The cosmological simulation code GADGET-2

Abstract

We discuss the cosmological simulation code GADGET-2, a new massively parallel TreeSPH code, capable of following a collisionless fluid with the N-body method, and an ideal gas by means of smoothed particle hydrodynamics (SPH). Our implementation of SPH manifestly conserves energy and entropy in regions free of dissipation, while allowing for fully adaptive smoothing lengths. Gravitational forces are computed with a hierarchical multipole expansion, which can optionally be applied in the form of a TreePM algorithm, where only short-range forces are computed with the `tree'-method while long-range forces are determined with Fourier techniques. Time integration is based on a quasi-symplectic scheme where long-range and short-range forces can be integrated with different timesteps. Individual and adaptive short-range timesteps may also be employed. The domain decomposition used in the parallelisation algorithm is based on a space-filling curve, resulting in high flexibility and tree force errors that do not depend on the way the domains are cut. The code is efficient in terms of memory consumption and required communication bandwidth. It has been used to compute the first cosmological N-body simulation with more than 10^10 dark matter particles, reaching a homogeneous spatial dynamic range of 10^5 per dimension in a 3D box. It has also been used to carry out very large cosmological SPH simulations that account for radiative cooling and star formation, reaching total particle numbers of more than 250 million. We present the algorithms used by the code and discuss their accuracy and performance using a number of test problems. GADGET-2 is publicly released to the research community.

submitted to MNRAS, 31 pages, 20 figures (reduced resolution), code available at http://www.mpa-garching.mpg.de/gadget

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• A fresh look at linear cosmological constraints on a decaying dark matter component
• Galactic Archaeology with asteroseismic ages: evidence for delayed gas infall in the formation of the Milky Way disc
• Understanding higher-order nonlocal halo bias at large scales by combining the power spectrum with the bispectrum
• The transition from population III to population II-I star formation
• Chemical Evolution in Hierarchical Models of Cosmic Structure II: The Formation of the Milky Way Stellar Halo and the Distribution of the Oldest Stars
• Cosmological $N$-body simulations with suppressed variance
• A Necessary Condition for Individual Time-Steps in SPH Simulations
• Intensity Mapping with Carbon Monoxide Emission Lines and the Redshifted 21 cm Line
• Contrasting Galaxy Formation from Quantum Wave Dark Matter, $\psi$DM, with $\Lambda$CDM, using Planck and Hubble Data
• A refined sub-grid model for black hole accretion and AGN feedback in large cosmological simulations
• Non-thermal pressure support in X-COP galaxy clusters
• Constraints on the Dark Matter Particle Mass from the Number of Milky Way Satellites
• The First Billion Years project - III: The impact of stellar radiation on the coevolution of Populations II and III
• The Meaning and Consequences of Star Formation Criteria in Galaxy Models with Resolved Stellar Feedback
• On the [CII]-SFR relation in high redshift galaxies
• Titans of the Early Universe: The Prato Statement on the Origin of the First Supermassive Black Holes
• Unexpectedly large mass loss during the thermal pulse cycle of the red giant R Sculptoris!
• Simulations of star formation in a gaseous disc around sgr A* - a failed AGN
• The MICE Grand Challenge Lightcone Simulation III: Galaxy lensing mocks from all-sky lensing maps
• Structure Finding in Cosmological Simulations: The State of Affairs
• Mock galaxy catalogs using the quick particle mesh method
• DEMNUni: The clustering of large-scale structures in the presence of massive neutrinos
• The Neutral Hydrogen Content of Galaxies in Cosmological Hydrodynamic Simulations
• The velocity function in the local environment from LCDM and LWDM constrained simulations
• Simulations of the grand design galaxy M51: a case study for analysing tidally induced spiral structure
• Implementation of feedback in SPH: towards concordance of methods
• Quantifying baryon effects on the matter power spectrum and the weak lensing shear correlation
• SubHaloes going Notts: The SubHalo-Finder Comparison Project
• A chronicle of galaxy mass assembly in the EAGLE simulation
• Euclid preparation: II. The EuclidEmulator -- A tool to compute the cosmology dependence of the nonlinear matter power spectrum
• Simulating the Universe with MICE: The abundance of massive clusters
• Cosmology with the shear-peak statistics
• Mass Function Predictions Beyond LCDM
• The UV continua and inferred stellar populations of galaxies at z ~ 7 - 9 revealed by the Hubble Ultra Deep Field 2012 campaign
• Impact of baryon physics on dark matter structures: a detailed simulation study of halo density profiles
• Weak Lensing Measurement of the Mass--Richness Relation of SDSS redMaPPer Clusters
• STARFORGE: Toward a comprehensive numerical model of star cluster formation and feedback
• Lightcone mock catalogues from semi-analytic models of galaxy formation - I. Construction and application to the BzK colour selection
• The Population of Dark Matter Subhaloes: Mass Functions and Average Mass Loss Rates
• Can Feedback Solve the Too Big to Fail Problem?
• Spitzer/MIPS Infrared Imaging of M31: Further Evidence for a Spiral/Ring Composite Structure
• A Density Independent Formulation of Smoothed Particle Hydrodynamics
• N-body Dark Matter Haloes with simple Hierarchical Histories
• Halo Stochasticity from Exclusion and non-linear Clustering
• Modified Gravity-GADGET: A new code for cosmological hydrodynamical simulations of modified gravity models
• The detectability of baryonic acoustic oscillations in future galaxy surveys
• The origin of ultra diffuse galaxies: stellar feedback and quenching
• Short-lived star-forming giant clumps in cosmological simulations of z~2 disks
• Modelling Baryon Acoustic Oscillations with Perturbation Theory and Stochastic Halo Biasing
• Simulations of Wide-Field Weak Lensing Surveys I: Basic Statistics and Non-Gaussian Effects
• The Star Formation Histories of Local Group Dwarf Galaxies II. Searching For Signatures of Reionization
• When Feedback Fails: The Scaling and Saturation of Star Formation Efficiency
• Bulk Viscosity Effects in Event-by-Event Relativistic Hydrodynamics
• Astrophysical Smooth Particle Hydrodynamics
• Consistent modelling of the meta-galactic UV background and the thermal/ionization history of the intergalactic medium
• Contributions to the accreted stellar halo: an atlas of stellar deposition
• Measurements of the UV background at 4.6 < z < 6.4 using the quasar proximity effect
• The Dust-to-Gas and Dust-to-Metals Ratio in Galaxies from z=0-6
• Vertical disc heating in Milky Way-sized galaxies in a cosmological context
• Constraints on neutrino masses from Lyman-alpha forest power spectrum with BOSS and XQ-100
• Large-scale Bias and Efficient Generation of Initial Conditions for Non-Local Primordial Non-Gaussianity
• The impact of galaxy formation on the total mass, mass profile and abundance of haloes
• Determining the Properties and Evolution of Red Galaxies from the Quasar Luminosity Function
• The Small Covering Factor of Cold Accretion Streams
• Tracing the Dark Matter Sheet in Phase Space
• And yet it moves: The dangers of artificially fixing the Milky Way center of mass in the presence of a massive Large Magellanic Cloud
• The power of infrared AGN selection in mergers: a theoretical study
• Long troughs in the Lyman-$\alpha$ forest below redshift 6 due to islands of neutral hydrogen
• An excess of small-scale gravitational lenses observed in galaxy clusters
• The MultiDark Database: Release of the Bolshoi and MultiDark Cosmological Simulations
• The Unorthodox Orbits of Substructure Halos
• Shaping the galaxy stellar mass function with supernova- and AGN-driven winds
• An MHD Gadget for cosmological simulations
• Dark Energy Survey Year 3 Results: Redshift Calibration of the Weak Lensing Source Galaxies
• Accurate, Meshless Methods for Magneto-Hydrodynamics
• Multi-Point Propagators in Cosmological Gravitational Instability
• A Theoretical Interpretation of the Black Hole Fundamental Plane
• The BAHAMAS project: the CMB--large-scale structure tension and the roles of massive neutrinos and galaxy formation
• The Sherwood simulation suite: overview and data comparisons with the Lyman-alpha forest at redshifts 2 < z < 5
• Galactic Centre stellar winds and Sgr A* accretion
• An algorithm to build mock galaxy catalogues using MICE simulations
• The Formation of High Redshift Submillimeter Galaxies
• Tracing Inflows and Outflows with Absorption Lines in Circumgalactic Gas
• Feedback first: the surprisingly weak effects of magnetic fields, viscosity, conduction, and metal diffusion on galaxy formation
• Galactic r-process enrichment by neutron star mergers in cosmological simulations of a Milky Way-mass galaxy
• Chemical signatures of formation processes in the stellar populations of simulated galaxies
• Supermassive black holes in cosmological simulations I: M_BH-M_star relation and black hole mass function
• Giant radio relics in galaxy clusters: reacceleration of fossil relativistic electrons?
• The upper bound on the lowest mass halo
• Massive and Refined. II. The statistical properties of turbulent motions in massive galaxy clusters with high spatial resolution
• Massive Halos in Millennium Gas Simulations: Multivariate Scaling Relations
• On the influence of ram-pressure stripping on the star formation of simulated spiral galaxies
• Tidal Effects and the Environment Dependence of Halo Assembly
• Blinded challenge for precision cosmology with large-scale structure: results from effective field theory for the redshift-space galaxy power spectrum
• Intracluster stars in simulations with AGN feedback
• Evolution of binary black holes in self gravitating discs: dissecting the torques
• Constraining the Statistics of Population III Binaries
• Large-scale dark matter simulations
• Properties of gas in and around galaxy haloes
• Angular momentum evolution of galaxies in EAGLE
• Minimizing the stochasticity of halos in large-scale structure surveys
• Simulating cosmic rays in clusters of galaxies - II. A unified scheme for radio halos and relics with predictions of the gamma-ray emission
• Precision measurement of the local bias of dark matter halos
• The quenching and morphological evolution of central galaxies is facilitated by the feedback-driven expulsion of circumgalactic gas
• Baryon Census in Hydrodynamical Simulations of Galaxy Clusters
• A Simple Technique for Predicting High-Redshift Galaxy Evolution
• Neutral hydrogen in galaxy halos at the peak of the cosmic star formation history
• Detecting the Rise and Fall of 21 cm Fluctuations with the Murchison Widefield Array
• The CO-H2 Conversion Factor in Disc Galaxies and Mergers
• Cosmological Tests of Gravity
• A direct measurement of the baryonic mass function of galaxies & implications for the galactic baryon fraction
• Reconstructing the Last Major Merger of the Milky Way with the H3 Survey
• The chosen few: the low mass halos that host faint galaxies
• Subsonic turbulence in smoothed particle hydrodynamics and moving-mesh simulations
• On Sizes, Kinematics, M/L Gradients, and Light Profiles of Massive Compact Galaxies at z~2
• On Lyman-limit Systems and the Evolution of the Intergalactic Ionizing Background
• On the impact of empirical and theoretical star formation laws on galaxy formation
• Forming Early-Type Galaxies in LambdaCDM Simulations -I. Assembly histories
• Matter power spectrum and the challenge of percent accuracy
• Subhalo abundance matching and assembly bias in the EAGLE simulation
• The number and size of subhalo-induced gaps in stellar streams
• The abundance of (not just) dark matter haloes
• The darkness that shaped the void: dark energy and cosmic voids
• Measuring Baryon Acoustic Oscillations along the line of sight with photometric redshifs: the PAU survey
• Mapping galaxy encounters in numerical simulations: The spatial extent of induced star formation
• The Bispectrum in the Effective Field Theory of Large Scale Structure
• Dissipation and Extra Light in Galactic Nuclei: I. Gas-Rich Merger Remnants
• Black Holes' Dark Dress: On the merger rate of a subdominant population of primordial black holes
• Cosmology with massive neutrinos I: towards a realistic modeling of the relation between matter, haloes and galaxies
• A Magellanic Origin of the DES Dwarfs
• Discovery of a Ringlike Dark Matter Structure in the Core of the Galaxy Cluster Cl 0024+17
• TreeCol: a novel approach to estimating column densities in astrophysical simulations
• Cosmic ray feedback in the FIRE simulations: constraining cosmic ray propagation with GeV gamma ray emission
• The one-dimensional power spectrum from the SDSS DR14 Ly$\alpha$ forests
• An efficient implementation of massive neutrinos in non-linear structure formation simulations
• Effects of AGN feedback on LCDM galaxies
• Moving mesh cosmology: the hydrodynamics of galaxy formation
• The EAGLE simulations: atomic hydrogen associated with galaxies
• Massive optimal data compression and density estimation for scalable, likelihood-free inference in cosmology
• A dark matter profile to model diverse feedback-induced core sizes of $\Lambda$CDM haloes
• Full-sky Gravitational Lensing Simulation for Large-area Galaxy Surveys and Cosmic Microwave Background Experiments
• Seeding the formation of cold gaseous clouds in Milky Way size halos
• Constraints from Ly-$\alpha$ forests on non-thermal dark matter including resonantly-produced sterile neutrinos
• Star formation and molecular hydrogen in dwarf galaxies: a non-equilibrium view
• Formation of Isolated Dwarf Galaxies with Feedback
• Dust Formation in Milky Way-like Galaxies
• Large-scale non-Gaussian mass function and halo bias: tests on N-body simulations
• The Warm DM halo mass function below the cut-off scale
• Growing the first bright quasars in cosmological simulations of structure formation
• Cluster Magnetic Fields from Galactic Outflows
• The Difficulty of Getting High Escape Fractions of Ionizing Photons from High-redshift Galaxies: a View from the FIRE Cosmological Simulations
• The impact of mechanical AGN feedback on the formation of massive early-type galaxies
• A Physical Model for z~2 Dust Obscured Galaxies
• X-ray coronae in simulations of disc galaxy formation
• A test suite for quantitative comparison of hydrodynamics codes in astrophysics
• The role of minor mergers in the recent star formation history of early-type galaxies
• The dust mass in z > 6 normal star forming galaxies
• `Eppur Si Muove': On The Motion of the Acoustic Peak in the Correlation Function
• High Performance P3M N-body code: CUBEP3M
• ELUCID - Exploring the Local Universe with reConstructed Initial Density field I: Hamiltonian Markov Chain Monte Carlo Method with Particle Mesh Dynamics
• Cosmology constraints from shear peak statistics in Dark Energy Survey Science Verification data
• Simulations of ram-pressure stripping in galaxy-cluster interactions
• Dark matter haloes determine the masses of supermassive black holes
• Quantifying the impact of mergers on the angular momentum of simulated galaxies
• A Measurement of Small Scale Structure in the 2.2 < z < 4.2 Lyman-alpha Forest
• The nature and evolution of the highly ionized near-zones in the absorption spectra of z~6 quasars
• The gas distribution in the outer regions of galaxy clusters
• Stellar Feedback & Bulge Formation in Clumpy Disks
• Insights into the content and spatial distribution of dust from the integrated spectral properties of galaxies
• A fundamental problem in our understanding of low mass galaxy evolution
• The dynamics and outcome of star formation with jets, radiation, winds, and supernovae in concert
• The Effect of Thermal Neutrino Motion on the Non-linear Cosmological Matter Power Spectrum
• On the role of AGN feedback on the thermal and chemodynamical properties of the hot intra-cluster medium
• The onion universe: all sky lightcone simulations in spherical shells
• Cosmological constraints with deep learning from KiDS-450 weak lensing maps
• The role of star-formation and AGN in dust heating of z = 0.3-2.8 galaxies - I. Evolution with redshift and luminosity
• The properties of satellite galaxies in simulations of galaxy formation
• Possible evidence for an inverted temperature-density relation in the intergalactic medium from the flux distribution of the Lyman-alpha forest
• Bias-Hardened CMB Lensing
• Strong lensing optical depths in a \LambdaCDM universe
• Metal and molecule cooling in simulations of structure formation
• Metal and molecule cooling in simulations of structure formation
• Cold accretion flows and the nature of high column density HI absorption at redshift 3
• The baryon fraction of LambdaCDM haloes
• Dissipation and Extra Light in Galactic Nuclei: III. 'Core' Ellipticals and 'Missing' Light
• Star formation quenching in simulated group and cluster galaxies: When, how, and why?
• The MUSIC of CLASH: predictions on the concentration-mass relation
• gevolution: a cosmological N-body code based on General Relativity
• SPHinXsys: an open-source multi-physics and multi-resolution library based on smoothed particle hydrodynamics
• Global structure and kinematics of stellar haloes in cosmological hydrodynamic simulations
• Modified Gravity N-body Code Comparison Project
• Rise and Fall of Radio Halos in Simulated Merging Galaxy Clusters
• Why stellar feedback promotes disc formation in simulated galaxies
• Vlasov methods in space physics and astrophysics
• Non-Equilibirum ionisation and cooling of metal-enriched gas in the presence of a photo-ionisation background
• Dark Energy Survey Year 1 Results: Methods for Cluster Cosmology and Application to the SDSS
• Using the Milky Way satellites to study interactions between cold dark matter and radiation
• The abundance of voids and the excursion set formalism
• Gaussian covariance matrices for anisotropic galaxy clustering measurements
• Recoiling Black Holes in Merging Galaxies: Relationship to AGN Lifetimes, Starbursts, and the M-sigma Relation
• N-body simulations of gravitational dynamics
• MAGIC Gamma-ray Telescope Observation of the Perseus Cluster of Galaxies: implications for cosmic rays, dark matter, and NGC1275
• How supernova explosions power galactic winds
• First Identification of 10-kpc Scale [CII] 158um Halos around Star-Forming Galaxies at z=5-7
• The distribution of neutral hydrogen around high-redshift galaxies and quasars in the EAGLE simulation
• Radial metallicity profiles for a large sample of galaxy clusters observed with XMM-Newton
• Revealing reionization with the thermal history of the intergalactic medium: new constraints from the Lyman-$\alpha$ flux power spectrum
• The ASTRID simulation: the evolution of Supermassive Black Holes
• One simulation to fit them all - changing the background parameters of a cosmological N-body simulation
• The AGORA High-Resolution Galaxy Simulations Comparison Project. II: Isolated Disk Test
• How to Zoom: Bias, Contamination, and Lagrange Volumes in Multimass Cosmological Simulations
• Multiple Impact Origin for the Moon
• Response of the Milky Way's disc to the Large Magellanic Cloud in a first infall scenario
• Neutrino mass in cosmology: status and prospects
• Lyman-$\alpha$ forest and non-linear structure characterization in Fuzzy Dark Matter cosmologies
• The origin of scatter in the stellar mass - halo mass relation of central galaxies in the EAGLE simulation
• ELUCID - Exploring the Local Universe with reConstructed Initial Density field III: Constrained Simulation in the SDSS Volume
• Tidal Tails Test the Equivalence Principle in the Dark Sector
• The impact of baryons on the spins and shapes of dark matter haloes
• The E-MOSAICS project: tracing galaxy formation and assembly with the age-metallicity distribution of globular clusters
• Interacting galaxies on FIRE-2: The connection between enhanced star formation and interstellar gas content
• Toward Unbiased Galaxy Cluster Masses from Line of Sight Velocity Dispersions
• Large fluctuations in the hydrogen-ionizing background and mean free path following the epoch of reionization
• KiDS-450: Cosmological Constraints from Weak Lensing Peak Statistics - II: Inference from Shear Peaks using N-body Simulations
• A 2-3 billion year old major merger paradigm for the Andromeda galaxy and its outskirts
• Simulating cosmic rays in clusters of galaxies - I. Effects on the Sunyaev-Zel'dovich effect and the X-ray emission
• Cosmology with massive neutrinos III: the halo mass function and an application to galaxy clusters
• The Aemulus Project I: Numerical Simulations for Precision Cosmology
• The effect of peculiar velocities on supernova cosmology
• The Universe at z>10: Predictions for JWST from the UniverseMachine DR1
• Do dwarf galaxies form in tidal tails?
• Non-linear Evolution of Baryon Acoustic Oscillations from Improved Perturbation Theory in Real and Redshift Spaces
• SPHS: Smoothed Particle Hydrodynamics with a higher order dissipation switch
• SPHGal: Smoothed Particle Hydrodynamics with improved accuracy for Galaxy simulations
• The COpernicus COmplexio: Statistical Properties of Warm Dark Matter Haloes
• Synthetic Galaxy Images and Spectra from the Illustris Simulation
• Debris from terrestrial planet formation: the Moon-forming collision
• Connecting the first galaxies with ultra faint dwarfs in the Local Group: chemical signatures of Population~III stars
• Stellar haloes of simulated Milky Way-like galaxies: Chemical and kinematic properties
• Minimally Parametric Power Spectrum Reconstruction from the Lyman-alpha Forest
• The alignment and shape of dark matter, stellar, and hot gas distributions in the EAGLE and cosmo-OWLS simulations
• Is AGN feedback necessary to form red elliptical galaxies?
• The Cosmic Web: Geometric Analysis
• A Theory for the Excitation of CO in Star Forming Galaxies
• Organized Chaos: Scatter in the relation between stellar mass and halo mass in small galaxies
• Multimessenger astronomy with pulsar timing and X-ray observations of massive black hole binaries
• A sharper view of Pal 5's tails: Discovery of stream perturbations with a novel non-parametric technique
• Galaxy metallicity scaling relations in the EAGLE simulations
• Through Thick and Thin - HI Absorption in Cosmological Simulations
• Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies
• An algorithm for the direct reconstruction of the dark matter correlation function from weak lensing and galaxy clustering
• Public data release of the FIRE-2 cosmological zoom-in simulations of galaxy formation
• The total infrared luminosity may significantly overestimate the star formation rate of recently quenched galaxies
• Dwarf Galaxies and the Cosmic Web
• Metal Cooling in Simulations of Cosmic Structure Formation
• 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
• The intergalactic medium over the last 10 billion years I: Lyman alpha absorption and physical conditions
• Voids in massive neutrino cosmologies
• Probing Cosmology with Weak Lensing Peak Counts
• The Ubiquity of Coeval Starbursts in Massive Galaxy Cluster Progenitors
• Combining perturbation theories with halo models
• Nonlinear structure formation in the Cubic Galileon gravity model
• Gravitational Heating Helps Make Massive Galaxies Red and Dead
• An accurate tool for the fast generation of dark matter halo catalogs
• Constraining $M_{\nu }$ with the Bispectrum I: Breaking Parameter Degeneracies
• Moving mesh cosmology: characteristics of galaxies and haloes
• Imprints of dark energy on cosmic structure formation: II) Non-Universality of the halo mass function
• High-precision predictions for the acoustic scale in the non-linear regime
• Simulating high-redshift galaxies
• The Effective Field Theory of Large Scale Structure at Two Loops: the apparent scale dependence of the speed of sound
• Simulations of supermassive black hole growth in high-redshift disk galaxies
• A non-ideal MHD Gadget: Simulating massive galaxy clusters
• Origin and properties of dual and offset active galactic nuclei in a cosmological simulation at z=2
• Planet formation signposts: observability of circumplanetary disks via gas kinematics
• Galaxy Simulation with Dust Formation and Destruction
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological implications of the Fourier space wedges of the final sample
• The Brightest Galaxies in the Dark Ages: Galaxies' Dust Continuum Emission During the Reionization Era
• The Concentration Dependence of the Galaxy-Halo Connection: Modeling Assembly Bias with Abundance Matching
• Virialization of the inner CGM in the FIRE simulations and implications for galaxy discs, star formation and feedback
• The nature of the Diffuse Gamma-Ray Background
• How long does it take to form a molecular cloud?
• Feedback from Active Galactic Nuclei in Galaxy Groups
• On the origin of cold dark matter halo density profiles
• Observable tests of self-interacting dark matter in galaxy clusters: cosmological simulations with SIDM and baryons
• Lyman-alpha Emission From Cosmic Structure I: Fluorescence
• The accretion history of dark matter halos I: The physical origin of the universal function
• On the Origin of Cores in Simulated Galaxy Clusters
• Variable accretion and emission from the stellar winds in the Galactic centre
• "Non-cold" dark matter at small scales: a general approach
• Star formation in metal-poor gas clouds
• A population of luminous accreting black holes with hidden mergers
• Cosmic Degeneracies I: Joint N-body Simulations of Modified Gravity and Massive Neutrinos
• The origin of the diverse morphologies and kinematics of Milky Way-mass galaxies in the FIRE-2 simulations
• The preferred direction of infalling satellite galaxies in the Local Group
• Weak-lensing mass calibration of redMaPPer galaxy clusters in Dark Energy Survey Science Verification data
• Lyman-$\alpha$ forest constraints on Primordial Black Holes as Dark Matter
• GAMER: a GPU-Accelerated Adaptive Mesh Refinement Code for Astrophysics
• Collisional Stripping and Disruption of Super-Earths
• Supersonic Gas Streams Enhance the Formation of Massive Black Holes in the Early Universe
• Mergers and Mass Accretion for Infalling Halos Both End Well Outside Cluster Virial Radii
• Phat ELVIS: The inevitable effect of the Milky Way's disk on its dark matter subhaloes
• Red & Dead CANDELS: massive passive galaxies at the dawn of the Universe
• The Nature and Origin of Low-Redshift O VI Absorbers
• Assembly bias and the dynamical structure of dark matter halos
• It's not easy being green: The evolution of galaxy colour in the EAGLE simulation
• Smoothly-Rising Star Formation Histories During the Reionization Epoch
• Antitruncated Stellar Disks via Minor Mergers
• Dark Matter Direct Detection Signals inferred from a Cosmological N-body Simulation with Baryons
• Linear perturbation theory for tidal streams and the small-scale CDM power spectrum
• Variable interstellar radiation fields in simulated dwarf galaxies: supernovae versus photoelectric heating
• Specific Angular Momentum of Disc Merger Remnants and the ${\lambda }_R$-Parameter
• Galaxy Cold Gas Contents in Modern Cosmological Hydrodynamic Simulations
• Constraint on neutrino masses from SDSS-III/BOSS Ly$\alpha$ forest and other cosmological probes
• The Quantity of Intracluster Light: Comparing Theoretical and Observational Measurement Techniques Using Simulated Clusters
• A profile in FIRE: resolving the radial distributions of satellite galaxies in the Local Group with simulations
• The intergalactic medium over the last 10 billion years II: Metal-line absorption and physical conditions
• The three dimensional skeleton: tracing the filamentary structure of the universe
• The $\text{Abacus}$ Cosmological $N$-body Code
• How rapidly do supermassive black hole "seeds" grow at early times?
• Non-Gaussian information from weak lensing data via deep learning
• The Nuclear Stellar Disk in Andromeda: A Fossil from the Era of Black Hole Growth
• The Aemulus Project II: Emulating the Halo Mass Function
• Redshift space distortions in f(R) gravity
• Connecting CO Intensity Mapping to Molecular Gas and Star Formation in the Epoch of Galaxy Assembly
• Enhanced Dense Gas Fraction in Ultra-Luminous Infrared Galaxies
• The Cosmic Code Comparison Project
• Probing the thermal state of the intergalactic medium at $z>5$ with the transmission spikes in high-resolution Ly$\alpha$ forest spectra
• Redshift-Space Clustering of SDSS Galaxies --- Luminosity Dependence, Halo Occupation Distribution, and Velocity Bias
• Far-infrared and dust properties of present-day galaxies in the EAGLE simulations
• The Hierarchical Structure and Dynamics of Voids
• Separate Universe Simulations
• Gas Clumping in Self-Consistent Reionisation Models
• The ASTRID Simulation: Galaxy Formation and Reionization
• Formation of cold filaments in cooling flow clusters
• Resolving Subhaloes' Lives with the Hierarchical Bound-Tracing Algorithm
• Modeling Nonlinear Evolution of Baryon Acoustic Oscillations: Convergence Regime of N-body Simulations and Analytic Models
• K+A Galaxies as the Aftermath of Gas-Rich Mergers: Simulating the Evolution of Galaxies as Seen by Spectroscopic Surveys
• Supermassive black holes in the EAGLE Universe. Revealing the observables of their growth
• Giant clumps in the FIRE simulations: a case study of a massive high-redshift galaxy
• The environment of bright QSOs at z ~ 6: Star forming galaxies and X-ray emission
• MassiveNuS: Cosmological Massive Neutrino Simulations
• Stellar GADGET: A smooth particle hydrodynamics code for stellar astrophysics and its application to Type Ia supernovae from white dwarf mergers
• The Hestia project: simulations of the Local Group
• Growing massive black holes through super-critical accretion of stellar-mass seeds
• A new way of setting the phases for cosmological multi-scale Gaussian initial conditions
• The first generation of stars in LCDM cosmology
• Hot X-ray coronae around massive spiral galaxies: a unique probe of structure formation models
• Shaken and Stirred: The Milky Way's Dark Substructures
• Baryon-induced dark matter cores in the EAGLE simulations
• Age velocity dispersion relations and heating histories in disc galaxies
• The Co-Evolution of Total Density Profiles and Central Dark Matter Fractions in Simulated Early-Type Galaxies
• Modeling the cosmological co-evolution of supermassive black holes and galaxies: I. BH scaling relations and the AGN luminosity function
• The interplay between chemical and mechanical feedback from the first generation of stars
• Lyman-alpha emitters gone missing: evidence for late reionization?
• Likelihood-free inference with neural compression of DES SV weak lensing map statistics
• Damped Lyman-alpha absorbers as a probe of stellar feedback
• Mismatch and Misalignment: Dark Haloes and Satellites of Disc Galaxies
• Simulations of Baryon Acoustic Oscillations II: Covariance matrix of the matter power spectrum
• Molecular Star Formation Rate Indicators in Galaxies
• Proper Motions, Orbits, and Tidal Influences of Milky Way Dwarf Spheroidal Galaxies
• Synthetic Gaia surveys from the FIRE cosmological simulations of Milky Way-mass galaxies
• Astraeus I: The interplay between galaxy formation and reionization
• The Growth of Massive Black Holes in Galaxy Merger Simulations with Feedback by Radiation Pressure
• Probing Cosmology with Weak Lensing Minkowski Functionals
• Halo assembly bias and the tidal anisotropy of the local halo environment
• How to distinguish starbursts and quiescently star-forming galaxies: The `bimodal' submillimetre galaxy population as a case study
• The vast thin plane of M31 co-rotating dwarfs: an additional fossil signature of the M31 merger and of its considerable impact in the whole Local Group
• Pushing back the limits: detailed properties of dwarf galaxies in a LCDM universe
• Second-order Lagrangian perturbation theory initial conditions for resimulations
• Joint constraints on thermal relic dark matter from strong gravitational lensing, the Lyman-$\alpha$ forest, and Milky Way satellites
• Probing Reionization with the 21 cm-Galaxy Cross Power Spectrum
• The effect of radial migration on galactic disks
• Is molecular gas necessary for star formation?
• Orbital structure of merger remnants: Trends with gas fraction in 1:1 mergers
• The First Galaxies: Assembly with Black Hole Feedback
• Sussing Merger Trees: The Merger Trees Comparison Project
• Modelling redshift space distortions in hierarchical cosmologies
• Forming disk galaxies in wet major mergers. I. Three fiducial examples
• Improved measurements of the intergalactic medium temperature around quasars: possible evidence for the initial stages of He-II reionisation at z~6
• Density split statistics: Cosmological constraints from counts and lensing in cells in DES Y1 and SDSS data
• The redshift evolution of escape fraction of hydrogen ionizing photons from galaxies
• Galaxy-Scale Outflows Driven by Active Galactic Nuclei
• Tracing kinematic (mis)alignments in CALIFA merging galaxies: Stellar and ionized gas kinematic orientations at every merger stage
• Should we believe the results of UV-mm galaxy SED modelling?
• The Topology of the Cosmic Web in Terms of Persistent Betti Numbers
• GreeM : Massively Parallel TreePM Code for Large Cosmological N-body Simulations
• Time dependent couplings in the dark sector: from background evolution to nonlinear structure formation
• The Caterpillar Project: A Large Suite of Milky Way Sized Halos
• The 6dF Galaxy Velocity Survey: Cosmological constraints from the velocity power spectrum
• The impact of type Ia supernovae on main sequence binary companions
• The Evolution in the Faint-End Slope of the Quasar Luminosity Function
• Moving Mesh Cosmology: Properties of Gas Disks
• Investigating the velocity structure and X-ray observable properties of simulated galaxy clusters with PHOX
• The influence of the environmental history on quenching star formation in a $\Lambda$CDM universe
• Alignments of galaxies within cosmic filaments from SDSS DR7
• The redshift evolution of massive galaxy clusters in the MACSIS simulations
• The origin of scatter in the star formation rate - stellar mass relation
• The Dependence of the Mass Assembly History of Cold Dark Matter Halos on Environment
• Low-mass halo perturbations in strong gravitational lenses at redshift z$\sim$0.5 are consistent with CDM
• The impact of assembly bias on the halo occupation in hydrodynamical simulations
• Simulations of the formation of stellar discs in the Galactic centre via cloud-cloud collisions
• The detailed structure and the onset of galaxy formation in low-mass gaseous dark matter haloes
• Structure and evolution of high-mass stellar mergers
• Are the ultra-high-redshift galaxies at z > 10 surprising in the context of standard galaxy formation models?
• The Mass-Discrepancy Acceleration Relation: a Natural Outcome of Galaxy Formation in Cold Dark Matter halos
• A giant impact as the likely origin of different twins in the Kepler-107 exoplanet system
• The splashback radius of halos from particle dynamics. II. Dependence on mass, accretion rate, redshift, and cosmology
• Simulating nonlinear cosmological structure formation with massive neutrinos
• Cosmic Voids and Void Lensing in the Dark Energy Survey Science Verification Data
• The Properties of Cosmic Velocity Fields
• Characterizing Diffused Stellar Light in simulated galaxy clusters
• Can Gas prevent the Destruction of Thin Stellar Discs by Minor Mergers?
• The fine-grained phase-space structure of Cold Dark Matter halos
• Simulating the gamma-ray emission from galaxy clusters: a universal cosmic ray spectrum and spatial distribution
• Scattering, Damping, and Acoustic Oscillations: Simulating the Structure of Dark Matter Halos with Relativistic Force Carriers
• The Dependence of Galaxy Formation on Cosmological Parameters: Can we distinguish the WMAP1 and WMAP3 Parameter Sets?
• On the Survival of Cool Clouds in the Circum-Galactic Medium
• The Effects of Accretion Luminosity upon Fragmentation in the Early Universe
• The MUSIC of Galaxy Clusters I: Baryon properties and Scaling Relations of the thermal Sunyaev-Zel'dovich Effect
• Hydrogen and Metal Line Absorption Around Low-Redshift Galaxies in Cosmological Hydrodynamic Simulations
• Simulating the physical properties of dark matter and gas inside the cosmic web
• TRAPHIC - Radiative Transfer for Smoothed Particle Hydrodynamics Simulations
• Forensics of Subhalo-Stream Encounters: The Three Phases of Gap Growth
• Grid Based Linear Neutrino Perturbations in Cosmological N-body Simulations
• Modeling baryonic physics in future weak lensing surveys
• Quasar Proximity Zones and Patchy Reionization
• The XXL Survey. XIII. Baryon content of the bright cluster sample
• Limit on the LMC mass from a census of its satellites
• Mergers, Starbursts, and Quenching in the Simba Simulation
• The Origins of AGN Obscuration: The 'Torus' as a Dynamical, Unstable Driver of Accretion
• Simulations of cosmic ray feedback by AGN in galaxy clusters
• On the formation of dwarf galaxies and stellar halos
• Three-dimensional simulations of the interaction between Type Ia supernova ejecta and their main sequence companions
• Transition of the initial mass function in the metal-poor environments
• Formation of Intermediate-Mass Black Holes through Runaway Collisions in the First Star Clusters
• Zooming in on accretion - I. The structure of halo gas
• Effects of Dark Matter Substructures on Gravitational Lensing: Results from the Aquarius Simulations
• The Fate of Substructures in Cold Dark Matter Haloes
• AGN jet feedback on a moving mesh: cocoon inflation, gas flows and turbulence
• Constraining $M_{\nu }$ with the Bispectrum II: The Total Information Content of the Galaxy Bispectrum
• Cluster Density Profiles as a Test of Modified Gravity
• ACCESS - V. Dissecting ram-pressure stripping through integral-field spectroscopy and multi-band imaging
• The structure of terrestrial bodies: Impact heating, corotation limits and synestias
• Black Hole-Galaxy Correlations without Self-Regulation
• Satellite Dwarf Galaxies in a Hierarchical Universe: The Prevalence of Dwarf-Dwarf Major Mergers
• MApping the Most Massive Overdensities (MAMMOTH) II -- Discovery of an Extremely Massive Overdensity BOSS1441 at $z=2.32$
• The drop in the cosmic star formation rate below redshift 2 is caused by a change in the mode of gas accretion and by AGN feedback
• z~2-9 Galaxies Magnified by the Hubble Frontier Field Clusters II: Luminosity Functions and Constraints on a Faint-End Turnover
• Early and Extended Helium Reionization Over More Than 600 Million Years of Cosmic Time
• Hot gas in massive halos drives both mass quenching and environment quenching
• The First Billion Years project: birthplaces of direct collapse black holes
• Galaxy formation in the Planck Millennium: the atomic hydrogen content of dark matter halos
• The Diversity and Variability of Star Formation Histories in Models of Galaxy Evolution
• The effects of baryons on the halo mass function
• CosmoGAN: creating high-fidelity weak lensing convergence maps using Generative Adversarial Networks
• The universal distribution of halo interlopers in projected phase space. Bias in galaxy cluster concentration and velocity anisotropy?
• The link between the assembly of the inner dark matter halo and the angular momentum evolution of galaxies in the EAGLE simulation
• FIREbox: Simulating galaxies at high dynamic range in a cosmological volume
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions
• Tidal stripping and the structure of dwarf galaxies in the Local Group
• Where are the Fossils of the First Galaxies? II. True Fossils, Ghost Halos, and the Missing Bright Satellites
• A Bayesian approach to the semi-analytic model of galaxy formation: methodology
• Bullet Cluster: A Challenge to LCDM Cosmology
• Direct collapse black hole formation from synchronized pairs of atomic cooling halos
• Barred galaxies in the EAGLE cosmological hydrodynamical simulation
• Supernova-driven winds in simulated dwarf galaxies
• The GRIFFIN project -- Formation of star clusters with individual massive stars in a simulated dwarf galaxy starburst
• Constraining Dark Matter -- Dark Radiation interactions with CMB, BAO, and Lyman-$\alpha$
• The photoheating of the intergalactic medium in synthesis models of the UV background
• Cosmological hydrodynamical simulations of galaxy clusters: X-ray scaling relations and their evolution
• Anisotropic Diffusion in Mesh-Free Numerical Magnetohydrodynamics
• Simulations of the Milky Way's central molecular zone -- I. Gas dynamics
• A Testable Conspiracy: Simulating Baryonic Effects on Self-Interacting Dark Matter Halos
• The baryon fraction in hydrodynamical simulations of galaxy clusters
• The Dependence of Subhalo Abundance on Halo Concentration
• Asymmetries in the inner regions of LCDM haloes
• The Formation of the Collisional Family around the Dwarf Planet Haumea
• A Constrained-Gradient Method to Control Divergence Errors in Numerical MHD
• The cosmic growth of the active black hole population at 1<z<2 in zCOSMOS, VVDS and SDSS
• Emulating the CFHTLenS Weak Lensing data: Cosmological Constraints from moments and Minkowski functionals
• Streams and caustics: the fine-grained structure of LCDM haloes
• The IRX-Beta Dust Attenuation Relation in Cosmological Galaxy Formation Simulations
• The Eating Habits of Milky Way Mass Halos: Destroyed Dwarf Satellites and the Metallicity Distribution of Accreted Stars
• The Impact of Inhomogeneous Reionization on the Satellite Galaxy Population of the Milky Way
• Does M31 result from an ancient major merger?
• The Physical and Photometric Properties of High-Redshift Galaxies in Cosmological Hydrodynamic Simulations
• Simulations of Early Baryonic Structure Formation with Stream Velocity: II. The Gas Fraction
• Recovering Stellar Population Properties and Redshifts from Broad-Band Photometry of Simulated Galaxies: Lessons for SED Modeling
• Probability Distribution Functions of Cosmological Lensing: Convergence, Shear, and Magnification
• The emptiness of voids: yet another over-abundance problem for the LCDM model
• Signature of primordial non-Gaussianity of phi^3-type in the mass function and bias of dark matter haloes
• The accretion history of dark matter halos II: The connections with the mass power spectrum and the density profile
• Diffuse stellar component in galaxy clusters and the evolution of the most massive galaxies at z<~1
• The Hubble sequence: just a vestige of merger events?
• Chemical evolution during gas-rich galaxy interactions
• The ATLAS3D Project-- VIII: Modelling the Formation and Evolution of Fast and Slow Rotator Early-Type Galaxies within $\Lambda$CDM
• A Population of Compact Elliptical Galaxies Detected with the Virtual Observatory
• The Preferential Tidal Stripping of Dark Matter versus Stars in Galaxies
• Metal Enrichment of the ICM: a 3-D Picture of Chemical and Dynamical Properties
• The cosmic history of the spin of dark matter haloes within the large scale structure
• The effect of baryons on redshift space distortions and cosmic density and velocity fields in the EAGLE simulation
• Optimal Constraints on Local Primordial Non-Gaussianity from the Two-Point Statistics of Large-Scale Structure
• Are peculiar velocity surveys competitive as a cosmological probe?
• On the Cluster Physics of Sunyaev-Zel'dovich and X-ray Surveys III: Measurement Biases and Cosmological Evolution of Gas and Stellar Mass Fractions
• The thermal history of the intergalactic medium down to redshift z=1.5: a new curvature measurement
• Radiative Feedback from high mass X-ray binaries on the formation of the first galaxies and early reionization
• On the radiative efficiencies, Eddington ratios, and duty cycles of luminous high-redshift quasars
• The Cosmic Ballet II: Spin alignment of galaxies and haloes with large-scale filaments in the EAGLE simulation
• On the rapid demise of Lyman-alpha emitters at z>7 due to the increasing incidence of optically thick absorption systems
• Fast Large-Scale Reionization Simulations
• The stellar-to-halo mass relation of GAMA galaxies from 100 square degrees of KiDS weak lensing data
• Warps and waves in the stellar discs of the Auriga cosmological simulations
• The Collision Between The Milky Way And Andromeda
• The stellar-to-halo mass relation for Local Group galaxies
• Cosmic distribution of highly ionized metals and their physical conditions in the EAGLE simulations
• Velocity correction for Hubble constant measurements from standard sirens
• The impact of local stellar radiation on the HI column density distribution
• Cosmological Structure Formation with Augmented Lagrangian Perturbation Theory
• The origin of diverse $\alpha$-element abundances in galaxy discs
• The Role of Black Hole Feedback on Size and Structural Evolution in Massive Galaxies
• The assembly of dusty galaxies at $z\ge 4$: statistical properties
• SWIFT: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications
• The effect of AGN feedback on the halo mass function
• Predictions for the relation between strong HI absorbers and galaxies at redshift 3
• Cosmic Shear Measurements with DES Science Verification Data
• The impact of primordial supersonic flows on early structure formation, reionization and the lowest-mass dwarf galaxies
• Decaying dark matter and the tension in ${\sigma }_8$
• LCDM predictions for galaxy protoclusters I: the relation between galaxies, protoclusters and quasars at z~6
• Numerical Convergence in Smoothed Particle Hydrodynamics
• Double-peaked Narrow-Line Signatures of Dual Supermassive Black Holes in Galaxy Merger Simulations
• Simulated X-ray galaxy clusters at the virial radius: slopes of the gas density, temperature and surface brightness profiles
• Phenotypic redshifts with self-organizing maps: A novel method to characterize redshift distributions of source galaxies for weak lensing
• X-ray mass proxies from hydrodynamic simulations of galaxy clusters (paper I)
• Properties of Dark Subhaloes from Gaps in Tidal Streams
• The Photon Underproduction Crisis
• The Copernicus Complexio: a high-resolution view of the small-scale Universe
• X-ray Emission from Hot Gas in Galaxy Mergers
• Bulges versus disks: the evolution of angular momentum in cosmological simulations of galaxy formation
• Cosmological simulation with dust formation and destruction
• The link between galaxy and black hole growth in the EAGLE simulation
• Observable tests of self-interacting dark matter in galaxy clusters: BCG wobbles in a constant density core
• How is Star Formation Quenched in Massive Galaxies?
• The Outer Rim Simulation: A Path to Many-Core Supercomputers
• A consistent and robust measurement of the thermal state of the IGM at $2\le z\le 4$ from a large sample of Ly$\alpha$ forest spectra: Evidence for late and rapid HeII reionization
• SNSPH: A Parallel 3-D Smoothed Particle Radiation Hydrodynamics Code
• Diffuse radio emission from clusters in the MareNostrum Universe simulation
• Dissipation and the Fundamental Plane: Observational Tests
• Is atomic carbon a good tracer of molecular gas in metal-poor galaxies?
• A re-interpretation of the Triangulum-Andromeda stellar clouds: a population of halo stars kicked out of the Galactic disk
• Formation and survival of Population III stellar systems
• The UDF05 Follow-up of the HUDF: I. The Faint-End Slope of the Lyman-Break Galaxy Population at z~5
• Constraining chameleon models with cosmology
• Simulated Milky Way analogues: implications for dark matter direct searches
• The environmental dependence of HI in galaxies in the EAGLE simulations
• A High-Fidelity Realization of the Euclid Code Comparison $N$-body Simulation with Abacus
• The fundamental plane of star formation in galaxies revealed by the EAGLE hydrodynamical simulations
• The Hierarchical Nature of the Spin Alignment of Dark Matter Haloes in Filaments
• Pressure of the hot gas in simulations of galaxy clusters
• ZOMG-I. How the cosmic web inhibits halo growth and generates assembly bias
• The Dependence of the Occupation of Galaxies on the Halo Formation Time
• A Comparison of Cosmological Codes: Properties of Thermal Gas and Shock Waves in Large Scale Structures
• ICE-COLA: Towards fast and accurate synthetic galaxy catalogues optimizing a quasi $N$-body method
• An uncertainty principle for star formation - II. A new method for characterising the cloud-scale physics of star formation and feedback across cosmic history
• Self-Regulated Black Hole Growth via Momentum Deposition in Galaxy Merger Simulations
• The simulated 21 cm signal during the epoch of reionization : full modeling of the Ly-alpha pumping
• Building disc structure and galaxy properties through angular momentum: The DARK SAGE semi-analytic model
• An iterative method for the construction of N-body galaxy models in collisionless equilibrium
• Lighting the Universe with filaments
• Tracing the Reionization-Epoch Intergalactic Medium with Metal Absorption Lines
• The effect of baryons on the inner density profiles of rich clusters
• The ARTEMIS simulations: stellar haloes of Milky Way-mass galaxies
• SIGAME simulations of the [CII], [OI] and [OIII] line emission from star forming galaxies at z ~ 6
• Understanding the Structural Scaling Relations of Early-Type Galaxies
• Spin alignments of spiral galaxies within the large-scale structure from SDSS DR7
• Galilean Equivalence for Galactic Dark Matter
• A new approach to simulating collisionless dark matter fluids
• Metal-Free Gas Supply at the Edge of Reionization: Late-Epoch Population III Star Formation
• A survey of dual active galactic nuclei in simulations of galaxy mergers: frequency and properties
• The gas fractions of dark matter haloes hosting simulated $\sim L^{\star }$ galaxies are governed by the feedback history of their black holes
• Accurate initial conditions for cosmological N-body simulations: Minimizing truncation and discreteness errors
• Galaxy mergers on a moving mesh: a comparison with smoothed-particle hydrodynamics
• Cosmic shear covariance: The log-normal approximation
• Feeding SMBHs through supersonic turbulence and ballistic accretion
• Weak Lensing by Galaxies in Groups and Clusters: I.--Theoretical Expectations
• The mass-Peak Patch algorithm for fast generation of deep all-sky dark matter halo catalogues and its N-Body validation
• Hunting for Galaxies and Halos in simulations with VELOCIraptor
• Quiescence correlates strongly with directly-measured black hole mass in central galaxies
• The assembly bias of dark matter haloes to higher orders
• Shape, spin and baryon fraction of clusters in the MareNostrum Universe
• The impact of baryonic processes on the two-point correlation functions of galaxies, subhaloes and matter
• On the identification of merger debris in the {\it Gaia} Era
• Orion's Bar: Physical Conditions across the Definitive H+ / H0 / H2 Interface
• The Chemo-Dynamical Groups of Galactic Globular Clusters
• GRB 100219A with X-shooter - abundances in a galaxy at z = 4.7
• An improved fitting formula for the dark matter bispectrum
• Gaps in globular cluster streams: giant molecular clouds can cause them too
• A consistent determination of the temperature of the intergalactic medium at redshift z=2.4
• Efficient early stellar feedback can suppress galactic outflows by reducing supernova clustering
• Neutrinos in Non-linear Structure Formation - The Effect on Halo Properties
• The relation between galaxy morphology and colour in the EAGLE simulation
• The universal nature of subhalo accretion
• CRKSPH - A Conservative Reproducing Kernel Smoothed Particle Hydrodynamics Scheme
• Effects of Massive Neutrinos on the Large-Scale Structure of the Universe
• The evolution of Black Hole scaling relations in galaxy mergers
• Generating Merger Trees for Dark Matter Haloes: A Comparison of Methods
• Mass transfer in white dwarf-neutron star binaries
• Energy equipartition between stellar and dark matter particles in cosmological simulations results in spurious growth of galaxy sizes
• The Nature of Sub-millimetre Galaxies in Cosmological Hydrodynamic Simulations
• The Angular Momentum Problem in Cosmological Simulations of Disk Galaxy Formation
• The imprint of neutrinos on clustering in redshift-space
• Galaxies in the EAGLE hydrodynamical simulation and in the Durham and Munich semi-analytical models
• When did Population III star formation end?
• The Source Density and Observability of Pair-Instability Supernovae from the First Stars
• Modelling the large scale structure of the Universe as a function of cosmology and baryonic physics
• Simulations of the star-forming molecular gas in an interacting M51-like galaxy
• Density split statistics: joint model of counts and lensing in cells
• Flickering AGN can explain the strong circumgalactic O VI observed by COS-Halos
• Cosmic Shear Results from the Deep Lens Survey - II: Full Cosmological Parameter Constraints from Tomography
• The splashback radius of halos from particle dynamics. I. The SPARTA algorithm
• Faint dwarfs as a test of DM models: WDM vs. CDM
• New Interpretable Statistics for Large Scale Structure Analysis and Generation
• Cosmological Simulations of Early Blackhole Formation: Halo Mergers, Tidal Disruption, and the Conditions for Direct Collapse
• Adventures of a tidally induced bar
• Dark Energy Survey Year 1 Results: Curved-Sky Weak Lensing Mass Map
• Accretion, feedback and galaxy bimodality: a comparison of the GalICS semi-analytic model and cosmological SPH simulations
• Trident: a universal tool for generating synthetic absorption spectra from astrophysical simulations
• Determining the stellar masses of submillimetre galaxies: the critical importance of star formation histories
• The Three Hundred Project: Backsplash galaxies in simulations of clusters
• Satellite Systems around Galaxies in Hydrodynamic Simulations
• Stellar diffusion in barred spiral galaxies
• The Dark Halo - Spheroid Conspiracy and the Origin of Elliptical Galaxies
• Constraints on the mass-richness relation from the abundance and weak lensing of SDSS clusters
• Numerical convergence of simulations of galaxy formation: the abundance and internal structure of cold dark matter haloes
• Hydrodynamical adaptive mesh refinement simulations of turbulent flows - II. Cosmological simulations of galaxy clusters
• The history of chemical enrichment in the intracluster medium from cosmological simulations
• Simulation techniques for cosmological simulations
• Initial Conditions for Accurate N-Body Simulations of Massive Neutrino Cosmologies
• Modelling [CI] emission from turbulent molecular clouds
• Some like it triaxial: the universality of dark matter halo shapes and their evolution along the cosmic time
• Numerical Simulations of Turbulent, Molecular Clouds Regulated by Radiation Feedback Forces I: Star Formation Rate and Efficiency
• Fast cosmic web simulations with generative adversarial networks
• On the intergalactic temperature-density relation
• An Extended Halo-based Group/Cluster finder: application to the DESI legacy imaging surveys DR8
• The Star-Forming Molecular Gas in High Redshift Submillimeter Galaxies
• A limit on eccentricity growth from global 3-D simulations of disc-planet interactions
• Cosmological and astrophysical constraints from the Lyman-alpha forest flux probability distribution function
• Simulations of Early Baryonic Structure Formation with Stream Velocity: I. Halo Abundance
• The Accuracy of Subhalo Detection
• The Role of Galactic Winds on Molecular Gas Emission from Galaxy Mergers
• Strong lensing in the MareNostrum Universe: biases in the cluster lens population
• The statistics of the subhalo abundance of dark matter haloes
• Cubic Halo Bias in Eulerian and Lagrangian Space
• Kinematics of Simulated Galaxies I: Connecting Dynamical and Morphological Properties of Early-Type Galaxies at Different Redshifts
• 2MTF VI. Measuring the velocity power spectrum
• Neural Networks for Full Phase-space Reweighting and Parameter Tuning
• The thermal Sunyaev Zel'dovich effect power spectrum in light of Planck
• Dark Energy Survey Year 3 results: curved-sky weak lensing mass map reconstruction
• The multiphase circumgalactic medium traced by low metal ions in EAGLE zoom simulations
• The effect of a massive object on an expanding universe
• The Growth of Red Sequence Galaxies in a Cosmological Hydrodynamic Simulation
• The phase space density of fermionic dark matter haloes
• Reionization by UV or X-ray sources
• How to constrain warm dark matter with the Lyman $\alpha$ forest
• Has JWST already falsified dark-matter-driven galaxy formation?
• Non-Gaussian statistics of critical sets in 2 and 3D: Peaks, voids, saddles, genus and skeleton
• Non-thermal processes in cosmological simulations
• Constrained simulations of the Local Group: on the radial distribution of substructures
• The Novel Probes Project -- Tests of Gravity on Astrophysical Scales
• No cores in dark matter-dominated dwarf galaxies with bursty star formation histories
• Orbit-based dynamical models of the Sculptor dSph galaxy
• SEREN - A new SPH code for star and planet formation simulations
• Novel constraints on non-cold (non-thermal) Dark Matter from Lyman-$\alpha$ forest data
• Review on Smoothed Particle Hydrodynamics: Methodology development and recent achievement
• Alignment between galaxies and large-scale structure
• SCORCH I: The Galaxy-Halo Connection in the First Billion Years
• The Structure of Halos: Implications for Group and Cluster Cosmology
• Perturbation Theory Reloaded II: Non-linear Bias, Baryon Acoustic Oscillations and Millennium Simulation In Real Space
• Characterizing the Pressure Smoothing Scale of the Intergalactic Medium
• A fully cosmological model of a Monoceros-like ring
• COSMOS2020: The cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z~5
• The core-cusp problem: a matter of perspective
• Low-Redshift Lyman Limit Systems as Diagnostics of Cosmological Inflows and Outflows
• The low-mass end of the baryonic Tully-Fisher relation
• Modeling the angular correlation function and its full covariance in Photometric Galaxy Surveys
• Low Surface Brightness Imaging of the Magellanic System: Imprints of Tidal Interactions between the Clouds in the Stellar Periphery
• The Stacked Thermal SZ Signal of Locally Brightest Galaxies in Planck Full Mission Data: Evidence for Galaxy Feedback?
• The Fundamentally Different Dynamics of Dust and Gas in Molecular Clouds
• The CoDECS project: a publicly available suite of cosmological N-body simulations for interacting dark energy models
• The Magellanic Stream System: I. Ram-pressure tails and the relics of the collision between the Magellanic Clouds
• The Lyman-alpha forest and WMAP year three
• The Self-Regulated Growth of Supermassive Black Holes
• Supermassive Star Formation via Super Competitive Accretion in Slightly Metal-enriched Clouds
• Splashback Shells of Cold Dark Matter Halos
• Large-scale inhomogeneities of the intracluster medium: improving mass estimates using the observed azimuthal scatter
• A numerical simulation of a "super-Earth" core delivery from ~ 100 AU to ~ 8 AU
• Modeling projection effects in optically-selected cluster catalogues
• The impact of radio feedback from active galactic nuclei in cosmological simulations: Formation of disk galaxies
• A 10 kpc stellar substructure at the edge of the Large Magellanic Cloud: perturbed outer disk or evidence for tidal stripping?
• The Dynamical and Chemical Evolution of Dwarf Spheroidal Galaxies with GEAR
• Boosting the accuracy of SPH techniques: Newtonian and special-relativistic tests
• How do galaxies acquire their mass?
• Nonlinear Structure Formation with the Environmentally Dependent Dilaton
• Interpreting measurements of the anisotropic galaxy power spectrum
• Fast galaxy bars continue to challenge standard cosmology
• GAMER-2: a GPU-accelerated adaptive mesh refinement code -- accuracy, performance, and scalability
• The First Galaxies: Assembly of Disks and Prospects for Direct Detection
• Cosmology in the era of Euclid and the Square Kilometre Array
• Fermi Bubbles in the Milky Way: the closest AGN feedback laboratory courtesy of Sgr A*?
• Interaction between massive planets on inclined orbits and circumstellar discs
• Reconstructing the cosmic density field with the distribution of dark matter halos
• The High-$z$ Universe Confronts Warm Dark Matter: Galaxy Counts, Reionization and the Nature of Dark Matter
• Where are the Fossils of the First Galaxies? I. Local Volume Maps and Properties of the Undetected Dwarfs
• Recovery from population III supernova explosions and the onset of second generation star formation
• The Dragonfly Nearby Galaxies Survey. III. The Luminosity Function of the M101 Group
• UNIT project: Universe $N$-body simulations for the Investigation of Theoretical models from galaxy surveys
• Torque-Limited Growth of Massive Black Holes in Galaxies Across Cosmic Time
• Formation history, structure and dynamics of discs and spheroids in simulated Milky Way mass galaxies
• The impact of Type Ia supernova explosions on helium companions in the Chandrasekhar-mass explosion scenario
• What is the (Dark) Matter with Dwarf Galaxies?
• Reconstructing the Initial Density Field of the Local Universe: Method and Test with Mock Catalogs
• An implementation of radiative transfer in the cosmological simulation code GADGET
• The Physical Properties and Detectability of Reionization-Epoch Galaxies
• On the Assembly of Dwarf Galaxies in Clusters and their Efficient Formation of Globular Clusters
• Formation sites of Population III star formation: The effects of different levels of rotation and turbulence on the fragmentation behavior of primordial gas
• AX-GADGET: a new code for cosmological simulations of Fuzzy Dark Matter and Axion models
• A model for the formation of stellar associations and clusters from giant molecular clouds
• Origin of strong magnetic fields in Milky-Way like galactic haloes
• Spatial Clustering of Dark Matter Halos: Secondary Bias, Neighbor Bias, and the Influence of Massive Neighbors on Halo Properties
• Numerical solution of the non-linear Schrodinger equation using smoothed-particle hydrodynamics
• The effect of dust cooling on low-metallicity star-forming clouds
• The Outer Stellar Halos of Galaxies: how Radial Merger Mass Deposition, Shells and Streams depend on Infall-Orbit Configurations
• The Kinematic Sunyaev-Zel'dovich Effect with Projected Fields II: prospects, challenges, and comparison with simulations
• Coarse-Grained Cosmological Perturbation Theory
• Cosmological Simulations of Decaying Dark Matter: Implications for Small-scale Structure of Dark Matter Halos
• nIFTy galaxy cluster simulations I: dark matter & non-radiative models
• The Life Cycle of the Central Molecular Zone. I: Inflow, Star Formation, and Winds
• High-Redshift Galaxy Kinematics: Constraints on Models of Disk Formation
• The evolution of embedded star clusters
• Resolving the high redshift Lyman-alpha forest in smoothed particle hydrodynamics simulations
• The relationship between the morphology and kinematics of galaxies and its dependence on dark matter halo structure in EAGLE
• The Tau of Galaxy Clusters
• The effects of a hot gaseous halo in galaxy major mergers
• Massive black hole pairs in clumpy, self-gravitating circumnuclear disks: stochastic orbital decay
• An adaptively refined phase-space element method for cosmological simulations and collisionless dynamics
• Orbital parameters of infalling satellite haloes in the hierarchical $\Lambda$CDM model
• On the Impact Origin of Phobos and Deimos I: Thermodynamic and Physical Aspects
• Unified galaxy power spectrum measurements from 6dFGS, BOSS, and eBOSS
• Dark matter-radiation interactions: the impact on dark matter haloes
• Environmental Dependence of Galaxy Merger Rate in ΛCDM Universe
• Comparing approximate methods for mock catalogues and covariance matrices II: Power spectrum multipoles
• Constraints on the identity of the dark matter from strong gravitational lenses
• Water/Icy Super-Earths: Giant Impacts and Maximum Water Content
• Missing dark matter in dwarf galaxies?
• Chemo-Archaeological Downsizing in a Hierarchical Universe: Impact of a Top Heavy IGIMF
• First Simulations of Axion Minicluster Halos
• The Imprint of Reionization on the Star Formation Histories of Dwarf Galaxies
• Reconstruction in Fourier space
• A minor merger origin for stellar inner discs and rings in spiral galaxies
• Sphenix: Smoothed Particle Hydrodynamics for the next generation of galaxy formation simulations
• Feedback reshapes the baryon distribution within haloes, in halo outskirts, and beyond: the closure radius from dwarfs to massive clusters
• Cosmic particle colliders: simulations of self-interacting dark matter with anisotropic scattering
• The Void Size Function in Dynamical Dark Energy Cosmologies
• Testing Sunyaev-Zel'dovich measurements of the hot gas content of dark matter haloes using synthetic skies
• The Effect of Fiber Collisions on the Galaxy Power Spectrum Multipole
• The impact of feedback from galaxy formation on the Lyman-alpha transmitted flux
• Substructure and galaxy formation in the Copernicus Complexio warm dark matter simulations
• On the nature of the barlens component in barred galaxies: what do boxy/peanut bulges look like when viewed face-on?
• The intergalactic medium thermal history at redshift z=1.7--3.2 from the Lyman alpha forest: a comparison of measurements using wavelets and the flux distribution
• nIFTy Cosmology: Galaxy/halo mock catalogue comparison project on clustering statistics
• A massive blow for $\Lambda$CDM $-$ the high redshift, mass, and collision velocity of the interacting galaxy cluster El Gordo contradicts concordance cosmology
• The origins of post-starburst galaxies at z<0.05
• On the Origin of Dwarf Elliptical Galaxies: The Fundamental Plane
• Physical viscosity in smoothed particle hydrodynamics simulations of galaxy clusters
• Large-Scale Clustering of Cosmic Voids
• Tidally induced bars of galaxies in clusters
• Sunyaev-Zel'dovich clusters in Millennium Gas simulations
• Comparing approximate methods for mock catalogues and covariance matrices I: correlation function
• Intrinsic alignments of galaxies in the EAGLE and cosmo-OWLS simulations
• A Lensing Survey of X-ray Luminous Galaxy Clusters at Redshift z ~ 0.2: II: CFH12k Weak Lensing Analysis and Global Correlations
• Linking galaxy structural properties and star formation activity to black hole activity with IllustrisTNG
• On the lifetime of merger features of equal-mass disk mergers
• Precession and accretion in circumbinary discs: The case of HD 104237
• Spatially unassociated galaxies contribute significantly to the blended submillimetre galaxy population: predictions for follow-up observations of ALMA sources
• Temperature Structure of the Intra-Cluster Medium from SPH and AMR simulations
• STARFORGE: The effects of protostellar outflows on the IMF
• Intrinsic galaxy shapes and alignments I: Measuring and modelling COSMOS intrinsic galaxy ellipticities
• Direct detection of self-interacting dark matter
• Quenching Massive Galaxies with On-the-fly Feedback in Cosmological Hydrodynamic Simulations
• Large scale bias and the inaccuracy of the peak-background split
• Modelling Shock Heating in Cluster Mergers: I. Moving Beyond the Spherical Accretion Model
• Simulations and symmetries
• Arc sensitivity to cluster ellipticity, asymmetries and substructures
• And yet it flips: connecting galactic spin and the cosmic web
• The Non-Linear Power Spectrum of the Lyman Alpha Forest
• The large-scale properties of simulated cosmological magnetic fields
• Density profiles of ultracompact minihalos: Implications for constraining the primordial power spectrum
• Photon underproduction crisis: Are QSOs sufficient to resolve it?
• How common is the Milky Way - satellite system alignment?
• Buried AGNs in Advanced Mergers:Mid-infrared color selection as a dual AGN finder
• Quantifying stellar radial migration in an N-body simulation: blurring, churning, and the outer regions of galaxy discs
• The environmental dependence of gas accretion onto galaxies: quenching satellites through starvation
• Dark Energy Survey Year 3 Results: Clustering Redshifts -- Calibration of the Weak Lensing Source Redshift Distributions with redMaGiC and BOSS/eBOSS
• CANDELS: The correlation between galaxy morphology and star formation activity at z~2
• Consequences of Mechanical and Radiative Feedback from Black Holes in Disc Galaxy Mergers
• The primordial environment of super massive black holes: large scale galaxy overdensities around $z\sim 6$ QSOs with LBT
• Baryon Cycling in the Low-Redshift Circumgalactic Medium: A Comparison of Simulations to the COS-Halos Survey
• Tree-based solvers for adaptive mesh refinement code FLASH - I: gravity and optical depths
• The Aurora radiation-hydrodynamical simulations of reionization: calibration and first results
• X-MAS2: Study Systematics on the ICM Metallicity Measurements
• Environmental dependence of bulge-dominated galaxy sizes in hierarchical models of galaxy formation. Comparison with the local Universe
• Cosmological constraints from noisy convergence maps through deep learning
• Abundance matching with the mean star formation rate: there is no missing satellites problem in the Milky Way above ${\mathbf{M}}_{200}\sim 10^9{\mathbf{M}}_{\odot }$
• N-body simulations with generic non-Gaussian initial conditions I: Power Spectrum and halo mass function
• Populations of filaments from the distribution of galaxies in numerical simulations
• Evolution of Massive Haloes in non-Gaussian Scenarios
• Beyond LIMD bias: a measurement of the complete set of third-order halo bias parameters
• The First Galaxies: Assembly under Radiative Feedback from the First Stars
• The Effect of Gas Physics on the Halo Mass Function
• Damped Lyman-alpha systems in high-resolution hydrodynamical simulations
• Impact of radial migration on stellar and gas radial metallicity distribution
• Covariance of cross-correlations: towards efficient measures for large-scale structure
• MApping the Most Massive Overdensities Through Hydrogen (MAMMOTH) I: Methodology
• Cosmic Shear Cosmology Beyond 2-Point Statistics: A Combined Peak Count and Correlation Function Analysis of DES-Y1
• Dark Energy Survey Year 1 Results: Cross-Correlation Redshifts - Methods and Systematics Characterization
• The fine line between total and partial tidal disruption events
• On the reach of perturbative descriptions for dark matter displacement fields
• Manifold-driven spirals in N-body barred galaxy simulations
• On the galaxy spiral arms' nature as revealed by rotation frequencies
• An analytic model for the bispectrum of galaxies in redshift space
• Shock finding on a moving-mesh: I. Shock statistics in non-radiative cosmological simulations
• Fast and accurate mock catalogue generation for low-mass galaxies
• A hypervelocity star with a Magellanic origin
• The formation of low metallicity globular clusters in dwarf galaxy mergers
• Resolving Cosmic Neutrino Structure: A Hybrid Neutrino N-body Scheme
• Unveiling Dark Matter free-streaming at the smallest scales with high redshift Lyman-alpha forest
• Constructing Regularized Cosmic Propagators
• Chemical mixing in smoothed particle hydrodynamics simulations
• A first direct measurement of the intergalactic medium temperature around a quasar at z=6
• The visibility of Lyman Alpha Emitters during reionization
• The peculiar Type Ia supernova iPTF14atg: Chandrasekhar-mass explosion or violent merger?
• The origin of ICM enrichment in the outskirts of present-day galaxy clusters from cosmological hydrodynamical simulations
• Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and galaxy-galaxy lensing using the MagLim lens sample
• Planes of satellites around Milky Way/M31-mass galaxies in the FIRE simulations and comparisons with the Local Group
• The role of dry mergers for the formation and evolution of brightest cluster galaxies
• On the impact of baryons on the halo mass function, bias, and cluster cosmology
• Energy- and momentum-conserving AGN feedback outflows
• Massive black hole evolution models confronting the n-Hz amplitude of the stochastic gravitational wave background
• The relative and absolute ages of old globular clusters in the LCDM framework
• Diversity in density profiles of self-interacting dark matter satellite halos
• Avoiding progenitor bias: The structural and mass evolution of Brightest Group and Cluster Galaxies in Hierarchical models since z~1
• Post-Newtonian dynamical modeling of supermassive black holes in galactic-scale simulations
• Constraining neutrino mass with tomographic weak lensing one-point probability distribution function and power spectrum
• The Tully-Fisher and mass-size relations from halo abundance matching
• 24.77 Pflops on a Gravitational Tree-Code to Simulate the Milky Way Galaxy with 18600 GPUs
• Clustering and Halo Abundances in Early Dark Energy Cosmological Models
• Radiation hydrodynamics simulations of the formation of direct-collapse supermassive stellar systems
• Are ultracompact minihalos really ultracompact?
• Steep Faint-end Slopes of Galaxy Mass and Luminosity Functions at z>=6 and the Implications for Reionisation
• The Morphologies and Alignments of Gas, Mass, and the Central Galaxies of CLASH Clusters of Galaxies
• The Abell 3391/95 galaxy cluster system: A 15 Mpc intergalactic medium emission filament, a warm gas bridge, infalling matter clumps, and (re-) accelerated plasma discovered by combining SRG/eROSITA data with ASKAP/EMU and DECam data
• Modeling of Emission Signatures of Massive Black Hole Binaries: I Methods
• Mapping Growth and Gravity with Robust Redshift Space Distortions
• Shedding Light on the Galaxy Luminosity Function
• On the Effects of Line-of-Sight Structures on Lensing Flux-ratio Anomalies in a LCDM Universe
• Ram pressure stripping in a galaxy formation model. I. A novel numerical approach
• Idealized models for galactic disk formation and evolution in 'realistic' LambdaCDM haloes
• Convergence of the critical cooling rate for protoplanetary disk fragmentation achieved; the key role of numerical dissipation of angular momentum
• N-body Integrators with Individual Time Steps from Hierarchical Splitting
• Primordial Non-Gaussianity from Biased Tracers: Likelihood Analysis of Real-Space Power Spectrum and Bispectrum
• Testing the theory of gravity with DESI: estimators, predictions and simulation requirements
• SN 2010lp---a Type Ia supernova from a violent merger of two carbon--oxygen White Dwarfs
• Reproducing properties of MW dSphs as descendants of DM-free TDGs
• The impact of baryonic discs on the shapes and profiles of self-interacting dark matter halos
• Dark matter statistics for large galaxy catalogs: power spectra and covariance matrices
• Dust scaling relations in a cosmological simulation
• Efficient common-envelope ejection through dust-driven winds
• The properties of "dark" ΛCDM halos in the Local Group
• Large-Scale Structure in Brane-Induced Gravity II. Numerical Simulations
• Integral constraints in spectroscopic surveys
• The First Stars: A Low-Mass Formation Mode
• Measuring the growth of matter fluctuations with third-order galaxy correlations
• The THESAN project: ionizing escape fractions of reionization-era galaxies
• Exploring the hydrostatic mass bias in MUSIC clusters: application to the NIKA2 mock sample
• Dynamical difference between the cD galaxy and the stellar diffuse component in simulated galaxy clusters
• Hierarchical Cosmic Shear Power Spectrum Inference
• PyUltraLight: A Pseudo-Spectral Solver for Ultralight Dark Matter Dynamics
• Stellar migrations and metal flows -- Chemical evolution of the thin disc of a simulated Milky Way analogous galaxy
• Feedback from supermassive black holes transforms centrals into passive galaxies by ejecting circumgalactic gas
• Cosmic voids in modified gravity models with massive neutrinos
• Enrichment and Pre-Heating in Intragroup Gas from Galactic Outflows
• DEMNUni: ISW, Rees-Sciama, and weak-lensing in the presence of massive neutrinos
• Effects of Varying the Three-Body Molecular Hydrogen Formation Rate in Primordial Star Formation
• Simulations of Axion Minihalos
• The formation of extremely diffuse galaxy cores by merging supermassive black holes
• Deviations from hydrostatic equilibrium in the circumgalactic medium: spinning hot haloes and accelerating flows
• Galaxy morphology, kinematics and clustering in a hydrodynamic simulation of a LambdaCDM universe
• A comparison of observed and simulated absorption from HI, CIV, and SiIV around $z\approx 2$ star-forming galaxies suggests redshift-space distortions are due to inflows
• Simulation of Astronomical Images from Optical Survey Telescopes using a Comprehensive Photon Monte Carlo Approach
• An N-body/SPH Study of Isolated Galaxy Mass Density Profiles
• Major Mergers Going Notts: Challenges for Modern Halo Finders
• Disruption of satellite galaxies in simulated groups and clusters: the roles of accretion time, baryons, and pre-processing
• Modeling the neutral hydrogen distribution in the post-reionization Universe: intensity mapping
• Properties of HI discs in the Auriga cosmological simulations
• The build up of the correlation between halo spin and the large scale structure
• Properties of the galaxy population in hydrodynamical simulations of clusters
• Quenching timescales of galaxies in the EAGLE simulations
• High-redshift quasars and their host galaxies I: kinematical and dynamical properties and their tracers
• One moment in time - modeling star formation in the Antennae
• Reionization in Technicolor
• Probing the galaxy-halo connection in UltraVISTA to $z\sim 2$
• The statistical properties of LCDM halo formation
• Cosmic web anisotropy is the primary indicator of halo assembly bias
• Dark Energy Survey Year 3 results: cosmological constraints from the analysis of cosmic shear in harmonic space
• The angle-averaged squeezed limit of nonlinear matter N-point functions
• A tale of two populations: surviving and destroyed dwarf galaxies and the build up of the Milky Way's stellar halo
• Formation histories of stars, clusters and globular clusters in the E-MOSAICS simulations
• The evolution of the star formation rate function in the EAGLE simulations: A comparison with UV, IR and H$\alpha$ observations from z ~ 8 to z ~ 0
• The Dynamical State of Dark Matter Haloes in Cosmological Simulations I: Correlations with Mass Assembly History
• First observational support for overlapping reionized bubbles generated by a galaxy overdensity
• Particle hydrodynamics with tessellation techniques
• Relativistic N-body simulations with massive neutrinos
• Chasing the Tail of Cosmic Reionization with Dark Gap Statistics in the Ly$\alpha$ Forest over $5<z<6$
• A rigorous EFT-based forward model for large-scale structure
• 3D Simulations of Betelgeuse's Bow Shock
• Do Mergers Spin up Dark Matter Halos?
• Starbursting [O III] emitters and quiescent [C II] emitters in the reionization era
• Computing General Relativistic effects from Newtonian N-body simulations: Frame dragging in the post-Friedmann approach
• The Lyman-alpha forest in a blazar-heated Universe
• Metal-poor star formation triggered by the feedback effects from Pop III stars
• Hot and Cooled baryons in SPH simulations of galaxy clusters: physics and numerics
• The Chandra survey of the COSMOS field II: source detection and photometry
• The separate and combined effects of baryon physics and neutrino free-streaming on large-scale structure
• The ${}^{12}$CO/${}^{13}$CO ratio in turbulent molecular clouds
• Spurious heating of stellar motions in simulated galactic disks by dark matter halo particles
• Fade to grey: systematic variation of the galaxy attenuation curves with galaxy properties in EAGLE
• Brightest cluster galaxies in cosmological simulations: achievements and limitations of AGN feedback models
• NGC6240: Merger-Induced Star Formation & Gas Dynamics
• Lyman-alpha Emitters and Lyman-break Galaxies at z=3-6 in Cosmological SPH Simulations
• Discreteness Effects in Lambda Cold Dark Matter Simulations: A Wavelet-Statistical View
• Quasar feedback: accelerated star formation and chaotic accretion
• Universality of dark matter haloes shape over six decades in mass: Insights from the Millennium XXL and SBARBINE simulations
• Scaling relations and mass bias in hydrodynamical f(R) gravity simulations of galaxy clusters
• Heating of the Intergalactic Medium by Hydrogen Reionization
• Escape of Lyman-alpha and continuum photons from star-forming galaxies
• Realistic simulations of gravitational lensing by galaxy clusters: extracting arc parameters from mock DUNE images
• On the onset of runaway stellar collisions in dense star clusters - II. Hydrodynamics of three-body interactions
• Improving fast generation of halo catalogs with higher-order Lagrangian perturbation theory
• The impact of Early Dark Energy on non-linear structure formation
• The Lyman-$\alpha$ forest as a diagnostic of the nature of the dark matter
• The Mildly Non-Linear Regime of Structure Formation
• Constraining the halo bispectrum in real and redshift space from perturbation theory and non-linear stochastic bias
• Quenching star formation in cluster galaxies
• Dual-criteria time stepping for weakly compressible smoothed particle hydrodynamics
• SZE Observables, Pressure Profiles and Center Offsets in Magneticum Simulation Galaxy Clusters
• Clarifying the effects of interacting dark energy on linear and nonlinear structure formation processes
• General relativistic corrections to $N$-body simulations and the Zel'dovich approximation
• Thinking Outside the Box: Effects of Modes Larger than the Survey on Matter Power Spectrum Covariance
• Alignments of Galaxy Group Shapes with Large Scale Structure
• SPHRAY: A Smoothed Particle Hydrodynamics Ray Tracer for Radiative Transfer
• On the linearity of tracer bias around voids
• Spatially adaptive radiation-hydrodynamical simulations of galaxy formation during cosmological reionization
• An EAGLE view of the missing baryons
• FIR line emission from high redshift galaxies
• The Non-Gaussian Halo Mass Function with fNL, gNL and tauNL
• Gravitational waves from Population III binary black holes formed by dynamical capture
• VINE -- A numerical code for simulating astrophysical systems using particles I: Description of the physics and the numerical methods
• From galactic nuclei to the halo outskirts: tracing supermassive black holes across cosmic history and environments
• The multiplicity and anisotropy of galactic satellite accretion
• The grouping, merging and survival of subhaloes in the simulated Local Group
• Implementation of Sink Particles in the Athena Code
• Galactic nuclei evolution with spinning black holes: method and implementation
• The angular momentum of cold dark matter haloes with and without baryons
• The surprising accuracy of isothermal Jeans modelling of self-interacting dark matter density profiles
• Shear Power Spectrum Reconstruction using Pseudo-Spectrum Method
• Probing the Circumgalactic Medium at High-Redshift Using Composite BOSS Spectra of Strong Lyman-alpha Forest Absorbers
• Physical properties of simulated galaxy populations at z=2 - I. Effect of metal-line cooling and feedback from star formation and AGN
• The Accretion Disc Particle Method for Simulations of Black Hole Feeding and Feedback
• A general explanation on the correlation of dark matter halo spin with the large scale environment
• Modeling the Dust Properties of z ~ 6 Quasars with ART^2 -- All-wavelength Radiative Transfer with Adaptive Refinement Tree
• Cosmological simulations of black hole growth II: how (in)significant are merger events for fuelling nuclear activity?
• New approach for precise computation of Lyman-alpha forest power spectrum with hydrodynamical simulations
• A new model to predict weak-lensing peak counts I. Comparison with $N$-body Simulations
• Breaking degeneracies in modified gravity with higher (than 2nd) order weak-lensing statistics
• The fully connected N-dimensional skeleton: probing the evolution of the cosmic web
• LYRA I: Simulating the multi-phase ISM of a dwarf galaxy with variable energy supernovae from individual stars
• Suppressing structure formation at dwarf galaxy scales and below: late kinetic decoupling as a compelling alternative to warm dark matter
• Identification of members in the central and outer regions of galaxy clusters
• Accretion Shocks in Clusters of Galaxies and their SZ Signature from Cosmological Simulations
• Dynamics of stream-subhalo interactions
• Cosmic voids in coupled dark energy cosmologies: the impact of halo bias
• Constraints on the CMB Temperature Evolution using Multi-Band Measurements of the Sunyaev Zel'dovich Effect with the South Pole Telescope
• A semi-analytic dynamical friction model for cored galaxies
• Turbulent Velocity Fields in SPH--simulated Galaxy Clusters
• Back in the saddle: Large-deviation statistics of the cosmic log-density field
• CMB weak-lensing beyond the Born approximation: a numerical approach
• Weak Lensing Light-Cones in Modified Gravity simulations with and without Massive Neutrinos
• Comparison of an X-ray selected sample of massive lensing clusters with the MareNostrum Universe LCDM simulation
• The Peaks Formalism and the Formation of Cold Dark Matter Haloes
• The Redshift Space Momentum Power Spectrum II: measuring the growth rate from the combined 2MTF and 6dFGSv surveys
• The cosmology dependence of weak lensing cluster counts
• Towards an understanding of the evolution of the scaling relations for supermassive black holes
• Dark matter-radiation interactions: the structure of Milky Way satellite galaxies
• Super-resolution emulator of cosmological simulations using deep physical models
• Modelling the circumstellar medium in RS Ophiuchi and its link to Type Ia supernovae
• Higher Order Contributions to the 21 cm Power Spectrum
• N-body methods for relativistic cosmology
• The nebular emission of star-forming galaxies in a hierarchical universe
• Distribution of Damped Lyman-alpha Absorbers in a Lambda Cold Dark Matter Universe
• HALOGEN: A tool for fast generation of mock halo catalogues
• Massive and refined: a sample of large galaxy clusters simulated at high resolution. I:Thermal gas and shock waves properties
• Why Are AGN and Host Galaxies Misaligned?
• Predicted Extension of the Sagittarius Stream to the Milky Way Virial Radius
• A Robust and Efficient Deep Learning Method for Dynamical Mass Measurements of Galaxy Clusters
• Does the dwarf galaxy system of the Milky Way originate from Andromeda?
• Lyman Alpha Emitter Evolution in the Reionization Epoch
• Simulating the assembly of galaxies at redshifts z = 6 - 12
• The Effects of AGN Feedback on Present-Day Galaxy Properties in Cosmological Simulations
• Cosmology from large scale galaxy clustering and galaxy-galaxy lensing with Dark Energy Survey Science Verification data
• Gamma-ray burst rate: high-redshift excess and its possible origins
• The CAMELS Multifield Dataset: Learning the Universe's Fundamental Parameters with Artificial Intelligence
• A sub-resolution multiphase interstellar medium model of star formation and SNe energy feedback
• Interpreting the observed UV continuum slopes of high-redshift galaxies
• New limits on light dark matter - proton cross section from the cosmic large-scale structure
• Hypervelocity runaways from the Large Magellanic Cloud
• The Impact of Box Size on the Properties of Dark Matter Haloes in Cosmological Simulations
• Bayesian emulator optimisation for cosmology: application to the Lyman-alpha forest
• On the dynamical state of galaxy clusters: insights from cosmological simulations II
• How galaxies lose their angular momentum
• Lyman Alpha Emitters and Lyman Break Galaxies: dichotomous twins?
• The Three Hundred Project: correcting for the hydrostatic-equilibrium mass bias in X-ray and SZ surveys
• On ths assembly history of stellar components in massive galaxies
• Towards an Optimal Reconstruction of Baryon Oscillations
• Euclid: Forecasts from redshift-space distortions and the Alcock-Paczynski test with cosmic voids
• Precision modeling of redshift-space distortions from multi-point propagator expansion
• ART^2 : Coupling Lyman-alpha Line and Multi-wavelength Continuum Radiative Transfer
• Stray, swing and scatter: angular momentum evolution of orbits and streams in aspherical potentials
• Verifying the consistency relation for the scale-dependent bias from local primordial non-Gaussianity
• Music from the heavens - Gravitational waves from supermassive black hole mergers in the EAGLE simulations
• The impact of feedback on the low redshift Intergalactic Medium
• Correlating galaxy colour and halo concentration: A tunable Halo Model of galactic conformity
• On the validity of the Born approximation for beyond-Gaussian weak lensing observables
• Dark Energy Survey Year 3 results: cosmology with moments of weak lensing mass maps -- validation on simulations
• Evolution of galaxy size--stellar mass relation from the Kilo Degree Survey
• Formation of tidally induced bars in galactic flybys: prograde versus retrograde encounters
• The CAMELS project: public data release
• An Efficient and Accurate Hybrid Method for Simulating Non-Linear Neutrino Structure
• The accuracy of semi-numerical reionization models in comparison with radiative transfer simulations
• The oxygen abundance gradients in the gas discs of galaxies in the EAGLE simulation
• rpSPH: a novel Smoothed Particle Hydrodynamics Algorithm
• Turbovelocity Stars: Kicks Resulting From the Tidal Disruption of Solitary Stars
• Weighing neutrinos with cosmic neutral hydrogen
• Is the black hole in NGC1277 really over-massive?
• N-body simulations with generic non-Gaussian initial conditions II: Halo bias
• Thermal and nonthermal dust sputtering in hydrodynamical simulations of the multiphase interstellar medium
• Revealing the tidal scars of the Small Magellanic Cloud
• Constrained Local UniversE Simulations: A Local Group Factory
• The formation of hot gaseous haloes around galaxies
• Metallicity dependence of the H/H${}_2$ and C${}^{+}$/C/CO distributions in a resolved self-regulating interstellar medium
• Bar Formation from Galaxy Flybys
• The DIANOGA simulations of galaxy clusters: characterizing star formation in proto-clusters
• Galactic Winds and Extended Lya Emission from the Host Galaxies of High Column Density QSO Absorption Systems
• Constraining the PopIII IMF with high-z GRBs
• Galaxy Infall Kinematics as a Test of Modified Gravity
• Large-scale assembly bias of dark matter halos
• The impact of the connectivity of the cosmic web on the physical properties of galaxies at its nodes
• Dark-Matter Decays and Self-Gravitating Halos
• Peaks above the Maxwellian Sea: A New Approach to Finding Substructure in N-Body Haloes
• The Importance of Quantum Pressure of Fuzzy Dark Matter on Lyman-Alpha Forest
• Deep learning dark matter map reconstructions from DES SV weak lensing data
• Impact of the cosmic background radiation on the initial mass function of metal-poor stars
• Quasar outflows at $z\ge 6$: the impact on the host galaxies
• Higher-order initial conditions for mixed baryon-CDM simulations
• Being KLEVER at cosmic noon: ionised gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts
• Shepherding Tidal Debris with the Galactic Bar: The Ophiuchus Stream
• On column density thresholds and the star formation rate
• Halo Shapes From Weak Lensing: The Impact of Galaxy--Halo Misalignment
• Using hierarchical octrees in Monte Carlo radiative transfer simulations
• The impact of AGN feedback and baryonic cooling on galaxy clusters as gravitational lenses
• The Sherwood-Relics simulations: overview and impact of patchy reionization and pressure smoothing on the intergalactic medium
• Baryon Acoustic Oscillations in 2D II: Redshift-space halo clustering in N-body simulations
• On the Self-Similar Appearance of Galaxy Clusters in X-rays
• New analytical solutions for chemical evolution models: characterizing the population of star-forming and passive galaxies
• A Study of the Effect of Bulges on Bar Formation in Disk galaxies
• Was the nineteenth century giant eruption of Eta Carinae a merger event in a triple system?
• Unfolding the Hierarchy of Voids
• An analytic approach to number counts of weak-lensing peak detections
• Three-Point Correlation Functions of SDSS Galaxies: Constraining Galaxy-Mass Bias
• Do AGN outflows quench or enhance star formation?
• Knowing the unknowns: uncertainties in simple estimators of galactic dynamical masses
• Carbon-Enhanced Metal-Poor Stars, the Cosmic Microwave Background, and the Stellar IMF in the Early Universe
• Pressure Support vs. Thermal Broadening in the Lyman-alpha Forest I: Effects of the Equation of State on Longitudinal Structure
• Constraining Neutrino Mass with the Tomographic Weak Lensing Bispectrum
• The Once and Future Andromeda Stream
• Scaling relations of Fuzzy Dark Matter haloes I: individual systems in their cosmological environment
• A Pulsed, Precessing Jet in Cepheus A
• The halo model in a massive neutrino cosmology
• Primordial Features from Linear to Nonlinear Scales
• Scaling relations between black holes and their host galaxies: comparing theoretical and observational measurements, and the impact of selection effects
• Remodeling the evolution of grain size distribution in galaxies
• On the temperature structure of the Galactic Centre cloud G0.253+0.016
• The chemical enrichment of the ICM from hydrodynamical simulations
• Galactic Simulations of r-process Elemental Abundances
• Absorption signatures of warm-hot gas at low redshift: OVI
• Connecting Reionization to the Local Universe
• How many radio relics await discovery?
• Machine learning cosmological structure formation
• The Epoch of IGM heating by early sources of X-rays
• Constraining neutrino mass with weak lensing Minkowski Functionals
• SURFS: Riding the waves with Synthetic UniveRses For Surveys
• The 21cm bispectrum during reionization: a tracer of the ionization topology
• Simulations of the Local Universe Constrained by Observational Peculiar Velocities
• Constraining neutrino mass with tomographic weak lensing peak counts
• Zooming in on Individual Star Formation: Low- and High-mass Stars
• Simulating Structure Formation of the Local Universe
• The effects of metallicity, UV radiation and non-equilibrium chemistry in high-resolution simulations of galaxies
• Rhapsody. I. Structural Properties and Formation History From a Statistical Sample of Re-simulated Cluster-size Halos
• Statistical properties of paired fixed fields
• Bar-formation as driver of gas inflows in isolated disc galaxies
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).IX. The effects of ram pressure stripping down to the scale of individual HII regions in the dwarf galaxy IC 3476
• Gravothermal evolution of dark matter halos with differential elastic scattering
• Statistical and Systematic Errors in Measurement of Weak-Lensing Minkowski Functionals: Application to Canada-France-Hawaii Lensing Survey
• Resolving The Generation of Starburst Winds in Galaxy Mergers
• Spatial fluctuations of the intergalactic temperature-density relation after hydrogen reionization
• Universal at last? The splashback mass function of dark matter halos
• Growth of brightest cluster galaxies via mergers since z = 1
• Blandford-Znajek jets in galaxy formation simulations: method and implementation
• Scale-dependent bias and bispectrum in neutrino separate universe simulations
• The UV, Lyman-alpha, and dark matter halo properties of high redshift galaxies
• Secular Damping of Stellar Bars in Spinning Dark Matter Halos
• A Self-interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties
• An exact general remeshing scheme applied to physically conservative voxelization
• Concordance cosmology without dark energy
• When the Jeans don't fit: How stellar feedback drives stellar kinematics and complicates dynamical modeling in low-mass galaxies
• Gravitational recoils of supermassive black holes in hydrodynamical simulations of gas rich galaxies
• Secondary Infall and the Pseudo-Phase-Space Density Profiles of Cold Dark Matter Halos
• The fundamental signature of star formation quenching from AGN feedback: A critical dependence of quiescence on supermassive black hole mass not accretion rate
• The Edge of the Galaxy
• The Birth and Growth of Neutralino Haloes
• Physics of Galactic Metals: Evolutionary Effects due to Production, Distribution, Feedback & Interaction with Black Holes
• Signatures of LCDM substructure in tidal debris
• GalaxyNet: Connecting galaxies and dark matter haloes with deep neural networks and reinforcement learning in large volumes
• Local Group Dwarf Galaxies: Nature And Nurture
• Tidal dwarf galaxies in cosmological simulations
• Genetically modified halos: towards controlled experiments in $\Lambda$CDM galaxy formation
• Identifying the subtle signatures of feedback from distant AGN using ALMA observations and the EAGLE hydrodynamical simulations
• The chemical evolution of a Milky Way-like galaxy: the importance of a cosmologically motivated infall law
• Photo-heating and the fate of hard photons during the reionisation of HeII by quasars
• Scientific Visualization in Astronomy: Towards the Petascale Astronomy Era
• The ThreeHundred: the structure and properties of cosmic filaments in the outskirts of galaxy clusters
• Astrophysical hydrodynamics with a high-order discontinuous Galerkin scheme and adaptive mesh refinement
• The imprint of cosmic reionisation on the luminosity function of galaxies
• Predictions and sensitivity forecasts for reionization-era [C II] line intensity mapping
• Global Star Formation Rates and Dust Emission Over the Galaxy Interaction Sequence
• Studying the Lyman-$\alpha$ optical depth fluctuations at $z\sim 5.5$ using fast semi-numerical methods
• Statistics of extreme objects in the Juropa Hubble Volume simulation
• Seeding Black Holes in Cosmological Simulations
• The observational signature of the first H II regions
• Galaxy-Galaxy Lensing in the DES Science Verification Data
• Resonant Sterile Neutrino Dark Matter in the Local and High-z Universe
• A New Model for the Milky Way Bar
• The natural emergence of the correlation between H2 and star formation rate surface densities in galaxy simulations
• The biasing of baryons on the cluster mass function and cosmological parameter estimation
• Modeling the nonlinear clustering in modified gravity models I: A fitting formula for matter power spectrum of f(R) gravity
• Three-dimensional hydrodynamical simulations of mass transfer in binary systems by a free wind
• Toward a robust inference method for the galaxy bispectrum: likelihood function and model selection
• The Velocity Field of the Local Universe from Measurements of Type Ia Supernovae
• Generation of highly inclined protoplanetary discs through single stellar flybys
• The Redshift-Space Cluster-Galaxy Cross-Correlation Function: I. Modeling Galaxy Infall onto Millennium Simulation Clusters and SDSS Groups
• The quiescent phase of galactic disc growth
• The interaction of core-collapse supernova ejecta with a companion star
• Mapping the Real Space Distributions of Galaxies in SDSS DR7: II. Measuring the growth rate, clustering amplitude of matter and biases of galaxies at redshift $0.1$
• Stellar feedback by radiation pressure and photoionization
• Photo-heating and supernova feedback amplify each other's effect on the cosmic star formation rate
• Lyman-alpha emitters gone missing: the different evolution of the bright and faint populations
• Redshift-space distortions with split densities
• Dense Molecular Gas: A Sensitive Probe of Stellar Feedback Models
• Intergalactic Lyman continuum photon budget in the past 5 billion years
• Using 3D Voronoi grids in radiative transfer simulations
• On the Origin of Dynamically Cold Rings Around the Milky Way
• Puffing up early-type galaxies by baryonic mass loss: numerical experiments
• Inverted initial conditions: exploring the growth of cosmic structure and voids
• Detection and extraction of signals from the epoch of reionization using higher order one-point statistics
• Forming massive seed black holes in high-redshift quasar host progenitors
• Multi-frequency, thermally coupled radiative transfer with TRAPHIC: Method and tests
• The Atacama Cosmology Telescope: Dynamical masses for 44 SZ-selected galaxy clusters over 755 square degrees
• High-z massive clusters as a test for dynamical coupled dark energy
• The clustering dynamics of primordial black boles in $N$-body simulations
• Finding cosmic voids and filament loops using topological data analysis
• Black hole evolution: II. Spinning black holes in a supernova-driven turbulent interstellar medium
• Machine Learning and Cosmological Simulations II: Hydrodynamical Simulations
• Counterrotating Stars in Simulated Galaxy Disks
• Dark Matter Deficient Galaxies Produced Via High-velocity Galaxy Collisions In High-resolution Numerical Simulations
• How does our choice of observable influence our estimation of the centre of a galaxy cluster? Insights from cosmological simulations
• Primordial non-Gaussianity without tails -- how to measure fNL with the bulk of the density PDF
• Self-gravitating fragmentation of eccentric accretion disks
• Simulations of common envelope evolution in triple systems: Circumstellar case
• Collision velocity of dust grains in self-gravitating protoplanetary discs
• AGN contamination of galaxy-cluster thermal X-ray emission: predictions for eRosita from cosmological simulations
• The luminosities of backsplash galaxies in constrained simulations of the Local Group
• Bayesian analysis of the dynamic cosmic web in the SDSS galaxy survey
• Kinetic AGN Feedback Effects on Cluster Cool Cores Simulated using SPH
• Bending Waves in the Milky Way's disc from halo substructure
• Extinguishing the FIRE: environmental quenching of satellite galaxies around Milky Way-mass hosts in simulations
• BCG Mass Evolution in Cosmological Hydro-Simulations
• Non-Gaussian Error Contribution to Likelihood Analysis of the Matter Power Spectrum
• Mocking the Weak Lensing universe: the LensTools python computing package
• Testing cosmology with a catalogue of voids in the BOSS galaxy surveys
• Using CO line ratios to trace the physical properties of molecular clouds
• Properties of Resonantly Produced Sterile Neutrino Dark Matter Subhalos
• Particle-Particle Particle-Tree: A Direct-Tree Hybrid Scheme for Collisional N-Body Simulations
• On the shape of dark matter halos from MultiDark Planck simulations
• Early structure formation in quintessence models and its implications for cosmic reionisation from first stars
• The latitude dependence of the rotation measures of NVSS sources
• Evaluating Galactic Habitability Using High Resolution Cosmological Simulations of Galaxy Formation
• The effect of intergalactic helium on hydrogen reionisation: implications for the sources of ionising photons at z > 6
• The Origin of the Microlensing Events Observed Towards the LMC and the Stellar Counterpart of the Magellanic Stream
• The impact of baryonic physics on the shape and radial alignment of substructures in cosmological dark matter haloes
• Size matters: abundance matching, galaxy sizes, and the Tully-Fisher relation in EAGLE
• Active galactic nuclei and massive galaxy cores
• Alignments between galaxies, satellite systems and haloes
• Intensity mapping with SDSS/BOSS Lyman-alpha emission, quasars and their Lyman-alpha forest
• The Magellanic Stream at 20 kpc: A New Orbital History for the Magellanic Clouds
• The Magellanic Corona and the formation of the Magellanic Stream
• Merger-induced galaxy transformations in the ARTEMIS simulations
• Under the Firelight: Stellar Tracers of the Local Dark Matter Velocity Distribution in the Milky Way
• Accurate Identification of Galaxy Mergers with Imaging
• Migration of massive black hole binaries in self--gravitating accretion discs: Retrograde versus prograde
• Phase-space structures II: Hierarchical Structure Finder
• The impact of quenching on galaxy profiles in the Simba simulation
• Using gaps in N-body tidal streams to probe missing satellites
• EMERGE: Empirical predictions of galaxy merger rates since $z\sim 6$
• Bondi-Hoyle-Littleton accretion and the upper mass stellar IMF
• Interpreting the evolution of galaxy colours from $z=8$ to $z=5$
• The Three Hundred Project: The evolution of galaxy cluster density profiles
• Spatial fluctuations in the spectral shape of the UV background at 2<z<3 and the reionization of helium
• The effect of variations in the input physics on the cosmic distribution of metals predicted by simulations
• Warm dark matter signatures on the 21cm power spectrum: Intensity mapping forecasts for SKA
• On the Segregation of Dark Matter Substructure
• The effect of environment on star forming galaxies at redshift 1 - First insight from PACS
• ColDICE: a parallel Vlasov-Poisson solver using moving adaptive simplicial tessellation
• Early massive clusters and the bouncing coupled dark energy
• Early formation of supermassive black holes via dark matter self-interactions
• The sizes of mini-voids in the local universe: an argument in favor of a warm dark matter model?
• Dynamical evolution of cosmic supermassive binary black holes and their gravitational wave radiation
• Metal enrichment of the intra-cluster medium over a Hubble time for merging and relaxed galaxy clusters
• Impact of Baryonic Processes on Weak Lensing Cosmology: Power Spectrum, Non-Local Statistics, and Parameter Bias
• Future Evolution of Bound Superclusters in an Accelerating Universe
• Rotation curve fitting and its fatal attraction to cores in realistically simulated galaxy observations
• Simulating the 21-cm signal from reionisation including non-linear ionisations and inhomogeneous recombinations
• The Limits of Bound Structures in the Accelerating Universe
• First-order Cosmological Perturbations Engendered by Point-like Masses
• Observing simulated galaxy clusters with PHOX: a novel X-ray photon simulator
• Toward an accurate mass function for precision cosmology
• Subparsec-scale dynamics of a dusty gas disk exposed to anisotropic AGN radiation with frequency-dependent radiative transfer
• A smooth particle hydrodynamics code to model collisions between solid, self-gravitating objects
• Moving mesh cosmology: properties of neutral hydrogen in absorption
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from multi-tracer BAO analysis with galaxies and voids
• Modelling the observed luminosity function and clustering evolution of Lyman-$\alpha$ emitters: growing evidence for late reionization
• Dependency of halo concentration on mass, redshift and fossilness in Magneticum hydrodynamic simulations
• The enrichment history of cosmic metals
• Smoothed Particle Magnetohydrodynamics IV - Using the Vector Potential
• Butterfly in a Cocoon, Understanding the origin and morphology of Globular Cluster Streams: The case of GD-1
• Cosmological Zoom Simulations of z = 2 Galaxies: The Impact of Galactic Outflows
• The evolution of galaxy cluster X-ray scaling relations
• From the Top Down and Back Up Again: Star Cluster Structure from Hierarchical Star Formation
• Testing Subhalo Abundance Matching in Cosmological Smoothed Particle Hydrodynamics Simulations
• Cosmological simulations of galaxy clusters with feedback from active galactic nuclei: profiles and scaling relations
• The impact of stellar feedback on hot gas in galaxy haloes: the Sunyaev-Zel'dovich effect and soft X-ray emission
• Empirical constraints on the formation of early-type galaxies
• The Outer Halos of Very Massive Galaxies: BCGs and their DSC in the Magneticum Simulations
• Baryon impact on weak lensing peaks and power spectrum: low-bias statistics and self-calibration in future surveys
• The origin of the $\alpha$-enhancement of massive galaxies
• Smoothed particle magnetohydrodynamics with a Riemann solver and the method of characteristics
• Electromagnetic Counterparts to Black Hole Mergers
• The large-scale environment of low surface brightness galaxies
• PySPH: a Python-based framework for smoothed particle hydrodynamics
• VoIgt profile Parameter Estimation Routine (VIPER): H I photoionization rate at z<0.5
• A look to the inside of haloes: a characterisation of the halo shape as a function of overdensity in the Planck cosmology
• WIMP searches with gamma rays in the Fermi era: challenges, methods and results
• Modelling neutral hydrogen in galaxies using cosmological hydrodynamical simulations
• Extragalactic gamma-ray background radiation from dark matter annihilation
• Calibrating an updated SPH scheme within GCD+
• Accurate emulator for the redshift-space power spectrum of dark matter halos and its application to galaxy power spectrum
• Calibration of semi-analytic models of galaxy formation using Particle Swarm Optimization
• Strong Dark Matter Self-interactions Diversify Halo Populations within and surrounding the Milky Way
• Non-linear hydrodynamics of axion dark matter: relative velocity effects and "quantum forces"
• Resolved galaxy scaling relations in the EAGLE simulation: star formation, metallicity and stellar mass on kpc scales
• Predicting FIR lines from simulated galaxies
• Formation of Warped Disks by Galactic Fly-by Encounters. I. Stellar Disks
• A First Look at Galaxy Flyby Interactions: I. Characterizing the Frequency of Flybys in a Cosmological Context
• Impact of H_2-based star formation model on the z>=6 luminosity function and the ionizing photon budget for reionization
• Cluster assembly and the origin of mass segregation in the STARFORGE simulations
• The star formation rate and stellar content contributions of morphological components in the EAGLE simulations
• Common envelope evolution of eccentric binaries
• The contributions of matter inside and outside of haloes to the matter power spectrum
• Can cluster merger shocks reproduce the luminosity and shape distribution of radio relics?
• Mixing in massive stellar mergers
• H0LiCOW VIII. A weak lensing measurement of the external convergence in the field of the lensed quasar HE0435$-$1223
• Numerical simulations of the possible origin of the two sub-parsec scale and counter-rotating stellar disks around SgrA*
• The Three Hundred Project: Ram pressure and gas content of haloes and subhaloes in the phase-space plane
• Witnessing galaxy assembly in an extended z~3 structure
• A combined analysis of 3D Weak Lensing, Lyman-alpha forest and WMAP year three data
• Linear response to long wavelength fluctuations using curvature simulations
• The impact of an evolving stellar initial mass function on early galaxies and reionisation
• Symphony: Cosmological Zoom-in Simulation Suites over Four Decades of Host Halo Mass
• Dust Evolution in Galaxy Cluster Simulations
• Fitting the nonlinear matter bispectrum by the Halofit approach
• Absorption signatures of warm-hot gas at low redshift: Broad HI Lyman-Alpha Absorbers
• The formation of Milky Way-mass disk galaxies in the first 500 million years of a cold dark matter universe
• SP(k) -- A hydrodynamical simulation-based model for the impact of baryon physics on the non-linear matter power spectrum
• Cosmology with galaxy-galaxy lensing on non-perturbative scales: Emulation method and application to BOSS LOWZ
• Modelling injection and feedback of Cosmic Rays in grid-based cosmological simulations: effects on cluster outskirts
• The Role of Gas In Maintaining Quasi-Steady Spiral Structure In Stellar Disks
• The BACCO simulation project: biased tracers in real space
• Peculiar Velocity Decomposition, Redshift Space Distortion and Velocity Reconstruction in Redshift Surveys. II. Dark Matter Velocity Statistics
• On the Dynamical Origin of the ICM Metallicity Evolution
• Simultaneous modelling of matter power spectrum and bispectrum in the presence of baryons
• Improving constraints on the growth rate of structure by modelling the density-velocity cross-correlation in the 6dF Galaxy Survey
• Inferring the IGM thermal history during reionisation with the Lyman-$\alpha$ forest power spectrum at redshift $z\simeq 5$
• Molecular Outflows in Galaxy Merger Simulations with Embedded AGN
• Models of Tidally Induced Gas Filaments in the Magellanic Stream
• The structure of gravitationally unstable gas-rich disk galaxies
• The influence of baryons on the mass distribution of dark matter halos
• Exploring the magnetized cosmic web through low frequency radio emission
• The merger-driven evolution of warm infrared luminous galaxies
• Caustics in growing Cold Dark Matter Haloes
• Kinetic or thermal AGN feedback in simulations of isolated and merging disk galaxies calibrated by the M-sigma relation
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• The Theoretical Astrophysical Observatory: Cloud-Based Mock Galaxy Catalogues
• Streams in the Aquarius stellar haloes
• Encounters of Merger and Accretion Shocks in Galaxy Clusters and their Effects on Intracluster Medium
• Evolution of N/O ratios in galaxies from cosmological hydrodynamical simulations
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 LRG sample: structure growth rate measurement from the anisotropic LRG correlation function in the redshift range 0.6 < z < 1.0
• Angular Signatures of Annihilating Dark Matter in the Cosmic Gamma-Ray Background
• Lyman-alpha Forest Constraints on Decaying Dark Matter
• The non-Gaussianity of the cosmic shear likelihood - or: How odd is the Chandra Deep Field South?
• Introducing EMP-Pathfinder: modelling the simultaneous formation and evolution of stellar clusters in their host galaxies
• Host galaxies of high-redshift quasars: supermassive black hole growth and feedback
• Reducing Noise in Cosmological N-body Simulations with Neutrinos
• Strong magnetic fields and large rotation measures in protogalaxies by supernova seeding
• Star Formation at Very Low Metallicity. IV. Fragmentation Does Not Depend on Metallicity for Cold Initial Conditions
• Unfolding the matter distribution using 3-D weak gravitational lensing
• Constraints on the star formation histories of galaxies from z~1 to z~0
• Tracing the Quenching History in Galaxy Clusters in the EAGLE Simulation
• Chronicling the reionization history at $6\lesssim z\lesssim 7$ with emergent quasar damping wings
• Galaxy simulation with the evolution of grain size distribution
• Cosmological perturbation theory for baryons and dark matter I: one-loop corrections in the RPT framework
• Vast planes of satellites in a high resolution simulation of the Local Group: comparison to Andromeda
• Impact of Scale Dependent Bias and Nonlinear Structure Growth on the ISW Effect: Angular Power Spectra
• Galactic inflow and wind recycling rates in the EAGLE simulations
• Large-Scale Structure Formation: from the first non-linear objects to massive galaxy clusters
• Realistic simulations of galaxy formation in f(R) modified gravity
• The Hydrodynamic Feedback of Cosmic Reionization on Small-Scale Structures and Its Impact on Photon Consumption during the Epoch of Reionization
• Simulations of Direct Collisions of Gas Clouds with the Central Black Hole
• Cosmic Emulation: The Concentration-Mass Relation for wCDM Universes
• Nonlinear clustering in models with primordial non-Gaussianity: the halo model approach
• An instability of feedback regulated star formation in galactic nuclei
• DISCO: A 3D Moving-Mesh Magnetohydrodynamics Code Designed for the Study of Astrophysical Disks
• The stability of stellar disks in Milky-Way sized dark matter halos
• The Effect of Primordial Non--Gaussianity on the Topology of Large-Scale Structure
• 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
• How well do cosmological simulations reproduce individual-halo properties?
• To beta or not to beta: can higher-order Jeans analysis break the mass-anisotropy degeneracy in simulated dwarfs?
• Reconstructing cosmic growth with kSZ observations in the era of Stage IV experiments
• Simulating the evolution of disc galaxies in a group environment. I. The influence of the global tidal field
• Joint deprojection of Sunyaev-Zeldovich and X-ray images of galaxy clusters
• Weak-Lensing Mass Calibration of the Atacama Cosmology Telescope Equatorial Sunyaev-Zeldovich Cluster Sample with the Canada-France-Hawaii Telescope Stripe 82 Survey
• Black hole spin and radio loudness in a LCDM universe
• A missing outskirts problem? Comparisons between stellar halos in the Dragonfly Nearby Galaxies Survey and the TNG100 simulation
• Multiphase, non-spherical gas accretion onto a black hole
• How Gas Accretion Feeds Galactic Disks
• Biases from neutrino bias: to worry or not to worry?
• The Signatures of Large-scale Temperature and Intensity Fluctuations in the Lyman-alpha Forest
• An $n$-th order Lagrangian Forward Model for Large-Scale Structure
• Reconstructing mass profiles of simulated galaxy clusters by combining Sunyaev-Zeldovich and X-ray images
• The cool side of Lyman Alpha Emitters
• Dark matter and halo bispectrum in redshift space: theory and applications
• Black Hole Formation in Fallback Supernova and the Spins of LIGO Sources
• Accurate mass and velocity functions of dark matter halos
• Magnetic field structure due to the global velocity field in spiral galaxies
• Nonlinear Biasing and Redshift-Space Distortions in Lagrangian Resummation Theory and N-body Simulations
• Precision cluster mass determination from weak lensing
• Scale Dependence of Halo Bispectrum from Non-Gaussian Initial Conditions in Cosmological N-body Simulations
• The GOGREEN survey: Post-infall environmental quenching fails to predict the observed age difference between quiescent field and cluster galaxies at z>1
• Bayesian inference from photometric redshift surveys
• The cosmological information of shear peaks: beyond the abundance
• CARPool: fast, accurate computation of large-scale structure statistics by pairing costly and cheap cosmological simulations
• The accretion of dark matter subhaloes within the cosmic web: primordial anisotropic distribution and its universality
• Self-Interacting Dark Matter and Small-Scale Gravitational Lenses in Galaxy Clusters
• How Biased Are Halo Properties in Cosmological Simulations?
• Cluster strong lensing in the Millennium Simulation: The effect of galaxies and structures along the line-of-sight
• GANDALF - Graphical Astrophysics code for N-body Dynamics And Lagrangian Fluids
• Galaxies undergoing ram-pressure stripping: the influence of the bulge on morphology and star formation rate
• Probing cosmology with weak lensing selected clusters I: Halo approach and all-sky simulations
• Weak Lensing Reveals a Tight Connection Between Dark Matter Halo Mass and the Distribution of Stellar Mass in Massive Galaxies
• The spatial and velocity bias of linear density peaks and proto-haloes in the Lambda cold dark matter cosmology
• GridSPT: Grid-based calculation for perturbation theory of large-scale structure
• Enriching the hot circumgalactic medium
• The central densities of Milky Way-mass galaxies in cold and self-interacting dark matter models
• PkANN - II. A non-linear matter power spectrum interpolator developed using artificial neural networks
• How low does it go? Too few Galactic satellites with standard reionization quenching
• Lagrangian or Eulerian; Real or Fourier? Not All Approaches to Large-Scale Structure Are Created Equal
• Cosmological Constraint on ${\Omega }_m$ and ${\sigma }_8$ from Cluster Abundances using the $GalWCat19$ Optical-Spectroscopic SDSS Catalog
• Transients from ONe White-Dwarf - Neutron-Star/Black-Hole Mergers
• Quasi-stationary states and the range of pair interactions
• Numerical overcooling in shocks
• EAGLE and Illustris-TNG predictions for resolved eROSITA X-ray observations of the circumgalactic medium around normal galaxies
• Observations of the Lyman series forest towards the redshift 7.1 quasar ULAS J1120+0641
• Evolution of dust extinction curves in galaxy simulation
• Galaxy Pairs in the Sloan Digital Sky Survey - X: Does gas content alter star formation rate enhancement in galaxy interactions?
• Optimized detection of shear peaks in weak lensing maps
• The dependence of tidal stripping efficiency on the satellite and host galaxy morphology
• The Sunyaev-Zel'dovich effects from a cosmological hydrodynamical simulation: large-scale properties and correlation with the soft X-ray signal
• $\nu \mathrm{CO}N\mathrm{CEPT}$: Cosmological neutrino simulations from the non-linear Boltzmann hierarchy
• The first galaxies: simulating their feedback-regulated assembly
• The first measurement of the quasar lifetime distribution
• Response function of the large-scale structure of the universe to the small scale inhomogeneities
• Modelling high redshift Lyman-alpha Emitters
• Thermal instabilities in cooling galactic coronae: fuelling star formation in galactic discs
• Impact of the non-Gaussian covariance of the weak lensing power spectrum and bispectrum on cosmological parameter estimation
• Quasar Ionization Front Lyα Emission in an Inhomogeneous Intergalactic Medium
• Advances in Constraining Intrinsic Alignment Models with Hydrodynamic Simulations
• Dark and luminous satellites of LMC-mass galaxies in the FIRE simulations
• Cold-Mode Accretion: Driving the Fundamental Mass-Metallicity Relation at z~2
• FAST: A Fully Asynchronous Split Time-Integrator for Self-Gravitating Fluid
• CO line ratios in molecular clouds: the impact of environment
• Structure of Dark Matter Halos in Warm Dark Matter models and in models with Long-Lived Charged Massive Particles
• Rotation rates, sizes, and star formation efficiencies of a representative population of simulated disc galaxies
• Baryonic effects on the matter bispectrum
• 2HOT: An Improved Parallel Hashed Oct-Tree N-Body Algorithm for Cosmological Simulation
• Formation of S0 galaxies through mergers. Evolution in the Tully-Fisher relation since $z\sim 1$
• Intermediate-Mass Black Hole Growth and Feedback in Dwarf Galaxies at High Redshifts
• Dark-ages Reionization & Galaxy Formation Simulation I: The dynamical lives of high redshift galaxies
• Globular Clusters in a Cosmological N-body Simulation
• Testing the effect of galactic feedback on the IGM at z ~ 6 with metal-line absorbers
• Self-Interacting Dark Matter and the Origin of Ultra-Diffuse Galaxies NGC1052-DF2 and -DF4
• Constrained Simulation of the Bullet Cluster
• Photon number conservation and the large-scale 21 cm power spectrum in semi-numerical models of reionization
• Global Gravitational Instabilities in Discs with Infall
• Robust covariance estimation of galaxy-galaxy weak lensing: validation and limitation of jackknife covariance
• Stellar orbits and the survival of metallicity gradients in simulated dwarf galaxies
• SWIFT: Using task-based parallelism, fully asynchronous communication, and graph partition-based domain decomposition for strong scaling on more than 100,000 cores
• The gas metallicity gradient and the star formation activity of disc galaxies
• Dynamical evolution of stars and gas of young embedded stellar sub-clusters
• 2D velocity fields of simulated interacting disc galaxies
• FOREVER22: galaxy formation in protocluster regions
• The dependence of the galaxy stellar-to-halo mass relation on galaxy morphology
• Hydrodynamic simulations with the Godunov SPH
• Constraining the second half of reionization with the Lyman-$\beta$ forest
• The Lyman alpha forest flux probability distribution at z>3
• Planetary Giant Impacts: Convergence of High-Resolution Simulations using Efficient Spherical Initial Conditions and SWIFT
• MUFASA: The assembly of the red sequence
• High-redshift JWST Observations and Primordial Non-Gaussianity
• Galactic Winds in Cosmological Simulations of the Circumgalactic Medium
• The spatial clustering of ROSAT All-Sky Survey Active Galactic Nuclei IV. More massive black holes reside in more massive dark matter halos
• How to add massive neutrinos to your $\Lambda$CDM simulation -- extending cosmology rescaling algorithms
• Origin of the high v_los feature in the Galactic bar
• Hydrodynamical simulations of galaxy clusters in dark energy cosmologies: II. c-M relation
• Lyman Break Galaxies at z = 4 - 6 in cosmological SPH Simulations
• Self-Similar Dynamical Relaxation of Dark Matter Halos in an Expanding Universe
• Clustering and redshift-space distortions in interacting dark energy cosmologies
• Osaka Feedback Model: Isolated Disk Galaxy Simulations
• Towards understanding the structure of voids in the cosmic web
• Constraining the Cosmic Baryon Distribution with Fast Radio Burst Foreground Mapping
• The Persistence of Large Scale Structures I: Primordial non-Gaussianity
• An accurate linear model for redshift space distortions in the void-galaxy correlation function
• The Stellar Mass Components of Galaxies: Comparing Semi-Analytical Models with Observation
• Computational issues in chemo-dynamical modelling of the formation and evolution of galaxies
• Duty Cycle and the Increasing Star Formation History of z>=6 Galaxies
• The First Billion Years of a Warm Dark Matter Universe
• Matter bispectrum of large-scale structure: Three-dimensional comparison between theoretical models and numerical simulations
• Quantifying distortions of the Lagrangian dark-matter mesh in cosmology
• Effect of radiative transfer on damped Lyman-alpha and Lyman limit systems in cosmological SPH simulations
• Machine Learning and Cosmological Simulations I: Semi-Analytical Models
• The assembly of dusty galaxies at $z\ge 4$: the build-up of stellar mass and its scaling relations with hints from early JWST data
• Deriving star formation histories from photometry using energy balance spectral energy distribution modelling
• Binary accretion rates: dependence on temperature and mass-ratio
• nIFTy Galaxy Cluster simulations IV: Quantifying the Influence of Baryons on Halo Properties
• On the relative bias of void tracers in the Dark Energy Survey
• Metal-line emission from the warm-hot intergalactic medium: I. Soft X-rays
• Does the CO-to-H2 conversion factor depend on the star formation rate?
• Galactic angular momentum in the IllustrisTNG simulation -- I. Connection to morphology, halo spin, and black hole mass
• Collisional stripping of planetary crusts
• Direct collapse black hole formation via high-velocity collisions of protogalaxies
• The simultaneous formation of cored, tangentially biased, and kinematically decoupled centers in massive early-type galaxies
• The impact of stellar and AGN feedback on halo-scale baryonic and dark matter accretion in the EAGLE simulations
• Anatomy of a buckling galactic bar
• Numerical convergence of hydrodynamical simulations of galaxy formation: the abundance and internal structure of galaxies and their cold dark matter haloes
• Impact of baryons on the cluster mass function and cosmological parameter determination
• Gravitational collapse and the thermal evolution of low-metallicity gas clouds in the early Universe
• Cosmic evolution of the CIV in high-resolution hydrodynamic simulations
• The kinetic SZ tomography with spectroscopic redshift surveys
• Time Delay Lens Modelling Challenge
• Cosmological constraints with weak lensing peak counts and second-order statistics in a large-field survey
• High redshift supermassive blackholes: accretion through cold flows
• Growing a `Cosmic Beast': Observations and Simulations of MACS J0717.5+3745
• COSMIC BIRTH: Efficient Bayesian Inference of the Evolving Cosmic Web from Galaxy Surveys
• Modeling Mid-Infrared Diagnostics of Obscured Quasars and Starbursts
• Extrasolar Planet Eccentricities from Scattering in the Presence of Residual Gas Disks
• AGN feedback, quiescence and CGM metal enrichment in early-type galaxies
• The Reionization of Carbon
• The earliest stars and their relics in the Milky Way
• Hot phase generation by supernovae: resolution, chemistry and thermal conduction
• A giant bar induced by a merger event at z=0.4?
• Rhapsody. II. Subhalo Properties and the Impact of Tidal Stripping From a Statistical Sample of Cluster-Size Halos
• Sustained super-Eddington accretion in high-redshift quasars
• Diffuse gas properties and stellar metallicities in cosmological simulations of disc galaxy formation
• Newborn spheroids at high redshift: when and how did the dominant, old stars in today's massive galaxies form?
• A detection of wobbling Brightest Cluster Galaxies within massive galaxy clusters
• An emulator for the Lyman-$\alpha$ forest in beyond-$\Lambda$CDM cosmologies
• Elucidating Galaxy Assembly Bias in SDSS
• Substructure and Scatter in the Mass-Temperature Relations of Simulated Clusters
• Detectability of the First Cosmic Explosions
• Cosmological constraints from Subaru weak lensing cluster counts
• Dust evolution in zoom-in cosmological simulations of galaxy formation
• Studying the properties of galaxy cluster morphology estimators
• Constraints on the redshift evolution of astrophysical feedback with Sunyaev-Zeldovich effect cross-correlations
• The Opacity of the Intergalactic Medium During Reionization: Resolving Small-Scale Structure
• On the signature of $z\sim 0.6$ superclusters and voids in the Integrated Sachs-Wolfe effect
• Sussing Merger Trees: the influence of the halo finder
• Splashback in galaxy clusters as a probe of cosmic expansion and gravity
• First detection of scale-dependent linear halo bias in $N$-body simulations with massive neutrinos
• Relative distribution of dark matter, gas, and stars around cosmic filaments in the IllustrisTNG simulation
• Next-to-leading resummation of cosmological perturbations via the Lagrangian picture: 2-loop correction in real and redshift spaces
• Environmental Effects on Real-Space and Redshift-Space Galaxy Clustering
• Measuring the mass distribution of voids with stacked weak lensing
• Gravitational redshifts from large-scale structure
• Linking gas and galaxies at high redshift: MUSE surveys the environments of six damped Lyman alpha galaxies at z~3
• The Impact of Different Physical Processes on the Statistics of Lyman-limit and Damped Lyman-alpha Absorbers
• Diagnosing galactic feedback with the line broadening in the low redshift Lyman-alpha forest
• The competition between confinement and ram pressure and its implications for galaxies in groups and clusters
• Solitons in the dark: non-linear structure formation with fuzzy dark matter
• Fossil stellar streams and their globular cluster populations in the E-MOSAICS simulations
• The MUSIC of Galaxy Clusters II: X-ray global properties and scaling relations
• Reducing distance errors for standard candles and standard sirens with weak-lensing shear and flexion maps
• Hierarchical clustering in chameleon $f(R)$ gravity
• Tomography of the intergalactic medium with Ly-alpha forests in close QSO pairs
• The impact of spectroscopic incompleteness in direct calibration of redshift distributions for weak lensing surveys
• Probing the stellar initial mass function with high-$z$ supernovae
• CLASH-VLT: Abell~S1063. Cluster assembly history and spectroscopic catalogue
• Cosmological baryon transfer in the SIMBA simulations
• The filling factor of intergalactic metals at redshift z=3
• The cosmic web of the Local Universe: cosmic variance, matter content and its relation to galaxy morphology
• Formation of the first star clusters and massive star binaries by fragmentation of filamentary primordial gas clouds
• Virial scaling of galaxies in clusters: bright to faint is cool to hot
• The better half -- Asymmetric star-formation due to ram pressure in the EAGLE simulations
• The early phases of galaxy clusters formation in IR: coupling hydrodynamical simulations with GRASIL3D
• The Persistent Percolation of Single-Stream Voids
• Sizes and ages of SDSS ellipticals: Comparison with hierarchical galaxy formation models
• Field Level Neural Network Emulator for Cosmological N-body Simulations
• Cosmology dependency of halo masses and concentrations in hydrodynamic simulations
• Sample variance in weak lensing: how many simulations are required?
• Efficient Computation of Galaxy Bias with Neutrinos and Other Relics
• Dark Energy Survey Year 3 Results: Exploiting small-scale information with lensing shear ratios
• Halo clustering and g_{NL}-type primordial non-Gaussianity
• The origin of the enhanced metallicity of satellite galaxies
• Power spectrum of halo intrinsic alignments in simulations
• AGN jet feedback on a moving mesh: gentle cluster heating by weak shocks and lobe disruption
• Measuring primordial non-Gaussianity through weak lensing peak counts
• The imprint of dissipation on the shapes of merger remnant LOSVDs
• The impact of numerical viscosity in SPH simulations of galaxy clusters
• Implications of hydrodynamical simulations for the interpretation of direct dark matter searches
• How well does CO emission measure the H${}_2$ mass of MCs?
• The journey of QSO haloes from z=6 to the present
• Neutral hydrogen in galaxy clusters: impact of AGN feedback and implications for intensity mapping
• Evolution of the cold gas properties of simulated post-starburst galaxies
• Unbiased Cosmology Inference from Biased Tracers using the EFT Likelihood
• The role of faint population III supernovae in forming CEMP stars in ultra-faint dwarf galaxies
• SIRIUS project. I. Star formation models for star-by-star simulations of star clusters and galaxy formation
• Size matters: the non-universal density profile of subhaloes in SPH simulations and implications for the Milky Way's dSphs
• The mass density field in simulated non-Gaussian scenarios
• Simulations of the merging galaxy cluster Abell 3376
• Probing the end of reionization with the near-zones of z > 6 QSOs
• Clustering of quasars in the First Year of the SDSS-IV eBOSS survey: Interpretation and halo occupation distribution
• Dark Energy Survey Year 1 Results: Calibration of redMaGiC Redshift Distributions in DES and SDSS from Cross-Correlations
• Recycled stellar ejecta as fuel for star formation and implications for the origin of the galaxy mass-metallicity relation
• Tools for computing the AGN feedback: radio-loudness distribution and the kinetic luminosity function
• A new Measurement of the Intergalactic Temperature at $z\sim 2.55-2.95$
• The origin of the 'blue tilt' of globular cluster populations in the E-MOSAICS simulations
• Suite of Hydrodynamical Simulations for the Lyman-Alpha Forest with Massive Neutrinos
• Numerical Simulations of the Lyman-alpha forest - A comparison of Gadget-2 and Enzo
• The dark matter assembly of the Local Group in constrained cosmological simulations of a LambdaCDM universe
• Optimal linear reconstruction of dark matter from halo catalogs
• Dark-matter decays and Milky Way satellite galaxies
• Galaxies going MAD: The Galaxy-Finder Comparison Project
• Characterizing the formation history of Milky Way-like stellar haloes with model emulators
• The little things matter: relating the abundance of ultrafaint satellites to the hosts' assembly history
• Cosmological Information in the Marked Power Spectrum of the Galaxy Field
• PkANN - I. Non-linear matter power spectrum interpolation through artificial neural networks
• Radio Halos From Simulations And Hadronic Models II: The Scaling Relations of Radio Halos
• A Fast Route to Non-Linear Clustering Statistics in Modified Gravity Theories
• On the galaxy-halo connection in the EAGLE simulation
• Galaxy properties and the cosmic web in simulations
• Ultra-Light Axion Dark Matter and its impacts on dark halo structure in $N$-body simulation
• Signatures of the M31-M32 Galactic Collision
• Dynamical cluster disruption and its implications for multiple population models in the E-MOSAICS simulations
• Ricci focusing, shearing, and the expansion rate in an almost homogeneous Universe
• What drives the evolution of gas kinematics in star-forming galaxies?
• An Evolutionary Model For Submillimeter Galaxies
• Joint halo mass function for modified gravity and massive neutrinos I: simulations and cosmological forecasts
• Winds of change: reionization by starburst galaxies
• TangoSIDM: Tantalizing models of Self-Interacting Dark Matter
• Massive Milky Way Satellites in Cold and Warm Dark Matter: Dependence on Cosmology
• Comparing galaxy formation in the L-GALAXIES semi-analytical model and the IllustrisTNG simulations
• Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
• A Hydrodynamical Solution for the "Twin-Tailed" Colliding Galaxy Cluster "El Gordo"
• Cosmological Implications of a Stellar Initial Mass Function that Varies with the Jeans Mass in Galaxies
• INFERNO: Galactic winds in dwarf galaxies with star-by-star simulations including runaway stars
• Testing the reliability of weak lensing cluster detections
• The Formation of Galaxies Hosting z~6 Quasars
• On the local variation of the Hubble constant
• Stellar Property Statistics of Massive Halos from Cosmological Hydrodynamics Simulations: Common Kernel Shapes
• The Nature of CO Emission From z~6 Quasars
• Local stochastic non-Gaussianity and N-body simulations
• GenetIC -- a new initial conditions generator to support genetically modified zoom simulations
• GRUMPY: a simple framework for realistic forward-modelling of dwarf galaxies
• Cosmological constraints from the convergence 1-point probability distribution
• A needle in a haystack? Catching Pop III stars in the Epoch of Reionization: I. Pop III star forming environments
• What Do Dark Matter Properties Tell Us About Their Mass Assembly Histories?
• Enrichment of the hot intracluster medium: numerical simulations
• Probing the metallicity and ionization state of the circumgalactic medium at z~6 and beyond with OI absorption
• Fully relativistic treatment of light neutrinos in $N$-body simulations
• Separate Universe Simulations with IllustrisTNG: baryonic effects on power spectrum responses and higher-order statistics
• Towards optimal cosmological parameter recovery from compressed bispectrum statistics
• A fast recursive coordinate bisection tree for neighbour search and gravity
• Predicting the density profiles of the first halos
• Filament profiles from WISExSCOS galaxies as probes of the impact of environmental effects
• The Halo Occupation Distribution of Active Galactic Nuclei
• On the effect of non-Gaussian lensing deflections on CMB lensing measurements
• Perturbation theory approach for the power spectrum: from dark matter in real space to massive haloes in redshift space
• On the Discrepancy between Theoretical and X-Ray Concentration-Mass Relations for Galaxy Clusters
• A comparison of black hole growth in galaxy mergers with Gasoline and Ramses
• Dependence of $X_{\mathrm{CO}}$ on metallicity, intensity, and spatial scale in a self-regulated interstellar medium
• Energy ejection in the collapse of a cold spherical self-gravitating cloud
• Robust Field-level Likelihood-free Inference with Galaxies
• First Light: exploring the Spectra of High-Redshift Galaxies in the Renaissance Simulations
• On the dissection of degenerate cosmologies with machine learning
• How fast do young star clusters expel their natal gas?: Estimating the upper limit of the gas expulsion time-scale
• Properties of the diffuse X-ray background in a high-resolution hydrodynamical simulation
• A closer look at using quasar near-zones as a probe of neutral hydrogen in the intergalactic medium
• Annihilation Signatures of Hidden Sector Dark Matter Within Early-Forming Microhalos
• The visibility of Lyman Alpha Emitters: constraining reionization, ionizing photons and dust
• Momentum-driven Winds from Radiatively Efficient Black Hole Accretion and Their Impact on Galaxies
• Sample variance and Lyman-alpha forest transmission statistics
• Gamma-rays from dark matter annihilations strongly constrain the substructure in halos
• Cosmology with Equivalence Principle Breaking in the Dark Sector
• Flybys, orbits, splashback: subhalos and the importance of the halo boundary
• The highest-speed local dark matter particles come from the Large Magellanic Cloud
• Statistics of cosmic density profiles from perturbation theory
• The large-scale environment from cosmological simulations I: The baryonic cosmic web
• The evolution of the oxygen abundance gradients in star-forming galaxies in the EAGLE simulations
• Dwarf spheroidal satellites of the Milky Way from dark matter free tidal dwarf galaxy progenitors: maps of orbits
• Quijote-PNG: Simulations of primordial non-Gaussianity and the information content of the matter field power spectrum and bispectrum
• Studying the WHIM with Gamma Ray Bursts
• Accretion Does Not Drive the Turbulence in Galactic Disks
• Primordial non-Gaussianities in the Intergalactic Medium
• Structure formation simulations with momentum exchange: alleviating tensions between high-redshift and low-redshift cosmological probes
• Is the Concentration of Dark Matter Halos at Virialization Universal ?
• Einasto Profiles and the Dark Matter Power Spectrum
• Clues on void evolution III: Structure and dynamics in void shells
• The Growth and Enrichment of the Intragroup Gas
• Stellar orbits in cosmological galaxy simulations: the connection to formation history and line-of-sight kinematics
• An interpretable machine learning framework for dark matter halo formation
• A Genetic Approach to the History of the Magellanic Clouds
• Molecular hydrogen regulated star formation in cosmological SPH simulations
• Dwarf Galaxies with Ionizing Radiation Feedback. I: Escape of Ionizing Photons
• The effect of baryons in the cosmological lensing PDFs
• Relativistic Interpretation of Newtonian Simulations for Cosmic Structure Formation
• The Line-of-Sight Proximity Effect and the Mass of Quasar Host Halos
• Effects of Ultraviolet Background and Local Stellar Radiation on the H_I Column Density Distribution
• Precision modelling of the matter power spectrum in a Planck-like Universe
• Exploring 21cm - Lyman Alpha emitter synergies for SKA
• Evolution of a disc-planet system with a binary companion on an inclined orbit
• Gaseous infall triggering starbursts in simulated dwarf galaxies
• Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations
• The Distribution of Satellites Around Central Galaxies in a Cosmological Hydrodynamical Simulation
• Modelling large-scale halo bias using the bispectrum
• Fast generation of ensembles of cosmological N-body simulations via mode-resampling
• On the cross-section of Dark Matter using substructure infall into galaxy clusters
• Simulations of Baryon Acoustic Oscillations I: Growth of Large-Scale Density Fluctuations
• Signatures of star cluster formation by cold collapse
• Simulating magnetic fields in the Antennae galaxies
• The merging cluster Abell 1758 revisited: multi-wavelength observations and numerical simulations
• The diverse evolutionary pathways of post-starburst galaxies
• Dark matter voids in the SDSS galaxy survey
• Metals in the z~3 intergalactic medium: results from an ultra-high signal-to-noise ratio UVES quasar spectrum
• Large scale structure simulations of inhomogeneous LTB void models
• The Mice at play in the CALIFA survey: A case study of a gas-rich major merger between first passage and coalescence
• Visualizing Astronomical Data with Blender
• Satellite dwarf galaxies: Stripped but not quenched
• Fingerprints of the initial conditions on the density profiles of cold and warm dark matter haloes
• Disk-stability constraints on the number of arms in spiral galaxies
• Missing baryons traced by the galaxy luminosity density in the large-scale WHIM filaments
• Dark matter annihilation radiation in hydrodynamic simulations of Milky Way haloes
• Dark Energy Survey Year 3 results: Magnification modeling and impact on cosmological constraints from galaxy clustering and galaxy-galaxy lensing
• Global simulations of self-gravitating magnetized protoplanetary disks
• Cosmology Inference from Biased Tracers using the EFT-based Likelihood
• Faint rapid red transients from Neutron star -- CO white-dwarf mergers
• Simulations of the formation and evolution of isolated dwarf galaxies - II. Angular momentum as a second parameter
• Astraeus V: The emergence and evolution of metallicity scaling relations during the Epoch of Reionization
• Blandford-Znajek jets in galaxy formation simulations: exploring the diversity of outflows produced by spin-driven AGN jets in Seyfert galaxies
• Faint-end Quasar Luminosity Functions from Cosmological Hydrodynamic Simulations
• The fate of the gaseous disks of galaxies that fall into clusters
• Simulating the effect of high column density absorbers on the one-dimensional Lyman-alpha forest flux power spectrum
• Splotch: Visualizing Cosmological Simulations
• An uncertainty principle for star formation -- III. The characteristic emission time-scales of star formation rate tracers
• The challenge of simulating the star cluster population of dwarf galaxies with resolved interstellar medium
• The origin of the red sequence galaxy population in the EAGLE simulation
• An application of machine learning techniques to galaxy cluster mass estimation using the MACSIS simulations
• The onset of star formation in primordial haloes
• The Host Halos of OI Absorbers in the Reionization Epoch
• The life and death of cosmic voids
• VINE -- A numerical code for simulating astrophysical systems using particles II: Implementation and performance characteristics
• Halo Histories vs. Galaxy Properties at z=0, I: The Quenching of Star Formation
• Dark Energy Survey Year 1 results: Validation of weak lensing cluster member contamination estimates from P(z) decomposition
• Dynamics of barred galaxies: effects of disk height
• Smoothed particle hydrodynamics simulations of gas and dust mixtures
• Properties of Submillimeter Galaxies in a Semi-analytic Model using the "Count Matching" Approach: Application to the ECDF-S
• On Modeling and Measuring the Temperature of the z~5 IGM
• The integrated 3-point correlation function of cosmic shear
• Infalling clouds on to supermassive black hole binaries - II. Binary evolution and the final parsec problem
• Relativistic distortions in the large-scale clustering of SDSS-III BOSS CMASS galaxies
• The scatter in the radial profiles of X-ray luminous galaxy clusters as diagnostic of the thermodynamical state of the ICM
• An Investigation of intra-cluster light evolution using cosmological hydro-dynamical simulations
• Streams on FIRE: Populations of Detectable Stellar Streams in the Milky Way and FIRE
• ALMA will determine the spectroscopic redshift z>8 with FIR [O III] emission lines
• Exploring the Thermal State of the Low-Density Intergalactic Medium at z=3 with an Ultra-High Signal-to-Noise QSO Spectrum
• The effect of Warm Dark Matter on galaxy properties: constraints from the stellar mass function and the Tully-Fisher relation
• A Halo Expansion (HEX) Technique for Approximating Simulated Dark Matter Haloes
• The specific star formation rate function at different mass scales and quenching: A comparison between cosmological models and SDSS
• The curiously circular orbit of Kepler-16b
• Fast Estimation of Gravitational and Primordial Bispectra in Large Scale Structures
• Observational Properties of Simulated Galaxies in Overdense and Average Regions at High Redshifts z= 6-12
• An Efficient Fokker-Planck Solver and its Application to Stochastic Particle Acceleration in Galaxy Clusters
• RADAMESH: Cosmological Radiative Transfer for Adaptive Mesh Refinement Simulations
• A forming, dust enshrouded disk at z=0.43: the first example of a late type disk rebuilt after a major merger?
• Predictions for anisotropic X-ray signatures in the circumgalactic medium: imprints of supermassive black hole driven outflows
• Velocity bias in the distribution of dark matter halos
• Infrared emission of $z\sim 6$ galaxies: AGN imprints
• The Cluster-EAGLE project: velocity bias and the velocity dispersion - mass relation of cluster galaxies
• General framework for cosmological dark matter bounds using $N$-body simulations
• General relativistic weak-field limit and Newtonian N-body simulations
• Kelvin-Helmholtz instabilities in Smoothed Particle Hydrodynamics
• Origami constraints on the initial-conditions arrangement of dark-matter caustics and streams
• Dark Matter Halo Profiles in Scale-Free Cosmologies
• Multicomponent and Variable Velocity Galactic Outflow in Cosmological Hydrodynamic Simulations
• Satellite Alignment: I. Distribution of Substructures and Their Dependence On Assembly History From N-Body Simulations
• Magellanic satellites in $\Lambda$CDM cosmological hydrodynamical simulations of the Local Group
• The impact of AGN feedback on the 1D power spectra from the Ly$\alpha$ forest using the Horizon-AGN suite of simulations
• The one-loop matter bispectrum as a probe of gravity and dark energy
• Modeling color-dependent galaxy clustering in cosmological simulations
• The first Super Massive Black Holes: indications from models for future observations
• The Bacco Simulation Project: Bacco Hybrid Lagrangian Bias Expansion Model in Redshift Space
• SUNGLASS: A new weak lensing simulation pipeline
• Subhaloes gone Notts: Spin across subhaloes and finders
• Were progenitors of local L* galaxies Lyman-alpha emitters at high redshift?
• The AGORA High-resolution Galaxy Simulations Comparison Project. III: Cosmological zoom-in simulation of a Milky Way-mass halo
• The origin of compact galaxies with anomalously high black hole masses
• Mass calibration of distant SPT galaxy clusters through expanded weak lensing follow-up observations with HST, VLT & Gemini-South
• Forecasts for the WFIRST High Latitude Survey using the BlueTides Simulation
• NGC 4993, the shell galaxy host of GW170817: constraints on the recent galactic merger
• Testing standard perturbation theory and the Eulerian local biasing scheme against N-body simulations
• Baryon effects on void statistics in the EAGLE simulation
• Upper Limit on the Milky Way Mass from the Orbit of the Sagittarius Dwarf Satellite
• Cosmology with clustering anisotropies: disentangling dynamic and geometric distortions in galaxy redshift surveys
• The host galaxies of long-duration GRBs in a cosmological hierarchical scenario
• The effect of massive neutrinos on the Sunyaev-Zeldovich and X-ray observables of galaxy clusters
• Does small scale structure significantly affect cosmological dynamics?
• Galaxy-galaxy weak-lensing measurement from SDSS: II. host halo properties of galaxy groups
• The Morphology-Density-Relation: Impact on the Satellite Fraction
• Tidal Disruptions of Stars by Binary Black Holes: Modifying the Spin Magnitudes and Directions of LIGO Sources in Dense Stellar Environments
• Surviving companions of Type Ia supernovae: theory and observations
• Can Early Dark Energy be Detected in Non-Linear Structure?
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for Galaxy Clustering Measurements
• A fast particle-mesh simulation of non-linear cosmological structure formation with massive neutrinos
• Dark Energy Survey Year 3 results: cosmology from combined galaxy clustering and lensing -- validation on cosmological simulations
• The Density Structure of Simulated Stellar Streams
• The roles of stellar feedback and galactic environment in star forming molecular clouds
• Signatures of the Many Supermassive Black Hole Mergers in a Cosmologically Forming Massive Early-Type Galaxy
• Hierarchical Galaxy Growth and Scatter in the Stellar Mass - Halo Mass Relation
• The FRB20190520B Sightline Intersects Foreground Galaxy Clusters
• The nature of assembly bias - II. Halo spin
• The probability of galaxy-galaxy strong lensing events in hydrodynamical simulations of galaxy clusters
• Density distribution of the cosmological matter field
• An alternative origin for debris rings of planetesimals
• The rotation of surviving companion stars after type Ia supernova explosions in the WD+MS scenario
• The resonant nature of tidal stirring of disky dwarf galaxies orbiting the Milky Way
• The Structure of Dissipative Dark Matter Halos
• Young star cluster populations in the E-MOSAICS simulations
• Constraints on dark radiation from cosmological probes
• The Signature of Large Scale Structures on the Very High Energy Gamma-Ray Sky
• Persistent homology of the cosmic web. I: Hierarchical topology in $\Lambda$CDM cosmologies
• The abundance and physical properties of O VII and O VIII X-ray absorption systems in the EAGLE simulations
• Constraining the Mass-Richness Relationship of redMaPPer Clusters with Angular Clustering
• Dynamic Monte Carlo radiation transfer in SPH. Radiation pressure force implementation
• Evolution of LMC/M33-mass dwarf galaxies in the EAGLE simulation
• The Non-Linear Matter Power Spectrum in Warm Dark Matter Cosmologies
• Dual Effects of Ram Pressure on Star Formation in Multi-phase Disk Galaxies with Strong Stellar Feedback
• Theoretical predictions for the effect of nebular emission on the broad band photometry of high-redshift galaxies
• Environmental Influences on the Morphology and Dynamics of Group Size Haloes
• Dark Matter in the Local Universe
• Bayesian forward modelling of cosmic shear data
• Optimal Weighting in Galaxy Surveys: Application to Redshift-Space Distortions
• PANDA: Extreme Scale Parallel K-Nearest Neighbor on Distributed Architectures
• The merger history of the complex cluster Abell 1758: a combined weak lensing and spectroscopic view
• Bias deconstructed: Unravelling the scale dependence of halo bias using real space measurements
• ERGO-ML I: Inferring the assembly histories of IllustrisTNG galaxies from integral observable properties via invertible neural networks
• Predicting the amount of hydrogen stripped by the supernova explosion for SN 2002cx-like SNe Ia
• From Discs to Bulges: effect of mergers on the morphology of galaxies
• Painting halos from cosmic density fields of dark matter with physically motivated neural networks
• Is there enough star formation in simulated protoclusters?
• The diversity of rotation curves of simulated galaxies with cusps and cores
• Voronoi volume function: A new probe of cosmology and galaxy evolution
• Pericentric passage-driven star formation in satellite galaxies and their hosts: CLUES from Local Group simulations
• The [CII]--SFR correlation in dwarf galaxies across cosmic time
• The diverse formation histories of simulated disc galaxies
• Feedback-Driven Evolution of the Far-Infrared Spectral Energy Distributions of Luminous and Ultraluminous Infrared Galaxies
• Impact of filaments on galaxy formation in their residing dark matter haloes
• Dark Matter Gravitational Clustering With a Long-Range Scalar Interaction
• Deadly dark matter cusps vs faint and extended star clusters: Eridanus II and Andromeda XXV
• Simulations of galaxy formation with radiative transfer: Hydrogen reionization and radiative feedback
• Galactic ménage à trois: Simulating magnetic fields in colliding galaxies
• Simulating Momentum Exchange in the Dark Sector
• Rhapsody-G simulations: galaxy clusters as baryonic closed boxes and the covariance between hot gas and galaxies
• A New Channel for the Formation of Kinematically Decoupled Cores in Early-type galaxies
• Revealing the properties of void galaxies and their assembly using the EAGLE simulation
• The Overlooked Potential of Generalized Linear Models in Astronomy - I: Binomial Regression
• Probing the Intergalactic Medium with Ly$\alpha$ and 21 cm Fluctuations
• Reproducing the Universe: a comparison between the EAGLE simulations and the nearby DustPedia galaxy sample
• Pre-processing, group accretion and the orbital trajectories of associated subhaloes
• A Candidate Dual AGN in a Double-peaked Emission-line Galaxy with Precessing Radio Jets
• Light cone anisotropy in 21 cm signal from the epoch of reionization
• Origin of Cosmic Chemical Abundances
• Chandra Survey of Nearby Highly Inclined Disc Galaxies - III: Comparison with Hydrodynamical Simulations of Circumgalactic Coronae
• Supermassive black hole ancestors
• Dynamical mass inference of galaxy clusters with neural flows
• Neutral CGM as damped Lyα absorbers at high redshift
• Sub-millimetre galaxies in cosmological hydrodynamic simulations: Source number counts and the spatial clustering
• The Covariance of Squeezed Bispectrum Configurations
• Supermassive Black Holes and Their Environments
• Growth of First Galaxies: Impacts of Star Formation and Stellar Feedback
• Impact of Supernova feedback on the Tully-Fisher relation
• Physical Correlations of the Scatter between Galaxy Mass, Stellar Content, and Halo Mass
• Cosmological Simulations of Multi-Component Cold Dark Matter
• Convergence properties of halo merger trees; halo and substructure merger rates across cosmic history
• Noise reduction for weak lensing mass mapping: An application of generative adversarial networks to Subaru Hyper Suprime-Cam first-year data
• The offsets between galaxies and their dark matter in Lambda-CDM
• Constraints on Galactic Intermediate Mass Black Holes
• Giant Radio Galaxies: I. Intergalactic Barometers
• The phase-space structure of tidally stripped halos
• The impact of spurious collisional heating on the morphological evolution of simulated galactic discs
• Spherical collapse, formation hysteresis and the deeply non-linear cosmological power spectrum
• Panchromatic SED modelling of spatially-resolved galaxies
• Comparing Fully General Relativistic and Newtonian Calculations of Structure Formation
• The impact of feedback and the hot halo on the rates of gas accretion onto galaxies
• The Inhomogeneous Reionization Times of Present-day Galaxies
• Spontaneous generation of bending waves in isolated Milky Way-like discs
• Protostellar collapse and fragmentation using an MHD GADGET
• The effects of ram-pressure stripping on the internal kinematics of simulated spiral galaxies
• Modelling supermassive black hole growth: towards an improved sub-grid prescription
• He II Proximity Effect and the Lifetime of Quasars
• Athena X-IFU synthetic observations of galaxy clusters to probe the chemical enrichment of the Universe
• The build-up of pseudobulges in a hierarchical universe
• Assembly bias in the local PNG halo bias and its implication for $f_{\mathrm{NL}}$ constraints
• Perturbation theory for modeling galaxy bias: validation with simulations of the Dark Energy Survey
• Climbing Halo Merger Trees with TreeFrog
• A journey from the outskirts to the cores of groups I: Color- and mass-segregation in 20K-zCOSMOS groups
• The evolution of galaxy metallicity scaling relations in cosmological hydrodynamical simulations
• Tidal origin of spiral arms in galaxies orbiting a cluster
• The velocity shear and vorticity across redshifts and non-linear scales
• Hydrodynamic Effects in the Symmetron and $f(R)$-gravity Models
• Radial profile and log-normal fluctuations of intra-cluster medium as an origin of systematic bias of spectroscopic temperature
• Reduced atmospheres of post-impact worlds: The early Earth
• CALIFA reveals Prolate Rotation in Massive Early-type Galaxies: A Polar Galaxy Merger Origin?
• The Radial Orbit Instability in Collisionless N-Body Simulations
• The Secondary Spin Bias of Dark Matter Haloes
• The Sloan Great Wall. Rich clusters
• The Cosmic Evolution of the IMF Under the Jeans Conjecture with Implications for Bottom-Heavy Ellipticals
• Initial Conditions for Idealised Clusters Mergers, simulating El Gordo
• WIMP DM and first stars: suppression of fragmentation in primordial star formation
• Hunting high and low: Disentangling primordial and late-time non-Gaussianity with cosmic densities in spheres
• SimpleX2: radiative transfer on an unstructured, dynamic grid
• JWST high-z galaxy constraints on warm and cold dark matter models
• The halo mass function in interacting Dark Energy models
• The Three Hundred Project: The influence of environment on simulated galaxy properties
• Constraints on the Nature of CID-42: Recoil Kick or Supermassive Black Hole Pair?
• Strong orientation dependence of surface mass density profiles of dark haloes at large scales
• The stellar metallicity gradients in galaxy discs in a cosmological scenario
• Effects of metal enrichment and metal cooling in galaxy growth and cosmic star formation history
• The Effects of Boxy/Peanut Bulges on Galaxy Models
• Inhomogeneous HeII reionization in Hydrodynamic Simulations
• Quenching and morphological evolution due to circumgalactic gas expulsion in a simulated galaxy with a controlled assembly history
• Detection of missing baryons in galaxy groups with kinetic Sunyaev-Zel'dovich effect
• Satellite Accretion Onto Massive Galaxies With Central Black Holes
• DES Y1 Results: Validating cosmological parameter estimation using simulated Dark Energy Surveys
• Offset between X-ray and optical centers in clusters of galaxies: connecting eROSITA data and simulations
• Disentangling the dark matter halo from the stellar halo
• Entropy of gas and dark matter in galaxy clusters
• Relativistic initial conditions for N-body simulations
• On the genealogy of the Orphan Stream
• Symplectic integrators in the shearing sheet
• Measuring primordial non-Gaussianity with weak-lensing surveys
• Stellar Encounters with Massive Star-Disk Systems
• Evidence for Short $\sim 1$ Myr Lifetimes from the He II Proximity Zones of $z\sim 4$ Quasars
• The fate of the Antennae galaxies
• A study of AGN and supernova feedback in simulations of isolated and merging disc galaxies
• A Fully Self-Consistent Cosmological Simulation Pipeline for Interacting Dark Energy Models
• Effects of the initial conditions on cosmological $N$-body simulations
• Ring Galaxies in the EAGLE Hydrodynamical Simulations
• An optimum time-stepping scheme for N-body simulations
• Orbital evidences for dark-matter-free Milky Way dwarf spheroidal galaxies
• Relating the structure of dark matter halos to their assembly and environment
• Lyman-$\alpha$ forest constraints on interacting dark sectors
• Code Comparison in Galaxy Scale Simulations with Resolved Supernova Feedback: Lagrangian vs. Eulerian Methods
• Spiral-Induced Star Formation in the Outer Disks of Galaxies
• The impact of correlated projections on weak lensing cluster counts
• Modeling for Stellar Feedback in Galaxy Formation Simulations
• Simulations of XUV Disks with a Star Formation Density Threshold
• Reducing sample variance: halo biasing, non-linearity and stochasticity
• Detecting Lyman Alpha Emitters in the Sub-millimeter
• Loops formed by tidal tails as fossil records of a major merger
• Missing cosmic metals revealed by X-ray absorption towards distant sources
• Priors on Lagrangian bias parameters from galaxy formation modelling
• Fast full N-body simulations of generic modified gravity: conformal coupling models
• Integrated Perturbation Theory and One-loop Power Spectra of Biased Tracers
• LyMAS: Predicting Large-Scale Lyman-alpha Forest Statistics from the Dark Matter Density Field
• Constraints on mixed dark matter from anomalous strong lens systems
• Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
• Numerical Simulations of Hot Halo Gas in Galaxy Mergers
• Towards a general parametrization of the warm dark matter halo mass function
• Can magnetized turbulence set the mass scale of stars?
• SCUBA-2 Ultra Deep Imaging Eao Survey (Studies) III: Multi-wavelength properties, luminosity functions and preliminary source catalog of 450-$\mu$m-selected galaxies
• Deconstructing Thermal Sunyaev-Zel'dovich - Gravitational Lensing Cross-Correlations: Implications for the Intracluster Medium
• Modeling asteroid collisions and impact processes
• Atmosphere loss in planet-planet collisions
• Constraint of Void Bias on Primordial non-Gaussianity
• Hydrostatic mass estimates of massive galaxy clusters: a study with varying hydrodynamics flavours and non-thermal pressure support
• Dynamic Localised Turbulent Diffusion and its Impact on the Galactic Ecosystem
• Adaptive optics imaging and optical spectroscopy of a multiple merger in a luminous infrared galaxy
• Galaxy Satellites and the Weak Equivalence Principle
• BlueTides simulation: establishing black hole-galaxy relations at high-redshift
• Cosmological constraints from galaxy clustering in the presence of massive neutrinos
• The global stability of M33: still a puzzle
• Large 21 cm signals from AGN-dominated reionization
• SPHYNX: an accurate density-based SPH method for astrophysical applications
• Tidally Induced Offset Disks in Magellanic Spiral Galaxies
• Metal-line emission from the warm-hot intergalactic medium: II. Ultraviolet
• The Formation of Rapidly Rotating Black Holes in High Mass X-ray Binaries
• Observations of metals in the $z\approx 3.5$ intergalactic medium and comparison to the EAGLE simulations
• Physical Properties of UDF12 Galaxies in Cosmological simulations
• Streams Going Notts: The tidal debris finder comparison project
• Deep Realistic Extragalactic Model (DREaM) Galaxy Catalogs: Predictions for a Roman Ultra-Deep Field
• The High Fraction of Thin Disk Galaxies Continues to Challenge ΛCDM Cosmology
• Properties of fossil groups in cosmological simulations and galaxy formation models
• Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency
• The impact of magnetic fields on cosmological galaxy mergers. I: Reshaping gas and stellar discs
• Lyman-α Forest and Cosmic Weak Lensing in a Warm Dark Matter Universe
• Intensity mapping with neutral hydrogen and the Hidden Valley simulations
• Constraints on warm dark matter from weak lensing in anomalous quadruple lenses
• Dark Energy Survey Year 1 Results: the lensing imprint of cosmic voids on the Cosmic Microwave Background
• Adiabatic scaling relations of galaxy clusters
• Pre-supernova feedback sets the star cluster mass function to a power law and reduces the cluster formation efficiency
• The Violent Youth of Bright and Massive Cluster Galaxies and their Maturation over 7 Billion Years
• The broadening of Lyman-alpha forest absorption lines
• Extragalactic archaeology with the C, N, and O chemical abundances
• The vertical structure of gaseous galaxy discs in cold dark matter halos
• Nonparametric 3D map of the IGM using the Lyman-alpha forest
• EvoL: The new Padova T-SPH parallel code for cosmological simulations - I. Basic code: gravity and hydrodynamics
• Magnetic buoyancy in simulated galactic discs with a realistic circum galactic medium
• Quenching and the UVJ diagram in the SIMBA cosmological simulation
• Measurement of the dark matter velocity anisotropy in galaxy clusters
• The Mixing and Transport Properties of the Intra Cluster Medium: a numerical study using tracers particles
• Sussing Merger Trees : The Impact of Halo Merger Trees on Galaxy Properties in a Semi-Analytic Model
• Magnetic fields in the formation of the first stars.--II Results
• An evolving and mass dependent ${\sigma }_{\text{sSFR}}$-${\mathrm{M}}_{\star }$ relation for galaxies
• Connecting the structure of dark matter haloes to the primordial power spectrum
• Simulating tidal streams in a high resolution dark matter halo
• The effect of early radiation in N-body simulations of cosmic structure formation
• Effects of Quasar Feedback in Galaxy Groups
• Line-of-sight velocity distributions of elliptical galaxies from collisionless mergers
• Remarks on mechanical approach to observable Universe
• The MillenniumTNG Project: Refining the one-halo model of red and blue galaxies at different redshifts
• Clumpy high-z galaxies as a testbed for feedback-regulated galaxy formation
• Merger Signatures in the Dynamics of Star-forming Gas
• N-body simulations of dark matter with frequent self-interactions
• How Unusual is the Milky Way's Assembly History?
• Lyman-αabsorption beyond the disk of simulated spiral galaxies
• A Redefinition of the Halo Boundary Leads to a Simple yet Accurate Halo Model of Large Scale Structure
• A measurement of galaxy halo mass from the surrounding HI Lyα absorption
• Kinematics of Simulated Galaxies II: Probing the Stellar Kinematics of Galaxies out to Large Radii
• Dark Matter Halo Environment for Primordial Star Formation
• A Zeldovich reconstruction method for measuring redshift space distortions using cosmic voids
• Modeling the Lyman-alpha Forest in Collisionless Simulations
• Infalling clouds onto super-massive black hole binaries - I. Formation of discs, accretion and gas dynamics
• Systematic errors in the measurement of neutrino masses due to baryonic feedback processes: Prospects for stage IV lensing surveys
• Nonspherical similarity solutions for dark halo formation
• Kinetic Sunyaev--Zel'dovich effect in rotating galaxy clusters from MUSIC simulations
• Numerical simulations of dwarf galaxy merger trees
• Beware of Fake $\nu$s: The Effect of Massive Neutrinos on the Nonlinear Evolution of Cosmic Structure
• Massive disc galaxies in cosmological hydrodynamical simulations are too dark matter-dominated
• Hydrodynamical simulations of galaxy clusters in dark energy cosmologies: I. general properties
• Brightest Cluster Galaxies: the centre can(not?) hold
• A scaling relation between merger rate of galaxies and their close pair count
• On the evolution of gas clouds exposed to AGN radiation. I. Three-dimensional radiation hydrodynamic simulations
• Testing gravity using the growth of large scale structure in the Universe
• Modeling the JWST high-redshift galaxies with a general formation scenario and the consistency with the $\Lambda$CDM model
• A Novel Approach to Visualizing Dark Matter Simulations
• Testing the Accuracy of Halo Occupation Distribution Modelling using Hydrodynamic Simulations
• Simulating intergalactic gas for DESI-like small scale Lymanα forest observations
• Stellar Disks in Aquarius Dark Matter Haloes
• DISPATCH: A Numerical Simulation Framework for the Exa-scale Era. I. Fundamentals
• Constraining the primordial magnetic field with dwarf galaxy simulations
• Numerical Simulations of Turbulent Molecular Clouds Regulated by Radiation Feedback Forces II: Radiation-Gas Interactions and Outflows
• Voids in cosmological simulations over cosmic time
• The IMF as a function of supersonic turbulence
• Cosmological exploitation of cosmic void statistics - New numerical tools in the CosmoBolognaLib to extract cosmological constraints from the void size function
• On the Stability of Satellite Planes I: Effects of Mass, Velocity, Halo Shape and Alignment
• Reconstructing cosmological initial conditions from galaxy peculiar velocities. III. Constrained simulations
• Likelihood Non-Gaussianity in Large-Scale Structure Analyses
• Spin alignment of dark matter haloes in the shells of the largest voids
• Shocks in the Stacked Sunyaev-Zel'dovich Profiles of Clusters II: Measurements from SPT-SZ + Planck Compton-y Map
• The impact of environment and mergers on the HI content of galaxies in hydrodynamic simulations
• The resolution bias: low resolution feedback simulations are better at destroying galaxies
• The role of feedback in accretion on Low Luminosity AGN: Sgr A* case study
• The Cosmological Simulation Code OpenGadget3 -- Implementation of Meshless Finite Mass
• Radiative properties of the first galaxies: rapid transition between blue and red
• Metals in the circumgalactic medium are out of ionization equilibrium due to fluctuating active galactic nuclei
• The impact of baryonic potentials on the gravothermal evolution of self-interacting dark matter haloes
• On the road to percent accuracy III: non-linear reaction of the matter power spectrum to massive neutrinos
• Cosmological N-Body Simulations with a Large-Scale Tidal Field
• On the effect of galactic outflows in cosmological simulations of disc galaxies
• Dark Matter Halos in Interacting Dark Energy Models: Formation History, Density Profile, Spin and Shape
• Convergence of AMR and SPH simulations - I. Hydrodynamical resolution and convergence tests
• Probing Galaxy Assembly Bias in BOSS Galaxies Using Void Probabilities
• Prospects for detecting the 21cm forest from the diffuse intergalactic medium with LOFAR
• Constraints on interacting dark energy models from galaxy Rotation Curves
• The impact of cosmic rays on dynamical balance and disk-halo interaction in Lstar disk galaxies
• The rise and fall of a challenger: the Bullet Cluster in $\Lambda$ Cold Dark Matter simulations
• Resolving the Complex Evolution of a Supermassive Black Hole Triplet in a Cosmological Simulation
• Cosmological Simulations of the Preheating Scenario for Galaxy Cluster Formation: Comparison to Analytic Models and Observations
• The importance of magnification effects in galaxy-galaxy lensing
• The First Stars: formation under X-ray feedback
• Internal kinematics of modelled interacting disc galaxies
• Finding Dwarf Galaxies From Their Tidal Imprints
• The cross-correlation between 21cm intensity mapping maps and the Lyman-alpha forest in the post-reionization era
• Non-linear damping of superimposed primordial oscillations on the matter power spectrum in galaxy surveys
• The Effect Of AGN Heating On The Low-Redshift Lyα Forest
• Testing the accuracy of the Hydro-PM approximation in numerical simulations of the Lyman-alpha forest
• Tidally induced spiral arm wraps encoded in phase space
• Simulations of Quintessential Cold Dark Matter: beyond the cosmological constant
• Relativistic SZ temperature scaling relations of groups and clusters derived from the BAHAMAS and MACSIS simulations
• Effects of cosmological parameters and star formation models on the cosmic star formation history in LambdaCDM cosmological simulations
• Dark Energy Survey Year 3 results: Marginalisation over redshift distribution uncertainties using ranking of discrete realisations
• Mapping the real space distributions of galaxies in SDSS DR7: I. Two Point Correlation Functions
• The eROSITA view of the Abell 3391/95 field: a case study from the Magneticum cosmological simulation
• Gamma-ray diagnostics of Type Ia supernovae: Predictions of observables from three-dimensional modeling
• The IRX-$\beta$ relation: Insights from simulations
• nIFTy Cosmology: the clustering consistency of galaxy formation models
• On the relation between radial alignment of dark matter subhalos and host mass in cosmological simulations
• No evidence for modifications of gravity from galaxy motions on cosmological scales
• Lyalpha versus X-ray heating in the high-z IGM
• The Impact of Coupled Dark Energy Cosmologies on the High-Redshift Intergalactic Medium
• The kinematics of globular cluster populations in the E-MOSAICS simulations and their implications for the assembly history of the Milky Way
• Maps of CMB lensing deflection from N-body simulations in Coupled Dark Energy Cosmologies
• 3D Radiation hydrodynamics of a dynamical torus
• Ringing the initial Universe: the response of overdensity and transformed-density power spectra to initial spikes
• EXP: N-body integration using basis function expansions
• The global structure of magnetic fields and gas in simulated Milky Way-analogue galaxies
• Soliton Formation and the Core-Halo Mass Relation: An Eigenstate Perspective
• The effects of a hot gaseous halo on disc thickening in galaxy minor mergers
• Applying Schwarzschild's orbit superposition method to barred or non-barred disc galaxies
• Investigating the Stellar Mass Growth Histories of Satellite Galaxies as a Function of Infall Time using Phase-Space
• Hints of dark photon dark matter from observations and hydrodynamical simulations of the low-redshift Lyman-$\alpha$ forest
• Enhanced mixing in giant impact simulations with a new Lagrangian method
• The splashback radius of halos from particle dynamics: III. Halo catalogs, merger trees, and host-subhalo relations
• Measuring the Tidal Response of Structure Formation: Anisotropic Separate Universe Simulations using TreePM
• Imprint of anisotropic primordial non-Gaussianity on halo intrinsic alignments in simulations
• Moving around the cosmological parameter space: a nonlinear power spectrum reconstruction based on high-resolution cosmic responses
• Simulated Galaxy Interactions as Probes of Merger Spectral Energy Distributions
• Reproducing cosmic evolution of galaxy population from $z=4$ to $0$
• Capture Formed Binaries via Encounters with Massive Protostars
• Andromeda II as a merger remnant
• Soft X-ray and ultra-violet metal-line emission from the gas around galaxies
• Disc galaxies formed from major mergers in Illustris
• Galaxy 2-Point Covariance Matrix Estimation for Next Generation Surveys
• Radio Emission in the Cosmic Web
• Sigma-Eight at the Percent Level: The EFT Likelihood in Real Space
• Towards Accurate Modelling of Galaxy Clustering on Small Scales: Testing the Standard $\Lambda \mathrm{CDM}$ + Halo Model
• An orbital perspective on the starvation, stripping, and quenching of satellite galaxies in the EAGLE simulations
• Precise Calibration of the One-Loop Bispectrum in the Effective Field Theory of Large Scale Structure
• Constraining self-interacting dark matter with scaling laws of observed halo surface densities
• Effects of stellar-mass primordial black holes on first star formation
• Hydrodynamical simulations of coupled and uncoupled quintessence models I: Halo properties and the cosmic web
• Quantifying AGN-Driven Metal-Enhanced Outflows in Chemodynamical Simulations
• ICE-COLA: fast simulations for weak lensing observables
• Mass loss in tidally stripped systems; the energy-based truncation method
• Migration and Mixing in the Galactic Disc from Encounters between Sagittarius and the Milky Way
• A Schwarzschild model of the Galactic bar with initial density from N-body simulations
• Primordial non-Gaussianities and zero bias tracers of the Large Scale Structure
• Multi-stream portrait of the Cosmic web
• The origin of abundance gradients in the Milky Way: the predictions of different models
• The SIBELIUS Project: E Pluribus Unum
• Galactic outflow and diffuse gas properties at z>=1 using different baryonic feedback models
• Can Coupled Dark Energy Speed Up the Bullet Cluster?
• The Matter Bispectrum in N-body Simulations with non-Gaussian Initial Conditions
• Semi-analytic galaxy formation in f(R)-gravity cosmologies
• The fully non-linear post-Friedmann frame-dragging vector potential: Magnitude and time evolution from N-body simulations
• ELUCID. VI: Cosmic variance of galaxy distribution in the local Universe
• No Evidence for Millimeter Continuum Source Overdensities in the Environments of $z\gtrsim 6$ Quasars
• Evolution induced by dry minor mergers onto fast-rotator S0 galaxies
• The evolution of the star formation rate function and cosmic star formation rate density of galaxies at $z\sim 1-4$
• The Effective Halo Model: Creating a Physical and Accurate Model of the Matter Power Spectrum and Cluster Counts
• Forming Pop III binaries in self-gravitating disks: how to keep the orbital angular momentum
• CLARA's view on the escape fraction of Lyman-Alpha photons in high redshift galaxies
• {\sc mirkwood:} Fast and Accurate SED Modeling Using Machine Learning
• Revealing the physical properties of gas accreting to haloes in the EAGLE simulations
• The radial acceleration relation in a $\Lambda$CDM universe
• Revealing the Structure and Internal Rotation of the Sagittarius Dwarf Spheroidal Galaxy with Gaia and Machine Learning
• Dust-Enshrouded AGN can Dominate Host-Galaxy-Scale Cold-Dust Emission
• A Short Introduction to Reionization Physics
• The evolution of the mass ratio of accreting binaries: the role of gas temperature
• Comparing halo bias from abundance and clustering
• Bondi-Hoyle-Lyttleton Accretion onto a Protoplanetary Disk
• Radiative cooling implementations in simulations of primordial star formation
• Star-forming galaxies are predicted to lie on a fundamental plane of mass, star formation rate and α-enhancement
• The Signatures of Self-Interacting Dark Matter and Subhalo Disruption on Cluster Substructure
• Neutrino Signatures on the High Transmission Regions of the Lyman-alpha Forest
• Baryon history and cosmic star formation in non-Gaussian cosmological models: numerical simulations
• On the origin of magnetic driven winds and the structure of the galactic dynamo in isolated galaxies
• A First Look at creating mock catalogs with machine learning techniques
• Simulations of galactic disks including a dark baryonic component
• Effect of Intergalactic Medium on the Observability of Lyman Alpha Emitters during Cosmic Reionization
• Measuring the Thermal Sunyaev-Zel'dovich Effect Through the Cross Correlation of Planck and WMAP Maps with ROSAT Galaxy Cluster Catalogs
• Do dark matter halos explain lensing peaks?
• Unbound Particles in Dark Matter Halos
• Semi-analytic forecasts for Roman -- the beginning of a new era of deep-wide galaxy surveys
• Physical properties of simulated galaxy populations at z=2 - II. Effects of cosmology, reionization and ISM physics
• Effects of large-scale environment on the assembly history of central galaxies
• Accelerated orbital decay of supermassive black hole binaries in merging nuclear star clusters
• Early structure formation from primordial density fluctuations with a blue-tilted power spectrum
• Panchromatic Spectral Energy Distributions of Dusty Galaxies with RADISHE. I. Predictions for Herschel: Correlating Colors with Galactic Energy Sources
• Galaxy cluster mergers as triggers for the formation of jellyfish galaxies: case study of the A901/2 system
• The origin of kinematically distinct cores and misaligned gas discs in galaxies from cosmological simulations
• Galaxy fields of LISA massive black hole mergers in a simulated Universe
• Impacts of the physical data model on the forward inference of initial conditions from biased tracers
• Influence of baryons on the orbital structure of dark matter haloes
• Tidal Imprints of a Dark Sub-Halo on the Outskirts of the Milky Way II. Perturber Azimuth
• One-point remapping of Lagrangian perturbation theory in the mildly non-linear regime of cosmic structure formation
• Binary formation and mass function variations in fragmenting discs with short cooling times
• Reionization of the Local Group of Galaxies
• Tomographic Intensity Mapping versus Galaxy Surveys: Observing the Universe in H-alpha emission with new generation instruments
• The Phase Space Structure of Dark Matter Halos
• Small-scale galaxy clustering in the EAGLE simulation
• Satellite galaxies in hydrodynamical simulations of Milky Way sized galaxies
• SPH Simulations of Black Hole Accretion: A Step to Model Black Hole Feedback in Galaxies
• Pressure Support vs. Thermal Broadening in the Lyman-alpha Forest II: Effects of the Equation of State on Transverse Structure
• How Baryonic Processes affect Strong Lensing properties of Simulated Galaxy Clusters
• Tidal evolution of dark matter annihilation rates in subhalos
• Cosmic filaments delay quenching inside clusters
• Robust PCA and MIC statistics of baryons in early mini-haloes
• Stochastic angular momentum slews and flips and their effect on discs in galaxy formation models
• Deriving the Hubble constant using Planck and XMM-Newton observations of galaxy clusters
• Scaling Rrelation in two situations of extreme mergers
• Simulated star formation rate functions at z~4-7, and the role of feedback in high-z galaxies
• Dissecting the thermal Sunyaev-Zeldovich-gravitational lensing cross-correlation with hydrodynamical simulations
• The DESI $N$-body Simulation Project I: Testing the Robustness of Simulations for the DESI Dark Time Survey
• Black hole feedback in a multiphase interstellar medium
• Structure Formation and Backreaction in Growing Neutrino Quintessence
• Osaka Feedback Model II: Modeling Supernova Feedback Based on High-Resolution Simulations
• Abundances, masses, and weak-lensing mass profiles of galaxy clusters as a function of richness and luminosity in LambdaCDM cosmologies
• Simulating the formation of a proto-cluster at z~2
• A divergence-cleaning scheme for cosmological SPMHD simulations
• A new smooth-$k$ space filter approach to calculate halo abundances
• Formation of star clusters and enrichment by massive stars in simulations of low-metallicity galaxies with a fully sampled initial stellar mass function
• Baryon acoustic oscillations reconstruction using convolutional neural networks
• Redshift-space streaming velocity effects on the Lyman-$\alpha$ forest baryon acoustic oscillation scale
• Massive Low Surface Brightness Galaxies in the EAGLE Simulation
• The Relation Between Halo Shape, Velocity Dispersion and Formation Time
• Simulating the Complexity of the Dark Matter Sheet I: Numerical Algorithms
• CODEX Weak Lensing: Concentration of Galaxy Clusters at z ~ 0.5
• The MUSIC of Galaxy Clusters III: Properties, evolution and Y-M scaling relation of protoclusters of galaxies
• Defeating stochasticity: coalescence timescales of massive black holes in galaxy mergers
• The central spheroids of Milky Way mass-sized galaxies
• Accelerated FDPS --- Algorithms to Use Accelerators with FDPS
• IQ Collaboratory II: The Quiescent Fraction of Isolated, Low Mass Galaxies Across Simulations and Observations
• Beyond two-point statistics: using the minimum spanning tree as a tool for cosmology
• The Halo Mass-Bias Redshift Evolution in the $\Lambda$CDM Cosmology
• The Three Hundred Project: the stellar and gas profiles
• Angular momentum and clustering properties of early dark matter halos
• Too dense to go through: The importance of low-mass clusters for satellite quenching
• Gravitational waves from in-spirals of compact objects in binary common-envelope evolution
• Cosmic voids uncovered -- first-order statistics of depressions in the biased density field
• SMBH Seeds from Dissipative Dark Matter
• Merger relics of cluster galaxies
• Formation of the first galaxies in the aftermath of the first supernovae
• Accurate tracer particles of baryon dynamics in the adaptive mesh refinement code Ramses
• Adaptive gravitational softening in GADGET
• Improved strong lensing modelling of galaxy clusters using the Fundamental Plane: Detailed mapping of the baryonic and dark matter mass distribution of Abell S1063
• Simultaneously constraining cosmology and baryonic physics via deep learning from weak lensing
• The Minimum Halo Mass for Star Formation at z = 6 - 8
• Thermal and dynamical properties of gas accreting onto a supermassive black hole in an AGN
• Perturbation theory challenge for cosmological parameters estimation: Matter power spectrum in real space
• Fast full $N$-body simulations of generic modified gravity: derivative coupling models
• IQ-Collaboratory 1.1: the Star-Forming Sequence of Simulated Central Galaxies
• Tidally induced bars in dwarf galaxies on different orbits around a Milky Way-like host
• The baryonic Tully-Fisher relation in the Simba simulation
• KiDS-1000 cosmology: Combined second- and third-order shear statistics
• The quasi-linear nearby Universe
• Deviations from tidal torque theory: evolution of the halo spin-filament alignment
• The Gravitational Lensing Signatures of BOSS Voids in the Cosmic Microwave Background
• Cosmology with cosmic web environments I. Real-space power spectra
• Evolution along the sequence of S0 Hubble types induced by dry minor mergers. I - Global bulge-to-disk structural relations
• The effect of feedback on the emission properties of the Warm-Hot Intergalactic Medium
• CRESCENDO: An on-the-fly Fokker-Planck Solver for Spectral Cosmic Rays in Cosmological Simulations
• Calibrated, cosmological hydrodynamical simulations with variable IMFs I: Method and effect on global galaxy scaling relations
• A Symplectic Integrator for Hill's Equations
• The need for obscured supermassive black hole growth to explain quasar proximity zones in the epoch of reionization
• Cosmic CARNage I: on the calibration of galaxy formation models
• Nebular line emission from z > 7 galaxies in cosmological simulations: rest-frame UV to Optical lines
• The Kennicutt-Schmidt Star Formation Relation at z~2
• How does gas cool in DM halos?
• Origin of highly $r$-process-enhanced stars in a cosmological zoom-in simulation of a Milky Way-like galaxy
• Quasar Clustering in Cosmological Hydrodynamic Simulations: Evidence for mergers
• Deciphering the Archaeological Record: Cosmological Imprints of Non-Minimal Dark Sectors
• The sparkling Universe: the coherent motions of cosmic voids
• The twisted dark matter halo of the Milky Way
• Simulations of the Sunyaev-Zeldovich Effect from Quasars
• Modeling Galaxy-Galaxy Weak Lensing with SDSS Groups
• Structure and rotation of young massive star clusters in a simulated dwarf starburst
• The effects of LMC-mass environments on their dwarf satellite galaxies in the FIRE simulations
• Cosmological $N$-body simulations including radiation perturbations
• Precision cosmology in muddy waters: Cosmological constraints and N-body codes
• What determines large scale galaxy clustering: halo mass or local density?
• Further constraining galaxy evolution models through the Size Function of SDSS Early-type galaxies
• Power spectrum for the small-scale Universe
• Power Spectra to 1% Accuracy between Dynamical Dark Energy Cosmologies
• Impact of AGN feedback on galaxies and their multiphase ISM across cosmic time
• Cusp or core? Revisiting the globular cluster timing problem in Fornax
• The phase-space structure of nearby dark matter as constrained by the SDSS
• Distribution of the very first PopIII stars and their relation to bright z~6 quasars
• Investigating Cluster Astrophysics and Cosmology with Cross-Correlation of the Thermal Sunyaev-Zel'dovich Effect and Weak Lensing
• Flows around galaxies. I. The dependency of galaxy connectivity on cosmic environments and effects on the star-formation rate
• Disentangling dark sector models using weak lensing statistics
• Combining Semi-analytic Models with Simulations of Galaxy Clusters: the Need for Heating from Active Galactic Nuclei
• Is NGC 5824 the Core of the Progenitor of the Cetus Stream?
• Cosmological Information in Skew Spectra of Biased Tracers in Redshift Space
• Small-scale structure and the Lyman-$\alpha$ forest baryon acoustic oscillation feature
• A coarse grained perturbation theory for the Large Scale Structure, with cosmology and time independence in the UV
• How does non-linear dynamics affect the baryon acoustic oscillation?
• The Concerted Impact of Galaxies and QSOs on the Ionization and Thermal State of the Intergalactic Medium
• Dark matter haloes in modified gravity and dark energy: interaction rate, small-, and large-scale alignment
• Full-sky ray-tracing simulation of weak lensing using ELUCID simulations: exploring galaxy intrinsic alignment and cosmic shear correlations
• Revealing the cosmic web dependent halo bias
• The Asymptotic Form of Cosmic Structure: Small Scale Power and Accretion History
• How much metals did the first stars provide to the ultra-faint dwarfs?
• DEMNUni: comparing nonlinear power spectra prescriptions in the presence of massive neutrinos and dynamical dark energy
• Exploring KSZ velocity reconstruction with $N$-body simulations and the halo model
• Prediction of H$\alpha$ and [OIII] Emission Line Galaxy Number Counts for Future Galaxy Redshift Surveys
• The distinct stellar metallicity populations of simulated Local Group dwarfs
• Non-linear matter power spectrum from Time Renormalisation Group: efficient computation and comparison with one-loop
• How gas flows shape the stellar-halo mass relation in the EAGLE simulation
• $\Lambda$CDM Predictions for the Satellite Population of M33
• Mapping "out-of-the-box" the properties of the baryons in massive halos
• Search of sub-parsec massive binary black holes through line diagnosis II
• Imprints of Chameleon f(R) Gravity on Galaxy Rotation Curves
• Constraining the inner density slope of massive galaxy clusters
• A Parametric Model for Self-Interacting Dark Matter Halos
• The Gentle Growth of Galaxies at High Redshifts in Overdense Environments
• Dispersal of tidal debris in a Milky-Way-sized dark matter halo
• Formation of massive stars under protostellar radiation feedback: Very metal-poor stars
• Observability of Low-Luminosity AGN in the Early Universe with JWST
• Evolution and Role of Mergers in the BCG-Cluster Alignment. A View from Cosmological Hydro-Simulations
• On the small scale turbulent dynamo in the intracluster medium: A comparison to dynamo theory
• Offsets between the X-ray and the Sunyaev-Zel'dovich-effect peaks in merging galaxy clusters and their cosmological implications
• The cosmic UV background and the beginning and end of star formation in simulated field dwarf galaxies
• High density of active galactic nuclei in the outskirts of distant galaxy clusters
• Fast Weak Lensing Simulations with Halo Model
• Tomographic weak lensing shear spectra from large N-body and hydrodynamical simulations
• Simulating the formation and evolution of galaxies: Multi-phase description of the interstellar medium, star formation, and energy feedback
• Constraining cosmology with shear peak statistics: tomographic analysis
• The cosmic web for density perturbations of various scales
• Linear and non-linear bias: predictions vs. measurements
• Early formation of moons around large trans-Neptunian objects via giant impacts
• RHAPSODY-G simulations II - Baryonic growth and metal enrichment in massive galaxy clusters
• Halo assembly bias from Separate Universe simulations
• Local gravitational redshifts can bias cosmological measurements
• Cosmology with photometric weak lensing surveys: constraints with redshift tomography of convergence peaks and moments
• Morphological and Rotation Structures of Circumgalactic Mg II Gas in the EAGLE Simulation and the Dependence on Galaxy Properties
• Tidal Torquing of Elliptical Galaxies in Cluster Environments
• Long duration gamma-ray bursts: hydrodynamic instabilities in collapsar disks
• Variational Integrators for the Gravitational N-Body Problem
• Remapping dark matter halo catalogues between cosmological simulations
• Dark-ages Reionization & Galaxy Formation Simulation II: Spin and concentration parameters for dark matter haloes during the Epoch of Reionization
• The evolution of barred galaxies in the EAGLE simulations
• A fitting formula for the non-Gaussian contribution to the lensing power spectrum covariance
• On the Cluster Physics of Sunyaev-Zel'dovich and X-ray Surveys IV: Characterizing Density and Pressure Clumping due to Infalling Substructures
• The mass function dependence on the dynamical state of dark matter haloes
• The Effect of Bulge Mass on Bar Pattern Speed in Disk Galaxies
• J-PLUS: Synthetic galaxy catalogues with emission lines for photometric surveys
• NGC 2276: a remarkable galaxy with a large number of ULXs
• Extended Lyman-alpha emission from interacting galaxies at high redshifts
• Cosmological Structure Formation in Decaying Dark Matter Models
• Probing the Circum-Galactic Medium with Fast Radio Bursts: Insights from the CAMELS Simulations
• Characterising the intra-cluster light in The Three Hundred simulations
• Density modulated star formation efficiency: implications for the observed abundance of ultra-violet luminous galaxies at z>10
• A dynamics-based density profile for dark haloes -- II. Fitting function
• The kinematics of local thick discs do not support an accretion origin
• Zel'dovich approximation and General Relativity
• Hybrid Cosmological Simulations with Stream Velocities
• The effect of gas accretion on the radial gas metallicity profile of simulated galaxies
• The Physical Origin of Galactic Conformity: From Theory to Observation
• Stellar feedback strongly alters the amplification and morphology of galactic magnetic fields
• Globular cluster numbers in dark matter haloes in a dual formation scenario: an empirical model within EMERGE
• The structural evolution of galaxies with both thin and thick discs
• Early Black Holes in Cosmological Simulations: Luminosity Functions and Clustering Behaviour
• Semi-analytic galaxies -- III. The impact of supernova feedback on the mass-metallicity relation
• Galaxy Formation in Heavily Overdense Regions at z~10: the Prevalence of Disks in Massive Halos
• X-ray metal line emission from the hot circumgalactic medium: probing the effects of supermassive black hole feedback
• Why Cosmic Voids Matter: Nonlinear Structure & Linear Dynamics
• The Origin of Extended Disk Galaxies at z=2
• The Mutual Interaction Between Population III Stars and Self-Annihilating Dark Matter
• Understanding redshift space distortions in density-weighted peculiar velocity
• Super massive black holes in star forming gaseous circumnuclear discs
• The impact of baryonic physics on the abundance, clustering, and concentration of halos
• Pressure profiles of distant galaxy clusters in the Planck catalog
• A new approach to determine optically thick H2 cooling and its effect on primordial star formation
• Gaussianizing the non-Gaussian lensing convergence field I: the performance of the Gaussianization
• Mask Effects on Cosmological Studies with Weak Lensing Peak Statistics
• Dark-ages reionization & galaxy formation simulation V: morphology and statistical signatures of reionization
• The optimal gravitational softening length for cosmological N-body simulations
• Halo Exclusion Criteria Impacts Halo Statistics
• Symplectic integration for the collisional gravitational $N$-body problem
• ELUCID V. Lighting dark matter halos with galaxies
• To the Galactic Virial Radius with Hyper Suprime-Cam
• Evolution along the sequence of S0 Hubble types induced by dry minor mergers. II - Bulge-disk coupling in the photometric relations through merger-induced internal secular evolution
• Primordial Earth mantle heterogeneity caused by the Moon-forming giant impact
• On the observability of coupled dark energy with cosmic voids
• Minkowski Functionals of SDSS-III BOSS : Hints of Possible Anisotropy in the Density Field?
• The formation of entropy cores in non-radiative galaxy cluster simulations: SPH versus AMR
• Kinematics and Structure of Star-forming Regions: Insights from Cold Collapse Models
• Deep spectroscopy in nearby galaxy clusters: III Orbital structure of galaxies in Abell 85
• Detecting neutral hydrogen in emission at redshift z ~ 1
• The Sheet of Giants: Unusual Properties of the Milky Way's Immediate Neighbourhood
• Halo intrinsic alignment: dependence on mass, formation time and environment
• Wavelet analysis of the formation of the cosmic web
• Modelling the thermal X-ray emission around the Galactic Centre from colliding Wolf-Rayet winds
• FROST: a momentum-conserving CUDA implementation of a hierarchical fourth-order forward symplectic integrator
• Chemical evolution of disc galaxies from cosmological simulations
• Weak-lensing-inferred scaling relations of galaxy clusters in the RCS2: mass-richness, mass-concentration, mass-bias, and more
• The effect of AGN feedback on the migration timescale of supermassive black holes binaries
• Quantification of stochastic fragmentation of self-gravitating discs
• Gas cooling in semi-analytic models and SPH simulations: are results consistent?
• Constraining Primordial Non-Gaussianity with Post-reconstructed Galaxy Bispectrum in Redshift Space
• Understanding the nature of luminous red galaxies (LRGs): Connecting LRGs to central and satellite subhalos
• The Gigaparsec WiggleZ Simulations: Characterising scale dependant bias and associated systematics in growth of structure measurements
• Cosmological DCBH formation sites hostile for their growth
• Visualization, Exploration and Data Analysis of Complex Astrophysical Data
• Extracting bias using the cross-bispectrum: An EoR and 21 cm-[CII]-[CII] case study
• N-body simulations with a cosmic vector for dark energy
• PRIYA: A New Suite of Lyman-alpha Forest Simulations for Cosmology
• Non-universality of halo profiles and implications for dark matter experiments
• Models of the Cosmological 21 cm Signal from the Epoch of Reionization Calibrated with Lyman-alpha and CMB Data
• On the algorithms of radiative cooling in semi-analytic models
• Molecular cloud regulated star formation in galaxies
• Counts of high-redshift GRBs as probe of primordial non-Gaussianities
• Testing LSST Dither Strategies for Survey Uniformity and Large-Scale Structure Systematics
• What Can We Learn by Combining the Skew Spectrum and the Power Spectrum?
• Cosmology dependence of galaxy cluster scaling relations
• Weak Lensing by Line-of-sight Halos as the Origin of Flux-ratio Anomalies in Quadruply Lensed QSOs
• Estimating CDM Particle Trajectories in the Mildly Non-Linear Regime of Structure Formation. Implications for the Density Field in Real and Redshift Space
• Exploring the posterior surface of the large scale structure reconstruction
• Cosmology inference at the field level from biased tracers in redshift-space
• Insights on the origin of ORCs from cosmological simulations
• The impact of AGN on stellar kinematics and orbits in simulated massive galaxies
• The Impact of Baryons on Cosmological Inference from Weak Lensing Statistics
• Populating H${}_2$ and CO in galaxy simulation with dust evolution
• Benchmarking and Scalability of Machine Learning Methods for Photometric Redshift Estimation
• Measuring the EoR Power Spectrum Without Measuring the EoR Power Spectrum
• Large-Scale Velocity Dispersion and the Cosmic Web
• Cosmological Newtonian limits on large spacetime scales
• Particle splitting in smoothed particle hydrodynamics based on Voronoi diagram
• The orientation of planes of dwarf galaxies in the quasi-linear Universe
• Evolution and Statistics of Non-Sphericity of Dark Matter Halos from Cosmological N-Body Simulation
• A new approach to cosmological structure formation with massive neutrinos
• Spurious Small-Scale Structure & Discreteness-Driven Relaxation in Cosmological Simulations
• Clustering with JWST: Constraining Galaxy Host Halo Masses, Satellite Quenching Efficiencies, and Merger Rates at z=4-10
• Euclid: The search for primordial features
• Massive quiescent galaxies at $z\sim 3$: a comparison of selection, stellar population and structural properties with simulation predictions
• Relative velocity of dark matter and barions in clusters of galaxies and measurements of their peculiar velocities
• The QSO proximity effect at redshift <z>=2.6 with the FLO approach
• KiDS-450: Enhancing cosmic shear with clipping transformations
• The stellar halo in Local Group Hestia simulations I. The in-situ component and the effect of mergers
• Modelling recombinations during cosmological reionization
• Cosmological information content in redshift-space power spectrum of SDSS-like galaxies in the quasi-nonlinear regime up to $k=0.3h$Mpc${}^{-1}$
• The Cosmic Baryon Partition between the IGM and CGM in the SIMBA Simulations
• The Three Hundred Project: Substructure in hydrodynamical and dark matter simulations of galaxy groups around clusters
• The void halo mass function: a promising probe of neutrino mass
• Weak lensing predictions for coupled dark energy cosmologies at non-linear scales
• A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
• Towards a non-Gaussian model of redshift space distortions
• Local simulations of MRI turbulence with meshless methods
• Primordial star formation: relative impact of H2 three-body rates and initial conditions
• Anisotropic halo assembly bias and redshift-space distortions
• Absorption features of high redshift galactic winds
• Constraints on decaying dark matter from weak lensing and cluster counts
• SMART: A new implementation of Schwarzschild's Orbit Superposition technique for triaxial galaxies and its application to an N-body merger simulation
• Galactic conformity measured in semi-analytic models
• Hydrodynamic capabilities of an SPH code incorporating an artificial conductivity term with a gravity-based signal velocity
• Morphological & Dynamical Properties of low redshift 2dFGRS Groups
• Mass-Metallicity Relation from Cosmological Hydrodynamical Simulations and X-ray Observations of Galaxy Groups and Clusters
• Galaxy clusters in simulations of the local Universe: a matter of constraints
• KiDS-1000 Cosmology: Constraints from density split statistics
• ZOMG II: Does the halo assembly history influence central galaxies and gas accretion?
• Fast Generation of Covariance Matrices for Weak Lensing
• MaNGIA: 10,000 mock galaxies for stellar population analysis
• The spatial distribution of neutral hydrogen as traced by low HI mass galaxies
• Weak lensing peak statistics in the era of large scale cosmological surveys
• The physical drivers of gas turbulence in simulated disc galaxies
• DEMNUni: The imprint of massive neutrinos on the cross-correlation between cosmic voids and CMB lensing
• The case against large intensity fluctuations in the z ~ 2.5 HeII Lyman-alpha forest
• Stellar feedback from HMXBs in cosmological hydrodynamical simulations
• Using Velocity Dispersion to Estimate Halo Mass: Is the Local Group in Tension with $\Lambda$CDM?
• Face-on accretion onto a protoplanetary disc
• Lyman-alpha Emitters in Cosmological Simulations I: Lyman-alpha Escape Fraction and Statistical Properties at z=3.1
• Cosmology with the pairwise kinematic SZ effect: Calibration and validation using hydrodynamical simulations
• The effect of warm gas on the buckling instability in galactic bars
• Two-Fluid Dusty Gas in Smoothed Particle Hydrodynamics: Fast and Implicit Algorithm for Stiff Linear Drag
• Simulations of core formation for frequent dark matter self-interactions
• The Detection and Statistics of Giant Arcs Behind CLASH Clusters
• Rest-frame UV line emission from the intergalactic medium at 2<z<5
• Measuring nonlocal Lagrangian peak bias
• Sunyaev-Zel'dovich profiles and scaling relations: modelling effects and observational biases
• New constraints on cosmological modified gravity theories from anisotropic three-point correlation functions of BOSS DR12 galaxies
• Morphology rather than environment drives the SFR-Mass relation in the local universe
• Cosmological gravity on all scales II: Model independent modified gravity $N$-body simulations
• Evolution of superclusters in the cosmic web
• The Origin of the Dust Extinction Curve in Milky Way-like Galaxies
• Star-formation driven outflows in local dwarf galaxies as revealed from [CII] observations by Herschel
• The imprint of dark matter haloes on the size and velocity dispersion evolution of early-type galaxies
• Detection and analysis of cluster-cluster filaments
• Kinematic analysis of EAGLE simulations: Evolution of ${\lambda }_{Re}$ and its connection with mergers and gas accretion
• Probing features in the primordial perturbation spectrum with large-scale structure data
• How accurate is it to update the cosmology of your halo catalogues?
• Parallel HOP: A Scalable Halo Finder for Massive Cosmological Data Sets
• Exploring the cosmological synergy between galaxy cluster and cosmic void number counts
• The evolution of the Lyman-alpha forest effective optical depth following HeII reionisation
• Migration and kinematics in growing disc galaxies with thin and thick discs
• On the detectability of visible-wavelength line emission from the local circumgalactic and intergalactic medium
• The Halo Void (Dust) Model of Large Scale Structure
• Self-Consistent Solution of Cosmological Radiation-Hydrodynamics and Chemical Ionization
• First star formation in ultra-light particle dark matter cosmology
• Neural physical engines for inferring the halo mass distribution function
• Probing Feedback via IGM tomography and Ly$\alpha$ forest with Subaru PFS, TMT/ELT, and JWST
• Are turbulent spheres suitable initial conditions for star-forming clouds?
• A new method to measure galaxy bias
• Rise and fall of post-starburst galaxies in Magneticum Pathfinder
• Highly r-process enhanced stars in ultra-faint dwarf galaxies
• Simulations of gas sloshing in galaxy cluster Abell 2052
• Deviations from tidal torque theory: environment dependences on halo angular momentum growth
• EAGLE-Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
• Turbulence driven by structure formation in the circum-galactic medium
• Non-local bias contribution to third-order galaxy correlations
• The effect of inhomogeneous reionisation on the Lyman-$\alpha$ forest power spectrum at redshift $z>4$: implications for thermal parameter recovery
• Probing the thermal history during reionization using a semi-numerical photon-conserving code SCRIPT
• The origin of prolate rotation in dwarf spheroidal galaxies formed by mergers of disky dwarfs
• How the diffuse Universe cools
• The energy budget and figure of Earth during recovery from the Moon-forming giant impact
• Characterizing dark interactions with the halo mass accretion history and structural properties
• Strategies for Detecting the Missing Hot Baryons in the Universe
• The 3D structure of CO depletion in high-mass prestellar regions
• The Next Generation Virgo Cluster Survey. IX. Estimating the Efficiency of Galaxy Formation on the Lowest-Mass Scales
• Biases and systematics in the observational derivation of galaxy properties: comparing different techniques on synthetic observations of simulated galaxies
• The Transition Region between Brightest Cluster Galaxies and Intra-Cluster Light in Galaxy Groups and Clusters
• Hot WHIM counterparts of FUV OVI absorbers: Evidence in the line-of-sight towards quasar 3C 273
• The Life Cycle of the Central Molecular Zone. II: Distribution of atomic and molecular gas tracers
• Structure formation in Multiple Dark Matter cosmologies with long-range scalar interactions
• Euclid: Modelling massive neutrinos in cosmology -- a code comparison
• Discovery of a new fundamental plane dictating galaxy cluster evolution from gravitational lensing
• Reducing biases on $H_0$ measurements using strong lensing and galaxy dynamics: results from the EAGLE simulation
• The Lives of High Redshift Mergers
• Dark-ages reionization and galaxy formation simulation--VII. The sizes of high-redshift galaxies
• On the streaming model for redshift-space distortions
• Giant planets and brown dwarfs on wide orbits: a code comparison project
• Intergalactic Dust Extinction in Hydrodynamic Cosmological Simulations
• The role of AGN feedback on the evolution of dwarf galaxies from cosmological simulations: SMBHs suppress star formation in low-mass galaxies
• Fornax globular cluster distributions: implications for the cusp-core problem
• The galaxy population in cold and warm dark matter cosmologies
• Tracing the gravitational potential using cosmic voids
• The clustering of the first galaxy halos
• GOTHIC: Gravitational oct-tree code accelerated by hierarchical time step controlling
• The Sunyaev-Zel'dovich temperature of the intracluster medium
• Evolution of the metal content of the intra-cluster medium with hydrodynamical simulations
• The entropy core in galaxy clusters: numerical and physical effects in cosmological grid simulations
• Dynamical friction-driven orbital circularisation in rotating discs: a semi-analytical description
• Cataloging Accreted Stars within Gaia DR2 using Deep Learning
• Halo Abundance and Assembly History with Extreme-Axion Wave Dark Matter at $z\ge 4$
• Dust properties of Lyman break galaxies in cosmological simulations
• Weighing neutrinos with the halo environment
• Three-point phase correlations: A new measure of non-linear large-scale structure
• The formation and evolution of star clusters in interacting galaxies
• CUBE: An Information-optimized parallel Cosmological $N$-body Algorithm
• The orbital structure of a tidally induced bar
• Radiative feedback and cosmic molecular gas: the role of different radiative sources
• High-resolution synthetic UV-submm images for Milky Way-mass simulated galaxies from the ARTEMIS project
• The two phases of core formation -- orbital evolution in the centres of ellipticals with supermassive black hole binaries
• Statistical correlation between the distribution of Ly$\alpha$ emitters and IGM HI at $z\sim 2.2$ mapped by Subaru/Hyper Suprime-Cam
• The mean free path of hydrogen ionizing photons during the epoch of reionization
• Non-thermal radio supernova remnants of exiled Wolf-Rayet stars
• Stellar Velocity Dispersion in Dissipative Galaxy Mergers with Star Formation
• Baryons Shaping Dark Matter Haloes
• The ultra-diffuse dwarf galaxies NGC 1052-DF2 and 1052-DF4 are in conflict with standard cosmology
• Angular Momentum of Early and Late Type Galaxies: Nature or Nurture?
• KETJU -- resolving small-scale supermassive black hole dynamics in GADGET-4
• Effects of Inner Halo Angular Momentum on the Peanut/X-shapes of Bars
• Intergalactic filaments spin
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• Towards physics responsible for large-scale Lyman-$\alpha$ forest bias parameters
• Properties of Wide-separation Lensed Quasars by Clusters of Galaxies in the SDSS
• Detectability of [CII] 158 micron emission from high-redshift galaxies: predictions for ALMA and SPICA
• Reconstructing the cosmological density and velocity fields from redshifted galaxy distributions using V-net
• Baryon Pasting Algorithm: Halo-based and Particle-based Pasting Methods
• Kinetic relaxation and nucleation of Bose stars in self-interacting wave dark matter
• Atomic and molecular gas from the epoch of reionization down to redshift 2
• Might we eventually understand the origin of the dark matter velocity anisotropy?
• Principles of supernova-driven winds
• DM haloes in the fifth-force cosmology
• On the relevance of chaos for halo stars in the Solar Neighbourhood
• Where do galaxies end? Comparing measurement techniques of hydrodynamic-simulation galaxies' integrated properties
• GOGREEN: a critical assessment of environmental trends in cosmological hydrodynamical simulations at z ~ 1
• The relation between star formation rate and stellar mass of galaxies at z $\sim$ 1-4
• ECO and RESOLVE: Galaxy Disk Growth in Environmental Context
• The host galaxy of GRB 980425 / SN1998bw: a collisional ring galaxy
• Subhaloes in Scale-Free Cosmologies
• The stellar halo in Local Group Hestia simulations II. The accreted component
• Detection of universality of dark matter profile from Subaru weak lensing measurements of 50 massive clusters
• The thick disk rotation-metallicity correlation as a fossil of an "inverse chemical gradient" in the early Galaxy
• On the evolution of cluster scaling relations
• Determination of Dark Matter Halo Mass from Dynamics of Satellite Galaxies
• Effect of non-equilibrium ionization on derived physical conditions of the high-$z$ intergalactic medium
• Constraints on AGN feedback from its Sunyaev-Zel'dovich imprint on the cosmic background radiation
• On the absence of dark matter in dwarf galaxies surrounding the Milky Way
• The miniJPAS survey: The role of group environment in quenching the star formation
• Consequences of the lack of azimuthal freedom in the modeling of lensing galaxies
• UniverseMachine: Predicting Galaxy Star Formation over Seven Decades of Halo Mass with Zoom-in Simulations
• Tidal Mass Loss from Collisionless Systems
• Black hole mass of central galaxies and cluster mass correlation in cosmological hydro-dynamical simulations
• The Role of Star-Formation and AGN in Dust Heating of z=0.3-2.8 Galaxies - II. Informing IR AGN fraction estimates through simulations
• The Local Hubble Flow: Is it a Manifestation of Dark Energy?
• Comparison of spatial distributions of Intracluster light and Dark Matter
• Explaining the scatter in the galaxy mass-metallicity relation with gas flows
• Study on the mapping of dark matter clustering from real space to redshift space
• Distinctive rings in the 21 cm signal of the epoch of reionization
• The reionization of galactic satellite populations
• Binary Capture Rates for Massive Protostars
• Helmholtz Decomposition of the Lagrangian Displacement
• Weak Lensing Peaks in Simulated Light-Cones: Investigating the Coupling between Dark Matter and Dark Energy
• Anisotropic separate universe simulations
• Bulk flow of halos in ΛCDM simulation
• Changes in the metallicity of gas giant planets due to pebble accretion
• Compressing the cosmological information in one-dimensional correlations of the Lyman-$\alpha$ forest
• Impact of inhomogeneous reionization on the Lyman-α forest
• Dust evolution with MUPPI in cosmological volumes
• GRay2: A General Purpose Geodesic Integrator for Kerr Spacetimes
• Co-evolution of Dust and Chemistry in Galaxy Simulations with a Resolved Interstellar Medium
• Color Magnitude Relation and Morphology of Low-Redshift ULIRGs in SDSS
• Velocity Structure Diagnostics of Simulated Galaxy Clusters
• A Physical Model of Lyman Alpha Emitters
• One line to run them all: SuperEasy massive neutrino linear response in $N$-body simulations
• The Three Hundred: Cluster Dynamical States and Relaxation Time Scale
• The galaxy-halo size relation of low-mass galaxies in FIRE
• A New Discrete Dynamical Friction Estimator Based on $N$-body Simulations
• An Observational Estimate for the Mean Secular Evolution Rate in Spiral Galaxies
• The segregation of baryons and dark matter during halo assembly
• The impact of cored density profiles on the observable quantities of dwarf spheroidal galaxies
• An alternative method to generate pre-initial conditions for cosmological $N$-body simulations
• Scaling relations between numerical simulations and physical systems they represent
• A hybrid SPH/N-body method for star cluster simulations
• Accurate initial conditions in mixed Dark Matter--Baryon simulations
• The giant arc statistics in the three year WMAP cosmological model
• The Future of the Local Large Scale Structure: the roles of Dark Matter and Dark Energy
• Massive Dark Matter Halos at High Redshift: Implications for Observations in the JWST Era
• Covariance matrices for galaxy cluster weak lensing: from virial regime to uncorrelated large-scale structure
• Bayesian Inference of Initial Conditions from Non-Linear Cosmic Structures using Field-Level Emulators
• Gravitational Lensing with Three-Dimensional Ray Tracing
• Metallicity map of the galaxy cluster A3667
• Clustering and redshift-space distortions in modified gravity models with massive neutrinos
• Quijote-PNG: Quasi-maximum likelihood estimation of Primordial Non-Gaussianity in the non-linear dark matter density field
• Exploring Galaxy Formation Models and Cosmologies with Galaxy Clustering
• The stellar halo in Local Group Hestia simulations III. Chemical abundance relations for accreted and in-situ stars
• Dianoga SIDM: galaxy cluster self-interacting dark matter simulations
• A Performance Comparison of Different Graphics Processing Units Running Direct N-Body Simulations
• Fallback supernova assembly of heavy binary neutron stars and light black hole-neutron star pairs and the common stellar ancestry of GW190425 and GW200115
• Modeling Intrinsic Galaxy Alignment in the MICE Simulation
• The Three Hundred project: galaxy cluster mergers and their impact on the stellar component of brightest cluster galaxies
• Excitation of vertical breathing motion in disc galaxies by tidally-induced spirals in fly-by interactions
• The Lyman-alpha forest in f(R) modified gravity
• Signature of the first galaxies in JWST deep field observations
• Interaction between dark matter sub-halos & galactic gaseous disk
• Modelling the cosmological Lyman-Werner background radiation field in the Early Universe
• The effect of stellar and AGN feedback on the low redshift Lyman-$\alpha$ forest in the Sherwood simulation suite
• The LSST-DESC 3x2pt Tomography Optimization Challenge
• The impact of spatial fluctuations in the ultra-violet background on intergalactic carbon and silicon
• Studying the Warm-Hot Intergalactic Medium in Emission
• Analyzing and Visualizing Cosmological Simulations with ParaView
• Most pseudo-bulges can be formed at later stages of major mergers
• The interaction of Type Iax supernova ejecta with a helium companion star
• On the importance of high redshift intergalactic voids
• Oscillating nonlinear large scale structure in growing neutrino quintessence
• Dark influences III. Structural characterization of minor mergers of dwarf galaxies with dark satellites
• Subhalo accretion through filaments
• WOMBAT: A Scalable and High Performance Astrophysical MHD Code
• Influence of baryonic physics on the merger time-scale of galaxies in N-body/hydrodynamical simulations
• High resolution simulations of the reionization of an isolated Milky Way - M31 galaxy pair
• The Thermal Proximity Effect: A New Probe of He II Reionization History and the Quasar Lifetime
• On the redshift evolution of the baryon and gas fraction in simulated groups and clusters of galaxies
• Comparing Simulations of AGN Feedback
• Convolution Lagrangian perturbation theory for biased tracers beyond general relativity
• Dynamics of Kicked and Accelerated Massive Black Holes in Galaxies
• Accurate Identification of Galaxy Mergers with Stellar Kinematics
• Stellar Bars in Counter-Rotating Dark Matter Halos: The Role of Halo Orbit Reversals
• AstraeusIV : Quantifying the star formation histories of galaxies in the Epoch of Reionization
• Precise Calibration of the One-Loop Trispectrum in the Effective Field Theory of Large Scale Structure
• Covariance of the matter power spectrum including the survey window function effect: N-body simulations vs. fifth-order perturbation theory on grid
• Taking measurements of the kinematic Sunyaev-Zel'dovich effect forward: including uncertainties from velocity reconstruction with forward modeling
• The two and three-loop matter bispectrum in perturbation theories
• Extracting cosmological parameters from N-body simulations using machine learning techniques
• Dark Matter Simulations with Primordial Black Holes in the Early Universe
• What do observations of the Lyman-alpha fraction tell us about reionization?
• The first constraint from SDSS galaxy-galaxy weak lensing measurements on interacting dark energy models
• Extended percolation analysis of the cosmic web
• MODA: a new algorithm to compute optical depths in multi-dimensional hydrodynamic simulations
• Phase-space structures I: A comparison of 6D density estimators
• Radiative feedback and cosmic molecular gas: numerical method
• Rigorous theoretical constraint on constant negative EoS parameter $\omega$ and its effect for the late Universe
• Observational Measures of Halo Properties Beyond Mass
• Lyman-α Emitters in the context of hierarchical galaxy formation: predictions for VLT/MUSE surveys
• Constraining interacting dark energy models with the halo concentration-mass relation
• Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6
• ZOMG III: The effect of Halo Assembly on the Satellite Population
• Cosmological and idealized simulations of dark matter haloes with velocity-dependent, rare and frequent self-interactions
• The median density of the Universe
• X-ray clusters of galaxies in conformal gravity
• Redshift evolution of the dark matter haloes shapes
• Low-mass galaxy formation and the ionizing photon budget during reionization
• What sets the splashback radius of dark matter haloes: accretion history or other properties?
• High-redshift quasars and their host galaxies II: multiphase gas and stellar kinematics
• A numerical twist on the observational spin parameter, ${\lambda }_R$
• Hierarchy of N-point functions in the LCDM and ReBEL cosmologies
• Milky Way-est: Cosmological Zoom-in Simulations with Large Magellanic Cloud and Gaia-Sausage-Enceladus Analogs
• The warm-hot circumgalactic medium around EAGLE-simulation galaxies and its detection prospects with X-ray line emission
• The $I\kappa \epsilon \alpha$ model of feedback-regulated galaxy formation
• Predicting the Neutral Hydrogen Content of Galaxies From Optical Data Using Machine Learning
• The variance of the locally measured Hubble parameter explained with different estimators
• Newtonian Limits of Isolated Cosmological Systems on Long Time Scales
• Less wrong: a more realistic initial condition for simulations of turbulent molecular clouds
• Comparison of cosmological simulations and deep submillimetre galaxy surveys
• Planet-disc interaction on a freely moving mesh
• Models of Distorted and Evolving Dark Matter Halos
• Large-scale 3D mapping of the intergalactic medium using the Lyman Alpha Forest
• On the width of cold fronts in clusters of galaxies due to conduction
• Why is the Milky Way X-factor Constant?
• Evolution of Neutral Oxygen During the Epoch of Reionization and its Use in Estimating the Neutral Hydrogen Fraction
• SimSpin -- Constructing mock IFS kinematic data cubes
• CMB constraints on a physical model of reionization
• Galaxy Flybys: Evolution of the Bulge, Disk, and Spiral Arms
• Baryonic mass budgets for haloes in the EAGLE simulation, including ejected and prevented gas
• Dating individual quasars with the HeII proximity effect
• The effects of the interaction on the kinematics, stellar population and metallicity of AM2322-821 with Gemini/GMOS
• Fast simulations of cosmic large-scale structure with massive neutrinos
• X-ray ionization of the intergalactic medium by quasars
• Response approach to the squeezed-limit bispectrum: application to the correlation of quasar and Lyman-$\alpha$ forest power spectrum
• The behaviour of shape and velocity anisotropy in dark matter haloes
• Enabling matter power spectrum emulation in beyond-$\Lambda$CDM cosmologies with COLA
• syren-halofit: A fast, interpretable, high-precision formula for the $\Lambda$CDM nonlinear matter power spectrum
• The large-scale correlations of multi-cell densities and profiles, implications for cosmic variance estimates
• An analytic toy model for relativistic accretion in Kerr spacetime
• Fitting and forecasting non-linear coupled dark energy
• The Radius of Baryonic Collapse in Disc Galaxy Formation
• Imprints of primordial non-Gaussianities in X-ray and SZ signals from galaxy clusters
• A numerical study of the effects of primordial non-Gaussianities on weak lensing statistics
• Demographics of Isolated Galaxies Along the Hubble Sequence
• Multipolar moments of weak lensing signal around clusters. Weighing filaments in harmonic space
• Effects of long-wavelength fluctuations in large galaxy surveys
• Dark energy perturbations in $N$-body simulations
• Non-linearities in the Lyman-$\alpha$ forest and in its cross-correlation with dark matter halos
• Impact of galactic distributions in celestial capture of dark matter
• The universal multiplicity function: counting halos and voids
• Absorption signatures of warm-hot gas at low redshift: NeVIII
• The Supersonic Project: rotational effects of supersonic motions on the first structures in the Universe
• Orbital classification in an N-body bar
• Running with BICEP2: Implications for Small-Scale Problems in CDM
• Constrained simulations of the local universe: II. The nature of the local Hubble flow
• Modelling galaxy clustering in redshift space with a Lagrangian bias formalism and $N$-body simulations
• Origins of carbon-enhanced metal-poor stars
• Cosmological Vlasov-Poisson Simulations of Structure Formation with Relic Neutrinos: Nonlinear Clustering and the Neutrino Mass
• The VLT LBG Redshift Survey - IV. Gas and galaxies at z ~ 3 in observations and simulations
• The evolution of the UV luminosity function of globular clusters in the E-MOSAICS simulations
• The joint statistics of mildly non-linear cosmological densities and slopes in count-in-cells
• Not a Copernican observer: biased peculiar velocity statistics in the local Universe
• The seeds of supermassive black holes and the role of local radiation and metal spreading
• Major mergers between dark matter haloes -- II. Profile and concentration changes
• Violent and mild relaxation of an isolated self-gravitating uniform and spherical cloud of particles
• Modelling the fraction of Lyman Break Galaxies with strong Lyman alpha emission at 5 < z < 7
• Magnetic field amplification and X-ray emission in galaxy minor mergers
• Galaxy and Mass Assembly (GAMA): Formation and Growth of Elliptical Galaxies in the Group Environment
• Probing large scale filaments with HI and ${}^3$HeII
• Three-dimensional simulations of the interaction between the nova ejecta, the accretion disk, and the companion star
• The AGN Luminosity Fraction in Merging Galaxies
• Zoomed cosmological simulations of Milky Way sized halos in f(R)-gravity
• The Last Journey. I. An Extreme-Scale Simulation on the Mira Supercomputer
• Numerical hydrodynamic simulations based on semi-analytic galaxy merger trees: method and Milky-Way like galaxies
• Encoding large scale cosmological structure with Generative Adversarial Networks
• Density-dependent clustering: I. Pulling back the curtains on motions of the BAO peak
• Excess of high-$z$ galaxies as a test for bumpy power spectrum of density perturbations
• Galactic forces rule dynamics of Milky Way dwarf galaxies
• Fisher Forecasts for Primordial non-Gaussianity from Persistent Homology
• The cosmic neutrino background as a collection of fluids in large-scale structure simulations
• The 21-cm forest as a simultaneous probe of dark matter and cosmic heating history
• Binary-disk interaction: Gap-Opening criteria
• Vlasov versus N-body: the Hénon sphere
• SOAP: A Python Package for Calculating the Properties of Galaxies and Halos Formed in Cosmological Simulations
• The metallicity distribution of HI systems in the EAGLE cosmological simulation
• Cosmic CARNage II: the evolution of the galaxy stellar mass function in observations and galaxy formation models
• Bullet Clusters in the MareNostrum Universe
• A stream come true: Connecting tidal tails, shells, streams, and planes with galaxy kinematics and formation history
• Properties of brightest group galaxies in cosmic web filaments
• Constraining the cross-section of dark matter with giant radial arcs in galaxy clusters
• The degeneracy between star-formation parameters in dwarf galaxy simulations and the Mstar-Mhalo relation
• On the spin-temperature evolution during the epoch of reionization
• On the Systematic Errors of Cosmological-Scale Gravity Tests using Redshift Space Distortion: Non-linear Effects and the Halo Bias
• Beyond CMB cosmic variance limits on reionization with the polarized SZ effect
• Galaxy halo expansions: a new biorthogonal family of potential-density pairs
• Star clusters forming in a low metallicity starburst -- rapid self-enrichment by (very) massive stars
• Velocity and mass bias in the distribution of dark matter halos
• Fast and reliable symplectic integration for planetary system $N$-body problems
• Gravitational wave fossils in nonlinear regime: halo tidal bias and intrinsic alignments from gravitational wave separate universe simulations
• The formation of the brightest cluster galaxy and intracluster light in cosmological N-body simulations with the Galaxy Replacement Technique
• The galaxy morphology-density relation in the EAGLE simulation
• The interconnection between galaxy mergers, AGN activity and rapid quenching of star formation in simulated post-merger galaxies
• What shapes the far-infrared spectral energy distributions of galaxies?
• New Signatures of the Milky Way Formation in the Local Halo and Inner Halo Streamers in the Era of Gaia
• Decomposition of galactic X-ray emission with Phox: Contributions from hot gas and XRBs
• The extended molecular envelope of the asymptotic giant branch star ${\pi }^1$ Gruis as seen by ALMA II. The spiral-outflow observed at high-angular resolution
• Is WMAP3 normalization compatible with the X-Ray cluster abundance?
• The origin of the [CII]-deficit in a simulated dwarf galaxies starburst
• Universal properties of violently relaxed gravitational structures
• GalWeight: A New and Effective Weighting Technique for Determining Galaxy Cluster and Group Membership
• Growth of Early Supermassive Black Holes and the High-Redshift Eddington Ratio Distribution
• The actual Rees--Sciama effect from the Local Universe
• Kinematics and physical properties of Southern interacting galaxies: the minor merger AM 2306-721
• Probing massive neutrinos with the Minkowski functionals of large-scale structure
• Enhanced star formation in $z\sim 6$ quasar companions
• Calibrated, cosmological hydrodynamical simulations with variable IMFs III: Spatially-resolved properties and evolution
• A black box for dark sector physics: Predicting dark matter annihilation feedback with conditional GANs
• SIMBA-C: An updated chemical enrichment model for galactic chemical evolution in the SIMBA simulation
• COWS: A filament finder for Hessian cosmic web identifiers
• Numerical simulations challenged on the prediction of massive subhalo abundance in galaxy clusters: the case of Abell 2142
• High resolution spectroscopy of the three dimensional cosmic web with close QSO groups
• Simulations of the Galaxy Cluster CIZA J2242.8+5301 I: Thermal Model and Shock Properties
• A semi-analytic model comparison: testing cooling models against hydrodynamical simulations
• Effect of Measurement Errors on Predicted Cosmological Constraints from Shear Peak Statistics with LSST
• Collapse and fragmentation of molecular clouds under pressure
• The Three Hundred project: Galaxy groups do not survive cluster infall
• The assembly history of the Galactic inner halo inferred from alpha-patterns
• Limits on non-canonical heating and turbulence in the intergalactic medium from the low redshift Lyman-alpha forest
• Galaxy properties in the cosmic web of EAGLE simulation
• PNG-UNITsims: Halo clustering response to primordial non-Gaussianities as a function of mass
• How the first stars shaped the faintest gas-dominated dwarf galaxies
• Self-interacting dark matter interpretation of Crater II
• Redshift-space distortions of galaxies, clusters and AGN: testing how the accuracy of growth rate measurements depends on scales and sample selections
• Dark matter halo occupation: environment and clustering
• The origin of X-ray coronae around simulated disc galaxies
• Velocity dispersion and dynamical mass for 270 galaxy clusters in the Planck PSZ1 catalogue
• Inevitable imprints of patchy reionization on the cosmic microwave background anisotropy
• Sharpening the dark matter signature in gravitational waveforms II: Numerical simulations with the NbodyIMRI code
• The PDF perspective on the tracer-matter connection: Lagrangian bias and non-Poissonian shot noise
• The Parsec-Scale Relationship Between I_CO and A_V in Local Molecular Clouds
• Vector dark energy and high-z massive clusters
• Core Formation in High-z Massive Haloes: Heating by Post Compaction Satellites and Response to AGN Outflows
• Testing one-loop galaxy bias: cosmological constraints from the power spectrum
• What do cluster counts really tell us about the Universe?
• The impact of ionizing radiation on the formation of a supermassive star in the early Universe
• The clustering properties of the first galaxies
• Likelihood-free Inference with Mixture Density Network
• Testing Hydrodynamics Schemes in Galaxy Disc Simulations
• Weak lensing calibration of mass bias in the REFLEX+BCS X-ray galaxy cluster catalogue
• New quasar proximity zone size measurements at $z\sim 6$ using the enlarged XQR-30 sample
• Impact of baryons in cosmic shear analyses with tomographic aperture mass statistics
• What galaxy masses perturb the local cosmic expansion?
• Black hole spin evolution in warped accretion discs
• Cosmological Vlasov-Poisson equations for dark matter: Recent developments and connections to selected plasma problems
• Large-scale variation in reionization history caused by Baryon-dark matter streaming velocity
• The stellar mass function and star formation rate-stellar mass relation of galaxies at z ~ 4 - 7
• Balmer breaks in simulated galaxies at z>6
• Reproducing the CO-to-H${}_2$ conversion factor in cosmological simulations of Milky Way-mass galaxies
• The moving mesh code Shadowfax
• Chemical evolution of giant molecular clouds in simulations of galaxies
• Virialization of high redshift dark matter haloes
• Massive black hole and gas dynamics in galaxy nuclei mergers. I. Numerical implementation
• Modelling the accretion and feedback of supermassive black hole binaries in gas-rich galaxy mergers
• A spatially resolved analysis of star-formation burstiness by comparing UV and H$\alpha$ in galaxies at z$\sim$1 with UVCANDELS
• Perturbation theory with dispersion and higher cumulants: non-linear regime
• The Effect of Thermal Velocities on Structure Formation in N-body Simulations of Warm Dark Matter
• AGN-driven quenching of satellite galaxies
• The large-scale environment from cosmological simulations II: The redshift evolution and distributions of baryons
• The Three Hundred Project: The gas disruption of infalling objects in cluster environments
• Multi-wavelength mock galaxy catalogs of the low-redshift Universe
• The Effect of Dark Matter Halo Shape on Bar Buckling and Boxy/Peanut Bulges
• Importance of Mock Observations in Validating Galaxy Properties for Cosmological Simulations
• Satellite galaxies in groups in the CIELO Project I. Gas removal from galaxies and its re-distribution in the intragroup medium
• Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
• Detecting low-mass haloes with strong gravitational lensing II: constraints on the density profiles of two detected subhaloes
• Detecting Galaxy Groups and AGNs populating the local Universe in the eROSITA era
• Non-Linear Matter Power Spectrum Modeling in Interacting Dark Energy Cosmologies
• The SRG/eROSITA All-Sky Survey: Constraints on AGN Feedback in Galaxy Groups
• Taking the Milky Way for a spin: disc formation in the ARTEMIS simulations
• HYMALAIA: A Hybrid Lagrangian Model for Intrinsic Alignments
• Quadratic shape biases in three-dimensional halo intrinsic alignments
• (DarkAI) Mapping the large-scale density field of dark matter using artificial intelligence
• Probing massive neutrinos with the Minkowski functionals of the galaxy distribution
• A jolt to the system: ram pressure on low-mass galaxies in simulations of the Local Group
• The Three Hundred project: A Machine Learning method to infer clusters of galaxies mass radial profiles from mock Sunyaev-Zel'dovich maps
• How identifying circumgalactic gas by line-of-sight velocity instead of the location in 3D space affects O VI measurements
• The In-situ Origins of Dwarf Stellar Outskirts in FIRE-2
• The survival of globular clusters in a cuspy Fornax
• The Cosmic Dispersion Measure in the EAGLE Simulations
• The redshift evolution of the baryonic Tully-Fisher relation in Simba
• The Impact of Outflows driven by Active Galactic Nuclei on Metals in and around Galaxies
• Density reconstruction from biased tracers and its application to primordial non-Gaussianity
• Time-symmetric integration in astrophysics
• A Faster Fourier Transform? Computing Small-Scale Power Spectra and Bispectra for Cosmological Simulations in $\mathcal{O}(N^2)$ Time
• Investigating Cosmological GAN Emulators Using Latent Space Interpolation
• Exploring extensions to the standard cosmological model and the impact of baryons on small scales
• Evolution of the grain size distribution in galactic discs
• Simultaneous evolution of the virial parameter and star formation rate in molecular clumps undergoing global hierarchical collapse
• The Schrödinger-Poisson method for Large-Scale Structure
• Massive neutrinos and degeneracies in Lyman-alpha forest simulations
• Partitioning the universe into gravitational basins using the cosmic velocity field
• Antlia2's role in driving the ripples in the outer gas disk of the Galaxy
• Unequal time correlators and the Zeldovich approximation
• Anatomy of Cosmic Tidal Reconstruction
• The effect of dark matter-dark radiation interactions on halo abundance -- a Press-Schechter approach
• Testing a quintessence model with Yukawa interaction from cosmological observations and N-body simulations
• The Indirect Influence of Quasars on Reionization
• Hydrodynamic simulations of the central molecular zone with realistic Galactic potential
• Quintessential Scale Dependence from Separate Universe Simulations
• Recovering the mass profile and orbit anisotropy of mock dwarf galaxies with Schwarzschild modelling
• Cosmology with Phase Statistics: Parameter Forecasts and Detectability of BAO
• The low abundance and insignificance of dark discs in simulated Milky Way galaxies
• Santa Barbara Cluster Comparison Test with DISPH
• Sussing Merger Trees: Stability and Convergence
• Cosmology with velocity dispersion counts: an alternative to measuring cluster halo masses
• The Local Value of $H_0$ in an Inhomogeneous Universe
• Effective Window Function for Lagrangian Halos
• Geometrical on-the-fly shock detection in SPH
• Dark influences II: gas and star formation in minor mergers of dwarf galaxies with dark satellites
• Dynamical evolution of massive black holes in galactic-scale N-body simulations - introducing the regularized tree code "rVINE"
• Black hole formation and growth with non-Gaussian primordial density perturbations
• Gas around galaxy haloes - II: hydrogen absorption signatures from the environments of galaxies at redshifts 2 < z < 3
• Simulating the 21cm forest detectable with LOFAR and SKA in the spectra of high-z GRBs
• Novel Adaptive softening for collisionless N-body simulations: Eliminating spurious halos
• Patchy blazar heating: diversifying the thermal history of the intergalactic medium
• Progenitors of Supernovae Type Ia and Chemical Enrichment in Hydrodynamical Simulations -I. The Single Degenerate Scenario
• Subhaloes gone Notts: Subhaloes as tracers of the dark matter halo shape
• The First Billion Years project: dark matter haloes going from contraction to expansion and back again
• On the mass assembly of low-mass galaxies in hydrodynamical simulations of structure formation
• Cold accretion in early galaxy formation and its Lyman-alpha signatures
• Semi-analytic galaxy formation in early dark energy cosmologies
• The Milky Way and Andromeda galaxies in a constrained hydrodynamical simulation: morphological evolution
• Effects of Baryon Mass Loss on Profiles of Large Galactic Dark Matter Haloes
• Boosting hierarchical structure formation with scalar-interacting dark matter
• Neutrinos in Non-linear Structure Formation - a Simple SPH Approach
• Kinematics in galactic tidal tails - A source for Hypervelocity stars?
• Simulating large-scale structure formation with magnetic fields
• Likelihood reconstruction method of real-space density and velocity power spectra from a redshift galaxy survey
• On the inconsistency between the estimates of cosmic star formation rate and stellar mass density of high redshift galaxies
• Termination of star formation by BH feedback in equal- and unequal-mass mergers of disk and elliptical galaxies
• Incidence Rate of GRB-host-DLAs at High Redshift
• Quantifying Baryonic Feedback on Warm-Hot Circumgalactic Medium in CAMELS Simulations
• The BAHAMAS project: Effects of dynamical dark energy on large-scale structure
• The Doppler effect on indirect detection of dark matter using dark matter only simulations
• From dusty filaments to massive stars: The case of NGC 7538 S
• Accretion of clumpy cold gas onto massive black hole binaries: a possible fast route to binary coalescence
• The ALPINE-ALMA [CII] Survey: the population of [CII]-undetected galaxies and their role in the ${\mathrm{L}}_{[\mathrm{CII}]}$-SFR relation
• What to expect from dynamical modelling of cluster haloes I. The information content of different dynamical tracers
• Towards time symmetric N-body integration
• Enabling parallel computing in CRASH
• Testing dark energy using pairs of galaxies in redshift space
• Schmidt-Kennicutt relations in SPH simulations of disc galaxies with effective thermal feedback from supernovae
• Leavers and remainers: Galaxies split by group-exit
• A comparison of SPH artificial viscosities and their impact on the Keplerian disk
• H2 chemistry in galaxy simulations: an improved supernova feedback model
• Insights into the origin of halo mass profiles from machine learning
• Efficient adiabatic hydrodynamical simulations of the high-redshift intergalactic medium
• Simulations of the merging galaxy cluster Abell 2034: what determines the level of separation between gas and dark matter
• Cosmological simulations of quasar fueling to sub-parsec scales using Lagrangian hyper-refinement
• Astraeus VI: Hierarchical assembly of AGN and their large-scale effect during the Epoch of Reionization
• On the Evolution of the Globular Cluster System in NGC 1052-DF2: Dynamical Friction, Globular-Globular Interactions and Galactic Tides
• Constraining the Noise-Free Distribution of Halo Spin Parameters
• Tidal disruptions in circumbinary discs (I): Star formation, dynamics, and binary evolution
• Cold versus Warm Dark Matter simulations of a galaxy group
• Nonlinearities in modified gravity cosmology I: signatures of modified gravity in the nonlinear matter power spectrum
• Properties and merger signatures of galaxies hosting LISA coalescing massive black hole binaries
• Dark matter halos in the multicomponent model. I. Substructure
• Modelling Non-Linear Effects of Dark Energy
• Constraining Reionization in Progress at z=5.7 with Lyman-$\alpha$ Emitters: Voids, Peaks, and Cosmic Variance
• The buildup of galaxies and their spheroids: the contributions of mergers, disc instabilities and star formation
• A possible sub-kiloparsec dual AGN buried behind the galaxy curtain
• Tidally induced morphology of M33 in hydrodynamical simulations of its recent interaction with M31
• Cosmic Microwave Background--Weak Lensing Correlation: Analytical and Numerical Study of Non-linearity and Implications for Dark Energy
• Effects of Multiphase Gas and Projection on X-ray Observables in Simulated Galaxy Clusters as Seen by eROSITA
• The early growth of supermassive black holes in cosmological hydrodynamic simulations with constrained Gaussian realizations
• Extreme value statistics of weak lensing shear peak counts
• The cosmological free-free signal from galaxy groups and clusters
• Physical properties of galaxies: toward a consistent comparison between hydrodynamical simulations and SDSS
• Sensitivity of primordial black hole abundance on the reheating phase
• The Connection between Mergers and AGN Activity in Simulated and Observed Massive Galaxies
• An Efficient Radiative Cooling Approximation for Use in Hydrodynamic Simulations
• Evolution of Late-type Galaxies in a Cluster Environment: Effects of High-speed Multiple Encounters with Early-type Galaxies
• Swarm Intelligence-based Extraction and Manifold Crawling Along the Large-Scale Structure
• Simulated metal and HI absorption lines at the conclusion of Reionization
• Seeking Observable Imprints of Small-Scale Structure on the Properties of Dark Matter Haloes
• Constraining quasar host halo masses with the strength of nearby Lyman-alpha forest absorption
• Primordial power spectrum and cosmology from black-box galaxy surveys
• How do Primordial Black Holes change the Halo Mass Function and Structure?
• Misaligned accretion on to supermassive black hole binaries
• Reionization Histories of Milky Way Mass Halos
• Numerical Challenges in Modeling Gravothermal Collapse in Self-Interacting Dark Matter Halos
• The NGC 4013 tale: a pseudo-bulged, late-type spiral shaped by a major merger
• Matter Distribution around Galaxies
• The dark side of FIRE: predicting the population of dark matter subhaloes around Milky Way-mass galaxies
• Numerical investigation of lenses with substructures using the perturbative method
• The SELGIFS data challenge: generating synthetic observations of CALIFA galaxies from hydrodynamical simulations
• Perturbation theory for the redshift-space matter power spectra after reconstruction
• Dark Matter Response to Galaxy Assembly History
• First Structure Formation under the Influence of Gas-Dark Matter Streaming Velocity and Density: Impact of the Baryons-trace-dark matter Approximation
• Characterising face-on accretion onto and the subsequent contraction of protoplanetary discs
• The Three Hundred project: connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
• Pushing down the low-mass halo concentration frontier with the Lomonosov cosmological simulations
• A Baryonic Effect on the Merger Timescale of Galaxy Clusters
• The AGORA High-resolution Galaxy Simulations Comparison Project. VI. Similarities and Differences in the Circumgalactic Medium
• Second-order Cosmological Perturbations Engendered by Point-like Masses
• Photometric Properties of the Most Massive High-Redshift Galaxies
• $\text{fRevolution}$ $-$ Relativistic Cosmological Simulations in $f(R)$ Gravity I: Methodology
• Combining spectroscopic and photometric surveys using angular cross-correlations II: Parameter constraints from different physical effects
• A Hybrid Fast Multipole Method for Cosmological N-body Simulations
• Stellar Bars in Spinning Halos: Delayed Buckling and Absence of Slowdown
• Astraeus VIII: A new framework for Lyman-$\alpha$ emitters applied to different reionisation scenarios
• Metal enrichment of the intra-cluster medium by thermally and cosmic-ray driven galactic winds
• Non-isotropic feedback from accreting spinning black holes
• Major mergers between dark matter haloes -- I. Predictions for size, shape, and spin
• SN-driven mechanism of cusp-core transformation: an appraisal
• PENTACLE: Parallelized Particle-Particle Particle-Tree Code for Planet Formation
• The halo mass function conditioned on density from the Millennium Simulation: insights into missing baryons and galaxy mass functions
• Using Lagrangian perturbation theory for precision cosmology
• Informing dark matter direct detection limits with the ARTEMIS simulations
• Modeling of weak lensing statistics. I. Power spectrum and bispectrum
• Formation and assembly history of stellar components in galaxies as a function of stellar and halo mass
• The changing circumgalactic medium over the last 10 Gyr I: physical and dynamical properties
• Impact of dark matter models on the EoR 21-cm signal bispectrum
• A comparative study of cosmological constraints from weak lensing using Convolutional Neural Networks
• The detectability of strong 21 centimetre forest absorbers from the diffuse intergalactic medium in late reionisation models
• Three-dimensional reconstruction of the intra-cluster medium
• A Very Fast And Angular Momentum Conserving Tree Code
• Lopsided galactic bars
• Improved Performances in Subsonic Flows of an SPH Scheme with Gradients Estimated using an Integral Approach
• Simulation view of galaxy clusters with low X-ray surface brightness
• ELUCID -- Exploring the Local Universe with the reConstructed Initial Density field. II: Reconstruction diagnostics, applied to numerical halo catalogs
• Mass and size growth of early-type galaxies by dry mergers in cluster environments
• Self-Similar Bumps and Wiggles: Isolating the Evolution of the BAO Peak with Power-law Initial Conditions
• The present-day gas content of simulated field dwarf galaxies
• Atomic and molecular gas as traced by [C II] emission
• Relation between standard perturbation theory and regularized multi-point propagator method
• Resolved simulations of jet-ISM interaction: Implications for gas dynamics and star formation
• Redshift-space limits of bound structures
• Numerical challenges for energy conservation in N-body simulations of collapsing self-interacting dark matter halos
• The cosmic spectral energy distribution in the EAGLE simulation
• Counts-in-Cylinders in the Sloan Digital Sky Survey with Comparisons to N-body Simulations
• Beyond Kaiser bias: mildly non-linear two-point statistics of densities in distant spheres
• Long-lived transient structure in collisionless self-gravitating systems
• The Three Hundred Project: the evolution of physical baryon profiles
• Modelling the evolution of PAH abundance in galaxies
• A neural network emulator for the Lyman-$\alpha$ 1D flux power spectrum
• Effect of the Metallicity on the X-ray Emission from the Warm-Hot Intergalactic Medium
• The $z\lesssim 1$ drop of cosmic dust abundance in a semi-analytic framework
• The Diffuse Gamma-Ray Flux from Clusters of Galaxies
• Anisotropic q-Gaussian velocity distributions in LambdaCDM halos
• Composite star formation histories of early-type galaxies from minor mergers: prospects for WFC3
• Co-accretion + giant impact origin of the Uranus system: Tilting Impact
• Overlapping inflows as catalysts of AGN activity - II: Relative importance of turbulence and inflow-disc interaction
• Simulations Find Our Accounting of Dust-Obscured Star Formation May Be Incomplete
• Stellar Mass Assembly of Brightest Cluster Galaxies at Late Times
• Renormalisation of linear halo bias in N-body simulations
• The dust attenuation law in $z\sim 6$ quasars
• Fast and realistic large-scale structure from machine-learning-augmented random field simulations
• On the coherent rotation of diffuse matter in numerical simulations of galaxy clusters
• Weak Lensing by Intergalactic Mini-Structures in Quadruple Lens Systems: Simulation and Detection
• The evolution of the baryon fraction in halos as a cause of scatter in the galaxy stellar mass in the EAGLE simulation
• The role of baryons in self-interacting dark matter mergers
• Applying scale-free mass estimators to the Local Group in Constrained Local Universe Simulations
• Tidal features of classical Milky Way satellites in a $\Lambda$CDM universe
• Groups and protocluster candidates in the CLAUDS and HSC-SSP joint deep surveys
• Energy balance SED modelling can be effective at high redshifts regardless of UV-FIR offsets
• A Moving Mesh Hydrodynamic Solver for ChaNGa
• Dark influences: imprints of dark satellites on dwarf galaxies
• Raytracing simulations of coupled dark energy models
• Tidally induced bars in gas-rich dwarf galaxies orbiting the Milky Way
• Evolution of the baryon fraction in the Local Group: accretion versus feedback at low and high z
• COVMOS: a new Monte Carlo approach for galaxy clustering analysis
• Stellar Spiral Structures in Triaxial Dark Matter Haloes
• Binary Disk interaction II: Gap-Opening criteria for unequal mass binaries
• The Adaptive TreePM: An Adaptive Resolution Code for Cosmological N-body Simulations
• A case study of hurdle and generalized additive models in astronomy: the escape of ionizing radiation
• The position-dependent matter density probability distribution function
• UV Background Fluctuations and Three-Point Correlations in the Large Scale Clustering of the Lyman-alpha Forest
• Implantation of Martian materials in the inner solar system by a mega impact on Mars
• Towards Accurate Field-Level Inference of Massive Cosmic Structures
• Dissecting galaxy formation models with Sensitivity Analysis -- A new approach to constrain the Milky Way formation history
• Cosmological Impact of Population III Binaries
• RABBITS -- I. The crucial role of nuclear star formation in driving the coalescence of supermassive black hole binaries
• Constraining dark energy via baryon acoustic oscillations in the (an)isotropic light-cone power spectrum
• Velocity dispersion of the brightest cluster galaxies in cosmological simulations
• The PAU survey: Ly$\alpha$ intensity mapping forecast
• Simulating extremely metal-poor gas and DLA metal content at redshift z=7
• Modeling Redshift-Space Clustering with Abundance Matching
• Clumpy galaxies in cosmological simulations: The effect of ISM model
• The Borg Cube Simulation: Cosmological Hydrodynamics with CRK-SPH
• Scalar perturbations in cosmological models with dark energy - dark matter interaction
• Systematically Asymmetric: A comparison of \hi\ profile asymmetries in real and simulated galaxies
• Morphology of galaxies with quiescent recent assembly history in a Lambda-CDM universe
• Accurate halo-galaxy mocks from automatic bias estimation and particle mesh gravity solvers
• Simulations of gas sloshing induced by a newly discovered gas poor substructure in galaxy cluster Abell 1644
• What Is Inside Matters: Simulated Green Valley Galaxies Have Centrally Concentrated Star Formation
• Constraints on the Evolution of the Galaxy Stellar Mass Function I: Role of Star Formation, Mergers and Stellar Stripping
• The Mystery of the $\sigma$-Bump -- A new Signature for Major Mergers in Early-type Galaxies?
• BE-HaPPY: Bias Emulator for Halo Power Spectrum including massive neutrinos
• Covariance of the redshift-space matter power spectrum after reconstruction
• The impact of dark energy on galaxy formation. What does the future of our Universe hold?
• Quantum algorithms for scientific computing
• Strongly Time-Variable Ultra-Violet Metal Line Emission from the Circum-Galactic Medium of High-Redshift Galaxies
• Redshift Space Distortion of 21cm line at 1<z<5 with Cosmological Hydrodynamic Simulations
• Evolution of skewness and kurtosis of cosmic density fields
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• The First Stars: formation under cosmic ray feedback
• Galaxy clustering with photometric surveys using PDF redshift information
• The First Billion Years Project: Finding Infant Globular Clusters at z=6
• Mufasa:The strength and evolution of galaxy conformity in various tracers
• 1-DREAM: 1D Recovery, Extraction and Analysis of Manifolds in noisy environments
• CSST large-scale structure analysis pipeline: I. constructing reference mock galaxy redshift surveys
• Covariances for cosmic shear and galaxy-galaxy lensing in the response approach
• 60 candidate high-velocity stars originating from the Sagittarius dwarf spheroidal galaxy in Gaia EDR3
• Probing Primordial Non-Gaussianity with Weak Lensing Minkowski Functionals
• The nonlinear evolution of baryonic overdensities in the early universe: Initial conditions of numerical simulations
• The evolution of a pre-heated Intergalactic Medium
• Structure formation in a mixed dark matter model with decaying sterile neutrino: the 3.5 keV X-ray line and the Galactic substructure
• Intra-cluster Globular Clusters in a Simulated Galaxy Cluster
• The cosmic web around the Coma cluster from constrained cosmological simulations: I. Filaments connected to Coma at $z=0$
• Wavelet analysis of baryon acoustic structures in the galaxy distribution
• Chemical evolution of local post-starburst galaxies: Implications for the mass-metallicity relation
• Reionization of the Milky Way, M31, and their satellites I: reionization history and star formation
• Setting firmer constraints on the evolution of the most massive, central galaxies from their local abundances and ages
• Searching for Dual Active Galactic Nuclei
• Competitive Accretion in Sheet Geometry and the Stellar IMF
• The SAGA Survey. V. Modeling Satellite Systems around Milky Way-mass Galaxies with Updated UniverseMachine
• Buckling instability in tidally induced galactic bars
• The Cosmic Web Around The Brightest Galaxies During The Epoch Of Reionization
• A Better Way to Define Dark Matter Haloes
• Strong lensing in the MareNostrum Universe II: scaling relations and optical depths
• Cosmological Simulations of Massive Compact High-z Galaxies
• Atmosphere Loss in Oblique Super-Earth Impacts
• Spin and structural halo properties at high redshift in a LCDM Universe
• Volume Statistics as a Probe of Large-Scale Structure
• The stellar mass function and evolution of the density profile of galaxy clusters from the Hydrangea simulations at $0<z<1.5$
• Smoothed Particle Radiation Hydrodynamics: Two-Moment method with Local Eddington Tensor Closure
• GalactICS with Gas
• Hybrid analytic and machine-learned baryonic property insertion into galactic dark matter haloes
• Probing modified gravitational-wave propagation with extreme mass-ratio inspirals
• Dynamical friction and evolution of black holes in cosmological simulations: a new implementation in OpenGadget3
• Autocorrelations of stellar light and mass at z~0 and ~1: From SDSS to DEEP2
• Star Formation in Simulated Galaxies: Understanding the Transition to Quiescence at $3\times 10^{10}$ M${}_{\odot }$
• Formation and relaxation of quasi-stationary states in particle systems with power law interactions
• Alignments of dark matter halos with large-scale tidal fields: mass and redshift dependence
• The Arrow of Time in the collapse of collisionless self-gravitating systems: non-validity of the Vlasov-Poisson equation during violent relaxation
• The sparkling Universe: a scenario for cosmic void motions
• Cosmological Probes of Structure Growth and Tests of Gravity
• On the formation of a quasi-stationary twisted disc after a tidal disruption event
• Forming disc galaxies in major mergers: III. The effect of angular momentum on the radial density profiles of disc galaxies
• The potential role of NGC 205 in generating Andromeda's vast thin co-rotating plane of satellite galaxies
• Evolution of Primordial Stars Powered by Dark Matter Annihilation up to the Main-Sequence Stage
• Explaining dark matter halo density profiles with neural networks
• Radio relics in cosmological simulations
• Intermediate-mass black holes in dwarf galaxies: the case of Holmberg II
• The impact of black hole seeding in cosmological simulations
• Exploring Mirror Twin Higgs Cosmology with Present and Future Weak Lensing Surveys
• Time Dependent Radiation Hydrodynamics on a Moving Mesh
• GalMod: a Galactic synthesis population model
• An attractor for dark matter structures
• Evolution of binary seeds in collapsing protostellar gas clouds
• Effects of chaos on the detectability of stellar streams
• Simulating the LOcal Web (SLOW) II: Properties of local galaxy clusters
• Barlenses in the CALIFA survey: combining the photometric and stellar population analysis
• Effects of neutrino mass and asymmetry on cosmological structure formation
• i-SPin: An integrator for multicomponent Schrödinger-Poisson systems with self-interactions
• Mildly Suppressed Star Formation in Central Regions of MaNGA Seyfert Galaxies
• Close Encounters of Tight Binary Stars with Stellar-mass Black Holes
• The Robustness of Cosmological Hydrodynamic Simulation Predictions to Changes in Numerics and Cooling Physics
• Cosmic Star Formation: a simple model of the SFRD(z)
• Constraints on ${\Omega }_{\mathrm{m}}$ and ${\sigma }_8$ from the potential-based cluster temperature function
• Warm Dark Haloes Accretion Histories and their Gravitational Signatures
• The Cluster-EAGLE project: a comparison of dynamical mass estimators using simulated clusters
• Formation of Andromeda II via a gas-rich major merger and an interaction with M31
• Spatial and orbital planes of the Milky Way satellites: unusual but consistent with $\Lambda$CDM
• Can we really measure fnl from the galaxy power spectrum?
• Should $N$-body integrators be symplectic everywhere in phase space?
• The Doubling of Stellar Black Hole Nuclei
• Azimuthal variations of oxygen abundance profiles in star-forming regions of disc galaxies in the EAGLE simulations
• The post-infall evolution of a satellite galaxy
• The Breakdown Scale of HI Bias Linearity
• Giant cold satellites from low-concentration haloes
• Baryonic properties of nearby galaxies across the stellar-to-total dynamical mass relation
• The fate of close encounters between binary stars and binary supermassive black holes
• Simulations of Galaxy Cluster Collisions with a Dark Plasma Component
• Unveiling the hosts of parsec-scale massive black hole binaries: morphology and electromagnetic signatures
• On the detectability of strong lensing in near-infrared surveys
• Fingerprints of the hierarchical building up of the structure on the gas kinematics of galaxies
• A hide-and-seek game: Looking for Population III stars during the Epoch of Reionization through the HeII$\lambda$1640 line
• Cross-correlation between the 21-cm signal and [OIII] emitters during early cosmic reionization
• Observational constraints of an anisotropic boost due to the projection effects using redMaPPer clusters
• The BAHAMAS project: Effects of a running scalar spectral index on large-scale structure
• SUPER VII. Morphology and kinematics of H$\alpha$ emission in AGN host galaxies at Cosmic noon using SINFONI
• Revising the merger scenario of the galaxy cluster Abell 1644: a new gas poor structure discovered by weak gravitational lensing
• The imprint of cosmological non-Gaussianities on primordial structure formation
• Dynamical friction from self-interacting dark matter
• Constrained simulations of the local universe: I. Mass and motion in the Local Volume
• The XXL Survey XIX. A realistic population of simulated X-ray AGN: Comparison of models with observations
• The effect of gravitational tides on dwarf spheroidal galaxies
• Constraining the cosmic UV background at z>3 with MUSE Lyman-α emission observations
• A general-purpose timestep criterion for simulations with gravity
• Multi-Scale Morphological Analysis of SDSS DR5 Survey using the Metric Space Technique
• Shedding light on low-mass subhalo survival and annihilation luminosity with numerical simulations
• Hydrodynamical simulations of coupled and uncoupled quintessence models II: Galaxy clusters
• ART${}^2$: A 3D Parallel Multi-wavelength Radiative Transfer Code for Continuum and Atomic and Molecular Lines
• Revised estimates of CMB $B$-mode polarization induced by patchy reionization
• Connections between galaxy properties and halo formation time in the cosmic web
• Mapping Lyman-alpha forest three-dimensional large scale structure in real and redshift space
• Hybrid-basis inference for large-scale galaxy clustering: combining spherical and Cartesian Fourier analyses
• Astraeus III: The environment and physical properties of reionization sources
• Bayesian redshift-space distortions correction from galaxy redshift surveys
• Reconsidering the dynamical states of galaxy clusters using PCA and UMAP
• Constraining Primordial Non-Gaussianity with Moments of the Large Scale Density Field
• Initial conditions for cosmological N-body simulations of the scalar sector of theories of Newtonian, Relativistic and Modified Gravity
• The effect of gas-dynamics on semi-analytic modeling of cluster galaxies
• Simulating the Effect of Non-Linear Mode-Coupling in Cosmological Parameter Estimation
• Stellar scattering and the formation of exponential discs in self-gravitating systems
• Planetary Embryo Collisions and the Wiggly Nature of Extreme Debris Disks
• The environmental dependence of neutral hydrogen in the GIMIC simulations
• Primordial magnetic fields: consistent initial conditions and impact on high-z structures
• Measurement of Void Bias Using Separate Universe Simulations
• Signatures of tidal disruption in the Milky Way globular cluster NGC 6981 (M72)
• Optimizing simulation parameters for weak lensing analyses involving non-Gaussian observables
• How Metals Are Transported In And Out Of A Galactic Disk: Dependence On The Hydrodynamic Schemes In Numerical Simulations
• A Consistent Comparison of Bias Models using Observational Data
• A warm mode of gas accretion on forming galaxies
• On the generation of triaxiality in the collapse of cold spherical self-gravitating systems
• COZMIC. I. Cosmological Zoom-in Simulations with Initial Conditions Beyond Cold Dark Matter
• Violent relaxation of ellipsoidal clouds
• The Effect of Particle Noise in N-body Simulations of Gravitational Lensing
• syren-new: Precise formulae for the linear and nonlinear matter power spectra with massive neutrinos and dynamical dark energy
• Mild evolution of the stellar metallicity gradients of disc galaxies
• The importance of secondary halos for strong lensing in massive galaxy clusters across redshift
• Modelling the star-formation activity and ionizing properties of high-redshift galaxies
• The Late-Time Light Curves of Type Ia Supernovae: Confronting Models with Observations
• The tidal evolution of the Fornax dwarf spheroidal and its globular clusters
• An estimate of the stochastic gravitational wave background from the MassiveBlackII simulation
• Constraints on sigma_8 from galaxy clustering in N-body simulations and semi-analytic models
• Influence of baryonic physics in galaxy simulations: a semi-analytic treatment of the molecular component
• On the total cosmological information in galaxy clustering: an analytical approach
• Tracking Halo Orbits and Their Mass Evolution around Large-scale Filaments
• Oxygen yields as a constraint on feedback processes in galaxies
• Quijote-PNG: The Information Content of the Halo Mass Function
• Properties of the Magellanic Corona
• Spatial matter density mapping of the STAGES Abell A901/2 supercluster field with 3D lensing
• N-body simulations of gravitational redshifts and other relativistic distortions of galaxy clustering
• The Correspondence between Convergence Peaks from Weak Lensing and Massive Dark Matter Haloes
• The Hateful Eight: Connecting Massive Substructures in Galaxy Clusters like Abell 2744 to their Dynamical Assembly State using the Magneticum Simulations
• Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
• MoLUSC: A MOck Local Universe Survey Constructor
• Tracing the gas at redshift 1.7-3.5 with the Lyman-alpha forest: the FLO approach
• Simulations of shell galaxies with GADGET-2: Multi-generation shell systems
• Star formation in mergers with cosmologically motivated initial conditions
• Precise Clustering and Density Evolution of redMaPPer Galaxy Clusters versus MXXL Simulation
• Giant impacts stochastically change the internal pressures of terrestrial planets
• Pointing to the minimum scatter: the generalized scaling relations for galaxy clusters
• Simplified galaxy formation with mesh-less hydrodynamics
• The dynamical state of Abell 2399: a bullet-like cluster
• General Relativistic Cosmological N-body Simulations I: time integration
• Brought to Light II: Revealing the Origins of Cloaked Spiral Features in Cluster Passive Dwarf Galaxies
• Geometry and growth contributions to cosmic shear observables
• Accuracy and precision of triaxial orbit models I: SMBH mass, stellar mass and dark-matter halo
• Topology and geometry of the dark matter web: a multistream view
• Observing relativistic features in large-scale structure surveys -- II: Doppler magnification in an ensemble of relativistic simulations
• Action-based Dynamical Modeling for the Milky Way Disk: The Influence of Spiral Arms
• Effect of supersonic relative motion between baryons and dark matter on collapsed objects
• On the deuterium abundance and the importance of stellar mass loss in the interstellar and intergalactic medium
• Evolution of stellar-gaseous disks in cosmological haloes
• Investigating the influence of magnetic fields upon structure formation with AMIGA - a C code for cosmological magnetohydrodynamics
• The clustering of baryonic matter. II: halo model and hydrodynamic simulations
• Is a top-heavy initial mass function needed to reproduce the submillimeter galaxy number counts?
• Variations of cosmic large-scale structure covariance matrices across parameter space
• Using Artificial Neural Networks to Constrain the Halo Baryon Fraction during Reionization
• Spherical symmetry breaking in cold gravitational collapse of isolated systems
• The effect of non-sphericity on mass and anisotropy measurements in dSph galaxies with Schwarzschild method
• Indra: a Public Computationally Accessible Suite of Cosmological $N$-body Simulations
• The alignment is in their stars: on the spin-alignment of stars in star clusters
• SDSS IV MaNGA: Discovery of an $H_{\alpha }$ blob associated with a dry galaxy pair -- ejected gas or a `dark' galaxy candidate?
• Statistical properties of SZ and X-ray cluster detections
• Towards 1% accurate galaxy cluster masses: Including baryons in weak-lensing mass inference
• The Sejong Suite: Cosmological Hydrodynamical Simulations with Massive Neutrinos, Dark Radiation, and Warm Dark Matter
• Modelling the next-to-leading order matter three-point correlation function using FFTLog
• Properties and observables of massive galaxies in self-interacting dark matter cosmologies
• Analytic and numerical realisations of a disk galaxy
• Star Formation and Gas Phase History of the Cosmic Web
• Role of ionizing background on the statistics of metal absorbers in hydrodynamical simulations
• ELUCID VII: Using Constrained Hydro Simulations to Explore the Gas Component of the Cosmic Web
• Separate Universe calibration of the dependence of halo bias on cosmic web anisotropy
• Calibrated, cosmological hydrodynamical simulations with variable IMFs II: Correlations between the IMF and global galaxy properties
• Rotation curve bifurcations as indicators of close recent galaxy encounters
• Flow-Based Likelihoods for Non-Gaussian Inference
• The role of physical and numerical viscosity in hydrodynamical instabilities
• Metal enrichment signatures of the first stars on high-z DLAs
• Star forming filaments in warm dark matter models
• Three- and two-point spatial correlations of intergalactic medium at $z\sim 2$ using projected quasar triplets
• Luminosity Distribution of Gamma-Ray Burst Host Galaxies at redshift z=1 in Cosmological Smoothed Particle Hydrodynamic Simulations: Implications for the Metallicity Dependence of GRBs
• From large-scale to protostellar disk fragmentation into close binary stars
• Simulating the Anisotropic Clustering of Luminous Red Galaxies with Subhalos: A Direct Confrontation with Observation and Cosmological Implications
• The spatial clustering of ROSAT all-sky survey Active Galactic Nuclei: V. The evolution of broad-line AGN clustering properties in the last 6 Gyr
• Field-Based Physical Inference From Peculiar Velocity Tracers
• Merger types forming the Virgo cluster in recent gigayears
• CMB lensing bi-spectrum: assessing analytical predictions against full-sky lensing simulations
• Decaying warm dark matter and structure formation
• Separate Universe Void Bias
• Prospects of detecting soft X-ray emission from typical WHIM filaments around massive clusters and the Coma cluster soft excess
• The impact and response of minihalos and the inter-halo medium on cosmic reionization
• Effect of primordial non-Gaussianities on the far-UV luminosity function of high-redshift galaxies: implications for cosmic reionization
• Expected properties of the Two-Point Autocorrelation Function of the IGM
• Evaluating hydrodynamical simulations with green valley galaxies
• On the general nature of 21cm-Lyman-$\alpha$ emitters cross-correlations during reionisation
• The cosmological simulation code $\mathrm{CO}N\mathrm{CEPT}1.0$
• Weak lensing detection of intra-cluster filaments with ground based data
• The impact of Self-Interacting Dark Matter on the Intrinsic Alignments of Galaxies
• Probabilistic cosmic web classification using fast-generated training data
• Halo mass and weak galaxy-galaxy lensing profiles in rescaled cosmological $N$-body simulations
• Buckling bars in nearly face-on galaxies observed with MaNGA
• An improved prescription for merger time-scales from controlled simulations
• Examining the effects of dark matter spikes on eccentric intermediate mass ratio inspirals using N-body simulations
• On the accuracy of dark matter halo merger trees and the consequences for semi-analytic models of galaxy formation
• Correlation function: biasing and fractal properties of the cosmic web
• Rapidly quenched galaxies in the Simba cosmological simulation and observations
• Heating and enriching the intracluster medium
• White dwarf deflagrations for Type Iax supernovae: Polarisation signatures from the explosion and companion interaction
• Grid-based calculations of redshift-space matter fluctuations from perturbation theory: UV sensitivity and convergence at the field level
• Anisotropy in the matter distribution beyond the baryonic acoustic oscillation scale
• The Halo Occupation Distribution of Black Holes: Dependence on Mass
• Is the star formation rate in $z\sim 6$ quasars overestimated?
• Evolution of Prolate Molecular Clouds at Hii Boundaries: II. Formation of BRCs of asymmetrical morphology
• Simulated evolution of the dark matter large-scale structure
• Redshift evolution of the hot intracluster gas metallicity in the C-EAGLE cluster simulations
• How Close Dark Matter Halos and MOND Are to Each Other: Three-Dimensional Tests Based on Gaia DR2
• Implications of the $z>5$ Lyman-$\alpha$ forest for the 21-cm power spectrum from the epoch of reionization
• Constraints on small-scale cosmological fluctuations from SNe lensing dispersion
• The large-scale structure around the Fornax-Eridanus Complex
• Fully relativistic treatment of decaying cold dark matter in $N$-body simulations
• Effect of Population III Multiplicity on Dark Star Formation
• Detecting clusters and groups of galaxies populating the local Universe in large optical spectroscopic surveys
• The effect of recombination radiation on the temperature and ionization state of partially ionized gas
• Signatures of a surviving helium-star companion in Type Ia supernovae and constraints on the progenitor companion of SN 2011fe
• On the small scale clustering of quasars: constraints from the MassiveBlack II simulation
• Globular cluster metallicity distributions in the E-MOSAICS simulations
• Magnetic fields do not suppress global star formation in low metallicity dwarf galaxies
• ColdSIM predictions of [C II] emission in primordial galaxies
• The effects of binary stars on galaxies and metal-enriched gas during reionization
• HyPhy: Deep Generative Conditional Posterior Mapping of Hydrodynamical Physics
• Simulating intergalactic quasar scintillation
• High Resolution Study of Planetesimal Formation by Gravitational Collapse of Pebble Clouds
• Characterising the Structure of Halo Merger Trees Using a Single Parameter: The Tree Entropy
• Constraining Dark Energy With Stacked Concave Lenses
• Galaxy formation with cold gas accretion and evolving stellar initial mass function
• The impact of spurious shear on cosmological parameter estimates from weak lensing observables
• The distribution and properties of DLAs at z $\le$ 2 in the EAGLE simulations
• Clumping factors of HII, HeII and HeIII
• Ly$\alpha$ forest power spectrum as an emerging window into the epoch of reionization and cosmic dawn
• Gaussianizing the non-Gaussian lensing convergence field II: the applicability to noisy data
• Host galaxies of long gamma-ray bursts in the Millennium Simulation
• Dynamics of finite and infinite self-gravitating systems with cold quasi-uniform initial conditions
• Evolution of Supermassive Black Holes from Cosmological Simulations
• Constraining the subgrid physics in simulations of isolated dwarf galaxies
• Effects of NII and H$\alpha$ Line Blending on the WFIRST Galaxy Redshift Survey
• The complete census of molecular hydrogen in a simulated disc galaxy
• Impact of Massive Neutrinos and Dark Radiation on the High-redshift Cosmic Web. I. Lyman-Alpha Forest Observables
• Spectral imaging of galaxy clusters with Planck
• Symmetry Breaking in d-Dimensional Self-gravitating Systems
• Assembly of the outer Galactic stellar halo in the hierarchical model
• Mapping the low surface brightness Universe in the UV band with Lya emission from IGM filaments
• Investigating the use of field solvers for simulating classical systems
• Prospects for Observing the low-density Cosmic Web in Lyman-alpha Emission
• Is patchy reionization an obstacle in detecting the primordial gravitational wave signal?
• A Sagittarius-Induced Origin for the Monoceros Ring
• How to Interpret Measurements of Diffuse Light in Stacked Observations of Groups and Clusters of Galaxies
• On the [$\alpha$/Fe]-[Fe/H] relations in early-type galaxies
• Chemical Abundance Patterns and the Early Environment of Dwarf Galaxies
• On the fragility of nuclear stellar discs against galaxy mergers: surviving photometric and kinematic signatures of nuclear discs
• Fingers-of-God effect of infalling satellite galaxies
• ${\mu }_{\star }$ Masses: Weak Lensing Calibration of the Dark Energy Survey Year 1 redMaPPer Clusters using Stellar Masses
• MIND THE GAP: Is The Too Big To Fail Problem Resolved?
• Gas accretion in Milky Way-like galaxies: temporal and radial dependencies
• Searching for the shadows of giants: characterising protoclusters with line of sight Lyman-α absorption
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines II. [C II], [O I], [O III], [N II] and [N III] up to z=6
• The environment of radio galaxies: A signature of AGN feedback at high redshifts
• A giant thin stellar stream in the Coma Galaxy Cluster
• Collisional relaxation of two-dimensional self-gravitating systems
• Impact of H${}_2$-driven star formation and stellar feedback from low-enrichment environments on the formation of spiral galaxies
• Simulating Hydrodynamics in Cosmology with CRK-HACC
• The First Billion Years project: gamma-ray bursts at z>5
• The role of environment in galaxy evolution in the SERVS Survey I: density maps and cluster candidates
• Why weak lensing cluster shapes are insensitive to self-interacting dark matter
• Effects of hot halo gas on the star formation and mass transfer during distant galaxy-galaxy encounters
• Constrained simulations of the Antennae Galaxies: Comparison with Herschel-PACS observations
• Cosmology using numerical relativity
• Neutral hydrogen in galactic fountains
• Metallicity distribution of the progenitor of the Giant Stellar Stream in the Andromeda Galaxy
• Ram pressure stripping in the EAGLE simulation
• Uncovering the Orbit of the Hercules Dwarf Galaxy
• Dark Energy Survey Year 3 Results: Redshift Calibration of the MagLim Lens Sample from the combination of SOMPZ and clustering and its impact on Cosmology
• Probing the dynamical state of galaxy clusters
• Unveiling the main sequence of galaxies at $z\ge 5$ with the James Webb Space Telescope: predictions from simulations
• Isotropic extragalactic flux from dark matter annihilations: lessons from interacting dark matter scenarios
• Machine Learning to identify ICL and BCG in simulated galaxy clusters
• The Origin of the Milky Way's Halo Age Distribution
• Euclid: Early Release Observations -- Unveiling the morphology of two Milky Way globular clusters out to their periphery
• The Galaxy Replacement Technique (GRT): a New Approach to Study Tidal Stripping and Formation of Intracluster Light in a Cosmological Context
• On the Edge: the relation between stellar and dark matter haloes of Milky Way-mass galaxies
• The environment and redshift dependence of accretion onto dark matter halos and subhalos
• Effects of Coupled Dark Energy on the Milky Way and its Satellites
• Effects of turbulence in the Circumnuclear Disk
• The Evolution of Stellar Velocity Dispersion During Dissipationless Galaxy Mergers
• Simulations of structure formation in interacting dark energy cosmologies
• Fitting a Self-Interacting Dark Matter Model to Data Ranging From Satellite Galaxies to Galaxy Clusters
• Galaxy-Galaxy Lensing in EAGLE: comparison with data from 180 square degrees of the KiDS and GAMA surveys
• Clumpy winds and the obscuration of Active Galactic Nuclei
• Ram pressure statistics for bent tail radio galaxies
• First emergence of cold accretion and supermassive star formation in the early universe
• Performance study of Lagrangian methods: reconstruction of large scale peculiar velocities and baryonic acoustic oscillations
• Euclid preparation. Modelling spectroscopic clustering on mildly nonlinear scales in beyond-$\Lambda$CDM models
• Galaxy clustering from the bottom up: A Streaming Model emulator I
• HI observations of IC 10 with the DRAO synthesis telescope
• ΛCDM is still not broken: empirical constraints on the star formation efficiency at z ~ 12-30
• Asymmetric velocity anisotropies in remnants of collisionless mergers
• Constraining Halo Occupation Distribution and Cosmic Growth Rate using Multipole Power Spectrum
• Statistical Properties of Thermal Sunyaev-Zel'dovich Maps
• Mixed Warm Dark Matter Constraints using Milky Way Satellite Galaxy Counts
• The supermassive black hole merger driven evolution of high-redshift red nuggets into present-day cored early-type galaxies
• Local Group progenitors: Lyman Alpha bright?
• NGC 147, NGC 185 and CassII: a genetic approach to orbital properties, star formation and tidal debris
• The Fabric of the Universe: Exploring the cosmic web in 3D prints and woven textiles
• Filament Hunting: Integrated HI 21cm Emission From Filaments Inferred by Galaxy Surveys
• Higher multipoles of the galaxy bispectrum in redshift space
• Dark matter halos in the multicomponent model. II. Density profiles of galactic halos
• Selecting ultra-faint dwarf candidate progenitors in cosmological N-body simulations at high redshifts
• Momentum space sampling of neutrinos in $N$-body simulations
• Cosmic Voids in Evolving Dark Sector Cosmologies: the High Redshift Universe
• Is the vast polar structure of dwarf galaxies a serious problem for lambda cold dark matter?
• Consistency Relations in Effective Field Theory
• Constraining cluster masses from the stacked phase space distribution at large radii
• On the Origin of the Monoceros Ring - I: Kinematics, proper motions, and the nature of the progenitor
• How do galaxy properties affect void statistics?
• Opening Reionization: Quantitative Morphology of the Epoch of Reionization and Its Connection to the Cosmic Density Field
• Dark Energy Survey Year 1 Results: Wide field mass maps via forward fitting in harmonic space
• Evolution of Prolate Molecular Clouds at HII Boundaries: I. Formation of fragment-core structures
• Einstein-Vlasov Calculations of Structure Formation
• Radial orbit instability in dwarf dark matter haloes
• The $n$-point streaming model: how velocities shape correlation functions in redshift space
• The bias of weighted dark matter halos from peak theory
• Constraining structure formation using EDGES
• Cosmological law of universal gravitation
• Cosmological Parameter Estimation from the Two-Dimensional Genus Topology -- Measuring the Shape of the Matter Power Spectrum
• Probing reionization using quasar near-zones at redshift z ~ 6
• Probing delayed-end reionization histories with the 21cm-LAE cross-power spectrum
• On $N$-body simulations of globular cluster stream
• The Local Void: for or against LCDM?
• Mock halo catalogs: assigning unresolved halo properties using correlations with local halo environment
• The Anisotropic Two-Point Correlation Functions of the Nonlinear Traceless Tidal Field in the Principal-Axis Frame
• Testing the fidelity of simulations of black hole - galaxy co-evolution at z ~ 1.5 with observations
• Satellite Alignment: III. Satellite Galaxies Spatial Distribution and their Dependence on Redshift with A Novel Galaxy Finder
• Deep Forest: Neural Network reconstruction of the Lyman-alpha forest
• Kinematics and Modeling of the Inner Region of M83
• Consistent SPH Simulations of Protostellar Collapse and Fragmentation
• Inconsistencies arising from the coupling of galaxy formation sub-grid models to Pressure-Smoothed Particle Hydrodynamics
• Clumpy accretion in pre-main-sequence stars as a source of perturbations in circumstellar disks
• The Column Densities of Molecular Gas across Cosmic Time: Bridging Observations and Simulations
• Phase-Space Density Profiles in Scale-Free Cosmologies
• A tale of two tails: insights from simulations into the formation of the peculiar dwarf galaxy NGC 1427A
• HI intensity mapping correlation function from UNIT simulations: BAO and observationally induced anisotropy
• Is the molecular KS relationship universal down to low metallicities?
• A simple way to improve AGN feedback prescription in SPH simulations
• Drivers of asymmetry in synthetic H I emission-line profiles of galaxies in the EAGLE simulation
• Nonlinear stochastic biasing of halos: Analysis of cosmological N-body simulations and perturbation theories
• Cosmological Constraints from Weak Lensing Peaks: Can Halo Models Accurately Predict Peak Counts?
• A Semi-Analytical Line Transfer (SALT) Model III: Galactic Inflows
• The origin of star-gas misalignments in simulated galaxies
• Galactic satellite systems in CDM, WDM and SIDM
• Reionization time of the Local Group and Local-Group-like halo pairs
• Cross-correlations of the Lyman-alpha forest with weak lensing convergence I: Analytical Estimates of S/N and Implications for Neutrino Mass and Dark Energy
• A Multi-Fidelity Emulator for the Lyman-$\alpha$ Forest Flux Power Spectrum
• The ultra-diffuse galaxy AGC 114905 needs dark matter
• Effects of structure formation on the expansion rate of the Universe: An estimate from numerical simulations
• The impact of environment on the dynamical structure of satellite systems
• Dark matter cores in massive high-$z$ galaxies formed by baryonic clumps
• A formation mechanism for "Wrong Way" Radio Relics
• Gas around galaxy haloes: methodology comparisons using hydrodynamical simulations of the intergalactic medium
• 3-D SPH simulations of the FUOR flares in the clumpy accretion model
• Star formation and bar instability in cosmological haloes
• Finite element modelling of perturbed stellar systems
• Matching the mass function of Milky Way satellites in competing dark matter models
• Heating of galactic gas by dark matter annihilation in ultracompact minihalos
• Novel Conservative Methods for Adaptive Force Softening in Collisionless and Multi-Species N-Body Simulations
• Galaxy cluster rotation revealed in the MACSIS simulations with the kinetic Sunyaev-Zeldovich effect
• Improving three-dimensional mass mapping with weak gravitational lensing using galaxy clustering
• FORECAST: a flexible software to forward model cosmological hydrodynamical simulations mimicking real observations
• The Origin and Evolution of the Mass-Metallicity Relation using GalICS
• Environmental dependence of AGN activity and star formation in galaxy clusters from Magneticum simulations
• SIDM Concerto: Compilation and Data Release of Self-interacting Dark Matter Zoom-in Simulations
• An analytic halo approach to the bispectrum of galaxies in redshift space
• Genus statistics using the Delaunay tessellation field estimation method: (I) tests with the Millennium Simulation and the SDSS DR7
• Phurbas: An Adaptive, Lagrangian, Meshless, Magnetohydrodynamics Code. II. Implementation and Tests
• Relaxation in N-body simulations of spherical systems
• Probing the high-z IGM with the hyperfine transition of ${}^3$He${}^{+}$
• Probing the cluster pressure profile with thermal Sunyaev-Zeldovich effect and weak lensing cross-correlation
• Dynamical masses and non-homology of massive elliptical galaxies grown by dry mergers
• The role of 3-body H${}_2$ formation in the fragmentation of primordial gas
• Fractal distributions of dark matter and gas in the MareNostrum Universe
• Devouring the Milky Way Satellites: Modeling Dwarf Galaxies with Galacticus
• Dynamical evolution of Milky Way globular clusters on the cosmological timescale I. Mass loss and interaction with the nuclear star cluster
• Cosmological applications of the Brown-York quasilocal mass
• Gas stripping and mixing in galaxy clusters: A numerical comparison study
• Semi-Analytic Model Predictions of Mass Segregation from Groups to Clusters
• Reconstructing Orbits of Galaxies in Extreme Regions (ROGER) II: reliability of projected phase-space in our understanding of galaxy populations
• LyMAS reloaded: improving the predictions of the large-scale Lyman-α forest statistics from dark matter density and velocity fields
• SPAMCART: a code for smoothed particle Monte Carlo radiative transfer
• Bringing faint active galactic nuclei (AGNs) to light: a view from large-scale cosmological simulations
• The BAHAMAS project: Evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum
• Galaxy-group (halo) alignments from SDSS DR7 and the ELUCID simulation
• Deep learning insights into cosmological structure formation
• Evolution of superclusters and supercluster cocoons in various cosmologies
• The Uchuu-GLAM BOSS and eBOSS LRG lightcones: Exploring clustering and covariance errors
• MAHGIC: A Model Adapter for the Halo-Galaxy Inter-Connection
• The Nature and Evolution of Early Massive Quenched Galaxies in the Simba-C Simulation
• Tracking the orbit of unresolved subhalos for semi-analytic models
• Towards the impact of GMC collisions on the star formation rate
• Terapixel imaging of cosmological simulations
• Dark Subhaloes and Disturbances in Extended HI Discs
• Confrontation of Top-Hat Spherical Collapse against Dark Halos from Cosmological N-Body Simulations
• The impact of assembly history on the X-ray detectability of halos. From galaxy groups to galaxy clusters
• Fast, large volume, GPU enabled simulations for the Ly-alpha forest: power spectrum forecasts for baryon acoustic oscillation experiments
• The 21-cm bispectrum from neutral hydrogen islands at z < 6
• The Stellar Halo and Tidal Streams of Messier 63
• Theoretical study of an LAE-CIV absorption pair at z = 5.7
• The effect of interacting dark energy on local measurements of the Hubble constant
• Probing Self-interacting Dark Matter with Disk Galaxies in Cluster Environments
• Cosmological N-body simulations with generic hot dark matter
• Environmental Effects of Dark Matter Haloes: The Clustering-Substructure relation of Group-size Haloes
• Galactic halos in cosmology with long-range scalar DM interaction
• Signatures of very massive stars: supercollapsars and their cosmological rate
• Galaxy growth from redshift 5 to 0 at fixed comoving number density
• Subaru Hyper Suprime-Cam excavates colossal over- and under-dense structures over 360 deg2 out to z=1
• The source-lens clustering effect in the context of lensing tomography and its self-calibration
• Angular diameter distance estimates from the Sunyaev-Zel'dovich effect in hydrodynamical cluster simulations
• Constraining the Fluctuating Gunn-Peterson Approximation Using Lyman-$\alpha$ Forest Tomography at $z=2$
• Imprint of baryons and massive neutrinos on velocity statistics
• Life after AGN switchoff: evolution and properties of fossil galactic outflows
• Dependence of the Star Formation Efficiency on the Parameters of Molecular Cloud Formation Simulations
• Projection effects of large-scale structures on weak-lensing peak abundances
• Constraints on dark matter self-interaction from galactic core size
• On the origin of wide-orbit ALMA planets: giant protoplanets disrupted by their cores
• The radial metallicity gradients in the Milky Way thick disk as fossil signatures of a primordial chemical distribution
• Signatures of Light Massive Relics on nonlinear structure formation
• Cosmology with Galaxy Clusters: Systematic Effects in the Halo Mass Function
• Voxel datacubes for 3D visualization in Blender
• The anisotropy of the power spectrum in periodic cosmological simulations
• Improving Photometric Redshift Estimates with Training Sample Augmentation
• Modeling iterative reconstruction and displacement field in the large scale structure
• The kinematic Sunyaev-Zel'dovich effect of the large-scale structure (II): the effect of modified gravity
• Classification algorithms applied to structure formation simulations
• Accurate Model of the Projected Velocity Distribution of Galaxies in Dark Matter Halos
• Bayesian Control Variates for optimal covariance estimation with pairs of simulations and surrogates
• Numerical simulations of bar formation in the Local Group
• MOND prediction of a new giant shell in the elliptical galaxy NGC3923
• Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies
• Star Streams in Triaxial Isochrone Potentials with Sub-Halos
• Halo abundances and shear in void models
• Fast Correlation Function Calculator -- A high-performance pair counting toolkit
• Testing General Relativity Using the Evolution of Linear Bias
• Synthetic X-ray and radio maps for two different models of Stephan's Quintet
• $S^5$: New insights from deep spectroscopic observations of the tidal tails of the globular clusters NGC 1261 and NGC 1904
• Galacto-forensic of LMC's orbital history as a probe for the dark matter potential in the outskirt of the Galaxy
• Relation between halo spin and cosmic web filaments at z=3
• The signal of decaying dark matter with hydrodynamical simulations
• Identifying Lyman Alpha Emitters powered by AGNs
• Mesh-free hydrodynamics in PKDGRAV3 for galaxy formation simulations
• Forming Young and Hypervelocity Stars in the Galactic Centre via Tidal Disruption of a Molecular Cloud
• Towards unveiling the large-scale nature of gravity with the wavelet scattering transform
• Connecting the Dots: Tracking Galaxy Evolution Using Constant Cumulative Number Density at 3<z<7
• A panchromatic view of star cluster formation in a simulated dwarf galaxy starburst
• Nonlinear growth of structure in cosmologies with damped matter fluctuations
• Probing the assembly of dwarf galaxies through cosmic time with damped Lyman-$\alpha$ absorption spectroscopy
• Gas clumping and its effect on hydrostatic bias in the MACSIS simulations
• The circumgalactic medium in Lyman-alpha: a new constraint on galactic outflow models
• Examining the Accuracy of Astrophysical Disk Simulations With a Generalized Hydrodynamical Test Problem
• Got plenty of nothing: cosmic voids as a probe of particle dark matter
• $\text{PineTree}$: A generative, fast, and differentiable halo model for wide-field galaxy surveys
• The thermal SZ tomography
• Zero average values of cosmological perturbations as an indispensable condition for the theory and simulations
• The age gradients of galaxies in EAGLE: outside-in quenching as the origin of young bulges in cluster galaxies
• Rapid Simulations of Halo and Subhalo Clustering
• Cusps in the center of galaxies: a real conflict with observations or a numerical artefact of cosmological simulations?
• The relation between Lyman-alpha absorbers and gas--rich galaxies in the local universe
• Screening maps of the local Universe I -- Methodology
• The impact of faint AGN discovered by JWST on reionization
• The biasing phenomenon
• The local dark matter distribution in self-interacting dark matter halos
• PHoToNs--A Parallel Heterogeneous & Threads oriented code for cosmological N-body simulation
• Structure and evolution of Zel'dovich pancakes as probes of dark energy models
• Field spheroid-dominated galaxies in a Λ-CDM Universe
• Cosmic metal invaders: Intergalactic OVII as a tracer of the warm-hot intergalactic medium within cosmic filaments in the EAGLE simulation
• Cosmological interpretation of the color-magnitude diagrams of galaxy clusters
• N-body simulations, halo mass functions, and halo density profile in $f(T)$ gravity
• Weak Lensing of Type Ia Supernovae from the Dark Energy Survey
• The gap of stellar mass in galaxy groups: another perspective of the Too-big-To-Fail problem in the Milky Way
• The Impact of Wind Scalings on Stellar Growth and the Baryon Cycle in Cosmological Simulations
• Simulating the impact of the Smith Cloud
• He abundances in disc galaxies -- I. Predictions from cosmological chemodynamical simulations
• Measuring the equation of state of the high-z intergalactic medium using curvature statistics
• The features of the Cosmic Web unveiled by the flip-flop field
• The Star-Formation Properties of the Observed and Simulated AGN Universe: BAT vs EAGLE
• RABBITS -- II. The impact of AGN feedback on coalescing supermassive black holes in disc and elliptical galaxy mergers
• Rapid Growth of Galactic Supermassive Black Holes through Accreting Giant Molecular Clouds during Major Mergers of their Host Galaxies
• A Modified TreePM Code
• Probing quasar lifetimes with proximate $21$-centimetre absorption in the diffuse intergalactic medium at redshifts $z\ge 6$
• Zoom-in cosmological hydrodynamical simulation of a star-forming barred, spiral galaxy at redshift z=2
• Leaving the dark ages with AMIGA
• Lattice Universe: examples and problems
• Damping of the baryon acoustic oscillations in the matter power spectrum as a probe of the growth factor
• Merge and strip: dark matter-free dwarf galaxies in clusters can be formed by galaxy mergers
• The Sunyaev-Zeldovich effect in superclusters of galaxies using gasdynamical simulations: the case of Corona Borealis
• Resolution Convergence in Cosmological Hydrodynamical Simulations Using Adaptive Mesh Refinement
• The AGORA High-Resolution Galaxy Simulations Comparison Project VII: Satellite quenching in zoom-in simulation of a Milky Way-mass halo
• On de-Sitter Geometry in Cosmic Void Statistics
• Measuring the temperature and profiles of Lyman-$\alpha$ absorbers
• Understanding the Dyer-Roeder approximation as a consequence of local cancellations of projected shear and expansion rate fluctuations
• Carbon envelopes around merging galaxies at z ~ 4.5
• Impetus: Consistent SPH calculations of 3D spherical Bondi accretion onto a black hole
• Star Formation and Chemical Enrichment in Protoclusters
• Environment from cross-correlations: connecting hot gas and the quenching of galaxies
• Absence of obvious tidal tails around the globular cluster NGC 6397
• Testing the galaxy collision induced formation scenario for the trail of dark matter deficient galaxies with the susceptibility of globular clusters to the tidal force
• Is There a Fundamental Line for Disk Galaxies?
• Deformation of Optics for Photon Monte Carlo Simulations
• Direct Collapse to Supermassive Black Hole Seeds: Comparing the AMR and SPH Approaches
• History of the gas fuelling star formation in eagle galaxies
• Recovering the Tidal Field in the Projected Galaxy Distribution
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• Cosmic Filaments from Cosmic Strings
• Origin and Evolution of Structure and Nucleosynthesis for Galaxies in the Local Group
• Locating Bound Structure in an Accelerating Universe
• Average Dark Matter Halo Sparsity Relations as Consistency Check of Mass Estimates in Galaxy Cluster Samples
• An Extra-Dimensional Model of Dark Matter
• Cross-correlating Sunyaev-Zel'dovich and Weak Lensing Maps
• Simulating the LOcal Web (SLOW) -- III: Synchrotron emission from the local cosmic web
• Cosmology and Cluster Halo Scaling Relations
• Colour-magnitude diagram in simulations of galaxy formation
• The Tail of Late-forming Dwarf Galaxies in $\Lambda$CDM
• Can Stellar Discs in a Cosmological Setting Avoid Forming Strong Bars?
• Cosmology with the kinetic Sunyaev-Zeldovich effect: Independent of the optical depth and ${\sigma }_8$
• Setting the Stage: Structures from Gaussian Random Fields
• Modelling Dark Matter Halo Spin using Observations and Simulations: application to UGC 5288
• Galaxy archaeology for wet mergers: Globular cluster age distributions in the Milky Way and nearby galaxies
• Extracting the astrophysics of reionization from the Ly$\alpha$ forest power spectrum: a first forecast
• Quijote-PNG: Quasi-maximum likelihood estimation of Primordial Non-Gaussianity in the non-linear halo density field
• Modeling Turbulence in Galactic Centers
• Particle ejection during mergers of dark matter halos
• Measuring the Effects of Artificial Viscosity in SPH Simulations of Rotating Fluid Flows
• Gravitational lensing in WDM cosmologies: The cross section for giant arcs
• Gravity or turbulence V: Star forming regions undergoing violent relaxation
• Remapping simulated halo catalogues in redshift space
• Stellar winds near massive black holes: The case of the S-stars
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Constraining the Galaxy-Halo Connection with Optimal Statistics
• Origin of stellar prolate rotation in a cosmologically simulated faint dwarf galaxy
• On the phase-space structure of galaxy clusters from cosmological simulations
• Anisotropic Halo Model
• Cosmological formation and chemical evolution of an elliptical galaxy
• The effects of peculiar velocities on the morphological properties of large-scale structure
• The environments and hosts of metal absorption at z>5
• Correlation functions in 2D and 3D as descriptors of the cosmic web
• Resolving the problem of galaxy clustering on small scales: any new physics needed?
• An Empirical Model For Intrinsic Alignments: Insights From Cosmological Simulations
• A general framework to test gravity using galaxy clusters VI: Realistic galaxy formation simulations to study clusters in modified gravity
• ASymba: HI global profile asymmetries in the Simba simulation
• MEGA: Merger graphs of structure formation
• Fast generation of mock galaxy catalogues with COLA
• A universal model for the evolution of tidally stripped systems
• Higher Order Hamiltonian Monte Carlo Sampling for Cosmological Large-Scale Structure Analysis
• SEAGLE--III: Towards resolving the mismatch in the dark-matter fraction in early-type galaxies between simulations and observations
• SMBH growth parameters in the early Universe of Millennium and Millennium-II simulations
• An Application of Wiener Hermite Expansion to Non-linear Evolution of Dark Matter
• Dust accretion in binary systems: implications for planets and transition discs
• Probing Brownstein-Moffat Gravity via Numerical Simulations
• Switching integrators reversibly in the astrophysical $N$-body problem
• Particle number dependence in the non-linear evolution of N-body self-gravitating systems
• Measuring Bias via the Consistency Relations of the Large Scale Structure
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations -- I. Constraining physical processes in local star-forming galaxies
• Backsplash galaxies and their impact on galaxy evolution: a three-stage, four-type perspective
• Multiplicity functions of quasars: Predictions from the MassiveBlackII simulation
• The Supersonic Project: The Early Evolutionary Path of SIGOs
• Primordial non-Gaussianity with Angular correlation function: Integral constraint and validation for DES
• Quintessential Isocurvature in Separate Universe Simulations
• Physical properties of terrestrial planets and water delivery in the habitable zone using N-body simulations with fragmentation
• Properties of the circumgalactic medium in simulations compared to observations
• Simulating stellar winds in AMUSE
• Impact of nonlinear growth of the large-scale structure on CMB B-mode delensing
• The Supersonic Project: The eccentricity and rotational support of SIGOs and DM GHOSts
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
• Chemodynamics of dwarf galaxies under ram-pressure
• Cosmological Simulation of Galaxy Groups and Clusters-I: Global Effect of Feedback from Active Galactic Nuclei
• The formation and stability of a cold disc made out of stellar winds in the Galactic Centre
• Observing the redshifted 21 cm signal around a bright QSO at $z\sim 10$
• Photometric and clustering properties of hydrodynamical galaxies in a cosmological volume: results at z=0
• Cosmic Degeneracies III: N-body Simulations of Interacting Dark Energy with Non-Gaussian Initial Conditions
• X-ray and Sunyaev-Zeldovich properties of the WHIM
• Constraining cosmological parameters from N-body simulations with Variational Bayesian Neural Networks
• Simulations of the merging cluster of galaxies Cygnus A
• Performance analysis of parallel gravitational $N$-body codes on large GPU cluster
• Cosmology with Galaxy Cluster Properties using Machine Learning
• The Baryon Cycle at High Redshifts: Effects of Galactic Winds on Galaxy Evolution in Overdense and Average Regions
• The extended Baryon Oscillation Spectroscopic Survey (eBOSS): testing a new approach to measure the evolution of the structure growth
• Global analysis of luminosity- and colour-dependent galaxy clustering in the Sloan Digital Sky Survey
• The cosmological analysis of X-ray cluster surveys: IV. Testing ASpiX with template-based cosmological simulations
• Molecular hydrogen in Lyman Alpha Emitters
• Can the Low Redshift Lyman Alpha Forest Constrain AGN Feedback Models?
• Simulations of Gravitational Heating Due to Early Matter Domination
• Discy dwarf disruption and the shape of the Galactic halo
• Nonlinearities in modified gravity cosmology. II. Impacts of modified gravity on the halo properties
• The kinetic Sunyaev-Zel'dovich tomography II: probing the circumgalactic medium
• Circumgalactic Medium on the Largest Scales: Detecting X-ray Absorption Lines with Large-Area Microcalorimeters
• Mergers all the way down: stellar collisions and kinematics of a dense hierarchically forming massive star cluster in a dwarf starburst
• Galaxy shapes in Magneticum. I. Connecting stellar and dark matter shapes to dynamical and morphological galaxy properties and the large-scale structure
• Disk galaxies are self-similar: the universality of the HI-to-Halo mass ratio for isolated disks
• The influence of mergers on the cluster temperature function and cosmological parameters derived from it
• The Effect of Multiple Cooling Channels on the Formation of Dark Compact Objects
• Modeling of weak lensing statistics. II. Configuration-space statistics
• REMIX SPH -- improving mixing in smoothed particle hydrodynamics simulations using a generalised, material-independent approach
• MUSCLE-UPS: Improved Approximations of the Matter Field with the Extended Press-Schechter Formalism and Lagrangian Perturbation Theory
• Interchanging Interactive 3-d Graphics for Astronomy
• Testing the SZ-based tomographic approach to the thermal history of the universe with pressure-density cross-correlations: Insights from the Magneticum simulation
• The origin of correlations between mass, metallicity and morphology in galaxies from the EAGLE simulation
• Photometry and Dynamics of the Minor Merger AM1219-430 with Gemini GMOS-S
• The Merger Dynamics of the Galaxy Cluster Abell 1775: New Insights from Chandra and XMM-Newton for a Cluster Simultaneously Hosting a WAT and a NAT Radio Sources
• Revisiting the large-scale CMB anomalies: The impact of the SZ signal from the Local Universe
• Multi-scale and multi-domain computational astrophysics
• Evolution mapping II: describing statistics of the non-linear cosmic velocity field
• The Dark Matter Halos of HI Selected Galaxies
• Using EAGLE simulations to study the effect of observational constraints on the determination of HI asymmetries in galaxies
• Predictions on the stellar-to-halo mass relation in the dwarf regime using the empirical model for galaxy formation EMERGE
• Ghostly Stellar Haloes and their Relationship to Ultra-faint Dwarfs
• Simulated vs. observed UV emission at high redshift: a hint for a clumpy ISM?
• Formation of free-floating planetary mass objects via circumstellar disk encounters
• Galaxy cluster aperture masses are more robust to baryonic effects than 3D halo masses
• Study on the mapping of halo clustering from real space to redshift space
• Model independent measurement of the growth rate from the consistency relations of the LSS
• Feeding of active galactic nuclei by dynamical perturbations
• Density Conversion between 1-D and 3-D Stellar Models with 1D-MESA2HYDRO-3D
• Resolving infall caustics in dark matter halos
• The Host Galaxy of the Recoiling Black Hole Candidate in 3C 186: An Old Major Merger Remnant at the Center of a z=1 Cluster
• Cosmological Constraints from Fourier Phase Statistics
• The abundance of satellite galaxies in the inner region of $\Lambda$CDM Milky Way sized haloes
• Validating galaxy clustering models with Fixed & Paired and Matched-ICs simulations: application to Primordial Non-Gaussianities
• The chemical imprint of the bursty nature of Milky Way's progenitors
• Redshift drift in a universe with structure II: Light rays propagated through a Newtonian N-body simulation
• Constraining Warm Dark Matter with high-$z$ supernova lensing
• Self-similar galaxy dynamics below the de Sitter scale of acceleration
• The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics
• Fast estimation of aperture-mass statistics I: aperture mass variance and an application to the CFHTLenS data
• The SAMI Galaxy Survey: understanding observations of large-scale outflows at low redshift with EAGLE simulations
• The Formation of a Milky Way-sized Disk Galaxy 1. A Comparison of Numerical Methods
• Extensions and applications of the iterative method
• BullFrog: Multi-step perturbation theory as a time integrator for cosmological simulations
• Reconstruction of the two-dimensional gravitational potential of galaxy clusters from X-ray and Sunyaev-Zel'dovich measurements
• Molecular Disk Properties in Early-Type Galaxies
• Towards an accurate model for the Antennae Galaxies
• Turbulent Pressure Support in Galaxy Clusters -- Impact of the Hydrodynamical Solver
• HSC-CLAUDS survey: The star formation rate functions since z ~ 2 and comparison with hydrodynamical simulations
• Emergence of Galactic Morphologies at Cosmic Dawn: Input from Numerical Modeling
• The formation history of the Milky Way disc with high-resolution cosmological simulations
• Large scale anisotropies on halo infall
• Hydrodynamical simulations of the tidal stripping of binary stars by massive black holes
• Impact of Cosmological Satellites on Stellar Discs: Dissecting One Satellite at a Time
• Cloud-cloud collisions triggering star formation in galaxy simulations
• The effect of softening on dynamical simulations of galaxies
• Does the chemothermal instability have any role in the fragmentation of primordial gas
• The role of the elaphrocentre in void galaxy formation
• Lyman-alpha forest-CMB cross-correlation and the search for the ionized baryons at high redshift
• Physics of a partially ionized gas relevant to galaxy formation simulations -- the ionization potential energy reservoir
• Galactic wind X-ray heating of the intergalactic medium during the Epoch of Reionization
• Simulating a slow bar in the low surface brightness galaxy UGC 628
• On the effects of rotation in primordial star-forming clouds
• The Lyman-beta forest as a cosmic thermometer
• Modeling Lyman-α Forest Cross-Correlations with LyMAS
• Can we distinguish early dark energy from a cosmological constant?
• Void Probability Function of Simulated Surveys of high-redshift Lyman-Alpha Emitters
• Determining all gas properties in galaxy clusters from the dark matter distribution alone
• Lagrangian Methods Of Cosmic Web Classification
• Addressing via N-body simulations the distribution of the satellite tidal debris in the Milky Way environment
• Phase-space structure analysis of self-gravitating collisionless spherical systems
• Hydrodynamical Simulations of the Triggering of Nuclear Activities by Minor Mergers of Galaxies
• The effect of primordial non-Gaussianity on the skeleton of cosmic shear maps
• Resolution criteria to avoid artificial clumping in Lagrangian hydrodynamic simulations with a multi-phase interstellar medium
• Constraints on Primordial Magnetic Fields from the Lyman-α forest
• New constraints on red-spiral galaxies from their kinematics in clusters of galaxies
• Studying the Warm Hot Intergalactic Medium in emission: a reprise
• Accretion of Small Satellites and Gas Inflows in a Disc Galaxy
• How do baryonic effects on the cosmic matter distribution vary with scale and local density environment?
• The CIDER simulations: Nonlinear structure formation in the Constrained Interacting Dark Energy Scenario
• On the coldness of the local Hubble flow: the role of baryons
• Comparing galaxy morphology in hydrodynamical simulation and in semi-analytic model
• Hitting the mark: Optimising Marked Power Spectra for Cosmology
• Redshift-space equal-time angular-averaged consistency relations of the gravitational dynamics
• Is J 133658.3-295105 a Radio Source at z >= 1.0 or at the Distance of M 83?
• Is GN-z11 powered by a super-Eddington massive black hole?
• Panchromatic Spectral Energy Distributions of simulated galaxies: results at redshift $z=0$
• The Three Hundred project: Estimating the dependence of gas filaments on the mass of galaxy clusters
• The quasi-adiabatic relaxation of haloes in the IllustrisTNG and EAGLE cosmological simulations
• How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations
• Matter in the beam: Weak lensing, substructures and the temperature of dark matter
• Hybrid multi-fluid-particle simulations of the cosmic neutrino background
• The Ophiuchus stream progenitor: a new type of globular cluster and its possible Sagittarius connection
• ΛCDM with baryons vs. MOND: the time evolution of the universal acceleration scale in the Magneticum simulations
• The halo 3-point correlation function: a methodological analysis
• Field-level simulation-based inference with galaxy catalogs: the impact of systematic effects
• Oxygen Loss from Simulated Galaxies and the Metal Flow Main Sequence: Predicting the Dependence on Mass and Environment
• Time evolution of gaps in stellar streams in axisymmetric Stäckel potentials
• Can $\Lambda$CDM model reproduce MOND-like behavior?
• Significance of void shape: Neutrino mass from Voronoi void halos?
• Halo Growth and Merger Rates as a Cosmological Test
• Beyond the Lognormal Approximation: a General Simulation Scheme
• Keeping It Real: Revisiting a Real-Space Approach to Running Ensembles of Cosmological N-body Simulations
• EMERGE: Constraining merging probabilities and timescales of close galaxy pairs
• Improved Tomographic Binning of 3x2pt Lens Samples: Neural Network Classifiers and Optimal Bin Assignments
• The Weak Lensing Peak Statistics in the Mocks by the inverse-Gaussianization Method
• Effect of small scale density perturbations on the formation of dark matter halo profiles
• The Lost Dwarfs of Centaurus A and the Formation of its Dark Globular Clusters
• Characteristic scale of star formation. I. Clump formation efficiency on local scales
• Weighing the Light Gravitino Mass with Weak Lensing Surveys
• Three- and two-point spatial correlations of IGM at $z\sim 2$: Cloud based analysis using simulations
• DEMNUni: cross-correlating the nonlinear ISWRS effect with CMB-lensing and galaxies in the presence of massive neutrinos
• The Effect of the Remnant Mass in Estimating Stellar Mass of Galaxies
• The Gas Accretion History of Low Mass Halos within the Cosmic Web from Cosmological Simulations
• Intra-Cluster Light as a Dynamical Clock for Galaxy Clusters: Insights from the MAGNETICUM, IllustrisTNG, Hydrangea and Horizon-AGN Simulations
• CHEX-MATE: the intracluster medium entropy distribution in the gravity-dominated regime
• Consistency relations for the Lagrangian halo bias and their implications
• Improved two-point correlation function estimates using glass-like distributions as a reference sample
• Quantification of the multi-streaming effect in Redshift Space Distortion
• King Ghidorah Supercluster: Mapping the light and dark matter in a new supercluster at z=0.55 using the Subaru Hyper Suprime-Cam
• Does spatial flatness forbid the turnaround epoch of collapsing structures?
• Correlation between centre offsets and gas velocity dispersion of galaxy clusters in cosmological simulations
• Identifying Dark Matter Haloes by the Caustic Boundary
• The metallicity and elemental abundance maps of kinematically atypical galaxies for constraining minor merger and accretion histories
• Modelling Star Cluster Formation: Gas Accretion
• FLY: MPI-2 High Resolution code for LSS Cosmological Simulations
• On The Role of Supermassive Black Holes in Quenching Star Formation in Local Central Galaxies
• EuroHPC SPACE CoE: Redesigning Scalable Parallel Astrophysical Codes for Exascale
• Connection Between Galaxies and HI in the Circumgalactic and Intergalactic Media: Variation According to Galaxy Stellar Mass and Star-formation Activity
• Photometric Redshifts of Submillimeter Galaxies
• Galaxy populations of ProtoClusters in cosmological hydrodynamical simulations
• Simulated [CII] in high-z galaxies
• Stable clustering and the resolution of dissipationless cosmological N-body simulations
• Improving the accuracy of simulated chaotic $N$-body orbits using smoothness
• Evolution and instabilities of disks harboring super massive black holes
• The morphology of star-forming gas and its alignment with galaxies and dark matter haloes in the EAGLE simulations
• Radial X-ray profiles of simulated galaxies: Contributions from hot gas and XRBs
• Magnetic dynamos in galaxy clusters: the crucial role of galaxy formation physics at high redshifts
• N-body lensed CMB maps: lensing extraction and characterization
• Lux ex tenebris: The imprint of annihilating dark matter on the intergalactic medium during Cosmic Dawn
• Does the structure of Pop III supernova ejecta affect the elemental abundance of extremely metal-poor stars?
• Modelling H${}_2$ and its effects on star formation using a joint implementation of GADGET-3 and KROME
• Simulating nearly edge-on sloshing in the galaxy cluster Abell 2199
• Predictions for Complex Distributions of Stellar Elemental Abundances in Low-Mass Galaxies
• Numerical convergence of pre-initial conditions on dark matter halo properties
• Correlations between mass, stellar kinematics and gas metallicity in EAGLE galaxies
• Confronting predictions of the galaxy stellar mass function with observations at high-redshift
• Forming disc galaxies in major mergers II. The central mass concentration problem and a comparison of GADGET3 with GIZMO
• Velocity dispersion vs cluster mass: a new scaling law with The Three Hundred clusters
• A sparse regression approach to modeling the relation between galaxy stellar masses and their host halos
• Viscous time lags between starburst and AGN activity
• Improving Black Hole Accretion Treatment in Hydrodynamical Simulations
• Magrathea-Pathfinder: A 3D adaptive-mesh code for geodesic ray tracing in $N$-body simulations
• The importance of the cosmic web and halo substructure for power spectra
• Galaxy populations in protoclusters at cosmic noon
• Probing satellite galaxies in the Local Group by using FAST
• Dynamically Produced Moving Groups in Interacting Simulations
• A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations
• Testing primordial non-Gaussianities on galactic scales at high redshift
• What can we learn from higher multipole power spectra of galaxy distribution in redshift space?
• Gravitational Fragmentation in Galaxy Mergers: A Stability Criteria
• Lyman alpha Properties of Simulated Galaxies in Overdense Regions: Effects of Galactic Winds at z > 6
• Temperature Structure and Mass-Temperature Scatter In Galaxy Clusters
• Compactified Cosmological Simulations of the Infinite Universe
• Quantifying the intrinsic variability due to randomness of the Auriga galaxy formation model
• Formation of disks with long-lived spiral arms from violent gravitational dynamics
• Cooling-induced structure formation and evolution in collapsars
• Fast Forward Modelling of Galaxy Spatial and Statistical Distributions
• Dark Matter Annihilation Feedback in cosmological simulations I: Code convergence and idealised halos
• Studying galaxy cluster morphological metrics with Mock-X
• An efficient hybrid method to produce high resolution large volume dark matter simulations for semi-analytic models of reionisation
• Response of the LMC's Bar to a Recent SMC Collision and Implications for the SMC's Dark Matter Profile
• Perturbative Gaussianizing transforms for cosmological fields
• NGC 4104: a shell galaxy in a forming fossil group
• Constraining the 21cm brightness temperature of the IGM at $z$=6.6 around LAEs with the Murchison Widefield Array
• On Dark Gravitational Wave Standard Sirens as Cosmological Inference and Forecasting the Constraint on Hubble Constant using Binary Black Holes Detected by Deci-hertz Observatory
• Extended Stellar Components of Galaxies & the Nature of Dark Matter
• Enabling Radiative Transfer on AMR grids in CRASH
• Studying neutral hydrogen structures during the epoch of reionization using fractal dimensions
• Large-Scale Structure Topology in Non-Standard Cosmologies: Impact of Dark Sector Physics
• Constraining cloud parameters using high density gas tracers in galaxies
• Lyman continuum leakage versus quenching with the James Webb Space Telescope: The spectral signatures of quenched star formation activity in reionization-epoch galaxies
• Halo Profile Evolution and Velocity Bias
• An interaction scenario of the galaxy pair NGC 3893/96 (KPG 302). A single passage?
• Disc-Halo Interactions in ΛCDM
• Angular momentum generation in cold gravitational collapse
• UV background fluctuations traced by metal ions at $z\approx 3$
• Suitable Initial Conditions for Newtonian Simulations with Massive Neutrinos
• The Impact of Photometric Redshift Errors on Lensing Statistics in Ray-Tracing Simulations
• Variations of the ISM Compactness Across the Main Sequence of Star-Forming Galaxies: Observations and Simulations
• A Novel Scheme for Dark Matter Annihilation Feedback in Cosmological Simulations
• Higher moments of primordial non-Gaussianity and N-body simulations
• Power spectrum response of large-scale structure in 1D and in 3D: tests of prescriptions for post-collapse dynamics
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• Machine Learning the Fates of Dark Matter Subhalos: A Fuzzy Crystal Ball
• Accelerating self-gravitating hydrodynamics simulations with adaptive force updates
• Peculiar Velocity Estimation from Kinetic SZ Effect using Deep Neural Networks
• Can tides explain the low dark matter density in Fornax?
• Detecting Massive Galaxies at High Redshift using the Dark Energy Survey
• On the variation in stellar $\alpha$-enhancements of star-forming galaxies in the EAGLE simulation
• Astrophysical Searches and Constraints on Ultralight Bosonic Dark Matter
• PhotoNs-GPU:A GPU accelerated cosmological simulation code
• Effects of Neutrino Masses and Asymmetries on Dark Matter Halo Assembly
• A toy model to test the accuracy of cosmological N-body simulations
• Satellite galaxy abundance dependency on cosmology in Magneticum simulations
• Accurate relativistic observables from post-processing light cone catalogues
• On the statistical theory of self-gravitating collisionless dark matter flow
• Astraeus VII: The environmental-dependent assembly of galaxies in the Epoch of Reionization
• Analyzing Planar Galactic Halo Distributions with Fuzzy/Cold Dark Matter Models
• Relative baryon-dark matter velocities in cosmological zoom simulations
• Reliable estimation of the column density in Smoothed Particle Hydrodynamic simulations
• Cosmological Simulation of Galaxy Groups and Clusters-II: Studying Different Modes of Feedback through X-ray Observations
• Complementary Cosmological Simulations
• CosmoDRAGoN simulations -- I. Dynamics and observable signatures of radio jets in cosmological environments
• The relationship between cluster environment and molecular gas content of star-forming galaxies in the EAGLE simulation
• A comprehensive study on the relation between the metal enrichment of ionised and atomic gas in star-forming galaxies
• Star formation concentration as a tracer of environmental quenching in action: a study of the Eagle and C-Eagle simulations
• Analysis of Dark Matter Halo Structure Formation in $N$-body Simulations with Machine Learning
• Dark Matter-Induced Baryonic Feedback in Galaxies
• The Spin Alignments in Galaxy Pairs as a Test of Bouncing Coupled Dark Energy
• Gamma rays from dark matter spikes in EAGLE simulations
• Systematic Study of Gravitational Waves from Galaxy Merger
• A two-phase model of galaxy formation: III. The formation of globular clusters
• The Lyman-limit photon mean free path at the end of late reionisation in the Sherwood-Relics simulations
• The Glow of Axion Quark Nugget Dark Matter: (I) Large Scale Structures
• VisIVOWeb: A WWW Environment for Large-Scale Astrophysical Visualization
• Inner structure of dark matter halos at high $z$ in cosmological models with non-power-law primordial spectra
• Capturing primordial non-Gaussian signatures in the late Universe by multi-scale extrema of the cosmic log-density field
• EDEN: Exploring Disks Embedded in N-body simulations of Milky-Way-mass halos from Symphony
• Euclid preparation. Simulations and nonlinearities beyond $\Lambda$CDM. 1. Numerical methods and validation
• Psi-GAN: A power-spectrum-informed generative adversarial network for the emulation of large-scale structure maps across cosmologies and redshifts
• COZMIC. II. Cosmological Zoom-in Simulations with Fractional non-CDM Initial Conditions
• DarkAI: Reconstructing the density, velocity and tidal field of dark matter from a DESI-like bright galaxy sample
• A solution to the S8 tension through neutrino-dark matter interactions
• Trial by FIRE: Probing the dark matter density profile of dwarf galaxies with GraphNPE
• Test of Cosmic Web-feeding Model for Star Formation in Galaxy Clusters in the COSMOS Field
• Statistical properties of filaments in the cosmic web
• Hungry or Not: How Stellar-Mass Black Holes Grow (or Don't) in Dark Matter Mini-Haloes at High-Resolution
• Disentangling the morpho-kinematic properties of a face-on merger at z~0.7
• Dissociation of dark matter and gas in cosmic large-scale structure
• Galaxy pairs in The Three Hundred simulations: a study on the performance of observational pair-finding techniques
• The relationship between substructure in 2D X-ray surface brightness images and weak lensing mass maps of galaxy clusters: A simulation study
• A Machine Learning Approach to Correct for Mass Resolution Effects in Simulated Halo Clustering Statistics
• Exploring the role of cosmological shock waves in the Dianoga simulations of galaxy clusters
• Visualizing Astrophysical N-body Systems
• Dark-ages reionization and galaxy formation simulation - IX. Economics of reionizing galaxies
• The kinematics of globular clusters systems in the outer halos of the Aquarius simulations
• The internal metallicity distributions of simulated galaxies from EAGLE, Illustris, and IllustrisTNG at z=1.8-4 as probed by Gamma Ray Burst hosts
• Neutrinos in N-body simulations
• The fragility of thin discs in galaxies -- I. Building tailored N-body galaxy models
• Full sky Integrated Sachs-Wolfe maps for the MICE Grand Challenge lightcone simulation
• The Diffusion Coefficient of the Splashback Mass Function as a Probe of Cosmology
• Observing EAGLE galaxies with JWST: predictions for Milky Way progenitors and their building blocks
• Dynamical Properties of Collisionless Star Streams
• Evaluating the origins of the secondary bias based on the correlation of halo properties with the linear density field
• The role of impact parameter in typical close galaxy flybys
• Galaxy pairs in The Three Hundred simulations II: studying bound ones and identifying them via machine learning
• Why does Einasto profile index $n\sim 6$ occur so frequently?
• Probing $z\gtrsim 6$ massive black holes with gravitational waves
• NIHAO-RiNG: A Comparison of Simulated Disc Galaxies from GASOLINE and GIZMO
• Spiral structure of the galactic disk and its influence on the rotational velocity curve
• Filament Formation via Collision-induced Magnetic Reconnection -- Formation of a Star Cluster
• Deep Forest: Neural Network reconstruction of intergalactic medium temperature
• Probing Yukawian Gravitational Potential by Numerical Simulations. II. Elliptical Galaxies
• The galaxy power spectrum on the lightcone: deep, wide-angle redshift surveys and the turnover scale
• Performance Optimisation of Smoothed Particle Hydrodynamics Algorithms for Multi/Many-Core Architectures
• Globular clusters vs dark matter haloes in strong lensing observations
• Measuring the velocity field from type Ia supernovae in an LSST-like sky survey
• Cosmological Inference with Cosmic Voids and Neural Network Emulators
• Growth of Ex-situ Diffuse Intragroup Light in Simulated Galaxy Groups
• Deep learning for cosmological parameter inference from a dark matter halo density field
• Die Hard: The On-Off-Cycle of Galaxies on the Star Formation Main Sequence
• Bimodal Formation Time Distribution for Infall Dark Matter Halos
• CEMPlifying reionization
• Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
• Disk Mass-to-Light ratio distribution from stellar population synthesis: Application to rotation curve decomposition of NGC 5278 (KPG 390A)
• The Noctua Suite of Simulations -- The Difficulty of Growing Massive Black Holes in Low-Mass Dwarf Galaxies
• Massive $\nu$s through the CNN lens: interpreting the field-level neutrino mass information in weak lensing
• Degeneracies between Modified Gravity and Baryonic Physics
• Can the homogeneity scale be used as a standard ruler?
• SPH simulations of structures in protoplanetary disks
• PSDF: Particle Stream Data Format for N-Body Simulations
• The Three Hundred Project: Modeling Baryon and Hot-Gas Fraction Evolution in Simulated Clusters
• Coalescence Rate of Supermassive Black Hole Binaries Derived from Cosmological Simulations: Detection Rates for LISA and ET
• Catastrophic events in protoplanetary disks and their observational manifestations
• A study on the multicolour evolution of Red Sequence galaxy populations: insights from hydrodynamical simulations and semi-analytical models
• N-body simulations of structure formation in thermal inflation cosmologies
• A High Throughput Workflow Environment for Cosmological Simulations
• A self-gravity module for the PLUTO code
• Euclid preparation. Simulating thousands of Euclid spectroscopic skies
• Simulating non-axisymmetric flows in disc galaxies
• Dark-ages Reionization and Galaxy Formation Simulation - XV. Stellar evolution and feedback in dwarf galaxies at high redshift
• The importance of the merging activity for the kinetic polarization of the Sunyaev-Zel'dovich signal from galaxy clusters
• On fragmentation of turbulent self-gravitating discs in the long cooling time regime
• A Study of the Merger History of the Galaxy Group HCG 62 Based on X-Ray Observations and SPH Simulations
• Probing the cosmic web in Ly$\alpha$ emission over large scales: an Intensity Mapping forecast for DECaLS/BASS and DESI
• Dark matter vorticity and velocity dispersion from truncated Dyson$\unicode{x2013}$Schwinger equations
• Inner Engine Shutdown from Transitions in the Angular Momentum Distribution in Collapsars
• The matter fluctuation amplitude inferred from the weak lensing power spectrum and correlation function in CFHTLenS data
• Predicting the Merger Fraction of Lyman alpha Emitters from Redshift z~3 to z~7
• Weak gravitational lensing as a probe of physical properties of substructures in dark matter halos
• Efficient implementation of the Time Renormalization Group
• Isolated dark matter deprived galaxies in hydrodynamical simulations: real objects or artefacts?
• Efficiently estimating mean, uncertainty and unconstrained large scale fraction of local Universe simulations with paired fixed fields
• Masked areas in shear peak statistics: a forward modeling approach
• Fitting functions on the cheap: the relative nonlinear matter power spectrum
• Cross-Correlation between Damped Ly-alpha Systems and Ly-break Galaxies in Cosmological SPH Simulations
• Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
• Assessing Disk Galaxy Stability through Time
• The Hierarchical Structure of Galactic Haloes: Classification and characterisation with Halo-OPTICS
• Flattening of dark matter cusps during mergers: model of M31
• Honing and proofing Astrophysical codes on the road to Exascale. Experiences from code modernization on many-core systems
• A-priori Validation of Subgrid-scale Models for Astrophysical Turbulence
• The influence of Equation of State on impact dynamics between Pluto-like bodies
• A Study of the Properties and Dynamics of the Disk of Satellites in a Milky-Way-like Galaxy System
• Interaction between the ejecta, the accretion disk, and the secondary star in the recurrent nova system U Sco
• The correlation of high-redshift galaxies with the thermal Sunyaev-Zel'dovich effect traces reionization
• Comparing binary systems from rotating parent gas structures with different total masses
• Perturbation-theory informed integrators for cosmological simulations
• Impacts of pre-initial conditions on anisotropic separate universe simulations: a boosted tidal response in the epoch of reionization
• FleCSPH: The Next Generation FleCSIble Parallel Computational Infrastructure for Smoothed Particle Hydrodynamics
• Disc fragmentation and oligarchic growth of protostellar systems in low-metallicity gas clouds
• Intertwined Formation of ${\mathrm{H}}_2$, Dust, and Stars in Cosmological Simulations
• Constraints on primordial non-Gaussianity using multitracer technique for skew spectrum
• Galaxy and halo properties around cosmic filaments from Sloan Digital Sky Survey Data Release 7 and the ELUCID simulation
• A Recipe to Probe Alternative Theories of Gravitation via N-body Numerical Simulations. I. Spiral Galaxies
• Impact of cosmological signatures in two-point statistics beyond the linear regime
• Breaking the Dark Degeneracy with the Drifting Coefficient of the Field Cluster Mass Function
• Metal distribution in the ICM - a comprehensive numerical study of twelve galaxy clusters
• COZMIC. III. Cosmological Zoom-in Simulations of Self-interacting Dark Matter with Suppressed Initial Conditions
• Measuring the Hubble constant through the galaxy pairwise peculiar velocity
• Properties of self-gravitating quasi-stationary states
• Properties of loss cone stars in a cosmological galaxy merger remnant
• Inferring Cosmological Parameters on SDSS via Domain-Generalized Neural Networks and Lightcone Simulations
• The BACCO Simulation Project: A baryonification emulator with Neural Networks
• Assessing theoretical uncertainties for cosmological constraints from weak lensing surveys
• Mean Motion Resonances With Nearby Moons: An Unlikely Origin For The Gaps Observed In The Ring Around The Exoplanet J1407b
• Oxygen emission in remnants of thermonuclear supernovae as a probe for their progenitor system
• Anisotropy and characteristic scales in halo density gradient profiles
• The luminosity of cluster galaxies in the Cluster-EAGLE simulations
• Mass-Dependent Baryon Acoustic Oscillation Signal and Halo Bias
• Bar instability and formation timescale across Toomre's $Q$ parameter and central mass concentration: slow bar formation or true stability
• Comparison of Bayesian inference methods using the Loreli II database of hydro-radiative simulations of the 21-cm signal
• A correlation between accreted stellar kinematics and dark matter halo spin in the ARTEMIS simulations
• The bias from hydrodynamic simulations: mapping baryon physics onto dark matter fields
• The Impact of Baryons on the Large-Scale Structure of the Universe
• Separating the memory of reionization from cosmology in the Ly$\alpha$ forest power spectrum at the post-reionization era
• Does slow and steady win the race? Investigating feedback processes in giant molecular clouds
• Impact of cosmic-ray propagation on the chemistry and ionisation fraction of dark clouds
• Effect of Separate Initial Conditions on the Lyman-$\alpha$ Forest in Simulations
• Constraining $f_{NL}$ using the Large-Scale Modulation of Small-Scale Statistics
• Density Fluctuations in the Intracluster Medium: An Attempt to Constrain Viscosity with Cosmological Simulations
• Cosmological Zoom-In Simulation of Odd Radio Circles as Merger-Driven Shocks in Galaxy Groups
• Improved Halo Model Calibrations for Mixed Dark Matter Models of Ultralight Axions
• Modeling Circumstellar Disc Fragmentation and Episodic Protostellar Accretion with Smoothed Particle Hydrodynamics in Cell
• New observational recipes for measuring dynamical state of galaxy clusters
• Joint cluster reconstructions: Combining free-form lensing and X-rays
• The Convergence of Particle-in-Cell Schemes for Cosmological Dark Matter Simulations
• Fuzzy dark matter simulations
• The Coarse Geometry of Merger Trees in ΛCDM
• Impact Dynamics of Moons Within a Planetary Potential
• The Flux Auto- and Cross-Correlation of the Lyman-alpha Forest. II. Modelling Anisotropies with Cosmological Hydrodynamic Simulations
• Spin transfer from dark matter to gas during halo formation
• Lognormal semi-numerical simulations of the Lyman-$\alpha$ forest: comparison with full hydrodynamic simulations
• Impact of primordial black holes on the formation of the first stars and galaxies
• Measuring neutrino mass and asymmetry with matter pairwise velocities
• Unveiling galaxy pair alignment in cosmic filaments: A 3D exploration using EAGLE simulation
• The origin of the metallicity distributions of the NE and W stellar shelves in the Andromeda Galaxy
• Dark matter haloes: a multistream view
• Angular momentum - mass relation for dark matter haloes
• A derivation of (half) the dark matter distribution function
• A Galactic Transformation -- Understanding the SMC's Structural and Kinematic Disequilibrium
• A New Multi-Scale Structure Finding Algorithm to Identify Cosmological Structure
• Rest-Frame Ultraviolet to Near Infrared Observations of an Interacting Lyman Break Galaxy at z = 4.42
• Alignment between Satellite and Central Galaxies in the EAGLE Simulation: Dependence on the Large-Scale Environments
• C2-GaMe: Classification of Cluster Galaxy Membership with Machine Learning
• GrGadget: an N-body TreePM relativistic code for cosmological simulations
• Mass accretion rates and multi-scale halo environment in cold and warm dark matter cosmologies
• Protruding bullet heads indicating dark matter pull
• Dynamic Zoom Simulations: a fast, adaptive algorithm for simulating lightcones
• Fourier imaging of non-linear structure formation
• Signature of Massive Neutrinos from the Clustering of Critical Points. I. Density-threshold-based Analysis in Configuration Space
• Fourth-order perturbative equations in Lagrangian perturbation theory for a cosmological dust fluid
• Gaseous Dynamical Friction: a Numerical Study of Extended Perturbers
• Dynamical Simulations of the First Globular Clusters
• The collaborative effect of ram pressure and merging on star formation and stripping fraction
• Kickstarting Reionization with the First Black Holes: the effects of second-order perturbation theory in pre-reionization volumes
• Late-Time Dark Matter Oscillations and the Core-Cusp Problem
• Position-dependent Voronoi probability distribution functions for matter and halos
• Intrinsic alignments of the extended radio continuum emission of galaxies in the EAGLE simulations
• Meshless Methods for Magnetohydrodynamics with Vector Potential
• Large-scale geometry and topology of gas fields: Effects of AGN and stellar feedback
• Measurement of redshift-space two- and three-point correlation of Ly$\alpha$ absorbers at $1.7<z<3.5$: Implications on evolution of the physical properties of IGM
• Effect of Priomordial non-Gaussianities on Galaxy Clusters Scaling Relations
• Including relativistic and primordial Non-Gaussianity contributions in cosmological simulations by modifying the initial condition
• A Detailed Numerical Analysis of Asymmetrical Density Distribution in Saturn's F ring During an Encounter with Prometheus
• Orbits and action changes during star-clump encounters responsible for the origin of exponential discs in dwarf galaxies
• A probabilistic framework for cosmological inference of peculiar velocities
• CLUES to the past: Local Group progenitors amongst high-redshift Lyman Break Galaxies
• Fast radio bursts as probes of feedback from active galactic nuclei
• Simulations of the accreted stellar halos of low-mass field galaxies
• Effects of Angular Momentum on Halo Profiles
• Evolution of Star Cluster Within Galaxy using Self-consistent Hybrid Hydro/N-body Simulation
• The extent of gravitationally bound structure in a ΛCDM universe
• Modelling Mechanical Heating in Star-Forming Galaxies: CO and 13CO Line Ratios as Sensitive Probes
• Modeling submillimeter galaxies in cosmological simulations: Contribution to the cosmic star formation density and predictions for future surveys
• The Three Hundred: $M_{sub}-V_{circ}$ relation
• Self-gravitating barotropic equilibrium configurations of rotating bodies with SPH
• Probabilistic Estimators of Lagrangian Shape Biases: Universal Relations and Physical Insights
• The Velocity Field Olympics: Assessing velocity field reconstructions with direct distance tracers
• Infall near clusters of galaxies: comparing gas and dark matter velocity profiles
• Two merging galaxy clusters with very hot shock fronts observed shortly before pericentric passage
• Star formation and stellar & AGN feedback in the absence of accretion, not gas stripping, set the quenching timescale in satellite galaxies
• Starting Cosmological Simulations from the Big Bang
• Role of ionizing background on the non-thermal broadening inferred for the aligned absorbers
• The Power of the Cosmic Web
• Formation of Compact Clusters from High Resolution Hybrid Cosmological Simulations
• Large scale environmental bias of the QSO line of sight proximity effect
• The Low Redshift survey at Calar Alto (LoRCA)
• Improving SDSS cosmological constraints through $\beta$-skeleton weighted correlation functions
• N-body simulations of dark matter-baryon interactions
• Diversifying halo structures in two-component self-interacting dark matter models via mass segregation
• Breaking the ${\tau }_{\mathrm{T}}-f$ degeneracy of the kinetic Sunyaev Zel'dovich cosmology in redshift space
• Solving the puzzle of subhalo spins
• A method to extract the redshift distortions beta parameter in configuration space from minimal cosmological assumptions
• Hydrodynamical chemistry simulations of the SZ effect and the impacts from primordial non-Gaussianities
• Dark-ages Reionization and Galaxy Formation Simulation - XIV. Gas accretion, cooling and star formation in dwarf galaxies at high redshift
• The COS-Holes Survey: Connecting Galaxy Black Hole Mass with the State of the CGM
• The eROSITA view on the halo mass-temperature relation: From low-mass groups to massive clusters
• Weak Lensing Constraints on Dark Matter-Baryon Interactions with $N$-Body Simulations and Machine Learning
• Properties of Central Regions of the Dark Matter Halos in the Model with a Bump in the Power Spectrum of Density Perturbations
• Assuming Ionization Equilibrium and the Impact on the Lyman-$\alpha$ Forest Power Spectrum during the End of Reionization at $8\ge z\ge 5$
• Study of Star-formation in Dual Nuclei Galaxies using UVIT observations
• Refueled and shielded - The early evolution of Tidal Dwarf Galaxies
• Abundance of peaks and dips in three-dimensional mass and halo density fields: a test for cosmology
• Testing the stability of supersonic ionized Bondi accretion flows with radiation hydrodynamics
• Simulation-based marginal likelihood for cluster strong lensing cosmology
• Damping of the Milky Way bar by manifold-driven spirals
• Cosmological Signatures of Dark Sector Physics: The Evolution of Haloes and Spin Alignment
• Protoplanet collisions: new scaling laws from SPH simulations
• Simulations of cm-wavelength Sunyaev-Zel'dovich galaxy cluster and point source blind sky surveys and predictions for the RT32/OCRA-f and the Hevelius 100-m radio telescope
• Isolating the extreme debris disc signature -- explorations of eccentric extreme debris discs formed by giant impacts
• The dynamical state of RXCJ1230.7+3439: a multi-substructured merging galaxy cluster
• Understanding Stellar Mass-Metallicity and Size Relations in Simulated Ultra-Faint Dwarf Galaxies
• Hidden Figures in the Sky: Evolution of low-surface brightness galaxies from a hydro-dynamical perspective
• The time evolution of bias
• Impact of Dynamical Friction on the Tidal Formation of NGC 1052-DF2
• Testing extensions to LCDM on small scales with forthcoming cosmic shear surveys
• The Three Hundred: Gas Properties Outside of Galaxy Cluster with the WHIM Contribution and Detection
• Generation of inclined protoplanetary discs and misaligned planets through mass accretion I: Coplanar secondary discs
• Field-Level Comparison and Robustness Analysis of Cosmological N-body Simulations
• Stellar Mass Segregation in Dark Matter Halos
• Average energy of the X-ray spectrum as a model-independent proxy for the mass of galaxy clusters
• Prospects for studying the mass and gas in protoclusters with future CMB observations
• The Three Hundred: The existence of massive dark matter-deficient satellite galaxies in cosmological simulations
• A Gravitational Double Scattering Mechanism for Generating High Velocity Objects
• Formation of accretion centers in simulations of colliding uniform density H${}_2$ cores
• Neural style transfer of weak lensing mass maps
• Quasi-spiral solution to the mixed intracluster medium and the universal entropy profile of galaxy clusters
• Clustering of K-band selected local galaxies
• Natively Periodic Fast Multipole Method: Approximating the Optimal Green Function
• Galactic chimney sweeping: the effect of 'gradual' stellar feedback mechanisms on the evolution of dwarf galaxies
• Exploring effects of IMF sampling and SN feedback injection on star formation and metallicity in ultra-faint dwarf galaxies
• The Evolution of the Baryon Distribution in the Universe from Cosmological Simulations
• Balancing the load: A Voronoi based scheme for parallel computations
• Probing the shape and internal structure of dark matter halos with the halo-shear-shear three-point correlation function
• Boundary conditions in hydrodynamic simulations of isolated galaxies and their impact on the gas-loss processes
• Weak lensing peak statistics -- steepness versus height
• Angular momentum distribution during the collapse of primordial star-forming clouds
• Reionization relics in the cross-correlation between the Ly$\alpha$ forest and 21 cm intensity mapping in the post-reionization era
• A Simulated Annealing algorithm to quantify patterns in astronomical data
• The Cosmic Mach Number as an Environment Measure for the Underlying Dark Matter Density Field
• Turbulence in Simulated Local Cluster Analogs: One-to-one comparisons between SLOW and XRISM/Hitomi
• FLORAH: A generative model for halo assembly histories
• Morphological evolution of disk galaxies and their concentration, asymmetry and clumpiness (CAS) properties in simulations across Toomre's $Q$ parameter
• Constraining blazar heating with the 2<z<3 Lyman-$\alpha$ forest
• Simulating realistic self-interacting dark matter models including small and large-angle scattering
• On the interaction of a Bonnor-Ebert sphere with a stellar wind
• GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations
• Modelling the Evolution of Ly$\alpha$ Blobs and Ly$\alpha$ Emitters
• On the statistical theory of self-gravitating collisionless dark matter flow: Scale and redshift variation of velocity and density distributions
• The imprint of dark subhaloes on the circumgalactic medium
• Lagrangian displacement field estimators in cosmology
• The Three Hundred Project: deducing the stellar splashback structure of galaxy clusters from their orbiting profiles
• Neural Network Reconstruction of Non-Gaussian Initial Conditions from Dark Matter Halos
• Influence of baryons on spatial distribution of matter: higher order correlation functions
• The impact of halo concentration on the Sunyaev Zel'dovich effect signal from massive galaxy clusters
• On the statistical theory of self-gravitating collisionless dark matter flow: high order kinematic and dynamic relations
• The weak connection between the stellar haloes and merger histories of Milky Way-mass galaxies
• Particle motion in weak relativistic gravitational fields
• Predicting stellar collision outcomes of main sequence stars
• Differentiating Warm Dark Matter Models through 21cm Line Intensity Mapping: A Convolutional Neural Network Approach
• The Gravitational Lensing Imprints of DES Y3 Superstructures on the CMB: A Matched Filtering Approach
• Stellar initial mass function variation in massive early-type galaxies: the potential role of the deuterium abundance
• Performance Enhancement of Tree-based Friends-of-friend Galaxy-finder for High-resolution Simulations of Galaxy Formation
• Refracting into Ultra Diffuse Galaxy NGC 1052-DF2 by Passing near the Center of NGC 1052
• Gurzadyan's Problem 5 and improvement of softenings for cosmological simulations using the PP method
• The physical properties and the evolution of the interacting system AM1204-292
• DARKSKIES: A suite of super-sampled zoom-in simulations of galaxy clusters with self-interacting dark matter
• Scalable Streaming Tools for Analyzing $N$-body Simulations: Finding Halos and Investigating Excursion Sets in One Pass
• Auriga Streams II: orbital properties of tidally disrupting satellites of Milky Way-mass galaxies
• Overlapping Inflow Events as Catalysts for Supermassive Black Hole Growth
• Clusternets: A deep learning approach to probe clustering dark energy
• Assembly Conformity of Structure Growth: Fossil versus Normal Groups of Galaxies
• Devouring The Centaurus A Satellites: Modeling Dwarf Galaxies with Galacticus
• Supernovae at the cosmic dawn
• The Assembly of the Virgo Cluster, Traced by its Galaxy Halos
• Continuous Simulation Data Stream: A dynamical timescale-dependent output scheme for simulations
• The Accretion Mode in Sub-Eddington Supermassive Black Holes: Getting into the Central Parsecs of Andromeda
• Dynamical analysis of Maclaurin disk with velocity dispersion and its influence on bar formation
• Cospatial 21 cm and metal-line absorbers in the epoch of reionization -- I : Incidence and observability
• Scale-dependent halo bias and the squeezed limit bispectrum in the presence of radiation
• The AGORA High-resolution Galaxy Simulations Comparison Project. X: Formation and Evolution of Galaxies at the High-redshift Frontier
• Gravitational collapse at low to moderate Mach numbers: The relationship between star formation efficiency and the fraction of mass in the massive object
• Properties of subhalos in the interacting dark matter scenario
• Applying a star formation model calibrated on high-resolution interstellar medium simulations to cosmological simulations of galaxy formation
• Feedback from intermediate mass black holes on dwarf galaxy morphology at z=2
• AstroGrid-D: Grid Technology for Astronomical Science
• A general relativistic extension to mesh-free methods for hydrodynamics
• Hermeian haloes: extreme objects with two interactions in the past
• SubDLe: identification of substructures in cosmological simulations with deep learning
• ForestFlow: predicting the Lyman-$\alpha$ forest clustering from linear to nonlinear scales
• Bye-bye, Local-in-matter-density Bias: The Statistics of the Halo Field Are Poorly Determined by the Local Mass Density
• Exploring the Universe with Metal-Poor Stars
• A deconstruction of methods to derive one-point lensing statistics
• X-ray stacking reveals average SMBH accretion properties of star-forming galaxies and their cosmic evolution over 4 <~ z <~ 7
• Reconstructing galaxy star formation histories from COSMOS2020 photometry using simulation-based inference
• Directional miscentering dependence in weak lensing mass bias
• Accelerating HI density predictions during the Epoch of Reionization using a GPR-based emulator on N-body simulations
• A universal and physically motivated threshold for Hessian-based cosmic web identification: V-Web case
• Novel Hydrodynamic Schemes Capturing Shocks and Contact Discontinuities and Comparison Study with Existing Methods
• Fast Generation of Weak Lensing Maps in Modified Gravity with COLA
• Annotation-guided AoS-to-SoA conversions and GPU offloading with data views in C++
• Studying baryon acoustic oscillations using photometric redshifts from the DESI Legacy Imaging survey DR9
• Too small to succeed: the difficulty of sustaining star formation in low-mass haloes
• An Observationally Driven Multifield Approach for Probing the Circum-Galactic Medium with Convolutional Neural Networks
• Measuring photo-ionization rate and mean free path of HeII ionizing photons at $2.5\le z\le 3.6$: Evidence for late and rapid HeII reionization Part-II
• Could M31 come from a major merger and eject the LMC away?
• Does stellar mass assembly history vary with environment?
• Three-dimensional shapelets and an automated classification scheme for dark matter haloes
• The Statistics of Cosmological Lyman-alpha Absorption
• Exploring the Angular Momentum -- Atomic Gas Content Connection with EAGLE and IllustrisTNG
• Simultaneously Modelling Dusty Star Forming Galaxies and Massive Quiescents: A Calibration Framework for Galaxy Formation Models
• Detecting Modeling Bias with Continuous Time Flow Models on Weak Lensing Maps
• Super-Eddington accretion in high-redshift quasar hosts: Black-hole driven outflows, galaxy quenching, and the nature of little red dots
• Cosmology with Topological Deep Learning
• An adaptive symplectic integrator for gravitational dynamics
• Identifying massive black hole binaries via light curve variability in optical time-domain surveys
• An improved model for the effect of correlated Si-III absorption on the one-dimensional Lyman-$\alpha$ forest power spectrum
• Star-forming galaxies in the cosmic web in the last 11 Gyr
• Perturbation theory challenge for cosmological parameters estimation II.: Matter power spectrum in redshift space
• Joint Lyα emitters - quasars reionization constraints
• The Effective Field Theory of Large Scale Structures of a Fuzzy Dark Matter Universe
• The signature of galaxy formation models in the power spectrum of the hydrogen 21cm line during reionization
• The First Star-by-star $N$-body/Hydrodynamics Simulation of Our Galaxy Coupling with a Surrogate Model
• High$-z$ [OI] emission lines: ColdSIM simulations and ALMA observations
• An attractor for the dynamical state of the intracluster medium
• The AIDA-TNG project: 3D halo shapes
• The impact of baryons on the sparsity of simulated galaxy clusters from The Three Hundred Project
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• On the Robustness of Cluster Clustering Covariance Calibration
• HI asymmetries in spatially resolved SIMBA galaxies
• Properties of Globular Clusters in Galaxy Clusters: Sensitivity from the Formation and Evolution of Globular Clusters
• The Effect of Corner Modes in the Initial Conditions of Cosmological Simulations
• Atomic and Molecular Phases of the Interstellar Medium
• Prospects for detecting the circum- and intergalactic medium in X-ray absorption using the extended intracluster medium as a backlight
• A New Residual Distribution Hydrodynamics Solver for Astrophysical Simulations
• The Intergalactic Stellar Population from Mergers of Elliptical Galaxies with Dark Matter halos
• Detection of Chemo-Kinematical Structures in Leo I
• Inferring halo masses with Graph Neural Networks
• PSI: Constructing ad-hoc Simplices to Interpolate High-Dimensional Unstructured Data
• The Three Hundred Project: dissecting the fundamental plane of galaxy clusters up to $z=1$
• The reach of next-to-leading-order perturbation theory for the matter bispectrum
• Dark matter mass loss in galaxy flybys: dependence on impact parameter
• Assembly bias in quadratic bias parameters of dark matter halos from forward modeling
• Modelling the chemical evolution of the Milky Way
• The Boosted Potential
• Metamorphosis of dwarf halo density profile under dark matter decays
• Understanding the large inferred Einstein radii of observed low-mass galaxy clusters
• HIKER: a halo-finding method based on kernel-shift algorithm
• Estimating power spectrum of discrete cosmic momentum field with fast Fourier transform
• gadfly: A pandas-based Framework for Analyzing GADGET Simulation Data
• The Pseudo Evolution of Galaxy-Cluster Masses and Its Connection to Mass Density Profile
• On the parallelization of stellar evolution codes
• The extreme initial kinetic energy allowed by a collapsing turbulent core
• Intermediate-Mass Black Hole Feedback in Dwarf Galaxies: a View from Cosmological Simulations
• Evolution of the degree of substructures in simulated galaxy clusters
• Entropy generation in merging galaxy clusters
• On the tidal environment of an outwardly migrated F-ring
• Triaxiality Inhibitors in N-Body Simulations
• Acceleration of the tree method with SIMD instruction set
• One-point Statistics in various cosmic environments in the presence of massive neutrinos
• On the tomographic cluster clustering as a cosmological probe
• Cosmological parameters from the joint analysis of Density Split and Second Order Statistics: an Emulator based on the Halo Occupation Distribution
• Scaling Relations in Dissipationless Spiral-like Galaxy Mergers
• Overmassive and Undermassive Massive Black Holes: The Role of Environment and Gravitational-Wave Recoils
• Instability of counter-rotating stellar disks
• Dark matter haloes in the multicomponent model. III. From dwarfs to galaxy clusters
• The Effect of Impact Parameters on the Formation of Massive Black Hole Binaries in Galactic Mergers
• Structure of the Stellar Neighborhood of CQ Tau in the Presence of a Companion in an Elongated Orbit
• "Observations" of simulated dwarf galaxies: Star-formation histories from color-magnitude diagrams
• ngravs: Distinct gravitational interactions in GADGET-2
• Emergence of red, star-forming galaxies (red misfits) in a ΛCDM universe
• Violent mergers revisited: The origin of the fastest stars in the Galaxy
• Impact of astrophysical effects on the dark matter mass constraint with 21cm intensity mapping
• A New Model For Including Galactic Winds in Simulations of Galaxy Formation II: Implementation of PhEW in Cosmological Simulations
• Limitation of symmetry breaking by gravitational collapse: the revisit of Lin-Mestel-Shu instability
• Cross Section Calculations in Theories of Self-Interacting Dark Matter
• On the universality of the halo mass function beyond $\Lambda$CDM cosmology
• Modeling and measuring the anisotropic halo 3-point correlation function: a coordinated study
• Towards Precision Cosmology With Improved PNLF Distances Using VLT-MUSE. III. Impact of Stellar Populations in Early-Type Galaxy
• Transients from Initial Conditions Based on Lagrangian Perturbation Theory in $N$-body Simulations III: The Case of GADGET-2 Code
• The Connection between Dusty Star-Forming Galaxies and the First Massive Quenched Galaxies
• Probing Time-Dependent Dark Energy with the Flux Power Spectrum of the Lyman $\alpha$ Forest
• Dipole Distortions in the Intergalactic Medium
• Modelling Giant Radio Halos
• Tracing the environmental history of observed galaxies via extended fast action minimization method
• Super-resolution simulation of the Fuzzy Dark Matter cosmological model
• Constraining Galaxy-Halo Connection Using Machine Learning
• Rings of star formation: Imprints of a close galaxy encounter
• Super sample covariance and the volume scaling of galaxy survey covariance matrices
• The aluminium-26 distribution in a cosmological simulation of a Milky Way-type Galaxy
• Probing the Type 3 interacting dark-energy model using matter pairwise velocity
• Simulating the galactic system in interaction AM 2229-735 and the formation of its polar structure
• Simulating gravitational motion, gas dynamics, and structure in the cosmos
• Multi-wavelength properties of $z\gtrsim 6$ LISA detectable events
• Selecting Clusters and Protoclusters via Stellar Mass Density: I. Method and tests on Mock HSC-SSP catalogs
• Perseus cluster in its X-ray entirety with SRG/eROSITA. Merger and Radio-Uroboroses
• Modeling the Cosmological Lyman-$\alpha$ Forest at the Field Level
• Dynamical friction and massive black hole orbits: analytical predictions and numerical solutions
• Breaking the cosmological invariance of the dark matter halos shape as a new probe of modified gravity
• Angular momentum and morphological sequence of massive galaxies through Dark Sage
• Dynamical Evolution of Voids with Surrounding Gravitational Tidal Field
• Comparing Extended System Interactions with Motions in Softened Potentials
• Erosive Hit-and-Run Impact Events: Debris Unbound
• Self-Interacting Dark Matter with Mass Segregation: A Unified Explanation of Dwarf Cores and Small-Scale Lenses
• Cosmological simulations with rare and frequent dark matter self-interactions
• Power Spectrum Emulators from Neural Networks and Tree-Based Methods
• Partial tidal disruption of White Dwarfs in off-equatorial orbits around Kerr black holes
• Extracting cosmological signals from foregrounds in deep mm maps of the sky
• An Interpretable AI Framework to Disentangle Self-Interacting and Cold Dark Matter in Galaxy Clusters: The CKAN Approach
• "Observing and Analyzing" Images From a Simulated High Redshift Universe
• Chemodynamics of BoötesI with $S^5$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints
• The Sagittarius stellar stream embedded in a fermionic dark matter halo
• The role of AGN feedback and gas viscosity in hydrodynamical simulations of galaxy clusters
• Star formation quenching precedes morphological transformation in COSMOS-WEB's richest galaxy groups
• A Random Walk Model for Halo Triaxiality
• Observing high redshift galaxy clusters through lensing of the Ostriker-Vishniac effect
• Asymmetrical thermonuclear supernovae triggered by the tidal disruption of white dwarfs
• Recoiling supermassive black holes in analytical and numerical galaxy potential
• Halo cluster shapes: Insights from simulated galaxies and ICL with prospects for weak lensing applications
• Effect of the cubic torus topology on cosmological perturbations
• Prometheus Induced Vorticity In Saturns F Ring
• Go with the Flow: The Self-Similar and Non-Linear Behaviour of Large-Scale In- and Outflows and the Impact of Accretion Shocks from Galaxies to Galaxy Clusters
• Excursion Sets with a "Perfect" Collapse Model
• Baryon-driven decontraction in Milky Way mass haloes
• The Extended Zel'dovich Mass Functions of Clusters and Isolated Clusters in the Presence of Primordial Non-Gaussianity
• Answers from the void: VIDE and its applications
• Exploring HI Galaxy Redshift Survey Strategies for the FAST Core Array Interferometry
• Disc instability and bar formation: view from the IllustrisTNG simulations
• Non-linear structure formation in the "Running FLRW" cosmological model
• Forecasting the Constraint on the Hu-Sawicki $f(R)$ Modified Gravity in the CSST $3\times 2$pt Photometric Survey
• Satellite Infall and Mass Deposition on the Galactic Centre
• Galaxy Velocity Bias in Cosmological Simulations: Towards Percent-level Calibration
• Absorption in the 21 cm Hydrogen Line at $z>10$ as a Sensitive Tool for the Construction of a Cosmological Model on Small Scales
• Velocity dispersion functions of pressure-supported galaxies in EAGLE simulations with varying active galactic nucleus feedback
• Back to basics: Little Red Dots as galaxies and dust-obscured AGNs in a synthetic NIRCam sky simulated with L-GalaxiesBH
• The progenitor galaxies of stellar haloes as "failed" Milky Ways
• 3D Smoothed Particle Hydrodynamics Models of Betelgeuse's Bow Shock
• Observational signatures of the surviving donor star in the double detonation model of Type Ia supernovae
• JERALD: high-fidelity dark matter, stellar mass and neutral hydrogen maps from fast N-body simulations
• Shape Analysis of HII Regions -- II. Synthetic Observations
• Three-Dimensional Filamentation Analysis of SDSS DR5 Survey
• Weighing Cosmic Structures with Clusters of Galaxies and the Intergalactic Medium
• Group infall of substructures on to a Milky Way-like dark halo
• Fast Generation of Large-scale Structure Density Maps via Generative Adversarial Networks
• Gravitational Self-force Errors of Poisson Solvers on Adaptively Refined Meshes
• Quenching of satellite galaxies of Milky Way analogues: reconciling theory and observations
• Unequal-mass mergers of dark matter haloes with rare and frequent self-interactions
• Linking the Internal Properties of Infant Globular Clusters to their Formation Environments
• Cosmological Simulations of Satellites around Isolated Dwarf Galaxies
• Empirical formulae to describe some physical properties of small groups of protogalaxies with multiplicity
• A Hydro-Particle-Mesh Code for Efficient and Rapid Simulations of the Intracluster Medium
• Quantifying Lyman-$\alpha$ emissions from reionization fronts
• Off-center black hole seed formation? Implications for high and low redshift massive black holes
• Stellar Feedback Effects on the Mass Distribution of Clouds and Cloud Complexes
• Searching for dark matter isocurvature initial conditions with N-body Simulations
• How non-thermal pressure impacts the modelling of star formation in galaxy formation simulations
• A revisited Correction to the Halo Mass Function for local-type Primordial non-Gaussianity
• Segmenting proto-halos with vision transformers
• The major merger origin of the Andromeda II kinematics
• An anti-correlation between barycentre offsets and velocity dispersion for highest overdensity subhalos in cosmological simulations
• Web-Halo Model (WHM): Accurate non-linear matter power spectrum predictions without free parameters
• Cosmological Simulations with Massive Neutrinos: Efficiency and Accuracy
• Variational autoencoder for generating realistic $N$-body simulations for dark matter halos
• Tracing cosmic voids with fast simulations
• Insights into the structure and kinematics of a Milky Way-like galaxy
• The DORCHA suite: nature, nurture, and the phase space distribution of the Milky Way's high redshift progenitors today
• Spikes in the SED and Ripples in the Outskirts of Galaxies
• Cosmological structure formation shocks and cosmic rays in hydrodynamical simulations
• Cosmic curl -- Features and convergence of the vorticity power spectrum in $N$-body simulations
• Accretion of self-interacting dark matter onto supermassive black holes
• Predicting large scale cosmological structure evolution with generative adversarial network-based autoencoders
• Searching optimal scales for reconstructing cosmological initial conditions using convolutional neural networks
• A redshift distortion free correlation function at third order in the nonlinear regime
• DIAPHANE: a Portable Radiation Transport Library for Astrophysical Applications
• Past and Future of CG J1720-67.8: Constraints from Observations and Models
• Structure Formation under Inelastic Two-Component Dark Matter: Halo Statistics and Matter Power Spectra in the High-$z$ Universe
• Fast Sampling of Cosmological Initial Conditions with Gaussian Neural Posterior Estimation
• Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling
• New leaves of the tree: percolation analysis for cosmic web with discrete points
• Void probability function in the Quijote simulations
• On the road to percent accuracy VI: the nonlinear power spectrum for interacting dark energy with baryonic feedback and massive neutrinos
• Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter
• Machine Learning for Galactic Archaeology: A chemistry-based neural network method for identification of accreted disc stars
• Spatial disconnection between stellar and dust emissions: the test of the Antennae Galaxies (Arp 244)
• HI and H${}_2$ gas evolution over cosmic times: ColdSIM
• Towards a universal model for the density profiles of dark matter haloes
• Environmental Effects on the Dynamical Evolution of Star Clusters in Turbulent Molecular Clouds
• Predictions for the X-ray circumgalactic medium of edge-on discs and spheroids
• Milky Way Satellite Census. IV. Constraints on Decaying Dark Matter from Observations of Milky Way Satellite Galaxies
• Entropy Production in Collisionless Systems. III. Results from Simulations
• About One-point Statistics of the Ratio of Two Fourier-transformed Cosmic Fields and an Application
• Dark Energy Survey Year 3 Results: Three-Point Shear Correlations and Mass Aperture Moments
• Cosmic voids and BAO with relative baryon-CDM perturbations
• What can the outskirts of galaxies tell us about dark matter?
• Halo spin and orientation in Interacting Dark Matter Dark Energy Cosmology
• Galactic tides and the Crater II dwarf spheroidal: a challenge to LCDM?
• A dynamics-based density profile for dark haloes. I. Algorithm and basic results
• Timing the last major merger of galaxy clusters with large halo sparsity
• Grouped star formation: converting sink particles to stars in hydrodynamical simulations
• On the Tidal Formation of Dark Matter Deficient Galaxies
• Hydrodynamics of Collisions and Close Encounters between Stellar Black Holes and Main-sequence Stars
• Response approach to the integrated shear 3-point correlation function: the impact of baryonic effects on small scales
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• A novel Cosmic Filament catalogue from SDSS data
• The Halo21 Absorption Modeling Challenge: Lessons From "Observing" Synthetic Circumgalactic Absorption Spectra
• Discovering the building blocks of dark matter halo density profiles with neural networks
• An empirical nonlinear power spectrum overdensity-response
• Galaxy mergers can initiate quenching by unlocking an AGN-driven transformation of the baryon cycle
• Generalized Boltzmann hierarchy for massive neutrinos in cosmology
• Hydromagnetic waves in an expanding universe -- cosmological MHD code tests using analytic solutions
• Galaxies in the central regions of simulated galaxy clusters
• Assembly Histories and Observational Properties of Simulated Early-type Galaxies
• The Metallicity Distribution Function in Outer Halo Fields of Simulated Elliptical Galaxies Compared to Observations of NGC 5128
• 3D models of the circumstellar environments of evolved stars: Formation of multiple spiral structures
• An Anti-halo Void Catalogue of the Local Super-Volume
• The Scaling Relation between Galaxy Luminosity and WHIM Density from EAGLE Simulations with application to SDSS data
• Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback
• High-Energy Neutrino Production in Clusters of Galaxies
• Ringing the universe with cosmic emptiness: void properties through a combined analysis of stacked weak gravitational and Doppler lensing
• A preliminary study about gravitational wave radiation and cosmic heat death
• Improving cosmological covariance matrices with machine learning
• Is the Sgr dSph a dark matter dominated system?
• Compact Groups in GDM Cosmological Simulations
• Quijote PNG: The information content of the halo power spectrum and bispectrum
• The small-scale turbulent dynamo in smoothed particle magnetohydrodynamics
• Simulated X-ray Emission in Galaxy Clusters with Feedback from Active Galactic Nuclei
• Assembly History and Internal Structure of Cluster Cold Dark Matter Haloes
• DLAs and Galaxy Formation
• Formation of spiral structure from the violent relaxation of self-gravitating disks
• Weak Lensing the non-Linear Ly-alpha Forest
• Prediction of Individual Halo Concentrations Across Cosmic Time Using Neural Networks
• Gravitational collapse from cold uniform asymmetric initial conditions
• Exploring the halo occupation distribution for moderate X-ray luminosity active galactic nuclei in the EAGLE cosmological simulation
• Chemical analysis of prestellar cores in Ophiuchus yields short timescales and rapid collapse
• Populating Galaxies Into Halos Via Machine Learning on the Simba Simulation
• Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window
• Cosmic Web-Halo Connection Between Twin Universes
• Long time-scale variability of X-ray binaries with late type giant companions
• Tidal adaptive softening and artificial fragmentation in cosmological simulations
• Numerical Study of Bar Suppression in Galaxy Models Due to Disc Heating
• Transferring Data from a Voronoi Mesh to an Adaptive Cartesian Grid in Pursuit of Self-consistent Top-down Star Formation
• The Baryon Budget of Galaxies across the First Billion Years
• A thick-disk galaxy model and simulations of equal-mass galaxy pair collisions
• Using the EAGLE simulations to elucidate the origin of disc surface brightness profile breaks as a function of mass and environment
• Simulating the complexity of the dark matter sheet II: halo and subhalo mass functions for non-cold dark matter models
• Testing growth rate dependence in cosmological perturbation theory using scale-free models
• Three-Dimensional Simulations of Type Ia Supernova Remnants I: Effects of a Main-Sequence Companion Star
• OpenGadget3 GPU solver tests
• Galaxy Proximate Damped Lyman-Alpha Systems and HI Reionization Topology in TECHNICOLOR DAWN
• Sample Variance in Cosmological Observations with a Narrow Field-of-View
• Collisional Dynamics of Stars and Dark Matter in Ultra-Faint Galaxies
• Imladris: a detailed and flexible model for galaxy simulations with individual stars
• A New Method to Simulate Dark Matter-Baryon Interactions and Application to an Isolated Disk Galaxy
• On the star formation rate and turbulent dissipation in galactic models
• Controlled Experiments on Dark-Matter Halo Structure and Galaxy Morphology I: What Sets Galaxy Sizes?
• Galaxy and black hole coevolution in dark matter haloes not captured by cosmological simulations
• Dynamic Zoom Simulations of structure formation beyond standard cosmology
• Nearest Neighbour-Based Statistics for 21cm-Galaxy Cross-Correlations in the Epoch of Reionization
• Can UVB variations reconcile simulated quasar absorption lines at high redshift?
• Spatially resolved stellar-to-total dynamical mass relation: Radial variations, gradients and profiles of galaxy stellar populations
• Formation of massive multiple-star systems: early migration and mergers
• The detection of relativistic corrections in cosmological N-body simulations
• Substructures in Minor Mergers' Tidal Streams
• The effects of a compressive velocity pulse on a collapsing turbulent clump
• Can Bars Erode Cuspy Halos ?
• Investigating the Relationship Between the Hot Gas and the Dark Matter Components of Galaxy Clusters
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
• Rapid sinking and efficient mergers of supermassive black holes in compact high-redshift galaxies
• Too small to form a galaxy: How the UV background determines the baryon fraction
• Validating the CROCODILE model within the AGORA galaxy simulation framework
• Effects of Supernova Feedback on the Formation of Galaxies
• Simulating High-Redshift Disk Galaxies: Applications to Long Duration Gamma-Ray Burst Hosts
• Particle loads for cosmological simulations with equal-mass dark matter and baryonic particles
• Quantifying Weighted Morphological Content of Large-Scale Structures via Simulation-Based Inference
• Selfgravitating disks in binary systems: an SPH approach -- I. Implementation of the code and reliability tests
• Slow neutrinos: non-linearity and momentum-space emulation
• Accelerating reionization constraints: An ANN-emulator framework for the SCRIPT Semi-numerical Model
• Ginnungagap -- a massively parallel cosmological initial conditions generator
• Braginskii Viscosity in Cosmological Simulations of Galaxy Clusters: Implementation, Validation, and First Application
• Formation of discs around super-massive black hole binaries
• On the consistency of jet feedback modelling across different astrophysics hydrodynamical codes
• A supernova scenario for magnetic fields and rotation measures in galaxies
• The origin of the intra-cluster light in The Three Hundred simulations
• Characterising large-scale structure with the REFLEX II cluster survey
• A Pearl in the Shell: an ultra-compact dwarf within the tidal debris surrounding spiral galaxy NGC 7531