A hyperluminous galaxy at z=2.8 found in a deep submillimetre survey
A New Survey for Giant Arcs
A Redshift z=6.56 Galaxy behind the Cluster Abell 370
A ring galaxy at z=1 lensed by the cluster Abell 370
A Systematic Search for Gravitationally Lensed Arcs in the Hubble Space Telescope WFPC2 Archive
Detecting compact dark matter in galaxy clusters via gravitational microlensing: A2218 and A370
Exploring Cluster Elliptical Galaxies as Cosmological Standard Rods
Faint Submillimeter Galaxies: Hubble Space Telescope Morphologies and Colors
Lensed galaxies in Abell 370. I. Modeling the number counts and redshift distribution of background sources
Mass Distributions of Hubble Space Telescope Galaxy Clusters from Gravitational Arcs
Probing early-type galaxy evolution with the Kormendy relation
Reduction of ringing effects by an improved deconvolution algorithm. Application to A370 CFHT image of gravitational arcs
Supernovae in deep Hubble Space Telescope galaxy cluster fields: cluster rates and field counts
The Counterarc to MS 1512-cB58 and a Companion Galaxy
The z=2.72 galaxy cB58: a gravitational fold arc lensed by the cluster MS1512+36
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1995-12-02T14:03:17Z/1996-03-19T21:53:56Z
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, Saglia comma Roberto P., 1997, 'THE EVOLUTION OF ELLIPTICAL GALAXIES IN DISTANT CLUSTERS', 1.0, European Space Agency, https://doi.org/10.5270/esa-pz80mue