A dataset provided by the European Space Agency

Name 12457
Title Through a Lens, Darkly - New Constraints on the Fundamental Components of the Cosmos
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12457;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-4mlf2es
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=12457&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
  • A magnified compact galaxy at redshift 9.51 with strong nebular emission lines
  • An excess of small-scale gravitational lenses observed in galaxy clusters
  • An Exquisitely Deep View of Quenching Galaxies through the Gravitational Lens: Stellar Population, Morphology, and Ionized Gas
  • A Strong He II l1640 Emitter with an Extremely Blue UV Spectral Slope at z = 8.16: Presence of Population III Stars?
  • 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
  • Dilution of chemical enrichment in galaxies 600 Myr after the Big Bang
  • 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 cores as seen with VLT/MUSE: New strong-lensing analyses of RX J2129.4 + 0009, MS 0451.6 - 0305, and MACS J2129.4 - 0741
  • 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
  • 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
  • Ly a emission strength and stellar properties of faint galaxies from 5 < z < 8.2
  • M32 Analogs? A Population of Massive Ultra-compact Dwarf and Compact Elliptical Galaxies in Intermediate-redshift Clusters
  • Multiband Galaxy Morphologies for CLASH: A Convolutional Neural Network Transferred from CANDELS
  • Multicomponent DHOST analysis in galaxy clusters
  • On the gravitational lensing interpretation of three gravitational wave detections in the mass gap by LIGO and Virgo
  • 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
  • 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 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 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
  • Unveiling the Dynamical State of Massive Clusters through the ICL Fraction
  • Weak lensing shear estimation beyond the shape-noise limit: a machine learning approach
Instrument ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage 2012-04-03T20:26:52Z/2012-07-20T17:28:48Z
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 2012-07-23T12:50:04Z
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, 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-4mlf2es