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)

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• A Simple Technique for Predicting High-Redshift Galaxy Evolution
• CFHTLenS: Co-evolution of galaxies and their dark matter haloes
• New Constraints on the Faint-end of the UV Luminosity Function at z~7-8 using the Gravitational Lensing of the Hubble Frontier Fields Cluster A2744
• EDGE: the mass-metallicity relation as a critical test of galaxy formation physics
• CEERS Spectroscopic Confirmation of NIRCam-Selected z > 8 Galaxy Candidates with JWST/NIRSpec: Initial Characterization of their Properties
• The Population of Giant Clumps in Simulated High-z Galaxies: In-situ and Ex-situ, Migration and Survival
• On the possible environmental effect in distributing heavy elements beyond individual gaseous halos
• The formation and hierarchical assembly of globular cluster populations
• Galaxy Stellar Mass Functions from z~10 to z~6 using the Deepest Spitzer/IRAC Data: No Significant Evolution in the Stellar-to-Halo Mass Ratio of Galaxies in the First Gyr of Cosmic Time
• Evolution of the UV LF from z~15 to z~8 Using New JWST NIRCam Medium-Band Observations over the HUDF/XDF
• Line-Intensity Mapping: 2017 Status Report
• Gravitational probes of dark matter physics
• The Baryon Cycle of Dwarf Galaxies: Dark, Bursty, Gas-Rich Polluters
• The Difficulty of Getting High Escape Fractions of Ionizing Photons from High-redshift Galaxies: a View from the FIRE Cosmological Simulations
• Galactic Dark Matter Halos and Globular Cluster Populations. III: Extension to Extreme Environments
• A distance of 13 Mpc resolves the claimed anomalies of the galaxy lacking dark matter
• New synthesis models of consistent extragalactic background light over cosmic time
• The galaxy-halo connection from a joint lensing, clustering and abundance analysis in the CFHTLenS/VIPERS field
• Extreme Value Statistics of the Halo and Stellar Mass Distributions at High Redshift: are JWST Results in Tension with ΛCDM?
• The fraction of dark matter within galaxies from the IllustrisTNG simulations
• Spreading out and staying sharp - Creating diverse rotation curves via baryonic and self-interaction effects
• Still Missing Dark Matter: KCWI High-Resolution Stellar Kinematics of NGC1052-DF2
• Giant Clumps in Simulated High-z Galaxies: Properties, Evolution and Dependence on Feedback
• ZFOURGE/CANDELS: On the Evolution of M* Galaxy Progenitors from z=3 to 0.5
• GAMA/H-ATLAS: A meta-analysis of SFR indicators - comprehensive measures of the SFR-M* relation and Cosmic Star Formation History at z < 0.4
• Disentangling satellite galaxy populations using orbit tracking in simulations
• Fundamental Mass-Spin-Morphology Relation of Spiral Galaxies
• The MOSDEF Survey: Dissecting the star-formation rate vs. stellar mass relation using H$\alpha$ and H$\beta$ emission lines at z ~ 2
• Reionization and high-redshift galaxies: the view from quasar absorption lines
• MUFASA: Galaxy star formation, gas, and metal properties across cosmic time
• The Evolution of the Baryons Associated with Galaxies Averaged over Cosmic Time and Space
• A Geometrically Supported $z\sim 10$ Candidate Multiply-Imaged by the Hubble Frontier Fields Cluster Abell 2744
• Observational Searches for Galaxies at z > 6
• Mining Circumgalactic Baryons in the Low-Redshift Universe
• Star cluster formation in cosmological simulations. I. Properties of young clusters
• The origin of scatter in the stellar mass - halo mass relation of central galaxies in the EAGLE simulation
• The E-MOSAICS project: tracing galaxy formation and assembly with the age-metallicity distribution of globular clusters
• The Universe at z>10: Predictions for JWST from the UniverseMachine DR1
• Using Cumulative Number Densities to Compare Galaxies across Cosmic Time
• NIHAO XV: The environmental impact of the host galaxy on galactic satellite and field dwarf galaxies
• An observational determination of the evolving extragalactic background light from the multiwavelength HST/CANDELS survey in the Fermi and CTA era
• The Structure of Multiphase Galactic Winds
• Connecting the first galaxies with ultra faint dwarfs in the Local Group: chemical signatures of Population~III stars
• First Light And Reionisation Epoch Simulations (FLARES) I: Environmental Dependence of High-Redshift Galaxy Evolution
• The alignment and shape of dark matter, stellar, and hot gas distributions in the EAGLE and cosmo-OWLS simulations
• Organized Chaos: Scatter in the relation between stellar mass and halo mass in small galaxies
• GOLDRUSH. II. Clustering of Galaxies at $z\sim 4-6$ Revealed with the Half-Million Dropouts Over the 100 deg${}^2$ Area Corresponding to 1 Gpc${}^3$
• HerMES: The Contribution to the Cosmic Infrared Background from Galaxies Selected by Mass and Redshift
• Efficiency of gas cooling and accretion at the disc-corona interface
• Zooming on the internal structure of $z\simeq 6$ galaxies
• The Swift Gamma-Ray Burst Host Galaxy Legacy Survey - I. Sample Selection and Redshift Distribution
• The Ubiquity of Coeval Starbursts in Massive Galaxy Cluster Progenitors
• Galaxy And Mass Assembly (GAMA): Stellar mass functions by Hubble type
• Dust attenuation in 2<z<3 star-forming galaxies from deep ALMA observations of the Hubble Ultra Deep Field
• Dark Matter Halos in Galaxies and Globular Cluster Populations
• The Relationship between Galaxy and Dark Matter Halo Size from z~3 to the present
• Semi-Analytic Galaxies - I. Synthesis of environmental and star-forming regulation mechanisms
• Dark-ages reionization and galaxy formation simulation - III. Modelling galaxy formation and the epoch of reionization
• Is the dark-matter halo spin a predictor of galaxy spin and size?
• The Dawes Review 8: Measuring the Stellar Initial Mass Function
• On the SFR-M${}_{\ast }$ main sequence archetypal star-formation history and analytical models
• Feedback from Active Galactic Nuclei in Galaxy Groups
• The accretion history of dark matter halos I: The physical origin of the universal function
• The origin of the diverse morphologies and kinematics of Milky Way-mass galaxies in the FIRE-2 simulations
• The Globular Cluster Systems of Ultra-Diffuse Galaxies in the Coma Cluster
• Ages of Type Ia Supernovae Over Cosmic Time
• The impact of chemistry on the structure of high-z galaxies
• SDSS IV MaNGA: The global and local stellar mass assemby histories of galaxies
• The impact of stellar feedback on the structure, size and morphology of galaxies in Milky Way size dark matter haloes
• Phat ELVIS: The inevitable effect of the Milky Way's disk on its dark matter subhaloes
• Mergers and Mass Accretion for Infalling Halos Both End Well Outside Cluster Virial Radii
• Stochastic modelling of star-formation histories II: star-formation variability from molecular clouds and gas inflow
• Rapid Environmental Quenching of Satellite Dwarf Galaxies in the Local Group
• Evidence for a change in the dominant satellite galaxy quenching mechanism at z=1
• Connecting CO Intensity Mapping to Molecular Gas and Star Formation in the Epoch of Galaxy Assembly
• The Argo Simulation: I. Quenching of Massive Galaxies at High Redshift as a Result of Cosmological Starvation
• Evolution of Stellar-to-Halo Mass Ratio at z=0-7 Identified by Clustering Analysis with the Hubble Legacy Imaging and Early Subaru/Hyper Suprime-Cam Survey Data
• RUBIES: Evolved Stellar Populations with Extended Formation Histories at $z\sim 7-8$ in Candidate Massive Galaxies Identified with JWST/NIRSpec
• Dark matter halos of massive elliptical galaxies at $z\sim 0.2$ are well described by the Navarro-Frenk-White profile
• The IMACS Cluster Building Survey: IV. The Log-normal Star Formation History of Galaxies
• Dwarf Galaxy Dark Matter Density Profiles Inferred from Stellar and Gas Kinematics
• The ASTRID Simulation: Galaxy Formation and Reionization
• Interpreting ALMA Observations of the ISM During the Epoch of Reionisation
• The Impact of the First Galaxies on Cosmic Dawn and Reionization
• The escape speed curve of the Galaxy obtained from Gaia DR2 implies a heavy Milky Way
• Dark Matter Heating and Early Core Formation in Dwarf Galaxies
• The MUSE-Wide Survey: Survey Description and First Data Release
• Baryon-induced dark matter cores in the EAGLE simulations
• How to quench a galaxy
• L-GALAXIES 2020: Spatially resolved cold gas phases, star formation and chemical enrichment in galactic discs
• Pushing back the limits: detailed properties of dwarf galaxies in a LCDM universe
• The ALPINE-ALMA [CII] survey: Molecular gas budget in the Early Universe as traced by [CII]
• Reconstruction of Galaxy Star Formation Histories through SED Fitting: The Dense Basis Approach
• The equilibrium view on dust and metals in galaxies: Galactic outflows drive low dust-to-metal ratios in dwarf galaxies
• The redshift evolution of escape fraction of hydrogen ionizing photons from galaxies
• Metallicity-constrained merger rates of binary black holes and the stochastic gravitational wave background
• The globular cluster systems of 54 Coma ultra-diffuse galaxies: statistical constraints from HST data
• A massive, dead disk galaxy in the early Universe
• Are the ultra-high-redshift galaxies at z > 10 surprising in the context of standard galaxy formation models?
• The DECam Local Volume Exploration Survey: Overview and First Data Release
• Reconciling the Diversity and Uniformity of Galactic Rotation Curves with Self-Interacting Dark Matter
• The origin of scatter in the star formation rate - stellar mass relation
• Baryon Cycles in the Biggest Galaxies
• The Mass-Independence of Specific Star Formation Rates in Galactic Disks
• The origin of the Milky Way globular clusters
• The Impact of Star Formation and Gamma-Ray Burst Rates at High Redshift on Cosmic Chemical Evolution and Reionization
• The KMOS Deep Survey (KDS) I: dynamical measurements of typical star-forming galaxies at z $\simeq$ 3.5
• The splashback radius of halos from particle dynamics. II. Dependence on mass, accretion rate, redshift, and cosmology
• The quenching and survival of ultra-diffuse galaxies in the Coma cluster
• Systematics in virial mass estimators for pressure-supported systems
• Rotation Curves in z~1-2 Star-Forming Disks: Evidence for Cored Dark Matter Distributions
• AREPO-RT: Radiation hydrodynamics on a moving mesh
• Measuring the star formation rate with gravitational waves from binary black holes
• Modeling the Formation of Globular Cluster Systems in the Virgo Cluster
• Limit on the LMC mass from a census of its satellites
• 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
• Stellar Absorption Line Analysis of Local Star-Forming Galaxies: The Relation Between Stellar Mass, Metallicity, Dust Attenuation and Star Formation Rate
• Formation of Globular Cluster Systems: From Dwarf Galaxies to Giants
• The stellar-to-halo mass relations of local galaxies segregates by color
• Space Warps II. New Gravitational Lens Candidates from the CFHTLS Discovered through Citizen Science
• Globular clusters indicate ultra diffuse galaxies are dwarfs
• The Impact of Modeling Assumptions in Galactic Chemical Evolution Models
• Satellite Dwarf Galaxies in a Hierarchical Universe: The Prevalence of Dwarf-Dwarf Major Mergers
• Lensing substructure quantification in RXJ1131-1231: A 2 keV lower bound on dark matter thermal relic mass
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Motivation, Design and Target Catalogue
• 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
• The COSMOS2015 galaxy stellar mass function: 13 billion years of stellar mass assembly in 10 snapshots
• z~2-9 Galaxies Magnified by the Hubble Frontier Field Clusters II: Luminosity Functions and Constraints on a Faint-End Turnover
• 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
• X-rays across the galaxy population I: tracing the main sequence of star formation
• The Diversity and Variability of Star Formation Histories in Models of Galaxy Evolution
• The stellar accretion origin of stellar population gradients in massive galaxies at large radii
• Spatially-resolved stellar kinematics of the ultra diffuse galaxy Dragonfly 44. I. Observations, kinematics, and cold dark matter halo fits
• Inspiraling Halo Accretion Mapped in Lyman-$\alpha$ Emission around a $z\sim 3$ Quasar
• FIREbox: Simulating galaxies at high dynamic range in a cosmological volume
• A Comparison between Semi-Analytic Model Predictions for the CANDELS Survey
• 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
• 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
• Modelling the number density of Halpha emitters for future spectroscopic near-IR space missions
• 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
• The REQUIEM Survey I: A Search for Extended Ly-Alpha Nebular Emission Around 31 z>5.7 Quasars
• Linking black-hole growth with host galaxies: The accretion-stellar mass relation and its cosmic evolution
• First predictions of the angular power spectrum of the astrophysical gravitational wave background
• Black Hole and Galaxy Coevolution from Continuity Equation and Abundance Matching
• Galactic Winds in Low-Mass Galaxies
• 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
• Sample variance in the local measurements of the Hubble constant
• Tidal stripping as a possible origin of the ultra diffuse galaxy lacking dark matter
• The Impact of Galactic Feedback on the Circumgalactic Medium
• New reaction rates for improved primordial D/H calculation and the cosmic evolution of deuterium
• The sizes of $z\sim 6-8$ lensed galaxies from the Hubble Frontier Fields Abell 2744 data
• Stochastic modeling of star-formation histories I: the scatter of the star-forming main sequence
• Kiloparsec Scale Properties of Star-Formation Driven Outflows at z~2.3 in the SINS/zC-SINF AO Survey
• 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
• Dark Matter Halos in Galaxies and Globular Cluster Populations. II: Metallicity and Morphology
• 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
• 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
• 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 Lonely Giant: The Sparse Satellite Population of M94 Challenges Galaxy Formation
• Star Formation and AGN Activity in Galaxy Clusters from $z=1-2$: a Multi-wavelength Analysis Featuring $Herschel$/PACS
• Quenching of Star Formation in SDSS Groups: Centrals, Satellites, and Galactic Conformity
• Spatially Resolved Star Formation and Inside-out Quenching in the TNG50 Simulation and 3D-HST Observations
• Demographics of Star-forming Galaxies since $z\sim 2.5$. I. The $UVJ$ Diagram in CANDELS
• ZOMG-I. How the cosmic web inhibits halo growth and generates assembly bias
• NIHAO IX: the role of gas inflows and outflows in driving the contraction and expansion of cold dark matter haloes
• The MASSIVE Survey - VII. The Relationship of Angular Momentum, Stellar Mass and Environment of Early-Type Galaxies
• Flat rotation curves and low velocity dispersions in KMOS star-forming galaxies at z~1
• COPSS II: The Molecular Gas Content of Ten Million Cubic Megaparsecs at $z\sim 3$
• Identifying true satellites of the Magellanic Clouds
• On the origin of the fundamental metallicity relation and the scatter in galaxy scaling relations
• Revealing the galaxy-halo connection in IllustrisTNG
• A survey of high-$z$ galaxies: SERRA simulations
• Detection of the LMC-induced sloshing of the Galactic halo
• Energy equipartition between stellar and dark matter particles in cosmological simulations results in spurious growth of galaxy sizes
• 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
• 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
• A lower fragmentation mass scale in high redshift galaxies and its implications on giant clumps: a systematic numerical study
• Faint dwarfs as a test of DM models: WDM vs. CDM
• Colours, Star formation Rates, and Environments of Star forming and Quiescent Galaxies at the Cosmic Noon
• MusE GAs FLOw and Wind (MEGAFLOW) I: First MUSE results on background quasars
• 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
• Supermassive black holes as the regulators of star formation in central galaxies
• 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
• The Progenitors of Local Ultra-massive Galaxies Across Cosmic Time: from Dusty Star-bursting to Quiescent Stellar Populations
• 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
• 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?
• 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
• The Most Massive Galaxies and Black Holes Allowed by $\Lambda$CDM
• SHAM Beyond Clustering: New Tests of Galaxy-Halo Abundance Matching with Galaxy Groups
• The Scaling of Stellar Mass and Central Stellar Velocity Dispersion for Quiescent galaxies at z < 0.7
• 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
• SCORCH I: The Galaxy-Halo Connection in the First Billion Years
• Far-infrared surveys of galaxy evolution
• 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
• Quantifying scatter in galaxy formation at the lowest masses
• The effect of metal enrichment and galactic winds on galaxy formation in cosmological zoom simulations
• The origin of the mass discrepancy-acceleration relation in $\Lambda$CDM
• Connecting stellar mass and star-formation rate to dark matter halo mass out to z ~ 2
• The formation of massive, quiescent galaxies at cosmic noon
• High Angular Momentum Halo Gas: a Feedback and Code-Independent Prediction of LCDM
• 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 Nature of Massive Transition Galaxies in CANDELS, GAMA, and Cosmological Simulations
• 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
• Galaxy and Mass Assembly (GAMA): The halo mass of galaxy groups from maximum-likelihood weak lensing
• The evolving far-IR galaxy luminosity function and dust-obscured star-formation rate density out to z~5
• A Systematic Look at the Effects of Radiative Feedback on Disc Galaxy Formation
• Line Overlap and Self-Shielding of Molecular Hydrogen in Galaxies
• Surveying Galaxy Proto-clusters in Emission: A Large-scale Structure at z=2.44 and the Outlook for HETDEX
• The dependence of cosmic ray driven galactic winds on halo mass
• When and where did GW150914 form?
• Coming of Age in the Dark Sector: How Dark Matter Haloes grow their Gravitational Potential Wells
• Hyper Suprime-Cam Subaru Strategic Program: A Mass-Dependent Slope of the Galaxy Size-Mass Relation at $z<1$
• Which galaxies dominate the neutral gas content of the Universe?
• 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
• On the OVI Abundance in the Circumgalactic Medium of Low-Redshift Galaxies
• Characterizing Intra-cluster light in the Hubble Frontier Fields
• Missing dark matter in dwarf galaxies?
• Chandra centres for COSMOS X-ray galaxy groups: Differences in stellar properties between central dominant and offset brightest group galaxies
• Baryonic effects for weak lensing. Part I. Power spectrum and covariance matrix
• On the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7<z<2.8
• MAHALO Deep Cluster Survey I. Accelerated and enhanced galaxy formation in the densest regions of a protocluster at z=2.5
• Reconciling the observed star-forming sequence with the observed stellar mass function
• The predicted luminous satellite populations around SMC and LMC-mass galaxies - A missing satellite problem around the LMC?
• Introducing the FirstLight project: UV luminosity function and scaling relations of primeval galaxies
• 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 $0<z<3$
• Log-normal star formation histories in simulated and observed galaxies
• Searching for Traces of Planck-Scale Physics with High Energy Neutrinos
• The ACS LCID project. X. The Star Formation History of IC 1613: Revisiting the Over-Cooling Problem
• Dust, CO and [CI]: Cross-calibration of molecular gas mass tracers in metal-rich galaxies across cosmic time
• Observational evidence of a slow downfall of star formation efficiency in massive galaxies during the last 10 Gyr
• Dark Matter Cores and Cusps in Spiral Galaxies and their Explanations
• Impact of inter-correlated initial binary parameters on double black hole and neutron star mergers
• Consequences of bursty star formation on galaxy observables at high redshifts
• Evolution of cosmic star formation in the SCUBA-2 Cosmology Legacy Survey
• Escape of ionizing radiation from high redshift dwarf galaxies: role of AGN feedback
• Simulated Milky Way analogues: implications for dark matter indirect searches
• The MOSDEF survey: a census of AGN-driven ionized outflows at $z=1.4-3.8$
• Abundance matching with the mean star formation rate: there is no missing satellites problem in the Milky Way above ${\mathbf{M}}_{200}\sim 10^9{\mathbf{M}}_{\odot }$
• Star Cluster Formation in Cosmological Simulations. II. Effects of Star Formation Efficiency and Stellar Feedback
• A Minimalist Feedback-Regulated Model for Galaxy Formation During the Epoch of Reionization
• Baryon Cycling in the Low-Redshift Circumgalactic Medium: A Comparison of Simulations to the COS-Halos Survey
• The properties of the first galaxies in the BLUETIDES simulation
• Fast Molecular Outflow from a Dusty Star-Forming Galaxy in the Early Universe
• ALMA 200-parsec Resolution Imaging of Smooth Cold Dusty Disks in Typical $z\sim 3$ Star-Forming Galaxies
• Expanded haloes, abundance matching and too-big-to-fail in the Local Group
• Ultraviolet to infrared emission of z>1 galaxies: Can we derive reliable star formation rates and stellar masses?
• Galactic rotation curves, the baryon-to-dark-halo-mass relation and space-time scale invariance
• \textsc{The Three Hundred} project: The \textsc{Gizmo-Simba} run
• JADES: The incidence rate and properties of galactic outflows in low-mass galaxies across 3 < z < 9
• The Impact of Scatter in the Galaxy UV Luminosity to Halo Mass Relation on Ly$\alpha$ Visibility During the Epoch of Reionization
• 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
• Halo mass estimates from the Globular Cluster populations of 175 Low Surface Brightness Galaxies in the Fornax Cluster
• A hypervelocity star with a Magellanic origin
• Delayed Star Formation in Isolated Dwarf Galaxies: HST Star Formation History of the Aquarius Dwarf Irregular
• 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
• Spatially-unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem
• Two-phase galaxy evolution: the cosmic star-formation histories of spheroids and discs
• Two New Calcium-Rich Gap Transients in Group and Cluster Environments
• The relative and absolute ages of old globular clusters in the LCDM framework
• Rotation and Mass in the Milky Way and Spiral Galaxies
• Projection effects on the observed angular spectrum of the astrophysical stochastic gravitational wave background
• Column Density Profiles of Multi-Phase Gaseous Halos
• The Three Causes of Low-Mass Assembly Bias
• 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
• The SINS/zC-SINF Survey of z~2 Galaxy Kinematics: Rest-frame Morphology, Structure, and Colors from Near-infrared Hubble Space Telescope Imaging
• New insights on the formation of nuclear star clusters
• MultiDark-Galaxies: data release and first results
• Enhanced tidal stripping of satellites in the galactic halo from dark matter self-interactions
• An unexpected high concentration for the dark substructure in the gravitational lens SDSSJ0946+1006
• Dark Matter in Dwarf Spheroidal Galaxies and Indirect Detection: A Review
• Precipitation-Regulated Star Formation in Galaxies
• Diverse Structural Evolution at z > 1 in Cosmologically Simulated Galaxies
• Orbital Decay of Supermassive Black Hole Binaries in Clumpy Multiphase Merger Remnants
• The properties of "dark" ΛCDM halos in the Local Group
• The masses of Local Group dwarf spheroidal galaxies: The death of the universal mass profile
• Galaxy And Mass Assembly (GAMA): Environmental Quenching of Centrals and Satellites in Groups
• The evolving relation between star-formation rate and stellar mass in the VIDEO Survey since $z=3$
• Evolution of Intrinsic Scatter in the SFR-Stellar Mass Correlation at 0.5<z<3
• The cosmic evolution of the spatially-resolved star formation rate and stellar mass of the CALIFA survey
• 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 tidal evolution of dark matter substructure -- II. The impact of artificial disruption on subhalo mass functions and radial profiles
• A model for core formation in dark matter haloes and ultra diffuse galaxies by outflow episodes
• A Census of Stellar Mass in 10 Massive Haloes at z~1 from the GCLASS Survey
• Trinity I: Self-Consistently Modeling the Dark Matter Halo-Galaxy-Supermassive Black Hole Connection from $z=0-10$
• Massive Compact Galaxies with High-Velocity Outflows: Morphological Analysis and Constraints on AGN Activity
• Major Mergers Going Notts: Challenges for Modern Halo Finders
• How baryons affect halos and large-scale structure: a unified picture from the Simba simulation
• Cold Filamentary Accretion and the Formation of Metal Poor Globular Clusters and Halo Stars
• 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
• The maximum accretion rate of hot gas in dark matter halos
• NIHAO V: Too big doesn't fail -- reconciling the conflict between LCDM predictions and the circular velocities of nearby field galaxies
• Quenching timescales of galaxies in the EAGLE simulations
• 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
• A unified explanation for the supernova rate-galaxy mass dependency based on supernovae discovered in Sloan galaxy spectra
• EDGE: The origin of scatter in ultra-faint dwarf stellar masses and surface brightnesses
• Two can play at that game: constraining the role of supernova and AGN feedback in dwarf galaxies with cosmological zoom-in simulations
• 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
• Did JWST observe imprints of axion miniclusters or primordial black holes?
• Reproducing sub-millimetre galaxy number counts with cosmological hydrodynamic simulations
• The Grism Lens-Amplified Survey from Space (GLASS). II. Gas-phase metallicity and radial gradients in an interacting system at z~2
• Predicting the locations of possible long-lived low-mass first stars: Importance of satellite dwarf galaxies
• The spatially-resolved star formation histories of CALIFA galaxies: Implications for galaxy formation
• Early Low-Mass Galaxies and Star-Cluster Candidates at z~6-9 Identified by the Gravitational Lensing Technique and Deep Optical/Near-Infrared Imaging
• An Empirical Model for the Star Formation History in Dark Matter Halos
• The Need for Speed: Escape velocity and dynamical mass measurements of the Andromeda galaxy
• Kinematics and simulations of the stellar stream in the halo of the Umbrella Galaxy
• On the Physical Origin of Galactic Conformity
• Evident black hole-bulge coevolution in the distant universe
• NIHAO XIII: Clumpy discs or clumpy light in high redshift galaxies?
• Properties of the stochastic astrophysical gravitational wave background: astrophysical sources dependencies
• Minor vs Major Mergers: The Stellar Mass Growth of Massive Galaxies from z=3 using Number Density Selection Techniques
• Counting Black Holes: The Cosmic Stellar Remnant Population and Implications for LIGO
• The Persistence of Population III Star Formation
• Galaxies lacking dark matter produced by close encounters in a cosmological simulation
• NIHAO XX: The impact of the star formation threshold on the cusp-core transformation of cold dark matter haloes
• The tidal evolution of dark matter substructure -- I. Subhalo density profiles
• Cosmological Galaxy Evolution with Superbubble Feedback I: Realistic Galaxies with Moderate Feedback
• A small-scale dynamo in feedback-dominated galaxies - II. The saturation phase and the final magnetic configuration
• NIHAO VI. The hidden discs of simulated galaxies
• Baryonic and dark matter distribution in cosmological simulations of spiral galaxies
• Low-mass galaxy assembly in simulations: regulation of early star formation by radiation from massive stars
• Cosmology with intensity mapping techniques using atomic and molecular lines
• NIHAO VIII: Circum-galactic medium and outflows - The puzzles of HI and OVI gas distributions
• An Intensity Mapping Detection of Aggregate CO Line Emission at 3 mm
• 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
• Modelling the Tucana III stream - a close passage with the LMC
• Origins of scaling relations of globular cluster systems
• Hidden depths in the local Universe: The Stellar Stream Legacy Survey
• 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
• Probing the Cool Interstellar and Circumgalactic Gas of Three Massive Lensing Galaxies at z=0.4-0.7
• 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
• Morphologies of ~190,000 Galaxies at z=0-10 Revealed with HST Legacy Data. III. Continuum Profile and Size Evolution of Lya Emitters
• The Radial Acceleration Relation in CLASH Galaxy Clusters
• The Milky Way's Halo and Subhalos in Self-Interacting Dark Matter
• The Galaxy Clustering Crisis in Abundance Matching
• Knocking on giants' doors: I. The evolution of the dust-to-stellar mass ratio in distant dusty galaxies
• Wet Compaction to a Blue Nugget: a Critical Phase in Galaxy Evolution
• 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
• Ultra diffuse galaxies in the MATLAS low-to-moderate density fields
• Fast Outflows Identified in Early Star-Forming Galaxies at $z=5-6$
• 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
• 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
• 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
• The Velocity Dispersion Function of Very Massive Galaxy Clusters: Abell 2029 and Coma
• Dissecting the high-z interstellar medium through intensity mapping cross-correlations
• Connecting Transitions in Galaxy Properties to Refueling
• Rhapsody. I. Structural Properties and Formation History From a Statistical Sample of Re-simulated Cluster-size Halos
• Search for CII Emission on Cosmological Scales at Redshift Z~2.6
• Phenomenological consequences of superfluid dark matter with baryon-phonon coupling
• Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey Description
• LoCuSS: Scaling relations between galaxy cluster mass, gas, and stellar content
• On the mass of the Local Group
• Elliptical Galaxies and Bulges of Disk Galaxies: Summary of Progress and Outstanding Issues
• Numerical resolution limits on subhalo abundance matching
• Semi-analytic forecasts for JWST -- VI. Simulated lightcones and galaxy clustering predictions
• Galactic disk winds driven by cosmic ray pressure
• Cosmic Neutron Star Merger Rate and Gravitational Waves constrained by the R Process Nucleosynthesis
• GalaxyNet: Connecting galaxies and dark matter haloes with deep neural networks and reinforcement learning in large volumes
• Evolution of the Mass-Metallicity Relation from Redshift $z\approx 8$ to the Local Universe
• Star Clusters in Evolving Galaxies
• AGN evolution from a galaxy evolution viewpoint
• The eROSITA Final Equatorial Depth Survey (eFEDS): X-ray emission around star-forming and quiescent galaxies at $0.05<z<0.3$
• Star Formation and Clumps in Cosmological Galaxy Simulations with Radiation Pressure Feedback
• The MaGICC volume: reproducing statistical properties of high redshift galaxies
• Emergence of an Ultra-Red Ultra-Massive Galaxy Cluster Core at $z=4$
• Constraining the CO intensity mapping power spectrum at intermediate redshifts
• The bias of the submillimetre galaxy population: SMGs are poor tracers of the most massive structures in the z ~ 2 Universe
• Constraining the evolution of CII intensity through the end stages of reionization
• COSMOS-Web: stellar mass assembly in relation to dark matter halos across $0.2<z<12$ of cosmic history
• The Dekel-Zhao profile: A mass-dependent dark-matter density profile with flexible inner slope and analytic potential, velocity dispersion, and lensing properties
• Accurate and Efficient Halo-based Galaxy Clustering Modelling with Simulations
• Predicting Galaxy Star Formation Rates via the Co-evolution of Galaxies and Halos
• The galaxy-halo connection of emission-line galaxies in IllustrisTNG
• CLASS_GWB: robust modeling of the astrophysical gravitational wave background anisotropies
• ALMA measures rapidly depleted molecular gas reservoirs in massive quiescent galaxies at z~1.5
• 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
• Star formation history, dust attenuation and extragalactic background light
• Impact of Lyman alpha pressure on metal-poor dwarf galaxies
• Search for Gamma-ray Emission from Dark Matter Annihilation in the Large Magellanic Cloud with the Fermi Large Area Telescope
• Under the Firelight: Stellar Tracers of the Local Dark Matter Velocity Distribution in the Milky Way
• The evolution of the star forming sequence in hierarchical galaxy formation models
• EMERGE: Empirical predictions of galaxy merger rates since $z\sim 6$
• 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
• NIHAO XII: galactic uniformity in a ΛCDM universe
• The stellar halos of ETGs in the IllustrisTNG simulations: the photometric and kinematic diversity of galaxies at large radii
• Light breeze in the local Universe
• The Correlation Between Halo Mass and Stellar Mass for the Most Massive Galaxies in the Universe
• Dynamical evolution of cosmic supermassive binary black holes and their gravitational wave radiation
• On The History and Future of Cosmic Planet Formation
• Two-Face(s): ionized and neutral gas winds in the local Universe
• Dynamical evidence for a morphology-dependent relation between the stellar and halo masses of galaxies
• The cumulative star-formation histories of dwarf galaxies with TNG50. I: Environment-driven diversity and connection to quenching
• Direct Insights into Observational Absorption Line Analysis Methods of the Circumgalactic Medium Using Cosmological Simulations
• Simulating the 21-cm signal from reionisation including non-linear ionisations and inhomogeneous recombinations
• Mg II Absorption at 2<z<7 with Magellan/FIRE, III. Full Statistics of Absorption Towards 100 High-Redshift QSOs
• NIHAO XIX: How supernova feedback shapes the galaxy baryon cycle
• Interpreting Short Gamma Ray Burst Progenitor Kicks and Time Delays Using the Host Galaxy-Dark Matter Halo Connection
• Empirical constraints on the formation of early-type galaxies
• SUPER I. Toward an unbiased study of ionized outflows in z~2 active galactic nuclei: survey overview and sample characterization
• Constraining the HI-Halo Mass Relation From Galaxy Clustering
• Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
• Constraining the Star Formation Histories in Dark Matter Halos: I. Central Galaxies
• A Foreground Masking Strategy for [CII] Intensity Mapping Experiments Using Galaxies Selected by Stellar Mass and Redshift
• Luminosity Functions and Host-to-Host Scatter of Dwarf Satellite Systems in the Local Volume
• Formation of elongated galaxies with low masses at high redshift
• Symphony: Cosmological Zoom-in Simulation Suites over Four Decades of Host Halo Mass
• 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
• 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
• On the origin of excess cool gas in quasar host halos
• 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
• Inferences on the Relations Between Central Black Hole Mass and Total Galaxy Stellar Mass in the high-redshift Universe
• A fresh look into the interacting dark matter scenario
• The edge of galaxy formation I: formation and evolution of MW-satellites analogues before accretion
• Effects of simulated cosmological magnetic fields on the galaxy population
• Spin-driven jet feedback in idealised simulations of galaxy groups and clusters
• Structural and dynamical modeling of WINGS clusters. II. The orbital anisotropies of elliptical, spiral and lenticular galaxies
• From massive spirals to dwarf irregulars: a new set of tight scaling relations for cold gas and stars driven by disc gravitational instability
• High-redshift galaxies and black holes in the eyes of JWST: a population synthesis model from infrared to X-rays
• Simultaneous modelling of matter power spectrum and bispectrum in the presence of baryons
• The Scale-Dependence of Halo Assembly Bias
• Host galaxies of high-redshift quasars: supermassive black hole growth and feedback
• An observer's guide to the (Local Group) dwarf galaxies: predictions for their own dwarf satellite populations
• The JWST Advanced Deep Extragalactic Survey: Discovery of an Extreme Galaxy Overdensity at $z=5.4$ with JWST/NIRCam in GOODS-S
• Structure Formation Models Weaken Limits on WIMP Dark Matter from Dwarf Spheroidal Galaxies
• Hunting Faint Dwarf Galaxies in the Field Using Integrated Light Surveys
• Dwarf Galaxy Formation with H2-Regulated Star Formation: II. Gas-Rich Dark Galaxies at Redshift 2.5
• Realistic simulations of galaxy formation in f(R) modified gravity
• Anomalously low metallicity regions in MaNGA star-forming galaxies: Accretion Caught in Action?
• Detecting Direct Collapse Black Holes: making the case for CR7
• Is diffuse intracluster light a good tracer of the galaxy cluster matter distribution?
• Andromeda XXI -- a dwarf galaxy in a low density dark matter halo
• Forming early-type galaxies without AGN feedback: a combination of merger-driven outflows and inefficient star formation
• 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
• Cosmological Galaxy Evolution with Superbubble Feedback II: The Limits of Supernovae
• Mg II absorbers: metallicity evolution and cloud morphology
• 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
• Swirls of FIRE: Spatially Resolved Gas Velocity Dispersions and Star Formation Rates in FIRE-2 Disk Environments
• The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to $z\sim 5$
• 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 Structure of the Circumgalactic Medium of Galaxies: Cool Accretion Inflow Around NGC 1097
• The Quest for Dusty Star-forming Galaxies at High Redshift z>4
• High redshift JWST predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves
• Galaxy spin as a formation probe: the stellar-to-halo specific angular momentum relation
• Rapid early coeval star formation and assembly of the most massive galaxies in the universe
• The SAMI Galaxy Survey: The internal orbital structure and mass distribution of passive galaxies from triaxial orbit-superposition Schwarzschild models
• PRIMUS+DEEP2: The Dependence of Galaxy Clustering on Stellar Mass and Specific Star Formation Rate at 0.2 < z < 1.2
• COSMOS2020: Discovery of a protocluster of massive quiescent galaxies at $z=2.77$
• The GEEC2 spectroscopic survey of Galaxy Groups at $0.8<z<1$
• TheHaloMod: An online calculator for the halo model
• Weak Lensing Reveals a Tight Connection Between Dark Matter Halo Mass and the Distribution of Stellar Mass in Massive Galaxies
• The first galaxies: simulating their feedback-regulated assembly
• 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
• Star formation at the edge of the Local Group: a rising star formation history in the isolated galaxy WLM
• On the origin of surprisingly cold gas discs in galaxies at high redshift
• Origin and evolution of ultra-diffuse galaxies in different environments
• Approximate Bayesian Computation in Large Scale Structure: constraining the galaxy-halo connection
• Dark and luminous satellites of LMC-mass galaxies in the FIRE simulations
• Incidence, scaling relations and physical conditions of ionised gas outflows in MaNGA
• Star Formation and Stellar Mass Assembly in Dark Matter Halos: From Giants to Dwarfs
• Line-of-sight effects in strong lensing: Putting theory into practice
• Self-Interacting Dark Matter and the Origin of Ultra-Diffuse Galaxies NGC1052-DF2 and -DF4
• Insights from probability distribution functions of intensity maps
• Validating Semi-Analytic Models of High-Redshift Galaxy Formation using Radiation Hydrodynamical Simulations
• The spatial clustering of ROSAT All-Sky Survey Active Galactic Nuclei IV. More massive black holes reside in more massive dark matter halos
• The dependence of the galaxy stellar-to-halo mass relation on galaxy morphology
• FOREVER22: galaxy formation in protocluster regions
• MOND Prediction for the Velocity Dispersion of the `Feeble Giant' Crater II
• Learning the Relationship between Galaxies Spectra and their Star Formation Histories using Convolutional Neural Networks and Cosmological Simulations
• Joint power spectrum and voxel intensity distribution forecast on the CO luminosity function with COMAP
• Galaxy disc scaling relations: A tight linear galaxy -- halo connection challenges abundance matching
• Osaka Feedback Model: Isolated Disk Galaxy Simulations
• A Systematic Study of the Stochastic Gravitational-Wave Background due to Stellar Core Collapse
• Evidence for Cold-stream to Hot-accretion Transition as Traced by Lyα Emission from Groups and Clusters at 2 < z < 3.3
• The correlation between the sizes of globular cluster systems and their host dark matter haloes
• Observational evidence of galaxy assembly bias
• Spatially resolved mass-to-light from the CALIFA survey. Mass-to-light ratio vs. color relations
• 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
• Baryonic Imprints on DM Halos: Population Statistics from Dwarf Galaxies to Galaxy Clusters
• UVUDF: UV Luminosity Functions at the cosmic high-noon
• The prevalence and properties of cold gas inflows and outflows around galaxies in the local Universe
• The simplest model of galaxy formation I: A formation history model of galaxy stellar mass growth
• Near-Field Limits on the Role of Faint Galaxies in Cosmic Reionization
• Stochastic gravitational wave background anisotropies in the mHz band: astrophysical dependencies
• Maximum redshift of gravitational wave merger events
• An analytical model for galaxy metallicity: What do metallicity relations tell us about star formation and outflow?
• On the intermediate-redshift central stellar mass-halo mass relation, and implications for the evolution of the most massive galaxies since z~1
• The Dwarfs Beyond: The Stellar-to-Halo Mass Relation for a New Sample of Intermediate Redshift Low Mass Galaxies
• Scaling relations and baryonic cycling in local star-forming galaxies: II. Gas content and star-formation efficiency
• The Strikingly Similar Relation between Satellite and Central Galaxies and Their Dark Matter Halos Since z=2
• Exploring the nature of the Lyman-$\alpha$ emitter CR7
• Early-type galaxy density profiles from IllustrisTNG: I. Galaxy correlations and the impact of baryons
• First results from SMAUG: The need for preventative stellar feedback and improved baryon cycling in semi-analytic models of galaxy formation
• Clustering, host halos and environment of z$\sim$2 galaxies as a function of their physical properties
• 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
• Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
• Evolution of Star-forming Galaxies from z = 0.7 to 1.2 with eBOSS Emission-line Galaxies
• An empirical representation of a physical model for the ISM [CII], CO, and [CI] emission at redshift $1\le z\le 9$
• A Fast Radio Burst Occurs Every Second throughout the Observable Universe
• Galaxy evolution in protoclusters
• Thick Disks in the Hubble Space Telescope Frontier Fields
• Radial Trends in IMF-Sensitive Absorption Features in Two Early-Type Galaxies: Evidence for Abundance-Driven Gradients
• Magnetogenesis around the first galaxies: the impact of different field seeding processes on galaxy formation
• Evolution of Galactic Outflows at $z\sim 0$-$2$ Revealed with SDSS, DEEP2, and Keck spectra
• Millimeter mapping at z~1: dust-obscured bulge building and disk growth
• The bias of DLAs at z ~ 2.3: contraining stellar feedback in shallow potential wells
• Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
• A limit on the warm dark matter particle mass from the redshifted 21 cm absorption line
• A simple model linking galaxy and dark matter evolution
• The Star-Formation Main Sequence: The Dependence of Specific Star Formation Rate and Its Dispersion on Galaxy Stellar Mass
• The role of faint population III supernovae in forming CEMP stars in ultra-faint dwarf galaxies
• The origin of the mass scales for maximal star formation efficiency and quenching: the critical role of Supernovae
• 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
• 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
• A single-merger scenario for the formation of the giant stream and the warp of M31
• A lensed protocluster candidate at $z=7.66$ identified in JWST observations of the galaxy cluster SMACS0723-7327
• Identification of High-Redshift Galaxy Overdensities in GOODS-N and GOODS-S
• The combined effect of AGN and supernovae feedback in launching massive molecular outflows in high-redshift galaxies
• 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
• Realistic mock observations of the sizes and stellar mass surface densities of massive galaxies in FIRE-2 zoom-in simulations
• GRUMPY: a simple framework for realistic forward-modelling of dwarf galaxies
• A Study of Massive and Evolved Galaxies at High Redshift
• The Immitigable Nature of Assembly Bias: The Impact of Halo Definition on Assembly Bias
• Timing the evolution of quiescent and star-forming local galaxies
• Star Formation Quenching Timescale of Central Galaxies in a Hierarchical Universe
• The Origin of r-process Enhanced Metal-Poor Halo Stars In Now-Destroyed Ultra-Faint Dwarf Galaxies
• New Analytic Solutions for Galaxy Evolution: Gas, Stars, Metals and Dust in local Early-Type Galaxies and in their high-z Starforming Progenitors
• The Stellar Mass, Star Formation Rate and Dark Matter Halo Properties of LAEs at $z\sim 2$
• The new semianalytic code GalICS 2.0 - Reproducing the galaxy stellar mass function and the Tully-Fisher relation simultaneously
• The H-alpha luminosity-dependent clustering of star-forming galaxies from z~0.8 to z~2.2 with HiZELS
• Early growth of typical high redshift black holes seeded by direct collapse
• From Diversity to Dichotomy, and Quenching: Milky-Way-Like and Massive-Galaxy Progenitors at 0.5<z<3.0
• Caught in the act: gas and stellar velocity dispersions in a fast quenching compact star-forming galaxy at z~1.7
• An Excess of Globular Clusters in UDGs Formed Through Tidal Heating
• 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
• Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations
• The LBT Satellites of Nearby Galaxies Survey (LBT-SONG): The Satellite Population of NGC 628
• The challenge of simultaneously matching the observed diversity of chemical abundance patterns in cosmological hydrodynamical simulations
• Formation of disk galaxies in preheated media: a preventative feedback model
• Rotation Curve Decomposition for Size-Mass Relations of Bulge, Disk, and Dark Halo in Spiral Galaxies
• Equilibrium model prediction for the scatter in the star-forming main sequence
• Young and turbulent: the early life of massive galaxy progenitors
• Impact of polarised extragalactic sources on the measurement of CMB B-mode anisotropies
• The Little Galaxies that Could (Reionize the Universe): Predicting Faint End Slopes & Escape Fractions at z > 4
• Simple halo model formalism for the cosmic infrared background and its correlation with the thermal Sunyaev Zel'dovich effect
• Halo Histories vs. Galaxy Properties at z=0, I: The Quenching of Star Formation
• Properties of Submillimeter Galaxies in a Semi-analytic Model using the "Count Matching" Approach: Application to the ECDF-S
• The effects of galaxy shape and rotation on the X-ray haloes of early-type galaxies - II. Numerical simulations
• Magellanic satellites in $\Lambda$CDM cosmological hydrodynamical simulations of the Local Group
• X-ray Emission From Hot Gas in Galaxy Groups and Clusters in Simba
• Formation of the largest galactic cores through binary scouring and gravitational wave recoil
• The Mass and Absorption Columns of Galactic Gaseous Halos
• NIHAO -- XXV. Convergence in the cusp-core transformation of cold dark matter haloes at high star formation thresholds
• New perspectives on the BOSS small-scale lensing discrepancy for the Planck $\Lambda$CDM Cosmology
• Dust formation, evolution, and obscuration effects in the very high-redshift universe
• ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
• On stellar mass loss from galaxies in groups and clusters
• Introducing galactic structure finder: the multiple stellar kinematic structures of a simulated Milky Way mass galaxy
• Stellar Velocity Dispersion: Linking Quiescent Galaxies to their Dark Matter Halos
• A Model of the Stochastic Gravitational-Wave Background due to Core Collapse to Black Holes
• Chasing Lyman alpha-emitting galaxies at z = 8.8
• Are Cosmological Gas Accretion Streams Multiphase and Turbulent?
• Cross-correlating Carbon Monoxide Line-intensity Maps with Spectroscopic and Photometric Galaxy Surveys
• AGN and their host galaxies in the local Universe: two mass independent Eddington ratio distribution functions characterize black hole growth
• The evolution of turbulent galactic discs: gravitational instability, feedback and accretion
• Revisiting the bulge-halo conspiracy I: Dependence on galaxy properties and halo mass
• A universal relation between the properties of supermassive black holes, galaxies, and dark matter halos
• The Morphology-Density-Relation: Impact on the Satellite Fraction
• Hierarchical Galaxy Growth and Scatter in the Stellar Mass - Halo Mass Relation
• Baryon effects on void statistics in the EAGLE simulation
• Creating a galaxy lacking dark matter in a dark matter dominated universe
• Forecasts for the WFIRST High Latitude Survey using the BlueTides Simulation
• A Detection of the Environmental Dependence of the Sizes and Stellar Haloes of Massive Central Galaxies
• The Relative Specific Type Ia Supernovae Rate From Three Years of ASAS-SN
• The Mass Profile of the Milky Way to the Virial Radius from the Illustris Simulation
• Phase-Space Spectral Line De-confusion in Intensity Mapping
• Emergence of the mass discrepancy-acceleration relation from dark matter-baryon interactions
• Where did the globular clusters of the Milky Way form? Insights from the E-MOSAICS simulations
• 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
• The Role of Cold Flows and Reservoirs in Galaxy Formation With Strong Feedback
• Constraining the last 7 billion years of galaxy evolution in semi-analytic models
• The diverse formation histories of simulated disc galaxies
• Search for Gamma-ray Emission from Dark Matter Annihilation in the Small Magellanic Cloud with the Fermi Large Area Telescope
• Towards a radially-resolved semi-analytic model for the evolution of disc galaxies tuned with machine learning
• Evolution of Star-formation Properties of High-redshift Cluster Galaxies since $z=2$
• 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
• NIHAO XVI: The properties and evolution of kinematically selected discs, bulges and stellar haloes
• Jet-driven AGN feedback on molecular gas and low star-formation efficiency in a massive local spiral galaxy with bright X-ray halo
• Low Angular Momentum in Clumpy, Turbulent Disk Galaxies
• Stellar splashback: the edge of the intracluster light
• Growth of First Galaxies: Impacts of Star Formation and Stellar Feedback
• Constraints on warm dark matter from UV luminosity functions of high-z galaxies with Bayesian model comparison
• GN-z11: The environment of an AGN at $z=$10.603
• Constraints on galaxy formation models from the galaxy stellar mass function and its evolution
• Co-orbiting planes of sub-halos are similarly unlikely around paired and isolated hosts
• NIHAO XXII: Introducing black hole formation, accretion and feedback into the NIHAO simulation suite
• The Incomplete Conditional Stellar Mass Function: Unveiling the Stellar Mass Functions of Galaxies at 0.1 < Z < 0.8 from BOSS Observations
• Clearing the hurdle: The mass of globular cluster systems as a function of host galaxy mass
• Scaling Relations for Galaxies Prior to Reionization
• The SLUGGS survey: inferring the formation epochs of metal-poor and metal-rich globular clusters
• The clustering of typical Ly$\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
• Matching the Evolution of the Stellar Mass Function Using Log-normal Star Formation Histories
• Priors on red galaxy stochasticity from hybrid effective field theory
• Tidal Distortions in NGC1052-DF2 and NGC1052-DF4: Independent Evidence for a Lack of Dark Matter
• The history of the dark and luminous side of Milky Way-like progenitors
• Unraveling the origin of magnetic fields in galaxies
• The emergence of dark matter-deficient ultra-diffuse galaxies driven by scatter in the stellar mass-halo mass relation and feedback from globular clusters
• The Three Hundred Project: The influence of environment on simulated galaxy properties
• SDSS IV MaNGA - Rotation Velocity Lags in the Extraplanar Ionized Gas from MaNGA Observations of Edge-on 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
• 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?
• Shock finding on a moving-mesh: II. Hydrodynamic shocks in the Illustris universe
• The role of gas infall in the evolution of disc galaxies
• A parametric study of possible solutions to the high-redshift overproduction of stars in modeled dwarf galaxies
• HectoMAP and Horizon Run 4: Dense Structures and Voids in the Real and Simulated Universe
• A synthetic model of the gravitational wave background from evolving binary compact objects
• 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 $z\approx 0.8$
• COMAP Early Science: V. Constraints and Forecasts at $z\sim 3$
• Great Balls of FIRE II: The evolution and destruction of star clusters across cosmic time in a Milky Way-mass galaxy
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• Bayesian inferences of galaxy formation from the K-band luminosity and HI mass functions of galaxies: constraining star formation and feedback
• ZFOURGE: Using Composite Spectral Energy Distributions to Characterize Galaxy Populations at 1<z<4
• GOODS-ALMA: Optically dark ALMA galaxies shed light on a cluster in formation at z = 3.5
• Lessons from cosmic history: The case for a linear star formation -- H2 relation
• Does the Galaxy-Halo Connection Vary with Environment?
• The ALMA Spectroscopic Survey in the HUDF: A model to explain observed 1.1 and 0.85 millimeter dust continuum number counts
• Galaxy formation in the brane world I: overview and first results
• The MUSE Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies at z=1
• Degeneracies Between Self-interacting Dark Matter and Supernova Feedback as cusp-core transformation mechanisms
• Physical Properties of UDF12 Galaxies in Cosmological simulations
• The GOGREEN survey: Transition Galaxies and The Evolution of Environmental Quenching
• Cosmic Vine: A z=3.44 large-scale structure hosting massive quiescent galaxies
• The vertical structure of gaseous galaxy discs in cold dark matter halos
• Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency
• Precision Tests of CO and [CII] Power Spectra Models against Simulated Intensity Maps
• On the Physical Requirements for a Pre-Reionization Origin of the Unresolved Near-Infrared Background
• The Impact of Environment on the Stellar Mass - Halo Mass Relation
• Cosmography using strongly lensed gravitational waves from binary black holes
• Formation channels of slowly rotating early-type galaxies
• How are galaxies assigned to halos? Searching for assembly bias in the SDSS galaxy clustering
• Constraints on the dynamical evolution of the galaxy group M81
• Star Formation and Environmental Quenching of GEEC2 Group Galaxies at z~1
• Brightest Cluster Galaxies in Cosmological Simulations with Adaptive Mesh Refinement: Successes and Failures
• Lyman-αabsorption beyond the disk of simulated spiral galaxies
• Blue Rest-Frame UV-Optical Colors in z~8 Galaxies from GREATS: Very Young Stellar Populations at ~650 Myr of Cosmic Time
• CANDELS Sheds Light on the Environmental Quenching of Low-mass Galaxies
• Herschel reveals a molecular outflow in a z = 2.3 ULIRG
• A scaling relation between merger rate of galaxies and their close pair count
• 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
• Quasar Sightline and Galaxy Evolution (QSAGE) Survey - I. The Galaxy Environment of OVI Absorbers up to z=1.4 around PKS 0232-04
• Formation of Globular Cluster Systems II: Impact of the Cutoff of the Cluster Initial Mass Function
• A Bayesian Population Model for the Observed Dust Attenuation in Galaxies
• COMAP Early Science: VII. Prospects for CO Intensity Mapping at Reionization
• 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
• Identification of galaxies that experienced a recent major drop of star formation
• The Spectroscopy and H-band Imaging of Virgo cluster galaxies (SHIVir) Survey: Scaling Relations and the Stellar-to-Total Mass Relation
• The Brightest Galaxies at Cosmic Dawn from Scatter in the Galaxy Luminosity versus Halo Mass Relation
• KMOS LENsing Survey (KLENS) : morpho-kinematic analysis of star-forming galaxies at $z\sim 2$
• Reproducing cosmic evolution of galaxy population from $z=4$ to $0$
• The kinematics of globular cluster populations in the E-MOSAICS simulations and their implications for the assembly history of the Milky Way
• A High-Resolution Investigation of the Multi-Phase ISM in a Galaxy during the First Two Billion Years
• {\sc mirkwood:} Fast and Accurate SED Modeling Using Machine Learning
• Probing the existence of a rich galaxy overdensity at z=5.2
• Rapid Filamentary Accretion as the Origin of Extended Thin Discs
• The Galaxy--Halo Connection in High-Redshift Universe: Details and Evolution of Stellar-to-Halo Mass Ratios of Lyman Break Galaxies on CFHTLS Deep Fields
• The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3
• The origin of dispersion in DLA metallicities
• Cosmic evolution of star-forming galaxies to $z\simeq 1.8$ in the faint low-frequency radio source population
• On the Orbital Decay of Globular Clusters in NGC1052-DF2: Testing a Baryon-Only Mass Model
• Tomographic Intensity Mapping versus Galaxy Surveys: Observing the Universe in H-alpha emission with new generation instruments
• Semi-Analytic Galaxies - II. Revealing the role of environmental and mass quenching in galaxy formation
• Satellites of Satellites: The Case for Carina and Fornax
• Origins of Scatter in the Relationship Between HCN 1-0 and Dense Gas Mass in the Galactic Center
• Formation of globular clusters in dwarf galaxies of the Local Group
• d1005+68: A New Faint Dwarf Galaxy in the M81 Group
• Formation and settling of a disc galaxy during the last 8 billion years in a cosmological simulation
• Stochastic angular momentum slews and flips and their effect on discs in galaxy formation models
• Semi-analytic forecasts for Roman -- the beginning of a new era of deep-wide galaxy surveys
• Star Formation Quenching in Green Valley Galaxies at $0.5\lesssim z\lesssim 1.0$ and Constraints with Galaxy Morphologies
• Simultaneously constraining cosmology and baryonic physics via deep learning from weak lensing
• Simulating the Spatial Distribution and Kinematics of Globular Clusters within Galaxy Clusters in Illustris
• The Minimum Halo Mass for Star Formation at z = 6 - 8
• The Pandora project. I: the impact of radiation and cosmic rays on baryonic and dark matter properties of dwarf galaxies
• Calibrated, cosmological hydrodynamical simulations with variable IMFs I: Method and effect on global galaxy scaling relations
• The MOSDEF Survey: Environmental dependence of the gas-phase metallicity of galaxies at $1.4\le z\le 2.6$
• 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
• The MUSE-Faint survey. II. The dark matter-density profile of the ultra-faint dwarf galaxy Eridanus 2
• IQ-Collaboratory 1.1: the Star-Forming Sequence of Simulated Central Galaxies
• Modelling the cosmic neutral hydrogen from DLAs and 21 cm observations
• Kinematics of the Circumgalactic Medium of a $z=0.77$ Galaxy from MgII Tomography
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• Cosmic CARNage I: on the calibration of galaxy formation models
• BIRTH of the COSMOS Field: Primordial and Evolved Density Reconstructions During Cosmic High Noon
• Confronting fuzzy dark matter with the rotation curves of nearby dwarf irregular galaxies
• Linear bias forecasts for emission line cosmological surveys
• Using Galaxy Pairs to Probe Star Formation During Major Halo Mergers
• Modelling of Lyman-alpha Emitting Galaxies and Ionized Bubbles at the Era of Reionization
• $\Lambda$CDM Predictions for the Satellite Population of M33
• SUPER V. ALMA continuum observations of z~2 AGN and the elusive evidence of outflows influencing star formation
• The angular momentum of disc galaxies at z=1
• The AGN-galaxy-halo connection: The distribution of AGN host halo masses to z=2.5
• The accreted stellar halo as a window on halo assembly in L* galaxies
• Gas flows in the circumgalactic medium around simulated high-redshift galaxies
• Probing Cosmic Dawn: Modelling the Assembly History, SEDs, and Dust Content of Selected $z\sim 9$ Galaxies
• The Observed Evolution of the Stellar Mass - Halo Mass Relation for Brightest Central Galaxies
• Globular Cluster Formation from Colliding Substructure
• A Census of the LyC Photons that Form the UV Background During Reionization
• Semi-analytic galaxies -- III. The impact of supernova feedback on the mass-metallicity relation
• Evolution of CIV Absorbers I. The Cosmic Incidence
• A cosmic stream of atomic carbon gas connected to a massive radio galaxy at redshift 3.8
• NIHAO III: The constant disc gas mass conspiracy
• Herschel observed Stripe 82 quasars and their host galaxies: connections between the AGN activity and the host galaxy star formation
• Density modulated star formation efficiency: implications for the observed abundance of ultra-violet luminous galaxies at z>10
• Distribution of streaming rates into high-redshift galaxies
• Balmer Break Galaxy Candidates at $z\sim 6$: a Potential View on the Star-Formation Activity at $z\gtrsim 14$
• The response of dark matter haloes to elliptical galaxy formation: a new test for quenching scenarios
• Morphological and Rotation Structures of Circumgalactic Mg II Gas in the EAGLE Simulation and the Dependence on Galaxy Properties
• The Active Assembly of the Virgo Cluster: Indications for Recent Group Infall From Early-Type Dwarf Galaxies
• ALMA Deep Field in SSA22: Blindly Detected CO Emitters and [CII] Emitter Candidates
• Local ultra faint dwarves as a product of Galactic processing during a Magellanic group infall
• 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
• Planck far-infrared detection of Hyper Suprime-Cam protoclusters at $\mathbf{z}\sim 4$: hidden AGN and star formation activity
• 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 evolution of the SFR and Sigma-SFR of galaxies in cosmic morning (4 < z < 10)
• The Impact of Baryons on Cosmological Inference from Weak Lensing Statistics
• From HI to Stars: HI Depletion in Starbursts and Star-Forming Galaxies in the ALFALFA H-alpha Survey
• ELUCID V. Lighting dark matter halos with galaxies
• The importance of galaxy formation histories in models of reionization
• 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
• The Intrinsic Scatter of Galaxy Scaling Relations
• A few StePS forward in unveiling the complexity of galaxy evolution: light-weighted stellar ages of intermediate redshift galaxies with WEAVE
• Bar-like galaxies in IllustrisTNG
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Probing the galaxy-halo connection with total satellite luminosity
• Star-formation driven outflows in local dwarf galaxies as revealed from [CII] observations by Herschel
• The Galaxy-Halo Connection for $1.5\lesssim z\lesssim 5$ as revealed by the \emph{Spitzer} Matching survey of the UltraVISTA ultra-deep Stripes
• The binary-host connection: astrophysics of gravitational wave binaries from their host galaxy properties
• Modelling a bright z = 6 galaxy at the faint end of the AGN luminosity function
• Stellar feedback from HMXBs in cosmological hydrodynamical simulations
• From EMBER to FIRE: predicting high resolution baryon fields from dark matter simulations with Deep Learning
• Intensity mapping from the sky: synergizing the joint potential of [OIII] and [CII] surveys at reionization
• Clustering with JWST: Constraining Galaxy Host Halo Masses, Satellite Quenching Efficiencies, and Merger Rates at z=4-10
• The missing dwarf galaxies of the Local Group
• Sensitivity of dark matter haloes to their accretion histories
• The Massive Satellite Population of Milky-Way Sized Galaxies
• ZOMG II: Does the halo assembly history influence central galaxies and gas accretion?
• The evolving AGN duty cycle in galaxies since z$\sim$3 as encoded in the X-ray luminosity function
• Demonstrating Diversity in Star Formation Histories with the CSI Survey
• Cosmic evolution of bars in simulations of galaxy formation
• The star-formation history of mass-selected galaxies from the VIDEO survey
• Dissecting the roles of mass and environment quenching in galaxy evolution with EAGLE
• Highly r-process enhanced stars in ultra-faint dwarf galaxies
• An exquisitely deep view of quenching galaxies through the gravitational lens: Stellar population, morphology, and ionized gas
• The growth of galactic bulges through mergers in LCDM haloes revisited. II. Morphological mix evolution
• GARROTXA Cosmological Simulations of Milky Way-sized Galaxies: General Properties, Hot Gas Distribution, and Missing Baryons
• A model of spectral line broadening in signal forecasts for line-intensity mapping experiments
• Entropy Driven Winds: Outflows and Fountains Lifted Gently by Buoyancy
• Precision Redshift-Space Galaxy Power Spectra using Zel'dovich Control Variates
• Exploring stellar evolution with gravitational-wave observations
• Distinguishing Dark Matter, Modified Gravity, and Modified Inertia with the Inner and Outer Parts of Galactic Rotation Curves
• Tracing the Sources of Reionization in Cosmological Radiation Hydrodynamics Simulations
• The Next Generation Virgo Cluster Survey. IX. Estimating the Efficiency of Galaxy Formation on the Lowest-Mass Scales
• Revisiting the Size-Luminosity Relation in the Era of Ultra Diffuse Galaxies
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• Characterising the Intracluster Light over the Redshift Range $0.2<z<0.8$ in the DES-ACT Overlap
• Black versus Dark: Rapid Growth of Supermassive Black Holes in Dark Matter Halos at z ~ 6
• EAGLE-Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
• Probing Cosmic Origins with CO and [CII] Emission Lines
• Cosmological Simulations of Dwarf Galaxies with Cosmic Ray Feedback
• AGN feedback and the origin and fate of the hot gas in early-type galaxies
• The phantom dark matter halos of the Local Volume in the context of modified Newtonian dynamics
• The relation between star formation rate and stellar mass of galaxies at z $\sim$ 1-4
• Prospects for distinguishing galaxy evolution models with surveys at redshifts $z\gtrsim 4$
• 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
• From starburst to quiescence: post-starburst galaxies and their large-scale clustering over cosmic time
• UniverseMachine: Predicting Galaxy Star Formation over Seven Decades of Halo Mass with Zoom-in Simulations
• Modeling the kinematics of globular cluster systems
• 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 evolution of galaxy intrinsic alignments in the MassiveBlack II universe
• How long do high-redshift massive black hole seeds remain outliers in black hole vs. host galaxy relations?
• 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 dependence of the X-ray AGN clustering on the properties of the host galaxy
• COSMOS2020: Identification of High-z Protocluster Candidates in COSMOS
• The miniJPAS survey: The role of group environment in quenching the star formation
• Feeding cosmic star formation: Exploring high-redshift molecular gas with CO intensity mapping
• Constraining the Milky Way halo kinematics via its Linear Response to the Large Magellanic Cloud
• The dark side of galaxy stellar populations I: The stellar-to-halo mass relation and the velocity dispersion - halo mass relation
• On the early evolution of Local Group dwarf galaxy types: star formation and supernova feedback
• RESOLVE and ECO: The Halo Mass-Dependent Shape of Galaxy Stellar and Baryonic Mass Functions
• Preprocessing, mass loss and mass segregation of galaxies in DM simulations
• Scaling relations and baryonic cycling in local star-forming galaxies. III. Outflows, effective yields and metal loading factors
• 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
• Evidence for a Massive Andromeda Galaxy Using Satellite Galaxy Proper Motions
• Cosmological evolution of the Nitrogen abundance
• Dark influences III. Structural characterization of minor mergers of dwarf galaxies with dark satellites
• Stellar Mass Function of Active and Quiescent Galaxies via the Continuity Equation
• 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
• A fast radio burst in the direction of the Virgo cluster
• AstraeusIV : Quantifying the star formation histories of galaxies in the Epoch of Reionization
• A population of ultraviolet-dim protoclusters detected in absorption
• 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
• Cosmological simulations of the same spiral galaxy: the impact of baryonic physics
• Testing the Relationship Between Bursty Star Formation and Size Fluctuations of Local Dwarf Galaxies
• Star formation quenching imprinted on the internal structure of naked red nuggets
• Measuring the delay time distribution of binary neutron stars. I. Through Scaling Relations of the Host Galaxies of Gravitational Wave Events
• 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
• ATLAS Probe: Breakthrough Science of Galaxy Evolution, Cosmology, Milky Way, and the Solar System
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• Galaxy Formation in Sterile Neutrino Dark Matter Models
• Cosmic variance in the nanohertz gravitational wave background
• A New Approach to Identifying the Most Powerful Gravitational Lensing Telescopes
• Charting the main sequence of star-forming galaxies out to redshifts z<5.7
• A Systematic Search for Galaxy Proto-Cluster Cores at $z\sim 2$
• Dark Matter Density Profiles in Dwarf Galaxies: Linking Jeans Modeling Systematics and Observation
• Enhanced Rates of Fast Radio Bursts from Galaxy Clusters
• A Search for Satellite Galaxies of Nearby Star-Forming Galaxies with Resolved Stars in LBT-SONG
• An empirical prediction for stellar metallicity distributions in nearby galaxies
• Constraining the recent star formation history of galaxies : an Approximate Bayesian Computation approach
• Edge-on HI-bearing ultra diffuse galaxy candidates in the 40% ALFALFA catalog
• Quantifying the power spectrum of small-scale structure in semi-analytic galaxies
• Evolution of dispersion in the cosmic deuterium abundance
• Satellite mass functions and the faint end of the galaxy mass-halo mass relation in LCDM
• 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
• A Uniform History for Galaxy Evolution
• 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
• Galaxy Lookback Evolution Models -- a Comparison with Magneticum Cosmological Simulations and Observations
• 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
• Connections between star cluster populations and their host galaxy nuclear rings
• Excess of high-$z$ galaxies as a test for bumpy power spectrum of density perturbations
• The global and radial stellar mass assembly of Milky Way-sized galaxies
• Cumulative Neutrino and Gamma-Ray Backgrounds from Halo and Galaxy Mergers
• Constraints on the HI Mass of NGC 1052-DF2
• Galaxy formation in the Planck cosmology II. Star formation histories and post-processing magnitude reconstruction
• 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
• Active Galactic Nuclei outflows in galaxy discs
• A controlled study of cold dust content in galaxies from $z=0-2$
• A scenario for ultra-diffuse satellite galaxies with low velocity dispersions: the case of [KKS 2000]04
• Spectral Distortion of the CMB by the Cumulative CO Emission from Galaxies throughout Cosmic History
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• Dark acoustic oscillations: Imprints on the matter power spectrum and the halo mass function
• The Dynamics and Distribution of Angular Momentum in HiZELS Star-Forming Galaxies at z = 0.8 - 3.3
• Constraining the intrinsic population of Long Gamma-Ray Bursts: implications for spectral correlations, cosmic evolution and their use as tracers of star formation
• SH$\alpha$DE: Survey description and mass-kinematics scaling relations for dwarf galaxies
• First direct dynamical detection of a dual supermassive black hole system at sub-kiloparsec separation
• The clustering of $z>7$ galaxies: Predictions from the BLUETIDES simulation
• An Explanation for Overrepresentation of Tidal Disruption Events in Post-starburst Galaxies
• The evolution of dwarf galaxy satellites with different dark matter density profiles in the ErisMod simulations. I. The early infalls
• 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
• Building robust AGN mock catalogs to unveil black hole evolution and for survey planning
• Tidal disruption events can power the observed AGN in dwarf galaxies
• How the first stars shaped the faintest gas-dominated dwarf galaxies
• Differences and similarities of stellar populations in LAEs and LBGs at $z\sim$ 3.4 - 6.8
• [OII] emitters in MultiDark-Galaxies and DEEP2
• The Effect of Adiabatic Compression on Dark Matter Halos and the Radial Acceleration Relation
• The origin of X-ray coronae around simulated disc galaxies
• Galaxy stellar mass assembly: the difficulty matching observations and semi-analytical predictions
• Long gamma-ray burst rate at very high redshift
• The environment and host haloes of the brightest z~6 Lyman-break galaxies
• Dark influences II: gas and star formation in minor mergers of dwarf galaxies with dark satellites
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• Surrogate modelling the Baryonic Universe II: on forward modelling the colours of individual and populations of galaxies
• Multi-wavelength mock galaxy catalogs of the low-redshift Universe
• On the mass assembly of low-mass galaxies in hydrodynamical simulations of structure formation
• The mass-metallicity relation as a ruler for galaxy evolution: insights from the James Webb Space Telescope
• Black hole formation and growth with non-Gaussian primordial density perturbations
• Exploring extensions to the standard cosmological model and the impact of baryons on small scales
• Measuring the Stellar Masses of z~7 Galaxies with Spitzer Ultrafaint Survey Program (SURFS UP)
• Star formation and AGN activity in the most luminous LINERs in the local universe
• The Variation of Rotation Curve Shapes as a Signature of the Effects of Baryons on Dark Matter Density Profiles
• The GOGREEN Survey: Constraining the Satellite Quenching Timescale in Massive Clusters at $\mathbf{z}\gtrsim 1$
• Importance of Mock Observations in Validating Galaxy Properties for Cosmological Simulations
• Study of gravitational fields and globular cluster systems of early-type galaxies
• The effect of dark matter-dark radiation interactions on halo abundance -- a Press-Schechter approach
• Galaxy rotation curves and universal scaling relations: comparison between phenomenological and fermionic dark matter profiles
• Prospects for 21cm-Galaxy Cross-Correlations with HERA and the Roman High-Latitude Survey
• 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
• Distortion of the luminosity function of high-redshift galaxies by gravitational lensing
• Feedback by supermassive black holes in galaxy evolution: impacts of accretion and outflows on the star formation rate
• 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 $z=4.9-7.0$
• Tidal stirring of satellites with shallow density profiles prevents them from being too big to fail
• The VLA Frontier Field Survey: A Comparison of the Radio and UV/optical size of $0.3\lesssim z\lesssim 3$ star-forming galaxies
• 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
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• 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
• LoCuSS: The Near-Infrared Luminosity and Weak-Lensing Mass Scaling Relation of Galaxy Clusters
• Characterising Tidal Features Around Galaxies in Cosmological Simulations
• 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
• Clustering Constraints on the Relative Sizes of Central and Satellite Galaxies
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• Dark Matter Response to Galaxy Assembly History
• TRINITY II: The Luminosity-dependent Bias of the Supermassive Black Hole Mass--Galaxy Mass Relation for Bright Quasars at $z=6$
• Informing dark matter direct detection limits with the ARTEMIS simulations
• The trajectories of galaxies in groups: mass loss and preprocessing
• Some observational tests of a minimal galaxy formation model
• A galaxy group candidate at z~3.7 in the COSMOS field
• A complete distribution of redshifts for sub-millimetre galaxies in the SCUBA-2 Cosmology Legacy Survey UDS field
• Local photoionization feedback effects on galaxies
• Quasi-equilibrium models of high-redshift disc galaxy evolution
• Detection and classification of supernovae beyond z~2 redshift with the James Webb Space Telescope
• The hidden satellites of massive galaxies and quasars at high-redshift
• Formation and assembly history of stellar components in galaxies as a function of stellar and halo mass
• Evidence for strong progenitor age dependence of type Ia supernova luminosity standardization process
• The changing circumgalactic medium over the last 10 Gyr I: physical and dynamical properties
• A Framework for Empirical Galaxy Phenomenology: The Scatter in Galaxy Ages and Stellar Metallicities
• Effects of feedback on galaxies in the VELA simulations: elongation, clumps and compaction
• Reversal of Fortune: Increased Star Formation Efficiencies in the Early Histories of Dwarf Galaxies?
• Properties of the interstellar medium in star-forming galaxies at redshifts 2 < z < 5 from the VANDELS survey
• Constraining the Mass of the Emerging Galaxy Cluster SpARCS1049+56 at z=1.71 with Infrared Weak Lensing
• Mass and size growth of early-type galaxies by dry mergers in cluster environments
• The baryon cycle of Seven Dwarfs with superbubble feedback
• Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
• Revisiting the bulge-halo conspiracy II: Towards explaining its puzzling dependence on redshift
• Setting firmer constraints on the evolution of the most massive, central galaxies from their local abundances and ages
• 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
• Quantifying the Origin and Distribution of Intracluster Light in a Fornax-like Cluster
• 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
• 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
• Magnetogenesis at Cosmic Dawn: Tracing the Origins of Cosmic Magnetic Fields
• Gas Accretion and Galactic Chemical Evolution: Theory and Observations
• Measuring Dark Matter in Galaxies: The Mass Fraction Within 5 Effective Radii
• The frequency of very young galaxies in the local Universe: I. A test for galaxy formation and cosmological models
• MaNGA galaxy properties -- II. A detailed comparison of observed and simulated spiral galaxy scaling relations
• NIHAO XXVI: Nature versus nurture, the Star Formation Main Sequence and the origin of its scatter
• A multiwavelength survey of HI-excess galaxies with surprisingly inefficient star formation
• The COSMOS-Web ring: in-depth characterization of an Einstein ring lensing system at z~2
• New empirical constraints on the cosmological evolution of gas and stars in galaxies
• Noema formIng Cluster survEy (NICE): Discovery of a starbursting galaxy group with a radio-luminous core at z=3.95
• Biases and Cosmic Variance in Molecular Gas Abundance Measurements
• Catalogue of model star clusters in the Milky Way and M31 galaxies
• A new class of dark matter-free dwarf galaxies? I. Clues from FCC 224, NGC 1052-DF2 and NGC 1052-DF4
• Combining high-z galaxy luminosity functions with Bayesian evidence
• The MUSE Hubble Ultra Deep Field Survey XVI. The angular momentum of low-mass star-forming galaxies. A cautionary tale and insights from TNG50
• The Impacts of Modeling Choices on the Inference of the Circumgalactic Medium Properties from Sunyaev-Zeldovich Observations
• Modeling Redshift-Space Clustering with Abundance Matching
• Effects of self-consistent rest-ultraviolet colours in semi-empirical galaxy formation models
• Constraints on the Evolution of the Galaxy Stellar Mass Function I: Role of Star Formation, Mergers and Stellar Stripping
• NOEMA formIng Cluster survEy (NICE): Characterizing eight massive galaxy groups at $1.5<z<4$ in the COSMOS field
• Halo Histories vs. Galaxy Properties at z=0, III: The Properties of Star-Forming Galaxies
• The impact of dark energy on galaxy formation. What does the future of our Universe hold?
• 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
• The Impact of Environment on Late Time Evolution of the Stellar Mass - Halo Mass Relation
• Compact Binary Merger Rate in Dark-Matter Spikes
• Dependence of galaxy clustering on UV-luminosity and stellar mass at $z\sim 4-7$
• Calibration of a star formation and feedback model for cosmological simulations with Enzo
• The Chandra COSMOS Legacy Survey: clustering dependence of Type 2 AGN on host galaxy properties
• Using cosmological simulations and synthetic absorption spectra to assess the accuracy of observationally derived CGM metallicities
• The Baryonic Collapse Efficiency of Galaxy Groups in the RESOLVE and ECO Surveys
• On the Impact of Neutron Star Binaries Natal-Kick Distribution on the Galactic r-process Enrichment
• Late Bloomer Galaxies: Growing Up in Cosmic Autumn
• HI Global Scaling Relations in the WISE-WHISP Survey
• 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
• Influence of ~7 keV sterile neutrino dark matter on the process of reionization
• 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
• The Differing Relationships Between Size, Mass, Metallicity and Core Velocity Dispersion of Central and Satellite Galaxies
• Gas around galaxy haloes - III: hydrogen absorption signatures around galaxies and QSOs in the Sherwood simulation suite
• Simplified galaxy formation with mesh-less hydrodynamics
• Using Artificial Neural Networks to Constrain the Halo Baryon Fraction during Reionization
• HOD modelling of high redshift galaxies using the BLUETIDES simulation
• 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 $z<0.7$
• 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
• A single galaxy population? statistical evidence that the Star-Forming Main Sequence might be the tip of the iceberg
• Galactic Habitability Re-Examined: Indications of Bimodality
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$. V: Properties of dark matter halos containing H$\alpha$ emitting galaxies
• Multiple regimes and coalescence timescales for massive black hole pairs ; the critical role of galaxy formation physics
• 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
• Bulge formation through disc instability -- I
• Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
• 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
• Cosmic Type Ia SN rate and constraints on SN Ia progenitors
• Investigating the $M_{GCS}-M_h$ Relation in the Most Massive Galaxies
• 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
• 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
• Radial Distributions of Surface Mass Density and Mass-to-Luminosity Ratio in Spiral Galaxies
• JADES: Rest-frame UV-to-NIR Size Evolution of Massive Quiescent Galaxies from Redshift z=5 to z=0.5
• 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
• A titanic interstellar medium ejection from a massive starburst galaxy at redshift 1.4
• GalICS 2.1: a new semianalytic model for cold accretion, cooling, feedback and their roles in galaxy formation
• Understanding the progenitor formation galaxies of merging binary black holes
• Dwarf galaxies as a probe of a primordially magnetized Universe
• AGN must be very efficient at powering outflows
• Explaining the enhanced star formation rate of Jellyfish galaxies in galaxy clusters
• Black hole mergers as tracers of spinning massive black hole and galaxy populations in the OBELISK simulation
• A partial inventory of observational anisotropies in single-dish line-intensity mapping
• The bright end of the galaxy luminosity function at $z\simeq 7$ from the VISTA VIDEO survey
• A millimeter-wave redshift search for the unlensed HyLIRG, HS1700.850.1
• The Luminosity Functions and Redshift Evolution of Satellites of Low-Mass Galaxies in the COSMOS Survey
• The metallicity and star formation activity of long gamma-ray burst hosts for z$<$3: insights from the Illustris simulation
• Non-parametric Morphologies of Mergers in the Illustris Simulation
• Detecting clusters and groups of galaxies populating the local Universe in large optical spectroscopic surveys
• Constraining Scatter in the Stellar Mass--Halo Mass Relation for Haloes Less Massive than the Milky Way
• Effect of primordial non-Gaussianities on the far-UV luminosity function of high-redshift galaxies: implications for cosmic reionization
• Galaxy And Mass Assembly (GAMA): The absence of stellar mass segregation in galaxy groups and consistent predictions from GALFORM and EAGLE simulations
• 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
• Resolved and Integrated Stellar Masses in the SDSS-IV/MaNGA Survey, Paper I: PCA spectral fitting & stellar mass-to-light ratio estimates
• Ionized Gas Outflows in Low Excitation Radio Galaxies Are Radiation Driven
• What Regulates Galaxy Evolution? Open Questions in Our Understanding of Galaxy Formation and Evolution
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• Comparing weak lensing peak counts in baryonic correction models to hydrodynamical simulations
• Large gas inflow driven by a matured galactic bar in the early Universe
• The Coevolution of Massive Quiescent Galaxies and Their Dark Matter Halos over the Last 6 Billion Years
• Investigating the impact of galaxies' compact binary hosting probability for gravitational-wave cosmology
• Mapping the low surface brightness Universe in the UV band with Lya emission from IGM filaments
• Baryonic Imprints on DM Halos: The concentration-mass relation in the CAMELS simulations
• The fate of a red nugget: In-situ star formation of satellites around a massive compact galaxy
• Halo Acceleration Relation
• Stellar Feedback and the Energy Budget of Late-Type Galaxies: Missing Baryons and Core Creation
• The evolution of cold neutral gas and the star formation history
• Spatially Resolved Gas-phase Metallicity in FIRE-2 Dwarfs: Late-Time Evolution of Metallicity Relations in Simulations with Feedback and Mergers
• Modified Gravity Theories in Light of the Anomalous Velocity Dispersion of NGC1052-DF2
• 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
• The Galaxy Replacement Technique (GRT): a New Approach to Study Tidal Stripping and Formation of Intracluster Light in a Cosmological Context
• On estimation of contamination from hydrogen cyanide in carbon monoxide line intensity mapping
• The transformation and quenching of simulated gas-rich dwarf satellites within a group environment
• Galaxy-Galaxy Lensing in EAGLE: comparison with data from 180 square degrees of the KiDS and GAMA surveys
• Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
• Distinguishing the impact and signature of black holes from different origins in early cosmic history
• On the Edge: the relation between stellar and dark matter haloes of Milky Way-mass galaxies
• Extragalactic Science with the Experiment for Cryogenic Large-aperture Intensity Mapping
• Compatibility of the Large Quasar Groups with the Concordance Cosmological Model
• 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
• Dark Energy Survey Year 1 Results: The effect of intracluster light on photometric redshifts for weak gravitational lensing
• Ironing the folds: The phase space chevrons of a GSE-like merger as a dark matter subhalo detector
• Galaxies of the $z\sim 2$ Universe. I. Grism-Selected Rest-Frame Optical Emission Line Galaxies
• Self-Interacting Dark Matter and the Delay of Super-Massive Black Hole Growth
• HI within and around observed and simulated galaxy discs -- Comparing MeerKAT observations with mock data from TNG50 and FIRE-2
• Simulating Deep Hubble Images With Semi-empirical Models of Galaxy Formation
• HI study of isolated and pair galaxies: the MIR SFR-M$\star$ sequence
• Matching the mass function of Milky Way satellites in competing dark matter models
• 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
• A universal angular momentum profile for dark matter haloes
• Looking for Traces of Non-minimally Coupled Dark Matter in the X-COP Galaxy Clusters Sample
• Investigating overdensities around z>6 galaxies through ALMA observations of [CII]
• Unveiling cosmological information on small scales with line intensity mapping
• 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
• Revealing the formation mechanism of the shell galaxy NGC474 with MUSE
• Interpreting the cosmic far-infrared background anisotropies using a gas regulator model
• An intergalactic medium temperature from a giant radio galaxy
• 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
• 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
• Dark matter fraction of low-mass cluster members probed by galaxy-scale strong lensing
• Over-density of SMGs in fields containing z~0.3 galaxies: magnification bias and the implications for studies of galaxy evolution
• Life after AGN switchoff: evolution and properties of fossil galactic outflows
• An empirical model to form and evolve galaxies in dark matter halos
• Feedback and dynamical masses in high-$z$ galaxies: the advent of high-resolution NIRSpec spectroscopy
• Applying Noether's theorem to matter in the Milky Way: evidence for external perturbations and non-steady-state effects from Gaia Data Release 2
• Searching for dark matter annihilation from individual halos: uncertainties, scatter and signal-to-noise ratios
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• Multiverse Predictions for Habitability: The Number of Stars and their Properties
• 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
• Galaxy growth from redshift 5 to 0 at fixed comoving number density
• Constraining the nature of dark matter with the star formation history of the faintest Local Group dwarf galaxy satellites
• Pre-supernova feedback mechanisms drive the destruction of molecular clouds in nearby star-forming disc galaxies
• Strong-lensing cosmography using third-generation gravitational-wave detectors
• Simulated stellar kinematics studies of high-redshift galaxies with the HARMONI Integral Field Spectrograph
• Using the Star Forming Main Sequence To Explore Quiescent Galaxies Across Cosmic Time
• Beacons In the Dark: Using Novae and Supernovae to Detect Dwarf Galaxies in the Local Universe
• A systematic search for galaxy protocluster cores at the transition epoch of their star formation activity
• Evolution of CIV Absorbers. II. Where does CIV live?
• Exploring Self-Interacting Dark Matter Halos with Diverse Baryonic Distributions: A Parametric Approach
• How dark are filaments in the cosmic web?
• Candidate high-redshift protoclusters and lensed galaxies in the Planck list of high-z sources overlapping with Herschel-SPIRE imaging
• Testing multiflavored ULDM models with SPARC
• 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
• Origin and Evolution of Structure and Nucleosynthesis for Galaxies in the Local Group
• Frequency of the dark matter subhalo collisions and bifurcation sequence arising formation of dwarf galaxies
• Dynamics and Shocks from H$\alpha$ Emission of Nearby Galaxy Mergers
• A semi-analytical perspective on massive galaxies at $z\sim 0.55$
• Faint Dwarfs in Nearby Groups
• 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
• A comparison of the R_h=ct and LCDM cosmologies based on the observed halo mass function
• Connection between galaxy morphology and dark-matter halo structure I: a running threshold for thin discs and size predictors from the dark sector
• A consistent model for both the HI and stellar mass functions of galaxies
• Constraints on Lorentz-invariance violation in the neutrino sector from the ultrahigh-energy event KM3-230213A
• Abundance matching for low mass galaxies in the CDM and FDM models
• Dust Properties of Local Dust-Obscured Galaxies with the Submillimeter Array
• The signal of decaying dark matter with hydrodynamical simulations
• Galaxy mass-size segregation in the cosmic web from the CAVITY parent sample
• Primordial Black Hole-Neutron Star Merger Rate in Modified Gravity
• Connecting the Dots: Tracking Galaxy Evolution Using Constant Cumulative Number Density at 3<z<7
• Auriga Streams I: disrupting satellites surrounding Milky Way-mass haloes at multiple resolutions
• The Impact of Wind Scalings on Stellar Growth and the Baryon Cycle in Cosmological Simulations
• MOCCA-SURVEY Database -- I. Tidal disruption events of white dwarfs in globular clusters and young massive clusters
• 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
• 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
• Reconciling Volumetric and Individual Galaxy Type Ia Supernova Rates
• 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
• First results from SMAUG: Insights into star formation conditions from spatially-resolved ISM properties in TNG50
• 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
• Confusion of extragalactic sources in the far infrared: a baseline assessment of the performance of PRIMAger in intensity and polarization
• ARTEMIS emulator: exploring the effect of cosmology and galaxy formation physics on Milky Way-mass haloes and their satellites
• PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at $0.2<z<0.9$
• Co-Evolution vs. Co-existence: The Effect of Accretion Modelling on the Evolution of Black Holes and Host Galaxies
• Probing the Mpc-scale environment of hyperluminous infrared galaxies at 2<z<4
• A Hyperactive FRB Pinpointed in an SMC-Like Satellite Host Galaxy
• Galactic wind X-ray heating of the intergalactic medium during the Epoch of Reionization
• The Dark Matter Halos of HI Selected Galaxies
• Characterizing simulated galaxy stellar mass histories
• Sunscreen: Photometric Signatures of Galaxies Partially Cloaked in Dyson Spheres
• The deconvolved distribution estimator: enhancing reionisation-era CO line-intensity mapping analyses with a cross-correlation analogue for one-point statistics
• The stellar mass function and efficiency of galaxy formation with a varying initial mass function
• 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
• Mapping the Universe in HD
• Constraining the host galaxy halos of massive black holes from LISA event rates
• Gamma-ray Production in the Extended Halo of the Galaxy and Possible Implications for the Origin of Galactic Cosmic Rays
• The XXL survey. XLIX. Linking the members star formation histories to the cluster mass assembly in the z=1.98 galaxy cluster XLSSC 122
• The THESAN-ZOOM project: Star-formation efficiencies in high-redshift galaxies
• Analysis of the spatially-resolved $V$-3.6$\mu$m colors and dust extinction in 257 nearby NGC and IC galaxies
• Possible evolution of the circum-galactic medium around QSOs with QSO age and cosmic time revealed by Ly$\alpha$ halos
• A Physical Model for the Quasar Luminosity Function Evolution between Cosmic Dawn and High Noon
• Ghostly Stellar Haloes and their Relationship to Ultra-faint Dwarfs
• Black hole feedback and the evolution of massive early-type galaxies
• PAC in DESI. I. Galaxy Stellar Mass Function into the $10^6{\mathrm{M}}_{\odot }$ Frontier
• The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
• 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
• Size, shade or shape? The contribution of galaxies of different types to the star-formation history of the Universe from SDSS-IV MaNGA
• Stellar Metallicity of Galaxies: New Insight on the Formation and Evolution of Low Surface Brightness Galaxies in the IllustrisTNG Simulation
• 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 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
• A break in the high-redshift stellar mass Tully-Fisher relation
• A comparison of ${\text{H}}_2$ formation models at high redshift
• Fingerprints of modified gravity on galaxies in voids
• Distribution of star formation rates during the rapid assembly of NGC 1399 as deduced from its globular cluster system
• The Effects of Dark Matter Annihilation on Cosmic Reionization
• Enhanced spectrum of primordial perturbations, galaxy formation and small scale structure
• The significant effects of stellar mass estimation on galaxy pair fractions
• EMERGE: Constraining merging probabilities and timescales of close galaxy pairs
• Impact of star formation models on the growth of simulated galaxies at high redshifts
• Diverse dark matter profiles in FIRE dwarfs: black holes, cosmic rays and the cusp-core enigma
• Where Did the Outskirts Go? Outer Stellar Haloes as a Sensitive Probe of Supernova Feedback
• Testing primordial non-Gaussianities on galactic scales at high redshift
• Classical bulges, supermassive blackholes and AGN feedback: Extension to low-mass galaxies
• Globular cluster ages and their relation to high-redshift stellar cluster formation times from different globular cluster models
• Imprint of the galactic acceleration scale on globular cluster systems
• Abundance matching tested on small scales with galaxy dynamics
• The extended Planetary Nebula Spectrograph (ePN.S) early-type galaxy survey: The specific angular momentum of ETGs
• From Gas to Stars Over Cosmic Time
• 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
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• JWST PRIMER: A deep JWST study of all ALMA-detected galaxies in PRIMER COSMOS -- dust-obscured star-formation history back to z $\simeq$ 7
• Compact Binary Merger Rate with Modified Gravity in Dark-Matter Spikes
• A rising tide: Intrinsic alignments since the turn of the millennium
• EDEN: Exploring Disks Embedded in N-body simulations of Milky-Way-mass halos from Symphony
• Cosmic star formation history with tomographic cosmic infrared background-galaxy cross-correlation
• Revisiting the Relationship between the Long GRB Rate and Cosmic Star Formation History Based on a Large Swift Sample
• Revealing the hidden cosmic feast: A z=4.3 galaxy group hosting two optically dark, efficiently star-forming galaxies
• Unveiling Multiple Physical Processes on a Cluster Galaxy at z=0.3 Using JWST
• The properties and environment of very young galaxies in the local Universe
• On the Effects of Local Environment on Active Galactic Nucleus (AGN) in the Horizon Run 5 Simulation
• A physical model for the redshift evolution of high-z Lyman-Break Galaxies
• Toward a stellar population catalog in the Kilo Degree Survey: the impact of stellar recipes on stellar masses and star formation rates
• Measuring Dust Attenuation Curves of SINGS/KINGFISH Galaxies Using Swift/UVOT Photometry
• Observations of Ly$\alpha$ Emitters at High Redshift
• A Multi-messenger view of Cosmic Dawn: Conquering the Final Frontier
• Predictions for Detecting a Turndown in the Baryonic Tully Fisher Relation
• Modelling the mass accretion histories of dark matter haloes using a Gamma formalism
• The Halo Masses of Galaxies to $z\sim 3$: A Hybrid Observational and Theoretical Approach
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• HELLO project: High-$z$ Evolution of Large and Luminous Objects
• Variations of the ISM Compactness Across the Main Sequence of Star-Forming Galaxies: Observations and Simulations
• Detecting Massive Galaxies at High Redshift using the Dark Energy Survey
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• A two-phase model of galaxy formation: III. The formation of globular clusters
• The resolved star formation history of M51a through successive Bayesian marginalization
• Local Two-Sample Testing: A New Tool for Analysing High-Dimensional Astronomical Data
• The Galaxy Halo Connection in Modified Gravity Cosmologies: Environment Dependence of Galaxy Luminosity function
• Scalar Stochastic Gravitational-Wave Background in Brans-Dicke Theory of Gravity
• Dynamical Properties of Molecular-forming Gas Clumps in Galaxies at the Epoch of Reionization
• AGN lifetimes in UV-selected galaxies: a clue to supermassive black hole-host galaxy coevolution
• Subhalo abundance matching using progenitor mass at varying redshift: Two modes of stellar mass growth imprinted into the Subaru HSC galaxy clustering
• Properties of galaxies at the faint end of the H$\alpha$ luminosity function at $z\sim 0.62$
• Inferring Cosmological Parameters on SDSS via Domain-Generalized Neural Networks and Lightcone Simulations
• Feeding and feedback from little monsters: AGN in dwarf galaxies
• AuriDESI: Mock Catalogues for the DESI Milky Way Survey
• 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
• Die Hard: The On-Off-Cycle of Galaxies on the Star Formation Main Sequence
• Fading Light, Fierce Winds: JWST Snapshot of a Sub-Eddington Quasar at Cosmic Dawn
• Globular Cluster Systems and X-Ray Atmospheres in Galaxies
• UV and NIR size of the low-mass field galaxies: the UV compact galaxies
• Star formation across cosmic time
• Galaxy formation from a timescale perspective
• Does radiative feedback make faint z>6 galaxies look small?
• The miniJPAS survey. Evolution of the luminosity and stellar mass functions of galaxies up to $z\sim 0.7$
• Lessons from the Local Group (and beyond) on dark matter
• EIG - II. Intriguing characteristics of the most extremely isolated galaxies
• Evolving beyond z=0: insights about the future of stars and the intergalactic medium
• Galaxy Assembly and Evolution in the P-Millennium simulation: galaxy clustering
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Deciphering the Kinematic Substructure of Local Dark Matter with LAMOST K Giants
• A Rich Satellite Population of the NGC 4437 Group and Implications of a Magnitude Gap for Galaxy Group Assembly History
• Leveraging cross-correlations and linear covariance-based filtering for line-intensity map reconstructions at linear scales
• Models of AGN feedback
• Tracing the Total Stellar Mass and Star Formation of High-Redshift Protoclusters
• A Galaxy-Halo Model for Multiple Cosmological Tracers
• Euclid preparation. Exploring the properties of proto-clusters in the Simulated Euclid Wide Survey
• Stacked phase-space density of galaxies around massive clusters: Comparison of dynamical and lensing masses
• Cosmic evolution of molecular gas mass density from an empirical relation between ${\mathrm{L}}_{1.4GHz}$ and ${\mathrm{L}}_{\mathrm{CO}}^{\prime }$
• New observational recipes for measuring dynamical state of galaxy clusters
• Three-Dimensional Stacking as a Line Intensity Mapping Statistic
• Evolution of dwarf galaxy observable parameters
• COMAP Pathfinder -- Season 2 results III. Implications for cosmic molecular gas content at "Cosmic Half-past Eleven"
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• Quenching vs. Quiescence: forming realistic massive ellipticals with a simple starvation model
• Morpho-Photometric Classification of KiDS DR5 Sources Based on Neural Networks: A Comprehensive Star-Quasar-Galaxy Catalog
• Impact of the turnover in the high-z galaxy luminosity function on the 21-cm signal during Cosmic Dawn and Epoch of Reionization
• An Empirical Mass Function Distribution
• 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
• The inflow and outflow rate evolution of local Milky Way-mass star-forming galaxies since z=1.3
• Radiation-driven dusty outflows from early galaxies
• Modeling spatially-resolved galactic H$\alpha$ emission for galaxy clustering
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
• Massive Black Hole Mergers
• A candidate quadruple AGN system at $z\sim 3$
• The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
• Spatial Distribution of OVI Covering Fractions in the Simulated Circumgalactic Medium
• Calibrating baryonic effects in cosmic shear with external data in the LSST era
• Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
• Cosmological prior for the $J$-factor estimation of dwarf spheroidal galaxies
• Applying a star formation model calibrated on high-resolution interstellar medium simulations to cosmological simulations of galaxy formation
• Star formation rates in nearby Markarian galaxies
• The origin of galaxy colour bimodality in the scatter of the Stellar-to-Halo Mass Relation
• An ALMA spectroscopic survey of the Planck high-redshift object PLCK G073.4-57.5 confirms two protoclusters
• How do the dynamics of the Milky Way -- Large Magellanic Cloud system affect gamma-ray constraints on particle dark matter?
• 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
• GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations
• Impact of supermassive black hole growth on star formation
• Direct Shear Mapping: Prospects for weak lensing studies of individual galaxy-galaxy lensing systems
• Stellar halos tracing the assembly of ultra-faint dwarf galaxies
• IllustrisTNG + Cosmic Rays with a Simple Transport Model: From Dwarfs to L${}^{\star }$ Galaxies
• Cosmic Vine: High abundance of massive galaxies and dark matter halos in a forming cluster at z=3.44
• Modelling the Evolution of Ly$\alpha$ Blobs and Ly$\alpha$ Emitters
• 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
• A MUSE view of the multiple interacting system HCG 31
• Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies: Black Hole Scaling Relations Are Not Biased by Selection Effects
• Pulsar B1237+25 Aberration/Retardation Analysis from Decimeter to Decameter Wavelength: Challenge to "Radius-to-Frequency Mapping"
• Analysis of the Intrinsic Mid-Infrared L-band to Visible--Near-Infrared Flux Ratios in Spectral Synthesis Models of Composite Stellar Populations
• ELG$\times$LRG distribution through dark matter halo dynamics
• 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
• The ALMaQUEST Survey XVII: Unveiling Multiple Quenching Pathways in Green Valley Galaxies via Molecular Gas and Quenching Timescale Analyses
• A Stochastic Theory of the Hierarchical Clustering III. The Non-universality and Non-stationarity of the Halo Mass Function
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• The Assembly of the Virgo Cluster, Traced by its Galaxy Halos
• Impact of Cosmic Variance on the Galaxy-Halo Connection for Lyman-$\alpha$ Emitters
• PASSAGES: The Discovery of a Strongly Lensed Protocluster Core Candidate at Cosmic Noon
• 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
• Simultaneously Modelling Dusty Star Forming Galaxies and Massive Quiescents: A Calibration Framework for Galaxy Formation Models
• Search for the Footprints of New Physics with Laboratory and Cosmic Neutrinos
• X-ray stacking reveals average SMBH accretion properties of star-forming galaxies and their cosmic evolution over 4 <~ z <~ 7
• SOFIA/HAWC+ detection of a gravitationally lensed starburst galaxy at $z$ = 1.03
• Euclid preparation: TBD. Cosmic Dawn Survey: evolution of the galaxy stellar mass function across 0.2<z<6.5 measured over 10 square degrees
• A Redshift Survey of the Coma Cluster (A1656): Understanding the Nature of Subhalos in the Weak-lensing Map
• Dark-Matter-Deficient Galaxies from Collisions: A New Probe of Bursty Feedback and Dark Matter Physics
• Dark energy, spatial curvature, and star formation efficiency from JWST photometric and spectroscopic high-redshift galaxies
• SEMPER I. Radio Predictions for Star-Forming Galaxies at $0<z<5$
• Compact dust-obscured star-formation and the origin of the galaxy bimodality
• Spatial correlations of extended cosmological structures
• A Submillimeter Continuum Survey of Local Dust-Obscured Galaxies
• Machine Learning vs. Spectral Energy Distribution Fitting: A Comparative Analysis of Accuracy in Stellar Mass Estimation
• 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
• Machine Learning the Dark Matter Halo Mass of Milky Way-Like Systems
• Properties of Globular Clusters in Galaxy Clusters: Sensitivity from the Formation and Evolution of Globular Clusters
• Constraining the halo-ISM connection through multi-transition carbon monoxide line-intensity mapping
• Submillimeter galaxy overdensities around physically associated quasar pairs
• MIGHTEE-HI: The star-forming properties of HI selected galaxies
• Linking Compact Dwarf Starburst Galaxies in the RESOLVE Survey to Downsized Blue Nuggets
• The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
• Removal of interloper contamination to line-intensity maps using correlations with ancillary tracers of the large-scale structure
• Nearby dwarf galaxies with extreme star formation rates: a window into dwarf-galaxy evolution in the early Universe
• The intervelocity of galaxy pairs in $\Lambda$CDM -- The observed velocity peak at ~130 km/s is not unique to MOND
• Constraints on dark matter models from the stellar cores observed in ultra-faint dwarf galaxies: Self-interacting dark matter
• Self-sustaining star formation fronts in filaments during cosmic dawn
• Super-Eddington accretion in high-redshift quasar hosts: Black-hole driven outflows, galaxy quenching, and the nature of little red dots
• Mapping luminous and dark matter in the Universe
• Dark Energy Survey Year 6 Results: Intra-Cluster Light from Redshift 0.2 to 0.5
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• Peculiar dark matter halos inferred from gravitational lensing as a manifestation of modified gravity
• Quenching Global Star Formation: Dominance of Gravitational Shock Heating at z<2
• NIHAO-LG: The uniqueness of Local Group dwarf galaxies
• Gas thermodynamics meets galaxy kinematics: Joint mass measurements for eROSITA galaxy clusters
• Gamma Analytical Modeling Evolution (GAME) I: The physical implications of deriving the stellar mass functions from z=0 to z=8
• Subhalo abundance and satellite spatial distribution in Milky Way-Andromeda-like paired haloes
• 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
• Star formation quenching precedes morphological transformation in COSMOS-WEB's richest galaxy groups
• A hierarchical clustering method for quantifying satellite abundance
• The Effect of Impact Parameters on the Formation of Massive Black Hole Binaries in Galactic Mergers
• Sub-Gyr variability around the SFMS and its contribution to the scatter
• ODIN: Using multiplicity of Lyman-Alpha Emitters to assess star formation activity in dark matter halos
• CHILES X: Molecular and atomic gas at intermediate redshift
• Dynamical evolution timescales for the supermassive black hole system in the galaxy NGC 7727 (Arp 222)
• Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future
• Far-infrared lines hidden in archival deep multi-wavelength surveys: Limits on [CII]-158$\mu$m at $z\sim 0.3-2.9$
• What triggers type Ia supernovae: Prompt detonations from primordial black holes or companion stars?
• Dark-matter-induced transients over cosmic time: The role of star formation history profiles
• Insights into the dependence of galaxy properties on the environment with explainable machine learning models
• 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
• 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
• 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
• Free-floating molecular clumps and gas mixing: hydrodynamic aftermaths of the intracluster$-$interstellar medium interaction
• Covariances of Galaxy Stellar Mass Functions and Correlation Functions
• Testing Lorentz Symmetry using High Energy Astrophysics Observations
• Reconstructing the mass accretion histories of nearby Red Nuggets with their globular cluster systems
• Constraints on the existence of dark matter haloes by the M81 group and the Hickson compact groups of galaxies
• Atmospheric pressure and molecular cloud formation in early-type galaxies
• The multi-component fitting to the star formation histories in the TNG simulation
• Extended Hernquist-Springel formalism for cosmic star formation
• 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
• The Cen A galaxy group: dynamical mass and missing baryons
• Resonant optical gating of suspended carbon nanotube transistor
• Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter
• A Mass Dependent Density Profile from Dwarfs to Clusters
• HI Observations of Baryon-Dominated Dwarf Galaxy Candidates
• Clustering and physical properties of AGN and Star-Forming Galaxies at fixed stellar mass: does assembly bias have a role in AGN activity?
• Merging massive black holes: the right place and the right time
• LYRA II: Cosmological dwarf galaxy formation with inhomogeneous Population III enrichment
• Effect of dust in circumgalactic haloes on the cosmic shear power spectrum
• Size-scaling of clump instabilities in turbulent, feedback regulated disks
• Forming off-center massive black hole binaries in dwarf galaxies through Jacobi capture
• Stochastic Gravitational-Wave Background from Stellar Core-Collapse Events
• Spider-Webb: enhanced star formation in low-mass galaxies within the Spiderweb protocluster revealed by JWST Pa$\beta$ narrow-band imaging
• Massive black holes and their galaxies
• 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
• Correlation between Outlying Halo Abundance and Host Halo Properties
• Astrophysical Black holes: An Explanation for the Galaxy Quenching
• The odd primordial halo of the Milky Way implied by Gaia. A shallow core, but a steep decline
• Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling
• Suppression of galactic outflows by cosmological infall and circumgalactic medium
• An empirical model of the extragalactic radio background
• Turbulence in the intragroup and circumgalactic medium
• Space Project for Astrophysical and Cosmological Exploration (SPACE), an ESA stand-alone mission and a possible contribution to the Origins Space Telescope
• Detecting the $\pi$-axiverse through parametric resonance
• 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
• The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
• Decoding the star forming properties of gas-rich galaxy pairs
• CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA
• The Photometric Analysis of the Environment Around Two Dusty Star-Forming Galaxies at $z\sim 2$
• Initial Investigations of the Outskirts of XLSSC 122
• Spatially resolved stellar-to-total dynamical mass relation: Radial variations, gradients and profiles of galaxy stellar populations
• Dwarf Galaxy Number Counts within 25 Mpc: Predictions from Local Group Analogues in TNG50
• 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?
• 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
• 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
• Origin of the spectacular tidal shells of galaxy NGC474
• Exploring the gaseous halos of z>3 radio galaxies with UVES and JWST/NIRSpec
• Forward-modelling the Luminosity, Distance, and Size distributions of the Milky Way Satellites
• Momentum deposition of supernovae with cosmic rays