The Average Star Formation Histories of Galaxies in Dark Matter Halos from z=0-8

Abstract

We present a robust method to constrain average galaxy star formation rates, star formation histories, and the intracluster light as a function of halo mass. Our results are consistent with observed galaxy stellar mass functions, specific star formation rates, and cosmic star formation rates from z=0 to z=8. We consider the effects of a wide range of uncertainties on our results, including those affecting stellar masses, star formation rates, and the halo mass function at the heart of our analysis. As they are relevant to our method, we also present new calibrations of the dark matter halo mass function, halo mass accretion histories, and halo-subhalo merger rates out to z=8. We also provide new compilations of cosmic and specific star formation rates; more recent measurements are now consistent with the buildup of the cosmic stellar mass density at all redshifts. Implications of our work include: halos near 10^12 Msun are the most efficient at forming stars at all redshifts, the baryon conversion efficiency of massive halos drops markedly after z ~ 2.5 (consistent with theories of cold-mode accretion), the ICL for massive galaxies is expected to be significant out to at least z ~ 1-1.5, and dwarf galaxies at low redshifts have higher stellar mass to halo mass ratios than previous expectations and form later than in most theoretical models. Finally, we provide new fitting formulae for star formation histories that are more accurate than the standard declining tau model. Our approach places a wide variety of observations relating to the star formation history of galaxies into a self-consistent framework based on the modern understanding of structure formation in LCDM. Constraints on the stellar mass-halo mass relationship and star formation rates are available for download at http://www.peterbehroozi.com/data.html .

Revised to match ApJ accepted version, with additional corrections to Figs. 18+19 (superseding published version)

References in corpus (32)

• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• Star Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies
• The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies
• K-corrections and filter transformations in the ultraviolet, optical, and near infrared
• UV Star Formation Rates in the Local Universe
• Galactic star formation and accretion histories from matching galaxies to dark matter haloes
• Transients from Initial Conditions in Cosmological Simulations
• The stellar mass assembly of galaxies from z=0 to z=4. Analysis of a sample selected in the rest-frame near-infrared with Spitzer
• Galaxy Evolution from Halo Occupation Distribution Modeling of DEEP2 and SDSS Galaxy Clustering
• PRIMUS: Constraints on Star Formation Quenching and Galaxy Merging, and the Evolution of the Stellar Mass Function From z=0-1
• Keck Spectroscopy of 3<z<7 Faint Lyman Break Galaxies: The Importance of Nebular Emission in Understanding the Specific Star Formation Rate and Stellar Mass Density
• The Spectral Energy Distributions Of z~8 Galaxies From The IRAC Ultra Deep Fields: Emission Lines, Stellar Masses, And Specific Star Formation Rates At 650 Myr
• On the Lack of Evolution in Galaxy Star Formation Efficiency
• The Galaxy Content of SDSS Clusters and Groups
• The Hierarchical Build-Up of Massive Galaxies and the Intracluster Light since z=1
• The Evolution of Stellar Mass and the Implied Star Formation History
• On the galaxy stellar mass function, the mass-metallicity relation, and the implied baryonic mass function
• The dependence of Star Formation on Galaxy Stellar Mass
• The star-formation history of K-selected galaxies
• Rapid dust production in submillimeter galaxies at z>4?
• The History of Cosmological Star Formation: Three Independent Approaches and a Critical Test Using the Extragalactic Background Light
• The H-alpha Luminosity Function and Star Formation Rate Volume Density at z=0.8 from the NEWFIRM H-alpha Survey
• MOIRCS Deep Survey IV: Evolution of Galaxy Stellar Mass Function Back to z ~ 3
• Dissecting the stellar mass-SFR correlation in z=1 star-forming disk galaxies
• Mapping the Dark Matter From UV Light at High Redshift: An Empirical Approach to Understand Galaxy Statistics
• The dust un-biased cosmic star formation history from the 20 cm VLA-COSMOS survey
• MOIRCS Deep Survey. VIII. Evolution of Star Formation Activity as a Function of Stellar Mass in Galaxies since z~3
• Carbon-Enhanced Metal-Poor Stars, the Cosmic Microwave Background, and the Stellar IMF in the Early Universe
• Modeling the three-point correlation function
• Rhapsody. II. Subhalo Properties and the Impact of Tidal Stripping From a Statistical Sample of Cluster-Size Halos
• A Census of Star-Forming Galaxies at z = 1-3 in the Subaru Deep Field
• Evidence for merging or disruption of red galaxies from the evolution of their clustering

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• Modeling the Formation of Globular Cluster Systems in the Virgo Cluster
• AREPO-RT: Radiation hydrodynamics on a moving mesh
• Systematics in virial mass estimators for pressure-supported systems
• Measuring the star formation rate with gravitational waves from binary black holes
• Rotation Curves in z~1-2 Star-Forming Disks: Evidence for Cored Dark Matter Distributions
• Stellar Absorption Line Analysis of Local Star-Forming Galaxies: The Relation Between Stellar Mass, Metallicity, Dust Attenuation and Star Formation Rate
• Timing the Early Assembly of the Milky Way with the H3 Survey
• Semi-analytic forecasts for JWST -- II. physical properties and scaling relations for galaxies at z = 4-10
• Limit on the LMC mass from a census of its satellites
• The stellar-to-halo mass relations of local galaxies segregates by color
• Globular clusters indicate ultra diffuse galaxies are dwarfs
• The Impact of Modeling Assumptions in Galactic Chemical Evolution Models
• Formation of Globular Cluster Systems: From Dwarf Galaxies to Giants
• Space Warps II. New Gravitational Lens Candidates from the CFHTLS Discovered through Citizen Science
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Motivation, Design and Target Catalogue
• Satellite Dwarf Galaxies in a Hierarchical Universe: The Prevalence of Dwarf-Dwarf Major Mergers
• On the kinematic detection of accreted streams in the Gaia era: a cautionary tale
• The Star Formation Histories of Local Group Dwarf Galaxies III. Characterizing Quenching in Low-Mass Galaxies
• Lensing substructure quantification in RXJ1131-1231: A 2 keV lower bound on dark matter thermal relic mass
• The Diversity and Variability of Star Formation Histories in Models of Galaxy Evolution
• z~2-9 Galaxies Magnified by the Hubble Frontier Field Clusters II: Luminosity Functions and Constraints on a Faint-End Turnover
• The COSMOS2015 galaxy stellar mass function: 13 billion years of stellar mass assembly in 10 snapshots
• X-rays across the galaxy population I: tracing the main sequence of star formation
• The galaxy UV luminosity function at z ~ 2 - 4; new results on faint-end slope and the evolution of luminosity density
• Discovery of a dark, massive, ALMA-only galaxy at z~5-6 in a tiny 3-millimeter survey
• Shadows in the Dark: Low-Surface-Brightness Galaxies Discovered in the Dark Energy Survey
• Spatially-resolved stellar kinematics of the ultra diffuse galaxy Dragonfly 44. I. Observations, kinematics, and cold dark matter halo fits
• The stellar accretion origin of stellar population gradients in massive galaxies at large radii
• A Comparison between Semi-Analytic Model Predictions for the CANDELS Survey
• Inspiraling Halo Accretion Mapped in Lyman-$\alpha$ Emission around a $z\sim 3$ Quasar
• The Column Density, Kinematics, and Thermal State of Metal-Bearing Gas within the Virial Radius of z~2 Star-Forming Galaxies in the Keck Baryonic Structure Survey
• FIREbox: Simulating galaxies at high dynamic range in a cosmological volume
• 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
• The Eating Habits of Milky Way Mass Halos: Destroyed Dwarf Satellites and the Metallicity Distribution of Accreted Stars
• The X-shooter/ALMA Sample of Quasars in the Epoch of Reionization. II. Black Hole Masses, Eddington Ratios, and the Formation of the First Quasars
• Modelling the number density of Halpha emitters for future spectroscopic near-IR space missions
• First predictions of the angular power spectrum of the astrophysical gravitational wave background
• Linking black-hole growth with host galaxies: The accretion-stellar mass relation and its cosmic evolution
• The REQUIEM Survey I: A Search for Extended Ly-Alpha Nebular Emission Around 31 z>5.7 Quasars
• 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
• Sample variance in the local measurements of the Hubble constant
• Galactic Winds in Low-Mass Galaxies
• The Impact of Galactic Feedback on the Circumgalactic Medium
• New reaction rates for improved primordial D/H calculation and the cosmic evolution of deuterium
• Quenching as a Contest between Galaxy Halos and their Central Black Holes
• The redshift-evolution of the distribution of star formation among dark matter halos as seen in the infrared
• The sizes of $z\sim 6-8$ lensed galaxies from the Hubble Frontier Fields Abell 2744 data
• Kiloparsec Scale Properties of Star-Formation Driven Outflows at z~2.3 in the SINS/zC-SINF AO Survey
• Stochastic modeling of star-formation histories I: the scatter of the star-forming main sequence
• The stellar-to-halo mass relation for Local Group galaxies
• HerMES: ALMA Imaging of Herschel-selected Dusty Star-forming Galaxies
• Spitzer bright, UltraVISTA faint sources in COSMOS: the contribution to the overall population of massive galaxies at z=3-7
• Early formation of massive, compact, spheroidal galaxies with classical profiles by violent disc instability or mergers
• Predicting the binary black hole population of the Milky Way with cosmological simulations
• Dark Matter Halos in Galaxies and Globular Cluster Populations. II: Metallicity and Morphology
• Is Main Sequence Galaxy Star Formation Controlled by Halo Mass Accretion?
• Dark Energy Survey Year 1 results: Detection of Intra-cluster Light at Redshift $\sim$ 0.25
• A small-scale dynamo in feedback-dominated galaxies as the origin of cosmic magnetic fields - I. The kinematic phase
• Overconsumption, outflows and the quenching of satellite galaxies
• A Lonely Giant: The Sparse Satellite Population of M94 Challenges Galaxy Formation
• Quenching of Star Formation in SDSS Groups: Centrals, Satellites, and Galactic Conformity
• Star Formation and AGN Activity in Galaxy Clusters from $z=1-2$: a Multi-wavelength Analysis Featuring $Herschel$/PACS
• Spatially Resolved Star Formation and Inside-out Quenching in the TNG50 Simulation and 3D-HST Observations
• ZOMG-I. How the cosmic web inhibits halo growth and generates assembly bias
• Demographics of Star-forming Galaxies since $z\sim 2.5$. I. The $UVJ$ Diagram in CANDELS
• Flat rotation curves and low velocity dispersions in KMOS star-forming galaxies at z~1
• The MASSIVE Survey - VII. The Relationship of Angular Momentum, Stellar Mass and Environment of Early-Type Galaxies
• NIHAO IX: the role of gas inflows and outflows in driving the contraction and expansion of cold dark matter haloes
• COPSS II: The Molecular Gas Content of Ten Million Cubic Megaparsecs at $z\sim 3$
• Identifying true satellites of the Magellanic Clouds
• Revealing the galaxy-halo connection in IllustrisTNG
• On the origin of the fundamental metallicity relation and the scatter in galaxy scaling relations
• Infrared color selection of massive galaxies at z > 3
• Star formation in galaxies at z~4-5 from the SMUVS survey: a clear starburst/main-sequence bimodality for Halpha emitters on the SFR-M* plane
• A survey of high-$z$ galaxies: SERRA simulations
• Energy equipartition between stellar and dark matter particles in cosmological simulations results in spurious growth of galaxy sizes
• Detection of the LMC-induced sloshing of the Galactic halo
• Faint dwarfs as a test of DM models: WDM vs. CDM
• MusE GAs FLOw and Wind (MEGAFLOW) I: First MUSE results on background quasars
• Colours, Star formation Rates, and Environments of Star forming and Quiescent Galaxies at the Cosmic Noon
• A lower fragmentation mass scale in high redshift galaxies and its implications on giant clumps: a systematic numerical study
• Modelling the large scale structure of the Universe as a function of cosmology and baryonic physics
• Galaxies in the EAGLE hydrodynamical simulation and in the Durham and Munich semi-analytical models
• Supermassive black holes as the regulators of star formation in central galaxies
• Molecular clouds in the Cosmic Snake normal star-forming galaxy 8 billion years ago
• The Obelisk simulation: galaxies contribute more than AGN to HI reionization of protoclusters
• Probing Cosmic Dawn with Emission Lines: Predicting Infrared and Nebular Line Emission for ALMA and JWST
• Spectroscopic Confirmation of a Protocluster at $z=3.37$ with a High Fraction of Quiescent Galaxies
• Dark matters on the scale of galaxies
• Wide-Field Survey of Dwarf Satellite Systems Around 10 Hosts in the Local Volume
• What Causes The Formation of Disks and End of Bursty Star Formation?
• Early-type Host Galaxies of Type Ia Supernovae. II. Evidence for Luminosity Evolution in Supernova Cosmology
• Hot-mode accretion and the physics of thin-disk galaxy formation
• The Progenitors of Local Ultra-massive Galaxies Across Cosmic Time: from Dusty Star-bursting to Quiescent Stellar Populations
• The Bursty Star Formation Histories of Low-mass Galaxies at $0.4<z<1$ Revealed by Star Formation Rates Measured from H$\beta$ and FUV
• SHAM Beyond Clustering: New Tests of Galaxy-Halo Abundance Matching with Galaxy Groups
• The Most Massive Galaxies and Black Holes Allowed by $\Lambda$CDM
• SCORCH I: The Galaxy-Halo Connection in the First Billion Years
• The route to massive black hole formation via merger-driven direct collapse: a review
• COSMOS2020: The cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z~5
• Galaxies in the Illustris simulation as seen by the Sloan Digital Sky Survey - II: Size-luminosity relations and the deficit of bulge-dominated galaxies in Illustris at low mass
• Far-infrared surveys of galaxy evolution
• The Scaling of Stellar Mass and Central Stellar Velocity Dispersion for Quiescent galaxies at z < 0.7
• 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
• High Angular Momentum Halo Gas: a Feedback and Code-Independent Prediction of LCDM
• The Nature of Massive Transition Galaxies in CANDELS, GAMA, and Cosmological Simulations
• A Keck Survey of Gravitationally-Lensed Star-Forming Galaxies: High Spatial Resolution Studies of Kinematics and Metallicity Gradients
• Predictions for the spatial distribution of the dust continuum emission in 1<z<5 star-forming galaxies
• The formation of massive, quiescent galaxies at cosmic noon
• Observations of environmental quenching in groups in the 11 Gyr since z=2.5: different quenching for central and satellite galaxies
• 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
• Going, going, gone dark: Quantifying the scatter in the faintest dwarf galaxies
• Black-Hole Growth is Mainly Linked to Host-Galaxy Stellar Mass rather than Star Formation Rate
• The evolving far-IR galaxy luminosity function and dust-obscured star-formation rate density out to z~5
• Galaxy and Mass Assembly (GAMA): The halo mass of galaxy groups from maximum-likelihood weak lensing
• Line Overlap and Self-Shielding of Molecular Hydrogen in Galaxies
• The dependence of cosmic ray driven galactic winds on halo mass
• A Systematic Look at the Effects of Radiative Feedback on Disc Galaxy Formation
• Surveying Galaxy Proto-clusters in Emission: A Large-scale Structure at z=2.44 and the Outlook for HETDEX
• When and where did GW150914 form?
• Hyper Suprime-Cam Subaru Strategic Program: A Mass-Dependent Slope of the Galaxy Size-Mass Relation at $z<1$
• Coming of Age in the Dark Sector: How Dark Matter Haloes grow their Gravitational Potential Wells
• The bright-end galaxy candidates at z ~ 9 from 79 independent HST fields
• The rise and fall of the star formation histories of blue galaxies at redshifts 0.2<z<1.4
• NIHAO-UHD: The properties of MW-like stellar disks in high resolution cosmological simulations
• Which galaxies dominate the neutral gas content of the Universe?
• Chandra centres for COSMOS X-ray galaxy groups: Differences in stellar properties between central dominant and offset brightest group galaxies
• On the OVI Abundance in the Circumgalactic Medium of Low-Redshift Galaxies
• Missing dark matter in dwarf galaxies?
• Characterizing Intra-cluster light in the Hubble Frontier Fields
• MAHALO Deep Cluster Survey I. Accelerated and enhanced galaxy formation in the densest regions of a protocluster at z=2.5
• On the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7<z<2.8
• Baryonic effects for weak lensing. Part I. Power spectrum and covariance matrix
• Introducing the FirstLight project: UV luminosity function and scaling relations of primeval galaxies
• The ACS LCID project. X. The Star Formation History of IC 1613: Revisiting the Over-Cooling Problem
• Spatially unassociated galaxies contribute significantly to the blended submillimetre galaxy population: predictions for follow-up observations of ALMA sources
• Relations Between the Sizes of Galaxies and their Dark Matter Halos at Redshifts $0<z<3$
• 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
• Searching for Traces of Planck-Scale Physics with High Energy Neutrinos
• Reconciling the observed star-forming sequence with the observed stellar mass function
• Impact of inter-correlated initial binary parameters on double black hole and neutron star mergers
• Observational evidence of a slow downfall of star formation efficiency in massive galaxies during the last 10 Gyr
• Dust, CO and [CI]: Cross-calibration of molecular gas mass tracers in metal-rich galaxies across cosmic time
• Dark Matter Cores and Cusps in Spiral Galaxies and their Explanations
• The properties of the first galaxies in the BLUETIDES simulation
• The MOSDEF survey: a census of AGN-driven ionized outflows at $z=1.4-3.8$
• Evolution of cosmic star formation in the SCUBA-2 Cosmology Legacy Survey
• Simulated Milky Way analogues: implications for dark matter indirect searches
• Abundance matching with the mean star formation rate: there is no missing satellites problem in the Milky Way above ${\mathbf{M}}_{200}\sim 10^9{\mathbf{M}}_{\odot }$
• Escape of ionizing radiation from high redshift dwarf galaxies: role of AGN feedback
• Baryon Cycling in the Low-Redshift Circumgalactic Medium: A Comparison of Simulations to the COS-Halos Survey
• Fast Molecular Outflow from a Dusty Star-Forming Galaxy in the Early Universe
• Star Cluster Formation in Cosmological Simulations. II. Effects of Star Formation Efficiency and Stellar Feedback
• Consequences of bursty star formation on galaxy observables at high redshifts
• A Minimalist Feedback-Regulated Model for Galaxy Formation During the Epoch of Reionization
• Galactic rotation curves, the baryon-to-dark-halo-mass relation and space-time scale invariance
• Ultraviolet to infrared emission of z>1 galaxies: Can we derive reliable star formation rates and stellar masses?
• Expanded haloes, abundance matching and too-big-to-fail in the Local Group
• JADES: The incidence rate and properties of galactic outflows in low-mass galaxies across 3 < z < 9
• \textsc{The Three Hundred} project: The \textsc{Gizmo-Simba} run
• ALMA 200-parsec Resolution Imaging of Smooth Cold Dusty Disks in Typical $z\sim 3$ Star-Forming Galaxies
• Halo mass estimates from the Globular Cluster populations of 175 Low Surface Brightness Galaxies in the Fornax Cluster
• Delayed Star Formation in Isolated Dwarf Galaxies: HST Star Formation History of the Aquarius Dwarf Irregular
• Rhapsody-G simulations I: the cool cores, hot gas and stellar content of massive galaxy clusters
• Equilibrium Model Constraints on Baryon Cycling Across Cosmic Time
• The Impact of Scatter in the Galaxy UV Luminosity to Halo Mass Relation on Ly$\alpha$ Visibility During the Epoch of Reionization
• The Effect of the AGN Feedback on the Interstellar Medium of Early-Type Galaxies: 2D Hydrodynamical Simulations of the Low-Rotation Case
• The Fates of the Circumgalactic Medium in the FIRE Simulations
• Two-phase galaxy evolution: the cosmic star-formation histories of spheroids and discs
• A hypervelocity star with a Magellanic origin
• Spatially-unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem
• The Three Causes of Low-Mass Assembly Bias
• Projection effects on the observed angular spectrum of the astrophysical stochastic gravitational wave background
• The Dramatic Size and Kinematic Evolution of Massive Early-Type Galaxies
• MAGIICAT III. Interpreting Self-Similarity of the Circumgalactic Medium with Virial Mass using MgII Absorption
• Rotation and Mass in the Milky Way and Spiral Galaxies
• The relative and absolute ages of old globular clusters in the LCDM framework
• Two New Calcium-Rich Gap Transients in Group and Cluster Environments
• Column Density Profiles of Multi-Phase Gaseous Halos
• Enhanced tidal stripping of satellites in the galactic halo from dark matter self-interactions
• New insights on the formation of nuclear star clusters
• Dark Matter in Dwarf Spheroidal Galaxies and Indirect Detection: A Review
• An unexpected high concentration for the dark substructure in the gravitational lens SDSSJ0946+1006
• MultiDark-Galaxies: data release and first results
• The SINS/zC-SINF Survey of z~2 Galaxy Kinematics: Rest-frame Morphology, Structure, and Colors from Near-infrared Hubble Space Telescope Imaging
• The properties of "dark" ΛCDM halos in the Local Group
• The cosmic evolution of the spatially-resolved star formation rate and stellar mass of the CALIFA survey
• Evolution of Intrinsic Scatter in the SFR-Stellar Mass Correlation at 0.5<z<3
• The evolving relation between star-formation rate and stellar mass in the VIDEO Survey since $z=3$
• Precipitation-Regulated Star Formation in Galaxies
• Galaxy And Mass Assembly (GAMA): Environmental Quenching of Centrals and Satellites in Groups
• Modeling the Connection Between Subhalos and Satellites in Milky Way-like Systems
• The ALMA Spectroscopic Survey in the HUDF: the molecular gas content of galaxies and tensions with IllustrisTNG and the Santa Cruz SAM
• Feedback from supermassive black holes transforms centrals into passive galaxies by ejecting circumgalactic gas
• The masses of Local Group dwarf spheroidal galaxies: The death of the universal mass profile
• The tidal evolution of dark matter substructure -- II. The impact of artificial disruption on subhalo mass functions and radial profiles
• Orbital Decay of Supermassive Black Hole Binaries in Clumpy Multiphase Merger Remnants
• Diverse Structural Evolution at z > 1 in Cosmologically Simulated Galaxies
• 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
• Massive Compact Galaxies with High-Velocity Outflows: Morphological Analysis and Constraints on AGN Activity
• Trinity I: Self-Consistently Modeling the Dark Matter Halo-Galaxy-Supermassive Black Hole Connection from $z=0-10$
• A model for core formation in dark matter haloes and ultra diffuse galaxies by outflow episodes
• How baryons affect halos and large-scale structure: a unified picture from the Simba simulation
• Probing the galaxy-halo connection in UltraVISTA to $z\sim 2$
• 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
• Quenching timescales of galaxies in the EAGLE simulations
• Cold Filamentary Accretion and the Formation of Metal Poor Globular Clusters and Halo Stars
• NIHAO V: Too big doesn't fail -- reconciling the conflict between LCDM predictions and the circular velocities of nearby field galaxies
• The maximum accretion rate of hot gas in dark matter halos
• Quasars Probing Quasars VIII. The Physical Properties of the Cool Circumgalactic Medium Surrounding z ~ 2-3 Massive Galaxies Hosting Quasars
• Preparing for low surface brightness science with the Vera C. Rubin Observatory: characterisation of tidal features from mock images
• EDGE: The origin of scatter in ultra-faint dwarf stellar masses and surface brightnesses
• The Grism Lens-Amplified Survey from Space (GLASS) X. Sub-kpc resolution gas-phase metallicity maps at cosmic noon behind the Hubble Frontier Fields cluster MACS1149.6+2223
• Starbursting [O III] emitters and quiescent [C II] emitters in the reionization era
• Return to [Log-]Normalcy: Rethinking Quenching, The Star Formation Main Sequence, and Perhaps Much More
• Two can play at that game: constraining the role of supernova and AGN feedback in dwarf galaxies with cosmological zoom-in simulations
• A unified explanation for the supernova rate-galaxy mass dependency based on supernovae discovered in Sloan galaxy spectra
• Reproducing sub-millimetre galaxy number counts with cosmological hydrodynamic simulations
• The spatially-resolved star formation histories of CALIFA galaxies: Implications for galaxy formation
• The Grism Lens-Amplified Survey from Space (GLASS). II. Gas-phase metallicity and radial gradients in an interacting system at z~2
• Early Low-Mass Galaxies and Star-Cluster Candidates at z~6-9 Identified by the Gravitational Lensing Technique and Deep Optical/Near-Infrared Imaging
• Predicting the locations of possible long-lived low-mass first stars: Importance of satellite dwarf galaxies
• Did JWST observe imprints of axion miniclusters or primordial black holes?
• Kinematics and simulations of the stellar stream in the halo of the Umbrella Galaxy
• The Need for Speed: Escape velocity and dynamical mass measurements of the Andromeda galaxy
• An Empirical Model for the Star Formation History in Dark Matter Halos
• Evident black hole-bulge coevolution in the distant universe
• NIHAO XIII: Clumpy discs or clumpy light in high redshift galaxies?
• Minor vs Major Mergers: The Stellar Mass Growth of Massive Galaxies from z=3 using Number Density Selection Techniques
• On the Physical Origin of Galactic Conformity
• Counting Black Holes: The Cosmic Stellar Remnant Population and Implications for LIGO
• Properties of the stochastic astrophysical gravitational wave background: astrophysical sources dependencies
• The tidal evolution of dark matter substructure -- I. Subhalo density profiles
• The Persistence of Population III Star Formation
• NIHAO XX: The impact of the star formation threshold on the cusp-core transformation of cold dark matter haloes
• Cosmological Galaxy Evolution with Superbubble Feedback I: Realistic Galaxies with Moderate Feedback
• Galaxies lacking dark matter produced by close encounters in a cosmological simulation
• Low-mass galaxy assembly in simulations: regulation of early star formation by radiation from massive stars
• Baryonic and dark matter distribution in cosmological simulations of spiral galaxies
• An Intensity Mapping Detection of Aggregate CO Line Emission at 3 mm
• NIHAO VIII: Circum-galactic medium and outflows - The puzzles of HI and OVI gas distributions
• NIHAO VI. The hidden discs of simulated galaxies
• Cosmology with intensity mapping techniques using atomic and molecular lines
• A small-scale dynamo in feedback-dominated galaxies - II. The saturation phase and the final magnetic configuration
• Modelling the Tucana III stream - a close passage with the LMC
• Luminous Quasars Do Not Live in the Most Overdense Regions of Galaxies at z~4
• Preventing Star Formation in Early-Type Galaxies with Late-Time Stellar Heating
• Origins of scaling relations of globular cluster systems
• Hidden depths in the local Universe: The Stellar Stream Legacy Survey
• Probing the Cool Interstellar and Circumgalactic Gas of Three Massive Lensing Galaxies at z=0.4-0.7
• Correlating galaxy colour and halo concentration: A tunable Halo Model of galactic conformity
• No Assembly Required: Mergers are Mostly Irrelevant for the Growth of Low-mass Dwarf Galaxies
• The Milky Way's Halo and Subhalos in Self-Interacting Dark Matter
• The Radial Acceleration Relation in CLASH Galaxy Clusters
• Morphologies of ~190,000 Galaxies at z=0-10 Revealed with HST Legacy Data. III. Continuum Profile and Size Evolution of Lya Emitters
• Prospects for chemically tagging stars in the Galaxy
• Constraining the physical properties of the first lensed $z\sim 10-16$ galaxy candidates with JWST
• Non-linearity and environmental dependence of the star forming galaxies Main Sequence
• The Galaxy Clustering Crisis in Abundance Matching
• 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
• 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
• Ultra diffuse galaxies in the MATLAS low-to-moderate density fields
• Rhapsody. I. Structural Properties and Formation History From a Statistical Sample of Re-simulated Cluster-size Halos
• 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
• Fast Outflows Identified in Early Star-Forming Galaxies at $z=5-6$
• Dissecting the high-z interstellar medium through intensity mapping cross-correlations
• Connecting Transitions in Galaxy Properties to Refueling
• The Nature of H$\beta +$[O{\sc iii}] and [O{\sc ii}] emitters to $z\sim 5$ with HiZELS: stellar mass functions and the evolution of EWs
• Phenomenological consequences of superfluid dark matter with baryon-phonon coupling
• Inferring the star formation histories of the most massive and passive early-type galaxies at z<0.3
• 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
• LoCuSS: Scaling relations between galaxy cluster mass, gas, and stellar content
• Search for CII Emission on Cosmological Scales at Redshift Z~2.6
• Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey Description
• The Velocity Dispersion Function of Very Massive Galaxy Clusters: Abell 2029 and Coma
• Numerical resolution limits on subhalo abundance matching
• On the mass of the Local Group
• GalaxyNet: Connecting galaxies and dark matter haloes with deep neural networks and reinforcement learning in large volumes
• Cosmic Neutron Star Merger Rate and Gravitational Waves constrained by the R Process Nucleosynthesis
• Semi-analytic forecasts for JWST -- VI. Simulated lightcones and galaxy clustering predictions
• Galactic disk winds driven by cosmic ray pressure
• Elliptical Galaxies and Bulges of Disk Galaxies: Summary of Progress and Outstanding Issues
• Constraining the CO intensity mapping power spectrum at intermediate redshifts
• Evolution of the Mass-Metallicity Relation from Redshift $z\approx 8$ to the Local Universe
• The bias of the submillimetre galaxy population: SMGs are poor tracers of the most massive structures in the z ~ 2 Universe
• Star Clusters in Evolving Galaxies
• COSMOS-Web: stellar mass assembly in relation to dark matter halos across $0.2<z<12$ of cosmic history
• AGN evolution from a galaxy evolution viewpoint
• The MaGICC volume: reproducing statistical properties of high redshift galaxies
• Star Formation and Clumps in Cosmological Galaxy Simulations with Radiation Pressure Feedback
• Constraining the evolution of CII intensity through the end stages of reionization
• Emergence of an Ultra-Red Ultra-Massive Galaxy Cluster Core at $z=4$
• The eROSITA Final Equatorial Depth Survey (eFEDS): X-ray emission around star-forming and quiescent galaxies at $0.05<z<0.3$
• ALMA measures rapidly depleted molecular gas reservoirs in massive quiescent galaxies at z~1.5
• Accurate and Efficient Halo-based Galaxy Clustering Modelling with Simulations
• 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
• CLASS_GWB: robust modeling of the astrophysical gravitational wave background anisotropies
• EPOCHS IV: SED Modelling Assumptions and their impact on the Stellar Mass Function at 6.5 < z < 13.5 using PEARLS and public JWST observations
• Predicting Galaxy Star Formation Rates via the Co-evolution of Galaxies and Halos
• Star formation history, dust attenuation and extragalactic background light
• 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
• NIHAO XII: galactic uniformity in a ΛCDM universe
• Propagation of Superluminal PeV IceCube Neutrinos: A High Energy Spectral Cutoff or New Constraints on Lorentz Invariance Violation
• Line intensity mapping with [CII] and CO(1-0) as probes of primordial non-Gaussianity
• Under the Firelight: Stellar Tracers of the Local Dark Matter Velocity Distribution in the Milky Way
• Light breeze in the local Universe
• The stellar halos of ETGs in the IllustrisTNG simulations: the photometric and kinematic diversity of galaxies at large radii
• 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
• On The History and Future of Cosmic Planet Formation
• Direct Insights into Observational Absorption Line Analysis Methods of the Circumgalactic Medium Using Cosmological Simulations
• Dynamical evolution of cosmic supermassive binary black holes and their gravitational wave radiation
• Simulating the 21-cm signal from reionisation including non-linear ionisations and inhomogeneous recombinations
• The cumulative star-formation histories of dwarf galaxies with TNG50. I: Environment-driven diversity and connection to quenching
• Mg II Absorption at 2<z<7 with Magellan/FIRE, III. Full Statistics of Absorption Towards 100 High-Redshift QSOs
• Dynamical evidence for a morphology-dependent relation between the stellar and halo masses of galaxies
• Two-Face(s): ionized and neutral gas winds in the local Universe
• Empirical constraints on the formation of early-type galaxies
• NIHAO XIX: How supernova feedback shapes the galaxy baryon cycle
• Constraining the HI-Halo Mass Relation From Galaxy Clustering
• Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
• SUPER I. Toward an unbiased study of ionized outflows in z~2 active galactic nuclei: survey overview and sample characterization
• Interpreting Short Gamma Ray Burst Progenitor Kicks and Time Delays Using the Host Galaxy-Dark Matter Halo Connection
• Formation of elongated galaxies with low masses at high redshift
• Constraining the Star Formation Histories in Dark Matter Halos: I. Central Galaxies
• From lenticulars to blue compact dwarfs: the stellar mass fraction is regulated by disc gravitational instability
• CONCERTO: High-fidelity simulation of millimeter line emissions of galaxies and [CII] intensity mapping
• A Foreground Masking Strategy for [CII] Intensity Mapping Experiments Using Galaxies Selected by Stellar Mass and Redshift
• Introducing piXedfit -- a Spectral Energy Distribution Fitting Code Designed for Resolved Sources
• A homogeneous measurement of the delay between the onsets of gas stripping and star formation quenching in satellite galaxies of groups and clusters
• Luminosity Functions and Host-to-Host Scatter of Dwarf Satellite Systems in the Local Volume
• Symphony: Cosmological Zoom-in Simulation Suites over Four Decades of Host Halo Mass
• On the origin of excess cool gas in quasar host halos
• From massive spirals to dwarf irregulars: a new set of tight scaling relations for cold gas and stars driven by disc gravitational instability
• Spin-driven jet feedback in idealised simulations of galaxy groups and clusters
• The physical nature of the cosmic accretion of baryons and dark matter into halos and their galaxies
• A Connection between Obscuration and Star Formation in Luminous Quasars
• Simultaneous modelling of matter power spectrum and bispectrum in the presence of baryons
• The edge of galaxy formation I: formation and evolution of MW-satellites analogues before accretion
• High-redshift galaxies and black holes in the eyes of JWST: a population synthesis model from infrared to X-rays
• A fresh look into the interacting dark matter scenario
• The Scale-Dependence of Halo Assembly Bias
• Host galaxies of high-redshift quasars: supermassive black hole growth and feedback
• Inferences on the Relations Between Central Black Hole Mass and Total Galaxy Stellar Mass in the high-redshift Universe
• Structural and dynamical modeling of WINGS clusters. II. The orbital anisotropies of elliptical, spiral and lenticular galaxies
• Effects of simulated cosmological magnetic fields on the galaxy population
• An observer's guide to the (Local Group) dwarf galaxies: predictions for their own dwarf satellite populations
• 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
• Structure Formation Models Weaken Limits on WIMP Dark Matter from Dwarf Spheroidal Galaxies
• Hunting Faint Dwarf Galaxies in the Field Using Integrated Light Surveys
• Is diffuse intracluster light a good tracer of the galaxy cluster matter distribution?
• Detecting Direct Collapse Black Holes: making the case for CR7
• Andromeda XXI -- a dwarf galaxy in a low density dark matter halo
• The JWST Advanced Deep Extragalactic Survey: Discovery of an Extreme Galaxy Overdensity at $z=5.4$ with JWST/NIRCam in GOODS-S
• Dwarf Galaxy Formation with H2-Regulated Star Formation: II. Gas-Rich Dark Galaxies at Redshift 2.5
• Forming early-type galaxies without AGN feedback: a combination of merger-driven outflows and inefficient star formation
• Anomalously low metallicity regions in MaNGA star-forming galaxies: Accretion Caught in Action?
• Realistic simulations of galaxy formation in f(R) modified gravity
• Cosmological Galaxy Evolution with Superbubble Feedback II: The Limits of Supernovae
• The Structural Evolution of Milky Way-like Star Forming Galaxies since z~1.3
• The Main Sequences of Starforming Galaxies and Active Galactic Nuclei at High Redshift
• The Quest for Dusty Star-forming Galaxies at High Redshift z>4
• On the Choice of Lens Density Profile in Time Delay Cosmography
• The Relationship Between Star-formation Activity and Galaxy Structural Properties in CANDELS and a Semi-analytic Model
• The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to $z\sim 5$
• Swirls of FIRE: Spatially Resolved Gas Velocity Dispersions and Star Formation Rates in FIRE-2 Disk Environments
• The Structure of the Circumgalactic Medium of Galaxies: Cool Accretion Inflow Around NGC 1097
• Mg II absorbers: metallicity evolution and cloud morphology
• Galaxy spin as a formation probe: the stellar-to-halo specific angular momentum relation
• The GEEC2 spectroscopic survey of Galaxy Groups at $0.8<z<1$
• TheHaloMod: An online calculator for the halo model
• The SAMI Galaxy Survey: The internal orbital structure and mass distribution of passive galaxies from triaxial orbit-superposition Schwarzschild models
• Rapid early coeval star formation and assembly of the most massive galaxies in the universe
• COSMOS2020: Discovery of a protocluster of massive quiescent galaxies at $z=2.77$
• Weak Lensing Reveals a Tight Connection Between Dark Matter Halo Mass and the Distribution of Stellar Mass in Massive Galaxies
• 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
• Self-Interacting Dark Matter and the Origin of Ultra-Diffuse Galaxies NGC1052-DF2 and -DF4
• Validating Semi-Analytic Models of High-Redshift Galaxy Formation using Radiation Hydrodynamical Simulations
• On the origin of surprisingly cold gas discs in galaxies at high redshift
• Star formation at the edge of the Local Group: a rising star formation history in the isolated galaxy WLM
• Insights from probability distribution functions of intensity maps
• Dark and luminous satellites of LMC-mass galaxies in the FIRE simulations
• 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
• The Co-Evolution of Galaxies and the Cool Circumgalactic Medium Probed with the SDSS and DESI Legacy Imaging Surveys
• Clumpy galaxies seen in H-alpha: inflated observed clump properties due to limited spatial resolution and sensitivity
• Line-of-sight effects in strong lensing: Putting theory into practice
• The first galaxies: simulating their feedback-regulated assembly
• Approximate Bayesian Computation in Large Scale Structure: constraining the galaxy-halo connection
• FOREVER22: galaxy formation in protocluster regions
• Galaxy disc scaling relations: A tight linear galaxy -- halo connection challenges abundance matching
• The spatial clustering of ROSAT All-Sky Survey Active Galactic Nuclei IV. More massive black holes reside in more massive dark matter halos
• Joint power spectrum and voxel intensity distribution forecast on the CO luminosity function with COMAP
• MOND Prediction for the Velocity Dispersion of the `Feeble Giant' Crater II
• A Systematic Study of the Stochastic Gravitational-Wave Background due to Stellar Core Collapse
• The dependence of the galaxy stellar-to-halo mass relation on galaxy morphology
• Learning the Relationship between Galaxies Spectra and their Star Formation Histories using Convolutional Neural Networks and Cosmological Simulations
• Osaka Feedback Model: Isolated Disk Galaxy Simulations
• The prevalence and properties of cold gas inflows and outflows around galaxies in the local Universe
• UVUDF: UV Luminosity Functions at the cosmic high-noon
• Evidence for Cold-stream to Hot-accretion Transition as Traced by Lyα Emission from Groups and Clusters at 2 < z < 3.3
• Stellar Mass--Gas-phase Metallicity Relation at $0.5\le z\le 0.7$: A Power Law with Increasing Scatter toward the Low-mass Regime
• The correlation between the sizes of globular cluster systems and their host dark matter haloes
• Baryonic Imprints on DM Halos: Population Statistics from Dwarf Galaxies to Galaxy Clusters
• Observational evidence of galaxy assembly bias
• Spatially resolved mass-to-light from the CALIFA survey. Mass-to-light ratio vs. color relations
• On the intermediate-redshift central stellar mass-halo mass relation, and implications for the evolution of the most massive galaxies since z~1
• The Strikingly Similar Relation between Satellite and Central Galaxies and Their Dark Matter Halos Since z=2
• Scaling relations and baryonic cycling in local star-forming galaxies: II. Gas content and star-formation efficiency
• Stochastic gravitational wave background anisotropies in the mHz band: astrophysical dependencies
• The Dwarfs Beyond: The Stellar-to-Halo Mass Relation for a New Sample of Intermediate Redshift Low Mass Galaxies
• Near-Field Limits on the Role of Faint Galaxies in Cosmic Reionization
• Maximum redshift of gravitational wave merger events
• The simplest model of galaxy formation I: A formation history model of galaxy stellar mass growth
• An analytical model for galaxy metallicity: What do metallicity relations tell us about star formation and outflow?
• Early-type galaxy density profiles from IllustrisTNG: I. Galaxy correlations and the impact of baryons
• Radial Trends in IMF-Sensitive Absorption Features in Two Early-Type Galaxies: Evidence for Abundance-Driven Gradients
• Thick Disks in the Hubble Space Telescope Frontier Fields
• Evolution of Star-forming Galaxies from z = 0.7 to 1.2 with eBOSS Emission-line Galaxies
• Galaxy evolution in protoclusters
• Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
• EMPRESS. IV. Extremely Metal-Poor Galaxies (EMPGs) Including Very Low-Mass Primordial Systems with M*=10^4--10^5 M_sun and 2--3% (O/H)_sun: High (Fe/O) Suggestive of Metal Enrichment by Hypernovae/Pair-Instability Supernovae
• Clustering, host halos and environment of z$\sim$2 galaxies as a function of their physical properties
• A Fast Radio Burst Occurs Every Second throughout the Observable Universe
• An empirical representation of a physical model for the ISM [CII], CO, and [CI] emission at redshift $1\le z\le 9$
• Exploring the nature of the Lyman-$\alpha$ emitter CR7
• First results from SMAUG: The need for preventative stellar feedback and improved baryon cycling in semi-analytic models of galaxy formation
• Evolution of Galactic Outflows at $z\sim 0$-$2$ Revealed with SDSS, DEEP2, and Keck spectra
• A lensed protocluster candidate at $z=7.66$ identified in JWST observations of the galaxy cluster SMACS0723-7327
• Millimeter mapping at z~1: dust-obscured bulge building and disk growth
• A limit on the warm dark matter particle mass from the redshifted 21 cm absorption line
• How robustly can we constrain the low-mass end of the $z\sim 6-7$ stellar mass function? -- The limits of lensing models and stellar population assumptions in the Hubble Frontier Fields
• The role of faint population III supernovae in forming CEMP stars in ultra-faint dwarf galaxies
• The Star-Formation Main Sequence: The Dependence of Specific Star Formation Rate and Its Dispersion on Galaxy Stellar Mass
• Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
• The origin of the mass scales for maximal star formation efficiency and quenching: the critical role of Supernovae
• The bias of DLAs at z ~ 2.3: contraining stellar feedback in shallow potential wells
• A simple model linking galaxy and dark matter evolution
• A single-merger scenario for the formation of the giant stream and the warp of M31
• Stellar mass functions of galaxies at 4<z<7 from an IRAC-selected sample in COSMOS/UltraVISTA: limits on the abundance of very massive galaxies
• Magnetogenesis around the first galaxies: the impact of different field seeding processes on galaxy formation
• The minimum metallicity of globular clusters and its physical origin -- implications for the galaxy mass-metallicity relation and observations of proto-globular clusters at high redshift
• GRUMPY: a simple framework for realistic forward-modelling of dwarf galaxies
• The combined effect of AGN and supernovae feedback in launching massive molecular outflows in high-redshift galaxies
• Identification of High-Redshift Galaxy Overdensities in GOODS-N and GOODS-S
• Realistic mock observations of the sizes and stellar mass surface densities of massive galaxies in FIRE-2 zoom-in simulations
• Caught in the act: gas and stellar velocity dispersions in a fast quenching compact star-forming galaxy at z~1.7
• New Analytic Solutions for Galaxy Evolution: Gas, Stars, Metals and Dust in local Early-Type Galaxies and in their high-z Starforming Progenitors
• The Immitigable Nature of Assembly Bias: The Impact of Halo Definition on Assembly Bias
• A Study of Massive and Evolved Galaxies at High Redshift
• Early growth of typical high redshift black holes seeded by direct collapse
• Star Formation Quenching Timescale of Central Galaxies in a Hierarchical Universe
• An Excess of Globular Clusters in UDGs Formed Through Tidal Heating
• The Stellar Mass, Star Formation Rate and Dark Matter Halo Properties of LAEs at $z\sim 2$
• Timing the evolution of quiescent and star-forming local galaxies
• The new semianalytic code GalICS 2.0 - Reproducing the galaxy stellar mass function and the Tully-Fisher relation simultaneously
• The Origin of r-process Enhanced Metal-Poor Halo Stars In Now-Destroyed Ultra-Faint Dwarf Galaxies
• The H-alpha luminosity-dependent clustering of star-forming galaxies from z~0.8 to z~2.2 with HiZELS
• From Diversity to Dichotomy, and Quenching: Milky-Way-Like and Massive-Galaxy Progenitors at 0.5<z<3.0
• The bending of the star-forming main sequence traces the cold- to hot-accretion transition mass over 0<z<4
• The evolution of the stellar mass versus halo mass relationship
• Impact of polarised extragalactic sources on the measurement of CMB B-mode anisotropies
• Formation of disk galaxies in preheated media: a preventative feedback model
• Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations
• Rotation Curve Decomposition for Size-Mass Relations of Bulge, Disk, and Dark Halo in Spiral Galaxies
• Young and turbulent: the early life of massive galaxy progenitors
• The LBT Satellites of Nearby Galaxies Survey (LBT-SONG): The Satellite Population of NGC 628
• Simple halo model formalism for the cosmic infrared background and its correlation with the thermal Sunyaev Zel'dovich effect
• The challenge of simultaneously matching the observed diversity of chemical abundance patterns in cosmological hydrodynamical simulations
• Equilibrium model prediction for the scatter in the star-forming main sequence
• The Little Galaxies that Could (Reionize the Universe): Predicting Faint End Slopes & Escape Fractions at z > 4
• Formation of the largest galactic cores through binary scouring and gravitational wave recoil
• Dust formation, evolution, and obscuration effects in the very high-redshift universe
• X-ray Emission From Hot Gas in Galaxy Groups and Clusters in Simba
• The effects of galaxy shape and rotation on the X-ray haloes of early-type galaxies - II. Numerical simulations
• The Mass and Absorption Columns of Galactic Gaseous Halos
• Halo Histories vs. Galaxy Properties at z=0, I: The Quenching of Star Formation
• New perspectives on the BOSS small-scale lensing discrepancy for the Planck $\Lambda$CDM Cosmology
• ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
• Properties of Submillimeter Galaxies in a Semi-analytic Model using the "Count Matching" Approach: Application to the ECDF-S
• NIHAO -- XXV. Convergence in the cusp-core transformation of cold dark matter haloes at high star formation thresholds
• Magellanic satellites in $\Lambda$CDM cosmological hydrodynamical simulations of the Local Group
• A Model of the Stochastic Gravitational-Wave Background due to Core Collapse to Black Holes
• AGN and their host galaxies in the local Universe: two mass independent Eddington ratio distribution functions characterize black hole growth
• Revisiting the bulge-halo conspiracy I: Dependence on galaxy properties and halo mass
• On stellar mass loss from galaxies in groups and clusters
• Stellar Velocity Dispersion: Linking Quiescent Galaxies to their Dark Matter Halos
• Are Cosmological Gas Accretion Streams Multiphase and Turbulent?
• Cross-correlating Carbon Monoxide Line-intensity Maps with Spectroscopic and Photometric Galaxy Surveys
• Introducing galactic structure finder: the multiple stellar kinematic structures of a simulated Milky Way mass galaxy
• Hierarchical Galaxy Growth and Scatter in the Stellar Mass - Halo Mass Relation
• Forecasts for the WFIRST High Latitude Survey using the BlueTides Simulation
• Creating a galaxy lacking dark matter in a dark matter dominated universe
• A universal relation between the properties of supermassive black holes, galaxies, and dark matter halos
• The Morphology-Density-Relation: Impact on the Satellite Fraction
• Baryon effects on void statistics in the EAGLE simulation
• Chasing Lyman alpha-emitting galaxies at z = 8.8
• The evolution of turbulent galactic discs: gravitational instability, feedback and accretion
• Search for Gamma-ray Emission from Dark Matter Annihilation in the Small Magellanic Cloud with the Fermi Large Area Telescope
• Where did the globular clusters of the Milky Way form? Insights from the E-MOSAICS simulations
• The Role of Cold Flows and Reservoirs in Galaxy Formation With Strong Feedback
• Emergence of the mass discrepancy-acceleration relation from dark matter-baryon interactions
• The Relative Specific Type Ia Supernovae Rate From Three Years of ASAS-SN
• Constraining the last 7 billion years of galaxy evolution in semi-analytic models
• Phase-Space Spectral Line De-confusion in Intensity Mapping
• A duality in the origin of bulges and spheroidal galaxies
• The dependence of galaxy clustering on stellar mass, star-formation rate and redshift at z = 0.8-2.2, with HiZELS
• A Detection of the Environmental Dependence of the Sizes and Stellar Haloes of Massive Central Galaxies
• The diverse formation histories of simulated disc galaxies
• The Mass Profile of the Milky Way to the Virial Radius from the Illustris Simulation
• Towards a radially-resolved semi-analytic model for the evolution of disc galaxies tuned with machine learning
• Co-orbiting planes of sub-halos are similarly unlikely around paired and isolated hosts
• Clearing the hurdle: The mass of globular cluster systems as a function of host galaxy mass
• The clustering of typical Ly$\alpha$ emitters from $z\sim 2.5-6$: host halo masses depend on Ly$\alpha$ and UV luminosities
• An alternate approach to measure specific star formation rates at 2<z<7
• NIHAO XXII: Introducing black hole formation, accretion and feedback into the NIHAO simulation suite
• Constraints on galaxy formation models from the galaxy stellar mass function and its evolution
• Constraints on warm dark matter from UV luminosity functions of high-z galaxies with Bayesian model comparison
• The SLUGGS survey: inferring the formation epochs of metal-poor and metal-rich globular clusters
• Low Angular Momentum in Clumpy, Turbulent Disk Galaxies
• Jet-driven AGN feedback on molecular gas and low star-formation efficiency in a massive local spiral galaxy with bright X-ray halo
• The Incomplete Conditional Stellar Mass Function: Unveiling the Stellar Mass Functions of Galaxies at 0.1 < Z < 0.8 from BOSS Observations
• Stellar splashback: the edge of the intracluster light
• Evolution of Star-formation Properties of High-redshift Cluster Galaxies since $z=2$
• NIHAO XVI: The properties and evolution of kinematically selected discs, bulges and stellar haloes
• JADES + JEMS: A Detailed Look at the Buildup of Central Stellar Cores and Suppression of Star Formation in Galaxies at Redshifts 3 < z < 4.5
• GN-z11: The environment of an AGN at $z=$10.603
• Scaling Relations for Galaxies Prior to Reionization
• Matching the Evolution of the Stellar Mass Function Using Log-normal Star Formation Histories
• Growth of First Galaxies: Impacts of Star Formation and Stellar Feedback
• The emergence of dark matter-deficient ultra-diffuse galaxies driven by scatter in the stellar mass-halo mass relation and feedback from globular clusters
• Unraveling the origin of magnetic fields in galaxies
• Galaxy Zoo: major galaxy mergers are not a significant quenching pathway
• The LOFAR Two-metre Sky Survey: the radio view of the cosmic star formation history
• The history of the dark and luminous side of Milky Way-like progenitors
• SDSS IV MaNGA - Rotation Velocity Lags in the Extraplanar Ionized Gas from MaNGA Observations of Edge-on Galaxies
• A new astrophysical solution to the Too Big To Fail problem - Insights from the MoRIA simulations
• Central galaxies in different environments: Do they have similar properties?
• The Three Hundred Project: The influence of environment on simulated galaxy properties
• Tidal Distortions in NGC1052-DF2 and NGC1052-DF4: Independent Evidence for a Lack of Dark Matter
• Shock finding on a moving-mesh: II. Hydrodynamic shocks in the Illustris universe
• Priors on red galaxy stochasticity from hybrid effective field theory
• Lessons from cosmic history: The case for a linear star formation -- H2 relation
• GOODS-ALMA: Optically dark ALMA galaxies shed light on a cluster in formation at z = 3.5
• Bayesian inferences of galaxy formation from the K-band luminosity and HI mass functions of galaxies: constraining star formation and feedback
• COMAP Early Science: V. Constraints and Forecasts at $z\sim 3$
• HectoMAP and Horizon Run 4: Dense Structures and Voids in the Real and Simulated Universe
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• A Statistical Semi-Empirical Model: Satellite galaxies in Groups and Clusters
• Observed trend in the star formation history and the dark matter fraction of galaxies at redshift $z\approx 0.8$
• Great Balls of FIRE II: The evolution and destruction of star clusters across cosmic time in a Milky Way-mass galaxy
• A parametric study of possible solutions to the high-redshift overproduction of stars in modeled dwarf galaxies
• ZFOURGE: Using Composite Spectral Energy Distributions to Characterize Galaxy Populations at 1<z<4
• The role of gas infall in the evolution of disc galaxies
• A synthetic model of the gravitational wave background from evolving binary compact objects
• Cosmic Vine: A z=3.44 large-scale structure hosting massive quiescent galaxies
• The MUSE Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies at z=1
• The GOGREEN survey: Transition Galaxies and The Evolution of Environmental Quenching
• Does the Galaxy-Halo Connection Vary with Environment?
• Physical Properties of UDF12 Galaxies in Cosmological simulations
• Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency
• The ALMA Spectroscopic Survey in the HUDF: A model to explain observed 1.1 and 0.85 millimeter dust continuum number counts
• Degeneracies Between Self-interacting Dark Matter and Supernova Feedback as cusp-core transformation mechanisms
• Galaxy formation in the brane world I: overview and first results
• The vertical structure of gaseous galaxy discs in cold dark matter halos
• Herschel reveals a molecular outflow in a z = 2.3 ULIRG
• Blue Rest-Frame UV-Optical Colors in z~8 Galaxies from GREATS: Very Young Stellar Populations at ~650 Myr of Cosmic Time
• Cosmography using strongly lensed gravitational waves from binary black holes
• Constraints on the dynamical evolution of the galaxy group M81
• A scaling relation between merger rate of galaxies and their close pair count
• Lyman-αabsorption beyond the disk of simulated spiral galaxies
• Formation channels of slowly rotating early-type galaxies
• The Impact of Environment on the Stellar Mass - Halo Mass Relation
• On the Physical Requirements for a Pre-Reionization Origin of the Unresolved Near-Infrared Background
• Brightest Cluster Galaxies in Cosmological Simulations with Adaptive Mesh Refinement: Successes and Failures
• CANDELS Sheds Light on the Environmental Quenching of Low-mass Galaxies
• How are galaxies assigned to halos? Searching for assembly bias in the SDSS galaxy clustering
• Star Formation and Environmental Quenching of GEEC2 Group Galaxies at z~1
• Precision Tests of CO and [CII] Power Spectra Models against Simulated Intensity Maps
• The Fate of Gas rich Satellites in Clusters
• On the cosmic evolution of the specific star formation rate
• GASS 3505: the prototype of HI-excess, passive galaxies
• Dark matter halos and scaling relations of extremely massive spiral galaxies from extended HI rotation curves
• Telltale signs of metal recycling in the circumgalactic medium of a $z\sim 0.77$ galaxy
• Hubble Space Telescope Observations of Two Faint Dwarf Satellites of Nearby LMC Analogs from MADCASH
• Observing AGN feedback with CO intensity mapping
• A Consistent Set of Empirical Scaling Relations for Spiral Galaxies: The $(v_{\max },M_{\mathrm{DM}})$-$({\sigma }_0,M_{\mathrm{BH}},\varphi )$ Relations
• Angular momentum of dwarf galaxies
• The impact of environment and mergers on the HI content of galaxies in hydrodynamic simulations
• Constraining thermal dust emission in distant galaxies with number counts and angular power spectra
• {\sc mirkwood:} Fast and Accurate SED Modeling Using Machine Learning
• A Bayesian Population Model for the Observed Dust Attenuation in Galaxies
• The Brightest Galaxies at Cosmic Dawn from Scatter in the Galaxy Luminosity versus Halo Mass Relation
• Formation of Globular Cluster Systems II: Impact of the Cutoff of the Cluster Initial Mass Function
• 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
• KMOS LENsing Survey (KLENS) : morpho-kinematic analysis of star-forming galaxies at $z\sim 2$
• The Spectroscopy and H-band Imaging of Virgo cluster galaxies (SHIVir) Survey: Scaling Relations and the Stellar-to-Total Mass Relation
• Identification of galaxies that experienced a recent major drop of star formation
• COMAP Early Science: VII. Prospects for CO Intensity Mapping at Reionization
• The kinematics of globular cluster populations in the E-MOSAICS simulations and their implications for the assembly history of the Milky Way
• Reproducing cosmic evolution of galaxy population from $z=4$ to $0$
• Quasar Sightline and Galaxy Evolution (QSAGE) Survey - I. The Galaxy Environment of OVI Absorbers up to z=1.4 around PKS 0232-04
• A High-Resolution Investigation of the Multi-Phase ISM in a Galaxy during the First Two Billion Years
• Origins of Scatter in the Relationship Between HCN 1-0 and Dense Gas Mass in the Galactic Center
• The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3
• Semi-analytic forecasts for Roman -- the beginning of a new era of deep-wide galaxy surveys
• Stochastic angular momentum slews and flips and their effect on discs in galaxy formation models
• Formation and settling of a disc galaxy during the last 8 billion years in a cosmological simulation
• d1005+68: A New Faint Dwarf Galaxy in the M81 Group
• Formation of globular clusters in dwarf galaxies of the Local Group
• Rapid Filamentary Accretion as the Origin of Extended Thin Discs
• Probing the existence of a rich galaxy overdensity at z=5.2
• 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
• Satellites of Satellites: The Case for Carina and Fornax
• Semi-Analytic Galaxies - II. Revealing the role of environmental and mass quenching in galaxy formation
• Tomographic Intensity Mapping versus Galaxy Surveys: Observing the Universe in H-alpha emission with new generation instruments
• On the Orbital Decay of Globular Clusters in NGC1052-DF2: Testing a Baryon-Only Mass Model
• Cosmic evolution of star-forming galaxies to $z\simeq 1.8$ in the faint low-frequency radio source population
• The origin of dispersion in DLA metallicities
• Confronting fuzzy dark matter with the rotation curves of nearby dwarf irregular galaxies
• The MOSDEF Survey: Environmental dependence of the gas-phase metallicity of galaxies at $1.4\le z\le 2.6$
• Kinematics of the Circumgalactic Medium of a $z=0.77$ Galaxy from MgII Tomography
• Linear bias forecasts for emission line cosmological surveys
• Simulating the Spatial Distribution and Kinematics of Globular Clusters within Galaxy Clusters in Illustris
• Cosmic CARNage I: on the calibration of galaxy formation models
• Star Formation Quenching in Green Valley Galaxies at $0.5\lesssim z\lesssim 1.0$ and Constraints with Galaxy Morphologies
• The Pandora project. I: the impact of radiation and cosmic rays on baryonic and dark matter properties of dwarf galaxies
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• The MUSE-Faint survey. II. The dark matter-density profile of the ultra-faint dwarf galaxy Eridanus 2
• Calibrated, cosmological hydrodynamical simulations with variable IMFs I: Method and effect on global galaxy scaling relations
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• Signatures of Dark Matter Halo Expansion in Galaxy Populations
• Modelling the cosmic neutral hydrogen from DLAs and 21 cm observations
• IQ-Collaboratory 1.1: the Star-Forming Sequence of Simulated Central Galaxies
• BIRTH of the COSMOS Field: Primordial and Evolved Density Reconstructions During Cosmic High Noon
• Simultaneously constraining cosmology and baryonic physics via deep learning from weak lensing
• The Minimum Halo Mass for Star Formation at z = 6 - 8
• Gas flows in the circumgalactic medium around simulated high-redshift galaxies
• The accreted stellar halo as a window on halo assembly in L* galaxies
• Modelling of Lyman-alpha Emitting Galaxies and Ionized Bubbles at the Era of Reionization
• The AGN-galaxy-halo connection: The distribution of AGN host halo masses to z=2.5
• Using Galaxy Pairs to Probe Star Formation During Major Halo Mergers
• The angular momentum of disc galaxies at z=1
• SUPER V. ALMA continuum observations of z~2 AGN and the elusive evidence of outflows influencing star formation
• $\Lambda$CDM Predictions for the Satellite Population of M33
• Globular Cluster Formation from Colliding Substructure
• Probing Cosmic Dawn: Modelling the Assembly History, SEDs, and Dust Content of Selected $z\sim 9$ Galaxies
• Balmer Break Galaxy Candidates at $z\sim 6$: a Potential View on the Star-Formation Activity at $z\gtrsim 14$
• A cosmic stream of atomic carbon gas connected to a massive radio galaxy at redshift 3.8
• Evolution of CIV Absorbers I. The Cosmic Incidence
• Semi-analytic galaxies -- III. The impact of supernova feedback on the mass-metallicity relation
• A Census of the LyC Photons that Form the UV Background During Reionization
• Density modulated star formation efficiency: implications for the observed abundance of ultra-violet luminous galaxies at z>10
• Herschel observed Stripe 82 quasars and their host galaxies: connections between the AGN activity and the host galaxy star formation
• ALMA Deep Field in SSA22: Blindly Detected CO Emitters and [CII] Emitter Candidates
• The Observed Evolution of the Stellar Mass - Halo Mass Relation for Brightest Central Galaxies
• The Active Assembly of the Virgo Cluster: Indications for Recent Group Infall From Early-Type Dwarf Galaxies
• The response of dark matter haloes to elliptical galaxy formation: a new test for quenching scenarios
• Local ultra faint dwarves as a product of Galactic processing during a Magellanic group infall
• Morphological and Rotation Structures of Circumgalactic Mg II Gas in the EAGLE Simulation and the Dependence on Galaxy Properties
• NIHAO III: The constant disc gas mass conspiracy
• Distribution of streaming rates into high-redshift galaxies
• On the (Lack of) Evolution of the Stellar Mass Function of Massive Galaxies from $z$=1.5 to 0.4
• [CII] halos in ALPINE galaxies: smoking-gun of galactic outflows?
• A Dynamical Model for Clustered Star Formation in the Galactic Disk
• From HI to Stars: HI Depletion in Starbursts and Star-Forming Galaxies in the ALFALFA H-alpha Survey
• A few StePS forward in unveiling the complexity of galaxy evolution: light-weighted stellar ages of intermediate redshift galaxies with WEAVE
• Planck far-infrared detection of Hyper Suprime-Cam protoclusters at $\mathbf{z}\sim 4$: hidden AGN and star formation activity
• The Impact of Baryons on Cosmological Inference from Weak Lensing Statistics
• The Intrinsic Scatter of Galaxy Scaling Relations
• The importance of galaxy formation histories in models of reionization
• ELUCID V. Lighting dark matter halos with galaxies
• The evolution of the SFR and Sigma-SFR of galaxies in cosmic morning (4 < z < 10)
• A Model Connecting Galaxy Masses, Star Formation Rates, and Dust Temperatures Across Cosmic Time
• Tidal disruption events in the first billion years of a galaxy
• The ALPINE-ALMA [CII] Survey: On the nature of an extremely obscured serendipitous galaxy
• An Intensity Mapping Constraint on the CO-Galaxy Cross Power Spectrum at Redshift ~ 3
• Modelling a bright z = 6 galaxy at the faint end of the AGN luminosity function
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Intensity mapping from the sky: synergizing the joint potential of [OIII] and [CII] surveys at reionization
• Sensitivity of dark matter haloes to their accretion histories
• Clustering with JWST: Constraining Galaxy Host Halo Masses, Satellite Quenching Efficiencies, and Merger Rates at z=4-10
• The binary-host connection: astrophysics of gravitational wave binaries from their host galaxy properties
• The missing dwarf galaxies of the Local Group
• From EMBER to FIRE: predicting high resolution baryon fields from dark matter simulations with Deep Learning
• Stellar feedback from HMXBs in cosmological hydrodynamical simulations
• ZOMG II: Does the halo assembly history influence central galaxies and gas accretion?
• Probing the galaxy-halo connection with total satellite luminosity
• The Massive Satellite Population of Milky-Way Sized Galaxies
• The Galaxy-Halo Connection for $1.5\lesssim z\lesssim 5$ as revealed by the \emph{Spitzer} Matching survey of the UltraVISTA ultra-deep Stripes
• Bar-like galaxies in IllustrisTNG
• Star-formation driven outflows in local dwarf galaxies as revealed from [CII] observations by Herschel
• The evolving AGN duty cycle in galaxies since z$\sim$3 as encoded in the X-ray luminosity function
• Cosmic evolution of bars in simulations of galaxy formation
• Characterising the Intracluster Light over the Redshift Range $0.2<z<0.8$ in the DES-ACT Overlap
• Probing Cosmic Origins with CO and [CII] Emission Lines
• Entropy Driven Winds: Outflows and Fountains Lifted Gently by Buoyancy
• A model of spectral line broadening in signal forecasts for line-intensity mapping experiments
• AGN feedback and the origin and fate of the hot gas in early-type galaxies
• Cosmological Simulations of Dwarf Galaxies with Cosmic Ray Feedback
• Exploring stellar evolution with gravitational-wave observations
• Tracing the Sources of Reionization in Cosmological Radiation Hydrodynamics Simulations
• GARROTXA Cosmological Simulations of Milky Way-sized Galaxies: General Properties, Hot Gas Distribution, and Missing Baryons
• The Next Generation Virgo Cluster Survey. IX. Estimating the Efficiency of Galaxy Formation on the Lowest-Mass Scales
• An exquisitely deep view of quenching galaxies through the gravitational lens: Stellar population, morphology, and ionized gas
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• Dissecting the roles of mass and environment quenching in galaxy evolution with EAGLE
• The growth of galactic bulges through mergers in LCDM haloes revisited. II. Morphological mix evolution
• Precision Redshift-Space Galaxy Power Spectra using Zel'dovich Control Variates
• The star-formation history of mass-selected galaxies from the VIDEO survey
• Demonstrating Diversity in Star Formation Histories with the CSI Survey
• Black versus Dark: Rapid Growth of Supermassive Black Holes in Dark Matter Halos at z ~ 6
• Highly r-process enhanced stars in ultra-faint dwarf galaxies
• EAGLE-Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
• Revisiting the Size-Luminosity Relation in the Era of Ultra Diffuse Galaxies
• Distinguishing Dark Matter, Modified Gravity, and Modified Inertia with the Inner and Outer Parts of Galactic Rotation Curves
• The miniJPAS survey: The role of group environment in quenching the star formation
• A Unique View of AGN-Driven Molecular Outflows: The Discovery of a Massive Galaxy Counterpart to a $z=2.4$ High-Metallicity Damped Lyman-$\alpha$ Absorber
• UniverseMachine: Predicting Galaxy Star Formation over Seven Decades of Halo Mass with Zoom-in Simulations
• Characterizing circumgalactic gas around massive ellipticals at z~0.4 III. The galactic environment of a chemically-pristine Lyman limit absorber
• Stellar and Dust Properties of a Complete Sample of Massive Dusty Galaxies at $1\le z\le 4$ from MAGPHYS Modeling of UltraVISTA DR3 and Herschel Photometry
• The relation between star formation rate and stellar mass of galaxies at z $\sim$ 1-4
• RESOLVE and ECO: The Halo Mass-Dependent Shape of Galaxy Stellar and Baryonic Mass Functions
• The evolution of galaxy intrinsic alignments in the MassiveBlack II universe
• The phantom dark matter halos of the Local Volume in the context of modified Newtonian dynamics
• The Spitzer/IRAC Legacy over the GOODS Fields: Full-Depth 3.6, 4.5, 5.8 and 8.0um Mosaics and Photometry for > 9000 Galaxies at z~3.5-10 from the GOODS Re-ionization Era wide-Area Treasury from Spitzer (GREATS)
• Angular Momentum of Early and Late Type Galaxies: Nature or Nurture?
• The dark side of galaxy stellar populations I: The stellar-to-halo mass relation and the velocity dispersion - halo mass relation
• Prospects for distinguishing galaxy evolution models with surveys at redshifts $z\gtrsim 4$
• The dependence of the X-ray AGN clustering on the properties of the host galaxy
• COSMOS2020: Identification of High-z Protocluster Candidates in COSMOS
• On the early evolution of Local Group dwarf galaxy types: star formation and supernova feedback
• From starburst to quiescence: post-starburst galaxies and their large-scale clustering over cosmic time
• Constraining the Milky Way halo kinematics via its Linear Response to the Large Magellanic Cloud
• Modeling the kinematics of globular cluster systems
• How long do high-redshift massive black hole seeds remain outliers in black hole vs. host galaxy relations?
• Feeding cosmic star formation: Exploring high-redshift molecular gas with CO intensity mapping
• AstraeusIV : Quantifying the star formation histories of galaxies in the Epoch of Reionization
• Massive Dark Matter Halos at High Redshift: Implications for Observations in the JWST Era
• A first estimate of the Milky Way dark matter halo spin
• Radio galaxies in ZFOURGE/NMBS: no difference in the properties of massive galaxies with and without radio-AGN out to z = 2.25
• Testing the Relationship Between Bursty Star Formation and Size Fluctuations of Local Dwarf Galaxies
• Stellar Mass Function of Active and Quiescent Galaxies via the Continuity Equation
• Dark influences III. Structural characterization of minor mergers of dwarf galaxies with dark satellites
• Evidence for a Massive Andromeda Galaxy Using Satellite Galaxy Proper Motions
• Cosmological simulations of Milky Way-sized galaxies
• CO($J$=1-0) mapping survey of 64 galaxies in the Fornax cluster with the ALMA Morita array
• Preprocessing, mass loss and mass segregation of galaxies in DM simulations
• A fast radio burst in the direction of the Virgo cluster
• Cosmological evolution of the Nitrogen abundance
• Cosmological simulations of the same spiral galaxy: the impact of baryonic physics
• On the inconsistency between cosmic stellar mass density and star formation rate up to $z\sim 8$
• The connection between the host halo and the satellite galaxies of the Milky Way
• A population of ultraviolet-dim protoclusters detected in absorption
• Scaling relations and baryonic cycling in local star-forming galaxies. III. Outflows, effective yields and metal loading factors
• Star formation quenching imprinted on the internal structure of naked red nuggets
• ATLAS Probe: Breakthrough Science of Galaxy Evolution, Cosmology, Milky Way, and the Solar System
• Edge-on HI-bearing ultra diffuse galaxy candidates in the 40% ALFALFA catalog
• Enhanced Rates of Fast Radio Bursts from Galaxy Clusters
• Constraining the recent star formation history of galaxies : an Approximate Bayesian Computation approach
• Evolution of dispersion in the cosmic deuterium abundance
• A Search for Satellite Galaxies of Nearby Star-Forming Galaxies with Resolved Stars in LBT-SONG
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• Galaxy Flybys: Evolution of the Bulge, Disk, and Spiral Arms
• Measuring the delay time distribution of binary neutron stars. I. Through Scaling Relations of the Host Galaxies of Gravitational Wave Events
• Quantifying the power spectrum of small-scale structure in semi-analytic galaxies
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• An empirical prediction for stellar metallicity distributions in nearby galaxies
• Don't Forget the Forest for the Trees: The Stellar-Mass Halo-Mass Relation in Different Environments
• Establishing the Non-Primordial Origin of Black Hole-Neutron Star Mergers
• Galaxy Formation in Sterile Neutrino Dark Matter Models
• Dark Matter Density Profiles in Dwarf Galaxies: Linking Jeans Modeling Systematics and Observation
• A New Approach to Identifying the Most Powerful Gravitational Lensing Telescopes
• Cosmic variance in the nanohertz gravitational wave background
• Satellite mass functions and the faint end of the galaxy mass-halo mass relation in LCDM
• Charting the main sequence of star-forming galaxies out to redshifts z<5.7
• A Systematic Search for Galaxy Proto-Cluster Cores at $z\sim 2$
• Galaxy Lookback Evolution Models -- a Comparison with Magneticum Cosmological Simulations and Observations
• Confronting the Magnetar Interpretation of Fast Radio Bursts Through Their Host Galaxy Demographics
• Stellar and Weak Lensing Profiles of Massive Galaxies in the Hyper-Suprime Cam Survey and in Hydrodynamic Simulations
• Comparing Simple Quasar Demographics Models
• A Uniform History for Galaxy Evolution
• The Outer Stellar Mass of Massive Galaxies: A Simple Tracer of Halo Mass with Scatter Comparable to Richness and Reduced Projection Effects
• Simulations of isolated dwarf galaxies formed in dark matter halos with different mass assembly histories
• nIFTy galaxy cluster simulations V: Investigation of the Cluster Infall Region
• Testing Galaxy Quenching Theories with Scatter in the Stellar to Halo Mass Relation
• The Cosmic Evolution of Magnesium Isotopes
• Cosmic CARNage II: the evolution of the galaxy stellar mass function in observations and galaxy formation models
• Searching for Environmental Effects on Galaxy Kinematics in Groups and Clusters at z~1 from the ORELSE Survey
• BEoRN: A fast and flexible framework to simulate the epoch of reionisation and cosmic dawn
• Excess of high-$z$ galaxies as a test for bumpy power spectrum of density perturbations
• Connections between star cluster populations and their host galaxy nuclear rings
• The global and radial stellar mass assembly of Milky Way-sized galaxies
• Cumulative Neutrino and Gamma-Ray Backgrounds from Halo and Galaxy Mergers
• Galaxy formation in the Planck cosmology II. Star formation histories and post-processing magnitude reconstruction
• Constraints on the HI Mass of NGC 1052-DF2
• The complementary roles of feedback and mergers in building the gaseous halo and the X-ray corona of Milky Way-sized galaxies
• MCSED: A flexible spectral energy distribution fitting code and its application to $z\sim 2$ emission-line galaxies
• Galaxy And Mass Assembly (GAMA): The Bright Void Galaxy Population in the Optical and Mid-IR
• A Mock Catalog of Gravitationally Lensed Quasars for the LSST Survey
• X-ray observations of dust obscured galaxies in the Chandra Deep Field South
• Cosmic Galaxy-IGM HI Relation at $z\sim 2-3$ Probed in the COSMOS/UltraVISTA $1.6$ deg${}^2$ Field
• Long gamma-ray burst rate at very high redshift
• How the first stars shaped the faintest gas-dominated dwarf galaxies
• SH$\alpha$DE: Survey description and mass-kinematics scaling relations for dwarf galaxies
• Spectral Distortion of the CMB by the Cumulative CO Emission from Galaxies throughout Cosmic History
• An Explanation for Overrepresentation of Tidal Disruption Events in Post-starburst Galaxies
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• A scenario for ultra-diffuse satellite galaxies with low velocity dispersions: the case of [KKS 2000]04
• The Dynamics and Distribution of Angular Momentum in HiZELS Star-Forming Galaxies at z = 0.8 - 3.3
• The clustering of $z>7$ galaxies: Predictions from the BLUETIDES simulation
• Constraining the intrinsic population of Long Gamma-Ray Bursts: implications for spectral correlations, cosmic evolution and their use as tracers of star formation
• Differences and similarities of stellar populations in LAEs and LBGs at $z\sim$ 3.4 - 6.8
• First direct dynamical detection of a dual supermassive black hole system at sub-kiloparsec separation
• Dark acoustic oscillations: Imprints on the matter power spectrum and the halo mass function
• [OII] emitters in MultiDark-Galaxies and DEEP2
• Building robust AGN mock catalogs to unveil black hole evolution and for survey planning
• Keck Spectroscopy of the Coma Cluster Ultra-Diffuse Galaxy Y358: Dynamical Mass in a Wider Context
• The formation of the brightest cluster galaxy and intracluster light in cosmological N-body simulations with the Galaxy Replacement Technique
• Tidal disruption events can power the observed AGN in dwarf galaxies
• The evolution of dwarf galaxy satellites with different dark matter density profiles in the ErisMod simulations. I. The early infalls
• The origin of X-ray coronae around simulated disc galaxies
• Active Galactic Nuclei outflows in galaxy discs
• Galaxy stellar mass assembly: the difficulty matching observations and semi-analytical predictions
• A controlled study of cold dust content in galaxies from $z=0-2$
• The Effect of Adiabatic Compression on Dark Matter Halos and the Radial Acceleration Relation
• The mass-metallicity relation as a ruler for galaxy evolution: insights from the James Webb Space Telescope
• Exploring extensions to the standard cosmological model and the impact of baryons on small scales
• Star formation and AGN activity in the most luminous LINERs in the local universe
• Importance of Mock Observations in Validating Galaxy Properties for Cosmological Simulations
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• Black hole formation and growth with non-Gaussian primordial density perturbations
• Dark influences II: gas and star formation in minor mergers of dwarf galaxies with dark satellites
• The Variation of Rotation Curve Shapes as a Signature of the Effects of Baryons on Dark Matter Density Profiles
• The environment and host haloes of the brightest z~6 Lyman-break galaxies
• Multi-wavelength mock galaxy catalogs of the low-redshift Universe
• The GOGREEN Survey: Constraining the Satellite Quenching Timescale in Massive Clusters at $\mathbf{z}\gtrsim 1$
• Surrogate modelling the Baryonic Universe II: on forward modelling the colours of individual and populations of galaxies
• Galaxy rotation curves and universal scaling relations: comparison between phenomenological and fermionic dark matter profiles
• Study of gravitational fields and globular cluster systems of early-type galaxies
• Prospects for 21cm-Galaxy Cross-Correlations with HERA and the Roman High-Latitude Survey
• On the mass assembly of low-mass galaxies in hydrodynamical simulations of structure formation
• The effect of dark matter-dark radiation interactions on halo abundance -- a Press-Schechter approach
• Measuring the Stellar Masses of z~7 Galaxies with Spitzer Ultrafaint Survey Program (SURFS UP)
• TRINITY II: The Luminosity-dependent Bias of the Supermassive Black Hole Mass--Galaxy Mass Relation for Bright Quasars at $z=6$
• Feedback by supermassive black holes in galaxy evolution: impacts of accretion and outflows on the star formation rate
• Distortion of the luminosity function of high-redshift galaxies by gravitational lensing
• Mass Modeling of Frontier Fields Cluster MACS J1149.5+2223 Using Strong and Weak Lensing
• CHORUS. III. Photometric and Spectroscopic Properties of Ly$\alpha$ Blobs at $z=4.9-7.0$
• Clustering Constraints on the Relative Sizes of Central and Satellite Galaxies
• The VLA Frontier Field Survey: A Comparison of the Radio and UV/optical size of $0.3\lesssim z\lesssim 3$ star-forming galaxies
• Tidal stirring of satellites with shallow density profiles prevents them from being too big to fail
• LoCuSS: The Near-Infrared Luminosity and Weak-Lensing Mass Scaling Relation of Galaxy Clusters
• Galaxy cluster luminosities and colours, and their dependence on cluster mass and merger state
• Candidate Massive Galaxies at $z\sim 4$ in the Dark Energy Survey
• Tracing stars in Milky Way satellites with A-SLOTH
• An empirical measurement of the Halo Mass Function from the combination of GAMA DR4, SDSS DR12, and REFLEX II data
• Towards a new modelling of gas flows in a semi-analytical model of galaxy formation and evolution
• Dark Matter Response to Galaxy Assembly History
• Mapping the "invisible" circumgalactic medium around a z $\sim$ 4.5 radio galaxy with MUSE
• Main Sequence Scatter is Real: The Joint Dependence of Galaxy Clustering on Star Formation and Stellar Mass
• Characterising Tidal Features Around Galaxies in Cosmological Simulations
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• FIR-luminous [CII] emitters in the ALMA-SCUBA-2 COSMOS survey (AS2COSMOS): The nature of submillimeter galaxies in a 10 comoving Mpc-scale structure at z~4.6
• The baryon cycle of Seven Dwarfs with superbubble feedback
• A Framework for Empirical Galaxy Phenomenology: The Scatter in Galaxy Ages and Stellar Metallicities
• Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
• Informing dark matter direct detection limits with the ARTEMIS simulations
• The trajectories of galaxies in groups: mass loss and preprocessing
• Effects of feedback on galaxies in the VELA simulations: elongation, clumps and compaction
• Properties of the interstellar medium in star-forming galaxies at redshifts 2 < z < 5 from the VANDELS survey
• The changing circumgalactic medium over the last 10 Gyr I: physical and dynamical properties
• Some observational tests of a minimal galaxy formation model
• Quasi-equilibrium models of high-redshift disc galaxy evolution
• A galaxy group candidate at z~3.7 in the COSMOS field
• Formation and assembly history of stellar components in galaxies as a function of stellar and halo mass
• A complete distribution of redshifts for sub-millimetre galaxies in the SCUBA-2 Cosmology Legacy Survey UDS field
• The hidden satellites of massive galaxies and quasars at high-redshift
• Detection and classification of supernovae beyond z~2 redshift with the James Webb Space Telescope
• Constraining the Mass of the Emerging Galaxy Cluster SpARCS1049+56 at z=1.71 with Infrared Weak Lensing
• Reversal of Fortune: Increased Star Formation Efficiencies in the Early Histories of Dwarf Galaxies?
• Local photoionization feedback effects on galaxies
• Evidence for strong progenitor age dependence of type Ia supernova luminosity standardization process
• Mass and size growth of early-type galaxies by dry mergers in cluster environments
• The impact of dark energy on galaxy formation. What does the future of our Universe hold?
• Constraints on the Evolution of the Galaxy Stellar Mass Function I: Role of Star Formation, Mergers and Stellar Stripping
• The Diversity of Growth Histories of Milky Way-mass Galaxies
• The cosmological star formation history from the Local Cosmological Volume of galaxies and constraints on the matter homogeneity
• The XXL Survey X: K-band luminosity - weak-lensing mass relation for groups and clusters of galaxies
• Magnetogenesis at Cosmic Dawn: Tracing the Origins of Cosmic Magnetic Fields
• Quantifying the Origin and Distribution of Intracluster Light in a Fornax-like Cluster
• NOEMA formIng Cluster survEy (NICE): Characterizing eight massive galaxy groups at $1.5<z<4$ in the COSMOS field
• Gamma-ray Bursts and the Early Star-formation History
• The evolution of compact massive quiescent and starforming galaxies derived from the $R_e-R_h$ and $M_{\mathrm{star}}-M_h$ relations
• Characterising the signatures of star-forming galaxies in the extra-galactic $\gamma$-ray background
• Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots
• Setting firmer constraints on the evolution of the most massive, central galaxies from their local abundances and ages
• 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
• Measuring Dark Matter in Galaxies: The Mass Fraction Within 5 Effective Radii
• Gas Accretion and Galactic Chemical Evolution: Theory and Observations
• The frequency of very young galaxies in the local Universe: I. A test for galaxy formation and cosmological models
• NIHAO XXVI: Nature versus nurture, the Star Formation Main Sequence and the origin of its scatter
• The COSMOS-Web ring: in-depth characterization of an Einstein ring lensing system at z~2
• A multiwavelength survey of HI-excess galaxies with surprisingly inefficient star formation
• Noema formIng Cluster survEy (NICE): Discovery of a starbursting galaxy group with a radio-luminous core at z=3.95
• New empirical constraints on the cosmological evolution of gas and stars in galaxies
• Biases and Cosmic Variance in Molecular Gas Abundance Measurements
• Catalogue of model star clusters in the Milky Way and M31 galaxies
• Combining high-z galaxy luminosity functions with Bayesian evidence
• A new class of dark matter-free dwarf galaxies? I. Clues from FCC 224, NGC 1052-DF2 and NGC 1052-DF4
• The MUSE Hubble Ultra Deep Field Survey XVI. The angular momentum of low-mass star-forming galaxies. A cautionary tale and insights from TNG50
• Modeling Redshift-Space Clustering with Abundance Matching
• The Impacts of Modeling Choices on the Inference of the Circumgalactic Medium Properties from Sunyaev-Zeldovich Observations
• Effects of self-consistent rest-ultraviolet colours in semi-empirical galaxy formation models
• Revisiting the bulge-halo conspiracy II: Towards explaining its puzzling dependence on redshift
• MaNGA galaxy properties -- II. A detailed comparison of observed and simulated spiral galaxy scaling relations
• Halo Histories vs. Galaxy Properties at z=0, III: The Properties of Star-Forming Galaxies
• HI Global Scaling Relations in the WISE-WHISP Survey
• The Differing Relationships Between Size, Mass, Metallicity and Core Velocity Dispersion of Central and Satellite Galaxies
• 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
• Gas around galaxy haloes - III: hydrogen absorption signatures around galaxies and QSOs in the Sherwood simulation suite
• Calibration of a star formation and feedback model for cosmological simulations with Enzo
• Compact Binary Merger Rate in Dark-Matter Spikes
• Dependence of galaxy clustering on UV-luminosity and stellar mass at $z\sim 4-7$
• Using cosmological simulations and synthetic absorption spectra to assess the accuracy of observationally derived CGM metallicities
• On the Impact of Neutron Star Binaries Natal-Kick Distribution on the Galactic r-process Enrichment
• The galaxy - halo connection in low mass halos
• Brightest group galaxies-II: the relative contribution of BGGs to the total baryon content of groups at z<1.3
• Angular clustering and host halo properties of [OII] emitters at $z>1$ in the Subaru HSC survey
• On estimating the cosmic molecular gas density from CO Line Intensity Mapping observations
• Late Bloomer Galaxies: Growing Up in Cosmic Autumn
• Influence of ~7 keV sterile neutrino dark matter on the process of reionization
• The Baryonic Collapse Efficiency of Galaxy Groups in the RESOLVE and ECO Surveys
• The Impact of Environment on Late Time Evolution of the Stellar Mass - Halo Mass Relation
• The Chandra COSMOS Legacy Survey: clustering dependence of Type 2 AGN on host galaxy properties
• Multiple regimes and coalescence timescales for massive black hole pairs ; the critical role of galaxy formation physics
• HOD modelling of high redshift galaxies using the BLUETIDES simulation
• Using Artificial Neural Networks to Constrain the Halo Baryon Fraction during Reionization
• 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 $z<0.7$
• Simplified galaxy formation with mesh-less hydrodynamics
• The Mass and Absorption Columns of Galactic Gaseous Halos II -- The High Ionization State Ions
• A minimal empirical model for the cosmic far-infrared background anisotropies
• The radial acceleration relation is a natural consequence of the baryonic Tully-Fisher relation
• Revisiting the Extreme Clustering of $z\approx 4$ Quasars with Large Volume Cosmological Simulations
• IceCube's astrophysical neutrino energy spectrum from CPT violation
• How feedback shapes galaxies: an analytic model
• The Manhattan Suite: Accelerated galaxy evolution in the early Universe
• The Stellar-to-Halo Mass Ratios of Passive and Star-Forming Galaxies at z~2-3 from the SMUVS survey
• The tidal evolution of the Fornax dwarf spheroidal and its globular clusters
• The galaxy's gas content regulated by the dark matter halo mass results in a super-linear M${}_{\mathrm{BH}}$-M${}_{\star }$ relation
• Galactic Habitability Re-Examined: Indications of Bimodality
• A single galaxy population? statistical evidence that the Star-Forming Main Sequence might be the tip of the iceberg
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$. V: Properties of dark matter halos containing H$\alpha$ emitting galaxies
• Evidence for gas-phase metal deficiency in massive protocluster galaxies at z~2.2
• The frequency of very young galaxies in the local Universe: II. The view from SDSS spectra
• Explaining the chemical trajectories of accreted and in-situ halo stars of the Milky Way
• Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
• Bulge formation through disc instability -- I
• Evidence for galaxy quenching in the green valley caused by a lack of a circumgalactic medium
• Lonely Little Red Dots: Challenges to the AGN-nature of little red dots through their clustering and spectral energy distributions
• On the kinetic Sunyaev-Zel'dovich effect as an observational probe for halo spin bias
• DIGS: Deep Inference of Galaxy Spectra with Neural Posterior Estimation
• Multiscale mass transport in z~6 galactic discs: fueling black holes
• A Tale of a Tail: A Tidally-Disrupting Ultra-Diffuse Galaxy in the M81 Group
• The Relevance of Dynamical Friction for the MW/LMC/SMC Triple System
• Ionized Gas Outflows in Low Excitation Radio Galaxies Are Radiation Driven
• The metallicity and star formation activity of long gamma-ray burst hosts for z$<$3: insights from the Illustris simulation
• What Regulates Galaxy Evolution? Open Questions in Our Understanding of Galaxy Formation and Evolution
• Radial Distributions of Surface Mass Density and Mass-to-Luminosity Ratio in Spiral Galaxies
• Testing galaxy formation models with galaxy stellar mass functions
• Testing baryon-induced core formation in $\Lambda$CDM: A comparison of the DC14 and coreNFW dark matter halo models on galaxy rotation curves
• Connecting SDSS central galaxies to their host halos using total satellite luminosity
• JADES: Rest-frame UV-to-NIR Size Evolution of Massive Quiescent Galaxies from Redshift z=5 to z=0.5
• A titanic interstellar medium ejection from a massive starburst galaxy at redshift 1.4
• Comparing weak lensing peak counts in baryonic correction models to hydrodynamical simulations
• The Luminosity Functions and Redshift Evolution of Satellites of Low-Mass Galaxies in the COSMOS Survey
• Understanding the progenitor formation galaxies of merging binary black holes
• Black hole mergers as tracers of spinning massive black hole and galaxy populations in the OBELISK simulation
• GalICS 2.1: a new semianalytic model for cold accretion, cooling, feedback and their roles in galaxy formation
• Bimodal morphologies of massive galaxies at the core of a protocluster at z=3.09 and the strong size growth of a brightest cluster galaxy
• Explaining the enhanced star formation rate of Jellyfish galaxies in galaxy clusters
• The bright end of the galaxy luminosity function at $z\simeq 7$ from the VISTA VIDEO survey
• A partial inventory of observational anisotropies in single-dish line-intensity mapping
• Detecting clusters and groups of galaxies populating the local Universe in large optical spectroscopic surveys
• Dwarf galaxies as a probe of a primordially magnetized Universe
• Investigating the $M_{GCS}-M_h$ Relation in the Most Massive Galaxies
• Constraining Scatter in the Stellar Mass--Halo Mass Relation for Haloes Less Massive than the Milky Way
• Galaxy And Mass Assembly (GAMA): The absence of stellar mass segregation in galaxy groups and consistent predictions from GALFORM and EAGLE simulations
• A millimeter-wave redshift search for the unlensed HyLIRG, HS1700.850.1
• Non-parametric Morphologies of Mergers in the Illustris Simulation
• Effect of primordial non-Gaussianities on the far-UV luminosity function of high-redshift galaxies: implications for cosmic reionization
• Resolved and Integrated Stellar Masses in the SDSS-IV/MaNGA Survey, Paper I: PCA spectral fitting & stellar mass-to-light ratio estimates
• Star-forming galaxies at low-redshift in the SHARDS survey
• A unifying evolutionary framework for infrared-selected obscured and unobscured quasar host haloes
• Downsizing of Star Formation Measured from the Clustered Infrared Background Correlated with Quasars
• Cosmic Type Ia SN rate and constraints on SN Ia progenitors
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• Large gas inflow driven by a matured galactic bar in the early Universe
• AGN must be very efficient at powering outflows
• Differentiable Predictions for Large Scale Structure with SHAMNet
• The Merger Rate of Primordial Black Hole-Neutron Star Binaries in Ellipsoidal-Collapse Dark Matter Halo Models
• Halo Acceleration Relation
• The fate of a red nugget: In-situ star formation of satellites around a massive compact galaxy
• The evolution of cold neutral gas and the star formation history
• The Galaxy Replacement Technique (GRT): a New Approach to Study Tidal Stripping and Formation of Intracluster Light in a Cosmological Context
• Investigating the impact of galaxies' compact binary hosting probability for gravitational-wave cosmology
• Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
• Stellar Feedback and the Energy Budget of Late-Type Galaxies: Missing Baryons and Core Creation
• On estimation of contamination from hydrogen cyanide in carbon monoxide line intensity mapping
• The Coevolution of Massive Quiescent Galaxies and Their Dark Matter Halos over the Last 6 Billion Years
• Extragalactic Science with the Experiment for Cryogenic Large-aperture Intensity Mapping
• Satellite content and quenching of star formation in galaxy groups at z~1.8
• Mass assembly history and infall time of the Fornax dwarf spheroidal galaxy
• Galaxy-Galaxy Lensing in EAGLE: comparison with data from 180 square degrees of the KiDS and GAMA surveys
• Mapping the low surface brightness Universe in the UV band with Lya emission from IGM filaments
• On the Edge: the relation between stellar and dark matter haloes of Milky Way-mass galaxies
• The transformation and quenching of simulated gas-rich dwarf satellites within a group environment
• Distinguishing the impact and signature of black holes from different origins in early cosmic history
• Modified Gravity Theories in Light of the Anomalous Velocity Dispersion of NGC1052-DF2
• Spatially Resolved Gas-phase Metallicity in FIRE-2 Dwarfs: Late-Time Evolution of Metallicity Relations in Simulations with Feedback and Mergers
• Baryonic Imprints on DM Halos: The concentration-mass relation in the CAMELS simulations
• Galaxies of the $z\sim 2$ Universe. I. Grism-Selected Rest-Frame Optical Emission Line Galaxies
• Selecting ultra-faint dwarf candidate progenitors in cosmological N-body simulations at high redshifts
• The XMM-Newton Wide Field Survey in the COSMOS Field: Clustering Dependence of X-ray Selected AGN on Host Galaxy Properties
• SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
• Ironing the folds: The phase space chevrons of a GSE-like merger as a dark matter subhalo detector
• Revealing the formation mechanism of the shell galaxy NGC474 with MUSE
• Simulating Deep Hubble Images With Semi-empirical Models of Galaxy Formation
• HI within and around observed and simulated galaxy discs -- Comparing MeerKAT observations with mock data from TNG50 and FIRE-2
• HI study of isolated and pair galaxies: the MIR SFR-M$\star$ sequence
• Compatibility of the Large Quasar Groups with the Concordance Cosmological Model
• Unveiling cosmological information on small scales with line intensity mapping
• Self-Interacting Dark Matter and the Delay of Super-Massive Black Hole Growth
• A new method to constrain the origins of dark matter-free galaxies and their unusual globular clusters
• The quenched mass portion of star-forming galaxies and the origin of the star formation sequence slope
• Matching the mass function of Milky Way satellites in competing dark matter models
• A universal angular momentum profile for dark matter haloes
• Investigating overdensities around z>6 galaxies through ALMA observations of [CII]
• Looking for Traces of Non-minimally Coupled Dark Matter in the X-COP Galaxy Clusters Sample
• Empirical Evidence of Non-Minimally Coupled Dark Matter in the Dynamics of Local Spiral Galaxies?
• Recent progress in simulating galaxy formation from the largest to the smallest scales
• An intergalactic medium temperature from a giant radio galaxy
• Interpreting the cosmic far-infrared background anisotropies using a gas regulator model
• A super-linear "radio-AGN main sequence'' links mean radio-AGN power and galaxy stellar mass since z$\sim$3
• Gas around galaxy haloes: methodology comparisons using hydrodynamical simulations of the intergalactic medium
• The Herschel Virgo Cluster Survey. XIX. Physical properties of low luminosity FIR sources at $z<$ 0.5
• Extreme Galaxies During Reionization: Testing ISM and Disk Models
• A too-many dwarf galaxy satellites problem in the M83 group
• Dark matter fraction of low-mass cluster members probed by galaxy-scale strong lensing
• Unveiling the Origin of Fast Radio Bursts by Optical Follow Up Observations
• Recoiling Supermassive Black Hole Escape Velocities from Dark Matter Halos
• Angular momentum evolution of stellar disks at high redshifts
• Over-density of SMGs in fields containing z~0.3 galaxies: magnification bias and the implications for studies of galaxy evolution
• Dark Energy Survey Year 1 Results: The effect of intracluster light on photometric redshifts for weak gravitational lensing
• Multiverse Predictions for Habitability: The Number of Stars and their Properties
• How dark are filaments in the cosmic web?
• Applying Noether's theorem to matter in the Milky Way: evidence for external perturbations and non-steady-state effects from Gaia Data Release 2
• Candidate high-redshift protoclusters and lensed galaxies in the Planck list of high-z sources overlapping with Herschel-SPIRE imaging
• Pre-supernova feedback mechanisms drive the destruction of molecular clouds in nearby star-forming disc galaxies
• Testing multiflavored ULDM models with SPARC
• Strong-lensing cosmography using third-generation gravitational-wave detectors
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• Using the Star Forming Main Sequence To Explore Quiescent Galaxies Across Cosmic Time
• Life after AGN switchoff: evolution and properties of fossil galactic outflows
• Galaxy growth from redshift 5 to 0 at fixed comoving number density
• Feedback and dynamical masses in high-$z$ galaxies: the advent of high-resolution NIRSpec spectroscopy
• An empirical model to form and evolve galaxies in dark matter halos
• Searching for dark matter annihilation from individual halos: uncertainties, scatter and signal-to-noise ratios
• Exploring Self-Interacting Dark Matter Halos with Diverse Baryonic Distributions: A Parametric Approach
• Explaining ultra-massive quiescent galaxies at $3<z<5$ in the context of their environments
• The CO universe: Modelling CO emission and H${}_2$ abundance in cosmological galaxy formation simulations
• Simulated stellar kinematics studies of high-redshift galaxies with the HARMONI Integral Field Spectrograph
• A systematic search for galaxy protocluster cores at the transition epoch of their star formation activity
• Constraining the nature of dark matter with the star formation history of the faintest Local Group dwarf galaxy satellites
• Beacons In the Dark: Using Novae and Supernovae to Detect Dwarf Galaxies in the Local Universe
• Evolution of CIV Absorbers. II. Where does CIV live?
• Connecting the Dots: Tracking Galaxy Evolution Using Constant Cumulative Number Density at 3<z<7
• The detection of ultra-faint low surface brightness dwarf galaxies in the Virgo Cluster: a Probe of Dark Matter and Baryonic Physics
• The Disturbed and Globular Cluster-Rich Ultra-diffuse Galaxy UGC 9050-Dw1
• Origin and Evolution of Structure and Nucleosynthesis for Galaxies in the Local Group
• Revealing the host galaxy of a quasar 2175 Å dust absorber at z = 2.12
• Reconciling Mass Functions with the Star-Forming Main Sequence Via Mergers
• A comparison of the R_h=ct and LCDM cosmologies based on the observed halo mass function
• Bar-driven Leading Spiral Arms in a Counter-rotating Dark Matter Halo
• SZ Scaling Relations of Galaxy Groups and Clusters Near the North Ecliptic Pole
• The dark side of galaxy stellar populations II: The dependence of star formation histories on halo mass and on the scatter of the main sequence
• Faint Dwarfs in Nearby Groups
• The Impact of Wind Scalings on Stellar Growth and the Baryon Cycle in Cosmological Simulations
• Frequency of the dark matter subhalo collisions and bifurcation sequence arising formation of dwarf galaxies
• Primordial Black Hole-Neutron Star Merger Rate in Modified Gravity
• MOCCA-SURVEY Database -- I. Tidal disruption events of white dwarfs in globular clusters and young massive clusters
• A semi-analytical perspective on massive galaxies at $z\sim 0.55$
• Connection between galaxy morphology and dark-matter halo structure I: a running threshold for thin discs and size predictors from the dark sector
• Auriga Streams I: disrupting satellites surrounding Milky Way-mass haloes at multiple resolutions
• Constraints on Lorentz-invariance violation in the neutrino sector from the ultrahigh-energy event KM3-230213A
• A consistent model for both the HI and stellar mass functions of galaxies
• Abundance matching for low mass galaxies in the CDM and FDM models
• Dust Properties of Local Dust-Obscured Galaxies with the Submillimeter Array
• Dynamics and Shocks from H$\alpha$ Emission of Nearby Galaxy Mergers
• The signal of decaying dark matter with hydrodynamical simulations
• Galaxy mass-size segregation in the cosmic web from the CAVITY parent sample
• First results from SMAUG: Insights into star formation conditions from spatially-resolved ISM properties in TNG50
• Multiwavelength dissection of a massive heavily dust-obscured galaxy and its blue companion at z $\sim$2
• Gravity and the Nonlinear Growth of Structure in the Carnegie-Spitzer-IMACS Redshift Survey
• GABE: Galaxy Assembly with Binary Evolution
• A general framework to test gravity using galaxy clusters VI: Realistic galaxy formation simulations to study clusters in modified gravity
• Ghostly Halos in Dwarf Galaxies: Constraints on the Star Formation Efficiency before Reionization
• A Universal Profile for Stacked Filaments from Cold Dark Matter Simulations
• A selection of Hα emitters at z = 2.1-2.5 using the Ks-band photometry of ZFOURGE
• Approximations to galaxy star formation rate histories: properties and uses of two examples
• Effects of feedback-free starburst galaxies on the 21-cm signal and reionization history
• Reconciling Volumetric and Individual Galaxy Type Ia Supernova Rates
• The very wide-field $gzK$ galaxy survey -- II. The relationship between star-forming galaxies at $z\sim 2$ and their host haloes based upon HOD modelling
• Intervening or associated? Machine learning classification of redshifted H I 21-cm absorption
• Insights on star formation histories and physical properties of $1.2\le z\lesssim 4$ Herschel-detected galaxies
• Cosmic star formation probed via parametric stack-fitting of known sources to radio imaging
• Using large galaxy surveys to distinguish z~0.5 quiescent galaxy models
• Properties of the circumgalactic medium in simulations compared to observations
• Dark matter halos and the M-σrelation for supermassive black holes
• The Stellar Mass - Halo Mass Relation for Low Mass X-ray Groups at 0.5<z<1 in the CDFS with CSI
• Galactic wind X-ray heating of the intergalactic medium during the Epoch of Reionization
• Co-Evolution vs. Co-existence: The Effect of Accretion Modelling on the Evolution of Black Holes and Host Galaxies
• Sunscreen: Photometric Signatures of Galaxies Partially Cloaked in Dyson Spheres
• Black hole feedback and the evolution of massive early-type galaxies
• Probing the Mpc-scale environment of hyperluminous infrared galaxies at 2<z<4
• Stellar Metallicity of Galaxies: New Insight on the Formation and Evolution of Low Surface Brightness Galaxies in the IllustrisTNG Simulation
• Confusion of extragalactic sources in the far infrared: a baseline assessment of the performance of PRIMAger in intensity and polarization
• Mapping the Universe in HD
• Ghostly Stellar Haloes and their Relationship to Ultra-faint Dwarfs
• Characterizing simulated galaxy stellar mass histories
• Lorentz violation footprints in the spectrum of high-energy cosmic neutrinos: Deformation of the spectrum of superluminal neutrinos from electron-positron pair production in vacuum
• The Dark Matter Halos of HI Selected Galaxies
• Size, shade or shape? The contribution of galaxies of different types to the star-formation history of the Universe from SDSS-IV MaNGA
• 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
• Possible evolution of the circum-galactic medium around QSOs with QSO age and cosmic time revealed by Ly$\alpha$ halos
• The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
• PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at $0.2<z<0.9$
• The XXL survey. XLIX. Linking the members star formation histories to the cluster mass assembly in the z=1.98 galaxy cluster XLSSC 122
• Gamma-ray Production in the Extended Halo of the Galaxy and Possible Implications for the Origin of Galactic Cosmic Rays
• ARTEMIS emulator: exploring the effect of cosmology and galaxy formation physics on Milky Way-mass haloes and their satellites
• Analysis of the spatially-resolved $V$-3.6$\mu$m colors and dust extinction in 257 nearby NGC and IC galaxies
• A Physical Model for the Quasar Luminosity Function Evolution between Cosmic Dawn and High Noon
• PAC in DESI. I. Galaxy Stellar Mass Function into the $10^6{\mathrm{M}}_{\odot }$ Frontier
• A Hyperactive FRB Pinpointed in an SMC-Like Satellite Host Galaxy
• The stellar mass function and efficiency of galaxy formation with a varying initial mass function
• The THESAN-ZOOM project: Star-formation efficiencies in high-redshift galaxies
• Constraining the host galaxy halos of massive black holes from LISA event rates
• The deconvolved distribution estimator: enhancing reionisation-era CO line-intensity mapping analyses with a cross-correlation analogue for one-point statistics
• Distribution of star formation rates during the rapid assembly of NGC 1399 as deduced from its globular cluster system
• Impact of star formation models on the growth of simulated galaxies at high redshifts
• Enhanced spectrum of primordial perturbations, galaxy formation and small scale structure
• A comparison of ${\text{H}}_2$ formation models at high redshift
• A Stochastic Theory of the Hierarchical Clustering II. Halo progenitor mass function and large-scale bias
• Explaining JWST star formation history at $z\sim 17$ by modifying $\Lambda$CDM
• Abundance matching tested on small scales with galaxy dynamics
• EMERGE: Constraining merging probabilities and timescales of close galaxy pairs
• Diverse dark matter profiles in FIRE dwarfs: black holes, cosmic rays and the cusp-core enigma
• JWST PRIMER: A deep JWST study of all ALMA-detected galaxies in PRIMER COSMOS -- dust-obscured star-formation history back to z $\simeq$ 7
• Fingerprints of modified gravity on galaxies in voids
• The fundamental plane of evolving red nuggets
• Insights on Metal Enrichment and Environmental Effect at $z\approx 5-7$ with JWST ASPIRE/EIGER and Chemical Evolution Model
• Where Did the Outskirts Go? Outer Stellar Haloes as a Sensitive Probe of Supernova Feedback
• The extended Planetary Nebula Spectrograph (ePN.S) early-type galaxy survey: The specific angular momentum of ETGs
• Testing primordial non-Gaussianities on galactic scales at high redshift
• Classical bulges, supermassive blackholes and AGN feedback: Extension to low-mass galaxies
• The Effects of Dark Matter Annihilation on Cosmic Reionization
• Imprint of the galactic acceleration scale on globular cluster systems
• From Gas to Stars Over Cosmic Time
• A break in the high-redshift stellar mass Tully-Fisher relation
• The significant effects of stellar mass estimation on galaxy pair fractions
• When relics were made: vigorous stellar rotation and low dark matter content in the massive ultra-compact galaxy GS-9209 at z=4.66
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• Globular cluster ages and their relation to high-redshift stellar cluster formation times from different globular cluster models
• Unveiling Multiple Physical Processes on a Cluster Galaxy at z=0.3 Using JWST
• EDEN: Exploring Disks Embedded in N-body simulations of Milky-Way-mass halos from Symphony
• Compact Binary Merger Rate with Modified Gravity in Dark-Matter Spikes
• Revealing the hidden cosmic feast: A z=4.3 galaxy group hosting two optically dark, efficiently star-forming galaxies
• Scalar Stochastic Gravitational-Wave Background in Brans-Dicke Theory of Gravity
• The Galaxy Halo Connection in Modified Gravity Cosmologies: Environment Dependence of Galaxy Luminosity function
• The resolved star formation history of M51a through successive Bayesian marginalization
• A two-phase model of galaxy formation: III. The formation of globular clusters
• Dynamical Properties of Molecular-forming Gas Clumps in Galaxies at the Epoch of Reionization
• A Multi-messenger view of Cosmic Dawn: Conquering the Final Frontier
• Detecting Massive Galaxies at High Redshift using the Dark Energy Survey
• AGN lifetimes in UV-selected galaxies: a clue to supermassive black hole-host galaxy coevolution
• Cosmic star formation history with tomographic cosmic infrared background-galaxy cross-correlation
• A physical model for the redshift evolution of high-z Lyman-Break Galaxies
• Local Two-Sample Testing: A New Tool for Analysing High-Dimensional Astronomical Data
• The Halo Masses of Galaxies to $z\sim 3$: A Hybrid Observational and Theoretical Approach
• Measuring Dust Attenuation Curves of SINGS/KINGFISH Galaxies Using Swift/UVOT Photometry
• Toward a stellar population catalog in the Kilo Degree Survey: the impact of stellar recipes on stellar masses and star formation rates
• The properties and environment of very young galaxies in the local Universe
• Observations of Ly$\alpha$ Emitters at High Redshift
• Predictions for Detecting a Turndown in the Baryonic Tully Fisher Relation
• On the Effects of Local Environment on Active Galactic Nucleus (AGN) in the Horizon Run 5 Simulation
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• Modelling the mass accretion histories of dark matter haloes using a Gamma formalism
• HELLO project: High-$z$ Evolution of Large and Luminous Objects
• Revisiting the Relationship between the Long GRB Rate and Cosmic Star Formation History Based on a Large Swift Sample
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• Variations of the ISM Compactness Across the Main Sequence of Star-Forming Galaxies: Observations and Simulations
• A rising tide: Intrinsic alignments since the turn of the millennium
• UV and NIR size of the low-mass field galaxies: the UV compact galaxies
• Does radiative feedback make faint z>6 galaxies look small?
• Globular Cluster Systems and X-Ray Atmospheres in Galaxies
• Die Hard: The On-Off-Cycle of Galaxies on the Star Formation Main Sequence
• Properties of galaxies at the faint end of the H$\alpha$ luminosity function at $z\sim 0.62$
• The miniJPAS survey. Evolution of the luminosity and stellar mass functions of galaxies up to $z\sim 0.7$
• Subhalo abundance matching using progenitor mass at varying redshift: Two modes of stellar mass growth imprinted into the Subaru HSC galaxy clustering
• The size function of massive satellites from the $R_e-R_h$ and $M_{star}-M_h$ relations: constraining the role of environment
• Anatomy of galactic star formation history: Roles of different modes of gas accretion, feedback, and recycling
• AuriDESI: Mock Catalogues for the DESI Milky Way Survey
• Feeding and feedback from little monsters: AGN in dwarf galaxies
• Star formation across cosmic time
• EIG - II. Intriguing characteristics of the most extremely isolated galaxies
• Galaxy formation from a timescale perspective
• Fading Light, Fierce Winds: JWST Snapshot of a Sub-Eddington Quasar at Cosmic Dawn
• Inferring Cosmological Parameters on SDSS via Domain-Generalized Neural Networks and Lightcone Simulations
• Lessons from the Local Group (and beyond) on dark matter
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• An Empirical Mass Function Distribution
• Radiation-driven dusty outflows from early galaxies
• The inflow and outflow rate evolution of local Milky Way-mass star-forming galaxies since z=1.3
• Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
• Evolution of dwarf galaxy observable parameters
• Cosmic evolution of molecular gas mass density from an empirical relation between ${\mathrm{L}}_{1.4GHz}$ and ${\mathrm{L}}_{\mathrm{CO}}^{\prime }$
• Massive Black Hole Mergers
• Leveraging cross-correlations and linear covariance-based filtering for line-intensity map reconstructions at linear scales
• A Rich Satellite Population of the NGC 4437 Group and Implications of a Magnitude Gap for Galaxy Group Assembly History
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• A Galaxy-Halo Model for Multiple Cosmological Tracers
• Calibrating baryonic effects in cosmic shear with external data in the LSST era
• Euclid: Early Release Observations of ram-pressure stripping in the Perseus cluster. Detection of parsec scale star formation with in the low surface brightness stripped tails of UGC 2665 and MCG +07-07-070
• Quenching vs. Quiescence: forming realistic massive ellipticals with a simple starvation model
• COMAP Pathfinder -- Season 2 results III. Implications for cosmic molecular gas content at "Cosmic Half-past Eleven"
• Euclid preparation. Exploring the properties of proto-clusters in the Simulated Euclid Wide Survey
• Evolving beyond z=0: insights about the future of stars and the intergalactic medium
• Impact of the turnover in the high-z galaxy luminosity function on the 21-cm signal during Cosmic Dawn and Epoch of Reionization
• Models of AGN feedback
• Stacked phase-space density of galaxies around massive clusters: Comparison of dynamical and lensing masses
• A candidate quadruple AGN system at $z\sim 3$
• Galaxy Assembly and Evolution in the P-Millennium simulation: galaxy clustering
• Spatial Distribution of OVI Covering Fractions in the Simulated Circumgalactic Medium
• Three-Dimensional Stacking as a Line Intensity Mapping Statistic
• New observational recipes for measuring dynamical state of galaxy clusters
• Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
• The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
• Tracing the Total Stellar Mass and Star Formation of High-Redshift Protoclusters
• Modeling spatially-resolved galactic H$\alpha$ emission for galaxy clustering
• Deciphering the Kinematic Substructure of Local Dark Matter with LAMOST K Giants
• Morpho-Photometric Classification of KiDS DR5 Sources Based on Neural Networks: A Comprehensive Star-Quasar-Galaxy Catalog
• GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations
• Analysis of the Intrinsic Mid-Infrared L-band to Visible--Near-Infrared Flux Ratios in Spectral Synthesis Models of Composite Stellar Populations
• Testing Models of Quasar Hosts With Strong Gravitational Lensing by Quasar Hosts
• The Galaxy Activity, Torus, and Outflow Survey (GATOS). Black hole mass estimation using machine learning
• A MUSE view of the multiple interacting system HCG 31
• Modelling the Evolution of Ly$\alpha$ Blobs and Ly$\alpha$ Emitters
• Pulsar B1237+25 Aberration/Retardation Analysis from Decimeter to Decameter Wavelength: Challenge to "Radius-to-Frequency Mapping"
• The ALMaQUEST Survey XVII: Unveiling Multiple Quenching Pathways in Green Valley Galaxies via Molecular Gas and Quenching Timescale Analyses
• ELG$\times$LRG distribution through dark matter halo dynamics
• Cosmic Vine: High abundance of massive galaxies and dark matter halos in a forming cluster at z=3.44
• Direct Shear Mapping: Prospects for weak lensing studies of individual galaxy-galaxy lensing systems
• The origin of galaxy colour bimodality in the scatter of the Stellar-to-Halo Mass Relation
• JWSTs PEARLS: NIRCam imaging and NIRISS spectroscopy of a $z=3.6$ star-forming galaxy lensed into a near-Einstein Ring by a $z=1.258$ massive elliptical galaxy
• PASSAGES: The Discovery of a Strongly Lensed Protocluster Core Candidate at Cosmic Noon
• Applying a star formation model calibrated on high-resolution interstellar medium simulations to cosmological simulations of galaxy formation
• An ALMA spectroscopic survey of the Planck high-redshift object PLCK G073.4-57.5 confirms two protoclusters
• Exploring effects of IMF sampling and SN feedback injection on star formation and metallicity in ultra-faint dwarf galaxies
• Understanding Stellar Mass-Metallicity and Size Relations in Simulated Ultra-Faint Dwarf Galaxies
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Impact of supermassive black hole growth on star formation
• Stellar halos tracing the assembly of ultra-faint dwarf galaxies
• IllustrisTNG + Cosmic Rays with a Simple Transport Model: From Dwarfs to L${}^{\star }$ Galaxies
• Globular cluster orbital decay in dwarf galaxies with MOND and CDM: Impact of supernova feedback
• A Recent Starbust in the Low Surface Brightness Galaxy UGC 628
• The Assembly of the Virgo Cluster, Traced by its Galaxy Halos
• A Stochastic Theory of the Hierarchical Clustering III. The Non-universality and Non-stationarity of the Halo Mass Function
• How do the dynamics of the Milky Way -- Large Magellanic Cloud system affect gamma-ray constraints on particle dark matter?
• Cosmological prior for the $J$-factor estimation of dwarf spheroidal galaxies
• Impact of Cosmic Variance on the Galaxy-Halo Connection for Lyman-$\alpha$ Emitters
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• Star formation rates in nearby Markarian galaxies
• Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies: Black Hole Scaling Relations Are Not Biased by Selection Effects
• The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
• Peculiar dark matter halos inferred from gravitational lensing as a manifestation of modified gravity
• Removal of interloper contamination to line-intensity maps using correlations with ancillary tracers of the large-scale structure
• Dark Energy Survey Year 6 Results: Intra-Cluster Light from Redshift 0.2 to 0.5
• Dark-Matter-Deficient Galaxies from Collisions: A New Probe of Bursty Feedback and Dark Matter Physics
• SOFIA/HAWC+ detection of a gravitationally lensed starburst galaxy at $z$ = 1.03
• Machine Learning vs. Spectral Energy Distribution Fitting: A Comparative Analysis of Accuracy in Stellar Mass Estimation
• Linking Compact Dwarf Starburst Galaxies in the RESOLVE Survey to Downsized Blue Nuggets
• The intervelocity of galaxy pairs in $\Lambda$CDM -- The observed velocity peak at ~130 km/s is not unique to MOND
• Dark energy, spatial curvature, and star formation efficiency from JWST photometric and spectroscopic high-redshift galaxies
• Compact dust-obscured star-formation and the origin of the galaxy bimodality
• X-ray stacking reveals average SMBH accretion properties of star-forming galaxies and their cosmic evolution over 4 <~ z <~ 7
• The informativeness of [C II] line-intensity mapping as a probe of the H I content and metallicity of galaxies at the end of reionization
• Nearby dwarf galaxies with extreme star formation rates: a window into dwarf-galaxy evolution in the early Universe
• Machine Learning the Dark Matter Halo Mass of Milky Way-Like Systems
• SEMPER I. Radio Predictions for Star-Forming Galaxies at $0<z<5$
• Constraining the halo-ISM connection through multi-transition carbon monoxide line-intensity mapping
• A Submillimeter Continuum Survey of Local Dust-Obscured Galaxies
• Mapping luminous and dark matter in the Universe
• Simultaneously Modelling Dusty Star Forming Galaxies and Massive Quiescents: A Calibration Framework for Galaxy Formation Models
• Quenching Global Star Formation: Dominance of Gravitational Shock Heating at z<2
• Self-sustaining star formation fronts in filaments during cosmic dawn
• Euclid preparation: TBD. Cosmic Dawn Survey: evolution of the galaxy stellar mass function across 0.2<z<6.5 measured over 10 square degrees
• Spatial correlations of extended cosmological structures
• Super-Eddington accretion in high-redshift quasar hosts: Black-hole driven outflows, galaxy quenching, and the nature of little red dots
• Search for the Footprints of New Physics with Laboratory and Cosmic Neutrinos
• MIGHTEE-HI: The star-forming properties of HI selected galaxies
• Constraints on dark matter models from the stellar cores observed in ultra-faint dwarf galaxies: Self-interacting dark matter
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• Submillimeter galaxy overdensities around physically associated quasar pairs
• A Redshift Survey of the Coma Cluster (A1656): Understanding the Nature of Subhalos in the Weak-lensing Map
• Properties of Globular Clusters in Galaxy Clusters: Sensitivity from the Formation and Evolution of Globular Clusters
• Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future
• Probabilistic Inference of the Structure and Orbit of Milky Way Satellites with Semi-Analytic Modeling
• The galactic acceleration scale is imprinted on globular cluster systems of early-type galaxies of most masses and on red and blue globular cluster subpopulations
• Insights into the dependence of galaxy properties on the environment with explainable machine learning models
• The MUSE Hubble Ultra Deep Field Survey XIV. The evolution of the Lya emitter fraction from z=3 to z=6
• Characterizing CO Emitters in the SSA22-AzTEC26 Field
• Dark-matter-induced transients over cosmic time: The role of star formation history profiles
• What triggers type Ia supernovae: Prompt detonations from primordial black holes or companion stars?
• The multi-component fitting to the star formation histories in the TNG simulation
• Free-floating molecular clumps and gas mixing: hydrodynamic aftermaths of the intracluster$-$interstellar medium interaction
• Far-infrared lines hidden in archival deep multi-wavelength surveys: Limits on [CII]-158$\mu$m at $z\sim 0.3-2.9$
• Covariances of Galaxy Stellar Mass Functions and Correlation Functions
• Gamma Analytical Modeling Evolution (GAME) I: The physical implications of deriving the stellar mass functions from z=0 to z=8
• Testing Lorentz Symmetry using High Energy Astrophysics Observations
• Dynamical evolution timescales for the supermassive black hole system in the galaxy NGC 7727 (Arp 222)
• Constraints on the existence of dark matter haloes by the M81 group and the Hickson compact groups of galaxies
• CHILES X: Molecular and atomic gas at intermediate redshift
• Gas thermodynamics meets galaxy kinematics: Joint mass measurements for eROSITA galaxy clusters
• ODIN: Using multiplicity of Lyman-Alpha Emitters to assess star formation activity in dark matter halos
• Atmospheric pressure and molecular cloud formation in early-type galaxies
• Sub-Gyr variability around the SFMS and its contribution to the scatter
• The Effect of Impact Parameters on the Formation of Massive Black Hole Binaries in Galactic Mergers
• NIHAO-LG: The uniqueness of Local Group dwarf galaxies
• Extended Hernquist-Springel formalism for cosmic star formation
• A hierarchical clustering method for quantifying satellite abundance
• Star formation quenching precedes morphological transformation in COSMOS-WEB's richest galaxy groups
• Strong Conformity and Assembly Bias: Towards a Physical Understanding of the Galaxy-Halo Connection in SDSS Clusters
• Cosmological Simulations of Satellites around Isolated Dwarf Galaxies
• A New Model For Including Galactic Winds in Simulations of Galaxy Formation II: Implementation of PhEW in Cosmological Simulations
• All the Massive Galaxy Overdensities during Reionization: JWST Rest-Frame Optical Selection Reveals Young, Chemically Evolved Galaxies Embedded in Dense, Neutral Gas at z > 5
• Reconstructing the mass accretion histories of nearby Red Nuggets with their globular cluster systems
• Subhalo abundance and satellite spatial distribution in Milky Way-Andromeda-like paired haloes
• Galaxies in X-ray Selected Clusters and Groups in Dark Energy Survey Data II: Hierarchical Bayesian Modeling of the Red-Sequence Galaxy Luminosity Function
• Main sequence of star formation and colour bimodality considering galaxy environment
• HI Observations of Baryon-Dominated Dwarf Galaxy Candidates
• The Photometric Analysis of the Environment Around Two Dusty Star-Forming Galaxies at $z\sim 2$
• Suppression of galactic outflows by cosmological infall and circumgalactic medium
• Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter
• Space Project for Astrophysical and Cosmological Exploration (SPACE), an ESA stand-alone mission and a possible contribution to the Origins Space Telescope
• Spider-Webb: enhanced star formation in low-mass galaxies within the Spiderweb protocluster revealed by JWST Pa$\beta$ narrow-band imaging
• LYRA II: Cosmological dwarf galaxy formation with inhomogeneous Population III enrichment
• Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling
• Effect of dust in circumgalactic haloes on the cosmic shear power spectrum
• Correlation between Outlying Halo Abundance and Host Halo Properties
• Initial Investigations of the Outskirts of XLSSC 122
• Stochastic Gravitational-Wave Background from Stellar Core-Collapse Events
• Massive black holes and their galaxies
• Size-scaling of clump instabilities in turbulent, feedback regulated disks
• The odd primordial halo of the Milky Way implied by Gaia. A shallow core, but a steep decline
• Merging massive black holes: the right place and the right time
• Spatially resolved stellar-to-total dynamical mass relation: Radial variations, gradients and profiles of galaxy stellar populations
• An empirical model of the extragalactic radio background
• Forming off-center massive black hole binaries in dwarf galaxies through Jacobi capture
• Dwarf Galaxy Number Counts within 25 Mpc: Predictions from Local Group Analogues in TNG50
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
• NeutralUniverseMachine: Predictions of HI gas in Different Theoretical Models
• Astrophysical Black holes: An Explanation for the Galaxy Quenching
• Controlled Experiments on Dark-Matter Halo Structure and Galaxy Morphology I: What Sets Galaxy Sizes?
• Comparison of Cross-Correlation Methods for Line Intensity Mapping
• The kinematic imprinting of environmental quenching in $z<0.2$ galaxies
• Could the high-mass black holes from gravitational-wave observations be explained by lensing?
• pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue
• Baryonic Ecosystem IN Galaxies (BEINGMgII) -- III. Cool gas reservoirs at $0.3\le z\le 1.6$ in the Dark Energy Survey
• Cross-correlations between mm-wave line-intensity mapping and weak lensing surveys: preliminary consideration of long-term prospects
• Detecting the $\pi$-axiverse through parametric resonance
• A Mass Dependent Density Profile from Dwarfs to Clusters
• The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
• Resonant optical gating of suspended carbon nanotube transistor
• Decoding the star forming properties of gas-rich galaxy pairs
• CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA
• Exploring the gaseous halos of z>3 radio galaxies with UVES and JWST/NIRSpec
• The Cen A galaxy group: dynamical mass and missing baryons
• Forward-modelling the Luminosity, Distance, and Size distributions of the Milky Way Satellites
• Turbulence in the intragroup and circumgalactic medium
• A quantitative assessment of completeness correction methods and public release of a versatile simulation code
• Estimating Transient Rates from Cosmological Simulations and BPASS
• Physics of star formation history and the luminosity function of galaxies therefrom
• Clustering and physical properties of AGN and Star-Forming Galaxies at fixed stellar mass: does assembly bias have a role in AGN activity?
• Origin of the spectacular tidal shells of galaxy NGC474
• 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
• Momentum deposition of supernovae with cosmic rays