A Hubble and Spitzer Space Telescope Survey for Gravitationally Lensed Galaxies: Further Evidence for a Significant Population of Low-Luminosity Galaxies beyond z = 7
A New Survey for Giant Arcs
A Systematic Search for Gravitationally Lensed Arcs in the Hubble Space Telescope WFPC2 Archive
Diffuse light and building history of the galaxy cluster Abell 2667
Faint end of the z ~ 3-7 luminosity function of Lyman-alpha emitters behind lensing clusters observed with MUSE
Inquiring into the nature of the Abell 2667 brightest cluster galaxy: physical properties from MUSE
Jellyfish: Evidence of Extreme Ram-pressure Stripping in Massive Galaxy Clusters
Source-plane Reconstruction of the Giant Gravitational Arc in A2667: A Candidate Wolf-Rayet Galaxy at z ~ 1
The A2667 Giant Arc at z = 1.03: Evidence for Large-Scale Shocks at High Redshift
The Density Profiles of Massive, Relaxed Galaxy Clusters. I. The Total Density Over Three Decades in Radius
The strong transformation of spiral galaxies infalling into massive clusters at z ~ 0.2
VIMOS-IFU survey of z ~ 0.2 massive galaxy clusters. I. Observations of the strong lensing cluster Abell 2667
z ~ 7-10 Galaxies Behind Lensing Clusters: Contrast with Field Search Results
Instrument
WFPC2, WFPC2/WFC
Temporal Coverage
2001-10-09T10:00:15Z/2001-10-10T23:29:55Z
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, Allen comma Steven W., 2002, 'Chandra and HST Observations of the Brightest Cluster Lenses', 1.0, European Space Agency, https://doi.org/10.5270/esa-0o6y2a9
