A Census of Optically Dark Massive Galaxies in the Early Universe from Magnification by Lensing Galaxy Clusters
A Census of Sub-kiloparsec Resolution Metallicity Gradients in Star-forming Galaxies at Cosmic Noon from HST Slitless Spectroscopy
ALMA Lensing Cluster Survey: ALMA-Herschel Joint Study of Lensed Dusty Star-forming Galaxies across z 0.5 - 6
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
Calibrating the Planck cluster mass scale with CLASH
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
Extensive Lensing Survey of Optical and Near-infrared Dark Objects (El Sonido): HST H-faint Galaxies behind 101 Lensing 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
JVLA 1.5 GHz Continuum Observation of CLASH Clusters. I. Radio Properties of the BCGs
Multiband Galaxy Morphologies for CLASH: A Convolutional Neural Network Transferred from CANDELS
Multicomponent DHOST analysis in galaxy clusters
Spectroscopically Confirmed Lya Emitters from Redshift 5 to 7 behind 10 Galaxy Cluster Lenses
Spectroscopic confirmation of an ultra-faint galaxy at the epoch of reionization
Spitzer Ultra Faint SUrvey Program (SURFS UP). I. An Overview
Star Formation in Intermediate Redshift 0.2 < z < 0.7 Brightest Cluster Galaxies
The ALMA-ALPAKA survey. I. High-resolution CO and CI kinematics of star-forming galaxies at z = 0.5-3.5
The faint end of the red sequence galaxy luminosity function: unveiling surface brightness selection effects with the CLASH clusters
The Grism Lens-Amplified Survey from Space (GLASS). VII. The Diversity of the Distribution of Star Formation in Cluster and Field Galaxies at 0.3 less than or equal to z less than or equal to 0.7
The Hawaii SCUBA-2 Lensing Cluster Survey: Are Low-luminosity Submillimeter Galaxies Detected in the Rest-frame UV?
The impact of satellite trails on Hubble Space Telescope observations
The missing light of the Hubble Ultra Deep Field
Weak lensing shear estimation beyond the shape-noise limit: a machine learning approach
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2012-12-31T17:30:41Z/2013-03-12T14:56:23Z
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, 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-9dxtrwh
