Near Infrared Imaging of the Proposed z=2 Cluster Behind CL 0939+4713 (Abell 851)
New Images of the Distant, Rich Cluster CL 0939+4713 with WFPC2
Subaru First-Light Deep Photometry of Galaxies in A 851 Field
Testing the hypothesis of the morphological transformation from field spiral to cluster S0
The Gemini/HST Galaxy Cluster Project: Redshift 0.2-1.0 Cluster Sample, X-Ray Data, and Optical Photometry Catalog
The mass distribution of CL0939+4713 obtained from a `weak lensing analysis of a WFPC2 image.
The morphological segregation of galaxies in clusters. III. The distant cluster CL 0939+4713 (Abell 851).
The Morphology of Distant Cluster Galaxies. II. HST Observations of Four Rich Clusters at z ~= 0.4
The role of E+A and post-starburst galaxies - II. Spectral energy distributions and comparison with observations
Ultraviolet Imaging of the Galaxy Cluster CL 0939+4713 (Abell 851) at z=0.41
XMM observation of the dynamically young galaxy cluster CL 0939+4713
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1994-01-10T12:31:17Z/1994-01-12T14:50:17Z
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, Sparks comma William B., 1994, 'EARLY RELEASE OBSERVATIONS OF DISTANT GALAXIES', 1.0, European Space Agency, https://doi.org/10.5270/esa-r7qndcy