A dataset provided by the European Space Agency

Name 13496
Title HST Frontier Fields - Observations of MACSJ0416.1-2403
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=13496;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-wvqtxbg
Author Lotz, Jennifer
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=13496&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
  • A complete census of Herschel-detected infrared sources within the HST Frontier Fields
  • A joint measurement of galaxy luminosity functions and large-scale field densities during the Epoch of Reionization
  • 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
  • ALMA uncovers the C II emission and warm dust continuum in a z = 8.31 Lyman break galaxy
  • A Measurement of the Assembly of Milky Way Analogs at Redshifts 0.5 < z < 2 with Resolved Stellar Mass and Star Formation Rate Profiles
  • An atlas of MUSE observations towards twelve massive lensing clusters
  • An automatic taxonomy of galaxy morphology using unsupervised machine learning
  • An Evaluation of 10 Lensing Models of the Frontier Fields Cluster MACS J0416.1-2403
  • A new estimate of galaxy mass-to-light ratios from flexion lensing statistics
  • A new framework for understanding systematic errors in cluster lens modelling - II. Constraint selection
  • A new framework for understanding systematic errors in cluster lens modelling - I. Selection and treatment of cluster member galaxies
  • A new high-precision strong lensing model of the galaxy cluster MACS J0416.1-2403. Robust characterization of the cluster mass distribution from VLT/MUSE deep observations
  • An extremely metal-poor star complex in the reionization era: Approaching Population III stars with JWST
  • An Increasing Stellar Baryon Fraction in Bright Galaxies at High Redshift
  • A refined mass distribution of the cluster MACS J0416.1-2403 from a new large set of spectroscopic multiply lensed sources
  • A state-of-the-art strong-lensing model of MACS J0416.1-2403 with the largest sample of spectroscopic multiple images
  • A Steep Decline in the Galaxy Space Density beyond Redshift 9 in the CANUCS UV Luminosity Function
  • A Submillimeter Survey of Faint Galaxies behind 10 Strong Lensing Clusters
  • Being KLEVER at cosmic noon: Ionized gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts
  • BUFFALO/Flashlights: Constraints on the abundance of lensed supergiant stars in the Spock galaxy at redshift 1
  • Bulge+disc decomposition of HFF and CANDELS galaxies: UVJ diagrams and stellar mass-size relations of galaxy components at 0.2 <= z <= 1.5
  • Candidate Population III stellar complex at z = 6.629 in the MUSE Deep Lensed Field
  • Characterizing Intracluster Light in the Hubble Frontier Fields
  • Constraints on Photoionization Feedback from Number Counts of Ultra-faint High-redshift Galaxies in the Frontier Fields
  • Constraints on the C II luminosity of a proto-globular cluster at z ~ 6 obtained with ALMA
  • Constraints on warm dark matter from UV luminosity functions of high-z galaxies with Bayesian model comparison
  • Core Mass Estimates in Strong Lensing Galaxy Clusters: A Comparison between Masses Obtained from Detailed Lens Models, Single-halo Lens Models, and Einstein Radii
  • CURLING - I. The influence of point-like image approximation on the outcomes of cluster strong lens modelling
  • Dark matter in galaxy clusters: Parametric strong-lensing approach
  • Dark twilight joined with the light of dawn to unveil the reionization history
  • Directly Observing the Galaxies Likely Responsible for Reionization
  • Dissection of the Collisional and Collisionless Mass Components in a Mini Sample of CLASH and HFF Massive Galaxy Clusters at z 0.4
  • Early Low-mass Galaxies and Star-cluster Candidates at z ~ 6-9 Identified by the Gravitational-lensing Technique and Deep Optical/Near-infrared Imaging
  • Enhanced cluster lensing models with measured galaxy kinematics
  • Evidence for enhanced star formation rates in z ~ 0.35 cluster galaxies undergoing ram pressure stripping
  • Evolution of Stellar-to-Halo Mass Ratio at z = 0 - 7 Identified by Clustering Analysis with the Hubble Legacy Imaging and Early Subaru/Hyper Suprime-Cam Survey Data
  • Evolution of the galaxy stellar mass functions and UV luminosity functions at z = 6-9 in the Hubble Frontier Fields
  • Evolution of the Ultraviolet Upturn at 0.3 < z < 1: Exploring Helium-rich Stellar Populations
  • Exotic image formation in strong gravitational lensing by clusters of galaxies - I. Cross-section
  • Exotic image formation in strong gravitational lensing by clusters of galaxies - II. Uncertainties
  • Exploring Effects on Magnifications due to Line-of-Sight Galaxies in the Hubble Frontier Fields
  • Exploring the physical properties of lensed star-forming clumps at 2 z 6
  • Extending the evolution of the stellar mass-size relation at z <= 2 to low stellar mass galaxies from HFF and CANDELS
  • Extensive Lensing Survey of Optical and Near-infrared Dark Objects (El Sonido): HST H-faint Galaxies behind 101 Lensing Clusters
  • Extremely Small Sizes for Faint z ~ 2-8 Galaxies in the Hubble Frontier Fields: A Key Input for Establishing Their Volume Density and UV Emissivity
  • First constraints on small-scale non-Gaussianity from UV galaxy luminosity functions
  • First Results from the KMOS Lens-Amplified Spectroscopic Survey (KLASS): Kinematics of Lensed Galaxies at Cosmic Noon
  • Flashlights: Properties of Highly Magnified Images Near Cluster Critical Curves in the Presence of Dark Matter Subhalos
  • Free-form lensing implications for the collision of dark matter and gas in the frontier fields cluster MACS J0416.1-2403
  • Frontier Fields Clusters: Chandra and JVLA View of the Pre-merging Cluster MACS J0416.1-2403
  • Frontier Fields: Combining HST, VLT, and Spitzer data to explore the z ~ 8 Universe behind the lensing cluster MACSJ0416.1-2403
  • Frontier Fields: High-redshift Predictions and Early Results
  • Full-data Results of Hubble Frontier Fields: UV Luminosity Functions at z ~ 6-10 and a Consistent Picture of Cosmic Reionization
  • Fundamental Physics with the Hubble Frontier Fields: Constraining Dark Matter Models with the Abundance of Extremely Faint and Distant Galaxies
  • Galaxy clustering measurements out to redshift z ~ 8 from Hubble Legacy Fields
  • Galaxy-galaxy lensing in the outskirts of CLASH clusters: constraints on local shear and testing mass-luminosity scaling relation
  • Galaxy luminosity function pipeline for cosmology and astrophysics
  • Galaxy pre-processing in substructures around z ~ 0.4 galaxy clusters
  • Gaussian Process Reconstruction of Reionization History
  • Gemini Frontier Fields: Wide-field Adaptive Optics Ks-band Imaging of the Galaxy Clusters MACS J0416.1-2403 and Abell 2744
  • Globular clusters in high-redshift dwarf galaxies: a case study from the Local Group
  • HFF-DeepSpace Photometric Catalogs of the 12 Hubble Frontier Fields, Clusters, and Parallels: Photometry, Photometric Redshifts, and Stellar Masses
  • Highly Magnified Stars in Lensing Clusters: New Evidence in a Galaxy Lensed by MACS J0416.1-2403
  • How robustly can we constrain the low-mass end of the z ~ 6-7 stellar mass function? The limits of lensing models and stellar population assumptions in the Hubble Frontier Fields
  • Hubble Frontier Field Clusters and Their Parallel Fields: Photometric and Photometric Redshift Catalogs
  • Hubble Frontier Fields: a high-precision strong-lensing analysis of galaxy cluster MACSJ0416.1-2403 using ~200 multiple images
  • Hubble Frontier Fields: the geometry and dynamics of the massive galaxy cluster merger MACSJ0416.1-2403
  • Image simulations for gravitational lensing with SKYLENS
  • Inferring the intergalactic medium neutral fraction at z 6-8 with low-luminosity Lyman break galaxies
  • Insight from JWST/Near Infrared Camera into galaxy overdensities around bright Lyman-alpha emitters during reionization: implications for ionized bubbles at z 9
  • Intracluster light: a luminous tracer for dark matter in clusters of galaxies
  • Intracluster light at the Frontier - II. The Frontier Fields Clusters
  • Joining Bits and Pieces of Reionization History
  • Joining X-Ray to Lensing: An Accurate Combined Analysis of MACS J0416.1-2403
  • JWSTs PEARLS: Mothra, a new kaiju star at z = 2.091 extremely magnified by MACS0416, and implications for dark matter models
  • Kinematics, turbulence, and star formation of z ~ 1 strongly lensed galaxies seen with MUSE
  • Lens models under the microscope: comparison of Hubble Frontier Field cluster magnification maps
  • Little Blue Dots in the Hubble Space Telescope Frontier Fields: Precursors to Globular Clusters?
  • Locations and Morphologies of Jellyfish Galaxies in A2744 and A370
  • Looking for dark matter trails in colliding galaxy clusters
  • Low-luminosity Galaxies in the Early Universe Have Observed Sizes Similar to Star Cluster Complexes
  • Ly a emission strength and stellar properties of faint galaxies from 5 < z < 8.2
  • MACS J0416.1-2403: Impact of line-of-sight structures on strong gravitational lensing modelling of galaxy clusters
  • Magnification Bias of Distant Galaxies in the Hubble Frontier Fields: Testing Wave Versus Particle Dark Matter Predictions
  • Magnifying the Early Episodes of Star Formation: Super Star Clusters at Cosmological Distances
  • Mapping substructure in the HST Frontier Fields cluster lenses and in cosmological simulations
  • Massive star cluster formation under the microscope at z = 6
  • Mass Profile Decomposition of the Frontier Fields Cluster MACS J0416-2403: Insights on the Dark-matter Inner Profile
  • Model-independent Mass Reconstruction of the Hubble Frontier Field Clusters with MARS Based on Self-consistent Strong-lensing Data
  • Morphologies of ~190,000 Galaxies at z = 0-10 Revealed with HST Legacy Data. II. Evolution of Clumpy Galaxies
  • Must Star-forming Galaxies Rapidly Get Denser before They Quench?
  • New Determinations of the UV Luminosity Functions from z 9 to 2 Show a Remarkable Consistency with Halo Growth and a Constant Star Formation Efficiency
  • New redshift z 9 galaxies in the Hubble Frontier Fields: implications for early evolution of the UV luminosity density
  • New Roads to the Small-scale Universe: Measurements of the Clustering of Matter with the High-redshift UV Galaxy Luminosity Function
  • Observations contradict galaxy size and surface brightness predictions that are based on the expanding universe hypothesis
  • On the Faint End of the Galaxy Luminosity Function in the Epoch of Reionization: Updated Constraints from the HST Frontier Fields
  • Paving the way for the JWST: witnessing globular cluster formation at z > 3
  • Physical properties of more than one thousand brightest cluster galaxies detected in the Canada-France-Hawaii Telescope Legacy Survey
  • Post-starburst Galaxies in the Centers of Intermediate-redshift Clusters
  • Precise Strong Lensing Mass Modeling of Four Hubble Frontier Field Clusters and a Sample of Magnified High-redshift Galaxies
  • Probability of magnification in the HubbleFrontier Fields clusters
  • Probing cosmic dawn: Ages and star formation histories of candidate z >= 9 galaxies
  • Probing the faint-end luminosity function of Lyman-alpha emitters at 3 < z < 7 behind 17 MUSE lensing clusters
  • Prospects for Strongly Lensed Supernovae Behind Hubble Frontier Fields Galaxy Clusters with the James Webb Space Telescope
  • Quantifying substructures in Hubble Frontier Field clusters: comparison with LCDM simulations
  • Rapid Reionization by the Oligarchs: The Case for Massive, UV-bright, Star-forming Galaxies with High Escape Fractions
  • Resolved Stellar Mass Maps of Galaxies in the Hubble Frontier Fields: Evidence for Mass Dependency in Environmental Quenching
  • Revealing the formation histories of the first stars with the cosmic near-infrared background
  • Searches for Population III pair-instability supernovae: Impact of gravitational lensing magnification
  • Search for Ha Emitters at z 7.8: A Constraint on the Ha-based Star Formation Rate Density
  • Searching for Highly Magnified Stars at Cosmological Distances: Discovery of a Redshift 0.94 Blue Supergiant in Archival Images of the Galaxy Cluster MACS J0416.1-2403
  • Setting the scene for BUFFALO: a study of the matter distribution in the HFF galaxy cluster MACS J0416.1-2403 and its parallel field
  • Shapes and alignments of dark matter haloes and their brightest cluster galaxies in 39 strong lensing clusters
  • Shock cooling of a red-supergiant supernova at redshift 3 in lensed images
  • Size-Luminosity Relations and UV Luminosity Functions at z = 6-9 Simultaneously Derived from the Complete Hubble Frontier Fields Data
  • Sizes of Lensed Lower-luminosity z = 4-8 Galaxies from the Hubble Frontier Field Program
  • Spectroscopically Confirmed Lya Emitters from Redshift 5 to 7 behind 10 Galaxy Cluster Lenses
  • Structure and Color Gradients of Ultradiffuse Galaxies in Distant Massive Galaxy Clusters
  • Systematic or signal? How dark matter misalignments can bias strong lensing models of galaxy clusters
  • Systematic versus statistical uncertainties in masses and magnifications of the Hubble Frontier Fields
  • Testing light-traces-mass in Hubble Frontier Fields Cluster MACS-J0416.1-2403
  • The 300 pc Resolution Imaging of a z = 8.31 Galaxy: Turbulent Ionized Gas and Potential Stellar Feedback 600 Million Years after the Big Bang
  • The ALMA-ALPAKA survey. I. High-resolution CO and CI kinematics of star-forming galaxies at z = 0.5-3.5
  • The ALMA Frontier Fields Survey. I. 1.1 mm continuum detections in Abell 2744, MACS J0416.1-2403 and MACS J1149.5+2223
  • The ALMA Frontier Fields Survey. III. 1.1 mm emission line identifications in Abell 2744, MACSJ 0416.1-2403, MACSJ 1149.5+2223, Abell 370, and Abell S1063
  • The ALMA Frontier Fields Survey. II. Multiwavelength Photometric analysis of 1.1 mm continuum sources in Abell 2744, MACSJ0416.1-2403 and MACSJ1149.5+2223
  • The ALMA Frontier Fields Survey. IV. Lensing-corrected 1.1 mm number counts in Abell 2744, MACS J0416.1-2403 and MACS J1149.5+2223
  • The ALMA Frontier Fields Survey. V. ALMA Stacking of Lyman-Break Galaxies in Abell 2744, Abell 370, Abell S1063, MACSJ0416.1-2403 and MACSJ1149.5+2223
  • The ASTRODEEP Frontier Fields catalogues. II. Photometric redshifts and rest frame properties in Abell-2744 and MACS-J0416
  • The BUFFALO HST Survey
  • The Dearth of z ~ 10 Galaxies in All HST Legacy Fields--The Rapid Evolution of the Galaxy Population in the First 500 Myr
  • The Distribution of Ultra-diffuse and Ultra-compact Galaxies in the Frontier Fields
  • The Evolution of the Galaxy Rest-frame Ultraviolet Luminosity Function over the First Two Billion Years
  • The Evolution of the Galaxy Stellar Mass Function at z = 4-8: A Steepening Low-mass-end Slope with Increasing Redshift
  • The evolution of the size-mass relation at z = 1-3 derived from the complete Hubble Frontier Fields data set
  • The extreme faint end of the UV luminosity function at z ~ 6 through gravitational telescopes: a comprehensive assessment of strong lensing uncertainties
  • The Frontier Fields lens modelling comparison project
  • The Frontier Fields: Survey Design and Initial Results
  • The Galaxy Starburst/Main-sequence Bimodality over Five Decades in Stellar Mass at z 3-6.5
  • The Grism Lens-amplified Survey from Space (Glass). IX. The Dual Origin of Low-mass Cluster Galaxies as Revealed by New Structural Analyses
  • The Grism Lens-Amplified Survey from Space (GLASS). VI. Comparing the Mass and Light in MACS J0416.1-2403 Using Frontier Field Imaging and GLASS Spectroscopy
  • 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 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 Kormendy relation of early-type galaxies as a function of wavelength in Abell S1063, MACS J0416.1-2403, and MACS J1149.5+2223
  • The Lensed Lyman-Alpha MUSE Arcs Sample (LLAMAS). I. Characterisation of extended Lyman-alpha halos and spatial offsets
  • The MAGPI Survey: impact of environment on the total internal mass distribution of galaxies in the last 5 Gyr
  • The MillenniumTNG project: the galaxy population at z >= 8
  • The missing light of the Hubble Ultra Deep Field
  • The MUSE Deep Lensed Field on the Hubble Frontier Field MACS J0416. Star-forming complexes at cosmological distances
  • The nongravitational interactions of dark matter in colliding galaxy clusters
  • The orthogonally aligned dark halo of an edge-on lensing galaxy in the Hubble Frontier Fields: a challenge for modified gravity
  • The search for galaxy cluster members with deep learning of panchromatic HST imaging and extensive spectroscopy
  • The shape of galaxy dark matter haloes in massive galaxy clusters: insights from strong gravitational lensing
  • The size-luminosity relation of lensed galaxies at z 6-9 in the Hubble Frontier Fields
  • The Stellar Mass Function in CANDELS and Frontier Fields: The Buildup of Low-mass Passive Galaxies since z 3
  • The Strongest Cluster Lenses: An Analysis of the Relation between Strong Gravitational Lensing Strength and the Physical Properties of Galaxy Clusters
  • The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10
  • The VLA Frontier Fields Survey: Deep, High-resolution Radio Imaging of the MACS Lensing Clusters at 3 and 6 GHz
  • The VLA Frontier Field Survey: A Comparison of the Radio and UV/Optical Size of 0.3 z 3 Star-forming Galaxies
  • The z ~ 6 Luminosity Function Fainter than -15 mag from the Hubble Frontier Fields: The Impact of Magnification Uncertainties
  • 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
  • Thick Disks in the Hubble Space Telescope Frontier Fields
  • Total mass density slopes of early-type galaxies using Jeans dynamical modelling at redshifts 0.29 < z < 0.55
  • Two peculiar fast transients in a strongly lensed host galaxy
  • Ultra-deep K-band Imaging of the Hubble Frontier Fields
  • Ultra-deep K S-band Imaging of the Hubble Frontier Fields
  • Unveiling the Dynamical State of Massive Clusters through the ICL Fraction
  • UV-continuum b slopes of individual z 2-6 clumps and their evolution
  • UV Spectral Slopes at z = 6-9 in the Hubble Frontier Fields: Lack of Evidence for Unusual or Population III Stellar Populations
  • Young Galaxy Candidates in the Hubble Frontier Fields. II. MACS J0416-2403
  • z 2-9 Galaxies Magnified by the Hubble Frontier Field Clusters. II. Luminosity Functions and Constraints on a Faint-end Turnover
  • z 2-9 Galaxies Magnified by the Hubble Frontier Field Clusters. I. Source Selection and Surface Density-Magnification Constraints from >2500 Galaxies
Instrument ACS, ACS/WFC, WFC3, WFC3/IR
Temporal Coverage 2014-01-05T15:34:24Z/2014-09-01T22:10:40Z
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 2014-09-02T00:44:33Z
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, Lotz comma Jennifer, 2014, 'HST Frontier Fields - Observations of MACSJ0416.1-2403', 1.0, European Space Agency, https://doi.org/10.5270/esa-wvqtxbg