Black Hole Mass Estimates Based on C IV are Consistent with Those Based on the Balmer Lines
Constraining VLBI-optical offsets in high redshift galaxies using strong gravitational lensing
Milliarcsecond X-Ray Astrometry to Resolve Inner Regions of AGN at z > 1 Using Gravitational Lensing
Near-Infrared Adaptive Optics Imaging of High-Redshift Quasars
Probing the Coevolution of Supermassive Black Holes and Galaxies Using Gravitationally Lensed Quasar Hosts
Probing the cool interstellar and circumgalactic gas of three massive lensing galaxies at z = 0.4-0.7
Self-similar Models for the Mass Profiles of Early-Type Lens Galaxies
SHARP - IV. An apparent flux-ratio anomaly resolved by the edge-on disc in B0712+472
The Evolution and Structure of Early-Type Field Galaxies: A Combined Statistical Analysis of Gravitational Lenses
The Evolution of a Mass-selected Sample of Early-Type Field Galaxies
The X-Ray Properties of Moderate-Redshift Galaxy Groups Selected by Association with Gravitational Lenses
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
2001-05-28T11:52:14Z/2002-10-08T00:54:57Z
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, Impey comma Chris D., 2003, 'Host Galaxies of Gravitationally Lensed Quasars', 1.0, European Space Agency, https://doi.org/10.5270/esa-1t8hdgn