Fingers of God

Abstract

Very long wavelength universal gravitational waves cannot now produce in clusters of galaxies velocity dispersions greater than that which these systems would possess if they were expanding with the Universe, if the Universe is not younger than $10^{10}$ yr and Hubble's constant is not less than 50 km/sec/ Mpc. A diagram shows that actual velocity dispersions are significantly greater than this limit.

Published long before the advent of large-scale redshift surveys, as "A Critique of Rees's Theory of Primordial Gravitational Radiation", this paper includes the first presentation of what has come to be known as the fingers-of-god effect. The effect is mentioned several hundred times in arXive papers, rarely with a wrong attribution, usually with none at all

Cited by in corpus (345)

• Large-Scale Galaxy Bias
• The 6dF Galaxy Survey: z \approx 0 measurement of the growth rate and sigma_8
• Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift Space
• Testing General Relativity in Cosmology
• Cosmological Parameters from the BOSS Galaxy Power Spectrum
• Baryon Acoustic Oscillations in 2D: Modeling Redshift-space Power Spectrum from Perturbation Theory
• Interpreting large-scale redshift-space distortion measurements
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the Quasar Sample in configuration space between redshift 0.8 and 2.2
• Cosmology from the Chinese Space Station Optical Survey (CSS-OS)
• Detecting filamentary pattern in the cosmic web: a catalogue of filaments for the SDSS
• Testing cosmological structure formation using redshift-space distortions
• The Clustering of Galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS): measuring growth rate and geometry with anisotropic clustering
• DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars
• Nonlinear perturbation theory with halo bias and redshift-space distortions via the Lagrangian picture
• Clustering of Low-Redshift (z <= 2.2) Quasars from the Sloan Digital Sky Survey
• The Subaru FMOS galaxy redshift survey (FastSound). IV. New constraint on gravity theory from redshift space distortions at $z\sim 1.4$
• Flux- and volume-limited groups/clusters for the SDSS galaxies: catalogues and mass estimation
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Measuring D_A and H at z=0.57 from the Baryon Acoustic Peak in the Data Release 9 Spectroscopic Galaxy Sample
• Non-linear perturbation theory extension of the Boltzmann code CLASS
• A 2.5% measurement of the growth rate from small-scale redshift space clustering of SDSS-III CMASS galaxies
• Galaxy evolution in the metric of the Cosmic Web
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): The growth of structures at $0.5<z<1.2$ from redshift-space distortions in the clustering of the PDR-2 final sample
• Galaxy spin alignment in filaments and sheets: observational evidence
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum between redshift 0.6 and 1.1
• Forecasting Cosmological Constraints from Redshift Surveys
• Blinded challenge for precision cosmology with large-scale structure: results from effective field theory for the redshift-space galaxy power spectrum
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the full shape of the clustering wedges in the data release 10 and 11 galaxy samples
• Cosmic flow from 2MASS redshift survey: The origin of CMB dipole and implications for LCDM cosmology
• Cosmological Parameters and Neutrino Masses from the Final Planck and Full-Shape BOSS Data
• The darkness that shaped the void: dark energy and cosmic voids
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: structure growth rate measurement from the anisotropic quasar power spectrum in the redshift range $0.8<z<2.2$
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Growth rate of structure measurement from anisotropic clustering analysis in configuration space between redshift 0.6 and 1.1 for the Emission Line Galaxy sample
• Nonlinear Perturbation Theory Integrated with Nonlocal Bias, Redshift-space Distortions, and Primordial Non-Gaussianity
• Merging groups and clusters of galaxies from the SDSS data. The catalogue of groups and potentially merging systems
• Infrared Resummation for Biased Tracers in Redshift Space
• Growth of Cosmic Structure: Probing Dark Energy Beyond Expansion
• Constraining Primordial non-Gaussianity with Bispectrum and Power Spectum from Upcoming Optical and Radio Surveys
• Consistent Modeling of Velocity Statistics and Redshift-Space Distortions in One-Loop Perturbation Theory
• Clustering of luminous red galaxies I: large scale redshift space distortions
• The galaxy power spectrum take on spatial curvature and cosmic concordance
• The Aemulus Project III: Emulation of the Galaxy Correlation Function
• Redshift space distortions in f(R) gravity
• Redshift-Space Clustering of SDSS Galaxies --- Luminosity Dependence, Halo Occupation Distribution, and Velocity Bias
• Measuring neutrino masses with large-scale structure: Euclid forecast with controlled theoretical error
• Cosmological information in the redshift-space bispectrum
• Redshift-weighted constraints on primordial non-Gaussianity from the clustering of the eBOSS DR14 quasars in Fourier space
• Modelling redshift space distortions in hierarchical cosmologies
• Velocity Bias from the Small Scale Clustering of SDSS-III BOSS Galaxies
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions
• Redshift space correlations and scale-dependent stochastic biasing of density peaks
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: the low redshift sample
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological constraints from the full shape of the clustering wedges
• Effects of Massive Neutrinos on the Large-Scale Structure of the Universe
• The Galaxy Power Spectrum and Bispectrum in Redshift Space
• Line-Intensity Mapping: Theory Review
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Luminosity and Color Dependence and Redshift Evolution
• Detection of Cosmological 21 cm Emission with the Canadian Hydrogen Intensity Mapping Experiment
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: exploring the Halo Occupation Distribution model for Emission Line Galaxies
• Rapid modelling of the redshift-space power spectrum multipoles for a masked density field
• Precision analysis of the redshift-space galaxy bispectrum
• Cosmology in the era of Euclid and the Square Kilometre Array
• Galaxy bispectrum, primordial non-Gaussianity and redshift space distortions
• UNIT project: Universe $N$-body simulations for the Investigation of Theoretical models from galaxy surveys
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: weighing the neutrino mass using the galaxy power spectrum of the CMASS sample
• Unmasking the Masked Universe: the 2M++ catalogue through Bayesian eyes
• Precision cosmology with voids in the final BOSS data
• Automatic unsupervised classification of all SDSS/DR7 galaxy spectra
• Cosmology with the Galaxy Bispectrum Multipoles: Optimal Estimation and Application to BOSS Data
• Complementarity of Weak Lensing and Peculiar Velocity Measurements in Testing General Relativity
• Ultra-light axions and the $S_8$ tension: joint constraints from the cosmic microwave background and galaxy clustering
• Galaxy Bispectrum from Massive Spinning Particles
• FAST-PT II: an algorithm to calculate convolution integrals of general tensor quantities in cosmological perturbation theory
• Testing the theory of gravity with DESI: estimators, predictions and simulation requirements
• Mapping Growth and Gravity with Robust Redshift Space Distortions
• Systematic Effects on Determination of the Growth Factor from Redshift-space Distortions
• The DEEP2 Galaxy Redshift Survey: Clustering Dependence on Galaxy Stellar Mass and Star Formation Rate at z~1
• Isolating relativistic effects in large-scale structure
• Cosmological constraints from the power spectrum of eBOSS emission line galaxies
• Galaxy and Mass Assembly (GAMA): Projected Galaxy Clustering
• Three-Point Correlation Functions of SDSS Galaxies: Luminosity and Color Dependence in Redshift and Projected Space
• Friends-of-friends galaxy group finder with membership refinement. Application to the local Universe
• Towards a measurement of the spectral runnings
• Euclid: Forecasts from redshift-space distortions and the Alcock-Paczynski test with cosmic voids
• Where are the Luminous Red Galaxies (LRGs)? Using correlation measurements and lensing to relate LRGs to dark matter halos
• Precision modeling of redshift-space distortions from multi-point propagator expansion
• PRIMUS: Galaxy Clustering as a Function of Luminosity and Color at 0.2<z<1
• Non-Gaussian Minkowski functionals & extrema counts in redshift space
• Tests of redshift-space distortions models in configuration space for the analysis of the BOSS final data release
• Modelling non-linear redshift-space distortions in the galaxy clustering pattern: systematic errors on the growth rate parameter
• Distribution function approach to redshift space distortions. Part II: N-body simulations
• Galaxy Infall Kinematics as a Test of Modified Gravity
• Optimizing large-scale structure data analysis with the theoretical error likelihood
• How well does the Friends-of-Friends algorithm recover group properties from galaxy catalogs limited in both distance and luminosity?
• Cosmological constraints without fingers of God
• Galaxy redshift-space bispectrum: the Importance of Being Anisotropic
• The matter distribution in the local Universe as derived from galaxy groups in SDSS DR12 and 2MRS
• Generating Log-normal Mock Catalog of Galaxies in Redshift Space
• Characterising filaments in the SDSS volume from the galaxy distribution
• The Impact of Foregrounds on Redshift Space Distortion Measurements With the Highly-Redshifted 21 cm Line
• Charting nearby dust clouds using Gaia data only
• 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 $0.1$
• Testing Gravity Using Large-Scale Redshift-Space Distortions
• Distribution function approach to redshift space distortions, Part III: halos and galaxies
• The Redshift-Space Cluster-Galaxy Cross-Correlation Function: I. Modeling Galaxy Infall onto Millennium Simulation Clusters and SDSS Groups
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for the Quasar Sample
• Redshift-space distortions with split densities
• Accurate and Efficient Halo-based Galaxy Clustering Modelling with Simulations
• Banana Split: Testing the Dark Energy Consistency with Geometry and Growth
• Modeling the large-scale redshift-space 3-point correlation function of galaxies
• A Practical Computational Method for the Anisotropic Redshift-Space 3-Point Correlation Function
• Accurate emulator for the redshift-space power spectrum of dark matter halos and its application to galaxy power spectrum
• Peculiar Velocity Decomposition, Redshift Space Distortion and Velocity Reconstruction in Redshift Surveys. II. Dark Matter Velocity Statistics
• Forecasts on Primordial non-Gaussianity from 21 cm Intensity Mapping experiments
• Peculiar velocities in redshift space: formalism, N-body simulations and perturbation theory
• Scale-Dependent Galaxy Bias from Massive Particles with Spin during Inflation
• Biases from neutrino bias: to worry or not to worry?
• Dark matter and halo bispectrum in redshift space: theory and applications
• Distribution function approach to redshift space distortions. Part V: perturbation theory applied to dark matter halos
• Nonlinear Biasing and Redshift-Space Distortions in Lagrangian Resummation Theory and N-body Simulations
• SPT-GMOS: A Gemini/GMOS-South Spectroscopic Survey of Galaxy Clusters in the SPT-SZ Survey
• Cosmological Constraint on ${\Omega }_m$ and ${\sigma }_8$ from Cluster Abundances using the $GalWCat19$ Optical-Spectroscopic SDSS Catalog
• Clustering of luminous red galaxies II: small scale redshift space distortions
• Clustering and redshift-space distortions in interacting dark energy cosmologies
• The VLT LBG Redshift Survey I: Clustering and Dynamics of ~1000 Galaxies at z~3
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: application to the SDSS-III BOSS DR12 galaxies
• Matter trispectrum: theoretical modelling and comparison to N-body simulations
• Precision cosmology with redshift-space bispectrum: a perturbation theory based model at one-loop order
• LIGER: mock relativistic light-cones from Newtonian simulations
• The impact of galaxy formation on satellite kinematics and redshift-space distortions
• Non-linear Redshift-Space Power Spectra
• Peculiar Velocity Decomposition, Redshift Space Distortion and Velocity Reconstruction in Redshift Surveys - I. The Methodology
• Intrinsic alignments of group and cluster galaxies in photometric surveys
• Baryon Acoustic Oscillation Theory and Modelling Systematics for the DESI 2024 results
• Evolution of Star-forming Galaxies from z = 0.7 to 1.2 with eBOSS Emission-line Galaxies
• The matter power spectrum in redshift space using effective field theory
• Galaxy power spectrum in redshift space: combining perturbation theory with the halo model
• FFT-PT: Reducing the two-loop large-scale structure power spectrum to low-dimensional radial integrals
• Quantifying the Redshift Space Distortion of the Bispectrum I: Primordial Non-Gaussianity
• Filament profiles from WISExSCOS galaxies as probes of the impact of environmental effects
• Large-scale redshift space distortions in modified gravity theories
• Perturbation theory approach for the power spectrum: from dark matter in real space to massive haloes in redshift space
• Alcock-Paczynski cosmological test
• Consistent Modified Gravity Analysis of Anisotropic Galaxy Clustering Using BOSS DR11
• Regarding the Line-of-Sight Baryonic Acoustic Feature in the Sloan Digital Sky Survey and Baryon Oscillation Spectroscopic Survey Luminous Red Galaxy Samples
• Impact of shell crossing and scope of perturbative approaches in real and redshift space
• Morphological Properties of Superclusters of Galaxies
• Improving the modelling of redshift-space distortions - II. A pairwise velocity model covering large and small scales
• Cosmology with clustering anisotropies: disentangling dynamic and geometric distortions in galaxy redshift surveys
• Using galaxy-galaxy weak lensing measurements to correct the Finger-of-God
• Probing the Radio Loud/Quiet AGN dichotomy with quasar clustering
• Edgeworth streaming model for redshift space distortions
• A comparison of cosmological filaments catalogues
• Observational constraints on early dark energy
• The SAMI Galaxy Survey: flipping of the spin-filament alignment correlates most strongly with growth of the bulge
• High-order 3D Voronoi tessellation for identifying Isolated galaxies, Pairs and Triplets
• Simulations of Galileon modified gravity: Clustering statistics in real and redshift space
• Mapping the real space distributions of galaxies in SDSS DR7: I. Two Point Correlation Functions
• Galaxy clustering, CMB and supernova data constraints on $\varphi$CDM model with massive neutrinos
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: Dynamical dark energy
• Interloper bias in future large-scale structure surveys
• The effect of cosmic web filaments on galaxy evolution
• Bayesian group finder based on marked point processes. Method and feasibility study using the 2MRS data set
• Estimating Covariance Matrices for Two- and Three-Point Correlation Function Moments in Arbitrary Survey Geometries
• Redshift-space distortions in massive neutrino and evolving dark energy cosmologies
• Neutrino mass and dark energy constraints from redshift-space distortions
• How to Falsify the GR+LambdaCDM Model with Galaxy Redshift Surveys
• The MOSDEF Survey: Environmental dependence of the gas-phase metallicity of galaxies at $1.4\le z\le 2.6$
• Measurement of marked correlation functions in SDSS-III Baryon Oscillation Spectroscopic Survey using LOWZ galaxies in Data Release 12
• The VIMOS Public Extragalactic Redshift Survey - Searching for Cosmic Voids
• Investigating the degeneracy between modified gravity and massive neutrinos with redshift-space distortions
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski test and volume effect: galaxy two-point correlation function
• Cosmology inference at the field level from biased tracers in redshift-space
• Cosmological information content in redshift-space power spectrum of SDSS-like galaxies in the quasi-nonlinear regime up to $k=0.3h$Mpc${}^{-1}$
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Never mind the gaps: comparing techniques to restore homogeneous sky coverage
• Multipole expansion for HI intensity mapping experiments: simulations and modelling
• Galaxy clusters in simulations of the local Universe: a matter of constraints
• Impacts of satellite galaxies on the redshift-space distortions
• On the streaming model for redshift-space distortions
• Nonlinear reconstruction of redshift space distortions
• A Radial Measurement of the Galaxy Tidal Alignment Magnitude with BOSS Data
• A direct detection of neutral hydrogen intensity mapping on Mpc scales at $z\approx 0.32$ and $z\approx 0.44$
• Modelling redshift-space distortion in the post-reionization $\mathrm{HI}$ 21-cm power spectrum
• Study on the mapping of dark matter clustering from real space to redshift space
• Imprints of local lightcone projection effects on the galaxy bispectrum. II
• Measuring Coherent Motions in the Universe
• Tidal alignments as a contaminant of the galaxy bispectrum
• Cosmological constraints from the power spectrum and bispectrum of 21cm intensity maps
• Clustering and redshift-space distortions in modified gravity models with massive neutrinos
• Real- and redshift-space halo clustering in $f(R)$ cosmologies
• GalWeight Application: A publicly-available catalog of dynamical parameters of 1,800 galaxy clusters from SDSS-DR13, ($GalWCat19$)
• Using peculiar velocity surveys to constrain the growth rate of structure with the wide-angle effect
• SDSS-IV MaNGA: Signatures of halo assembly in kinematically misaligned galaxies
• Connected structure in the 2dFGRS
• The HI intensity mapping bispectrum including observational effects
• Quantifying the Redshift Space Distortion of the Bispectrum II: Induced Non-Gaussianity at Second Order Perturbation
• The BINGO Project VI: HI Halo Occupation Distribution and Mock Building
• Power spectrum multipole expansion for HI intensity mapping experiments: unbiased parameter estimation
• Probing primordial non-Gaussianity with the power spectrum and bispectrum of future 21cm intensity maps
• Effects of Linear Redshift Space Distortions and Perturbation Theory on BAOs: A 3D Spherical Analysis
• On the Systematic Errors of Cosmological-Scale Gravity Tests using Redshift Space Distortion: Non-linear Effects and the Halo Bias
• Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model - I. Magnitude counts, redshift distribution, colour bimodality, and galaxy clustering
• Cosmic Velocity Field Reconstruction Using AI
• A detection of baryon acoustic oscillations from the distribution of galaxy clusters
• Impact of bias and redshift-space modelling for the halo power spectrum: Testing the effective field theory of large-scale structure
• An Accurate Fitting Function For Scale-dependent Growth Rate in Hu-Sawicki $f(R)$ Gravity
• Unbiased Cosmological Parameter Estimation from Emission Line Surveys with Interlopers
• Bayesian cosmic density field inference from redshift space dark matter maps
• The Effects of Galaxy Assembly Bias on the Inference of Growth Rate from Redshift-Space Distortions
• The Anisotropic Line Correlation Function as a Probe of Anisotropies in Galaxy Surveys
• 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
• Cosmological Vlasov-Poisson equations for dark matter: Recent developments and connections to selected plasma problems
• Blind Observers of the Sky
• Non-Linear Matter Power Spectrum Modeling in Interacting Dark Energy Cosmologies
• (DarkAI) Mapping the large-scale density field of dark matter using artificial intelligence
• Nonlinear Redshift-Space Distortions in the Harmonic-space Galaxy Power Spectrum
• Likelihood reconstruction method of real-space density and velocity power spectra from a redshift galaxy survey
• Studying large-scale structure probes of modified gravity with COLA
• Modelling the post-reionization neutral hydrogen ($\mathrm{HI}$) 21-cm bispectrum
• Redshift space distortions of the {\rm HI} 21-cm intensity mapping signal due to the internal motions within galaxies
• Decomposition of Spectra from Redshift Distortion Maps
• Radiative Transfer Distortions of Lyman-$\alpha$ Emitters: a New Fingers-of-God Damping in the Clustering in Redshift Space
• Beta-Skeleton Analysis of the Cosmic Web
• The Clustering Of Galaxies Around Radio-Loud AGNs
• Compressed baryon acoustic oscillation analysis is robust to modified-gravity models
• Tight $H_0$ constraint from galaxy redshfit surveys: combining baryon acoustic osillation measurements and Alcock-Paczynski test
• Exploring the Redshift-Space Peculiar Velocity Field and its Power Spectrum
• Redshift Space Distortion of 21cm line at 1<z<5 with Cosmological Hydrodynamic Simulations
• Cosmological Information from the Small-scale Redshift Space Distortions
• Redshift-space correlation functions in large galaxy cluster surveys
• Reducing the Variance of Redshift Space Distortion Measurements from Mock Galaxy Catalogues with Different Lines of Sight
• Reconstruction of halo power spectrum from redshift-space galaxy distribution: cylinder-grouping method and halo exclusion effect
• Bayesian redshift-space distortions correction from galaxy redshift surveys
• Cosmological Tests using Redshift Space Clustering in BOSS DR11
• The Stellar Kinematics of Void Dwarf Galaxies Using KCWI
• The Integrated Bispectrum in Modified Gravity Theories
• Hybrid modeling of redshift space distortions
• The redshift dependence of Alcock-Paczynski effect: cosmological constraints from the current and next generation observations
• Grid-based calculations of redshift-space matter fluctuations from perturbation theory: UV sensitivity and convergence at the field level
• Correlated orientations of the axes of large quasar groups on Gpc scales
• Search and analysis of giant radio galaxies with associated nuclei (SAGAN) IV. Interplay with the Supercluster environment
• Simulating the Anisotropic Clustering of Luminous Red Galaxies with Subhalos: A Direct Confrontation with Observation and Cosmological Implications
• Galaxy Clustering in 3D and Modified Gravity Theories
• AMICO galaxy clusters in KiDS-DR3: Cosmological constraints from angular power spectrum and correlation function
• Probing gravity with redshift-space distortions: effects of tracer bias and sample selection
• Fingers-of-God effect of infalling satellite galaxies
• Cornering Extended Starobinsky Inflation with CMB and SKA
• The Voronoi tessellation method in astronomy
• Ellipsoidal collapse and the redshift space probability distribution function of dark matter
• Consistency Relations in Effective Field Theory
• The $n$-point streaming model: how velocities shape correlation functions in redshift space
• Ensemble Average of Three-Dimensional Minkowski Tensors of a Gaussian Random Field in Redshift Space
• Anisotropic Extinction Distortion of the Galaxy Correlation Function
• Higher multipoles of the galaxy bispectrum in redshift space
• Constraining Halo Occupation Distribution and Cosmic Growth Rate using Multipole Power Spectrum
• Intrinsic Alignment as an RSD Contaminant in the DESI Survey
• Dissecting a miniature universe: A multi-wavelength view of galaxy quenching in the Shapley supercluster
• Fisher matrix for multiple tracers: model independent constraints on the redshift distortion parameter
• Unexpected dancing partners: Tracing the coherence between the spin and motion of dark matter halos
• Validating the methodology for constraining the linear growth rate from clustering anisotropies
• Constraining Cosmological Parameters using the Cluster Mass-Richness Relation
• Neural network reconstruction of density and velocity fields from the 2MASS Redshift Survey
• Minkowski Tensors in Redshift Space -- Beyond the Plane Parallel Approximation
• An Observed Transition of Galaxy Spins on the Void Surfaces
• Using the Modified Nearest Neighbor Method to Correct Fiber-collision Effects on Galaxy Clustering
• Exploring neutrino interactions in light of present and upcoming galaxy surveys
• Subtracting the kinetic Sunyaev-Zeldovich effect from the cosmic microwave background with surveys of large-scale structure
• Quantifying the redshift space distortion of the bispectrum III : Detection prospects of the multipole moments
• Using the Mark Weighted Correlation Functions to Improve the Constraints on Cosmological Parameters
• Fast generation of mock galaxy catalogues with COLA
• Correlation functions in 2D and 3D as descriptors of the cosmic web
• The effects of peculiar velocities on the morphological properties of large-scale structure
• The two-loop power spectrum in redshift space
• Cosmological constraints from the redshift dependence of the volume effect using the galaxy 2-point correlation function across the line-of-sight
• GEO-FPT: a model of the galaxy bispectrum at mildly non-linear scales
• Redshift-space equal-time angular-averaged consistency relations of the gravitational dynamics
• A field-level emulator for modified gravity
• Cosmology with cosmic web environments II. Redshift-space auto and cross power spectra
• The parameter-free Finger-Of-God model and its application to 21cm intensity mapping
• Nonlinear redshift space distortion in halo ellipticity correlations: Analytical model and N-body simulations
• Study on the mapping of halo clustering from real space to redshift space
• Quantification of the multi-streaming effect in Redshift Space Distortion
• Removing Interlopers From Intensity Mapping Probes Of Primordial Non-Gaussianity
• SCONCE: A cosmic web finder for spherical and conic geometries
• Unveiling the Universe with Emerging Cosmological Probes
• A rising tide: Intrinsic alignments since the turn of the millennium
• Probing the Anisotropy and Non-Gaussianity in the Redshift Space through the Conditional Moments of the First Derivative
• Propagation of gravitational waves in an expanding background in the presence of a point mass
• DarkAI: Reconstructing the density, velocity and tidal field of dark matter from a DESI-like bright galaxy sample
• Finding proto-clusters to trace galaxy evolution: I. The finder and its performance
• Constraining Brans-Dicke cosmology with the CSST galaxy clustering spectroscopic survey
• Ray-tracing log-normal simulation for weak gravitational lensing: application to the cross-correlation with galaxies
• Beyond boundaries of redshift surveys: assessing mass fluctuations on "super-survey" scales
• The Arecibo Galaxy Environment Survey (AGES) XI: the expanded Abell 1367 field. Data catalogue and HI census over the surveyed volume
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: Possibility of estimateing the non-linear systematics using fast simulations
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• Detection of pure warm-hot intergalactic medium emission from a $7.2$ Mpc long filament in the Shapley supercluster using X-ray spectroscopy
• Breaking the ${\tau }_{\mathrm{T}}-f$ degeneracy of the kinetic Sunyaev Zel'dovich cosmology in redshift space
• Measuring neutrino mass imprinted on the anisotropic galaxy clustering
• Tracing gaseous filaments connected to galaxy clusters: the case study of Abell 2744
• Cosmology with voids from the Nancy Grace Roman Space Telescope
• A method to extract the redshift distortions beta parameter in configuration space from minimal cosmological assumptions
• Kinematics of MgII Absorbers from the Redshift-space Distortion Around Massive Quiescent Galaxies
• Cluster-counterpart Voids: Void Identification from Galaxy Density Field
• Catalog-level blinding on the bispectrum for DESI-like galaxy surveys
• The Large Scale Structure in the Universe: From Power-Laws to Acoustic Peaks
• Extending evolution mapping to massive neutrinos with COMET
• Towards a multi-tracer neutrino mass measurement with line-intensity mapping
• Self-calibrating BAO measurements in the presence of Small Displacement Interlopers
• The Correlation Function and Detection of Baryon Acoustic Oscillation Peak from the Spectroscopic SDSS GalWCat Galaxy Cluster Catalogue
• Photometric redshift galaxies as tracers of the filamentary network
• Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
• A model of the anisotropic correlation function xi(rp, pi) in redshift space including redshift errors
• Squeezing information from radio surveys to probe the primordial Universe
• Redshift-space galaxy bispectrum in presence of massive neutrinos: A multipole expansion approach for Euclid
• 6x2pt: Forecasting gains from joint weak lensing and galaxy clustering analyses with spectroscopic-photometric galaxy cross-correlations
• On the tomographic cluster clustering as a cosmological probe
• Perturbation theory challenge for cosmological parameters estimation II.: Matter power spectrum in redshift space
• Parameter inference with non-linear galaxy clustering: accounting for theoretical uncertainties
• Reconstruction of real-space linear matter power spectrum from multipoles of BOSS DR12 results
• Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations
• Characterization of the warm--hot intergalactic medium near the Coma cluster through high--resolution spectroscopy of X Comae
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• Toward accurate measurement of property-dependent galaxy clustering I. Comparison of the Vmax method and the "shuffled" method
• Glass-Like Random Catalogues for Two-Point Estimates on the Light Cone
• Impact of Redshift Space Distortion on Persistent Homology of cosmic matter density field
• AVISM: Algorithm for Void Identification in coSMology
• Preliminary clustering properties of the DESI BGS bright targets using DR9 Legacy Imaging Surveys
• The large-scale monopole of the power spectrum in a Euclid-like survey: wide-angle effects, lensing, and the `finger of the observer'
• Improving cosmological constraints via galaxy intrinsic alignment in full-shape analysis
• Transients from Initial Conditions Based on Lagrangian Perturbation Theory in $N$-body Simulations III: The Case of GADGET-2 Code
• Adaptive friends-of-friends algorithm for identifying gravitationally bound cosmological structures
• Modeling and measuring the anisotropic halo 3-point correlation function: a coordinated study
• Lagrangian space remapping and the angular momentum reconstruction from cosmic structures
• Euclid preparation. 3D reconstruction of the cosmic web with simulated Euclid Deep spectroscopic samples
• Investigating the Constraints on Primordial Features with Future Cosmic Microwave Background and Galaxy Surveys
• Tracing Signatures of Modified Gravity in Redshift-Space Galaxy Bispectrum Multipoles: Prospects for Euclid
• Cosmology with the Redshift-Space Galaxy Bispectrum Monopole at One-Loop Order
• From Redshift to Real Space: Combining Linear Theory With Neural Networks
• Cosmological constraints from the density gradient weighted correlation function
• Anisotropic Counts-in-Cells in Redshift Space: A New Route to Cosmological Constraints from Galaxy Surveys
• Limits on the Inferred Hubble Constant Bias from a Local McVittie Gravitational Field
• Probing dark energy using anisotropies in the clustering of post-EoR HI distribution
• Model-agnostic interpretation of 10 billion years of cosmic evolution traced by BOSS and eBOSS data
• From the Densest Clusters to the Emptiest Voids: No Evidence For Environmental Effects on the Galaxy Size-Mass Relation at Low Redshift