3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts, and Stellar Masses
ALMA Lensing Cluster Survey: Hubble Space Telescope and Spitzer Photometry of 33 Lensed Fields Built with CHArGE
ALMA Lensing Cluster Survey: Properties of Millimeter Galaxies Hosting X-Ray-detected Active Galactic Nuclei
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
An Exquisitely Deep View of Quenching Galaxies through the Gravitational Lens: Stellar Population, Morphology, and Ionized Gas
A quantitative assessment of completeness correction methods and public release of a versatile simulation code
A3COSMOS and A3GOODSS: Continuum source catalogues and multi-band number counts
Axion Decay and Anisotropy of Near-IR Extragalactic Background Light
Bright submillimeter galaxies do trace galaxy protoclusters
Brown Dwarf Candidates in the JADES and CEERS Extragalactic Surveys
CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z > 2
CLEAR: Emission-line Ratios at Cosmic High Noon
CLEAR: Spatially Resolved Emission Lines and Active Galactic Nuclei at 0.6 < z < 1.3
CLEAR: Survey Overview, Data Analysis, and Products
CLEAR: The Gas-phase Metallicity Gradients of Star-forming Galaxies at 0.6 < z < 2.6
Cosmic evolution of radio-excess active galactic nuclei in quiescent and star-forming galaxies across 0 < z < 4
COSMOS-DASH: The Evolution of the Galaxy Size-Mass Relation since z ~ 3 from New Wide-field WFC3 Imaging Combined with CANDELS/3D-HST
Delving deep: A population of extremely dusty dwarfs observed by JWST
Differential attenuation in star-forming galaxies at 0.3 z 1.5 in the SHARDS/CANDELS field
Early Growth of the Star Formation Rate Function in the Epoch of Reionization: An Approach with Rest-frame Optical Emissions
Euclid preparation. XXX. Performance assessment of the NISP red grism through spectroscopic simulations for the wide and deep surveys
Evolution of N/O abundance ratios and ionization parameters from z ~ 0 to 2 investigated by the direct temperature method*+
Exploring the Gas-phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
Galaxy cluster cores as seen with VLT/MUSE: New strong-lensing analyses of RX J2129.4 + 0009, MS 0451.6 - 0305, and MACS J2129.4 - 0741
HALO7D II: The Halo Velocity Ellipsoid and Velocity Anisotropy with Distant Main-sequence Stars
Insight from JWST/Near Infrared Camera into galaxy overdensities around bright Lyman-alpha emitters during reionization: implications for ionized bubbles at z 9
Learning Spectral Templates for Photometric Redshift Estimation from Broadband Photometry
Massive Dead Galaxies at z ~ 2 with HST Grism Spectroscopy. I. Star Formation Histories and Metallicity Enrichment
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
MIGHTEE: Multi-wavelength counterparts in the COSMOS field
Minor Merger Growth in Action: JWST Detects Faint Blue Companions around Massive Quiescent Galaxies at 0.5 <= z <= 3.0
Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology
Near-infrared Spectroscopy of Five Ultra-massive Galaxies at 1.7 < z < 2.7
Near-IR Weak-lensing (NIRWL) Measurements in the CANDELS Fields. I. Point-spread Function Modeling and Systematics
Probing the Dawn of Galaxies at z ~ 9-12: New Constraints from HUDF12/XDF and CANDELS data
Robust identification of active galactic nuclei through HST optical variability in GOODS-S: comparison with the X-ray and mid-IR-selected samples
Spatially resolved star formation and inside-out quenching in the TNG50 simulation and 3D-HST observations
Sunyaev-Zeldovich effect and X-ray scaling relations from weak lensing mass calibration of 32 South Pole Telescope selected galaxy clusters
The 3D-HST Survey: Hubble Space Telescope WFC3/G141 Grism Spectra, Redshifts, and Emission Line Measurements for ~ 100,000 Galaxies
The ALMA-ALPAKA survey. I. High-resolution CO and CI kinematics of star-forming galaxies at z = 0.5-3.5
The CANDELS/SHARDS Multiwavelength Catalog in GOODS-N: Photometry, Photometric Redshifts, Stellar Masses, Emission-line Fluxes, and Star Formation Rates
The Cosmos in Its Infancy: JADES Galaxy Candidates at z > 8 in GOODS-S and GOODS-N
The faint end of the red sequence galaxy luminosity function: unveiling surface brightness selection effects with the CLASH clusters
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 MAGPI survey: evolution of radial trends in star formation activity across cosmic time
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 MOSDEF Survey: Electron Density and Ionization Parameter at z ~ 2.3
The Roles of Morphology and Environment on the Star Formation Rate-Stellar Mass Relation in COSMOS from 0 < z < 3.5
The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10
The VANDELS survey: a measurement of the average Lyman-continuum escape fraction of star-forming galaxies at z = 3.5
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
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2011-11-07T09:03:18Z/2012-09-27T08:32:11Z
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.
