Abell 851 and the Role of Starbursts in Cluster Galaxy Evolution
A Cluster of Nascent Galaxies at Z = 2?
A simultaneous maximum likelihood approach for galaxy-galaxy lensing and cluster lens reconstruction
Detectability and incidence of E+A galaxies in the distant cluster Cl0939+472 (z=0.41).
Evolution of Infrared-selected Galaxies in Z approximately 0.4 Clusters
Optical Signatures of High-Redshift Galaxy Clusters
Spitzer 24 mm Detections of Starburst Galaxies in Abell 851
The life-cycle of star formation in distant clusters
The Morphology of Distant Cluster Galaxies. I. HST Observations of CL 0939+4713
The Morphology of Distant Cluster Galaxies. II. HST Observations of Four Rich Clusters at z ~= 0.4
Instrument
WFPC/WFC
Temporal Coverage
1992-03-23T01:06:17Z/1992-03-25T12:30:57Z
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, Dressler comma Alan, 1993, 'MORPHOLOGY OF GALAXIES IN CLUSTERS AT Z = 0.5 : CYCLE 1 OBSERVATIONS - PART 2', 1.0, European Space Agency, https://doi.org/10.5270/esa-h16ux3y