A 7 deg2 survey for galaxy-scale gravitational lenses with the HST imaging archive
Assembly of the Red Sequence in Infrared-selected Galaxy Clusters from the IRAC Shallow Cluster Survey
Harnessing the Hubble Space Telescope Archives: A Catalog of 21,926 Interacting Galaxies
Ha Star Formation Rates of z > 1 Galaxy Clusters in the IRAC Shallow Cluster Survey
Lens Models and Magnification Maps of the Six Hubble Frontier Fields Clusters
Measuring the total infrared light from galaxy clusters at z = 0.5-1.6: connecting stellar populations to dusty star formation
Merger-driven Growth of Intermediate-mass Black Holes: Constraints from Hubble Space Telescope Imaging of Hyper-luminous X-Ray Sources
Molecular gas in two companion cluster galaxies at z = 1.2
PyGFit: A Tool for Extracting PSF Matched Photometry
Star Formation and AGN Activity in Galaxy Clusters from z=1-2: a Multi-Wavelength Analysis Featuring Herschel/PACS
Star Formation in High-redshift Cluster Ellipticals
The Era of Star Formation in Galaxy Clusters
The HST See Change Program. I. Survey Design, Pipeline, and Supernova Discoveries
The impact of satellite trails on Hubble Space Telescope observations
X-ray Emission from Two Infrared-selected Galaxy Clusters at z > 1.4 in the IRAC Shallow Cluster Survey
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR
Temporal Coverage
2009-12-28T03:21:38Z/2011-02-03T04:01:00Z
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, Stanford comma Spencer Adam, 2012, 'Spectroscopy of IR-Selected Galaxy Clusters at 1 < z < 1.5', 1.0, European Space Agency, https://doi.org/10.5270/esa-si878vr