A Catalog of Morphological Types in 10 Distant Rich Clusters of Galaxies
A Comparison of Direct and Indirect Mass Estimates for Distant Clusters of Galaxies
A New Survey for Giant Arcs
An ISOCAM survey through gravitationally lensing galaxy clusters. IV. Luminous infrared galaxies in Cl 0024+1654 and the dynamical status of clusters
A panoramic Ha imaging survey of the z= 0.4 cluster Cl0024.0+1652 with Subaru
A Spectroscopic Catalog of 10 Distant Rich Clusters of Galaxies
A Spectroscopic Redshift for the Cl 0024+16 Multiple Arc System: Implications for the Central Mass Distribution
A Systematic Search for Gravitationally Lensed Arcs in the Hubble Space Telescope WFPC2 Archive
A Wide-Field Hubble Space Telescope Study of the Cluster Cl 0024+16 at z = 0.4. I. Morphological Distributions to 5 Mpc Radius
A Wide-Field Hubble Space Telescope Survey of the Cluster Cl 0024+16 at z = 0.4. III. Spectroscopic Signatures of Environmental Evolution in Early-Type Galaxies
Color Gradients in Early-Type Galaxies in Clusters at Redshift 0.37-0.56
Constraints on the Evolution of S0 Galaxies in Rich Clusters at Moderate Redshift
Dynamical Evidence for Environmental Evolution of Intermediate-Redshift Spiral Galaxies
Evidence for Tidal Stripping of Dark Matter Halos in Massive Cluster Lenses
Evolution of the Stellar Mass-Metallicity Relation. I. Galaxies in the z ~ 0.4 Cluster Cl0024
Evolution of the Stellar Mass-Metallicity Relation. II. Constraints on Galactic Outflows from the Mg Abundances of Quiescent Galaxies
Evolution since z = 0.5 of the Morphology-Density Relation for Clusters of Galaxies
Evolution since z = 1 of the Morphology-Density Relation for Galaxies
GALEX Observations of Passive Spirals in the Cluster Cl 0024+17: Clues to the Formation of S0 Galaxies
Mass Distributions of Hubble Space Telescope Galaxy Clusters from Gravitational Arcs
New Constraints on the Luminosity Evolution of Spheroidal Galaxies in Distant Clusters
On the Evolution of the Molecular Gas Fraction of Star-Forming Galaxies
On the Nature of the Strong Emission-Line Galaxies in Cluster CL 0024+1654: Are Some the Progenitors of Low-Mass Spheroidals?
Testing the hypothesis of the morphological transformation from field spiral to cluster S0
The evolving galaxy population of cluster Cl0024+1654
The role of E+A and post-starburst galaxies - II. Spectral energy distributions and comparison with observations
The spatially resolved dynamics of dusty starburst galaxies in a z ~ 0.4 cluster: beginning the transition from spirals to S0s
The Survival of Dark Matter Halos in the Cluster Cl 0024+16
The Tully-Fisher Relation in Cluster Cl 0024+1654 at z=0.4
Unlensing Multiple Arcs in 0024+1654: Reconstruction of the Source Image
XMM-Newton study of the lensing cluster of galaxies CL 0024+17
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1994-10-11T09:43:16Z/1994-10-14T18:39:36Z
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, Turner et al., 1995, 'DEEP WF IMAGING OF THE GIANT LUMINOUS ARCS IN CL0024+16: CYCLE4 MEDIUM', 1.0, European Space Agency, https://doi.org/10.5270/esa-4qt7hnk
