A multiwavelength strong lensing analysis of baryons and dark matter in the dynamically active cluster AC 114
EROs found behind lensing clusters. II. Empirical properties, classification, and SED modelling based on multi-wavelength observations
High-resolution Near-infrared Imaging of Submillimeter Galaxies
Intense Star Formation and Feedback at High Redshift: Spatially Resolved Properties of the z = 2.6 Submillimeter Galaxy SMM J14011+0252
LoCuSS: first results from strong-lensing analysis of 20 massive galaxy clusters at z = 0.2
Near-IR search for lensed supernovae behind galaxy clusters. I. Observations and transient detection efficiency
Reconciling galaxy cluster shapes, measured by theorists versus observers
Resolved spectroscopy of gravitationally lensed galaxies: global dynamics and star-forming clumps on ~100 pc scales at 1 < z < 4
The cluster galaxy luminosity function at z = 0.3: a recent origin for the faint-end upturn?
The emission line properties of gravitationally lensed 1.5 < z < 5 galaxies
The impact of satellite trails on Hubble Space Telescope observations
Unveiling C II clumps in a lensed star-forming galaxy at z ~ 3.4
z ~ 7-10 Galaxies Behind Lensing Clusters: Contrast with Field Search Results
ZEN2: a narrow J-band search for z ~ 9 Lya emitting galaxies directed towards three lensing clusters
Instrument
ACS, ACS/WFC, NICMOS, NICMOS/NIC3
Temporal Coverage
2004-11-14T02:44:31Z/2005-07-16T10:45:38Z
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, Pello comma Roser, 2006, 'Morphology of z ~ 7-10 galaxies viewed through gravitational telescopes', 1.0, European Space Agency, https://doi.org/10.5270/esa-dnjawtv