3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts, and Stellar Masses
A Calibration of NICMOS Camera 2 for Low Count Rates
A CANDELS-3D-HST synergy: Resolved Star Formation Patterns at 0.7 < z < 1.5
Active Galactic Nuclei Selection and Demographics: A New Age with JWST/MIRI
A Duality in the Origin of Bulges and Spheroidal Galaxies
A dusty compact object bridging galaxies and quasars at cosmic dawn
A galaxy rapidly forming stars 700 million years after the Big Bang at redshift 7.51
A JWST/NIRSpec First Census of Broad-line AGNs at z = 4-7: Detection of 10 Faint AGNs with M BH 106-108 M and Their Host Galaxy Properties
A Lyman Break Galaxy in the Epoch of Reionization from Hubble Space Telescope Grism Spectroscopy
A Molecular Line Scan in the Hubble Deep Field North
A Molecular Line Scan in the Hubble Deep Field North: Constraints on the CO Luminosity Function and the Cosmic H2 Density
An enhanced merger fraction within the galaxy population of the SSA22 protocluster at z = 3.1
A new derivation of the Hubble constant from g-ray attenuation using improved optical depths for the Fermi and CTA era
A possible bright ultraviolet flash from a galaxy at redshift z 11
A possible large-scale alignment of galaxy spin directions - Analysis of 10 datasets from SDSS, Pan-STARRS, and HST
A Remarkably Luminous Galaxy at z=11.1 Measured with Hubble Space Telescope Grism Spectroscopy
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 Simulation-driven Deep Learning Approach for Separating Mergers and Star-forming Galaxies: The Formation Histories of Clumpy Galaxies in All of the CANDELS Fields
A3COSMOS and A3GOODSS: Continuum source catalogues and multi-band number counts
A surprising abundance of massive quiescent galaxies at 3 < z < 5 in the first data from JWST CEERS
Being KLEVER at cosmic noon: Ionized gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts
Bulge Growth and Quenching since z = 2.5 in CANDELS/3D-HST
CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey
CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey--The Hubble Space Telescope Observations, Imaging Data Products, and Mosaics
Constraining constant and tomographic coupled dark energy with low-redshift and high-redshift probes
Constraints on the galaxy `main sequence at z > 5: the stellar mass of HDF850.1
Contamination of Broadband Photometry by Nebular Emission in High-redshift Galaxies: Investigations with Kecks MOSFIRE Near-infrared Spectrograph
Deep JVLA Imaging of GOODS-N at 20 cm
Definitive upper bound on the negligible contribution of quasars to cosmic reionization
Delving deep: A population of extremely dusty dwarfs observed by JWST
Density perturbations for running vacuum: a successful approach to structure formation and to the s8-tension
Determining Cosmological-model-independent H 0 with Gravitationally Lensed Supernova Refsdal
Distinguishing Mergers and Disks in High-redshift Observations of Galaxy Kinematics
Dust Attenuation, Bulge Formation, and Inside-out Quenching of Star Formation in Star-forming Main Sequence Galaxies at z ~ 2
Dust attenuation, dust content, and geometry of star-forming galaxies
Evidence for GN-z11 as a luminous galaxy at redshift 10.957
Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang
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
Exploring the Gas-phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
Extremely Red Galaxies at z = 5-9 with MIRI and NIRSpec: Dusty Galaxies or Obscured Active Galactic Nuclei?
Galaxy build-up in the first 1.5 Gyr of cosmic history: insights from the stellar mass function at z 4-9 from JWST NIRCam observations
Galaxy Quenching at the High Redshift Frontier: A Fundamental Test of Cosmological Models in the Early Universe with JWST-CEERS
Galaxy spin direction distribution in HST and SDSS show similar large-scale asymmetry
Gamma-ray bursts, quasars, baryonic acoustic oscillations, and supernovae Ia: new statistical insights and cosmological constraints
Inference of the cosmic rest-frame from supernovae Ia
Investigating the Effect of Galaxy Interactions on Star Formation at 0.5 < z < 3.0
JWST PRIMER: a new multifield determination of the evolving galaxy UV luminosity function at redshifts z 9 - 15
JWST Sneaks a Peek at the Stellar Morphology of z 2 Submillimeter Galaxies: Bulge Formation at Cosmic Noon
Large-scale asymmetry in galaxy spin directions: Analysis of galaxies with spectra in DES, SDSS, and DESI Legacy Survey
Late-time acceleration due to a generic modification of gravity and the Hubble tension
Linking galaxy structural properties and star formation activity to black hole activity with IllustrisTNG
Mass assembly history of dark matter haloes in the light of H0 tension
MCSED: A Flexible Spectral Energy Distribution Fitting Code and Its Application to z ~ 2 Emission-line Galaxies
Model-independent test of the running Hubble constant from the Type Ia supernovae and the Hubble parameter data
Modelling and interpreting spectral energy distributions of galaxies with BEAGLE
Morphologies of ~190,000 Galaxies at z = 0-10 Revealed with HST Legacy Data. III. Continuum Profile and Size Evolution of Lya Emitters
Nature versus nurture: what regulates star formation in satellite galaxies?
Near-IR Weak-lensing (NIRWL) Measurements in the CANDELS Fields. I. Point-spread Function Modeling and Systematics
New technique to select recent fast-quenching galaxies at z 2 using the optical colours
NIHAO-UHD: the properties of MW-like stellar discs in high-resolution cosmological simulations
Nonparametric reconstruction of interaction in the cosmic dark sector
Obscured AGN enhancement in galaxy pairs at cosmic noon: evidence from a probabilistic treatment of photometric redshifts
Observational constraints on the deceleration parameter in a tilted universe
Observational Constraints on the Merger History of Galaxies since z 6: Probabilistic Galaxy Pair Counts in the CANDELS Fields
Observational constraints on the tilted flat-XCDM and the untilted nonflat XCDM dynamical dark energy inflation parameterizations
Observations of Environmental Quenching in Groups in the 11 GYR since z = 2.5: Different Quenching for Central and Satellite Galaxies
Optical-faint, Far-infrared-bright Herschel Sources in the CANDELS Fields: Ultra-luminous Infrared Galaxies at z > 1 and the Effect of Source Blending
Optically Faint Massive Balmer Break Galaxies at z > 3 in the CANDELS/GOODS Fields
Phantom dark energy as a natural selection of evolutionary processes a ^ la genetic algorithm and cosmological tensions
Photometric Redshift Calibration Requirements for WFIRST Weak-lensing Cosmology: Predictions from CANDELS
Potential signature of a quadrupolar hubble expansion in Pantheon+supernovae
Probing the Star Formation Main Sequence Down to 108 M at 1.0 < z < 3.0
Reconstructing the Assembly of Massive Galaxies. II. Galaxies Develop Massive and Dense Stellar Cores as They Evolve and Head toward Quiescence at Cosmic Noon
Reducing the Uncertainty on the Hubble Constant up to 35% with an Improved Statistical Analysis: Different Best-fit Likelihoods for Type Ia Supernovae, Baryon Acoustic Oscillations, Quasars, and Gamma-Ray Bursts
Simulations of the WFIRST Supernova Survey and Forecasts of Cosmological Constraints
SMA Observations on Faint Submillimeter Galaxies with S 850 < 2 mJy: Ultra Dusty Low-luminosity Galaxies at High Redshift
Spatially resolved star formation and inside-out quenching in the TNG50 simulation and 3D-HST observations
Spectral Energy Distribution Fitting of HETDEX Pilot Survey Lya Emitters in COSMOS and GOODS-N
Texas Spectroscopic Search for Lya Emission at the End of Reionization I. Constraining the Lya Equivalent-width Distribution at 6.0 < z < 7.0
The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Evolution of the Molecular Gas in CO-selected Galaxies
The ALPINE-ALMA CII survey. Dust mass budget in the early Universe
The ALPINE-ALMA C II survey. Luminosity function of serendipitous C II line emitters at z ~ 5
The ALPINE-ALMA CII survey. The contribution of major mergers to the galaxy mass assembly at z ~ 5
The Assembly of Milky-Way-like Galaxies Since z ~ 2.5
The ASTRODEEP-GS43 catalogue: New photometry and redshifts for the CANDELS GOODS-South field
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 Size and Morphology at z ~ 0.5-3.0 in the GOODS-N Region with Hubble Space Telescope/WFC3 Data
The evolution of the X-ray luminosity functions of unabsorbed and absorbed AGNs out to z~ 5
The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) Survey Design, Reductions, and Detections
The Impact of Inclination-dependent Attenuation on Ultraviolet Star Formation Rate Tracers
The impact of satellite trails on Hubble Space Telescope observations
The Magellan M2FS Spectroscopic Survey of High-redshift Galaxies: The Brightest Lyman-break Galaxies at z ~ 6
The MAGPI survey: evolution of radial trends in star formation activity across cosmic time
The mass-metallicity-star formation rate relation at z 2 with 3D Hubble Space Telescope
The missing light of the Hubble Ultra Deep Field
The MOSDEF Survey: AGN Multi-wavelength Identification, Selection Biases, and Host Galaxy Properties
The MOSDEF survey: an improved Voronoi binning technique on spatially resolved stellar populations at z ~ 2
The MOSDEF Survey: Dissecting the Star Formation Rate versus Stellar Mass Relation Using Ha and Hb Emission Lines at z ~ 2
The MOSDEF Survey: Electron Density and Ionization Parameter at z ~ 2.3
The MOSDEF survey: the dependence of H a-to-UV SFR ratios on SFR and size at z 2
The MOSDEF survey: towards a complete census of the z 2.3 star-forming galaxy population
The MOSFIRE Deep Evolution Field (MOSDEF) Survey: Rest-frame Optical Spectroscopy for ~1500 H-selected Galaxies at 1.37 < z < 3.8
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 O IIIl5007 equivalent width distribution at z 2: the redshift evolution of the extreme emission line galaxies
The Pantheon+ Analysis: Cosmological Constraints
The Pantheon+ Analysis: SuperCal-fragilistic Cross Calibration, Retrained SALT2 Light-curve Model, and Calibration Systematic Uncertainty
The Pantheon+ Analysis: The Full Data Set and Light-curve Release
The Physical Properties of Massive Green Valley Galaxies as a Function of Environments at 0.5 < z < 2.5 in 3D-HST/Candels Fields
The Stellar Mass Function in CANDELS and Frontier Fields: The Buildup of Low-mass Passive Galaxies since z 3
The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10
The UV spectral slope b and stellar population of most active star-forming galaxies at z ~ 4
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
TRINITY I: self-consistently modelling the dark matter halo-galaxy-supermassive black hole connection from z = 0-10
Two Massive, Compact, and Dust-obscured Candidate z 8 Galaxies Discovered by JWST
Two SNe Ia at Redshift ~2: Improved Classification and Redshift Determination with Medium-band Infrared Imaging
Type Ia Supernova Distances at Redshift >1.5 from the Hubble Space Telescope Multi-cycle Treasury Programs: The Early Expansion Rate
Type Ia Supernova Rate Measurements to Redshift 2.5 from CANDELS: Searching for Prompt Explosions in the Early Universe
Using 3D and 2D analysis for analyzing large-scale asymmetry in galaxy spin directions
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2012-03-30T05:18:40Z/2012-07-21T12:07:55Z
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.
European Space Agency, Faber comma Sandra M., 2012, 'Galaxy Assembly and the Evolution of Structure over the First Third of Cosmic Time - III', 1.0, European Space Agency, https://doi.org/10.5270/esa-7kxmp1k
