Asteroid Trails in Hubble Space TelescopeWFPC2 Images: First Results
A weak lensing survey in the fields of z~1 luminous radio sources
Cold gas kinematics in an L* spiral Galaxy at z = 0.437: The nature of Damped Lyman-alpha absorbers
Constraints on the Cluster Environments and Hot Spot Magnetic Field Strengths of the Radio Sources 3C 280 and 3C 254
Deep Spectroscopy in the Field of 3C 212
Deep WFPC2 and Ground-Based Imaging of a Complete Sample of 3C Quasars and Galaxies.
Discovery of Optical Emission in the Hot Spots of Three 3CR Quasars: High-Energy Particle Acceleration in Powerful Radio Hot Spots
Discovery of the Galaxy Proximity Effect and Implications for Measurements of the Ionizing Background Radiation at Low Redshifts
Hubble Space Telescope Imaging of Compact Steep-Spectrum Radio Sources
Optical-Radio Alignment in Compact Steep-Spectrum Radio Sources
Probing the Evolution of the Galaxy Interaction/Merger Rate Using Collisional Ring Galaxies
The Aligned z~1 Radio Galaxy 3C 280
The Gaseous Extent of Galaxies and the Origin of Lya Absorption Systems. III. Hubble Space Telescope Imaging of Lya-absorbing Galaxies at z < 1
The Origins of X-Ray Emission from the Hot Spots of FR II Radio Sources
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1994-08-22T02:27:16Z/1995-04-22T05:14:57Z
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, Stockton et al., 1996, 'LUMINOSITIES AND MORPHOLOGIES OF A COMPLETE 3CR SAMPLE OF RADIO GALAXIES AND QUASAR HOSTS', 1.0, European Space Agency, https://doi.org/10.5270/esa-6ntytsi