A Census of Optically Dark Massive Galaxies in the Early Universe from Magnification by Lensing Galaxy Clusters
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: Three Strongly Lensed Images of a Candidate z 11 Galaxy
CLUMP-3D: Three-dimensional Shape and Structure of 20 CLASH Galaxy Clusters from Combined Weak and Strong Lensing
Comparison of hydrostatic and lensing cluster mass estimates: A pilot study in MACS J0647.7+7015
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
Geometric Corroboration of the Earliest Lensed Galaxy at z 10.8 from Robust Free-form Modelling
Jellyfish galaxy candidates in MACS J0717.5+3745 and 39 other clusters of the DAFT/FADA and CLASH surveys
JWST Reveals a Possible z 11 Galaxy Merger in Triply Lensed MACS0647-JD
Large size scatter of passively evolving lensed galaxies at z ~ 2 in CLASH.
M32 Analogs? A Population of Massive Ultra-compact Dwarf and Compact Elliptical Galaxies in Intermediate-redshift Clusters
Multiband Galaxy Morphologies for CLASH: A Convolutional Neural Network Transferred from CANDELS
Searching for filaments and large-scale structure around DAFT/FADA clusters
Shapes and alignments of dark matter haloes and their brightest cluster galaxies in 39 strong lensing clusters
Spatially Resolved Stellar Populations of 0.3 < z < 6.0 Galaxies in WHL 0137-08 and MACS 0647+70 Clusters as Revealed by JWST: How Do Galaxies Grow and Quench over Cosmic Time?
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 Projected Dark and Baryonic Ellipsoidal Structure of 20 CLASH Galaxy Clusters
The Radial Acceleration Relation in CLASH Galaxy Clusters
Two Lensed Star Candidates at z 4.8 behind the Galaxy Cluster MACS J0647.7+7015
Weak lensing reveals a tight connection between dark matter halo mass and the distribution of stellar mass in massive galaxies
Weak lensing shear estimation beyond the shape-noise limit: a machine learning approach
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2011-10-05T04:38:55Z/2011-11-29T20:28:48Z
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, 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-jddq1ht
