A Systematic Search for Gravitationally Lensed Arcs in the Hubble Space Telescope WFPC2 Archive
Combining Lens Distortion and Depletion to Map the Mass Distribution of A1689
Hidden star-formation in the cluster of galaxies Abell 1689
Measuring the matter distribution within z = 0.2 cluster lenses with XMM-Newton
Near-IR search for lensed supernovae behind galaxy clusters. I. Observations and transient detection efficiency
Parametric strong gravitational lensing analysis of Abell 1689
Supernovae in deep Hubble Space Telescope galaxy cluster fields: cluster rates and field counts
The Sizes of Galaxy Halos in Galaxy Cluster Abell 1689
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1996-06-27T07:02:16Z/1997-06-22T18:37:34Z
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, Tyson comma J. Anthony, 1998, 'Direct Measurement of The Mass Distribution in the Rich Cluster Abell 1689', 1.0, European Space Agency, https://doi.org/10.5270/esa-ije568e