A High Merger Fraction in the Rich Cluster MS 1054-03 at Z = 0.83: Direct Evidence for Hierarchical Formation of Massive Galaxies
A New Survey for Giant Arcs
A Systematic Search for Gravitationally Lensed Arcs in the Hubble Space Telescope WFPC2 Archive
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
Dusty ERO Search behind Two Massive Clusters
Evolution in the Color-Magnitude Relation of Early-Type Galaxies in Clusters of Galaxies at z~=1
Evolution of the near-infrared in rich galaxy clusters
Evolution since z = 1 of the Morphology-Density Relation for Galaxies
Luminosity Evolution of Early-Type Galaxies to z = 0.83: Constraints on Formation Epoch and O
Mass Distributions of Hubble Space Telescope Galaxy Clusters from Gravitational Arcs
Measurements of O and L from 42 High-Redshift Supernovae
Supernovae in deep Hubble Space Telescope galaxy cluster fields: cluster rates and field counts
The distribution of star-forming galaxies in intermediate redshift galaxy clusters
The Hubble diagram of type Ia supernovae as a function of host galaxy morphology
The Mass, Baryonic Fraction, and X-Ray Temperature of the Luminous, High-Redshift Cluster of Galaxies MS 0451.6-0305
The nature of a gravitationally lensed submillimetre arc in MS0451.6-0305: two interacting galaxies at z~ 2.9?
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1995-11-15T13:19:17Z/1997-05-02T16:09:14Z
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, Donahue comma Megan, 1998, 'WFPC Observations of Distant, X-ray Luminous Clusters of Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-kucsi3m
