A 30 kpc Chain of Beads on a String Star Formation between Two Merging Early Type Galaxies in the Core of a Strong-lensing Galaxy Cluster
A Comparison of Rest-frame Ultraviolet and Optical Emission-line Diagnostics in the Lensed Galaxy SDSS J1723+3411 at Redshift z = 1.3293
An Atlas of Color-selected Quiescent Galaxies at z > 3 in Public JWST Fields
A population of luminous accreting black holes with hidden mergers
Beads-on-a-string Star Formation Tied to One of the Most Powerful Active Galactic Nucleus Outbursts Observed in a Cool-core Galaxy Cluster
Constraints on the Lyman Continuum Escape from Low-mass Lensed Galaxies at 1.3 <= z <= 3.0
Discovery of a Lensed Ultrabright Submillimeter Galaxy at z = 2.0439
LBT/ARGOS adaptive optics observations of z ~ 2 lensed galaxies
REQUIEM-2D Methodology: Spatially Resolved Stellar Populations of Massive Lensed Quiescent Galaxies from Hubble Space Telescope 2D Grism Spectroscopy
Resolving Clumpy versus Extended Lya in Strongly Lensed, High-redshift Lya Emitters
Resolving Quiescent Galaxies at z 2. I. Search for Gravitationally Lensed Sources and Characterization of Their Structure, Stellar Populations, and Line Emission
Resolving the H I in damped Lyman a systems that power star formation
Spatial Variation in Strong Line Ratios and Physical Conditions in Two Strongly Lensed Galaxies at z 1.4
Star Formation at z = 2.481 in the Lensed Galaxy SDSS J1110+6459. II. What is Missed at the Normal Resolution of the Hubble Space Telescope?
Star Formation at z = 2.481 in the Lensed Galaxy SDSS J1110 = 6459. I. Lens Modeling and Source Reconstruction
Star Formation at z = 2.481 in the Lensed Galaxy SDSS J1110+6459: Star Formation Down to 30 pc Scales
Star Formation in Intermediate Redshift 0.2 < z < 0.7 Brightest Cluster Galaxies
Strong Lens Models for 37 Clusters of Galaxies from the SDSS Giant Arcs Survey
The Cheshire Cat Gravitational Lens: The Formation of a Massive Fossil Group
The impact of satellite trails on Hubble Space Telescope observations
The Magellan Evolution of Galaxies Spectroscopic and Ultraviolet Reference Atlas (MegaSaura). I. The Sample and the Spectra
The Mass Distribution of the Strong Lensing Cluster SDSS J1531+3414
The Physical Conditions, Metallicity and Metal Abundance Ratios in a Highly Magnified Galaxy at z = 3.6252
Ultra-bright CO and C I Emission in a Lensed z = 2.04 Submillimeter Galaxy with Extreme Molecular Gas Properties
Instrument
WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2012-11-29T00:32:03Z/2014-03-13T02:59:37Z
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, Gladders et al., 2014, 'Resolving the Star Formation in Distant Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-yhk9ca4