Simulating the joint evolution of quasars, galaxies and their large-scale distribution

Abstract

The cold dark matter model has become the leading theoretical paradigm for the formation of structure in the Universe. Together with the theory of cosmic inflation, this model makes a clear prediction for the initial conditions for structure formation and predicts that structures grow hierarchically through gravitational instability. Testing this model requires that the precise measurements delivered by galaxy surveys can be compared to robust and equally precise theoretical calculations. Here we present a novel framework for the quantitative physical interpretation of such surveys. This combines the largest simulation of the growth of dark matter structure ever carried out with new techniques for following the formation and evolution of the visible components. We show that baryon-induced features in the initial conditions of the Universe are reflected in distorted form in the low-redshift galaxy distribution, an effect that can be used to constrain the nature of dark energy with next generation surveys.

Nature, in press, 42 pages, 11 Figures, Supplementary Information included, movie available http://www.mpa-garching.mpg.de/galform/millennium

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• Impact of baryon physics on dark matter structures: a detailed simulation study of halo density profiles
• Evolution of the Color-Magnitude Relation in Galaxy Clusters at z ~1 from the ACS Intermediate Redshift Cluster Survey
• Evidence for a ~300 Mpc Scale Under-density in the Local Galaxy Distribution
• The stellar-to-halo mass relation over the past 12 Gyr
• Lightcone mock catalogues from semi-analytic models of galaxy formation - I. Construction and application to the BzK colour selection
• Quasar Luminosity Functions from Joint Evolution of Black Holes and Host Galaxies
• Inside-out or Outside-in: The topology of reionization in the photon-starved regime suggested by Lyman-alpha forest data
• Herschel-ATLAS: a binary HyLIRG pinpointing a cluster of starbursting proto-ellipticals
• A new model of galaxy formation: How sensitive are predicted galaxy luminosities to the choice of SPS model?
• On the formation and physical properties of the Intra-Cluster Light in hierarchical galaxy formation models
• Strong bimodality in the host halo mass of central galaxies from galaxy-galaxy lensing
• The detectability of baryonic acoustic oscillations in future galaxy surveys
• N-body Dark Matter Haloes with simple Hierarchical Histories
• The Missing Massive Satellites of the Milky Way
• The WIRCam Deep Survey I: Counts, colours and mass-functions derived from near-infrared imaging in the CFHTLS deep fields
• Reproducing the Stellar Mass/Halo Mass Relation in Simulated LCDM Galaxies: Theory vs Observational Estimates
• Simulations of Wide-Field Weak Lensing Surveys I: Basic Statistics and Non-Gaussian Effects
• Simulation of the Cosmic Evolution of Atomic and Molecular Hydrogen in Galaxies
• Intensity Mapping of the [CII] Fine Structure Line during the Epoch of Reionization
• Local Gravity versus Local Velocity: Solutions for $\beta$ and nonlinear bias
• CANDELS+3D-HST: compact SFGs at z~2-3, the progenitors of the first quiescent galaxies
• Initial conditions to cosmological N-body simulations, or how to run an ensemble of simulations
• The role of cold gas and environment on the stellar mass - metallicity relation of nearby galaxies
• Measurements of the UV background at 4.6 < z < 6.4 using the quasar proximity effect
• The Correlation of Star Formation Quenching with Internal Galaxy Properties and Environment
• On the origin of the faint-end of the red sequence in high density environments
• The evolution of star formation histories of quiescent galaxies
• Dark Matter Halo Merger Histories Beyond Cold Dark Matter: I - Methods and Application to Warm Dark Matter
• A New Method for Estimating Dark Matter Halo Masses using Globular Cluster Systems
• Initial Conditions for Large Cosmological Simulations
• The Impact of Star Formation Feedback on the Circumgalactic Medium
• Tracing the Dark Matter Sheet in Phase Space
• Superdense galaxies and the mass-size relation at low redshift
• The Spitzer Extragalactic Representative Volume Survey (SERVS): survey definition and goals
• The Local Nanohertz Gravitational-Wave Landscape From Supermassive Black Hole Binaries
• The MultiDark Database: Release of the Bolshoi and MultiDark Cosmological Simulations
• Shaping the galaxy stellar mass function with supernova- and AGN-driven winds
• A census of metals and baryons in stars in the local Universe
• Galaxy alignments: Observations and impact on cosmology
• Large Structures and Galaxy Evolution in COSMOS at z < 1.1
• Dependence of Interstellar Turbulent Pressure on Supernova Rate
• Quantifying cosmic variance
• The Sherwood simulation suite: overview and data comparisons with the Lyman-alpha forest at redshifts 2 < z < 5
• Gravitational-wave Limits from Pulsar Timing Constrain Supermassive Black Hole Evolution
• The upper bound on the lowest mass halo
• Galaxy clustering in the NEWFIRM Medium Band Survey: the relationship between stellar mass and dark matter halo mass at 1 < z < 2
• Massive Halos in Millennium Gas Simulations: Multivariate Scaling Relations
• Supermassive black holes in cosmological simulations I: M_BH-M_star relation and black hole mass function
• The spin and orientation of dark matter halos within cosmic filaments
• Intracluster stars in simulations with AGN feedback
• Globular cluster formation in the context of galaxy formation and evolution
• The impact of companions on stellar evolution
• On Halo Formation Times and Assembly Bias
• Large-scale dark matter simulations
• The HI content of star-forming galaxies at z = 0.24
• The velocity width function of galaxies from the 40% ALFALFA survey: shedding light on the cold dark matter overabundance problem
• Size--luminosity relations and UV luminosity functions at $z=6-9$ simultaneously derived from the complete Hubble Frontier Fields data
• The Spine of the Cosmic Web
• r-Process Nucleosynthesis: Connecting Rare-Isotope Beam Facilities with the Cosmos
• The SDSS DR6 Luminosity Functions of Galaxies
• The ACS Fornax Cluster Survey. VIII. The Luminosity Function of Globular Clusters in Virgo and Fornax Early-Type Galaxies and its Use as a Distance Indicator
• Dark matter halo properties of GAMA galaxy groups from 100 square degrees of KiDS weak lensing data
• Dynamical masses of early-type galaxies at z~2: Are they truly superdense?
• The Formation Rates of Population III Stars and Chemical Enrichment of Halos during the Reionization Era
• On the impact of empirical and theoretical star formation laws on galaxy formation
• Matter power spectrum and the challenge of percent accuracy
• Modelling galaxy clustering in a high resolution simulation of structure formation
• Rejuvenating the matter power spectrum: restoring information with a logarithmic density mapping
• Mergers and Mass Accretion Rates in Galaxy Assembly: The Millennium Simulation Compared to Observations of z~2 Galaxies
• The abundance of (not just) dark matter haloes
• Galaxy And Mass Assembly (GAMA): Galaxy close-pairs, mergers, and the future fate of stellar mass
• Mass Calibration and Cosmological Analysis of the SPT-SZ Galaxy Cluster Sample Using Velocity Dispersion ${\sigma }_v$ and X-ray $Y_{\text{X}}$ Measurements
• Early assembly of the most massive galaxies
• Galaxy alignments: Theory, modelling and simulations
• Mapping galaxy encounters in numerical simulations: The spatial extent of induced star formation
• The Rising Star-Formation Histories of Distant Galaxies and Implications for Gas Accretion with Time
• Information field theory for cosmological perturbation reconstruction and non-linear signal analysis
• Assembly History and Structure of Galactic Cold Dark Matter Halos
• Gas driven massive black hole binaries: signatures in the nHz gravitational wave background
• General relativity and cosmic structure formation
• X-ray cavities in a sample of 83 SPT-selected clusters of galaxies: Tracing the evolution of AGN feedback in clusters of galaxies out to z=1.2
• Gas filaments of the cosmic web located around active galaxies in a proto-cluster
• The Vimos VLT Deep Survey: Global properties of 20000 galaxies in the I_AB<=22.5 WIDE survey
• Moving mesh cosmology: the hydrodynamics of galaxy formation
• A Unifying Theory of Dark Energy and Dark Matter: Negative Masses and Matter Creation within a Modified $\Lambda$CDM Framework
• Unifying X-ray Scaling Relations from Galaxies to Clusters
• The Effective Number Density of Galaxies for Weak Lensing Measurements in the LSST Project
• Effects of AGN feedback on LCDM galaxies
• SDSS-IV MaNGA: Stellar angular momentum of about 2300 galaxies: unveiling the bimodality of massive galaxy properties
• Probing the missing baryons with the Sunyaev-Zel'dovich effect from filaments
• Dust Formation in Milky Way-like Galaxies
• Growing the first bright quasars in cosmological simulations of structure formation
• X-ray coronae in simulations of disc galaxy formation
• The growth of dark matter halos: evidence for significant smooth accretion
• Predictions for ASKAP Neutral Hydrogen Surveys
• High Performance P3M N-body code: CUBEP3M
• Precision cosmology from future lensed gravitational wave and electromagnetic signals
• Size Evolution of Spheroids in a Hierarchical Universe
• `Eppur Si Muove': On The Motion of the Acoustic Peak in the Correlation Function
• Building galaxies by accretion and in-situ star formation
• Acoustic oscillations in the SDSS DR4 Luminous Red Galaxy sample power spectrum
• Measuring the matter density using baryon oscillations in the SDSS
• The Atomic to Molecular Transition and its Relation to the Scaling Properties of Galaxy Disks in the Local Universe
• Predictions for the CO emission of galaxies from a coupled simulation of galaxy formation and photon dominated regions
• Insights into the content and spatial distribution of dust from the integrated spectral properties of galaxies
• The Spiderweb galaxy: a forming massive cluster galaxy at z~2
• Non-linear structure formation and the acoustic scale
• Scientific Discovery with the James Webb Space Telescope
• The Next Generation Virgo Cluster Survey. VIII. The Spatial Distribution of Globular Clusters in the Virgo Cluster
• The properties of satellite galaxies in simulations of galaxy formation
• Physical Properties of Galaxies from z=2-4
• The dominant role of mergers in the size evolution of massive early-type galaxies since z ~ 1
• The onion universe: all sky lightcone simulations in spherical shells
• The baryon fraction of LambdaCDM haloes
• Understanding the shape of the halo-mass and galaxy-mass cross-correlation functions
• Strong lensing optical depths in a \LambdaCDM universe
• Star formation quenching in simulated group and cluster galaxies: When, how, and why?
• Black Hole Growth in Hierarchical Galaxy Formation
• The recycling of gas and metals in galaxy formation: predictions of a dynamical feedback model
• Spin-independent elastic WIMP scattering and the DAMA annual modulation signal
• The Weak Lensing Signal and the Clustering of BOSS Galaxies II: Astrophysical and Cosmological Constraints
• The ACS Fornax Cluster Survey. VI. The Nuclei of Early-Type Galaxies in the Fornax Cluster
• A Public, K-Selected, Optical-to-Near-Infrared Catalog of the Extended Chandra Deep Field South (ECDFS) from the MUltiwavelength Survey by Yale-Chile (MUSYC)
• Magnetohydrodynamic Simulations of Disk Galaxy Formation: the Magnetization of The Cold and Warm Medium
• Dark Matter and Fundamental Physics with the Cherenkov Telescope Array
• Global structure and kinematics of stellar haloes in cosmological hydrodynamic simulations
• Models and Simulations for the Photometric LSST Astronomical Time Series Classification Challenge (PLAsTiCC)
• The Shapes and Alignments of Dark Matter Halos
• First Results from Z-FOURGE: Discovery of a Candidate Cluster at z = 2.2 in COSMOS
• The UV galaxy luminosity function at z=3-5 from the CFHT Legacy Survey Deep fields
• Supermassive Black Holes from Ultra-Strongly Self-Interacting Dark Matter
• The DEEP2 galaxy redshift survey: the evolution of the blue fraction in groups and the field
• Mergers, AGN, and 'Normal' Galaxies: Contributions to the Distribution of Star Formation Rates and Infrared Luminosity Functions
• Balance among gravitational instability, star formation, and accretion determines the structure and evolution of disk galaxies
• N-body simulations of gravitational dynamics
• SDSS DR7 superclusters. The catalogues
• Indirect and direct search for dark matter
• From galactic bars to the Hubble tension: weighing up the astrophysical evidence for Milgromian gravity
• How do central and satellite galaxies quench? -- Insights from spatially resolved spectroscopy in the MaNGA survey
• The Extended Virgo Cluster Catalog
• Implementation and performance of FDPS: A Framework Developing Parallel Particle Simulation Codes
• The Different Physical Mechanisms that Drive the Star-Formation Histories of Giant and Dwarf Galaxies
• Cosmological Constraints from Galaxy Clustering and the Mass-to-Number Ratio of Galaxy Clusters
• One simulation to fit them all - changing the background parameters of a cosmological N-body simulation
• Observational Searches for Galaxies at z > 6
• A new measurement of the evolving near-infrared galaxy luminosity function out to z~4: a continuing challenge to theoretical models of galaxy formation
• The MOSDEF survey: a stellar mass-SFR-metallicity relation exists at $z\sim 2.3$
• ELUCID - Exploring the Local Universe with reConstructed Initial Density field III: Constrained Simulation in the SDSS Volume
• Science with the TianQin observatory: Preliminary results on massive black hole binaries
• The origin of scatter in the stellar mass - halo mass relation of central galaxies in the EAGLE simulation
• The Luminosity Dependence of the Galaxy Merger Rate
• Toward Unbiased Galaxy Cluster Masses from Line of Sight Velocity Dispersions
• The population of Milky Way satellites in the LambdaCDM cosmology
• The impact of baryons on the spins and shapes of dark matter haloes
• Evolution in the Halo Masses of Isolated Galaxies between z~1 and z~0: From DEEP2 to SDSS
• Binary Quasars at High Redshift I: 24 New Quasar Pairs at z ~ 3-4
• Supermassive black holes do not correlate with dark matter halos of galaxies
• The Extraordinary Amount of Substructure in the Hubble Frontier Fields Cluster Abell 2744
• The evolution of the mass-size relation for early type galaxies from z~1 to the present: dependence on environment, mass-range and detailed morphology
• SHARDS: an optical spectro-photometric survey of distant galaxies
• Satellite abundances around bright isolated galaxies
• The SAURON project - XV. Modes of star formation in early-type galaxies and the evolution of the red sequence
• A hybrid model for the evolution of galaxies and Active Galactic Nuclei in the infrared
• Synthetic Galaxy Images and Spectra from the Illustris Simulation
• NIHAO XV: The environmental impact of the host galaxy on galactic satellite and field dwarf galaxies
• Analytical properties of Einasto dark matter haloes
• The Impact of Assembly Bias on the Galaxy Content of Dark Matter Halos
• Are galactic star formation and quenching governed by local, global or environmental phenomena?
• LoCuSS: The steady decline and slow quenching of star formation in cluster galaxies over the last four billion years
• Outskirts of Galaxy Clusters
• First Light And Reionisation Epoch Simulations (FLARES) I: Environmental Dependence of High-Redshift Galaxy Evolution
• Evolution in the black hole mass-bulge mass relation: a theoretical perspective
• The Cosmic Web: Geometric Analysis
• A snapshot on galaxy evolution occurring in the Great Wall: the role of Nurture at z=0
• Characterization and history of the Helmi streams with Gaia DR2
• Multimessenger astronomy with pulsar timing and X-ray observations of massive black hole binaries
• Galaxy Mergers and Dark Matter Halo Mergers in LCDM: Mass, Redshift, and Mass-Ratio Dependence
• Combining Lens Distortion and Depletion to Map the Mass Distribution of A1689
• The distribution of atomic hydrogen in EAGLE galaxies: morphologies, profiles, and HI holes
• Substructure of the galaxy clusters in the REXCESS sample: observed statistics and comparison to numerical simulations
• Moving mesh cosmology: characteristics of galaxies and haloes
• Environmental Dependence of Dark Matter Halo Growth I: Halo Merger Rates
• An accurate tool for the fast generation of dark matter halo catalogs
• The clustering of narrow-line AGN in the local Universe
• HBT+: an improved code for finding subhalos and building merger trees in cosmological simulations
• BLAST: Correlations in the Cosmic Far-Infrared Background at 250, 350, and 500 microns Reveal Clustering of Star-Forming Galaxies
• Galactic outflow rates in the EAGLE simulations
• High-precision predictions for the acoustic scale in the non-linear regime
• A close-pair binary in a distant triple supermassive black-hole system
• Stellar velocity profiles and line strengths out to four effective radii in the early-type galaxies NGC 3379 and NGC 821
• The dark matter halos of dwarf galaxies: a challenge for the LCDM paradigm?
• Dark-ages reionization and galaxy formation simulation - III. Modelling galaxy formation and the epoch of reionization
• Confronting theoretical models with the observed evolution of the galaxy population out to z=4
• The nature of the Diffuse Gamma-Ray Background
• A Universe of Ultra-Diffuse Galaxies: Theoretical Predictions from $\Lambda$CDM Simulations
• The effects of environment on morphological evolution between 0<z<1.2 in the COSMOS Survey
• On the Origin of Cores in Simulated Galaxy Clusters
• Relative merits of different types of rest-frame optical observations to constrain galaxy physical parameters
• Heavily Obscured Quasar Host Galaxies at z~2 are Disks, Not Major Mergers
• Galaxy Zoo: The Environmental Dependence of Bars and Bulges in Disc Galaxies
• Resolving the Discrepancy of Galaxy Merger Fraction Measurements at z ~ 0 - 3
• Ages of Type Ia Supernovae Over Cosmic Time
• The density field of the 10k zCOSMOS galaxies
• The flip-side of galaxy formation: A combined model of Galaxy Formation and Cluster Heating
• Baryonic impact on the dark matter distribution in Milky Way-size galaxies and their satellites
• The origin of the diverse morphologies and kinematics of Milky Way-mass galaxies in the FIRE-2 simulations
• The mass of our Milky Way
• A Comparative Study of Density Field Estimation for Galaxies: New Insights into the Evolution of Galaxies with Environment in COSMOS out to z~3
• Assembly bias and the dynamical structure of dark matter halos
• Do submillimeter galaxies really trace the most massive dark matter halos? Discovery of a high-z cluster in a highly active phase of evolution
• An optical group catalogue to z = 1 from the zCOSMOS 10k sample
• Galaxies in SDSS and DEEP2: a quiet life on the blue sequence?
• Where do Wet, Dry, and Mixed Galaxy Mergers Occur? A Study of the Environments of Close Galaxy Pairs in the DEEP2 Galaxy Redshift Survey
• Sensitivity Projections for Dark Matter Searches with the Fermi Large Area Telescope
• Cluster Galaxies Die Hard
• Merger Rates of Dark-Matter Haloes
• The Properties of Galaxies in Voids
• Simulating the Bullet Cluster
• Evidence for a change in the dominant satellite galaxy quenching mechanism at z=1
• The Parameter Space of Galaxy Formation
• The halo merger rate in the Millennium Simulation and implications for observed galaxy merger fractions
• The impact of galactic properties and environment on the quenching of central and satellite galaxies: A comparison between SDSS, Illustris and L-Galaxies
• Modeling Nonlinear Evolution of Baryon Acoustic Oscillations: Convergence Regime of N-body Simulations and Analytic Models
• The Hierarchical Structure and Dynamics of Voids
• Massive star formation in Wolf-Rayet galaxies. IV: Colours, chemical composition analysis and metallicity-luminosity relations
• The environment of bright QSOs at z ~ 6: Star forming galaxies and X-ray emission
• Cluster Mass Calibration at High Redshift: HST Weak Lensing Analysis of 13 Distant Galaxy Clusters from the South Pole Telescope Sunyaev-Zel'dovich Survey
• (Mis-)Interpreting supernovae observations in a lumpy universe
• Planes of satellite galaxies and the cosmic web
• Cluster number counts dependence on dark energy inhomogeneities and coupling to dark matter
• The evolution of the brightest cluster galaxies since z~1 from the ESO Distant Cluster Survey (EDisCS)
• The first generation of stars in LCDM cosmology
• Reionization and galaxy inference from the high-redshift Lyα forest
• Detecting Effects of Filaments on Galaxy Properties in the Sloan Digital Sky Survey III
• A Radio Census of Binary Supermassive Black Holes
• Connection between Newtonian simulations and general relativity
• Mismatch and Misalignment: Dark Haloes and Satellites of Disc Galaxies
• Modeling the cosmological co-evolution of supermassive black holes and galaxies: I. BH scaling relations and the AGN luminosity function
• Where will supersymmetric dark matter first be seen?
• What is the largest Einstein radius in the universe?
• Sussing Merger Trees: The Merger Trees Comparison Project
• Second-order Lagrangian perturbation theory initial conditions for resimulations
• Galaxy And Mass Assembly (GAMA): The large scale structure of galaxies and comparison to mock universes
• Observational constraints on the redshift evolution of X-ray scaling relations of galaxy clusters out to z ~ 1.5
• Orbital structure of merger remnants: Trends with gas fraction in 1:1 mergers
• L-GALAXIES 2020: Spatially resolved cold gas phases, star formation and chemical enrichment in galactic discs
• The environmental dependence of the stellar mass function at z~1: Comparing cluster and field between the GCLASS and UltraVISTA surveys
• Moving Mesh Cosmology: Properties of Gas Disks
• UV-to-FIR analysis of Spitzer/IRAC sources in the Extended Groth Strip II: Photometric redshifts, Stellar masses and Star formation rates
• The metallicity bimodality of globular cluster systems: a test of galaxy assembly and of the evolution of the galaxy mass-metallicity relation
• Lyman break galaxies, Lya emitters and a radio galaxy in a protocluster at z=4.1
• A consistent measure of the merger histories of massive galaxies using close-pair statistics I: Major mergers at $z<3.5$
• The Energetics and Lifetimes of Local Radio Active Galactic Nuclei
• Strongly lensed repeating Fast Radio Bursts as precision probes of the universe
• A Runaway Black Hole in COSMOS: Gravitational Wave or Slingshot Recoil?
• Hubble Space Telescope Weak-lensing Study of the Galaxy Cluster XMMU J2235.3-2557 at z=1.4: A Surprisingly Massive Galaxy Cluster when the Universe is One-third of its Current Age
• The Halo Mass Function from Excursion Set Theory. II. The Diffusing Barrier
• The Dark Universe
• The Impossibly Early Galaxy Problem
• The Dependence of the Mass Assembly History of Cold Dark Matter Halos on Environment
• Cosmic Voids: structure, dynamics and galaxies
• Simulating nonlinear cosmological structure formation with massive neutrinos
• The Mean and Scatter of the Velocity Dispersion-Optical Richness Relation for maxBCG Galaxy Clusters
• Constructing Merger Trees that Mimic N-Body Simulations
• Modeling the Formation of Globular Cluster Systems in the Virgo Cluster
• The Substructure Hierarchy in Dark Matter Haloes
• Galaxy morphology in the LambdaCDM cosmology
• H0LiCOW III. Quantifying the effect of mass along the line of sight to the gravitational lens HE 0435-1223 through weighted galaxy counts
• Black Hole Mass Scaling Relations for Early-Type Galaxies: $M_{BH}$-$M_{\ast ,sph}$ and $M_{BH}$-$M_{\ast ,gal}$
• Early structure in LCDM
• Cosmic Web and Star Formation Activity in Galaxies at z~1
• The fine-grained phase-space structure of Cold Dark Matter halos
• Rotation Curves in z~1-2 Star-Forming Disks: Evidence for Cored Dark Matter Distributions
• The Dependence of Galaxy Formation on Cosmological Parameters: Can we distinguish the WMAP1 and WMAP3 Parameter Sets?
• Gas-rich mergers and feedback are ubiqitous amongst starbursting radio galaxies, as revealed by JVLA, IRAM PdBI and Herschel
• Mergers, Starbursts, and Quenching in the Simba Simulation
• A Quantification of the Butterfly Effect in Cosmological Simulations and Implications for Galaxy Scaling Relations
• H0LiCOW XII. Lens mass model of WFI2033-4723 and blind measurement of its time-delay distance and $H_0$
• The XMM Cluster Survey: The build up of stellar mass in Brightest Cluster Galaxies at high redshift
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). A precise measurement of the galaxy stellar mass function and the abundance of massive galaxies at redshifts 0.5<z<1.3
• Angular momentum properties of haloes and their baryon content in the Illustris simulation
• Size and velocity-dispersion evolution of early-type galaxies in a Lambda cold dark matter universe
• MOIRCS Deep Survey IV: Evolution of Galaxy Stellar Mass Function Back to z ~ 3
• eLISA: Astrophysics and cosmology in the millihertz regime
• Towards a Holistic View of the Heating and Cooling of the Intracluster Medium
• Observational constraints on inhomogeneous cosmological models without dark energy
• The Fate of Substructures in Cold Dark Matter Haloes
• The Impact of Modeling Assumptions in Galactic Chemical Evolution Models
• Cluster Density Profiles as a Test of Modified Gravity
• The KBC void and Hubble tension contradict $\Lambda$CDM on a Gpc scale $-$ Milgromian dynamics as a possible solution
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Motivation, Design and Target Catalogue
• The IMACS Cluster Building Survey: II. Spectral Evolution of Galaxies in the Epoch of Cluster Assembly
• From voids to filaments: environmental transformations of galaxies in the SDSS
• Modelling Element Abundances in Semi-analytic Models of Galaxy Formation
• Localizing merging black holes with sub-arcsecond precision using gravitational-wave lensing
• Clues on void evolution II: Measuring density and velocity profiles on SDSS galaxy redshift space distortions
• Approximate Bayesian Computation for Astronomical Model Analysis: A Case Study in Galaxy Demographics and Morphological Transformation at High Redshift
• Dissecting the Red Sequence - III. Mass-to-Light Variations in 3D Fundamental Plane Space
• Galaxy formation in the Planck Millennium: the atomic hydrogen content of dark matter halos
• The effects of baryons on the halo mass function
• Gas Infall and Stochastic Star Formation in Galaxies in the Local Universe
• The Properties of Sub-mm Galaxies in Hierarchical Models
• Bullet Cluster: A Challenge to LCDM Cosmology
• Constraining the primordial initial mass function with stellar archaeology
• A Comparison between Semi-Analytic Model Predictions for the CANDELS Survey
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Luminosity and stellar mass dependence of galaxy clustering at 0.5<z<1.1
• Cosmic ray-driven galactic winds: streaming or diffusion?
• The stellar accretion origin of stellar population gradients in massive galaxies at large radii
• Insights on the astrophysics of supermassive black hole binaries from pulsar timing observations
• Asymmetries in the inner regions of LCDM haloes
• The Initial Conditions of the Universe from Constrained Simulations
• Halo masses for optically-selected and for radio-loud AGN from clustering and galaxy-galaxy lensing
• The Environments of Active Galactic Nuclei within the zCOSMOS Density Field
• UNCOVERing the extended strong lensing structures of Abell 2744 with the deepest JWST imaging
• Host galaxy morphologies of X-ray selected AGN: assessing the significance of different black hole fueling mechanisms to the accretion density of the Universe at z~1
• Dependence of cosmic shear covariances on cosmology - Impact on parameter estimation
• Variation of galactic cold gas reservoirs with stellar mass
• Modelling the number density of Halpha emitters for future spectroscopic near-IR space missions
• Pre-Processing and Post-Processing in Group-Cluster Mergers
• The zCOSMOS 20k Group Catalog
• The radial distribution of galaxies in groups and clusters
• The Cosmic Decline in the H2/HI-Ratio in Galaxies
• Probability Distribution Functions of Cosmological Lensing: Convergence, Shear, and Magnification
• The survival of dark matter halos in the cluster Cl0024+16
• Disentangling galaxy environment and host halo mass
• Growth rate of cosmological perturbations at z ~ 0.1 from a new observational test
• Contribution of stripped nuclear clusters to globular cluster and ultra-compact dwarf galaxy populations
• Galaxy Kinematics with VIRUS-P: The Dark Matter Halo of M87
• The Angular Clustering of Distant Galaxy Clusters
• On the puzzling plateau in the specific star formation rate at z=2-7
• On Detecting Halo Assembly Bias with Galaxy Populations
• Galaxy environment in the 3D-HST fields. Witnessing the onset of satellite quenching at z ~ 1-2
• Predictions for the Angular Dependence of Gas Mass Flow Rate and Metallicity in the Circumgalactic Medium
• LoCuSS: The mid-infrared Butcher-Oemler effect
• Limits on Pop III star formation with the most iron-poor stars
• Void Statistics in Large Galaxy Redshift Surveys: Does Halo Occupation of Field Galaxies Depend on Environment?
• The stellar velocity dispersion of a compact massive galaxy at z=1.80 using X-Shooter: confirmation of the evolution in the mass-size and mass-dispersion relations
• The effects of cosmic rays on the formation of Milky Way-mass galaxies in a cosmological context
• Breaking the Degeneracies Between Cosmology and Galaxy Bias
• The spatial clustering of X-ray selected AGN in the XMM-COSMOS field
• Particle Production During Inflation: Observational Constraints and Signatures
• Star Formation and Metallicity Gradients in Semi-analytic Models of Disk Galaxy Formation
• The cosmic history of the spin of dark matter haloes within the large scale structure
• Large scale opacity fluctuations in the Lyman alpha forest: evidence for QSOs dominating the ionising UV background at z ~ 5.5-6 ?
• The Dynamical State and Mass-Concentration Relation of Galaxy Clusters
• Constraints on cosmic hemispherical power anomalies from quasars
• The dynamical state of brightest cluster galaxies and the formation of clusters
• On the radiative efficiencies, Eddington ratios, and duty cycles of luminous high-redshift quasars
• SWIFT: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications
• HerMES: ALMA Imaging of Herschel-selected Dusty Star-forming Galaxies
• The Environments of High Redshift QSOs
• Measuring the Average Evolution of Luminous Galaxies at z<3: The Rest-frame Optical Luminosity Density, Spectral Energy Distribution, and Stellar Mass Density
• Pre-processing of galaxies in cosmic filaments around AMASCFI clusters in the CFHTLS
• The Copernicus Complexio: a high-resolution view of the small-scale Universe
• LCDM predictions for galaxy protoclusters I: the relation between galaxies, protoclusters and quasars at z~6
• In a hot bubble: why does superbubble feedback work, but isolated supernovae do not?
• Fractal Dimension as a measure of the scale of Homogeneity
• Modeling the cosmological co-evolution of supermassive black holes and galaxies: II. The clustering of quasars and their dark environment
• The evolution of dust-obscured star formation activity in galaxy clusters relative to the field over the last 9 billion years
• Cosmographic Constraints and Cosmic Fluids
• Galaxy evolution in the infra-red: comparison of a hierarchical galaxy formation model with SPITZER data
• Superclusters of galaxies from the 2dF redshift survey. I. The catalogue
• Is Main Sequence Galaxy Star Formation Controlled by Halo Mass Accretion?
• Probing cluster formation under extreme conditions: massive star clusters in blue compact galaxies
• The Outer Rim Simulation: A Path to Many-Core Supercomputers
• Galaxy Formation with BECDM -- II. Cosmic Filaments and First Galaxies
• The impact of baryons on massive galaxy clusters: halo structure and cluster mass estimates
• The real-space clustering of luminous red galaxies around z<0.6 quasars in the Sloan Digital Sky Survey
• How is Star Formation Quenched in Massive Galaxies?
• The Growth Efficiency of High-Redshift Black Holes
• The Mass Assembly of Fossil Groups of Galaxies in the Millennium Simulation
• Star Formation and AGN Activity in Galaxy Clusters from $z=1-2$: a Multi-wavelength Analysis Featuring $Herschel$/PACS
• The environmental dependence of HI in galaxies in the EAGLE simulations
• Black Hole Mass Scaling Relations for Spiral Galaxies. I. $M_{\mathrm{BH}}$-$M_{\ast ,\mathrm{sph}}$
• Reconstructing the Cosmic Velocity and Tidal Fields with Galaxy Groups Selected from the Sloan Digital Sky Survey
• The WiggleZ Dark Energy Survey: High Resolution Kinematics of Luminous Star-Forming Galaxies
• Discovery of a rich proto-cluster at z=2.9 and associated diffuse cold gas in the VIMOS Ultra-Deep Survey (VUDS)
• The XXL Survey III. Luminosity-temperature relation of the Bright Cluster Sample
• Building disc structure and galaxy properties through angular momentum: The DARK SAGE semi-analytic model
• MOSFIRE Spectroscopy of Quiescent Galaxies at 1.5 < z < 2.5. I - Evolution of Structural and Dynamical Properties
• An Extremely Massive Quiescent Galaxy at $z=3.493$: Evidence of Insufficiently Rapid Quenching Mechanisms in Theoretical Models
• An uncertainty principle for star formation - II. A new method for characterising the cloud-scale physics of star formation and feedback across cosmic history
• Dynamics of the Magellanic Clouds in a LCDM Universe
• Dark Matter Halo Growth II: Diffuse Accretion and its Environmental Dependence
• Does a 'stochastic' background of gravitational waves exist in the pulsar timing band?
• A Periodically Varying Luminous Quasar at z=2 from the Pan-STARRS1 Medium Deep Survey: A Candidate Supermassive Black Hole Binary in the Gravitational Wave-Driven Regime
• Prospects for gravitational-wave detection and supermassive black hole astrophysics with pulsar timing arrays
• A new approach to simulating collisionless dark matter fluids
• The low-end of the black hole mass function at cosmic dawn
• Unravelling the complex structure of AGN-driven outflows: I. Kinematics and sizes
• Baryon acoustic signature in the clustering of density maxima
• Strong lensing optical depths in a LCDM universe II: the influence of the stellar mass in galaxies
• Evolution in the H I Gas Content of Galaxy Groups: Pre-Processing and Mass Assembly in the Current Epoch
• The Beginning and Evolution of the Universe
• Weak lensing from space: first cosmological constraints from three-point shear statistics
• Detecting and Characterizing Young Quasars I: Systemic Redshifts and Proximity Zones Measurements
• Cosmic shear covariance: The log-normal approximation
• Revealing the galaxy-halo connection in IllustrisTNG
• The Growth in Size and Mass of Cluster Galaxies since z=2
• Gone after one orbit: How cluster environments quench galaxies
• Quiescence correlates strongly with directly-measured black hole mass in central galaxies
• Interactions between multiple supermassive black holes in galactic nuclei: a solution to the final parsec problem
• The Fossil Phase in the Life of a Galaxy Group
• Weak Lensing by Galaxies in Groups and Clusters: I.--Theoretical Expectations
• Hunting for Galaxies and Halos in simulations with VELOCIraptor
• The alignment of satellite galaxies and cosmic filaments: observations and simulations
• The Splashback Feature around DES Galaxy Clusters: Galaxy Density and Weak Lensing Profiles
• Measuring the cosmic evolution of dark energy with baryonic oscillations in the galaxy power spectrum
• The clustering of H-alpha emitters at z=2.23 from HiZELS
• Intensity Mapping of Lyman-alpha Emission During the Epoch of Reionization
• Tidal debris morphology and the orbits of satellite galaxies
• Primordial blackholes and gravitational waves for an inflection-point model of inflation
• Constraints on the properties of warm dark matter using the satellite galaxies of the Milky Way
• Insight Into the Formation of the Milky Way Through Cold Halo Substructure. I. The ECHOS of Milky Way Formation
• Spinning dark matter halos promote bar formation
• Planck Intermediate Results. XI: The gas content of dark matter halos: the Sunyaev-Zeldovich-stellar mass relation for locally brightest galaxies
• Was Star-Formation Suppressed in High-Redshift Minihalos?
• Density split statistics: joint model of counts and lensing in cells
• The Luminosity Dependence of Quasar Clustering
• The zCOSMOS Survey. The dependence of clustering on luminosity and stellar mass at z=0.2-1
• MusE GAs FLOw and Wind (MEGAFLOW) I: First MUSE results on background quasars
• Recovering Redshift Distributions with Cross-Correlations: Pushing The Boundaries
• Universal fitting formulae for baryon oscillation surveys
• Numerical convergence of simulations of galaxy formation: the abundance and internal structure of cold dark matter haloes
• Elemental Abundances in Milky Way-like Galaxies from a Hierarchical Galaxy Formation Model
• A spectroscopic survey of dwarf galaxies in the Coma Cluster: Stellar populations, environment and downsizing
• Environmental quenching and hierarchical cluster assembly: Evidence from spectroscopic ages of red-sequence galaxies in Coma
• Compact groups in theory and practice - III. Compact groups of galaxies in the Sixth Data Release of the Sloan Digital Sky Survey
• The Three Hundred Project: Backsplash galaxies in simulations of clusters
• Clustering of Lyman Break Galaxies at z=4 and 5 in The Subaru Deep Field: Luminosity Dependence of The Correlation Function Slope
• Cosmological Simulations of Early Blackhole Formation: Halo Mergers, Tidal Disruption, and the Conditions for Direct Collapse
• Studying the emergence of the red sequence through galaxy clustering: host halo masses at z > 2
• The Horizon Run N-body Simulation: Baryon Acoustic Oscillations and Topology of Large Scale Structure of the Universe
• Spectroscopic Confirmation of a Protocluster at $z=3.37$ with a High Fraction of Quiescent Galaxies
• The Gas Consumption History to z ~ 4
• The Influence of Large-Scale Structure on Halo Shapes and Alignments
• The Accuracy of Subhalo Detection
• Mock weak lensing analysis of simulated galaxy clusters: bias and scatter in mass and concentration
• Physical properties underlying observed kinematics of satellite galaxies
• Supermassive Black Holes in the Hierarchical Universe: A General Framework and Observational Tests
• Detailed dust modelling in the L-Galaxies semi-analytic model of galaxy formation
• The scale of homogeneity of the galaxy distribution in SDSS DR6
• Milky Way Mass and Potential Recovery Using Tidal Streams in a Realistic Halo
• The statistics of the subhalo abundance of dark matter haloes
• A Virtual Sky with Extragalactic HI and CO Lines for the SKA and ALMA
• A Systematic Survey of Protoclusters at $z\sim 3-6$ in the CFHTLS Deep Fields
• Non-Baryonic Dark Matter in Cosmology
• Timing the formation and assembly of early-type galaxies via spatially resolved stellar populations analysis
• PRECESSION: Dynamics of spinning black-hole binaries with python
• A dormant, overmassive black hole in the early Universe
• SEREN - A new SPH code for star and planet formation simulations
• Perturbation Theory Reloaded II: Non-linear Bias, Baryon Acoustic Oscillations and Millennium Simulation In Real Space
• The First Stars in The Universe
• Effects of large-scale structure on the accuracy of weak lensing mass measurements
• Panchromatic Hubble Andromeda Treasury XVIII. The High-mass Truncation of the Star Cluster Mass Function
• A giant elliptical galaxy with a lightweight initial mass function
• A simple model to link the properties of quasars to the properties of dark matter halos out to high redshift
• The Void Phenomenon Explained
• A fully cosmological model of a Monoceros-like ring
• First test of Verlinde's theory of Emergent Gravity using Weak Gravitational Lensing measurements
• Alignment between galaxies and large-scale structure
• Correcting the z~8 Galaxy Luminosity Function for Gravitational Lensing Magnification Bias
• The route to massive black hole formation via merger-driven direct collapse: a review
• Clues on void evolution I: Large scale galaxy distributions around voids
• The New Horizon Run Cosmological N-Body Simulations
• Galaxy-galaxy lensing constraints on the relation between baryons and dark matter in galaxies in the Red Sequence Cluster Survey 2
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Environmental effects shaping the galaxy stellar mass function
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Luminosity and Color Dependence and Redshift Evolution
• The Stacked Thermal SZ Signal of Locally Brightest Galaxies in Planck Full Mission Data: Evidence for Galaxy Feedback?
• The effect of metal enrichment and galactic winds on galaxy formation in cosmological zoom simulations
• General Relativistic N-body simulations in the weak field limit
• Discovery of a protocluster at z~6
• Black Holes in the Early Universe
• First Light And Reionisation Epoch Simulations (FLARES) II: The Photometric Properties of High-Redshift Galaxies
• Galaxy and Mass Assembly (GAMA): Fine filaments of galaxies detected within voids
• A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): JWST Reveals a Filamentary Structure around a z=6.61 Quasar
• The formation of massive, quiescent galaxies at cosmic noon
• Simulated observations of sub-millimetre galaxies: the impact of single-dish resolution and field variance
• The Largest Gravitational Lens: MACS J0717.5+3745 (z=0.546)
• The mass assembly of galaxy groups and the evolution of the magnitude gap
• The SPLASH Survey: A Spectroscopic Portrait of Andromeda's Giant Southern Stream
• Binary super-massive black hole environments diminish the gravitational-wave signal in the pulsar timing band
• Extending cosmological tests of General Relativity with the Square Kilometre Array
• Triplets of supermassive black holes: Astrophysics, Gravitational Waves and Detection
• Intrinsic galaxy shapes and alignments II: Modelling the intrinsic alignment contamination of weak lensing surveys
• The Challenge of the Largest Structures in the Universe to Cosmology
• The satellites of the Milky Way - Insights from semi-analytic modelling in a LambdaCDM cosmology
• Reconstructing the cosmic density field with the distribution of dark matter halos
• The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos
• \textsc{CompaSO}: A new halo finder for competitive assignment to spherical overdensities
• Gravitational Anomalies in the Solar System?
• Probing the stability of superheavy dark matter particles with high-energy neutrinos
• H${}_2$-based star formation laws in hierarchical models of galaxy formation
• What is the (Dark) Matter with Dwarf Galaxies?
• Gravitational waves and stalled satellites from massive galaxy mergers at z <= 1
• The Halo Mass Function from Excursion Set Theory. III. Non-Gaussian Fluctuations
• The Hot Interstellar Medium of Normal Elliptical Galaxies. I. A Chandra Gas Gallery and Comparison of X-ray and Optical Morphology
• Reconstructing the Initial Density Field of the Local Universe: Method and Test with Mock Catalogs
• Detecting the integrated Sachs-Wolfe effect with stacked voids
• Origin of strong magnetic fields in Milky-Way like galactic haloes
• The most luminous quasars do not live in the most massive dark matter haloes at any redshift
• The Gemini Deep Deep Survey: VIII. When Did Early-type Galaxies Form?
• Galaxy and Mass Assembly (GAMA): The halo mass of galaxy groups from maximum-likelihood weak lensing
• keV Sterile Neutrino Dark Matter from Singlet Scalar Decays: The Most General Case
• The kinematics of ionized gas in Lyman-Break Analogs at z ~ 0.2
• AMICO: optimised detection of galaxy clusters in photometric surveys
• On the Assembly of Dwarf Galaxies in Clusters and their Efficient Formation of Globular Clusters
• Galaxy Cluster Mass Reconstruction Project: I. Methods and first results on galaxy-based techniques
• Surveying Galaxy Proto-clusters in Emission: A Large-scale Structure at z=2.44 and the Outlook for HETDEX
• Late-stage galaxy mergers in COSMOS to z~1
• Coming of Age in the Dark Sector: How Dark Matter Haloes grow their Gravitational Potential Wells
• Modelling and interpreting the dependence of clustering on the spectral energy distributions of galaxies
• The Taipan Galaxy Survey: Scientific Goals and Observing Strategy
• Constraining the Dark Energy Equation of State with Cosmic Voids
• Improving the precision of time-delay cosmography with observations of galaxies along the line of sight
• Assembly Bias and Splashback in Galaxy Clusters
• Anisotropies in the astrophysical gravitational-wave background: Predictions for the detection of compact binaries by LIGO and Virgo
• The VIMOS-VLT Deep Survey - The evolution of galaxy clustering per spectral type to z~1.5
• Which galaxies dominate the neutral gas content of the Universe?
• Cosmological performance of SKA HI galaxy surveys
• Spatially resolved kinematics and stellar populations of brightest cluster and group galaxies
• Statistics of Voids in the 2dF Galaxy Redshift Survey
• The rise and fall of the star formation histories of blue galaxies at redshifts 0.2<z<1.4
• Satellite abundances around bright isolated galaxies II: radial distribution and environmental effects
• Discovery of a large number of candidate proto-clusters traced by ~15 Mpc-scale galaxy overdensities in COSMOS
• Hidden in plain sight: a massive, dusty starburst in a galaxy protocluster at z=5.7 in the COSMOS field
• Chandra centres for COSMOS X-ray galaxy groups: Differences in stellar properties between central dominant and offset brightest group galaxies
• Clustering of Star-forming Galaxies Near a Radio Galaxy at z=5.2
• Environmental Dependence of Galaxy Merger Rate in ΛCDM Universe
• Galaxy formation in the Planck cosmology - IV. Mass and environmental quenching, conformity and clustering
• An adaptively refined phase-space element method for cosmological simulations and collisionless dynamics
• Testing the binary hypothesis: pulsar timing constraints on supermassive black hole binary candidates
• NIHAO-UHD: The properties of MW-like stellar disks in high resolution cosmological simulations
• Simulations of Baryon Oscillations
• Hiding in plain sight: An abundance of compact massive spheroids in the local Universe
• Integral Field Spectroscopy of 2.0<z<2.7 Sub-mm Galaxies; gas morphologies and kinematics
• LoCuSS: A Dynamical Analysis of X-ray AGN in Local Clusters
• Back to the Future: Estimating Initial Globular Cluster Masses from their Present Day Stellar Mass Functions
• On the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7<z<2.8
• Fast cold gas in hot AGN outflows
• Reconstructing the Near-IR Background Fluctuations from known Galaxy Populations using Multiband Measurements of Luminosity Functions
• MAHALO Deep Cluster Survey I. Accelerated and enhanced galaxy formation in the densest regions of a protocluster at z=2.5
• Evaporating the Milky Way halo and its satellites with inelastic self-interacting dark matter
• Gas and galaxies in filament between clusters of galaxies: The study of A399-A401
• The LSST DESC DC2 Simulated Sky Survey
• Discovery of the largest known lensed images formed by a critically convergent lensing cluster
• What does strong gravitational lensing? The mass and redshift distribution of high-magnification lenses
• Emerging spatial curvature can resolve the tension between high-redshift CMB and low-redshift distance ladder measurements of the Hubble constant
• Prediction of the Cosmic Evolution of the CO-Luminosity Functions
• Satellite Galaxies and Fossil Groups in the Millennium Simulation
• Incorporating interactive 3-dimensional graphics in astronomy research papers
• The Spitzer-HETDEX Exploratory Large-Area Survey
• Modeling the reconstructed BAO in Fourier space
• Dark Sky Simulations: Early Data Release
• Galaxy formation in semi-analytic models and cosmological hydrodynamic zoom simulations
• An Overdensity of Galaxies near the Most Distant Radio-Loud Quasar
• Log-normal star formation histories in simulated and observed galaxies
• Dissecting and Modelling Galaxy Assembly Bias
• Simulating Subhalos at High Redshift: Merger Rates, Counts, and Types
• Sunyaev-Zel'dovich clusters in Millennium Gas simulations
• Intrinsic galaxy shapes and alignments I: Measuring and modelling COSMOS intrinsic galaxy ellipticities
• Neutron star mergers and rare core-collapse supernovae as sources of r-process enrichment in simulated galaxies
• Ultra-diffuse galaxies in the Auriga simulations
• Are mergers responsible for universal halo properties?
• Baryon oscillations
• Monte Carlo Markov Chain Parameter Estimation in Semi-Analytic Models of Galaxy Formation
• Merger-Induced Metallicity Dilution in Cosmological Galaxy Formation Simulations
• Radial distribution of stars, gas and dust in SINGS galaxies. III. Modeling the evolution of the stellar component in galaxy disks
• On the formation of the first quasars
• Formation of galactic nuclei with multiple supermassive black holes at high redshifts
• Direct detection of self-interacting dark matter
• A dynamical model of supernova feedback: gas outflows from the interstellar medium
• Simulations of the formation and evolution of isolated dwarf galaxies
• Environmental dependence in the ellipsoidal collapse model
• Super-Sample Signal
• Modelling Shock Heating in Cluster Mergers: I. Moving Beyond the Spherical Accretion Model
• Stellar Kinematics and Structural Properties of Virgo Cluster Dwarf Early-Type Galaxies from the SMAKCED Project III. Rotation versus Pressure Support
• Star Cluster Formation in Cosmological Simulations. II. Effects of Star Formation Efficiency and Stellar Feedback
• Determining the full satellite population of a Milky Way-mass halo in a highly resolved cosmological hydrodynamic simulation
• The primordial environment of super massive black holes: large scale galaxy overdensities around $z\sim 6$ QSOs with LBT
• Substructure in lensing clusters and simulations
• How common is the Milky Way - satellite system alignment?
• The optically unbiased GRB host (TOUGH) survey. VI. Radio observations at z<1 and consistency with typical star-forming galaxies
• Star formation in extremely faint dwarf galaxies
• Dwarf galaxy populations in present-day galaxy clusters: I. Abundances and red fractions
• Tracing Galaxies Through Cosmic Time with Number Density Selection
• The Effect of Gas Physics on the Halo Mass Function
• The orientation of galaxy dark matter haloes around cosmic voids
• Electromagnetic counterparts of supermassive black hole binaries resolved by pulsar timing arrays
• Constraints on the missing baryons from the kinetic Sunyaev-Zeldovich effect in Planck data
• Dark Matter Halos of Disk Galaxies: Constraints from the Tully-Fisher Relation
• Baryon Dynamics, Dark Matter Substructure, and Galaxies
• Status, Challenges and Directions in Indirect Dark Matter Searches
• An analysis of the evolving comoving number density of galaxies in hydrodynamical simulations
• The origin of the atomic and molecular gas contents of early-type galaxies. I. A new test of galaxy formation physics
• The Overdense Environment of a Large Lyman-alpha Nebula at z~2.7
• How Rare is the Bullet Cluster?
• Dark matter scaling relations and the assembly epoch of Coma early-type galaxies
• Clustering properties of BzK-selected galaxies in GOODS-N: environmental quenching and triggering of star formation at z ~ 2
• Anisotropic Locations of Satellite Galaxies: Clues to the Orientations of Galaxies within their Dark Matter Halos
• Cosmological perturbation theory in 1+1 dimensions
• Understanding black hole mass assembly via accretion and mergers at late times in cosmological simulations
• The Role of Dust in the Early Universe I : Protogalaxy Evolution
• Reconstructing the Lensing Mass in the Universe from Photometric Catalogue Data
• The role of dry mergers for the formation and evolution of brightest cluster galaxies
• The integrated Sachs-Wolfe imprints of cosmic superstructures: a problem for ΛCDM
• High-Redshift Star Formation in a Time-Dependent Lyman-Werner Background
• Detection of galaxy assembly bias
• The Spatial Distribution of Galactic Satellites in the LCDM Cosmology
• The galaxy environment of a QSO at z ~ 5.7
• On the impact of baryons on the halo mass function, bias, and cluster cosmology
• The MillenniumTNG Project: High-precision predictions for matter clustering and halo statistics
• Galaxy Cluster Mass Estimation from Stacked Spectroscopic Analysis
• Schrödinger method as N-body double and UV completion of dust
• A New Force in the Dark Sector?
• The Stellar Mass Growth of Brightest Cluster Galaxies in the IRAC Shallow Cluster Survey
• Void Ellipticity Distribution as a Probe of Cosmology
• MAGIICAT III. Interpreting Self-Similarity of the Circumgalactic Medium with Virial Mass using MgII Absorption
• Galaxy Zoo: Bulgeless Galaxies With Growing Black Holes
• Ram pressure stripping in a galaxy formation model. I. A novel numerical approach
• NIHAO X: Reconciling the local galaxy velocity function with Cold Dark Matter via mock HI observations
• The Effects of Environment on the Evolution of the Galaxy Stellar Mass Function
• Luminosity dependence of the spatial and velocity distributions of galaxies: Semi-analytic models versus the Sloan Digital Sky Survey
• Massive black hole seeds born via direct gas collapse in galaxy mergers: their properties, statistics and environment
• Dwarf Galaxies in CDM, WDM, and SIDM: Disentangling Baryons and Dark Matter Physics
• The Halo Occupation Distribution of SDSS Quasars
• Full-sky map of the ISW and Rees-Sciama effect from Gpc simulations
• The evolving relation between star-formation rate and stellar mass in the VIDEO Survey since $z=3$
• Dust scaling relations in a cosmological simulation
• Cosmological Simulations for Combined-Probe Analyses: Covariance and Neighbour-Exclusion Bias
• Search for extended gamma-ray emission from the Virgo galaxy cluster with Fermi-LAT
• A Large Number of z > 6 Galaxies around a QSO at z = 6.43: Evidence for a Protocluster?
• Alignments of Voids in the Cosmic Web
• How robust are predictions of galaxy clustering?
• The Evolution of Assembly Bias
• The evolution of Lyman-break galaxies in CDM
• MAHALO Deep Cluster Survey II. Characterizing massive forming galaxies in the Spiderweb protocluster at z=2.2
• The Density and Pseudo-Phase-Space Density Profiles of CDM halos
• Cosmic Cartography of the Large-Scale Structure with Sloan Digital Sky Survey Data Release 6
• The diverse dark matter density at sub-kiloparsec scales in Milky Way satellites:implications for the nature of dark matter
• Galaxy morphology, kinematics and clustering in a hydrodynamic simulation of a LambdaCDM universe
• The Varied Fates of z~2 Star-forming Galaxies
• An N-body/SPH Study of Isolated Galaxy Mass Density Profiles
• A Census of Stellar Mass in 10 Massive Haloes at z~1 from the GCLASS Survey
• How baryons affect halos and large-scale structure: a unified picture from the Simba simulation
• An early phase of environmental effects on galaxy properties unveiled by near-infrared spectroscopy of protocluster galaxies at z>2
• The SDSS-GALEX viewpoint of the truncated red sequence in field environments at z~0
• The Dynamical State of Dark Matter Haloes in Cosmological Simulations I: Correlations with Mass Assembly History
• The Gaia DR3 view of dynamical substructure in the stellar halo near the Sun
• The VIMOS VLT Deep Survey: the contribution of minor mergers to the growth of L_B >= L*_B galaxies since z ~ 1 from spectroscopically identified pairs
• A z=2.5 protocluster associated with the radio galaxy MRC 2104-242: star formation and differing mass functions in dense environments
• High Eccentricities and High Masses Characterize Gravitational-wave Captures in Galactic Nuclei as Seen by Earth-based Detectors
• The statistical properties of LCDM halo formation
• Properties of the galaxy population in hydrodynamical simulations of clusters
• Cold Filamentary Accretion and the Formation of Metal Poor Globular Clusters and Halo Stars
• Times, environments and channels of bulge formation in a LambdaCDM cosmology
• The Spatial Clustering of ROSAT All-Sky Survey AGN: I. The cross-correlation function with SDSS Luminous Red Galaxies
• Milky Way mass constraints from the Galactic satellite gap
• The VLT LBG Redshift Survey - III. The clustering and dynamics of Lyman-break galaxies at z ~ 3
• Exploring the evolutionary paths of the most massive galaxies since z~2
• The mid-life crisis of the Milky Way and M31
• Towards Precision LSST Weak-Lensing Measurement - I: Impacts of Atmospheric Turbulence and Optical Aberration
• The Role of Galaxies and AGN in Reionising the IGM - I: Keck Spectroscopy of 5 < z < 7 Galaxies in the QSO Field J1148+5251
• LoCuSS: Hydrostatic Mass Measurements of the High-$L_X$ Cluster Sample -- Cross-calibration of Chandra and XMM-Newton
• Halo and Galaxy Formation Histories from the Millennium Simulation: Public release of a VO-oriented and SQL-queryable database for studying the evolution of galaxies in the LambdaCDM cosmogony
• The quenching of galaxies, bulges, and disks since cosmic noon: A machine learning approach for identifying causality in astronomical data
• The Chandra survey of the COSMOS field II: source detection and photometry
• A catalog of merging dwarf galaxies in the local universe
• Dark-ages reionization & galaxy formation simulation IV: UV luminosity functions of high-redshift galaxies
• The Dynamics of Galaxy Pairs in a Cosmological Setting
• Recovering the nonlinear density field from the galaxy distribution with a Poisson-Lognormal filter
• The evolution of the red sequence slope in massive galaxy clusters
• Instability of Supersonic Cold Streams Feeding Galaxies I: Linear Kelvin-Helmholtz Instability with Body Modes
• The XMM-Newton survey of the ELAIS-S1 field. I: Number counts, angular correlation function and X-ray spectral properties
• Photometric Redshifts with the LSST: Evaluating Survey Observing Strategies
• The origin of the atomic and molecular gas contents of early-type galaxies. II. Misaligned gas accretion
• Reproducing sub-millimetre galaxy number counts with cosmological hydrodynamic simulations
• Mass assembly of galaxies: Smooth accretion versus mergers
• The evolution of galaxies from primeval irregulars to present-day ellipticals
• Model-independent determination of $H_0$ and ${\Omega }_{K0}$ from strong lensing and type Ia supernovae
• How does galaxy environment matter? The relationship between galaxy environments, colour and stellar mass at 0.4 < z < 1 in the Palomar/DEEP2 survey
• From Voids to Coma: the prevalence of pre-processing in the local Universe
• GASP XXI. Star formation rates in the tails of galaxies undergoing ram-pressure stripping
• Intragroup diffuse light in compact groups of galaxies II. HCG 15, 35 and 51
• Massive star formation in Wolf-Rayet galaxies. V: Star formation rates, masses and the importance of galaxy interactions
• Galaxy and Mass Assembly (GAMA): Projected Galaxy Clustering
• An Empirical Model for the Star Formation History in Dark Matter Halos
• Analytical Approach to Subhaloes Population in Dark Matter Haloes
• Quasars: What turns them off?
• Minor vs Major Mergers: The Stellar Mass Growth of Massive Galaxies from z=3 using Number Density Selection Techniques
• Painting galaxies into dark matter halos using machine learning
• The multiplicity and anisotropy of galactic satellite accretion
• An Artificial Neural Network Approach For Ranking Quenching Parameters In Central Galaxies
• Extracting Angular Diameter Distance and Expansion Rate of the Universe from Two-dimensional Galaxy Power Spectrum at High Redshifts: Baryon Acoustic Oscillation Fitting versus Full Modeling
• The star formation history of galaxies: the role of galaxy mass, morphology and environment
• No overdensity of Lyman Alpha Emitting Galaxies around a quasar at z~5.7
• Stellar Kinematics in the Complicated Inner Spheroid of M31: Discovery of Substructure Along the Southeastern Minor Axis and its Relationship to the Giant Southern Stream
• Modeling the Dust Properties of z ~ 6 Quasars with ART^2 -- All-wavelength Radiative Transfer with Adaptive Refinement Tree
• Towards a measurement of the spectral runnings
• The Mass Assembly History of Spheroidal Galaxies: Did Newly-Formed Systems Arise Via Major Mergers?
• Concentrations of Dark Haloes Emerge from Their Merger Histories
• Modelling galaxy stellar mass evolution from z~0.8 to today
• Cosmological simulations of black hole growth II: how (in)significant are merger events for fuelling nuclear activity?
• First results from SMAUG: Uncovering the Origin of the Multiphase Circumgalactic Medium with a Comparative Analysis of Idealized and Cosmological Simulations
• The clustering of radio galaxies at z~0.55 from the 2SLAQ LRG survey
• Improved Constraints on the Gravitational Lens Q0957+561. II. Strong Lensing
• The angular momentum of cold dark matter haloes with and without baryons
• Galaxy And Mass Assembly (GAMA): The dependence of the galaxy luminosity function on environment, redshift and colour
• Comparison of an X-ray selected sample of massive lensing clusters with the MareNostrum Universe LCDM simulation
• Variations of the initial mass function in semi-analytical models: implications for the mass assembly and the chemical enrichment of galaxies in the GAEA model
• The VIMOS Ultra Deep Survey: The reversal of the star-formation rate $-$ density relation at $2<z<5$
• On the Structure of Hot Gas in Halos: Implications for the Lx-Tx Relation & Missing Baryons
• Thermodynamic perturbations in the X-ray halo of 33 clusters of galaxies observed with Chandra ACIS
• Gravitational wave cosmology with extreme mass-ratio inspirals
• What shapes a galaxy? - Unraveling the role of mass, environment and star formation in forming galactic structure
• Empirical H-alpha emitter count predictions for dark energy surveys
• Higher Order Contributions to the 21 cm Power Spectrum
• A proto-cluster at z=2.45
• The Rich Globular Cluster System of Abell 1689 and the Radial Dependence of the Globular Cluster Formation Efficiency
• Cosmology with intensity mapping techniques using atomic and molecular lines
• Globular Cluster Formation Within The Aquarius Simulation
• The Clustering Characteristics of HI-Selected Galaxies from the 40% ALFALFA Survey
• Inhomogeneous Cosmology with Numerical Relativity
• Tidal Disruption of Satellite Galaxies in a Semi-Analytic Model of Galaxy Formation
• Reproducing the assembly of massive galaxies within the hierarchical cosmogony
• A giant ring-like structure at 0.78<z<0.86 displayed by GRBs
• Luminous Quasars Do Not Live in the Most Overdense Regions of Galaxies at z~4
• MASSIV: Mass Assembly Survey with SINFONI in VVDS. V. The major merger rate of star-forming galaxies at 0.9 < z < 1.8 from IFS-based close pairs
• The halo model for cosmology: a pedagogical review
• The Beginning and the End: The Meaning of Life in a Cosmological Perspective
• A Systematic Search for Periodically Varying Quasars in Pan-STARRS1: An Extended Baseline Test in Medium Deep Survey Field MD09
• Halo model description of the non-linear dark matter power spectrum at $k\gg 1$ Mpc${}^{-1}$
• Are z~5 QSOs found in the most massive high redshift over-densities?
• The First Generation of Star-Forming Haloes
• Robust Velocity-induced Acoustic Oscillations at Cosmic Dawn
• Reconstructing cosmological initial conditions from galaxy peculiar velocities. I. Reverse Zeldovich Approximation
• The Impact of the Fiducial Cosmology Assumption on BAO Cosmological Parameter Inference
• The velocity function of gas-rich galaxies
• The influence of environment on satellite galaxies in the GAEA semi-analytic model
• Dark matter halo abundances, clustering and assembly histories at high redshift
• Deducing the Lifetime of Short Gamma-Ray Burst Progenitors from Host Galaxy Demography
• Pulsars and Gravity
• PRIMUS: Galaxy Clustering as a Function of Luminosity and Color at 0.2<z<1
• The Impact of Box Size on the Properties of Dark Matter Haloes in Cosmological Simulations
• The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations
• The impact of baryon physics on the structure of high-redshift galaxies
• Absence of self-averaging and of homogeneity in the large scale galaxy distribution
• Dark Energy in Practice
• Pulsar Timing Array Analysis for Black Hole Backgrounds
• Quantifying Cosmic Superstructures
• The NOAO Fundamental Plane Survey - III. Variations in the stellar populations of red-sequence galaxies from the cluster core to the virial radius
• Predictions for deep galaxy surveys with JWST from $\Lambda$CDM
• Cosmic Web Reconstruction through Density Ridges: Method and Algorithm
• Dwarf elliptical galaxies as ancient tidal dwarf galaxies
• Einstein's Universe: Cosmological structure formation in numerical relativity
• Hubble Space Telescope Grism Spectroscopy of Extreme Starbursts Across Cosmic Time: The Role of Dwarf Galaxies in the Star Formation History of the Universe
• Halo Shapes From Weak Lensing: The Impact of Galaxy--Halo Misalignment
• Predictions for Herschel from LambdaCDM: unveiling the cosmic star formation history
• Galaxy formation with L-GALAXIES: Modelling the environmental dependency of galaxy evolution and comparing with observations
• Properties of the cosmological filament between two clusters: A possible detection of a large-scale accretion shock by $Suzaku$
• The SCUBA-2 Cosmology Legacy Survey: Ultraluminous star-forming galaxies in a z=1.6 cluster
• The origin of dust in galaxies across cosmic time
• Galaxy and Mass Assembly (GAMA): halo formation times and halo assembly bias on the cosmic web
• Where Do Galaxies End?
• Halo Substructure Boosts to the Signatures of Dark Matter Annihilation
• On the occurrence of galaxy harassment
• AGN clustering in the local Universe: an unbiased picture from Swift-BAT
• Probing non-spherical dark halos in the Galactic dwarf galaxies
• Superclusters of galaxies from the 2dF redshift survey. II. Comparison with simulations
• The baryonic mass function of galaxies
• 3D-Matched-Filter Galaxy Cluster Finder I: Selection Functions and CFHTLS Deep Clusters
• The impact of AGN feedback and baryonic cooling on galaxy clusters as gravitational lenses
• The Orbital Ellipticity of Satellite Galaxies and the Mass of the Milky Way
• Cosmological constraints from the CFHTLenS shear measurements using a new, accurate and flexible way of predicting nonlinear mass clustering
• The Zurich Environmental Study (ZENS) of Galaxies in Groups along the Cosmic Web. I. Which Environment Affects Galaxy Evolution?
• The Effect of Star Formation on the Redshift Evolution of Interstellar Metals, Atomic and Molecular Gas in Galaxies
• Thresholded Power Law Size Distributions of Instabilities in Astrophysics
• Efficient computation of the gravitational wave spectrum emitted by eccentric massive black hole binaries in stellar environments
• GA-NIFS: The core of an extremely massive proto-cluster at the Epoch of Reionization probed with JWST/NIRSpec
• Power spectrum of the maxBCG sample: detection of acoustic oscillations using galaxy clusters
• Axion Miniclusters in Modified Cosmological Histories
• Persistence of the Color-Density Relation and Efficient Environmental Quenching to $z\sim 1.4$
• Searching for large-scale structures around high-redshift radio galaxies with Herschel
• The galaxy power spectrum: precision cosmology from large scale structure?
• Interstellar filaments and star formation
• The clustering of SDSS galaxy groups: mass and color dependence
• Constraining the dark energy equation of state using LISA observations of spinning Massive Black Hole binaries
• A semi-analytic model comparison - gas cooling and galaxy mergers
• A flexible modelling of galaxy assembly bias
• Anisotropies in the astrophysical gravitational-wave background: The impact of black hole distributions
• The 21 cm signal and the interplay between dark matter annihilations and astrophysical processes
• Stellar binary black holes in the LISA band: a new class of standard sirens
• The Impact of Recent Advances in Laboratory Astrophysics on our Understanding of the Cosmos
• Scaling relations between black holes and their host galaxies: comparing theoretical and observational measurements, and the impact of selection effects
• Characterising and Identifying Galaxy Protoclusters
• Testing the predictions of the cold dark matter model for the sizes, colours, morphologies and luminosities of galaxies with the SDSS
• Two New Catalogues of Superclusters of Abell/ACO Galaxy Clusters out to redshift 0.15
• The Extended Spatial Distribution of Globular Clusters in the Core of the Fornax Cluster
• Combining clustering and abundances of galaxy clusters to test cosmology and primordial non-Gaussianity
• Topology of structure in the Sloan Digital Sky Survey: model testing
• Simulating Structure Formation of the Local Universe
• Massive star formation in Wolf-Rayet galaxies: II. Optical spectroscopy results
• The Norma Cluster (ACO 3627): I. A Dynamical Analysis of the Most Massive Cluster in the Great Attractor
• Illuminating the dark ages: Cosmic backgrounds from accretion onto primordial black hole dark matter
• The atomic Hydrogen content of the post-reionization Universe
• NGC6240: A triple nucleus system in the advanced or final state of merging
• A Lightcone Catalogue from the Millennium-XXL Simulation
• A SINFONI view of flies in the Spiderweb: a galaxy cluster in the making
• The rest-frame $K$-band luminosity function of galaxies in clusters to $z=1.3$
• Inhomogeneities in the universe
• Inferring the star formation histories of the most massive and passive early-type galaxies at z<0.3
• Constraints on the shapes of galaxy dark matter haloes from weak gravitational lensing
• Cosmology with Doppler Lensing
• The matter distribution in the local Universe as derived from galaxy groups in SDSS DR12 and 2MRS
• The Redshift Evolution of the Mass Function of Cold Gas in Hierarchical Galaxy Formation Models
• A Comparison of Galaxy Merger History Observations and Predictions from Semi-Analytic Models
• Triggering and Delivery Algorithms for AGN Feedback
• SURFS: Riding the waves with Synthetic UniveRses For Surveys
• Galaxy Number Counts and Implications for Strong Lensing
• Properties of Dark Matter Halos as a Function of Local Environment Density
• Deep observations of CO line emission from star-forming galaxies in a cluster candidate at z=1.5
• Filamentary Large Scale Structure Traced by Six Ly-alpha Blobs at z=2.3
• The coherent motion of Cen A dwarf satellite galaxies remains a challenge for $\Lambda$CDM cosmology
• H0LiCOW II. Spectroscopic survey and galaxy-group identification of the strong gravitational lens system HE0435-1223
• Collapsed Dark Matter Structures
• A First Site of Galaxy Cluster Formation: Complete Spectroscopy of a Protocluster at $z=6.01$
• The MUSE Ultra Deep Field (MUDF). II. Survey design and the gaseous properties of galaxy groups at 0.5 < z < 1.5
• MUSE Analysis of Gas around Galaxies (MAGG) -- I: Survey design and the environment of a near pristine gas cloud at z~3.5
• GalaxyNet: Connecting galaxies and dark matter haloes with deep neural networks and reinforcement learning in large volumes
• Scientific Visualization in Astronomy: Towards the Petascale Astronomy Era
• Forming intracluster gas in a galaxy protocluster at a redshift of 2.16
• The clustering of galaxies as a function of their photometrically-estimated atomic gas content
• The role of major mergers in shaping galaxies at 2<z<4 in the VUDS and VVDS surveys
• Cosmic Flows : Green Bank and Parkes HI observations
• Discovery of a Very Large Structure at Z=3.78
• Numerical resolution limits on subhalo abundance matching
• On the definition of superclusters
• The intrinsic bispectrum of the Cosmic Microwave Background [PhD thesis]
• Red Giants in the Small Magellanic Cloud. I. Disk and Tidal Stream Kinematics
• Secondary Infall and the Pseudo-Phase-Space Density Profiles of Cold Dark Matter Halos
• Proto-groups at 1.8<z<3 in the zCOSMOS-deep sample
• Statistics of extreme objects in the Juropa Hubble Volume simulation
• BayeSED: A General Approach to Fitting the Spectral Energy Distribution of Galaxies
• The real shape of non-Gaussianities
• The merger rates and sizes of galaxies across the peak epoch of star formation from the HiZELS survey
• The Weak Clustering of Gas-Rich Galaxies
• Quantifying the Cosmic Web I: The large-scale halo ellipticity-ellipticity and ellipticity-direction correlations
• DEMNUni: Massive neutrinos and the bispectrum of large scale structures
• Improved reconstructions of random media using dilation and erosion processes
• A Giant Protocluster of Galaxies at Redshift 5.7
• Evidence for the inside-out growth of the stellar mass distribution in galaxy clusters since z~1
• The similarity of the stellar mass fractions of galaxy groups and clusters
• Public Release of A-SLOTH: Ancient Stars and Local Observables by Tracing Halos
• AzTEC/ASTE 1.1 mm survey of SSA22: Counterpart identification and photometric redshift survey of submillimeter galaxies
• nIFTy galaxy cluster simulations II: radiative models
• Triggering of merger-induced starbursts by the tidal field of galaxy groups and clusters
• Time-delay cosmographic forecasts with strong lensing and JWST stellar kinematics
• An HST/ACS investigation of the spatial and chemical structure and sub-structure of NGC 891, a Milky Way analogue
• The Atacama Cosmology Telescope: Dynamical masses for 44 SZ-selected galaxy clusters over 755 square degrees
• Theoretical and observational constraints on the HI intensity power spectrum
• The Extreme Small Scales: Do Satellite Galaxies Trace Dark Matter?
• The masses of satellites in GAMA galaxy groups from 100 square degrees of KiDS weak lensing data
• On the Correlation between Spin Parameter and Halo Mass
• Spectroscopic Confirmation of a Protocluster at z=3.786
• BCG Mass Evolution in Cosmological Hydro-Simulations
• Machine Learning and Cosmological Simulations II: Hydrodynamical Simulations
• The Millennium Run Observatory: First Light
• Inverted initial conditions: exploring the growth of cosmic structure and voids
• Gravitational waves and pulsar timing: stochastic background, individual sources and parameter estimation
• GASP XXIX -- Unwinding the arms of spiral galaxies via ram-pressure stripping
• Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters
• Discovery of a supercluster in the ZOA in Vela
• On the formation time scale of massive cluster ellipticals based on deep near-IR spectroscopy at z~2
• L-GALAXIES 2020: The evolution of radial metallicity profiles and global metallicities in disc galaxies
• 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 Dynamics of Subhalos in Warm Dark Matter Models
• The clustering of Ly-alpha emitters in a LambdaCDM Universe
• Phase-space structures II: Hierarchical Structure Finder
• Direct evidence of AGN-feedback: a post starburst galaxy stripped of its gas by AGN-driven winds
• The evolution of SMBH spin and AGN luminosities for $z<6$ within a semi-analytic model of galaxy formation
• High-quality strong lens candidates in the final Kilo Degree survey footprint
• Searching for diffuse light in the M96 Group
• Testing general scalar-tensor gravity and massive gravity with cluster lensing
• Annual Modulation in Direct Dark Matter Searches
• Discovery of a stellar tidal stream around the Whale galaxy, NGC 4631
• The Rise of Active Galactic Nuclei in the GAlaxy Evolution and Assembly semi-analytic model
• The Herschel Bright Sources (HerBS): Sample definition and SCUBA-2 observations
• Recoiling Supermassive Black Holes: a search in the Nearby Universe
• The rapid evolution of AGN feedback in brightest cluster galaxies: switching from quasar-mode to radio-mode feedback
• Early structure formation in quintessence models and its implications for cosmic reionisation from first stars
• The Colors of Central and Satellite Galaxies in zCOSMOS out to z ~ 0.8 and Implications for Quenching
• Going Beyond the Galaxy Power Spectrum: an Analysis of BOSS Data with Wavelet Scattering Transforms
• The growth of disks and bulges during hierarchical galaxy formation. I: fast evolution vs secular processes
• Influence of Electric Charge and Modified Gravity on Density Irregularities
• T-ReX: a graph-based filament detection method
• Cold gas in cluster cores: Global stability analysis and non-linear simulations of thermal instability
• Detecting and Characterizing Young Quasars II: Four Quasars at $z\sim 6$ with Lifetimes $<10^4$ years
• The evolution of the star forming sequence in hierarchical galaxy formation models
• Equilibrium Structure and Radial Oscillations of Dark Matter Admixed Neutron Stars
• A Tale of Dwarfs and Giants: Using a z=1.62 Cluster to Understand How the Red Sequence Grew Over The Last 9.5 Billion Years
• The ALPINE-ALMA [CII] survey: The contribution of major mergers to the galaxy mass assembly at z~5
• Rotation curve fitting and its fatal attraction to cores in realistically simulated galaxy observations
• Clustering properties of galaxies selected in stellar mass: Breaking down the link between luminous and dark matter in massive galaxies from z=0 to z=2
• Early formation of supermassive black holes via dark matter self-interactions
• The First Generation of Virgo Cluster Dwarf Elliptical Galaxies?
• A flexible subhalo abundance matching model for galaxy clustering in redshift space
• The VANDELS survey: the relation between UV continuum slope and stellar metallicity in star-forming galaxies at z~3
• Future Evolution of Bound Superclusters in an Accelerating Universe
• Slow-then-rapid quenching as traced by tentative evidence for enhanced metallicities of cluster galaxies at z~0.2 in the slow quenching phase
• The role of submillimetre galaxies in hierarchical galaxy formation
• The evolution of Brightest Cluster Galaxies in a hierarchical universe
• Cosmic Web Reconstruction through Density Ridges: Catalogue
• Separate Universe Consistency Relation and Calibration of Halo Bias
• Dependency of halo concentration on mass, redshift and fossilness in Magneticum hydrodynamic simulations
• An Extreme Starburst in Close Proximity to the Central Galaxy of a Rich Galaxy Cluster at z=1.7
• Substructure in the Most Massive GEEC Groups: Field-like Populations in Dynamically Active Groups
• Instability of Supersonic Cold Streams Feeding Galaxies III: Kelvin-Helmholtz Instability in Three Dimensions
• Galaxy and Mass Assembly (GAMA): Redshift Space Distortions from the Clipped Galaxy Field
• Disentangling the Cosmic Web Towards FRB 190608
• Constraining the HI-Halo Mass Relation From Galaxy Clustering
• Luminous superclusters: remnants from inflation
• Far-Ultraviolet & X-ray Observations of VV 114: Feedback in a Local Analog to Lyman Break Galaxies
• Exploring SMBH Assembly with Semi-analytic Modelling
• An analytical model for the accretion of dark matter subhalos
• An iterative reconstruction of cosmological initial density fields
• Linear perturbative theory of the discrete cosmological N-body problem
• Cosmological simulations of galaxy clusters with feedback from active galactic nuclei: profiles and scaling relations
• An ideal mass assignment scheme for measuring the Power Spectrum with FFTs
• The multidimensional dependence of halo bias in the eye of a machine: a tale of halo structure, assembly and environment
• Cosmography with cluster strong lenses: the influence of substructure and line-of-sight halos
• The evolution of galaxy cluster X-ray scaling relations
• How to Grow a Healthy Merger Tree
• How closely do baryons follow dark matter on large scales?
• Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
• Structure formation in the quasispherical Szekeres model
• Calibration of semi-analytic models of galaxy formation using Particle Swarm Optimization
• The VIMOS-VLT Deep Survey. The dependence of clustering on galaxy stellar mass at z~1
• Cosmological Backreaction from Perturbations
• Shot noise in the astrophysical gravitational-wave background
• Absorption signatures of warm-hot gas at low redshift: Broad HI Lyman-Alpha Absorbers
• The velocity field of 2MRS Ks=11.75 galaxies: constraints on beta and bulk flow from the luminosity function
• H0LiCOW VIII. A weak lensing measurement of the external convergence in the field of the lensed quasar HE0435$-$1223
• Star formation history of galaxies from z=0 to z=0.7 A backward approach to the evolution of star-forming galaxies
• The Growth of Intracluster Light in XCS-HSC Galaxy Clusters from $0.1<z<0.5$
• Tracing the Quenching Journey across Cosmic Time
• Non-Gaussian halo assembly bias
• Planck intermediate results. XXXVII. Evidence of unbound gas from the kinetic Sunyaev-Zeldovich effect
• AGN-Host Galaxy Connection: Morphology and Colours of X-ray Selected AGN at z < 2
• A First Look at Galaxy Flyby Interactions: I. Characterizing the Frequency of Flybys in a Cosmological Context
• The Role of Gas In Maintaining Quasi-Steady Spiral Structure In Stellar Disks
• Measuring the growth rate of structure with Type IA Supernovae from LSST
• Massive and old quiescent galaxies at high redshift
• Physical drivers of galaxies' cold-gas content: exploring environmental and evolutionary effects with DARK SAGE
• CEERS Key Paper III: The Resolved Host Properties of AGN at 3 < z < 5 with JWST
• The Theoretical Astrophysical Observatory: Cloud-Based Mock Galaxy Catalogues
• An observer's guide to the (Local Group) dwarf galaxies: predictions for their own dwarf satellite populations
• Constraints on black hole fuelling modes from the clustering of X-ray AGN
• The Chandra Deep Fields: Lifting the Veil on Distant Active Galactic Nuclei and X-Ray Emitting Galaxies
• The non-Gaussianity of the cosmic shear likelihood - or: How odd is the Chandra Deep Field South?
• Galaxy And Mass Assembly (GAMA): Testing galaxy formation models through the most massive galaxies in the Universe
• Streams in the Aquarius stellar haloes
• Chemical evolution of Local Group dwarf galaxies in a cosmological context -- I. A new modelling approach and its application to the Sculptor dwarf spheroidal galaxy
• Impact of Foregrounds on HI Intensity Mapping Cross-Correlations with Optical Surveys
• Inferring the IGM thermal history during reionisation with the Lyman-$\alpha$ forest power spectrum at redshift $z\simeq 5$
• Quenching low-mass satellite galaxies: evidence for a threshold ICM density
• Red Star Forming Galaxies and Their Environment at z=0.4 Revealed by Panoramic H-alpha Imaging
• The Impact of Galaxy Cluster Mergers on Cosmological Parameter Estimation from Surveys of the Sunyaev-Zel'dovich Effect
• Observational signatures of a warped disk associated with cold-flow accretion
• The SAMI Galaxy Survey: Observing the environmental quenching of star formation in GAMA groups
• Mapping dark matter with cosmic magnification
• Photometric redshifts: estimating their contamination and distribution using clustering information
• Cosmic Emulation: The Concentration-Mass Relation for wCDM Universes
• Galaxies in X-ray Selected Clusters and Groups in Dark Energy Survey Data I: Stellar Mass Growth of Bright Central Galaxies Since z~1.2
• Theoretical Systematics of Future Baryon Acoustic Oscillation Surveys
• Dark Energy Constraints from Baryon Acoustic Oscillations
• Compact Groups of Galaxies selected by stellar mass: The 2MASS Compact Group Catalogue
• Galactic inflow and wind recycling rates in the EAGLE simulations
• Spectroscopy of luminous z>7 galaxy candidates and sources of contamination in z>7 galaxy searches
• The Ellipticity Distribution of Ambiguously Blended Objects
• The Accretion of Gas onto Galaxies as Traced by their Satellites
• Disentangling the AGN and Star-Formation connection using XMM-Newton
• Dwarf galaxy populations in present-day galaxy clusters - II. The history of early-type and late-type dwarfs
• Cosmology in 2D: the concentration-mass relation for galaxy clusters
• Reconstructing the distribution of haloes and mock galaxies below the resolution limit in cosmological simulations
• A direct measurement of galaxy major and minor merger rates and stellar mass accretion histories at $z<3$ using galaxy pairs in the REFINE survey
• Evolution of the Early-Type Galaxy Fraction in Clusters since z = 0.8
• How well do cosmological simulations reproduce individual-halo properties?
• Evolution of blue E/S0 galaxies from z~1: merger remnants or disk rebuilding galaxies?
• A wide angle tail radio galaxy in the COSMOS field: evidence for cluster formation
• Accurate Modeling of Weak Lensing with the sGL Method
• Rejuvenating Power Spectra II: the Gaussianized galaxy density field
• A new spin on disks of satellite galaxies
• AGN-driven outflows and the formation of Ly$\alpha$ nebulae around high-z quasars
• Accurate mass and velocity functions of dark matter halos
• The stability of stellar disks in Milky-Way sized dark matter halos
• The structure and assembly history of cluster-size haloes in Self-Interacting Dark Matter
• The Evolution of Galaxies in X-ray Luminous Groups
• Galaxy Formation as a Cosmological Tool. I: The Galaxy Merger History as a Measure of Cosmological Parameters
• Merger induced scatter and bias in the cluster mass - Sunyaev-Zeldovich effect scaling relation
• Pairwise Velocities of Dark Matter Halos: a Test for the Lambda Cold Dark Matter Model using the Bullet Cluster
• Speeding up $N$-body simulations of modified gravity: Chameleon screening models
• Discovering the Unexpected in Astronomical Survey Data
• Optimal filtering of optical and weak lensing data to search for galaxy clusters: application to the COSMOS field
• The hard X-ray emission of the luminous infrared galaxy NGC 6240 as observed by NuSTAR
• The Diversity of Diffuse Ly$\alpha$ Nebulae around Star-Forming Galaxies at High Redshift
• Cluster Magnification & the Mass-Richness Relation in CFHTLenS
• Detecting clusters of galaxies and active galactic nuclei in an eROSITA all-sky survey digital twin
• Caught in the cosmic web: Environmental effect on halo concentrations, shape, and spin
• LoCuSS: The infall of X-ray groups onto massive clusters
• The effect of thermally pulsating asymptotic giant branch stars on the evolution of the rest-frame near-infrared galaxy luminosity function
• Search for Compensated Isocurvature Perturbations with Planck Power Spectra
• Formation and Evolution of Binary Neutron Stars: Mergers and Their Host Galaxies
• The role of HD cooling in primordial star formation
• An optical/NIR survey of globular clusters in early-type galaxies II. Ages of GC systems and the relation to galaxy morphology
• Numerical overcooling in shocks
• Cluster strong lensing in the Millennium Simulation: The effect of galaxies and structures along the line-of-sight
• Enriching the hot circumgalactic medium
• Observational selection biases in time-delay strong lensing and their impact on cosmography
• A study of the circum-galactic medium at z ~ 0.6 using DLA-galaxies
• A KiDS weak lensing analysis of assembly bias in GAMA galaxy groups
• Kinematic constraints on the stellar and dark matter content of spiral and S0 galaxies
• A Serendipitous XMM Survey of the SDSS: the evolution of the colour-magnitude diagram of X-ray AGN from z=0.8 to z=0.1
• Galaxy cluster searches by photometric redshifts in the CFHTLS
• The nature of assembly bias - I. Clues from a LCDM cosmology
• Rotation rates, sizes, and star formation efficiencies of a representative population of simulated disc galaxies
• Dark and luminous satellites of LMC-mass galaxies in the FIRE simulations
• Resolution-independent modeling of environmental effects in semi-analytic models of galaxy formation that include ram-pressure stripping of both hot and cold gas
• Star Clusters Around Recoiled Black Holes in the Milky Way Halo
• Systematic effects in the sound horizon scale measurements
• No excess of bright galaxies around the redshift 7.1 quasar ULAS J1120+0641
• Constraints on Dark Matter Annihilation in Clusters of Galaxies from Diffuse Radio Emission
• Superclusters of galaxies in the 2dF redshift survey. III. The properties of galaxies in superclusters
• Galaxy Clustering Topology in the Sloan Digital Sky Survey Main Galaxy Sample: a Test for Galaxy Formation Models
• Capturing Halos at High Redshifts
• SINFONI-HiZELS: The dynamics, merger rates & metallicity gradients of `typical' star-forming galaxies at $z$ = 0.8-2.2
• Expected number of massive galaxy relics in the present-day Universe
• The structural and photometric properties of early-type galaxies in hierarchical models
• ETHOS -- an effective theory of structure formation: predictions for the high-redshift Universe -- abundance of galaxies and reionization
• Solving the Vlasov equation in two spatial dimensions with the Schrödinger method
• HI-selected Galaxies in Hierarchical Models of Galaxy Formation and Evolution
• Hydrodynamical simulations of galaxy clusters in dark energy cosmologies: II. c-M relation
• Constraining the Cosmic Baryon Distribution with Fast Radio Burst Foreground Mapping
• Future virialized structures: An analysis of superstructures in SDSS-DR7
• Assembly of filamentary void galaxy configurations
• Quantifying Photometric Redshift Errors in the Absence of Spectroscopic Redshifts
• Recurring flares from supermassive black hole binaries: implications for tidal disruption candidates and OJ 287
• Fossil Groups Origins: I. RX J105453.3+552102 a very massive and relaxed system at z~0.5
• Where do "red and dead" early-type void galaxies come from?
• Star-forming blue ETGs in two newly discovered galaxy overdensities in the HUDF at z=1.84 and 1.9: unveiling the progenitors of passive ETGs in cluster cores
• Massive Galaxies are Larger in Dense Environments: Environmental Dependence of Mass-Size Relation of Early-Type Galaxies
• The Mass Dependence of Dwarf Satellite Galaxy Quenching
• The Stellar Mass Components of Galaxies: Comparing Semi-Analytical Models with Observation
• The Late Stellar Assembly of Massive Cluster Galaxies Via Major Merging
• Search for 511 keV Emission in Satellite Galaxies of the Milky Way with INTEGRAL/SPI
• Mining the gap: evolution of the magnitude gap in X-ray galaxy groups from the 3 square degree XMM coverage of CFHTLS
• The Formation and Evolution of Virgo Cluster Galaxies - II. Stellar Populations
• A New Statistical Model for Population III Supernova Rates: Discriminating Between $\Lambda$CDM and WDM Cosmologies
• Learning the Relationship between Galaxies Spectra and their Star Formation Histories using Convolutional Neural Networks and Cosmological Simulations
• Baryon fractions in clusters of galaxies: evidence against a preheating model for entropy generation
• Velocity Anisotropy and Shape Bias in the Caustic Technique
• Galaxy cluster searches based on photometric redshifts in the four CFHTLS Wide fields
• The environments of high redshift radio galaxies and quasars: probes of protoclusters
• Absence of anti-correlations and of baryon acoustic oscillations in the galaxy correlation function from the Sloan Digital Sky Survey DR7
• Towards quantitative control on discreteness error in the non-linear regime of cosmological N body simulations
• Galaxy populations in the Hydra I cluster from the VEGAS survey II. The ultra-diffuse galaxy population
• Compact groups in theory and practice - I. The spatial properties of compact groups
• The Building Up of the Black Hole Mass - Stellar Mass Relation
• The VLT LBG Redshift Survey I: Clustering and Dynamics of ~1000 Galaxies at z~3
• Impact of baryons on the cluster mass function and cosmological parameter determination
• Deriving star formation histories from photometry using energy balance spectral energy distribution modelling
• Clipping the Cosmos: The Bias and Bispectrum of Large Scale Structure
• Forecast for FAST: from Galaxies Survey to Intensity Mapping
• Machine Learning and Cosmological Simulations I: Semi-Analytical Models
• Modeling The Large Scale Bias of Neutral Hydrogen
• Red Sequence Cluster Finding in the Millennium Simulation
• Metal-line emission from the warm-hot intergalactic medium: I. Soft X-rays
• Galaxy Zoo: Chiral correlation function of galaxy spins
• Cluster Abell 520: a perspective based on member galaxies. A cluster forming at the crossing of three filaments?
• Study of Dark-Matter Admixed Neutron Stars using the Equation of State from the Rotational Curves of Galaxies
• Origin of the galaxy HI size-mass relation
• The simplest model of galaxy formation I: A formation history model of galaxy stellar mass growth
• On the influence of halo mass accretion history on galaxy properties and assembly bias
• The Environmental Dependence of Galaxy Properties at z=2
• On the shear estimation bias induced by the spatial variation of colour across galaxy profiles
• First Light And Reionisation Epoch Simulations (FLARES) IV: The size evolution of galaxies at $z\ge 5$
• A detection of wobbling Brightest Cluster Galaxies within massive galaxy clusters
• The earliest stars and their relics in the Milky Way
• Ram pressure histories of cluster galaxies
• High Redshift Galaxy Populations and their Descendants
• On the origin of star-gas counterrotation in low-mass galaxies
• Diffuse gas properties and stellar metallicities in cosmological simulations of disc galaxy formation
• Order out of Randomness : Self-Organization Processes in Astrophysics
• The impact of galaxy formation on satellite kinematics and redshift-space distortions
• A modified star formation law as a solution to open problems in galaxy evolution
• Exploring the nature of the Lyman-$\alpha$ emitter CR7
• Cosmological baryon transfer in the SIMBA simulations
• Accurate weak lensing of standard candles. I. Flexible cosmological fits
• The origin of the enhanced metallicity of satellite galaxies
• A near-IR study of the host galaxies of 2Jy radio sources at 0.03 < z < 0.5: I - the data
• Cosmic Ballet III: halo spin evolution in the cosmic web
• The strong correlation between post-starburst fraction and environment
• A Deficit of Faint Red Galaxies in the Possible Large-Scale Structures around the RDCS J1252.9-2927 Cluster at z=1.24
• The competition between confinement and ram pressure and its implications for galaxies in groups and clusters
• Building a control sample for galaxy pairs
• Dark energy as a mirage
• Broadband Photometry of 105 Giant Arcs: Redshift Constraints and Implications for Giant Arc Statistics
• What is the best way to measure baryonic acoustic oscillations?
• Compact groups from the Millennium Simulations: I. Their Nature and the completeness of the Hickson sample
• Galaxy evolution in protoclusters
• Reducing distance errors for standard candles and standard sirens with weak-lensing shear and flexion maps
• Cosmology dependency of halo masses and concentrations in hydrodynamic simulations
• The Phase Space of z~1.2 SpARCS Clusters: Using Herschel to probe Dust Temperature as a Function of Environment and Accretion History
• The nonlinear matter power spectrum
• Early-type galaxy density profiles from IllustrisTNG: I. Galaxy correlations and the impact of baryons
• Redshift-space effects in voids and their impact on cosmological tests. Part I: the void size function
• The origin of the mass scales for maximal star formation efficiency and quenching: the critical role of Supernovae
• Galaxy properties and the cosmic web in simulations
• Optimal linear reconstruction of dark matter from halo catalogs
• Pulsar Timing Constraints on the Fermi Massive Black-Hole Binary Blazar Population
• How runaway stars boost galactic outflows
• Very large scale correlations in the galaxy distribution
• The early-type galaxies NGC 1407 and NGC 1400 - II: star formation and chemical evolutionary history
• Stellar mass functions of galaxies at 4<z<7 from an IRAC-selected sample in COSMOS/UltraVISTA: limits on the abundance of very massive galaxies
• Constraints on the Accretion History of Massive Black Holes from Faint X-ray Counts
• Galaxy population properties of the massive X-ray luminous galaxy cluster XDCP J0044.0-2033 at z=1.58: red-sequence formation, massive galaxy assembly, and central star formation activity
• A Comprehensive GALEX Ultraviolet Catalog of Star Clusters in M31 and a Study of the Young Clusters
• Probing the end of reionization with the near-zones of z > 6 QSOs
• A simple model linking galaxy and dark matter evolution
• Clustering of i-dropout galaxies at z=6 in GOODS and the UDF
• The DEEP2 Galaxy Redshift Survey: The Voronoi-Delaunay Method catalog of galaxy groups
• Simulated ΛCDM analogues of the thin Plane of Satellites around the Andromeda galaxy are not kinematically coherent structures
• Evolution of Galactic Outflows at $z\sim 0$-$2$ Revealed with SDSS, DEEP2, and Keck spectra
• Deep 1.1 mm-wavelength imaging of the GOODS-S field by AzTEC/ASTE - I. Source catalogue and number counts
• The journey of QSO haloes from z=6 to the present
• What sets the central structure of dark matter haloes?
• The Via Lactea INCITE Simulation: Galactic Dark Matter Substructure at High Resolution
• High-resolution double morphology of the most distant known radio quasar at z=6.12
• Building a Predictive Model of Galaxy Formation - I: Phenomenological Model Constrained to the $z=0$ Stellar Mass Function
• Comparing galaxy formation in the L-GALAXIES semi-analytical model and the IllustrisTNG simulations
• Nongaussianity from Particle Production During Inflation
• Ricci focusing, shearing, and the expansion rate in an almost homogeneous Universe
• Group-finding with photometric redshifts: The Photo-z Probability Peaks algorithm
• Kinematics of CIV and [OIII] emission in luminous high-redshift quasars
• The Luminosity, Colour and Morphology dependence of galaxy filaments in the Sloan Digital Sky Survey Data Release Four
• Discovery of a Proto-cluster Associated with a Ly-$\alpha$ Blob Pair at z=2.3
• Environmental effects in the interaction and merging of galaxies in zCOSMOS
• First results on the cluster galaxy population from the Subaru Hyper Suprime-Cam survey. III. Brightest cluster galaxies, stellar mass distribution, and active galaxies
• 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
• TDCOSMO. IX. Systematic comparison between lens modelling software programs: time delay prediction for WGD 2038-4008
• Substructure in the stellar halo near the Sun. I. Data-driven clustering in Integrals of Motion space
• The Next Generation Virgo Cluster Survey (NGVS). XXIV. The Red Sequence to $\sim$10${}^6$ L${}_{\odot }$ and Comparisons with Galaxy Formation Models
• Scale-dependent bias and the halo model
• Is there a relationship between AGN and star formation in IR-bright AGNs?
• The Nature of CO Emission From z~6 Quasars
• FORGE -- the f(R) gravity cosmic emulator project I: Introduction and matter power spectrum emulator
• Environments of z>5 quasars: searching for protoclusters at submillimetre wavelengths
• Modeling the Redshift Evolution of the Normal Galaxy X-ray Luminosity Function
• Numerical evolution of multiple black holes with accurate initial data
• Caustic Skeleton & Cosmic Web
• Absence of thermalization for systems with long-range interactions coupled to a thermal bath
• Comprehensive Gas Characterization of a $z=2.5$ Protocluster: A Cluster Core Caught in the Beginning of Virialization?
• Shallow Dark Matter Cusps in Galaxy Clusters
• The Generation of Vorticity in Cosmological N-body Simulations
• The emergence of passive galaxies in the early Universe
• Empirical predictions for (sub-)millimeter line and continuum deep fields
• The Void Galaxy Survey: Photometry, structure and identity of void galaxies
• Role of Galaxy Mergers in Cosmic Star Formation History
• The HIX galaxy survey II: HI kinematics of HI eXtreme galaxies
• Revealing components of the galaxy population through nonparametric techniques
• The evolution of the stellar mass versus halo mass relationship
• SPIDER IX - Classifying Galaxy Groups according to their Velocity Distribution
• Study of star-forming galaxies in SDSS up to redshift 0.4 II. Evolution from the fundamental parameters: mass, metallicity & SFR
• An interpretable machine learning framework for dark matter halo formation
• A tale of two populations: the stellar mass of central and satellite galaxies
• Estimating cosmic velocity fields from density fields and tidal tensors
• 3\%-accurate predictions for the clustering of dark matter, haloes and subhaloes, over a wide range of cosmologies and scales
• Does black-hole growth depend on the cosmic environment?
• Embedding realistic surveys in simulations through volume remapping
• Tidal Disruption of Stellar Objects by Hard Supermassive Black Hole Binaries
• Sample variance and Lyman-alpha forest transmission statistics
• The H-alpha luminosity-dependent clustering of star-forming galaxies from z~0.8 to z~2.2 with HiZELS
• Predicting Hα emission line galaxy counts for future galaxy redshift surveys
• Dark matter dynamics in Galactic center
• Modelling the cosmic spectral energy distribution and extragalactic background light over all time
• Einasto Profiles and the Dark Matter Power Spectrum
• Stellar mass functions of galaxies, disks and spheroids at z~0.1
• The Effects of Patchy Reionization on Satellite Galaxies of the Milky Way
• Properties of satellite galaxies in the SDSS photometric survey: luminosities, colours and projected number density profiles
• Triggering Active Galactic Nuclei in galaxy clusters
• Astrometric evidence for a population of dislodged AGN
• Timing the evolution of quiescent and star-forming local galaxies
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). The decline of cosmic star formation: quenching, mass, and environment connections
• Are red 2MASS QSOs young?
• Multi-flavour SMBH seeding and evolution in cosmological environments
• Ultimate age-dating method for galaxy groups; clues from the Millennium Simulations
• On the dissection of degenerate cosmologies with machine learning
• Redshift and distances in a ΛCDM cosmology with non-linear inhomogeneities
• The many lives of active galactic nuclei-II: The formation and evolution of radio jets and their impact on galaxy evolution
• The effect of baryons in the cosmological lensing PDFs
• Probing the cosmic web: inter-cluster filament detection using gravitational lensing
• Reversal or no reversal: the evolution of the star formation rate-density relation up to z~1.6
• Simulations of Baryon Acoustic Oscillations I: Growth of Large-Scale Density Fluctuations
• Determining star-formation rates in Active Galactic Nuclei hosts via stellar population synthesis
• Young and turbulent: the early life of massive galaxy progenitors
• The Line-of-Sight Proximity Effect and the Mass of Quasar Host Halos
• On the nature of the sources of the cosmic infrared background
• Unveiling the Important Role of Groups in the Evolution of Massive Galaxies: Insights from an Infrared Passive Sequence at Intermediate Redshift
• Learning effective physical laws for generating cosmological hydrodynamics with Lagrangian Deep Learning
• Perturbation Theory of the Cosmological Log-Density Field
• Equilibrium model prediction for the scatter in the star-forming main sequence
• CFHTLenS: The Environmental Dependence of Galaxy Halo Masses from Weak Lensing
• Precision modelling of the matter power spectrum in a Planck-like Universe
• A New Method to Quantify Environment and Model Ram-Pressure Stripping in N-Body Simulations
• The Cosmic Evolution of Faint Satellite Galaxies as a Test of Galaxy Formation and the Nature of Dark Matter
• Shock waves in capillary collapse of colloids: a model system for two--dimensional screened Newtonian gravity
• Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations
• Baryons in the CosmicWeb of IllustrisTNG -- II: the Connection among Galaxies, Halos, their Formation Time and their Location in the Cosmic Web
• Effects of the size of cosmological N-Body simulations on physical quantities -- I: Mass Function
• Evaluating the ability of triaxial Schwarzschild modelling to estimate properties of galaxies from the Illustris simulation
• The growth of brightest cluster galaxies in the TNG300 simulation:dissecting the contributions from mergers and in situ star formation
• How Do Galaxies trace a large scale structure?: A case study around a massive protocluster at $z=3.13$
• Finding Galaxy Groups In Photometric Redshift Space: the Probability Friends-of-Friends (pFoF) Algorithm
• Matched filter optimization of kSZ measurements with a reconstructed cosmological flow field
• Simulating magnetic fields in the Antennae galaxies
• Recent Arrival of Faint Cluster Galaxies on the Red-sequence: Luminosity Functions from 119 square degrees of CFHTLS
• Massive star formation in Wolf-Rayet galaxies: I. Optical and NIR photometric results
• Extremely Metal-Poor Galaxies: The Environment
• GaBoDS: The Garching-Bonn Deep Survey: VII. Probing galaxy bias using weak gravitational lensing
• Morphological Properties of Superclusters of Galaxies
• Simulated void galaxies in the standard cold dark matter model
• Realistic estimation for the detectability of dark matter sub-halos with Fermi-LAT
• ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
• Nature versus nurture: what regulates star formation in satellite galaxies?
• Structural Analysis of the SDSS Cosmic Web I.Nonlinear Density Field Reconstructions
• The properties of early-type galaxies in the Ursa Major cluster
• On the measurements of assembly bias and splashback radius using optically selected galaxy clusters
• Fossil Groups in the Millennium Simulation. Evolution of the Brightest Galaxies
• The two formation pathways of S0 galaxies
• The splashback radius of optically selected clusters with Subaru HSC Second Public Data Release
• Redshift distribution and luminosity function of long gamma-ray bursts from cosmological simulations
• The stellar mass content of distant galaxy groups
• Excursion Set Theory for generic moving barriers and non-Gaussian initial conditions
• Interacting galaxies in the IllustrisTNG simulations -- III: (the rarity of) quenching in post-merger galaxies
• Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies in the Local Universe I. - The Effect of the Group Environment on Star Formation in Spiral Galaxies
• Data augmentation for machine learning redshifts applied to SDSS galaxies
• The view from the boundary: a new void stacking method
• Modelling Galaxy Merger Timescales and Tidal Destruction
• Linearisation with Cosmological Perturbation Theory
• Major Cluster Mergers and the Location of the Brightest Cluster Galaxy
• Dark matter stripping in galaxy clusters: a look at the Stellar to Halo Mass relation in the Illustris simulation
• An accurate low-redshift measurement of the cosmic neutral hydrogen density
• The mass dependence of dark matter halo alignments with large-scale structure
• A bias in cosmic shear from galaxy selection: results from ray-tracing simulations
• Iron in galaxy groups and clusters: Confronting galaxy evolution models with a newly homogenised dataset
• Evidence for Early Filamentary Accretion from the Andromeda Galaxy's Thin Plane of Satellites
• The first Super Massive Black Holes: indications from models for future observations
• The Q Continuum Simulation: Harnessing the Power of GPU Accelerated Supercomputers
• The effect of dwarf galaxies disruption in semi-analytic models
• Morphologies of Galaxies in and around a Protocluster at z=2.300
• Star formation activity and gas stripping in the Cluster Projected Phase-Space (CPPS)
• Warm dark matter and the ionization history of the Universe
• Two major accretion epochs in M31 from two distinct populations of globular clusters
• Does small scale structure significantly affect cosmological dynamics?
• Stellar Masses of Lyman Break Galaxies, Lyman Alpha Emitters and Radio Galaxies in Overdense Regions at z=4-6
• Radio source feedback in galaxy evolution
• Towards understanding the relation between the gas and the attenuation in galaxies at kpc scales
• Subhalo statistics of galactic halos: beyond the resolution limit
• The velocity anisotropy of the Milky Way satellite system
• Subhaloes gone Notts: Spin across subhaloes and finders
• Connecting and dissecting galaxies' angular momenta and neutral gas in a hierarchical universe: cue DARK SAGE
• Instability of Supersonic Cold Streams Feeding Galaxies II. Nonlinear Evolution of Surface and Body Modes of Kelvin-Helmholtz Instability
• The Halo Occupation Distribution of X-ray-Bright Active Galactic Nuclei: A Comparison with Luminous Quasars
• Dark Matter Gravitational Clustering With a Long-Range Scalar Interaction
• Statistical and systematic errors in redshift-space distortion measurements from large surveys
• The dependence of galaxy clustering on stellar mass, star-formation rate and redshift at z = 0.8-2.2, with HiZELS
• The Chandra COSMOS Legacy survey: the z>3 sample
• Electroweak Phase Transition with an SU(2) Dark Sector
• A tale of two feedbacks: star-formation in the host galaxies of radio-AGN
• On the common mass scale of the Milky Way satellites
• Photo-z Performance for Precision Cosmology
• Galactic Tides and the Shape and Orientation of Dwarf Galaxy Satellites
• The VIMOS VLT Deep Survey: the group catalogue
• The Environment of Galaxies at Low Redshift
• Eppur si muove: Positional and kinematic correlations of satellite pairs in the low Z universe
• The Lopsidedness of Satellite Galaxy Systems in $\Lambda$CDM simulations
• Chemical Signature of a Major Merger in the Early Formation of Small Magellanic Cloud
• Nature versus Nurture: The curved spine of the galaxy cluster X-ray luminosity -- temperature relation
• Estimating the effective lifetime of the $z\sim 6$ quasar population from the composite proximity zone profile
• Estimating Luminosity Function Constraints from High-Redshift Galaxy Surveys
• ERGO-ML I: Inferring the assembly histories of IllustrisTNG galaxies from integral observable properties via invertible neural networks
• The merger history of the complex cluster Abell 1758: a combined weak lensing and spectroscopic view
• Close companions to Brightest Cluster Galaxies: Support for minor mergers and downsizing
• An enhanced fraction of starbursting galaxies among high Eddington ratio AGNs
• Implementation of a Parallel Tree Method on a GPU
• Galaxy pairs align with galactic filaments
• Estimates of Fast Radio Burst Dispersion Measures from Cosmological Simulations
• Effects on Galaxy Evolution: Pair Interactions versus Environment
• The galaxies that reionized the Universe
• Astrophysical constraints on massive black hole binary evolution from Pulsar Timing Arrays
• WFIRST Science Investigation Team "Cosmology with the High Latitude Survey" Annual Report 2017
• Extrinsic Sources of Scatter in the Richness-Mass Relation of Galaxy Clusters
• Supermassive Black Holes and Their Environments
• Climbing Halo Merger Trees with TreeFrog
• Planck Intermediate Results. XXXVI. Optical identification and redshifts of Planck SZ sources with telescopes in the Canary Islands Observatories
• Galaxy formation on the largest scales: The impact of astrophysics on the BAO peak
• The diverse galaxy counts in the environment of high-redshift massive black holes in Horizon-AGN
• The cosmological analysis of X-ray cluster surveys: I- A new method for interpreting number counts
• nIFTY galaxy cluster simulations III: The Similarity & Diversity of Galaxies & Subhaloes
• Luminous Red Galaxies in hierarchical cosmologies
• The SLUGGS survey: inferring the formation epochs of metal-poor and metal-rich globular clusters
• 4098 galaxy clusters to z~0.6 in the Sloan Digital Sky Survey equatorial Stripe 82
• Chandra Survey of Nearby Highly Inclined Disc Galaxies - III: Comparison with Hydrodynamical Simulations of Circumgalactic Coronae
• Probing the Radio Loud/Quiet AGN dichotomy with quasar clustering
• Black hole growth and AGN feedback under clumpy accretion
• GRAMSES: a new route to general relativistic $N$-body simulations in cosmology. Part I. Methodology and code description
• The evolution of galaxy metallicity scaling relations in cosmological hydrodynamical simulations
• Convergence properties of halo merger trees; halo and substructure merger rates across cosmic history
• The Red and Featureless Outer Disks of Nearby Spiral Galaxies
• Structural and Dynamical Properties of Galaxies in a Hierarchical Universe: Sizes and Specific Angular Momenta
• Tree method for quantum vortex dynamics
• Combining FOF and halo-based algorithms for the identification of galaxy groups
• Panchromatic SED modelling of spatially-resolved galaxies
• The insignificant evolution of the richness-mass relation of galaxy clusters
• The integrated Sachs-Wolfe effect in the AvERA cosmology
• A near-infrared study of the multi-phase outflow in the type-2 quasar J1509+0434
• Spin-dependent exotic interactions
• Weak Lensing Galaxy Cluster Field Reconstruction
• Diffuse light in the young cluster of galaxies CL J1449+0856 at z=2.07
• AzTEC half square degree survey of the SHADES fields - II. Identifications, redshifts, and evidence for large-scale structure
• The galaxy-subhalo connection in low-redshift galaxy clusters from weak gravitational lensing
• Dependence of GAMA galaxy halo masses on the cosmic web environment from 100 square degrees of KiDS weak lensing data
• The XXL survey XV: Evidence for dry merger driven BCG growth in XXL-100-GC X-ray clusters
• Cosmic Voids and Galaxy Bias in the Halo Occupation Framework
• The growth of galactic bulges through mergers in LCDM haloes revisited. I. Present-day properties
• The history of the dark and luminous side of Milky Way-like progenitors
• The Radial Orbit Instability in Collisionless N-Body Simulations
• Evidence of ongoing AGN-driven feedback in a quiescent post starburst E+A galaxy
• Magnification as a Probe of Dark Matter Halos at high redshift
• Robust determination of the major merger fraction at z = 0.6 in Groth Strip
• TDCOSMO 2025: Cosmological constraints from strong lensing time delays
• Star formation and stellar populations in the Wolf-Rayet(?) luminous compact blue galaxy IRAS 08339+6517
• Environmental Effects on the Metal Enrichment of Low Mass Galaxies in Nearby Clusters
• Isolated elliptical galaxies in the local Universe
• The 500 ks Chandra observation of the z = 6.31 QSO SDSS J1030+0524
• Searching for galaxy clusters in the Kilo-Degree Survey
• Relativistic numerical cosmology with Silent Universes
• The origin of peak-offsets in weak-lensing maps
• The mass of the Milky Way and M31 using the method of least action
• Local SDSS galaxies in the Herschel Stripe82 survey: A critical assessment of optically-derived star-formation rates
• Hubble Diagram Dispersion From Large-Scale Structure
• Testing phenomenological and theoretical models of dark matter density profiles with galaxy clusters
• Semi-Analytic Model Predictions of the Galaxy Population in Proto-clusters
• The Three Hundred Project: The influence of environment on simulated galaxy properties
• The spatial distribution of cold gas in hierarchical galaxy formation models
• Predicting the X-ray polarization of type-2 Seyfert galaxies
• The galaxy - dark matter halo connection: which galaxy properties are correlated with the host halo mass?
• Strong MgII systems in quasar and gamma-ray burst spectra
• Brighter galaxy bias: underestimating the velocity dispersions of galaxy clusters
• KAT-7 Science Verification: Cold Gas, Star Formation, and Substructure in the Nearby Antlia Cluster
• The DES view of the Eridanus supervoid and the CMB Cold Spot
• The Role of Dissipation in the Scaling Relations of Cosmological Merger Remnants
• Breaking the self-averaging properties of spatial galaxy fluctuations in the Sloan Digital Sky Survey - Data Release Six
• Looking for the first galaxies: Lensing or blank fields?
• Metal-line emission from the warm-hot intergalactic medium: II. Ultraviolet
• Multi-Component Dark Matter in a Non-Abelian Dark Sector
• The MillenniumTNG Project: The impact of baryons and massive neutrinos on high-resolution weak gravitational lensing convergence maps
• Evidence for a high-z ISW signal from supervoids in the distribution of eBOSS quasars
• GOODS-ALMA: Optically dark ALMA galaxies shed light on a cluster in formation at z = 3.5
• Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
• A coherent method for the detection and estimation of continuous gravitational wave signals using a pulsar timing array
• A parametric study of possible solutions to the high-redshift overproduction of stars in modeled dwarf galaxies
• Probing spatial homogeneity with LTB models: a detailed discussion
• Tracing galaxy populations through cosmic time: A critical test of methods for connecting the same galaxies between different redshifts at $z<3$
• Mergers and Star Formation: The environment and Stellar Mass Growth of the Progenitors of Ultra-Massive Galaxies since z = 2
• A weak gravitational lensing recalibration of the scaling relations linking the gas properties of dark halos to their mass
• The spatial clustering of mid-IR selected star forming galaxies at z ~ 1 in the GOODS fields
• Black Holes in Pseudobulges: demography and models
• The Contribution of Halos with Different Mass Ratios to the Overall Growth of Cluster-Sized Halos
• Why does the clustering of haloes depend on their formation history
• Quantification of discreteness effects in cosmological N-body simulations: II. Evolution up to shell crossing
• Comparing galaxy populations in compact and loose groups of galaxies
• Weak Lensing Observables in the Halo Model
• Warm molecular and ionized gas kinematics in the Type-2 quasar J0945+1737
• Properties of fossil groups in cosmological simulations and galaxy formation models
• The Impact of Gas Stripping and Stellar Mass Loss on Satellite Galaxy Evolution
• The High Fraction of Thin Disk Galaxies Continues to Challenge ΛCDM Cosmology
• A comparative study of satellite galaxies in Milky Way-like galaxies from HSC, DECaLS and SDSS
• Extragalactic gamma-ray signal from Dark Matter annihilation: a power spectrum based computation
• Dust emission and star formation in Stephan's Quintet
• The Group Evolution Multiwavelength Study (GEMS): the Sample and Datasets
• The New Numerical Galaxy Catalog (${\nu }^2$GC): An Updated Semi-analytic Model of Galaxy and AGN with Large Cosmological N-body Simulation
• The Size, Shape and Orientation of Cosmological Voids in the Sloan Digital Sky Survey
• Galaxy formation in the brane world I: overview and first results
• Constraints on the evolution of the relationship between HI mass and halo mass in the last 12 Gyr
• Globular Cluster Systems of Early-type Galaxies in Low-density Environments
• H I content in Coma cluster substructure
• Statistics of galaxy mergers: bridging the gap between theory and observation
• Probing the assembly history and dynamical evolution of massive black hole binaries with pulsar timing arrays
• (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies III. Environments
• Sloshing Gas in the Core of the Most Luminous Galaxy Cluster RXJ1347.5-1145
• The boundary of cosmic filaments
• Quantified HI Morphology I: Multi-Wavelengths Analysis of the THINGS Galaxies
• Cosmic Vine: A z=3.44 large-scale structure hosting massive quiescent galaxies
• Structure and substructure analysis of DAFT/FADA galaxy clusters in the [0.4-0.9] redshift range
• Primordial star clusters at extreme magnification
• The Role of Ram Pressure Stripping in the Quenching of Cluster Star Formation
• The formation history of massive cluster galaxies as revealed by CARLA
• Connecting the structure of dark matter haloes to the primordial power spectrum
• Streams Going Notts: The tidal debris finder comparison project
• The Evolving Effect Of Cosmic Web Environment On Galaxy Quenching
• A blind HI survey in the Ursa Major region
• Kinematics of Simulated Galaxies II: Probing the Stellar Kinematics of Galaxies out to Large Radii
• The core of the massive cluster merger MACS J0417.5-1154 as seen by VLT/MUSE
• Precision Tests of CO and [CII] Power Spectra Models against Simulated Intensity Maps
• Mixed dark matter: matter power spectrum and halo mass function
• Statistics of Substructures in Dark Matter Haloes
• Discovery of a Supercluster in the eROSITA Final Equatorial Depth Survey: X-ray Properties, Radio Halo, and Double Relics
• Numerical simulations of dwarf galaxy merger trees
• Galaxy formation in the PLANCK cosmology - III. The high-redshift universe
• Age and metallicity gradients in fossil ellipticals
• A measurement of galaxy halo mass from the surrounding HI Lyα absorption
• "Grandeur in this view of life": N-body simulation models of the Galactic habitable zone
• Characterising superclusters with the galaxy cluster distribution
• The Clustering and Host Halos of Galaxy Mergers at High Redshift
• Can giant radio halos probe the merging rate of galaxy clusters?
• The 6dF Galaxy Survey: Dependence of halo occupation on stellar mass
• The MillenniumTNG Project: Intrinsic alignments of galaxies and halos
• The Impact of Environment on the Stellar Mass - Halo Mass Relation
• Testing Cold Dark Matter with the hierarchical buildup of stellar light
• Variation of the subhalo abundance in dark matter halos
• Simulations of Quintessential Cold Dark Matter: beyond the cosmological constant
• The effect of non-equilibrium metal cooling on the interstellar medium
• Vortex density fluctuations in quantum turbulence
• Accelerated galaxy growth and environmental quenching in a protocluster at z=3.24
• Optimal non-linear transformations for large scale structure statistics
• Formation of massive disk galaxies in the IllustrisTNG simulation
• Mock observations with the Millennium simulation: Cosmological downsizing and intermediate redshift observations
• Non-circular motions and the cusp-core discrepancy in dwarf galaxies
• The challenge of large and empty voids in the SDSS DR7 redshift survey
• A Robust Measure of Cosmic Structure beyond the Power-Spectrum: Cosmic Filaments and the Temperature of Dark Matter
• An extremely dense group of massive galaxies at the centre of the protocluster at z = 3.09 in the SSA22 field
• Voids and the Cosmic Web: cosmic depressions & spatial complexity
• The VIMOS-VLT Deep Survey: Evolution in the Halo Occupation Number since z $\sim$ 1
• Precise Cosmological Constraints from BOSS Galaxy Clustering with a Simulation-Based Emulator of the Wavelet Scattering Transform
• The bright end of the colour-magnitude relation of cluster galaxies
• Adaptive Mesh Refinement Simulations of the Ionization Structure and Kinematics of Damped Ly$\alpha$ Systems with Self-consistent Radiative Transfer
• Gas accretion regulates the scatter of the mass-metallicity relation
• Identification of filamentary structures in the environment of superclusters of galaxies in the Local Universe
• ORCA: The Overdense Red-sequence Cluster Algorithm
• Spectro-photometric close pairs in GOODS-S: major and minor companions of intermediate-mass galaxies
• GBT Detection of Polarization-dependent HI Absorption and HI Outflows in Local ULIRGs and Quasars
• The Role of Active Galactic Nuclei in the Quenching of Massive Galaxies in the SQuiGGLE Survey
• Exact nonlinear inhomogeneities in $\Lambda$CDM cosmology
• What triggers black-hole growth? Insights from star formation rates
• The lack of star formation gradients in galaxy groups up to z~1.6
• Reproducing cosmic evolution of galaxy population from $z=4$ to $0$
• Galaxy assembly bias of central galaxies in the Illustris simulation
• Rejuvenating the Matter Power Spectrum III: The Cosmology Sensitivity of Gaussianized Power Spectra
• SEAGLE - I: A pipeline for simulating and modeling strong lenses from cosmological hydrodynamic simulations
• Galaxy environments over cosmic time: the non-evolving radial galaxy distributions around massive galaxies since z=1.6
• Spatial and luminosity distributions of galactic satellites
• Group quenching and galactic conformity at low redshift
• Strong lensing statistics in large, z~<0.2 surveys: bias in the lens galaxy population
• Ultra-Red Galaxies Signpost Candidate Proto-Clusters at High Redshift
• The Impact of Observing Strategy on Cosmological Constraints with LSST
• Newtonian versus relativistic cosmology
• Multiple Dark Matter as a self-regulating mechanism for dark sector interactions
• The close pair fraction of BCGs since $z=0.5$: major mergers dominate recent BCG stellar mass growth
• Rotation of Cosmic Voids and Void-Spin Statistics
• Very Compact Dense Galaxy Overdensity with δ ~ 130 Identified at z ~ 8: Implications for Early Protocluster and Cluster-Core Formation
• The WSRT ZoA Perseus-Pisces Filament wide-field HI imaging survey I. HI catalogue and atlas
• How Does Radio AGN Feedback Feed Back?
• Insight Into the Formation of the Milky Way Through Cold Halo Substructure. II. The Elemental Abundances of ECHOS
• ELUCID. VI: Cosmic variance of galaxy distribution in the local Universe
• Semi-analytic galaxy formation in f(R)-gravity cosmologies
• Individual and Group Galaxies in CNOC1 clusters
• Scale dependence of galaxy biasing investigated by weak gravitational lensing: An assessment using semi-analytic galaxies and simulated lensing data
• Ram pressure stripping of disk galaxies in galaxy clusters
• Mass and Metallicity Requirement in Stellar Models for Galactic Chemical Evolution Applications
• An optical view of the filament region of Abell 85
• Low-power radio galaxy environments in the Subaru/XMM-Newton Deep Field at z~0.5
• The HI Velocity Function: a test of cosmology or baryon physics?
• Tidal Stripping in the Adiabatic Limit
• The kinematics of globular cluster populations in the E-MOSAICS simulations and their implications for the assembly history of the Milky Way
• No Evidence for Millimeter Continuum Source Overdensities in the Environments of $z\gtrsim 6$ Quasars
• The evolution of the star formation rate function and cosmic star formation rate density of galaxies at $z\sim 1-4$
• Overdensities of Submillimetre-Bright Sources around Candidate Protocluster Cores Selected from the South Pole Telescope Survey
• Soft coincidence in late acceleration
• ACCESS: NIR Luminosity Function and Stellar Mass Function of Galaxies in the Shapley Supercluster Environment
• Galaxy And Mass Assembly: search for a population of high-entropy galaxy groups
• The Mass Function of Unprocessed Dark Matter Halos and Merger Tree Branching Rates
• Stochastic angular momentum slews and flips and their effect on discs in galaxy formation models
• Tomographic Intensity Mapping versus Galaxy Surveys: Observing the Universe in H-alpha emission with new generation instruments
• Compact groups in theory and practice -- IV. The connection to large-scale structure
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• Cosmological simulation in tides: power spectra and halo shape responses, and shape assembly bias
• Formation and Evolution of Early-Type Galaxies. III Star formation history as a function of mass and over-density
• Effects of large-scale environment on the assembly history of central galaxies
• Large-scale fluctuations in the distribution of galaxies from the Two Degree Field Galaxy Redshift Survey
• Stability of Cool Cores During Galaxy Cluster Growth: A Joint $Chandra$/SPT Analysis of 67 Galaxy Clusters Along a Common Evolutionary Track Spanning 9 Gyr
• The DESI $N$-body Simulation Project I: Testing the Robustness of Simulations for the DESI Dark Time Survey
• Evolution of the cluster optical galaxy luminosity function in the CFHTLS : breaking the degeneracy between mass and redshift
• A First Look at creating mock catalogs with machine learning techniques
• Cosmology with clusters of galaxies
• Forward and backward galaxy evolution in comoving number density space
• Extensions to the halo occupation distribution model for more accurate clustering predictions
• The New Numerical Galaxy Catalogue (ν^2 GC): Properties of Active Galactic Nuclei and Their Host Galaxies
• Fully-Coupled Simulation of Cosmic Reionization. I: Numerical Methods and Tests
• Abundances, masses, and weak-lensing mass profiles of galaxy clusters as a function of richness and luminosity in LambdaCDM cosmologies
• The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3
• Post-Newtonian Cosmological Modelling
• Strong lensing of submillimetre galaxies: A tracer of foreground structure?
• Multiple non-spherical structures from the extrema of Szekeres scalars
• And In The Darkness Unbind Them: High-Resolution Simulations of Dark Matter Subhalo Disruption in a Milky Way-like Tidal Field
• Influence of baryons on the orbital structure of dark matter haloes
• The Optical Luminosity Function of Void Galaxies in the SDSS and ALFALFA Surveys
• The Galaxy--Halo Connection in High-Redshift Universe: Details and Evolution of Stellar-to-Halo Mass Ratios of Lyman Break Galaxies on CFHTLS Deep Fields
• Physical properties of simulated galaxy populations at z=2 - II. Effects of cosmology, reionization and ISM physics
• Weak lensing study of 16 DAFT/FADA clusters: substructures and filaments
• Brightest galaxies as halo centre tracers in SDSS DR7
• X-ray and SZ constraints on the properties of hot CGM
• Discovery of an Overdensity of Lyman-alpha Emitters Around a $\mathrm{z}\sim 4$ QSO with the Large Binocular Telescope
• Strongly Coupled Dark Energy Cosmologies: preserving LCDM success and easing low scale problems II - Cosmological simulations
• Linear bias forecasts for emission line cosmological surveys
• Simulating the Complexity of the Dark Matter Sheet I: Numerical Algorithms
• LOFAR insights into the epoch of reionization from the cross power spectrum of 21cm emission and galaxies
• The XMM Cluster Survey: Evidence for energy injection at high redshift from evolution of the X-ray luminosity-temperature relation
• Bounding the mass of ultralight bosonic Dark Matter particles with the motion of the S2 star around Sgr A*
• A Spectroscopic Survey of the Fields of 28 Strong Gravitational Lenses: The Redshift Catalog
• Probing wave-optics effects and low-mass dark matter halos with lensing of gravitational waves from massive black holes
• Relative clustering and the joint halo occupation distribution of red-sequence and blue-cloud galaxies in COMBO-17
• The metallicity properties of simulated long-GRB galaxy hosts and the Fundamental Metallicity Relation
• Kelvin-Helmholtz Instability in Self-Gravitating Streams
• Triaxial collapse and virialisation of dark-matter haloes
• Observed Properties of Dark Matter on Small Spatial Scales
• The need for obscured supermassive black hole growth to explain quasar proximity zones in the epoch of reionization
• Applying the Analytic Theory of Colliding Ring Galaxies
• The ALHAMBRA survey: evolution of galaxy clustering since $z\sim 1$
• Constraining SIDM with halo shapes: revisited predictions from realistic simulations of early-type galaxies
• Sufficient observables for large scale structure in galaxy surveys
• Deviations from tidal torque theory: evolution of the halo spin-filament alignment
• Adaptive gravitational softening in GADGET
• The Largest Gravitationally Bound Structures: The Corona Borealis Supercluster - Mass and Bound Extent
• Baryon acoustic oscillations reconstruction using convolutional neural networks
• The MUSIC of Galaxy Clusters III: Properties, evolution and Y-M scaling relation of protoclusters of galaxies
• CFHTLenS: Higher-order galaxy-mass correlations probed by galaxy-galaxy-galaxy lensing
• Convergence of Galaxy Properties with Merger Tree Temporal Resolution
• Dark Matter
• A Petal of the Sunflower: Photometry of the Stellar Tidal Stream in the Halo of Messier 63 (NGC 5055)
• Turbulence in the Intergalactic Medium
• MaGICC-WDM: the effects of warm dark matter in hydrodynamical simulations of disc galaxy formation
• A Robust Estimator of the Small-Scale Galaxy Correlation Function
• Effects Of Circum-nuclear Disk Gas Evolution And The Spin Of Central Black Holes
• Cluster-Supercluster Alignments
• The role of massive halos in the Star Formation History of the Universe
• Cool circumgalactic gas of passive galaxies from cosmological inflow
• The Dearth of Chemically Enriched Warm-Hot Circumgalactic Gas
• Testing homogeneity in the Sloan Digital Sky Survey Data Release Twelve with Shannon entropy
• Preprocessing Among the Infalling Galaxy Population of EDisCS Clusters
• Large Scale Structure in Absorption: Gas within and around Galaxy Voids
• Abell 2744: Too much substructure for Lambda CDM?
• Evolution of active galactic nuclei
• The cosmic evolution of massive black holes and galaxy spheroids: global constraints at redshift z<~1.2
• Combining Semi-analytic Models with Simulations of Galaxy Clusters: the Need for Heating from Active Galactic Nuclei
• Modeling Galaxy-Galaxy Weak Lensing with SDSS Groups
• The evolution of the UV-to-mm extragalactic background light: evidence for a top-heavy initial mass function?
• Gravitational redshift and asymmetric redshift-space distortions for stacked clusters
• Black hole clustering and duty cycles in the Illustris simulation
• Cosmological simulations of massive black hole seeds: predictions for next generation electromagnetic and gravitational wave observations
• Distribution of the very first PopIII stars and their relation to bright z~6 quasars
• Power Spectra to 1% Accuracy between Dynamical Dark Energy Cosmologies
• Optical validation and characterization of Planck PSZ1 sources at the Canary Islands observatories. I. First year of ITP13 observations
• The evolution of the galaxy content of dark matter haloes
• Full-sky ray-tracing simulation of weak lensing using ELUCID simulations: exploring galaxy intrinsic alignment and cosmic shear correlations
• The impact of AGN-driven winds on physical and observable galaxy sizes
• An optical and X-ray study of the fossil group RX J1340.6+4018
• Evolution of the Major Merger Galaxy Pair Fraction at z < 1
• Radio signatures from encounters between Neutron Stars and QCD-Axion Minihalos around Primordial Black Holes
• Lyman Alpha and MgII as Probes of Galaxies and their Environments
• The Effect of Coupled Dark Energy on the Alignment between Dark Matter and Galaxy Distributions in Clusters
• Merger and Ring Galaxy Formation Rates at z<=2
• The physical drivers of the atomic hydrogen-halo mass relation
• Towards accurate modelling of the ISW effect, the non-linear contribution
• HerMES: SPIRE/Sub-millimetre Emission from Radio Selected AGN
• A new twist to an old story: HE 0450-2958, and the ULIRG$\to$(optically bright QSO) transition hypothesis
• The Origin of the Hubble Sequence in Lambda-CDM Cosmology
• Linking haloes to galaxies: how many halo properties are needed?
• Extragalactic gamma-ray signal from dark matter annihilation: an appraisal
• Nonlinearity in the dynamics of photoinduced nucleation process
• The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching
• No Ly$\alpha$ emitters detected around a QSO at z=6.4: Suppressed by the QSO?
• What determines large scale galaxy clustering: halo mass or local density?
• Powerful quasar outflow in a massive disc galaxy at $z\sim 5$
• Dissecting the Red Sequence. IV. The Role of Truncation in the Two-Dimensional Family of Early-Type Galaxy Star Formation Histories
• Disentangling dark sector models using weak lensing statistics
• I. Apples to apples $A^2$: realistic galaxy simulated catalogs and photometric redshift predictions for next-generation surveys
• Strong stellar-driven outflows shape the evolution of galaxies at cosmic dawn
• The Fundamental Relation between Halo Mass and Galaxy Group Properties
• Are the halo occupation predictions consistent with large scale galaxy clustering?
• Tidal Torquing of Elliptical Galaxies in Cluster Environments
• The OH line contamination of 21 cm intensity fluctuation measurements for z=1~4
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• Reconstructing the galaxy density field with photometric redshifts: I. Methodology and validation on stellar mass functions
• How covariant is the galaxy luminosity function?
• Shadow of black hole surrounded by magnetized plasma: Axion-plasmon cloud
• On the orbital and internal evolution of cluster galaxies
• VLBI studies of DAGN and SMBHB hosting galaxies
• The spatial distribution of Milky Way satellites, gaps in streams and the nature of dark matter
• The mass function dependence on the dynamical state of dark matter haloes
• On the contribution of large scale structure to strong gravitational lensing
• Galaxy populations in massive z=0.2-0.9 clusters: I. Analysis of spectroscopy
• The evolution of the mass-metallicity relations from the VANDELS survey and the GAEA Semi-Analytic model
• Galaxy Bias and ${\sigma }_8$ from Counts in Cells from the SDSS Main Sample
• The fraction of early-type galaxies in low redshift groups and clusters of galaxies
• Stellar halos from The Dragonfly Edge-on Galaxies Survey
• The cosmological dependence of halo and galaxy assembly bias
• Groups in the Millennium Simulation and in SDSS DR7
• Probing dark energy with future redshift surveys: A comparison of emission line and broad band selection in the near infrared
• Redshift-Space Enhancement of Line-of-Sight Baryon Acoustic Oscillations in the SDSS Main-Galaxy Sample
• Dwarf spheroidal galaxies and Bose-Einstein condensate dark matter
• The Physical Origin of Galactic Conformity: From Theory to Observation
• The Nonlinear Evolution of Galaxy Intrinsic Alignments
• Early Black Holes in Cosmological Simulations: Luminosity Functions and Clustering Behaviour
• The effects of massive neutrinos on the linear point of the correlation function
• The WFC3 Galactic Bulge Treasury Program: A First Look at Resolved Stellar Population Tools
• An Extremely Deep Wide-Field Near-Infrared Survey: Bright Galaxy Counts and Local Large Scale Structure
• The mass discrepancy-acceleration relation: a universal maximum dark matter acceleration and implications for the ultra-light scalar field dark matter model
• The SPLASH survey: Quiescent galaxies are more strongly clustered but are not necessarily located in high-density environments
• Testing keV sterile neutrino dark matter in future direct detection experiments
• Galaxy evolution in merging clusters: The passive core of the "Train Wreck" cluster of galaxies, A520
• Candidate Clusters of Galaxies at $z>1.3$ Identified in the Spitzer SPT Deep Field Survey
• Dilution in elliptical galaxies: Implications for the relation between metallicity, stellar mass and star formation rate
• Dark-ages Reionization & Galaxy Formation Simulation II: Spin and concentration parameters for dark matter haloes during the Epoch of Reionization
• The influence of halo assembly on galaxies and galaxy groups
• Galaxy Formation in Heavily Overdense Regions at z~10: the Prevalence of Disks in Massive Halos
• Remapping dark matter halo catalogues between cosmological simulations
• Computational Physics on Graphics Processing Units
• Perturbation Theory for BAO reconstructed fields: one-loop results in real-space matter density field
• Super massive black holes in star forming gaseous circumnuclear discs
• The optimal gravitational softening length for cosmological N-body simulations
• Gas cooling in semi-analytic models and SPH simulations: are results consistent?
• AGN feedback and the origin of the $\alpha$ enhancement in early type galaxies - insights from the GAEA model
• Galaxy populations in the Hydra I cluster from the VEGAS survey I. Optical properties of a large sample of dwarf galaxies
• Galaxy groups in the 2MASS Redshift Survey
• Molecular cloud regulated star formation in galaxies
• History and destiny of an emerging early-type galaxy: New IFU insights on the major-merger remnant NGC7252
• A new approach to determine optically thick H2 cooling and its effect on primordial star formation
• Galaxy Zoo: Multi-Mergers and the Millennium Simulation
• Narrow-band surveys for very high redshift Lyman-alpha emitters
• Constraining the halo mass function with observations
• Galactic magnetic fields and hierarchical galaxy formation
• VINTERGATAN-GM: The cosmological imprints of early mergers on Milky-Way-mass galaxies
• Detecting neutral hydrogen in emission at redshift z ~ 1
• Cosmology dependence of galaxy cluster scaling relations
• Probing dark energy models with extreme pairwise velocities of galaxy clusters from the DEUS-FUR simulations
• The Orientation of Galaxies in Galaxy Clusters
• Cosmicflows-3: The South Pole Wall
• Non-universality of halo profiles and implications for dark matter experiments
• Multi-wavelength properties of radio and machine-learning identified counterparts to submillimeter sources in S2COSMOS
• Approximating photo-$z$ PDFs for large surveys
• CFHTLenS: Weak lensing constraints on the ellipticity of galaxy-scale matter haloes and the galaxy-halo misalignment
• ELUCID V. Lighting dark matter halos with galaxies
• The Lack of Structural and Dynamical Evolution of Elliptical Galaxies since z ~ 1.5: Clues from Self-Consistent Hydrodynamical Simulations
• Possible identification of massive and evolved galaxies At z > 5
• How AGN feedback drives the size growth of the first quasars
• Non-fiducial cosmological test from geometrical and dynamical distortions around voids
• On the recovery of Local Group motion from galaxy redshift surveys
• Dark Matter Subhalos and the X-ray Morphology of the Coma Cluster
• Clipping the Cosmos II: Cosmological information from non-linear scales
• Probing the Existence of a Dark Matter Isothermal Core Using Gravity Modes
• Luminous Red Galaxies in Simulations: Cosmic Chronometers?
• Complex structures in galaxy cluster fields: implications for gravitational lensing mass models
• The host galaxies of z=7 quasars: predictions from the BlueTides simulation
• Leveraging 3D-HST Grism Redshifts to Quantify Photometric Redshift Performance
• On Physical Scales of Dark Matter Halos
• Massive elliptical galaxies : From cores to haloes
• Massive, red galaxies in a hierarchical universe I. Counts of Extremely Red Objects and basic properties
• Dissecting Galaxy Formation: II. Comparing Substructure in Pure Dark Matter and Baryonic Models
• Formation, Evolution and Properties of Isolated Field Elliptical Galaxies
• Mapping the stellar population and gas excitation of MaNGA galaxies with MEGACUBES. Results for AGN versus control sample
• Some statistical remarks on the Giant GRB Ring
• Structure in the 3D Galaxy Distribution: I. Methods and Example Results
• The Three Hundred Project: Substructure in hydrodynamical and dark matter simulations of galaxy groups around clusters
• The QSO proximity effect at redshift <z>=2.6 with the FLO approach
• Mapping the large scale structure around a z=1.46 galaxy cluster in 3-D using two adjacent narrow-band filters
• Local stability of a gravitating filament: a dispersion relation
• The Effects of Varying Cosmological Parameters on Halo Substructure
• The Galaxy-Halo Connection for $1.5\lesssim z\lesssim 5$ as revealed by the \emph{Spitzer} Matching survey of the UltraVISTA ultra-deep Stripes
• The Dark Side of QSO Formation at High Redshifts
• The MillenniumTNG Project: The large-scale clustering of galaxies
• The missing dwarf galaxies of the Local Group
• ETHOS -- An effective parametrization and classification for structure formation: the non-linear regime at $z\gtrsim 5$
• Conditional Mass Functions and Merger Rates of Dark Matter Halos in the Ellipsoidal Collapse Model
• Galactic conformity measured in semi-analytic models
• How accurate is it to update the cosmology of your halo catalogues?
• Age and Metallicities of Cluster Galaxies: A1185 and Coma
• Clarifying Forecasts of Dark Energy Constraints from Baryon Acoustic Oscillations
• Mass segregation trends in SDSS galaxy groups
• Photometric Redshifts with the LSST II: The Impact of Near-Infrared and Near-Ultraviolet Photometry
• The Core-Cusp Problem Revisited: ULDM vs. CDM
• Revealing the cosmic reionisation history with fast radio bursts in the era of Square Kilometre Array
• Probing features in the primordial perturbation spectrum with large-scale structure data
• Probing the dark-matter halos of cluster galaxies with weak lensing
• Cosmological Newtonian limits on large spacetime scales
• Rapid build-up of the stellar content in the protocluster core SPT2349$-$56 at $z=4.3$
• Understanding the shape of the galaxy two-point correlation function at z~1 in the COSMOS field
• Imaging the Cosmic Matter Distribution using Gravitational Lensing of Pregalactic HI
• ALMA reveals large overdensity and strong clustering of galaxies in quasar environments at $z\sim 4$
• From EMBER to FIRE: predicting high resolution baryon fields from dark matter simulations with Deep Learning
• What do simulations predict for the galaxy stellar mass function and its evolution in different environments?
• Small Bites: Star formation recipes in extreme dwarfs
• A Subhalo-Galaxy Correspondence Model of Galaxy Formation
• Massive quiescent galaxies at $z\sim 3$: a comparison of selection, stellar population and structural properties with simulation predictions
• S0 galaxies in the Coma cluster: Environmental dependence of the S0 offset from the Tully-Fisher relation
• On the buildup of massive early-type galaxies at z<~1. I- Reconciling their hierarchical assembly with mass-downsizing
• The candidate cluster and protocluster catalog (CCPC) II: Spectroscopically identified structures spanning 2 < z < 6.6
• Charming Dark Matter
• Wide-Field Optical Spectroscopy of Abell 133: A Search for Filaments Reported in X-ray Observations
• The dusty, albeit ultraviolet bright infancy of galaxies
• The Evolution of Star Formation Activity in Cluster Galaxies Over $0.15<z<1.5$
• Collisionless Stellar Hydrodynamics as an Efficient Alternative to N-body Methods
• Implications of the remarkable homogeneity of galaxy groups and clusters
• Cosmological gravity on all scales II: Model independent modified gravity $N$-body simulations
• The stellar halo in Local Group Hestia simulations I. The in-situ component and the effect of mergers
• Persistent fluctuations in the distribution of galaxies from the Two degree Field Galaxy Redshift Survey
• Evolution of galaxy groups in the Illustris simulation
• Associating Host Galaxy Candidates to Massive Black Hole Binaries resolved by Pulsar Timing Arrays
• The growth of galactic bulges through mergers in LCDM haloes revisited. II. Morphological mix evolution
• Ionized Outflows in Nearby Quasars are Poorly Coupled to their Host Galaxies
• Stellar Mass Growth of Brightest Cluster Galaxy Progenitors in COSMOS Since z ~ 3
• Characteristic Scales of Baryon Acoustic Oscillations from Perturbation Theory: Non-linearity and Redshift-Space Distortion Effects
• The GOGREEN survey: the internal dynamics of clusters of galaxies at redshift 0.9-1.4
• The star-formation history of mass-selected galaxies from the VIDEO survey
• Investigating The Growing Population of Massive Quiescent Galaxies at Cosmic Noon
• Statistics of Dark Matter Halos from the Excursion Set Approach
• Obscured and powerful AGN and starburst activities at z~3.5
• Measures of galaxy environment -- II. Rank-ordered mark correlations
• Revisiting the Lensed Fraction of High-Redshift Quasars
• A unified model for the clustering of quasars and galaxies at $z\approx 6$
• Testing for a large local void by investigating the Near-Infrared Galaxy Luminosity Function
• Decoding the spectra of SDSS early-type galaxies: New indicators of age and recent star formation
• Infrared-Faint Radio Sources: A Cosmological View - AGN Number Counts, the Cosmic X-Ray Background and SMBH Formation
• Evidence for the line of sight structure in the largest Hubble Frontier Field cluster, MACSJ0717.5+3745
• The Luminosity Function of bright QSOs at z~4 and implications for the cosmic ionizing background
• On the stellar populations of massive galaxies
• Testing the homogeneity of the Universe using gamma-ray bursts
• Lensed arc statistics: comparison of Millennium-simulation galaxy clusters to Hubble Space Telescope observations of an X-ray selected sample
• Gemini NIFS survey of feeding and feedback processes in nearby Active Galaxies: VI -- Stellar Populations
• The connection between the cusp-to-core transformation and observational universalities of DM halos
• Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.2$\lesssim$$z$$\lesssim$0.9
• The Escape Fraction of Ionizing Photons During the Epoch of Reionization: observability with the Square Kilometre Array
• Detecting and Characterizing Mg II absorption in DESI Survey Validation Quasar Spectra
• Euclid preparation III. Galaxy cluster detection in the wide photometric survey, performance and algorithm selection
• The Magnetic Field of the Irregular Galaxy NGC 4214
• Evolution of [OIII]5007 emission-line profiles in narrow emission-line galaxies
• Targeting supermassive black hole binaries and gravitational wave sources for the pulsar timing array
• Spin Flips - II. Evolution of dark matter halo spin orientation, and its correlation with major mergers
• The HST/ACS Coma Cluster Survey - VII. Structure and Assembly of Massive Galaxies in the Center of the Coma Cluster
• Characterizing dark interactions with the halo mass accretion history and structural properties
• Why are AGN found in High Mass Galaxies?
• Spectroscopic Confirmation of two Extremely Massive Protoclusters BOSS1244 and BOSS1542 at $z=2.24$
• The clustering of the first galaxy halos
• Evolution of compact and fossil groups of galaxies from semi-analytical models of galaxy formation
• A Study of Outflows in Luminous Quasars at Redshift $\sim 0.4-0.8$
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• The evolution of streams in a time-dependent potential
• Do group dynamics play a role in the evolution of member galaxies?
• Living with Neighbors. I. Observational Clues to Hydrodynamic Impact of Neighboring Galaxies on Star Formation
• Four dual AGN candidates observed with the VLBA
• The dark side of galaxy stellar populations I: The stellar-to-halo mass relation and the velocity dispersion - halo mass relation
• Effect of inhomogeneities on high precision measurements of cosmological distances
• Determining neutrino properties using future galaxy redshift surveys
• No evidence for a significant evolution of $M_{\bullet }$-$M_{\ast }$ relation in massive galaxies up to z$\sim$4
• DustPedia - the relationships between stars, gas and dust for galaxies residing in different environments
• Flat Rotation Curves of $z\sim 1$ Star-Forming Galaxies and Evidence of Disk-Scale Length Evolution
• A new methodology to test galaxy formation models using the dependence of clustering on stellar mass
• The zCOSMOS-Bright survey: the clustering of early and late galaxy morphological types since z~1
• Multiband gravitational wave cosmology with stellar origin black hole binaries
• Bayesian weak lensing tomography: Reconstructing the 3D large-scale distribution of matter with a lognormal prior
• The evolution of galaxy star formation activity in massive halos
• Effects of Inner Halo Angular Momentum on the Peanut/X-shapes of Bars
• Intergalactic filaments spin
• Fuzzy dark matter black holes and droplets
• CUBE: An Information-optimized parallel Cosmological $N$-body Algorithm
• HACC Cosmological Simulations: First Data Release
• Properties of Galaxies in Cosmic Filaments around the Virgo Cluster
• RESOLVE and ECO: The Halo Mass-Dependent Shape of Galaxy Stellar and Baryonic Mass Functions
• Environments of Nearby Quasars in Sloan Digital Sky Survey
• Observational evidence that positive and negative AGN feedback depends on galaxy mass and jet power
• A new method for the determination of the growth rate from galaxy redshift surveys
• Measures of Galaxy Environment - III. Difficulties in identifying proto-clusters at z ~ 2
• A roadmap to cosmological parameter analysis with third-order shear statistics I: Modelling and validation
• Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
• The effects of halo alignment and shape on the clustering of galaxies
• The ultra-diffuse dwarf galaxies NGC 1052-DF2 and 1052-DF4 are in conflict with standard cosmology
• UniverseMachine: Predicting Galaxy Star Formation over Seven Decades of Halo Mass with Zoom-in Simulations
• The formation and evolution of star clusters in interacting galaxies
• The halo light cone catalogues of \Abacus{AbacusSummit}
• Scaling relations between numerical simulations and physical systems they represent
• Weak Lensing Peaks in Simulated Light-Cones: Investigating the Coupling between Dark Matter and Dark Energy
• Robotic Reverberation Mapping of the Southern Seyfert NGC 3783
• The halo mass function and inner structure of ETHOS haloes at high redshift
• Evolution of environment dependent galaxy properties in the Sloan Digital Sky Survey
• Evolutionary Map of the Universe: Tracing Clusters to High Redshift
• New insights on the recoiling/binary black hole candidate J0927+2943 via molecular gas observations
• Quenching or Bursting: the Role of Stellar Mass, Environment, and Specific Star Formation Rate to $z$ $\sim$ 1
• H0LiCOW XI. A weak lensing measurement of the external convergence in the field of the lensed quasar B1608+656 using HST and Subaru deep imaging
• From the core to the outskirts: structure analysis of three massive galaxy clusters
• Spatial Clustering of High Redshift Lyman Break Galaxies
• Evolution in the Disks and Bulges of Group Galaxies since z=0.4
• Driving the Growth of the Earliest Supermassive Black Holes with Major Mergers of Host Galaxies
• Non-Spherical Szekeres models in the language of Cosmological Perturbations
• Testing the Evolution of the Correlations between Supermassive Black Holes and their Host Galaxies using Eight Strongly Lensed Quasars
• Confronting Cold Dark Matter Predictions with Observed Galaxy Rotations
• Properties of Long Gamma-Ray Burst Host Galaxies in Cosmological Simulation
• Constructing high-fidelity halo merger trees in AbacusSummit
• Measuring the Density Fields around Bright Quasars at $z\sim 6$ with XQR-30 Spectra
• Electromagnetic signatures of supermassive black hole binaries resolved by PTAs
• The Clustering Evolution of Dusty Star-Forming Galaxies
• The Effect of Tidal Stripping on Composite Stellar Populations in Dwarf Spheroidal Galaxies
• The DESI PRObabilistic Value-Added Bright Galaxy Survey (PROVABGS) Mock Challenge
• The Three Hundred project: galaxy cluster mergers and their impact on the stellar component of brightest cluster galaxies
• The stellar halo in Local Group Hestia simulations III. Chemical abundance relations for accreted and in-situ stars
• Taking advantage of photometric galaxy catalogues to determine the halo occupation distribution
• On the Cosmic Web Elongation in Fuzzy Dark Matter Cosmologies: Effects on Density Profiles, Shapes and Alignments of Halos
• On the scatter in the relation between stellar mass and halo mass: random or halo formation time dependent?
• Radio galaxies in ZFOURGE/NMBS: no difference in the properties of massive galaxies with and without radio-AGN out to z = 2.25
• Light versus dark in strong-lens galaxies: Dark matter haloes that are rounder than their stars
• The effect of stellar and AGN feedback on the low redshift Lyman-$\alpha$ forest in the Sherwood simulation suite
• SDSS-IV MaNGA: Signatures of halo assembly in kinematically misaligned galaxies
• Accurate initial conditions in mixed Dark Matter--Baryon simulations
• DETECTIFz galaxy groups in the REFINE survey -- 1. Group detection and quenched fraction evolution at $z<2.5$
• The dark matter halo shape of edge-on disk galaxies - I. HI observations
• Modeling the QSO luminosity and spatial clustering at low redshifts
• Probing Dark Energy with Baryonic Acoustic Oscillations at High Redshifts
• Studying Inter-Cluster Galaxy Filaments Through Stacking GMBCG Galaxy Cluster Pairs
• The impact of inelastic self-interacting dark matter on the dark matter structure of a Milky Way halo
• Massive relic galaxies prefer dense environments
• Large-scale Structure and Dynamics of the Most X-ray Luminous Galaxy Cluster Known -- RX J1347-1145
• Cosmic variance in the nanohertz gravitational wave background
• The structure and evolution of a forming galaxy cluster at z = 1.62
• Discovery of Protoclusters at z~3.7 & 4.9: Embedded in Primordial Superclusters
• On the cosmological evolution of the black hole - host galaxy relation in quasars
• Stellar Kinematics and Populations of Early-Type Galaxies with the SAURON and OASIS Integral-Field Spectrographs
• MIGHTEE-HI: The relation between the HI gas in galaxies and the cosmic web
• Quark Matter Induced Extensive Air Showers
• Tracing the Mass Growth and Star Formation Rate Evolution of Massive Galaxies from z~6 to z~1 in the Hubble Ultra-Deep Field
• Dark matter powered stars: Constraints from the extragalactic background light
• Accretion-Induced Collapse of Dark Matter Admixed White Dwarfs -- I: Formation of Low-mass Neutron Stars
• The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmic Flows and Cosmic Web from Luminous Red Galaxies
• Exploring the diversity and similarity of radially anisotropic Milky Way-like stellar haloes: implications for disrupted dwarf galaxy searches
• Understanding the Unique Assembly History of Central Group Galaxies
• Galaxy clusters and groups in the ALHAMBRA Survey
• Probing Asymmetric Structures in the Outskirts of Galaxies
• A Compact Cluster of Massive Red Galaxies at a Redshift of 1.51
• Predicting sub-millimeter flux densities from global galaxy properties
• The $I\kappa \epsilon \alpha$ model of feedback-regulated galaxy formation
• Redshift evolution of stellar mass versus gas fraction relation in 0<z<2 regime: observational constraint for galaxy formation models
• SimSpin -- Constructing mock IFS kinematic data cubes
• HELP : The Herschel Extragalactic Legacy Project & The Coming of Age of Multi-Wavelength Astrophysics
• The statistics of voids as a tool to constrain cosmological parameters: sigma_8 and Omega_m h
• The VANDELS survey: Discovery of massive overdensities of galaxies at z>2
• Evolution of Group Galaxies from the First Red-Sequence Cluster Survey
• A Multiwavelength Study of Binary Quasars and Their Environments
• The median density of the Universe
• Newtonian Limits of Isolated Cosmological Systems on Long Time Scales
• The Evolution of Active Galactic Nuclei in Warm Dark Matter Cosmology
• A New Approach to Identifying the Most Powerful Gravitational Lensing Telescopes
• Morphological evolution and galactic sizes in the L-Galaxies SA model
• Gravitational Wave Hotspots: Ranking Potential Locations of Single-Source Gravitational Wave Emission
• Galaxy And Mass Assembly: Estimating galaxy group masses via caustic analysis
• Lensing Model of MACS J1149.5+2223 - I. Cluster mass reconstruction
• Influence of Projection in Cluster Cosmology Studies
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• Brightest Group Galaxies: Stellar Mass and Star Formation Rate (paper I)
• Unveiling the mask on the ULIRG-to-QSO transition object [H89]1821+643 at z=0.3: a gas-poor/gas-rich galaxy merger and the implications for CO-based dynamical mass estimates
• Suzaku observations of the type 2 QSO in the central galaxy of the Phoenix cluster
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Measuring nonlinear galaxy bias at z~0.8
• Chronology of the chemical enrichment of the old Galactic stellar populations
• Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
• Precision Prediction for the Cosmological Density Distribution
• Numerical hydrodynamic simulations based on semi-analytic galaxy merger trees: method and Milky-Way like galaxies
• Bullet Clusters in the MareNostrum Universe
• Known Unknowns of Dark Matter Annihilation over Cosmic Time
• Weak lensing mass modeling bias and the impact of miscentring
• STRIDES: Spectroscopic and photometric characterization of the environment and effects of mass along the line of sight to the gravitational lenses DES J0408-5354 and WGD 2038-4008
• The VLT LBG Redshift Survey - IV. Gas and galaxies at z ~ 3 in observations and simulations
• The AGN Luminosity Fraction in Merging Galaxies
• Precision Prediction of the Log Power Spectrum
• The Variation of the Galaxy Luminosity Function with Group Properties
• Ultramassive black holes in the most massive galaxies: $M_{\mathrm{BH}}-\sigma$ versus $M_{\mathrm{BH}}-R_{\mathrm{b}}$
• Into the Lyα jungle: exploring the circumgalactic medium of galaxies at z ~ 4-5 with MUSE
• High-resolution, 3D radiative transfer modelling V. A detailed model of the M51 interacting pair
• Galaxies at Redshift ~0.5 Around Three Closely Spaced Quasar Sightlines
• Encoding large scale cosmological structure with Generative Adversarial Networks
• Observing the First Stars and Black Holes
• What Powers the Most Relativistic Jets? II: Flat Spectrum Radio Quasars
• Evolution of the galaxy luminosity function in progenitors of fossil groups
• The WIRCam Deep Survey II: Mass Selected Clustering
• The (black hole mass)-(color) relations for early- and late-type galaxies: red and blue sequences
• Detecting Mass Substructure in Galaxy Clusters: An Aperture Mass Statistic for Gravitational Flexion
• nIFTy galaxy cluster simulations V: Investigation of the Cluster Infall Region
• Velocity and mass bias in the distribution of dark matter halos
• Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model - I. Magnitude counts, redshift distribution, colour bimodality, and galaxy clustering
• A Massive Spiral Galaxy in the Zone of Avoidance
• Galaxy And Mass Assembly (GAMA): The Bright Void Galaxy Population in the Optical and Mid-IR
• Precision Cosmology: Successes and Challenges
• Absorption signatures of warm-hot gas at low redshift: NeVIII
• A study on the statistical significance of mutual information between morphology of a galaxy and its large-scale environment
• From rest-frame luminosity functions to observer-frame colour distributions: tackling the next challenge in cosmological simulations
• The Future of Scientific Simulations: from Artificial Life to Artificial Cosmogenesis
• The Effects of Dwarf Galaxies on the Orbital Evolution of Galactic Globular Clusters
• Properties of brightest group galaxies in cosmic web filaments
• Galaxy formation in the Planck cosmology II. Star formation histories and post-processing magnitude reconstruction
• Searches for Population III pair-instability supernovae: Predictions for ULTIMATE-Subaru and WFIRST
• The actual Rees--Sciama effect from the Local Universe
• The LSST DESC Data Challenge 1: Generation and Analysis of Synthetic Images for Next Generation Surveys
• A semi-analytic model comparison: testing cooling models against hydrodynamical simulations
• Scatter in Sunyaev--Zel'dovich effect scaling relations explained by inter-cluster variance in mass accretion histories
• X-rays and hard UV radiation From the First Galaxies: Ionization Bubbles and 21 cm Observations
• Wave turbulence in self-gravitating Bose gases and nonlocal nonlinear optics
• A common explanation of the Hubble tension and anomalous cold spots in the CMB
• 21st Century Statistical and Computational Challenges in Astrophysics
• Optically selected fossil groups; X-ray observations and galaxy properties
• Pulsar timing arrays and the challenge of massive black hole binary astrophysics
• Building robust AGN mock catalogs to unveil black hole evolution and for survey planning
• A Local Leaky-box Model for the Local Stellar Surface Density - Gas Surface Density - Gas Phase Metallicity Relation
• Dark matter halo occupation: environment and clustering
• Understanding large-scale structure in the SSA22 protocluster region using cosmological simulations
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Exploring the dependence of the three-point correlation function on stellar mass and luminosity at 0.5<z<1.1
• Nuclear absorption and emission in the AGN merger NGC 6240: the hard X-ray view
• An Accurate Cluster Selection Function for the J-PAS Narrow-Band wide-field survey
• The candidate cluster and protocluster catalog (CCPC) of spectroscopically identified structures spanning $2.74<z<3.71$
• Clustering of star-forming galaxies detected in mid-infrared with the Spitzer wide-area survey
• Fossil groups in the Millennium simulation. From the brightest to the faintest galaxies during the past 8 Gyr
• The interconnection between galaxy mergers, AGN activity and rapid quenching of star formation in simulated post-merger galaxies
• Detecting nanohertz gravitational waves with pulsar timing arrays
• A hot X-ray filament associated with A3017 galaxy cluster
• PNG-UNITsims: Halo clustering response to primordial non-Gaussianities as a function of mass
• Redshift-space distortions of galaxies, clusters and AGN: testing how the accuracy of growth rate measurements depends on scales and sample selections
• Distinguishing general relativity and $f(R)$ gravity with the gravitational lensing Minkowski functionals
• Living with Neighbors. II. Statistical Analysis of Flybys and Mergers of Dark Matter Halos in Cosmological Simulations
• The Variation of Galaxy Morphological Type with the Shear of Environment
• Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups
• The nonlinear biasing of the 10k zCOSMOS galaxies up to z~1
• A Direct Measurement of the Mean Occupation Function of Quasars: Breaking Degeneracies between Halo Occupation Distribution Models
• Constructing mock catalogues for the REFLEX II galaxy cluster sample
• A clustering-based self-calibration of the richness-to-mass relation of CAMIRA galaxy clusters out to $z\approx 1.1$ in the Hyper Suprime-Cam survey
• Imprints of dark matter on the structural properties of minimally deformed compact stars
• Where can we really find the First Stars' Remnants today?
• Planes of satellites around simulated disc galaxies: I.- Finding high-quality planar configurations from positional information and their comparison to MW/M31 data
• Two phase galaxy formation: The Gas Content of Normal Galaxies
• Stellar Mass and color dependence of the three-point correlation function of galaxies in the local universe
• Galactic Warps in Triaxial Halos
• Universal Merger Histories of Dark-Matter Haloes
• Enhanced star formation in $z\sim 6$ quasar companions
• Luminosity bias: from haloes to galaxies
• Observing Merger Trees in a New Light
• KiDS+GAMA: The weak lensing calibrated stellar-to-halo mass relation of central and satellite galaxies
• On the role of feedback in shaping the cosmic abundance and clustering of neutral atomic hydrogen in galaxies
• Galaxy And Mass Assembly (GAMA): 'No Smoking' zone for giant elliptical galaxies?
• Determine the galaxy bias factors on large scales using bispectrum method
• Ultra-Compact Dwarfs in the Fossil Group NGC 1132
• The Evolution of Sizes and Specific Angular Momenta in Hierarchical Models of Galaxy Formation and Evolution
• HI Intensity Mapping for Clustering-Based Redshift Estimation
• Merger histories of brightest group galaxies from MUSE stellar kinematics
• Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
• Massive galaxy formation caught in action at z~5 with JWST
• Semi-analytic galaxy formation in early dark energy cosmologies
• Multi-wavelength scaling relations in galaxy groups: a detailed comparison of GAMA and KiDS observations to BAHAMAS simulations
• Another baryon miracle? Testing solutions to the "missing dwarfs" problem
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• Ionizing photon production and escape fractions during cosmic reionization in the TNG50 simulation
• Dark Energy Survey Year 3 results: imprints of cosmic voids and superclusters in the Planck CMB lensing map
• Halo Assembly Bias in the Quasi-linear Regime
• Subhaloes gone Notts: the clustering properties of subhaloes
• The Evolution of K* and the Halo Occupation Distribution since z=1.5: Observations vs. Simulations
• The assembly bias of emission line galaxies
• Importance of Mock Observations in Validating Galaxy Properties for Cosmological Simulations
• A z~3 radio galaxy and its protocluster: evidence for a superstructure?
• Assessing the reliability of Friends-of-Friends groups on the future Javalambre Physics of the Accelerating Universe Astrophysical Survey
• Dark Matter in Cosmology
• The galaxy correlation function as a constraint on galaxy formation physics
• Block Time Step Storage Scheme for Astrophysical N-body Simulations
• Investigation of two colliding solitonic cores in Fuzzy Dark Matter models
• S-PLUS DR1 galaxy clusters and groups catalogue using PzWav
• The Quasar Mass-Luminosity Plane II: High Mass Turnoff Evolution and a Synchronization Puzzle
• The spectroscopically confirmed huge cosmic structure at z=0.55
• A gravitational lensing detection of filamentary structures connecting luminous red galaxies
• Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
• Galaxy size trends as a consequence of cosmology
• II. Apples to apples $A^2$: cluster selection functions for next-generation surveys
• The luminosity-redshift relation in brane-worlds: II. Confrontation with experimental data
• Molecular gas and Star Formation Properties in Early Stage Mergers: SMA CO(2-1) Observations of the LIRGs NGC 3110 and NGC 232
• Effects of biasing on the galaxy power spectrum at large scales
• Perturbation theory for nonlinear halo power spectrum: the renormalized bias and halo bias
• What Sets Temperature Gradients in Galaxy Clusters? Implications for non-thermal pressure support and mass-observable scaling relations
• Evolution of the Milky Way in Semi-Analytic Models: Detecting Cold Gas at z=3 with ALMA and SKA
• Dark Matter Response to Galaxy Assembly History
• Improving Hickson-like compact group finders in redshift surveys: an implementation in the SDSS
• Herschel-ATLAS: detection of a far-infrared population around galaxy clusters
• Protocluster detection in simulations of HSC-SSP and the 10-year LSST forecast, using PCcones
• The HI mass function as a probe of photoionisation feedback on low mass galaxy formation
• The clustering of dark matter halos: scale-dependent bias on quasi-linear scales
• Exploring the Cosmic Evolution of Habitability with Galaxy Merger Trees
• Dissecting the complex environment of a distant quasar with MUSE
• Gravothermal collapse of Self-Interacting Dark Matter halos as the Origin of Intermediate Mass Black Holes in Milky Way satellites
• Mock galaxy redshift catalogues from simulations: implications for Pan-STARRS1
• A Simple Proposal for Radial 3D Needlets
• The role of Pop III stars and early black holes in the 21cm signal from Cosmic Dawn
• Luminosity distance in Swiss cheese cosmology with randomized voids. II. Magnification probability distributions
• Cold versus Warm Dark Matter simulations of a galaxy group
• The submillimetre view of massive clusters at z~0.8-1.6
• Constraining the Noise-Free Distribution of Halo Spin Parameters
• Wide and deep near-UV (360nm) galaxy counts and the extragalactic background light with the Large Binocular Camera
• Mapping the "invisible" circumgalactic medium around a z $\sim$ 4.5 radio galaxy with MUSE
• Testing approximate predictions of displacements of cosmological dark matter halos
• On the dependence of galaxy morphologies on galaxy mergers
• In the whirlpool's coils: tracing substructure from combined optical/X-ray data in the galaxy cluster A1300
• Extending Recovery of the Primordial Matter Power Spectrum
• Extension and estimation of correlations in Cold Dark Matter models
• The effect of Large Magellanic Cloud on the satellite galaxy population in Milky Way analogous Galaxies
• The gamma-ray and Optical Variability Analysis of the BL Lac Object 3FGL J0449.4-4350
• A New Model for Dark Matter Halos Hosting Quasars
• The CAVITY project. The spatially resolved stellar population properties of galaxies in voids
• Assembly history of subhalo populations in galactic and cluster sized dark haloes
• Characterising Tidal Features Around Galaxies in Cosmological Simulations
• Feedback by supermassive black holes in galaxy evolution: impacts of accretion and outflows on the star formation rate
• The distribution of dark matter and gas spanning six megaparsecs around the post-merger galaxy cluster MS0451-03
• An empirical measurement of the Halo Mass Function from the combination of GAMA DR4, SDSS DR12, and REFLEX II data
• Resolved Star Formation Efficiency in the Antennae Galaxies
• The Size Distribution of Void Filaments in a LCDM Cosmology
• Nearby Galaxies in the 2micron All Sky Survey I. K-band Luminosity Functions
• Galaxy cluster luminosities and colours, and their dependence on cluster mass and merger state
• A high-resolution cosmological simulation of a strong gravitational lens
• A new parallel simulation technique
• Dark Matter Halo Mergers I: Dependence on Environment & Redshift Evolution
• Assessing the Predictive Power of Galaxy Formation Models: A Comparison of Predicted and Observed Rest-Frame Optical Luminosity Functions at 2.0<z<3.3
• Statistics of biased tracers in variance-suppressed simulations
• Non-linear gravitational clustering of cold matter in an expanding universe: indications from 1D toy models
• The evolution of star formation activity in galaxy groups
• Stellar Mass Assembly of Brightest Cluster Galaxies at Late Times
• The MIP Ensemble Simulation: Local Ensemble Statistics in the Cosmic Web
• Gravitational Dynamics of an Infinite Shuffled Lattice: Particle Coarse-grainings, Non-linear Clustering and the Continuum Limit
• MeTACAST: Target- and Context-aware Spatial Selection in VR
• Topology of non-linear structure in the 2dF Galaxy Redshift Survey
• The dearth of difference between central and satellite galaxies II. Comparison of observations with L-GALAXIES and EAGLE in star formation quenching
• Testing the evolutionary pathways of galaxies and their supermassive black holes and the impact of feedback from Active Galactic Nuclei via large multiwavelength datasets
• The halo mass function conditioned on density from the Millennium Simulation: insights into missing baryons and galaxy mass functions
• Finding closure: approximating Vlasov-Poisson using finitely generated cumulants
• Simulation view of galaxy clusters with low X-ray surface brightness
• Clustering of SZ clusters on a past light-cone: acoustic oscillations and constraints on dark energy
• Some observational tests of a minimal galaxy formation model
• A finer view of the conditional galaxy luminosity function and magnitude-gap statistics
• Cosmological Constraints from applying SHAM to rescaled cosmological simulations
• Evolution of isolated overdensities as a control on cosmological N body simulations
• Evolution of the Stellar Mass Function and Infrared Luminosity Function of Galaxies since $z=1.2$
• The Milky Way's dark matter halo appears to be lopsided
• Effects of galaxy environment on merger fraction
• A Hybrid Fast Multipole Method for Cosmological N-body Simulations
• Mass and size growth of early-type galaxies by dry mergers in cluster environments
• Galaxies behind the Galactic plane: First results and perspectives from the VVV Survey
• Stellar Population Synthesis of star forming clumps in galaxy pairs and non-interacting spiral galaxies
• The nuclear activity and central structure of the elliptical galaxy NGC 5322
• Configuration entropy of the Cosmic Web: Can voids mimic the dark energy?
• Single Colour Diagnostics of the Mass-to-light Ratio: Predictions from Galaxy Formation Models
• Modified Dark Matter: Relating Dark Energy, Dark Matter and Baryonic Matter
• Morphological evolution of supermassive black hole merger hosts and multimessenger signatures
• Effects of center offset and noise on weak-lensing derived concentration-mass relation of dark matter halos
• Zipf's law for cosmic structures: how large are the greatest structures in the universe?
• Counts-in-Cylinders in the Sloan Digital Sky Survey with Comparisons to N-body Simulations
• The influence of Red Spiral Galaxies on the Shape of the Local K-Band Luminosity Function
• Insights from Simulations of Star Formation
• The diversity of assembly histories leading to disc galaxy formation in a LambdaCDM model
• On Mass Concentrations & Magnitude Gaps of Galaxy Systems in the CS82 Survey
• Modelling the dusty universe II: The clustering of submillimetre-selected galaxies
• SARCS strong lensing galaxy groups: I - optical, weak lensing, and scaling laws
• The IllustrisTNG Simulations: Public Data Release
• Theoretical reevaluations of the black hole mass - bulge mass relation - I. Effect of the seed black hole mass
• Fast and realistic large-scale structure from machine-learning-augmented random field simulations
• Early Black Hole Formation by Accretion of Gas and Dark Matter
• Noiseless Gravitational Lensing Simulations
• The orientations of galaxy groups and formation of the Local Supercluster
• The Adaptive TreePM: An Adaptive Resolution Code for Cosmological N-body Simulations
• The SAGA Survey. V. Modeling Satellite Systems around Milky Way-mass Galaxies with Updated UniverseMachine
• Constraints on a scale-dependent bias from galaxy clustering
• Are the 2dFGRS superstructures a problem for hierarchical models?
• Extended Tully-Fisher Relations using HI Stacking
• On the initial shear field of the cosmic web
• The MUSE-Wide survey: Detection of a clustering signal from Lyman-α-emitters at 3<z<6
• On the origin of intrinsic alignment in cosmic shear measurements: an analytic argument
• There and back again: understanding the critical properties of backsplash galaxies
• The Diversity of Growth Histories of Milky Way-mass Galaxies
• Discovery of a Supercluster at $z\sim$0.91 and Testing the $\Lambda$CDM Cosmological Model
• Fossil Groups in the Millennium Simulation: Their environment and its evolution
• The impact of the dynamical state of galaxy groups on the stellar populations of central galaxies
• Scaling Relations and X-ray Properties of Moderate-Luminosity Galaxy Clusters from 0.3 < z < 0.6 with XMM-Newton
• The complex universe: recent observations and theoretical challenges
• Network Analysis of Cosmic Structures : Network Centrality and Topological Environment
• Using member galaxy luminosities as halo mass proxies of galaxy groups
• Gas Accretion and Galactic Chemical Evolution: Theory and Observations
• Tangential Velocity of the Dark Matter in the Bullet Cluster from Precise Lensed Image Redshifts
• Milky Way type galaxies in a LCDM cosmology
• The Clustering and Halo Masses of Star Forming Galaxies at z<1
• Modelling the dusty universe I: Introducing the artificial neural network and first applications to luminosity and colour distributions
• Probability Friends-of-Friends (PFOF) Group Finder: Performance Study and Observational Data Applications on Photometric Surveys
• The Stellar Mass - Black Hole Mass Relation at $z\sim 2$ Down to ${\mathcal{M}}_{\mathrm{BH}}\sim 10^7{M}_{\odot }$ Determined by HETDEX
• Maximum Likelihood Random Galaxy Catalogues and Luminosity Function Estimation
• The Cosmic Web Around The Brightest Galaxies During The Epoch Of Reionization
• The frequency of very young galaxies in the local Universe: I. A test for galaxy formation and cosmological models
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• The spatial distribution of X-ray selected AGN in the Chandra deep fields: a theoretical perspective
• Constraining dark energy via baryon acoustic oscillations in the (an)isotropic light-cone power spectrum
• Monte Carlo Physarum Machine: Characteristics of Pattern Formation in Continuous Stochastic Transport Networks
• The First Billion Years Project: Finding Infant Globular Clusters at z=6
• Keck Deep Fields. IV. Luminosity Dependent Clustering and Galaxy Downsizing in UV-Selected Galaxies at z=4, 3, and 2
• Galaxy Clusters at 0.9<z<1.7 in the AKARI NEP deep field
• Imaging the environment of a z = 6.3 submillimeter galaxy with SCUBA-2
• Characterising the signatures of star-forming galaxies in the extra-galactic $\gamma$-ray background
• Analytical shear and flexion of Einasto dark matter haloes
• Dark-ages Reionization & Galaxy Formation Simulation VIII. Suppressed growth of dark matter halos during the Epoch of Reionization
• Generating mock galaxy catalogues for flux-limited samples like the DESI Bright Galaxy Survey
• Satellite quenching and morphological transformation of galaxies in groups and clusters
• SpatialTouch: Exploring Spatial Data Visualizations in Cross-reality
• The Baryonic Collapse Efficiency of Galaxy Groups in the RESOLVE and ECO Surveys
• Probing large scale homogeneity and periodicity in the LRG distribution using Shannon entropy
• Brightest group galaxies-II: the relative contribution of BGGs to the total baryon content of groups at z<1.3
• A Merger Tree with Microsolar Mass Resolution: Application to $\gamma$-ray Emission from Subhalo Population
• Compact groups in theory and practice - II. Comparing the observed and predicted nature of galaxies in compact groups
• Halo concentrations from extended Press-Schechter merger histories
• Evolution of the infrared Tully-Fisher relation up to z=1.4
• Hybrid analytic and machine-learned baryonic property insertion into galactic dark matter haloes
• Imaging of diffuse HI absorption structure in the SSA22 proto-cluster region at z = 3.1
• Modelling the shapes of the largest gravitationally bound objects
• Baryonic properties of nearby galaxies across the stellar-to-total dynamical mass relation
• Matter power spectra in dynamical-Dark Energy cosmologies
• What Powers the Most Relativistic Jets? I: BL Lacs
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). The matter density and baryon fraction from the galaxy power spectrum at redshift $0.6<z<1.1$
• The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations
• Evolution of dark matter velocity dispersion
• Science Pipelines for the Square Kilometre Array
• Entrainment of Hot Gas into Cold Streams: The Origin of Excessive Star-formation Rates at Cosmic Noon
• Scalar field dark matter as an alternative explanation for the anisotropic distribution of satellite galaxies
• Compactness of Cold Gas in High-Redshift Galaxies
• A new tool to determine masses and mass profiles using gravitational flexion
• Testing Dark Matter Halo Models of Quasars With Thermal Sunyaev-Zeldovich Effect
• Constraint on the mass of fuzzy dark matter from the rotation curve of the Milky Way
• A random-walk model for dark matter halo spins
• Application of the iterative reconstruction to simulated galaxy fields
• Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation
• Mass Functions, Luminosity Functions, and Completeness Measurements from Clustering Redshifts
• Probing Theories of Gravity with Phase Space-Inferred Potentials of Galaxy Clusters
• The Spitzer Extragalactic Representative Volume Survey (SERVS): The Environments of High-z SDSS Quasi-Stellar-Objects
• The Effect of Assembly Bias on Redshift Space Distortions
• Spatial Structures In the Globular Cluster Distribution of the Ten Brightest Virgo Galaxies
• Dark Energy Detected with Supervoids and Superclusters
• Topology of Luminous Red Galaxies from the Sloan Digital Sky Survey
• Towards precise galaxy evolution: a comparison between spectral indices of $z\sim 1$ galaxies in the IllustrisTNG simulation and the LEGA-C survey
• Towards optimal estimation of the galaxy power spectrum
• Spin and structural halo properties at high redshift in a LCDM Universe
• The anatomy of the NGC 5044 group -- II. Stellar populations and star-formation histories
• Statistical properties of the linear tidal shear
• Multi-Scale Morphological Analysis of SDSS DR5 Survey using the Metric Space Technique
• Large-scale Ferrofluid Simulations on Graphics Processing Units
• The SMBH mass versus M_G sigma^2 relation: A comparison between real data and numerical models
• Connections between galaxy properties and halo formation time in the cosmic web
• Physical constraints on the central mass and baryon content of satellite galaxies
• Normalization of the Matter Power Spectrum via Higher-Order Angular Correlations of Luminous Red Galaxies
• Revising the merger scenario of the galaxy cluster Abell 1644: a new gas poor structure discovered by weak gravitational lensing
• The environments of Ly$\alpha$ blobs I: Wide-field Ly$\alpha$ imaging of TN J1338-1942, a powerful radio galaxy at $z\simeq 4.1$ associated with a giant Ly$\alpha$ nebula
• Self-similarity in the chemical evolution of galaxies and the delay time distribution of SNe Ia
• The Impact of Environment on Late Time Evolution of the Stellar Mass - Halo Mass Relation
• Cosmic Star Formation: a simple model of the SFRD(z)
• POLAR -- I: linking the 21-cm signal from the epoch of reionization to galaxy formation
• Rosella: A mock catalogue from the P-Millennium simulation
• The Effects of X-Ray and UV Background Radiation on the Low-Mass Slope of the Galaxy Mass Function
• Dusty MgII Absorbers: Implications for the GRB/Quasar Incidence Discrepancy
• Revisiting the Extreme Clustering of $z\approx 4$ Quasars with Large Volume Cosmological Simulations
• The VIMOS VLT Deep Survey: Testing the gravitational instability paradigm at z ~ 1
• Dynamical History Of The Local Group In $\Lambda$CDM $\mathrm{II}$ $-$ Including External Perturbers In 3D
• The environmental dependence of neutral hydrogen in the GIMIC simulations
• A derivation of masses and total luminosities of galaxy groups and clusters in the maxBCG catalogue
• A warm mode of gas accretion on forming galaxies
• Discrepancies Between JWST Observations and Simulations of Quenched Massive Galaxies at $z>3$: A Comparative Study With IllustrisTNG and ASTRID
• AGN and quasar science with aperture masking interferometry on the James Webb Space Telescope
• Colour and infall time distributions of satellite galaxies in simulated Milky-Way analogs
• The HI mass function in the Parkes HI Zone of Avoidance survey
• Fractal Holography: a geometric re-interpretation of cosmological large scale structure
• Stacking Caustic Masses from Galaxy Clusters
• The effect of gas-dynamics on semi-analytic modeling of cluster galaxies
• A new method for testing isotropy with Shannon entropy
• Lopsided Galaxies in a cosmological context: a new galaxy-halo connection
• The Stellar-to-Halo Mass Ratios of Passive and Star-Forming Galaxies at z~2-3 from the SMUVS survey
• Gravitational entropy and the cosmological no-hair conjecture
• Abundance ratios in dwarf elliptical galaxies
• Strongly lensed neutral hydrogen emission: detection predictions with current and future radio interferometers
• Measuring the total infrared light from galaxy clusters at z=0.5-1.6: connecting stellar populations to dusty star formation
• Primordial magnetic fields: consistent initial conditions and impact on high-z structures
• The dark matter halo density profile, spiral arm morphology and black hole mass of M33
• Cosmic Web Dissection in Fuzzy Dark Matter Cosmologies
• Exploring the AGN-Merger Connection in Arp 245 I: Nuclear Star Formation and Gas Outflow in NGC 2992
• Constraints on sigma_8 from galaxy clustering in N-body simulations and semi-analytic models
• Not All Subhaloes Are Created Equal: Modelling the Diversity of Subhalo Density Profiles in TNG50
• The sign of active galactic nucleus quenching in a merger remnant with radio jets
• SMM J04135+10277: A Candidate Early-Stage "Wet-Dry" Merger of Two Massive Galaxies at z=2.8
• Statistical properties of dark matter mini-haloes at z >= 15
• Prospects of strongly lensed fast radio bursts: Simultaneous measurement of post-Newtonian parameter and Hubble constant
• Active Galaxy Nuclei at high redshifts: properties and environment of Type 1 and 2 AGNs
• Inferring Gravitational Potentials from Mass Densities in Cluster-sized Halos
• The whole picture of the large-scale structure of the CL1604 supercluster at z$\sim$0.9
• Merger history trees of dark matter haloes in moving barrier models
• Massive, red galaxies in a hierarchical universe-II Clustering of Extremely Red Objects
• A 1-dimensional hydrodynamic model for accretion, cooling and heating of gas in dark matter halos from $z=6$ to $z=0$
• How feedback shapes galaxies: an analytic model
• A short survey of matter-antimatter evolution in the primordial universe
• Imaging Spectroscopy of Ionized Gaseous Nebulae around Optically Faint AGN at Redshift z ~ 2
• The Effect of Particle Noise in N-body Simulations of Gravitational Lensing
• An estimate of the stochastic gravitational wave background from the MassiveBlackII simulation
• Euclid preparation. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary Fields
• Revisiting the fundamental metallicity relation with observation and simulation
• Spherical collapse in Generalized Dark Matter models
• Testing Dark Energy with the Advanced Liquid-Mirror Probe of Asteroids, Cosmology and Astrophysics
• Topology and geometry of the dark matter web: a multistream view
• Substructure within the SSA22 protocluster at $z\approx 3.09$
• Clustering of Extremely Red Objects in Elais-N1 from the UKIDSS DXS with optical photometry from Pan-STARRS1 and Subaru
• Physical properties of AGN host galaxies as a probe of SMBH feeding mechanisms
• Blending bias impacts the host halo masses derived from a cross-correlation analysis of bright sub-millimetre galaxies
• Precise Clustering and Density Evolution of redMaPPer Galaxy Clusters versus MXXL Simulation
• The clustering and halo occupation distribution of Lyman-break galaxies at $z\sim 4$
• The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
• Retrieving the three-dimensional matter power spectrum and galaxy biasing parameters from lensing tomography
• Exploring the non-linear density field in the Millennium simulations with tessellations - I. The probability distribution function
• HST F160W Imaging of Very Massive Galaxies at $1.5<z<3.0$: Diversity of Structures and the Effect of Close Pairs on Number Density Estimates
• CMASS galaxy sample and the ontological status of the cosmological principle
• Correlation function: biasing and fractal properties of the cosmic web
• Galaxy clusters in the SDSS Stripe 82 based on galaxy photometric redshifts
• Conditions for direct black hole seed collapse near a radio-loud quasar 1 Gyr after the Big Bang
• The Peculiar Velocity Correlation Function
• What kind of science is cosmology?
• The sparkling Universe: Clustering of voids and void clumps
• An Overdensity of Lyman Break Galaxies Around the Hot Dust-Obscured Galaxy WISE J224607.56$-$052634.9
• A parametric physical model for the intracluster medium and its use in joint SZ/X-ray analyses of galaxy clusters
• Merger Histories and Environments of Dwarf AGN in IllustrisTNG
• A thin disk in higher dimensional space-time and dark matter interpretation
• A unifying evolutionary framework for infrared-selected obscured and unobscured quasar host haloes
• The Sejong Suite: Cosmological Hydrodynamical Simulations with Massive Neutrinos, Dark Radiation, and Warm Dark Matter
• Future sensitivity of neutrino telescopes to dark matter annihilations from the cosmic diffuse neutrino signal
• K-CLASH: Strangulation and Ram Pressure Stripping in Galaxy Cluster Members at 0.3 < z < 0.6
• On the properties of compact groups identified in different photometric bands
• Cosmology Requirements on Supernova Photometric Redshift Systematics for Rubin LSST and Roman Space Telescope
• Farpoint: A High-Resolution Cosmology Simulation at the Gigaparsec Scale
• ERGO-ML: Comparing IllustrisTNG and HSC galaxy images via contrastive learning
• Nature versus nurture: relic nature and environment of the most massive passive galaxies at $z<0.5$
• Probabilistic cosmic web classification using fast-generated training data
• Local Group Analogs in $\Lambda$CDM cosmological simulations
• Brightest Cluster Galaxies Are Statistically Special From $z=0.3$ to $z=1$
• Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model. II. The colour-density relation up to z=1.5
• Tunable filter imaging of high redshift quasar fields
• The fate of the interstellar medium in early-type galaxies. III. The mechanism of ISM removal and quenching of star formation
• The effect of dark matter resolution on the collapse of baryons in high redshift numerical simulations
• Galaxy Structural Analysis with the Curvature of the Brightness Profile
• The formation pathways of compact elliptical galaxies
• Weak lensing detection of intra-cluster filaments with ground based data
• Halo mass and weak galaxy-galaxy lensing profiles in rescaled cosmological $N$-body simulations
• TOPCAT: Desktop Exploration of Tabular Data for Astronomy and Beyond
• The Cosmic Evolution of Halo Pairs: I. Global Trends
• A group-galaxy cross-correlation function analysis in zCOSMOS
• Reducing the Impact of Weak-lensing Errors on Gravitational-wave Standard Sirens
• Anisotropy in the matter distribution beyond the baryonic acoustic oscillation scale
• Indra: a Public Computationally Accessible Suite of Cosmological $N$-body Simulations
• A hadronic emission model for black hole-disc impacts in the blazar OJ 287
• Galaxy Clusters in the Line of Sight to Background Quasars: II. Environmental effects on the sizes of baryonic halo sizes
• Satellites in the field and lens galaxies: SDSS/COSMOS vs. SLACS/CLASS
• Physics of galactic colliders: high speed satellites in LCDM vs MONDian cosmology
• Exploring the relation between dust mass and galaxy properties using Dusty SAGE
• Models of gravitational lens candidates from Space Warps CFHTLS
• The Cosmic Large-Scale Structure in X-rays (CLASSIX) cluster survey IV: Superclusters in the local Universe at z <= 0.03
• Ageing and Quenching through the ageing diagram: predictions from simulations and observational constraints
• Surface mass density of the Einasto family of dark matter haloes: Are they Sersic-like?
• Observations of the High Redshift Universe
• ERGO-ML: Towards a robust machine learning model for inferring the fraction of accreted stars in galaxies from integral-field spectroscopic maps
• Hot Gas, Cold Gas and Sub-Halos in a Lyman-alpha Blob at Redshift 2.38
• Internal Cluster Structure
• Constraints on small-scale cosmological fluctuations from SNe lensing dispersion
• Two phase galaxy formation: The Evolutionary Properties of Galaxies
• Merger history of central galaxies in Semi-Analytic Models of galaxy formation
• Modeling active galactic nuclei: ongoing problems for the faint-end of the luminosity function
• The Califa and Hipass velocity function for all morphological galaxy types
• The luminosity bias relation from filaments in the Sloan Digital Sky Survey Data Release Four
• An improved prescription for merger time-scales from controlled simulations
• Bimodal morphologies of massive galaxies at the core of a protocluster at z=3.09 and the strong size growth of a brightest cluster galaxy
• On the complexity and the information content of cosmic structures
• Dust-obscured star formation and the contribution of galaxies escaping UV/optical color selections at z~2
• TDCOSMO XIV: Practical Techniques for Estimating External Convergence of Strong Gravitational Lens Systems and Applications to the SDSS J0924+0219 System
• A methodology to select galaxies just after the quenching of star formation
• The evolution of the density of galaxy clusters and groups: denser environments at higher redshifts
• The Clustering of Extremely Red Objects
• Heating and enriching the intracluster medium
• X-ray morphology of cluster-mass haloes in self-interacting dark matter
• Galaxy And Mass Assembly (GAMA): The absence of stellar mass segregation in galaxy groups and consistent predictions from GALFORM and EAGLE simulations
• Herschel-ATLAS/GAMA: What determines the far-infrared properties of radio-galaxies?
• The influence of the matter along the line of sight and in the lens environment on the strong gravitational lensing
• Predictions for the FAST telescope's CRAFTS Extra-Galactic HI Survey
• Host galaxy properties and environment of obscured and unobscured X-ray selected Active Galactic Nuclei in the COSMOS survey
• Impact of cosmic filaments on the gas accretion rate of dark matter halos
• Void-Supercluster Alignments
• Unveiling the largest structures in the nearby Universe: Discovery of the Quipu superstructure
• AGN pairs: chance superpositions or black hole binaries?
• The Ursa Major cluster redefined as a `supergroup'
• The Variance and Covariance of Counts-in-Cells Probabilities
• Dynamical analysis of strong-lensing galaxy groups at intermediate redshift
• The relationship between gas and galaxies at z<1 using the Q0107 quasar triplet
• What has quenched the massive spiral galaxies?
• Minimum star-forming halo mass in axion cosmology
• Extremely Massive Quasars are not Good Proxies for Dense Environments Compared to Massive Galaxies: Environments of Extremely Massive Quasars and Galaxies
• A Radio-to-millimeter Census of Star-forming Galaxies in Protocluster 4C~23.56 at z = 2.5 : Global and local gas kinematics
• Galaxy triplets in Sloan Digital Sky Survey Data Release 7 - III. Analysis of Configuration and Dynamics
• Testing the conditional mass function of dark matter halos against numerical N-body simulations
• Searching for the shadows of giants: characterising protoclusters with line of sight Lyman-α absorption
• Dynamical analysis of clusters of galaxies from cosmological simulations
• Compact groups from semi-analytical models of galaxy formation -- III: purity and completeness of Hickson-like catalogues
• The infrared-luminous progenitors of high-z quasars
• Toward Solving the Puzzle: Dissecting the Complex Merger A521 with Multi-wavelength Data
• Incorporating galaxy cluster triaxiality in stacked cluster weak lensing analyses
• An adapted filter function for density split statistics in weak lensing
• Clusters of galaxies: setting the stage
• Peaks and dips in Gaussian random fields: a new algorithm for the shear eigenvalues, and the excursion set theory
• A new perspective on the stellar Mass-Metallicity Relation of quiescent galaxies from the LEGA-C survey
• Host galaxies of long gamma-ray bursts in the Millennium Simulation
• Discovering Large-Scale Structure at $2<z<5$ in the C3VO Survey
• Do you see what I see? Exploring the consequences of luminosity limits in black hole-galaxy evolution studies
• The nature and descendants of Lyman-break galaxies in the LambdaCDM cosmology
• Unveiling the main sequence of galaxies at $z\ge 5$ with the James Webb Space Telescope: predictions from simulations
• A Comparison of Galaxy Group Luminosity Functions from Semi-Analytic Models
• Clustering of galaxies at 3.6 microns in the Spitzer Wide-area Infrared Extragalactic legacy survey
• The average submillimetre properties of Lyman-alpha Blobs at z=3
• Detection of WHIM in the Planck data using Stack First approach
• Modelling the spectral energy distribution of galaxies: introducing the artificial neural network
• Dynamics of finite and infinite self-gravitating systems with cold quasi-uniform initial conditions
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• Shell-like structures in our cosmic neighbourhood
• Stochastic Processes as the Origin of the Double-Power Law Shape of the Quasar Luminosity Function
• The MUSE-Wide survey: Three-dimensional clustering analysis of Lyman-$\alpha$ emitters at $3.3<z<6$
• Assembly Bias of Dwarf-sized Dark Matter Haloes
• Detection of Prominent Stellar Disks in the Progenitors of Present-day Massive Elliptical Galaxies
• Mapping the low surface brightness Universe in the UV band with Lya emission from IGM filaments
• The MODEST questions: challenges and future directions in stellar cluster research
• Galaxy-Galaxy Lensing in EAGLE: comparison with data from 180 square degrees of the KiDS and GAMA surveys
• Massive Quiescent Galaxies at z>3 in The Millennium Simulation Populated by A Semi-analytic Galaxy Formation Model
• The Coevolution of Massive Quiescent Galaxies and Their Dark Matter Halos over the Last 6 Billion Years
• The MAGPI Survey: Impact of environment on the total internal mass distribution of galaxies in the last 5 Gyr
• Large Scale Overdensity of Lyman Break Galaxies Around the z=6.3 Ultraluminous Quasar J0100+2802
• Physical Conditions and Extension of the Coronal Line Region in IC 5063
• A new framework for numerical simulations of structure formation
• Semi-Analytic Galaxy Formation in Massive Neutrino Cosmologies
• Void Galaxy Distribution: A Challenge for $\Lambda$CDM
• Revised Mass-to-Light Ratios For Nearby Galaxy Groups and Clusters
• Large Molecular Gas Reservoirs in Star Forming Cluster Galaxies
• Fitting a Self-Interacting Dark Matter Model to Data Ranging From Satellite Galaxies to Galaxy Clusters
• Compact groups from semi-analytical models of galaxy formation -- I: a comparative study of frequency and nature
• Unravelling the Cosmic Web: An analysis of the SDSS DR14 with the Local Dimension
• The nature of the nearest compact group of galaxies from precise distance measurements
• Baryon oscillations in galaxy and matter power-spectrum covariance matrices
• The Anisotropic Two-Point Correlation Functions of the Nonlinear Traceless Tidal Field in the Principal-Axis Frame
• Consequences of dark matter self-annihilation for galaxy formation
• Genus statistics using the Delaunay tessellation field estimation method: (I) tests with the Millennium Simulation and the SDSS DR7
• Simulating Deep Hubble Images With Semi-empirical Models of Galaxy Formation
• Star Formation in High-Redshift Cluster Ellipticals
• Voids and Superstructures: correlations and induced large-scale velocity flows
• Quenching or Bursting: Star Formation Acceleration--A New Methodology for Tracing Galaxy Evolution
• Unraveling the complex structure of AGN-driven outflows: IV. Comparing AGNs with and without strong outflows
• Compact groups from semi-analytical models of galaxy formation -- II: Different assembly channels
• Physical properties of more than one thousand brightest cluster galaxies detected in the Canada France Hawaii Telescope Legacy Survey
• Shaping the Milky Way: The interplay of mergers and cosmic filaments
• A novel approach to cosmological non-linearities as an effective fluid
• Characterisation of local halo building blocks: Thamnos and Sequoia
• SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
• Demographics of Tidal Disruption Events with L-Galaxies: I. Volumetric TDE rates and the abundance of Nuclear Star Clusters
• Environmental dependence of AGN activity and star formation in galaxy clusters from Magneticum simulations
• Galaxy cluster mass accretion rates from IllustrisTNG
• The Unusual Milky Way-Local Sheet System: Implications for Spin Strength and Alignment
• Deep Spitzer/IRAC Data for z~10 galaxies Reveal Blue Balmer Break Colors: Young Stellar Populations at ~500 Myr of Cosmic Time
• Dark matter cores in massive high-$z$ galaxies formed by baryonic clumps
• KiDS+VIKING+GAMA: Halo occupation distributions and correlations of satellite numbers with a new halo model of the galaxy-matter bispectrum for galaxy-galaxy-galaxy lensing
• Quenching, bursting and galaxy shapes: colour transformation as a function of morphology
• Cosmological Constraints from Weak Lensing Peaks: Can Halo Models Accurately Predict Peak Counts?
• On the absence of backsplash analogues to NGC 3109 in the $\Lambda$CDM framework
• Satellite Alignment: III. Satellite Galaxies Spatial Distribution and their Dependence on Redshift with A Novel Galaxy Finder
• Sloshing of Galaxy Cluster Core Plasma in the Presence of Self-Interacting Dark Matter
• A Cosmological Solution to the Impossibly Early Galaxy Problem
• Resolution of the apparent discrepancy between the number of massive subhaloes in Abell 2744 and ΛCDM
• The Fabric of the Universe: Exploring the cosmic web in 3D prints and woven textiles
• Post-Newtonian parameter $\gamma$ and the deflection of light in ghost-free massive bimetric gravity
• Heating of galactic gas by dark matter annihilation in ultracompact minihalos
• Confronting semi-analytic galaxy models with galaxy-matter correlations observed by CFHTLenS
• Vector Dark Matter Detection using the Quantum Jump of Atoms
• Compatibility of the Large Quasar Groups with the Concordance Cosmological Model
• Gravitational microlensing as a probe for dark matter clumps
• The XMM Cluster Survey: evolution of the velocity dispersion -- temperature relation over half a Hubble time
• On the complementarity of pulsar timing and space laser interferometry for the individual detection of supermassive black hole binaries
• The MeSsI (Merging Systems Identification) Algorithm & Catalogue
• Can We Detect the Color-Density Relation with Photometric Redshifts?
• The bias of weighted dark matter halos from peak theory
• Log-transforming the matter power spectrum
• Millennium Simulation Dark Matter Haloes: Multi-fractal and Lacunarity Analysis with Homogeneity Transition
• Background, foreground and nearby matter influence on strong gravitational lenses
• Improving three-dimensional mass mapping with weak gravitational lensing using galaxy clustering
• The dark matter content of the blue compact dwarf NGC 2915
• On the Anticorrelation Between Galaxy Light Concentration and X-ray-to-Optical Flux Ratio
• Lopsided Satellite Distributions around Isolated Host Galaxies in a LCDM Universe
• Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies
• The Subtle Effects of Mergers on Star Formation in Nearby Galaxies
• Not Hydro: Using Neural Networks to estimate galaxy properties on a Dark-Matter-Only simulation
• Nonlinear Density Fluctuation Field Theory for Large Scale Structure
• Missing Baryons, from Clusters to Groups of Galaxies
• The Bridge Effect of Void Filaments
• How dark are filaments in the cosmic web?
• Dark-ages reionization and galaxy formation simulation XI: Clustering and halo masses of high redshift galaxies
• Cosmological applications of the Brown-York quasilocal mass
• Ionized Gas Kinematics along the Large-Scale Radio Jets in Type 2 AGNs
• Abundance and group coalescence timescales of compact groups of galaxies in the EAGLE simulation
• The Tessellation-Level-Tree: characterising the nested hierarchy of density peaks and their spatial distribution in cosmological N-body simulations
• Evolution of CIV Absorbers. II. Where does CIV live?
• Astrophysics in 2006
• Charged Fuzzy Dark Matter Black Holes
• Mass estimators in the Gaia era
• An empirical model to form and evolve galaxies in dark matter halos
• The Size Evolution of Elliptical Galaxies
• Shining Light on Merging Galaxies I: The Ongoing Merger of a Quasar with a `Green Valley' Galaxy
• On the nature of Small Galaxy Systems
• Quiescent luminous red galaxies (LRGs) as cosmic chronometers: on the significance of mass and environmental dependence
• Gas stripping and mixing in galaxy clusters: A numerical comparison study
• Terapixel imaging of cosmological simulations
• The first GLIMPSE of the faint galaxy population at Cosmic Dawn with JWST: The evolution of the ultraviolet luminosity function across z~9-15
• Constraints on precipitation-limited hot halos from massive galaxies to galaxy clusters
• The scale dependence of mass assembly in galaxies
• Environmental Effects of Dark Matter Haloes: The Clustering-Substructure relation of Group-size Haloes
• On the Evolution of the Bi-Modal Distribution of Galaxies in the Plane of Specific Star Formation Rate versus Stellar Mass
• The cooler past of the intracluster medium in TNG-Cluster
• Uncovering substructure with wavelets: proof of concept using Abell 2744
• Effect of observational holes in fractal analysis of galaxy survey masks
• Galaxy populations in groups and clusters: evidence for a characteristic stellar mass scale at $M_{\ast }\sim 10^{9.5}{M}_{\odot }$
• Search for dark matter particles in proton-proton collisions at sqrt(s) = 8 TeV using the razor variables
• Detecting baryon acoustic oscillations by 3d weak lensing
• Remapping simulated halo catalogues in redshift space
• Detection of the velocity shear effect on the spatial distributions of the galactic satellites in isolated systems
• Recoiling Supermassive Black Holes in Spin-flip Radio Galaxies
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• Connecting the Dots: Tracking Galaxy Evolution Using Constant Cumulative Number Density at 3<z<7
• Role of Feedback in AGN-HOST Coevolution: A Study from Partially Obscured Active Galactic Nuclei
• Auriga Streams I: disrupting satellites surrounding Milky Way-mass haloes at multiple resolutions
• Measuring the BAO peak position with different galaxy selections
• The inhomogenous reionization of the inter-galactic medium by metal-poor globular clusters
• The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship
• A comparison of the R_h=ct and LCDM cosmologies based on the observed halo mass function
• Ram pressure profiles in galaxy groups and clusters
• The Star Formation and AGN luminosity relation: Predictions from a semi-analytical model
• Non-linear cosmological collapse of quintessence
• Using the Modified Nearest Neighbor Method to Correct Fiber-collision Effects on Galaxy Clustering
• Discovery of large scale shock fronts correlated with the radio halo and radio relic in the A2163 galaxy cluster
• Starburst galaxies in semi-analytic models of galaxy formation and evolution
• Tightening weak lensing constraints on the ellipticity of galaxy-scale dark matter haloes
• Revisiting the clustering of narrow-line AGN in the local Universe: Joint dependence on stellar mass and color
• The contribution of star-forming galaxies to fluctuations in the cosmic background light
• Impetus: Consistent SPH calculations of 3D spherical Bondi accretion onto a black hole
• An Optical Analysis of the Merging Cluster Abell 3888
• Characterising Strong Lensing Galaxy Clusters using the Millennium-XXL and MOKA simulations
• The ecology of dark matter haloes I: The rates and types of halo interactions
• The nature of H$\alpha$-selected galaxies along the large-scale structure at z=0.4 revealed by Subaru Hyper Suprime-Cam survey
• Overdensity of VVV galaxies behind the Galactic bulge
• Cosmic Cartography: Bayesian reconstruction of the galaxy density informed by large-scale structure
• Using galaxy pairs as cosmological tracers
• A consistent model for both the HI and stellar mass functions of galaxies
• The abundance and colours of galaxies in high redshift clusters in the cold dark matter cosmology
• The environmental dependence of the red galaxy sequence
• Modelling Dark Matter Halo Spin using Observations and Simulations: application to UGC 5288
• Population Gradients in the SDSS Galaxy Catalog. The role of merging
• Origin and Evolution of Structure and Nucleosynthesis for Galaxies in the Local Group
• Understanding AGN-host connection in partially obscured active galactic nuclei. Part III: Properties of ROSAT-selected SDSS AGNs
• Extracting galaxy merger timescales I: Tracking haloes with WhereWolf and spinning orbits with OrbWeaver
• Halo Counts-in-cells for Cosmological Models with Different Dark Energy
• A semi-analytical perspective on massive galaxies at $z\sim 0.55$
• Spitzer observations of Abell 1763 - II: Constraining the nature of activity in the cluster-feeding filament with VLA and XMM-Newton data
• The Ultramarine Simulation: properties of dark matter haloes before redshift 5.5
• The virialization density of peaks with general density profiles under spherical collapse
• A Modified TreePM Code
• Galaxy rotation favors prolate dark matter haloes
• Rapid Simulations of Halo and Subhalo Clustering
• An Extra-Dimensional Model of Dark Matter
• On the Evolution of High-Redshift Active Galactic Nuclei
• Clusters of galaxies and the cosmic web with SKA
• On the weak lensing masses of a new sample of galaxy groups
• Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
• Three-dimensional modeling of the HI kinematics of NGC 2915
• History of the gas fuelling star formation in eagle galaxies
• Reconciling Mass Functions with the Star-Forming Main Sequence Via Mergers
• Local alignments of parsec-scale AGN radiojets
• Statistical properties of filaments in weak gravitational lensing
• Resolution Convergence in Cosmological Hydrodynamical Simulations Using Adaptive Mesh Refinement
• Setting the Stage: Structures from Gaussian Random Fields
• Statistics of Dark Matter Halos in the Excursion Set Peak Framework
• Simulating a stellar contact binary merger -- I. Stellar models
• Photometric and clustering properties of hydrodynamical galaxies in a cosmological volume: results at z=0
• Geometry and Morphology of the Cosmic Web: Analyzing Spatial Patterns in the Universe
• On merger bias and the clustering of quasars
• Autocorrelations of stellar light and mass in the low-redshift Universe
• Data Compression in the Petascale Astronomy Era: a GERLUMPH case study
• Semi-analytic galaxy formation in coupled dark energy cosmologies
• Removal and mixing of the coronal gas from satellites in galaxy groups: cooling the intragoup gas
• Interpreting the galaxy group CG J1720-67.8 through evolutionary synthesis models
• Recovering dark-matter clustering from galaxies with Gaussianization
• A Direct Linkage Between AGN Outflows in The Narrow-line Regions and The X-ray Emission From The Accretion disks
• Third-order cosmological perturbations of zero-pressure multi-component fluids: Pure general relativistic nonlinear effects
• A potentially pure test of cosmic geometry: galaxy clusters and the real space Alcock-Paczynski test
• The Impact of the Dusty Torus on Obscured Quasar Halo Mass Measurements
• Angular momentum evolution in Dark Matter haloes: a study of the Bolshoi and Millennium simulations
• Approximations to galaxy star formation rate histories: properties and uses of two examples
• Missing Dwarf Problem in Galaxy Clusters
• The Tully-Fisher relation for flat galaxies
• Expanding Universe and Dynamical Compactification Using Yang-Mills Instantons
• SMBH growth parameters in the early Universe of Millennium and Millennium-II simulations
• GABE: Galaxy Assembly with Binary Evolution
• Can fermionic dark matter mimic supermassive black holes?
• The Anisotropy in the Galaxy Velocity Field Originated from the Gravitational Pancaking Effect
• Simultaneous effect of Modified Gravity and Primordial Non-Gaussianity in Large Scale Structure Observations
• MEGA: Merger graphs of structure formation
• Structure in the 3D Galaxy Distribution: II. Voids and Watersheds of Local Maxima and Minima
• Can a conditioning on stellar mass explain the mutual information between morphology and environment?
• Correlation functions in 2D and 3D as descriptors of the cosmic web
• Ridges in the Dark Energy Survey for cosmic trough identification
• Biasing relation, environmental dependencies and estimation of the growth rate from star forming galaxies
• On Escaping a Galaxy Cluster in an Accelerating Universe
• An Empirical Determination of the Dependence of the Circumgalactic Mass Cooling Rate and Feedback Mass Loading Factor on Galactic Stellar Mass
• Interchanging Interactive 3-d Graphics for Astronomy
• The Subaru HSC weak lensing mass-observable scaling relations of spectroscopic galaxy groups from the GAMA survey
• AKARI near-infrared background fluctuations arise from normal galaxy populations
• Weak lensing measurement of the mass-richness relation using the SDSS database
• Combining Strong Lensing and Dynamics in Galaxy Clusters: integrating MAMPOSSt within LENSTOOL I. Application on SL2S J02140-0535
• Horizon Run 3: Topology as a Standard Ruler
• A general framework to test gravity using galaxy clusters VI: Realistic galaxy formation simulations to study clusters in modified gravity
• Connecting traces of galaxy evolution: the missing core mass -- morphological fine structure relation
• Resolving the problem of galaxy clustering on small scales: any new physics needed?
• LARgE Survey. I. Dead Monsters: the Massive End of the Passive Galaxy Stellar Mass Function at Cosmic Noon
• Searches for Population III Pair-Instability Supernovae: Impact of Gravitational Lensing Magnification
• The alignment between brightest cluster galaxies and host clusters
• Dark matter halo mass functions and density profiles from mass and energy cascade
• Enhancement of HI absorption associated with the $z=3.1$ large-scale proto-cluster and characteristic structures with AGNs sculptured over Gpc scale in the SSA22 field
• Cosmology with Galaxy Cluster Properties using Machine Learning
• The effect of pressure-anisotropy-driven kinetic instabilities on magnetic field amplification in galaxy clusters
• HerMES: The Submillimeter Spectral Energy Distributions of Herschel/SPIRE-Detected Galaxies
• MeerKAT's discovery of a radio relic in the bimodal merging cluster A2384
• Damped Lyman-$\alpha$ absorbers and atomic hydrogen in galaxies: the view of the GAEA model
• MAGAZ3NE: Massive, Extremely Dusty Galaxies at $z\sim 2$ Lead to Photometric Overestimation of Number Densities of the Most Massive Galaxies at $3<z<4$
• Star formation history and transition epoch of cluster galaxies based on the Horizon-AGN simulation
• Validating the clustering predictions of empirical models with the FLAMINGO simulations
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• From Halos to Galaxies. VI. Improved halo mass estimation for SDSS groups and measurement of the halo mass function
• Ongoing Star Formation In AGN Host Galaxy Disks: A View From Core-collapse Supernovae
• The coevolution of the velocity and mass functions of galaxies and dark haloes
• An Extended Zel'dovich Model for the Halo Mass Function
• On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn
• The role of mergers and gas accretion in black hole growth and galaxy evolution
• Galaxy and Mass Assembly (GAMA): the clustering of galaxy groups
• The influence of Hickson-like compact group environment on galaxy luminosities
• Galaxy And Mass Assembly (GAMA) Survey: The Merging Potential of Brightest Group Galaxies
• Galaxy cluster optical mass proxies from probabilistic memberships
• Variation of the stellar initial mass function in semi-analytical models III: testing the cosmic ray regulated integrated galaxy-wide initial mass function
• Particle initialization effects on Lyman-$\alpha$ forest statistics in cosmological SPH simulations
• Incoherent localized structures and hidden coherent solitons from the gravitational instability of the Schrödinger-Poisson equation
• Mapping the Arnold web with a GPU-supercomputer
• Luminous satellite galaxies in gravitational lenses
• Baryonic Effects on Lagrangian Clustering and Angular Momentum Reconstruction
• Co-Evolution vs. Co-existence: The Effect of Accretion Modelling on the Evolution of Black Holes and Host Galaxies
• Ultra-fine dark matter structure in the Solar neighbourhood
• Comparing Galaxy Clustering in Horizon-AGN Simulated Lightcone Mocks and VIDEO Observations
• Foreground Removal of CO Intensity Mapping Using Deep Learning
• VST-GAME: Galaxy Assembly as a function of Mass and Environment with VST. Photometric assessment and density field of MACSJ0416
• Cosmological radiative transfer for the line-of-sight proximity effect
• CALSAGOS: Clustering ALgorithmS Applied to Galaxies in Overdense Systems
• Resolution criteria to avoid artificial clumping in Lagrangian hydrodynamic simulations with a multi-phase interstellar medium
• The mass accretion history of dark matter haloes down to Earth mass
• The stellar mass function and efficiency of galaxy formation with a varying initial mass function
• Herschel-ATLAS/GAMA:How does the far-IR luminosity function depend on galaxy group properties?
• Probing the roles of orientation and multi-scale gas distributions in shaping the obscuration of Active Galactic Nuclei through cosmic time
• Active galactic nuclei cores in infrared-faint radio sources: Very long baseline interferometry observations using the Very Long Baseline Array
• Deriving galaxy cluster velocity anisotropy profiles from a joint analysis of dynamical and weak lensing data
• JWST + ALMA ubiquitously discover companion systems within $\lesssim 18$kpc around four $z$$\approx$3.5 luminous radio-loud AGN
• Characterizing simulated galaxy stellar mass histories
• Stability of Rotating Self-Gravitating Filaments:Stability of Rotating Self-Gravitating Filaments: Effects of Magnetic Field
• Angular Momentum Evolution in Dark Matter Halos
• Gradient Pattern Analysis of Cosmic Structure Formation: Norm and Phase Statistics
• Ecology of dark matter haloes -II. Effects of interactions on the alignment of halo pairs
• Astrophysical Particle Simulations on Heterogeneous CPU-GPU Systems
• Cosmic Reionization and the First Nonlinear Structures in the Universe
• The Origin of the Large-Scale Structure in the Universe: Theoretical and Statistical Aspects
• Predicting the frequencies of young and of tiny galaxies
• Origin of the Chemical Elements
• On the reliability of photometric and spectroscopic tracers of halo relaxation
• Environments of a sample of AzTEC submillimetre galaxies in the COSMOS field
• Chemodynamical Properties and Ages of Metal-Poor Stars in S-PLUS
• Dark Energy Survey Year 3 Results: Constraints on cosmological parameters and galaxy bias models from galaxy clustering and galaxy-galaxy lensing using the redMaGiC sample
• Comparing galaxy morphology in hydrodynamical simulation and in semi-analytic model
• Are compact groups hostile towards faint galaxies?
• On the detectability of massive black hole merger eventsby LISA
• Statistical physics for cosmic structures
• Giga-z: A 100,000 Object Superconducting Spectrophotometer for LSST Follow-up
• Euclid preparation. LI. Forecasting the recovery of galaxy physical properties and their relations with template-fitting and machine-learning methods
• Zooming in on the Circumgalactic Medium with GIBLE: Tracing the Origin and Evolution of Cold Clouds
• Measuring the thermal and ionization state of the low-$z$ IGM using likelihood free inference
• The distribution of galaxies gravitational field stemming from their tidal interaction
• The low mass end of the neutral gas mass and velocity width functions of galaxies in $\Lambda$CDM
• UV to FIR catalogue of a galaxy sample in nearby clusters: SEDs and environmental trends
• The shape distribution of superclusters in SDSS DR 12
• Accurate Masses for Navarro-Frenk-White Dark Matter Haloes
• Quantifying parameter errors due to the peculiar velocities of type Ia supernovae
• L-GALAXIES 2020: The formation and chemical evolution of stellar haloes in Milky Way Analogues and galaxy clusters
• Can we distinguish early dark energy from a cosmological constant?
• Co-evolution of supermassive black holes with galaxies from semi-analytic model: stochastic gravitational wave background and black hole clustering
• Kinetic Field Theory for Cosmic Structure Formation
• Two Component Baryonic-Dark Matter Structure Formation in Top-Hat Model
• The Orbital Distribution of Satellite Galaxies
• Electron Energy Distributions in the Extended Gas Nebulae associated with High-z AGN: Maxwell-Boltzmann vs. kappa distributions
• ARTEMIS emulator: exploring the effect of cosmology and galaxy formation physics on Milky Way-mass haloes and their satellites
• The spatial distribution of satellites in galaxy clusters
• Accurate Analytic Mass-Scale Relations for Dark Matter Haloes of all Masses and Redshifts
• Stable clustering and the resolution of dissipationless cosmological N-body simulations
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• The feasibility of constraining DM interactions with high-redshift observations by JWST
• Cosmic ray backgrounds for dark matter indirect detection
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• Filamentary Baryons and Where to Find Them: A forecast of synchrotron radiation from merger and accretion shocks in the local Cosmic Web
• Euclid preparation LXX. Forecasting detection limits for intracluster light in the Euclid Wide Survey
• Accurate Modeling of the Projected Galaxy Clustering in Photometric Surveys: I. Tests with Mock Catalogs
• Multiwavelength analysis of low surface brightness galaxies to study possible dark matter signature
• Kinematics of the ionized and molecular gas in nearby luminous infrared interacting galaxies
• Light path averages in spacetimes with non-vanishing average spatial curvature
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• Dark Matter Annihilation Feedback in cosmological simulations I: Code convergence and idealised halos
• Magnification bias in the shear-ratio test: a viable mitigation strategy
• Conservation of radial actions in time-dependent spherical potentials
• The origin of redshift asymmetries: How LambdaCDM explains anomalous redshift
• A sparse regression approach to modeling the relation between galaxy stellar masses and their host halos
• Halo shapes constrained from a pure sample of central galaxies in KiDS-1000
• Magnetic dynamos in galaxy clusters: the crucial role of galaxy formation physics at high redshifts
• Andromeda XXV -- a dwarf galaxy with a low central dark matter density
• Intra-Cluster Light as a Dynamical Clock for Galaxy Clusters: Insights from the MAGNETICUM, IllustrisTNG, Hydrangea and Horizon-AGN Simulations
• The morphology of star-forming gas and its alignment with galaxies and dark matter haloes in the EAGLE simulations
• Mid-IR cosmological spectrophotometric surveys from space: Measuring AGN and star formation at the Cosmic Noon with a SPICA-like mission
• 2D Surface Brightness Modelling of Large 2MASS Galaxies I: Photometry and Structural Parameters
• X-ray Absorption Lines in the Warm-Hot Intergalactic Medium: Probing Chandra observations with the CAMEL simulations
• The Space Density of Intermediate Redshift, Extremely Compact, Massive Starburst Galaxies
• The Effects of Linear Matter Power Spectrum Enhancement on Dark Matter Substructure
• A Stochastic Theory of the Hierarchical Clustering II. Halo progenitor mass function and large-scale bias
• Optimizing high redshift galaxy surveys for environmental information
• The impact of the cosmological constant on past and future star formation
• The metallicity and elemental abundance maps of kinematically atypical galaxies for constraining minor merger and accretion histories
• Quantifying the intrinsic variability due to randomness of the Auriga galaxy formation model
• Evidence of Turbulence-like Universality on the Formation of Galaxy-sized Dark Matter Haloes
• Cosmic Web & Caustic Skeleton: non-linear Constrained Realizations -- 2D case studies
• Clustering, Cosmology and a New Era of Black Hole Demographics -- I. The Conditional Luminosity Function of Active Galactic Nuclei
• Dynamical analysis of the cluster pair: A3407 + A3408
• NGC 765 - A disturbed H I giant
• On The Role of Supermassive Black Holes in Quenching Star Formation in Local Central Galaxies
• The Evolution of Radio Galaxies and X-ray Point Sources in Coma Cluster Progenitors Since z~1.2
• An efficient and robust method to estimate halo concentration
• Screening vs. gevolution: in chase of a perfect cosmological simulation code
• Gusts in the Headwind: Uncertainties in Direct Dark Matter Detection
• Harnessing the Hubble Space Telescope Archives: A Catalogue of 21,926 Interacting Galaxies
• Inferring redshift and galaxy properties via a multi-task neural net with probabilistic outputs: An application to simulated MOONS spectra
• Hubble flow variations as a test for inhomogeneous cosmology
• HI HOD -- I. The Halo Occupation Distribution of HI Galaxies
• LARgE Survey -- II. The Dark Matter Halos and the Progenitors and Descendants of Ultra-Massive Passive Galaxies at Cosmic Noon
• Globular cluster ages and their relation to high-redshift stellar cluster formation times from different globular cluster models
• Semi-Numerical Simulation of Reionization with Semi-Analytical Modeling of Galaxy Formation
• SCONCE: A cosmic web finder for spherical and conic geometries
• The growth of disks and bulges during hierarchical galaxy formation. II: metallicity, stellar populations and dynamical evolution
• Probing supervoids with weak lensing
• Measurement of halo properties with weak lensing shear and flexion
• Beyond the Lognormal Approximation: a General Simulation Scheme
• Measuring galaxy environment with the synergy of future photometric and spectroscopic surveys
• Semi-empirical catalog of early-type galaxy-halo systems: dark matter density profiles, halo contraction and dark matter annihilation strength
• Evolution of black hole and galaxy growth in a semi-numerical galaxy formation model
• MAMBO -- An empirical galaxy and AGN mock catalogue for the exploitation of future surveys
• Self-Interacting Dark Matter Scattering Rates Through Cosmic Time
• SQuIGG$\vec{L}$E: Observational Evidence of Low Ongoing Star Formation Rates in Gas-Rich Post-Starburst Galaxies
• The Occurrence of Compact Groups of Galaxies Through Cosmic Time
• A Random Walk Model for Dark Matter Halo Concentrations
• FLY: MPI-2 High Resolution code for LSS Cosmological Simulations
• An efficient hybrid method to produce high resolution large volume dark matter simulations for semi-analytic models of reionisation
• The effect of AGN feedback on the X-ray morphologies of clusters -- simulations vs. observations
• Clusters in the Disperse cosmic web
• The Mass Density Profile and Star Formation History of Gaussian and Non-Gaussian Clusters
• Deep spectroscopy of 9C J1503+4528: a very young CSS radio source at z=0.521
• The Two-Point Correlation Function of Gamma-ray Bursts
• Satellite galaxies in the Illustris-1 simulation: anisotropic locations around relatively isolated hosts
• Understanding Galaxy Formation and Evolution
• Mapping the working of environmental effects in A963
• Void alignment and density profile applied to measuring cosmological parameters
• Modeling the Alignment Profile of Satellite Galaxies in Clusters
• Measuring galaxy-galaxy-galaxy-lensing with higher precision and accuracy
• A Novel Scheme for Dark Matter Annihilation Feedback in Cosmological Simulations
• An Ising model for galaxy bias
• The velocity function of dark matter halos at r=20 kpc: Remarkably little evolution since z ~ 4
• Simulating Kilonovae in the ΛCDM Universe
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• Dark Matter with N-Body Numerical Simulations
• Cosmological model dependence of the galaxy luminosity function: far-infrared results in the Lemaitre-Tolman-Bondi model
• A rising tide: Intrinsic alignments since the turn of the millennium
• Can tides explain the low dark matter density in Fornax?
• Energy Efficiency trends in HPC: what high-energy and astrophysicists need to know
• Assessing the reliability of the Bisous filament finder
• Finding proto-clusters to trace galaxy evolution: I. The finder and its performance
• Bayesian Cosmic Web Reconstruction: BARCODE for Clusters
• Psi-GAN: A power-spectrum-informed generative adversarial network for the emulation of large-scale structure maps across cosmologies and redshifts
• Revealing the hidden cosmic feast: A z=4.3 galaxy group hosting two optically dark, efficiently star-forming galaxies
• Lopsided distribution of MATLAS and ELVES dwarf satellite systems around isolated host galaxies
• Observations of Ly$\alpha$ Emitters at High Redshift
• The Degeneracy of Galaxy Formation Models
• On the asymptotic behaviour of cosmic density-fluctuation power spectra
• Satellite galaxy abundance dependency on cosmology in Magneticum simulations
• Trial by FIRE: Probing the dark matter density profile of dwarf galaxies with GraphNPE
• Visualizing Astrophysical N-body Systems
• A Large Scale Structure at Redshift 1.71 in the Lockman Hole
• Statistical properties of filaments in the cosmic web
• A Pair of Early- and Late-Forming Galaxy Cluster Samples: a Novel Way of Studying Halo Assembly Bias Assisted by a Constrained Simulation
• $Spitzer$-selected $z>1.3$ protocluster candidates in the LSST Deep Drilling Fields
• Semi-analytical frameworks for subhalos from the smallest to the largest scale
• An expanded merger-tree description of cluster evolution
• Analyzing Planar Galactic Halo Distributions with Fuzzy/Cold Dark Matter Models
• Complementary Cosmological Simulations
• Preprocessing in small groups: Three simulated galaxies interacting prior to cluster infall
• ALMA 1.1mm Observations of a Conservative Sample of High Redshift Massive Quiescent Galaxies in SHELA
• Strong gravitational lensing by AGNs as a probe of the quasar-host relations in the distant Universe
• Estimating small angular scale CMB anisotropy with high resolution N-body simulations: weak lensing
• An Analytic Formula for the Supercluster Mass Function
• Clustering Properties of Low-Luminosity Star-Forming galaxies at z = 0.24 and 0.40 in the Subaru Deep Field
• Deficit of Luminous and Normal Red Galaxies in Cosmic Voids
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• Infall Profiles for Supercluster-Scale Filaments
• Substructure in the Globular Cluster Populations of the Virgo Cluster Elliptical Galaxies M84 and M86
• Baryon acoustic scale at $z_{\eff} = 0.166$ with the SDSS blue galaxies
• Determining the time before or after a galaxy merger event
• Foreground biases in strong gravitational lensing
• Constraining cosmological parameters using void statistics from the SDSS survey
• Euclid preparation. Sensitivity to non-standard particle dark matter model
• Characterizing the Best Cosmic Telescopes with the Millennium Simulations
• Influence of mergers on LyC escape of high redshift galaxies
• Galaxy-galaxy(-galaxy) lensing as a sensitive probe of galaxy evolution
• A toy model to test the accuracy of cosmological N-body simulations
• A comparison between semi-analytical gas cooling models and cosmological hydrodynamical simulations
• Alpha Shape Topology of the Cosmic Web
• Dry Merger Rate and Post-merger Fraction in the Coma Cluster Core
• Degradation analysis in the estimation of photometric redshifts from non-representative training sets
• The Halo Masses of Galaxies to $z\sim 3$: A Hybrid Observational and Theoretical Approach
• A hybrid multi resolution scheme to efficiently model the structure of reionization on the largest scales
• VisIVOWeb: A WWW Environment for Large-Scale Astrophysical Visualization
• CADISHI: Fast parallel calculation of particle-pair distance histograms on CPUs and GPUs
• Cosmic Cartography II: completing galaxy catalogs for gravitational-wave cosmology
• Evolution of matter and galaxy clustering in cosmological hydrodynamical simulations
• Euclid preparation. Simulating thousands of Euclid spectroscopic skies
• Red Dragon: A Redshift-Evolving Gaussian Mixture Model for Galaxies
• Measuring the growth of structure by matching dark matter haloes to galaxies with VIPERS and SDSS
• Paicos: A Python package for analysis of (cosmological) simulations performed with Arepo
• Recent stellar mass assembly of low-mass star-forming galaxies at redshifts 0.3 < z < 0.9
• Weak lensing magnification of Type Ia Supernovae from the Pantheon sample
• Gravitational Turbulence: the Small-Scale Limit of the Cold-Dark-Matter Power Spectrum
• The redshift distribution of BL Lacs and FSRQs
• KiDS+VIKING+GAMA: Testing semi-analytic models of galaxy evolution with galaxy-galaxy-galaxy lensing
• The galaxy power spectrum on the lightcone: deep, wide-angle redshift surveys and the turnover scale
• The preferentially magnified active nucleus in IRAS F10214+4724 - I. Lens model and spatially resolved radio emission
• Testing galaxy formation models with the stellar mass-halo mass relations for star-forming and quiescent galaxies
• The fate of the interstellar medium in early-type galaxies. IV. The impact of stellar feedback, mergers, and black holes on the cold ISM in simulated galaxies
• Dark-ages Reionization and Galaxy Formation Simulation - XV. Stellar evolution and feedback in dwarf galaxies at high redshift
• A Scaling Relation of the Evolving Tidal Fields in a LCDM Cosmology
• The influence of weak lensing on measurements of the Hubble constant with quad-image gravitational lenses
• MeV neutrino dark matter: Relic density, lepton flavour violation and electron recoil
• Understanding the cosmic web
• CFHTLenS: Galaxy bias as function of scale, stellar mass, and colour. Conflicts with predictions by semi-analytic models
• Unravelling the orbits of cluster galaxy populations according to their dominant gas ionization source
• The Beylkin-Cramer Summation Rule and A New Fast Algorithm of Cosmic Statistics for Large Data Sets
• Premature supermassive black hole mergers in cosmological simulations of structure formation
• Formation of satellites from cold collapse
• Magnesium isotope ratios in Milky Way and dwarf galaxy stars
• A High Throughput Workflow Environment for Cosmological Simulations
• Sub-MeV Bosonic Dark Matter, Misalignment Mechanism and Galactic Dark Matter Halo Luminosities
• Satellite Galaxies in the Illustris-1 Simulation: Poor Tracers of the Mass Distribution
• The Schr$\ddot{o}$dinger-Poisson equations as the large-N limit of the Newtonian N-body system: applications to the large scale dark matter dynamics
• The Impact of Non-Equipartition on Cosmological Parameter Estimation from Sunyaev-Zel'dovich Surveys
• Bose-Einstein Condensate Dark Matter Halos confronted with galactic rotation curves
• RX J1548.9+0851, a fossil cluster?
• Temporal Self-Organization in Galaxy Formation
• The Fates of Merging Supermassive Black Holes and a Proposal for a New Class of X-Ray Sources
• The formation and disruption of globular cluster populations in simulations of present-day $L^{\ast }$ galaxies with controlled assembly histories
• Quantifying the Projected Suppression of Cluster Escape Velocity Profiles
• The Bias of the Log Power Spectrum for Discrete Surveys
• Thinking outside the halo: Tracing the large-scale distribution of diffuse cosmic metals with semi-analytic models
• A comparison of the excess mass around CFHTLenS galaxy-pairs to predictions from a semi-analytic model using galaxy-galaxy-galaxy lensing
• Oct-tree Method on GPU
• Bimodal Formation Time Distribution for Infall Dark Matter Halos
• Constraining Dynamical Dark Energy Models through the Abundance of High-Redshift Supermassive Black Holes
• Large scale correlations in gas traced by MgII absorbers around low mass galaxies
• Transverse velocities and matter gradient correlations: a new signal and a new challenge to moving-lens analyses
• Unraveling emission line galaxy conformity at z~1 with DESI early data
• Joint constraints on galaxy bias and ${\sigma }_8$ through the N-pdf of the galaxy number density
• Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
• The miniJPAS & J-NEP surveys: Identification and characterization of the Ly$\alpha$ Emitter population and the Ly$\alpha$ Luminosity Function
• Cosmology in One Dimension: The Two Component Universe
• Gravitational fluctuations of the galaxy distribution
• The internal metallicity distributions of simulated galaxies from EAGLE, Illustris, and IllustrisTNG at z=1.8-4 as probed by Gamma Ray Burst hosts
• Detecting and Characterizing Young Quasars. III. The Impact of Gravitational Lensing Magnification
• Characterizing the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias
• The Circular Velocity Function of Group Galaxies
• Non-Gaussian assembly bias from a semi-analytic galaxy formation model
• Local variations of the Stellar Velocity Ellipsoid-I: the disc of galaxies in the Auriga simulations
• First Light and Reionisation Epoch Simulations (FLARES) X: Environmental Galaxy Bias and Survey Variance at High Redshift
• What is the optimal way to measure the galaxy power spectrum?
• Low Metallicity Galaxies from the Dark Energy Survey
• An observational signal of the void shape correlation and its link to the cosmic web
• The Rotational Profiles of Cluster Galaxies
• A study of relative velocity statistics in Lagrangian perturbation theory with PINOCCHIO
• A Search for Neutron Star Precession and Interstellar Magnetic Field Variations via Multiepoch Pulsar Polarimetry
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• Anisotropy and characteristic scales in halo density gradient profiles
• Protoclusters at z=5.7: A view from the MultiDark galaxies
• An observational detection of the bridge effect of void filaments
• Euclid preparation. Optical emission-line predictions of intermediate-z galaxy populations in GAEA for the Euclid Deep and Wide Surveys
• Understanding the AGN-Host Connection in Broad Mgii Emission Selected AGN-Host Hybrid Qausars
• Probing Satellite Halos with Weak Gravitational Lensing
• On rates of supernovae strongly lensed by galactic haloes in Millennium Simulation
• Studying light propagation in a locally homogeneous universe through an extended Dyer-Roeder approach
• Formation of Compact Clusters from High Resolution Hybrid Cosmological Simulations
• Dynamics of One-dimensional Self-gravitating Systems Using Hermite-Legendre Polynomials
• Sample variance in N--body simulations and impact on tomographic shear predictions
• A New Multi-Scale Structure Finding Algorithm to Identify Cosmological Structure
• High-Performance Astrophysical Simulations and Analysis with Python
• Scaling of the 1-halo terms with bias
• Bayesian analysis of cosmic structures
• Simulation-based marginal likelihood for cluster strong lensing cosmology
• Star formation and black hole accretion activity in rich local clusters of galaxies
• Locations of Satellite Galaxies in the Two-Degree Field Galaxy Redshift Survey
• On the problem of deformed spherical systems in Modified Newtonian Dynamics
• A Galaxy-Halo Model for Multiple Cosmological Tracers
• Cosmic Acceleration from Causal Backreaction in a Smoothly Inhomogeneous Universe
• The galaxy environment in GAMA G3C groups using the Kilo Degree Survey Data Release 3
• Intermediate Mass Black Holes: A brief review
• Dark-ages Reionization and Galaxy Formation Simulation - XIV. Gas accretion, cooling and star formation in dwarf galaxies at high redshift
• Spectroscopic characterization of the protocluster of galaxies around 7C 1756+6520 at z ~ 1.4
• Comment on "Hubble flow variations as a test for inhomogeneous cosmology"
• An unusual transient following the short GRB 071227
• Bound Dark Matter (BDM) towards solving the Small Scale Structure Problem
• Infall of galaxies onto groups
• Dependence of the ratio of total to visible mass on observable properties of SDSS MaNGA galaxies
• A near-infrared study of the obscured 3C129 galaxy cluster
• Cosmological boost factor for dark matter annihilation at redshifts of $z=10$-$100$ using the power spectrum approach
• Optical Microlensing by Primordial Black Holes with IACTs
• The THREEHUNDRED project: the effect of baryon processes at galaxy cluster scale
• Making use of sub-resolution halos in N-body simulations
• Galaxy and Mass Assembly (GAMA): Mid-infrared properties as tracers of galaxy environment
• Investigating the Dominant Environmental Quenching Process in UVCANDELS/COSMOS Groups
• The Dawn of Black Holes
• Conditional Colour-Magnitude Distribution of Central Galaxies in Galaxy Formation Models
• The hot gas distribution, X-ray luminosity and baryon budget in the L-Galaxies semi-analytic model of galaxy formation
• Exploring the multiband gravitational wave background with a semi-analytic galaxy formation model
• The long-lasting effect of X-ray preheating in the post-reionization intergalactic medium
• The influence of baryons on low-mass haloes
• The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity
• The PAU Survey: The quasar UV and Ly$\alpha$ luminosity functions at $2.7<z<5.3$
• Euclid preparation. Exploring the properties of proto-clusters in the Simulated Euclid Wide Survey
• First Light And Reionisation Epoch Simulations (FLARES) XVI: Size Evolution of Massive Dusty Galaxies at Cosmic Dawn from UV to IR
• Galaxy Assembly and Evolution in the P-Millennium simulation: galaxy clustering
• Bayesian analysis of spatially distorted cosmic signals from Poissonian data
• Introducing cosmosTNG: simulating galaxy formation with constrained realizations of the COSMOS field
• How do uncertainties in galaxy formation physics impact field-level galaxy bias?
• Simulations of the accreted stellar halos of low-mass field galaxies
• Modeling submillimeter galaxies in cosmological simulations: Contribution to the cosmic star formation density and predictions for future surveys
• Probing large-scale structures with the two-point function and the power spectrum: insights into cosmic clustering evolution
• Quantifying the Impact of Incompleteness on Identifying and Interpreting Galaxy Protocluster Populations with the TNG-Cluster Simulation
• The Milky Way in context: The formation of galactic discs and chemical sequences from a cosmological perspective
• Modelling the selection of galaxy groups with end to end simulations
• Microlensing of dark matter models in the Milky Way
• The impact of ram pressure on cluster galaxies, insights from GAEA and TNG
• Assessing the dark matter content of two quasar host galaxies at z~6 through gas kinematics
• Applying machine learning to Galactic Archaeology: how well can we recover the origin of stars in Milky Way-like galaxies?
• Active Galactic Nuclei in the Green Valley at z$\sim$0.7
• Three Spectacular HII-buried-AGN Galaxies from SDSS
• Digging deeper into NGC\,6868 I: stellar population
• Local variations of the Stellar Velocity Ellipsoid-II: the effect of the bar in the inner regions of Auriga galaxies
• ZFIRE: The Beginning of the End for Massive Galaxies at z ~ 2 and Why Environment Matters
• The Star Formation Reference Survey. IV. Stellar mass distribution of local star-forming galaxies
• The Formation and Evolution of Massive Galaxies
• The Effects of $\Lambda$CDM Dark Matter Substructure on the Orbital Evolution of Star Clusters
• Introduction to Tidal Streams
• A rare case of FR I interaction with a hot X-ray bridge in the A2384 galaxy cluster
• Warm dark matter model with a few keV mass is bad for the too-big-to-fail problem
• Cosmic Pathways for Compact Groups in the Milli-Millennium Simulation
• The Coarse Geometry of Merger Trees in ΛCDM
• Stochastic Absorption of the Light of Background Sources due to Intergalactic Neutral Hydrogen I. Testing different line-number evolution models via the cosmic flux decrement
• Evolution of the real-space correlation function from next generation cluster surveys
• Ultraviolet background fluctuations with clustered sources
• Characterising cosmic inhomogeneity with anomalous diffusion
• Solving the puzzle of subhalo spins
• The strongest gravitational lenses: IV. The order statistics of the largest Einstein radii with cluster mergers
• The Search for Million Degree Gas Through The NVII Hyperfine Line
• Evidence for the Evolution of Young Early-Type Galaxies in the GOODS/CDF-S Field
• Post-Newtonian Gravity in Cosmology
• The origin of the galaxy size-stellar metallicity relation: A semi-analytical perspective
• Cosmic Acceleration from Causal Backreaction with Recursive Nonlinearities
• CLASH-VLT: The variance in the velocity anisotropy profiles of galaxy clusters
• Predicting the Sufficient-Statistics Power Spectrum for Galaxy Surveys: A Recipe for $P_{A\ast }(k)$
• Searching for galaxy clusters in the VST-KiDS Survey
• The time evolution of bias
• Beyond the Halo: Redefining environment with unbound matter in N-body simulations
• Measuring galaxy abundance and clustering at high redshift from incomplete spectroscopic data: Tests on mock catalogs
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• Performance Enhancement of Tree-based Friends-of-friend Galaxy-finder for High-resolution Simulations of Galaxy Formation
• Inferring the density and membership of stellar streams with flexible models: The GD-1 stream in Gaia Data Release 3
• The present-day globular cluster kinematics of lenticular galaxies from the E-MOSAICS simulations and their relation to the galaxy assembly histories
• The Cosmic Mach Number as an Environment Measure for the Underlying Dark Matter Density Field
• Lagrangian Volume Deformations around Simulated Galaxies
• Astroinformatics Challenges from Next-generation Radio Continuum Surveys
• The energy shear of protohaloes
• High-redshift AGN population in radiation-hydrodynamics simulations
• Approximate methods for the generation of dark matter halo catalogs in the age of precision cosmology
• Fast radiative transfer of dust reprocessing in semi-analytic models with artificial neural networks
• SLICE: SPT-CL J0546-5345 -- A prominent strong-lensing cluster at $z=1.07$
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• Environmental Effects on the Star Formation Activity at z~0.9 in the COSMOS Field
• Cosmological parameters from Galaxy Clusters: an Introduction
• The influence of superstructures on bright galaxy environments: clustering properties
• The Diversity of Environments Around Luminous Quasars at Redshift $z\sim 6$
• Inferring Host Dark Matter Halo Masses of Individual Galaxies from Neighboring Galaxy Counts
• Physically motivated modeling of LyC escape fraction during reionization
• A graph model for the clustering of dark matter halos
• The velocity--shape alignment of clusters and the kinetic Sunyaev--Zeldovich effect
• Observed Cosmological Reexpansion in Minimal QFT with Bose and Fermi Fields
• Mapping dark matter and finding filaments: calibration of lensing analysis techniques on simulated data
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• Exploring the Cosmic Web in the Sloan Digital Sky Survey Data Release Seven using the Local Dimension
• GrAviPaSt's Lens to the Past: Unveiling the Evolution of Filamentary Structures
• Stochastic Super-resolution of Cosmological Simulations with Denoising Diffusion Models
• Using dust to constrain dark matter models
• A Full Accounting of the Visible Mass in SDSS MaNGA Disk Galaxies
• High performance cosmological simulations on a grid of supercomputers
• Merger rates of dark matter haloes: a comparison between EPS and N-body results
• More than just halo mass: Modelling how the red galaxy fraction depends on multiscale density in a HOD framework
• Testing extensions to LCDM on small scales with forthcoming cosmic shear surveys
• Bright siren without electromagnetic counterpart by LISA-Taiji-TianQin network
• Anisotropy of Nanohertz Gravitational Wave Background and Source Clustering from Supermassive Binary Black Holes Based on Cosmological Simulation
• Star formation histories of massive red spiral galaxies in the local universe
• Quantifying the effect of field variance on the H$\alpha$ luminosity function with the New Numerical Galaxy Catalogue (${\nu }^2$GC)
• Structure in Galaxy Distribution. III. Fourier Transforming the Universe
• Effects of Biases in Virial Mass Estimation on Cosmic Synchronization of Quasar Accretion
• Sensitivity and Insensitivity of Galaxy Cluster Surveys to New Physics
• AstroGrid-D: Grid Technology for Astronomical Science
• Dust sub-millimetre emission in green valley galaxies
• Galaxy Interactions, Star Formation History, and Bulgeless Galaxies
• Integrated HI emission in galaxy groups and clusters
• The SAMI Galaxy Survey: The relationship between galaxy rotation and the motion of neighbours
• Simulations and Observations of the Microwave Universe
• Caught in the cosmic web: environmental effects on subhalo abundance and internal density profiles
• DARKSKIES: A suite of super-sampled zoom-in simulations of galaxy clusters with self-interacting dark matter
• Effective Operators for Dark Matter Interactions
• Impact of Cosmic Variance on the Galaxy-Halo Connection for Lyman-$\alpha$ Emitters
• Spectral Signatures of Quasar Ages at z~3
• A Heating Model for the Millennium Gas Run
• FAST drift scan survey for HI intensity mapping: simulation on hunting HI filament with pairwise stacking
• A Multiple Dry Merger at z=0.18: Witnessing The Assembly of a Massive Elliptical Galaxy
• Dissecting the mass quenching in TNG50: Galaxy size determines the quenching mode
• The Formation of M101-alike Galaxies in the Cold Dark Matter Model
• Accreted stars and stellar haloes of simulated galaxies in TNG50
• The Complexity and Information Content of Simulated Universes
• Low-resolution near-infrared spectroscopic signatures of unresolved ultracool companions to M dwarfs
• Constraints on the galaxy formation models during epoch of reionization with high redshift observations
• Evolution of Cluster Alignments as Evidence of Large-scale Structure Formation in the Universe
• The environment of QSO triplets at 1 $\lesssim$ z $\lesssim$ 1.5
• A 15 Mpc rotating galaxy filament at redshift z = 0.032
• Gravitational interaction signatures in isolated galaxy triplet systems: a photometric analysis
• Orientation of galaxies in structures
• Bending the web: exploring the impact of modified gravity on the density field and halo properties within the cosmic web
• On the spin distributions of $\Lambda$CDM haloes
• An Improved and Parallel Version of a Scalable Algorithm for Analyzing Time Series Data
• Testing an entropy estimator related to the dynamical state of galaxy clusters
• Evolution of the star formation rate surface density main sequence. Insights from a semi-analytic simulation since $z=12$
• Merging history of massive galaxies at 3<z<6
• Merger Tree-based Galaxy Matching: A Comparative Study Across Different Resolutions
• Constrained correlation functions from the Millennium Simulation
• Witnessing the formation of a brightest cluster galaxy at z>2
• Pearls on a string: Dark and bright galaxies on a strikingly straight and narrow filament
• The size and mass evolution of the massive galaxies over cosmic time
• The Hidden Role of Anisotropies in Shaping Structure Formation in Cosmological N-Body Simulations
• Distinguishing thermal histories of dark matter from structure formation
• Searching for Intragroup Light in Deep U-band Imaging of the COSMOS Field
• Method for Determining AGN Accretion Phase in Field Galaxies
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• Dust contribution to the panchromatic galaxy emission
• A MeerKAT study of a neutral hydrogen rich grouping of galaxies with megaparsec-scale filamentary-like structure
• The dynamical evolution of the stellar clumps in the Sparkler galaxy
• Properties of the Environment of Galaxies in Clusters of Galaxies CL 0024+1654 and RX J0152.7-1357
• What is the right way to quench star formation in semi-analytic model of galaxy formation?
• Does stellar mass assembly history vary with environment?
• Predicting Steady States of One-dimensional Collisionless Gravitating Systems
• A sparse regression approach for populating dark matter halos and subhalos with galaxies
• Halo concentration strengthens dark matter constraints in galaxy-galaxy strong lensing analyses
• Long-term implications of observing an expanding cosmological civilization
• SZ power spectrum and cluster numbers from an extended merger-tree model
• Energy Ranking Preservation in a N-Body Cosmological Simulation
• The AIDA-TNG project: 3D halo shapes
• Submillimeter galaxy overdensities around physically associated quasar pairs
• Upcoming SKA precursor surveys and sensitivity to HI mass function
• Galaxy Cluster Mass Estimation Through The Splashback Radius
• Non-Gaussian statistics in galaxy weak lensing: compressed three-point correlations and cosmological forecasts
• Estimating infall times of galaxies around clusters: how accurately can it be done with observational data?
• Detector Optimization Studies and Light Higgs Decay into Muons at CLIC
• Euclid preparation: TBD. Cosmic Dawn Survey: evolution of the galaxy stellar mass function across 0.2<z<6.5 measured over 10 square degrees
• Chandra and XMM-Newton observations of the merging cluster of galaxies PLCK G036.7+14.9
• Mock X-ray observations of hot gas with L-Galaxies semi-analytic models of galaxy formation
• The imprints of massive neutrinos on the three-point correlation function of large-scale structures
• The FLAMINGO simulations data release
• The intervelocity of galaxy pairs in $\Lambda$CDM -- The observed velocity peak at ~130 km/s is not unique to MOND
• Exploring the Universe with Metal-Poor Stars
• Evolution of Cosmic Voids in the Schrodinger-Poisson Formalism
• Cosmology with Cosmic Voids
• The HST-Hyperion Survey: Companion Fraction and Overdensity in a z ~ 2.5 Proto-supercluster
• Delensing for Precision Cosmology: Optimizing Future CMB B-mode Surveys to Constrain r
• A statistical test to identify differences in clustering structures
• Holographic Principle and the Second Law in Stephani Cosmology Revisited
• The probability distribution of 3-D shapes of galaxy clusters from 2-D X-ray images
• Magnetic Reconnection as a Potential Driver of X-ray Variability in Active Galactic Nuclei
• Visualization in Astrophysics: Developing New Methods, Discovering Our Universe, and Educating the Earth
• VEGA: Voids idEntification using Genetic Algorithm
• CLASH-VLT velocity anisotropy profiles in a stack of massive galaxy clusters
• Exploring the anisotropic gravitational wave background from all-sky mock gravitational wave event catalogues
• The relation of galaxies and dark matter haloes to the filamentary cosmic web
• Self-similarity and stable clustering in a family of scale-free cosmologies
• Build-up and survival of the disc: From numerical models of galaxy formation to the Milky Way
• Can we constrain the evolution of HI bias using configuration entropy?
• Directional miscentering dependence in weak lensing mass bias
• Extracting cosmological signals from foregrounds in deep mm maps of the sky
• Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
• The Environments of Star-Forming Galaxies Detected in the SFACT Survey: Do Mergers and Interactions Drive the Star Formation?
• The invariance of group occupation across the cosmic web
• Effects of light-mass fermionic dark matter on the equilibrium and stability of white dwarfs
• An Interpretable AI Framework to Disentangle Self-Interacting and Cold Dark Matter in Galaxy Clusters: The CKAN Approach
• Scaling relations of early-type galaxies in MOND
• Deciphering galaxy images using machine vision -- Combining variational autoencoder and principal component analysis for feature extraction
• Morphological Feature Distances Among the Spectral Types of SDSS Galaxies
• The richest superclusters. I. Morphology
• The implications of overmassive black holes at $z>5$ for quasar and black hole growth
• Baryon Acoustic Oscillations from galaxy surveys
• Obscured and unobscured X-ray AGNs I: Host galaxy properties
• Quantifying the impact of detection bias from blended galaxies on cosmic shear surveys
• Cosmic structure from the path integral of classical mechanics and its comparison to standard perturbation theory
• Adaptive friends-of-friends algorithm for identifying gravitationally bound cosmological structures
• Massive Star Clusters in the Semi-Analytical Galaxy Formation Model L-Galaxies 2020
• Cross Section Calculations in Theories of Self-Interacting Dark Matter
• On the dependence of galaxy assembly bias on the selection criteria, number density, and redshift of galaxy samples
• Compact groups from semi-analytical models of galaxy formation -- VI: Evolution of the two first-ranked galaxies
• Are dark matter and dark energy omnipresent?
• Two categories of UV-upturn galaxies revealed by semi-analytic models
• JERALD: high-fidelity dark matter, stellar mass and neutral hydrogen maps from fast N-body simulations
• How Many Bursts Does it Take to Form a Core at the Center of a Galaxy?
• Predicting halo occupation and galaxy assembly bias with machine learning
• Exploring the evolution of red and blue galaxies in different cosmic web environments using IllustrisTNG simulation
• Past, present and Future of the Scaling Relations of Galaxies and Active Galactic Nuclei
• MOSS I: Double radio relics in the Saraswati supercluster
• How to Price Shared Optimizations in the Cloud
• Estimating the Masses of Supercluster-Scale Filaments from Redshift Dispersions
• The VIMOS VLT Deep Survey. The different assembly history of passive and star-forming L_B >= L*_B galaxies in the group environment at z < 1
• Probing the Large-Scale Homogeneity of the Universe with Galaxy Redshift Surveys
• Testing the thermal Sunyaev-Zel'dovich power spectrum of a halo model using hydrodynamical simulations
• The haloes that reionized the Universe
• Estimating the mass of galactic components using machine learning algorithms
• Merging Rates of the First Objects and the Formation of First Mini-Filaments in Models with Massive Neutrinos
• Cosmic Dragons: A Two-Component Mixture Model of COSMOS Galaxies
• Dissecting the Thermal SZ Power Spectrum by Halo Mass and Redshift in SPT-SZ Data and Simulations
• The Galaxy and its stellar halo - insights from a hybrid cosmological approach
• Validating the Universe in a Box
• Graviton spectrum in simplified Dark Matter models with graviton mediators in the de Sitter space
• Can we constrain galaxy geometry parameters using spatially integrated SED fitting?
• Early-type Dwarf Galaxies in the Local Universe. Evidence of Ex-situ Growth
• Discovery of a New Quasar: SDSS J022155.26-064916.6
• Cosmological evolution of gas and supermassive black holes in idealized isolated halos
• Extended Hernquist-Springel formalism for cosmic star formation
• Unequal-mass mergers of dark matter haloes with rare and frequent self-interactions
• First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmic dawn
• A Hydro-Particle-Mesh Code for Efficient and Rapid Simulations of the Intracluster Medium
• Constraining the mSUGRA parameter space using the entropy of dark matter halos
• Dynamical masses of early-type galaxies at z~2
• The effect of hydrodynamics alone on the subhalo population in a $\Lambda$CDM rich cluster sized dark matter halo
• Dark matter haloes in the multicomponent model. III. From dwarfs to galaxy clusters
• Angular momentum and morphological sequence of massive galaxies through Dark Sage
• Transients from Initial Conditions Based on Lagrangian Perturbation Theory in $N$-body Simulations III: The Case of GADGET-2 Code
• Particle Physics in the Sky and Astrophysics Underground: Connecting the Universe's Largest and Smallest Scales
• Discovery of a New Blue Quasar: SDSS J022218.03-062511.1
• Gravity-mediated Dark Matter models in the de Sitter space
• Impact of Gravitational Slingshot of Dark Matter on Galactic Halo Profiles
• Evolution of the Pancaking Effect in a LCDM Cosmology
• Fast generation of mock maps from realistic catalogs of astrophysical objects
• Dark Energy Simulations
• The S-PLUS Fornax Project (S+FP): An extragalactic catalog covering $\sim$ 5 virial radii around NGC 1399 with galaxy properties
• Halo detection via large-scale Bayesian inference
• ngravs: Distinct gravitational interactions in GADGET-2
• Faint galaxies in the Zone of Avoidance revealed by JWST/NIRCam
• Galaxy assembly bias in cosmological hydrodynamical simulations: a comparison between SIMBA and IllustrisTNG
• Statistical Properties of Cold Streams In Massive Star-Forming Halos in TNG50
• Star clusters as building blocks for dSph galaxies formation
• High-Redshift Galactic Outflows: Orientation Effects, Kinematics, and Metallicity in TNG50 and SERRA
• J-PAS: First Identification, Physical Properties and Ionization Efficiency of Extreme Emission Line Galaxies
• HR-GO II: chemical abundances of low-$E$ retrograde dynamically-tagged-groups: Revealing Thamnos as a very metal-poor substructure
• The Galaxy Evolution Probe
• Fueling and feedback mechanisms at the nodes of the cosmic web
• Capturing dual AGN activity and kiloparsec-scale outflows in IRAS 20210+1121
• Indicator Power Spectra: Surgical Excision of Non-linearities and Covariance Matrices for Counts in Cells
• The BUFFALO HST Survey
• Quasar clustering at redshift 6
• From Black Holes to Cosmology : The Universe in the Computer
• Yellow Post-Asymptotic-Giant-Branch Stars as Standard Candles. I. Calibration of the Luminosity Function in Galactic Globular Clusters
• Understanding galaxy formation and evolution through an all-sky submillimetre spectroscopic survey
• The Splashback Mass Function of Galaxy Clusters from Photometric Data
• Galaxy clustering in the VVV Near-IR Galaxy Catalogue
• Entropy Production in Collisionless Systems. III. Results from Simulations
• Observed cosmic evolution of galaxy dust properties with metallicity and tensions with models
• Constraining the shape of Milky Way satellites with distance gradients
• Tips learned from panchromatic modeling of AGNs
• The SRG/eROSITA all-sky survey: The morphologies of clusters of galaxies: II. The intrinsic distributions of morphological parameters
• On the Orbital Velocity of Isolated Galaxy Pairs: a test of gravity in the low acceleration regime
• (1+1)-Dimensional Schrödinger-Poisson equation with contact interaction
• Testing the key role of the stellar mass-halo mass relation in galaxy merger rates and morphologies via DECODE, a novel Discrete statistical sEmi-empiriCal mODEl
• Cylindrical cosmological simulations with StePS
• The Dark Side Properties of Galaxies Requires (viable) Modifications to the Verlinde's Emergent Gravity Theory
• Particle loads for cosmological simulations with equal-mass dark matter and baryonic particles
• The Distribution of Satellite Galaxies in the TNG100 Simulation
• Cross-correlations between X-ray clusters and the general galaxy population
• Validating the CROCODILE model within the AGORA galaxy simulation framework
• Euclid: A blue galaxy population and a brightest cluster galaxy in the making in a $z\sim 1.74$ MaDCoWS2 galaxy cluster candidate
• A lightcone catalogue from the Millennium-XXL simulation: improved spatial interpolation and colour distributions for the DESI BGS
• Fast Baryonic Field Painting for Sunyaev-Zel'dovich Analyses: Transfer Function vs. Hybrid Effective Field Theory
• Cosmological bounds on dark matter annihilation using dark ages 21-cm signal
• Massive Neutrinos Promote the Size Growth of Early-Type Galaxies
• First Steps Toward a Method for Estimating Cosmological Parameters using Strong Lensing, X-ray and Dynamics Total Mass Estimates
• Variational autoencoder for generating realistic $N$-body simulations for dark matter halos
• Phase-space perturbation theory for cosmic large-scale structure
• Assembly History and Internal Structure of Cluster Cold Dark Matter Haloes
• Large-scale peculiar velocities through the galaxy luminosity function at z ~ 0.1
• The Filament Rift: $\Lambda$CDM's Structural Challenge Against Observation
• Controlled Experiments on Dark-Matter Halo Structure and Galaxy Morphology I: What Sets Galaxy Sizes?
• Scaling Relations Between Low-mass Black Holes and Their Host Galaxies
• Beowulf Analysis Symbolic INterface BASIN: Interactive Parallel Data Analysis for Everyone
• Primordial Fluctuations in String Cosmology
• The History of Galaxy Mergers in IllustrisTNG
• The early gaseous and stellar mass assembly of Milky Way-type galaxy halos
• Visualising Matter and Cosmologies: A Transhistorical Example
• Tracing Cosmological Signature with Doppler Lensing: Insights from Cosmological Simulations
• Molecular Cloud Fragmentation and Core Collapse
• Euclid preparation. 3D reconstruction of the cosmic web with simulated Euclid Deep spectroscopic samples
• The Journey to Dominance: How BCGs Evolve Differently from Other Massive Galaxies
• Are globular clusters the natural outcome of regular high-redshift star formation?
• A multiwavelength study of near- and mid-infrared selected galaxies at high redshift: ERGs, AGN-identification and the contribution from dust
• Contrasting evolutionary pathways of fast- and slow-rotating galaxies in the green valley
• Euclid preparation. Predicting star-forming galaxy scaling relations with the spectral stacking code SpectraPyle
• POLAR-II: modeling star formation history of galaxies on the 21-cm signal from Epoch of Reionization
• VADER - A Satellite Mission Concept For High Precision Dark Energy Studies
• Cosmic velocity, density and halo mass function: Insights from deep learning
• Estimating Transient Rates from Cosmological Simulations and BPASS
• Merging Galaxy Clusters and the Search for New Physics of Dark Matter: A Review
• ScaleFree: Dynamic KDE for Multiscale Point Cloud Exploration in VR
• Spheroid ages, kinematics and BH relations
• Galaxies in the central regions of simulated galaxy clusters
• Mass transport in galaxy discs limits black hole growth to sub-Eddington rates
• Exploring the effect of baryons on the radial distribution of satellite galaxies with GAMA and IllustrisTNG
• Constraining the MOdified Newtonian Dynamics from spherically symmetrical hydrodynamic accretion
• Sahyadri: A simulation suite for the cosmology dependence of the Cosmic Web
• Dark Universe and distribution of Matter as Quantum Imprinting: the Quantum Origin of Universe
• Starburst galaxies in the Hydra I cluster
• Streaming Velocity Effects on the Post-reionization 21 cm Baryon Acoustic Oscillation Signal
• Compact Groups in GDM Cosmological Simulations
• The structural elements of the cosmic web
• PatchworkWave: A Multipatch Infrastructure for Multiphysics/Multiscale/Multiframe/Multimethod Simulations at Arbitrary Order
• Disk Sizes in a LCDM Universe
• Using Unreal Engine to Visualize a Cosmological Volume
• Mentari: A pipeline to model the galaxy SED using semi analytic models
• Joint Optical-HI mock catalogues and prospects for upcoming HI surveys
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
• UV bright red-sequence galaxies: a comparative study between UV upturn and UV weak systems
• Ultra-fast model emulation with PRISM; analyzing the Meraxes galaxy formation model
• The formation of blue cluster in local Universe
• Third-Generation Calibrations for MeerKAT observation
• A general framework for unbiased tests of gravity using galaxy clusters
• The Photometric Analysis of the Environment Around Two Dusty Star-Forming Galaxies at $z\sim 2$
• Black Hole-Galaxy Correlations in Cluster Zoomed-in Simulations: GIZMO-SIMBA and TNG-Cluster