A dataset provided by the European Space Agency

Name 12065
Title Through a Lens, Darkly - New Constraints on the Fundamental Components of the Cosmos
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12065;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-mqwakf9
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=12065&mission=hst
Publication
  • A Census of Optically Dark Massive Galaxies in the Early Universe from Magnification by Lensing Galaxy Clusters
  • A Census of Star-forming Galaxies in the Z ~ 9-10 Universe based on HST+Spitzer Observations over 19 Clash Clusters: Three Candidate Z ~ 9-10 Galaxies and Improved Constraints on the Star Formation Rate Density at Z ~ 9.2
  • A detection of wobbling brightest cluster galaxies within massive galaxy clusters
  • A free-form prediction for the reappearance of supernova Refsdal in the Hubble Frontier Fields cluster MACSJ1149.5+2223
  • 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: Full Spectral Energy Distribution Analysis of z ~ 0.5-6 Lensed Galaxies Detected with millimeter Observations
  • 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 Search for Population III Galaxies in CLASH. I. Singly-imaged Candidates at High Redshift
  • Being KLEVER at cosmic noon: Ionized gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts
  • Calibrating the Planck cluster mass scale with CLASH
  • CLASH: accurate photometric redshifts with 14 HST bands in massive galaxy cluster cores
  • CLASH: A Census of Magnified Star-forming Galaxies at z ~ 6-8
  • CLASH: Extreme Emission-line Galaxies and Their Implication on Selection of High-redshift Galaxies
  • CLASH: Joint Analysis of Strong-lensing, Weak-lensing Shear, and Magnification Data for 20 Galaxy Clusters
  • CLASH: Mass Distribution in and around MACS J1206.2-0847 from a Full Cluster Lensing Analysis
  • CLASH: The Concentration-Mass Relation of Galaxy Clusters
  • CLASH-VLT: A VIMOS Large Programme to Map the Dark Matter Mass Distribution in Galaxy Clusters and Probe Distant Lensed Galaxies
  • CLASH-VLT: Strangulation of cluster galaxies in MACS J0416.1-2403 as seen from their chemical enrichment
  • CLASH-X: A Comparison of Lensing and X-Ray Techniques for Measuring the Mass Profiles of 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 lensing and multi-probe analysis of MACS J1206.2-0847, a remarkably regular cluster
  • CLUMP-3D: Three-dimensional Shape and Structure of 20 CLASH Galaxy Clusters from Combined Weak and Strong Lensing
  • Cluster-cluster lensing and the case of Abell 383
  • Cluster-galaxy weak lensing
  • Coevolution of brightest cluster galaxies and intracluster light using CLASH
  • Constraining the galaxy mass content in the core of A383 using velocity dispersion measurements for individual cluster members
  • Constraints on the Lyman Continuum Escape from Low-mass Lensed Galaxies at 1.3 <= z <= 3.0
  • Constraints on the Mass, Concentration, and Nonthermal Pressure Support of Six CLASH Clusters from a Joint Analysis of X-Ray, SZ, and Lensing Data
  • Core Mass Estimates in Strong Lensing Galaxy Clusters: A Comparison between Masses Obtained from Detailed Lens Models, Single-halo Lens Models, and Einstein Radii
  • Crowded Field Galaxy Photometry: Precision Colors in the CLASH Clusters
  • Dark matter fraction of low-mass cluster members probed by galaxy-scale strong lensing
  • Discovery of a New Fundamental Plane Dictating Galaxy Cluster Evolution from Gravitational Lensing
  • Discovery of a possibly old galaxy at z= 6.027, multiply imaged by the massive cluster Abell 383
  • Early Science with the Large Millimeter Telescope: Detection of Dust Emission in Multiple Images of a Normal Galaxy at z > 4 Lensed by a Frontier Fields Cluster
  • Evidence for anisotropic quenching in massive galaxy clusters at z 0.5
  • Evidence for enhanced star formation rates in z ~ 0.35 cluster galaxies undergoing ram pressure stripping
  • 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
  • First Results from the KMOS Lens-Amplified Spectroscopic Survey (KLASS): Kinematics of Lensed Galaxies at Cosmic Noon
  • High-resolution Spectroscopy of a Young, Low-metallicity Optically Thin L = 0.02L* Star-forming Galaxy at z = 3.12
  • Hubble Space Telescope Combined Strong and Weak Lensing Analysis of the CLASH Sample: Mass and Magnification Models and Systematic Uncertainties
  • Inference of the cosmic rest-frame from supernovae Ia
  • 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
  • Jellyfish: the origin and distribution of extreme ram-pressure stripping events in massive galaxy clusters
  • JVLA 1.5 GHz Continuum Observation of CLASH Clusters. I. Radio Properties of the BCGs
  • LBT/LUCI Spectroscopic Observations of z7 Galaxies
  • Lensed Type Ia supernovae as probes of cluster mass models
  • Lensing Constraints on the Mass Profile Shape and the Splashback Radius of Galaxy Clusters
  • Lens Models and Magnification Maps of the Six Hubble Frontier Fields Clusters
  • Link between brightest cluster galaxy properties and large scale extensions of 38 DAFT/FADA and CLASH clusters in the redshift range 0.2 < z < 0.9
  • Measurement of the Relativistic Sunyaev-Zeldovich Correction in RX J1347.5-1145
  • Metal Deficiency in Two Massive Dead Galaxies at z ~ 2
  • Model-independent characterisation of strong gravitational lenses
  • Molecular gas in CLASH brightest cluster galaxies at z ~ 0.2 - 0.9
  • Morphological evolution of cluster red sequence galaxies in the past 9 Gyr
  • Multiband Galaxy Morphologies for CLASH: A Convolutional Neural Network Transferred from CANDELS
  • Multicomponent DHOST analysis in galaxy clusters
  • Observable tests of self-interacting dark matter in galaxy clusters: BCG wobbles in a constant density core
  • Observable tests of self-interacting dark matter in galaxy clusters: cosmological simulations with SIDM and baryons
  • Observational constraints on the deceleration parameter in a tilted universe
  • On the Origin of the Scatter in the Red Sequence: An Analysis of Four CLASH Clusters
  • On the Stellar Masses of Giant Clumps in Distant Star-forming Galaxies
  • Post-starburst Galaxies in the Centers of Intermediate-redshift Clusters
  • Primordial alignment of elliptical galaxies in intermediate redshift clusters
  • Probing Dark Matter Subhalos in Galaxy Clusters Using Highly Magnified Stars
  • Probing vainsthein-screening gravity with galaxy clusters using internal kinematics and strong and weak lensing
  • Progenitor Evolution and Dark Energy Time Variation from CLASH SNe Ia
  • Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.2 z 0.9
  • Reconciling galaxy cluster shapes, measured by theorists versus observers
  • Resolving Quiescent Galaxies at z 2. I. Search for Gravitationally Lensed Sources and Characterization of Their Structure, Stellar Populations, and Line Emission
  • Revised Lens Model for the Multiply Imaged Lensed Supernova, SN Refsdal in MACS J1149+2223
  • Shapes and alignments of dark matter haloes and their brightest cluster galaxies in 39 strong lensing clusters
  • Spitzer UltRa Faint SUrvey Program (SURFS UP). II. IRAC-detected Lyman-Break Galaxies at 6 z 10 behind Strong-lensing Clusters
  • Star Formation Activity in CLASH Brightest Cluster Galaxies
  • Star Formation in Intermediate Redshift 0.2 < z < 0.7 Brightest Cluster Galaxies
  • Submillimeter Observations of CLASH 2882 and the Evolution of Dust in this Galaxy
  • SuperBoRG: Exploration of Point Sources at z ~ 8 in HST Parallel Fields
  • SuperBoRG: Search for the Brightest of Reionizing Galaxies and Quasars in HST Parallel Imaging Data
  • Ten billion years of brightest cluster galaxy alignments
  • 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 ALMA Reionization Era Bright Emission Line Survey: The molecular gas content of galaxies at z 7
  • The ASTRODEEP Frontier Fields catalogues. I. Multiwavelength photometry of Abell-2744 and MACS-J0416
  • The Cluster Lensing and Supernova Survey with Hubble: An Overview
  • The Cluster Lensing and Supernova Survey with Hubble (CLASH): Strong-lensing Analysis of A383 from 16-band HST/WFC3/ACS Imaging
  • The cosmic timeline implied by the JWST reionization crisis
  • The Density Profiles of Massive, Relaxed Galaxy Clusters. I. The Total Density Over Three Decades in Radius
  • The Detection and Statistics of Giant Arcs behind CLASH Clusters
  • The Evolution of Star formation Activity in Cluster Galaxies over 0.15 < z < 1.5
  • 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). V. Extent and Spatial Distribution of Star Formation in z ~ 0.5 Cluster Galaxies
  • The Grism Lens-amplified Survey from Space (GLASS). XII. Spatially Resolved Galaxy Star Formation Histories and True Evolutionary Paths at z > 1
  • The Hawaii SCUBA-2 Lensing Cluster Survey: Radio-detected Submillimeter Galaxies in the HST Frontier Fields
  • The impact of satellite trails on Hubble Space Telescope observations
  • The missing light of the Hubble Ultra Deep Field
  • The Morphologies and Alignments of Gas, Mass, and the Central Galaxies of CLASH Clusters of Galaxies
  • The Physical Properties of Luminous z 8 Galaxies and Implications for the Cosmic Star Formation Rate Density from 0.35 deg2 of (Pure-)Parallel HST Observations
  • The Projected Dark and Baryonic Ellipsoidal Structure of 20 CLASH Galaxy Clusters
  • The Radial Acceleration Relation in CLASH Galaxy Clusters
  • The Rate of Core Collapse Supernovae to Redshift 2.5 from the CANDELS and CLASH Supernova Surveys
  • The Relationship Between Brightest Cluster Galaxy Star Formation and the Intracluster Medium in CLASH
  • The search for galaxy cluster members with deep learning of panchromatic HST imaging and extensive spectroscopy
  • The Three Hundred project: dissecting the Fundamental Plane of galaxy clusters up to z = 1
  • The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10
  • The UV luminosity functions of bright z > 8 galaxies: determination from 0.41 deg2 of HST observations along 300 independent sightlines
  • The z = 9-10 galaxy population in the Hubble Frontier Fields and CLASH surveys: the z = 9 luminosity function and further evidence for a smooth decline in ultraviolet luminosity density at z>= 8
  • Three Gravitationally Lensed Supernovae behind CLASH Galaxy Clusters
  • Triaxiality, principal axis orientation and non-thermal pressure in Abell 383
  • Type-Ia Supernova Rates to Redshift 2.4 from CLASH: The Cluster Lensing And Supernova Survey with Hubble
  • Unveiling the Dynamical State of Massive Clusters through the ICL Fraction
  • Weak lensing shear estimation beyond the shape-noise limit: a machine learning approach
  • z 2-9 Galaxies Magnified by the Hubble Frontier Field Clusters. II. Luminosity Functions and Constraints on a Faint-end Turnover
  • LCDM not dead yet: massive high-z Balmer break galaxies are less common than previously reported
Instrument ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage 2010-11-18T21:43:23Z/2011-03-01T13:26:26Z
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 2011-03-01T21:03:45Z
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-mqwakf9