Dark Matter Substructure in Galactic Halos

Abstract

We use numerical simulations to examine the substructure within galactic and cluster mass halos that form within a hierarchical universe. Clusters are easily reproduced with a steep mass spectrum of thousands of substructure clumps that closely matches observations. However, the survival of dark matter substructure also occurs on galactic scales, leading to the remarkable result that galaxy halos appear as scaled versions of galaxy clusters. The model predicts that the virialised extent of the Milky Way's halo should contain about 500 satellites with circular velocities larger than Draco and Ursa-Minor i.e. bound masses > 10^8Mo and tidally limited sizes > kpc. The substructure clumps are on orbits that take a large fraction of them through the stellar disk leading to significant resonant and impulsive heating. Their abundance and singular density profiles has important implications for the existence of old thin disks, cold stellar streams, gravitational lensing and indirect/direct detection experiments.

Astrophysical Journal Letters. 4 pages, latex. Simulation images and movies at http://star-www.dur.ac.uk:80/~moore/

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• Atomic Hydrogen Gas in Dark-Matter Minihalos and the Compact High Velocity Clouds
• Boson Stars from Self-Interacting Dark Matter
• NIHAO XV: The environmental impact of the host galaxy on galactic satellite and field dwarf galaxies
• Bending and Breathing Modes of the Galactic Disk
• Neutralino annihilation into gamma-rays in the Milky Way and in external galaxies
• Anisotropy in the Distribution of Satellite Galaxy Orbits
• Detection of substructure with adaptive optics integral field spectroscopy of the gravitational lens B1422+231
• Leo P: An Unquenched Very Low-Mass Galaxy
• Stellar kinematics and metallicities in the Leo I dwarf spheroidal galaxy -- wide field implications for galactic evolution
• The Clumpiness of Cold Dark Matter: Implications for the Annihilation Signal
• The ACS LCID project. V. The Star Formation History of the Dwarf Galaxy \objectname[]{LGS-3}: Clues for Cosmic Reionization and Feedback
• The total satellite population of the Milky Way
• Dwarf Galaxies and the Cosmic Web
• HBT+: an improved code for finding subhalos and building merger trees in cosmological simulations
• Cosmological bounds on dark matter-neutrino interactions
• Discovery of an ultra-diffuse galaxy in the Pisces-Perseus supercluster
• Reopening the window on charged dark matter
• Small-Scale Structure in the SDSS and LCDM: Isolated L* Galaxies with Bright Satellites
• On the Baryon Fractions in Clusters and Groups of Galaxies
• A Quantitative Study of Interacting Dark Matter in Halos
• Extended Lyman Alpha Emission Around Young Quasars: a Constraint on Galaxy Formation
• Exploring Halo Substructure with Giant Stars: The Velocity Dispersion Profiles of the Ursa Minor and Draco Dwarf Spheroidals At Large Angular Separations
• Evidence of self-interacting cold dark matter from galactic to galaxy cluster scales
• Linear Cosmological Structure Limits on Warm Dark Matter
• Diverse Stellar Haloes in Nearby Milky Way-Mass Disc Galaxies
• How Common are the Magellanic Clouds?
• Baryonic impact on the dark matter distribution in Milky Way-size galaxies and their satellites
• The Formation of a Disk Galaxy within a Growing Dark Halo
• "Non-cold" dark matter at small scales: a general approach
• The mass of our Milky Way
• The preferred direction of infalling satellite galaxies in the Local Group
• Phat ELVIS: The inevitable effect of the Milky Way's disk on its dark matter subhaloes
• Jeans Analysis for Dwarf Spheroidal Galaxies in Wave Dark Matter
• The impact of stellar feedback on the structure, size and morphology of galaxies in Milky Way size dark matter haloes
• Structure and Subhalo Population of Halos in a Self-Interacting Dark Matter Cosmology
• Towards a Resolution of the Galactic Spin Crisis: Mergers, Feedback, and Spin Segregation
• Boson Stars and Oscillatons: A Review
• The phase-space structure of cold dark-matter halos: Insights into the Galactic halo
• To Circularize or Not to Circularize? -- Orbital Evolution of Satellite Galaxies
• A profile in FIRE: resolving the radial distributions of satellite galaxies in the Local Group with simulations
• Linear perturbation theory for tidal streams and the small-scale CDM power spectrum
• The surface brightness of dark matter: unique signatures of neutralino annihilation in the Galactic halo
• The dependence on environment of Cold Dark Matter Halo properties
• The Population of Weak MgII Absorbers. II The Properties of Single-Cloud Systems
• Full calculation of clumpiness boost factors for antimatter cosmic rays in the light of Lambda-CDM N-body simulation results
• Resolving Subhaloes' Lives with the Hierarchical Bound-Tracing Algorithm
• The Primeval Populations of the Ultra-Faint Dwarf Galaxies
• The Hierarchical Structure and Dynamics of Voids
• Probing dark matter structure down to $10^7$ solar masses: flux ratio statistics in gravitational lenses with line of sight halos
• Insight into the baryon-gravity relation in galaxies
• How well can cold-dark-matter substructures account for the observed radio flux-ratio anomalies?
• The Hestia project: simulations of the Local Group
• The SPLASH Survey: Internal Kinematics, Chemical Abundances, and Masses of the Andromeda I, II, III, VII, X, and XIV dSphs
• Formation of Dwarf Galaxies during the Cosmic Reionization
• Planes of satellite galaxies and the cosmic web
• The Formation of the First Globular Clusters in Dwarf Galaxies Before the Epoch of Reionization
• In the Wake of Dark Giants: New Signatures of Dark Matter Self Interactions in Equal Mass Mergers of Galaxy Clusters
• Converting non-relativistic dark matter to radiation
• Dark Matter Heating and Early Core Formation in Dwarf Galaxies
• The discovery of seven extremely low surface brightness galaxies in the field of the nearby spiral galaxy M101
• Novel constraints on the particle nature of dark matter from stellar streams
• Radial distribution and strong lensing statistics of satellite galaxies and substructure using high resolution LCDM hydrodynamical simulations
• Galactic halo cusp-core: tidal compression in mergers
• Evidence for the Hierarchical Formation of the Galactic Spheroid
• Formation epochs, star formation histories and sizes of massive early-type galaxies in cluster and field environments at z=1.2: insights from the rest-frame UV
• A spectroscopic confirmation of the Bootes II dwarf spheroidal
• Pushing back the limits: detailed properties of dwarf galaxies in a LCDM universe
• Joint constraints on thermal relic dark matter from strong gravitational lensing, the Lyman-$\alpha$ forest, and Milky Way satellites
• Neutrinos from Inert Doublet Dark Matter
• Descendants of the first stars: the distinct chemical signature of second generation stars
• Dark matter in Draco and the Local Group: Implications for direct detection experiments
• Chandra Observation of RXJ1720.1+2638: a Nearly Relaxed Cluster with a Fast Moving Core?
• Second-order Lagrangian perturbation theory initial conditions for resimulations
• The galactic antiproton spectrum at high energies: background expectation vs. exotic contributions
• The Anisotropic Distribution of M 31 Satellite Galaxies: A Polar Great Plane of Early-Type Companions
• The Signature of Galactic Tides in Local Group Dwarf Spheroidals
• Dwarf galaxy formation with H2-regulated star formation
• Modeling The Structure And Dynamics of Dwarf Spheroidal Galaxies with Dark Matter And Tides
• All about baryons: revisiting SIDM predictions at small halo masses
• Abundance of Field Galaxies
• Constraints on dark matter scenarios from measurements of the galaxy luminosity function at high redshifts
• Dark halo properties from rotation curves
• The Next Generation Fornax Survey (NGFS): II. The Central Dwarf Galaxy Population
• The Abundance of Low-luminosity Lyman alpha Emitters at High Redshift
• Prospects of detecting gamma-ray emission from galaxy clusters: cosmic rays and dark matter annihilations
• Light-element Abundance Variations in the Milky Way Halo
• Galactic cirri in deep optical imaging
• Star Formation, Supernovae Feedback and the Angular Momentum Problem in Numerical CDM Cosmogony: Half Way There?
• Solving the small-scale structure puzzles with dissipative dark matter
• Environmental Dependence of Cold Dark Matter Halo Formation
• Asymmetric Dark Matter Stars
• Simulating nonlinear cosmological structure formation with massive neutrinos
• Scattering, Damping, and Acoustic Oscillations: Simulating the Structure of Dark Matter Halos with Relativistic Force Carriers
• At the survey limits: discovery of the Aquarius 2 dwarf galaxy in the VST ATLAS and the SDSS data
• The Substructure Hierarchy in Dark Matter Haloes
• Statistics of Satellite Galaxies Around Milky Way-Like Hosts
• Early structure in LCDM
• Galaxy formation in pre-processed dark halos
• Heating of Galactic Disks by Infalling Satellites
• Galactic Substructure and Dark Matter Annihilation in the Milky Way Halo
• Reconstructing Galaxy Histories from Globular Clusters
• Collisional dark matter and the structure of dark halos
• Cosmological Constraints on an Invisibly Decaying Higgs Boson
• The Fate of Substructures in Cold Dark Matter Haloes
• Inflation, cold dark matter, and the central density problem
• Internal properties and environments of dark matter halos
• Phase transitions between dilute and dense axion stars
• The Resolved Structure and Dynamics of an Isolated Dwarf Galaxy: A VLT and Keck Spectroscopic Survey of WLM
• Kinematical and chemical vertical structure of the Galactic thick disk II. A lack of dark matter in the solar neighborhood
• Effects of Dark Matter Substructures on Gravitational Lensing: Results from the Aquarius Simulations
• The Formation of the First Stars in the Universe
• Satellites of LMC-Mass Dwarfs: Close Friendships Ruined by Milky Way Mass Halos
• Dissecting Galaxy Formation: I. Comparison Between Pure Dark Matter and Baryonic Models
• High resolution imaging of the anomalous flux-ratio gravitational lens system CLASS B2045+265: Dark or luminous satellites?
• Tidal debris of dwarf spheroidals as a probe of structure formation models
• Evolution of spiral galaxies in modified gravity
• Search for Dark Matter from the Galactic Halo with the IceCube Neutrino Observatory
• Where are the Fossils of the First Galaxies? II. True Fossils, Ghost Halos, and the Missing Bright Satellites
• Analytic Cross Sections for Substructure Lensing
• Satellites of Simulated Galaxies: survival, merging, and their relation to the dark and stellar halos
• Resonant stripping as the origin of dwarf spheroidal galaxies
• Are sterile neutrinos consistent with clusters, the CMB and MOND?
• Turning the Tides on the Ultra-Faint Dwarf Spheroidal Galaxies: Coma Berenices and Ursa Major II
• The faint end of the Centaurus A satellite luminosity function
• The Masses and Shapes of Dark Matter Halos from Galaxy-Galaxy Lensing in the CFHTLS
• The Imprint of Warm Dark Matter on the Cosmological 21-cm Signal
• Hydrodynamic simulations of merging clusters of galaxies
• Mass modelling of dwarf spheroidal galaxies: the effect of unbound stars from tidal tails and the Milky Way
• Sensitivity of Next-Generation Tritium Beta-Decay Experiments for keV-Scale Sterile Neutrinos
• The Dependence of Subhalo Abundance on Halo Concentration
• Andromeda X, A New Dwarf Spheroidal Satellite of M31: Photometry
• The radial distribution of galaxies in groups and clusters
• Streams and caustics: the fine-grained structure of LCDM haloes
• The luminosity function of the Virgo Cluster from M_B=-22 to M_B=-11
• Dark Matter Problem in Disk Galaxies
• Andromeda Dwarfs in Light of MOND. II. Testing Prior Predictions
• The Impact of Inhomogeneous Reionization on the Satellite Galaxy Population of the Milky Way
• Simulations of the heating of the Galactic stellar disc
• DGSAT: Dwarf Galaxy Survey with Amateur Telescopes I. Discovery of low surface brightness systems around nearby spiral galaxies
• The emptiness of voids: yet another over-abundance problem for the LCDM model
• Shell Structure in the Fornax Dwarf Spheroidal Galaxy
• Models of the ICM with Heating and Cooling: Explaining the Global and Structural X-ray Properties of Clusters
• Giant cluster arcs as a constraint on the scattering cross-section of dark matter
• Constraints on dark matter and the shape of the Milky Way dark halo from the 511 keV line
• Internal kinematics and dynamical models of dwarf spheroidal galaxies around the Milky Way
• Self-Consistent Modeling of Reionization in Cosmological Hydrodynamical Simulations
• Dwarf Spheroidals in MOND
• The stellar-to-halo mass relation of GAMA galaxies from 100 square degrees of KiDS weak lensing data
• Galactic Archaeology. The dwarfs that survived and perished
• On the nature of the Milky Way satellites
• Too Many, Too Few, or Just Right? The Predicted Number and Distribution of Milky Way Dwarf Galaxies
• Gravothermal Collapse of Self-Interacting Dark Matter Halos and the Origin of Massive Black Holes
• Formation of the Galactic stellar halo I. Structure and kinematics
• Searches for Dark Matter annihilation signatures in the Segue 1 satellite galaxy with the MAGIC-I telescope
• Cosmological particle-in-cell simulations with ultralight axion dark matter
• Anomalous Flux Ratios in Gravitational Lenses: For or Against CDM?
• The Copernicus Complexio: a high-resolution view of the small-scale Universe
• Indirect searches for sterile neutrinos at a high-luminosity Z-factory
• Galaxy Groups at Intermediate Redshift
• Testing the Warm Dark Matter paradigm with large-scale structures
• Bar-Induced Evolution of Dark Matter Cusps
• Galaxy Formation with BECDM -- II. Cosmic Filaments and First Galaxies
• The phase-space structure of a dark-matter halo: Implications for dark-matter direct detection experiments
• Space- and Ground-Based Gamma-Ray Astrophysics
• A Dark Hydrogen Cloud in the Virgo Cluster
• The Rotation Velocity Attributable to Dark Matter at Intermediate Radii in Disk Galaxies
• Positrons and antiprotons from inert doublet model dark matter
• Galactic Substructure and Direct Detection of Dark Matter
• The ISLAndS project II: The Lifetime Star Formation Histories of Six Andromeda dSphs
• A Lonely Giant: The Sparse Satellite Population of M94 Challenges Galaxy Formation
• Tidal Signatures in the Faintest Milky Way Satellites: The Detailed Properties of Leo V, Pisces II and Canes Venatici II
• Star Stream Folding by Dark Galactic Sub-Halos
• Discovery of Andromeda XIV: A Dwarf Spheroidal Dynamical Rogue in the Local Group?
• Probing dark matter substructure in the gravitational lens HE0435-1223 with the WFC3 grism
• Lighting the Universe with filaments
• Not too big, not too small: the dark halos of the dwarf spheroidals in the Milky Way
• The Observed and Predicted Spatial Distribution of Milky Way Satellite Galaxies
• The evolution of substructure II: linking dynamics to environment
• Dark Matter Subhaloes in Numerical Simulations
• On the Structure of Dark Matter Halos at the Damping Scale of the Power Spectrum with and without Relict Velocities
• Subaru Mid-infrared Imaging of the Quadruple Lenses PG1115+080 and B1422+231: Limits on Substructure Lensing
• A Robust Determination of Milky Way Satellite Properties using Hierarchical Mass Modeling
• The Beginning and Evolution of the Universe
• The Effects of Photoionization on Galaxy Formation -- III: Environmental Dependence in the Luminosity Function
• Mapping substructure in the HST Frontier Fields cluster lenses and in cosmological simulations
• The inner structure of haloes in Cold+Warm dark matter models
• Measuring the power spectrum of dark matter substructure using strong gravitational lensing
• Kinetic decoupling of neutralino dark matter
• The Detectability of Neutralino Clumps via Atmospheric Cherenkov Telescopes
• Constraints on dark matter particles from theory, galaxy observations and N-body simulations
• Limits on the Radiative Decay of Sterile Neutrino Dark Matter from the Unresolved Cosmic and Soft X-ray Backgrounds
• Gaps in globular cluster streams: giant molecular clouds can cause them too
• Abundance of damped Lyman-alpha absorbers in cosmological SPH simulations
• Warm dark matter does not do better than cold dark matter in solving small-scale inconsistencies
• Did the Milky Way dwarf satellites enter the halo as a group?
• On the Distribution of Orbital Poles of Milky Way Satellites
• The Comparative Chemical Evolution of an Isolated Dwarf Galaxy: A VLT and Keck Spectroscopic Survey of WLM
• The Abundance and Radial Distribution of Satellite Galaxies
• Destruction of small-scale dark matter clumps in the hierarchical structures and galaxies
• Satellite Systems around Galaxies in Hydrodynamic Simulations
• A New Prescription for Protogalactic Feedback and Outflows: Where Have All the Baryons Gone?
• Galaxy Formation Spanning Cosmic History
• Dark matter within high surface brightness spiral galaxies
• Self-Scattering for Dark Matter with an Excited State
• Intracluster stellar population properties from N-body cosmological simulations -- I. Constraints at $z=0$
• Dark stars: gravitational and electromagnetic observables
• Delayed Recombination
• Metal Abundances and Kinematics of Bright Metal-Poor Giants Selected from the LSE Survey: Implications for the Metal-Weak Thick Disk
• Effects of baryon removal on the structure of dwarf spheroidal galaxies
• Charged-particle decay and suppression of small-scale power
• Dark matters on the scale of galaxies
• Constraints on New Neutrino Interactions via Light Abelian Vector Bosons
• Wide-Field Survey of Dwarf Satellite Systems Around 10 Hosts in the Local Volume
• The asymptotic tidal remnants of cold dark matter subhalos
• A Large Dark Matter Core in the Fornax Dwarf Spheroidal Galaxy?
• The M101 Satellite Luminosity Function and the Halo to Halo Scatter Among Local Volume Hosts
• Constraining sterile neutrino dark matter by phase-space density observations
• How to Quench a Dwarf Galaxy: The Impact of Inhomogeneous Reionization on Dwarf Galaxies and Cosmic Filaments
• How cold is Dark Matter? Constraints from Milky Way Satellites
• Fitting Gravitational Lenses: Truth or Delusion
• The Link between Galactic Satellite Orbits and Subhalo Accretion
• Cosmological Origin of the Stellar Velocity Dispersions in Massive Early-Type Galaxies
• On the formation of extended galactic disks by tidally disrupted dwarf galaxies
• The origin of failed subhaloes and the common mass scale of the Milky Way satellite galaxies
• Novel constraints on non-cold (non-thermal) Dark Matter from Lyman-$\alpha$ forest data
• Constrained simulations of the Local Group: on the radial distribution of substructures
• Westerbork HI observations of high-velocity clouds near M31 and M33
• Low energy antideuterons: shedding light on dark matter
• The Carina Project: II. Stellar Populations
• Complex Structure of Galaxy Cluster Abell 1689: Evidence for a Merger from X-ray data?
• Early Formation and Late Merging of the Giant Galaxies
• Discovery of a Faint Old Stellar System at 150 kpc
• Substructure of fuzzy dark matter haloes
• Strong Turbulence in the Cool Cores of Galaxy Clusters: Can Tsunamis Solve the Cooling Flow Problem?
• Fossils of Reionization in the Local Group
• Halo properties in models with dynamical Dark Energy
• Identifying Lenses with Small-Scale Structure. II. Fold Lenses
• A Catalog of Ultra-compact High Velocity Clouds from the ALFALFA Survey: Local Group Galaxy Candidates?
• Where are the high velocity clouds?
• Declining rotation curves of galaxies as a test of gravitational theory
• Delving Deeper into the Tumultuous Lives of Galactic Dwarfs: Modeling Star Formation Histories
• Halo Mass Profiles and Low Surface Brightness Galaxies Rotation Curves
• Halo Substructure and Disk Heating in a Lambda CDM Universe
• Star Formation in Sculptor Group Dwarf Irregular Galaxies and the Nature of "Transition" Galaxies
• Merger Histories in Warm Dark Matter Structure Formation Scenario
• The Dragonfly Nearby Galaxies Survey. III. The Luminosity Function of the M101 Group
• The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos
• Ultra-light Dark Matter is Incompatible with the Milky Way's Dwarf Satellites
• The satellites of the Milky Way - Insights from semi-analytic modelling in a LambdaCDM cosmology
• The failures of the standard model of cosmology require a new paradigm
• What is the (Dark) Matter with Dwarf Galaxies?
• Discovery of a close pair of faint dwarf galaxies in the halo of Centaurus A
• Cosmology and Convention
• The early-type dwarf galaxy population of the Hydra I cluster
• The effect of feedback and reionization on star formation in low-mass dwarf galaxy haloes
• Are Great Disks Defined by Satellite Galaxies in Milky-Way Type Halos Rare in $\Lambda$CDM model?
• The VIMOS VLT Deep Survey: Evolution of the non-linear galaxy bias up to z=1.5
• The NGC 5846 Group: Dynamics and the Luminosity Function to M_R=-12
• Effective Dark Matter Model: Relic density, CDMS II, Fermi LAT and LHC
• keV Sterile Neutrino Dark Matter from Singlet Scalar Decays: The Most General Case
• Cosmological Simulations of Decaying Dark Matter: Implications for Small-scale Structure of Dark Matter Halos
• A Systematic Look at the Effects of Radiative Feedback on Disc Galaxy Formation
• Cosmological constraints on quintessential halos
• Indirect signals from light neutralinos in supersymmetric models without gaugino mass unification
• The depletion of gas in high-redshift dwarf galaxies from an inhomogeneous reionization
• The Imprint of Reionization on the Star Formation Histories of Dwarf Galaxies
• Orbital parameters of infalling satellite haloes in the hierarchical $\Lambda$CDM model
• Dark matter-radiation interactions: the impact on dark matter haloes
• Dipolar Dark Matter and Dark Energy
• Deep HST Imaging of Sextans A I. The Spatially Resolved Recent Star Formation History
• Satellite abundances around bright isolated galaxies II: radial distribution and environmental effects
• Satellites and Haloes of Dwarf Galaxies
• Determining orbits for the Milky Way's dwarfs
• The SWELLS survey. II. Breaking the disk-halo degeneracy in the spiral galaxy gravitational lens SDSS J2141-0001
• Antiprotons from primordial black holes
• Fourteen candidate RR Lyrae star streams in the inner Galaxy
• Kinematics and Metallicity of M31 Red Giants: The Giant Southern Stream and Discovery of a Second Cold Component at R = 20 kpc
• Substructure and galaxy formation in the Copernicus Complexio warm dark matter simulations
• The Abell Cluster A586 and the Detection of the Equivalence Principle
• Making Counter-Orbiting Tidal Debris: The Origin of the Milky Way Disc of Satellites
• A New Milky Way Satellite Discovered In The Subaru/Hyper Suprime-Cam Survey
• Evaporating the Milky Way halo and its satellites with inelastic self-interacting dark matter
• Constraints on dark matter physics from dwarf galaxies through galaxy cluster haloes
• Cosmological Structure Formation under MOND: a new numerical solver for Poisson's equation
• Incorporating interactive 3-dimensional graphics in astronomy research papers
• Satellite Galaxies and Fossil Groups in the Millennium Simulation
• Simulating Subhalos at High Redshift: Merger Rates, Counts, and Types
• Galaxy formation in semi-analytic models and cosmological hydrodynamic zoom simulations
• The ACS LCID project. X. The Star Formation History of IC 1613: Revisiting the Over-Cooling Problem
• The ALP miracle revisited
• The Formation of the Local Group Planes of Galaxies
• On the identification of substructure in phase-space using orbital frequencies
• Scalar Field Dark Matter: Helping or Hurting Small-Scale Problems in Cosmology?
• The dwarf galaxy satellite system of Centaurus A
• Dark Matter Halos with Cores from Hierarchical Structure Formation
• Tidal evolution of disky dwarf galaxies in the Milky Way potential: the formation of dwarf spheroidals
• How common is the Milky Way - satellite system alignment?
• Abundance matching with the mean star formation rate: there is no missing satellites problem in the Milky Way above ${\mathbf{M}}_{200}\sim 10^9{\mathbf{M}}_{\odot }$
• Inside the whale: the structure and dynamics of the isolated Cetus dwarf spheroidal
• Substructure in lensing clusters and simulations
• Expanded haloes, abundance matching and too-big-to-fail in the Local Group
• On the persistence of two small-scale problems in ΛCDM
• Dark Matter And $B_s\to {\mu }^{+}{\mu }^{-}$ With Minimal $S{O}_{10}$ Soft SUSY Breaking
• The mass of the Milky Way out to 100 kpc using halo stars
• Simply split SIMPs
• Galactic rotation curves, the baryon-to-dark-halo-mass relation and space-time scale invariance
• Fuzzy Dark Matter Soliton Cores around Supermassive Black Holes
• Searches for New Milky Way Satellites from the First Two Years of Data of the Subaru/Hyper Suprime-Cam Survey: Discovery of Cetus~III
• VERITAS Search for VHE Gamma-ray Emission from Dwarf Spheroidal Galaxies
• The role of luminous substructure in the gravitational lens system MG 2016+112
• GASP. X: APEX detection of molecular gas in the tails and in the disks of ram-pressure stripped galaxies
• The First Galaxies: Assembly under Radiative Feedback from the First Stars
• Effects of baryonic and dark matter substructure on the Pal 5 stream
• Bulk QCD Thermodynamics and Sterile Neutrino Dark Matter
• Small-scale clumps of dark matter
• AGN feedback in dwarf galaxies?
• The observability of gamma-rays from neutralino annihilations in Milky Way substructure
• Neutralino Annihilation at the Galactic Center Revisited
• X-ray line signal from 7 keV axino dark matter decay
• The second data release from the European Pulsar Timing Array: VI. Challenging the ultralight dark matter paradigm
• Next decade of sterile neutrino studies
• 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
• An unexpected high concentration for the dark substructure in the gravitational lens SDSSJ0946+1006
• The abundance of satellites around Milky Way- and M31-like galaxies with the TNG50 simulation: a matter of diversity
• Early Structure Formation and Reionization in a Cosmological Model with a Running Primordial Power Spectrum
• Semi-Analytical Models for the Formation of Disk Galaxies II. Dark Matter versus Modified Newtonian Dynamics
• The Epoch of Reionization in Models with Reduced Small Scale Power
• The Leo-I group: new dwarf galaxy and UDG candidates
• NIHAO X: Reconciling the local galaxy velocity function with Cold Dark Matter via mock HI observations
• Is the sky falling? Searching for stellar streams in the local Milky Way disc in the CORAVEL and RAVE surveys
• The SWELLS Survey. I. A large spectroscopically selected sample of edge-on late-type lens galaxies
• Shedding Light on the Galaxy Luminosity Function
• Modeling the Connection Between Subhalos and Satellites in Milky Way-like Systems
• Exploring Dark Matter with Milky Way substructure
• IMAGINE: A comprehensive view of the interstellar medium, Galactic magnetic fields and cosmic rays
• The properties of "dark" ΛCDM halos in the Local Group
• Core-collapse, evaporation and tidal effects: the life story of a self-interacting dark matter subhalo
• The abundance spread in the Bootes I dwarf spheroidal galaxy
• The signature of substructure on gravitational lensing in the LCDM cosmological model
• Sub-GeV dark matter as pseudo-Goldstone from the seesaw scale
• The masses of Local Group dwarf spheroidal galaxies: The death of the universal mass profile
• Dwarf Galaxies in CDM, WDM, and SIDM: Disentangling Baryons and Dark Matter Physics
• Self-Interacting Dark Matter through the Higgs Portal
• Cosmology with a dynamically screened scalar interaction in the dark sector
• The diverse dark matter density at sub-kiloparsec scales in Milky Way satellites:implications for the nature of dark matter
• Deviations from hydrostatic equilibrium in the circumgalactic medium: spinning hot haloes and accelerating flows
• Eddington-Born-Infeld gravity and the large scale structure of the Universe
• Disruption of satellite galaxies in simulated groups and clusters: the roles of accretion time, baryons, and pre-processing
• Scaling Laws for Dark Matter Halos in Late-Type and Dwarf Spheroidal Galaxies
• Lower Mass Bounds on FIMP Dark Matter Produced via Freeze-In
• The Varied Fates of z~2 Star-forming Galaxies
• The Fate of the First Galaxies. III. Properties of Primordial Dwarf Galaxies and their Impact on the Intergalactic Medium
• The BOSS Emission-Line Lens Survey. III. : Strong Lensing of Ly$\alpha$ Emitters by Individual Galaxies
• Stealth Galaxies in the Halo of the Milky Way
• A new low mass for the Hercules dSph: the end of a common mass scale for the dwarfs?
• MeV Dark Matter and Small Scale Structure
• Revealing dark matter substructure with anisotropies in the diffuse gamma-ray background
• Self-similar energetics in large clusters of galaxies
• Galactic Archaeology with Gaia
• NIHAO V: Too big doesn't fail -- reconciling the conflict between LCDM predictions and the circular velocities of nearby field galaxies
• Clustering properties of a sterile neutrino dark matter candidate
• Cosmic ray feedback from supernovae in dwarf galaxies
• Milky Way mass constraints from the Galactic satellite gap
• Two can play at that game: constraining the role of supernova and AGN feedback in dwarf galaxies with cosmological zoom-in simulations
• The Hubble Space Telescope Survey of M31 Satellite Galaxies I. RR Lyrae-based Distances and Refined 3D Geometric Structure
• Discovery of a new faint dwarf galaxy associated with NGC 253
• Resolved Dwarf Galaxy Searches within ~5 Mpc with the Vera Rubin Observatory and Subaru Hyper Suprime-Cam
• Shaken, not blown: the gentle baryonic feedback of nearby starburst dwarf galaxies
• Enrichment history of r-process elements shaped by a merger of neutron star pairs
• The Star Formation History of Leo T from Hubble Space Telescope Imaging
• Evidence of enrichment by individual supernova from elemental abundance ratios in the very metal-poor dSph galaxy Bootes I
• Extrinsic Radio Variability of JVAS/CLASS Gravitational Lenses
• GASTRO library I: the simulated chemodynamical properties of several GSE-like stellar halos
• Simulations of Strong Gravitational Lensing with Substructure
• Major Mergers of Galaxy Haloes: Cuspy or Cored Inner Density Profile?
• An Empirical Model for the Star Formation History in Dark Matter Halos
• The Leo IV dwarf spheroidal galaxy: color-magnitude diagram and pulsating stars
• The early-type dwarf galaxy population of the Centaurus cluster
• Serendipitous discovery of the unidentified extended TeV gamma-ray source HESS J1303-631
• On the morphologies, gas fractions, and star formation rates of small galaxies
• Analytical Approach to Subhaloes Population in Dark Matter Haloes
• Matter Power Spectrum in Hidden Neutrino Interacting Dark Matter Models: A Closer Look at the Collision Term
• Metal-Poor Stars and the Chemical Enrichment of the Universe
• Discovery of a red ultra-diffuse galaxy in a nearby void based on its globular cluster luminosity function
• Spectroscopic Survey of the Galaxy with Gaia II. The expected science yield from the Radial Velocity Spectrometer
• Signatures of Hierarchical Clustering in Dark Matter Detection Experiments
• New low surface brightness dwarf galaxies in the Centaurus group
• From galactic nuclei to the halo outskirts: tracing supermassive black holes across cosmic history and environments
• Super Heavy Dark Matter in light of BICEP2, Planck and Ultra High Energy Cosmic Rays Observations
• The Star Formation Rate Distribution Function of the Local Universe
• Gamma-ray background anisotropy from galactic dark matter substructure
• Effects of dynamical evolution on the distribution of substructures
• Accurate determination of the mass distribution in spiral galaxies III. Fabry-Perot imaging spectroscopy of 6 spiral galaxies
• X-ray line signal from decaying axino warm dark matter
• Discovery of Multiply Imaged Galaxies behind the Cluster and Lensed Quasar SDSS J1004+4112
• Suppressing structure formation at dwarf galaxy scales and below: late kinetic decoupling as a compelling alternative to warm dark matter
• SHARP - IV. An apparent flux ratio anomaly resolved by the edge-on disc in B0712+472
• Subhalo destruction in the Apostle and Auriga simulations
• Gas depletion in Local Group dwarfs on ~250 kpc scales: Ram pressure stripping assisted by internal heating at early times
• Dark Matter in the minimal Inverse Seesaw mechanism
• Substructure in the lens HE 0435-1223
• Cosmic Positron Signature from Dark Matter in the Littlest Higgs Model with T-parity
• Dark matter-radiation interactions: the structure of Milky Way satellite galaxies
• Impact of Dark Matter Microhalos on Signatures for Direct and Indirect Detection
• Kinematics of hypervelocity stars in the triaxial halo of the Milky Way
• An all-sky study of compact, isolated high-velocity clouds
• Small-scale structure formation properties of chilled sterile neutrinos as dark matter
• Static, spherically symmetric solutions with a scalar field in Rastall gravity
• Fast and energetic AGN-driven outflows in simulated dwarf galaxies
• Halo model description of the non-linear dark matter power spectrum at $k\gg 1$ Mpc${}^{-1}$
• Sterile neutrinos as subdominant warm dark matter
• Cosmology with the Large Synoptic Survey Telescope: an Overview
• The abundance of dark galaxies
• Tully-Fisher Relation and its Implications for Halo Density Profile and Self-interacting Dark Matter
• TeV $\gamma$-radiation from Dark Matter annihilation in the Galactic center
• Observational constraints on stellar feedback in dwarf galaxies
• In Pursuit of the Least Luminous Galaxies
• The velocity function of gas-rich galaxies
• Dark radiation from particle decay: cosmological constraints and opportunities
• Black hole in quantum wave dark matter
• Density profile slope in Dwarfs and environment
• Closing in on Resonantly Produced Sterile Neutrino Dark Matter
• Early galaxy formation in warm dark matter cosmologies
• High-Redshift Galaxy Outflows and the Formation of Dwarf Galaxies
• The impact of baryon physics on the structure of high-redshift galaxies
• Constraining the Projected Radial Distribution of Galactic Satellites with the Sloan Digital Sky Survey
• Lensing Optical Depth for Substructure and Isolated Dark Matter Halos
• Singlet-Doublet Dark Matter Freeze-in: LHC displaced signatures versus cosmology
• Bose-Einstein-condensed scalar field dark matter and the gravitational wave background from inflation: new cosmological constraints and its detectability by LIGO
• The effect of a disc on the population of cuspy and cored dark matter substructures in Milky Way-like galaxies
• Dark-Matter Decays and Self-Gravitating Halos
• Modeling Tidal Streams in evolving dark matter halos
• Prospects for chemically tagging stars in the Galaxy
• A New Giant Stellar Structure in the Outer Halo of M31
• New dwarf galaxy candidates in the Centaurus group
• Indirect detection of light neutralino dark matter in the NMSSM
• Dwarf elliptical galaxies as ancient tidal dwarf galaxies
• Halo Substructure Boosts to the Signatures of Dark Matter Annihilation
• 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
• Revealing the tidal scars of the Small Magellanic Cloud
• Asymmetric dark matter: residual annihilations and self-interactions
• ALFALFA Discovery of the Nearby Gas-rich Dwarf Galaxy Leo P. V. Neutral Gas Dynamics and Kinematics
• Globular Cluster Systems and the Missing Satellite Problem: Implications for Cold Dark Matter Models
• The halo+cluster system of the Galactic globular cluster NGC1851
• The Extended Star Formation History of the Andromeda Spheroid at Twenty One Kiloparsecs on the Minor Axis
• The baryonic mass function of galaxies
• Warm Dark Matter Constraints Using Milky-Way Satellite Observations and Subhalo Evolution Modeling
• The origin of low-surface-brightness galaxies in the dwarf regime
• Challenges in Detecting Gamma-Rays From Dark Matter Annihilations in the Galactic Center
• Implications of O and Mg abundances in metal-poor halo stars for stellar iron yields
• Effective Fluid Description of the Dark Universe
• Dark Matter signals from Draco and Willman 1: Prospects for MAGIC II and CTA
• A Targeted Survey for HI Clouds in Galaxy Groups
• How to Reconcile the Observed Velocity Function of Galaxies with Theory
• 3FGL Demographics Outside the Galactic Plane using Supervised Machine Learning: Pulsar and Dark Matter Subhalo Interpretations
• Connecting Reionization to the Local Universe
• Constraining the photon coupling of ultra-light dark-matter axion-like particles by polarization variations of parsec-scale jets in active galaxies
• Palomar 13: An Unusual Stellar System in the Galactic Halo
• Constraints on Warm Dark Matter models from high-redshift long gamma-ray bursts
• Detecting Dark Matter Substructures around the Milky Way with Gaia
• Self-interacting dark matter from an SU(3)_L \otimes U(1)_N electroweak model
• The Satellite Luminosity Functions of Galaxies in SDSS
• Modeling the Impact of Baryons on Subhalo Populations with Machine Learning
• Resolving phenomenological problems with strongly-interacting-massive-particle models with dark vector resonances
• Rhapsody. I. Structural Properties and Formation History From a Statistical Sample of Re-simulated Cluster-size Halos
• A Search for Light Fermionic Dark Matter Absorption on Electrons in PandaX-4T
• Probing the Epoch of Reionization with Milky Way Satellites
• A Comparison of Galaxy Merger History Observations and Predictions from Semi-Analytic Models
• Abundance ratios of red giants in low mass ultra faint dwarf spheroidal galaxies
• Dwarf Dark Matter Halos
• Signatures of LCDM substructure in tidal debris
• The Edge of the Galaxy
• Testing the Hypothesis of the Morphological Transformation from Field Spiral to Cluster S0
• On mini-halo encounters with stars
• The imprint of cosmic reionisation on the luminosity function of galaxies
• Radio, optical and infrared observations of CLASS B0128+437
• The early-type dwarf galaxy population of the Fornax cluster
• The Gamma-Ray-Flux Probability Distribution Function from Galactic Halo Substructure
• Boötes IV: A New Milky Way Satellite Discovered in the Subaru Hyper Suprime-Cam Survey and Implications for the Missing Satellite Problem
• SHARP - II. Mass structure in strong lenses is not necessarily dark matter substructure: A flux ratio anomaly from an edge-on disc
• The Evolution of Substructure in Galaxy, Group and Cluster Haloes II: Global Properties
• Resonant Sterile Neutrino Dark Matter in the Local and High-z Universe
• Observational Constraints on the Self Interacting Dark Matter Scenario and the Growth of Supermassive Black Holes
• Gravitational Waves as a New Probe of Bose-Einstein Condensate Dark Matter
• Sub-structure of the outer Galactic Halo from the 2 Micron All Sky Survey
• Boosting the annihilation boost: Tidal effects on dark matter subhalos and consistent luminosity modeling
• Constraints on the mass-concentration relation of cold dark matter halos with 11 strong gravitational lenses
• Star Clusters in Evolving Galaxies
• Self-interacting dark matter and Higgs bosons in the SU(3)_C x SU(3)_L x U(1)_N model with right-handed neutrinos
• Astrometric Perturbations in Substructure Lensing
• Limits on Supersymmetric Dark Matter From EGRET Observations of the Galactic Center Region
• 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
• Time-delay cosmographic forecasts with strong lensing and JWST stellar kinematics
• The Effective Theory of Self-Interacting Dark Matter
• An HST/ACS investigation of the spatial and chemical structure and sub-structure of NGC 891, a Milky Way analogue
• The luminosities of backsplash galaxies in constrained simulations of the Local Group
• An HI Survey of Six Local Group Analogs. II. HI properties of group galaxies
• On the Origin of Dynamically Cold Rings Around the Milky Way
• The distribution and morphologies of Fornax Cluster dwarf galaxies suggest they lack dark matter
• Dynamical and photometric imprints of feedback processes on the early evolution of E/S0 galaxies
• Dissecting a galaxy: mass distribution of 2237+0305
• The Carina Project: I. Bright Variable Stars
• The masses of satellites in GAMA galaxy groups from 100 square degrees of KiDS weak lensing data
• Extracting the Gamma Ray Signal from Dark Matter Annihilation in the Galactic Center Region
• Luminous Satellites of Early-Type Galaxies I: Spatial Distribution
• Active galactic nuclei and massive galaxy cores
• Subaru Mid-infrared Imaging of the Quadruple Lenses. II. Unveiling Lens Structure of MG0414+0534 and Q2237+030
• A Keck/DEIMOS spectroscopic survey of the faint M31 satellites And IX, And XI, And XII, and And XIII
• Hints against the cold and collisionless nature of dark matter from the galaxy velocity function
• On the assembly of the Milky Way dwarf satellites and their common mass scale
• The Baryons in the Milky Way Satellites
• Properties of Resonantly Produced Sterile Neutrino Dark Matter Subhalos
• Neutralino Dark Matter in Mirage Mediation
• The Dynamics of Subhalos in Warm Dark Matter Models
• Stellar Archaeology in the Galactic halo with Ultra-Faint Dwarfs: VII. Hercules
• Searching for diffuse light in the M96 Group
• Using gaps in N-body tidal streams to probe missing satellites
• Substructure around M31 : Evolution and Effects
• Clustering properties of galaxies selected in stellar mass: Breaking down the link between luminous and dark matter in massive galaxies from z=0 to z=2
• MOKA: a new tool for Strong Lensing Studies
• The phase-space distribution of infalling dark matter subhalos
• Draco, a flawless dwarf galaxy
• The Spatial Distribution of the Galactic First Stars I: High-Resolution N-body Approach
• Early formation of supermassive black holes via dark matter self-interactions
• Suppression of Star Formation in Low-Mass Galaxies Caused by the Reionization of their Local Neighborhood
• The sizes of mini-voids in the local universe: an argument in favor of a warm dark matter model?
• Small scale aspects of warm dark matter : power spectra and acoustic oscillations
• Bounds on velocity-dependent dark matter-proton scattering from Milky Way satellite abundance
• Searching for dark matter sterile neutrino in laboratory
• Violence in the Dark Ages
• An analytical model for the accretion of dark matter subhalos
• Subhalo Demographics in the Illustris Simulation: Effects of Baryons and Halo-to-Halo Variation
• A clear Dark Matter gamma ray line generated by the Green-Schwarz mechanism
• Phase space mass bound for fermionic dark matter from dwarf spheroidal galaxies
• Observational signatures of feedback in QSO absorption spectra
• Gas and stellar spiral structures in tidally perturbed disc galaxies
• Environmental mechanisms shaping the nature of dwarf spheroidal galaxies; the view of computer simulations
• Dark-Halo Cusp: Asymptotic Convergence
• Living with ghosts in Horava-Lifshitz gravity
• Luminosity Functions and Host-to-Host Scatter of Dwarf Satellite Systems in the Local Volume
• Finite Source Effects in Strong Lensing: Implications for the Substructure Mass Scale
• Radio constraints on dark matter annihilation in the galactic halo and its substructures
• Probing the nature of dark matter with accreted globular cluster streams
• A robust estimate of the Milky Way mass from rotation curve data
• Structure of the Galactic Stellar Halo Prior to Disk Formation
• Simulations of minor mergers. II. The phase-space structure of thick discs
• WIMP searches with gamma rays in the Fermi era: challenges, methods and results
• PAndAS in the mist: The stellar and gaseous mass within the halos of M31 and M33
• Direct and Indirect Detection of Neutralino Dark Matter In Selected Supersymmetry Breaking Scenarios
• Cosmic ray propagation and dark matter in light of the latest AMS-02 data
• The Structure of the Sagittarius Stellar Stream as Traced by Blue Horizontal Branch Stars
• Lepton flavor violating decays of vector quarkonia and of the $Z$ boson
• Bailing Out the Milky Way: Variation in the Properties of Massive Dwarfs Among Galaxy-Sized Systems
• Abundance of substructure in clusters of galaxies
• The Role of Gas In Maintaining Quasi-Steady Spiral Structure In Stellar Disks
• Numerical Simulations of High Redshift Star Formation in Dwarf Galaxies
• A fresh look into the interacting dark matter scenario
• An observer's guide to the (Local Group) dwarf galaxies: predictions for their own dwarf satellite populations
• Constraining Warm Dark Matter using QSO gravitational lensing
• Lyman-alpha Forest Constraints on Decaying Dark Matter
• A Realistic Model for Spatial and Mass Distributions of Dark Halo Substructures: An Analytic Approach
• The edge of galaxy formation I: formation and evolution of MW-satellites analogues before accretion
• A Keck/DEIMOS Kinematic Study of Andromeda IX: dark matter on the smallest galactic scales
• IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation
• Midlife Crises in Dwarf Galaxies in the NGC 5353/4 Group
• Microlensing of the Lensed Quasar SDSS0924+0219
• The Galaxy Luminosity Function from M_R = -25 to M_R = -9
• Dodelson-Widrow Production of Sterile Neutrino Dark Matter with Non-Trivial Initial Abundance
• Numerical Color-Magnitude Diagram Analysis of SDSS Data and Application to the New Milky Way satellites
• A Cosmic Coincidence: The Power-Law Galaxy Correlation Function
• Neutrino masses, leptogenesis and dark matter from small lepton number violation?
• About the morphology of dwarf spheroidal galaxies and their dark matter content
• An HI survey of six Local Group analogs: I. Survey description and the search for high-velocity clouds
• Fast and Slow Rotators in the Densest Environments: a SWIFT IFS study of the Coma Cluster
• Self-gravitating Vector Dark Matter
• The Splashback Radius of Planck-SZ clusters
• The universal rotation curve of low surface brightness galaxies IV: the interrelation between dark and luminous matter
• Detection of Substructure in the Gravitationally Lensed Quasar MG0414+0534 using Mid-Infrared and Radio VLBI Observations
• The shape of dark matter subhalos in the Aquarius simulations
• Emergence of a Dark Force in Corpuscular Gravity
• A missing outskirts problem? Comparisons between stellar halos in the Dragonfly Nearby Galaxies Survey and the TNG100 simulation
• The stellar structure and kinematics of dwarf spheroidal galaxies formed by tidal stirring
• Hunting the lightest lightest neutralinos
• The stability of stellar disks in Milky-Way sized dark matter halos
• Can cosmological simulations capture the diverse satellite populations of observed Milky Way analogues?
• How Biased Are Halo Properties in Cosmological Simulations?
• How low does it go? Too few Galactic satellites with standard reionization quenching
• Galaxy And Mass Assembly (GAMA): the red fraction and radial distribution of satellite galaxies
• Substructure Boosts to Dark Matter Annihilation from Sommerfeld Enhancement
• The dependence of tidal stripping efficiency on the satellite and host galaxy morphology
• Equilibrium configurations of 11eV sterile neutrinos in MONDian galaxy clusters
• The signature of dark energy on the local Hubble flow
• New Low Surface Brightness Dwarf Galaxies Detected Around Nearby Spirals
• Ruling out 3 keV warm dark matter using 21 cm-EDGES data
• Multipole Models of Four-Image Gravitational Lenses with Anomalous Flux Ratios
• Strong lensing signatures of luminous structure and substructure in early-type galaxies
• The LMC geometry and outer stellar populations from early DES data
• Globular Clusters in a Cosmological N-body Simulation
• The Influence of Galactic Outflows on the Formation of Nearby Dwarf Galaxies
• A Cosmological Kinetic Theory for the Evolution of Cold Dark Matter Halos with Substructure: Quasi-Linear Theory
• TriAnd and its Siblings: Satellites of Satellites in the Milky Way Halo
• Suppressing Linear Power on Dwarf Galaxy Halo Scales
• Analytical Solutions to the Mass-Anisotropy Degeneracy with Higher Order Jeans Analysis: A General Method
• The Bulge-Halo Connection in Galaxies: A Physical Interpretation of the Vcirc-sigma_0 Relation
• Signatures of Self-Interacting Dark Matter in the Matter Power Spectrum and the CMB
• Dark and luminous satellites of LMC-mass galaxies in the FIRE simulations
• Where are the High Velocity Clouds in Local Group Analogs?
• Are Newly Discovered HI High Velocity Clouds Minihalos in the Local Group?
• Structure of Dark Matter Halos in Warm Dark Matter models and in models with Long-Lived Charged Massive Particles
• Supersonic Relative Velocity between Dark Matter and Baryons: A Review
• Mapping the Galactic Halo III. Simulated Observations of Tidal Streams
• XENON1T Anomaly and its Implication for Decaying Warm Dark Matter
• ETHOS -- an effective theory of structure formation: predictions for the high-redshift Universe -- abundance of galaxies and reionization
• Stacking the Invisibles: A Guided Search for Low-Luminosity Milky Way Satellites
• Testing fundamental physics with distant star clusters: theoretical models for pressure-supported stellar systems
• An Improved Model for the Dynamical Evolution of Dark Matter Subhaloes
• Gauge mediation in supergravity and gravitino dark matter
• Shedding light on the small-scale crisis with CMB spectral distortions
• PeV Neutrinos and a 3.5 keV X-Ray Line from a PeV Scale Supersymmetric Neutrino Sector
• Dark Matter Indirect Signatures
• Constraints on Small-Scale Structures of Dark Matter from Flux Anomalies in Quasar Gravitational Lenses
• Reannihilation of self-interacting dark matter
• Collider and Dark Matter Phenomenology of Models with Mirage Unification
• Uncertain Times: The Redshift-Time Relation from Cosmology and Stars
• Confronting LCDM with Gravitational Lensing Constraints on Small Scale Structure
• Dwarf Galaxy Discoveries from the KMTNet Supernova Program I. The NGC 2784 Galaxy Group
• On the Random Motion of Nuclear Objects in a Fuzzy Dark Matter Halo
• A blind HI survey in the Canes Venatici region
• The Dwarfs Beyond: The Stellar-to-Halo Mass Relation for a New Sample of Intermediate Redshift Low Mass Galaxies
• Rhapsody. II. Subhalo Properties and the Impact of Tidal Stripping From a Statistical Sample of Cluster-Size Halos
• Newly discovered dwarf galaxies in the MATLAS low density fields
• An SDSS Survey For Resolved Milky Way Satellite Galaxies I: Detection Limits
• Effects of Early Cosmic Reionization on the Substructure Problem in Galactic Halo
• Dynamical Evidence of a Solitonic Core of $10^9{M}_{\odot }$ in the Milky Way
• Halo Structures of Gravitational Lens Galaxies
• Circular velocity profiles of dark matter haloes
• Galaxy stability within a self-interacting dark matter halo
• Motivations for a Large Self-Interacting Dark Matter Cross Section from Milky Way Satellites
• The joint evolution of baryons and dark matter haloes
• Structure of Axion Miniclusters
• Roll of the Dice: A Stochastically Sampled IMF Alters the Stellar Content of Simulated Dwarf Galaxies
• Dwarf Galaxies in the NGC 1023 Group
• Radio AGN in nearby dwarf galaxies: the important role of AGN in dwarf-galaxy evolution
• The Density Profile of Cluster-scale Dark Matter Halos
• Constraints on the merging timescale of luminous red galaxies, or, where do all the halos go?
• Dark radiation from the axino solution of the gravitino problem
• A detection of wobbling Brightest Cluster Galaxies within massive galaxy clusters
• Cosmological Constraints on Invisible Decay of Dark Matter
• Origin of Two Distinct Populations in Dwarf Spheroidal Galaxies
• Superdense cosmological dark matter clumps
• Andromeda XXIX: A New Dwarf Spheroidal Galaxy 200kpc from Andromeda
• Hunting for super-heavy dark matter with the highest-energy cosmic rays
• Probing dark matter with star clusters: a dark matter core in the ultra-faint dwarf Eridanus II
• Ultra Compact Dwarf galaxies in Abell 1689: a photometric study with the ACS
• Prospects for Detecting Neutrino Signals from Annihilating/Decaying Dark Matter to Account for the PAMELA and ATIC results
• Cosmological simulations in MOND: the cluster scale halo mass function with light sterile neutrinos
• Early-Type galaxies at z ~ 1.3. III. On the dependence of Formation Epochs and Star Formation Histories on Stellar Mass and Environment
• Solitons in the dark: non-linear structure formation with fuzzy dark matter
• Determining the WIMP mass using the complementarity between direct and indirect searches and the ILC
• Modified Dust and the Small Scale Crisis in CDM
• A limit on the warm dark matter particle mass from the redshifted 21 cm absorption line
• Dissipative Dark Matter on FIRE: I. Structural and kinematic properties of dwarf galaxies
• Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
• Cold Dark Matter's Small Scale Crisis Grows Up
• Self-interacting dark matter from late decays and the $H_0$ tension
• Too small to succeed? Lighting up massive dark matter subhaloes of the Milky Way
• A wide-field photometric survey for extratidal tails around five metal-poor globular clusters in the Galactic halo
• The full Boltzmann hierarchy for dark matter-massive neutrino interactions
• Unstable Cold Dark Matter and the Cuspy Halo Problem in Dwarf Galaxies
• The dark matter assembly of the Local Group in constrained cosmological simulations of a LambdaCDM universe
• Dark-matter decays and Milky Way satellite galaxies
• Ultra-Light Axion Dark Matter and its impacts on dark halo structure in $N$-body simulation
• Dark matter from late decays and the small-scale structure problems
• Galaxy evolution from strong lensing statistics: the differential evolution of the velocity dispersion function in concord with the LambdaCDM paradigm
• The Density Profile of the Dark Matter Halo of NGC 4605
• Simulated ΛCDM analogues of the thin Plane of Satellites around the Andromeda galaxy are not kinematically coherent structures
• Cold Dark Matter Substructures in Early-Type Galaxy Halos
• Dynamical Effects of CDM Subhalos on a Galactic Disk
• Size matters: the non-universal density profile of subhaloes in SPH simulations and implications for the Milky Way's dSphs
• Looking for a Heavy Higgsino LSP in Collider and Dark Matter Experiments
• Viscous dark matter growth in (neo-)Newtonian cosmology
• Detection of a Companion Lens Galaxy using the Mid-infrared Flux Ratios of the Gravitationally Lensed Quasar H1413+117
• Stellar Metallicities and Kinematics in a Gas-Rich Dwarf Galaxy: First Calcium Triplet Spectroscopy of RGB Stars in WLM
• The Satellite Luminosity Function of M101 into the Ultra-Faint Dwarf Galaxy Regime
• Gravitational lensing as a probe of cold dark matter subhalos
• Galaxy Clusters in the Context of Superfluid Dark Matter
• Satellite Galaxy Number Density Profiles in the Sloan Digital Sky Survey
• Structure Formation with Scalar Field Dark Matter: The Fluid Approach
• Pulsar timing residual induced by ultralight tensor dark matter
• Massive Milky Way Satellites in Cold and Warm Dark Matter: Dependence on Cosmology
• The Detection of Pure Dark Matter Objects with Bent Multiply Imaged Radio Jets
• The Halos and Environments of Nearby Galaxies (HERON) I: Imaging, Sample Characteristics, and Envelope Diameters
• What sets the central structure of dark matter haloes?
• The Via Lactea INCITE Simulation: Galactic Dark Matter Substructure at High Resolution
• The Evolution of Substructure in Galaxy, Group and Cluster Haloes III: Comparison with Simulations
• High-resolution imaging of compact high-velocity clouds (II)
• The Role of Heating and Enrichment in Galaxy Formation
• Fate of scalar dark matter solitons around supermassive galactic black holes
• Have Atmospheric Cerenkov Telescopes Observed Dark Matter?
• The Effects of Patchy Reionization on Satellite Galaxies of the Milky Way
• The effect of low mass substructures on the Cusp lensing relation
• Flybys, orbits, splashback: subhalos and the importance of the halo boundary
• A 2MASS All-Sky View of the Sagittarius Dwarf Galaxy: VII. Kinematics of the Main Body of the Sagittarius dSph
• Upper limits on DM annihilation cross sections from the first AMS-02 antiproton data
• Cold dark matter plus not-so-clumpy dark relics
• The Distribution of Satellite Galaxies in a Lambda-CDM Universe
• Properties of satellite galaxies in the SDSS photometric survey: luminosities, colours and projected number density profiles
• Milky Way total Mass derived by Rotation Curve and Globular Cluster kinematics from Gaia EDR3
• Constraining Primordial Black Holes using Fast Radio Burst Gravitational-Lens Interferometry with CHIME/FRB
• Dynamical evidence for a strong tidal interaction between the Milky Way and its satellite, Leo V
• Theoretical Aspects of Gravitational Lensing in TeVeS
• Constraining ultralight vector dark matter with the Parkes Pulsar Timing Array second data release
• Multiple Ultralight Axionic Wave Dark Matter and Astronomical Structures
• Effects of Unstable Dark Matter on Large-Scale Structure and Constraints from Future Surveys
• Relics of structure formation: extra-planar gas and high-velocity clouds around the Andromeda Galaxy
• Satellite dwarf galaxies: Stripped but not quenched
• Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations
• Joint constraints on the Galactic dark matter halo and Galactic Centre from hypervelocity stars
• On the density of Cold Dark Matter
• No evidence for a dark matter disk within 4 kpc from the Galactic plane
• The LBT Satellites of Nearby Galaxies Survey (LBT-SONG): The Satellite Population of NGC 628
• On the density profile of dark matter substructure in gravitational lens galaxies
• A Comprehensive Archival Search for Counterparts to Ultra-Compact High Velocity Clouds: Five Local Volume Dwarf Galaxies
• Fingerprints of the initial conditions on the density profiles of cold and warm dark matter haloes
• Using dwarf satellite proper motions to determine their origin
• On Ellipsoidal Collapse and Primordial Black-Hole Formation
• Dwarf galaxies in the Dynamically Evolved NGC 1407 Group
• Wormholes in the f(R,L,T) theory of gravity
• Observations of radio-quiet quasars at 10mas resolution by use of gravitational lensing
• The Tidal Streams of Disrupting Subhaloes in Cosmological Dark Matter Haloes
• A Dark Census: Statistically Detecting the Satellite Populations of Distant Galaxies
• Reconciling MOND and dark matter?
• The Observational Mass Function of Loose Galaxy Groups
• Tidal Stirring of Disky Dwarfs with Shallow Dark Matter Density Profiles: Enhanced Transformation into Dwarf Spheroidals
• The Cosmic Evolution of Faint Satellite Galaxies as a Test of Galaxy Formation and the Nature of Dark Matter
• Mechanisms of Baryon Loss for Dark Satellites in Cosmological SPH Simulations
• Axino warm dark matter and ${\Omega }_b-{\Omega }_{DM}$ coincidence
• Variable stars in the field of the Hydra II ultra-faint dwarf galaxy
• The effect of Warm Dark Matter on galaxy properties: constraints from the stellar mass function and the Tully-Fisher relation
• Streams on FIRE: Populations of Detectable Stellar Streams in the Milky Way and FIRE
• Warm FIRE: Simulating Galaxy Formation with Resonant Sterile Neutrino Dark Matter
• On the status of superheavy dark matter
• Hubble Space Telescope Observations of NGC 253 Dwarf Satellites: Discovery of Three Ultra-faint Dwarf Galaxies
• Simulated void galaxies in the standard cold dark matter model
• Core-Halo Mass Relation in Scalar Field Dark Matter Models and its Consequences for the Formation of Supermassive Black Holes
• Subhalo statistics of galactic halos: beyond the resolution limit
• From Images to Dark Matter: End-To-End Inference of Substructure From Hundreds of Strong Gravitational Lenses
• Evidence for Early Filamentary Accretion from the Andromeda Galaxy's Thin Plane of Satellites
• On prospects for dark matter indirect detection in the Constrained MSSM
• The Effect of a Single Supernova Explosion on the Cuspy Density Profile of a Small-Mass Dark Matter Halo
• Warm dark matter and the ionization history of the Universe
• On the stark difference in satellite distributions around the Milky Way and Andromeda
• A persistent excess of galaxy-galaxy strong lensing observed in galaxy clusters
• The velocity anisotropy of the Milky Way satellite system
• With and without spectroscopy: Gaia DR2 proper motions of seven Ultra-Faint Dwarf Galaxies
• The clustering of ultra-high energy cosmic rays and their sources
• High Resolution HI Observations of the Galaxy NGC404: a dwarf S0 with abundant Interstellar gas
• The Nature of the Density Clump in the Fornax Dwarf Spheroidal Galaxy
• Strong lensing reveals jets in a sub-microJy radio quiet quasar
• Small-scale shear: Peeling off diffuse subhalos with gravitational waves
• On the scarcity of Magellanic Cloud-like satellites
• A Keck/DEIMOS spectroscopic survey of the faint M31 satellites And XV and And XVI
• Exploring the hidden Universe: A novel phenomenological approach for recovering arbitrary gravitational-wave millilensing configurations
• The Absence of Stars in Compact High-Velocity Clouds
• The Density Structure of Simulated Stellar Streams
• Substructure Lensing: Effects of Galaxies, Globular Clusters & Satellite Streams
• Implications of Milky Way Substructures for the Nature of Dark Matter
• New distances of unresolved dwarf elliptical galaxies in the vicinity of the Local Group
• Galaxy formation with radiative and chemical feedback
• Propagation of high-energy neutrinos in a background of ultralight scalar dark matter
• Constraints on cosmological viscosity and self interacting dark matter from gravitational wave observations
• Eppur si muove: Positional and kinematic correlations of satellite pairs in the low Z universe
• How Late can the Dark Matter form in our universe?
• Power spectrum tomography of dark matter annihilation with local galaxy distribution
• Ultra-Compact High Velocity Clouds as Minihalos and Dwarf Galaxies
• Neutron Star Stability in Light of the Neutron Decay Anomaly
• Dark matter from the scalar sector of 3-3-1 models without exotic electric charges
• Phase-Space Structure of Dark-Matter Haloes: Scale-Invariant PDF Driven by Substructure
• Indirect Detection of Dark Matter with gamma rays
• Generalised teleparallel quintom dark energy non-minimally coupled with the scalar torsion and a boundary term
• Dark Matter in the Local Universe
• On the common mass scale of the Milky Way satellites
• Astrometric Microlensing by Local Dark Matter Subhalos
• Spontaneous generation of bending waves in isolated Milky Way-like discs
• Growth of First Galaxies: Impacts of Star Formation and Stellar Feedback
• Two Local Volume Dwarf Galaxies Discovered in 21 cm Emission: Pisces A and B
• Constraints on thick disc and halo parameters from HST photometry of field stars in the Galaxy
• Population III Star Formation in a Lambda WDM Universe
• ASOHF: a new adaptive spherical overdensity halo finder
• Status of Cold Dark Matter Cosmology
• An HI survey of the Centaurus and Sculptor Groups - Constraints on the space density of low mass galaxies
• Stellar Substructures around the Hercules Dwarf Spheroidal Galaxy
• Cosmological Simulations of Multi-Component Cold Dark Matter
• The tangential velocity excess of the Milky Way satellites
• The Influence of Mass-Loss from a Star Cluster on its Dynamical Friction -- I. Clusters without Internal Evolution
• The Expected Mass Function for Low Mass Galaxies in a CDM Cosmology: Is There a Problem?
• Observation of small scale structure using sextupole lensing
• The effect of tides on the Fornax dwarf spheroidal galaxy
• Constraints on warm dark matter from UV luminosity functions of high-z galaxies with Bayesian model comparison
• The galaxy-subhalo connection in low-redshift galaxy clusters from weak gravitational lensing
• Satellites in MW-like hosts: Environment dependence and close pairs
• ALMA Imprint of Intergalactic Dark Structures in the Gravitational Lens SDP.81
• Dark Matter And $B_s\to {\mu }^{+}{\mu }^{-}$ With Minimal $S{O}_{10}$ Soft SUSY Breaking II
• Anomalies in Time Delays of Lensed Gravitational Waves and Dark Matter Substructures
• Lyman-$\alpha$ forest constraints on interacting dark sectors
• Probing the Low Surface Brightness Dwarf Galaxy Population of the Virgo Cluster
• Damped Lyman alpha systems and galaxy formation models - II. High ions and Lyman limit systems
• Neutral Hydrogen Clouds near Early-Type Dwarf Galaxies of the Local Group
• Constraints on anharmonic corrections of Fuzzy Dark Matter
• Detection of satellite remnants in the Galactic Halo with Gaia - I. The effect of the Galactic background, observational errors and sampling
• LCDM Satellites and HI Companions - The Arecibo ALFA Survey of NGC 2903
• The Survey of Centaurus A's Baryonic Structures (SCABS). II. The Extended Globular Cluster System of NGC5128 and its Nearby Environment
• Light to Mass Variations with Environment
• Probing the small-scale structure in strongly lensed systems via transdimensional inference
• Asymmetric Surface Brightness Structure of Caustic Crossing Arc in SDSS J1226+2152: A Case for Dark Matter Substructure
• Probing for Dark Matter within Spiral Galaxy Disks
• Lifetime Constraints for Late Dark Matter Decay
• The infall of dwarf satellite galaxies are influenced by their host's massive accretions
• Constraints on mixed dark matter from anomalous strong lens systems
• Dependence of the Local Reionization History on Halo Mass and Environment: Did Virgo Reionize the Local Group?
• Gravitational cooling and density profile near caustics in collisionless dark matter haloes
• Evolution of perturbations and cosmological constraints in decaying dark matter models with arbitrary decay mass products
• Impact of cosmological satellites on the vertical heating of the Milky Way disc
• Tidal-induced lopsidedness in Magellanic-type galaxies
• SHIELD: Neutral Gas Kinematics and Dynamics
• Arecibo imaging of compact high-velocity clouds
• The impact of correlated projections on weak lensing cluster counts
• Effelsberg HI observations of compact high-velocity clouds
• Delayed pulsar kicks from the emission of sterile neutrinos
• Extended Source Effects in Substructure Lensing
• Galaxy Formation: Warm Dark Matter, Missing Satellites, and the Angular Momentum Problem
• Quark stars with 2.6 $M_{\odot }$ in a non-minimal geometry-matter coupling theory of gravity
• Tidal radii of globular clusters and the mass of the Milky Way
• Galaxy Satellites and the Weak Equivalence Principle
• Wavelet Approach to Search for Sterile Neutrinos in Tritium $\beta$-Decay Spectra
• HI Observations of Five Groups of Galaxies
• Dragonfly imaging of the galaxy NGC5907: a revised view of the iconic stellar stream
• Structure formation in a $\Lambda$ $viscous$ CDM universe
• Precision Cosmology
• A comparative study of satellite galaxies in Milky Way-like galaxies from HSC, DECaLS and SDSS
• Using distant globular clusters as a test for gravitational theories
• Modelling the Milky Way through adiabatic compression of cold dark matter halo
• Simulating tidal streams in a high resolution dark matter halo
• Dark Matter Signatures in the Anisotropic Radio Sky
• The Dark Matter Annihilation Signal from Dwarf Galaxies and Subhalos
• Jeans type instability of a complex self-interacting scalar field in general relativity
• Mapping the Tidal Disruption of the Hercules Dwarf: A Wide-Field DECam Imaging Search for RR Lyrae Stars
• A Wide-Field View of Leo II -- A Structural Analysis Using the SDSS
• Companions to Isolated Elliptical Galaxies: Revisiting the Bothun-Sullivan Sample
• Nature of branon dark matter
• Equation of State of Dark Matter after Planck Data
• Streams Going Notts: The tidal debris finder comparison project
• Early-type dwarf galaxies in clusters: a mixed bag with various origins?
• Warm Dark Matter in B-L Inverse Seesaw
• Statistics of Substructures in Dark Matter Haloes
• The Smith Cloud and its dark matter halo: Survival of a Galactic disc passage
• Low-mass suppression of the satellite luminosity function due to the supersonic baryon--cold-dark-matter relative velocity
• Schrödinger-Poisson Solitons: Perturbation Theory
• Early formation of galaxies initiated by clusters of primordial black holes
• Constraining the Collisional Nature of the Dark Matter Through Observations of Gravitational Wakes
• The Cluster Galaxy Circular Velocity Function
• The Effects of Dark Matter and Baryonic Physics on the Milky Way Subhalo Population in the Presence of the Large Magellanic Cloud
• The scaling relations of galaxy clusters and their dark matter halos
• Mixed dark matter: matter power spectrum and halo mass function
• Satellite number density profiles of primary galaxies in the 2dFGRS
• Constraining the primordial magnetic field with dwarf galaxy simulations
• Constraining global properties of the Draco dwarf spheroidal galaxy
• Identifying Dark Matter Annihilation Products In The Diffuse Gamma Ray Background
• Multifield Ultralight Dark Matter
• The Cold Dark Matter crisis on galactic and subgalactic scales
• High-Velocity Clouds in the Nearby Spiral Galaxy M 83
• Carbon Stars and other Luminous Stellar Populations in M33
• The Clustering and Host Halos of Galaxy Mergers at High Redshift
• Indirect search for dark matter: prospects for GLAST
• Integral Field Spectroscopy of the Quadruply Lensed Quasar 1RXS J1131-1231: New Light on Lens Substructures
• The challenge of large and empty voids in the SDSS DR7 redshift survey
• Bound and unbound substructures in Galaxy-scale Dark Matter haloes
• Self-heating dark matter via semi-annihilation
• Using CMB spectral distortions to distinguish between dark matter solutions to the small-scale crisis
• The baryonic mass-velocity relation; clues to feedback processes during structure formation and the cosmic baryon inventory
• Discovery and analysis of low-surface-brightness galaxies in the environment of NGC 1052
• The Milky Way system in LCDM cosmological simulations
• The Lens Galaxy In PG1115+080 is an Ellipse
• Density Variations in the NW Star Stream of M31
• Solar Neutrinos as a Probe of Dark Matter-Neutrino Interactions
• On Dark Matter Annihilation in the Local Group
• On the isolated dwarf galaxies: from cuspy to flat dark matter density profiles and metallicity gradients
• Hubble Space Telescope Observations of Two Faint Dwarf Satellites of Nearby LMC Analogs from MADCASH
• Variation of the subhalo abundance in dark matter halos
• The dark matter transfer function: free streaming, particle statistics and memory of gravitational clustering
• Morphological Evolution of Dwarf Galaxies in the Local Group
• Origin of Delta N_eff as a Result of an Interaction between Dark Radiation and Dark Matter
• The SIBELIUS Project: E Pluribus Unum
• Models of Disk Evolution: Confrontation with Observations
• Dark radiation and small-scale structure problems with decaying particles
• Has DAMA Detected Self-Interacting Dark Matter?
• The effects of a hot gaseous halo on disc thickening in galaxy minor mergers
• Dwarf Galaxy Mass Estimators vs. Cosmological Simulations
• Soliton Formation and the Core-Halo Mass Relation: An Eigenstate Perspective
• Tidal Stripping in the Adiabatic Limit
• Constraining self-interacting dark matter with scaling laws of observed halo surface densities
• 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
• Pegasus W: An Ultra-Faint Dwarf Galaxy Outside the Halo of M31 Not Quenched by Reionization
• Impact of kinetic and potential self-interactions on scalar dark matter
• Free-free absorption in the gravitational lens JVAS B0218+357
• Spatial Origin of Galactic Cosmic Rays in Diffusion Models: II- Exotic Primary Cosmic Rays
• Dark satellites and the morphology of dwarf galaxies
• Axionic Mirage Mediation
• Toward Understanding the origin of the Fundamental Plane for Early-Type Galaxies
• A low pre-infall mass for the Carina dwarf galaxy from disequilibrium modelling
• Perturbations of ultralight vector field dark matter
• Does the Milky Way Obey Spiral Galaxy Scaling Relations?
• The Mass Function of Unprocessed Dark Matter Halos and Merger Tree Branching Rates
• Using wavelets to capture deviations from smoothness in galaxy-scale strong lenses
• The Signatures of Self-Interacting Dark Matter and Subhalo Disruption on Cluster Substructure
• And In The Darkness Unbind Them: High-Resolution Simulations of Dark Matter Subhalo Disruption in a Milky Way-like Tidal Field
• ETHOS - an Effective Theory of Structure Formation: detecting dark matter interactions through the Lyman-$\alpha$ forest
• Cosmological searches for a non-cold dark matter component
• Charting Unexplored Dwarf Galaxy Territory With RR Lyrae
• Galaxy subgroups in galaxy clusters
• Tidal Imprints of a Dark Sub-Halo on the Outskirts of the Milky Way II. Perturber Azimuth
• Satellite galaxies in hydrodynamical simulations of Milky Way sized galaxies
• Simulations of galactic disks including a dark baryonic component
• Encounters between spherical galaxies II: systems with dark halo
• A search for low surface brightness dwarf galaxies in different environments
• Discs in early-type lensing galaxies: effects on magnification ratios and measurements of $H_0$
• MaGICC-WDM: the effects of warm dark matter in hydrodynamical simulations of disc galaxy formation
• Observed Properties of Dark Matter on Small Spatial Scales
• Improved strong lensing modelling of galaxy clusters using the Fundamental Plane: Detailed mapping of the baryonic and dark matter mass distribution of Abell S1063
• Local Group Dwarf Galaxies and the Fundamental Manifold of Spheroids
• Evolution of linear wave dark matter perturbations in the radiation-dominant era
• Modelling the dynamical evolution of the Bootes dwarf spheroidal galaxy
• Gravitational Lensing - Einstein's Unfinished Symphony
• Constraints and cosmography of $\Lambda$CDM in presence of viscosity
• Confronting fuzzy dark matter with the rotation curves of nearby dwarf irregular galaxies
• Fine Structure of Dark Matter Halos and its Effect on Terrestrial Detection Experiments
• Three-dimensional Mapping of CDM Substructure at Submillimeter Wavelengths
• Gamma-Ray Constraints on Neutralino Dark Matter Clumps in the Galactic Halo
• Predictably Missing Satellites: Subhalo Abundance in Milky Way-like Halos
• A deep view on the Virgo cluster core
• Where are All the Gas-Bearing Local Dwarf Galaxies? Quantifying Possible Impacts of Reionization
• Constraints on Chameleon f(R)-Gravity from Galaxy Rotation Curves of the SPARC Sample
• Estimating the warm dark matter mass from strong lensing images with truncated marginal neural ratio estimation
• The Bound Mass of Substructures in Dark Matter Halos
• The Missing Satellite Problem in 3D
• Structural analysis of the Sextans dwarf spheroidal galaxy
• Probing wave-optics effects and low-mass dark matter halos with lensing of gravitational waves from massive black holes
• Constraints on dark matter-neutrino scattering from the Milky-Way satellites and subhalo modeling for dark acoustic oscillations
• Constraints on self-interacting Q-ball dark matter
• Comparison between the Logotropic and $\Lambda$CDM models at the cosmological scale
• $\Lambda$CDM Predictions for the Satellite Population of M33
• Joining X-ray to lensing: an accurate combined analysis of MACS J0416.1$-$2403
• Power spectrum for the small-scale Universe
• The Angular Momentum Distribution within Halos in Different Dark Matter Models
• Simulating the H2 content of high-redshift galaxies
• Flattened structures of dwarf satellites around massive host galaxies in the MATLAS low-to-moderate density fields
• Under the sword of Damocles: plausible regeneration of dark matter cusps at the smallest galactic scales
• Degenerate sterile neutrino dark matter in the cores of galaxies
• Measuring the Small-Scale Matter Power Spectrum with High-Resolution CMB Lensing
• Constraining warm dark matter with 21 cm line fluctuations due to minihalos
• Evidence for a Galactic Origin of Very Short Gamma Ray Bursts and Primordial Black Hole Sources
• Dispersal of tidal debris in a Milky-Way-sized dark matter halo
• Warm Dark Matter and Cosmic Reionization
• Initial Conditions for Imperfect Dark Matter
• A census of the expected properties of classical Milky Way dwarfs in Milgromian dynamics
• Biased Galaxy Formation And Measurements Of Beta
• Globular Cluster Formation from Colliding Substructure
• Free streaming in mixed dark matter
• Morphological properties of galaxies in different Local Volume environments
• Towards constraining warm dark matter with stellar streams through neural simulation-based inference
• Understanding the Results of Galaxy-Galaxy Lensing using Galaxy-Mass Correlation in Numerical Simulations
• Constraints on the epoch of dark matter formation from Milky Way satellites
• Effects of galaxy--satellite interactions on bar formation
• $Z^{\prime }$ portal to Chern-Simons Dark Matter
• The mass-metallicity relation of tidal dwarf galaxies
• Cosmological Structure Formation in Decaying Dark Matter Models
• The Cosmological Significance of High-Velocity Cloud Complex H
• Statistical properties of the dark matter haloes of dwarf galaxies and correlations with the environment
• On the equilibrium morphology of systems drawn from spherical collapse experiments
• Stellar and Gas properties of High HI Mass-to-Light Ratio Galaxies in the Local Universe
• Noise-driven evolution in stellar systems: A universal halo profile
• Testing keV sterile neutrino dark matter in future direct detection experiments
• Star Formation and Feedback in Dwarf Galaxies
• Decaying Superheavy Dark Matter and Subgalactic Structure of the Universe
• The abundance of dwarf galaxies around low-mass giants in the Local Volume
• SDSS Survey for Resolved Milky Way Satellite Galaxies II: High-Velocity Clouds in the Early Data Release
• Dark matter detection in the BMSSM
• Dissecting Galaxy Formation: II. Comparing Substructure in Pure Dark Matter and Baryonic Models
• A Wide Field Survey of Satellite Galaxies around the Spiral Galaxy M106
• The HI environment of the Sculptor dwarf spheroidal galaxy
• Can proper motions of dark-matter subhalos be detected?
• Searching For Dark Matter with Neutrino Telescopes
• High-energetic Cosmic Antiprotons from Kaluza-Klein Dark Matter
• On measuring the Galactic dark matter halo with hypervelocity stars
• Dark Matter Subhalos and the X-ray Morphology of the Coma Cluster
• Assessing the impact of bulk and shear viscosities on large scale structure formation
• Completely dark galaxies: their existence, properties, and strategies for finding them
• The non-thermal superbubble in IC 10: the generation of cosmic ray electrons caught in the act
• Primordial Black Hole Merger Rate in Ellipsoidal-Collapse Dark Matter Halo Models
• Degenerate Sub-keV Fermion Dark Matter from a Solution to the Hubble Tension
• On the metallicity distribution of the peculiar globular cluster M22
• Simulations of core formation for frequent dark matter self-interactions
• Compact HI clouds from the GALFA-HI survey
• The Spectrum of Darkonium in the Sun
• High-resolution three-dimensional simulations of gas removal from ultrafaint dwarf galaxies. I. Stellar feedback
• Relating the Diverse Merger Histories and Satellite Populations of Nearby Galaxies
• A New Method to Constrain the Appearance and Disappearance of Observed Jellyfish Galaxy Tails
• ETHOS -- An effective parametrization and classification for structure formation: the non-linear regime at $z\gtrsim 5$
• Implications of Compressed Supersymmetry for Collider and Dark Matter Searches
• Formulation and constraints on decaying dark matter with finite mass daughter particles
• The Effects of Varying Cosmological Parameters on Halo Substructure
• Gas Accretion by Globular Clusters and Nucleated Dwarf Galaxies and the Formation of the Arches and Quintuplet Clusters
• Modeling star formation in dwarf spheroidal galaxies: a case for extended dark matter halos
• Self-interacting freeze-in dark matter in a singlet doublet scenario
• Scalar Field Dark Matter Spectator During Inflation: The Effect of Self-interaction
• Could Dark Matter Interactions be an Alternative to Dark Energy ?
• Reionization in the Warm Dark Matter Model
• Sub-GeV galactic cosmic-ray antiprotons from primordial black holes in the Randall-Sundrum braneworld
• Confirmation of Planet-Mass Objects in Extragalactic Systems
• Low Scale Leptogenesis and Dark Matter Candidates in an Extended Seesaw Model
• Shapes of Milky-Way-Mass Galaxies with Self-Interacting Dark Matter
• DGSAT: Dwarf Galaxy Survey with Amateur Telescopes II. A catalogue of isolated nearby edge-on disk galaxies and the discovery of new low surface brightness systems
• A cosmological study of the star formation history in the solar neighbourhood
• The connection between the cusp-to-core transformation and observational universalities of DM halos
• Dark Matter Bound State Formation in Fermionic $Z_2$ DM model with Light Dark Photon and Dark Higgs Boson
• Decaying Dark Matter and the Deficit of Dwarf Haloes
• History of Hydrogen Reionization in the Cold Dark Matter Model
• Nonthermal dark matter in mirage mediation
• Cosmic Renaissance: The First Sources of Light
• Impact of sterile neutrino dark matter on core-collapse supernovae
• Looking at the Fundamental Plane through a gravitational lens
• Fast Identification of Bound Structures in Large N-body Simulations
• The Milky Way's rotation curve with superfluid dark matter
• Cosmological Simulations of Dwarf Galaxies with Cosmic Ray Feedback
• Baryonic effects on the detectability of annihilation radiation from dark matter subhaloes around the Milky Way
• Cosmic evolution of bars in simulations of galaxy formation
• The role of AGN feedback on the evolution of dwarf galaxies from cosmological simulations: SMBHs suppress star formation in low-mass galaxies
• A MegaCam Survey of Outer Halo Satellites. I. Description of the Survey
• On dark matter - dark radiation interaction and cosmic reionization
• The Very Knotty Lenser: exploring the role of regularization in source and potential reconstructions using Gaussian Process Regression
• Are ancient dwarf satellites the building blocks of the Galactic halo?
• Constraints via the Event Horizon Telescope for Black Hole Solutions with Dark Matter under the Generalized Uncertainty Principle Minimal Length Scale Effect
• Looking for a heavy wino LSP in collider and dark matter experiments
• Discovery prospects with the Dark-photons & Axion-Like particles Interferometer
• Subhaloes in Scale-Free Cosmologies
• Two Distant Halo Velocity Groups Discovered by the Palomar Transient Factory
• GOGREEN: a critical assessment of environmental trends in cosmological hydrodynamical simulations at z ~ 1
• Dark Matter Search in Space: Combined Analysis of Cosmic Ray Antiproton-to-Proton Flux Ratio and Positron Flux Measured by AMS-02
• Endothermic self-interacting dark matter in Milky Way-like dark matter haloes
• Extended stellar substructure surrounding the Boötes I dwarf spheroidal galaxy
• Serendipitous discovery of RR Lyrae stars in the Leo V ultra-faint galaxy
• The SPLASH Survey: A Spectroscopic Analysis of the Metal-Poor, Low-Luminosity M31 dSph Satellite Andromeda X
• The reionization of galactic satellite populations
• The effect of tides on the Sculptor dwarf spheroidal galaxy
• QSO Absorption Line Constraints on Intragroup High-Velocity Clouds
• Long-Range Correlations in Self-Gravitating N-Body Systems
• Andromeda IX: Properties of the Smallest M 31 Dwarf Satellite Galaxy
• Is a Simple Collisionless Relic Dark Matter Particle Ruled Out?
• Constraints of the Clumpyness of Dark Matter Halos Through Heating of the Disk Galaxies
• Galaxy And Mass Assembly (GAMA): detection of low-surface-brightness galaxies from SDSS data
• The halo mass function and inner structure of ETHOS haloes at high redshift
• Constraints on nature of ultra light dark matter particles with 21cm forest
• Gravitationally Bound Bose Condensates with Rotation
• The impact of cored density profiles on the observable quantities of dwarf spheroidal galaxies
• Scalar dark matter and leptogenesis in the minimal scotogenic model
• The Missing Satellite Problem Outside of the Local Group: I -- Pilot Observation
• HI Observations of an Ultra-Compact High-Velocity Cloud
• Cosmology with Long-Lived Charged Massive Particles
• Real- and redshift-space halo clustering in $f(R)$ cosmologies
• Analytical Approach to the Mass Distribution Function of Subhalos and Cold Fronts in Galaxy Clusters
• Constraining Warm Dark Matter and Pop III stars with the Global 21-cm Signal
• On the Cosmic Web Elongation in Fuzzy Dark Matter Cosmologies: Effects on Density Profiles, Shapes and Alignments of Halos
• Distant star clusters of the Milky Way in MOND
• 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 effects of Non-Gaussian initial conditions on the structure and substructure of Cold Dark Matter halos
• Light Dark Matter Annihilations into Two Photons
• Effects of halo substructure on the power spectrum and bispectrum
• High resolution simulations of the reionization of an isolated Milky Way - M31 galaxy pair
• N-body simulations of the Carina dSph in MOND
• Gravitational Lensing by Dark Matter Halos with Non-universal Density Profiles
• Sterile neutrinos produced near the EW scale I: mixing angles, MSW resonances and production rates
• Constraining interacting dark energy models with the halo concentration-mass relation
• The StEllar Counterparts of COmpact high velocity clouds (SECCO) survey. I. Photos of ghosts
• Extracting the Dark Matter Profile of a Relaxed Galaxy Cluster
• Models of Distorted and Evolving Dark Matter Halos
• The faintest radio source yet: EVLA observations of the gravitational lens SDSS J1004+4112
• Gamma rays from the neutralino dark matter annihilations in the Milky Way substructures
• Discovery of an isolated dark dwarf galaxy in the nearby universe
• Illuminating Dark Matter Halo Density Profiles Without Subhaloes
• ZOMG III: The effect of Halo Assembly on the Satellite Population
• Satellite Survival in Highly Resolved Milky Way Class Halos
• Impact of Dark Matter Substructure on the Matter and Weak Lensing Power Spectra
• The inner structure of dwarf sized halos in Warm and Cold Dark Matter cosmologies
• Gravitational Lensing of Supernova Neutrinos
• Mixed (Cold+Warm) Dark Matter in the Bino-Wino co-annihilation scenario
• Predictions for the Abundance of High-redshift Galaxies in a Fuzzy Dark Matter Universe
• Update on the Cetus Polar Stream and its Progenitor
• Galaxy Luminosity Functions in WINGS clusters
• Self-heating of Strongly Interacting Massive Particles
• Phase-space structures I: A comparison of 6D density estimators
• Giant Galaxies, Dwarfs, and Debris Survey. I. Dwarf Galaxies and Tidal Features Around NGC 7331
• The sense of rotation of subhaloes in cosmological dark matter haloes
• Ursa Major II - Reproducing the observed properties through tidal disruption
• Swift XRT Observations of the Possible Dark Galaxy VIRGOHI 21
• Neutrino As The Dark Force
• Evolution of a dwarf satellite galaxy embedded in a scalar field dark matter halo
• Inferring Astrophysics and Dark Matter Properties from 21cm Tomography using Deep Learning
• Self-interacting dark matter and cosmology of a light scalar mediator
• Typical density profile for warm dark matter haloes
• Higgs-portal Scalar Dark Matter: Scattering Cross Section and Observable Limits
• Stellar Systems in the direction of the Hickson Compact Group 44 - I. Low Surface Brightness Galaxies
• Running with BICEP2: Implications for Small-Scale Problems in CDM
• Kinematic Evidence for Halo Substructure in Spiral Galaxies
• A Search for Stellar Populations in High Velocity Clouds
• Warm dark matter constraints from high-$z$ Direct Collapse Black Holes using the JWST
• The impact of $\Lambda$CDM substructure and baryon-dark matter transition on the image positions of quad galaxy lenses
• Dark Matter-baryon segregation in the non-linear evolution of coupled Dark Energy model
• Astrophysical Tests of Dark Matter Self-Interactions
• Towards a Phylogenetic Analysis of Galaxy Evolution : a Case Study with the Dwarf Galaxies of the Local Group
• Limits to gauge coupling in the dark sector set by the non-observation of instanton-induced decay of Super-Heavy Dark Matter in the Pierre Auger Observatory data
• Self-Interacting Superfluid Dark Matter Droplets
• Precision Cosmology: Successes and Challenges
• Photoionized Gas in Dark-Matter Minihalos in the Galactic Halo and Local Group
• Systematizing the Effective Theory of Self-Interacting Dark Matter
• Evolution of the Phase-Space Density of Dark Matter Halos and Mixing Effects in Merger Events
• The stellar mass in and around isolated central galaxies: connections to the total mass distribution through galaxy-galaxy lensing in the Hyper Suprime-Cam survey
• Clouds Toward the Virgo Cluster Periphery: Gas-rich Optically Inert Galaxies
• Cosmological Simulations of Two-Component Wave Dark Matter
• The PAndAS View of the Andromeda Satellite System. III. Dwarf galaxy detection limits
• A high baryon fraction in massive haloes at z~3
• Palomar 13: a velocity dispersion inflated by binaries ?
• The Failure of Self-Interacting Dark Matter to solve the Overabundance of Dark Satellites and the Soft Core Question
• The Three Hundred project: Galaxy groups do not survive cluster infall
• Viscosity in cosmic fluids
• The Missing Satellite Problem Outside of the Local Group. II. Statistical Properties of Satellites of Milky Way-like Galaxies
• Comparing galactic satellite properties in hydrodynamical and Nbody simulations
• Galactic Substructure and Energetic Neutrinos from the Sun and the Earth
• Effect of dark matter annihilation on gas cooling and star formation
• Around The Way: Testing $\Lambda$CDM with Milky Way Stellar Stream Constraints
• Searching for Stars in Compact High-Velocity Clouds. I First Results from VLT and 2MASS
• Experimental identification of non-pointlike dark-matter candidates
• Gaseous Tidal Debris found in the NGC 3783 Group
• The Expected Properties of Dark Lenses
• Warm dark matter at small scales: peculiar velocities and phase space density
• Novel Adaptive softening for collisionless N-body simulations: Eliminating spurious halos
• Loss of star forming gas in SDSS galaxies
• Cosmic ray $e^{+}{e}^{-}$ spectrum excess and peak feature observed by the DAMPE experiment from dark matter
• Reconciling $S_8$: Insights from Interacting Dark Sectors
• Re-Examining Astrophysical Constraints on the Dark Matter Model
• The Effect of Thermal Velocities on Structure Formation in N-body Simulations of Warm Dark Matter
• Another baryon miracle? Testing solutions to the "missing dwarfs" problem
• Late decaying 2-component dark matter scenario as an explanation of the AMS-02 positron excess
• Giant disk galaxies : Where environment trumps mass in galaxy evolution
• The effect of dark matter-dark radiation interactions on halo abundance -- a Press-Schechter approach
• Mond - a review
• Distinguishing Supersymmetry From Universal Extra Dimensions or Little Higgs Models With Dark Matter Experiments
• Smooth Particle Lensing
• The AGORA High-resolution Galaxy Simulations Comparison Project. V: Satellite Galaxy Populations In A Cosmological Zoom-in Simulation of A Milky Way-mass Halo
• The number of tidal dwarf satellite galaxies in dependence of bulge index
• Dark influences II: gas and star formation in minor mergers of dwarf galaxies with dark satellites
• Exploring extensions to the standard cosmological model and the impact of baryons on small scales
• Detection of satellite remnants in the Galactic Halo with Gaia III. Detection limits for Ultra Faint Dwarf Galaxies
• AGN and Dwarf Galaxy Gas Kinematics
• Is a co-rotating Dark Disk a threat to Dark Matter Directional Detection ?
• The dependence of subhalo abundance matching on galaxy photometry and selection criteria
• Sterile neutrino dark matter in warped extra dimensions
• Gravitational wave probes on self-interacting dark matter surrounding an intermediate mass black hole
• Dark matter halos in the multicomponent model. I. Substructure
• The dark side of FIRE: predicting the population of dark matter subhaloes around Milky Way-mass galaxies
• The effect of Large Magellanic Cloud on the satellite galaxy population in Milky Way analogous Galaxies
• Planar distribution of the galaxies in the Local Group: a statistical and dynamical analysis
• The massive dark halo of the compact, early-type galaxy NGC 1281
• Resequencing the Hubble sequence and the quadratic (black hole mass)-(spheroid stellar mass) relation for elliptical galaxies
• Quasar Mesolensing - Direct Probe to Substructures around Galaxies -
• One never walks alone: the effect of the perturber population on subhalo measurements in strong gravitational lenses
• Probing chiral and flavored $Z^{\prime }$ from cosmic bursts through neutrino interactions
• Primordial Black Hole Merger Rate in Self-Interacting Dark Matter Halo Models
• Quantifying tidal stream disruption in a simulated Milky Way
• Tracing stars in Milky Way satellites with A-SLOTH
• Hunting for dark halo substructure using submilliarcsecond-scale observations of macrolensed radio jets
• The mass loss process in dwarf galaxies from 3D hydrodynamical simulations: the role of dark matter and starbursts
• Confronting Models of Dwarf Galaxy Quenching with Observations of the Local Group
• Towards resolving strongly-interacting dark sectors at colliders
• Nonlinear resonant oscillation of gravitational potential induced by ultralight axion in $f(R)$ gravity
• Collision tomography: Physical properties of possible progenitors of the Andromeda stellar stream
• Cosmological Evolution of Supergiant Star-Forming Clouds
• A panoramic view of the Local Group dwarf galaxy NGC 6822
• Reionization Histories of Milky Way Mass Halos
• Numerical investigation of lenses with substructures using the perturbative method
• Detection of Satellite Remnants in the Galactic Halo with Gaia - II. A modified Great Circle Cell Method
• Anisotropy of dark matter annihilation with respect to the Galactic plane
• A Model of Interacting Dark Matter and Dark Radiation for $H_0$ and ${\sigma }_8$ Tensions
• Cold versus Warm Dark Matter simulations of a galaxy group
• Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
• Analytic Relations for Magnifications and Time Delays in Gravitational Lenses with Fold and Cusp Configurations
• Detecting Axion Dark Matter through the Radio Signal from Omega Centauri
• Remnants of Galactic subhalos and their impact on indirect dark matter searches
• The Dynamical Evolution of Substructure
• Noiseless Gravitational Lensing Simulations
• The baryon cycle of Seven Dwarfs with superbubble feedback
• The SLUGGS Survey: The Inner Dark Matter Density Slope of the Massive Elliptical Galaxy NGC 1407
• The CN-CH positive correlation in the globular cluster NGC 5286
• Dark influences: imprints of dark satellites on dwarf galaxies
• Dark Matter Halos from the Inside Out
• Small scale clustering of late forming dark matter
• Gravitino dark matter from increased thermal relic particles
• Identifying galaxy candidates in WSRT HI imaging of ultra-compact high velocity clouds
• Probing the Halo From the Solar Vicinity to the Outer Galaxy: Connecting Stars in Local Velocity Structures to Large-Scale Clouds
• Through a Smoother Lens: An expected absence of LCDM substructure detections from hydrodynamic and dark matter only simulations
• Reversal of Fortune: Increased Star Formation Efficiencies in the Early Histories of Dwarf Galaxies?
• Applying scale-free mass estimators to the Local Group in Constrained Local Universe Simulations
• Perturbative signature of substructures in strong gravitational lenses
• KMTNet Nearby Galaxy Survey II. Searching for Dwarf Galaxies in Deep and Wide-field Images of the NGC 1291 system
• Non-linear gravitational clustering of cold matter in an expanding universe: indications from 1D toy models
• Improving the Angular Resolution of EGRET and New Limits on Supersymmetric Dark Matter Near the Galactic Center
• Structure formation in a mixed dark matter model with decaying sterile neutrino: the 3.5 keV X-ray line and the Galactic substructure
• Galactic nebular lines in the fiber spectra of background QSOs: Reaching a hundred QSO-galaxy pairs with spectroscopic and photometric measurements
• Push it to the limit: Local Group constraints on high-redshift stellar mass functions for Mstar > 10^5 Msun
• Constraints on sterile neutrino dark matter from XMM--Newton observation of M33
• New Surface Brightness Fluctuations Spectroscopic Technique: NGC4449 and its Stellar Tidal Stream
• Confusing the extragalactic neutrino flux limit with a neutrino propagation limit
• Substructure lensing in galaxy clusters as a constraint on low-mass sterile neutrinos in tensor-vector-scalar theory: The straight arc of Abell 2390
• Absence of HI in the Bootes Dwarf Spheroidal Galaxy
• The frequency of very young galaxies in the local Universe: I. A test for galaxy formation and cosmological models
• RR Lyrae Variable Stars in the Crater II Dwarf Galaxy
• Dynamical flows through Dark Matter Haloes II: one and two points statistics at the virial radius
• Prospects of detecting dark matter through cosmic-ray antihelium with the antiproton constraints
• Faint Satellite Population of the NGC-3175 Group - a Local Group Analogue
• Spherical Collapse in Modified Newtonian Dynamics (MOND)
• Sizing from the Smallest Scales: The Mass of the Milky Way
• Environmental effect on the subhalo abundance -- a solution to the missing dwarf problem
• Constraining SuperWIMPy and Warm Subhalos with Future Submillilensing
• Gravitational orbits in the expanding universe revisited
• Snowmass-2013 Cosmic Frontier 3 (CF3) Working Group Summary: Non-WIMP dark matter
• New Local Volume Dwarf Galaxy Candidates from the DESI Legacy Imaging Surveys
• Dissecting galaxy formation models with Sensitivity Analysis -- A new approach to constrain the Milky Way formation history
• Dark energy from dark radiation in strongly coupled cosmologies with no fine tuning
• Statistics of Magnification Perturbations by Substructure in the Cold Dark Matter Cosmological Model
• Fluctuations in strongly coupled cosmologies
• A tight scaling relation of dark matter in galaxy clusters
• Characterizing dw1335-29, a recently discovered dwarf satellite of M83
• The Search for Intergalactic Hydrogen Clouds in Voids
• Physical constraints on the central mass and baryon content of satellite galaxies
• Small scale structures in coupled scalar field dark matter
• Explaining dark matter halo density profiles with neural networks
• Scalar field dark matter as an alternative explanation for the anisotropic distribution of satellite galaxies
• NOIRCAT - The Northern HIPASS Optical/IR Catalogue
• The potential role of NGC 205 in generating Andromeda's vast thin co-rotating plane of satellite galaxies
• Strongly Interacting Neutrino Portal Dark Matter
• On the Formation of Giant Elliptical Galaxies and Globular Clusters
• A Deep Photometric Look at Two of Andromeda's Dwarf Spheroidals: X and XVII
• BVRI Surface Photometry of Isolated Spiral Galaxies
• Detection of an Optical Counterpart to the ALFALFA Ultra-compact High Velocity Cloud AGC 249525
• Reconstruction of Cluster Masses using Particle Based Lensing I: Application to Weak Lensing
• The effect of gravitational tides on dwarf spheroidal galaxies
• Decoding Dark Matter Substructure without Supervision
• Calibration of a star formation and feedback model for cosmological simulations with Enzo
• Can decaying dark matter scenarios alleviate both $H_0$ and ${\sigma }_8$ tensions?
• Warm Dark Haloes Accretion Histories and their Gravitational Signatures
• Calibration of Surface Brightness Fluctuations for Dwarf Galaxies in the Hyper Suprime-Cam $gi$ Filter System
• A Merger Tree with Microsolar Mass Resolution: Application to $\gamma$-ray Emission from Subhalo Population
• Atomic hydrogen, star formation and feedback in the lowest mass Blue Compact Dwarf galaxies
• European Spallation Source as a searching tool for an ultralight scalar field
• The edge of galaxy formation III: The effects of warm dark matter on Milky Way satellites and field dwarfs
• Interacting Scalar Radiation and Dark Matter in Cosmology
• The Effect of Satellite Galaxies on Gravitational Lensing Flux Ratios
• The post-infall evolution of a satellite galaxy
• Attack of the Flying Snakes : Formation of Isolated HI Clouds By Fragmentation of Long Streams
• The Potential of the Dwarf Galaxy Triangulum II for Dark Matter Indirect Detection
• The Merian Survey: Design, Construction, and Characterization of a Filter Set Optimized to Find Dwarf Galaxies and Measure their Dark Matter Halo Properties with Weak Lensing
• Using Artificial Neural Networks to Constrain the Halo Baryon Fraction during Reionization
• Internal dynamics and dynamical friction effects in the dwarf spheroidal galaxy in Fornax
• The kinematics of the Local Group in a cosmological context
• The mass distribution of a moderate redshift galaxy group and brightest group galaxy from gravitational lensing and kinematics
• Polytropic spheres modelling dark matter halos of dwarf galaxies
• A short survey of matter-antimatter evolution in the primordial universe
• Probing cold dark matter subhalos with simulated ALMA observations of macrolensed sub-mm galaxies
• COZMIC. I. Cosmological Zoom-in Simulations with Initial Conditions Beyond Cold Dark Matter
• Ultra-deep Imaging: Structure of Disks and Haloes
• Searching for Dark Clumps with Gravitational-Wave Detectors
• Not All Subhaloes Are Created Equal: Modelling the Diversity of Subhalo Density Profiles in TNG50
• The prolate dark matter halo of the Andromeda galaxy
• A lower limit on the dark particle mass from dSphs
• Star Streams and the Assembly History of the Galaxy
• Asymmetric dark matter with a spontaneously broken $U(1{)}^{\prime }$: self-interaction and gravitational waves
• Identifying Anomalies in Gravitational Lens Time Delays
• A Counterpart to the Radial Orbit Instability in Triaxial Stellar Systems
• Searching for Stars in Compact High-Velocity Clouds. II
• The effects of the small-scale behaviour of dark matter power spectrum on CMB spectral distortion
• SDSS IV MaNGA: Discovery of an $H_{\alpha }$ blob associated with a dry galaxy pair -- ejected gas or a `dark' galaxy candidate?
• Inflation and the dwarf galaxy problem
• Constraining warm dark matter mass with cosmic reionization and gravitational wave
• Model-independent constraints on ultra-light dark matter from the SPARC data
• Illuminating the Darkest Galaxies
• Characterising the Structure of Halo Merger Trees Using a Single Parameter: The Tree Entropy
• Quantum tunneling rate of dilute axion stars close to the maximum mass
• X-Ray Shapes of Elliptical Galaxies and Implications for Self-Interacting Dark Matter
• On wave dark matter in spiral and barred galaxies
• The Luminosity Functions and Redshift Evolution of Satellites of Low-Mass Galaxies in the COSMOS Survey
• Local Group dSph radio survey with ATCA (I): Observations and background sources
• What Regulates Galaxy Evolution? Open Questions in Our Understanding of Galaxy Formation and Evolution
• Local Group Analogs in $\Lambda$CDM cosmological simulations
• BDM Dark Matter: CDM with a core profile and a free streaming scale
• Predictions for the FAST telescope's CRAFTS Extra-Galactic HI Survey
• keV Warm Dark Matter via the Supersymmetric Higgs Portal
• Radial structure, inflow & central mass of stationary radiative galaxy clusters
• The Cosmic Evolution of Halo Pairs: I. Global Trends
• X-ray morphology of cluster-mass haloes in self-interacting dark matter
• The Galaxy Stellar Mass Function and Low Surface Brightness Galaxies from Core-Collapse Supernovae
• Understanding dwarf galaxies as galactic building blocks
• Two phase galaxy formation: The Evolutionary Properties of Galaxies
• Analytic and numerical realisations of a disk galaxy
• Satellites in the field and lens galaxies: SDSS/COSMOS vs. SLACS/CLASS
• The Star-Forming Dwarf Galaxy Populations of two z ~ 0.4 Clusters: MS1512.4+3647 and Abell 851
• Massive Black Holes in Dwarf Spheroidal Galaxy Haloes?
• Keck Spectroscopy of Globular Clusters in the Virgo Cluster Dwarf Elliptical VCC 1386
• The Discovery of New Galaxy Members in the NGC 5044 and NGC 1052 Groups
• CMB Spectral Distortion Constraints on Thermal Inflation
• The luminosity function of diverse satellite galaxy systems
• Dark Matter Studies Entrain Nuclear Physics
• Stability of Satellite Planes in M31 II: Effects of the Dark Subhalo Population
• Dissipative dark matter halos: The steady state solution
• Constraints on conformal ultralight dark matter couplings from the European Pulsar Timing Array
• Degeneracies between baryons and dark matter: the challenge of constraining the nature of dark matter with JWST
• The environment and redshift dependence of accretion onto dark matter halos and subhalos
• Searching for Optical Counterparts to Ultra-compact High Velocity Clouds: Possible Detection of a Counterpart to AGC 198606
• Fitting a Self-Interacting Dark Matter Model to Data Ranging From Satellite Galaxies to Galaxy Clusters
• Cosmic Voids in Evolving Dark Sector Cosmologies: the Low Redshift Universe
• Is GBT 1355+5439 a dark galaxy?
• The ACS LCID Project XI. On the early time resolution of LG dwarf galaxy SFHs: Comparing the effects of reionization in models with observations
• Dark Matter Subhalos in the Ursa Minor Dwarf Galaxy
• Density fields and halo mass functions in the Geometrical Adhesion toy Model
• Isotropic extragalactic flux from dark matter annihilations: lessons from interacting dark matter scenarios
• Non-Relativistic Formation of Scalar Clumps as a Candidate for Dark Matter
• Dwarf Galaxy Discoveries from the KMTNet Supernova Program II. The NGC 3585 Group and Its Dynamical State
• The evolution of the photometric properties of Local Group dwarf spheroidal galaxies
• Mitigating Foreground Bias to the CMB Lensing Power Spectrum for a CMB-HD Survey
• Merging of Low-Mass Systems and the Origin of the Fundamental Plane
• Analyzing the Flux Anomalies of the Large-Separation Lensed Quasar SDSS J1029+2623
• Transient Weak-Lensing by Cosmological Dark Matter Microhaloes
• Assembly of the outer Galactic stellar halo in the hierarchical model
• Effects of Coupled Dark Energy on the Milky Way and its Satellites
• Cosmological constraints on the velocity-dependent baryon-dark matter coupling
• MIND THE GAP: Is The Too Big To Fail Problem Resolved?
• Prospects for Determining the Mass Distributions of Galaxy Clusters on Large Scales Using Weak Gravitational Lensing
• Dynamical consequences of CDM merger trees
• Luminosity-Diameter Relations for Globular Clusters and Dwarf Spheroidal Galaxies
• A Second Shell in the Fornax dSph Galaxy
• SCALAR: an AMR code to simulate axion-like dark matter models
• Do High-Velocity Clouds trace the Dark Matter subhalo population?
• Discovery of an Ultra-Faint Dwarf Galaxy in the Intracluster Field of the Virgo Center : A fossil of the First Galaxies?
• Clumpiness enhancement of charged cosmic rays from dark matter annihilation with Sommerfeld effect
• A too-many dwarf satellite galaxies problem in the MATLAS low-to-moderate density fields
• The time evolution of gaps in tidal streams
• Exploring the low-mass regime of galaxy-scale strong lensing: Insights into the mass structure of cluster galaxies
• Degenerate Fermion Dark Matter from a Broken $U(1{)}_{\mathrm{B}-\mathrm{L}}$ Gauge Symmetry
• Type Ia supernovae in a hierarchical galaxy formation model: the Milky Way
• Dynamical response to supernova-induced gas removal in two-component spherical galaxies
• Is the vast polar structure of dwarf galaxies a serious problem for lambda cold dark matter?
• The eccentricity enhancement effect of intermediate-mass-ratio-inspirals: dark matter and black hole mass
• Consequences of dark matter self-annihilation for galaxy formation
• Parity Dependence in Strong Lens Systems as a Probe of Dark Matter Substructure
• Explaining the observed velocity dispersion of dwarf galaxies by baryonic mass loss during the first collapse
• The cluster galaxy luminosity function at $z=0.3$: a recent origin for the faint-end upturn ?
• Study of a viscous $\Lambda$WDM model: Near equilibrium condition, entropy production, and cosmological constraints
• Dwarf Galaxies: Important Clues to Galaxy Formation
• Non-sphericity of ultralight axion dark matter haloes in the Galactic dwarf spheroidal galaxies
• Cuspy dark matter density profiles in massive dwarf galaxies
• Reconciliation of MOND and Dark Matter theory
• MACHOs in dark matter haloes
• Dwarf Galaxies in Voids: Dark Matter Halos and Gas Cooling
• Dark Matter Decaying into a Fermi Sea of Neutrinos
• Cosmic Voids in Evolving Dark Sector Cosmologies: the High Redshift Universe
• The dark matter content of the blue compact dwarf NGC 2915
• An Alternative Channel For High-Mass Binary Black Holes-----Dark Matter Accretion Onto Black Hole
• Decaying axinolike dark matter: Discriminative solution to small-scale issues
• Cosmological implications of a Dark Matter self-interaction energy density
• Vector-like technineutron Dark Matter: is a QCD-type Technicolor ruled out by XENON100?
• Quantifying the abundance of faint, low-redshift satellite galaxies in the COSMOS survey
• The Dark Knight Falters
• Probing Oscillons of Ultra-Light Axion-like Particle by 21cm Forest
• $\gamma$-ray flux from Dark Matter Annihilation in Galactic Caustics
• Halo Scaling Relations and Hydrostatic Mass Bias in the Simba Simulation From Realistic Mock X-ray Catalogues
• Leo IV & V - A possible dwarf galaxy pair ?
• Stellar populations of massive elliptical galaxies in very rich clusters
• Gamma-rays From Warm WIMP Dark Matter Annihilation
• Dwarf Galaxy Sized Monopoles as Dark Matter?
• Properties of galaxy halos in Clusters and Voids
• Search for MeV-Scale Axionlike Particles and Dark Photons with PandaX-4T
• Anomalous Ionization in the Central Molecular Zone by sub-GeV Dark Matter
• New dwarf galaxy candidates in the sphere of influence of the Local Volume spiral galaxy NGC2683
• The Structure of Dark Matter Halos in an Annihilating Dark Matter Model
• Probing sub-galactic mass structure with the power spectrum of surface-brightness anomalies in high-resolution observations of galaxy-galaxy strong gravitational lenses. I. Power-spectrum measurement and feasibility study
• Constraining SN feedback: a tug of war between reionization and the Milky Way satellites
• A search for neutrino signal from dark matter annihilation in the center of the Milky Way with Baikal NT200
• Absence of Dwarf Galaxies at High Redshifts: Evidence from a Galaxy Group
• Observations of the Lensed Quasar Q2237+0305 with CanariCam at GTC
• Gravitational microlensing as a probe for dark matter clumps
• Gravitational Lensing Effects on High Redshift Type II Supernova Studies with NGST
• Determining Supersymmetric Parameters With Dark Matter Experiments
• There is no universal acceleration scale in galaxies
• The OTELO survey. II. The faint-end of the H$\alpha$ luminosity function at z $\sim$ 0.40
• Universal scaling laws and density slope for dark matter haloes
• Devouring the Milky Way Satellites: Modeling Dwarf Galaxies with Galacticus
• A self-consistent hydrostatic mass modelling of pressure supported dwarf galaxy Leo T
• The Galactic positron flux and dark matter substructures
• Using the redshift evolution of the Lyman-$\alpha$ effective opacity as a probe of dark matter models
• Tidal stripping stellar substructures around four metal-poor globular clusters in the Galactic bulge
• A Comparison of Outflow Properties in AGN Dwarfs vs. Star Forming Dwarfs
• Impact of distance determinations on Galactic structure. II. Old tracers
• Simulating the formation of cosmic structure
• GHOSTS I: A New Faint very Isolated Dwarf Galaxy at D = 12 +/- 2 Mpc
• Dense gas clouds and the Unidentified EGRET sources
• The eROSITA Final Equatorial-Depth Survey (eFEDS) -- Splashback radius of X-ray galaxy clusters using galaxies from HSC survey
• Statistical properties of substructures around Milky Way-sized haloes and their implications for the formation of stellar streams
• Star Streams in Triaxial Isochrone Potentials with Sub-Halos
• Modeling lens potentials with continuous neural fields in galaxy-scale strong lenses
• New dwarf galaxy candidates in the sphere of influence of the Sombrero galaxy
• Model-free analysis of quadruply imaged gravitationally lensed systems and substructured galaxies
• EDGE: the puzzling ellipticity of Eridanus II's star cluster and its implications for dark matter at the heart of an ultra-faint dwarf
• Rapidly spinning dark matter-admixed neutron stars
• Detecting sterile dark matter in space
• Spectroscopic confirmation of the dwarf spheroidal galaxy d0944+71 as a member of the M81 group of galaxies
• Distribution of merging and post-merging galaxies in nearby galaxy clusters
• Linking the Metallicity Distribution of Galactic Halo Stars to the Enrichment History of the Universe
• Proper motion measurements for stars up to $100$ kpc with Subaru HSC and SDSS Stripe 82
• Environment from cross-correlations: connecting hot gas and the quenching of galaxies
• Gravitino Dark Matter with Weak-Scale Right-Handed Sneutrino
• Gravitational lensing in WDM cosmologies: The cross section for giant arcs
• Rotation in Gravitational Lenses
• The gap of stellar mass in galaxy groups: another perspective of the Too-big-To-Fail problem in the Milky Way
• Extracting galaxy merger timescales I: Tracking haloes with WhereWolf and spinning orbits with OrbWeaver
• Formation and Radiative Feedback of First Objects and First Galaxies
• Frequency of the dark matter subhalo collisions and bifurcation sequence arising formation of dwarf galaxies
• Nonlinear growth of structure in cosmologies with damped matter fluctuations
• The detection of a massive chain of dark HI clouds in the GAMA G23 Field
• Parameterizing the Outflow from a Central Black Hole in Dwarf Spheroidal Galaxies: A 3D Hydrodynamic Simulation
• The Epoch of Assembly of Two Galaxy Groups: A comparative study
• Gravity- and temperature-driven phase transitions in a model for collapsed axionic condensates
• Faint Dwarfs in Nearby Groups
• X-ray Clusters of Galaxies as Cosmological Tools
• An Extra-Dimensional Model of Dark Matter
• Origin and Evolution of Structure and Nucleosynthesis for Galaxies in the Local Group
• Extragalactic HI survey with FAST : First look of the pilot survey results
• Abundance matching for low mass galaxies in the CDM and FDM models
• Scope of strongly self-interacting thermal WIMPs in a minimal $U(1{)}_D$ extension and its future prospects
• Orbital pericenters and the inferred dark matter halo structure of satellite galaxies
• Searching for Dark Matter in Messier 33
• Time-delayed neutrino emission from supernovae as a probe of dark matter-neutrino interactions
• Formation of Galactic Bulges
• Observing the stellar halo of Andromeda in cosmological simulations: the Auriga2PAndAS pipeline
• Tip of the red giant branch distance to the nearby dwarf galaxy [TT2009] 25 in the NGC 891 group
• Dark matter perturbations and viscosity: a causal approach
• The Distance and Properties of Hydrogen Clouds in the Leading Arm of the Magellanic System
• A comparison between the detection of gamma rays and positrons from neutralino annihilation
• The origin of type-I profiles in cluster lenticulars: An interplay between ram pressure stripping and tidally-induced spiral migration
• Characterization and dynamics of the peculiar stream Jhelum, A tentative role for the Sagittarius dwarf galaxy
• Variability of GeV gamma-ray emission in QSO B0218+357 due to microlensing on intermediate size structures
• Tidal features and disc thicknesses of edge-on galaxies in the SDSS Stripe 82
• Rapid onset of the 21-cm signal suggests a preferred mass range for dark matter particle
• K-essence scalar dark matter solitons around supermassive black holes
• On the separation between baryonic and dark matter: evidence for phantom dark matter?
• Axisymmetric Schwarzschild models of an isothermal axisymmetric mock dwarf spheroidal galaxy
• Structure Formation with Two Periods of Inflation: Beyond PLaIn $\Lambda$CDM
• A new test for the stable clustering hypothesis
• Missing Dwarf Problem in Galaxy Clusters
• Rotation curves of galaxies and the stellar mass-to-light ratio
• Accretion of Self-interacting Scalar Field Dark Matter Onto a Reissner-Nordström Black Hole
• The Effect of Multiple Cooling Channels on the Formation of Dark Compact Objects
• Constraints on long-lived electrically charged massive particles from anomalous strong lens systems
• Are Over-massive Haloes of Ultra Diffuse Galaxies Consistent with Extended MOND?
• Euclid: Early Release Observations of diffuse stellar structures and globular clusters as probes of the mass assembly of galaxies in the Dorado group
• A bag of tricks: Using proper motions of Galactic stars to identify the Hercules ultra-faint dwarf galaxy members
• Discovery of New Dwarf Galaxy near The Isolated Spiral Galaxy NGC 6503
• Probing the Warm Dark Matter with High-z Quasar Luminosity Function
• Constraining Mixed Dark Matter models with high redshift Lyman-alpha forest data
• Probing dark matter haloes of spiral galaxies at poorly explored distances using satellite kinematics
• Tidal Debris as a Dark Matter Probe
• Mass Limits on Neutralino Dark Matter
• Milky Way simulations: the Galaxy, its stellar halo and its satellites - insights from a hybrid cosmological approach
• Reconstruction of small-scale galaxy cluster substructure with lensing flexion
• Hα Dots: Direct-Method Metal Abundances of Low-Luminosity Star-Forming Systems
• An Accurate Comprehensive Approach to Substructure: III. Masses and Formation Times of the Host Haloes
• Bounds on sterile neutrino lifetime and mixing angle with active neutrinos by global 21 cm signal
• The spatial distribution of satellites in galaxy clusters
• Modified initial power spectrum and too big to fail problem
• Impact of Cosmological Satellites on Stellar Discs: Dissecting One Satellite at a Time
• The MUSE-Faint survey. III. Constraining scalar field dark matter with Antlia B
• Performance Assessment of the KASI-Deep Rolling Imaging Fast-optics Telescope pathfinder
• Luminous satellite galaxies in gravitational lenses
• Maximum entropy distributions of dark matter in $\Lambda$CDM cosmology
• Matter in the beam: Weak lensing, substructures and the temperature of dark matter
• Can substructure in the Galactic Halo explain the ATIC and PAMELA results?
• On the coldness of the local Hubble flow: the role of baryons
• Observational Constraints on the Modified Gravity Model (MOG) Proposed by Moffat: Using the Magellanic System
• Cosmology of fermionic dark matter
• The abundance of satellite galaxies in the inner region of $\Lambda$CDM Milky Way sized haloes
• Satellite survival in cold dark matter cosmology
• Hidden from view: Coupled Dark Sector Physics and Small Scales
• Reconstruction of $f(T,\mathcal{T})$ Lagrangian for various cosmological scenarios
• Is There a Universal Mass Function?
• Predictions on the stellar-to-halo mass relation in the dwarf regime using the empirical model for galaxy formation EMERGE
• Anisotropies in Cosmological 21 cm Background by Oscillons/I-balls of Ultra-light Axion-like Particle
• Accretion of Small Satellites and Gas Inflows in a Disc Galaxy
• Condensation of Galactic Cold Dark Matter
• The StEllar Counterparts of COmpact high velocity clouds (SECCO) survey. II. Sensitivity of the survey and an Atlas of Synthetic Dwarf Galaxies
• Local Group(s)
• The Carnegie-Chicago Hubble Program: Discovery of the Most Distant Ultra-faint Dwarf Galaxy in the Local Universe
• The low mass end of the neutral gas mass and velocity width functions of galaxies in $\Lambda$CDM
• ARTEMIS emulator: exploring the effect of cosmology and galaxy formation physics on Milky Way-mass haloes and their satellites
• Dark halo microphysics and massive black hole scaling relations in galaxies
• Modeling the core-halo mass relation in fuzzy dark matter halos
• Modelling ultra-fine structure in dark matter halos
• Universal subhalo accretion in cold and warm dark matter cosmologies
• Trading kinetic energy: How late kinetic decoupling of dark matter changes $N_{\text{eff}}$
• Constraining Warm Dark Matter with high-$z$ supernova lensing
• Time evolution of gaps in stellar streams in axisymmetric Stäckel potentials
• Measuring the distances to quasars at high redshifts with strong lensing
• Extended Stellar Components of Galaxies & the Nature of Dark Matter
• Tidal Dwarf Galaxies at Intermediate Redshifts
• Resolved Stellar Populations as Tracers of Outskirts
• Diverse dark matter profiles in FIRE dwarfs: black holes, cosmic rays and the cusp-core enigma
• Universal dark halo scaling relation for the dwarf spheroidal satellites
• Static structure of chameleon dark Matter as an explanation of dwarf spheroidal galactic core
• The Invisible Dilaton
• A 125 GeV Higgs Boson Mass and Gravitino Dark Matter in R-invariant Direct Gauge Mediation
• Probing satellite galaxies in the Local Group by using FAST
• Constraining Ultra-light Axions with Galaxy Cluster Number Counts
• Probing the nature of Dark Matter through the metal enrichment of the intergalactic medium
• Resolution of the small scale structure issues with dissipative dark matter from multiple Standard Model sectors
• Impact of a Warm Dark Matter late-time velocity dispersion on large-scale structures
• Fluorescent rings in star-free dark matter haloes
• Andromeda XXV -- a dwarf galaxy with a low central dark matter density
• When quantum corrections alter the predictions of classical field theory for scalar field dark matter
• An analytical approach to the dwarf galaxies cusp problem
• Substructure and the Cusp and Fold Relations
• The feasibility of constraining DM interactions with high-redshift observations by JWST
• On the structure of Small Magellanic Cloud star clusters
• Dark matter dominated dwarf disc galaxy Segue 1
• The Realistic Scattering of Puffy Dark Matter
• Thermal Relic of Self-Interacting Dark Matter with Retarded Decay of Mediator
• Probing the Structure of Dark Matter in Galaxy Halos and Clusters using Supernovae
• Multiresolution Analysis of Substructure in Dark Matter Halos
• A Spitzer-MIPS search for dust in compact high-velocity HI clouds
• The Properties of Satellite Galaxies in External Systems. I. Morphology and Structural Parameters
• Detecting the dark matter annihilation at the ground EAS detectors
• Analytic approach to astrometric perturbations of critical curves by substructures
• Dwarf Galaxies as Cosmological Probes
• Coherent Self-Interactions of Dark Matter in the Bullet Cluster
• The history and mass content of cluster galaxies in the EAGLE simulation
• Understanding Dwarf Galaxies in order to Understand Dark Matter
• Probing Dark Star Parameters Through $f$-Mode Gravitational Wave Signals
• Understanding Galaxy Formation and Evolution
• From gas to galaxies
• Constraining supersymmetry from the satellite experiments
• Exploring the Dark Matter Disc Model in Dwarf Galaxies: Insights from the LITTLE THINGS Sample
• A link between feedback outflows and satellite galaxy suppression
• Warm Dark Matter Model of Galaxy Formation
• Testing $\Lambda$CDM With Dwarf Galaxy Morphology
• Galaxy-galaxy and galaxy-cluster lensing with the SDSS and FIRST surveys
• Local reionizations histories with merger tree of HII regions
• A 5deg x 5deg deep HI survey of the M81 group: II. HI distribution and kinematics of IC 2574 and HIJASS J1021+68
• On the Galactic Halos Rotation by Planck Data
• Small-scale Effects of Thermal Inflation on Halo Abundance at High-$z$, Galaxy Substructure Abundance and 21-cm Power Spectrum
• GalaxyFlow: Upsampling Hydrodynamical Simulations for Realistic Mock Stellar Catalogs
• Power Spectrum and Intermittency of Ly$\alpha$ Transmitted Flux of QSO He2347-4342
• Trial by FIRE: Probing the dark matter density profile of dwarf galaxies with GraphNPE
• Detecting Triaxiality in the Galactic Dark Matter Halo through Stellar Kinematics II: Dependence on Dark Matter and Gravity Nature
• Dwarf Galaxy Clustering and Missing Satellites
• Explaining the formation of bulges with MOND
• Mass Modeling the Andromeda Dwarf Galaxies: Andromeda VI and Andromeda XXIII
• Interacting photon-baryon fluid, warm dark matter and the first acoustic peak
• Disc-Halo Interactions in ΛCDM
• Strong Lensing by Subhalos in the Dwarf-Galaxy Mass Range II: Detection Probabilities
• A Novel Scheme for Dark Matter Annihilation Feedback in Cosmological Simulations
• An Oxford SWIFT Integral Field Spectroscopy study of 14 early-type galaxies in the Coma cluster
• Is High-Velocity Cloud Complex C Associated with the Galactic Warp?
• Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory
• Hollow cores in Warm Dark Matter halos from the Vlasov-Poisson equation
• The Circular Velocity Function of Group Galaxies
• Low Mass Pseudoscalar Dark Matter in an Extended B - L Model
• Structure and Evolution of Dwarf Galaxies
• Weak Lensing by Minifilament or Minivoid as the Origin of Flux-ratio Anomalies in Lensed Quasar MG0414+0534
• Fractals vs. halos: Asymptotic scaling without fractal properties
• Evanescent Matter
• Theoretical lower limits on sizes of ultra faint dwarf galaxies from dynamical friction
• Forecasts for Warm Dark Matter from Photometric Galaxy Surveys
• Gravity and Nonlinear Symmetry Realisation
• Constraining warm dark matter power spectrum using the cross-correlation of HI 21 cm signal and the Lyman-$\alpha$ forest
• Flattening of dark matter cusps during mergers: model of M31
• SDSS-IV MaNGA: the physical origin of off-galaxy H$\alpha$ blobs in the local Universe
• Constraining Ultra Light Dark Matter with the Galactic Nuclear Star Cluster
• Signatures of reionization feedback in the near-infrared background
• Galaxy Groups: Proceedings from a Swinburne University Workshop
• Super-Resonant Dark Matter
• A Study of the Properties and Dynamics of the Disk of Satellites in a Milky-Way-like Galaxy System
• Constraining Hot Dark Matter Sub-Species with Weak Lensing and the Cosmic Microwave Background Radiation
• Characterizing the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias
• Novel electrically charged wormhole, black hole and black bounce exact solutions in hybrid metric-Palatini gravity
• STRRINGS: STReams in Residual Images of Nearby GalaxieS
• Magnesium isotope ratios in Milky Way and dwarf galaxy stars
• Inhomogenous Primordial Baryon Distributions on Sub-Galactic Scales: High-z Galaxy Formation with WDM
• Nature and Environment of Very Luminous Galaxies
• The Hierarchical Structure of Galactic Haloes: Classification and characterisation with Halo-OPTICS
• Pair Lines of Sight Observations of Multiphase Gas Bearing O VI in a Galaxy Environment
• Velocity Variations in the Phoenix-Hermus Star Stream
• Temporal Self-Organization in Galaxy Formation
• The Arecibo Galaxy Environment Survey VIII : Discovery of an Isolated Dwarf Galaxy in the Local Volume
• Probing baryonic processes and gastrophysics in the formation of the Milky Way dwarf satellites: I. metallicity distribution properties
• Bar-driven injection of intergalactic matter into galactic halos
• Detecting Dark Matter in High Velocity Clouds
• Constraints on the Dark Matter Annihilations by Neutrinos with Substructure Effects Included
• Evolution of dwarf spheroidal satellites in the common surface-density dark halos
• Effects of Angular Momentum on Halo Profiles
• F-mode Oscillations of Neutron Stars with Dark Matter from Neutron Decay: Implications for Gravitational-Wave Detectability
• The Properties of Satellite Galaxies in External Systems. II. Photometry and Colors
• Measurement of Substructure from the Kinematics of the GD-1 Stellar Stream
• Problems with the Current Cosmological Paradigm
• Structural and Photometric Properties of the Andromeda Satellite Dwarf Galaxy Lacerta I from Deep Imaging with WIYN pODI
• The Effects of $\Lambda$CDM Dark Matter Substructure on the Orbital Evolution of Star Clusters
• New short period stellar pulsators at large Galactocentric distances
• Self-interacting Dark Matter with Scalar Dilepton Mediator
• Clues to the nature of dark matter from first galaxies
• nuMSM and its experimental tests
• Relating the HI Gas Structure of Spiral Disks to Passing Satellites
• Cosmological Signatures of Dark Sector Physics: The Evolution of Haloes and Spin Alignment
• Fingerprint matching of beyond-WIMP dark matter: neural network approach
• Dark Matter Annihilation Feedback in Cosmological Simulations II: The Influence on Gas and Halo Structure
• The Magellanic Group and the Seven Dwarfs
• Fundamental properties of the dark and the luminous matter from Low Surface Brightness discs
• A Rich Satellite Population of the NGC 4437 Group and Implications of a Magnitude Gap for Galaxy Group Assembly History
• Estimation of the Mass of Dark Matter Using the Observed Mass Profiles of Late-Type Galaxies
• Constraining Ultralight Axions with Galaxy Surveys
• Probing the mass function of halo dark matter via microlensing
• Demise of Faint Satellites around Isolated Early-type Galaxies
• Prospects for a local detection of dark matter with future missions to Uranus and Neptune
• KMTNet Nearby Galaxy Survey: Overview and a Survey Description
• Image Flux Ratios of Gravitationally Lensed HS 0810+2554 with High Resolution Infrared Imaging
• Star Formation in Satellite Galaxies
• Neutrino Coannihilation on Dark-Matter Relics?
• A Dark Galaxy in the Virgo Cluster Imaged at 21-cm
• Cosmological Zoom-In Simulations of Milky Way Host Mass Dark Matter Halos with a Blue-Tilted Primordial Power Spectrum
• A VLA monitoring study of JVAS B1422+231: investigation of time delays and detection of extrinsic variability
• Gravitational wave lensing: probing Fuzzy Dark Matter with LISA
• Is there a dwarf galaxy satellite-of-satellite problem in $\Lambda$CDM?
• DES to HSC: Detecting low surface brightness galaxies in the Abell 194 cluster using transfer learning
• Collapsed and Extended Cold Dark Matter Haloes in Softened N-Body Gravity
• Neutralino Dark Matter as the Source of the WMAP Haze
• Testing extensions to LCDM on small scales with forthcoming cosmic shear surveys
• Roche Lobe Overflow from Dwarf Stellar Systems
• Six Higgs Doublets Model for Dark Matter
• Comparing simulated Milky Way satellite galaxies with observations using unsupervised clustering
• Exploring the evolution of a dwarf spheroidal galaxy with SPH simulations: I. Stellar feedback
• Feedback from intermediate mass black holes on dwarf galaxy morphology at z=2
• DARKSKIES: A suite of super-sampled zoom-in simulations of galaxy clusters with self-interacting dark matter
• Dwarf Galaxies in the Halo of NGC 891
• Sub-keV dark matter can strongly ionize molecular clouds
• Born to be Starless: Revisiting the Missing Satellite Problem
• FIMP Dark Matter in bulk viscous non-standard cosmologies
• Using dust to constrain dark matter models
• Subhalos are Anisotropically Distributed and Aligned with the Smooth Matter Distribution of Their Host Halos
• Do the Unidentified EGRET Sources Trace Annihilating Dark Matter in the Local Group?
• Kinetic recoupling of dark matter
• Non-thermal warm dark matter limits from small-scale structure
• Revisiting Puffy Dark Matter with Novel Insights: Partial Wave Analysis
• Connecting dark matter, baryogenesis and neutrinoless double beta decay in a $A_4\otimes Z_8$ based $\nu$2HDM
• Gamma rays from dark matter annihilation in the Draco and observability at ARGO
• Machine-guided Exploration and Calibration of Astrophysical Simulations
• Giant monopoles as a dark matter candidate
• Dark matter and low scale leptogenesis in a flavor symmetric neutrino two Higgs doublet model($\nu$2HDM)
• Can dark matter see itself?
• The imprint of dark subhaloes on the circumgalactic medium
• MeV scale model of SIMP dark matter, neutrino mass and leptogenesis
• Properties of subhalos in the interacting dark matter scenario
• Bosonic dark matter halos: excited states and relaxation in the potential of the ground state
• Spiked Monopoles
• Satellites in the Local Group and Other Nearby Groups
• Constraint on Matter Power Spectrum on $10^6-10^9{M}_{\odot }$ Scales from ${\tau }_e$
• The Effect of Cosmological Background Dynamics on the Spherical Collapse in MOND
• Galaxies OBserved as Low-luminosity Identified Nebulae (GOBLIN): a catalog of 43,000 high-probability dwarf galaxy candidates in the UNIONS survey
• Metallicity and kinematical clues to the formation of the Local Group
• Too small to succeed: the difficulty of sustaining star formation in low-mass haloes
• Globular Clusters as Candidates for Gravitational Lenses to Explain Quasar-Galaxy Associations
• Complexity in small-scale dwarf spheroidal galaxies
• Implications for the missing low-mass galaxies (satellites) problem from cosmic shear
• The Origin of the Large Magellanic Cloud Globular Cluster NGC 2005
• Quantifying the Detectability of Milky Way Satellites with Image Simulations: a Case Study with KiDS
• Chameleon Gravity as an Alternative to Dark Matter
• The THESAN project: environmental drivers of Local Group reionization
• Constraints on Dark Matter annihilation and Its Equation of State after Planck Data
• CO and HI observations of an enigmatic cloud
• Co-interacting dark matter and conformally coupled light scalars
• Self-similarity and stable clustering in a family of scale-free cosmologies
• Constraints on superheavy dark matter decaying into $h\nu$, $Z\nu$ and $W\ell$ -- Benchmark example within an extended seesaw framework
• The Stromlo Missing Satellites Survey
• MONDian predictions for Newtonian M/L ratios for ultrafaint dSphs
• Three-dimensional shapelets and an automated classification scheme for dark matter haloes
• Precision Astrometry, Galactic Mergers, Halo Substructure and Local Dark Matter
• Dark halo densities, substructure, and the initial power spectrum
• Phenomenology of one zero texture Yukawa matrix in a flavor symmetric scotogenic model
• Resolving the extended stellar halos of nearby galaxies: the wide-field PISCeS survey
• Dark Matter and Fundamental Physics Searches with IACTs
• Search for dark matter in compact hydrogen clouds
• Core collapse in resonant self-interacting dark matter across two decades in halo mass
• A new test for the Galactic formation and evolution -- prediction for the orbital eccentricity distribution of the halo stars
• DELVE Milky Way Satellite Galaxy Census I: Satellite Population and Survey Selection Function in DES, DELVE, and Pan-STARRS
• 3-3-1 Self Interacting Dark Matter and the Galaxy Core-Cusp problem
• Metamorphosis of dwarf halo density profile under dark matter decays
• The Effective Field Theory of Large Scale Structures of a Fuzzy Dark Matter Universe
• A new perspective on galactic dynamics
• The Upper Bound of the Second Higgs Boson Mass in Minimal Gauge Mediation with the Gravitino Warm Dark Matter
• Exploring the Universe with Metal-Poor Stars
• EDGES of the dark forest: A new absorption window into the composite dark matter and large scale structure
• Gravity-mediated Dark Matter models in the de Sitter space
• The HI Detection of Low Column Density Clouds and Galaxies
• Graviton spectrum in simplified Dark Matter models with graviton mediators in the de Sitter space
• Transient star B/R ratio and star formation in $z\gtrsim 1$ lensed galaxies
• Emulating the Non-Linear Matter Power-Spectrum in Mixed Axion Dark Matter Models
• HI and Galaxy Formation in Loose Groups
• Matching the dark matter profiles of dSph galaxies with those of simulated satellites: a two parameter comparison
• On the Size Evolution of a Galactic Disk in Hierarchical Merging of Cold Dark Matter Halos
• Non-linear structure formation in the "Running FLRW" cosmological model
• Determining the primordial helium abundance and UV background using fluorescent emission in star-free dark matter haloes
• Nearest neighbour analysis as a new probe for fuzzy dark matter
• WIMP decay as a possible Warm Dark Matter model
• Dark Energy Simulations
• Fundamental fields around compact objects: Massive spin-2 fields, Superradiant instabilities and Stars with dark matter cores
• A Model For Intergalactic Filaments and Galaxy Formation During the First Gigayear
• Hierarchical Merger of Primordial Black Holes in Dwarf Galaxies
• A Random Walk Model for Halo Triaxiality
• SAURON observations of Sa bulges: the formation of a kinematically decoupled core in NGC5953
• "Observations" of simulated dwarf galaxies: Star-formation histories from color-magnitude diagrams
• Subhalo abundance and satellite spatial distribution in Milky Way-Andromeda-like paired haloes
• Cross Section Calculations in Theories of Self-Interacting Dark Matter
• On a critical acceleration scale of dark matter in Lambda-CDM and dynamical dark energy
• The Hierarchical Structure of Galactic Haloes: Generalised N-Dimensional Clustering with CluSTAR-ND
• A flat faint end of the Fornax cluster galaxy luminosity function
• The dwarf low surface brightness population in different environments of the Local Universe
• Red Halos of Galaxies - Reservoirs of Baryonic Dark Matter?
• "Dark galaxies" and local very metal-poor gas-rich galaxies: possible interrelations
• An analytical model of surface mass densities of cold dark matter haloes - with an application to MACHO microlensing optical depths
• A hierarchical clustering method for quantifying satellite abundance
• Prospects for CDM sub-halo detection using high angular resolution observations
• Bounding the photon mass with cosmological propagation of fast radio bursts
• The high energy window of probing dark matter with cosmic-ray antideuterium and antihelium
• Implications of the first AMS-02 antiproton data for dark matter
• The effect of hydrodynamics alone on the subhalo population in a $\Lambda$CDM rich cluster sized dark matter halo
• The Lowest Metallicity Stars in the LMC: Clues from MaGICC Simulations
• Dark matter haloes in the multicomponent model. III. From dwarfs to galaxy clusters
• Cosmological implications of electromagnetically interacting dark matter: milli-charged particles and atoms with singly and doubly charged dark matter
• Searching for an Intrinsic Stellar Population in Compact High-Velocity Clouds
• On the Detectability of Galactic Dark Matter Annihilation into Monochromatic Gamma-rays
• Effect of dark matter halo substructures on galaxy rotation curves
• Spectroscopic confirmation of hydrogen alpha-selected satellite galaxies
• Measuring the halo mass function in loose groups
• Light on Dark Matter
• Timing Mass of the Local Group
• Investigation of mass substructure in gravitational lens system SDP.81 with ALMA long-baseline observations
• How Does Feedback Affect Milky Way Satellite Formation?
• Abundance and phase-space distribution of subhalos in cosmological N-body simulations: testing numerical convergence and correction methods
• Observational constraints on phenomenological emergent dark energy and barotropic dark matter characterized by a constant equation of state parameter
• Thermodynamics of an universe with Decaying Cold Dark Matter
• HI in Local Group analogs: what does it tell us about galaxy formation?
• Producing and constraining self-interacting hidden sector dark matter
• Compact Groups in GDM Cosmological Simulations
• CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA
• Structure Formation under Inelastic Two-Component Dark Matter: Halo Statistics and Matter Power Spectra in the High-$z$ Universe
• Non-Standard Structure Formation Scenarios
• Probing Dark Matter with Strong Gravitational Lensing through an Effective Density Slope
• Complexity in small-scale dwarf spheroidal galaxies
• Constraining D-foam via the 21-cm Line
• A relic from a past merger event in the Large Magellanic Cloud
• Rotation curves with the multistate Scalar Field Dark Matter model
• Comparing dark matter and MOND hyphotheses from the distribution function of A, F, early-G stars in the solar neighbourhood
• Formation of Disk Galaxies: On the Angular Momentum Problem, the Tully-Fisher Relation and Magnetohydrodynamics
• The shapes of dark matter dominated dwarf spheroidal stellar density profiles
• Near-Field Cosmology with the Lowest-Mass Galaxies
• What is the amount of baryonic dark matter in galaxies?
• Comparison of simulations and semi-analytical model for WDM subhalo mass functions
• Addressing the too-big-to-fail problem and the void phenomenon through a modified initial power spectrum
• What can the outskirts of galaxies tell us about dark matter?
• Probing non-thermal light DM with structure formation and $N_{\mathrm{eff}}$
• Lensed stars in galaxy-galaxy strong lensing -- a JWST prediction for the Cosmic Horseshoe
• Epicyclic Density Variations in the Indus Stellar Stream
• The tidal features of the classical Milky Way satellites: Expected in MOND but inconsistent with cold dark matter models
• ALMA Measurement of 10 kpc-scale Lensing Power Spectra towards the Lensed Quasar MG J0414+0534
• Galactic Scaling Rules in a Modified Dynamical Model
• Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues
• Substructure in Dwarf Galaxies
• Formation of dwarf galaxies and small-scale problems of CDM
• The Exploration of Local VolumE Satellites (ELVES) Survey: A Nearly Volume-Limited Sample of Nearby Dwarf Satellite Systems
• Dark Matter Phenomenology: Sterile Neutrino Portal and Gravitational Portal in Extra-Dimensions
• HI Observations of Baryon-Dominated Dwarf Galaxy Candidates
• The tidal evolution of satellite galaxies in cosmological simulations: insights from COLIBRE
• WIMP Dark Matter Searches in Reticulum II Using MeerKAT
• Perspective of Galactic dark matter subhalo detection on Fermi from the EGRET observation
• Dwarf galaxies in Hickson Compact Groups
• Extending the SAGA Survey (xSAGA) I: Satellite Radial Profiles as a Function of Host Galaxy Properties
• Discovering the building blocks of dark matter halo density profiles with neural networks
• Super Interacting Dark Sector: An Improvement on Self-Interacting Dark Matter via Scaling Relations of Galaxy Clusters
• Investigating the Impacts of AGN Activities on Dwarf Galaxies with FAST HI Observations
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations IV. Testing warm dark matter cosmologies with galaxy scaling relations: A joint simulation-observation study using DREAMS simulations
• Constraining the shape of Milky Way satellites with distance gradients
• The nature of the X-ray sources in dwarf galaxies in nearby clusters from the KIWICS
• Compact High-Velocity Clouds at High Resolution
• Probing Dark Matter Substructure with Image Number Anomaly in Strong Lensing Systems
• Tidal adaptive softening and artificial fragmentation in cosmological simulations