A Census of Optically Dark Massive Galaxies in the Early Universe from Magnification by Lensing Galaxy 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
Constraints on the Mass, Concentration, and Nonthermal Pressure Support of Six CLASH Clusters from a Joint Analysis of X-Ray, SZ, and Lensing Data
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
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
Multiband Galaxy Morphologies for CLASH: A Convolutional Neural Network Transferred from CANDELS
Multicomponent DHOST analysis in galaxy clusters
Separating galaxies from the cluster dark matter halo in Abell 611
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
Testing the Collisionless Nature of Dark Matter with the Radial Acceleration Relation in Galaxy Clusters
Testing the Universality of the Fundamental Metallicity Relation at High Redshift Using Low-mass Gravitationally Lensed Galaxies
The Density Profiles of Massive, Relaxed Galaxy Clusters. I. The Total Density Over Three Decades in Radius
The faint end of the red sequence galaxy luminosity function: unveiling surface brightness selection effects with the CLASH clusters
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
Unveiling the Dynamical State of Massive Clusters through the ICL Fraction
Weak lensing shear estimation beyond the shape-noise limit: a machine learning approach
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2012-01-28T02:22:06Z/2012-05-17T11:27:29Z
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 comma Marc, 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-3p7vecc
