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Cosmological simulations with self-interacting dark matter – I. Constant-density cores and substructure
111/111 checkable references clean · checked 2026-07-25
Every reference with a DOI in the deposited reference list resolved to a known work in Crossref or DataCite at the dated check, and none carried a retraction, withdrawal, or removal notice.
11 without a DOI — not checked. A reference deposited without a DOI is never matched by title or guessed at; it stays outside the checked set, and this line discloses that.
The 111 checked references that resolve
resolves10.1111/j.1365-2966.2005.09492.x
Formation and evolution of self-interacting dark matter haloes
resolves10.1111/j.1365-2966.2011.19684.x
Dark matter cores and cusps: the case of multiple stellar populations in dwarf spheroidals
resolves10.1086/340296
<i>Chandra</i>Observations of the Lensing Cluster EMSS 1358+6245: Implications for Self‐interacting Dark Matter
resolves10.1086/367794
Early-Type Galaxies in the Sloan Digital Sky Survey. III. The Fundamental Plane
resolves10.1111/j.1745-3933.2011.01074.x
Too big to fail? The puzzling darkness of massive Milky Way subhaloes
resolves10.1111/j.1365-2966.2012.20695.x
The Milky Way’s bright satellites as an apparent failure of ΛCDM
resolves10.1111/j.1365-2966.2011.19740.x
Hierarchical formation of bulgeless galaxies - II. Redistribution of angular momentum via galactic fountains
resolves10.1088/0004-637X/757/1/22
CLASH: PRECISE NEW CONSTRAINTS ON THE MASS PROFILE OF THE GALAXY CLUSTER A2261
resolves10.1086/344259
Structure and Subhalo Population of Halos in a Self‐interacting Dark Matter Cosmology
resolves10.1088/0004-637X/760/1/71
THE STELLAR INITIAL MASS FUNCTION IN EARLY-TYPE GALAXIES FROM ABSORPTION LINE SPECTROSCOPY. II. RESULTS
resolves10.1051/0004-6361:20010398
A wide-field spectroscopic survey of the cluster of galaxies Cl0024+1654
resolves10.1051/0004-6361:20020230
A wide-field spectroscopic survey of the cluster of galaxies Cl0024+1654
resolves10.1086/318417
Halo Properties in Cosmological Simulations of Self‐interacting Cold Dark Matter
resolves10.1086/367606
The Failure of Self‐Interacting Dark Matter to Solve the Overabundance of Dark Satellites and the Soft Core Question
resolves10.1146/annurev-astro-082708-101659
Dark Matter Candidates from Particle Physics and Methods of Detection
resolves10.1103/PhysRevLett.104.151301
Halo-Shape and Relic-Density Exclusions of Sommerfeld-Enhanced Dark Matter Explanations of Cosmic Ray Excesses
resolves10.1111/j.1365-2966.2012.21623.x
The dark matter haloes of dwarf galaxies: a challenge for the Λ cold dark matter paradigm?
resolves10.1046/j.1365-8711.2000.03555.x
Evidence of self-interacting cold dark matter from galactic to galaxy cluster scales
resolves10.1038/nature08640
Bulgeless dwarf galaxies and dark matter cores from supernova-driven outflows
resolves10.1111/j.1365-2966.2012.20696.x
Cuspy no more: how outflows affect the central dark matter and baryon distribution in Λ cold dark matter galaxies
resolves10.1103/PhysRevD.38.2357
Cross sections, relic abundance, and detection rates for neutralino dark matter
resolves10.1088/0004-637X/717/1/420
TRACING THE PECULIAR DARK MATTER STRUCTURE IN THE GALAXY CLUSTER Cl 0024+17 WITH INTRACLUSTER STARS AND GAS
resolves10.1086/517498
Discovery of a Ringlike Dark Matter Structure in the Core of the Galaxy Cluster Cl 0024+17
resolves10.1086/172935
Hierarchical galaxy formation - Overmerging and the formation of an X-ray cluster
resolves10.1086/317074
The Fundamental Plane of Gravitational Lens Galaxies and The Evolution of Early‐Type Galaxies in Low‐Density Environments
resolves10.1111/j.1365-2966.2011.18684.x
Gravothermal collapse of isolated self-interacting dark matter haloes: N-body simulation versus the fluid model
resolves10.1088/0067-0049/192/2/18
SEVEN-YEAR<i>WILKINSON MICROWAVE ANISOTROPY PROBE</i>(<i>WMAP</i>) OBSERVATIONS: COSMOLOGICAL INTERPRETATION
resolves10.1086/527543
Mass Models for Low Surface Brightness Galaxies with High‐Resolution Optical Velocity Fields
resolves10.1088/2041-8205/710/2/L161
THE CASE AGAINST WARM OR SELF-INTERACTING DARK MATTER AS EXPLANATIONS FOR CORES IN LOW SURFACE BRIGHTNESS GALAXIES
resolves10.1111/j.1365-2966.2010.17273.x
SPIDER - III. Environmental dependence of the Fundamental Plane of early-type galaxies
resolves10.1103/PhysRevLett.106.171302
Cores in Dwarf Galaxies from Dark Matter with a Yukawa Potential
resolves10.1088/0004-637X/738/1/55
A COMPLETE SPECTROSCOPIC SURVEY OF THE MILKY WAY SATELLITE SEGUE 1: DARK MATTER CONTENT, STELLAR MEMBERSHIP, AND BINARY PROPERTIES FROM A BAYESIAN ANALYSIS
resolves10.1111/j.1365-2966.2007.12225.x
The effects of ellipticity and substructure on estimates of cluster density profiles based on lensing and kinematics
resolves10.1111/j.1365-2966.2012.20537.x
Triaxiality, principal axis orientation and non-thermal pressure in Abell 383
resolves10.1088/0004-637X/713/1/491
UNVEILING THE THREE-DIMENSIONAL STRUCTURE OF GALAXY CLUSTERS: RESOLVING THE DISCREPANCY BETWEEN X-RAY AND LENSING MASSES
resolves10.1088/0004-637X/729/1/37
RECONSTRUCTING THE TRIAXIALITY OF THE GALAXY CLUSTER A1689: SOLVING THE X-RAY AND STRONG LENSING MASS DISCREPANCY
resolves10.1088/0004-637X/706/2/1078
THE DISTRIBUTION OF DARK MATTER OVER THREE DECADES IN RADIUS IN THE LENSING CLUSTER ABELL 611
resolves10.1088/2041-8205/728/2/L39
THE DARK MATTER DISTRIBUTION IN A383: EVIDENCE FOR A SHALLOW DENSITY CUSP FROM IMPROVED LENSING, STELLAR KINEMATIC, AND X-RAY DATA
resolves10.1088/0004-6256/142/1/24
THE CENTRAL SLOPE OF DARK MATTER CORES IN DWARF GALAXIES: SIMULATIONS VERSUS THINGS
resolves10.1016/j.newast.2003.12.004
Stellar and dynamical masses of ellipticals in the Sloan Digital Sky Survey
resolves10.1088/2041-8205/759/2/L42
THE COUPLING BETWEEN THE CORE/CUSP AND MISSING SATELLITE PROBLEMS
resolves10.1046/j.1365-8711.2003.05925.x
The inner structure of CDM haloes -- I. A numerical convergence study
resolves10.1086/587859
Constraints on the Self‐Interaction Cross Section of Dark Matter from Numerical Simulations of the Merging Galaxy Cluster 1E 0657−56
resolves10.1111/j.1365-2966.2004.07775.x
A dynamical model for the distribution of dark matter and gas in galaxy clusters
resolves10.1111/j.1365-2966.2012.21432.x
Infall times for Milky Way satellites from their present-day kinematics
resolves10.1088/0004-637X/690/1/154
THE CLUSTER LENS ACO 1703: REDSHIFT CONTRAST AND THE INNER PROFILE
resolves10.1111/j.1365-2966.2011.20144.x
Dwarf spheroidal galaxy kinematics and spiral galaxy scaling laws
resolves10.1086/432593
The Dark Halo of NGC 5963 as a Constraint on Dark Matter Self‐Interaction at the Low‐Velocity Regime
resolves10.1086/382146
The Dark Matter Distribution in the Central Regions of Galaxy Clusters: Implications for Cold Dark Matter
resolves10.1086/524652
Separating Baryons and Dark Matter in Cluster Cores: A Full Two‐dimensional Lensing and Dynamic Analysis of Abell 383 and MS 2137−23
resolves10.1086/427684
High‐Resolution Measurements of the Halos of Four Dark Matter–Dominated Galaxies: Deviations from a Universal Density Profile
resolves10.1088/0004-637X/733/1/46
A COMPLETE SPECTROSCOPIC SURVEY OF THE MILKY WAY SATELLITE SEGUE 1: THE DARKEST GALAXY
resolves10.1016/0550-3213(85)90537-1
Cosmological constraints on the properties of weakly interacting massive particles
resolves10.1086/592102
Hundreds of Milky Way Satellites? Luminosity Bias in the Satellite Luminosity Function
resolves10.1088/0004-637X/726/2/108
FROM GALAXY CLUSTERS TO ULTRA-FAINT DWARF SPHEROIDALS: A FUNDAMENTAL CURVE CONNECTING DISPERSION-SUPPORTED GALAXIES TO THEIR DARK MATTER HALOS
resolves10.1088/0004-637X/742/1/16
GALAXIES IN ΛCDM WITH HALO ABUNDANCE MATCHING: LUMINOSITY-VELOCITY RELATION, BARYONIC MASS-VELOCITY RELATION, VELOCITY FUNCTION, AND CLUSTERING
resolves10.1088/0004-637X/714/2/1470
THE MASS STRUCTURE OF THE GALAXY CLUSTER Cl0024+1654 FROM A FULL LENSING ANALYSIS OF JOINT SUBARU AND ACS/NIC3 OBSERVATIONS
resolves10.1088/0004-637X/755/1/56
CLASH: MASS DISTRIBUTION IN AND AROUND MACS J1206.2-0847 FROM A FULL CLUSTER LENSING ANALYSIS
resolves10.1088/0004-637X/742/1/20
A METHOD FOR MEASURING (SLOPES OF) THE MASS PROFILES OF DWARF SPHEROIDAL GALAXIES
resolves10.1088/0004-637X/742/2/117
THE CLUSTER LENSING AND SUPERNOVA SURVEY WITH<i>HUBBLE</i>(CLASH): STRONG-LENSING ANALYSIS OF A383 FROM 16-BAND<i>HST</i>/WFC3/ACS IMAGING
resolves10.1088/0004-637X/761/1/71
BARYONS MATTER: WHY LUMINOUS SATELLITE GALAXIES HAVE REDUCED CENTRAL MASSES
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