A near-infrared morphological comparison of high-redshift submillimetre and radio galaxies: massive star-forming discs versus relaxed spheroids
Harnessing the Hubble Space Telescope Archives: A Catalog of 21,926 Interacting Galaxies
High-Resolution Millimeter Imaging of Submillimeter Galaxies
High-resolution Near-infrared Imaging of Submillimeter Galaxies
Optical and near-infrared integral field spectroscopy of the SCUBA galaxy N2 850.4
The impact of satellite trails on Hubble Space Telescope observations
The link between submillimetre galaxies and luminous ellipticals: near-infrared IFU spectroscopy of submillimetre galaxies
Instrument
ACS, ACS/WFC, WFPC2, WFPC2/PC
Temporal Coverage
2003-09-03T11:04:15Z/2004-07-27T19:12:51Z
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, Almaini et al., 2005, 'A morphological study of EROs and sub-mm sources in a unique deep field', 1.0, European Space Agency, https://doi.org/10.5270/esa-3bfx9y1