Galactic star formation and accretion histories from matching galaxies to dark matter haloes

Abstract

We present a new statistical method to determine the relationship between the stellar masses of galaxies and the masses of their host dark matter haloes over the entire cosmic history from z~4 to the present. This multi-epoch abundance matching (MEAM) model self-consistently takes into account that satellite galaxies first become satellites at times earlier than they are observed. We employ a redshift-dependent parameterization of the stellar-to-halo mass relation to populate haloes and subhaloes in the Millennium simulations with galaxies, requiring that the observed stellar mass functions at several redshifts be reproduced simultaneously. Using merger trees extracted from the dark matter simulations in combination with MEAM, we predict the average assembly histories of galaxies, separating into star formation within the galaxies (in-situ) and accretion of stars (ex-situ). The peak star formation efficiency decreases with redshift from 23% at z=0 to 9% at z=4 while the corresponding halo mass increases from 10^11.8M\odot to 10^12.5M\odot. The star formation rate of central galaxies peaks at a redshift which depends on halo mass; for massive haloes this peak is at early cosmic times while for low-mass galaxies the peak has not been reached yet. In haloes similar to that of the Milky-Way about half of the central stellar mass is assembled after z=0.7. In low-mass haloes, the accretion of satellites contributes little to the assembly of their central galaxies, while in massive haloes more than half of the central stellar mass is formed ex-situ with significant accretion of satellites at z<2. We find that our method implies a cosmic star formation history and an evolution of specific star formation rates which are consistent with those inferred directly. We present convenient fitting functions for stellar masses, star formation rates, and accretion rates as functions of halo mass and redshift.

20 pages, 12 figures, 1 table, submitted to MNRAS

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• Spatially-resolved stellar kinematics of the ultra diffuse galaxy Dragonfly 44. I. Observations, kinematics, and cold dark matter halo fits
• Falling outer rotation curves of star-forming galaxies at 0.6 < z < 2.6 probed with KMOS^3D and SINS/ZC-SINF
• Supernova feedback in numerical simulations of galaxy formation: separating physics from numerics
• Gas accretion and galactic fountain flows in the Auriga cosmological simulations: angular momentum and metal re-distribution
• The surprising inefficiency of dwarf satellite quenching
• The Eating Habits of Milky Way Mass Halos: Destroyed Dwarf Satellites and the Metallicity Distribution of Accreted Stars
• Black Hole and Galaxy Coevolution from Continuity Equation and Abundance Matching
• Tidal stripping as a possible origin of the ultra diffuse galaxy lacking dark matter
• Quenching as a Contest between Galaxy Halos and their Central Black Holes
• Kiloparsec Scale Properties of Star-Formation Driven Outflows at z~2.3 in the SINS/zC-SINF AO Survey
• The evolution of the Tully-Fisher relation between z~2.3 and z~0.9 with KMOS^3D
• The effects of cosmic rays on the formation of Milky Way-mass galaxies in a cosmological context
• The stellar-to-halo mass relation of GAMA galaxies from 100 square degrees of KiDS weak lensing data
• First results from the MADCASH Survey: A Faint Dwarf Galaxy Companion to the Low Mass Spiral Galaxy NGC 2403 at 3.2 Mpc
• A young star-forming galaxy at z = 3.5 with an extended Ly\,$\alpha$ halo seen with MUSE
• Peak star formation efficiency and no missing baryons in massive spirals
• The Near Infrared Imager and Slitless Spectrograph for the James Webb Space Telescope -- II. Wide Field Slitless Spectroscopy
• A Deep Search For Faint Galaxies Associated With Very Low-redshift C IV Absorbers: III. The Mass- and Environment-dependent Circumgalactic Medium
• Early formation of massive, compact, spheroidal galaxies with classical profiles by violent disc instability or mergers
• Is Main Sequence Galaxy Star Formation Controlled by Halo Mass Accretion?
• A small-scale dynamo in feedback-dominated galaxies as the origin of cosmic magnetic fields - I. The kinematic phase
• The Formation of Isolated Ultra-Diffuse Galaxies in Romulus25
• A Lonely Giant: The Sparse Satellite Population of M94 Challenges Galaxy Formation
• Quenching of Star Formation in SDSS Groups: Centrals, Satellites, and Galactic Conformity
• Hot Atmospheres, Cold Gas, AGN Feedback and the Evolution of Early Type Galaxies: a Topical Perspective
• An enigmatic population of luminous globular clusters in a galaxy lacking dark matter
• Demographics of Star-forming Galaxies since $z\sim 2.5$. I. The $UVJ$ Diagram in CANDELS
• A Local Universe Host for the Repeating Fast Radio Burst FRB 20181030A
• ZOMG-I. How the cosmic web inhibits halo growth and generates assembly bias
• The effect of baryons on the inner density profiles of rich clusters
• Spatially Resolved Star Formation and Inside-out Quenching in the TNG50 Simulation and 3D-HST Observations
• The mass discrepancy acceleration relation in a $\Lambda$CDM context
• The gas fractions of dark matter haloes hosting simulated $\sim L^{\star }$ galaxies are governed by the feedback history of their black holes
• Identifying true satellites of the Magellanic Clouds
• A mass-dependent slope of the galaxy size-mass relation out to z~3: further evidence for a direct relation between median galaxy size and median halo mass
• Revealing the galaxy-halo connection in IllustrisTNG
• The Growth in Size and Mass of Cluster Galaxies since z=2
• Interactions between multiple supermassive black holes in galactic nuclei: a solution to the final parsec problem
• A unified model for the maximum mass-scales of molecular clouds, stellar clusters, and high-redshift clumps
• Detection of the LMC-induced sloshing of the Galactic halo
• Diversity of dark matter density profiles in the Galactic dwarf spheroidal satellites
• A survey of high-$z$ galaxies: SERRA simulations
• Spinning dark matter halos promote bar formation
• Colours, Star formation Rates, and Environments of Star forming and Quiescent Galaxies at the Cosmic Noon
• MusE GAs FLOw and Wind (MEGAFLOW) I: First MUSE results on background quasars
• High-Precision Dark Halo Virial Masses from Globular Cluster Numbers: Implications for Globular Cluster Formation and Galaxy Assembly
• The Origin and Evolution of Fast and Slow Rotators in the Illustris Simulation
• Dark matters on the scale of galaxies
• Simulating Groups and the IntraGroup Medium: The Surprisingly Complex and Rich Middle Ground Between Clusters and Galaxies
• The Progenitors of Local Ultra-massive Galaxies Across Cosmic Time: from Dusty Star-bursting to Quiescent Stellar Populations
• What Causes The Formation of Disks and End of Bursty Star Formation?
• The Most Massive Galaxies and Black Holes Allowed by $\Lambda$CDM
• COSMOS2020: The cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z~5
• Low Surface Brightness Imaging of the Magellanic System: Imprints of Tidal Interactions between the Clouds in the Stellar Periphery
• Connecting stellar mass and star-formation rate to dark matter halo mass out to z ~ 2
• Quantifying scatter in galaxy formation at the lowest masses
• The origin of the mass discrepancy-acceleration relation in $\Lambda$CDM
• The effect of metal enrichment and galactic winds on galaxy formation in cosmological zoom simulations
• The formation of massive, quiescent galaxies at cosmic noon
• The MillenniumTNG Project: The galaxy population at $z\ge 8$
• Evolution of the atomic and molecular gas content of galaxies in dark matter haloes
• The morphologies of massive galaxies from z~3 - Witnessing the 2 channels of bulge growth
• The High-$z$ Universe Confronts Warm Dark Matter: Galaxy Counts, Reionization and the Nature of Dark Matter
• Emulation of baryonic effects on the matter power spectrum and constraints from galaxy cluster data
• Going, going, gone dark: Quantifying the scatter in the faintest dwarf galaxies
• Galaxy and Mass Assembly (GAMA): The halo mass of galaxy groups from maximum-likelihood weak lensing
• The most luminous quasars do not live in the most massive dark matter haloes at any redshift
• Local Volume TiNy Titans: Gaseous Dwarf-Dwarf Interactions in the Local Universe
• Hyper Suprime-Cam Subaru Strategic Program: A Mass-Dependent Slope of the Galaxy Size-Mass Relation at $z<1$
• A Systematic Look at the Effects of Radiative Feedback on Disc Galaxy Formation
• Chandra centres for COSMOS X-ray galaxy groups: Differences in stellar properties between central dominant and offset brightest group galaxies
• NIHAO-UHD: The properties of MW-like stellar disks in high resolution cosmological simulations
• AGN-Driven Outflows in Dwarf Galaxies
• A tale of two sites -- I: Inferring the properties of minihalo-hosted galaxies from current observations
• A hydrodynamical halo model for weak-lensing cross correlations
• The Imprint of Reionization on the Star Formation Histories of Dwarf Galaxies
• What does strong gravitational lensing? The mass and redshift distribution of high-magnification lenses
• Baryonic effects for weak lensing. Part I. Power spectrum and covariance matrix
• The Spitzer-HETDEX Exploratory Large-Area Survey
• Introducing the FirstLight project: UV luminosity function and scaling relations of primeval galaxies
• The predicted luminous satellite populations around SMC and LMC-mass galaxies - A missing satellite problem around the LMC?
• Log-normal star formation histories in simulated and observed galaxies
• Dark Matter Cores and Cusps in Spiral Galaxies and their Explanations
• Baryon Cycling in the Low-Redshift Circumgalactic Medium: A Comparison of Simulations to the COS-Halos Survey
• Determining the full satellite population of a Milky Way-mass halo in a highly resolved cosmological hydrodynamic simulation
• The properties of the first galaxies in the BLUETIDES simulation
• Environmental dependence of bulge-dominated galaxy sizes in hierarchical models of galaxy formation. Comparison with the local Universe
• Fuzzy Dark Matter and Dark Matter Halo Cores
• Characterizing the Circumgalactic Medium of Nearby Galaxies with HST/COS and HST/STIS Absorption-Line Spectroscopy: II. Methods and Models
• The Molecular and Ionized Gas Phases of an AGN-driven Outflow in a Typical Massive Galaxy at z=2
• JADES: The incidence rate and properties of galactic outflows in low-mass galaxies across 3 < z < 9
• Expanded haloes, abundance matching and too-big-to-fail in the Local Group
• The Fates of the Circumgalactic Medium in the FIRE Simulations
• The Impact of Scatter in the Galaxy UV Luminosity to Halo Mass Relation on Ly$\alpha$ Visibility During the Epoch of Reionization
• Equilibrium Model Constraints on Baryon Cycling Across Cosmic Time
• Origins and Demographics of Wandering Black Holes
• A hypervelocity star with a Magellanic origin
• Understanding black hole mass assembly via accretion and mergers at late times in cosmological simulations
• VINTERGATAN II: the history of the Milky Way told by its mergers
• MAGIICAT III. Interpreting Self-Similarity of the Circumgalactic Medium with Virial Mass using MgII Absorption
• Post-Newtonian dynamical modeling of supermassive black holes in galactic-scale simulations
• The physics of gas phase metallicity gradients in galaxies
• Avoiding progenitor bias: The structural and mass evolution of Brightest Group and Cluster Galaxies in Hierarchical models since z~1
• The Dramatic Size and Kinematic Evolution of Massive Early-Type Galaxies
• X-ray Scaling Relation in Early-Type Galaxies: Dark Matter as a Primary Factor in Retaining Hot Gas
• The host dark matter halos of [OII] emitters at 0.5< z< 1.5
• Enhanced tidal stripping of satellites in the galactic halo from dark matter self-interactions
• Feedback from supermassive black holes transforms centrals into passive galaxies by ejecting circumgalactic gas
• CLEAR: The Gas-Phase Metallicity Gradients of Star-Forming Galaxies at 0.6 < z < 2.6
• Dynamical signatures of a LCDM-halo and the distribution of the baryons in M33
• The properties of "dark" ΛCDM halos in the Local Group
• Orbital Decay of Supermassive Black Hole Binaries in Clumpy Multiphase Merger Remnants
• The evolving relation between star-formation rate and stellar mass in the VIDEO Survey since $z=3$
• The COS Absorption Survey of Baryon Harbors (CASBaH): Warm-hot Circumgalactic Gas Reservoirs Traced by Ne VIII Absorption
• The formation of extremely diffuse galaxy cores by merging supermassive black holes
• Disruption of satellite galaxies in simulated groups and clusters: the roles of accretion time, baryons, and pre-processing
• A Census of Stellar Mass in 10 Massive Haloes at z~1 from the GCLASS Survey
• Major Mergers Going Notts: Challenges for Modern Halo Finders
• Circumgalactic Mg II Emission from an Isotropic Starburst Galaxy Outflow Mapped by KCWI
• Preparing for low surface brightness science with the Vera C. Rubin Observatory: characterisation of tidal features from mock images
• Dissecting the Local Environment of FRB 190608 in the Spiral Arm of its Host Galaxy
• Galactic Archaeology with Gaia
• The MaGICC Baryon Cycle: The Enrichment History of Simulated Disc Galaxies
• 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
• A tale of two populations: surviving and destroyed dwarf galaxies and the build up of the Milky Way's stellar halo
• Brightest cluster galaxies in cosmological simulations: achievements and limitations of AGN feedback models
• The quenching of galaxies, bulges, and disks since cosmic noon: A machine learning approach for identifying causality in astronomical data
• Shaken, not blown: the gentle baryonic feedback of nearby starburst dwarf galaxies
• The Dynamics of Galaxy Pairs in a Cosmological Setting
• The clustering of luminous red galaxies at z $\sim$ 0.7 from eBOSS and BOSS data
• GASTRO library I: the simulated chemodynamical properties of several GSE-like stellar halos
• Scale-dependent bias in the BAO-scale intergalactic neutral hydrogen
• A deep survey of short GRB host galaxies over $z\sim 0-2$: implications for offsets, redshifts, and environments
• An Empirical Model for the Star Formation History in Dark Matter Halos
• The effect of the LMC on the Milky Way system
• On the Physical Origin of Galactic Conformity
• NIHAO XIII: Clumpy discs or clumpy light in high redshift galaxies?
• The surprising accuracy of isothermal Jeans modelling of self-interacting dark matter density profiles
• Equilibrium models of the Milky Way mass are biased high by the LMC
• Mass Transport and Turbulence in Gravitationally Unstable Disk Galaxies. I: The Case of Pure Self-Gravity
• Cosmological Galaxy Evolution with Superbubble Feedback I: Realistic Galaxies with Moderate Feedback
• MUSEQuBES: Calibrating the redshifts of Ly α emitters using stacked circumgalactic medium absorption profiles
• NIHAO XX: The impact of the star formation threshold on the cusp-core transformation of cold dark matter haloes
• NIHAO VIII: Circum-galactic medium and outflows - The puzzles of HI and OVI gas distributions
• Baryonic and dark matter distribution in cosmological simulations of spiral galaxies
• Low-mass galaxy assembly in simulations: regulation of early star formation by radiation from massive stars
• NIHAO VI. The hidden discs of simulated galaxies
• A small-scale dynamo in feedback-dominated galaxies - II. The saturation phase and the final magnetic configuration
• Precision Scaling Relations for Disk Galaxies in the Local Universe
• Active Galactic Nuclei and their Large-scale Structure: an eROSITA mock catalogue
• Quiescent Ultra-diffuse galaxies in the field originating from backsplash orbits
• Modelling the Tucana III stream - a close passage with the LMC
• The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations
• Hidden depths in the local Universe: The Stellar Stream Legacy Survey
• No Assembly Required: Mergers are Mostly Irrelevant for the Growth of Low-mass Dwarf Galaxies
• Statistics of Dark Matter Substructure: III. Halo-to-Halo Variance
• An assessment of the "too big to fail" problem for field dwarf galaxies in view of baryonic feedback effects
• Ionized and molecular gas kinematics in a z=1.4 star-forming galaxy
• The Massive End of the Stellar Mass Function
• The Galaxy Clustering Crisis in Abundance Matching
• Where Do Galaxies End?
• Absorption-Line Detections of $10^{5-6}$ K Gas in Spiral-Rich Groups of Galaxies
• Persistence of the Color-Density Relation and Efficient Environmental Quenching to $z\sim 1.4$
• Wet Compaction to a Blue Nugget: a Critical Phase in Galaxy Evolution
• Knocking on giants' doors: I. The evolution of the dust-to-stellar mass ratio in distant dusty galaxies
• The effect of the deforming dark matter haloes of the Milky Way and the Large Magellanic Cloud on the Orphan-Chenab stream
• The Argo Simulation: II. The Early Build-up of the Hubble Sequence
• Dissecting the Gaseous Halos of z~2 Damped Ly$\alpha$ Systems with Close Quasar Pairs
• Reignition of Star Formation in Dwarf Galaxies
• How to Reconcile the Observed Velocity Function of Galaxies with Theory
• The evolution of superluminous supernova LSQ14mo and its interacting host galaxy system
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): Downsizing of the blue cloud and the influence of galaxy size on mass quenching over the last eight billion years
• The effects of metallicity, UV radiation and non-equilibrium chemistry in high-resolution simulations of galaxies
• A Lightcone Catalogue from the Millennium-XXL Simulation
• The rest-frame optical (900nm) galaxy luminosity function at z~4-7: abundance matching points to limited evolution in the Mstar/Mhalo ratio at z>4
• Connecting Transitions in Galaxy Properties to Refueling
• A Dichotomy in Satellite Quenching Around L* Galaxies
• Numerical resolution limits on subhalo abundance matching
• CGM${}^2$ I: The Extent of the Circumgalactic Medium Traced by Neutral Hydrogen
• GalaxyNet: Connecting galaxies and dark matter haloes with deep neural networks and reinforcement learning in large volumes
• H0LiCOW II. Spectroscopic survey and galaxy-group identification of the strong gravitational lens system HE0435-1223
• Semi-analytic forecasts for JWST -- VI. Simulated lightcones and galaxy clustering predictions
• Physics of Galactic Metals: Evolutionary Effects due to Production, Distribution, Feedback & Interaction with Black Holes
• Galactic disk winds driven by cosmic ray pressure
• On the mass of the Local Group
• Star Formation and Clumps in Cosmological Galaxy Simulations with Radiation Pressure Feedback
• Constraining the CO intensity mapping power spectrum at intermediate redshifts
• Galaxies flowing in the oriented saddle frame of the cosmic web
• Constraining the evolution of CII intensity through the end stages of reionization
• Breaking degeneracies in the first galaxies with clustering
• The quiescent phase of galactic disc growth
• The bias of the submillimetre galaxy population: SMGs are poor tracers of the most massive structures in the z ~ 2 Universe
• The eROSITA Final Equatorial Depth Survey (eFEDS): X-ray emission around star-forming and quiescent galaxies at $0.05<z<0.3$
• The biasing of baryons on the cluster mass function and cosmological parameter estimation
• The MaGICC volume: reproducing statistical properties of high redshift galaxies
• Predicting Galaxy Star Formation Rates via the Co-evolution of Galaxies and Halos
• Glimpsing the Imprint of Local Environment on the Galaxy Stellar Mass Function
• Search for Gamma-ray Emission from Dark Matter Annihilation in the Large Magellanic Cloud with the Fermi Large Area Telescope
• The galaxy-halo connection of emission-line galaxies in IllustrisTNG
• The distribution of mass components in simulated disc galaxies
• Machine Learning and Cosmological Simulations II: Hydrodynamical Simulations
• Impact of Lyman alpha pressure on metal-poor dwarf galaxies
• The Dekel-Zhao profile: A mass-dependent dark-matter density profile with flexible inner slope and analytic potential, velocity dispersion, and lensing properties
• Size matters: abundance matching, galaxy sizes, and the Tully-Fisher relation in EAGLE
• Light breeze in the local Universe
• Complex AGN feedback in the Teacup galaxy. A powerful ionised galactic outflow, jet-ISM interaction, and evidence for AGN-triggered star formation in a giant bubble
• The Correlation Between Halo Mass and Stellar Mass for the Most Massive Galaxies in the Universe
• EMERGE: Empirical predictions of galaxy merger rates since $z\sim 6$
• The evolution of the star forming sequence in hierarchical galaxy formation models
• Quantifying the Stellar Halo's Response to the LMC's Infall with Spherical Harmonics
• The cumulative star-formation histories of dwarf galaxies with TNG50. I: Environment-driven diversity and connection to quenching
• Dynamical evidence for a morphology-dependent relation between the stellar and halo masses of galaxies
• The Frequency of Dwarf Galaxy Multiples at Low Redshift in SDSS vs. Cosmological Expectations
• Two-Face(s): ionized and neutral gas winds in the local Universe
• Direct Insights into Observational Absorption Line Analysis Methods of the Circumgalactic Medium Using Cosmological Simulations
• A flexible subhalo abundance matching model for galaxy clustering in redshift space
• Exploring SMBH Assembly with Semi-analytic Modelling
• NIHAO XIX: How supernova feedback shapes the galaxy baryon cycle
• Empirical constraints on the formation of early-type galaxies
• Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
• Disentangling the Cosmic Web Towards FRB 190608
• NIHAO XXI: The emergence of Low Surface Brightness galaxies
• Interpreting Short Gamma Ray Burst Progenitor Kicks and Time Delays Using the Host Galaxy-Dark Matter Halo Connection
• HST Proper Motions of NGC 147 and NGC 185: Orbital Histories and Test of Dynamically Coherent Andromeda Satellite Plane
• Tracing Black Hole and Galaxy Co-evolution in the Romulus Simulations
• CONCERTO: High-fidelity simulation of millimeter line emissions of galaxies and [CII] intensity mapping
• Constraining the Star Formation Histories in Dark Matter Halos: I. Central Galaxies
• Formation of elongated galaxies with low masses at high redshift
• Luminosity Functions and Host-to-Host Scatter of Dwarf Satellite Systems in the Local Volume
• From lenticulars to blue compact dwarfs: the stellar mass fraction is regulated by disc gravitational instability
• Introducing EMP-Pathfinder: modelling the simultaneous formation and evolution of stellar clusters in their host galaxies
• From massive spirals to dwarf irregulars: a new set of tight scaling relations for cold gas and stars driven by disc gravitational instability
• Multi-tracer intensity mapping: Cross-correlations, Line noise & Decorrelation
• The edge of galaxy formation I: formation and evolution of MW-satellites analogues before accretion
• An observer's guide to the (Local Group) dwarf galaxies: predictions for their own dwarf satellite populations
• Galaxy And Mass Assembly (GAMA): Testing galaxy formation models through the most massive galaxies in the Universe
• A fresh look into the interacting dark matter scenario
• High resolution study of the cluster complexes in a lensed spiral at redshift ~1.5; constraints on the bulge formation and disk evolution
• Galaxies in X-ray Selected Clusters and Groups in Dark Energy Survey Data I: Stellar Mass Growth of Bright Central Galaxies Since z~1.2
• Metal-enriched halo gas across galaxy overdensities over the last 10 billion years
• The impact of gas disc flaring on rotation curve decomposition and revisiting baryonic and dark-matter relations for nearby galaxies
• Structure Formation Models Weaken Limits on WIMP Dark Matter from Dwarf Spheroidal Galaxies
• Hunting Faint Dwarf Galaxies in the Field Using Integrated Light Surveys
• Estimating the Mass of the Milky Way Using the Ensemble of Classical Satellite Galaxies
• Vast planes of satellites in a high resolution simulation of the Local Group: comparison to Andromeda
• MaNGA DynPop -- I. Quality-assessed stellar dynamical modelling from integral-field spectroscopy of 10K nearby galaxies: a catalogue of masses, mass-to-light ratios, density profiles and dark matter
• The Structural Evolution of Milky Way-like Star Forming Galaxies since z~1.3
• Cosmological Galaxy Evolution with Superbubble Feedback II: The Limits of Supernovae
• The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to $z\sim 5$
• Does circumgalactic OVI trace low-pressure gas beyond the accretion shock? Clues from HI and low-ion absorption, line kinematics, and dust extinction
• Galactic ionising photon budget during the Epoch of Reionisation in the Cosmic Dawn II simulation
• Orbits of massive satellite galaxies: II. Bayesian Estimates of the Milky Way and Andromeda masses using high precision astrometry and cosmological simulations
• The Quest for Dusty Star-forming Galaxies at High Redshift z>4
• The Main Sequences of Starforming Galaxies and Active Galactic Nuclei at High Redshift
• 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
• Galaxy spin as a formation probe: the stellar-to-halo specific angular momentum relation
• High redshift JWST predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves
• PRIMUS+DEEP2: The Dependence of Galaxy Clustering on Stellar Mass and Specific Star Formation Rate at 0.2 < z < 1.2
• Detecting clusters of galaxies and active galactic nuclei in an eROSITA all-sky survey digital twin
• Dark and luminous satellites of LMC-mass galaxies in the FIRE simulations
• KiDS-1000: Combined halo-model cosmology constraints from galaxy abundance, galaxy clustering and galaxy-galaxy lensing
• Incidence, scaling relations and physical conditions of ionised gas outflows in MaNGA
• Origin and evolution of ultra-diffuse galaxies in different environments
• Star Formation and Stellar Mass Assembly in Dark Matter Halos: From Giants to Dwarfs
• Self-Interacting Dark Matter and the Origin of Ultra-Diffuse Galaxies NGC1052-DF2 and -DF4
• Reionization inference from the CMB optical depth and E-mode polarization power spectra
• O VI Emission Imaging of a Galaxy with the Hubble Space Telescope: a Warm Gas Halo Surrounding the Intense Starburst SDSS J115630.63+500822.1
• Osaka Feedback Model: Isolated Disk Galaxy Simulations
• The dependence of the galaxy stellar-to-halo mass relation on galaxy morphology
• Galaxy disc scaling relations: A tight linear galaxy -- halo connection challenges abundance matching
• The Cusp/Core problem: supernovae feedback versus the baryonic clumps and dynamical friction model
• Search for 511 keV Emission in Satellite Galaxies of the Milky Way with INTEGRAL/SPI
• The hot circumgalactic medium in the eROSITA All-Sky Survey I. X-ray surface brightness profiles
• Baryonic Imprints on DM Halos: Population Statistics from Dwarf Galaxies to Galaxy Clusters
• The Strikingly Similar Relation between Satellite and Central Galaxies and Their Dark Matter Halos Since z=2
• The evolution of clustering length, large-scale bias and host halo mass at 2<z<5 in the VIMOS Ultra Deep Survey (VUDS)
• On the intermediate-redshift central stellar mass-halo mass relation, and implications for the evolution of the most massive galaxies since z~1
• Two Growing Modes and the Morphology-Quiescence Relation in Galaxies
• The simplest model of galaxy formation I: A formation history model of galaxy stellar mass growth
• The difference in metallicity distribution functions of halo stars and globular clusters as a function of galaxy type: A tracer of globular cluster formation and evolution
• Scaling relations and baryonic cycling in local star-forming galaxies: II. Gas content and star-formation efficiency
• An analytical model for galaxy metallicity: What do metallicity relations tell us about star formation and outflow?
• Hot phase generation by supernovae: resolution, chemistry and thermal conduction
• AGN feedback, quiescence and CGM metal enrichment in early-type galaxies
• The New Galaxy Evolution Paradigm Revealed by the Herschel Surveys
• On the origin of the mass-metallicity gradient relation in the local Universe
• An empirical representation of a physical model for the ISM [CII], CO, and [CI] emission at redshift $1\le z\le 9$
• Cosmological baryon transfer in the SIMBA simulations
• Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
• First results from SMAUG: The need for preventative stellar feedback and improved baryon cycling in semi-analytic models of galaxy formation
• Deep MUSE observations in the HDFS. Morpho-kinematics of distant star-forming galaxies down to $10^8$M${}_{\odot }$
• Evolution of Star-forming Galaxies from z = 0.7 to 1.2 with eBOSS Emission-line Galaxies
• Constraints on the circumburst environments of short gamma-ray bursts
• A constant characteristic volume density of dark matter haloes from SPARC rotation curve fits
• First results from the VIRIAL survey: the stellar content of $UVJ$-selected quiescent galaxies at $1.5<z<2$ from KMOS
• MHONGOOSE -- A MeerKAT Nearby Galaxy HI Survey
• A Preferential Growth Channel for Supermassive Black Holes in Elliptical Galaxies at z<2
• Signatures of stellar accretion in MaNGA early-type galaxies
• The origin of the mass scales for maximal star formation efficiency and quenching: the critical role of Supernovae
• Millimeter mapping at z~1: dust-obscured bulge building and disk growth
• The bias of DLAs at z ~ 2.3: contraining stellar feedback in shallow potential wells
• Realistic mock observations of the sizes and stellar mass surface densities of massive galaxies in FIRE-2 zoom-in simulations
• A tale of two sites -- II: Inferring the properties of minihalo-hosted galaxies with upcoming 21-cm interferometers
• Modeling the Baryon Cycle in Low Mass Galaxy Encounters: the Case of NGC 4490 & NGC 4485
• 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
• The combined effect of AGN and supernovae feedback in launching massive molecular outflows in high-redshift galaxies
• Timing the evolution of quiescent and star-forming local galaxies
• From Diversity to Dichotomy, and Quenching: Milky-Way-Like and Massive-Galaxy Progenitors at 0.5<z<3.0
• Stellar orbits in cosmological galaxy simulations: the connection to formation history and line-of-sight kinematics
• Black Hole Growth and Feedback in Isolated Romulus25 Dwarf Galaxies
• The Immitigable Nature of Assembly Bias: The Impact of Halo Definition on Assembly Bias
• New Analytic Solutions for Galaxy Evolution: Gas, Stars, Metals and Dust in local Early-Type Galaxies and in their high-z Starforming Progenitors
• The Stellar Mass, Star Formation Rate and Dark Matter Halo Properties of LAEs at $z\sim 2$
• Momentum-driven Winds from Radiatively Efficient Black Hole Accretion and Their Impact on Galaxies
• Evidences against cuspy dark matter halos in large galaxies
• The Origin of r-process Enhanced Metal-Poor Halo Stars In Now-Destroyed Ultra-Faint Dwarf Galaxies
• The evolution of the stellar mass versus halo mass relationship
• The highest-speed local dark matter particles come from the Large Magellanic Cloud
• Equilibrium model prediction for the scatter in the star-forming main sequence
• Formation of disk galaxies in preheated media: a preventative feedback model
• A Break in Spiral Galaxy Scaling Relations at the Upper Limit of Galaxy Mass
• Integral-Field Spectroscopy of Fast Outflows in Dwarf Galaxies with AGN
• A Deficit of Dark Matter from Jeans Modeling of the Ultra-diffuse Galaxy NGC 1052-DF2
• Simple halo model formalism for the cosmic infrared background and its correlation with the thermal Sunyaev Zel'dovich effect
• Rotation Curve Decomposition for Size-Mass Relations of Bulge, Disk, and Dark Halo in Spiral Galaxies
• The LBT Satellites of Nearby Galaxies Survey (LBT-SONG): The Satellite Population of NGC 628
• The Cluster-EAGLE project: velocity bias and the velocity dispersion - mass relation of cluster galaxies
• Formation of the largest galactic cores through binary scouring and gravitational wave recoil
• Magellanic satellites in $\Lambda$CDM cosmological hydrodynamical simulations of the Local Group
• Warm FIRE: Simulating Galaxy Formation with Resonant Sterile Neutrino Dark Matter
• A semi-analytic study of self-interacting dark-matter haloes with baryons
• Halo Histories vs. Galaxy Properties at z=0, I: The Quenching of Star Formation
• NIHAO -- XXV. Convergence in the cusp-core transformation of cold dark matter haloes at high star formation thresholds
• X-ray Emission From Hot Gas in Galaxy Groups and Clusters in Simba
• Cold or Warm? Constraining Dark Matter with Primeval Galaxies and Cosmic Reionization after Planck
• The FRB20190520B Sightline Intersects Foreground Galaxy Clusters
• A universal relation between the properties of supermassive black holes, galaxies, and dark matter halos
• On stellar mass loss from galaxies in groups and clusters
• Introducing galactic structure finder: the multiple stellar kinematic structures of a simulated Milky Way mass galaxy
• Revisiting the bulge-halo conspiracy I: Dependence on galaxy properties and halo mass
• Creating a galaxy lacking dark matter in a dark matter dominated universe
• The Morphology-Density-Relation: Impact on the Satellite Fraction
• Dark matter stripping in galaxy clusters: a look at the Stellar to Halo Mass relation in the Illustris simulation
• Baryon effects on void statistics in the EAGLE simulation
• Where did the globular clusters of the Milky Way form? Insights from the E-MOSAICS simulations
• The dependence of galaxy clustering on stellar mass, star-formation rate and redshift at z = 0.8-2.2, with HiZELS
• Towards a radially-resolved semi-analytic model for the evolution of disc galaxies tuned with machine learning
• Constraining the last 7 billion years of galaxy evolution in semi-analytic models
• Is there enough star formation in simulated protoclusters?
• The Mass Profile of the Milky Way to the Virial Radius from the Illustris Simulation
• The Role of Cold Flows and Reservoirs in Galaxy Formation With Strong Feedback
• Search for Gamma-ray Emission from Dark Matter Annihilation in the Small Magellanic Cloud with the Fermi Large Area Telescope
• The diverse formation histories of simulated disc galaxies
• Simulating disc galaxy bulges that are consistent with observed scaling relations
• MUSEQuBES: Characterizing the circumgalactic medium of redshift $\approx 3.3$ Ly$\alpha$ emitters
• Thermal Instability of Halo Gas Heated by Streaming Cosmic Rays
• Jet-driven AGN feedback on molecular gas and low star-formation efficiency in a massive local spiral galaxy with bright X-ray halo
• The star formation history of Eridanus II: on the role of SNe feedback in the quenching of ultra-faint dwarf galaxies
• Constraints on warm dark matter from UV luminosity functions of high-z galaxies with Bayesian model comparison
• NIHAO XXII: Introducing black hole formation, accretion and feedback into the NIHAO simulation suite
• NIHAO XVI: The properties and evolution of kinematically selected discs, bulges and stellar haloes
• The Incomplete Conditional Stellar Mass Function: Unveiling the Stellar Mass Functions of Galaxies at 0.1 < Z < 0.8 from BOSS Observations
• Matching the Evolution of the Stellar Mass Function Using Log-normal Star Formation Histories
• The clustering of radio galaxies: biasing and evolution versus stellar mass
• The emergence of dark matter-deficient ultra-diffuse galaxies driven by scatter in the stellar mass-halo mass relation and feedback from globular clusters
• The Main Sequence and the Fundamental Metallicity Relation in MaGICC Galaxies: Evolution and Scatter
• A new astrophysical solution to the Too Big To Fail problem - Insights from the MoRIA simulations
• Overdensity of submillimeter galaxies around the $z\simeq 2.3$ MAMMOTH-1 nebula
• Central galaxies in different environments: Do they have similar properties?
• The edge of galaxy formation II: evolution of Milky Way satellite analogues after infall
• Galaxies Probing Galaxies in PRIMUS - II. The Coherence Scale of the Cool Circumgalactic Medium
• The kinematics of massive quiescent galaxies at $1.4<z<2.1$: dark matter fractions, IMF variation, and the relation to local early-type galaxies
• HectoMAP and Horizon Run 4: Dense Structures and Voids in the Real and Simulated Universe
• Observed trend in the star formation history and the dark matter fraction of galaxies at redshift $z\approx 0.8$
• A Statistical Semi-Empirical Model: Satellite galaxies in Groups and Clusters
• Modeling for Stellar Feedback in Galaxy Formation Simulations
• FLIMFLAM DR1: The First Constraints on the Cosmic Baryon Distribution from 8 FRB sightlines
• A parametric study of possible solutions to the high-redshift overproduction of stars in modeled dwarf galaxies
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• The radial acceleration relation in galaxy clusters
• Intensity mapping with neutral hydrogen and the Hidden Valley simulations
• Gaia-DR2 extended kinematical maps. Part II: Dynamics in the Galactic disk explaining radial and vertical velocities
• Constraints on the evolution of the relationship between HI mass and halo mass in the last 12 Gyr
• RIGEL: Simulating dwarf galaxies at solar mass resolution with radiative transfer and feedback from individual massive stars
• Statistics of galaxy mergers: bridging the gap between theory and observation
• Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency
• Dust in the Wind: Composition and Kinematics of Galaxy Outflows at the Peak Epoch of Star Formation
• Does the Galaxy-Halo Connection Vary with Environment?
• The New Numerical Galaxy Catalog (${\nu }^2$GC): An Updated Semi-analytic Model of Galaxy and AGN with Large Cosmological N-body Simulation
• Brightest Cluster Galaxies in Cosmological Simulations with Adaptive Mesh Refinement: Successes and Failures
• The effects of AGN feedback on the structural and dynamical properties of Milky Way-mass galaxies in cosmological simulations
• Massive Star-Forming Galaxies Have Converted Most of Their Halo Gas into Stars
• Formation channels of slowly rotating early-type galaxies
• Massive disc galaxies in cosmological hydrodynamical simulations are too dark matter-dominated
• Lyman-αabsorption beyond the disk of simulated spiral galaxies
• Stellar Mass-to-light Ratios: Composite Bulge+Disk Models and the Baryonic Tully-Fisher Relation
• Dark Matter Trapping by Stellar Bars: The Shadow Bar
• The Impact of Environment on the Stellar Mass - Halo Mass Relation
• Globular Clusters Formed within Dark Halos I: present-day abundance, distribution and kinematics
• Dark MaGICC: the effect of Dark Energy on galaxy formation. Cosmology does matter
• Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
• A Consistent Set of Empirical Scaling Relations for Spiral Galaxies: The $(v_{\max },M_{\mathrm{DM}})$-$({\sigma }_0,M_{\mathrm{BH}},\varphi )$ Relations
• Discovery of a Quadruple Lens in CANDELS with a Record Lens Redshift z=1.53
• Metal line emission from galaxy haloes at z~1
• Dark matter halos and scaling relations of extremely massive spiral galaxies from extended HI rotation curves
• A Galaxy Redshift Survey near HST/COS AGN Sight Lines
• The impact of baryonic potentials on the gravothermal evolution of self-interacting dark matter haloes
• Hubble Space Telescope Observations of Two Faint Dwarf Satellites of Nearby LMC Analogs from MADCASH
• Compaction-Driven Black Hole Growth
• The kinematics of globular cluster populations in the E-MOSAICS simulations and their implications for the assembly history of the Milky Way
• The Next Generation Virgo Cluster Survey (NGVS). XXXV. First Kinematical Clues of Overly-Massive Dark Matter Halos in Several Ultra-Diffuse Galaxies in the Virgo Cluster
• Reproducing cosmic evolution of galaxy population from $z=4$ to $0$
• Tidal Stripping in the Adiabatic Limit
• The Galaxy--Halo Connection in High-Redshift Universe: Details and Evolution of Stellar-to-Halo Mass Ratios of Lyman Break Galaxies on CFHTLS Deep Fields
• The Kinematics and Dark Matter Fractions of TNG50 Galaxies at z=2 from an Observational Perspective
• Tidal destruction in a low mass galaxy environment: the discovery of tidal tails around DDO 44
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• The stellar mass - halo mass relation from galaxy clustering in VUDS: a high star formation efficiency at z~3
• The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3
• Origins of Scatter in the Relationship Between HCN 1-0 and Dense Gas Mass in the Galactic Center
• Formation and settling of a disc galaxy during the last 8 billion years in a cosmological simulation
• Calibrated, cosmological hydrodynamical simulations with variable IMFs I: Method and effect on global galaxy scaling relations
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• The central spheroids of Milky Way mass-sized galaxies
• Constraints on Chameleon f(R)-Gravity from Galaxy Rotation Curves of the SPARC Sample
• Evaporation of planetary atmospheres due to XUV illumination by quasars
• The Pandora project. I: the impact of radiation and cosmic rays on baryonic and dark matter properties of dwarf galaxies
• What's in a name? Quantifying the interplay between the Definition, Orientation, and Shape of Ultra-diffuse Galaxies Using the Romulus Simulations
• Constraining the Warm Dark Matter Particle Mass through Ultra-Deep UV Luminosity Functions at z=2
• Simulating the Spatial Distribution and Kinematics of Globular Clusters within Galaxy Clusters in Illustris
• MaGICC-WDM: the effects of warm dark matter in hydrodynamical simulations of disc galaxy formation
• Cross-calibration of CO- vs dust-based gas masses and assessment of the dynamical mass budget in Herschel-SDSS Stripe82 galaxies
• Stellar-to-halo mass relation of cluster galaxies
• Cosmic CARNage I: on the calibration of galaxy formation models
• Supernovae feedback propagation: the role of turbulence
• MaNGA DynPop -- III. Stellar dynamics versus stellar population relations in 6000 early-type and spiral galaxies: Fundamental Plane, mass-to-light ratios, total density slopes, and dark matter fractions
• The role of massive halos in the Star Formation History of the Universe
• Stars behind bars II: A cosmological formation scenario for the Milky Way's central stellar structure
• Using Galaxy Pairs to Probe Star Formation During Major Halo Mergers
• $\Lambda$CDM Predictions for the Satellite Population of M33
• The Mass Dependance of Satellite Quenching in Milky Way-like Halos
• The angular momentum of disc galaxies at z=1
• Cool circumgalactic gas of passive galaxies from cosmological inflow
• Powerful quasar outflow in a massive disc galaxy at $z\sim 5$
• Simulating the H2 content of high-redshift galaxies
• Modelling of Lyman-alpha Emitting Galaxies and Ionized Bubbles at the Era of Reionization
• Gas flows in the circumgalactic medium around simulated high-redshift galaxies
• GA-NIFS: Multi-phase analysis of a star-forming galaxy at $z\sim 5.5$
• Gas Accretion Can Drive Turbulence in Galaxies
• Distribution of streaming rates into high-redshift galaxies
• NIHAO III: The constant disc gas mass conspiracy
• On the (Lack of) Evolution of the Stellar Mass Function of Massive Galaxies from $z$=1.5 to 0.4
• The cosmic web of X-ray active galactic nuclei seen through the eROSITA Final Equatorial Depth Survey (eFEDS)
• The Observed Evolution of the Stellar Mass - Halo Mass Relation for Brightest Central Galaxies
• On Physical Scales of Dark Matter Halos
• The mass accretion rate of galaxy clusters: a measurable quantity
• ELUCID V. Lighting dark matter halos with galaxies
• Forward Modeling of Double Neutron Stars: Insights from Highly-Offset Short Gamma-Ray Bursts
• How AGN feedback drives the size growth of the first quasars
• The impact of the Large Magellanic Cloud on dark matter direct detection signals
• An ALMA survey of the SCUBA-2 Cosmology Legacy SurveyUKIDSS/UDS Field: Halo Masses for Submillimetre Galaxies
• The distribution of satellites around massive galaxies at 1<z<3 in ZFOURGE/CANDELS: dependence on star formation activity
• ZOMG II: Does the halo assembly history influence central galaxies and gas accretion?
• The imprint of dark matter haloes on the size and velocity dispersion evolution of early-type galaxies
• NIHAO XXIV: Rotation or pressure supported systems? Simulated Ultra Diffuse Galaxies show a broad distribution in their stellar kinematics
• Discovery of a Strong Lensing Galaxy Embedded in a Cluster at z = 1.62
• The missing dwarf galaxies of the Local Group
• Orbital dynamics and histories of satellite galaxies around Milky Way-mass galaxies in the FIRE simulations
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Sensitivity of dark matter haloes to their accretion histories
• Stellar feedback from HMXBs in cosmological hydrodynamical simulations
• Compact Starburst Galaxies with Fast Outflows: Central Escape Velocities and Stellar Mass Surface Densities from Multi-band Hubble Space Telescope Imaging
• Characterising the Intracluster Light over the Redshift Range $0.2<z<0.8$ in the DES-ACT Overlap
• The role of AGN feedback on the evolution of dwarf galaxies from cosmological simulations: SMBHs suppress star formation in low-mass galaxies
• Cosmic evolution of bars in simulations of galaxy formation
• Dissecting the roles of mass and environment quenching in galaxy evolution with EAGLE
• Simba: The average properties of the circumgalactic medium of $2\le z\le 3$ quasars are determined primarily by stellar feedback
• The Next Generation Virgo Cluster Survey. IX. Estimating the Efficiency of Galaxy Formation on the Lowest-Mass Scales
• Entropy Driven Winds: Outflows and Fountains Lifted Gently by Buoyancy
• A unified model for the clustering of quasars and galaxies at $z\approx 6$
• High resolution near-infrared imaging of submillimeter galaxies
• The growth of galactic bulges through mergers in LCDM haloes revisited. II. Morphological mix evolution
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• Revisiting the Size-Luminosity Relation in the Era of Ultra Diffuse Galaxies
• Constraining the Milky Way halo kinematics via its Linear Response to the Large Magellanic Cloud
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• Constraining AGN triggering mechanisms through the clustering analysis of active black holes
• On the early evolution of Local Group dwarf galaxy types: star formation and supernova feedback
• The phantom dark matter halos of the Local Volume in the context of modified Newtonian dynamics
• The dark side of galaxy stellar populations I: The stellar-to-halo mass relation and the velocity dispersion - halo mass relation
• Angular Momentum of Early and Late Type Galaxies: Nature or Nurture?
• Growth of Supermassive Black Hole Seeds in ETG Star-Forming Progenitors: Multiple Merging of Stellar Compact Remnants via Gaseous Dynamical Friction and Gravitational Wave Emission
• From starburst to quiescence: post-starburst galaxies and their large-scale clustering over cosmic time
• Effects of the environment on galaxies in the Catalogue of Isolated Galaxies: physical satellites and large scale structure
• UniverseMachine: Predicting Galaxy Star Formation over Seven Decades of Halo Mass with Zoom-in Simulations
• A first estimate of the Milky Way dark matter halo spin
• Testing the Relationship Between Bursty Star Formation and Size Fluctuations of Local Dwarf Galaxies
• A Deep Search for Faint Galaxies Associated with Very Low-Redshift C IV Absorbers: A Case with Cold-Accretion Characteristics
• Cosmological simulations of Milky Way-sized galaxies
• Evidence for a Massive Andromeda Galaxy Using Satellite Galaxy Proper Motions
• Dark influences III. Structural characterization of minor mergers of dwarf galaxies with dark satellites
• SHAM through the lens of a hydrodynamical simulation
• Massive Dark Matter Halos at High Redshift: Implications for Observations in the JWST Era
• Scaling relations and baryonic cycling in local star-forming galaxies. III. Outflows, effective yields and metal loading factors
• A Fundamental Test for Galaxy Formation Models: Matching the Lyman-$\alpha$ Absorption Profiles of Galactic Halos over Three Decades in Distance
• Stellar Mass Function of Active and Quiescent Galaxies via the Continuity Equation
• Charting the main sequence of star-forming galaxies out to redshifts z<5.7
• A Search for Satellite Galaxies of Nearby Star-Forming Galaxies with Resolved Stars in LBT-SONG
• Satellite mass functions and the faint end of the galaxy mass-halo mass relation in LCDM
• The interplay between feedback, accretion, transport and winds in setting gas-phase metal distribution in galaxies
• Construct the emission line galaxy-host halo connection through auto and cross correlations
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• ATLAS Probe: Breakthrough Science of Galaxy Evolution, Cosmology, Milky Way, and the Solar System
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• Brightest Group Galaxies: Stellar Mass and Star Formation Rate (paper I)
• Galaxy Flybys: Evolution of the Bulge, Disk, and Spiral Arms
• Exploring the diversity and similarity of radially anisotropic Milky Way-like stellar haloes: implications for disrupted dwarf galaxy searches
• The halo mass function of late-type galaxies from HI kinematics
• Measuring the delay time distribution of binary neutron stars. I. Through Scaling Relations of the Host Galaxies of Gravitational Wave Events
• Generating Synthetic Cosmological Data with GalSampler
• A hidden population of massive black holes in simulated dwarf galaxies
• 21cmfish: Fisher-matrix framework for fast parameter forecasts from the cosmic 21-cm signal
• Beyond Ultra-diffuse Galaxies. I. Mass--Size Outliers among the Satellites of Milky Way Analogs
• Orbital decay of Globular Clusters in the galaxy with little dark matter
• Simulations of isolated dwarf galaxies formed in dark matter halos with different mass assembly histories
• Testing Galaxy Quenching Theories with Scatter in the Stellar to Halo Mass Relation
• Systematic uncertainties from halo asphericity in dark matter searches
• A high baryon fraction in massive haloes at z~3
• Towards a higher mass for NGC1052-DF2: an analysis based on full distribution functions
• The neutral hydrogen distribution in large-scale haloes from 21-cm intensity maps
• How the first stars shaped the faintest gas-dominated dwarf galaxies
• Photometric Objects around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. I. Methods
• A scenario for ultra-diffuse satellite galaxies with low velocity dispersions: the case of [KKS 2000]04
• The Effect of Adiabatic Compression on Dark Matter Halos and the Radial Acceleration Relation
• SH$\alpha$DE: Survey description and mass-kinematics scaling relations for dwarf galaxies
• Galaxy properties in the cosmic web of EAGLE simulation
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• The Thermal Sunyaev-Zel'dovich Effect from Massive, Quiescent 0.5 $\le$ z $\le$ 1.5 Galaxies
• The origin of X-ray coronae around simulated disc galaxies
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Exploring the dependence of the three-point correlation function on stellar mass and luminosity at 0.5<z<1.1
• Building robust AGN mock catalogs to unveil black hole evolution and for survey planning
• Galaxy Evolution at High Redshift: Obscured Star Formation, GRB Rates, Cosmic Reionization, and Missing Satellites
• Chemical evolution of giant molecular clouds in simulations of galaxies
• The stellar mass in and around isolated central galaxies: connections to the total mass distribution through galaxy-galaxy lensing in the Hyper Suprime-Cam survey
• On the Kinematics of Cold, Metal-enriched Galactic Fountain Flows in Nearby Star-forming Galaxies
• Formation of globular clusters with multiple stellar populations from massive gas clumps in high-z gas-rich dwarf galaxies
• Keck Spectroscopy of the Coma Cluster Ultra-Diffuse Galaxy Y358: Dynamical Mass in a Wider Context
• On the mass assembly of low-mass galaxies in hydrodynamical simulations of structure formation
• Strong lensing with superfluid dark matter
• KiDS+GAMA: The weak lensing calibrated stellar-to-halo mass relation of central and satellite galaxies
• Dark influences II: gas and star formation in minor mergers of dwarf galaxies with dark satellites
• Cosmology with velocity dispersion counts: an alternative to measuring cluster halo masses
• AGN and Dwarf Galaxy Gas Kinematics
• The survival of globular clusters in a cuspy Fornax
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• The effect of dark matter-dark radiation interactions on halo abundance -- a Press-Schechter approach
• The dominant origin of diffuse Ly$\alpha$ halos around LAEs explored by SED fitting and clustering analysis
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• CAVITY, Calar Alto Void Integral-field Treasury surveY and project extension
• Characterising Tidal Features Around Galaxies in Cosmological Simulations
• LoCuSS: The Near-Infrared Luminosity and Weak-Lensing Mass Scaling Relation of Galaxy Clusters
• Galaxy size trends as a consequence of cosmology
• Clustering Constraints on the Relative Sizes of Central and Satellite Galaxies
• Galaxy morphoto-Z with neural Networks (GaZNets). I. Optimized accuracy and outlier fraction from Imaging and Photometry
• Circumnuclear Media of Quiescent Supermassive Black Holes
• Unraveling the interplay between SIDM and baryons in MW halos: defining where baryons dictate heat transfer
• Incorporating baryon-driven contraction of dark matter halos in rotation curve fits
• Discovery of a red backsplash galaxy candidate near M81
• The buildup of galaxies and their spheroids: the contributions of mergers, disc instabilities and star formation
• TRINITY II: The Luminosity-dependent Bias of the Supermassive Black Hole Mass--Galaxy Mass Relation for Bright Quasars at $z=6$
• Some observational tests of a minimal galaxy formation model
• Local photoionization feedback effects on galaxies
• The present-day gas content of simulated field dwarf galaxies
• The changing circumgalactic medium over the last 10 Gyr I: physical and dynamical properties
• Reignited star formation in dwarf galaxies quenched during reionization
• Dark influences: imprints of dark satellites on dwarf galaxies
• Navarro-Frenk-White dark matter profile and the dark halos around disk systems
• BASS. XXXVI. Constraining the Local Supermassive Black Hole - Halo Connection with BASS DR2 AGN
• The evolution of star formation activity in galaxy groups
• Galactic winds - How to launch galactic outflows in typical Lyman-break galaxies
• From spirals to lenticulars: evidence from the rotation curves and mass models of three early-type galaxies
• The baryon cycle of Seven Dwarfs with superbubble feedback
• Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
• Similarities and uniqueness of Ly$\alpha$ emitters among star-forming galaxies at z=2.5
• Mass and size growth of early-type galaxies by dry mergers in cluster environments
• Tracing the Local Volume galaxy halo-to-stellar mass ratio with satellite kinematics
• Evolution of the Gas Mass Fraction of Progenitors to Today's Massive Galaxies: ALMA Observations in the CANDELS GOODS-S Field
• Effects of feedback on galaxies in the VELA simulations: elongation, clumps and compaction
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Hierarchical scaling and biasing
• The Case for Strangulation in Low-Mass Hosts: DDO 113
• A new class of dark matter-free dwarf galaxies? I. Clues from FCC 224, NGC 1052-DF2 and NGC 1052-DF4
• Mufasa:The strength and evolution of galaxy conformity in various tracers
• Quantifying the Origin and Distribution of Intracluster Light in a Fornax-like Cluster
• Magnetogenesis at Cosmic Dawn: Tracing the Origins of Cosmic Magnetic Fields
• Revisiting the bulge-halo conspiracy II: Towards explaining its puzzling dependence on redshift
• New empirical constraints on the cosmological evolution of gas and stars in galaxies
• Setting firmer constraints on the evolution of the most massive, central galaxies from their local abundances and ages
• Halo Histories vs. Galaxy Properties at z=0, III: The Properties of Star-Forming Galaxies
• Predicting fully self-consistent satellite richness, galaxy growth and starformation rates from the STastical sEmi-Empirical modeL STEEL
• Bar ages derived for the first time in nearby galaxies: Insights on secular evolution from the TIMER sample
• AMICO galaxy clusters in KiDS-DR3: galaxy population properties and their redshift dependence
• The Black Hole Mass Function Across Cosmic Times II. Heavy Seeds and (Super)Massive Black Holes
• Measuring Dark Matter in Galaxies: The Mass Fraction Within 5 Effective Radii
• The evolution of compact massive quiescent and starforming galaxies derived from the $R_e-R_h$ and $M_{\mathrm{star}}-M_h$ relations
• Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots
• Morphology of galaxies with quiescent recent assembly history in a Lambda-CDM universe
• EDGE: Dark matter core creation depends on the timing of star formation
• The Diversity of Growth Histories of Milky Way-mass Galaxies
• Stars on the edge: Galactic tides and the outskirts of the Sculptor dwarf spheroidal
• The frequency of very young galaxies in the local Universe: I. A test for galaxy formation and cosmological models
• The Chandra COSMOS Legacy Survey: clustering dependence of Type 2 AGN on host galaxy properties
• Exploring the High-Mass End of the Stellar Mass Function of Star Forming Galaxies at Cosmic Noon
• PANORAMIC: Discovery of an Ultra-Massive Grand-Design Spiral Galaxy at $z\sim 5.2$
• The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations
• Dependence of galaxy clustering on UV-luminosity and stellar mass at $z\sim 4-7$
• 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
• Normalized additional velocity distribution: testing the radial profile of dark matter halos and MOND
• A Study of Central Galaxy Rotation with Stellar Mass and Environment
• The Differing Relationships Between Size, Mass, Metallicity and Core Velocity Dispersion of Central and Satellite Galaxies
• The Impact of Environment on Late Time Evolution of the Stellar Mass - Halo Mass Relation
• The edge of galaxy formation III: The effects of warm dark matter on Milky Way satellites and field dwarfs
• Calibration of a star formation and feedback model for cosmological simulations with Enzo
• Brightest group galaxies-II: the relative contribution of BGGs to the total baryon content of groups at z<1.3
• On the Impact of Neutron Star Binaries Natal-Kick Distribution on the Galactic r-process Enrichment
• Energy transfer from baryons to dark matter as a unified solution to small-scale structure issues of the $\Lambda$CDM model
• MUSEQuBES: The relation between Ly$\alpha$ emitters and C IV absorbers at $z\approx 3.3$
• The Robustness of Cosmological Hydrodynamic Simulation Predictions to Changes in Numerics and Cooling Physics
• The Baryonic Collapse Efficiency of Galaxy Groups in the RESOLVE and ECO Surveys
• Late Bloomer Galaxies: Growing Up in Cosmic Autumn
• The tidal evolution of the Fornax dwarf spheroidal and its globular clusters
• Not-so-little Red Dots: Two massive and dusty starbursts at z~5-7 pushing the limits of star formation discovered by JWST in the COSMOS-Web survey
• Bulge formation through disc instability -- I
• WISDOM Project -- XIII. Feeding molecular gas to the supermassive black hole in the starburst AGN-host galaxy Fairall 49
• A shallow dark matter halo in Ultra Diffuse Galaxy AGC 242019: are UDGs structurally similar to low surface brightness galaxies?
• Using Artificial Neural Networks to Constrain the Halo Baryon Fraction during Reionization
• Stellar Kinematics and Environment at z~0.8 in the LEGA-C Survey: Massive, Slow-Rotators are Built First in Overdense Environments
• How feedback shapes galaxies: an analytic model
• The effects of local stellar radiation and dust depletion on non-equilibrium interstellar chemistry
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$. V: Properties of dark matter halos containing H$\alpha$ emitting galaxies
• The Properties of Radio and Mid-infrared Detected Galaxies and the Effect of Environment on the Co-evolution of AGN and Star Formation at $z\sim 1$
• A minimal empirical model for the cosmic far-infrared background anisotropies
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. IV. High Precision Constraints on the Evolution of Stellar-Halo Mass Relation at Redshift $z<0.7$
• Star formation in mergers with cosmologically motivated initial conditions
• Kinematics and Mass Distributions for Non-Spherical Deprojected Sérsic Density Profiles and Applications to Multi-Component Galactic Systems
• Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
• The frequency of very young galaxies in the local Universe: II. The view from SDSS spectra
• A Precise Benchmark for Cluster Scaling Relations: Fundamental Plane, Mass Plane and IMF in the Coma Cluster from Dynamical Models
• Testing galaxy formation models with galaxy stellar mass functions
• AGN must be very efficient at powering outflows
• Dwarf galaxies as a probe of a primordially magnetized Universe
• Detecting clusters and groups of galaxies populating the local Universe in large optical spectroscopic surveys
• Constraining Scatter in the Stellar Mass--Halo Mass Relation for Haloes Less Massive than the Milky Way
• The Origin of the Relation Between Stellar Angular Momentum and Stellar Mass in Nearby Disk-dominated galaxies
• Differentiable Predictions for Large Scale Structure with SHAMNet
• Constraining warm dark matter mass with cosmic reionization and gravitational wave
• The Luminosity Functions and Redshift Evolution of Satellites of Low-Mass Galaxies in the COSMOS Survey
• Effect of primordial non-Gaussianities on the far-UV luminosity function of high-redshift galaxies: implications for cosmic reionization
• A Holistic Review of a Galactic Interaction
• Modelling the formation of today's massive ellipticals
• What has quenched the massive spiral galaxies?
• On the dark matter haloes inner structure and galaxy morphology
• A systematic study of the inner rotation curves of galaxies observed as part of the GASS and COLD GASS surveys
• Spatially Resolved Gas-phase Metallicity in FIRE-2 Dwarfs: Late-Time Evolution of Metallicity Relations in Simulations with Feedback and Mergers
• Cosmic evolution of the H2 mass density and the epoch of molecular gas
• Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
• The Clustering of Undetected High-redshift Black Holes and Their Signatures in Cosmic Backgrounds
• MHONGOOSE discovery of a gas-rich low-surface brightness galaxy in the Dorado Group
• On the Edge: the relation between stellar and dark matter haloes of Milky Way-mass galaxies
• Galaxy-Galaxy Lensing in EAGLE: comparison with data from 180 square degrees of the KiDS and GAMA surveys
• The Galaxy Replacement Technique (GRT): a New Approach to Study Tidal Stripping and Formation of Intracluster Light in a Cosmological Context
• Light or heavy supermassive black hole seeds: the role of internal rotation in the fate of supermassive stars
• Satellite content and quenching of star formation in galaxy groups at z~1.8
• The CGM-GRB Study. I. Uncovering The CircumGalactic Medium around GRB hosts at redshifts 2-6
• Self-gravitating Equilibria of Non-minimally Coupled Dark Matter Halos
• Stellar Feedback and the Energy Budget of Late-Type Galaxies: Missing Baryons and Core Creation
• Constraining the subgrid physics in simulations of isolated dwarf galaxies
• Around the Spindle galaxy: the dark halo mass of NGC3115
• Dark matter fraction of low-mass cluster members probed by galaxy-scale strong lensing
• Recent progress in simulating galaxy formation from the largest to the smallest scales
• A too-many dwarf galaxy satellites problem in the M83 group
• Accurate Computation of the Screening of Scalar Fifth Forces in Galaxies
• A new gas cooling model for semi-analytical galaxy formation models
• HI intensity mapping correlation function from UNIT simulations: BAO and observationally induced anisotropy
• Ironing the folds: The phase space chevrons of a GSE-like merger as a dark matter subhalo detector
• HI within and around observed and simulated galaxy discs -- Comparing MeerKAT observations with mock data from TNG50 and FIRE-2
• Selecting ultra-faint dwarf candidate progenitors in cosmological N-body simulations at high redshifts
• Dark Matter in Fractional Gravity I: Astrophysical Tests on Galactic Scales
• The XMM-Newton Wide Field Survey in the COSMOS Field: Clustering Dependence of X-ray Selected AGN on Host Galaxy Properties
• The quenched mass portion of star-forming galaxies and the origin of the star formation sequence slope
• Simulating Deep Hubble Images With Semi-empirical Models of Galaxy Formation
• A universal angular momentum profile for dark matter haloes
• Tracing the co-evolution path of super massive black holes and spheroids with AKARI-selected ultra-luminous IR galaxies at intermediate redshifts
• Applying Noether's theorem to matter in the Milky Way: evidence for external perturbations and non-steady-state effects from Gaia Data Release 2
• CGM${}^2$ $+$ CASBaH: The Mass Dependence of H~I Ly$\alpha$-Galaxy Clustering and the Extent of the CGM
• Exploring Self-Interacting Dark Matter Halos with Diverse Baryonic Distributions: A Parametric Approach
• An empirical model to form and evolve galaxies in dark matter halos
• A Comparison of Outflow Properties in AGN Dwarfs vs. Star Forming Dwarfs
• Pre-supernova feedback mechanisms drive the destruction of molecular clouds in nearby star-forming disc galaxies
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• Probing the Diffuse Lyman-alpha Emission on Cosmological Scales: Lyα Emission Intensity Mapping Using the Complete SDSS-IV eBOSS Survey
• Evolution of CIV Absorbers. II. Where does CIV live?
• Shutting down or powering up a (U)LIRG? Merger components in distinctly different evolutionary states in IRAS 19115-2124 (The Bird)
• The weak dependence of velocity dispersion on disk fractions, mass-to-light ratio and redshift: Implications for galaxy and black hole evolution
• Ages and metallicities of quiescent galaxies: confronting broadband ($UVJ$) colours with stellar absorption lines
• Galaxy growth from redshift 5 to 0 at fixed comoving number density
• Age and metal gradients in massive quiescent galaxies at $0.6\lesssim z\lesssim 1.0$: implications for quenching and assembly histories
• Empirical estimation of host galaxy dispersion measure towards well localized fast radio bursts
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic survey. II. Morphology, Color and Size Dependences of the Stellar-halo Mass Relation for Massive Galaxies
• EDGE: the puzzling ellipticity of Eridanus II's star cluster and its implications for dark matter at the heart of an ultra-faint dwarf
• Cosmological interpretation of the color-magnitude diagrams of galaxy clusters
• A Two-Parameter Matching Scheme for Massive Galaxies and Dark Matter Haloes
• Galaxy mass-size segregation in the cosmic web from the CAVITY parent sample
• The signal of decaying dark matter with hydrodynamical simulations
• RABBITS -- II. The impact of AGN feedback on coalescing supermassive black holes in disc and elliptical galaxy mergers
• The Tail of Late-forming Dwarf Galaxies in $\Lambda$CDM
• Connection between galaxy morphology and dark-matter halo structure I: a running threshold for thin discs and size predictors from the dark sector
• The abundance and colours of galaxies in high redshift clusters in the cold dark matter cosmology
• Auriga Streams I: disrupting satellites surrounding Milky Way-mass haloes at multiple resolutions
• The Fundamental Plane Relation of Early-Type Galaxies: Environmental Dependence
• The detection of ultra-faint low surface brightness dwarf galaxies in the Virgo Cluster: a Probe of Dark Matter and Baryonic Physics
• Abundance matching for low mass galaxies in the CDM and FDM models
• Bursty Star Formation in Dwarfs is Sensitive to Numerical Choices in Supernova Feedback Models
• Gravity and the Nonlinear Growth of Structure in the Carnegie-Spitzer-IMACS Redshift Survey
• The Stellar Mass - Halo Mass Relation for Low Mass X-ray Groups at 0.5<z<1 in the CDFS with CSI
• The GMRT archive atomic gas survey -- II. Mass modelling and dark matter halo properties across late-type spirals
• A galactic outflow traced by its extended Mg II emission out to a $\sim 30$ kpc radius in the Hubble Ultra Deep Field with MUSE
• Properties of the circumgalactic medium in simulations compared to observations
• Damped Lyman-$\alpha$ absorbers and atomic hydrogen in galaxies: the view of the GAEA model
• Using large galaxy surveys to distinguish z~0.5 quiescent galaxy models
• Using KCWI to Explore the Chemical Inhomogeneities and Evolution of J1044+0353
• The Magellanic Clouds are very rare in the IllustrisTNG simulations
• Disk galaxies are self-similar: the universality of the HI-to-Halo mass ratio for isolated disks
• GABE: Galaxy Assembly with Binary Evolution
• Growth of Massive Black Hole Seeds by Migration of Stellar and Primordial Black Holes: Gravitational Waves and Stochastic Background
• Constraints on galaxy formation from the cosmic-far-infrared-background\,$-$\,optical-imaging cross-correlation using \textit{Herschel} and UNIONS
• ARTEMIS emulator: exploring the effect of cosmology and galaxy formation physics on Milky Way-mass haloes and their satellites
• Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies in the Local Universe II. -- Direct Measurement of the Dependencies on Redshift and Host Halo Mass of Stellar Mass Growth in Central Disk Galaxies
• The impact of the halo spin-concentration relation on disc scaling laws
• PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at $0.2<z<0.9$
• Characterizing simulated galaxy stellar mass histories
• Co-Evolution vs. Co-existence: The Effect of Accretion Modelling on the Evolution of Black Holes and Host Galaxies
• Exploring galaxy dark matter halos across redshifts with strong quasar absorbers
• Mass-morphology relation of TNG50 galaxies
• The Dark Matter Halos of HI Selected Galaxies
• Type Ia Supernova Magnitude Step from the local Dark Matter Environment
• Galaxy assembly bias in the stellar-to-halo mass relation for red central galaxies from SDSS
• Evidence of Extended Dust and Feedback around z$\approx$1 Quiescent Galaxies via Millimeter Observations
• A physically motivated galaxy size definition across different state-of-the-art hydrodynamical simulations
• Constraining dark matter annihilation with HSC Low Surface Brightness Galaxies
• Accurate Measurement of the Lensing Magnification by BOSS CMASS Galaxies and Its Implications for Cosmology and Dark Matter
• Comparing Galaxy Clustering in Horizon-AGN Simulated Lightcone Mocks and VIDEO Observations
• Search for Missing Links Between Two Extreme Wind Speed Profiles : Dark Energy Accretion and Adiabatic Fluid Accretion
• MusE GAs FLOw and Wind (MEGAFLOW) XI. Scaling relations between outflows and host galaxy properties
• Accreting Black Holes in Dark Matter Halos
• The Formation of a Milky Way-sized Disk Galaxy 1. A Comparison of Numerical Methods
• NIHAO XXVIII: Collateral effects of AGN on dark matter concentration and stellar kinematics
• LARgE Survey -- II. The Dark Matter Halos and the Progenitors and Descendants of Ultra-Massive Passive Galaxies at Cosmic Noon
• Probing gaseous halos of galaxies with radio jets
• EMERGE: Constraining merging probabilities and timescales of close galaxy pairs
• The extended Planetary Nebula Spectrograph (ePN.S) early-type galaxy survey: The specific angular momentum of ETGs
• Globular Cluster Counts around 700 Nearby Galaxies
• From Gas to Stars Over Cosmic Time
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• The variation of the gas content of galaxy groups and pairs compared to isolated galaxies
• MaNGA AGN dwarf galaxies (MAD) -- II. AGN outflows in dwarf galaxies
• Modeling the Cosmic Dispersion Measure in the D < 120 Mpc Local Universe
• A partial Lyman limit system tracing intragroup gas at $z\approx 0.8$ towards HE1003+0149
• The Isophotal Structure of Star-forming Galaxies at $0.5<z<1.8$ in CANDELS: Implications for the Evolution of Galaxy Structure
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• Abundance matching tested on small scales with galaxy dynamics
• Early-type galaxy density profiles from IllustrisTNG: III. Effects on outer kinematic structure
• The significant effects of stellar mass estimation on galaxy pair fractions
• A break in the high-redshift stellar mass Tully-Fisher relation
• No Evolution in the Half-mass Radius of Milky Way-type Galaxies over the Last 10 Gyr
• Predictions for Detecting a Turndown in the Baryonic Tully Fisher Relation
• An Escaping Outflow in a Galaxy with an Intermediate-mass Black Hole
• Shape noise and dispersion in precision weak lensing
• The velocity function of dark matter halos at r=20 kpc: Remarkably little evolution since z ~ 4
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• Toward a stellar population catalog in the Kilo Degree Survey: the impact of stellar recipes on stellar masses and star formation rates
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• Dynamical Properties of Molecular-forming Gas Clumps in Galaxies at the Epoch of Reionization
• The properties and environment of very young galaxies in the local Universe
• A physical model for the redshift evolution of high-z Lyman-Break Galaxies
• HELLO project: High-$z$ Evolution of Large and Luminous Objects
• AGN lifetimes in UV-selected galaxies: a clue to supermassive black hole-host galaxy coevolution
• The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data
• The Noctua Suite of Simulations -- The Difficulty of Growing Massive Black Holes in Low-Mass Dwarf Galaxies
• Decoupled Black Hole Accretion and Quenching: The Relationship Between BHAR, SFR, and Quenching in Milky Way and Andromeda-mass Progenitors Since z = 2.5
• Subhalo abundance matching using progenitor mass at varying redshift: Two modes of stellar mass growth imprinted into the Subaru HSC galaxy clustering
• Isolated dark matter deprived galaxies in hydrodynamical simulations: real objects or artefacts?
• Galaxy-galaxy lensing in the VOICE deep survey
• Testing galaxy formation models with the stellar mass-halo mass relations for star-forming and quiescent galaxies
• The dynamical impact of cosmic rays in the Rhea magnetohydrodynamics simulations
• Intertwined Formation of ${\mathrm{H}}_2$, Dust, and Stars in Cosmological Simulations
• MaNGA AGN dwarf galaxies (MAD). III. The role of mergers and environment in active galactic nucleus activity in dwarf galaxies
• Globular Cluster Systems and X-Ray Atmospheres in Galaxies
• Anatomy of galactic star formation history: Roles of different modes of gas accretion, feedback, and recycling
• Flattening of dark matter cusps during mergers: model of M31
• The galaxy counterpart of the high-metallicity and 16 kpc impact parameter DLA towards Q0918+1636 - a challenge to galaxy formation models?
• Galaxy kinematics across different environments in the RXJ1347-1145 cluster complex
• Massive dusty multiphase outflow in local merger shows no sign of slowing on kiloparsec scales
• Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra-I cluster IV. A study of the Globular Cluster population in four UDGs
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Modelling the selection of galaxy groups with end to end simulations
• An H$\alpha$ kinematic survey of the $Herschel$ Reference Survey -- I. Fabry-Perot observations with the 1.93m telescope at OHP
• The Milky Way in context: The formation of galactic discs and chemical sequences from a cosmological perspective
• Diving into dangerous tides: The impact of galaxy cluster tidal environments on satellite galaxy mass densities
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• The SRG/eROSITA All-Sky Survey. The Weak-Lensing Mass Calibration and the Stellar Mass-to-Halo Mass Relation from the Hyper Suprime-Cam Subaru Strategic Program
• Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
• Star formation and stellar & AGN feedback in the absence of accretion, not gas stripping, set the quenching timescale in satellite galaxies
• The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
• The inflow and outflow rate evolution of local Milky Way-mass star-forming galaxies since z=1.3
• Clues to the nature of dark matter from first galaxies
• Fundamental properties of the dark and the luminous matter from Low Surface Brightness discs
• Galaxy Assembly and Evolution in the P-Millennium simulation: galaxy clustering
• Quenching vs. Quiescence: forming realistic massive ellipticals with a simple starvation model
• Spatial Distribution of OVI Covering Fractions in the Simulated Circumgalactic Medium
• MaNGA DynPop. VII. A Unified Bulge-Disk-Halo Model for Explaining Diversity in Circular Velocity Curves of 6000 Spiral and Early-Type Galaxies
• Hubble Space Telescope Captures UGC~12591: Bulge/Disc Properties, Star Formation and `Missing Baryons' Census in a Very Massive and Fast Spinning Hybrid Galaxy
• A Shallow Slope for the Stellar Mass--Angular Momentum Relation of Star-Forming Galaxies at $1.5<z<2.5$
• Improved SED-Fitting Assumptions Result in Inside-Out Quenching at $z\sim 0.5$ and Quenching at All Radii Simultaneously at $z\sim 1$
• Cosmological prior for the $J$-factor estimation of dwarf spheroidal galaxies
• How do the dynamics of the Milky Way -- Large Magellanic Cloud system affect gamma-ray constraints on particle dark matter?
• Predicting HCN, HCO${}^{+}$, multi-transition CO, and dust emission of star-forming galaxies -- Extension to luminous infrared galaxies and the role of cosmic ray ionization
• Improving photometric redshifts with Ly$\alpha$ tomography
• Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• Barions and $\Lambda$CDM Model Problems
• A path towards constraining the evolution of the interstellar medium and outflows in the Milky Way using APOGEE
• The origin of galaxy colour bimodality in the scatter of the Stellar-to-Halo Mass Relation
• Deciphering Baryonic Feedback from ACT tSZ Galaxy Clusters
• LATIS: Comparing Galaxy and IGM Tomography Maps as Tracers of Large-scale Structure and Protoclusters at $z\sim 2.5$
• Associations of dwarf galaxies in a $\Lambda$CDM Universe
• Modelling the Evolution of Ly$\alpha$ Blobs and Ly$\alpha$ Emitters
• IllustrisTNG + Cosmic Rays with a Simple Transport Model: From Dwarfs to L${}^{\star }$ Galaxies
• Relatively Fast and Reasonably Furious: Evidence for Increased Burstiness in Smaller Halos at Cosmic Dawn
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations -- II. Constraining cosmology and astrophysical processes with early- and late-type galaxies
• Impact of supermassive black hole growth on star formation
• The "Little Dark Dot": Evidence for Self-interacting Dark Matter in the Strong Lens SDSS J0946+1006?
• A Recent Starbust in the Low Surface Brightness Galaxy UGC 628
• Neutral hydrogen in the post-reionization universe
• The environmental dependence of the stellar mass fundamental plane of early-type galaxies
• The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
• Dark energy, spatial curvature, and star formation efficiency from JWST photometric and spectroscopic high-redshift galaxies
• Updated Models for the Creation of a Low-z QSO Absorber by a Dwarf Galaxy Wind
• Build-up and survival of the disc: From numerical models of galaxy formation to the Milky Way
• A Bending in the Size-mass Relation of Star-forming Galaxies across $0.5<z<6.0$ at a Critical Stellar Mass of $10^{10}{M}_{\odot }$ Revealed by JWST
• HI-bearing dark galaxies predictions from constrained Local Group simulations: how many and where to find them
• SEMPER I. Radio Predictions for Star-Forming Galaxies at $0<z<5$
• Mapping luminous and dark matter in the Universe
• What is the right way to quench star formation in semi-analytic model of galaxy formation?
• Exploring Milky Way rotation curves with Gaia DR3: a comparison between $\Lambda$CDM, MOND, and General Relativistic approaches
• Estimating the contribution of foreground halos to the FRB 180924 dispersion measure
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• The Role of Mass and Environment on Satellite distributions around Milky Way analogs in the Romulus25 simulation
• Probabilistic Inference of the Structure and Orbit of Milky Way Satellites with Semi-Analytic Modeling
• JERALD: high-fidelity dark matter, stellar mass and neutral hydrogen maps from fast N-body simulations
• The Origin of the Gas and Its Low Star Formation Efficiency in Quiescent Galaxies
• Measuring the Stellar-to-Halo Mass Relation at $\sim 10^{10}$ Solar masses, using forthcoming space-based imaging of galaxy-galaxy strong lenses
• How Many Bursts Does it Take to Form a Core at the Center of a Galaxy?
• Insights into the dependence of galaxy properties on the environment with explainable machine learning models
• Recoiling supermassive black holes in analytical and numerical galaxy potential
• Self-Interacting Dark Matter with Mass Segregation: A Unified Explanation of Dwarf Cores and Small-Scale Lenses
• Reconstructing the mass accretion histories of nearby Red Nuggets with their globular cluster systems
• AGN with massive black holes have closer galactic neighbors: k-Nearest-Neighbor statistics of an unbiased sample of AGN at z~0.03
• Bridging Simulations and Observations: New Insights into Galaxy Formation Simulations via Out-of-Distribution Detection and Bayesian Model Comparison
• The Lowest Metallicity Stars in the LMC: Clues from MaGICC Simulations
• Magnetic fields in galactic environments probed by Fast Radio Bursts
• Gas thermodynamics meets galaxy kinematics: Joint mass measurements for eROSITA galaxy clusters
• Extended Hernquist-Springel formalism for cosmic star formation
• Mapping the Distorted Dark Matter Distribution of the LMC-SMC System Prior to Milky Way Infall with Basis Function Expansions
• Baryon-driven decontraction in Milky Way mass haloes
• An Enhanced Isothermal Jeans Approach to Constraining Dark Matter Self-Interactions from Galactic Kinematics
• Photometric Objects Around Cosmic Webs (PAC). VI. High Satellite Fraction of Quasars
• Probing baryonic feedback with fast radio bursts: joint analyses with cosmic shear and galaxy clustering
• On the Tidal Formation of Dark Matter Deficient Galaxies
• Testing the key role of the stellar mass-halo mass relation in galaxy merger rates and morphologies via DECODE, a novel Discrete statistical sEmi-empiriCal mODEl
• Large Molecular Gas Reservoirs in Ancestors of Milky Way-Mass Galaxies 9 Billion Years Ago
• The orbital dynamics of the LMC and SMC about the Milky Way
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
• The effects of self-interacting dark matter on the stripping of galaxies that fall into clusters
• A Near-Infrared look at AGN Feedback in Bulgeless Galaxies
• Hierarchal formation and growth of galaxies through dynamical friction
• Spatially resolved stellar-to-total dynamical mass relation: Radial variations, gradients and profiles of galaxy stellar populations
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• Cross-checking SMBH mass estimates in NGC 6958 -- I: Stellar dynamics from adaptive optics-assisted MUSE observations
• Dwarf Galaxy Number Counts within 25 Mpc: Predictions from Local Group Analogues in TNG50
• Resolved molecular gas and star-formation in massive unquenched spirals : I. UGC 8179
• Bridging Galaxy Dynamics and Baryon Efficiency of 40 EDGE-CALIFA galaxies
• Initial Mass Function for Massive Galaxies at z$\sim$1
• The NIKA2 cosmological legacy survey at 2 mm: catalogs, colors, redshift distributions, and implications for deep surveys
• The satellite population around luminous red galaxies in the 25 square degree DESI Legacy Imaging Surveys Early Data Release
• LYRA II: Cosmological dwarf galaxy formation with inhomogeneous Population III enrichment
• Controlled Experiments on Dark-Matter Halo Structure and Galaxy Morphology I: What Sets Galaxy Sizes?
• The Cen A galaxy group: dynamical mass and missing baryons
• Estimating major merger rates and spin parameters ab initio via the clustering of critical events
• The tidal evolution of satellite galaxies in cosmological simulations: insights from COLIBRE
• Clustering properties of TGSS radio sources
• The odd primordial halo of the Milky Way implied by Gaia. A shallow core, but a steep decline
• CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA
• The vertical structure of the stellar disk in NGC 551
• Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter
• Tracing the evolution of brightest galaxies and diffuse light in galaxy groups
• Rapid sinking and efficient mergers of supermassive black holes in compact high-redshift galaxies
• Challenges of standard halo models in constraining galaxy properties from CIB anisotropies
• A Mass Dependent Density Profile from Dwarfs to Clusters