| Publication |
- 1.75 h -1 kpc Separation Dual Active Galactic Nuclei at z = 0.36 in the Cosmos Field
- 3D-DASH: The Evolution of Size, Shape, and Intrinsic Scatter in Populations of Young and Old Quiescent Galaxies at 0.5 < z < 3
- A 1.4 deg2 blind survey for C II, C III and C IV at z ~ 0.7-1.5 - I. Nature, morphologies and equivalent widths
- A Catalog of 204 Offset and Dual Active Galactic Nuclei (AGNs): Increased AGN Activation in Major Mergers and Separations under 4 kpc
- A Catalog of AGN Host Galaxies Observed with HST/ACS: Correlations between Star Formation and AGN Activity
- A cautionary tale of Ly C escape fraction estimates from high-redshift galaxies
- Accurate shear measurement with faint sources
- A Coherent Study of Emission Lines from Broadband Photometry: Specific Star Formation Rates and O III/Hb Ratio at 3 > z > 6
- A coincidence of disturbed morphology and blue UV colour: minor-merger-driven star formation in early-type galaxies at z~ 0.6
- A Comparison of the Morphological Properties between Local and z ~ 1 Infrared Luminous Galaxies: Are Local and High-z (U)LIRGs Different?
- A Comparison of Weak-Lensing Measurements from Ground- and Space-Based Facilities
- A Constant Limiting Mass Scale for Flat Early-type Galaxies from z ~ 1 to z = 0: Density Evolves but Shapes Do Not
- Active Galactic Nuclei and Host Galaxies in COSMOS-Web. I. NIRCam Images, Point-spread-function Models and Initial Results on X-Ray-selected Broad-line AGNs at 0.35 z 3.5
- Active galactic nuclei vs. host galaxy properties in the COSMOS field
- Active Galactic Nucleus Host Galaxy Morphologies in COSMOS
- A Far-infrared Characterization of 24 mm Selected Galaxies at 0 < z < 2.5 using Stacking at 70 mm and 160 mm in the COSMOS Field
- A Higher Efficiency of Converting Gas to Stars Pushes Galaxies at z ~ 1.6 Well Above the Star-forming Main Sequence
- A High Space Density of L* Active Galactic Nuclei at z ~ 4 in the COSMOS Field
- A journey from the outskirts to the cores of groups. I. Color- and mass-segregation in 20K-zCOSMOS groups
- A large, deep 3 deg2 survey of H a, O III, and O II emitters from LAGER: constraining luminosity functions
- A Large Population of Massive Compact Post-starburst Galaxies at z > 1: Implications for the Size Evolution and Quenching Mechanism of Quiescent Galaxies
- ALMA Imaging of Gas and Dust in a Galaxy Protocluster at Redshift 5.3: C II Emission in Typical Galaxies and Dusty Starbursts 1 Billion Years after the Big Bang
- ALMA Measures Rapidly Depleted Molecular Gas Reservoirs in Massive Quiescent Galaxies at z ~ 1.5
- ALMA Millimeter/Submillimeter Sources among Spitzer SMUVS Galaxies at z > 2 in the COSMOS Field
- ALMA Reveals Metals yet No Dust within Multiple Components in CR7
- ALMA Reveals the Molecular Gas Properties of Five Star-forming Galaxies across the Main Sequence at 3
- A Low Escape Fraction of Ionizing Photons of L > L* Lyman Break Galaxies at z = 3.3
- A massive compact quiescent galaxy at z = 2 with a complete Einstein ring in JWST imaging
- A Massive Molecular Gas Reservoir in the z = 5.3 Submillimeter Galaxy AzTEC-3
- A Morphological Classification Model to Identify Unresolved PanSTARRS1 Sources: Application in the ZTF Real-time Pipeline
- A Morphological Classification Model to Identify Unresolved PanSTARRS1 Sources. II. Update to the PS1 Point Source Catalog
- A Morphological Study of Galaxies Hosting Optical Variability-selected AGNs in the COSMOS Field
- A Multiwavelength Study of a Sample of 70 mm Selected Galaxies in the COSMOS Field. II. The Role of Mergers in Galaxy Evolution
- A multi-wavelength study of the gravitational lens COSMOS J095930+023427
- A multiwavelength study of (ultra)luminous infrared galaxies in the cosmos field
- An ALMA survey of submillimetre galaxies in the COSMOS field: Physical properties derived from energy balance spectral energy distribution modelling
- An ALMA survey of submillimetre galaxies in the COSMOS field: The extent of the radio-emitting region revealed by 3 GHz imaging with the Very Large Array
- Analogues of primeval galaxies two billion years after the Big Bang
- An Alternate Approach to Measure Specific Star Formation Rates at 2lt zlt 7
- Analysis of ~106 Spiral Galaxies from Four Telescopes Shows Large-Scale Patterns of Asymmetry in Galaxy Spin Directions
- Analysis of a custom support vector machine for photometric redshift estimation and the inclusion of galaxy shape information
- Analytical weak-lensing shear responses of galaxy properties and galaxy detection
- A New Method to Separate Star-forming from AGN Galaxies at Intermediate Redshift: The Submillijansky Radio Population in the VLA-COSMOS Survey
- An Exponential Decline at the Bright End of the z = 6 Galaxy Luminosity Function
- 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 of z ~ 1.5 galaxies and their local analogues with adaptive optics
- An indirect measurement of gas evolution in galaxies at 0.5 < z < 2.0
- An Ultradeep Multiband Very Large Array Survey of the Faint Radio Sky (COSMOS-XS): New Constraints on the Optically Dark Population
- A Potential Galaxy Threshing System in the COSMOS Field
- A Preferential Growth Channel for Supermassive Black Holes in Elliptical Galaxies at z 2
- A random forest-based selection of optically variable AGN in the VST-COSMOS field
- Are High-redshift Galaxies Hot? Temperature of z > 5 Galaxies and Implications for Their Dust Properties
- A robust morphological classification of high-redshift galaxies using support vector machines on seeing limited images. II. Quantifying morphological k-correction in the COSMOS field at 1 < z < 2: Ks band vs. I band
- A Runaway Black Hole in COSMOS: Gravitational Wave or Slingshot Recoil?
- A Search for H-Dropout Lyman Break Galaxies at z 12-16
- A study of the abundances and Lya emission of ultraviolet selected samples of star forming galaxies in the local universe
- A3COSMOS and A3GOODSS: Continuum source catalogues and multi-band number counts
- A3COSMOS: Dissecting the gas content of star-forming galaxies across the main sequence at 1.2 <= z < 1.6
- Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS). I. Robust ALMA Continuum Photometry Catalogs and Stellar Mass and Star Formation Properties for ~700 Galaxies at z = 0.5-6
- A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE). XV. The Ha luminosity function of the Virgo cluster
- A Weak Lensing Study of X-ray Groups in the Cosmos Survey: Form and Evolution of the Mass-Luminosity Relation
- A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). I. The Optical Counterparts of FIRST Radio Sources
- A Wide-Angle Tail Radio Galaxy in the COSMOS Field: Evidence for Cluster Formation
- A z = 2.5 protocluster associated with the radio galaxy MRC 2104-242: star formation and differing mass functions in dense environments
- Bar pattern speed evolution over the last 7 Gyr
- Bars in early- and late-type discs in COSMOS
- Black hole accretion and host galaxies of obscured quasars in XMM-COSMOS
- Blending and obscuration in weak-lensing magnification
- Bootes. IV. A new Milky Way satellite discovered in the Subaru Hyper Suprime-Cam Survey and implications for the missing satellite problem
- Broadband Selection, Spectroscopic Identification, and Physical Properties of a Population of Extreme Emission-line Galaxies at 3 < z < 3.7
- Bulge formation inside quiescent lopsided stellar disks: Connecting accretion, star formation, and morphological transformation in a z ~ 3 galaxy group
- Bulge Growth and Quenching since z = 2.5 in CANDELS/3D-HST
- Bulgeless Galaxies at Intermediate Redshift: Sample Selection, Color Properties, and the Existence of Powerful Active Galactic Nuclei
- Can we use weak lensing to measure total mass profiles of galaxies on 20 kpc scales?
- Central concentration of asymmetric features in post-starburst galaxies at z 0.8
- Chandra High-resolution observations of CID-42, a Candidate Recoiling Supermassive Black Hole
- Characterization and photometric performance of the Hyper Suprime-Cam Software Pipeline
- Characterization of star-forming dwarf galaxies at 0.1 z 0.9 in VUDS: probing the low-mass end of the mass-metallicity relation
- Characterization of Two 2 mm detected Optically Obscured Dusty Star-forming Galaxies
- Characterizing elusive, faint dusty star-forming galaxies: a lensed, optically undetected ALMA galaxy at z 3.3
- Charge transfer inefficiency in the Hubble Space Telescope since Servicing Mission 4
- Chitah: Strong-gravitational-lens Hunter in Imaging Surveys
- Classification of Extremely Red Objects in the Cosmos Field
- Classifying stars, galaxies, and AGNs in CLAUDS + HSC-SSP using gradient boosted decision trees
- Cluster and field elliptical galaxies at z 1.3. The marginal role of the environment and the r^ance of the galaxy central regions
- Color and Stellar Population Gradients in Passively Evolving Galaxies at z ~ 2 from HST/WFC3 Deep Imaging in the Hubble Ultra Deep Field
- Compact Galaxies at intermediate redshifts quench faster than normal-sized Galaxies
- Comparison of star formation rates from Ha and infrared luminosity as seen by Herschel
- Complete IRAC Mapping of the CFHTLS-DEEP, MUSYC, and NMBS-II Fields
- Comprehensive Gas Characterization of a z = 2.5 Protocluster: A Cluster Core Caught in the Beginning of Virialization?
- Compton thick AGN in the XMM-COSMOS survey
- Constraints on Quenching of Z 2 Massive Galaxies from the Evolution of the Average Sizes of Star-forming and Quenched Populations in COSMOS
- Constraints on the Faint End of the Quasar Luminosity Function at z ~ 5 in the COSMOS Field
- Constraints on the nature of CID-42: recoil kick or supermassive black hole pair?
- Constraints on Two Active Galactic Nuclei in the Merger Remnant COSMOS J100043.15+020637.2
- COSBO: The MAMBO 1.2 Millimeter Imaging Survey of the COSMOS Field
- Cosmic Evolution of Barred Galaxies up to z 0.84
- Cosmic evolution of radio-excess active galactic nuclei in quiescent and star-forming galaxies across 0 < z < 4
- Cosmic Evolution of Virial and Stellar Mass in Massive Early-type Galaxies
- Cosmological Constraints from Multiple Probes in the Dark Energy Survey
- Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data
- COSMOS2020: A Panchromatic View of the Universe to z 10 from Two Complementary Catalogs
- COSMOS2020: Cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z ~ 5
- COSMOS2020: Manifold learning to estimate physical parameters in large galaxy surveys
- COSMOS2020: The galaxy stellar mass function. The assembly and star formation cessation of galaxies at 0.2< z <= 7.5
- COSMOS2020: UV-selected galaxies at z >= 7.5
- COSMOS 5921+0638: characterization and analysis of a new strong gravitationally lensed AGN
- COSMOS: Hubble Space Telescope Observations
- COSMOS Morphological Classification with the Zurich Estimator of Structural Types (ZEST) and the Evolution Since z = 1 of the Luminosity Function of Early, Disk, and Irregular Galaxies
- Cosmos Photometric Redshifts with 30-Bands for 2-deg2
- COSMOS: Stochastic Bias from Measurements of Weak Lensing and Galaxy Clustering
- COSMOS: Three-dimensional Weak Lensing and the Growth of Structure
- COSMOS weak-lensing constraints on modified gravity
- COSMOS-Web: Intrinsically Luminous z 10 Galaxy Candidates Test Early Stellar Mass Assembly
- Counterparts of candidate dusty starbursts at z > 6
- Dark Energy Survey Y3 results: blending shear and redshift biases in image simulations
- Dark Energy Survey Year 1 results: the impact of galaxy neighbours on weak lensing cosmology with IM3SHAPE
- Dark Energy Survey Year 1 Results: The Photometric Data Set for Cosmology
- Dark Energy Survey Year 1 results: weak lensing shape catalogues
- Dark Energy Survey Year 3 Results: Deep Field optical + near-infrared images and catalogue
- Dark matter maps reveal cosmic scaffolding
- 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
- Deblending galaxies with variational autoencoders: A joint multiband, multi-instrument approach
- Deep Extragalactic VIsible Legacy Survey: Data Release 1 blended spectra search for candidate strong gravitational lenses
- Deep extragalactic visible legacy survey (DEVILS): stellar mass growth by morphological type since z = 1
- Deep GALEX Imaging of the COSMOS HST Field: A First Look at the Morphology of z ~ 0.7 Star-forming Galaxies
- Deep generative models for galaxy image simulations
- Deep Near-infrared Spectroscopy of Passively Evolving Galaxies at z >~ 1.4
- DEIMOS spectroscopy of z = 6 protocluster candidate in COSMOS - a massive protocluster embedded in a large-scale structure?
- Designing future dark energy space missions. I. Building realistic galaxy spectro-photometric catalogs and their first applications
- Determining the fraction of reddened quasars in COSMOS with multiple selection techniques from X-ray to radio wavelengths
- Different higher order kinematics between star-forming and quiescent galaxies based on the SAMI, MAGPI, and LEGA-C surveys
- Diffuse light in the young cluster of galaxies CL J1449+0856 at z = 2.07
- Digging into Dark Matter with Weak Gravitational Lensing
- Direct observational evidence for a large transient galaxy population in groups at 0.85 < z < 1
- Discovery of a rich proto-cluster at z = 2.9 and associated diffuse cold gas in the VIMOS Ultra-Deep Survey (VUDS)
- Discovery of bright z 7 galaxies in the UltraVISTA survey
- Discovery of Massive, Mostly Star Formation Quenched Galaxies with Extremely Large Lya Equivalent Widths at z ~ 3
- Distant galaxy clusters in the COSMOS field found by HIROCS
- Do gravitational lens galaxies have an excess of luminous substructure?
- Dust Attenuation, Bulge Formation, and Inside-out Quenching of Star Formation in Star-forming Main Sequence Galaxies at z ~ 2
- Dust giant: Extended and clumpy star-formation in a massive dusty galaxy at z = 1.38
- Dust Properties of C II Detected z ~ 5.5 Galaxies: New HST/WFC3 Near-IR Observations
- Early Science with the Large Millimeter Telescope: CO and C II Emission in the z = 4.3 AzTEC J095942.9+022938 (COSMOS AzTEC-1)
- Early-type Galaxies in the Chandra COSMOS Survey
- Edge-on galaxies in the HST COSMOS field: the evolution of stellar discs up to z 0.5
- Enhancement of the Spitzer Infrared Array Camera (IRAC) distortion correction for parallax measurements
- Environmental Effects in the Interaction and Merging of Galaxies in zCOSMOS
- Environmental Effects on the Stellar Mass Function in a z ~ 3.3 Overdensity of Galaxies in the COSMOS Field
- Environmental Impacts on the Rest-frame UV Size and Morphology of Star-forming Galaxies at z 2
- ESASky SSOSS: Solar System Object Search Service and the case of Psyche
- Euclid preparation. XIII. Forecasts for galaxy morphology with the Euclid Survey using deep generative models
- Euclid preparation - XXIII. Derivation of galaxy physical properties with deep machine learning using mock fluxes and H-band images
- Evidence for a Population of High-Redshift Submillimeter Galaxies from Interferometric Imaging
- Evidence for extended gaseous reservoirs around AGN at cosmic noon from ALMA CO(3-2) observations
- Evidence for major mergers of galaxies at 2 z < 4 in the VVDS and VUDS surveys
- Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang
- Evidence of the accelerated expansion of the Universe from weak lensing tomography with COSMOS
- Evolution in the Black Hole--Galaxy Scaling Relations and the Duty Cycle of Nuclear Activity in Star-forming Galaxies
- Evolution in the Dust Lane Fraction of Edge-on L* V Spiral Galaxies Since z = 0.8
- Evolution of blue E/S0 galaxies from z ~ 1: merger remnants or disk-rebuilding galaxies?
- Evolution of Blue E/S0 Galaxies from z ~ 1: Merger Remnants or Disk Rebuilding Galaxies?
- Evolution of the Bar Fraction in COSMOS: Quantifying the Assembly of the Hubble Sequence
- Evolution of the Fraction of Clumpy Galaxies at 0.2 < z < 1.0 in the COSMOS Field
- Evolution of the Frequency of Luminous (>=L*V) Close Galaxy Pairs at z < 1.2 in the COSMOS Field
- Evolution of the Quasar Luminosity Function over 3 < z < 5 in the COSMOS Survey Field
- Evolution of the specific star formation rate function at z< 1.4 Dissecting the mass-SFR plane in COSMOS and GOODS
- Evolution of the Spiral Structure of Galaxies from HST COSMOS Field Data
- Evolution of the Stellar-to-dark Matter Relation: Separating Star-forming and Passive Galaxies from z = 1 to 0
- Exploring the environment, magnetic fields, and feedback effects of massive high-redshift galaxies with C II
- Exploring the evolution of dust temperature using spectral energy distribution fitting in a large photometric survey
- Extended X-ray emission from non-thermal sources in the COSMOS field: a detailed study of a large radio galaxy at z= 1.168
- Extinction law in ultraluminous infrared galaxies at z~ 1
- Extreme emission-line galaxies out to z ~ 1 in zCOSMOS. I. Sample and characterization of global properties
- Fast rotating and low-turbulence discs at z 4.5: Dynamical evidence of their evolution into local early-type galaxies
- Feedback Regulated Star Formation in Cool Core Clusters of Galaxies
- FERENGI: Redshifting Galaxies from SDSS to GEMS, STAGES, and COSMOS
- Filling in the Quasar Redshift Gap at z ~ 5.5. II. A Complete Survey of Luminous Quasars in the Post-reionization Universe
- First Catalog of Strong Lens Candidates in the COSMOS Field
- First data release of the Hyper Suprime-Cam Subaru Strategic Program
- First HETDEX Spectroscopic Determinations of Lya and UV Luminosity Functions at z = 2-3: Bridging a Gap between Faint AGNs and Bright Galaxies
- First Results from the JWST Early Release Science Program Q3D: The Warm Ionized Gas Outflow in z 1.6 Quasar XID 2028 and Its Impact on the Host Galaxy
- Flat rotation curves and low velocity dispersions in KMOS star-forming galaxies at z ~ 1
- FMOS near-IR spectroscopy of Herschel-selected galaxies: star formation rates, metallicity and dust attenuation at z ~ 1
- Formation and evolution of early-type galaxies: spectro-photometry from cosmo-chemo-dynamical simulations
- From Images to Dark Matter: End-to-end Inference of Substructure from Hundreds of Strong Gravitational Lenses
- G10/COSMOS: 38 band (far-UV to far-IR) panchromatic photometry using LAMBDAR
- Galactic winds and stellar populations in Lyman a emitting galaxies at z ~ 3.1
- Galaxies at redshifts 5 to 6 with systematically low dust content and high C II emission
- Galaxies Probing Galaxies in PRIMUS. I. Sample, Spectroscopy, and Characteristics of the zsim 0.5 Mg II-absorbing Circumgalactic Medium
- Galaxy classification: deep learning on the OTELO and COSMOS databases
- Galaxy Clusters at High Redshift and Evolution of Brightest Cluster Galaxies
- Galaxy number counts and implications for strong lensing
- Galaxy populations in massive galaxy clusters to z = 1.1: colour distribution, concentration, halo occupation number and red sequence fraction
- Galaxy Stellar Mass Assembly Between 0.2 < z < 2 from the S-COSMOS Survey
- Galaxy Structure and Mode of Star Formation in the SFR-Mass Plane from z ~ 2.5 to z ~ 0.1
- Galaxy-wide outflows in z ~ 1.5 luminous obscured quasars revealed through near-IR slit-resolved spectroscopy
- Galaxy Zoo: an independent look at the evolution of the bar fraction over the last eight billion years from HST-COSMOS
- Galaxy Zoo: Are bars responsible for the feeding of active galactic nuclei at 0.2 < z < 1.0?
- Galaxy Zoo: morphological classifications for 120 000 galaxies in HST legacy imaging
- GALFIT-ing AGN Host Galaxies in COSMOS: HST versus Subaru
- Giant Metrewave Radio Telescope observations of neutral atomic hydrogen gas in the COSMOS field at z ~ 0.37
- GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with 4,000,000 Galaxies at z 2-7: Galaxy-AGN Transition, Star Formation Efficiency, and Implication for Evolution at z > 10
- Gravitational lenses and lens candidates identified from the COSMOS field
- Gravitational lensing in the supernova legacy survey (SNLS)
- GREAT3 results - I. Systematic errors in shear estimation and the impact of real galaxy morphology
- Green Galaxies in the COSMOS Field
- HALO7D II: The Halo Velocity Ellipsoid and Velocity Anisotropy with Distant Main-sequence Stars
- Harnessing the Hubble Space Telescope Archives: A Catalog of 21,926 Interacting Galaxies
- hCOSMOS: A Dense Spectroscopic Survey of r <= 21.3 Galaxies in the COSMOS field
- HETDEX Public Source Catalog 1: 220 K Sources Including Over 50 K Lya Emitters from an Untargeted Wide-area Spectroscopic Survey
- Highest Redshift Image of Neutral Hydrogen in Emission: A CHILES Detection of a Starbursting Galaxy at z = 0.376
- HiZELS: a high-redshift survey of Ha emitters - II. The nature of star-forming galaxies at z = 0.84
- HOLISMOKES. II. Identifying galaxy-scale strong gravitational lenses in Pan-STARRS using convolutional neural networks
- Host Galaxy and Nuclear Properties of IR-selected AGNs with and without Outflow Signatures
- Host Galaxy Identification for Supernova Surveys
- Host galaxy properties and environment of obscured and unobscured X-ray selected active galactic nuclei in the COSMOS survey
- HR-COSMOS: Kinematics of star-forming galaxies at z 0.9
- 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
- Hubble Space Telescope/Advanced Camera for Surveys Morphology of Lya Emitters at Redshift 5.7 in the COSMOS Field
- Ha and 4000 A Break Measurements for ~3500 K-selected Galaxies at 0.5 < z < 2.0
- Ha Emitting Galaxies at z ~ 0.6 in the Deep And Wide Narrow-band Survey
- Identification of Two Bright z > 3 Submillimeter Galaxy Candidates in the COSMOS Field
- Impact of point spread function higher moments error on weak gravitational lensing
- In and out star formation in z 1.5 quiescent galaxies from rest-frame UV spectroscopy and the far-infrared
- Infrared Selection of Obscured Active Galactic Nuclei in the COSMOS Field
- Intrinsic galaxy shapes and alignments - I. Measuring and modelling COSMOS intrinsic galaxy ellipticities
- Inverse stellar population age gradients of post-starburst galaxies at z = 0.8 with LEGA-C
- Investigating Clumpy Galaxies in the Sloan Digital Sky Survey Stripe 82 Using the Galaxy Zoo
- Investigating evidence for different black hole accretion modes since redshift z ~ 1
- Investigating the Effect of Galaxy Interactions on the Enhancement of Active Galactic Nuclei at 0.5 < z < 3.0
- Ionised gas structure of 100 kpc in an over-dense region of the galaxy group COSMOS-Gr30 at z 0.7
- Joint Survey Processing. II. Stellar Proper Motions in the COSMOS Field from Hubble Space Telescope ACS and Subaru Telescope HSC Observations
- KASHz: No evidence for ionised outflows instantaneously suppressing star formation in moderate luminosity AGN at z ~ 1.4-2.6
- KiDS-1000: Constraints on the intrinsic alignment of luminous red galaxies
- KiDS+VIKING-450: An internal-consistency test for cosmic shear tomography with a colour-based split of source galaxies
- KROSS: mapping the Ha emission across the star formation sequence at z 1
- Larger sizes of massive quiescent early-type galaxies in clusters than in the field at 0.8 < z < 1.5
- Large-scale fluctuations in the number density of galaxies in independent surveys of deep fields
- Large-scale Structure around a z=2.1 Cluster
- Large-scale Structures in COSMOS2020: Evolution of Star Formation Activity in Different Environments at 0.4 < z < 4
- Late-Stage Galaxy Mergers in Cosmos to z ~ 1
- LEGA-C: Analysis of Dynamical Masses from Ionized Gas and Stellar Kinematics at z 0.8
- LensFlow: A Convolutional Neural Network in Search of Strong Gravitational Lenses
- Linking black hole growth with host galaxies: the accretion-stellar mass relation and its cosmic evolution
- Long tidal tails in merging galaxies and their implications
- Luminous Red Galaxies: Selection and Classification By Combining Optical and Infrared Photometry
- Luminous Satellites. II. Spatial Distribution, Luminosity Function, and Cosmic Evolution
- Lyman Break and ultraviolet-selected galaxies at z ~ 1 - II. PACS 100 mm/160 mm FIR detections
- Lyman break and ultraviolet-selected galaxies at z ~ 1 - I. Stellar populations from the ALHAMBRA survey
- Lyman continuum escape fraction of faint galaxies at z 3.3 in the CANDELS/GOODS-North, EGS, and COSMOS fields with LBC
- Magnification by Galaxy Group Dark Matter Halos
- Major-merger Galaxy Pairs in the COSMOS Field--Mass-dependent Merger Rate Evolution since z = 1
- Mapping Obscuration to Reionization with ALMA (MORA): 2 mm Efficiently Selects the Highest-redshift Obscured Galaxies
- Mass assembly in quiescent and star-forming galaxies since z 4 from UltraVISTA
- Measuring Structural Parameters Through Stacking Galaxy Images
- Measuring the Geometry of the Universe from Weak Gravitational Lensing behind Galaxy Groups in the HST COSMOS Survey
- Merger induced clump formation in distant infrared luminous starburst galaxies
- Merging Galaxies with Tidal Tails in COSMOS to z = 1
- Method for analyzing the spatial distribution of galaxies on gigaparsec scales. II. Application to a grid of the HUDF-FDF-COSMOS-HDF surveys
- Method for improving line flux and redshift measurements with narrowband filters
- Mid-infrared Selection of Active Galactic Nuclei with the Wide-Field Infrared Survey Explorer. I. Characterizing WISE-selected Active Galactic Nuclei in COSMOS
- MIGHTEE: the nature of the radio-loud AGN population
- Minor Mergers or Progenitor Bias? The Stellar Ages of Small and Large Quenched Galaxies
- Mitigating bias in deep learning: training unbiased models on biased data for the morphological classification of galaxies
- MMT spectroscopy of Lyman-alpha at z 7: evidence for accelerated reionization around massive galaxies
- Modeling intrinsic galaxy alignment in the MICE simulation
- Molecular Gas Contents and Scaling Relations for Massive, Passive Galaxies at Intermediate Redshifts from the LEGA-C Survey
- Molecular Gas in a Submillimeter Galaxy at z = 4.5: Evidence for a Major Merger at 1 Billion Years after the Big Bang
- Molecular gas in distant brightest cluster galaxies
- Molecular gas in radio galaxies in dense megaparsec-scale environments at z = 0.4-2.6
- Molecular Gas Reservoirs in Massive Quiescent Galaxies at z 0.7 Linked to Late-time Star Formation
- Morphological Evolution of the Hosts of Far-infrared/Submillimeter Galaxies
- Morphological evolution of z ~ 1 galaxies from deep K-band AO imaging in the COSMOS deep field
- Morphological Properties of Lya Emitters at Redshift 4.86 in the Cosmos Field: Clumpy Star Formation or Merger?
- Morphological properties of star-forming galaxies: Connecting the morphological evolution of galaxies and the decline of the star formation rate density of the Universe in the past 9 billion years
- Morphologies of Radio-, X-ray-, and Mid-infrared-selected Active Galactic Nuclei
- Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology
- Multiobject Spectroscopy of Young Star Clusters in NGC 4676
- Multiresolution angular momentum measurements of z 1.5-2 star-forming galaxies
- Multiwavelength dissection of a massive heavily dust-obscured galaxy and its blue companion at z~2
- Narrow-line X-Ray-selected Galaxies in the Chandra-COSMOS Field. I. Optical Spectroscopic Catalog
- New Constraints on the Evolution of the Stellar-to-dark Matter Connection: A Combined Analysis of Galaxy-Galaxy Lensing, Clustering, and Stellar Mass Functions from z = 0.2 to z =1
- New criteria for the selection of galaxy close pairs from cosmological simulations: evolution of the major and minor merger fraction in MUSE deep fields
- New insights from deep VLA data on the potentially recoiling black hole CID-42 in the COSMOS field
- Newly Quenched Galaxies as the Cause for the Apparent Evolution in Average Size of the Population
- No evidence for Population III stars or a Direct Collapse Black Hole in the z = 6.6 Lyman-a emitter CR7
- Noise-based Detection and Segmentation of Nebulous Objects
- Non-linearity and environmental dependence of the star-forming galaxies main sequence
- Normal, dust-obscured galaxies in the epoch of reionization
- Obscured active galactic nuclei triggered in compact star-forming galaxies
- Obscured AGN at z ~ 1 from the zCOSMOS-Bright Survey. I. Selection and optical properties of a Ne v-selected sample
- Obscured GOODS Active Galactic Nuclei and Their Host Galaxies at z < 1.25: The Slow Black Hole Growth Phase
- Obscured star formation in bright z 7 Lyman-break galaxies
- Of Genes and Machines: Application of a Combination of Machine Learning Tools to Astronomy Data Sets
- Ongoing growth of the brightest cluster galaxies via major dry mergers in the last ~6 Gyr
- On the Gas Content, Star Formation Efficiency, and Environmental Quenching of Massive Galaxies in Protoclusters at z 2.0-2.5
- On the nature of Ha emitters at z ~ 2 from the HiZELS survey: physical properties, Lya escape fraction and main sequence
- On the UV compactness and morphologies of typical Lyman a emitters from z ~ 2 to z ~ 6
- Optical Selection of Faint Active Galactic Nuclei in the COSMOS Field
- Panchromatic spectral energy distributions of Herschel sources
- Pan-STARRS1 variability of XMM-COSMOS AGN. I. Impact on photometric redshifts
- Perturbative reconstruction of a gravitational lens: when mass does not follow light
- PHIBSS2: survey design and z = 0.5 - 0.8 results. Molecular gas reservoirs during the winding-down of star formation
- Photometric Redshift and Classification for the XMM-COSMOS Sources
- Photo-z-SQL: Integrated, flexible photometric redshift computation in a database
- Physical and Morphological Properties of O II Emitting Galaxies in the HETDEX Pilot Survey
- Physical Characterization of an Unlensed, Dusty Star-forming Galaxy at z = 5.85
- Physical Properties of Lya Emitters at z ~ 0.3 from UV-to-FIR Measurements
- Physical properties of z > 4 submillimeter galaxies in the COSMOS field
- Pixelated Reconstruction of Foreground Density and Background Surface Brightness in Gravitational Lensing Systems Using Recurrent Inference Machines
- Pixel-based correction for Charge Transfer Inefficiency in the Hubble Space Telescope Advanced Camera for Surveys
- Precision simulation of ground-based lensing data using observations from space
- Predicting emission line fluxes and number counts of distant galaxies for cosmological surveys
- Probabilistic Association of Transients to their Hosts (PATH)
- Properties of IR-selected active galactic nuclei
- Protoclusters as drivers of stellar mass growth in the early Universe, a case study: Taralay - a massive protocluster at z 4.57
- Pushing the limits of the Gaia space mission by analyzing galaxy morphology
- Quantifying the abundance of faint, low-redshift satellite galaxies in the COSMOS survey
- Quiescent Compact Galaxies at Intermediate Redshift in the COSMOS Field. II. The Fundamental Plane of Massive Galaxies
- Quiescent Compact Galaxies at Intermediate Redshift in the COSMOS Field. The Number Density
- Radio and far-IR emission associated with a massive star-forming galaxy candidate at z 6.8: a radio-loud AGN in the reionization era?
- Radio-optical galaxy shape correlations in the COSMOS field
- Rates and Properties of Supernovae Strongly Gravitationally Lensed by Elliptical Galaxies in Time-domain Imaging Surveys
- Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at 1.5 < z < 6.4
- Redshift and stellar mass dependence of intrinsic shapes of disc-dominated galaxies from COSMOS observations below z = 1.0
- Revealing the cosmic evolution of boxy/peanut-shaped bulges from HST COSMOS and SDSS
- Revealing the Impact of Critical Stellar Central Density on Galaxy Quenching through Cosmic Time
- Revealing the relation between black hole growth and host-galaxy compactness among star-forming galaxies
- Revisiting Galaxy Evolution in Morphology in the Cosmic Evolution Survey Field (COSMOS-ReGEM). I. Merging Galaxies
- RINGFINDER: Automated Detection of Galaxy-scale Gravitational Lenses in Ground-based Multi-filter Imaging Data
- Satellites in the field and lens galaxies: SDSS/COSMOS versus SLACS/CLASS
- SDSS-IV/SPIDERS: A catalogue of X-ray selected AGN properties. Spectral properties and black hole mass estimates for SPIDERS SDSS DR14 type 1 AGN
- Search of strong lens systems in the Dark Energy Survey using convolutional neural networks
- Secular Evolution and a Non-evolving Black-hole-to-galaxy Mass Ratio in the Last 7 Gyr
- Seeing in the dark - II. Cosmic shear in the Sloan Digital Sky Survey
- Sersic galaxy models in weak lensing shape measurement: model bias, noise bias and their interaction
- Shapes of galaxies hosting radio-loud AGNs with z <= 1
- SHELS: Testing Weak-Lensing Maps with Redshift Surveys
- Simulating the Cosmos: The Fraction of Merging Galaxies at High Redshift
- SINFONI spectra of heavily obscured AGNs in COSMOS: Evidence of outflows in a MIR/O target at z ~ 2.5
- Size evolution of star-forming galaxies with 2 <z < 4.5 in the VIMOS Ultra-Deep Survey
- Sizing up Lya and Lyman Break Galaxies
- Spatially Resolved Stellar Kinematics from LEGA-C: Increased Rotational Support in z ~ 0.8 Quiescent Galaxies
- Spectral Energy Distribution Fitting of HETDEX Pilot Survey Lya Emitters in COSMOS and GOODS-N
- Spectral Energy Distributions of Low-luminosity Radio Galaxies at z ~1-3: A High-z View of the Host/AGN Connection
- Spectral Energy Distributions of Type 1 Active Galactic Nuclei in the COSMOS Survey. I. The XMM-COSMOS Sample
- Spectral Energy Distributions of Type 1 AGNs
- Spectroscopic Confirmation of an Extreme Starburst at Redshift 4.547
- Spectroscopic Confirmation of an Ultra Massive and Compact Galaxy at z = 3.35: a Detailed Look at an Early Progenitor of Local Giant Ellipticals
- Spectroscopic observations of PHz G237.01+42.50: A galaxy protocluster at z = 2.16 in the Cosmos field
- Spectroscopic Study of Star-forming Galaxies in Filaments and the Field at z ~ 0.5: Evidence for Environmental Dependence of Electron Density
- Spectroscopy of Luminous z > 7 Galaxy Candidates and Sources of Contamination in z > 7 Galaxy Searches
- Starburst galaxies in the COSMOS field: clumpy star-formation at redshift 0 < z < 0.5
- Starburst to Quiescent from HST/ALMA: Stars and Dust Unveil Minor Mergers in Submillimeter Galaxies at z ~ 4.5
- Star formation and AGN activity in the most luminous LINERs in the local universe
- Star formation histories of UV-luminous galaxies at z 6.8: implications for stellar mass assembly at early cosmic times
- Star formation in far-IR AGN and non-AGN galaxies in the green valley - II. Morphological analysis
- Star Formation in LINER Host Galaxies at z ~ 0.3
- Star formation of far-IR AGN and non-AGN galaxies in the green valley: possible implication of AGN positive feedback
- Star formation quenching in green valley galaxies at 0.5 z 1.0 and constraints with galaxy morphologies
- Star Formation Rates in Lyman Break Galaxies: Radio Stacking of LBGs in the COSMOS Field and the Sub-mJy Radio Source Population
- Star-Galaxy Classification in Multi-band Optical Imaging
- Star-galaxy classification in the Dark Energy Survey Y1 data set
- Stars, Gas, and Star Formation of Distant Post-starburst Galaxies
- Stellar angular momentum of disk galaxies at z 0.7 in the MAGIC survey. I. Impact of the environment
- Stellar Dynamical Models for 797 z 0.8 Galaxies from LEGA-C
- Stellar Populations in type Ia supernova host galaxies at intermediate-high redshift: Star formation and metallicity enrichment histories
- Stellar populations of galaxies in the ALHAMBRA survey up to z ~ 1. IV. Properties of quiescent galaxies on the stellar mass-size plane
- Strange quasar candidates with abnormal astrometric characteristics from Gaia EDR3 and SDSS (SQUAB-II): optical identifications
- Strong lensing in UNIONS: Toward a pipeline from discovery to modeling
- Strongly lensed candidates from the HSC transient survey
- Strong Lyman-a emission in an overdense region at z = 6.8: a very large (R 3 physical Mpc) ionized bubble in COSMOS?
- Studying Large- and Small-Scale Environments of Ultraviolet Luminous Galaxies
- Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). II. Discovery of 32 quasars and luminous galaxies at 5.7 < z <= 6.8
- Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). V. Quasar Luminosity Function and Contribution to Cosmic Reionization at z = 6
- Subaru Hyper Suprime-Cam revisits the large-scale environmental dependence on galaxy morphology over 360 deg2 at z = 0.3-0.6
- (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies. IV. Physical properties derived from spectral energy distributions
- Supercal: Cross-calibration of Multiple Photometric Systems to Improve Cosmological Measurements with Type Ia Supernovae
- Supermassive black hole activity in the Cosmic Evolution Survey
- Survey of Gravitationally Lensed Objects in HSC Imaging (SuGOHI) - VII. Discovery and confirmation of three strongly lensed quasars
- Target Selection and Validation of DESI Quasars
- Testing the Breathing Mode in Intermediate-mass Galaxies and Its Predicted Star Formation Rate-size Anti-correlation
- Testing the surface brightness fluctuation method on dwarf galaxies in the COSMOS field
- The Accretion History of AGN: The Spectral Energy Distributions of X-Ray-luminous Active Galactic Nuclei
- The Advanced Camera for Surveys General Catalog: Structural Parameters for Approximately Half a Million Galaxies
- The Ages, Metallicities, and Element Abundance Ratios of Massive Quenched Galaxies at z 1.6
- The ALHAMBRA Survey: Bayesian photometric redshifts with 23 bands for 3 deg
- The ALHAMBRA survey: reliable morphological catalogue of 22 051 early- and late-type galaxies
- The ALMA-ALPINE CII survey: Kennicutt-Schmidt relation in four massive main-sequence galaxies at z ~ 4.5
- The ALPINE-ALMA CII survey. Circumgalactic medium pollution and gas mixing by tidal stripping in a merging system at z ~ 4.57
- The ALPINE-ALMA CII survey: Data processing, catalogs, and statistical source properties
- The ALPINE-ALMA C II survey: Investigation of 10 galaxies at z 4.5 with O II and C II line emission - ISM properties and O II-SFR relation
- The ALPINE-ALMA C II survey. Luminosity function of serendipitous C II line emitters at z ~ 5
- The ALPINE-ALMA C II Survey: Multiwavelength Ancillary Data and Basic Physical Measurements
- The ALPINE-ALMA CII survey. Survey strategy, observations, and sample properties of 118 star-forming galaxies at 4 < z < 6
- 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 Angular Clustering of WISE-selected Active Galactic Nuclei: Different Halos for Obscured and Unobscured Active Galactic Nuclei
- The Angular Correlations of Galaxies in the COSMOS Field
- The angular momentum of disc galaxies at z = 1
- The Assembly History of Disk Galaxies. II. Probing the Emerging Tully-Fisher Relation during 1 < z < 1.7
- The AzTEC/SMA Interferometric Imaging Survey of Submillimeter-selected High-redshift Galaxies
- The bolometric output and host-galaxy properties of obscured AGN in the XMM-COSMOS survey
- The bright end of the galaxy luminosity function at z7: before the onset of mass quenching?
- The Brightest Galaxies in the Dark Ages: Galaxies Dust Continuum Emission during the Reionization Era
- The Brightest z 8 Galaxies over the COSMOS UltraVISTA Field
- The Buildup of the Hubble Sequence in the Cosmos Field
- The Bulk of the Black Hole Growth Since z ~ 1 Occurs in a Secular Universe: No Major Merger-AGN Connection
- The CALYMHA survey: Lya escape fraction and its dependence on galaxy properties at z = 2.23
- The CFHTLS-Deep Catalog of Interacting Galaxies. I. Merger Rate Evolution to z = 1.2
- The CFHTLS strong lensing legacy survey. I. Survey overview and T0002 release sample
- The CFHTLS-Strong Lensing Legacy Survey (SL2S): Investigating the Group-scale Lenses with the SARCS Sample
- The Chandra COSMOS Legacy Survey: Compton thick AGN at high redshift
- The Chandra COSMOS Legacy survey: optical/IR identifications
- The Chandra COSMOS Survey. III. Optical and Infrared Identification of X-Ray Point Sources
- The Chandra-COSMOS survey - IV. X-ray spectra of the bright sample
- The Colors and Sizes of Recently Quenched Galaxies: A Result of Compact Starburst before Quenching
- The Compact Structures of Massive z ~ 0.7 Post-starburst Galaxies in the SQuIGG$vec{L}$E Sample
- The Cosmic Evolution of Faint Satellite Galaxies as a Test of Galaxy Formation and the Nature of Dark Matter
- The Cosmic Evolution Survey (COSMOS): A Large-Scale Structure at z=0.73 and the Relation of Galaxy Morphologies to Local Environment
- The Cosmic Evolution Survey (COSMOS): Overview
- The Cosmic Evolution Survey (COSMOS): The Morphological Content and Environmental Dependence of the Galaxy Color-Magnitude Relation at z ~ 0.7
- The COSMOS Survey: Hubble Space Telescope Advanced Camera for Surveys Observations and Data Processing
- The dark matter haloes of moderate luminosity X-ray AGN as determined from weak gravitational lensing and host stellar masses
- The debiased morphological transformations of galaxies since z = 3 in CANDELS
- The DEIMOS 10K Spectroscopic Survey Catalog of the COSMOS Field
- The Dependence of Galactic Outflows on the Properties and Orientation of zCOSMOS Galaxies at z ~ 1
- The dependence of star formation activity on environment and stellar mass at z~ 1 from the HiZELS-Ha survey
- The Dependence of Star Formation Activity on Stellar Mass Surface Density and Sersic Index in zCOSMOS Galaxies at 0.5 < z < 0.9 Compared with SDSS Galaxies at 0.04 < z < 0.08
- The dominant role of mergers in the size evolution of massive early-type galaxies since z ~ 1
- The Effect of Environment on the Properties of the Most Massive Galaxies at 0.5 < z < 2.5 in the COSMOS-DASH Field
- The Effects of Environment on Morphological Evolution at 0<z<1.2 in the COSMOS Survey
- The Estimation of Star Formation Rates and Stellar Population Ages of High-redshift Galaxies from Broadband Photometry
- The Evolution of Early- and Late-type Galaxies in the Cosmic Evolution Survey up to z 1.2
- The evolution of gas-phase metallicity and resolved abundances in star-forming galaxies at z 0.6-1.8
- The Evolution of the Luminosity Function for Luminous Compact Blue Galaxies to z = 1
- The evolution of the mass-size relation for early-type galaxies from z ~ 1 to the present: dependence on environment, mass range and detailed morphology
- The Evolution of the Number Density of Large Disk Galaxies in COSMOS
- The Evolution of the Quenching of Star Formation in Cluster Galaxies since z ~ 1
- The faint end of the red sequence galaxy luminosity function: unveiling surface brightness selection effects with the CLASH clusters
- The Faint-End Slopes of Galaxy Luminosity Functions in the COSMOS Field
- The faint radio sky: VLBA observations of the COSMOS field
- The First Release COSMOS Optical and Near-IR Data and Catalog
- The first-year shear catalog of the Subaru Hyper Suprime-Cam Subaru Strategic Program Survey
- The FMOS-COSMOS Survey of Star-forming Galaxies at z~1.6. III. Survey Design, Performance, and Sample Characteristics
- The Fundamental Plane in the LEGA-C Survey: Unraveling the M/L Ratio Variations of Massive Star-forming and Quiescent Galaxies at z ~ 0.8
- The HETDEX Pilot Survey. II. The Evolution of the Lya Escape Fraction from the Ultraviolet Slope and Luminosity Function of 1.9 < z < 3.8 LAEs
- The HETDEX Pilot Survey. IV. The Evolution of O II Emitting Galaxies from z ~ 0.5 to z ~ 0
- The Ha Luminosity Function and Star Formation Rate at z 0.24 in the COSMOS 2 Square Degree Field
- The impact from survey depth and resolution on the morphological classification of galaxies
- The impact of cosmic variance on simulating weak lensing surveys
- The Impact of Galaxy Interactions on Active Galactic Nucleus Activity in zCOSMOS
- The impact of satellite trails on Hubble Space Telescope observations
- The Intrinsic Scatter along the Main Sequence of Star-forming Galaxies at z ~ 0.7
- The KMOS Redshift One Spectroscopic Survey (KROSS): rotational velocities and angular momentum of z 0.9 galaxies
- The Large Early Galaxy Astrophysics Census (LEGA-C) Data Release 2: Dynamical and Stellar Population Properties of z 1 Galaxies in the COSMOS Field
- The Large Early Galaxy Astrophysics Census (LEGA-C) Data Release 3: 3000 High-quality Spectra of Ks-selected Galaxies at z > 0.6
- The Luminosity and Mass Functions of Low-mass Stars in the Galactic Disk. II. The Field
- The luminosity functions and redshift evolution of satellites of low-mass galaxies in the COSMOS survey
- The Lyman continuum escape fraction of galaxies at z = 3.3 in the VUDS-LBC/COSMOS field
- The Mass Scale of High-redshift Galaxies: Virial Mass Estimates Calibrated with Stellar Dynamical Models from LEGA-C
- The measurement and applications of the faint source correlation function
- The Merian survey: design, construction, and characterization of a filter set optimized to find dwarf galaxies and measure their dark matter halo properties with weak lensing
- The Metallicity Evolution of Blue Compact Dwarf Galaxies from the Intermediate Redshift to the Local Universe
- The missing satellite problem in 3D
- The Molecular Gas Content and Fuel Efficiency of Starbursts at z ~ 1.6 with ALMA
- The morphological mix of dwarf galaxies in the nearby Universe
- The morphology of galaxies in the Baryon Oscillation Spectroscopic Survey
- The Most Massive Galaxies at 3.0 <= z < 4.0 in the Newfirm Medium-band Survey: Properties and Improved Constraints on the Stellar Mass Function
- The most obscured AGN in the COSMOS field
- The Nature of Optically Dull Active Galactic Nuclei in COSMOS
- The NEWFIRM Medium-band Survey: Photometric Catalogs, Redshifts, and the Bimodal Color Distribution of Galaxies out to z ~ 3
- The Number Densities and Stellar Populations of Massive Galaxies at 3 < z < 6: A Diverse, Rapidly Forming Population in the Early Universe
- The Obscured Fraction of Active Galactic Nuclei in the XMM-COSMOS Survey: A Spectral Energy Distribution Perspective
- The O III Profiles of Far-infrared Active and Inactive Optically Selected Green Valley Galaxies
- The Opacity of Galactic Disks at z ~ 0.7
- The Optical Spectra of 24 mm Galaxies in the COSMOS Field. I. Spitzer MIPS Bright Sources in the zCOSMOS-Bright 10k Catalog
- The Palomar Transient Factory Core-collapse Supernova Host-galaxy Sample. I. Host-galaxy Distribution Functions and Environment Dependence of Core-collapse Supernovae
- The PAU survey: star-galaxy classification with multi narrow-band data
- The Physical Properties of Luminous z 8 Galaxies and Implications for the Cosmic Star Formation Rate Density from 0.35 deg2 of (Pure-)Parallel HST Observations
- The physical scale of the far-infrared emission in the most luminous submillimetre galaxies - II. Evidence for merger-driven star formation
- The possible evolution of pitch angles of spiral galaxies
- The Pre-He White Dwarf in the Post-mass Transfer Binary EL CVn
- The production and escape of Lyman-Continuum radiation from star-forming galaxies at z ~ 2 and their redshift evolution
- The properties of AGN in dwarf galaxies identified via SED fitting
- The Quasar-LBG Two-point Angular Cross-correlation Function at z~4 in the COSMOS Field
- The Quasar Luminosity Function at z 5 via Deep Learning and Bayesian Information Criterion
- The radio-loud AGN population at z 1 in the COSMOS field. I. selection and spectral energy distributions
- The rapid transition from star formation to AGN-dominated rest-frame ultraviolet light at z 4
- The Recent Burstiness of Star Formation in Galaxies at z ~ 4.5 from Ha Measurements
- The Redshift Evolution of Early-Type Galaxies in COSMOS: Do Massive Early-Type Galaxies Form by Dry Mergers?
- The redshift evolution of major merger triggering of luminous AGNs: a slight enhancement at z ~ 2
- The redshift evolution of the S0 fraction for z < 1 in COSMOS
- The Rise and Fall of Passive Disk Galaxies: Morphological Evolution Along the Red Sequence Revealed by COSMOS
- The Role of Bars in AGN Fueling in Disk Galaxies Over the Last Seven Billion Years
- The Role of Galaxy Interaction in the SFR-M * Relation: Characterizing Morphological Properties of Herschel-selected Galaxies at 0.2 < z < 1.5
- The role of interactions in the formation and evolution of galaxies
- The Shear Testing Programme 2: Factors affecting high-precision weak-lensing analyses
- The Size-Mass Relation at Rest-frame 1.5 mm from JWST/NIRCam in the COSMOS-WEB and PRIMER-COSMOS Fields
- The Spectrally Resolved Lya Emission of Three Lya-selected Field Galaxies at z ~ 2.4 from the HETDEX Pilot Survey
- The Stability of the Point-Spread Function of the Advanced Camera for Surveys on the Hubble Space Telescope and Implications for Weak Gravitational Lensing
- The Stellar-age Dependence of X-Ray Emission from Normal Star-forming Galaxies in the GOODS Fields
- The stellar and dark matter distributions in elliptical galaxies from the ensemble of strong gravitational lenses
- The Stellar Content of the COSMOS Field as Derived from Morphological and SED-based Star/Galaxy Separation
- The stellar mass function of quiescent galaxies in 2 < z < 2.5 protoclusters
- The Stellar Mass Fundamental Plane and Compact Quiescent Galaxies at z < 0.6
- The Stellar-to-halo Mass Ratios of Passive and Star-forming Galaxies at z ~ 2-3 from the SMUVS Survey
- The stellar-to-halo mass relation over the past 12 Gyr. I. Standard LCDM model
- The Strength of the 2175 A Feature in the Attenuation Curves of Galaxies at 0.1 < z 3
- The structural and size evolution of star-forming galaxies over the last 11 Gyr
- The structural properties of nearby dwarf galaxies in low-density environments - size, surface brightness, and colour gradients
- The structures of distant galaxies - III. The merger history of over 20000 massive galaxies at z < 1.2
- The Third Gravitational Lensing Accuracy Testing (GREAT3) Challenge Handbook
- The Tully-Fisher relation in dense groups at z ~ 0.7 in the MAGIC survey
- The UV luminosity functions of bright z > 8 galaxies: determination from 0.41 deg2 of HST observations along 300 independent sightlines
- The Velocity Dispersion Function for Massive Quiescent and Star-forming Galaxies at 0.6 < z <= 1.0
- The VIMOS Ultra-Deep Survey: ~10 000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2 < z 6
- The VIMOS Ultra-Deep Survey: A major merger origin for the high fraction of galaxies at 2 < z < 6 with two bright clumps
- The VIMOS Ultra-Deep Survey: Emerging from the dark, a massive proto-cluster at z 4.57
- The VIMOS Ultra-Deep Survey: evidence for AGN feedback in galaxies with CIII-l1908 A emission 10.8 to 12.5 Gyr ago
- The VLA-COSMOS 3 GHz Large Project: Evolution of Specific Star Formation Rates out to z ~ 5
- The VLA-COSMOS Perspective on the Infrared-Radio Relation. I. New Constraints on Selection Biases and the Non-Evolution of the Infrared/Radio Properties of Star-Forming and Active Galactic Nucleus Galaxies at Intermediate and High Redshift
- The VLA-COSMOS Survey. I. Radio Identifications from the Pilot Project
- The VLT LEGA-C Spectroscopic Survey: The Physics of Galaxies at a Lookback Time of 7 Gyr
- The XMM-Newton Wide-Field Survey in the COSMOS Field. III. Optical Identification and Multiwavelength Properties of a Large Sample of X-Ray-Selected Sources
- The XMM-Newton Wide-Field Survey in the COSMOS Field. IV. X-Ray Spectral Properties of Active Galactic Nuclei
- The XMM-Newton Wide-field Survey in the Cosmos Field (XMM-COSMOS): Demography and Multiwavelength Properties of Obscured and Unobscured Luminous Active Galactic Nuclei
- The zCOSMOS redshift survey: evolution of the light in bulges and discs since z ~ 0.8
- The zCOSMOS redshift survey: the role of environment and stellar mass in shaping the rise of the morphology-density relation from z ~ 1
- The zCOSMOS redshift survey: the three-dimensional classification cube and bimodality in galaxy physical properties
- The zCOSMOS-SINFONI Project. I. Sample Selection and Natural-seeing Observations
- The zCOSMOS survey: the role of the environment in the evolution of the luminosity function of different galaxy types
- Three Dusty Star-forming Galaxies at z ~ 1.5: Mergers and Disks on the Main Sequence
- Three Lyman-a-emitting filaments converging to a massive galaxy group at z = 2.91: discussing the case for cold gas infall
- Towards emulating cosmic shear data: revisiting the calibration of the shear measurements for the Kilo-Degree Survey
- Tracing outflows in the AGN forbidden region with SINFONI
- Two Massive, Compact, and Dust-obscured Candidate z 8 Galaxies Discovered by JWST
- Two years of optical and NIR observations of the superluminous supernova UID 30901 discovered by the UltraVISTA SN survey
- Ultradeep IRAC Imaging Over the HUDF and GOODS-South: Survey Design and Imaging Data Release
- Ultraluminous X-ray sources out to z ~ 0.3 in the COSMOS field
- Ultramassive dense early-type galaxies: Velocity dispersions and number density evolution since z = 1.6
- UltraVISTA: a new ultra-deep near-infrared survey in COSMOS
- Uncovering a Massive z 7.7 Galaxy Hosting a Heavily Obscured Radio-loud Active Galactic Nucleus Candidate in COSMOS-Web
- Understanding the Unique Assembly History of Central Group Galaxies
- Unveiling Sizes of Compact AGN Hosts with ALMA
- Unveiling the nature of bright z 7 galaxies with the Hubble Space Telescope
- Variability-selected active galactic nuclei in the VST-SUDARE/VOICE survey of the COSMOS field
- VIS3COS. II. Nature and nurture in galaxy structure and morphology
- Weak gravitational lensing shear measurement with FPFS: analytical mitigation of noise bias and selection bias
- Weak Gravitational Lensing with COSMOS: Galaxy Selection and Shape Measurements
- Weak Lensing Calibrated M-T Scaling Relation of Galaxy Groups in the COSMOS Fieldsstarf
- Weak lensing from space: first cosmological constraints from three-point shear statistics
- Weak-lensing mass reconstruction using sparsity and a Gaussian random field
- Weak Lensing Measurement of Galaxy Clusters in the CFHTLS-Wide Survey
- Weak lensing shear calibration with simulations of the HSC survey
- What is the Physical Origin of Strong Lya Emission? I. Demographics of Lya Emitter Structures
- What is the Physical Origin of Strong Lya Emission? II. Gas Kinematics and Distribution of Lya Emitters
- X-ray selected narrow-line active galactic nuclei in the COSMOS field: Nature of optically dull active galactic nuclei
- X-shooter reveals powerful outflows in z ~ 1.5 X-ray selected obscured quasi-stellar objects
- zCOSMOS 20k: satellite galaxies are the main drivers of environmental effects in the galaxy population at least to z ~ 0.7
- zCOSMOS: A Large VLT/VIMOS Redshift Survey Covering 0 < z < 3 in the COSMOS Field
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