The Structure of Cold Dark Matter Halos

Abstract

We use N-body simulations to investigate the structure of dark halos in the standard Cold Dark Matter cosmogony. Halos are excised from simulations of cosmologically representative regions and are resimulated individually at high resolution. We study objects with masses ranging from those of dwarf galaxy halos to those of rich galaxy clusters. The spherically averaged density profiles of all our halos can be fit over two decades in radius by scaling a simple ``universal'' profile. The characteristic overdensity of a halo, or equivalently its concentration, correlates strongly with halo mass in a way which reflects the mass dependence of the epoch of halo formation. Halo profiles are approximately isothermal over a large range in radii, but are significantly shallower than $r^{-2}$ near the center and steeper than $r^{-2}$ near the virial radius. Matching the observed rotation curves of disk galaxies requires disk mass-to-light ratios to increase systematically with luminosity. Further, it suggests that the halos of bright galaxies depend only weakly on galaxy luminosity and have circular velocities significantly lower than the disk rotation speed. This may explain why luminosity and dynamics are uncorrelated in observed samples of binary galaxies and of satellite/spiral systems. For galaxy clusters, our halo models are consistent both with the presence of giant arcs and with the observed structure of the intracluster medium, and they suggest a simple explanation for the disparate estimates of cluster core radii found by previous authors. Our results also highlight two shortcomings of the CDM model. CDM halos are too concentrated to be consistent with the halo parameters inferred for dwarf irregulars, and the predicted abundance of galaxy halos is larger than the observed abundance of galaxies.

compressed and uuencoded PS file. 22 pages including 14 figures. 447875 bytes. Submitted to ApJ on August 1, 1995

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• Dynamical Blueprints for Galaxies
• Dark Quest. I. Fast and Accurate Emulation of Halo Clustering Statistics and Its Application to Galaxy Clustering
• Galaxy threshing and the origin of ultra-compact dwarf galaxies in the Fornax cluster
• The Mass Profile and Accretion History of Cold Dark Matter Halos
• The SPTpol Extended Cluster Survey
• Universal thermodynamic properties of the intracluster medium over two decades in radius in the X-COP sample
• Phase-space Analysis in the Group and Cluster environment: Time since Infall and Tidal Mass Loss
• Simulations of Cosmic Chemical Enrichment
• Growth and activity of black holes in galaxy mergers with varying mass ratios
• Small-scale clumps in the galactic halo and dark matter annihilation
• Understanding the shape and diversity of dwarf galaxy rotation curves in LCDM
• Feedback and metal enrichment in cosmological SPH simulations I. A model for chemical enrichment
• Impact of Cluster Physics on the Sunyaev-Zel'dovich Power Spectrum
• A Test of the Collisional Dark Matter Hypothesis from Cluster Lensing
• Galactic accretion and the outer structure of galaxies in the CDM model
• Ram pressure stripping of halo gas in disk galaxies: Implications on galactic star formation in different environments
• The Phoenix Project: the Dark Side of Rich Galaxy Clusters
• Observational Evidence for Primordial Black Holes: A Positivist Perspective
• Gravitational lensing of wormholes in the galactic halo region
• The Luminosity Profile and Structural Parameters of the Andromeda Galaxy
• A universal density slope - velocity anisotropy relation for relaxed structures
• Intrinsic alignments of SDSS-III BOSS LOWZ sample galaxies
• Constraining the Galaxy's dark halo with RAVE stars
• Cosmic ray feedback in hydrodynamical simulations of galaxy formation
• Possible existence of wormholes in the galactic halo region
• (In)direct Detection of Boosted Dark Matter
• Cooling, AGN Feedback and Star Formation in Simulated Cool-Core Galaxy Clusters
• MAMPOSSt: Modelling Anisotropy and Mass Profiles of Observed Spherical Systems. I. Gaussian 3D velocities
• The hidden giant: discovery of an enormous Galactic dwarf satellite in Gaia DR2
• Hydrodynamical simulations of cluster formation with central AGN heating
• Suppressing star formation in quiescent galaxies with supermassive black hole winds
• A new measurement of the bulk flow of X-ray luminous clusters of galaxies
• Evolution of the atomic and molecular gas content of galaxies
• Light Dark Matter at Neutrino Experiments
• Dwarf galaxy annihilation and decay emission profiles for dark matter experiments
• Moving mesh cosmology: numerical techniques and global statistics
• The mass of a halo
• Non-thermal pressure support in X-COP galaxy clusters
• Gamma Rays from Kaluza-Klein Dark Matter
• General Relativity and Cosmology: Unsolved Questions and Future Directions
• Power Spectrum Covariance of Weak Gravitational Lensing
• Halo Cores and Phase Space Densities: Observational Constraints on Dark Matter Physics and Structure Formation
• CFHTLenS: The relation between galaxy dark matter haloes and baryons from weak gravitational lensing
• Prospects for Indirect Detection of Neutralino Dark Matter
• Wino Dark Matter Under Siege
• The Cold Dark Matter Halos of Local Group Dwarf Spheroidals
• Structure Finding in Cosmological Simulations: The State of Affairs
• A High Resolution Search for Dark-Matter Axions
• The Impact of Galaxy Formation on the Sunyaev-Zeldovich Effect of Galaxy Clusters
• Clumpy Streams from Clumpy Halos: Detecting Missing Satellites with Cold Stellar Structures
• Effect of the galactic halo modeling on the DAMA/NaI annual modulation result: an extended analysis of the data for WIMPs with a purely spin-independent coupling
• Dynamical modelling of luminous and dark matter in 17 Coma early-type galaxies
• Evidence for dark matter in the inner Milky Way
• The distribution and kinematics of early high-sigma peaks in present-day haloes: implications for rare objects and old stellar populations
• CLASH-VLT: The mass, velocity-anisotropy, and pseudo-phase-space density profiles of the z=0.44 galaxy cluster MACS 1206.2-0847
• Clumpy Neutralino Dark Matter
• Mock galaxy catalogs using the quick particle mesh method
• Quantifying baryon effects on the matter power spectrum and the weak lensing shear correlation
• The SAGA Survey. II. Building a Statistical Sample of Satellite Systems around Milky Way-like Galaxies
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum between redshift 0.6 and 1.1
• Evidence Of Dark Matter Annihilations In The WMAP Haze
• HST Observations of 10 Two-Image Gravitational Lenses
• Weak Lensing Measurement of the Mass--Richness Relation of SDSS redMaPPer Clusters
• The DiskMass Survey. VII. The distribution of luminous and dark matter in spiral galaxies
• Impact of baryon physics on dark matter structures: a detailed simulation study of halo density profiles
• X-ray and Sunyaev-Zel'dovich Effect Measurements of the Gas Mass Fraction in Galaxy Clusters
• Spectral Gamma-ray Signatures of Cosmological Dark Matter Annihilation
• CLASH-VLT: Insights on the mass substructures in the Frontier Fields Cluster MACS J0416.1-2403 through accurate strong lens modeling
• Modeling Galaxy-Mass Correlations in Dissipationless Simulations
• Red Galaxy Growth and the Halo Occupation Distribution
• On the formation and physical properties of the Intra-Cluster Light in hierarchical galaxy formation models
• Pre-Heated Isentropic Gas in Groups of Galaxies
• N-body Dark Matter Haloes with simple Hierarchical Histories
• Subaru Weak Lensing Study of Seven Merging Clusters: Distributions of Mass and Baryons
• Time-Dependent Models for Dark Matter at the Galactic Center
• Detection of Sub-TeV Gamma-Rays from the Galactic Center Direction by CANGAROO-II
• Kinematics of the stellar halo and the mass distribution of the Milky Way using BHB stars
• Simulation of the Cosmic Evolution of Atomic and Molecular Hydrogen in Galaxies
• Baryonic Pinching of Galactic Dark Matter Halos
• Bar Diagnostics in Edge-On Spiral Galaxies. III. N-Body Simulations of Disks
• Rotation Curve and Mass Distribution in the Galactic Center --- From Black Hole to Entire Galaxy ---
• A dynamically cold disk galaxy in the early Universe
• Galaxy threshing and the formation of ultra-compact dwarf galaxies
• Neutrino physics with the PTOLEMY project: active neutrino properties and the light sterile case
• Power spectrum normalization from the local abundance of rich clusters of galaxies
• Detection of the Splashback Radius and Halo Assembly bias of Massive Galaxy Clusters
• TeV Gamma-Ray Observations of the Galactic Center
• First Structure Formation: I. Primordial Star Forming Regions in hierarchical models
• A wide-field HI mosaic of Messier 31. II.The disk warp, rotation and the dark matter halo
• The Orbital Histories of Magellanic Satellites Using Gaia DR2 Proper Motions
• Observability of Dual Active Galactic Nuclei in Merging Galaxies
• Determining the Properties and Evolution of Red Galaxies from the Quasar Luminosity Function
• Off the Beaten Path: A New Approach to Realistically Model The Orbital Decay of Supermassive Black Holes in Galaxy Formation Simulations
• Dark matter in the Milky Way, II. the HI gas distribution as a tracer of the gravitational potential
• Dynamical constraints on the dark matter distribution in the Milky Way
• GASP IX. Jellyfish galaxies in phase-space: an orbital study of intense ram-pressure stripping in clusters
• And yet it moves: The dangers of artificially fixing the Milky Way center of mass in the presence of a massive Large Magellanic Cloud
• The Large-scale and Small-scale Clustering of Lyman-Break Galaxies at 3.5 < z< 5.5 from the GOODS survey
• The Dance of Heating and Cooling in Galaxy Clusters: 3D Simulations of Self-Regulated AGN Outflows
• Tracing the Dark Matter Sheet in Phase Space
• Massive binary black holes in galactic nuclei and their path to coalescence
• Galactic Halos of Fluid Dark Matter
• Neutrino Constraints on the Dark Matter Total Annihilation Cross Section
• Dark Matter Evidence, Particle Physics Candidates and Detection Methods
• Separation of Stellar Populations by an Evolving Bar: Implications for the Bulge of the Milky Way
• Shaping the galaxy stellar mass function with supernova- and AGN-driven winds
• A High-Resolution Rotation Curve of NGC 6822: A Test-case for Cold Dark Matter
• Dynamical insight into dark-matter haloes
• A Theoretical Interpretation of the Black Hole Fundamental Plane
• The dark matter halos of massive, relaxed galaxy clusters observed with Chandra
• The Evolution and Origin of Ionized Gas Velocity Dispersion from $z\sim 2.6$ to $z\sim 0.6$ with KMOS${}^{3D}$
• Vertical structure of a supernova-driven turbulent magnetized ISM
• Feedback first: the surprisingly weak effects of magnetic fields, viscosity, conduction, and metal diffusion on galaxy formation
• DarkSUSY 6 : An Advanced Tool to Compute Dark Matter Properties Numerically
• Cosmic antiprotons as a probe for supersymmetric dark matter?
• An algorithm to build mock galaxy catalogues using MICE simulations
• SDSS galaxy bias from halo mass-bias relation and its cosmological implications
• AGN feedback and triggering of star formation in galaxies
• Massive Halos in Millennium Gas Simulations: Multivariate Scaling Relations
• Galaxy clustering in the NEWFIRM Medium Band Survey: the relationship between stellar mass and dark matter halo mass at 1 < z < 2
• Mechanical AGN Feedback: Controlling the Thermodynamical Evolution of Elliptical Galaxies
• Substructure in Dark Halos: Orbital Eccentricities and Dynamical Friction
• Physical Implications of the X-ray Properties of Galaxy Groups and Clusters
• Properties of gas in and around galaxy haloes
• Galaxy merging, the Fundamental Plane of elliptical galaxies, and the Mbh-sigma relation
• How universal are the density profiles of dark halos?
• Simulating cosmic rays in clusters of galaxies - II. A unified scheme for radio halos and relics with predictions of the gamma-ray emission
• GeV excess in the Milky Way: The Role of Diffuse Galactic gamma ray Emission template
• The Disk and Dark Halo Mass of the Barred Galaxy NGC 4123. II. Fluid-Dynamical Models
• Modeling the formation and evolution of star cluster populations in galaxy simulations
• From star clusters to dwarf galaxies: The properties of dynamically hot stellar systems
• LoCuSS: Weak-lensing mass calibration of galaxy clusters
• Observational Tests of the Mass-Temperature Relation for Galaxy Clusters
• Quintessential Haloes around Galaxies
• The mass of the Milky Way from satellite dynamics
• Dynamical masses of early-type galaxies: a comparison to lensing results and implications for the stellar IMF and the distribution of dark matter
• Halo Mass and Assembly History Exposed in the Faint Outskirts: the Stellar and Dark Matter Haloes of Illustris Galaxies
• High-Resolution Measurements of the Dark Matter Halo of NGC 2976: Evidence for a Shallow Density Profile
• The Evolution of Substructure in Galaxy, Group and Cluster Haloes I: Basic Dynamics
• Constraining primordial non-Gaussianity with future galaxy surveys
• Distinguishing black holes from naked singularities through their accretion disk properties
• Neutralino Annihilation into a Photon and a Z boson
• Searching for massive clusters in weak lensing surveys
• How AGN Jets Heat the Intracluster Medium -- Insights from Hydrodynamic Simulations
• Constraints on primordial black holes from Galactic gamma-ray background
• Assembly History and Structure of Galactic Cold Dark Matter Halos
• Galaxy alignments: Theory, modelling and simulations
• Gamma-ray Constraints on Decaying Dark Matter and Implications for IceCube
• Bosonic Dark Matter in Neutron Stars and its Effect on Gravitational Wave Signal
• Voids in a $\Lambda$CDM Universe
• Strong gravitational lensing of explosive transients
• Decaying Dark Matter and the PAMELA Anomaly
• Pre-launch estimates for GLAST sensitivity to Dark Matter annihilation signals
• Dissipation and Extra Light in Galactic Nuclei: I. Gas-Rich Merger Remnants
• Galaxy Cores as Relics of Black Hole Mergers
• Detailed Chemical Abundances in the r-Process-Rich Ultra-Faint Dwarf Galaxy Reticulum 2
• Disentangling Baryons and Dark Matter in the Spiral Gravitational Lens B1933+503
• A new probe of dark matter properties: gravitational waves from an intermediate mass black hole embedded in a dark matter mini-spike
• The Atacama Cosmology Telescope: Combined kinematic and thermal Sunyaev-Zel'dovich measurements from BOSS CMASS and LOWZ halos
• Essential physics of early galaxy formation
• Stringent and Robust Constraints on the Dark Matter Annihilation Cross Section From the Region of the Galactic Center
• A Two Micron All-Sky Survey View of the Sagittarius Dwarf Galaxy: II. Swope Telescope Spectroscopy of M Giant Stars in the Dynamically Cold Sagittarius Tidal Stream
• First star-forming structures in fuzzy cosmic filaments
• Measuring the non-thermal pressure in early type galaxy atmospheres: A comparison of X-ray and optical potential profiles in M87 and NGC1399
• Dynamics of dwarf galaxies disfavor stellar-mass black hole dark matter
• The ghost of a dwarf galaxy: fossils of the hierarchical formation of the nearby spiral galaxy NGC 5907
• Explaining the entropy excess in clusters and groups of galaxies without additional heating
• Gravitational probes of dark matter physics
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2
• MAGIICAT II. General Characteristics of the MgII Absorbing Circumgalactic Medium
• The Cusp/Core Problem in Galactic Halos: Long-Slit Spectra for a Large Dwarf Galaxy Sample
• The Observed Concentration-Mass Relation for Galaxy Clusters
• Limits on Dark Matter Annihilation Signals from the Fermi LAT 4-year Measurement of the Isotropic Gamma-Ray Background
• Evolution of bias in different cosmological models
• Farthest Neighbor: The Distant Milky Way Satellite Eridanus II
• Missing Mass in Collisional Debris from Galaxies
• The Gravitational Potential Near the Sun From SEGUE K-dwarf Kinematics
• The Shape of the Gravitational Potential in Cold Dark Matter Halos
• Evidence for a Triaxial Milky Way Dark Matter Halo from the Sagittarius Stellar Tidal Stream
• Formation of Isolated Dwarf Galaxies with Feedback
• Three-Point Correlations in Weak Lensing Surveys: Model Predictions and Applications
• The Physical Nature of Starburst-Driven Galactic Outflows
• Fitting galactic rotation curves with conformal gravity and a global quadratic potential
• The Canadian Cluster Comparison Project: weak lensing masses and SZ scaling relations
• Study of the Sextans dwarf spheroidal galaxy from the DART CaII triplet survey
• Probing the missing baryons with the Sunyaev-Zel'dovich effect from filaments
• Evidence for an Intermediate-Mass Milky Way from Gaia DR2 Halo Globular Cluster Motions
• Density profiles of LCDM clusters
• Extended gamma-ray emission from Coy Dark Matter
• A Robust Excess in the Cosmic-Ray Antiproton Spectrum: Implications for Annihilating Dark Matter
• Constraining the WDM Particle Mass with Milky Way Satellites
• CLASH: Precise New Constraints on the Mass Profile of Abell 2261
• High Resolution Optical Velocity Fields of 11 Low Surface Brightness Galaxies
• A precise extragalactic test of General Relativity
• Virial masses and the baryon fraction in galaxies
• The role of minor mergers in the recent star formation history of early-type galaxies
• X-ray coronae in simulations of disc galaxy formation
• On the Orbits of Infalling Satellite Halos
• Baryons and weak lensing power spectra
• Formation and evolution of the Magellanic Clouds. I.Origin of structural, kinematical, and chemical properties of the Large Magellanic Cloud
• Galaxies in X-ray Groups I: Robust Membership Assignment and the Impact of Group Environments on Quenching
• Simulations of ram-pressure stripping in galaxy-cluster interactions
• Sneutrino cold dark matter, a new analysis: relic abundance and detection rates
• Dynamical Centers and Non-Circular Motions in THINGS Galaxies: Implications for Dark Matter Halos
• The Origin of the Density Distribution of Disk Galaxies: A New Problem for the Standard Model of Disk Formation
• On the Efficiency of the Tidal Stirring Mechanism for the Origin of Dwarf Spheroidals: Dependence on the Orbital and Structural Parameters of the Progenitor Disky Dwarfs
• A Chandra X-ray Study of Cygnus A - III. The Cluster of Galaxies
• The angular momentum distribution and baryon content of star forming galaxies at z~1-3
• The Strong Gravitational Lens Finding Challenge
• Intracluster light and the extended stellar envelopes of cD galaxies: An analytical description
• The core density of dark matter halos: a critical challenge to the Lambda-CDM paradigm?
• Hidden On-Shell Mediators for the Galactic Center Gamma-Ray Excess
• Transformation from spirals into S0s with bulge growth in groups of galaxies
• Dynamical properties of z $\sim 4.5$ dusty star-forming galaxies and their connection with local early type galaxies
• Anisotropy of the cosmic gamma-ray background from dark matter annihilation
• Microlensing-Based Estimate of the Mass Fraction in Compact Objects in Lens
• The Angular Momentum Content of Dwarf Galaxies: New Challenges for the Theory of Galaxy Formation
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: structure growth rate measurement from the anisotropic quasar power spectrum in the redshift range $0.8<z<2.2$
• On the physical origin of dark matter density profiles
• The baryon fraction of LambdaCDM haloes
• Cluster Mass Profiles from a Bayesian Analysis of Weak Lensing Distortion and Magnification Measurements: Applications to Subaru Data
• Cold Dark Matter Substructure and Galactic Disks II: Dynamical Effects of Hierarchical Satellite Accretion
• Nonthermal Emissions from Particles Accelerated by Turbulence in Clusters of Galaxies
• Dark Nuclei I: Cosmology and Indirect Detection
• Gravitational Lens Statistics for Generalized NFW Profiles: Parameter Degeneracy and Implications for Self-Interacting Cold Dark Matter
• CDM and Strong Lensing: Concord or Conflict?
• The fraction of dark matter within galaxies from the IllustrisTNG simulations
• The pattern speed of the Milky Way bar from transverse velocities
• Understanding the shape of the halo-mass and galaxy-mass cross-correlation functions
• Abundant molecular gas and inefficient star formation in intracluster regions: Ram pressure stripped tail of the Norma galaxy ESO137-001
• Lyman-alpha emission properties of simulated galaxies: interstellar medium structure and inclination effects
• Non-thermal dark matter via Affleck-Dine baryogenesis and its detection possibility
• Group-cluster merging and the formation of starburst galaxies
• Cosmic Ménage à Trois: The Origin of Satellite Galaxies On Extreme Orbits
• Dissipation and Extra Light in Galactic Nuclei: III. 'Core' Ellipticals and 'Missing' Light
• Investigating the Andromeda Stream: I. Simple Analytic Bulge-Disk-Halo Model for M31
• A Precision Search for WIMPs with Charged Cosmic Rays
• Implications of CoGeNT and DAMA for Light WIMP Dark Matter
• The recycling of gas and metals in galaxy formation: predictions of a dynamical feedback model
• Spin-independent elastic WIMP scattering and the DAMA annual modulation signal
• The MUSIC of CLASH: predictions on the concentration-mass relation
• The Weak Lensing Signal and the Clustering of BOSS Galaxies II: Astrophysical and Cosmological Constraints
• Direct measurement of dark matter halo ellipticity from two-dimensional lensing shear maps of 25 massive clusters
• Cool core cycles: Cold gas and AGN jet feedback in cluster cores
• Gamma-ray spectroscopy of Positron Annihilation in the Milky Way
• Detecting dark matter WIMPs in the Draco dwarf: a multi-wavelength perspective
• Magnetohydrodynamic Simulations of Disk Galaxy Formation: the Magnetization of The Cold and Warm Medium
• The Luminosity-Weighted or `Marked' Correlation Function
• Semi-Analytical Models for the Formation of Disk Galaxies: I. Constraints from the Tully-Fisher Relation
• CLASH-VLT: A Highly Precise Strong Lensing Model of the Galaxy Cluster RXC J2248.7-4431 (Abell S1063) and Prospects for Cosmography
• The dwarf galaxy DDO 47 as a dark matter laboratory: testing cusps hiding in triaxial halos
• The universal rotation curve of dwarf disk galaxies
• Direct Detection of Hawking Radiation from Asteroid-Mass Primordial Black Holes
• What determines satellite galaxy disruption?
• Rotation curves of UMa galaxies in the context of modified Newtonian dynamics
• On determining the cluster abundance normalization
• Indirect and direct search for dark matter
• Inverse Compton constraints on the Dark Matter e+e- excesses
• Density profile of dark matter haloes and galaxies in the Horizon-AGN simulation: the impact of AGN feedback
• The structure of dark matter halos in hierarchical clustering theories
• N-body simulations of gravitational dynamics
• Origin and evolution of halo bias in linear and non-linear regimes
• The BOSS Emission-Line Lens Survey. II. Investigating Mass-Density Profile Evolution in the SLACS+BELLS Strong Gravitational Lens Sample
• Effect of Hot Baryons on the Weak-Lensing Shear Power Spectrum
• Black Hole Space-time In Dark Matter Halo
• Implementation and performance of FDPS: A Framework Developing Parallel Particle Simulation Codes
• A Geometrically Supported $z\sim 10$ Candidate Multiply-Imaged by the Hubble Frontier Fields Cluster Abell 2744
• Core creation in galaxies and haloes via sinking massive objects
• The Inner Structure of LCDM Halos II: Halo Mass Profiles and LSB Rotation Curves
• A new viable region of the inert doublet model
• Optical-to-virial velocity ratios of local disk galaxies from combined kinematics and galaxy-galaxy lensing
• The cold veil of the Milky Way stellar halo
• Cooling flows within galactic haloes: the kinematics and properties of infalling multi-phase gas
• Searching for Primordial Black Holes in the radio and X-ray sky
• Accurate Determination of the Mass Distribution in Spiral Galaxies: II. Testing the Shape of Dark Halos
• The Planetary Nebula System and Dynamics in the Outer Halo of NGC 5128
• Tidal alignment of galaxies
• The velocity dispersion and mass profile of the Milky Way
• A Grand Rotation Curve and Dark Matter Halo in the Milky Way Galaxy
• Fate of Supermassive Black Holes and Evolution of the M(BH)-sigma Relation in Merging Galaxies: The Effect of Gaseous Dissipation
• Response of the Milky Way's disc to the Large Magellanic Cloud in a first infall scenario
• The population of Milky Way satellites in the LambdaCDM cosmology
• WIMPs at the Galactic Center
• Parametric Strong Gravitational Lensing Analysis of Abell 1689
• Galactic star formation enhanced and quenched by ram pressure in groups and clusters
• Investigating the Andromeda Stream: III. A Young Shell System in M31
• Black Hole Shadow of Sgr A${}^{\ast }$ in Dark Matter Halo
• Exploring Halo Substructure with Giant Stars X. Extended Dark Matter or Tidal Disruption?: The Case for the Leo I Dwarf Spheroidal Galaxy
• Tidal Tails Test the Equivalence Principle in the Dark Sector
• Discovering Inelastic Thermal-Relic Dark Matter at Colliders
• A light scalar WIMP through the Higgs portal and CoGeNT
• Suzaku Observation of Abell 1689: Anisotropic Temperature and Entropy Distributions Associated with the Large-Scale Structure
• Dark matter response to galaxy formation
• The Gas Content and Stripping of Local Group Dwarf Galaxies
• The Aemulus Project I: Numerical Simulations for Precision Cosmology
• Fitting the Gamma-Ray Spectrum from Dark Matter with DMFIT: GLAST and the Galactic Center Region
• The Extraordinary Amount of Substructure in the Hubble Frontier Fields Cluster Abell 2744
• Interacting Dark Matter disguised as Warm Dark Matter
• Fitting the Galactic Center Gamma-Ray Excess with Cascade Annihilations
• Pairing of Supermassive Black Holes in unequal-mass galaxy mergers
• Non-circular motions and the diversity of dwarf galaxy rotation curves
• N-Body Simulations for Coupled Scalar Field Cosmology
• Do dwarf galaxies form in tidal tails?
• Ultra Fast Outflows: Galaxy-Scale Active Galactic Nucleus Feedback
• The COpernicus COmplexio: Statistical Properties of Warm Dark Matter Haloes
• Astrophysical Probes of Unification
• Atomic Hydrogen Gas in Dark-Matter Minihalos and the Compact High Velocity Clouds
• Satellite abundances around bright isolated galaxies
• X-Ray Probing of the Central Regions of Clusters of Galaxies
• Secondary star formation within massive star clusters: Origin of multiple stellar populations in globular clusters
• Cluster-galaxy weak lensing
• Galaxies in X-ray Groups. II. A Weak Lensing Study of Halo Centering
• Kinematics of Milky Way Satellites in a Lambda Cold Dark Matter Universe
• Outskirts of Galaxy Clusters
• The velocity modulation of galaxy properties in and near clusters: quantifying the decrease in star formation in backsplash galaxies
• Radial Mixing in Galactic Disks: The Effects of Disk Structure and Satellite Bombardment
• Galaxy-galaxy Lensing: Dissipationless Simulations Versus the Halo Model
• Bending and Breathing Modes of the Galactic Disk
• Maximum Disk Mass Models for Spiral Galaxies
• The impact of mergers on relaxed X-ray clusters - II. Effects on global X-ray and SZ properties and their scaling relations
• Analytical properties of Einasto dark matter haloes
• The Distribution of Dark Matter Over 3 Decades in Radius in the Lensing Cluster Abell 611
• Organized Chaos: Scatter in the relation between stellar mass and halo mass in small galaxies
• The RASS-SDSS Galaxy Cluster Survey. III. Scaling relations of galaxy clusters
• High Energy Positrons From Annihilating Dark Matter
• Detection of substructure with adaptive optics integral field spectroscopy of the gravitational lens B1422+231
• The Clumpiness of Cold Dark Matter: Implications for the Annihilation Signal
• Dynamical Measurements of Black Hole Masses in Four Brightest Cluster Galaxies at 100 Mpc
• Dark Matter Dynamics and Indirect Detection
• Temperature and entropy profiles of nearby cooling flow clusters observed with XMM-Newton
• Signatures of Topological Defects
• The total satellite population of the Milky Way
• GOLDRUSH. II. Clustering of Galaxies at $z\sim 4-6$ Revealed with the Half-Million Dropouts Over the 100 deg${}^2$ Area Corresponding to 1 Gpc${}^3$
• Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre
• The Mass Of The Coma Cluster From Weak Lensing In The Sloan Digital Sky Survey
• The black hole mass distribution in early-type galaxies: cusps in HST photometry interpreted through adiabatic black hole growth
• Constraints on Sterile Neutrino Dark Matter
• On the Schrodinger-Poisson--Vlasov-Poisson correspondence
• The PN.S Elliptical Galaxy Survey: the dark matter in NGC 4494
• Multi-wavelength study of XMMU J2235.3-2557: the most massive galaxy cluster at z > 1
• Constraints on Dark Matter annihilations from reionization and heating of the intergalactic gas
• The dark matter halos of dwarf galaxies: a challenge for the LCDM paradigm?
• Stellar velocity profiles and line strengths out to four effective radii in the early-type galaxies NGC 3379 and NGC 821
• A Highly Magnified Star at Redshift 6.2
• Gamma ray constraints on Decaying Dark Matter
• The nature of the Diffuse Gamma-Ray Background
• The case for a cold dark matter cusp in Draco
• Dynamical Friction of a Circular-Orbit Perturber in a Gaseous Medium
• Rotating Black Hole Shadow in Perfect Fluid Dark Matter
• The Dawes Review 8: Measuring the Stellar Initial Mass Function
• The Galactic Center as a Dark Matter Gamma-Ray Source
• On the origin of cold dark matter halo density profiles
• Flat Central Density Profile and Constant DM Surface Density in Galaxies from Scalar Field Dark Matter
• Too Hot, Too Cold or Just Right? Implications of a 21-cm Signal for Dark Matter Annihilation and Decay
• On the Origin of Cores in Simulated Galaxy Clusters
• Ultra-Light Dark Matter in Ultra-Faint Dwarf Galaxies
• Galaxy Zoo: The Environmental Dependence of Bars and Bulges in Disc Galaxies
• Anatomy of the Bar Instability in Cuspy Dark Matter Halos
• Weak Gravitational Flexion
• Resolving astrophysical uncertainties in dark matter direct detection
• A novel search for high-frequency gravitational waves with low-mass axion haloscopes
• MusE GAs FLOw and Wind (MEGAFLOW) II. A study of gas accretion around $z\approx 1$ star-forming galaxies with background quasars
• The origin of the diverse morphologies and kinematics of Milky Way-mass galaxies in the FIRE-2 simulations
• The Formation of a Disk Galaxy within a Growing Dark Halo
• Weak-lensing mass calibration of redMaPPer galaxy clusters in Dark Energy Survey Science Verification data
• Intracluster light: a luminous tracer for dark matter in clusters of galaxies
• Volumetric star formation laws of disc galaxies
• The Aemulus Project III: Emulation of the Galaxy Correlation Function
• Redshift Evolution of Galaxy Cluster Densities
• The virial theorem and the dark matter problem in hybrid metric-Palatini gravity
• Baryonic impact on the dark matter distribution in Milky Way-size galaxies and their satellites
• Chaotic cold accretion on to black holes in rotating atmospheres
• Ultrahigh Energy Cosmic Rays: The state of the art before the Auger Observatory
• Constraining Dissipative Dark Matter Self-Interactions
• The mass of our Milky Way
• Constraining dark energy from the abundance of weak gravitational lenses
• X-Ray and Optical Microlensing in the Lensed Quasar PG 1115+080
• Modeling Angular-Momentum History in Dark-Matter Halos
• X-ray Temperature and Mass Measurements to the Virial Radius of Abell 1413 with Suzaku
• Beyond Assembly Bias: Exploring Secondary Halo Biases for Cluster-size Haloes
• Astrophysical Probes of the Vainshtein Mechanism: Stars and Galaxies
• The Sensitivity of Harassment to Orbit: Mass Loss from Early-Type Dwarfs in Galaxy Clusters
• Towards a Resolution of the Galactic Spin Crisis: Mergers, Feedback, and Spin Segregation
• The Quantity of Intracluster Light: Comparing Theoretical and Observational Measurement Techniques Using Simulated Clusters
• The phase-space structure of cold dark-matter halos: Insights into the Galactic halo
• The surface brightness of dark matter: unique signatures of neutralino annihilation in the Galactic halo
• Do globular clusters possess Dark Matter halos? A case study in NGC 2419
• The Structure and Clustering of Lyman Break Galaxies
• Sensitivity Projections for Dark Matter Searches with the Fermi Large Area Telescope
• A profile in FIRE: resolving the radial distributions of satellite galaxies in the Local Group with simulations
• Boson Stars and Oscillatons: A Review
• TeV gamma-rays and the largest masses and annihilation cross sections of neutralino dark matter
• KiDS-1000 Methodology: Modelling and inference for joint weak gravitational lensing and spectroscopic galaxy clustering analysis
• Central mass-to-light ratios and dark matter fractions in early-type galaxies
• Evolution of Stellar-to-Halo Mass Ratio at z=0-7 Identified by Clustering Analysis with the Hubble Legacy Imaging and Early Subaru/Hyper Suprime-Cam Survey Data
• The Cusp/Core problem and the Secondary Infall Model
• CLASH-VLT: Dissecting the Frontier Fields Galaxy Cluster MACS J0416.1-2403 with $\sim 800$ Spectra of Member Galaxies
• A massive stellar bulge in a regularly rotating galaxy 1.2 billion years after the Big Bang
• Superheavy dark matter and IceCube neutrino signals:bounds on decaying dark matter
• Dark matter halos of massive elliptical galaxies at $z\sim 0.2$ are well described by the Navarro-Frenk-White profile
• Dwarf Galaxy Dark Matter Density Profiles Inferred from Stellar and Gas Kinematics
• Orbits of Massive Satellite Galaxies: I. A Close Look at the Large Magellanic Cloud and a New Orbital History for M33
• The Dark Matter Distribution in Abell 383: Evidence for a Shallow Density Cusp from Improved Lensing, Stellar Kinematic and X-ray Data
• The Orbit of the Orphan Stream
• SDSS-IV MaNGA: Global stellar population and gradients for about 2000 early-type and spiral galaxies on the mass-size plane
• The ESO Nearby Abell Cluster Survey. XII. The mass and mass-to-light-ratio profiles of rich clusters
• A comprehensive catalog of dark matter halo models for SPARC galaxies
• AutoLens: Automated Modeling of a Strong Lens's Light, Mass and Source
• Template Rotation Curves for Disk Galaxies
• Hierarchical Formation of Dark Matter Halos and the Free Streaming Scale
• Ellipticity of dark matter halos with galaxy-galaxy weak lensing
• Ultra-Light Dark Matter Resonates with Binary Pulsars
• The 2dF-SDSS LRG and QSO survey: evolution of the clustering of luminous red galaxies since z = 0.6
• Frontier Fields: High-Redshift Predictions and Early Results
• Structure formation in large-volume cosmological simulations of fuzzy dark matter: Impact of the non-linear dynamics
• An extensive study of dynamical friction in dwarf galaxies: the role of stars, dark matter, halo profiles and MOND
• Dark Matter Annihilation in Substructures Revised
• Detection of the kinematic Sunyaev-Zel'dovich effect with DES Year 1 and SPT
• A volume-limited sample of X-ray galaxy groups and clusters - I. Radial entropy and cooling time profiles
• The constant density region of the dark halos of spiral galaxies
• Baryon-induced dark matter cores in the EAGLE simulations
• Modelling the line-of-sight contribution in substructure lensing
• Angular momentum transport and disk morphology in SPH simulations of galaxy formation
• Radial distribution and strong lensing statistics of satellite galaxies and substructure using high resolution LCDM hydrodynamical simulations
• Gamma Ray Line Constraints on Effective Theories of Dark Matter
• Mismatch and Misalignment: Dark Haloes and Satellites of Disc Galaxies
• Prospects for Beyond the Standard Model Physics Searches at the Deep Underground Neutrino Experiment
• Chandra Observations of the Lensing Cluster EMSS 1358+6245: Implications for Self-Interacting Dark Matter
• On the capture of dark matter by neutron stars
• Halo Profiles and the Concentration-Mass Relation for a ΛCDM Universe
• Subaru through a different lens: microlensing by extended dark matter structures
• Proper Motions, Orbits, and Tidal Influences of Milky Way Dwarf Spheroidal Galaxies
• The Dark Matter Density Profile of the Fornax Dwarf
• Is every strong lens model unhappy in its own way? Uniform modelling of a sample of 13 quadruply+ imaged quasars
• The Growth of Massive Black Holes in Galaxy Merger Simulations with Feedback by Radiation Pressure
• CosmoDC2: A Synthetic Sky Catalog for Dark Energy Science with LSST
• On determining the shape of matter distributions
• The Planetary Nebula System of M33
• A deep search for decaying dark matter with XMM-Newton blank-sky observations
• Where will supersymmetric dark matter first be seen?
• Dependence of the Inner DM Profile on the Halo Mass
• Galactic halo cusp-core: tidal compression in mergers
• Parkes Pulsar Timing Array constraints on ultralight scalar-field dark matter
• Evidence of Halo Assembly Bias in Massive Clusters
• Pushing back the limits: detailed properties of dwarf galaxies in a LCDM universe
• On The Formation of Disk Galaxies and Massive Central Objects
• Joint constraints on thermal relic dark matter from strong gravitational lensing, the Lyman-$\alpha$ forest, and Milky Way satellites
• Dark matter in Draco and the Local Group: Implications for direct detection experiments
• Massive Coronae of Galaxies
• Second-order Lagrangian perturbation theory initial conditions for resimulations
• Cosmic shear statistics in the Suprime-Cam 2.1 sq deg field: Constraints on Omega_m and sigma_8
• Neutrinos from Inert Doublet Dark Matter
• On the road to percent accuracy: nonlinear reaction of the matter power spectrum to dark energy and modified gravity
• Shape of Dark Matter Haloes in the Illustris Simulation: Effects of Baryons
• Detecting Lensing-Induced Diffraction in Astrophysical Gravitational Waves
• Experimental Constraints on Self-consistent Reionization Models
• Arc Statistics in Triaxial Dark Matter Halos: Testing the Collisionless Cold Dark Matter Paradigm
• The environmental dependence of the stellar mass function at z~1: Comparing cluster and field between the GCLASS and UltraVISTA surveys
• The Signature of Galactic Tides in Local Group Dwarf Spheroidals
• Weak Lensing by High-Redshift Clusters of Galaxies - I: Cluster Mass Reconstruction
• All about baryons: revisiting SIDM predictions at small halo masses
• Time dependent couplings in the dark sector: from background evolution to nonlinear structure formation
• Detecting Axion Dark Matter with Radio Lines from Neutron Star Populations
• Quasars Probing Galaxies: I. Signatures of Gas Accretion at Redshift Approximately 0.2
• Low-mass halo perturbations in strong gravitational lenses at redshift z$\sim$0.5 are consistent with CDM
• Directional statistics for WIMP direct detection
• Reconciling the Diversity and Uniformity of Galactic Rotation Curves with Self-Interacting Dark Matter
• Galaxy formation using halo merger histories taken from N-body simulations
• The detailed structure and the onset of galaxy formation in low-mass gaseous dark matter haloes
• LoCuSS: Calibrating Mass-Observable Scaling Relations for Cluster Cosmology with Subaru Weak Lensing Observations
• The local high velocity tail and the Galactic escape speed
• The Galactic Center GeV Excess from a Series of Leptonic Cosmic-Ray Outbursts
• The splashback radius of halos from particle dynamics. II. Dependence on mass, accretion rate, redshift, and cosmology
• Kinematics of tidal tails in interacting galaxies: Tidal Dwarf Galaxies and projection effects
• Observations and Theoretical Implications of the Large Separation Lensed Quasar SDSS J1004+4112
• Early structure in LCDM
• AREPO-RT: Radiation hydrodynamics on a moving mesh
• The Substructure Hierarchy in Dark Matter Haloes
• Global fits of GUT-scale SUSY models with GAMBIT
• A History of HI Stripping in Virgo: A Phase-space View of VIVA Galaxies
• The mass distribution of the Fornax dSph: constraints from its globular cluster distribution
• COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses IX. Time delays, lens dynamics and baryonic fraction in HE 0435-1223
• Connection Between the Circumgalactic Medium and the Interstellar Medium of Galaxies: Results from the COS-GASS Survey
• Rotation Curves in z~1-2 Star-Forming Disks: Evidence for Cored Dark Matter Distributions
• Dark Matter Strikes Back at the Galactic Center
• Quantitative Estimates of Environmental Effects on the Star Formation Rate of Disk Galaxies in Clusters of Galaxies
• Scattering, Damping, and Acoustic Oscillations: Simulating the Structure of Dark Matter Halos with Relativistic Force Carriers
• Dark matter in elliptical galaxies: I. Is the total mass density profile of the NFW form or even steeper?
• The Proper Motion Field of the Small Magellanic Cloud: Kinematic Evidence for its Tidal Disruption
• H0LiCOW XII. Lens mass model of WFI2033-4723 and blind measurement of its time-delay distance and $H_0$
• Collisional dark matter and the structure of dark halos
• An inventory of the stellar initial mass function in early-type galaxies
• Modeling baryonic physics in future weak lensing surveys
• Constraining Dark Halo Potentials with Tidal Tails
• AGN self-regulation in cooling flow clusters
• The SRG/eROSITA all-sky survey: Cosmology constraints from cluster abundances in the western Galactic hemisphere
• Dark matter searches with Cherenkov telescopes: nearby dwarf galaxies or local galaxy clusters?
• Nearest Neighbor: The Low-Mass Milky Way Satellite Tucana III
• Effects of Dark Matter Substructures on Gravitational Lensing: Results from the Aquarius Simulations
• Estimating the dark matter halo mass of our Milky Way using dynamical tracers
• Mass and Hot Baryons in Massive Galaxy Clusters from Subaru Weak Lensing and AMiBA SZE Observations
• Inflation, cold dark matter, and the central density problem
• The Luminosity-Temperature Relation for Groups and Clusters of Galaxies
• The circumgalactic medium of eBOSS emission line galaxies: signatures of galactic outflows in gas distribution and kinematics
• On the formation of dwarf galaxies and stellar halos
• Astrophysical uncertainties on direct detection experiments
• Simulations of cosmic ray feedback by AGN in galaxy clusters
• Antiprotons from dark matter annihilation in the Galaxy: astrophysical uncertainties
• The Globular Cluster System of NGC 1399. II. Kinematics of a Large Sample of Globular Clusters
• Scrutinizing the evidence for dark matter in cosmic-ray antiprotons
• Galactic Center Gamma-Ray Excess from Dark Matter Annihilation: Is There A Black Hole Spike?
• Sunyaev-Zel'dovich-Measured Pressure Profiles from the Bolocam X-ray/SZ Galaxy Cluster Sample
• KiDS-450: Cosmological Constraints from Weak Lensing Peak Statistics-I: Inference from Analytical Prediction of High Signal-to-Noise Ratio Convergence Peaks
• The ongoing assembly of a central cluster galaxy: Phase-space substructures in the halo of M87
• The universal distribution of halo interlopers in projected phase space. Bias in galaxy cluster concentration and velocity anisotropy?
• Measuring the dark matter environments of black hole binaries with gravitational waves
• Can dry merging explain the size evolution of early-type galaxies?
• Collapse of a self-gravitating Bose-Einstein condensate with attractive self-interaction
• High resolution imaging of the anomalous flux-ratio gravitational lens system CLASS B2045+265: Dark or luminous satellites?
• Gamma rays and positrons from a decaying hidden gauge boson
• Two body relaxation in CDM simulations
• Global Probes of the Impact of Baryons on Dark Matter Halos
• Generation of mock tidal streams
• Gas density and X-ray surface brightness profiles of clusters of galaxies from dark matter halo potentials: beyond the isothermal beta model
• Tidal stripping and the structure of dwarf galaxies in the Local Group
• Barred galaxies in the EAGLE cosmological hydrodynamical simulation
• Search for Dark Matter from the Galactic Halo with the IceCube Neutrino Observatory
• Deep symbolic regression for physics guided by units constraints: toward the automated discovery of physical laws
• Decomposition of the visible and dark matter in the Einstein ring 0047-2808 by semi-linear inversion
• On the Importance of Electroweak Corrections for Majorana Dark Matter Indirect Detection
• Baryonic clues to the puzzling diversity of dwarf galaxy rotation curves
• Analytic Cross Sections for Substructure Lensing
• SILCC VI -- Multi-phase ISM structure, stellar clustering, and outflows with supernovae, stellar winds, ionising radiation and cosmic rays
• A Comparison between Semi-Analytic Model Predictions for the CANDELS Survey
• On the Progenitor of Binary Neutron Star Merger GW170817
• Velocity-dependent Self-interacting Dark Matter from Groups and Clusters of Galaxies
• Search for dark matter annihilation signatures in H.E.S.S. observations of Dwarf Spheroidal Galaxies
• Unstable Relics as a Source of Galactic Positrons
• The Clustering of Massive Halos
• Falling outer rotation curves of star-forming galaxies at 0.6 < z < 2.6 probed with KMOS^3D and SINS/ZC-SINF
• The halo model as a versatile tool to predict intrinsic alignments
• A Telescope Search for Decaying Relic Axions
• The Masses and Shapes of Dark Matter Halos from Galaxy-Galaxy Lensing in the CFHTLS
• A Statistical Analysis of Supersymmetric Dark Matter in the MSSM after WMAP
• The Cloud Factory I: Generating resolved filamentary molecular clouds from galactic-scale forces
• An Alternative Origin for Hypervelocity Stars
• Combining weak and strong cluster lensing: Applications to simulations and MS 2137
• Model-based pattern speed estimates for 38 barred galaxies
• Dark Atoms: Asymmetry and Direct Detection
• Dark stars at the Galactic centre - the main sequence
• Neutron stars: new constraints on asymmetric dark matter
• Decaying Dark Matter in Light of the PAMELA and Fermi LAT Data
• The impact of cluster mergers on arc statistics
• The shape of the dark matter halo in the early-type galaxy NGC 2974
• First Star Signature in Infrared Background Anisotropies
• Dark Matter in the Milky Way's Dwarf Spheroidal Satellites
• Thermal conduction in cosmological SPH simulations
• Halo-to-Halo Similarity and Scatter in the Velocity Distribution of Dark Matter
• Galaxy Kinematics with VIRUS-P: The Dark Matter Halo of M87
• Luminous and Dark Matter in the Milky Way
• Green Bank and Effelsberg Radio Telescope Searches for Axion Dark Matter Conversion in Neutron Star Magnetospheres
• Robust HI kinematics of gas-rich ultra-diffuse galaxies: hints of a weak-feedback formation scenario
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: the low redshift sample
• Contribution of stripped nuclear clusters to globular cluster and ultra-compact dwarf galaxy populations
• Constraining the role of star cluster mergers in nuclear cluster formation: Simulations confront integral-field data
• Stream-orbit misalignment I: The dangers of orbit-fitting
• The accretion history of dark matter halos II: The connections with the mass power spectrum and the density profile
• Letter of Intent: Jinping Neutrino Experiment
• Limitations to the "basic'' HOD model and beyond
• Semi-Analytical Models for Lensing by Dark Halos: I. Splitting Angles
• Indirect Search for Neutralino Dark Matter with High Energy Neutrinos
• Low Redshift Baryon Acoustic Oscillation Measurement from the Reconstructed 6-degree Field Galaxy Survey
• Breaking the Degeneracies Between Cosmology and Galaxy Bias
• The importance of major mergers in the build up of stellar mass in brightest cluster galaxies at z=1
• Internal kinematics and dynamical models of dwarf spheroidal galaxies around the Milky Way
• Clusters of galaxies in the local universe
• The evolution of the Tully-Fisher relation between z~2.3 and z~0.9 with KMOS^3D
• The Halo Boundary of Galaxy Clusters in the SDSS
• The dark degeneracy and interacting cosmic components
• Small scatter and nearly-isothermal mass profiles to four half-light radii from two-dimensional stellar dynamics of early-type galaxies
• Dark matter annihilation or unresolved astrophysical sources? Anisotropy probe of the origin of cosmic gamma-ray background
• The Collision Between The Milky Way And Andromeda
• Peak star formation efficiency and no missing baryons in massive spirals
• Indirect Searches for Decaying Dark Matter
• A weighty interpretation of the Galactic Centre excess
• Revealing the complex nature of the strong gravitationally lensed system H-ATLAS J090311.6+003906 using ALMA
• Searching for Dark Matter with Future Cosmic Positron Experiments
• Investigating the Origins of Dark Matter Halo Density Profiles
• The stellar-to-halo mass relation of GAMA galaxies from 100 square degrees of KiDS weak lensing data
• The Dynamical State and Mass-Concentration Relation of Galaxy Clusters
• Mapping the Dark Side with DEIMOS: Globular Clusters, X-ray Gas, and Dark Matter in the NGC 1407 Group
• Interpreting the Observed Clustering of Red Galaxies at z~3
• Dynamics of Stars and Globular Clusters in M87
• Full-shape cosmology analysis of SDSS-III BOSS galaxy power spectrum using emulator-based halo model: a $5\%$ determination of ${\sigma }_8$
• The Gravitational Force Field of the Galaxy Measured From the Kinematics of RR Lyrae in Gaia
• The Robustness of Dark Matter Density Profiles in Dissipationless Mergers
• Orbital decomposition of CALIFA spiral galaxies
• Minimum mass of galaxies from BEC or scalar field dark matter
• Dark and Baryonic Matter in Bright Spiral Galaxies: II. Radial Distributions for 34 Galaxies
• The Copernicus Complexio: a high-resolution view of the small-scale Universe
• The real-space clustering of luminous red galaxies around z<0.6 quasars in the Sloan Digital Sky Survey
• Bar-Induced Evolution of Dark Matter Cusps
• The X-ray Halo Scaling Relations of Supermassive Black Holes
• The Sloan Lens ACS Survey. XII. Extending Strong Lensing to Lower Masses
• Galaxy Formation with BECDM -- II. Cosmic Filaments and First Galaxies
• The Kinematic Signature of Face-On Peanut-Shaped Bulges
• Density Profiles of CDM Microhalos and their Implications for Annihilation Boost Factors
• Simulating the interaction of jets with the intra-cluster medium
• Coevolution of dust, gas, and stars in galaxies - I. Spatial distributions and scaling-relations of dust and molecular hydrogen
• Dark matter-neutrino interactions through the lens of their cosmological implications
• $S^5$: Probing the Milky Way and Magellanic Clouds potentials with the 6-D map of the Orphan-Chenab stream
• Cosmological Constraints From Weak Lensing Peak Statistics With CFHT Stripe 82 Survey
• Space- and Ground-Based Gamma-Ray Astrophysics
• Redshift space bias and beta from the halo model
• The halo model and numerical simulations
• Galaxy Groups at Intermediate Redshift
• Gravitational polarization and the phenomenology of MOND
• Model-Independent Bound on the Dark Matter Lifetime
• Self-Interacting Dark Matter from the Hidden Heterotic-String Sector
• Disc galaxy evolution models in a hierarchical formation scenario: structure and dynamics
• Density-potential pairs for spherical stellar systems with Sersic light-profiles and (optional) power-law cores
• Scaling Laws in the Distribution of Galaxies
• TDCOSMO. XII. Improved Hubble constant measurement from lensing time delays using spatially resolved stellar kinematics of the lens galaxy
• The Mass Assembly of Fossil Groups of Galaxies in the Millennium Simulation
• Cosmology and the Halo Occupation Distribution from Small-Scale Galaxy Clustering in the Sloan Digital Sky Survey
• Dissipation and the Fundamental Plane: Observational Tests
• Constraining the Matter Power Spectrum Normalization using the SDSS/RASS and REFLEX Cluster surveys
• The outer halo globular cluster system of M31 - II. Kinematics
• Constraining chameleon models with cosmology
• Detailed comparison of the structures and kinematics of simulated and observed barred galaxies
• The Hubble Constant
• Positrons and antiprotons from inert doublet model dark matter
• Building disc structure and galaxy properties through angular momentum: The DARK SAGE semi-analytic model
• LoCuSS: The Sunyaev-Zel'dovich Effect and Weak Lensing Mass Scaling Relation
• A model for the postcollapse equilibrium of cosmological structure: truncated isothermal spheres from top-hat density perturbations
• Dynamics of the Magellanic Clouds in a LCDM Universe
• The Angular Momentum Distribution of Gas and Dark Matter in Galactic Halos
• The Ursa Major Cluster of Galaxies. II. Bimodality of the Distribution of Central Surface Brightnesses
• Search for neutrinos from decaying dark matter with IceCube
• H.E.S.S. constraints on Dark Matter annihilations towards the Sculptor and Carina Dwarf Galaxies
• Probing dark matter substructure in the gravitational lens HE0435-1223 with the WFC3 grism
• Simple models of cooling flows
• Not too big, not too small: the dark halos of the dwarf spheroidals in the Milky Way
• The Baryon Fractions and Mass-to-Light Ratios of Early-Type Galaxies
• The effect of baryons on the inner density profiles of rich clusters
• The Dark Disk of the Milky Way
• Antiprotons from Dark Matter: Current constraints and future sensitivities
• The redshift space power spectrum in the halo model
• Dark matter content and internal dynamics of NGC 4697: NMAGIC particle models from slit data and planetary nebulae velocities
• Identifying true satellites of the Magellanic Clouds
• Diffuse X-Ray Emission from Late-Type Galaxy Haloes
• A survey of dual active galactic nuclei in simulations of galaxy mergers: frequency and properties
• The mass discrepancy acceleration relation in a $\Lambda$CDM context
• Dancing to ChaNGa: A Self-Consistent Prediction For Close SMBH Pair Formation Timescales Following Galaxy Mergers
• Interplay among Cooling, AGN Feedback and Anisotropic Conduction in the Cool Cores of Galaxy Clusters
• Structure of Dark Matter Halos From Hierarchical Clustering. III. Shallowing of The Inner Cusp
• How galaxies form stars: the connection between local and global star formation in galaxy simulations
• Possible existence of wormholes in the central regions of halos
• Cores of Dark Matter Halos Correlate with Disk Scale Lengths
• Dark matter spikes in the vicinity of Kerr black holes
• Limits on the Radiative Decay of Sterile Neutrino Dark Matter from the Unresolved Cosmic and Soft X-ray Backgrounds
• Neutrino Clustering in Cold Dark Matter Halos : Implications for Ultra High Energy Cosmic Rays
• RASS-SDSS Galaxy Cluster Survey. VII. On the Cluster Mass to Light ratio and the Halo Occupation Distribution
• The Detectability of Neutralino Clumps via Atmospheric Cherenkov Telescopes
• On the identification of merger debris in the {\it Gaia} Era
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Gravity test from the combination of redshift-space distortions and galaxy-galaxy lensing at $0.5<z<1.2$
• Dark matter profiles and annihilation in dwarf spheroidal galaxies: prospectives for present and future gamma-ray observatories - I. The classical dSphs
• Formation times, mass growth histories and concentrations of dark matter haloes
• Search for Neutrinos from Dark Matter Self-Annihilations in the center of the Milky Way with 3 years of IceCube/DeepCore
• Revealing the galaxy-halo connection in IllustrisTNG
• Dark matter effect on the weak deflection angle by black holes at the center of Milky Way and M87 galaxies
• Gravitational wave probes of dark matter: challenges and opportunities
• Diversity of dark matter density profiles in the Galactic dwarf spheroidal satellites
• X-ray, lensing and Sunyaev Zel'dovich triaxial analysis of Abell 1835 out to R_{200}
• The Splashback Feature around DES Galaxy Clusters: Galaxy Density and Weak Lensing Profiles
• The Hot Gas Content of Low-Luminosity Early-Type Galaxies and the Implications Regarding Supernova Heating and AGN Feedback
• Tidal debris morphology and the orbits of satellite galaxies
• Diurnal and Annual Modulation of Cold Dark Matter Signals
• Investigating halo substructures with annual modulation signature
• Strong-Lensing Analysis of MACS,J0717.5+3745 from Hubble Frontier Fields observations: How well can the mass distribution be constrained?
• Weak-Lensing Mass Calibration of ACTPol Sunyaev-Zel'dovich Clusters with the Hyper Suprime-Cam Survey
• Quenching Cluster Cooling Flows with Recurrent Hot Plasma Bubbles
• The devil is in the tails: the role of globular cluster mass evolution on stream properties
• Radial constraints on the Initial Mass Function from TiO features and Wing-Ford band in Early-type Galaxies
• Gamma-ray Signal from Earth-mass Dark Matter Microhalos
• Cosmic ray driven Galactic winds
• Dark matter annihilation and decay from non-spherical dark halos in the Galactic dwarf satellites
• A Tail of Two Populations: Chemo-dynamics of the Sagittarius Stream and Implications for its Original Mass
• Strong Upper Limits on Sterile Neutrino Warm Dark Matter
• Antimatter Signatures of Gravitino Dark Matter Decay
• Galactic neutron stars I. Space and velocity distributions in the disk and in the halo
• The splashback radius of halos from particle dynamics. I. The SPARTA algorithm
• Self-Interacting Dark Matter Subhalos in the Milky Way's Tides
• The Cosmic Axion Background
• Direct formation of supermassive black holes in metal-enriched gas at the heart of high-redshift galaxy mergers
• Simulated Dark-Matter Halos as a Test of Nonextensive Statistical Mechanics
• The Dark Halo - Spheroid Conspiracy and the Origin of Elliptical Galaxies
• Naturalness of Light Neutralino Dark Matter in pMSSM after LHC, XENON100 and Planck Data
• Satellite Systems around Galaxies in Hydrodynamic Simulations
• Towards the Final Word on Neutralino Dark Matter
• Gaia DR2 in 6D: Searching for the fastest stars in the Galaxy
• Rotation of Halo Populations in the Milky Way and M31
• Constraints on the mass-richness relation from the abundance and weak lensing of SDSS clusters
• Density profiles of dark matter haloes: diversity and dependence on environment
• Gravitational Wave Background from a Cosmological Population of Core-Collapse Supernovae
• Numerical convergence of simulations of galaxy formation: the abundance and internal structure of cold dark matter haloes
• A 40-billion solar mass black hole in the extreme core of Holm 15A, the central galaxy of Abell 85
• Physical properties underlying observed kinematics of satellite galaxies
• The XMM Cluster Survey: Testing chameleon gravity using the profiles of clusters
• Updated cosmic-ray and radio constraints on light dark matter: Implications for the GeV gamma-ray excess at the Galactic center
• Some like it triaxial: the universality of dark matter halo shapes and their evolution along the cosmic time
• Mock weak lensing analysis of simulated galaxy clusters: bias and scatter in mass and concentration
• Kerr-Newman-AdS Black Hole Surrounded by Perfect Fluid Matter in Rastall Gravity
• Properties of gas clumps and gas clumping factor in the intra cluster medium
• Effects of baryon removal on the structure of dwarf spheroidal galaxies
• Cores and Cusps in the Dwarf Spheroidals
• Models of the Cosmic Horseshoe Gravitational Lens
• Measuring neutrino masses and dark energy with weak lensing tomography
• Discovery of Ultra-Compact Dwarf Galaxies in the Virgo Cluster
• The Velocity Function of Galaxies
• The asymptotic tidal remnants of cold dark matter subhalos
• Diffuse Baryons in Groups and Clusters of Galaxies
• The SAURON Project - XIV. No escape from V${}_{\mathrm{esc}}$: a global and local parameter in early-type galaxy evolution
• Dark matters on the scale of galaxies
• Mass-to-light ratio gradients in early-type galaxy haloes
• Using Galaxy Two-point Correlation Functions to Determine the Redshift Distributions of Galaxies Binned by Photometric Redshift
• $e^{\pm }$ Excesses in the Cosmic Ray Spectrum and Possible Interpretations
• Cosmic rays from Leptonic Dark Matter
• Intense Gamma-Ray Lines from Hidden Vector Dark Matter Decay
• How to break the density-anisotropy degeneracy in spherical stellar systems
• Molecular Gas Dominated 50 kpc Ram Pressure Stripped Tail of the Coma Galaxy D100
• Two Disk Components from a Gas Rich Disk-Disk Merger
• The Orbital Evolution Induced by Baryonic Condensation in Triaxial Halos
• A Large Dark Matter Core in the Fornax Dwarf Spheroidal Galaxy?
• GASP II. A MUSE view of extreme ram-pressure stripping along the line of sight: kinematics of the jellyfish galaxy JO201
• Strong lensing models of eight CLASH clusters from extensive spectroscopy: accurate total mass reconstructions in the cores
• Non-Baryonic Dark Matter in Cosmology
• A determination of H_0 with the CLASS gravitational lens B1608+656: II. Mass models and the Hubble constant from lensing
• Dark Energy Survey Year 3 results: curved-sky weak lensing mass map reconstruction
• Effect of halo modelling on WIMP exclusion limits
• High Energy Positrons and the WMAP Haze from Exciting Dark Matter
• Cosmological Origin of the Stellar Velocity Dispersions in Massive Early-Type Galaxies
• The dark matter interpretation of the 3.5-keV line is inconsistent with blank-sky observations
• Reopening the Higgs portal for Singlet Scalar Dark Matter
• The phase space density of fermionic dark matter haloes
• Stellar Streams as Probes of Dark Halo Mass and Morphology: A Bayesian Reconstruction
• Gravitational contraction versus Supernova driving and the origin of the velocity dispersion-size relation in molecular clouds
• Prospects to verify a possible dark matter hint in cosmic antiprotons with antideuterons and antihelium
• Regularized orbit models unveiling the stellar structure and dark matter halo of the Coma elliptical NGC 4807
• Constraints on dark matter annihilation from CMB observations before Planck
• Absolute HST Proper Motion (HSTPROMO) of Distant Milky Way Globular Clusters: Galactocentric Space Velocities and the Milky Way Mass
• Low energy antideuterons: shedding light on dark matter
• The Highest Resolution Mass Map of Galaxy Cluster Substructure To Date Without Assuming Light Traces Mass: LensPerfect Analysis of Abell 1689
• X-ray Emission from Haloes of Simulated Disc Galaxies
• Simulations of the dynamics of magnetised jets and cosmic rays in galaxy clusters
• Supermassive Black Hole Formation at High Redshifts via Direct Collapse: Physical Processes in the Early Stage
• No cores in dark matter-dominated dwarf galaxies with bursty star formation histories
• The Structure of Halos: Implications for Group and Cluster Cosmology
• Outflows Driven by Quasars in High-Redshift Galaxies with Radiation Hydrodynamics
• Status of Dark Matter in the Universe
• Stellar Structure of Dark Stars: a first phase of Stellar Evolution due to Dark Matter Annihilation
• The Novel Probes Project -- Tests of Gravity on Astrophysical Scales
• Efficient solution of the anisotropic spherically-aligned axisymmetric Jeans equations of stellar hydrodynamics for galactic dynamics
• A giant elliptical galaxy with a lightweight initial mass function
• The Large-scale Distribution of Cool Gas around Luminous Red Galaxies
• Please repeat: Strong lensing of gravitational waves as a probe of compact binary and galaxy populations
• The route to massive black hole formation via merger-driven direct collapse: a review
• Orbit-based dynamical models of the Sculptor dSph galaxy
• Galaxy-galaxy lensing constraints on the relation between baryons and dark matter in galaxies in the Red Sequence Cluster Survey 2
• A Cross-Correlation Analysis of Mg II Absorption Line Systems and Luminous Red Galaxies from the SDSS DR5
• The CoDECS project: a publicly available suite of cosmological N-body simulations for interacting dark energy models
• The origin of the mass discrepancy-acceleration relation in $\Lambda$CDM
• The Self-Regulated Growth of Supermassive Black Holes
• Detecting the Stimulated Decay of Axions at Radio Frequencies
• Quenching of Satellite Galaxies at the Outskirts of Galaxy Clusters
• DarkBit: A GAMBIT module for computing dark matter observables and likelihoods
• Higgs in Space!
• Constraining dark matter late-time energy injection: decays and p-wave annihilations
• The New Horizon Run Cosmological N-Body Simulations
• The PAMELA and ATIC Excesses From a Nearby Clump of Neutralino Dark Matter
• Scaling Properties of Galaxy Groups
• Evidence Against Dark Matter Halos Surrounding the Globular Clusters MGC1 and NGC 2419
• Reproducing the Kinematics of Damped Lyman-alpha Systems
• Substructure of fuzzy dark matter haloes
• A Measurement of Gravitational Lensing of the Cosmic Microwave Background by Galaxy Clusters Using Data from the South Pole Telescope
• Fast rotating and low-turbulence discs at $z\simeq 4.5$: Dynamical evidence of their evolution into local early-type galaxies
• Multi-Step Cascade Annihilations of Dark Matter and the Galactic Center Excess
• The impact of radio feedback from active galactic nuclei in cosmological simulations: Formation of disk galaxies
• Signatures of Majorana dark matter with t-channel mediators
• Galaxy Cluster Mass Reconstruction Project: II. Quantifying scatter and bias using contrasting mock catalogues
• Model comparison of the dark matter profiles of Fornax, Sculptor, Carina and Sextans
• Improved Modeling of the Mass Distribution of Disk Galaxies by the Einasto Halo Model
• Hiding Cusps in Cores: Kinematics of Disk Galaxies in Triaxial Dark Matter Halos
• The Dynamical and Chemical Evolution of Dwarf Spheroidal Galaxies with GEAR
• Closing the Loop: A Self-Consistent Model of Optical, X-ray, and SZ Scaling Relations for Clusters of Galaxies
• Mimicking dark matter in galaxy clusters through a non-minimal gravitational coupling with matter
• Gamma rays from the annihilation of singlet scalar dark matter
• Exoplanets as Sub-GeV Dark Matter Detectors
• Go with the Flow: Understanding Inflow Mechanisms in Galaxy Collisions
• Hunt for Light Primordial Black Hole Dark Matter with Ultra-High-Frequency Gravitational Waves
• Effects of cluster galaxies on arc statistics
• Gas and dark matter in the Sculptor group: NGC 300
• Declining rotation curves of galaxies as a test of gravitational theory
• Gravitational Lensing Signatures of Axion Dark Matter Minihalos in Highly Magnified Stars
• Subaru Weak-Lensing Survey of Dark Matter Subhalos in the Coma Cluster : Subhalo Mass Function and Statistical Properties
• Probing the Intrinsic Shape and Alignment of Dark Matter Haloes using SDSS Galaxy Groups
• Halo Substructure and Disk Heating in a Lambda CDM Universe
• Constraints on dark matter annihilation from AMS-02 results
• Heavy Dark Matter Annihilation from Effective Field Theory
• Boosted Dark Matter in IceCube and at the Galactic Center
• Loop-induced dark matter direct detection signals from gamma-ray lines
• Deep high-resolution X-ray spectra from cool-core clusters
• Feedback from Galaxy Formation: Escaping Ionizing Radiation from Galaxies at High Redshift
• How do galaxies acquire their mass?
• GAMER-2: a GPU-accelerated adaptive mesh refinement code -- accuracy, performance, and scalability
• Halo Mass Profiles and Low Surface Brightness Galaxies Rotation Curves
• CLASH: Complete Lensing Analysis of the Largest Cosmic Lens MACS J0717.5+3745 and Surrounding Structures
• The Cluster Velocity Dispersion of the Abell 2199 cD Halo of NGC 6166
• Action-based distribution functions for spheroidal galaxy components
• The HST/ACS Coma Cluster Survey: I - Survey Objectives and Design
• Future Evolution of Structure in an Accelerating Universe
• Indirect Detection of Kaluza-Klein Dark Matter
• Bispectrum and Nonlinear Biasing of Galaxies: Perturbation Analysis, Numerical Simulation and SDSS Galaxy Clustering
• \textsc{CompaSO}: A new halo finder for competitive assignment to spherical overdensities
• Effect of a dark matter halo on the determination of black hole masses
• Boosted Dark Matter Interpretation of the XENON1T Excess
• Probing the stability of superheavy dark matter particles with high-energy neutrinos
• The satellites of the Milky Way - Insights from semi-analytic modelling in a LambdaCDM cosmology
• Hidden Sector Hydrogen as Dark Matter: Small-scale Structure Formation Predictions and the Importance of Hyperfine Interactions
• Galaxy Cluster Mass Reconstruction Project: I. Methods and first results on galaxy-based techniques
• A survey for large image-separation lensed quasars
• Comparing Masses in Literature (CoMaLit)-I. Bias and scatter in weak lensing and X-ray mass estimates of clusters
• The formation of ultra-compact dwarf galaxies and nucleated dwarf galaxies
• Emulation of baryonic effects on the matter power spectrum and constraints from galaxy cluster data
• Some aspects of generalized modified gravity models
• Effective Dark Matter Model: Relic density, CDMS II, Fermi LAT and LHC
• The impact of mergers on relaxed X-ray clusters - III. Effects on compact cool cores
• Λ CDM is Consistent with SPARC Radial Acceleration Relation
• Spatial Clustering of Dark Matter Halos: Secondary Bias, Neighbor Bias, and the Influence of Massive Neighbors on Halo Properties
• The Caustic Ring Model of the Milky Way Halo
• A Comparison of Semi-Analytic and Smoothed Particle Hydrodynamics Galaxy Formation
• Galaxy and Mass Assembly (GAMA): The halo mass of galaxy groups from maximum-likelihood weak lensing
• Constraining heavy dark matter with cosmic-ray antiprotons
• A Population of Massive Globular Clusters in NGC 5128
• Indirect signals from light neutralinos in supersymmetric models without gaugino mass unification
• The Life Cycle of the Central Molecular Zone. I: Inflow, Star Formation, and Winds
• Explaining the DAMA Signal with WIMPless Dark Matter
• Primordial Black Holes
• SDSS-IV MaNGA: What Shapes The Distribution Of Metals In Galaxies? Exploring The Roles Of The Local Gas Fraction And Escape Velocity
• High-Redshift Galaxy Kinematics: Constraints on Models of Disk Formation
• The Destruction of Thin Stellar Disks Via Cosmologically Common Satellite Accretion Events
• Mini-dark halos with intermediate mass black holes
• De-contamination of cosmological 21-cm maps
• Heating of Milky Way disc Stars by Dark Matter Fluctuations in Cold Dark Matter and Fuzzy Dark Matter Paradigms
• Do Baryons Alter the Halos of Low Surface Brightness Galaxies?
• Antiprotons from primordial black holes
• Missing dark matter in dwarf galaxies?
• Orbital parameters of infalling satellite haloes in the hierarchical $\Lambda$CDM model
• cD galaxy contribution to the strong lensing cross sections of galaxy clusters
• First Simulations of Axion Minicluster Halos
• Satellite abundances around bright isolated galaxies II: radial distribution and environmental effects
• The extent of chemically enriched gas around star-forming dwarf galaxies
• AGN-Driven Outflows in Dwarf Galaxies
• An adaptively refined phase-space element method for cosmological simulations and collisionless dynamics
• Determining orbits for the Milky Way's dwarfs
• On the role of electroweak bremsstrahlung for indirect dark matter signatures
• Invisible Neutrino Decay Resolves IceCube's Track and Cascade Tension
• Constraints on Decaying Dark Matter from the Isotropic Gamma-Ray Background
• Indirect dark matter searches in Gamma- and Cosmic Rays
• Sphenix: Smoothed Particle Hydrodynamics for the next generation of galaxy formation simulations
• Group, field and isolated early-type galaxies II. Global trends from nuclear data
• Strong lensing signatures of self-interacting dark matter in low-mass halos
• Properties of host haloes of Lyman-break galaxies and Lyman-alpha Emitters from their number densities and angular clustering
• Search for Dark Matter Annihilation Signals from the Fornax Galaxy Cluster with H.E.S.S
• Searching for dark matter halos in the Suprime-Cam 2 sq deg field
• On the nature of the barlens component in barred galaxies: what do boxy/peanut bulges look like when viewed face-on?
• The Dark Matter Profiles in the Milky Way
• The LSST DESC DC2 Simulated Sky Survey
• The angular momentum-mass relation: a fundamental law from dwarf irregulars to massive spirals
• Modeling the dynamical evolution of the M87 globular cluster system
• The Spitzer-HETDEX Exploratory Large-Area Survey
• Updating the MACHO fraction of the Milky Way dark halo with improved mass models
• The outer profile of dark matter halos: an analytical approach
• Constraining $f(R)$ Gravity Theory Using Weak Lensing Peak Statistics from the Canada-France-Hawaii-Telescope Lensing Survey
• Physical viscosity in smoothed particle hydrodynamics simulations of galaxy clusters
• Dissecting and Modelling Galaxy Assembly Bias
• Testing Gravity Using Galaxy Clusters: New Constraints on Beyond Horndeski Theories
• Dark Photon Stars: Formation and Role as Dark Matter Substructure
• Mass Modeling of Disk Galaxies: Constraints, Degeneracies and Adiabatic Contraction
• Dark Matter Annihilation Rates with Velocity-Dependent Annihilation Cross Sections
• Simulating Subhalos at High Redshift: Merger Rates, Counts, and Types
• Satellite Galaxies and Fossil Groups in the Millennium Simulation
• Heavy decaying dark matter and IceCube high energy neutrinos
• Dark matter axion detection in the radio/mm-waveband
• Frontier Fields: Subaru Weak-Lensing Analysis of the Merging Galaxy Cluster A2744
• Galactic center $\gamma$-ray excess in hidden sector DM models with dark gauge symmetries: local $Z_3$ symmetry as an example
• Gamma-ray detection from gravitino dark matter decay in the $\mu \nu$SSM
• Determining the Nature of Dark Matter with Astrometry
• Direct Constraints on Minimal Supersymmetry from Fermi-LAT Observations of the Dwarf Galaxy Segue 1
• Model-independent dark matter annihilation bound from the diffuse gamma ray flux
• Celestial-Body Focused Dark Matter Annihilation Throughout the Galaxy
• What next for the CMSSM and the NUHM: Improved prospects for superpartner and dark matter detection
• Are mergers responsible for universal halo properties?
• Dark Matter Densities during the Formation of the First Stars and in Dark Stars
• Gravitational-wave imprints of compact and galactic-scale environments in extreme-mass-ratio binaries
• On the identification of substructure in phase-space using orbital frequencies
• Dominant dark matter and a counter rotating disc: MUSE view of the low luminosity S0 galaxy NGC 5102
• What Does The PAMELA Antiproton Spectrum Tell Us About Dark Matter?
• The Evolution of the Dark Halo Spin Parameters lambda and lambda' in a LCDM Universe: The Role of Minor and Major Mergers
• Testing MeV dark matter with neutrino detectors
• The elliptical power law profile lens
• Conservative Constraints on Dark Matter Annihilation into Gamma Rays
• Dark Matter Cores and Cusps in Spiral Galaxies and their Explanations
• Two photon annihilation of Kaluza-Klein dark matter
• Dark Matter Density Spikes around Primordial Black Holes
• Abundance matching with the mean star formation rate: there is no missing satellites problem in the Milky Way above ${\mathbf{M}}_{200}\sim 10^9{\mathbf{M}}_{\odot }$
• Dark matter distribution function from non-extensive statistical mechanics
• On DDO154 and Cold Dark Matter halo profiles
• The Effect of Environment on Shear in Strong Gravitational Lenses
• Analytical model for non-thermal pressure in galaxy clusters - III. Removing the hydrostatic mass bias
• Earth-mass haloes and the emergence of NFW density profiles
• Fuzzy Dark Matter and Dark Matter Halo Cores
• A measurement of large-scale peculiar velocities of clusters of galaxies: technical details
• Which AGN Jets Quench Star Formation in Massive Galaxies?
• Dark Matter Halos with Cores from Hierarchical Structure Formation
• Density profiles of ultracompact minihalos: Implications for constraining the primordial power spectrum
• Discrete dynamical modelling of omega Centauri
• GASP XXIII: A jellyfish galaxy as an astrophysical laboratory of the baryonic cycle
• Gravitational potential and X-ray luminosities of early-type galaxies observed with XMM-Newton and Chandra
• The role of luminous substructure in the gravitational lens system MG 2016+112
• Status, Challenges and Directions in Indirect Dark Matter Searches
• Radial Alignment in Simulated Clusters
• The impact of the observed baryon distribution in haloes on the total matter power spectrum
• Expanded haloes, abundance matching and too-big-to-fail in the Local Group
• Recognising Axionic Dark Matter by Compton and de-Broglie Scale Modulation of Pulsar Timing
• Integral X-ray constraints on sub-GeV Dark Matter
• The concentration-mass relation of clusters of galaxies from the OmegaWINGS survey
• Where do the 3.5 keV photons come from? A morphological study of the Galactic Center and of Perseus
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: anisotropic clustering analysis in configuration-space
• JADES: The incidence rate and properties of galactic outflows in low-mass galaxies across 3 < z < 9
• A 5x10^9 Solar Mass Black Hole in NGC 1277 from Adaptive Optics Spectroscopy
• How effective is harassment on infalling late-type dwarfs?
• Clues to the "Magellanic Galaxy" from Cosmological Simulations
• Galaxy cluster mass profiles
• Fitting dwarf galaxy rotation curves with conformal gravity
• Constraining dark matter halo profiles and galaxy formation models using spiral arm morphology. I. Method outline
• The Role of Dust in the Early Universe I : Protogalaxy Evolution
• Kinematics of Outer Halo Globular Clusters in M31
• Merger vs. Accretion and the Structure of Dark Matter Halos
• Dark matter scaling relations and the assembly epoch of Coma early-type galaxies
• Bounds on Dark Matter Interactions with Electroweak Gauge Bosons
• Origin of E+A galaxies: I. Physical properties of E+A's formed from galaxy merging and interaction
• Feeding black holes at galactic centres by capture from isothermal cusps
• AGN Heating in Simulated Cool-Core Clusters
• Exploring Halo Substructure with Giant Stars VIII: The Extended Structure of the Sculptor Dwarf Spheroidal Galaxy
• Structure and Population of the Andromeda Stellar Halo from a Subaru/Suprime-Cam Survey
• A multi-messenger study of the Milky Way's stellar disc and bulge with LISA, Gaia and LSST
• Source Selection for Cluster Weak Lensing Measurements in the Hyper Suprime-Cam Survey
• How Rare is the Bullet Cluster?
• RASS-SDSS Galaxy Cluster Survey. V. The X-ray-Underluminous Abell Clusters
• Velocity Dispersions of CNOC Clusters and the Evolution of the Cluster Abundance
• Small-scale clumps of dark matter
• The structural and dynamical properties of compact elliptical galaxies
• Search for Dark Matter Annihilation in the Galactic Center with IceCube-79
• The Tully-Fisher and mass-size relations from halo abundance matching
• Precessing jets and X-ray bubbles from NGC1275 (3C84) in the Perseus galaxy cluster: a view from 3D numerical simulations
• Rotation and Mass in the Milky Way and Spiral Galaxies
• 24.77 Pflops on a Gravitational Tree-Code to Simulate the Milky Way Galaxy with 18600 GPUs
• Self-interacting Warm Dark Matter
• Chaotic Dispersal of Tidal Debris
• Indirect Detection of Neutrino Portal Dark Matter
• Noisy weak-lensing convergence peak statistics near clusters of galaxies and beyond
• AGN feedback in dwarf galaxies?
• Antiproton constraints on the GeV gamma-ray excess: a comprehensive analysis
• Redistributing hot gas around galaxies: do cool clouds signal a solution to the overcooling problem?
• Massive black hole evolution models confronting the n-Hz amplitude of the stochastic gravitational wave background
• Mass distribution in the core of MACS J1206: robust modeling from an exceptionally large sample of central multiple images
• Are ring galaxies the ancestors of giant low surface brightness galaxies?
• Are ultracompact minihalos really ultracompact?
• Neutralino Annihilation at the Galactic Center Revisited
• Phase Space Models of the Dwarf Spheroidal Galaxies
• A Chandra Study of the Complex Structure in the Core of 2A 0335+096
• The observability of gamma-rays from neutralino annihilations in Milky Way substructure
• On Dark Peaks and Missing Mass: A Weak Lensing Mass Reconstruction of the Merging Cluster System Abell 520
• The role of dry mergers for the formation and evolution of brightest cluster galaxies
• Foreground Mismodeling and the Point Source Explanation of the Fermi Galactic Center Excess
• Cosmic-Ray Neutrinos from the Decay of Long-Lived Particle and the Recent IceCube Result
• Dust-regulated galaxy formation and evolution:A new chemodynamical model with live dust particles
• On the Effects of Line-of-Sight Structures on Lensing Flux-ratio Anomalies in a LCDM Universe
• Modeling Intra-Cluster Gas in Triaxial Dark Halos : An Analytical Approach
• Weak lensing Analysis of X-Ray-selected XXL Galaxy Groups and Clusters with Subaru HSC Data
• The ZZ' kinetic mixing in the light of the recent direct and indirect dark matter searches
• Prospects for dark matter searches in the pMSSM
• New insights on the formation of nuclear star clusters
• Modelling galaxy halos using dark matter with pressure
• Luminosity-Dependent Quasar Lifetimes: Reconciling the Optical and X-ray Quasar Luminosity Functions
• Detection of Leptonic Dark Matter
• Gravitational microlensing by dark matter in extended structures
• Gravitational waves from Extreme Mass Ratio Inspirals in non-pure Kerr spacetimes
• Dark matter annihilation effects on the first stars
• Indirect Detection Analysis: Wino Dark Matter Case Study
• Semi-Analytical Models for the Formation of Disk Galaxies II. Dark Matter versus Modified Newtonian Dynamics
• Signatures of Dark Matter Scattering Inelastically Off Nuclei
• Testing the theory of gravity with DESI: estimators, predictions and simulation requirements
• CoMaLit III. Literature Catalogs of weak Lensing Clusters of galaxies (LC^2)
• H-alpha Kinematics of the SINGS Nearby Galaxies Survey. II
• Mining for Dark Matter Substructure: Inferring subhalo population properties from strong lenses with machine learning
• Shocks and angular momentum flips: a different path to feeding the nuclear regions of merging galaxies
• Seeding Supermassive Black Holes with Self-Interacting Dark Matter: A Unified Scenario with Baryons
• Signatures of minor mergers in the Milky Way disc I: The SEGUE stellar sample
• Dwarf Galaxies in CDM, WDM, and SIDM: Disentangling Baryons and Dark Matter Physics
• Orbital Decay of Supermassive Black Hole Binaries in Clumpy Multiphase Merger Remnants
• Scaling Relations for Dark Matter Annihilation and Decay Profiles in Dwarf Spheroidal Galaxies
• VIMOS Ultra-Deep Survey (VUDS): Witnessing the Assembly of a Massive Cluster at z~3.3
• Cosmic Rays from Leptophilic Dark Matter Decay via Kinetic Mixing
• The mass and angular momentum distribution of simulated massive early-type galaxies to large radii
• An Iterative Method for Constructing Equilibrium Phase Models of Stellar Systems
• Dynamical signatures of a LCDM-halo and the distribution of the baryons in M33
• The demographics of neutron star - white dwarf mergers: rates, delay-time distributions and progenitors
• Brief History of Ultra-light Scalar Dark Matter Models
• Improving time-delay cosmography with spatially resolved kinematics
• Search for extended gamma-ray emission from the Virgo galaxy cluster with Fermi-LAT
• The properties of "dark" ΛCDM halos in the Local Group
• The Evolution of Assembly Bias
• Recovering cores and cusps in dark matter haloes using mock velocity field observations
• Simulations of Axion Minihalos
• Circumscribing Late Dark Matter Decays Model Independently
• Non-linear Integrated Sachs-Wolfe Effect
• The Density and Pseudo-Phase-Space Density Profiles of CDM halos
• Scaling Laws for Dark Matter Halos in Late-Type and Dwarf Spheroidal Galaxies
• Morphology of Galaxy Clusters: A Cosmological Model-Independent Test of the Cosmic Distance-Duality Relation
• The Graininess of Dark Matter Haloes
• Disruption of satellite galaxies in simulated groups and clusters: the roles of accretion time, baryons, and pre-processing
• Weak Gravitational Lensing Bispectrum
• A model for core formation in dark matter haloes and ultra diffuse galaxies by outflow episodes
• Unveiling the nature of dark matter with high redshift 21 cm line experiments
• HI study of the warped spiral galaxy NGC5055: a disk/dark matter halo offset?
• Deviations from hydrostatic equilibrium in the circumgalactic medium: spinning hot haloes and accelerating flows
• GW$\times$LSS: Chasing the Progenitors of Merging Binary Black Holes
• Collisionally Regenerated Dark Matter Structures in Galactic Nuclei
• Mirror Dark Matter and Core Density of Galaxies
• Constraints on the low-mass end of the mass-metallicity relation at z=1-2 from lensed galaxies
• Dark matter and pulsar signals for Fermi LAT, PAMELA, ATIC, HESS and WMAP data
• Conserved actions, maximum entropy and dark matter halos
• Reionization in Technicolor
• Self-consistent construction of virialized wave dark matter halos
• Properties of the galaxy population in hydrodynamical simulations of clusters
• Signatures of minor mergers in Milky Way-like disc kinematics: Ringing revisited
• Possible Evidence for MeV Dark Matter In Dwarf Spheroidals
• Galactic Archaeology with Gaia
• Cosmic web anisotropy is the primary indicator of halo assembly bias
• A Comparison of Gas Dynamics in SPH and Semi-analytic Models of Galaxy Formation
• Two new tests to the distance duality relation with galaxy clusters
• Galactic 511 keV line from MeV millicharged dark matter
• The Cluster Lensing and Supernova Survey with Hubble (CLASH): Strong Lensing Analysis of Abell 383 from 16-Band HST WFC3/ACS Imaging
• AMS-02 positron excess: new bounds on dark matter models and hint for primary electron spectrum hardening
• Constraining heavy decaying dark matter with the high energy gamma-ray limits
• Spurious heating of stellar motions in simulated galactic disks by dark matter halo particles
• Young Galaxy Candidates in the Hubble Frontier Fields. I. Abell 2744
• Can Light Dark Matter Solve the Core-Cusp Problem?
• Cosmological evolution of a complex scalar field with repulsive or attractive self-interaction
• The impact of stellar feedback on the density and velocity structure of the interstellar medium
• Hydrodynamic representation of the Klein-Gordon-Einstein equations in the weak field limit: I. General formalism and perturbations analysis
• Dark Matter Sees The Light
• The Host Galaxy of the Lensed Quasar Q 0957+561
• The impact of Early Dark Energy on non-linear structure formation
• The Onset of Gravothermal Core Collapse in Velocity Dependent Self-Interacting Dark Matter Subhaloes
• Kinematics of globular cluster systems and the formation of early-type galaxies
• The Sphericalization of Dark Matter Halos by Galaxy Disks
• The clustering of luminous red galaxies at z $\sim$ 0.7 from eBOSS and BOSS data
• The Disk and Dark Halo Mass of the Barred Galaxy NGC 4123. I. Observations
• Analytical model for non-thermal pressure in galaxy clusters
• The Keck Baryonic Structure Survey: Using foreground/background galaxy pairs to trace the structure and kinematics of circumgalactic neutral hydrogen at $z\sim 2$
• Cross-correlating Planck CMB lensing with SDSS: Lensing-lensing and galaxy-lensing cross-correlations
• Galactic cannibalism and CDM density profiles
• The Effect of Cooling on the Density Profile of Hot Gas in Clusters of Galaxies: Is Additional Physics Needed?
• Young galaxies: what turns them on?
• Flavourful $Z^{\prime }$ portal for vector-like neutrino Dark Matter and $R_{K^{(\ast )}}$
• Mass and galaxy distributions of four massive galaxy clusters from Dark Energy Survey Science Verification data
• Chemical evolution in a model for the joint formation of quasars and spheroids
• Probing astrophysical environment with eccentric extreme mass-ratio inspirals
• Gamma Rays from Clusters and Groups of Galaxies: Cosmic Rays versus Dark Matter
• The Return of the Templates: Revisiting the Galactic Center Excess with Multi-Messenger Observations
• Birds of a Feather? Magellan/IMACS Spectroscopy of the Ultra-Faint Satellites Grus II, Tucana IV, and Tucana V
• Major Mergers of Galaxy Haloes: Cuspy or Cored Inner Density Profile?
• On the morphologies, gas fractions, and star formation rates of small galaxies
• 2D kinematic signatures of boxy/peanut bulges
• The Complex Structure of the Cl 1604 Supercluster at z~0.9
• Eddington-Born-Infeld action for dark energy and dark matter
• Kinematics and simulations of the stellar stream in the halo of the Umbrella Galaxy
• A Possible Explanation of Low Energy $\gamma$-ray Excess from Galactic Centre and Fermi Bubble by a Dark Matter Model with Two Real Scalars
• Review of Observational Evidence for Dark Matter in the Universe and in upcoming searches for Dark Stars
• Serendipitous discovery of the unidentified extended TeV gamma-ray source HESS J1303-631
• Extreme mass-ratio inspirals in ultra-light dark matter
• The Need for Speed: Escape velocity and dynamical mass measurements of the Andromeda galaxy
• SKAO HI Intensity Mapping: Blind Foreground Subtraction Challenge
• Catalogues of Active Galactic Nuclei From Gaia and unWISE Data
• A new model to predict weak-lensing peak counts II. Parameter constraint strategies
• The angular momentum of cold dark matter haloes with and without baryons
• Improved Constraints on the Gravitational Lens Q0957+561. II. Strong Lensing
• From galactic nuclei to the halo outskirts: tracing supermassive black holes across cosmic history and environments
• Tomographic galaxy clustering with the Subaru Hyper Suprime-Cam first year public data release
• Stellar Kinematics in the Complicated Inner Spheroid of M31: Discovery of Substructure Along the Southeastern Minor Axis and its Relationship to the Giant Southern Stream
• Metal enrichment processes
• Dynamical evolution of globular cluster systems in clusters of galaxies I. The case of NGC 1404 in the Fornax cluster
• Search for 100 MeV to 10 GeV gamma-ray lines in the Fermi-LAT data and implications for gravitino dark matter in the $\mu \nu$SSM
• Concentrations of Dark Haloes Emerge from Their Merger Histories
• Breaking degeneracies in modified gravity with higher (than 2nd) order weak-lensing statistics
• Resolution of dark matter problem in f(T) gravity
• Effective Models for Statistical Studies of Galaxy-Scale Gravitational Lensing
• A Revised LCDM Mass Model For The Andromeda Galaxy
• A new model to predict weak-lensing peak counts I. Comparison with $N$-body Simulations
• The clustering of radio galaxies at z~0.55 from the 2SLAQ LRG survey
• Models of dark matter halos based on statistical mechanics: II. The fermionic King model
• Dark Matter Annihilation and Primordial Star Formation
• The Higgs Portal to Cosmology
• Signatures of Hierarchical Clustering in Dark Matter Detection Experiments
• Nonextensive theory of dark matter and gas density profiles
• A measurement of the Hubble constant from angular diameter distances to two gravitational lenses
• Mass Transport and Turbulence in Gravitationally Unstable Disk Galaxies. I: The Case of Pure Self-Gravity
• On the origin of the stellar halo and multiple stellar populations in the globular cluster NGC 1851
• Constraining the NFW Potential with Observations and Modeling of LSB Galaxy Velocity Fields
• Where the world stands still: turnaround as a strong test of ΛCDM cosmology
• Galaxy clustering from COMBO-17: The halo occupation distribution at <z>=0.6
• Structure Formation Inside Triaxial Dark Matter Halos: Galactic Disks, Bulges and Bars
• Accurate determination of the mass distribution in spiral galaxies III. Fabry-Perot imaging spectroscopy of 6 spiral galaxies
• Mass-to-Light Ratios of Galaxy Groups from Weak Lensing
• The failure of stellar feedback, magnetic fields, conduction, and morphological quenching in maintaining red galaxies
• Dynamics of stream-subhalo interactions
• Semi-implicit anisotropic cosmic ray transport on an unstructured moving mesh
• The Case for Axion Dark Matter
• Spectral Line De-confusion in an Intensity Mapping Survey
• The Near-IR Background Intensity and Anisotropies During The Epoch of Reionization
• The High-Energy Tail of the Galactic Center Gamma-Ray Excess
• Prospects for probing gravitational waves from primordial black hole binaries
• Strong Gravitational Lensing Time Delay Statistics and the Density Profile of Dark Halos
• Disk-Bulge-Halo Models for the Andromeda Galaxy
• Hydrodynamical simulations of Galactic fountains II: evolution of multiple fountains
• Disc Heating: Comparing the Milky Way with Cosmological Simulations
• Dynamical Modeling of Galaxy Mergers using Identikit
• Decaying vs Annihilating Dark Matter in Light of a Tentative Gamma-Ray Line
• The Effect of Gravitational Recoil on Black Holes Forming in a Hierarchical Universe
• Velocity Dependence from Resonant Self-Interacting Dark Matter
• Hydrostatic Chandra X-ray analysis of SPT-selected galaxy clusters - I. Evolution of profiles and core properties
• Dry mergers and the formation of early-type galaxies: constraints from lensing and dynamics
• Cosmic Positron Signature from Dark Matter in the Littlest Higgs Model with T-parity
• Multi-wavelength features of Fermi Bubbles as signatures of a Galactic wind
• Dark Stars: A Review
• Off-Center Collisions between Clusters of Galaxies
• Combined search for neutrinos from dark matter self-annihilation in the Galactic Centre with ANTARES and IceCube
• A sub-resolution multiphase interstellar medium model of star formation and SNe energy feedback
• Dark matter halo properties from galaxy-galaxy lensing
• Neutrino Signals from Annihilating/Decaying Dark Matter in the Light of Recent Measurements of Cosmic Ray Electron/Positron Fluxes
• Top-philic dark matter within and beyond the WIMP paradigm
• Probing dark matter annihilation in the Galaxy with antiprotons and gamma rays
• From Weak Lensing to non-Gaussianity via Minkowski Functionals
• Kinematics of hypervelocity stars in the triaxial halo of the Milky Way
• Antiproton constraints on dark matter annihilations from internal electroweak bremsstrahlung
• The First Generation of Star-Forming Haloes
• Where are the Luminous Red Galaxies (LRGs)? Using correlation measurements and lensing to relate LRGs to dark matter halos
• Simulating the dynamics and non-thermal emission of relativistic magnetised jets I. Dynamics
• The ARAUCARIA Project: VLT-FORS spectroscopy of blue supergiants in NGC 3109 - Classifications, first abundances and kinematics
• The Impact of Box Size on the Properties of Dark Matter Haloes in Cosmological Simulations
• Formation and Evolution of Galactic Halos in Clusters of Galaxies
• The pre-processing of subhaloes in SDSS groups and clusters
• Investigating Gamma-Ray Lines from Dark Matter with Future Observatories
• An FRB Sent Me a DM: Constraining the Electron Column of the Milky Way Halo with Fast Radio Burst Dispersion Measures from CHIME/FRB
• Multi-wavelength astronomical searches for primordial black holes
• Anisotropy probe of galactic and extra-galactic Dark Matter annihilations
• Five-percent measurements of the growth rate from simulation-based modelling of redshift-space clustering in BOSS LOWZ
• The inert doublet model in the light of Fermi-LAT gamma-ray data: a global fit analysis
• Heated Cooling Flows
• Two-Phased Intra-Cluster Medium in the Centaurus Cluster of Galaxies
• On ths assembly history of stellar components in massive galaxies
• A supra-massive population of stellar-mass black holes in the globular cluster Palomar 5
• Halo model description of the non-linear dark matter power spectrum at $k\gg 1$ Mpc${}^{-1}$
• The total mass and dark halo properties of the Small Magellanic Cloud
• Three-dimensional Multi-probe Analysis of the Galaxy Cluster A1689
• The WIMP Forest: Indirect Detection of a Chiral Square
• Supersymmetric Dark Matter and the Extragalactic Gamma Ray Background
• Arc Statistics
• Globular Clusters in Dense Clusters of Galaxies
• Heated Disc Stars in the Stellar Halo
• Density profiles of dark matter haloes on Galactic and Cluster scales
• The origin and tidal evolution of cuspy triaxial haloes
• Searching for galaxy clusters using the aperture mass statistics in 50 VLT fields
• Neutralino Warm Dark Matter
• The impact of galaxy harassment on the globular cluster systems of early-type cluster dwarf galaxies
• Stopping Cooling Flows with Jets
• The effect of an expanding universe on massive objects
• Modelling non-linear redshift-space distortions in the galaxy clustering pattern: systematic errors on the growth rate parameter
• The impact of baryon physics on the structure of high-redshift galaxies
• Mass, velocity anisotropy, and pseudo phase-space density profiles of Abell 2142
• Ultra-high energy cosmic rays from annihilation of superheavy dark matter
• Ionized and molecular gas kinematics in a z=1.4 star-forming galaxy
• Can Dark Matter Annihilation Dominate the Extragalactic Gamma-Ray Background?
• Combining Stellar Populations with Orbit-Superposition Dynamical Modelling - the Formation History of the Lenticular Galaxy NGC 3115
• Astrophysical neutrinos flavored with Beyond the Standard Model physics
• HICOSMO - Cosmology with a complete sample of galaxy clusters: I. Data analysis, sample selection and luminosity-mass scaling-relation
• Correlating galaxy colour and halo concentration: A tunable Halo Model of galactic conformity
• Exploring for sub-MeV Boosted Dark Matter from Xenon Electron Direct Detection
• Dark Matter Capture in the First Stars: a Power Source and Limit on Stellar Mass
• Spurious Point Source Signals in the Galactic Center Excess
• The Rotation Curve, Mass Distribution and Dark Matter Content of the Milky Way from Classical Cepheids
• Fast radio bursts from activities of neutron stars newborn in BNS mergers: offset, birth rate and observational properties
• Positron/Gamma-Ray Signatures of Dark Matter Annihilation and Big-Bang Nucleosynthesis
• Indirect detection of light neutralino dark matter in the NMSSM
• A predictive model of BEC dark matter halos with a solitonic core and an isothermal atmosphere
• LambdaCDM Halo Density Profiles: where do actual halos converge to NFW ones?
• On the occurrence of galaxy harassment
• 3D motions in the Sculptor dwarf galaxy as a glimpse of a new era
• How Dark Matter Reionized The Universe
• Weak lensing measurement of galaxy clusters in the CFHTLS-Wide survey
• Cosmological Effects of Powerful AGN Outbursts in Galaxy Clusters: Insights from an XMM-Newton Observation of MS0735+7421
• Either neutralino dark matter or cuspy dark halos
• The Gaia-ESO Survey: a quiescent Milky Way with no significant dark/stellar accreted disc
• The Stellar Populations of NGC 3109: Another Dwarf Irregular Galaxy with a Population II Stellar Halo
• Halo Substructure Boosts to the Signatures of Dark Matter Annihilation
• Probing non-spherical dark halos in the Galactic dwarf galaxies
• Dark-Matter Decays and Self-Gravitating Halos
• Modeling Tidal Streams in evolving dark matter halos
• X-ray emission from high-redshift miniquasars: self-regulating the population of massive black holes through global warming
• Galaxy Formation and the Kinematics of Damped Lyman Alpha Systems
• Hydrodynamical simulations of Galactic fountains I: evolution of single fountains
• Variations in the width, density, and direction of the Palomar 5 tidal tails
• CMB photons shedding light on dark matter
• The early early type: discovery of a passive galaxy at z=3
• The Swift/BAT AGN Spectroscopic Survey -- IX. The Clustering Environments of an Unbiased Sample of Local AGN
• Probing Dark Matter Substructure with Pulsar Timing
• Clustering of sub-millimeter galaxies in a self-regulated baryon collapse model
• The Impact of Radio AGN Bubble Composition on the Dynamics and Thermal Balance of the Intracluster Medium
• GA-NIFS: The core of an extremely massive proto-cluster at the Epoch of Reionization probed with JWST/NIRSpec
• Constraints on dark matter self-interaction from the internal density profiles of X-COP galaxy clusters
• Multi-Dimensional Density Estimation and Phase Space Structure Of Dark Matter Halos
• Are galaxies extending?
• The Initial Mass Function in the Nearest Strong Lenses from SNELLS: Assessing the Consistency of Lensing, Dynamical, and Spectroscopic Constraints
• Nuclear coups: dynamics of black holes in galaxy mergers
• The effect of the deforming dark matter haloes of the Milky Way and the Large Magellanic Cloud on the Orphan-Chenab stream
• The Orbital Ellipticity of Satellite Galaxies and the Mass of the Milky Way
• Knowing the unknowns: uncertainties in simple estimators of galactic dynamical masses
• On the Self-Similar Appearance of Galaxy Clusters in X-rays
• A measurement of the secondary-CMB and millimeter-wave-foreground bispectrum using 800 square degrees of South Pole Telescope data
• The 21 cm signal and the interplay between dark matter annihilations and astrophysical processes
• The nature of voids: I. Watershed void finders and their connection with theoretical models
• How well does the Friends-of-Friends algorithm recover group properties from galaxy catalogs limited in both distance and luminosity?
• Magnetised winds in dwarf galaxies
• The impact of going beyond the Maxwell distribution in direct dark matter detection rates
• Challenges in Detecting Gamma-Rays From Dark Matter Annihilations in the Galactic Center
• N-body Simulations for Extended Quintessence Models
• Constraints on WIMP Annihilation for Contracted Dark Matter in the Inner Galaxy with the Fermi-LAT
• Inconsistency in theories of violent-relaxation
• Tomographic measurement of the intergalactic gas pressure through galaxy-tSZ cross-correlations
• Production and attenuation of cosmic-ray boosted dark matter
• Measuring the dark flow with public X-ray cluster data
• Characterising stellar halo populations I: An extended distribution function for halo K giants
• Effective Fluid Description of the Dark Universe
• Planetary Nebulae in Face-On Spiral Galaxies. III. Planetary Nebula Kinematics and Disk Mass
• A new stochastic approach to cumulative weak lensing
• TeV Scale Singlet Dark Matter
• Self-interacting dark matter from an SU(3)_L \otimes U(1)_N electroweak model
• Boosted dark matter from diffuse supernova neutrinos
• HI Kinematics Along The Minor Axis of M82
• Ships Passing in the Night: Spectroscopic Analysis of Two Ultra-Faint Satellites in the Constellation Carina
• Modelling the correlation between the thermal Sunyaev Zel'dovich effect and the cosmic infrared background
• Unstable Gravitino Dark Matter and Neutrino Flux
• The effects of metallicity, UV radiation and non-equilibrium chemistry in high-resolution simulations of galaxies
• Inferring the mass of sub-millimetre galaxies by exploiting their gravitational magnification of background galaxies
• Semi-analytic Simulations of Galactic Winds: Volume Filling Factor, Ejection of Metals and Parameter Study
• Search for Boosted Dark Matter Interacting With Electrons in Super-Kamiokande
• The Core Structure of Galaxy Clusters from Gravitational Lensing
• Tidal disruption of globular clusters in dwarf galaxies with triaxial dark matter haloes
• A Search for Light Fermionic Dark Matter Absorption on Electrons in PandaX-4T
• Constraints on the shapes of galaxy dark matter haloes from weak gravitational lensing
• Detecting Dark Matter Substructures around the Milky Way with Gaia
• Gamma Rays From The Galactic Center and the WMAP Haze
• Bar-formation as driver of gas inflows in isolated disc galaxies
• Halo modelling in chameleon theories
• Results of a Search for Cold Flows of Dark Matter Axions
• The Next Generation Virgo cluster Survey. V. modelling the dynamics of M87 with the Made-to-Measure method
• Dark halo response and the stellar initial mass function in early-type and late-type galaxies
• Non-Gaussian Aspects of Thermal and Kinetic Sunyaev-Zel'dovich Effects
• Extraterrestrial Axion Search with the Breakthrough Listen Galactic Center Survey
• Galactic fountains and their connection with high and intermediate velocity clouds
• Wide-field kinematics of globular clusters in the Leo I group
• Polar Ring Galaxies and the Tully Fisher relation: implications for the dark halo shape
• Measuring Dark Matter Profiles Non-Parametrically in Dwarf Spheroidals: An Application to Draco
• Seeing double: strong gravitational lensing of high-redshift supernovae
• LoCuSS: A Comparison of Sunyaev-Zel'dovich Effect and Gravitational Lensing Measurements of Galaxy Clusters
• Large Scale Pressure Fluctuations and Sunyaev-Zel'dovich Effect
• The chemical evolution of a Milky Way-like galaxy: the importance of a cosmologically motivated infall law
• The Virgo stellar over-density: Mapping the infall of the Sagittarius tidal stream onto the Milky Way disk
• Secondary Infall and the Pseudo-Phase-Space Density Profiles of Cold Dark Matter Halos
• Properties of Dark Matter Halos as a Function of Local Environment Density
• Weak Lensing by Large-Scale Structure: A Dark Matter Halo Approach
• Dwarf Dark Matter Halos
• Connecting early and late universe by $f(R)$ gravity
• Kaluza-Klein Dark Matter and Galactic Antiprotons
• Unscrambling the lensed galaxies in JWST images behind SMACS0723
• Secular Damping of Stellar Bars in Spinning Dark Matter Halos
• A Self-interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties
• The ThreeHundred: the structure and properties of cosmic filaments in the outskirts of galaxy clusters
• Strategies for Determining the Nature of Dark Matter
• Multiple Chemodynamic Stellar Populations of the Ursa Minor Dwarf Spheroidal Galaxy
• Modelling Void Abundance in Modified Gravity
• Dark-matter admixed white dwarfs
• Warps and Bars from the External Tidal Torques of Tumbling Dark Halos
• The Nonlinear Cosmological Matter Power Spectrum with Massive Neutrinos I: The Halo Model
• Particle Dark Matter Constraints from the Draco Dwarf Galaxy
• The Projected Dark and Baryonic Ellipsoidal Structure of 20 CLASH Galaxy Clusters
• Measuring cluster masses with CMB lensing: a statistical approach
• The Edge of the Galaxy
• Constraining the Rastall parameters in static spacetimes with galaxy-scale strong gravitational lensing
• All-flavour Search for Neutrinos from Dark Matter Annihilations in the Milky Way with IceCube/DeepCore
• Stellar Bar Evolution in Cuspy and Flat-Cored Triaxial CDM Halos
• On the Density profile slope of Clusters of Galaxies
• Information content in the halo-model dark-matter power spectrum
• On mini-halo encounters with stars
• The impact of baryons on the direct detection of dark matter
• Direct detection of dark matter: a critical review
• Systematic trends in total-mass profiles from dynamical models of early-type galaxies
• The Evolution of Substructure in Galaxy, Group and Cluster Haloes II: Global Properties
• A Warm Molecular Hydrogen Tail Due to Ram Pressure Stripping of a Cluster Galaxy
• The Redshift-Space Cluster-Galaxy Cross-Correlation Function: I. Modeling Galaxy Infall onto Millennium Simulation Clusters and SDSS Groups
• Observational Constraints on the Self Interacting Dark Matter Scenario and the Growth of Supermassive Black Holes
• Boosting the annihilation boost: Tidal effects on dark matter subhalos and consistent luminosity modeling
• Anomaly Induced Dark Matter Decay and PAMELA/ATIC Experiments
• The Dynamics of Merging Clusters: A Monte Carlo Solution Applied to the Bullet and Musket Ball Clusters
• Dynamical friction in cuspy galaxies
• Limits on Supersymmetric Dark Matter From EGRET Observations of the Galactic Center Region
• Optimal capture of non-Gaussianity in weak lensing surveys: power spectrum, bispectrum and halo counts
• 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
• Neutrino Mass and Dark Matter in light of recent AMS-02 results
• The Two-Halo Term in Stacked Thermal Sunyaev-Zel'dovich Measurements: Implications for Self-Similarity
• Miscentring in Galaxy Clusters: Dark Matter to Brightest Cluster Galaxy Offsets in 10,000 SDSS Clusters
• The natural emergence of the correlation between H2 and star formation rate surface densities in galaxy simulations
• Search of Dark Matter Annihilation in the Galactic Centre using the ANTARES Neutrino Telescope
• Nuclear Spirals in the inner Milky Way
• The EDGE-CALIFA survey: validating stellar dynamical mass models with CO kinematics
• Multiphase gas in the circumgalactic medium: relative role of $t_{\mathrm{cool}}/t_{\mathrm{ff}}$ and density fluctuations
• Dark baryons and rotation curves
• Public Release of A-SLOTH: Ancient Stars and Local Observables by Tracing Halos
• Constraints on the mass-concentration relation of cold dark matter halos with 11 strong gravitational lenses
• Faint extended Lyalpha emission due to star formation at the centre of high-column density QSO absorption systems
• HI Imaging Observations of Superthin Galaxies. I. UGC7321
• The WIMP annual modulation signal and non-standard halo models
• Non-radial motion and the NFW profile
• The Dekel-Zhao profile: A mass-dependent dark-matter density profile with flexible inner slope and analytic potential, velocity dispersion, and lensing properties
• Planck Sunyaev-Zel'dovich Cluster Mass Calibration using Hyper Suprime-Cam Weak Lensing
• The rapid onset of stellar bars in the baryon-dominated centers of disk galaxies
• The luminosities of backsplash galaxies in constrained simulations of the Local Group
• Phenomenology of Dark Matter annihilation into a long-lived intermediate state
• Stellar Structure and Tests of Modified Gravity
• Dissecting a galaxy: mass distribution of 2237+0305
• Extracting the Gamma Ray Signal from Dark Matter Annihilation in the Galactic Center Region
• The geometry of the gas surrounding the Central Molecular Zone: on the origin of localised molecular clouds with extreme velocity dispersions
• Search for Gamma-ray Emission from Dark Matter Annihilation in the Large Magellanic Cloud with the Fermi Large Area Telescope
• Cosmology: small scale issues revisited
• Time-delay cosmographic forecasts with strong lensing and JWST stellar kinematics
• Dark Stars: a new look at the First Stars in the Universe
• Dark Matter Deficient Galaxies Produced Via High-velocity Galaxy Collisions In High-resolution Numerical Simulations
• Galaxy And Mass Assembly (GAMA): impact of the group environment on galaxy star formation
• A Consistent Picture Emerges: A Compact X-ray Continuum Emission Region in the Gravitationally Lensed Quasar SDSS J0924+0219
• Bending Waves in the Milky Way's disc from halo substructure
• Testing general scalar-tensor gravity and massive gravity with cluster lensing
• Luminous Satellites of Early-Type Galaxies I: Spatial Distribution
• Probing Particle Physics with IceCube
• Mass Distributions of HST Galaxy Clusters from Gravitational Arcs
• WIMP astronomy and particle physics with liquid-noble and cryogenic direct-detection experiments
• On the assembly of the Milky Way dwarf satellites and their common mass scale
• Cold gas in cluster cores: Global stability analysis and non-linear simulations of thermal instability
• Self-Similar Solutions of Triaxial Dark Matter Halos
• The Baryons in the Milky Way Satellites
• The Core-Cusp Problem in Cold Dark Matter Halos and Supernova Feedback: Effects of Oscillation
• Spin flips I: Evolution of the angular momentum orientation of Milky Way-mass dark matter haloes
• A New Direction in Dark-Matter Complementarity: Dark-Matter Decay as a Complementary Probe of Multi-Component Dark Sectors
• Arc Statistics in Cosmological Models with Dark Energy
• The Atacama Cosmology Telescope: Detection of the Pairwise Kinematic Sunyaev-Zel'dovich Effect with SDSS DR15 Galaxies
• Weak lensing mass map and peak statistics in Canada-France-Hawaii Telescope Stripe 82 survey
• Inferring the gravitational potential of the Milky Way with a few precisely measured stars
• Multiple density discontinuities in the merging galaxy cluster CIZA J2242.8+5301
• Unifying leptogenesis, dark matter and high-energy neutrinos with right-handed neutrino mixing via Higgs portal
• Identikit 1: A Modeling Tool for Interacting Disk Galaxies
• Nonthermal Emission from Accreting and Merging Clusters of Galaxies
• Gravitoelectromagnetism, Solar System Test and Weak-Field Solutions in $f(T,B)$ Gravity with Observational Constraints
• Dynamical models for the Sculptor dwarf spheroidal in a Lambda CDM universe
• On the dynamics of the Small Magellanic Cloud through high-resolution ASKAP HI observations
• What Makes the Family of Barred Disc Galaxies So Rich: Damping Stellar Bars in Spinning Haloes
• Annual Modulation in Direct Dark Matter Searches
• Hints against the cold and collisionless nature of dark matter from the galaxy velocity function
• The SLUGGS Survey: Dark matter fractions at large radii and assembly epochs of early-type galaxies from globular cluster kinematics
• Size matters: abundance matching, galaxy sizes, and the Tully-Fisher relation in EAGLE
• Active galactic nuclei and massive galaxy cores
• GaBoDS: The Garching-Bonn Deep Survey -- I. Anatomy of galaxy clusters in the background of NGC 300
• Calorimetric Dark Matter Detection With Galactic Center Gas Clouds
• Dynamical evidence for a morphology-dependent relation between the stellar and halo masses of galaxies
• Rotation curve fitting and its fatal attraction to cores in realistically simulated galaxy observations
• Gravothermal solutions of SIDM halos: mapping from constant to velocity-dependent cross section
• Globular Clusters as Tracers of Stellar Bimodality in Elliptical Galaxies: The Case of NGC 1399
• 3.55 keV photon lines from axion to photon conversion in the Milky Way and M31
• MOKA: a new tool for Strong Lensing Studies
• Merging Cluster Collaboration: A Panchromatic Atlas of Radio Relic Mergers
• Impact of Baryonic Processes on Weak Lensing Cosmology: Power Spectrum, Non-Local Statistics, and Parameter Bias
• The Three Hundred Project: The evolution of galaxy cluster density profiles
• Cosmic Rays or Turbulence can Suppress Cooling Flows (Where Thermal Heating or Momentum Injection Fail)
• Indirect, Direct and Collider Detection of Neutralino Dark Matter
• Search for Dark Matter with GLAST
• Addressing the too big to fail problem with baryon physics and sterile neutrino dark matter
• The radial profiles of the different mass components in galaxy clusters
• Heating groups and clusters of galaxies: the role of AGN jets
• Self-interacting inelastic dark matter: A viable solution to the small scale structure problems
• Systematic variations of central mass density slopes in early-type galaxies
• Implications of multiple high-redshift galaxy clusters
• On the universality of density profiles
• ColDICE: a parallel Vlasov-Poisson solver using moving adaptive simplicial tessellation
• The SLUGGS Survey: The mass distribution in early-type galaxies within five effective radii and beyond
• Substructure around M31 : Evolution and Effects
• Dark Matter Direct Search Rates in Simulations of the Milky Way and Sagittarius Stream
• Search for dark matter towards the Galactic Centre with 11 years of ANTARES data
• Two lensed star candidates at $z\simeq 4.8$ behind the galaxy cluster MACS J0647.7+7015
• Prospects of antideuteron detection from dark matter annihilations or decays at AMS-02 and GAPS
• Cosmography with cluster strong lenses: the influence of substructure and line-of-sight halos
• Phase space mass bound for fermionic dark matter from dwarf spheroidal galaxies
• Calibration of bias and scatter involved in cluster mass measurements using optical weak gravitational lensing
• PINOCCHIO and the hierarchical build-up of dark matter haloes
• Secondary antiprotons as a Galactic Dark Matter probe
• From the Top Down and Back Up Again: Star Cluster Structure from Hierarchical Star Formation
• Investigation of circular geodesics in a rotating charged black hole in the presence of perfect fluid dark matter
• Lopsided galaxies: the case of NGC 891
• The Waning of the WIMP: Endgame?
• On Star Formation and the Non-Existence of Dark Galaxies
• Neutrino experiments probe hadrophilic light dark matter
• A clear Dark Matter gamma ray line generated by the Green-Schwarz mechanism
• Subhalo Demographics in the Illustris Simulation: Effects of Baryons and Halo-to-Halo Variation
• Dark Matter Annihilation Signatures from Electroweak Bremsstrahlung
• The spherical collapse model and cluster formation beyond the $\Lambda$ cosmology: Indications for a clustered dark energy?
• 3D simulations with boosted primordial power spectra and ultracompact minihalos
• Axisymmetric orbit models of N-body merger remnants: a dependency of reconstructed mass on viewing angle
• The SLUGGS Survey: Breaking degeneracies between dark matter, anisotropy and the IMF using globular cluster subpopulations in the giant elliptical NGC 5846
• The EMU view of the Large Magellanic Cloud: Troubles for sub-TeV WIMPs
• Existence of traversable wormholes in the spherical stellar systems
• Numerical and Analytical Predictions for the Large-Scale Sunyaev-Zel'dovich Effect
• Neutrino propagation in the galactic dark matter halo
• A New Approach to Detailed Structural Decomposition from the SPLASH and PHAT Surveys: Kicked-up Disk Stars in the Andromeda Galaxy?
• Indefinitely Flat Circular Velocities and the Baryonic Tully-Fisher Relation from Weak Lensing
• A critical reassessment of particle Dark Matter limits from dwarf satellites
• Dependency of halo concentration on mass, redshift and fossilness in Magneticum hydrodynamic simulations
• Constraining the Milky Way Mass Profile with Phase-Space Distribution of Satellite Galaxies
• The massive relic galaxy NGC 1277 is dark matter deficient. From dynamical models of integral-field stellar kinematics out to five effective radii
• Can LIGO Detect Non-Annihilating Dark Matter?
• Mass, shape and thermal properties of A1689 by a multi-wavelength X-ray, lensing and Sunyaev-Zel'dovich analysis
• The Enigmatic Galactic Center Excess: Spurious Point Sources and Signal Mismodeling
• Statistics of dark matter haloes expected from weak lensing surveys
• CFHTLenS and RCSLenS: Testing Photometric Redshift Distributions Using Angular Cross-Correlations with Spectroscopic Galaxy Surveys
• Finite Source Effects in Strong Lensing: Implications for the Substructure Mass Scale
• The Flattened Dark Matter Halo of M31 as Deduced from the Observed HI Scale Heights
• From lenticulars to blue compact dwarfs: the stellar mass fraction is regulated by disc gravitational instability
• Proper motion of gamma-rays from microhalo sources
• Direct and Indirect Detection of Neutralino Dark Matter In Selected Supersymmetry Breaking Scenarios
• Entropy Evolution in Galaxy Groups and Clusters; A Comparison of External and Internal Heating
• The PAMELA and ATIC Signals From Kaluza-Klein Dark Matter
• Subaru weak-lensing study of A2163: bimodal mass structure
• Deep XMM and Chandra observations of ClJ1226.9+3332: A detailed X-ray mass analysis of a z=0.89 galaxy cluster
• Accurate emulator for the redshift-space power spectrum of dark matter halos and its application to galaxy power spectrum
• Probing the nature of dark matter with accreted globular cluster streams
• Probing Small-Scale Power Spectra with Pulsar Timing Arrays
• A Spectro-photometric Search for Galaxy Clusters in SDSS
• Elastic and Inelastic Scattering of Cosmic-Rays on Sub-GeV Dark Matter
• Dark-Halo Cusp: Asymptotic Convergence
• A homogeneous measurement of the delay between the onsets of gas stripping and star formation quenching in satellite galaxies of groups and clusters
• The Growth of Intracluster Light in XCS-HSC Galaxy Clusters from $0.1<z<0.5$
• Spherical galaxy models as equilibrium configurations in nonextensive statistics
• A blind ATCA HI survey of the Fornax galaxy cluster: properties of the HI detections
• Dark matter substructure modelling and sensitivity of the Cherenkov Telescope Array to Galactic dark halos
• A Quantitative Link Between Globular Clusters and the Stellar Halos in Elliptical Galaxies
• Primordial-black-hole mergers in dark-matter spikes
• The origin and properties of massive prolate galaxies in the Illustris simulation
• Neutralino Gamma-ray Signals from Accreting Halo Dark Matter
• A simluated TCDM cosmology cluster catalogue: the NFW profile and the temperature-mass scaling relations
• Chemo-orbital evidence from SDSS/SEGUE G-type dwarf stars for a mixed origin of the Milky Way's thick disk
• Cluster abundance in chameleon $f(R)$ gravity I: toward an accurate halo mass function prediction
• Dark matter spike around Bumblebee black holes
• Two-Body Relaxation in Cosmological Simulations
• Chemistry of the Most Metal-poor Stars in the Bulge and the z > 10 Universe
• Unveiling Hidden Physics at the LHC
• Dynamical Mass Measurements of Contaminated Galaxy Clusters Using Machine Learning
• Multi wavelength study of the gravitational lens system RXS J1131-1231: II Lens model and source reconstruction
• Mock galaxy shape catalogs in the Subaru Hyper Suprime-Cam Survey
• The structure of gravitationally unstable gas-rich disk galaxies
• An Analytic Model of the Physical Properties of Galaxy Clusters
• Constraining Warm Dark Matter using QSO gravitational lensing
• Transient Radio Signatures from Neutron Star Encounters with QCD Axion Miniclusters
• Lensing degeneracies and mass substructure
• Streams in the Aquarius stellar haloes
• Structural and dynamical modeling of WINGS clusters. II. The orbital anisotropies of elliptical, spiral and lenticular galaxies
• In-spiraling Clumps in Blue Compact Dwarf Galaxies
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• The XMM Cluster Survey: Forecasting cosmological and cluster scaling-relation parameter constraints
• The Black Hole in the Compact, High-dispersion Galaxy NGC 1271
• Spin-driven jet feedback in idealised simulations of galaxy groups and clusters
• SILCC VII -- Gas kinematics and multiphase outflows of the simulated ISM at high gas surface densities
• MRK 1216 & NGC 1277 - An orbit-based dynamical analysis of compact, high velocity dispersion galaxies
• Further evidence for large central mass-to-light ratios in early-type galaxies: the case of ellipticals and lenticulars in the Abell~262 cluster
• Bailing Out the Milky Way: Variation in the Properties of Massive Dwarfs Among Galaxy-Sized Systems
• Universal Scaling Relations in Scale-Free Structure Formation
• Galactic Anisotropy as Signature of ``Top-Down'' Mechanisms of Ultra-High Energy Cosmic Rays
• Induced Nested Galactic Bars Inside Assembling Dark Matter Halos
• First star formation with dark matter annihilation
• Building gas rings and rejuvenating S0 galaxies through minor mergers
• A Unique Multi-Messenger Signal of QCD Axion Dark Matter
• Halo ellipticity of GAMA galaxy groups from KiDS weak lensing
• Spherical galaxy models with power law logarithmic slope
• The Magellanic Squall: Gas Replenishment from the Small to Large Magellanic Cloud
• Microlensing of the Lensed Quasar SDSS0924+0219
• Dark matter density profiles from the Jeans equation
• Mock Lightcones and Theory Friendly Catalogs for the CANDELS Survey
• Mass and Concentration estimates from Weak and Strong Gravitational Lensing: a Systematic Study
• Secluded singlet fermionic dark matter driven by the Fermi gamma-ray excess
• Inelastic Dark Matter As An Efficient Fuel For Compact Stars
• Probing the Outskirts of the Early Stage Galaxy Cluster Merger A1750
• The formation and evolution of young low-mass stars within halos with high concentration of dark matter particles
• Cosmic Emulation: The Concentration-Mass Relation for wCDM Universes
• Measuring the circum- and inter-galactic baryon contents with fast radio bursts
• Exploring the Galaxy's halo and very metal-weak thick disk with SkyMapper and Gaia DR2
• XMM-Newton Observation of an X-ray Trail Between the Spiral Galaxy NGC6872 and the Central Elliptical NGC6876 in the Pavo Group
• Kinetic Sunyaev-Zel'dovich effect from halo rotation
• An HI survey of six Local Group analogs: I. Survey description and the search for high-velocity clouds
• Merger of Dark Matter Axion Clumps and Resonant Photon Emission
• Distinguishing Dark Matter from Unresolved Point Sources in the Inner Galaxy with Photon Statistics
• Evolution of Phase-Space Density in Dark Matter Halos
• A nearby recent supernova that ejected the runaway star zeta Oph, the pulsar PSRB1706-16, and 60-Fe found on Earth
• The signature of primordial black holes in the dark matter halos of galaxies
• The shape of dark matter subhalos in the Aquarius simulations
• Can cosmological simulations capture the diverse satellite populations of observed Milky Way analogues?
• Accurate Modeling of Weak Lensing with the sGL Method
• Dark matter in the classical dwarf spheroidal galaxies: a robust constraint on the astrophysical factor for gamma-ray flux calculations
• Precision cluster mass determination from weak lensing
• Characterizing the Nature of the Unresolved Point Sources in the Galactic Center
• Self-consistent models of cuspy triaxial galaxies with dark matter haloes
• CLUMP-3D. Testing $\Lambda$CDM with galaxy cluster shapes
• 3D simulations of the early stages of AGN jets: geometry, thermodynamics and backflow
• A unified solution to the small scale problems of the $\Lambda$CDM model
• Virgo Cluster and field dwarf ellipticals in 3D - II. Internal dynamics points to tidal harassment?
• Derivation of the core mass -- halo mass relation of fermionic and bosonic dark matter halos from an effective thermodynamical model
• MaNGA DynPop -- I. Quality-assessed stellar dynamical modelling from integral-field spectroscopy of 10K nearby galaxies: a catalogue of masses, mass-to-light ratios, density profiles and dark matter
• Kinematic deprojection and mass inversion of spherical systems of known velocity anisotropy
• Constraints on Galactic Wino Densities from Gamma Ray Lines
• Cosmic Mass Functions from Gaussian Stochastic Diffusion Processes
• Search with EGRET for a Gamma Ray Line from the Galactic Center
• Reconstructing cosmic growth with kSZ observations in the era of Stage IV experiments
• Weak Lensing from Space II: Dark Matter Mapping
• Probing the shape and history of the Milky Way halo with orbital spectral analysis
• Hunting the lightest lightest neutralinos
• Orbits of massive satellite galaxies: II. Bayesian Estimates of the Milky Way and Andromeda masses using high precision astrometry and cosmological simulations
• Reconstructing the distribution of haloes and mock galaxies below the resolution limit in cosmological simulations
• Spending too much time at the Galactic bar: chaotic fanning of the Ophiuchus stream
• To beta or not to beta: can higher-order Jeans analysis break the mass-anisotropy degeneracy in simulated dwarfs?
• Cosmic-Ray Diffusion Suppression in Star-forming Regions Inhibits Clump Formation in Gas-rich Galaxies
• An analytical model for the non-linear redshift-space power spectrum
• Inner cusps of the first dark matter haloes: Formation and survival in a cosmological context
• The nature of voids: II. Tracing underdensities with biased galaxies
• The stellar structure and kinematics of dwarf spheroidal galaxies formed by tidal stirring
• Pairwise sums in colourings of the reals
• YZiCS: Unveiling Quenching History of Cluster Galaxies Using Phase-space Analysis
• Substructure Boosts to Dark Matter Annihilation from Sommerfeld Enhancement
• Stellar mass-to-light ratio gradients in galaxies: correlations with mass
• Fluctuations in the High-Redshift Lyman-Werner and Lyman-alpha Radiation Backgrounds
• Bounds on Long-lived Dark Matter Mediators from Neutron Stars
• Direct versus indirect detection in mSUGRA with self-consistent halo models
• Action-based dynamical models of dwarf spheroidal galaxies: application to Fornax
• Galaxy And Mass Assembly (GAMA): the red fraction and radial distribution of satellite galaxies
• Caught in the cosmic web: Environmental effect on halo concentrations, shape, and spin
• Galaxy spin as a formation probe: the stellar-to-halo specific angular momentum relation
• Weak lensing analysis of RXC J2248.7-4431
• Low energy IceCube data and a possible Dark Matter related excess
• Chandra Analysis and Mass Estimation of the Lensing Cluster of Galaxies CL0024+17
• The SAMI Galaxy Survey: The internal orbital structure and mass distribution of passive galaxies from triaxial orbit-superposition Schwarzschild models
• Weak Lensing Mass Measurements of Substructures in COMA Cluster with Subaru/Suprime-Cam
• The Universal Einstein Radius Distribution from 10,000 SDSS Clusters
• The Inner Caustics of Cold Dark Matter Halos
• IceCube Events from Heavy DM decays through the Right-handed Neutrino Portal
• Gaugino coannihilations
• The splashback boundary of haloes in hydrodynamic simulations
• Reconstructing the Velocity Distribution of WIMPs from Direct Dark Matter Detection Data
• An XMM-Newton observation of the massive, relaxed galaxy cluster ClJ1226.9+3332 at z=0.89
• Limits on the power-law mass and luminosity density profiles of elliptical galaxies from gravitational lensing systems
• The LMC geometry and outer stellar populations from early DES data
• Constrained Simulation of the Bullet Cluster
• Constraining dark matter annihilation with the isotropic $\gamma$-ray background: updated limits and future potential
• The 400d Galaxy Cluster Survey weak lensing programme: III: Evidence for consistent WL and X-ray masses at $z\approx 0.5$
• Probing the diffuse baryon distribution with the lensing-tSZ cross-correlation
• Stellar orbits and the survival of metallicity gradients in simulated dwarf galaxies
• Serendipitous Discovery of an Overdensity of Lyman-Alpha Emitters at z~4.8 in the Cl1604 Supercluster Field
• Probing the nature of dark matter via gravitational waves lensed by small dark matter halos
• Constraints on Dark Matter Annihilation in Clusters of Galaxies from Diffuse Radio Emission
• Mapping the 3-D Dark Matter potential with weak shear
• Reconstructing Three-dimensional Structure of Underlying Triaxial Dark Halos From Xray and Sunyaev-Zel'dovich Effect Observations of Galaxy Clusters
• Testing the effect of galactic feedback on the IGM at z ~ 6 with metal-line absorbers
• A Cosmological Kinetic Theory for the Evolution of Cold Dark Matter Halos with Substructure: Quasi-Linear Theory
• Line-of-sight effects in strong lensing: Putting theory into practice
• Star Clusters Around Recoiled Black Holes in the Milky Way Halo
• Implications of Recent Measurements of the Milky Way Rotation for the Orbit of the Large Magellanic Cloud
• Thermal instabilities in cooling galactic coronae: fuelling star formation in galactic discs
• Analytical Solutions to the Mass-Anisotropy Degeneracy with Higher Order Jeans Analysis: A General Method
• Radiative Transfer Effects on the Lya Forest
• MACHOs in M31? Absence of evidence but not evidence of absence
• A Search for Dark Matter Annihilation with the Whipple 10m Telescope
• Simultaneous Estimation of Time Delays and Quasar Structure
• Physical properties and scaling relations of molecular clouds: the effect of stellar feedback
• Improving Weak Lensing Mass Map Reconstructions using Gaussian and Sparsity Priors: Application to DES SV
• Dark Energy Survey Year 1 Results: Methodology and Projections for Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions
• The SLUGGS Survey: A comparison of total-mass profiles of early-type galaxies from observations and cosmological simulations, to $\sim$4 effective radii
• Introducing CGOLS: The Cholla Galactic OutfLow Simulation Suite
• Formation of LISA Black Hole Binaries in Merging Dwarf Galaxies: the Imprint of Dark Matter
• Interpreting the Clustering of Distant Red Galaxies
• CHAMP Cosmic Rays
• Light mixed sneutrinos as thermal dark matter
• Dark and luminous satellites of LMC-mass galaxies in the FIRE simulations
• Cosmic Ray Boosted Sub-GeV Gravitationally Interacting Dark Matter in Direct Detection
• Quasars and galaxy formation
• Weak and strong lensing analysis of the triaxial matter distribution of A1689
• Dark Matter and Synchrotron Emission from Galactic Center Radio Filaments
• Two Lensed z~3 Lyman Break Galaxies Discovered in the SDSS Giant Arcs Survey
• Rotation rates, sizes, and star formation efficiencies of a representative population of simulated disc galaxies
• Bispectrum of the Sunyaev-Zel'dovich Effect
• Constraints on the assembly history of the Milky Way's smooth, diffuse stellar halo from the metallicity-dependent, radially-dominated velocity anisotropy profiles probed with K giants and BHB stars using LAMOST, SDSS/SEGUE, and Gaia
• Structure and kinematics of tidally limited satellite galaxies in LCDM
• A fussy revisitation of antiprotons as a tool for Dark Matter searches
• Characterizing gravitational instability in turbulent multi-component galactic discs
• The Tully-Fisher relation of distant cluster galaxies
• Cosmological perturbations on local systems
• A Measurement of CMB Cluster Lensing with SPT and DES Year 1 Data
• Hydrodynamical simulations of galaxy clusters in dark energy cosmologies: II. c-M relation
• Computational issues in chemo-dynamical modelling of the formation and evolution of galaxies
• Deformed black hole immersed in dark matter spike
• From cusps to cores: a stochastic model
• Composite Dark Matter and LHC Interplay
• Dark Energy Survey Year 1 Results: Constraining Baryonic Physics in the Universe
• Testing dark matter and geometry sustained circular velocities in the Milky Way with Gaia DR2
• Kinematics and Mass Modeling of Messier 33: Halpha observations
• Starburst--driven galactic outflows
• Glueball scattering cross section in lattice SU(2) Yang-Mills theory
• The Cusp/Core problem: supernovae feedback versus the baryonic clumps and dynamical friction model
• The impact of baryons on dark matter haloes
• Dark matter cores in the Fornax and Sculptor dwarf galaxies: joining halo assembly and detailed star formation histories
• Galaxy disc scaling relations: A tight linear galaxy -- halo connection challenges abundance matching
• 2D Bayesian automated tilted-ring fitting of disk galaxies in large HI galaxy surveys: 2DBAT
• Connection between dynamically derived IMF normalisation and stellar population parameters
• Chandra deep observation of XDCP J0044.0-2033, a massive galaxy cluster at z>1.5
• Star-forming blue ETGs in two newly discovered galaxy overdensities in the HUDF at z=1.84 and 1.9: unveiling the progenitors of passive ETGs in cluster cores
• First measurement of the bulk flow of nearby galaxies using the cosmic microwave background
• Search for 511 keV Emission in Satellite Galaxies of the Milky Way with INTEGRAL/SPI
• MeV Dark Matter Complementarity and the Dark Photon Portal
• The morphology of the Milky Way - II. Reconstructing CO maps from disc galaxies with live stellar distributions
• Parameterised models for the lensing cluster Abell 1689
• Gravitational clustering of cosmic relic neutrinos in the Milky Way
• The Next Generation Virgo Cluster Survey. IV. NGC 4216: A Bombarded Spiral in the Virgo Cluster
• Gravitational lensing in modified Newtonian dynamics
• Quasinormal modes of black holes embedded in halos of matter
• Astrophysical Configurations with Background Cosmology: Probing Dark Energy at Astrophysical Scales
• A fast method for computing strong-lensing cross sections: Application to merging clusters
• Towards Robust Constraints on Axion Dark Matter using PSR J1745-2900
• Cosmological constraints with weak lensing peak counts and second-order statistics in a large-field survey
• Dissipationless collapse, weak homology and central cores of elliptical galaxies
• The Impact of Halo Properties, Energy Feedback and Projection Effects on the Mass-SZ Flux Relation
• The properties of energetically unbound stars in stellar clusters
• The Origin of Weak Lensing Convergence Peaks
• Hot gaseous atmospheres in galaxy groups and clusters are both heated and cooled by X-ray cavities
• Accretion Disk Size Measurement and Time Delays in the Lensed Quasar WFI 2033-4723
• Tracing the X-ray emitting intra-cluster medium of clusters of galaxies beyond r_200
• Infall caustics in dark matter halos?
• Dark matter subhaloes as gamma-ray sources and candidates in the first Fermi-LAT catalogue
• Tomographic-spectral approach for dark matter detection in the cross-correlation between cosmic shear and diffuse gamma-ray emission
• Dynamical Dark Matter and the Positron Excess in Light of AMS
• Could wormholes form in dark matter galactic halos?
• AGN-stimulated Cooling of Hot Gas in Elliptical Galaxies
• First Gaia dynamical model of the Milky Way disc with six phase space coordinates: a test for galaxy dynamics
• X-Ray Observations and the Structure of Elliptical Galaxies
• Matter bispectrum of large-scale structure: Three-dimensional comparison between theoretical models and numerical simulations
• Can winds driven by active galactic nuclei account for the extragalactic gamma-ray and neutrino backgrounds?
• Wide-Field Hubble Space Telescope Observations of the Globular Cluster System in NGC1399
• Dark matter halos and the anisotropy of ultra-high energy cosmic rays
• nIFTy Galaxy Cluster simulations IV: Quantifying the Influence of Baryons on Halo Properties
• Radio galaxy feedback in X-ray selected groups from COSMOS: the effect on the ICM
• PeV Neutrinos and a 3.5 keV X-Ray Line from a PeV Scale Supersymmetric Neutrino Sector
• Radial orbital anisotropy and the Fundamental Plane of elliptical galaxies
• Neutrino clustering around spherical dark matter halos
• The joint evolution of baryons and dark matter haloes
• Sculpting Andromeda -- made-to-measure models for M31's bar and composite bulge: dynamics, stellar and dark matter mass
• Probing dark matter with star clusters: a dark matter core in the ultra-faint dwarf Eridanus II
• Stars and Halos of Degenerate Relativistic Heavy-Neutrino and Neutralino Matter
• Global fits of the Non-Universal Higgs Model
• Probing Gravitino Dark Matter with PAMELA and Fermi
• Mass-temperature relation of galaxy clusters: implications from the observed luminosity-temperature relation and X-ray temperature function
• The Galactic Dust-Up: Modeling Dust Evolution in FIRE
• Mixed Neutralino Dark Matter in Nonuniversal Gaugino Mass Models
• Monochromatic dark neutrinos and boosted dark matter in noble liquid direct detection
• Apparent and average acceleration of the Universe
• Ultra-deep catalog of X-ray groups in the Extended Chandra Deep Field South
• Can multistate dark matter annihilation explain the high-energy cosmic ray lepton anomalies?
• Galaxy stability within a self-interacting dark matter halo
• More examples of structure formation in the Lemaitre-Tolman model
• Quasar-Galaxy and Galaxy-Galaxy Cross-Correlations: Model Predictions with Realistic Galaxies
• The strongest gravitational lenses: I. The statistical impact of cluster mergers
• Effects of the dissolution of low-concentration globular clusters on the evolution of globular cluster systems
• Superdense cosmological dark matter clumps
• R-Parity Breaking via Type II Seesaw, Decaying Gravitino Dark Matter and PAMELA Positron Excess
• The MOND Fundamental Plane
• WALLABY Early Science - III. An HI Study of the Spiral Galaxy NGC 1566
• Bayesian Implications of Current LHC Supersymmetry and Dark Matter Detection Searches for the Constrained MSSM
• Probing the Core Structure of Dark Halos with Tangential and Radial Arc Statistics
• Pegasus IV: Discovery and Spectroscopic Confirmation of an Ultra-Faint Dwarf Galaxy in the Constellation Pegasus
• AGN feedback, quiescence and CGM metal enrichment in early-type galaxies
• Identifying Stellar Streams in Gaia DR2 with Data Mining Techniques
• The Density Profile of Cluster-scale Dark Matter Halos
• Combined searches for dark matter in dwarf spheroidal galaxies observed with the MAGIC telescopes, including new data from Coma Berenices and Draco
• Structure of Axion Miniclusters
• The Distribution of Stellar Orbits in the Giant Elliptical Galaxy NGC 2320
• X-ray Mass Estimates at $z\sim 0.3$ for the CNOC Cluster Sample
• Searching for the GD-1 Stream Progenitor in Gaia DR2 with Direct N-body Simulations
• The Role of Penetrating Gas Streams in Setting the Dynamical State of Galaxy Clusters
• Lukewarm dark matter: Bose condensation of ultralight particles
• Cosmological Constraints on Invisible Decay of Dark Matter
• Resolving flows around black holes: numerical technique and applications
• Possible Indications of a Clumpy Dark Matter Halo
• Can TeVeS avoid Dark Matter on galactic scales?
• Figure Rotation of Cosmological Dark Matter Halos
• Minisuperspace quantum cosmology in $f(Q)$ gravity
• Ram pressure histories of cluster galaxies
• On the surface density of dark matter haloes
• The gravitational field of X-COP galaxy clusters
• Fitting rotation curve of galaxies by de Rham-Gabadadze-Tolley massive gravity
• Relaxing the Cosmological Moduli Problem by Low-scale Inflation
• Accurate weak lensing of standard candles. I. Flexible cosmological fits
• Constraining Dark Matter lifetime with a deep gamma-ray survey of the Perseus Galaxy Cluster with MAGIC
• Compact groups from the Millennium Simulations: I. Their Nature and the completeness of the Hickson sample
• Analysing surveys of our Galaxy -- II. Determining the potential
• Anisotropic Models for Globular Clusters, Galactic Bulges and Dark Halos
• X-ray emission from the Sombrero galaxy: a galactic-scale outflow
• Mapping Extragalactic Dark Matter Annihilation with Galaxy Surveys: A Systematic Study of Stacked Group Searches
• The Pisces-Cetus Supercluster: a remarkable filament of galaxies in the 2dF Galaxy Redshift Survey and Sloan Digital Sky surveys
• Improved optical mass tracer for galaxy clusters calibrated using weak lensing measurements
• Cosmology dependency of halo masses and concentrations in hydrodynamic simulations
• Full Lensing Analysis of Abell 1703: Comparison of Independent Lens-Modelling Techniques
• Intrinsic alignments of group and cluster galaxies in photometric surveys
• Uncertainties of Cosmic Ray Spectra and Detectability of Antiproton mSUGRA Contributions With PAMELA
• Probing galaxy evolution in massive clusters using ACT and DES: splashback as a cosmic clock
• The clustering and evolution of H-alpha emitters at z~1 from HiZELS
• Galactic cannibalism in the galaxy cluster C0337-2522 at z=0.59
• Determining the WIMP mass using the complementarity between direct and indirect searches and the ILC
• Solitons in the dark: non-linear structure formation with fuzzy dark matter
• The 2dF QSO Redshift Survey - X. Lensing of Background QSOs by Galaxy Groups
• Impact of Primordial Ultracompact Minihaloes on the Intergalactic Medium and First Structure Formation
• The halo mass function and filaments in full cosmological simulations with fuzzy dark matter
• Dark matter from late decays and the small-scale structure problems
• Dissipative Dark Matter on FIRE: I. Structural and kinematic properties of dwarf galaxies
• Kiloparsec view of a typical star-forming galaxy when the Universe was $\sim$1 Gyr old II. Regular rotating disk and evidence for baryon dominance on galactic scales
• Modified Dust and the Small Scale Crisis in CDM
• A single-merger scenario for the formation of the giant stream and the warp of M31
• The Multi-Epoch Nearby Cluster Survey: type Ia supernova rate measurement in z~0.1 clusters and the late-time delay time distribution
• Structure, Kinematics, and Chemical Enrichment Patterns after Major Gas-Rich Disc-Disc Mergers
• Precision Measurement of The Most Distant Spectroscopically Confirmed Supernova Ia with the Hubble Space Telescope
• Fast Winds Drive Slow Shells: A Model for the Circumgalactic Medium as Galactic Wind-Driven Bubbles
• Spin 3/2 Particle as a Dark Matter Candidate: an Effective Field Theory Approach
• Boosted Self-interacting Dark Matter in a Multi-component Dark Matter Model
• Soliton Oscillations and Revised Constraints from Eridanus II of Fuzzy Dark Matter
• The Mass Distribution and Rotation Curve in the Galaxy
• Black Hole Growth in Dark Matter and the M_{bh} - σRelation
• Information content in the halo-model dark-matter power spectrum II: Multiple cosmological parameters
• Improved Cosmic-Ray Injection Models and the Galactic Center Gamma-Ray Excess
• Global torques and stochasticity as the drivers of massive black hole pairing in the young Universe
• Dark-matter decays and Milky Way satellite galaxies
• Boosted Dark Matter at the Deep Underground Neutrino Experiment
• Discovery of the Central Excess Brightness in Hard X-rays in the Cluster of Galaxies Abell 1795
• Bringing the Galaxy's dark halo to life
• A spectroscopic survey of Andromeda's Western Shelf
• A constant characteristic volume density of dark matter haloes from SPARC rotation curve fits
• Update on decaying and annihilating heavy dark matter with the 6-year IceCube HESE data
• A Supersymmetric B-L Dark Matter Model and the Observed Anomalies in the Cosmic Rays
• The bias of DLAs at z ~ 2.3: contraining stellar feedback in shallow potential wells
• The large extent of dark matter haloes probed by the formation of tidal dwarf galaxies
• Millicharge or Decay: A Critical Take on Minimal Dark Matter
• Weak Lensing Results of the Merging Cluster A1758
• On the average density profile of dark-matter halos in the inner regions of massive early-type galaxies
• Size matters: the non-universal density profile of subhaloes in SPH simulations and implications for the Milky Way's dSphs
• The Density Profile of the Dark Matter Halo of NGC 4605
• Indirect Evidence for Dark Matter Density Spikes around Stellar-Mass Black Holes
• Unstable Cold Dark Matter and the Cuspy Halo Problem in Dwarf Galaxies
• A Search for Axionic Dark Matter Using the Magnetar PSR J1745-2900
• Detailed XMM-Newton Observation of the Cluster of Galaxies Abell 1060
• Suzaku observations of the Hydra A cluster out to the virial radius
• Multimass spherical structure models for N-body simulations
• The clustering of galaxies and galaxy clusters: constraints on primordial non-Gaussianity from future wide-field surveys
• Gravitational Lens Time Delays in CDM
• Core-halo mass relation of ultralight axion dark matter from merger history
• Probing Dark Matter Subhalos in Galaxy Clusters Using Highly Magnified Stars
• Predicting the hypervelocity star population in Gaia
• Missing black holes in brightest cluster galaxies as evidence for the occurrence of superkicks in nature
• Large-scale redshift space distortions in modified gravity theories
• Satellite Galaxy Number Density Profiles in the Sloan Digital Sky Survey
• MOND predictions of "halo" phenomenology in disc galaxies
• The Photometric and Kinematic Structure of Face-On Disk Galaxies. I. Sample Definition, H-alpha Integral Field Spectroscopy, and HI Line-Widths
• Squared temperature-temperature power spectrum as a probe of the CMB bispectrum
• Have Atmospheric Cerenkov Telescopes Observed Dark Matter?
• Fate of scalar dark matter solitons around supermassive galactic black holes
• TDCOSMO. IX. Systematic comparison between lens modelling software programs: time delay prediction for WGD 2038-4008
• The Via Lactea INCITE Simulation: Galactic Dark Matter Substructure at High Resolution
• Galactic Tide and Local Stellar Perturbations on the Oort Cloud: Creation of Interstellar Comets
• Indirect Detection of Self-Interacting Asymmetric Dark Matter
• IceCube astrophysical neutrinos without a spectral cutoff and (10^15-10^17) eV cosmic gamma radiation
• The Hyper-MUCHFUSS project: probing the Galactic halo with sdB stars
• What sets the central structure of dark matter haloes?
• Constraining the Milky Way Halo Shape Using Thin Streams
• An Ultra Metal-poor Star Near the Hydrogen-burning Limit
• What Do Dark Matter Properties Tell Us About Their Mass Assembly Histories?
• On the Discrepancy between Theoretical and X-Ray Concentration-Mass Relations for Galaxy Clusters
• Towards optimal cosmological parameter recovery from compressed bispectrum statistics
• Gravitational lensing as a probe of cold dark matter subhalos
• Galactic structure explained with dissipative mirror dark matter
• Radiation Pressure Driven Galactic Winds from Self-Gravitating Discs
• Predicting the density profiles of the first halos
• Projected central dark matter fractions and densities in massive early-type galaxies from the Sloan Digital Sky Survey
• Looking for a Heavy Higgsino LSP in Collider and Dark Matter Experiments
• Testing the reliability of weak lensing cluster detections
• A lensed radio jet at milli-arcsecond resolution I: Bayesian comparison of parametric lens models
• The SRG/eROSITA All-Sky Survey: Dark Energy Survey Year 3 Weak Gravitational Lensing by eRASS1 selected Galaxy Clusters
• Chandra and XMM-Newton Detection of Large-scale Diffuse X-ray Emission from the Sombrero Galaxy
• INFERNO: Galactic winds in dwarf galaxies with star-by-star simulations including runaway stars
• Dirac gaugino as leptophilic dark matter
• Dark matter dominance at all radii in the superthin galaxy UGC 7321
• Ultra-Diffuse Galaxies in the Perseus Cluster: Comparing Galaxy Properties with Globular Cluster System Richness
• Feeding vs. Falling: The growth and collapse of molecular clouds in a turbulent interstellar medium
• Galaxy rotation curves from General Relativity with Renormalization Group corrections
• The nature of the ISM in galaxies during the star-formation activity peak of the Universe
• Cluster Mass Profiles from Weak Lensing II
• Search for gravitational waves from high-mass-ratio compact-binary mergers of stellar mass and sub-solar mass black holes
• The SAGA Survey. III. A Census of 101 Satellite Systems around Milky Way-mass Galaxies
• A comparison of black hole growth in galaxy mergers with Gasoline and Ramses
• Constraining churning and blurring in the Milky Way using large spectroscopic surveys -- an exploratory study
• Stellar 3-D kinematics in the Draco dwarf spheroidal galaxy
• Anisotropic satellite galaxy quenching modulated by supermassive black hole activity
• Evolving topologically deformed wormholes supported in the dark matter halo
• Modeling the Baryon Cycle in Low Mass Galaxy Encounters: the Case of NGC 4490 & NGC 4485
• The DiskMass Survey. IV. The Dark-Matter-Dominated Galaxy UGC 463
• GASP XXVI. HI Gas in Jellyfish Galaxies: The case of JO201 and JO206
• Substructure Detection Reanalyzed: Dark Perturber shown to be a Line-of-Sight Halo
• Massive HI clouds with no optical counterparts as high-density regions of intragroup HI rings and arcs
• The dynamically selected stellar halo of the Galaxy with Gaia and the tilt of the velocity ellipsoid
• Triaxial strong-lensing analysis of the z > 0.5 MACS clusters: the mass-concentration relation
• Ricci focusing, shearing, and the expansion rate in an almost homogeneous Universe
• The Evolution of Substructure in Galaxy, Group and Cluster Haloes III: Comparison with Simulations
• Implications of Feebly Interacting Dark Sector on Neutron Star Properties and Constraints from GW170817
• Viscous dark matter growth in (neo-)Newtonian cosmology
• Bar slowdown and the distribution of dark matter in barred galaxies
• Ultimate age-dating method for galaxy groups; clues from the Millennium Simulations
• The effect of low mass substructures on the Cusp lensing relation
• Halo evolution in the presence of a disc bar
• A Tale of Two Portals: Testing Light, Hidden New Physics at Future $e^{+}{e}^{-}$ Colliders
• Simulating the Cooling Flow of Cool-Core Clusters
• Adiabatic compression and indirect detection of supersymmetric dark matter
• Efficacy of early stellar feedback in low gas surface density environments
• The Distribution of Satellite Galaxies in a Lambda-CDM Universe
• HI clouds in the proximity of M33
• Stellar Velocity Dispersion and Dynamical Mass of the Ultra-Diffuse Galaxy NGC 5846_UDG1 from the Keck Cosmic Web Imager
• Optical Cluster-Finding with An Adaptive Matched-Filter Technique: Algorithm and Comparison with Simulations
• A rumble in the dark: signatures of self-interacting dark matter in Super-Massive Black Hole dynamics and galaxy density profiles
• Evidences against cuspy dark matter halos in large galaxies
• The Contribution Of Inverse Compton Scattering To The Diffuse Extragalactic Gamma-Ray Background From Annihilating Dark Matter
• Imprints of Dark Energy on Cosmic Structure Formation: III. Sparsity of Dark Matter Halo Profiles
• Sensitivity of CTA to dark matter signals from the Galactic Center
• Project Dinos I: A joint lensing-dynamics constraint on the deviation from the power law in the mass profile of massive ellipticals
• Energy ejection in the collapse of a cold spherical self-gravitating cloud
• Non-parametric strong lens inversion of SDSS J1004+4112
• On the origin of the angular momentum properties of gas and dark matter in galactic halos and its implications
• A Study of Massive and Evolved Galaxies at High Redshift
• A kinematic study of the irregular dwarf galaxy NGC 2366 using HI and Halpha observations
• Is the Concentration of Dark Matter Halos at Virialization Universal ?
• Multiple Ultralight Axionic Wave Dark Matter and Astronomical Structures
• On the Initial Mass Function and tilt of the Fundamental Plane of massive early-type galaxies
• The mass-concentration relation in massive galaxy clusters at redshift ~1
• SIBELIUS-DARK: a galaxy catalogue of the Local Volume from a constrained realisation simulation
• Exploring the liminality: properties of haloes and subhaloes in borderline $f(R)$ gravity
• The many lives of active galactic nuclei-II: The formation and evolution of radio jets and their impact on galaxy evolution
• TDCOSMO. VII. Boxyness/discyness in lensing galaxies : Detectability and impact on $H_0$
• How Accurately Can We Detect the Splashback Radius of Dark Matter Halos and its Correlation With Accretion Rate?
• A global fit of the $\gamma$-ray galactic center excess within the scalar singlet Higgs portal model
• A neural simulation-based inference approach for characterizing the Galactic Center $\gamma$-ray excess
• GaBoDS: The Garching-Bonn Deep Survey -- II. Confirmation of EIS cluster candidates by weak gravitational lensing
• The core-cusp problem in cold dark matter halos and supernova feedback: Effects of Mass Loss
• On the Origin of the Inner Structure of Halos
• Extended HI spiral structure and the figure rotation of triaxial dark halos
• Are Compact High-Velocity Clouds Extragalactic Objects?
• Deriving the velocity distribution of Galactic Dark Matter particles from rotation curve data
• Why does the Jeans Swindle work?
• Kinetic Sunyaev-Zeldovich effect from galaxy cluster rotation
• Search for gamma-ray spectral lines with the DArk Matter Particle Explorer
• On the density profile of dark matter substructure in gravitational lens galaxies
• Ring galaxies from off-centre collisions
• Multipole analysis of IceCube data to search for dark matter accumulated in the Galactic halo
• Interpretation of AMS-02 Results: Correlations among Dark Matter Signals
• Reconciling MOND and dark matter?
• Cold gas disks in main-sequence galaxies at cosmic noon: Low turbulence, flat rotation curves, and disk-halo degeneracy
• Dark matter in galaxies
• Pseudo Rotation Curve connecting the Galaxy, Dark Halo, and Local Group
• On the density of Cold Dark Matter
• Anti-deuterons from heavy Dark Matter
• On the Stellar Kinematics and Mass of the Virgo Ultra-Diffuse Galaxy VCC 1287
• SDSS1133: An Unusually Persistent Transient in a Nearby Dwarf Galaxy
• Joint constraints on the Galactic dark matter halo and Galactic Centre from hypervelocity stars
• On Ellipsoidal Collapse and Primordial Black-Hole Formation
• Astrophysical constraints on extended gravity models
• Missing baryons traced by the galaxy luminosity density in the large-scale WHIM filaments
• Dark Cosmic Rays
• Tidal Stirring of Disky Dwarfs with Shallow Dark Matter Density Profiles: Enhanced Transformation into Dwarf Spheroidals
• Dark matter annihilation radiation in hydrodynamic simulations of Milky Way haloes
• Constraints on small-scale primordial power by annihilation signals from extragalactic dark matter minihalos
• Satellite dwarf galaxies: Stripped but not quenched
• Fingerprints of the initial conditions on the density profiles of cold and warm dark matter haloes
• Annihilation vs. Decay: Constraining dark matter properties from a gamma-ray detection
• Dark Energy Survey Year 1 Results: galaxy mock catalogues for BAO
• A Dark Matter Interpretation of the ANITA Anomalous Events
• Reconstructing the gravitational field of the local universe
• Dark galaxies or tidal debris? Kinematical clues to the origin of massive isolated HI clouds
• Extended MSSM Neutralinos as the Source of the PAMELA Positron Excess
• Clocking the formation of today's largest galaxies: Wide field integral spectroscopy of Brightest Cluster Galaxies and their surroundings
• An analytic investigation of the scatter in the integrated X-ray properties of galaxy groups and clusters
• Rotation Curve Decomposition for Size-Mass Relations of Bulge, Disk, and Dark Halo in Spiral Galaxies
• Imprints of primordial non-Gaussianity on the number counts of cosmic shear peaks
• Gaseous infall triggering starbursts in simulated dwarf galaxies
• Constraining Cluster Virialization Mechanism and Cosmology using Thermal-SZ-selected clusters from Future CMB Surveys
• Probing Galaxy Dark Matter Haloes in COSMOS with Weak Lensing Flexion
• Do current WIMP direct measurements constrain light relic neutralinos?
• Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters
• The Mice at play in the CALIFA survey: A case study of a gas-rich major merger between first passage and coalescence
• Novel Gamma-ray Spectral Features in the Inert Doublet Model
• CLASH-VLT: a full dynamical reconstruction of the mass profile of Abell S1063 from 1 kpc out to the virial radius
• Evaluating the ability of triaxial Schwarzschild modelling to estimate properties of galaxies from the Illustris simulation
• Formation of disk galaxies in preheated media: a preventative feedback model
• TDCOSMO III: Dark matter substructure meets dark energy -- the effects of (sub)halos on strong-lensing measurements of $H_0$
• Supernovae and AGN driven galactic outflows
• Secondary infall and dark matter haloes
• Shapley Supercluster Survey (ShaSS): Galaxy Evolution from Filaments to Cluster Cores
• A textbook example of ram-pressure stripping in the Hydra A/A780 cluster
• Simulating the Fermi Bubbles as Forward Shocks Driven by AGN Jets
• On the Origin of Density Cusps in Elliptical Galaxies
• The Role of the Radial Orbit Instability in Dark Matter Halo Formation and Structure
• Simulations of the flocculent spiral M33: what drives the spiral structure?
• The nature of dark matter and the density profile and central behavior of relaxed halos
• Collisional baryonic dark matter halos
• The Fornax Cluster VLT Spectroscopic Survey II - Planetary Nebulae kinematics within 200 kpc of the cluster core
• Feedback from galactic stellar bulges and hot gaseous haloes of galaxies
• The fate of the gaseous disks of galaxies that fall into clusters
• Dark Energy Survey Year 1 results: Validation of weak lensing cluster member contamination estimates from P(z) decomposition
• Thin accretion disk luminosity and its image around rotating black holes in perfect fluid dark matter
• On the status of superheavy dark matter
• Dark Matter Halo Profiles in Scale-Free Cosmologies
• Streams on FIRE: Populations of Detectable Stellar Streams in the Milky Way and FIRE
• Multiwavelength Analysis of Dark Matter Annihilation and RX-DMFIT
• Structure and dynamics of galaxies with a low surface brightness disc. I. The stellar and ionised-gas kinematics
• Milky Way Mass with K Giants and BHB Stars Using LAMOST, SDSS/SEGUE, and Gaia: 3D Spherical Jeans Equation and Tracer Mass Estimator
• Efficient Production of Sound Waves by AGN Jets in the Intracluster Medium
• New perspectives on the BOSS small-scale lensing discrepancy for the Planck $\Lambda$CDM Cosmology
• Collisions of Dark Matter Axion Stars with Astrophysical Sources
• Radiatively decaying scalar dark matter through U(1) mixings and the Fermi 130 GeV gamma-ray line
• Constraints on leptophilic dark matter from the AMS-02 experiment
• Realistic estimation for the detectability of dark matter sub-halos with Fermi-LAT
• Fast Estimation of Gravitational and Primordial Bispectra in Large Scale Structures
• Modelling Galaxy Merger Timescales and Tidal Destruction
• The splashback radius of optically selected clusters with Subaru HSC Second Public Data Release
• Correlations between Triaxial Shapes and Formation History of Dark Matter Haloes
• Correlation between galaxies and QSO in the SDSS:na signal from gravitational lensing magnification?
• The view from the boundary: a new void stacking method
• SUSY Implications from WIMP Annihilation into Scalars at the Galactic Centre
• Weak Gravitational Lensing by Dark Clusters
• The return of the merging galaxy subclusters of El Gordo?
• Simulated void galaxies in the standard cold dark matter model
• Breaking a dark degeneracy: The gamma-ray signature of early matter domination
• Formation of the largest galactic cores through binary scouring and gravitational wave recoil
• The Black Hole Mass in Brightest Cluster Galaxy NGC 6086
• ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
• A Halo Expansion (HEX) Technique for Approximating Simulated Dark Matter Haloes
• Starbursts in low-mass haloes at Cosmic Dawn. I. The critical halo mass for star formation
• Dissecting the Gamma-Ray Background in Search of Dark Matter
• A universal relation between the properties of supermassive black holes, galaxies, and dark matter halos
• Imitating accelerated expansion of the Universe by matter inhomogeneities - corrections of some misunderstandings
• Chasing Lyman alpha-emitting galaxies at z = 8.8
• Gas dynamics in dwarf galaxies as testbeds for dark matter and galaxy evolution
• Hypervelocity Stars from the Andromeda Galaxy
• Marked clustering statistics in $f(R)$ gravity cosmologies
• Small-scale shear: Peeling off diffuse subhalos with gravitational waves
• The Effect of Many Minor Mergers on the Size Growth of Compact Quiescent Galaxies
• Concentration, Ellipsoidal Collapse, and the Densest Dark Matter haloes
• Dark matter stripping in galaxy clusters: a look at the Stellar to Halo Mass relation in the Illustris simulation
• The velocity anisotropy of the Milky Way satellite system
• Dark Matter Microhalos From Simplified Models
• On stellar mass loss from galaxies in groups and clusters
• The clustering of ultra-high energy cosmic rays and their sources
• Radial density profiles of time-delay lensing galaxies
• Formation of a giant HI bridge between M31 and M33 from their tidal interaction
• Accurate Weak Lensing of Standard Candles. II. Measuring sigma8 with Supernovae
• On prospects for dark matter indirect detection in the Constrained MSSM
• Search for Cosmic-ray Boosted Sub-GeV Dark Matter using Recoil Protons at Super-Kamiokande
• The Q Continuum Simulation: Harnessing the Power of GPU Accelerated Supercomputers
• Accretion disk luminosity for black holes surrounded by dark matter with tangential pressure
• The effect of fluctuating fuzzy axion haloes on stellar dynamics: a stochastic model
• Deep Learning the Morphology of Dark Matter Substructure
• Kinematics of the faintest gas rich galaxy in the Local Group: DDO210
• Large-scale inhomogeneities may improve the cosmic concordance of supernovae
• The central dark matter distribution of NGC 2976
• Core-Collapse Supernovae in Binaries as the Origin of Galactic Hyper-Runaway Stars
• Scalar dark matter, Type II Seesaw and the DAMPE cosmic ray $e^{+}+e^{-}$ excess
• Studying the merging cluster Abell 3266 with eROSITA
• Strong lensing statistics and the power spectrum normalisation
• The Structure of Dissipative Dark Matter Halos
• Constraints on the halo density profile using HI flaring in the outer Galaxy
• Fitting functions for dark matter density profiles
• Secondary infall model and dark matter scaling relations in intermediate redshift early - type galaxies
• Sensitivity of cosmic-ray experiments to ultra-high-energy photons: reconstruction of the spectrum and limits on the superheavy dark matter
• Dark matter from the scalar sector of 3-3-1 models without exotic electric charges
• New constraints on the dark matter-neutrino and dark matter-photon scattering cross sections from TXS 0506+056
• Deadly dark matter cusps vs faint and extended star clusters: Eridanus II and Andromeda XXV
• The diversity of rotation curves of simulated galaxies with cusps and cores
• The inner dark matter distribution of the Cosmic Horseshoe (J1148+1930) with gravitational lensing and dynamics
• Intracluster light is already abundant at redshift beyond unity
• Gaia EDR3 in 6D: Searching for unbound stars in the Galaxy
• Landau equation for self-gravitating classical and quantum particles: Application to dark matter
• Velocity dispersion profile in dark matter halos
• The power of teaming up HST and Gaia: the first proper motion measurement of the distant cluster NGC 2419
• The bar pattern speed of NGC 4431
• KAT-7 Science Verification: Using HI Observations of NGC 3109 to Understand its Kinematics and Mass Distribution
• The Isotropic Radio Background and Annihilating Dark Matter
• Galaxy rotation curves in modified gravity models
• The dependence of galaxy clustering on stellar mass, star-formation rate and redshift at z = 0.8-2.2, with HiZELS
• Search for Gamma-ray Emission from Dark Matter Annihilation in the Small Magellanic Cloud with the Fermi Large Area Telescope
• The Non-Linear Matter Power Spectrum in Warm Dark Matter Cosmologies
• The merger history of the complex cluster Abell 1758: a combined weak lensing and spectroscopic view
• Indirect Detection of Dark Matter with gamma rays
• Propagation of high-energy neutrinos in a background of ultralight scalar dark matter
• Evolution of the Dark Matter Phase-Space Density Distributions of LCDM Halos
• Constraints on Dark Matter Annihilation/Decay from the Isotropic Gamma-Ray Background
• Gravitational wave of intermediate-mass black holes in Population III star clusters
• Galactic Tides and the Shape and Orientation of Dwarf Galaxy Satellites
• Gamma-ray Constraints on Dark Matter Annihilation into Charged Particles
• The formation of dusty cold gas filaments from galaxy cluster simulations
• Cusp-to-core transition in low-mass dwarf galaxies induced by dynamical heating of cold dark matter by primordial black holes
• Robust cosmic-ray constraints on $p$-wave annihilating MeV dark matter
• Galaxy cluster strong lensing cosmography: cosmological constraints from a sample of regular galaxy clusters
• Astrometric Microlensing by Local Dark Matter Subhalos
• Spatially Resolved Spectroscopy of the E+A Galaxies in the z=0.32 Cluster AC114
• The volumetric star formation law for nearby galaxies -- Extension to dwarf galaxies and low-density regions
• Gamma-Ray Background from Neutralino Annihilation in the First Cosmological Objects
• Direct Detection of Dark Matter Substructure in Strong Lens Images with Convolutional Neural Networks
• The Dark Matter Distributions in Low-Mass Disk Galaxies. II. The Inner Density Profiles
• Detecting WIMPs in the Microwave Sky
• Tracing Kinematic and Chemical Properties of Sagittarius Stream by K-Giants, M-Giants, and BHB stars
• Formation of the Galactic bulge from a two-component stellar disk: Explaining cylindrical rotation and vertical metallicity gradient
• IDCS J1426.5+3508: Cosmological implications of a massive, strong lensing cluster at Z = 1.75
• Locations of Accretion Shocks around Galaxy Clusters and the ICM properties: insights from Self-Similar Spherical Collapse with arbitrary mass accretion rates
• Inverse-Compton ghosts and double-lobed radio sources in the X-ray sky
• Evolution of central dark matter of early-type galaxies up to z ~ 0.8
• The regulation of star formation in cool-core clusters: imprints on the stellar populations of brightest cluster galaxies
• The Magellanic Stream: break up and accretion onto the hot Galactic corona
• Gamma-ray and synchrotron emission from neutralino annihilation in the Large Magellanic Cloud
• Wide binaries in ultra-faint galaxies: a window onto dark matter on the smallest scales
• An HI survey of the Centaurus and Sculptor Groups - Constraints on the space density of low mass galaxies
• Spontaneous generation of bending waves in isolated Milky Way-like discs
• Population syntheses of millisecond pulsars from the Galactic Disk and Bulge
• Observations of dark and luminous matter: the radial distribution of satellite galaxies around massive red galaxies
• Observation of small scale structure using sextupole lensing
• The aftermath of the Great Collision between our Galaxy and the Large Magellanic Cloud
• Constraining nuclear star cluster formation using MUSE-AO observations of the early-type galaxy FCC47
• Parasitic black holes: the swallowing of a fuzzy dark matter soliton
• Darwin Tames an Andromeda Dwarf: Unraveling the Orbit of NGC 205 Using a Genetic Algorithm
• Radio and Deep Chandra Observations of the Disturbed Cool Core Cluster Abell 133
• The impact of spurious collisional heating on the morphological evolution of simulated galactic discs
• Light Higgs Boson, Light Dark Matter and Gamma Rays
• Intermediate-mass black holes and ultraluminous X-ray sources in the Cartwheel ring galaxy
• Evolution of Hot Gas and Dark Halos in Group-Dominant Elliptical Galaxies: Influence of Cosmic Inflow
• RC100: Rotation Curves of 100 Massive Star-Forming Galaxies at z=0.6-2.5 Reveal Little Dark Matter on Galactic Scales
• Tidal Dwarf Galaxies and missing baryons
• Optical appearance of black holes surrounded by a dark matter halo
• The phase-space structure of tidally stripped halos
• The Fornax3D project: Assembly histories of lenticular galaxies from a combined dynamical and population orbital analysis
• The Stellar Distribution Function and Local Vertical Potential from Gaia DR2
• Comparing Accretion Disks and Dark Matter Spikes in Intermediate Mass Ratio Inspirals
• Structural and Dynamical Properties of Galaxies in a Hierarchical Universe: Sizes and Specific Angular Momenta
• A thermal-kinetic subgrid model for supernova feedback in simulations of galaxy formation
• Modelling supermassive black hole growth: towards an improved sub-grid prescription
• The 511 keV Excess and Primordial Black Holes
• Non--power law behavior of the radial profile of phase--space density of halos
• An imaging survey of a uniform sample of Brightest Cluster Galaxies and Intracluster Light
• Constraints on Galactic Intermediate Mass Black Holes
• Indirect Search for Dark Matter from the Galactic Center and Halo with the Super-Kamiokande Detector
• Status of Cold Dark Matter Cosmology
• The build-up of pseudobulges in a hierarchical universe
• The kinematics of massive quiescent galaxies at $1.4<z<2.1$: dark matter fractions, IMF variation, and the relation to local early-type galaxies
• An environmental dependence of the physical and structural properties in the Hydra Cluster galaxies
• Probing for Dark Matter within Spiral Galaxy Disks
• Reliability of the dark matter clustering in cosmological N-body simulation on scales below the mean separation length of particles
• Updated Constraints on Primordial Black Hole Evaporation
• Keck Integral-Field Spectroscopy of M87 Reveals an Intrinsically Triaxial Galaxy and a Revised Black Hole Mass
• The little galaxy that could: Kinematics of Camelopardalis B
• Non-linear Galaxy Power Spectrum and Cosmological Parameters
• The isolated interacting galaxy pair NGC 5426/27 (Arp 271)
• The necessity of dark matter in MOND within galactic scales
• The edge of galaxy formation II: evolution of Milky Way satellite analogues after infall
• Relativistic numerical cosmology with Silent Universes
• A Neural Network Gravitational Arc Finder based on the Mediatrix filamentation Method
• The Nature of Dark Matter
• Modeling the gravitational potential of a cosmological dark matter halo with stellar streams
• Dark Matter And $B_s\to {\mu }^{+}{\mu }^{-}$ With Minimal $S{O}_{10}$ Soft SUSY Breaking II
• On the genealogy of the Orphan Stream
• KiDS-Legacy calibration: unifying shear and redshift calibration with the SKiLLS multi-band image simulations
• Lifetime Constraints for Late Dark Matter Decay
• GASP and MaNGA surveys shed light on the enigma of the gas metallicity gradients in disk galaxies
• Interstellar Gas Heating by Primordial Black Holes
• Made-to-Measure Dark Matter Haloes, Elliptical Galaxies and Dwarf Galaxies in Action Coordinates
• On an alternative mechanism for the black hole echoes
• How baryons can significantly bias cluster count cosmology
• Asymmetric Surface Brightness Structure of Caustic Crossing Arc in SDSS J1226+2152: A Case for Dark Matter Substructure
• Antideuterons from dark matter annihilations and hadronization model dependence
• Cloning Hubble Deep Fields II: Models for Evolution by Bright Galaxy Image Transformation
• Anisotropy of Ultra High Energy Cosmic Rays in the Dark Matter Halo Model
• Right-handed Sneutrino Dark Matter in Supersymmetric B-L Model
• Measuring gravity at cosmological scales
• Neutral Hydrogen Clouds near Early-Type Dwarf Galaxies of the Local Group
• Hunting for Heavy Winos in the Galactic Center
• An optimum time-stepping scheme for N-body simulations
• Slowly rotating Bose Einstein Condensate galactic dark matter halos, and their rotation curves
• MAGI: many-component galaxy initialiser
• Strong orientation dependence of surface mass density profiles of dark haloes at large scales
• Probing the small-scale structure in strongly lensed systems via transdimensional inference
• The history of the dark and luminous side of Milky Way-like progenitors
• Exceptional Composite Dark Matter
• A new astrophysical solution to the Too Big To Fail problem - Insights from the MoRIA simulations
• Populating the Galaxy with pulsars -- II. Galactic dynamics
• Binary pulsars as dark-matter probes
• The Impact of Molecular Gas on Mass Models of Nearby Galaxies
• ALMA Imprint of Intergalactic Dark Structures in the Gravitational Lens SDP.81
• Testing phenomenological and theoretical models of dark matter density profiles with galaxy clusters
• Estimating the Galactic Mass Profile in the Presence of Incomplete Data
• Brighter galaxy bias: underestimating the velocity dispersions of galaxy clusters
• Dynamical Models of Elliptical Galaxies -- II. M87 and its Globular Clusters
• Initial Conditions for Idealised Clusters Mergers, simulating El Gordo
• The Contribution of z<6 Sources to the Spatial Coherence in the Unresolved Cosmic near-Infrared and X-ray Backgrounds
• A study of AGN and supernova feedback in simulations of isolated and merging disc galaxies
• Accretion of Galaxy Groups into Galaxy Clusters
• The Red Dead Redemption Survey of Circumgalactic Gas About Massive Galaxies. I. Mass and Metallicity of the Cool Phase
• The Semi-Hooperon: Gamma-ray and anti-proton excesses in the Galactic Center
• Testing Bose-Einstein Condensate dark matter models with the SPARC galactic rotation curves data
• Probing decaying heavy dark matter with the 4-year IceCube HESE data
• Understanding `galaxy groups' as a unique structure in the universe
• The Formation of S0 Galaxies with Counter-Rotating Neutral and Molecular Hydrogen
• Evidence for a high-z ISW signal from supervoids in the distribution of eBOSS quasars
• GOODS-ALMA: Optically dark ALMA galaxies shed light on a cluster in formation at z = 3.5
• Extended Source Effects in Substructure Lensing
• An extended Pal 5 stream in Gaia DR2
• Constraining Supersymmetric Dark Matter With Synchrotron Measurements
• Modeling Galaxy Clustering by Color
• Mass Calibration of Optically Selected DES clusters using a Measurement of CMB-Cluster Lensing with SPTpol Data
• On the over-concentration problem of strong lensing clusters
• Hydrostatic mass estimates of massive galaxy clusters: a study with varying hydrodynamics flavours and non-thermal pressure support
• Observed trend in the star formation history and the dark matter fraction of galaxies at redshift $z\approx 0.8$
• New mass bound on fermionic dark matter from a combined analysis of classical dSphs
• Cross-correlation of the thermal Sunyaev-Zel'dovich effect and weak gravitational lensing: Planck and Subaru Hyper Suprime-Cam first-year data
• Alignment of Brightest Cluster Galaxies with their Host Clusters
• Boosted Dark Matter at Neutrino Experiments
• The Mass, Baryonic Fraction, and X-ray Temperature of the Luminous, High Redshift Cluster of Galaxies, MS0451.6-0305
• Kinematics of two dwarf galaxies in the NGC 6946 group
• SDSS--IV MaNGA : The Inner Density Slopes of nearby galaxies
• Ram pressure drag - the effects of ram pressure on dark matter and stellar disk dynamics
• The global stability of M33: still a puzzle
• Dark matter scattering cross section and dynamics in dark Yang-Mills theory
• Halo Concentration, Galaxy Red Fraction, and Gas Properties of Optically-defined Merging Clusters
• The role of gas infall in the evolution of disc galaxies
• Optimized analysis method for indirect dark matter searches with Imaging Air Cherenkov Telescopes
• A Photometric and Kinematic Analysis of UDG1137+16 (dw1137+16): Probing Ultra-Diffuse Galaxy Formation in a Group Environment
• Radially extended kinematics and stellar populations of the massive ellipticals NGC1600, NGC4125 and NGC7619. Constraints on the outer dark halo density profile
• Self Similar Spherical Collapse Revisited: a Comparison between Gas and Dark Matter Dynamics
• Active galactic nucleus jet feedback in hydrostatic halos
• A unified solution to the small scale problems of the $\Lambda$CDM model II: introducing parent-satellite interaction
• Gravitational softening as a smoothing operation
• Quark stars with 2.6 $M_{\odot }$ in a non-minimal geometry-matter coupling theory of gravity
• Non-Kolmogorov turbulence in multiphase intracluster medium driven by cold gas precipitation and AGN jets
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• CLUMP-3D. Three dimensional lensing and multi-probe analysis of MACS J1206.2-0847, a remarkably regular cluster
• Controlling and leveraging small-scale information in tomographic galaxy-galaxy lensing
• Sneutrino Dark Matter and the Observed Anomalies in Cosmic Rays
• Bayesian inferences of galaxy formation from the K-band luminosity and HI mass functions of galaxies: constraining star formation and feedback
• Galaxy Satellites and the Weak Equivalence Principle
• Sensitivity of the Cherenkov Telescope Array to the detection of a dark matter signal in comparison to direct detection and collider experiments
• Dark Matter Signatures in the Anisotropic Radio Sky
• AGN heating, thermal conduction and Sunyaev-Zeldovich effect in galaxy groups and clusters
• The vertical structure of gaseous galaxy discs in cold dark matter halos
• Globular clusters as tracers of the dark matter content of dwarfs in galaxy clusters
• Time Delay and Accretion Disk Size Measurements in the Lensed Quasar SBS 0909+532 from Multiwavelength Microlensing Analysis
• The Anisotropy of the Ultra-High Energy Cosmic Rays
• Gravitational ringing and superradiant instabilities of the Kerr-like black holes in a dark matter halo
• Evolutionary tracks of tidally stirred disky dwarf galaxies
• Differentiable Strong Lensing: Uniting Gravity and Neural Nets through Differentiable Probabilistic Programming
• Globular clusters as tracers of the dark matter halo: insights from the E-MOSAICS simulations
• A Dark Matter Model with Non-Abelian Gauge Symmetry
• Box/peanut-shaped bulges in action space
• Merging history of three bimodal clusters
• The Inflaton Portal to a Highly decoupled EeV Dark Matter Particle
• Measurement of the dark matter velocity anisotropy in galaxy clusters
• Ruling out thermal dark matter with a black hole induced spiky profile in the M87 galaxy
• The hunt for the Milky Way's accreted disc
• On distortion of the background radiation spectrum by wormholes: kinematic Sunyaev-Zel'dovich effect
• Axion Miniclusters Made Easy
• On the Spiral Structure of NGC 2915 and Dark Matter
• Validating a minimal galaxy bias method for cosmological parameter inference using HSC-SDSS mock catalogs
• Gamma Ray Lines from a Universal Extra Dimension
• The dark matter halos of the bluest low surface brightness galaxies
• Interactions of Astrophysical Neutrinos with Dark Matter: A model building perspective
• CLUES on Fermi-LAT prospects for the extragalactic detection of munuSSM gravitino Dark Matter
• Dark matter halo cores and the tidal survival of Milky Way satellites
• A novel approach to optimize the regularization and evaluation of dynamical models using a model selection framework
• Dynamical Models of Elliptical Galaxies -- I. Simple Methods
• Cosmic Ray Driven Outflows from the Large Magellanic Cloud: Contributions to the LMC Filament
• Weak Lensing Observables in the Halo Model
• Constraints on the evolution of the relationship between HI mass and halo mass in the last 12 Gyr
• Connecting the structure of dark matter haloes to the primordial power spectrum
• Boosted Dark Matter and its implications for the features in IceCube HESE data
• A Comparison of Metal Enrichment Histories in Rich Clusters and Individual Luminous Elliptical Galaxies
• The Effects of radial inflow of gas and galactic fountains on the chemical evolution of M31
• Degeneracies Between Self-interacting Dark Matter and Supernova Feedback as cusp-core transformation mechanisms
• Dark Matter in the MSSM
• Neutrinos from captured dark matter annihilation in a galactic population of neutron stars
• Extragalactic gamma-ray signal from Dark Matter annihilation: a power spectrum based computation
• Complete ionisation of the neutral gas: why there are so few detections of 21-cm hydrogen in high redshift radio galaxies and quasars
• The DEEP2 Galaxy Redshift Survey: Probing the Evolution of Dark Matter Halos around Isolated Galaxies at z ~ 1
• Precision Cosmology
• The Effects of Massive Substructures on Image Multiplicities in Gravitati onal Lenses
• Search for $\gamma$-ray emission from dark matter particle interactions from Andromeda and Triangulum Galaxies with the Fermi Large Area Telescope
• The Effects of Ram-pressure Stripping and Supernova Winds on the Tidal Stirring of Disky Dwarfs: Enhanced Transformation into Dwarf Spheroidals
• Anisotropic cosmic optical background bound for decaying dark matter in light of the LORRI anomaly
• Sound Waves Excitation by Jet-Inflated Bubbles in Clusters of Galaxies
• Mass Models for Spiral Galaxies from 2-D Velocity Maps
• On the Origin of Cusps in Stellar Systems
• Cosmological Constraints from the Large Scale Weak Lensing of SDSS MaxBCG Clusters
• The Smith Cloud and its dark matter halo: Survival of a Galactic disc passage
• Solar Wakes of Dark Matter Flows
• Closing in on mass-degenerate dark matter scenarios with antiprotons and direct detection
• Completeness in Photometric and Spectroscopic Searches for Clusters
• The Clustering and Host Halos of Galaxy Mergers at High Redshift
• What determines the flatness of X-shaped structures in edge-on galaxies
• Synchrotron Emission from Dark Matter Annihilation: Predictions for Constraints from Non-detections of Galaxy Clusters with New Radio Surveys
• The Cold Dark Matter crisis on galactic and subgalactic scales
• The MillenniumTNG Project: Refining the one-halo model of red and blue galaxies at different redshifts
• The shapes of Milky Way satellites: looking for signatures of tidal stirring
• A discrete chemo-dynamical model of the giant elliptical galaxy NGC 5846: dark matter fraction, internal rotation and velocity anisotropy out to six effective radii
• A dwarf-dwarf merger and dark matter core as a solution to the Globular Cluster problems in the Fornax dSph
• Massive disc galaxies in cosmological hydrodynamical simulations are too dark matter-dominated
• Cosmic ray driven winds in the Galactic environment and the cosmic ray spectrum
• Statistical detection of a tidal stream associated with the globular cluster M68 using Gaia data
• Vector Fermion-Portal Dark Matter: Direct Detection and Galactic Center Gamma-Ray Excess
• Neutrinos from Dark Matter annihilations at the Galactic Centre
• Searching for Sub-GeV Dark Matter in the Galactic Centre using Hyper-Kamiokande
• Schrödinger-Poisson Solitons: Perturbation Theory
• A robust mass estimator for dark matter subhalo perturbations in strong gravitational lenses
• Effect of the heating rate on the stability of the three-phase interstellar medium
• Universal Profiles of the Intracluster Medium from Suzaku X-Ray and Subaru Weak Lensing Obesrvations
• The effects of baryonic cooling on the concentration-mass relation
• Effects of quintessence on observations of Type Ia SuperNovae in the clumpy Universe
• First lensing measurements of SZ-discovered clusters
• The modified dynamics (MOND) predicts an absolute maximum to the acceleration produced by `dark halos'
• LCDM halo substructure properties revealed with high resolution and large volume cosmological simulations
• CMB-Cluster Lensing
• Kinematic properties of the field elliptical NGC 7507
• Estimating non-circular motions in barred galaxies using numerical N-body simulations
• Numerical simulations of dwarf galaxy merger trees
• From giant clumps to clouds -- II. The emergence of thick disc kinematics from the conditions of star formation in high redshift gas rich galaxies
• Simulating galaxy evolution with a non-universal stellar initial mass function
• From giant clumps to clouds -- III. The connection between star formation and turbulence in the ISM
• Early formation of galaxies initiated by clusters of primordial black holes
• N-body simulations of dark matter with frequent self-interactions
• Multifield Ultralight Dark Matter
• A tidal disruption model for the gamma-ray burst of GRB 060614
• Detecting Dark Matter Cores in Galaxy Clusters with Strong Lensing
• The case for decaying spin-3/2 dark matter
• Antideuteron Limits on Decaying Dark Matter with a Tuned Formation Model
• Lack of nuclear clusters in dwarf spheroidal galaxies: implications for massive black holes formation and the cusp/core problem
• Shock and Splash: Gas and Dark Matter Halo Boundaries around LambdaCDM Galaxy Clusters
• Constraining the primordial magnetic field with dwarf galaxy simulations
• On the stability of tidal streams in action space
• Tidal truncation of gas replenishment and global suppression of galactic star formation in distant clusters
• Ringing of a black hole in a dark matter halo
• Probing Cosmic-Ray Accelerated Light Dark Matter with IceCube
• Non-minimally coupled dark matter: effective pressure and structure formation
• On relaxation processes in collisionless mergers
• Turbulence and the formation of filaments, loops and shock fronts in NGC 1275 in the Perseus Galaxy Cluster
• Improved $(g-2{)}_{\mu }$ Measurements and Wino/Higgsino Dark Matter
• Detection of Quasar Feedback from the Thermal Sunyaev-Zel'dovich Effect in Planck
• The effect of non-equilibrium metal cooling on the interstellar medium
• Non-circular motions and the cusp-core discrepancy in dwarf galaxies
• How reliable is the kinematical evidence for dark matter: the effects of non-sphericity, substructure and streaming motions
• Is The Gamma-Ray Source 3FGL J2212.5+0703 A Dark Matter Subhalo?
• Challenges and Opportunities of Gravitational Wave Searches above 10 kHz
• Complementarity of Galactic radio and collider data in constraining WIMP dark matter models
• PICS: Simulations of Strong Gravitational Lensing in Galaxy Clusters
• Phase-space structure of protohalos: Vlasov versus Particle-Mesh
• Did Sgr cause the vertical waves in the solar neighbourhood?
• Bright and Dark Matter in Elliptical Galaxies: Mass and Velocity Distributions from Self-consistent Hydrodynamical Simulations
• A gradient based method for modeling baryons and matter in halos of fast simulations
• Exploring the astrophysics of dark atoms
• New minimal, median, and maximal propagation models for dark matter searches with Galactic cosmic rays
• The dynamics of z~1 clusters of galaxies from the GCLASS survey
• Role of clusters of galaxies in the evolution of the metal budget in the Universe
• Constraining thermal dust emission in distant galaxies with number counts and angular power spectra
• Prospects For Detecting Dark Matter With GLAST In Light Of The WMAP Haze
• Growing Massive Black Holes in a Local Group Environment: the Central Supermassive, Slowly Sinking, and Ejected Populations
• On the CGM Fundamental Plane: The Halo Mass Dependency of Circumgalactic HI
• Analysing surveys of our Galaxy I: basic astrometric data
• A Black Hole Mass Determination for the Compact Galaxy Mrk 1216
• Bayesian Mass Estimates of the Milky Way: including measurement uncertainties with hierarchical Bayes
• First results on the cluster galaxy population from the Subaru Hyper Suprime-Cam survey. II. Faint end color-magnitude diagrams and radial profiles of red and blue galaxies at $0.1<z<1.1$
• Analyzing γ-rays of the Galactic Center with Deep Learning
• Recurrent Axinovae and their Cosmological Constraints
• The importance of magnification effects in galaxy-galaxy lensing
• Neutralino, axion and axino cold dark matter in minimal, hypercharged and gaugino AMSB
• GASP XXVII: Gas-phase metallicity scaling relations in disk galaxies with and without ram-pressure stripping
• Indirect search for dark matter: prospects for GLAST
• Formation and evolution of early-type galaxies. II. Models with quasi-cosmological initial conditions
• Dark matter halos and scaling relations of extremely massive spiral galaxies from extended HI rotation curves
• Can a negative-mass cosmology explain dark matter and dark energy?
• Formation of Dwarf Spheroidal Galaxies Via Mergers of Disky Dwarfs
• On the sensitivity of CTA to gamma-ray boxes from multi-TeV dark matter
• THE NEXT GENERATION VIRGO CLUSTER SURVEY. XIV. Shell feature early-type dwarf galaxies in the Virgo cluster
• On the road to percent accuracy III: non-linear reaction of the matter power spectrum to massive neutrinos
• The Solar neighbourhood in angle coordinates: the Hyades moving group
• A Consistent Set of Empirical Scaling Relations for Spiral Galaxies: The $(v_{\max },M_{\mathrm{DM}})$-$({\sigma }_0,M_{\mathrm{BH}},\varphi )$ Relations
• Discovery of a Quadruple Lens in CANDELS with a Record Lens Redshift z=1.53
• Using Weak Lensing to find Halo Masses
• The evolution of the metallicity gradient and the star formation efficiency in disc galaxies
• Analysis of galactic tides and stars on CDM microhalos
• Identification of All Dark Matter as Black Holes
• On spatial distributions of old globular clusters in clusters of galaxies
• Inside a Beehive: the Multiple Merging Processes in the Galaxy Cluster Abell 2142
• Angular Signatures of Dark Matter in the Diffuse Gamma Ray Background
• Constraints on interacting dark energy models from galaxy Rotation Curves
• Formation of S0s via disc accretion around high-redshift compact ellipticals
• Confronting Galactic and Extragalactic $\gamma$-ray observed by Fermi-LAT with Annihilating Dark Matter in Inert Higgs Doublet Model
• A potential WIMP signature for the caustic ring halo model
• Gravitational imaging through a triple source plane lens: revisiting the $\Lambda$CDM-defying dark subhalo in SDSSJ0946+1006
• Finding Dwarf Galaxies From Their Tidal Imprints
• Galactic Signatures of Decaying Dark Matter
• A 3.55 keV line from $\text{DM}\to a\to \gamma$: predictions for cool-core and non-cool-core clusters
• Phase-space correlation in stellar streams of the Milky Way halo: The clash of Kshir and GD-1
• Dark matter annihilation from intermediate-mass black holes: Contribution to the extragalactic gamma-ray background
• PAMELA/ATIC anomaly from the meta-stable extra dark matter component and the leptophilic Yukawa interaction
• Dark matter-baryon scaling relations from Einasto halo fits to SPARC galaxy rotation curves
• Gravitational Lensing of Schwarzschild and Charged Black Holes Immersed in Perfect Fluid Dark Matter Halo
• Bar instability in cosmological halos
• Dynamical model of the Milky Way using APOGEE and Gaia data
• Gravitational Lens Statistics and The Density Profile of Dark Halos
• Stochastic Axion Dark Matter in Axion Landscape
• An orbital perspective on the starvation, stripping, and quenching of satellite galaxies in the EAGLE simulations
• From Snakes to Stars, the Statistics of Collapsed Objects - I. Lower--order Clustering Properties
• Multiple dynamical components in Local Group dwarf spheroidals
• The stellar halo of isolated central galaxies in the Hyper Suprime-Cam imaging survey
• The Spectroscopy and H-band Imaging of Virgo cluster galaxies (SHIVir) Survey: Scaling Relations and the Stellar-to-Total Mass Relation
• On the Determination of Rotation Velocity and Dynamical Mass of Galaxies Based on Integrated H I Spectra
• Modified gravity models and the central cusp of dark matter halos in galaxies
• Strong Optimized Conservative Fermi-LAT Constraints on Dark Matter Models from the Inclusive Photon Spectrum
• Pixel lensing: Microlensing towards M31
• Individual and Group Galaxies in CNOC1 clusters
• Hydrodynamical simulations of coupled and uncoupled quintessence models I: Halo properties and the cosmic web
• Self-Similar Spherical Collapse with Tidal Torque
• Reconciling optical and X-ray mass estimates: the case of the elliptical galaxy NGC3379
• The dark matter profile of the Milky Way: a non-parametric reconstruction
• Discovery of Hot Gas in Outflow in NGC3379
• Jeans instability and turbulent gravitational collapse of Bose-Einstein Condensate dark matter halos
• Spatial Origin of Galactic Cosmic Rays in Diffusion Models: II- Exotic Primary Cosmic Rays
• Dark Matter Halo Properties vs. Local Density and Cosmic Web Location
• Ultra High Energy Cosmic Rays: propagation in the Galaxy and anisotropy
• Explaining the ANITA Anomaly with Inelastic Boosted Dark Matter
• The Effective Halo Model: Creating a Physical and Accurate Model of the Matter Power Spectrum and Cluster Counts
• Soliton Formation and the Core-Halo Mass Relation: An Eigenstate Perspective
• Boosted Dark Matter Quarrying at Surface Neutrino Detectors
• Mass models from high-resolution HI data of the dwarf galaxy NGC 1560
• Has DAMA Detected Self-Interacting Dark Matter?
• The SIBELIUS Project: E Pluribus Unum
• Spatial and luminosity distributions of galactic satellites
• The radial acceleration relation in a $\Lambda$CDM universe
• Dark Grand Unification in the Axiverse: Decaying Axion Dark Matter and Spontaneous Baryogenesis
• A Multi-Wavelength Analysis of Annihilating Dark Matter as the Origin of the Gamma-Ray Emission from M31
• Galaxy Kinematics and Mass Calibration in Massive SZE Selected Galaxy Clusters to z=1.3
• Scale dependence of galaxy biasing investigated by weak gravitational lensing: An assessment using semi-analytic galaxies and simulated lensing data
• SEAGLE - I: A pipeline for simulating and modeling strong lenses from cosmological hydrodynamic simulations
• Detecting the Sagittarius stream with LAMOST DR4 M giants \& Gaia DR2
• Systematic Effects on Tangential and Radial Arc Statistics: The Finite Source Size and Ellipticities of the Lens and Source
• The Massive Galaxy Cluster XMMU J1230.3+1339 at z ~ 1: Colour-magnitude relation, Butcher-Oemler effect, X-ray and weak lensing mass estimates
• The emergence of universal relations in the AdS black holes thermodynamics
• Milking the spherical cow: on aspherical dynamics in spherical coordinates
• Multiple Dark Matter as a self-regulating mechanism for dark sector interactions
• Mass loss in tidally stripped systems; the energy-based truncation method
• Simplified Dark Matter Models Confront the Gamma Ray Excess
• Resolving the discrepancy between lensing and X-ray mass estimates of the complex galaxy cluster Abell 1689
• Mapping Dark Matter with Extragalactic Stellar Streams: the Case of Centaurus A
• Chemodynamic evolution of dwarf galaxies in tidal fields
• Reionisation in sterile neutrino cosmologies
• CMB Polarization towards Clusters as a Probe of the Integrated Sachs-Wolfe Effect
• Tidal Stripping in the Adiabatic Limit
• Halo Dark Matter and Ultra-High Energy Cosmic Rays
• Exploring compact binary merger host galaxies and environments with $\mathrm{zELDA}$
• Impact of kinetic and potential self-interactions on scalar dark matter
• Constraining self-interacting dark matter with scaling laws of observed halo surface densities
• Primordial black holes and the observed Galactic 511 keV line
• Scalelengths in Dark Matter Halos
• Neutrino clustering in the Milky Way and beyond
• How Baryonic Processes affect Strong Lensing properties of Simulated Galaxy Clusters
• The lens and source of the optical Einstein ring gravitational lens ER 0047-2808
• X-ray Measurements of the Gravitational Potential Profile in the Central Region of the Abell 1060 Cluster of Galaxies
• Mass profile decomposition of the Frontier Fields cluster MACS J0416-02403. Insights on the Dark-Matter inner profile
• A universal velocity distribution of relaxed collisionless structures
• The last 6 Gyr of dark matter assembly in massive galaxies from the Kilo Degree Survey
• Feedback by AGN Jets and Wide-Angle Winds on a Galactic Scale
• Galaxy And Mass Assembly: search for a population of high-entropy galaxy groups
• Delayed star formation in high-redshift stream-fed galaxies
• Synchronized formation of starburst and poststarburst galaxies in merging clusters of galaxies
• The Dark Matter Distribution in the Spiral $NGC3198$ out to 0.22 $R_{vir}$
• Formation of intracluster globular clusters
• The Kinematics and Dark Matter Fractions of TNG50 Galaxies at z=2 from an Observational Perspective
• Contribution of Lensed SCUBA Galaxies to the Cosmic Infrared Background
• A First Look at creating mock catalogs with machine learning techniques
• The different baryonic Tully-Fisher relations at low masses
• Probability of the most massive cluster under non-Gaussian initial conditions
• Probing the existence of a rich galaxy overdensity at z=5.2
• The innate origin of radial and vertical gradients in a simulated galaxy disc
• And In The Darkness Unbind Them: High-Resolution Simulations of Dark Matter Subhalo Disruption in a Milky Way-like Tidal Field
• Weak lensing study of 16 DAFT/FADA clusters: substructures and filaments
• A new model to predict weak-lensing peak counts III. Filtering technique comparisons
• Systematic errors induced by the elliptical power-law model in galaxy-galaxy strong lens modeling
• Satellite quenching was not important for z$\sim$1 clusters: most quenching occurred during infall
• The Phase Space Structure of Dark Matter Halos
• Formation of inflaton halos after inflation
• Formation and Evolution of Early-Type Galaxies. III Star formation history as a function of mass and over-density
• Dark matter subhalos and unidentified sources in the Fermi 3FGL source catalog
• First Constraints on Compact Dark Matter from Fast Radio Burst Microstructure
• Compact groups in theory and practice -- IV. The connection to large-scale structure
• Testing strong lensing subhalo detection with a cosmological simulation
• An almost dark galaxy with the mass of the Small Magellanic Cloud
• Mass distribution in the most X-ray-luminous galaxy cluster RX J1347.5-1145 studied with XMM-Newton
• Realistic fluids as source for dynamically accreting black holes in a cosmological background
• Subaru Weak Lensing survey -- II: Multi-object Spectroscopy and Cluster Masses
• Probing the Galactic Halo with RR Lyrae Stars. II. The Substructures of the Milky Way
• Oxygen, sulfur, and iron radial abundance gradients of classical Cepheids across the Galactic thin disk
• Strong lensing constraints on the velocity dispersion and density profile of elliptical galaxies
• Evolution of dust and molecular hydrogen in the Magellanic System
• Evolution of dark matter microhalos through stellar encounters
• Influence of baryons on the orbital structure of dark matter haloes
• Using wavelets to capture deviations from smoothness in galaxy-scale strong lenses
• Extensions to the halo occupation distribution model for more accurate clustering predictions
• Tidal evolution of dark matter annihilation rates in subhalos
• Inferring the impact of feedback on the matter distribution using the Sunyaev Zel'dovich effect: Insights from CAMELS simulations and ACT+DES data
• Cold Dark Matter in non-Standard Cosmologies, PAMELA, ATIC and Fermi LAT
• Modeling the evolution of infrared galaxies : clustering of galaxies in the Cosmic Infrared Background
• Shapes of Stellar Systems and Dark Halos from Simulations of Galaxy Major Mergers
• Axion minivoids and implications for direct detection
• Near-Infrared Coronal Line Observations of Dwarf Galaxies hosting AGN-driven Outflows
• Casimir effect in Extended Theories of Gravity
• The Formation of Compact Elliptical Galaxies in The Vicinity of A Massive Galaxy: The Role of Ram-pressure Confinement
• A population of galaxy-scale jets discovered using LOFAR
• Herschel-ATLAS/GAMA: SDSS cross-correlation induced by weak lensing
• CODEX Weak Lensing: Concentration of Galaxy Clusters at z ~ 0.5
• The MUSE-Faint survey. II. The dark matter-density profile of the ultra-faint dwarf galaxy Eridanus 2
• Formation of giant globular cluster G1 and the origin of the M31 stellar halo
• Gamma-Ray Constraints on Neutralino Dark Matter Clumps in the Galactic Halo
• Signatures of clumpy dark matter in the global 21 cm background signal
• Modeling Evolution of Galactic Bars at Cosmic Dawn
• The power spectrum amplitude from clusters revisited: σ_8 using simulations with preheating and cooling
• Particle Annihilation in Cold Dark Matter Micropancakes
• Investigating the Uniformity of the Excess Gamma rays towards the Galactic Center Region
• Cosmic Structure Formation with Kinetic Field Theory
• Scalar modes in extended hybrid metric-Palatini gravity: weak field phenomenology
• Probing a dark matter density spike at the Galactic Center
• Strong Lensing by Galaxies
• Probing the Relation Between X-ray-Derived and Weak-Lensing-Derived Masses for Shear-Selected Galaxy Clusters: I. A781
• Brightest galaxies as halo centre tracers in SDSS DR7
• Superradiance of charged black holes embedded in dark matter halos
• Extending the Hyades
• Effects of the complex mass distribution of dark matter halos on weak lensing cluster surveys
• Signatures of Dark Matter Halo Expansion in Galaxy Populations
• The Bound Mass of Substructures in Dark Matter Halos
• Predictably Missing Satellites: Subhalo Abundance in Milky Way-like Halos
• Ram-Pressure Stripping of Galaxies in High-Redshift Clusters and Influence of ICM Heating
• Vlasov-Poisson in 1D for initially cold systems: post-collapse Lagrangian perturbation theory
• Simulating the Spatial Distribution and Kinematics of Globular Clusters within Galaxy Clusters in Illustris
• CFHTLenS: Higher-order galaxy-mass correlations probed by galaxy-galaxy-galaxy lensing
• Static Configurations of Dark Energy and Dark Matter
• Structural properties of non-spherical dark halos in Milky Way and Andromeda dwarf spheroidal galaxies
• Constraints and cosmography of $\Lambda$CDM in presence of viscosity
• The scatter in the galaxy-halo connection: a machine learning analysis
• Could the Fermi-LAT detect gamma-rays from dark matter annihilation in the dwarf galaxies of the Local Group?
• Kinematics and Mass Profile of AWM 7
• Rising Jet-Inflated Bubbles in Clusters of Galaxies
• Confronting the Galactic Center Gamma Ray Excess With a Light Scalar Dark Matter
• Three-dimensional Mapping of CDM Substructure at Submillimeter Wavelengths
• Constraining Decaying Dark Matter with Fermi LAT Gamma-rays
• Wormholes supported by phantom energy from Shan-Chen cosmological fluids
• SMBH Seeds from Dissipative Dark Matter
• Evolution of Dark Matter Halos and their Radio Emissions
• Confronting fuzzy dark matter with the rotation curves of nearby dwarf irregular galaxies
• Hobby-Eberly Telescope Observations of the Dark Halo in NGC 821
• Improved strong lensing modelling of galaxy clusters using the Fundamental Plane: Detailed mapping of the baryonic and dark matter mass distribution of Abell S1063
• Modelling the Milky Way's globular cluster system
• Orbital ingredients for cooking X-structures in edge-on galaxies
• Relative clustering and the joint halo occupation distribution of red-sequence and blue-cloud galaxies in COMBO-17
• Stellar Stream and Halo Structure in the Andromeda Galaxy From a Subaru/Hyper Suprime-Cam Survey
• Cosmic-Ray Positrons Strongly Constrain Leptophilic Dark Matter
• Stellar-to-halo mass relation of cluster galaxies
• Calibrating the Galaxy Halo - Black Hole Relation Based on the Clustering of Quasars
• Inferring the concentration of dark matter subhalos perturbing strongly lensed images
• Impact of dark matter subhalos on extended HI disks of galaxies: Possible formation of HI fine structures and stars
• Mass-to-light ratios from the fundamental plane of spiral galaxy disks
• Constraints on self-interacting Q-ball dark matter
• Constraining H0 from Chandra Observations of Q0957+561
• Disentangling dark sector models using weak lensing statistics
• Radio signatures from encounters between Neutron Stars and QCD-Axion Minihalos around Primordial Black Holes
• Simulation tests of galaxy cluster constraints on chameleon gravity
• Imprints of Chameleon f(R) Gravity on Galaxy Rotation Curves
• Lagrangian cosmological perturbation theory at shell-crossing
• The mass-concentration relationship of virialized halos and its impact on cosmological observables
• Probing a massive radio galaxy with gravitational lensing
• CLUMP-3D: Three-dimensional Shape and Structure of 20 CLASH Galaxy Clusters from Combined Weak and Strong Lensing
• The Dearth of Chemically Enriched Warm-Hot Circumgalactic Gas
• Tidal Tracks and Artificial Disruption of Cold Dark Matter Halos
• MaNGA DynPop -- III. Stellar dynamics versus stellar population relations in 6000 early-type and spiral galaxies: Fundamental Plane, mass-to-light ratios, total density slopes, and dark matter fractions
• Quasar Clustering in Cosmological Hydrodynamic Simulations: Evidence for mergers
• An artificial neural network to discover Hypervelocity stars: Candidates in Gaia DR1/TGAS
• The Angular Momentum Distribution within Halos in Different Dark Matter Models
• Constraining warm dark matter with 21 cm line fluctuations due to minihalos
• Constraining the inner density slope of massive galaxy clusters
• Comparison between the Logotropic and $\Lambda$CDM models at the cosmological scale
• Neutrino Halos in Clusters of Galaxies and their Weak Lensing Signature
• Revisiting dynamical friction: the role of global modes and local wakes
• THESEUS Insights into ALP, Dark Photon and Sterile Neutrino Dark Matter
• N-Body Code with Adaptive Mesh Refinement
• Abell 2744: Too much substructure for Lambda CDM?
• The Observed Mass Profiles of Dark Halos and The Formation Epochs of Galaxies
• Do active galactic nuclei convert dark matter into visible particles?
• Mass Calibration of the CODEX Cluster Sample using SPIDERS Spectroscopy -- I. The Richness-Mass Relation
• Investigating Cluster Astrophysics and Cosmology with Cross-Correlation of the Thermal Sunyaev-Zel'dovich Effect and Weak Lensing
• The Sunyaev-Zel'dovich effect in WMAP data
• $\Lambda$CDM Predictions for the Satellite Population of M33
• Extracting the Subhalo Mass Function from Strong Lens Images with Image Segmentation
• The interstellar medium distribution, gas kinematics, and system dynamics of the far-infrared luminous quasar SDSS J2310+1855 at $z=6.0$
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the growth rate of structure from the small-scale clustering of the luminous red galaxy sample
• Clues to the origin of Fermi Bubbles from OVIII/OVII line ratio
• Constraints on the Mass, Concentration, and Nonthermal Pressure Support of Six CLASH Clusters from a Joint Analysis of X-ray, SZ, and Lensing Data
• Gravitational redshift and asymmetric redshift-space distortions for stacked clusters
• Cusp or core? Revisiting the globular cluster timing problem in Fornax
• On the Cusp around Central Black Holes in Luminous Elliptical Galaxies
• Refining the M_BH-V_c scaling relation with HI rotation curves of water megamaser galaxies
• A Brief Review on Dark Matter Annihilation Explanation for $e^{\pm }$ Excesses in Cosmic Ray
• Galaxy orbits and the intracluster gas temperature in clusters
• MOND and the Universal Rotation Curve: similar phenomenologies
• Structural and dynamical modeling of WINGS clusters. I. The distribution of cluster galaxies of different morphological classes within regular and irregular clusters
• A Formation Scenario for the Disk of Satellites: Accretion of Satellites during Mergers
• Evidence for inhomogeneous reionization in the local Universe from metal-poor globular cluster systems
• A cosmological context for compact massive galaxies
• Constraints on light dark matter particles using white dwarf stars
• Higgs funnel region of SUSY dark matter for small $\tan \beta$ and renormalization group effects on pseudoscalar Higgs boson with scalar mass non-universality
• Under the sword of Damocles: plausible regeneration of dark matter cusps at the smallest galactic scales
• Gravitational Lensing by a Compound Population of Halos: Standard Models
• A hydrodynamical study of outflows in starburst galaxies with different driving mechanisms
• Toward a Minimum Branching Fraction for Dark Matter Annihilation into Electromagnetic Final States
• Constraining Primordial Magnetic Fields with Future Cosmic Shear Surveys
• Lyman Alpha and MgII as Probes of Galaxies and their Environments
• New XMM-Newton observation of the Phoenix cluster: properties of the cool core
• The polytropic approximation and X-ray scaling relations: constraints on gas and dark matter profiles for galaxy groups and clusters
• The many reasons that the rotation curves of low-mass galaxies can fail as tracers of their matter distributions
• A dynamics-based density profile for dark haloes -- II. Fitting function
• The cosmic UV background and the beginning and end of star formation in simulated field dwarf galaxies
• Modeling the Phase-Space Distribution around Massive Halos
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• Impact of dark matter galactic halo models on wormhole geometry within $f(Q,T)$ gravity
• Fermionic Semi-Annihilating Dark Matter
• Superfluid Dark Matter around Black Holes
• Long-term orbital evolution of Galactic satellites and the effects on their star formation histories
• The Star Cluster Population of the Collisional Ring Galaxy NGC 922
• Two-portal Dark Matter
• Constraining Logotropic Unified Dark Energy Models
• A comparison of the strong lensing properties of the Sersic and the NFW profiles
• Origin of structural and kinematical properties of the Small Magellanic Cloud
• Kaluza-Klein Dark Matter, Electrons and Gamma Ray Telescopes
• Statistical properties of the dark matter haloes of dwarf galaxies and correlations with the environment
• Possibility of the Traversable Wormholes in the Galactic Halos within $4D$ Einstein-Gauss-Bonnet Gravity
• Orbital Torus Imaging: Using Element Abundances to Map Orbits and Mass in the Milky Way
• Dynamical constraints on the dark matter distribution of the Sculptor dwarf spheroidal from stellar proper motions
• On the orbital and internal evolution of cluster galaxies
• Cosmological Structure Formation in Decaying Dark Matter Models
• Virial shocks are suppressed in cosmic ray-dominated galaxy halos
• Ly-alpha Clouds Associated with Pop III Objects in Cold Dark Matter Models
• Environmental Quenching and Galactic Conformity in the Galaxy Cross-Correlation Signal
• Upward muon signals at neutrino detectors as a probe of dark matter properties
• Fast Weak Lensing Simulations with Halo Model
• Probing Hierarchical Clustering by Scale-Scale Correlations of Wavelet Coefficients
• Feedback in AGN heating of galaxy clusters
• Cosmic Axion Force
• Formation of the Andromeda Giant Stream: Asymmetric Structure and Disc Progenitor
• Testing Dark Matter and Modifications to Gravity using Local Milky Way Observables
• Fermi-LAT Sensitivity to Dark Matter Annihilation in Via Lactea II Substructure
• MOND and IMF variations in early-type galaxies from $ATLA{S}^{3D}$
• Euclid preparation. XXXII. Evaluating the weak lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
• The Origin of Extended Disk Galaxies at z=2
• The WIMP capture process for dark stars in the early universe
• Effective field theory interpretation of searches for dark matter annihilation in the Sun with the IceCube Neutrino Observatory
• The mass function dependence on the dynamical state of dark matter haloes
• Measuring galaxy cluster masses with CMB lensing using a Maximum Likelihood estimator: Statistical and systematic error budgets for future experiments
• Hydrodynamic simulations of the triaxial bulge of M31
• Groups in the Millennium Simulation and in SDSS DR7
• Mass-gap extreme mass ratio inspirals
• Image segmentation for analyzing galaxy-galaxy strong lensing systems
• Can the dark matter halo be a collisionless ensemble of axion stars?
• Photoionisation and Heating of a Supernova Driven, Turbulent, Interstellar Medium
• GA-NIFS: Multi-phase analysis of a star-forming galaxy at $z\sim 5.5$
• Dark Matter And The Habitability of Planets
• Cusps and Triaxiality
• Feedback, scatter and structure in the core of the PKS 0745-191 galaxy cluster
• The First Direct Search for Inelastic Boosted Dark Matter with COSINE-100
• Density Profiles of Collisionless Equilibria. I. Spherical Isotropic Systems
• Discovery of a disrupting open cluster far into the Milky Way halo: a recent star formation event in the leading arm of the Magellanic stream?
• X-ray Radiation from the Annihilation of Dark Matter at the Galactic Center
• The effects of a disc field on the bulge surface brightness
• The spatial distribution of Milky Way satellites, gaps in streams and the nature of dark matter
• Is the compact object associated with HESS J1731-347 a strange quark star?
• SARCS strong-lensing galaxy groups: II - mass-concentration relation and strong-lensing bias
• Effects of early dark energy on strong cluster lensing
• Galaxy And Mass Assembly (GAMA): The effect of galaxy group environment on active galactic nuclei
• Magnetic fields and the outer rotation curve of M31
• Non-universality of halo profiles and implications for dark matter experiments
• The impact of baryonic physics on the abundance, clustering, and concentration of halos
• Heavy decaying dark matter at future neutrino radio telescopes
• $\text{matryoshka}$: Halo Model Emulator for the Galaxy Power Spectrum
• Bars formed in galaxy merging and their classification with deep learning
• Probing galaxy bias and intergalactic gas pressure with KiDS Galaxies-tSZ-CMB lensing cross-correlations
• Sensitivity of Neutrino Mass Experiments to the Cosmic Neutrino Background
• On Physical Scales of Dark Matter Halos
• Testing MONDian Dark Matter with Galactic Rotation Curves
• Dynamical self-friction: how mass loss slows you down
• Stacked Weak Lensing Mass Calibration: Estimators, Systematics, and Impact on Cosmological Parameter Constraints
• Dark matter detection in the BMSSM
• Mask Effects on Cosmological Studies with Weak Lensing Peak Statistics
• Dark Matter and LHC: What is the Connection?
• Comparing X-ray and Dynamical Mass Profiles in the Early-Type Galaxy NGC 4636
• Including massive neutrinos in thermal Sunyaev Zeldovich power spectrum and cluster counts analyses
• The distribution of satellites around massive galaxies at 1<z<3 in ZFOURGE/CANDELS: dependence on star formation activity
• Weak-lensing-inferred scaling relations of galaxy clusters in the RCS2: mass-richness, mass-concentration, mass-bias, and more
• Violent Buckling Benefits Galactic Bars
• The orbital PDF: general inference of the gravitational potential from steady-state tracers
• CFHTLenS: Weak lensing constraints on the ellipticity of galaxy-scale matter haloes and the galaxy-halo misalignment
• A Multi-frequency analysis of dark matter annihilation interpretations of recent anti-particle and gamma-ray excesses in cosmic structures
• Strong gravitational lensing: why no central black holes?
• Search for Gamma-ray Spectral Lines from Dark Matter Annihilation up to 100 TeV towards the Galactic Center with MAGIC
• Gravitational Flexion by Elliptical Dark Matter Haloes
• Dark Matter in Galaxies: evidences and challenges
• Vector disformal transformation of generalized Proca theory
• Entropy principle and complementary second law of thermodynamics for self-gravitating systems
• Probing dark energy models with extreme pairwise velocities of galaxy clusters from the DEUS-FUR simulations
• Complex structures in galaxy cluster fields: implications for gravitational lensing mass models
• Dark Matter Structures In The Deep Lens Survey
• A Survey of Satellite Galaxies around NGC 4258
• The Influence of Concentration and Dynamical State on Scatter in the Galaxy Cluster Mass-Temperature Relation
• Completely dark galaxies: their existence, properties, and strategies for finding them
• Ursa Major III/UNIONS 1: the darkest galaxy ever discovered?
• Tests of Gravity with Galaxy Clusters
• The portrait of Malin 2: a case study of a giant low surface brightness galaxy
• Decaying Superheavy Dark Matter and Subgalactic Structure of the Universe
• Self-consistent massive disks in triaxial dark matter halos
• On the fragmentation of filaments in a molecular cloud simulation
• The evolution of galaxy groups and of galaxies therein
• N-body simulations with a cosmic vector for dark energy
• Dark Matter from a gas of wormholes
• Searching For Dark Matter with Neutrino Telescopes
• Primordial Black Hole Merger Rate in Ellipsoidal-Collapse Dark Matter Halo Models
• H-ATLAS/GAMA: Magnification Bias Tomography. Astrophysical constraints above $\sim 1$ arcmin
• A low upper mass limit for the central black hole in the late-type galaxy NGC 4414
• Gravitational Collapse in One Dimension
• Constraining the halo mass function with observations
• Assessing the impact of bulk and shear viscosities on large scale structure formation
• Possible smoking-gun evidence for initial mass segregation in re-virialized post-gas expulsion globular clusters
• Towards an improved model of self-interacting dark matter haloes
• Calibrating Cluster Number Counts with CMB lensing
• Cross-correlation of DES Y3 lensing and ACT/$Planck$ thermal Sunyaev Zel'dovich Effect I: Measurements, systematics tests, and feedback model constraints
• Prompt cusps and the dark matter annihilation signal
• Constrained Cosmological Simulations of Dark Matter Halos
• Wide-Field Optical Spectroscopy of Abell 133: A Search for Filaments Reported in X-ray Observations
• A Swing of the Pendulum: The Chemodynamics of the Local Stellar Halo Indicate Contributions from Several Radial Merger Events
• Galaxy cluster's rotation
• p-wave Annihilating Dark Matter from a Decaying Predecessor and the Galactic Center Excess
• A Malin 1 'cousin' with counter-rotation: internal dynamics and stellar content of the giant low surface brightness galaxy UGC 1922
• Theoretical predictions for dark matter detection in dwarf irregular galaxies with gamma rays
• Ultra High Energy Cosmic Rays from Cosmological Relics
• Testing the Halo Model Against the SDSS Photometric Survey
• SMART: A new implementation of Schwarzschild's Orbit Superposition technique for triaxial galaxies and its application to an N-body merger simulation
• The Three Hundred Project: Substructure in hydrodynamical and dark matter simulations of galaxy groups around clusters
• What Sets the Slope of the Molecular Kennicutt-Schmidt Relation?
• Dark Matter Bars in Spinning Halos
• Anisotropies in the Diffuse Gamma-Ray Background from Dark Matter with Fermi LAT: a closer look
• Shapes of Milky-Way-Mass Galaxies with Self-Interacting Dark Matter
• Dark matter profiles of SPARC galaxies: a challenge to fuzzy dark matter
• Galactic rotation curves in brane world models
• Lensing constraints on ultradense dark matter halos
• Origin of chemical and dynamical properties of the Galactic thick disk
• Search for cold and hot gas in the ram pressure stripped Virgo dwarf galaxy IC3418
• A multi-wavelength strong lensing analysis of baryons and dark matter in the dynamically active cluster AC 114
• Source Ellipticity and the Statistics of Lensed Arcs
• What to expect from dynamical modelling of galactic haloes II: the spherical Jeans equation
• Simulations of core formation for frequent dark matter self-interactions
• Axions: From Magnetars and Neutron Star Mergers to Beam Dumps and BECs
• SHAPing the Gas: Understanding Gas Shapes in Dark Matter Haloes with Interpretable Machine Learning
• Substructure at High Speed II: The Local Escape Velocity and Milky Way Mass with Gaia DR2
• The Effects of Varying Cosmological Parameters on Halo Substructure
• Constraining the dark matter contribution of $\gamma$ rays in Cluster of galaxies using Fermi-LAT data
• Constraints on decaying dark matter from weak lensing and cluster counts
• Stellar Signatures of AGN Jet Triggered Star Formation
• Is Sextans dwarf galaxy in a scalar field dark matter halo?
• A model for the metallicity evolution of damped Lyman-alpha systems
• Astrophysics of Bertrand Space-times
• Cosmological information content in redshift-space power spectrum of SDSS-like galaxies in the quasi-nonlinear regime up to $k=0.3h$Mpc${}^{-1}$
• The lensing properties of subhaloes in massive elliptical galaxies in sterile neutrino cosmologies
• Evolution of star cluster systems in isolated galaxies: first results from direct $N$-body simulations
• Discovery of a Strong Lensing Galaxy Embedded in a Cluster at z = 1.62
• Orbital support and evolution of flat profiles of bars (shoulders)
• Collisions between Dark Matter Confined High Velocity Clouds and Magnetized Galactic Disks: The Smith Cloud
• Finslerian MOND vs. observations of Bullet Cluster 1E0657-558
• Confronting the Moduli-Induced LSP Problem
• Star-formation driven outflows in local dwarf galaxies as revealed from [CII] observations by Herschel
• The Core-Cusp Problem Revisited: ULDM vs. CDM
• Cosmological Imprints of Pre-Inflationary Particles
• CMSSM Spectroscopy in light of PAMELA and ATIC
• Formation of the off-center bar in the Large Magellanic Cloud: A collision with a dark satellite ?
• Formation of Wormholes by Dark Matter in the Galaxy Dragonfly 44
• Assessing the Importance of Noise from Thermal Sunyaev-Zel{'}dovich Signals for CMB Cluster Surveys and Cluster Cosmology
• The existence and detection of optically dark galaxies by 21cm surveys
• Sub-GeV galactic cosmic-ray antiprotons from primordial black holes in the Randall-Sundrum braneworld
• Alas, the dark matter structures were not that trivial
• Core or cusps: The central dark matter profile of a redshift one strong lensing cluster with a bright central image
• Infrared Emission from Intracluster Dust Grains and Constraints on Dust Properties
• The Globular Cluster System of NGC 6822
• Disk Assembly and the M_BH-sigma Relation of Supermassive Black Holes
• Fornax globular cluster distributions: implications for the cusp-core problem
• The origin of the relation between metallicity and size in star-forming galaxies
• Dark Stars: Improved Models and First Pulsation Results
• Dark Matter Decay to a Photon and a Neutrino: the Double Monochromatic Smoking Gun Scenario
• Splashback radius of nonspherical dark matter halos from cosmic density and velocity fields
• Study of the Gamma-ray Spectrum from the Galactic Center in view of Multi-TeV Dark Matter Candidates
• The observable properties of galaxy accretion events in Milky Way-like galaxies in the FIRE-2 cosmological simulations
• Breaking the Vainshtein screening in clusters of galaxies
• Power Spectrum Normalisation and the Non-Gaussian Halo Model
• Estimating the Dark Halo Mass from the Relative Thickness of Stellar Disks
• The probability distribution function of the SZ power spectrum: an analytical approach
• Adiabatically compressed wave dark matter halo and intermediate-mass ratio inspirals
• Spin Flips - II. Evolution of dark matter halo spin orientation, and its correlation with major mergers
• Mass-concentration relation of clusters of galaxies from CFHTLenS
• The Turn-Down of the Baryonic Tully-Fisher Relation and Changing Baryon Fractions at Low Galaxy Masses
• Transient Radio Lines from Axion Miniclusters and Axion Stars
• Globular cluster formation with multiple stellar populations: self-enrichment in fractal massive molecular clouds
• Exploring the Physical Properties of the Cool Circumgalactic Medium with a Semi-Analytic Model
• Galaxy Formation and Evolution. II. Energy Balance, Star Formation and Feed-back
• Effects of the halo concentration distribution on strong-lensing optical depth and X-ray emission
• Soliton Merger Rates and Enhanced Axion Dark Matter Decay
• Decaying Dark Matter and the Deficit of Dwarf Haloes
• The Interplay of Kinetic and Radiative Feedback in Galaxy Clusters
• Do the stellar populations of the brightest two group galaxies depend on the magnitude gap?
• Tests of Gravity Theories Using Supermassive Black Holes
• The Dark Side of 4321
• Tracing the gravitational potential using cosmic voids
• Evolution of compact and fossil groups of galaxies from semi-analytical models of galaxy formation
• Formation of Dark Matter Torii Around Supermassive Black Holes Via The Eccentric Kozai-Lidov Mechanism
• Gauge Mediated Supersymmetry Breaking and Multi-TeV Gamma-Rays from the Galactic Center
• The GOGREEN survey: the internal dynamics of clusters of galaxies at redshift 0.9-1.4
• Clustering of the IR Background Light with Spitzer: Contribution from Resolved Sources
• Optimizing weak lensing mass estimates for cluster profile uncertainty
• One Thousand and One Clusters: Measuring the Bulk Flow with the Planck ESZ and X-Ray Selected Galaxy Cluster Catalogs
• GOTHIC: Gravitational oct-tree code accelerated by hierarchical time step controlling
• Gamma-Ray Emission from Molecular Clouds Generated by Penetrating Cosmic Rays
• The Halo Void (Dust) Model of Large Scale Structure
• Models of rotating coronae
• Subaru weak-lensing measurement of a z = 0.81 cluster discovered by the Atacama Cosmology Telescope Survey
• A Very Large (${\theta }_E\gtrsim 40$") Strong Gravitational Lens Selected with the Sunyaev-Zel'dovich Effect: PLCK G287.0+32.9 ($z$ = 0.38)
• The stretching of Hercules
• Stellar Mass to Halo Mass Scaling Relation for X-ray Selected Low Mass Galaxy Clusters and Groups out to Redshift $z\approx 1$
• The velocity anisotropy - density slope relation
• Intrinsic Alignments and Splashback Radius of Dark Matter Halos from Cosmic Density and Velocity Fields
• Dark matter in galaxies and growth of giant black holes
• On the relevance of chaos for halo stars in the Solar Neighbourhood
• Influence of AGN jets on the magnetized ICM
• The Integrated Sachs-Wolfe Signal from BOSS Super-Structures
• A Search for Dark Matter Lines at the Galactic Center with 14 Years of Fermi Data
• Probing Boson Stars with Extreme Mass Ratio Inspirals
• Improved Constraints on the Gravitational Lens Q0957+561. I. Weak Lensing
• Cosmological Parameter Determination in Free-Form Strong Gravitational Lens Modeling
• The 130 GeV gamma-ray line and generic dark matter model building constraints from continuum gamma rays, radio and antiproton data
• Dark matter searches
• Detection of universality of dark matter profile from Subaru weak lensing measurements of 50 massive clusters
• Spacetime metrics and ringdown waveforms for galactic black holes surrounded by a dark matter spike
• Effect of inhomogeneities on high precision measurements of cosmological distances
• On the early evolution of Local Group dwarf galaxy types: star formation and supernova feedback
• The Scientific Reach of Multi-Ton Scale Dark Matter Direct Detection Experiments
• Metal-mass-to-light ratios of the Perseus cluster out to the virial radius
• Consequences of the lack of azimuthal freedom in the modeling of lensing galaxies
• The Atacama Cosmology Telescope: High-Resolution Sunyaev-Zel'dovich Array Observations of ACT SZE-selected Clusters from the Equatorial Strip
• Might we eventually understand the origin of the dark matter velocity anisotropy?
• Dark Matter Search in Space: Combined Analysis of Cosmic Ray Antiproton-to-Proton Flux Ratio and Positron Flux Measured by AMS-02
• Mapping Dark Matter in the Milky Way using Normalizing Flows and Gaia DR3
• Constraining the properties of gaseous halos via cross-correlations of upcoming galaxy surveys and thermal Sunyaev-Zel'dovich maps
• Linear Sigma Dark Matter
• Wormholes with a barotropic equation of state admitting a one-parameter group of conformal motions
• The Accretion and Cooling of Preheated Gas in Dark Matter Halos
• Probing dark matter crests with white dwarfs and IMBHs
• Constraints via the Event Horizon Telescope for Black Hole Solutions with Dark Matter under the Generalized Uncertainty Principle Minimal Length Scale Effect
• Galactic Dark Matter Population as the Source of Neutrino Masses
• Steepened inner density profiles of group galaxies via interactions: An N-body analysis
• Friends-of-Friends Groups and Clusters in the 2SLAQ Catalogue
• Where do galaxies end? Comparing measurement techniques of hydrodynamic-simulation galaxies' integrated properties
• Massive black holes at high redshifts from superconducting cosmic strings
• Clues on Regularity in the Structure and Kinematics of Elliptical Galaxies from Self-consistent Hydrodynamical Simulations: the Dynamical Fundamental Plane
• When was the Large Magellanic Cloud accreted onto the Galaxy ?
• Galactic fountains and outflows in star forming dwarf galaxies: ISM expulsion and chemical enrichment
• The Origin of Large-scale HI structures in the Magellanic Bridge
• Kinematics of the Tucana Dwarf Galaxy: An Unusually Dense Dwarf in the Local Group
• Fuzzy dark matter black holes and droplets
• Baryon Pasting Algorithm: Halo-based and Particle-based Pasting Methods
• Comprehensive Constraints on a Spin-3/2 Singlet Particle as a Dark Matter Candidate
• The effect of tides on the Sculptor dwarf spheroidal galaxy
• The Milky Way's bar structural properties from gravitational waves
• Metal diffusion in smoothed particle hydrodynamics simulations of dwarf galaxies
• The Power of Halometry
• The Sloan Nearby Cluster Weak Lensing Survey
• Constraints on AGN feedback from its Sunyaev-Zel'dovich imprint on the cosmic background radiation
• Measuring the hydrostatic mass bias in galaxy clusters by combining Sunyaev-Zel'dovich and CMB lensing data
• Separation of the visible and dark matter in the Einstein ring LBG J213512.73-010143
• Spitzer, Gaia, and the Potential of the Milky Way
• The flat density profiles of massive, and relaxed galaxy clusters
• Semi-annihilating $Z_3$ Dark Matter for XENON1T Excess
• Using LISA-like Gravitational Wave Detectors to Search for Primordial Black Holes
• Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
• Projected Axis Ratios of Galaxy Clusters in the Horizon-AGN Simulation: Impact of Baryon Physics and Comparison with Observations
• Weak-lensing calibration of a stellar mass-based mass proxy for redMaPPer and Voronoi Tessellation clusters in SDSS Stripe 82
• Close Encounters of Wide Binaries Induced by the Galactic Tide: Implications for Stellar Mergers and Gravitational-Wave Sources
• Dark-matter dynamical friction versus gravitational-wave emission in the evolution of compact-star binaries
• Constraints on the dark matter annihilation from Fermi-LAT observation of M31
• Baryons Shaping Dark Matter Haloes
• Angular Momentum of Early and Late Type Galaxies: Nature or Nurture?
• A new methodology to test galaxy formation models using the dependence of clustering on stellar mass
• Light on curved backgrounds
• The Effective Field Theory of Large-Scale Structure and Multi-tracer
• The Effects of the Peak-Peak Correlation on the Peak Model of Hierarchical Clustering
• Looking for a heavy wino LSP in collider and dark matter experiments
• The prediction of rotation curves in gas-dominated dwarf galaxies with modified dynamics
• Signatures of primordial black hole dark matter at DUNE and THEIA
• The orbital PDF: the dynamical state of Milky Way sized haloes and the intrinsic uncertainty in the determination of their masses
• Star formation and environment in clusters up to z~2.2
• Weak Lensing Peak Finding: Estimators, Filters, and Biases
• An investigation of open clusters Berkeley 68 and Stock 20 using CCD UBV and Gaia DR3 data
• The dichotomy of dark matter fraction and total mass density slope of galaxies over five dex in mass
• Updated Constraints and Future Prospects on Majoron Dark Matter
• Global anisotropy of arrival directions of ultra-high-energy cosmic rays: capabilities of space-based detectors
• TDCOSMO VI: Distance Measurements in Time-delay Cosmography under the Mass-sheet transformation
• Gravitino Dark Matter and Neutrino Masses in Partial Split Supersymmetry
• Prospects for detecting gravitational waves from eccentric subsolar mass compact binaries
• Adaptive mesh refinement simulations of collisional ring galaxies: effects of the interaction geometry
• The Lack of Non-Thermal Motions in Galaxy Cluster Cores
• The ESO Nearby Abell Cluster Survey IX. The morphology-radius and morphology-density relations in rich galaxy clusters
• Weak-lensing mass bias in merging galaxy clusters
• The error budget of the Dark Flow measurement
• The Galactic globular cluster system as a fossil record of reionization
• A robust estimator of mutual information for deep learning interpretability
• Weak Lensing Peaks in Simulated Light-Cones: Investigating the Coupling between Dark Matter and Dark Energy
• On the Cosmic Web Elongation in Fuzzy Dark Matter Cosmologies: Effects on Density Profiles, Shapes and Alignments of Halos
• Spin-axion coupling
• First Identification of a CMB Lensing Signal Produced by $1.5$ Million Galaxies at $z\sim$4: Constraints on Matter Density Fluctuations at High Redshift
• A Detection of CMB-Cluster Lensing using Polarization Data from SPTpol
• Radio emission from dark matter annihilation in the Large Magellanic Cloud
• Detailed SZ study of 19 LoCuSS galaxy clusters: masses and temperatures out to the virial radius
• Momentum-driven feedback and the Mass-sigma relation in non-isothermal galaxies
• The 400d Galaxy Cluster Survey weak lensing programme: II: Weak lensing study of seven clusters with MMT/Megacam
• Excitation of vertical breathing motion in disc galaxies by tidally-induced spirals in fly-by interactions
• Boxes, Boosts, and Energy Duality: Understanding the Galactic-Center Gamma-Ray Excess through Dynamical Dark Matter
• Early Observations of the MHONGOOSE Galaxies: Getting Ready for MeerKAT
• The global mass - to - light ratio of SLACS lenses
• Hunting for Dark Matter and New Physics with GECCO
• Using the Multi-Object Adaptive Optics demonstrator RAVEN to observe metal-poor stars in and towards the Galactic Centre
• Light versus dark in strong-lens galaxies: Dark matter haloes that are rounder than their stars
• Modeling the Ages and Metallicities of Early-Type Galaxies in Fundamental Plane Space
• The Most Distant Stars in the Milky Way
• Indirect Detection of eV Dark Matter via Infrared Spectroscopy
• Gravitational Lensing by Dark Matter Halos with Non-universal Density Profiles
• Wave Dark Matter and Ultra Diffuse Galaxies
• Dark impact and galactic star formation: Origin of the Gould belt
• The halo mass function and inner structure of ETHOS haloes at high redshift
• Population III X-ray Binaries and their Impact on the Early Universe
• Revisiting the Role of M31 in the Dynamical History of the Magellanic Clouds
• LoCuSS: The splashback radius of massive galaxy clusters and its dependence on cluster merger history
• Scalar field haloes as gravitational lenses
• The Atacama Cosmology Telescope: Weighing distant clusters with the most ancient light
• Weak Lensing Analysis of CODEX Clusters using Dark Energy Camera Legacy Survey : Mass-Richness Relation
• Investigating the effect of Milky Way dwarf spheroidal galaxies extension on dark matter searches with Fermi-LAT data
• Rotation Curves of Galaxies by Fourth Order Gravity
• Inference from the small scales of cosmic shear with current and future Dark Energy Survey data
• Gravitational waves and neutrino oscillations in Chern-Simons axion gravity
• Dark matter concentrations in galactic nuclei according to polytropic models
• Systematics in lensing reconstruction: Dark matter rings in the sky?
• The Galactic potential and the asymmetric distribution of hypervelocity stars
• Stellar Bars in Counter-Rotating Dark Matter Halos: The Role of Halo Orbit Reversals
• Dark and luminous mass components of Omega Centauri with stellar kinematics
• Azimuthal asymmetry in cosmic-ray boosted dark matter flux
• The impact of cored density profiles on the observable quantities of dwarf spheroidal galaxies
• Predicting the dark matter velocity distribution in galactic structures: tests against hydrodynamic cosmological simulations
• A minor merger scenario for the ultraluminous X-ray source ESO 243-49 HLX-1
• On the evolution of cooling cores in X-ray galaxy clusters
• Dynamical signatures of infall around galaxy clusters: a generalized Jeans equation
• GalWeight Application: A publicly-available catalog of dynamical parameters of 1,800 galaxy clusters from SDSS-DR13, ($GalWCat19$)
• The orbital phase space of contracted dark matter halos
• Impact of the Galactic Disk and Large Magellanic Cloud on the Trajectories of Hypervelocity Stars Ejected from the Galactic Center
• Two-Phase ICM in the Central Region of the Rich Cluster of Galaxies Abell 1795: A Joint Chandra, XMM-Newton, and Suzaku View
• Multiwavelength investigations of co-evolution of bright custer galaxies
• Implications of the XENON1T Excess on the Dark Matter Interpretation
• K-mouflage effects on clusters of galaxies
• Cosmology with Long-Lived Charged Massive Particles
• Revisiting the Fermionic Dark Matter Absorption on Electron Target
• Dynamics of Kicked and Accelerated Massive Black Holes in Galaxies
• Mass modelling of a superthin galaxy, FGC1540
• The origin of the diffuse non-thermal X-ray and radio emission in the Ophiuchus cluster of galaxies
• Cosmological and idealized simulations of dark matter haloes with velocity-dependent, rare and frequent self-interactions
• Chemical and Photometric Evolution of the Local Group Galaxy NGC 6822 in a Cosmological Context
• A Lyman limit system associated with galactic winds
• Self-similar collapse and the structure of dark matter halos: A fluid approach
• Gamma rays from the neutralino dark matter annihilations in the Milky Way substructures
• A Systematic Study of Hidden Sector Dark Matter: Application to the Gamma-Ray and Antiproton Excesses
• The origin and formation of cuspy density profiles through violent relaxation of stellar systems
• Constraints on the Galactic Centre environment from Gaia hypervelocity stars
• Gaia-DR2 extended kinematical maps. Part III: Rotation curves analysis, dark matter, and Modified Newtonian dynamics tests
• Establishing the Non-Primordial Origin of Black Hole-Neutron Star Mergers
• Satellite mass functions and the faint end of the galaxy mass-halo mass relation in LCDM
• Gas rotation in galaxy clusters: signatures and detectability in X-rays
• Primordial pollution of globular clusters within their host dwarfs embedded in dark matter halos at high redshifts
• Forming stars on a viscous timescale: the key to exponential stellar profiles in disk galaxies?
• Astrophysical limitations to the identification of dark matter: indirect neutrino signals vis-a-vis direct detection recoil rates
• The Uchuu-UniverseMachine dataset: Galaxies in and around Clusters
• The behaviour of shape and velocity anisotropy in dark matter haloes
• Ultra-High-Energy Neutrinos from Primordial Black Holes
• On the generation of asymmetric warps in disk galaxies
• Galaxy Flybys: Evolution of the Bulge, Disk, and Spiral Arms
• An Ultimate Target for Dark Matter Searches
• Accelerating Earth-Bound Dark Matter
• ALMA observations of lensed Herschel sources : Testing the dark-matter halo paradigm
• Orbital roulette: a new method of gravity estimation from observed motions
• Embedding globular clusters in dark matter minihalos solves the cusp-core and timing problems in the Fornax dwarf galaxy
• The oblateness of the Milky Way dark matter halo from the stellar streams of NGC 3201, M68, and Palomar 5
• Probing Energetic Light Dark Matter with Multi-Particle Tracks Signatures at DUNE
• A critical analysis of high-redshift, massive galaxy clusters: I
• The Gamma Ray Detection Capabilities of the Alpha Magnetic Spectrometer
• The Dark Matter Haloes of Chandra X-ray Galaxy Clusters and Baryons Effect
• Polarized image of a rotating black hole surrounded by a cold dark matter halo
• The halo mass function of late-type galaxies from HI kinematics
• Cosmic rays through the Higgs portal
• Evolution of Group Galaxies from the First Red-Sequence Cluster Survey
• A dynamo amplifies the magnetic field of a Milky-Way-like galaxy
• Illuminating Dark Matter Halo Density Profiles Without Subhaloes
• Core mass -- halo mass relation of bosonic and fermionic dark matter halos harbouring a supermassive black hole
• Suppressed radio emission in supercluster galaxies: enhanced ram pressure in merging clusters?
• From linear to non-linear scales: analytical and numerical predictions for the weak lensing convergence
• Luminosity functions consistent with a pulsar-dominated Galactic Center Excess
• Mass distribution in rotating thin-disk galaxies according to Newtonian dynamics
• Impact of Dark Matter Substructure on the Matter and Weak Lensing Power Spectra
• Extracting the Dark Matter Profile of a Relaxed Galaxy Cluster
• Prompt cusp formation from the gravitational collapse of peaks in the initial cosmological density field
• Mass distribution and orbital anisotropy of early-type galaxies: constraints from the Mass Plane
• A Model of Metastable EeV Dark Matter
• Diffuse Radio Emission from Galaxy Clusters in the LOFAR Two-metre Sky Survey Deep Fields
• Tidal effects of dark matter halo around a galactic black hole
• Probing Cosmology and Cluster Astrophysics with Multi-Wavelength Surveys I. Correlation Statistics
• Constraining interacting dark energy models with the halo concentration-mass relation
• Evidence of a fast bar in the weakly-interacting galaxy NGC 4264 with MUSE
• Alone on a wide wide sea. The origin of SECCO 1, an isolated star-forming gas cloud in the Virgo cluster
• Chiral Dark Sector
• Galaxy-Mass Correlations on 10 Mpc Scales in the Deep Lens Survey
• Detectability of the gravitational redshift effect from the asymmetric galaxy clustering
• Radiative Feedback in Relic HII Regions at High-Redshift
• Physical evolution of dark matter halo around the depletion boundary
• The cold mode: A phenomenological model for the evolution of density perturbations in the intracluster medium
• Probing Light Dark Matter through Cosmic-Ray Cooling in Active Galactic Nuclei
• Probing the mass distribution in groups of galaxies using gravitational lensing
• 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
• The Coupling of Galactic Dark Matter Halos with Stellar Bars
• Formation of N-rich field stars in the high-density building blocks of the Galactic bulge
• Dwarf Spheroidal Satellite Formation in a Reionized Local Group
• Higher-order Convergence Statistics for Three-dimensional Weak Gravitational Lensing
• Illuminating dark matter and primordial black holes with interstellar antiprotons
• PACT. II. Pressure profiles of galaxy clusters using Planck and ACT
• Intrinsic alignments of galaxies and their effects on weak lensing detections of mass concentrations
• The Most Metal-poor Stars in the Inner Bulge
• A New Algorithm to Quantify Maximum Discs in Galaxies
• The non-Gaussian tail of cosmic-shear statistics
• Constraining dark matter halo profiles and galaxy formation models using spiral arm morphology. II. Dark and stellar mass concentrations for 13 nearby face-on galaxies
• The degeneracy between star-formation parameters in dwarf galaxy simulations and the Mstar-Mhalo relation
• MARS: A New Maximum Entropy-Regularized Strong Lensing Mass Reconstruction Method
• Smallest Remnants of Early Matter Domination
• Searching for Boosted Dark Matter via Dark-Strahlung
• Testing Verlinde's emergent gravity in early-type galaxies
• The Variation of the Galaxy Luminosity Function with Group Properties
• Shining Primordial Black Holes
• Peculiar acceleration
• Self-interacting Dark Scalar Spikes around Black Holes via Relativistic Bondi Accretion
• Universal predictions of screened modified gravity on cluster scales
• A Halo Model Approach to the $21\mathrm{cm}$ and $\mathrm{Ly}\alpha$ Cross-correlation
• The impact of $\Lambda$CDM substructure and baryon-dark matter transition on the image positions of quad galaxy lenses
• Violent and mild relaxation of an isolated self-gravitating uniform and spherical cloud of particles
• Entering the Era of Dark Matter Astronomy? Near to Long-Term Forecasts in X-Ray and Gamma-Ray Bands
• Synthetic ${}^{26}$Al emission from galactic-scale superbubble simulations
• Reconstruction of Radio Relics and X-ray Tails in an Off-axis Cluster Merger: Hydrodynamical Simulations of A115
• Astrophysical Tests of Dark Matter Self-Interactions
• Velocity reconstruction with the cosmic microwave background and galaxy surveys
• The detection of sub-solar mass dark matter halos
• Connecting turbulent velocities and magnetic fields in galaxy cluster simulations with active galactic nuclei jets
• The Radius of Baryonic Collapse in Disc Galaxy Formation
• Massive stars and globular cluster formation
• Phase-space structure of cold dark matter halos inside splashback: multi-stream flows and self-similar solution
• New insights on the dissociative merging galaxy cluster Abell 2034
• The Last Journey. I. An Extreme-Scale Simulation on the Mira Supercomputer
• Optimal filters for the moving lens effect
• Direct/indirect detection signatures of nonthermally produced dark matter
• Is the Universe Simpler than LCDM?
• Dark matter density profiles: A comparison of nonextensive theory with N-body simulations
• A ~600 pc view of the strongly-lensed, massive main sequence galaxy J0901: a baryon-dominated, thick turbulent rotating disk with a clumpy cold gas ring at z = 2.259
• The Supersonic Project: rotational effects of supersonic motions on the first structures in the Universe
• How rare is the Bullet Cluster (in a $\Lambda$CDM universe)?
• On the structure of globular cluster systems in elliptical galaxies
• Could pressureless dark matter have pressure?
• Confronting Galactic center and dwarf spheroidal gamma-ray observations with cascade annihilation models
• Observational Evidence of Evolving Dark Matter Profiles at $z\le 1$
• Major mergers between dark matter haloes -- II. Profile and concentration changes
• The Grism lens-amplified survey from space (GLASS). VIII. The influence of the cluster properties on Halpha emitter galaxies at 0.3<z<0.7
• Is it possible to tell the difference between fermionic and bosonic hot dark matter?
• Relation between the Turnaround radius and virial mass in $f(R)$ model
• Dark Matter decay and annihilation in the Local Universe: CLUES from Fermi
• Gravitational wave probes of particle dark matter: a review
• Pairwise velocities in the Halo Model: Luminosity and Scale Dependence
• Absorption Line Signatures of Gas in Mini Dark Matter Halos
• Hydrodynamic simulations of an isolated star-forming gas cloud in the Virgo cluster
• Cosmological gamma ray and neutrino backgrounds due to neutralino dark matter annihilation
• Galaxy Zoo: constraining the origin of spiral arms
• Detecting strongly lensed supernovae at z ~ 5-7 with LSST
• Self-interactions of ULDM to the rescue?
• Supersymmetric dark matter in M31: can one see neutralino annihilation with CELESTE?
• The SATIN project I: Turbulent multi-phase ISM in Milky Way simulations with SNe feedback from stellar clusters
• Scaling relations for globular cluster systems in early-type galaxies
• Triaxiality, principal axis orientation and non-thermal pressure in Abell 383
• Bayesian analysis for rotational curves with $\ell$-boson stars as a dark matter component
• Nonlinear Gravitational Clustering: dreams of a paradigm
• Slow evolution of elliptical galaxies induced by dynamical friction III. Role of density concentration and pressure anisotropy
• X-ray Measurement of Dark Matter "Temperature" in Abell 1795
• The PAndAS View of the Andromeda Satellite System. IV Global properties
• The role of bars on the dynamical-friction driven inspiral of massive perturbers
• Fragmentation in Dusty Low-Metallicity Star Forming Halos
• Systematic uncertainties from halo asphericity in dark matter searches
• Gravitational waves from dark matter collapse in a star
• Running with BICEP2: Implications for Small-Scale Problems in CDM
• Dark matter in disk galaxies I: a Markov Chain Monte Carlo method and application to DDO 154
• The Missing Satellite Problem Outside of the Local Group. II. Statistical Properties of Satellites of Milky Way-like Galaxies
• The neutral hydrogen distribution in large-scale haloes from 21-cm intensity maps
• Enhanced star formation in $z\sim 6$ quasar companions
• Tensor-vector-scalar-modified gravity: from small scale to cosmology
• Hadronically decaying heavy dark matter and high-energy neutrino limits
• Simulations of the Galaxy Cluster CIZA J2242.8+5301 I: Thermal Model and Shock Properties
• Indirect Detection of Dirac Right-Handed Neutrino Dark Matter
• The inner structure of very massive elliptical galaxies: implications for the inside-out formation mechanism of z~2 galaxies
• Cosmological Simulations of Two-Component Wave Dark Matter
• The tidal stream generated by the globular cluster NGC 3201
• Effect of Measurement Errors on Predicted Cosmological Constraints from Shear Peak Statistics with LSST
• hybrid-Lenstool: A self-consistent algorithm to model galaxy clusters with strong- and weak-lensing simultaneously
• Possible Connection between Dark Matter and Supermassive Black Holes
• Formation of globular clusters with multiple stellar populations from massive gas clumps in high-z gas-rich dwarf galaxies
• Galactic wormholes: Geometry, stability, and echoes
• Characteristic Size and Mass of Galaxies in the Bose-Einstein Condensate Dark Matter Model
• Action-based models for dwarf spheroidal galaxies and globular clusters
• A high baryon fraction in massive haloes at z~3
• Separating Galaxies from the Cluster Dark Matter Halo in Abell 611
• Towards a higher mass for NGC1052-DF2: an analysis based on full distribution functions
• Predictive model of fermionic dark matter halos with a quantum core and an isothermal atmosphere
• Density spikes near black holes in self-interacting dark matter halos and indirect detection constraints
• A robust lower limit on the amplitude of matter fluctuations in the universe from cluster abundance and weak lensing
• Probing black holes in a dark matter spike of M87 using quasinormal modes
• Do we know the mass of a black hole? Mass of some cosmological black hole models
• Numerical simulations challenged on the prediction of massive subhalo abundance in galaxy clusters: the case of Abell 2142
• A MUSE view of the massive merging galaxy cluster ACT-CL J0102-4915 (El Gordo) at z = 0.87: robust strong lensing model and data release
• Back-in-time dynamics of the cluster IE 0657-56 (the Bullet System)
• Euclid preparation. XLI. Galaxy power spectrum modelling in real space
• GalWeight: A New and Effective Weighting Technique for Determining Galaxy Cluster and Group Membership
• Lensing clusters of galaxies in the SDSS-III
• Testing redMaPPer centring probabilities using galaxy clustering and galaxy-galaxy lensing
• The PDF perspective on the tracer-matter connection: Lagrangian bias and non-Poissonian shot noise
• A scenario for ultra-diffuse satellite galaxies with low velocity dispersions: the case of [KKS 2000]04
• The SAMI Galaxy Survey: Environmental analysis of the orbital structures of passive galaxies
• Chemical evolution of giant molecular clouds in simulations of galaxies
• Bending instability in galactic discs. Advocacy of the linear theory
• ATIC/PAMELA anomaly from fermionic decaying Dark Matter
• Weak Lensing Mass Reconstruction of the Galaxy Cluster Abell 209
• What galaxy masses perturb the local cosmic expansion?
• Hydrostatic equilibrium profiles for gas in elliptical galaxies
• The Three Hundred project: Galaxy groups do not survive cluster infall
• Wormhole formations in the galactic halos supported by dark matter models and global monopole charge within $f(Q)$ gravity
• Around The Way: Testing $\Lambda$CDM with Milky Way Stellar Stream Constraints
• On the Gravitational Wave Background from Black Hole Binaries after the First LIGO Detections
• Weak lensing measurements of the APEX-SZ galaxy cluster sample
• ALP dark matter with non-periodic potentials: parametric resonance, halo formation and gravitational signatures
• Beyond the Ultra-deep Frontier Fields And Legacy Observations (BUFFALO): a high-resolution strong + weak-lensing view of Abell 370
• MUSE spectroscopy and deep observations of a unique compact JWST target, lensing cluster CLIO
• First Detection of Cosmic Microwave Background Lensing and Lyman-α Forest Bispectrum
• The Far-Away Blues: Exploring the Furthest Extents of the Boötes I Ultra Faint Dwarf Galaxy
• Subsonic accretion and dynamical friction for a black hole moving through a self-interacting scalar dark matter cloud
• Possible formation of wormholes from dark matter in an isothermal galactic halo and void
• Infrared observations of gravitational lensing in Abell 2219 with CIRSI
• Astrophysical Uncertainties in the Cosmic Ray Electron and Positron Spectrum From Annihilating Dark Matter
• Heavy dark matter particle annihilation in dwarf spheroidal galaxies: radio signals at the SKA telescope
• A Chandra study of Abell 795 -- a sloshing cluster with a FR0 radio galaxy at its center
• Horizon growth of supermassive black hole seeds fed with collisional dark matter
• Modelling the accretion and feedback of supermassive black hole binaries in gas-rich galaxy mergers
• Orbit-Superposition Dynamical Modeling of Barred Galaxies
• Effects of mass models on dynamical mass estimate: the case of ultra diffuse galaxy NGC1052-DF2
• UGC 1378 -- a Milky Way-sized galaxy embedded in a giant low-surface brightness disc
• Star Formation History in Barred Spiral Galaxies. AGN Feedback
• Ophiuchus: an optical view of a very massive cluster of galaxies hidden behind the Milky Way
• The Origin of Buckling Instability in Galactic Bars: Searching for the Scapegoat
• Galactic Origin of Relativistic Bosons and XENON1T Excess
• TDCOSMO VIII: Cosmological distance measurements in light of the mass-sheet degeneracy -- forecasts from strong lensing and IFU stellar kinematics
• The strongest gravitational lenses: II. Is the large Einstein radius of MACS J0717.5+3745 in conflict with LCDM?
• How many arcminute-separation lenses are expected in the 2dF QSO survey?
• Giant Low Surface Brightness Galaxies : Evolution in Isolation
• Evolution of the luminosity-to-halo mass relation of LRGs from a combined SDSS-DR10+RCS2 analysis
• Free-form Grale lens inversion of galaxy clusters with up to 1000 multiple images
• Dark Matter on Top
• The Shape of Galaxy Cluster Dark Matter Haloes: Systematics of Its Imprint on Cluster Gas, and Comparison to Observations
• The haloes of merger remnants
• The clustering of $z>7$ galaxies: Predictions from the BLUETIDES simulation
• A study of the NGC 1193 and NGC 1798 open clusters using CCD UBV photometric and Gaia EDR3 data
• Keck Spectroscopy of the Coma Cluster Ultra-Diffuse Galaxy Y358: Dynamical Mass in a Wider Context
• Circumstellar Dust, PAHs, and Stellar Populations in Early-Type Galaxies: Insights from GALEX and WISE
• Most of the cool CGM of star-forming galaxies is not produced by supernova feedback
• Kinematics of the OVI Circumgalactic Medium: Halo Mass Dependence and Outflow Signatures
• The Race to Find Split Higgsino Dark Matter
• Orbital and escape dynamics in barred galaxies - II. The 3D system: Exploring the role of the normally hyperbolic invariant manifolds
• Age dissection of the vertical breathing motions in Gaia DR2: evidence for spiral driving
• A determination of dark matter bispectrum with a large set of N-body simulations
• An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
• The survival of globular clusters in a cuspy Fornax
• Cosmology with the sub-millimetre galaxies magnification bias: Tomographic Analysis
• On the Origin of Mass--Metallicity Relations, Blue Tilts, and Scaling Relations for Metal-poor Globular Cluster Systems
• Dark Matter in Cosmology
• Dark Matter Microhalos in the Solar Neighborhood: Pulsar Timing Signatures of Early Matter Domination
• Monoenergetic Gamma-Rays from Non-Minimal Kaluza-Klein Dark Matter Annihilations
• Density perturbations in the gas of wormholes
• KiDS+GAMA: The weak lensing calibrated stellar-to-halo mass relation of central and satellite galaxies
• Studying the Dynamical Properties of 20 Nearby Galaxy Clusters
• A Tight Connection Between Direct and Indirect Detection of Dark Matter through Higgs Portal Couplings to a Hidden Sector
• EMPRESS. III. Morphology, Stellar Population, and Dynamics of Extremely Metal Poor Galaxies (EMPGs): Are EMPGs Local Analogs of High-$z$ Young Galaxies?
• Modelling the asymmetry of the halo cross-correlation function with relativistic effects at quasi-linear scales
• Exploring extensions to the standard cosmological model and the impact of baryons on small scales
• Galactic-Centre Gamma Rays in CMSSM Dark Matter Scenarios
• Anti-Deuterons and Anti-Helium Nuclei from Annihilating Dark Matter
• A search for the third lensed image in JVAS B1030+074
• Periapsis shifts in dark matter distribution around a black hole
• Amending the halo model to satisfy cosmological conservation laws
• Escalating core formation with dark matter self-heating
• Constraining the multi-scale dark-matter distribution in CASSOWARY 31 with strong gravitational lensing and stellar dynamics
• The Bimodal Absorption System Imaging Campaign (BASIC) I. A Dual Population of Low-metallicity Absorbers at z $<1$
• The Response of Dark Matter Haloes to Gas Ejection: CuspCore II
• Antlia2's role in driving the ripples in the outer gas disk of the Galaxy
• Astrophysical Observations of a Dark Matter-Baryon Fifth Force
• SEAGLE--II: Constraints on feedback models in galaxy formation from massive early type strong lens galaxies
• Classifying globular clusters and applying them to estimate the mass of the Milky Way
• The OSIRIS Lens-Amplified Survey (OLAS) I: Dynamical Effects of Stellar Feedback in Low Mass Galaxies at z ~ 2
• Cosmic evolution of metal densities: the enrichment of the Inter-Galactic Medium
• Estimating the Milky Way's Mass via Hierarchical Bayes: A Blind Test on MUGS2 Simulated Galaxies
• Smooth Particle Lensing
• Dust in galaxy clusters: Modeling at millimeter wavelengths and impact on Planck cluster cosmology
• Magnification Bias of Distant Galaxies in the Hubble Frontier Fields: Testing Wave vs. Particle Dark Matter Predictions
• Stellar halos and elliptical galaxy formation: Origin of dynamical properties of the planetary nebular systems
• GHASP: an H$\alpha$ kinematical survey of spiral galaxies - XI. Distribution of luminous and dark matter in spiral and irregular nearby galaxies using WISE photometry
• Hamiltonians of Spherically Symmetric, Scale-Free Galaxies in Action-Angle Coordinates
• Classifying orbits in galaxy models with a prolate or an oblate dark matter halo component
• Absorber Model: the Halo-like model for the Lyman-alpha forest
• Outflow or galactic wind: The fate of ionized gas in the halos of dwarf galaxies
• $J$-factors for self-interacting dark matter in 20 dwarf spheroidal galaxies
• Multi-wavelength scaling relations in galaxy groups: a detailed comparison of GAMA and KiDS observations to BAHAMAS simulations
• Indirect Search for Dark Matter in M31 with the CELESTE Experiment
• Modelling Baryonic Effects on Galaxy Cluster Mass Profiles
• HOD-Dependent Systematics in Emission Line Galaxies for the DESI 2024 BAO analysis
• Imprints of gravitational lensing in the Planck CMB data at the location of WISExSCOS galaxies
• Dark Matter-Neutrino Interaction in Light of Collider and Neutrino Telescope Data
• Divergence of Perturbation Theory in Large Scale Structures
• Euler-Heisenberg black hole surrounded by quintessence in the background of perfect fluid dark matter: Thermodynamics, Shadows and Quasinormal modes
• Detecting low-mass haloes with strong gravitational lensing II: constraints on the density profiles of two detected subhaloes
• Searching the Footprint of WIMPZILLAs
• Distinguishing Supersymmetry From Universal Extra Dimensions or Little Higgs Models With Dark Matter Experiments
• The environment and host haloes of the brightest z~6 Lyman-break galaxies
• Recovering the mass profile and orbit anisotropy of mock dwarf galaxies with Schwarzschild modelling
• Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
• Periodic orbits and their gravitational wave radiations in black hole with dark matter halo
• Generalised model-independent characterisation of strong gravitational lenses I: Theoretical foundations
• Probing Halos of Galaxies at Very Large Radii using Background QSOs
• Significant enhancement of ${\mathrm{H}}_2$ formation in disk galaxies under strong ram pressure
• What to expect from dynamical modelling of galactic haloes
• Potential--density pairs for spherical galaxies and bulges: the influence of scalar fields
• Updated galactic radio constraints on Dark Matter
• The Effect of Thermal Velocities on Structure Formation in N-body Simulations of Warm Dark Matter
• Formalism for the Subhalo Mass Function in the Tidal-limit Approximation
• Study of gravitational fields and globular cluster systems of early-type galaxies
• Is the late buckling stage inevitable in the bar life?
• Effects of Preheated Clusters on the CMB Spectrum
• Observation of the new emission line at ~3.5 keV in X-ray spectra of galaxies and galaxy clusters
• Galaxy rotation curves and universal scaling relations: comparison between phenomenological and fermionic dark matter profiles
• Generalized Tachyonic Teleparallel cosmology
• Constraints on the Baryonic Compression and Implications for the Fraction of Dark Halo Lenses
• Radio Relics Tracing the Projected Mass Distribution in CIZA J2242.8+5301
• Dynamical analysis of galaxy cluster merger Abell 2146
• Dark influences II: gas and star formation in minor mergers of dwarf galaxies with dark satellites
• Diffuse gamma-ray background and cosmic-ray positrons from annihilating dark matter
• Cosmological Studies from HSC-SSP Tomographic Weak Lensing Peak Abundances
• The Variation of Rotation Curve Shapes as a Signature of the Effects of Baryons on Dark Matter Density Profiles
• Galactic Dark Matter and Bertrand Space-times
• The cusp-core problem in gas-poor dwarf spheroidal galaxies
• Dark Matter Astrometry: Accuracy of sub-halo positions for the measurement of self-interaction cross sections
• An Alternative Formation Model for Antideuterons from Dark Matter
• AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis
• Central Mass Profiles of the Nearby Cool-core Galaxy Clusters Hydra A and A478
• A Multi-Wavelength Mass Analysis of RCS2 J232727.6-020437, a ~3x10${}^{15}$M${}_{\odot }$ Galaxy Cluster at z=0.7
• Subhaloes gone Notts: the clustering properties of subhaloes
• Mesh-free free-form lensing I: Methodology and application to mass reconstruction
• Are dwarf spheroidal galaxies dark matter dominated or remnants of disrupted larger satellite galaxies? -- A possible test
• The structure of the Milky Way based on unWISE 3.4$\mu$m integrated photometry
• The Effect of Dark Matter Halo Shape on Bar Buckling and Boxy/Peanut Bulges
• Accretion disks around naked singularities
• Multi-wavelength mock galaxy catalogs of the low-redshift Universe
• The clustering of baryonic matter. I: a halo-model approach
• Recent Result of the AMS-02 Experiment and Decaying Gravitino Dark Matter in Gauge Mediation
• The First Billion Years project: dark matter haloes going from contraction to expansion and back again
• Probing of the Interactions Between the Hot Plasmas and Galaxies in Clusters from z=0.1 to 0.9
• Bounds on graviton mass using weak lensing and SZ effect in galaxy clusters
• A novel JEAnS analysis of the Fornax dwarf using evolutionary algorithms: mass follows light with signs of an off-centre merger
• Sterile neutrinos, dark matter, and resonant effects in ultra high energy regimes
• Merging Hierarchical Triple Black Hole Systems with Intermediate-mass Black Holes in Population III Star Clusters
• A high-resolution cosmological simulation of a strong gravitational lens
• The U-shaped distribution of globular cluster specific frequencies in a biased globular cluster formation scenario
• A Parallel Tree-SPH code for Galaxy Formation
• Comparing Dark Energy Survey and HST-CLASH observations of the galaxy cluster RXC J2248.7-4431: implications for stellar mass versus dark matter
• Detecting Axion Dark Matter through the Radio Signal from Omega Centauri
• Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
• Waves from the Centre: Probing PBH and other Macroscopic Dark Matter with LISA
• Higher-order Statistics of Weak Lensing Shear and Flexion
• Cuspy and fractured black hole shadows in a toy model with axisymmetry
• Inferring the Intermediate Mass Black Hole Number Density from Gravitational Wave Lensing Statistics
• Probing dark matter models with neutrinos from the Galactic center
• Cold dark energy constraints from the abundance of galaxy clusters
• Face-on structure of barlenses and boxy bars: an insight from spectral dynamics
• Complexity on dwarf galaxies scale: A bimodal distribution function in Sculptor
• Dark matter halos in the multicomponent model. I. Substructure
• Probing chiral and flavored $Z^{\prime }$ from cosmic bursts through neutrino interactions
• Studying large-scale structure probes of modified gravity with COLA
• Gravothermal collapse of Self-Interacting Dark Matter halos as the Origin of Intermediate Mass Black Holes in Milky Way satellites
• The mass loss process in dwarf galaxies from 3D hydrodynamical simulations: the role of dark matter and starbursts
• Evolution of Late-type Galaxies in a Cluster Environment: Effects of High-speed Multiple Encounters with Early-type Galaxies
• Towards a new modelling of gas flows in a semi-analytical model of galaxy formation and evolution
• Dark Matter and IMF normalization in Virgo dwarf early-type galaxies
• Weighing the Galactic dark matter halo: a lower mass limit from the fastest halo star known
• Galaxies in X-ray Groups. III. Satellite Color and Morphology Transformations
• Diffuse flux of ultra-high energy photons from cosmic-ray interactions in the disk of the Galaxy and implications for the search for decaying super-heavy dark matter
• Antideuterons from Dark Matter Decay
• Fast generation of mock galaxy catalogues in modified gravity models with COLA
• Weak Lensing of the CMB: Power Spectrum Covariance
• Varying alpha from N-body Simulations
• Probing dark matter signals in neutrino telescopes through angular power spectrum
• Comparing different mass estimators for a large subsample of the {\it Planck}-ESZ clusters
• GHASP: an H$\alpha$ kinematical survey of spiral galaxies -- XIII. Distribution of luminous and dark matter in spiral and irregular nearby galaxies using H$\alpha$ and HI rotation curves and WISE photometry
• Variation of $\alpha$ from a Dark Matter Force
• Small-scale anisotropy of the cosmic background radiation and scattering by cloudy plasma
• AGN Jet Power, Formation of X-ray Cavities, and FR I/II Dichotomy in Galaxy Clusters
• Search for dark matter annihilation in the dwarf irregular galaxy WLM with H.E.S.S
• The distribution of dark matter and gas spanning six megaparsecs around the post-merger galaxy cluster MS0451-03
• The massive dark halo of the compact, early-type galaxy NGC 1281
• Spiral flows in cool-core galaxy clusters
• Exploring Relations Between BCG \& Cluster Properties in the SPectroscopic IDentification of eROSITA Sources Survey from $0.05<z<0.3$
• Hydrodynamics of galactic dark matter
• Dark Stars Powered by Self-Interacting Dark Matter
• The Variation of Gas Mass Distribution in Galaxy Clusters: Effects of Preheating and Shocks
• Imaging dark matter at the smallest scales with $z\approx 1$ lensed stars
• Tracing stars in Milky Way satellites with A-SLOTH
• Higgsino Dark Matter Confronts 14 years of Fermi Gamma Ray Data
• Numerical investigation of lenses with substructures using the perturbative method
• Can Supermassive Black Holes alter Cold Dark Matter cusps through accretion?
• Improved particle spray algorithm for modeling globular cluster streams
• UGC 7069: The largest ring galaxy
• An Iterative Method for the Construction of Equilibrium N-Body Models for Stellar Disks
• The accretion history of the Milky Way. I. How it shapes globular clusters and dwarf galaxies
• Black Holes in our Galactic Halo: Compatibility with FGST and PAMELA Data and Constraints on the First Stars
• Schwarzschild Black Hole Surrounded by Perfect Fluid Dark Matter in the presence of Quintessence Matter Field
• The anatomy of the NGC 5044 group - I. Group membership and dynamics
• Constraints on electron-scattering interpretation of XENON1T excess
• Anisotropy of dark matter annihilation with respect to the Galactic plane
• Confronting Models of Dwarf Galaxy Quenching with Observations of the Local Group
• Nonlinear resonant oscillation of gravitational potential induced by ultralight axion in $f(R)$ gravity
• A Comparison of Weak Lensing Measurements From Ground- and Space-Based Facilities
• Stellar and Gaseous Disk Structures in Cosmological Galaxy Equilibrium Models
• The submillimetre view of massive clusters at z~0.8-1.6
• The relative impact of baryons and cluster shape on weak lensing mass estimates of galaxy clusters
• Testing MOdified Gravity (MOG) theory and dark matter model in Milky Way using the local observables
• Hunting for dark halo substructure using submilliarcsecond-scale observations of macrolensed radio jets
• H-Band and Spectroscopic Properties of Abell 1644
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• The Fornax3D project: Environmental effects on the assembly of dynamically cold disks in Fornax cluster galaxies
• Maturing Satellite Kinematics into a Competitive Probe of the Galaxy-Halo Connection
• Constraining dark matter annihilation with cosmic ray antiprotons using neural networks
• Improving models of the cosmic infrared background using CMB lensing mass maps
• A comparison between direct and indirect dark matter search
• Search for a dark-matter induced Cosmic Axion Background with ADMX
• Orbital distribution of infalling satellite halos across cosmic time
• Metallicity and Kinematics of the Galactic halo from the LAMOST sample stars
• Schmidt-Kennicutt relations in SPH simulations of disc galaxies with effective thermal feedback from supernovae
• Spectroscopic analysis of Milky Way outer halo satellites: Aquarius II and Bootes II
• Multiwavelength Analysis of A1240, the Double Radio Relic Merging Galaxy Cluster Embedded in a ~80 Mpc-long Cosmic Filament
• Enlightening the dynamical evolution of Galactic open clusters: an approach using Gaia DR3 and analytical descriptions
• $\gamma$-ray and $\nu$ searches for dark matter subhalos in the Milky Way with a baryonic potential
• Second Moment of Halo Occupation Number
• Decaying neutralino dark matter in anomalous $U(1{)}_H$ models
• Spatial distribution of dark matter in and around galaxy clusters traced by galaxies, gas and intracluster stars in a simulated universe
• The Milky Way's dark matter halo appears to be lopsided
• The role of baryons in self-interacting dark matter mergers
• The stellar mass to light ratio in the isolated spiral NGC 4414
• Morphology driven evolution of barred galaxies in OMEGAWINGS Clusters
• Modeling globular clusters in the TNG50 simulation: predictions from dwarfs to giants
• Signals of dark matter in a supersymmetric two dark matter model
• Raytracing simulations of coupled dark energy models
• The present-day gas content of simulated field dwarf galaxies
• Breaking cosmic degeneracies: Disentangling neutrinos and modified gravity with kinematic information
• The Effect of Substructure on Mass Estimates of Galaxies
• SN-driven mechanism of cusp-core transformation: an appraisal
• Do low surface brightness galaxies have dense disks?
• Searching for Dark Matter Annihilation in the Smith High-Velocity Cloud
• A Precise Analytical Approximation for the Deprojection of the Sérsic Profile
• Stellar Bars in Spinning Halos: Delayed Buckling and Absence of Slowdown
• A unified scenario for the origin of spiral and elliptical galaxy structural scaling laws
• The Impact of Cluster Structure and Dynamical State on Scatter in the Sunyaev-Zel'dovich Flux-Mass Relation
• Major mergers between dark matter haloes -- I. Predictions for size, shape, and spin
• Constraining the primordial curvature perturbation using dark matter substructure
• The Layzer-Irvine equation in theories with non-minimal coupling between matter and curvature
• Dark influences: imprints of dark satellites on dwarf galaxies
• Navarro-Frenk-White dark matter profile and the dark halos around disk systems
• A finer view of the conditional galaxy luminosity function and magnitude-gap statistics
• Modified Dark Matter: Relating Dark Energy, Dark Matter and Baryonic Matter
• Quantum Foam, Gravitational Thermodynamics, and the Dark Sector
• Time Delays for the Giant Quadruple Lensed Quasar SDSS J1004+4112: Prospects for Determining the Density Profile of the Lensing Cluster
• Constraining Dark Matter Properties with Gamma-Rays from the Galactic Center with Fermi-LAT
• Real and counterfeit cores: how feedback expands halos and disrupts tracers of inner gravitational potential in dwarf galaxies
• Cosmological constraints with the sub-millimetre galaxies Magnification Bias after large scale bias corrections
• Constraints on Cold H_2 Clouds from Gravitational Microlensing Searches
• Statistical Microlensing Toward Magnified High-Redshift Star Clusters
• Simulations of globular clusters within their parent galaxies: multiple stellar populations and internal kinematics
• Velocity Distribution of Dark Matter Spike around Schwarzschild Black Holes and Effects on Gravitational Waves from EMRIs
• A study of dark matter halos and gas properties in clusters of galaxies from ROSAT data
• Radiative Seesaw Model and DAMPE Excess from Leptophilic Gauge Symmetry
• Dark Matter "Transporting" Mechanism Explaining Positron Excesses
• Numerical challenges for energy conservation in N-body simulations of collapsing self-interacting dark matter halos
• From spirals to lenticulars: evidence from the rotation curves and mass models of three early-type galaxies
• Dynamical modelling of a remarkable four-armed barred spiral galaxy ESO 566-24
• Dark Matter Line Searches with the Cherenkov Telescope Array
• Hunting A Wandering Supermassive Black Hole in M31 Halo -- Hermitage of Black Hole
• A Numerical Renormalization Solution for Self-Similar Cosmic Structure Formation
• The Shape of Dark Matter Haloes, V. Analysis of observations of edge-on galaxies
• Gamma-ray anisotropies from dark matter in the Milky Way: the role of the radial distribution
• QSSC re-examined for the newly discovered SNe Ia
• Applying scale-free mass estimators to the Local Group in Constrained Local Universe Simulations
• Effects of center offset and noise on weak-lensing derived concentration-mass relation of dark matter halos
• Gas Accretion in Star-Forming Galaxies
• The Distribution of Dark and Luminous Matter in the Unique Galaxy Cluster Merger Abell 2146
• Observational consistency and future predictions for a 3.5 keV ALP to photon line
• Cosmic-ray antiprotons in the AMS-02 era: A sensitive probe of dark matter
• The baryon cycle of Seven Dwarfs with superbubble feedback
• Noiseless Gravitational Lensing Simulations
• Numerical modelling of Auriga's Wheel - a new ring galaxy
• Subhalo sinking and off-center massive black holes in dwarf galaxies
• Further support for a trio of mass-to-light deviations in Abell 370: free-form Grale lens inversion using BUFFALO strong lensing data
• Extreme mass ratio inspirals in rotating dark matter spikes
• Formation and evolution of molecular hydrogen in disk galaxies with different masses and Hubble types
• The Pristine survey XVIII: C-19: Tidal debris of a dark matter-dominated globular cluster?
• Reignited star formation in dwarf galaxies quenched during reionization
• Matrix method for perturbed black hole metric with discontinuity
• Pre- and post-processing of cluster galaxies out to $5\times R_{200}$: The extreme case of A2670
• Strong lensing by fermionic dark matter in galaxies
• Dark halo structure in the Carina dwarf spheroidal galaxy: joint analysis of multiple stellar components
• The low dark matter content of the lenticular galaxy NGC 3998
• Dark matter caustics and the enhancement of self-annihilation flux
• Enhanced Line Signals from Annihilating Kaluza-Klein Dark Matter
• Bending waves excited by irregular gas inflow along warps
• Fast and realistic large-scale structure from machine-learning-augmented random field simulations
• The Case for Strangulation in Low-Mass Hosts: DDO 113
• Stars and gas in the very large interacting galaxy NGC 6872
• Neutrino lines from MeV dark matter annihilation and decay in JUNO
• Galactic winds - How to launch galactic outflows in typical Lyman-break galaxies
• Effects of Non-Circular Motions on Azimuthal Color Gradients
• Smoothing Rotation Curves and Mass Profiles
• Effect of the initial mass function on the dynamical SMBH mass estimate in the nucleated early-type galaxy FCC 47
• Dark Higgs Channel for FERMI GeV $\gamma$-ray Excess
• On the Clustering of Faint Red Galaxies
• The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray properties of Subaru optically-selected clusters
• The mass distribution in Spirals
• Turbulence decay in the density-stratified intracluster medium
• Gamma-ray detection from neutralino annihilation in non--universal SUGRA scenarios
• Cosmological and Environmental Influences on Hot Gas Observed in Elliptical Galaxies
• How chameleons core dwarfs with cusps
• Are rotation curves in NGC 6946 and the Milky Way magnetically supported?
• Black Holes, Dark Matter Spikes, and Constraints on Simplified Models with $t$-Channel Mediators
• Stellar dynamics in the strong-lensing central galaxy of Abell 1201: A low stellar mass-to-light ratio, a large central compact mass, and a standard dark matter halo
• Probing WHIM around Galaxy Clusters with Fast Radio Bursts and the Sunyaev-Zel'dovich effect
• Dynamical masses of brightest cluster galaxies I: stellar velocity anisotropy and mass-to-light ratios
• The Distribution of Dark Matter in the Halo of the early-type galaxy NGC 4636
• Deflection of light by wormholes and its shadow due to dark matter within modified symmetric teleparallel gravity formalism
• Test of Weak Equivalence Principle with the multi-band timing of the Crab Pulsar
• It's a Breeze: The Circumgalactic Medium of a Dwarf Galaxy is Easy to Strip
• A Redshift Survey of the Nearby Galaxy Cluster Abell 2199: Comparison of the Spatial and Kinematic Distributions of Galaxies with the Intracluster Medium
• Tidal Stripping and Post-Merger Relaxation of Dark Matter Halos: Causes and Consequences of Mass Loss
• Confronting the DAMPE Excess with the Scotogenic Type-II Seesaw Model
• The SRG/eROSITA All-Sky Survey: Weak-Lensing of eRASS1 Galaxy Clusters in KiDS-1000 and Consistency Checks with DES Y3 & HSC-Y3
• The SRG-eROSITA All-Sky Survey : Constraints on f(R) Gravity from Cluster Abundance
• PeV scale Supersymmetry breaking and the IceCube neutrino flux
• Novel Gamma-Ray Signatures of PeV-Scale Dark Matter
• Intra-cluster Globular Clusters in a Simulated Galaxy Cluster
• On the relevance of chaos for halo stars in the solar neighbourhood II
• Generating mock galaxy catalogues for flux-limited samples like the DESI Bright Galaxy Survey
• Correlation Between the Halo Concentration (c) and the Virial Mass (Mvir) Determined from X-ray Clusters
• Chandra and XMM-Newton Observations of the Bimodal Planck SZ-detected Cluster PLCKG345.40-39.34 (A3716) with High and Low Entropy Subcluster Cores
• Improving the Angular Resolution of EGRET and New Limits on Supersymmetric Dark Matter Near the Galactic Center
• The dynamical structure of dark matter halos with universal properties
• Searching for Exploding Black Holes
• Dark matter annihilation into right-handed neutrinos and the galactic center gamma-ray excess
• Inferences from surface brightness fluctuations of Zwicky 3146 via the Sunyaev-Zeldovich effect and X-ray observations
• Gravitational waves from binary black holes in a self-interacting scalar dark matter cloud
• Formation of ultra-compact blue dwarf galaxies and their evolution into nucleated dwarfs
• Dark Stars: A New Study of the FIrst Stars in the Universe
• Constraining SuperWIMPy and Warm Subhalos with Future Submillilensing
• Can AMS-02 discriminate the origin of an anti-proton signal?
• Strong lensing in the MareNostrum Universe II: scaling relations and optical depths
• The structure of spiral galaxies: radial profiles in stellar Mass-to-Light ratio and the Dark Matter distribution
• Closing the Window on Strongly Interacting Dark Matter
• Dark Matter from Binary Tetrahedral Flavor Symmetry
• A combined X-ray, optical and radio view of the merging galaxy cluster MACS J0417.5-1154
• The First Fall is the Hardest: The Importance of Peculiar Galaxy Dynamics at Infall Time for Tidal Stripping Acting at the Centers of Groups and Clusters
• Effects of environment on sSFR profiles of late-type galaxies in the CALIFA survey
• Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-$y$-maps from SPT and Planck
• QSOs sigposting cluster size halos as gravitational lenses: halo mass, projected mass density profile and concentration at $z\sim 0.7$
• The tilt of the velocity ellipsoid in the Milky Way with Gaia DR2
• The Search for Intergalactic Hydrogen Clouds in Voids
• Substructure lensing in galaxy clusters as a constraint on low-mass sterile neutrinos in tensor-vector-scalar theory: The straight arc of Abell 2390
• A Phantom Menace: On the Morphology of the Galactic Center Excess
• An Inpainting Approach to Tackle the Kinematic and Thermal SZ Induced Biases in CMB-Cluster Lensing Estimators
• High-order matrix method with delimited expansion domain
• Galactic rotation dynamics in a new $f(\mathcal{R})$ gravity model
• Indirect dark-matter detection with MadDM v3.2 -- Lines and Loops
• Gravitational orbits in the expanding universe revisited
• Boosted Self-Interacting Dark Matter and XENON1T Excess
• Constraints on dark matter annihilation from the Event Horizon Telescope Observations of M87${}^{\star }$
• Annihilations of superheavy dark matter in superdense clumps
• Bounds on WIMP dark matter from galaxy clusters at low redshift
• A Survey for Large Separation Lensed FIRST Quasars
• Testing non-local gravity by clusters of galaxies
• Astrophysical Implications of a Visible Dark Matter Sector from a Custodially Warped-GUT
• On the Probability Distribution of Cosmological Microlensing Optical Depths
• Implications for Dark Matter Direct Detection in the Presence of LIGO-Motivated Primordial Black Holes
• Warm-hot gas in groups and galaxies toward H2356-309
• A minor merger scenario for the ultraluminous X-ray source ESO 243-49 HLX-1 - II. Constraints from photometry
• Structure formation in a mixed dark matter model with decaying sterile neutrino: the 3.5 keV X-ray line and the Galactic substructure
• Searching for primordial black holes with stochastic gravitational-wave background in the space-based detector frequency band
• Cluster detection from surface-brightness fluctuations in SDSS data
• The evolution of compact massive quiescent and starforming galaxies derived from the $R_e-R_h$ and $M_{\mathrm{star}}-M_h$ relations
• Cosmological simulations of self-interacting Bose-Einstein condensate dark matter
• Active gas features in three HSC-SSP CAMIRA clusters revealed by high angular resolution analysis of MUSTANG-2 SZE and XXL X-ray observations
• Collisional dark matter density profiles around supermassive black holes
• Comparing hypervelocity star populations from the Large Magellanic Cloud and the Milky Way
• Uncovering fossils of the distant Milky Way with UNIONS: NGC 5466 and its stellar stream
• Cosmic structures from a mathematical perspective 1. Dark matter halo mass density profiles
• Characteristics of Effective Dark Matter in Nonlocal Gravity
• Presence of red giant population in the foreground stellar sub-structure of the Small Magellanic Cloud
• The Central Mass and Phase-Space Densities of Dark Matter Halos: Cosmological Implications
• Linking nearby stellar streams to more distant halo overdensities
• Extended lens reconstructions with Grale: exploiting time domain, substructural and weak-lensing information
• Dynamical Modeling of Galaxies and Supermassive Black Holes: Axisymmetry in Triaxial Schwarzschild Orbit Superposition Models
• The Clustering and Halo Masses of Star Forming Galaxies at z<1
• Analytic marginalization of $N(z)$ uncertainties in tomographic galaxy surveys
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• Stellar proper motions in the outskirts of classical dwarf spheroidal galaxies with Gaia EDR3
• The Age-Metallicity-Specific Orbital Energy Relation for the Milky Way's Globular Cluster System Confirms the Importance of Accretion for Its Formation
• A slow bar in the dwarf irregular galaxy NGC 3741
• Possible features of galactic halo with electric field and observational constraints
• A heuristic wave equation parameterizing BEC dark matter halos with a quantum core and an isothermal atmosphere
• NIHAO XXVI: Nature versus nurture, the Star Formation Main Sequence and the origin of its scatter
• Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots
• The Capodimonte Deep Field I - Presentation of the survey and first follow-up studies
• The distribution of two-dimensional eccentricity of Sunyaev-Zeldovich Effect and X-ray surface brightness profiles
• Luminosity distance in Swiss cheese cosmology with randomized voids and galaxy halos
• A general relativistic approach to the Navarro-Frenk-White (NFW) galactic halos
• No need for dark matter in galaxy clusters within Galileon theory
• Robustness of dark matter constraints and interplay with collider searches for New Physics
• A direct black hole mass measurement in a Little Red Dot at the Epoch of Reionization
• Analytical shear and flexion of Einasto dark matter haloes
• Herschel and Hubble study of a lensed massive dusty starbursting galaxy at $z\sim 3$
• Accurate halo-galaxy mocks from automatic bias estimation and particle mesh gravity solvers
• The density profiles of Dark Matter halos in Spiral Galaxies
• Physical constraints on the central mass and baryon content of satellite galaxies
• The HST See Change Program: I. Survey Design, Pipeline, and Supernova Discoveries
• The Effect of Satellite Galaxies on Gravitational Lensing Flux Ratios
• Search for Boosted Dark Matter in COSINE-100
• Constraining extended cosmologies with GW$\times$LSS cross-correlations
• On the detectability of strong lensing in near-infrared surveys
• Cosmological Probes of Structure Growth and Tests of Gravity
• Formation of Andromeda II via a gas-rich major merger and an interaction with M31
• Disc dichotomy signature in the vertical distribution of [Mg/Fe] and the delayed gas infall scenario
• The Sensitivity of Future Gamma-Ray Telescopes to Primordial Black Holes
• Influence of local structure on relic neutrino abundances and anisotropies
• Planck/SDSS Cluster Mass and Gas Scaling Relations for a Volume-Complete redMaPPer Sample
• A general-purpose timestep criterion for simulations with gravity
• Revising the merger scenario of the galaxy cluster Abell 1644: a new gas poor structure discovered by weak gravitational lensing
• CLASH-VLT: The inner slope of the MACS J1206.2-0847 dark matter density profile
• Non-Universal Gaugino Masses, CDMS, and the LHC
• Mass modelling of superthin galaxies: IC5249, UGC7321 and IC2233
• The phase-diagram of the IGM and the entropy floor of groups and clusters: are clusters born warm?
• Isolated and non-isolated dark matter halos and the NFW profile
• The Milky Way, Coming into Focus: Precision Astrometry Probes its Evolution, and its Dark Matter
• A general study of decaying scalar dark matter: existing limits and projected radio signals at the SKA
• Modeling the black holes surrounded by a dark matter halo in the galactic center of M87
• The influences of the Magellanic Clouds on the Galaxy: Pole shift, warp, and star formation history
• Strong Evolution in the Luminosity-Velocity Relation at z>1?
• A Spectroscopic Survey of the Fields of 28 Strong Gravitational Lenses: Implications for $H_0$
• Patchy Screening of the CMB from Dark Photons
• A BCG with offset cooling: is the AGN feedback cycle broken in A2495?
• Dark energy and key physical parameters of clusters of galaxies
• Attack of the Flying Snakes : Formation of Isolated HI Clouds By Fragmentation of Long Streams
• Lensed Image Angles: New Statistical Evidence for Substructure
• Cosmology with the submillimetre galaxies magnification bias: Proof of concept
• The edge of galaxy formation III: The effects of warm dark matter on Milky Way satellites and field dwarfs
• Spin and structural halo properties at high redshift in a LCDM Universe
• Intermediate-mass black holes in dwarf galaxies: the case of Holmberg II
• The interacting galaxy pair KPG 390: H$\alpha$ kinematics
• A slightly oblate dark matter halo revealed by a retrograde precessing Galactic disk warp
• Quantifying the stellar ages of dynamically separated bulges and disks of CALIFA spiral galaxies
• Constraining the Magnetic Effects on HI Rotation Curves and the Need for Dark Halos
• A new fitting-function to describe the time evolution of a galaxy's gravitational potential
• Mass of clusters in simulations
• Searching for Machos (and other Dark Matter Candidates) in a Simulated Galaxy
• The orbital evolution of UFDs and GCs in an evolving Galactic potential
• The stellar mass function and evolution of the density profile of galaxy clusters from the Hydrangea simulations at $0<z<1.5$
• AMICO galaxy clusters in KiDS-DR3: measuring the splashback radius from weak gravitational lensing
• An attractor for dark matter structures
• Hydrodynamical simulations of coupled and uncoupled quintessence models II: Galaxy clusters
• Morphology of low-redshift compact galaxy clusters I. Shapes and radial profiles
• Genesis of morpho-kinematic lopsidedness in minor merger of galaxies
• CODEX Weak Lensing Mass Catalogue and implications on the mass-richness relation
• Dynamical friction and evolution of black holes in cosmological simulations: a new implementation in OpenGadget3
• Comparisons between isothermal and NFW mass profiles for strong-lensing galaxy clusters
• Modeling the star formation in galaxies using the Chemo - dynamical SPH code
• Suppressed Star Formation by a Merging Cluster System
• Reconstructing WIMP properties through an interplay of signal measurements in direct detection, Fermi-LAT, and CTA searches for dark matter
• Domain of validity for pseudo-elliptical NFW lens models
• High resolution science with high redshift galaxies
• A Long Stream of Metal-Poor Cool Gas around a Massive Starburst Galaxy at z = 2.67
• The role of dust destruction and dust growth in the evolution of the interstellar medium
• Dynamics of Stellar Disk Tilting from Satellite Mergers
• The Tight Empirical Relation between Dark Matter Halo Mass and Flat Rotation Velocity for Late-Type Galaxies
• Modelling the shapes of the largest gravitationally bound objects
• Direct Dark Matter Detection with Velocity Distribution in the Eddington approach
• Star Cluster Evolution in Dark Matter Dominated Galaxies
• Non-Gaussianity of the Cosmic Infrared Background anisotropies II : Predictions of the bispectrum and constraints forecast
• A Robust Approach to Constraining Dark Matter from Gamma-Ray Data
• Measuring line-of-sight shear with Einstein rings: a proof of concept
• The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations
• Giant cold satellites from low-concentration haloes
• Galactic Shapiro Delay to the Crab Pulsar and limit on Einstein's Equivalence Principle Violation
• Energy transfer from baryons to dark matter as a unified solution to small-scale structure issues of the $\Lambda$CDM model
• Exponents of non-linear clustering in scale-free one dimensional cosmological simulations
• Dependence of galaxy clustering on UV-luminosity and stellar mass at $z\sim 4-7$
• Gravitational lens modelling in a citizen science context
• Radial alignment of elliptical galaxies by the tidal force of a cluster of galaxies
• Multi-probe analysis of the galaxy cluster CL J1226.9+3332: Hydrostatic mass and hydrostatic-to-lensing bias
• Galaxy-lens determination of $H_0$: the effect of the ellipse+shear modeling assumption
• Investigating the detection of dark matter subhalos as extended sources with Fermi-LAT
• Constraining the origin of stellar binary black hole mergers by detections of their lensed host galaxies and gravitational wave signals
• Axion Echos from the Supernova Graveyard
• Globular clusters as tracers of the host galaxy mass distribution: the Fornax dSph test case
• The complex interplay of AGN jet-inflated bubbles and the intracluster medium
• Halo concentrations from extended Press-Schechter merger histories
• Cosmology through arc statistics I: sensitivity to ${\Omega }_m$ and ${\sigma }_8$
• Gamma Rays from Superheavy Relic Particles in the Halo
• EDGE: The shape of dark matter haloes in the faintest galaxies
• The anatomy of the NGC 5044 group -- II. Stellar populations and star-formation histories
• Constraints on differential Shapiro delay between neutrinos and photons from IceCube-170922A
• Estimating the local dark matter density in a non-axisymmetric wobbling disc
• Temperature and Entropy Profiles to the Virial Radius of Abell 1246 Cluster Observed with Suzaku
• The non-evolving internal structure of early-type galaxies: the case study SDSS J0728+3835 at z = 0.206
• The BAHAMAS project: Effects of a running scalar spectral index on large-scale structure
• The contribution of dissolving star clusters to the population of ultra-faint objects in the outer halo of the Milky Way
• Simulations of Galaxy Cluster Collisions with a Dark Plasma Component
• The Kinematic Sunyaev-Zel'dovich Effect with ACT, DES, and BOSS: a Novel Hybrid Estimator
• Compact Binary Merger Rate in Dark-Matter Spikes
• The Galactic One-Way Shapiro Delay to PSR B1937+21
• Sensitivity of the Cherenkov Telescope Array to TeV photon emission from the Large Magellanic Cloud
• Cross Correlation between the Thermal Sunyaev-Zel'dovich Effect and Projected Galaxy Density Field
• The importance of secondary halos for strong lensing in massive galaxy clusters across redshift
• Micro galaxies in LCDM
• Extragalactic diffuse gamma-rays from dark matter annihilation: revised prediction and full modelling uncertainties
• Relic density and PAMELA events in a heavy wino dark matter model with Sommerfeld effect
• Modelling high-resolution ALMA observations of strongly lensed dustystar forming galaxies detected by Herschel
• FAST-ASKAP Synergy: Quantifying Coexistent Tidal and Ram Pressure Strippings in the NGC 4636 Group
• Using H$\alpha$ Filaments to Probe AGN Feedback in Galaxy Clusters
• Coarse Graining the Distribution Function of Cold Dark Matter
• A Counterpart to the Radial Orbit Instability in Triaxial Stellar Systems
• The Correspondence between Convergence Peaks from Weak Lensing and Massive Dark Matter Haloes
• A 1-dimensional hydrodynamic model for accretion, cooling and heating of gas in dark matter halos from $z=6$ to $z=0$
• A Precise Benchmark for Cluster Scaling Relations: Fundamental Plane, Mass Plane and IMF in the Coma Cluster from Dynamical Models
• Axion minicluster streams in the solar neighbourhood
• Not All Subhaloes Are Created Equal: Modelling the Diversity of Subhalo Density Profiles in TNG50
• Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
• Impact of substructure on local dark matter searches
• Gas fueling and nuclear disk formation in merging between a central black hole and a gas clump
• The clustering of baryonic matter. II: halo model and hydrodynamic simulations
• Non-linear clustering during the BEC dark matter phase transition
• Optimal Softening for N-Body Halo Simulations
• Brought to Light II: Revealing the Origins of Cloaked Spiral Features in Cluster Passive Dwarf Galaxies
• Cosmic Ray Anomalies and Dark Matter Annihilation to Muons via a Higgs Portal Hidden Sector
• A photometric and astrometric study of the open clusters NGC 1664 and NGC 6939
• Distinguishing between $\Lambda$CDM and $f(R)$ gravity models using halo ellipticity correlations in simulations
• Jellyfish: Resolving the kinematics of extreme ram-pressure stripping at $z\sim 0.3$
• Absolute electron and positron fluxes from PAMELA/Fermi and Dark Matter
• A Very Simple Cusped Halo Model
• Evolution of stellar-gaseous disks in cosmological haloes
• Gamma Ray Constraints on Flavor Violating Asymmetric Dark Matter
• The Escape Velocity Profile of the Milky Way from Gaia DR3
• Density Profiles of Collisionless Equilibria. II. Anisotropic Spherical Systems
• Comment on "Scalar-tensor gravity coupled to a global monopole and flat rotation curves" by Lee and Lee
• Ram pressure stripping: An analytical approach
• A short survey of matter-antimatter evolution in the primordial universe
• A Chandra Study of Radial Temperature Profiles of the Intra-Cluster Medium in 50 Galaxy Clusters
• The Higgs intense--coupling regime in constrained SUSY models and its astrophysical implications
• Probing fermionic asymmetric dark matter cores using global neutron star properties
• Neutrinophilic Dark Matter in the epoch of IceCube and Fermi-LAT
• Fractal Holography: a geometric re-interpretation of cosmological large scale structure
• A Versatile and Accurate Method for Halo Mass Determination from Phase-Space Distribution of Satellite Galaxies
• On the effect of angular momentum on the prompt cusp formation via the gravitational collapse
• Constraining the Milky Way Dark Matter Density Profile with Gamma-Rays with Fermi-LAT
• The effect of stellar encounters on the dark matter annihilation signal from prompt cusps
• The Relevance of Dynamical Friction for the MW/LMC/SMC Triple System
• Probing cold dark matter subhalos with simulated ALMA observations of macrolensed sub-mm galaxies
• Precise Clustering and Density Evolution of redMaPPer Galaxy Clusters versus MXXL Simulation
• Measuring the total infrared light from galaxy clusters at z=0.5-1.6: connecting stellar populations to dusty star formation
• A weak lensing analysis of a STIS dark-lens candidate
• Joint Gas and Stellar Dynamical Models of WLM: An isolated dwarf galaxy within a cored, prolate DM halo
• Simulations of globular clusters within their parent galaxies: Metallicity spreads and anomalous precursor populations
• Axion Dark Radiation: Hubble Tension and Hyper-kamiokande Neutrino Experiment
• WISDOM Project -- XIII. Feeding molecular gas to the supermassive black hole in the starburst AGN-host galaxy Fairall 49
• Dense DM clumps seeded by cosmic string loops and DM annihilation
• Euclid Preparation XXXIII. Characterization of convolutional neural networks for the identification of galaxy-galaxy strong lensing events
• A Halo Model with Environment Dependence: Theoretical Considerations
• Energy-dependent Boosted Dark Matter from Diffuse Supernova Neutrino Background
• Testing the interaction of dark energy to dark matter through the analysis of virial relaxation of clusters Abell Clusters A586 and A1689 using realistic density profiles
• Discovery of a double radio relic in ZwCl1447.2+2619: A rare testbed for shock acceleration models with a peculiar surface brightness ratio
• K-CLASH: spatially-resolving star-forming galaxies in field and cluster environments at $z\approx 0.2$-$0.6$
• Discriminating power of milli-lensing observations for dark matter models
• The prolate dark matter halo of the Andromeda galaxy
• Dynamical Models for NGC 6503 using a Markov Chain Monte Carlo Technique
• Evidence for a Rotational Component in the Circumgalactic Medium of Nearby Galaxies
• Strange Quark Stars as Probe of Dark Matter
• Structure and dynamics of the supercluster of galaxies SC0028-0005
• Galaxy Tagging: photometric redshift refinement and group richness enhancement
• The Circumgalactic Medium of Submillimeter Galaxies. I. First Results from a Radio-Identified Sample
• Explaining the Energetic AGN Outburst of MS0735+7421 with Massive Slow Jets
• Identikit 2: An Algorithm for Reconstructing Galactic Collisions
• The universality of the rapid neutron-capture process revealed by a possible disrupted dwarf galaxy star
• Gas outflows in Seyfert galaxies: effects of star formation versus AGN feedbacks
• The mass distribution of a moderate redshift galaxy group and brightest group galaxy from gravitational lensing and kinematics
• A shallow dark matter halo in Ultra Diffuse Galaxy AGC 242019: are UDGs structurally similar to low surface brightness galaxies?
• Slow evolution of elliptical galaxies induced by dynamical friction
• Data-Based Optimal Bandwidth for Kernel Density Estimation of Statistical Samples
• The effects of the small-scale behaviour of dark matter power spectrum on CMB spectral distortion
• Strong Lensing Analysis of the Cluster RCS0224-0002 at $z=0.77$
• The Hateful Eight: Connecting Massive Substructures in Galaxy Clusters like Abell 2744 to their Dynamical Assembly State using the Magneticum Simulations
• Milky Way and M31 rotation curves: $\Lambda$CDM vs. MOND
• Optimizing Energetic Light Dark Matter Searches in Dark Matter and Neutrino Experiments
• Wormholes admitting conformal Killing vectors and supported by generalized Chaplygin gas
• Reconsidering the dynamical states of galaxy clusters using PCA and UMAP
• The ALMA-CRISTAL survey: Resolved kinematic studies of main sequence star-forming galaxies at 4<z<6
• Future Island Universes in a Background Universe Accelerated by Cosmological Constant and by Quintessence
• The radial dependence of dark matter distribution in M33
• Mapping the dark matter halo of early-type galaxy NGC 2974 through orbit-based models with combined stellar and cold gas kinematics
• Effect of Population III Multiplicity on Dark Star Formation
• Dark Matter in Galaxies: Observational overview
• Flat rotation curves using scalar-tensor theories
• A thin disk in higher dimensional space-time and dark matter interpretation
• The ground-state of General Relativity, Topological Theories and Dark Matter
• Rotation curve bifurcations as indicators of close recent galaxy encounters
• Realistic triaxial density--potential--force profiles for stellar systems and dark matter halos
• Radial structure, inflow & central mass of stationary radiative galaxy clusters
• Signatures of the Baryon Acoustic Oscillations on 21cm Emission Background
• Numerical simulations on the relative importance of starbursts and AGN in ultra-luminous infrared galaxies
• Testing modified gravity at large distances with the HI Nearby Galaxy Survey's rotation curves
• The Clustering of Extremely Red Objects
• Modeling HI distribution and kinematics in the edge-on dwarf irregular galaxy KK250
• A common surface-density scale for the Milky Way and Andromeda dwarf satellites as a constraint on dark matter models
• Footprint of Triplet Scalar Dark Matter in Direct, Indirect Search and Invisible Higgs Decay
• The effect of dark matter resolution on the collapse of baryons in high redshift numerical simulations
• Future sensitivity of neutrino telescopes to dark matter annihilations from the cosmic diffuse neutrino signal
• Inert Dark Matter in Type-II Seesaw
• Search for gamma-ray line features from Milky Way satellites with Fermi-LAT Pass 8 data
• Formation and evolution of blue compact dwarfs: The origin of their steep rotation curves
• Testing baryon-induced core formation in $\Lambda$CDM: A comparison of the DC14 and coreNFW dark matter halo models on galaxy rotation curves
• The Extended Disk Galaxy Exploration Science Survey: Description and Surface Brightness Profile Properties
• Mass models of gas-rich void dwarf galaxies
• Characterising the Structure of Halo Merger Trees Using a Single Parameter: The Tree Entropy
• MeerKAT-16 HI observation of the dIrr galaxy WLM
• Separate Universe calibration of the dependence of halo bias on cosmic web anisotropy
• Unveiling the internal structure of Hercules supercluster
• Potential Black Hole Seeding of the Spiral Galaxy NGC 4424 via an Infalling Star Cluster
• Illuminating the Darkest Galaxies
• How Close Dark Matter Halos and MOND Are to Each Other: Three-Dimensional Tests Based on Gaia DR2
• TDCOSMO VIII: A key test of systematics in the hierarchical method of time-delay cosmography
• Analytical approach to core-halo structure of fuzzy dark matter
• The Quest for the Nature of the Dark Matter: The Need of a New Paradigm
• Luminous giants populate the dense Cosmic Web: The radio luminosity-environmental density relation for radio galaxies in action
• A million-solar-mass object detected at cosmological distance using gravitational imaging
• On the Formation of GW231123 in Population III Star Clusters
• Geodesics and scalar perturbations of Schwarzschild black holes embedded in a Dehnen-type dark matter halo with quintessence
• Extreme mass ratio inspirals in dark matter halos: dynamics and distinguishability of halo models
• Constraints on dark matter with future MeV gamma-ray telescopes
• Signatures of dark and baryonic structures on weakly lensed gravitational waves
• Novel bounds on decaying axionlike particle dark matter from the cosmic background
• On the Galactic rotation curve inferred from the Jeans equations Assessing its robustness using Gaia DR3 and cosmological simulations
• Examining the effects of dark matter spikes on eccentric intermediate mass ratio inspirals using N-body simulations
• The magnetised and thermally unstable tails of jellyfish galaxies
• Primordial Black Hole Merger Rate in $f(R)$ Gravity
• The Spectacular Tidal Tails of Globular Cluster M3 (NGC 5272)
• Constraints on late-forming exploding black holes
• A physical and concise halo model based on the depletion radius
• The Merger Rate of Primordial Black Hole-Neutron Star Binaries in Ellipsoidal-Collapse Dark Matter Halo Models
• Residuals of an Equilibrium Model for the Galaxy Reveal a State of Disequilibrium in the Solar Neighborhood
• X-ray morphology of cluster-mass haloes in self-interacting dark matter
• The halo model with beyond-linear halo bias: unbiasing cosmological constraints from galaxy-galaxy lensing and clustering
• Comparing weak lensing peak counts in baryonic correction models to hydrodynamical simulations
• Multi-component DHOST analysis in galaxy clusters
• Dark Matter search in dwarf irregular galaxies with the Fermi Large Area Telescope
• Farpoint: A High-Resolution Cosmology Simulation at the Gigaparsec Scale
• Search for gas accretion imprints in voids: II. The galaxy Ark 18 as a result of a dwarf-dwarf merger
• Super-sample covariance of the thermal Sunyaev-Zel'dovich effect
• Correlation function: biasing and fractal properties of the cosmic web
• RELICS: A Very Large (${\theta }_E\sim 40"$) Cluster Lens -- RXC J0032.1+1808
• The Dragonfly Edge-on Galaxies Survey: Shaping the outer disc of NGC 4565 via accretion
• Searching for Solar Siblings in APOGEE and $Gaia$ DR2 with N-body Simulations
• Calibrating the cosmic distance ladder using gravitational-wave observations
• Galaxy rotation curves using a non-parametric regression method: core, cusp and fuzzy scalar field dark matter models
• Search for Dark Matter Gamma-ray Emission from the Andromeda Galaxy with the High-Altitude Water Cherenkov Observatory
• Downsizing of Star Formation Measured from the Clustered Infrared Background Correlated with Quasars
• Merger history of central galaxies in Semi-Analytic Models of galaxy formation
• Kinetic Field Theory: Exact free evolution of Gaussian phase-space correlations
• Halo mass and weak galaxy-galaxy lensing profiles in rescaled cosmological $N$-body simulations
• Multiwavelength study of X-ray Luminous Clusters in the Hyper Suprime-Cam Subaru Strategic Program S16A field
• Next Generation Virgo Cluster Survey. XXI. The weak lensing masses of the CFHTLS and NGVS RedGOLD galaxy clusters and calibration of the optical richness
• Using galaxy pairs to investigate the three-point correlation function in the squeezed limit
• Description of the evolution of inhomogeneities on a Dark Matter halo with the Vlasov equation
• HI in the Outskirts of Nearby Galaxies
• 3FGL J1924.8-1034 : A Spatially-Extended Stable Unidentified GeV Source?
• Galaxy Clustering in 3D and Modified Gravity Theories
• Probing the gaseous halo of galaxies through non-thermal emission from AGN-driven outflows
• The X-shooter Lens Survey - II. Sample presentation and spatially resolved kinematics
• Non-virialised clusters for detection of Dark Energy-Dark Matter interaction
• Phase Space dynamics of triaxial collapse: Joint density-velocity evolution
• Plan beta: Core or Cusp?
• Internal Cluster Structure
• Chandra and optical/IR observations of CXOJ1415.2+3610, a massive, newly discovered galaxy cluster at z~1.5
• Exploring the non-linear density field in the Millennium simulations with tessellations - I. The probability distribution function
• The rates and time-delay distribution of multiply imaged supernovae behind lensing clusters
• Mass and pressure constraints on galaxy clusters from interferometric SZ observations
• Surface mass density of the Einasto family of dark matter haloes: Are they Sersic-like?
• Simple Models for the Distribution of Dark Matter
• An examination of magnetized outflows from active galactic nuclei in galaxy clusters
• The effects of primordial non-Gaussianity on giant-arc statistics
• Simulated evolution of the dark matter large-scale structure
• The Halo Occupation Distribution of Black Holes: Dependence on Mass
• Estimate of dark halo ellipticity by lensing flexion
• A parametric physical model for the intracluster medium and its use in joint SZ/X-ray analyses of galaxy clusters
• Pressure from dark matter annihilation and the rotation curve of spiral galaxies
• Galaxy-Galaxy Lensing by Non-Spherical Haloes I:Theoretical Considerations
• The lensing efficiencies of MACS X-ray selected versus RCS optically selected galaxy clusters
• Testing the Dark Matter Annihilation Model for the WMAP Haze
• Muon Fluxes and Showers from Dark Matter Annihilation in the Galactic Center
• BDM Dark Matter: CDM with a core profile and a free streaming scale
• Neutralino dark matter stars can not exist
• keV Warm Dark Matter via the Supersymmetric Higgs Portal
• The spacetime associated with galactic dark matter halos
• Observational Cosmology
• Halo asphericity and the shear 3-pt function
• Massive Black Holes in Dwarf Spheroidal Galaxy Haloes?
• The potential-energy tensors for subsystems. IV. Homeoidally striated density profiles with a central cusp
• Cluster Mass Estimate and a Cusp of the Mass Density Distribution in Clusters of Galaxies
• Gaussian Peaks and Clusters of Galaxies
• Scale Invariance of Rich Cluster Abundance: A Possible Test for Models of Structure Formation
• Density cusps: restrictions on non-axisymmetric models
• High-Resolution Simulations of Cluster Formation
• Multi-GeV photons from electron-dark matter scattering near Active Galactic Nuclei
• Dark Matter and Cosmology: CDM with a Cosmological Constant ($\Lambda$CDM) vs. CDM with Hot Dark Matter (CHDM)
• A Second Shell in the Fornax dSph Galaxy
• The Distribution of Mass in the Orion Dwarf Galaxy
• Isotropic extragalactic flux from dark matter annihilations: lessons from interacting dark matter scenarios
• Asymmetric velocity anisotropies in remnants of collisionless mergers
• Microwave background anisotropies and non-linear structures II. Numerical computations
• Exploring SUSY light Higgs boson scenarios via dark matter experiments
• Comparing the dark matter models, modified Newtonian dynamics and modified gravity in accounting for the galaxy rotation curves
• An efficient positive potential-density pair expansion for modelling galaxies
• Testing Cold Dark Matter Models At Moderate to High Redshift
• Is there a disk of satellites around the Milky Way?
• Environmental screening of dark matter haloes in $f(R)$ gravity
• The Universal Rotation Curve of Spiral Galaxies
• Dark matter substructure cannot explain properties of the Fermi Galactic Centre excess
• Ultra High Energy Cosmic Rays & Super-heavy Dark Matter
• Dark Matter Subhalos in the Ursa Minor Dwarf Galaxy
• The time evolution of gaps in tidal streams
• Starburst Nuclei as Light Dark Matter Laboratories
• Fitting a Self-Interacting Dark Matter Model to Data Ranging From Satellite Galaxies to Galaxy Clusters
• Cy 2201-3201: An Edge-on Spiral Gravitational Lens
• Clouds accreting from the IGM are not able to feed the star formation of low-redshift disc galaxies
• Dark Matter Prospects in Deflected Mirage Mediation
• New metrics to probe the dynamical state of galaxy clusters
• Gamma rays from Dark Matter Annihilation in the Central Region of the Galaxy
• The transformation and quenching of simulated gas-rich dwarf satellites within a group environment
• The projected gravitational potential of the galaxy cluster MACS~J1206 derived from galaxy kinematics
• Active galactic nuclei jets simulated with smoothed particle hydrodynamics
• Monochromatic neutrino lines from sneutrino dark matter
• Project Dinos II: Redshift evolution of dark and luminous matter density profiles in strong-lensing elliptical galaxies across 0.1 < z < 0.9
• Incorporating galaxy cluster triaxiality in stacked cluster weak lensing analyses
• Dynamical consequences of CDM merger trees
• The LMC impact on the kinematics of the Milky Way satellites: clues from the running solar apex
• An Interpretation of Flat Density Cores of Clusters of Galaxies by Degeneracy Pressure of Fermionic Dark Matter: A Case Study of Abell 1689
• The isotropic center of NGC 5419 -- A core in formation?
• Inflow of low-metallicity cool gas in the halo of the Andromeda galaxy
• Ram Pressure Stripping and ISM disc Truncation : Prediction vs. Observation
• Decaying dark matter with heavy axino
• Muonphilic Dark Matter explanation of gamma-ray galactic center excess: a comprehensive analysis
• Seen and unseen tidal caustics in the Andromeda galaxy
• Metallicity distribution of the progenitor of the Giant Stellar Stream in the Andromeda Galaxy
• The virial theorem in Eddington-Born-Infeld gravity
• CP Violating Lepton Asymmetry from B Decays in Supersymmetric Grand Unified Theories
• Time Delay of Light in the Gravitational lensing of Supermassive Black Holes in Dark Matter Halos
• Search for gamma-ray line signals around the black hole at the galactic center with DAMPE observation
• The photoionization effect of the ultraviolet background on the colour-magnitude relation of elliptical galaxies
• Tidal Torques and Galactic Warps
• Revisiting the luminosity function of single halo white dwarfs
• Culminating the peak CUSP to descry the dark side of halos
• An indirect dark matter search with diffuse gamma rays from the Galactic Centre with the Alpha Magnetic Spectrometer
• Mass estimation in the outer non-equilibrium region of galaxy clusters
• Stringent constraint on the radio signal from dark matter annihilation in dwarf spheroidal galaxies using the TGSS
• Self-gravitating Equilibria of Non-minimally Coupled Dark Matter Halos
• Core Fragmentation in Simplest Superfluid Dark Matter Scenario
• ${\mu }_{\star }$ Masses: Weak Lensing Calibration of the Dark Energy Survey Year 1 redMaPPer Clusters using Stellar Masses
• Using LSST Microlensing to Constrain Dark Compact Objects in Spherical and Disk Configurations
• Astronomy with energy dependent flavour ratios of extragalactic neutrinos
• Vector modes in $\Lambda$CDM: the gravitomagnetic potential in dark matter haloes from relativistic $N$-body simulations
• Gravitational anti-screening as an alternative to dark matter
• SHALOS: Statistical Herschel-ATLAS Lensed Objects Selection
• A Comparison of Galaxy Group Luminosity Functions from Semi-Analytic Models
• Analytical halo models of cosmic tidal fields
• The Morphology of the Thermal Sunyaev-Zel'dovich Sky
• Fast cloud-cloud collisions in a strongly barred galaxy: Suppression of massive star formation
• Ram pressure stripping in the EAGLE simulation
• Halo Acceleration Relation
• Boltzmann hierarchies for self-interacting warm dark matter scenarios
• A z=1.85 galaxy group in CEERS: evolved, dustless, massive intra-halo light and a brightest group galaxy in the making
• Group galaxy number density profiles far out: is the 'one-halo' term NFW out to $>10$ virial radii?
• Uncovering the Orbit of the Hercules Dwarf Galaxy
• Evolution of Dark Matter Phase-Space Density Distributions in Equal-Mass Halo Mergers
• Cold Mode Gas Accretion on Two Galaxy Groups at z$\sim$2
• Tidal Disruption Events and Dark Matter Scatterings with Neutrinos and Photons
• Improved mass constraints for two nearby strong-lensing elliptical galaxies from Hubble Space Telescope Imaging
• Is a Bose-Einstein Condensate a good candidate for Dark Matter? A test with Galaxy Rotation Curves
• Mass Calibration of the CODEX Cluster Sample using SPIDERS Spectroscopy -- II. The X-ray Luminosity-Mass Relation
• Constraints on cosmic strings from ultracompact minihalos
• Mass assembly history and infall time of the Fornax dwarf spheroidal galaxy
• A new framework for numerical simulations of structure formation
• Gravitational lensing in low-redshift clusters of galaxies: the arc-like object in Abell 3408 and its lensing interpretation
• A systematic study of the inner rotation curves of galaxies observed as part of the GASS and COLD GASS surveys
• A New Collisional Ring Galaxy at z = 0.111: Auriga's Wheel
• Dynamical Models for Disk Galaxies with Triaxial Halos
• A hyper-runaway white dwarf in Gaia DR2 as a Type Iax supernova primary remnant candidate
• Hydrostatic Mass Profiles of Galaxy Clusters in the eROSITA Survey
• Cluster-Cluster Lensing and the Case of Abell 383
• On the dark matter haloes inner structure and galaxy morphology
• The Anisotropy of the Extragalactic Radio Background from Dark Matter Annihilation
• The special growth history of central galaxies in groups and clusters
• MHONGOOSE discovery of a gas-rich low-surface brightness galaxy in the Dorado Group
• Numerical Simulations of Galaxy Formation
• The COSMOS-Web Lens Survey (COWLS) I: Discovery of >100 high redshift strong lenses in contiguous JWST imaging
• A redshift survey of the nearby galaxy cluster Abell 2107: Global rotation of the cluster and its connection to large-scale structures in the universe
• Prospects for Detecting Gamma Rays from Annihilating Dark Matter in Dwarf Galaxies in the Era of DES and LSST
• Stellar Feedback and the Energy Budget of Late-Type Galaxies: Missing Baryons and Core Creation
• A Model for the Density Distribution of Virialized CDM Halos
• On the absence of gravitational lensing of the cosmic microwave background
• Effects of hot halo gas on the star formation and mass transfer during distant galaxy-galaxy encounters
• Phase-Space Density Profiles in Scale-Free Cosmologies
• Looking for Traces of Non-minimally Coupled Dark Matter in the X-COP Galaxy Clusters Sample
• JUNO sensitivity to the annihilation of MeV dark matter in the galactic halo
• Dark Matter Mounds: towards a realistic description of dark matter overdensities around black holes
• Multi-TeV dark matter density in the inner Milky Way halo: spectral and dynamical constraints
• Environmental dependence of AGN activity and star formation in galaxy clusters from Magneticum simulations
• Nested solitons in two-field fuzzy dark matter
• Additional bounds on the pre Big--Bang--Nucleosynthesis Expansion by means of $\gamma$-rays from the Galactic Center
• Accurate Computation of the Screening of Scalar Fifth Forces in Galaxies
• Isolated pulsar population synthesis with simulation-based inference
• Hydrostatic gas distributions: global estimates of temperature and abundance
• Formation of emission line dots and extremely metal-deficient dwarfs from almost dark galaxies
• Star formation and bar instability in cosmological haloes
• A search for neutrino signal from dark matter annihilation in the center of the Milky Way with Baikal NT200
• Consequences of dark matter self-annihilation for galaxy formation
• Gravitational microlensing as a probe for dark matter clumps
• Golden gravitational lensing systems from the Sloan Lens ACS Survey. II. SDSS J1430+4105: A precise inner total mass profile from lensing alone
• Kinematics and dynamics of the M51-type galaxy pair NGC 3893/96 (KPG 302)
• Two cosmological models for clusters of galaxies
• The Dark Matter distribution function and Halo Thermalization from the Eddington equation in Galaxies
• Heating of galactic gas by dark matter annihilation in ultracompact minihalos
• A universal angular momentum profile for dark matter haloes
• Natural emergence of neutrino masses and dark matter from $R$-symmetry
• The role of shell crossing on the existence and stability of trapped matter shells in spherical inhomogeneous Λ-CDM models
• Clustering of MgII absorption line systems around massive galaxies: an important constraint on feedback processes in galaxy formation
• Cosmic Ray Anomalies from the MSSM?
• Plasma Constraints on the Cosmological Abundance of Magnetic Monopoles and the Origin of Cosmic Magnetic Fields
• Resolution of the apparent discrepancy between the number of massive subhaloes in Abell 2744 and ΛCDM
• Cosmological implications of a Dark Matter self-interaction energy density
• What the Milky Way's Dwarfs tell us about the Galactic Center extended excess
• A solution to the problems of cusps and rotation curves in dark matter halos in the cosmological standard model
• Diagnostics of Baryonic Cooling in Lensing Galaxies
• Dark matter halos in the multicomponent model. II. Density profiles of galactic halos
• Stellar mass dependence of the 21-cm signal around the first star and its impact on the global signal
• Manifestly Gauge Invariant Perturbations of Scalar-Tensor Theories of Gravity
• Decaying axinolike dark matter: Discriminative solution to small-scale issues
• An Alternative Channel For High-Mass Binary Black Holes-----Dark Matter Accretion Onto Black Hole
• Impact of radio sources and cosmic infrared background on thermal Sunyaev-Zel'dovich - gravitational lensing cross correlation
• Testing gravity with halo density profiles observed through gravitational lensing
• Ram pressure stripping of the hot gaseous haloes of galaxies using the k-epsilon sub-grid turbulence model
• GHASP: an H$\alpha$ kinematics survey of spiral galaxies - XII. Distribution of luminous and dark matter in spiral and irregular nearby galaxies using R${}_c$-band photometry
• Detectability of Weak Lensing Modifications under Galileon Theories
• Dark Matter In Disk Galaxies II: Density Profiles as Constraints on Feedback Scenarios
• A Clustering Analysis of the Morphology of the 130 GeV Gamma-Ray Feature
• Dark Matter Signatures of Supermassive Black Hole Binaries
• Globular clusters as probes of dark matter cusp-core transformations
• Where Do Cooling Flows Cool?
• The SFR-radius connection: data and implications for wind strength and halo concentration
• The Bosma effect revisited - I. HI and stellar disc scaling models
• The radial acceleration relation and dark baryons in MOND
• Statistical Properties of Thermal Sunyaev-Zel'dovich Maps
• Classifying the formation processes of S0 galaxies using Convolutional Neural Networks
• The eccentricity enhancement effect of intermediate-mass-ratio-inspirals: dark matter and black hole mass
• The parallelism between galaxy clusters and early-type galaxies: I. The light and mass profiles
• Properties of galaxy halos in Clusters and Voids
• Using GAMA to probe the impact of small-scale galaxy physics on nonlinear redshift-space distortions
• The Small Scale Velocity Dispersion of Galaxies: A Comparison of Cosmological Simulations
• Deep learning the astrometric signature of dark matter substructure
• The impact of turbulent mixing on the galactic r-process enrichment by binary neutron star mergers
• Signals of Axion Like Dark Matter in Time Dependent Polarization of Light
• The Discovery of a Hidden Broad Line AGN in a Bulgeless Galaxy: Keck NIR Spectroscopic Observations of SDSS J085153.64+392611.76
• Modeling Photoionized Turbulent Material in the Circumgalactic Medium II: Effect of Turbulence within a Stratified Medium
• Analyzing the Galactic pulsar distribution with machine learning
• Black hole fueling in galaxy mergers: A high-resolution analysis
• Searching for eV-mass Axion-like Particles with Cross Correlations between Line Intensity and Weak Lensing Maps
• The Structure of Dark Matter Halos in an Annihilating Dark Matter Model
• The Puzzling Origin of Massive Compact Galaxies in MaNGA
• The Fine Structure and Outskirts of DDO 154
• Constraining density and metallicity of the Milky Way's hot gas halo from O VII spectra and ram-pressure stripping
• Stellar Shocks From Dark Matter Asteroid Impacts
• Searching for pseudo Nambu-Goldstone boson dark matter production in association with top quarks
• Empirical Evidence of Non-Minimally Coupled Dark Matter in the Dynamics of Local Spiral Galaxies?
• The ALFALFA HI velocity width function
• Solving the Cusp-Core Problem with a Novel Scalar Field Dark Matter
• Cuspy dark matter density profiles in massive dwarf galaxies
• Where are the missing baryons in clusters?
• Rotating Kerr-Newman space-times in Metric-Affine Gravity
• Likelihood-free Forward Modeling for Cluster Weak Lensing and Cosmology
• Fermi bubbles: the collimated outburst needed to explain forward-shock edges
• The first detection of weak gravitational shear in infrared observations: Abell 1689
• $J$-factors for Velocity-dependent Dark Matter
• Dark matter produced from neutrinos
• An intergalactic medium temperature from a giant radio galaxy
• Constraints on ultralight axions, vector gauge bosons, and unparticles from geodetic and frame-dragging measurements
• Galactic satellite systems in CDM, WDM and SIDM
• The cosmology dependence of the concentration-mass-redshift relation
• Dust grain size evolution in local galaxies: a comparison between observations and simulations
• Dynamical limits on galactic winds, halo machos and intergalactic globular clusters
• Properties of globular clusters formed in dark matter mini-halos
• Flat spectrum radio quasars and BL Lacs dominate the anisotropy of the unresolved gamma-ray background
• Neutrino astronomy as a probe of physics beyond the Standard Model: decay of sub-MeV $B$-$L$ gauge boson dark matter
• The dark matter content of the blue compact dwarf NGC 2915
• Halo Occupation Distribution of Emission Line Galaxies: fitting method with Gaussian Processes
• Classifying the satellite plane membership of Centaurus A's dwarf galaxies using orbital alignment constraints
• KiDS+VIKING+GAMA: Halo occupation distributions and correlations of satellite numbers with a new halo model of the galaxy-matter bispectrum for galaxy-galaxy-galaxy lensing
• Scaling relations of z~0.25-1.5 galaxies in various environments from the morpho-kinematic analysis of the MAGIC sample
• Origin of rotational kinematics in the globular cluster system of M31: A new clue to the bulge formation
• Turbulent Heating in a Stratified Medium
• Black Hole Solutions and Pressure Terms in Induced Gravity with Higgs Potential
• Black Holes and Galactic Density Cusps : From Black Hole to Bulge
• The Local Group Symbiotic Star Population and its Tenuous Link with Type Ia Supernovae
• Superheavy dark matter as UHECR source versus the SUGAR data
• Matching the mass function of Milky Way satellites in competing dark matter models
• Baryon oscillations in galaxy and matter power-spectrum covariance matrices
• Ironing the folds: The phase space chevrons of a GSE-like merger as a dark matter subhalo detector
• Lens modelling and H_0 estimate in quadruply lensed systems
• Dark Matter in X-rays: Revised XMM-Newton Limits and New Constraints from eROSITA
• On the Merger Rate of Primordial Black Holes in Cosmic Voids
• The PSZ-MCMF catalogue of Planck clusters over the DES region
• Direct tests of General Relativity under screening effect with galaxy-scale strong lensing systems
• Galaxy clusters in high definition: a dark matter search
• Reconstructing the extended structure of multiple sources strongly lensed by the ultra-massive elliptical galaxy SDSS J0100+1818
• The SRG/eROSITA All-Sky Survey : Subaru/HSC-SSP weak-lensing mass measurements for the eRASS1 Galaxy Clusters
• Effect of a High-Precision Semi-Analytical Mass Function on the Merger Rate of Primordial Black Holes in Dark Matter Halos
• MeV to multi-TeV thermal WIMPs: most conservative limits
• Thermodynamics of static and stationary black holes in Einstein-Gauss-Bonnet gravity with dark matter
• Improved analytical modeling of the non-linear power spectrum in modified gravity cosmologies
• CHANCES, the Chilean Cluster Galaxy Evolution Survey: Selection and initial characterisation of clusters and superclusters
• The Dark Halo of NGC 5963 as a Constraint on Dark Matter Self-Interaction at the Low Velocity Regime
• Galaxy cluster rotation revealed in the MACSIS simulations with the kinetic Sunyaev-Zeldovich effect
• Anomalous Ionization in the Central Molecular Zone by sub-GeV Dark Matter
• Constraining Chameleon screening using galaxy cluster dynamics
• Unified view of scalar and vector dark matter solitons
• Stochastic Wave Dark Matter with Fermi-LAT $\gamma$-ray Pulsar Timing Array
• Chandra observations of the galaxy group AWM 5: cool core re-heating and thermal conduction suppression
• Structure of visible and dark matter components in spiral galaxies at redshifts z = 0.5-0.9
• Confrontation of Top-Hat Spherical Collapse against Dark Halos from Cosmological N-Body Simulations
• The first shear measurements from precision weak lensing
• Testing gravity with the Milky Way: Yukawa potential
• Gamma-Ray Constraints on the First Stars from Annihilation of Light WIMPs
• Density and metallicity of the Milky-Way circumgalactic gas
• Hadronic Interactions of Energetic Charged Particles in Protogalactic Outflow Environments and Implications for the Early Evolution of Galaxies
• Lensing in the Hercules Supercluster
• KiDS+VIKING-450: An internal-consistency test for cosmic shear tomography with a colour-based split of source galaxies
• Galactic Center constraints on self-interacting sterile neutrinos from fermionic dark matter ("ino") models
• On the Prospects for Detecting a Net Photon Circular Polarization Produced by Decaying Dark Matter
• Order statistics applied to the most massive and most distant galaxy clusters
• Towards Testing Sterile Neutrino Dark Matter with Spectrum-Roentgen-Gamma Mission
• Mind the gap: The discrepancy between simulation and reality drives interpretations of the Galactic Center Excess
• Comparing bulge RR Lyrae stars with bulge giants -- Insight from 3D kinematics
• Joint cosmology and mass calibration from tSZ cluster counts and cosmic shear
• Constraining superheavy decaying dark matter with directional ultra-high energy gamma-ray limits
• Simulations of galaxy cluster mergers with velocity-dependent, rare and frequent self-interactions
• A Universal Profile of the Dark Matter Halo and the Two-point Correlation Function
• Gravitational lensing by elliptical galaxies
• Dynamical evolutin of quintessence dark energy in collapsing dark matter halos
• Tracing the co-evolution path of super massive black holes and spheroids with AKARI-selected ultra-luminous IR galaxies at intermediate redshifts
• Free-form modelling of galaxy clusters: a Bayesian and data-driven approach
• Microwave Background Anisotropies and Nonlinear Structures I. Improved Theoretical Models
• Non-Gaussian Shape Discrimination with Spectroscopic Galaxy Surveys
• On Galaxies and Homology
• Bayes-X: a Bayesian inference tool for the analysis of X-ray observations of galaxy clusters
• The mass and dynamical state of Abell 2218
• The effect of cluster magnetic field on the Sunyaev Zeldovich power spectrum
• Mass Distribution in Hickson Compact Groups of Galaxies
• Role of galactic gaseous halos in recycling enriched winds from bulges to disks: A new bulge-disk chemical connection
• Magnetic fields in massive spirals: The role of feedback and initial conditions
• Using Fractal Dimensionality in the Search for Source Models of Ultra-High Energy Cosmic Rays
• Direct Simulation Monte Carlo for astrophysical flows: II. Ram pressure dynamics
• $S^5$: New insights from deep spectroscopic observations of the tidal tails of the globular clusters NGC 1261 and NGC 1904
• HI Vertical Structure of Nearby Edge-on Galaxies from CHANG-ES
• Right-Handed Neutrino Dark Matter with Forbidden Annihilation
• A Statistical and Multiwavelength Photometric Analysis of a Young Embedded Open Star Cluster: IC 1590
• Testing the Weak Equivalence Principle using Optical and Near-Infrared Crab Pulses
• Testing Modified Dark Matter with Galaxy Clusters: Does Dark Matter know about the Cosmological Constant?
• Wormhole solutions under the effect of dark matter in $f(R,L_m)$ gravity
• Testing multiflavored ULDM models with SPARC
• A spherical scalar-tensor galaxy model
• KiDS-1000: Weak lensing and intrinsic alignment around luminous red galaxies
• Chemical enrichment in isolated barred spiral galaxies
• The galaxy luminosity function around groups
• Signatures of Light Massive Relics on nonlinear structure formation
• The Structural and Kinematic Evolution of Central Star Clusters in Dwarf Galaxies and Their Dependence on Dark Matter Halo Profiles
• Uncovering substructure with wavelets: proof of concept using Abell 2744
• Local clustering of relic neutrinos with kinetic field theory
• Constraints on dark matter self-interaction from galactic core size
• CHEX-MATE: CLUster Multi-Probes in Three Dimensions (CLUMP-3D), I. Gas Analysis Method using X-ray and Sunyaev-Zel'dovich Effect Data
• Two-mediator dark matter models and cosmic electron excess
• ERO R1 in CL0939+4713 field - Evidence for an S0-like galaxy at z \sim 1.5
• Precision cosmology with baryons: non-radiative hydrodynamics of galaxy groups
• Cosmic Radio Background from Primordial Black Holes at Cosmic Dawn
• Probing compact dark matter objects with microlensing in gravitationally lensed quasars
• A Comparison of Outflow Properties in AGN Dwarfs vs. Star Forming Dwarfs
• Cold dark matter protohalo structure around collapse: Lagrangian cosmological perturbation theory versus Vlasov simulations
• Projection effects of large-scale structures on weak-lensing peak abundances
• Virial Sequences for Thick Discs and Haloes: Flattening and Global Anisotropy
• Local Stellar Kinematics from RAVE data -- VIII. Effects of the Galactic Disc Perturbations on Stellar Orbits of Red Clump Stars
• Dark and luminous matter in the NGC 3992 group of galaxies, II. The dwarf companions UGC 6923, UGC 6940, UGC 6969, and the Tully-Fisher relation
• Determining Supersymmetric Parameters With Dark Matter Experiments
• Impact of tidal environment on galaxy clustering in GAMA
• The weak dependence of velocity dispersion on disk fractions, mass-to-light ratio and redshift: Implications for galaxy and black hole evolution
• Testing DM halos using rotation curves and lensing: A warning on the determination of the halo mass
• Using large scale structure data and a halo model to constrain Generalised Dark Matter
• When Leaving the Solar System: Dark Matter Makes a Difference
• Thermodynamic Evolution of Secluded Vector Dark Matter: Conventional WIMPs and Nonconventional WIMPs
• SASHIMI-SIDM: Semi-analytical subhalo modelling for self-interacting dark matter at sub-galactic scales
• Reconstructing the projected gravitational potential of galaxy clusters from galaxy kinematics
• Evolution of CIV Absorbers. II. Where does CIV live?
• Variation in the Stellar Mass Function Along Stellar Streams
• Model-Independent Mass Reconstruction of the Hubble Frontier Field Clusters with MARS Based on Self-Consistent Strong Lensing Data
• The Infrared Medium-Deep Survey II: How to Trigger Radio-AGN? Hints from Their Environments
• The Chemical Composition of Extreme-Velocity Stars
• A Search for the 3.5 keV Line from the Milky Way's Dark Matter Halo with HaloSat
• Galaxy rotation curves disfavor traditional and self-interacting dark matter halos, preferring a disk component or Einasto function
• Brought to Light I: Quantification of Disk Substructure in Dwarf Early-Type Galaxies
• Cosmology with Galaxy Clusters: Systematic Effects in the Halo Mass Function
• Probing Self-interacting Dark Matter with Disk Galaxies in Cluster Environments
• Resolving Fermi, PAMELA and ATIC anomalies in split supersymmetry without R-parity
• On the Mass Loading of AGN-Driven Outflows in Elliptical Galaxies and Clusters
• Constraining neutrino-DM interactions with Milky Way dwarf spheroidals and supernova neutrinos
• Terrestrial Probes of Electromagnetically Interacting Dark Radiation
• Combining Optical and X-ray Observations of Galaxy Clusters to Constrain Cosmological Parameters
• Gravitational Collapse of Baryonic and Dark matter
• Tilted outer and inner structures in edge-on galaxies?
• `Upper-Limit Lensing': Constraining galaxy stellar masses with singly-imaged background sources
• Probing the structure of the cold dark matter halo with ancient mica
• Searching for dark matter annihilation from individual halos: uncertainties, scatter and signal-to-noise ratios
• On the Origin of Metal-poor Stars in the Solar Neighborhood
• MIFAL: fully automated Multiple-Image Finder ALgorithm for strong-lens modelling -- proof of concept
• Dilaton dominance relaxes LHC and cosmological constraints in supersymmetric models
• Galaxy Halo Masses from Weak Gravitational Lensing
• The signal of decaying dark matter with hydrodynamical simulations
• Cross-correlating Sunyaev-Zel'dovich and Weak Lensing Maps
• The degeneracy of M33 mass modelling and its physical implications
• Constraint on dark matter central density in the Eddington inspired Born-Infeld (EiBI) gravity with input from Weyl gravity
• A deeper look into the structure of ΛCDM haloes: correlations between halo parameters from Einasto fits
• New observational constraints on interacting dark energy using galaxy clusters virial equilibrium states
• Gas sloshing in Abell 2204: Constraining the properties of the magnetized intracluster medium
• Extended Chameleons
• Neutrino Masses, Leptogenesis and Decaying Dark Matter
• The origin of type-I profiles in cluster lenticulars: An interplay between ram pressure stripping and tidally-induced spiral migration
• Dark Matter at the Galactic Center
• Model Independent analysis of MeV scale dark matter: II. Implications from $e^{-}{e}^{+}$ colliders and Direct Detection
• Screening maps of the local Universe I -- Methodology
• Searching for correlations in GAIA DR2 unbound star trajectories
• Confronting recent AMS-02 positron fraction and Fermi-LAT Extragalactic Gamma-Ray Background measurements with gravitino dark matter
• Dark matter inside early-type galaxies as function of mass and redshift
• Jeans that fit: weighing the mass of the Milky Way analogues in the $\Lambda \mathrm{CDM}$ universe
• What made discy galaxies giant?
• Chemodynamical study of two CEMP-no stars from the Hamburg/ESO Survey
• Star Formation of Merging Disk Galaxies with AGN Feedback Effects
• New Light on Dark Extended Lenses with the Roman Space Telescope
• Dark Matter Annihilation in the Circumgalactic Medium at High Redshifts
• The virialization density of peaks with general density profiles under spherical collapse
• Probing the black holes in a dark matter halo of M87 using gravitational wave echoes
• Dark matter indirect signals with long-lived mediators
• Statistical ensembles of virialized halo matter density profiles
• The Logotropic Dark Fluid: Observational and Thermodynamic Constraints
• Cosmic Ray Antihelium from a Strongly Coupled Dark Sector
• Lagrangian Statistics of Dark Halos in a LCDM Cosmology
• Evolution of the phase-space density and the Jeans scale for dark matter derived from the Vlasov-Einstein equation
• The thermal and gravitational energy densities in the large-scale structure of the Universe
• Reconstructing a Model for Gravity at Large Distances from Dark Matter Density Profiles
• Jointly fitting weak lensing, X-ray and Sunyaev-Zel'dovich data to constrain scalar-tensor theories with clusters of galaxies
• Lessons from the first multiply imaged supernova II: A parametric strong-lensing model for the galaxy cluster MACS J1149.5+2223
• Harnessing the Population Statistics of Subhalos to Search for Annihilating Dark Matter
• The Dark Matter Distributions in Low-Mass Disk Galaxies. I. H$\alpha$ Observations Using the Palomar Cosmic Web Imager
• Dynamical friction of radio galaxies in galaxy clusters
• Effects of Chameleon Scalar Field on Rotation Curves of the Galaxies
• Hawking evaporation of cosmogenic black holes in TeV-gravity models
• MaNGA DynPop -- IV. Stacked total density profile of galaxy groups and clusters from combining dynamical models of integral-field stellar kinematics and galaxy-galaxy lensing
• New X-shaped bulge photometric model as a tool for measuring B/PS bulges and their X-structures in photometric studies
• Primordial Black Hole-Neutron Star Merger Rate in Modified Gravity
• Formation of massive globular clusters with dark matter and its implication on dark matter annihilation
• Weak-lensing Mass Reconstruction of Galaxy Clusters with Convolutional Neural Network
• Probing Saraswati's heart: evaluating the dynamical state of the massive galaxy cluster A2631 through a comprehensive weak-lensing and dynamical analysis
• Empirical constraints on alternative gravity theories from gravitational lensing
• Tightening weak lensing constraints on the ellipticity of galaxy-scale dark matter haloes
• One-Dimensional Fuzzy Dark Matter Models: Structure Growth and Asymptotic Dynamics
• Absence of obvious tidal tails around the globular cluster NGC 6397
• Seeing dark matter via acceleration radiation
• Cloud properties across spatial scales in simulations of the interstellar medium
• Bar-driven Leading Spiral Arms in a Counter-rotating Dark Matter Halo
• A Trail of the Invisible: Blue Globular Clusters Trace the Radial Density Distribution of the Dark Matter -- Case Study of NGC 4278
• Frequency of the dark matter subhalo collisions and bifurcation sequence arising formation of dwarf galaxies
• Halo Mass-Concentration Relation at High-Mass End
• Active Galactic Nuclei and Transformation of Dark Matter into Visible Matter
• Light Propagation in Inhomogeneous Universes. III. Distributions of Image Separations
• Measuring Feedback Using the Intergalactic Medium State and Evolution Inferred from the Soft X-ray Background
• An Extra-Dimensional Model of Dark Matter
• Bursty Star Formation in Dwarfs is Sensitive to Numerical Choices in Supernova Feedback Models
• Traversable Wormholes Sourced by Dark Matter in Loop Quantum Cosmology
• Cosmic-ray knee and diffuse gamma, e+ and pbar fluxes from collisions of cosmic rays with dark matter
• Rapid Simulations of Halo and Subhalo Clustering
• EDGE: the puzzling ellipticity of Eridanus II's star cluster and its implications for dark matter at the heart of an ultra-faint dwarf
• Characterization and dynamics of the peculiar stream Jhelum, A tentative role for the Sagittarius dwarf galaxy
• The Andromeda Gamma-Ray Excess: Background Systematics of the Millisecond Pulsars and Dark Matter Interpretations
• The spherical collapse model with shell crossing
• Is the radio emission in the Bullet cluster due to Dark Matter annihilation?
• Neutrino winds on the sky
• Got plenty of nothing: cosmic voids as a probe of particle dark matter
• Scalar-field Pressure in Induced Gravity with Higgs Potential and Dark Matter
• The origin of cores and density profiles of gaseous baryonic structures
• The viability of ultralight bosonic dark matter in dwarf galaxies
• Energy extraction through magnetic reconnection from a Kerr-Newman black hole in perfect fluid dark matter
• Photometric vs dynamical stellar masses and their impact on scaling relations in nearby disc galaxies
• Density Profile Asymptotes at the Centre of Dark Matter Halos
• Biases to primordial non-Gaussianity measurements from CMB secondary anisotropies
• Quasi-Local Evolution of the Cosmic Gravitational Clustering in Halo Model
• Constraining the physics of star formation from CIB-cosmic shear cross-correlations
• Minihalos as probes of the inflationary spectrum: accurate boost factor calculation and new CMB constraints
• Gravitino Dark Matter with Weak-Scale Right-Handed Sneutrino
• Self-gravitating fluid systems and galactic dark matter
• A comparison between the detection of gamma rays and positrons from neutralino annihilation
• Dynamical friction in the primordial neutrino sea
• Is There a Fundamental Line for Disk Galaxies?
• Simulating SZ intensity maps of giant AGN cocoons
• Big Bounce Genesis and Possible Experimental Tests -- A Brief Review
• How to calculate dark matter direct detection exclusion limits that are consistent with gamma rays from annihilation in the Milky Way halo
• Piercing of a solitonic boson star by a black hole
• Subtracting the kinetic Sunyaev-Zeldovich effect from the cosmic microwave background with surveys of large-scale structure
• Dark Matter in B-L Supersymmetric Standard Model with Inverse Seesaw
• A Chandra Study of the Image Power Spectra of 41 Cool Core and Non-Cool Core Galaxy Clusters
• Halo Model Analysis of Cluster Statistics
• Characterising Strong Lensing Galaxy Clusters using the Millennium-XXL and MOKA simulations
• The quasar-galaxy cross SDSS J1320+1644: A probable large-separation lensed quasar
• Dark Stars and Boosted Dark Matter Annihilation Rates
• Velocity Structure of Self-Similar Spherically Collapsed Halos
• High-redshift microlensing and the spatial distribution of dark matter in the form of MACHOs
• The interaction of dark matter cusp with the baryon component in disk galaxies
• Nonlinear growth of structure in cosmologies with damped matter fluctuations
• Cosmic Transients, Einstein's Equivalence Principle and Dark Matter Halos
• Can we use Weak Lensing to Measure Total Mass Profiles of Galaxies on 20 kiloparsec Scales?
• A weak lensing analysis of the PLCK G100.2-30.4 cluster
• A Likely Super Massive Black Hole Revealed by its Einstein Radius in Hubble Frontier Fields Images
• Solitons and halos for self-interacting scalar dark matter
• Constraints on the primordial power spectrum of small scales using the neutrino signals from the dark matter decay
• Gravitational Lensing by Burkert Halos
• The insight into the dark side. I. The pitfalls of the dark halo parameters estimation
• A possible challenge for Cold and Warm Dark Matter
• Photometry and dynamics of the minor mergers AM\,1228-260 and AM\,2058-381
• Determining the nature of orbits in disk galaxies with non spherical nuclei
• How well do third-order aperture mass statistics separate E- and B-modes?
• Lensing dispersion of supernova flux: a probe of nonlinear structure growth
• Fireball anti-nucleosynthesis
• The nature of the progenitor of the M31 North-western stream: globular clusters as milestones of its orbit
• Voronoi Tessellation and Non-parametric Halo Concentration
• Imprint of primordial non-Gaussianity on dark matter halo profiles
• Unveiling the Influence of Dark Matter in Axially Symmetric Galaxies
• ARCRAIDER I: Detailed optical and X-ray analysis of the cooling flow cluster Z3146
• Spherically symmetric and static solutions in $f(R)$ gravity coupled with EM fields
• Collisional interaction limits between dark matters and baryons in `cooling flow' clusters
• Suzaku X-ray Follow-up Observation of Weak-lensing-detected Halos in the Field around ZwCl0823.2+0425
• Core-Cusp revisited and Dark Matter Phase Transition Constrained at O(0.1) eV with LSB Rotation Curve
• The dynamics of Galactic centre pulsars: constraining pulsar distances and intrinsic spin-down
• A new formation model for omega Centauri: the crossroad of astrophysical processes
• Towards understanding thermal history of the Universe through direct and indirect detection of dark matter
• The Supersonic Project: The eccentricity and rotational support of SIGOs and DM GHOSts
• A Froggatt-Nielsen Model for Leptophilic Scalar Dark Matter Decay
• Stirring N-body systems: Universality of end states
• Gravitational Lensing of Spherically Symmetric Black Holes in Dark Matter Halos
• Constraining the Milky Way Mass with Its Hot Gaseous Halo
• Early-Type Galaxies: Elliptical and S0 Galaxies, or Fast and Slow Rotators
• Revisiting GeV-scale annihilating dark matter with the AMS-02 positron fraction
• Galaxy shapes in Magneticum. I. Connecting stellar and dark matter shapes to dynamical and morphological galaxy properties and the large-scale structure
• Unifying static analysis of gravitational structures with a scale-dependent scalar field gravity as an alternative to dark matter
• Testing emergent gravity with mass densities of galaxy clusters
• Testing feasibility of scalar-tensor gravity by scale dependent mass and coupling to matter
• Resolving the inner accretion flow towards the central supermassive black hole in SDSS J1339+1310
• Quasi-stellar objects and galaxy mass density profiles derived using the submillimetre galaxies magnification bias
• DHOST gravity in Ultra-diffuse galaxies -- Part II: NGC 1052-DF4 and Dragonfly 44
• A semi-analytic model of pairwise velocity distribution between dark matter halos
• How much dark matter is there inside early-type galaxies?
• Light neutralino dark matter in $U(1{)}_X$SSM
• Disk galaxies are self-similar: the universality of the HI-to-Halo mass ratio for isolated disks
• The Stellar Mass - Halo Mass Relation for Low Mass X-ray Groups at 0.5<z<1 in the CDFS with CSI
• The effect of a cusped matter distribution on the formation of brightest cluster members
• On the Cosmic-Ray Spectra of Three-Body Lepton-Flavor-Violating Dark Matter Decays
• An excess of excesses examined via dark matter radio emissions from galaxies
• An off-centred bulge or a satellite? Hydrodynamical $N$-body simulations of the disc galaxy NGC 5474
• Effective Theory for Electroweak Doublet Dark Matter
• On Escaping a Galaxy Cluster in an Accelerating Universe
• Gravitational Lensing of Anisotropic Sources
• A galactic weigh-in: mass models of SINGS galaxies using chemospectrophotometric galactic evolution models
• Dynamical masses of brightest cluster galaxies II: constraints on the stellar IMF
• A Possible Relic Star Cluster in the Sextans Dwarf Galaxy
• Prospects for $\gamma$-ray observations of the Perseus galaxy cluster with the Cherenkov Telescope Array
• Radial Acceleration Relation from Ultra-light Scalar Dark matter
• Interpreting the Fermi-LAT gamma ray excess in the simplified framework
• SMBH growth parameters in the early Universe of Millennium and Millennium-II simulations
• The XMM Cluster Survey: The Halo Occupation Number of BOSS galaxies in X-ray clusters
• Thermal Fluctuations of Dark Matter in Bouncing Cosmology
• Cosmology with Galaxy Cluster Properties using Machine Learning
• The Galactic Center Excess from Z3 Scalar Semi-Annihilations
• Aether scalar tensor theory: Hamiltonian Formalism
• A new test for the stable clustering hypothesis
• Probing galaxy evolution through HI 21-cm emission and absorption: current status and prospects with the Square Kilometre Array
• On the anti-correlation between pericentric distance and inner dark matter density of Milky Way's dwarf spheroidal galaxies
• Constraints on dark matter and astrophysics from tomographic $\gamma$-ray cross-correlations
• The phenomenology of the external field effect in cold dark matter models
• An Empirical Determination of the Dependence of the Circumgalactic Mass Cooling Rate and Feedback Mass Loading Factor on Galactic Stellar Mass
• Illuminating Black Hole Shadow with Dark Matter Annihilation
• 511 keV Line Emission from Nearby Spherical Dwarf Galaxies
• Discy dwarf disruption and the shape of the Galactic halo
• The metallic winds in dwarf galaxies
• Kinematical asymmetry in the dwarf irregular galaxy WLM and a perturbed halo potential
• How an era of kination impacts substructure and the dark matter annihilation rate
• Axisymmetric Schwarzschild models of an isothermal axisymmetric mock dwarf spheroidal galaxy
• A new logotropic model based on a complex scalar field with a logarithmic potential
• Neutrino Mass Limit from Galaxy Cluster Number Density Evolution
• Signatures of afterglows from light dark matter boosted by supernova neutrinos in current and future large underground detectors
• Search for the gamma-ray spectral lines with the DAMPE and the Fermi-LAT observations
• Testing the Dark Matter Caustic Theory Against Observations in the Milky Way
• Galactic Pure Lovelock Blackholes: Geometry, stability, and Hawking temperature
• Evidence of bimodal physical properties of intervening, optically-thin CIII absorbers at z ~ 2.5
• Line-of-sight Elongation and Hydrostatic Mass Bias of the Frontier Fields Galaxy Cluster Abell 370
• A Survey for Large Separation Lensed FIRST Quasars, II. Magnification Bias and Redshift Distribution
• Thermalization, Fragmentation and Tidal Disruption: The Complex Galactic Dynamics of Dark Matter Superfluidity
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations -- I. Constraining physical processes in local star-forming galaxies
• Search for secluded dark matter towards the Galactic Centre with the ANTARES neutrino telescope
• Exploiting magnification bias in ultradeep submillimetre-wave surveys using ALMA
• Non-Halo Structures and their Effects on Gravitational Lensing
• Combining Strong Lensing and Dynamics in Galaxy Clusters: integrating MAMPOSSt within LENSTOOL I. Application on SL2S J02140-0535
• CHAM: a fast algorithm of modelling non-linear matter power spectrum in the sCreened HAlo Model
• Test the Weak Cosmic Supervision Conjecture in Dark Matter-Black Hole System
• The GMRT archive atomic gas survey -- II. Mass modelling and dark matter halo properties across late-type spirals
• Probing dark-matter effects with gravitational waves using the parameterized post-Einsteinian framework
• Radio frequency emissions from dark-matter-candidate magnetized quark nuggets interacting with matter
• The Subaru HSC weak lensing mass-observable scaling relations of spectroscopic galaxy groups from the GAMA survey
• The Carousel Lens: A Well-Modeled Strong Lens with Multiple Lensed Sources
• Galactic disc heating by density granulation in fuzzy dark matter simulations
• The self-confinement of electrons and positrons from dark matter
• The Dark Matter problem
• The effect of pressure-anisotropy-driven kinetic instabilities on magnetic field amplification in galaxy clusters
• BANG-MaNGA: A census of kinematic discs and bulges across mass and star formation in the local Universe
• GCN: a gaseous Galactic halo stream?
• Are symmetric tidal streams possible with long-range dark-matter forces?
• SIMPly add a dark photon
• Formation of Transitional cE/UCD Galaxies through Massive/Dwarf Disc Galaxy Mergers
• Black holes and Galactic density cusps -- I. Radial orbit cusps and bulges
• Coincident SZ and $\gamma$-ray signals from cluster virial shocks
• Determining Satellite Infall Times Using Machine Learning
• A disrupted bulgeless satellite galaxy as counterpart of the ultraluminous X-ray source ESO 243-49 HLX-1
• Modeling the Void H I Column Density Spectrum
• MUSCLE-UPS: Improved Approximations of the Matter Field with the Extended Press-Schechter Formalism and Lagrangian Perturbation Theory
• Missing Dwarf Problem in Galaxy Clusters
• Relativistic distortions in galaxy density-ellipticity correlations: gravitational redshift and peculiar velocity effects
• Pamela, FGST and Sub-Tev Dark Matter
• Detecting Dark Compact Objects in Gaia DR4: A Data Analysis Pipeline for Transient Astrometric Lensing Searches
• Dark matter halos and the M-σrelation for supermassive black holes
• Implications of the Universal Temperature Profile for Galaxy Clusters
• Type II Seesaw with scalar dark matter in light of AMS-02, DAMPE and Fermi-LAT
• Using large galaxy surveys to distinguish z~0.5 quiescent galaxy models
• Rotation curves of galaxies and the stellar mass-to-light ratio
• Constraints on dark matter annihilation from M87: Signatures of prompt and inverse-Compton gamma rays
• Removal and mixing of the coronal gas from satellites in galaxy groups: cooling the intragoup gas
• ALETHEIA: Hunting for Low-mass Dark Matter with Liquid Helium TPCs
• Testing Grumiller's modified gravity at galactic scales
• Cluster-lensing: A Python Package for Galaxy Clusters & Miscentering
• Repository for extended dark matter object constraints
• Photometry and Dynamics of the Minor Merger AM1219-430 with Gemini GMOS-S
• Goldstone models of modified gravity
• The Relationship Between Baryons and Dark Matter in Extended Galaxy Halos
• Constraints on Cold Dark Matter in the Gamma-ray Halo of NGC 253
• Joint HST, VLT/MUSE and XMM-Newton observations to constrain the mass distribution of the two strong lensing galaxy clusters: MACS J0242.5-2132 & MACS J0949.8+1708
• Reliable mass calculation in spherical gravitating systems
• Suppression of thermal conduction in non-cooling flow clusters
• CDM models with a steplike initial power spectrum
• The morphological dependent Tully-Fisher relation of spiral galaxies
• Constraining Dark Energy From Splitting Angle Statistic of Strong Gravitational Lenses
• The impact of the halo spin-concentration relation on disc scaling laws
• NGC 6822 as a probe of dwarf galactic evolution
• The abundance of satellite galaxies in the inner region of $\Lambda$CDM Milky Way sized haloes
• Halo formation and evolution in scalar field dark matter and cold dark matter: New insights from the fluid approach
• Rotation Curves and Nonextensive Statistics
• Stellar velocity dispersion and initial mass function gradients in dissipationless galaxy mergers
• Recovering the mass distribution of an extended gravitational lens
• The Dark Matter Halos of HI Selected Galaxies
• The effect of softening on dynamical simulations of galaxies
• Characterising bars in low surface brightness galaxies
• Cosmic shear statistics in cosmologies with non-Gaussian initial conditions
• Is the non-isothermal double $\beta$-model incompatible with no time evolution of galaxy cluster gas mass fraction ?
• The central dark matter fraction of massive early-type galaxies
• SDSS J1640+1932: a spectacular galaxy-quasar strong lens system
• Testing generalized scalar-tensor theories of gravity with clusters of galaxies
• First direct identification of the barlens vertical structure in galaxy models
• Galactic space-times in modified theories of gravity
• Dark Energy Survey Year 3 Results: Constraints on cosmological parameters and galaxy bias models from galaxy clustering and galaxy-galaxy lensing using the redMaGiC sample
• A Gemini view of the galaxy cluster RXC J1504-0248: insights on the nature of the central gaseous filaments
• The Effect of the Angular Momentum in the Formation and Evolution of Low Surface Brightness Galaxies
• Transonic galactic outflows in a dark matter halo with a central black hole and its application to the Sombrero galaxy
• Spiral galaxies rotation curves in the Horava - Lifshitz gravity theory
• Dark halo microphysics and massive black hole scaling relations in galaxies
• Statistics of the Sunyaev-Zel'dovich Effect power spectrum
• Optical and X-ray profiles in the REXCESS sample of galaxy clusters
• Can galactic dark matter substructure contribute to the cosmic gamma-ray anisotropy?
• Lower mass normalization of the stellar initial mass function for dense massive early-type galaxies at z ~ 1.4
• A sensitive search for unknown spectral emission lines in the diffuse X-ray background with XMM-Newton
• Cross-Correlation Forecast of CSST Spectroscopic Galaxy and MeerKAT Neutral Hydrogen Intensity Mapping Surveys
• On the origin of the asymmetric dwarf galaxy distribution around Andromeda
• Shape Profiles and Orientation Bias for Weak and Strong Lensing Cluster Halos
• Evolution and feedback of AGN Jets of different Cosmic-ray Composition
• Classification of gamma-ray targets for velocity-dependent and subhalo-boosted dark-matter annihilation
• Simplified dark matter models in the light of AMS-02 antiproton data
• High accuracy on $H_0$ constraints from gravitational wave lensing events
• The SAMI Galaxy Survey: understanding observations of large-scale outflows at low redshift with EAGLE simulations
• Universal subhalo accretion in cold and warm dark matter cosmologies
• Addressing $\gamma$-ray emissions from dark matter annihilations in 45 milky way satellite galaxies and in extragalactic sources with particle dark matter models
• Weak-Lensing Analysis of the Complex Cluster Merger Abell 746 with Subaru/Hyper Suprime-Cam
• Revisiting simplified dark matter models in terms of AMS-02 and Fermi-LAT
• Simulating a slow bar in the low surface brightness galaxy UGC 628
• Non-adiabatic evolution of dark sector in the presence of $U(1{)}_{L_{\mu }-L_{\tau }}$ gauge symmetry
• Constraining dark matter annihilation with HSC Low Surface Brightness Galaxies
• Phase-space structure analysis of self-gravitating collisionless spherical systems
• Joint Strong and Weak Lensing Analysis of the Massive Cluster Field J0850+3604
• The Last Journey. II. SMACC -- Subhalo Mass-loss Analysis using Core Catalogs
• Near-infrared Extragalactic Background Light Fluctuations on Nonlinear Scales
• Cooling flows and the entropy of the intragroup medium
• What to expect when using globular clusters as tracers of the total mass distribution in Milky Way-mass galaxies
• Highly-magnified, Multiply-imaged radio counterparts of the Sub-mm Starburst Emission in the Cluster-Lens MS0451.6-0305
• Strong Lensing and $H_0$
• Extensions and applications of the iterative method
• Upper limits on the dark matter content in globular clusters
• Condensation of Galactic Cold Dark Matter
• The quasi-adiabatic relaxation of haloes in the IllustrisTNG and EAGLE cosmological simulations
• Super-exponential cutoff as a probe of annihilating dark matter
• Core Structure of Intracluster Gas: Effects of Radiative Cooling on Core Sizes
• The RINGS Survey I: Halpha and HI Velocity Maps of Galaxy NGC 2280
• Evolution of the high-mass end of the stellar initial mass functions in starburst galaxies
• Galactic phase transition at Ec=0.11 eV from rotation curves of cored LSB galaxies and nonperturbative dark matter mass
• Comparing Lensing and Stellar Orbital Models of a Nearby Massive Strong-Lens Galaxy
• Determining all gas properties in galaxy clusters from the dark matter distribution alone
• Warped Radion Dark Matter
• Molecular Gas of the Most Massive Spiral Galaxies I: a Case Study of NGC 5908
• MIRACLE I.: Unveiling the Multi-Phase, Multi-Scale physical properties of the Active Galaxy NGC 424 with MIRI, MUSE, and ALMA
• New constraints on cosmic ray-boosted dark matter from the LUX-ZEPLIN experiment
• Type Ia Supernova Magnitude Step from the local Dark Matter Environment
• Possible explanation of indirect gamma ray signatures from hidden sector fermionic dark matter
• Empirical velocity profiles for galactic rotation curves
• Cosmological test of local position invariance from the asymmetric galaxy clustering
• Radio bounds on the mixed dark matter scenarios of primordial black holes and WIMPs
• Detecting Low-Mass Perturbers in Cluster Lenses using Curved Arc Bases
• Directional Sensitivity of the NEWSdm Experiment to Cosmic Ray Boosted Dark Matter
• Galactic Geology: Probing Time-Varying Dark Matter Signals with Paleo-Detectors
• Galaxy Bulges As Tests of CDM vs MOND in Strong Gravity
• Comparing Galaxy Clustering in Horizon-AGN Simulated Lightcone Mocks and VIDEO Observations
• Dark Matter with multi-annihilation channels and AMS-02 positron excess and antiproton
• Constraining the mass-concentration relation through weak lensing peak function
• EMPRESS. XII. Statistics on the Dynamics and Gas Mass Fraction of Extremely-Metal Poor Galaxies
• Connecting direct and indirect detection with a dark spike in the cosmic-ray electron spectrum
• A counter-image to the gravitational arc in Abell 1201: Evidence for IMF variations, or a $10^{10}$M${}_{\odot }$ black hole?
• The Mass Distribution of the Unusual Merging Cluster Abell 2146 from Strong Lensing
• Quantifying the influence of bars on action-based dynamical modelling of disc galaxies
• Gravitational Lensing by Galaxy Groups in the Hubble Deep Field
• Emergence of Galactic Morphologies at Cosmic Dawn: Input from Numerical Modeling
• Primordial Feature at the Scale of Superclusters of Galaxies
• An excursion into the core of the cluster lens Abell 1689
• The double-power approach to spherically symmetric astrophysical systems
• A Richness Study of 14 Distant X-ray Clusters From the 160 Square Degree Survey
• The interacting pair of galaxies Arp 82: Integral field spectroscopy and numerical simulations
• Strong lensing by subhalos in the dwarf-galaxy mass range I: Image separations
• Growth of disc-like pseudo-bulges in SDSS DR7 since z = 0.1
• Velocity Distributions from Nonextensive Thermodynamics
• Accretion of Small Satellites and Gas Inflows in a Disc Galaxy
• A Cusp-Core like challenge for Modified Newtonian Dynamics
• Consequences of using a smooth cosmic distance in a lumpy universe: I
• Constraining primordial non-Gaussianity with cosmological weak lensing: shear and flexion
• The MUSE-Faint survey. III. Constraining scalar field dark matter with Antlia B
• A Random Walk Model for Dark Matter Halo Concentrations
• Merging between a Central Massive Black Hole and a Compact Stellar System: A Clue to the Origin of M31'S Nucleus
• DeepGalaxy: Deducing the Properties of Galaxy Mergers from Images Using Deep Neural Networks
• Thermal Regulation and the Star-Forming Main Sequence
• Fermi-LAT measurement of the diffuse gamma-ray emission and constraints on the Galactic Dark Matter signal
• Imprint of the galactic acceleration scale on globular cluster systems
• A decaying neutralino as dark matter and its gamma ray spectrum
• Conservation of radial actions in time-dependent spherical potentials
• Clustering in the Phase Space of Dark Matter Haloes. I. Results from the Aquarius simulations
• A pseudo-spectrum analysis of galaxy-galaxy lensing
• Modelling H${}_2$ and its effects on star formation using a joint implementation of GADGET-3 and KROME
• Halo shapes constrained from a pure sample of central galaxies in KiDS-1000
• Probing the Halo Gas Distribution in the Inner Galaxy with Fermi Bubble Observations
• Connecting multi-lepton anomalies at the LHC and in Astrophysics with MeerKAT/SKA
• On the Origin of Dust in Galaxy Clusters at Low to Intermediate Redshift
• Dynamical Modeling of NGC 6809: Selecting the best model using Bayesian Inference
• Origins and Interpretation of Tidal Debris
• Resonant Assisted Annihilation
• Non-explosive pre-supernova feedback in the COLIBRE model of galaxy formation
• Viscous time lags between starburst and AGN activity
• Stability and pulsation of the first dark stars
• Tidal Suppression of Fuzzy Dark Matter Heating in Milky Way Satellite Galaxies
• MAGIC and the Search for Signatures of Supersymmetric Dark Matter
• SEEDisCS II. Molecular gas in galaxy clusters and their large scale structure: low gas fraction galaxies, the case of CL1301.7$-$1139
• A panoramic view of the circumgalactic medium in the photoionized precipitation model
• Nonclassicality of axion-like dark matter through gravitational self-interactions
• Beyond Mass: Detecting Secondary Halo Properties with Galaxy-Galaxy Lensing
• Consistent use of Type Ia supernovae highly magnified by galaxy clusters to constrain the cosmological parameters
• Revisit NGC 5466 Tidal Stream with $Gaia$, SDSS/SEGUE and LAMOST
• Cosmic microwave background constraints on extended dark matter objects
• LEGA-C: analysis of dynamical masses from ionized gas and stellar kinematics at z~0.8
• Late-forming black holes and the antiproton, gamma-ray, and anti-helium excesses
• Andromeda XXV -- a dwarf galaxy with a low central dark matter density
• Testing the Origins of Neutrino Mass with Supernova Neutrino Time Delay
• On Mechanics and Thermodynamics of a stellar galaxy in a two-component virial system and the Fundamental Plane
• The Lost Dwarfs of Centaurus A and the Formation of its Dark Globular Clusters
• Hidden Higgs Portal Vector Dark Matter for the Galactic Center Gamma-Ray Excess from the Two-Step Cascade Annihilation, and Muon g-2
• Z-bursts from the Virgo cluster
• Star cluster formation from giant molecular clouds in the Small Magellanic Cloud about 2 Gyr ago: their origin, structures, and kinematics
• Correlation between centre offsets and gas velocity dispersion of galaxy clusters in cosmological simulations
• Dynamics of dwarf galaxies in $f(R)$ gravity
• Numerical convergence of pre-initial conditions on dark matter halo properties
• cp3-bench: A tool for benchmarking symbolic regression algorithms tested with cosmology
• The distribution of annihilation luminosities in dark matter substructure
• Kinematic signatures of impulsive supernova feedback in dwarf galaxies
• Gas accretion and Ram Pressure Stripping of Haloes in Void Walls
• The survival of dynamical fossils in dwarf spheroidal galaxies in conventional and modified dynamics
• The ALMA-CRISTAL survey: Extended [CII] emission in an interacting galaxy system at z ~ 5.5
• Modelling the Track of the GD-1 Stellar Stream Inside a Host with a Fermionic Dark Matter Core-Halo Distribution
• HI HOD -- I. The Halo Occupation Distribution of HI Galaxies
• CHEX-MATE: the intracluster medium entropy distribution in the gravity-dominated regime
• Secular evolution of galaxies and galaxy clusters in decaying dark matter cosmology
• A Comparison of Simple Mass Estimators for Galaxy Clusters
• A major galaxy cluster merger caught by eROSITA: weak lensing mass distribution and kinematic description
• Galaxy cluster mass density profile derived using the submillimetre galaxies magnification bias
• Euclid preparation LXXI. Simulations and nonlinearities beyond $\mathsf{\Lambda }$CDM. 3. Constraints on $f(R)$ models from the photometric primary probes
• Black Hole Feeding and Feedback in a Compact Galaxy
• Observational constraint on axion dark matter in a realistic halo profile with gravitational waves
• The extended Planetary Nebula Spectrograph (ePN.S) early-type galaxy survey: The specific angular momentum of ETGs
• Gravitational Lensing in More Realistic Dark Matter Halo Models
• Dynamical mass distribution and velocity structure of the Galactic centre
• Red-Giant Branch Stellar Cores as Macroscopic Dark Matter Detectors
• A Systematic Effective Operator Analysis of Semi-Annihilating Dark Matter
• Diffuse $\gamma$-rays and $\bar{p}$ flux from dark matter annihilation -- a model for consistent results with EGRET and cosmic ray data
• Anticipating the XRISM search for the decay of resonantly produced sterile neutrino dark matter
• Accurate Analytic Mass-Scale Relations for Dark Matter Haloes of all Masses and Redshifts
• Dynamics of Molecular Gas in the Central Region of the Quasar IZwicky1
• Forming disc galaxies in major mergers II. The central mass concentration problem and a comparison of GADGET3 with GIZMO
• Evolution and instabilities of disks harboring super massive black holes
• Polytropic dark halos of elliptical galaxies
• The prediction of using LHAASO's cosmic-ray electron measurements to constrain decaying heavy dark matter
• Primordial density perturbations with running spectral index: impact on non-linear cosmic structures
• A plausible link between dynamically unsettled molecular gas and the radio jet in NGC 6328
• Search for Features in the Cosmic-Ray Electron and Positron spectrum measured by the Fermi Large Area Telescope
• $G$ Objects and primordial black holes
• Higgs Dark Matter in UEDs: A Good WIMP with Bad Detection Prospects
• Propagation of cosmic rays in the foam-like Universe
• Anthropic constraints on the cosmological constant from Sun's motion through the Milky Way
• NIHAO XXVIII: Collateral effects of AGN on dark matter concentration and stellar kinematics
• Constraining the three-dimensional orbits of galaxies under ram pressure stripping with convolutional neural networks
• Confronting the Galactic 511 keV emission with $B-L$ gauge boson dark matter
• Ultra-light Dark Matter Search with Astrophysical Neutrino Flavour
• Strong lens search in the ESO public Survey KiDS
• Cosmological gravity on all scales III: non-linear matter power spectrum in phenomenological modified gravity
• Investigating the Dark Matter Halo of NGC 5128 using a Discrete Dynamical Model
• Boosted Dark Matter From Centaurus A and Its Detection
• Effective Star Formation Rates for Cosmological Applications
• Galactic Sun's motion in the Cold Dark Matter, MOdified Newtonian Dynamics and MOdified Gravity scenarios
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• LISA double white dwarf binaries as Galactic accelerometers
• Seeking Self-Regulating Simulations of Idealized Milky Way-Like Galaxies
• When quantum corrections alter the predictions of classical field theory for scalar field dark matter
• SUSY dark matter --A collider Physicist's Perspective--
• The Structure of Cold Dark Matter Halos: Recent Insights from High Resolution Simulations
• Profiles of dark-matter haloes at high redshift
• Baryonic Post-Processing of N-body Simulations, with Application to Fast Radio Bursts
• Correlations of the feedback energy and BCG radio luminosity in galaxy clusters
• The Nature and Origin of the Non-Void Lyman alpha Cloud Population
• Intrinsic size correlations in weak lensing
• Galaxy clusters at z~1 imaged by ALMA with the Sunyaev-Zel'dovich effect
• Synchrotron Emission from Dark Matter in Galactic Subhalos. A Look into the Smith Cloud
• Measurement of halo properties with weak lensing shear and flexion
• Sensitivities of IceCube DeepCore Detector to Signatures of Low-Mass Dark Matter in the Galactic Halo
• Stringy Newton Gravity with $H$-flux
• Haloes at the ragged edge: The importance of the splashback radius
• Indirect Detection Imprint of a CP Violating Dark Sector
• Dark Matter Annihilation Feedback in cosmological simulations I: Code convergence and idealised halos
• Issues for the Next Generation of Galaxy Surveys
• Primordial Black-Hole-Based Pathways to Little Red Dots
• Fluorescent rings in star-free dark matter haloes
• New Constraints on Decaying Dark Matter from INTEGRAL/SPI
• The clustering of LRGs in the DECaLS DR8 footprint: distance constraints from baryon acoustic oscillations using photometric redshifts
• Modified Kerr black holes surrounded by dark matter spike
• MaNGA DynPop -- VI. Matter density slopes from dynamical models of 6000 galaxies versus cosmological simulations: the interplay between baryonic and dark matter
• Anisotropic strong lensing as a probe of dark matter self-interactions
• Probing the Structure of Dark Matter in Galaxy Halos and Clusters using Supernovae
• Rescuing The Primordial Black Holes all-Dark Matter Hypothesis from The Fast Radio Bursts Tension
• Steady-state conduction-driven temperature profile in clusters of galaxies
• The hydrostatic-to-lensing mass bias from resolved X-ray and optical-IR data
• "Non-Local" Effects from Boosted Dark Matter in Indirect Detection
• Universal dark halo scaling relation for the dwarf spheroidal satellites
• The importance of the cosmic web and halo substructure for power spectra
• Modelling the evolution of the Galactic disc scale height traced by open clusters
• Entropy Production in Collisionless Systems. II. Arbitrary Phase-Space Occupation Numbers
• When relics were made: vigorous stellar rotation and low dark matter content in the massive ultra-compact galaxy GS-9209 at z=4.66
• Where are the Fermi Lines Coming From?
• Extended radio AGN at z ~ 1 in the ORELSE survey: The confining effect of dense environments
• The CMB lensing imprint of cosmic voids detected in the WISE-Pan-STARRS luminous red galaxy catalog
• The differential energy distribution of the universal density profile of dark halo
• Measuring the mass and concentration of dark matter halos from the velocity dispersion profile of their stars
• The Distribution of Dark Matter in Galaxies: Constant-Density Dark Halos Envelop the Stellar Disks
• Analyzing Planar Galactic Halo Distributions with Fuzzy/Cold Dark Matter Models
• Self-gravitating Newtonian models of fermions with anisotropy and cutoff energy in their distribution function
• Characterizing the Best Cosmic Telescopes with the Millennium Simulations
• On galaxy rotation curves from a continuum mechanics approach to modified gravity
• When Dark Matter interacts with Cosmic Rays or Interstellar Matter: A Morphological Study
• Distinguishing Neutrino Mass Hierarchies using Dark Matter Annihilation Signals at IceCube
• Dark matter in massive galaxies
• Testing the dark matter origin of the WMAP-Planck Haze with radio observations of Spiral Galaxies
• Halo Profile Evolution and Velocity Bias
• Complementarity of Gamma-ray and LHC Searches for Neutralino Dark Matter in the Focus Point Region
• The M-sigma Relation of Super Massive Black Holes from the Scalar Field Dark Matter
• Kinematics of M51-type interacting galaxies
• Strong Lensing In The Inner Halo Of Galaxy Clusters
• Galaxy-galaxy and galaxy-cluster lensing with the SDSS and FIRST surveys
• Observational properties of rigidly rotating dust configurations
• Indirect searches of Galactic diffuse dark matter in INO-MagICAL detector
• Visible and Dark Matter Profiles in a Non-Minimally Coupled Model
• Search for Scalar Dark Matter via Pseudoscalar Portal Interactions: In Light of the Galactic Center Gamma-Ray Excess
• On the Efficiency of Thermal Conduction in Galaxy Clusters
• Phenomenology of Colored Radiative Neutrino Mass Model and Its Implications on the Cosmic-ray Observations
• Searching for light from a dark matter clump
• Interpretations of galactic center gamma-ray excess confronting the PandaX-II constraints on dark matter-neutron spin-dependent scatterings in the NMSSM
• The Halo Masses of Galaxies to $z\sim 3$: A Hybrid Observational and Theoretical Approach
• Simulation studies of dark energy clustering induced by the formation of dark matter halos
• Gravitationally Focused Dark Matter Around Compact Stars
• Detecting Triaxiality in the Galactic Dark Matter halo through Stellar Kinematics
• Multi-Component Decomposition of Cosmic Infrared Background Fluctuations
• Dwarf Galaxies as Cosmological Probes
• The Spin Alignments in Galaxy Pairs as a Test of Bouncing Coupled Dark Energy
• Kinematics and dynamics of the luminous infrared galaxy pair NGC 5257/58 (Arp 240)
• Testing $\Lambda$CDM With Dwarf Galaxy Morphology
• Suppressing the thermal SZ-induced variance in CMB-cluster lensing estimators
• Towards a Model-Independent Measurement of the Halo Mass Function with Observables
• Constraints on Quasi-dilaton Massive Gravity
• Gravitational Potential from small-scale clustering in action space: Application to Gaia DR2
• Slowly rotating Bose-Einstein Condensate confronted with the rotation curves of 12 dwarf galaxies
• Motion of Particles in Solar and Galactic Systems by Using Neumann Boundary Condition
• Angular momentum in cluster Spherical Collapse Model
• Estimate of halo ellipticity as a function of radius with flexions
• On the Cooling Flow Problem in the Gaseous Halo of the Milky Way
• Search for decaying heavy dark matter in an effective interaction framework: a comparison of $\gamma$-ray and radio observations
• Power spectrum response of large-scale structure in 1D and in 3D: tests of prescriptions for post-collapse dynamics
• Modeling the Alignment Profile of Satellite Galaxies in Clusters
• Gravitational entropy of wormholes with exotic matter and in galactic halos
• Probing annihilations and decays of low-mass galactic dark matter in IceCube DeepCore array: Track events
• Dark Fluxes from Accreting Black Holes and Direct Detections
• On interpretation of recent proper motion data for the Large Magellanic Cloud
• Can tides explain the low dark matter density in Fornax?
• The effect of finite halo size on the clustering of neutral hydrogen
• An expanded merger-tree description of cluster evolution
• Origin of optically passive spiral galaxies with dusty star-forming regions: Outside-in truncation of star formation?
• Understanding the "Feeble Giant" Crater II with tidally stretched Wave Dark Matter
• Magnetic fields and Sunyaev-Zel'dovich effect in galaxy clusters
• Neutrino point source searches for dark matter spikes
• Cosmic star formation history with tomographic cosmic infrared background-galaxy cross-correlation
• The X-ray Angular Power Spectrum of Extended Sources in the eROSITA Final Equatorial Depth Survey
• Towards Optimal Foreground Mitigation Strategies for Interferometric HI Intensity Mapping in the Low-Redshift Universe
• Fermi Constrains Dark Matter Origin of High Energy Positron Anomaly
• Subaru HSC weak lensing of SDSS redMaPPer cluster satellite galaxies: Empirical upper limit on orphan fractions
• Semi-analytical frameworks for subhalos from the smallest to the largest scale
• Testing the Collisionless Nature of Dark Matter with the Radial Acceleration Relation in Galaxy Clusters
• A Lensing View On The Fundamental Plane
• What is the super-sample covariance? A fresh perspective for second-order shear statistics
• Small scale clustering of BOSS galaxies: dependence on luminosity, color, age, stellar mass, specific star formation rate and other properties
• Exotic Image Formation in Strong Gravitational Lensing by Clusters of Galaxies -- IV. Elliptical NFW Lenses and Hyperbolic Umbilics
• Constraining $p$-wave Dark Matter Annihilation with Gamma-ray Observations of M87
• Decomposing galaxies with BANG: an automated morpho-kinematical decomposition of the SDSS-DR17 MaNGA survey
• Cluster profiles from beyond-the-QE CMB lensing mass maps
• Dark Matter Fraction in Disk-Like Galaxies Over the Past 10 Gyr
• The distribution, kinematics and luminosities of extreme helium stars as probes of their origin and evolution
• Evaluating the variance of individual halo properties in constrained cosmological simulations
• Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory
• Analytic approach to astrometric perturbations of critical curves by substructures
• Supernova-Neutrino-Boosted Dark Matter from All Galaxies
• The baryon mass function for galaxy clusters
• Weak lensing of strong lensing: beyond the tidal regime
• Mass Modeling and Kinematics of Galaxy Clusters in Modified Gravity
• Inner structure of dark matter halos at high $z$ in cosmological models with non-power-law primordial spectra
• Compact Binary Merger Rate with Modified Gravity in Dark-Matter Spikes
• EDEN: Exploring Disks Embedded in N-body simulations of Milky-Way-mass halos from Symphony
• LensWatch. II. Improved Photometry and Time-delay Constraints on the Strongly Lensed Type Ia Supernova 2022qmx ("SN Zwicky") with HST Template Observations
• Interactions of ultrahigh-energy cosmic rays with photons in the galactic center
• Euclid preparation: Determining the weak lensing mass accuracy and precision for galaxy clusters
• Power Spectrum and Intermittency of Ly$\alpha$ Transmitted Flux of QSO He2347-4342
• On the impact of AGN feedback modes onto the turbulent properties of the multiphase ICM
• Boosted dark matter from semi-annihilations in the galactic center
• A MARVEL-ous study of how well galaxy shapes reflect Dark Matter halo shapes in Cold Dark Matter Simulations
• Turbulent gas-rich discs at high redshift: origin of thick stellar discs through 3D 'baryon sloshing'
• Faster than SAM: An empirical model for the tidal evolution of dark matter substructure around strong gravitational lenses
• Dark Spin-2 Field Solitons as a Source of Electromagnetic Radiation
• Prospects of future MeV telescopes in probing weak-scale Dark Matter
• SHARP -- IX. The dense, low-mass perturbers in B1938+666 and J0946+1006: implications for cold and self-interacting dark matter
• Map-level baryonification: unified treatment of weak lensing two-point and higher-order statistics
• NOEMA${}^{3D}$: A first kpc resolution study of a $z\sim 1.5$ main sequence barred galaxy channeling gas into a growing bulge
• Leo I: the classical dwarf spheroidal galaxy with the highest dark-matter density
• Constraining supersymmetry from the satellite experiments
• Testing black holes in a perfect fluid dark matter environment using quasinormal modes
• Mass Modeling the Andromeda Dwarf Galaxies: Andromeda VI and Andromeda XXIII
• A serendipitous discovery of HI-rich galaxy groups with MeerKAT
• Are there more galaxies than we see around high-$z$ quasars?
• On the Galactic Halos Rotation by Planck Data
• Pierre Auger Observatory and Super Heavy Dark Matter
• Reliability of merger tree realizations of dark halos in the Monte-Carlo modeling of galaxy formation
• Dissociation of dark matter and gas in cosmic large-scale structure
• Existence of Tidal Tails for the Globular Cluster NGC 5824
• Dynamical cluster masses from photometric surveys
• Comparison of hydrostatic and lensing cluster mass estimates:a pilot study in MACS J0647.7+7015
• Modeling Photoionized Turbulent Material in the Circumgalactic Medium III: Effects of Co-rotation and Magnetic Fields
• How stars formed in warps settle into (and contaminate) thick discs
• Shape noise and dispersion in precision weak lensing
• Clustering of cosmic string loops
• The effect of our local motion on the Sandage-Loeb test of the cosmic expansion
• A 5deg x 5deg deep HI survey of the M81 group: II. HI distribution and kinematics of IC 2574 and HIJASS J1021+68
• Denuded Dwarfs Demystified: Gas Loss from dSph Progenitors and Implications for the Minimum Mass of Galaxies
• Constraining primordial black holes in dark matter with kinematics of dwarf galaxies
• The quantity of dark matter in early-type galaxies and its relation to the environment
• NGC 7457: Evidence for merger-driven cylindrical rotation in disc galaxies
• Constraining Dark Matter and Ultra-High Energy Cosmic Ray Sources with Fermi-LAT Diffuse Gamma Ray Background
• A spiral galaxy's mass distribution uncovered through lensing and dynamics
• High-Scale SUSY Breaking Models in light of the BICEP2 Result
• Reconstructing the Thermal Sunyaev-Zel'dovich Effect in 3D
• Kinematic study of planetary nebulae in NGC 6822
• Made-To-Measure Models of Self-Similar Triaxial Halos with Steep Inner Density Gradients
• Detecting Triaxiality in the Galactic Dark Matter Halo through Stellar Kinematics II: Dependence on Dark Matter and Gravity Nature
• Self-gravitating systems in Extended Gravity
• Systematic Study of Gravitational Waves from Galaxy Merger
• Dynamical and gravitational lensing properties of a new phenomenological model of elliptical galaxies
• Merger as Intermittent Accretion
• Origin of lower velocity dispersions of ultra-compact dwarf galaxy populations in clusters of galaxies
• The mass distribution in Spiral galaxies
• Detecting the dark matter annihilation at the ground EAS detectors
• Do gravitational lens galaxies have an excess of luminous substructure?
• Constraining cosmology with the velocity function of low-mass galaxies
• Flattening of dark matter cusps during mergers: model of M31
• Globular clusters vs dark matter haloes in strong lensing observations
• MNELLS: The MUSE Nearby Early-Type Galaxy Lens Locator Survey
• Structure and kinematics of the polar ring galaxies: new observations and estimation of the dark halo shape
• Indirect detection prospects for d${}^{\ast }$(2380) dark matter
• Masked areas in shear peak statistics: a forward modeling approach
• Cosmic ray knee and new physics at the TeV scale
• Where has all the $r$-process gone? Timescales for GRB-Kilonovae to Enrich their Host Galaxies
• Disk Mass-to-Light ratio distribution from stellar population synthesis: Application to rotation curve decomposition of NGC 5278 (KPG 390A)
• The Noctua Suite of Simulations -- The Difficulty of Growing Massive Black Holes in Low-Mass Dwarf Galaxies
• Probing Self-Interacting Dark Matter via Gravitational-Wave Background from Eccentric Supermassive Black Hole Mergers
• Cosmology and Astrophysics with the Diffuse eRASS1 X-ray Angular Power Spectrum
• Assessing Disk Galaxy Stability through Time
• Quantifying the Projected Suppression of Cluster Escape Velocity Profiles
• Intermediate mass ratio inspirals in dark matter halos
• Gravitational Lensing by Spherical Lenses
• A measurement of cluster masses using Planck and SPT-SZ CMB lensing
• The correlation of high-redshift galaxies with the thermal Sunyaev-Zel'dovich effect traces reionization
• Gravothermalizing into primordial black holes, boson stars, and cannibal stars
• DESI Mock Challenge: Constructing DESI galaxy catalogues based on FastPM simulations
• Baryonic Ecosystem in Galaxies (BEINGMgII) -- II. Unveiling the Nature of Galaxies Harboring Cool Gas Reservoirs
• Probing $z\gtrsim 6$ massive black holes with gravitational waves
• Dark matter annihilation into leptons through gravity portals
• The case for two-dimensional galaxy-galaxy lensing
• Explaining the PeV Neutrino Fluxes at KM3NeT and IceCube with Quasi-Extremal Primordial Black Holes
• Linear analysis of the gravitational beam-plasma instability
• Detecting Extragalactic Axion-like Dark Matter with Polarization Measurements of Fast Radio Bursts
• Astrophysical constraints from synchrotron emission on very massive decaying dark matter
• Capture rate of weakly interacting massive particles (WIMPs) in binary star systems
• Evidence for a large off-centered galactic outflow and its connection to the extraplanar diffuse ionized gas in IC 1553
• Galactic breeze origin for the Fermi bubbles emission
• CEMPlifying reionization
• On the theory of mass loss in dwarf galaxies: I - basic equations and the case of wave/thermal driven winds
• Effective Cross Section of Fuzzy Dark Matter Halos
• A Recipe to Probe Alternative Theories of Gravitation via N-body Numerical Simulations. I. Spiral Galaxies
• Measuring the ICM velocity structure within the A3266 galaxy cluster
• A cosmologically motivated description of the dark matter halo profile for the Low Surface Brightness Galaxy, Malin 1
• Seeing the halo rotation of nearby spiral galaxies using Planck data
• The role of Dark Matter annihilation in the radio emission of the galaxy cluster A520
• Generalised scalar-tensor theories of gravity and pressure profiles of galaxy clusters
• Modeling the Initial Conditions of Interacting Galaxy Pairs Using Identikit
• The ALMA-CRISTAL Survey: Complex kinematics of the galaxies at the end of the Reionization Era
• Black strings from dark matter
• Dark matter as the source of neutrino mass: theory overview and experimental prospects
• Search for Dark Matter Annihilation to gamma-rays from SPT-SZ selected Galaxy Clusters
• Bose-Einstein condensate and degenerate Fermi cored dark matter halos
• Hollow cores in Warm Dark Matter halos from the Vlasov-Poisson equation
• On the abundance of gravitational arcs produced by submillimeter galaxies at radio and submm wavelengths
• The impact of weak lensing on Type Ia supernovae luminosity distances
• Novel electrically charged wormhole, black hole and black bounce exact solutions in hybrid metric-Palatini gravity
• Fast multiscale galaxy cluster detection with weak lensing: towards a mass-selected sample
• A Universal SFDM Halo Mass for the Andromeda and Milky Way's dSphs?
• Crazy heart: kinematics of the "star pile" in Abell 545
• Polarized gamma rays from dark matter annihilations
• Modelling the escape of Lyman Continuum photons from galaxies in the Epoch of Reionization
• Phenomenology of a two-component dark matter model
• Diffuse X-Ray and Gamma-Ray Limits on Boson Stars that Interact with Nuclei
• Monte-Carlo Modeling of Non-Gravitational Heating Processes in Galaxy Clusters
• A Simulation Based Inference Approach to the Dynamics of the MW-LMC System -- Validation
• On the Origin and Nature of Dark Matter
• Euclid preparation. Simulating thousands of Euclid spectroscopic skies
• Outer and inner mass distributions of the irregular galaxies UGC 4284 and UGC 11861: Constraining the baryonic content through stellar population synthesis studies
• Recent Observations of the Rotation of Distant Galaxies and the Implication for Dark Matter
• Entropy Production in Collisionless Systems. I. Large Phase-Space Occupation Numbers
• Photoelectric heating effects on the evolution of luminous disk galaxies
• The Maxwell--Boltzmann gas with non-standard self--interactions: a novel approach to galactic dark matter
• Dark Matter as an active gravitational agent in cloud complexes
• A Stringent Upper Limit on Dark Matter Self-Interaction Cross Section from Cluster Strong Lensing
• Non-orientable wormholes as portals to the mirror world
• The XXL Survey LI. Pressure profile and $Y_{\mathrm{SZ}}$-$M$ scaling relation in three low-mass galaxy clusters at $z\sim 1$ observed with NIKA2
• Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies
• Do neutrinos bend? Consequences of an ultralight gauge field as dark matter
• Molar mass estimate of dark matter from the dark mass distribution measurements
• Total and dark mass from observations of galaxy centers with Machine Learning
• Formation of massive black holes in ultra-compact dwarf galaxies: migration of primordial intermediate-mass black holes in N-body simulation
• Dark matter annihilation in $\omega$ Centauri: Astrophysical implications derived from the MWA radio data
• Implications for Pulsar Timing Arrays of Sub-solar Black Hole Detections: From LVK to Einstein Telescope and Cosmic Explorer
• Tidal Tails of Nearby Open Clusters. II. A Review of Simulated Properties and the Reliability of Observational Catalogues
• Energy Conservation in the thin layer approximation: I. The spherical classic case for supernovae remnants
• Jeans modeling of axisymmetric galaxies with multiple stellar populations
• A new method to break the mass sheet degeneracy using aperture moments
• Spherical accretion in giant elliptical galaxies: multi-transonicity, shocks, and implications on AGN feedback
• Self-Similar Shocks and Winds in Galaxy Clusters
• Mass - concentration relation and weak lensing peak counts
• A Modified Dynamical Model of Cosmology I. Theory
• GravSphere2: A higher-order Jeans method for mass-modeling spherical stellar systems
• CFHTLenS: Galaxy bias as function of scale, stellar mass, and colour. Conflicts with predictions by semi-analytic models
• The Hierarchical Structure of Galactic Haloes: Classification and characterisation with Halo-OPTICS
• Calibrating galaxy formation effects in galactic tests of fundamental physics
• Unravelling the orbits of cluster galaxy populations according to their dominant gas ionization source
• Satellite Galaxies in the Illustris-1 Simulation: Poor Tracers of the Mass Distribution
• The H$\alpha$ luminosity and stellar mass dependent clustering of star-forming galaxies at $0.7<z<1.5$ with 3D-HST
• Super-Resonant Dark Matter
• Cosmological Simulations with Scale-Free Initial Conditions I: Adiabatic Hydrodynamics
• Milgrom Relation Models for Spiral Galaxies from Two-Dimensional Velocity Maps
• A Deep Chandra Observation of the Distant Galaxy Cluster MS1137.5+6625
• The distinguishing factor for gravity models: stellar population synthesis
• Composite Dark Matter and Neutrino Masses from a Light Hidden Sector
• Transverse velocities and matter gradient correlations: a new signal and a new challenge to moving-lens analyses
• Displaced Lepton Jet Signatures from Self-Interacting Dark Matter Bound States
• A Search for Annihilating Dark Matter in 47 Tucanae and Omega Centauri
• Dequantization of electric charge: Probing scenarios of cosmological multi-component dark matter
• AMS-02 antiprotons and dark matter: Trimmed hints and robust bounds
• Dynamical models of the elliptical galaxy NGC 4494
• All-sky limits on Sterile Neutrino Galactic Dark Matter obtained with SRG/ART-XC after two years of operations
• The effect of cosmic variance on the characteristics of dust polarization power spectra
• Secondary halo bias through cosmic time II: Reconstructing halo properties using clustering information
• A Study of the Merger History of the Galaxy Group HCG 62 Based on X-Ray Observations and SPH Simulations
• The bi-modal ${}^7$Li distribution of the Milky Way's thin-disk dwarf stars: The role of Galactic-scale events and stellar evolution
• Central densities of dark matter halos in FIRE-2 simulations of low-mass galaxies with cold dark matter and self-interacting dark matter
• Bose-Einstein Condensate Dark Matter Halos confronted with galactic rotation curves
• Concurrent infall of satellites: Collective effects changing the overall picture
• High Velocity-dispersion Cold Gas in ULIRG Outflows. I: Direct Simulations
• Clash of Titans: a MUSE dynamical study of the extreme cluster merger SPT-CL J0307-6225
• The art of building a smooth cosmic distance ladder in a perturbed universe
• Baryon Pasting the Uchuu Lightcone Simulation
• Orbits and adiabatic contraction in scalar field dark matter halos: revisiting the cusp-core problem in dwarf galaxies
• Modeling the Mass Distribution and Gravitational Potential of Nearby Disk Galaxies: Implications for the ISM Dynamical Equilibrium
• Dark Matter Substructure or Source Model Systematics? A Case Study of Cluster Lens Abell S1063
• Smallest Halos in Thermal Wino Dark Matter
• 21-cm Constraints on Dark Matter Annihilation after an Early Matter-Dominated Era
• Requirements to Detect the Monoenergetic Photon Signature of Thermal Cold Dark Matter in PeV-Scale Split Supersymmetry
• Searching for dark matter subhalos in the Fermi-LAT catalog with Bayesian neural networks
• Relativistic rotation curve for cosmological structures
• Simulation of a strategy for the pixel lensing of M87 using the Hubble Space Telescope
• Weak Lensing by Minifilament or Minivoid as the Origin of Flux-ratio Anomalies in Lensed Quasar MG0414+0534
• Effect of turbulent reacceleration on electrons produced by dark matter annihilation in the Coma cluster
• Evolution of massive quiescent galaxies via envelope accretion
• Halo Density Profiles Consistent with Asymmetric M-B Velocity Distributions-Implications on Direct Dark Matter Searches
• Neutrinophilic DM annihilation in a model with $U(1{)}_{L_{\mu }-L_{\tau }}\times U(1{)}_H$ gauge symmetry
• The Dependency of Bar Formation Timescale on Disk Mass Fraction, Toomre $Q$, and Scale Height
• Neutralino annihilation gamma-rays from clumps and the LMC
• The kinetic Sunyaev-Zel'dovich effect from the diffuse gas in the Local Group
• Structure formation and quasi-spherical collapse from initial curvature perturbations with numerical relativity simulations
• Dynamical mirages: how bar-induced resonant trapping can mimic substructure clustering in dynamical parameter spaces
• Mass decomposition of SLACS lens galaxies in Weyl conformal gravity
• Anisotropic Models of Dark Halos
• Einasto profile as the halo model solution coupled to the depletion radius
• The fragility of thin discs in galaxies -- I. Building tailored N-body galaxy models
• Total mass distributions of Sersic galaxies from photometry $&$ cent\ ral velocity dispersion
• Ultra-local models of modified gravity without kinetic term
• Dark Kinetic Heating of Exoplanets and Brown Dwarfs
• Weak lensing magnification of Type Ia Supernovae from the Pantheon sample
• Gravitational Collapse in an Expanding Universe: Scaling Relations for Two-Dimensional Collapse Revisited
• What Could be the Observational Signature of Dark Matter in Globular Clusters?
• Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
• Observational constraint on axion dark matter with gravitational waves
• CARMA observations of massive Planck-discovered cluster candidates at z>0.5 associated with WISE overdensities: Breaking the size-flux degeneracy
• Baryon effects on the dark matter halos constrained from strong gravitational lensing
• Numerical implementation of the Cubic Galileon model in PINOCCHIO
• Ultrahigh energy cosmic rays from dark matter annihilation
• New near-infrared observations and lens-model constraints for UM673
• On the accuracy of the Perturbative Approach for Strong Lensing: Local Distortion for Pseudo-Elliptical Models
• The KALEIDOSCOPE survey : A new strong and weak gravitational lensing view of the massive galaxy cluster MACS J1423.8+2404
• Non-Baryonic Dark Matter
• Probing the Galactic Potential with Next-Generation Observations of Disk Stars
• Non-Gaussian Signatures in the Lens Deformations of the CMB Sky. A New Ray-Tracing Procedure
• Analytical analysis of the origin of core-cusp matter density distributions in galaxies
• Globular clusters in \textsc{OrbIT}: complete dynamical characterisation of the globular cluster population of the Milky Way through updated orbital reconstruction
• On the tilt of Fundamental Plane by Clausius' virial maximum theory
• Science Potential for Stellar-mass Black Holes as Neighbors of Sgr A*
• Bayesian analysis of spatially distorted cosmic signals from Poissonian data
• Intrinsic correlations of galaxy sizes in a hydrodynamical cosmological simulation
• Dark Coincidences: Small-Scale Solutions with Refracted Gravity and MOND
• Heating of the intracluster medium by buoyant bubbles and sound waves
• The origin of the metallicity distributions of the NE and W stellar shelves in the Andromeda Galaxy
• Prospects for a local detection of dark matter with future missions to Uranus and Neptune
• Dark sector domain walls could explain the observed planes of satellites
• Influence of Magnetic Fields on the Gas Rotation in the Galaxy $NGC6946$
• Properties of Central Regions of the Dark Matter Halos in the Model with a Bump in the Power Spectrum of Density Perturbations
• The circular velocity and halo mass functions of galaxies in the nearby Universe
• In Search of Extraterrestrial Artificial Intelligence Through Dyson Sphere-like structures around Primordial Black Holes
• The Milky Way satellite galaxy Leo T: A perturbed cored dwarf
• The Impact of Dark Matter on Gravitational Wave Detection by Space-based Interferometers
• Why there are no elliptical galaxies more flattened than E7: thirty years later
• Soft Gamma Rays from Heavy WIMPs
• Evolution of cold streams in hot gaseous halos
• A derivation of (half) the dark matter distribution function
• Two-component, ideal, self-gravitating fluids: the fractional virial potential energy
• Dark Matter Angular Momentum Profile from the Jeans Equation
• A radio-frequency WIMP search with the MeerKAT Galaxy Cluster Legacy Survey
• Gravitational wave background from primordial black holes in globular clusters
• The gravitational force field of proto-pancakes
• The Density Parity Model for the Evolution of the Subhalo Inner Spin Alignments with the Cosmic Web
• Universal multi-stream radial structures of cold dark matter halos
• Gravitational Waves from Primordial Black Hole Dark Matter Spikes
• Exploring HOD-dependent systematics for the DESI 2024 Full-Shape galaxy clustering analysis
• The collaborative effect of ram pressure and merging on star formation and stripping fraction
• Homeoidally striated density profiles: sequences of virial equilibrium configurations with constant anisotropy parameters
• Did IceCube discover Dark Matter around Blazars?
• Search for Inelastic Boosted Dark Matter with the ICARUS Detector at the Gran Sasso Underground National Laboratory
• Strong Constraints on Dark Photon and Scalar Dark Matter Decay from INTEGRAL and AMS-02 data
• Lensing-Induced Structure of Submillimeter Sources: Implications for the Microwave Background
• An integrated Sachs-Wolfe effect vs redshift test for the cosmological parameters
• The Three Hundred Project hydrodynamical simulations: Hydrodynamical weak-lensing cluster mass biases and richnesses using different hydro models
• zoomies: A tool to infer stellar age from vertical action in Gaia data
• Resolving the mass--anisotropy degeneracy of the spherically symmetric Jeans equation II: optimum smoothing and model validation
• Muon anomalous magnetic moment and positron excess at AMS-02 in a gauged horizontal symmetric model
• The influence of baryons on low-mass haloes
• Mass content of UGC 6446 and UGC 7524 through HI rotation curves: deriving the stellar discs from stellar population synthesis models
• Radial Acceleration and Tully-Fisher Relations in Conformal Gravity
• On the structure of galactic halos and the microwave temperature maps
• Extension of Minimal Fermionic Dark Matter Model : A Study with Two Higgs Doublet Model
• Unlocking Discovery Potential for Decaying Dark Matter and Faint X-ray Sources with XRISM
• Bounds on neutrino-DM interactions from TXS 0506+056 neutrino outburst
• Interplay between Black Holes and Ultralight Dark Matter: Analytic Solutions
• Structural and dynamical modeling of WINGS clusters. III. The pseudo phase-space density profile
• Improving lensing cluster mass estimate with flexion
• MIMAC potential discovery and exclusion of neutralinos in the MSSM and NMSSM
• Bound Dark Matter (BDM) towards solving the Small Scale Structure Problem
• Modelling the impact of intrinsic size and luminosity correlations on magnification estimation
• The north-south asymmetry of the ALFALFA HI velocity width function
• Testing the weak equivalence principle with the binary neutron star merger GW170817: the gravitational contribution of the host galaxy
• A Potentially Detectable Gamma-Ray Line in the Fermi Galactic Center Excess -- In Light of One-Step Cascade Annihilations of Secluded (Vector) Dark Matter via the Higgs Portal
• CHEX-MATE: Multi-probe analysis of Abell 1689
• Black Hole Critical Collapse in Infinite Dimensions: Continuous Self-Similar Solutions
• Enhancements to velocity-dependent dark matter interactions from tidal streams and shells in the Andromeda galaxy
• Evolution of dwarf spheroidal satellites in the common surface-density dark halos
• Axion signals from neutron star populations
• Recovering the pattern speeds of edge-on barred galaxies via an orbit-superposition method
• Influence of Cooled Interstellar Gas on the Fundamental Plane for Elliptical Galaxies
• Shadows and Observational Images of a Schwarzschild-like Black Hole Surrounded by a Dehnen-type Dark Matter Halo
• Strong Lensing Probabilities in a Cosmological Model with a Running Primordial Power Spectrum
• Statistics for dark matter subhalo searches in gamma rays from a kinematically constrained population model: Fermi-LAT-like telescopes
• Boosting Asymmetric Charged DM via Thermalization
• Collapsed and Extended Cold Dark Matter Haloes in Softened N-Body Gravity
• Dark Matter Annihilation Feedback in Cosmological Simulations II: The Influence on Gas and Halo Structure
• The secular evolution of a uniform density star cluster immersed in a compressible galactic tidal field
• Diving into dangerous tides: The impact of galaxy cluster tidal environments on satellite galaxy mass densities
• A forward-modelling method to infer the dark matter particle mass from strong gravitational lenses
• Dynamical friction in rotating ultralight dark matter galactic cores
• Halo Concentrations and the Fundamental Plane of Galaxy Clusters
• Hawking Radiation Signatures from Primordial Black Holes Transiting the Inner Solar System: Prospects for Detection
• Evolution of dwarf galaxy observable parameters
• Mysterious Globular Cluster System of the Peculiar Massive Galaxy M85
• A new non-parametric method to infer galaxy cluster masses from weak lensing
• Signatures of Fuzzy Dark Matter Inside Radial Critical Curves
• Modelling the selection of galaxy groups with end to end simulations
• Astrophysical Constraints on Dark Energy
• Dark Matter Annihilation via Breit-Wigner Enhancement with Heavier Mediator
• Evolution of Power Spectrum in Non-Gaussian Models
• New observational recipes for measuring dynamical state of galaxy clusters
• Proca-stinated Cosmology II: Matter, Halo, and Lensing Statistics in the vector Galileon
• Modeling HF-QPOs in Microquasars and AGNs: Charged Particles around Black Holes with CDM Halos
• Boosted dark matter versus dark matter-induced neutrinos from single and stacked blazars
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Destruction of the central black hole gas reservoir through head-on galaxy collisions
• Analytic approach to perturbed Einstein ring with elliptical NFW lens model
• Indirect searches for realistic sub-GeV Dark Matter models
• Stacked phase-space density of galaxies around massive clusters: Comparison of dynamical and lensing masses
• Gravitational radiation reaction around a static black hole surrounded by a Dehnen type dark matter halo
• Estimation of the Mass of Dark Matter Using the Observed Mass Profiles of Late-Type Galaxies
• Gravitational Fugacity as the seed of self-organized violent relaxaton process toward Local Virial relation
• Fuzzy dark matter simulations
• Evolving beyond z=0: insights about the future of stars and the intergalactic medium
• New constraints on radiative seesaw models from IceCube and other neutrino detectors
• Low surface brightness galaxies mass profiles as a consequence of galactic evolution
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Galaxy formation with wave/fuzzy dark matter: The core-halo structure and the solitonic imprint
• Semi analytical description of formation of galaxies and clusters of galaxies
• Effects of Angular Momentum on Halo Profiles
• Dynamics of One-dimensional Self-gravitating Systems Using Hermite-Legendre Polynomials
• The unusually high dark matter concentration of the galaxy group NGC 1600
• Galaxy cluster number counts with individual lensing mass estimates: forecasts for Euclid
• Cluster density slopes from Dark Matter-Baryons Energy Transfer
• On the behaviour of streams in angle and frequency spaces in different potentials
• Galaxy cluster mass bias from projected mass maps: The Three Hundred-NIKA2 LPSZ twin samples
• The impact of halo concentration on the Sunyaev Zel'dovich effect signal from massive galaxy clusters
• A high-resolution view of the source-plane magnification near cluster caustics in wave dark matter models
• Predicting the Non-Thermal Pressure in Galaxy Clusters
• Constraints on the parameters of keV-scale mass annihilating Dark Matter obtained with SRG/ART-XC observations
• Cosmological implications of the Gaia Milky Way declining rotation curve
• Hawking Radiation of Nonrelativistic Scalars: Applications to Pion and Axion Production
• Globular cluster orbital decay in dwarf galaxies with MOND and CDM: Impact of supernova feedback
• Simulating Binary Primordial Black Hole Mergers in Dark Matter Halos
• Cosmological parameters from lenses distance ratio
• Gravitational waves from an eccentric population of primordial black holes orbiting Sgr A${}^{\star }$
• Quantum Theory of Cold Dark Matter Halos
• One Stream or Two -- Exploring Andromeda's North West Stream
• Stellar halos tracing the assembly of ultra-faint dwarf galaxies
• Simulating realistic self-interacting dark matter models including small and large-angle scattering
• AMS-02 fits Dark Matter
• Barions and $\Lambda$CDM Model Problems
• Soft X-ray excess of clusters: a thermal filament model, and the strong lensing of background galaxy groups
• Using dust to constrain dark matter models
• Interference in Fuzzy Dark Matter Filaments: Idealised Models and Statistics
• A Parameter-free Statistical Measurement of Halos with Power Spectra
• The mass distribution in an assembling super galaxy group at $z=0.37$
• Constraining eV-scale axion-like particle dark matter: insights from the M87 Galaxy
• Vertical kinematics of the thick disc at 4.5 < R < 9.5 kpc
• On Equation of State of Dark Matter around Massive Black Holes
• On the Fast Track: Rapid construction of stellar stream paths
• Detection for Intermediate-mass Binary Black Holes in Population III Star Clusters with TianQin
• The abundance of lensing protoclusters
• MaNGA DynPop. VII. A Unified Bulge-Disk-Halo Model for Explaining Diversity in Circular Velocity Curves of 6000 Spiral and Early-Type Galaxies
• Forming the local starburst galaxy Haro 11 through hydrodynamical merger simulations
• Searching for strong lensing by late-type galaxies in UNIONS
• PASSAGES: The Discovery of a Strongly Lensed Protocluster Core Candidate at Cosmic Noon
• JWSTs PEARLS: NIRCam imaging and NIRISS spectroscopy of a $z=3.6$ star-forming galaxy lensed into a near-Einstein Ring by a $z=1.258$ massive elliptical galaxy
• Measurement of the dark matter velocity anisotropy profile in galaxy clusters
• Stellar Mass Segregation in Dark Matter Halos
• Dust Evolution in Simulated Multiphase Galactic Outflows
• Dynamics of tidal spiral arms: Machine learning-assisted identification of equations and application to the Milky Way
• A Physical Bias in Cosmological Simulations
• The cusp-halo relation
• Detectability of dark matter density distribution via gravitational waves from binary black holes in the Galactic center
• Extreme AGN feedback in the fossil galaxy group SDSSTG 4436
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• SLICE: SPT-CL J0546-5345 -- A prominent strong-lensing cluster at $z=1.07$
• Sub-keV dark matter can strongly ionize molecular clouds
• Lensing by black holes within astrophysical environments
• CLASH-VLT: The variance in the velocity anisotropy profiles of galaxy clusters
• Hermeian haloes: extreme objects with two interactions in the past
• Einstein@Home Searches for Gamma-ray Pulsars in the Inner Galaxy
• Cosmic Vine: High abundance of massive galaxies and dark matter halos in a forming cluster at z=3.44
• The radial acceleration relation at the EDGE of galaxy formation: testing its universality in low-mass dwarf galaxies
• Detecting Intermediate-Mass Black Holes out to 20 Mpc with ELT/HARMONI: The Case of FCC 119
• Search for GeV-scale Dark Matter from the Galactic Center with IceCube-DeepCore
• Dark Matter Constituents
• Bounds from multi-messenger astronomy on the Super Heavy Dark Matter
• Halo heating from fluctuating gas in a model dwarf
• How do the dynamics of the Milky Way -- Large Magellanic Cloud system affect gamma-ray constraints on particle dark matter?
• Observational properties of a Schwarzschild black hole surrounded by a Dehnen-type dark matter halo
• A precessing jet from an active galactic nucleus drives gas outflow from a disk galaxy
• A dense dark matter core of the subhalo in the strong lensing system JVAS B1938+666
• Structure and kinematics of the interacting group NGC 5098/5096
• HST Grism Observations of a z~1.8 Cluster Candidate from the Clusters Occupied by Bent Radio AGN (COBRA) Survey
• Feedback from intermediate mass black holes on dwarf galaxy morphology at z=2
• Caustic and hydrostatic mass bias: Implications for modified gravity
• Stellar angular momentum of disk galaxies at z = 0.7 in the MAGIC survey I. Impact of the environment
• Dark Matter constraints from Planck observations of the Galactic polarized synchrotron emission
• Barless flocculent galaxies: a dynamic puzzle
• WSRT observations and surface photometry of two unusual spiral galaxies
• On the detectability of gravitational waves from primordial black holes orbiting Sgr A*
• On the use of X-ray and gamma-ray telescopes for identifying the origin of electrons and positrons observed by ATIC, Fermi, and PAMELA
• Weak lensing peak statistics -- steepness versus height
• Constraining new fundamental physics with multiwavelength astrometry
• The fragility of thin discs in galaxies -- II. Thin discs as tracers of the assembly history of galaxies
• Confronting cosmic ray electron and positron excesses with hybrid triplet Higgs portal dark matter
• CO kinematics unveil outflows plausibly driven by a young jet in the Gigahertz Peaked Radio Core of NGC6328
• Gravitational Lensing By a Massive Object in a Dark Matter Halo. II. Shear, Phase, and Image Geometry
• Galaxy Correlation Function and Local Density from Photometric Redshifts Using the Stochastic Order Redshift Technique (SORT)
• Neutralino Dark Matter as the Source of the WMAP Haze
• Thin-disk models in an Integrable Weyl-Dirac theory
• ASCA Observation of the Nearest Gravitational Lensing Cluster Candidate -- A 3408
• Sensitivity of CTA to gamma-ray emission from the Perseus galaxy cluster
• Stellar Dynamical Modeling - Accuracy of 3D Density Estimation for Edge-on Axisymmetric Galaxies
• Synthetic Galaxy Clusters and Observations Based on Dark Energy Survey Year 3 Data
• Distribution of Phantom Dark Matter in Dwarf Spheroidals
• Baryonic Tully-Fisher test of Grumiller's modified gravity model
• Effects of Formation Epoch Distribution on X-Ray Luminosity and Temperature Functions of Galaxy Clusters
• Non-relativistic Boson Stars as N-Body Quantum Systems
• Mapping dark matter and finding filaments: calibration of lensing analysis techniques on simulated data
• A new way to constrain the densities of intra-group medium in groups of galaxies with convolutional neural networks
• On the shape of the local bubble
• On the Stability of Quasi-Equilibrium Self-Gravitating Configurations in a Tidal Field
• Effect of lensing magnification on type Ia supernova cosmology
• Axion-like particle searches with MeerKAT and SKA
• Local Stability of Galactic Discs in Modified Dynamics
• Results from the SuperModel Analysis of the X-COP Galaxy Clusters Sample
• Traversable wormholes and the Brouwer fixed-point theorem
• The Possible Equation Of State Of Dark Matter in Low Surface Brightness Galaxies
• Cosmic Ray Electron and Positron Excesses from a Fourth Generation Heavy Majorana Neutrino
• Can dark matter see itself?
• The Assembly of the Virgo Cluster, Traced by its Galaxy Halos
• An analytic distribution function for a massless cored stellar system in a cuspy dark matter halo
• The gamma-ray spectral feature from Kaluza-Klein dark matter annihilation and its observability
• The slingshot effect as a probe of transverse motions of galaxies
• Some Implications of the Leptonic Annihilation of Dark Matter: Possible Galactic Radio Emission Signatures and the Excess Radio Flux of Extragalactic Origin
• Properties of subhalos in the interacting dark matter scenario
• Extragalactic neutrinos as tracers of Dark Matter?
• The connection between halo concentrations and assembly histories: a probe of gravity?
• Dark Matter implications of the Fermi-LAT measurement of anisotropies in the diffuse gamma-ray background: status report
• Tail wavelets in the merger of binary compact objects
• Semi-analytic modelling of the europium production by neutron star mergers in the halo of the Milky Way
• Microwave background anisotropies due to non-linear structures in open and Lambda universes
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• Poisson type relativistic perfect fluid spheres
• Astrophysical aspects of milli-charged dark matter in a Higgs-Stueckelberg model
• The kinematical center and mass profile of the Local Group
• Probabilistic galactic dynamics I - the Sun and GJ 710 with Monte Carlo, linearised and unscented treatments
• TeV SUSY dark matter confronted with the current direct and indirect detection data
• More than just halo mass: Modelling how the red galaxy fraction depends on multiscale density in a HOD framework
• Moderate Galaxy-Galaxy Lensing
• Impact of radiation feedback on the assembly of star clusters in galactic context
• The RINGS Survey III: Medium-Resolution Halpha Fabry-Perot Kinematic Dataset
• Mean Occupation Function of High Redshift Quasars from the Planck Cluster Catalog
• Missing baryons in shells around galaxy clusters
• Three-dimensional axisymmetric sources for Majumdar-Papapetrou type spacetimes
• Wormholes in a viscous universe
• Strong Lensing Analysis of the Galaxy Cluster MACS J1319.9+7003 and the Discovery of a Shell Galaxy
• The Dark Matter Contribution to Galactic Diffuse Gamma Ray Emission
• On the Origin of the Variety of Velocity Dispersion Profiles of Galaxies
• Inelastic Scattering of Dark Matter with Heavy Cosmic Rays
• From particles to orbits: precise dark matter density profiles using dynamical information
• Dissecting Cosmological Filaments at High Redshifts: Emergence of Spaghetti-type Flow Inside DM Haloes
• Detecting Boosted Dark Photons with Gaseous Detectors
• A full reconstruction of two galaxy clusters intra-cluster medium with strong gravitational lensing
• Evidence for axion miniclusters with an increased central density
• Are there any extragalactic high speed dark matter particles in the Solar neighborhood?
• FLORAH: A generative model for halo assembly histories
• Limits on Early Matter Domination from the Isotropic Gamma-Ray Background
• Prospects for studying the mass and gas in protoclusters with future CMB observations
• Gravitational lensing by an ellipsoidal Navarro--Frenk--White dark-matter halo: An analytic solution and its properties
• Impact of Dynamical Friction on the Tidal Formation of NGC 1052-DF2
• Gamma rays from dark matter annihilation in the Draco and observability at ARGO
• On Stellar Migration from Andromeda to the Milky Way
• Intrinsic alignment from multiple shear estimates: A first application to data and forecasts for Stage IV
• Gravitational lenses in the dark Universe
• 3-3-1 Self Interacting Dark Matter and the Galaxy Core-Cusp problem
• Metallicity and kinematical clues to the formation of the Local Group
• Segue 2 Recently Collided with the Cetus-Palca Stream: New Opportunities to Constrain Dark Matter in an Ultra-Faint Dwarf
• Extreme Galaxy-scale Outflows Are Frequent among Luminous Early Quasars
• Direct and Indirect Detection of Neutralino Dark Matter and Collider Signatures in an $SO(10)$ Model with Two Intermediate Scales
• A Model Independent Method to Study Dark Matter induced Leptons and Gamma rays
• The final candidate from the JVAS/CLASS search for 6 arcsec to 15 arcsec image separation lensing
• Gravitational and distributed heating effects of a cD galaxy on the hydrodynamical structure of its host cluster
• The Ring Produced by an Extra-Galactic Superbubble in Flat Cosmology
• Discovery of Galactic center ejected star in DESI DR1
• CLASH-VLT velocity anisotropy profiles in a stack of massive galaxy clusters
• Star-forming galaxies in the cosmic web in the last 11 Gyr
• Hunting dark matter in galaxy clusters with non-thermal electrons
• A Redshift Survey of the Coma Cluster (A1656): Understanding the Nature of Subhalos in the Weak-lensing Map
• Primordial Black Hole Mergers as Probes of Dark Matter in Galactic Center
• Searching for rotation in X-COP galaxy clusters
• Cosmological Dark Matter in a Conformal Model
• Dark matter, extra-terrestrial gamma-rays and the MSSM: a viability study
• The Intergalactic Stellar Population from Mergers of Elliptical Galaxies with Dark Matter halos
• Formation and Evolution of sub-structures in tidal tails: Spherical dark matter haloes
• Supersymmetric chameleons and ultra-local models
• Directional Direct Detection of MeV Scale Boosted Dark Matter in Two Component Dark Matter Scenario via Dark Photon Interaction
• Probing lepton flavor violating dark matter scenarios via astrophysical photons and positrons
• Chaotic orbital dynamics of pulsating stars around black holes surrounded by dark matter halos
• Searching for Dark Matter Annihilation with IceCube and P-ONE
• Bounds on ALP-Mediated Dark Matter Models from Celestial Objects
• An implementation of nDGP gravity in Pinocchio
• Halo Pressure Profile through the Skew Cross-Power Spectrum of Sunyaev-Zel'dovich Effect and CMB Lensing in $\text{Planck}$
• Hypergeometric viable models in $f(R)$ gravity
• The dynamical evolution of the stellar clumps in the Sparkler galaxy
• Rotation curve decompositions with Gaussian Processes: taking into account data correlations leads to unbiased results
• Analytical insight into dark matter subhalo boost factors for Sommerfeld-enhanced $s$- and $p$-wave $\gamma$-ray signals
• Light propagation around a Kerr-like black hole immersed in an inhomogeneous anisotropic plasma in Rastall gravity: Analytical solutions to the equations of motion
• AVID: Formation and evolution of a coalesced major merger of late-type dwarf galaxies (VCC 479) on the outskirts of the Virgo cluster
• Probing black holes via quasinormal modes in a dark energy-induced dark matter
• Properties of Globular Clusters in Galaxy Clusters: Sensitivity from the Formation and Evolution of Globular Clusters
• The Kaleidoscope Survey: Strong Gravitational Lensing in Galaxy Clusters with Radial Arcs
• Core collapse in resonant self-interacting dark matter across two decades in halo mass
• When Freeze-out occurs due to a non-Boltzmann suppression: A study of degenerate dark sector
• Confronting the dark matter capture rate with a continuous gravitational wave probe of local neutron stars
• Directional Neutrino Searches for Galactic Center Dark Matter at Large Underground LArTPCs
• Galaxy Cluster Mass Estimation Through The Splashback Radius
• X-ray study of the double source plane gravitational lens system Eye of Horus observed with XMM-Newton
• EROS/MACHO Gravitational Microlensing Events Toward LMC in Evans Halo Model
• Self-Interacting Dark-Matter Spikes and the Final-Parsec Problem: Bayesian constraints from the NANOGrav 15-Year Gravitational-Wave Background
• Distribution Function of Dark Matter with Constant Anisotropy
• Microlensing towards the LMC revisited by adopting a non-Gaussian velocity distribution for the sources
• Triaxiality Inhibitors in N-Body Simulations
• Putting all the X in one basket: Updated X-ray constraints on sub-GeV Dark Matter
• Dark matter and alternative recipes for the missing mass
• A principle of corresponding states for two-component, self-gravitating fluids
• Searching for axion-like particles with SPHEREx
• Diffuse astrophysical neutrinos from dark matter around blazars
• Cosmological abundance of primordial black holes in mixed dark matter scenarios incorporating Kaluza-Klein dark matter
• Self-gravitating clusters of Bose-Einstein gas with planar, cylindrical, or spherical symmetry: gaseous density profiles and onset of condensation
• Is PSR J0514$-$4002E in a PBH-NS binary?
• Predicting Steady States of One-dimensional Collisionless Gravitating Systems
• Peculiar dark matter halos inferred from gravitational lensing as a manifestation of modified gravity
• Darker matter generating from the dark
• On the Outskirts of Dark Matter Haloes
• Semi-Analytic Modeling of Dark Matter Subhalo Encounters with Thin Stellar Streams: Statistical Predictions for GD-1-like Streams in CDM
• Dynamics of Companion Galaxies of Early-Type Galaxies
• The role of elliptic integrals in calculating the gravitational lensing of a charged Weyl black hole surrounded by plasma
• A numerical fit of analytical to simulated density profiles in dark matter haloes
• Constraints on superheavy dark matter decaying into $h\nu$, $Z\nu$ and $W\ell$ -- Benchmark example within an extended seesaw framework
• Predicting the Scaling Relations between the Dark Matter Halo Mass and Observables from Generalised Profiles II: Intracluster Gas Emission
• Investigating sub-MeV dark matter annihilation to neutrinos using direct detection experiments
• General circular velocity relation of a test particle in a 3D gravitational potential: application to the rotation curves analysis and total mass determination of UGC 8490 and UGC 9753
• Dark Matter, Dark Energy and Fundamental Acceleration
• New Analysis of the Proper Motions of the Magellanic Clouds using HST/WFPC2
• The electron plus positron spectrum from annihilation of Kaluza-Klein dark matter in the Galaxy
• COOL-LAMPS. VII. Quantifying Strong-lens Scaling Relations with 177 Cluster-scale Strong Gravitational Lenses in DECaLS
• Tidally-induced radial migration waves in LMC-like galaxies
• Revisiting the effect of lens mass models in cosmological applications of strong gravitational lensing
• DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [OII] Luminosity
• High-resolution HI mapping of nearby extremely metal-poor blue compact dwarf galaxies
• $\overline{\text{D}}$arkRayNet: Emulation of cosmic-ray antideuteron fluxes from dark matter
• Correlation between the Mean Matter Density and the Width of the Saturated Lyman Alpha Absorption
• A test of galaxy cluster fundamental plane for the X-COP sample
• A necessary condition for best fitting analytical to simulated density profiles in dark matter haloes
• Strong lensing cross sections for isothermal models - I. Finite source effects in the circular case
• Kinematic Lensing Inference II: Cluster Lensing with $\mathcal{O}$(1) Galaxies
• EDGES of the dark forest: A new absorption window into the composite dark matter and large scale structure
• The AIDA-TNG project: dark matter profiles and concentrations in alternative dark matter models
• The Three Hundred Project: dissecting the fundamental plane of galaxy clusters up to $z=1$
• Study of Various Dark Matter Halo Profiles in Milky Way and M31 Galaxies within the Standard Cosmology Framework
• Signature of biased range in the non-dynamical Chern-Simons modified gravity and its measurements with satellite-satellite tracking missions: Theoretical studies
• Linearity: galaxy formation encounters an unanticipated empirical relation
• Ultra-High Energy Cosmic Rays: The Annihilation of Super-Heavy Relics
• One-point Statistics in various cosmic environments in the presence of massive neutrinos
• Distances and Cosmology From Galaxy Cluster CMB Data
• Updated Models for the Creation of a Low-z QSO Absorber by a Dwarf Galaxy Wind
• Dark matter mass loss in galaxy flybys: dependence on impact parameter
• On the Encounter Rate of Open Star Clusters
• The AIDA-TNG project: 3D halo shapes
• Fermi Normal Coordinates and Fermion Curvature Couplings in General Relativity
• The Influence of Subhaloes on Host Halo Properties
• Too small to succeed: the difficulty of sustaining star formation in low-mass haloes
• Mass scaling relations for dark halos from an analytic universal outer density profile
• Bounds on galaxy stochasticity from halo occupation distribution modeling
• Maximally informed Bayesian modelling of disc galaxies
• Dark Energy Survey Year 3 Results: Galaxy mock catalogs for BAO analysis
• Search for dark matter with IACTs and the Cherenkov Telescope Array
• The Fourcade-Figueroa galaxy: a clearly disrupted superthin edge-on galaxy
• Head-on collisions of fuzzy/cold dark matter subhalos
• Axion Structure Formation II: The Wrath of Collapse
• Generalization of Rindler Potential at Cluster Scales in Randers-Finslerian Spacetime: a Possible Explanation of the Bullet Cluster 1E0657-558?
• Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
• Testing an entropy estimator related to the dynamical state of galaxy clusters
• HI-bearing dark galaxies predictions from constrained Local Group simulations: how many and where to find them
• The SRG/eROSITA all-sky survey: Constraints on Ultra-light Axion Dark Matter through Galaxy Cluster Number Counts
• Shining Light on Cosmogenic Axions with Neutrino Experiments
• Ring Formation from an Oscillating Black Hole
• The Outer Galactic Halo As Probed By RR Lyr Stars From the Palomar Transient Facility + Keck
• Electroweak Dark Matter
• Toward Gravitational Lensing in Modified Theories of Gravity
• Analytic Solutions for Navarro--Frenk--White Lens Models for Low Characteristic Convergences
• Selection Function of Clusters in Dark Energy Survey Year 3 Data from Cross-Matching with South Pole Telescope Detections
• Independent Measurements of the Dynamical Masses of Six Galaxy Clusters in the Local Universe
• A New Approach to Free-Form Cluster Lens Modeling Inspired by the JPEG Image Compression Method
• Diverse Rotation Curves of Galaxies in a Simulated Universe: the Observed Dependence on Stellar Mass and Morphology Reproduced
• Chemical enrichment by collapsars as the origin of the unusually high [Ba/Fe] in a massive star cluster of the dwarf galaxy NGC 1569
• A Predicted Relation between the Temperature and Density Profile of Cluster Hot Gas
• The SLUGGS survey: a new mask design to reconstruct the stellar populations and kinematics of both inner and outer galaxy regions
• The LPSZ-CLASH galaxy cluster sample: combining lensing and hydrostatic mass estimates
• Primordial black holes in Randall-Sundrum: Cosmological signatures
• Examining early-type galaxy scaling relations using simple dynamical models
• Observations of the Fermi bubbles and the Galactic center excess with the DArk Matter Particle Explorer
• Right-handed sneutrino and gravitino multicomponent dark matter in light of neutrino detectors
• The probability distribution of 3-D shapes of galaxy clusters from 2-D X-ray images
• Gravitational Redshift from Galaxy Clusters -- a Relativistic Approach
• Metamorphosis of dwarf halo density profile under dark matter decays
• Dark Matter and Fundamental Physics Searches with IACTs
• Effects of non-vanishing dark matter pressure in the Milky Way galaxy
• Ashes of FIRE: Modeling Dust Grain Size Evolution in the Local Group with FIRE
• Resolving the outer density profile of dark matter halo in Andromeda galaxy
• Chandra Studies of the X-ray Gas Properties of Fossil Systems
• Quantifying the Milky Way, LMC and their interaction using all-sky kinematics of outer halo stars
• On the morphology of $\gamma -$ray emission induced by $e^{\pm }$ from annihilating self-interacting dark matter
• A "Universal" Density Profile for the Outer Stellar Halos of Galaxies
• Dark matter signals and cosmic ray anomalies in an extended seesaw model
• Morphology of dark matter haloes beyond triaxiality
• The Hierarchical Structure of Galactic Haloes: Generalised N-Dimensional Clustering with CluSTAR-ND
• Simulating cosmic ray electron spectra and radio emission from an AGN jet outburst in a cool-core cluster
• Cross Section Calculations in Theories of Self-Interacting Dark Matter
• The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray stacking analysis of Subaru's optically selected clusters spanning low richness regime
• Matter environments around black holes: geodesics, light rings, and ultracompact configurations
• Modelling Giant Radio Halos
• Noble gravitational atoms: Self-gravitating black hole scalar wigs with angular momentum number
• Galaxies with Fuzzy Dark Matter
• Cluster environment quenches the star formation of low-mass satellite galaxies from the inside-out
• Ringdown of a black hole sourced by a Burkert-density effective anisotropic source
• HSC-XXL : Baryon budget of the 136 XXL Groups and Clusters
• Iterative mean-field approach to the spherical collapse of dark matter halos
• Rotation Curves in z~1-2 Star-Forming Disks: Comparison of Dark Matter Fractions and Disk Properties for Different Fitting Methods
• A hierarchical clustering method for quantifying satellite abundance
• Unequal-mass mergers of dark matter haloes with rare and frequent self-interactions
• Constraining Merging Galaxy Clusters with X-ray and Lensing Simulations and Observations: The case of Abell 2146
• Searching for Neutrinos from WIMP Annihilations in the Galactic Stellar Disk
• Using Strong Lensing to Detect Subhalos with Steep Inner Density Profiles
• Estimating Cluster Masses from SDSS Multi-band Images with Transfer Learning
• A Hydro-Particle-Mesh Code for Efficient and Rapid Simulations of the Intracluster Medium
• Baryon-driven decontraction in Milky Way mass haloes
• Threading the Magellanic Needle: Hypervelocity Stars Trace the Past Location of the LMC
• Searching for Dark Matter Particles with Compton Scattering Approach
• Eridanus IV: an Ultra-Faint Dwarf Galaxy Candidate Discovered in the DECam Local Volume Exploration Survey
• Predicting halo occupation and galaxy assembly bias with machine learning
• Neutrinos from stars in the Milky Way
• Does the Reionization Model Influence the Constraints on Dark Matter Decay or Annihilation?
• Parametric strong lensing model of the galaxy cluster Abell 2390 from Euclid and MUSE observations
• Effect of dark matter halo substructures on galaxy rotation curves
• Outflows from starburst galaxies with various driving mechanisms and their X-ray properties
• Explaining AMS-02 positron excess and muon anomalous magnetic moment in dark left-right gauge model
• To observe, or not to observe, quantum-coherent dark matter in the Milky Way, that is a question
• The Galactic potential and dark matter density from angular stellar accelerations
• LHAASO Galactic Plane $\gamma$-rays Strongly Constrain Heavy Dark Matter
• Holes within galaxies: the egg or the hen?
• Bounding the photon mass with cosmological propagation of fast radio bursts
• Two-phase formation of galaxies: the coevolution between galaxies and dark matter halos
• Orbit-based structural decomposition and stellar population recovery for edge-on barred galaxies
• Energy Conservation in the thin layer approximation: IV. The light curve for supernovae
• Signatures of large-scale cold fronts in the optically-selected merging cluster HSC J085024+001536
• Search for a photon peak from keV-scale dark matter annihilation with NuSTAR: Constraints on $⟨\sigma v⟩$ after 11 years of observations
• Post-Newtonian properties of EMRI with Power Law Potential
• Self-gravitating dark matter gets in shape
• Testing the Dark Universe through the Layzer-Irvine Equation
• Dark Matter spikes around Sgr A* in $\gamma$-rays
• An analytical model of surface mass densities of cold dark matter haloes - with an application to MACHO microlensing optical depths
• Pattern dark matter and galaxy scaling relations
• Renzo's rule revisited: A statistical study of galaxies' baryon - dark matter coupling
• Dissecting the Strong-lensing Galaxy Cluster MS 0440.5+0204. I. The Mass Density Profile
• MrMARTIAN: A Multi-resolution Mass Reconstruction Algorithm Combining Free-form and Analytic Components
• Constraining Gamma-ray Lines from Dark Matter Annihilation using Fermi-LAT and H.E.S.S. data
• SILCC -- IX. The multi-phase interstellar medium at low metallicity
• INTEGRAL, eROSITA and Voyager Constraints on Light Bosonic Dark Matter: ALPs, Dark Photons, Scalars, $B-L$ and $L_i-L_j$ Vectors
• Dynamical friction and massive black hole orbits: analytical predictions and numerical solutions
• Detecting Dark Photons from Atomic Rearrangement in the Galaxy
• Determining the primordial helium abundance and UV background using fluorescent emission in star-free dark matter haloes
• Phase space of static wormholes sustained by an isotropic perfect fluid
• Limits on Dark Matter Annihilation from the Shape of Radio Emission in M31
• Conformal Gravity and the Radial Acceleration Relation
• Macroscopic states in Bose-Einstein condensate dark matter model with axionlike interaction
• Scalarization and superradiant instability of black hole induced by dark matter halo in the scalar-tensor theory of gravity
• Matching the dark matter profiles of dSph galaxies with those of simulated satellites: a two parameter comparison
• A Mean-Field Approach to Simulating the Merging of Collisionless Stellar Systems Using a Particle-Based Method
• Modeling Dark Matter Halos with Nonlinear Field Theories
• Winds versus jets: a comparison between black hole feedback modes in simulations of idealized galaxy groups and clusters
• Local virial relation and velocity anisotropy in self-gravitating system
• Milky Way globular cluster dynamics: are they preferentially co-rotating?
• Dark matter haloes in the multicomponent model. III. From dwarfs to galaxy clusters
• Massive Star Clusters in the Semi-Analytical Galaxy Formation Model L-Galaxies 2020
• Plausible Indication of Gamma-Ray Absorption by Dark Matter in NGC 1068
• Dark matter according to the tensor-four-scalars theory
• It is Feasible to Directly Measure Black Hole Masses in the First Galaxies
• Poisson type conformastat spherically symmetric anisotropic fluid spacetimes
• Disk galaxies and their dark halos as self-organized patterns
• Cosmological implications of electromagnetically interacting dark matter: milli-charged particles and atoms with singly and doubly charged dark matter
• Emulating the Non-Linear Matter Power-Spectrum in Mixed Axion Dark Matter Models
• New model of density distribution for fermionic dark matter halos
• Orbital dynamics in galactic potentials under mass transfer
• Modelling Gaia photometry signals of dark halos
• Multi-transonic spherical-type flows around massive black holes: galactic potential induced standing isothermal shocks
• General relativistic quasi-spherical accretion in a dark matter halo
• Dark matter properties implied by gamma ray interstellar emission models
• The Integrated Cluster Finder for the ARCHES project
• On the Assembly Bias of Cool Core Clusters Traced by H$\alpha$ Nebulae
• Dark Stars: Dark Matter in the First Stars leads to a New Phase of Stellar Evolution
• Towards characterizing dark matter subhalo perturbations in stellar streams with graph neural networks
• Venice: a multi-scale operator-splitting algorithm for multi-physics simulations
• AMICO-WL: an optimal filtering algorithm for galaxy cluster detections with weak lensing
• Dark matter halo dynamics in 2D Vlasov Simulations: a self-similar approach
• Measuring the Stellar-to-Halo Mass Relation at $\sim 10^{10}$ Solar masses, using forthcoming space-based imaging of galaxy-galaxy strong lenses
• Distribution Function in Center of Dark Matter Halo
• Biases in inferring dark matter profiles from dynamical and lensing measurements
• Kinematics of the Sagittarius Dwarf Spheroidal core: A 5D Analysis for a 6D Methodology with Gaia DR3
• Can hidden correlations mimic a variable fine structure constant?
• Searching for dark matter annihilating into light long-lived mediators from stars inside dwarf spheroidal galaxies
• Many body gravity and the galaxy rotation curves
• How Black Holes Stop Their Host Galaxy from Growing Without AGN Feedback
• A Relativistic Tensorial Model for Fractional Interaction between Dark Matter and Gravity
• GeV excess and phenomenological astrophysics modeling
• How Many Bursts Does it Take to Form a Core at the Center of a Galaxy?
• Detecting stable massive neutral particles through particle lensing
• Testing local position invariance with odd multipoles of galaxy clustering statistics
• The APOSTLE simulations: Rotation curves derived from synthetic 21-cm observations
• Retuning radio astronomy for axion dark matter with neutron stars
• Measuring the boson mass of fuzzy dark matter with stellar proper motions
• Radiation and energy release in a background field of axion-like dark matter
• Dark matter in ALFALFA galaxies: Investigating galaxy-halo connection
• Effects of light-mass fermionic dark matter on the equilibrium and stability of white dwarfs
• An Interpretable AI Framework to Disentangle Self-Interacting and Cold Dark Matter in Galaxy Clusters: The CKAN Approach
• HerS-3: An Exceptional Einstein Cross Reveals a Massive Dark Matter Halo
• Prospects for Cosmology with Cluster Mass Profiles
• Revisiting Galaxy Cluster Scaling Relations through Dark Matter-Gas Coherence: Scatter Dependence on Dynamical State
• Milky Way Mass Through Escape Velocity Curve from LAMOST K Giants
• Supplying Dark Energy from Scalar Field Dark Matter
• Helium reionization in the presence of self-annihilating clumpy dark matter
• Overmassive and Undermassive Massive Black Holes: The Role of Environment and Gravitational-Wave Recoils
• MIGHTEE: The dark matter haloes, duty cycle and mechanical feedback from radio-AGN up to $z\sim 2.5$
• The Baryonic Mass Estimates of the Milky Way Halo in the form of High Velocity Clouds
• Production of antimatter in the galaxy
• Comparing radial migration in dark matter and MOND regimes
• Constructing Merger Trees of Density Peaks Using Phase-Space Watershed Segmentation Algorithm
• Cusped Mass Density Profiles and Magnification Ratios of Double Image Gravitational Lenses
• Self-gravitating quantum stars with a globally relevant Bohm potential
• Constraining dark photon parameters based on the very high energy observations of blazars
• Exploiting Machine Learning and Disequilibrium in Galaxy Clusters to Obtain a Mass Profile
• Gravitational signatures of ALP dark matter fragmentation
• Refracted Gravity Solutions from Small to Large Scales
• A semi-analytic estimate for the effective sound speed counterterm in the EFTofLSS
• Cored Dark Matter halos in the Cosmic Neutrino Background
• Data-driven modeling of rotation curves with artificial neural networks
• What is the amount of baryonic dark matter in galaxies?
• Dark Matter Universal Properties in Galaxies
• Analysing the Effect on CMB in a Parity and Charge Parity Violating Varying Alpha Theory
• Merging Galaxy Clusters and the Search for New Physics of Dark Matter: A Review
• Structure-wide dark matter density depletion induced by local degeneracies
• Scattering meets absorption in dark matter detection
• Charge distribution of the gauge-mediation type Q ball
• Phase spirals induced by the gas warp
• Equilibrium of stellar dynamical systems in the context of the Vlasov-Poisson model
• Combined analyses of the antiproton production from cosmic-ray interactions and its possible dark matter origin
• SCF-FDPS: A Fast $N$-body Code for Simulating Disk-halo Systems
• SHARP VIII: J0924+0219 lens mass distribution and time-delay prediction through adaptive-optics imaging
• Probing the large-scale structure with 21cm-galaxy cross-bispectrum: Estimates from simulations and forecasts for upcoming cosmological surveys
• Multiple UHECR Events from Galactic hadron jets
• A Non-parametric Method for the Inference of Halo Occupation Distributions
• Simulating Jellyfish Galaxies: A Case Study for a Gas-Rich Dwarf Galaxy
• Role of the companion lensing galaxy in the CLASS gravitational lens B1152+199
• GalPort: Investigation of the bar in action-angle space
• Wrinkles in Time. II. Stellar Age Trends in Kinematic Signatures from Transient Spiral Structure
• Constraints on extended axion structures from the lensing of fast radio bursts
• Gravitational emissions and light curves of quasi-periodic orbits in Schwarzschild spacetime embedded in a Dehnen-type dark matter halo
• 130GeV gamma-ray line through axion conversion
• Electron-positron Annihilation Lines and Decaying Sterile Neutrinos
• The role of dark matter in the galaxy mass-size relationship
• AutoKnots: Adaptive Knot Allocation for Spline Interpolation
• Constraining branon dark matter from observations of the Segue 1 dwarf spheroidal galaxy with the MAGIC telescopes
• Properties of the Intracluster Medium Assuming an Einasto Dark Matter Profile
• The orbital dynamics of the LMC and SMC about the Milky Way
• Detecting dark matter substructure with lensed quasars in optical bands
• Initial Mass Function for Massive Galaxies at z$\sim$1
• Tidal stripping as a mechanism for placing globular clusters on wide orbits: the case of MGC1 in M31
• Uncertainties in measuring the dark matter signal from Milky Way satellites using Cherenkov telescopes
• Prediction of Individual Halo Concentrations Across Cosmic Time Using Neural Networks
• Simulating High-Redshift Disk Galaxies: Applications to Long Duration Gamma-Ray Burst Hosts
• Self-gravitating system of semidegenerate fermions as central objects and dark matter halos in galaxies
• Tidal Limit of Stellar Systems in Two-Power Density Models
• The Effects of Cosmic-Ray Diffusion and Radiative Cooling on the Galactic Wind from the Milky Way
• Probing late-time annihilations of oscillating asymmetric dark matter via rotation curves of galaxies
• Superbubbles as the source of dynamical friction: gas migration, stellar and dark matter contributions
• Entropy Production in Collisionless Systems. III. Results from Simulations
• Galactic Scaling Rules in a Modified Dynamical Model
• The Non-universal Pseudo Phase-Space Density Profiles of Symphony Host Halos
• Universal Basic Mass Density inside Dark Matter Halos
• Correlation between Outlying Halo Abundance and Host Halo Properties
• Hubble Expansion Signature on Simulated Halo Density Profiles: A Path to Observing the Turnaround Radius
• Constraining Asymmetric DM Properties by Black Hole Formation in Neutron Stars and Population III Stars
• Leptogenesis from composite singlets
• First evidence of a collision between two unrelated open clusters in the Milky Way
• Triplet Dark Matter from leptogenesis
• Detecting low-mass haloes with strong gravitational lensing I: the effect of data quality and lensing configuration
• Galactic tides and the Crater II dwarf spheroidal: a challenge to LCDM?
• Forecasting the potential of weak lensing magnification to enhance LSST large-scale structure analyses
• Impact of Sommerfeld enhancement on helium reionization via WIMP dark matter
• Collisional Dynamics of Stars and Dark Matter in Ultra-Faint Galaxies
• A dynamics-based density profile for dark haloes. I. Algorithm and basic results
• The interface of gravity and dark energy
• Discovering the building blocks of dark matter halo density profiles with neural networks
• Origin of the spectacular tidal shells of galaxy NGC474
• Kinematic Mapping of Giant Arcs: A New Method to Locate Lensing Critical Curves
• Probing Dark Matter Substructure with Image Number Anomaly in Strong Lensing Systems
• Assembly History and Internal Structure of Cluster Cold Dark Matter Haloes
• On the Kinematic Morphology around Halos
• The origin of ionized gas in retired galaxies: dynamical clues
• Heavy dark matter in rapidly evolving massive stars
• The Sensitivity of PUEO to Cosmogenic Neutrinos and Exotic Physics Scenarios
• What Can Gamma-rays from Space tell us About the Madala Hypothesis?
• DarkMix: Mixture Models for the Detection and Characterization of Dark Matter Halos
• Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos
• The Distribution of Satellite Galaxies in the TNG100 Simulation
• Gravity as embedding theory and the distribution of matter in galaxies
• Dark Energy and Extending the Geodesic Equations of Motion: A Spectrum of Galactic Rotation Curves
• Modeling the Accretion of High-Velocity Clouds from a Rotating Halo
• Cross-checking SMBH mass estimates in NGC 6958 -- I: Stellar dynamics from adaptive optics-assisted MUSE observations
• In medio stat virtus: enrichment history in poor galaxy clusters
• The Splashback Mass Function of Galaxy Clusters from Photometric Data
• CWTHF: Subhalo Identification with Continuous Wavelet Transform
• Independent Evidence for earlier formation epochs of fossil groups of galaxies through the intracluster light: the case for RX J100742.53+380046.6
• Numerical Study of Bar Suppression in Galaxy Models Due to Disc Heating
• The $10\mathrm{kpc}$ collar of early-type galaxies -- probing evolution by focusing on the inner stellar density profile
• Determination of Dark Matter Properties at High-Energy Colliders
• Weak gravitational flexion in various spacetimes: Exotic lenses and modified gravity
• A bar stability criterion distinguishing between modified gravity and dark matter in galaxies
• Constraints on dark matter annihilation and turbulent reacceleration set by high-frequency observations of the radio halo in the Coma cluster
• Mock Catalogs of Strongly Lensed Gravitational Waves via A Halo Model Approach with Ground-based Detectors
• Evidence for merging or disruption of red galaxies from the evolution of their clustering
• Galaxy rotation curves in the light of the Spinor Theory of Gravity
• Modeling Cosmological Evolution of Jetted Seyfert Galaxies for z<10
• The cosmic journey of dust grains -- from nucleation to planetary system
• 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
• Controlled Experiments on Dark-Matter Halo Structure and Galaxy Morphology I: What Sets Galaxy Sizes?
• Single- and double-headed odd radio circles in the LOFAR surveys
• ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations
• CLASH-VLT: The Fifth Force in Chameleon Gravity from Joint Lensing and Kinematics Cluster Mass Profiles
• The potential of diffuse Galactic Ridge neutrino measurements to constrain dark matter
• The dynamical state of bars in cluster dwarf galaxies: The cases of NGC 4483 and NGC 4516
• Dynamical Properties and Velocity Dispersion-Mass Relation of $z\sim 1$ Galaxy Clusters from the GOGREEN and GCLASS Surveys
• Mergers as a Probe of Particle Dark Matter
• Comparison of Modeling SPARC spiral galaxies' rotation curves: halo models vs MOND
• Self-similarity of the mass distribution in rich galaxy clusters up z~1 tracked with weak lensing
• Studying dark matter with MadDM: lines and loops
• Physics beyond the Standard Model with the DSA-2000
• Accretion of self-interacting dark matter onto supermassive black holes
• Antinuclei from Primordial Black Holes
• A short review on joint weak and strong cluster lens-mass reconstruction
• Detecting a physical difference between the CDM halos in simulation and in nature
• Mapping the evolution of supernova-neutrino-boosted dark matter within the Milky Way
• Spherically Symmetric Potentials in Quadratic $f(R)$ Gravity
• Calibrating the SIDM Gravothermal Catastrophe with N-body Simulations
• Towards a universal model for the density profiles of dark matter haloes
• Broken Expectations: The Effects of Modelling Assumptions on the Inferred Dark Matter Distribution in the Milky Way's Satellites
• Multi-component, axisymmetric dynamical models of dSphs based on distribution functions: inferences on dark matter and intermediate-mass black holes in Draco and Ursa Minor
• Constraining the MOdified Newtonian Dynamics from spherically symmetrical hydrodynamic accretion
• Linking the KM3-230213A Neutrino Event to Dark Matter Decay and Gravitational Wave signals
• Diffusion of Cosmic Antiprotons Generated throughout the Dark Matter Halo -- A Semi-Analytical Solution for a Linear Galactic Wind Model
• A probabilistic deep learning model to distinguish cusps and cores in dwarf galaxies
• SDSS-IV MaNGA: A Catalogue of Spectroscopically Detected Strong Galaxy-Galaxy Lens Candidates
• Wiener filtering and multi-tracer techniques for dark matter cross-correlations between gamma-ray emission and galaxy catalogs
• Modeling Multiphase Galactic Outflows: A Multifluid Moving Mesh Approach
• Calculation of Dark Matter as a Feature of Space-Time
• Estimating galaxy masses from kinematics of globular cluster systems: a new method based on deep learning
• Why most molecular clouds are gravitationally dominated
• Resolving circumgalactic gas flows around a z$\approx$3.6 quasar using MUSE and ALMA
• The Hydrostatic Mass Bias and the ${\sigma }_8$ Tension: A Multi-Probe Forecast for Stage-IV/V Surveys
• Constraints on dark and visible mass in galaxies from strong gravitational lensing
• Gravitational memory meets astrophysical environments: exploring a new frontier through osculations
• DHOST gravity in Ultra-diffuse galaxies -- Part I: the case of NGC1052-DF2
• Dynamical models of spheroidal multi-component stellar systems
• Milky-Way-like stars in a galaxy core 8 billion years ago revealed by gravitational lensing
• Charged wormholes supported by 2-fluid immiscible matter particles
• Structure Formation under Inelastic Two-Component Dark Matter: Halo Statistics and Matter Power Spectra in the High-$z$ Universe
• Gravitational Lensing By a Massive Object in a Dark Matter Halo. I. Critical Curves and Caustics
• A Mass Dependent Density Profile from Dwarfs to Clusters
• Distinguishing Dark Matter Cusps from Cores using Globular Clusters
• The shapes of dark matter dominated dwarf spheroidal stellar density profiles
• Imprints of flavor anomalies on neutrino oscillations through dark matter halo
• The Galactic Pizza: Flat Rotation Curves in the Context of Cosmological Time-Energy Coupling
• On the flat galactic rotational curves in $f(\mathcal{R})$ gravity
• Tensorial solution of the Poisson equation and the dark matter amount and distribution of UGC 8490 and UGC 9753
• The SRG/eROSITA All-Sky Survey $J$-Band Follow-Up Observations for Selected High-Redshift Galaxy Cluster Candidates
• Simulating the complexity of the dark matter sheet II: halo and subhalo mass functions for non-cold dark matter models
• A Pearl in the Shell: an ultra-compact dwarf within the tidal debris surrounding spiral galaxy NGC 7531
• Post-collapse Lagrangian perturbation theory in three dimensions
• Probing Dark Matter with Strong Gravitational Lensing through an Effective Density Slope
• Systematic variation of central mass density slope in early-type galaxies
• Constraints on cosmic rays in the Milky Way circumgalactic medium from OVIII observations
• Rotational Curves of the Milky Way Galaxy and Andromeda Galaxy in Light of Vacuum Polarization around Eicheon
• Quantifying the Rarity of the Local Super-Volume
• Effects of Hawking evaporation on PBH distributions
• Dissecting the strong lensing galaxy cluster MS 0440$+$0204 II. New optical spectroscopic observations in a wider area and cluster dynamical state
• A z$\sim$1 galactic-scale outflow transversally mapped to $\sim$50 kpc through gravitational-arc tomography
• A Near-Infrared look at AGN Feedback in Bulgeless Galaxies
• Stochastic gravitational wave background from the collisions of dark matter halos
• Exact Solutions with Asymptotically Flat Galactic Rotation Curves
• How black holes turn cusps into cores
• Boson dark matter halos with a dominant noncondensed component
• Studying The Effect of Radiation Pressure on Evolution of a Population III Stellar Cluster
• Piercing of a boson star by a black hole
• Effect of dark matter halos on the orbital and escape dynamics of barred galaxies