Simba: Cosmological Simulations with Black Hole Growth and Feedback

Abstract

We introduce the Simba simulations, the next generation of the Mufasa cosmological galaxy formation simulations run with Gizmo's meshless finite mass hydrodynamics. Simba includes updates to Mufasa's sub-resolution star formation and feedback prescriptions, and introduces black hole growth via the torque-limited accretion model of Anglés-Alcázar et al. (2017) from cold gas and Bondi accretion from hot gas, along with black hole feedback via kinetic bipolar outflows and X-ray energy. Ejection velocities are taken to be ~10^3 km/s at high Eddington ratios, increasing to ~8000 km/s at Eddington ratios below 2%, with a constant momentum input of 20L/c. Simba further includes an on-the-fly dust production, growth, and destruction model. Our Simba run with (100 Mpc/h)^3 and 1024^3 gas elements reproduces numerous observables, including galaxy stellar mass functions at z=0-6, the stellar mass--star formation rate main sequence, HI and H2 fractions, the mass-metallicity relation at z=0 and z=2, star-forming galaxy sizes, hot gas fractions in massive halos, and z=0 galaxy dust properties. However, Simba also yields an insufficiently sharp truncation of the z=0 mass function, and too-large sizes for low-mass quenched galaxies. We show that Simba's jet feedback is primarily responsible for quenching massive galaxies.

arXiv comment25 pages, MNRAS accepted, some new figures

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• MIGHTEE: Deep 1.4 GHz Source Counts and the Sky Temperature Contribution of Star Forming Galaxies and Active Galactic Nuclei
• From Nuclear to Circumgalactic: Zooming in on AGN-Driven Outflows at z~2.2 with SINFONI
• Arkenstone I: A Novel Method for Robustly Capturing High Specific Energy Outflows In Cosmological Simulations
• High Molecular-Gas to Dust Mass Ratios Predicted in Most Quiescent Galaxies
• Finding universal relations in subhalo properties with artificial intelligence
• Gravitational imaging through a triple source plane lens: revisiting the $\Lambda$CDM-defying dark subhalo in SDSSJ0946+1006
• 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
• Breaking baryon-cosmology degeneracy with the electron density power spectrum
• Physics of ULIRGs with MUSE and ALMA: The PUMA project I. Properties of the survey and first MUSE data results
• Massive Black Hole Mergers with Orbital Information: Predictions from the ASTRID Simulation
• High-resolution synthetic UV-submm images for simulated Milky Way-type galaxies from the Auriga project
• The hot circumgalactic medium in the eROSITA All-Sky Survey II. Scaling relations between X-ray luminosity and galaxies' mass
• Formation and Morphology of the First Galaxies in the Cosmic Morning
• Can Cosmological Simulations Reproduce the Spectroscopically Confirmed Galaxies Seen at $z\ge 10$?
• MIGHTEE-HI: Evolution of HI scaling relations of star-forming galaxies at $z<0.5$
• {\sc mirkwood:} Fast and Accurate SED Modeling Using Machine Learning
• Quenching Timescales in the IllustrisTNG Simulation
• The Impact of Type Ia Supernovae in Quiescent Galaxies: II. Energetics and Turbulence
• Star Formation Suppresion by Tidal Removal of Cold Molecular Gas from an Intermediate-Redshift Massive Post-Starburst Galaxy
• Inferring the impact of feedback on the matter distribution using the Sunyaev Zel'dovich effect: Insights from CAMELS simulations and ACT+DES data
• Regulation of Star Formation by a Hot Circumgalactic Medium
• Stellar feedback-regulated black hole growth: driving factors from nuclear to halo scales
• 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
• Deciphering the imprint of AGN feedback in Seyfert galaxies: Nuclear-scale molecular gas deficits
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• CO Emission, Molecular Gas, and Metallicity in Main-Sequence Star-Forming Galaxies at $z\sim 2.3$
• Accurate predictions from small boxes: variance suppression via the Zel'dovich approximation
• On the relative effect of nodes and filaments of the cosmic web on the quenching of galaxies and the orientation of their spin
• Too dense to go through: The importance of low-mass clusters for satellite quenching
• IQ Collaboratory II: The Quiescent Fraction of Isolated, Low Mass Galaxies Across Simulations and Observations
• The BPT Diagram in Cosmological Galaxy Formation Simulations: Understanding the Physics Driving Offsets at High-Redshift
• The baryonic Tully-Fisher relation in the Simba simulation
• UV to submillimetre luminosity functions of TNG50 galaxies
• Probing the $z\gtrsim 6$ quasars in a universe with IllustrisTNG physics: Impact of gas-based black hole seeding models
• Rivers of Gas I.: Unveiling The Properties of High Redshift Filaments
• Impact of AGN feedback on galaxies and their multiphase ISM across cosmic time
• Deep Investigation of Neutral Gas Origins (DINGO): HI stacking experiments with early science data
• The impact of AGN-driven winds on physical and observable galaxy sizes
• How gas flows shape the stellar-halo mass relation in the EAGLE simulation
• Mixing matters
• Global Simulations of Galactic Discs: Violent Feedback from Clustered Supernovae during Bursts of Star Formation
• How Well Can We Measure Galaxy Dust Attenuation Curves? The Impact of the Assumed Star-Dust Geometry Model in SED Fitting
• Characterising the intra-cluster light in The Three Hundred simulations
• The evolution of the mass-metallicity relations from the VANDELS survey and the GAEA Semi-Analytic model
• Towards a consistent framework of comparing galaxy mergers in observations and simulations
• Redshift-dependent galaxy formation efficiency at $z=5-13$ in the FirstLight simulations
• A New Model For Including Galactic Winds in Simulations of Galaxy Formation I: Introducing the Physically Evolved Winds (PhEW) Model
• On the Environments of Giant Radio Galaxies
• X-ray metal line emission from the hot circumgalactic medium: probing the effects of supermassive black hole feedback
• Probing the Circum-Galactic Medium with Fast Radio Bursts: Insights from the CAMELS Simulations
• Density modulated star formation efficiency: implications for the observed abundance of ultra-violet luminous galaxies at z>10
• The Stellar Mass Function in CANDELS and Frontier Fields: the build-up of low mass passive galaxies since z~3
• Dust temperature uncertainties hamper the inference of dust and molecular gas masses from the dust continuum emission of quiescent high-redshift galaxies
• PRIYA: A New Suite of Lyman-alpha Forest Simulations for Cosmology
• VLA Legacy Survey of Molecular Gas in Massive Star-forming Galaxies at High Redshift
• The Interaction between AGN and Starburst Activity in the Circumnuclear Region of NGC 7469 as Viewed with JWST
• An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS Field (AS2COSPEC): Physical Properties of z=2-5 Ultra- and Hyperluminous Infrared Galaxies
• How AGN feedback drives the size growth of the first quasars
• The SZ flux-mass ($Y$-$M$) relation at low halo masses: improvements with symbolic regression and strong constraints on baryonic feedback
• Augmenting astrophysical scaling relations with machine learning: application to reducing the Sunyaev-Zeldovich flux-mass scatter
• A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
• Unveiling hidden active nuclei in MaNGA star-forming galaxies with HeII$\lambda$4686 line emission
• The Origin of the Dust Extinction Curve in Milky Way-like Galaxies
• GLASS: Generator for Large Scale Structure
• The Cosmic Baryon Partition between the IGM and CGM in the SIMBA Simulations
• Cosmic evolution of radio-AGN feedback: confronting models with data
• Effects of Active Galactic Nucleus Feedback on Cold Gas Depletion and Quenching of Central Galaxies
• From EMBER to FIRE: predicting high resolution baryon fields from dark matter simulations with Deep Learning
• Atomic Gas Scaling Relations of Star-forming Galaxies at $z\approx 1$
• No Tension: JWST Galaxies at $z>10$ Consistent with Cosmological Simulations
• Molecular Gas Reservoirs in Massive Quiescent Galaxies at $\mathrm{z}\sim 0.7$ Linked to Late Time Star Formation
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• Evidence that Shocks Destroy Small PAH Molecules in Low-luminosity Active Galactic Nuclei
• AGN feedback in action in the molecular gas ring of the Seyfert galaxy NGC7172
• DEVILS: Cosmic evolution of SED-derived metallicities and their connection to star-formation histories
• Simba: The average properties of the circumgalactic medium of $2\le z\le 3$ quasars are determined primarily by stellar feedback
• HIFlow: Generating Diverse HI Maps and Inferring Cosmology while Marginalizing over Astrophysics using Normalizing Flows
• The CGM at Cosmic Noon with KCWI: Outflows from a Star-forming Galaxy at z=2.071
• Investigating The Growing Population of Massive Quiescent Galaxies at Cosmic Noon
• Understanding the relation between thermal Sunyaev-Zeldovich decrement and halo mass using the SIMBA and TNG simulations
• Cool circumgalactic gas in galaxy clusters: connecting the DESI legacy imaging survey and SDSS DR16 MgII absorbers
• The dark side of galaxy stellar populations I: The stellar-to-halo mass relation and the velocity dispersion - halo mass relation
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• Atomic Gas Dominates the Baryonic Mass of Star-forming Galaxies at $z\approx 1.3$
• Atomic and molecular gas from the epoch of reionization down to redshift 2
• Machine Learning methods to estimate observational properties of galaxy clusters in large volume cosmological N-body simulations
• High-resolution synthetic UV-submm images for Milky Way-mass simulated galaxies from the ARTEMIS project
• The bivariate gas-stellar mass distributions and the mass functions of early- and late-type galaxies at $z\sim 0$
• The Three Hundred: Cluster Dynamical States and Relaxation Time Scale
• KURVS: The outer rotation curve shapes and dark matter fractions of $z\sim 1.5$ star-forming galaxies
• Nonparametric galaxy morphology from UV to submm wavelengths
• A Framework for Modeling Polycyclic Aromatic Hydrocarbon Emission in Galaxy Evolution Simulations
• The atomic-to-molecular hydrogen transition in the TNG50 simulation: Using realistic UV fields to create spatially resolved HI maps
• On the redshift evolution of the baryon and gas fraction in simulated groups and clusters of galaxies
• The CGM${}^2$ Survey: Quenching and the Transformation of the Circumgalactic Medium
• Impact of gas spin and Lyman-Werner flux on black hole seed formation in cosmological simulations: implications for direct collapse
• Baryonic mass budgets for haloes in the EAGLE simulation, including ejected and prevented gas
• The FLAMINGO project: Baryon effects on the matter power spectrum
• MIGHTEE-HI: The relation between the HI gas in galaxies and the cosmic web
• Predicting sub-millimeter flux densities from global galaxy properties
• Black hole -- galaxy scaling relations in FIRE: the importance of black hole location and mergers
• A hidden population of massive black holes in simulated dwarf galaxies
• Exploring over 700 massive quiescent galaxies at z = 2-7: Demographics and stellar mass functions
• In pursuit of giants: II. Evolution of dusty quiescent galaxies over the last six billion years from the hCOSMOS survey
• Infrared luminosity functions and dust mass functions in the EAGLE simulation
• Neural networks as optimal estimators to marginalize over baryonic effects
• AGN Feedback in Groups and Clusters of Galaxies
• Limits on non-canonical heating and turbulence in the intergalactic medium from the low redshift Lyman-alpha forest
• Effects of Spatial Discretization in Lyman-alpha Line Radiation Transfer Simulations
• SIMBA-C: An updated chemical enrichment model for galactic chemical evolution in the SIMBA simulation
• Photometric Objects around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. I. Methods
• Efficient long-range AGN feedback affects the low redshift Lyman-$\alpha$ forest
• The NEWFIRM HETDEX Survey: Photometric Catalog and a Conservative Sample of Massive Quiescent Galaxies at z=3-5 over 17.5 deg^2 in the SHELA Field
• Spherical accretion: Bondi, Michel and rotating black holes
• Modelling the accretion and feedback of supermassive black hole binaries in gas-rich galaxy mergers
• Comparisons between fast algorithms for the continuous wavelet transform and applications in cosmology: the 1D case
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• Reading the tea leaves in the $M_{\mathrm{bh}}$-$M_{\ast ,\mathrm{sph}}$ and $M_{\mathrm{bh}}$-$R_{\mathrm{e},\mathrm{sph}}$ diagrams: dry and gaseous mergers with remnant angular momentum
• The Impact of Outflows driven by Active Galactic Nuclei on Metals in and around Galaxies
• The importance of stochasticity in determining galaxy emissivities and UV LFs during cosmic dawn and reionization
• The JCMT SCUBA-2 Survey of the James Webb Space Telescope North Ecliptic Pole Time-Domain Field
• Detecting Galaxy Groups and AGNs populating the local Universe in the eROSITA era
• ALMACAL IX: multi-band ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background
• EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies
• The redshift evolution of the baryonic Tully-Fisher relation in Simba
• MIGHTEE-HI: The HI mass-stellar mass relation over the last billion years
• The properties of wind and jet from a super-Eddington accretion flow around a supermassive black hole
• Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
• AGN accretion and black hole growth across compact and extended galaxy evolution phases
• Cosmological simulations of quasar fueling to sub-parsec scales using Lagrangian hyper-refinement
• The low redshift Lyman-$\alpha$ Forest as a constraint for models of AGN feedback
• Quantifying Baryonic Feedback on Warm-Hot Circumgalactic Medium in CAMELS Simulations
• On the origin of star formation quenching in massive galaxies at $z\gtrsim 3$ in the cosmological simulations IllustrisTNG
• Unraveling the interplay between SIDM and baryons in MW halos: defining where baryons dictate heat transfer
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• The AGORA High-resolution Galaxy Simulations Comparison Project. VI. Similarities and Differences in the Circumgalactic Medium
• Multifield Cosmology with Artificial Intelligence
• An ALMA view of 11 Dusty Star Forming Galaxies at the peak of Cosmic Star Formation History
• Observational Evidence for Large-Scale Gas Heating in a Galaxy Protocluster at z=2.30
• The intrinsic SFRF and sSFRF of galaxies: comparing SDSS observation with IllustrisTNG simulation
• The Three Hundred Project: the evolution of physical baryon profiles
• Relic galaxy analogues in Illustris TNG50: the formation pathways of surviving red nuggets in a cosmological simulation
• The galaxy-halo connection of disc galaxies over six orders of magnitude in stellar mass
• Environmental dependence of the mass-metallicity relation in cosmological hydrodynamical simulations
• The changing circumgalactic medium over the last 10 Gyr I: physical and dynamical properties
• Real and counterfeit cores: how feedback expands halos and disrupts tracers of inner gravitational potential in dwarf galaxies
• Data Compression and Inference in Cosmology with Self-Supervised Machine Learning
• Do galaxies die? Different views from simulations and observations in the Local Universe
• The IllustrisTNG Simulations: Public Data Release
• Revisiting the [C II]${}_{158\mu \text{m}}$ line-intensity mapping power spectrum from the EoR using non-uniform line-luminosity scatter
• The Stellar Mass - Black Hole Mass Relation at $z\sim 2$ Down to ${\mathcal{M}}_{\mathrm{BH}}\sim 10^7{M}_{\odot }$ Determined by HETDEX
• Interacting galaxies in the IllustrisTNG simulations -- V: Comparing the influence of star-forming vs. passive companions
• Determining AGN luminosity histories using present-day outflow properties: a neural-network based approach
• Reionization with Simba: How much does astrophysics matter in modeling cosmic reionization?
• Spatially offset black holes in the Horizon-AGN simulation and comparison to observations
• Formation of S0s in extreme environments III: the role of environment in the formation pathways
• QSOFEED: The relationship between star formation and AGN Feedback
• The observed cosmic star formation rate density has an evolution which resembles a Γ(a, bt) distribution and can be described successfully by only 2 parameters
• JWST's PEARLS: resolved study of the stellar and dust components in starburst galaxies at cosmic noon
• The Obsidian model: Three regimes of black hole feedback
• Outflow densities and ionisation mechanisms in the NLRs of the prototypical Seyfert galaxies NGC 1068 and NGC 4151
• Nonparametric galaxy morphology from stellar and nebular emission with the CALIFA sample
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. III. Accurate Measurement of Galaxy Stellar Mass Function with the Aid of Cosmological Redshift Surveys
• Evidence for non-merger co-evolution of galaxies and their supermassive black holes
• Impact of gas based seeding on supermassive black hole populations at $z\ge 7$
• The stellar mass function and evolution of the density profile of galaxy clusters from the Hydrangea simulations at $0<z<1.5$
• Dynamical friction and evolution of black holes in cosmological simulations: a new implementation in OpenGadget3
• Entrainment of Hot Gas into Cold Streams: The Origin of Excessive Star-formation Rates at Cosmic Noon
• Cosmology with Persistent Homology: a Fisher Forecast
• ART${}^2$: A 3D Parallel Multi-wavelength Radiative Transfer Code for Continuum and Atomic and Molecular Lines
• Hybrid analytic and machine-learned baryonic property insertion into galactic dark matter haloes
• The effects of local stellar radiation and dust depletion on non-equilibrium interstellar chemistry
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• Excitation and acceleration of molecular outflows in LIRGs: The extended ESO 320-G030 outflow on 200-pc scales
• The Physical Origin of the Mass-Size Relation and Its Scatter of Disk Galaxies
• X-raying CAMELS: Constraining Baryonic Feedback in the Circum-Galactic Medium with the CAMELS simulations and eRASS X-ray Observations
• The frequency of very young galaxies in the local Universe: II. The view from SDSS spectra
• Modelling the star-formation activity and ionizing properties of high-redshift galaxies
• The Manhattan Suite: Accelerated galaxy evolution in the early Universe
• Percent-level constraints on baryonic feedback with spectral distortion measurements
• Synthesizing Stellar Populations in South Pole Telescope Galaxy Clusters: I. Ages of Quiescent Member Galaxies at 0.3 < z < 1.4
• Supermassive black holes in merger-free galaxies have higher spins which are preferentially aligned with their host galaxy
• Fisher matrix for the one-loop galaxy power spectrum: measuring expansion and growth rates without assuming a cosmological model
• ERGO-ML: Comparing IllustrisTNG and HSC galaxy images via contrastive learning
• The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
• Simulations of black hole fueling in isolated and merging galaxies with an explicit, multiphase ISM
• Modelling the galaxy-halo connection with semi-recurrent neural networks
• Correlated orientations of the axes of large quasar groups on Gpc scales
• A multi-tracer empirically-driven approach to line-intensity mapping lightcones
• Unravelling the physics of multiphase AGN winds through emission line tracers
• GalICS 2.1: a new semianalytic model for cold accretion, cooling, feedback and their roles in galaxy formation
• Forecasting the success of the WEAVE Wide-Field Cluster Survey on the extraction of the cosmic web filaments around galaxy clusters
• Rapidly quenched galaxies in the Simba cosmological simulation and observations
• The Shape and Scatter of The Galaxy Main Sequence for Massive Galaxies at Cosmic Noon
• No evidence for excess AGN activity in recently quenched massive galaxies at cosmic noon
• ERGO-ML: Towards a robust machine learning model for inferring the fraction of accreted stars in galaxies from integral-field spectroscopic maps
• The fate of the interstellar medium in early-type galaxies. III. The mechanism of ISM removal and quenching of star formation
• The bright end of the galaxy luminosity function at $z\simeq 7$ from the VISTA VIDEO survey
• The THESAN-ZOOM project: Population III star formation continues until the end of reionization
• Baryonic Imprints on DM Halos: The concentration-mass relation in the CAMELS simulations
• The evolution of cosmic ray electrons in the cosmic web: seeding by AGN, star formation and shocks
• HI intensity mapping with the MIGHTEE survey: power spectrum estimates
• Active galactic nuclei jets simulated with smoothed particle hydrodynamics
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines II. [C II], [O I], [O III], [N II] and [N III] up to z=6
• A Dusty Dawn: Galactic Dust Buildup at $z\gtrsim 5$
• Impact of H${}_2$-driven star formation and stellar feedback from low-enrichment environments on the formation of spiral galaxies
• MIND THE GAP: Is The Too Big To Fail Problem Resolved?
• Testing Galaxy Formation Simulations with Damped Lyman-$\alpha$ Abundance and Metallicity Evolution
• SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
• Galaxy And Mass Assembly: Group and field galaxy morphologies in the star-formation rate - stellar mass plane
• Formation of a barred galaxy in a major merger: The role of AGN feedback
• Halo Scaling Relations and Hydrostatic Mass Bias in the Simba Simulation From Realistic Mock X-ray Catalogues
• FORECAST: a flexible software to forward model cosmological hydrodynamical simulations mimicking real observations
• First Light And Reionisation Epoch Simulations (FLARES) XII: The consequences of star-dust geometry on galaxies in the EoR
• The Physical Nature of Circumgalactic Medium Absorbers in Simba
• An Orientation Bias in Observations of Submillimetre Galaxies
• Inconsistencies arising from the coupling of galaxy formation sub-grid models to Pressure-Smoothed Particle Hydrodynamics
• Progenitor-mass-dependent yields amplify intrinsic scatter in dwarf-galaxy elemental abundance ratios
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• CGM${}^2$ $+$ CASBaH: The Mass Dependence of H~I Ly$\alpha$-Galaxy Clustering and the Extent of the CGM
• A Comparison of Star-Forming Clumps and Tidal Tails in Local Mergers and High Redshift Galaxies
• The extent of intergalactic metal enrichment from galactic winds during the Cosmic Dawn
• The Nature and Evolution of Early Massive Quenched Galaxies in the Simba-C Simulation
• Painting baryons onto N-body simulations of galaxy clusters with image-to-image deep learning
• Questioning Planck-selected star-forming high-redshift galaxy protoclusters and their fate
• Bringing faint active galactic nuclei (AGNs) to light: a view from large-scale cosmological simulations
• Cosmic Sands: The Origin of Dusty, Star-forming Galaxies in the Epoch of Reionization
• The hot gas mass fraction in halos. From Milky Way-like groups to massive clusters
• Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies
• The first GLIMPSE of the faint galaxy population at Cosmic Dawn with JWST: The evolution of the ultraviolet luminosity function across z~9-15
• Cosmic evolution of radio-excess AGNs in quiescent and star-forming galaxies across $0<z<4$
• How does the radio enhancement of broad absorption line quasars relate to colour and accretion rate?
• PRIMER & JADES reveal an abundance of massive quiescent galaxies at 2 < z < 5
• The impact of assembly history on the X-ray detectability of halos. From galaxy groups to galaxy clusters
• Modelling the evolution and influence of dust in cosmological simulations that include the cold phase of the interstellar medium
• ALMACAL. XI. Over-densities as signposts to proto-clusters? A cautionary tale
• Hydrodynamic simulations of the Disk of Gas Around Supermassive black holes (HDGAS) -I; Molecular Gas Dynamics
• The Star-Formation Properties of the Observed and Simulated AGN Universe: BAT vs EAGLE
• The connection between stellar mass, age and quenching timescale in massive quiescent galaxies at $z\simeq 1$
• Tracing the evolutionary pathways of dust and cold gas in high-z quiescent galaxies with SIMBA
• Evolution of the grain size distribution in Milky Way-like galaxies in post-processed IllustrisTNG simulations
• Cosmic metal invaders: Intergalactic OVII as a tracer of the warm-hot intergalactic medium within cosmic filaments in the EAGLE simulation
• Simultaneous Dependence of Matter Clustering on Scale and Environment
• Hybrid-chimes: A model for radiative cooling and the abundances of ions and molecules in simulations of galaxy formation
• Mesh-free hydrodynamics in PKDGRAV3 for galaxy formation simulations
• COALAS III: The ATCA CO(1-0) look at the growth and death of H$\alpha$ emitters in the Spiderweb protocluster at z=2.16
• An environment-dependent halo mass function as a driver for the early quenching of $z\ge 1.5$ cluster galaxies
• Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
• AGN and Star Formation at Cosmic Noon: Comparison of Data to Theoretical Models
• Revealing the Galaxy-Halo Connection Through Machine Learning
• Average X-ray properties of galaxy groups. From Milky Way-like halos to massive clusters
• A common origin for the Fundamental Plane of quiescent and star-forming galaxies in the EAGLE simulations
• Disk galaxies are self-similar: the universality of the HI-to-Halo mass ratio for isolated disks
• Accretion onto supermassive and intermediate mass black holes in cosmological simulations
• Learning the Universe: Cosmological and Astrophysical Parameter Inference with Galaxy Luminosity Functions and Colours
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. -- III. Stellar metallicity drivers in MaNGA and TNG50
• Measuring the baryonic Tully-Fisher relation below the detection threshold
• Can the Low Redshift Lyman Alpha Forest Constrain AGN Feedback Models?
• Constraints on galactic outflows from the metallicity-stellar mass-SFR relation of EAGLE simulation and SDSS galaxies
• The origin of correlations between mass, metallicity and morphology in galaxies from the EAGLE simulation
• Formation and fate of low metallicity stars in IllustrisTNG50
• Surveying the onset and evolution of supermassive black holes at high-z with AXIS
• Boundless baryons: how diffuse gas contributes to anisotropic tSZ signal around simulated Three Hundred clusters
• Star formation history and transition epoch of cluster galaxies based on the Horizon-AGN simulation
• ASymba: HI global profile asymmetries in the Simba simulation
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations -- I. Constraining physical processes in local star-forming galaxies
• Validating the clustering predictions of empirical models with the FLAMINGO simulations
• An exploration of the properties of cluster profiles for the thermal and kinetic Sunyaev-Zel'dovich effects
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• COSMOS Brightest Group Galaxies -- III: Evolution of stellar ages
• Quantifying Observational Projection Effects with a Simulation-based hot CGM model
• On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn
• Detection of the Mass-Dependent Dual-Type Transition of Galaxy Spins in IllustrisTNG Simulations
• Black hole feedback and the evolution of massive early-type galaxies
• Searching for the shadows of giants II: the effect of local ionisation on the Lyman-$\alpha$ absorption signatures of protoclusters at redshift $z\sim 2.4$
• Hyenas: X-ray Bubbles and Cavities in the Intra-Group Medium
• The Dark Matter Halos of HI Selected Galaxies
• PAC in DESI. I. Galaxy Stellar Mass Function into the $10^6{\mathrm{M}}_{\odot }$ Frontier
• Studying the Warm Hot Intergalactic Medium in emission: a reprise
• A power spectrum approach to the search for Axion-like Particles from resolved galaxy clusters using CMB as a backlight
• The Three Hundred project: Estimating the dependence of gas filaments on the mass of galaxy clusters
• Cosmology from one galaxy in a void?
• Distinguishing AGN Feedback Models with the Thermal Sunyaev-Zel'dovich Effect
• Expanding on the Fundamental Metallicity Relation in Dwarf Galaxies with MUSE
• 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
• On the connection between AGN radiative feedback and massive black hole spin
• Galaxy And Mass Assembly (GAMA) Survey: The Merging Potential of Brightest Group Galaxies
• The quasi-adiabatic relaxation of haloes in the IllustrisTNG and EAGLE cosmological simulations
• HSC-CLAUDS survey: The star formation rate functions since z ~ 2 and comparison with hydrodynamical simulations
• On the detectability of massive black hole merger eventsby LISA
• Field-level simulation-based inference with galaxy catalogs: the impact of systematic effects
• How do baryonic effects on the cosmic matter distribution vary with scale and local density environment?
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• Resolution criteria to avoid artificial clumping in Lagrangian hydrodynamic simulations with a multi-phase interstellar medium
• When relics were made: vigorous stellar rotation and low dark matter content in the massive ultra-compact galaxy GS-9209 at z=4.66
• Improving Black Hole Accretion Treatment in Hydrodynamical Simulations
• X-ray Absorption Lines in the Warm-Hot Intergalactic Medium: Probing Chandra observations with the CAMEL simulations
• Correlations between mass, stellar kinematics and gas metallicity in EAGLE galaxies
• The formation of compact massive relic galaxies in MOND
• The impact of the cosmological constant on past and future star formation
• Studying galaxy cluster morphological metrics with Mock-X
• Velocity dispersion vs cluster mass: a new scaling law with The Three Hundred clusters
• Disparate Effects of Circumgalactic Medium Angular Momentum in IllustrisTNG and SIMBA
• 2mm Observations and the Search for High-Redshift Dusty Star-forming Galaxies
• RUBIES spectroscopically confirms the high number density of quiescent galaxies from $2<\mathbf{z}<5$
• Quantifying the intrinsic variability due to randomness of the Auriga galaxy formation model
• A Diffused Background from Axion-like Particles in the Microwave Sky
• ALMA 1.1mm Observations of a Conservative Sample of High Redshift Massive Quiescent Galaxies in SHELA
• The relationship between cluster environment and molecular gas content of star-forming galaxies in the EAGLE simulation
• The Three Hundred Project: Mapping The Matter Distribution in Galaxy Clusters Via Deep Learning from Multiview Simulated Observations
• $\text{slick}$: Modeling a Universe of Molecular Line Luminosities in Hydrodynamical Simulations
• HELLO project: High-$z$ Evolution of Large and Luminous Objects
• Star-forming and Quiescent Central Galaxies Cluster Similarly: Implications for the Galaxy-Halo Connection
• Cosmological Simulation of Galaxy Groups and Clusters-II: Studying Different Modes of Feedback through X-ray Observations
• The evolution of supermassive blackhole mass--bulge mass relation by a semi-analytic model, ${\nu }^2$GC
• NeutralUniverseMachine: How Filaments and Dark Matter Halo Influence the Galaxy Cold Gas Content
• Empirical Dust Attenuation Model Leads to More Realistic UVJ Diagram for TNG100 Galaxies
• Astrophysics with the Laser Interferometer Space Antenna
• Mitigating baryon feedback bias in cosmic shear through a theoretical error covariance in the matter power spectrum
• Inpainting hydrodynamical maps with deep learning
• MIGHTEE-HI: The direct detection of neutral hydrogen in galaxies at $z>0.25$
• COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase
• The JWST EXCELS Survey: gas-phase metallicity evolution at 2 < z < 8
• A rising tide: Intrinsic alignments since the turn of the millennium
• COSMOS2020: Disentangling the Role of Mass and Environment in Star Formation Activity of Galaxies at $0.4<z<4$
• Global Preventive Feedback of Powerful Radio Jets on Galaxy Formation
• Modelling the mass accretion histories of dark matter haloes using a Gamma formalism
• Measuring Galaxy Asymmetries in 3D
• Measurements of the angular momentum-mass relations in the Simba simulation
• The global energetics of radio AGN kinetic feedback in the local universe
• First Light and Reionisation Epoch Simulations (FLARES) X: Environmental Galaxy Bias and Survey Variance at High Redshift
• DESI Mock Challenge: Constructing DESI galaxy catalogues based on FastPM simulations
• Estimation of the Galaxy Quenching Rate in the Illustris Simulation
• The environments of the radio galaxy population in SIMBA
• Recent Observations of the Rotation of Distant Galaxies and the Implication for Dark Matter
• Probing the Epoch of Reionization using synergies of line intensity mapping
• Red riding on hood: Exploring how galaxy colour depends on environment
• CO(1--0) imaging reveals 10-kiloparsec molecular gas reservoirs around star-forming galaxies at high redshift
• Intrinsic mass-richness relation of clusters from THE THREE HUNDRED hydrodynamic simulations
• Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
• Predictive uncertainty on improved astrophysics recovery from multifield cosmology
• Identifying Galaxy Cluster Mergers with Deep Neural Networks using Idealized Compton-y and X-ray maps
• Intertwined Formation of ${\mathrm{H}}_2$, Dust, and Stars in Cosmological Simulations
• The Three Hundred-NIKA2 Sunyaev-Zeldovich Large Program twin samples: Synthetic clusters to support real observations
• The ALPINE-ALMA [CII] Survey: Unveiling the baryon evolution in the ISM of $z\sim 5$ star-forming galaxies
• Cross-correlation between soft X-rays and galaxies A new benchmark for galaxy evolution models
• Measuring Resolved Star Formation Histories from High-Precision Color-Magnitude Diagrams with StarFormationHistories.jl
• Cloudy-Maraston: Integrating nebular continuum and line emission with the Maraston stellar population synthesis models
• The THREEHUNDRED project: the effect of baryon processes at galaxy cluster scale
• Modeling submillimeter galaxies in cosmological simulations: Contribution to the cosmic star formation density and predictions for future surveys
• The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
• Retrieving the hot circumgalactic medium physics from the X-ray radial profile from eROSITA with an IlustrisTNG-based forward model
• Jellyfish galaxies with the IllustrisTNG simulations -- Supermassive black hole activity in dense environments with ram-pressure stripped satellites
• pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population
• Modelling the selection of galaxy groups with end to end simulations
• syren-baryon: Analytic emulators for the impact of baryons on the matter power spectrum
• LATIS: A Sample of IGM-selected Protoclusters and Protogroups at $z\sim 2.5$
• Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
• First Light And Reionisation Epoch Simulations (FLARES) XVI: Size Evolution of Massive Dusty Galaxies at Cosmic Dawn from UV to IR
• IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
• A systematic study of AGN feedback in a disk galaxy I: global overview
• The Qz5 Survey (I): How the HI Mass Density of the Universe Evolves With Cosmic Time
• Impact of cosmic web on the properties of galaxies in IllustrisTNG simulations
• TODDLERS: A New UV to Millimeter Emission Library for Star-Forming Regions. II. Star Formation Rate Indicators Using Auriga Zoom Simulations
• The Dawn of Black Holes
• Large-scale geometry and topology of gas fields: Effects of AGN and stellar feedback
• Neutral hydrogen lensing simulations in the Hubble Frontier Fields
• The PAU Survey: The quasar UV and Ly$\alpha$ luminosity functions at $2.7<z<5.3$
• Conditional Colour-Magnitude Distribution of Central Galaxies in Galaxy Formation Models
• The Three Hundred: $M_{sub}-V_{circ}$ relation
• Role of ionizing background on the non-thermal broadening inferred for the aligned absorbers
• Applying unsupervised learning to resolve evolutionary histories and explore the galaxy-halo connection in IllustrisTNG
• The Three Hundred Project hydrodynamical simulations: Hydrodynamical weak-lensing cluster mass biases and richnesses using different hydro models
• The stellar mass function of quiescent and star-forming galaxies and its dependence on morphology in COSMOS-Web
• Using dust to constrain dark matter models
• The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization
• The origin of galaxy colour bimodality in the scatter of the Stellar-to-Halo Mass Relation
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• Strong Evidence for Cosmic Ray-Supported $\sim$L${}^{\ast }$ Galaxy Halos via X-ray \& tSZ Constraints
• Cosmology with One Galaxy: Auto-Encoding the Galaxy Properties Manifold
• Applying a star formation model calibrated on high-resolution interstellar medium simulations to cosmological simulations of galaxy formation
• The Dependence of Dark Matter Halo Properties on the Morphology of Their Central Galaxies from Weak Lensing
• CLIMBER: Galaxy-Halo Connection Constraints from Next-Generation Surveys
• Born to be Starless: Revisiting the Missing Satellite Problem
• IllustrisTNG + Cosmic Rays with a Simple Transport Model: From Dwarfs to L${}^{\star }$ Galaxies
• AGN -- host galaxy photometric decomposition using a fast, accurate and precise deep learning approach
• The Three Hundred Project: deducing the stellar splashback structure of galaxy clusters from their orbiting profiles
• Constraining black hole-galaxy scaling relations from the large-scale clustering of Active Galactic Nuclei and implied mean radiative efficiency
• Extreme AGN feedback in the fossil galaxy group SDSSTG 4436
• The Three Hundred: Gas Properties Outside of Galaxy Cluster with the WHIM Contribution and Detection
• Galaxy cluster mass bias from projected mass maps: The Three Hundred-NIKA2 LPSZ twin samples
• Core to Cosmic Edge: SIMBA-C's New Take on Abundance Profiles in the Intragroup Medium at z = 0
• The impact of halo concentration on the Sunyaev Zel'dovich effect signal from massive galaxy clusters
• Emission Line Diagnostics for IMBHs in Dwarf Galaxies: Accounting for BH Seeding and ULX Excitation
• Prospects for studying the mass and gas in protoclusters with future CMB observations
• FLAMINGO: Galaxy formation and feedback effects on the gas density and velocity fields
• The breakBRD Breakdown: Using IllustrisTNG to Track the Quenching of an Observationally-Motivated Sample of Centrally Star-Forming Galaxies
• Identifying Halos in Cosmological Simulations with Continuous Wavelet Analysis: The 2D Case
• A MeerKAT study of a neutral hydrogen rich grouping of galaxies with megaparsec-scale filamentary-like structure
• SIGAME v3: Gas Fragmentation in Post-processing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling
• A 15 Mpc rotating galaxy filament at redshift z = 0.032
• Star-forming galaxies in the cosmic web in the last 11 Gyr
• Impact of cosmic web on galaxy properties and their correlations: Insights from Principal Component Analysis
• Kennicutt-Schmidt relation of galaxies over 13 billion years in the COLIBRE hydrodynamical simulations
• The AIDA-TNG project: dark matter profiles and concentrations in alternative dark matter models
• The FLAMINGO simulations data release
• Assessing the connection between galactic conformity and assembly-type bias
• An Observationally Driven Multifield Approach for Probing the Circum-Galactic Medium with Convolutional Neural Networks
• The impact of baryons on the sparsity of simulated galaxy clusters from The Three Hundred Project
• Simultaneously Modelling Dusty Star Forming Galaxies and Massive Quiescents: A Calibration Framework for Galaxy Formation Models
• HI asymmetries in spatially resolved SIMBA galaxies
• 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
• MIGHTEE-HI: The star-forming properties of HI selected galaxies
• Probabilistic Lagrangian bias estimators and the cumulant bias expansion
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• The Circumgalactic Medium from the CAMELS Simulations: Forecasting Constraints on Feedback Processes from Future Sunyaev-Zeldovich Observations
• X-ray stacking reveals average SMBH accretion properties of star-forming galaxies and their cosmic evolution over 4 <~ z <~ 7
• Inferring halo masses with Graph Neural Networks
• Predicting far-infrared maps of galaxies via machine learning techniques
• Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations
• Reconstructing galaxy star formation histories from COSMOS2020 photometry using simulation-based inference
• Mechanisms Affecting Galaxies Nearby and Environmental Trends (MAGNET)
• Extended Hernquist-Springel formalism for cosmic star formation
• Overmassive and Undermassive Massive Black Holes: The Role of Environment and Gravitational-Wave Recoils
• Reduced Gas Accretion onto Galaxies due to Effects of External Giant Radio Lobes
• Exploring the evolution of red and blue galaxies in different cosmic web environments using IllustrisTNG simulation
• Soft X-ray line emission from hot gas in intervening galaxy halos and diffuse gas in the cosmic web
• The Three Hundred Project: A fast semi-analytic model emulator of hydrodynamical galaxy cluster simulations
• Gamma Analytical Modeling Evolution (GAME) I: The physical implications of deriving the stellar mass functions from z=0 to z=8
• First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmic dawn
• One latent to fit them all: a unified representation of baryonic feedback on matter distribution
• Constraining Galaxy-Halo Connection Using Machine Learning
• Radio Galaxies in SIMBA: A MIGHTEE Comparison
• WALLABY Pilot Survey & ASymba: Comparing HI Detection Asymmetries to the SIMBA Simulation
• Emergence of red, star-forming galaxies (red misfits) in a ΛCDM universe
• CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform
• Effect of cosmic rays and ionizing radiation on observational ultraviolet plasma diagnostics in the circumgalactic medium
• A Hydro-Particle-Mesh Code for Efficient and Rapid Simulations of the Intracluster Medium
• Investigating the residuals in the $M_{\bullet }-M_{\ast }$ relation using the SIMBA cosmological simulation
• Predicting the resolved CO emission of $z=1-3$ star-forming galaxies
• Disc instability and bar formation: view from the IllustrisTNG simulations
• General relativistic quasi-spherical accretion in a dark matter halo
• Winds versus jets: a comparison between black hole feedback modes in simulations of idealized galaxy groups and clusters
• Candidate cosmic filament in the GJ526 field, mapped with the NIKA2 camera
• Beyond mirkwood: Enhancing SED Modeling with Conformal Predictions
• Dipole Distortions in the Intergalactic Medium
• A New Model For Including Galactic Winds in Simulations of Galaxy Formation II: Implementation of PhEW in Cosmological Simulations
• Dynamical friction and massive black hole orbits: analytical predictions and numerical solutions
• The Three Hundred : contrasting clusters galaxy density in hydrodynamical and dark matter simulations
• Galaxy assembly bias in cosmological hydrodynamical simulations: a comparison between SIMBA and IllustrisTNG
• Effects of Varied Cosmic Ray Feedback from AGN on Massive Galaxy Properties
• ARCHITECTS I: Impact of subgrid physics on the simulated properties of the circumgalactic medium
• Observed structural parameters of EAGLE galaxies: reconciling the mass-size relation in simulations with local observations
• Time-Dependent Cosmic Ray Halos from Bursty Star Formation and Active Galactic Nuclei: Semi-Analytic Formalism and Galaxy Formation Implications
• Fast Baryonic Field Painting for Sunyaev-Zel'dovich Analyses: Transfer Function vs. Hybrid Effective Field Theory
• Sahyadri: A simulation suite for the cosmology dependence of the Cosmic Web
• On the consistency of jet feedback modelling across different astrophysics hydrodynamical codes
• Tracing correlations between galaxy properties across the Cosmic Web: An IllustrisTNG-based study
• Mocking IFU observations and metallicity diagnostics from cosmological simulations
• Dark Matter profiles of "in silico" galaxies: deep learning inference
• The black hole population in low-mass galaxies in large-scale cosmological simulations
• Kiloparsec-scale imaging of the CO(1-0)-traced cold molecular gas reservoir in a z~3.4 submillimeter galaxy
• The Metallicity Distribution Function in Outer Halo Fields of Simulated Elliptical Galaxies Compared to Observations of NGC 5128
• Modeling Multiphase Galactic Outflows: A Multifluid Moving Mesh Approach
• The origin of the intra-cluster light in The Three Hundred simulations
• A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
• NeutralUniverseMachine: Predictions of HI gas in Different Theoretical Models
• Populating Galaxies Into Halos Via Machine Learning on the Simba Simulation
• QSOFEED: Investigating warm molecular, low- and high-ionization atomic gas in six type-2 quasars with GTC/EMIR
• Observed cosmic evolution of galaxy dust properties with metallicity and tensions with models
• How non-thermal pressure impacts the modelling of star formation in galaxy formation simulations
• Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback
• Identification of Candidate Halos Hosting Massive Black Hole Seeds in the $\text{Renaissance}$ Simulations with Support Vector Machines
• A comparison of dust content and properties in GAMA/G10-COSMOS/3D-HST and SIMBA cosmological simulations
• Atomic hydrogen reservoirs in quiescent galaxies at z = 0.4
• The interplay between AGN feedback and precipitation of the intracluster medium in simulations of galaxy groups and clusters
• Validating the CROCODILE model within the AGORA galaxy simulation framework
• Semi-empirical constraints on the HI mass function of star-forming galaxies and ${\Omega }_{\mathrm{HI}}$ at $z\sim 0.37$ from interferometric surveys
• Galaxy and black hole coevolution in dark matter haloes not captured by cosmological simulations
• Cosmological gravity on all scales V: MCMC forecasts combining large scale structure and CMB lensing for binned phenomenological modified gravity
• The influence of the Cosmic Web on the properties of dwarf galaxies in the Fornax-Eridanus Supercluster
• Imladris: a detailed and flexible model for galaxy simulations with individual stars
• Mass transport in galaxy discs limits black hole growth to sub-Eddington rates
• The Thermodynamic and Kinematic Evolution of Circumgalactic Gas around $z=1$ in the IllustrisTNG model
• Bound or blown: the fate of hot gas in galaxy groups
• ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations
• AGN Feedback: The impact of galactic-scale radio jets on the interstellar medium in starbursting obscured AGN
• The hidden circumgalactic medium
• Black Hole-Galaxy Correlations in Cluster Zoomed-in Simulations: GIZMO-SIMBA and TNG-Cluster
• Galaxy mergers can initiate quenching by unlocking an AGN-driven transformation of the baryon cycle
• Mainly on the Plane: Observing the Extended, Ionized Disks of Milky Way Analogs in IllustrisTNG
• Deep Learning generated observations of galaxy clusters from dark-matter-only simulations
• The Baryon Budget of Galaxies across the First Billion Years
• Massive black holes and their galaxies
• Exploring supermassive black hole physics and galaxy quenching across halo mass in FIRE cosmological zoom simulations
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• Now you see it, now you don't: Star formation truncation precedes the loss of molecular gas by ~100 Myr in massive post-starburst galaxies at z~0.6
• Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations
• Entropy plateaus can emerge from gas replacement at a characteristic halo mass in simulated groups and clusters of galaxies
• Combining LOFAR and Apertif Data for Understanding the Life Cycle of Radio Galaxies
• The Nature of High-Redshift Massive Quiescent Galaxies -- Searching for RUBIES-UDS-QG-z7 in FLARES
• Simulating High-Velocity Clouds in the Observational Plane: An Initial Study with the Smith Cloud
• Predicting Halo Formation Time Using Machine Learning
• The contribution of stars, dust, neutral gas and supermassive black holes in galaxies to the cosmic baryon inventory
• Exploring the halo occupation distribution for moderate X-ray luminosity active galactic nuclei in the EAGLE cosmological simulation
• A new technique to isolate kinematically anomalous gas in HI data cubes
• Dust and gas modelling in radiative transfer simulations of disc-dominated galaxies with RADMC-3D
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations