A dataset provided by the European Space Agency

Name 12456
Title Through a Lens, Darkly - New Constraints on the Fundamental Components of the Cosmos
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12456;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-pl3d5x8
Author Postman, Marc
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=12456&mission=hst
Publication
  • 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
  • An excess of small-scale gravitational lenses observed in 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
  • 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
  • JVLA 1.5 GHz Continuum Observation of CLASH Clusters. I. Radio Properties of the BCGs
  • K-CLASH: spatially resolving star-forming galaxies in field and cluster environments at z 0.2-0.6
  • 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
  • M32 Analogs? A Population of Massive Ultra-compact Dwarf and Compact Elliptical Galaxies in Intermediate-redshift Clusters
  • MIFAL: fully automated Multiple-Image Finder ALgorithm for strong-lens modelling - proof of concept
  • Multiband Galaxy Morphologies for CLASH: A Convolutional Neural Network Transferred from CANDELS
  • Multicomponent DHOST analysis in galaxy clusters
  • Reconciling galaxy cluster shapes, measured by theorists versus observers
  • Starbursting brightest cluster galaxy: a Herschel view of the massive cluster MACS J1931.8-2634
  • Star Formation in Intermediate Redshift 0.2 < z < 0.7 Brightest Cluster Galaxies
  • 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
  • Testing the Collisionless Nature of Dark Matter with the Radial Acceleration Relation in Galaxy Clusters
  • Testing the Limits of AGN Feedback and the Onset of Thermal Instability in the Most Rapidly Star-forming 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 Dust and Molecular Gas in the Brightest Cluster Galaxy in MACS 1931.8-2635
  • 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
  • The search for galaxy cluster members with deep learning of panchromatic HST imaging and extensive spectroscopy
  • The VLT-MUSE and ALMA view of the MACS 1931.8-2635 brightest cluster galaxy
  • Ultraviolet Morphology and Unobscured UV Star Formation Rates of CLASH Brightest Cluster 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 2012-04-10T07:04:37Z/2012-06-25T17:56:22Z
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.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 2012-06-27T14:18:47Z
Last Update 2025-01-25
Keywords Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Postman et al., 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-pl3d5x8