Galaxy and Mass Assembly (GAMA): survey diagnostics and core data release

Abstract

The Galaxy And Mass Assembly (GAMA) survey has been operating since February 2008 on the 3.9-m Anglo-Australian Telescope using the AAOmega fibre-fed spectrograph facility to acquire spectra with a resolution of R~1300 for 120,862 SDSS selected galaxies. The target catalogue constitutes three contiguous equatorial regions centred at 9h (G09), 12h (G12) and 14.5h (G15) each of 12 x 4 sq.deg to limiting fluxes of r < 19.4, r < 19.8, and r < 19.4 mag respectively (and additional limits at other wavelengths). Spectra and reliable redshifts have been acquired for over 98 per cent of the galaxies within these limits. Here we present the survey footprint, progression, data reduction, redshifting, re-redshifting, an assessment of data quality after 3 years, additional image analysis products (including ugrizYJHK photometry, Sersic profiles and photometric redshifts), observing mask, and construction of our core survey catalogue (GamaCore). From this we create three science ready catalogues: GamaCoreDR1 for public release, which includes data acquired during year 1 of operations within specified magnitude limits (February 2008 to April 2008); GamaCoreMainSurvey containing all data above our survey limits for use by the GAMA team and collaborators; and GamaCoreAtlasSv containing year 1, 2 and 3 data matched to Herschel-ATLAS Science Demonstration data. These catalogues along with the associated spectra, stamps and profiles can be accessed via the GAMA website: http://www.gama-survey.org/

Submitted to MNRAS. MySQL database and data downloads available now from http://www.gama-survey.org/

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• The SAMI Galaxy Survey: Decomposed Stellar Kinematics of Galaxy Bulges and Disks
• Formation of disk galaxies in preheated media: a preventative feedback model
• Aperture corrections for disk galaxy properties derived from the CALIFA survey. Balmer emission lines in spiral galaxies
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). The coevolution of galaxy morphology and colour to z~1
• Shapley Supercluster Survey (ShaSS): Galaxy Evolution from Filaments to Cluster Cores
• The XXL Survey: VI. The 1000 brightest X-ray point sources
• Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies in the Local Universe I. - The Effect of the Group Environment on Star Formation in Spiral Galaxies
• The SAMI Galaxy Survey: A Range in S0 Properties Indicating Multiple Formation Pathways
• Evolution of the galaxy stellar mass function: evidence for an increasing $M^{\ast }$ from $z=2$ to the present day
• A 325-MHz GMRT survey of the Herschel-ATLAS/GAMA fields
• A cooperative approach among methods for photometric redshifts estimation: an application to KiDS data
• The SAMI Galaxy Survey: Satellite galaxies undergo little structural change during their quenching phase
• GAMA/H-ATLAS: The Local Dust Mass Function and Cosmic Density as a Function of Galaxy Type - A Benchmark for Models of Galaxy Evolution
• The quiescent fraction of isolated low surface brightness galaxies: Observational constraints
• The galaxy-halo connection in the VIDEO Survey at 0.5<z<1.7
• A MeerKAT view of pre-processing in the Fornax A group
• Candidate high-z proto-clusters among the Planck compact sources, as revealed by Herschel-SPIRE
• Combining Dark Energy Survey Science Verification Data with Near Infrared Data from the ESO VISTA Hemisphere Survey
• On the 3D structure of the mass, metallicity, and SFR space for SF galaxies
• Updated Results on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Reproducing the Universe: a comparison between the EAGLE simulations and the nearby DustPedia galaxy sample
• Radio Detection of VIK J2318$-$3113, the Most Distant Radio-Loud Quasar ($z$=6.44)
• INSPIRE: INvestigating Stellar Population In RElics -- I. Survey presentation and pilot program
• Galaxy And Mass Assembly (GAMA): The 325 MHz Radio Luminosity Function of AGN and Star Forming Galaxies
• Dependence of GAMA galaxy halo masses on the cosmic web environment from 100 square degrees of KiDS weak lensing data
• Structural and Dynamical Properties of Galaxies in a Hierarchical Universe: Sizes and Specific Angular Momenta
• The LOFAR Two-metre Sky Survey: the radio view of the cosmic star formation history
• Clustering of infrared-bright dust-obscured galaxies revealed by the Hyper Suprime-Cam and WISE
• The kinematics of massive quiescent galaxies at $1.4<z<2.1$: dark matter fractions, IMF variation, and the relation to local early-type galaxies
• The first sample of spectroscopically confirmed ultra-compact massive galaxies in the Kilo Degree Survey
• A comparison of cosmological filaments catalogues
• Offset between X-ray and optical centers in clusters of galaxies: connecting eROSITA data and simulations
• Searching for galaxy clusters in the Kilo-Degree Survey
• LOFAR observations of the XMM-LSS field
• The SAMI Galaxy Survey: stellar population gradients of central galaxies
• Testing modified gravity using a marked correlation function
• Dust continuum, CO, and [C I] 1-0 lines: self-consistent H2 mass estimates and the possibility of globally CO-dark galaxies at $z=0.35$
• KiDS-1000: Constraints on the intrinsic alignment of luminous red galaxies
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• The SAMI Galaxy Survey: flipping of the spin-filament alignment correlates most strongly with growth of the bulge
• A deep / wide 1-2 GHz snapshot survey of SDSS Stripe 82 using the Karl G. Jansky Very Large Array in a compact hybrid configuration
• Stellar mass -- halo mass relation for the brightest central galaxies of X-ray clusters since z~0.65
• The High Fraction of Thin Disk Galaxies Continues to Challenge ΛCDM Cosmology
• The dust mass function from z~0 to z~2
• An evolving and mass dependent ${\sigma }_{\text{sSFR}}$-${\mathrm{M}}_{\star }$ relation for galaxies
• Galaxy And Mass Assembly (GAMA): The environments of high- and low- excitation radio galaxies
• Star-forming early- and quiescent late-type galaxies in the local Universe
• H-ATLAS: A Candidate High Redshift Cluster/Protocluster of Star-Forming Galaxies
• The Wide Area VISTA Extra-galactic Survey (WAVES)
• Massive disc galaxies in cosmological hydrodynamical simulations are too dark matter-dominated
• Gas-phase metallicity profiles of the Bluedisk galaxies: Is metallicity in a local star-formation regulated equilibrium?
• Herschel-ATLAS: Correlations between Dust and Gas in Local Submm-Selected Galaxies
• GAMA/H-ATLAS: The ultraviolet spectral slope and obscuration in galaxies
• J-PLUS: On the identification of new cluster members in the double galaxy cluster A2589 & A2593 using PDFs
• Galaxy and Mass Assembly (GAMA): Demonstrating the power of WISE in the study of Galaxy Groups to $z<0.1$
• GAMA/H-ATLAS: Linking the Properties of Sub-mm Detected and Undetected Early-Type Galaxies: I. z$\le$0.06 Sample
• The importance of magnification effects in galaxy-galaxy lensing
• The SAMI Galaxy Survey: Mass and Environment as Independent Drivers of Galaxy Dynamics
• Non-parametric Morphologies of Galaxies in the EAGLE Simulation
• Predicting star formation properties of galaxies using deep learning
• KiDS-i-800: Comparing weak gravitational lensing measurements in same-sky surveys
• Spatial and luminosity distributions of galactic satellites
• The fate of the interstellar medium in early-type galaxies. I. First direct measurement of the timescale of dust removal
• A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). II. Physical Properties derived from the SED Fitting with Optical, Infrared, and Radio Data
• Group quenching and galactic conformity at low redshift
• The eROSITA Final Equatorial-Depth Survey (eFEDS): A multiwavelength view of WISE mid-infrared galaxies/active galactic nuclei
• Void Galaxies Follow a Distinct Evolutionary Path in the Environmental COntext Catalog
• Galaxy And Mass Assembly (GAMA): The Consistency of GAMA and WISE Derived Mass-to-Light Ratios
• VALES: II. The physical conditions of interstellar gas in normal star-forming galaxies up to z=0.2 revealed by ALMA
• Reaching for the Edge I: Probing the Outskirts of Massive Galaxies with HSC, DECaLS, SDSS, and Dragonfly
• Small-scale galaxy clustering in the EAGLE simulation
• Galaxy And Mass Assembly (GAMA): Galaxies at the faint end of the Halpha luminosity function
• Galaxy And Mass Assembly: search for a population of high-entropy galaxy groups
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• Brightest galaxies as halo centre tracers in SDSS DR7
• Galaxy And Mass Assembly (GAMA): Blue spheroids within 87 Mpc
• UV to submillimetre luminosity functions of TNG50 galaxies
• A multi-wavelength exploration of the [CII]/IR ratio in H-ATLAS/GAMA galaxies out to z=0.2
• Herschel-ATLAS/GAMA: SDSS cross-correlation induced by weak lensing
• Towards automatic classification of all WISE sources
• Large Scale Structure in CHILES
• Forward modeling of galaxy populations for cosmological redshift distribution inference
• Deep Investigation of Neutral Gas Origins (DINGO): HI stacking experiments with early science data
• ProFuse: Physical Multi-Band Structural Decomposition of Galaxies and the Mass-Size-Age Plane
• Revealing the cosmic web dependent halo bias
• Galaxy And Mass Assembly: Automatic Morphological Classification of Galaxies Using Statistical Learning
• Optical properties of infrared-bright dust-obscured galaxies viewed with Subaru Hyper Suprime-Cam
• Galaxy and Mass Assembly (GAMA): Accurate number densities & environments of massive ultracompact galaxies at 0.02 < z < 0.3
• The evolution of the UV-to-mm extragalactic background light: evidence for a top-heavy initial mass function?
• A GBT Survey of the HALOGAS Galaxies and Their Environments I: Revealing the full extent of HI around NGC891, NGC925, NGC4414 & NGC4565
• Do the observational data favor a local void?
• Evolution of the Major Merger Galaxy Pair Fraction at z < 1
• GAMA+KiDS: Alignment of galaxies in galaxy groups and its dependence on galaxy scale
• GAMA+KiDS: Empirical correlations between halo mass and other galaxy properties near the knee of the stellar-to-halo mass relation
• Dwarf AGNs from Variability for the Origins of Seeds (DAVOS): Intermediate-mass black hole demographics from optical synoptic surveys
• Mitigating the Impact of the DESI Fiber Assignment on Galaxy Clustering
• The VIMOS Public Extragalactic Redshift Survey - Searching for Cosmic Voids
• J-PLUS: 2-D analysis of the stellar population in NGC 5473 and NGC 5485
• The SAMI Galaxy Survey: a new method to estimate molecular gas surface densities from star formation rates
• Towards a consistent framework of comparing galaxy mergers in observations and simulations
• Galaxy Zoo: Finding offset discs and bars in SDSS galaxies
• Young, Star-forming Galaxies and their local Counterparts: the Evolving Relationship of Mass-SFR-Metallicity since z ~ 2.1
• The SAMI Galaxy Survey: the drivers of gas and stellar metallicity differences in galaxies
• H-ATLAS/GAMA: Magnification Bias Tomography. Astrophysical constraints above $\sim 1$ arcmin
• Galaxy and Mass Assembly (GAMA): Colour and luminosity dependent clustering from calibrated photometric redshifts
• A Model Connecting Galaxy Masses, Star Formation Rates, and Dust Temperatures Across Cosmic Time
• Galaxy And Mass Assembly (GAMA): The effect of galaxy group environment on active galactic nuclei
• Galaxy And Mass Assembly (GAMA): Bulge-disk decomposition of KiDS data in the nearby universe
• The KMOS Galaxy Evolution Survey (KGES): the angular momentum of star-forming galaxies over the last ~10 Gyr
• Characterising the target selection pipeline for the Dark Energy Spectroscopic Instrument Bright Galaxy Survey
• SKYSURF: Constraints on Zodiacal Light and Extragalactic Background Light through Panchromatic HST All-Sky Surface-Brightness Measurements: I. Survey Overview and Methods
• Photometric redshifts with machine learning, lights and shadows on a complex data science use case
• Galaxy And Mass Assembly (GAMA): Timescales for galaxies crossing the green valley
• Low Surface Brightness Galaxy catalogue selected from the alpha.40-SDSS DR7 Survey and Tully-Fisher relation
• Using an Artificial Neural Network to Classify Multi-component Emission Line Fits
• The SAMI Galaxy Survey: gas content and interaction as the drivers of kinematic asymmetry
• The Massive Satellite Population of Milky-Way Sized Galaxies
• A search for the lenses in the Herschel Bright Sources (HerBS) Sample
• Morphology rather than environment drives the SFR-Mass relation in the local universe
• Building the largest spectroscopic sample of ultra-compact massive galaxies with the Kilo Degree Survey
• KiDS-1000 Cosmology: Constraints from density split statistics
• SHELS: Optical Spectral Properties of WISE 22 μm-selected Galaxies
• Testing for a large local void by investigating the Near-Infrared Galaxy Luminosity Function
• Galaxy and Mass Assembly (GAMA): Extended Intra-Group Light in a group at $z=0.2$ from deep Hyper-Suprime Cam images
• DES Science Portal: Computing Photometric Redshifts
• The dependence of intrinsic alignment of galaxies on wavelength using KiDS and GAMA
• Statistical analysis of probability density functions for photometric redshifts through the KiDS-ESO-DR3 galaxies
• Statistical Analysis of Galaxy Surveys-IV: An objective way to quantify the impact of superstructures on galaxy clustering statistics
• The SAMI Galaxy Survey: The discovery of a luminous, low-metallicity H II complex in the dwarf galaxy GAMA J141103.98-003242.3
• Characterising the evolving $K$-band luminosity function using the UltraVISTA, CANDELS and HUDF surveys
• The Evolution of Brightest Cluster Galaxies in the Nearby Universe I: Colours and Stellar Masses from the Sloan Digital Sky Survey and Wide Infrared Survey Explorer
• Unveiling the atomic hydrogen-halo mass relation via spectral stacking
• Quantifying the role of ram pressure stripping of galaxies within galaxy groups
• ECO and RESOLVE: Galaxy Disk Growth in Environmental Context
• Luminous red galaxies in the Kilo Degree Survey: selection with broad-band photometry and weak lensing measurements
• RESOLVE and ECO: The Halo Mass-Dependent Shape of Galaxy Stellar and Baryonic Mass Functions
• A new methodology to test galaxy formation models using the dependence of clustering on stellar mass
• The PAU Survey: Spectral features and galaxy clustering using simulated narrow band photometry
• Galaxy And Mass Assembly (GAMA): Bivariate functions of H$\alpha$ star forming galaxies
• Confronting Cold Dark Matter Predictions with Observed Galaxy Rotations
• A Quick Look at the 3GHz Radio Sky. II. Hunting for DRAGNs in the VLA Sky Survey
• Preprocessing, mass loss and mass segregation of galaxies in DM simulations
• SDSS-IV MaNGA: Signatures of halo assembly in kinematically misaligned galaxies
• The DESI PRObabilistic Value-Added Bright Galaxy Survey (PROVABGS) Mock Challenge
• The SAMI Galaxy Survey: the difference between ionised gas and stellar velocity dispersions
• The environment and characteristics of low redshift galaxies detected by the Herschel-ATLAS
• Galaxy And Mass Assembly (GAMA): detection of low-surface-brightness galaxies from SDSS data
• What is Important? Morphological Asymmetries are Useful Predictors of Star Formation Rates of Star-forming Galaxies in SDSS Stripe 82
• Conditional HI mass functions and the HI-to-halo mass relation in the local Universe
• The SAMI galaxy survey: Galaxy Interactions and Kinematic Anomalies in Abell 119
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• GAMA/DEVILS: Cosmic star formation and AGN activity over 12.5 billion years
• Galaxy And Mass Assembly: Estimating galaxy group masses via caustic analysis
• Cross-correlation of WMAP7 and the WISE Full Data Release
• Morphological evolution and galactic sizes in the L-Galaxies SA model
• Multi-frequency studies of galaxies and groups: I. Environmental effect on galaxy stellar mass and morphology
• Systematic biases in determining dust attenuation curves through galaxy SED fitting
• WALLABY Early Science - I. The NGC 7162 Galaxy Group
• Infrared luminosity functions and dust mass functions in the EAGLE simulation
• The extended ROSAT-ESO Flux-Limited X-ray Galaxy Cluster Survey (REFLEX II) V. Exploring a local underdensity in the Southern Sky
• Galaxy and Mass Assembly (GAMA): merging galaxies and their properties
• Galaxy And Mass Assembly (GAMA): Properties and evolution of red spiral galaxies
• Galaxy And Mass Assembly (GAMA): The Bright Void Galaxy Population in the Optical and Mid-IR
• From rest-frame luminosity functions to observer-frame colour distributions: tackling the next challenge in cosmological simulations
• The frequency of dust lanes in edge-on spiral galaxies identified by Galaxy Zoo in KiDS imaging of GAMA targets
• Galaxy and Mass Assembly (GAMA): Formation and Growth of Elliptical Galaxies in the Group Environment
• The OTELO survey. I. Description, data reduction, and multi-wavelength catalogue
• Across the Green Valley with HST grisms: colour evolution, crossing time-scales and the growth of the red sequence at $z=1.0-1.8$
• GAMA/H-ATLAS: Common star-formation rate indicators and their dependence on galaxy physical parameters
• The observability of galaxy merger signatures in nearby gas-rich spirals
• An Analysis Framework for Understanding the Origin of Nuclear Activity in Low-Power Radio Galaxies
• Galaxy And Mass Assembly (GAMA): Galaxy colour gradients versus colour, structure and luminosity
• The SAMI Galaxy Survey: Environmental analysis of the orbital structures of passive galaxies
• Euclid preparation. XLI. Galaxy power spectrum modelling in real space
• Galaxy And Mass Assembly (GAMA) Blended Spectra Catalog: Strong Galaxy-Galaxy Lens and Occulting Galaxy Pair Candidates
• Evolution of the luminosity-to-halo mass relation of LRGs from a combined SDSS-DR10+RCS2 analysis
• MUSE spectroscopy and deep observations of a unique compact JWST target, lensing cluster CLIO
• Multi-resolution filtering: an empirical method for isolating faint, extended emission in Dragonfly data and other low resolution images
• On the connection between the metal-enriched intergalactic medium and galaxies: an OVI-galaxy cross-correlation study at $z<1$
• The PAU Survey: Intrinsic alignments and clustering of narrow-band photometric galaxies
• Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups
• H-ATLAS/GAMA: The nature and characteristics of optically red galaxies detected at submillimetre wavelengths
• New Radio-Loud QSOs at the end of the Re-ionisation Epoch
• pop-cosmos: A comprehensive picture of the galaxy population from COSMOS data
• RedMaPPer: Evolution and Mass Dependence of the Conditional Luminosity Functions of Red Galaxies in Galaxy Clusters
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• Galaxy And Mass Assembly (GAMA): the interplay between galaxy mass, SFR and heavy element abundance in paired galaxy sets
• The ALHAMBRA survey : $B-$band luminosity function of quiescent and star-forming galaxies at $0.2\le z<1$ by PDF analysis
• Galaxy And Mass Assembly: the evolution of the cosmic spectral energy distribution from z = 1 to z = 0
• The Evolution of Sizes and Specific Angular Momenta in Hierarchical Models of Galaxy Formation and Evolution
• The miniJPAS survey: Identification and characterization of the emission line galaxies down to $z<0.35$ in the AEGIS field
• AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis
• The Dynamics and Energetics of Remnant and Restarting RLAGN
• Cosmology with the sub-millimetre galaxies magnification bias: Tomographic Analysis
• KiDS+GAMA: The weak lensing calibrated stellar-to-halo mass relation of central and satellite galaxies
• Probing star formation and ISM properties using galaxy disk inclination I: Evolution in disk opacity since $z\sim 0.7$
• Multi-wavelength scaling relations in galaxy groups: a detailed comparison of GAMA and KiDS observations to BAHAMAS simulations
• Galaxy And Mass Assembly (GAMA): 'No Smoking' zone for giant elliptical galaxies?
• Cosmology with velocity dispersion counts: an alternative to measuring cluster halo masses
• H-ATLAS/GAMA: Quantifying the Morphological Evolution of the Galaxy Population Using Cosmic Calorimetry
• On the role of feedback in shaping the cosmic abundance and clustering of neutral atomic hydrogen in galaxies
• The SAMI Galaxy Survey: Using Tidal Streams and Shells to Trace the Dynamical Evolution of Massive Galaxies
• The SAMI Galaxy Survey: Kinematics of Dusty Early-Type Galaxies
• Galaxy and Mass Assembly (GAMA): Small-scale anisotropic galaxy clustering and the pairwise velocity dispersion of galaxies
• The XXL Survey: XII. Optical spectroscopy of X-ray-selected clusters and the frequency of AGN in superclusters
• A Machine Learning Approach to Measuring the Quenched Fraction of Low-Mass Satellites Beyond the Local Group
• An empirical measurement of the Halo Mass Function from the combination of GAMA DR4, SDSS DR12, and REFLEX II data
• Exploring Relations Between BCG \& Cluster Properties in the SPectroscopic IDentification of eROSITA Sources Survey from $0.05<z<0.3$
• Non-Universal Stellar Initial Mass Functions: Large Uncertainties in Star Formation Rates at $z\approx 2-4$ and Other Astrophysical Probes
• Galaxy morphoto-Z with neural Networks (GaZNets). I. Optimized accuracy and outlier fraction from Imaging and Photometry
• Ubiquitous [OII] Emission in Quiescent Galaxies at z ~ 0.85
• Dust and Power: Unravelling the merger - active galactic nucleus connection in the second half of cosmic history
• The PAU survey: Estimating galaxy photometry with deep learning
• The cosmic spectral energy distribution in the EAGLE simulation
• Predicting the global far-infrared SED of galaxies via machine learning techniques
• Herschel-ATLAS/GAMA: spatial clustering of low-redshift sub-mm galaxies
• The Hector Survey: integral field spectroscopy of 100,000 galaxies
• Cosmological constraints with the sub-millimetre galaxies Magnification Bias after large scale bias corrections
• A Herschel-ATLAS study of dusty spheroids: probing the minor-merger process in the local Universe
• Galaxy and Mass Assembly (GAMA): Witnessing the assembly of the cluster Abell 1882
• Estimating Photometric Redshifts for X-ray sources in the X-ATLAS field, using machine-learning techniques
• Single Colour Diagnostics of the Mass-to-light Ratio: Predictions from Galaxy Formation Models
• A direct and robust method to observationally constrain the halo mass function via the submillimeter magnification bias: Proof of concept
• Ubiquitous radio emission in quasars: predominant AGN origin and a connection to jets, dust and winds
• Galaxy And Mass Assembly (GAMA): The environmental dependence of the galaxy main sequence
• The SAMI Galaxy Survey: Bayesian Inference for Gas Disk Kinematics using a Hierarchical Gaussian Mixture Model
• Evolution of the Stellar Mass Function and Infrared Luminosity Function of Galaxies since $z=1.2$
• SKYSURF: Constraints on Zodiacal Light and Extragalactic Background Light through Panchromatic HST All-Sky Surface-Brightness Measurements: II. First Limits on Diffuse Light at 1.25, 1.4, and 1.6 microns
• Galaxy And Mass Assembly (GAMA): The unimodal nature of the dwarf galaxy population
• Using member galaxy luminosities as halo mass proxies of galaxy groups
• The SAMI Galaxy Survey: The role of disc fading and progenitor bias in kinematic transitions
• H-ATLAS/GAMA and HeViCS - Dusty Early-Type Galaxies in Different Environments
• The impact of the dynamical state of galaxy groups on the stellar populations of central galaxies
• Maximum Likelihood Random Galaxy Catalogues and Luminosity Function Estimation
• Self-consistent bulge/disk/halo galaxy dynamical modeling using integral field kinematics
• Constraining the duration of ram pressure stripping features in the optical from the direction of jellyfish galaxy tails
• The role of stellar mass and environment for cluster blue fraction, AGN fraction and star-formation indicators from a targeted analysis of Abell 1691
• The ALHAMBRA survey: 2-D analysis of the stellar populations in massive early-type galaxies at z < 0.3
• QSOs sigposting cluster size halos as gravitational lenses: halo mass, projected mass density profile and concentration at $z\sim 0.7$
• A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). IV. Rapidly Growing (Super-)Massive Black Holes in Extremely Radio-Loud Galaxies
• Forensic reconstruction of galaxy colour evolution and population characterisation
• Galaxy and Mass Assembly (GAMA): A $\text{WISE}$ study of the activity of emission-line systems in G23
• Deep Extragalactic VIsible Legacy Survey (DEVILS): The emergence of bulges and decline of disk growth since $z=1$
• Galaxy And Mass Assembly (GAMA): Comparing Visually and Spectroscopically Identified Galaxy Merger Samples
• The ALHAMBRA survey: tight dependence of the optical mass-to-light ratio on galaxy colour up to z = 1.5
• Physical Properties of Local Star-Forming Analogues to z~5 Lyman Break Galaxies
• More is better: Strong constraints on the stellar properties of LEGA-C z ~ 1 galaxies with Prospector
• The second Herschel-ATLAS Data Release - III: optical and near-infrared counterparts in the North Galactic Plane field
• {\em Herschel}-ATLAS/GAMA: The Environmental Density of Far-Infrared Bright Galaxies at $z\le 0.5$
• PopSED: Population-Level Inference for Galaxy Properties from Broadband Photometry with Neural Density Estimation
• Characterizing the satellites of massive galaxies up to z~2: young populations to build the outskirts of nearby massive galaxies
• Minimising the impact of scale-dependent galaxy bias on the joint cosmological analysis of large scale structures
• Star Formation in Simulated Galaxies: Understanding the Transition to Quiescence at $3\times 10^{10}$ M${}_{\odot }$
• Cosmology with the submillimetre galaxies magnification bias: Proof of concept
• An Extensive Photometric Catalog of CALIFA Galaxies
• The Nature of Low Surface Brightness Galaxies in the Hyper Suprime-Cam Survey
• Colour matters: the effects of lensing on the positional offsets between optical and submillimetre galaxies in Herschel-ATLAS
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. III. Accurate Measurement of Galaxy Stellar Mass Function with the Aid of Cosmological Redshift Surveys
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Evolution of the ${\sigma }_{\mathrm{SFR}}$-M${}_{\star }$ relation and implications for self-regulated star formation
• Measuring the delay time distribution of binary neutron stars. III. Using the individual star formation histories of gravitational wave event host galaxies in the local universe
• K-CLASH: spatially-resolving star-forming galaxies in field and cluster environments at $z\approx 0.2$-$0.6$
• Galaxy Tagging: photometric redshift refinement and group richness enhancement
• Clustering of red-sequence galaxies in the fourth data release ofthe Kilo-Degree Survey
• Spherical collapse in Generalized Dark Matter models
• Galaxy quenching timescales from a forensic reconstruction of their colour evolution
• Spatially resolved mock observations of stellar kinematics: full radiative transfer treatment of simulated galaxies
• The SAMI Galaxy Survey: galaxy spin is more strongly correlated with stellar population age than mass or environment
• Herschel-ATLAS : The spatial clustering of low and high redshift submillimetre galaxies
• J-PLUS: The star formation main sequence and rate density at d < 75 Mpc
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Stellar Mass Growth by Morphological Type since $z=1$
• A radiative transfer model for the spiral galaxy M33
• Do galaxy mergers prefer under-dense environments?
• Detection of spatial clustering in the 1000 richest SDSS DR8 redMaPPer clusters with Nearest Neighbor distributions
• A single galaxy population? statistical evidence that the Star-Forming Main Sequence might be the tip of the iceberg
• K-CLASH: Strangulation and Ram Pressure Stripping in Galaxy Cluster Members at 0.3 < z < 0.6
• The fate of the interstellar medium in early-type galaxies. III. The mechanism of ISM removal and quenching of star formation
• Mixture Models for Photometric Redshifts
• Galaxy And Mass Assembly (GAMA): The absence of stellar mass segregation in galaxy groups and consistent predictions from GALFORM and EAGLE simulations
• Measuring the HI mass function below the detection threshold
• Reconstructing the galaxy density field with photometric redshifts: II. Environment-dependent galaxy evolution since $z\simeq 3$
• Merger history of central galaxies in Semi-Analytic Models of galaxy formation
• ASKAP Commissioning Observations of the GAMA 23 Field
• The halo model with beyond-linear halo bias: unbiasing cosmological constraints from galaxy-galaxy lensing and clustering
• Constraining the Radio Properties of the $z$=6.44 QSO VIK J2318$-$3113
• The Galaxy Stellar Mass Function and Low Surface Brightness Galaxies from Core-Collapse Supernovae
• The formation pathways of compact elliptical galaxies
• Herschel-ATLAS/GAMA: What determines the far-infrared properties of radio-galaxies?
• Optimising commensality of radio continuum and spectral line observations in the era of the SKA
• An adapted filter function for density split statistics in weak lensing
• The SAMI Galaxy Survey: Gas Streaming and Dynamical M/L in Rotationally Supported Systems
• Panchromatic Photometry of Low-redshift, Massive Galaxies Selected from SDSS Stripe 82
• Far-Ultraviolet and Far-Infrared Bivariate Luminosity Function of Galaxies: Complex Relation between Stellar and Dust Emission
• ALMA observations of massive molecular gas reservoirs in dusty early-type galaxies
• The OTELO survey: Nature and mass-metallicity relation for H$\alpha$ emitters at $z\sim 0.4$
• Galaxy and Mass Assembly (GAMA): Probing the merger histories of massive galaxies via stellar populations
• How to Interpret Measurements of Diffuse Light in Stacked Observations of Groups and Clusters of Galaxies
• The MAGPI Survey: Impact of environment on the total internal mass distribution of galaxies in the last 5 Gyr
• Galaxy-Galaxy Lensing in EAGLE: comparison with data from 180 square degrees of the KiDS and GAMA surveys
• FLASH Pilot Survey: Detections of associated 21 cm HI absorption in GAMA galaxies at 0.42 < z <1.00
• The $XXL$ survey: XL. Obscuration properties of red AGN in $XXL-N$
• The SAMI Galaxy Survey: Kinematics of stars and gas in brightest group galaxies; the role of group dynamics
• Galaxy And Mass Assembly (GAMA): The group HI mass as a function of halo mass
• The 2-degree Field Lensing Survey: photometric redshifts from a large new training sample to r<19.5
• Wide Area VISTA Extra-galactic Survey (WAVES): Unsupervised star-galaxy separation on the WAVES-Wide photometric input catalogue using UMAP and $\mathrm{HDBSCAN}$
• New-generation dust emission templates for star-forming galaxies
• Galaxy And Mass Assembly: Group and field galaxy morphologies in the star-formation rate - stellar mass plane
• Searching for Dark Matter Signals from Local Dwarf Spheroidal Galaxies at Low Radio Frequencies in the GLEAM Survey
• MAGIC: Muse gAlaxy Groups In Cosmos -- A survey to probe the impact of environment on galaxy evolution over the last 8 Gyr
• Over-density of SMGs in fields containing z~0.3 galaxies: magnification bias and the implications for studies of galaxy evolution
• Discovery of a Bimodal Environmental Distribution of Compact Ellipticals in the Local Universe
• Bayesian fitting of multi-Gaussian expansion models to galaxy images
• DESI Complete Calibration of the Color-Redshift Relation (DC3R2): Results from early DESI data
• The first shear measurements from precision weak lensing
• An Optical Spectrum of the Diffuse Galactic Light from BOSS and IRIS
• Subaru Hyper Suprime-Cam excavates colossal over- and under-dense structures over 360 deg2 out to z=1
• Galaxy And Mass Assembly: Galaxy Zoo spiral arms and star formation rates
• The Infrared Properties of Sources Matched in the WISE all-sky and Herschel-ATLAS Surveys
• Local Volume HI Survey: the far-infrared radio correlation
• Modelling the evolution and influence of dust in cosmological simulations that include the cold phase of the interstellar medium
• TEGLIE: Transformer encoders as strong gravitational lens finders in KiDS
• Galaxy And Mass Assembly (GAMA): Defining Passive Galaxy Samples and Searching for the UV Upturn
• Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
• SAMI-HI: The HI view of the H$\alpha$ Tully-Fisher relation and data release
• Tomography-based observational measurements of the halo mass function via the submillimeter magnification bias
• A radiation transfer model for the Milky Way. II The global properties and large scale structure
• Long-term stability of fibre-optic transmission for multi-object spectroscopy
• The XXL Survey: XXXIV. Double irony in XXL-North. A tale of two radio galaxies in a supercluster at z = 0.14
• Artificial neural network based calibrations for the prediction of galactic [NII] $\lambda$ 6584 and H$\alpha$ line luminosities
• BASILISK: Bayesian Hierarchical Inference of the Galaxy-Halo Connection using Satellite Kinematics--I. Method and Validation
• The detection of a massive chain of dark HI clouds in the GAMA G23 Field
• The SAMI Galaxy Survey: Using concentrated star-formation and stellar population ages to understand environmental quenching
• Non-Parametric Cell-Based Photometric Proxies for Galaxy Morphology: Methodology and Application to the Morphologically-Defined Star Formation -- Stellar Mass Relation of Spiral Galaxies in the Local Universe
• Ageing and Quenching through the ageing diagram II: physical characterization of galaxies
• Emission-line Stacking of 21cm Intensity Maps with MeerKLASS: Inference Pipeline and Application to the L-band Deep-field Data
• Cosmological surveys with multi-object spectrographs
• Galaxy-scale gravitational lens candidates from the Hyper Suprime-Cam imaging survey and the Galaxy And Mass Assembly spectroscopic survey
• The SAMI Galaxy Survey: The contribution of different kinematic classes to the stellar mass function of nearby galaxies
• The Dragonfly Wide Field Survey. II. Accurate Total Luminosities and Colors of Nearby Massive Galaxies and Implications for the Galaxy Stellar Mass Function
• The GALAH Survey: Relative throughputs of the 2dF fibre positioner and the HERMES spectrograph from stellar targets
• The Subaru HSC weak lensing mass-observable scaling relations of spectroscopic galaxy groups from the GAMA survey
• On the origin of red spirals: Does assembly bias play a role?
• Quasi-stellar objects and galaxy mass density profiles derived using the submillimetre galaxies magnification bias
• Probing galaxy evolution through HI 21-cm emission and absorption: current status and prospects with the Square Kilometre Array
• Ridges in the Dark Energy Survey for cosmic trough identification
• SYNMAG Photometry: A Fast Tool for Catalog-Level Matched Colors of Extended Sources
• Connecting MeerKAT radio continuum properties to GAMA optical emission-line and WISE mid-infrared activity
• Galaxy and Mass Assembly (GAMA): the clustering of galaxy groups
• The faint end of the 250 micron luminosity function at z < 0.5
• VEXAS: VISTA EXtension to Auxiliary Surveys -- Data Release 2: Machine-learning based classification of sources in the Southern Hemisphere
• The Loneliest Galaxies in the Universe: A GAMA and GalaxyZoo Study on Void Galaxy Morphology
• The SAMI Galaxy Survey: embedded discs and radial trends in outer dynamical support across the Hubble sequence
• Detection, size, measurement and structural analysis limits for the 2MASS, UKIDSS-LAS & VISTA VIKING surveys
• Assessing Mass Loss and Stellar-to-Halo Mass Ratio of Satellite Galaxies: A Galaxy-Galaxy Lensing Approach Utilizing DECaLS DR8 Data
• PAC in DESI. I. Galaxy Stellar Mass Function into the $10^6{\mathrm{M}}_{\odot }$ Frontier
• Galaxy And Mass Assembly (GAMA): Stellar-to-Dynamical Mass Relation I. Constraining the Precision of Stellar Mass Estimates
• Herschel-ATLAS/GAMA:How does the far-IR luminosity function depend on galaxy group properties?
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• Galaxy Mergers in the Epoch of Reionization II: Major Merger-Triggered Star Formation and AGN Activities at $z=$ 4.5-8.5
• Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies in the Local Universe II. -- Direct Measurement of the Dependencies on Redshift and Host Halo Mass of Stellar Mass Growth in Central Disk Galaxies
• The PAU Survey: Photometric redshift estimation in deep wide fields
• Selection of powerful radio galaxies with machine learning
• Intrinsic galaxy alignments in the KiDS-1000 bright sample: dependence on colour, luminosity, morphology, and galaxy scale
• Galaxy And Mass Assembly (GAMA) Survey: The Merging Potential of Brightest Group Galaxies
• FRB Line-of-sight Ionization Measurement From Lightcone AAOmega Mapping Survey: the First Data Release
• Mass-morphology relation of TNG50 galaxies
• VEXAS: the VISTA EXtension to Auxiliary Surveys -- Data Release 1: the Southern Galactic Hemisphere
• Halo shapes constrained from a pure sample of central galaxies in KiDS-1000
• Galaxy And Mass Assembly (GAMA): the signatures of galaxy interactions as viewed from small scale galaxy clustering
• The XMM Cluster Survey: An independent demonstration of the fidelity of the eFEDS galaxy cluster data products and implications for future studies
• Galaxy cluster mass density profile derived using the submillimetre galaxies magnification bias
• Supersoft, luminous X-ray sources in galactic nuclei
• PEARLS: Low Stellar Density Galaxies in the El Gordo Cluster Observed with JWST
• Comprehensive view on a $z\sim 6.5$ radio-loud QSO: from the radio to the optical/NIR to the X-ray band
• The Many Assembly Histories of Massive Void Galaxies as Revealed by Integral Field Spectroscopy
• The XMM Cluster Survey: Exploring scaling relations and completeness of the Dark Energy Survey Year 3 redMaPPer cluster catalogue
• SCONCE: A cosmic web finder for spherical and conic geometries
• Galaxy-halo size relation from Sloan Digital Sky Survey Data Release 7 and the ELUCID simulation
• The variation of the gas content of galaxy groups and pairs compared to isolated galaxies
• The SAMI Galaxy Survey: Detection of Environmental Dependence of Galaxy Spin in Observations and Simulations Using Marked Correlation Functions
• Galaxy And Mass Assembly (GAMA): The environmental impact on SFR and metallicity in galaxy groups
• Assembly bias evidence in close galaxy pairs
• High-$z$ radio Quasars in RACS I: Selection, identification, and multi-wavelength properties
• The SAMI Galaxy Survey: rules of behaviour for spin-ellipticity radial tracks in galaxies
• Galaxy Properties Derived with Spectral Energy Distribution Fitting in the Hawaii-Hubble Deep Field-North
• Enhancing Photometric Redshift Catalogs Through Color-Space Analysis: Application to KiDS-Bright Galaxies
• A serendipitous discovery of HI-rich galaxy groups with MeerKAT
• The MAGPI survey: The interdependence of the mass, star formation rate, and metallicity in galaxies at z~0.3
• The SAMI Galaxy Survey: Trends in [α/Fe] as a Function of Morphology and Environment
• Star formation concentration as a tracer of environmental quenching in action: a study of the Eagle and C-Eagle simulations
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• Toward a stellar population catalog in the Kilo Degree Survey: the impact of stellar recipes on stellar masses and star formation rates
• NeutralUniverseMachine: How Filaments and Dark Matter Halo Influence the Galaxy Cold Gas Content
• The Shape of FIREbox Galaxies and a Potential Tension with Low-mass Disks
• Shape noise and dispersion in precision weak lensing
• Age-Divided Mean Stellar Populations from Full Spectrum Fitting as the Simplified Star Formation and Chemical Evolution History of a Galaxy: Methodology and Reliability
• Degradation analysis in the estimation of photometric redshifts from non-representative training sets
• Correlating galaxy shapes and initial conditions: an observational study
• The XXL Survey XLV. Linking the ages of optically selected groups to their X-ray emission
• COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase
• Cosmological constraints from galaxy clustering and galaxy-galaxy lensing with extended SubHalo Abundance Matching
• The Sami Galaxy Survey: stellar populations of passive spiral galaxies in different environment
• AMICO galaxy clusters in KiDS-1000: cosmological constraints and mass calibration from counts and weak lensing
• The XXL Survey: IX. Optical overdensity and radio continuum analysis of a supercluster at $z=0.43$
• Searching for low-redshift faint galaxies with MMT/Hectospec
• Dark Energy Survey Deep Field photometric redshift performance and training incompleteness assessment
• Galaxy and Mass Assembly (GAMA): Low-redshift Quasars and Inactive Galaxies Have Similar Neighbors
• Red riding on hood: Exploring how galaxy colour depends on environment
• UV and NIR size of the low-mass field galaxies: the UV compact galaxies
• SAMI-HI: the connection between global asymmetry in the ionised and neutral atomic hydrogen gas in galaxies
• The SAMI Galaxy Survey: Disk-halo interactions in radio-selected star-forming galaxies
• KiDS+VIKING+GAMA: Testing semi-analytic models of galaxy evolution with galaxy-galaxy-galaxy lensing
• Dust effects on the derived Sersic indexes of disks and bulges in spiral galaxies
• The case for two-dimensional galaxy-galaxy lensing
• A morphological segmentation approach to determining bar lengths
• Galaxy and Mass Assembly (GAMA): Mid-infrared properties as tracers of galaxy environment
• IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
• IllustrisTNG in the HSC-SSP: No Shortage of Thin Disk Galaxies in TNG50
• Morpho-Photometric Classification of KiDS DR5 Sources Based on Neural Networks: A Comprehensive Star-Quasar-Galaxy Catalog
• An Optimized Ly$\alpha$ Forest Inversion Tool Based on a Quantitative Comparison of Existing Reconstruction Methods
• The 2.4 $\mu$m Galaxy Luminosity Function as Measured Using WISE. III. Measurement Results
• The circular velocity and halo mass functions of galaxies in the nearby Universe
• A search for HI absorption in distant star-forming galaxies with ASKAP-FLASH -- I. Selection and analysis of the radio sample
• Modeling Strong Lenses from Wide-Field Ground-Based Observations in KiDS and GAMA
• A new approach to finding galaxy groups using Markov Clustering
• AMICO galaxy clusters in KiDS-1000: cosmological sample
• An Empirical Mass Function Distribution
• Galaxy and Mass Assembly (GAMA): Probing galaxy-group correlations in redshift space with the halo streaming model
• Model-Independent Test for Gravity using Intensity Mapping and Galaxy Clustering
• Deep Large Binocular Camera r-band Observations of the GOODS-N Field
• Spectrophotometric redshifts for $\mathrm{z}\sim 1$ galaxies and predictions for number densities with WFIRST and Euclid
• GAMA 526784: the progenitor of a globular cluster-rich ultra-diffuse galaxy? I. Star clusters, stellar body and ionised gas properties
• The unusual ISM in Blue and Dusty Gas Rich Galaxies (BADGRS)
• Galaxy And Mass Assembly (GAMA): The M-Z relation for galaxy groups
• HMFcalc: An Online Tool for Calculating Dark Matter Halo Mass Functions
• Probing Satellite Halos with Weak Gravitational Lensing
• HI Intensity Mapping with the MIGHTEE Survey: First Results of the HI Power Spectrum
• A Global Census of Metals in the Universe
• Inferring Host Dark Matter Halo Masses of Individual Galaxies from Neighboring Galaxy Counts
• The SAMI Galaxy Survey: The relationship between galaxy rotation and the motion of neighbours
• Searching for galaxy clusters in the VST-KiDS Survey
• On the Origin of the Variety of Velocity Dispersion Profiles of Galaxies
• Uncovering the truth about M101, NGC 3938, and their significant others through radiative transfer
• FPFS Shear Estimator: Systematic Tests on the Hyper Suprime-Cam Survey First Year Data
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• Direct Shear Mapping: Prospects for weak lensing studies of individual galaxy-galaxy lensing systems
• Pulsar B1237+25 Aberration/Retardation Analysis from Decimeter to Decameter Wavelength: Challenge to "Radius-to-Frequency Mapping"
• Dust sub-millimetre emission in green valley galaxies
• Deep Extragalactic VIsible Legacy Survey (DEVILS): First Data Release Covering The D10 (COSMOS) Region
• Echoes from the dark: Galaxy catalog incompleteness in standard siren cosmology
• Evolution of the star formation rate surface density main sequence. Insights from a semi-analytic simulation since $z=12$
• The role of gas stripping in the quenching of satellite galaxies using SHARK v2.0
• The SAMI Survey: Evidence for dynamical coupling of ionised gas and young stellar populations
• Galactic bars and active galactic nucleus fuelling in the second half of cosmic history
• Star-forming galaxies in the cosmic web in the last 11 Gyr
• The galaxy luminosity function in the LAMOST Complete Spectroscopic Survey of Pointing Area at the Southern Galactic Cap
• Relighting the fire in Hickson Compact Group (HCG) 15: magnetised fossil plasma revealed by the SKA Pathfinders & Precursors
• FAST drift scan survey for HI intensity mapping: simulation on hunting HI filament with pairwise stacking
• On the Dichotomy between Normal and Dwarf Ellipticals
• Cosmic Insights from Galaxy Clusters: Exploring Magnification Bias on Sub-millimeter Galaxies
• Euclid: Constraining ensemble photometric redshift distributions with stacked spectroscopy
• Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
• SEMPER I. Radio Predictions for Star-Forming Galaxies at $0<z<5$
• Galaxy evolution within the Kilo-Degree Survey
• Impact of the large-scale cosmic web on the X-ray emitting circumgalactic medium
• Methodological refinement of the submillimeter galaxy cross-correlation function measurements and their uncertainty estimation
• Panchromatic properties of galaxies in wide-field optical spectroscopic and photometric surveys
• A group finder algorithm optimised for the study of local galaxy environment
• The LEGA-C and SAMI Galaxy Surveys: Quiescent Stellar Populations and the Mass-Size Plane across 6 Gyr
• Toward accurate measurement of property-dependent galaxy clustering: II. Tests of the smoothed density-corrected $V_{\max }$ method
• Galaxy And Mass Assembly: A new approach to quantifying dust in galaxies
• Dust removal timescale in galaxies across cosmic time
• Measuring Cosmic Density of Neutral Hydrogen via Stacking the DINGO-VLA Data
• The intragroup light in KiDS+GAMA groups: A stacking analysis
• Covariances of Galaxy Stellar Mass Functions and Correlation Functions
• Using Deep Learning Methods to Detect for Ultra-diffuse Galaxies in KiDS
• Mechanisms Affecting Galaxies Nearby and Environmental Trends (MAGNET)
• ATCA detections of massive molecular gas reservoirs in dusty, high-z radio galaxies
• Tracing the environmental history of observed galaxies via extended fast action minimization method
• Measuring the evolution of stellar bars with the host galaxy's spin
• Emergence of red, star-forming galaxies (red misfits) in a ΛCDM universe
• The GAMA Panchromatic Survey
• Signatures of large-scale cold fronts in the optically-selected merging cluster HSC J085024+001536
• The 2.4 $\mu$m Galaxy Luminosity Function as Measured Using WISE. II. Sample Selection
• Galaxy And Mass Assembly (GAMA): From filaments to voids, how extreme environment affects gas metallicity and SFR in galaxies
• The VIMOS VLT Deep Survey. The different assembly history of passive and star-forming L_B >= L*_B galaxies in the group environment at z < 1
• Hosts and environments: a (large-scale) radio history of AGN and star-forming galaxies
• Faint galaxies in the Zone of Avoidance revealed by JWST/NIRCam
• Galaxy And Mass Assembly (GAMA): The Dependence of Star Formation on Surface Brightness in Low Redshift Galaxies
• Cosmic magnification on high-redshift submillimeter galaxies
• The contribution of stars, dust, neutral gas and supermassive black holes in galaxies to the cosmic baryon inventory
• Hybrid-z: Enhancing Kilo-Degree Survey bright galaxy sample photometric redshifts with deep learning
• A MOND model applied to the rotation curve of galaxies
• Deep ASKAP EMU Survey of the GAMA23 field: Properties of radio sources
• TOPz: Photometric redshifts using template fitting applied to the GAMA survey
• Extending the SAGA Survey (xSAGA) I: Satellite Radial Profiles as a Function of Host Galaxy Properties
• Mapping Nearby Galaxies with Apache Point Observatory: Group and field galaxies' morphologies in the colour-magnitude plane
• GalSBI-SPS: a stellar population synthesis-based galaxy population model for cosmology and galaxy evolution applications
• Observed structural parameters of EAGLE galaxies: reconciling the mass-size relation in simulations with local observations
• The effect of spiral arms on the Sérsic photometry of galaxies
• Galaxy Evolution in the Local Universe: Group Richness Effects on Mergers and Non-Mergers
• Galaxy quenching across the Cosmic Web: disentangling mass and environment with SDSS DR18
• Exploring the effect of baryons on the radial distribution of satellite galaxies with GAMA and IllustrisTNG
• A lightcone catalogue from the Millennium-XXL simulation: improved spatial interpolation and colour distributions for the DESI BGS
• The SAMI Galaxy Survey: first 1000 galaxies
• CNN photometric redshifts in the SDSS at $r\le 20$
• AMICO galaxy clusters in KiDS-DR3: the impact of estimator statistics on the luminosity-mass scaling relation
• A novel Cosmic Filament catalogue from SDSS data
• Sahyadri: A simulation suite for the cosmology dependence of the Cosmic Web
• Euclid preparation. 3D reconstruction of the cosmic web with simulated Euclid Deep spectroscopic samples
• AMICO galaxy clusters in KiDS-1000: Splashback radius from weak lensing and cluster-galaxy correlation function
• Galaxy And Mass Assembly: A Comparison between Galaxy-Galaxy Lens Searches in KiDS/GAMA
• CHILES XII: The H I evolution of Luminous Compact Blue Galaxies between 0<z<0.48