A dataset provided by the European Space Agency

Name 9978
Title The Ultra Deep Field with ACS
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=9978;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-501qmxy
Author Beckwith, Steven
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=9978&mission=hst
Publication
  • A 1.4 deg2 blind survey for C II, C III and C IV at z ~ 0.7-1.5 - I. Nature, morphologies and equivalent widths
  • Accurate PSF-matched photometry and photometric redshifts for the extreme deep field with the Chebyshev-Fourier functions
  • A critical analysis of the ultraviolet continuum slopes (b) of high-redshift galaxies: no evidence (yet) for extreme stellar populations at z > 6
  • A faint red stellar halo around an edge-on disc galaxy in the Hubble Ultra Deep Field
  • A forming disk at z ~ 0.6: collapse of a gaseous disk or major merger remnant?
  • A joint measurement of galaxy luminosity functions and large-scale field densities during the Epoch of Reionization
  • ALMA constraints on star-forming gas in a prototypical z = 1.5 clumpy galaxy: the dearth of CO(5-4) emission from UV-bright clumps
  • A method to search for strong galaxy-galaxy lenses in optical imaging surveys
  • An Analysis of ALMA Deep Fields and the Perceived Dearth of High-z Galaxies
  • A new multifield determination of the galaxy luminosity function at z = 7-9 incorporating the 2012 Hubble Ultra-Deep Field imaging
  • An Increasing Stellar Baryon Fraction in Bright Galaxies at High Redshift
  • An infrared view of the coevolution of massive blackholes and galaxies
  • A Physical Approach to the Identification of High-z Mergers: Morphological Classification in the Stellar Mass Domain.
  • A quantitative assessment of completeness correction methods and public release of a versatile simulation code
  • A Redshift-independent Efficiency Model: Star Formation and Stellar Masses in Dark Matter Halos at z 4
  • A Redshift z ~ 5.4 Lya Emitting Galaxy with Linear Morphology in the GRAPES/Hubble Ultra Deep Field
  • 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 Very Compact Dense Galaxy Overdensity with d 130 Identified at z ~ 8: Implications for Early Protocluster and Cluster Core Formation
  • Axion Decay and Anisotropy of Near-IR Extragalactic Background Light
  • A z = 3.045 Lya emitting halo hosting a QSO and a possible candidate for AGN-triggered star formation.
  • Bipolar outflows out to 10 kpc for massive galaxies at redshift z 1
  • Brown Dwarf Candidates in the JADES and CEERS Extragalactic Surveys
  • Bulge and Clump Evolution in Hubble Ultra Deep Field Clump Clusters, Chains and Spiral Galaxies
  • Bulge Formation by the Coalescence of Giant Clumps in Primordial Disk Galaxies
  • Candidates of z ~= 5.5-7 Galaxies in the Hubble Space Telescope Ultra Deep Field
  • Classification of extremely red objects in the Hubble Ultra Deep Field
  • Clues to Active Galactic Nucleus Growth from Optically Variable Objects in the Hubble Ultra Deep Field
  • Clustering dependence on Lya luminosity from MUSE surveys at 3 < z < 6
  • Clustering of i775 Dropout Galaxies at z ~ 6 in GOODS and the UDF
  • Cluster mass calibration at high redshift: HST weak lensing analysis of 13 distant galaxy clusters from the South Pole Telescope Sunyaev-Zeldovich Survey
  • Cold dust and stellar emissions in dust-rich galaxies observed with ALMA: a challenge for SED-fitting techniques
  • Color, 3D simulated images with shapelets
  • Colour jumps across the spiral arms of Hubble Ultra Deep Field galaxies
  • Constraints on the star-formation rate of z ~ 3 LBGs with measured metallicity in the CANDELS GOODS-South field
  • Contamination on Lyman continuum emission at z >~ 3: implication on the ionizing radiation evolution
  • Cosmic Variance and Its Effect on the Luminosity Function Determination in Deep High-z Surveys
  • Cross-correlation between X-Ray and Optical/Near-infrared Background Intensity Fluctuations
  • Deep Keck u-Band Imaging of the Hubble Ultra Deep Field: A Catalog of z ~ 3 Lyman Break Galaxies
  • Designing future dark energy space missions. I. Building realistic galaxy spectro-photometric catalogs and their first applications
  • Did galaxy assembly and supermassive black-hole growth go hand-in-hand?
  • Discovery of a galaxy overdensity around a powerful, heavily obscured FRII radio galaxy at z = 1.7: star formation promoted by large-scale AGN feedback?
  • Disc scalelengths out to redshift 5.8
  • Empirical Predictions for (Sub-)millimeter Line and Continuum Deep Fields
  • Evidence for a Massive Poststarburst Galaxy at z~6.5
  • Evolution in the Continuum Morphological Properties of Lya-emitting Galaxies from z = 3.1 to z = 2.1
  • 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 Intergalactic Opacity: Implications for the Ionizing Background, Cosmic Star Formation, and Quasar Activity
  • Evolution of the UV LF from z 15 to z 8 using new JWST NIRCam medium-band observations over the HUDF/XDF
  • Extended and filamentary Lya emission from the formation of a protogalactic halo at z = 2.63
  • Extragalactic background light: a measurement at 400 nm using dark cloud shadow - II. Spectroscopic separation of the dark clouds light, and results
  • Faint U-Band Dropouts in the WFPC2 Parallels of the Hubble Ultra Deep Field
  • FIGS--Faint Infrared Grism Survey: Description and Data Reduction
  • Filamentary infall of cold gas and escape of Lya and hydrogen ionizing radiation from an interacting high-redshift galaxy
  • First constraints on the stellar mass function of star-forming clumps at the peak of cosmic star formation
  • Flexion measurement in simulations of Hubble Space Telescope data
  • Fluctuation of the background sky in the Hubble Extremely Deep Field (XDF) and its origin
  • Galaxies at z ~ 6: The UV Luminosity Function and Luminosity Density from 506 HUDF, HUDF Parallel ACS Field, and GOODS i-Dropouts
  • Galaxies in the Hubble Ultra Deep Field. I. Detection, Multiband Photometry, Photometric Redshifts, and Morphology
  • Galaxy clustering measurements out to redshift z ~ 8 from Hubble Legacy Fields
  • Galaxy evolution by color-log(n) type since redshift unity in the Hubble Ultra Deep Field
  • Galaxy luminosity function pipeline for cosmology and astrophysics
  • Galaxy Morphologies in the Hubble Ultra Deep Field: Dominance of Linear Structures at the Detection Limit
  • Galaxy Size Evolution at High Redshift and Surface Brightness Selection Effects: Constraints from the Hubble Ultra Deep Field
  • Globular cluster systems in nearby dwarf galaxies - III. Formation efficiencies of old globular clusters
  • GOODS-ALMA: 1.1 mm galaxy survey. I. Source catalog and optically dark galaxies
  • HALO7D II: The Halo Velocity Ellipsoid and Velocity Anisotropy with Distant Main-sequence Stars
  • High-Redshift Extremely Red Objects in the Hubble Space Telescope Ultra Deep Field Revealed by the GOODS Infrared Array Camera Observations
  • High resolution science with high redshift galaxies
  • HOLISMOKES. IV. Efficient mass modeling of strong lenses through deep learning
  • Hubble Space Telescope/Advanced Camera for Surveys Confirmation of the Dark Substructure in A520
  • Hubble Ultra Deep Field-JD2: Mid-Infrared Evidence for a z ~ 2 Luminous Infrared Galaxy
  • HUDF 1619--A candidate for polar-ring galaxies in the Hubble Ultra Deep Field
  • Illuminating gas inflows/outflows in the MUSE deepest fields: Lya nebulae around forming galaxies at z 3.3
  • Improving PSF modelling for weak gravitational lensing using new methods in model selection
  • Interacting galaxies in deep fields of the Hubble Space Telescope
  • Is the Gini Coefficient a Stable Measure of Galaxy Structure?
  • JEMS: A Deep Medium-band Imaging Survey in the Hubble Ultra Deep Field with JWST NIRCam and NIRISS
  • Lensing Signals in the Hubble Ultra Deep Field Using All Second-Order Shape Deformations
  • Life beyond 30: Probing the -20 < M UV < -17 Luminosity Function at 8 < z < 13 with the NIRCam Parallel Field of the MIRI Deep Survey
  • Luminosities, Masses and Star Formation Rates of Galaxies at High Redshift
  • Luminous Compact Blue Galaxies up to z~1 in the Hubble Space Telescope Ultra Deep Field. I. Small Galaxies or Blue Centers of Massive Disks?
  • Lyman alpha galaxies: Physical properties and effects of dust at high redshift
  • Massive Clumps in Local Galaxies: Comparisons with High-redshift Clumps
  • Measuring Sizes of Ultra-faint Dwarf Galaxies
  • Metallicity evolution, metallicity gradients, and gas fractions at z ~ 3.4
  • Method for analyzing the spatial distribution of galaxies on gigaparsec scales. II. Application to a grid of the HUDF-FDF-COSMOS-HDF surveys
  • 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
  • Morphological Evolution of Galaxies from Ultra-deep Hubble Space Telescope Wide Field Camera 3 Imaging: The Hubble Sequence at z ~ 2
  • Morphologies of ~190,000 Galaxies at z = 0-10 Revealed with HST Legacy Data. II. Evolution of Clumpy Galaxies
  • Morphologies of ~190,000 Galaxies at z = 0-10 Revealed with HST Legacy Data. III. Continuum Profile and Size Evolution of Lya Emitters
  • Morphology and Evolution of Emission-Line Galaxies in the Hubble Ultra Deep Field
  • Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology
  • Morphology of Spitzer 24 mm Detected Galaxies in the UDF: The Links between Star Formation and Galaxy Morphology
  • Moving Objects in the Hubble Ultra Deep Field
  • Multi-wavelength View of Kiloparsec-scale Clumps in Star-forming Galaxies at z ~ 2
  • MUSE Spectroscopic Identifications of Ultra-faint Emission Line Galaxies with M UV ~ -15
  • Near-Infrared Properties of Faint X-Ray Sources from NICMOS Imaging in the Chandra Deep Fields
  • Near-infrared properties of i-drop galaxies in the Hubble Ultra Deep Field
  • Nearly all the sky is covered by Lyman-a emission around high-redshift galaxies
  • New Constraints on the Lyman Continuum Escape Fraction at z~1.3
  • 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 star-forming galaxies at z 7 from Wide Field Camera Three imaging
  • NGDEEP Epoch 1: The Faint End of the Luminosity Function at z 9-12 from Ultradeep JWST Imaging
  • No Overdensity of Lyman-Alpha Emitting Galaxies around a Quasar at z ~ 5.7
  • Observational aspects of galactic accretion at redshift 3.3
  • Observations and modeling of a clumpy galaxy at z = 1.6. Spectroscopic clues to the origin and evolution of chain galaxies
  • Observations of Thick Disks in the Hubble Space Telescope Ultra Deep Field
  • On the characteristics of tidal structures of interacting galaxies
  • On the Nature of Sub-Millimeter Galaxies
  • On the Origin of Exponential Disks at High Redshift
  • On the Stellar Masses of Giant Clumps in Distant Star-forming Galaxies
  • On the Stellar Populations in Faint Red Galaxies in the Hubble Ultra Deep Field
  • ORIGIN: Blind detection of faint emission line galaxies in MUSE datacubes
  • Origins of weak lensing systematics, and requirements on future instrumentation (or knowledge of instrumentation)
  • Overconfidence in photometric redshift estimation
  • Photo-z-SQL: Integrated, flexible photometric redshift computation in a database
  • Physical Properties of Sub-galactic Clumps at 0.5 <= Z <= 1.5 in the UVUDF
  • PICS: Simulations of Strong Gravitational Lensing in Galaxy Clusters
  • Pitch angles of distant spiral galaxies
  • Point spread function tails and the measurements of diffuse stellar halo light around edge-on disc galaxies
  • Precise Mass Determination of SPT-CL J2106-5844, the Most Massive Cluster at z > 1
  • Predicting the number of giant arcs expected in the next-generation wide-field surveys from space
  • Properties of galaxies reproduced by a hydrodynamic simulation
  • Quantifying the physical properties of high-redshift galaxies: A multi-wavelength survey on the progenitors of local galaxies
  • Radius-dependent Luminosity Evolution of Blue Galaxies in GOODS-N
  • Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at 1.5 < z < 6.4
  • Redshift identification of X-ray-selected active galactic nuclei in the J1030 field: searching for large-scale structures and high-redshift sources
  • Resolving the Galaxies within a Giant Lya Nebula: Witnessing the Formation of a Galaxy Group?
  • Rest-frame UV Colors for Faint Galaxies at z ~ 9-16 with the JWST NGDEEP Survey
  • Revealing the formation histories of the first stars with the cosmic near-infrared background
  • Robust identification of active galactic nuclei through HST optical variability in GOODS-S: comparison with the X-ray and mid-IR-selected samples
  • Searching for Low Surface Brightness Galaxies in the Hubble Ultra Deep Field: Implications for the Star Formation Efficiency in Neutral Gas at z~3
  • Simulating and interpreting deep observations in the Hubble Ultra Deep Field with the JWST/NIRSpec low-resolution `prism
  • Simulating Deep Hubble Images with Semi-empirical Models of Galaxy Formation
  • 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
  • Star Formation from DLA Gas in the Outskirts of Lyman Break Galaxies at z ~ 3
  • Star Formation History of the Hubble Ultra Deep Field: Comparison with the Hubble Deep Field-North
  • Star Formation in Damped Lyman-alpha systems and the Outskirts of Lyman Break Galaxies
  • Stars in the Hubble Ultra Deep Field
  • Statistics of interacting galaxies at z ~ 0.7
  • Stellar Disk Truncations at High z: Probing Inside-Out Galaxy Formation
  • Stellar haloes of disc galaxies at z ~ 1
  • Stellar Populations of Late-Type Bulges at z 1 in the Hubble Ultra Deep Field
  • Strong lens modelling: comparing and combining Bayesian neural networks and parametric profile fitting
  • Strong magnesium(II) absorbers and their relation to galaxies
  • Structural and physical properties of high redshift galaxies in the Hubble Ultra Deep Field
  • Sunyaev-Zeldovich effect and X-ray scaling relations from weak lensing mass calibration of 32 South Pole Telescope selected galaxy clusters
  • Suppression of dwarf galaxy formation by cosmic reionization
  • Tadpole Galaxies in the Hubble Ultra Deep Field
  • Testing Gravitational Lensing as the Source of Enhanced Strong Mg II Absorption toward Gamma-Ray Bursts
  • The abundance of z 10 galaxy candidates in the HUDF using deep JWST NIRCam medium-band imaging
  • The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Molecular Gas Reservoirs in High-redshift Galaxies
  • The ALMA Spectroscopic Survey in the HUDF: A Search for C II Emitters at 6 <= z <= 8
  • The ALMA Spectroscopic Survey in the HUDF: Deep 1.2 mm Continuum Number Counts
  • The analysis of effective galaxies number count for Chinese Space Station Optical Survey (CSS-OS) by image simulation
  • The baryonic content and Tully-Fisher relation at z ~ 0.6
  • The Bivariate Size-Luminosity Relations for Lyman Break Galaxies at z ~ 4-5
  • The contribution of faint galaxy wings to source-subtracted near-infrared background fluctuations
  • The contribution of faint Lyman-a emitters to extended Lyman-a halos constrained by MUSE clustering measurements
  • The contribution of high-redshift galaxies to cosmic reionization: new results from deep WFC3 imaging of the Hubble Ultra Deep Field
  • The Cosmos in Its Infancy: JADES Galaxy Candidates at z > 8 in GOODS-S and GOODS-N
  • The Deepest Supernova Search is Realized in the Hubble Ultra Deep Field Survey
  • The Effect of Surface Brightness Dimming in the Selection of High-z Galaxies
  • The End of the White Dwarf Cooling Sequence in M4: An Efficient Approach
  • The Environments of High-Redshift Quasi-Stellar Objects
  • The Evolution of Galaxy Number Density at z < 8 and Its Implications
  • The Evolution of Stellar Mass in Galaxies in the NICMOS Ultra Deep Field
  • 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 X-ray luminosity functions of unabsorbed and absorbed AGNs out to z~ 5
  • The expected detection of dust emission from high-redshift Lyman a galaxies
  • The galaxy luminosity-size relation and selection biases in the Hubble Ultra Deep Field
  • The Great Observatories Origins Deep Survey: Constraints on the Lyman Continuum Escape Fraction Distribution of Lyman-break Galaxies at 3.4 < z < 4.5
  • The GREATS H b + O III luminosity function and galaxy properties at z ~ 8: walking the way of JWST
  • The hidden side of cosmic star formation at z > 3. Bridging optically dark and Lyman-break galaxies with GOODS-ALMA
  • 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 Hubble Ultra Deep Field
  • The impact of satellite trails on Hubble Space Telescope observations
  • The Importance of Secondary Halos for Strong Lensing in Massive Galaxy Clusters across Redshift
  • The JWST Advanced Deep Extragalactic Survey: Discovery of an Extreme Galaxy Overdensity at z = 5.4 with JWST/NIRCam in GOODS-S
  • The Long Lives of Giant Clumps and the Birth of Outflows in Gas-rich Galaxies at High Redshift
  • The mean Ha EW and Lyman-continuum photon production efficiency for faint z 4-5 galaxies
  • The measurement and applications of the faint source correlation function
  • The Morphological Diversities among Star-forming Galaxies at High Redshifts in the Great Observatories Origins Deep Survey
  • The MUSE Hubble Ultra Deep Field surveys: Data release II
  • 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. XI. Constraining the low-mass end of the stellar mass - star formation rate relation at z < 1
  • The MUSE Hubble Ultra Deep Field Survey. XVI. The angular momentum of low-mass star-forming galaxies: A cautionary tale and insights from TNG50
  • The Onset of Spiral Structure in the Universe
  • The outskirts of spiral galaxies: touching stellar halos at z~0 and z~1
  • The Possible Detection of Cosmological Reionization Sources
  • The possible detection of high-redshift Type II QSOs in deep fields
  • The Rest-Frame Far-Ultraviolet Morphologies of Star-forming Galaxies at z ~ 1.5 and 4
  • The Star Formation Rate Efficiency of Neutral Atomic-dominated Hydrogen Gas in the Outskirts of Star-forming Galaxies from z ~ 1 to z ~3
  • The star formation rate of the Universe at z~ 6 from the Hubble Ultra-Deep Field
  • The Stellar Mass Density and Specific Star Formation Rate of the Universe at z ~ 7
  • The strong gravitational lens finding challenge
  • The Structure and Star Formation History of Early-Type Galaxies in the Ultra Deep Field/GRAPES Survey
  • The structures of distant galaxies - II. Diverse galaxy structures and local environments at z = 4-6 implications for early galaxy assembly
  • The UDF05 Follow-up of the Hubble Ultra Deep Field. III. The Luminosity Function at z ~ 6
  • The UDF05 Follow-up of the Hubble Ultra Deep Field. I. The Faint-End Slope of the Lyman Break Galaxy Population at z ~ 5
  • The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10
  • The unbiased measurement of ultraviolet spectral slopes in low-luminosity galaxies at z 7
  • The UV 2175A attenuation bump and its correlation with PAH emission at z 2
  • The UV Luminosity Function of Star-forming Galaxies via Dropout Selection at Redshifts z ~ 7 and 8 from the 2012 Ultra Deep Field Campaign
  • Three Lya Emitters at z ~ 6: Early GMOS/Gemini Data from the GLARE Project
  • Tolman Test from z = 0.1 to z = 5.5: Preliminary Results challenge the Expanding Universe Model
  • Towards an understanding of dark matter: Precise gravitational lensing analysis complemented by robust photometric redshifts
  • Tracing galaxy assembly: A study of merging and emission-line galaxies
  • Tracing Galaxy Assembly: Tadpole Galaxies in the Hubble Ultra Deep Field
  • Tracing the Mass Growth and Star Formation Rate Evolution of Massive Galaxies from z ~ 6 to z ~ 1 in the Hubble Ultra-Deep Field
  • Tracing the rise of supermassive black holes. A panchromatic search for faint, unobscured quasars at z 6 with COSMOS-Web and other surveys
  • Ultraviolet luminosity density of the universe during the epoch of reionization
  • Using Resolved Galaxies in Hubble Space Telescope Images to Measure Absolute Proper Motions
  • UV Continuum Slope and Dust Obscuration from z ~ 6 to z ~ 2: The Star Formation Rate Density at High Redshift
  • UV Luminosity Functions at z~4, 5, and 6 from the Hubble Ultra Deep Field and Other Deep Hubble Space Telescope ACS Fields: Evolution and Star Formation History
  • UV surface brightness of galaxies from the local universe to z ~ 5
  • Weighing El Gordo with a Precision Scale: Hubble Space Telescope Weak-lensing Analysis of the Merging Galaxy Cluster ACT-CL J0102-4915 at z = 0.87
  • Weighing simulated galaxy clusters using lensing and X-ray
  • Wide-field Hubble Space Telescope Observations of the Globular Cluster System in NGC 1399
  • z ~ 7-10 Galaxies in the HUDF and GOODS Fields: UV Luminosity Functions
  • z ~ 7 Galaxy Candidates from NICMOS Observations Over the HDF-South and the CDF-South and HDF-North Goods Fields
Instrument ACS, ACS/HRC, ACS/WFC
Temporal Coverage 2003-09-24T08:34:14Z/2004-01-15T07:57:48Z
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 2004-03-16T00:00:00Z
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, Beckwith comma Steven, 2004, 'The Ultra Deep Field with ACS', 1.0, European Space Agency, https://doi.org/10.5270/esa-501qmxy