Asteroid Trails in Hubble Space TelescopeWFPC2 Images: First Results
Disentangling star formation and AGN activity in powerful infrared luminous radio galaxies at 1 < z < 4
Evidence for powerful AGN winds at high redshift: dynamics of galactic outflows in radio galaxies during the Quasar Era
HST images and properties of the most distant radio galaxies
HST Images of the Extremely Clumpy Radio Galaxy 1138-262 at z = 2.2
Ha emitters in z~ 2 protoclusters: evidence for faster evolution in dense environments
JWST discovers an AGN ionization cone but only weak radiatively driven feedback in a powerful z 3.5 radio-loud AGN
Kinematically quiet haloes around z~ 2.5 radio galaxies. Keck spectroscopy
Probing the Evolution of the Galaxy Interaction/Merger Rate Using Collisional Ring Galaxies
UV and optical emission lines from the z ~ 2.6 radio galaxy 0828+193: spatially resolved measurements
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1995-08-05T07:19:17Z/1995-11-18T21:07:17Z
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, Miley et al., 1996, 'MORPHOLOGIES OF HIGH--REDSHIFT RADIO GALAXIES', 1.0, European Space Agency, https://doi.org/10.5270/esa-nqjhzsi