A Brightest Cluster Galaxy with an Extremely Large Flat Core
A Census of Optically Dark Massive Galaxies in the Early Universe from Magnification by Lensing Galaxy Clusters
A Multiply-Imaged z ~ 6.3 Lyman Alpha Emitter candidate behind Abell 2261
A Radio Relic and a Search for the Central Black Hole in the Abell 2261 Brightest Cluster Galaxy
A stringent upper limit on dark matter self-interaction cross-section from cluster strong lensing
Calibrating the Planck cluster mass scale with CLASH
Chandra Observations of Abell 2261 Brightest Cluster Galaxy, a Candidate Host to a Recoiling Black Hole
CLASH: A Census of Magnified Star-forming Galaxies at z ~ 6-8
CLASH: Joint Analysis of Strong-lensing, Weak-lensing Shear, and Magnification Data for 20 Galaxy Clusters
CLASH: Precise New Constraints on the Mass Profile of the Galaxy Cluster A2261
CLUMP-3D: Testing LCDM with Galaxy Cluster Shapes
CLUMP-3D: the lack of non-thermal motions in galaxy cluster cores
CLUMP-3D: Three-dimensional Shape and Structure of 20 CLASH Galaxy Clusters from Combined Weak and Strong Lensing
Cluster-galaxy weak lensing
Evidence for anisotropic quenching in massive galaxy clusters at z 0.5
Evidence for Ubiquitous High-equivalent-width Nebular Emission in z ~ 7 Galaxies: Toward a Clean Measurement of the Specific Star-formation Rate Using a Sample of Bright, Magnified Galaxies
Extensive Lensing Survey of Optical and Near-infrared Dark Objects (El Sonido): HST H-faint Galaxies behind 101 Lensing Clusters
Jellyfish galaxy candidates in MACS J0717.5+3745 and 39 other clusters of the DAFT/FADA and CLASH surveys
Lensing Constraints on the Mass Profile Shape and the Splashback Radius of Galaxy Clusters
Multiband Galaxy Morphologies for CLASH: A Convolutional Neural Network Transferred from CANDELS
Multicomponent DHOST analysis in galaxy clusters
Physical properties of brightest cluster galaxies up to redshift 1.80 based on HST data
Reconciling galaxy cluster shapes, measured by theorists versus observers
Shapes and alignments of dark matter haloes and their brightest cluster galaxies in 39 strong lensing clusters
Star Formation in Intermediate Redshift 0.2 < z < 0.7 Brightest Cluster Galaxies
Star Formation, Nebulae, and Active Galactic Nuclei in CLASH Brightest Cluster Galaxies. I. Dependence on Core Entropy of Intracluster Medium
Ten billion years of brightest cluster galaxy alignments
Testing the Collisionless Nature of Dark Matter with the Radial Acceleration Relation in Galaxy Clusters
The impact of satellite trails on Hubble Space Telescope observations
The missing light of the Hubble Ultra Deep Field
The Most Massive Galaxies with Large Depleted Cores: Structural Parameter Relations and Black Hole Masses
The Projected Dark and Baryonic Ellipsoidal Structure of 20 CLASH Galaxy Clusters
The Quest for the Largest Depleted Galaxy Core: Supermassive Black Hole Binaries and Stalled Infalling Satellites
The Radial Acceleration Relation in CLASH Galaxy Clusters
Weak lensing shear estimation beyond the shape-noise limit: a machine learning approach
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2011-03-09T13:53:17Z/2011-05-21T04:45:03Z
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, Postman et al., 2011, 'Through a Lens, Darkly - New Constraints on the Fundamental Components of the Cosmos', 1.0, European Space Agency, https://doi.org/10.5270/esa-iru7sxk
