ALMA imaging of SDP.81 - II. A pixelated reconstruction of the CO emission lines
ALMA Observations of the Gravitational Lens SDP.9
Chandra and ALMA observations of the nuclear activity in two strongly lensed star-forming galaxies
Gravitational Lens Models Based on Submillimeter Array Imaging of Herschel-selected Strongly Lensed Sub-millimeter Galaxies at z > 1.5
Herschel *-ATLAS: deep HST/WFC3 imaging of strongly lensed submillimetre galaxies
Herschel-ATLAS: modelling the first strong gravitational lenses
High Dense Gas Fraction in Intensely Star-forming Dusty Galaxies
High-resolution ALMA observations of SDP.81. II. Molecular clump properties of a lensed submillimeter galaxy at z = 3.042
High-resolution ALMA observations of SDP.81. I. The innermost mass profile of the lensing elliptical galaxy probed by 30 milli-arcsecond images
Probing general relativity in galactic scales at z 0.3
Revealing the complex nature of the strong gravitationally lensed system H-ATLAS J090311.6+003906 using ALMA
The far-infrared/radio correlation for a sample of strongly lensed dusty star-forming galaxies detected by Herschel
The Innermost Mass Distribution of the Gravitational Lens SDP.81 from ALMA Observations
The missing light of the Hubble Ultra Deep Field
The Second-generation z (Redshift) and Early Universe Spectrometer. I. First-light Observation of a Highly Lensed Local-ulirg Analog at High-z
Instrument
WFC3, WFC3/IR
Temporal Coverage
2011-04-04T09:10:28Z/2011-04-14T11:05:22Z
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, Negrello comma Mattia, 2012, 'High resolution Near-Infrared imaging of the first sub-mm selected gravitational lens candidates in the Herschel ATLAS', 1.0, European Space Agency, https://doi.org/10.5270/esa-y5ugwu6
