A dataset provided by the European Space Agency

Name 12452
Title Through a Lens, Darkly - New Constraints on the Fundamental Components of the Cosmos
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12452;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-s6bkzw2
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=12452&mission=hst
Publication
  • A Census of Optically Dark Massive Galaxies in the Early Universe from Magnification by Lensing Galaxy Clusters
  • ALMA Lensing Cluster Survey: ALMA-Herschel Joint Study of Lensed Dusty Star-forming Galaxies across z 0.5 - 6
  • ALMA Lensing Cluster Survey: A spectral stacking analysis of C II in lensed z ~ 6 galaxies
  • 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 atlas of MUSE observations towards twelve massive lensing clusters
  • 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: Discovery of a Bright z ~= 6.2 Dwarf Galaxy Quadruply Lensed by MACS J0329.6-0211
  • 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: 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
  • Galaxy-galaxy lensing in the outskirts of CLASH clusters: constraints on local shear and testing mass-luminosity scaling relation
  • 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
  • Lensing Constraints on the Mass Profile Shape and the Splashback Radius of Galaxy Clusters
  • Locations and Morphologies of Jellyfish Galaxies in A2744 and A370
  • Lost but not forgotten: intracluster light in galaxy groups and 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
  • On the origin of the intracluster light in massive galaxy clusters
  • Probing the faint-end luminosity function of Lyman-alpha emitters at 3 < z < 7 behind 17 MUSE lensing clusters
  • Shapes and alignments of dark matter haloes and their brightest cluster galaxies in 39 strong lensing clusters
  • 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
  • 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 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 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
  • 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 2011-08-18T04:51:11Z/2011-11-01T19:57:53Z
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 2011-11-01T21:32:29Z
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 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-s6bkzw2