Toward a halo mass function for precision cosmology: the limits of universality

Abstract

We measure the mass function of dark matter halos in a large set of collisionless cosmological simulations of flat LCDM cosmology and investigate its evolution at z<~2. Halos are identified as isolated density peaks, and their masses are measured within a series of radii enclosing specific overdensities. We argue that these spherical overdensity masses are more directly linked to cluster observables than masses measured using the friends-of-friends algorithm (FOF), and are therefore preferable for accurate forecasts of halo abundances. Our simulation set allows us to calibrate the mass function at z=0 for virial masses in the range 10^{11} Msol/h < M < 10^{15} Msol/h, to <~ 5%. We derive fitting functions for the halo mass function in this mass range for a wide range of overdensities, both at z=0 and earlier epochs. In addition to these formulae, which improve on previous approximations by 10-20%, our main finding is that the mass function cannot be represented by a universal fitting function at this level of accuracy. The amplitude of the "universal" function decreases monotonically by ~20-50%, depending on the mass definition, from z=0 to 2.5. We also find evidence for redshift evolution in the overall shape of the mass function.

19 emulateapj pages, 15 figures, submitted to Apj

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• The cosmological analysis of X-ray cluster surveys: II- Application of the CR-HR method to the XMM archive
• First Sunyaev-Zel'dovich mapping with the NIKA2 camera: Implication of cluster substructures for the pressure profile and mass estimate
• Properties of the stochastic astrophysical gravitational wave background: astrophysical sources dependencies
• Tomographic galaxy clustering with the Subaru Hyper Suprime-Cam first year public data release
• Halo model and halo properties in Galileon gravity cosmologies
• High-energy gamma-ray and neutrino backgrounds from clusters of galaxies and radio constraints
• The Non-Gaussian Halo Mass Function with fNL, gNL and tauNL
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: mock galaxy catalogues for the low-redshift sample
• Carbon Monoxide Intensity Mapping at Moderate Redshifts
• SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV
• The cosmology dependence of weak lensing cluster counts
• An Intensity Mapping Detection of Aggregate CO Line Emission at 3 mm
• From Galaxy Clusters to Ultra-Faint Dwarf Spheroidals: A Fundamental Curve Connecting Dispersion-supported Galaxies to Their Dark Matter Halos
• HALOGEN: A tool for fast generation of mock halo catalogues
• The halo model for cosmology: a pedagogical review
• Verifying the consistency relation for the scale-dependent bias from local primordial non-Gaussianity
• Cosmological limits on neutrino unknowns versus low redshift priors
• PRIMUS: Galaxy Clustering as a Function of Luminosity and Color at 0.2<z<1
• Cosmology with the Large Synoptic Survey Telescope: an Overview
• The velocity function of gas-rich galaxies
• Arc Statistics
• Chameleon Halo Modeling in f(R) Gravity
• Gravitational wave lensing as a probe of halo properties and dark matter
• HICOSMO - Cosmology with a complete sample of galaxy clusters: I. Data analysis, sample selection and luminosity-mass scaling-relation
• The Observed Growth of Massive Galaxy Clusters III: Testing General Relativity on Cosmological Scales
• Statistics of Dark Matter Substructure: III. Halo-to-Halo Variance
• SPT-CL J0205-5829: A z = 1.32 Evolved Massive Galaxy Cluster in the South Pole Telescope Sunyaev-Zel'dovich Effect Survey
• Dark-Matter Decays and Self-Gravitating Halos
• On the Self-Similar Appearance of Galaxy Clusters in X-rays
• Three-Point Correlation Functions of SDSS Galaxies: Constraining Galaxy-Mass Bias
• Halo bias in Lagrangian Space: Estimators and theoretical predictions
• The Argo Simulation: II. The Early Build-up of the Hubble Sequence
• A measurement of the secondary-CMB and millimeter-wave-foreground bispectrum using 800 square degrees of South Pole Telescope data
• Galaxy bias and primordial non-Gaussianity: insights from galaxy formation simulations with IllustrisTNG
• Spherical collapse in $\nu \Lambda CDM$
• How many radio relics await discovery?
• IDCS J1426.5+3508: Sunyaev-Zel'dovich Measurement of a Massive IR-selected Cluster at z=1.75
• Machine learning cosmological structure formation
• Tomographic measurement of the intergalactic gas pressure through galaxy-tSZ cross-correlations
• Combining clustering and abundances of galaxy clusters to test cosmology and primordial non-Gaussianity
• Universal at last? The splashback mass function of dark matter halos
• On Combining Galaxy Clustering and Weak Lensing to Unveil Galaxy Biasing via the Halo Model
• CLUMPY v3: $\gamma$-ray and $\nu$ signals from dark matter at all scales
• Cosmological constraints from thermal Sunyaev Zeldovich power spectrum revisited
• Rhapsody. I. Structural Properties and Formation History From a Statistical Sample of Re-simulated Cluster-size Halos
• A comparison of structure formation in minimally and non-minimally coupled quintessence models
• Search for CII Emission on Cosmological Scales at Redshift Z~2.6
• Dissecting the high-z interstellar medium through intensity mapping cross-correlations
• Genetically modified halos: towards controlled experiments in $\Lambda$CDM galaxy formation
• Designing an Inflation Galaxy Survey: how to measure $\sigma (f_{\mathrm{NL}})\sim 1$ using scale-dependent galaxy bias
• Modelling Void Abundance in Modified Gravity
• The Large-Scale 3-point correlation function of SDSS Luminous Red Galaxies
• Statistics of extreme objects in the Juropa Hubble Volume simulation
• Galaxy-Galaxy Lensing in the DES Science Verification Data
• Evidence for the inside-out growth of the stellar mass distribution in galaxy clusters since z~1
• The biasing of baryons on the cluster mass function and cosmological parameter estimation
• Optimal capture of non-Gaussianity in weak lensing surveys: power spectrum, bispectrum and halo counts
• Mapping the Real Space Distributions of Galaxies in SDSS DR7: II. Measuring the growth rate, clustering amplitude of matter and biases of galaxies at redshift $0.1$
• Distant galaxy clusters in the XMM Large Scale Structure survey
• Precision cosmology with a wide area XMM cluster survey
• A large sample of shear selected clusters from the Hyper Suprime-Cam Subaru Strategic Program S16A wide field mass maps
• How does our choice of observable influence our estimation of the centre of a galaxy cluster? Insights from cosmological simulations
• Fundamental Physics from Future Weak-Lensing Calibrated Sunyaev-Zel'dovich Galaxy Cluster Counts
• Accurate and Efficient Halo-based Galaxy Clustering Modelling with Simulations
• Banana Split: Testing the Dark Energy Consistency with Geometry and Growth
• The Extreme Small Scales: Do Satellite Galaxies Trace Dark Matter?
• CLASS_GWB: robust modeling of the astrophysical gravitational wave background anisotropies
• The potential of X-ray cluster surveys to constrain primordial non-Gaussianity
• Calibrating the Planck Cluster Mass Scale with CLASH
• Imprints of relativistic effects on the asymmetry of the halo cross-correlation function: from linear to non-linear scales
• Toward a Universal Formulation of the Halo Mass Function
• Galaxy Cluster Scaling Relations between Bolocam Sunyaev-Zel'dovich Effect and Chandra X-ray Measurements
• On the shape of dark matter halos from MultiDark Planck simulations
• Dynamical evidence for a morphology-dependent relation between the stellar and halo masses of galaxies
• The Cosmic Thermal History Probed by Sunyaev-Zeldovich Effect Tomography
• The Atacama Cosmology Telescope: Physical Properties of Sunyaev-Zel'dovich Effect Clusters on the Celestial Equator
• Cosmic variance of the galaxy cluster weak lensing signal
• Constraining galaxy cluster temperatures and redshifts with eROSITA survey data
• Implications of multiple high-redshift galaxy clusters
• Toward an accurate mass function for precision cosmology
• HICOSMO - Cosmology with a complete sample of galaxy clusters: II. Cosmological results
• The Growth of Brightest Cluster Galaxies and Intracluster Light Over the Past Ten Billion Years
• Separate Universe Consistency Relation and Calibration of Halo Bias
• Resolving Small-Scale Dark Matter Structures Using Multi-Source Indirect Detection
• The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray Properties and Scaling Relations of Galaxy Clusters and Groups
• Cosmic voids in modified gravity scenarios
• Orientation Bias of Optically Selected Galaxy Clusters and Its Impact on Stacked Weak Lensing Analyses
• Constraining the Star Formation Histories in Dark Matter Halos: I. Central Galaxies
• Ultraviolet Luminosity Density of the Universe During the Epoch of Reionization
• The extended Northern ROSAT Galaxy Cluster Survey (NORAS II) I. Survey Construction and First Results
• Cluster abundance in chameleon $f(R)$ gravity I: toward an accurate halo mass function prediction
• The contributions of matter inside and outside of haloes to the matter power spectrum
• Linear response to long wavelength fluctuations using curvature simulations
• Luminosity Functions and Host-to-Host Scatter of Dwarf Satellite Systems in the Local Volume
• Quenching low-mass satellite galaxies: evidence for a threshold ICM density
• Mass bias evolution in tSZ cluster cosmology
• Mock galaxy shape catalogs in the Subaru Hyper Suprime-Cam Survey
• Cosmology with galaxy-galaxy lensing on non-perturbative scales: Emulation method and application to BOSS LOWZ
• The Galaxy-Halo/Subhalo connection: Mass relations and implications for some satellite occupational distributions
• On the origin of excess cool gas in quasar host halos
• Conservative Constraints on Dark Matter from the Fermi-LAT Isotropic Diffuse Gamma-Ray Background Spectrum
• Mock catalogs for the extragalactic X-ray sky: simulating AGN surveys with Athena and with the AXIS probe
• Forecasts on Primordial non-Gaussianity from 21 cm Intensity Mapping experiments
• A Self-Calibrating Halo-Based Group Finder: Application to SDSS
• Large-Scale Structure Formation: from the first non-linear objects to massive galaxy clusters
• Forecasts on dark energy from the X-ray cluster survey with eROSITA: constraints from counts and clustering
• Reconstructing the distribution of haloes and mock galaxies below the resolution limit in cosmological simulations
• The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to $z\sim 5$
• On the origin of gas-poor galaxies in galaxy clusters using cosmological hydrodynamic simulations
• Galaxy Formation as a Cosmological Tool. I: The Galaxy Merger History as a Measure of Cosmological Parameters
• Accurate mass and velocity functions of dark matter halos
• The Main Sequences of Starforming Galaxies and Active Galactic Nuclei at High Redshift
• The Quest for Dusty Star-forming Galaxies at High Redshift z>4
• Weak-Lensing Mass Calibration of the Atacama Cosmology Telescope Equatorial Sunyaev-Zeldovich Cluster Sample with the Canada-France-Hawaii Telescope Stripe 82 Survey
• Predictions for local PNG bias in the galaxy power spectrum and bispectrum and the consequences for $f_{\mathrm{NL}}$ constraints
• Detecting clusters of galaxies and active galactic nuclei in an eROSITA all-sky survey digital twin
• TheHaloMod: An online calculator for the halo model
• Caught in the cosmic web: Environmental effect on halo concentrations, shape, and spin
• Cosmological Constraint on ${\Omega }_m$ and ${\sigma }_8$ from Cluster Abundances using the $GalWCat19$ Optical-Spectroscopic SDSS Catalog
• Evidence of pre-processing and a dependence on dynamical state for low-mass satellite galaxies
• A Self-consistent Framework for Multiline Modeling in Line Intensity Mapping Experiments
• Properties of Dark Matter Haloes and their Correlations: the Lesson from Principal Component Analysis
• The XMM-LSS survey: the Class 1 cluster sample over the extended 11 deg${}^2$ and its spatial distribution
• Bispectrum of the Sunyaev-Zel'dovich Effect
• 2HOT: An Improved Parallel Hashed Oct-Tree N-Body Algorithm for Cosmological Simulation
• Interpreting the Clustering of Distant Red Galaxies
• Robust covariance estimation of galaxy-galaxy weak lensing: validation and limitation of jackknife covariance
• Dark-ages Reionization & Galaxy Formation Simulation I: The dynamical lives of high redshift galaxies
• A volumetric deep Convolutional Neural Network for simulation of mock dark matter halo catalogues
• COSMOS: Stochastic bias from measurements of weak lensing and galaxy clustering
• Probing Cosmic Reionization and Molecular Gas Growth with TIME
• Towards understanding the structure of voids in the cosmic web
• Chandra deep observation of XDCP J0044.0-2033, a massive galaxy cluster at z>1.5
• Can we neglect relativistic temperature corrections in the Planck thermal SZ analysis?
• High-redshift JWST Observations and Primordial Non-Gaussianity
• Measuring the X-ray luminosities of SDSS DR7 clusters from RASS
• Joint power spectrum and voxel intensity distribution forecast on the CO luminosity function with COMAP
• Impact of baryons on the cluster mass function and cosmological parameter determination
• How well do we know the Halo Mass Function?
• Forecast for FAST: from Galaxies Survey to Intensity Mapping
• Numerical convergence of hydrodynamical simulations of galaxy formation: the abundance and internal structure of galaxies and their cold dark matter haloes
• Effect of radiative transfer on damped Lyman-alpha and Lyman limit systems in cosmological SPH simulations
• Matter bispectrum of large-scale structure: Three-dimensional comparison between theoretical models and numerical simulations
• Maximum redshift of gravitational wave merger events
• The strongest gravitational lenses: I. The statistical impact of cluster mergers
• Neutrinos and dark energy after Planck and BICEP2: data consistency tests and cosmological parameter constraints
• The Hunt for Primordial Interactions in the Large Scale Structures of the Universe
• Constraints on the redshift evolution of astrophysical feedback with Sunyaev-Zeldovich effect cross-correlations
• Stochastic gravitational wave background anisotropies in the mHz band: astrophysical dependencies
• The evolution of clustering length, large-scale bias and host halo mass at 2<z<5 in the VIMOS Ultra Deep Survey (VUDS)
• On the intermediate-redshift central stellar mass-halo mass relation, and implications for the evolution of the most massive galaxies since z~1
• Testing Cosmology with Extreme Galaxy Clusters
• A combined measurement of cosmic growth and expansion from clusters of galaxies, the CMB and galaxy clustering
• Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
• Revisiting The First Galaxies: The epoch of Population III stars
• Solitons in the dark: non-linear structure formation with fuzzy dark matter
• Clustering, host halos and environment of z$\sim$2 galaxies as a function of their physical properties
• Discovering gravitationally lensed gravitational waves: predicted rates, candidate selection, and localization with the Vera Rubin Observatory
• Coupled Quintessence and the Halo Mass Function
• Probing galaxy evolution in massive clusters using ACT and DES: splashback as a cosmic clock
• Mapping the allowed parameter space for decaying dark matter models
• The clustering of galaxies and galaxy clusters: constraints on primordial non-Gaussianity from future wide-field surveys
• The DEEP2 Galaxy Redshift Survey: The Voronoi-Delaunay Method catalog of galaxy groups
• Detection of Stacked Filament Lensing Between SDSS Luminous Red Galaxies
• Constraints on modified gravity from the observed X-ray luminosity function of galaxy clusters
• The halo mass function and filaments in full cosmological simulations with fuzzy dark matter
• The journey of QSO haloes from z=6 to the present
• First Results from COPSS: The CO Power Spectrum Survey
• Photometric redshifts for galaxies in the Subaru Hyper Suprime-Cam and unWISE and a catalogue of identified clusters of galaxies
• A Comparative Study of Local Galaxy Clusters: II: X-ray and SZ Scaling Relations
• Excursion Set Halo Mass Function and Bias in a Stochastic Barrier Model of Ellipsoidal Collapse
• Building a Predictive Model of Galaxy Formation - I: Phenomenological Model Constrained to the $z=0$ Stellar Mass Function
• Neutrino constraints: what large-scale structure and CMB data are telling us?
• Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
• Growth of Cosmic Structure
• Sensitivity of galaxy cluster dark energy constraints to halo modeling uncertainties
• Richness-mass relation self-calibration for galaxy clusters
• The Bias and Mass Function of Dark Matter Halos in Non-Markovian Extension of the Excursion Set Theory
• Joint halo mass function for modified gravity and massive neutrinos I: simulations and cosmological forecasts
• The evolution of the stellar mass versus halo mass relationship
• The primordial matter power spectrum on sub-galactic scales
• Cosmological and Astrophysical Implications of the Sunyaev-Zel'dovich Effect
• New Analytic Solutions for Galaxy Evolution: Gas, Stars, Metals and Dust in local Early-Type Galaxies and in their high-z Starforming Progenitors
• The Progenitors of Calcium-Strong Transients
• Rotation Curve Decomposition for Size-Mass Relations of Bulge, Disk, and Dark Halo in Spiral Galaxies
• Virialisation-induced curvature as a physical explanation for dark energy
• Constraining Cluster Virialization Mechanism and Cosmology using Thermal-SZ-selected clusters from Future CMB Surveys
• Simple halo model formalism for the cosmic infrared background and its correlation with the thermal Sunyaev Zel'dovich effect
• Impact of polarised extragalactic sources on the measurement of CMB B-mode anisotropies
• Cosmological Constraint Precision of the Photometric and Spectroscopic Multi-probe Surveys of China Space Station Telescope (CSST)
• Imprints of primordial non-Gaussianity on the number counts of cosmic shear peaks
• A high precision semi-analytic mass function
• Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters
• Cross-correlation of DES Y3 lensing and ACT/$Planck$ thermal Sunyaev Zel'dovich Effect II: Modeling and constraints on halo pressure profiles
• Combined analysis of galaxy cluster number count, thermal Sunyaev-Zel'dovich power spectrum, and bispectrum
• Angular power spectrum of galaxies in the 2MASS Redshift Survey
• High-energy neutrinos from sources in clusters of galaxies
• Detection of intercluster gas in superclusters using the thermal Sunyaev-Zel'dovich effect
• Mind the Gap: Tightening the Mass-Richness Relation with Magnitude Gaps
• Non-universality of the mass function: dependence on the growth rate and power spectrum shape
• Chasing Lyman alpha-emitting galaxies at z = 8.8
• Galaxy-galaxy weak-lensing measurement from SDSS: II. host halo properties of galaxy groups
• Revisiting the bulge-halo conspiracy I: Dependence on galaxy properties and halo mass
• PRIMUS: One- and Two-Halo Galactic Conformity at $0.2<z<1$
• Dissecting the Gamma-Ray Background in Search of Dark Matter
• Aemulus $\nu$: Precise Predictions for Matter and Biased Tracer Power Spectra in the Presence of Neutrinos
• The Impact of Theoretical Uncertainties in the Halo Mass Function and Halo Bias on Precision Cosmology
• Mass calibration of distant SPT galaxy clusters through expanded weak lensing follow-up observations with HST, VLT & Gemini-South
• Cold or Warm? Constraining Dark Matter with Primeval Galaxies and Cosmic Reionization after Planck
• The Q Continuum Simulation: Harnessing the Power of GPU Accelerated Supercomputers
• Luminous Red Galaxy Halo Density Field Reconstruction and Application to Large Scale Structure Measurements
• AMBER: A Semi-numerical Abundance Matching Box for the Epoch of Reionization
• Biasing and the search for primordial non-Gaussianity beyond the local type
• Voronoi volume function: A new probe of cosmology and galaxy evolution
• Satellite Quenching, Galaxy Inner Density and the Halo Environment
• A comparative study of radio halo occurrence in SZ and X-ray selected galaxy cluster samples
• IDCS J1426.5+3508: Cosmological implications of a massive, strong lensing cluster at Z = 1.75
• Estimating Luminosity Function Constraints from High-Redshift Galaxy Surveys
• Galaxy Cluster Mass Reconstruction Project: III. The impact of dynamical substructure on cluster mass estimates
• Bias deconstructed: Unravelling the scale dependence of halo bias using real space measurements
• Cosmological parameters constraints from galaxy cluster mass function measurements in combination with other cosmological data
• Updated Results on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Where stars form and live at high redshift: clues from the infrared
• The cosmological analysis of X-ray cluster surveys: I- A new method for interpreting number counts
• Probing the Intergalactic Medium with Ly$\alpha$ and 21 cm Fluctuations
• The clustering of typical Ly$\alpha$ emitters from $z\sim 2.5-6$: host halo masses depend on Ly$\alpha$ and UV luminosities
• The statistical nature of the brightest group galaxies
• Halo abundances within the cosmic web
• Stellar mass-gap as a probe of halo assembly history and concentration: youth hidden among old fossils
• Spherical collapse, formation hysteresis and the deeply non-linear cosmological power spectrum
• XXL Survey groups and clusters in the Hyper Suprime-Cam Survey. Scaling relations between X-ray properties and weak lensing mass
• The halo mass function in interacting Dark Energy models
• Foreground Biases on Primordial Non-Gaussianity Measurements from the CMB Temperature Bispectrum: Implications for Planck and Beyond
• Priors on red galaxy stochasticity from hybrid effective field theory
• Effects of the initial conditions on cosmological $N$-body simulations
• Head-to-Toe Measurement of El Gordo: Improved Analysis of the Galaxy Cluster ACT-CL J0102-4915 with New Wide-field Hubble Space Telescope Imaging Data
• Weakly Lensed Gravitational Waves: Probing Cosmic Structures with Wave-Optics Features
• How baryons can significantly bias cluster count cosmology
• Constraints on $S_8$ from a full-scale and full-shape analysis of redshift-space clustering and galaxy-galaxy lensing in BOSS
• The REFLEX II galaxy cluster survey: power spectrum analysis
• Galaxy downsizing evidenced by hybrid evolutionary tracks
• Deconstructing Thermal Sunyaev-Zel'dovich - Gravitational Lensing Cross-Correlations: Implications for the Intracluster Medium
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• Galaxy Cluster Mass Reconstruction Project - IV. Understanding the effects of imperfect membership on cluster mass estimation
• Halo Concentration, Galaxy Red Fraction, and Gas Properties of Optically-defined Merging Clusters
• Most massive halos with Gumbel Statistics
• Combining cluster number counts and galaxy clustering
• Cluster candidates around low power radio-galaxies at z~1-2 in COSMOS
• The XXL survey: XLVI. Forward cosmological analysis of the C1 cluster sample
• Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency
• The redshift evolution of X-ray and Sunyaev-Zel'dovich scaling relations in the FABLE simulations
• Chandra Measurements of a Complete Sample of X-ray Luminous Galaxy Clusters: The Luminosity-Mass Relation
• Cross-correlation of cosmic far-infrared background anisotropies with large scale structures
• A Prescription for Galaxy Biasing Evolution as a Nuisance Parameter
• Intensity mapping cross-correlations II: HI halo models including shot noise
• Cosmological Constraints from Galaxy Clustering and the Mass-to-Number Ratio of Galaxy Clusters: Marginalizing over the Physics of Galaxy Formation
• The 6dF Galaxy Survey: Dependence of halo occupation on stellar mass
• Recombination clumping factor during cosmic reionization
• Cosmological Constraints from the Large Scale Weak Lensing of SDSS MaxBCG Clusters
• On the Physical Requirements for a Pre-Reionization Origin of the Unresolved Near-Infrared Background
• A Redefinition of the Halo Boundary Leads to a Simple yet Accurate Halo Model of Large Scale Structure
• How are galaxies assigned to halos? Searching for assembly bias in the SDSS galaxy clustering
• Super-sample covariance approximations and partial sky coverage
• Quantifying the Line-of-Sight Halo Contribution to the Dark Matter Convergence Power Spectrum from Strong Gravitational Lenses
• The sum of the masses of the Milky Way and M31: a likelihood-free inference approach
• The rise and fall of a challenger: the Bullet Cluster in $\Lambda$ Cold Dark Matter simulations
• Mapping the real space distributions of galaxies in SDSS DR7: I. Two Point Correlation Functions
• Dark Matter Halos in Interacting Dark Energy Models: Formation History, Density Profile, Spin and Shape
• A Method for Measuring the Bias of High-Redshift Galaxies from Cosmic Variance
• Shocks in the Stacked Sunyaev-Zel'dovich Profiles of Clusters II: Measurements from SPT-SZ + Planck Compton-y Map
• The Correlated Formation Histories of Massive Galaxies and Their Dark Matter Halos
• Reconstructing cosmological initial conditions from galaxy peculiar velocities. III. Constrained simulations
• Accounting for Cosmic Variance in Studies of Gravitationally-Lensed High-Redshift Galaxies in the Hubble Frontier Field Clusters
• Observing AGN feedback with CO intensity mapping
• Simulations of Galileon modified gravity: Clustering statistics in real and redshift space
• Constraining cosmology with a new all-sky Compton parameter map from the Planck PR4 data
• A general framework to test gravity using galaxy clusters I: Modelling the dynamical mass of haloes in $f(R)$ gravity
• Cosmological Radio Emission induced by WIMP Dark Matter
• Self-calibration of weak lensing systematic effects using combined two- and three-point statistics
• Reionisation in sterile neutrino cosmologies
• COMAP Early Science: VII. Prospects for CO Intensity Mapping at Reionization
• Hydrodynamical simulations of coupled and uncoupled quintessence models I: Halo properties and the cosmic web
• The high redshift star-formation history from carbon-monoxide intensity maps
• A new model to predict weak-lensing peak counts III. Filtering technique comparisons
• Rapid simulation rescaling from standard to modified gravity models
• Estimating f_NL and g_NL from Massive High-Redshift Galaxy Clusters
• Probing lens-induced gravitational-wave birefringence as a test of general relativity
• The most massive objects in the Universe
• Impacts of the physical data model on the forward inference of initial conditions from biased tracers
• Inferring the impact of feedback on the matter distribution using the Sunyaev Zel'dovich effect: Insights from CAMELS simulations and ACT+DES data
• A closer look at CMB constraints on WIMP dark matter
• Modeling the evolution of infrared galaxies : clustering of galaxies in the Cosmic Infrared Background
• The Mass Function of Unprocessed Dark Matter Halos and Merger Tree Branching Rates
• Learning to Concentrate: Multi-tracer Forecasts on Local Primordial Non-Gaussianity with Machine-Learned Bias
• Projected-Field Kinetic Sunyaev-Zel'dovich Cross-Correlations: Halo Model and Forecasts
• Measuring the Thermal Sunyaev-Zel'dovich Effect Through the Cross Correlation of Planck and WMAP Maps with ROSAT Galaxy Cluster Catalogs
• Comparing halo bias from abundance and clustering
• Impact of systematics on cosmological parameters from future Galaxy Clusters surveys
• Primordial Non-Gaussianity and Extreme-Value Statistics of Galaxy Clusters
• The Galaxy--Halo Connection in High-Redshift Universe: Details and Evolution of Stellar-to-Halo Mass Ratios of Lyman Break Galaxies on CFHTLS Deep Fields
• Annealing a Follow-up Program: Improvement of the Dark Energy Figure of Merit for Optical Galaxy Cluster Surveys
• Baryon-CDM isocurvature galaxy bias with IllustrisTNG
• Estimating the warm dark matter mass from strong lensing images with truncated marginal neural ratio estimation
• Weak Lensing Analysis of SPT selected Galaxy Clusters using Dark Energy Survey Science Verification Data
• SMBH Seeds from Dissipative Dark Matter
• Simulation-based inference of dynamical galaxy cluster masses with 3D convolutional neural networks
• On the Properties of Spectroscopically-Confirmed Ultra-Diffuse Galaxies Across Environment
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• Cosmological Evidence Modelling: a new simulation-based approach to constrain cosmology on non-linear scales
• Quantifying the rareness of extreme galaxy clusters
• Probing wave-optics effects and low-mass dark matter halos with lensing of gravitational waves from massive black holes
• Cosmology with the CMB temperature-polarization correlation
• Weak-lensing mass calibration of the Sunyaev-Zel'dovich effect using APEX-SZ galaxy clusters
• The X-ray luminosity-temperature relation of a complete sample of low-mass galaxy clusters
• Warm Dark Matter and Cosmic Reionization
• An observational proxy of halo assembly time and its correlation with galaxy properties
• Modeling Extragalactic Foregrounds and Secondaries for Unbiased Estimation of Cosmological Parameters From Primary CMB Anisotropy
• Revealing the cosmic web dependent halo bias
• What determines large scale galaxy clustering: halo mass or local density?
• A Flexible Analytic Model of Cosmic Variance in the First Billion Years
• Statistical uncertainties and systematic errors in weak lensing mass estimates of galaxy clusters
• The 400d Galaxy Cluster Survey Weak Lensing Programme: I: MMT/Megacam Analysis of CL0030+2618 at z=0.50
• Exact Extreme Value Statistics and the Halo Mass Function
• Mass functions and bias of dark matter halos
• Cross-correlation of galaxies and galaxy clusters in the Sloan Digital Sky Survey and the importance of non-Poissonian shot noise
• On the current status of Modified Gravity
• Comparing gravitational redshifts of SDSS galaxy clusters with the magnification redshift enhancement of background BOSS galaxies
• Mass Calibration of the CODEX Cluster Sample using SPIDERS Spectroscopy -- I. The Richness-Mass Relation
• The role of massive halos in the Star Formation History of the Universe
• Cosmological constraints from abundance, weak-lensing and clustering of galaxy clusters: application to the SDSS
• Conditions for detecting lensed Population III galaxies in blind surveys with the James Webb Space Telescope, the Roman Space Telescope and Euclid
• Are the halo occupation predictions consistent with large scale galaxy clustering?
• Fast Weak Lensing Simulations with Halo Model
• Constraints on neutrino masses from the study of the nearby large-scale structure and galaxy cluster counts
• The mass function dependence on the dynamical state of dark matter haloes
• An application of extreme value statistics to the most massive galaxy clusters at low and high redshifts
• Halo assembly bias from Separate Universe simulations
• A Census of the LyC Photons that Form the UV Background During Reionization
• Remapping dark matter halo catalogues between cosmological simulations
• The Massive and Distant Clusters of WISE Survey: MOO J1142+1527, A 10${}^{15}$ M${}_{\odot }$ Galaxy Cluster at z=1.19
• Offsets between the X-ray and the Sunyaev-Zel'dovich-effect peaks in merging galaxy clusters and their cosmological implications
• Constraining cosmology with shear peak statistics: tomographic analysis
• An improved model of HII bubbles during the epoch of reionization
• Extending the $L_{\mathrm{X}}-T$ relation from clusters to groups-Impact of cool core nature, AGN feedback, and selection effects
• Euclid preparation. XXXII. Evaluating the weak lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
• (No) dimming of X-ray clusters beyond z~1 at fixed mass: crude redhshifts and masses from raw X-ray and SZ data
• Circular Polarization of the Astrophysical Gravitational Wave Background
• Excursion set theory for modified gravity: Eulerian versus Lagrangian environments
• Constraining the halo mass function with observations
• Probing Cosmology with Dark Matter Halo Sparsity Using X-ray Cluster Mass Measurements
• Augmenting astrophysical scaling relations with machine learning: application to reducing the Sunyaev-Zeldovich flux-mass scatter
• Tests of Gravity with Galaxy Clusters
• Cosmology dependence of galaxy cluster scaling relations
• Stacked Weak Lensing Mass Calibration: Estimators, Systematics, and Impact on Cosmological Parameter Constraints
• Including massive neutrinos in thermal Sunyaev Zeldovich power spectrum and cluster counts analyses
• On Physical Scales of Dark Matter Halos
• ELUCID V. Lighting dark matter halos with galaxies
• $\text{matryoshka}$: Halo Model Emulator for the Galaxy Power Spectrum
• Probing galaxy bias and intergalactic gas pressure with KiDS Galaxies-tSZ-CMB lensing cross-correlations
• Halo Exclusion Criteria Impacts Halo Statistics
• Constraining neutrino properties with a Euclid-like galaxy cluster survey
• Galaxy groups in the 2MASS Redshift Survey
• Cross-Correlation of the Extragalactic Gamma-ray Background with Luminous Red Galaxies
• An Intensity Mapping Constraint on the CO-Galaxy Cross Power Spectrum at Redshift ~ 3
• N-body simulations with a cosmic vector for dark energy
• Exploring Cosmic Origins with CORE: Cluster Science
• Halo Occupation Distribution Modeling of Green Valley Galaxies
• The SZ flux-mass ($Y$-$M$) relation at low halo masses: improvements with symbolic regression and strong constraints on baryonic feedback
• Cosmological constraints on dark matter annihilation and decay: Cross-correlation analysis of the extragalactic $\gamma$-ray background and cosmic shear
• Cross-correlation of DES Y3 lensing and ACT/$Planck$ thermal Sunyaev Zel'dovich Effect I: Measurements, systematics tests, and feedback model constraints
• Comparison of Sunyaev-Zel'dovich measurements from Planck and from the Arcminute Microkelvin Imager for 99 galaxy clusters
• Clustering dark energy and halo abundances
• Large Scale Anisotropic Bias from Primordial non-Gaussianity
• "Little red dots" cannot reside in the same dark matter halos as comparably luminous unobscured quasars
• The Massive Satellite Population of Milky-Way Sized Galaxies
• The role of the eROSITA all-sky survey in searches for sterile neutrino dark matter
• A Consistent Approach to Falsifying Lambda-CDM with Rare Galaxy Clusters
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• Parallel HOP: A Scalable Halo Finder for Massive Cosmological Data Sets
• The imprint of $f(R)$ gravity on weak gravitational lensing I: Connection between observables and large scale structure
• The Galaxy-Halo Connection for $1.5\lesssim z\lesssim 5$ as revealed by the \emph{Spitzer} Matching survey of the UltraVISTA ultra-deep Stripes
• Exploring the cosmological synergy between galaxy cluster and cosmic void number counts
• Assessing the Importance of Noise from Thermal Sunyaev-Zel{'}dovich Signals for CMB Cluster Surveys and Cluster Cosmology
• Spatially Offset Active Galactic Nuclei. II: Triggering in Galaxy Mergers
• Constraints on decaying dark matter from weak lensing and cluster counts
• Measuring nonlocal Lagrangian peak bias
• Calibrating Cluster Number Counts with CMB lensing
• Conditional Probabilities in the Excursion Set Theory. Generic Barriers and non-Gaussian Initial Conditions
• The extended ROSAT-ESO Flux-Limited X-ray Galaxy Cluster Survey (REFLEX II) VII The Mass Function of Galaxy Clusters
• The Effects of Varying Cosmological Parameters on Halo Substructure
• Computation of the Halo Mass Function Using Physical Collapse Parameters: Application to Non-Standard Cosmologies
• Strategies for Detecting the Missing Hot Baryons in the Universe
• The Next Generation Virgo Cluster Survey. IX. Estimating the Efficiency of Galaxy Formation on the Lowest-Mass Scales
• C${}^3$-Cluster Clustering Cosmology I. New constraints on the cosmic growth rate at z~0.3 from redshift-space clustering anisotropies
• Mass-concentration relation of clusters of galaxies from CFHTLenS
• Stellar Mass to Halo Mass Scaling Relation for X-ray Selected Low Mass Galaxy Clusters and Groups out to Redshift $z\approx 1$
• A direct detection of neutral hydrogen intensity mapping on Mpc scales at $z\approx 0.32$ and $z\approx 0.44$
• The Halo Void (Dust) Model of Large Scale Structure
• The Dipole of the Astrophysical Gravitational-Wave Background
• The Influence of Galaxy Formation Physics on Weak Lensing Tests of General Relativity
• Mass Variance from Archival X-ray Properties of Dark Energy Survey Year-1 Galaxy Clusters
• Understanding the non-linear clustering of high redshift galaxies
• EFTofLSS meets simulation-based inference: ${\sigma }_8$ from biased tracers
• On the starting redshift for cosmological simulations: Focusing on halo properties
• The locations of halo formation and the peaks formalism
• Optimizing weak lensing mass estimates for cluster profile uncertainty
• Statistics of Dark Matter Halos from the Excursion Set Approach
• A unified model for the clustering of quasars and galaxies at $z\approx 6$
• The Power of Halometry
• Testing flatness of the universe with probes of cosmic distances and growth
• Baryon Pasting Algorithm: Halo-based and Particle-based Pasting Methods
• Constraining the properties of gaseous halos via cross-correlations of upcoming galaxy surveys and thermal Sunyaev-Zel'dovich maps
• Weak Lensing Peak Finding: Estimators, Filters, and Biases
• Linking a universal gas density profile to the core-excised X-ray luminosity in galaxy clusters up to z ~ 1.1
• Effect of halo bias and Lyman Limit Systems on the history of cosmic reionization
• Structure Formation and the Global 21-cm Signal in the Presence of Coulomb-like Dark Matter-Baryon Interactions
• Retrieving cosmological information from small-scale CMB foregrounds II. The kinetic Sunyaev Zel'dovich effect
• Cluster Mergers and the Origin of the ARCADE-2 Excess
• Primordial non-Gaussianity with $\mu$-type and $y$-type spectral distortions: exploiting Cosmic Microwave Background polarization and dealing with secondary sources
• Radio Scattering Horizons for Galactic and Extragalactic Transients
• Covariance matrices for halo number counts and correlation functions
• Press-Schechter primordial black hole mass functions and their observational constraints
• Feeding cosmic star formation: Exploring high-redshift molecular gas with CO intensity mapping
• From starburst to quiescence: post-starburst galaxies and their large-scale clustering over cosmic time
• Bayesian Inference of Initial Conditions from Non-Linear Cosmic Structures using Field-Level Emulators
• Cosmological constraints from the power spectrum and bispectrum of 21cm intensity maps
• Cosmology and Astrophysics from Relaxed Galaxy Clusters V: Consistency with Cold Dark Matter Structure Formation
• Cluster counts: calibration issue or new physics?
• Coupling parsec and gigaparsec scales: primordial non-Gaussianity with multi-tracer intensity mapping
• Cosmological constraints from the observed angular cross-power spectrum between Sunyaev-Zel'dovich and X-ray surveys
• A short review on clustering dark energy
• Stellar Mass Function of Active and Quiescent Galaxies via the Continuity Equation
• Taking measurements of the kinematic Sunyaev-Zel'dovich effect forward: including uncertainties from velocity reconstruction with forward modeling
• Impact of the mean pressure profile of galaxy clusters on the cosmological constraints from the $Planck$ tSZ power spectrum
• LoCuSS: The splashback radius of massive galaxy clusters and its dependence on cluster merger history
• Dianoga SIDM: galaxy cluster self-interacting dark matter simulations
• Removing the giants and learning from the crowd: a new SZ power spectrum method and revised Compton $y$-map analysis
• Weak Lensing Analysis of CODEX Clusters using Dark Energy Camera Legacy Survey : Mass-Richness Relation
• Prospects for detecting gravitational waves from eccentric subsolar mass compact binaries
• The Total Mass of Dark Matter Haloes
• Weak Lensing Peaks in Simulated Light-Cones: Investigating the Coupling between Dark Matter and Dark Energy
• GalWeight Application: A publicly-available catalog of dynamical parameters of 1,800 galaxy clusters from SDSS-DR13, ($GalWCat19$)
• New constraints on the mass bias of galaxy clusters from the power spectra of the thermal Sunyaev-Zeldovich effect and cosmic shear
• CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc
• Detectability of the gravitational redshift effect from the asymmetric galaxy clustering
• Halo Properties and Mass Functions of Groups/Clusters from the DESI Legacy Imaging Surveys DR9
• Cosmology with the largest galaxy cluster surveys: Going beyond Fisher matrix forecasts
• Magnitude Gap Statistics and the Conditional Luminosity Function
• Galaxy And Mass Assembly: Estimating galaxy group masses via caustic analysis
• Galaxy-Mass Correlations on 10 Mpc Scales in the Deep Lens Survey
• Probing primordial non-Gaussianity with the power spectrum and bispectrum of future 21cm intensity maps
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• Establishing the Non-Primordial Origin of Black Hole-Neutron Star Mergers
• Probing Cosmology and Cluster Astrophysics with Multi-Wavelength Surveys I. Correlation Statistics
• A critical analysis of high-redshift, massive galaxy clusters: I
• ALMA observations of lensed Herschel sources : Testing the dark-matter halo paradigm
• Influence of Projection in Cluster Cosmology Studies
• Aging Halos: Implications of the Magnitude Gap on Conditional Statistics of Stellar and Gas Properties of Massive Halos
• A New Approach to Identifying the Most Powerful Gravitational Lensing Telescopes
• Constraining f(R) Gravity with Planck Sunyaev-Zel'dovich Clusters
• Comparing Simple Quasar Demographics Models
• Cosmological Vlasov-Poisson Simulations of Structure Formation with Relic Neutrinos: Nonlinear Clustering and the Neutrino Mass
• Running with BICEP2: Implications for Small-Scale Problems in CDM
• Cosmic Infrared Background anisotropies as a window into primordial non-Gaussianity
• How to Build a Catalogue of Linearly-Evolving Cosmic Voids
• Velocity and mass bias in the distribution of dark matter halos
• Euclid: Effect of sample covariance on the number counts of galaxy clusters
• Excess of high-$z$ galaxies as a test for bumpy power spectrum of density perturbations
• The Outer Stellar Mass of Massive Galaxies: A Simple Tracer of Halo Mass with Scatter Comparable to Richness and Reduced Projection Effects
• Optical-SZE Scaling Relations for DES Optically Selected Clusters within the SPT-SZ Survey
• Velocity reconstruction with the cosmic microwave background and galaxy surveys
• Confronting the Magnetar Interpretation of Fast Radio Bursts Through Their Host Galaxy Demographics
• Effects of long-wavelength fluctuations in large galaxy surveys
• The co-evolution of black hole growth and star formation from a cross-correlation analysis between quasars and the cosmic infrared background
• 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 $z\gtrsim 1$
• PSZSPT: a joint Planck and SPT-SZ cluster catalog
• The universal multiplicity function: counting halos and voids
• X-ray Cluster Constraints on Non-Gaussianity
• Evidence for the Fifth Element Astrophysical status of Dark Energy
• Stacked lensing estimators and their covariance matrices: Excess surface mass density vs. Lensing shear
• Cosmological Constraints from Galaxy Cluster Sparsity, Cluster Gas Mass Fraction and Baryon Acoustic Oscillations Data
• New Analytic Solutions for Galaxy Evolution II: Wind Recycling, Galactic Fountains and Late-Type Galaxies
• A clustering-based self-calibration of the richness-to-mass relation of CAMIRA galaxy clusters out to $z\approx 1.1$ in the Hyper Suprime-Cam survey
• The strongest gravitational lenses: II. Is the large Einstein radius of MACS J0717.5+3745 in conflict with LCDM?
• Universal Merger Histories of Dark-Matter Haloes
• Non-Gaussian Scatter in Cluster Scaling Relations
• Velocity dispersion and dynamical mass for 270 galaxy clusters in the Planck PSZ1 catalogue
• Clustering of Gravitational Wave and Supernovae events: a multitracer analysis in Luminosity Distance Space
• Extracting HI Astrophysics from Interferometric Intensity Mapping
• Galaxy Clusters as a probe of early dark energy
• RedMaPPer: Evolution and Mass Dependence of the Conditional Luminosity Functions of Red Galaxies in Galaxy Clusters
• Taming assembly bias for primordial non-Gaussianity
• Non-Gaussianity of secondary anisotropies from ACTPol and Planck
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• Vector dark energy and high-z massive clusters
• Primordial trispectrum from kSZ tomography
• Covariance in the Thermal SZ-Weak Lensing Mass Scaling Relation of Galaxy Clusters
• Connecting optical and X-ray tracers of galaxy cluster relaxation
• Prospects for high-z cluster detections with Planck, based on a follow-up of 28 candidates using MegaCam@CFHT
• 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
• Understanding large-scale structure in the SSA22 protocluster region using cosmological simulations
• The clustering of $z>7$ galaxies: Predictions from the BLUETIDES simulation
• Quasar Host Environments: The view from Planck
• Helium Reionization Simulations. I. Modeling Quasars as Radiation Sources
• Constructing mock catalogues for the REFLEX II galaxy cluster sample
• Weak lensing calibration of mass bias in the REFLEX+BCS X-ray galaxy cluster catalogue
• Host Dark Matter Halos of WISE-selected Obscured & Unobscured Quasars: Evidence for Evolution
• Practical Cosmology with Lenses
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogs for the Emission Line Galaxy Sample
• Multi-wavelength mock galaxy catalogs of the low-redshift Universe
• Statistical Properties of Radio Halos in Galaxy Clusters and Origin of Seed Electrons for Reacceleration
• Quintessential Scale Dependence from Separate Universe Simulations
• Subhaloes gone Notts: the clustering properties of subhaloes
• The clustering of baryonic matter. I: a halo-model approach
• Effective Window Function for Lagrangian Halos
• Detecting Galaxy Groups and AGNs populating the local Universe in the eROSITA era
• The SRG/eROSITA All-Sky Survey: Constraints on AGN Feedback in Galaxy Groups
• Joint Analysis of Galaxy-Galaxy Lensing and Galaxy Clustering: Methodology and Forecasts for DES
• eROSITA cluster cosmology forecasts: cluster temperature substructure bias
• The effect of dark matter-dark radiation interactions on halo abundance -- a Press-Schechter approach
• Cosmology with velocity dispersion counts: an alternative to measuring cluster halo masses
• The environment and host haloes of the brightest z~6 Lyman-break galaxies
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
• Prospects for 21cm-Galaxy Cross-Correlations with HERA and the Roman High-Latitude Survey
• Modelling the asymmetry of the halo cross-correlation function with relativistic effects at quasi-linear scales
• Amending the halo model to satisfy cosmological conservation laws
• Post-inflationary axion isocurvature perturbations facing CMB and large-scale structure
• The BAHAMAS project: Effects of dynamical dark energy on large-scale structure
• Seeking dark matter with $\gamma$-ray attenuation
• Non-Gaussian Halo Mass Function and Non-Spherical Halo Collapse: Theory vs. Simulations
• The cosmological free-free signal from galaxy groups and clusters
• Maturing Satellite Kinematics into a Competitive Probe of the Galaxy-Halo Connection
• Counts of galaxy clusters as cosmological probes: the impact of baryonic physics
• Chandra Observations of the Planck ESZ Sample: A Re-Examination of Masses and Mass Proxies
• TRINITY II: The Luminosity-dependent Bias of the Supermassive Black Hole Mass--Galaxy Mass Relation for Bright Quasars at $z=6$
• One never walks alone: the effect of the perturber population on subhalo measurements in strong gravitational lenses
• Issues in joint SZ and optical cluster finding
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• Halo models of HI selected galaxies
• The local PNG bias of neutral Hydrogen, ${\mathrm{H}}_{\mathrm{I}}$
• The 21cm radiation from minihalos as a probe of small primordial non-Gaussianity
• Inadequacy of internal covariance estimation for super-sample covariance
• The clustering of dark matter halos: scale-dependent bias on quasi-linear scales
• Perturbation theory for nonlinear halo power spectrum: the renormalized bias and halo bias
• Cosmology with galaxy cluster weak lensing: statistical limits and experimental design
• Effects of Multiphase Gas and Projection on X-ray Observables in Simulated Galaxy Clusters as Seen by eROSITA
• Analysis of Sunyaev-Zel'dovich Effect Mass-Observable Relations using South Pole Telescope Observations of an X-ray Selected Sample of Low Mass Galaxy Clusters and Groups
• Hierarchical inference of the relationship between Concentration and Mass in Galaxy Groups and Clusters
• Cold dark energy constraints from the abundance of galaxy clusters
• A high-resolution cosmological simulation of a strong gravitational lens
• Constraints on Modified Gravity from Sunyaev-Zeldovich Cluster Surveys
• The Diffuse Gamma-Ray Flux from Clusters of Galaxies
• The evolution of star formation activity in galaxy groups
• Effects of Completeness and Purity on Cluster Dark Energy Constraints
• The halo mass function conditioned on density from the Millennium Simulation: insights into missing baryons and galaxy mass functions
• Velocity dispersion and dynamical masses for 388 Galaxy Clusters and groups. Calibrating the $M_{\mathrm{SZ}}$--$M_{\mathrm{dyn}}$ scaling relation for the PSZ2 sample
• Quasi-equilibrium models of high-redshift disc galaxy evolution
• Global radiation signature from early structure formation
• Modeling of weak lensing statistics. I. Power spectrum and bispectrum
• An Accurate Analytic Model for the Thermal Sunyaev-Zel'dovich One-Point PDF
• Impact of ICM disturbances on the mean pressure profile of galaxy clusters: a prospective study of the NIKA2 SZ large program with MUSIC synthetic clusters
• Tully-Fisher Distances and Dynamical Mass Constraints for 24 Host Galaxies of Reverberation-Mapped AGN
• Constraining isocurvature perturbations with the 21cm emission from minihaloes
• Effects of center offset and noise on weak-lensing derived concentration-mass relation of dark matter halos
• Constraining the Mass of the Emerging Galaxy Cluster SpARCS1049+56 at z=1.71 with Infrared Weak Lensing
• Small scale clustering of late forming dark matter
• Testing dark matter warmness and quantity via the reduced relativistic gas model
• A direct and robust method to observationally constrain the halo mass function via the submillimeter magnification bias: Proof of concept
• Mass Bias of Weak Lensing Shear-selected Galaxy Cluster Samples
• Evolution mapping: a new approach to describe matter clustering in the non-linear regime
• Analytical halo model of galactic conformity
• Scaling Relations and X-ray Properties of Moderate-Luminosity Galaxy Clusters from 0.3 < z < 0.6 with XMM-Newton
• Virial halo mass function in the $Planck$ cosmology
• A Better Way to Define Dark Matter Haloes
• Optical Galaxy Clusters in the Deep Lens Survey
• Covariances for cosmic shear and galaxy-galaxy lensing in the response approach
• The abundance of dark matter haloes down to Earth mass
• The SRG/eROSITA All-Sky Survey : Constraints on the structure growth from cluster number counts
• The SRG/eROSITA All-Sky Survey: Weak-Lensing of eRASS1 Galaxy Clusters in KiDS-1000 and Consistency Checks with DES Y3 & HSC-Y3
• Revisiting the bulge-halo conspiracy II: Towards explaining its puzzling dependence on redshift
• The SRG-eROSITA All-Sky Survey : Constraints on f(R) Gravity from Cluster Abundance
• The frequency of very young galaxies in the local Universe: I. A test for galaxy formation and cosmological models
• Accuracy of analytical models of the large-scale matter distribution
• Active gas features in three HSC-SSP CAMIRA clusters revealed by high angular resolution analysis of MUSTANG-2 SZE and XXL X-ray observations
• Probing dark energy with the next generation X-ray surveys of galaxy clusters
• Validation of Selection Function, Sample Contamination and Mass Calibration in Galaxy Cluster Samples
• Can ultralight dark matter explain the age-velocity dispersion relation of the Milky Way disc: A revised and improved treatment
• Relationship between the CMB, SZ Cluster Counts, and Local Hubble Parameter Measurements in a Simple Void Model
• Impact of Population III homogeneous stellar evolution on early cosmic reionisation
• Constraints on $f(R)$ and nDGP Modified Gravity Model Parameters with Cluster Abundances and Galaxy Clustering
• Modelling the shapes of the largest gravitationally bound objects
• CODEX Weak Lensing Mass Catalogue and implications on the mass-richness relation
• AMICO galaxy clusters in KiDS-DR3: measuring the splashback radius from weak gravitational lensing
• The Milky Way, Coming into Focus: Precision Astrometry Probes its Evolution, and its Dark Matter
• Explaining dark matter halo density profiles with neural networks
• Large-scale bias of dark matter halos
• Understanding matched filters for precision cosmology
• Non-Gaussianity of the Cosmic Infrared Background anisotropies II : Predictions of the bispectrum and constraints forecast
• Cosmic Star Formation: a simple model of the SFRD(z)
• The BAHAMAS project: Effects of a running scalar spectral index on large-scale structure
• Neutrino Mass Inference from SZ Surveys
• Cosmology with XMM galaxy clusters: the X-CLASS/GROND catalogue and photometric redshifts
• The Ultraviolet Detection of Diffuse Gas in Galaxy Groups
• The Breakdown Scale of HI Bias Linearity
• Patchy Screening of the CMB from Dark Photons
• On estimating the cosmic molecular gas density from CO Line Intensity Mapping observations
• High-redshift galaxy groups as seen by Athena/WFI
• Redshift-space correlation functions in large galaxy cluster surveys
• On the Redshift Evolution of MgII Absorption Systems
• Lyman-$\alpha$ Polarization Intensity Mapping
• Measurement of redshift dependent cross correlation of HSC clusters and Fermi $\gamma$ rays
• Measuring line-of-sight shear with Einstein rings: a proof of concept
• Impact of gas based seeding on supermassive black hole populations at $z\ge 7$
• Towards optimal estimation of the galaxy power spectrum
• Predicting the CIB-$\varphi$ contamination in the cross-correlation of the tSZ effect and $\varphi$
• Cross Correlation between the Thermal Sunyaev-Zel'dovich Effect and Projected Galaxy Density Field
• Forecasting the Cross-Correlation of the CSST galaxy survey with the FAST HI Intensity Map
• Extragalactic diffuse gamma-rays from dark matter annihilation: revised prediction and full modelling uncertainties
• Merger-driven evolution of the effective stellar initial mass function of massive early-type galaxies
• Revisiting the Extreme Clustering of $z\approx 4$ Quasars with Large Volume Cosmological Simulations
• Constraining the galaxy-halo connection of infrared-selected unWISE galaxies with galaxy clustering and galaxy-CMB lensing power spectra
• Future Cosmology: New Physics and Opportunity from the China Space Station Telescope (CSST)
• The clustering of baryonic matter. II: halo model and hydrodynamic simulations
• Lonely Little Red Dots: Challenges to the AGN-nature of little red dots through their clustering and spectral energy distributions
• The Probability Distribution of Astrophysical Gravitational-Wave Background Fluctuations
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• The Clusters Hiding in Plain Sight (CHiPS) survey: Complete sample of extreme BCG clusters
• Halo Mass Definition and Multiplicity Function
• Discriminating power of milli-lensing observations for dark matter models
• The Stellar-to-Halo Mass Ratios of Passive and Star-Forming Galaxies at z~2-3 from the SMUVS survey
• Cross-correlation between thermal Sunyaev-Zeldovich effect and the integrated Sachs-Wolfe effect
• Chandra and optical/IR observations of CXOJ1415.2+3610, a massive, newly discovered galaxy cluster at z~1.5
• Signatures of dark and baryonic structures on weakly lensed gravitational waves
• Mass and pressure constraints on galaxy clusters from interferometric SZ observations
• On the small scale clustering of quasars: constraints from the MassiveBlack II simulation
• How accurate is our knowledge of galaxy bias?
• Future sensitivity of neutrino telescopes to dark matter annihilations from the cosmic diffuse neutrino signal
• Cosmology based on $f(R)$ gravity with $\mathcal{O}(1)$ eV sterile neutrino
• The SWIFT AGN and Cluster Survey I: Number Counts of AGN and Galaxy Clusters
• Compensated Isocurvature Perturbations in the Galaxy Power Spectrum
• RELICS: A Very Large (${\theta }_E\sim 40"$) Cluster Lens -- RXC J0032.1+1808
• The FLAMINGO project: Baryonic impact on weak gravitational lensing convergence peak counts
• The Extreme Tail of the Non-Gaussian Mass Function
• Downsizing of Star Formation Measured from the Clustered Infrared Background Correlated with Quasars
• Decaying warm dark matter and structure formation
• Number Counts and Dynamical Vacuum Cosmologies
• The Merger Rate of Primordial Black Hole-Neutron Star Binaries in Ellipsoidal-Collapse Dark Matter Halo Models
• A Halo Occupation Interpretation Of Quasars At $z\sim 1.5$ Using Very Small Scale Clustering Information
• Observing relativistic features in large-scale structure surveys -- I: Multipoles of the power spectrum
• A partial inventory of observational anisotropies in single-dish line-intensity mapping
• Cluster Probes of Dark Energy Clustering
• Precise Mass Determination of SPT-CL J2106-5844, the Most Massive Cluster at z>1
• Dark matter halo creation in moving barrier models
• Testing the conditional mass function of dark matter halos against numerical N-body simulations
• Mass Calibration of the CODEX Cluster Sample using SPIDERS Spectroscopy -- II. The X-ray Luminosity-Mass Relation
• Constraining CMB temperature evolution with Sunyaev-Zel'dovich galaxy clusters from the Atacama Cosmology Telescope
• Isotropic extragalactic flux from dark matter annihilations: lessons from interacting dark matter scenarios
• Density fields and halo mass functions in the Geometrical Adhesion toy Model
• Prospects for Observing the low-density Cosmic Web in Lyman-alpha Emission
• Cluster-Cluster Lensing and the Case of Abell 383
• Primordial magnetic fields with X-ray and S-Z cluster survey
• Exploring compensated isocurvature perturbations with CMB spectral distortion anisotropies
• AMICO galaxy clusters in KiDS-DR3: Cosmological constraints from angular power spectrum and correlation function
• Biases on cosmological parameter estimators from galaxy cluster number counts
• Probing gravity with redshift-space distortions: effects of tracer bias and sample selection
• The star formation history in the last 10 billion years from CIB cross-correlations
• Constraining thawing and freezing models with cluster number counts
• Cluster counts. II. Tensions, massive neutrinos, and modified gravity
• The Anisotropy of the Extragalactic Radio Background from Dark Matter Annihilation
• Galaxy clustering from the bottom up: A Streaming Model emulator I
• ΛCDM is still not broken: empirical constraints on the star formation efficiency at z ~ 12-30
• Unveiling cosmological information on small scales with line intensity mapping
• The cosmological analysis of X-ray cluster surveys; III. 4D X-ray observable diagrams
• Testing the accuracy of likelihoods for cluster abundance cosmology
• Impact of radio sources and cosmic infrared background on thermal Sunyaev-Zel'dovich - gravitational lensing cross correlation
• HI intensity mapping correlation function from UNIT simulations: BAO and observationally induced anisotropy
• An analytic halo approach to the bispectrum of galaxies in redshift space
• Searching for eV-mass Axion-like Particles with Cross Correlations between Line Intensity and Weak Lensing Maps
• An Optical Observational Cluster Mass Function at $z\sim 1$ with the ORELSE Survey
• Gas around galaxy haloes: methodology comparisons using hydrodynamical simulations of the intergalactic medium
• Constraining low redshift [CII] Emission by Cross-Correlating FIRAS and BOSS Data
• Novel Conservative Methods for Adaptive Force Softening in Collisionless and Multi-Species N-Body Simulations
• Neutrino mass constraints beyond linear order: cosmology dependence and systematic biases
• Formation of the large-scale structure of the Universe
• Dwarf Galaxies in Voids: Dark Matter Halos and Gas Cooling
• Nonlinear reconstruction of features in the primordial power spectrum from large-scale structure
• Galaxy cluster rotation revealed in the MACSIS simulations with the kinetic Sunyaev-Zeldovich effect
• Constraints On Duty Cycles Of Quasars At Z $\sim$ 6
• Improved analytical modeling of the non-linear power spectrum in modified gravity cosmologies
• Retrieving cosmological information from small-scale CMB foregrounds I. The thermal Sunyaev Zel'dovich effect
• On the Merger Rate of Primordial Black Holes in Cosmic Voids
• The $f(R)$ halo mass function in the cosmic web
• Constraining Cosmological Parameters using the Cluster Mass-Richness Relation
• The BAHAMAS project: Evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum
• A Stochastic Theory of the Hierarchical Clustering I. Halo Mass Function
• Debiased Galaxy Cluster Pressure Profiles from X-ray Observations and Simulations
• Halo abundances and shear in void models
• On the Abundance of Extreme Voids
• Optical follow-up study of 32 high-redshift galaxy cluster candidates from Planck with the William Herschel Telescope
• Order statistics applied to the most massive and most distant galaxy clusters
• Confrontation of Top-Hat Spherical Collapse against Dark Halos from Cosmological N-Body Simulations
• Evidence of dark energy in different cosmological observations
• Signatures of Light Massive Relics on nonlinear structure formation
• The Importance of Being Interpretable: Toward An Understandable Machine Learning Encoder for Galaxy Cluster Cosmology
• Validating the methodology for constraining the linear growth rate from clustering anisotropies
• Early Quenching of Massive Protocluster Galaxies Around z=2.2 Radio Galaxies
• Strong-lensing cosmography using third-generation gravitational-wave detectors
• Measurement of Galaxy Cluster Integrated Comptonization and Mass Scaling Relations with the South Pole Telescope
• Halo Masses of MgII absorbers at z\sim 0.5 from SDSS DR7
• Beacons In the Dark: Using Novae and Supernovae to Detect Dwarf Galaxies in the Local Universe
• Numerical simulations of dark matter haloes produce polytropic central cores when reaching thermodynamic equilibrium
• Cosmology with Galaxy Clusters: Systematic Effects in the Halo Mass Function
• Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing run
• Painting baryons onto N-body simulations of galaxy clusters with image-to-image deep learning
• The extended ROSAT-ESO Flux-Limited X-ray Galaxy Cluster Survey (REFLEX II) VI. Effect of massive neutrinos on the cosmological constraints from clusters
• Sunyaev-Zel'dovich Signal from Quasar Hosts: Implications for Detection of Quasar Feedback
• The impact of braiding covariance and in-survey covariance on next-generation galaxy surveys
• $\text{PineTree}$: A generative, fast, and differentiable halo model for wide-field galaxy surveys
• Modeling the cross power spectrum of Sunyaev-Zel'dovich and X-ray surveys
• Cosmological interpretation of the color-magnitude diagrams of galaxy clusters
• Statistics of Dark Matter Halos in the Excursion Set Peak Framework
• Screening maps of the local Universe I -- Methodology
• Dynamical friction in the primordial neutrino sea
• Extending Semi-numeric Reionisation Models to the First Stars and Galaxies
• BASILISK: Bayesian Hierarchical Inference of the Galaxy-Halo Connection using Satellite Kinematics--I. Method and Validation
• Remapping simulated halo catalogues in redshift space
• Cosmological feedback from a halo assembly perspective
• The thermal and gravitational energy densities in the large-scale structure of the Universe
• Star Formation and Chemical Enrichment in Protoclusters
• X-ray galaxy clusters abundance and mass temperature scaling
• What can the spatial distribution of galaxy clusters tell about their scaling relations?
• Constraints on Neutrino Mass from Sunyaev--Zeldovich Cluster Surveys
• Halo Counts-in-cells for Cosmological Models with Different Dark Energy
• A joint analysis of AMI and CARMA observations of the recently discovered SZ galaxy cluster system AMI-CL J0300+2613
• Neutrino winds on the sky
• Constraining the intracluster pressure profile from the thermal SZ power spectrum
• The effect of the morphological quenching mechanism on star formation activity at 0.5 < z < 1.5 in 3D-HST/CANDELS
• The influence of primordial magnetic fields on the spherical collapse model in cosmology
• Leverage on small-scale primordial non-Gaussianity through cross-correlations between CMB $E$-mode and $\mu$-distortion anisotropies
• Can we use Weak Lensing to Measure Total Mass Profiles of Galaxies on 20 kiloparsec Scales?
• The virialization density of peaks with general density profiles under spherical collapse
• The effect of selection -- a tale of cluster mass measurement bias induced by correlation and projection
• Tomography-based observational measurements of the halo mass function via the submillimeter magnification bias
• Recent developments in astrophysical and cosmological exploitation of microwave surveys
• Probing superheavy dark matter through lunar radio observations of ultrahigh-energy neutrinos and the impacts of neutrino cascades
• The coevolution of the velocity and mass functions of galaxies and dark haloes
• Reconstruction of small-scale galaxy cluster substructure with lensing flexion
• Dark Matter Pollution in the Diffuse Supernova Neutrino Background
• Statistics of Two-point Correlation and Network Topology for Lyman Alpha Emitters at $z\approx 2.67$
• Global analysis of luminosity- and colour-dependent galaxy clustering in the Sloan Digital Sky Survey
• An Extended Zel'dovich Model for the Halo Mass Function
• Dark matter halo mass functions and density profiles from mass and energy cascade
• MUSCLE-UPS: Improved Approximations of the Matter Field with the Extended Press-Schechter Formalism and Lagrangian Perturbation Theory
• The cosmological analysis of X-ray cluster surveys: IV. Testing ASpiX with template-based cosmological simulations
• The Stellar Mass - Halo Mass Relation for Low Mass X-ray Groups at 0.5<z<1 in the CDFS with CSI
• A semi-analytic model of pairwise velocity distribution between dark matter halos
• Inverse-Compton Scattering of the Cosmic Infrared Background
• How well do third-order aperture mass statistics separate E- and B-modes?
• Damped Lyman-$\alpha$ absorbers and atomic hydrogen in galaxies: the view of the GAEA model
• Why are we still using 3D masses for cluster cosmology?
• Hydrodynamical Simulations of Galaxy Clusters with Galcons
• Galaxy flows within 8,000 km/s from Numerical Action methods
• A Universal Profile for Stacked Filaments from Cold Dark Matter Simulations
• Characterizing the Conditional Galaxy Property Distribution using Gaussian Mixture Models
• Joint signal extraction from galaxy clusters in X-ray and SZ surveys: A matched-filter approach
• Efficient simulation of discrete galaxy populations and associated radiation fields during the first billion years
• Probing interacting dark sector models with future weak lensing-informed galaxy cluster abundance constraints from SPT-3G and CMB-S4
• Cross Correlation of the Extragalactic Gamma-ray Background with Thermal Sunyaev-Zel'dovich Effect in the Cosmic Microwave Background
• Testing the SZ-based tomographic approach to the thermal history of the universe with pressure-density cross-correlations: Insights from the Magneticum simulation
• Estimates of cluster masses in screened modified gravity
• Constraints on dark matter and astrophysics from tomographic $\gamma$-ray cross-correlations
• Learning the Universe: Cosmological and Astrophysical Parameter Inference with Galaxy Luminosity Functions and Colours
• Multiplicity functions of quasars: Predictions from the MassiveBlackII simulation
• The influence of mergers on the cluster temperature function and cosmological parameters derived from it
• On Escaping a Galaxy Cluster in an Accelerating Universe
• Lensing dispersion of supernova flux: a probe of nonlinear structure growth
• Mapping the Universe in HD
• The CIB-lensing bispectrum: impact on primordial non-Gaussianity and detectability for the Planck mission
• Constraining the non-gravitational scattering of baryons and dark matter with early cosmic structure formation
• Exploring the mass and redshift dependence of the cluster pressure profile with stacks on thermal SZ maps
• The parameter-free Finger-Of-God model and its application to 21cm intensity mapping
• An Eddington ratio-driven origin for the ${\mathrm{L}}_{\mathrm{X}}-{\mathrm{M}}_{\ast }$ relation in quiescent and star forming active galaxies
• Small-scale clumping of dark matter and the mean free path of ionizing photons at $z=6$
• Constraints on galaxy formation from the cosmic-far-infrared-background\,$-$\,optical-imaging cross-correlation using \textit{Herschel} and UNIONS
• Cosmic shear statistics in cosmologies with non-Gaussian initial conditions
• The impact of the halo spin-concentration relation on disc scaling laws
• Cosmological Constraints on the Global Star Formation Law of Galaxies: Insights From Baryon Acoustic Oscillation Intensity Mapping
• The HalfDome Multi-Survey Cosmological Simulations: N-body Simulations
• Galaxy cluster aperture masses are more robust to baryonic effects than 3D halo masses
• Constraining primordial non-Gaussianity with cosmological weak lensing: shear and flexion
• The deconvolved distribution estimator: enhancing reionisation-era CO line-intensity mapping analyses with a cross-correlation analogue for one-point statistics
• CMB Anisotropy Due to Filamentary Gas: Power Spectrum and Cosmological Parameter Bias
• The integrated angular bispectrum
• On the modelling of the excesses of galaxy clusters over high-mass thresholds
• SZ/X-ray scaling relations using X-ray data and Planck Nominal maps
• A Local Universe model for constrained simulations
• X-ray properties of X-CLASS-redMaPPer galaxy cluster sample: The luminosity-temperature relation
• The Planck SZ Cluster Catalog: Expected X-ray Properties
• A general framework to test gravity using galaxy clusters V: A self-consistent pipeline for unbiased constraints of $f(R)$ gravity
• The strongest gravitational lenses: III. The order statistics of the largest Einstein radii
• The Velocity Distribution Function of Galaxy Clusters as a Cosmological Probe
• Reconstruction of the two-dimensional gravitational potential of galaxy clusters from X-ray and Sunyaev-Zel'dovich measurements
• The effect of local universe constraints on halo abundance and clustering
• On the ISW-cluster cross-correlation in future surveys
• 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
• Constraining Ultra-light Axions with Galaxy Cluster Number Counts
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• X-ray cluster cosmology
• Removing Interlopers From Intensity Mapping Probes Of Primordial Non-Gaussianity
• Halo mass function in scale invariant models
• Self-calibrating optical galaxy cluster selection bias using cluster, galaxy, and shear cross-correlations
• A comparison of ${\text{H}}_2$ formation models at high redshift
• Cosmology in the non-linear regime : the small scale miracle
• Multi-wavelength consensus of large-scale linear bias
• Improving Constraints on Fundamental Physics Parameters with the Clustering of Sunyaev-Zeldovich Selected Galaxy Clusters
• A Diffused Background from Axion-like Particles in the Microwave Sky
• Explaining JWST star formation history at $z\sim 17$ by modifying $\Lambda$CDM
• Galaxy clusters as probes for cosmology and dark matter
• A pseudo-spectrum analysis of galaxy-galaxy lensing
• CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation
• The Effects of Dark Matter Annihilation on Cosmic Reionization
• Euclid preparation LXX. Forecasting detection limits for intracluster light in the Euclid Wide Survey
• The importance of the cosmic web and halo substructure for power spectra
• What can we learn from higher multipole power spectra of galaxy distribution in redshift space?
• Constraints on dark energy from the CSST galaxy clusters
• The BINGO project VIII: On the recoverability of the BAO signal on HI intensity mapping simulations
• Dark matter halo assembly bias: environmental dependence in the non-Markovian excursion set theory
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• Abundance matching tested on small scales with galaxy dynamics
• Toward the low-scatter selection of X-ray clusters: Galaxy cluster detection with eROSITA through cluster outskirts
• A forecast for the detection of the power asymmetry from galaxy surveys
• Keeping It Real: Revisiting a Real-Space Approach to Running Ensembles of Cosmological N-body Simulations
• The Structure of 2MASS Galaxy Clusters
• Primordial density perturbations with running spectral index: impact on non-linear cosmic structures
• Improvements in the X-ray luminosity function and constraints on the Cosmological parameters from X-ray luminous clusters
• Small-scale Effects of Thermal Inflation on Halo Abundance at High-$z$, Galaxy Substructure Abundance and 21-cm Power Spectrum
• Forecasting cosmological parameter constraints using multiple sparsity measurements as tracers of the mass profiles of dark matter haloes
• Toward More Realistic Mass Functions For Ultradense Dark Matter Halos
• asimulation: Domain formation and impact on observables in resolved cosmological simulations of the (a)symmetron
• The environment-dependence of the growth of the most massive objects in the Universe
• Deep learning insights into non-universality in the halo mass function
• Cluster Assembly Times as a Cosmological Test
• Importance of intracluster scattering and relativistic corrections from tSZ effect with Cosmic Infrared Background
• An Analytic Formula for the Supercluster Mass Function
• Higher moments of primordial non-Gaussianity and N-body simulations
• Dynamical cluster masses from photometric surveys
• Reconstructing the Thermal Sunyaev-Zel'dovich Effect in 3D
• Tidal shear and the consistency of microscopic Lagrangian halo approaches
• AGN lifetimes in UV-selected galaxies: a clue to supermassive black hole-host galaxy coevolution
• A Multi-messenger view of Cosmic Dawn: Conquering the Final Frontier
• Searching for velocity-dependent dark matter annihilation signals from extragalactic halos
• Trial by FIRE: Probing the dark matter density profile of dwarf galaxies with GraphNPE
• Constraining the Neutrino Mass with the Drifting Coefficient of the Field Cluster Mass Function
• Evaluating the variance of individual halo properties in constrained cosmological simulations
• 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
• Cosmic star formation history with tomographic cosmic infrared background-galaxy cross-correlation
• Cluster Cosmology with the Velocity Distribution Function of the HeCS-SZ Sample
• Towards Accurate Modeling of Line-Intensity Mapping One-Point Statistics: Including Extended Profiles
• An expanded merger-tree description of cluster evolution
• HD 42659: The only known roAp star in a spectroscopic binary observed with B photometry, TESS and SALT
• The cosmological analysis of X-ray cluster surveys: VI. Inference based on analytically simulated observable diagrams
• PITSZI: Probing Intra-cluster medium Turbulence with Sunyaev-Zel'dovich Imaging -- Application to the triple merging cluster MACS J0717.5+3745
• Cosmological constraints from the EFT power spectrum and tree-level bispectrum of 21cm intensity maps
• Cosmology and Astrophysics with the Diffuse eRASS1 X-ray Angular Power Spectrum
• The powerful lens galaxy cluster PLCK G287.0+32.9 (${\theta }_E\sim 43^{\prime \prime }$)
• The Diffusion Coefficient of the Splashback Mass Function as a Probe of Cosmology
• Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Resolving the Hot and Ionized Universe through the Sunyaev-Zeldovich effect
• Universality of the halo mass function in screened gravity theories
• Mass bias and cosmological constraints from Planck cluster clustering
• Forecasts for Warm Dark Matter from Photometric Galaxy Surveys
• Sensitivity of the Global 21-cm Signal to Dark Matter-Baryon Scattering
• Environmental effects on halo abundance and weak lensing peak statistics toward large underdense regions
• Great Balls of FIRE IV. The contribution of massive star clusters to the astrophysical population of merging binary black holes
• A Machine Learning Approach to Enhancing eROSITA Observations
• Galaxy formation from a timescale perspective
• Metal distribution in the ICM - a comprehensive numerical study of twelve galaxy clusters
• Bayesian recalibration of Planck galaxy cluster scaling relations including relativistic Sunyaev-Zel'dovich corrections
• The information content of Cosmic Infrared Background anisotropies
• Baryon effects on the dark matter halos constrained from strong gravitational lensing
• Bimodal Formation Time Distribution for Infall Dark Matter Halos
• Cosmic Variance and the Inhomogeneous UV Luminosity Function of Galaxies During Reionization
• Weak gravitational lensing as a probe of physical properties of substructures in dark matter halos
• AMICO galaxy clusters in KiDS-1000: cosmological constraints and mass calibration from counts and weak lensing
• Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
• Modelling the selection of galaxy groups with end to end simulations
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• The Three Hundred Project hydrodynamical simulations: Hydrodynamical weak-lensing cluster mass biases and richnesses using different hydro models
• A Galaxy-Halo Model for Multiple Cosmological Tracers
• Learning the Universe: Learning to Optimize Cosmic Initial Conditions with Non-Differentiable Structure Formation Models
• CGM cloud sizes from refractive FRB scattering
• Bias-Limited Extraction of Cosmological Parameters
• Doppler boosted dust emission and CIB-galaxy cross-correlations: a new probe of cosmology and astrophysics
• AMICO galaxy clusters in KiDS-DR3: constraints on $\Lambda$CDM from extreme value statistics
• The strongest gravitational lenses: IV. The order statistics of the largest Einstein radii with cluster mergers
• Shedding light on the star formation rate-halo accretion rate connection and halo quenching mechanism via DECODE, the Discrete statistical sEmi-empiriCal mODEl
• Leveraging cross-correlations and linear covariance-based filtering for line-intensity map reconstructions at linear scales
• Mass accretion rates and multi-scale halo environment in cold and warm dark matter cosmologies
• Stacked phase-space density of galaxies around massive clusters: Comparison of dynamical and lensing masses
• Scaling of the 1-halo terms with bias
• Massive Black Hole Mergers
• Mass assembly history of dark matter halos in the light of $H_0$ tension
• Machine Learning and Structure Formation in Modified Gravity
• Frequency-Domain Distribution of Astrophysical Gravitational-Wave Backgrounds
• Voids and Halos in Voids statistics as a probe of the Expansion History of the Universe
• Accurate halo mass functions from the simplest excursion set theory
• Gravitational wave background from primordial black holes in globular clusters
• An Empirical Mass Function Distribution
• COMAP Pathfinder -- Season 2 results III. Implications for cosmic molecular gas content at "Cosmic Half-past Eleven"
• Constraints on the Neutrino Mass from SZ Surveys
• Evolution of the Deterministic Collapse Barrier of the Field Clusters as a Probe of Cosmology
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Future Radio Continuum Cosmology Clustering Surveys
• Galaxy Assembly and Evolution in the P-Millennium simulation: galaxy clustering
• Inferring Host Dark Matter Halo Masses of Individual Galaxies from Neighboring Galaxy Counts
• Cosmological constraints from Sunyaev-Zeldovich cluster counts: an approach to account for missing redshifts
• Simulations of cm-wavelength Sunyaev-Zel'dovich galaxy cluster and point source blind sky surveys and predictions for the RT32/OCRA-f and the Hevelius 100-m radio telescope
• BASILISK II. Improved Constraints on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Mean maps for cosmic web structures in cosmological initial conditions
• Measuring the scatter of the mass-richness relation in galaxy clusters in photometric imaging surveys by means of their correlation function
• The Cosmological analysis of X-ray cluster surveys VII. Bypassing scaling relations with Lagrangian Deep Learning and Simulation-based inference
• SLICE: SPT-CL J0546-5345 -- A prominent strong-lensing cluster at $z=1.07$
• CHEX-MATE: The Impact of Triaxiality and Orientation on Planck SZ Cluster Selection and Weak Lensing Mass Measurements
• Disentangling the Halo: Joint Model for Measurements of the Kinetic Sunyaev-Zeldovich Effect and Galaxy-Galaxy Lensing
• Structure Formation with Warm White Noise: Effects of Finite Number Density and Velocity Dispersion in Particle and Wave Dark Matter
• Towards a multi-tracer neutrino mass measurement with line-intensity mapping
• Strong gravitational lensing with upcoming wide-field radio surveys
• On the Abundance of Extreme Voids II: A Survey of Void Mass Functions
• Improving Galaxy Cluster Selection with the Outskirt Stellar Mass of Galaxies
• The imprints of galaxy cluster internal dynamics on the Sunyaev-Zeldovich effect
• Convergence of halo statistics: code comparison between Rockstar and CompaSO using scale-free simulations
• The impact of halo concentration on the Sunyaev Zel'dovich effect signal from massive galaxy clusters
• Constraining the Star Formation Rate using Joint CIB Continuum and [CII] Intensity Mapping
• Cosmic Census: Relative Distributions of Dark Matter, Galaxies and Diffuse Gas
• A Stochastic Theory of the Hierarchical Clustering III. The Non-universality and Non-stationarity of the Halo Mass Function
• The Splashback Mass Function in the Presence of Massive Neutrinos
• Three-Dimensional Reconstruction of Weak Lensing Mass Maps with a Sparsity Prior. I. Cluster Detection
• The mass and galaxy distribution around SZ-selected clusters
• Properties beyond mass for unresolved haloes across redshift and cosmology using correlations with local halo environment
• The Cosmic Mach Number as an Environment Measure for the Underlying Dark Matter Density Field
• Bounds on galaxy stochasticity from halo occupation distribution modeling
• Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
• Forecasting the $Y_{500}-M_{500}$ scaling relation from the NIKA2 SZ Large Program
• Optical Confirmation of X-ray selected Galaxy clusters from the Swift AGN and Cluster survey with MDM and Pan-STARRS Data (Paper III)
• XMM-Newton follow-up of a sample of apparent low surface brightness galaxy groups detected in the ROSAT All-Sky Survey
• The impact of baryons on the sparsity of simulated galaxy clusters from The Three Hundred Project
• Primordial black holes in Randall-Sundrum: Cosmological signatures
• ECHO21: a tool for modelling global 21-cm signal from dark ages to reionization
• A Multifrequency approach of the cosmological parameter estimation in presence of extragalactic point sources
• The SRG/eROSITA all-sky survey: Constraints on Ultra-light Axion Dark Matter through Galaxy Cluster Number Counts
• Euclid preparation: TBD. Cosmic Dawn Survey: evolution of the galaxy stellar mass function across 0.2<z<6.5 measured over 10 square degrees
• A first look at quasar-galaxy clustering at $z\simeq 7.3$
• An Order Statistics Approach to the Halo Model for Galaxies
• Constraints on the galaxy formation models during epoch of reionization with high redshift observations
• The uncommon intracluster medium features of the first massive clusters selected independently of their baryon content
• Accelerating HI density predictions during the Epoch of Reionization using a GPR-based emulator on N-body simulations
• Aemulus $\nu$: Precision halo mass functions in w$\nu$CDM cosmologies
• Confirmation of NIKA2 investigation of the Sunyaev-Zel'dovich effect by using synthetic clusters of galaxies
• Galaxies and Cluster of Galaxies as Peak Patches of the Density Field
• The informativeness of [C II] line-intensity mapping as a probe of the H I content and metallicity of galaxies at the end of reionization
• Estimators for the cross-pairwise kSZ effect: forecasts for the dark energy and modified gravity parameters with Simons Observatory and CMB-S4
• The Pseudo Evolution of Galaxy-Cluster Masses and Its Connection to Mass Density Profile
• Constraining the halo-ISM connection through multi-transition carbon monoxide line-intensity mapping
• Direct correlation of line intensity mapping and CMB lensing from evolution along the lightcone
• Overdense fireworks in GOODS-N: Unveiling a record number of massive dusty star forming galaxies at z$\sim$5.2 with the N2CLS
• A halo model approach to describe clustering and emission of the two main star forming galaxy populations for Cosmic Infrared Background studies
• HIKER: a halo-finding method based on kernel-shift algorithm
• Primordial Black Hole Mergers as Probes of Dark Matter in Galactic Center
• Removal of interloper contamination to line-intensity maps using correlations with ancillary tracers of the large-scale structure
• ZTF SN Ia DR2: Impact of the galaxy cluster environment on the stretch distribution of Type Ia supernovae
• Galaxy cluster count cosmology with simulation-based inference
• EDGES of the dark forest: A new absorption window into the composite dark matter and large scale structure
• Dark energy, spatial curvature, and star formation efficiency from JWST photometric and spectroscopic high-redshift galaxies
• Sunyaev-Zel'dovich galaxy clusters number counts : consequences of cluster scaling laws evolution
• Forecasts for cosmological measurements based on the angular power spectra of AGN and clusters of galaxies in the SRG/eROSITA all-sky survey
• Cluster science from ROSAT to eROSITA
• Mass function and assembly of dark halos: an approach to inventory isolated overdense regions in random fields
• SZ power spectrum and cluster numbers from an extended merger-tree model
• On the Outskirts of Dark Matter Haloes
• VST ATLAS Galaxy Cluster Catalogue I: cluster detection and mass calibration
• AMI-CL J0300+2613: a Galactic anomalous-microwave-emission ring masquerading as a galaxy cluster
• Cosmic magnification on high-redshift submillimeter galaxies
• Systematic effects on the upcoming NIKA2 LPSZ scaling relation
• Constraints on the normal branch of DGP gravity from SPT galaxy clusters with DES and HST weak-lensing mass calibration and from Planck PR4 CMB anisotropies
• X-ray flux -- mass relation for $z\gtrsim 0.7$ galaxy clusters
• STRAWBERRY: Finding haloes in the gravitational potential
• On the first crossing distributions in fractional Brownian motion and the mass function of dark matter haloes
• Effects of dynamical friction on perturbations for evolving dark energy
• Momentum transfer models of interacting dark energy
• A Hydro-Particle-Mesh Code for Efficient and Rapid Simulations of the Intracluster Medium
• Exploiting Non-linear Scales in Galaxy-Galaxy Lensing and Galaxy Clustering: A Forecast for the Dark Energy Survey
• Strong Conformity and Assembly Bias: Towards a Physical Understanding of the Galaxy-Halo Connection in SDSS Clusters
• Selecting Clusters and Protoclusters via Stellar Mass Density: II. Application to HSC-SSP Observations
• Extended Hernquist-Springel formalism for cosmic star formation
• Adaptive friends-of-friends algorithm for identifying gravitationally bound cosmological structures
• HSC-XXL : Baryon budget of the 136 XXL Groups and Clusters
• Cosmic backgrounds from the radio to the far-infrared: recent results and perspectives from cosmological and astrophysical surveys
• The Swift AGN and Cluster Survey. II. Cluster Confirmation with SDSS Data
• The SRG/eROSITA All-Sky Survey. Detection of shock-heated gas beyond the halo boundary into the accretion region
• The Three Hundred : contrasting clusters galaxy density in hydrodynamical and dark matter simulations
• On the virialization threshold for halo mass functions
• The invariance of group occupation across the cosmic web
• The Extended Zel'dovich Mass Functions of Clusters and Isolated Clusters in the Presence of Primordial Non-Gaussianity
• A semi-analytic estimate for the effective sound speed counterterm in the EFTofLSS
• DUCA: Dynamic Universe Cosmological Analysis. I. The halo mass function in dynamical dark energy cosmologies
• Probing baryonic feedback with fast radio bursts: joint analyses with cosmic shear and galaxy clustering
• Euclid preparation. L. Calibration of the linear halo bias in $\Lambda (\nu )$CDM cosmologies
• Weighing Cosmic Structures with Clusters of Galaxies and the Intergalactic Medium
• An X-ray-Emitting Proto-Cluster at $z\approx 5.7$ Reveals Rapid Structure Growth
• The non-thermal secondary CMB anisotropies from a cosmic distribution of radio galaxy lobes
• Identification of low redshift groups and clusters of galaxies in the X-CLASS survey and the X-ray luminosity-temperature relation
• Excursion Sets with a "Perfect" Collapse Model
• Dissecting the Thermal SZ Power Spectrum by Halo Mass and Redshift in SPT-SZ Data and Simulations
• The multi-dimensional halo assembly bias can be preserved when enhancing halo properties with HALOSCOPE
• Non-linear structure formation in the "Running FLRW" cosmological model
• Angular correlation functions of bright Lyman-break galaxies at $3\lesssim \mathbf{z}\lesssim 5$
• The pairwise and cross-pairwise y-type polarised kinetic Sunyaev Zeldovich effect from transverse velocity of galaxy clusters
• Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future
• Path integral approach for merger rates of dark matter haloes
• A hierarchical clustering method for quantifying satellite abundance
• Optimization and Quality Assessment of Baryon Pasting for Intracluster Gas using the Borg Cube Simulation
• On the universality of the halo mass function beyond $\Lambda$CDM cosmology
• Neutrino Constrains to the Diffuse Gamma-Ray Emission from Accretion Shocks
• Impact of a Rapid Diluted Energy Density on the halo mass function
• Simulation budgeting for hybrid effective field theories
• Testing the key role of the stellar mass-halo mass relation in galaxy merger rates and morphologies via DECODE, a novel Discrete statistical sEmi-empiriCal mODEl
• Searching for dark matter isocurvature initial conditions with N-body Simulations
• Revisiting secondary CMB distortions due to kinetic Sunyaev-Zel'dovich effect from quasar bubbles before reionization
• Biased Domain Walls and the Origin of Early Massive Structures
• The halo finding problem revisited: a deep revision of the ASOHF code
• Segmenting proto-halos with vision transformers
• Detecting the $\pi$-axiverse through parametric resonance
• Mass functions from the excursion set model
• Lagrangian Perturbation Theory for Biased Tracers: Significance of the Number Conservation
• Challenges of standard halo models in constraining galaxy properties from CIB anisotropies
• Built-in precision: Improving cluster cosmology through the self-calibration of a galaxy cluster sample
• An Anti-halo Void Catalogue of the Local Super-Volume
• Catalogs of optically-selected clusters and photometric luminous red galaxies from the Hyper Suprime-Cam Subaru Strategic Program final year dataset
• Sahyadri: A simulation suite for the cosmology dependence of the Cosmic Web
• The SRG/eROSITA all-sky survey: The morphologies of clusters of galaxies: II. The intrinsic distributions of morphological parameters
• Slicing cluster mass functions with a Bayesian razor
• The Hydrostatic Mass Bias and the ${\sigma }_8$ Tension: A Multi-Probe Forecast for Stage-IV/V Surveys
• On Weak Lensing Response Functions
• AMICO galaxy clusters in KiDS-1000: Splashback radius from weak lensing and cluster-galaxy correlation function
• Spectroscopic galaxy redshifts in the Peanut cluster -- a massive nearly head-on cluster merger shortly after pericenter passage
• Mock Catalogs of Strongly Lensed Gravitational Waves via A Halo Model Approach with Ground-based Detectors
• Cluster gravitational redshifts: uncertainties and survey requirements
• Improving cosmological covariance matrices with machine learning
• Multi-scale weak lensing detection of galaxy clusters with source redshift tomography
• Bound or blown: the fate of hot gas in galaxy groups
• Constraints on the dark energy dipole from large-scale structures
• The Splashback Mass Function of Galaxy Clusters from Photometric Data
• Impact of the calibration of the Halo Mass Function on galaxy cluster number count cosmology
• Universality of the halo mass function in modified gravity cosmologies
• Fisher matrix for multiple tracers: the information in the cross-spectra
• Streaming Velocity Effects on the Post-reionization 21 cm Baryon Acoustic Oscillation Signal
• Self-similarity of the mass distribution in rich galaxy clusters up z~1 tracked with weak lensing
• Cosmology with galaxy clusters: impact of theoretical and observational systematic uncertainties
• Towards a universal model for the density profiles of dark matter haloes
• Combining Planck and SPT cluster catalogs: cosmological analysis and impact on Planck scaling relation calibration
• Cross-correlations between mm-wave line-intensity mapping and weak lensing surveys: preliminary consideration of long-term prospects
• Cosmic velocity, density and halo mass function: Insights from deep learning
• Compact star forming galaxies as the progenitors of compact quiescent galaxies: clustering result
• DUCA: Dynamic Universe Cosmological Analysis. II. The impact of clustering dark energy on the halo mass function
• A revisited Correction to the Halo Mass Function for local-type Primordial non-Gaussianity