Measurements of the Cosmological Parameters O and L from the First Seven Supernovae at z >= 0.35
New Constraints on the Luminosity Evolution of Spheroidal Galaxies in Distant Clusters
Probing early-type galaxy evolution with the Kormendy relation
Probing the Evolution of the Galaxy Interaction/Merger Rate Using Collisional Ring Galaxies
Quantitative measure of evolution of bright cluster galaxies at moderate redshifts
Testing the hypothesis of the morphological transformation from field spiral to cluster S0
The distribution of star-forming galaxies in intermediate redshift galaxy clusters
The Fundamental Plane and the evolution of the M/L ratio of early-type field galaxies up to z~ 1
The Fundamental Plane of Gravitational Lens Galaxies and The Evolution of Early-Type Galaxies in Low-Density Environments
The Gemini/HST Galaxy Cluster Project: Redshift 0.2-1.0 Cluster Sample, X-Ray Data, and Optical Photometry Catalog
The Homogeneity of Spheroidal Populations in Distant Clusters
The Hubble diagram of type Ia supernovae as a function of host galaxy morphology
The Look-back Time Evolution of Far-Ultraviolet Flux from Elliptical Galaxies: The Fornax Cluster and A2670
The nuclear radio-optical properties of intermediate-redshift FR II radio galaxies and quasars
The Origins of X-Ray Emission from the Hot Spots of FR II Radio Sources
The role of E+A and post-starburst galaxies - II. Spectral energy distributions and comparison with observations
The role of environment in the morphological transformation of galaxies in 9 rich intermediate redshift clusters
The Slope of the Cluster Elliptical Red Sequence: A Probe of Cluster Evolution
The Star Formation Epoch of the Most Massive Early-Type Galaxies
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1994-04-18T06:10:17Z/1995-01-14T13:08:57Z
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, Dressler comma Alan, 1996, 'MORPHOLOGICAL EVOLUTION OF GALAXIES IN CLUSTERS AT Z = 0.5', 1.0, European Space Agency, https://doi.org/10.5270/esa-mbpdq3z