3D-HST Grism Spectroscopy of a Gravitationally Lensed, Low-metallicity Starburst Galaxy at z = 1.847
3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts, and Stellar Masses
A 7 deg2 survey for galaxy-scale gravitational lenses with the HST imaging archive
A CANDELS-3D-HST synergy: Resolved Star Formation Patterns at 0.7 < z < 1.5
A catalog of polychromatic bulge-disc decompositions of ~17.600 galaxies in CANDELS
A Close Look at Lya Emitters with JWST/NIRCam at z 3.1
Active Galactic Nuclei Selection and Demographics: A New Age with JWST/MIRI
A JWST investigation into the bar fraction at redshifts 1 <= z <= 3
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 Large Massive Quiescent Galaxy Sample at z ~ 1.2
An ALMA survey of the SCUBA-2 cosmology legacy survey UKIDSS/UDS field: Dust attenuation in high-redshift Lyman-break galaxies
An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: high-resolution dust continuum morphologies and the link between sub-millimetre galaxies and spheroid formation
An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: source catalogue and properties
Analysis of ~106 Spiral Galaxies from Four Telescopes Shows Large-Scale Patterns of Asymmetry in Galaxy Spin Directions
An Atlas of Color-selected Quiescent Galaxies at z > 3 in Public JWST Fields
A new derivation of the Hubble constant from g-ray attenuation using improved optical depths for the Fermi and CTA era
A new multifield determination of the galaxy luminosity function at z = 7-9 incorporating the 2012 Hubble Ultra-Deep Field imaging
Angular momentum of z ~ 1.5 galaxies and their local analogues with adaptive optics
An Ha Impression of Lya Galaxies at z 6 with Deep JWST/NIRCam Imaging
An observational determination of the evolving extragalactic background light from the multiwavelength HST/CANDELS survey in the Fermi and CTA era
An optimal ALMA image of the Hubble Ultra Deep Field in the era of JWST: obscured star formation and the cosmic far-infrared background
A Redshift-independent Efficiency Model: Star Formation and Stellar Masses in Dark Matter Halos at z 4
A remarkably high fraction of strong Lya emitters amongst luminous redshift 6.0 < z < 6.5 Lyman-break galaxies in the UKIDSS Ultra-Deep Survey
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
A unique distant submillimeter galaxy with an X-ray-obscured radio-luminous active galactic nucleus
Automated distant galaxy merger classifications from Space Telescope images using the Illustris simulation
Automatic identification of outliers in Hubble Space Telescope galaxy images
A Window on the Earliest Star Formation: Extreme Photoionization Conditions of a High-ionization, Low-metallicity Lensed Galaxy at z ~ 2*
Being KLEVER at cosmic noon: Ionized gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts
Bulge+disc decomposition of HFF and CANDELS galaxies: UVJ diagrams and stellar mass-size relations of galaxy components at 0.2 <= z <= 1.5
Bulge Growth and Quenching since z = 2.5 in CANDELS/3D-HST
CANDELS Multiwavelength Catalogs: Source Identification and Photometry in the CANDELS UKIDSS Ultra-deep Survey Field
CANDELS Observations of the Environmental Dependence of the Color-Mass-Morphology Relation at z = 1.6
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
Candels: The Evolution of Galaxy Rest-frame Ultraviolet Colors from z = 8 to 4
CANDELS: The Progenitors of Compact Quiescent Galaxies at z ~ 2
CANDELSz7: a large spectroscopic survey of CANDELS galaxies in the reionization epoch
Can intrinsic alignments of elongated low-mass galaxies be used to map the cosmic web at high redshift?
Caught in the Act: The Assembly of Massive Cluster Galaxies at z = 1.62
Cluster Cosmology Constraints from the 2500 deg2 SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope
Cluster mass calibration at high redshift: HST weak lensing analysis of 13 distant galaxy clusters from the South Pole Telescope Sunyaev-Zeldovich Survey
CMU DeepLens: deep learning for automatic image-based galaxy-galaxy strong lens finding
Compact star-forming galaxies preferentially quenched to become PSBs in z < 1 clusters
Comparison of Observed Galaxy Properties with Semianalytic Model Predictions Using Machine Learning
Conditions for galaxy quenching at 0.5 < z < 2.5 from CANDELS: compact cores and environment
Confirmation of Small Dynamical and Stellar Masses for Extreme Emission Line Galaxies at z ~ 2
Deep CO(1-0) Observations of z = 1.62 Cluster Galaxies with Substantial Molecular Gas Reservoirs and Normal Star Formation Efficiencies
Deep rest-frame far-UV spectroscopy of the giant Lyman a emitter `Himiko
Definitive upper bound on the negligible contribution of quasars to cosmic reionization
Delving deep: A population of extremely dusty dwarfs observed by JWST
Dependence of galaxy clustering on UV luminosity and stellar mass at z ~ 4-7
Detecting outliers in astronomical images with deep generative networks
Detecting the edges of galaxies with deep learning
Discovery of a Strong Lensing Galaxy Embedded in a Cluster at z = 1.62
Distinguishing Mergers and Disks in High-redshift Observations of Galaxy Kinematics
Does black hole growth depend fundamentally on host-galaxy compactness?
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 a correlation between the sizes of quiescent galaxies and local environment to z ~ 2
Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang
Evident black hole-bulge coevolution in the distant universe
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
Expanded Search for z ~ 10 Galaxies from HUDF09, ERS, and CANDELS Data: Evidence for Accelerated Evolution at z > 8?
Exploring AGN and star formation activity of massive galaxies at cosmic noon
Exploring the Gas-phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
Extending the evolution of the stellar mass-size relation at z <= 2 to low stellar mass galaxies from HFF and CANDELS
Extreme Emission-line Galaxies in CANDELS: Broadband-selected, Starbursting Dwarf Galaxies at z > 1
Extremely Low Molecular Gas Content in a Compact, Quiescent Galaxy at z = 1.522
Extremely Red Galaxies at z = 5-9 with MIRI and NIRSpec: Dusty Galaxies or Obscured Active Galactic Nuclei?
From Naked Spheroids to Disky Galaxies: How Do Massive Disk Galaxies Shape Their Morphology?
From peculiar morphologies to Hubble-type spirals: the relation between galaxy dynamics and morphology in star-forming galaxies at z ~ 1.5
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 Evolution in All Five CANDELS Fields and IllustrisTNG: Morphological, Structural, and the Major Merger Evolution to z 3
Galaxy Formation at z > 3 Revealed by Narrowband-selected O III Emission Line Galaxies
Galaxy Merger Rates up to z ~ 3 Using a Bayesian Deep Learning Model: A Major-merger Classifier Using IllustrisTNG Simulation Data
Galaxy Mergers up to z < 2.5. II. AGN Incidence in Merging Galaxies at Separations of 3-15 kpc
Galaxy Mergers up to Z < 2.5. I. The Star Formation Properties of Merging Galaxies at Separations of 3-15 kpc
Galaxy Quenching at the High Redshift Frontier: A Fundamental Test of Cosmological Models in the Early Universe with JWST-CEERS
Galaxy Sizes Since z = 2 from the Perspective of Stellar Mass Distribution within Galaxies
Galaxy Stellar Mass Functions from ZFOURGE/CANDELS: An Excess of Low-mass Galaxies since z = 2 and the Rapid Buildup of Quiescent Galaxies
Galaxy Structure and Mode of Star Formation in the SFR-Mass Plane from z ~ 2.5 to z ~ 0.1
Half-mass Radii for ~7000 Galaxies at 1.0 <= z <= 2.5: Most of the Evolution in the Mass-Size Relation Is Due to Color Gradients
High Equivalent Width of Ha+N II Emission in z 8 Lyman-break Galaxies from IRAC 5.8 mm Observations: Evidence for Efficient Lyman-continuum Photon Production in the Epoch of Reionization
How Robust are the Size Measurements of High-redshift Compact Galaxies?
HST/WFC3 Confirmation of the Inside-out Growth of Massive Galaxies at 0 < z < 2 and Identification of Their Star-forming Progenitors at z ~ 3
IDCS J1426.5+3508: Weak Lensing Analysis of a Massive Galaxy Cluster at z = 1.75
Identification and characterization of six spectroscopically confirmed massive protostructures at 2.5 < z < 4.5
Identifying Lya emitter candidates with Random Forest: Learning from galaxies in the CANDELS survey
Implications of Increased Central Mass Surface Densities for the Quenching of Low-mass Galaxies
Improved photometric redshifts with colour-constrained galaxy templates for future wide-area surveys
Inference of the cosmic rest-frame from supernovae Ia
Internal Structure of Molecular Gas in a Main-sequence Galaxy With a UV Clump at z = 1.45
Investigating the Effect of Galaxy Interactions on Star Formation at 0.5 < z < 3.0
Investigating the Effect of Galaxy Interactions on the Enhancement of Active Galactic Nuclei at 0.5 < z < 3.0
Ionized gas kinematics and chemical abundances of low-mass star-forming galaxies at z ~ 3
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
JWSTs PEARLS: A JWST/NIRCam View of ALMA Sources
Large-scale Structures in the CANDELS Fields: The Role of the Environment in Star Formation Activity
Linking galaxy structural properties and star formation activity to black hole activity with IllustrisTNG
Local Analogs to High-redshift Galaxies. I. Characterization of Dust Emission and Star Formation History
Lower-luminosity Galaxies Could Reionize the Universe: Very Steep Faint-end Slopes to the UV Luminosity Functions at z >= 5-8 from the HUDF09 WFC3/IR Observations
Mass assembly history of dark matter haloes in the light of H0 tension
Massive post-starburst galaxies at z > 1 are compact proto-spheroids
Mass-metallicity relation and fundamental metallicity relation at z 2
Metal-enriched galactic outflows shape the mass-metallicity relationship
Millimeter Mapping at z ~ 1: Dust-obscured Bulge Building and Disk Growth
Mock light-cones and theory friendly catalogues for the CANDELS survey
Morpheus: A Deep Learning Framework for the Pixel-level Analysis of Astronomical Image Data
Morphologies of ~190,000 Galaxies at z = 0-10 Revealed with HST Legacy Data. III. Continuum Profile and Size Evolution of Lya Emitters
Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology
Nature versus nurture: what regulates star formation in satellite galaxies?
Near infrared spectroscopy and star-formation histories of 3 <= z <= 4 quiescent galaxies
Near-IR Weak-lensing (NIRWL) Measurements in the CANDELS Fields. I. Point-spread Function Modeling and Systematics
New empirical constraints on the cosmological evolution of gas and stars in galaxies
New image statistics for detecting disturbed galaxy morphologies at high redshift
New technique to select recent fast-quenching galaxies at z 2 using the optical colours
Nonparametric Star Formation History Reconstruction with Gaussian Processes. I. Counting Major Episodes of Star Formation
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
Observations contradict galaxy size and surface brightness predictions that are based on the expanding universe hypothesis
Observations of Environmental Quenching in Groups in the 11 GYR since z = 2.5: Different Quenching for Central and Satellite Galaxies
Observations of the initial formation and evolution of spiral galaxies at 1 < z < 3 in the CANDELS fields
Optical-faint, Far-infrared-bright Herschel Sources in the CANDELS Fields: Ultra-luminous Infrared Galaxies at z > 1 and the Effect of Source Blending
PdBI Cold Dust Imaging of Two Extremely Red H - 4.5 > 4 Galaxies Discovered with SEDS and CANDELS
Photometric Redshift Calibration Requirements for WFIRST Weak-lensing Cosmology: Predictions from CANDELS
Photometry of high-redshift blended galaxies using deep learning
Probabilistic model for dynamic galaxy decomposition
Probing the Star Formation Main Sequence Down to 108 M at 1.0 < z < 3.0
Quantifying Non-parametric Structure of High-redshift Galaxies with Deep Learning
Quenching and morphological transformation in semi-analytic models and CANDELS
Quenching as a Contest between Galaxy Halos and Their Central Black Holes
Reconstructing the Assembly of Massive Galaxies. II. Galaxies Develop Massive and Dense Stellar Cores as They Evolve and Head toward Quiescence at Cosmic Noon
Red and dead CANDELS: massive passive galaxies at the dawn of the Universe
Rest-frame ultraviolet spectra of massive galaxies at z ~ 3: evidence of high-velocity outflows
Revealing the formation histories of the first stars with the cosmic near-infrared background
Revealing the Stellar Mass and Dust Distributions of Submillimeter Galaxies at Redshift 2
Searching for Islands of Reionization: A Potential Ionized Bubble Powered by a Spectroscopic Overdensity at z = 8.7
Selection of Massive Evolved Galaxies at 3 <= z <= 4.5 in the CANDELS Fields
SIMBA: Cosmological simulations with black hole growth and feedback
Simulations of the WFIRST Supernova Survey and Forecasts of Cosmological Constraints
Size-Stellar Mass Relation and Morphology of Quiescent Galaxies at z >= 3 in Public JWST Fields
Space Densities and Emissivities of Active Galactic Nuclei at z > 4
Spatially Resolved Properties of Galaxies from CANDELS+MUSE: Radial Extinction Profile and Insights on Quenching
Spatially resolved star formation and inside-out quenching in the TNG50 simulation and 3D-HST observations
Spectroscopic Confirmation of the Rich z = 1.80 Galaxy Cluster JKCS 041 using the WFC3 Grism: Environmental Trends in the Ages and Structure of Quiescent Galaxies
Stellar, Gas, and Dust Emission of Star-forming Galaxies out to z ~ 2
Stellar Populations of Lya-emitting Galaxies in the HETDEX Survey. I. An Analysis of LAEs in the GOODS-N Field
Strong size evolution of disc galaxies since z = 1. Readdressing galaxy growth using a physically motivated size indicator
Structural analysis of massive galaxies using HST deep imaging at z < 0.5
Structural Evolution of Early-type Galaxies to z = 2.5 in CANDELS
Structural Parameters of Galaxies in CANDELS
Subkiloparsec Imaging of Lya Emission in a Low-mass, Highly Ionized, Gravitationally Lensed Galaxy at z = 1.84
Sunyaev-Zeldovich effect and X-ray scaling relations from weak lensing mass calibration of 32 South Pole Telescope selected galaxy clusters
Supermassive black holes at high redshift are expected to be obscured by their massive host galaxies interstellar medium
Testing the accuracy of 3D-HST photometric redshift estimates as reference samples for deep weak lensing studies
The abundance of massive compact galaxies at 1.0 < z < 3.0 in 3D-HST/CANDELS
The ages, masses and star formation rates of spectroscopically confirmed z ~ 6 galaxies in CANDELS
The Ages of Passive Galaxies in a z = 1.62 Protocluster
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 ASTRODEEP-GS43 catalogue: New photometry and redshifts for the CANDELS GOODS-South field
The building up of observed stellar scaling relations of massive galaxies and the connection to black hole growth in the TNG50 simulation
The Carnegie-Irvine Galaxy Survey. VI. Quantifying Spiral Structure
The clustering properties of high-redshift passive galaxies
The connection between mergers and AGN activity in simulated and observed massive galaxies
The connection between stellar mass, age, and quenching time-scale in massive quiescent galaxies at z 1
The Dearth of z ~ 10 Galaxies in All HST Legacy Fields--The Rapid Evolution of the Galaxy Population in the First 500 Myr
The Discovery of the Most Distant Known Type Ia Supernova at Redshift 1.914
The Dwarfs beyond: The Stellar-to-halo Mass Relation for a New Sample of Intermediate Redshift Low-mass Galaxies
The Effect of the Morphological Quenching Mechanism on Star Formation Activity at 0.5 < z < 1.5 in 3D-HST/CANDELS
The evolution of gas-phase metallicity and resolved abundances in star-forming galaxies at z 0.6-1.8
The evolution of the galaxy stellar-mass function over the last 12 billion years from a combination of ground-based and HST surveys
The Far-infrared Emission of the First Massive Galaxies
The GOGREEN survey: constraining the satellite quenching time-scale in massive clusters at z 1
The GOGREEN Survey: Evidence of an Excess of Quiescent Disks in Clusters at 1.0
The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) Survey Design, Reductions, and Detections
The impact of black hole scaling relation assumptions on the mass density of black holes
The Impact of Inclination-dependent Attenuation on Ultraviolet Star Formation Rate Tracers
The impact of satellite trails on Hubble Space Telescope observations
The KMOS3D Survey: Data Release and Final Survey Paper
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 Dependence of Structure, Star Formation Rate, and Mass Assembly Mode at 0.5 < z < 2.5
The mass-metallicity relation at z ~ 1.4 revealed with Subaru/FMOS
The mass-metallicity-star formation rate relation at z 2 with 3D Hubble Space Telescope
The merger rates and sizes of galaxies across the peak epoch of star formation from the HiZELS survey
The missing light of the Hubble Ultra Deep Field
The morphologies of massive galaxies at 1 < z < 3 in the CANDELS-UDS field: compact bulges, and the rise and fall of massive discs
The Morphologies of Massive Galaxies at 1<z<3 in the CANDELS-UDS Field: Compact Bulges, and the Rise and Fall of Massive Disks
The Morphology-Density Relationship in 1 < z < 2 Clusters
The MOSDEF survey: a comprehensive analysis of the rest-optical emission-line properties of z ~ 2.3 star-forming galaxies
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: Environmental Dependence of the Gas-phase Metallicity of Galaxies at 1.4 <= z <= 2.6
The MOSDEF survey: probing resolved stellar populations at z 2 Using a new bayesian-defined morphology metric called patchiness
The MOSDEF survey: the dependence of H a-to-UV SFR ratios on SFR and size at z 2
The MOSDEF survey: the mass-metallicity relationship and the existence of the FMR at z 1.5
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 MUSE Hubble Ultra Deep Field Survey. XII. Mg II emission and absorption in star-forming galaxies
The Nature of Extremely Red H - 4.5 > 4 Galaxies Revealed with SEDS and CANDELS
The Nature of Ha-selected Galaxies at z > 2. II. Clumpy Galaxies and Compact Star-forming Galaxies
The nature of sub-millimetre galaxies II: an ALMA comparison of SMG dust heating mechanisms
The O IIIl5007 equivalent width distribution at z 2: the redshift evolution of the extreme emission line galaxies
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 progenitors of the first red sequence galaxies at z ~ 2
The redshift and mass dependence on the formation of the Hubble sequence at z > 1 from CANDELS/UDS
The Redshift Evolution of Rest-UV Spectroscopic Properties in Lyman-break Galaxies at z ~ 2-4
The relationship between dust and C I at z = 1 and beyond
The role of gas kinematics in setting metallicity gradients at high redshift
The SCUBA-2 Cosmology Legacy Survey: demographics of the 450-mm population
The size and pervasiveness of Ly a-UV spatial offsets in star-forming galaxies at z ~ 6
The size-luminosity relation at z = 7 in CANDELS and its implication on reionization
The sizes, masses and specific star formation rates of massive galaxies at 1.3 < z < 1.5: strong evidence in favour of evolution via minor mergers
The star formation history and the nature of the mass-metallicity relation of passive galaxies at 1.0 < z < 1.4 from VANDELS
The Star Formation Rate-Radius Connection: Data and Implications for Wind Strength and Halo Concentration
The Stellar Mass Function in CANDELS and Frontier Fields: The Buildup of Low-mass Passive Galaxies since z 3
The Structural Evolution of Milky-Way-like Star-forming Galaxies since z ~ 1.3
The structural properties of classical bulges and discs from z ~ 2
The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10
The unexpectedly large dust and gas content of quiescent galaxies at z > 1.4
The UV spectral slope b and stellar population of most active star-forming galaxies at z ~ 4
The VANDELS ESO public spectroscopic survey. Final data release of 2087 spectra and spectroscopic measurements
The VANDELS survey: The relation between the UV continuum slope and stellar metallicity in star-forming galaxies at z ~ 3
The VANDELS survey: the role of ISM and galaxy physical properties in the escape of Lya emission in z ~ 3.5 star-forming galaxies
Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 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
Ultrafaint C II Emission in a Redshift = 2 Gravitationally Lensed Metal-poor Dwarf Galaxy
UNIVERSEMACHINE: The correlation between galaxy growth and dark matter halo assembly from z = 0-10
UVI colour gradients of 0.4 < z < 1.4 star-forming main-sequence galaxies in CANDELS: dust extinction and star formation profiles
What is the Physical Origin of Strong Lya Emission? I. Demographics of Lya Emitter Structures
When VLT Meets HST: The HUGS Survey
X-UDS: The Chandra Legacy Survey of the UKIDSS Ultra Deep Survey Field
ZFIRE: Measuring Electron Density with O II as a Function of Environment at z = 1.62
ZFOURGE: Using Composite Spectral Energy Distributions to Characterize Galaxy Populations at 1 < z < 4
SSFR-M * Diagram: A Valuable Galaxy Evolution Diagnostic to Complement (s)SFR-M * Diagrams
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2010-11-08T02:52:12Z/2011-01-10T02:47:12Z
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., 2011, 'Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey -- UDS Field', 1.0, European Space Agency, https://doi.org/10.5270/esa-npg08q3
