| Publication |
- 1000 High-redshift Galaxies with Spatially-resolved Spectroscopy: Angular Momentum over 10 Billion Years
- 3D-HST: A Wide-field Grism Spectroscopic Survey with the Hubble Space Telescope
- 3D-HST Emission Line Galaxies at z ~ 2: Discrepancies in the Optical/UV Star Formation Rates
- 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 Bayesian Population Model for the Observed Dust Attenuation in Galaxies
- A CANDELS-3D-HST synergy: Resolved Star Formation Patterns at 0.7 < z < 1.5
- A Comprehensive Study of Lya Emission in the High-redshift Galaxy Population
- A Consistent Study of Metallicity Evolution at 0.8 < z < 2.6
- Active Galactic Nucleus Properties of ~1 Million Member Galaxies of Galaxy Groups and Clusters at z < 1.4 Based on the Subaru Hyper Suprime-Cam Survey
- A Diverse Population of z 2 ULIRGs Revealed by JWST Imaging
- Ages of Massive Galaxies at 0.5 > z > 2.0 from 3D-HST Rest-frame Optical Spectroscopy
- AGN accretion and black hole growth across compact and extended galaxy evolution phases
- AGN-host connection at 0.5 < z < 2.5: A rapid evolution of AGN fraction in red galaxies during the last 10 Gyr
- AGN Selection and Demographics in GOODS-S/HUDF from X-Ray to Radio
- A Large Population of Obscured AGN in Disguise as Low-luminosity AGN in Chandra Deep Field South
- ALMA reveals starburst-like interstellar medium conditions in a compact star-forming galaxy at z 2 using CI and CO
- 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
- A massive, quiescent, population II galaxy at a redshift of 2.1
- Analysis of a custom support vector machine for photometric redshift estimation and the inclusion of galaxy shape information
- An Atlas of Color-selected Quiescent Galaxies at z > 3 in Public JWST Fields
- An automatic taxonomy of galaxy morphology using unsupervised machine learning
- An Enigmatic Population of Luminous Globular Clusters in a Galaxy Lacking Dark Matter
- A new, faint population of X-ray transients
- Angular momentum evolution of galaxies over the past 10 Gyr: a MUSE and KMOS dynamical survey of 400 star-forming galaxies from z = 0.3 to 1.7
- Angular Momentum Evolution of Stellar Disks at High Redshifts
- An Older, More Quiescent Universe from Panchromatic SED Fitting of the 3D-HST Survey
- An Updated Dust-to-Star Geometry: Dust Attenuation Does Not Depend on Inclination in 1.3 <=z <=2.6 Star-forming Galaxies from MOSDEF
- A population of red candidate massive galaxies 600 Myr after the Big Bang
- A Population of Short-duration Gamma-Ray Bursts with Dwarf Host Galaxies
- Are star formation rates of galaxies bimodal?
- Are the host galaxies of long gamma-ray bursts more compact than star-forming galaxies of the field?
- A Second Galaxy Missing Dark Matter in the NGC 1052 Group
- A Spectroscopic Sample of Massive, Quiescent z ~ 2 Galaxies: Implications for the Evolution of the Mass-Size Relation
- A steep bandpass interference filter with FWHM 11nm centered at 1254nm for studying Lyman Alpha signatures of highly redshifted galaxies
- AstroSat detection of Lyman continuum emission from a z = 1.42 galaxy
- A3COSMOS and A3GOODSS: Continuum source catalogues and multi-band number counts
- Automatic Classification of Galaxy Morphology: A Rotationally-invariant Supervised Machine-learning Method Based on the Unsupervised Machine-learning Data Set
- Automatic Morphological Classification of Galaxies: Convolutional Autoencoder and Bagging-based Multiclustering Model
- A WFC3 Grism Emission Line Redshift Catalog in the GOODS-South Field
- A Window on the Earliest Star Formation: Extreme Photoionization Conditions of a High-ionization, Low-metallicity Lensed Galaxy at z ~ 2*
- A z = 1.85 galaxy group in CEERS: Evolved, dustless, massive intra-halo light and a brightest group galaxy in the making
- Beyond the Local Volume. II. Population Scaleheights and Ages of Ultracool Dwarfs in Deep HST/WFC3 Parallel Fields
- Beyond the Local Volume. I. Surface Densities of Ultracool Dwarfs in Deep HST/WFC3 Parallel Fields
- Beyond UVJ: Color Selection of Galaxies in the JWST Era
- Bright compact bulges at intermediate redshifts
- Brighter and More Massive Galaxies in the Vicinity of Lya Nebulae
- 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-forming Galaxies with an Extended Rotating Disk at z ~ 2
- Bulge Growth and Quenching since z = 2.5 in CANDELS/3D-HST
- CANDELS Multi-wavelength Catalogs: Source Identification and Photometry in the CANDELS COSMOS Survey Field
- CANDELS Multi-wavelength Catalogs: Source Identification and Photometry in the CANDELS Extended Groth Strip
- Changing physical conditions in star-forming galaxies between redshifts 0 < z < 4: O III/H b evolution
- Cluster and field elliptical galaxies at z 1.3. The marginal role of the environment and the r^ance of the galaxy central regions
- 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
- Clusters of galaxies up to z = 1.5 identified from photometric data of the Dark Energy Survey and unWISE
- Color Gradients and Half-mass Radii of Galaxies Out to z = 2 in the CANDELS/3D-HST Fields: Further Evidence for Important Differences in the Evolution of Mass-weighted and Light-weighted Sizes
- Compact galaxies and the size-mass galaxy distribution from a colour-selected sample at 0.04 < z < 0.15 supplemented by ugrizYJHK photometric redshifts
- Compact Star-forming Galaxies as Old Starbursts Becoming Quiescent
- Completing the Census of AGN in GOODS-S/HUDF: New Ultradeep Radio Imaging and Predictions for JWST
- Confirmation of Small Dynamical and Stellar Masses for Extreme Emission Line Galaxies at z ~ 2
- Connecting Galactic Outflows and Star Formation: Inferences from Ha Maps and Absorption-line Spectroscopy at 1 z 1.5
- Connection between Stellar Mass Distributions within Galaxies and Quenching Since z = 2
- Constraining the Low-mass Slope of the Star Formation Sequence at 0.5 < z < 2.5
- Cosmic evolution and metal aversion in superluminous supernova host galaxies
- DAVOS: Dwarf Active Galactic Nuclei from Variability for the Origins of Seeds: Properties of Variability-selected Active Galactic Nuclei in the COSMOS Field and Expectations for the Rubin Observatory
- Deep CO(1-0) Observations of z = 1.62 Cluster Galaxies with Substantial Molecular Gas Reservoirs and Normal Star Formation Efficiencies
- Deep ugrizY imaging and DEEP2/3 spectroscopy: a photometric redshift testbed for LSST and public release of data from the DEEP3 Galaxy Redshift Survey
- Delving deep: A population of extremely dusty dwarfs observed by JWST
- Detecting episodes of star formation using Bayesian model selection
- Direct Measurements of Dust Attenuation in z ~ 1.5 Star-forming Galaxies from 3D-HST: Implications for Dust Geometry and Star Formation Rates
- Discovery of a Strong Lensing Galaxy Embedded in a Cluster at z = 1.62
- Dual constraints with ALMA: new O III 88-mm and dust-continuum observations reveal the ISM conditions of luminous LBGs at z 7
- Dust attenuation and Ha emission in a sample of galaxies observed with Herschel at 0.6 < z < 1.6
- Dust attenuation in z ~ 1 galaxies from Herschel and 3D-HST Ha measurements
- Dust Heating By Low-mass Stars in Massive Galaxies at z< 1
- Dust Temperature of Compact Star-forming Galaxies at z ~ 1-3 in 3D-HST/CANDELS
- Early- and late-stage mergers among main sequence and starburst galaxies at 0.2 <= z <= 2
- Environments of a sample of AzTEC submillimetre galaxies in the COSMOS field
- Euclid preparation. VIII. The Complete Calibration of the Colour-Redshift Relation survey: VLT/KMOS observations and data release
- Euclid preparation. XXX. Performance assessment of the NISP red grism through spectroscopic simulations for the wide and deep surveys
- Evidence for a Low Lyman Continuum Escape Fraction in Three Massive, Ultraviolet-bright Galaxies at z > 7
- Evidence for Inside-out Galaxy Growth and Quenching of a z ~ 2 Compact Galaxy From High-resolution Molecular Gas Imaging
- Evidence for non-smooth quenching in massive galaxies at z ~ 1
- Evidence for Non-stellar Rest-frame Near-IR Emission Associated with Increased Star Formation in Galaxies at z ~ 1
- Evidence for Wide-spread Active Galactic Nucleus-driven Outflows in the Most Massive z ~ 1-2 Star-forming Galaxies
- Evolution in the Black Hole--Galaxy Scaling Relations and the Duty Cycle of Nuclear Activity in Star-forming Galaxies
- Evolution of cosmic star formation in the SCUBA-2 Cosmology Legacy Survey
- Evolution of spatially resolved star formation main sequence and surface density profiles in massive disc galaxies at 0 z 1: inside-out stellar mass buildup and quenching
- 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 anti-truncated stellar profiles of S0 galaxies since z = 0.6 in the SHARDS survey. II. Structural and photometric evolution
- Evolution of the anti-truncated stellar profiles of S0 galaxies since z = 0.6 in the SHARDS survey. I. Sample and methods
- Exploring the correlation between Ha-to-UV ratio and burstiness for typical star-forming galaxies at z 2
- 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?
- FIGS--Faint Infrared Grism Survey: Description and Data Reduction
- Finding dusty AGNs from the JWST CEERS survey with mid-infrared photometry
- First data release of the Hyper Suprime-Cam Subaru Strategic Program
- First Infrared-Based Implications for the Dust Attenuation and Star Formation of Typical Lya Emitters
- First Results from the 3D-HST Survey: The Striking Diversity of Massive Galaxies at z > 1
- First Results from the VIRIAL Survey: The Stellar Content of UVJ-selected Quiescent Galaxies at 1.5 < z < 2 from KMOS
- Flat rotation curves and low velocity dispersions in KMOS star-forming galaxies at z ~ 1
- Formation of disc galaxies around z ~ 2
- Forming Compact Massive Galaxies
- Forward modeling of galaxy kinematics in slitless spectroscopy
- From Diversity to Dichotomy, and Quenching: Milky-Way-like and Massive Galaxy Progenitors at 0.5 < z <3.0
- From Exoplanets to Quasars: Detection of Potential Damped Lya Absorbing Galaxies Using Angular Differential Imaging
- Galaxies of the z ~ 2 Universe. I. Grism-selected Rest-frame Optical Emission-line Galaxies
- Galaxy Environment in the 3D-HST Fields: Witnessing the Onset of Satellite Quenching at z ~ 1-2
- Galaxy Merger Candidates in High-redshift Cluster Environments
- Galaxy Sizes Since z = 2 from the Perspective of Stellar Mass Distribution within Galaxies
- Galaxy Structure as a Driver of the Star Formation Sequence Slope and Scatter
- GAMA/G10-COSMOS/3D-HST: Evolution of the galaxy stellar mass function over 12.5 Gyr
- GAMA/G10-COSMOS/3D-HST: the 0 < z < 5 cosmic star formation history, stellar-mass, and dust-mass densities
- Growth of Bulges in Disk Galaxies Since z ~ 1
- Hidden Little Monsters: Spectroscopic Identification of Low-mass, Broad-line AGNs at z > 5 with CEERS
- High Dense Gas Fraction in a Gas-rich Star-forming Galaxy at z = 1.2
- High Gas Fraction in a CO-detected Main-sequence Galaxy at z > 3
- High-precision Photometric Redshifts from Spitzer/IRAC: Extreme 3.6 - 4.5 Colors Identify Galaxies in the Redshift Range z ~ 6.6 - 6.9
- High-redshift Massive Quiescent Galaxies Are as Flat as Star-forming Galaxies: The Flattening of Galaxies and the Correlation with Structural Properties in CANDELS/3D-HST
- How Accurate Are Infrared Luminosities from Monochromatic Photometric Extrapolation?
- How Dead are Dead Galaxies? Mid-infrared Fluxes of Quiescent Galaxies at Redshift 0.3 < z < 2.5: Implications for Star Formation Rates and Dust Heating
- How Lyman Alpha Emission Depends on Galaxy Stellar Mass
- HST Emission Line Galaxies at z ~ 2: Comparing Physical Properties of Lyman Alpha and Optical Emission Line Selected Galaxies
- HST Grism Confirmation of Two z ~ 2 Structures from the Clusters around Radio-loud AGN (CARLA) Survey
- HST Grism-derived Forecasts for Future Galaxy Redshift Surveys
- HST Ha grism spectroscopy of ROLES: a flatter low-mass slope for the z ~ 1 SSFR-mass relation
- Hubble Space Telescope Emission Line Galaxies at z ~ 2: The Lya Escape Fraction
- Hubble Space Telescope Emission-line Galaxies at z ~ 2: The Mystery of Neon
- Hubble Space Telescope Grism Spectroscopy of Extreme Starbursts across Cosmic Time: The Role of Dwarf Galaxies in the Star Formation History of the Universe
- Ha Equivalent Widths from the 3D-HST Survey: Evolution with Redshift and Dependence on Stellar Mass
- Identification and characterization of six spectroscopically confirmed massive protostructures at 2.5 < z < 4.5
- Imaging of diffuse H I absorption structure in the SSA22 protocluster region at z = 3.1
- Integrated and resolved dust attenuation in clumpy star-forming galaxies at 0.07 < z < 0.14
- Ionized-gas Metallicity of the Strong O IIIl5007 Emission-line Compact Galaxies in the LAMOST Survey
- IROCKS: Spatially Resolved Kinematics of z ~ 1 Star-forming Galaxies
- JWST/NIRSpec Balmer-line Measurements of Star Formation and Dust Attenuation at z 3-6
- JWST/NIRSpec spectroscopy of z = 7-9 star-forming galaxies with CEERS: new insight into bright Lya emitters in ionized bubbles
- JWST reveals a high fraction of disk breaks at 1 <= z <= 3
- KMOS3D: Dynamical Constraints on the Mass Budget in Early Star-forming Disks
- Large-scale Star-formation-driven Outflows at 1 < z < 2 in the 3D-HST Survey
- Learning Spectral Templates for Photometric Redshift Estimation from Broadband Photometry
- Leveraging 3D-HST Grism Redshifts to Quantify Photometric Redshift Performance
- Local galaxies with compact cores as the possible descendants of massive compact quiescent galaxies at high redshift
- Looking ahead to the sky with the Square Kilometre Array: simulating flux densities and resolved radio morphologies of 0 < z < 2.5 star-forming galaxies
- Low Gas Fractions Connect Compact Star-forming Galaxies to Their z ~ 2 Quiescent Descendants
- Lyman-alpha spectroscopy of extreme O III emitting galaxies at z 2-3: implications for Lya visibility and LyC leakage at z > 6
- Lyman Continuum Escape Fraction from Low-mass Starbursts at z = 1.3
- Lyman Continuum Escape Fraction of Star-forming Dwarf Galaxies at z ~ 1
- Lyman Continuum Leakers in the AstroSat Ultraviolet Deep Field: Extreme-ultraviolet Emitters at the Cosmic Noon
- Lya Emission Line Profiles of Extreme O III- emitting Galaxies at z 2: Implications for Lya Visibility in the Reionization Era
- Lya Halos around O III-selected Galaxies in HETDEX
- MAGPHYS+photo-z: Constraining the Physical Properties of Galaxies with Unknown Redshifts
- MAHALO Deep Cluster Survey I. Accelerated and enhanced galaxy formation in the densest regions of a protocluster at z = 2.5
- MAHALO Deep Cluster Survey II. Characterizing massive forming galaxies in the Spiderweb protocluster at z = 2.2
- Major Mergers Are Not the Dominant Trigger for High-accretion AGNs at z ~ 2
- Mapping the Morphology and Kinematics of a Lya-selected Nebula at z = 3.15 with MUSE
- Mass assembly in quiescent and star-forming galaxies since z 4 from UltraVISTA
- Massive compact quiescent galaxies in the M versus se plane: insights from stellar population properties
- Mass-metallicity relation and fundamental metallicity relation at z 2
- Measuring size evolution of distant, faint galaxies in the radio regime
- Measuring Stellar Masses of Emission-line Galaxies at 1.2 < z < 1.9
- MIGHTEE: Multi-wavelength counterparts in the COSMOS field
- Millimeter Mapping at z ~ 1: Dust-obscured Bulge Building and Disk Growth
- MMT/MMIRS spectroscopy of z = 1.3 - 2.4 extreme O III emitters: implications for galaxies in the reionization era
- Molecular and Ionized Gas Phases of an AGN-driven Outflow in a Typical Massive Galaxy at z 2
- Morpho-kinematics of z ~ 1 galaxies probe the hierarchical scenario
- Morphological Parameters and Associated Uncertainties for 8 Million Galaxies in the Hyper Suprime-Cam Wide Survey
- Morphological Transformation and Star Formation Quenching of Massive Galaxies at 0.5 <= z <= 2.5 in 3D-HST/CANDELS
- Morphologies of ~190,000 Galaxies at z = 0-10 Revealed with HST Legacy Data. II. Evolution of Clumpy Galaxies
- 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 ~190,000 Galaxies at z = 0-10 Revealed with HST Legacy Data. I. Size Evolution
- Morphology and the Color-mass Diagram as Clues to Galaxy Evolution at z&approx1
- Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology
- MOSFIRE Spectroscopy of Quiescent Galaxies at 1.5 < z < 2.5. I. Evolution of Structural and Dynamical Properties
- MOSFIRE Spectroscopy of Quiescent Galaxies at 1.5 < z < 2.5. II. Star Formation Histories and Galaxy Quenching
- Multiple Emission Lines of Ha Emitters at z ~ 2.3 from the Broad- and Medium-band Photometry in the ZFOURGE Survey
- Nature of Faint Radio Sources in GOODS-North and GOODS-South Fields. I. Spectral Index and Radio-FIR Correlation
- Near-infrared Spectroscopy of Five Ultra-massive Galaxies at 1.7 < z < 2.7
- New insight on the nature of cosmic reionizers from the CEERS survey
- Newly Discovered Bright z ~ 9-10 Galaxies and Improved Constraints on Their Prevalence Using the Full CANDELS Area
- New technique to select recent fast-quenching galaxies at z 2 using the optical colours
- No evidence for a significant AGN contribution to cosmic hydrogen reionization
- No Overdensity of Lyman-Alpha Emitting Galaxies around a Quasar at z ~ 5.7
- No strong dependence of Lyman continuum leakage on physical properties of star-forming galaxies at z 3.5
- Nowhere to hide: Radio-faint AGN in the GOODS-N field. II. Multi-wavelength AGN selection techniques and host galaxy properties
- Observations of Environmental Quenching in Groups in the 11 GYR since z = 2.5: Different Quenching for Central and Satellite Galaxies
- Observed UV Continuum Slopes (b) of Galaxies at z = 0.40-0.75 in the GOODS-North Field
- Observing Galaxy Mergers at the Epoch of Reionization
- One Plane for All: Massive Star-forming and Quiescent Galaxies Lie on the Same Mass Fundamental Plane at z ~ 0 and z ~ 0.7
- On the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7 < z < 2.8
- On the Transition of the Galaxy Quenching Mode at 0.5 < z < 1 in CANDELS
- Outside the Lyman-break box: detecting Lyman continuum emitters at 3.5 < z < 5.1 with CLAUDS
- Overturning the Case for Gravitational Powering in the Prototypical Cooling Lya Nebula
- Phibss: Molecular Gas Content and Scaling Relations in z ~ 1-3 Massive, Main-sequence Star-forming Galaxies
- Physical properties of the CDFS X-ray sources through fitting spectral energy distributions
- 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?
- Plateau de Bure High-z Blue Sequence Survey 2 (PHIBSS2): Search for Secondary Sources, CO Luminosity Functions in the Field, and the Evolution of Molecular Gas Density through Cosmic Time
- Polycyclic aromatic hydrocarbon luminous galaxies in JWST CEERS data
- Precise weak lensing constraints from deep high-resolution Ks images: VLT/HAWK-I analysis of the super-massive galaxy cluster RCS2 J 232727.7-020437 at z = 0.70
- Predicting Quiescence: The Dependence of Specific Star Formation Rate on Galaxy Size and Central Density at 0.5 < z < 2.5
- Properties of LBGs with OIII detection at z ~ 3.5. The importance of including nebular emission data in SED fitting
- Quasars Have Fewer Close Companions than Normal Galaxies
- Quenched fractions in the IllustrisTNG simulations: comparison with observations and other theoretical models
- Quiescent galaxies in a virialized cluster at redshift 2: evidence for accelerated size growth
- Radio Loud AGNs are Mergers
- Redshifting galaxies from DESI to JWST CEERS: Correction of biases and uncertainties in quantifying morphology
- Rejuvenated galaxies with very old bulges at the origin of the bending of the main sequence and of the green valley
- Resolving ambiguities in the inferred star formation histories of intense O III emitters in the reionization Era
- Resolving the Discrepancy of Galaxy Merger Fraction Measurements at z ~ 0-3
- Rest-frame UV spectroscopy of extreme O III emitters at 1.3 < z < 3.7: toward a high-redshift UV reference sample for JWST
- Rotating Starburst Cores in Massive Galaxies at z = 2.5
- Short GRB Host Galaxies. II. A Legacy Sample of Redshifts, Stellar Population Properties, and Implications for Their Neutron Star Merger Origins
- SILVERRUSH. V. Census of Lya, O III l5007, Ha, and C II 158 mm Line Emission with ~1000 LAEs at z = 4.9-7.0 Revealed with Subaru/HSC
- Similarities and uniqueness of Ly a emitters among star-forming galaxies at z = 2.5
- SKYSURF: Constraints on Zodiacal Light and Extragalactic Background Light through Panchromatic HST All-sky Surface-brightness Measurements: II. First Limits on Diffuse Light at 1.25, 1.4, and 1.6 mm
- SKYSURF: Constraints on Zodiacal Light and Extragalactic Background Light through Panchromatic HST All-sky Surface-brightness Measurements. I. Survey Overview and Methods
- Spatially Extended Low-ionization Emission Regions (LIERs) at z ~ 0.9
- Spatially Resolved Dust Maps from Balmer Decrements in Galaxies at z ~ 1.4
- Spatially resolved Kennicutt-Schmidt relation at z 7 and its connection with the interstellar medium properties
- Spatially resolved mass-metallicity relation at z ~ 0.26 from the MUSE-Wide Survey
- 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
- Spectrophotometric Redshifts in the Faint Infrared Grism Survey: Finding Overdensities of Faint Galaxies
- Spectroscopic Confirmation of an Ultra Massive and Compact Galaxy at z = 3.35: a Detailed Look at an Early Progenitor of Local Giant Ellipticals
- Spectroscopy of an extreme O III emitting active galactic nucleus at z = 3.212: implications for the reionization era
- Spitzers View of the Candidate Cluster and Protocluster Catalog (CCPC)
- Star-forming Blue ETGs in Two Newly Discovered Galaxy Overdensities in the HUDF at z=1.84 and 1.9: Unveiling the Progenitors of Passive ETGs in Cluster Cores
- Star-forming galaxies at low-redshift in the SHARDS survey
- Statistics of galaxy mergers: bridging the gap between theory and observation
- Stellar, Gas, and Dust Emission of Star-forming Galaxies out to z ~ 2
- Stellar Mass Growth of Brightest Cluster Galaxy Progenitors in COSMOS Since z ~ 3
- Stellar populations and star formation histories of the most extreme O III emitters at z = 1.3 - 3.7
- Strongly baryon-dominated disk galaxies at the peak of galaxy formation ten billion years ago
- Structural and morphological properties of ultraluminous infrared galaxies at 1<z<3
- Structural Evolution in Massive Galaxies at z ~ 2
- Structures, Stellar Population Properties, AGN Fractions, and Environments of Massive Compact Galaxies at 1 < z < 2 in 3D-HST/CANDELS
- Subkiloparsec Imaging of Lya Emission in a Low-mass, Highly Ionized, Gravitationally Lensed Galaxy at z = 1.84
- Submillimeter Galaxies as Progenitors of Compact Quiescent Galaxies
- Sunyaev-Zeldovich effect and X-ray scaling relations from weak lensing mass calibration of 32 South Pole Telescope selected galaxy clusters
- Super-deblended Dust Emission in Galaxies. I. The GOODS-North Catalog and the Cosmic Star Formation Rate Density out to Redshift 6
- Surface brightness profiles of blue compact dwarf galaxies in the GOODS-N and GOODS-S field
- SXDF-ALMA 1.5 arcmin2 Deep Survey: A Compact Dusty Star-forming Galaxy at z = 2.5
- Testing Diagnostics of Nuclear Activity and Star Formation in Galaxies at z > 1
- Testing the accuracy of 3D-HST photometric redshift estimates as reference samples for deep weak lensing studies
- Tests of Catastrophic Outlier Prediction in Empirical Photometric Redshift Estimation with Redshift Probability Distributions
- The 3D-HST Survey: Hubble Space Telescope WFC3/G141 Grism Spectra, Redshifts, and Emission Line Measurements for ~ 100,000 Galaxies
- The Ages of Passive Galaxies in a z = 1.62 Protocluster
- The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Molecular Gas Reservoirs in High-redshift Galaxies
- The ALMA Spectroscopic Survey in the HUDF: The Cosmic Dust and Gas Mass Densities in Galaxies up to z ~ 3
- The ALPINE-ALMA CII survey: Double stellar population and active galactic nucleus activity in a galaxy at z ~ 5.5
- The ALPINE-ALMA C II Survey: Size of Individual Star-forming Galaxies at z = 4-6 and Their Extended Halo Structure
- The ALPINE-ALMA C II Survey: The Infrared-Radio Correlation and Active Galactic Nucleus Fraction of Star-forming Galaxies at z 4.4-5.9
- The ALPINE-ALMA CII survey. The nature, luminosity function, and star formation history of dusty galaxies up to z 6
- The average dust attenuation curve at z 1.3 based on HST grism surveys
- The Chandra Deep Field-South Survey: 7 Ms Source Catalogs
- The Compact Star-forming Galaxies at 2<z<3 in 3D-HST/CANDELS: AGN and Non-AGN Physical Properties
- The Constant Average Relationship between Dust-obscured Star Formation and Stellar Mass from z = 0 to z = 2.5
- The contribution of faint Lyman-a emitters to extended Lyman-a halos constrained by MUSE clustering measurements
- The cosmic spectral energy distribution in the EAGLE simulation
- The Dust Attenuation Curve versus Stellar Mass for Emission Line Galaxies at z ~ 2
- The Effect of Environment on Star Formation Activity and Morphology at 0.5 < z < 2.5 in CANDELS
- The Effect of the Morphological Quenching Mechanism on Star Formation Activity at 0.5 < z < 1.5 in 3D-HST/CANDELS
- The eMERGE Survey - I: Very Large Array 5.5 GHz observations of the GOODS-North Field
- The Environment of z > 1 3CR Radio Galaxies and QSOs: From Proto-clusters to Clusters of Galaxies?
- The Evolution and Origin of Ionized Gas Velocity Dispersion from z ~ 2.6 to z ~ 0.6 with KMOS3D
- The evolution of the equivalent width of the Ha emission line and specific star formation rate in star-forming galaxies at 1 < z < 5
- The Evolution of the Fractions of Quiescent and Star-forming Galaxies as a Function of Stellar Mass Since z = 3: Increasing Importance of Massive, Dusty Star-forming Galaxies in the Early Universe
- The Evolution of the Quenching of Star Formation in Cluster Galaxies since z ~ 1
- The Evolution of the Star-Forming Interstellar Medium Across Cosmic Time
- The Evolution of the Tully-Fisher Relation between z ~ 2.3 and z ~ 0.9 with KMOS3D
- The Fate of a Red Nugget: In Situ Star Formation of Satellites around a Massive Compact Galaxy
- The FENIKS Survey: Multiwavelength Photometric Catalog in the UDS Field, and Catalogs of Photometric Redshifts and Stellar Population Properties
- The FourStar Galaxy Evolution Survey (ZFOURGE): Ultraviolet to Far-infrared Catalogs, Medium-bandwidth Photometric Redshifts with Improved Accuracy, Stellar Masses, and Confirmation of Quiescent Galaxies to z ~ 3.5
- The GOGREEN survey: dependence of galaxy properties on halo mass at z > 1 and implications for environmental quenching
- The GOGREEN survey: transition galaxies and the evolution of environmental quenching
- The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-redshift Galaxies
- The HDUV Survey: Six Lyman Continuum Emitter Candidates at z ~ 2 Revealed by HST UV Imaging
- The HETDEX Survey: The Lya Escape Fraction from 3D-HST Emission-Line Galaxies at z ~ 2
- The HSC-SSP Transient Survey: Implications from Early Photometry and Rise Time of Normal Type Ia Supernovae
- The Hubble Deep Hydrogen Alpha (HDHa) Project. I. Catalog of Emission-line Galaxies
- The Ha and O III l5007 Luminosity Functions of 1.2 < z < 1.9 Emission-line Galaxies from Hubble Space Telescope (HST) Grism Spectroscopy
- The H a luminosity and stellar mass dependent clustering of star-forming galaxies at 0.7 < z < 1.5 with 3D-HST
- The impact of black hole scaling relation assumptions on the mass density of black holes
- The impact of satellite trails on Hubble Space Telescope observations
- The JWST Extragalactic Mock Catalog: Modeling Galaxy Populations from the UV through the Near-IR over 13 Billion Years of Cosmic History
- The Kinematics of Massive Quiescent Galaxies at 1.4 < z < 2.1: Dark Matter Fractions, IMF Variation, and the Relation to Local Early-type Galaxies
- The KMOS Cluster Survey (KCS). II. The Effect of Environment on the Structural Properties of Massive Cluster Galaxies at Redshift 1.39 < z < 1.61
- The KMOS Cluster Survey (KCS). I. The Fundamental Plane and the Formation Ages of Cluster Galaxies at Redshift 1.4 < z < 1.6
- The KMOS3D Survey: Data Release and Final Survey Paper
- The KMOS3D Survey: Rotating Compact Star-forming Galaxies and the Decomposition of Integrated Line Widths
- The Lockman-SpReSO project. Galactic flows in a sample of far-infrared galaxies
- The Lyman Continuum Escape Fraction of Emission Line-selected z ~ 2.5 Galaxies Is Less Than 15%
- The MAGPI survey: evolution of radial trends in star formation activity across cosmic time
- The Mass, Color, and Structural Evolution of Todays Massive Galaxies Since z ~ 5
- The Mass-Metallicity Relation at z 1-2 and Its Dependence on the Star Formation Rate
- 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 missing satellite problem in 3D
- The Morphological Evolution, AGN Fractions, Dust Content, Environments, and Downsizing of Massive Green Valley Galaxies at 0.5 < z < 2.5 in 3D-HST/CANDELS
- The Morphologies of Massive Galaxies from z ~ 3--Witnessing the Two Channels of Bulge Growth
- The MOSDEF Survey: A Census of AGN-driven Ionized Outflows at z = 1.4-3.8
- The MOSDEF Survey: AGN Multi-wavelength Identification, Selection Biases, and Host Galaxy Properties
- The MOSDEF survey: a new view of a remarkable z = 1.89 merger
- The MOSDEF survey: an improved Voronoi binning technique on spatially resolved stellar populations at z ~ 2
- The MOSDEF Survey: A Stellar Mass-SFR-Metallicity Relation Exists at z ~ 2.3
- The MOSDEF survey: differences in SFR and metallicity for morphologically selected mergers at z ~ 2
- The MOSDEF survey: direct-method metallicities and ISM conditions at z ~ 1.5-3.5
- The MOSDEF Survey: Direct Observational Constraints on the Ionizing Photon Production Efficiency, x ion, 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: Dynamical and Baryonic Masses and Kinematic Structures of Star-forming Galaxies at 1.4 <= z <= 2.6
- 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: Measurements of Balmer Decrements and the Dust Attenuation Curve at Redshifts z ~ 1.4-2.6
- The MOSDEF Survey: Metallicity Dependence of PAH Emission at High Redshift and Implications for 24 mm Inferred IR Luminosities and Star Formation Rates at z ~ 2
- The MOSDEF Survey: No Significant Enhancement in Star Formation or Deficit in Metallicity in Merging Galaxy Pairs at 1.5 z 3.5
- The MOSDEF Survey: Optical Active Galactic Nucleus Diagnostics 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: The Nature of Mid-infrared Excess Galaxies and a Comparison of IR and UV Star Formation Tracers at z ~ 2
- The MOSDEF Survey: The Prevalence and Properties of Galaxy-wide AGN-driven Outflows 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 MUSE-Wide survey: A first catalogue of 831 emission line galaxies
- The MUSE-Wide survey: a measurement of the Ly a emitting fraction among z > 3 galaxies
- The Neon Gap: Probing Ionization with Dwarf Galaxies at z 1
- The Number Density Evolution of Extreme Emission Line Galaxies in 3D-HST: Results from a Novel Automated Line Search Technique for Slitless Spectroscopy
- 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 Thickness of Stellar Disks to z ~ 2
- The Radial Distribution of Star Formation in Galaxies at z ~ 1 from the 3D-HST Survey
- The Relation between Dynamical Mass-to-light Ratio and Color for Massive Quiescent Galaxies out to z ~ 2 and Comparison with Stellar Population Synthesis Models
- The Relation between O III/Hb and Specific Star Formation Rate in Galaxies at z ~ 2
- The relationship between dust and C I at z = 1 and beyond
- The Rest-frame Optical (900 nm) Galaxy Luminosity Function at z ~ 4-7: Abundance Matching Points to Limited Evolution in the M STAR/M HALO Ratio at z >= 4
- The SCUBA-2 Cosmology Legacy Survey: the EGS deep field - III. The evolution of faint submillimetre galaxies at z < 4
- The Significance of Thermally Pulsing Asymptotic Giant Branch Stars in Post-starburst Galaxies
- The Size Evolution of Star-forming Galaxies since z ~ 7 Using ZFOURGE
- The Sizes of Candidate z~9-10 Galaxies: Confirmation of the Bright CANDELS Sample and Relation with Luminosity and Mass.
- The Sizes of Quasar Host Galaxies in the Hyper Suprime-Cam Subaru Strategic Program
- The spatial extent and distribution of star formation in 3D-HST mergers at z ~ 1.5
- The stellar-to-halo mass relation over the past 12 Gyr. I. Standard LCDM model
- The Structural Evolution of Milky-Way-like Star-forming Galaxies since z ~ 1.3
- The VANDELS survey: Discovery of massive overdensities of galaxies at z > 2. Location of Lya-emitting galaxies with respect to environment
- Third data release of the Hyper Suprime-Cam Subaru Strategic Program
- Tight Correlations between Massive Galaxy Structural Properties and Dynamics: The Mass Fundamental Plane was in Place by z ~ 2
- Ultrafaint C II Emission in a Redshift = 2 Gravitationally Lensed Metal-poor Dwarf Galaxy
- Unbiased Cosmological Parameter Estimation from Emission-line Surveys with Interlopers
- Where Stars Form: Inside-out Growth and Coherent Star Formation from HST Ha Maps of 3200 Galaxies across the Main Sequence at 0.7 < z < 1.5
- X-rays across the galaxy population - III. The incidence of AGN as a function of star formation rate
- X-rays across the galaxy population - II. The distribution of AGN accretion rates as a function of stellar mass and redshift.
- X-rays across the galaxy population - I. Tracing the main sequence of star formation
- Young, Star-forming Galaxies and Their Local Counterparts: The Evolving Relationship of Mass-SFR-Metallicity Since z ~ 2.1
- ZFIRE: 3D Modeling of Rotation, Dispersion, and Angular Momentum of Star-forming Galaxies at z ~ 2
- ZFIRE: The Evolution of the Stellar Mass Tully-Fisher Relation to Redshift ~2.2
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| Keywords |
Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2 |
