Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe

Abstract

We introduce the Illustris Project, a series of large-scale hydrodynamical simulations of galaxy formation. The highest resolution simulation, Illustris-1, covers a volume of $(106.5\mathrm{Mpc}{)}^3$, has a dark mass resolution of $6.26\times 10^6{\mathrm{M}}_{\odot }$, and an initial baryonic matter mass resolution of $1.26\times 10^6{\mathrm{M}}_{\odot }$. At $z=0$ gravitational forces are softened on scales of $710\mathrm{pc}$, and the smallest hydrodynamical gas cells have an extent of $48\mathrm{pc}$. We follow the dynamical evolution of $2\times 1820^3$ resolution elements and in addition passively evolve $1820^3$ Monte Carlo tracer particles reaching a total particle count of more than $18$ billion. The galaxy formation model includes: primordial and metal-line cooling with self-shielding corrections, stellar evolution, stellar feedback, gas recycling, chemical enrichment, supermassive black hole growth, and feedback from active galactic nuclei. At $z=0$ our simulation volume contains about $40,000$ well-resolved galaxies covering a diverse range of morphologies and colours including early-type, late-type and irregular galaxies. The simulation reproduces reasonably well the cosmic star formation rate density, the galaxy luminosity function, and baryon conversion efficiency at $z=0$. It also qualitatively captures the impact of galaxy environment on the red fractions of galaxies. The internal velocity structure of selected well-resolved disk galaxies obeys the stellar and baryonic Tully-Fisher relation together with flat circular velocity curves. In the well-resolved regime the simulation reproduces the observed mix of early-type and late-type galaxies. Our model predicts a halo mass dependent impact of baryonic effects on the halo mass function and the masses of haloes caused by feedback from supernova and active galactic nuclei.

arXiv comment32 pages, 26 figures. MNRAS accepted. The official Illustris website can be found at http://www.illustris-project.org

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• Tidal stripping and the structure of dwarf galaxies in the Local Group
• The link between the assembly of the inner dark matter halo and the angular momentum evolution of galaxies in the EAGLE simulation
• Inspiraling Halo Accretion Mapped in Lyman-$\alpha$ Emission around a $z\sim 3$ Quasar
• FIREbox: Simulating galaxies at high dynamic range in a cosmological volume
• The Dependence of Subhalo Abundance on Halo Concentration
• The faint end of the Centaurus A satellite luminosity function
• Modelling galaxy clustering: halo occupation distribution versus subhalo matching
• Zooming in on major mergers: dense, starbursting gas in cosmological simulations
• The Impact of Galactic Feedback on the Circumgalactic Medium
• Limitations to the "basic'' HOD model and beyond
• Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium
• Stochastic modeling of star-formation histories I: the scatter of the star-forming main sequence
• The effects of cosmic rays on the formation of Milky Way-mass galaxies in a cosmological context
• Tidally induced bars in Illustris galaxies
• The effect of baryons on redshift space distortions and cosmic density and velocity fields in the EAGLE simulation
• Atomic hydrogen in IllustrisTNG galaxies: the impact of environment parallelled with local 21-cm surveys
• Mass assembly and morphological transformations since $z\sim 3$ from CANDELS
• Numerical Convergence in Smoothed Particle Hydrodynamics
• The Massive Ancient Galaxies At $z>3$ NEar-infrared (MAGAZ3NE) Survey: Confirmation of Extremely Rapid Star-Formation and Quenching Timescales for Massive Galaxies in the Early Universe
• The Copernicus Complexio: a high-resolution view of the small-scale Universe
• The impact of baryonic physics on the subhalo mass function and implications for gravitational lensing
• Cosmological simulation with dust formation and destruction
• Dark Matter Superfluidity and Galactic Dynamics
• Galaxy Formation with BECDM -- II. Cosmic Filaments and First Galaxies
• The uniformity and time-invariance of the intra-cluster metal distribution in galaxy clusters from the IllustrisTNG simulations
• The THESAN project: Lyman-alpha emission and transmission during the Epoch of Reionization
• SDSS IV MaNGA - The spatially resolved transition from star formation to quiescence
• A census of cool core galaxy clusters in IllustrisTNG
• Spatially Resolved Star Formation and Inside-out Quenching in the TNG50 Simulation and 3D-HST Observations
• The physics of multiphase gas flows: fragmentation of a radiatively cooling gas cloud in a hot wind
• NIHAO IX: the role of gas inflows and outflows in driving the contraction and expansion of cold dark matter haloes
• The origin of most massive black holes at high-z: BLUETIDES and the next quasar frontier
• Mapping substructure in the HST Frontier Fields cluster lenses and in cosmological simulations
• The low-end of the black hole mass function at cosmic dawn
• Formation and Incidence of Shell Galaxies in the Illustris Simulation
• Quiescence correlates strongly with directly-measured black hole mass in central galaxies
• Revealing the galaxy-halo connection in IllustrisTNG
• Efficient early stellar feedback can suppress galactic outflows by reducing supernova clustering
• The KMOS Redshift One Spectroscopic Survey (KROSS): rotational velocities and angular momentum of z~0.9 galaxies
• Star formation in galaxies at z~4-5 from the SMUVS survey: a clear starburst/main-sequence bimodality for Halpha emitters on the SFR-M* plane
• The splashback radius of halos from particle dynamics. I. The SPARTA algorithm
• Galaxies in the EAGLE hydrodynamical simulation and in the Durham and Munich semi-analytical models
• Self-Interacting Dark Matter Subhalos in the Milky Way's Tides
• Modelling the large scale structure of the Universe as a function of cosmology and baryonic physics
• Colours, Star formation Rates, and Environments of Star forming and Quiescent Galaxies at the Cosmic Noon
• Simulations of the star-forming molecular gas in an interacting M51-like galaxy
• Host galaxies of merging compact objects: mass, star formation rate, metallicity and colours
• Numerical convergence of simulations of galaxy formation: the abundance and internal structure of cold dark matter haloes
• Supermassive black holes as the regulators of star formation in central galaxies
• The Origin and Evolution of Fast and Slow Rotators in the Illustris Simulation
• The Obelisk simulation: galaxies contribute more than AGN to HI reionization of protoclusters
• The masses and metallicities of stellar haloes reflect galactic merger histories
• Trident: a universal tool for generating synthetic absorption spectra from astrophysical simulations
• From light to baryonic mass: the effect of the stellar mass-to-light ratio on the Baryonic Tully-Fisher relation
• MIGHTEE-HI: The HI emission project of the MeerKAT MIGHTEE survey
• Black Hole - Galaxy Scaling Relationships for Active Galactic Nuclei with Reverberation Masses
• Simulating Groups and the IntraGroup Medium: The Surprisingly Complex and Rich Middle Ground Between Clusters and Galaxies
• Gas-phase metallicity gradients of TNG50 star-forming galaxies
• Massive Close Pairs Measure Rapid Galaxy Assembly in Mergers at High Redshift
• Repeated mergers, mass-gap black holes, and formation of intermediate-mass black holes in nuclear star clusters
• Timing the formation and assembly of early-type galaxies via spatially resolved stellar populations analysis
• Chaos and Variance in Galaxy Formation
• Advanced LIGO Constraints on Neutron Star Mergers and R-Process Sites
• Combined Solar System and rotation curve constraints on MOND
• Galaxies in the Illustris simulation as seen by the Sloan Digital Sky Survey - II: Size-luminosity relations and the deficit of bulge-dominated galaxies in Illustris at low mass
• COSMOS2020: The cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z~5
• Panchromatic Hubble Andromeda Treasury XVIII. The High-mass Truncation of the Star Cluster Mass Function
• Line-Intensity Mapping: Theory Review
• Outflows Driven by Quasars in High-Redshift Galaxies with Radiation Hydrodynamics
• The SAMI Galaxy Survey: comparing 3D spectroscopic observations with galaxies from cosmological hydrodynamical simulations
• The Scaling of Stellar Mass and Central Stellar Velocity Dispersion for Quiescent galaxies at z < 0.7
• A dormant, overmassive black hole in the early Universe
• Galaxy gas as obscurer: II. Separating the galaxy-scale and nuclear obscurers of Active Galactic Nuclei
• No cores in dark matter-dominated dwarf galaxies with bursty star formation histories
• The Novel Probes Project -- Tests of Gravity on Astrophysical Scales
• The Hubble Sequence at $z\sim 0$ in the IllustrisTNG simulation with deep learning
• Reproducing the Kinematics of Damped Lyman-alpha Systems
• Consistent lensing and clustering in a low-$S_8$ Universe with BOSS, DES Year 3, HSC Year 1 and KiDS-1000
• Galaxy Zoo: Morphological Classifications for 120,000 Galaxies in HST Legacy Imaging
• A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): JWST Reveals a Filamentary Structure around a z=6.61 Quasar
• First Light And Reionisation Epoch Simulations (FLARES) II: The Photometric Properties of High-Redshift Galaxies
• Fast Radio Bursts and cosmological tests
• The Nature of Massive Transition Galaxies in CANDELS, GAMA, and Cosmological Simulations
• High Angular Momentum Halo Gas: a Feedback and Code-Independent Prediction of LCDM
• The MillenniumTNG Project: The galaxy population at $z\ge 8$
• Fast galaxy bars continue to challenge standard cosmology
• A Deep Learning Approach to Galaxy Cluster X-ray Masses
• Galaxy Merger Rates up to z $\sim$ 3 using a Bayesian Deep Learning Model $-$ A Major-Merger classifier using IllustrisTNG Simulation data
• Lens galaxies in the Illustris simulation: power-law models and the bias of the Hubble constant from time-delays
• Hunting for Massive Black Holes in Dwarf Galaxies
• On the Assembly of Dwarf Galaxies in Clusters and their Efficient Formation of Globular Clusters
• Emulation of baryonic effects on the matter power spectrum and constraints from galaxy cluster data
• Major Merging History in CANDELS. I. Evolution of the Incidence of Massive Galaxy-Galaxy Pairs from z=3 to z~0
• JADES: A large population of obscured, narrow line AGN at high redshift
• Black Hole -- Galaxy Correlations in Simba
• Large-scale mass distribution in the Illustris simulation
• The relationship between the morphology and kinematics of galaxies and its dependence on dark matter halo structure in EAGLE
• Identifying Galaxy Mergers in Observations and Simulations with Deep Learning
• On the OVI Abundance in the Circumgalactic Medium of Low-Redshift Galaxies
• Galaxy Zoo: the effect of bar-driven fueling on the presence of an active galactic nucleus in disc galaxies
• AGN-Driven Outflows in Dwarf Galaxies
• The vertical motion history of disk stars throughout the Galaxy
• The rapid growth phase of supermassive black holes
• Towards accurate cosmological predictions for rapidly oscillating scalar fields as dark matter
• MAHALO Deep Cluster Survey I. Accelerated and enhanced galaxy formation in the densest regions of a protocluster at z=2.5
• Gas and galaxies in filament between clusters of galaxies: The study of A399-A401
• Intrinsic alignments of galaxies in the MassiveBlack-II simulation: analysis of two-point statistics
• Probing Massive Black Hole Binary Populations with LISA
• Evaporating the Milky Way halo and its satellites with inelastic self-interacting dark matter
• Feedback reshapes the baryon distribution within haloes, in halo outskirts, and beyond: the closure radius from dwarfs to massive clusters
• Introducing the FirstLight project: UV luminosity function and scaling relations of primeval galaxies
• Linking galaxy structural properties and star formation activity to black hole activity with IllustrisTNG
• Massive BH Binaries as Periodically-Variable AGN
• Log-normal star formation histories in simulated and observed galaxies
• Scalar Field Dark Matter: Helping or Hurting Small-Scale Problems in Cosmology?
• Metallicity of stars formed throughout the cosmic history based on the observational properties of star forming galaxies
• The Multi-Wavelength Tully-Fisher relation with spatially resolved HI kinematics
• Storm in a "Teacup": a radio-quiet quasar with ~10kpc radio-emitting bubbles and extreme gas kinematics
• The large-scale properties of simulated cosmological magnetic fields
• And yet it flips: connecting galactic spin and the cosmic web
• The properties of the first galaxies in the BLUETIDES simulation
• Intrinsic Alignments of Galaxies in the Illustris Simulation
• An analysis of the evolving comoving number density of galaxies in hydrodynamical simulations
• Populations of filaments from the distribution of galaxies in numerical simulations
• Galactic rotation curves, the baryon-to-dark-halo-mass relation and space-time scale invariance
• The impact of the observed baryon distribution in haloes on the total matter power spectrum
• The unorthodox evolution of major merger remnants into star-forming spiral galaxies
• The MUSE Hubble Ultra Deep Field Survey. IX. Evolution of galaxy merger fraction since z~6
• On the persistence of two small-scale problems in ΛCDM
• The inner structure of early-type galaxies in the Illustris simulation
• Shock finding on a moving-mesh: I. Shock statistics in non-radiative cosmological simulations
• The Tully-Fisher and mass-size relations from halo abundance matching
• On the impact of baryons on the halo mass function, bias, and cluster cosmology
• Post-Newtonian dynamical modeling of supermassive black holes in galactic-scale simulations
• The MillenniumTNG Project: High-precision predictions for matter clustering and halo statistics
• Interacting galaxies in the IllustrisTNG simulations -- I: Triggered star formation in a cosmological context
• Massive black hole evolution models confronting the n-Hz amplitude of the stochastic gravitational wave background
• Formation channels of single and binary stellar-mass black holes
• The structural and dynamical properties of compact elliptical galaxies
• The SAMI Galaxy Survey: Data Release One with Emission-line Physics Value-Added Products
• The impact of baryonic discs on the shapes and profiles of self-interacting dark matter halos
• Early- and late-stage mergers among main sequence and starburst galaxies at 0.2<z<2
• The ALMA Spectroscopic Survey in the HUDF: the molecular gas content of galaxies and tensions with IllustrisTNG and the Santa Cruz SAM
• Dust scaling relations in a cosmological simulation
• The Evolution of the Fractions of Quiescent and Star-forming Galaxies as a Function of Stellar Mass Since z=3: Increasing Importance of Massive, Dusty Star-forming Galaxies in the Early Universe
• A little FABLE: exploring AGN feedback in dwarf galaxies with cosmological simulations
• How baryons affect halos and large-scale structure: a unified picture from the Simba simulation
• Trinity I: Self-Consistently Modeling the Dark Matter Halo-Galaxy-Supermassive Black Hole Connection from $z=0-10$
• Disruption of satellite galaxies in simulated groups and clusters: the roles of accretion time, baryons, and pre-processing
• The diverse dark matter density at sub-kiloparsec scales in Milky Way satellites:implications for the nature of dark matter
• Deviations from hydrostatic equilibrium in the circumgalactic medium: spinning hot haloes and accelerating flows
• Multi-tracer extension of the halo model: probing quenching and conformity in eBOSS
• Spin evolution and feedback of supermassive black holes in cosmological simulations
• Properties of HI discs in the Auriga cosmological simulations
• Dynamical Friction Modeling of Massive Black Holes in Cosmological Simulations and Effects on Merger Rate Predictions
• Hot Gaseous Coronae around Spiral Galaxies: Probing the Illustris Simulation
• Molecular Gas Contents and Scaling Relations for Massive Passive Galaxies at Intermediate Redshifts from the LEGA-C Survey
• High-redshift quasars and their host galaxies I: kinematical and dynamical properties and their tracers
• Dark Energy Survey Year 3 results: cosmological constraints from the analysis of cosmic shear in harmonic space
• High Eccentricities and High Masses Characterize Gravitational-wave Captures in Galactic Nuclei as Seen by Earth-based Detectors
• ELUCID IV: Galaxy Quenching and its Relation to Halo Mass, Environment, and Assembly Bias
• SPECULATOR: Emulating stellar population synthesis for fast and accurate galaxy spectra and photometry
• 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
• Dark-ages Reionization and Galaxy Formation Simulation - X. The small contribution of quasars to reionization
• Spurious heating of stellar motions in simulated galactic disks by dark matter halo particles
• The quenching of galaxies, bulges, and disks since cosmic noon: A machine learning approach for identifying causality in astronomical data
• Chasing passive galaxies in the early Universe: a critical analysis in CANDELS GOODS-South
• The buildup of strongly barred galaxies in the TNG100 simulation
• The fate of disk galaxies in IllustrisTNG clusters
• The THESAN project: predictions for multi-tracer line intensity mapping in the epoch of reionization
• Supermassive black holes in cosmological simulations II: the AGN population and predictions for upcoming X-ray missions
• First Light And Reionisation Epoch Simulations (FLARES) V: The redshift frontier
• Galaxy-halo alignments in the Horizon-AGN cosmological hydrodynamical simulation
• Distinguishing Mergers and Disks in High Redshift Observations of Galaxy Kinematics
• Painting galaxies into dark matter halos using machine learning
• An Artificial Neural Network Approach For Ranking Quenching Parameters In Central Galaxies
• An EAGLE's View of Ex-situ Galaxy Growth
• Black-hole-regulated star formation in massive galaxies
• What shapes a galaxy? - Unraveling the role of mass, environment and star formation in forming galactic structure
• The evolution of the Milky Way: New insights from open clusters
• LYRA I: Simulating the multi-phase ISM of a dwarf galaxy with variable energy supernovae from individual stars
• NIHAO XX: The impact of the star formation threshold on the cusp-core transformation of cold dark matter haloes
• The colors of satellite galaxies in the Illustris Simulation
• Baryonic and dark matter distribution in cosmological simulations of spiral galaxies
• Co-evolution of massive black holes and their host galaxies at high redshift: discrepancies from six cosmological simulations and the key role of JWST
• Fast and energetic AGN-driven outflows in simulated dwarf galaxies
• Black hole feeding and feedback: the physics inside the "subgrid"
• NIHAO VIII: Circum-galactic medium and outflows - The puzzles of HI and OVI gas distributions
• The information content of stellar halos: Stellar population gradients and accretion histories in early-type Illustris galaxies
• NIHAO VI. The hidden discs of simulated galaxies
• The Effects of AGN Feedback on Present-Day Galaxy Properties in Cosmological Simulations
• SHARP - IV. An apparent flux ratio anomaly resolved by the edge-on disc in B0712+472
• Quiescent Ultra-diffuse galaxies in the field originating from backsplash orbits
• Light, medium-weight or heavy? The nature of the first supermassive black hole seeds
• QSO obscuration at high redshift ($z\gtrsim 7$): Predictions from the BlueTides simulation
• The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations
• Predictions for deep galaxy surveys with JWST from $\Lambda$CDM
• The relationship between fine galaxy stellar morphology and star formation activity in cosmological simulations: a deep learning view
• Tracing Outflowing Metals in Simulations of Dwarf and Spiral Galaxies
• On the evolution of galaxy spin in a cosmological hydrodynamic simulation of galaxy clusters
• The origin of dust in galaxies across cosmic time
• The Milky Way's Halo and Subhalos in Self-Interacting Dark Matter
• Being KLEVER at cosmic noon: ionised gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts
• The Galaxy Clustering Crisis in Abundance Matching
• The physical origins and dominant emission mechanisms of Lyman-alpha halos: results from the TNG50 simulation in comparison to MUSE observations
• Probing the nature of dark matter by forward modeling flux ratios in strong gravitational lenses
• Galaxy formation with L-GALAXIES: Modelling the environmental dependency of galaxy evolution and comparing with observations
• Powderday: Dust Radiative Transfer for Galaxy Simulations
• The Argo Simulation: II. The Early Build-up of the Hubble Sequence
• The interplay of Self-Interacting Dark Matter and baryons in shaping the halo evolution
• Dissecting the Gaseous Halos of z~2 Damped Ly$\alpha$ Systems with Close Quasar Pairs
• Automated Distant Galaxy Merger Classifications from Space Telescope Images using the Illustris Simulation
• Future constraints on halo thermodynamics from combined Sunyaev-Zel'dovich measurements
• A flexible modelling of galaxy assembly bias
• Systematic search for tidal features around nearby galaxies: I. Enhanced SDSS imaging of the Local Volume
• Scaling relations between black holes and their host galaxies: comparing theoretical and observational measurements, and the impact of selection effects
• The spin alignment of galaxies with the large-scale tidal field in hydrodynamic simulations
• The origin of low-surface-brightness galaxies in the dwarf regime
• Galaxy bias and primordial non-Gaussianity: insights from galaxy formation simulations with IllustrisTNG
• Galaxy mergers moulding the circum-galactic medium - I. The impact of a major merger
• Triggering and Delivery Algorithms for AGN Feedback
• Statistical properties of paired fixed fields
• The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- I: Halo Gas Properties and the Role of SMBH Feedback
• The Velocity Dispersion Function of Very Massive Galaxy Clusters: Abell 2029 and Coma
• The coherent motion of Cen A dwarf satellite galaxies remains a challenge for $\Lambda$CDM cosmology
• The fundamental signature of star formation quenching from AGN feedback: A critical dependence of quiescence on supermassive black hole mass not accretion rate
• Identifying the subtle signatures of feedback from distant AGN using ALMA observations and the EAGLE hydrodynamical simulations
• GalaxyNet: Connecting galaxies and dark matter haloes with deep neural networks and reinforcement learning in large volumes
• Probing 3D Structure with a Large MUSE Mosaic: Extending the Mass Model of Frontier Field Abell 370
• Intrinsic alignments of disk and elliptical galaxies in the MassiveBlack-II and Illustris simulations
• When the Jeans don't fit: How stellar feedback drives stellar kinematics and complicates dynamical modeling in low-mass galaxies
• RAiSE II: resolved spectral evolution in radio AGN
• Flux-ratio anomalies from discs and other baryonic structures in the Illustris simulation
• The Impact of Galactic Winds on the Angular Momentum of Disk Galaxies in the Illustris Simulation
• Hydrogen Reionization in the Illustris universe
• Machine Learning and Cosmological Simulations II: Hydrodynamical Simulations
• The galaxy-halo connection of emission-line galaxies in IllustrisTNG
• ALMA measures rapidly depleted molecular gas reservoirs in massive quiescent galaxies at z~1.5
• Impact of Lyman alpha pressure on metal-poor dwarf galaxies
• EMERGE: Empirical predictions of galaxy merger rates since $z\sim 6$
• T-ReX: a graph-based filament detection method
• The ALPINE-ALMA [CII] survey: The contribution of major mergers to the galaxy mass assembly at z~5
• Evaluating Galactic Habitability Using High Resolution Cosmological Simulations of Galaxy Formation
• A Slippery Slope: Systematic Uncertainties in the Line Width Baryonic Tully-Fisher Relation
• The SLUGGS Survey: Dark matter fractions at large radii and assembly epochs of early-type galaxies from globular cluster kinematics
• A three-phase amplification of the cosmic magnetic field in galaxies
• The stellar halos of ETGs in the IllustrisTNG simulations: the photometric and kinematic diversity of galaxies at large radii
• The impact of quenching on galaxy profiles in the Simba simulation
• Introducing a new, robust galaxy finder algorithm for simulations
• Mg II Absorption at 2<z<7 with Magellan/FIRE, III. Full Statistics of Absorption Towards 100 High-Redshift QSOs
• Simulations of Jet Heating in Galaxy Clusters: Successes and Challenges
• Assessing the Jeans Anisotropic Multi-Gaussian Expansion method with the Illustris simulation
• Merging Cluster Collaboration: A Panchromatic Atlas of Radio Relic Mergers
• Dynamical evolution of cosmic supermassive binary black holes and their gravitational wave radiation
• New criteria for the selection of galaxy close pairs from cosmological simulations: evolution of the major and minor merger fraction in MUSE deep fields
• The baryon content of groups and clusters of galaxies in the FABLE simulations
• Rotation curve fitting and its fatal attraction to cores in realistically simulated galaxy observations
• Baryonic effects for weak lensing. Part II. Combination with X-ray data and extended cosmologies
• Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
• Galaxy bias from forward models: linear and second-order bias of IllustrisTNG galaxies
• Herschel-ATLAS: Revealing dust build-up and decline across gas, dust and stellar mass selected samples: I. Scaling relations
• Dust in and around galaxies: dust in cluster environments and its impact on gas cooling
• The mass, colour, and structural evolution of today's massive galaxies since z~5
• Empirical constraints on the formation of early-type galaxies
• Constraining the HI-Halo Mass Relation From Galaxy Clustering
• Galaxy gas as obscurer: I. GRBs x-ray galaxies and find a N_H ~ M* relation
• Barred Galaxies in the IllustrisTNG Simulation
• Expectations of the size evolution of massive galaxies at $3\le z\le 6$ from the TNG50 simulation: the CEERS/JWST view
• The merger and assembly histories of Milky Way- and M31-like galaxies with TNG50: disk survival through mergers
• NIHAO XIX: How supernova feedback shapes the galaxy baryon cycle
• Subhalo Demographics in the Illustris Simulation: Effects of Baryons and Halo-to-Halo Variation
• Redshift and luminosity evolution of the intrinsic alignments of galaxies in Horizon-AGN
• Thermal and radiative AGN feedback have a limited impact on star formation in high-redshift galaxies
• Host galaxy properties of mergers of stellar binary black holes and their implications for advanced LIGO gravitational wave sources
• Fitting the nonlinear matter bispectrum by the Halofit approach
• The origin and properties of massive prolate galaxies in the Illustris simulation
• The star formation rate and stellar content contributions of morphological components in the EAGLE simulations
• Extensions to models of the galaxy-halo connection
• Host galaxies of high-redshift quasars: supermassive black hole growth and feedback
• IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation
• The formation of Milky Way-mass disk galaxies in the first 500 million years of a cold dark matter universe
• On the Appearance of Thresholds in the Dynamical Model of Star Formation
• Effects of simulated cosmological magnetic fields on the galaxy population
• The stellar halos of ETGs in the IllustrisTNG simulations: II. Accretion, merger history, and dark halo connection
• Stellar Halos in Illustris- Probing the Histories of Milky Way-Mass Galaxies
• SFHs OF $Z\sim 1$ Galaxies in LEGA-C
• The Shapes of the Rotation Curves of Star-forming Galaxies Over the Last $\approx$10 Gyr
• Simulating the interstellar medium of galaxies with radiative transfer, non-equilibrium thermochemistry, and dust
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• The edge of galaxy formation I: formation and evolution of MW-satellites analogues before accretion
• Simultaneous modelling of matter power spectrum and bispectrum in the presence of baryons
• Merger of compact stars in the two-families scenario
• Galactic inflow and wind recycling rates in the EAGLE simulations
• Realistic simulations of galaxy formation in f(R) modified gravity
• Bulge plus disc and Sérsic decomposition catalogues for 16,908 galaxies in the SDSS Stripe 82 co-adds: A detailed study of the $ugriz$ structural measurements
• Bounding Alternative Theories of Gravity with Multi-Band GW Observations
• Forecasts on dark energy from the X-ray cluster survey with eROSITA: constraints from counts and clustering
• Estimating the Mass of the Milky Way Using the Ensemble of Classical Satellite Galaxies
• Mock catalogs for the extragalactic X-ray sky: simulating AGN surveys with Athena and with the AXIS probe
• Detailed HI kinematics of Tully-Fisher calibrator galaxies
• A missing outskirts problem? Comparisons between stellar halos in the Dragonfly Nearby Galaxies Survey and the TNG100 simulation
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Identification of AGN through SED Fitting and the Evolution of the Bolometric AGN Luminosity Function
• The Relationship Between Star-formation Activity and Galaxy Structural Properties in CANDELS and a Semi-analytic Model
• On the origin of gas-poor galaxies in galaxy clusters using cosmological hydrodynamic simulations
• Accurate mass and velocity functions of dark matter halos
• Cosmological Galaxy Evolution with Superbubble Feedback II: The Limits of Supernovae
• Orbits of massive satellite galaxies: II. Bayesian Estimates of the Milky Way and Andromeda masses using high precision astrometry and cosmological simulations
• SDSS IV MaNGA: Visual Morphological and Statistical Characterization of the DR15 sample
• KASHz: No evidence for ionised outflows instantaneously suppressing star formation in moderate luminosity AGN at $z$$\sim$$1.4$-$2.6$
• A direct measurement of galaxy major and minor merger rates and stellar mass accretion histories at $z<3$ using galaxy pairs in the REFINE survey
• The structure and assembly history of cluster-size haloes in Self-Interacting Dark Matter
• Predictions for local PNG bias in the galaxy power spectrum and bispectrum and the consequences for $f_{\mathrm{NL}}$ constraints
• On the Origin of Diffuse Ionized Gas in the Antennae Galaxy
• Mapping stellar content to dark matter halos - III.Environmental dependence and conformity of galaxy colours
• Black-hole remnants from black-hole--neutron-star mergers
• The effects of host galaxy properties on merging compact binaries detectable by LIGO
• Constraining baryonic feedback and cosmology with weak-lensing, X-ray, and kinematic Sunyaev-Zeldovich observations
• Self-Interacting Dark Matter and Small-Scale Gravitational Lenses in Galaxy Clusters
• Weak Lensing Reveals a Tight Connection Between Dark Matter Halo Mass and the Distribution of Stellar Mass in Massive Galaxies
• The accretion of dark matter subhaloes within the cosmic web: primordial anisotropic distribution and its universality
• The splashback boundary of haloes in hydrodynamic simulations
• High redshift JWST predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves
• The central densities of Milky Way-mass galaxies in cold and self-interacting dark matter models
• Galaxy Zoo: Unwinding the Winding Problem - Observations of Spiral Bulge Prominence and Arm Pitch Angles Suggest Local Spiral Galaxies are Winding
• Origin and evolution of ultra-diffuse galaxies in different environments
• A moving mesh unstaggered constrained transport scheme for magnetohydrodynamics
• Advances in Constraining Intrinsic Alignment Models with Hydrodynamic Simulations
• Testing the effect of galactic feedback on the IGM at z ~ 6 with metal-line absorbers
• Validating Semi-Analytic Models of High-Redshift Galaxy Formation using Radiation Hydrodynamical Simulations
• A JWST Survey of the Supernova Remnant Cassiopeia A
• Common Envelope Evolution on a Moving Mesh
• A quartet of black holes and a missing duo: probing the low-end of the Mbh - sigma relation with the adaptive optics assisted integral-field spectroscopy
• The merger-starburst connection across cosmic times
• Sub one percent mass fractions of young stars in red massive galaxies
• Increasing blackhole feedback induced quenching with anisotropic thermal conduction
• ETHOS -- an effective theory of structure formation: predictions for the high-redshift Universe -- abundance of galaxies and reionization
• Modeling Galactic Conformity with the Color-Halo Age Relation in the Illustris Simulation
• Dark Energy Survey Year 1 Results: Constraining Baryonic Physics in the Universe
• Learning the Relationship between Galaxies Spectra and their Star Formation Histories using Convolutional Neural Networks and Cosmological Simulations
• MUFASA: The assembly of the red sequence
• Galaxy And Mass Assembly (GAMA): The sSFR-M* relation part I - ${\sigma }_{\mathrm{sSFR}}$-M* as a function of sample, SFR indicator and environment
• The dependence of the galaxy stellar-to-halo mass relation on galaxy morphology
• On CMB B-Mode Non-Gaussianity
• FOREVER22: galaxy formation in protocluster regions
• Morphological decomposition of TNG50 galaxies: methodology and catalogue
• YZiCS: Preprocessing of dark halos in the hydrodynamic zoom-in simulation of clusters
• Galactic angular momentum in the IllustrisTNG simulation -- I. Connection to morphology, halo spin, and black hole mass
• The rise and fall of stellar discs across the peak of cosmic star formation history: mergers versus smooth accretion
• Semi-analytic forecasts for JWST -- V. AGN luminosity functions and helium reionization at z = 2-7
• Machine Learning and Cosmological Simulations I: Semi-Analytical Models
• Growing a `Cosmic Beast': Observations and Simulations of MACS J0717.5+3745
• nIFTy Galaxy Cluster simulations IV: Quantifying the Influence of Baryons on Halo Properties
• The host galaxies of double compact objects merging in the local Universe
• Direct Measurement of the HI-Halo Mass Relation through Stacking
• The manifestation of secondary halo bias on the galaxy population from IllustrisTNG300
• No signs of star formation being regulated in the most luminous quasars at z~2 with ALMA
• The Cosmic Microwave Background: The history of its experimental investigation and its significance for cosmology
• Strong-lensing Measurement of the Mass-density Profile out to 3 Effective Radii for $z\sim 0.5$ Early-type Galaxies
• Radiation-MagnetoHydrodynamics simulations of cosmic ray feedback in disc galaxies
• Order out of Randomness : Self-Organization Processes in Astrophysics
• Kinematic decomposition of IllustrisTNG disk galaxies: morphology and relation with morphological structures
• On the origin of star-gas counterrotation in low-mass galaxies
• On the influence of halo mass accretion history on galaxy properties and assembly bias
• Galaxy Mergers in the Epoch of Reionization I: A JWST Study of Pair Fractions, Merger Rates, and Stellar Mass Accretion Rates at $z=4.5-11.5$
• A detection of wobbling Brightest Cluster Galaxies within massive galaxy clusters
• Origin of the galaxy HI size-mass relation
• Formation of a Malin 1 analogue in IllustrisTNG by stimulated accretion
• AGN feedback, quiescence and CGM metal enrichment in early-type galaxies
• Climbing to the top of the galactic mass ladder: evidence for frequent prolate-like rotation among the most massive galaxies
• Imprints of temperature fluctuations on the $z\sim 5$ Lyman-$\alpha$ forest: a view from radiation-hydrodynamic simulations of reionization
• Efficient Computation of Galaxy Bias with Neutrinos and Other Relics
• AGN jet feedback on a moving mesh: gentle cluster heating by weak shocks and lobe disruption
• Following The Cosmic Evolution Of Pristine Gas I: Implications For Milky Way Halo Stars
• Cosmological baryon transfer in the SIMBA simulations
• DeepMerge II: Building Robust Deep Learning Algorithms for Merging Galaxy Identification Across Domains
• First results from SMAUG: The need for preventative stellar feedback and improved baryon cycling in semi-analytic models of galaxy formation
• The origin of the enhanced metallicity of satellite galaxies
• Early-type galaxy density profiles from IllustrisTNG: I. Galaxy correlations and the impact of baryons
• Signatures of stellar accretion in MaNGA early-type galaxies
• Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
• WISDOM project - IV. A molecular gas dynamical measurement of the supermassive black hole mass in NGC 524
• Gravitational Lensing and the Power Spectrum of Dark Matter Substructure: Insights from the ETHOS N-body Simulations
• Realistic galaxy image simulation via score-based generative models
• Metal enrichment in the circumgalactic medium and Lyα haloes around quasars at z $\sim$3
• Extreme kinematic misalignment in IllustrisTNG galaxies: the origin, structure and internal dynamics of galaxies with a large-scale counterrotation
• The SAMI Galaxy Survey: a statistical approach to an optimal classification of stellar kinematics in galaxy surveys
• Comprehensive Gas Characterization of a $z=2.5$ Protocluster: A Cluster Core Caught in the Beginning of Virialization?
• The emergence of passive galaxies in the early Universe
• Separate Universe Simulations with IllustrisTNG: baryonic effects on power spectrum responses and higher-order statistics
• Galaxies lacking dark matter in the Illustris simulation
• A machine learning approach to mapping baryons onto dark matter haloes using the EAGLE and C-EAGLE simulations
• Beyond halo mass: quenching galaxy mass assembly at the edge of filaments
• Realistic mock observations of the sizes and stellar mass surface densities of massive galaxies in FIRE-2 zoom-in simulations
• Caustic Skeleton & Cosmic Web
• INFERNO: Galactic winds in dwarf galaxies with star-by-star simulations including runaway stars
• The Next Generation Virgo Cluster Survey (NGVS). XXIV. The Red Sequence to $\sim$10${}^6$ L${}_{\odot }$ and Comparisons with Galaxy Formation Models
• The combined effect of AGN and supernovae feedback in launching massive molecular outflows in high-redshift galaxies
• Constraining the Baryonic Feedback with Cosmic Shear Using the DES Year-3 Small-Scale Measurements
• The KMOS${}^{3D}$ Survey: rotating compact star forming galaxies and the decomposition of integrated line widths
• TDCOSMO. VII. Boxyness/discyness in lensing galaxies : Detectability and impact on $H_0$
• Barred galaxies in the Illustris-1 and TNG100 simulations
• The Faber-Jackson relation and Fundamental Plane from halo abundance matching
• Efficacy of early stellar feedback in low gas surface density environments
• New Analytic Solutions for Galaxy Evolution: Gas, Stars, Metals and Dust in local Early-Type Galaxies and in their high-z Starforming Progenitors
• The evolution of the stellar mass versus halo mass relationship
• The nature of H-alpha star-forming galaxies at z~0.4 in and around Cl 0939+4713: the environment matters
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). The decline of cosmic star formation: quenching, mass, and environment connections
• Triggering Active Galactic Nuclei in galaxy clusters
• Cosmic shear with small scales: DES-Y3, KiDS-1000 and HSC-DR1
• Stellar mass functions of galaxies, disks and spheroids at z~0.1
• The Growth and Enrichment of the Intragroup Gas
• Momentum-driven Winds from Radiatively Efficient Black Hole Accretion and Their Impact on Galaxies
• Characterizing hydrostatic mass bias with Mock-X
• Baryons in the CosmicWeb of IllustrisTNG -- II: the Connection among Galaxies, Halos, their Formation Time and their Location in the Cosmic Web
• The Little Galaxies that Could (Reionize the Universe): Predicting Faint End Slopes & Escape Fractions at z > 4
• Young and turbulent: the early life of massive galaxy progenitors
• The growth of brightest cluster galaxies in the TNG300 simulation:dissecting the contributions from mergers and in situ star formation
• RAMSES-RTZ: Non-Equilibrium Metal Chemistry and Cooling Coupled to On-The-Fly Radiation Hydrodynamics
• Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations
• The limited role of galaxy mergers in driving stellar mass growth over cosmic time
• The LBT Satellites of Nearby Galaxies Survey (LBT-SONG): The Satellite Population of NGC 628
• The high redshift SFR-M* relation is sensitive to the employed star formation rate and stellar mass indicators: Towards addressing the tension between observations and simulations
• From Stellar Halos to Intracluster Light: the physics of the Intra-Halo Stellar Component in cosmological hydrodynamical simulations
• Evaluating the ability of triaxial Schwarzschild modelling to estimate properties of galaxies from the Illustris simulation
• High redshift JWST predictions from IllustrisTNG: III. Infrared luminosity functions, obscured star formation and dust temperature of high-redshift galaxies
• Identifying kinematic structures in simulated galaxies using unsupervised machine learning
• Physical origin of the large-scale conformity in the specific star formation rates of galaxies
• Interacting galaxies in the IllustrisTNG simulations -- III: (the rarity of) quenching in post-merger galaxies
• Realistic estimation for the detectability of dark matter sub-halos with Fermi-LAT
• The Mass and Absorption Columns of Galactic Gaseous Halos
• Simulating the effect of high column density absorbers on the one-dimensional Lyman-alpha forest flux power spectrum
• $\text{Mangrove}$: Learning Galaxy Properties from Merger Trees
• Predictions for anisotropic X-ray signatures in the circumgalactic medium: imprints of supermassive black hole driven outflows
• HST grism spectroscopy of z~3 massive quiescent galaxies: Approaching the metamorphosis
• NIHAO -- XXV. Convergence in the cusp-core transformation of cold dark matter haloes at high star formation thresholds
• The specific star formation rate function at different mass scales and quenching: A comparison between cosmological models and SDSS
• X-ray Emission From Hot Gas in Galaxy Groups and Clusters in Simba
• The Morphology-Density relationship in 1<z<2 clusters
• Forecasts for the WFIRST High Latitude Survey using the BlueTides Simulation
• Creating a galaxy lacking dark matter in a dark matter dominated universe
• The first Super Massive Black Holes: indications from models for future observations
• Submillimetre galaxies in cosmological hydrodynamical simulations -- an opportunity for constraining feedback models
• A universal relation between the properties of supermassive black holes, galaxies, and dark matter halos
• Large-scale jets from active galactic nuclei as a source of ICM heating: cavities and shocks
• Correlations Between Black Holes and Host Galaxies in the Illustris and IllustrisTNG Simulations
• From Dark Matter to Galaxies with Convolutional Networks
• Stellar Velocity Dispersion: Linking Quiescent Galaxies to their Dark Matter Halos
• The sensitivity of stellar feedback to IMF averaging versus IMF sampling in galaxy formation simulations
• PRIMUS: One- and Two-Halo Galactic Conformity at $0.2<z<1$
• Baryon effects on void statistics in the EAGLE simulation
• Dark matter stripping in galaxy clusters: a look at the Stellar to Halo Mass relation in the Illustris simulation
• The Radio Galaxy Population in the SIMBA SImulations
• The effect of differential accretion on the Gravitational Wave Background and the present day MBH Binary population
• VALES: I. The molecular gas content in star-forming dusty H-ATLAS galaxies up to z=0.35
• Galaxies in the Illustris simulation as seen by the Sloan Digital Sky Survey - I: Bulge+disc decompositions, methods, and biases
• The merger history of the complex cluster Abell 1758: a combined weak lensing and spectroscopic view
• Is there enough star formation in simulated protoclusters?
• Superluminous Spiral Galaxies
• The Incidence of Low-Metallicity Lyman-Limit Systems at z~3.5: Implications for the Cold-Flow Hypothesis of Baryonic Accretion
• MC${}^2$: Multi-wavelength and dynamical analysis of the merging galaxy cluster ZwCl 0008.8+5215: An older and less massive Bullet Cluster
• Extreme ionised outflows are more common when the radio emission is compact in AGN host galaxies
• Accelerated Bayesian SED Modeling using Amortized Neural Posterior Estimation
• Jet Feedback and the Photon Underproduction Crisis in Simba
• Estimates of Fast Radio Burst Dispersion Measures from Cosmological Simulations
• Galactic angular momentum in cosmological zoom-in simulations. I. Disk and bulge components and the galaxy--halo connection
• Time Evolution of Galaxy Scaling Relations in Cosmological Simulations
• The Mass Profile of the Milky Way to the Virial Radius from the Illustris Simulation
• Towards a radially-resolved semi-analytic model for the evolution of disc galaxies tuned with machine learning
• NIHAO XXII: Introducing black hole formation, accretion and feedback into the NIHAO simulation suite
• Morphological signatures of mergers in the TNG50 simulation and the Kilo-Degree Survey: the merger fraction from dwarfs to Milky Way-like galaxies
• The origin of metal-poor stars on prograde disk orbits in FIRE simulations of Milky Way-mass galaxies
• A thermal-kinetic subgrid model for supernova feedback in simulations of galaxy formation
• The star formation histories of dwarf galaxies in Local Group cosmological simulations
• Mass of the dynamically hot inner stellar halo predicts the ancient accreted stellar mass
• A 16 deg${}^2$ survey of emission-line galaxies at z<1.5 in HSC-SSP PDR1
• The impact of spurious collisional heating on the morphological evolution of simulated galactic discs
• Tidally induced warps of spiral galaxies in IllustrisTNG
• The Red and Featureless Outer Disks of Nearby Spiral Galaxies
• Reproducing the Universe: a comparison between the EAGLE simulations and the nearby DustPedia galaxy sample
• Low Angular Momentum in Clumpy, Turbulent Disk Galaxies
• The descendants of the first quasars in the BlueTides simulation
• An alternate approach to measure specific star formation rates at 2<z<7
• Cosmic variance of $z>7$ galaxies: Prediction from BlueTides
• Local SDSS galaxies in the Herschel Stripe82 survey: A critical assessment of optically-derived star-formation rates
• The edge of galaxy formation II: evolution of Milky Way satellite analogues after infall
• First Results on Dark Matter Substructure from Astrometric Weak Lensing
• Shock finding on a moving-mesh: II. Hydrodynamic shocks in the Illustris universe
• The MBHBM* Project -- I: Measurement of the Central Black Hole Mass in Dwarf Galaxy NGC 3504 Using Molecular Gas Kinematics
• Dust Obscured Star Forming Galaxies in the Early Universe
• The stellar metallicity gradients in galaxy discs in a cosmological scenario
• DES Y1 Results: Validating cosmological parameter estimation using simulated Dark Energy Surveys
• The mass assembly of high-redshift black holes
• Quenching and morphological evolution due to circumgalactic gas expulsion in a simulated galaxy with a controlled assembly history
• Galaxy interactions in IllustrisTNG-100, I: The power and limitations of visual identification
• Cooling in a Dissipative Dark Sector
• The Three Hundred Project: The influence of environment on simulated galaxy properties
• Controlling and leveraging small-scale information in tomographic galaxy-galaxy lensing
• SDSS--IV MaNGA : The Inner Density Slopes of nearby galaxies
• A redshift-dependent IRX-$\beta$ dust attenuation relation for TNG50 galaxies
• Dynamic Localised Turbulent Diffusion and its Impact on the Galactic Ecosystem
• The Angular Momentum of the Circumgalactic Medium in the TNG100 Simulation
• Accretion of Galaxy Groups into Galaxy Clusters
• Reconstructing the Assembly of Massive Galaxies. I: The Importance of the Progenitor Effect in the Observed Properties of Quiescent Galaxies at $z\approx 2$
• Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
• A parametric study of possible solutions to the high-redshift overproduction of stars in modeled dwarf galaxies
• Cosmic filaments in galaxy cluster outskirts: quantifying finding filaments in redshift space
• Probing Dark Matter Self-interaction with Ultra-faint Dwarf Galaxies
• How Environment Affects Galaxy Metallicity through Stripping and Formation History: Lessons from the Illustris Simulation
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• Statistical modelling of the cosmological dispersion measure
• Active galactic nucleus jet feedback in hydrostatic halos
• Tracing galaxy populations through cosmic time: A critical test of methods for connecting the same galaxies between different redshifts at $z<3$
• A Statistical Semi-Empirical Model: Satellite galaxies in Groups and Clusters
• Priors on Lagrangian bias parameters from galaxy formation modelling
• The Impact of Dust on the Sizes of Galaxies in the Epoch of Reionization
• A weak gravitational lensing recalibration of the scaling relations linking the gas properties of dark halos to their mass
• Modeling for Stellar Feedback in Galaxy Formation Simulations
• The Pristine Dwarf-Galaxy survey -- IV. Probing the outskirts of the dwarf galaxy Boötes I
• BlueTides simulation: establishing black hole-galaxy relations at high-redshift
• Gravitational Self-Lensing in Populations of Massive Black Hole Binaries
• Total density profile of massive early-type galaxies in Horizon-AGN simulation: impact of AGN feedback and comparison with observations
• Passive galaxies in the early Universe: ALMA confirmation of z~3-5 candidates in the CANDELS GOODS-South field
• RIGEL: Simulating dwarf galaxies at solar mass resolution with radiative transfer and feedback from individual massive stars
• Connecting the structure of dark matter haloes to the primordial power spectrum
• GA-NIFS: High number of dual active galactic nuclei at z~3
• The vertical structure of gaseous galaxy discs in cold dark matter halos
• The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- II: Cold, Dense Gas Clouds and High-Velocity Cloud Analogs
• The redshift evolution of X-ray and Sunyaev-Zel'dovich scaling relations in the FABLE simulations
• Globular clusters as tracers of the dark matter content of dwarfs in galaxy clusters
• On the Dynamics of Supermassive Black Holes in Gas-Rich, Star-Forming Galaxies: the Case for Nuclear Star Cluster Coevolution
• Simulated Bars May Be Shorter But Are Not Slower Than Observed: TNG50 vs. MaNGA
• The impact of magnetic fields on cosmological galaxy mergers. I: Reshaping gas and stellar discs
• Deep Realistic Extragalactic Model (DREaM) Galaxy Catalogs: Predictions for a Roman Ultra-Deep Field
• Statistics of galaxy mergers: bridging the gap between theory and observation
• Massive disc galaxies in cosmological hydrodynamical simulations are too dark matter-dominated
• Stellar Dynamics and Star-Formation Histories of z $\sim$ 1 Radio-loud Galaxies
• Statistical strong lensing. I. Constraints on the inner structure of galaxies from samples of a thousand lenses
• Dark Matter Trapping by Stellar Bars: The Shadow Bar
• AGN Selection Methods Have Profound Impacts on the Distributions of Host Galaxy Properties
• The core of the massive cluster merger MACS J0417.5-1154 as seen by VLT/MUSE
• Testing the Accuracy of Halo Occupation Distribution Modelling using Hydrodynamic Simulations
• The Pristine Dwarf-Galaxy survey -- III. Revealing the nature of the Milky Way globular cluster Sagittarius II
• On the effect of galactic outflows in cosmological simulations of disc galaxies
• Molecular hydrogen in IllustrisTNG galaxies: carefully comparing signatures of environment with local CO & SFR data
• Properties and Origin of Galaxy Velocity Bias in the Illustris Simulation
• A Comparison of Circumgalactic MgII Absorption between the TNG50 Simulation and the MEGAFLOW Survey
• The Contribution of In-situ and Ex-situ Star Formation in Early-Type Galaxies: MaNGA versus IllustrisTNG
• A gradient based method for modeling baryons and matter in halos of fast simulations
• The host galaxies of double compact objects across cosmic time
• The impact of environment and mergers on the HI content of galaxies in hydrodynamic simulations
• A study of stellar orbit fractions: simulated IllustrisTNG galaxies compared to CALIFA observations
• The Evolutionary Pathways of Disk-, Bulge-, and Halo-dominated Galaxies
• Correlations in the three-dimensional Lyman-alpha forest contaminated by high column density absorbers
• A Consistent Set of Empirical Scaling Relations for Spiral Galaxies: The $(v_{\max },M_{\mathrm{DM}})$-$({\sigma }_0,M_{\mathrm{BH}},\varphi )$ Relations
• Formation of massive disk galaxies in the IllustrisTNG simulation
• The Grism lens-amplified survey from space (GLASS). VII. The diversity of the distribution of star formation in cluster and field galaxies at 0.3<z<0.7
• Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
• Arkenstone I: A Novel Method for Robustly Capturing High Specific Energy Outflows In Cosmological Simulations
• The Conditional Colour-Magnitude Distribution: I. A Comprehensive Model of the Colour-Magnitude-Halo Mass Distribution of Present-Day Galaxies
• Not So Heavy Metals: Black Hole Feedback Enriches The Circumgalactic Medium
• The resolution bias: low resolution feedback simulations are better at destroying galaxies
• Galaxies with prolate rotation in Illustris
• The kinematics of globular cluster populations in the E-MOSAICS simulations and their implications for the assembly history of the Milky Way
• On the Determination of Rotation Velocity and Dynamical Mass of Galaxies Based on Integrated H I Spectra
• {\sc mirkwood:} Fast and Accurate SED Modeling Using Machine Learning
• Enhancing AGN efficiency and cool-core formation with anisotropic thermal conduction
• Galaxy assembly bias of central galaxies in the Illustris simulation
• Galactic outflow and diffuse gas properties at z>=1 using different baryonic feedback models
• SEAGLE - I: A pipeline for simulating and modeling strong lenses from cosmological hydrodynamic simulations
• Disc galaxies formed from major mergers in Illustris
• Monsters in the Dark: Predictions for Luminous Galaxies in the Early Universe from the BlueTides Simulation
• Can Cosmological Simulations Reproduce the Spectroscopically Confirmed Galaxies Seen at $z\ge 10$?
• SDSS-IV MaNGA: Uncovering the Angular Momentum Content of Central and Satellite Early-type Galaxies
• Inhomogeneous cosmology and backreaction: Current status and future prospects
• Quantifying AGN-Driven Metal-Enhanced Outflows in Chemodynamical Simulations
• The morphology and kinematics of the gaseous circumgalactic medium of Milky Way mass galaxies -- II. comparison of IllustrisTNG and Illustris simulation results
• Massive Black Hole Mergers with Orbital Information: Predictions from the ASTRID Simulation
• Defining the (Black Hole)-Spheroid Connection with the Discovery of Morphology-Dependent Substructure in the $M_{\mathrm{BH}}$--${\mathrm{n}}_{\mathrm{sph}}$ and $M_{\mathrm{BH}}$--${\mathrm{R}}_{\mathrm{e},\mathrm{sph}}$ Diagrams: New Tests for Advanced Theories and Realistic Simulations
• The formation of low surface brightness galaxies in the IllustrisTNG simulation
• Group quenching and galactic conformity at low redshift
• North Ecliptic Pole merging galaxy catalogue
• Does the Milky Way Obey Spiral Galaxy Scaling Relations?
• $R_{\mathrm{e}}$. I. Understanding galaxy sizes, associated luminosity densities, and the artificial division of the early-type galaxy population
• The locations of features in the mass distribution of merging binary black holes are robust against uncertainties in the metallicity-dependent cosmic star formation history
• An observational test for star formation prescriptions in cosmological hydrodynamical simulations
• Reaching for the Edge I: Probing the Outskirts of Massive Galaxies with HSC, DECaLS, SDSS, and Dragonfly
• Formation and settling of a disc galaxy during the last 8 billion years in a cosmological simulation
• The Close AGN Reference Survey (CARS): No obvious signature of AGN feedback on star formation, but subtle trends
• Forward and backward galaxy evolution in comoving number density space
• Emission from the circumgalactic medium: from cosmological zoom-in simulations to multiwavelength observables
• The First Quiescent Galaxies in TNG300
• Simulating the effect of photoheating feedback during reionization
• ETHOS - an Effective Theory of Structure Formation: detecting dark matter interactions through the Lyman-$\alpha$ forest
• WARPFIELD Population Synthesis: The physics of (extra-)Galactic star formation and feedback driven cloud structure and emission from sub-to-kpc scales
• $\mathrm{S}\mathrm{IM}\mathrm{BIG}$: Mock Challenge for a Forward Modeling Approach to Galaxy Clustering
• Testing strong lensing subhalo detection with a cosmological simulation
• The stellar halo of the Milky Way traced by blue horizontal-branch stars in the Subaru Hyper Suprime-Cam Survey
• Extensions to the halo occupation distribution model for more accurate clustering predictions
• Small-scale galaxy clustering in the EAGLE simulation
• Tidal destruction in a low mass galaxy environment: the discovery of tidal tails around DDO 44
• Fifth force constraints from the separation of galaxy mass components
• A deep learning view of the census of galaxy clusters in IllustrisTNG
• Strong Lensing by Galaxies
• Morphology and kinematics of orbital components in CALIFA galaxies across the Hubble sequence
• Probing the $z\gtrsim 6$ quasars in a universe with IllustrisTNG physics: Impact of gas-based black hole seeding models
• IQ-Collaboratory 1.1: the Star-Forming Sequence of Simulated Central Galaxies
• Constraining SIDM with halo shapes: revisited predictions from realistic simulations of early-type galaxies
• Modeling Evolution of Galactic Bars at Cosmic Dawn
• Do AGN triggering mechanisms vary with radio power? II. The importance of mergers as a function of radio power and optical luminosity
• UV to submillimetre luminosity functions of TNG50 galaxies
• The impact of galactic feedback on the shapes of dark-matter haloes
• Direct Detection of Mirror Matter in Twin Higgs Models
• Small- and Large-Scale Galactic Conformity in SDSS DR7
• Simulating the Spatial Distribution and Kinematics of Globular Clusters within Galaxy Clusters in Illustris
• IQ Collaboratory II: The Quiescent Fraction of Isolated, Low Mass Galaxies Across Simulations and Observations
• The Missing Satellite Problem in 3D
• Baryon-CDM isocurvature galaxy bias with IllustrisTNG
• Deviations from tidal torque theory: evolution of the halo spin-filament alignment
• Rivers of Gas I.: Unveiling The Properties of High Redshift Filaments
• Barred spiral galaxies in modified gravity theories
• Supernovae feedback propagation: the role of turbulence
• Massive Low Surface Brightness Galaxies in the EAGLE Simulation
• The Pandora project. I: the impact of radiation and cosmic rays on baryonic and dark matter properties of dwarf galaxies
• The halo of M49 and its environment as traced by planetary nebulae
• Abell 2744: Too much substructure for Lambda CDM?
• Cosmological simulations of massive black hole seeds: predictions for next generation electromagnetic and gravitational wave observations
• Uncertainties in supernova input rates drive qualitative differences in simulations of galaxy evolution
• Gas outflows from the z= 7.54 quasar : predictions from the BlueTides Simulation
• Observability of intermittent radio sources in galaxy groups and clusters
• Mixing matters
• The extended epoch of galaxy formation: age dating of ~3600 galaxies with 2<z<6.5 in the VIMOS Ultra-Deep Survey
• On the formation of massive quiescent galaxies with diverse morphologies in the TNG50 simulation
• What drives galaxy quenching? A deep connection between galaxy kinematics and quenching in the local Universe
• DM halo morphological types of MW-like galaxies in the TNG50 simulation: Simple, Twisted, or Stretched
• Black hole clustering and duty cycles in the Illustris simulation
• Discriminating Topology in Galaxy Distributions using Network Analysis
• Gas flows in the circumgalactic medium around simulated high-redshift galaxies
• The evolution of the UV-to-mm extragalactic background light: evidence for a top-heavy initial mass function?
• Barred galaxies in cosmological zoom-in simulations: the importance of feedback
• How gas flows shape the stellar-halo mass relation in the EAGLE simulation
• The Stripe 82 1-2 GHz Very Large Array Snapshot Survey: host galaxy properties and accretion rates of radio galaxies
• The Illustris Simulation: Supermassive Black Hole - Galaxy Connection Beyond the Bulge
• Tracing the anemic stellar halo of M101
• Towards a consistent framework of comparing galaxy mergers in observations and simulations
• The Local Group: The Ultimate Deep Field
• Global Simulations of Galactic Discs: Violent Feedback from Clustered Supernovae during Bursts of Star Formation
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• Evolution of star formation rate-density relation over cosmic time in a simulated universe: the observed reversal reproduced
• Gas Accretion Can Drive Turbulence in Galaxies
• Effects of galaxy--satellite interactions on bar formation
• Stellar halos from The Dragonfly Edge-on Galaxies Survey
• The response of dark matter haloes to elliptical galaxy formation: a new test for quenching scenarios
• VINTERGATAN IV: Cosmic phases of star formation in Milky Way-like galaxies
• The evolution of barred galaxies in the EAGLE simulations
• The dispersion measure of Fast Radio Bursts host galaxies: estimation from cosmological simulations
• The impact of Lyman-$\alpha$ radiative transfer on large-scale clustering in the Illustris simulation
• Stellar ages and masses in the solar neighbourhood: Bayesian analysis using spectroscopy and Gaia DR1 parallaxes
• The Active Assembly of the Virgo Cluster: Indications for Recent Group Infall From Early-Type Dwarf Galaxies
• RHAPSODY-G simulations II - Baryonic growth and metal enrichment in massive galaxy clusters
• Bar resilience to flybys in a cosmological framework
• NIHAO III: The constant disc gas mass conspiracy
• The Physical Origin of Galactic Conformity: From Theory to Observation
• Size distribution of galaxies in SDSS DR7: weak dependence on halo environment
• The impact of baryonic physics on the abundance, clustering, and concentration of halos
• The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies
• Constraining the halo mass function with observations
• Cosmological insights into the assembly of the radial and compact stellar halo of the Milky Way
• The impact of ionised outflows from z$\sim$2.5 quasars is not through instantaneous in-situ quenching: the evidence from ALMA and VLT/SINFONI
• SDSS-IV MaNGA: Internal mass distributions and orbital structures of early-type galaxies and their dependence on environment
• Can Assembly Bias Explain the Lensing Amplitude of the BOSS CMASS Sample in a Planck Cosmology?
• The host galaxies of z=7 quasars: predictions from the BlueTides simulation
• History and destiny of an emerging early-type galaxy: New IFU insights on the major-merger remnant NGC7252
• The SZ flux-mass ($Y$-$M$) relation at low halo masses: improvements with symbolic regression and strong constraints on baryonic feedback
• Galaxy And Mass Assembly (GAMA): Bulge-disk decomposition of KiDS data in the nearby universe
• Dark Matter Bars in Spinning Halos
• Galactic conformity measured in semi-analytic models
• Wide-Field Optical Spectroscopy of Abell 133: A Search for Filaments Reported in X-ray Observations
• From EMBER to FIRE: predicting high resolution baryon fields from dark matter simulations with Deep Learning
• On the environmental influence of groups and clusters of galaxies beyond the virial radius: Galactic conformity at few Mpc scales
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• Testing the presence of multiple photometric components in nearby early-type galaxies using SDSS
• The galaxy size to halo spin relation of disk galaxies in cosmological hydrodynamical simulations
• Fast Generation of Covariance Matrices for Weak Lensing
• Effects of Active Galactic Nucleus Feedback on Cold Gas Depletion and Quenching of Central Galaxies
• Galaxy clusters in local Universe simulations without density constraints: a long uphill struggle
• Star-formation driven outflows in local dwarf galaxies as revealed from [CII] observations by Herschel
• A tight relation between the age distributions of stellar clusters and the properties of the interstellar medium in the host galaxy
• SHARP -- VI. Evidence for CO (1-0) molecular gas extended on kpc-scales in AGN star forming galaxies at high redshift
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Generative deep fields: arbitrarily sized, random synthetic astronomical images through deep learning
• Modelling the M*-SFR relation at high redshift: untangling factors driving biases in the intrinsic scatter measurement
• Towards an improved model of self-interacting dark matter haloes
• The Galaxy-Halo Connection for $1.5\lesssim z\lesssim 5$ as revealed by the \emph{Spitzer} Matching survey of the UltraVISTA ultra-deep Stripes
• The role of AGN feedback on the evolution of dwarf galaxies from cosmological simulations: SMBHs suppress star formation in low-mass galaxies
• Reducing biases on $H_0$ measurements using strong lensing and galaxy dynamics: results from the EAGLE simulation
• The Interplay of Kinetic and Radiative Feedback in Galaxy Clusters
• Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor
• DEVILS: Cosmic evolution of SED-derived metallicities and their connection to star-formation histories
• EAGLE-Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
• Biases and systematics in the observational derivation of galaxy properties: comparing different techniques on synthetic observations of simulated galaxies
• The nature of damped HI absorbers probed by cosmological simulations: satellite accretion and outflows
• Simba: The average properties of the circumgalactic medium of $2\le z\le 3$ quasars are determined primarily by stellar feedback
• Molecular Gas Reservoirs in Massive Quiescent Galaxies at $\mathrm{z}\sim 0.7$ Linked to Late Time Star Formation
• GARROTXA Cosmological Simulations of Milky Way-sized Galaxies: General Properties, Hot Gas Distribution, and Missing Baryons
• Stellar Mass Growth of Brightest Cluster Galaxy Progenitors in COSMOS Since z ~ 3
• Explaining the scatter in the galaxy mass-metallicity relation with gas flows
• The Impact of baryonic physics on the kinetic Sunyaev-Zel'dovich Effect
• Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
• Empirically-motivated early feedback: momentum input by stellar feedback in galaxy simulations inferred through observations
• Numerical modelling of the lobes of radio galaxies in cluster environments -- IV. Remnant radio galaxies
• Machine Learning methods to estimate observational properties of galaxy clusters in large volume cosmological N-body simulations
• Angular Momentum of Early and Late Type Galaxies: Nature or Nurture?
• Renormalization-group flow of the effective action of cosmological large-scale structures
• Stacked star formation rate profiles of bursty galaxies exhibit 'coherent' star formation
• The stellar populations of high-redshift dwarf galaxies
• Consequences of the lack of azimuthal freedom in the modeling of lensing galaxies
• The ultra-diffuse dwarf galaxies NGC 1052-DF2 and 1052-DF4 are in conflict with standard cosmology
• Non-thermal radio supernova remnants of exiled Wolf-Rayet stars
• The evolution of galaxy intrinsic alignments in the MassiveBlack II universe
• x-cut Cosmic Shear: Optimally Removing Sensitivity to Baryonic and Nonlinear Physics with an Application to the Dark Energy Survey Year 1 Shear Data
• Tidal disruption events from massive black hole binaries: predictions for ongoing and future surveys
• Galaxy Zoo: Morphological classification of galaxy images from the Illustris simulation
• Testing the Relationship Between Bursty Star Formation and Size Fluctuations of Local Dwarf Galaxies
• SHAM through the lens of a hydrodynamical simulation
• Nonparametric galaxy morphology from UV to submm wavelengths
• A Fundamental Test for Galaxy Formation Models: Matching the Lyman-$\alpha$ Absorption Profiles of Galactic Halos over Three Decades in Distance
• The fundamental metallicity relation emerges from the local anti-correlation between star formation rate and gas-phase metallicity existing in disk galaxies
• The impact of inelastic self-interacting dark matter on the dark matter structure of a Milky Way halo
• On the redshift evolution of the baryon and gas fraction in simulated groups and clusters of galaxies
• Dark-matter-deficient galaxies in hydrodynamical simulations
• Merging galaxies produce outliers from the Fundamental Metallicity Relation
• KURVS: The outer rotation curve shapes and dark matter fractions of $z\sim 1.5$ star-forming galaxies
• The galaxy-halo size relation of low-mass galaxies in FIRE
• The effect of stellar and AGN feedback on the low redshift Lyman-$\alpha$ forest in the Sherwood simulation suite
• Are fossil groups early-forming galaxy systems?
• The DESI PRObabilistic Value-Added Bright Galaxy Survey (PROVABGS) Mock Challenge
• Stellar populations across the black hole mass - velocity dispersion relation
• An FMOS Survey of moderate-luminosity broad-line AGN in COSMOS, SXDS and E-CDF-S
• The Three Hundred project: galaxy cluster mergers and their impact on the stellar component of brightest cluster galaxies
• The Clustering Evolution of Dusty Star-Forming Galaxies
• The bivariate gas-stellar mass distributions and the mass functions of early- and late-type galaxies at $z\sim 0$
• Accurate initial conditions in mixed Dark Matter--Baryon simulations
• Real- and redshift-space halo clustering in $f(R)$ cosmologies
• An improved probabilistic approach for linking progenitor and descendant galaxy populations using comoving number density
• Redshift evolution of stellar mass versus gas fraction relation in 0<z<2 regime: observational constraint for galaxy formation models
• Hot and counter-rotating star-forming disk galaxies in IllustrisTNG and their real-world counterparts
• Gas-phase metallicity break radii of star-forming galaxies in IllustrisTNG
• A numerical twist on the observational spin parameter, ${\lambda }_R$
• Impact of gas spin and Lyman-Werner flux on black hole seed formation in cosmological simulations: implications for direct collapse
• The stellar mass - size relation for cluster galaxies at z=1 with high angular resolution from the Gemini/GeMS multi-conjugate adaptive optics system
• Star formation quenching imprinted on the internal structure of naked red nuggets
• Black hole -- galaxy scaling relations in FIRE: the importance of black hole location and mergers
• Do AGN triggering mechanisms vary with radio power? I.Optical morphologies of radio-intermediate HERGs
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. I. Construction and analysis of the mock data cubes
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• Conditional HI mass functions and the HI-to-halo mass relation in the local Universe
• The FLAMINGO project: Baryon effects on the matter power spectrum
• The warm-hot circumgalactic medium around EAGLE-simulation galaxies and its detection prospects with X-ray line emission
• Aging Halos: Implications of the Magnitude Gap on Conditional Statistics of Stellar and Gas Properties of Massive Halos
• Cosmic Reionization On Computers: Numerical and Physical Convergence
• Predicting sub-millimeter flux densities from global galaxy properties
• Systematic errors in strong gravitational lensing reconstructions, a numerical simulation perspective
• REQUIEM-2D: Spatially Resolved Stellar Populations from HST 2D Grism Spectroscopy
• Predictions for the Abundance of High-redshift Galaxies in a Fuzzy Dark Matter Universe
• The THESAN project: connecting ionized bubble sizes to their local environments during the Epoch of Reionization
• Dark Matter Superfluidity
• Constraints on Cosmology and Baryonic Feedback with the Deep Lens Survey Using Galaxy-Galaxy and Galaxy-Mass Power Spectra
• The SAMI galaxy survey: Galaxy Interactions and Kinematic Anomalies in Abell 119
• The Velocity Dispersion Function for Quiescent Galaxies in the Local Universe
• Redshift evolution of the dark matter haloes shapes
• The formation of supermassive black holes from Population III.1 seeds. II. Evolution to the local universe
• Infrared luminosity functions and dust mass functions in the EAGLE simulation
• The Supersonic Project: rotational effects of supersonic motions on the first structures in the Universe
• Considerations for the Observability of Kinematically Offset Binary AGN
• Zoomed cosmological simulations of Milky Way sized halos in f(R)-gravity
• Simulation techniques for modified gravity
• The metal enrichment of passive galaxies in cosmological simulations of galaxy formation
• TARDIS Paper II: Synergistic Density Reconstruction from Lyman-alpha Forest and Spectroscopic Galaxy Surveys with Applications to Protoclusters and the Cosmic Web
• Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
• LIMFAST. I. A Semi-Numerical Tool for Line Intensity Mapping
• nIFTy galaxy cluster simulations V: Investigation of the Cluster Infall Region
• Stellar and Weak Lensing Profiles of Massive Galaxies in the Hyper-Suprime Cam Survey and in Hydrodynamic Simulations
• Exploring the Dust Content of Galactic Winds With Herschel. II. Nearby Dwarf Galaxies
• Testing Galaxy Quenching Theories with Scatter in the Stellar to Halo Mass Relation
• Astrophysical Tests of Dark Matter Self-Interactions
• Prospects for Recovering Galaxy Intrinsic Shapes from Projected Quantities
• What Are Those Tiny Things? A First Study of Compact Star Clusters in the SMACS0723 Field with JWST
• Impact of Baryonic Physics on Intrinsic Alignments
• Spherical Cows in Dark Matter Indirect Detection
• Encoding large scale cosmological structure with Generative Adversarial Networks
• Redshift Evolution of the Fundamental Plane Relation in the IllustrisTNG Simulation
• Reconciling galaxy cluster shapes, measured by theorists vs observers
• The Dependence of Halo Mass on Galaxy Size at Fixed Stellar Mass Using Weak Lensing
• Observing the host galaxies of high-redshift quasars with JWST: predictions from the BlueTides simulation
• The SATIN project I: Turbulent multi-phase ISM in Milky Way simulations with SNe feedback from stellar clusters
• Constraining the cross-section of dark matter with giant radial arcs in galaxy clusters
• Intermittent AGN episodes drive outflows with a large spread of observable loading factors
• Cosmological Vlasov-Poisson equations for dark matter: Recent developments and connections to selected plasma problems
• The SAMI Galaxy Survey: Environmental analysis of the orbital structures of passive galaxies
• The interconnection between galaxy mergers, AGN activity and rapid quenching of star formation in simulated post-merger galaxies
• REQUIEM-2D: A diversity of formation pathways in a sample of spatially-resolved massive quiescent galaxies at z~2
• Impact of baryons in cosmic shear analyses with tomographic aperture mass statistics
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• A high baryon fraction in massive haloes at z~3
• The assembly of spheroid-dominated galaxies in the EAGLE simulation
• Bayesian cosmic density field inference from redshift space dark matter maps
• The clustering of $z>7$ galaxies: Predictions from the BLUETIDES simulation
• SPRAI: Coupling of radiative feedback and primordial chemistry in moving mesh hydrodynamics
• The Effect of Galactic Feedback on Gas Accretion and Wind Recycling
• On the connection between the metal-enriched intergalactic medium and galaxies: an OVI-galaxy cross-correlation study at $z<1$
• The Carnegie-Irvine Galaxy Survey. IV. A Method to Determine the Average Mass Ratio of Mergers That Built Massive Elliptical Galaxies
• Evolution of the luminosity-to-halo mass relation of LRGs from a combined SDSS-DR10+RCS2 analysis
• Galaxy properties in the cosmic web of EAGLE simulation
• Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• Evidence of extended cold molecular gas and dust halos around $\mathbf{z}\sim 2.3$ Extremely Red Quasars with ALMA
• Dynamical evolution of massive black holes in galactic-scale N-body simulations - introducing the regularized tree code "rVINE"
• The large-scale environment from cosmological simulations II: The redshift evolution and distributions of baryons
• Mapping Accreted Stars in Early-Type Galaxies Across the Mass-Size Plane
• Importance of Mock Observations in Validating Galaxy Properties for Cosmological Simulations
• Star-Gas Misalignment in Galaxies: II. Origins Found from the Horizon-AGN Simulation
• WISDOM project -- VI. Exploring the relation between supermassive black hole mass and galaxy rotation with molecular gas
• Star-gas misalignment in galaxies: I. The properties of galaxies from the Horizon-AGN simulation and comparisons to SAMI
• The assembly bias of emission line galaxies
• SEAGLE--II: Constraints on feedback models in galaxy formation from massive early type strong lens galaxies
• Voyage through the Hidden Physics of the Cosmic Web
• Estimating the Milky Way's Mass via Hierarchical Bayes: A Blind Test on MUGS2 Simulated Galaxies
• The effect of dark matter-dark radiation interactions on halo abundance -- a Press-Schechter approach
• AGN-driven quenching of satellite galaxies
• An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
• Detecting Galaxy Groups and AGNs populating the local Universe in the eROSITA era
• The galaxy correlation function as a constraint on galaxy formation physics
• Gas around galaxy haloes - II: hydrogen absorption signatures from the environments of galaxies at redshifts 2 < z < 3
• The Impact of Outflows driven by Active Galactic Nuclei on Metals in and around Galaxies
• Multi-wavelength mock galaxy catalogs of the low-redshift Universe
• Exploring Relations Between BCG \& Cluster Properties in the SPectroscopic IDentification of eROSITA Sources Survey from $0.05<z<0.3$
• Cosmology from Clustering, Cosmic Shear, CMB Lensing, and Cross Correlations: Combining Rubin Observatory and Simons Observatory
• Characterising Tidal Features Around Galaxies in Cosmological Simulations
• On the origin of star formation quenching in massive galaxies at $z\gtrsim 3$ in the cosmological simulations IllustrisTNG
• Exploring the Cosmic Evolution of Habitability with Galaxy Merger Trees
• Tidally induced morphology of M33 in hydrodynamical simulations of its recent interaction with M31
• The Effect of Environment on Milky Way-mass galaxies in a Constrained Simulation of the Local Group
• Resolved Star Formation Efficiency in the Antennae Galaxies
• A tiny host galaxy for the first giant black hole: $z=7.5$ quasar in BlueTides
• Does jackknife scale really matter for accurate large-scale structure covariances?
• Evolution of dwarf galaxies hosting GW150914-like events
• Cosmological simulations of quasar fueling to sub-parsec scales using Lagrangian hyper-refinement
• H2 chemistry in galaxy simulations: an improved supernova feedback model
• Unraveling the interplay between SIDM and baryons in MW halos: defining where baryons dictate heat transfer
• The SELGIFS data challenge: generating synthetic observations of CALIFA galaxies from hydrodynamical simulations
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• The low redshift Lyman-$\alpha$ Forest as a constraint for models of AGN feedback
• Resonant scattering of the OVII X-ray emission line in the circumgalactic medium of TNG50 galaxies
• The early growth of supermassive black holes in cosmological hydrodynamic simulations with constrained Gaussian realizations
• Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
• The buildup of galaxies and their spheroids: the contributions of mergers, disc instabilities and star formation
• MultiDark-Clusters: Galaxy Cluster Mock Light-Cones, eROSITA and the Cluster Power Spectrum
• Physical properties of galaxies: toward a consistent comparison between hydrodynamical simulations and SDSS
• Simulating the Carbon Footprint of Galactic Halos
• ETHOS - an effective theory of structure formation: formation of the first haloes and their stars
• The Three Hundred project: connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
• The IllustrisTNG Simulations: Public Data Release
• Morphological evolution of supermassive black hole merger hosts and multimessenger signatures
• Groups and protocluster candidates in the CLAUDS and HSC-SSP joint deep surveys
• Effects of feedback on galaxies in the VELA simulations: elongation, clumps and compaction
• A Framework for Empirical Galaxy Phenomenology: The Scatter in Galaxy Ages and Stellar Metallicities
• A Moving Mesh Hydrodynamic Solver for ChaNGa
• Do galaxies die? Different views from simulations and observations in the Local Universe
• The diversity of assembly histories leading to disc galaxy formation in a LambdaCDM model
• ALMA [N ıı] 205 μm Imaging Spectroscopy of the Lensed Submillimeter galaxy ID 141 at redshift 4.24
• The Case for Strangulation in Low-Mass Hosts: DDO 113
• Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
• On Mass Concentrations & Magnitude Gaps of Galaxy Systems in the CS82 Survey
• LLAMA: Stellar populations in the nuclei of ultra hard X-ray selected AGN and matched inactive galaxies
• The cosmic spectral energy distribution in the EAGLE simulation
• The evolution of the baryon fraction in halos as a cause of scatter in the galaxy stellar mass in the EAGLE simulation
• Through a Smoother Lens: An expected absence of LCDM substructure detections from hydrodynamic and dark matter only simulations
• The morphology and kinematics of neutral hydrogen in the vicinity of z=0 galaxies with Milky Way masses -- a study with the Illustris simulation
• Probing cosmic isotropy in the Local Universe
• Local Group star formation in warm and self-interacting dark matter cosmologies
• Non-isotropic feedback from accreting spinning black holes
• The intrinsic SFRF and sSFRF of galaxies: comparing SDSS observation with IllustrisTNG simulation
• Modeling globular clusters in the TNG50 simulation: predictions from dwarfs to giants
• Formation and assembly history of stellar components in galaxies as a function of stellar and halo mass
• Real and counterfeit cores: how feedback expands halos and disrupts tracers of inner gravitational potential in dwarf galaxies
• Group-scale intrinsic galaxy alignments in the Illustris-TNG and MassiveBlack-II simulations
• A Mixture of LBG Overdensities in the Fields of Three $6<z<7$ Quasars: Implications for the Robustness of Photometric Selection
• Mufasa:The strength and evolution of galaxy conformity in various tracers
• The building up of observed stellar scaling relations of massive galaxies and the connection to black hole growth in the TNG50 simulation
• DS+: a method for the identification of cluster substructures
• Dark-ages Reionization and Galaxy Formation Simulation - XIII. AGN quenching of high-redshift star formation in ZF-COSMOS-20115
• Generating mock galaxy catalogues for flux-limited samples like the DESI Bright Galaxy Survey
• Detecting the Figure Rotation of Dark Matter Halos with Tidal Streams
• How to Detect an Astrophysical Nanohertz Gravitational-Wave Background
• The intermediate-ionization lines as virial broadening estimators for Population A quasars
• Biases and Cosmic Variance in Molecular Gas Abundance Measurements
• There and back again: understanding the critical properties of backsplash galaxies
• Out of sight, out of mind? The impact of correlated clustering in substructure lensing
• The Impacts of Modeling Choices on the Inference of the Circumgalactic Medium Properties from Sunyaev-Zeldovich Observations
• The Obsidian model: Three regimes of black hole feedback
• Galaxies with Shells in the Illustris Simulation: Metallicity Signatures
• Strongly Time-Variable Ultra-Violet Metal Line Emission from the Circum-Galactic Medium of High-Redshift Galaxies
• Push it to the limit: Local Group constraints on high-redshift stellar mass functions for Mstar > 10^5 Msun
• Dark-ages Reionization & Galaxy Formation Simulation VIII. Suppressed growth of dark matter halos during the Epoch of Reionization
• Probing the CGM of Low-redshift Dwarf Galaxies Using FIRE Simulations
• The Borg Cube Simulation: Cosmological Hydrodynamics with CRK-SPH
• An accurate analytic mass model for lensing galaxies
• Galaxy merger challenge: A comparison study between machine learning-based detection methods
• Determining AGN luminosity histories using present-day outflow properties: a neural-network based approach
• Supermassive black hole fueling in IllustrisTNG: Impact of environment
• The cosmic web around the Coma cluster from constrained cosmological simulations: I. Filaments connected to Coma at $z=0$
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• Predicting fully self-consistent satellite richness, galaxy growth and starformation rates from the STastical sEmi-Empirical modeL STEEL
• The Smith Cloud: surviving a high speed transit of the Galactic disc
• Colour gradients of low-redshift galaxies in the DESI Legacy Imaging Survey
• The MUSE Hubble Ultra Deep Field Survey XVI. The angular momentum of low-mass star-forming galaxies. A cautionary tale and insights from TNG50
• Galactic coronae in Milky Way-like galaxies: the role of stellar feedback in gas accretion
• Interactive 3D Visualization for Theoretical Virtual Observatories
• PopSED: Population-Level Inference for Galaxy Properties from Broadband Photometry with Neural Density Estimation
• Effective Dark Matter Halo catalog in $f(R)$ gravity
• A discrete chemo-dynamical model of M87's globular clusters: Kinematics extending to ~ 400 kpc
• Galaxy-lens determination of $H_0$: the effect of the ellipse+shear modeling assumption
• Small scale structures in coupled scalar field dark matter
• Inferring the Morphology of Stellar Distribution in TNG50: Twisted and Twisted-Stretched shapes
• Hybrid analytic and machine-learned baryonic property insertion into galactic dark matter haloes
• The impact of black hole seeding in cosmological simulations
• Towards precise galaxy evolution: a comparison between spectral indices of $z\sim 1$ galaxies in the IllustrisTNG simulation and the LEGA-C survey
• Impact of gas based seeding on supermassive black hole populations at $z\ge 7$
• Time Dependent Radiation Hydrodynamics on a Moving Mesh
• Calibration of a star formation and feedback model for cosmological simulations with Enzo
• Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation
• The LEGA-C of nature and nurture in stellar populations of galaxies at z~0.6-1.0: D4000 and H-delta reveal different assembly histories for quiescent galaxies in different environments
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Evolution of the ${\sigma }_{\mathrm{SFR}}$-M${}_{\star }$ relation and implications for self-regulated star formation
• Shedding light on low-mass subhalo survival and annihilation luminosity with numerical simulations
• SUPER VII. Morphology and kinematics of H$\alpha$ emission in AGN host galaxies at Cosmic noon using SINFONI
• The Robustness of Cosmological Hydrodynamic Simulation Predictions to Changes in Numerics and Cooling Physics
• Fossil group origins IX. Probing the formation of fossil galaxy groups with stellar population gradients of their central galaxies
• Exploring the High-Mass End of the Stellar Mass Function of Star Forming Galaxies at Cosmic Noon
• Close Encounters of Tight Binary Stars with Stellar-mass Black Holes
• Low-Surface-Brightness Galaxies are missing in the observed Stellar Mass Function
• Two channels for the formation of compact dwarf galaxies in clusters of galaxies
• We are not the 99 percent: quantifying asphericity in the distribution of Local Group satellites
• Late Bloomer Galaxies: Growing Up in Cosmic Autumn
• Cosmic Ray Driven Outflows in an Ultraluminous Galaxy
• Modelling the star-formation activity and ionizing properties of high-redshift galaxies
• Star formation in mergers with cosmologically motivated initial conditions
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines I. The [C II] 158 microns line at z~0
• The Duration of Star Formation in Galactic Giant Molecular Clouds. I. The Great Nebula in Carina
• Local Group Dwarf Galaxy Detection Limit in the CSST survey
• The whole picture of the large-scale structure of the CL1604 supercluster at z$\sim$0.9
• Discrepancies Between JWST Observations and Simulations of Quenched Massive Galaxies at $z>3$: A Comparative Study With IllustrisTNG and ASTRID
• The Manhattan Suite: Accelerated galaxy evolution in the early Universe
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• The impact of galaxy selection on the splashback boundaries of galaxy clusters
• How feedback shapes galaxies: an analytic model
• A Precise Benchmark for Cluster Scaling Relations: Fundamental Plane, Mass Plane and IMF in the Coma Cluster from Dynamical Models
• On the kinetic Sunyaev-Zel'dovich effect as an observational probe for halo spin bias
• HOD modelling of high redshift galaxies using the BLUETIDES simulation
• Euclid preparation. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary Fields
• Stellar-mass black-hole binaries in LISA: characteristics and complementarity with current-generation interferometers
• A 1-dimensional hydrodynamic model for accretion, cooling and heating of gas in dark matter halos from $z=6$ to $z=0$
• Accuracy and precision of triaxial orbit models I: SMBH mass, stellar mass and dark-matter halo
• Simplified galaxy formation with mesh-less hydrodynamics
• Lopsided Galaxies in a cosmological context: a new galaxy-halo connection
• The tidal evolution of the Fornax dwarf spheroidal and its globular clusters
• Galactic Habitability Re-Examined: Indications of Bimodality
• The Effects of Metallicity and Abundance Pattern of the ISM on Supernova Feedback
• The Luminosity Functions and Redshift Evolution of Satellites of Low-Mass Galaxies in the COSMOS Survey
• AGN must be very efficient at powering outflows
• Galaxy Structural Analysis with the Curvature of the Brightness Profile
• The metallicity and star formation activity of long gamma-ray burst hosts for z$<$3: insights from the Illustris simulation
• Properties and observables of massive galaxies in self-interacting dark matter cosmologies
• Analysis of the galaxy size versus stellar mass relation
• The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
• The effect of dark matter resolution on the collapse of baryons in high redshift numerical simulations
• ERGO-ML: Towards a robust machine learning model for inferring the fraction of accreted stars in galaxies from integral-field spectroscopic maps
• X-ray morphology of cluster-mass haloes in self-interacting dark matter
• The impact of mass map truncation on strong lensing simulations
• ERGO-ML: Comparing IllustrisTNG and HSC galaxy images via contrastive learning
• Simulations of black hole fueling in isolated and merging galaxies with an explicit, multiphase ISM
• The fate of the interstellar medium in early-type galaxies. III. The mechanism of ISM removal and quenching of star formation
• Revealing a Highly-Dynamic Cluster Core in Abell 1664 with Chandra
• The Sejong Suite: Cosmological Hydrodynamical Simulations with Massive Neutrinos, Dark Radiation, and Warm Dark Matter
• The Califa and Hipass velocity function for all morphological galaxy types
• Impact of cosmic filaments on the gas accretion rate of dark matter halos
• Evaluating hydrodynamical simulations with green valley galaxies
• Non-parametric Morphologies of Mergers in the Illustris Simulation
• A Halo Occupation Interpretation Of Quasars At $z\sim 1.5$ Using Very Small Scale Clustering Information
• Constraints on small-scale cosmological fluctuations from SNe lensing dispersion
• Cosmic evolution of black hole-spin and galaxy orientations: clues from the NewHorizon and Galactica simulations
• Halo mass and weak galaxy-galaxy lensing profiles in rescaled cosmological $N$-body simulations
• The large-scale structure around the Fornax-Eridanus Complex
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs -- II. The catalogue
• Galaxy properties from J-PAS narrow-band photometry
• Identifying the progenitors of present-day early-type galaxies in observational surveys: correcting `progenitor bias' using the Horizon-AGN simulation
• Morphology and surface photometry of a sample of isolated early-type galaxies from deep imaging
• Stellar Feedback and the Energy Budget of Late-Type Galaxies: Missing Baryons and Core Creation
• Unveiling the main sequence of galaxies at $z\ge 5$ with the James Webb Space Telescope: predictions from simulations
• The THESAN-ZOOM project: Population III star formation continues until the end of reionization
• Little Red Dots as Direct-collapse Black Hole Nurseries
• Simulating Hydrodynamics in Cosmology with CRK-HACC
• Detection of Prominent Stellar Disks in the Progenitors of Present-day Massive Elliptical Galaxies
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• The Coevolution of Massive Quiescent Galaxies and Their Dark Matter Halos over the Last 6 Billion Years
• Planting a Lyman alpha forest on AbacusSummit
• General Relativistic Hydrodynamics on a Moving-mesh I: Static Spacetimes
• Gas Accretion and Star Formation Rates
• Toward Solving the Puzzle: Dissecting the Complex Merger A521 with Multi-wavelength Data
• Searching for the shadows of giants: characterising protoclusters with line of sight Lyman-α absorption
• MIND THE GAP: Is The Too Big To Fail Problem Resolved?
• Impact of H${}_2$-driven star formation and stellar feedback from low-enrichment environments on the formation of spiral galaxies
• The impact of magnetic fields on cosmological galaxy mergers -- II. Modified angular momentum transport and feedback
• Prospects for Detecting Signs of Life on Exoplanets in the JWST Era
• Do you see what I see? Exploring the consequences of luminosity limits in black hole-galaxy evolution studies
• Galaxies and Halos on Graph Neural Networks: Deep Generative Modeling Scalar and Vector Quantities for Intrinsic Alignment
• RAiSE X: searching for radio galaxies in X-ray surveys
• Boltzmann hierarchies for self-interacting warm dark matter scenarios
• Recent progress in simulating galaxy formation from the largest to the smallest scales
• The Fornax Cluster VLT Spectroscopic Survey IV -- Cold kinematical substructures in the Fornax core from COSTA
• nIFTy Galaxy Cluster simulations VI: The dynamical imprint of substructure on gaseous cluster outskirts
• Testing the fidelity of simulations of black hole - galaxy co-evolution at z ~ 1.5 with observations
• Compact Galaxies at Intermediate Redshifts Quench Faster than Normal-sized Galaxies
• Saying Hallo to M94's Stellar Halo: Investigating the Accretion History of the Largest Pseudobulge Host in the Local Universe
• Resolution of the apparent discrepancy between the number of massive subhaloes in Abell 2744 and ΛCDM
• A Cosmological Solution to the Impossibly Early Galaxy Problem
• Exploring the Fate of Stellar Core Collapse with Supernova Relic Neutrinos
• Active Galactic Nucleus Feedback in an Elliptical Galaxy with the Most Updated AGN Physics: Parameter Explorations
• How do galaxy properties affect void statistics?
• IllustrisTNG Insights: Factors Affecting the Presence of Bars in Disk Galaxies
• Confronting semi-analytic galaxy models with galaxy-matter correlations observed by CFHTLenS
• Galaxies with kinematically distinct cores in Illustris
• Inconsistencies arising from the coupling of galaxy formation sub-grid models to Pressure-Smoothed Particle Hydrodynamics
• Sloshing of Galaxy Cluster Core Plasma in the Presence of Self-Interacting Dark Matter
• Evolution of Starburst Galaxies in the Illustris Simulation
• The Column Densities of Molecular Gas across Cosmic Time: Bridging Observations and Simulations
• Satellite Alignment: III. Satellite Galaxies Spatial Distribution and their Dependence on Redshift with A Novel Galaxy Finder
• A novel approach to cosmological non-linearities as an effective fluid
• Gas Accretion and Angular Momentum
• Uncovering Mass Segregation with Galaxy Analogues in Dark Matter Simulations
• Extreme Spheres: Counts-in-cells for 21cm intensity mapping
• A Semi-Analytical Line Transfer (SALT) Model III: Galactic Inflows
• Translators of galaxy morphology indicators between observation and simulation
• Galaxy formation physics behind bar formation: A view from cosmological hydrodynamical simulations
• New dwarf galaxy candidates in the sphere of influence of the Local Volume spiral galaxy NGC2683
• Photoevaporation of Molecular Clouds in Regions of Massive Star Formation as Revealed Through H${}_2$ and Br$\gamma$ Emission
• Clustering of MgII absorption line systems around massive galaxies: an important constraint on feedback processes in galaxy formation
• Mock Observations: Formation and Evolution of diffuse light in Galaxy Groups and Clusters in the IllustrisTNG Simulations
• Anisotropic satellite accretion onto the Local Group with HESTIA
• Angular momentum evolution of bulge stars in disc galaxies in NIHAO
• How dark are filaments in the cosmic web?
• Tracing Dark Matter Halos with Satellite Kinematics and the Central Stellar Velocity Dispersion of Galaxies
• Bringing faint active galactic nuclei (AGNs) to light: a view from large-scale cosmological simulations
• Life after AGN switchoff: evolution and properties of fossil galactic outflows
• Constraining the Fluctuating Gunn-Peterson Approximation Using Lyman-$\alpha$ Forest Tomography at $z=2$
• BUDHIES V: The baryonic Tully-Fisher relation at z=0.2 based on direct HI detections
• Exploring the thermal energy contents of the intergalactic medium with the Sunyaev-Zel'dovich effect
• High-fidelity reproduction of central galaxy joint distributions with Neural Networks
• Imprint of baryons and massive neutrinos on velocity statistics
• MARTINI: Mock Array Radio Telescope Interferometry of the Neutral ISM
• Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies
• Galaxy growth from redshift 5 to 0 at fixed comoving number density
• The ALPINE-ALMA [CII] Survey: CGM pollution and gas mixing by tidal stripping in a merging system at z~4.57
• Orbital and Radiative Properties of Wandering Intermediate-Mass Black Holes in the ASTRID Simulation
• Impact of uncertainties in the halo velocity profile on direct detection of sub-GeV dark matter
• The Tessellation-Level-Tree: characterising the nested hierarchy of density peaks and their spatial distribution in cosmological N-body simulations
• Testing the Breathing Mode in Intermediate Mass Galaxies and its Predicted Star Formation Rate-Size Anti-Correlation
• Cosmological applications of the Brown-York quasilocal mass
• Tilted outer and inner structures in edge-on galaxies?
• New dwarf galaxy candidates in the sphere of influence of the Sombrero galaxy
• Testing the Impact of Satellite Anisotropy on Large and Small Scale Intrinsic Alignments using Hydrodynamical Simulations
• LyMAS reloaded: improving the predictions of the large-scale Lyman-α forest statistics from dark matter density and velocity fields
• From Galactic Chemical Evolution to Cosmic Supernova Rates Synchronized with Core-Collapse Supernovae Limited to the Narrow Progenitor Mass Range
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• The Large-scale Effect of Environment on Galactic Conformity
• Jeans that fit: weighing the mass of the Milky Way analogues in the $\Lambda \mathrm{CDM}$ universe
• The BlueTides Mock Image Catalogue: Simulated observations of high-redshift galaxies and predictions for JWST imaging surveys
• Observational constraints in Delta Gravity: CMB and supernovas
• Orbital pericenters and the inferred dark matter halo structure of satellite galaxies
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Constraining the Galaxy-Halo Connection with Optimal Statistics
• Discovery of large scale shock fronts correlated with the radio halo and radio relic in the A2163 galaxy cluster
• Modeling Nearly Spherical Pure-Bulge Galaxies with a Stellar Mass-to-Light Ratio Gradient under the $\Lambda$CDM and MOND Paradigms: II. The Orbital Anisotropy of Slow Rotators within the Effective Radius
• The Star Formation and AGN luminosity relation: Predictions from a semi-analytical model
• A comparison of the R_h=ct and LCDM cosmologies based on the observed halo mass function
• A robust determination of halo environment in the cosmic field
• Reconciling Mass Functions with the Star-Forming Main Sequence Via Mergers
• The signal of decaying dark matter with hydrodynamical simulations
• A study of the HI gas fractions of galaxies at z ~ 1
• Connecting the Dots: Tracking Galaxy Evolution Using Constant Cumulative Number Density at 3<z<7
• Populating The Milky Way: Characterising Planet Demographics by Combining Galaxy Formation Simulations and Planet Population Synthesis Models
• Acausality in Superfluid Dark Matter and MOND-like Theories
• Colour-magnitude diagram in simulations of galaxy formation
• AGN and Star Formation at Cosmic Noon: Comparison of Data to Theoretical Models
• An HSC view of the CMASS galaxy sample. Halo mass as a function of stellar mass, size and Sérsic index
• Cosmological interpretation of the color-magnitude diagrams of galaxy clusters
• Impact of baryonic feedback on HSC Y1 weak lensing non-Gaussian statistics
• BASILISK: Bayesian Hierarchical Inference of the Galaxy-Halo Connection using Satellite Kinematics--I. Method and Validation
• Resolution Convergence in Cosmological Hydrodynamical Simulations Using Adaptive Mesh Refinement
• The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship
• Mesh-free hydrodynamics in PKDGRAV3 for galaxy formation simulations
• Not all peaks are created equal: the early growth of Supermassive Black Holes
• An Absence of Radio-Loud Active Galactic Nuclei in Geometrically Flat Quiescent Galaxies: Implications for Maintenance-Mode Feedback Models
• Global analysis of luminosity- and colour-dependent galaxy clustering in the Sloan Digital Sky Survey
• Measuring Star-Formation Histories, Distances, and Metallicities with Pixel Color-Magnitude Diagrams I: Model Definition and Mock Tests
• WVTICs -- SPH initial conditions for everyone
• Detection of the Mass-Dependent Dual-Type Transition of Galaxy Spins in IllustrisTNG Simulations
• Probabilistic model for dynamic galaxy decomposition
• Refining the mass estimate for the intermediate-mass black hole candidate in NGC 3319
• Predictions for LISA and PTA based on SHARK galaxy simulations
• Detecting preheating in proto-clusters with Lyman-$\alpha$ Forest Tomography
• The Baltimore Oriole's Nest: Cool Winds from the Inner and Outer Parts of a Star-Forming Galaxy at z=1.3
• Statistics of Two-point Correlation and Network Topology for Lyman Alpha Emitters at $z\approx 2.67$
• Numerical simulations of AGN wind feedback on black hole accretion: probing down to scales within the sphere of influence
• SEAGLE--III: Towards resolving the mismatch in the dark-matter fraction in early-type galaxies between simulations and observations
• The Supersonic Project: The Early Evolutionary Path of SIGOs
• The Supersonic Project: The eccentricity and rotational support of SIGOs and DM GHOSts
• Prospects of Probing Dark Matter Condensates with Gravitational Waves
• Dark against luminous matter around isolated central galaxies: a comparative study between modern surveys and Illustris-TNG
• Cosmology with Galaxy Cluster Properties using Machine Learning
• Outflows in the Gaseous Discs of Active Galaxies and their impact on Black Hole Scaling Relations
• Cosmological Simulation of Galaxy Groups and Clusters-I: Global Effect of Feedback from Active Galactic Nuclei
• Can the Low Redshift Lyman Alpha Forest Constrain AGN Feedback Models?
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. -- III. Stellar metallicity drivers in MaNGA and TNG50
• Reconciling Volumetric and Individual Galaxy Type Ia Supernova Rates
• Galaxy shapes in Magneticum. I. Connecting stellar and dark matter shapes to dynamical and morphological galaxy properties and the large-scale structure
• Validating the clustering predictions of empirical models with the FLAMINGO simulations
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• Near-infrared spectroscopy of 5 ultra-massive galaxies at 1.7 < z < 2.7
• Can HI 21 cm line trace the Missing Baryons in the Filamentary Structures?
• Outskirts of Nearby Disk Galaxies: Star Formation and Stellar Populations
• Implications of galaxy buildup for putative IMF variations in massive galaxies
• The Impact of the Dusty Torus on Obscured Quasar Halo Mass Measurements
• The relationship between galaxy and halo sizes in the Illustris and IllustrisTNG simulations
• Star formation history and transition epoch of cluster galaxies based on the Horizon-AGN simulation
• Multiple stellar populations in Schwarzschild modeling and the application to the Fornax dwarf
• Galaxy flows within 8,000 km/s from Numerical Action methods
• Formation and fate of low metallicity stars in IllustrisTNG50
• The Baryon Cycle at High Redshifts: Effects of Galactic Winds on Galaxy Evolution in Overdense and Average Regions
• Testing the SZ-based tomographic approach to the thermal history of the universe with pressure-density cross-correlations: Insights from the Magneticum simulation
• Performance analysis of parallel gravitational $N$-body codes on large GPU cluster
• Discrimination of heavy elements originating from Pop III stars in z = 3 intergalactic medium
• High-redshift test of gravity using enhanced growth of small structures probed by the neutral hydrogen distribution
• Star Formation in Massive Galaxies at Redshift $z\sim 0.5$
• The Formation of a Milky Way-sized Disk Galaxy 1. A Comparison of Numerical Methods
• Cosmology with cosmic web environments II. Redshift-space auto and cross power spectra
• Modified initial power spectrum and too big to fail problem
• On the detectability of massive black hole merger eventsby LISA
• The Direct-Method Oxygen Abundance of Typical Dwarf Galaxies at Cosmic High-Noon
• Galaxy And Mass Assembly (GAMA) Survey: The Merging Potential of Brightest Group Galaxies
• Addressing via N-body simulations the distribution of the satellite tidal debris in the Milky Way environment
• The Grism Lens-Amplified Survey from Space (GLASS). XII. Spatially Resolved Galaxy Star Formation Histories and True Evolutionary Paths at z > 1
• Measuring Star Formation Histories, Distances, and Metallicities with Pixel Color-Magnitude Diagrams II: Applications to Nearby Elliptical Galaxies
• Mitigating baryonic effects with a theoretical error covariance
• Emergence of Galactic Morphologies at Cosmic Dawn: Input from Numerical Modeling
• Probing the azimuthal environment of galaxies around clusters. From cluster core to cosmic filaments
• Comparing galaxy morphology in hydrodynamical simulation and in semi-analytic model
• A Local Universe model for constrained simulations
• Solution of the dark matter riddle within standard model physics: From black holes, galaxies and clusters to cosmology
• The MUSE-Faint survey. III. Constraining scalar field dark matter with Antlia B
• Resolution criteria to avoid artificial clumping in Lagrangian hydrodynamic simulations with a multi-phase interstellar medium
• Searching for the shadows of giants II: the effect of local ionisation on the Lyman-$\alpha$ absorption signatures of protoclusters at redshift $z\sim 2.4$
• HSC-CLAUDS survey: The star formation rate functions since z ~ 2 and comparison with hydrodynamical simulations
• Field-level simulation-based inference with galaxy catalogs: the impact of systematic effects
• Constraining galaxy-halo connection with high-order statistics
• Galaxy Mergers in the Epoch of Reionization II: Major Merger-Triggered Star Formation and AGN Activities at $z=$ 4.5-8.5
• What to expect when using globular clusters as tracers of the total mass distribution in Milky Way-mass galaxies
• The Origin of Massive Compact Galaxies: Lessons from IllustrisTNG
• Stellar Metallicity of Galaxies: New Insight on the Formation and Evolution of Low Surface Brightness Galaxies in the IllustrisTNG Simulation
• Galaxy assembly bias in the stellar-to-halo mass relation for red central galaxies from SDSS
• Stellar velocity dispersion and initial mass function gradients in dissipationless galaxy mergers
• On the connection between AGN radiative feedback and massive black hole spin
• Real galaxy mergers from galaxy pair catalogs
• The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
• ARTEMIS emulator: exploring the effect of cosmology and galaxy formation physics on Milky Way-mass haloes and their satellites
• What is the real accretion rate onto a black hole for low angular momentum accretion?
• VALES V: A kinematic analysis of the molecular gas content in $H$-ATLAS galaxies at $z\sim 0.03-0.35$ using ALMA
• Euclid preparation. LXVIII. Extracting physical parameters from galaxies with machine learning
• The impact of the cosmological constant on past and future star formation
• Magnification bias in the shear-ratio test: a viable mitigation strategy
• NIHAO XXVIII: Collateral effects of AGN on dark matter concentration and stellar kinematics
• Bursty star formation feedback and cooling outflows
• Studying galaxy cluster morphological metrics with Mock-X
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• Observational Diagnostics of Gas Flows: Insights from Cosmological Simulations
• Gravitational Waves from Massive Black Hole Mergers in ASTRID: Predictions for LISA
• Measuring the mass and concentration of dark matter halos from the velocity dispersion profile of their stars
• Host Galaxy Demographics Of Individually Detectable Supermassive Black-hole Binaries with Pulsar Timing Arrays
• EMERGE: Constraining merging probabilities and timescales of close galaxy pairs
• Assembly bias evidence in close galaxy pairs
• Mid-IR cosmological spectrophotometric surveys from space: Measuring AGN and star formation at the Cosmic Noon with a SPICA-like mission
• Triple and Quadruple Black Holes in the ASTRID Simulation at $z\sim 2$
• Connection Between Galaxies and HI in the Circumgalactic and Intergalactic Media: Variation According to Galaxy Stellar Mass and Star-formation Activity
• Active galactic nuclei feedback in an elliptical galaxy (III): the impacts and fate of cosmological inflow
• Moving and Reactive Boundary Conditions in Moving-Mesh Hydrodynamics
• Haloes at the ragged edge: The importance of the splashback radius
• Cosmic Web & Caustic Skeleton: non-linear Constrained Realizations -- 2D case studies
• Disparate Effects of Circumgalactic Medium Angular Momentum in IllustrisTNG and SIMBA
• Quenched, bulge-dominated, but dynamically cold galaxies in IllustrisTNG and their real-world counterparts
• Diverse dark matter profiles in FIRE dwarfs: black holes, cosmic rays and the cusp-core enigma
• Turbulence-induced deviation between baryonic field and dark matter field in the spatial distribution of the Universe
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• Galaxy populations in protoclusters at cosmic noon
• Anisotropic correlation functions as tracers of central galaxy alignments in simulations
• Early-type galaxy density profiles from IllustrisTNG: III. Effects on outer kinematic structure
• Magnetic dynamos in galaxy clusters: the crucial role of galaxy formation physics at high redshifts
• Improving Black Hole Accretion Treatment in Hydrodynamical Simulations
• A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations
• SCONCE: A cosmic web finder for spherical and conic geometries
• IllustrisTNG Snapshots for 10 Gyr of Dynamical Evolution of Brightest Cluster Galaxies and Their Host Clusters
• The feasibility of constraining DM interactions with high-redshift observations by JWST
• Asymmetric Drift of Andromeda Analogs in the IllustrisTNG Simulation
• Accurate Modeling of the Projected Galaxy Clustering in Photometric Surveys: I. Tests with Mock Catalogs
• The Next Generation Virgo Cluster Survey. XXXIII. Stellar Population Gradients in the Virgo Cluster Core Globular Cluster System
• Local Two-Sample Testing: A New Tool for Analysing High-Dimensional Astronomical Data
• The evolution of supermassive blackhole mass--bulge mass relation by a semi-analytic model, ${\nu }^2$GC
• Measuring galaxy-galaxy-galaxy-lensing with higher precision and accuracy
• MOND implications for spectral line profiles of shell galaxies: shell formation history and mass-velocity scaling relations
• Boosting Line Intensity Map Signal-to-Noise with the Ly-$\alpha$ Forest Cross-Correlation
• Cosmological Simulations of Stellar Halos with Gaia Sausage-Enceladus Analogues: Two Sausages, One Bun?
• Mass Reconstruction of Galaxy-scale Strong Gravitational Lenses Using a Broken Power-law Model
• Dark-ages reionization and galaxy formation simulation - IX. Economics of reionizing galaxies
• NeutralUniverseMachine: How Filaments and Dark Matter Halo Influence the Galaxy Cold Gas Content
• CosmoDRAGoN simulations -- I. Dynamics and observable signatures of radio jets in cosmological environments
• Spatially Resolved Circumgalactic Medium around a Star-Forming Galaxy Driving a Galactic Outflow at $z\approx 0.8$
• Supra-galactic Colour Patterns in Globular Cluster Systems
• Stacking Redshifted 21cm Images of HII Regions Around High Redshift Galaxies as a Probe of Early Reionization
• The Effect of Accretion Environment at Large Radius on Hot Accretion Flows
• The effects of the orbital configurations of mergers on reshaping galaxy structures
• Subaru HSC weak lensing of SDSS redMaPPer cluster satellite galaxies: Empirical upper limit on orphan fractions
• A rising tide: Intrinsic alignments since the turn of the millennium
• The MAGPI survey: The interdependence of the mass, star formation rate, and metallicity in galaxies at z~0.3
• Global Preventive Feedback of Powerful Radio Jets on Galaxy Formation
• Astrophysics with the Laser Interferometer Space Antenna
• An Escaping Outflow in a Galaxy with an Intermediate-mass Black Hole
• Resummed Kinetic Field Theory: Using Mesoscopic Particle Hydrodynamics to Describe Baryonic Matter in a Cosmological Framework
• Substructure in the Globular Cluster Populations of the Virgo Cluster Elliptical Galaxies M84 and M86
• Satellite galaxies in the Illustris-1 simulation: anisotropic locations around relatively isolated hosts
• AGN lifetimes in UV-selected galaxies: a clue to supermassive black hole-host galaxy coevolution
• Self-Interacting Dark Matter in Cosmology: accurate numerical implementation and observational constraints
• Growth of Linear Perturbations in a Universe with Superfluid Dark Matter
• Gas Inflow and Outflow Histories in Disk Galaxies as Revealed from Observations of Distant Star-Forming Galaxies
• The dark matter bispectrum from effective viscosity and one-particle irreducible vertices
• Revisiting the Relationship between the Long GRB Rate and Cosmic Star Formation History Based on a Large Swift Sample
• The history and mass content of cluster galaxies in the EAGLE simulation
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• HELLO project: High-$z$ Evolution of Large and Luminous Objects
• A comparison between semi-analytical gas cooling models and cosmological hydrodynamical simulations
• Baryon acoustic scale at $z_{\eff} = 0.166$ with the SDSS blue galaxies
• The fragility of thin discs in galaxies -- I. Building tailored N-body galaxy models
• Measuring Resolved Star Formation Histories from High-Precision Color-Magnitude Diagrams with StarFormationHistories.jl
• Intertwined Formation of ${\mathrm{H}}_2$, Dust, and Stars in Cosmological Simulations
• Isolated dark matter deprived galaxies in hydrodynamical simulations: real objects or artefacts?
• The spatial distribution deviation and the power suppression of baryons from dark matter
• Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
• Efficiently estimating mean, uncertainty and unconstrained large scale fraction of local Universe simulations with paired fixed fields
• Central galaxy alignments. Dependence on the mass and the large-scale environment
• Low-redshift quasars in the SDSS Stripe 82 II: associated companion galaxies and signature of star formation
• A Sea of Black Holes: Characterizing the LISA Signature for Stellar-Origin Black Hole Binaries
• Estimation of the Galaxy Quenching Rate in the Illustris Simulation
• Lessons from the Local Group (and beyond) on dark matter
• The galaxy bias profile of cosmic voids
• Dark-ages Reionization and Galaxy Formation Simulation - XV. Stellar evolution and feedback in dwarf galaxies at high redshift
• Dark matter deficient galaxies in the Illustris flat-$\Lambda$CDM model structure formation simulation
• KiDS+VIKING+GAMA: Testing semi-analytic models of galaxy evolution with galaxy-galaxy-galaxy lensing
• Premature supermassive black hole mergers in cosmological simulations of structure formation
• Evolution of massive quiescent galaxies via envelope accretion
• Orbit properties of massive prolate galaxies in the Illustris simulation
• Bimodal Formation Time Distribution for Infall Dark Matter Halos
• Precision Pollution - The effects of enrichment yields and timing on galactic chemical evolution
• Using Artificial Intelligence and real galaxy images to constrain parameters in galaxy formation simulations
• Domain adaptation techniques for improved cross-domain study of galaxy mergers
• Cosmic Stillness: High Quiescent Galaxy Fractions Across Upper Mass Scales in the Early Universe to z = 7 with JWST
• Does radiative feedback make faint z>6 galaxies look small?
• Stellar and Black Hole Mass Densities as Empirical Tracers of Co-evolution Show Lock-step Growth since $z\sim 3$
• The fate of the interstellar medium in early-type galaxies. IV. The impact of stellar feedback, mergers, and black holes on the cold ISM in simulated galaxies
• Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies
• Can Cooling and Heating Functions be Modeled with Homogeneous Radiation Fields?
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• Structure and large scale environment of galaxy pairs in the S-PLUS DR4
• Testing galaxy formation models with the stellar mass-halo mass relations for star-forming and quiescent galaxies
• N-body simulations of structure formation in thermal inflation cosmologies
• The OTELO survey: the star formation rate evolution of low-mass galaxies
• The scaling relations of galaxies back in time: the road toward virialization
• The internal metallicity distributions of simulated galaxies from EAGLE, Illustris, and IllustrisTNG at z=1.8-4 as probed by Gamma Ray Burst hosts
• The BACCO Simulation Project: A baryonification emulator with Neural Networks
• Searching for dark matter subhalos in the Fermi-LAT catalog with Bayesian neural networks
• Galactic Cosmic-Ray Induced Production of Lithium in the Small Magellanic Cloud
• Satellite Galaxies in the Illustris-1 Simulation: Poor Tracers of the Mass Distribution
• Galaxy-galaxy lensing in the VOICE deep survey
• Evolution of matter and galaxy clustering in cosmological hydrodynamical simulations
• Anatomy of galactic star formation history: Roles of different modes of gas accretion, feedback, and recycling
• A Maximum Parsimony analysis of the effect of the environment on the evolution of galaxies
• Relativistic imprints on dispersion measure space distortions
• Sensitivity analysis of a galaxy formation model
• Resummed Kinetic Field Theory: a model of coupled baryonic and dark matter
• On the scatter of the present-day stellar metallicity-mass relation of cluster dwarf galaxies
• Tiny galaxies and dark substructures: exploring the "dark" subhaloes in TNG50
• Introduction to Tidal Streams
• Probing the earliest phases in the formation of massive galaxies with simulated HST+JWST imaging data from Illustris
• Differences in the Physical Properties of Satellite Galaxies within Relaxed and Disturbed Galaxy Groups and Clusters
• Evolution of X-ray galaxy Cluster Properties in a Representative Sample (EXCPReS). Optimal binning for temperature profile extraction
• The Dawn of Black Holes
• Panchromatic SED fitting codes and modelling techniques
• The Qz5 Survey (I): How the HI Mass Density of the Universe Evolves With Cosmic Time
• Star formation and black hole accretion activity in rich local clusters of galaxies
• Conditional Colour-Magnitude Distribution of Central Galaxies in Galaxy Formation Models
• MOCCA-Survey Database: Extra Galactic Globular Clusters. III. The population of black holes in Milky Way and Andromeda-like galaxies
• Evolution of dwarf galaxy observable parameters
• Untangling Stellar Components of Galaxies: Evaluation of Dynamical Decomposition Methods in Simulated Galaxies with GalaxyChop
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Jellyfish galaxies with the IllustrisTNG simulations -- Supermassive black hole activity in dense environments with ram-pressure stripped satellites
• IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• Reconstructing the LISA massive black hole binary population via iterative kernel density estimation
• TODDLERS: A New UV to Millimeter Emission Library for Star-Forming Regions. II. Star Formation Rate Indicators Using Auriga Zoom Simulations
• An Improved and Physically-Motivated Scheme for Matching Galaxies with Dark Matter Halos
• Improving Performance of Zoom-In Cosmological Simulations using Initial Conditions with Customized Grids
• Evolving beyond z=0: insights about the future of stars and the intergalactic medium
• Cosmological boost factor for dark matter annihilation at redshifts of $z=10$-$100$ using the power spectrum approach
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• Galaxy Manifold: Characterizing and understanding galaxies with two parameters
• The influence of baryons on low-mass haloes
• Inferring Mbh-Mbulge Evolution from the Gravitational Wave Background
• Dark matter haloes: a multistream view
• Dwarf-Dwarf interactions and their influence on star formation : Insights from post-merger galaxies
• A fully Lagrangian, non-parametric bias model for dark-matter halos
• The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
• Large-scale geometry and topology of gas fields: Effects of AGN and stellar feedback
• The viability of low-mass subhaloes as targets for gamma-ray dark matter searches
• Modelling the selection of galaxy groups with end to end simulations
• Quenching vs. Quiescence: forming realistic massive ellipticals with a simple starvation model
• GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations
• Reconstructing HI power spectrum with minimal parameters using the dark matter distribution beyond halos
• Exploring selection biases in FRB dispersion-galaxy cross-correlations with magnetohydrodynamical simulations
• The origin of galaxy colour bimodality in the scatter of the Stellar-to-Halo Mass Relation
• A new strategy for matching observed and simulated lensing galaxies
• Disentangling the Halo: Joint Model for Measurements of the Kinetic Sunyaev-Zeldovich Effect and Galaxy-Galaxy Lensing
• Assembly Conformity of Structure Growth: Fossil versus Normal Groups of Galaxies
• Feedback from intermediate mass black holes on dwarf galaxy morphology at z=2
• Born to be Starless: Revisiting the Missing Satellite Problem
• Elliptical (E) and ellicular (ES) galaxies in the M_bh-M_*,sph diagram, and a merger-driven explanation for the origin of ES galaxies, anti-truncated stellar discs in lenticular galaxies, and the Sersicification of E galaxy light profiles
• Core to Cosmic Edge: SIMBA-C's New Take on Abundance Profiles in the Intragroup Medium at z = 0
• A study of Neural networks point source extraction on simulated Fermi/LAT Telescope images
• Exploring the evolution of a dwarf spheroidal galaxy with SPH simulations: I. Stellar feedback
• Impact of supermassive black hole growth on star formation
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• The breakBRD Breakdown: Using IllustrisTNG to Track the Quenching of an Observationally-Motivated Sample of Centrally Star-Forming Galaxies
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Redshift and stellar mass dependence of intrinsic shapes of disc-dominated galaxies from COSMOS observations below $z=1.0$
• The evolution of the barred galaxy population in the TNG50 simulation
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• The Gemini/HST Galaxy Cluster Project: Environment Effects on the Stellar Populations in the Lynx Clusters at z=1.27
• Performance Enhancement of Tree-based Friends-of-friend Galaxy-finder for High-resolution Simulations of Galaxy Formation
• Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies
• Comparison of Low-Mass and High-Mass Star Formation
• The Circumgalactic Medium from the CAMELS Simulations: Forecasting Constraints on Feedback Processes from Future Sunyaev-Zeldovich Observations
• Can we constrain the evolution of HI bias using configuration entropy?
• The THESAN project: environmental drivers of Local Group reionization
• The AIDA-TNG project: dark matter profiles and concentrations in alternative dark matter models
• What is the right way to quench star formation in semi-analytic model of galaxy formation?
• Signatures of simulated spiral arms on radial actions
• Quantitatively rating galaxy simulations against real observations with anomaly detection
• Photometric and Kinematic Misalignments and Their Evolution Among Fast and Slow Rotators in the Illustris Simulation
• The AIDA-TNG project: 3D halo shapes
• The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
• Observational biases on rotation curves from IFU data at cosmic noon
• LeMMINGs. V. Nuclear activity and bulge properties: a detailed multi-component decomposition of $e$-MERLIN Palomar galaxies with $HST$
• Dynamical disequilibrium in dwarf galaxies: rethinking gas dynamics, rotation curves, and dark matter inference
• New insights on low-mass dark matter subhalo tidal tracks via numerical simulations
• Thermal X-ray signatures in late-stage unequal-mass massive black hole binary mergers
• Dynamics of merging: Post-merger mixing and relaxation of an Illustris galaxy
• Virial models and Anisotropy of Velocity Dispersion in e-galaxies
• Simultaneously Modelling Dusty Star Forming Galaxies and Massive Quiescents: A Calibration Framework for Galaxy Formation Models
• Probabilistic Lagrangian bias estimators and the cumulant bias expansion
• Classifying merger stages with adaptive deep learning and cosmological hydrodynamical simulations
• The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z=3.55$
• Spatial field reconstruction with INLA: Application to simulated galaxies
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• Unsupervised Domain Adaptation for Constraining Star Formation Histories
• Stirring the cosmic pot: how black hole feedback shapes the matter power spectrum in the Fable simulations
• AMADA-Analysis of Multidimensional Astronomical Datasets
• FAST drift scan survey for HI intensity mapping: simulation on hunting HI filament with pairwise stacking
• Exploring the halo-galaxy connection with probabilistic approaches
• The signature of galaxy formation models in the power spectrum of the hydrogen 21cm line during reionization
• Assessment of Dark Matter Models Using Dark Matter Correlations across Dwarf Spheroidal Galaxies
• Gravitational Wave Peep Contributions to Background Signal Confusion Noise for LISA
• Investigating the residuals in the $M_{\bullet }-M_{\ast }$ relation using the SIMBA cosmological simulation
• MUSEQuBES: Physical conditions, origins, and multi-element abundances of the circumgalactic medium of an isolated, star-forming dwarf galaxy at z=0.57
• Simulation budgeting for hybrid effective field theories
• Black hole merger rates for LISA and LGWA from semi-analytical modelling of light seeds
• Variability in Cosmological Hydrodynamical Simulations: how Stochastic Processes, Numerical Effects, and Reproducibility Limits impact Predictability
• Reduced Gas Accretion onto Galaxies due to Effects of External Giant Radio Lobes
• The catalogue of virtual early-type galaxies from IllustrisTNG: validation and real observation consistency
• Radio Galaxies in SIMBA: A MIGHTEE Comparison
• A novel analysis of contamination in Lyman-break galaxy samples at $\mathbf{z}\sim 6-8$: spatial correlation with intermediate-redshift galaxies at $\mathbf{z}\sim 1.3-2$
• The multi-component fitting to the star formation histories in the TNG simulation
• Effect of cosmic rays and ionizing radiation on observational ultraviolet plasma diagnostics in the circumgalactic medium
• Towards an Observational Detection of Halo Spin Bias using Spin-Orbit Coherence
• Beyond mirkwood: Enhancing SED Modeling with Conformal Predictions
• Galaxy-galaxy strong lens perturbations: line-of-sight haloes versus lens subhaloes
• The stability of galaxies in an expanding universe obtained by Newtonian dynamics
• Extended Hernquist-Springel formalism for cosmic star formation
• Bridging Simulations and Observations: New Insights into Galaxy Formation Simulations via Out-of-Distribution Detection and Bayesian Model Comparison
• Dipole Distortions in the Intergalactic Medium
• A hierarchical clustering method for quantifying satellite abundance
• Absorption systems at $z\sim 2$ as a probe of the circum galactic medium: a probabilistic approach
• Disc instability and bar formation: view from the IllustrisTNG simulations
• The LEGA-C and SAMI Galaxy Surveys: Quiescent Stellar Populations and the Mass-Size Plane across 6 Gyr
• Testing the thermal Sunyaev-Zel'dovich power spectrum of a halo model using hydrodynamical simulations
• The NewHorizon Simulation -- To Bar Or Not To Bar
• How well is angular momentum accretion modelled in semi-analytic galaxy formation models?
• Recoiling supermassive black holes in analytical and numerical galaxy potential
• DeepMerge: Classifying High-redshift Merging Galaxies with Deep Neural Networks
• The Stellar Chemical Abundances of Simulated Massive Galaxies at $z=2$
• A novel Cosmic Filament catalogue from SDSS data
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• A Simulation Driven Deep Learning Approach for Separating Mergers and Star Forming Galaxies: The Formation Histories of Clumpy Galaxies in all the CANDELS Fields
• Yellow Post-Asymptotic-Giant-Branch Stars as Standard Candles. I. Calibration of the Luminosity Function in Galactic Globular Clusters
• Stellar populations of stellar halos: Results from the Illustris simulation
• Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in IllustrisTNG
• The impact of black hole feedback on the UV luminosity and stellar mass assembly of high-redshift galaxies
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• Observed structural parameters of EAGLE galaxies: reconciling the mass-size relation in simulations with local observations
• Lack of influence of the environment in the earliest stages of massive galaxy formation
• Determining the Dark Matter distribution in galaxies with Deep Learning
• Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window
• Understanding the Galaxy
• The link between star formation and gas in nearby galaxies
• Wind accretion onto compact objects
• High and low Sérsic index bulges in Milky Way- and M31-like galaxies: origin and connection to the bar with TNG50
• Predicting large scale cosmological structure evolution with generative adversarial network-based autoencoders
• Predictions for the X-ray circumgalactic medium of edge-on discs and spheroids
• The black hole population in low-mass galaxies in large-scale cosmological simulations
• Populating Galaxies Into Halos Via Machine Learning on the Simba Simulation
• Review on Dark Matter Tools
• Mimicking the halo-galaxy connection using machine learning
• Shape asymmetries and the relation between lopsidedness and radial alignment in simulated galaxies
• Boosting (In)direct Detection of Dark Matter
• Merger rates of intermediate-mass black hole binaries in nuclear star clusters
• The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
• Reconciling concentration to virial mass relations
• Exploring realistic nanohertz gravitational-wave backgrounds
• First Steps Toward a Method for Estimating Cosmological Parameters using Strong Lensing, X-ray and Dynamics Total Mass Estimates
• Structure Formation under Inelastic Two-Component Dark Matter: Halo Statistics and Matter Power Spectra in the High-$z$ Universe
• The Galactic Pizza: Flat Rotation Curves in the Context of Cosmological Time-Energy Coupling
• Astrophysical Black holes: An Explanation for the Galaxy Quenching
• Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling
• DeepVoid: A Deep Learning Void Detector
• Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback
• Numerical Study of Bar Suppression in Galaxy Models Due to Disc Heating
• Black Hole-Galaxy Correlations in Cluster Zoomed-in Simulations: GIZMO-SIMBA and TNG-Cluster
• Bound or blown: the fate of hot gas in galaxy groups
• Euclid: A blue galaxy population and a brightest cluster galaxy in the making in a $z\sim 1.74$ MaDCoWS2 galaxy cluster candidate
• Constraining the population of dark matter halo shapes using hierarchical inference with extragalactic stellar streams
• Entropy plateaus can emerge from gas replacement at a characteristic halo mass in simulated groups and clusters of galaxies
• Sahyadri: A simulation suite for the cosmology dependence of the Cosmic Web
• Galaxy quenching across the Cosmic Web: disentangling mass and environment with SDSS DR18
• The frame-dragging vector potential on galaxy scales from Dark-Matter-only Newtonian $N$-body simulations
• The intricate link between galaxy dynamics and intrinsic shape (or why so-called prolate rotation is a misnomer)
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• Beyond single tracers: CNN-based inference of galaxy mass profiles from combined gas and stellar kinematics
• Cavendish experiment with fast radio bursts on cosmological scales
• Unravelling the role of merger histories in the population of In situ stars: linking IllustrisTNG cosmological simulation to H3 survey
• Gas flows in galaxy mergers: supersonic turbulence in bridges, accretion from the circumgalactic medium, and metallicity dilution
• The lens SW05 J143454.4+522850: a fossil group at redshift 0.6?