High-resolution Near-infrared Imaging of Submillimeter Galaxies
Hubble Space Telescope Morphologies of z ~ 2 Dust-obscured Galaxies. II. Bump Sources
Kiloparsec-scale Imaging of the CO(1-0)-traced Cold Molecular Gas Reservoir in a z 3.4 Submillimeter Galaxy
Mapping the Clumpy Structures within Submillimeter Galaxies Using Laser-Guide Star Adaptive Optics Spectroscopy
Observing Cold Gas in Submillimeter Galaxies: Detection of CO (1-->0) Emission in SMM J13120+4242 with the Green Bank Telescope
Optical and near-infrared integral field spectroscopy of the SCUBA galaxy N2 850.4
Submillimeter Galaxies at z ~ 2: Evidence for Major Mergers and Constraints on Lifetimes, IMF, and CO-H2 Conversion Factor
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
The nature of dust-obscured galaxies at z~2
Instrument
ACS, ACS/WFC, NICMOS, NICMOS/NIC2
Temporal Coverage
2003-10-09T11:50:21Z/2004-08-12T14:30:28Z
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, Chapman et al., 2005, 'A near-IR imaging survey of submm galaxies with spectroscopic redshifts', 1.0, European Space Agency, https://doi.org/10.5270/esa-iydhcmh