Kinematics, turbulence, and star formation of z ~ 1 strongly lensed galaxies seen with MUSE
LoCuSS: connecting the dominance and shape of brightest cluster galaxies with the assembly history of massive clusters
Mass Distributions of Hubble Space Telescope Galaxy Clusters from Gravitational Arcs
Measuring the matter distribution within z = 0.2 cluster lenses with XMM-Newton
New Constraints on the Luminosity Evolution of Spheroidal Galaxies in Distant Clusters
On the evolutionary status of early-type galaxies in clusters at z~ 0.2 - I. The Fundamental Plane
Redshift survey of gravitational arclets in Abell 2390.
Resolving the Stellar Populations in a z=4 Lensed Galaxy
Testing the connection between the X-ray and submillimetre source populations using Chandra
The emission line properties of gravitationally lensed 1.5 < z < 5 galaxies
The Slope of the Cluster Elliptical Red Sequence: A Probe of Cluster Evolution
Two multiple-imaged Z = 4.05 galaxies in the cluster-lens Abell 2390
z ~ 7-10 Galaxies Behind Lensing Clusters: Contrast with Field Search Results
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1994-12-10T04:33:17Z/1995-05-16T06:06:17Z
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, Fort et al., 1996, 'GRAVITATIONAL LENSING STUDIES WITH HST: DARK MATTER AND HIGH REDSHIFT GALAXIES -- CYCLE4 HIGH', 1.0, European Space Agency, https://doi.org/10.5270/esa-ji79e6h