B-band galaxy counts as a function of morphological type
Catalog of Galaxy Morphology in Four Rich Clusters: Luminosity Evolution of Disk Galaxies at 0.33 < z < 0.83
Constraints on the Size Evolution of Brightest Cluster Galaxies
Merger-driven Growth of Intermediate-mass Black Holes: Constraints from Hubble Space Telescope Imaging of Hyper-luminous X-Ray Sources
Resolved spectroscopy of gravitationally lensed galaxies: global dynamics and star-forming clumps on ~100 pc scales at 1 < z < 4
Spectroscopy of Luminous Compact Blue Galaxies in Distant Clusters. II. Physical Properties of dE Progenitor Candidates
The distribution of star-forming galaxies in intermediate redshift galaxy clusters
The Nature of E+A Galaxies in Intermediate-Redshift Clusters
The role of environment in the morphological transformation of galaxies in 9 rich intermediate redshift clusters
Unveiling C II clumps in a lensed star-forming galaxy at z ~ 3.4
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1998-12-21T01:58:14Z/1999-09-07T00:12:53Z
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, Schade comma David, 2000, 'Quantitative measures of the evolution of the cluster galaxy population', 1.0, European Space Agency, https://doi.org/10.5270/esa-v9ozwaf