Measuring and Modelling the Redshift Evolution of Clustering: the Hubble Deep Field North

Abstract

(abridged) The evolution of galaxy clustering from z=0 to z=4.5 is analyzed using the angular correlation function and the photometric redshift distribution of galaxies brighter than I_{AB}\le 28.5 in the HDF North. The reliability of the photometric redshift estimates is discussed on the basis of the available spectroscopic redshifts, comparing different codes and investigating the effects of photometric errors. The redshift bins in which the clustering properties are measured are then optimized to take into account the uncertainties of the photometric redshifts. The results show that the comoving correlation length has a small decrease in the range 0<z<1 followed by an increase at higher z. We compare these results with the theoretical predictions of a variety of cosmological models belonging to the general class of CDM. The comparison with the expected mass clustering evolution indicates that the observed high-redshift galaxies are biased tracers of the dark matter with an effective bias b strongly increasing with redshift. Assuming an Einstein-de Sitter universe, we obtain b\simeq 2 at z=2 and b\simeq 5 at z=4. A comparison of the clustering amplitudes that we measured at z=3 with those reported for LBG suggests that the clustering depends on the abundance of the objects: more abundant objects are less clustered, as expected in the paradigm of hierarchical galaxy formation. The strong clustering and high bias measured at z=3 are consistent with the expected density of massive haloes predicted for the various cosmologies here considered. At z=4, the strong clustering observed in the HDF requires a significant fraction of massive haloes to be already formed by that epoch. This feature could be a discriminant test for the cosmological parameters if confirmed by future observations.

23 pages, Latex using MN style, figures enclosed. Version accepted for publication in MNRAS

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• On the Classification of UGC1382 as a Giant Low Surface Brightness Galaxy
• Weak Lensing Tomographic Redshift Distribution Inference for the Hyper Suprime-Cam Subaru Strategic Program three-year shape catalogue
• Spatial distribution of stellar mass and star formation activity at 0.2<z<1.2 across and along the Main Sequence
• Super-solar metallicity at the position of the ultra-long GRB130925A
• VLT Spectroscopy of Galaxies Lensed by Abell AC114: Implication for the Mass Model and the Study of Low-Luminosity Galaxies at High-Redshift
• The Spectral Energy Distributions of Active Galactic Nuclei
• Stellar Populations of Lyman Break Galaxies at z=1-3 in the HST/WFC3 Early Release Science Observations
• The Spectral Energy Distributions of Active Galactic Nuclei
• MUSE integral-field spectroscopy towards the Frontier Fields cluster Abell S1063: II. Properties of low luminosity Lyman alpha emitters at z>3
• The first sample of spectroscopically confirmed ultra-compact massive galaxies in the Kilo Degree Survey
• High redshift evolution of optically and IR-selected galaxies: a comparison with CDM scenarios
• Star Formation Quenching in High-redshift Large-scale Structure: Post-starburst Galaxies in the Cl1604 Supercluster at $z\sim 0.9$
• An environmental dependence of the physical and structural properties in the Hydra Cluster galaxies
• The Oxford-Dartmouth Thirty Degree Survey II: Clustering of Bright Lyman Break Galaxies - Strong Luminosity Dependent Bias at z=4
• A Photometrically Detected Forming Cluster of Galaxies at Redshift 1.6 in the GOODS Field
• A Comprehensive Bayesian Discrimination of the Simple Stellar Population Model, Star Formation History and Dust Attenuation Law in the Spectral Energy Distribution Modeling of Galaxies
• Analysis of a Custom Support Vector Machine for Photometric Redshift Estimation and the Inclusion of Galaxy Shape Information
• SCUBA-2 Ultra Deep Imaging Eao Survey (Studies) III: Multi-wavelength properties, luminosity functions and preliminary source catalog of 450-$\mu$m-selected galaxies
• HectoMAP and Horizon Run 4: Dense Structures and Voids in the Real and Simulated Universe
• Quiescent Galaxy Size and Spectroscopic Evolution: Combining HSC Imaging and Hectospec Spectroscopy
• A Physical Approach to the Identification of High-z Mergers: Morphological Classification in the Stellar Mass Domain
• A new method to assign galaxy cluster membership using photometric redshifts
• Velocity Dispersions of Brightest Cluster Galaxies and Their Host Clusters
• A Supernova Candidate at z=0.092 in XMM-Newton Archival Data
• Constraining the galaxy mass content in the core of A383 using velocity dispersion measurements for individual cluster members
• Are Type Ia Supernovae in Restframe $H$ Brighter in More Massive Galaxies?
• The ALPINE-ALMA [CII] survey: dust attenuation curves at z=4.4-5.5
• Dust-obscured star-formation in the outskirts of XMMU J2235.3-2557, a massive galaxy cluster at z=1.4
• The MUSE Hubble Ultra Deep Field Survey: III. Testing photometric redshifts to 30th magnitude
• SHELS: Complete Redshift Surveys of Two Widely Separated Fields
• Comparing Dense Galaxy Cluster Redshift Surveys with Weak Lensing Maps
• Nature of Faint Radio Sources in GOODS-North and GOODS-South Fields - I. Spectral Index and Radio-FIR Correlation
• ALMACAL III: A combined ALMA and MUSE Survey for Neutral, Molecular, and Ionised Gas in an HI-Absorption-Selected System
• A Method for Measuring the Bias of High-Redshift Galaxies from Cosmic Variance
• Fuzzy Dark Matter as a Solution to Reconcile the Stellar Mass Density of High-z Massive Galaxies and Reionization History
• Mergers as triggers for nuclear activity: A near-IR study of the close environment of AGN in the VISTA-VIDEO survey
• Kpc-scale Properties of Emission-line Galaxies
• Close-up view of a luminous star-forming galaxy at z=2.95
• Photometric Redshifts in the Hawaii-Hubble Deep Field-North (H-HDF-N)
• Photometric Redshifts from SDSS Images with an Interpretable Deep Capsule Network
• Multi-wavelength characterisation of z~2 clustered, dusty star forming galaxies discovered by Planck
• A critical appraisal of the SED fitting method to estimate photometric redshifts
• A combined VANDELS and LEGA-C study: the evolution of quiescent galaxy size, stellar mass and age from $\text{z}=0.6$ to $\text{z}=1.3$
• ALMA constraints on star-forming gas in a prototypical z=1.5 clumpy galaxy: the dearth of CO(5-4) emission from UV-bright clumps
• Massive, Absorption-selected Galaxies at Intermediate Redshifts
• North Ecliptic Pole merging galaxy catalogue
• A VLT/FORS2 spectroscopic survey in the HDF-S
• Quasar Sightline and Galaxy Evolution (QSAGE) Survey - I. The Galaxy Environment of OVI Absorbers up to z=1.4 around PKS 0232-04
• The Dependence of the Mass-Metallicity Relation on Large Scale Environment
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• Evolution of the cluster optical galaxy luminosity function in the CFHTLS : breaking the degeneracy between mass and redshift
• CHILES: HI morphology and galaxy environment at z=0.12 and z=0.17
• Galactic winds and the Lya forest
• Characterising the Circum-Galactic Medium of Damped Lyman-$\alpha$ Absorbing Galaxies
• The last 6 Gyr of dark matter assembly in massive galaxies from the Kilo Degree Survey
• The Next Generation Virgo Cluster Survey. XV. The photometric redshift estimation for background sources
• Star formation of X-ray AGN in COSMOS: The role of AGN activity and galaxy stellar mass
• The complex physics of dusty star-forming galaxies at high redshifts as revealed by Herschel and Spitzer
• The Environment of Massive Quiescent Compact Galaxies at $0.1<z<0.4$ in the COSMOS Field
• The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3
• The ASTRODEEP Frontier Fields Catalogues III. Multiwavelength photometry and rest frame properties of MACS-J0717 and MACS-J1149
• A multi-wavelength analysis of a collection of short-duration GRBs observed between 2012-2015
• A Carbon/Oxygen-dominated Atmosphere Days After Explosion for the "Super-Chandrasekhar" Type Ia SN 2020esm
• Stellar-to-halo mass relation of cluster galaxies
• Herschel observations of gamma-ray burst host galaxies: implications for the topology of the dusty interstellar medium
• Propagating sample variance uncertainties in redshift calibration: simulations, theory and application to the COSMOS2015 data
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• Euclid: Early Release Observations -- Deep anatomy of nearby galaxies
• Improving the reliability of photometric redshift with machine learning
• The luminous host galaxy, faint supernova and rapid afterglow rebrightening of GRB 100418A
• Pan-STARRS1 variability of XMM-COSMOS AGN. I. Impact on photometric redshifts
• COSMOS2020: Manifold Learning to Estimate Physical Parameters in Large Galaxy Surveys
• Catalogs of Compact Groups of Galaxies from the Enhanced SDSS DR12
• Environmental Quenching and Galactic Conformity in the Galaxy Cross-Correlation Signal
• Spectroscopic and Photometric Redshift Estimation by Neural Networks For the China Space Station Optical Survey (CSS-OS)
• New High-z Fermi BL Lacs with the Photometric Dropout Technique
• The ALPINE-ALMA [CII] Survey: On the nature of an extremely obscured serendipitous galaxy
• A Method to Distinguish Quiescent and Dusty Star-forming Galaxies with Machine Learning
• Stellar masses, metallicity gradients and suppressed star formation revealed in a new sample of absorption selected galaxies
• A Study of Quasar Selection in the Dark Energy Survey Supernova fields
• Galaxy counterparts of intervening high-z sub-DLAs/DLAs and MgII absorbers towards gamma-ray bursts
• The GOGREEN survey: Dependence of galaxy properties on halo mass at z > 1 and implications for environmental quenching
• New HI 21-cm absorbers at low and intermediate redshifts
• Photometric redshifts with machine learning, lights and shadows on a complex data science use case
• Discovery of the first quadruple gravitationally lensed quasar candidate with Pan-STARRS
• CFHTLenS: Weak lensing constraints on the ellipticity of galaxy-scale matter haloes and the galaxy-halo misalignment
• X-ray AGN in the XMM-LSS galaxy clusters: no evidence of AGN suppression
• SPIDER - V. Measuring Systematic Effects in Early-Type Galaxy Stellar Masses from Photometric SED Fitting
• XXL-HSC: The link between AGN activity and star formation in the Early Universe ($z⩾3.5$)
• Discovery of a PRS associated with FRB 20240114A
• The Galaxy-Halo Connection for $1.5\lesssim z\lesssim 5$ as revealed by the \emph{Spitzer} Matching survey of the UltraVISTA ultra-deep Stripes
• Building the largest spectroscopic sample of ultra-compact massive galaxies with the Kilo Degree Survey
• Elentári: A $z\sim 3.3$ Proto-Supercluster in COSMOS
• The stellar content of the COSMOS field as derived from morphological and SED based gtar/galaxy Separation
• Luminosity Functions beyond the spectroscopic limit. I. Method and near-infrared LFs in the HDF-N and HDF-S
• KiDS-1000 Cosmology: Constraints from density split statistics
• Galaxy Clustering Evolution in the UH8K Weak Lensing Fields
• Statistical analysis of probability density functions for photometric redshifts through the KiDS-ESO-DR3 galaxies
• 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
• Subaru weak-lensing measurement of a z = 0.81 cluster discovered by the Atacama Cosmology Telescope Survey
• Implications of the Environments of Radio-detected AGN in a Complex Protostructure at z$\sim$3.3
• Photometric redshifts for X-ray-selected active galactic nuclei in the eROSITA era
• SN 2022ann: A type Icn supernova from a dwarf galaxy that reveals helium in its circumstellar environment
• The first Hubble diagram and cosmological constraints using superluminous supernova
• The star-formation history of mass-selected galaxies from the VIDEO survey
• VVDS-SWIRE: Clustering evolution from a spectroscopic sample of galaxies with redshift 0.2<z<2.1 selected from Spitzer IRAC 3.6 micron and 4.5 micron photometry
• The Efficacy of Galaxy Shape Parameters in Photometric Redshift Estimation: A Neural Network Approach
• The evolution of the cluster optical galaxy luminosity function between z=0.4 and 0.9 in the DAFT/FADA survey
• Classification and environmental properties of X-ray selected point-like sources in the XMM-LSS field
• Evidence that Gamma-ray Burst 130702A Exploded in a Dwarf Satellite of a Massive Galaxy
• The host galaxy of GRB 980425 / SN1998bw: a collisional ring galaxy
• Characterising the evolving $K$-band luminosity function using the UltraVISTA, CANDELS and HUDF surveys
• The miniJPAS survey: The role of group environment in quenching the star formation
• A Molecular gas rich GRB host galaxy at the peak of cosmic star formation
• Flat Rotation Curves of $z\sim 1$ Star-Forming Galaxies and Evidence of Disk-Scale Length Evolution
• The 2-10 keV unabsorbed luminosity function of AGN from the XMM-Newton LSS, CDFS and COSMOS surveys
• The Spitzer Matching Survey of the UltraVISTA Ultra-deep Stripes (SMUVS): the Evolution of Dusty and Non-Dusty Galaxies with Stellar Mass at z=2-6
• The Host Haloes of Lyman Break Galaxies and Sub-millimeter Sources
• The VIMOS Ultra Deep Survey: The role of HI kinematics and HI column density on the escape of Lyalpha photons in star-forming galaxies at 2<z<4
• Clustering and redshift-space distortions in modified gravity models with massive neutrinos
• Galaxy classification: deep learning on the OTELO and COSMOS databases
• The impact of the Star Formation Histories on the SFR-M${}_{\ast }$ relation at z$\ge$2
• The environments of intermediate-redshift QSOs: 0.3 < z < 0.7
• The Morphological Transformation of Red Sequence Galaxies in Clusters since $z\sim 1$
• MIGHTEE-HI: The relation between the HI gas in galaxies and the cosmic web
• Exploring Photometric Redshifts as an Optimization Problem: An Ensemble MCMC and Simulated Annealing-Driven Template-Fitting Approach
• The XXL Survey VIII: MUSE characterisation of intracluster light in a z$\sim$0.53 cluster of galaxies
• The first Infrared study of the close environment of a long Gamma-Ray Burst
• The impact of JWST broad-band filter choice on photometric redshift estimation
• An extinction free AGN selection by 18-band SED fitting in mid-infrared in the AKARI NEP deep field
• Euclid: The selection of quiescent and star-forming galaxies using observed colours
• The Clustering of X-ray Luminous Quasars
• Comparison of the properties of two fossil groups of galaxies with the normal group NGC 6034 based on multiband imaging and optical spectroscopy
• A Comparison of Photometric Redshift Techniques for Large Radio Surveys
• STRIDES: Spectroscopic and photometric characterization of the environment and effects of mass along the line of sight to the gravitational lenses DES J0408-5354 and WGD 2038-4008
• Extracting Photometric Redshift from Galaxy Flux and Image Data using Neural Networks in the CSST Survey
• Euclid preparation: VIII. The Complete Calibration of the Colour-Redshift Relation survey: VLT/KMOS observations and data release
• CLASH: Extending galaxy strong lensing to small physical scales with distant sources highly-magnified by galaxy cluster members
• Clumpiness of Observed and Simulated Cold Circumgalactic Gas
• The Cosmic Microwave Background and the Stellar Initial Mass Function
• A Census of WISE-selected Dual and Offset AGN Across the Sky: New Constraints on Merger-Driven Triggering of Obscured AGN
• Wide Field Imaging of the Hubble Deep Field South Region II: The Evolution of Galaxy Clustering at z<1
• The host galaxy properties of variability selected AGN in the Pan-STARRS1 Medium-Deep Survey
• The OTELO survey. I. Description, data reduction, and multi-wavelength catalogue
• A Molecular Einstein Ring Toward the z=3.93 Submillimeter Galaxy MM18423+593
• AGN X-ray luminosity function and absorption function in the Early Universe ($3\le z\le 6$)
• pop-cosmos: A comprehensive picture of the galaxy population from COSMOS data
• Extinction-free Census of AGNs in the $AKARI$/IRC North Ecliptic Pole Field from 23-band Infrared Photometry from Space Telescopes
• The PAU Survey: Intrinsic alignments and clustering of narrow-band photometric galaxies
• Quasi-stellar objects in the ALHAMBRA survey. I. Photometric redshift accuracy based on a 23 optical-NIR filter photometry
• Photometric Redshifts with Surface Brightness Priors
• GRB 140102A: Insight into Prompt Spectral Evolution and Early Optical Afterglow Emission
• The faint end of the red sequence galaxy luminosity function: unveiling surface brightness selection effects with the CLASH clusters
• The complex case of MACSJ0717.5+3745 and its extended filament: intra-cluster light, galaxy luminosity function, and galaxy orientations
• A photo-z cautionary tale: Redshift confirmation of COSBO-7 at z=2.625
• Separating Galaxies from the Cluster Dark Matter Halo in Abell 611
• Comparison of Observed Galaxy Properties with Semianalytic Model Predictions using Machine Learning
• The environment and host haloes of the brightest z~6 Lyman-break galaxies
• The HectoMAP Redshift Survey: First Data Release
• Herschel Far-IR counterparts of SDSS galaxies: Analysis of commonly used Star Formation Rate estimates
• New high-z BL Lacs using the photometric method with Swift and SARA
• Photometric redshift estimates using Bayesian neural networks in the CSST survey
• Augmenting machine learning photometric redshifts with Gaussian mixture models
• Steep extinction towards GRB 140506A reconciled from host galaxy observations: Evidence that steep reddening laws are local
• Molecular gas in radio galaxies in dense Mpc-scale environments at $z=0.4-2.6$
• The distribution of faint satellites around central galaxies in the CFHT Legacy Survey
• Genuine Retrieval of the AGN Host Stellar Population (GRAHSP)
• [Ultra] Luminous Infrared Galaxies selected at 90 $\mu$m in the AKARI deep field: a study of AGN types contributing to their infrared emission
• The Accretion History of AGN: A Newly Defined Population of Cold Quasars
• The first catalogue of spectroscopically confirmed red nuggets at z~0.7 from the VIPERS survey. Linking high-z red nuggets and local relics
• Webb's PEARLS: Bright 1.5--2.0 micron Dropouts in the Spitzer/IRAC Dark Field
• Optically-selected clusters at 0.8 < z < 1.3 in the EIS Cluster Survey
• The Stellar Mass Fundamental Plane and Compact Quiescent Galaxies at z < 0.6
• Spatially resolved properties of galaxies from CANDELS+MUSE: Radial extinction profile and insights on quenching
• Bright Lyman $\alpha$ emitters among Spitzer SMUVS galaxies in the MUSE/COSMOS field
• SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) IV: Spatial clustering and halo masses of 450-$\mu$m-selected sub-millimeter galaxies
• The distribution of dark matter and gas spanning six megaparsecs around the post-merger galaxy cluster MS0451-03
• Orphan GRB afterglow searches with the Pan-STARRS1 COSMOS survey
• Detailed Afterglow Modeling and Host Galaxy Properties of the Dark GRB 111215A
• The Cosmological Constant and Quintessence from a Correlation Function Comoving Fine Feature in the 2dF Quasar Redshift Survey
• Calibrating photometric redshift measurements with the Multi-channel Imager (MCI) of the China Space Station Telescope (CSST)
• Inferring the photometric and size evolution of galaxies from image simulations
• PhotoRedshift-MML: a multimodal machine learning method for estimating photometric redshifts of quasars
• Probing Intra-Halo Light with Galaxy Stacking in CIBER Images
• Comparing Dark Energy Survey and HST-CLASH observations of the galaxy cluster RXC J2248.7-4431: implications for stellar mass versus dark matter
• Hybrid photometric redshifts for sources in the COSMOS and XMM-LSS fields
• A Composite Likelihood Approach for Inference under Photometric Redshift Uncertainty
• The Exotic Type Ic Broad-Lined Supernova SN 2018gep: Blurring the Line Between Supernovae and Fast Optical Transients
• The Type Ia supernovae rate with Subaru/XMM-Newton Deep Survey
• Estimating redshift distributions using Hierarchical Logistic Gaussian processes
• The Pan-STARRS1 Medium-deep Survey: Star Formation Quenching in Group and Cluster Environments
• Euclid preparation. XXI. Intermediate-redshift contaminants in the search for $z>6$ galaxies within the Euclid Deep Survey
• Effects of galaxy environment on merger fraction
• Photometric redshift estimation of galaxies in the DESI Legacy Imaging Surveys
• The star formation rate cookbook at 1 < z < 3: Extinction-corrected relations for UV & [OII]λ3727 luminosities
• ELDAR, a new method to identify AGN in multi-filter surveys: the ALHAMBRA test-case
• Recovering the properties of high redshift galaxies with different JWST broad-band filters
• SMBH accretion properties of radio-selected AGN out to z~4
• AMICO galaxy clusters in KiDS-DR3: galaxy population properties and their redshift dependence
• Photometric Redshift Estimation with Galaxy Morphology using Self-Organizing Maps
• Molecular gas in AzTEC/C159: a star-forming disk galaxy 1.3Gyr after the Big Bang
• GRB 051008: A long, spectrally-hard dust-obscured GRB in a Lyman-Break Galaxy at z ~ 2.8
• Extremely Red Submillimeter Galaxies: New z>~4-6 Candidates Discovered using ALMA and Jansky VLA
• Discovery of a Supercluster at $z\sim$0.91 and Testing the $\Lambda$CDM Cosmological Model
• Properties of star forming galaxies in AKARI Deep Field-South
• Cosmology with XMM galaxy clusters: the X-CLASS/GROND catalogue and photometric redshifts
• X-ray luminosity-star formation rate scaling relation: Constraints from the eROSITA Final Equatorial Depth Survey (eFEDS)
• VLT/X-Shooter Near-Infrared Spectroscopy and HST Imaging of Gravitationally-Lensed z~2 Compact Quiescent Galaxies
• JWST PRIMER: A lack of outshining in four normal z =4-6 galaxies from the ALMA-CRISTAL Survey
• CircleZ: Reliable Photometric redshifts for AGN computed using only photometry from Legacy Survey Imaging for DESI
• The XXL Survey: XXXVII. The role of the environment in shaping the stellar population properties of galaxies at 0.1<z<0.5
• Morphology & Environment's Role on the Star Formation Rate -- Stellar Mass Relation in COSMOS from 0 < z < 3.5
• A Complete Spectroscopic Census of Abell 2029: A Tale of Three Histories
• Clustering of red-sequence galaxies in the fourth data release ofthe Kilo-Degree Survey
• The XXL Survey: XXII. The XXL-North spectrophotometric sample and galaxy stellar mass function in X-ray detected groups and clusters
• The ALPINE-ALMA [CII] Survey: Investigation of 10 Galaxies at $z\sim 4.5$ with [OII] and [CII] Line Emission $-$ ISM Properties and [OII]$-$SFR Relation
• The UV luminosity function at 0.6 < z < 1 from UVCANDELS
• K-CLASH: spatially-resolving star-forming galaxies in field and cluster environments at $z\approx 0.2$-$0.6$
• The Stellar-to-Halo Mass Ratios of Passive and Star-Forming Galaxies at z~2-3 from the SMUVS survey
• HectoMAP: The Complete Redshift Survey (Data Release 2)
• Photometric Redshifts and Systematic Variations in the SEDs of Luminous Red Galaxies from the SDSS DR7
• Absorption-selected galaxies trace the low-mass, late-type, star-forming population at $z\sim 2-3$
• The Fastest Galaxy Evolution in an Unbiased Compact Group Sample with WISE
• Galaxy clustering measurements out to redshift z$\sim$8 from Hubble Legacy Fields
• Galaxy clusters in the SDSS Stripe 82 based on galaxy photometric redshifts
• PKS 2123-463: a confirmed gamma-ray blazar at high redshift
• Of Genes and Machines: application of a combination of machine learning tools to astronomy datasets
• The bright end of the galaxy luminosity function at $z\simeq 7$ from the VISTA VIDEO survey
• Next Generation Virgo Cluster Survey. XXI. The weak lensing masses of the CFHTLS and NGVS RedGOLD galaxy clusters and calibration of the optical richness
• A Machine Learning Approach to Predict Missing Flux Densities in Multi-band Galaxy Surveys
• The faint radio source population at 15.7 GHz - II. Multi-wavelength properties
• Pairwise velocity dispersion of galaxies at high redshift: theoretical predictions
• Discovery of an unusually compact lensed Lyman Break Galaxy from the Hyper Suprime-Cam Survey
• Statistical stellar mass corrections for high-z galaxies observed with JWST broad-band filters due to template degeneracies
• Optical-faint, Far-infrared-bright Herschel Sources in the CANDELS Fields: Ultra-Luminous Infrared Galaxies at z>1 and the Effect of Source Blending
• Supernova 2020wnt: An Atypical Superluminous Supernova with a Hidden Central Engine
• The OTELO survey as a morphological probe. Last ten Gyr of galaxy evolution. The mass--size relation up to z=2
• Radial Distribution Of ISM Gas-phase Metallicity In CLASH Clusters at z~0.35: A New Outlook On Environmental Impact On Galaxy Evolution
• The Coevolution of Massive Quiescent Galaxies and Their Dark Matter Halos over the Last 6 Billion Years
• The OTELO survey: Nature and mass-metallicity relation for H$\alpha$ emitters at $z\sim 0.4$
• Hunting distant BL Lacs with the photometric technique using Swift and SARA
• The 2175 Å dust feature in star-forming galaxies at $1.3\le z\le 1.8$: the dependence on stellar mass and specific star formation rate
• The COSMOS-Web Lens Survey (COWLS) I: Discovery of >100 high redshift strong lenses in contiguous JWST imaging
• Large Scale Overdensity of Lyman Break Galaxies Around the z=6.3 Ultraluminous Quasar J0100+2802
• A First Look into the Nature of JWST/MIRI 7.7 micron Sources from SMACS 0723
• Simulation-based inference of deep fields: galaxy population model and redshift distributions
• "Red" but Not "Dead": Actively Star-forming Brightest Cluster Galaxies at Low Redshifts
• PhotoWeb redshift: boosting photometric redshift accuracy with large spectroscopic surveys
• Hubble Frontier Field Clusters and their Parallel Fields: Photometric and Photometric Redshift Catalogs
• The Apertif science verification campaign - Characteristics of polarised radio sources
• Dark matter fraction of low-mass cluster members probed by galaxy-scale strong lensing
• Physical properties of more than one thousand brightest cluster galaxies detected in the Canada France Hawaii Telescope Legacy Survey
• The obscured hyper-energetic GRB 120624B hosted by a luminous compact galaxy at z = 2.20
• Dark Matter Fraction in z~1 Star-Forming Galaxies
• Photometric Redshifts in the North Ecliptic Pole Wide Field based on a Deep Optical Survey with Hyper Suprime-Cam
• Photometric Redshift Biases from Galaxy Evolution
• Does AGN Fraction Depend on Redshift or Luminosity? An Extinction-Free Test by 18-band Mid-infrared SED Fitting in the AKARI NEP Wide Field
• The Origin of \lya Absorption Systems at $z>1$---Implications from the Hubble Deep Field
• Emission line selected galaxies at $z=0.6-2$ in GOODS South: Stellar masses, SFRs, and large scale structure
• The Infrared Medium-Deep Survey II: How to Trigger Radio-AGN? Hints from Their Environments
• The XXL Survey: XXX. Characterisation of the XLSSsC N01 supercluster and analysis of the galaxy stellar populations
• Machine learning synthetic spectra for probabilistic redshift estimation: SYTH-Z
• Getting ready for the LSST data -- estimating the physical properties of $z<2.5$ main sequence galaxies
• Multicolor Photometry Study of the Galaxy Cluster A2589: Dynamics, Luminosity Function and Star Formation History
• Tracing Dark Matter Halos with Satellite Kinematics and the Central Stellar Velocity Dispersion of Galaxies
• The OTELO survey. II. The faint-end of the H$\alpha$ luminosity function at z $\sim$ 0.40
• The ALPINE-ALMA [CII] Survey: CGM pollution and gas mixing by tidal stripping in a merging system at z~4.57
• Multicolor photometry of the galaxies in the central region of Abell 2634
• Systematic errors on optical-SED stellar mass estimates for galaxies across cosmic time and their impact on cosmology
• pop-cosmos: Scaleable inference of galaxy properties and redshifts with a data-driven population model
• KiDS-1000: Weak lensing and intrinsic alignment around luminous red galaxies
• Improving machine learning-derived photometric redshifts and physical property estimates using unlabelled observations
• High redshift LBGs from deep broadband imaging for future spectroscopic surveys
• A Spectroscopic Census of X-ray Systems in the COSMOS Field
• Size and Spectroscopic Evolution of HectoMAP Quiescent Galaxies
• A weak lensing view of the downsizing of star-forming galaxies
• Ultracool dwarfs candidates based on six years of the Dark Energy Survey data
• Linking galaxies to dark matter haloes at $z\sim 1$ : dependence of galaxy clustering on stellar mass and specific star formation rate
• The Role of Bulge Formation in the Homogenization of Stellar Populations at $z\sim 2$ as revealed by Internal Color Dispersion in CANDELS
• The Infrared Luminosity Function of AKARI 90$\mu$m Galaxies in the Local Universe
• The luminous, massive and solar metallicity galaxy hosting the Swift gamma-ray burst, GRB 160804A at z = 0.737
• RCS2 J232727.6-020437: An Efficient Cosmic Telescope at $z=0.6986$
• The ESO-Sculptor Survey: Evolution of late-type galaxies at redshifts 0.1-0.5
• Tightening weak lensing constraints on the ellipticity of galaxy-scale dark matter haloes
• Large Size Scatter of Passively Evolving Lensed Galaxies at z~2 in CLASH
• No Need for Extreme Stellar Masses at z~7: A Test-case Study of COS-87259
• Influence of star-forming galaxy selection on the galaxy main sequence
• eROSITA Final Equatorial-Depth Survey (eFEDS): eFEDS X-ray view of WERGS Radio Galaxies selected by the Subaru/HSC and VLA/FIRST survey
• Variation of optical and infrared properties of galaxies with their surface brightness
• Near-Infrared Survey and Photometric Redshifts in the Extended GOODS-North field
• Multiwavelength observations of GRB 140629A. A long burst with an achromatic jet break in the optical and X-ray afterglow
• MAGAZ3NE: Massive, Extremely Dusty Galaxies at $z\sim 2$ Lead to Photometric Overestimation of Number Densities of the Most Massive Galaxies at $3<z<4$
• Data Deluge in Astrophysics: Photometric Redshifts as a Template Use Case
• Photo-z Quality Cuts and their Effect on the Measured Galaxy Clustering
• VST-GAME: Galaxy Assembly as a function of Mass and Environment with VST. Photometric assessment and density field of MACSJ0416
• Environmental Effects on AGN activity via Extinction-free Mid-Infrared Census
• Fundamental Physics and Cosmology with TianQin
• SN 2016hil-- a Type II supernova in the remote outskirts of an elliptical host and its origin
• A search for Population III galaxies in CLASH. I. Singly-imaged candidates at high redshift
• Where are the absorbers towards Q2302+029?
• CALSAGOS: Clustering ALgorithmS Applied to Galaxies in Overdense Systems
• The Morphological Transformation of Red-Sequence Galaxies in the Distant Cluster XMMU J1229+0151
• Selection of powerful radio galaxies with machine learning
• Starbursting Brightest Cluster Galaxy: a Herschel view of the massive cluster MACS J1931.8-2634
• Comparing Galaxy Clustering in Horizon-AGN Simulated Lightcone Mocks and VIDEO Observations
• The less and the more IGM transmitted galaxies from z~2.7 to z~6 from VANDELS and VUDS
• MIGHTEE-HI: Discovery of an HI-rich galaxy group at z = 0.044 with MeerKAT
• RAiSERed: radio continuum redshifts for lobed AGNs
• A Compact Starburst Core in the Dusty Lyman Break Galaxy Westphal-MD11
• MUSE-ALMA Haloes IX: Morphologies and Stellar Properties of Gas-rich Galaxies
• X-ray spectral properties of dust-obscured galaxies in the XMM-SERVS coverage of the XMM-LSS field
• Optically-detected galaxy cluster candidates in the $AKARI$ North Ecliptic Pole field based on photometric redshift from Subaru Hyper Suprime-Cam
• Euclid preparation. XXXI. The effect of the variations in photometric passbands on photometric-redshift accuracy
• Thermal Regulation and the Star-Forming Main Sequence
• Estimating Photometric Redshifts for Galaxies from the DESI Legacy Imaging Surveys with Bayesian Neural Networks Trained by DESI EDR
• Estimating Spectra from Photometry
• Tully-Fisher Relation of Late-type Galaxies at $0.6\le z\le 2.5$
• Leveraging Machine Learning for Accurate and Fast Stellar Mass Estimation of Galaxies
• Iris: an Extensible Application for Building and Analyzing Spectral Energy Distributions
• Cosmological model dependence of the galaxy luminosity function: far-infrared results in the Lemaitre-Tolman-Bondi model
• Enhancing Photometric Redshift Catalogs Through Color-Space Analysis: Application to KiDS-Bright Galaxies
• Candidate fossil groups in the CFHTLS: a probabilistic approach
• Degradation analysis in the estimation of photometric redshifts from non-representative training sets
• The faint radio source population at 15.7 GHz -- IV. The dominance of core emission in faint radio galaxies
• Active galactic nuclei catalog from the AKARI NEP Wide field
• Revealing Dusty Supernovae in High-Redshift (Ultra-)Luminous InfraRed Galaxies Through Near-Infrared Integrated Light Variability
• Toward a stellar population catalog in the Kilo Degree Survey: the impact of stellar recipes on stellar masses and star formation rates
• The Lockman-SpReSO project. Description, target selection, observations and preliminary results
• ALPINE: A Large Survey to Understand Teenage Galaxies
• Tracing Recent Star Formation of Red Early-type Galaxies out to $z$ $\sim$ 1
• Constraints on the galaxy "main sequence" at z>5: the stellar mass of HDF850.1
• Learning Spectral Templates for Photometric Redshift Estimation from Broadband Photometry
• Narrow band selected high redshift galaxy candidates contaminated by lower redshift O[III] ultrastrong emitter line galaxies
• Multicolor Photometry of the Nearby Galaxy Cluster A119
• Detecting episodes of star formation using Bayesian model selection
• The XXL Survey: IX. Optical overdensity and radio continuum analysis of a supercluster at $z=0.43$
• A Study of Selection Methods for H alpha Emitting Galaxies at z~1.3 for the Subaru/FMOS Galaxy Redshift Survey for Cosmology (FastSound)
• The 3XMM/SDSS Stripe 82 Galaxy Cluster Survey II. X-ray and optical properties of the cluster sample
• Cosmic Stillness: High Quiescent Galaxy Fractions Across Upper Mass Scales in the Early Universe to z = 7 with JWST
• Quenching of Galaxies at Cosmic Noon: Understanding the Effect of Environment
• Dark Energy Survey Deep Field photometric redshift performance and training incompleteness assessment
• Rejection criteria based on outliers in the KiDS photometric redshifts and PDF distributions derived by machine learning
• Galaxy-galaxy lensing in the VOICE deep survey
• Cosmic reflections I: the structural diversity of simulated and observed low-mass galaxy analogues
• Cosmological constraints from galaxy clustering and galaxy-galaxy lensing with extended SubHalo Abundance Matching
• Applying Information Theory to Design Optimal Filters for Photometric Redshifts
• Bringing manifold learning and dimensionality reduction to SED fitters
• pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population
• CLAP. I. Resolving miscalibration for deep learning-based galaxy photometric redshift estimation
• A Multiply-Imaged z $\sim$ 6.3 Lyman Alpha Emitter candidate behind Abell 2261
• Machine Learning Classification of COSMOS2020 Galaxies: Quiescent vs. Star-Forming
• Clustering of galaxies around GRB sight-lines
• Role of AGNs in the Luminous Infrared Galaxy phase since z ~ 3
• The KALEIDOSCOPE survey : A new strong and weak gravitational lensing view of the massive galaxy cluster MACS J1423.8+2404
• Photometric Selection of type 1 Quasars in the XMM-LSS Field with Machine Learning and the Disk-Corona Connection
• 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
• A giant central red disk galaxy at redshift $z=0.76$: challenge to theories of galaxy formation
• Machine learning applications in astrophysics: Photometric redshift estimation
• Optically Faint Radio Sources: Reborn AGN?
• GRB 190114C in the nuclear region of an interacting galaxy -- A detailed host analysis using ALMA, HST and VLT
• Dusty Universe viewed by AKARI far infrared detector
• Galaxy and Mass Assembly (GAMA): Mid-infrared properties as tracers of galaxy environment
• From VIPERS to SDSS: Unveiling galaxy spectra evolution over 9 Gyr through unsupervised machine-learning
• Counterparts of Candidate Dusty Starbursts at z > 6
• Optimizing Redshift Distribution Inference through Joint Self-Calibration and Clustering-Redshift Synergy
• Molecular gas in cool-core brightest cluster galaxies at $z\simeq 0.4$
• Identification and Properties of Isolated Field Elliptical Galaxies from CFHTLS-W1
• The ALPINE-ALMA [CII] survey: The infrared-radio correlation and AGN fraction of star-forming galaxies at z $\sim$ 4.4-5.9
• Far-IR dust properties of highly dust obscured AGNs from the AKARI and WISE all-sky surveys
• Chandra Survey in the AKARI North Ecliptic Pole Deep Field Optical/Infrared Identifications of X-ray Sources
• CFHQSIR: a Y-band extension of the CFHTLS-Wide survey
• A Ly-alpha nebula at z~3.3
• Unveiling the enigma of ATLAS17aeu
• The OTELO survey: Revealing a population of low-luminosity current/active star-forming galaxies at z$\sim 0.9$
• Compact dust-obscured star-formation and the origin of the galaxy bimodality
• Enhanced AGN Activity in Overdense Galactic Environments at $2<z<4$
• Pz Cats: Photometric redshift catalogs based on DES Y3 BAO sample
• Exploring the physical properties of Type II Quasar candidates at intermediate redshifts with CIGALE
• COSMOS2025: Machine Learning Classification of Early- and Late-type Galaxies at 0 < z < 3
• Euclid preparation. Estimating galaxy physical properties using CatBoost chained regressors with attention
• Characterizing the outer disk of eXtended-UV galaxies in the optical domain with deep surveys
• Pearls on a string: Dark and bright galaxies on a strikingly straight and narrow filament
• Machine Learning vs. Spectral Energy Distribution Fitting: A Comparative Analysis of Accuracy in Stellar Mass Estimation
• Bridging between the integrated and resolved main sequence of star formation
• The dust-star interplay in late-type galaxies at z < 0.5: forecasts for the JWST
• Euclid Preparation: XIV. The Complete Calibration of the Color-Redshift Relation (C3R2) Survey: Data Release 3
• Angular correlation functions of bright Lyman-break galaxies at $3\lesssim \mathbf{z}\lesssim 5$
• Probability density estimation of photometric redshifts based on machine learning
• The S-PLUS Fornax Project (S+FP): An extragalactic catalog covering $\sim$ 5 virial radii around NGC 1399 with galaxy properties
• Non-Sequential Neural Network for Simultaneous, Consistent Classification and Photometric Redshifts of OTELO Galaxies
• MUSE-ALMA Haloes XIII. Molecular gas in $z\sim 0.5$ HI-selected galaxies
• Lenses In VoicE (LIVE): Searching for strong gravitational lenses in the VOICE@VST survey using Convolutional Neural Networks
• MIGHTEE: The dark matter haloes, duty cycle and mechanical feedback from radio-AGN up to $z\sim 2.5$
• GLACE survey: OSIRIS/GTC tuneable imaging of the galaxy cluster ZwCl 0024.0+1652 II. The mass--metallicity relationship and the effect of the environment
• X-ray polarimetric features of Gamma-ray Bursts across varied redshifts and hints for Axion-Like-Particles
• A novel analysis of contamination in Lyman-break galaxy samples at $\mathbf{z}\sim 6-8$: spatial correlation with intermediate-redshift galaxies at $\mathbf{z}\sim 1.3-2$
• Evaluating the Accuracy of Non-parametric Galaxy Morphological Indicator Measurements in the CSST Imaging Survey
• The ROSAT Raster Survey in the North-Ecliptic Pole Field: X-ray Catalogue and Optical Identifications
• Euclid: Discovery of bright $z\simeq 7$ Lyman-break galaxies in UltraVISTA and Euclid COSMOS
• COSMOS2025: A Machine Learning Census of Massive Quiescent Galaxies at $2.5<\text{z}<5$
• The BUFFALO HST Survey
• Using a Neural Network Classifier to Select Galaxies with the Most Accurate Photometric Redshifts
• Photometric Redshift Estimation Using Scaled Ensemble Learning
• TOPz: Photometric redshifts using template fitting applied to the GAMA survey
• The Evolution of the SFR-M_* relation at 0.1<z<4: Environmental and Morphological Dependencies
• Euclid: Early Release Observations. Weak gravitational lensing analysis of Abell 2390
• Star formation at z$\sim$0.9 from the OTELO survey: A comprehensive view combining deep optical spectroscopy and infrared data
• pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue
• J-HERTz: J-PLUS Heritage Exploration of Radio Targets at z $<$ 5
• Identification of Compact Groups of Galaxies in IllustrisTNG300
• Photometric redshifts for the S-PLUS Survey: is machine learning up to the task?
• The X-ray statistical properties of dust-obscured galaxies detected by eROSITA
• Quasar clustering at redshift 6
• Time Delay Cosmography: Analysis of Quadruply Lensed QSO SDSSJ1433 from Wendelstein Observatory
• GalSBI: Phenomenological galaxy population model for cosmology using simulation-based inference
• Structural evolution of quiescent galaxies at intermediate redshifts at UV and red rest-frame wavelengths
• Synergy between Roman and PRIMA imaging capabilities for large extragalactic surveys
• CNN photometric redshifts in the SDSS at $r\le 20$
• Deep ATCA and VLA radio observations of short-GRB host galaxies. Constraints on star-formation rates, afterglow flux, and kilonova radio flares
• The Redshifts from 122 Bands: Comparative Redshift Forecast for Low-Resolution Spectra from SPHEREx and 7-Dimensional Sky Survey (7DS)
• A Spectroscopic View of the JWST/GTO Strong Lensing Cluster A1489
• GalSBI-SPS: a stellar population synthesis-based galaxy population model for cosmology and galaxy evolution applications
• Photometric Redshift Estimation with Convolutional Neural Networks and Galaxy Images: A Case Study of Resolving Biases in Data-Driven Methods
• Identification of high-redshift X-ray active galactic nuclei in the 4XMM-DR11 serendipitous catalogue using DES data: Comparative analysis with optically-selected QSOs
• The miniJPAS survey quasar selection I: Mock catalogues for classification