulating and characterizing gravitational arcs
A Systematic Search for Gravitationally Lensed Arcs in the Hubble Space Telescope WFPC2 Archive
Deep Near-Infrared Luminosity Function of a Cluster of Galaxies at Z=0.3
Detecting compact dark matter in galaxy clusters via gravitational microlensing: A2218 and A370
Diffuse stellar emission in X-ray luminous galaxy clusters at z ~ 0.3. I. Is the diffuse optical light boosted and rejuvenated in merging clusters?
Distinguishing Local and Global Influences on Galaxy Morphology: A Hubble Space Telescope Comparison of High and Low X-Ray Luminosity Clusters
Evidence for Tidal Stripping of Dark Matter Halos in Massive Cluster Lenses
Evidence of Cosmic Evolution of the Stellar Initial Mass Function
Evolution of Cluster Ellipticals at 0.2 < z < 1.2 from Hubble Space Telescope Imaging,
Galaxies under the Cosmic Microscope: A Gemini Multiobject Spectrograph Study of Lensed Disk Galaxy 289 in A2218
Galaxy properties in low X-ray luminosity clusters at z=0.25
Gravitational Microlensing of Giant Luminous Arcs: a Test for Compact Dark Matter in Clusters of Galaxies
Hubble Space Telescope Observations of Giant Arcs: High-Resolution Imaging of Distant Field Galaxies
Hubble Space Telescope Observations of the Lensing Cluster Abell 2218
Identification of a gravitationally lensed z=2.515 star-forming galaxy
LoCuSS: connecting the dominance and shape of brightest cluster galaxies with the assembly history of massive clusters
Measuring the matter distribution within z = 0.2 cluster lenses with XMM-Newton
Molecular Gas and Dust at z=2.6 in SMM J14011+0252: A Strongly Lensed Ultraluminous Galaxy, Not a Huge Massive Disk
Morphological Studies of the Galaxy Populations in Distant ``Butcher-Oemler Clusters with the Hubble Space Telescope. II. AC 103, AC 118, and AC 114 at Z = 0.31
New Constraints on the Luminosity Evolution of Spheroidal Galaxies in Distant Clusters
Number counts and redshift distribution of gravitational arclets as a probe of galaxy evolution
Optical and Near-Infrared Structural Properties of Cluster Galaxies at z ~ 0.3
Spectroscopic confirmation of redshifts predicted by gravitational lensing
Testing a Coupling Relation between Visible and Dark Matter in the MS 2137-2353 Cluster Core
The early-type galaxy population in Abell 2218
The emission line properties of gravitationally lensed 1.5 < z < 5 galaxies
The evolution of cluster E and S0 galaxies measured from the Fundamental Plane
The Evolution of the Galactic Morphological Types in Clusters
The Lensed Arc Production Efficiency of Galaxy Clusters: A Comparison of Matched Observed and Simulated Samples
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1994-09-03T04:08:16Z/1995-06-11T01:25:37Z
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, Couch comma Warrick J., 1996, 'GALAXY POPULATIONS IN INTERMEDIATE REDSHIFT CLUSTERS: CYCLE 4 CARRY-OVER', 1.0, European Space Agency, https://doi.org/10.5270/esa-trig47u
