Cold dark matter haloes in the Planck era: evolution of structural parameters for Einasto and NFW profiles

Abstract

We present the evolution of the structure of relaxed cold dark matter haloes in the cosmology from the Planck satellite. Our simulations cover 5 decades in halo mass, from dwarf galaxies to galaxy clusters. Due to the increased matter density and power spectrum normalization the concentration mass relation in the Planck cosmology has a 20 percent higher normalization at redshift z=0 compared to WMAP cosmology. We confirm that CDM haloes are better described by the Einasto profile; for example, at scales near galaxy half-light radii CDM haloes have significantly steeper density profiles than implied by NFW fits. There is a scatter of 0.2 dex in the Einasto shape parameter at fixed halo mass, adding further to the diversity of CDM halo profiles. The evolution of the concentration mass relation in our simulations is not reproduced by any of the analytic models in the literature. We thus provide a simple fitting formula that accurately describes the evolution between redshifts z=5 to z=0 for both NFW and Einasto fits. Finally, the observed concentrations and halo masses of spiral galaxies, groups and clusters of galaxies at low redshifts are in good agreement with our simulations, suggesting only mild halo response to galaxy formation on these scales.

18 pages, 18 figures, accepted to MNRAS, minor changes to previous version

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• The GOGREEN survey: the internal dynamics of clusters of galaxies at redshift 0.9-1.4
• 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
• On the early evolution of Local Group dwarf galaxy types: star formation and supernova feedback
• Kinematics of the Tucana Dwarf Galaxy: An Unusually Dense Dwarf in the Local Group
• Using LISA-like Gravitational Wave Detectors to Search for Primordial Black Holes
• Scaling Relations of Halo Cores for Self-Interacting Dark Matter
• Dark-matter-deficient galaxies in hydrodynamical simulations
• Do halos that form early, have high concentration, are part of a pair, or contain a central galaxy potential host more pronounced planes of satellite galaxies?
• Prospects for detecting gravitational waves from eccentric subsolar mass compact binaries
• Backflows by AGN jets: Global properties and influence on SMBH accretion
• A first estimate of the Milky Way dark matter halo spin
• Weak Lensing Analysis of CODEX Clusters using Dark Energy Camera Legacy Survey : Mass-Richness Relation
• From the core to the outskirts: structure analysis of three massive galaxy clusters
• Cosmology and Astrophysics from Relaxed Galaxy Clusters V: Consistency with Cold Dark Matter Structure Formation
• Halo Properties and Mass Functions of Groups/Clusters from the DESI Legacy Imaging Surveys DR9
• Illuminating Dark Matter Halo Density Profiles Without Subhaloes
• A general framework to test gravity using galaxy clusters IV: Cluster and halo properties in DGP gravity
• Cosmological and idealized simulations of dark matter haloes with velocity-dependent, rare and frequent self-interactions
• Constraining interacting dark energy models with the halo concentration-mass relation
• The halo mass function of late-type galaxies from HI kinematics
• Major mergers between dark matter haloes -- II. Profile and concentration changes
• Galaxy Zoo: constraining the origin of spiral arms
• Extending empirical constraints on the SZ-mass scaling relation to higher redshifts via HST weak lensing measurements of nine clusters from the SPT-SZ survey at $z\gtrsim 1$
• Characterizing fast radio bursts through statistical cross-correlations
• 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
• Which Milky Way masses are consistent with the slightly declining 5-25 kpc rotation curve?
• The halo mass of optically-luminous quasars at z=1-2 measured via gravitational deflection of the cosmic microwave background
• Weak lensing mass modeling bias and the impact of miscentring
• Evolution of the luminosity-to-halo mass relation of LRGs from a combined SDSS-DR10+RCS2 analysis
• A Multiwavelength Study of ELAN Environments (AMUSE${}^2$). Mass budget, satellites spin alignment and gas infall in a massive $z\sim 3$ quasar host halo
• Multi-wavelength Analysis of the Merging Galaxy Cluster A115
• A high baryon fraction in massive haloes at z~3
• Tidal disruption events can power the observed AGN in dwarf galaxies
• Towards a higher mass for NGC1052-DF2: an analysis based on full distribution functions
• Velocity dispersion and dynamical mass for 270 galaxy clusters in the Planck PSZ1 catalogue
• A scenario for ultra-diffuse satellite galaxies with low velocity dispersions: the case of [KKS 2000]04
• How the first stars shaped the faintest gas-dominated dwarf galaxies
• The Effect of Adiabatic Compression on Dark Matter Halos and the Radial Acceleration Relation
• First Weak-lensing Results from "See Change": Quantifying Dark Matter in the Two Z>1.5 High-redshift Galaxy Clusters SPT-CL J2040-4451 and IDCS J1426+3508
• Orbit-Superposition Dynamical Modeling of Barred Galaxies
• Keck Spectroscopy of the Coma Cluster Ultra-Diffuse Galaxy Y358: Dynamical Mass in a Wider Context
• The Variation of Rotation Curve Shapes as a Signature of the Effects of Baryons on Dark Matter Density Profiles
• An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
• Galaxy rotation curves and universal scaling relations: comparison between phenomenological and fermionic dark matter profiles
• The Bimodal Absorption System Imaging Campaign (BASIC) I. A Dual Population of Low-metallicity Absorbers at z $<1$
• The cusp-core problem in gas-poor dwarf spheroidal galaxies
• Strong lensing with superfluid dark matter
• Post-inflationary axion isocurvature perturbations facing CMB and large-scale structure
• The galaxy correlation function as a constraint on galaxy formation physics
• Exploring extensions to the standard cosmological model and the impact of baryons on small scales
• AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis
• Another baryon miracle? Testing solutions to the "missing dwarfs" problem
• Escalating core formation with dark matter self-heating
• Fast generation of mock galaxy catalogues in modified gravity models with COLA
• A portrait of the Vast Polar Structure as a young phenomenon: hints from its member satellites
• Galaxy Formation with Local Photoionization Feedback -II. Effect of X-Ray Emission from Binaries and Hot Gas
• Dark Matter and IMF normalization in Virgo dwarf early-type galaxies
• The massive dark halo of the compact, early-type galaxy NGC 1281
• The distribution of dark matter and gas spanning six megaparsecs around the post-merger galaxy cluster MS0451-03
• Hierarchical inference of the relationship between Concentration and Mass in Galaxy Groups and Clusters
• Primordial Black Hole Merger Rate in Self-Interacting Dark Matter Halo Models
• Pushing down the low-mass halo concentration frontier with the Lomonosov cosmological simulations
• MG-MAMPOSSt: A code to test modifications of gravity with the dynamics of galaxy clusters
• FIR-luminous [CII] emitters in the ALMA-SCUBA-2 COSMOS survey (AS2COSMOS): The nature of submillimeter galaxies in a 10 comoving Mpc-scale structure at z~4.6
• Is GW170817 a Multimessenger Neutron Star-Primordial Black Hole Merger?
• MUSE-ALMA Halos VI: Coupling Atomic, Ionised & Molecular Gas Kinematics of Galaxies
• Incorporating baryon-driven contraction of dark matter halos in rotation curve fits
• On the change of old neutron star masses with galactocentric distance
• The Fornax3D project: Environmental effects on the assembly of dynamically cold disks in Fornax cluster galaxies
• Subhalo sinking and off-center massive black holes in dwarf galaxies
• From spirals to lenticulars: evidence from the rotation curves and mass models of three early-type galaxies
• HSTPROMO Internal Proper Motion Kinematics of Dwarf Spheroidal Galaxies: I. Velocity Anisotropy and Dark Matter Cusp Slope of Draco
• Constraining the Mass of the Emerging Galaxy Cluster SpARCS1049+56 at z=1.71 with Infrared Weak Lensing
• A finer view of the conditional galaxy luminosity function and magnitude-gap statistics
• The Concentration-Mass Relation of Massive, Dynamically Relaxed Galaxy Clusters: Agreement Between Observations and $\Lambda$CDM Simulations
• The galaxy-halo connection of disc galaxies over six orders of magnitude in stellar mass
• Local photoionization feedback effects on galaxies
• The SLUGGS Survey: The Inner Dark Matter Density Slope of the Massive Elliptical Galaxy NGC 1407
• Unveiling the Fast Acceleration of AGN-Driven Winds at Kiloparsec Scales
• A new class of dark matter-free dwarf galaxies? I. Clues from FCC 224, NGC 1052-DF2 and NGC 1052-DF4
• Characteristics of Effective Dark Matter in Nonlocal Gravity
• Deflection of light by wormholes and its shadow due to dark matter within modified symmetric teleparallel gravity formalism
• Searching for primordial black holes with stochastic gravitational-wave background in the space-based detector frequency band
• Dynamical masses of brightest cluster galaxies I: stellar velocity anisotropy and mass-to-light ratios
• The evolution of compact massive quiescent and starforming galaxies derived from the $R_e-R_h$ and $M_{\mathrm{star}}-M_h$ relations
• QSOs sigposting cluster size halos as gravitational lenses: halo mass, projected mass density profile and concentration at $z\sim 0.7$
• The COSMOS-Web ring: in-depth characterization of an Einstein ring lensing system at z~2
• Detecting the Figure Rotation of Dark Matter Halos with Tidal Streams
• SUPER VIII. Fast and Furious at $z\sim 2$: obscured type-2 active nuclei host faster ionised winds than type-1 systems
• CLASH-VLT: The inner slope of the MACS J1206.2-0847 dark matter density profile
• CODEX Weak Lensing Mass Catalogue and implications on the mass-richness relation
• Patchy Screening of the CMB from Dark Photons
• The stellar mass function and evolution of the density profile of galaxy clusters from the Hydrangea simulations at $0<z<1.5$
• Compact Binary Merger Rate in Dark-Matter Spikes
• The edge of galaxy formation III: The effects of warm dark matter on Milky Way satellites and field dwarfs
• The Luminous X-Ray Halos of Two Compact Elliptical Galaxies
• 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
• A discrete chemo-dynamical model of M87's globular clusters: Kinematics extending to ~ 400 kpc
• Quantifying the stellar ages of dynamically separated bulges and disks of CALIFA spiral galaxies
• On the Impact of Neutron Star Binaries Natal-Kick Distribution on the Galactic r-process Enrichment
• Testing the parametric model for self-interacting dark matter using matched halos in cosmological simulations
• Probing cold dark matter subhalos with simulated ALMA observations of macrolensed sub-mm galaxies
• The radial acceleration relation is a natural consequence of the baryonic Tully-Fisher relation
• The Flatness and Sudden Evolution of the Intergalactic Ionizing Background
• The ALMA-CRISTAL survey: Resolved kinematic studies of main sequence star-forming galaxies at 4<z<6
• Bulge formation through disc instability -- I
• The radial dependence of dark matter distribution in M33
• Joint Gas and Stellar Dynamical Models of WLM: An isolated dwarf galaxy within a cored, prolate DM halo
• On the choice of the most suitable indicator for the assembly state of dark matter haloes through cosmic time
• Extragalactic diffuse gamma-rays from dark matter annihilation: revised prediction and full modelling uncertainties
• Kinematics and Mass Distributions for Non-Spherical Deprojected Sérsic Density Profiles and Applications to Multi-Component Galactic Systems
• Discriminating power of milli-lensing observations for dark matter models
• A Versatile and Accurate Method for Halo Mass Determination from Phase-Space Distribution of Satellite Galaxies
• WISDOM Project -- XIII. Feeding molecular gas to the supermassive black hole in the starburst AGN-host galaxy Fairall 49
• Not All Subhaloes Are Created Equal: Modelling the Diversity of Subhalo Density Profiles in TNG50
• The Relevance of Dynamical Friction for the MW/LMC/SMC Triple System
• A shallow dark matter halo in Ultra Diffuse Galaxy AGC 242019: are UDGs structurally similar to low surface brightness galaxies?
• The Super-NFW model: an analytic dynamical model for cold dark matter haloes and elliptical galaxies
• Dynamical modelling and origin of gas turbulence in z $\sim$ 4.5 galaxies
• Micro galaxies in LCDM
• Isothermal Bondi accretion in two-component Jaffe galaxies with a central black hole
• Precise Mass Determination of SPT-CL J2106-5844, the Most Massive Cluster at z>1
• Characterising the Structure of Halo Merger Trees Using a Single Parameter: The Tree Entropy
• Testing baryon-induced core formation in $\Lambda$CDM: A comparison of the DC14 and coreNFW dark matter halo models on galaxy rotation curves
• The Merger Rate of Primordial Black Hole-Neutron Star Binaries in Ellipsoidal-Collapse Dark Matter Halo Models
• A New Interpretation of the Mass-Temperature Relation and Mass Calibration of Galaxy Clusters Based on the Fundamental Plane
• Centrally Concentrated H I Distribution Enhances Star Formation in Galaxies
• Properties and observables of massive galaxies in self-interacting dark matter cosmologies
• Radial Distribution Of ISM Gas-phase Metallicity In CLASH Clusters at z~0.35: A New Outlook On Environmental Impact On Galaxy Evolution
• The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
• Future sensitivity of neutrino telescopes to dark matter annihilations from the cosmic diffuse neutrino signal
• Calibrating the Planck Cluster Mass Scale with Cluster Velocity Dispersions
• GalICS 2.1: a new semianalytic model for cold accretion, cooling, feedback and their roles in galaxy formation
• Next Generation Virgo Cluster Survey. XXI. The weak lensing masses of the CFHTLS and NGVS RedGOLD galaxy clusters and calibration of the optical richness
• Prospects for Determining the Mass Distributions of Galaxy Clusters on Large Scales Using Weak Gravitational Lensing
• MHONGOOSE discovery of a gas-rich low-surface brightness galaxy in the Dorado Group
• Core Fragmentation in Simplest Superfluid Dark Matter Scenario
• Stellar Feedback and the Energy Budget of Late-Type Galaxies: Missing Baryons and Core Creation
• Time Delay of Light in the Gravitational lensing of Supermassive Black Holes in Dark Matter Halos
• Clouds accreting from the IGM are not able to feed the star formation of low-redshift disc galaxies
• On the link between nuclear star cluster and globular cluster system mass, nucleation fraction and environment
• Inflow of low-metallicity cool gas in the halo of the Andromeda galaxy
• Group galaxy number density profiles far out: is the 'one-halo' term NFW out to $>10$ virial radii?
• The Clustering of Undetected High-redshift Black Holes and Their Signatures in Cosmic Backgrounds
• Gravitational redshifting of galaxies in the SPIDERS cluster catalogue
• Sunyaev--Zel'dovich profile fitting with joint AMI-Planck analysis
• Toward Solving the Puzzle: Dissecting the Complex Merger A521 with Multi-wavelength Data
• The Unusually High Halo Concentration of the Fossil Group NGC 6482: Evidence for Weak Adiabatic Contraction
• Mass Calibration of the CODEX Cluster Sample using SPIDERS Spectroscopy -- II. The X-ray Luminosity-Mass Relation
• Effects of Coupled Dark Energy on the Milky Way and its Satellites
• Probing dark energy via galaxy cluster outskirts
• Constraining Chameleon screening using galaxy cluster dynamics
• The cosmology dependence of the concentration-mass-redshift relation
• The Puzzling Origin of Massive Compact Galaxies in MaNGA
• Effect of a High-Precision Semi-Analytical Mass Function on the Merger Rate of Primordial Black Holes in Dark Matter Halos
• On the Merger Rate of Primordial Black Holes in Cosmic Voids
• Cuspy dark matter density profiles in massive dwarf galaxies
• Accurate Computation of the Screening of Scalar Fifth Forces in Galaxies
• Empirical Evidence of Non-Minimally Coupled Dark Matter in the Dynamics of Local Spiral Galaxies?
• Looking for Traces of Non-minimally Coupled Dark Matter in the X-COP Galaxy Clusters Sample
• The SRG/eROSITA All-Sky Survey : Subaru/HSC-SSP weak-lensing mass measurements for the eRASS1 Galaxy Clusters
• Dark Matter in Fractional Gravity I: Astrophysical Tests on Galactic Scales
• Searching for Dark Matter Sub-structure with HAWC
• The impact of turbulent mixing on the galactic r-process enrichment by binary neutron star mergers
• Over-density of SMGs in fields containing z~0.3 galaxies: magnification bias and the implications for studies of galaxy evolution
• Decaying axinolike dark matter: Discriminative solution to small-scale issues
• Supermassive black hole seeds from sub-keV dark matter
• Exploring Self-Interacting Dark Matter Halos with Diverse Baryonic Distributions: A Parametric Approach
• Simulations of galaxy cluster mergers with velocity-dependent, rare and frequent self-interactions
• Subhalo effective density slope measurements from HST strong lensing data with neural likelihood-ratio estimation
• The hot gas mass fraction in halos. From Milky Way-like groups to massive clusters
• The impact of assembly history on the X-ray detectability of halos. From galaxy groups to galaxy clusters
• Testing multiflavored ULDM models with SPARC
• Constraints on precipitation-limited hot halos from massive galaxies to galaxy clusters
• Non-steady heating of cool cores of galaxy clusters by ubiquitous turbulence and AGN
• Angular momentum evolution of bulge stars in disc galaxies in NIHAO
• The spatial distribution of globular clusters in dwarf spheroidal galaxies and the timing problem
• The BAHAMAS project: Evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum
• Searching for dark matter annihilation from individual halos: uncertainties, scatter and signal-to-noise ratios
• Jointly fitting weak lensing, X-ray and Sunyaev-Zel'dovich data to constrain scalar-tensor theories with clusters of galaxies
• EDGE: the puzzling ellipticity of Eridanus II's star cluster and its implications for dark matter at the heart of an ultra-faint dwarf
• Average X-ray properties of galaxy groups. From Milky Way-like halos to massive clusters
• Neutrino winds on the sky
• Photometric vs dynamical stellar masses and their impact on scaling relations in nearby disc galaxies
• $i(cm)z$, a semi-analytic model for the thermodynamic properties in galaxy clusters: calibrations with mass and redshift, and implication for the hydrostatic bias
• A deeper look into the structure of ΛCDM haloes: correlations between halo parameters from Einasto fits
• Dynamic equilibrium sets atomic content of galaxies across cosmic time
• Primordial Black Hole-Neutron Star Merger Rate in Modified Gravity
• The Ultramarine Simulation: properties of dark matter haloes before redshift 5.5
• Dark matter indirect signals with long-lived mediators
• Dark Matter Annihilation in the Circumgalactic Medium at High Redshifts
• Cluster-lensing: A Python Package for Galaxy Clusters & Miscentering
• Quantifying and controlling biases in dark matter halo concentration estimates
• Rotation curves of galaxies and the stellar mass-to-light ratio
• Pushing the Limits of Detectability: Mixed Dark Matter from Strong Gravitational Lenses
• Beyond Ultra-diffuse Galaxies. II. Environmental Quenching of Mass-Size Outliers among the Satellites of Milky Way Analogs
• Voronoi Tessellation and Non-parametric Halo Concentration
• Inferring subhalo effective density slopes from strong lensing observations with neural likelihood-ratio estimation
• Dark matter halos and the M-σrelation for supermassive black holes
• Gravitational Lensing of Spherically Symmetric Black Holes in Dark Matter Halos
• The GMRT archive atomic gas survey -- II. Mass modelling and dark matter halo properties across late-type spirals
• Disk galaxies are self-similar: the universality of the HI-to-Halo mass ratio for isolated disks
• Thermalization, Fragmentation and Tidal Disruption: The Complex Galactic Dynamics of Dark Matter Superfluidity
• The Entire Virial Radius of the Fossil Cluster RXJ1159+5531: II. Dark Matter and Baryon Fraction
• Quasi-stellar objects and galaxy mass density profiles derived using the submillimetre galaxies magnification bias
• Type Ia Supernova Magnitude Step from the local Dark Matter Environment
• Constraining dark matter annihilation with HSC Low Surface Brightness Galaxies
• The impact of the halo spin-concentration relation on disc scaling laws
• Detecting Low-Mass Perturbers in Cluster Lenses using Curved Arc Bases
• Classification of gamma-ray targets for velocity-dependent and subhalo-boosted dark-matter annihilation
• A Hyperactive FRB Pinpointed in an SMC-Like Satellite Host Galaxy
• Cross-Correlation Forecast of CSST Spectroscopic Galaxy and MeerKAT Neutral Hydrogen Intensity Mapping Surveys
• The Dark Matter Halos of HI Selected Galaxies
• Joint Strong and Weak Lensing Analysis of the Massive Cluster Field J0850+3604
• Physical modelling of galaxy clusters using Einasto dark matter profiles
• The ALMA-CRISTAL survey: Extended [CII] emission in an interacting galaxy system at z ~ 5.5
• NIHAO XXVIII: Collateral effects of AGN on dark matter concentration and stellar kinematics
• Diverse dark matter profiles in FIRE dwarfs: black holes, cosmic rays and the cusp-core enigma
• Abundance matching tested on small scales with galaxy dynamics
• Andromeda XXV -- a dwarf galaxy with a low central dark matter density
• No globular cluster progenitors in Milky Way satellite galaxies
• The extended Planetary Nebula Spectrograph (ePN.S) early-type galaxy survey: The specific angular momentum of ETGs
• NGC 4104: a shell galaxy in a forming fossil group
• MaNGA DynPop -- VI. Matter density slopes from dynamical models of 6000 galaxies versus cosmological simulations: the interplay between baryonic and dark matter
• Galaxy cluster mass density profile derived using the submillimetre galaxies magnification bias
• Investigating the Dark Matter Halo of NGC 5128 using a Discrete Dynamical Model
• Simulated [CII] in high-z galaxies
• Self-Interacting Dark Matter Scattering Rates Through Cosmic Time
• LEGA-C: analysis of dynamical masses from ionized gas and stellar kinematics at z~0.8
• Numerical convergence of pre-initial conditions on dark matter halo properties
• Studying galaxy cluster morphological metrics with Mock-X
• Gravitational Lensing in More Realistic Dark Matter Halo Models
• Measuring the mass and concentration of dark matter halos from the velocity dispersion profile of their stars
• 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
• Probing sub-eV Dark Matter decays with PTOLEMY
• From "universal" profiles to "universal" scaling laws in X-ray galaxy clusters
• Compact Binary Merger Rate with Modified Gravity in Dark-Matter Spikes
• Can tides explain the low dark matter density in Fornax?
• Analyzing Planar Galactic Halo Distributions with Fuzzy/Cold Dark Matter Models
• NGC 7457: Evidence for merger-driven cylindrical rotation in disc galaxies
• Decomposing galaxies with BANG: an automated morpho-kinematical decomposition of the SDSS-DR17 MaNGA survey
• Mass Modeling the Andromeda Dwarf Galaxies: Andromeda VI and Andromeda XXIII
• The shape of dark matter haloes: results from weak lensing in the Ultraviolet Near-Infrared Optical Northern Survey (UNIONS)
• CHEX-MATE: exploring the kinematical properties of Planck galaxy clusters
• Type I shell galaxies as a test of gravity models
• The information on halo properties contained in spectroscopic observations of late-type galaxies
• Relaxing Constraints on Dark Matter Annihilation Near the Supermassive Black Hole in M87
• No need for dark matter: resolved kinematics of the ultra-diffuse galaxy AGC 114905
• An Accurate P${}^3$M Algorithm for Gravitational Lensing Studies in Simulations
• On the scattering of a high-energy cosmic ray electrons off the dark matter
• HI 21 cm observation and mass models of the extremely thin galaxy FGC 1440
• AMICO galaxy clusters in KiDS-1000: cosmological constraints and mass calibration from counts and weak lensing
• Total and dark mass from observations of galaxy centers with Machine Learning
• The dark side of early galaxies: $\text{geko}$ uncovers dark-matter fractions at $z\sim 4-6$
• Constraining cosmology with the velocity function of low-mass galaxies
• Why does Einasto profile index $n\sim 6$ occur so frequently?
• Outer and inner mass distributions of the irregular galaxies UGC 4284 and UGC 11861: Constraining the baryonic content through stellar population synthesis studies
• The Double Galaxy Cluster Abell 2465 III. X-ray and Weak-lensing Observations
• Measurement of Substructure from the Kinematics of the GD-1 Stellar Stream
• Halo Concentrations and the Fundamental Plane of Galaxy Clusters
• Science Potential for Stellar-mass Black Holes as Neighbors of Sgr A*
• The SLACS strong lens sample, debiased. II. Lensing-only constraints on the stellar IMF and dark matter contraction in early-type galaxies
• CHEX-MATE: Multi-probe analysis of Abell 1689
• An H$\alpha$ kinematic survey of the $Herschel$ Reference Survey -- I. Fabry-Perot observations with the 1.93m telescope at OHP
• Mass content of UGC 6446 and UGC 7524 through HI rotation curves: deriving the stellar discs from stellar population synthesis models
• Quenching vs. Quiescence: forming realistic massive ellipticals with a simple starvation model
• Assessing the dark matter content of two quasar host galaxies at z~6 through gas kinematics
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Warm dark matter model with a few keV mass is bad for the too-big-to-fail problem
• Statistics for dark matter subhalo searches in gamma rays from a kinematically constrained population model: Fermi-LAT-like telescopes
• Late-Time Dark Matter Oscillations and the Core-Cusp Problem
• Structural and dynamical modeling of WINGS clusters. III. The pseudo phase-space density profile
• Star formation drivers across the M33 disk
• Signatures of Fuzzy Dark Matter Inside Radial Critical Curves
• Shadows and Observational Images of a Schwarzschild-like Black Hole Surrounded by a Dehnen-type Dark Matter Halo
• The unusually high dark matter concentration of the galaxy group NGC 1600
• QSO MUSEUM III: the circumgalactic medium in Ly$\alpha$ emission around 120 $z\sim 3$ quasars covering the SDSS parameter space. Witnessing the instantaneous AGN feedback on halo scales
• Hermeian haloes: extreme objects with two interactions in the past
• Dark matter halo concentrations: a short review
• The imprint of dark subhaloes on the circumgalactic medium
• Dark matter inner slope and concentration in galaxies: from the Fornax dwarf to M87
• 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
• The impact of halo concentration on the Sunyaev Zel'dovich effect signal from massive galaxy clusters
• Refracting into Ultra Diffuse Galaxy NGC 1052-DF2 by Passing near the Center of NGC 1052
• Relic neutrino clustering in the Milky Way
• From particles to orbits: precise dark matter density profiles using dynamical information
• Hidden Figures in the Sky: Evolution of low-surface brightness galaxies from a hydro-dynamical perspective
• Structure and kinematics of the interacting group NGC 5098/5096
• MaNGA DynPop. VII. A Unified Bulge-Disk-Halo Model for Explaining Diversity in Circular Velocity Curves of 6000 Spiral and Early-Type Galaxies
• The "Little Dark Dot": Evidence for Self-interacting Dark Matter in the Strong Lens SDSS J0946+1006?
• Bayesian WIMP detection with the Cherenkov Telescope Array
• Amaryllis: a digital twin of the earliest galaxies in the Universe
• Searching for Dark Matter Annihilation with IceCube and P-ONE
• The uncommon intracluster medium features of the first massive clusters selected independently of their baryon content
• Toward Gravitational Lensing in Modified Theories of Gravity
• Gas dynamics in an AGN-host galaxy at $z\simeq 2.6$: regular rotation, non-circular motions, and mass models
• Modelling the photometric and morphological evolution of disc galaxies in the cluster environment
• The AIDA-TNG project: dark matter profiles and concentrations in alternative dark matter models
• HI-bearing dark galaxies predictions from constrained Local Group simulations: how many and where to find them
• 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
• Extreme Galaxy-scale Outflows Are Frequent among Luminous Early Quasars
• JWST Discovery of Strong Lensing from a Galaxy Cluster at Cosmic Noon: Giant Arcs and a Highly Concentrated Core of XLSSC 122
• The dynamical evolution of the stellar clumps in the Sparkler galaxy
• Exploring Milky Way rotation curves with Gaia DR3: a comparison between $\Lambda$CDM, MOND, and General Relativistic approaches
• Metamorphosis of dwarf halo density profile under dark matter decays
• Simultaneous emergence of curved spacetime and quantum mechanics
• Two analytic relations connecting the hot gas astrophysics with the cold dark matter model for galaxy clusters
• Analytical insight into dark matter subhalo boost factors for Sommerfeld-enhanced $s$- and $p$-wave $\gamma$-ray signals
• The spherical Fast Multipole Method (sFMM) for Gravitational Lensing Simulation
• Dark and visible matter distribution in Coma cluster: theory vs observations
• Magnetising galaxies with cold inflows
• Weak lensing of bright standard sirens: prospects for ${\sigma }_8$
• Dark matter haloes in the multicomponent model. III. From dwarfs to galaxy clusters
• Self-Interacting Dark Matter with Mass Segregation: A Unified Explanation of Dwarf Cores and Small-Scale Lenses
• Extended Hernquist-Springel formalism for cosmic star formation
• An Enhanced Isothermal Jeans Approach to Constraining Dark Matter Self-Interactions from Galactic Kinematics
• Gas thermodynamics meets galaxy kinematics: Joint mass measurements for eROSITA galaxy clusters
• Renzo's rule revisited: A statistical study of galaxies' baryon - dark matter coupling
• Unequal-mass mergers of dark matter haloes with rare and frequent self-interactions
• MUSE-DARK-II: 3D morpho-kinematic modelling of lensed galaxies. Tully-Fisher relation of $z\sim 1$ star-forming galaxies
• Observed versus Simulated Halo c-Mvir Relations
• A Relativistic Tensorial Model for Fractional Interaction between Dark Matter and Gravity
• On the origin of Sérsic profiles of galaxies and Einasto profiles of dark-matter halos
• AMiBA: Cluster Sunyaev-Zel'dovich Effect Observations with the Expanded 13-Element Array
• Dark matter in ALFALFA galaxies: Investigating galaxy-halo connection
• Cosmic magnification on high-redshift submillimeter galaxies
• Timing Mass of the Local Group
• Dissecting the Strong-lensing Galaxy Cluster MS 0440.5+0204. I. The Mass Density Profile
• Chemodynamics of BoötesI with $S^5$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints
• The stellar orbit distribution in present-day galaxies inferred from the CALIFA survey
• Cored Dark Matter halos in the Cosmic Neutrino Background
• Rotation Curves in z~1-2 Star-Forming Disks: Comparison of Dark Matter Fractions and Disk Properties for Different Fitting Methods
• Massive Star Clusters in the Semi-Analytical Galaxy Formation Model L-Galaxies 2020
• A Salpeter IMF and an NFW halo: Disentangling the dark and stellar mass of an elliptical galaxy through precise lens modelling of a double-source-plane system
• Controlled Experiments on Dark-Matter Halo Structure and Galaxy Morphology I: What Sets Galaxy Sizes?
• Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues
• Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos
• Milky-Way-like stars in a galaxy core 8 billion years ago revealed by gravitational lensing
• The odd primordial halo of the Milky Way implied by Gaia. A shallow core, but a steep decline
• The vertical structure of the stellar disk in NGC 551
• A bar stability criterion distinguishing between modified gravity and dark matter in galaxies
• Reconciling concentration to virial mass relations
• Broken Expectations: The Effects of Modelling Assumptions on the Inferred Dark Matter Distribution in the Milky Way's Satellites
• A self-consistent wave description of axion miniclusters and their survival in the galaxy
• Towards a universal model for the density profiles of dark matter haloes
• Galaxy rotation curves in the light of the Spinor Theory of Gravity
• Probing Dark Matter with Strong Gravitational Lensing through an Effective Density Slope
• DHOST gravity in Ultra-diffuse galaxies -- Part I: the case of NGC1052-DF2
• SDSS-IV MaNGA: A Catalogue of Spectroscopically Detected Strong Galaxy-Galaxy Lens Candidates
• Cross-checking SMBH mass estimates in NGC 6958 -- I: Stellar dynamics from adaptive optics-assisted MUSE observations
• Cosmic Reionization On Computers: Baryonic Effects on Halo Concentrations During the Epoch of Reionization
• Properties of the Intracluster Medium Assuming an Einasto Dark Matter Profile
• Accretion of self-interacting dark matter onto supermassive black holes
• Spherically Symmetric Potentials in Quadratic $f(R)$ Gravity
• Euclid: Early Release Observations. Weak gravitational lensing analysis of Abell 2390
• Tensorial solution of the Poisson equation and the dark matter amount and distribution of UGC 8490 and UGC 9753
• Extragalactic Searches for Dark Matter Annihilation
• A general framework for unbiased tests of gravity using galaxy clusters
• A Pearl in the Shell: an ultra-compact dwarf within the tidal debris surrounding spiral galaxy NGC 7531
• Fuzzy dark matter dynamical friction: stalling of globular clusters induced by dynamical heatings
• The Non-universal Pseudo Phase-Space Density Profiles of Symphony Host Halos
• Prediction of Individual Halo Concentrations Across Cosmic Time Using Neural Networks
• Heavy dark matter in rapidly evolving massive stars
• Initial Investigations of the Outskirts of XLSSC 122
• Constraining the population of dark matter halo shapes using hierarchical inference with extragalactic stellar streams