A 7 deg2 survey for galaxy-scale gravitational lenses with the HST imaging archive
Cl 1103.7-1245 at z = 0.96: the highest redshift galaxy cluster in the EDisCS survey
Determining the Halo Mass Scale Where Galaxies Lose Their Gas
Disc colours in field and cluster spiral galaxies at 0.5 z 0.8
Discovery of a single faint AGN in a large sample of z > 5 Lyman break galaxies
EDisCS - the ESO distant cluster survey. Sample definition and optical photometry
Evolution of red-sequence cluster galaxies from redshift 0.8 to 0.4: ages, metallicities, and morphologies
Evolution of the early-type galaxy fraction in clusters since z = 0.8
Firedec: a two-channel finite-resolution image deconvolution algorithm
Frequency and properties of bars in cluster and field galaxies at intermediate redshifts
Galaxy sizes as a function of environment at intermediate redshift from the ESO Distant Cluster Survey
Harnessing the Hubble Space Telescope Archives: A Catalog of 21,926 Interacting Galaxies
Intracluster light in clusters of galaxies at redshifts 0.4 < z < 0.8
Ionized gas discs in elliptical and S0 galaxies at z < 1
Link between brightest cluster galaxy properties and large scale extensions of 38 DAFT/FADA and CLASH clusters in the redshift range 0.2 < z < 0.9
Mass profile and dynamical status of the z ~ 0.8 galaxy cluster LCDCS 0504
On the role of the post-starburst phase in the buildup of the red sequence of intermediate-redshift clusters
On the Shapes and Structures of High-redshift Compact Galaxies
Photometric selection of z ~ 5 Lyman break galaxies in the ESO Remote Galaxy Survey
Quantitative measure of evolution of bright cluster galaxies at moderate redshifts
Red Nuggets at High Redshift: Structural Evolution of Quiescent Galaxies Over 10 Gyr of Cosmic History
Spectroscopy of clusters in the ESO distant cluster survey (EDisCS). II.. Redshifts, velocity dispersions, and substructure for clusters in the last 15 fields
Spectroscopy of z~ 5 Lyman break galaxies in the ESO Remote Galaxy Survey
Superdense Massive Galaxies in the ESO Distant Cluster Survey (EDisCS)
The colour-magnitude relation of elliptical and lenticular galaxies in the ESO Distant Cluster Survey
The DAFT/FADA survey. I. Photometric redshifts along lines of sight to clusters in the z = 0.4, 0.9 interval
The effect of the environment on the gas kinematics and the structure of distant galaxies
The effect of the environment on the structure, morphology and star formation history of intermediate-redshift galaxies
The Environments of Starburst and Post-Starburst Galaxies at z = 0.4-0.8
The evolution of early-type galaxies in clusters from z~ 0.8 to z ~ 0: the ellipticity distribution and the morphological mix
The evolution of the brightest cluster galaxies since z ~ 1 from the ESO Distant Cluster Survey (EDisCS)
The Evolution of the Star Formation Activity in Galaxies and Its Dependence on Environment
The fundamental plane of EDisCS galaxies. The effect of size evolution
The galaxy stellar mass function and its evolution with time show no dependence on global environment
The impact of satellite trails on Hubble Space Telescope observations
The Morphological Content of 10 EDisCS Clusters at 0.5 < z < 0.8
The orbital velocity anisotropy of cluster galaxies: evolution
The Relation between Star Formation, Morphology, and Local Density in High-Redshift Clusters and Groups
The time delay between star formation quenching and morphological transformation of galaxies in clusters: a phase-space view of EDisCS
Instrument
ACS, ACS/HRC, ACS/WFC
Temporal Coverage
2002-05-27T02:11:06Z/2004-05-24T11:29:59Z
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, Dalcanton comma Julianne, 2005, 'Galaxy Evolution in the Richest Clusters at z=0.8: the EDisCS Cluster Sample', 1.0, European Space Agency, https://doi.org/10.5270/esa-k67ahwt