The 3D power spectrum of galaxies from the SDSS

Abstract

We measure the large-scale real-space power spectrum P(k) using a sample of 205,443 galaxies from the Sloan Digital Sky Survey, covering 2417 square degrees with mean redshift z~0.1. We employ a matrix-based method using pseudo-Karhunen-Loeve eigenmodes, producing uncorrelated minimum-variance measurements in 22 k-bands of both the clustering power and its anisotropy due to redshift-space distortions, with narrow and well-behaved window functions in the range 0.02 h/Mpc < k < 0.3h/Mpc. We pay particular attention to modeling, quantifying and correcting for potential systematic errors, nonlinear redshift distortions and the artificial red-tilt caused by luminosity-dependent bias. Our final result is a measurement of the real-space matter power spectrum P(k) up to an unknown overall multiplicative bias factor. Our calculations suggest that this bias factor is independent of scale to better than a few percent for k<0.1h/Mpc, thereby making our results useful for precision measurements of cosmological parameters in conjunction with data from other experiments such as the WMAP satellite. As a simple characterization of the data, our measurements are well fit by a flat scale-invariant adiabatic cosmological model with h Omega_m =0.201+/- 0.017 and L* galaxy sigma_8=0.89 +/- 0.02 when fixing the baryon fraction Omega_b/Omega_m=0.17 and the Hubble parameter h=0.72; cosmological interpretation is given in a companion paper.

41 ApJ pages, 40 figs. Power spectrum data, likelihood software and ppt pics available at http://www.hep.upenn.edu/~max/sdsspower.html

References in corpus (108)

• Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
• The Sloan Digital Sky Survey: Technical Summary
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
• The 2dF Galaxy Redshift Survey: Spectra and redshifts
• Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons
• Stable clustering, the halo model and nonlinear cosmological power spectra
• Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample
• The Sloan Digital Sky Survey Photometric Camera
• The u'g'r'i'z' Standard Star Network
• The Galaxy Luminosity Function and Luminosity Density at Redshift z=0.1
• Spectroscopic Target Selection for the Sloan Digital Sky Survey: The Luminous Red Galaxy Sample
• Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Quasar Sample
• Karhunen-Loeve eigenvalue problems in cosmology: how should we tackle large data sets?
• The First Data Release of the Sloan Digital Sky Survey
• Power Spectrum Analysis of Three-Dimensional Redshift Surveys
• Power Spectra for Cold Dark Matter and its Variants
• Astrometric Calibration of the Sloan Digital Sky Survey
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectrum
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• The 2dF Galaxy Redshift Survey: correlation functions, peculiar velocities and the matter density of the Universe
• Reconstructing the linear power spectrum of cosmological mass fluctuations
• The Broad-band Optical Properties of Galaxies with Redshifts 0.0 < z < 0.2
• A photometricity and extinction monitor at the Apache Point Observatory
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• The Luminosity Function of Galaxies in SDSS Commissioning Data
• Galaxy Clustering in Early SDSS Redshift Data
• An Efficient Algorithm for Positioning Tiles in the Sloan Digital Sky Survey
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• Estimating Fixed Frame Galaxy Magnitudes in the SDSS
• The Las Campanas Redshift Survey
• The PSCz Catalogue
• The Updated Zwicky Catalog (UZC)
• Biasing and Hierarchical Statistics in Large-scale Structure
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• The 2dF Galaxy Redshift Survey: Luminosity dependence of galaxy clustering
• Measuring cosmological parameters with galaxy surveys
• Cosmic Confusion: Degeneracies among Cosmological Parameters Derived from Measurements of Microwave Background Anisotropies
• How to measure CMB power spectra without losing information
• Galaxy Clusters in Hubble Volume Simulations: Cosmological Constraints from Sky Survey Populations
• Stochastic Nonlinear Galaxy Biasing
• Parameter constraints for flat cosmologies from CMB and 2dFGRS power spectra
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• Linear Redshift Distortions: A Review
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• Bianchi Type-I Anisotropic Dark Energy Models with Constant Deceleration Parameter
• Investigating dark energy experiments with principal components
• Internal space structure generalization of the quintom cosmological scenario
• Non-minimally Coupled Quintom Model Inspired by String Theory
• Correlated Primordial Perturbations in Light of CMB and LSS Data
• Cosmological Inflation in f(Q, T) Gravity
• Recovering the Inflationary Potential and Primordial Power Spectrum With a Slow Roll Prior: Methodology and Application to WMAP 3 Year Data
• Are Great Disks Defined by Satellite Galaxies in Milky-Way Type Halos Rare in $\Lambda$CDM model?
• Comparison of Approaches to Quantum Correction of Black Hole Thermodynamics
• Reconstruction of Deceleration Parameters from Recent Cosmic Observations
• Unmasking the Masked Universe: the 2M++ catalogue through Bayesian eyes
• A Note on Crossing the Phantom Divide in Hybrid Dark Energy Model
• ShapeFit: extracting the power spectrum shape information in galaxy surveys beyond BAO and RSD
• Statistics of Voids in the 2dF Galaxy Redshift Survey
• Separating intrinsic alignment and galaxy-galaxy lensing
• Dynamics in Nonlocal Cosmological Models Derived from String Field Theory
• Increasing the effective number of neutrinos with decaying particles
• FLRW solutions in $f(Q)$ theory: the effect of using different connections
• Supernovae constraints on models of dark energy revisited
• Dependence of Barred Galaxy Fraction on Galaxy Properties and Environment
• K-Chameleon and the Coincidence Problem
• Constraints on large scale inhomogeneities from WMAP-5 and SDSS: confrontation with recent observations
• Reconstruction of Hessence Dark Energy and the Latest Type Ia Supernovae Gold Dataset
• N-Body Simulations of Alternate Gravity Models
• Wide Angle Effects in Future Galaxy Surveys
• Dark Matter Cores and Cusps in Spiral Galaxies and their Explanations
• The updated luminosity correlations of gamma-ray bursts and cosmological implications
• Cosmology with the Galaxy Bispectrum Multipoles: Optimal Estimation and Application to BOSS Data
• Indication for Primordial Anisotropies in the Neutrino Background from WMAP and SDSS
• A Modified Holographic Dark Energy Model with Infrared Infinite Extra Dimension(s)
• Cosmological bounds on the equation of state of dark matter
• Reconstruction of general scalar-field dark energy models
• Two scalar field cosmology: Conservation laws and exact solutions
• Constraints on f(R) Cosmology in the Palatini Formalism
• Deflection of light by black holes and massless wormholes in massive gravity
• Galaxy Bias and Halo-Occupation Numbers from Large-Scale Clustering
• The 2dF Galaxy Redshift Survey: higher order galaxy correlation functions
• Searches for New Milky Way Satellites from the First Two Years of Data of the Subaru/Hyper Suprime-Cam Survey: Discovery of Cetus~III
• CMBR Constraint on a Modified Chaplygin Gas Model
• Covariance of cross-correlations: towards efficient measures for large-scale structure
• Structure formation in a string-inspired modification of the cold dark matter model
• Cosmological perturbation theory in 1+1 dimensions
• Cosmological Models and Gamma-Ray Bursts Calibrated by Using Pade Method
• CMB and Matter Power Spectra of Early f(R) Cosmology in Palatini Formalism
• An analytic model for the bispectrum of galaxies in redshift space
• From Galaxy-Galaxy Lensing to Cosmological Parameters
• Inflation in Entropic Cosmology: Primordial Perturbations and non-Gaussianities
• Testing homogeneity on large scales in the Sloan Digital Sky Survey Data Release One
• On Minimally-Parametric Primordial Power Spectrum Reconstruction and the Evidence for a Red Tilt
• Tests of Gravity from Imaging and Spectroscopic Surveys
• Slow Roll Reconstruction: Constraints on Inflation from the 3 Year WMAP Dataset
• Time Lumps in Nonlocal Stringy Models and Cosmological Applications
• A Concept for A Dark Matter Detector Using Liquid Helium-4
• The dark energy equation of state
• First underground results with NEWAGE-0.3a direction-sensitive dark matter detector
• Luminosity dependence of the spatial and velocity distributions of galaxies: Semi-analytic models versus the Sloan Digital Sky Survey
• Primordial black holes and stochastic gravitational wave background from inflation with a noncanonical spectator field
• General Analytic Solutions of Scalar Field Cosmology with Arbitrary Potential
• Cosmic Cartography of the Large-Scale Structure with Sloan Digital Sky Survey Data Release 6
• On the growth of structure in theories with a dynamical preferred frame
• Systematic Effects on Determination of the Growth Factor from Redshift-space Distortions
• Estimation of Primordial Spectrum with post-WMAP 3 year data
• Tracking Dark Energy with the ISW effect: short and long-term predictions
• Eddington-Born-Infeld gravity and the large scale structure of the Universe
• Tension of the $E_G$ statistic and RSD data with Planck/$\Lambda$CDM and implications for weakening gravity
• Analysis of the Yukawa gravitational potential in $f(R)$ gravity II: relativistic periastron advance
• Non-local SFT Tachyon and Cosmology
• Transformation of Morphology and Luminosity Classes of the SDSS Galaxies
• The State Equation of the Yang-Mills field Dark Energy Models
• Revisiting the Baryon Fractions of Galaxy Clusters: A Comparison with WMAP 3-year Results
• Growth Index of DGP Model and Current Growth Rate Data
• Pilgrim Dark Energy
• Magnetized CMB observables: a dedicated numerical approach
• Observing the clustering properties of galaxy clusters in dynamical dark-energy cosmologies
• Observational Requirements for Lyman-alpha Forest Tomographic Mapping of Large-Scale Structure at z ~ 2
• Constraining $f(R)$ gravity by the Large Scale Structure
• De Sitter Universe in Nonlocal Gravity
• An improved cosmological bound on the thermal axion mass
• Cosmological Constraints from a Combination of Galaxy Clustering & Lensing -- II. Fisher Matrix Analysis
• Spherical collapse model with shear and angular momentum in dark energy cosmologies
• Cosmological constraints from the power spectrum of eBOSS emission line galaxies
• Analyze This! A Cosmological Constraint Package for CMBEASY
• Three-Point Correlation Functions of SDSS Galaxies: Luminosity and Color Dependence in Redshift and Projected Space
• Holographic Dark Energy in Brans-Dicke Theory
• Observational Constraints on New Exact Inflationary Scalar-field Solutions
• A 14 $h^{-3}$ Gpc${}^3$ study of cosmic homogeneity using BOSS DR12 quasar sample
• Erasing the Milky Way: new cleaning technique applied to GBT intensity mapping data
• Axion constraints in non-standard thermal histories
• Constraints on the Primordial Power Spectrum from High Resolution Lyman-alpha Forest Spectra and WMAP
• Present bounds on the relativistic energy density in the Universe from cosmological observables
• Probing the Epoch of Early Baryonic Infall Through 21cm Fluctuations
• Correlated isocurvature perturbations from mixed inflaton-curvaton decay
• Neutrino masses and cosmic radiation density: Combined analysis
• Tidal alignments as a contaminant of redshift space distortions
• PRIMUS: Galaxy Clustering as a Function of Luminosity and Color at 0.2<z<1
• Kaluza-Klein cosmological model in $f(R,T)$ gravity with $\Lambda (T)$
• Where are the Luminous Red Galaxies (LRGs)? Using correlation measurements and lensing to relate LRGs to dark matter halos
• Scale Dependent Galaxy Bias in the SDSS as a function of Luminosity and Colour
• Modelling non-linear redshift-space distortions in the galaxy clustering pattern: systematic errors on the growth rate parameter
• Constraining the Projected Radial Distribution of Galactic Satellites with the Sloan Digital Sky Survey
• The environmental dependence of galaxy clustering in the Sloan Digital Sky Survey
• Do WMAP data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
• Dark Energy in Practice
• MCMC analysis of WMAP3 and SDSS data points to broken symmetry inflaton potentials and provides a lower bound on the tensor to scalar ratio
• Dark Energy Model in Anisotropic Bianchi Type-III Space-Time with Variable EoS Parameter
• Interacting Ghost Dark Energy in Brans-Dicke Theory
• The Importance of Quantum Pressure of Fuzzy Dark Matter on Lyman-Alpha Forest
• The initial conditions of the universe: how much isocurvature is allowed?
• Implications of the Curvaton on Inflationary Cosmology
• Cosmology of neutrinos and extra light particles after WMAP3
• The impact of the connectivity of the cosmic web on the physical properties of galaxies at its nodes
• The galaxy power spectrum: precision cosmology from large scale structure?
• Reconstruction of the primordial power spectrum of curvature perturbations using multiple data sets
• Do Bars Trigger Activity in Galactic Nuclei?
• Bounds on CDM and neutrino isocurvature perturbations from CMB and LSS data
• Cosmological hydrogen recombination: The effect of extremely high-n states
• Reconstruction of primordial density fields
• Testing the phenomenological interacting dark energy with observational $H(z)$ data
• Cosmological constraints without fingers of God
• Cosmology Without Windows: Quadratic Estimators for the Galaxy Power Spectrum
• Revisit of the Interaction between Holographic Dark Energy and Dark Matter
• Stochastic backgrounds of relic gravitons: a theoretical appraisal
• Constraints on Primordial Black Holes by Distortions of Cosmic Microwave Background
• The VIMOS-VLT Deep Survey: Luminosity dependence of clustering at z~1
• All-Sky Analysis of the General Relativistic Galaxy Power Spectrum
• Squeezing the window on isocurvature modes with the Lyman-alpha forest
• Constraining Lorentz violation with cosmology
• Is the Number of Giant Arcs in LCDM Consistent With Observations?
• Topology of structure in the Sloan Digital Sky Survey: model testing
• Simulating Structure Formation of the Local Universe
• Strategies for Determining the Nature of Dark Matter
• Sloan Digital Sky Survey III Photometric Quasar Clustering: Probing the Initial Conditions of the Universe using the Largest Volume
• Features in Dark Energy Equation of State and Modulations in the Hubble Diagram
• The Projected Dark and Baryonic Ellipsoidal Structure of 20 CLASH Galaxy Clusters
• The Nonlinear Cosmological Matter Power Spectrum with Massive Neutrinos I: The Halo Model
• Limits on deviations from the inverse-square law on megaparsec scales
• Constraining the Cosmological Parameters and Transition Redshift with Gamma-Ray Bursts and Supernovae
• The Bright End of the Luminosity Function of Red Sequence Galaxies
• Precision cosmology with a wide area XMM cluster survey
• Galaxy clustering constraints on deviations from Newtonian gravity at cosmological scales
• {\sc CosmoNet}: fast cosmological parameter estimation in non-flat models using neural networks
• Boötes IV: A New Milky Way Satellite Discovered in the Subaru Hyper Suprime-Cam Survey and Implications for the Missing Satellite Problem
• The Evolution of Substructure in Galaxy, Group and Cluster Haloes II: Global Properties
• Orbital evolution of the Carina dwarf galaxy and self-consistent star formation history determination
• A New Equation of State for Dark Energy Model
• Galaxy Activity in Merging Binary Galaxy Clusters
• Compensated Isocurvature Perturbations and the Cosmic Microwave Background
• Reconstructing a general inflationary action
• Shear and rotation in Chaplygin cosmology
• Tracing mass and light in the Universe: where is the dark matter?
• The Relevance of the Cosmological Constant for Lensing
• Forecasting the Bayes factor of a future observation
• Extracting the Gamma Ray Signal from Dark Matter Annihilation in the Galactic Center Region
• Constraints on Cold Dark Matter Accelerating Cosmologies and Cluster Formation
• A New Independent Limit on the Cosmological Constant/Dark Energy from the Relativistic Bending of Light by Galaxies and Clusters of Galaxies
• Do Large-Scale Inhomogeneities Explain Away Dark Energy?
• Cosmological Constraints on the Modified Entropic Force Model
• Galaxy redshift surveys selected by neutral hydrogen using FAST
• Alleviation of Cosmic Age Problem In Interacting Dark Energy Model
• Accelerating universe from gravitational leakage into extra dimensions: confrontation with SNeIa
• On what scale should inflationary observables be constrained?
• Cosmology Without Window Functions: Cubic Estimators for the Galaxy Bispectrum
• The abundance of galaxy clusters in MOND: Cosmological simulations with massive neutrinos
• Holographic dark energy in a universe with spatial curvature and massive neutrinos: a full Markov Chain Monte Carlo exploration
• Constraint on the Effective Number of Neutrino Species from the WMAP and SDSS LRG Power Spectra
• The Atacama Cosmology Telescope: Detection of Sunyaev-Zel'dovich Decrement in Groups and Clusters Associated with Luminous Red Galaxies
• Conformally related metrics and Lagrangians and their physical interpretation in cosmology
• A tale of two (or more) $h$'s
• The Spatial Clustering of Low Luminosity AGN
• An ideal mass assignment scheme for measuring the Power Spectrum with FFTs
• Photometric Redshifts for the Dark Energy Survey and VISTA and Implications for Large Scale Structure
• Non-adiabatic-like accelerated expansion of the late universe in entropic cosmology
• The UNAM-KIAS Catalog of Isolated Galaxies
• Holographic hessence models
• $f(R)$-gravity from Killing Tensors
• Cosmic tomographies: baryon acoustic oscillations and weak lensing
• Stochastic backgrounds of relic gravitons, T$\Lambda$CDM paradigm and the stiff ages
• Holographic f(T)-gravity model with power-law entropy correction
• Generalized Holographic and Ricci Dark Energy Models
• Remarks on the formulation of the cosmological constant/dark energy problems
• The isocurvature fraction after WMAP 3-year data
• Observational constraints on Gauss-Bonnet cosmology
• VoIgt profile Parameter Estimation Routine (VIPER): H I photoionization rate at z<0.5
• Dynamics of Quintom and Hessence Energies in Loop Quantum Cosmology
• Another thread in the tapestry of stellar feedback: X-ray binaries
• Holographic Dark Energy Model with Hubble Horizon as an IR Cut-off
• Hints of Isocurvature Perturbations in the Cosmic Microwave Background?
• Cosmological inference from Bayesian forward modelling of deep galaxy redshift surveys
• Holographic Ricci dark energy: Interacting model and cosmological constraints
• Isotropy of the early universe from CMB anisotropies
• Peculiar Velocity Decomposition, Redshift Space Distortion and Velocity Reconstruction in Redshift Surveys. II. Dark Matter Velocity Statistics
• A Simple Model for Quintessential Inflation
• Matter Power Spectrum Covariance Matrix from the DEUS-PUR ΛCDM simulations: Mass Resolution and non-Gaussian Errors
• The XMM Cluster Survey: Forecasting cosmological and cluster scaling-relation parameter constraints
• Dynamical Analysis of an Integrable Cubic Galileon Cosmological Model
• Breaking scale invariance from a singular inflaton potential
• Methods for Bayesian power spectrum inference with galaxy surveys
• Dark Energy and Neutrino Masses from Future Measurements of the Expansion History and Growth of Structure
• How to Distinguish Dark Energy and Modified Gravity?
• Bayesian optimal reconstruction of the primordial power spectrum
• Scalar-Tensor Gravity Cosmology: Noether symmetries and analytical solutions
• Cheng-Weyl Vector Field and its Cosmological Application
• Determining Cosmological Parameters with Latest Observational Data
• Constraints on f(R) theory and Galileons from the latest data of galaxy redshift surveys
• Testing the effect of $H_0$ on $f{\sigma }_8$ tension using a Gaussian Process method
• The Alcock-Paczynski test in redshifted twenty one centimeter maps
• GOODS-Herschel: the impact of galaxy-galaxy interactions on the far-infrared properties of galaxies
• The GEEC2 spectroscopic survey of Galaxy Groups at $0.8<z<1$
• The Universal Einstein Radius Distribution from 10,000 SDSS Clusters
• Confrontation of MOND Predictions with WMAP First Year Data
• Equilibrium configurations of 11eV sterile neutrinos in MONDian galaxy clusters
• Triaxial haloes, intrinsic alignments and the dark matter power spectrum
• Interacting Energy Components and Observational $H(z)$ Data
• Generalized Chaplygin gas model, supernovae and cosmic topology
• Conditions and instability in $f(R)$ gravity with non-minimal coupling between matter and geometry
• Noether symmetries and stability of ideal gas solution in Galileon Cosmology
• Dark Energy or Apparent Acceleration Due to a Relativistic Cosmological Model More Complex than FLRW?
• The DEEP2 Galaxy Redshift Survey: The Evolution of Void Statistics from z~1 to z~0
• Yang-Mills condensate dark energy coupled with matter and radiation
• Magnetogenesis, spectator fields and CMB signatures
• 21 cm observation of LSS at z~1 Instrument sensitivity and foreground subtraction
• Activity in galactic nuclei of cluster and field galaxies in the local universe
• Theoretical tools for CMB physics
• Do observations prove that cosmological neutrinos are thermally distributed?
• The impact of Galactic synchrotron emission on CMB anisotropy measurements. I. Angular power spectrum analysis of total intensity all-sky surveys
• Duty Cycle and the Increasing Star Formation History of z>=6 Galaxies
• Is cosmology compatible with sterile neutrinos?
• Constraining the Cosmic Baryon Distribution with Fast Radio Burst Foreground Mapping
• Reconstructing f(R) theory according to holographic dark energy
• Averaging in Spherically Symmetric Cosmology
• Astrophysical Configurations with Background Cosmology: Probing Dark Energy at Astrophysical Scales
• New light on Dark Cosmos
• Hints of Modified Gravity in Cosmos and in the Lab?
• Baryon Oscillations and Consistency Tests for Photometrically-Determined Redshifts of Very Faint Galaxies
• Clustering and redshift-space distortions in interacting dark energy cosmologies
• Mitigating contamination in LSS surveys: a comparison of methods
• Cosmological parameter forecasts for HI intensity mapping experiments using the angular power spectrum
• Coincidence Problem in YM Field Dark Energy Model
• Prospects for Constraining Neutrino Mass Using Planck and Lyman-Alpha Forest Data
• Latest astronomical constraints on some nonlinear parametric dark energy models
• Dynamics of Quintessence with Thermal Interactions
• Interacting model of new agegraphic dark energy: observational constraints and age problem
• Cosmic Structure and Dynamics of the Local Universe
• Observational Constraints to Ricci Dark Energy Model by Using: SN, BAO, OHD, fgas Data Sets
• Forecast for FAST: from Galaxies Survey to Intensity Mapping
• Environmental dependence of AGN activity. I.: the effects of host galaxy
• Observational Constraints on Silent Quartessence
• Search for sterile neutrinos in a universe of vacuum energy interacting with cold dark matter
• Interaction between dark energy and dark matter: observational constraints from OHD, BAO, CMB and SNe Ia
• Probing Dynamics of Dark Energy with Supernova, Galaxy Clustering and the Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations
• Features of galactic halo in a brane world model and observational constraints
• Hierarchical clustering in chameleon $f(R)$ gravity
• Peculiar Velocity Decomposition, Redshift Space Distortion and Velocity Reconstruction in Redshift Surveys - I. The Methodology
• Slow-Roll Suppression of Adiabatic Instabilities in Coupled Scalar Field-Dark Matter Models
• Is the evidence for dark energy secure?
• What is the best way to measure baryonic acoustic oscillations?
• Appeasing the Phantom Menace?
• Anisotropic brane gravity with a confining potential
• Scalar Field Dark Energy Perturbations and their Scale Dependence
• Cosmic perturbations with running G and Lambda
• Field Level Neural Network Emulator for Cosmological N-body Simulations
• Mass Function of Rich Galaxy Clusters and Its Constraint on sigma_8
• Clustering on very small scales from a large sample of confirmed quasar pairs: Does quasar clustering track from Mpc to kpc scales?
• Attractors, Statefinders and Observational Measurement for Chameleonic Brans--Dicke Cosmology
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Consistent multi-wavelength photometry for the DEVILS regions (COSMOS, XMMLSS & ECDFS)
• Testing gravity with motion of satellites around galaxies: Newtonian gravity against Modified Newtonian Dynamics
• Boundary Effective Field Theory and Trans-Planckian Perturbations: Astrophysical Implications
• Simulated ΛCDM analogues of the thin Plane of Satellites around the Andromeda galaxy are not kinematically coherent structures
• Modified Dust and the Small Scale Crisis in CDM
• The spherical collapse model in time varying vacuum cosmologies
• Tests of General Relativity on Astrophysical Scales
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: combining correlated Gaussian posterior distributions
• Dynamics of a two scalar field cosmological model with phantom terms
• Cosmological neutrinos
• Cosmological Simulation for Fuzzy Dark Matter Model
• Revisiting the parametrization of Equation of State of Dark Energy via SNIa Data
• Cartan symmetries and global dynamical systems analysis in a higher-order modified teleparallel theory
• Cosmological surveys with the Australian Square Kilometre Array Pathfinder
• Constraints on Kinematic Model from Recent Cosmic Observations: SN Ia, BAO and Observational Hubble Data
• The growth index of matter perturbations and modified gravity
• Dynamical symmetries and observational constraints in scalar field cosmology
• Dark energy with polytropic equation of state
• The Evolution of Substructure in Galaxy, Group and Cluster Haloes III: Comparison with Simulations
• Testing one-loop galaxy bias: Power spectrum
• What sets the central structure of dark matter haloes?
• Clues on void evolution III: Structure and dynamics in void shells
• Reconstruction Procedure in Nonlocal Cosmological Models
• Effects of time-varying $\beta$ in SNLS3 on constraining interacting dark energy models
• A Hybrid Deep Learning Approach to Cosmological Constraints From Galaxy Redshift Surveys
• Cosmology with Equivalence Principle Breaking in the Dark Sector
• Inflationary Perturbations and Precision Cosmology
• Possibility of realizing weak gravity in redshift space distortion measurements
• Cosmological observations in a modified theory of gravity (MOG)
• Properties of Cosmological Filaments extracted from Eulerian Simulations
• Unbiased methods for removing systematics from galaxy clustering measurements
• Coupled Quintessence and Phantom Based On a Dilaton
• Can extra dimensional effects replace dark matter ?
• Accelerating dark energy models with anisotropic fluid in Bianchi type-$V{I}_0$ space-time
• A new method to measure the mass of galaxy clusters
• 3-loop Yang-Mills Condensate Dark Energy Model And Its Cosmological Constraints
• Structural Analysis of the SDSS Cosmic Web I.Nonlinear Density Field Reconstructions
• Cosmological Solutions of a Nonlocal Model with a Perfect Fluid
• The Next Generation Fornax Survey (NGFS): III. Revealing the Spatial Substructure of the Dwarf Galaxy Population inside half of Fornax's Virial Radius
• Modified Holographic Dark Energy
• Revisiting the Cosmological Constraints on the Interacting Dark Energy Models
• $f(R)$ gravity theories in the Palatini Formalism constrained from strong lensing
• Unbiased pseudo-Cl power spectrum estimation with mode projection
• Persistent homology of the cosmic web. I: Hierarchical topology in $\Lambda$CDM cosmologies
• The footprint of large scale cosmic structure on the ultra-high energy cosmic ray distribution
• The Signature of Large Scale Structures on the Very High Energy Gamma-Ray Sky
• Anthropic predictions for neutrino masses
• Scale-dependent Galaxy Bias
• Measuring the 2D Baryon Acoustic Oscillation signal of galaxies in WiggleZ: Cosmological constraints
• A First Glimpse of String Theory in the Sky?
• Large Scale Structure of the Universe
• Halo stochasticity in global clustering analysis
• Crossing of the w=-1 Barrier in Two-Fluid Viscous Modified Gravity
• Some remarks about non-minimally coupled scalar field models
• Extended Zee model for Neutrino Mass, Leptogenesis and Sterile Neutrino like Dark Matter
• Luminous Red Galaxy Halo Density Field Reconstruction and Application to Large Scale Structure Measurements
• When Did Cosmic Acceleration Start ?
• Exploring the Systematic Uncertainties of Type Ia Supernovae as Cosmological Probes
• Dynamics in nonlocal linear models in the Friedmann-Robertson-Walker metric
• New Agegraphic Dark Energy in $f(R)$ Gravity
• Light Deflection, Lensing, and Time Delays from Gravitational Potentials and Fermat's Principle in the Presence of a Cosmological Constant
• Stability analysis and Observational Measurement in Chameleonic Generalised Brans--Dicke Cosmology
• Scaling Exponents for Lattice Quantum Gravity in Four Dimensions
• Constraints on the Inflationary Expansion from Three Year WMAP, small scale CMB anisotropies and Large Scale Structure Data Sets
• The dependence of the pairwise velocity dispersion on galaxy properties
• Population III Star Formation in a Lambda WDM Universe
• 2-FAST: Fast and accurate computation of projected two-point functions
• Variable Equation of State for Generalized Dark Energy Model
• Difficulty of detecting minihalos via $\gamma$-rays from dark matter annihilation
• Supersymmetric dark matter search via spin-dependent interaction with He3
• Dynamical symmetries in Brans-Dicke cosmology
• Using galaxy-galaxy weak lensing measurements to correct the Finger-of-God
• Cosmic Constraint on Ricci Dark Energy Model
• Beyond $\Lambda$CDM constraints from the full shape clustering measurements from BOSS and eBOSS
• Muon Fluxes From Dark Matter Annihilation
• Cosmic Voids and Galaxy Bias in the Halo Occupation Framework
• Holographic Dark Energy Models and Higher Order Generalizations in Dynamical Chern-Simons Modified Gravity
• Breaking the self-averaging properties of spatial galaxy fluctuations in the Sloan Digital Sky Survey - Data Release Six
• Cosmic filaments in galaxy cluster outskirts: quantifying finding filaments in redshift space
• Cosmological Evolution and Exact Solutions in a Fourth-order Theory of Gravity
• IceHEP High Energy Physics at the South Pole
• QCD ghost f(T)-gravity model
• Constraining the evolution of dark energy with type Ia supernovae and gamma-ray bursts
• HectoMAP and Horizon Run 4: Dense Structures and Voids in the Real and Simulated Universe
• $\Lambda$-CDM Universe: A Phenomenological Approach With Many Possibilities
• Inflaton dark matter from incomplete decay
• Primordial Neutrinos, Cosmological Perturbations in Interacting Dark-Energy Model: CMB and LSS
• Reconstructing a String-Inspired Quintom Model of Dark Energy
• Dynamics of holographic vacuum energy in the DGP model
• Testing gaussianity, homogeneity and isotropy with the cosmic microwave background
• Radiative corrections to co-annihilation processes
• Observational signatures of the theories beyond Horndeski
• Extended Born-Infeld Dynamics and Cosmology
• Cosmological perturbations in SFT inspired non-local scalar field models
• Observational constraints on cosmic strings: Bayesian analysis in a three dimensional parameter space
• Cosmological Constraints from Hubble parameter $H(z)$ and SN Ia observations
• LtU-ILI: An All-in-One Framework for Implicit Inference in Astrophysics and Cosmology
• Validating a minimal galaxy bias method for cosmological parameter inference using HSC-SDSS mock catalogs
• Beyond Two Dark Energy Parameters
• Transit cosmological models with observational constraints in f(Q, T) gravity
• Speed from light: growth rate and bulk flow at z ~ 0.1 from improved SDSS DR13 photometry
• Constraints on Dark Energy Models Including Gamma Ray Bursts
• Asymmetric Gravitational Lenses in TeVeS and Application to the Bullet Cluster
• Non-Gaussianity in Large Scale Structure and Minkowski Functionals
• The full Fisher matrix for galaxy surveys
• Affine parameterization of the dark sector: costraints from WMAP5 and SDSS
• Mapping the real space distributions of galaxies in SDSS DR7: I. Two Point Correlation Functions
• The Angular Power Spectra of Photometric SDSS LRGs
• Late Forming Dark Matter in Theories of Neutrino Dark Energy
• Sub-Megaparsec Individual Photometric Redshift Estimation from Cosmic Web Constraints
• On the isolated dwarf galaxies: from cuspy to flat dark matter density profiles and metallicity gradients
• Constraints on Lorentz Invariance Violation with gamma-ray bursts via a Markov Chain Monte Carlo approach
• Cosmological constraints on general, single field inflation
• Constraining thermal dust emission in distant galaxies with number counts and angular power spectra
• Voids and the Cosmic Web: cosmic depressions & spatial complexity
• Radio Emission in the Cosmic Web
• MIMAC : A Micro-TPC Matrix of Chambers for direct detection of Wimps
• Localization of nonlocal cosmological models with quadratic potentials in the case of double roots
• Crossing of $\omega =-1$ with Tachyon and Non-minimal Derivative Coupling
• Color Dependence in the Spatial Distribution of Satellite Galaxies
• Towards Accurate Modelling of Galaxy Clustering on Small Scales: Testing the Standard $\Lambda \mathrm{CDM}$ + Halo Model
• Using Multipoles of the Correlation Function to Measure H(z), D_A(z), and β(z) from Sloan Digital Sky Survey Luminous Red Galaxies
• Weak lensing study of 16 DAFT/FADA clusters: substructures and filaments
• Star Formation and Substructure in Galaxy Clusters
• Evolution of density perturbations in decaying vacuum cosmology: The case of non-zero perturbations in the cosmological term
• Galaxy Cluster Bulk Flows and Collision Velocities in QUMOND
• The solution of the cosmological constant problem from the inhomogeneous equation of state - a hint from modified gravity?
• Galaxy clustering constraints on deviations from Newtonian gravity at cosmological scales II: Perturbative and numerical analyses of power spectrum and bispectrum
• The Cosmic Neutrino Background and the Age of the Universe
• Testing the DGP model with gravitational lensing statistics
• Testing for dynamical dark energy models with redshift-space distortions
• WMAP 5-year constraints on lepton asymmetry and radiation energy density: Implications for Planck
• Galaxy clustering and projected density profiles as traced by satellites in photometric surveys: Methodology and luminosity dependence
• Semi-analytical approach to magnetized temperature autocorrelations
• Phenomenology of $\Lambda$-CDM model: a possibility of accelerating Universe with positive pressure
• Power Spectrum Shape from Peculiar Velocity Data
• The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3
• The ALHAMBRA survey: evolution of galaxy clustering since $z\sim 1$
• Deviations from tidal torque theory: evolution of the halo spin-filament alignment
• Kelvin-Helmholtz Instability in Self-Gravitating Streams
• Conformal Transformations and Weak Field Limit of Scalar-Tensor Gravity
• Probing Inflation and Dark Energy with Current Cosmological Observations
• Analysis of scalar perturbations in cosmological models with a non-local scalar field
• The nature of the Sloan Digital Sky Survey galaxies in various classes based on morphology, colour and spectral features - III. Environments
• Large Scale Clustering of Sloan Digital Sky Survey Quasars: Impact of the Baryon Density and the Cosmological Constant
• Measurement of marked correlation functions in SDSS-III Baryon Oscillation Spectroscopic Survey using LOWZ galaxies in Data Release 12
• Observational Constraints on Dark Energy Models with $\Lambda$ as an Equilibrium Point
• Evolution of mass and velocity filed in comic web: comparison between baryonic and dark matter
• Forecasting neutrino masses from combining KATRIN and the CMB: Frequentist and Bayesian analyses
• Power Spectrum of Cosmic Momentum Field Measured from the SFI Galaxy Sample
• Galactic rotation curves inspired by a noncommutative-geometry background
• The nature of the SDSS galaxies in various classes based on morphology, colour and spectral features -- I. Optical properties
• Fourier Phase Analysis of SDSS Galaxies
• Constraints on Neutrino Mass and Light Degrees of Freedom in Extended Cosmological Parameter Spaces
• Gravity, antimatter and the Dirac-Milne universe
• Cosmological Constraints on Variable Warm Dark Matter
• Catalogs of Compact Groups of Galaxies from the Enhanced SDSS DR12
• Thermodynamical aspects of relativistic hydrodynamics in f(R,G) gravity
• Bouncing universe with the non-minimally coupled scaler field and its reconstructing
• Generalized CMB initial conditions with pre-equality magnetic fields
• Solving the main cosmological puzzles with a generalized time varying vacuum energy
• Properties of clumps and filaments around galaxy clusters
• The dark flow induced small scale kinetic Sunyaev Zel'dovich effect
• Reconstructing generalized ghost condensate model with dynamical dark energy parametrizations and observational datasets
• Understanding the nature of luminous red galaxies (LRGs): Connecting LRGs to central and satellite subhalos
• Galaxy redshift surveys with sparse sampling
• Exploring Large-scale Structure with Billions of Galaxies
• Perturbation Theory for BAO reconstructed fields: one-loop results in real-space matter density field
• Using the cluster mass function from weak lensing to constrain neutrino masses
• Exploring star formation using the filaments in the Sloan Digital Sky Survey Data Release Five (SDSS DR5)
• Exact cosmological solution of a Scalar-Tensor Gravity theory compatible with the $\Lambda CDM$ model
• Damped Lyα Absorption Systems in Semi-Analytic Models with Multiphase Gas
• Constraining power of cosmological observables: blind redshift spots and optimal ranges
• Multiplicative errors in the galaxy power spectrum: self-calibration of unknown photometric systematics for precision cosmology
• The thermal Sunyaev-Zel'dovich Signature of Baryons in the Local Universe
• Cosmological neutrino bounds for non-cosmologists
• An improved limit on the neutrino mass with CMB and redshift-dependent halo bias-mass relations from SDSS, DEEP2, and Lyman-Break Galaxies
• Deviation from the Cosmological Constant or Systematic Errors?
• Self-accelerating the normal DGP branch
• Weak lensing and dark energy: the impact of dark energy on nonlinear dark matter clustering
• Some FRW Models of Accelerating Universe with Dark Energy
• Null Energy Condition Violation and Classical Stability in the Bianchi I Metric
• Constraints on Resonant Particle Production during Inflation from the Matter and CMB Power Spectra
• The Cosmological Constant Problem, an Inspiration for New Physics
• Dark energy parameterizations and their effect on dark halos
• The $\Lambda$CDM growth rate of structure revisited
• Collider, direct and indirect detection of supersymmetric dark matter
• A Radial Measurement of the Galaxy Tidal Alignment Magnitude with BOSS Data
• Generalized Chaplygin gas model: Cosmological consequences and statefinder diagnosis
• Measuring the geometry of the Universe in the presence of isocurvature modes
• Cosmological Models and Latest Observational Data
• Revealing modified gravity signal in matter and halo hierarchical clustering
• New integrable models and analytical solutions in $f(R)$~cosmology with an ideal gas
• Understanding the origin of CMB constraints on Dark Energy
• Accelerating bianchi type dark energy cosmological model with cosmic string in f(T) Gravity
• The Galaxy Cross-Correlation Function as a Probe of the Spatial Distribution of Galactic Satellites
• Exploring the evolution of color-luminosity parameter $\beta$ and its effects on parameter estimation
• Non-thermal radio supernova remnants of exiled Wolf-Rayet stars
• Re-examining the Too-Big-To-Fail Problem for Dark Matter Haloes with Central Density Cores
• Neutrino masses and mixings in the baryon triality constrained minimal supersymmetric standard model
• ECO and RESOLVE: Galaxy Disk Growth in Environmental Context
• Study on the mapping of dark matter clustering from real space to redshift space
• Tidal alignments as a contaminant of the galaxy bispectrum
• Constraining the Nature of Dark Energy using the SKA
• Large-scale magnetic fields, curvature fluctuations and the thermal history of the Universe
• High-resolution temporal constraints on the dynamics of dark energy
• Anisotropies in the Cosmic Neutrino Background after WMAP 5-year Data
• Cosmological implications from the full shape of the large-scale power spectrum of the SDSS DR7 luminous red galaxies
• Galaxy peculiar velocities and evolution-bias
• Cosmic Dynamics in $F(R,\varphi )$ Gravity
• A brief note on how to unify dark matter, dark energy, and inflation
• Constraints on a decomposed dark fluid with constant adiabatic sound speed by jointing the geometry test and growth rate after Planck data
• Nonlinear Effects in the Amplitude of Cosmological Density Fluctuations
• A new model for the full shape of the large-scale power spectrum
• Gamma rays from the neutralino dark matter annihilations in the Milky Way substructures
• Vacuum Energy as the Origin of the Gravitational Constant
• A Robust Distance Measurement and Dark Energy Constraints from the Spherically-Averaged Correlation Function of Sloan Digital Sky Survey Luminous Red Galaxies
• Cosmic strings interacting with dark strings
• Fixed points and FLRW cosmologies: Flat case
• A more general interacting model of holographic dark energy
• Roche Lobe Underfilling of the Secondary Star in PSR J102347.6+003841?
• k-essence in the DGP brane-world cosmology
• Evidence for the Fifth Element Astrophysical status of Dark Energy
• From the Spectrum to Inflation : An Inverse Formula for the General Slow-Roll Spectrum
• Simulating MOS science on the ELT: Ly$\alpha$ forest tomography
• The 2MASS galaxy angular power spectrum: Probing the galaxy distribution to Gigaparsec scales
• Crossing the phantom divide line as an effect of quantum transitions
• Attractor Solution in Coupled Yang-Mills Field Dark Energy Models
• Testing the interaction model with cosmological data and gamma-ray bursts
• Higher neutrino mass allowed if Cold Dark Matter and Dark Energy are coupled
• Anisotropic Dark Energy Bianchi Type III Cosmological Models in Brans Dicke Theory of Gravity
• Revised WMAP constraints on neutrino masses and other extensions of the minimal $\Lambda$CDM model
• Cosmological constraints from Radial Baryon Acoustic Oscillation measurements and Observational Hubble data
• Corrected holographic dark energy with power-law entropy and Hubble Horizon cut-off in FRW Universe
• Redshift-space distortions of galaxies, clusters and AGN: testing how the accuracy of growth rate measurements depends on scales and sample selections
• The impact of neutrino masses on the determination of dark energy properties
• Testing one-loop galaxy bias: cosmological constraints from the power spectrum
• Heteroclinic orbit and tracking attractor in cosmological model with a double exponential potential
• Bayesian cosmic density field inference from redshift space dark matter maps
• Stellar Mass and color dependence of the three-point correlation function of galaxies in the local universe
• Self-interacting holographic dark energy
• Sounds of instability from generalized QCD ghost dark energy
• The Cosmic Microwave Background and Inflation Parameters
• Combined constraints on Cardassian models from supernovae, CMB and large-scale structure observations
• Vacuum Condensate Picture of Quantum Gravity
• The effect of dark strings on semilocal strings
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• Continuous wavelet analysis of matter clustering using the Gaussian-derived wavelet
• Likelihood reconstruction method of real-space density and velocity power spectra from a redshift galaxy survey
• Group-galaxy correlations in redshift space as a probe of the growth of structure
• Extending Recovery of the Primordial Matter Power Spectrum
• A tensor theory of space-time as a strained material continuum
• Beta-Skeleton Analysis of the Cosmic Web
• Dissipative dark matter and the rotation curves of dwarf galaxies
• Constraints on Quintessence From Using Cosmological Data
• Evolving dark energy equation of state and CMB/LSS cross-correlation
• Constraints on the DGP Universe Using Observational Hubble parameter
• Using the filaments in the LCRS to test the LambdaCDM model
• Non-comoving Cosmology
• Extension and estimation of correlations in Cold Dark Matter models
• Constraints on self-interacting Bose-Einstein condensate dark matter using large-scale observables
• Improved calculation of relic gravitational waves
• Noether symmetries and duality transformations in cosmology
• Dynamics of Quintessential Inflation
• What it takes to measure a fundamental difference between dark matter and baryons: the halo velocity anisotropy
• Markov-chain reconstruction of the 2dF Galaxy Redshift Survey real-space power spectrum
• A New Type of Dark Energy Model
• Measurement of Redshift Space Power Spectrum for BOSS galaxies and the Growth Rate at redshift 0.57
• Frequent Spin Reorientation of Galaxies due to Local Interactions
• How do galactic winds affect the Lyalpha forest?
• Tracing the cosmic velocity field at z ~ 0.1 from galaxy luminosities in the SDSS DR7
• Galaxy redshift abundance periodicity from Fourier analysis of number counts $N(z)$ using SDSS and 2dF GRS galaxy surveys
• Distance-redshift from an optical metric that includes absorption
• Extragalactic Point Source Search in WMAP 61 and 94 GHz Data
• Cosmological constraints on polytropic gas model
• Internal Extinction in the SDSS Late-Type Galaxies
• Parameterizing the Power Spectrum: Beyond the Truncated Taylor Expansion
• Unknown selection effect simulates redshift periodicity in quasar number counts from Sloan Digital Sky Survey
• Conservative Estimates of the Mass of the Neutrino from Cosmology
• Transverse Wave Propagation in Relativistic Two-fluid Plasmas around Schwarzschild-de Sitter Black Hole
• New constraint on the cosmological background of relativistic particles
• Gravitational Lensing Constraints on Dynamical and Coupled Dark Energy
• A Study of Environmental Effects on Galaxy Spin Using MaNGA Data
• Out of sight, out of mind? The impact of correlated clustering in substructure lensing
• Network Analysis of Cosmic Structures : Network Centrality and Topological Environment
• Possible features of galactic halo with electric field and observational constraints
• Probing Dark Energy with Supernovae : a concordant or a convergent model?
• Dynamical friction in Bose-Einstein condensed self-interacting dark matter at finite temperatures, and the Fornax dwarf spheroidal
• Global dynamics in Einstein-Gauss-Bonnet scalar field cosmology with matter
• The Halo Spin Transition as a Probe of Dark Energy
• Cosmological simulations of self-interacting Bose-Einstein condensate dark matter
• Substructure lensing in galaxy clusters as a constraint on low-mass sterile neutrinos in tensor-vector-scalar theory: The straight arc of Abell 2390
• Constraints on Dark Energy Parameters from Correlations of CMB with LSS
• Star Formation and Supercluster Environment of 107 Nearby Galaxy Clusters
• On general features of warm dark matter with reduced relativistic gas
• Bayesian power-spectrum inference with foreground and target contamination treatment
• The nature of the SDSS galaxies in various classes based on morphology, colour and spectral features - II. Multi-wavelength properties
• Constraints on the velocity profiles of galaxies from strong lensing statistics and semi-analytical modelling of galaxy formation
• Cosmological neutrino mass limit and the dynamics of dark energy
• Catch Me if You Can: Biased Distribution of Ly$\alpha$-emitting Galaxies according to the Viewing Direction
• Evolution of dark matter velocity dispersion
• Cosmological constraints in the presence of ionizing and resonance radiation at recombination
• Dynamics and constraints of the dissipative Liouville cosmology
• Dark matter interacts with variable vacuum energy
• Dark Energy Models With Variable Equation Of State Parameter
• Autocorrelations of stellar light and mass at z~0 and ~1: From SDSS to DEEP2
• Entrainment of Hot Gas into Cold Streams: The Origin of Excessive Star-formation Rates at Cosmic Noon
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). The matter density and baryon fraction from the galaxy power spectrum at redshift $0.6<z<1.1$
• Constraining a double component dark energy model using type Ia supernovae data
• Stability of a modified Jordan-Brans-Dicke theory in the dilatonic frame
• Effects of a time-varying color-luminosity parameter $\beta$ on the cosmological constraints of modified gravity models
• Cosmological Constraints on the DGP braneworld model with Gamma-ray bursts
• Matter Power Spectrum for Convex Quartessence
• The Fastest Galaxy Evolution in an Unbiased Compact Group Sample with WISE
• Testing Dark Energy with the Advanced Liquid-Mirror Probe of Asteroids, Cosmology and Astrophysics
• Instability in interacting dark sector: An appropriate Holographic Ricci dark energy model
• Cosmic Web Dissection in Fuzzy Dark Matter Cosmologies
• Distances of Quasars and Quasar-Like Galaxies: Further Evidence that QSOs may be Ejected from Active Galaxies
• Delayed Recombination and Standard Rulers
• Correlation function: biasing and fractal properties of the cosmic web
• Weighing neutrinos in the presence of a running primordial spectral index
• The Integrated Sachs-Wolfe Effect in Time Varying Vacuum Model
• Impact of cosmic filaments on the gas accretion rate of dark matter halos
• How accurate is our knowledge of galaxy bias?
• Using machine learning to compress the matter transfer function $T(k)$
• Constraints from observational data for a running cosmological constant and warm dark matter with curvature
• The luminosity bias relation from filaments in the Sloan Digital Sky Survey Data Release Four
• Modifying Gravity at Low Redshift
• The large-scale structure around the Fornax-Eridanus Complex
• Probing dark matter caustics with weak lensing
• A Halo Occupation Interpretation Of Quasars At $z\sim 1.5$ Using Very Small Scale Clustering Information
• Surveying the dark side
• Retrieving the three-dimensional matter power spectrum and galaxy biasing parameters from lensing tomography
• Searching for MgII absorbers in and around galaxy clusters
• MEDUSA: Minkowski functionals estimated from Delaunay tessellations of the three-dimensional large-scale structure
• Satellites in the field and lens galaxies: SDSS/COSMOS vs. SLACS/CLASS
• A minimal set of invariants as a systematic approach to higher order gravity models
• A Dark Energy Model in Lyra Manifold
• Dark energy, integrated Sachs-Wolfe effect and large-scale magnetic fields
• Dark Energy Nature in Logarithmic $f(R,T)$ Cosmology
• Plasma dark matter direct detection
• Modeling galactic halos with predominantly quintessential matter
• Peaks and dips in Gaussian random fields: a new algorithm for the shear eigenvalues, and the excursion set theory
• Fractal Approach to Large-Scale Galaxy Distribution
• On the Hojman conservation quantities in Cosmology
• Clusters of galaxies: setting the stage
• Dynamical Dark Energy model parameters with or without massive neutrinos
• AMICO galaxy clusters in KiDS-DR3: Cosmological constraints from angular power spectrum and correlation function
• Non-commutative Power-law Inflation: Mode Equation and Spectra Index
• Field Theory of the Correlation Function of Mass Density Fluctuations for Self-Gravitating Systems
• Cosmology With A Dark Refraction Index
• Modular thermal inflation without slow-roll approximation
• Geometric and dynamic distortions in anisotropic galaxy clustering
• Nontrivial Geometries: Bounds on the Curvature of the Universe
• A Coarse-Grained Field Theory for Density Fluctuations and Correlation Functions of Galactic Objects
• Minisuperspace Quantization of $f\left(T,B\right)$ Cosmology
• The Dynamics of Inhomogeneous Cosmologies
• Wide Field Surveys and Astronomical Discovery Space
• Generalized models of unification of dark matter and dark energy
• Bianchi type-VI anisotropic dark energy model with varying EoS parameter
• Analysis of the Spatial Distribution of Galaxies by Multiscale Methods
• Probing galaxy density profiles with future supernova surveys
• Can Measurements of Electric Dipole Moments Determine the Seesaw Parameters?
• Dissecting a miniature universe: A multi-wavelength view of galaxy quenching in the Shapley supercluster
• A Deep Redshift Survey of the Perseus Cluster: Spatial Distribution and Kinematics of Galaxies
• Cosmological Parameter Estimation from the Two-Dimensional Genus Topology -- Measuring the Expansion History using the Genus Amplitude as a Standard Ruler
• Observational tests for oscillating expansion rate of the Universe
• Orbital Dependence of Galaxy Properties in Satellite Systems of Galaxies
• Constraints on $\Lambda (t)$-cosmology with power law interacting dark sectors
• Relaxing the Cosmological Constraints on Unparticle Dark Component
• An alternative approach to modelling a cosmic void and its effect on the cosmic microwave background
• Weyl Anomaly and Initial Singularity Crossing
• Entropy and statefinder diagnosis in chameleon cosmology
• Observational constraints on the braneworld model with brane-bulk energy exchange
• Uneven flows: On cosmic bulk flows, local observers, and gravity
• GECO: Galaxy Evolution COde - A new semi-analytical model of galaxy formation
• Probing for variation of neutrino mass with current observations
• Dark Energy Cosmology with the Alternative Cosmic Microwave Background Data
• Asymptotic behavior of Cardassian cosmologies with exponential potentials
• Implications of cosmic strings with time-varying tension on CMB and large scale structure
• Nonsingular density profiles of dark matter halos and Strong gravitational lensing
• Ellipsoidal configurations in the de Sitter spacetime
• A Modified Generalized Chaplygin Gas as the Unified Dark Matter-Dark Energy Revisited
• Similarity solutions for the Wheeler-DeWitt equation in $f\left(R\right)$-cosmology
• The study of Kantowski-Sachs perfect fluid cosmological model in modified gravity
• Spatial Periodicity of Galaxy Number Counts, CMB Anisotropy, and SNIa Hubble Diagram Based on the Universe Accompanied by a Non-Minimally Coupled Scalar Field
• Higher Dimensional Dark Energy Investigation with Variable $\Lambda$ and $G$
• How dark are filaments in the cosmic web?
• Weak gravity on a $\Lambda$CDM background
• Perturbations of the Yang-Mills field in the universe
• Non-minimally coupled quintessence DE model with a cubic galileon term --A Dynamical System Analysis
• Discrete Spectrum of Inflationary Fluctuations
• Crossing the Phantom Divide in Extended Dvali-Gabadadze-Porrati Gravity
• The current status of observational cosmology
• Scale dependence of the primordial spectrum from combining the three-year WMAP, Galaxy Clustering, Supernovae, and Lyman-alpha forests
• Decaying dark energy in light of the latest cosmological dataset
• Noncommutative wormhole in de Rham-Gabadadze-Tolley like massive gravity
• Unexpected dancing partners: Tracing the coherence between the spin and motion of dark matter halos
• Nonlinear Density Fluctuation Field Theory for Large Scale Structure
• Time Variable Cosmological Constants from the Age of Universe
• $f(T,B)$ gravity in a Friedmann-Lema\^ıtre-Robertson-Walker universe with nonzero spatial curvature
• Time variable $\Lambda$ and the accelerating Universe
• Detection of the velocity shear effect on the spatial distributions of the galactic satellites in isolated systems
• Constraint on dark matter central density in the Eddington inspired Born-Infeld (EiBI) gravity with input from Weyl gravity
• Field Equation of Correlation Function of Mass Density Fluctuation for Self-Gravitating Systems
• The DESI One-Percent Survey: Modelling the clustering and halo occupation of all four DESI tracers with Uchuu
• Holographic Λ(t)CDM model in a non-flat universe
• Using the Mark Weighted Correlation Functions to Improve the Constraints on Cosmological Parameters
• The biasing phenomenon
• Stability analysis in Modified Non-Local Gravity
• On the holographic dark energy in chameleon scalar-tensor cosmology
• Wasserstein distance as a new tool for discriminating cosmologies through the topology of large scale structure
• Massive Neutrinos in Cosmology
• Probing modified gravity in cosmic filaments
• A Cosmological Model with Dark Spinor Source
• A Phantom does not Result from a Backreaction
• Imprints of the cosmic void evolution on the baryon processes inside galaxy haloes
• Fingerprints of Anomalous Primordial Universe on the Abundance of Large Scale Structures
• A Comparison of Quintessence and Nonlinear Born-Infeld Scalar Field Using Gold Supernova data
• Why CMB physics?
• Strong lensing, cosmology and lensing halos
• Evolution of magnetic component in Yang-Mills condensate dark energy models
• Conformal symmetry of gravity and the cosmological constant problem
• Field Equation of Correlation Function of Mass Density Fluctuation for Self-Gravitating Systems
• The Extended Analysis On New Generalized Chaplygin Gas
• Simultaneous effect of Modified Gravity and Primordial Non-Gaussianity in Large Scale Structure Observations
• Lightcone Averaging and Precision Cosmology
• Recovering dark-matter clustering from galaxies with Gaussianization
• The Properties of Type Ia Supernova Host Galaxies from the Sloan Digital Sky Survey
• Clustering and descendants of MUSYC galaxies at z<1.5
• Ghost dark energy with sign-changeable interaction term
• Geometry and Morphology of the Cosmic Web: Analyzing Spatial Patterns in the Universe
• Mixture Models in Astronomy
• Nuclear starburst activity induced by elongated bulges in spiral galaxies
• Age problem in holographic dark energy
• Scalar Field as Dark Energy Accelerating Expansion of the Universe
• The cluster-galaxy cross-spectrum: an additional probe of cosmological and halo parameters
• Collider searches and cosmology in the MSSM with heavy scalars
• Mixed fluid cosmological model in $f(R,T)$ gravity
• Correlation functions in 2D and 3D as descriptors of the cosmic web
• Generalized Model of Interacting Dark Energy and Dark Matter : Phase Portrait Analysis of Evolving Universe
• Structure formation in a Dirac-Milne universe: comparison with the standard cosmological model
• Quintessence models with an oscillating equation of state and their potentials
• Accretion of Self-interacting Scalar Field Dark Matter Onto a Reissner-Nordström Black Hole
• Machine learning unveils the linear matter power spectrum of modified gravity
• Cosmological constraints on $f(Q)$ gravity models in the non-coincident formalism
• LRS Bianchi I model with constant deceleration parameter
• Cosmological surveys with multi-object spectrographs
• Modeling the core-halo mass relation in fuzzy dark matter halos
• Tracking the validity of the quasi-static and sub-horizon approximations in modified gravity
• Relativistic effects in the large-scale structure with effective dark energy fluids
• A Better Way to Reconstruct Dark Energy Models ?
• Quadratic integrals of a multi-scalar cosmological model
• Dark energy in thermal equilibrium with the cosmological horizon?
• Optimal machine-driven acquisition of future cosmological data
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• Probing Ricci dark energy model with perturbations by using WMAP seven-year cosmic microwave background measurements, BAO and Type Ia supernovae
• A Method for the Precision Mass Measurement of the Stop Quark at the International Linear Collider
• A new model for dark matter fluid sphere
• A Viable Dark Fluid Model
• Scenario of Accelerating Universe from the Phenomenological Λ- Models
• Relating information entropy and mass variance to measure bias and non-Gaussianity
• Cosmic filament spin -- II: filament spin and its impact on galaxy spin-filament alignment in a cosmological simulation
• Measuring the Galaxy-Galaxy-Mass Three-point Correlation Function with Weak Gravitational Lensing
• Gravitational Fluctuations as an Alternative to Inflation
• Study on the mapping of halo clustering from real space to redshift space
• Primordial density perturbations with running spectral index: impact on non-linear cosmic structures
• Z-bursts from the Virgo cluster
• A direct probe of cosmological power spectra of the peculiar velocity field and the gravitational lensing magnification from photometric redshift surveys
• A minimal set of invariants as a systematic approach to higher order gravity models: Physical and Cosmological Constraints
• Quantification of the multi-streaming effect in Redshift Space Distortion
• Dark matter annihilation and non-thermal Sunyaev-Zel'dovich effect: I. galaxy cluster
• Inhomogeneous spacetimes in Einstein-æther Cosmology
• Higher Curvature Brane Corrections to the DGP Model
• Modeling Post-Reionization HI Distributions in Fuzzy Dark Matter Cosmologies Using Conditional Normalizing Flows
• Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae
• A search for nontoroidal topological lensing in the Sloan Digital Sky Survey quasar catalog
• The dependence of cluster galaxy properties on the central entropy of their host cluster
• The exact analytical solution of the linear structure growth rate in LCDM cosmology and its cosmological applications
• Dynamics of k-essence in loop quantum cosmology
• A note on observational signatures in superluminal unified dark matter models
• Modified Teleparallel $f(T)$ Gravity, DESI BAO and the $H_0$ Tension
• The Gas Accretion History of Low Mass Halos within the Cosmic Web from Cosmological Simulations
• The morphology of star-forming gas and its alignment with galaxies and dark matter haloes in the EAGLE simulations
• Improved two-point correlation function estimates using glass-like distributions as a reference sample
• Testing the local-void alternative to dark energy using galaxy pairs
• Universal dark halo scaling relation for the dwarf spheroidal satellites
• Cosmic Growth Signatures of Modified Gravitational Strength
• Troubles for observing the inflaton potential
• New cosmological solutions in hybrid metric-Palatini gravity from dynamical symmetries
• Forecasting cosmological parameter constraints using multiple sparsity measurements as tracers of the mass profiles of dark matter haloes
• Investigation of Bouncing Universe and Phantom Crossing in Modified Gravity Coupled with Weyl Tensor and its Reconstruction
• Complementary Cosmological Simulations
• Using simulated Tianqin gravitational wave data and electromagnetic wave data to study the coincidence problem and Hubble tension problem
• Clustering Properties of Low-Luminosity Star-Forming galaxies at z = 0.24 and 0.40 in the Subaru Deep Field
• Alpha Shape Topology of the Cosmic Web
• Local Supercluster Dynamics: External Tidal Impact of the PSCz sample traced by Optimized Numerical Least Action Method
• Anisotropic Cosmological Model with Variable G and Lambda
• A Possible Late Time $\Lambda$CDM-like Background Cosmology in Relativistic MOND Theory
• Isocurvature initial conditions for second order Boltzmann solvers
• Large-scale structure and the Cardassian fluid
• Bayesian Cosmic Web Reconstruction: BARCODE for Clusters
• Multiscalar-torsion Cosmology: Exact and Analytic Solutions from Noether Symmetries
• Gravitational instability of the primordial plasma: anisotropic evolution of structure seeds
• Type Ia supernovae as speed sensors at intermediate redshifts
• $C^{\infty }$ perturbations of FRW models with a cosmological constant
• Unified dark fluid with fast transition: including entropic perturbations
• Dynamical System Analysis of a Three Fluid Cosmological Model : An Invariant Manifold approach
• Phantom Divide Crossing with General Non-minimal Kinetic Coupling
• A very extended reionization epoch ?
• Role of a periodic varying deceleration parameter in Particle creation with higher dimensional FLRW Universe
• A new method to probe the mass density and the cosmological constant using configuration entropy
• Constraining Ultra Light Dark Matter with the Galactic Nuclear Star Cluster
• On the Gravitational Collapse of a Gas Cloud in Presence of Bulk Viscosity
• Dynamical system analysis in multiscalar-torsion cosmology
• Improving Constraint on ${\Omega }_m$ from SDSS Using Marked Correlation Functions
• Growth rate of matter perturbations as a probe of large-scale magnetism
• The galactic spin of AGN galaxies
• A scalar field dark matter model and its role in the large scale structure formation in the Universe
• Can the coincidence problem be solved by a cosmological model of coupled dark energy and dark matter?
• Stability analysis and observational constraints in scalar tensor theory
• Non-Gaussianity of the density distribution in accelerating universes
• Symmetries of Differential equations and Applications in Relativistic Physics
• Constraining Neutrinos and Dark Energy with Galaxy Clustering in the Dark Energy Survey
• The architecture of Abell 1386 and its relationship to the Sloan Great Wall
• Deep learning for cosmological parameter inference from a dark matter halo density field
• Testing the Consistence of Gamma Ray Burst Data-set and Supernovae Union2
• Bayesian analysis of running holographic Ricci dark energy
• Towards a covariant model for cosmic self-acceleration
• Bulk scalar field in brane-worlds with induced gravity inspired by the $\mathcal{L}(R)$ term
• Improving SDSS cosmological constraints through $\beta$-skeleton weighted correlation functions
• Bias-Limited Extraction of Cosmological Parameters
• Sky surveys and deep fields of ground-based and space telescopes
• Determining accurate measurements of the growth rate from the galaxy correlation function in simulations
• An analysis method for time ordered data processing of Dark Matter experiments
• Revisiting metric perturbations in tensor-vector-scalar theory
• Tracing gaseous filaments connected to galaxy clusters: the case study of Abell 2744
• Modeling spatially-resolved galactic H$\alpha$ emission for galaxy clustering
• Cosmic filament spin -- I: a comparative study in observation
• Density fluctuations on mm and Mpc scales
• A spherical hydrodynamical model of cosmic voids in ΛCDM and beyond
• Can anisotropy in the galaxy distribution tell the bias?
• Collapse of spherical overdensities in superfluid models of dark matter
• Cluster-counterpart Voids: Void Identification from Galaxy Density Field
• Latest Cosmological Constraints on Cardassian expansion models including the updated Gamma-ray bursts
• Analytic solution and Noether symmetries for the hyperbolic inflationary model in the Jordan frame
• Evolution of dwarf spheroidal satellites in the common surface-density dark halos
• A method to extract the redshift distortions beta parameter in configuration space from minimal cosmological assumptions
• Cosmic Reionization Study : Principle Component Analysis After Planck
• Clustering properties and halo masses for central galaxies in the local Universe
• The size and shape dependence of the SDSS galaxy bispectrum
• Variational symmetries and superintegrability in multifield cosmology
• Upper limits on neutrino masses from cosmology
• Environmental history of filament galaxies: stellar mass assembly and star-formation of filament galaxies
• Effects of Cosmic Strings on Free Streaming
• Cosmic Microwave Background Polarization
• Observational constraints in scalar tensor theory with tachyonic potential
• The time evolution of bias
• Constraining light fermionic dark matter with binary pulsars
• Structure in Galaxy Distribution. III. Fourier Transforming the Universe
• Clustering of K-band selected local galaxies
• Cosmological constraints from galaxy clustering
• Caught in the cosmic web: environmental effects on subhalo abundance and internal density profiles
• N-body self-consistent stars-halo modeling of the Fornax dwarf galaxy
• Method of determining cosmological parameter ranges with samples of candles with an intrinsic distribution
• CMB lensing forecasts for constraining the primordial perturbations: adding to the CMB temperature and polarization information
• Systematic bias in the estimate of cluster mass and the fluctuation amplitude from cluster abundance statistics
• An Improved Photometric Calibration of the Sloan Digital Sky Survey Imaging Data
• Is it possible to observationally distinguish adiabatic Quartessence from LambdaCDM?
• Interpretable and physics-informed emulator for the linear matter power spectrum from machine learning
• MIMAC : a micro-TPC detector for non-baryonic dark matter search
• Unification of Dark Matter and Dark Energy in a Modified Entropic Force Model
• Dissecting Cosmological Filaments at High Redshifts: Emergence of Spaghetti-type Flow Inside DM Haloes
• A Physical Bias in Cosmological Simulations
• Cosmic evolution with a general Gaussian type scale factor
• Lagrangian Volume Deformations around Simulated Galaxies
• The Cosmic Microwave Background anisotropies: open problems
• From Large Telescopes to the MUltiplexed Survey Telescope (MUST)
• A New Approach to Testing Dark Energy Models by Observations
• Gauss Bonnet dark energy Chaplygin Gas Model
• Spectro-photometric and Weak Lensing Survey of a Supercluster and Typical Field Region -- I. Spectroscopic Redshift Measurements
• A study of multiscale density fluctuation measurements
• Stochastic Order Redshift Technique (SORT): a simple, efficient and robust method to improve cosmological redshift measurements
• Cosmology with Galaxy Correlations
• Exact Solutions and Constraints on the Dark Energy Model in FRW Universe
• Gravitational Fluctuations as an Alternative to Inflation II. CMB Angular Power Spectrum
• Non-vacuum relativistic extensions of MOND using metric theories of gravity with curvature-matter couplings and their applications to the accelerated expansion of the Universe without dark components
• Forecasts for cosmological measurements based on the angular power spectra of AGN and clusters of galaxies in the SRG/eROSITA all-sky survey
• Glass-Like Random Catalogues for Two-Point Estimates on the Light Cone
• Spatial correlations of extended cosmological structures
• Constraints on scalar-tensor theories from observations
• Do data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
• FAST drift scan survey for HI intensity mapping: simulation on hunting HI filament with pairwise stacking
• Can we constrain the evolution of HI bias using configuration entropy?
• Dynamics of the universe as a "test 3-brane" in a 5D bulk
• Pre-heating of the intergalactic medium by gravitational collapse and ultraviolet background
• Comment on "The Real Problem with MOND" by Scott Dodelson, arXiv:1112.1320
• Relativistic stars in $f(Q)$-gravity: Exact analytic solution for the power-law case $f(Q)=Q+b{Q}^{\nu }$
• Toward accurate measurement of property-dependent galaxy clustering I. Comparison of the Vmax method and the "shuffled" method
• Global-String and Vortex Superfluids in a Supersymmetric Scenario
• Stability of HDE model with sign-changeable interaction in Brans-Dicke theory
• On the Size Evolution of a Galactic Disk in Hierarchical Merging of Cold Dark Matter Halos
• K-Inflation with a Dark Energy Coupling
• Massive neutrinos and dark energy
• Faint galaxies in the Zone of Avoidance revealed by JWST/NIRCam
• Cosmological constraints on Neutrino - Dark Matter interactions
• Cosmic Microwave Background anisotropies: the power spectrum and beyond
• Painlevé analysis for the cosmological field equations in Weyl Integrable Spacetime
• On the fairness of the main galaxy sample of SDSS
• Detecting and analysing the topology of the cosmic web with spatial clustering algorithms I: Methods
• Angular Power Spectrum in Modular Invariant Inflation Model
• Scale-free power spectrums in the delayed cosmology
• Non-Gaussianity of the density distribution in accelerating universes II:N-body simulations
• Geometric and thermodynamic properties in Gauss-Bonnet gravity
• The Power Spectrum of Cosmological Number Densities
• Cosmology behind the mask: Constraining the parameters of $\Lambda$CDM with the unmasked galaxy density field from VIPERS
• Non-linear effects in early Universe cosmology
• Tracing the environmental history of observed galaxies via extended fast action minimization method
• Largest scales from the largest galaxy surveys: the pseudo Karhunen-Loève method
• Cosmological Constraints on the Undulant Universe
• Revisiting Agegraphic Dark Energy in Brans-Dicke Cosmology
• An effective fluid description of scalar-vector-tensor theories under the sub-horizon and quasi-static approximations
• Computer Model Calibration using the Ensemble Kalman Filter
• Cosmological constraints from the density gradient weighted correlation function
• Dark Matter Energy Deposition and Production from the Table-Top to the Cosmos
• Constraints on Energy Conditions in $f(R,L_m)$ Gravity
• Shape, alignment, and mass distribution of baryonic and dark-matter halos in one EAGLE simulation
• Dynamics of tachyon dark energy on large scales and its imprint on observed galaxy power spectrum
• An empirical nonlinear power spectrum overdensity-response
• Enhancing Cosmological Constraints by Two-dimensional $\beta$-cosmic-web Weighted Angular Correlation Functions
• Phase space analysis of Rényi Holographic dark energy model
• A Non-parametric Method for the Inference of Halo Occupation Distributions
• Euclid preparation. 3D reconstruction of the cosmic web with simulated Euclid Deep spectroscopic samples
• Dynamical friction shear and rotation in Chaplygin cosmology
• Differentiable Fuzzy Cosmic-Web for Field Level Inference
• It's Always Darkest Before the Cosmic Dawn: Early Results from Novel Tools and Telescopes for 21 cm Cosmology
• Nonrelativistic superfluids in cosmology from a relativistic approach: Revisiting two formulations of superfluidity
• Model-agnostic interpretation of 10 billion years of cosmic evolution traced by BOSS and eBOSS data
• The quintessence field as a perfect cosmic fluid of constant pressure
• Biasing phenomenon
• Constraints on self-interaction cross-sections of dark matter in universal bound states from direct detection