The 2dF Galaxy Redshift Survey: Spectra and redshifts

Abstract

The 2dF Galaxy Redshift Survey (2dFGRS) is designed to measure redshifts for approximately 250000 galaxies. This paper describes the survey design, the spectroscopic observations, the redshift measurements and the survey database. The 2dFGRS uses the 2dF multi-fibre spectrograph on the Anglo-Australian Telescope, which is capable of observing 400 objects simultaneously over a 2-degree diameter field. The source catalogue for the survey is a revised and extended version of the APM galaxy catalogue, and the targets are galaxies with extinction-corrected magnitudes brighter than b_J=19.45. The main survey regions are two declination strips, one in the southern Galactic hemisphere spanning 80deg x 15deg around the SGP, and the other in the northern Galactic hemisphere spanning 75deg x 10deg along the celestial equator; in addition, there are 99 fields spread over the southern Galactic cap. The survey covers 2000 sq.deg and has a median depth of z=0.11. Adaptive tiling is used to give a highly uniform sampling rate of 93% over the whole survey region. Redshifts are measured from spectra covering 3600A-8000A at a two-pixel resolution of 9.0A and a median S/N of 13 per pixel. All redshift identifications are visually checked and assigned a quality parameter Q in the range 1-5; Q>=3 redshifts are 98.4% reliable and have an rms uncertainty of 85 km/s. The overall redshift completeness for Q>=3 redshifts is 91.8%, but this varies with magnitude from 99% for the brightest galaxies to 90% for objects at the survey limit. The 2dFGRS database is available on the WWW at http://www.mso.anu.edu.au/2dFGRS

accepted by MNRAS; version with high-resolution figures at http://www.mso.anu.edu.au/2dFGRS/Public/Publications; accompanies the 2dFGRS 100k Release, now available at http://www.mso.anu.edu.au/2dFGRS

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• Beyond the Linear-Order Relativistic Effect in Galaxy Clustering: Second-Order Gauge-Invariant Formalism
• The FLAMINGOS Extragalactic Survey
• The Rise of the First Stars: Supersonic Streaming, Radiative Feedback, and 21-cm Cosmology
• H-ATLAS/GAMA: Dusty early-type galaxies and passive spirals
• The SAMI Galaxy Survey: the third and final data release
• The LOFAR Two Metre Sky Survey: Deep Fields Data Release 1 -- III. Host-galaxy identifications and value added catalogues
• GRB 060505: A possible short-duration gamma-ray burst in a star forming region at redshift of 0.09
• Kinematic Properties and Stellar Populations of Faint Early-Type Galaxies. I. Velocity Dispersion Measurements of Central Coma Galaxies
• The stellar population histories of early-type galaxies. III. The Coma Cluster
• Cosmological Signatures of Interacting Neutrinos
• Cosmic Voids and Void Lensing in the Dark Energy Survey Science Verification Data
• Detection of strong clustering of red K-selected galaxies at 2<z_phot<4 in the Hubble Deep Field South
• The evolution of the ultraviolet and infrared luminosity densities in the universe at 0<z<1
• Galaxy morphology in the LambdaCDM cosmology
• The Dependence of Galaxy Formation on Cosmological Parameters: Can we distinguish the WMAP1 and WMAP3 Parameter Sets?
• Cosmic Web and Star Formation Activity in Galaxies at z~1
• Fossil evidence for spin alignment of SDSS galaxies in filaments
• Galaxy groups in the 2dF redshift survey: The catalogue
• The evolution of the galaxy stellar mass function over the last twelve billion years from a combination of ground-based and HST surveys
• Bayesian power-spectrum inference for Large Scale Structure data
• A scheme to deal accurately and efficiently with complex angular masks in galaxy surveys
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Motivation, Design and Target Catalogue
• A Note on Tsallis Holographic Dark Energy
• Clues on void evolution II: Measuring density and velocity profiles on SDSS galaxy redshift space distortions
• Galaxy Pairs in the 2dFGRS II. Effects of interactions on star formation in groups and clusters
• Incidence of WISE-Selected Obscured AGNs in Major Mergers and Interactions from the SDSS
• Satellites of Simulated Galaxies: survival, merging, and their relation to the dark and stellar halos
• Giant radio galaxies in the LOFAR Two-metre Sky Survey-I
• Observational constraints on the linear fluctuation growth rate
• Populating Dark Matter Haloes with Galaxies: Comparing the 2dFGRS with Mock Galaxy Redshift Surveys
• Matter power spectrum: from Ly$\alpha$ forest to CMB scales
• The SAMI Galaxy Survey: Cubism and covariance, putting round pegs into square holes
• Evolution of the Radio Loud Galaxy Population
• Red-sequence galaxies with young stars and dust: The cluster Abell 901/902 seen with COMBO-17
• Constraining f(R) gravity in the Palatini formalism
• The mass profile of galaxy clusters out to ~2 r200
• The Evolution of the Optical and Near-Infrared Galaxy Luminosity Functions and Luminosity Densities to z~2
• AEGIS: The Morphologies of Green Galaxies at 0.4<z<1.2
• SDSS Galaxy Clustering: Luminosity & Colour Dependence and Stochasticity
• Galaxy Kinematics with VIRUS-P: The Dark Matter Halo of M87
• Three Different Types of Galaxy Alignment within Dark Matter Halos
• GROWTH on S190814bv: Deep Synoptic Limits on the Optical/Near-Infrared Counterpart to a Neutron Star-Black Hole Merger
• Redshift-Space Distortions with the Halo Occupation Distribution II: Analytic Model
• The Pantheon+ Analysis: Evaluating Peculiar Velocity Corrections in Cosmological Analyses with Nearby Type Ia Supernovae
• Mapping Large-Scale Structures Behind the Galactic Plane: The Second CIZA Subsample
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological constraints from the full shape of the clustering wedges
• Low Redshift Baryon Acoustic Oscillation Measurement from the Reconstructed 6-degree Field Galaxy Survey
• Growth factor parametrization and modified gravity
• Breaking the Degeneracies Between Cosmology and Galaxy Bias
• The spatial clustering of X-ray selected AGN in the XMM-COSMOS field
• Void Statistics in Large Galaxy Redshift Surveys: Does Halo Occupation of Field Galaxies Depend on Environment?
• The SAMI Galaxy Survey: Spatially resolving the environmental quenching of star formation in GAMA galaxies
• A 2dF spectroscopic study of globular clusters in NGC 5128: Probing the formation history of the nearest giant Elliptical
• MegaZ-LRG: A photometric redshift catalogue of one million SDSS Luminous Red Galaxies
• Viscous dark fluid universe
• A Deep Search For Faint Galaxies Associated With Very Low-redshift C IV Absorbers: III. The Mass- and Environment-dependent Circumgalactic Medium
• The Las Campanas IR Survey. II. Photometric redshifts, comparison with models and clustering evolution
• High redshift quasars in the COSMOS survey: the space density of z>3 X-ray selected QSOs
• Pre-processing of galaxies in cosmic filaments around AMASCFI clusters in the CFHTLS
• Galaxy And Mass Assembly (GAMA): Refining the Local Galaxy Merger Rate using Morphological Information
• Superclusters of galaxies from the 2dF redshift survey. I. The catalogue
• The Halo Distribution of 2dF Galaxies
• Fractal Dimension as a measure of the scale of Homogeneity
• The Central Engines of Fermi Blazars
• Shear Selected Cluster Cosmology I: Tomography and Optimal Filtering
• The Cross-Correlation between Galaxies and Groups: Probing the Galaxy Distribution in and around Dark Matter Haloes
• The WiggleZ Dark Energy Survey: the selection function and z=0.6 galaxy power spectrum
• The Mass Assembly of Fossil Groups of Galaxies in the Millennium Simulation
• Where are the stars?
• The Phase-Space Parameters of Brightest Halo Galaxies
• CAIRNS: The Cluster And Infall Region Nearby Survey III. Environmental Dependence of H-alpha Properties of Galaxies
• Does a 'stochastic' background of gravitational waves exist in the pulsar timing band?
• The Beginning and Evolution of the Universe
• Galaxy Colour, Morphology, and Environment in the Sloan Digital Sky Survey
• OzDES multifibre spectroscopy for the Dark Energy Survey: Three year results and first data release
• Luminous K-band Selected Quasars from UKIDSS
• Revealing the galaxy-halo connection in IllustrisTNG
• Cosmological constraints on a decomposed Chaplygin gas
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Gravity test from the combination of redshift-space distortions and galaxy-galaxy lensing at $0.5<z<1.2$
• Dynamics of Interacting Quintessence Models: Observational Constraints
• The Las Campanas/AAT Rich Cluster Survey III: Spectroscopic Studies of X-ray Bright Galaxy Clusters at z~0.1
• Galaxy and Mass Assembly (GAMA): Exploring the WISE Cosmic Web in G12
• The X-ray to [Ne V]3426 flux ratio: discovering heavily obscured AGN in the distant Universe
• The clustering of H-alpha emitters at z=2.23 from HiZELS
• Statistical Analysis of Galaxy Surveys-II. The 3-point galaxy correlation function measured from the 2dFGRS
• The Abundance and Radial Distribution of Satellite Galaxies
• Discovery of a large-scale filament connected to the massive galaxy cluster MACSJ0717.5+3745 at z=0.55
• The subhalo - satellite connection and the fate of disrupted satellite galaxies
• Evolution of the universe in entropic cosmologies via different formulations
• Studying the emergence of the red sequence through galaxy clustering: host halo masses at z > 2
• A Multiwavelength Study of a Sample of 70 micron Selected Galaxies in the COSMOS Field I: Spectral Energy Distributions and Luminosities
• An Extended Halo-based Group/Cluster finder: application to the DESI legacy imaging surveys DR8
• Constraints on the Alignment of Galaxies in Galaxy Clusters from $\sim$14,000 Spectroscopic Members
• The Herschel-ATLAS Data Release 1 Paper II: Multi-wavelength counterparts to submillimetre sources
• The ALMA Fornax Cluster Survey I: stirring and stripping of the molecular gas in cluster galaxies
• The Influence of Large-Scale Structure on Halo Shapes and Alignments
• HELP: The Herschel Extragalactic Legacy Project
• Cosmological parameter estimation using Very Small Array data out to l=1500
• The Effect of Large-Scale Structure on the SDSS Galaxy Three-Point Correlation Function
• The SAMI Galaxy Survey: The cluster redshift survey, target selection and cluster properties
• Radio galaxies in the 2SLAQ Luminous Red Galaxy Survey: I. The evolution of low-power radio galaxies to z~0.7
• Timing the formation and assembly of early-type galaxies via spatially resolved stellar populations analysis
• The VIMOS VLT Deep Survey - The evolution of galaxy clustering to z=2 from first epoch observations
• Clues on void evolution I: Large scale galaxy distributions around voids
• The 2dF Galaxy Redshift Survey: Wiener Reconstruction of the Cosmic Web
• Alignment between galaxies and large-scale structure
• Galaxy clustering, photometric redshifts and diagnosis of systematics in the DES Science Verification data
• Fourier analysis of luminosity-dependent galaxy clustering
• The New Horizon Run Cosmological N-Body Simulations
• The VANDELS ESO public spectroscopic survey: final Data Release of 2087 spectra and spectroscopic measurements
• P-MaNGA: Gradients in Recent Star Formation Histories as Diagnostics for Galaxy Growth and Death
• Shapes and Sizes of Voids in the LCDM Universe: Excursion Set Approach
• The Spitzer mid-infrared AGN survey. I - optical and near-infrared spectroscopy of candidate obscured and normal AGN selected in the mid-infrared
• SDSS-IV MaNGA: stellar population gradients as a function of galaxy environment
• The Nature of Massive Transition Galaxies in CANDELS, GAMA, and Cosmological Simulations
• Isolating Triggered Star Formation
• Upper limits on neutrino masses from the 2dFGRS and WMAP: the role of priors
• Galaxy and Mass Assembly (GAMA): Fine filaments of galaxies detected within voids
• Redshift-Space Distortions with the Halo Occupation Distribution I: Numerical Simulations
• Probing the Intrinsic Shape and Alignment of Dark Matter Haloes using SDSS Galaxy Groups
• The Observations of Redshift Evolution in Large Scale Environments (ORELSE) Survey : I. The Survey Design and First Results on Cl 0023+0423 at z = 0.84 and RX J1821.6+6827 at z = 0.82
• CLASH: Complete Lensing Analysis of the Largest Cosmic Lens MACS J0717.5+3745 and Surrounding Structures
• Galaxy interactions I: Major and minor mergers
• The Local Hole in the Galaxy Distribution: Evidence from 2MASS
• Newtonian Perturbations on Models with Matter Creation
• The Three-Point Correlation Function of Luminous Red Galaxies in the Sloan Digital Sky Survey
• Tracing The Sound Horizon Scale With Photometric Redshift Surveys
• Observational Evidence for an Age Dependence of Halo Bias
• Reconstructing the cosmic density field with the distribution of dark matter halos
• The Millennium Galaxy Catalogue: Dynamically Close Galaxy Pairs and the Global Merger Rate
• Observational constraints on the optical and near-infrared emission from the neutron star-black hole binary merger S190814bv
• Galaxy and Mass Assembly (GAMA): The halo mass of galaxy groups from maximum-likelihood weak lensing
• The VIMOS VLT Deep Survey: Evolution of the non-linear galaxy bias up to z=1.5
• The Taipan Galaxy Survey: Scientific Goals and Observing Strategy
• The zCOSMOS survey: the role of the environment in the evolution of the luminosity function of different galaxy types
• The evolution of the number density of compact galaxies
• Modelling and interpreting the dependence of clustering on the spectral energy distributions of galaxies
• Satellite abundances around bright isolated galaxies II: radial distribution and environmental effects
• Low-Surface-Brightness Galaxies in the Sloan Digital Sky Survey. I. Search Method and Test Sample
• The Spatial Clustering of ROSAT All-Sky Survey AGNs III. Expanded Sample and Comparison with Optical AGNs
• Statistics of Voids in the 2dF Galaxy Redshift Survey
• Preheating by Previrialization and its Impact on Galaxy Formation
• Clustering of Lyman alpha emitters at z ~ 4.5
• Measuring dark energy properties with 3D cosmic shear
• The 3-point function in large scale structure: redshift distortions and galaxy bias
• Substructure and galaxy formation in the Copernicus Complexio warm dark matter simulations
• Satellite Galaxies and Fossil Groups in the Millennium Simulation
• Unified dark energy models : a phenomenological approach
• Constraining amplitude and slope of the mass fluctuation spectrum using cluster baryon mass function
• Prediction of the Cosmic Evolution of the CO-Luminosity Functions
• Measuring the mean and scatter of the X-ray luminosity -- optical richness relation for maxBCG galaxy clusters
• Wide Angle Effects in Future Galaxy Surveys
• The 2-degree Field Lensing Survey: design and clustering measurements
• xGASS: Gas-rich central galaxies in small groups and their connections to cosmic web gas feeding
• Groups of galaxies in the SDSS Data Release 5. A group-finder and a catalogue
• Search and analysis of giant radio galaxies with associated nuclei (SAGAN) -- I : New sample and multi-wavelength studies
• nIFTy Cosmology: Galaxy/halo mock catalogue comparison project on clustering statistics
• A clear and measurable signature of modified gravity in the galaxy velocity field
• And yet it flips: connecting galactic spin and the cosmic web
• The Orientation of Satellite Galaxies: Evidence of Elongation in the Direction of the Host
• ZFIRE: A KECK/MOSFIRE Spectroscopic Survey of Galaxies in Rich Environments at z~2
• Viable Palatini-f(R) cosmologies with generalized dark matter
• Old and young bulges in late-type disk galaxies
• The Baryon Content of Dark Matter Halos: Empirical Constraints from MgII Absorbers
• How common is the Milky Way - satellite system alignment?
• Galaxy And Mass Assembly (GAMA): The galaxy luminosity function within the cosmic web
• The SAMI Galaxy Survey: Quenching of star formation in clusters I. Transition galaxies
• The orientation of galaxy dark matter haloes around cosmic voids
• Tracing Galaxies Through Cosmic Time with Number Density Selection
• The 2dF Galaxy Redshift Survey: higher order galaxy correlation functions
• Predictions on the angular power spectrum of clustered extragalactic point sources at CMB frequencies from flat and all--sky 2D-simulations
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: anisotropic clustering analysis in configuration-space
• The Suppression of Star Formation and the Effect of Galaxy Environment in Low-Redshift Galaxy Groups
• Spatial and kinematic alignments between central and satellite halos
• Anisotropic Locations of Satellite Galaxies: Clues to the Orientations of Galaxies within their Dark Matter Halos
• Constraints on the coupled quintessence from cosmic microwave background anisotropy and matter power spectrum
• The 2dF Galaxy Redshift Survey: voids and hierarchical scaling models
• An analytic model for the bispectrum of galaxies in redshift space
• Inter-cluster Filaments of Galaxies Programme: Abundance and Distribution of Filaments in the 2dFGRS Catalogue
• Void Ellipticity Distribution as a Probe of Cosmology
• Effects of galaxy interactions in different environments
• The SAMI Galaxy Survey: Data Release One with Emission-line Physics Value-Added Products
• Luminosity dependence of the spatial and velocity distributions of galaxies: Semi-analytic models versus the Sloan Digital Sky Survey
• Angular distribution of satellite galaxies from the Sloan Digital Sky Survey Data Release 4
• Large Scale Structure in the SDSS DR1 Galaxy Survey
• Large Scale Structure in the SDSS Galaxy Survey
• The Dependence of the Galaxy Luminosity Function on Large-Scale Environment
• CAIRNS: The Cluster And Infall Region Nearby Survey II. Environmental Dependence of Infrared Mass-to-Light Ratios
• The Local Hole revealed by galaxy counts and redshifts
• Cosmological dynamics with non-linear interactions
• A z=2.5 protocluster associated with the radio galaxy MRC 2104-242: star formation and differing mass functions in dense environments
• Fast simulations for intensity mapping experiments
• The Three-point Correlation Function of Galaxies Determined from the 2dF Galaxy Redshift Survey
• Transformation of Morphology and Luminosity Classes of the SDSS Galaxies
• The DEEP2 Galaxy Redshift Survey: Clustering Dependence on Galaxy Stellar Mass and Star Formation Rate at z~1
• Environmental Dependence of Local Luminous Infrared Galaxies
• High Eccentricities and High Masses Characterize Gravitational-wave Captures in Galactic Nuclei as Seen by Earth-based Detectors
• Differences in Faraday Rotation Between Adjacent Extragalactic Radio Sources as a Probe of Cosmic Magnetic Fields
• The Anisotropic Distribution of Satellite Galaxies
• A Cosmic Void Catalog of SDSS DR12 BOSS Galaxies
• The luminosity-dependent high-redshift turnover in the steep spectrum radio luminosity function: clear evidence for downsizing in the radio-AGN population
• Cosmological Constraints from a Combination of Galaxy Clustering & Lensing -- II. Fisher Matrix Analysis
• VLT-VIMOS integral field spectroscopy of luminous and ultraluminous infrared galaxies. I. The sample and first results
• Observational Requirements for Lyman-alpha Forest Tomographic Mapping of Large-Scale Structure at z ~ 2
• STAGES: the Space Telescope A901/2 Galaxy Evolution Survey
• DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
• The Millennium Galaxy Catalogue: The photometric accuracy, completeness and contamination of the 2dFGRS and SDSS-EDR & DR1 datasets
• Mass profiles and galaxy orbits in nearby galaxy clusters from the analysis of the projected phase-space
• The zCOSMOS 10k-sample: the role of galaxy stellar mass in the colour-density relation up to z=1
• The star formation activity in cosmic voids
• Three-Point Correlation Functions of SDSS Galaxies: Luminosity and Color Dependence in Redshift and Projected Space
• Galaxy and Mass Assembly (GAMA): Projected Galaxy Clustering
• CMB Anisotropy of the Poincare Dodecahedron
• The 2dF Galaxy Redshift Survey: Hierarchical galaxy clustering
• Active Galactic Nucleus Pairs from the Sloan Digital Sky Survey. II. Evidence for Tidally Enhanced Star Formation and Black Hole Accretion
• The star formation history of galaxies: the role of galaxy mass, morphology and environment
• From galactic nuclei to the halo outskirts: tracing supermassive black holes across cosmic history and environments
• The clustering of radio galaxies at z~0.55 from the 2SLAQ LRG survey
• Catalog of Visually Classified Galaxies in the Local ($z\sim 0.01$) Universe
• The GALEX-SDSS NUV & FUV Flux Density and Local Star-Formation Rate
• Galaxy clustering from COMBO-17: The halo occupation distribution at <z>=0.6
• Bayesian Analysis of the Chaplygin Gas and Cosmological Constant Models using the SNe Ia Data
• Signatures of the Primordial Universe from Its Emptiness: Measurement of Baryon Acoustic Oscillations from Minima of the Density Field
• Precise photometric redshifts with a narrow-band filter set: The PAU Survey at the William Herschel Telescope
• Shapes of clusters and groups of galaxies: Comparison of model predictions with observations
• ALFALFA HI Data Stacking III. Comparison of environmental trends in HI gas mass fraction and specific star formation rate
• PRIMUS: Galaxy Clustering as a Function of Luminosity and Color at 0.2<z<1
• The Millennium Galaxy Catalogue: Exploring the Color-Concentration Bimodality via Bulge-Disc Decomposition
• Halo model description of the non-linear dark matter power spectrum at $k\gg 1$ Mpc${}^{-1}$
• The Build-up of the Red Sequence in the galaxy cluster MS1054-0321 at z=0.831
• The Impact of the Fiducial Cosmology Assumption on BAO Cosmological Parameter Inference
• Galaxy Groups in the 2dFGRS: the number density of groups
• Evolution of Star Forming and Active Galaxies in Nearby Clusters
• Eridanus - A Supergroup in the Local Universe?
• Do WMAP data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
• Absence of self-averaging and of homogeneity in the large scale galaxy distribution
• Quantifying Cosmic Superstructures
• The 6dF Galaxy Survey: Fundamental Plane Data
• Evolution of galaxy size--stellar mass relation from the Kilo Degree Survey
• Towards a physical picture of star-formation quenching: the photometric properties of recently-quenched galaxies in the Sloan Digital Sky Survey
• Calibration errors unleashed: effects on cosmological parameters and requirements for large-scale structure surveys
• Filaments in observed and mock galaxy catalogues
• The Observed Growth of Massive Galaxy Clusters III: Testing General Relativity on Cosmological Scales
• Mining Weak Lensing Surveys
• The Origin of Faint Tidal Features Around Galaxies in the RESOLVE Survey
• The angular power spectrum of NVSS radio galaxies
• Three-Point Correlation Functions of SDSS Galaxies: Constraining Galaxy-Mass Bias
• The 2dF Galaxy Redshift Survey: The clustering of galaxy groups
• On the luminosity function of galaxies in groups in the Sloan Digital Sky Survey
• The Zurich Environmental Study (ZENS) of Galaxies in Groups along the Cosmic Web. I. Which Environment Affects Galaxy Evolution?
• The Galaxy Angular Correlation Functions and Power Spectrum from the Two Micron All Sky Survey
• On the universality of void density profiles
• On the Luminosity Dependence of the Galaxy Pairwise Velocity Dispersion
• Testing coupled dark energy with next-generation large-scale observations
• The 2dF Galaxy Redshift Survey: Clustering properties of radio galaxies
• The galaxy power spectrum: precision cosmology from large scale structure?
• The evolution of the luminosity functions in the FORS Deep Field from low to high redshift: II. The red bands
• A Study of Catalogued Nearby Galaxy Clusters in the SDSS-DR4: I. Cluster Global Properties
• Superclusters of galaxies from the 2dF redshift survey. II. Comparison with simulations
• Kinetic k-essence ghost dark energy model
• The baryonic mass function of galaxies
• Optimal Extraction of Fibre Optic Spectroscopy
• The clustering of SDSS galaxy groups: mass and color dependence
• The Sloan Digital Sky Survey Peculiar Velocity Catalogue
• Two New Catalogues of Superclusters of Abell/ACO Galaxy Clusters out to redshift 0.15
• On the realistic validation of photometric redshifts, or why Teddy will never be Happy
• Optical Substructure and BCG Offsets of Sunyaev-Zel'dovich and X-ray Selected Galaxy Clusters
• Multi-Object Spectroscopy Field Configuration by Simulated Annealing
• Redshift inference from the combination of galaxy colors and clustering in a hierarchical Bayesian model
• RCSED - A Value-Added Reference Catalog of Spectral Energy Distributions of 800,299 Galaxies in 11 Ultraviolet, Optical, and Near-Infrared Bands: Morphologies, Colors, Ionized Gas and Stellar Populations Properties
• Aperture-free star formation rate of SDSS star-forming galaxies
• The importance of the local density in shaping the galaxy stellar mass functions
• Searching for rotating galaxy clusters in SDSS and 2dFGRS
• Studying galaxy troughs and ridges using Weak Gravitational Lensing with the Kilo-Degree Survey
• Inhomogeneities in the universe
• Constraining evolution in the Halo Model using galaxy redshift surveys
• The Satellite Luminosity Functions of Galaxies in SDSS
• Evidence for HI replenishment in massive galaxies through gas accretion from the cosmic web
• Substructure in the cold front cluster Abell 3667
• The distribution of AGN in a large sample of galaxy clusters
• Automated detection of filaments in the large scale structure of the universe
• All-Sky Analysis of the General Relativistic Galaxy Power Spectrum
• The matter distribution in the local Universe as derived from galaxy groups in SDSS DR12 and 2MRS
• Quasar and galaxy classification in Gaia Data Release 2
• The intrinsic bispectrum of the Cosmic Microwave Background [PhD thesis]
• The clustering of galaxies as a function of their photometrically-estimated atomic gas content
• The Virial Mass Function of Nearby SDSS Galaxy Clusters
• Characterising filaments in the SDSS volume from the galaxy distribution
• The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from DR12 galaxy clustering -- towards an accurate model
• On the distribution of stellar masses in gamma-ray burst host galaxies
• First Results from a Photometric Survey of Strong Gravitational Lens Environments
• The Projected Dark and Baryonic Ellipsoidal Structure of 20 CLASH Galaxy Clusters
• Limits on deviations from the inverse-square law on megaparsec scales
• A Pilot Survey for KX QSOs in the UKIDSS Ultra Deep Survey Field
• Scientific Visualization in Astronomy: Towards the Petascale Astronomy Era
• Numerical resolution limits on subhalo abundance matching
• Archetypal analysis of galaxy spectra
• An ASKAP search for a radio counterpart to the first high-significance neutron star-black hole merger LIGO/Virgo S190814bv
• Spatial distribution of galactic halos and their merger histories
• GalaxyCount: a JAVA calculator of galaxy counts and variances in multiband wide-field surveys to 28 AB mag
• Extending the infrared radio correlation
• The last stand before MAP: cosmological parameters from lensing, CMB and galaxy clustering
• First results of the XI Groups Project: Studying an unbiased sample of galaxy groups
• The Weak Clustering of Gas-Rich Galaxies
• Reliability of the detection of the Baryon Acoustic Peak
• The Canada-France deep fields survey-II: Lyman-break galaxies and galaxy clustering at z~3
• The 2dF Galaxy Redshift Survey: constraints on cosmic star-formation history from the cosmic spectrum
• The Herschel-ATLAS Data Release 2, Paper I. Submillimeter and Far-infrared Images of the South and North Galactic Poles: The Largest Herschel Survey of the Extragalactic Sky
• Joint analysis of anisotropic power spectrum, bispectrum and trispectrum: application to N-body simulations
• The WiggleZ Dark Energy Survey: measuring the cosmic growth rate with the two-point galaxy correlation function
• Broadband, radio spectro-polarimetric study of 100 radiative-mode and jet-mode AGN
• Galaxy And Mass Assembly (GAMA): impact of the group environment on galaxy star formation
• Spin flips I: Evolution of the angular momentum orientation of Milky Way-mass dark matter haloes
• Modelling galaxy clustering: Is new physics needed in galaxy formation models?
• The DEEP2 Galaxy Redshift Survey: Spectral classification of galaxies at z~1
• The Sloan Digital Sky Survey: The Cosmic Spectrum and Star-Formation History
• The Aemulus Project V: Cosmological constraint from small-scale clustering of BOSS galaxies
• Mass-to-Light Ratios of 2dF Galaxies
• The kinematics and spatial distribution of stellar populations in E+A galaxies
• The SDSS u-band Galaxy Survey: Luminosity functions and evolution
• Central stellar populations of early-type galaxies in low-density environments
• A Redshift Survey of Nearby Galaxy Groups: the Shape of the Mass Density Profile
• The UNAM-KIAS Catalog of Isolated Galaxies
• Luminous superclusters: remnants from inflation
• The evolution of galaxy cluster X-ray scaling relations
• The extragalactic radio-source population at 95 GHz
• The Monopole Moment of the Three-Point Correlation Function of the 2-degree Field Galaxy Redshift Survey
• The large-scale environment of low surface brightness galaxies
• Modeling the three-point correlation function
• SHELS: A Complete Galaxy Redshift Survey with R$\le$20.6
• Constraining the Star Formation Histories in Dark Matter Halos: I. Central Galaxies
• The Growth of Intracluster Light in XCS-HSC Galaxy Clusters from $0.1<z<0.5$
• Discovery of 5000 Active Galactic Nuclei behind the Magellanic Clouds
• Galaxy interactions II: High density environments
• A Spectro-photometric Search for Galaxy Clusters in SDSS
• Substructure Analysis of Selected Low Richness 2dFGRS Clusters of Galaxies
• Galaxy And Mass Assembly (GAMA): The Life and Times of L* Galaxies
• The SAMI Galaxy Survey: Observing the environmental quenching of star formation in GAMA groups
• The Local Hole in the Galaxy Distribution: New Optical Evidence
• The Size of the Longest Filaments in the Universe
• ZENS IV. Similar Morphological Changes associated with Mass- and Environment-Quenching, and the Relative importance of Bulge Growth versus the Fading of Disks
• hCOSMOS: a dense spectroscopic survey of $r⩽21.3$ galaxies in the COSMOS field
• The Accretion of Gas onto Galaxies as Traced by their Satellites
• The WiggleZ Dark Energy Survey: Final Data Release and the Metallicity of UV-Luminous Galaxies
• The 2dF Galaxy Redshift Survey: The population of nearby radio galaxies at the 1 mJy level
• The Two-Point Correlation of Galaxy Groups: Probing the Clustering of Dark Matter Haloes
• Luminosity function of galaxies in groups in the SDSS DR7: the dependence on mass, environment and galaxy type
• The PyCASSO database: Spatially resolved stellar population properties for CALIFA galaxies
• Satellite Kinematics I: A New Method to Constrain the Halo Mass-Luminosity Relation of Central Galaxies
• A Cosmic Coincidence: The Power-Law Galaxy Correlation Function
• Clustering of Luminous Red Galaxies III: Detection of the Baryon Acoustic Peak in the 3-point Correlation Function
• The Heraklion Extragalactic Catalogue (HECATE): a value-added galaxy catalogue for multi-messenger astrophysics
• Improving Galaxy Clustering Measurements with Deep Learning: analysis of the DECaLS DR7 data
• Exploring the Morphology of RAVE Stellar Spectra
• How robust are the constraints on cosmology and galaxy evolution from the lens-redshift test?
• The Observed Growth of Massive Galaxy Clusters IV: Robust Constraints on Neutrino Properties
• The Structure of the Circumgalactic Medium of Galaxies: Cool Accretion Inflow Around NGC 1097
• Bivariate Galaxy Luminosity Functions in the Sloan Digital Sky Survey
• Growth factor parametrization in curved space
• The GEEC2 spectroscopic survey of Galaxy Groups at $0.8<z<1$
• Transient cosmic acceleration from interacting fluids
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). A Support Vector Machine classification of galaxies, stars and AGNs
• Galaxy And Mass Assembly (GAMA): the red fraction and radial distribution of satellite galaxies
• Detecting clusters of galaxies and active galactic nuclei in an eROSITA all-sky survey digital twin
• Galaxy groups in the 2dF redshift survey: Effects of Environment on Star Formation
• Enhancing stellar spectroscopy with extreme adaptive optics and photonics
• SPT-GMOS: A Gemini/GMOS-South Spectroscopic Survey of Galaxy Clusters in the SPT-SZ Survey
• Intrinsic Alignment of Cluster Galaxies: the Redshift Evolution
• Cosmological parameter estimation and Bayesian model comparison using VSA data
• Full-sky maps for gravitational lensing of the CMB
• The dependence of halo bias on age, concentration and spin
• Structure and dynamics of the Shapley Supercluster
• The Australia Telescope Large Area Survey: Spectroscopic Catalogue and Radio Luminosity Functions
• The GOGREEN and GCLASS Surveys: First Data Release
• Dark Energy Survey Year 1 results: The relationship between mass and light around cosmic voids
• A Brighter Past: Galaxy Luminosity Function At High Redshifts
• Superclusters of galaxies in the 2dF redshift survey. III. The properties of galaxies in superclusters
• Galaxy Orbits for Galaxy Clusters in Sloan Digital Sky Survey and 2dF Galaxy Redshift Survey
• Triaxial haloes, intrinsic alignments and the dark matter power spectrum
• Activity in galactic nuclei of cluster and field galaxies in the local universe
• Galaxy Clustering Topology in the Sloan Digital Sky Survey Main Galaxy Sample: a Test for Galaxy Formation Models
• 2023 Astrophotonics Roadmap: pathways to realizing multi-functional integrated astrophotonic instruments
• Galaxy groups in the 2dF redshift survey: Galaxy Spectral Type Segregation in Groups
• Future virialized structures: An analysis of superstructures in SDSS-DR7
• Accelerating Universe in Hybrid and Logarithmic Teleparallel Gravity
• Where do "red and dead" early-type void galaxies come from?
• Like a spider in its web: a study of the Large Scale Structure around the Coma cluster
• The Large Area Radio Galaxy Evolution Spectroscopic Survey (LARGESS): Survey design, data catalogue and GAMA/WiggleZ spectroscopy
• WFMOS - Sounding the Dark Cosmos
• Mining the gap: evolution of the magnitude gap in X-ray galaxy groups from the 3 square degree XMM coverage of CFHTLS
• GMRT observation of neutral atomic hydrogen gas in the COSMOS field at $z\sim 0.37$
• Improving Photometric Redshift Estimation using GPz: size information, post processing and improved photometry
• Weak Lensing and CMB: Parameter forecasts including a running spectral index
• The Gravitational Lens -- Galaxy Group Connection. II. Groups Associated with B2319+051 and B1600+434
• Weak Lensing Discovery and Tomography of a Cluster at z=0.68
• Environmental Enhancement of Loose Groups around Rich Clusters of Galaxies
• Mitigating contamination in LSS surveys: a comparison of methods
• What produces the far-infrared/submm emission in the most luminous QSOs?
• The Properties of Spiral Galaxies: Confronting Hierarchical Galaxy Formation Models with Observations
• The Young Supernova Experiment Data Release 1 (YSE DR1): Light Curves and Photometric Classification of 1975 Supernovae
• Substructure and the halo model of large-scale structure
• Baryon fractions in clusters of galaxies: evidence against a preheating model for entropy generation
• The Galaxy Optical Luminosity Function from the AGN and Galaxy Evolution Survey (AGES)
• Angular correlation function of 1.5 million LRGs: clustering evolution and a search for BAO
• Environmental Effects on Real-Space and Redshift-Space Galaxy Clustering
• The KPNO/Deeprange Distant Cluster Survey: I. The Catalog & the Space Density of Intermediate Redshift Clusters
• Contiguous redshift parameterizations of the growth index
• Building a control sample for galaxy pairs
• The strong correlation between post-starburst fraction and environment
• What is the best way to measure baryonic acoustic oscillations?
• Cosmic Physics: The High Energy Frontier
• The clustering and evolution of H-alpha emitters at z~1 from HiZELS
• The 2dF QSO Redshift Survey - X. Lensing of Background QSOs by Galaxy Groups
• Structural properties of discs and bulges of early-type galaxies
• A modified star formation law as a solution to open problems in galaxy evolution
• High Metallicity, Photoionised Gas in Intergalactic Large-Scale Filaments
• The clustering properties of radio-selected AGN and star-forming galaxies up to redshifts z~3
• Galaxy and Mass Assembly (GAMA): The evolution of bias in the radio source population to z ~ 1.5
• Cold Dark Matter's Small Scale Crisis Grows Up
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: combining correlated Gaussian posterior distributions
• PRIMUS: Enhanced Specific Star Formation Rates In Close Galaxy Pairs
• The growth of linear perturbations in the DGP model
• The Millennium Galaxy Catalogue: On the natural sub-division of galaxies
• Structures in the Great Attractor Region
• Characterization of hexabundles: Initial results
• RESOLVE Survey Photometry and Volume-limited Calibration of the Photometric Gas Fractions Technique
• The XMM-SERVS survey: XMM-Newton point-source catalogs for the W-CDF-S and ELAIS-S1 fields
• Power spectrum of the SDSS luminous red galaxies: constraints on cosmological parameters
• Entropic cosmology in a dissipative universe
• The spectral-type/luminosity and the spectral type/satellite-density relations in the 2dFGRS
• Line strengths of early-type galaxies
• The SAGA Survey. III. A Census of 101 Satellite Systems around Milky Way-mass Galaxies
• The Luminosity, Colour and Morphology dependence of galaxy filaments in the Sloan Digital Sky Survey Data Release Four
• The Zurich Environmental Study of Galaxies in Groups along the Cosmic Web. III. Galaxy Photometric Measurements and the Spatially-Resolved Color Properties of Early- and Late-Type Satellites in Diverse Environments
• A large H$\alpha$ survey of star formation in relaxed and merging galaxy cluster environments at $z\sim 0.15-0.3$
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Angular clustering tomography and its cosmological implications
• Satellite Galaxy Number Density Profiles in the Sloan Digital Sky Survey
• Large scale structure in the HI Parkes All-Sky Survey: Filling the Voids with HI galaxies?
• The RESOLVE Survey Atomic Gas Census and Environmental Influences on Galaxy Gas Reservoirs
• Evidence against a supervoid causing the CMB Cold Spot
• Creating mock catalogues of stellar haloes from cosmological simulations
• Redshift inference from the combination of galaxy colors and clustering in a hierarchical Bayesian model $-$ Application to realistic $N$-body simulations
• AKARI Near-Infrared Spectroscopy of Luminous Infrared Galaxies
• Clusters and groups of galaxies in the 2dF galaxy redshift survey
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). The decline of cosmic star formation: quenching, mass, and environment connections
• Toward understanding rich superclusters
• Clues on void evolution III: Structure and dynamics in void shells
• Constraints on growth index parameters from current and future observations
• The fifth data release of the Kilo Degree Survey: Multi-epoch optical/NIR imaging covering wide and legacy-calibration fields
• Extracting Star Formation Histories from Medium-resolution Galaxy Spectra
• The [OII]/Halpha ratio of emission line galaxies in the 2dF redshift survey
• Exact relativistic beta decay endpoint spectrum
• Missing baryons traced by the galaxy luminosity density in the large-scale WHIM filaments
• Shapley Supercluster Survey (ShaSS): Galaxy Evolution from Filaments to Cluster Cores
• The structure of cosmic voids in a LCDM Universe
• Phantom-Like Behavior in $f(R)$-Gravity
• Probing the cosmic web: inter-cluster filament detection using gravitational lensing
• PINGS: the PPAK IFS Nearby Galaxies Survey
• Clustering of photometric luminous red galaxies I : Growth of Structure and Baryon Acoustic Feature
• Exploring galaxy colour in different environments of the cosmic web with SDSS
• Morphological Properties of Superclusters of Galaxies
• GaBoDS: The Garching-Bonn Deep Survey: VII. Probing galaxy bias using weak gravitational lensing
• Testing Isotropy in the Local Universe
• A New Algorithm for the Detection of Inter-cluster Galaxy Filaments using Galaxy Orientation Alignments
• Integrated photonic building blocks for next-generation astronomical instrumentation I: the multimode waveguide
• The 2dF-SDSS LRG and QSO Survey: The Star Formation Histories of Luminous Red Galaxies
• An all-sky optical catalogue of radio / X-ray sources
• A 325-MHz GMRT survey of the Herschel-ATLAS/GAMA fields
• NIR Luminosity Function of Galaxies in Close Major-Merger Pairs and Mass Dependence of Merger Rate
• Radio source feedback in galaxy evolution
• Observational constraints on particle production during inflation
• Empirical Photometric Redshifts of Luminous Red Galaxies and Clusters in SDSS
• The nature of assembly bias - III. Observational properties
• Large Scale Structure of the Universe
• From Dark Matter to Galaxies with Convolutional Networks
• Differences in the AGN Populations of Groups and Clusters: Clues to AGN Evolution
• Nature versus Nurture: The curved spine of the galaxy cluster X-ray luminosity -- temperature relation
• A search for distant radio galaxies from SUMSS and NVSS: I. Sample definition, radio and K-band imaging
• The Integrated Sachs-Wolfe Effect in Interacting Dark Energy Models
• Spatially Resolved Spectroscopy of the E+A Galaxies in the z=0.32 Cluster AC114
• The DEEP Groth Strip Survey. I. The Sample
• Internal kinematics of groups of galaxies in the Sloan Digital Sky Survey data release 7
• Fractal Dimensions of a Weakly Clustered Distribution and the Scale of Homogeneity
• Probing the Radio Loud/Quiet AGN dichotomy with quasar clustering
• The Color Bimodality in Galaxy Clusters since z = 0.9
• More galaxies in the Local Volume imaged in H-alpha
• FLASH redshift survey - I. Observations and Catalogue
• Galaxy groups in the 2dF galaxy redshift survey: Luminosity and Mass Statistics
• A UV to Mid-IR Study of AGN Selection
• Galaxy And Mass Assembly (GAMA): The 325 MHz Radio Luminosity Function of AGN and Star Forming Galaxies
• Massive Dark Matter Halos around Bright Isolated Galaxies in the 2dFGRS
• The build-up of pseudobulges in a hierarchical universe
• Do model emission line galaxies live in filaments at z~1?
• Ultraluminous Infrared Galaxies in the AKARI All Sky Survey
• Dynamical mass inference of galaxy clusters with neural flows
• Wide-angle tail galaxies in ATLAS
• The Canada-France Deep Fields III: Photometric Redshift Distribution to I(AB) ~ 24
• ROXA: a new multi-frequency selected large sample of blazars with SDSS and 2dF optical spectroscopy
• A comparison of cosmological filaments catalogues
• Non-linear Galaxy Power Spectrum and Cosmological Parameters
• Can Planck-scale physics be seen in the cosmic microwave background ?
• Brighter galaxy bias: underestimating the velocity dispersions of galaxy clusters
• The Environment of Active Galaxies in the SDSS-DR4
• Extragalactic Large-Scale Structures behind the Southern Milky Way. IV. Redshifts Obtained with MEFOS
• Cosmic Voids and Galaxy Bias in the Halo Occupation Framework
• Observational Constraints on Accelerating Brane Cosmology with Exchange between the Bulk and Brane
• Source subtraction for the extended Very Small Array and 33-GHz source count estimates
• Analysing Large Scale Structure: I. Weighted Scaling Indices and Constrained Randomisation
• The dark haloes of early-type galaxies in low-density environments: XMM-Newton and Chandra observations of NGC 57, NGC 7796 and IC 1531
• Emission-lines calibrations of the Star Formation Rate from the Sloan Digital Sky Survey
• The SAMI Galaxy Survey: flipping of the spin-filament alignment correlates most strongly with growth of the bulge
• Distribution of satellite galaxies in high redshift groups
• Observed trend in the star formation history and the dark matter fraction of galaxies at redshift $z\approx 0.8$
• Cosmic filaments in galaxy cluster outskirts: quantifying finding filaments in redshift space
• The POlarised GLEAM Survey (POGS) I: First Results from a Low-Frequency Radio Linear Polarisation Survey of the Southern Sky
• The XMM-Newton/2dF survey I: X-ray properties of normal galaxies
• The spatial clustering of mid-IR selected star forming galaxies at z ~ 1 in the GOODS fields
• Observational detection of correlation between galaxy spins and initial conditions
• Comparing galaxy populations in compact and loose groups of galaxies
• The Zurich Environmental Study (ZENS) of Galaxies in Groups along the Cosmic Web. II. Galaxy Structural Measurements and the Concentration of Morphologically Classified Satellites in Diverse Environments
• The boundary of cosmic filaments
• The environment of HI-bearing ultra diffuse galaxies in the ALFALFA survey
• Using head-tail galaxies to constrain the intracluster magnetic field: an in-depth study of PKS J0334-3900
• Observations and properties of candidate high frequency GPS radio sources in the AT20G survey
• The High-Mass End of the Red Sequence at z~0.55 from SDSS-III/BOSS: completeness, bimodality and luminosity function
• Galaxy And Mass Assembly (GAMA): The environments of high- and low- excitation radio galaxies
• The XMM-Newton/2dF survey - II. The nature of X-ray faint optically bright X-ray sources
• Testing Cold Dark Matter with the hierarchical buildup of stellar light
• The core of the massive cluster merger MACS J0417.5-1154 as seen by VLT/MUSE
• Satellite number density profiles of primary galaxies in the 2dFGRS
• Confronting dark energy models mimicking $\Lambda$CDM epoch with observational constraints: future cosmological perturbations decay or future Rip?
• The pairwise velocity dispersion of galaxies: luminosity dependence and a new test of galaxy formation models
• The Oxford-Dartmouth Thirty Degree Survey I: Observations and Calibration of a Wide-Field Multi-Band Survey
• The SuperCOSMOS all-sky galaxy catalogue
• A blind HI survey in the Ursa Major region
• Testing the Accuracy of Halo Occupation Distribution Modelling using Hydrodynamic Simulations
• Easylife: the data reduction and survey handling system for VIPERS
• New southern blue compact dwarf galaxies in the 2dF Galaxy Redshift Survey
• Late Forming Dark Matter in Theories of Neutrino Dark Energy
• The generality of inflation in closed cosmological models with some quintessence potentials
• Galaxy groups in the 2dF galaxy redshift survey: Large Scale Structure with Groups
• The amazing diversity in the hot gas content of an X-ray unbiased massive galaxy clusters sample
• The growth factor of matter perturbations in an f(R) gravity
• The 1000 Brightest HIPASS Galaxies: Newly Cataloged Galaxies
• Finding Dwarf Galaxies From Their Tidal Imprints
• No Periodicities in 2dF Redshift Survey Data
• The Angular Power Spectra of Photometric SDSS LRGs
• Spectrophotometric properties of galaxies at intermediate redshifts (z ~ 0.2--1.0) II. The Luminosity -- Metallicity relation
• Spectrophotometric properties of galaxies at intermediate redshifts (z ~ 0.2--1.0) I. Sample description, photometric properties and spectral measurements
• Identification of filamentary structures in the environment of superclusters of galaxies in the Local Universe
• Mapping the real space distributions of galaxies in SDSS DR7: I. Two Point Correlation Functions
• The importance of magnification effects in galaxy-galaxy lensing
• Finding the brightest cosmic beacons in the Southern Hemisphere
• Las Campanas Loose Groups in the Supercluster-Void Network
• Rotation of Cosmic Voids and Void-Spin Statistics
• Using Multipoles of the Correlation Function to Measure H(z), D_A(z), and β(z) from Sloan Digital Sky Survey Luminous Red Galaxies
• The correlation function of galaxy clusters and detection of baryon acoustic oscillations
• Towards Accurate Modelling of Galaxy Clustering on Small Scales: Testing the Standard $\Lambda \mathrm{CDM}$ + Halo Model
• Mysterious Coherence in Several-Megaparsec Scales Between Galaxy Rotation and Neighbor Motion
• Quintessence from Shape Moduli
• Discovery of a Solitaire Dwarf Galaxy in the APPLES Survey
• The WSRT ZoA Perseus-Pisces Filament wide-field HI imaging survey I. HI catalogue and atlas
• Evidence for Morphology and Luminosity Transformation of Galaxies at High Redshifts
• Strong lensing statistics in large, z~<0.2 surveys: bias in the lens galaxy population
• Galaxy 2-Point Covariance Matrix Estimation for Next Generation Surveys
• SDSS-IV MaNGA: Uncovering the Angular Momentum Content of Central and Satellite Early-type Galaxies
• Void Galaxies Follow a Distinct Evolutionary Path in the Environmental COntext Catalog
• Optical Properties of Host Galaxies of Extragalactic Nuclear Water Masers
• Statistical analysis of galaxy surveys - III: The non-linear clustering of red and blue galaxies in the 2dFGRS
• The effect of cosmic web filaments on galaxy evolution
• Spatial and luminosity distributions of galactic satellites
• Large-scale fluctuations in the distribution of galaxies from the Two Degree Field Galaxy Redshift Survey
• Cosmology in General Massive Gravity Theories
• An Unbiassed Census of Active Galactic Nuclei in the Two Micron All Sky Survey
• An all-sky Atlas of Radio/X-ray Associations
• Shape Alignments of Satellite Galaxies
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• Effects of large-scale environment on the assembly history of central galaxies
• X-ray spectral studies of TeV gamma-ray emitting blazars
• Mass, Light and Colour of the Cosmic Web in the Supercluster SCL2243-0935 (z=0.447)
• Abundances, masses, and weak-lensing mass profiles of galaxy clusters as a function of richness and luminosity in LambdaCDM cosmologies
• Cosmic filaments delay quenching inside clusters
• Galaxy And Mass Assembly (GAMA): The Consistency of GAMA and WISE Derived Mass-to-Light Ratios
• Galaxy clustering and projected density profiles as traced by satellites in photometric surveys: Methodology and luminosity dependence
• ETHOS - an Effective Theory of Structure Formation: detecting dark matter interactions through the Lyman-$\alpha$ forest
• Galaxy distribution and extreme value statistics
• Backreaction in Cosmology
• Mapping the Universe: The 2010 Russell Lecture
• The RASS--6dFGS catalogue: a sample of X-ray selected AGN from the 6dF Galaxy Survey
• Dark Matter
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): ${\Omega }_{{\mathrm{m}}_0}$ from the galaxy clustering ratio measured at $z\sim 1$
• Shear-Selected Clusters From the Deep Lens Survey III: Masses from Weak Lensing
• The Influence of Environment on the Circumgalactic Medium
• Aperture effects on the oxygen abundance determinations from CALIFA data
• The abundance of compact quiescent galaxies since z ~ 0.6
• Statefinder diagnosis for holographic dark energy in the DGP braneworld
• 2dFGRS and SDSS Galaxy Group Density Profiles
• Evolution of the Major Merger Galaxy Pair Fraction at z < 1
• Revealing the cosmic web dependent halo bias
• Testing homogeneity in the Sloan Digital Sky Survey Data Release Twelve with Shannon entropy
• An observational proxy of halo assembly time and its correlation with galaxy properties
• The dependence of galaxy clustering on tidal environment in the Sloan Digital Sky Survey
• Galaxy and Mass Assembly (GAMA): Accurate number densities & environments of massive ultracompact galaxies at 0.02 < z < 0.3
• Galaxy And Mass Assembly: Automatic Morphological Classification of Galaxies Using Statistical Learning
• Properties and environment of Radio Emitting Galaxies in the VLA-zCOSMOS survey
• WMAP constraints on Cardassian model
• ProFuse: Physical Multi-Band Structural Decomposition of Galaxies and the Mass-Size-Age Plane
• Further constraining galaxy evolution models through the Size Function of SDSS Early-type galaxies
• The spectroscopic follow-up of the QUBRICS bright quasar survey
• Modeling Galaxy-Galaxy Weak Lensing with SDSS Groups
• Alignments of Group Galaxies with Neighboring Groups
• Large Scale Structure in Absorption: Gas within and around Galaxy Voids
• Stellar mass-metallicity relation throughout the large-scale structure of the Universe: CAVITY mother sample
• The optical morphology of A3667 re-examined
• Properties of the KISS Green Pea Galaxies
• A Search for Gravitationally Lensed Quasars and Quasar Pairs in Pan-STARRS1: Spectroscopy and Sources of Shear in the Diamond 2M1134$-$2103
• The SDSS-IV eBOSS: emission line galaxy catalogues at z=0.8 and study of systematic errors in the angular clustering
• J-PLUS: 2-D analysis of the stellar population in NGC 5473 and NGC 5485
• Mitigating the Impact of the DESI Fiber Assignment on Galaxy Clustering
• Luminous Red Galaxy Clustering at z~0.7 - First Results using AAOmega
• A Divided Universe: Red and Blue Galaxies and their Preferred Environments
• Where are the z=4 Lyman Break Galaxies? Results from Conditional Luminosity Function Models of Luminosity-dependent Correlation Functions
• The SAMI Galaxy Survey: a new method to estimate molecular gas surface densities from star formation rates
• Redshift-Space Enhancement of Line-of-Sight Baryon Acoustic Oscillations in the SDSS Main-Galaxy Sample
• Large-scale growth evolution in the Szekeres inhomogeneous cosmological models with comparison to growth data
• Ultraluminous and Hyperluminous Infrared Galaxies in the SDSS, 2dFGRS and 6dFGS
• Two 100 Mpc-scale structures in the 3-D distribution of radio galaxies and their implications
• The influence of halo assembly on galaxies and galaxy groups
• Brightest group galaxies and the large-scale environment
• XMP gas-rich dwarfs in nearby voids: results of BTA spectroscopy
• Testing modified gravity models with recent cosmological observations
• Galaxy and Mass Assembly (GAMA): Colour and luminosity dependent clustering from calibrated photometric redshifts
• Eddington's Demon: Inferring Galaxy Mass Functions and other Distributions from Uncertain Data
• A search for distant radio galaxies from SUMSS and NVSS: II. Optical Spectroscopy
• Star formation and the environment of nearby field galaxies
• Massive elliptical galaxies : From cores to haloes
• Structure in the 3D Galaxy Distribution: I. Methods and Example Results
• Sky Surveys
• The 2MASS redshift survey galaxy group catalogue derived from a graph-theory based friends-of-friends algorithm
• Two-Dimensional Topology of the 2dF Galaxy Redshift Survey
• Forecast of Neutrino Cosmology from the CSST Photometric Galaxy Clustering and Cosmic Shear Surveys
• Effects of superstructure environment on galaxy groups
• The Second Data Release of the Beijing-Arizona Sky Survey
• Mapping the large scale structure around a z=1.46 galaxy cluster in 3-D using two adjacent narrow-band filters
• Origin of the Cosmic Network: Nature vs Nurture
• Holographic Dark Energy from a Modified GBIG Scenario
• Assessing the photometric redshift precision of the S-PLUS survey: the Stripe-82 as a test-case
• Constraints on Resonant Particle Production during Inflation from the Matter and CMB Power Spectra
• Abell 1201: The anatomy of a cold front cluster from combined optical and X-ray data
• Deprojecting Densities from Angular Cross-Correlations
• Wide-Field Optical Spectroscopy of Abell 133: A Search for Filaments Reported in X-ray Observations
• The importance of interloper removal in galaxy clusters: saving more objects for the Jeans analysis
• The Ultraviolet Galaxy Luminosity Function from GALEX data: Color Dependent Evolution at Low Redshift
• Persistent fluctuations in the distribution of galaxies from the Two degree Field Galaxy Redshift Survey
• A TESS Dress Rehearsal: Planetary Candidates and Variables from K2 Campaign 17
• The spatial distribution of neutral hydrogen as traced by low HI mass galaxies
• Exploring the Sharma-Mittal HDE models with different diagnostic tools
• Environmental dependence of the galaxy stellar mass function in the Dark Energy Survey Science Verification Data
• The environments and clustering properties of 2dFGRS-selected starburst galaxies
• Multiplicative errors in the galaxy power spectrum: self-calibration of unknown photometric systematics for precision cosmology
• Large Scale Magnetic Fields: Galaxy Two-Point correlation function
• The MillenniumTNG Project: The large-scale clustering of galaxies
• The WiggleZ Dark Energy Survey: small-scale clustering of Lyman Break Galaxies at z < 1
• Integrated spectra extraction based on signal-to-noise optimization using Integral Field Spectroscopy
• DES Science Portal: Computing Photometric Redshifts
• Do the stellar populations of the brightest two group galaxies depend on the magnitude gap?
• History of Hydrogen Reionization in the Cold Dark Matter Model
• Statistical analysis of probability density functions for photometric redshifts through the KiDS-ESO-DR3 galaxies
• A method for testing the cosmic homogeneity with Shannon entropy
• Statistical Analysis of Galaxy Surveys-IV: An objective way to quantify the impact of superstructures on galaxy clustering statistics
• Testing for a large local void by investigating the Near-Infrared Galaxy Luminosity Function
• Why are AGN found in High Mass Galaxies?
• SHELS: Optical Spectral Properties of WISE 22 μm-selected Galaxies
• A new search for distant radio galaxies in the southern hemisphere - I. Sample definition and radio properties
• XMM observes ClJ0152.7-1357: A massive galaxy cluster forming at merger crossroads at z=0.83
• The rise and fall of an extraordinary Ca-rich transient -- The discovery of ATLAS19dqr/SN 2019bkc
• Targeting supermassive black hole binaries and gravitational wave sources for the pulsar timing array
• The Fornax Cluster Spectroscopic Survey: A Sample of Confirmed Cluster Dwarfs
• Lensed arc statistics: comparison of Millennium-simulation galaxy clusters to Hubble Space Telescope observations of an X-ray selected sample
• Testing isotropy in the Universe using photometric and spectroscopic data from the SDSS
• Inter-cluster Filaments of Galaxies Programme: Pilot Study Survey and Results
• Galaxy Luminosities in 2PIGG groups
• The Stripe 82 1-2 GHz Very Large Array Snapshot Survey: Multiwavelength Counterparts
• Removing Imaging Systematics from Galaxy Clustering Measurements with Obiwan : Application to the SDSS-IV extended Baryon Oscillation Spectroscopic Survey Emission Line Galaxy Sample
• The effects of halo alignment and shape on the clustering of galaxies
• The Sloan Digital Sky Survey
• The detection of the imprint of filaments on cosmic microwave background lensing
• Weak-lensing calibration of a stellar mass-based mass proxy for redMaPPer and Voronoi Tessellation clusters in SDSS Stripe 82
• Photon-Axion mixing in an inhomogeneous universe
• Intergalactic filaments spin
• Non-linear general relativistic effects in the observed redshift
• ECO and RESOLVE: Galaxy Disk Growth in Environmental Context
• Ultra-luminous Infrared Galaxies in Sloan Digital Sky Survey Data Release 6
• Galaxy star formation in different environments
• CO-CAVITY pilot survey: Molecular gas and star formation in void galaxies
• Unveiling the atomic hydrogen-halo mass relation via spectral stacking
• Characterising the evolving $K$-band luminosity function using the UltraVISTA, CANDELS and HUDF surveys
• RESOLVE and ECO: The Halo Mass-Dependent Shape of Galaxy Stellar and Baryonic Mass Functions
• A Quick Look at the 3GHz Radio Sky. II. Hunting for DRAGNs in the VLA Sky Survey
• Canceling out intensity mapping foregrounds
• Large-scale density and velocity field reconstructions with neural networks
• Preprocessing, mass loss and mass segregation of galaxies in DM simulations
• Fast Radio Bursts counterparts in the scenario of supergiant pulses
• Large-scale analysis of the SDSS-III DR8 photometric luminous galaxies angular correlation function
• Studying Inter-Cluster Galaxy Filaments Through Stacking GMBCG Galaxy Cluster Pairs
• Spectroscopy of QUBRICS quasar candidates: 1672 new redshifts and a Golden Sample for the Sandage Test of the Redshift Drift
• SFR estimations from z=0 to z=0.9 -- A comparison of SFR calibrators for star-forming galaxies
• Exploring Galaxy Formation Models and Cosmologies with Galaxy Clustering
• The Westerbork Coma Survey: A blind, deep, high-resolution HI survey of the Coma cluster
• The environment and characteristics of low redshift galaxies detected by the Herschel-ATLAS
• The First Mid-IR View of the Star-forming Properties of Nearby Galaxy Groups
• Phenomenological Reconstruction of $f(T)$ Teleparallel Gravity
• XMP gas-rich dwarfs in Nearby Voids: results of SALT spectroscopy
• The unrelaxed dynamical structure of the galaxy cluster Abell 85
• Luminosity segregation in three clusters of galaxies (A119, 2443, 2218)
• Galaxy And Mass Assembly (GAMA): Bivariate functions of H$\alpha$ star forming galaxies
• Connected structure in the 2dFGRS
• The nature of the relative bias between galaxies of different spectral type in 2dFGRS
• Peculiar Velocities into the Next Generation: Cosmological Parameters From Large Surveys without Bias from Nonlinear Structure
• The Combined NVSS-FIRST Galaxies (CoNFIG) Sample - I. Sample Definition, Classification and Evolution
• Holographic kinetic k-essence model
• The diverse X-ray properties of four truly isolated elliptical galaxies: NGC 2954, NGC 6172, NGC 7052, and NGC 7785
• Modified GBIG Scenario as an Alternative for Dark Energy
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• Multi-frequency studies of galaxies and groups: I. Environmental effect on galaxy stellar mass and morphology
• Large Scale Structures in COSMOS2020: Evolution of Star Formation Activity in Different Environments at 0.4 < z < 4
• Fiber Assignment in Next-generation Wide-field Spectrographs
• The luminosity function of galaxies to $M_{BgVriz}\sim -14$ in $z\sim 0.3$ clusters
• MIGHTEE-HI: The relation between the HI gas in galaxies and the cosmic web
• The Large Peculiar Velocity of the cD Galaxy in Abell 3653
• The SAMI galaxy survey: Galaxy Interactions and Kinematic Anomalies in Abell 119
• Suppressed radio emission in supercluster galaxies: enhanced ram pressure in merging clusters?
• A deep i-selected multi-waveband galaxy catalogue in the COSMOS field
• Catalog of Radio Galaxies with z>0.3. I:Construction of the Sample
• The evolution of extragalactic radio sources
• A Robust Distance Measurement and Dark Energy Constraints from the Spherically-Averaged Correlation Function of Sloan Digital Sky Survey Luminous Red Galaxies
• On an Analytical Framework for Voids: Their abundances, density profiles and local mass functions
• The stellar mass - size relation for cluster galaxies at z=1 with high angular resolution from the Gemini/GeMS multi-conjugate adaptive optics system
• Lopsided Satellite Distributions around Isolated Host Galaxies
• Halo based reconstruction of the cosmic mass density field
• The 2dF Galaxy Redshift Survey: correlation with the ROSAT-ESO Flux Limited X-ray (REFLEX) galaxy cluster survey
• Galaxy and Mass Assembly (GAMA): merging galaxies and their properties
• Probing large scale filaments with HI and ${}^3$HeII
• Star Formation and AGN Feedback in the Local Universe: Combining LOFAR and MaNGA
• Crawling the Cosmic Network: Exploring the Morphology of Structure in the Galaxy Distribution
• Not a Copernican observer: biased peculiar velocity statistics in the local Universe
• Faint Companions of Isolated 2MIG Galaxies
• The Evolution and Environments of X-ray Emitting Active Galactic Nuclei in High-Redshift Large-Scale Structures
• Galaxy Rotation Coherent with the Motions of Neighbors: Discovery of Observational Evidence
• The Probabilistic Random Forest applied to the selection of quasar candidates in the QUBRICS Survey
• A detection of baryon acoustic oscillations from the distribution of galaxy clusters
• Low-Density Structures in the Local Universe. II. Nearby Cosmic Voids
• Simulating MOS science on the ELT: Ly$\alpha$ forest tomography
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Measuring nonlinear galaxy bias at z~0.8
• Evolution of the galaxy luminosity function in progenitors of fossil groups
• Evolution of hierarchical clustering in the CFHTLS-Wide since z~1
• Lower Mass Black Holes in the GOODS? Off-nuclear X-ray Sources
• Galaxy And Mass Assembly (GAMA): The Bright Void Galaxy Population in the Optical and Mid-IR
• Inhomogeneity-induced variance of cosmological parameters
• The Variation of the Galaxy Luminosity Function with Group Properties
• Correlating galaxy morphologies and spectra in the 2dFGRS
• Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model - I. Magnitude counts, redshift distribution, colour bimodality, and galaxy clustering
• An estimate of the electron density in filaments of galaxies at z~0.1
• Stellar Mass and color dependence of the three-point correlation function of galaxies in the local universe
• Euclid preparation. XLI. Galaxy power spectrum modelling in real space
• The peculiar velocities of satellites of external disk galaxies
• The neutral hydrogen distribution in large-scale haloes from 21-cm intensity maps
• A black box for dark sector physics: Predicting dark matter annihilation feedback with conditional GANs
• Large extra dimensions, the galaxy power spectrum and the end of inflation
• The evolution of the bi-modal colour distribution of galaxies in SDSS groups
• Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups
• Best values of parameters for interacting HDE with GO IR-cutoff in Brans-Dicke cosmology
• Photometric Objects around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. I. Methods
• Higher neutrino mass allowed if Cold Dark Matter and Dark Energy are coupled
• The stellar populations of early-type galaxies -- II. The effects of environment and mass
• Holographic dark energy with the sign-changeable interaction term
• On the connection between the metal-enriched intergalactic medium and galaxies: an OVI-galaxy cross-correlation study at $z<1$
• The Evolution of [OII] Emission from Cluster Galaxies
• VICS82: the VISTA-CFHT Stripe 82 near-infrared survey
• Projected Three-Point Correlation Functions and Galaxy Bias
• Host Galaxy Spectra and Consequences for SN Typing From The SDSS SN Survey
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Star formation history of passive galaxies
• The 3-D clustering of radio galaxies in the TONS survey
• Density preturbations in a finite scale factor singularity universe
• The HectoMAP Redshift Survey: First Data Release
• A search for the third lensed image in JVAS B1030+074
• Nonlinear Redshift-Space Distortions in the Harmonic-space Galaxy Power Spectrum
• The growth of matter perturbations in the f(T) gravity
• The XMM-Newton/2dF survey IV. The X-ray spectral properties of the hard sources
• The ALHAMBRA survey : $B-$band luminosity function of quiescent and star-forming galaxies at $0.2\le z<1$ by PDF analysis
• Compact Groups of Galaxies in Sloan Digital Sky Survey and LAMOST Spectral Survey: I. The Catalogs
• (DarkAI) Mapping the large-scale density field of dark matter using artificial intelligence
• The Global, Local and Cluster Galaxy Luminosity Function
• The power spectrum of galaxy clustering in the APM survey
• Extragalactic Water Masers, Geometric Estimation of H_o and Characterization of Dark Energy
• The cosmic web in Lyman-alpha emission
• The Evolution of K* and the Halo Occupation Distribution since z=1.5: Observations vs. Simulations
• Wobbling galaxy spin axes in dense environments
• Neutrino mass constraints on $\mu$-decay and ${\pi }^0\to \nu \bar{\nu }$
• Photometric Selection of Emission Line Galaxies, Clustering Analysis and a Search for the ISW effect
• Galaxy and Mass Assembly (GAMA): Small-scale anisotropic galaxy clustering and the pairwise velocity dispersion of galaxies
• PRIMUS: Obscured Star Formation on the Red Sequence
• An Active Instance-based Machine Learning method for Stellar Population Studies
• The Hubble Space Telescope WFPC2 B-Band Parallel Survey: A Study of Galaxy Morphology for 18 < B < 27 mag
• The size of the longest filament in the Luminous Red Galaxy distribution
• The spectroscopically confirmed huge cosmic structure at z=0.55
• Using the filaments in the LCRS to test the LambdaCDM model
• An empirical measurement of the Halo Mass Function from the combination of GAMA DR4, SDSS DR12, and REFLEX II data
• The first catalogue of spectroscopically confirmed red nuggets at z~0.7 from the VIPERS survey. Linking high-z red nuggets and local relics
• A gravitational lensing detection of filamentary structures connecting luminous red galaxies
• Interacting Tsallis and Rényi Holographic Dark Energy with Hybrid Expansion Law
• Two-dimensional kinematics of SLACS lenses - IV. The complete VLT-VIMOS data set
• The K-band luminosity functions of cluster galaxies
• Extending Recovery of the Primordial Matter Power Spectrum
• Constraints on Quintessence From Using Cosmological Data
• Predictions for the detection of Tidal Streams with Gaia using Great Circle Methods
• Scientific Objectives of the Hot Universe Baryon Surveyor (HUBS) Mission
• Improving Hickson-like compact group finders in redshift surveys: an implementation in the SDSS
• The Millennium Galaxy Catalogue: Star counts and the Structure of the Galactic Stellar Halo
• Compact Groups of Galaxies in Sloan Digital Sky Survey and LAMOST Spectral Survey. II. Dynamical Properties of Isolated and Embedded Groups
• Abell 2384: the galaxy population of a cluster post-merger
• ASTRO-F - Super IRAS - The All Sky Infra-Red Survey
• Mock galaxy redshift catalogues from simulations: implications for Pan-STARRS1
• The Faint End Slopes Of Galaxy Luminosity Functions In The COSMOS 2-Square Degree Field
• The Zurich Environmental Study (ZENS) of Galaxies in Groups along the Cosmic Web. V. Properties and Frequency of Merging Satellites and Centrals in Different Environments
• Evolution of the baryon fraction in the Local Group: accretion versus feedback at low and high z
• The Hector Survey: integral field spectroscopy of 100,000 galaxies
• The halo mass function conditioned on density from the Millennium Simulation: insights into missing baryons and galaxy mass functions
• Radio galaxies and their magnetic fields out to z <= 3
• ELUCID -- Exploring the Local Universe with the reConstructed Initial Density field. II: Reconstruction diagnostics, applied to numerical halo catalogs
• A Complete Cosmological Scenario in Teleparallel Gravity
• Double barred galaxies at intermediate redshifts: A feasibility study
• Galaxy redshift abundance periodicity from Fourier analysis of number counts $N(z)$ using SDSS and 2dF GRS galaxy surveys
• A brief review on cosmological analysis of galaxy surveys with multiple tracers
• Eigenmode Analysis of Galaxy Distributions in Redshift Space
• Estimate of neutrino masses from Koide's relation
• Topology of non-linear structure in the 2dF Galaxy Redshift Survey
• The Clustering Of Galaxies Around Radio-Loud AGNs
• Effects of galaxy environment on merger fraction
• Potential Importance of Binary Evolution in UV-Optical Spectral Fitting of Early-Type Galaxies
• How do galactic winds affect the Lyalpha forest?
• Gravitational Lensing Constraints on Dynamical and Coupled Dark Energy
• Radio Observations of the Hubble Deep Field South Region IV: Optical Properties of the Faint Radio Population
• Topology of large-scale structure in the 2dF Galaxy Redshift Survey
• Galaxy and Mass Assembly (GAMA): Witnessing the assembly of the cluster Abell 1882
• SARCS strong lensing galaxy groups: I - optical, weak lensing, and scaling laws
• The z=0.54 LoBAL Quasar SDSS J085053.12+445122.5: II. The Nature of Partial Covering in the Broad-Absorption-Line Outflow
• Unknown selection effect simulates redshift periodicity in quasar number counts from Sloan Digital Sky Survey
• The local universe in the era of large surveys. I. Spectral classification of S0 galaxies
• Integral Field spectroscopy of two HI rich E+A galaxies
• Detecting the Baryons in Matter Power Spectra
• The spatial distribution of X-ray selected AGN in the Chandra deep fields: a theoretical perspective
• The ALHAMBRA survey: 2-D analysis of the stellar populations in massive early-type galaxies at z < 0.3
• Searching for primordial non-Gaussianity in Planck CMB maps using a combined estimator
• Are the 2dFGRS superstructures a problem for hierarchical models?
• Exploring the sub-eV neutrino mass range with supernova neutrinos
• ELG Spectroscopic Systematics Analysis of the DESI Data Release 1
• An HI intensity mapping survey with a Phased Array Feed
• The effects of stellar populations on galaxy scaling relations in the 6dF Galaxy Survey
• Redshifts in the Southern Abell Redshift Survey Clusters. I. The Data
• The Diversity of Growth Histories of Milky Way-mass Galaxies
• The galaxy population of the complex cluster system Abell 3921
• The Tiling Algorithm for the 6dF Galaxy Survey
• Evolution of the Most Massive Galaxies to z ~ 0.6: II. The link between radio AGN activity and star formation
• RHDE models in FRW Universe with two IR cut-offs with redshift parametrization
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): On the correct recovery of the count-in-cell probability distribution function
• Wavelet analysis of baryon acoustic structures in the galaxy distribution
• Chemical evolution of local post-starburst galaxies: Implications for the mass-metallicity relation
• Redshifts and Velocity Dispersions of Galaxy Clusters in the Horologium-Reticulum Supercluster
• Identifying the 3FHL catalog: I. Archival Swift Observations and Source Classification
• The complex universe: recent observations and theoretical challenges
• Galaxy and Mass Assembly (GAMA): A $\text{WISE}$ study of the activity of emission-line systems in G23
• Warm-hot gas in groups and galaxies toward H2356-309
• The Capodimonte Deep Field I - Presentation of the survey and first follow-up studies
• CSST large-scale structure analysis pipeline: I. constructing reference mock galaxy redshift surveys
• Optical spectral classification of southern ultraluminous infrared galaxies
• Detecting Baryon Acoustic Oscillations
• Robustness of the covariance matrix for galaxy clustering measurements
• Morphology & Environment's Role on the Star Formation Rate -- Stellar Mass Relation in COSMOS from 0 < z < 3.5
• HIR4: cosmology from a simulated neutral hydrogen full sky using Horizon Run 4
• Autocorrelations of stellar light and mass at z~0 and ~1: From SDSS to DEEP2
• The Environment on few Mpc scales of Infrared Luminous Galaxies at Redshifts z~1
• Simulating the LOcal Web (SLOW) II: Properties of local galaxy clusters
• Nature and completeness of galaxies detected in the Two Micron All Sky Survey
• Submillimetre observations of galaxy clusters with BLAST: the star-formation activity in Abell 3112
• Dynamical segregation of galaxies in groups and clusters
• The effect of the environment on the Faber Jackson relation
• Large-scale structure and matter in the universe
• Probing large scale homogeneity and periodicity in the LRG distribution using Shannon entropy
• 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
• Herschel-ATLAS : The spatial clustering of low and high redshift submillimetre galaxies
• Constraining Galileon gravity from observational data with growth rate
• Central velocity dispersion catalog of LAMOST-DR7 galaxies
• Level sets estimation and Vorob'ev expectation of random compact sets
• Interacting entropy-corrected holographic Chaplygin gas model
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• Particle physics implications of the WMAP neutrino mass bound
• The whole picture of the large-scale structure of the CL1604 supercluster at z$\sim$0.9
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. IV. High Precision Constraints on the Evolution of Stellar-Halo Mass Relation at Redshift $z<0.7$
• End effects in optical fibres
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$. V: Properties of dark matter halos containing H$\alpha$ emitting galaxies
• Decoding X-ray observations from centres of galaxy clusters using MCMC
• The SOAR Gravitational Arc Survey - I: Survey overview and photometric catalogs
• The large-scale structure around the Fornax-Eridanus Complex
• Exploring the non-linear density field in the Millennium simulations with tessellations - I. The probability distribution function
• Clustering tomography: measuring cosmological distances through angular clustering in thin redshift shells
• Weak lensing detection of intra-cluster filaments with ground based data
• On the relation between Lya absorbers and local galaxy filaments
• Forecasting the success of the WEAVE Wide-Field Cluster Survey on the extraction of the cosmic web filaments around galaxy clusters
• The Integrated Sachs-Wolfe Effect in Interacting Dark Matter-Dark Energy Models
• The luminosity bias relation from filaments in the Sloan Digital Sky Survey Data Release Four
• Dynamics of Abell 3266 - I. An Optical View of a Complex Merging Cluster
• Galaxy interactions in filaments and sheets: effects of the large-scale structures versus the local density
• Observations of the High Redshift Universe
• Star Formation and Gas Phase History of the Cosmic Web
• Searching for HI imprints in cosmic web filaments with 21-cm intensity mapping
• Stellar populations in superclusters of galaxies
• Can Strong Gravitational Lensing Constrain Dark Energy?
• Evolution of Galaxy Luminosity Function and Luminosity Function by Density Environment at 0.03<z<0.5
• The SRG/eROSITA All-Sky Survey: X-ray beacons at late cosmic dawn
• The impact and mitigation of broad absorption line quasars in Lyman$-\alpha$ forest correlations
• Detecting clusters and groups of galaxies populating the local Universe in large optical spectroscopic surveys
• Green valley galaxies in the cosmic web: internal versus environmental quenching
• Clusters of galaxies: setting the stage
• A redshift survey of the nearby galaxy cluster Abell 2107: Global rotation of the cluster and its connection to large-scale structures in the universe
• The MUSE-Wide survey: Three-dimensional clustering analysis of Lyman-$\alpha$ emitters at $3.3<z<6$
• Performance study of Lagrangian methods: reconstruction of large scale peculiar velocities and baryonic acoustic oscillations
• Power-law solutions and accelerated expansion in scalar-tensor theories
• Dynamical analysis of strong-lensing galaxy groups at intermediate redshift
• Large Scale Structure in the ELAIS S1 Survey
• A More Efficient Search for H2O Megamaser Galaxies : The Power of the X-ray and Mid-infrared Photometry
• Star-Forming, Rotating Spheroidal Galaxies in the GAMA and SAMI Surveys
• The Millennium Galaxy Catalogue: a census of local compact galaxies
• Spectroscopic QUasar Extractor and redshift (z) EstimatorSQUEzE I: Methodology
• Cross Correlations of X-ray and Optically Selected Clusters With Near Infrared and Optical Galaxies
• Assembly Bias of Dwarf-sized Dark Matter Haloes
• Properties of Voids in the 2dFGRS Galaxy Survey
• A Coarse-Grained Field Theory for Density Fluctuations and Correlation Functions of Galactic Objects
• Dynamical Dark Energy model parameters with or without massive neutrinos
• Conditional Cumulants in Weakly Non-linear Regime
• Stochastic Processes as the Origin of the Double-Power Law Shape of the Quasar Luminosity Function
• Detection of WHIM in the Planck data using Stack First approach
• Schwarzschild Lecture 2014: HectoMAPping The Universe
• The Anisotropic Two-Point Correlation Functions of the Nonlinear Traceless Tidal Field in the Principal-Axis Frame
• Unravelling the Cosmic Web: An analysis of the SDSS DR14 with the Local Dimension
• HI intensity mapping with MeerKAT: forecast for delay power spectrum measurement using interferometer mode
• Forecasts of cosmological constraints from HI intensity mapping with FAST, BINGO & SKA-I
• Anisotropic Extinction Distortion of the Galaxy Correlation Function
• Detection of 20-30 Mpc-scale Galaxy Structures Embedded in 100 Mpc-scale Structures of Quasars and MgII Absorbers at z~0.8 and z~1.2
• Holistic spectroscopy: Complete reconstruction of a wide-field, multi-object spectroscopic image using a photonic comb
• An alternative approach to modelling a cosmic void and its effect on the cosmic microwave background
• A survey for dwarf galaxy remnants around fourteen globular clusters in the outer halo
• Consequences of dark matter self-annihilation for galaxy formation
• The 2-degree Field Lensing Survey: photometric redshifts from a large new training sample to r<19.5
• Analyzing Baryon Acoustic Oscillations in Sparse Spectroscopic Samples via Cross-Correlation with Dense Photometry
• Estimation of Photometric Redshifts. I. Machine Learning Inference for Pan-STARRS1 Galaxies Using Neural Networks
• Wide Field Surveys and Astronomical Discovery Space
• Boundary Corrections in Fractal Analysis of Galaxy Surveys
• Testing isotropy in the Two Micron All-Sky redshift survey with information entropy
• Multi-object spectroscopy of low redshift EIS clusters. I
• Filament Hunting: Integrated HI 21cm Emission From Filaments Inferred by Galaxy Surveys
• Ellipsoidal configurations in the de Sitter spacetime
• A Modified Generalized Chaplygin Gas as the Unified Dark Matter-Dark Energy Revisited
• Consistency of nonlinear interacting ghost dark energy with recent observations
• Cosmological Parameter Estimation from the Two-Dimensional Genus Topology -- Measuring the Expansion History using the Genus Amplitude as a Standard Ruler
• The role of major gas-rich mergers on the evolution of galaxies from the blue cloud to the red sequence
• The ACT-DR5 MCMF Galaxy Cluster Catalog
• Confronting semi-analytic galaxy models with galaxy-matter correlations observed by CFHTLenS
• Compatibility of the Large Quasar Groups with the Concordance Cosmological Model
• Genus statistics using the Delaunay tessellation field estimation method: (I) tests with the Millennium Simulation and the SDSS DR7
• Observational tests for oscillating expansion rate of the Universe
• Near Infrared spectroscopic indices for unresolved stellar populations. I. Template galaxy spectra
• Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
• Searching for X-ray luminous 'normal' galaxies in 2dfGRS
• The first shear measurements from precision weak lensing
• Simulating the formation of cosmic structure
• The galaxy luminosity function around groups
• Cosmological models of generalized ghost pilgrim dark energy (GGPDE) in the gravitation theory of Saez-Ballester
• The FSVS Cluster Catalogue: Galaxy Clusters and Groups in the Faint Sky Variability Survey
• Galaxy populations in groups and clusters: evidence for a characteristic stellar mass scale at $M_{\ast }\sim 10^{9.5}{M}_{\odot }$
• Probing Hot Gas in Galaxy Groups through the Sunyaev-Zeldovich Effect
• Weak Lensing Measurement of Filamentary Structure with the SDSS BOSS and Subaru Hyper Suprime-Cam Data
• Unexpected dancing partners: Tracing the coherence between the spin and motion of dark matter halos
• Large Density Perturbations from Reheating to Standard Model particles due to the Dynamics of the Higgs Boson during Inflation
• Cosmic crystallography using short-lived objects - active galactic nuclei
• Subaru Hyper Suprime-Cam excavates colossal over- and under-dense structures over 360 deg2 out to z=1
• Nonlinear Density Fluctuation Field Theory for Large Scale Structure
• Galaxy and Mass Assembly (GAMA): The Weak Environmental Dependence of Quasar Activity at 0.1<z<0.35
• The evolution of galaxy clustering since z=1 from the Calar Alto Deep Imaging Survey
• Spatial Periodicity of Galaxy Number Counts, CMB Anisotropy, and SNIa Hubble Diagram Based on the Universe Accompanied by a Non-Minimally Coupled Scalar Field
• Cosmological dynamics of a non-minimally coupled bulk scalar field in DGP setup
• Holographic dilatonic model of dark energy
• The CatSouth Quasar Candidate Catalog for the Southern Sky and a Unified All-Sky Catalog Based on Gaia DR3
• On the Evolution of the Bi-Modal Distribution of Galaxies in the Plane of Specific Star Formation Rate versus Stellar Mass
• Principal Component Analysis of Weak Lensing Surveys
• Astronomical Applications of Multi-Core Fiber Technology
• The SAMI Galaxy Survey: Using concentrated star-formation and stellar population ages to understand environmental quenching
• Cosmological forecasts from photometric measurements of the angular correlation function
• An Introduction into the Theory of Cosmological Structure Formation
• Revisiting the clustering of narrow-line AGN in the local Universe: Joint dependence on stellar mass and color
• The stellar populations of early-type galaxies -- I. Observations, line-strengths and stellar population parameters
• Interacting holographic tachyon model of dark energy
• Link between radio-loud AGNs and host-galaxy shape
• Halo Model Analysis of Cluster Statistics
• Using galaxy pairs as cosmological tracers
• The ESO-Sculptor Survey: Evolution of late-type galaxies at redshifts 0.1-0.5
• First results with the ORPHEUS dark matter detector
• The 2dF BL Lac Survey II
• The detection of a massive chain of dark HI clouds in the GAMA G23 Field
• Spatial density fluctuations and selection effects in galaxy redshift surveys
• The Jiao Tong University Spectroscopic Telescope Project
• Cosmological Analysis of Modified Holographic Ricci Dark Energy in Chern-Simons Modified Gravity
• Cosmic Filaments from Cosmic Strings
• An Optical Analysis of the Merging Cluster Abell 3888
• Ghost dark energy with sign-changeable interaction term
• Morphology-based query for galaxy image databases
• Are dumbbell brightest cluster members signposts to galaxy cluster activity?
• Angular clustering of z~2 star-forming and passive galaxies in 2.5 square degrees of deep CFHT imaging
• Photo-z Quality Cuts and their Effect on the Measured Galaxy Clustering
• Improved parametrization of the growth index for dark energy and DGP models
• Clustering and descendants of MUSYC galaxies at z<1.5
• An HST/COS Observation of Broad Ly$\alpha$ Emission and Associated Absorption Lines of the BL Lacertae Object H 2356-309
• Antisymmetric Cross-correlation between H I and CO Line Intensity Maps as a New Probe of Cosmic Reionization
• Pre-processing of Galaxies in the Early Stages of Cluster Formation in Abell 1882 at $z$=0.139
• The 2dF Galaxy Redshift Survey as a Cosmological Laboratory
• The Properties of Type Ia Supernova Host Galaxies from the Sloan Digital Sky Survey
• Cosmological surveys with multi-object spectrographs
• Phantom-Like Behavior of a DGP-Inspired Scalar-Gauss-Bonnet Gravity
• Combining Strong Lensing and Dynamics in Galaxy Clusters: integrating MAMPOSSt within LENSTOOL I. Application on SL2S J02140-0535
• Characterizing SL2S galaxy groups using the Einstein radius
• Phantom-like effects in asymmetric brane embedding with induced gravity and the Gauss-Bonnet term in the Bulk
• GABE: Galaxy Assembly with Binary Evolution
• Deep UV Luminosity Functions at the Infall Region of the Coma Cluster
• On the Environmental Dependence of Galaxy Properties Established by the Initial Cosmological Conditions
• The gravitational and lensing-ISW bispectrum of 21cm radiation
• Analytical solutions of the geodesic equation in the space-time of a black hole surrounded by perfect fluid in Rastall theory
• Discord in Concordance Cosmology and Anomalously Massive Early Galaxies
• Demographics of Sloan Digital Sky Survey galaxies along the Hubble sequence
• Interpreting the galaxy group CG J1720-67.8 through evolutionary synthesis models
• Reconstructions of $f(\mathcal{P})$ and $f(\mathcal{Q})$ gravity models from $(m,n)$-type Barrow Holographic Dark Energy: Analysis and Observational Constraints
• Discovery of a Large-scale Wall in the Direction of Abell 22
• Beyond the galaxy luminosity function
• Photometric and clustering properties of hydrodynamical galaxies in a cosmological volume: results at z=0
• The influence of Hickson-like compact group environment on galaxy luminosities
• Structure in the 3D Galaxy Distribution: II. Voids and Watersheds of Local Maxima and Minima
• The LEDA galaxy distribution: I. Maps of the Local Universe
• An optimised tiling pattern for multi-object spectroscopic surveys: application to the 4MOST survey
• The GALAH Survey: Relative throughputs of the 2dF fibre positioner and the HERMES spectrograph from stellar targets
• The Origin of the Large-Scale Structure in the Universe: Theoretical and Statistical Aspects
• Stacked reverberation lags at high redshift
• The Three Hundred project: Estimating the dependence of gas filaments on the mass of galaxy clusters
• UV to FIR catalogue of a galaxy sample in nearby clusters: SEDs and environmental trends
• The spatial distribution of satellites in galaxy clusters
• Reconstructing the Triaxial Shapes of Dark Matter Halos from the Anisotropic Spatial Distributions of their Substructures in the Concordance Cosmology
• Evolution of dissipative and non-dissipative universes in holographic cosmological models with a power-law term
• Multi-object spectroscopy of low redshift EIS clusters. II
• Galaxy evolution in compact groups II. Witnessing the influence of major structures in their evolution
• Realistic Equations of State for the Primeval Universe
• Galaxy And Mass Assembly (GAMA): Stellar-to-Dynamical Mass Relation I. Constraining the Precision of Stellar Mass Estimates
• The PAU Survey: Photometric redshift estimation in deep wide fields
• PAC in DESI. I. Galaxy Stellar Mass Function into the $10^6{\mathrm{M}}_{\odot }$ Frontier
• Statistical physics for cosmic structures
• Using the 2-MASS Photometric Redshift Survey to optimize LIGO Follow-Up Observations
• A New Approach to the Optimal Target Selection Problem
• Star Formation in Ultraluminous Infrared Galaxies Probed with AKARI Near-Infrared Spectroscopy
• The Structure of 2MASS Galaxy Clusters
• Two-point statistics without bins: A continuous-function generalization of the correlation function estimator for large-scale structure
• Estimation of Photometric Redshifts. II. Identification of Out-of-Distribution Data with Neural Networks
• The Southern 2MASS AGN Survey: spectroscopic follow-up with 6dF
• The local Universe in the era of large surveys -- II. Multi-wavelength characterisation of activity in nearby S0 galaxies
• Searching in HI for Massive Low Surface Brightness Galaxies: Samples from HyperLeda and the UGC
• Semi-Numerical Simulation of Reionization with Semi-Analytical Modeling of Galaxy Formation
• Identification of 4876 Bent-Tail Radio Galaxies in the FIRST Survey Using Deep Learning Combined with Visual Inspection
• The Gas Accretion History of Low Mass Halos within the Cosmic Web from Cosmological Simulations
• Accurate Modeling of the Projected Galaxy Clustering in Photometric Surveys: I. Tests with Mock Catalogs
• The X-ray Zurich Environmental Study (X-ZENS). I. Chandra and XMM-Newton observations of AGNs in galaxies in nearby groups
• PRIMUS: The Effect of Physical Scale on the Luminosity-Dependence of Galaxy Clustering via Cross-Correlations
• Cosmology in One Dimension: Vlasov Dynamics
• Expansion and Growth of Structure Observables in a Macroscopic Gravity Averaged Universe
• Optimizing high redshift galaxy surveys for environmental information
• Integrated perturbation theory for cosmological tensor fields. IV. Full-sky formulation
• COMBO-17 measurements of the effect of environment on the type-dependent galaxy luminosity function
• Identifications of FIRST radio sources in the NOAO Deep-Wide Field Survey
• Comparison of two optical cluster finding algorithms for the new generation of deep galaxy surveys
• Galaxy And Mass Assembly (GAMA): the signatures of galaxy interactions as viewed from small scale galaxy clustering
• Magnification bias in the shear-ratio test: a viable mitigation strategy
• Supersoft, luminous X-ray sources in galactic nuclei
• Observational determination of the galaxy bias from cosmic variance with a random pointing survey: Clustering of z~2 galaxies from Hubble's BoRG survey
• Perturbation Theory Remixed: Improved Nonlinearity Modeling beyond Standard Perturbation Theory
• 2MASS Galaxies in the Fornax Cluster Spectroscopic Survey
• A $K_s$-band selected catalogue of objects in the ALHAMBRA survey
• Satellite galaxies in the Illustris-1 simulation: anisotropic locations around relatively isolated hosts
• Shape noise and dispersion in precision weak lensing
• The infrared-radio relation in the local universe
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• Transient Accelerating Scalar Models with Exponential Potential
• Enhancing Photometric Redshift Catalogs Through Color-Space Analysis: Application to KiDS-Bright Galaxies
• The warm-hot intergalactic medium in inter-cluster filaments -- A forecast for HUBS observations based on eRASS1 superclusters
• The Aquarius Superclusters II. Spectroscopic and Photometric Data
• Simulating Kilonovae in the ΛCDM Universe
• Constraining cosmological parameters using void statistics from the SDSS survey
• SED-inferred properties and morphology of Lyman-break galaxies at $z\sim 1$ in the CDF-S
• The maximum extent of the filaments and sheets in the cosmic web: an analysis of the SDSS DR17
• Galaxy groups in the 2dF galaxy redshift survey: A Compactness Analysis of Groups
• Simulation of complex phenomena in optical fibres
• A composite K-band Luminosity Function for Cluster Galaxies
• Quantifying the Bull's Eye Effect
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): PCA-based automatic cleaning and reconstruction of survey spectra
• A Machine Learning Approach to Correct for Mass Resolution Effects in Simulated Halo Clustering Statistics
• Collision-free motion planning for fiber positioner robots: discretization of velocity profiles
• DarkAI: Reconstructing the density, velocity and tidal field of dark matter from a DESI-like bright galaxy sample
• Statistically significant length scale of filaments as a robust measure of galaxy distribution
• The Effects of Relativistic Corrections on Cosmological Parameter Estimations from SZE Cluster Surveys
• Galaxy-galaxy(-galaxy) lensing as a sensitive probe of galaxy evolution
• The X-Ray Zurich Environmental Study (X-ZENS). II. X-ray Observations of the Diffuse Intragroup Medium in Galaxy Groups
• Dark Energy Survey Deep Field photometric redshift performance and training incompleteness assessment
• MaNGA AGN dwarf galaxies (MAD). III. The role of mergers and environment in active galactic nucleus activity in dwarf galaxies
• The probabilistic random forest applied to the QUBRICS survey: improving the selection of high-redshift quasars with synthetic data
• Search for anomalous features in gamma-ray blazar spectra corrected for the absorption on the extragalactic background light
• Galaxy Groups: Proceedings from a Swinburne University Workshop
• Measuring the velocity field from type Ia supernovae in an LSST-like sky survey
• Black holes inside cosmic voids
• Abell 2626 and friends: large and small scale structure
• On the nature of high X-ray luminosities in SDSS galaxies
• The Environments of Low and High Luminosity Radio Galaxies at Moderate Redshifts
• The WiggleZ Dark Energy Survey: Galaxy Evolution at 0.25 < z < 0.75 Using The Second Red-Sequence Cluster Survey (RCS-2)
• A Scaling Relation of the Evolving Tidal Fields in a LCDM Cosmology
• Theories of Everything and Hawking's Wave Function of the Universe
• Status and Perspectives of Neutrino Physics
• Inferring Cosmological Parameters on SDSS via Domain-Generalized Neural Networks and Lightcone Simulations
• A young galaxy cluster in the old Universe
• Dust Distribution during Reionization
• Anomalous anisotropic cross-correlations between WMAP CMB maps and SDSS galaxy distribution and implications on the dark flow scenario
• Magnetic fields in galaxies: I. Radio disks in local late-type galaxies
• The architecture of Abell 1386 and its relationship to the Sloan Great Wall
• Nonsingular and accelerated expanding universe from effective Yang-Mills theory
• A new method to probe the mass density and the cosmological constant using configuration entropy
• Nucleation regions in the Large-Scale Structure I. A catalogue of cores in nearby rich superclusters
• Joint constraints on galaxy bias and ${\sigma }_8$ through the N-pdf of the galaxy number density
• Nature and Environment of Very Luminous Galaxies
• Clustering Measurements of broad-line AGNs: Review and Future
• The Star Formation Rate-Density Relationship at Redshift Three
• Non-Linearly Interacting Ghost Dark Energy in Brans-Dicke Cosmology
• Variability and transient search in the SUDARE-VOICE field: a new method to extract the light curves
• Can anisotropy in the galaxy distribution tell the bias?
• Peaks in the cosmological density field: parameter constraints from 2dF Galaxy Redshift Survey data
• Cosmological Signatures of Dark Sector Physics: The Evolution of Haloes and Spin Alignment
• Compact groups of galaxies in GAMA -- Probing the densest minor systems at intermediate redshifts
• SpecPT (Spectroscopy Pre-trained Transformer) Model for Extragalactic Spectroscopy: I. Architecture and Automated Redshift Measurement
• Sky surveys and deep fields of ground-based and space telescopes
• A New Multi-Scale Structure Finding Algorithm to Identify Cosmological Structure
• Cosmic filament spin -- I: a comparative study in observation
• Euclid preparation. Spatially resolved stellar populations of local galaxies with Euclid: a proof of concept using synthetic images with the TNG50 simulation
• Star Formation in Satellite Galaxies
• Self-interacting Dark Matter with Scalar Dilepton Mediator
• Millimeter-wave observations of Euclid Deep Field South using the South Pole Telescope: A data release of temperature maps and catalogs
• The Low Redshift survey at Calar Alto (LoRCA)
• Faint 1.4 GHz sources in the 2dF Galaxy Redshift Survey
• Dark Energy Survey Year 3 Results: Deep Field Optical + Near-Infrared Images and Catalogue
• Practical Statistics for the Voids Between Galaxies
• Modified cosmology through generalized mass-to-horizon entropy: observational constraints from DESI DR2 BAO data
• Locations of Satellite Galaxies in the Two-Degree Field Galaxy Redshift Survey
• Spectroscopic detection of quasars in the 2dF Galaxy Redshift Survey
• The Velocity Field Around Groups of Galaxies
• An Optimized Ly$\alpha$ Forest Inversion Tool Based on a Quantitative Comparison of Existing Reconstruction Methods
• Searching for Radio Transients with Inverted Spectra in Epoch 1 of VLASS and VCSS, and Identification of a Sample of Candidate Relativistic Nuclear Transients
• Improving SDSS cosmological constraints through $\beta$-skeleton weighted correlation functions
• The VST ATLAS Quasar Survey I: Catalogue
• Reconstructions of Einstein-Aether Gravity from Barrow Agegraphic and New Barrow Agegraphic Dark Energy models: Examinations and Observational Limits
• Small-Scale Dynamical Coherence Accompanied with Galaxy Conformity
• A new approach to finding galaxy groups using Markov Clustering
• The Formation and Evolution of Massive Galaxies
• Enabling the next generation of scientific discoveries by embracing photonic technologies
• Application of Multicore Optical Fibers in Astronomy
• The XMM-SERVS X-ray eXtended Galaxy Cluster (XVXGC) catalog
• The XMM-Newton/2dF survey-VIII: The extended X-ray sources
• Constraining Inflationary Scenarios with Braneworld Models and Second Order Cosmological Perturbations
• The Multi-wavelength Extreme Starburst Sample of Luminous Galaxies Part I: Sample Characteristics
• Groups of dwarf galaxies in the Local supercluster
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• New formulae for the Hubble Constant in a Euclidean Static Universe
• Spectro-photometric and Weak Lensing Survey of a Supercluster and Typical Field Region -- I. Spectroscopic Redshift Measurements
• The influence of superstructures on bright galaxy environments: clustering properties
• Power-law solutions for TeVeS
• Pulsar B1237+25 Aberration/Retardation Analysis from Decimeter to Decameter Wavelength: Challenge to "Radius-to-Frequency Mapping"
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• Phenomenology of Hybrid Scenarios of Neutrino Dark Energy
• Mass limits for heavy neutrinos
• SDSS J122958.84+000138.0: A Compact, Optically red galaxy
• Associations of dwarf galaxies in a $\Lambda$CDM Universe
• On the cosmological viability of the Hu-Sawicki type modified induced gravity
• Deep Extragalactic VIsible Legacy Survey (DEVILS): First Data Release Covering The D10 (COSMOS) Region
• Cosmology with Galaxy Correlations
• The Photometric Maximum in Cosmicflows-2
• Constraints on Galaxy Structure and Evolution from the Light of Nearby Systems
• GrAviPaSt's Lens to the Past: Unveiling the Evolution of Filamentary Structures
• Lagrangian Volume Deformations around Simulated Galaxies
• Exploring the Cosmic Web in the Sloan Digital Sky Survey Data Release Seven using the Local Dimension
• A new Bowen Fluorescence Flare and Extreme Coronal Line Emitter discovered by SRG/eROSITA
• The h-index in Australian Astronomy
• Field Target Allocation and Routing Algorithms for Starbugs
• Photometric redshift galaxies as tracers of the filamentary network
• Galaxy distribution and evolution around a sample of 2dF groups
• Direct Shear Mapping: Prospects for weak lensing studies of individual galaxy-galaxy lensing systems
• Caustic and hydrostatic mass bias: Implications for modified gravity
• The HST-Hyperion Survey: Companion Fraction and Overdensity in a z ~ 2.5 Proto-supercluster
• Modified cosmology through generalized mass-to-horizon entropy: implications for structure growth and primordial gravitational waves
• Star-forming galaxies in the cosmic web in the last 11 Gyr
• Spectral Synthesis via Mean Field approach Independent Component Analysis
• The stellar and hot gas content of low-mass galaxy clusters
• Galaxy structures - Groups, clusters and superclusters
• Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations
• Z-Sequence: Photometric redshift predictions for galaxy clusters with sequential random k-nearest neighbours
• Revisiting the Cosmological Principle in a Cellular Framework
• Exploring Galaxy Properties of eCALIFA with Contrastive Learning
• Spatial correlations of extended cosmological structures
• Spatial clustering in the ESO-Sculptor Survey: two-point correlation functions by galaxy type at redshifts 0.1 - 0.5
• Completeness II: A signal-to-noise approach for completeness estimators applied to galaxy magnitude-redshift surveys
• Dust contribution to the panchromatic galaxy emission
• On the angular distribution of IceCube high-energy events
• VEGA: Voids idEntification using Genetic Algorithm
• Observable predictions of generalised inflationary scenarios
• Evolution of star-forming dwarf galaxies in different environments
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• Tensor anisotropy as a tracer of cosmic voids
• The clustering properties of high-redshift passive galaxies
• Color Transformations of Photometric Measurements of Galaxies in Optical and Near-Infrared Wide-Field Imaging Surveys
• The probability distribution of 3-D shapes of galaxy clusters from 2-D X-ray images
• Luminosity Bias (II): The Cosmic Web of the First Stars
• Monopole Fluctuations in Galaxy Surveys
• Do data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
• Stability of HDE model with sign-changeable interaction in Brans-Dicke theory
• Can we constrain the evolution of HI bias using configuration entropy?
• The relation of galaxies and dark matter haloes to the filamentary cosmic web
• Triplets of Quasars at high redshift I: Photometric data
• Inhomegeneous cosmological models and fine-tuning of the initial state
• A three dimensional object point process for detection of cosmic filaments
• Modeling and measuring the anisotropic halo 3-point correlation function: a coordinated study
• The XMM-Newton/2dF survey - V. the radio properties of the X-ray population
• The Neighborhood Function and Its Application to Identifying Large-Scale Structure in the Comoving Universe Frame
• The richest superclusters. I. Morphology
• Perspectives for studying the dark energy at z>2 with galaxy surveys
• Two categories of UV-upturn galaxies revealed by semi-analytic models
• Probing the spatial and velocity anisotropies in stellar halos from the Aquarius simulations
• Applying Vision Transformers on Spectral Analysis of Astronomical Objects
• Impact of the large-scale cosmic web on the X-ray emitting circumgalactic medium
• Hyper Suprime-Cam Y3 results: photo-$z$ bias calibration with lensing shear ratios and cosmological constraints from cosmic shear
• Faint galaxies in the Zone of Avoidance revealed by JWST/NIRCam
• CSST Slitless Spectra: Target Detection and Classification with YOLO
• The FIRST radio survey: Panchromatic properties of FIRST radio sources identified in the Bootes and Cetus fields
• Measurement of the Hubble constant using the Dark Energy Survey Year 6 Gold galaxy catalogue and the fourth Gravitational-Wave Transient Catalogue
• Mechanisms Affecting Galaxies Nearby and Environmental Trends (MAGNET)
• Transients from Initial Conditions Based on Lagrangian Perturbation Theory in $N$-body Simulations III: The Case of GADGET-2 Code
• Largest scales from the largest galaxy surveys: the pseudo Karhunen-Loève method
• Gas thermodynamics meets galaxy kinematics: Joint mass measurements for eROSITA galaxy clusters
• Heterogeneity of Inverted Calcium II H:K Ratio Cluster Galaxies
• A group finder algorithm optimised for the study of local galaxy environment
• CDM and Baryons as Distinct Fluids in a Linear Approximation for the Growth of Structure
• Particle Physics in the Sky and Astrophysics Underground: Connecting the Universe's Largest and Smallest Scales
• Hosts and environments: a (large-scale) radio history of AGN and star-forming galaxies
• Detecting and analysing the topology of the cosmic web with spatial clustering algorithms I: Methods
• Tracing the environmental history of observed galaxies via extended fast action minimization method
• Panchromatic properties of galaxies in wide-field optical spectroscopic and photometric surveys
• Estimating the completeness of the QUBRICS Survey with 3501 QSO redshifts from Gaia DR3 spectra
• Virgo Filaments VI: H$\alpha$ clumps in the filaments around the Virgo galaxy cluster
• The Manticore Project II: Bayesian digital twins of cosmic structure across the SDSS and BOSS volumes
• Using the large scale quasar clustering to constrain flat quintessential universes
• Hybrid-z: Enhancing Kilo-Degree Survey bright galaxy sample photometric redshifts with deep learning
• Mentari: A pipeline to model the galaxy SED using semi analytic models
• The formation of blue cluster in local Universe
• A Non-parametric Method for the Inference of Halo Occupation Distributions
• Diagnosing Systematic Effects Using the Inferred Initial Power Spectrum
• Determining the Dark Matter distribution in galaxies with Deep Learning
• The BINGO project X. Cosmological parameter constraints from HI Intensity Mapping lognormal simulations
• Euclid preparation. 3D reconstruction of the cosmic web with simulated Euclid Deep spectroscopic samples
• Galaxy And Mass Assembly (GAMA): Deconstructing the galaxy stellar mass function by star formation and environment
• Discovery of 178 Giant Radio Galaxies in 1059 deg${}^2$ of the Rapid ASKAP Continuum Survey at 888 MHz
• Where's Swimmy?: Mining unique color features buried in galaxies by deep anomaly detection using Subaru Hyper Suprime-Cam data
• Spatially Dependent Photometric Activity of M dwarfs in the Solar Cylinder
• Recent Advances in Large-Scale Structure and Galaxy Formation Studies
• Citations to Australian Astronomy: 5 and 10 Year Benchmarks
• Disk Sizes in a LCDM Universe
• Multiple rooks of chess - a generic integral field unit deployment technique
• Observational assessment of the viability of de Sitter-Gödel-de Sitter phase transition
• Natural inflation in Palatini $F(R)$
• Spikes in the SED and Ripples in the Outskirts of Galaxies
• Tracing correlations between galaxy properties across the Cosmic Web: An IllustrisTNG-based study
• The Filament Rift: $\Lambda$CDM's Structural Challenge Against Observation
• Galaxy quenching across the Cosmic Web: disentangling mass and environment with SDSS DR18
• Cosmic Dipoles from Large-Scale Structure Surveys
• Mapping the dark matter using weak lensing
• Cosmological bounds on dark matter annihilation using dark ages 21-cm signal
• Coupling light into optical fibres near the diffraction limit
• Sample Variance in Cosmological Observations with a Narrow Field-of-View
• The structural elements of the cosmic web
• An emulation-based model for the projected correlation function
• The intergalactic medium in the cosmic web
• Maps of the Cosmos: The Cosmic Microwave Background
• Quintessence reconstruction of interacting HDE in a non-flat universe
• $\Lambda$CDM, $\Lambda$DGP and extended phantom-like cosmologies
• Challenges in Stellar Population Studies
• Enhancing Cosmological Constraints by Two-dimensional $\beta$-cosmic-web Weighted Angular Correlation Functions
• Redshifts of Objects near 3C 220.3
• A catalogue of Type 2 active galactic nuclei in the 6dF Galaxy Survey