A physical model for cosmological simulations of galaxy formation: multi-epoch validation

Abstract

We present a multi-epoch analysis of the galaxy populations formed within the cosmological hydrodynamical simulations presented in Vogelsberger et al. (2013). These simulations explore the performance of a recently implemented feedback model which includes primordial and metal line radiative cooling with self-shielding corrections; stellar evolution with associated mass loss and chemical enrichment; feedback by stellar winds; black hole seeding, growth and merging; and AGN quasar- and radio-mode heating with a phenomenological prescription for AGN electro-magnetic feedback. We illustrate the impact of the model parameter choices on the resulting simulated galaxy population properties at high and intermediate redshifts. We demonstrate that our scheme is capable of producing galaxy populations that broadly reproduce the observed galaxy stellar mass function extending from redshift z=0 to z=3. We also characterise the evolving galactic B-band luminosity function, stellar mass to halo mass ratio, star formation main sequence, Tully-Fisher relation, and gas-phase mass-metallicity relation and confront them against recent observational estimates. This detailed comparison allows us to validate elements of our feedback model, while also identifying areas of tension that will be addressed in future work.

22 pages, 10 figures, submitted to MNRAS. Volume-rendering movies and high-resolution images can be found at http://www.cfa.harvard.edu/itc/research/arepogal/

References in corpus (50)

• Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
• Star Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies
• UV Star Formation Rates in the Local Universe
• A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: I. Galaxy Mergers & Quasar Activity
• A Semi-Analytic Model for the Co-evolution of Galaxies, Black Holes, and Active Galactic Nuclei
• The Mass-Metallicity Relation at z~2
• A unified model for AGN feedback in cosmological simulations of structure formation
• Star Formation and Feedback in Smoothed Particle Hydrodynamic Simulations--I. Isolated Galaxies
• A New Calculation of the Ionizing Background Spectrum and the Effects of HeII Reionization
• Cosmological Simulations of Intergalactic Medium Enrichment from Galactic Outflows
• The stellar mass assembly of galaxies from z=0 to z=4. Analysis of a sample selected in the rest-frame near-infrared with Spitzer
• Forming Disk Galaxies in Lambda CDM Simulations
• Direct cosmological simulations of the growth of black holes and galaxies
• Mass, Metal, and Energy Feedback in Cosmological Simulations
• The 2013 Release of Cloudy
• A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: II. Formation of Red Ellipticals
• Moving mesh cosmology: tracing cosmological gas accretion
• Bimodal gas accretion in the Horizon-MareNostrum galaxy formation simulation
• z~7-10 Galaxies in the HUDF and GOODS fields, and their UV Luminosity Functions
• On the onset of galactic winds in quiescent star forming galaxies
• A Revised Model for the Formation of Disk Galaxies: Low Spin and Dark-Halo Expansion
• The Importance of Mergers for the Origin of Intracluster Stars in Cosmological Simulations of Galaxy Clusters
• The Origin and Evolution of the Mass-Metallicity Relationship for Galaxies: Results from Cosmological N-Body Simulations
• Effects of Supernova Feedback on the Formation of Galaxy Disks
• HeII Reionization and its Effect on the IGM
• Evolution of the Intergalactic Opacity: Implications for the Ionizing Background, Cosmic Star Formation, and Quasar Activity
• A Direct Precision Measurement of the Intergalactic Lyman-alpha Opacity at 2<z<4.2
• Bursting and Quenching in Massive Galaxies without Major Mergers or AGNs
• Simulations of Cosmic Chemical Enrichment
• An Observed Fundamental Plane Relation for Supermassive Black Holes
• A Theoretical Interpretation of the Black Hole Fundamental Plane
• The Formation and Evolution of Intracluster Light
• Following the flow: tracer particles in astrophysical fluid simulations
• The onion universe: all sky lightcone simulations in spherical shells
• IMAGES-III: The evolution of the Near-Infrared Tully-Fisher relation over the last 6 Gyr
• Full-Sky Weak Lensing Simulation with 70 Billion Particles
• The Large-Scale Orientations of Disk Galaxies
• Measuring nebular temperatures: the effect of new collision strengths with equilibrium and kappa-distributed electron energies
• The rest-frame optical luminosity functions of galaxies at 2<z<3.5
• The Halpha-based Star Formation Rate Density of the Universe at z=0.84
• The Self-Regulated Growth of Supermassive Black Holes
• The impact of radio feedback from active galactic nuclei in cosmological simulations: Formation of disk galaxies
• The dust un-biased cosmic star formation history from the 20 cm VLA-COSMOS survey
• z~7-10 Galaxies behind Lensing Clusters: Contrast with Field Search Results
• Quasars: What turns them off?
• Clues for the origin of the fundamental metallicity relations. I: The hierarchical building up of the structure
• Absorption signatures of warm-hot gas at low redshift: OVI
• Rotation rates, sizes, and star formation efficiencies of a representative population of simulated disc galaxies
• The Tully-Fisher relation and its evolution with redshift in cosmological simulations of disc galaxy formation
• Infrared Spectral Energy Distributions of z~0.7 Star-Forming Galaxies

Cited by in corpus (260)

• Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
• Simulating Galaxy Formation with the IllustrisTNG Model
• First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
• The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
• Galaxies on FIRE (Feedback In Realistic Environments): Stellar Feedback Explains Cosmologically Inefficient Star Formation
• Physical Models of Galaxy Formation in a Cosmological Framework
• First results from the IllustrisTNG simulations: A tale of two elements -- chemical evolution of magnesium and europium
• Introducing the Illustris Project: the evolution of galaxy populations across cosmic time
• First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time
• The merger rate of galaxies in the Illustris Simulation: a comparison with observations and semi-empirical models
• De Re Metallica: The cosmic chemical evolution of galaxies
• The Illustris simulation: the evolving population of black holes across cosmic time
• How to Measure Galaxy Star Formation Histories II: Nonparametric Models
• The Illustris Simulation: Public Data Release
• Deriving Physical Properties from Broadband Photometry with Prospector: Description of the Model and a Demonstration of its Accuracy Using 129 Galaxies in the Local Universe
• The stellar mass assembly of galaxies in the Illustris simulation: growth by mergers and the spatial distribution of accreted stars
• The optical morphologies of galaxies in the IllustrisTNG simulation: a comparison to Pan-STARRS observations
• The Origin and Evolution of the Galaxy Mass-Metallicity Relation
• The Cosmic Baryon Cycle and Galaxy Mass Assembly in the FIRE Simulations
• Modelling and interpreting spectral energy distributions of galaxies with BEAGLE
• The Confinement of Star-Forming Galaxies into a Main Sequence through Episodes of Gas Compaction, Depletion, and Replenishment
• The formation of disc galaxies in high resolution moving-mesh cosmological simulations
• The MassiveBlack-II Simulation: The Evolution of Halos and Galaxies to z~0
• The CAMELS project: Cosmology and Astrophysics with MachinE Learning Simulations
• The star-formation activity of IllustrisTNG galaxies: main sequence, UVJ diagram, quenched fractions, and systematics
• The Formation of Massive, Compact Galaxies at z=2 in the Illustris Simulation
• The star formation main sequence and stellar mass assembly of galaxies in the Illustris simulation
• (Star)bursts of FIRE: observational signatures of bursty star formation in galaxies
• An Older, More Quiescent Universe from Panchromatic SED Fitting of the 3D-HST Survey
• Massive Black Hole Binary Mergers in Dynamical Galactic Environments
• How stellar feedback simultaneously regulates star formation and drives outflows
• Spatially-Resolved Star Formation Main Sequence of Galaxies in the CALIFA Survey
• The evolution of the mass-metallicity relation in IllustrisTNG
• Galactic Angular Momentum in the Illustris Simulation: Feedback and the Hubble Sequence
• The cosmic merger rate of neutron stars and black holes
• Radiative feedback and the low efficiency of galaxy formation in low-mass haloes at high redshift
• The Impact of Enhanced Halo Resolution on the Simulated Circumgalactic Medium
• Galaxy Morphology and Star Formation in the Illustris Simulation at z=0
• The role of mergers and halo spin in shaping galaxy morphology
• Baryons in the CosmicWeb of IllustrisTNG - I: Gas in Knots, Filaments, Sheets and Voids
• The cosmic merger rate of stellar black hole binaries from the Illustris simulation
• COSMOS2020: The Galaxy Stellar Mass Function: the assembly and star formation cessation of galaxies at $0.2<z\le 7.5$
• The abundance, distribution, and physical nature of highly ionized oxygen OVI, OVII, and OVIII in IllustrisTNG
• Ejective and preventative: the IllustrisTNG black hole feedback and its effects on the thermodynamics of the gas within and around galaxies
• Resolving small-scale cold circumgalactic gas in TNG50
• The Gravitational Wave Background from Massive Black Hole Binaries in Illustris: spectral features and time to detection with pulsar timing arrays
• Supermassive black holes in cosmological simulations I: M_BH-M_star relation and black hole mass function
• Metal flows of the circumgalactic medium, and the metal budget in galactic halos
• The FMOS-Cosmos Survey of Star-Forming Galaxies at z~1.6 II. The Mass-Metallicity Relation and the Dependence on Star Formation Rate and Dust Extinction
• Neutral hydrogen in galaxy halos at the peak of the cosmic star formation history
• EDGE: the mass-metallicity relation as a critical test of galaxy formation physics
• Halo Mass and Assembly History Exposed in the Faint Outskirts: the Stellar and Dark Matter Haloes of Illustris Galaxies
• The impact of feedback on cosmological gas accretion
• Quenched fractions in the IllustrisTNG simulations: comparison with observations and other theoretical models
• Dust Formation in Milky Way-like Galaxies
• The MillenniumTNG Project: The hydrodynamical full physics simulation and a first look at its galaxy clusters
• High redshift JWST predictions from IllustrisTNG: Dust modelling and galaxy luminosity functions
• Simulating the dust content of galaxies: successes and failures
• Jellyfish galaxies with the IllustrisTNG simulations: I. Gas-stripping phenomena in the full cosmological context
• The MOSDEF Survey: Dissecting the star-formation rate vs. stellar mass relation using H$\alpha$ and H$\beta$ emission lines at z ~ 2
• The FABLE simulations: A feedback model for galaxies, groups and clusters
• The properties of merging black holes and neutron stars across cosmic time
• Synthetic Galaxy Images and Spectra from the Illustris Simulation
• Recoiling black holes: prospects for detection and implications of spin alignment
• The impact of galactic properties and environment on the quenching of central and satellite galaxies: A comparison between SDSS, Illustris and L-Galaxies
• Zooming in on accretion - II. Cold Circumgalactic Gas Simulated with a super-Lagrangian Refinement Scheme
• Damped Lyman-alpha absorbers as a probe of stellar feedback
• The diverse evolutionary paths of simulated high-z massive, compact galaxies to z=0
• Shape of Dark Matter Haloes in the Illustris Simulation: Effects of Baryons
• Atomic and molecular gas in IllustrisTNG galaxies at low redshift
• Modeling the atomic-to-molecular transition in cosmological simulations of galaxy formation
• Single Sources in the Low-Frequency Gravitational Wave Sky: properties and time to detection by pulsar timing arrays
• Similar star formation rate and metallicity evolution timescales drive the fundamental metallicity relation
• The COSMOS2015 galaxy stellar mass function: 13 billion years of stellar mass assembly in 10 snapshots
• Hot gas in massive halos drives both mass quenching and environment quenching
• The Impact of Galactic Feedback on the Circumgalactic Medium
• Atomic hydrogen in IllustrisTNG galaxies: the impact of environment parallelled with local 21-cm surveys
• Galaxy And Mass Assembly (GAMA): Refining the Local Galaxy Merger Rate using Morphological Information
• 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
• 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
• Galaxy mergers on a moving mesh: a comparison with smoothed-particle hydrodynamics
• Mapping substructure in the HST Frontier Fields cluster lenses and in cosmological simulations
• Formation and Incidence of Shell Galaxies in the Illustris Simulation
• The MUSE Hubble Ultra Deep Field Survey XI. Constraining the low-mass end of the stellar mass - star formation rate relation at $z<1$
• The KMOS Redshift One Spectroscopic Survey (KROSS): rotational velocities and angular momentum of z~0.9 galaxies
• MusE GAs FLOw and Wind (MEGAFLOW) I: First MUSE results on background quasars
• 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
• 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
• Reproducing the Kinematics of Damped Lyman-alpha Systems
• High Angular Momentum Halo Gas: a Feedback and Code-Independent Prediction of LCDM
• A Deep Learning Approach to Galaxy Cluster X-ray Masses
• On the Assembly of Dwarf Galaxies in Clusters and their Efficient Formation of Globular Clusters
• Why do high-redshift galaxies show diverse gas-phase metallicity gradients?
• Large-scale mass distribution in the Illustris simulation
• Probing Massive Black Hole Binary Populations with LISA
• Massive BH Binaries as Periodically-Variable AGN
• Log-normal star formation histories in simulated and observed galaxies
• Metallicity of stars formed throughout the cosmic history based on the observational properties of star forming galaxies
• The Metal Abundances across Cosmic Time ($\mathcal{M}\mathcal{A}\mathcal{C}\mathcal{T}$) Survey. II. Evolution of the Mass-Metallicity Relation over 8 Billion Years, using [OIII]$\lambda$4363Å-based Metallicities
• An analysis of the evolving comoving number density of galaxies in hydrodynamical simulations
• Equilibrium Model Constraints on Baryon Cycling Across Cosmic Time
• Interacting galaxies in the IllustrisTNG simulations -- II: Star formation in the post-merger stage
• The abundance of satellites around Milky Way- and M31-like galaxies with the TNG50 simulation: a matter of diversity
• A little FABLE: exploring AGN feedback in dwarf galaxies with cosmological simulations
• Diverse Structural Evolution at z > 1 in Cosmologically Simulated Galaxies
• The ALMA Spectroscopic Survey in the HUDF: the molecular gas content of galaxies and tensions with IllustrisTNG and the Santa Cruz SAM
• Hot Gaseous Coronae around Spiral Galaxies: Probing the Illustris Simulation
• SPECULATOR: Emulating stellar population synthesis for fast and accurate galaxy spectra and photometry
• The dust-continuum size of TNG50 galaxies at $z=1-5$: a comparison with the distribution of stellar light, stars, dust and H${}_2$
• X-ray Signatures of Black Hole Feedback: Hot Galactic Atmospheres in IllustrisTNG and X-ray Observations
• The colors of satellite galaxies in the Illustris Simulation
• What shapes a galaxy? - Unraveling the role of mass, environment and star formation in forming galactic structure
• The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations
• The physical origins and dominant emission mechanisms of Lyman-alpha halos: results from the TNG50 simulation in comparison to MUSE observations
• The interplay of Self-Interacting Dark Matter and baryons in shaping the halo evolution
• Automated Distant Galaxy Merger Classifications from Space Telescope Images using the Illustris Simulation
• Statistical properties of paired fixed fields
• The Impact of Galactic Winds on the Angular Momentum of Disk Galaxies in the Illustris Simulation
• Hydrogen Reionization in the Illustris universe
• Size matters: abundance matching, galaxy sizes, and the Tully-Fisher relation in EAGLE
• The evolution of the star forming sequence in hierarchical galaxy formation models
• L-GALAXIES 2020: The evolution of radial metallicity profiles and global metallicities in disc galaxies
• Mg II Absorption at 2<z<7 with Magellan/FIRE, III. Full Statistics of Absorption Towards 100 High-Redshift QSOs
• The baryon content of groups and clusters of galaxies in the FABLE simulations
• Assessing the Jeans Anisotropic Multi-Gaussian Expansion method with the Illustris simulation
• Dust in and around galaxies: dust in cluster environments and its impact on gas cooling
• Subhalo Demographics in the Illustris Simulation: Effects of Baryons and Halo-to-Halo Variation
• IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation
• The MOSDEF Survey: Metallicity Dependence of the PAH Emission at High Redshift and Implications for 24 micron-inferred IR Luminosities and Star Formation Rates at z~2
• A missing outskirts problem? Comparisons between stellar halos in the Dragonfly Nearby Galaxies Survey and the TNG100 simulation
• 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
• Formation of S0 galaxies through mergers. Evolution in the Tully-Fisher relation since $z\sim 1$
• Testing the effect of galactic feedback on the IGM at z ~ 6 with metal-line absorbers
• Baryonic effects on the matter bispectrum
• Modeling Galactic Conformity with the Color-Halo Age Relation in the Illustris Simulation
• ETHOS -- an effective theory of structure formation: predictions for the high-redshift Universe -- abundance of galaxies and reionization
• The host galaxies of double compact objects merging in the local Universe
• The impact of stellar and AGN feedback on halo-scale baryonic and dark matter accretion in the EAGLE simulations
• Galactic angular momentum in the IllustrisTNG simulation -- I. Connection to morphology, halo spin, and black hole mass
• Diffuse gas properties and stellar metallicities in cosmological simulations of disc galaxy formation
• Origin of the galaxy HI size-mass relation
• On the origin of the mass-metallicity gradient relation in the local Universe
• Early-type galaxy density profiles from IllustrisTNG: I. Galaxy correlations and the impact of baryons
• Galaxies lacking dark matter in the Illustris simulation
• Comparing galaxy formation in the L-GALAXIES semi-analytical model and the IllustrisTNG simulations
• The emergence of passive galaxies in the early Universe
• Galaxy And Mass Assembly (GAMA): The inferred mass--metallicity relation from z=0 to 3.5 via forensic SED fitting
• 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
• High redshift JWST predictions from IllustrisTNG: III. Infrared luminosity functions, obscured star formation and dust temperature of high-redshift galaxies
• The growth of brightest cluster galaxies in the TNG300 simulation:dissecting the contributions from mergers and in situ star formation
• Submillimetre galaxies in cosmological hydrodynamical simulations -- an opportunity for constraining feedback models
• Galaxies in the Illustris simulation as seen by the Sloan Digital Sky Survey - I: Bulge+disc decompositions, methods, and biases
• The Mass Profile of the Milky Way to the Virial Radius from the Illustris Simulation
• The Incidence of Low-Metallicity Lyman-Limit Systems at z~3.5: Implications for the Cold-Flow Hypothesis of Baryonic Accretion
• Early chemo-dynamical evolution of dwarf galaxies deduced from enrichment of r-process elements
• Shock finding on a moving-mesh: II. Hydrodynamic shocks in the Illustris universe
• Gravitational Self-Lensing in Populations of Massive Black Hole Binaries
• How Environment Affects Galaxy Metallicity through Stripping and Formation History: Lessons from the Illustris Simulation
• Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
• Globular clusters as tracers of the dark matter content of dwarfs in galaxy clusters
• The host galaxies of double compact objects across cosmic time
• A gradient based method for modeling baryons and matter in halos of fast simulations
• A study of stellar orbit fractions: simulated IllustrisTNG galaxies compared to CALIFA observations
• Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
• Molecular hydrogen in IllustrisTNG galaxies: carefully comparing signatures of environment with local CO & SFR data
• Non-parametric Morphologies of Galaxies in the EAGLE Simulation
• Enhancing AGN efficiency and cool-core formation with anisotropic thermal conduction
• The combined and respective roles of imaging and stellar kinematics in identifying galaxy merger remnants
• Reproducing cosmic evolution of galaxy population from $z=4$ to $0$
• Forward and backward galaxy evolution in comoving number density space
• The Missing Satellite Problem in 3D
• IQ Collaboratory II: The Quiescent Fraction of Isolated, Low Mass Galaxies Across Simulations and Observations
• 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
• Towards a consistent framework of comparing galaxy mergers in observations and simulations
• The importance of preventive feedback: inference from observations of the stellar masses and metallicities of Milky Way dwarf galaxies
• Chemical pre-processing of cluster galaxies over the past 10 billion years in the IllustrisTNG simulations
• EAGLE-Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
• DEVILS: Cosmic evolution of SED-derived metallicities and their connection to star-formation histories
• The Stripe 82 Massive Galaxy Project III: A Lack of Growth Among Massive Galaxies
• The Impact of baryonic physics on the kinetic Sunyaev-Zel'dovich Effect
• Galaxy Zoo: Morphological classification of galaxy images from the Illustris simulation
• Gas-phase metallicity break radii of star-forming galaxies in IllustrisTNG
• Spherical Cows in Dark Matter Indirect Detection
• Considerations for the Observability of Kinematically Offset Binary AGN
• Stellar and Weak Lensing Profiles of Massive Galaxies in the Hyper-Suprime Cam Survey and in Hydrodynamic Simulations
• A disturbing FABLE of mergers, feedback, turbulence, and mass biases in simulated galaxy clusters
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
• Quantifying Baryonic Feedback on Warm-Hot Circumgalactic Medium in CAMELS Simulations
• Unraveling the interplay between SIDM and baryons in MW halos: defining where baryons dictate heat transfer
• Simulating the Carbon Footprint of Galactic Halos
• ETHOS - an effective theory of structure formation: formation of the first haloes and their stars
• Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
• Realistic synthetic integral field spectroscopy with RealSim-IFS
• The IllustrisTNG Simulations: Public Data Release
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• Redshift Space Distortion of 21cm line at 1<z<5 with Cosmological Hydrodynamic Simulations
• Morphology of galaxies with quiescent recent assembly history in a Lambda-CDM universe
• Galaxies with Shells in the Illustris Simulation: Metallicity Signatures
• NIHAO XXVI: Nature versus nurture, the Star Formation Main Sequence and the origin of its scatter
• Variations in the slope of the resolved star-forming main sequence: a tool for constraining the mass of star-forming regions
• Cosmic Ray Driven Outflows in an Ultraluminous Galaxy
• Detecting the halo heating from AGN feedback with ALMA
• Dynamical modelling and origin of gas turbulence in z $\sim$ 4.5 galaxies
• Non-parametric Morphologies of Mergers in the Illustris Simulation
• The metallicity and star formation activity of long gamma-ray burst hosts for z$<$3: insights from the Illustris simulation
• Extreme Spheres: Counts-in-cells for 21cm intensity mapping
• Differential rotation of the halo traced by the K-giant stars
• Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies
• The Host Galaxies of Radio AGN: New Views from Combining LoTSS and MaNGA Observations
• On the Cosmic Evolution of Fe/Mg in QSO Absorption Line Systems
• Simultaneous Dependence of Matter Clustering on Scale and Environment
• Cosmological interpretation of the color-magnitude diagrams of galaxy clusters
• Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
• A field-level emulator for modeling baryonic effects across hydrodynamic simulations
• Can HI 21 cm line trace the Missing Baryons in the Filamentary Structures?
• Cosmological Simulation of Galaxy Groups and Clusters-I: Global Effect of Feedback from Active Galactic Nuclei
• The Tully-Fisher relation from SDSS-MaNGA: Physical causes of scatter and variation at different radii
• How do baryonic effects on the cosmic matter distribution vary with scale and local density environment?
• Expanding on the Fundamental Metallicity Relation in Dwarf Galaxies with MUSE
• Where binary neutron stars merge: predictions from IllustrisTNG
• The Direct-Method Oxygen Abundance of Typical Dwarf Galaxies at Cosmic High-Noon
• Physical Origins of Outflowing Cold Clouds in Local Star-forming Dwarf Galaxies
• Host Galaxy Demographics Of Individually Detectable Supermassive Black-hole Binaries with Pulsar Timing Arrays
• Observational Diagnostics of Gas Flows: Insights from Cosmological Simulations
• Early-type galaxy density profiles from IllustrisTNG: III. Effects on outer kinematic structure
• The feasibility of constraining DM interactions with high-redshift observations by JWST
• Variations of the ISM Compactness Across the Main Sequence of Star-Forming Galaxies: Observations and Simulations
• HELLO project: High-$z$ Evolution of Large and Luminous Objects
• Revisiting the Relationship between the Long GRB Rate and Cosmic Star Formation History Based on a Large Swift Sample
• Anatomy of galactic star formation history: Roles of different modes of gas accretion, feedback, and recycling
• FIRST J1419+3940 as the First Observed Radio Flare from a Neutron Star Merger
• Premature supermassive black hole mergers in cosmological simulations of structure formation
• Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies
• Measuring Resolved Star Formation Histories from High-Precision Color-Magnitude Diagrams with StarFormationHistories.jl
• Galaxy formation with wave/fuzzy dark matter: The core-halo structure and the solitonic imprint
• IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
• An H$\alpha$ kinematic survey of the $Herschel$ Reference Survey -- I. Fabry-Perot observations with the 1.93m telescope at OHP
• IllustrisTNG in the HSC-SSP: No Shortage of Thin Disk Galaxies in TNG50
• The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
• Jellyfish galaxies with the IllustrisTNG simulations -- Supermassive black hole activity in dense environments with ram-pressure stripped satellites
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• Stirring the cosmic pot: how black hole feedback shapes the matter power spectrum in the Fable simulations
• The signature of galaxy formation models in the power spectrum of the hydrogen 21cm line during reionization
• The AIDA-TNG project: dark matter profiles and concentrations in alternative dark matter models
• Signatures of AGN induced metal loss in the stellar population
• Interactions among intermediate redshift galaxies. The case of SDSSJ134420.86+663717.8
• Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations IV. Testing warm dark matter cosmologies with galaxy scaling relations: A joint simulation-observation study using DREAMS simulations
• Boosting (In)direct Detection of Dark Matter
• Structure Formation under Inelastic Two-Component Dark Matter: Halo Statistics and Matter Power Spectra in the High-$z$ Universe
• Dwarf Galaxy Number Counts within 25 Mpc: Predictions from Local Group Analogues in TNG50