A dataset provided by the European Space Agency

Name 10086
Title The Ultra Deep Field with ACS
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=10086;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-r9gntsi
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=10086&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
  • Active and Passive Galaxies at z ~ 2: Rest-frame Optical Morphologies with WFC3
  • A faint red stellar halo around an edge-on disc galaxy in the Hubble Ultra Deep Field
  • A KS and IRAC Selection of High-redshift Extremely Red Objects
  • A measurement of the faint source correlation function in the GOODS and UDF surveys
  • 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
  • An infrared view of the coevolution of massive blackholes and galaxies
  • 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 robust sample of galaxies at redshifts 6.0<z<8.7: stellar populations, star formation rates and stellar masses
  • 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
  • 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
  • Candels: The Evolution of Galaxy Rest-frame Ultraviolet Colors from z = 8 to 4
  • Central Blue Clumps in Elliptical Galaxies of the Hubble 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
  • Clues to galaxy evolution from the major merger rate at high redshift
  • 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
  • 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
  • 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
  • Diffuse light in the young cluster of galaxies CL J1449+0856 at z = 2.07
  • Discovery of a Very Large (20 kpc) Galaxy at z = 3.72
  • Disc scalelengths out to redshift 5.8
  • Edge-on Galaxies in the Hubble Ultra Deep Field
  • Empirical Predictions for (Sub-)millimeter Line and Continuum Deep Fields
  • Euclid preparation. IV. Impact of undetected galaxies on weak-lensing shear measurements
  • Evidence for a Massive Poststarburst Galaxy at z~6.5
  • Evidence for TP-AGB Stars in High-Redshift Galaxies, and Their Effect on Deriving Stellar Population Parameters
  • 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 UV LF from z 15 to z 8 using new JWST NIRCam medium-band observations over the HUDF/XDF
  • 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
  • First gas-phase metallicity gradients of 0.1 z 0.8 galaxies with MUSE
  • Flexion measurement in simulations of Hubble Space Telescope data
  • 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 Morphologies in the Hubble Ultra Deep Field: Dominance of Linear Structures at the Detection Limit
  • High-Redshift Extremely Red Objects in the Hubble Space Telescope Ultra Deep Field Revealed by the GOODS Infrared Array Camera Observations
  • HOLISMOKES. VI. New galaxy-scale strong lens candidates from the HSC-SSP imaging survey
  • 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
  • Inferred galaxy properties during Cosmic Dawn from early JWST photometry results
  • Lensed arc statistics: comparison of Millennium simulation galaxy clusters to Hubble Space Telescope observations of an X-ray selected sample
  • 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
  • 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?
  • Massive Clumps in Local Galaxies: Comparisons with High-redshift Clumps
  • Measuring Sizes of Ultra-faint Dwarf Galaxies
  • Measuring the Average Molecular Gas Content of Star-forming Galaxies 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
  • Modelling and interpreting spectral energy distributions of galaxies with BEAGLE
  • 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
  • MUSE Spectroscopic Identifications of Ultra-faint Emission Line Galaxies with M UV ~ -15
  • 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
  • No evidence for Lyman a emission in spectroscopy of z > 7 candidate galaxies
  • No Overdensity of Lyman-Alpha Emitting Galaxies around a Quasar at z ~ 5.7
  • Observations of Thick Disks in the Hubble Space Telescope Ultra Deep Field
  • On the characteristics of tidal structures of interacting galaxies
  • On the Origin of Exponential Disks at High Redshift
  • On the Stellar Masses of Giant Clumps in Distant Star-forming Galaxies
  • Optimising and comparing source-extraction tools using objective segmentation quality criteria
  • 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
  • Properties of galaxies reproduced by a hydrodynamic simulation
  • Resolved Galaxies in the Hubble Ultra Deep Field: Star Formation in Disks at High Redshift
  • 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 Deep Hubble Images with Semi-empirical Models of Galaxy Formation
  • Sizes of LYa-emitting Galaxies and Their Rest-frame Ultraviolet Components at z = 3.1
  • 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 History of the Hubble Ultra Deep Field: Comparison with the Hubble Deep Field-North
  • Star-forming galaxies at z 8-9 from Hubble Space Telescope/WFC3: implications for reionization
  • Stars in the Hubble Ultra Deep Field
  • Statistics of interacting galaxies at z ~ 0.7
  • 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
  • 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 ALMA Spectroscopic Survey Large Program: The Infrared Excess of z = 1.5-10 UV-selected Galaxies and the Implied High-redshift Star Formation History
  • The analysis of effective galaxies number count for Chinese Space Station Optical Survey (CSS-OS) by image simulation
  • The Bivariate Size-Luminosity Relations for Lyman Break Galaxies at z ~ 4-5
  • The colour distribution of galaxies at redshift five
  • The contribution of faint Lyman-a emitters to extended Lyman-a halos constrained by MUSE clustering measurements
  • 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 Environments of High-Redshift Quasi-Stellar Objects
  • The Evolution of Mass-Size Relation for Lyman Break Galaxies from z = 1 to z = 7
  • 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 Function During the Reionization Epoch
  • The galaxy luminosity-size relation and selection biases in the Hubble Ultra Deep Field
  • 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 mean Ha EW and Lyman-continuum photon production efficiency for faint z 4-5 galaxies
  • The Morphological Diversities among Star-forming Galaxies at High Redshifts in the Great Observatories Origins Deep Survey
  • The MUSE eXtremely deep field: first panoramic view of an Mg II emitting intragroup medium
  • The MUSE eXtremely Deep Field: Individual detections of Lya haloes around rest-frame UV-selected galaxies at z 2.9-4.4
  • The MUSE Hubble Ultra Deep Field Survey. III. Testing photometric redshifts to 30th magnitude
  • The MUSE Hubble Ultra Deep Field Survey. II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies
  • 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. XIII. Spatially resolved spectral properties of Lyman a haloes around star-forming galaxies at z > 3
  • The MUSE Hubble Ultra Deep Field Survey. XII. Mg II emission and absorption in star-forming galaxies
  • 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 Rest-frame Ultraviolet Light Profile Shapes of Lya-emitting Galaxies at z = 3.1
  • The star formation rate of the Universe at z~ 6 from the Hubble Ultra-Deep Field
  • The Structure and Star Formation History of Early-Type Galaxies in the Ultra Deep Field/GRAPES Survey
  • The structures of distant galaxies - I. Galaxy structures and the merger rate to z ~ 3 in the Hubble Ultra-Deep Field
  • The tumultuous formation of the Hubble sequence at z > 1 examined with HST/Wide-Field Camera-3 observations of the Hubble Ultra Deep Field
  • 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
  • Toward Precision LSST Weak-Lensing Measurement. I. Impacts of Atmospheric Turbulence and Optical Aberration
  • Towards an understanding of dark matter: Precise gravitational lensing analysis complemented by robust photometric redshifts
  • 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
  • Ultradeep IRAC Imaging Over the HUDF and GOODS-South: Survey Design and Imaging Data Release
  • Ultraviolet luminosity density of the universe during the epoch of reionization
  • UV surface brightness of galaxies from the local universe to z ~ 5
  • UVUDF: Ultraviolet Through Near-infrared Catalog and Photometric Redshifts of Galaxies in the Hubble Ultra Deep Field
Instrument ACS, ACS/WFC
Temporal Coverage 2003-12-16T20:12:49Z/2004-01-02T22:28:58Z
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-r9gntsi