A dataset provided by the European Space Agency

Name 12067
Title Through a Lens, Darkly - New Constraints on the Fundamental Components of the Cosmos
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12067;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-uv9817w
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=12067&mission=hst
Publication
  • 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
  • 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: Three-dimensional Shape and Structure of 20 CLASH Galaxy Clusters from Combined Weak and Strong Lensing
  • Cluster-galaxy weak lensing
  • Constraining the Neutral Fraction of Hydrogen in the IGM at Redshift 7.5
  • 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
  • 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
  • Large size scatter of passively evolving lensed galaxies at z ~ 2 in CLASH.
  • 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
  • Multiband Galaxy Morphologies for CLASH: A Convolutional Neural Network Transferred from CANDELS
  • Multicomponent DHOST analysis in galaxy clusters
  • Prospects for Extending the Mass-Metallicity Relation to Low Mass at High Redshift: A Case Study at z ~ 1
  • Reconciling galaxy cluster shapes, measured by theorists versus observers
  • Resolved spectroscopy of gravitationally lensed galaxies: global dynamics and star-forming clumps on ~100 pc scales at 1 < z < 4
  • Searching for filaments and large-scale structure around DAFT/FADA clusters
  • Shapes and alignments of dark matter haloes and their brightest cluster galaxies in 39 strong lensing 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
  • Testing the Collisionless Nature of Dark Matter with the Radial Acceleration Relation in Galaxy Clusters
  • 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 Grism Lens-Amplified Survey from Space (GLASS) - XIII. G800L optical spectra from the parallel fields
  • The impact of satellite trails on Hubble Space Telescope observations
  • The missing light of the Hubble Ultra Deep Field
  • The Origin and Evolution of Metallicity Gradients: Probing the Mode of Mass Assembly at z ~= 2
  • The Projected Dark and Baryonic Ellipsoidal Structure of 20 CLASH Galaxy Clusters
  • The Radial Acceleration Relation in CLASH Galaxy Clusters
  • Unveiling C II clumps in a lensed star-forming galaxy at z ~ 3.4
  • 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 2011-09-22T11:44:30Z/2011-12-29T15:52:47Z
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 2011-12-29T18:48:42Z
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., 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-uv9817w