A Comparison of the Morphological Properties between Local and z ~ 1 Infrared Luminous Galaxies: Are Local and High-z (U)LIRGs Different?
HST/WFPC2 imaging of the QDOT ultraluminous infrared galaxy sample
Quasi-Stellar Objects, Ultraluminous Infrared Galaxies, and Mergers
The Halo Masses of Galaxies to z ~ 3: A Hybrid Observational and Theoretical Approach
The MURALES survey. I. A dual AGN in the radio galaxy 3C 459?
The Relationship between Stellar Light Distributions of Galaxies and Their Formation Histories
The Structural Properties of Isolated Galaxies, Spiral-Spiral Pairs, and Mergers: The Robustness of Galaxy Morphology during Secular Evolution
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1998-11-30T02:52:14Z/1999-06-27T06:57:13Z
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, Rowan-Robinson comma Michael, 2000, 'SNAPSHOT Survey of Ultraluminous Infrared Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-hhmjie2