A Census of Optically Dark Massive Galaxies in the Early Universe from Magnification by Lensing Galaxy Clusters
A GMOS/IFU Study of Jellyfish Galaxies in Massive Clusters
Calibrating the Planck cluster mass scale with CLASH
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
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
JVLA 1.5 GHz Continuum Observation of CLASH Clusters. I. Radio Properties of the BCGs
Lensed Type Ia supernovae as probes of cluster mass models
Lensing Constraints on the Mass Profile Shape and the Splashback Radius of Galaxy Clusters
Lost but not forgotten: intracluster light in galaxy groups and clusters
MIFAL: fully automated Multiple-Image Finder ALgorithm for strong-lens modelling - proof of concept
Multiband Galaxy Morphologies for CLASH: A Convolutional Neural Network Transferred from CANDELS
Multicomponent DHOST analysis in galaxy clusters
Reconciling galaxy cluster shapes, measured by theorists versus observers
Star Formation in Intermediate Redshift 0.2 < z < 0.7 Brightest Cluster Galaxies
Testing the Collisionless Nature of Dark Matter with the Radial Acceleration Relation in Galaxy Clusters
The faint end of the red sequence galaxy luminosity function: unveiling surface brightness selection effects with the CLASH clusters
The growth of brightest cluster galaxies and intracluster light over the past 10 billion years
The impact of satellite trails on Hubble Space Telescope observations
The missing light of the Hubble Ultra Deep Field
The Projected Dark and Baryonic Ellipsoidal Structure of 20 CLASH Galaxy Clusters
The Radial Acceleration Relation in CLASH Galaxy Clusters
Three Gravitationally Lensed Supernovae behind 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
2012-03-26T14:15:04Z/2012-06-17T18:14:30Z
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., 2012, 'Through a Lens, Darkly - New Constraints on the Fundamental Components of the Cosmos', 1.0, European Space Agency, https://doi.org/10.5270/esa-lr2fc05
