A dataset provided by the European Space Agency

Name 12440
Title Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey -- GOODS-South Field, Non-SNe-Searched Visits
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12440;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-w8l64oh
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=12440&mission=hst
Publication
  • 3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts, and Stellar Masses
  • A CANDELS-3D-HST synergy: Resolved Star Formation Patterns at 0.7 < z < 1.5
  • A catalog of polychromatic bulge-disc decompositions of ~17.600 galaxies in CANDELS
  • Active Galactic Nuclei Selection and Demographics: A New Age with JWST/MIRI
  • 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
  • A large, deep 3 deg2 survey of H a, O III, and O II emitters from LAGER: constraining luminosity functions
  • A Large Massive Quiescent Galaxy Sample at z ~ 1.2
  • ALMA Measures Rapidly Depleted Molecular Gas Reservoirs in Massive Quiescent Galaxies at z ~ 1.5
  • A Mass-dependent Slope of the Galaxy Size-Mass Relation out to z ~ 3: Further Evidence for a Direct Relation between Median Galaxy Size and Median Halo Mass
  • A new derivation of the Hubble constant from g-ray attenuation using improved optical depths for the Fermi and CTA era
  • An Exponential Decline at the Bright End of the z = 6 Galaxy Luminosity Function
  • An Ha Impression of Lya Galaxies at z 6 with Deep JWST/NIRCam Imaging
  • An observational determination of the evolving extragalactic background light from the multiwavelength HST/CANDELS survey in the Fermi and CTA era
  • A possible large-scale alignment of galaxy spin directions - Analysis of 10 datasets from SDSS, Pan-STARRS, and HST
  • A Redshift-independent Efficiency Model: Star Formation and Stellar Masses in Dark Matter Halos at z 4
  • 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
  • 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
  • A unique distant submillimeter galaxy with an X-ray-obscured radio-luminous active galactic nucleus
  • Automated distant galaxy merger classifications from Space Telescope images using the Illustris simulation
  • Automatic identification of outliers in Hubble Space Telescope galaxy images
  • Being KLEVER at cosmic noon: Ionized gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts
  • Blue Rest-frame UV-optical Colors in z 8 Galaxies from GREATS: Very Young Stellar Populations at 650 Myr of Cosmic Time
  • Bright Lyman-a emitters among Spitzer SMUVS galaxies in the MUSE/COSMOS field
  • 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: 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
  • CANDELSz7: a large spectroscopic survey of CANDELS galaxies in the reionization epoch
  • Can intrinsic alignments of elongated low-mass galaxies be used to map the cosmic web at high redshift?
  • Cluster Cosmology Constraints from the 2500 deg2 SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope
  • Clustering dependence on Lya luminosity from MUSE surveys at 3 < z < 6
  • Cluster mass calibration at high redshift: HST weak lensing analysis of 13 distant galaxy clusters from the South Pole Telescope Sunyaev-Zeldovich Survey
  • Compact star-forming galaxies preferentially quenched to become PSBs in z < 1 clusters
  • Comparison of Observed Galaxy Properties with Semianalytic Model Predictions Using Machine Learning
  • CONGRUENTS (COsmic-ray, Neutrino, Gamma-ray and Radio Non-Thermal Spectra) - II. Population-level correlations between galactic infrared, radio, and g-ray emission
  • COSMOS-DASH: The Evolution of the Galaxy Size-Mass Relation since z ~ 3 from New Wide-field WFC3 Imaging Combined with CANDELS/3D-HST
  • Definitive upper bound on the negligible contribution of quasars to cosmic reionization
  • Delving deep: A population of extremely dusty dwarfs observed by JWST
  • Dependence of galaxy clustering on UV luminosity and stellar mass at z ~ 4-7
  • Detecting outliers in astronomical images with deep generative networks
  • Discovery of Lyman Break Galaxies at z ~ 7 from the zFourGE Survey
  • Distinguishing Mergers and Disks in High-redshift Observations of Galaxy Kinematics
  • Dual constraints with ALMA: new O III 88-mm and dust-continuum observations reveal the ISM conditions of luminous LBGs at z 7
  • Dust attenuation and Ha emission in a sample of galaxies observed with Herschel at 0.6 < z < 1.6
  • 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
  • Effect of galaxy mergers on star-formation rates
  • Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang
  • Evidence of Very Low Metallicity and High Ionization State in a Strongly Lensed, Star-forming Dwarf Galaxy at z= 3.417
  • Evident black hole-bulge coevolution in the distant universe
  • Evolution of N/O abundance ratios and ionization parameters from z ~ 0 to 2 investigated by the direct temperature method*+
  • 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 Fraction of Clumpy Galaxies at 0.2 < z < 1.0 in the COSMOS Field
  • Exploring AGN and star formation activity of massive galaxies at cosmic noon
  • Exploring the Gas-phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
  • Extending the evolution of the stellar mass-size relation at z <= 2 to low stellar mass galaxies from HFF and CANDELS
  • 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?
  • Fraction of Clumpy Star-forming Galaxies at 0.5 <= z <= 3 in UVCANDELS: Dependence on Stellar Mass and Environment
  • From Naked Spheroids to Disky Galaxies: How Do Massive Disk Galaxies Shape Their Morphology?
  • 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 Evolution in All Five CANDELS Fields and IllustrisTNG: Morphological, Structural, and the Major Merger Evolution to z 3
  • Galaxy Merger Rates up to z ~ 3 Using a Bayesian Deep Learning Model: A Major-merger Classifier Using IllustrisTNG Simulation Data
  • Galaxy Mergers up to z < 2.5. II. AGN Incidence in Merging Galaxies at Separations of 3-15 kpc
  • Galaxy Mergers up to Z < 2.5. I. The Star Formation Properties of Merging Galaxies at Separations of 3-15 kpc
  • Galaxy Morphology Network: A Convolutional Neural Network Used to Study Morphology and Quenching in ~100,000 SDSS and ~20,000 CANDELS Galaxies
  • Galaxy Quenching at the High Redshift Frontier: A Fundamental Test of Cosmological Models in the Early Universe with JWST-CEERS
  • Galaxy Sizes Since z = 2 from the Perspective of Stellar Mass Distribution within Galaxies
  • Galaxy spin direction distribution in HST and SDSS show similar large-scale asymmetry
  • Galaxy Stellar Mass Functions from ZFOURGE/CANDELS: An Excess of Low-mass Galaxies since z = 2 and the Rapid Buildup of Quiescent Galaxies
  • GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies
  • GOODS-ALMA: Optically dark ALMA galaxies shed light on a cluster in formation at z = 3.5
  • Half-mass Radii for ~7000 Galaxies at 1.0 <= z <= 2.5: Most of the Evolution in the Mass-Size Relation Is Due to Color Gradients
  • HALO7D. III. Chemical Abundances of Milky Way Halo Stars from Medium-resolution Spectra
  • HALO7D II: The Halo Velocity Ellipsoid and Velocity Anisotropy with Distant Main-sequence Stars
  • HALO7D I. The Line-of-sight Velocities of Distant Main-sequence Stars in the Milky Way Halo
  • 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?
  • Hubble Imaging of the Ionizing Radiation from a Star-forming Galaxy at Z=3.2 with fesc>50%
  • 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
  • Implications of Increased Central Mass Surface Densities for the Quenching of Low-mass Galaxies
  • Inference of the cosmic rest-frame from supernovae Ia
  • Investigating the Dominant Environmental Quenching Process in UVCANDELS/COSMOS Groups
  • Investigating the Effect of Galaxy Interactions on Star Formation at 0.5 < z < 3.0
  • Investigating the Effect of Galaxy Interactions on the Enhancement of Active Galactic Nuclei at 0.5 < z < 3.0
  • Ionized gas kinematics and chemical abundances of low-mass star-forming galaxies at z ~ 3
  • Ionizing the intergalactic medium by star clusters: the first empirical evidence
  • 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
  • KROSS: mapping the Ha emission across the star formation sequence at z 1
  • KURVS: the outer rotation curve shapes and dark matter fractions of z 1.5 star-forming galaxies
  • Large-scale asymmetry in galaxy spin directions: Analysis of galaxies with spectra in DES, SDSS, and DESI Legacy Survey
  • Large-scale Structures in the CANDELS Fields: The Role of the Environment in Star Formation Activity
  • Linking galaxy structural properties and star formation activity to black hole activity with IllustrisTNG
  • Local Analogs to High-redshift Galaxies. I. Characterization of Dust Emission and Star Formation History
  • Lower-luminosity Obscured AGN Host Galaxies Are Not Predominantly in Major-merging Systems at Cosmic Noon
  • Low Star Formation Activity and Low Gas Content of Quiescent Galaxies at z = 3.5-4.0 Constrained with ALMA
  • Lya and C III emission in z = 7-9 Galaxies: accelerated reionization around luminous star-forming systems?
  • Mass assembly history of dark matter haloes in the light of H0 tension
  • Mock light-cones and theory friendly catalogues for the CANDELS survey
  • Modelling and interpreting spectral energy distributions of galaxies with BEAGLE
  • Morphologies of ~190,000 Galaxies at z = 0-10 Revealed with HST Legacy Data. III. Continuum Profile and Size Evolution of Lya Emitters
  • Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology
  • MOSEL: Strong OIII 5007 A Emitting Galaxies at (3 < z < 4) from the ZFOURGE Survey
  • MOSEL Survey: Tracking the Growth of Massive Galaxies at 2 < z < 4 Using Kinematics and the IllustrisTNG Simulation
  • MOSFIRE Absorption Line Spectroscopy of z > 2 Quiescent Galaxies: Probing a Period of Rapid Size Growth
  • Nature versus nurture: what regulates star formation in satellite galaxies?
  • Near infrared spectroscopy and star-formation histories of 3 <= z <= 4 quiescent galaxies
  • Near-IR Weak-lensing (NIRWL) Measurements in the CANDELS Fields. I. Point-spread Function Modeling and Systematics
  • New criteria for the selection of galaxy close pairs from cosmological simulations: evolution of the major and minor merger fraction in MUSE deep fields
  • 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
  • Nonparametric Star Formation History Reconstruction with Gaussian Processes. I. Counting Major Episodes of Star Formation
  • 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
  • Observations of Environmental Quenching in Groups in the 11 GYR since z = 2.5: Different Quenching for Central and Satellite Galaxies
  • Observations of the initial formation and evolution of spiral galaxies at 1 < z < 3 in the CANDELS fields
  • On the AGN Nature of Two UV-bright Sources at zspec ~ 5.5 in the CANDELS Fields: An Update on the AGN Space Density at M1450 ~ -22.5
  • Photometric Redshift Calibration Requirements for WFIRST Weak-lensing Cosmology: Predictions from CANDELS
  • Photometric Redshift Estimation with Galaxy Morphology Using Self-organizing Maps
  • Photometry of high-redshift blended galaxies using deep learning
  • Plateau de Bure High-z Blue Sequence Survey 2 (PHIBSS2): Search for Secondary Sources, CO Luminosity Functions in the Field, and the Evolution of Molecular Gas Density through Cosmic Time
  • Probabilistic model for dynamic galaxy decomposition
  • Probing the Star Formation Main Sequence Down to 108 M at 1.0 < z < 3.0
  • Quantifying Non-parametric Structure of High-redshift Galaxies with Deep Learning
  • Quenching as a Contest between Galaxy Halos and Their Central Black Holes
  • Reconstructing the Assembly of Massive Galaxies. II. Galaxies Develop Massive and Dense Stellar Cores as They Evolve and Head toward Quiescence at Cosmic Noon
  • Reconstructing the Assembly of Massive Galaxies. I. The Importance of the Progenitor Effect in the Observed Properties of Quiescent Galaxies at z 2
  • Red and dead CANDELS: massive passive galaxies at the dawn of the Universe
  • Revealing the formation histories of the first stars with the cosmic near-infrared background
  • Revealing the Impact of Critical Stellar Central Density on Galaxy Quenching through Cosmic Time
  • Revealing the Stellar Mass and Dust Distributions of Submillimeter Galaxies at Redshift 2
  • Rotation Curves in z ~ 1-2 Star-forming Disks: Evidence for Cored Dark Matter Distributions
  • Rotation in C II-emitting gas in two galaxies at a redshift of 6.8
  • Searching for Islands of Reionization: A Potential Ionized Bubble Powered by a Spectroscopic Overdensity at z = 8.7
  • Shape, colour, and distance in weak gravitational flexion
  • Simulations of the WFIRST Supernova Survey and Forecasts of Cosmological Constraints
  • Space Densities and Emissivities of Active Galactic Nuclei at z > 4
  • Spatially Resolved Properties of Galaxies from CANDELS+MUSE: Radial Extinction Profile and Insights on Quenching
  • Spatially resolved star formation and inside-out quenching in the TNG50 simulation and 3D-HST observations
  • Spectral Energy Distribution Fitting of HETDEX Pilot Survey Lya Emitters in COSMOS and GOODS-N
  • 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
  • Spectroscopic observations of PHz G237.01+42.50: A galaxy protocluster at z = 2.16 in the Cosmos field
  • Stellar, Gas, and Dust Emission of Star-forming Galaxies out to z ~ 2
  • Stellar Populations of Lya-emitting Galaxies in the HETDEX Survey. I. An Analysis of LAEs in the GOODS-N Field
  • Strategies for Obtaining Robust Spectral Energy Distribution Fitting Parameters for Galaxies at z ~ 1 and z ~ 2 in the Absence of Infrared Data
  • Structural analysis of massive galaxies using HST deep imaging at z < 0.5
  • Structural Parameters of Galaxies in CANDELS
  • Structure and kinematics of a massive galaxy at z ~ 7
  • Structure and Morphology of X-Ray-selected Active Galactic Nucleus Hosts at 1 < z < 3 in the CANDELS-COSMOS Field
  • Submillimeter Galaxies as Progenitors of Compact Quiescent Galaxies
  • Sunyaev-Zeldovich effect and X-ray scaling relations from weak lensing mass calibration of 32 South Pole Telescope selected galaxy clusters
  • The abundance of massive compact galaxies at 1.0 < z < 3.0 in 3D-HST/CANDELS
  • The ALMA Reionization Era Bright Emission Line Survey: The molecular gas content of galaxies at z 7
  • The ALMA Spectroscopic Survey in the HUDF: CO Luminosity Functions and the Molecular Gas Content of Galaxies through Cosmic History
  • The ALMA Spectroscopic Survey in the HUDF: Nature and Physical Properties of Gas-mass Selected Galaxies Using MUSE Spectroscopy
  • 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 Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques
  • The ASTRODEEP-GS43 catalogue: New photometry and redshifts for the CANDELS GOODS-South field
  • The bright end of the galaxy luminosity function at z7: before the onset of mass quenching?
  • The building up of observed stellar scaling relations of massive galaxies and the connection to black hole growth in the TNG50 simulation
  • The Carnegie-Irvine Galaxy Survey. VI. Quantifying Spiral Structure
  • The clustering properties of high-redshift passive galaxies
  • The connection between mergers and AGN activity in simulated and observed massive galaxies
  • The contribution of faint Lyman-a emitters to extended Lyman-a halos constrained by MUSE clustering measurements
  • 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 Effect of the Morphological Quenching Mechanism on Star Formation Activity at 0.5 < z < 1.5 in 3D-HST/CANDELS
  • The emergence of passive galaxies in the early Universe
  • The evolution of gas-phase metallicity and resolved abundances in star-forming galaxies at z 0.6-1.8
  • The evolution of the galaxy stellar-mass function over the last 12 billion years from a combination of ground-based and HST surveys
  • The Far-infrared Emission of the First Massive Galaxies
  • The Fundamental Plane of Massive Quiescent Galaxies at z ~ 2
  • The GOGREEN survey: constraining the satellite quenching time-scale in massive clusters at z 1
  • The GOGREEN Survey: Evidence of an Excess of Quiescent Disks in Clusters at 1.0
  • The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) Survey Design, Reductions, and Detections
  • The Impact of Inclination-dependent Attenuation on Ultraviolet Star Formation Rate Tracers
  • The impact of satellite trails on Hubble Space Telescope observations
  • The KMOS galaxy evolution survey (KGES): the angular momentum of star-forming galaxies over the last 10 Gyr
  • The KMOS3D Survey: Data Release and Final Survey Paper
  • The luminosity functions and redshift evolution of satellites of low-mass galaxies in the COSMOS survey
  • 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 missing light of the Hubble Ultra Deep Field
  • The Morphology-Density Relationship in 1 < z < 2 Clusters
  • The MOSDEF-LRIS survey: detection of inflowing gas towards three star-forming galaxies at z 2
  • 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: Detection of O IIIl4363 and the Direct-method Oxygen Abundance of a Star-forming Galaxy at z = 3.08
  • 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: Environmental Dependence of the Gas-phase Metallicity of Galaxies at 1.4 <= z <= 2.6
  • The MOSDEF survey: probing resolved stellar populations at z 2 Using a new bayesian-defined morphology metric called patchiness
  • The MOSDEF survey: the dependence of H a-to-UV SFR ratios on SFR and size at z 2
  • The MOSDEF survey: the mass-metallicity relationship and the existence of the FMR at z 1.5
  • 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 MUSE Hubble Ultra Deep Field Survey. XII. Mg II emission and absorption in star-forming galaxies
  • The MUSE-Wide Survey: survey description and first data release
  • The O IIIl5007 equivalent width distribution at z 2: the redshift evolution of the extreme emission line galaxies
  • The Physical Drivers of the Luminosity-weighted Dust Temperatures in High-redshift Galaxies
  • 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 relationship between dust and C I at z = 1 and beyond
  • The Role of Galaxy Interaction in the SFR-M * Relation: Characterizing Morphological Properties of Herschel-selected Galaxies at 0.2 < z < 1.5
  • The Roles of Morphology and Environment on the Star Formation Rate-Stellar Mass Relation in COSMOS from 0 < z < 3.5
  • The SCUBA-2 Cosmology Legacy Survey: demographics of the 450-mm population
  • The size and pervasiveness of Ly a-UV spatial offsets in star-forming galaxies at z ~ 6
  • The Spectrally Resolved Lya Emission of Three Lya-selected Field Galaxies at z ~ 2.4 from the HETDEX Pilot Survey
  • The Star Formation Rate-Radius Connection: Data and Implications for Wind Strength and Halo Concentration
  • 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 structural properties of classical bulges and discs from z ~ 2
  • The Structure of Massive Quiescent Galaxies at Z ~ 3 in the CANDELS-COSMOS Field
  • The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10
  • The unexpectedly large dust and gas content of quiescent galaxies at z > 1.4
  • The UV spectral slope b and stellar population of most active star-forming galaxies at z ~ 4
  • The X-SHOOTER Lyman a survey at z = 2 (XLS-z2) I: what makes a galaxy a Lyman a emitter?
  • Three-Dimensional Optimal Spectral Extraction (TDOSE) from integral field spectroscopy
  • Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 5
  • 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 Rate Measurements to Redshift 2.5 from CANDELS: Searching for Prompt Explosions in the Early Universe
  • Unbiased Differential Size Evolution and the Inside-out Growth of Galaxies in the Deep CANDELS GOODS Fields at 1 <= z <= 7
  • UNIVERSEMACHINE: The correlation between galaxy growth and dark matter halo assembly from z = 0-10
  • Using 3D and 2D analysis for analyzing large-scale asymmetry in galaxy spin directions
  • What are the Progenitors of Compact, Massive, Quiescent Galaxies at z = 2.3? The Population of Massive Galaxies at z > 3 from NMBS and CANDELS
  • What is the Physical Origin of Strong Lya Emission? I. Demographics of Lya Emitter Structures
  • X-shooter Spectroscopy and HST Imaging of 15 Massive Quiescent Galaxies at z 2
  • 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 2011-12-06T16:22:43Z/2012-04-15T10:15:35Z
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 2012-04-16T15:43:45Z
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, Faber comma Sandra M., 2012, 'Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey -- GOODS-South Field, Non-SNe-Searched Visits', 1.0, European Space Agency, https://doi.org/10.5270/esa-w8l64oh