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
Calibrating the Planck cluster mass scale with CLASH
CLASH: Complete Lensing Analysis of the Largest Cosmic Lens MACS J0717.5+3745 and Surrounding Structures
CLASH: Joint Analysis of Strong-lensing, Weak-lensing Shear, and Magnification Data for 20 Galaxy Clusters
CLUMP-3D: Three-dimensional Shape and Structure of 20 CLASH Galaxy Clusters from Combined Weak and Strong Lensing
Constraining the Neutral Fraction of Hydrogen in the IGM at Redshift 7.5
Detecting gravitationally lensed Population III galaxies with the Hubble Space Telescope and the James Webb Space Telescope
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
Evolution of the Ultraviolet Upturn at 0.3 < z < 1: Exploring Helium-rich Stellar Populations
Extensive Lensing Survey of Optical and Near-infrared Dark Objects (El Sonido): HST H-faint Galaxies behind 101 Lensing Clusters
HFF-DeepSpace Photometric Catalogs of the 12 Hubble Frontier Fields, Clusters, and Parallels: Photometry, Photometric Redshifts, and Stellar Masses
Hubble Frontier Field free-form mass mapping of the massive multiple-merging cluster MACSJ0717.5+3745
Imaging the Thermal and Kinematic Sunyaev-Zeldovich Effect Signals in a Sample of 10 Massive Galaxy Clusters: Constraints on Internal Velocity Structures and Bulk Velocities
Jellyfish galaxy candidates in MACS J0717.5+3745 and 39 other clusters of the DAFT/FADA and CLASH surveys
Mass and magnification maps for the Hubble Space Telescope Frontier Fields clusters: implications for high-redshift studies
Molecular gas and star formation activity in luminous infrared galaxies in clusters at intermediate redshifts
Multiband Galaxy Morphologies for CLASH: A Convolutional Neural Network Transferred from CANDELS
Searching for filaments and large-scale structure around DAFT/FADA clusters
Spectroscopically Confirmed Lya Emitters from Redshift 5 to 7 behind 10 Galaxy Cluster Lenses
Spitzer Ultra Faint SUrvey Program (SURFS UP). I. An Overview
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 by a node of the cosmic web. The core of MACS J0717.5+3745 at z = 0.55
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 Discovery of Lensed Radio and X-Ray Sources behind the Frontier Fields Cluster MACS J0717.5+3745 with the JVLA and Chandra
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 impact of satellite trails on Hubble Space Telescope observations
The missing light of the Hubble Ultra Deep Field
The most massive galaxies in clusters are already fully grown at z ~ 0.5
The Projected Dark and Baryonic Ellipsoidal Structure of 20 CLASH Galaxy Clusters
The Radial Acceleration Relation in CLASH Galaxy Clusters
Through the Looking GLASS: HST Spectroscopy of Faint Galaxies Lensed by the Frontier Fields Cluster MACSJ0717.5+3745
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
Young Galaxy Candidates in the Hubble Frontier Fields. III. MACS J0717.5+3745
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2011-08-31T21:58:50Z/2011-12-09T00:47:29Z
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 et al., 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-95laptt