A dataset provided by the European Space Agency

Name 12498
Title Did Galaxies Reionize the Universe?
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12498;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-luqtag8
Author Ellis, Richard S.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=12498&mission=hst
Publication
  • A bottom-up search for Lyman-continuum leakage in the Hubble Ultra Deep Field
  • Accurate PSF-matched photometry and photometric redshifts for the extreme deep field with the Chebyshev-Fourier functions
  • A Comparison of the Stellar, CO, and Dust-continuum Emission from Three Star-forming HUDF Galaxies at z ~ 2
  • A deep ALMA image of the Hubble Ultra Deep Field
  • A Deep ALMA Image of the Hubble Ultra Deep Field
  • A joint measurement of galaxy luminosity functions and large-scale field densities during the Epoch of Reionization
  • A Large Population of Faint 8 < z < 16 Galaxies Found in the First JWST NIRCam Observations of the NGDEEP Survey
  • ALMA 200 pc Resolution Imaging of Smooth Cold Dusty Disks in Typical z ~ 3 Star-forming Galaxies
  • 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
  • ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Survey Description
  • ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-Selected z = 2-10 Galaxies as a Function of UV-Continuum Slope and Stellar Mass
  • A Multiwavelength Study of Tadpole Galaxies in the Hubble Ultra Deep Field
  • 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
  • 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 Very Compact Dense Galaxy Overdensity with d 130 Identified at z ~ 8: Implications for Early Protocluster and Cluster Core Formation
  • Brown Dwarf Candidates in the JADES and CEERS Extragalactic Surveys
  • 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
  • Constraining the cosmic UV background at z > 3 with MUSE Lyman-a emission observations
  • Dust attenuation in 2 < z < 3 star-forming galaxies from deep ALMA observations of the Hubble Ultra Deep Field
  • ETHOS - an effective theory of structure formation: predictions for the high-redshift Universe - abundance of galaxies and reionization
  • Evidence for Reduced Specific Star Formation Rates in the Centers of Massive Galaxies at z = 4
  • Evolution of Intrinsic Scatter in the SFR-Stellar Mass Correlation at 0.5 < z < 3
  • 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
  • FIGS--Faint Infrared Grism Survey: Description and Data Reduction
  • First constraints on small-scale non-Gaussianity from UV galaxy luminosity functions
  • First gas-phase metallicity gradients of 0.1 z 0.8 galaxies with MUSE
  • First light and reionization epoch simulations (FLARES) X III: the lyman-continuum emission of high-redshift galaxies
  • Galaxy clustering measurements out to redshift z ~ 8 from Hubble Legacy Fields
  • Galaxy luminosity function pipeline for cosmology and astrophysics
  • Galaxy Stellar Mass Functions from z 10 to z 6 using the Deepest Spitzer/Infrared Array Camera Data: No Significant Evolution in the Stellar-to-halo Mass Ratio of Galaxies in the First Gigayear of Cosmic Time
  • High-precision Photometric Redshifts from Spitzer/IRAC: Extreme 3.6 - 4.5 Colors Identify Galaxies in the Redshift Range z ~ 6.6 - 6.9
  • JWST and ALMA Imaging of Dust-obscured, Massive Substructures in a Typical z 3 Star-forming Disk Galaxy
  • Keck-I MOSFIRE Spectroscopy of the z ~ 12 Candidate Galaxy UDFj-39546284
  • 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
  • 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
  • Morphologies of ~190,000 Galaxies at z = 0-10 Revealed with HST Legacy Data. II. Evolution of Clumpy Galaxies
  • Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology
  • Moving Objects in the Hubble Ultra Deep Field
  • Nature and Nurture? Comparing Lya Detections in UV-bright and Fainter O III+Hb Emitters at z 8 with Keck/MOSFIRE
  • Near-IR Weak-lensing (NIRWL) Measurements in the CANDELS Fields. I. Point-spread Function Modeling and Systematics
  • New Constraints on Cosmic Reionization from the 2012 Hubble Ultra Deep Field Campaign
  • 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
  • Non-parametric analysis of the rest-frame UV sizes and morphological disturbance amongst L* galaxies at 4 < z < 8
  • Photometric Constraints on the Redshift of z ~ 10 Candidate UDFj-39546284 from Deeper WFC3/IR+ACS+IRAC Observations over the HUDF
  • Physical Properties of Sub-galactic Clumps at 0.5 <= Z <= 1.5 in the UVUDF
  • Probing the Dawn of Galaxies at z ~ 9-12: New Constraints from HUDF12/XDF and CANDELS data
  • Properties of galaxies reproduced by a hydrodynamic simulation
  • Real or Interloper? The Redshift Likelihoods of z > 8 Galaxies in the HUDF12
  • 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
  • Sunyaev-Zeldovich effect and X-ray scaling relations from weak lensing mass calibration of 32 South Pole Telescope selected galaxy clusters
  • Testing models of quasar hosts with strong gravitational lensing by quasar hosts
  • The 2012 Hubble Ultra Deep Field (UDF12): Observational Overview
  • The Abundance of Star-forming Galaxies in the Redshift Range 8.5-12: New Results from the 2012 Hubble Ultra Deep Field Campaign
  • 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: Continuum Number Counts, Resolved 1.2 mm Extragalactic Background, and Properties of the Faintest Dusty Star-forming Galaxies
  • The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Evolution of the Molecular Gas in CO-selected Galaxies
  • The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Search for CII Line and Dust Emission in 6
  • The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Nature of the Faintest Dusty Star-forming Galaxies
  • 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 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 cosmic assembly of stellar haloes in massive early-type Galaxies
  • 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 Evolution of Galaxy Number Density at z < 8 and Its Implications
  • 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 Fate of a Red Nugget: In Situ Star Formation of Satellites around a Massive Compact Galaxy
  • The Galaxy Starburst/Main-sequence Bimodality over Five Decades in Stellar Mass at z 3-6.5
  • The galaxy UV luminosity function at z 2-4; new results on faint-end slope and the evolution of luminosity density
  • 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 Ha Luminosity Function of Galaxies at z 4.5
  • The impact of satellite trails on Hubble Space Telescope observations
  • The ionizing photon production efficiency at z 6 for Lyman-alpha emitters using JEMS and MUSE
  • 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 missing light of the Hubble Ultra Deep Field
  • 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 Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies at z 1
  • The MUSE eXtremely deep field: first panoramic view of an Mg II emitting intragroup medium
  • 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. I. Survey description, data reduction, and source detection
  • 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. 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 MUSE Hubble Ultra Deep Field Survey. XIV. Evolution of the Lya emitter fraction from z = 3 to z = 6
  • The MUSE Hubble Ultra Deep Field Survey. X. Lya equivalent widths at 2.9 < z < 6.6
  • The Next Generation Deep Extragalactic Exploratory Public (NGDEEP) Survey
  • The Role of Bulge Formation in the Homogenization of Stellar Populations at z~2 as revealed by Internal Color Dispersion in CANDELS
  • The systematic search for z 5 active galactic nuclei in the Chandra Deep Field South
  • 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 continua and inferred stellar populations of galaxies at z 7-9 revealed by the Hubble Ultra-Deep Field 2012 campaign
  • 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 VANDELS survey: dust attenuation in star-forming galaxies at z = 3-4
  • 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
  • UV-continuum Slopes of >4000 z ~ 4-8 Galaxies from the HUDF/XDF, HUDF09, ERS, CANDELS-South, and CANDELS-North Fields
  • UV Luminosity Functions at Redshifts z ~ 4 to z ~ 10: 10,000 Galaxies from HST Legacy Fields
  • UVUDF: Ultraviolet Imaging of the Hubble Ultra Deep Field with Wide-Field Camera 3
  • UVUDF: Ultraviolet Through Near-infrared Catalog and Photometric Redshifts of Galaxies in the Hubble Ultra Deep Field
  • UVUDF: UV Luminosity Functions at the Cosmic High Noon
  • VLT/XSHOOTER and Subaru/MOIRCS spectroscopy of HUDF.YD3: no evidence for Lyman a emission at z = 8.55
  • 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 2012-08-04T20:06:02Z/2012-09-16T17:50:43Z
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 2012-12-16T22:14:35Z
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, Ellis comma Richard S., 2012, 'Did Galaxies Reionize the Universe?', 1.0, European Space Agency, https://doi.org/10.5270/esa-luqtag8