A free-form lensing grid solution for A1689 with new multiple images
A Highly Magnified Supernova at z = 1.703 behind the Massive Galaxy Cluster A1689
ALMA Reveals Extended Cool Gas and Hot Ionized Outflows in a Typical Star-forming Galaxy at Z = 7.13
An excursion into the core of the cluster lens Abell 1689
SMA Observations on Faint Submillimeter Galaxies with S 850 < 2 mJy: Ultra Dusty Low-luminosity Galaxies at High Redshift
Specific Frequencies and Luminosity Profiles of Cluster Galaxies and Intracluster Light in Abell 1689
The Detection of O III l4363 in a Lensed, Dwarf Galaxy at z = 2.59: Testing Metallicity Indicators and Scaling Relations at High Redshift and Low Mass
The Direct-method Oxygen Abundance of Typical Dwarf Galaxies at Cosmic High Noon
The Gemini/HST Galaxy Cluster Project: Redshift 0.2-1.0 Cluster Sample, X-Ray Data, and Optical Photometry Catalog
The Hawaii SCUBA-2 Lensing Cluster Survey: Are Low-luminosity Submillimeter Galaxies Detected in the Rest-frame UV?
The impact of satellite trails on Hubble Space Telescope observations
The Most Ancient Spiral Galaxy: A 2.6-Gyr-old Disk with a Tranquil Velocity Field
The origin of the observed Ly a EW distribution of dwarf galaxies at z 2
The Rich Globular Cluster System of Abell 1689 and the Radial Dependence of the Globular Cluster Formation Efficiency
Three-dimensional Multi-probe Analysis of the Galaxy Cluster A1689
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2010-05-29T15:38:37Z/2010-07-08T21:26:15Z
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, Blakeslee comma John P., 2011, 'The Extreme Globular Cluster System of Abell 1689: The Ultimate Test of Universal Formation Efficiency', 1.0, European Space Agency, https://doi.org/10.5270/esa-upoglr5