The Aquarius Project: the subhalos of galactic halos

Abstract

We have performed the largest ever particle simulation of a Milky Way-sized dark matter halo, and present the most comprehensive convergence study for an individual dark matter halo carried out thus far. We have also simulated a sample of 6 ultra-highly resolved Milky-way sized halos, allowing us to estimate the halo-to-halo scatter in substructure statistics. In our largest simulation, we resolve nearly 300,000 gravitationally bound subhalos within the virialized region of the halo. Simulations of the same object differing in mass resolution by factors up to 1800 accurately reproduce the largest subhalos with the same mass, maximum circular velocity and position, and yield good convergence for the abundance and internal properties of dark matter substructures. We detect up to four generations of subhalos within subhalos, but contrary to recent claims, we find less substructure in subhalos than in the main halo when regions of equal mean overdensity are compared. The overall substructure mass fraction is much lower in subhalos than in the main halo. Extrapolating the main halo's subhalo mass spectrum down to an Earth mass, we predict the mass fraction in substructure to be well below 3% within 100 kpc, and to be below 0.1% within the Solar Circle. The inner density profiles of subhalos show no sign of converging to a fixed asymptotic slope and are well fit by gently curving profiles of Einasto form. The mean concentrations of isolated halos are accurately described by the fitting formula of Neto et al. down to maximum circular velocities of 1.5 km/s, an extrapolation over some 5 orders of magnitude in mass. However, at equal maximum circular velocity, subhalos are more concentrated than field halos, with a characteristic density that is typically ~2.6 times larger and increases towards the halo centre.

Submitted to MNRAS on 08/08/2008, 30 pages, 29 figures. Full resolution version, images, and videos available at http://www.mpa-garching.mpg.de/aquarius

References in corpus (13)

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• Deep XMM Observations of Draco rule out at the 99% Confidence Level a Dark Matter Decay Origin for the 3.5 keV Line
• The Distribution of Metals in Cosmological Hydrodynamical Simulations of Dwarf Disk Galaxies
• Vaex: Big Data exploration in the era of Gaia
• Indirect Detection of Neutrino Portal Dark Matter
• The Spatial Distribution of Galactic Satellites in the LCDM Cosmology
• Small-scale clumps of dark matter
• The Three Causes of Low-Mass Assembly Bias
• Mining for Dark Matter Substructure: Inferring subhalo population properties from strong lenses with machine learning
• The abundance of satellites around Milky Way- and M31-like galaxies with the TNG50 simulation: a matter of diversity
• The Next Generation Virgo Cluster Survey (NGVS). XIII. The Luminosity and Mass Function of Galaxies in the Core of the Virgo Cluster and the Contribution from Disrupted Satellites
• The impact of baryonic discs on the shapes and profiles of self-interacting dark matter halos
• On the Effects of Line-of-Sight Structures on Lensing Flux-ratio Anomalies in a LCDM Universe
• CLUMPY: a code for gamma-ray signals from dark matter structures
• Idealized models for galactic disk formation and evolution in 'realistic' LambdaCDM haloes
• Enhanced tidal stripping of satellites in the galactic halo from dark matter self-interactions
• Dark Matter in Dwarf Spheroidal Galaxies and Indirect Detection: A Review
• The masses of Local Group dwarf spheroidal galaxies: The death of the universal mass profile
• Scaling Relations for Dark Matter Annihilation and Decay Profiles in Dwarf Spheroidal Galaxies
• Modeling the Connection Between Subhalos and Satellites in Milky Way-like Systems
• Stellar migrations and metal flows -- Chemical evolution of the thin disc of a simulated Milky Way analogous galaxy
• Search for extended gamma-ray emission from the Virgo galaxy cluster with Fermi-LAT
• The tidal evolution of dark matter substructure -- II. The impact of artificial disruption on subhalo mass functions and radial profiles
• The BOSS Emission-Line Lens Survey. III. : Strong Lensing of Ly$\alpha$ Emitters by Individual Galaxies
• The diverse dark matter density at sub-kiloparsec scales in Milky Way satellites:implications for the nature of dark matter
• Scaling Laws for Dark Matter Halos in Late-Type and Dwarf Spheroidal Galaxies
• Substructure in the stellar halos of the Aquarius simulations
• Disruption of satellite galaxies in simulated groups and clusters: the roles of accretion time, baryons, and pre-processing
• Dark matter in the solar system I: The distribution function of WIMPs at the Earth from solar capture
• The Density and Pseudo-Phase-Space Density Profiles of CDM halos
• Properties of HI discs in the Auriga cosmological simulations
• The First Tidally Disrupted Ultra-Faint Dwarf Galaxy? - Spectroscopic Analysis of the Tucana III Stream
• The Dynamical State of Dark Matter Haloes in Cosmological Simulations I: Correlations with Mass Assembly History
• Hunting Dark Matter Gamma-Ray Lines with the Fermi LAT
• Stealth Galaxies in the Halo of the Milky Way
• The MaGICC Baryon Cycle: The Enrichment History of Simulated Disc Galaxies
• Milky Way mass constraints from the Galactic satellite gap
• Escape of Lyman-alpha and continuum photons from star-forming galaxies
• Constraints on the annihilation cross section of dark matter particles from anisotropies in the diffuse gamma-ray background measured with Fermi-LAT
• Dissecting the Evolution of Dark Matter Subhaloes in the Bolshoi Simulation
• The Onset of Gravothermal Core Collapse in Velocity Dependent Self-Interacting Dark Matter Subhaloes
• CLUMPY: Jeans analysis, $\gamma$-ray and neutrino fluxes from dark matter (sub-)structures
• Metal-Poor Stars and the Chemical Enrichment of the Universe
• General relativistic corrections to $N$-body simulations and the Zel'dovich approximation
• The distribution of gas in the Local Group from constrained cosmological simulations: the case for Andromeda and the Milky Way galaxies
• On The Gamma-Ray Emission From Reticulum II and Other Dwarf Galaxies
• Populations of double white dwarfs in Milky Way satellites and their detectability with LISA
• The angular momentum of cold dark matter haloes with and without baryons
• Quantifying dwarf satellites through gravitational imaging: the case of SDSS J120602.09+514229.5
• Can filamentary accretion explain the orbital poles of the Milky Way satellites?
• The multiplicity and anisotropy of galactic satellite accretion
• Stringent Constraints On The Dark Matter Annihilation Cross Section From Subhalo Searches With The Fermi Gamma-Ray Space Telescope
• The surprising accuracy of isothermal Jeans modelling of self-interacting dark matter density profiles
• Discovery of a red ultra-diffuse galaxy in a nearby void based on its globular cluster luminosity function
• Detailed Abundances in the Ultra-faint Magellanic Satellites Carina II and III
• The tidal evolution of dark matter substructure -- I. Subhalo density profiles
• Projection effects in the strong lensing study of subhaloes
• Gamma-ray background anisotropy from galactic dark matter substructure
• The Redshift Space Momentum Power Spectrum II: measuring the growth rate from the combined 2MTF and 6dFGSv surveys
• Dynamics of stream-subhalo interactions
• Decaying vs Annihilating Dark Matter in Light of a Tentative Gamma-Ray Line
• Subhalo destruction in the Apostle and Auriga simulations
• SHARP - IV. An apparent flux ratio anomaly resolved by the edge-on disc in B0712+472
• Baryonic and dark matter distribution in cosmological simulations of spiral galaxies
• Dark Stars: A Review
• Substructure in the lens HE 0435-1223
• Gas depletion in Local Group dwarfs on ~250 kpc scales: Ram pressure stripping assisted by internal heating at early times
• Dark Matter Subhalos In the Fermi First Source Catalog
• Dark matter-radiation interactions: the structure of Milky Way satellite galaxies
• Static, spherically symmetric solutions with a scalar field in Rastall gravity
• From Galaxy Clusters to Ultra-Faint Dwarf Spheroidals: A Fundamental Curve Connecting Dispersion-supported Galaxies to Their Dark Matter Halos
• Globular Cluster Formation Within The Aquarius Simulation
• Lessons from the Auriga discs: The hunt for the Milky Way's ex-situ disc is not yet over
• Halo model description of the non-linear dark matter power spectrum at $k\gg 1$ Mpc${}^{-1}$
• Reconstructing cosmological initial conditions from galaxy peculiar velocities. I. Reverse Zeldovich Approximation
• ART^2 : Coupling Lyman-alpha Line and Multi-wavelength Continuum Radiative Transfer
• Probing the nature of dark matter particles with stellar streams
• Investigating Gamma-Ray Lines from Dark Matter with Future Observatories
• Statistics of Dark Matter Substructure: III. Halo-to-Halo Variance
• Singlet-Doublet Dark Matter Freeze-in: LHC displaced signatures versus cosmology
• The impact of baryon physics on the structure of high-redshift galaxies
• Probing the nature of dark matter by forward modeling flux ratios in strong gravitational lenses
• Halo Substructure Boosts to the Signatures of Dark Matter Annihilation
• Thermal Relics in Modified Cosmologies: Bounds on Evolution Histories of the Early Universe and Cosmological Boosts for PAMELA
• The Galaxy Clustering Crisis in Abundance Matching
• Aurigaia: mock Gaia DR2 stellar catalogues from the Auriga cosmological simulations
• Peaks above the Maxwellian Sea: A New Approach to Finding Substructure in N-Body Haloes
• Probing non-spherical dark halos in the Galactic dwarf galaxies
• The effect of a disc on the population of cuspy and cored dark matter substructures in Milky Way-like galaxies
• The origin of pseudobulges in cosmological simulations of galaxy formation
• Variations in the width, density, and direction of the Palomar 5 tidal tails
• Examining The Fermi-LAT Third Source Catalog In Search Of Dark Matter Subhalos
• The Orbital Ellipticity of Satellite Galaxies and the Mass of the Milky Way
• Focusing on Warm Dark Matter with Lensed High-redshift Galaxies
• Knowing the unknowns: uncertainties in simple estimators of galactic dynamical masses
• Warm Dark Matter Constraints Using Milky-Way Satellite Observations and Subhalo Evolution Modeling
• Scaling relations of Fuzzy Dark Matter haloes I: individual systems in their cosmological environment
• The 21 cm signal and the interplay between dark matter annihilations and astrophysical processes
• Dark Matter signals from Draco and Willman 1: Prospects for MAGIC II and CTA
• 3FGL Demographics Outside the Galactic Plane using Supervised Machine Learning: Pulsar and Dark Matter Subhalo Interpretations
• Constraints on WIMP Annihilation for Contracted Dark Matter in the Inner Galaxy with the Fermi-LAT
• Testing the predictions of the cold dark matter model for the sizes, colours, morphologies and luminosities of galaxies with the SDSS
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).IX. The effects of ram pressure stripping down to the scale of individual HII regions in the dwarf galaxy IC 3476
• Probing the Epoch of Reionization with Milky Way Satellites
• Tidal disruption of globular clusters in dwarf galaxies with triaxial dark matter haloes
• Modeling the Impact of Baryons on Subhalo Populations with Machine Learning
• StarGO: A New Method to Identify the Galactic Origins of Halo Stars
• CLUMPY v3: $\gamma$-ray and $\nu$ signals from dark matter at all scales
• Rhapsody. I. Structural Properties and Formation History From a Statistical Sample of Re-simulated Cluster-size Halos
• Detecting Dark Matter Substructures around the Milky Way with Gaia
• The Satellite Luminosity Functions of Galaxies in SDSS
• The Velocity Dispersion Function of Very Massive Galaxy Clusters: Abell 2029 and Coma
• SURFS: Riding the waves with Synthetic UniveRses For Surveys
• The Birth and Growth of Neutralino Haloes
• Secondary Infall and the Pseudo-Phase-Space Density Profiles of Cold Dark Matter Halos
• The formation of shell galaxies similar to NGC 7600 in the cold dark matter cosmogony
• Six More Ultra-Faint Milky Way Companions Discovered in the DECam Local Volume Exploration Survey
• The Gamma-Ray-Flux Probability Distribution Function from Galactic Halo Substructure
• Local Group Dwarf Galaxies: Nature And Nurture
• The angular power spectrum of the diffuse gamma-ray emission as measured by the Fermi Large Area Telescope and constraints on its Dark Matter interpretation
• The Edge of the Galaxy
• Measuring Dark Matter Profiles Non-Parametrically in Dwarf Spheroidals: An Application to Draco
• Genetically modified halos: towards controlled experiments in $\Lambda$CDM galaxy formation
• Observability of Dark Matter Substructure with Pulsar Timing Correlations
• Multiple Chemodynamic Stellar Populations of the Ursa Minor Dwarf Spheroidal Galaxy
• External versus internal triggers of bar formation in cosmological zoom-in simulations
• Boosting the annihilation boost: Tidal effects on dark matter subhalos and consistent luminosity modeling
• Characterization of Dark-Matter-induced anisotropies in the diffuse gamma-ray background
• Constraints on the mass-concentration relation of cold dark matter halos with 11 strong gravitational lenses
• The prevalence of pseudo-bulges in the Auriga simulations
• A description of the Galactic Center excess in the Minimal Supersymmetric Standard Model
• Boötes IV: A New Milky Way Satellite Discovered in the Subaru Hyper Suprime-Cam Survey and Implications for the Missing Satellite Problem
• Tracing the first stars and galaxies of the Milky Way
• Introducing the LBT Imaging of Galactic Halos and Tidal Structures (LIGHTS) survey. A preview of the low surface brightness Universe to be unveiled by LSST
• SHARP - II. Mass structure in strong lenses is not necessarily dark matter substructure: A flux ratio anomaly from an edge-on disc
• Cosmology: small scale issues revisited
• Hydrogen Reionization in the Illustris universe
• The Dekel-Zhao profile: A mass-dependent dark-matter density profile with flexible inner slope and analytic potential, velocity dispersion, and lensing properties
• Inverted initial conditions: exploring the growth of cosmic structure and voids
• Bending Waves in the Milky Way's disc from halo substructure
• The impact of baryonic physics on the shape and radial alignment of substructures in cosmological dark matter haloes
• Using gaps in N-body tidal streams to probe missing satellites
• Double dark matter vision: twice the number of compact-source lenses with narrow-line lensing and the WFC3 grism
• The Baryons in the Milky Way Satellites
• T-ReX: a graph-based filament detection method
• Modelling galaxy clustering: Is new physics needed in galaxy formation models?
• Searching for diffuse light in the M96 Group
• Dynamical models for the Sculptor dwarf spheroidal in a Lambda CDM universe
• Under the Firelight: Stellar Tracers of the Local Dark Matter Velocity Distribution in the Milky Way
• PAMELA, DAMA, INTEGRAL and Signatures of Metastable Excited WIMPs
• Shallowed cusp slope of dark matter in disc galaxy formation through clump clusters
• Addressing the too big to fail problem with baryon physics and sterile neutrino dark matter
• Quantifying the Stellar Halo's Response to the LMC's Infall with Spherical Harmonics
• Warm dark matter signatures on the 21cm power spectrum: Intensity mapping forecasts for SKA
• A constraint on light primordial black holes from the interstellar medium temperature
• Robust identification of isotropic diffuse gamma rays from Galactic dark matter
• Self-interacting inelastic dark matter: A viable solution to the small scale structure problems
• On the Segregation of Dark Matter Substructure
• ColDICE: a parallel Vlasov-Poisson solver using moving adaptive simplicial tessellation
• Cosmological simulations of galaxy clusters with feedback from active galactic nuclei: profiles and scaling relations
• Subhalo Demographics in the Illustris Simulation: Effects of Baryons and Halo-to-Halo Variation
• An analytical model for the accretion of dark matter subhalos
• Substructure in the Most Massive GEEC Groups: Field-like Populations in Dynamically Active Groups
• Properties of Local Group galaxies in hydrodynamical simulations of sterile neutrino dark matter cosmologies
• Resolving Small-Scale Dark Matter Structures Using Multi-Source Indirect Detection
• A detailed study of Andromeda XIX, an extreme local analogue of ultra diffuse galaxies
• H.E.S.S. limits on line-like dark matter signatures in the 100 GeV to 2 TeV energy range close to the Galactic Centre
• The evolution of galaxy cluster X-ray scaling relations
• The Galactic Halo in Mixed Dark Matter Cosmologies
• Luminosity Functions and Host-to-Host Scatter of Dwarf Satellite Systems in the Local Volume
• A look to the inside of haloes: a characterisation of the halo shape as a function of overdensity in the Planck cosmology
• WIMP searches with gamma rays in the Fermi era: challenges, methods and results
• Probing the nature of dark matter with accreted globular cluster streams
• New Constraints on the Mass of Fermionic Dark Matter from Dwarf Spheroidal Galaxies
• Strong Dark Matter Self-interactions Diversify Halo Populations within and surrounding the Milky Way
• The Dynamics of Star Stream Gaps
• Modeling dark matter subhalos in a constrained galaxy: Global mass and boosted annihilation profiles
• Extragalactic gamma-ray background radiation from dark matter annihilation
• Dark matter substructure modelling and sensitivity of the Cherenkov Telescope Array to Galactic dark halos
• Probing Small-Scale Power Spectra with Pulsar Timing Arrays
• Nonlinear evolution of dark matter subhalos and applications to warm dark matter
• High-resolution spectroscopy of the GD-1 stellar stream localizes the perturber near the orbital plane of Sagittarius
• Bailing Out the Milky Way: Variation in the Properties of Massive Dwarfs Among Galaxy-Sized Systems
• A fresh look into the interacting dark matter scenario
• Structural and dynamical modeling of WINGS clusters. II. The orbital anisotropies of elliptical, spiral and lenticular galaxies
• Bars in hydrodynamical cosmological simulations
• Chemical evolution of Local Group dwarf galaxies in a cosmological context -- I. A new modelling approach and its application to the Sculptor dwarf spheroidal galaxy
• Galactic PeV neutrinos from dark matter annihilation
• Streams in the Aquarius stellar haloes
• An observer's guide to the (Local Group) dwarf galaxies: predictions for their own dwarf satellite populations
• Caustics in growing Cold Dark Matter Haloes
• Primordial dark matter halos from fifth forces
• Searching For Dark Matter Subhalos In the Fermi-LAT Second Source Catalog
• Black holes surrounded by generic matter distributions: polar perturbations and energy flux
• Estimating the Mass of the Milky Way Using the Ensemble of Classical Satellite Galaxies
• Structure Formation Models Weaken Limits on WIMP Dark Matter from Dwarf Spheroidal Galaxies
• Quantum fluctuations masquerade as halos: Bounds on ultra-light dark matter from quadruply-imaged quasars
• Detecting Gamma-Ray Anisotropies from Decaying Dark Matter: Prospects for Fermi LAT
• The stability of stellar disks in Milky-Way sized dark matter halos
• Impact of Dark Matter Velocity Distributions on Capture Rates in the Sun
• DASH: a library of dynamical subhalo evolution
• The shape of dark matter subhalos in the Aquarius simulations
• A new spin on disks of satellite galaxies
• A unified solution to the small scale problems of the $\Lambda$CDM model
• The structure and assembly history of cluster-size haloes in Self-Interacting Dark Matter
• The Main Sequences of Starforming Galaxies and Active Galactic Nuclei at High Redshift
• Dark matter in the classical dwarf spheroidal galaxies: a robust constraint on the astrophysical factor for gamma-ray flux calculations
• How well do cosmological simulations reproduce individual-halo properties?
• The signature of primordial black holes in the dark matter halos of galaxies
• Substructure Boosts to Dark Matter Annihilation from Sommerfeld Enhancement
• Universal properties of Dark Matter halos
• Enriching the hot circumgalactic medium
• Caught in the cosmic web: Environmental effect on halo concentrations, shape, and spin
• How Biased Are Halo Properties in Cosmological Simulations?
• Star Clusters Around Recoiled Black Holes in the Milky Way Halo
• A comparison of the distribution of satellite galaxies around Andromeda and the results of $\Lambda$CDM simulations
• Dark and luminous satellites of LMC-mass galaxies in the FIRE simulations
• The dynamics of satellite disruption in cold dark matter haloes
• Constraining dark matter annihilation with the isotropic $\gamma$-ray background: updated limits and future potential
• Sommerfeld-Enhanced $J$-Factors For Dwarf Spheroidal Galaxies
• Wino Dark Matter and Future dSph Observations
• Detection of Strong Epicyclic Density Spikes in the GD-1 Stellar Stream. An Absence of Evidence for the Influence of Dark Matter Subhalos?
• An Improved Model for the Dynamical Evolution of Dark Matter Subhaloes
• The impact of baryons on dark matter haloes
• Self-Similar Dynamical Relaxation of Dark Matter Halos in an Expanding Universe
• Constraints on dark matter annihilation by radio observations of M31
• Constraining resonant dark matter self-interactions with strong gravitational lenses
• The Photometric Metallicity and Carbon Distributions of the Milky Way's Halo and Solar Neighborhood from S-PLUS Observations of SDSS Stripe 82
• Constraints on Small-Scale Structures of Dark Matter from Flux Anomalies in Quasar Gravitational Lenses
• Wide-Field Hubble Space Telescope Observations of the Globular Cluster System in NGC1399
• Numerical convergence of hydrodynamical simulations of galaxy formation: the abundance and internal structure of galaxies and their cold dark matter haloes
• ATIC, PAMELA, HESS, Fermi and nearby Dark Matter subhalos
• The effect of baryons on the variance and the skewness of the mass distribution in the universe at small scales
• Dark matter subhaloes as gamma-ray sources and candidates in the first Fermi-LAT catalogue
• An evidence for indirect detection of dark matter from galaxy clusters in Fermi-LAT data
• Searching for the GD-1 Stream Progenitor in Gaia DR2 with Direct N-body Simulations
• Detecting the disruption of dark-matter halos with stellar streams
• Sustained super-Eddington accretion in high-redshift quasars
• The joint evolution of baryons and dark matter haloes
• Dust evolution in zoom-in cosmological simulations of galaxy formation
• The Dwarfs Beyond: The Stellar-to-Halo Mass Relation for a New Sample of Intermediate Redshift Low Mass Galaxies
• Diffuse gas properties and stellar metallicities in cosmological simulations of disc galaxy formation
• Radial Distributions of Dwarf Satellite Systems in the Local Volume
• The earliest stars and their relics in the Milky Way
• On the Power Spectrum of Dark Matter Substructure in Strong Gravitational Lenses
• The cosmic web of the Local Universe: cosmic variance, matter content and its relation to galaxy morphology
• A self-consistent phase-space distribution function for the anisotropic Dark Matter halo of the Milky Way
• Too small to succeed? Lighting up massive dark matter subhaloes of the Milky Way
• The origin and fate of the Gaia phase-space snail
• Weighing the Galactic disk using phase-space spirals II. Most stringent constraints to a thin dark disk using Gaia EDR3
• The little things matter: relating the abundance of ultrafaint satellites to the hosts' assembly history
• The Abundance and Structure of Subhaloes near the Free Streaming Scale and Their Impact on Indirect Dark Matter Searches
• Dark-matter decays and Milky Way satellite galaxies
• Search for Gamma-Ray Lines towards Galaxy Clusters with the Fermi-LAT
• A model explaining neutrino masses and the DAMPE cosmic ray electron excess
• Size matters: the non-universal density profile of subhaloes in SPH simulations and implications for the Milky Way's dSphs
• Update on decaying and annihilating heavy dark matter with the 6-year IceCube HESE data
• Fermi-LAT Observations of Gamma-Ray Emission Towards the Outer Halo of M31
• Dissipational versus Dissipationless Galaxy Formation and the Dark Matter Content of Galaxies
• Magnetogenesis around the first galaxies: the impact of different field seeding processes on galaxy formation
• Cold Dark Matter Substructures in Early-Type Galaxy Halos
• Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
• Gravitational lensing as a probe of cold dark matter subhalos
• Creating mock catalogues of stellar haloes from cosmological simulations
• What sets the central structure of dark matter haloes?
• Satellite Galaxy Number Density Profiles in the Sloan Digital Sky Survey
• Massive Milky Way Satellites in Cold and Warm Dark Matter: Dependence on Cosmology
• Gamma-ray boxes from axion-mediated dark matter
• Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
• Testing one-loop galaxy bias: Power spectrum
• The primordial matter power spectrum on sub-galactic scales
• Chemical enrichment in very low-metallicity environments: Bootes I
• The Effects of Patchy Reionization on Satellite Galaxies of the Milky Way
• Structure formation simulations with momentum exchange: alleviating tensions between high-redshift and low-redshift cosmological probes
• Deriving the velocity distribution of Galactic Dark Matter particles from rotation curve data
• Gamma-rays from dark matter annihilations strongly constrain the substructure in halos
• Observing dynamical friction in galaxy clusters
• Dark matter annihilation radiation in hydrodynamic simulations of Milky Way haloes
• Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations
• On the cross-section of Dark Matter using substructure infall into galaxy clusters
• A Dark Census: Statistically Detecting the Satellite Populations of Distant Galaxies
• Contamination of stellar-kinematic samples and uncertainty about dark matter annihilation profiles in ultrafaint dwarf galaxies: the example of Segue I
• Novel Gamma-ray Spectral Features in the Inert Doublet Model
• CFHTLenS: The Environmental Dependence of Galaxy Halo Masses from Weak Lensing
• TDCOSMO III: Dark matter substructure meets dark energy -- the effects of (sub)halos on strong-lensing measurements of $H_0$
• Galactic synchrotron emission from WIMPs at radio frequencies
• SHARP - I. A high-resolution multi-band view of the infra-red Einstein ring of JVAS B1938+666
• Annihilation vs. Decay: Constraining dark matter properties from a gamma-ray detection
• Multipole analysis of IceCube data to search for dark matter accumulated in the Galactic halo
• A Halo Expansion (HEX) Technique for Approximating Simulated Dark Matter Haloes
• Renegade Subhaloes in the Local Group
• Galaxy Clusters as Reservoirs of Heavy Dark Matter and High-Energy Cosmic Rays: Constraints from Neutrino Observations
• First Galaxy-Galaxy Lensing Measurement of Satellite Halo Mass in the CFHT Stripe-82 Survey
• Realistic estimation for the detectability of dark matter sub-halos with Fermi-LAT
• The Smith Cloud: high-velocity accretion and dark-matter confinement
• Were progenitors of local L* galaxies Lyman-alpha emitters at high redshift?
• The probability of galaxy-galaxy strong lensing events in hydrodynamical simulations of galaxy clusters
• Warm dark matter and the ionization history of the Universe
• Dissecting the Gamma-Ray Background in Search of Dark Matter
• On the stark difference in satellite distributions around the Milky Way and Andromeda
• The Cosmic Abundance of Classical Milky Way Satellites
• Subhalo statistics of galactic halos: beyond the resolution limit
• Subhaloes gone Notts: Spin across subhaloes and finders
• The cosmic X-ray and gamma-ray background from dark matter annihilation
• Deep spectroscopic luminosity function of Abell 85: no evidence for a steep upturn of the faint-end slope
• Substructure Lensing: Effects of Galaxies, Globular Clusters & Satellite Streams
• Dynamical Evolution of Primordial Dark Matter Haloes through Mergers
• Dark Matter in the Local Universe
• The Clustering of Orbital Poles Induced by the LMC: Hints for the Origin of Planes of Satellites
• Astrometric Microlensing by Local Dark Matter Subhalos
• Galaxy formation with radiative and chemical feedback
• Deadly dark matter cusps vs faint and extended star clusters: Eridanus II and Andromeda XXV
• gamma-rays from annihilating dark matter in galaxy clusters: stacking vs single source analysis
• Impact of filaments on galaxy formation in their residing dark matter haloes
• Comprehensive Assessment of the Too-Big-to-Fail Problem
• Simulating Momentum Exchange in the Dark Sector
• Galactic Tides and the Shape and Orientation of Dwarf Galaxy Satellites
• A black hole window into p-wave dark matter annihilation
• Fitting functions for dark matter density profiles
• The diverse formation histories of simulated disc galaxies
• Dark Matter Interpretation of the Fermi-LAT Observations Toward the Outer Halo of M31
• Direct Detection of Dark Matter Substructure in Strong Lens Images with Convolutional Neural Networks
• Early chemo-dynamical evolution of dwarf galaxies deduced from enrichment of r-process elements
• On the common mass scale of the Milky Way satellites
• Galactic Center Radio Constraints on Gamma-Ray Lines from Dark Matter Annihilation
• Ultra-Compact High Velocity Clouds as Minihalos and Dwarf Galaxies
• The galaxy-subhalo connection in low-redshift galaxy clusters from weak gravitational lensing
• The star formation histories of dwarf galaxies in Local Group cosmological simulations
• Neutrinos in IceCube/KM3NeT as probes of Dark Matter Substructures in Galaxy Clusters
• The Redshift-Space Momentum Power Spectrum I: Optimal Estimation From Peculiar Velocity Surveys
• The modified gravity lightcone simulation project I: Statistics of matter and halo distributions
• The SEGUE K Giant Survey. III. Quantifying Galactic Halo Substructure
• Measuring subhalo mass in redMaPPer clusters with CFHT Stripe 82 Survey
• Measuring the slopes of mass profiles for dwarf spheroidals in triaxial CDM potentials
• The phase-space structure of tidally stripped halos
• Pre-processing, group accretion and the orbital trajectories of associated subhaloes
• Asymmetric Surface Brightness Structure of Caustic Crossing Arc in SDSS J1226+2152: A Case for Dark Matter Substructure
• Ring Galaxies in the EAGLE Hydrodynamical Simulations
• Corrective effect of many-body interactions in dynamical friction
• The Fermi Gamma-Ray Haze from Dark Matter Annihilations and Anisotropic Diffusion
• Modeling the gravitational potential of a cosmological dark matter halo with stellar streams
• Probing the small-scale structure in strongly lensed systems via transdimensional inference
• First Results on Dark Matter Substructure from Astrometric Weak Lensing
• The halo mass function in interacting Dark Energy models
• The history of the dark and luminous side of Milky Way-like progenitors
• Origins of sharp cosmic-ray electron structures and the DAMPE excess
• Stellar Wakes from Dark Matter Subhalos
• Impact of cosmological satellites on the vertical heating of the Milky Way disc
• A unified solution to the small scale problems of the $\Lambda$CDM model II: introducing parent-satellite interaction
• The Pristine Dwarf-Galaxy survey -- IV. Probing the outskirts of the dwarf galaxy Boötes I
• Towards a general parametrization of the warm dark matter halo mass function
• Sensitivity of the Cherenkov Telescope Array to the detection of a dark matter signal in comparison to direct detection and collider experiments
• Streams Going Notts: The tidal debris finder comparison project
• Properties of fossil groups in cosmological simulations and galaxy formation models
• Simulating tidal streams in a high resolution dark matter halo
• Structure and substructure analysis of DAFT/FADA galaxy clusters in the [0.4-0.9] redshift range
• The Dark Matter Annihilation Signal from Dwarf Galaxies and Subhalos
• Pseudo-Nambu-Goldstone dark matter and two-Higgs-doublet models
• Structure formation in a $\Lambda$ $viscous$ CDM universe
• Beyond subhalos: Probing the collective effect of the Universe's small-scale structure with gravitational lensing
• Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency
• Search for $\gamma$-ray emission from dark matter particle interactions from Andromeda and Triangulum Galaxies with the Fermi Large Area Telescope
• Extragalactic gamma-ray signal from Dark Matter annihilation: a power spectrum based computation
• The Smith Cloud and its dark matter halo: Survival of a Galactic disc passage
• Stellar Disks in Aquarius Dark Matter Haloes
• Constraining the primordial magnetic field with dwarf galaxy simulations
• The Effects of Dark Matter and Baryonic Physics on the Milky Way Subhalo Population in the Presence of the Large Magellanic Cloud
• Cosmology with Stacked Cluster Weak Lensing and Cluster-Galaxy Cross-Correlations
• Yule-Simpson's paradox in Galactic Archaeology
• LCDM halo substructure properties revealed with high resolution and large volume cosmological simulations
• The effects of AGN feedback on the structural and dynamical properties of Milky Way-mass galaxies in cosmological simulations
• A robust mass estimator for dark matter subhalo perturbations in strong gravitational lenses
• Bound and unbound substructures in Galaxy-scale Dark Matter haloes
• The Pristine Dwarf-Galaxy survey -- III. Revealing the nature of the Milky Way globular cluster Sagittarius II
• Density Variations in the NW Star Stream of M31
• The Milky Way system in LCDM cosmological simulations
• On the sensitivity of CTA to gamma-ray boxes from multi-TeV dark matter
• Hubble Space Telescope Observations of Two Faint Dwarf Satellites of Nearby LMC Analogs from MADCASH
• Explaining the DAMPE data with scalar dark matter and gauged $U(1{)}_{L_e-L_{\mu }}$ interaction
• Scalar dark matter interpretation of the DAMPE data with U(1) gauge interactions
• Variation of the subhalo abundance in dark matter halos
• Quantifying the Line-of-Sight Halo Contribution to the Dark Matter Convergence Power Spectrum from Strong Gravitational Lenses
• Confronting Galactic and Extragalactic $\gamma$-ray observed by Fermi-LAT with Annihilating Dark Matter in Inert Higgs Doublet Model
• Unidentified Gamma-ray Sources as Targets for Indirect Dark Matter Detection with the Fermi-Large Area Telescope
• Globular Clusters Formed within Dark Halos I: present-day abundance, distribution and kinematics
• Is The Gamma-Ray Source 3FGL J2212.5+0703 A Dark Matter Subhalo?
• Sensitivity of strong lensing observations to dark matter substructure: a case study with Euclid
• On the effect of galactic outflows in cosmological simulations of disc galaxies
• Probing sub-galactic mass structure with the power spectrum of surface-brightness anomalies in high-resolution observations of galaxy-galaxy strong gravitational lenses. II.Observational constraints on the sub-galactic matter power spectrum
• Self-Similar Spherical Collapse with Tidal Torque
• Decaying dark matter: a stacking analysis of galaxy clusters to improve on current limits
• Reproducing cosmic evolution of galaxy population from $z=4$ to $0$
• Tidal Stripping in the Adiabatic Limit
• First constraints on Fuzzy Dark Matter from the dynamics of stellar streams in the Milky Way
• Spatial and luminosity distributions of galactic satellites
• Multiple Dark Matter as a self-regulating mechanism for dark sector interactions
• Cosmological Radio Emission induced by WIMP Dark Matter
• Constraining the Sommerfeld enhancement with Cherenkov telescope observations of dwarf galaxies
• Spectral and spatial analysis of the dark matter subhalo candidates among Fermi Large Area Telescope unidentified sources
• Stochastic angular momentum slews and flips and their effect on discs in galaxy formation models
• Satellite galaxies in hydrodynamical simulations of Milky Way sized galaxies
• Charting Unexplored Dwarf Galaxy Territory With RR Lyrae
• Satellites of Satellites: The Case for Carina and Fornax
• Influence of baryons on the orbital structure of dark matter haloes
• Internal Alignments of Red Versus Blue Discs in Dark Matter Halos
• Dark satellites and the morphology of dwarf galaxies
• Gamma rays from the Galactic Centre region: a review
• Galaxy subgroups in galaxy clusters
• And In The Darkness Unbind Them: High-Resolution Simulations of Dark Matter Subhalo Disruption in a Milky Way-like Tidal Field
• Cosmological searches for a non-cold dark matter component
• Gamma Rays From Dark Matter Subhalos Revisited: Refining the Predictions and Constraints
• Signatures of clumpy dark matter in the global 21 cm background signal
• Convergence of Galaxy Properties with Merger Tree Temporal Resolution
• Intermediate Mass Black Holes and Nearby Dark Matter Point Sources: A Critical Reassessment
• Gamma rays and neutrinos from dark matter annihilation in galaxy clusters
• A general framework to test gravity using galaxy clusters II: A universal model for the halo concentration in $f(R)$ gravity
• MaGICC-WDM: the effects of warm dark matter in hydrodynamical simulations of disc galaxy formation
• Modeling GD-1 Gaps in a Milky-Way Potential
• Modeling Evolution of Galactic Bars at Cosmic Dawn
• Non-universality of dark-matter halos: cusps, cores, and the central potential
• Solar WIMPs Unraveled: Experiments, astrophysical uncertainties, and interactive Tools
• Estimating the warm dark matter mass from strong lensing images with truncated marginal neural ratio estimation
• Gravitational Lensing - Einstein's Unfinished Symphony
• Adaptive Optics Observations of B0128+437: A Low-Mass, High-Redshift Gravitational Lens
• Coy Dark Matter and the anomalous magnetic moment
• Dispersal of tidal debris in a Milky-Way-sized dark matter halo
• Is NGC 5824 the Core of the Progenitor of the Cetus Stream?
• Constraining the inner density slope of massive galaxy clusters
• The effects of LMC-mass environments on their dwarf satellite galaxies in the FIRE simulations
• Under the sword of Damocles: plausible regeneration of dark matter cusps at the smallest galactic scales
• Gravitational redshift and asymmetric redshift-space distortions for stacked clusters
• Constraints on dark matter-neutrino scattering from the Milky-Way satellites and subhalo modeling for dark acoustic oscillations
• Re-ionizing the Universe without Stars
• Near-Infrared K and L' Flux Ratios in Six Lensed Quasars
• Extragalactic gamma-ray signal from dark matter annihilation: an appraisal
• Extracting the Subhalo Mass Function from Strong Lens Images with Image Segmentation
• Impact of AGN feedback on galaxies and their multiphase ISM across cosmic time
• Imprints of Chameleon f(R) Gravity on Galaxy Rotation Curves
• Globular Cluster Formation from Colliding Substructure
• Effects of galaxy--satellite interactions on bar formation
• Euclid preparation. XXXII. Evaluating the weak lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
• Constraining Dark Matter in Galactic Substructure
• Galaxy Pairs in the Local Group
• The spatial distribution of Milky Way satellites, gaps in streams and the nature of dark matter
• SatGen -- II. Assessing the impact of a disc potential on subhalo populations
• Towards constraining warm dark matter with stellar streams through neural simulation-based inference
• Velocity Dispersion of the GD-1 Stellar Stream
• The SAGA Survey. IV. The Star Formation Properties of 101 Satellite Systems around Milky Way-mass Galaxies
• Image segmentation for analyzing galaxy-galaxy strong lensing systems
• Possibility of the Traversable Wormholes in the Galactic Halos within $4D$ Einstein-Gauss-Bonnet Gravity
• The orbital PDF: general inference of the gravitational potential from steady-state tracers
• Non-universality of halo profiles and implications for dark matter experiments
• Constraining the substructure of dark matter haloes with galaxy-galaxy lensing
• Dissecting Galaxy Formation: II. Comparing Substructure in Pure Dark Matter and Baryonic Models
• On Physical Scales of Dark Matter Halos
• Measuring the vertical response of the Galactic disc to an infalling satellite
• Multi-messenger constraints on the annihilating dark matter interpretation of the positron excess
• Dark matter detection in the BMSSM
• Chemical evolution of disc galaxies from cosmological simulations
• The Three Hundred Project: Substructure in hydrodynamical and dark matter simulations of galaxy groups around clusters
• Spurious Small-Scale Structure & Discreteness-Driven Relaxation in Cosmological Simulations
• A Two-Point Correlation Function For Galactic Halo Stars
• The physical drivers of gas turbulence in simulated disc galaxies
• The lensing properties of subhaloes in massive elliptical galaxies in sterile neutrino cosmologies
• Anisotropies in the Diffuse Gamma-Ray Background from Dark Matter with Fermi LAT: a closer look
• Probing the galaxy-halo connection with total satellite luminosity
• Constraining the dark matter contribution of $\gamma$ rays in Cluster of galaxies using Fermi-LAT data
• The Effects of Varying Cosmological Parameters on Halo Substructure
• Reionization in the Warm Dark Matter Model
• Prompt cusps and the dark matter annihilation signal
• Self-interacting freeze-in dark matter in a singlet doublet scenario
• The Massive Satellite Population of Milky-Way Sized Galaxies
• Astrophysical and cosmological probes of dark matter
• Confronting the Moduli-Induced LSP Problem
• Baryonic effects on the detectability of annihilation radiation from dark matter subhaloes around the Milky Way
• Diffuse gamma-ray constraints on dark matter revisited. I: the impact of subhalos
• On the starting redshift for cosmological simulations: Focusing on halo properties
• Cosmological Simulations of Dwarf Galaxies with Cosmic Ray Feedback
• Cosmic evolution of bars in simulations of galaxy formation
• The Next Generation Virgo Cluster Survey. IX. Estimating the Efficiency of Galaxy Formation on the Lowest-Mass Scales
• Is the Dark Disc contribution to Dark Matter Signals important ?
• Biases and systematics in the observational derivation of galaxy properties: comparing different techniques on synthetic observations of simulated galaxies
• The Einasto model for dark matter haloes
• The galaxy population in cold and warm dark matter cosmologies
• Characterizing dark interactions with the halo mass accretion history and structural properties
• Euclid: Modelling massive neutrinos in cosmology -- a code comparison
• Dark Matter in Astrophysics/Cosmology
• The Power of Halometry
• Kinematics of the Tucana Dwarf Galaxy: An Unusually Dense Dwarf in the Local Group
• Endothermic self-interacting dark matter in Milky Way-like dark matter haloes
• On the relevance of chaos for halo stars in the Solar Neighbourhood
• Constraints on the dark matter annihilation from Fermi-LAT observation of M31
• Is ram-pressure stripping an efficient mechanism to remove gas in galaxies?
• The 130 GeV gamma-ray line and generic dark matter model building constraints from continuum gamma rays, radio and antiproton data
• The orbital PDF: the dynamical state of Milky Way sized haloes and the intrinsic uncertainty in the determination of their masses
• Constraints via the Event Horizon Telescope for Black Hole Solutions with Dark Matter under the Generalized Uncertainty Principle Minimal Length Scale Effect
• Cluster Mergers and the Origin of the ARCADE-2 Excess
• Hitting the Bull's-eye: The Radial Profile of Accretion and Star Formation in the Milky Way
• Subhaloes in Scale-Free Cosmologies
• The evolution of streams in a time-dependent potential
• The Missing Satellite Problem Outside of the Local Group: I -- Pilot Observation
• New evidence for dark matter
• The halo mass function and inner structure of ETHOS haloes at high redshift
• Gravitationally Bound Bose Condensates with Rotation
• The impact of inelastic self-interacting dark matter on the dark matter structure of a Milky Way halo
• The Effects of Halo-to-Halo Variation on Substructure Lensing
• The connection between the host halo and the satellite galaxies of the Milky Way
• The Morphology of the Galactic Dark Matter Synchrotron Emission with Self-Consistent Cosmic Ray Diffusion Models
• Velocity-dependent J-factors for annihilation radiation from cosmological simulations
• Interaction between dark matter sub-halos & galactic gaseous disk
• Dust evolution with MUPPI in cosmological volumes
• Dark impact and galactic star formation: Origin of the Gould belt
• Preprocessing, mass loss and mass segregation of galaxies in DM simulations
• A new calibration method of sub-halo orbital evolution for semi-analytic models
• Leptons from Dark Matter Annihilation in Milky Way Subhalos
• Galaxy Formation in Sterile Neutrino Dark Matter Models
• Satellite mass functions and the faint end of the galaxy mass-halo mass relation in LCDM
• Systematic errors in strong gravitational lensing reconstructions, a numerical simulation perspective
• Milky Way-est: Cosmological Zoom-in Simulations with Large Magellanic Cloud and Gaia-Sausage-Enceladus Analogs
• Cosmic Reionization On Computers: Numerical and Physical Convergence
• Quantifying the power spectrum of small-scale structure in semi-analytic galaxies
• A general framework to test gravity using galaxy clusters IV: Cluster and halo properties in DGP gravity
• Molecular Chemistry for Dark Matter II: Recombination, Molecule Formation, and Halo Mass Function in Atomic Dark Matter
• Satellite Survival in Highly Resolved Milky Way Class Halos
• Prompt cusp formation from the gravitational collapse of peaks in the initial cosmological density field
• Redshift evolution of the dark matter haloes shapes
• Amplitude and phase fluctuations of gravitational waves magnified by strong gravitational lensing
• Redshift evolution of stellar mass versus gas fraction relation in 0<z<2 regime: observational constraint for galaxy formation models
• ZOMG III: The effect of Halo Assembly on the Satellite Population
• Running with BICEP2: Implications for Small-Scale Problems in CDM
• Zoomed cosmological simulations of Milky Way sized halos in f(R)-gravity
• Fluctuations of the gravitational field generated by a random population of extended substructures
• Astrophysical Tests of Dark Matter Self-Interactions
• Vlasov versus N-body: the Hénon sphere
• On the Origin of Flux Ratio Anomaly in Quadruple Lens Systems
• Constraining the Milky Way assembly history with Galactic Archaeology. Ludwig Biermann Award Lecture 2015
• The Normalization and Slope of the Dark Matter (Sub-)Halo Mass Function on Sub-Galactic Scales
• The impact of $\Lambda$CDM substructure and baryon-dark matter transition on the image positions of quad galaxy lenses
• Dense Dark Matter Hairs Spreading Out from Earth, Jupiter and Other Compact Bodies
• Is the Universe Simpler than LCDM?
• Higgs-portal Scalar Dark Matter: Scattering Cross Section and Observable Limits
• Stochastic tidal heating by random interactions with extended substructures
• Numerical hydrodynamic simulations based on semi-analytic galaxy merger trees: method and Milky-Way like galaxies
• The detection of sub-solar mass dark matter halos
• Entering the Era of Dark Matter Astronomy? Near to Long-Term Forecasts in X-Ray and Gamma-Ray Bands
• The substructures in the local stellar halo from Gaia and LAMOST
• Angular distribution of gamma-ray emission from velocity-dependent dark matter annihilation in subhalos
• Planes of satellites around simulated disc galaxies: I.- Finding high-quality planar configurations from positional information and their comparison to MW/M31 data
• Comparing galactic satellite properties in hydrodynamical and Nbody simulations
• Enhanced star formation in $z\sim 6$ quasar companions
• Annihilating Dark Matter Search with 12 Years of Fermi LAT Data in Nearby Galaxy Clusters
• Black hole spin evolution in warped accretion discs
• Tidal evolution of cored and cuspy dark matter halos
• Practical Cosmology with Lenses
• Clustering in the Phase Space of Dark Matter Haloes. II. Stable Clustering and Dark Matter Annihilation
• Cold accretion in early galaxy formation and its Lyman-alpha signatures
• Improving the Sensitivity of Gamma-Ray Telescopes to Dark Matter Annihilation in Dwarf Spheroidal Galaxies
• Sussing Merger Trees: Stability and Convergence
• The cusp-core problem in gas-poor dwarf spheroidal galaxies
• The low abundance and insignificance of dark discs in simulated Milky Way galaxies
• Are Lines From Unassociated Gamma-Ray Sources Evidence For Dark Matter Annihilation?
• Subhaloes gone Notts: Subhaloes as tracers of the dark matter halo shape
• The galaxy correlation function as a constraint on galaxy formation physics
• Exploring extensions to the standard cosmological model and the impact of baryons on small scales
• The AGORA High-resolution Galaxy Simulations Comparison Project. V: Satellite Galaxy Populations In A Cosmological Zoom-in Simulation of A Milky Way-mass Halo
• What to expect from dynamical modelling of galactic haloes
• Novel Adaptive softening for collisionless N-body simulations: Eliminating spurious halos
• Galactic-Centre Gamma Rays in CMSSM Dark Matter Scenarios
• On the correlation between the local dark matter and stellar velocities
• Estimating the Milky Way's Mass via Hierarchical Bayes: A Blind Test on MUGS2 Simulated Galaxies
• Subhaloes gone Notts: the clustering properties of subhaloes
• Milky Way archaeology using RR Lyrae and type II Cepheids I. The Orphan stream in 7D using RR Lyrae stars
• Cosmic ray $e^{+}{e}^{-}$ spectrum excess and peak feature observed by the DAMPE experiment from dark matter
• Massive galaxy formation caught in action at z~5 with JWST
• On the Flaring of Thick Disc of Galaxies: Insights from Simulations
• The Milky Way and Andromeda galaxies in a constrained hydrodynamical simulation: morphological evolution
• Re-Examining Astrophysical Constraints on the Dark Matter Model
• Universal clustering of dark matter in phase space
• A search for dark matter in Triangulum II with the MAGIC telescopes
• Tidal stirring of satellites with shallow density profiles prevents them from being too big to fail
• A high-resolution cosmological simulation of a strong gravitational lens
• Assembly history of subhalo populations in galactic and cluster sized dark haloes
• Seeking Observable Imprints of Small-Scale Structure on the Properties of Dark Matter Haloes
• Dark matter capture by the Sun: revisiting velocity distribution uncertainties
• Hunting for dark halo substructure using submilliarcsecond-scale observations of macrolensed radio jets
• Predictions for the detection of Tidal Streams with Gaia using Great Circle Methods
• Metallicity and Kinematics of the Galactic halo from the LAMOST sample stars
• A panoramic view of the Local Group dwarf galaxy NGC 6822
• Dark matter halos in the multicomponent model. I. Substructure
• The SELGIFS data challenge: generating synthetic observations of CALIFA galaxies from hydrodynamical simulations
• The mass loss process in dwarf galaxies from 3D hydrodynamical simulations: the role of dark matter and starbursts
• Dark Matter: The evidence from astronomy, astrophysics and cosmology
• The Proper Motion of Pyxis: the first use of Adaptive Optics in tandem with HST on a faint halo object
• The dark side of FIRE: predicting the population of dark matter subhaloes around Milky Way-mass galaxies
• Dark Matter implications of Fermi-LAT measurement of anisotropies in the diffuse gamma-ray background
• $\gamma$-ray and $\nu$ searches for dark matter subhalos in the Milky Way with a baryonic potential
• Physical properties of galaxies: toward a consistent comparison between hydrodynamical simulations and SDSS
• Cold versus Warm Dark Matter simulations of a galaxy group
• Quantifying tidal stream disruption in a simulated Milky Way
• Dark Matter Response to Galaxy Assembly History
• Orbital distribution of infalling satellite halos across cosmic time
• The Effect of Environment on Milky Way-mass galaxies in a Constrained Simulation of the Local Group
• Real and counterfeit cores: how feedback expands halos and disrupts tracers of inner gravitational potential in dwarf galaxies
• Subhalo sinking and off-center massive black holes in dwarf galaxies
• Modified Dark Matter: Relating Dark Energy, Dark Matter and Baryonic Matter
• Dark influences: imprints of dark satellites on dwarf galaxies
• Comparing semi-analytic particle tagging and hydrodynamical simulations of the Milky Way's stellar halo
• The baryon cycle of Seven Dwarfs with superbubble feedback
• Informing dark matter direct detection limits with the ARTEMIS simulations
• Noiseless Gravitational Lensing Simulations
• Local Group star formation in warm and self-interacting dark matter cosmologies
• Gamma-ray anisotropies from dark matter in the Milky Way: the role of the radial distribution
• The MIP Ensemble Simulation: Local Ensemble Statistics in the Cosmic Web
• Dark Matter Halos from the Inside Out
• Non-linear gravitational clustering of cold matter in an expanding universe: indications from 1D toy models
• Evidence for Substructure in Ursa Minor Dwarf Spheroidal Galaxy using a Bayesian Object Detection Method
• MeTACAST: Target- and Context-aware Spatial Selection in VR
• Constraining Dark Matter Properties with Gamma-Rays from the Galactic Center with Fermi-LAT
• Non-isotropic feedback from accreting spinning black holes
• Searching for Dark Matter Annihilation in the Smith High-Velocity Cloud
• Origin of Non-axisymmetric Features of Virgo Cluster Early-type Dwarf Galaxies. I. Bar Formation and Recurrent Buckling
• Primordial Black Hole as a Source of the Boost Factor
• Dark matter protohalos in MSSM-9 and implications for direct and indirect detection
• Modeling globular clusters in the TNG50 simulation: predictions from dwarfs to giants
• Gamma-ray signatures of annihilation to charged leptons in dark matter substructure
• Remnants of Galactic subhalos and their impact on indirect dark matter searches
• Strong lensing constraints on primordial black holes as a dark matter candidate
• Dark-ages Reionization and Galaxy Formation Simulation - XIII. AGN quenching of high-redshift star formation in ZF-COSMOS-20115
• On the relevance of chaos for halo stars in the solar neighbourhood II
• Faint Satellite Population of the NGC-3175 Group - a Local Group Analogue
• Cosmic explosions, life in the Universe and the Cosmological Constant
• Stellar Spiral Structures in Triaxial Dark Matter Haloes
• Structure formation in a mixed dark matter model with decaying sterile neutrino: the 3.5 keV X-ray line and the Galactic substructure
• Fluctuations in strongly coupled cosmologies
• Dissecting galaxy formation models with Sensitivity Analysis -- A new approach to constrain the Milky Way formation history
• Constraints on dark matter annihilation and decay from the large-scale structure of the nearby universe
• TeV Dark Matter Searches in the Extragalactic Gamma-Ray Sky
• Evolution of subhalo orbits in a smoothly-growing host halo potential
• Constraints on the Galactic Inner Halo Assembly History from the Age Gradient of Blue Horizontal-branch Stars
• A Redshift Survey of the Nearby Galaxy Cluster Abell 2199: Comparison of the Spatial and Kinematic Distributions of Galaxies with the Intracluster Medium
• The Smith Cloud: surviving a high speed transit of the Galactic disc
• Dark energy from dark radiation in strongly coupled cosmologies with no fine tuning
• Shape and kinematics of elliptical galaxies: evolution due to merging at z < 1.5
• A new fitting-function to describe the time evolution of a galaxy's gravitational potential
• Dark matter electron anisotropy: a universal upper limit
• Decoding Dark Matter Substructure without Supervision
• The potential role of NGC 205 in generating Andromeda's vast thin co-rotating plane of satellite galaxies
• Cosmic Flow Measurement and Mock Sampling Algorithm of Cosmicflows-4 Tully-Fisher Catalogue
• Investigating the detection of dark matter subhalos as extended sources with Fermi-LAT
• A random-walk model for dark matter halo spins
• Calibration of a star formation and feedback model for cosmological simulations with Enzo
• SpatialTouch: Exploring Spatial Data Visualizations in Cross-reality
• Hydrodynamical simulations of coupled and uncoupled quintessence models II: Galaxy clusters
• Small scale structures in coupled scalar field dark matter
• Shedding light on low-mass subhalo survival and annihilation luminosity with numerical simulations
• The Milky Way, Coming into Focus: Precision Astrometry Probes its Evolution, and its Dark Matter
• A Merger Tree with Microsolar Mass Resolution: Application to $\gamma$-ray Emission from Subhalo Population
• COZMIC. I. Cosmological Zoom-in Simulations with Initial Conditions Beyond Cold Dark Matter
• The effect of secular galactic growth on the evolution of star clusters
• On the effect of angular momentum on the prompt cusp formation via the gravitational collapse
• Statistical properties of dark matter mini-haloes at z >= 15
• On self-gravitating strange dark matter halos around galaxies
• Extragalactic diffuse gamma-rays from dark matter annihilation: revised prediction and full modelling uncertainties
• Pantheon+ constraints on dark energy and modified gravity: An evidence of dynamical dark energy
• A decade of dark matter searches with ground-based Cherenkov telescopes
• Discovery of a thin stellar stream in the SLAMS survey
• Formation of proto-globular cluster candidates in cosmological simulations of dwarf galaxies at $z>4$
• Constraining the Milky Way Dark Matter Density Profile with Gamma-Rays with Fermi-LAT
• The Escape Velocity Profile of the Milky Way from Gaia DR3
• Sensitivity of the Cherenkov Telescope Array to dark subhalos
• Not All Subhaloes Are Created Equal: Modelling the Diversity of Subhalo Density Profiles in TNG50
• Impact of substructure on local dark matter searches
• Probing cold dark matter subhalos with simulated ALMA observations of macrolensed sub-mm galaxies
• Micro galaxies in LCDM
• The prolate dark matter halo of the Andromeda galaxy
• Chemo-dynamical simulations of dwarf galaxy evolution
• The effect of dark matter resolution on the collapse of baryons in high redshift numerical simulations
• Galactic diffuse gamma rays --- recalculation based on the new measurements of cosmic electron spectrum
• A halo of trapped interstellar matter surrounding the solar system
• Testing the Dark Matter Annihilation Model for the WMAP Haze
• Search for Dark Matter Gamma-ray Emission from the Andromeda Galaxy with the High-Altitude Water Cherenkov Observatory
• Characterising the Structure of Halo Merger Trees Using a Single Parameter: The Tree Entropy
• Dark Matter search in dwarf irregular galaxies with the Fermi Large Area Telescope
• Gamma-ray sensitivity to dark matter subhalo modelling at high latitudes
• Particle tagging and its implications for stellar population dynamics
• A titanic interstellar medium ejection from a massive starburst galaxy at redshift 1.4
• 3FGL J1924.8-1034 : A Spatially-Extended Stable Unidentified GeV Source?
• Dark Matter Studies Entrain Nuclear Physics
• Properties and observables of massive galaxies in self-interacting dark matter cosmologies
• Simulated evolution of the dark matter large-scale structure
• Satellites in the field and lens galaxies: SDSS/COSMOS vs. SLACS/CLASS
• Search for dark matter annihilation signals from unidentified Fermi-LAT objects with H.E.S.S
• Illuminating the Darkest Galaxies
• Galaxy And Mass Assembly (GAMA): The absence of stellar mass segregation in galaxy groups and consistent predictions from GALFORM and EAGLE simulations
• Star forming filaments in warm dark matter models
• Robustness of the Galactic Center Excess Morphology Against Masking
• The Luminosity Functions and Redshift Evolution of Satellites of Low-Mass Galaxies in the COSMOS Survey
• A million-solar-mass object detected at cosmological distance using gravitational imaging
• What kind of science is cosmology?
• Future sensitivity of neutrino telescopes to dark matter annihilations from the cosmic diffuse neutrino signal
• Culminating the peak CUSP to descry the dark side of halos
• Search for gamma-ray line signals around the black hole at the galactic center with DAMPE observation
• Clumpiness enhancement of charged cosmic rays from dark matter annihilation with Sommerfeld effect
• Mass assembly history and infall time of the Fornax dwarf spheroidal galaxy
• Dark matter substructure cannot explain properties of the Fermi Galactic Centre excess
• Impact of H${}_2$-driven star formation and stellar feedback from low-enrichment environments on the formation of spiral galaxies
• Prospects for Detecting Gamma Rays from Annihilating Dark Matter in Dwarf Galaxies in the Era of DES and LSST
• An Accurate Comprehensive Approach to Substructure: I. Accreted Subhaloes
• The Anisotropy of the Extragalactic Radio Background from Dark Matter Annihilation
• Boosting small-scale structure via primordial black holes and implications for sub-GeV dark matter annihilation
• Fuzzy Aquarius: evolution of a Milky-way like system in the Fuzzy Dark Matter scenario
• Enhanced n-body annihilation of dark matter and its indirect signatures
• Dark Matter Subhalos in the Ursa Minor Dwarf Galaxy
• Gas accretion in Milky Way-like galaxies: temporal and radial dependencies
• On $N$-body simulations of globular cluster stream
• Neutron star mass in dark matter clumps
• Selecting ultra-faint dwarf candidate progenitors in cosmological N-body simulations at high redshifts
• Cosmological implications of a Dark Matter self-interaction energy density
• Ironing the folds: The phase space chevrons of a GSE-like merger as a dark matter subhalo detector
• Searching for Dark Matter Sub-structure with HAWC
• Disentangling cosmic-ray and dark-matter induced gamma-rays in galaxy clusters?
• Matching the mass function of Milky Way satellites in competing dark matter models
• Dwarf Galaxy Sized Monopoles as Dark Matter?
• The Bosma effect revisited - I. HI and stellar disc scaling models
• The cosmology dependence of the concentration-mass-redshift relation
• Gravitational microlensing as a probe for dark matter clumps
• The dark matter content of the blue compact dwarf NGC 2915
• Novel Conservative Methods for Adaptive Force Softening in Collisionless and Multi-Species N-Body Simulations
• Drivers of asymmetry in synthetic H I emission-line profiles of galaxies in the EAGLE simulation
• Modeling Photoionized Turbulent Material in the Circumgalactic Medium II: Effect of Turbulence within a Stratified Medium
• A solution to the problems of cusps and rotation curves in dark matter halos in the cosmological standard model
• A Clustering Analysis of the Morphology of the 130 GeV Gamma-Ray Feature
• Testing the dark matter subhalo hypothesis of the gamma-ray source 3FGL J2212.5+0703
• New dwarf galaxy candidates in the sphere of influence of the Local Volume spiral galaxy NGC2683
• A survey for dwarf galaxy remnants around fourteen globular clusters in the outer halo
• The shapes and alignments of the satellites of the Milky Way and Andromeda
• Overcoming Gamma Ray Constraints with Annihilating Dark Matter in Milky Way Subhalos
• Satellite group infall into the Milky Way: exploring the Crater-Leo case with new HST proper motions
• The Dark Knight Falters
• Testing gravity with halo density profiles observed through gravitational lensing
• Dark matter halos in the multicomponent model. II. Density profiles of galactic halos
• Cosmic Ray Anomalies from the MSSM?
• Limits on Dark Matter annihilation cross sections to gamma-ray lines with subhalo distribution in N-body simulation and Fermi LAT data
• Resolution of the apparent discrepancy between the number of massive subhaloes in Abell 2744 and ΛCDM
• Explaining the observed velocity dispersion of dwarf galaxies by baryonic mass loss during the first collapse
• Uncovering Mass Segregation with Galaxy Analogues in Dark Matter Simulations
• Charged Fuzzy Dark Matter Black Holes
• Microlensing optical depth, event rate, and limits on compact objects in dark matter based on 20 yr of OGLE observations of the Small Magellanic Cloud
• New dwarf galaxy candidates in the sphere of influence of the Sombrero galaxy
• Dark Matter 2013
• The BAHAMAS project: Evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum
• SASHIMI-SIDM: Semi-analytical subhalo modelling for self-interacting dark matter at sub-galactic scales
• Spatial extension of dark subhalos as seen by Fermi-LAT and implications for WIMP constraints
• Sommerfeld-enhanced dark matter searches with dwarf spheroidal galaxies
• Direct detection and CMB constraints on light DM scenario of top quark asymmetry and dijet excess at Tevatron
• Star Streams in Triaxial Isochrone Potentials with Sub-Halos
• Direct Detection Anomalies in light of $Gaia$ Data
• Exploiting flux ratio anomalies to probe warm dark matter in future large scale surveys
• Dark Matter annihilation energy output and its effects on the high-z IGM
• Orbital scattering by random interactions with extended substructures
• Dark Stars and Boosted Dark Matter Annihilation Rates
• The local dark matter distribution in self-interacting dark matter halos
• Stellar streams and dark substructure: the diffusion regime
• MaNGA DynPop -- IV. Stacked total density profile of galaxy groups and clusters from combining dynamical models of integral-field stellar kinematics and galaxy-galaxy lensing
• Prospects for Detecting Gaps in Globular Cluster Stellar Streams in External Galaxies with the Nancy Grace Roman Space Telescope
• Constraining dark matter sub-structure with the dynamics of astrophysical systems
• The Epoch of Assembly of Two Galaxy Groups: A comparative study
• Formation and Radiative Feedback of First Objects and First Galaxies
• The inhomogenous reionization of the inter-galactic medium by metal-poor globular clusters
• Origin and Evolution of Structure and Nucleosynthesis for Galaxies in the Local Group
• Auriga Streams I: disrupting satellites surrounding Milky Way-mass haloes at multiple resolutions
• Cusps in the center of galaxies: a real conflict with observations or a numerical artefact of cosmological simulations?
• The Ultramarine Simulation: properties of dark matter haloes before redshift 5.5
• Cosmic Transients, Einstein's Equivalence Principle and Dark Matter Halos
• Modified holographic Ricci dark energy coupled to interacting relativistic and non-relativistic dark matter in the nonflat universe
• How to calculate dark matter direct detection exclusion limits that are consistent with gamma rays from annihilation in the Milky Way halo
• Harnessing the Population Statistics of Subhalos to Search for Annihilating Dark Matter
• Colour-magnitude diagram in simulations of galaxy formation
• Dark matter indirect detection signals and the nature of neutrinos in the supersymmetric $U(1{)}_{B-L}$ extension of the standard model
• Census of Gaseous Satellites around Local Spiral Galaxies
• Setting the Stage: Structures from Gaussian Random Fields
• Jeans that fit: weighing the mass of the Milky Way analogues in the $\Lambda \mathrm{CDM}$ universe
• Dwarf spheroidal $J$-factor likelihoods for generalized NFW profiles
• BASILISK: Bayesian Hierarchical Inference of the Galaxy-Halo Connection using Satellite Kinematics--I. Method and Validation
• Modelling the dynamical friction timescale of sinking satellite
• Kinematics of Milky Way Satellites: Mass Estimates, Rotation Limits, and Proper Motions
• An Accurate Comprehensive Approach to Substructure: II. Stripped Subhaloes
• An Accurate Comprehensive Approach to Substructure: III. Masses and Formation Times of the Host Haloes
• Milky Way simulations: the Galaxy, its stellar halo and its satellites - insights from a hybrid cosmological approach
• Cosmic Degeneracies III: N-body Simulations of Interacting Dark Energy with Non-Gaussian Initial Conditions
• Prospects for $\gamma$-ray observations of the Perseus galaxy cluster with the Cherenkov Telescope Array
• Dark matter halo mass functions and density profiles from mass and energy cascade
• Removal and mixing of the coronal gas from satellites in galaxy groups: cooling the intragoup gas
• Quantifying and controlling biases in dark matter halo concentration estimates
• Constraints to dark matter annihilation from high-latitude HAWC unidentified sources
• Dating the tidal disruption of globular clusters with Gaia data on their stellar streams
• On the DM interpretation of the origin of non-thermal phenomena in galaxy clusters
• A possible challenge for Cold and Warm Dark Matter
• How an era of kination impacts substructure and the dark matter annihilation rate
• Searching for High Energy Neutrino counterpart signals; The case of the Fermi Bubbles signal and of Dark Matter annihilation in the inner Galaxy
• Constraints on ultracompact minihalos from the extragalactic gamma-ray background observation
• Constraints on dark matter annihilation from M87: Signatures of prompt and inverse-Compton gamma rays
• Emergence of Galactic Morphologies at Cosmic Dawn: Input from Numerical Modeling
• Can substructure in the Galactic Halo explain the ATIC and PAMELA results?
• Assessing Mass Loss and Stellar-to-Halo Mass Ratio of Satellite Galaxies: A Galaxy-Galaxy Lensing Approach Utilizing DECaLS DR8 Data
• Classification of gamma-ray targets for velocity-dependent and subhalo-boosted dark-matter annihilation
• Galactic Geology: Probing Time-Varying Dark Matter Signals with Paleo-Detectors
• The CIDER simulations: Nonlinear structure formation in the Constrained Interacting Dark Energy Scenario
• Interlopers speak out: studying the dark universe using small-scale lensing anisotropies
• Tetrahedral collapse: a rotational toy model of simultaneous dark-matter halo, filament and wall formation
• Planes of satellites around simulated disk galaxies II: Time-persistent planes of kinematically-coherent satellites in $\Lambda$CDM
• Analysis of Fermi-LAT data from Tucana-II: Possible constraints on the Dark Matter models with an intriguing hint of a signal
• Modified initial power spectrum and too big to fail problem
• The abundance of satellite galaxies in the inner region of $\Lambda$CDM Milky Way sized haloes
• Interpretation of the cosmic ray positron and electron excesses with an annihilating-decaying dark matter scenario
• Can galactic dark matter substructure contribute to the cosmic gamma-ray anisotropy?
• Towards a Bullet-proof test for indirect signals of dark matter
• Time evolution of gaps in stellar streams in axisymmetric Stäckel potentials
• Search for line signal candidates in the Fermi-LAT data
• Condensation of Galactic Cold Dark Matter
• The formation history of the Milky Way disc with high-resolution cosmological simulations
• Ultra-fine dark matter structure in the Solar neighbourhood
• Impact of Cosmological Satellites on Stellar Discs: Dissecting One Satellite at a Time
• The effect of local universe constraints on halo abundance and clustering
• The Formation of a Milky Way-sized Disk Galaxy 1. A Comparison of Numerical Methods
• Addressing via N-body simulations the distribution of the satellite tidal debris in the Milky Way environment
• The low mass end of the neutral gas mass and velocity width functions of galaxies in $\Lambda$CDM
• Secular evolution of galaxies and galaxy clusters in decaying dark matter cosmology
• Effect of small scale density perturbations on the formation of dark matter halo profiles
• Two-Point Separation Functions for Modeling Wide Binary Systems in Nearby Dwarf Galaxies
• The impact of filaments on dwarf galaxy properties in the Auriga simulations
• Anisotropic strong lensing as a probe of dark matter self-interactions
• Quantifying the intrinsic variability due to randomness of the Auriga galaxy formation model
• A Random Walk Model for Dark Matter Halo Concentrations
• The Origin of Star Formation in Early-type Galaxies Inferred from Spatially Resolved Spectroscopy
• Revisit NGC 5466 Tidal Stream with $Gaia$, SDSS/SEGUE and LAMOST
• Extended Stellar Components of Galaxies & the Nature of Dark Matter
• The Structure of Cold Dark Matter Halos: Recent Insights from High Resolution Simulations
• Searches for Particle Dark Matter with gamma-rays
• The prediction of using LHAASO's cosmic-ray electron measurements to constrain decaying heavy dark matter
• Ubiquity of density slope oscillations in the central regions of galaxy and cluster-sized systems
• Multiwavelength analysis of low surface brightness galaxies to study possible dark matter signature
• Low-metallicity stellar halo populations as tracers of dark matter haloes
• The distribution of annihilation luminosities in dark matter substructure
• The Lost Dwarfs of Centaurus A and the Formation of its Dark Globular Clusters
• Shell galaxies: kinematical signature of shells, satellite galaxy disruption and dynamical friction
• Clustering in the Phase Space of Dark Matter Haloes. I. Results from the Aquarius simulations
• Size Evolution of Early-Type Galaxies and Massive Compact Objects as the Dark Matter
• MaNGA DynPop -- VI. Matter density slopes from dynamical models of 6000 galaxies versus cosmological simulations: the interplay between baryonic and dark matter
• Kinematics and dynamics of the luminous infrared galaxy pair NGC 5257/58 (Arp 240)
• Faster than SAM: An empirical model for the tidal evolution of dark matter substructure around strong gravitational lenses
• Gaps in stellar streams as a result of globular cluster fly-bys
• Made-To-Measure Models of Self-Similar Triaxial Halos with Steep Inner Density Gradients
• Saas-Fee Lecture Notes: Multi-messenger Astronomy and Dark Matter
• Searches for Particle Dark Matter: An Introduction
• The [C II] line emission as an interstellar medium probe in the MARIGOLD galaxies
• Substructure in the Globular Cluster Populations of the Virgo Cluster Elliptical Galaxies M84 and M86
• Euclid preparation: Determining the weak lensing mass accuracy and precision for galaxy clusters
• EDEN: Exploring Disks Embedded in N-body simulations of Milky-Way-mass halos from Symphony
• Can tides explain the low dark matter density in Fornax?
• Substructure at High Speed I: Inferring the Escape Velocity in the Presence of Kinematic Substructure
• $\text{slick}$: Modeling a Universe of Molecular Line Luminosities in Hydrodynamical Simulations
• Evaluating the variance of individual halo properties in constrained cosmological simulations
• Emergence of a stellar cusp by a dark matter cusp in a low-mass compact ultra-faint dwarf galaxy
• Strong Lensing by Subhalos in the Dwarf-Galaxy Mass Range II: Detection Probabilities
• Estimate of halo ellipticity as a function of radius with flexions
• Evolution of Low Mass Galactic Subhalos and Dependence on Concentration
• Constraining Dark Matter Microphysics with the Annihilation Signal from Subhalos
• Testing the dark matter origin of the WMAP-Planck Haze with radio observations of Spiral Galaxies
• Dark matter in massive galaxies
• Dwarf Galaxy Clustering and Missing Satellites
• Disc-Halo Interactions in ΛCDM
• PhotoNs-GPU:A GPU accelerated cosmological simulation code
• Cosmological simulations of the same spiral galaxy: connecting the dark matter distribution of the host halo with the subgrid baryonic physics
• The kinematics of globular clusters systems in the outer halos of the Aquarius simulations
• Stellar Populations in a semi-analytic model I: bulges of Milky Way-like galaxies
• A Novel Scheme for Dark Matter Annihilation Feedback in Cosmological Simulations
• Understanding Dwarf Galaxies in order to Understand Dark Matter
• Forward modelling of quasar light curves and the cosmological matter power spectrum on milliparsec scales
• SHARP -- IX. The dense, low-mass perturbers in B1938+666 and J0946+1006: implications for cold and self-interacting dark matter
• Velocity-dependent J-factors for Milky Way dwarf spheroidal analogues in cosmological simulations
• The luminosity of cluster galaxies in the Cluster-EAGLE simulations
• Boosting the 21 cm forest signals by the clumpy substructures
• Velocity Variations in the Phoenix-Hermus Star Stream
• Precision Pollution - The effects of enrichment yields and timing on galactic chemical evolution
• A test of invariance of dark matter halo surface density using multiwavelength mock galaxy catalogues
• Search for Dark Matter Annihilation to gamma-rays from SPT-SZ selected Galaxy Clusters
• Central densities of dark matter halos in FIRE-2 simulations of low-mass galaxies with cold dark matter and self-interacting dark matter
• The influence of dark matter halo on the stellar stream asymmetry via dynamical friction
• AuriDESI: Mock Catalogues for the DESI Milky Way Survey
• Low Energy INTEGRAL Positrons from eXciting Dark Matter
• Dark Matter Subhalos, Strong Lensing and Machine Learning
• Co-Interacting Dark Matter
• Probing baryonic processes and gastrophysics in the formation of the Milky Way dwarf satellites: I. metallicity distribution properties
• Bimodal Formation Time Distribution for Infall Dark Matter Halos
• Dynamical Properties of Collisionless Star Streams
• The Hierarchical Structure of Galactic Haloes: Classification and characterisation with Halo-OPTICS
• Globular clusters vs dark matter haloes in strong lensing observations
• Evanescent Matter
• A Study of the Properties and Dynamics of the Disk of Satellites in a Milky-Way-like Galaxy System
• Searching for dark matter subhalos in the Fermi-LAT catalog with Bayesian neural networks
• Demise of Faint Satellites around Isolated Early-type Galaxies
• Dark sector domain walls could explain the observed planes of satellites
• Constraining the distribution of dark matter in inner galaxy with indirect detection signal: The case of tentative 130 gev γ-ray line
• Structural and dynamical modeling of WINGS clusters. III. The pseudo phase-space density profile
• The neutron-capture and alpha-elements abundance ratios scatter in old stellar populations. Cosmological simulations of the stellar halo
• On rates of supernovae strongly lensed by galactic haloes in Millennium Simulation
• Probing Satellite Halos with Weak Gravitational Lensing
• Gaseous Dynamical Friction: a Numerical Study of Extended Perturbers
• The viability of low-mass subhaloes as targets for gamma-ray dark matter searches
• Cosmological Zoom-In Simulations of Milky Way Host Mass Dark Matter Halos with a Blue-Tilted Primordial Power Spectrum
• The effect of environment on the mass assembly history of the Milky Way and M31
• Measurement of Substructure from the Kinematics of the GD-1 Stellar Stream
• Statistics for dark matter subhalo searches in gamma rays from a kinematically constrained population model: Fermi-LAT-like telescopes
• The Effects of $\Lambda$CDM Dark Matter Substructure on the Orbital Evolution of Star Clusters
• Introduction to Tidal Streams
• Improving Performance of Zoom-In Cosmological Simulations using Initial Conditions with Customized Grids
• A large change in the predicted number of small halos due to a small amplitude oscillating inflaton potential
• Fingerprint matching of beyond-WIMP dark matter: neural network approach
• Warm dark matter model with a few keV mass is bad for the too-big-to-fail problem
• Building Blocks of the Milky Way's Accreted Spheroid
• Testing the uniqueness of gravitational lens mass models
• Dark-ages Reionization and Galaxy Formation Simulation - XIV. Gas accretion, cooling and star formation in dwarf galaxies at high redshift
• Solving the puzzle of subhalo spins
• Tomography of stellar halos: what does anisotropy in a stellar halo tell us?
• Dark Matter implications of the Fermi-LAT measurement of anisotropies in the diffuse gamma-ray background: status report
• BASILISK II. Improved Constraints on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• A study of Neural networks point source extraction on simulated Fermi/LAT Telescope images
• On the behaviour of streams in angle and frequency spaces in different potentials
• Machine-guided Exploration and Calibration of Astrophysical Simulations
• The imprint of dark subhaloes on the circumgalactic medium
• The Possible Equation Of State Of Dark Matter in Low Surface Brightness Galaxies
• Signatures of Synchrotron Radiation from the Annihilation of Dark Matter at the Galactic Centre
• A graph model for the clustering of dark matter halos
• A general relativistic extension to mesh-free methods for hydrodynamics
• Observing the very low-surface brightness dwarfs in a deep field in the VIRGO cluster: constraints on Dark Matter scenarios
• Giant monopoles as a dark matter candidate
• Radio Signal by Galactic Dark Matter
• Semi-analytic modelling of the europium production by neutron star mergers in the halo of the Milky Way
• Sensitivity of CTA to gamma-ray emission from the Perseus galaxy cluster
• A pilot survey of stellar tidal streams in nearby spiral galaxies
• Properties of subhalos in the interacting dark matter scenario
• The Dark Matter Contribution to Galactic Diffuse Gamma Ray Emission
• Spherical harmonics analysis of Fermi gamma-ray data and the Galactic dark matter halo
• Quantifying Departures from Equilibrium with the Spherical Jeans Equation
• Prospects for measuring dark matter microphysics with observations of dwarf spheroidal galaxies
• Dissecting Cosmological Filaments at High Redshifts: Emergence of Spaghetti-type Flow Inside DM Haloes
• Dark Resonance
• Caught in the cosmic web: environmental effects on subhalo abundance and internal density profiles
• Is the stellar mass-stellar metallicity relation universal in the Milky Way satellites and beyond?
• Stellar-gas kinematic misalignments in EAGLE: lifetimes and longevity of misaligned galaxies
• New probe of modified gravity
• HIKER: a halo-finding method based on kernel-shift algorithm
• Resolving Dark Matter Subhalos With Future Sub-GeV Gamma-Ray Telescopes
• Is the gamma-ray emission around the Coma galaxy cluster a dark matter origin?
• Visualization in Astrophysics: Developing New Methods, Discovering Our Universe, and Educating the Earth
• The Milky Way's total satellite population and constraining the mass of the warm dark matter particle
• Indirect Dark Matter Signals
• Analytical insight into dark matter subhalo boost factors for Sommerfeld-enhanced $s$- and $p$-wave $\gamma$-ray signals
• Exploring the Universe with Metal-Poor Stars
• A Redshift Survey of the Coma Cluster (A1656): Understanding the Nature of Subhalos in the Weak-lensing Map
• Large-k Limit of Multi-Point Propagators in the RG Formalism
• Ringing Regularity: Gravitational Perturbations and Quasinormal Modes of Einasto-Supported Black Holes
• The AIDA-TNG project: dark matter profiles and concentrations in alternative dark matter models
• Numerical effects on the stripping of dark matter and stars in IllustrisTNG galaxy groups and clusters
• New insights on low-mass dark matter subhalo tidal tracks via numerical simulations
• Super-Eddington accretion in high-redshift quasar hosts: Black-hole driven outflows, galaxy quenching, and the nature of little red dots
• Addressing the core-cusp and diversity problem of dwarf and disk galaxies using cold collisionless DARKexp theory
• The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
• Dark Matter Internal Pair Production -- A Novel Direct Detection Mechanism
• Bounding the Cosmological Constant using Galactic Rotation Curves from the SPARC Dataset
• Exploring the Angular Momentum -- Atomic Gas Content Connection with EAGLE and IllustrisTNG
• Prospects for annihilating dark matter from M31 and M33 observations with the Cherenkov Telescope Array
• SZ effects from annihilating dark matter in the Milky Way: smooth halo, subhalos and intermediate-mass-black-holes
• Implications for the missing low-mass galaxies (satellites) problem from cosmic shear
• Dark Matter and Fundamental Physics Searches with IACTs
• Probing the spatial and velocity anisotropies in stellar halos from the Aquarius simulations
• The mass profile of NGC 3377 from a Bayesian approach
• Dark Energy Simulations
• Assessment of Dark Matter Models Using Dark Matter Correlations across Dwarf Spheroidal Galaxies
• Observational constraints on phenomenological emergent dark energy and barotropic dark matter characterized by a constant equation of state parameter
• Impact of baryons on the population of Galactic subhalos and implications for dark matter searches
• Halo cluster shapes: Insights from simulated galaxies and ICL with prospects for weak lensing applications
• Limits in late time conversion of cold dark matter into dark radiation
• The Hierarchical Structure of Galactic Haloes: Generalised N-Dimensional Clustering with CluSTAR-ND
• Effect of dark matter halo substructures on galaxy rotation curves
• Investigation of mass substructure in gravitational lens system SDP.81 with ALMA long-baseline observations
• Subhalo abundance and satellite spatial distribution in Milky Way-Andromeda-like paired haloes
• Galaxy-galaxy strong lens perturbations: line-of-sight haloes versus lens subhaloes
• Cosmic positron excess: is the dark matter solution a good bet?
• The impact of cosmic filaments on the abundance of satellite galaxies
• Dark matter haloes in the multicomponent model. III. From dwarfs to galaxy clusters
• Milky Way globular cluster dynamics: are they preferentially co-rotating?
• Robustness of Neural Ratio and Posterior Estimators to Distributional Shifts for Population-Level Dark Matter Analysis in Strong Gravitational Lensing
• Dark matter in ALFALFA galaxies: Investigating galaxy-halo connection
• Detecting the hidden population of low-mass haloes in strong lenses
• On the Detectability of Galactic Dark Matter Annihilation into Monochromatic Gamma-rays
• Impact of Gravitational Slingshot of Dark Matter on Galactic Halo Profiles
• Matching the dark matter profiles of dSph galaxies with those of simulated satellites: a two parameter comparison
• VST-SMASH: VST Survey of Mass Assembly and Structural Hierarchy I. Survey presentation and deep photometry of IC 5332: tracing the mass assembly in the challenging faintest-end regime
• An Accurate Comprehensive Approach to Substructure: IV. Dynamical Friction
• The Density of Dark Matter in the Galactic Bulge and Implications for Indirect Detection
• How does the stellar disk of the Milky Way get its gas?
• Machine Learning for Galactic Archaeology: A chemistry-based neural network method for identification of accreted disc stars
• Assembly History and Internal Structure of Cluster Cold Dark Matter Haloes
• On the detection of stellar wakes in the Milky Way: a deep learning approach
• Tensorial solution of the Poisson equation and the dark matter amount and distribution of UGC 8490 and UGC 9753
• Epicyclic Density Variations in the Indus Stellar Stream
• Modeling supernova feedback in galaxy formation simulations with energy-conserving momentum injection
• Extragalactic Searches for Dark Matter Annihilation
• LSST Strong Lensing Systems Dark Matter Sensitivity Analysis with Neural Ratio Estimators
• Collisional Dynamics of Stars and Dark Matter in Ultra-Faint Galaxies
• The tidal evolution of satellite galaxies in cosmological simulations: insights from COLIBRE
• Imprints of tidal interactions on the stellar distribution of satellite galaxies: implications for dark matter deficient galaxies
• Galaxy simulations in the Gaia era
• ScaleFree: Dynamic KDE for Multiscale Point Cloud Exploration in VR
• Slow neutrinos: non-linearity and momentum-space emulation
• How to Build an Empirical Speed Distribution for Dark Matter in the Solar Neighborhood
• White dwarfs in the building blocks of the Galactic spheroid
• Monophotons from Scalar Portal Dark Matter at Neutrino Experiments
• Quasinormal modes of regular black holes surrounded by skewed dark matter distributions
• 130GeV gamma-ray line through axion conversion
• The DORCHA suite: nature, nurture, and the phase space distribution of the Milky Way's high redshift progenitors today
• A Mass Dependent Density Profile from Dwarfs to Clusters
• Excess of substructure due to primordial black holes
• Comparison of simulations and semi-analytical model for WDM subhalo mass functions
• Broken Expectations: The Effects of Modelling Assumptions on the Inferred Dark Matter Distribution in the Milky Way's Satellites
• Structure Formation under Inelastic Two-Component Dark Matter: Halo Statistics and Matter Power Spectra in the High-$z$ Universe
• Super Interacting Dark Sector: An Improvement on Self-Interacting Dark Matter via Scaling Relations of Galaxy Clusters
• Search for Galactic dark matter substructures with Cherenkov telescopes
• Dark Matter Energy Deposition and Production from the Table-Top to the Cosmos
• Detecting low-mass haloes with strong gravitational lensing I: the effect of data quality and lensing configuration
• Energetic neutrinos from the Sun and Earth and dark matter substructure
• Uncertainties in measuring the dark matter signal from Milky Way satellites using Cherenkov telescopes
• Milky Way Satellite Census. IV. Constraints on Decaying Dark Matter from Observations of Milky Way Satellite Galaxies
• Machine-Learned Dark Matter Subhalo Candidates in the 4FGL-DR2: Search for the Perturber of the GD-1 Stream
• Scaling Relations Between Low-mass Black Holes and Their Host Galaxies
• A general framework for unbiased tests of gravity using galaxy clusters
• Pseudo-observation of spiral galaxies in the radio band to verify depolarization models