A Census of Optically Dark Massive Galaxies in the Early Universe from Magnification by Lensing Galaxy Clusters
ALMA Lensing Cluster Survey: Hubble Space Telescope and Spitzer Photometry of 33 Lensed Fields Built with CHArGE
ALMA Lensing Cluster Survey: Properties of Millimeter Galaxies Hosting X-Ray-detected Active Galactic Nuclei
CLUMP-3D: the lack of non-thermal motions in galaxy cluster cores
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
Galaxy cluster strong lensing cosmography. Cosmological constraints from a sample of regular galaxy clusters
Insight from JWST/Near Infrared Camera into galaxy overdensities around bright Lyman-alpha emitters during reionization: implications for ionized bubbles at z 9
Jellyfish galaxy candidates in MACS J0717.5+3745 and 39 other clusters of the DAFT/FADA and CLASH surveys
K-CLASH: spatially resolving star-forming galaxies in field and cluster environments at z 0.2-0.6
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
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
Strong lensing models of eight CLASH clusters from extensive spectroscopy: Accurate total mass reconstructions in the cores
Systematic search for lensed X-ray sources in the CLASH fields
The ALMA-ALPAKA survey. I. High-resolution CO and CI kinematics of star-forming galaxies at z = 0.5-3.5
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 search for galaxy cluster members with deep learning of panchromatic HST imaging and extensive spectroscopy
Weak lensing shear estimation beyond the shape-noise limit: a machine learning approach
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2013-04-14T13:16:58Z/2013-07-09T13:55:05Z
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., 2013, 'Through a Lens, Darkly - New Constraints on the Fundamental Components of the Cosmos', 1.0, European Space Agency, https://doi.org/10.5270/esa-o8tpdnq
