COSMOS2020: A panchromatic view of the Universe to $z\sim 10$ from two complementary catalogs

Abstract

The Cosmic Evolution Survey (COSMOS) has become a cornerstone of extragalactic astronomy. Since the last public catalog in 2015, a wealth of new imaging and spectroscopic data has been collected in the COSMOS field. This paper describes the collection, processing, and analysis of this new imaging data to produce a new reference photometric redshift catalog. Source detection and multi-wavelength photometry is performed for 1.7 million sources across the $2{\mathrm{deg}}^2$ of the COSMOS field, $\sim$966,000 of which are measured with all available broad-band data using both traditional aperture photometric methods and a new profile-fitting photometric extraction tool, The Farmer, which we have developed. A detailed comparison of the two resulting photometric catalogs is presented. Photometric redshifts are computed for all sources in each catalog utilizing two independent photometric redshift codes. Finally, a comparison is made between the performance of the photometric methodologies and of the redshift codes to demonstrate an exceptional degree of self-consistency in the resulting photometric redshifts. The $i<21$ sources have sub-percent photometric redshift accuracy and even the faintest sources at $25<i<27$ reach a precision of $5\%$. Finally, these results are discussed in the context of previous, current, and future surveys in the COSMOS field. Compared to COSMOS2015, reaches the same photometric redshift precision at almost one magnitude deeper. Both photometric catalogs and their photometric redshift solutions and physical parameters will be made available through the usual astronomical archive systems (ESO Phase 3, IPAC IRSA, and CDS).

39 pages, 21 figures, accepted for publication in The Astrophysical Journal Supplement Series. Production of IRAC mosaics are presented in Moneti et al. "Euclid Preparation: XVIII. Cosmic Dawn Survey. Spitzer observations of the Euclid deep fields and calibration fields" which has been posted simultaneously. Catalogs can be accessed online now at https://cosmos2020.calet.org

References in corpus (46)

• The NumPy array: a structure for efficient numerical computation
• Cosmic Star Formation History
• Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties
• Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
• The Cosmic Evolution Survey (COSMOS) -- Overview
• The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies
• EAZY: A Fast, Public Photometric Redshift Code
• New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit
• COSMOS Photometric Redshifts with 30-bands for 2-deg2
• zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field
• Detection of quiescent galaxies in a bicolor sequence from z=0-2
• The Hubble Ultra Deep Field
• UltraVISTA: a new ultra-deep near-infrared survey in COSMOS
• The Evolution of L and T Dwarfs in Color-Magnitude Diagrams
• PRIMUS: Constraints on Star Formation Quenching and Galaxy Merging, and the Evolution of the Stellar Mass Function From z=0-1
• Weak Gravitational Lensing with COSMOS: Galaxy Selection and Shape Measurements
• Photometric redshift and classification for the XMM-COSMOS sources
• The Cosmic Evolution Survey (COSMOS): Subaru Observations of the HST COSMOS Field
• The VIMOS Ultra-Deep Survey: ~10,000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2<z<~6
• A massive proto-cluster of galaxies at a redshift of z {\approx} 5.3
• A Turnover in the Galaxy Main Sequence of Star Formation at $M_{\ast }\sim 10^{10}{M}_{\odot }$ for Redshifts $z<1.3$
• A lack of evolution in the very bright-end of the galaxy luminosity function from z = 8-10
• MegaPipe: the MegaCam image stacking pipeline at the Canadian Astronomical Data Centre
• Star Formation at $4<z<6$ From the Spitzer Large Area Survey with Hyper-Suprime-Cam (SPLASH)
• ALMA Imaging of Gas and Dust in a Galaxy Protocluster at Redshift 5.3: [CII] Emission in "Typical" Galaxies and Dusty Starbursts ~1 Billion Years after the Big Bang
• Water Clouds in Y Dwarfs and Exoplanets
• A Massive Molecular Gas Reservoir in the z=5.3 Submillimeter Galaxy AzTEC-3
• CANDELS Multiwavelength Catalogs: Source Identification and Photometry in the CANDELS COSMOS Survey Field
• The VLA-COSMOS 3 GHz Large Project: Evolution of specific star formation rates out to $z\sim 5$
• The Complete Calibration of the Color-Redshift Relation (C3R2) Survey: Analysis and Data Release 2
• The Hawk-I UDS and GOODS Survey (HUGS): Survey design and deep K-band number counts
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$ VI: Redshift and emission-line catalog and basic properties of star-forming galaxies
• T-PHOT version 2.0: improved algorithms for background subtraction, local convolution, kernel registration, and new options
• The 0.1<z<1.65 evolution of the bright end of the [OII] luminosity function
• Beyond UVJ: More Efficient Selection of Quiescent Galaxies With UV / Mid-IR Fluxes
• Physical Characterization of an Unlensed Dusty Star-Forming Galaxy at $z=5.85$
• COLDz: A High Space Density of Massive Dusty Starburst Galaxies ~1 Billion Years after the Big Bang
• Probing the galaxy-halo connection in UltraVISTA to $z\sim 2$
• Horizon-AGN virtual observatory - 1. SED-fitting performance and forecasts for future imaging surveys
• Quasars in the COSMOS Field
• Galaxy Sizes Since $z=2$ from the Perspective of Stellar Mass Distribution within Galaxies
• ConvPhot: A Profile-Matching Algorithm for Precision Photometry
• The Synthetic Emission Line COSMOS catalog: H$\alpha$ and [OII] galaxy luminosity functions and counts at $0.3<z<2.5$
• X-shooter Spectroscopy and HST Imaging of 15 Ultra Massive Quiescent Galaxies at $z\gtrsim 2$
• An Application of Multi-band Forced Photometry to One Square Degree of SERVS: Accurate Photometric Redshifts and Implications for Future Science
• Bright Lyman $\alpha$ emitters among Spitzer SMUVS galaxies in the MUSE/COSMOS field

Cited by in corpus (256)

• Euclid. I. Overview of the Euclid mission
• The evolution of the galaxy UV luminosity function at redshifts z ~ 8-15 from deep JWST and ground-based near-infrared imaging
• The Early Data Release of the Dark Energy Spectroscopic Instrument
• Full spectrum fitting with photometry in pPXF: stellar population versus dynamical masses, non-parametric star formation history and metallicity for 3200 LEGA-C galaxies at redshift z~0.8
• An Atlas of Color-selected Quiescent Galaxies at $z>3$ in Public $JWST$ Fields
• COSMOS2020: The Galaxy Stellar Mass Function: the assembly and star formation cessation of galaxies at $0.2<z\le 7.5$
• The Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques
• Forecasting the detection capabilities of third-generation gravitational-wave detectors using $\text{GWFAST}$
• New Observational $H(z)$ Data from Full-Spectrum Fitting of Cosmic Chronometers in the LEGA-C Survey
• A Search for H-Dropout Lyman Break Galaxies at z~12-16
• COSMOS2020: The cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z~5
• The Sparkler: Evolved High-Redshift Globular Clusters Captured by JWST
• Euclid preparation: XVIII. Cosmic Dawn Survey. Spitzer observations of the Euclid deep fields and calibration fields
• COSMOS-Web: stellar mass assembly in relation to dark matter halos across $0.2<z<12$ of cosmic history
• ALMA Confirmation of an Obscured Hyperluminous Radio-Loud AGN at $z=6.853$ Associated with a Dusty Starburst in the 1.5 deg${}^2$ COSMOS Field
• Tracing the Quenching Journey across Cosmic Time
• The ALMA-ALPAKA survey I: high-resolution CO and [CI] kinematics of star-forming galaxies at z = 0.5-3.5
• Characterization of Two 2mm-detected Optically-Obscured Dusty Star-Forming Galaxies
• COSMOS2020: Discovery of a protocluster of massive quiescent galaxies at $z=2.77$
• A new estimate of the cosmic star formation density from a radio-selected sample, and the contribution of $H$-dark galaxies at $z\ge 3$
• COSMOS2020: Exploring the dawn of quenching for massive galaxies at 3 < z < 5 with a new colour selection method
• Spectral Energy Distributions in Three Deep-Drilling Fields of the Vera C. Rubin Observatory Legacy Survey of Space and Time: Source Classification and Galaxy Properties
• A lensed protocluster candidate at $z=7.66$ identified in JWST observations of the galaxy cluster SMACS0723-7327
• An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS field (AS2COSPEC): Survey Description and First Results
• COSMOS2025: The COSMOS-Web galaxy catalog of photometry, morphology, redshifts, and physical parameters from JWST, HST, and ground-based imaging
• Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
• A new look at the infrared properties of z $\sim$ 5 galaxies
• No Redshift Evolution of Dust Temperatures from $0<z<2$
• ASTRODEEP-JWST: NIRCam-HST multiband photometry and redshifts for half a million sources in six extragalactic deep fields
• The early Universe was dust-rich and extremely hot
• GA-NIFS: High number of dual active galactic nuclei at z~3
• COSMOS2020: Ubiquitous AGN Activity of Massive Quiescent Galaxies at $0<z<5$ Revealed by X-ray and Radio Stacking
• Beyond UVJ: Color Selection of Galaxies in the JWST Era
• $JWST$ Insight Into a Lensed $HST$-dark Galaxy and its Quiescent Companion at $z=2.58$
• MIGHTEE-HI: Evolution of HI scaling relations of star-forming galaxies at $z<0.5$
• The ALMA-CRISTAL survey: Widespread dust-obscured star formation in typical star-forming galaxies at z=4-6
• Star formation of X-ray AGN in COSMOS: The role of AGN activity and galaxy stellar mass
• [CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST
• Value Added Catalog of physical properties of more than 1.3 million galaxies from the DESI Survey
• The Size-Mass relation at Rest-Frame $1.5\mu$m from JWST/NIRCam in the COSMOS-WEB and PRIMER-COSMOS fields
• COSMOS2020: Manifold Learning to Estimate Physical Parameters in Large Galaxy Surveys
• Evaluating Lya Emission as a Tracer of the Largest Cosmic Structure at z~2.47
• Elentári: A $z\sim 3.3$ Proto-Supercluster in COSMOS
• Combining the CLAUDS & HSC-SSP surveys: U+grizy(+YJHKs) photometry and photometric redshifts for 18M galaxies in the 20 deg2 of the HSC-SSP Deep and ultraDeep fields
• A${}^3$COSMOS and A${}^3$GOODSS: Continuum Source Catalogues and Multi-band Number Counts
• COSMOS2020: UV selected galaxies at $z\ge 7.5$
• The ALMA-CRISTAL survey: Gas, dust, and stars in star-forming galaxies when the Universe was ~1 Gyr old I. Survey overview and case studies
• Hierarchical Bayesian inference of photometric redshifts with stellar population synthesis models
• COSMOS2020: Identification of High-z Protocluster Candidates in COSMOS
• Constraints on Supermassive Black Hole Binaries from JWST and NANOGrav
• A population of ultraviolet-dim protoclusters detected in absorption
• The fundamental plane of black hole activity for low-luminosity radio active galactic nuclei across 1 < z < 4
• The morphological mix of dwarf galaxies in the nearby Universe
• Mapping the Growth of Supermassive Black Holes as a Function of Galaxy Stellar Mass and Redshift
• A hidden active galactic nucleus powering bright [O III] nebulae in a protocluster at $z=4.5$ revealed by JWST
• What boost galaxy mergers in two massive galaxy protoclusters at z = 2.24
• Large Scale Structures in COSMOS2020: Evolution of Star Formation Activity in Different Environments at 0.4 < z < 4
• What Are Those Tiny Things? A First Study of Compact Star Clusters in the SMACS0723 Field with JWST
• Stochastic Modelling of Star Formation Histories III. Constraints from Physically-Motivated Gaussian Processes
• Extracting Photometric Redshift from Galaxy Flux and Image Data using Neural Networks in the CSST Survey
• Multimessenger study of merging massive black holes in the OBELISK simulation: gravitational waves, electromagnetic counterparts, and their link to galaxy and black hole populations
• On the Significance of Rare Objects at High Redshift: The Impact of Cosmic Variance
• pop-cosmos: A comprehensive picture of the galaxy population from COSMOS data
• Weak-Lensing Detection of Intracluster Filaments in the Coma Cluster
• Euclid: Early Release Observations -- Overview of the Perseus cluster and analysis of its luminosity and stellar mass functions
• JWST/MIRI reveals the true number density of massive galaxies in the early Universe
• WEAVE-StePS. A stellar population survey using WEAVE at WHT
• Anatomy of an ionized bubble: NIRCam grism spectroscopy of the $z=6.6$ double-peaked Lyman-$\alpha$ emitter COLA1 and its environment
• Hybrid photometric redshifts for sources in the COSMOS and XMM-LSS fields
• The stellar mass function of quiescent galaxies in 2 < z < 2.5 protoclusters
• Euclid preparation. XXI. Intermediate-redshift contaminants in the search for $z>6$ galaxies within the Euclid Deep Survey
• High Resolution HST Imaging Survey of Local Star-Forming Galaxies I: Spatially-Resolved Obscured Star Formation with H$\alpha$ and Paschen-$\beta$ Recombination Lines
• Probing the Timescale of the 1.4 GHz Radio emissions as a Star formation tracer
• A galaxy group candidate at z~3.7 in the COSMOS field
• The SRG/eROSITA All-Sky Survey: Weak-Lensing of eRASS1 Galaxy Clusters in KiDS-1000 and Consistency Checks with DES Y3 & HSC-Y3
• Dust attenuation, dust content and geometry of star-forming galaxies
• NOEMA formIng Cluster survEy (NICE): Characterizing eight massive galaxy groups at $1.5<z<4$ in the COSMOS field
• Probing magnetic fields in the circumgalactic medium using polarization data from MIGHTEE
• Noema formIng Cluster survEy (NICE): Discovery of a starbursting galaxy group with a radio-luminous core at z=3.95
• The COSMOS-Web ring: in-depth characterization of an Einstein ring lensing system at z~2
• An ultra-deep multi-band VLA survey of the faint radio sky (COSMOS-XS): New constraints on the cosmic star formation history
• Illuminating the Dark Side of Cosmic Star Formation III: Building the largest homogeneous sample of Radio-Selected Dusty Star-Forming Galaxies in COSMOS with PhoEBO
• JWST PRIMER: A lack of outshining in four normal z =4-6 galaxies from the ALMA-CRISTAL Survey
• Relaxed blue ellipticals: accretion-driven stellar growth is a key evolutionary channel for low mass elliptical galaxies
• More is better: Strong constraints on the stellar properties of LEGA-C z ~ 1 galaxies with Prospector
• ODIN: Improved Narrowband Ly$\alpha$ Emitter Selection Techniques for $z$ = 2.4, 3.1, and 4.5
• JWST's first glimpse of a z > 2 forming cluster reveals a top-heavy stellar mass function
• Clumps as multiscale structures in cosmic noon galaxies
• LeMoN: Lens Modelling with Neural networks -- I. Automated modelling of strong gravitational lenses with Bayesian Neural Networks
• Euclid preparation. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary Fields
• Not-so-little Red Dots: Two massive and dusty starbursts at z~5-7 pushing the limits of star formation discovered by JWST in the COSMOS-Web survey
• JWST and ALMA discern the assembly of structural and obscured components in a high-redshift starburst galaxy
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• A Machine Learning Approach to Predict Missing Flux Densities in Multi-band Galaxy Surveys
• Implications of a Temperature Dependent IMF III: Mass Growth and Quiescence
• The archival discovery of a strong Lyman-$\alpha$ and [CII] emitter at z = 7.677
• Detection of anisotropic satellite quenching in galaxy clusters up to $z\sim 1$
• Simulation-based inference of deep fields: galaxy population model and redshift distributions
• Large Scale Overdensity of Lyman Break Galaxies Around the z=6.3 Ultraluminous Quasar J0100+2802
• COSMOS-Web: The emergence of the Hubble Sequence
• COSMOS-Web: A history of galaxy migrations over the stellar mass-star formation rate plane
• Discovering Large-Scale Structure at $2<z<5$ in the C3VO Survey
• The COSMOS-Web deep galaxy group catalog up to $z=3.7$
• Impact of stellar population synthesis choices on forward modelling-based redshift distribution estimates
• New constraints on the evolution of the MHI-M* scaling relation combining CHILES and MIGHTEE-HI data
• 3D-DASH: The Widest Near-Infrared Hubble Space Telescope Survey
• A super-linear "radio-AGN main sequence'' links mean radio-AGN power and galaxy stellar mass since z$\sim$3
• MAGIC: Muse gAlaxy Groups In Cosmos -- A survey to probe the impact of environment on galaxy evolution over the last 8 Gyr
• AMICO-COSMOS galaxy cluster and group catalogue up to $z=2$: Sample properties and X-ray counterparts
• Introducing the Texas Euclid Survey for Lyman Alpha (TESLA) Survey: Initial Study Correlating Galaxy Properties to Lyman-Alpha Emission
• Improving Photometric Redshift Estimates with Training Sample Augmentation
• Evolution of the spiral structure of galaxies from the HST COSMOS field
• Cosmic evolution of radio-excess AGNs in quiescent and star-forming galaxies across $0<z<4$
• Machine learning synthetic spectra for probabilistic redshift estimation: SYTH-Z
• A${}^3$COSMOS: Measuring the cosmic dust-attenuated star formation rate density at $4<z<5$
• The redshift evolution of the S0 fraction for $z<1$ in COSMOS
• Obscured AGN enhancement in galaxy pairs at cosmic noon: evidence from a probabilistic treatment of photometric redshifts
• pop-cosmos: Scaleable inference of galaxy properties and redshifts with a data-driven population model
• CONCERTO: Extracting the power spectrum of the [C II ] emission line
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• Evolution of the Sérsic Index up to z=2.5 from JWST and HST
• The Ly$\alpha$, CIV, and HeII nebulae around J1000+0234: a galaxy pair at the center of a galaxy overdensity at $z=4.5$
• Less Wound and More Asymmetric: JWST Confirms the Evolution of Spiral Structure in Galaxies at $z\lesssim 3$
• MIDIS. Near-infrared rest-frame morphology of massive galaxies at $3<z<5$ in the Hubble eXtreme Deep Field
• Joint Survey Processing I: Compact oddballs in the COSMOS field -- low-luminosity Quasars at z > 6?
• No Need for Extreme Stellar Masses at z~7: A Test-case Study of COS-87259
• Exploring the Intrinsic Scatter of the Star-Forming Galaxy Main Sequence at redshift 0.5 to 3.0
• Line-of-sight Elongation and Hydrostatic Mass Bias of the Frontier Fields Galaxy Cluster Abell 370
• Dark Energy Survey Year 6 Results: Cell-based Coadds and Metadetection Weak Lensing Shape Catalogue
• The structural properties of nearby dwarf galaxies in low density environments -- size, surface brightness and colour gradients
• Halfway to the Peak: The JWST MIRI 5.6 micron number counts and source population
• MAGAZ3NE: Massive, Extremely Dusty Galaxies at $z\sim 2$ Lead to Photometric Overestimation of Number Densities of the Most Massive Galaxies at $3<z<4$
• COSMOS Brightest Group Galaxies -- III: Evolution of stellar ages
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• Probabilistic and progressive deblended far-infrared and sub-millimetre point source catalogues I. Methodology and first application in the COSMOS field
• The PAU Survey: galaxy stellar population properties estimates with narrowband data
• Euclid preparation. LI. Forecasting the recovery of galaxy physical properties and their relations with template-fitting and machine-learning methods
• PAC in DESI. I. Galaxy Stellar Mass Function into the $10^6{\mathrm{M}}_{\odot }$ Frontier
• Weak-Lensing Analysis of the Complex Cluster Merger Abell 746 with Subaru/Hyper Suprime-Cam
• COSMOS2020: Investigating the AGN-obscured accretion phase at $z\sim 1$ via [NeV] selection
• A Cohesive Deep Drilling Field Strategy for LSST Cosmology
• Inferring redshift and galaxy properties via a multi-task neural net with probabilistic outputs: An application to simulated MOONS spectra
• Cluster candidates with massive quiescent galaxies at $z\sim 2$
• SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). V. Confusion-limited Submillimeter Galaxy Number Counts at 450 $\mu$m and Data Release for the COSMOS Field
• Preparation for CSST: Star-galaxy Classification using a Rotationally Invariant Supervised Machine Learning Method
• Euclid: Identifying the reddest high-redshift galaxies in the Euclid Deep Fields with gradient-boosted trees
• Euclid preparation. XXXI. The effect of the variations in photometric passbands on photometric-redshift accuracy
• Going deeper into the dark with COSMOS-Web: JWST unveils the total contribution of Radio-Selected NIRfaint galaxies to the cosmic Star Formation Rate Density
• Revealing the hidden cosmic feast: A z=4.3 galaxy group hosting two optically dark, efficiently star-forming galaxies
• Overdensity of Lyman-Break Galaxy Candidates Around Hot Dust-Obscured Galaxies
• Test of Cosmic Web-feeding Model for Star Formation in Galaxy Clusters in the COSMOS Field
• COSMOS2020: Disentangling the Role of Mass and Environment in Star Formation Activity of Galaxies at $0.4<z<4$
• COSMOS-Web galaxy groups: Evolution of red sequence and quiescent galaxy fraction
• JWST Discovery of a High-Redshift Tidal Disruption Event Candidate in COSMOS-Web
• MARTA: Temperature-temperature relationships and strong-line metallicity calibrations from multiple auroral-line detections at cosmic noon
• Unraveling emission line galaxy conformity at z~1 with DESI early data
• Behind the dust veil: A panchromatic view of an optically dark galaxy at z=4.82
• Gas properties as a function of environment in the proto-supercluster Hyperion at z ~ 2.45
• Photometric IGM tomography with Subaru/HSC: the large-scale structure of Ly$\alpha$ emitters and IGM transmission in the COSMOS field at $z\sim 5$
• The miniJPAS survey. Evolution of the luminosity and stellar mass functions of galaxies up to $z\sim 0.7$
• The Compilation and Validation of the Spectroscopic Redshift Catalogs for the DESI-COSMOS and DESI-XMMLSS Fields
• AMICO galaxy clusters in KiDS-1000: cosmological constraints and mass calibration from counts and weak lensing
• The relationship of SMBHs and host galaxies at $z<4$ in the deep optical variability-selected AGN sample in the COSMOS field
• Cosmic reflections I: the structural diversity of simulated and observed low-mass galaxy analogues
• CONCERTO at APEX -- On-sky performance in continuum
• Introducing cosmosTNG: simulating galaxy formation with constrained realizations of the COSMOS field
• The SRG/eROSITA All-Sky Survey. The Weak-Lensing Mass Calibration and the Stellar Mass-to-Halo Mass Relation from the Hyper Suprime-Cam Subaru Strategic Program
• pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population
• Data-Space Validation of High-Dimensional Models by Comparing Sample Quantiles
• The Ly$\alpha$ and Continuum Origins Survey. III. Investigating the Link between Galaxy Morphology, Merger Properties and LyC Escape
• Machine Learning Classification of COSMOS2020 Galaxies: Quiescent vs. Star-Forming
• "Dust Giant": Extended and Clumpy Star-Formation in a Massive Dusty Galaxy at $z=1.38$
• The Earliest Stage of Galactic Star Formation
• An ultra-high-resolution map of (dark) matter
• A${}^3$COSMOS: The dust content of massive quiescent galaxies and its evolution with cosmic time
• Insights into environmental quenching at $z\sim 1$: an enhancement of faint, low-mass passive galaxies in clusters
• The Radio Spectral Energy Distribution and Star Formation Calibration in MIGHTEE-COSMOS Highly Star-Forming Galaxies at 1.5 < z < 3.5
• MUSUBI (MegaCam Ultra-deep Survey: $u^{\ast }$-Band Imaging)-Data for the COSMOS and SXDS Fields
• An efficient unsupervised classification model for galaxy morphology: Voting clustering based on coding from ConvNeXt large model
• Black hole mass of a quiescent galaxy hosting a Type 1 AGN at z=2.09: Implications for black hole - galaxy co-evolution and AGN quenching at high redshift
• The quasar luminosity function at $z\sim 5$ via deep learning and Bayesian information criterion
• AGN -- host galaxy photometric decomposition using a fast, accurate and precise deep learning approach
• Central Concentration of Asymmetric Features in Post-starburst Galaxies at $z\sim 0.8$
• Galaxy Correlation Function and Local Density from Photometric Redshifts Using the Stochastic Order Redshift Technique (SORT)
• Deep Extragalactic VIsible Legacy Survey (DEVILS): First Data Release Covering The D10 (COSMOS) Region
• LATIS: Comparing Galaxy and IGM Tomography Maps as Tracers of Large-scale Structure and Protoclusters at $z\sim 2.5$
• Testing the Surface Brightness Fluctuation Method on Dwarf Galaxies in the COSMOS Field
• Measuring galaxy abundance and clustering at high redshift from incomplete spectroscopic data: Tests on mock catalogs
• Cosmic Vine: High abundance of massive galaxies and dark matter halos in a forming cluster at z=3.44
• Formation of Substructure in Luminous Submillimeter Galaxies (FOSSILS): Evidence of Multiple Pathways to Trigger Starbursts in Luminous Submillimeter Galaxies
• [CII] luminosity models and large-scale image cubes based on COSMOS 2020 and ALPINE-ALMA [CII] data back to the epoch of reionisation
• The stellar mass function of quiescent and star-forming galaxies and its dependence on morphology in COSMOS-Web
• Effects of Environment on the Size Evolution of Quiescent Galaxies: Comparing Galaxies in Clusters and in the Field at Two Rest-frame Wavelengths
• The effect of environment on the properties of the most massive galaxies at $0.5<z<2.5$ in the cosmos-dash field
• Stellar angular momentum of disk galaxies at z = 0.7 in the MAGIC survey I. Impact of the environment
• Reconstructing AGN X-ray spectral parameter distributions with Bayesian methods II: Population inference
• Zangetsu: A Candidate of Isolated, Quiescent, and Backsplash Ultra-Diffuse Galaxy in the COSMOS Field
• Measuring the gas reservoirs in $10^8<$ M${}_{\star }<10^{11}$ M${}_{\odot }$ galaxies at $1\le z\le 3$
• COSMOS2025: Machine Learning Classification of Early- and Late-type Galaxies at 0 < z < 3
• The Jet Paths of Radio AGN and their Cluster Weather
• ULTIMATE-deblending I. A 50-band Ultraviolet to Mid-infrared Photometric Catalog Combining Space- and Ground-based Data in the JWST/PRIMER survey
• Classifying merger stages with adaptive deep learning and cosmological hydrodynamical simulations
• Euclid preparation: TBD. Cosmic Dawn Survey: evolution of the galaxy stellar mass function across 0.2<z<6.5 measured over 10 square degrees
• Do Red Galaxies Form More Stars Than Blue Galaxies?
• Reconstructing galaxy star formation histories from COSMOS2020 photometry using simulation-based inference
• Evolution of the star formation rate surface density main sequence. Insights from a semi-analytic simulation since $z=12$
• Exploring the X-ray-radio connection for AGN via measurements of the multi-dimensional luminosity function
• Tracing obscured galaxy build-up at high redshift using deep radio surveys
• ALMA Lensing Cluster Survey: Dust mass measurements as a function of redshift, stellar-mass and star formation rate, from z=1 to z=5
• DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [OII] Luminosity
• 6x2pt: Forecasting gains from joint weak lensing and galaxy clustering analyses with spectroscopic-photometric galaxy cross-correlations
• Nearby dwarf galaxies with extreme star formation rates: a window into dwarf-galaxy evolution in the early Universe
• Impact of redshift distribution uncertainties on Lyman-break galaxy cosmological parameter inference
• The HST-Hyperion Survey: Companion Fraction and Overdensity in a z ~ 2.5 Proto-supercluster
• A High-resolution Far-infrared Survey to Probe Black Hole-Galaxy Co-evolution
• SEMPER I. Radio Predictions for Star-Forming Galaxies at $0<z<5$
• SUNRISE-3D: Sharp UNveiling of AGN feedback Regulation and its Impact on Star-formation at the cosmic noon Epoch
• Angular correlation functions of bright Lyman-break galaxies at $3\lesssim \mathbf{z}\lesssim 5$
• Obscured and unobscured X-ray AGNs I: Host galaxy properties
• Far-infrared lines hidden in archival deep multi-wavelength surveys: Limits on [CII]-158$\mu$m at $z\sim 0.3-2.9$
• The Physical Properties of Star-Forming Galaxies with Strong [O III] Lines at z=3.25
• The Radio Galaxy Environment Reference Survey (RAGERS): a submillimetre study of the environments of massive radio-quiet galaxies at $z=1-3$
• SHAPE. I. A SOM-SED hybrid approach for efficient galaxy parameter estimation leveraging JWST
• CHILES X: Molecular and atomic gas at intermediate redshift
• Photometrically Selected Protocluster Candidates at z~9-10 in the JWST COSMOS-Web field
• Deblending the MIGHTEE-COSMOS survey with XID+: The resolved radio source counts to $S_{1.4}\approx 5\mu$Jy
• The major merger-active galactic nucleus connection up to the cosmic noon
• Identifying Compton-thick active galactic nuclei in the COSMOS. II. Searching among mid-infrared selected AGNs
• Uncovering the MIR emission of quiescent galaxies with $JWST$
• Selecting Clusters and Protoclusters via Stellar Mass Density: II. Application to HSC-SSP Observations
• Selecting Clusters and Protoclusters via Stellar Mass Density: I. Method and tests on Mock HSC-SSP catalogs
• Reconstructing the Assembly of Massive Galaxies. III: Quiescent Galaxies Loose Angular Momentum as They Evolve in a Mass-dependent Fashion
• The Dark Energy Survey Supernova Program results: Type Ia Supernova brightness correlates with host galaxy dust
• The Spitzer Extragalactic Representative Volume Survey and DeepDrill extension: clustering of near-infrared galaxies
• The near infrared airglow continuum conundrum. Constraints for ground-based faint object spectroscopy
• pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue
• A multiwavelength study of an early galaxy group merger in COSMOS revealed by two tailed radio galaxies at z = 0.35
• Quiescent Host Galaxies of Extended Quasars Revealed by Spectrophotometric Decomposition
• COSMOS2025: A Machine Learning Census of Massive Quiescent Galaxies at $2.5<\text{z}<5$
• An empirical model of the extragalactic radio background
• The Evolution of the SFR-M_* relation at 0.1<z<4: Environmental and Morphological Dependencies
• Oxyster: A Circumgalactic Low-ionization Oxygen Nebula next to a Starburst Galaxy at $z\sim 1$
• Optimizing the Roman Space Telescope High-Latitude Wide Area Survey for mitigating chromatic PSF effects on shear measurement
• AGILE: an end-to-end Rubin-LSST simulation of AGNs, galaxies, and stars I. Software description and first data release
• Highly Efficient Selection of High-Redshift Emission-Line Galaxies for future DESI-like surveys with Deep Multi-band Imaging
• Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations
• The Redshifts from 122 Bands: Comparative Redshift Forecast for Low-Resolution Spectra from SPHEREx and 7-Dimensional Sky Survey (7DS)
• GalSBI-SPS: a stellar population synthesis-based galaxy population model for cosmology and galaxy evolution applications
• The Photometric Analysis of the Environment Around Two Dusty Star-Forming Galaxies at $z\sim 2$
• Euclid: Discovery of bright $z\simeq 7$ Lyman-break galaxies in UltraVISTA and Euclid COSMOS
• GalSBI: Phenomenological galaxy population model for cosmology using simulation-based inference
• Semi-empirical constraints on the HI mass function of star-forming galaxies and ${\Omega }_{\mathrm{HI}}$ at $z\sim 0.37$ from interferometric surveys
• The NIKA2 cosmological legacy survey at 2 mm: catalogs, colors, redshift distributions, and implications for deep surveys
• A gradient boosting and broadband approach to finding Lyman-α emitting galaxies beyond narrowband surveys
• Euclid: Early Release Observations. Weak gravitational lensing analysis of Abell 2390
• Noema formIng Cluster survEy (NICE): A Census of Star Formation and Cold Gas Properties in Massive protoclusters at 1.5<z<4