A dataset provided by the European Space Agency

Name 12062
Title Galaxy Assembly and the Evolution of Structure over the First Third of Cosmic Time - III
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12062;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-p0c4gr8
Author Faber, Sandra M.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=12062&mission=hst
Publication
  • 3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts, and Stellar Masses
  • A 7 deg2 survey for galaxy-scale gravitational lenses with the HST imaging archive
  • A Calibration of NICMOS Camera 2 for Low Count Rates
  • A CANDELS-3D-HST synergy: Resolved Star Formation Patterns at 0.7 < z < 1.5
  • Accurate PSF-matched photometry and photometric redshifts for the extreme deep field with the Chebyshev-Fourier functions
  • A Critical Assessment of Photometric Redshift Methods: A CANDELS Investigation
  • Active Galactic Nuclei Selection and Demographics: A New Age with JWST/MIRI
  • Active Galactic Nucleus Feedback at z ~ 2 and the Mutual Evolution of Active and Inactive Galaxies
  • A JWST/NIRSpec First Census of Broad-line AGNs at z = 4-7: Detection of 10 Faint AGNs with M BH 106-108 M and Their Host Galaxy Properties
  • ALMA reveals a warm and compact starburst around a heavily obscured supermassive black hole at z = 4.75
  • A multiwavelength study of a massive, active galaxy at z ~ 2: coupling the kinematics of the ionized and molecular gas
  • A Multiwavelength Study of Tadpole Galaxies in the Hubble Ultra Deep Field
  • Analysis of the SFR-M* plane at z < 3: single fitting versus multi-Gaussian decomposition
  • A new derivation of the Hubble constant from g-ray attenuation using improved optical depths for the Fermi and CTA era
  • A new multifield determination of the galaxy luminosity function at z = 7-9 incorporating the 2012 Hubble Ultra-Deep Field imaging
  • A quantitative assessment of completeness correction methods and public release of a versatile simulation code
  • A Rest-frame Optical View on z ~ 4 Galaxies. I. Color and Age Distributions from Deep IRAC Photometry of the IUDF10 and GOODS Surveys
  • A Simulation-driven Deep Learning Approach for Separating Mergers and Star-forming Galaxies: The Formation Histories of Clumpy Galaxies in All of the CANDELS Fields
  • A Spatially Resolved Study of Cold Dust, Molecular Gas, H II Regions, and Stars in the z = 2.12 Submillimeter Galaxy ALESS67.1
  • A Submillimeter Perspective on the GOODS Fields (SUPER GOODS). III. A Large Sample of ALMA Sources in the GOODS-S
  • A3COSMOS and A3GOODSS: Continuum source catalogues and multi-band number counts
  • A surprising abundance of massive quiescent galaxies at 3 < z < 5 in the first data from JWST CEERS
  • Axion Decay and Anisotropy of Near-IR Extragalactic Background Light
  • Being KLEVER at cosmic noon: Ionized gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts
  • Brown Dwarf Candidates in the JADES and CEERS Extragalactic Surveys
  • Bulge+disc decomposition of HFF and CANDELS galaxies: UVJ diagrams and stellar mass-size relations of galaxy components at 0.2 <= z <= 1.5
  • Bulge Growth and Quenching since z = 2.5 in CANDELS/3D-HST
  • CANDELS Multiwavelength Catalogs: Source Identification and Photometry in the CANDELS UKIDSS Ultra-deep Survey Field
  • CANDELS: The Contribution of the Observed Galaxy Population to Cosmic Reionization
  • CANDELS: The Correlation between Galaxy Morphology and Star Formation Activity at z ~ 2
  • CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey
  • CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey--The Hubble Space Telescope Observations, Imaging Data Products, and Mosaics
  • CANDELS: The Progenitors of Compact Quiescent Galaxies at z ~ 2
  • Combining ALMA with HST and VLT to Find the Counterparts of Submillimetre Galaxies
  • Compact star-forming galaxies preferentially quenched to become PSBs in z < 1 clusters
  • Conditions for galaxy quenching at 0.5 < z < 2.5 from CANDELS: compact cores and environment
  • CONGRUENTS (COsmic-ray, Neutrino, Gamma-ray and Radio Non-Thermal Spectra) - II. Population-level correlations between galactic infrared, radio, and g-ray emission
  • Constraining constant and tomographic coupled dark energy with low-redshift and high-redshift probes
  • Constraining the bright-end of the UV luminosity function for z 7-9 galaxies: results from CANDELS/GOODS-South
  • Constraints on the star-formation rate of z ~ 3 LBGs with measured metallicity in the CANDELS GOODS-South field
  • Deblending Galaxies with Generative Adversarial Networks
  • Definitive upper bound on the negligible contribution of quasars to cosmic reionization
  • Delving deep: A population of extremely dusty dwarfs observed by JWST
  • Density perturbations for running vacuum: a successful approach to structure formation and to the s8-tension
  • Determining Cosmological-model-independent H 0 with Gravitationally Lensed Supernova Refsdal
  • Distinguishing Mergers and Disks in High-redshift Observations of Galaxy Kinematics
  • Dust Attenuation, Bulge Formation, and Inside-out Quenching of Star Formation in Star-forming Main Sequence Galaxies at z ~ 2
  • Dust attenuation, dust content, and geometry of star-forming galaxies
  • Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang
  • Evidence for two modes of black hole accretion in massive galaxies at z~2
  • 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 Sizes of Galaxies over 7 < z < 12 Revealed by the 2012 Hubble Ultra Deep Field Campaign
  • Exploring the Gas-phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
  • Extended Ha over compact far-infrared continuum in dusty submillimeter galaxies. Insights into dust distributions and star-formation rates at z ~ 2
  • Extremely Low Molecular Gas Content in a Compact, Quiescent Galaxy at z = 1.522
  • Extremely Red Galaxies at z = 5-9 with MIRI and NIRSpec: Dusty Galaxies or Obscured Active Galactic Nuclei?
  • Galaxy build-up in the first 1.5 Gyr of cosmic history: insights from the stellar mass function at z 4-9 from JWST NIRCam observations
  • Galaxy Quenching at the High Redshift Frontier: A Fundamental Test of Cosmological Models in the Early Universe with JWST-CEERS
  • Galaxy Stellar Mass Functions from ZFOURGE/CANDELS: An Excess of Low-mass Galaxies since z = 2 and the Rapid Buildup of Quiescent Galaxies
  • Gamma-ray bursts, quasars, baryonic acoustic oscillations, and supernovae Ia: new statistical insights and cosmological constraints
  • GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies
  • HALO7D II: The Halo Velocity Ellipsoid and Velocity Anisotropy with Distant Main-sequence Stars
  • Harnessing the Hubble Space Telescope Archives: A Catalog of 21,926 Interacting Galaxies
  • High Equivalent Width of Ha+N II Emission in z 8 Lyman-break Galaxies from IRAC 5.8 mm Observations: Evidence for Efficient Lyman-continuum Photon Production in the Epoch of Reionization
  • How Robust are the Size Measurements of High-redshift Compact Galaxies?
  • Identification and characterization of six spectroscopically confirmed massive protostructures at 2.5 < z < 4.5
  • Identifying Lya emitter candidates with Random Forest: Learning from galaxies in the CANDELS survey
  • Inference of the cosmic rest-frame from supernovae Ia
  • Investigating the Effect of Galaxy Interactions on Star Formation at 0.5 < z < 3.0
  • Ionized gas kinematics and chemical abundances of low-mass star-forming galaxies at z ~ 3
  • JKCS 041: a Coma cluster progenitor at z = 1.803
  • JWST PRIMER: a new multifield determination of the evolving galaxy UV luminosity function at redshifts z 9 - 15
  • JWST Sneaks a Peek at the Stellar Morphology of z 2 Submillimeter Galaxies: Bulge Formation at Cosmic Noon
  • Keck Spectroscopy of 3 < z < 7 Faint Lyman Break Galaxies: The Importance of Nebular Emission in Understanding the Specific Star Formation Rate and Stellar Mass Density
  • Keck Spectroscopy of Faint 3 < z < 7 Lyman Break Galaxies. III. The Mean Ultraviolet Spectrum at z ~= 4
  • Late-time acceleration due to a generic modification of gravity and the Hubble tension
  • Linking galaxy structural properties and star formation activity to black hole activity with IllustrisTNG
  • Listening to galaxies tuning at z ~ 2.5-3.0: The first strikes of the Hubble fork
  • Luminous and High Stellar Mass Candidate Galaxies at z 8 Discovered in the Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey
  • Mass assembly history of dark matter haloes in the light of H0 tension
  • MCSED: A Flexible Spectral Energy Distribution Fitting Code and Its Application to z ~ 2 Emission-line Galaxies
  • Metallicity evolution, metallicity gradients, and gas fractions at z ~ 3.4
  • MIDIS: JWST NIRCam and MIRI Unveil the Stellar Population Properties of Lya Emitters and Lyman-break Galaxies at z 3-7
  • MIDIS: Strong (Hb+O III) and Ha Emitters at Redshift z 7-8 Unveiled with JWST NIRCam and MIRI Imaging in the Hubble eXtreme Deep Field
  • Minor Merger Growth in Action: JWST Detects Faint Blue Companions around Massive Quiescent Galaxies at 0.5 <= z <= 3.0
  • Model-independent test of the running Hubble constant from the Type Ia supernovae and the Hubble parameter data
  • Moderate-luminosity Growing Black Holes from 1.25 < z < 2.7: Varied Accretion in Disk-dominated Hosts
  • Molecular gas on large circumgalactic scales at z = 3.47
  • Morphologies of ~190,000 Galaxies at z = 0-10 Revealed with HST Legacy Data. III. Continuum Profile and Size Evolution of Lya Emitters
  • Morphologies of z ~ 0.7 AGN host galaxies in CANDELS: no trend of merger incidence with AGN luminosity
  • Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology
  • Nature versus nurture: what regulates star formation in satellite galaxies?
  • Near-IR Weak-lensing (NIRWL) Measurements in the CANDELS Fields. I. Point-spread Function Modeling and Systematics
  • New empirical constraints on the cosmological evolution of gas and stars in galaxies
  • New technique to select recent fast-quenching galaxies at z 2 using the optical colours
  • NIHAO-UHD: the properties of MW-like stellar discs in high-resolution cosmological simulations
  • Nonparametric reconstruction of interaction in the cosmic dark sector
  • Obscured AGN enhancement in galaxy pairs at cosmic noon: evidence from a probabilistic treatment of photometric redshifts
  • Observational constraints on the deceleration parameter in a tilted universe
  • Observational Constraints on the Merger History of Galaxies since z 6: Probabilistic Galaxy Pair Counts in the CANDELS Fields
  • Observational constraints on the tilted flat-XCDM and the untilted nonflat XCDM dynamical dark energy inflation parameterizations
  • Observations of Environmental Quenching in Groups in the 11 GYR since z = 2.5: Different Quenching for Central and Satellite Galaxies
  • Optically Faint Massive Balmer Break Galaxies at z > 3 in the CANDELS/GOODS Fields
  • Phantom dark energy as a natural selection of evolutionary processes a ^ la genetic algorithm and cosmological tensions
  • Photometric Redshift Calibration Requirements for WFIRST Weak-lensing Cosmology: Predictions from CANDELS
  • Potential signature of a quadrupolar hubble expansion in Pantheon+supernovae
  • Probing the Dawn of Galaxies at z ~ 9-12: New Constraints from HUDF12/XDF and CANDELS data
  • Probing the Star Formation Main Sequence Down to 108 M at 1.0 < z < 3.0
  • Properties of galaxies reproduced by a hydrodynamic simulation
  • Properties of Submillimeter Galaxies in the CANDELS GOODS-South Field
  • Quantifying Non-parametric Structure of High-redshift Galaxies with Deep Learning
  • Quenching and morphological transformation in semi-analytic models and CANDELS
  • Reconstructing the Assembly of Massive Galaxies. II. Galaxies Develop Massive and Dense Stellar Cores as They Evolve and Head toward Quiescence at Cosmic Noon
  • Reducing the Uncertainty on the Hubble Constant up to 35% with an Improved Statistical Analysis: Different Best-fit Likelihoods for Type Ia Supernovae, Baryon Acoustic Oscillations, Quasars, and Gamma-Ray Bursts
  • Robust identification of active galactic nuclei through HST optical variability in GOODS-S: comparison with the X-ray and mid-IR-selected samples
  • Selection of Massive Evolved Galaxies at 3 <= z <= 4.5 in the CANDELS Fields
  • Serendipitous Discovery of a Massive cD Galaxy at z = 1.096: Implications for the Early Formation and Late Evolution of cD Galaxies
  • SIMBA: Cosmological simulations with black hole growth and feedback
  • Simulations of the WFIRST Supernova Survey and Forecasts of Cosmological Constraints
  • SKYSURF-3: Testing Crowded Object Catalogs in the Hubble eXtreme Deep Field Mosaics to Study Sample Incompleteness from an Extragalactic Background Light Perspective
  • SKYSURF-4: Panchromatic Hubble Space Telescope All-Sky Surface-brightness Measurement Methods and Results
  • Slow Evolution of the Specific Star Formation Rate at z > 2: The Impact of Dust, Emission Lines, and a Rising Star Formation History
  • Smooth(er) Stellar Mass Maps in CANDELS: Constraints on the Longevity of Clumps in High-redshift Star-forming Galaxies
  • Spatially resolved star formation and inside-out quenching in the TNG50 simulation and 3D-HST observations
  • Spectroscopic Confirmation of the Rich z = 1.80 Galaxy Cluster JKCS 041 using the WFC3 Grism: Environmental Trends in the Ages and Structure of Quiescent Galaxies
  • Stellar Populations of Lya-emitting Galaxies in the HETDEX Survey. I. An Analysis of LAEs in the GOODS-N Field
  • Structural Evolution of Early-type Galaxies to z = 2.5 in CANDELS
  • Structural Parameters of Galaxies in CANDELS
  • Studying the physical properties of tidal features - I. Extracting morphological substructure in CANDELS observations and VELA simulations
  • Supermassive black holes at high redshift are expected to be obscured by their massive host galaxies interstellar medium
  • Texas Spectroscopic Search for Lya Emission at the End of Reionization I. Constraining the Lya Equivalent-width Distribution at 6.0 < z < 7.0
  • The ALPINE-ALMA CII survey. Dust mass budget in the early Universe
  • The ALPINE-ALMA C II survey. Luminosity function of serendipitous C II line emitters at z ~ 5
  • The ALPINE-ALMA CII survey. The contribution of major mergers to the galaxy mass assembly at z ~ 5
  • The Assembly of Milky-Way-like Galaxies Since z ~ 2.5
  • The ASTRODEEP-GS43 catalogue: New photometry and redshifts for the CANDELS GOODS-South field
  • The Cosmos in Its Infancy: JADES Galaxy Candidates at z > 8 in GOODS-S and GOODS-N
  • The Dearth of z ~ 10 Galaxies in All HST Legacy Fields--The Rapid Evolution of the Galaxy Population in the First 500 Myr
  • The debiased morphological transformations of galaxies since z = 3 in CANDELS
  • The evolution of the X-ray luminosity functions of unabsorbed and absorbed AGNs out to z~ 5
  • The hidden side of cosmic star formation at z > 3. Bridging optically dark and Lyman-break galaxies with GOODS-ALMA
  • The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) Survey Design, Reductions, and Detections
  • The HST eXtreme Deep Field (XDF): Combining All ACS and WFC3/IR Data on the HUDF Region into the Deepest Field Ever
  • The Hubble Legacy Field GOODS-S Photometric Catalog
  • The Impact of Inclination-dependent Attenuation on Ultraviolet Star Formation Rate Tracers
  • The impact of satellite trails on Hubble Space Telescope observations
  • The JWST Advanced Deep Extragalactic Survey: Discovery of an Extreme Galaxy Overdensity at z = 5.4 with JWST/NIRCam in GOODS-S
  • The KMOS Deep Survey (KDS) - I. Dynamical measurements of typical star-forming galaxies at z 3.5
  • The Magellan M2FS Spectroscopic Survey of High-redshift Galaxies: The Brightest Lyman-break Galaxies at z ~ 6
  • The MAGPI survey: evolution of radial trends in star formation activity across cosmic time
  • The mass-metallicity-star formation rate relation at z 2 with 3D Hubble Space Telescope
  • The mean Ha EW and Lyman-continuum photon production efficiency for faint z 4-5 galaxies
  • The missing light of the Hubble Ultra Deep Field
  • The MOSDEF survey: a comprehensive analysis of the rest-optical emission-line properties of z ~ 2.3 star-forming galaxies
  • The MOSDEF Survey: AGN Multi-wavelength Identification, Selection Biases, and Host Galaxy Properties
  • The MOSDEF survey: an improved Voronoi binning technique on spatially resolved stellar populations at z ~ 2
  • The MOSDEF survey: differences in SFR and metallicity for morphologically selected mergers at z ~ 2
  • The MOSDEF Survey: Dissecting the Star Formation Rate versus Stellar Mass Relation Using Ha and Hb Emission Lines at z ~ 2
  • The MOSDEF Survey: Electron Density and Ionization Parameter at z ~ 2.3
  • The MOSDEF survey: the dependence of H a-to-UV SFR ratios on SFR and size at z 2
  • The MOSDEF survey: towards a complete census of the z 2.3 star-forming galaxy population
  • The MOSFIRE Deep Evolution Field (MOSDEF) Survey: Rest-frame Optical Spectroscopy for ~1500 H-selected Galaxies at 1.37 < z < 3.8
  • The Most Luminous z ~ 9-10 Galaxy Candidates Yet Found: The Luminosity Function, Cosmic Star-formation Rate, and the First Mass Density Estimate at 500 Myr
  • The MUSE Hubble Ultra Deep Field Survey. VIII. Extended Lyman-a haloes around high-z star-forming galaxies
  • The MUSE Hubble Ultra Deep Field Survey. XII. Mg II emission and absorption in star-forming galaxies
  • The MUSE-Wide survey: Three-dimensional clustering analysis of Lyman-a emitters at 3.3 < z < 6
  • The O IIIl5007 equivalent width distribution at z 2: the redshift evolution of the extreme emission line galaxies
  • The Pantheon+ Analysis: Cosmological Constraints
  • The Pantheon+ Analysis: SuperCal-fragilistic Cross Calibration, Retrained SALT2 Light-curve Model, and Calibration Systematic Uncertainty
  • The Pantheon+ Analysis: The Full Data Set and Light-curve Release
  • The Physical Properties of Massive Green Valley Galaxies as a Function of Environments at 0.5 < z < 2.5 in 3D-HST/Candels Fields
  • The Physical Properties of Star-forming Galaxies with Strong O III Lines at z = 3.25
  • The Progenitors of the Compact Early-type Galaxies at High Redshift
  • The progenitors of the first red sequence galaxies at z ~ 2
  • The Properties of Ha Emission-line Galaxies at Z = 2.24
  • The properties of (sub-)millimetre-selected galaxies as revealed by CANDELS HST WFC3/IR imaging in GOODS-South
  • The Stellar Mass Function in CANDELS and Frontier Fields: The Buildup of Low-mass Passive Galaxies since z 3
  • The Structural Evolution of Milky-Way-like Star-forming Galaxies since z ~ 1.3
  • The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10
  • The UV Luminosity Function of Star-forming Galaxies via Dropout Selection at Redshifts z ~ 7 and 8 from the 2012 Ultra Deep Field Campaign
  • The UV spectral slope b and stellar population of most active star-forming galaxies at z ~ 4
  • The VANDELS survey: The relation between the UV continuum slope and stellar metallicity in star-forming galaxies at z ~ 3
  • The VANDELS survey: the role of ISM and galaxy physical properties in the escape of Lya emission in z ~ 3.5 star-forming galaxies
  • Tight Correlations between Massive Galaxy Structural Properties and Dynamics: The Mass Fundamental Plane was in Place by z ~ 2
  • To Stack or Not to Stack: Spectral Energy Distribution Properties of Lya-emitting Galaxies at z = 2.1
  • Tracing the rise of supermassive black holes. A panchromatic search for faint, unobscured quasars at z 6 with COSMOS-Web and other surveys
  • TRINITY I: self-consistently modelling the dark matter halo-galaxy-supermassive black hole connection from z = 0-10
  • Two Massive, Compact, and Dust-obscured Candidate z 8 Galaxies Discovered by JWST
  • Type Ia Supernova Distances at Redshift >1.5 from the Hubble Space Telescope Multi-cycle Treasury Programs: The Early Expansion Rate
  • Type Ia Supernova Rate Measurements to Redshift 2.5 from CANDELS: Searching for Prompt Explosions in the Early Universe
  • Ultraviolet luminosity density of the universe during the epoch of reionization
  • UNIVERSEMACHINE: The correlation between galaxy growth and dark matter halo assembly from z = 0-10
  • What is the Physical Origin of Strong Lya Emission? I. Demographics of Lya Emitter Structures
  • When VLT Meets HST: The HUGS Survey
  • X-Ray Selected AGN Host Galaxies are Similar to Inactive Galaxies out to z = 3: Results from CANDELS/CDF-S
  • ZFOURGE: Using Composite Spectral Energy Distributions to Characterize Galaxy Populations at 1 < z < 4
  • SSFR-M * Diagram: A Valuable Galaxy Evolution Diagnostic to Complement (s)SFR-M * Diagrams
Instrument ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage 2011-07-28T15:36:47Z/2012-02-18T14:36:45Z
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 2012-02-18T20:43:28Z
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, Faber comma Sandra M., 2012, 'Galaxy Assembly and the Evolution of Structure over the First Third of Cosmic Time - III', 1.0, European Space Agency, https://doi.org/10.5270/esa-p0c4gr8