| Publication |
- A 7 deg2 survey for galaxy-scale gravitational lenses with the HST imaging archive
- 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
- A catalog of polychromatic bulge-disc decompositions of ~17.600 galaxies in CANDELS
- Accurate PSF-matched photometry and photometric redshifts for the extreme deep field with the Chebyshev-Fourier functions
- A comparative analysis of denoising algorithms for extragalactic imaging surveys
- A Critical Assessment of Photometric Redshift Methods: A CANDELS Investigation
- Active Galactic Nuclei Selection and Demographics: A New Age with JWST/MIRI
- Active Galactic Nucleus Feedback at z ~ 2 and the Mutual Evolution of Active and Inactive Galaxies
- A dominant population of optically invisible massive galaxies in the early Universe
- 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
- ALMA resolves turbulent, rotating CII emission in a young starburst galaxy at z = 4.8
- ALMA reveals a warm and compact starburst around a heavily obscured supermassive black hole at z = 4.75
- A magnetar-powered X-ray transient as the aftermath of a binary neutron-star merger
- A massive stellar bulge in a regularly rotating galaxy 1.2 billion years after the Big Bang
- A multiwavelength study of a massive, active galaxy at z ~ 2: coupling the kinematics of the ionized and molecular gas
- A Multiwavelength Study of Tadpole Galaxies in the Hubble Ultra Deep Field
- An ALMA view of 11 dusty star-forming galaxies at the peak of cosmic star formation history
- Analysis of ~106 Spiral Galaxies from Four Telescopes Shows Large-Scale Patterns of Asymmetry in Galaxy Spin Directions
- Analysis of the SFR-M* plane at z < 3: single fitting versus multi-Gaussian decomposition
- 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
- An observational determination of the evolving extragalactic background light from the multiwavelength HST/CANDELS survey in the Fermi and CTA era
- A possible large-scale alignment of galaxy spin directions - Analysis of 10 datasets from SDSS, Pan-STARRS, and HST
- A puzzling non-detection of O III and C II from a z 7.7 galaxy observed with ALMA
- A quantitative assessment of completeness correction methods and public release of a versatile simulation code
- 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
- A Spatially Resolved Study of Cold Dust, Molecular Gas, H II Regions, and Stars in the z = 2.12 Submillimeter Galaxy ALESS67.1
- A Submillimeter Perspective on the GOODS Fields (SUPER GOODS). III. A Large Sample of ALMA Sources in the GOODS-S
- A Submillimeter Perspective on the GOODS Fields (SUPER GOODS). IV. The Submillimeter Properties of X-Ray Sources in the CDF-S
- A Submillimeter Perspective on the GOODS Fields (SUPER GOODS). V. Deep 450 mm Imaging
- 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 Type Ia Supernova at Redshift 1.55 in Hubble Space Telescope Infrared Observations from CANDELS
- Axion Decay and Anisotropy of Near-IR Extragalactic Background Light
- Being KLEVER at cosmic noon: Ionized gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts
- Blue Rest-frame UV-optical Colors in z 8 Galaxies from GREATS: Very Young Stellar Populations at 650 Myr of Cosmic Time
- Brown Dwarf Candidates in the JADES and CEERS Extragalactic Surveys
- Bulge Growth and Quenching since z = 2.5 in CANDELS/3D-HST
- CANDELS Meets GSWLC: Evolution of the Relationship between Morphology and Star Formation Since z = 2
- CANDELS Multi-wavelength Catalogs: Source Detection and Photometry in the GOODS-South Field
- CANDELS Multiwavelength Catalogs: Source Identification and Photometry in the CANDELS UKIDSS Ultra-deep Survey Field
- CANDELS: The Contribution of the Observed Galaxy Population to Cosmic Reionization
- CANDELS: The Correlation between Galaxy Morphology and Star Formation Activity at z ~ 2
- 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 Progenitors of Compact Quiescent Galaxies at z ~ 2
- CLEAR. I. Ages and Metallicities of Quiescent Galaxies at 1.0 < z < 1.8 Derived from Deep Hubble Space Telescope Grism Data
- Clustering dependence on Lya luminosity from MUSE surveys at 3 < z < 6
- Combining ALMA with HST and VLT to Find the Counterparts of Submillimetre Galaxies
- 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
- CONGRUENTS (COsmic-ray, Neutrino, Gamma-ray and Radio Non-Thermal Spectra) - II. Population-level correlations between galactic infrared, radio, and g-ray emission
- Constraining constant and tomographic coupled dark energy with low-redshift and high-redshift probes
- Constraining the Assembly of Normal and Compact Passively Evolving Galaxies from Redshift z = 3 to the Present with CANDELS
- Constraining the bright-end of the UV luminosity function for z 7-9 galaxies: results from CANDELS/GOODS-South
- Constraints on the star-formation rate of z ~ 3 LBGs with measured metallicity in the CANDELS GOODS-South field
- Deblending Galaxies with Generative Adversarial Networks
- Deep Spitzer/IRAC Data for z 10 Galaxies Reveal Blue Balmer Break Colors: Young Stellar Populations at 500 Myr of Cosmic Time
- Definitive upper bound on the negligible contribution of quasars to cosmic reionization
- Delay Time Distributions of Type Ia Supernovae from Galaxy and Cosmic Star Formation Histories
- 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
- Detecting outliers in astronomical images with deep generative networks
- Detecting the edges of galaxies with deep learning
- Determining Cosmological-model-independent H 0 with Gravitationally Lensed Supernova Refsdal
- 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
- Early Growth of the Star Formation Rate Function in the Epoch of Reionization: An Approach with Rest-frame Optical Emissions
- Effect of galaxy mergers on star-formation rates
- Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang
- Evidence for two modes of black hole accretion in massive galaxies at z~2
- 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
- Evolution of the Sizes of Galaxies over 7 < z < 12 Revealed by the 2012 Hubble Ultra Deep Field Campaign
- Exploring the Gas-phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
- Extended Ha over compact far-infrared continuum in dusty submillimeter galaxies. Insights into dust distributions and star-formation rates at z ~ 2
- Extending the evolution of the stellar mass-size relation at z <= 2 to low stellar mass galaxies from HFF and CANDELS
- 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?
- First gas-phase metallicity gradients of 0.1 z 0.8 galaxies with MUSE
- FORECAST: A flexible software to forward model cosmological hydrodynamical simulations mimicking real observations
- Fraction of Clumpy Star-forming Galaxies at 0.5 <= z <= 3 in UVCANDELS: Dependence on Stellar Mass and Environment
- From Naked Spheroids to Disky Galaxies: How Do Massive Disk Galaxies Shape Their Morphology?
- 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 Inclination and the IRX-b Relation: Effects on UV Star Formation Rate Measurements at Intermediate to High Redshifts
- Galaxy Merger Rates up to z ~ 3 Using a Bayesian Deep Learning Model: A Major-merger Classifier Using IllustrisTNG Simulation Data
- Galaxy Morphology Network: A Convolutional Neural Network Used to Study Morphology and Quenching in ~100,000 SDSS and ~20,000 CANDELS Galaxies
- 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
- Galaxy Stellar Mass Functions from ZFOURGE/CANDELS: An Excess of Low-mass Galaxies since z = 2 and the Rapid Buildup of Quiescent Galaxies
- Gamma-ray bursts, quasars, baryonic acoustic oscillations, and supernovae Ia: new statistical insights and cosmological constraints
- GOODS-ALMA: 1.1 mm galaxy survey. I. Source catalog and optically dark galaxies
- GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies
- GOODS-ALMA: Optically dark ALMA galaxies shed light on a cluster in formation at z = 3.5
- GOODS-ALMA: The slow downfall of star formation in z = 2-3 massive galaxies
- GOODS-ALMA: Using IRAC and VLA to probe fainter millimeter galaxies
- HALO7D II: The Halo Velocity Ellipsoid and Velocity Anisotropy with Distant Main-sequence Stars
- 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?
- How the spectral energy distribution and galaxy morphology constrain each other, with application to morphological selection using galaxy colours
- HST Imaging of the Ionizing Radiation from a Star-forming Galaxy at z = 3.794
- 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
- Improved photometric redshifts with colour-constrained galaxy templates for future wide-area surveys
- Inference of the cosmic rest-frame from supernovae Ia
- Integral field spectroscopy of luminous infrared main-sequence galaxies at cosmic noon
- 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
- JEMS: A Deep Medium-band Imaging Survey in the Hubble Ultra Deep Field with JWST NIRCam and NIRISS
- JKCS 041: a Coma cluster progenitor at z = 1.803
- 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
- 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
- Keck Spectroscopy of Faint 3 < z < 7 Lyman Break Galaxies. III. The Mean Ultraviolet Spectrum at z ~= 4
- Large-scale asymmetry in galaxy spin directions: Analysis of galaxies with spectra in DES, SDSS, and DESI Legacy Survey
- Large-scale Structures in the CANDELS Fields: The Role of the Environment in Star Formation Activity
- 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
- Listening to galaxies tuning at z ~ 2.5-3.0: The first strikes of the Hubble fork
- Local Analogs to High-redshift Galaxies. I. Characterization of Dust Emission and Star Formation History
- Lower-luminosity Obscured AGN Host Galaxies Are Not Predominantly in Major-merging Systems at Cosmic Noon
- Luminous and High Stellar Mass Candidate Galaxies at z 8 Discovered in the Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey
- Mass assembly history of dark matter haloes in the light of H0 tension
- Measuring the Heating and Cooling of the Interstellar Medium at High Redshift: PAH and C II Observations of the Same Star-forming Galaxies at z ~ 2
- Metallicity evolution, metallicity gradients, and gas fractions at z ~ 3.4
- 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
- Mock light-cones and theory friendly catalogues for the CANDELS survey
- 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
- Moderate-luminosity Growing Black Holes from 1.25 < z < 2.7: Varied Accretion in Disk-dominated Hosts
- Molecular gas on large circumgalactic scales at z = 3.47
- 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
- Morphologies of z ~ 0.7 AGN host galaxies in CANDELS: no trend of merger incidence with AGN luminosity
- Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology
- MOSEL: Strong OIII 5007 A Emitting Galaxies at (3 < z < 4) from the ZFOURGE Survey
- Multiresolution angular momentum measurements of z 1.5-2 star-forming galaxies
- 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 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
- 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
- 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
- Observations of the initial formation and evolution of spiral galaxies at 1 < z < 3 in the CANDELS fields
- On the Absence of High-redshift AGNs: Little Growth in the Supermassive Black Hole Population at High Redshifts
- On the AGN Nature of Two UV-bright Sources at zspec ~ 5.5 in the CANDELS Fields: An Update on the AGN Space Density at M1450 ~ -22.5
- On the Impact of Inclination-dependent Attenuation on Derived Star Formation Histories: Results from Disk Galaxies in the Great Observatories Origins Deep Survey Fields
- 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
- Photometric Redshift Estimation with Galaxy Morphology Using Self-organizing Maps
- Photometry of high-redshift blended galaxies using deep learning
- Physical Characterization of an Unlensed, Dusty Star-forming Galaxy at z = 5.85
- Piercing through Highly Obscured and Compton-thick AGNs in the Chandra Deep Fields. II. Are Highly Obscured AGNs the Missing Link in the Merger-triggered AGN-Galaxy Coevolution Models?
- Potential signature of a quadrupolar hubble expansion in Pantheon+supernovae
- Probabilistic model for dynamic galaxy decomposition
- Probing the Dawn of Galaxies at z ~ 9-12: New Constraints from HUDF12/XDF and CANDELS data
- Probing the Star Formation Main Sequence Down to 108 M at 1.0 < z < 3.0
- Properties of galaxies reproduced by a hydrodynamic simulation
- Properties of Submillimeter Galaxies in the CANDELS GOODS-South Field
- PSFGAN: a generative adversarial network system for separating quasar point sources and host galaxy light
- 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
- Reconstructing the Assembly of Massive Galaxies. I. The Importance of the Progenitor Effect in the Observed Properties of Quiescent Galaxies at z 2
- 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
- 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
- Robust identification of active galactic nuclei through HST optical variability in GOODS-S: comparison with the X-ray and mid-IR-selected samples
- Searching for fast extragalactic X-ray transients in Chandra surveys
- 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
- Serendipitous Discovery of a Massive cD Galaxy at z = 1.096: Implications for the Early Formation and Late Evolution of cD Galaxies
- SIMBA: Cosmological simulations with black hole growth and feedback
- Simulations of the WFIRST Supernova Survey and Forecasts of Cosmological Constraints
- 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
- Slow Evolution of the Specific Star Formation Rate at z > 2: The Impact of Dust, Emission Lines, and a Rising Star Formation History
- Smooth(er) Stellar Mass Maps in CANDELS: Constraints on the Longevity of Clumps in High-redshift Star-forming Galaxies
- 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
- Starbursts in and out of the star-formation main sequence
- Star Formation Rate Function at z 4.5: An Analysis from Rest UV to Optical
- Stellar, Gas, and Dust Emission of Star-forming Galaxies out to z ~ 2
- Stellar masses of giant clumps in CANDELS and simulated galaxies using machine learning
- Stellar Populations of Lya-emitting Galaxies in the HETDEX Survey. I. An Analysis of LAEs in the GOODS-N Field
- Strategies for Obtaining Robust Spectral Energy Distribution Fitting Parameters for Galaxies at z ~ 1 and z ~ 2 in the Absence of Infrared Data
- 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
- Supermassive black holes at high redshift are expected to be obscured by their massive host galaxies interstellar medium
- Surface Brightness Evolution of Galaxies in the CANDELS GOODS Fields up to z ~ 6: High-z Galaxies Are Unique or Remain Undetected
- 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 abundance of massive compact galaxies at 1.0 < z < 3.0 in 3D-HST/CANDELS
- The Accretion History of AGN: The Spectral Energy Distributions of X-Ray-luminous Active Galactic Nuclei
- 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: The Nature of the Faintest Dusty Star-forming Galaxies
- The ALMA Spectroscopic Survey in the HUDF: CO Luminosity Functions and the Molecular Gas Content of Galaxies through Cosmic History
- The ALMA Spectroscopic Survey in the HUDF: Nature and Physical Properties of Gas-mass Selected Galaxies Using MUSE Spectroscopy
- The ALPINE-ALMA CII survey. Small Lya-CII velocity offsets in main-sequence galaxies at 4.4 < z < 6
- The ALPINE-ALMA CII survey. Survey strategy, observations, and sample properties of 118 star-forming galaxies at 4 < z < 6
- 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 Bright End of the Ultraviolet Luminosity Function at z ~ 8: New Constraints from CANDELS Data in GOODS-South
- 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 C II emission as a molecular gas mass tracer in galaxies at low and high redshifts
- 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 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 debiased morphological transformations of galaxies since z = 3 in CANDELS
- The diffuse g-ray background is dominated by star-forming galaxies
- The Effect of the Morphological Quenching Mechanism on Star Formation Activity at 0.5 < z < 1.5 in 3D-HST/CANDELS
- The emergence of passive galaxies in the early Universe
- The evolution of the galaxy stellar-mass function over the last 12 billion years from a combination of ground-based and HST surveys
- The evolution of the X-ray luminosity functions of unabsorbed and absorbed AGNs out to z~ 5
- The Far-infrared Emission of the First Massive Galaxies
- The GREATS H b + O III luminosity function and galaxy properties at z ~ 8: walking the way of JWST
- The hidden side of cosmic star formation at z > 3. Bridging optically dark and Lyman-break galaxies with GOODS-ALMA
- The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) Survey Design, Reductions, and Detections
- 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 Impact of Inclination-dependent Attenuation on Ultraviolet Star Formation Rate Tracers
- The impact of satellite trails on Hubble Space Telescope observations
- The JWST Advanced Deep Extragalactic Survey: Discovery of an Extreme Galaxy Overdensity at z = 5.4 with JWST/NIRCam in GOODS-S
- The KMOS Deep Survey (KDS) - I. Dynamical measurements of typical star-forming galaxies at z 3.5
- 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 Mass Dependence of Structure, Star Formation Rate, and Mass Assembly Mode at 0.5 < z < 2.5
- The mass evolution of the first galaxies: stellar mass functions and star formation rates at 4 < z < 7 in the CANDELS GOODS-South field
- The mass-metallicity-star formation rate relation at z 2 with 3D Hubble Space Telescope
- 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 Morphology-Density Relationship in 1 < z < 2 Clusters
- 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: differences in SFR and metallicity for morphologically selected mergers 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 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 motivation for flexible star-formation histories from spatially resolved scales within galaxies
- 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. XII. Mg II emission and absorption in star-forming galaxies
- The MUSE-Wide Survey: survey description and first data release
- The MUSE-Wide survey: Three-dimensional clustering analysis of Lyman-a emitters at 3.3 < z < 6
- The O III+H b equivalent width distribution at z 7: implications for the contribution of galaxies to reionization
- 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 Physical Properties of Star-forming Galaxies with Strong O III Lines at z = 3.25
- The prevalence of galaxy overdensities around UV-luminous Lyman ?? emitters in the Epoch of Reionization
- The Progenitors of the Compact Early-type Galaxies at High Redshift
- The progenitors of the first red sequence galaxies at z ~ 2
- The Properties of Ha Emission-line Galaxies at Z = 2.24
- The properties of (sub-)millimetre-selected galaxies as revealed by CANDELS HST WFC3/IR imaging in GOODS-South
- 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 Spitzer/IRAC Legacy over the GOODS Fields: Full-depth 3.6, 4.5, 5.8, and 8.0 mm Mosaics and Photometry for >9000 Galaxies at z 3.5-10 from the GOODS Reionization Era Wide-area Treasury from Spitzer (GREATS)
- 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 Stellar Mass Structure of Massive Galaxies from z = 0 to z = 2.5: Surface Density Profiles and Half-mass Radii
- 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 UV continuum slopes of early star-forming galaxies in JADES
- 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 UV spectral slope b and stellar population of most active star-forming galaxies at z ~ 4
- 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
- Tight Correlations between Massive Galaxy Structural Properties and Dynamics: The Mass Fundamental Plane was in Place by z ~ 2
- Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 5
- To Stack or Not to Stack: Spectral Energy Distribution Properties of Lya-emitting Galaxies at z = 2.1
- 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
- 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
- Ultraviolet luminosity density of the universe during the epoch of reionization
- Unbiased Differential Size Evolution and the Inside-out Growth of Galaxies in the Deep CANDELS GOODS Fields at 1 <= z <= 7
- UNIVERSEMACHINE: The correlation between galaxy growth and dark matter halo assembly from z = 0-10
- UV and Lya luminosity functions of galaxies and star formation rate density at the end of HI reionization from the VIMOS UltraDeep Survey (VUDS)
- 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-ray emission of z > 2.5 active galactic nuclei can be obscured by their host galaxies
- X-Ray Selected AGN Host Galaxies are Similar to Inactive Galaxies out to z = 3: Results from CANDELS/CDF-S
- 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
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| Keywords |
Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2 |
