A dataset provided by the European Space Agency

Name 12534
Title The Panchromatic Hubble Ultra Deep Field: Ultraviolet Coverage
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12534;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-tjgoq11
Author Teplitz, Harry
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=12534&mission=hst
Publication
  • A bottom-up search for Lyman-continuum leakage in the Hubble Ultra Deep Field
  • A joint measurement of galaxy luminosity functions and large-scale field densities during the Epoch of Reionization
  • A multiband map of the natural night sky brightness including Gaia and Hipparcos integrated starlight
  • A quantitative assessment of completeness correction methods and public release of a versatile simulation code
  • Axion Decay and Anisotropy of Near-IR Extragalactic Background Light
  • Bipolar outflows out to 10 kpc for massive galaxies at redshift z 1
  • Brown Dwarf Candidates in the JADES and CEERS Extragalactic Surveys
  • Calibration of weak-lensing shear in the Kilo-Degree Survey
  • 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
  • Constraints on the Lyman continuum escape fraction for faint star-forming galaxies
  • Discovery of a Very Large (20 kpc) Galaxy at z = 3.72
  • Evolution of Intrinsic Scatter in the SFR-Stellar Mass Correlation at 0.5 < z < 3
  • Evolution of the UV LF from z 15 to z 8 using new JWST NIRCam medium-band observations over the HUDF/XDF
  • First gas-phase metallicity gradients of 0.1 z 0.8 galaxies with MUSE
  • Galaxy clustering measurements out to redshift z ~ 8 from Hubble Legacy Fields
  • Galaxy luminosity function pipeline for cosmology and astrophysics
  • GAMA/DEVILS: constraining the cosmic star formation history from improved measurements of the 0.3-2.2 mm extragalactic background light
  • HDUV: The Hubble Deep UV Legacy Survey
  • Illuminating gas inflows/outflows in the MUSE deepest fields: Lya nebulae around forming galaxies at z 3.3
  • Limits on Lyman Continuum Escape from z = 2.2 Ha-emitting Galaxies
  • Linear: A Novel Algorithm for Reconstructing Slitless Spectroscopy from HST/WFC3
  • Lyman continuum leaker candidates at z ~ 3-4 in the HDUV based on a spectroscopic sample of MUSE LAEs
  • Measurements of Extragalactic Background Light from the Far UV to the Far IR from Deep Ground- and Space-based Galaxy Counts
  • 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
  • Millimeter Mapping at z ~ 1: Dust-obscured Bulge Building and Disk Growth
  • 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
  • Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology
  • MUSE Spectroscopic Identifications of Ultra-faint Emission Line Galaxies with M UV ~ -15
  • 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
  • Physical Properties of Sub-galactic Clumps at 0.5 <= Z <= 1.5 in the UVUDF
  • Robust identification of active galactic nuclei through HST optical variability in GOODS-S: comparison with the X-ray and mid-IR-selected samples
  • Simulating and interpreting deep observations in the Hubble Ultra Deep Field with the JWST/NIRSpec low-resolution `prism
  • Sunyaev-Zeldovich effect and X-ray scaling relations from weak lensing mass calibration of 32 South Pole Telescope selected galaxy clusters
  • Testing the accuracy of 3D-HST photometric redshift estimates as reference samples for deep weak lensing studies
  • The abundance of z 10 galaxy candidates in the HUDF using deep JWST NIRCam medium-band imaging
  • The AstroSat UV deep field north: direct determination of the UV luminosity function and its evolution from z 0.8-0.4
  • 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 Dearth of z ~ 10 Galaxies in All HST Legacy Fields--The Rapid Evolution of the Galaxy Population in the First 500 Myr
  • The Fate of a Red Nugget: In Situ Star Formation of Satellites around a Massive Compact Galaxy
  • The HDUV Survey: Six Lyman Continuum Emitter Candidates at z ~ 2 Revealed by HST UV Imaging
  • The hidden side of cosmic star formation at z > 3. Bridging optically dark and Lyman-break galaxies with GOODS-ALMA
  • The Hubble Legacy Field GOODS-S Photometric Catalog
  • The impact of satellite trails on Hubble Space Telescope observations
  • The Lyman Continuum Escape Fraction of Emission Line-selected z ~ 2.5 Galaxies Is Less Than 15%
  • The Lyman Continuum Escape Fraction of Galaxies and AGN in the GOODS Fields
  • 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 Extremely Deep Field: The cosmic web in emission at high redshift
  • 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. VII. Fe II* emission in 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. XV. The mean rest-UV spectra of Lya emitters at z > 3
  • The Rest-frame Ultraviolet Structure of 0.5 < z < 1.5 Galaxies
  • The star formation burstiness and ionizing efficiency of low-mass galaxies
  • The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10
  • The UV Continuum of z > 1 Star-forming Galaxies in the Hubble Ultraviolet UltraDeep 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
  • 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
Instrument ACS, ACS/WFC, WFC3, WFC3/UVIS
Temporal Coverage 2012-03-02T00:19:36Z/2012-09-07T23:29:15Z
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 2012-09-08T02:43:31Z
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, Teplitz comma Harry, 2012, 'The Panchromatic Hubble Ultra Deep Field: Ultraviolet Coverage', 1.0, European Space Agency, https://doi.org/10.5270/esa-tjgoq11