Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation

Abstract

(Abridged) The WMAP 5-year data strongly limit deviations from the minimal LCDM model. We constrain the physics of inflation via Gaussianity, adiabaticity, the power spectrum shape, gravitational waves, and spatial curvature. We also constrain the properties of dark energy, parity-violation, and neutrinos. We detect no convincing deviations from the minimal model. The parameters of the LCDM model, derived from WMAP combined with the distance measurements from the Type Ia supernovae (SN) and the Baryon Acoustic Oscillations (BAO), are: Omega_b=0.0456+-0.0015, Omega_c=0.228+-0.013, Omega_Lambda=0.726+-0.015, H_0=70.5+-1.3 km/s/Mpc, n_s=0.960+-0.013, tau=0.084+-0.016, and sigma_8=0.812+-0.026. With WMAP+BAO+SN, we find the tensor-to-scalar ratio r<0.22 (95% CL), and n_s>1 is disfavored regardless of r. We obtain tight, simultaneous limits on the (constant) equation of state of dark energy and curvature. We provide a set of "WMAP distance priors," to test a variety of dark energy models. We test a time-dependent w with a present value constrained as -0.33<1+w_0<0.21 (95% CL). Temperature and matter fluctuations obey the adiabatic relation to within 8.9% and 2.1% for the axion and curvaton-type dark matter, respectively. The TE and EB spectra constrain cosmic parity-violation. We find the limit on the total mass of neutrinos, sum(m_nu)<0.67 eV (95% CL), which is free from the uncertainty in the normalization of the large-scale structure data. The effective number of neutrino species is constrained as N_{eff} = 4.4+-1.5 (68%), consistent with the standard value of 3.04. Finally, limits on primordial non-Gaussianity are -9<f_{NL}^{local}<111 and -151<f_{NL}^{equil}<253 (95% CL) for the local and equilateral models, respectively.

52 pages, 21 figures, accepted for publication in ApJS. (v2) References added. Cosmological parameters updated with the latest union supernova compilation (Kowalski et al. arXiv:0804.4142)

References in corpus (412)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• Dynamics of dark energy
• HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
• The Cosmological Constant and Dark Energy
• Evidence for oscillation of atmospheric neutrinos
• Efficient Computation of CMB anisotropies in closed FRW models
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
• Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
• Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• Big-Bang nucleosynthesis (Particle Data Group mini-review)
• The Cosmological Parameters 2006
• Cosmological parameters from SDSS and WMAP
• Cosmological Imprint of an Energy Component with General Equation of State
• 4D Gravity on a Brane in 5D Minkowski Space
• Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
• Cosmological Constant - the Weight of the Vacuum
• Direct Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory
• Non-Gaussian features of primordial fluctuations in single field inflationary models
• The Case for a Positive Cosmological Lambda-term
• First Results from KamLAND: Evidence for Reactor Anti-Neutrino Disappearance
• Cosmology and the Fate of Dilatation Symmetry
• Quintessence, Cosmic Coincidence, and the Cosmological Constant
• A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation
• Exploring the Expansion History of the Universe
• Accelerating Universes with Scaling Dark Matter
• The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set
• Baryonic Features in the Matter Transfer Function
• The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
• A Line of Sight Approach to Cosmic Microwave Background Anisotropies
• k-Inflation
• The 3D power spectrum of galaxies from the SDSS
• New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results
• Cosmological Results from High-z Supernovae
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
• Improved Cosmological Constraints from New, Old and Combined Supernova Datasets
• The Ekpyrotic Universe: Colliding Branes and the Origin of the Hot Big Bang
• Exponential potentials and cosmological scaling solutions
• New Constraints on ${\Omega }_M$, ${\Omega }_{\Lambda }$, and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST
• Cosmological Constraints from the SDSS Luminous Red Galaxies
• Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis
• Hybrid Inflation
• MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on angular scales of 10 arcminutes to 5 degrees
• 4-Year COBE DMR Cosmic Microwave Background Observations: Maps and Basic Results
• Non-Gaussianity from Inflation: Theory and Observations
• Quintessence and the Rest of the World
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Inflation
• An All-Sky Analysis of Polarization in the Microwave Background
• Perturbations in k-inflation
• Measurement of Neutrino Oscillation with KamLAND: Evidence of Spectral Distortion
• Weak Gravitational Lensing of the CMB
• DBI in the Sky
• Acoustic Signatures in the Primary Microwave Background Bispectrum
• Massive neutrinos and cosmology
• Cosmological parameter analysis including SDSS Ly-alpha forest and galaxy bias: constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy
• Inflation Dynamics and Reheating
• Solar 8B and hep Neutrino Measurements from 1258 Days of Super-Kamiokande Data
• Statistics of Cosmic Microwave Background Polarization
• Accelerated Universe from Gravity Leaking to Extra Dimensions
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Emission
• Signature of Gravity Waves in Polarization of the Microwave Background
• A General Analytic Formula for the Spectral Index of the Density Perturbations produced during Inflation
• Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis
• Small Scale Cosmological Perturbations: An Analytic Approach
• Cluster Abundance Constraints on Quintessence Models
• Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey
• DarkSUSY: Computing Supersymmetric Dark Matter Properties Numerically
• Cosmology with a Primordial Scaling Field
• Indications of Neutrino Oscillation in a 250 km Long-baseline Experiment
• Effects of Cosmological Moduli Fields on Cosmic Microwave Background
• Reconstructing the Inflaton Potential --- an Overview
• A Probe of Primordial Gravity Waves and Vorticity
• A measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave background
• Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRS
• A general proof of the conservation of the curvature perturbation
• Scalar Speed Limits and Cosmology: Acceleration from D-cceleration
• The primordial density perturbation in the curvaton scenario
• Nongaussian Isocurvature Perturbations from Inflation
• Measurement of the Total Active 8B Solar Neutrino Flux at the Sudbury Neutrino Observatory with Enhanced Neutral Current Sensitivity
• BVRI Light Curves for 22 Type Ia Supernovae
• Asymmetries in the CMB anisotropy field
• Adiabatic and entropy perturbations from inflation
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Tests of Gaussianity
• Second-Order Cosmological Perturbations from Inflation
• Cosmological Signature of New Parity-Violating Interactions
• Cosmological parameters from combining the Lyman-alpha forest with CMB, galaxy clustering and SN constraints
• Large Scale Structure and Supersymmetric Inflation without Fine Tuning
• Constraints on Neutrino Oscillations Using 1258 Days of Super-Kamiokande Solar Neutrino Data
• From Big Crunch to Big Bang
• The inflationary prediction for primordial non-gaussianity
• A high resolution foreground cleaned CMB map from WMAP
• The significance of the largest scale CMB fluctuations in WMAP
• Scrutinizing Exotic Cosmological Models Using ESSENCE Supernova Data Combined with Other Cosmological Probes
• How long before the end of inflation were observable perturbations produced?
• Natural Inflation: Particle Physics Models, Power Law Spectra for Large Scale Structure, and Constraints from COBE
• Primordial Nucleosynthesis in the Precision Cosmology Era
• The Absolute Luminosities of the Calan/Tololo Type Ia Supernovae
• Neutrinos in cosmology
• The Microwave Anisotropy Probe (MAP) Mission
• Ghost Inflation
• A new mechanism for generating density perturbations from inflation
• Observation of muon neutrino disappearance with the MINOS detectors and the NuMI neutrino beam
• The Large Scale Structure of f(R) Gravity
• Detection of non-Gaussianity in the WMAP 1-year data using spherical wavelets
• The axis of evil
• The Three--Point Correlation Function of the Cosmic Microwave Background in Inflationary Models
• Gravitational Lensing Effect on Cosmic Microwave Background Polarization
• The shape of non-Gaussianities
• Inflationary Cosmology
• Is the low-l microwave background cosmic?
• Assisted inflation
• 23 High Redshift Supernovae from the IfA Deep Survey: Doubling the SN Sample at z>0.7
• Weighing Neutrinos with Galaxy Surveys
• The Sunyaev-Zel'dovich angular power spectrum as a probe of cosmological parameters
• Structure Formation with Generalized Dark Matter
• A Parameterized Post-Friedmann Framework for Modified Gravity
• A Measurement of the Angular Power Spectrum of the CMB from l = 100 to 400
• Very weak lensing in the CFHTLS Wide: Cosmology from cosmic shear in the linear regime
• A discriminating probe of gravity at cosmological scales
• Axion Cosmology
• Signatures of Relativistic Neutrinos in CMB Anisotropy and Matter Clustering
• UBVRI Light Curves of 44 Type Ia Supernovae
• High Resolution Observations of the CMB Power Spectrum with ACBAR
• An improved limit on the axion-photon coupling from the CAST experiment
• Limits on non-Gaussianities from WMAP data
• Large-scale structure, the cosmic microwave background, and primordial non-gaussianity
• String Cosmology: A Review
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectra
• Large Scale Structure as a Probe of Gravitational Slip
• The Anisotropy of the Microwave Background to l = 3500: Deep Field Observations with the Cosmic Background Imager
• New Ekpyrotic Cosmology
• Correlation of CMB with large-scale structure: I. ISW Tomography and Cosmological Implications
• The Atmospheric Neutrino Flavor Ratio from a 3.9 Fiducial Kiloton-Year Exposure of Soudan 2
• Extended Mosaic Observations with the Cosmic Background Imager
• Testing the cosmological principle of isotropy: local power spectrum estimates of the WMAP data
• Cosmic Structure Growth and Dark Energy
• SALT: a Spectral Adaptive Light curve Template for Type Ia Supernovae
• Cosmic-Ray Nuclei, Antiprotons and Gamma-rays in the Galaxy: a New Diffusion Model
• Adiabatic Modes in Cosmology
• Multipole Vectors--a new representation of the CMB sky and evidence for statistical anisotropy or non-Gaussianity at 2<=l<=8
• Distinguishing Modified Gravity from Dark Energy
• Dynamics of Linear Perturbations in f(R) Gravity
• The first WIMPy halos
• Crossing the Phantom Divide: Dark Energy Internal Degrees of Freedom
• Improved Calculation of the Primordial Gravitational Wave Spectrum in the Standard Model
• A precision calculation of the effective number of cosmological neutrinos
• Hemispherical power asymmetry in the three-year Wilkinson Microwave Anisotropy Probe sky maps
• Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications
• Evidence of vorticity and shear at large angular scales in the WMAP data: a violation of cosmological isotropy?
• On the large-angle anomalies of the microwave sky
• The Anisotropy of the Microwave Background to l = 3500: Mosaic Observations with the Cosmic Background Imager
• CBR Anisotropy and the Running of the Scalar Spectral Index
• The Uncorrelated Universe: Statistical Anisotropy and the Vanishing Angular Correlation Function in WMAP Years 1-3
• Measuring primordial non-Gaussianity in the cosmic microwave background
• New dark energy constraints from supernovae, microwave background and galaxy clustering
• Enhanced Non-Gaussianity from Excited Initial States
• Observational Constraints on Dark Energy and Cosmic Curvature
• Density Perturbations in the Ekpyrotic Scenario
• Detection of primordial non-Gaussianity (fNL) in the WMAP 3-year data at above 99.5% confidence
• Reconstructing the primordial power spectrum
• A Measurement of the CMB <EE> Spectrum from the 2003 Flight of BOOMERANG
• Cosmology with x-matter
• Observational Tests of Modified Gravity
• Inflation after WMAP3: Confronting the Slow-Roll and Exact Power Spectra with CMB Data
• Minkowski Functionals used in the Morphological Analysis of Cosmic Microwave Background Anisotropy Maps
• A Measurement of the Angular Power Spectrum of the CMB Temperature Anisotropy from the 2003 Flight of Boomerang
• The foundations of observing dark energy dynamics with the Wilkinson Microwave Anisotropy Probe
• Cosmic Temperature Fluctuations from Two Years of COBE DMR Observations
• Probing Cosmic Acceleration Beyond the Equation of State: Distinguishing between Dark Energy and Modified Gravity Models
• Correlated adiabatic and isocurvature perturbations from double inflation
• The non-Gaussian Cold Spot in the 3-year WMAP data
• Global, Exact Cosmic Microwave Background Data Analysis Using Gibbs Sampling
• Primordial trispectrum from inflation
• The Effect of Physical Assumptions on the Calculation of Microwave Background Anisotropies
• Cosmological Parameters from Cosmic Background Imager Observations and Comparisons with BOOMERANG, DASI, and MAXIMA
• Power spectrum estimation from high-resolution maps by Gibbs sampling
• Spontaneous Isotropy Breaking: A Mechanism for CMB Multipole Alignments
• Testing LCDM with the Growth Function δ(a): Current Constraints
• High sensitivity measurements of the CMB power spectrum with the extended Very Small Array
• The essence of quintessence and the cost of compression
• Complete constraints on a nonminimally coupled chaotic inflationary scenario from the cosmic microwave background
• Beyond genus statistics: a unifying approach to the morphology of cosmic structure
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Foreground Emission
• Cosmological constraints on f(R) gravity theories within the Palatini approach
• Neutrino masses and the number of neutrino species from WMAP and 2dFGRS
• Detecting a small perturbation through its non-Gaussianity
• The Angular Dependence of the Three-Point Correlation Function of the Cosmic Microwave Background Radiation as Predicted by Inflationary Cosmologies
• Causality and CPT violation from an Abelian Chern-Simons-like term
• Polarization of the Microwave Background in Reionized Models
• Large-Scale Anisotropic Correlation Function of SDSS Luminous Red Galaxies
• Measuring Statistical isotropy of the CMB anisotropy
• New generalized Chaplygin gas as a scheme for unification of dark energy and dark matter
• Cosmological Perturbations From Inhomogeneous Reheating, Freeze-Out, and Mass Domination
• Matter Effects in Upward-Going Muons and Sterile Neutrino Oscillations
• Searching for CPT Violation with Cosmic Microwave Background Data from WMAP and BOOMERANG
• The Cosmic Microwave Background Bispectrum and Inflation
• Lorentz-violating electrodynamics and the cosmic microwave background
• Isocurvature Perturbations in Multiple Inflationary Models
• Multi-Throat Brane Inflation
• Deuterium Abundance in the Most Metal-Poor Damped Lyman alpha System: Converging on Omega_baryons
• Non-Gaussian Signatures in the Temperature Fluctuation Observed by the Wilkinson Microwave Anisotropy Probe
• The Imprint of Gravitational Waves on the Cosmic Microwave Background
• Testing for Non-Gaussianity in the Wilkinson Microwave Anisotropy Probe Data: Minkowski Functionals and the Length of the Skeleton
• The Angular Trispectra of CMB Temperature and Polarization
• Cosmic microwave background measurements can discriminate among inflation models
• Angular Trispectrum of CMB Temperature Anisotropy from Primordial Non-Gaussianity with the Full Radiation Transfer Function
• The non-Gaussian Cold Spot in WMAP: significance, morphology and foreground contribution
• Pyrotechnic Universe
• SDSS galaxy bias from halo mass-bias relation and its cosmological implications
• The Inflationary Trispectrum for Models with Large Non-Gaussianities
• Asymmetries in the local curvature of the WMAP data
• Inflation and WMAP three year data: Features have a Future!
• Neutrino masses and the dark energy equation of state - relaxing the cosmological neutrino mass bound
• Non-Gaussianity of the derived maps from the first-year WMAP data
• Cosmic Density Perturbations from Late-Decaying Scalar Condensations
• Effective number of neutrinos and baryon asymmetry from BBN and WMAP
• A Cosmic Microwave Background feature consistent with a cosmic texture
• Possible evidence for an inverted temperature-density relation in the intergalactic medium from the flux distribution of the Lyman-alpha forest
• A measurement of the polarization-temperature angular cross power spectrum of the Cosmic Microwave Background from the 2003 flight of BOOMERANG
• Primordial power spectrum from WMAP
• Observational constraints on the curvaton model of inflation
• Non-Gaussianities in New Ekpyrotic Cosmology
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Beam Profiles and Window Functions
• An improved measurement of the flux distribution of the Ly-alpha forest in QSO absorption spectra: the effect of continuum fitting, metal contamination and noise properties
• The Wilkinson Microwave Anisotropy Probe (WMAP) Source Catalog
• Non-Gaussianity from Preheating
• Optical and Infrared Photometry of the Type Ia Supernovae 1991T, 1991bg, 1999ek, 2001bt, 2001cn, 2001cz, and 2002bo
• Dark Energy: the Cosmological Challenge of the Millennium
• Application of Monte Carlo Algorithms to the Bayesian Analysis of the Cosmic Microwave Background
• Primordial Non-Gaussianity and Analytical Formula for Minkowski Functionals of the Cosmic Microwave Background and Large-scale Structure
• Probing polarization states of primordial gravitational waves with CMB anisotropies
• The simplest curvaton model
• Isocurvature bounds on axions revisited
• Figure of Merit for Dark Energy Constraints from Current Observational Data
• The neutrino mass bound from WMAP-3, the baryon acoustic peak, the SNLS supernovae and the Lyman-alpha forest
• The Axis of Evil revisited
• Measurement of the cosmic microwave background bispectrum on the COBE DMR sky maps
• Parametrized Post-Friedmann Signatures of Acceleration in the CMB
• Density perturbations in generalized Einstein scenarios and constraints on nonminimal couplings from the Cosmic Microwave Background
• CMB Anisotropies at Second Order I
• String-inspired cosmology: Late time transition from scaling matter era to dark energy universe caused by a Gauss-Bonnet coupling
• Non-Gaussian Density Fluctuations from Entropically Generated Curvature Perturbations in Ekpyrotic Models
• Polarization of the Microwave Background due to Primordial Gravitational Waves
• Effect on cosmic microwave background polarization of coupling of quintessence to pseudoscalar formed from the electromagnetic field and its dual
• Improved Measurement of the Angular Power Spectrum of Temperature Anisotropy in the CMB from Two New Analyses of BOOMERANG Observations
• Limits on Primordial Non-Gaussianity from Minkowski Functionals of the WMAP Temperature Anisotropies
• Higher-Order Gravitational Perturbations of the Cosmic Microwave Background
• Implications of the Cosmic Background Imager Polarization Data
• Current cosmological bounds on neutrino masses and relativistic relics
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP)Observations: Beam Maps and Window Functions
• Non-gaussianity from the trispectrum in general single field inflation
• Constraining Isocurvature Initial Conditions with WMAP 3-year data
• The Hot and Cold Spots in the WMAP Data are Not Hot and Cold Enough
• Model-Independent Reconstruction of the Primordial Power Spectrum from WMAP Data
• CMB Anisotropies at Second-Order II: Analytical Approach
• Non-Gaussianities from ekpyrotic collapse with multiple fields
• Gravitational Leptogenesis and Its Signatures in CMB
• Constraining Neutrino Masses by CMB Experiments Alone
• Higher Criticism Statistic: Detecting and Identifying Non-Gaussianity in the WMAP First Year Data
• Optimal Estimation of Non-Gaussianity
• Cosmology with High-redshift Galaxy Survey: Neutrino Mass and Inflation
• Constraints on Dark Energy from Supernovae, Gamma Ray Bursts, Acoustic Oscillations, Nucleosynthesis and Large Scale Structure and the Hubble constant
• Wavelets and WMAP non-Gaussianity
• Primordial Neutrinos
• A late-time transition in the cosmic dark energy?
• Comparing Infrared Dirac-Born-Infeld Brane Inflation to Observations
• CMB polarization as a direct test of Inflation
• A preference for a non-zero neutrino mass from cosmological data
• Comparing Brane Inflation to WMAP
• Lattice calculation of non-Gaussianity from preheating
• Neutrino Mass and Baryon Asymmetry from Dirac Seesaw
• Optical and Infrared Photometry of the Type Ia Supernovae 1999da, 1999dk, 1999gp, 2000bk, and 2000ce
• Bounds on isocurvature perturbations from CMB and LSS data
• Observational bounds on the cosmic radiation density
• A CPT anomaly
• Reconstructing the primordial power spectrum - a new algorithm
• Finding Evidence for Massive Neutrinos using 3D Weak Lensing
• Optical and Infrared Photometry of the Nearby Type Ia Supernovae 1999ee, 2000bh, 2000ca, and 2001ba
• The CDM isocurvature perturbation in the curvaton scenario
• The Lyman-alpha forest and WMAP year three
• Correlated mixtures of adiabatic and isocurvature cosmological perturbations
• Bayesian model selection and isocurvature perturbations
• Inflation versus Cyclic Predictions for Spectral Tilt
• Improved Measurements of the CMB Power Spectrum with ACBAR
• Cosmic Microwave Background anisotropies from second order gravitational perturbations
• Multipole vector anomalies in the first-year WMAP data: a cut-sky analysis
• Constraints on mode couplings and modulation of the CMB with WMAP data
• Constraining Inflation with Cosmic Microwave Background Polarization
• Correlated Primordial Perturbations in Light of CMB and LSS Data
• Statistical Isotropy of the Wilkinson Microwave Anisotropy Probe Data: A Bipolar Power Spectrum Analysis
• Constraints on CPT violation from WMAP three year polarization data: a wavelet analysis
• Bianchi Type VII_h Models and the WMAP 3-year Data
• Indication for Primordial Anisotropies in the Neutrino Background from WMAP and SDSS
• Must Cosmological Perturbations Remain Non-Adiabatic After Multi-Field Inflation?
• Testing Primordial Non-Gaussianity in CMB Anisotropies
• Small Scale Perturbations in a General MDM Cosmology
• On using the CMB shift parameter in tests of models of dark energy
• Constraints on a mixed inflaton and curvaton scenario for the generation of the curvature perturbation
• BPS Branes in Cosmology
• Minkowski Functional Description of Microwave Background Gaussianity
• Very Large Primordial Non-Gaussianity from multi-field: Application to Massless Preheating
• Intuitive understanding of non-gaussianity in ekpyrotic and cyclic models
• On Minimally-Parametric Primordial Power Spectrum Reconstruction and the Evidence for a Red Tilt
• Neutrino Masses from Cosmological Probes
• A re-analysis of the three-year WMAP temperature power spectrum and likelihood
• Nonequilibrium Corrections to the Spectra of Massless Neutrinos in the Early Universe - Addendum
• Brane inflation and the WMAP data: a Bayesian analysis
• Estimation of Primordial Spectrum with post-WMAP 3 year data
• Bayesian Power Spectrum Analysis of the First-Year WMAP data
• Testing Global Isotropy of Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Data: Temperature Analysis
• Estimation of Polarized Power Spectra by Gibbs sampling
• Mapping the large-scale anisotropy in the WMAP data
• Polarization and Anisotropy of the Microwave Sky
• Correlating anomalies of the microwave sky: The Good, the Evil and the Axis
• Seed perturbations for primordial magnetic fields from MSSM flat directions
• Comparison of Standard Ruler and Standard Candle constraints on Dark Energy Models
• Improved Constraints on the Gravitational Lens Q0957+561. II. Strong Lensing
• Constraints on isocurvature models from the WMAP first-year data
• Linear Power Spectra in Cold+Hot Dark Matter Models: Analytical Approximations and Applications
• Present bounds on the relativistic energy density in the Universe from cosmological observables
• Mimicking Lambda with a spin-two ghost condensate
• Fast Estimator of Primordial Non-Gaussianity from Temperature and Polarization Anisotropies in the Cosmic Microwave Background II: Partial Sky Coverage and Inhomogeneous Noise
• Measuring the cosmological background of relativistic particles with WMAP
• MCMC analysis of WMAP3 and SDSS data points to broken symmetry inflaton potentials and provides a lower bound on the tensor to scalar ratio
• Gravitational lensing of cosmic microwave background anisotropies and cosmological parameter estimation
• Constraints on the cosmic neutrino background
• Neutrino mass limits from SDSS, 2dFGRS and WMAP
• Cosmology of neutrinos and extra light particles after WMAP3
• The initial conditions of the universe: how much isocurvature is allowed?
• Natural Inflation: status after WMAP 3-year data
• Numerical experiments with p F- and q D-strings: the formation of (p,q) bound states
• Testing CPT Symmetry with CMB Measurements
• Impact of Secondary non-Gaussianities on the Search for Primordial Non-Gaussianity with CMB Maps
• Bounds on CDM and neutrino isocurvature perturbations from CMB and LSS data
• The galaxy power spectrum: precision cosmology from large scale structure?
• A sub-horizon framework for probing the relationship between the cosmological matter distribution and metric perturbations
• Squeezing the window on isocurvature modes with the Lyman-alpha forest
• Isocurvature, non-gaussianity and the curvaton model
• Principal Power of the CMB
• Testing for double inflation with WMAP
• Reconstructing the Primordial Spectrum from WMAP Data by the Cosmic Inversion Method
• Cosmological Parameter Constraints as Derived from the Wilkinson Microwave Anisotropy Probe Data via Gibbs Sampling and the Blackwell-Rao Estimator
• Non-parametric reconstruction of the primordial power spectrum at horizon scales from WMAP data
• On Precision Measurement of the Mean Curvature
• Cosmological Neutrino Background Revisited
• Smoothing spline primordial power spectrum reconstruction
• Multiple Methods for Estimating the Bispectrum of the Cosmic Microwave Background with Application to the MAXIMA Data
• The isocurvature fraction after WMAP 3-year data
• A combined analysis of 3D Weak Lensing, Lyman-alpha forest and WMAP year three data
• Hints of Isocurvature Perturbations in the Cosmic Microwave Background?
• WMAP, neutrino degeneracy and non-Gaussianity constraints on isocurvature perturbations in the curvaton model of inflation
• Coleman-Weinberg Potential In Good Agreement With WMAP
• Cleaned Three-Year WMAP CMB Map: Magnitude of the Quadrupole and Alignment of Large Scale Modes
• On Perturbation Spectra of N-flation
• The QMAP and MAT/TOCO Experiments for Measuring Anisotropy in the Cosmic Microwave Background
• Probing Dynamics of Dark Energy with Supernova, Galaxy Clustering and the Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations
• Precision of Inflaton Potential Reconstruction from CMB Using the General Slow-Roll Approximation
• A new search for features in the primordial power spectrum
• Search for non-Gaussianity in pixel, harmonic and wavelet space: compared and combined
• Cosmic Inversion: Reconstructing primordial spectrum from CMB anisotropy
• New constraints on the observable inflaton potential from WMAP and SDSS
• The New Ekpyrotic Ghost
• Testing Cosmology with Cosmic Sound Waves
• 3-point temperature anisotropies in WMAP: Limits on CMB non-Gaussianities and non-linearities
• Contributions of point extragalactic sources to the Cosmic Microwave Background bispectrum
• Testing Gaussian random hypothesis with the cosmic microwave background temperature anisotropies in the three-year WMAP data
• The footprint of large scale cosmic structure on the ultra-high energy cosmic ray distribution
• A Scaling Index Analysis of the WMAP three year data: Signatures of non-Gaussianities and Asymmetries in the CMB
• A Consistency Relation in Cosmology
• Solar System planetary orbital motions and dark matter
• Detecting neutrino mass difference with cosmology
• Point-Source Power in 3 Year Wilkinson Microwave Anisotropy Probe Data
• On using the WMAP distance priors in constraining the time evolving equation of state of dark energy
• Limits on primordial power spectrum resolution: An inflationary flow analysis
• GRB 051221A and Tests of Lorentz Symmetry
• Constraining Cosmological Parameters by the Cosmic Inversion Method
• Extragalactic Foregrounds of the Cosmic Microwave Background: Prospects for the MAP Mission
• Inflaton potential reconstruction without slow-roll
• The integrated bispectrum as a test of CMB non-Gaussianity: detection power and limits on f_NL with WMAP data
• Direct Wavelet Expansion of the Primordial Power Spectrum
• Genus Topology of the Cosmic Microwave Background from the WMAP 3-Year Data
• Bayesian analysis of the low-resolution polarized 3-year WMAP sky maps
• Cosmological Constraints on Isocurvature and Tensor Perturbations
• Wavelet Band Powers of the Primordial Power Spectrum from CMB Data
• A Stochastic Measure for Eternal Inflation
• Non-Gaussianity analysis on local morphological measures of WMAP data
• Optimizing future imaging survey of galaxies to confront dark energy and modified gravity models
• Cosmological neutrino bounds for non-cosmologists
• Measuring the geometry of the Universe in the presence of isocurvature modes
• Determining neutrino properties using future galaxy redshift surveys
• CMB Temperature Polarization Correlation and Primordial Gravitational Waves
• Cosmic Inversion II --An iterative method for reproducing the primordial spectrum from the CMB data--
• Joint constraints on the lepton asymmetry of the Universe and neutrino mass from the Wilkinson Microwave Anisotropy Probe
• Implications of Spacetime Quantization for the Bahcall-Waxman Neutrino Bound
• Measuring the Three Point Correlation Function of the Cosmic Microwave Background
• Topological Twisting of Multiple M2-brane Theory
• Cosmological Problems with Multiple Axion-like Fields
• More on crinkles in the last scattering surface
• Estimating the bispectrum of the Very Small Array data
• Constraining Primordial Non-Gaussianities from the WMAP2 2-1 Cumulant Correlator Power Spectrum
• Bianchi VII_h models and the cold spot texture
• Baryogenesis from Gravitational Decay of TeV-Particles in Theories with Low Scale Gravity
• Cosmological Solutions with Torsion in a Model of de Sitter Gauge Theory of Gravity
• Testing Gaussianity on Archeops Data
• Evolution of the fine-structure constant in the non-linear regime
• Massive Neutrinos in Cosmology
• On the solutions to accelerating cosmologies
• Density perturbations from both the inflaton and the curvaton
• Neutrinos and BBN (and the CMB)

Cited by in corpus (4326)

• Astropy: A Community Python Package for Astronomy
• Planck 2015 results. XIII. Cosmological parameters
• Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• Planck 2013 results. XVI. Cosmological parameters
• Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
• Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
• Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
• f(R) theories
• LSST: from Science Drivers to Reference Design and Anticipated Data Products
• Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
• The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
• Planck 2018 results. X. Constraints on inflation
• Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
• The Average Star Formation Histories of Galaxies in Dark Matter Halos from z=0-8
• Observation of an anomalous positron abundance in the cosmic radiation
• Axion Cosmology
• String Axiverse
• Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
• Planck 2018 results. I. Overview and the cosmological legacy of Planck
• f(T) teleparallel gravity and cosmology
• Dark Matter Candidates from Particle Physics and Methods of Detection
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
• Data Tables for Lorentz and CPT Violation
• Observational Probes of Cosmic Acceleration
• Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived Parameters
• Dark torsion as the cosmic speed-up
• New cosmological constraints on primordial black holes
• Revising the Halofit Model for the Nonlinear Matter Power Spectrum
• Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements
• Planck 2013 results. XXII. Constraints on inflation
• Substructures in hydrodynamical cluster simulations
• Discrete Flavor Symmetries and Models of Neutrino Mixing
• Chandra Cluster Cosmology Project III: Cosmological Parameter Constraints
• KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing
• Cosmology and Fundamental Physics with the Euclid Satellite
• The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations
• A Comprehensive Analysis of Uncertainties Affecting the Stellar Mass - Halo Mass Relation for 0<z<4
• 21-cm cosmology
• Cold dark matter haloes in the Planck era: evolution of structural parameters for Einasto and NFW profiles
• Halos and galaxies in the standard cosmological model: results from the Bolshoi simulation
• The WiggleZ Dark Energy Survey: Joint measurements of the expansion and growth history at z < 1
• Challenges for $\Lambda$CDM: An update
• Monodromy in the CMB: Gravity Waves and String Inflation
• Cosmology and fundamental physics with the Euclid satellite
• Structure and Formation of Elliptical and Spheroidal Galaxies
• Quintom Cosmology: Theoretical implications and observations
• Cosmological simulations of the growth of supermassive black holes and feedback from active galactic nuclei: method and tests
• The physics driving the cosmic star formation history
• The Diversity and Similarity of Simulated Cold Dark Matter Halos
• Dark Matter Annihilation in The Galactic Center As Seen by the Fermi Gamma Ray Space Telescope
• Results from the Final Exposure of the CDMS II Experiment
• Dark Energy
• Galaxy Clustering in the Completed SDSS Redshift Survey: The Dependence on Color and Luminosity
• A Redetermination of the Hubble Constant with the Hubble Space Telescope from a Differential Distance Ladder
• 21cmFAST: A Fast, Semi-Numerical Simulation of the High-Redshift 21-cm Signal
• Varying constants, Gravitation and Cosmology
• Chandra Cluster Cosmology Project II: Samples and X-ray Data Reduction
• How do galaxies populate Dark Matter halos?
• A New Calculation of the Ionizing Background Spectrum and the Effects of HeII Reionization
• Concentration, Spin and Shape of Dark Matter Haloes as a Function of the Cosmological Model: WMAP1, WMAP3 and WMAP5 results
• First-year Sloan Digital Sky Survey-II (SDSS-II) Supernova Results: Hubble Diagram and Cosmological Parameters
• Chemical enrichment in cosmological, smoothed particle hydrodynamics simulations
• Statistics of 207 Lya Emitters at a Redshift Near 7: Constraints on Reionization and Galaxy Formation Models
• The Primordial Inflation Explorer (PIXIE): A Nulling Polarimeter for Cosmic Microwave Background Observations
• The Second Catalog of Active Galactic Nuclei Detected by the Fermi Large Area Telescope
• Clustering of Luminous Red Galaxies IV: Baryon Acoustic Peak in the Line-of-Sight Direction and a Direct Measurement of H(z)
• A glimpse of the end of the dark ages: the gamma-ray burst of 23 April 2009 at redshift 8.3
• Gravitationally Consistent Halo Catalogs and Merger Trees for Precision Cosmology
• Fluctuating Glasma initial conditions and flow in heavy ion collisions
• Primordial Non-Gaussianities from Inflation Models
• The star formation history of mass-selected galaxies in the COSMOS field
• Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
• Age-dating Luminous Red Galaxies observed with the Southern African Large Telescope
• Compaction and Quenching of High-z Galaxies in Cosmological Simulations: Blue and Red Nuggets
• Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Are There Cosmic Microwave Background Anomalies?
• Quasi-Single Field Inflation and Non-Gaussianities
• The Sloan Lens ACS Survey. X. Stellar, Dynamical, and Total Mass Correlations of Massive Early-type Galaxies
• Galactic stellar haloes in the CDM model
• Planck 2013 results. XXIII. Isotropy and statistics of the CMB
• One Hundred First Stars : Protostellar Evolution and the Final Masses
• Cosmology with cosmic shear observations: a review
• The WiggleZ Dark Energy Survey: Survey Design and First Data Release
• The Canada-France High-z Quasar Survey: nine new quasars and the luminosity function at redshift 6
• Model-independent evidence in favor of an end to reionization by z~6
• Electrodynamics with Lorentz-violating operators of arbitrary dimension
• The type IIB string axiverse and its low-energy phenomenology
• The First Galaxies
• The 6dF Galaxy Survey: z \approx 0 measurement of the growth rate and sigma_8
• A Measurement of the Damping Tail of the Cosmic Microwave Background Power Spectrum with the South Pole Telescope
• The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9
• GRB 090423 at a redshift of z~8.1
• Planck 2018 results. VII. Isotropy and Statistics of the CMB
• COLOSSUS: A python toolkit for cosmology, large-scale structure, and dark matter halos
• The Physics of Cosmic Acceleration
• Cosmological Constraints from the Clustering of the Sloan Digital Sky Survey DR7 Luminous Red Galaxies
• Gravitational Wave Tests of General Relativity with Ground-Based Detectors and Pulsar Timing Arrays
• CMB Constraints on WIMP Annihilation: Energy Absorption During the Recombination Epoch
• Simulations on a Moving Mesh: The Clustered Formation of Population III Protostars
• Carnegie Hubble Program: A Mid-Infrared Calibration of the Hubble Constant
• Holographic Dark Energy
• Strong Lensing by Galaxies
• The Baryonic Tully-Fisher Relation of Gas Rich Galaxies as a Test of LCDM and MOND
• Reionization and Cosmology with 21 cm Fluctuations
• Planck 2013 Results. XXIV. Constraints on primordial non-Gaussianity
• SNLS3: Constraints on Dark Energy Combining the Supernova Legacy Survey Three Year Data with Other Probes
• Mergers and Bulge Formation in Lambda-CDM: Which Mergers Matter?
• The Primordial Lithium Problem
• Dissecting the Gravitational Lens B1608+656. II. Precision Measurements of the Hubble Constant, Spatial Curvature, and the Dark Energy Equation of State
• Hidden Charged Dark Matter
• Finite-time future singularities in modified Gauss-Bonnet and $\mathcal{F}(R,G)$ gravity and singularity avoidance
• The First Catalog of Active Galactic Nuclei Detected by the Fermi Large Area Telescope
• Matter and Antimatter in the Universe
• First Dark Matter Results from the XENON100 Experiment
• Bright AGN Source List from the First Three Months of the Fermi Large Area Telescope All-Sky Survey
• Planck 2015 results. XVI. Isotropy and statistics of the CMB
• Gravitationally lensed quasars and supernovae in future wide-field optical imaging surveys
• Standard Model Higgs boson mass from inflation: two loop analysis
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measurements of the growth of structure and expansion rate at z=0.57 from anisotropic clustering
• Equation of state for dark energy in $f(T)$ gravity
• The Enrichment of the Intergalactic Medium with Adiabatic Feedback I: Metal Cooling and Metal Diffusion
• Oscillations in the CMB from Axion Monodromy Inflation
• Gravitational wave background as a probe of the primordial black hole abundance
• Running Inflation in the Standard Model
• Exploring short gamma-ray bursts as gravitational-wave standard sirens
• Baryon Acoustic Oscillations in 2D: Modeling Redshift-space Power Spectrum from Perturbation Theory
• Bolometric luminosities and Eddington ratios of X-ray selected Active Galactic Nuclei in the XMM-COSMOS survey
• The X-ray to optical-UV luminosity ratio of X-ray selected Type 1 AGN in XMM-COSMOS
• Inflation scenario via the Standard Model Higgs boson and LHC
• The Canadian Cluster Comparison Project: detailed study of systematics and updated weak lensing masses
• Non-Gaussianities in Single Field Inflation and their Optimal Limits from the WMAP 5-year Data
• Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS
• The Atacama Cosmology Telescope: Cosmological Parameters from the 2008 Power Spectra
• New Model of Inflation with Non-minimal Derivative Coupling of Standard Model Higgs Boson to Gravity
• Reconstruction of f(R, T) gravity describing matter dominated and accelerated phases
• Standard Model Higgs boson mass from inflation
• Inflationary Universe with Anisotropic Hair
• The distribution of stellar mass in the low-redshift Universe
• Updated Values of Running Quark and Lepton Masses
• Approaches to Understanding Cosmic Acceleration
• Features of heavy physics in the CMB power spectrum
• Ekpyrotic and Cyclic Cosmology
• Reconstructing the history of structure formation using redshift distortions
• On initial conditions for the Hot Big Bang
• A Natural Framework for Chaotic Inflation
• The Quest for B Modes from Inflationary Gravitational Waves
• Measuring the cosmological parameters with the Ep,i-Eiso correlation of Gamma-Ray Bursts
• The Many Manifestations of Downsizing: Hierarchical Galaxy Formation Models confront Observations
• An Upper Limit on the Stochastic Gravitational-Wave Background of Cosmological Origin
• Evidence for the accelerated expansion of the Universe from weak lensing tomography with COSMOS
• Preheating in the Standard Model with the Higgs-Inflaton coupled to gravity
• The Confinement of Star-Forming Galaxies into a Main Sequence through Episodes of Gas Compaction, Depletion, and Replenishment
• A Revised Parallel-Sequence Morphological Classification of Galaxies: Structure and Formation of S0 and Spheroidal Galaxies
• Gamma-ray Light Curves and Variability of Bright Fermi-Detected Blazars
• Hubble Residuals of Nearby Type Ia Supernovae Are Correlated with Host Galaxy Masses
• The Hubble Constant
• Galacticus: A Semi-Analytic Model of Galaxy Formation
• Primordial magnetogenesis
• The Observed Growth of Massive Galaxy Clusters I: Statistical Methods and Cosmological Constraints
• Inflationary cosmology in modified gravity theories
• The WiggleZ Dark Energy Survey: Improved Distance Measurements to z = 1 with Reconstruction of the Baryonic Acoustic Feature
• The formation of the first stars and galaxies
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectra
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). An unprecedented view of galaxies and large-scale structure at 0.5<z<1.2
• The Atacama Cosmology Telescope: Cosmological parameters from three seasons of data
• Eddington-limited accretion and the black hole mass function at redshift 6
• A Measurement of the Cosmic Microwave Background Damping Tail from the 2500-square-degree SPT-SZ survey
• Early star-forming galaxies and the reionization of the Universe
• Galaxy Formation Theory
• The Physics of the Intergalactic Medium
• Glasma flux tubes and the near side ridge phenomenon at RHIC
• New Perspective on Galaxy Clustering as a Cosmological Probe: General Relativistic Effects
• Modeling the Metallicity Distribution of Globular Clusters
• Cosmological constant and vacuum energy: old and new ideas
• Measurement of 21 cm brightness fluctuations at z ~ 0.8 in cross-correlation
• Electromagnetic Transients Powered by Nuclear Decay in the Tidal Tails of Coalescing Compact Binaries
• Radio-Loud Narrow-Line Seyfert 1 as a New Class of Gamma-Ray AGN
• Dark Matter, Baryogenesis and Neutrino Oscillations from Right Handed Neutrinos
• Modeling the Anisotropic Two-Point Galaxy Correlation Function on Small Scales and Improved Measurements of H(z), D_A(z), and f(z)sigma_8(z) from the Sloan Digital Sky Survey DR7 Luminous Red Galaxies
• CMB constraints on Dark Matter models with large annihilation cross-section
• Particle physics models of inflation and curvaton scenarios
• Stellar and total baryon mass fractions in groups and clusters since redshift 1
• The Relation Between SFR and Stellar Mass for Galaxies at 3.5 $\le z\le$ 6.5 in CANDELS
• Dark energy two decades after: Observables, probes, consistency tests
• Reconstruction of $f(T)$ gravity: Rip cosmology, finite-time future singularities and thermodynamics
• Science with the Murchison Widefield Array
• First dark matter search results from a 4-kg CF${}_3$I bubble chamber operated in a deep underground site
• Dark Matter Search Results from the Complete Exposure of the PICO-60 C${}_3$F${}_8$ Bubble Chamber
• Galaxies in LCDM with Halo Abundance Matching: luminosity-velocity relation, baryonic mass-velocity relation, velocity function and clustering
• Axion Cosmology Revisited
• Bayesian Strong Gravitational-Lens Modeling on Adaptive Grids: Objective Detection of Mass Substructure in Galaxies
• Dark Matter Search Results from the PICO-60 C${}_3$F${}_8$ Bubble Chamber
• Toy Models for Galaxy Formation versus Simulations
• Observations of the MIssing Baryons in the warm-hot intergalactic medium
• Large non-Gaussianities with Intermediate Shapes from Quasi-Single Field Inflation
• Absorption line systems in simulated galaxies fed by cold streams
• Cosmological Tests of Gravity
• The Characteristic Star Formation Histories of Galaxies at Redshifts z~2-7
• Supermassive Black Hole Formation by Direct Collapse: Keeping Protogalactic Gas H_2--Free in Dark Matter Halos with Virial Temperatures T_vir >~ 10^4 K
• Cosmological bounds on pseudo Nambu-Goldstone bosons
• Weighing simulated galaxy clusters using lensing and X-ray
• How Massless Neutrinos Affect the Cosmic Microwave Background Damping Tail
• The Effect of Host Galaxies on Type Ia Supernovae in the SDSS-II Supernova Survey
• Evolution of Density Profiles in High-z Galaxies: Compaction and Quenching Inside-Out
• The Baryonic Assembly of Dark Matter Halos
• Evolution of the cosmological mass density of neutral gas from Sloan Digital Sky Survey II - Data Release 7
• The Atacama Cosmology Telescope: Sunyaev Zel'dovich Selected Galaxy Clusters at 148 GHz in the 2008 Survey
• Ionizing Photon Escape Fractions from High Redshift Dwarf Galaxies
• Cosmological simulations of the formation of the stellar haloes around disc galaxies
• Neutrino mass limit from tritium beta decay
• The halo mass function through the cosmic ages
• An Imprint of Super-Structures on the Microwave Background due to the Integrated Sachs-Wolfe Effect
• High-redshift clumpy discs and bulges in cosmological simulations
• The formation of disc galaxies in a LCDM universe
• The WiggleZ Dark Energy Survey: Final data release and cosmological results
• Improved Distances to Type Ia Supernovae with Two Spectroscopic Subclasses
• The Assembly of Supermassive Black Holes at High Redshifts
• Atomic Dark Matter
• The primordial abundance of 4He: evidence for non-standard big bang nucleosynthesis
• Relativistic cosmology and large-scale structure
• Asymptotic freedom in inflationary cosmology with a non-minimally coupled Higgs field
• The Stellar Mass Density and Specific Star Formation Rate of the Universe at z~7
• Measurement of Baryon Acoustic Oscillations in the Lyman-alpha Forest Fluctuations in BOSS Data Release 9
• The Baryon Content of Cosmic Structures
• Holographic dark energy models: A comparison from the latest observational data
• The first ultraviolet quasar stacked spectrum at z=2.4 from WFC3
• LoCuSS: Subaru Weak Lensing Study of 30 Galaxy Clusters
• Increasing evidence for hemispherical power asymmetry in the five-year WMAP data
• The Atacama Cosmology Telescope: The Receiver and Instrumentation
• Evidence for Quadratic Tidal Tensor Bias from the Halo Bispectrum
• Dark Matter Search Results from the PICO-2L C${}_3$F${}_8$ Bubble Chamber
• Semi-Analytic Galaxy Evolution (SAGE): Model Calibration and Basic Results
• nbodykit: an open-source, massively parallel toolkit for large-scale structure
• Cosmological Constraints from Galaxy Clusters in the 2500 square-degree SPT-SZ Survey
• Determination of z~0.8 neutral hydrogen fluctuations using the 21 cm intensity mapping auto-correlation
• Curing singularities in cosmological evolution of F(R) gravity
• Improved measurements of the temperature and polarization of the CMB from QUaD
• The accretion history of dark matter halos III: A physical model for the concentration-mass relation
• HeII Reionization and its Effect on the IGM
• Large-angle anomalies in the CMB
• Cosmological Evolution With Interaction Between Dark Energy And Dark Matter
• Supersymmetry Without Prejudice
• Compact High-Redshift Galaxies Are the Cores of the Most Massive Present-Day Spheroids
• MOJAVE. XVII. Jet Kinematics and Parent Population Properties of Relativistically Beamed Radio-Loud Blazars
• Viscous Cosmology for Early- and Late-Time Universe
• Cosmological Constraints from Sunyaev-Zel'dovich-Selected Clusters with X-ray Observations in the First 178 Square Degrees of the South Pole Telescope Survey
• Particle Models and the Small-Scale Structure of Dark Matter
• Bounce cosmology from $F(R)$ gravity and $F(R)$ bigravity
• Scale invariance, unimodular gravity and dark energy
• Determination of Dark Energy by the Einstein Telescope: Comparing with CMB, BAO and SNIa Observations
• Hunting for Primordial Non-Gaussianity in the Cosmic Microwave Background
• The dust content of galaxies from z = 0 to z = 9
• Keeping the Universe ionised: Photo-heating and the clumping factor of the high-redshift intergalactic medium
• Decaying Dark Matter can explain the electron/positron excesses
• Gauge singlet scalar as inflaton and thermal relic dark matter
• MOJAVE: Monitoring of Jets in Active Galactic Nuclei with VLBA Experiments. VIII. Faraday rotation in parsec-scale AGN jets
• The Coyote Universe II: Cosmological Models and Precision Emulation of the Nonlinear Matter Power Spectrum
• Galaxy Properties from the Ultra-violet to the Far-Infrared: Lambda-CDM models confront observations
• Completing the Census of Ly-alpha Emitters at the Reionization Epoch
• f(R,T) Cosmological Models in Phase Space
• A Hubble Diagram for Quasars
• A Model For Halo Formation With Axion Mixed Dark Matter
• Cosmological Constraints from a Combination of Galaxy Clustering and Lensing -- I. Theoretical Framework
• Dark Matter Halo Profiles of Massive Clusters: Theory vs. Observations
• Mergers in Lambda-CDM: Uncertainties in Theoretical Predictions and Interpretations of the Merger Rate
• Non-singular exponential gravity: a simple theory for early- and late-time accelerated expansion
• Mirror dark matter: Cosmology, galaxy structure and direct detection
• Dark Matter through the Axion Portal
• The tight relation between X-ray and ultraviolet luminosity of quasars
• MOJAVE XIII. Parsec-Scale AGN Jet Kinematics Analysis Based on 19 years of VLBA Observations at 15 GHz
• The Effective Field Theory of Multifield Inflation
• Hylogenesis: A Unified Origin for Baryonic Visible Matter and Antibaryonic Dark Matter
• The WiggleZ Dark Energy Survey: testing the cosmological model with baryon acoustic oscillations at z=0.6
• The effect of neutrinos on the matter distribution as probed by the Intergalactic Medium
• Theoretical Models of Dark Energy
• The Baryonic Acoustic Feature and Large-Scale Clustering in the SDSS LRG Sample
• Phase-space structure in the local dark matter distribution and its signature in direct detection experiments
• Cluster Constraints on f(R) Gravity
• Discriminating Between the Physical Processes that Drive Spheroid Size Evolution
• Breit-Wigner Enhancement of Dark Matter Annihilation
• The z=5 Quasar Luminosity Function from SDSS Stripe 82
• Improved constraints on the primordial power spectrum at small scales from ultracompact minihalos
• Estimators for CMB Statistical Anisotropy
• Holography for Cosmology
• Identifying Elusive Electromagnetic Counterparts to Gravitational Wave Mergers: an end-to-end simulation
• Local-Group tests of dark-matter Concordance Cosmology: Towards a new paradigm for structure formation
• Simultaneous constraints on the growth of structure and cosmic expansion from the multipole power spectra of the SDSS DR7 LRG sample
• Vector Higgs-portal dark matter and the invisible Higgs
• Observational information for f(T) theories and Dark Torsion
• Constraints on Perturbative f(R) Gravity via Neutron Stars
• Instability of anisotropic cosmological solutions supported by vector fields
• Lyman-alpha Cooling Emission from Galaxy Formation
• There's no place like home? Statistics of Milky Way-mass dark matter halos
• Substructure depletion in the Milky Way halo by the disk
• Towards a cosmological neutrino mass detection
• Resonant Non-Gaussianity
• Perturbations in generalized multi-field inflation
• Probing New Physics Models of Neutrinoless Double Beta Decay with SuperNEMO
• The First Billion Years Project: The escape fraction of ionizing photons in the epoch of reionization
• Signatures of Initial State Modifications on Bispectrum Statistics
• The Atacama Cosmology Telescope: Two-Season ACTPol Spectra and Parameters
• Hydrodynamical N-body simulations of coupled dark energy cosmologies
• CLASH: The Concentration-Mass Relation of Galaxy Clusters
• What Do We Know About Lorentz Invariance?
• Can WIMP Dark Matter overcome the Nightmare Scenario?
• The Effects of Gas on Morphological Transformation in Mergers: Implications for Bulge and Disk Demographics
• Dark Matter from R^2-gravity
• Fermi/LAT discovery of gamma-ray emission from a relativistic jet in the narrow-line quasar PMN J0948+0022
• The cluster gas mass fraction as a cosmological probe: a revised study
• Leptonic CP violation
• On the interplay between star formation and feedback in galaxy formation simulations
• Lensing is Low: Cosmology, Galaxy Formation, or New Physics?
• Super-Hubble de Sitter Fluctuations and the Dynamical RG
• Equilateral Non-Gaussianity and New Physics on the Horizon
• Dust of Dark Energy
• Dark Matter Axions Revisited
• Distance Priors from Planck Final Release
• The inert doublet model of dark matter revisited
• Simulations of the Microwave Sky
• Comparison Of Reionization Models: Radiative Transfer Simulations And Approximate, Semi-Numeric Models
• Star Formation in Semi-Analytic Galaxy Formation Models with Multiphase Gas
• Scale-dependent bias induced by local non-Gaussianity: A comparison to N-body simulations
• Non-thermal Dark Matter and the Moduli Problem in String Frameworks
• A Novel Test of the Modified Newtonian Dynamics with Gas Rich Galaxies
• Light inflaton Hunter's Guide
• Asymmetric WIMP dark matter
• Sensitivity of gamma-ray telescopes for detection of magnetic fields in intergalactic medium
• Hubble expansion & Structure Formation in Time Varying Vacuum Models
• Simulations of the Sunyaev-Zel'dovich Power Spectrum with AGN Feedback
• The Tully-Fisher relations of early-type spiral and S0 galaxies
• Unitarizing Higgs Inflation
• Halo mass function and scale-dependent bias from N-body simulations with non-Gaussian initial conditions
• On the Stellar Populations and Evolution of Star-Forming Galaxies at 6.3 < z < 8.6
• Is cosmic acceleration slowing down?
• KiDS-450: Testing extensions to the standard cosmological model
• Self-Accelerating Universe in Galileon Cosmology
• Carnegie Supernova Project: Observations of Type IIn supernovae
• MOJAVE - XIV. Shapes and opening angles of AGN jets
• Massive hidden photons as lukewarm dark matter
• Dynamical Dark Matter: I. Theoretical Overview
• Dark coupling
• Holographic Ricci dark energy: Current observational constraints, quintom feature, and the reconstruction of scalar-field dark energy
• Optimal limits on f_{NL}^{local} from WMAP 5-year data
• Luminosity function and radial distribution of Milky Way Satellites in a LCDM Universe
• Constraints on Dark Matter Annihilation in Clusters of Galaxies with the Fermi Large Area Telescope
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the large-scale two-point correlation function
• Supernova PTF 09uj: A possible shock breakout from a dense circumstellar wind
• Evolution of the atomic and molecular gas content of galaxies
• Understanding higher-order nonlocal halo bias at large scales by combining the power spectrum with the bispectrum
• The Coyote Universe III: Simulation Suite and Precision Emulator for the Nonlinear Matter Power Spectrum
• General Relativity and Cosmology: Unsolved Questions and Future Directions
• Primordial non-Gaussianity and Bispectrum Measurements in the Cosmic Microwave Background and Large-Scale Structure
• Color-Magnitude Relations of Active and Non-Active Galaxies in the Chandra Deep Fields: High-Redshift Constraints and Stellar-Mass Selection Effects
• The First Billion Years project - III: The impact of stellar radiation on the coevolution of Populations II and III
• Measurement of Cosmic Microwave Background Polarization Power Spectra from Two Years of BICEP Data
• Simulating cosmic reionization: How large a volume is large enough?
• The Redshift Evolution of LCDM Halo Parameters: Concentration, Spin, and Shape
• The Carnegie Supernova Project I: analysis of stripped-envelope supernova light curves
• Neutron Stars in f(R) Gravity with Perturbative Constraints
• The velocity function in the local environment from LCDM and LWDM constrained simulations
• Mock galaxy catalogs using the quick particle mesh method
• LRS Bianchi Type I Models with Anisotropic Dark Energy and Constant Deceleration Parameter
• Cosmological Constraints from Strong Gravitational Lensing in Galaxy Clusters
• Revisiting Bimaximal Neutrino Mixing in a Model with S4 Discrete Symmetry
• Probing reheating temperature of the universe with gravitational wave background
• Lyman Alpha Blobs as an Observational Signature of Cold Accretion Streams into Galaxies
• Mass Function Predictions Beyond LCDM
• The X-ray cluster survey with eROSITA: forecasts for cosmology, cluster physics and primordial non-Gaussianity
• RegPT: Direct and fast calculation of regularized cosmological power spectrum at two-loop order
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements and the strong power of normalized growth rate on constraining dark energy
• Higgs searches and singlet scalar dark matter: Combined constraints from XENON 100 and the LHC
• A VLBA survey of the core shift effect in AGN jets I. Evidence for dominating synchrotron opacity
• Mimetic $F(R)$ gravity: inflation, dark energy and bounce
• Early-time light curves of Type Ib/c supernovae from the SDSS-II Supernova Survey
• Small-scale dynamo action during the formation of the first stars and galaxies. I. The ideal MHD limit
• An M Theory Solution to the Strong CP Problem and Constraints on the Axiverse
• Cosmic Flows on 100 Mpc/h Scales: Standardized Minimum Variance Bulk Flow, Shear and Octupole Moments
• Study on anisotropic strange stars in $f(R,T)$ gravity: An embedding approach under simplest linear functional of matter-geometry coupling
• The evolution of the Cosmic Microwave Background Temperature: Measurements of TCMB at high redshift from carbon monoxide excitation
• The Impact of Non-Gaussian Errors on Weak Lensing Surveys
• Conformal symmetry and accelerating cosmology in teleparallel gravity
• First-Year Sloan Digital Sky Survey-II (SDSS-II) Supernova Results: Constraints on Non-Standard Cosmological Models
• Upper Bound of 0.28 eV on the Neutrino Masses from the Largest Photometric Redshift Survey
• Measurements of Secondary Cosmic Microwave Background Anisotropies with the South Pole Telescope
• Deuterium Abundance in the Most Metal-Poor Damped Lyman alpha System: Converging on Omega_baryons
• Fermi Large Area Telescope Observations of Misaligned AGN
• Semi-analytic forecasts for JWST - I. UV luminosity functions at z = 4 - 10
• Observational constraints on an interacting dark energy model
• Measurements of the UV background at 4.6 < z < 6.4 using the quasar proximity effect
• On the relation between AGN gamma-ray emission and parsec-scale radio jets
• Constraining the unexplored period between reionization and the dark ages with observations of the global 21 cm signal
• Cosmological Constraints from a Combination of Galaxy Clustering and Lensing -- III. Application to SDSS Data
• Observables sensitive to absolute neutrino masses. II
• A New Method for Estimating Dark Matter Halo Masses using Globular Cluster Systems
• Pre-galactic metal enrichment - The chemical signatures of the first stars
• Review of local non-Gaussianity from multi-field inflation
• Primordial Curvature Fluctuation and Its Non-Gaussianity in Models with Modulated Reheating
• Statefinder Diagnosis for Ricci Dark Energy
• The Atacama Cosmology Telescope: A Measurement of the Cosmic Microwave Background Power Spectrum at 148 and 218 GHz from the 2008 Southern Survey
• Mass profiles of Galaxy Clusters from X-ray analysis
• X-ray Properties of the First SZE-selected Galaxy Cluster Sample from the South Pole Telescope
• Influence of global cosmological expansion on local dynamics and kinematics
• New physics from the polarised light of the cosmic microwave background
• Quasars Are Not Light-Bulbs: Testing Models of Quasar Lifetimes with the Observed Eddington Ratio Distribution
• Stochastic Gravitational Wave Background from Coalescing Binary Black Holes
• Intracluster stars in simulations with AGN feedback
• Icosahedral (A5) Family Symmetry and the Golden Ratio Prediction for Solar Neutrino Mixing
• The Galaxy Luminosity Function during the Reionization Epoch
• Minimizing the stochasticity of halos in large-scale structure surveys
• Thermodynamics of cosmological horizons in $f(T)$ gravity
• 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
• Warm Dark Matter in Low Scale Left-Right Theory
• Exploring the effects of galaxy formation on matter clustering through a library of simulation power spectra
• Gravity-driven Lyman-alpha blobs from cold streams into galaxies
• On Relating the Genesis of Cosmic Baryons and Dark Matter
• The Atacama Cosmology Telescope: Cosmology from Galaxy Clusters Detected via the Sunyaev-Zel'dovich Effect
• Combining cluster observables and stacked weak lensing to probe dark energy: Self-calibration of systematic uncertainties
• Deducing the nature of dark matter from direct and indirect detection experiments in the absence of collider signatures of new physics
• Using the Full Power of the Cosmic Microwave Background to Probe Axion Dark Matter
• Ghost instabilities of cosmological models with vector fields nonminimally coupled to the curvature
• The Formation Rates of Population III Stars and Chemical Enrichment of Halos during the Reionization Era
• Gravitational-Wave Constraints on the Abundance of Primordial Black Holes
• General CMB and Primordial Bispectrum Estimation I: Mode Expansion, Map-Making and Measures of f_NL
• Heavy Neutrinos and Lepton Flavour Violation in Left-Right Symmetric Models at the LHC
• A Deep HST Search for Escaping Lyman Continuum Flux at z~1.3: Evidence for an Evolving Ionizing Emissivity
• The Population of Giant Clumps in Simulated High-z Galaxies: In-situ and Ex-situ, Migration and Survival
• Mass Calibration and Cosmological Analysis of the SPT-SZ Galaxy Cluster Sample Using Velocity Dispersion ${\sigma }_v$ and X-ray $Y_{\text{X}}$ Measurements
• Measuring Baryon Acoustic Oscillations along the line of sight with photometric redshifs: the PAU survey
• Simple exercises to flatten your potential
• Rotational Support of Giant Clumps in High-z Disc Galaxies
• The Bispectrum in the Effective Field Theory of Large Scale Structure
• D3-brane Potentials from Fluxes in AdS/CFT
• The Delay of Population III Star Formation by Supersonic Streaming Velocities
• Inflation and the Scale Dependent Spectral Index: Prospects and Strategies
• The Black Hole Mass Scale of Classical and Pseudo Bulges in Active Galaxies
• Spectral Energy Distributions of Local Luminous And Ultraluminous Infrared Galaxies
• Large-scale non-Gaussian mass function and halo bias: tests on N-body simulations
• LoCuSS: A Comparison of Cluster Mass Measurements from XMM-Newton and Subaru - Testing Deviation from Hydrostatic Equilibrium and Non-Thermal Pressure Support
• The Canadian Cluster Comparison Project: weak lensing masses and SZ scaling relations
• Breakdown of Semiclassical Methods in de Sitter Space
• A New Approach to Systematic Uncertainties and Self-Consistency in Helium Abundance Determinations
• Growing the first bright quasars in cosmological simulations of structure formation
• The LOFAR window on star-forming galaxies and AGN - curved radio SEDs and IR-radio correlation at $0<z<2.5$
• Discovery of a Giant Lya Emitter Near the Reionization Epoch
• The X-ray Cluster Normalization of the Matter Power Spectrum
• GeV Gamma-Ray Attenuation and the High-Redshift UV Background
• High Performance P3M N-body code: CUBEP3M
• Non-perturbative and self-consistent models of neutron stars in R-squared gravity
• Probing interaction and spatial curvature in the holographic dark energy model
• Observational constraints on cosmological solutions of $f(Q)$ theories
• The Great Observatories Origins Deep Survey: Constraints on the Lyman Continuum Escape Fraction Distribution of Lyman--Break Galaxies at 3.4<z<4.5
• A Measurement of Small Scale Structure in the 2.2 < z < 4.2 Lyman-alpha Forest
• Commissioning Run of the CRESST-II Dark Matter Search
• Nonparametric Reconstruction of the Dark Energy Equation of State
• Reconstructing the massive black hole cosmic history through gravitational waves
• The large-scale cross-correlation of Damped Lyman Alpha Systems with the Lyman Alpha Forest: First Measurements from BOSS
• Identifications and Photometric Redshifts of the 2 Ms Chandra Deep Field-South Sources
• Hidden On-Shell Mediators for the Galactic Center Gamma-Ray Excess
• Inflationary universe from perfect fluid and $F(R)$ gravity and its comparison with observational data
• The evolution of active galactic nuclei and their spins
• The properties of satellite galaxies in simulations of galaxy formation
• PAndAS' cubs: discovery of two new dwarf galaxies in the surroundings of the Andromeda and Triangulum galaxies
• On the importance of heavy fields during inflation
• Slow-roll inflation with a Gauss-Bonnet correction
• Improved dark matter search results from PICO-2L Run 2
• The radio/gamma-ray connection in Active Galactic Nuclei in the era of the Fermi Large Area Telescope
• The Influence of Modification of Gravity on the Dynamics of Radiating Spherical Fluids
• The Obscured Fraction of AGN in the XMM-COSMOS Survey: A Spectral Energy Distribution Perspective
• Giant Clumps in Simulated High-z Galaxies: Properties, Evolution and Dependence on Feedback
• Probing modifications of General Relativity using current cosmological observations
• The Detectability of Lyman Alpha Emission from Galaxies during the Epoch of Reionization
• Direct measurement of dark matter halo ellipticity from two-dimensional lensing shear maps of 25 massive clusters
• Cosmic Birefringence from Planck Data Release 4
• Ultradeep Infrared Array Camera Observations of sub-L* z~7 and z~8 Galaxies in the Hubble Ultra Deep Field: the Contribution of Low-Luminosity Galaxies to the Stellar Mass Density and Reionization
• Global structure and kinematics of stellar haloes in cosmological hydrodynamic simulations
• First Results from Z-FOURGE: Discovery of a Candidate Cluster at z = 2.2 in COSMOS
• Crossing of the phantom divide in modified gravity
• Non-linear isocurvature perturbations and non-Gaussianities
• Improved Limits on Spin-Dependent WIMP-Proton Interactions from a Two Liter CF${}_3$I Bubble Chamber
• Models for Little Rip Dark Energy
• The Shapes and Alignments of Dark Matter Halos
• Heavy fields, reduced speeds of sound and decoupling during inflation
• Quasars as standard candles I: The physical relation between disc and coronal emission
• Cosmic Evolution of Size and Velocity Dispersion for Early Type Galaxies
• Constraints on the induced gravitational wave background from primordial black holes
• Balance among gravitational instability, star formation, and accretion determines the structure and evolution of disk galaxies
• Gravitational waves from an early matter era
• Asymptotically Safe Inflation
• The Hunt for New Physics at the Large Hadron Collider
• Structure formation from non-Gaussian initial conditions: multivariate biasing, statistics, and comparison with N-body simulations
• Entropic cosmology for a generalized black-hole entropy
• Optical-to-virial velocity ratios of local disk galaxies from combined kinematics and galaxy-galaxy lensing
• How to Zoom: Bias, Contamination, and Lagrange Volumes in Multimass Cosmological Simulations
• Primordial non-Gaussianity, scale-dependent bias, and the bispectrum of galaxies
• MOJAVE: Monitoring of Jets in Active Galactic Nuclei with VLBA Experiments. XI. Spectral distributions
• A new viable region of the inert doublet model
• Observational constraints on Galileon cosmology
• Testing Parity-Violating Mechanisms with Cosmic Microwave Background Experiments
• No further gravitational wave modes in $F(T)$ gravity
• An Electron Fixed Target Experiment to Search for a New Vector Boson A' Decaying to e+e-
• Complete Cosmic History with a dynamical Lambda(H) term
• Evidence of Gunn-Peterson damping wings in high-z quasar spectra: strengthening the case for incomplete reionization
• The impact of baryons on the spins and shapes of dark matter haloes
• Suzaku Observation of Abell 1689: Anisotropic Temperature and Entropy Distributions Associated with the Large-Scale Structure
• Supermassive black holes do not correlate with dark matter halos of galaxies
• Cosmological parameters from large scale structure - geometric versus shape information
• The effect of peculiar velocities on supernova cosmology
• Dark Matter Searches with Astroparticle Data
• Polarized Blazar X-rays imply particle acceleration in shocks
• The most extreme ultraluminous X-ray sources: evidence for intermediate-mass black holes?
• Inflation and primordial non-Gaussianities of "generalized Galileons"
• Fitting the Gamma-Ray Spectrum from Dark Matter with DMFIT: GLAST and the Galactic Center Region
• Dark matter and a new gauge boson through kinetic mixing
• Cluster-galaxy weak lensing
• Astrophysical Probes of Unification
• Bayesian Analysis of Inflation II: Model Selection and Constraints on Reheating
• Non-linear Evolution of Baryon Acoustic Oscillations from Improved Perturbation Theory in Real and Redshift Spaces
• Field Theory at a Lifshitz Point
• Lepton asymmetry and the cosmic QCD transition
• Robust Neutrino Constraints by Combining Low Redshift Observations with the CMB
• Dark Matter Search Results from the PICO-60 CF${}_3$I Bubble Chamber
• Constraints on cosmological models from strong gravitational lensing systems
• Trapped Inflation
• Cosmological evolution in exponential gravity
• Physics searches at the LHC
• Constraining the limiting brightness temperature and Doppler factors for the largest sample of radio bright blazars
• Using the Noether symmetry approach to probe the nature of dark energy
• An algorithm for the direct reconstruction of the dark matter correlation function from weak lensing and galaxy clustering
• Cosmological parameter constraints from SDSS luminous red galaxies: a new treatment of large-scale clustering
• The ACS LCID project. V. The Star Formation History of the Dwarf Galaxy \objectname[]{LGS-3}: Clues for Cosmic Reionization and Feedback
• Constraining Running Non-Gaussianity
• Improved estimation of radiated axions from cosmological axionic strings
• Dark Matter Candidates
• Lunar laser ranging: the millimeter challenge
• Constraints on Hydrodynamical Subgrid Models from Quasar Absorption Line Studies of the Simulated Circumgalactic Medium
• Power spectra from an inflaton coupled to the Gauss-Bonnet term
• Imprints of dark energy on cosmic structure formation: II) Non-Universality of the halo mass function
• Combining perturbation theories with halo models
• Spectral Lags and the Lag-Luminosity Relation: An Investigation with Swift BAT Gamma-ray Bursts
• Probing Cosmology with Weak Lensing Peak Counts
• Structure Formation and Microlensing with Axion Miniclusters
• Efficiency of gas cooling and accretion at the disc-corona interface
• High-precision predictions for the acoustic scale in the non-linear regime
• Thermal production of ultrarelativistic right-handed neutrinos: Complete leading-order results
• Constraints on Dark Matter annihilations from reionization and heating of the intergalactic gas
• Unveiling the corona of the Milky Way via ram-pressure stripping of dwarf satellites
• Inflaton Fragmentation and Oscillon Formation in Three Dimensions
• Suppression and Spatial Variation of Early Galaxies and Minihalos
• Near-zone sizes and the rest frame extreme ultra-violet spectral index of the highest redshift quasars
• A Model of TeV Scale Physics for Neutrino Mass, Dark Matter and Baryon Asymmetry and its Phenomenology
• CMB polarization features from inflation versus reionization
• Discriminating between a Stochastic Gravitational Wave Background and Instrument Noise
• Realistic Simulations of the Galactic Polarized Foreground: Consequences for 21-cm Reionization Detection Experiments
• Strongly Coupled Perturbations in Two-Field Inflationary Models
• The nature of the Diffuse Gamma-Ray Background
• Triplet Scalars and Dark Matter at the LHC
• Reconstructing the Distortion Function for Nonlocal Cosmology
• Holography for inflation using conformal perturbation theory
• The impact of stellar feedback on the structure, size and morphology of galaxies in Milky Way size dark matter haloes
• Axion cold dark matter in non-standard cosmologies
• Smoothly-Rising Star Formation Histories During the Reionization Epoch
• CMB Constraints on Primordial non-Gaussianity from the Bispectrum (f_{NL}) and Trispectrum (g_{NL} and τ_{NL}) and a New Consistency Test of Single-Field Inflation
• Relic densities including Sommerfeld enhancements in the MSSM
• Power of Observational Hubble Parameter Data: a Figure of Merit Exploration
• Fitting the Phenomenological MSSM
• Thermodynamics and classification of cosmological models in the Horava-Lifshitz theory of gravity
• First-year Sloan Digital Sky Survey-II (SDSS-II) supernova results: consistency and constraints with other intermediate-redshift datasets
• The Atacama Cosmology Telescope: A Measurement of the 600< ell <8000 Cosmic Microwave Background Power Spectrum at 148 GHz
• The Matter Bounce Curvaton Scenario
• The QCD nature of Dark Energy
• The Large-Scale Orientations of Disk Galaxies
• Light propagation in statistically homogeneous and isotropic dust universes
• The "in-in" Formalism and Cosmological Perturbations
• Parity violation constraints using 2006-2007 QUaD CMB polarization spectra
• Average observational quantities in the timescape cosmology
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Signs of neutrino mass in current cosmological datasets
• Nonlocal Models of Cosmic Acceleration
• Statistical anisotropy of the curvature perturbation from vector field perturbations
• Thermal production of relativistic Majorana neutrinos: Strong enhancement by multiple soft scattering
• CFHTLenS tomographic weak lensing: Quantifying accurate redshift distributions
• Enhancement of Dark Matter Annihilation via Breit-Wigner Resonance
• Dynamics of Galactic Disks and Mergers at z~1.6: Spatially Resolved Spectroscopy with Keck Laser Guide Star Adaptive Optics
• Local non-Gaussianity from inflation
• Comprehensive Two-Point Analyses of Weak Gravitational Lensing Surveys
• Cosmography with strong lensing of LISA gravitational wave sources
• Spherical collapse in quintessence models with zero speed of sound
• Cluster Mass Calibration at High Redshift: HST Weak Lensing Analysis of 13 Distant Galaxy Clusters from the South Pole Telescope Sunyaev-Zel'dovich Survey
• (Mis-)Interpreting supernovae observations in a lumpy universe
• Scale dependence of local f_NL
• How well can cold-dark-matter substructures account for the observed radio flux-ratio anomalies?
• Gamma-Ray and Parsec-Scale Jet Properties of a Complete Sample of Blazars From the MOJAVE Program
• Density perturbations in general modified gravitational theories
• Planes of satellite galaxies and the cosmic web
• Neutrino Decays over Cosmological Distances and the Implications for Neutrino Telescopes
• Non-Gaussian Spikes from Chaotic Billiards in Inflation Preheating
• A transition from parabolic to conical shape as a common effect in nearby AGN jets
• The Atacama Cosmology Telescope: a measurement of the primordial power spectrum
• On the capture of dark matter by neutron stars
• Probing Primordial Gravitational Waves: Ali CMB Polarization Telescope
• Cosmological Constraints on $f(G)$ Dark Energy Models
• The ACS LCID project. VI. The SFH of the Tucana dSph and the relative ages of the isolated dSph galaxies
• Probing Cosmology with Weak Lensing Minkowski Functionals
• Scant evidence for thawing quintessence
• Modelling redshift space distortions in hierarchical cosmologies
• Primordial features due to a step in the inflaton potential
• Action Dynamics of the Local Supercluster
• Line Transfer through Clumpy, Large-Scale Outflows: Lyman Alpha Absorption and Halos around Starforming Galaxies
• Volume Modulus Inflation and the Gravitino Mass Problem
• Formation of massive protostars in atomic cooling haloes
• AGNfitter: A Bayesian MCMC approach to fitting spectral energy distributions of AGN
• PKS 1502+106: a new and distant gamma-ray blazar in outburst discovered by the Fermi Large Area Telescope
• The First Galaxies: Assembly with Black Hole Feedback
• Fermi Large Area Telescope and multi-wavelength observations of the flaring activity of PKS 1510-089 between 2008 September and 2009 June
• Probing Reionization with the 21 cm-Galaxy Cross Power Spectrum
• Quasistars and the cosmic evolution of massive black holes
• Clustering of quasars in SDSS-IV eBOSS : study of potential systematics and bias determination
• X-ray observations of the galaxy cluster PKS 0745-191: To the virial radius, and beyond
• Dynamical Dark Matter: II. An Explicit Model
• The Sensitivity of the Parkes Pulsar Timing Array to Individual Sources of Gravitational Waves
• Six more quasars at redshift 6 discovered by the Canada-France High-z Quasar Survey
• Integrated Dynamical Approach to Relativistic Heavy Ion Collisions
• Updated constraints on the cosmic string tension
• Time dependent couplings in the dark sector: from background evolution to nonlinear structure formation
• On the proper treatment of massless fields in Euclidean de Sitter space
• Was reionization complete by z ~ 5-6?
• Signatures of Non-Gaussianity in the Curvaton Model
• The Dark Universe
• CDM Accelerating Cosmology as an Alternative to LCDM model
• Anomalous parity asymmetry of the Wilkinson Microwave Anisotropy Probe power spectrum data at low multipoles
• Planck pre-launch status: the Planck-LFI programme
• Foregrounds for observations of the cosmological 21 cm line: II. Westerbork observations of the fields around 3C196 and the North Celestial Pole
• Perturbative Lorentz and CPT violation for neutrino and antineutrino oscillations
• Galactic fountains and the rotation of disc-galaxy coronae
• X-ray groups and clusters of galaxies in the Subaru-XMM Deep Field
• Low-threshold analysis of CDMS shallow-site data
• The Atacama Cosmology Telescope: Physical Properties and Purity of a Galaxy Cluster Sample Selected via the Sunyaev-Zel'dovich Effect
• LoCuSS: Calibrating Mass-Observable Scaling Relations for Cluster Cosmology with Subaru Weak Lensing Observations
• Statistics of Satellite Galaxies Around Milky Way-Like Hosts
• Bouncing Cosmology made simple
• Primordial non-Gaussianities in general modified gravitational models of inflation
• An Effective Theory of Dirac Dark Matter
• Observational constraints on viable f(R) parametrizations with geometrical and dynamical probes
• Analysis of broad-lined Type Ic supernovae from the (intermediate) Palomar Transient Factory
• Weak lensing power spectra for precision cosmology: Multiple-deflection, reduced shear and lensing bias corrections
• Thermodynamics in $F(R)$ gravity with phantom crossing
• Dark matter searches with Cherenkov telescopes: nearby dwarf galaxies or local galaxy clusters?
• Quantitative Spectroscopy of Blue Supergiant Stars in the Disk of M81: Metallicity, Metallicity Gradient and Distance
• Comprehensive Observations of the Bright and Energetic Type Iax SN 2012Z: Interpretation as a Chandrasekhar Mass White Dwarf Explosion
• Characterizing Foreground for redshifted 21-cm radiation: 150 MHz GMRT observations
• Semi-analytic forecasts for JWST -- II. physical properties and scaling relations for galaxies at z = 4-10
• Aetherizing Lambda: Barotropic Fluids as Dark Energy
• Coupled dark matter-dark energy in light of near Universe observations
• Adiabatic initial conditions for perturbations in interacting dark energy models
• Measuring the Speed of Dark: Detecting Dark Energy Perturbations
• Planck pre-launch status: High Frequency Instrument polarization calibration
• The Fate of Substructures in Cold Dark Matter Haloes
• Notes on Ghost Dark Energy
• A Finely-Predicted Higgs Boson Mass from A Finely-Tuned Weak Scale
• Reionization simulations powered by GPUs I: the structure of the Ultraviolet radiation field
• Halo Clustering with Non-Local Non-Gaussianity
• Dipolar Dark Matter
• Mass and Hot Baryons in Massive Galaxy Clusters from Subaru Weak Lensing and AMiBA SZE Observations
• Black Hole-Galaxy Correlations without Self-Regulation
• On the Cosmology of Type IIA Compactifications on SU(3)-structure Manifolds
• Non-linear violent disc instability with high Toomre's Q in high-redshift clumpy disc galaxies
• Scale-dependent bias of galaxies and mu-type distortion of the cosmic microwave background spectrum from single-field inflation with a modified initial state
• Constraints on primordial density perturbations from induced gravitational waves
• Hot gas in massive halos drives both mass quenching and environment quenching
• Effective Field Theory and Decoupling in Multi-field Inflation: An Illustrative Case Study
• MOJAVE: XVIII. Kinematics and Inner Jet Evolution of Bright Radio-Loud Active Galaxies
• A Comparison between Semi-Analytic Model Predictions for the CANDELS Survey
• Scalaron the mighty: producing dark matter and baryon asymmetry at reheating
• Mixed axion/neutralino cold dark matter in supersymmetric models
• Redshift space correlations and scale-dependent stochastic biasing of density peaks
• The cosmic web and the orientation of angular momenta
• A Bayesian approach to the semi-analytic model of galaxy formation: methodology
• Discrete dark matter
• Phenomenological Consequences of See-Saw in S4 Based Models
• Testing the Void against Cosmological data: fitting CMB, BAO, SN and H0
• Leptogenesis from first principles in the resonant regime
• Non-Gaussianity beyond slow roll in multi-field inflation
• Non-linear Power Spectrum including Massive Neutrinos: the Time-RG Flow Approach
• More on QCD Ghost Dark Energy
• Generalizing the running vacuum energy model and comparing with the entropic-force models
• Dark Matter as the signal of Grand Unification
• An Accelerating Cosmology Without Dark Energy
• Dark Atoms: Asymmetry and Direct Detection
• Dark stars at the Galactic centre - the main sequence
• Likelihood-Free Cosmological Inference with Type Ia Supernovae: Approximate Bayesian Computation for a Complete Treatment of Uncertainty
• Evidence for a Lower Value for $H_0$ from Cosmic Chronometers Data?
• Trace-anomaly driven inflation in $f(T)$ gravity and in minimal massive bigravity
• Could the Cosmological Recombination Spectrum Help Us Understand Annihilating Dark Matter?
• A Comparison of Six Photometric Redshift Methods Applied to 1.5 Million Luminous Red Galaxies
• Observational constraints on holographic dark energy with varying gravitational constant
• Hubble expansion and structure formation in the "running FLRW model" of the cosmic evolution
• Exact reconstruction with directional wavelets on the sphere
• Curvature vs Distances: testing the FLRW cosmology
• The Impact of Inhomogeneous Reionization on the Satellite Galaxy Population of the Milky Way
• Reheating via a generalized non-minimal coupling of curvature to matter
• Quasars Probing Quasars IV: Joint Constraints on the Circumgalactic Medium from Absorption and Emission
• Constraint on Coupled Dark Energy Models from Observations
• Probability Distribution Functions of Cosmological Lensing: Convergence, Shear, and Magnification
• Subaru Weak Lensing Measurements of Four Strong Lensing Clusters: Are Lensing Clusters Over-Concentrated?
• Simulations of Early Baryonic Structure Formation with Stream Velocity: II. The Gas Fraction
• The accretion history of dark matter halos II: The connections with the mass power spectrum and the density profile
• Neutrino and axion hot dark matter bounds after WMAP-7
• The Inert Doublet Model and Inelastic Dark Matter
• Morphology and Molecular Gas Fractions of Local Luminous Infrared Galaxies as a Function of Infrared Luminosity and Merger Stage
• Nonlinear power spectrum in the presence of massive neutrinos: perturbation theory approach, galaxy bias and parameter forecasts
• On Detecting Halo Assembly Bias with Galaxy Populations
• Signature of primordial non-Gaussianity of phi^3-type in the mass function and bias of dark matter haloes
• How to De-Rotate the Cosmic Microwave Background Polarization
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological constraints from the full shape of the clustering wedges
• keV Neutrino Model Building
• The ATLAS3D Project-- VIII: Modelling the Formation and Evolution of Fast and Slow Rotator Early-Type Galaxies within $\Lambda$CDM
• Inflationary Cosmology as a Probe of Primordial Quantum Mechanics
• N-Body Simulations of DGP and Degravitation Theories
• Dark Energy from the Thermal Sunyaev Zeldovich Power Spectrum
• Optimal Constraints on Local Primordial Non-Gaussianity from the Two-Point Statistics of Large-Scale Structure
• Particle Production During Inflation: Observational Constraints and Signatures
• On the Dark Sector Interactions
• The first (nearly) model-independent constraint on the neutral hydrogen fraction at z~5--6
• A sufficient condition for de Sitter vacua in type IIB string theory
• Bayesian Analysis of Inflation: Parameter Estimation for Single Field Models
• The Environments of High Redshift QSOs
• Viscous dark fluid universe
• Lepton Flavour Violation and theta(13) in Minimal Resonant Leptogenesis
• Cosmological Tests of General Relativity with Future Tomographic Surveys
• Early formation of massive, compact, spheroidal galaxies with classical profiles by violent disc instability or mergers
• High Redshift Metals I.: The Decline of C IV at z > 5.3
• The Atacama Cosmology Telescope: Cross-Correlation of CMB Lensing and Quasars
• A covariant approach to general field space metric in multi-field inflation
• How is Star Formation Quenched in Massive Galaxies?
• Multiwavelength monitoring of the enigmatic Narrow-Line Seyfert 1 PMN J0948+0022 in March-July 2009
• Non-Gaussianity and statistical anisotropy from vector field populated inflationary models
• The evolution of the Compton thick fraction and the nature of obscuration for AGN in the Chandra Deep Field South
• Fractal Dimension as a measure of the scale of Homogeneity
• HI as a Probe of the Large Scale Structure in the Post-Reionization Universe
• Neutrino Interferometry for High-Precision Tests of Lorentz Symmetry with IceCube
• On the Use of Ly-alpha Emitters as Probes of Reionization
• Gamma rays from ultracompact primordial dark matter minihalos
• Neutrino physics from precision cosmology
• Cosmic Distance Duality Relation and the Shape of Galaxy Clusters
• Positrons and antiprotons from inert doublet model dark matter
• Galactic chemical evolution in hierarchical formation models - I. Early-type galaxies in the local Universe
• The WiggleZ Dark Energy Survey: the selection function and z=0.6 galaxy power spectrum
• Kiloparsec-scale Radio Structures in Narrow-line Seyfert 1 Galaxies
• Inflation with multiple sound speeds: a model of multiple DBI type actions and non-Gaussianities
• Estimating the H I gas fractions of galaxies in the local Universe
• Dynamics of the Magellanic Clouds in a LCDM Universe
• H.E.S.S. constraints on Dark Matter annihilations towards the Sculptor and Carina Dwarf Galaxies
• Bayesian analysis of an anisotropic universe model: systematics and polarization
• Energy Conditions and Stability in generalized $f(R)$ gravity with arbitrary coupling between matter and geometry
• The simulated 21 cm signal during the epoch of reionization : full modeling of the Ly-alpha pumping
• Searches for the role of spin and polarization in gravity
• MOJAVE XIX: Brightness Temperatures and Intrinsic Properties of Blazar Jets
• Understanding the Structural Scaling Relations of Early-Type Galaxies
• Identifying true satellites of the Magellanic Clouds
• Collider Constraints on Dipole-Interacting Dark Matter
• The inner structure of haloes in Cold+Warm dark matter models
• Metal-Free Gas Supply at the Edge of Reionization: Late-Epoch Population III Star Formation
• The Faint End of the z=5 Quasar Luminosity Function from the CFHTLS
• Bayesian Selection of sign(mu) within mSUGRA in Global Fits Including WMAP5 Results
• Systematic approach to leptogenesis in nonequilibrium QFT: vertex contribution to the CP-violating parameter
• Holographic Systematics of D-brane Inflation
• Some Anisotropic Dark Energy Models in Bianchi Type-V Space-time
• 3D Velocity and Density Reconstructions of the Local Universe with Cosmicflows-1
• P-nflation: generating cosmic Inflation with p-forms
• Robust Cosmological Bounds on Neutrinos and their Combination with Oscillation Results
• First Season QUIET Observations: Measurements of CMB Polarization Power Spectra at 43 GHz in the Multipole Range 25 <= ell <= 475
• Neutrinos in Non-linear Structure Formation - The Effect on Halo Properties
• Effects of Massive Neutrinos on the Large-Scale Structure of the Universe
• The merger-driven evolution of massive galaxies
• Curvaton with Polynomial Potential
• The universal nature of subhalo accretion
• The Nature of Sub-millimetre Galaxies in Cosmological Hydrodynamic Simulations
• Inflation and non-minimal scalar-curvature coupling in gravity and supergravity
• A Population of X-ray Weak Quasars: PHL 1811 Analogs at High Redshift
• Some Bianchi Type-V Models of Accelerating Universe with Dark Energy
• Common Origin of mu-tau and CP Breaking in Neutrino Seesaw, Baryon Asymmetry, and Hidden Flavor Symmetry
• Gamma-ray Signal from Earth-mass Dark Matter Microhalos
• Role of Cosmic Rays in the Circumgalactic Medium
• BINGO: A code for the efficient computation of the scalar bi-spectrum
• The Source Density and Observability of Pair-Instability Supernovae from the First Stars
• Vector Curvaton with varying Kinetic Function
• The POLARBEAR Experiment
• CMB bispectrum from primordial magnetic fields on large angular scales
• On the quantum fate of singularities in a dark-energy dominated universe
• Matter parity as the origin of scalar Dark Matter
• A public catalogue of stellar masses, star formation and metallicity histories and dust content from the Sloan Digital Sky Survey using VESPA
• Interpreting the Evolution of the Size - Luminosity Relation for Disk Galaxies from Redshift 1 to the Present
• Solar neutrino spectrum, sterile neutrinos and additional radiation in the Universe
• Multiscale cosmology and structure-emerging Dark Energy: A plausibility analysis
• Naturalness and Focus Points with Non-Universal Gaugino Masses
• Analytic Minkowski Functionals of the Cosmic Microwave Background: Second-order Non-Gaussianity with Bispectrum and Trispectrum
• The scale of homogeneity of the galaxy distribution in SDSS DR6
• Simulations of Early Baryonic Structure Formation with Stream Velocity: I. Halo Abundance
• Constraints and analytical solutions of $f(R)$ theories of gravity using Noether symmetries
• The CMB cold spot: texture, cluster or void?
• Ultraviolet Complete Quantum Gravity
• Constraining the interaction strength between dark matter and visible matter: I. fermionic dark matter
• The WiggleZ Dark Energy Survey: constraining galaxy bias and cosmic growth with 3-point correlation functions
• Cosmological and astrophysical constraints from the Lyman-alpha forest flux probability distribution function
• The Horizon Run N-body Simulation: Baryon Acoustic Oscillations and Topology of Large Scale Structure of the Universe
• Cosmokinetics: A joint analysis of Standard Candles, Rulers and Cosmic Clocks
• Strong lensing in the MareNostrum Universe: biases in the cluster lens population
• Can we measure the neutrino mass hierarchy in the sky?
• The non-adiabatic pressure in general scalar field systems
• Mapping the Dark Matter From UV Light at High Redshift: An Empirical Approach to Understand Galaxy Statistics
• A Field Theory Model for Dark Matter and Dark Energy in Interaction
• Future singularities and Teleparallelism in Loop Quantum Cosmology
• Improving measurements of H(z) and Da(z) by analyzing clustering anisotropies
• Voids as a Precision Probe of Dark Energy
• Intense Gamma-Ray Lines from Hidden Vector Dark Matter Decay
• Improved constraints on cosmological parameters from SNIa data
• Galaxy-Scale Strong Lensing Tests of Gravity and Geometric Cosmology: Constraints and Systematic Limitations
• Vector field models of modified gravity and the dark sector
• RadioAstron Observations of the Quasar 3C273: a Challenge to the Brightness Temperature Limit
• The Effective Field Theory of Dark Matter and Structure Formation: Semi-Analytical Results
• The CMB Bispectrum
• Reionization by UV or X-ray sources
• The PN.S Elliptical Galaxy Survey: a standard LCDM halo around NGC 4374?
• Topology and Sizes of HII Regions during Cosmic Reionization
• The Growth of Red Sequence Galaxies in a Cosmological Hydrodynamic Simulation
• A generalized local ansatz and its effect on halo bias
• The cosmic microwave background temperature bispectrum from scalar perturbations induced by primordial magnetic fields
• 1-loop Perturbative Corrections to the Matter and Galaxy Bispectrum with non-Gaussian Initial Conditions
• Harrison--Zeldovich spectrum from conformal invariance
• Radio Counterparts of Compact Binary Mergers detectable in Gravitational Waves: A Simulation for an Optimized Survey
• Evolution of Metric Perturbations in Quintom Bounce model
• The Highest Resolution Mass Map of Galaxy Cluster Substructure To Date Without Assuming Light Traces Mass: LensPerfect Analysis of Abell 1689
• Effects of large-scale structure on the accuracy of weak lensing mass measurements
• UV-protected (Natural) Inflation: Primordial Fluctuations and non-Gaussian Features
• Supermassive Black Hole Formation at High Redshifts via Direct Collapse: Physical Processes in the Early Stage
• The 125 GeV Higgs in the NMSSM in light of LHC results and astrophysics constraints
• Comparison of dark energy models: A perspective from the latest observational data
• Exploring the Energetics of Intracluster Gas with a Simple and Accurate Model
• On the full trispectrum in single field DBI-inflation
• Dynamic vacuum variable and equilibrium approach in cosmology
• Supersymmetric Hybrid Inflation Redux
• A Scale-Dependent Power Asymmetry from Isocurvature Perturbations
• The New Horizon Run Cosmological N-Body Simulations
• Asymmetric Dark Matter and Dark Radiation
• Finite-time singularities in f(R, T) gravity and the effect of conformal anomaly
• Reproducing the Kinematics of Damped Lyman-alpha Systems
• Cosmic history of viable exponential gravity: Equation of state oscillations and growth index from inflation to dark energy era
• Cosmological dynamics of tachyonic teleparallel dark energy
• Sub-eV scalar dark matter through the super-renormalizable Higgs portal
• Consistent lensing and clustering in a low-$S_8$ Universe with BOSS, DES Year 3, HSC Year 1 and KiDS-1000
• Galaxy-galaxy lensing constraints on the relation between baryons and dark matter in galaxies in the Red Sequence Cluster Survey 2
• GUT-inspired SUSY and the muon g-2 anomaly: prospects for LHC 14 TeV
• Current Observational Constraints to Holographic Dark Energy Model with New Infrared cut-off via Markov Chain Monte Carlo Method
• Baryon Content of Massive Galaxy Clusters at z=0-0.6
• Evidence Against Dark Matter Halos Surrounding the Globular Clusters MGC1 and NGC 2419
• The Dynamical and Chemical Evolution of Dwarf Spheroidal Galaxies with GEAR
• On the use of semi-numerical simulations in predicting the 21-cm signal from the epoch of reionization
• Running Spectral Index from Inflation with Modulations
• The Matryoshka Run (II): Time Dependent Turbulence Statistics, Stochastic Particle Acceleration and Microphysics Impact in a Massive Galaxy Cluster
• Neutrino constraints from future nearly all-sky spectroscopic galaxy surveys
• Mimicking dark matter in galaxy clusters through a non-minimal gravitational coupling with matter
• Anisotropic Universe Models with Perfect Fluid and Scalar Field in f(R,T) Gravity
• High Angular Momentum Halo Gas: a Feedback and Code-Independent Prediction of LCDM
• The phenomenological approach to modeling the dark energy
• Investigating dark energy experiments with principal components
• Relative Role of Stars and Quasars in Cosmic Reionization
• Primordial Non-Gaussianities of General Multiple Field Inflation
• The First Galaxies: Assembly of Disks and Prospects for Direct Detection
• Bianchi Type-I Anisotropic Dark Energy Models with Constant Deceleration Parameter
• Can neutralinos in the MSSM and NMSSM scenarios still be light?
• The Cluster Velocity Dispersion of the Abell 2199 cD Halo of NGC 6166
• Signals for Lorentz violation in gravitational waves
• Rapidly Rising Transients from Subaru Hyper Suprime-Cam Transient Survey
• CLASH: Complete Lensing Analysis of the Largest Cosmic Lens MACS J0717.5+3745 and Surrounding Structures
• The Challenge of the Largest Structures in the Universe to Cosmology
• The Lag-Luminosity Relation in the GRB Source-Frame: An Investigation with Swift BAT Bursts
• Dark matter in UED : the role of the second KK level
• Large non-Gaussianities in the Effective Field Theory Approach to Single-Field Inflation: the Bispectrum
• When scalar field is kinetically coupled to the Einstein tensor
• How do galaxies acquire their mass?
• Measurement of the Crab nebula polarization at 90 GHz as a calibrator for CMB experiments
• Dark Force Detection in Low Energy e-p Collisions
• Thermal history of the plasma and high-frequency gravitons
• Observational issues in loop quantum cosmology
• Constraining the evolutionary history of Newton's constant with gravitational wave observations
• Cosmological constant, violation of cosmological isotropy and CMB
• Tracing The Sound Horizon Scale With Photometric Redshift Surveys
• New Neutrino Mass Bounds from Sloan Digital Sky Survey III Data Release 8 Photometric Luminous Galaxies
• Dark Matter with Dirac and Majorana Gaugino Masses
• The Halo Mass Function from Excursion Set Theory. III. Non-Gaussian Fluctuations
• Extended Slow-Roll Conditions and Rapid-Roll Conditions
• On the Issue of the ζSeries Convergence and Loop Corrections in the Generation of Observable Primordial Non-Gaussianity in Slow-Roll Inflation. Part I: the Bispectrum
• What is the (Dark) Matter with Dwarf Galaxies?
• Dark energy and dark matter from nonlocal ghost-free gravity theory
• Connecting massive galaxies to dark matter halos in BOSS - I. Is galaxy color a stochastic process in high-mass halos?
• Effective $F(T)$ gravity from the higher-dimensional Kaluza-Klein and Randall-Sundrum theories
• Testing Models of Intrinsic Brightness Variations in Type Ia Supernovae, and their Impact on Measuring Cosmological Parameters
• De-Rotation of the Cosmic Microwave Background Polarization: Full-Sky Formalism
• Two bright z > 6 quasars from VST ATLAS and a new method of optical plus mid-infra-red colour selection
• Star Formation Feedback and Metal Enrichment History Of The Intergalactic Medium
• The Kinetic Sunyaev-Zel'dovich effect as a probe of the physics of cosmic reionization: the effect of self-regulated reionization
• Hunting for Supermassive Black Holes in Nearby Galaxies with the Hobby-Eberly Telescope
• The mode of gas accretion onto star-forming galaxies
• Some aspects of generalized modified gravity models
• 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
• Gluino NLSP, Dark Matter via Gluino Coannihilation, and LHC Signatures
• On Classification of Models of Large Local-Type Non-Gaussianity
• X-ray and Multiwavelength Insights into the Nature of Weak Emission-Line Quasars at Low Redshift
• Anisotropic Inflation from Charged Scalar Fields
• Does the entropy of the Universe tend to a maximum?
• Relic density and CMB constraints on dark matter annihilation with Sommerfeld enhancement
• Relic gravitational waves from light primordial black holes
• Cosmic microwave background with Brans-Dicke gravity II: constraints with the WMAP and SDSS data
• Relaxation of Blazar Induced Pair Beams in Cosmic Voids
• Large non-Gaussianities in the Effective Field Theory Approach to Single-Field Inflation: the Trispectrum
• Serendipitous discoveries in nonlocal gravity theory
• Evolution of Infrared Luminosity functions of Galaxies in the AKARI NEP-Deep field: Revealing the cosmic star formation history hidden by dust
• Dependence of Barred Galaxy Fraction on Galaxy Properties and Environment
• Constraining the interaction strength between dark matter and visible matter: II. scalar, vector and spin-3/2 dark matter
• Color Dispersion and Milky Way Reddening Among Type Ia Supernovae
• How Far Are We from the Quantum Theory of Gravity?
• The Constrained NMSSM with a 126 GeV Higgs boson: A global analysis
• FLRW solutions in $f(Q)$ theory: the effect of using different connections
• z~7 galaxy candidates from NICMOS observations over the HDF South and the CDF-S and HDF-N GOODS fields
• Testing the dark energy with gravitational lensing statistics
• Consistent Scenarios for Cosmic-Ray Excesses from Sommerfeld-Enhanced Dark Matter Annihilation
• Localizing compact binary inspirals on the sky using ground-based gravitational wave interferometers
• Consistency among distance measurements: transparency, BAO scale and accelerated expansion
• Semi-analytic forecasts for JWST -- IV. Implications for cosmic reionization and LyC escape fraction
• A search for dark matter in events with one jet and missing transverse energy in pp-bar collisions at sqrt(s) = 1.96 TeV
• Slow-Roll Thawing Quintessence
• Simulating Subhalos at High Redshift: Merger Rates, Counts, and Types
• Anisotropic non-Gaussianity from vector field perturbations
• Spectral Energy Distributions of Type 1 AGN in the COSMOS Survey I - The XMM-COSMOS Sample
• Introducing the FirstLight project: UV luminosity function and scaling relations of primeval galaxies
• The ACS LCID project. X. The Star Formation History of IC 1613: Revisiting the Over-Cooling Problem
• A k-essence Model Of Inflation, Dark Matter and Dark Energy
• Constraints on large scale inhomogeneities from WMAP-5 and SDSS: confrontation with recent observations
• A model with interaction of dark components and recent observational data
• Galaxy Bias and its Effects on the Baryon Acoustic Oscillations Measurements
• Resistive Magnetic Field Generation at Cosmic Dawn
• Modified Entropic Force
• The updated luminosity correlations of gamma-ray bursts and cosmological implications
• High-Redshift Metals. II. Probing Reionization Galaxies with Low-Ionization Absorption Lines at Redshift Six
• A Hubble Space Telescope Study of Lyman Limit Systems: Census and Evolution
• M-flation: Inflation From Matrix Valued Scalar Fields
• A Model of Universe Anisotropization
• The cosmic microwave background bispectrum from the non-linear evolution of the cosmological perturbations
• Oscillations in the inflaton potential?
• A Modified Holographic Dark Energy Model with Infrared Infinite Extra Dimension(s)
• Quenching Massive Galaxies with On-the-fly Feedback in Cosmological Hydrodynamic Simulations
• Cosmic Rays from Dark Matter Annihilation and Big-Bang Nucleosynthesis
• What next for the CMSSM and the NUHM: Improved prospects for superpartner and dark matter detection
• F-GAMMA: Variability Doppler factors of blazars from multiwavelength monitoring
• Observational constraints on generalized Proca theories
• Gluonic vacuum, q-theory, and the cosmological constant
• The first gamma-ray outburst of a Narrow-Line Seyfert 1 Galaxy: the case of PMN J0948+0022 in July 2010
• The kinetic dark-mixing in the light of CoGENT and XENON100
• Primordial Non-Gaussianity in the Cosmic Microwave Background
• Overdensities of Y-dropout Galaxies from the Brightest-of-Reionizing Galaxies Survey: A Candidate Protocluster at Redshift z~8
• Dark Energy, Inflation and Extra Dimensions
• Effect of the dilaton field and plasma medium on deflection angle by black holes in Einstein-Maxwell-dilaton-axion theory
• Soft L_e-L_mu-L_tau flavour symmetry breaking and sterile neutrino keV Dark Matter
• Neutral hydrogen optical depth near star-forming galaxies at z~2.4 in the Keck Baryonic Structure Survey
• Spontaneous B-L Breaking as the Origin of the Hot Early Universe
• Broad Line Radio Galaxies Observed with Fermi-LAT: The Origin of the GeV Gamma-Ray Emission
• A Comparison of Thawing and Freezing Dark Energy Parametrizations
• Higher order corrections of the extended Chaplygin gas cosmology with varying $G$ and $\Lambda$
• The ACS LCID project. IX. Imprints of the early Universe in the radial variation of the star formation history of dwarf galaxies
• Two scalar field cosmology: Conservation laws and exact solutions
• A survey of luminous high-redshift quasars with SDSS and WISE II. the bright end of the quasar luminosity function at z ~ 5
• Felix: A Topology based Framework for Visual Exploration of Cosmic Filaments
• A Naturally Large Four-Point Function in Single Field Inflation
• Testing GRBs as Standard Candles
• VERITAS Search for VHE Gamma-ray Emission from Dwarf Spheroidal Galaxies
• Model independent analysis of dark matter points to a particle mass at the keV scale
• Covariance of cross-correlations: towards efficient measures for large-scale structure
• Observational constraints on holographic tachyonic dark energy in interaction with dark matter
• Inflating in a Trough: Single-Field Effective Theory from Multiple-Field Curved Valleys
• Interpreting the unresolved intensity of cosmologically redshifted line radiation
• UV-dropout Galaxies in the GOODS-South Field from WFC3 Early Release Science Observations
• Non-Gaussian Fingerprints of Self-Interacting Curvaton
• How flat can you get? A model comparison perspective on the curvature of the Universe
• Locating the gamma-ray emission region of the flat spectrum radio quasar PKS 1510-089
• Dry Mergers: A Crucial Test for Galaxy Formation
• Directional detection as a strategy to discover Galactic Dark Matter
• Shock Breakout in Type II Plateau Supernovae: Prospects for High Redshift Supernova Surveys
• Fast and accurate mock catalogue generation for low-mass galaxies
• Relativistic Stars in dRGT Massive Gravity
• Black Hole Remnants in the Early Universe
• Inflation with Multi-Vector-Hair: The Fate of Anisotropy
• A first direct measurement of the intergalactic medium temperature around a quasar at z=6
• Understanding black hole mass assembly via accretion and mergers at late times in cosmological simulations
• Sterile Neutrinos in Light of Recent Cosmological and Oscillation Data: a Multi-Flavor Scheme Approach
• The connection between gamma-ray emission and millimeter flares in Fermi/LAT blazars
• A high-significance detection of non-Gaussianity in the WMAP 5-year data using directional spherical wavelets
• Study of possible systematics in the L*X - Ta* correlation of Gamma Ray Bursts
• A VLA search for 5 GHz radio transients and variables at low Galactic latitudes
• New aspects of leptogenesis bounds
• Dark energy model with higher derivative of Hubble parameter
• On Features and Nongaussianity from Inflationary Particle Production
• Parameters in a Class of Leptophilic Dark Matter Models from PAMELA, ATIC and FERMI
• Star Formation History and Chemical Evolution of the Sextans Dwarf Spheroidal Galaxy
• The Unanticipated Phenomenology of the Blazar PKS~2131$-$021: A Unique Super-Massive Black Hole Binary Candidate
• Column Density Profiles of Multi-Phase Gaseous Halos
• X-ray absorption evolution in Gamma-Ray Bursts: intergalactic medium or evolutionary signature of their host galaxies?
• Characterization of the BICEP Telescope for High-Precision Cosmic Microwave Background Polarimetry
• The art of modeling CO, [CI], and [CII] in cosmological galaxy formation models
• The Stellar Mass Growth of Brightest Cluster Galaxies in the IRAC Shallow Cluster Survey
• The roadmap for unification in galaxy group selection:. I. A search for extended X-ray emission in the CNOC2 survey
• Scattering of Dark Matter and Dark Energy
• CMB lensing and primordial non-Gaussianity
• Search for dark matter produced in association with bottom or top quarks in $\sqrt{s}$ = 13 TeV pp collisions with the ATLAS detector
• Third-Order Density Perturbation and One-Loop Power Spectrum in Dark-Energy-Dominated Universe
• The Matryoshka Run: Eulerian Refinement Strategy to Study Statistics of Turbulence in Virialized Cosmic Structures
• Spherical collapse model in dark energy cosmologies
• The ZZ' kinetic mixing in the light of the recent direct and indirect dark matter searches
• Weak lensing Analysis of X-Ray-selected XXL Galaxy Groups and Clusters with Subaru HSC Data
• Cosmic Microwave Background Observables of Small Field Models of Inflation
• The SWELLS Survey. I. A large spectroscopically selected sample of edge-on late-type lens galaxies
• On the Effects of Line-of-Sight Structures on Lensing Flux-ratio Anomalies in a LCDM Universe
• An Estimate of the Primordial Non-Gaussianity Parameter f_NL Using the Needlet Bispectrum from WMAP
• Radiative contribution to neutrino masses and mixing in $\mu \nu$SSM
• Dark matter and sub-GeV hidden U(1) in GMSB models
• Generation of Primordial Magnetic Fields on Linear Over-density Scales
• Dark matter annihilation effects on the first stars
• Inflationary universe from higher-derivative quantum gravity
• The GMRT EoR Experiment: Limits on Polarized Sky Brightness at 150 MHz
• Indirect Detection Analysis: Wino Dark Matter Case Study
• Warm Inflation with a General Form of the Dissipative Coefficient
• Trace-anomaly driven inflation in modified gravity and the BICEP2 result
• Irreversible thermodynamic description of interacting dark energy - dark matter cosmological models
• Fermion Masses and Flavor Mixings in a Model with $S_4$ Flavor Symmetry
• Curvaton Dynamics and the Non-Linearity Parameters in Curvaton Model
• Stellar migrations and metal flows -- Chemical evolution of the thin disc of a simulated Milky Way analogous galaxy
• Standard Clock in Primordial Density Perturbations and Cosmic Microwave Background
• Entropic-force dark energy reconsidered
• Diverse Structural Evolution at z > 1 in Cosmologically Simulated Galaxies
• Seeing Through the Trough: Outflows and the Detectability of Lyman Alpha Emission from the First Galaxies
• Thermodynamics in $f(R)$ gravity in the Palatini formalism
• New Constraints on the Primordial Magnetic Field
• Resonant Destruction as a Possible Solution to the Cosmological Lithium Problem
• Structure formation in a nonlocally modified gravity model
• A geometric description of the non-Gaussianity generated at the end of multi-field inflation
• Tension of the $E_G$ statistic and RSD data with Planck/$\Lambda$CDM and implications for weakening gravity
• Anomalous parity asymmetry of WMAP power spectrum data at low multpoles: is it cosmological or systematics?
• de Sitter Vacua in Type IIB String Theory: Classical Solutions and Quantum Corrections
• A distortion of very--high--redshift galaxy number counts by gravitational lensing
• Constraining the MSSM with universal gaugino masses and implication for searches at the LHC
• Scaling Laws for Dark Matter Halos in Late-Type and Dwarf Spheroidal Galaxies
• Relic density of neutrinos with primordial asymmetries
• LensExtractor: A Convolutional Neural Network in Search of Strong Gravitational Lenses
• Cosmological dynamics with non-linear interactions
• Nuclear Star Clusters from Clustered Star Formation
• Dark matter in the solar system I: The distribution function of WIMPs at the Earth from solar capture
• Constraining cosmological parameters by Gamma Ray Burst X - ray afterglow lightcurves
• Cosmological Parameter Uncertainties from SALT-II Type Ia Supernova Light Curve Models
• A new framework for studying spherically symmetric static solutions in f(R) gravity
• Extra U(1) as natural source of a monochromatic gamma ray line
• Self-similar energetics in large clusters of galaxies
• Primordial gravity wave fossils and their use in testing inflation
• Tensor Detection Severely Constrains Axion Dark Matter
• Model-independent cosmological constraints from the CMB
• Confronting Simulations of Optically Thick Gas in Massive Halos with Observations at z=2-3
• Non-Gaussianity and the Cosmic Microwave Background Anisotropies
• Ekpyrotic Non-Gaussianity -- A Review
• Formation of intermediate-mass black holes as primordial black holes in the inflationary cosmology with running spectral index
• Cosmic variance of the local Hubble flow in large-scale cosmological simulations
• Search for Production of Invisible Final States in Single-Photon Decays of Upsilon(1S)
• Neutrino coupling to cosmological background: A review on gravitational Baryo/Leptogenesis
• The Luminosity Function of Lyman alpha Emitters at Redshift z=7.7
• Low Mass Neutralino Dark Matter in the MSSM with Constraints from $B_s\to {\mu }^{+}{\mu }^{-}$ and Higgs Search Limits
• An MCMC determination of the primordial helium abundance
• The Holographic Universe
• Axion isocurvature fluctuations with extremely blue spectrum
• The Search for a Primordial Magnetic Field
• Supercollapsars and their X-ray Bursts
• Cosmic Bulk Flow and the Local Motion from Cosmicflows-2
• H_2 Suppression with Shocking Inflows: Testing a Pathway for Supermassive Black Hole Formation
• Escape of Lyman-alpha and continuum photons from star-forming galaxies
• A General Study of the Influence of Catastrophic Photometric Redshift Errors on Cosmology with Cosmic Shear Tomography
• De Sitter Universe in Nonlocal Gravity
• Electroweak Beautygenesis: From b {\to} s CP-violation to the Cosmic Baryon Asymmetry
• GRB 091127: The cooling break race on magnetic fuel
• Mini-quenching of $z=4-8$ galaxies by bursty star formation
• The-wiZZ: Clustering redshift estimation for everyone
• Nuclear astrophysics: the unfinished quest for the origin of the elements
• Vibrational level population of H${}_2$ and H${}_2^{+}$ in the early Universe
• Primordial perturbation with a modified dispersion relation
• Three-Point Correlation Functions of SDSS Galaxies: Luminosity and Color Dependence in Redshift and Projected Space
• Leptogenesis in the two right-handed neutrino model revisited
• Observational Constraints on New Exact Inflationary Scalar-field Solutions
• Constraints on the Dark Side of the Universe and Observational Hubble Parameter Data
• Acceleration of Universe by Nonlinear Electromagnetic Fields
• Slow-roll k-essence
• Mass profiles and galaxy orbits in nearby galaxy clusters from the analysis of the projected phase-space
• Cosmology of Holographic and New Agegraphic $f(R,T)$ Models
• The two-component jet of GRB 080413B
• The mass of the dark matter particle from theory and observations
• Large Non-Gaussianity Implication for Curvaton Scenario
• Constraining cosmic curvature by using age of galaxies and gravitational lenses
• Cosmological Evolution in f(R,T) theory with Collisional Matter
• Clarifying the effects of interacting dark energy on linear and nonlinear structure formation processes
• An Empirical Model for the Star Formation History in Dark Matter Halos
• A parton picture of de Sitter space during slow-roll inflation
• Sub-mm Emission Line Deep Fields: CO and [CII] Luminosity Functions out to z = 6
• Is a step in the primordial spectral index favored by CMB data ?
• Bayesian inference of galaxy formation from the K-band luminosity function of galaxies: tensions between theory and observation
• Improved Constraints on the Gravitational Lens Q0957+561. II. Strong Lensing
• Gravitational lenses as cosmic rulers: density of dark matter and dark energy from time delays and velocity dispersions
• New approach for precise computation of Lyman-alpha forest power spectrum with hydrodynamical simulations
• Light sterile neutrino production in the early universe with dynamical neutrino asymmetries
• Extracting Angular Diameter Distance and Expansion Rate of the Universe from Two-dimensional Galaxy Power Spectrum at High Redshifts: Baryon Acoustic Oscillation Fitting versus Full Modeling
• Dark matter and a suppression mechanism for neutrino masses in the Higgs triplet model
• First results from SMAUG: Uncovering the Origin of the Multiphase Circumgalactic Medium with a Comparative Analysis of Idealized and Cosmological Simulations
• Consistency of the growth rate in different environments with the 6dF Galaxy Survey: measurement of the void-galaxy and galaxy-galaxy correlation functions
• Estimating the impact of recombination uncertainties on the cosmological parameter constraints from cosmic microwave background experiments
• Jet collimation in NGC 315 and other nearby AGN
• Revisiting mGMSB in light of a 125 GeV Higgs
• Running vacuum in the Universe: phenomenological status in light of the latest observations, and its impact on the ${\sigma }_8$ and $H_0$ tensions
• CMB Polarization Systematics, Cosmological Birefringence and the Gravitational Waves Background
• Halo model and halo properties in Galileon gravity cosmologies
• Natural Warm Inflation
• Comparison of an X-ray selected sample of massive lensing clusters with the MareNostrum Universe LCDM simulation
• The influence of structure formation on the cosmic expansion
• Primordial black hole constraints for curvaton models with predicted large non-Gaussianity
• Simple Types of Anisotropic Inflation
• Dark Matter and Electroweak Symmetry Breaking in Models with Warped Extra Dimensions
• Cosmic Ray Positron and Electron Excess from Hidden-Fermion Dark Matter Decays
• Non-Universal Gaugino Masses and Natural Supersymmetry
• Constraining a spatially dependent rotation of the Cosmic Microwave Background Polarization
• The Peaks Formalism and the Formation of Cold Dark Matter Haloes
• Resonant Leptogenesis in the Minimal B-L Extended Standard Model at TeV
• Precious Metals in SDSS Quasar Spectra I: Tracking the Evolution of Strong, 1.5 < z < 4.5 CIV Absorbers with Thousands of Systems
• Are gamma-ray bursts the sources of ultra-high energy cosmic rays?
• Interstellar Scintillation and the Radio Counterpart of the Fast Radio Burst FRB150418
• Thermodynamical, geometrical and Poincaré methods for charged black holes in presence of quintessence
• The CMB bispectrum in the squeezed limit
• WIMP Dark Matter and Baryogenesis
• The nature of dark matter from the global high redshift HI 21 cm signal
• A General Analysis of Non-Gaussianity from Isocurvature Perturbations
• Generating Primordial Black Holes Via Hilltop-Type Inflation Models
• Heal the world: Avoiding the cosmic doomsday in the holographic dark energy model
• Influence of nuclear physics inputs and astrophysical conditions on Th/U chronometer
• Simulating the assembly of galaxies at redshifts z = 6 - 12
• On the generalization of McVittie's model for an inhomogeneity in a cosmological spacetime
• The Cosmic Microwave Background in an Inhomogeneous Universe - why void models of dark energy are only weakly constrained by the CMB
• HerMES: Halo Occupation Number and Bias Properties of Dusty Galaxies from Angular Clustering Measurements
• Majorana Phases and Leptogenesis in See-Saw Models with A_4 Symmetry
• Genetic Algorithms and Supernovae Type Ia Analysis
• Pangenesis in a Baryon-Symmetric Universe: Dark and Visible Matter via the Affleck-Dine Mechanism
• Constraints on non-flat cosmologies with massive neutrinos after Planck 2015
• Lyman Alpha Emitter Evolution in the Reionization Epoch
• A Multi-wavelength Study of the Sunyaev-Zel'dovich Effect in the Triple-Merger Cluster MACS J0717.5+3745 with MUSTANG and Bolocam
• Yukawa Unification and Neutralino Dark Matter in SU(4)_c \times SU(2)_L \times SU(2)_R
• On the Populations of Radio Galaxies with Extended Morphology at z<0.3
• Precision modeling of redshift-space distortions from multi-point propagator expansion
• A 2% Distance to z = 0.35 by Reconstructing Baryon Acoustic Oscillations - III : Cosmological Measurements and Interpretation
• Lyman Alpha Emitters and Lyman Break Galaxies: dichotomous twins?
• ART^2 : Coupling Lyman-alpha Line and Multi-wavelength Continuum Radiative Transfer
• Results from the Wilkinson Microwave Anisotropy Probe
• Improved limits on short-wavelength gravitational waves from the cosmic microwave background
• Successful type I Leptogenesis with SO(10)-inspired mass relations
• Fingerprints of Primordial Universe Paradigms as Features in Density Perturbations
• Chemical Evolution on the Scale of Clusters of Galaxies: A Conundrum?
• Suppression of HD-cooling in protogalactic gas clouds by Lyman-Werner radiation
• Primordial Non-Gaussianity and the NRAO VLA Sky Survey
• Consistently violating the non-Gaussian consistency relation
• Cosmology with the Large Synoptic Survey Telescope: an Overview
• Can dark energy be expressed as a power series of the Hubble parameter?
• Where are the Luminous Red Galaxies (LRGs)? Using correlation measurements and lensing to relate LRGs to dark matter halos
• Cosmic strings and their induced non-Gaussianities in the cosmic microwave background
• How the Scalar Field of Unified Dark Matter Models Can Cluster
• Dark Energy in Practice
• Minimal Inflation
• The Observed Growth of Massive Galaxy Clusters III: Testing General Relativity on Cosmological Scales
• Evolution of Galaxy Shapes from Prolate to Oblate through Compaction Events
• Dark radiation from particle decay: cosmological constraints and opportunities
• The scalar bi-spectrum in the Starobinsky model: The equilateral case
• Observational Evidence for Cosmological-Scale Extra Dimensions
• Do WMAP data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
• Visible and dark matter from a first-order phase transition in a baryon-symmetric universe
• The impact of feedback on the low redshift Intergalactic Medium
• Oscillations in the inflaton potential: Complete numerical treatment and comparison with the recent and forthcoming CMB datasets
• Multifield Cosmological Perturbations at Third Order and the Ekpyrotic Trispectrum
• CMB Lensing Constraints on Neutrinos and Dark Energy
• Distribution function approach to redshift space distortions. Part II: N-body simulations
• Dark Energy Model in Anisotropic Bianchi Type-III Space-Time with Variable EoS Parameter
• Thermal Relics in Modified Cosmologies: Bounds on Evolution Histories of the Early Universe and Cosmological Boosts for PAMELA
• A Constraint on Planck-scale Modifications to Electrodynamics with CMB polarization data
• What can the observation of nonzero curvature tell us?
• The origin of pseudobulges in cosmological simulations of galaxy formation
• Sachs-Wolfe at second order: the CMB bispectrum on large angular scales
• Quasars as standard candles II: The non linear relation between UV and X-ray emission at high redshifts
• Confronting Dark Energy Models using Galaxy Cluster Number Counts
• Non-Gaussianity from violation of slow-roll in multiple inflation
• 21cm-line bispectrum as method to probe Cosmic Dawn and Epoch of Reionization
• Do Bars Trigger Activity in Galactic Nuclei?
• A status report on the observability of cosmic bubble collisions
• Effective relational dynamics of a nonintegrable cosmological model
• The Swift/BAT AGN Spectroscopic Survey -- IX. The Clustering Environments of an Unbiased Sample of Local AGN
• Three-Point Correlation Functions of SDSS Galaxies: Constraining Galaxy-Mass Bias
• Low-Energy Effective Field Theory for Chromo-Natural Inflation
• The core shift effect in the blazar 3C 454.3
• Reconstruction of the primordial power spectrum of curvature perturbations using multiple data sets
• Kinetic k-essence ghost dark energy model
• Baryon Acoustic Oscillations in 2D II: Redshift-space halo clustering in N-body simulations
• Consistency condition for inflation from (broken) conformal symmetry
• Fermionic Dark Matter in Radiative Inverse Seesaw Model with U(1)_{B-L}
• A critical analysis of the UV Luminosity Function at redshift~7 from deep WFC3 data
• Stable Higgs Bosons as Cold Dark Matter
• Non-minimally coupled vector curvaton
• The first Fermi multifrequency campaign on BL Lacertae: characterizing the low-activity state of the eponymous blazar
• The bolometric output and host-galaxy properties of obscured AGN in the XMM-COSMOS survey
• Cosmography beyond standard candles and rulers
• Constraining neutrino mass with weak lensing Minkowski Functionals
• Connecting Reionization to the Local Universe
• A measurement of the secondary-CMB and millimeter-wave-foreground bispectrum using 800 square degrees of South Pole Telescope data
• Cosmological Perturbations at Second Order and Recombination Perturbed
• Testing the phenomenological interacting dark energy with observational $H(z)$ data
• Adiabatic Ekpyrosis: Scale-Invariant Curvature Perturbations from a Single Scalar Field in a Contracting Universe
• Very Long Baseline Array Imaging of Parsec-scale Radio Emissions in Nearby Radio-quiet Narrow-line Seyfert 1 Galaxies
• Degree-Scale CMB Polarization Measurements from Three Years of BICEP1 Data
• Dark Matter signals from Draco and Willman 1: Prospects for MAGIC II and CTA
• Nonlinear Electromagnetic Fields As a Source of Universe Acceleration
• Detecting sterile neutrinos with KATRIN like experiments
• An estimate of the local ISW signal, and its impact on CMB anomalies
• Bispectrum signatures of a modified vacuum in single field inflation with a small speed of sound
• Testing the predictions of the cold dark matter model for the sizes, colours, morphologies and luminosities of galaxies with the SDSS
• Higgs Boson Mass from t-b-tau Yukawa Unification
• Faraday rotation, stochastic magnetic fields and CMB maps
• TeV Scale Singlet Dark Matter
• The Curvature Perturbation in the Axion-type Curvaton Model
• On the full quantum trispectrum in multi-field DBI inflation
• Stochastic backgrounds of relic gravitons: a theoretical appraisal
• Direct Numerical Simulation of Reionization II: Recombinations, Clumping Factors, and the Photon Budget for Reionization
• The Effect of Galactic Properties on the Escape Fraction of Ionizing Photons
• Resonant leptogenesis and tribimaximal leptonic mixing with A4 symmetry
• Full-sky lensing reconstruction of gradient and curl modes from CMB maps
• Prompt emission polarimetry of Gamma Ray Bursts with ASTROSAT CZT-Imager
• Baryon Budget of the Hot Circumgalactic Medium of Massive Spiral Galaxies
• Identification of Dark Matter particles with LHC and direct detection data
• Reconciling leptogenesis with observable mu --> e gamma rates
• Constraints on the shapes of galaxy dark matter haloes from weak gravitational lensing
• First Cosmological Constraints on Dark Energy from the Radial Baryon Acoustic Scale
• A sub-horizon framework for probing the relationship between the cosmological matter distribution and metric perturbations
• Anisotropic dark energy model with a hybrid scale factor
• Primordial non-Gaussianity from the covariance of galaxy cluster counts
• Neutrino masses and beyond-$\Lambda$CDM cosmology with LSST and future CMB experiments
• ALMA HCN and HCO+ J=3-2 observations of optical Seyfert and luminous infrared galaxies -- Confirmation of elevated HCN-to-HCO+ flux ratios in AGNs --
• A connection between $\gamma$-ray and parsec-scale radio flares in the blazar 3C 273
• Probing the Epoch of Reionization with Milky Way Satellites
• Multi-field DBI inflation: introducing bulk forms and revisiting the gravitational wave constraints
• Measuring the Integrated Sachs-Wolfe Effect
• Dark halo response and the stellar initial mass function in early-type and late-type galaxies
• Hubble parameter data constraints on dark energy
• Gravitational waves: Classification, Methods of detection, Sensitivities, and Sources
• Elliptical Galaxies and Bulges of Disk Galaxies: Summary of Progress and Outstanding Issues
• Preheating and the non-gaussianity of the curvature perturbation
• The Large-Scale 3-point correlation function of SDSS Luminous Red Galaxies
• Non-unitary Leptonic Mixing and Leptogenesis
• Phenomenological investigation of a quantum gravity extension of inflation with the Starobinsky potential
• Dynamical compactification from de Sitter space
• The 21cm Power Spectrum After Reionization
• The cosmological background of vector modes
• Primordial backgrounds of relic gravitons
• Constraints on amplitudes of curvature perturbations from primordial black holes
• Primordial non-Gaussianity in the large scale structure of the Universe
• The Sommerfeld enhancement for scalar particles and application to sfermion co-annihilation regions
• The UV, Lyman-alpha, and dark matter halo properties of high redshift galaxies
• Statistics of extreme objects in the Juropa Hubble Volume simulation
• Late and early time phenomenology of Higgs-dependent cutoff
• The impact of baryons on the direct detection of dark matter
• An Empirical Study of the Relationship between Lyα and UV selected Galaxies: Do Theorists and Observers `Select' the Same Objects?
• Flavor symmetries, leptogenesis and the absolute neutrino mass scale
• Non-gaussianity from the trispectrum and vector field perturbations
• Baryon and Dark Matter Genesis from Strongly Coupled Strings
• Determining the Neutrino Mass Hierarchy with Cosmology
• Reconstructing Quintom from Ricci Dark Energy
• Probing Resonant Leptogenesis at the LHC
• Distribution function approach to redshift space distortions, Part III: halos and galaxies
• Constraining dark energy with gamma-ray bursts
• Isocurvature forecast in the anthropic axion window
• Unanswered Questions in the Electroweak Theory
• Boosting the annihilation boost: Tidal effects on dark matter subhalos and consistent luminosity modeling
• Modified Gravity Explains Dark Matter?
• Difficulties Distinguishing Dark Energy from Modified Gravity via Redshift Distortions
• The observational signature of the first H II regions
• Resurrecting No-Scale Supergravity Phenomenology
• Testing Yukawa-like potentials from f(R)-gravity in elliptical galaxies
• Matter Non-conservation in the Universe and Dynamical Dark Energy
• A model of interacting holographic dark energy at the Ricci's scale
• Finding all flux vacua in an explicit example
• Forecasting the Cosmological Constraints with Anisotropic Baryon Acoustic Oscillations from Multipole Expansion
• High-z massive clusters as a test for dynamical coupled dark energy
• Pseudo-Dirac Dark Matter Leaves a Trace
• Isotropic cosmic birefringence from early dark energy
• Constraints on Cold Dark Matter Accelerating Cosmologies and Cluster Formation
• A Ly-alpha Emitter with an Extremely Large Rest-frame Equivalent Width of ~900A at z=6.5: A Candidate of Population III-dominated Galaxy?
• A Map of the Integrated Sachs-Wolfe Signal from Luminous Red Galaxies
• Puffing up early-type galaxies by baryonic mass loss: numerical experiments
• Co-genesis of Matter and Dark Matter with Vector-like Fourth Generation Leptons
• A theory of extra radiation in the Universe
• Theoretical and observational constraints on the HI intensity power spectrum
• Photo-heating and supernova feedback amplify each other's effect on the cosmic star formation rate
• Primordial non-Gaussianity without tails -- how to measure fNL with the bulk of the density PDF
• Accelerating dark energy models in bianchi Type-V space-time
• Turbulent Amplification and Structure of the Intracluster Magnetic Field
• Lorentz boost and non-Gaussianity in multi-field DBI-inflation
• Cosmological simulations of galaxy formation with cosmic rays
• The impact of baryonic physics on the shape and radial alignment of substructures in cosmological dark matter haloes
• Triviality and vacuum stability bounds in the three-loop neutrino mass model
• Leptogenesis in the Exceptional Supersymmetric Standard Model: flavour dependent lepton asymmetries
• Is backreaction really small within concordance cosmology?
• Upper Limits on the VHE gamma-ray Emission from the Willman 1 Satellite Galaxy with the MAGIC telescope
• Tidal disruption rate of stars by supermassive black holes obtained by direct N-body simulations
• Holographic dark energy in a universe with spatial curvature and massive neutrinos: a full Markov Chain Monte Carlo exploration
• The latitude dependence of the rotation measures of NVSS sources
• Frequentist Analysis of the Parameter Space of Minimal Supergravity
• Gravitational Lensing Simulations I : Covariance Matrices and Halo Catalogues
• Dark Matter Disc Enhanced Neutrino Fluxes from the Sun and Earth
• Cosmology of the selfaccelerating third order Galileon
• CMB anisotropies at second order III: bispectrum from products of the first-order perturbations
• The Core-Cusp Problem in Cold Dark Matter Halos and Supernova Feedback: Effects of Oscillation
• Kadanoff-Baym Equations with Non-Gaussian Initial Conditions: The Equilibrium Limit
• A Quintom scenario with mixed kinetic terms
• Non-Gaussian Error Contribution to Likelihood Analysis of the Matter Power Spectrum
• Observational constraints on the interacting Ricci dark energy model
• Alleviation of Cosmic Age Problem In Interacting Dark Energy Model
• LCDM Model in f(T) Gravity: Reconstruction, Thermodynamics and Stability
• Bounce solutions in viscous fluid cosmology
• Natural Multi-Higgs Model with Dark Matter and CP Violation
• Cosmological consequences of a possible $\Lambda$-dark matter interaction
• iPTF15dtg: a double-peaked Type Ic Supernova from a massive progenitor
• The CMB temperature bispectrum induced by cosmic strings
• Non-Gaussianity from massless preheating
• Detecting Bispectral Acoustic Oscillations from Inflation Using a New Flexible Estimator
• The Atacama Cosmology Telescope: Detection of Sunyaev-Zel'dovich Decrement in Groups and Clusters Associated with Luminous Red Galaxies
• Clustering properties of galaxies selected in stellar mass: Breaking down the link between luminous and dark matter in massive galaxies from z=0 to z=2
• Neutrino mass constraint with the Sloan Digital Sky Survey power spectrum of luminous red galaxies and perturbation theory
• Conformally related metrics and Lagrangians and their physical interpretation in cosmology
• Constraints from muon g-2 and LFV processes in the Higgs Triplet Model
• Constraining galaxy cluster temperatures and redshifts with eROSITA survey data
• Chaotic Inflation in Supergravity with Heisenberg Symmetry
• Toward an accurate mass function for precision cosmology
• Non-adiabatic-like accelerated expansion of the late universe in entropic cosmology
• Forecasted 21 cm constraints on compensated isocurvature perturbations
• Searching for Dark Matter with X-ray Observations of Local Dwarf Galaxies
• The spherical collapse model and cluster formation beyond the $\Lambda$ cosmology: Indications for a clustered dark energy?
• A clear Dark Matter gamma ray line generated by the Green-Schwarz mechanism
• Neutrinos in the holographic dark energy model: constraints from latest measurements of expansion history and growth of structure
• Exact dark energy star solutions
• The problem of the initial conditions in flavoured leptogenesis and the tauon N_2-dominated scenario
• Constraining the EoR model parameters with the 21cm bispectrum
• Non-standard primordial fluctuations and nongaussianity in string inflation
• The Spectral Energy Distribution of Powerful Starburst Galaxies I: Modelling the Radio Continuum
• $f(R)$-gravity from Killing Tensors
• Cosmological Zoom Simulations of z = 2 Galaxies: The Impact of Galactic Outflows
• Minimal Supersymmetric Inverse Seesaw: Neutrino masses, lepton flavour violation and LHC phenomenology
• Reconstruction of the Scalar Field Potential in Inflationary Models with a Gauss-Bonnet term
• Stochastic backgrounds of relic gravitons, T$\Lambda$CDM paradigm and the stiff ages
• Primordial Magnetic Field Limits from CMB Trispectrum - Scalar Modes and Planck Constraints
• Large-Angle Correlations in the Cosmic Microwave Background
• Calibrating Galaxy Redshifts Using Absorption by the Surrounding Intergalactic Medium
• What Sets the Sizes of the Faintest Galaxies?
• Comments on scalar-tensor representation of nonlocally corrected gravity
• The High Redshift Integrated Sachs-Wolfe Effect
• Tunneling cosmological state revisited: Origin of inflation with a non-minimally coupled Standard Model Higgs inflaton
• Cosmological Parameters Degeneracies and Non-Gaussian Halo Bias
• Linear response to long wavelength fluctuations using curvature simulations
• Formation of Warped Disks by Galactic Fly-by Encounters. I. Stellar Disks
• Generalized Holographic and Ricci Dark Energy Models
• Non-Gaussianity and the CMB Bispectrum: confusion between Primordial and Lensing-Rees Sciama contribution?
• Constraints on Cosmological Models and Reconstructing the Acceleration History of the Universe with Gamma-Ray Burst Distance Indicators
• A First Look at Galaxy Flyby Interactions: I. Characterizing the Frequency of Flybys in a Cosmological Context
• Future CMB constraints on cosmic birefringence and implications for fundamental physics
• Cosmological tachyon condensation
• Dirac Neutrinos with $S_4$ Flavor Symmetry in Warped Extra Dimensions
• Signatures of a Graviton Mass in the Cosmic Microwave Background
• The cosmology of an holographic induced gravity model with curvature effects
• Neutrino-Flavoured Sneutrino Dark Matter
• B-mode CMB Polarization from Patchy Screening during Reionization
• Extragalactic gamma-ray background radiation from dark matter annihilation
• Phenomenology of WIMPy baryogenesis models
• Constraints from CMB on Spacetime Noncommutativity and Causality Violation
• Analytic solution for matter density perturbations in a class of viable cosmological f(R) models
• Early-type galaxies in the PEARS survey: Probing the stellar populations at moderate redshift
• Generalized Noether symmetry in f(T) gravity
• Holographic Dark Energy Model with Hubble Horizon as an IR Cut-off
• Revising the predictions of inflation for the cosmic microwave background anisotropies
• High-redshift star formation rate up to z~8.3 derived from gamma-ray bursts and influence of background cosmology
• Structure formation with scalar field dark matter: the field approach
• A Strategy to Measure the Dark Energy Equation of State using the HII galaxy Hubble Relation & X-ray AGN Clustering: Preliminary Results
• Subaru weak-lensing study of A2163: bimodal mass structure
• Reconstructing the Cosmic Expansion History up to Redshift z=6.29 with the Calibrated Gamma-Ray Bursts
• From Cavendish to PLANCK: Constraining Newton's Gravitational Constant with CMB Temperature and Polarization Anisotropy
• The Cosmic Near Infrared Background II: Fluctuations
• Non-gaussianity at tree and one-loop levels from vector field perturbations
• Unified dark energy and dark matter from a scalar field different from quintessence
• Higgs-Dilaton cosmology: Are there extra relativistic species?
• The Hubble constant inferred from 18 time-delay lenses
• Cosmic bulk flows on 50 {h}^{-1}Mpc scales: A Bayesian hyper-parameter method and multishells likelihood analysis
• Improving constraints on the growth rate of structure by modelling the density-velocity cross-correlation in the 6dF Galaxy Survey
• Lyman Alpha Driven Outflows Around Star Forming Galaxies
• Central mass and luminosity of Milky Way satellites in the LCDM model
• Exploring the magnetized cosmic web through low frequency radio emission
• The foreground wedge and 21 cm BAO surveys
• The non-Gaussianity of the cosmic shear likelihood - or: How odd is the Chandra Deep Field South?
• Multi-frequency imaging of the galaxy cluster Abell 2163 using the Sunyaev-Zel'dovich Effect
• Galaxy-CMB and galaxy-galaxy lensing on large scales: sensitivity to primordial non-Gaussianity
• Dark Matter Through the Neutrino Portal
• Combined local and equilateral non-Gaussianities from multifield DBI inflation
• The Subdominant Curvaton
• An effective field theory for non-relativistic Majorana neutrinos
• Primordial Trispectrum from Entropy Perturbations in Multifield DBI Model
• Generalised DBI-Quintessence
• Long-rising Type II supernovae from PTF and CCCP
• Ion chemistry in the early universe: revisiting the role of HeH+ with new quantum calculations
• A new method for calculating the primordial bispectrum in the squeezed limit
• Enhancement of the annihilation of dark matter in a radiative seesaw model
• SN2013fs and SN2013fr: Exploring the circumstellar-material diversity in Type II supernovae
• Dynamical Analysis of an Integrable Cubic Galileon Cosmological Model
• Cosmological perturbation theory for baryons and dark matter I: one-loop corrections in the RPT framework
• Minimal Supersymmetric Hybrid Inflation, Flipped SU(5) and Proton Decay
• Systematic biases on galaxy haloes parameters from Yukawa-like gravitational potentials
• High redshift cosmography: new results and implication for dark energy
• Dark Energy and Neutrino Masses from Future Measurements of the Expansion History and Growth of Structure
• The Halo Bispectrum in N-body Simulations with non-Gaussian Initial Conditions
• Evading Weinberg's no-go theorem to construct mass dimension one fermions: Constructing darkness
• Spatial curvature and cosmological tests of general relativity
• Forecasts on dark energy from the X-ray cluster survey with eROSITA: constraints from counts and clustering
• Constraints on early dark energy from CMB lensing and weak lensing tomography
• Do the cosmological observational data prefer phantom dark energy?
• The IR stability of de Sitter QFT: Physical initial conditions
• Impact of Scale Dependent Bias and Nonlinear Structure Growth on the ISW Effect: Angular Power Spectra
• Dark matter in the solar system III: The distribution function of WIMPs at the Earth from gravitational capture
• The formation and evolution of young low-mass stars within halos with high concentration of dark matter particles
• Higgs and Sparticle Spectroscopy with Gauge-Yukawa Unification
• The pre-inflationary and inflationary fast-roll eras and their signatures in the low CMB multipoles
• The New Model of Chemical Evolution of r-process Elements Based on The Hierarchical Galaxy Formation I: Ba and Eu
• Reconstruction of scalar field theories realizing inflation consistent with the Planck and BICEP2 results
• Modeling The Star Forming Universe at z=2: Impact of Cold Accretion Flows
• N-flation from multiple DBI type actions
• Inferring the Redshift Distribution of the Cosmic Infrared Background
• Dynamical system analysis for nonminimal torsion-matter coupled gravity
• Scale Dependence of Halo Bispectrum from Non-Gaussian Initial Conditions in Cosmological N-body Simulations
• Bayesian Analysis and Constraints on Kinematic Models from Union SNIa
• Detectability of cold streams into high-redshift galaxies by absorption lines
• Simulations of Wide-Field Weak Lensing Surveys II: Covariance Matrix of Real Space Correlation Functions
• Vorticity of IGM Velocity Field on Large Scales
• Bayesian optimal reconstruction of the primordial power spectrum
• The Observed Growth of Massive Galaxy Clusters IV: Robust Constraints on Neutrino Properties
• The cosmological information of shear peaks: beyond the abundance
• Tachyonic Teleparallel Dark Energy
• Cosmographic parameters in model-independent approaches
• $w$-cosmological singularities
• Fitting the Constitution SNIa Data with Redshift Binned Parameterization Method
• The Big Bounce in Rainbow Universe
• Two dark matter components in N_{DM}MSSM and dark matter extension of the minimal supersymmetric standard model and the high energy positron spectrum in PAMELA/HEAT data
• How well do cosmological simulations reproduce individual-halo properties?
• Revisit of cosmic age problem
• Gauss-Bonnet dark energy by Lagrange multipliers
• The Spectrum of the Axion Dark Sector
• Pairwise Velocities of Dark Matter Halos: a Test for the Lambda Cold Dark Matter Model using the Bullet Cluster
• The Presence of Weak Active Galactic Nuclei in High Redshift Star Forming Galaxies
• One-loop graviton corrections to the curvature perturbation from inflation
• Accurate Modeling of Weak Lensing with the sGL Method
• Constraints on cosmological models from lens redshift data
• Scalar-Tensor Gravity Cosmology: Noether symmetries and analytical solutions
• A Unified Approach to Variational Derivatives of Modified Gravitational Actions
• A unified solution to the small scale problems of the $\Lambda$CDM model
• The cool side of Lyman Alpha Emitters
• A Minimal Inflation Scenario
• Cosmological evolution and statefinder diagnostic for new holographic dark energy model in non flat universe
• The spatial and velocity bias of linear density peaks and proto-haloes in the Lambda cold dark matter cosmology
• On Adiabatic Renormalization of Inflationary Perturbations
• Dynamics of a scalar field in Robertson-Walker spacetimes
• Universal properties of Dark Matter halos
• Attractive Lagrangians for Noncanonical Inflation
• The Clustering of Galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Measuring H(z) and D_A(z) at z = 0.57 with Clustering Wedges
• Substructure Boosts to Dark Matter Annihilation from Sommerfeld Enhancement
• Growth factor parametrization in curved space
• Future CMB cosmological constraints in a dark coupled universe
• Self-similarity and universality of void density profiles in simulation and SDSS data
• Cluster strong lensing in the Millennium Simulation: The effect of galaxies and structures along the line-of-sight
• On the Possibility of Anisotropic Curvature in Cosmology
• GridSPT: Grid-based calculation for perturbation theory of large-scale structure
• Implications for Primordial Non-Gaussianity (f_NL) from weak lensing masses of high-z galaxy clusters
• Critical Formation of Trapped Surfaces in the Collision of Non-expanding Gravitational Shock Waves in de Sitter Space-Time
• Generating Scale-Invariant Perturbations from Rapidly-Evolving Equation of State
• Swiss Cheese and a Cheesy CMB
• t-b-tau Yukawa unification for mu < 0 with a sub-TeV sparticle spectrum
• Probing the scale dependence of non-Gaussianity with spectral distortions of the cosmic microwave background
• Optimized detection of shear peaks in weak lensing maps
• Mapping systematic errors in helium abundance determinations using Markov Chain Monte Carlo
• Full-sky maps for gravitational lensing of the CMB
• Mapping stellar content to dark matter halos - III.Environmental dependence and conformity of galaxy colours
• Reconciling the Muon g-2 and Dark Matter Relic Density with the LHC Results in Nonuniversal Gaugino Mass Models
• Constraints on the generalized Chaplygin gas model including gamma-ray bursts via a Markov Chain Monte Carlo approach
• Evidence for extra radiation? Profile likelihood versus Bayesian posterior
• Transient cosmic acceleration from interacting fluids
• Unveiling the Dynamics of the Universe
• Caught in the cosmic web: Environmental effect on halo concentrations, shape, and spin
• Observational constraints on thawing quintessence models
• Ruling out the Modified Chaplygin Gas Cosmologies
• Cosmic vector for dark energy: constraints from SN, CMB and BAO
• Response function of the large-scale structure of the universe to the small scale inhomogeneities
• Detection of 21-cm, H2 and Deuterium absorption at z>3 along the line-of-sight to J1337+3152
• The inferred evolution of the cold gas properties of CANDELS galaxies at 0.5 < z < 3.0
• A combined radio and GeV gamma-ray view of the 2012 and 2013 flares of Mrk 421
• Cosmological constraints on a light non-thermal sterile neutrino
• Warm natural inflation
• Kinematic constraints on the stellar and dark matter content of spiral and S0 galaxies
• Low Mass Gluino within the Sparticle Landscape, Implications for Dark Matter, and Early Discovery Prospects at LHC-7
• Primordial Magnetism in the CMB: Exact Treatment of Faraday Rotation and WMAP7 Bounds
• Explaining PAMELA and WMAP data through Coannihilations in Extended SUGRA with Collider Implications
• TASI 2008 Lectures on Dark Matter
• Limits on Isocurvature Perturbations from Non-Gaussianity in WMAP Temperature Anisotropies
• Features in the primordial power spectrum? A frequentist analysis
• Noether symmetries and stability of ideal gas solution in Galileon Cosmology
• Fragmentation in the First Galaxies
• Joint 3D modelling of the polarized Galactic synchrotron and thermal dust foreground diffuse emission
• Perturbation of the metric around a spherical body from a nonminimal coupling between matter and curvature
• The discreet charm of higgsino dark matter - a pocket review
• Position-dependent power spectra of the 21-cm signal from the epoch of reionization
• Multifield consequences for D-brane inflation
• Dark-ages Reionization & Galaxy Formation Simulation I: The dynamical lives of high redshift galaxies
• Dynamical Dark Energy simulations: high accuracy Power Spectra at high redshift
• Clustering and redshift-space distortions in interacting dark energy cosmologies
• Probing CPT Violation with CMB Polarization Measurements
• A fuller flavour treatment of N_2-dominated leptogenesis
• Cosmological constraints of phantom dark energy models
• Duty Cycle and the Increasing Star Formation History of z>=6 Galaxies
• The Lyman alpha forest flux probability distribution at z>3
• Vorticity generation at second order in cosmological perturbation theory
• Dark matter and collider phenomenology of split-UED
• Estimation of Cosmological Parameters from HI Observations of Post-reionization Epoch
• A Consistent Test of the Distance-Duality Relation with Galaxy Clusters and Type Ia Supernave
• The Cusp/Core problem: supernovae feedback versus the baryonic clumps and dynamical friction model
• Constraining Fundamental Physics with Future CMB Experiments
• AMEND: A Model Explaining Neutrino masses and Dark matter testable at the LHC and MEG
• GUT Inflation and Proton Decay after WMAP5
• First measurement of the bulk flow of nearby galaxies using the cosmic microwave background
• Introduction to dark matter experiments
• Non-minimally coupled scalar field cosmology on the phase plane
• Constraints on dark energy from H II starburst galaxy apparent magnitude versus redshift data
• Inflationary trispectrum from graviton exchange
• From Big to Little Rip in modified F(R,G) gravity
• Phantom cosmological model with observational constraints in $f(Q)$ gravity
• Unified Model of k-Inflation, Dark Matter & Dark Energy
• Stagflation -- Bose-Einstein condensation in the early universe
• Second-order matter perturbations in a LambdaCDM cosmology and non-Gaussianity
• Recovering the HII region size statistics from 21-cm tomography
• An X-ray and Multiwavelength Survey of Highly Radio-Loud Quasars at z > 4: Jet-Linked Emission in the Brightest Radio Beacons of the Early Universe
• Dynamical Dark Matter and the Positron Excess in Light of AMS
• Tachyacoustic Cosmology: An Alternative to Inflation
• Observational Constraints on Exponential Gravity
• Observational Constraints to Ricci Dark Energy Model by Using: SN, BAO, OHD, fgas Data Sets
• The impact of stellar and AGN feedback on halo-scale baryonic and dark matter accretion in the EAGLE simulations
• Synoptic Sky Surveys and the Diffuse Supernova Neutrino Background: Removing Astrophysical Uncertainties and Revealing Invisible Supernovae
• Modulated Reheating and Large Non-Gaussianity in String Cosmology
• Dirac Neutralinos and Electroweak Scalar Bosons of N=1/N=2 Hybrid Supersymmetry at Colliders
• CFHTLS weak-lensing constraints on the neutrino masses
• Is cosmic birefringence due to dark energy or dark matter? A tomographic approach
• Cosmic evolution of the CIV in high-resolution hydrodynamic simulations
• Quantified naturalness from Bayesian statistics
• Testing for X-ray-SZ Differences and Redshift Evolution in the X-ray Morphology of Galaxy Clusters
• The WIRCAM Deep Infrared Cluster Survey I: Groups and Clusters at z > 1.1
• How well do we know the Halo Mass Function?
• The Premature Formation of High Redshift Galaxies
• T(13) Flavor Symmetry and Decaying Dark Matter
• CoGeNT, DAMA, and Light Neutralino Dark Matter
• Experimental constraints on the uncoupled Galileon model from SNLS3 data and other cosmological probes
• Observed parity-odd CMB temperature bispectrum
• Exact solutions and spacetime singularities in nonlocal gravity
• Global fits of the Non-Universal Higgs Model
• Contiguous redshift parameterizations of the growth index
• The Origin and Distribution of Cold Gas in the Halo of a Milky Way-Mass Galaxy
• Bayesian Implications of Current LHC Supersymmetry and Dark Matter Detection Searches for the Constrained MSSM
• Forecast constraints on cosmic strings from future CMB, pulsar timing and gravitational wave direct detection experiments
• Number Counts and Non-Gaussianity
• Multi-messenger Detection Rates and distributions of Binary Neutron Star Mergers and Their Cosmological Implications
• On the signature of $z\sim 0.6$ superclusters and voids in the Integrated Sachs-Wolfe effect
• Cosmological bouncing scenarios in symmetric teleparallel gravity
• Relic Gravitational Waves with A Running Spectral Index and Its Constraints at High Frequencies
• Testing Lorentz Invariance with Ultra High Energy Cosmic Ray Spectrum
• Constraints on Primordial Non-Gaussianity from a Needlet Analysis of the WMAP-5 Data
• Observing the Big Bounce with Tensor Modes in the Cosmic Microwave Background: Phenomenology and Fundamental LQC Parameters
• Non-Gaussianity and large-scale structure in a two-field inflationary model
• Non-Gaussianity Consistency Relation for Multi-field Inflation
• Investigating Emission Line Galaxy Surveys with the Sloan Digital Sky Survey Telescope
• Scale-dependent halo bias from scale-dependent growth
• Next-to-leading resummation of cosmological perturbations via the Lagrangian picture: 2-loop correction in real and redshift spaces
• Interaction between dark energy and dark matter: observational constraints from OHD, BAO, CMB and SNe Ia
• Testing the Running of non-Gaussianity through the CMB mu-distortion and the Halo Bias
• Cosmological models with Lagrange Multiplier Field
• Applications of Bayesian model averaging to the curvature and size of the Universe
• Testing general relativity with the multipole spectra of the SDSS luminous red galaxies
• Cosmological reconstruction of $f(T,\mathcal{T})$ Gravity
• The Sloan Digital Sky Survey Quasar Lens Search. IV. Statistical Lens Sample from the Fifth Data Release
• Mixed Neutralino Dark Matter in Nonuniversal Gaugino Mass Models
• Looking Beyond Lambda with the Union Supernova Compilation
• Update of D3/D7-Brane Inflation on K3 x T^2/Z_2
• Hubble parameter reconstruction from a principal component analysis: minimizing the bias
• Neutrinos and dark energy after Planck and BICEP2: data consistency tests and cosmological parameter constraints
• Chasing the non-linear evolution of matter power spectrum with numerical resummation method: solution of closure equations
• Current Constraints on Anisotropic and Isotropic Dark Energy Models
• The earliest stars and their relics in the Milky Way
• Dark energy: investigation and modeling
• Can multistate dark matter annihilation explain the high-energy cosmic ray lepton anomalies?
• The Late Reionization of Filaments
• Broken S3 Symmetry in the Neutrino Mass Matrix and Non-Zero theta_{13}
• Probing the stellar initial mass function with high-$z$ supernovae
• Reheating in Models with Non-minimal Coupling in metric and Palatini formalisms
• Accurate weak lensing of standard candles. I. Flexible cosmological fits
• Effects of cosmological model assumptions on galaxy redshift survey measurements
• Long-term monitoring of PKS 0537-441 with Fermi-LAT and multiwavelength observations
• Sandage-Loeb test for the new agegraphic and Ricci dark energy models
• A combined measurement of cosmic growth and expansion from clusters of galaxies, the CMB and galaxy clustering
• Impact of Primordial Ultracompact Minihaloes on the Intergalactic Medium and First Structure Formation
• Massive Photon and Dark Energy
• Andromeda's Parachute: A Bright Quadruply Lensed Quasar at z=2.377
• Appeasing the Phantom Menace?
• Reducing distance errors for standard candles and standard sirens with weak-lensing shear and flexion maps
• HD/H2 Molecular Clouds in the Early Universe: The Problem of Primordial Deuterium
• Mass Function of Rich Galaxy Clusters and Its Constraint on sigma_8
• Cosmic variance limited Baryon Acoustic Oscillations from the DEUS-FUR $\Lambda$CDM simulation
• Primordial perturbations and non-Gaussianities from modulated trapping
• Cosmography of f(R) - brane cosmology
• Background history and cosmic perturbations for a general system of self-conserved dynamical dark energy and matter
• Testable dark energy predictions from current data
• Holographic Ricci dark energy in Randall-Sundrum braneworld: Avoidance of big rip and steady state future
• Axion Searches with Helioscopes and astrophysical signatures for axion(-like) particles
• Shedding Light on the Dark Sector with Direct WIMP Production
• Determining the WIMP mass using the complementarity between direct and indirect searches and the ILC
• Non-vacuum Solutions of Bianchi Type VI_0 Universe in f(R) Gravity
• Mapping the allowed parameter space for decaying dark matter models
• Anisotropic Trispectrum of Curvature Perturbations Induced by Primordial Non-Abelian Vector Fields
• Testing statistics of the CMB B-mode polarization toward unambiguously establishing quantum fluctuation of vacuum
• Constraining reionization using 21 cm observations in combination with CMB and Lyman-alpha forest data
• Cosmic perturbations with running G and Lambda
• Probing the Effective Number of Neutrino Species with Cosmic Microwave Background
• H.E.S.S. observations of the globular clusters NGC 6388 and M 15 and search for a Dark Matter signal
• On the scalar consistency relation away from slow roll
• Cosmology dependency of halo masses and concentrations in hydrodynamic simulations
• A Simplified Quantum Gravitational Model of Inflation
• On the relative abundance of LiH and LiH+ molecules in the early universe: new results from quantum reactions
• Non-Minimal Sneutrino Inflation, Peccei-Quinn Phase Transition and non-Thermal Leptogenesis
• Global stability analysis for cosmological models with non-minimally coupled scalar fields
• On the determination of curvature and dynamical Dark Energy
• The clustering of galaxies and galaxy clusters: constraints on primordial non-Gaussianity from future wide-field surveys
• The Inhomogeneous Ionizing Background Following Reionization
• The dark matter assembly of the Local Group in constrained cosmological simulations of a LambdaCDM universe
• The Quijote CMB Experiment
• Too small to succeed? Lighting up massive dark matter subhaloes of the Milky Way
• Stars, Dust, and the Growth of UV-Selected Sub-L* Galaxies at Redshift z~2
• Measuring primordial non-Gaussianity through weak lensing peak counts
• The growth of linear perturbations in the DGP model
• The spherical collapse model in time varying vacuum cosmologies
• Constraints on modified gravity from the observed X-ray luminosity function of galaxy clusters
• Dark energy model with variable $q$ and $\omega$ in LRS Bianchi-II space-time
• Joint growth rate measurements from redshift-space distortions and peculiar velocities in the 6dF Galaxy Survey
• A Supersymmetric B-L Dark Matter Model and the Observed Anomalies in the Cosmic Rays
• Structure, Kinematics, and Chemical Enrichment Patterns after Major Gas-Rich Disc-Disc Mergers
• Discovery of 16 New z ~ 5.5 Quasars : Filling in the Redshift Gap of Quasar Color Selection
• Studying topological structure in the epoch of reionization with 3D-Minkowski functionals of 21cm line fluctuations
• Dark Energy and the Return of the Phoenix Universe
• New Interaction between Dark Energy and Dark Matter Changes Sign during Cosmological Evolution
• Galaxy power spectrum in redshift space: combining perturbation theory with the halo model
• Scale-invariant perturbations in ekpyrotic cosmologies without fine-tuning of initial conditions
• New Constraints on variations of the fine structure constant from CMB anisotropies
• Scale Dependent Local Non-Gaussianity from Loops
• A Hydrodynamical Solution for the "Twin-Tailed" Colliding Galaxy Cluster "El Gordo"
• TeV Gamma-ray Astronomy: A Summary
• Projected central dark matter fractions and densities in massive early-type galaxies from the Sloan Digital Sky Survey
• Non-Gaussianity and Baryonic Isocurvature Fluctuations in the Curvaton Scenario
• The growth index of matter perturbations and modified gravity
• First results on the cluster galaxy population from the Subaru Hyper Suprime-Cam survey. III. Brightest cluster galaxies, stellar mass distribution, and active galaxies
• Strongly Scale-dependent Non-Gaussianity
• Nongaussianity from Particle Production During Inflation
• Cosmological Constraints on Decaying Dark Matter
• Use of event-level neutrino telescope data in global fits for theories of new physics
• Weighing the Local Group in the Presence of Dark Energy
• Constraining warm dark matter with cosmic shear power spectra
• Cosmological investigations of (extended) nonlinear massive gravity schemes with non-minimal coupling
• Cosmological constraints on generalized Chaplygin gas model: Markov Chain Monte Carlo approach
• Interacting Cosmological Fluids and the Coincidence Problem
• CMB Polarization Systematics Due to Beam Asymmetry: Impact on Cosmological Birefringence
• Massive Milky Way Satellites in Cold and Warm Dark Matter: Dependence on Cosmology
• How well will ton-scale dark matter direct detection experiments constrain minimal supersymmetry?
• Sensitivity of galaxy cluster dark energy constraints to halo modeling uncertainties
• Gauss-Bonnet Inflation after Planck2018
• Universally Leptophilic Dark Matter From Non-Abelian Discrete Symmetry
• Will there be again a transition from acceleration to deceleration in course of the dark energy evolution of the universe?
• The nature of the ISM in galaxies during the star-formation activity peak of the Universe
• Consequences of energy conservation violation: Late time solutions of $\Lambda (T)CDM$ subclass of $f(R,T)$ gravity using dynamical system approach
• Cartan symmetries and global dynamical systems analysis in a higher-order modified teleparallel theory
• Cosmic acceleration from modified gravity with Palatini formalism
• Dynamical symmetries and observational constraints in scalar field cosmology
• The structure function of variable 1.4 GHz radio sources based on NVSS and FIRST observations
• Cosmological surveys with the Australian Square Kilometre Array Pathfinder
• Gravitational lensing as a probe of cold dark matter subhalos
• Selecting a Model of Supersymmetry Breaking Mediation
• Anisotropic bispectrum of curvature perturbations from primordial non-Abelian vector fields
• Weak lensing predictions for modified gravities at non-linear scales
• Reconstruction Procedure in Nonlocal Cosmological Models
• Chemical enrichment in very low-metallicity environments: Bootes I
• Effects of time-varying $\beta$ in SNLS3 on constraining interacting dark energy models
• Structure Formation in Modified Gravity Scenarios
• Studying the WHIM with Gamma Ray Bursts
• Analytic rotating black hole solutions in $N$-dimensional $f(T)$ gravity
• The visibility of Lyman Alpha Emitters: constraining reionization, ionizing photons and dust
• Constraints on f_nl and g_nl from the analysis of the N-pdf of the CMB large scale anisotropies
• Imprints of Dark Energy on Cosmic Structure Formation: III. Sparsity of Dark Matter Halo Profiles
• Early Dark Energy at High Redshifts: Status and Perspectives
• Constraining chameleon field theories using the GammeV afterglow experiments
• Sample variance and Lyman-alpha forest transmission statistics
• Constraints on the anisotropy of dark energy
• Oscillations of the F(R) dark energy in the accelerating universe
• Non-Minimally Gravity-Coupled Inflationary Models
• The core-cusp problem in cold dark matter halos and supernova feedback: Effects of Mass Loss
• $\nu$-Two Higgs Doublet Model and its Collider Phenomenology
• Light Stop from b-tau Yukawa Unification
• Screening of cosmological constant for De Sitter Universe in non-local gravity, phantom-divide crossing and finite-time future singularities
• Measuring Redshift-Space Distortions using Photometric Surveys
• Hot-Dust-Poor Quasars in Mid-Infrared and Optically Selected Samples
• Constraints on growth index parameters from current and future observations
• Generation of Circular Polarization of the Cosmic Microwave Background
• Probing deviations from General Relativity with the Euclid spectroscopic survey
• Simultaneous Ultraviolet and Optical Emission-line Profiles of Quasars: Implications for Black Hole Mass Determination
• Probing dark energy and neutrino mass from upcoming lensing experiments of CMB and galaxies
• Reconciling MOND and dark matter?
• Reconstructing $f(R)$ Theory from Ricci Dark Energy
• Imprints of primordial non-Gaussianity on the number counts of cosmic shear peaks
• Parsec-scale structures and diffuse bands in a translucent interstellar medium at z 0.079
• Light dark matter in the NMSSM: upper bounds on direct detection cross sections
• Edge Detection, Cosmic Strings and the South Pole Telescope
• Revisiting light neutralino scenarios in the MSSM
• A high precision semi-analytic mass function
• Studying 21cm power spectrum with one-point statistics
• Cosmological observations in a modified theory of gravity (MOG)
• Accelerating dark energy models with anisotropic fluid in Bianchi type-$V{I}_0$ space-time
• Search for Dark Matter
• Matter power spectrum from a Lagrangian-space regularization of perturbation theory
• Cosmic equation of state from combined angular diameter distances: Does the tension with luminosity distances exist?
• A Break in Spiral Galaxy Scaling Relations at the Upper Limit of Galaxy Mass
• Precision modelling of the matter power spectrum in a Planck-like Universe
• Supernovae and AGN driven galactic outflows
• HD molecules at high redshift: The absorption system at z=2.3377 towards Q 1232+082
• Light paths of normal and phantom Einstein-Maxwell-dilaton black holes
• A New Method to Quantify Environment and Model Ram-Pressure Stripping in N-Body Simulations
• Unified Dark Matter models with fast transition
• Conformally Friedmann-Lemaitre-Robertson-Walker cosmologies
• Scale-Dependent Non-Gaussianity as a Generalization of the Local Model
• Probing the cosmic web: inter-cluster filament detection using gravitational lensing
• Modelling large-scale halo bias using the bispectrum
• Measuring the Dark Force at the LHC
• Scalar Contribution to the Graviton Self-Energy during Inflation
• The Cosmic Evolution of Faint Satellite Galaxies as a Test of Galaxy Formation and the Nature of Dark Matter
• Effects of Ultraviolet Background and Local Stellar Radiation on the H_I Column Density Distribution
• Cosmological parameters after WMAP5: forecasts for Planck and future galaxy surveys
• Cosmology Inference from Biased Tracers using the EFT-based Likelihood
• A Phenomenological Model for the Early Universe
• Cosmological implications and structure formation from a time varying vacuum
• First Science with SAMI: A Serendipitously Discovered Galactic Wind in ESO 185-G031
• Renegade Subhaloes in the Local Group
• Two ultimate tests of constrained supersymmetry
• Orientation of cosmic web filaments with respect to the underlying velocity field
• Separating E and B types of polarization on an incomplete sky
• Fractal initial conditions and natural parameter values in hybrid inflation
• Primordial Non-Gaussianities from the Trispectra in Multiple Field Inflationary Models
• Reconstruction of f(T) gravity according to holographic dark energy
• Regarding the Line-of-Sight Baryonic Acoustic Feature in the Sloan Digital Sky Survey and Baryon Oscillation Spectroscopic Survey Luminous Red Galaxy Samples
• A step towards testing general relativity using weak gravitational lensing and redshift surveys
• The Jubilee ISW Project I: simulated ISW and weak lensing maps and initial power spectra results
• Tension in the Recent Type Ia Supernovae Datasets
• Lyman-alpha transfer in primordial hydrogen recombination
• ALMA Observations of Nearby Luminous Infrared Galaxies with Various AGN Energetic Contributions Using Dense Gas Tracers
• A Gravitational Mechanism for Cosmological Screening
• The Atacama Cosmology Telescope: A Measurement of the Thermal Sunyaev-Zel'dovich Effect Using the Skewness of the CMB Temperature Distribution
• Multicomponent and Variable Velocity Galactic Outflow in Cosmological Hydrodynamic Simulations
• Possible antigravity regions in $F(R)$ theory?
• ALMA Detection of the Vibrationally Excited HCN J=4-3 Emission Line in the AGN-Hosting Luminous Infrared Galaxy IRAS 20551-4250
• Estimating relic magnetic fields from CMB temperature correlations
• Revising the observable consequences of slow-roll inflation
• Light Dark Matter Candidate in B-L Gauged Radiative Inverse Seesaw
• M87 black hole mass and spin estimate through the position of the jet boundary shape break
• Preinflationary dynamics in loop quantum cosmology: Monodromy Potential
• Fully Loop-Quantum-Cosmology-corrected propagation of gravitational waves during slow-roll inflation
• Polarised foreground removal at low radio frequencies using rotation measure synthesis: uncovering the signature of hydrogen reionisation
• Modified Holographic Dark Energy
• Non-minimal kinetic coupling and the phenomenology of dark energy
• Inflation, baryogenesis and gravitino dark matter at ultra low reheat temperatures
• A solution to the anisotropy problem in bouncing cosmologies
• Cosmological Solutions of a Nonlocal Model with a Perfect Fluid
• The Importance of Slow-roll Corrections During Multi-field Inflation
• Adaptive Mesh Refinement Simulations of Galaxy Formation: Exploring Numerical and Physical Parameters
• Parameter estimation for coalescing massive binary black holes with LISA using the full 2-post-Newtonian gravitational waveform and spin-orbit precession
• Improved constraints on primordial non-Gaussianity for the Wilkinson Microwave Anisotropy Probe 5-yr data
• Global integrability of cosmological scalar fields
• The Impact of Theoretical Uncertainties in the Halo Mass Function and Halo Bias on Precision Cosmology
• Inflation driven by scalar field with non-minimal kinetic coupling with Higgs and quadratic potentials
• Inflationary signatures of single-field models beyond slow-roll
• Notes on teleparallel cosmology with nonminimally coupled scalar field
• Kinetic decoupling of WIMPs: analytic expressions
• High-energy sources at low radio frequency: the Murchison Widefield Array view of Fermi blazars
• Can Early Dark Energy be Detected in Non-Linear Structure?
• Hierarchical Galaxy Growth and Scatter in the Stellar Mass - Halo Mass Relation
• Orbital anisotropy in cosmological haloes revisited
• No observational constraints from hypothetical collisions of hypothetical dark halo primordial black holes with galactic objects
• Observing Dark Stars with JWST
• Constraints on the sum of neutrino masses using cosmological data including the latest extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample
• Were progenitors of local L* galaxies Lyman-alpha emitters at high redshift?
• A geometric solution to the coincidence problem, and the size of the landscape as the origin of hierarchy
• Eternal inflation predicts that time will end
• Revisiting the WMAP - NVSS angular cross correlation. A skeptic's view
• Excursion Sets and Non-Gaussian Void Statistics
• Non-Gaussianity from resonant curvaton decay
• Direct Collapse to Supermassive Black Hole Seeds with Radiative Transfer: Isolated Halos
• Measuring the 2D Baryon Acoustic Oscillation signal of galaxies in WiggleZ: Cosmological constraints
• Constraining the dark fluid
• Kaluza-Klein Cosmology With Modified Holographic Dark Energy
• Single-field inflation constraints from CMB and SDSS data
• How to generate a significant effective temperature for cold dark matter, from first principles
• A novel teleparallel dark energy model
• Primordial features and Planck polarization
• Forecasts for Dark Energy Measurements with Future HI Surveys
• Halo abundances in the f_{nl} model
• The effect of massive neutrinos on the Sunyaev-Zeldovich and X-ray observables of galaxy clusters
• The formation of CDM haloes I: Collapse thresholds and the ellipsoidal collapse model
• The Primordial Inflation Polarization Explorer (PIPER)
• Constraints on dark energy from the lookback time versus redshift test
• Luminous Red Galaxy Halo Density Field Reconstruction and Application to Large Scale Structure Measurements
• The galaxies that reionized the Universe
• Quintessence with Yukawa Interaction
• SUGRA Hybrid Inflation with Shift Symmetry
• Leptogenesis, Gravitino Dark Matter and Entropy Production
• Avoiding the blue spectrum and the fine-tuning of initial conditions in hybrid inflation
• Observational constraints on K-inflation models
• Gravitational Wave Background and Non-Gaussianity as a Probe of the Curvaton Scenario
• $\alpha$-vacuum and inflationary bispectrum
• Tight constraints on F- and D-term hybrid inflation scenarios
• Mass function and bias of dark matter halos for non-Gaussian initial conditions
• Exploring the Systematic Uncertainties of Type Ia Supernovae as Cosmological Probes
• LUX likelihood and limits on spin-independent and spin-dependent WIMP couplings with LUXCalc
• Optimal dataset combining in f_nl constraints from large scale structure in an idealised case
• Estimating Luminosity Function Constraints from High-Redshift Galaxy Surveys
• The Atacama Cosmology Telescope: Calibration with WMAP Using Cross-Correlations
• Dark matter scaling relations in intermediate z haloes
• Intrinsic Physical Conditions and Structure of Relativistic Jets in Active Galactic Nuclei
• The extreme limit of the generalized Chaplygin gas
• A parametrization for the growth index of linear matter perturbations
• Phenomenological Constraints on Axion Models of Dynamical Dark Matter
• Optimal Weighting in Galaxy Surveys: Application to Redshift-Space Distortions
• Impact of Galactic polarized emission on B-mode detection at low multipoles
• Using a phenomenological model to test the coincidence problem of dark energy
• Secondary infall model and dark matter scaling relations in intermediate redshift early - type galaxies
• Fluctuations of cosmological birefringence and the effect on CMB B-mode polarization
• Reheating after f(R) inflation
• The clustering of galaxy clusters in cosmological models with non-Gaussian initial conditions: Predictions for future surveys
• Non-Gaussianity in single field models without slow-roll
• A comparison of hard X-ray photon indices and iron \ka emission lines in X-ray luminous narrow- and broad-line Seyfert 1 galaxies
• On the Issue of the ζSeries Convergence and Loop Corrections in the Generation of Observable Primordial Non-Gaussianity in Slow-Roll Inflation. Part II: the Trispectrum
• The stellar evolution of Luminous Red Galaxies, and its dependence on colour, redshift, luminosity and modelling
• The Trispectrum in the Multi-brid Inflation
• Non-Minimal Inflation Revisited
• Prospects of observing a quasar HII region during the Epoch of Reionization with redshifted 21cm
• Unified Dark Matter scalar field models with fast transition
• Calculable inverse-seesaw neutrino masses in supersymmetry
• A direct measurement of tomographic lensing power spectra from CFHTLenS
• Leptogenesis origin of Dirac gaugino dark matter
• Shedding Light on Dark Matter at Colliders
• CMB Scale Dependent Non-Gaussianity from Massive Gravity during Inflation
• A Re-analysis of Gravitino Dark Matter in the Constrained MSSM
• Primordial B-mode Diagnostics and Self Calibrating the CMB Polarization
• Limits on Cosmological Birefringence from the Ultraviolet Polarization of Distant Radio Galaxies
• MOJAVE XVI: Multi-Epoch Linear Polarization Properties of Parsec-Scale AGN Jet Cores
• Cold Dark Matter Isocurvature Perturbations: Constraints and Model Selection
• VLBA observations of a rare multiple quasar imaging event caused by refraction in the interstellar medium
• Integrated Sachs-Wolfe Effect for Gravitational Radiation
• Dark Matter as a Guide Toward a Light Gluino at the LHC
• Coannihilation Scenarios and Particle Spectroscopy in SU(4)_c x SU(2)_L x SU(2)_R
• Using galaxy-galaxy weak lensing measurements to correct the Finger-of-God
• Lensing reconstruction from PLANCK sky maps: inhomogeneous noise
• Saving Natural Inflation
• The connection between black hole mass and Doppler boosted emission in BL Lacertae type objects
• Breaking the Degeneracy: Optimal Use of Three-point Weak Lensing Statistics
• Adjoint SUSY $SU(5)$ Grand Unified Model with $S_4$ Flavor Symmetry
• Signatures of Primordial non-Gaussianities in the Matter Power-Spectrum and Bispectrum: the Time-RG Approach
• Fourth-order gravity as the inflationary model revisited
• Convergence properties of halo merger trees; halo and substructure merger rates across cosmic history
• Cosmic distance duality and cosmic transparency
• Dark Energy from graviton-mediated interactions in the QCD vacuum
• Primordial Perturbations in Einstein-Aether and BPSH Theories
• Interacting viscous dark fluids
• Neutrino Fluxes from CMSSM LSP Annihilations in the Sun
• Dynamical symmetries in Brans-Dicke cosmology
• The holographic induced gravity model with a Ricci dark energy: smoothing the little rip and big rip through Gauss-Bonnet effects?
• Properties of Type II Plateau Supernova SNLS-04D2dc: Multicolor Light Curves of Shock Breakout and Plateau
• Constraints on the Holographic Dark Energy Model from Type Ia Supernovae, WMAP7, Baryon Acoustic Oscillation and Redshift-Space Distortion
• Probing non-standard gravity with the growth index: a background independent analysis
• Gamma Ray Burst and star formation rates: The physical origin for the redshift evolution of their ratio
• Massive black holes in central cluster galaxies
• What if Supersymmetry Breaking Unifies beyond the GUT Scale?
• The evolution of the helium-ionizing background at z ~ 2-3
• Conservation of the nonlinear curvature perturbation in generic single-field inflation
• Stellar Populations of Lyman Break Galaxies at z=1-3 in the HST/WFC3 Early Release Science Observations
• A model-independent test for scale-dependent non-Gaussianities in the CMB
• Supermassive Black Hole Formation at High Redshifts Through a Primordial Magnetic Field
• Impact of Chandra calibration uncertainties on galaxy cluster temperatures: application to the Hubble Constant
• From the early to the late time universe within $f(T,\mathcal{T})$ gravity
• Use of delta N formalism - Difficulties in generating large local-type non-Gaussianity during inflation -
• Phenomenology of SUSY SU(5) with type I+III seesaw
• Polarizing Bubble Collisions
• More about the Tolman-Oppenheimer-Volkoff equations for the generalized Chaplygin gas
• A Search for the Dark Matter Annual Modulation in South Pole Ice
• Dark Matter Annihilation around Intermediate Mass Black Holes: an update
• Two- and Three-Dimensional Probes of Parity in Primordial Gravity Waves
• The history of the dark and luminous side of Milky Way-like progenitors
• On the Correlation Between the Spin-Independent and Spin-Dependent Direct Detection of Dark Matter
• Muon Fluxes From Dark Matter Annihilation
• Free scalar dark matter candidates in R^2-inflation: the light, the heavy and the superheavy
• Gauss-Bonnet Chameleon Mechanism of Dark Energy
• PTF11mnb: the first analog of supernova 2005bf
• Spectral Energy Distributions of Type 1 AGN in XMM-COSMOS Survey II - Shape Evolution
• Evidence of internal rotation and a helical magnetic field in the jet of the quasar NRAO150
• WMAP 7 year constraints on CPT violation from large angle CMB anisotropies
• The velocity shear and vorticity across redshifts and non-linear scales
• A Markov Chain Monte Carlo Algorithm for analysis of low signal-to-noise CMB data
• Cosmic Discordance: Detection of a modulation in the primordial fluctuation spectrum
• COSMOS weak-lensing constraints on modified gravity
• CMB Beam Systematics: Impact on Lensing Parameter Estimation
• Weak Evolution of the Mass-metallicity Relation at Cosmic Dawn in the FirstLight Simulations
• Measuring primordial non-Gaussianity with weak-lensing surveys
• KiDS-Legacy calibration: unifying shear and redshift calibration with the SKiLLS multi-band image simulations
• Revisiting Metastable Dark Energy and Tensions in the Estimation of Cosmological Parameters
• High Redshift Standard Candles: Predicted Cosmological Constraints
• MOJAVE. XX. Persistent Linear Polarization Structure in Parsec-scale AGN Jets
• Quantum Gravity Corrections and Entropy at the Planck time
• Analysis of Generalized Ghost Pilgrim Dark Energy in Non-flat FRW Universe
• Universality of the Volume Bound in Slow-Roll Eternal Inflation
• Deep learning approach for identification of HII regions during reionization in 21-cm observations
• Direct Detection of Dynamical Dark Matter
• N-vaton
• Understanding `galaxy groups' as a unique structure in the universe
• Cosmological Evolution and Exact Solutions in a Fourth-order Theory of Gravity
• Saraswati: An Extremely Massive ~ 200 Megaparsec Scale Supercluster
• Supernovae as seen by off-center observers in a local void
• Robustness to systematics for future dark energy probes
• Detecting Lyman Alpha Emitters in the Sub-millimeter
• SNIa-Cosmology Analysis Results from Simulated LSST Images: from Difference Imaging to Constraints on Dark Energy
• Combining perturbation theories with halo models for the matter bispectrum
• A parametric study of possible solutions to the high-redshift overproduction of stars in modeled dwarf galaxies
• Double Type-II Seesaw, Baryon Asymmetry and Dark Matter for Cosmic e^\pm Excesses
• The impact of correlated projections on weak lensing cluster counts
• Dilaton-assisted Dark Matter
• Constraints on the neutrino parameters by future cosmological 21cm line and precise CMB polarization observations
• Sloshing in its cD halo: MUSE kinematics of the central galaxy NGC 3311
• Short-Term Radio Variability and Parsec-Scale Structure in a Gamma-Ray Narrow-Line Seyfert 1 Galaxy 1H 0323+342
• The Implications of Gunn-Peterson Troughs in the HeII Lyman-alpha Forest
• The wedge bias in reionization 21-cm power spectrum measurements
• Weak lensing signal in Unified Dark Matter models
• Anisotropic inflation in Gauss-Bonnet gravity
• Machine learning constraints on deviations from general relativity from the large scale structure of the Universe
• Galaxy downsizing evidenced by hybrid evolutionary tracks
• Constraints on the Reheating Parameters after Gauss-Bonnet Inflation from the Primordial Gravitational Waves
• Inflaton dark matter from incomplete decay
• Detecting relic gravitational waves in the CMB: Optimal parameters and their constraints
• First constraints on the running of non-Gaussianity
• On using the WMAP distance priors in constraining the time evolving equation of state of dark energy
• Path Integral for Inflationary Perturbations
• Multi-field Inflation with a Random Potential
• Cosmic propagators at two-loop order
• Alignment of Brightest Cluster Galaxies with their Host Clusters
• Bayesian inferences of galaxy formation from the K-band luminosity and HI mass functions of galaxies: constraining star formation and feedback
• Comparison of Recent SnIa datasets
• The mass function of nearby black hole candidates
• Observational constraints on cosmic neutrinos and dark energy revisited
• Chern-Simons EM-flation
• Model-independent constraints on ${\Omega }_m$ and $H(z)$ from the link between geometry and growth
• Bimetric structure formation: non-Gaussian predictions
• Observable effects of anisotropic bubble nucleation
• Confronting the relaxation mechanism for a large cosmological constant with observations
• Oscillations in the Primordial Bispectrum: Mode Expansion
• The Cosmological Constant Problem, Dark Energy, and the Landscape of String Theory
• General parity-odd CMB bispectrum estimation
• Matter and Dark Matter from False Vacuum Decay
• Dark Matter in the MSSM
• Precious Metals in SDSS Quasar Spectra II: Tracking the Evolution of Strong, 0.4 < z < 2.3 MgII Absorbers with Thousands of Systems
• Cosmological perturbations in SFT inspired non-local scalar field models
• Fluctuations in the Ionizing Background During and After Helium Reionization
• Dark Matter Signatures in the Anisotropic Radio Sky
• Dark energy from scalar field with Gauss Bonnet and non-minimal kinetic coupling
• Probing the Epoch of Reionization with the Lyman Alpha Forest at z~4-5
• Curvaton reheating in logamediate inflationary model
• FirstLight III: Rest-frame UV-optical spectral energy distributions of simulated galaxies at cosmic dawn
• Damping of Primordial Gravitational Waves from Generalized Sources
• Distance Priors from \emph{Planck} 2015 data
• ALMA Investigation of Vibrationally Excited HCN/HCO+/HNC Emission Lines in the AGN-Hosting Ultraluminous Infrared Galaxy IRAS 20551-4250
• Validating a minimal galaxy bias method for cosmological parameter inference using HSC-SDSS mock catalogs
• Cosmic age, Statefinder and $Om$ diagnostics in the decaying vacuum cosmology
• Figures of merit for present and future dark energy probes
• Multi-Stream Inflation
• Including birefringence into time evolution of CMB: current and future constraints
• Directional Variations of the Non-Gaussianity Parameter f_NL
• Testing the imprint of non-standard cosmologies on void profiles using Monte Carlo random walks
• Testing gaussianity, homogeneity and isotropy with the cosmic microwave background
• The stellar populations of quiescent ultra-diffuse galaxies from optical to mid-infrared spectral energy distribution fitting
• Transit cosmological models with observational constraints in f(Q, T) gravity
• SALT2 Versus SALT3: Updated Model Surfaces and Their Impacts on Type Ia Supernova Cosmology
• On Non-Gaussianities in Multi-Field Inflation (N fields): Bi- and Tri-spectra beyond Slow-Roll
• Primordial Non-Gaussianity in Models with Dark Matter Isocurvature Fluctuations
• Predictions from Star Formation in the Multiverse
• Isocurvature modes in the CMB bispectrum
• First lensing measurements of SZ-discovered clusters
• On Non-Canonical Kinetic Terms and the Tilt of the Power Spectrum
• Residual Hubble-bubble effects on supernova cosmology
• Direct Detection of the Cosmic Neutrino Background Including Light Sterile Neutrinos
• Graviton Corrections to Maxwell's Equations
• Primordial Helium Abundance from CMB: a constraint from recent observations and a forecast
• Dark Energy Content of Nonlinear Electromagnetism
• Following the Cosmic Evolution of Pristine Gas III: The Observational Consequences of the Unknown Properties of Population III Stars
• Cosmological parameter extraction and biases from type Ia supernova magnitude evolution
• Testing gravity using the growth of large scale structure in the Universe
• Can high-redshift Hubble diagrams rule out the standard model of cosmology in the context of cosmographic method?
• Modified scalar and tensor spectra in spinor driven inflation
• Hybrid natural inflation from non Abelian discrete symmetry
• Two-fluid atmosphere from decelerating to accelerating FRW dark energy models
• Electroweak Baryogenesis, CDM and Anomaly-free Supersymmetric U(1)-prime Models
• Non-minimally coupled dark matter: effective pressure and structure formation
• Effects of Dark Energy Perturbations on Cosmological Tests of General Relativity
• Non-Gaussianity from Isocurvature Perturbations : Analysis of Trispectrum
• The 6dF Galaxy Survey: Dependence of halo occupation on stellar mass
• Monopoles, strings and dark matter
• Phantom without ghost
• What is half a neutrino? Reviewing cosmological constraints on neutrinos and dark radiation
• Extending the Hubble diagram by gamma ray bursts
• Qualitative analysis of Kantowski-Sachs metric in a generic class of $f(R)$ models
• Beware of Fake $\nu$s: The Effect of Massive Neutrinos on the Nonlinear Evolution of Cosmic Structure
• Reconstruction of k-essence model
• Bright Lyman-alpha Emitters at z~9: constraints on the luminosity function from HiZELS
• Minimal Dirac Fermionic Dark Matter with Nonzero Magnetic Dipole Moment
• Search for inelastic dark matter with the CDMS II experiment
• Cosmological attractor inflation from the RG-improved Higgs sector of finite gauge theory
• Neutralino, axion and axino cold dark matter in minimal, hypercharged and gaugino AMSB
• Bayesian Comparison of Interacting Scenarios
• Predictions for the 21cm-galaxy cross-power spectrum observable with LOFAR and Subaru
• Effects of cosmological parameters and star formation models on the cosmic star formation history in LambdaCDM cosmological simulations
• Warm tachyonic inflation in warped background
• A tale of dark matter capture, sub-dominant WIMPs, and neutrino observatories
• The y-sky: diffuse spectral distortions of the cosmic microwave background
• Big Rip and Little Rip solutions in scalar model with kinetic and Gauss Bonnet couplings
• Bright High z SnIa: A Challenge for LCDM?
• MOJAVE: Monitoring of Jets in Active Galactic Nuclei with VLBA Experiments. IX. Nuclear opacity
• Studying the Sources of Cosmic Reionization with 21-cm Fluctuations
• Modified f(G) gravity models with curvature-matter coupling
• Constraints on Lorentz Invariance Violation with gamma-ray bursts via a Markov Chain Monte Carlo approach
• A New Statistic for Analyzing Baryon Acoustic Oscillations
• Simulations of Quintessential Cold Dark Matter: beyond the cosmological constant
• Cosmic Constraint to DGP Brane Model: Geometrical and Dynamical Perspectives
• A QSO host galaxy and its Lyalpha emission at z=6.43
• Search for Gamma Ray Bursts with the Argo-YBJ Detector in Scaler Mode
• The Impact of Coupled Dark Energy Cosmologies on the High-Redshift Intergalactic Medium
• A Measurement of Arcminute Anisotropy in the Cosmic Microwave Background with the Sunyaev-Zel'dovich Array
• Big Bang Nucleosynthesis constraints on $f(T,\mathcal{T})$ gravity
• Inflation in non-minimal matter-curvature coupling theories
• Supergravity Higgs Inflation and Shift Symmetry in Electroweak Theory
• Direct Collapse to Supermassive Black Hole Seeds with Radiation Transfer: Cosmological Halos
• Sneutrino Dark Matter: Symmetry Protection and Cosmic Ray Anomalies
• Light Neutralino in the MSSM: a playground for dark matter, flavor physics and collider experiments
• The growth factor of matter perturbations in an f(R) gravity
• Hubble tension as a guide for refining the early Universe: Cosmologies with explicit local Lorentz and diffeomorphism violation
• A Method for Measuring the Bias of High-Redshift Galaxies from Cosmic Variance
• Exploring the disk-jet connection in NGC 315
• Agegraphic dark energy: growth index and cosmological implications
• Detailed study of geodesics in the Kerr-Newman-(A)dS spactime and the rotating charged black hole spacetime in $f(R)$ gravity
• Bimodal radio variability in OVRO-40m-monitored blazars
• Determining the escape fraction of ionizing photons during reionization with the GRB derived star-formation rate
• Induced cosmological constant and other features of asymmetric brane embedding
• An Estimator for statistical anisotropy from the CMB bispectrum
• Structure formation in the Deser-Woodard nonlocal gravity model: a reappraisal
• Cosmological magnetic field survival
• Resonant scattering and recombination of pseudo-degenerate WIMPs
• Non-Gaussianity from Axionic Curvaton
• A Common Framework for Dark Matter, Leptogenesis and Neutrino Masses
• Astrophysical limits on light NMSSM neutralinos
• Moving around the cosmological parameter space: a nonlinear power spectrum reconstruction based on high-resolution cosmic responses
• ELUCID. VI: Cosmic variance of galaxy distribution in the local Universe
• Robustness of cosmic neutrino background detection in the cosmic microwave background
• Dark Matter via Many Copies of the Standard Model
• Cosmography with cluster strong lensing
• Correction to Lagrangian for Bouncing Cosmologies in $f(Q)$ Gravity
• Reionization constraints from five-year WMAP data
• Effect of Background Evolution on the Curvaton Non-Gaussianity
• Localization of nonlocal cosmological models with quadratic potentials in the case of double roots
• Weak lensing and the Dyer-Roeder approximation
• The correlation function of galaxy clusters and detection of baryon acoustic oscillations
• Observational constraints of a power spectrum from super-inflation in Loop Quantum Cosmology
• Measuring the reionization optical depth without large-scale CMB polarization
• The Matter Bispectrum in N-body Simulations with non-Gaussian Initial Conditions
• Surface convection and red giants radii measurements
• TXS 0128+554: A Young Gamma-Ray Emitting AGN With Episodic Jet Activity
• Modified holographic dark energy in DGP brane world
• Using Multipoles of the Correlation Function to Measure H(z), D_A(z), and β(z) from Sloan Digital Sky Survey Luminous Red Galaxies
• Determination of neutrino mass hierarchy by 21 cm line and CMB B-mode polarization observations
• Effects of the sources of reionization on 21-cm redshift-space distortions
• Quasar Photometric Redshifts and Candidate Selection: A New Algorithm Based on Optical and Mid-Infrared Photometric Data
• Semi-analytic galaxy formation in f(R)-gravity cosmologies
• On the non-Gaussianity from Recombination
• Detection of Signals from Cosmic Reionization using Radio Interferometric Signal Processing
• Multiple Dark Matter as a self-regulating mechanism for dark sector interactions
• Stochastic Gravitational Wave Background from Neutron Star r-mode Instability Revisited
• A Multiband Study of the Galaxy Populations of the First Four Sunyaev--Zeldovich Effect selected Galaxy Clusters
• The impact of a strongly first-order phase transition on the abundance of thermal relics
• Extracting cosmological information from the angular power spectrum of the 2MASS Photometric Redshift catalogue
• New Generalizations of Cosmography Inspired by the Pade Approximant
• Supernova light-curve fitters and Dark Energy
• Submillimeter Galaxy Number Counts and Magnification by Galaxy Clusters
• Averaging Robertson-Walker Cosmologies
• Constraining DGP Gravity from Observational Data
• Varying couplings in the early universe: correlated variations of $\alpha$ and $G$
• A Non-minimally Coupled Quintom Dark Energy Model on the Warped DGP Brane
• Physical properties of Herschel selected galaxies in a semi-analytic galaxy formation model
• Inflation and Reheating in Spontaneously Generated Gravity
• Cold Dark Matter in non-Standard Cosmologies, PAMELA, ATIC and Fermi LAT
• Reionization of the Local Group of Galaxies
• Chameleonic Generalized Brans--Dicke model and late-time acceleration
• Impact of calibration errors on CMB component separation using FastICA and ILC
• Probability of the most massive cluster under non-Gaussian initial conditions
• Multi-scale analysis of turbulence evolution in the density stratified intracluster medium
• Population statistics of beamed sources. II: Evaluation of Doppler factor estimates
• Abundances, masses, and weak-lensing mass profiles of galaxy clusters as a function of richness and luminosity in LambdaCDM cosmologies
• Towards a solution of the cosmological constant problem
• Cosmological matching conditions for gravitational waves at second order
• The Deuterium Abundance in the Local Interstellar Medium
• Measuring redshift through X-ray spectroscopy of galaxy clusters: results from Chandra data and future prospects
• Analytical Approach for the Determination of the Luminosity Distance in a Flat Universe with Dark Energy
• Stellar Black Holes and the Origin of Cosmic Acceleration
• Polytropic dark matter flows illuminate dark energy and accelerated expansion
• Evolution of Dark Energy Perturbations in Scalar-Tensor Cosmologies
• A Geometrical Approach to Strong Gravitational Lensing in f(R) Gravity
• Fully-Coupled Simulation of Cosmic Reionization. I: Numerical Methods and Tests
• Galaxy Cluster Bulk Flows and Collision Velocities in QUMOND
• One-point remapping of Lagrangian perturbation theory in the mildly non-linear regime of cosmic structure formation
• Baryon history and cosmic star formation in non-Gaussian cosmological models: numerical simulations
• Probing Population III Stars in Galaxy IOK-1 at z = 6.96 through He II Emission
• The solution of the cosmological constant problem from the inhomogeneous equation of state - a hint from modified gravity?
• Cosmic birefringence tomography and calibration-independence with reionization signals in the CMB
• Neutrino Signatures on the High Transmission Regions of the Lyman-alpha Forest
• Needlet Bispectrum Asymmetries in the WMAP 5-year Data
• Characterisation of the non-Gaussianity of radio and IR point-sources at CMB frequencies
• Active Galactic Nucleus Environments and Feedback to Neighboring Galaxies at $z\sim 5$ Probed by Lyman-Alpha Emitters
• A search for concentric circles in the 7-year WMAP temperature sky maps
• Warm Absorber Energetics in Broad Line Radio Galaxies
• Hydrodynamical simulations and semi-analytic models of galaxy formation: two sides of the same coin
• Radio morphology-accretion mode link in FRII low-excitation radio galaxies
• Naturalness of Neutralino Dark Matter
• A new approach to non-commutative inflation
• Detecting and distinguishing topological defects in future data from the CMBPol satellite
• Sources of $H_0$-tensions in dark energy scenarios
• The right-handed sneutrino as thermal dark matter in U(1) extensions of the MSSM
• $CPT$ Violating Electrodynamics and Chern-Simons Modified Gravity
• Numerical calculation of second order perturbations
• Global fits of the Minimal Universal Extra Dimensions scenario
• Parameter dependence of magnetized CMB observables
• Inverse volume corrections from loop quantum gravity and the primordial tensor power spectrum in slow-roll inflation
• Cosmicflows-3: Cold Spot Repeller?
• 3-pt Statistics of Cosmological Stochastic Gravitational Waves
• The Canada-France High-z Quasar Survey: 1.2mm Observations
• Vacuum polarization by a cosmic string in de Sitter spacetime
• Gaugino mass non-universality in an SO(10) supersymmetric Grand Unified Theory: low-energy spectra and collider signals
• Casimir densities for a plate in de Sitter spacetime
• The effect of feedback on the emission properties of the Warm-Hot Intergalactic Medium
• Thermodynamics in Closed Universe with Entropy Corrections
• Tolman IV fluid sphere in f(R, T) gravity
• Analysis of scalar perturbations in cosmological models with a non-local scalar field
• Origin of inflation in CFT driven cosmology: $R^2$-gravity and non-minimally coupled inflaton models
• Do non-relativistic neutrinos constitute the dark matter?
• Probing Dark Energy Dynamics from Current and Future Cosmological Observations
• The BOSS-WiggleZ overlap region II: dependence of cosmic growth on galaxy type
• Transition dynamics in the ${\Lambda }_{\mathrm{s}}$CDM model: Implications for bound cosmic structures
• Compressed sensing reconstruction of a string signal from interferometric observations of the cosmic microwave background
• Dark energy reconstruction based on the PADE approximation; an expansion around the $\Lambda$CDM
• Improving timing sensitivity in the microhertz frequency regime: limits from PSR J1713$+$0747 on gravitational waves produced by super-massive black-hole binaries
• The earliest galaxies seen in 21 cm line absorption
• Optimal constraint on g_NL from CMB
• Quintessential Kination and Thermal Production of Gravitinos and Axinos
• Slow-roll inflation in (R+R*4) gravity
• Cosmological Implications of the Effective Field Theory of Cosmic Acceleration
• Cosmic Microwave Background Acoustic Peak Locations
• Investigation of Dark Matter in Minimal 3-3-1 Models
• High-density Molecular Gas Properties of the Starburst Galaxy NGC 1614 Revealed with ALMA
• Constraining Scalar Singlet Dark Matter with CDMS, XENON and DAMA and Prediction for Direct Detection Rates
• Signatures of clumpy dark matter in the global 21 cm background signal
• Theoretical Aspects of Quintom Models
• Hobby-Eberly Telescope Observations of the Dark Halo in NGC 821
• Baryon Asymmetry of the Universe without Boltzmann or Kadanoff-Baym
• Annealing a Follow-up Program: Improvement of the Dark Energy Figure of Merit for Optical Galaxy Cluster Surveys
• CMB Lensing Constraints on Dark Energy and Modified Gravity Scenarios
• The distribution of Lyman-limit absorption systems during and after reionization
• The initial shear field in models with primordial local non-Gaussianity and implications for halo and void abundances
• Constraining the time variation of the coupling constants from cosmic microwave background: effect of Λ_{QCD}
• Inhomogeneous viscous fluids in FRW universe and finite-future time singularities
• SO(10) Yukawa Unification with mu < 0
• Conformal Transformations and Weak Field Limit of Scalar-Tensor Gravity
• Initial Conditions for Non-Canonical Inflation
• How does non-linear dynamics affect the baryon acoustic oscillation?
• A decade of joint MOJAVE-Fermi AGN monitoring: localisation of the gamma-ray emission region
• Suzaku View of the Swift/Bat Active Galactic Nuclei. IV. Nature of Two Narrow-Line Radio Galaxies (3C 403 and IC 5063)
• Constructing Infrared Finite Propagators in Inflating Space-time
• Domain wall solution in $F(R)$ gravity and variation of the fine structure constant
• The Cosmic V-Web
• Narrowing down the possible explanations of cosmic acceleration with geometric probes
• Update on the Direct Detection of Dark Matter in MSSM Models with Non-Universal Higgs Masses
• Constraining the $\Lambda$CDM and Galileon models with recent cosmological data
• Precision cosmology in muddy waters: Cosmological constraints and N-body codes
• Decoding the bispectrum of single-field inflation
• Exact Extreme Value Statistics and the Halo Mass Function
• The cosmic evolution of massive black holes and galaxy spheroids: global constraints at redshift z<~1.2
• The ISW-tSZ cross correlation: ISW extraction out of pure CMB data
• Weak lensing statistics from the Coyote Universe
• R-parity preserving super-WIMP decays
• Non-universal gaugino and scalar masses, hadronically quiet trileptons and the Large Hadron Collider
• A Meandering Inflaton
• Hybrid Natural Low Scale Inflation
• Quantum Back-Reaction in Scale Invariant Induced Gravity Inflation
• A cosmological context for compact massive galaxies
• A Theory of a Spot
• Super Hilltop Inflation
• The extreme blazar AO 0235+164 as seen by extensive ground and space radio observations
• Approximate Analytic Spectra of Reionized CMB Anisotropies and Polarization generated by Relic Gravitational Waves
• Cosmological Constraints from Moments of the Thermal Sunyaev-Zel'dovich Effect
• No Large Scale Curvature Perturbations during Waterfall of Hybrid Inflation
• Observational Constraints on Dark Energy Models with $\Lambda$ as an Equilibrium Point
• Genesis of Dark Energy: Dark Energy as Consequence of Release and Two-stage Tracking Cosmological Nuclear Energy
• Gravitational waves, dark energy and inflation
• A_4-based neutrino masses with Majoron decaying dark matter
• Inflation of universe due to nonlinear electrodynamics
• The Dearth of Chemically Enriched Warm-Hot Circumgalactic Gas
• The Reconstruction of Constant Jerk Parameter with $f(R,T)$ Gravity
• Evolution of mass and velocity filed in comic web: comparison between baryonic and dark matter
• Analyzing Cosmic Bubble Collisions
• The Topology and Size of the Universe from CMB Temperature and Polarization Data
• Observational constraints on bimetric gravity
• Higgs funnel region of SUSY dark matter for small $\tan \beta$ and renormalization group effects on pseudoscalar Higgs boson with scalar mass non-universality
• The mass-concentration relationship of virialized halos and its impact on cosmological observables
• Cross-correlation Study between the Cosmological 21-cm Signal and the kinetic Sunyaev-Zel'dovich effect
• Bayesian analysis of anisotropic cosmologies: Bianchi VII_h and WMAP
• Detecting relics of a thermal gravitational wave background in the early Universe
• Separable and non-separable multi-field inflation and large non-Gaussianity
• Distribution of streaming rates into high-redshift galaxies
• Spheroidal post-mergers in the local Universe
• Inflationary potentials in DBI models
• Kaehler Potentials for Hilltop F-term Hybrid Inflation
• Observing the Multiverse with Cosmic Wakes
• Evolution of CIV Absorbers I. The Cosmic Incidence
• Slow-roll freezing quintessence
• Scalar tilt from broken conformal invariance
• The response of dark matter haloes to elliptical galaxy formation: a new test for quenching scenarios
• Generalised nonminimally gravity-matter coupled theory
• Sneutrino Inflation with Asymmetric Dark Matter
• Constraints on the pMSSM from LAT Observations of Dwarf Spheroidal Galaxies
• Observational Tests of Gauss-Bonnet Like Dark Energy Model
• First observational constraints on tensor non-Gaussianity sourced by primordial magnetic fields from cosmic microwave background
• The Ysz--Yx Scaling Relation as Determined from Planck and Chandra
• Large scale alignment anomalies of CMB anisotropies: a new test for residuals applied to WMAP 5yr maps
• Constraints on Neutrino Mass and Light Degrees of Freedom in Extended Cosmological Parameter Spaces
• Probing features in inflaton potential and reionization history with future CMB space observations
• The First Decade of Science with Chandra and XMM-Newton
• Breaking the scale invariance of the primordial power spectrum in Horava-Lifshitz Cosmology
• Inflationary universe from higher derivative quantum gravity coupled with scalar electrodynamics
• Dark Energy from Gauss-Bonnet and non-minimal couplings
• A Quasar-Galaxy Mixing Diagram: Quasar Spectral Energy Distribution Shapes in the Optical to Near-Infrared
• Minimal Dark Matter and Leptogenesis
• First experimental constraints on the disformally coupled Galileon model
• The polytropic approximation and X-ray scaling relations: constraints on gas and dark matter profiles for galaxy groups and clusters
• The micro-structure of the intergalactic medium I: the 21cm signature from dynamical minihaloes
• Modelling the Accelerating Universe with $f(Q)$ Gravity: Observational Consistency
• Tri-Bimaximal Neutrino Mixing and the $T_{13}$ Flavor Symmetry
• Nambu-Goldstone Dark Matter and Cosmic Ray Electron and Positron Excess
• The distribution of Omega_k from the scale-factor cutoff measure
• The importance of preventive feedback: inference from observations of the stellar masses and metallicities of Milky Way dwarf galaxies
• Is Dark Energy Dynamical in the DESI Era? A Critical Review
• Detections of Faint Lyman-alpha Emitters at z = 5.7: Galaxy Building Blocks and Engines of Reionization
• Chaotic inflation in F(R) supergravity
• The Cosmic Near Infrared Background III: Fluctuations, Reionization and the Effects of Minimum Mass and Self-regulation
• Self-Calibrated Cluster Counts as a Probe of Primordial Non-Gaussianity
• Energy Conditions in Higher Derivative $f(R,\square R,T)$ Gravity
• The temperature of hot gas halos of early-type galaxies
• Noether symmetric classical and quantum scalar field cosmology
• Distance Measurements from Supernovae and Dark Energy Constraints
• Searches for Supersymmetry at High-Energy Colliders
• Inflationary Scalars Don't Affect Gravitons at One Loop
• Casimir densities for a spherical boundary in de Sitter spacetime
• Will the tachyonic Universe survive the Big Brake?
• Kinematic Cusps With Two Missing Particles I: Antler Decay Topology
• Simulations of BAO reconstruction with a quasar Lyman-alpha survey
• A fitting formula for the non-Gaussian contribution to the lensing power spectrum covariance
• CMB Temperature and Matter Power Spectrum in a Decay Vacuum Dark Energy Model
• A preserved high-z compact progenitor in the heart of NGC3311 revealed with MUSE 2D stellar population analysis
• Reconstruction of the primordial power spectrum from CMB data
• Local gravitational redshifts can bias cosmological measurements
• Revealing Cosmic Rotation
• Through the Looking Glass: Why the "Cosmic Horizon" is not a horizon
• Can we detect Hot or Cold spots in the CMB with Minkowski Functionals?
• Search for primordial non-Gaussianity in the quasars of SDSS-III BOSS DR9
• Model- and calibration-independent test of cosmic acceleration
• Assisted dark energy
• Neutrinos from Kaluza-Klein dark matter in the Sun
• L.R.S. Bianchi type II Stiff Fluid cosmological model with Decaying Vacuum Energy Density $\Lambda$ in general relativity
• Probing the Existence of a Dark Matter Isothermal Core Using Gravity Modes
• Quantum Stress Tensor Fluctuations of a Conformal Field and Inflationary Cosmology
• Hybrid Inflation Revisited in Light of WMAP5
• Neutrino sector impacts SUSY dark matter
• Testing nonstandard cosmological models with SNLS3 supernova data and other cosmological probes
• Tensors, non-Gaussianities, and the future of potential reconstruction
• Perturbations of Matter Fields in the Second-order Gauge-invariant Cosmological Perturbation Theory
• Dark Viscous Fluid coupled with Dark Matter and future singularity
• Southern Cosmology Survey I: Optical Cluster Detections and Predictions for the Southern Common-Area Millimeter-Wave Experiments
• B-mode Detection with an Extended Planck Mission
• Constraining neutrino properties with a Euclid-like galaxy cluster survey
• The Hubble rate in averaged cosmology
• Prospects for Indirect Detection of Sneutrino Dark Matter with IceCube
• Effect of Helium Sedimentation on X-ray Measurements of Galaxy Clusters
• Using Host Galaxy Photometric Redshifts to Improve Cosmological Constraints with Type Ia Supernova in the LSST Era
• Weak-lensing-inferred scaling relations of galaxy clusters in the RCS2: mass-richness, mass-concentration, mass-bias, and more
• Probing the dynamical behavior of dark energy
• Superpotential method for chiral cosmological models connected with modified gravity
• Type II Seesaw Higgs Triplet as the inflaton for Chaotic Inflation and Leptogenesis
• Revival of the Deser-Woodard nonlocal gravity model: Comparison of the original nonlocal form and a localized formulation
• Power spectrum modelling of galaxy and radio intensity maps including observational effects
• Circles-in-the-sky searches and observable cosmic topology in a flat Universe
• Nonlinear cosmological consistency relations and effective matter stresses
• Lensed CMB temperature and polarization maps from the Millennium Simulation
• Electric-magnetic duality and the conditions of inflationary magnetogenesis
• SUSY and Higgs Signatures Implied by Cancellations in $b\to s\gamma$
• Interpreting the Transmission Windows of Distant Quasars
• Subaru Adaptive-optics High-spatial-resolution Infrared K- and L'-band Imaging Search for Deeply Buried Dual AGNs in Merging Galaxies
• The Radio Signatures of the First Supernovae
• The look-elsewhere effect from a unified Bayesian and frequentist perspective
• Cosmological Tests Using the Angular Size of Galaxy Clusters
• Large scale directional anomalies in the WMAP 5yr ILC map
• Solving the main cosmological puzzles with a generalized time varying vacuum energy
• A Cosmological Underdensity Does Not Solve the Hubble Tension
• Light neutralino dark matter in the MSSM and its implication for LHC searches for staus
• Observational Signatures of Gravitational Couplings in DBI Inflation
• Properties of scalar perturbations generated by conformal scalar field
• The Gigaparsec WiggleZ Simulations: Characterising scale dependant bias and associated systematics in growth of structure measurements
• Subtraction of Bright Point Sources from Synthesis Images of the Epoch of Reionization
• Coupling between cold dark matter and dark energy from neutrino mass experiments
• ${\varphi }^4$ inflation is not excluded
• Improving reconstruction of the baryon acoustic peak : the effect of local environment
• High-resolution three-dimensional simulations of gas removal from ultrafaint dwarf galaxies. I. Stellar feedback
• Weak lensing predictions for coupled dark energy cosmologies at non-linear scales
• Some FRW Models of Accelerating Universe with Dark Energy
• Observational constraints on phantom power-law cosmology
• Scale-Dependent Bias of Galaxies from Baryonic Acoustic Oscillations
• Cosmology with Photometric Surveys of Type Ia Supernovae
• A magnified glance into the dark sector: probing cosmological models with strong lensing in A1689
• Non singular bounce in modified gravity
• Cosmic age test in inhomogeneous cosmological models mimicking $\Lambda$CDM on the light cone
• Stochastic gravitational waves from a new type of modified Chaplygin gas
• Constraining power of cosmological observables: blind redshift spots and optimal ranges
• How accurate is it to update the cosmology of your halo catalogues?
• Revisit of constraints on holographic dark energy: SNLS3 dataset with the effects of time-varying $\beta$ and different light-curve fitters
• Relative velocity of dark matter and barions in clusters of galaxies and measurements of their peculiar velocities
• Chemistry of heavy elements in the Dark Ages
• BeyondPlanck I. Global Bayesian analysis of the Planck Low Frequency Instrument data
• Anisotropic String Cosmological Models in Heckmann-Suchuking Space-Time
• Scale invariance vs conformal invariance
• Multi-frequency study of the gamma-ray flaring BL Lac object PKS 2233-148 in 2009-2012
• AstroSat-CZTI detection of variable prompt emission polarization in GRB 171010A
• Non-Gaussianity, Isocurvature Perturbation, Gravitational Waves and a No-Go Theorem for Isocurvaton
• Grand Rip and Grand Bang/Crunch cosmological singularities
• Self-accelerating the normal DGP branch
• Cosmological data analysis of f(R) gravity models
• The Global Star-Formation Law by Supernova Feedback
• The QSO proximity effect at redshift <z>=2.6 with the FLO approach
• Null Energy Condition Violation and Classical Stability in the Bianchi I Metric
• Reionization in the Warm Dark Matter Model
• Could Dark Matter Interactions be an Alternative to Dark Energy ?
• Cosmological evolution, future singularities, Little Rip and Pseudo-Rip in viable f(R) theories and their scalar-tensor counterpart
• Clarifying Forecasts of Dark Energy Constraints from Baryon Acoustic Oscillations
• K2: A new method for the detection of galaxy clusters based on CFHTLS multicolor images
• The Entropic Landscape
• Multifrequency radiation hydrodynamics simulations of H2 line emission in primordial, star-forming clouds
• Anisotropies in the Diffuse Gamma-Ray Background from Dark Matter with Fermi LAT: a closer look
• 125 GeV Higgs Boson from t-b-tau Yukawa Unification
• CMSSM Spectroscopy in light of PAMELA and ATIC
• The evolution of primordial magnetic field since its generation
• The Delay Times of Type Ia Supernova
• A method for testing the cosmic homogeneity with Shannon entropy
• The Deformable Universe
• Optimizing weak lensing mass estimates for cluster profile uncertainty
• VLBI detection of the HST-1 feature in the M87 jet at 2 cm
• Secondary graviton spectra and waterfall-like fields
• Systematics of multi-field effects at the end of warped brane inflation
• On Minkowski Functionals of CMB polarization
• Reconstruction of new holographic scalar field models of dark energy in Brans-Dicke Universe
• Computation of the Halo Mass Function Using Physical Collapse Parameters: Application to Non-Standard Cosmologies
• Observational constraints on Horava-Lifshitz cosmology
• Non-linear weak lensing forecasts
• Generalized Chaplygin gas model: Cosmological consequences and statefinder diagnosis
• Interacting Two-Fluid Viscous Dark Energy Models In Non-Flat Universe
• Inverse see-saw, leptogenesis, observable proton decay and ${\Delta }_{\mathrm{R}}^{\pm \pm }$ in SUSY SO(10) with heavy W_R
• The Effects of Rayleigh Scattering on the CMB and Cosmic Structure
• The clustering of the first galaxy halos
• The WiggleZ Dark Energy Survey: small-scale clustering of Lyman Break Galaxies at z < 1
• A divergence-free parametrization for dynamical dark energy
• Coexistence of a non thermal jet and a complex ultra fast X-ray outflow in a moderately luminous AGN
• Continuous Mid-Infrared Star Formation Rate Indicators: Diagnostics for 0<z<3 Star Forming Galaxies
• The Influence of Galaxy Formation Physics on Weak Lensing Tests of General Relativity
• Nonlinear Spinor Fields in Bianchi type-I spacetime: Problems and Possibilities
• Updated Axion CDM energy density
• On the starting redshift for cosmological simulations: Focusing on halo properties
• Discovery of gamma-ray emission from the Broad Line Radio Galaxy Pictor A
• Constraint on noncommutative spacetime from PLANCK data
• Analysis of non-Gaussian CMB maps based on the N-pdf. Application to WMAP data
• Cosmology of a generalised version of holographic dark energy in presence of bulk viscosity and its inflationary dynamics through slow roll parameters
• F-term Stabilization of Odd Axions in LARGE Volume Scenario
• On the impact of intergalactic dust on cosmology with type Ia supernovae
• Constraining Dark Matter properties with the first generation of stars
• Cosmological Simulations of Dwarf Galaxies with Cosmic Ray Feedback
• Exploring the relation between (sub-)millimeter radiation and gamma-ray emission in blazars with Planck and Fermi
• Hartree Approximation to the One Loop Quantum Gravitational Correction to the Graviton Mode Function on de Sitter
• On the streaming model for redshift-space distortions
• Probing neutralino dark matter in the MSSM & the NMSSM with directional detection
• Dark matter searches at LHC
• Quantum backreaction in evolving FLRW spacetimes
• A Measurement of Primordial Non-Gaussianity Using WMAP 5-Year Temperature Skewness Power Spectrum
• CMB likelihood approximation by a Gaussianized Blackwell-Rao estimator
• Scalar perturbations in conformal rolling scenario with intermediate stage
• A new method to measure galaxy bias
• Observational constraints on decaying vacuum dark energy model
• Global Fits of the Large Volume String Scenario to WMAP5 and Other Indirect Constraints Using Markov Chain Monte Carlo
• The formation of CDM haloes II: collapse time and tides
• Cosmology and thermodynamics of FRW universe with bulk viscous stiff fluid
• SO(10) GUT in Four and Five Dimensions: A Review
• Evidence of non-thermal X-ray emission from radio lobes of Cygnus A
• Baryon Number, Lepton Number, and Operator Dimension in the SMEFT with Flavor Symmetries
• Primordial non-Gaussianity in the bispectra of large-scale structure
• An optical/NIR survey of globular clusters in early-type galaxies. I. Introduction and data reduction procedures
• EWSB from the soft portal into Dark Matter and prediction for direct detection
• New integrable models and analytical solutions in $f(R)$~cosmology with an ideal gas
• A Lyman alpha halo around a quasar at redshift z=6.4
• Cosmology with nonminimal kinetic coupling and a Higgs-like potential
• Constraining AGN triggering mechanisms through the clustering analysis of active black holes
• Sparticle Spectroscopy with Neutralino Dark matter from t-b-tau Quasi-Yukawa Unification
• Dirac Born Infeld (DBI) Cosmic Strings
• Unveiling the nature of the gamma-ray emitting AGN PKS 0521-36
• Minimal Flavor Violation in the Minimal U(1)_{B-L} Model and Resonant Leptogenesis
• Nuclear processes in Astrophysics: Recent progress
• Vacuum energy density kicked by the electroweak crossover
• Two-Fluid Dark Energy Models in Bianchi Type-III Universe with Variable Deceleration Parameter
• Impact of modulation on CMB B-mode polarization experiments
• New Approaches to Probing Minkowski Functionals
• Isolating the Lyman Alpha Forest BAO Anomaly
• Bayesian comparison of nonstandard cosmologies using type Ia supernovae and BAO data
• Anomaly mediated SUSY breaking scenarios in the light of cosmology and in the dark (matter)
• Sterile neutrino dark matter, CDMS-II and a light Higgs boson
• Investigating the accelerated expansion of the Universe through updated constraints on viable $f(R)$ models within the metric formalism
• Model independent constraints on mass-varying neutrino scenarios
• Gamma-ray burst contributions to constraining the evolution of dark energy
• Radiative Corrections to the Neutralino Dark Matter Relic Density - an Effective Coupling Approach
• Uniting cosmological epochs through the twister solution in cosmology with non-minimal coupling
• The Hydra I cluster core. I. Stellar populations in the cD galaxy NGC 3311
• When LEP and Tevatron combined with WMAP and XENON100 shed light on the nature of Dark Matter
• The Atacama Cosmology Telescope: High-Resolution Sunyaev-Zel'dovich Array Observations of ACT SZE-selected Clusters from the Equatorial Strip
• Measuring Unified Dark Matter with 3D Cosmic Shear
• Population III Star Clusters in the Reionized Universe
• Jet Power of Jetted Active Galactic Nuclei: Implication for Evolution and Unification
• The Return of the Phoenix Universe
• Higgs Inflation, Quantum Smearing and the Tensor to Scalar Ratio
• One-loop corrections to the power spectrum in general single-field inflation
• High cadence, linear and circular polarization monitoring of OJ 287 - Helical magnetic field in a bent jet
• A solution of the strong CP problem via the Peccei-Quinn mechanism through the Nieh-Yan modified gravity and cosmological implications
• Exploring the evolution of color-luminosity parameter $\beta$ and its effects on parameter estimation
• Scalar and fermionic vacuum currents in de Sitter spacetime with compact dimensions
• Constraints on Lorentz Invariance and CPT Violation using Optical Photometry and Polarimetry of Active Galaxies BL Lacertae and S5 B0716+714
• Testing flatness of the universe with probes of cosmic distances and growth
• Understanding the origin of CMB constraints on Dark Energy
• Detecting the power spectrum turnover with HI intensity mapping
• DM haloes in the fifth-force cosmology
• Future constraints on neutrino isocurvature perturbations in the curvaton scenario
• On the relevance of chaos for halo stars in the Solar Neighbourhood
• Constraints on Dark Matter Annihilation Cross Section in Scenarios of Brane-World and Quintessence
• Reducing the Spectral Index in Supernatural Inflation
• Inflationary predictions in scalar-tensor DBI inflation
• Does fractal Universe describe a complete cosmic scenario?
• Mass-metallicity relation of dwarf galaxies and its dependency on time: clues from resolved systems and comparison with massive galaxies
• Axions, Inflation and the Anthropic Principle
• Tidal alignments as a contaminant of the galaxy bispectrum
• Galaxy cluster angular size data constraints on dark energy
• Constraints upon the spectral indices of relic gravitational waves by LIGO S5
• Isocurvature Perturbations and Non-Gaussianity of Gravitationally Produced Nonthermal Dark Matter
• The Morphology of the Galactic Dark Matter Synchrotron Emission with Self-Consistent Cosmic Ray Diffusion Models
• Accelerating Dark Energy Cosmological Model in Two Fluid with Hybrid Scale Factor
• Growth of spherical overdensities in scalar-tensor cosmologies
• A comparison of perturbations in fluid and scalar field models of dark energy
• Constraints on cosmological birefringence from Planck and Bicep2/Keck data
• Statistical Properties of Scale-Invariant Helical Magnetic Fields and Applications to Cosmology
• Using the Topology of Large Scale Structure to constrain Dark Energy
• Non-linear relativistic contributions to the cosmological weak-lensing convergence
• Atomic Ionization by keV-scale Pseudoscalar Dark Matter Particles
• Constraints on a decomposed dark fluid with constant adiabatic sound speed by jointing the geometry test and growth rate after Planck data
• Emergent universe scenario and the low CMB multipoles
• Baryogenesis via Leptogenesis in Adjoint SU(5)
• Weak Scale Baryogenesis in a Supersymmetric Scenario with R-parity violation
• Probing modified gravity theories with the Sandage-Loeb test
• The molecular gas properties in local Seyfert 2 galaxies
• Clustering and lifetime of Lyman Alpha Emitters in the Epoch of Reionization
• Smoking guns of a bounce in modified theories of gravity through the spectrum of the gravitational waves
• Modelling the cosmological Lyman-Werner background radiation field in the Early Universe
• Redshifted intergalactic 3He+ 8.7 GHz hyperfine absorption
• GRB 091029: At the limit of the fireball scenario
• Characterization of the distribution of the Llyαemitters in the 53W002 field at z = 2.4
• Quintessence and phantom dark energy from ghost D-branes
• Conformal Gravity: Dark Matter and Dark Energy
• Modified GBIG Scenario as an Alternative for Dark Energy
• On the Suppression of Parametric Resonance and the Viability of Tachyonic Preheating after Multi-Field Inflation
• Hot and cold spots counts as probes of non-Gaussianity in the CMB
• Effects of Velocity-Dependent Dark Matter Annihilation on the Energy Spectrum of the Extragalactic Gamma-ray Background
• Decaying Hidden Gaugino as a Source of PAMELA/ATIC Anomalies
• Bayesian model comparison in cosmology with Population Monte Carlo
• Multi-Field Inflation on the Landscape
• Inflation might be caused by the right
• Physics of the cosmic microwave background anisotropy
• Constraints on the Intracluster Dust Emission in the Coma Cluster of Galaxies
• The Correlation between Black Hole Mass and Stellar Mass for Classical Bulges and the Cores of Ellipticals
• Neutrino Constraints on Inelastic Dark Matter after CDMS II
• Wavelet domain Bayesian denoising of string signal in the cosmic microwave background
• Quantum Coherence of Relic Neutrinos
• Cosmological Consequences of New Dark Energy Models in Einstein-Aether Gravity
• Very Special (de Sitter) Relativity
• Cosmological implications from the full shape of the large-scale power spectrum of the SDSS DR7 luminous red galaxies
• Spherical collapse model and cluster number counts in power law $f(T)$ gravity
• Acceleration of Galactic Supershells by Lyman Alpha Radiation
• The Galactic Center Region Gamma Ray Excess from A Supersymmetric Leptophilic Higgs Model
• Searching for non-Gaussianity in the WMAP data
• Horava-Lifshitz cosmology with generalized Chaplygin gas
• Modeling the Ages and Metallicities of Early-Type Galaxies in Fundamental Plane Space
• The Effects of Halo-to-Halo Variation on Substructure Lensing
• Changes in the halo formation rates due to features in the primordial spectrum
• Modified Gravity: the CMB, Weak Lensing and General Parameterisations
• On Primordial Density Perturbation and Decaying Speed of Sound
• The impact of spatial fluctuations in the ultra-violet background on intergalactic carbon and silicon
• Studying the Warm-Hot Intergalactic Medium in Emission
• Cosmology with Standard Sirens: the Importance of the Shape of the Lensing Magnification Distribution
• Cosmic variance in the nanohertz gravitational wave background
• A Robust Distance Measurement and Dark Energy Constraints from the Spherically-Averaged Correlation Function of Sloan Digital Sky Survey Luminous Red Galaxies
• Friedmann cosmology with decaying vacuum density in Brans-Dicke theory
• First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Effects of Chromatic Corrections to Supernova Photometry on Measurements of Cosmological Parameters
• Parameterizing scalar-tensor theories for cosmological probes
• Dark Radiation and Decaying Matter
• The statistics of voids as a tool to constrain cosmological parameters: sigma_8 and Omega_m h
• Neutralino Dark Matter in BMSSM Effective Theory
• Do cosmological data rule out $f(\mathcal{R})$ with $w\ne -1$?
• Quintessential power-law cosmology: dark energy equation of state
• Limits on decaying dark energy density models from the CMB temperature-redshift relation
• New cosmological constraints with extended-Baryon Oscillation Spectroscopic Survey DR14 quasar sample
• syren-halofit: A fast, interpretable, high-precision formula for the $\Lambda$CDM nonlinear matter power spectrum
• Quantum Gravity inspired nonlocal gravity model
• Helium Sedimentation and the UV Upturn in Brightest Cluster Galaxies
• Active Galactic Nuclei: Sources for ultra high energy cosmic rays?
• Scale-dependent power spectrum from initial excited-de Sitter modes
• Non-Gaussianity from Self-Ordering Scalar Fields
• Influence of Projection in Cluster Cosmology Studies
• Observing the circumgalactic medium of simulated galaxies through synthetic absorption spectra
• Physical parameters of active galactic nuclei derived from properties of jet geometry transition region
• Statistical coverage for supersymmetric parameter estimation: a case study with direct detection of dark matter
• Crossing of Phantom Divide in $F(R)$ Gravity
• What Are S0 Galaxies?
• Levitating Dark Matter
• Lyman-α Emitters in the context of hierarchical galaxy formation: predictions for VLT/MUSE surveys
• Renormalization group evolution of neutrino masses and mixing in seesaw models: A review
• The Impact of Nonlinear Structure Formation on the Power Spectrum of Transverse Momentum Fluctuations and the Kinetic Sunyaev-Zel'dovich Effect
• Probing the Cosmic X-ray and MeV Gamma-ray Background Radiation through the Anisotropy
• Extrapolating the Evolution of Galaxy Sizes to the Epoch of Reionization
• Tribimaximal mixing in neutrino mass matrices with texture zeros or vanishing minors
• Turbulence in the Inter-galactic Medium: Solenoidal and Dilatational Motions, and the Impact of Numerical Viscosity
• Increasing the Fisher Information Content in the Matter Power Spectrum by Non-linear Wavelet Weiner Filtering
• A large scale coherent magnetic field: interactions with free streaming particles and limits from the CMB
• Dynamical system analysis for DBI dark energy interacting with dark matter
• Panglossian Prospects for Detecting Neutralino Dark Matter in Light of Natural Priors
• CP Violation in the SUSY Seesaw: Leptogenesis and Low Energy
• Gravitational Wave Constraints on Multi-Brane Inflation
• A new model for the full shape of the large-scale power spectrum
• Galaxy-Mass Correlations on 10 Mpc Scales in the Deep Lens Survey
• Observational constraints on supermassive dark stars
• A conventional approach to the dark-energy concept
• High-redshift blazars through nustar eyes
• Constraining SUSY with Heavy Scalars -- using the CMB
• Constraints on the High-l Power Spectrum of Millimeter-wave Anisotropies from APEX-SZ
• Quantum Gravity and Inflation
• Dark Energy: The Shadowy Reflection of Dark Matter?
• Cosmology with the largest galaxy cluster surveys: Going beyond Fisher matrix forecasts
• Non-Gaussianity from Axion Monodromy Inflation
• Statistical Analysis of future Neutrino Mass Experiments including Neutrino-less Double Beta Decay
• The WiggleZ Dark Energy Survey: Probing the Epoch of Radiation Domination using Large Scale Structure
• The detection of sub-solar mass dark matter halos
• Evidence for Merger-Driven Activity in the Clustering of High Redshift Quasars
• Intrinsic uncertainty on the nature of dark energy
• LHC-7 supersymmetry search interpretation within the pMSSM
• Optimizing future experimental probes of inflation
• Comparison of Frames: Jordan vs Einstein Frame for a Non-minimal Dark Energy Model
• Effects of Linear Redshift Space Distortions and Perturbation Theory on BAOs: A 3D Spherical Analysis
• ALMA Multiple-Transition Molecular Line Observations of the Ultraluminous Infrared Galaxy IRAS 20551-4250: Different HCN, HCO+, HNC Excitation and Implications for Infrared Radiative Pumping
• Testing cosmic acceleration for $w(z)$ parameterizations using $f_{gas}$ measurements in galaxy clusters
• Cosmological Problems with Multiple Axion-like Fields
• A dark matter model that reconciles tensions between the cosmic-ray $e^{\pm }$ excess and the gamma-ray and CMB constraints
• Probing bulk viscous matter-dominated models with Gamma-ray bursts
• Anisotropic f(Q) gravity model with bulk viscosity
• Testing the equal-time angular-averaged consistency relation of the gravitational dynamics in N-body simulations
• General relativistic effects on non-linear power spectra
• Spectral Index in Curvaton Scenario
• Cosmic Polarization Rotation: an Astrophysical Test of Fundamental Physics
• Constraining dark matter halo profiles and galaxy formation models using spiral arm morphology. II. Dark and stellar mass concentrations for 13 nearby face-on galaxies
• Imprints of primordial non-Gaussianities in X-ray and SZ signals from galaxy clusters
• Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model - I. Magnitude counts, redshift distribution, colour bimodality, and galaxy clustering
• A numerical study of the effects of primordial non-Gaussianities on weak lensing statistics
• Preheating in Dirac-Born-Infeld inflation
• Probing large-scale magnetism with the Cosmic Microwave Background
• A Search for Oxygen in the Low-Density Lyman-alpha Forest Using the Sloan Digital Sky Survey
• Invisible Higgs decay with B\to Kν\barν constraint
• Generation of Curvature Perturbations with Extra Anisotropic Stress
• Unparticle dark energy
• Neutralino reconstruction in supersymmetry with long-lived staus
• Negative vacuum energy densities and the causal diamond measure
• The Relativistic Jet Orientation and Host Galaxy of the Peculiar Blazar PKS 1413+135
• Evidence for the Fifth Element Astrophysical status of Dark Energy
• Impact of bias and redshift-space modelling for the halo power spectrum: Testing the effective field theory of large-scale structure
• Efficiency of Thermal Conduction in a Magnetised Circumgalactic Medium
• Consistency Relation for multifield inflation scenario with all loop contributions
• Stable Charged Radiating Systems Associated with Tilted Observers
• Noether Symmetries of Some Homogeneous Universe Models in Curvature Corrected Scalar-Tensor Gravity
• Crossing the phantom divide line as an effect of quantum transitions
• SUSY Renormalization Group Effects in Ultra High Energy Neutrinos
• Regulating the infrared by mode matching: A massless scalar in expanding spaces with constant deceleration
• Radiative Feedback in Relic HII Regions at High-Redshift
• Star Formation in the Multiverse
• Submillimeter sources behind the massive lensing clusters A370 and A2390
• On the growth of perturbations in interacting dark energy and dark matter fluids
• k-essence in the DGP brane-world cosmology
• Gravitino cosmology in supersymmetric warm inflation
• Statefinder diagnosis for the extended holographic Ricci dark energy model without and with interaction
• Observational signatures of a non-singular bouncing cosmology
• SDSS J092712.64+294344.0: recoiling black hole or merging galaxies?
• Thermodynamics of Spinor Quintom
• Large-Scale Magnetic Fields, Dark Energy and QCD
• Inhomogeneity-induced variance of cosmological parameters
• Viscous Coupled Fluids in Inflationary Cosmology
• Non-gaussianity in the foreground-reduced CMB maps
• Cardassian Universe Constrained by Latest Observations
• Deep learning approach for identification of HII regions during reionization in 21-cm observations -- II. foreground contamination
• Statistical hierarchy of varying speed of light cosmologies
• Running vacuum in Brans-Dicke theory: a possible cure for the ${\sigma }_8$ and $H_0$ tensions
• Fine-tuning challenges for the matter bounce scenario
• The jet collimation profile at high resolution in BL Lacertae
• Not a Copernican observer: biased peculiar velocity statistics in the local Universe
• Secluded Dark Matter Coupled to a Hidden CFT
• Cosmological dynamics of interacting dark energy and dark matter in viable models of f(R) gravity
• CMB polarimetry with BICEP: instrument characterization, calibration, and performance
• Why have supersymmetric particles not been observed?
• Constraints on Primordial non-Gaussianity from Future HI Intensity Mapping Experiments
• Curvature perturbation and waterfall dynamics in hybrid inflation
• Cosmological properties of a generic (\cal R)^2-supergravity
• Galaxy Peculiar Velocities From Large-Scale Supernova Surveys as a Dark Energy Probe
• Universal Merger Histories of Dark-Matter Haloes
• Weak Gravitational Lensing as a Method to Constrain Unstable Dark Matter
• Precise Measurement of the Radial Baryon Acoustic Oscillation Scales in Galaxy Redshift Surveys
• Suzaku View of the Swift/BAT Active Galactic Nuclei. V. Torus Structure of Two Luminous Radio-loud AGNs (3C 206 and PKS 0707-35)
• Consistency of LCDM with Geometric and Dynamical Probes
• Non-Gaussianity of secondary anisotropies from ACTPol and Planck
• Cross-correlation of the HI 21-cm Signal and Lyman-alpha Forest: A Probe Of Cosmology
• The unification of inflation and late-time acceleration in the frame of $k$-essence
• Constraints on neutrino masses from WMAP5 and BBN in the lepton asymmetric universe
• The trispectrum in ghost inflation
• Observational constraints on the oscillating dark energy cosmologies
• Isocurvature modes and Baryon Acoustic Oscillations II: gains from combining CMB and Large Scale Structure
• An Analysis Framework for Understanding the Origin of Nuclear Activity in Low-Power Radio Galaxies
• Cosmological CPT Violation and CMB Polarization Measurements
• String Necklaces and Primordial Black Holes from Type IIB Strings
• Multicomponent multiscatter capture of Dark Matter
• Seeing through the String Landscape - a String Hunter's Companion in Particle Physics and Cosmology
• Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity
• Constraints on the neutrino mass and the primordial magnetic field from the matter density fluctuation parameter ${\sigma }_8$
• Constraints on the Redshift Evolution of the L_X-SFR Relation from the Cosmic X-Ray Backgrounds
• On the full Boltzmann equations for Leptogenesis
• Cosmological Constraints on Strongly Coupled Moduli from Cosmic Strings
• Higher neutrino mass allowed if Cold Dark Matter and Dark Energy are coupled
• What do cluster counts really tell us about the Universe?
• Covariance in the Thermal SZ-Weak Lensing Mass Scaling Relation of Galaxy Clusters
• Higher-Order Gauss-Bonnet Cosmology
• Weak lensing reconstruction through cosmic magnification I: a minimal variance map reconstruction
• Cosmic Polarization Rotation, Cosmological Models, and the Detectability of Primordial Gravitational Waves
• Non-universal scalar mass scenario with Higgs funnel region of SUSY dark matter: a signal-based analysis for the Large Hadron Collider
• On Cross-correlations between Curvature and Isocurvature Perturbations during Inflation
• A 3% Determination of $H_0$ at Intermediate Redshifts
• Testing CPT Symmetry with Current and Future CMB Measurements
• Forecasts on the contamination induced by unresolved point sources in primordial non-Gaussianity beyond Planck
• Numerical evaluation of the three-point scalar-tensor cross-correlations and the tensor bi-spectrum
• Generation of large-scale magnetic fields from inflation in teleparallelism
• Testing Oscillating Primordial Spectrum and Oscillating Dark Energy with Astronomical Observations
• Testing the interaction model with cosmological data and gamma-ray bursts
• Comparing galactic satellite properties in hydrodynamical and Nbody simulations
• CFHTLenS: A Gaussian likelihood is a sufficient approximation for a cosmological analysis of third-order cosmic shear statistics
• BOOMERanG Constraints on Primordial Non-Gaussianity from Analytical Minkowski Functionals
• Neutrino mass from cosmology: Impact of high-accuracy measurement of the Hubble constant
• Cosmological constraints from Radial Baryon Acoustic Oscillation measurements and Observational Hubble data
• Sources of contamination to weak lensing tomography: redshift-dependent shear measurement bias
• A New Chemical Evolution Model for Dwarf Spheroidal Galaxies based on Observed Long Star Formation Histories
• Corrected holographic dark energy with power-law entropy and Hubble Horizon cut-off in FRW Universe
• CoGeNT, DAMA, and Neutralino Dark Matter in the Next-To-Minimal Supersymmetric Standard Model
• How to detect gravitational waves through the cross-correlation of the galaxy distribution with the CMB polarization
• AGN X-ray luminosity function and absorption function in the Early Universe ($3\le z\le 6$)
• Dynamical Effect of the Turbulence of IGM on the Baryon Fraction Distribution
• Measuring Planck beams with planets
• Revisiting the Amati and Yonetoku Correlations with Swift GRBs
• The disappearance of Lyman alpha blobs: a GALEX search at z=0.8
• Analysis of Spitzer-IRS spectra of hyperluminous infrared galaxies
• Clustering of star-forming galaxies detected in mid-infrared with the Spitzer wide-area survey
• A dynamical system representation of generalized Rastall gravity
• Density Fluctuations in Thermal Inflation and Non-Gaussianity
• Non-minimal kinetic coupling and Chaplygin gas cosmology
• Ultra-compact structure in radio quasars as a cosmological probe: a revised study of the interaction between cosmic dark sectors
• The growth of matter perturbations in the f(T) gravity
• A Multi-Wavelength Mass Analysis of RCS2 J232727.6-020437, a ~3x10${}^{15}$M${}_{\odot }$ Galaxy Cluster at z=0.7
• Non-Gaussianity in WMAP Data Due to the Correlation of CMB Lensing Potential with Secondary Anisotropies
• Dark matter in minimal supergravity with type-II seesaw
• Searching for hidden mirror symmetries in CMB fluctuations from WMAP 7 year maps
• Cosmological evolution of warm dark matter fluctuations I: Efficient computational framework with Volterra integral equations
• Viscous Fluids and Gauss-Bonnet Modified Gravity
• Diffuse gamma-ray background and cosmic-ray positrons from annihilating dark matter
• Positronium oscillations to Mirror World revisited
• Time and distance constraints on accelerating cosmological models
• Consistency Test of Dark Energy Models
• Anatomy of bispectra in general single-field inflation -- modal expansions
• Local non-Gaussianity in the Cosmic Microwave Background the Bayesian way
• Cosmological acceleration
• Enhanced Inflation in the Dirac-Born-Infeld framework
• Bianchi type II models in the presence of perfect fluid and anisotropic dark energy
• A 83Krm Source for Use in Low-background Liquid Xenon Time Projection Chambers
• Dark Matter Constraints from a Cosmic Index of Refraction
• The Inflationary Wavefunction and its Initial Conditions
• Semi-analytic galaxy formation in early dark energy cosmologies
• Thick Brane Isotropization in a Generalized 5D Anisotropic Standing Wave Braneworld Model
• Study of gravitational fields and globular cluster systems of early-type galaxies
• Fitting oscillating string gas cosmology to supernova data
• How Flat is Our Universe Really?
• Testing General Relativity with LISA including Spin Precession and Higher Harmonics in the Waveform
• Cold accretion in early galaxy formation and its Lyman-alpha signatures
• A longitudinal gauge degree of freedom and the Pais Uhlenbeck field
• Subaru FOCAS Spectroscopic Observations of High-Redshift Supernovae
• Dark Energy Survey Year 3 results: imprints of cosmic voids and superclusters in the Planck CMB lensing map
• Properties and uncertainties of scalar field models of dark energy with barotropic equation of state
• Suzaku Observation of the Brightest Broad-Line Radio Galaxy 4C 50.55 (IGR J 21247+5058)
• Constraints on general primordial non-Gaussianity using wavelets for the Wilkinson Microwave anisotropy probe 7-year data
• New Constraints on Anisotropic Rotation of CMB Polarization
• Angular dependence of primordial trispectra and CMB spectral distortions
• Cosmological evolution of equation of state for dark energy in G-essence models
• Using Big Bang Nucleosynthesis to Extend CMB Probes of Neutrino Physics
• Potentially Large One-loop Corrections to WIMP Annihilation
• Two radiative inverse seesaw models, dark matter, and baryogenesis
• Doubly imaged quasar SDSS J1515+1511: time delay and lensing galaxies
• Anisotropic power-law inflation in a two-scalar-field model with a mixed kinetic term
• Does accelerating universe indicates Brans-Dicke theory
• Detectability of large-scale power suppression in the galaxy distribution
• Filaments and sheets of the warm-hot intergalactic medium
• Removing BAO-peak Shifts with Local Density Transforms
• Tomography from the Next Generation of Cosmic Shear Experiments for Viable f(R) Models
• Effects of Baryon Mass Loss on Profiles of Large Galactic Dark Matter Haloes
• Tension between SN and BAO: current status and future forecasts
• Reconstructing f(R) Gravity from a Chaplygin Scalar Field in de Sitter Spacetimes
• Host Galaxy Spectra and Consequences for SN Typing From The SDSS SN Survey
• Minimal cut-off vacuum state constraints from CMB bispectrum statistics
• The First Billion Years project: dark matter haloes going from contraction to expansion and back again
• A Glimpse at Quasar Host Galaxy Far-UV Emission, Using DLAs as Natural Coronagraphs
• Dynamical System Analysis for a phantom model
• Modelling Baryonic Effects on Galaxy Cluster Mass Profiles
• Local non-Gaussianity from rapidly varying sound speeds
• CMB constraints on running non-Gaussianity
• Reconstructing cosmic acceleration from modified and non-minimal gravity: The Yang-Mills case
• Primordial Nucleosynthesis: The Predicted and Observed Abundances and Their Consequences
• Population statistics of beamed sources. I: A new model for blazars
• Generalized Swiss-cheese cosmologies: Mass scales
• Effect of asphericity in caustic mass estimates of galaxy clusters
• The Parkes Galactic Meridian Survey (PGMS): observations and CMB polarization foreground analysis
• Standard Coupling Unification in SO(10), Hybrid Seesaw Neutrino Mass and Leptogenesis, Dark Matter, and Proton Lifetime Predictions
• Gauge-Higgs Dark Matter
• Cosmological Einstein-Maxwell model with $g$-essence
• Inhomogeneous viscous fluids for inflation
• The Cosmic Neutrino Background Anisotropy - Linear Theory
• Implications of the latest XENON100 and cosmic ray antiproton data for isospin violating dark matter
• The XMM-Newton deep survey in the CDF-S VI. Obscured AGN selected as infrared power-law galaxies
• Long-Term Multiwavelength Studies of High-Redshift Blazar 0836+710
• Inflation with multiple vector fields and non-Gaussianities
• No-boundary measure and preference for large e-foldings in multi-field inflation
• Star formation trends in high-redshift galaxy surveys: the elephant or the tail?
• Dark Matter Response to Galaxy Assembly History
• Signatures of Pseudoscalar Photon Mixing in CMB Radiation
• A study of phantom scalar field cosmology using Lie and Noether symmetries
• A study of simulated histories of reionization with merger trees of HII regions
• The effect of asymmetric beams in the Wilkinson Microwave Anisotropy Probe experiment
• Elementary Theorems Regarding Blue Isocurvature Perturbations
• Improvement of energy-momentum tensor and non-Gaussianities in holographic cosmology
• Spherical collapse model in agegraphic dark energy cosmologies
• Group Averaging of massless scalar fields in 1+1 de Sitter
• The degenerate gravitino scenario
• Local Features with Large Spiky non-Gaussianities during Inflation
• Confronting Tracker Field Quintessence with Data
• Nonlinearities in modified gravity cosmology I: signatures of modified gravity in the nonlinear matter power spectrum
• High-frequency very long baseline interferometry studies of NRAO 530
• Primordial Trispectrum from Isocurvature Fluctuations
• Primordial Spikes from Wrapped Brane Inflation
• Probing Reionization with Quasar Spectra: the Impact of the Intrinsic Lyman-alpha Emission Line Shape Uncertainty
• Ergodicity and Gaussianity for Spherical Random Fields
• Dynamics of Dirac-Born-Infeld dark energy interacting with dark matter
• Topology beyond the horizon: how far can it be probed?
• Cosmic Neutrino Last Scattering Surface
• Mock galaxy redshift catalogues from simulations: implications for Pan-STARRS1
• Ghosts in asymmetric brane gravity and the decoupled stealth limit
• Constraints on the Generalized Chaplygin Gas Model from Gamma-Ray Bursts
• Matter Distribution around Galaxies
• On a possible compensation of the QCD vacuum contribution to the Dark Energy
• Lensing reconstruction of cluster-mass cross-correlation with cosmic microwave background polarization
• The Contribution of Supernovae to Cosmic Reionization
• Evolution of the curvature perturbation during and after multi-field inflation
• Probing the nature of cosmic acceleration
• Observational constraints of the gravitational waves in the Brans-Dicke theory: Einstein frame and Jordan-Brans-Dicke frame
• Non-thermal Gravitino Dark Matter in Gauge Mediation
• Noether symmetries and duality transformations in cosmology
• Exploring the Role of Axions and Other WISPs in the Dark Universe
• Effects of the size of cosmological N-Body simulations on physical quantities - III: Skewness
• Combining cosmological and local bounds on bimetric theory
• Dark Matter - Dark Energy coupling biasing parameter estimates from CMB data
• Supersymmetric mass spectra for gravitino dark matter with a high reheating temperature
• Evidence for horizon-scale power from CMB polarization
• Anisotropic bulk viscous string cosmological models of the Universe under a time-dependent deceleration parameter
• Constraints from the CMB temperature and other common observational data-sets on variable dark energy density models
• Constraints on dark energy models from radial baryon acoustic scale measurements
• A population of Type Ibc supernovae with massive progenitors; broad lightcurves not uncommon in (i)PTF
• Spectroscopic Confirmation of a z=2.79 Multiply Imaged Luminous Infrared Galaxy Behind the Bullet Cluster
• Symmetry and anti-symmetry of the CMB anisotropy pattern
• Relation between standard perturbation theory and regularized multi-point propagator method
• New Primordial-Magnetic-Field Limit from The Latest LIGO S5 data
• Causality and Primordial Tensor Modes
• Fruitbat: A Python Package for Estimating Redshifts of Fast Radio Bursts
• Constraints from neutrino masses and muon (g-2) in the bilinear R-parity violating supersymmetric model
• Effect of the Metallicity on the X-ray Emission from the Warm-Hot Intergalactic Medium
• DeepSZ: Identification of Sunyaev-Zel'dovich Galaxy Clusters using Deep Learning
• Dominant Multipoles in WMAP5 Mosaic Data Correlation Maps
• The complexity that the first stars brought to the Universe: Fragility of metal enriched gas in a radiation field
• Inflation with racetrack superpotential and matter field
• Primordial curvature perturbation during and at the end of multi-field inflation
• An efficient probe of the cosmological CPT violation
• Rotating a Curvaton Brane in a Warped Throat
• The Probability Distribution for Non-Gaussianity Estimators
• Implications of the lens redshift distribution of strong lensing systems: cosmological parameters and the global properties of early-type galaxies
• De Broglie-Bohm Prediction of Quantum Violations for Cosmological Super-Hubble Modes
• G.A.S. II: Dust extinction in galaxies; Luminosity functions and InfraRed eXcess
• Extension of a radiative neutrino mass model based on a cosmological view point
• The impact of XENON100 and the LHC on Supersymmetric Dark Matter
• Late time cosmological scenarios from scalar field with Gauss Bonnet and non-minimal kinetic couplings
• Cosmological constraints on the generalized holographic dark energy
• Nonlocal Inflation
• Forecast for the Planck precision on the tensor to scalar ratio and other cosmological parameters
• Primordial Black Hole as a Source of the Boost Factor
• Cosmology in One Dimension: Fractal Geometry, Power Spectra and Correlation
• Discrimination between Lambda-CDM, quintessence, and modified gravity models using wide area surveys
• New method to constrain the relativistic free-streaming gas in the Universe
• ATAT: Astronomical Transformer for time series And Tabular data
• Tilt and Running of Cosmological Observables in Generalized Single-Field Inflation
• Constraints on Circumnuclear Disk through Free-Free Absorption in the Nucleus of 3C 84 with KaVA and KVN at 43 and 86 GHz
• Primordial Features as Evidence for Inflation
• Fields Annihilation and Particles Creation in DBI inflation
• Applying scale-free mass estimators to the Local Group in Constrained Local Universe Simulations
• Extended Cosmology in Palatini f(R)-theories
• Utilizing Type Ia Supernovae in a Large, Fast, Imaging Survey to Constrain Dark Energy
• First simultaneous optical/near-infrared imaging of an X-ray selected, high-redshift cluster of galaxies with GROND: the galaxy population of XMMU J0338.7+0030 at z=1.1
• Constraints from the decay B_s -> mu mu and LHC limits on Supersymmetry
• Evolution of the baryon fraction in the Local Group: accretion versus feedback at low and high z
• Using Lagrangian perturbation theory for precision cosmology
• Unmodified Gravity
• Kahler moduli double inflation
• Constant surface gravity and density profile of dark matter
• Can particle creation phenomena replace dark energy?
• $f(\varphi )R$-models for inflation
• Reconciling low multipole anomalies and reheating in single field inflationary models
• Relic gravitational waves in the light of 7-year Wilkinson Microwave Anisotropy Probe data and improved prospects for the Planck mission
• Extremely-Metal Poor Stars in the Milky Way: A Second Generation Formed after Reionization
• Inflation with improved D3-brane potential and the fine tunings associated with the model
• Loop Corrections to Cosmological Perturbations in Multi-field Inflationary Models
• Simulating X-ray Supercavities and Their Impact on Galaxy Clusters
• Barrow Holographic Dark Energy Model with GO Cut-off -- An Alternative Perspective
• Constraining the interacting dark energy models from weak gravity conjecture and recent observations
• Low-Scale Gauge Mediation and Composite Messenger Dark Matter
• The Thermal Abundance of Semi-Relativistic Relics
• Scalar perturbations in p-nflation: the 3-form case
• Lensing Bias to CMB Measurements of Compensated Isocurvature Perturbations
• Reconstructing Cosmological Matter Perturbations using Standard Candles and Rulers
• The nonlinear evolution of baryonic overdensities in the early universe: Initial conditions of numerical simulations
• Scalar cosmological perturbations from inflationary black holes
• Cosmological implications of conformal field theory
• The Cosmological Constant in the Quantum Multiverse
• Modification of the 21-cm power spectrum by X-rays during the epoch of reionisation
• Leptogenesis from Additional Higgs Doublets
• B polarization of cosmic background radiation from second-order scattering sources
• Observational Constraints on Modified Chaplygin Gas in Horava-Lifshitz Gravity
• Observational constraints on dark energy cosmological model parameters
• Dark energy from dark radiation in strongly coupled cosmologies with no fine tuning
• Stable indications of relic gravitational waves in Wilkinson Microwave Anisotropy Probe data and forecasts for the Planck mission
• A correlation between the highest energy cosmic rays and nearby active galactic nuclei detected by Fermi
• CMB component separation in the pixel domain
• A case study of hurdle and generalized additive models in astronomy: the escape of ionizing radiation
• The role of curvature in the slowing down acceleration scenario
• Perfect fluid and F(T) gravity descriptions of inflationary universe and comparison with obervational data
• Cosmological Impact of Population III Binaries
• Where to look for natural supersymmetry
• The Race Between Stars and Quasars in Reionizing Cosmic Hydrogen
• Circular dichroism, magnetic knots and the spectropolarimetry of the Cosmic Microwave Background
• Maximum Entropy deconvolution of Primordial Power Spectrum
• f(T) cosmology against the cosmographic method: A new study using mock and observational data
• Properties of scalar wave emission in a scalar-tensor theory with kinetic screening
• General CMB bispectrum analysis using wavelets and separable modes
• Overall observational constraints on the running parameter λof Horava-Lifshitz gravity
• Leptogenesis, Z' bosons, and the reheating temperature of the Universe
• Non-Gaussianity in three fluid curvaton model
• Virial halo mass function in the $Planck$ cosmology
• Study of the Spectrum of Inflaton Perturbations
• Time-Varying Dark Energy Constraints From the Latest SN Ia, BAO and SGL
• The frequency of very young galaxies in the local Universe: I. A test for galaxy formation and cosmological models
• Wavelet analysis of baryon acoustic structures in the galaxy distribution
• Cosmological evolution of thermal relic particles in $f(R)$ gravity
• Quantum Fields on Noncommutative Spacetimes: Theory and Phenomenology
• Strong lensing in the MareNostrum Universe II: scaling relations and optical depths
• Type Ia supernova parameter estimation: a comparison of two approaches using current datasets
• Multi-wavelength Searches for Particle Dark Matter
• An HI intensity mapping survey with a Phased Array Feed
• Constraints on Dark Energy Parameters from Correlations of CMB with LSS
• Supersymmetric Higgses beyond the MSSM: An update with flavour and Dark Matter constraints
• Neutrino Dispersion Relations from a Dark Energy Model
• Constraining Delay Time Distribution of Binary Neutron Star Mergers from Host Galaxy Properties
• On the operation of the chemothermal instability in primordial star-forming clouds
• Forecasting neutrino masses from galaxy clustering in the Dark Energy Survey combined with the Planck Measurements
• Sharp inflaton potentials and bi-spectra: Effects of smoothening the discontinuity
• Building a Better Understanding of the High Redshift BOSS Galaxies as Tools for Cosmology
• Radio Supernovae in the Great Survey Era
• Dark Stars: A New Study of the FIrst Stars in the Universe
• Roles of Modified Chaplygin-Jacobi and Chaplygin-Abel Gases in FRW Universe
• Effect of model-dependent covariance matrix for studying Baryon Acoustic Oscillations
• Inhomogeneous viscous fluids in FRW universe
• VERA monitoring of the radio jet 3C 84 during 2007--2013: detection of non-linear motion
• Direct and Indirect Detection and LHC Signals of Bino-Higgsino Dark Matter
• Two fossil groups of galaxies at z~0.4 in the COSMOS: accelerated stellar-mass build-up, different progenitors
• Non-Canonical Inflation in Supergravity
• X-ray Cluster Cosmology
• Constraints on moduli cosmology from the production of dark matter and baryon isocurvature fluctuations
• Calibration of a star formation and feedback model for cosmological simulations with Enzo
• Detecting Baryon Acoustic Oscillations
• Influences of Dark Energy and dark matter on Gravitational Time Advancement
• Ultra-faint dwarf galaxies as a test of early enrichment and metallicity-dependent star formation
• Application of Bayesian model averaging to measurements of the primordial power spectrum
• Constraining Light Gravitino Mass from Cosmic Microwave Background
• Energy transfer from baryons to dark matter as a unified solution to small-scale structure issues of the $\Lambda$CDM model
• Non-Universal Gaugino Masses, CDMS, and the LHC
• The active and passive populations of Extremely Red Objects
• Low-Metallicity Star Formation in High-Redshift Galaxies at z~8
• Cosmic Ray Spectra in Nambu-Goldstone Dark Matter Models
• Fair scans of the seesaw. Consequences for predictions on LFV processes
• Equation of State of Neutron Stars with Junction Conditions in the Starobinsky Model
• Cosmological Constraints on the Higgs Boson Mass
• Can we explain cosmic birefringence without a new light field beyond Standard Model?
• The nonlinear probability distribution function in models with local primordial non-Gaussianity
• Environmentally Selected WIMP Dark Matter with High-Scale Supersymmetry Breaking
• Probing the light Higgs pole resonance annihilation of dark matter in the light of XENON100 and CDMS-II observations
• $\Lambda$CDM-type cosmological model and observational constraints
• Weak lensing reconstruction through cosmic magnification. II. Improved power spectrum determination and map-making
• The NMSSM with F-theory unified boundary conditions
• Evolution of Anisotropies in Eddington-Born-Infeld Cosmology
• How Delicate is Brane-Antibrane Inflation?
• Topology of Luminous Red Galaxies from the Sloan Digital Sky Survey
• Statefinder Parameters for Different Dark Energy Models with Variable G Correction in Kaluza-Klein Cosmology
• Constraints on Supersymmetry from Relic Density compared with future Higgs Searches at the LHC
• Non-Gaussianity as a signature of thermal initial condition of inflation
• Sunyaev-Zel'dovich observations of galaxy clusters out to the virial radius with the Arcminute Microkelvin Imager
• The anatomy of the NGC 5044 group -- II. Stellar populations and star-formation histories
• Systematic Effects on the Genus Topology of Large Scale Structure of the Universe
• Selection constraints on high redshift quasar searches in the VISTA kilo-degree infrared galaxy survey
• CMB polarization as a probe of the anomalous nature of the Cold Spot
• Improved cosmological constraints on the curvature and equation of state of dark energy
• Can we really measure fnl from the galaxy power spectrum?
• Possible dark energy imprints in gravitational wave spectrum of mixed neutron-dark-energy stars
• DGP and DGPish cosmologies from $f(Q)$ actions
• Cosmic polarimetry in magnetoactive plasmas
• Dynamics and Constraints of the Massive Gravitons Dark Matter Flat Cosmologies
• Dark Matter from the Inflaton Field
• Autocorrelations of stellar light and mass at z~0 and ~1: From SDSS to DEEP2
• Kaluza-Klein Cosmology with Varying G and $\Lambda$
• A new class of holographic dark energy models in LRS Bianchi Type-I
• Dynamics and constraints of the dissipative Liouville cosmology
• Evolution of perturbations in distinct classes of canonical scalar field models of dark energy
• Sourcing curvature modes with entropy perturbations in non-singular bouncing cosmologies
• Structure formation in dark energy cosmologies described by PADE parameterization
• Construction of gauge-invariant variables of linear metric perturbations on an arbitrary background spacetime
• A significant hardening and rising shape detected in the MeV/GeV nuFnu spectrum from the recently-discovered very-high-energy blazar S4 0954+65 during the bright optical flare in 2015 February
• An interacting model for the cosmological dark sector
• Detecting Relic Gravitational Waves in the CMB: Comparison of Planck and Ground-based Experiments
• Lyman alpha absorbers in motion: consequences of gravitational lensing for the cosmological redshift drift experiment
• Mapping the Kinematically Decoupled Core in NGC 1407 with MUSE
• Low-scale Inflation and Supersymmetry Breaking in Racetrack Models
• The Halo Occupation Distribution of HI from 21cm Intensity Mapping at Moderate Redshifts
• Investigating the influence of magnetic fields upon structure formation with AMIGA - a C code for cosmological magnetohydrodynamics
• A sudden dramatic change and recovery of magneto-environment of a repeating fast radio burst
• Gauge-invariant perturbations at second order in two-field inflation
• Cosmic microwave background with Brans-Dicke Gravity: I. Covariant Formulation
• Extending BEAMS to incorporate correlated systematic uncertainties
• Dynamical-Screening and the Phantom-Like Effects in a DGP-Inspired $F(R,\varphi )$ Model
• Discovering the constrained NMSSM with tau leptons at the LHC
• Lepton Flavor Model and Decaying Dark Matter in The Binary Icosahedral Group Symmetry
• SUSY dark matter and lepton flavor violation
• Measuring BAO and non-Gaussianity via QSO clustering
• The Reactor Anomaly after Daya Bay and RENO
• Statefinder parameters for quantum effective Yang-Mills condensate dark energy model
• Modification of the 21-cm power spectrum by quasars during the epoch of reionisation
• Uncorrelated estimates of the primordial power spectrum
• The Age-Redshift Relation For Luminous Red Galaxies Obtained From the Full Spectrum Fitting and Its Cosmological Implications
• Possible Detection of Apparent Superluminal inward motion in Markarian 421 after the Giant X-ray flare in February, 2010
• Benchmarks and Explanations for Deep Learning Estimates of X-ray Galaxy Cluster Masses
• Impact of string and monopole-type junctions on domain wall dynamics: implications for dark energy
• Gravitino Dark Matter and Non-Gaussianity
• Imprints of non-standard Dark Energy and Dark Matter Models on the 21cm Intensity Map Power Spectrum
• Predictions of a Natural SUSY Dark Matter Model for Direct and Indirect Detection Experiments
• Reconstruction of halo power spectrum from redshift-space galaxy distribution: cylinder-grouping method and halo exclusion effect
• Recovering the origins of the lenticular galaxy NGC 3115 using multi-band imaging
• Cosmology with Peculiar Velocities: Observational Effects
• pMSSM Dark Matter Searches on Ice
• Phase-space analysis of the cosmological 3-fluid problem: Families of attractors and repellers
• De-Sitter nonlinear sigma model and accelerating universe
• Primordial Non-Gaussianity and the Statistics of Weak Lensing and other Projected Density Fields
• Coherent dynamics of Rydberg atoms in cosmic microwave background radiation
• Non-Minimal Warm Inflation and Perturbations on the Warped DGP Brane with Modified Induced Gravity
• A model independent measure of the large scale curvature of the Universe
• Electromagnetic two-point functions and Casimir densities for a conducting plate in de Sitter spacetime
• Brane Inflation and the Overshoot Problem
• Constraining the Milky Way Dark Matter Density Profile with Gamma-Rays with Fermi-LAT
• On the realization of the MSSM inflation
• Distance Probes of Dark Energy
• The Higgs Boson is found: What is next?
• The escape fraction of ionizing photons from high redshift galaxies
• Braneworld Model of Dark Matter: Structure Formation
• Ultralight dark photon as a model for early universe dark matter
• Effects of a time-varying color-luminosity parameter $\beta$ on the cosmological constraints of modified gravity models
• Detectability of the 21 cm-CMB cross-correlation from the EoR
• Sudden Future Singularity models as an alternative to Dark Energy?
• FLRW accelerating universe with interactive dark energy
• Cosmological Perturbations and the Running Cosmological Constant Model
• Stability of a modified Jordan-Brans-Dicke theory in the dilatonic frame
• Normalized General Relativity: Non-closed Universe and Zero Cosmological Constant
• Scale-dependent non-Gaussianities in the WMAP data as identified by using surrogates and scaling indices
• Searching for planar signatures in WMAP
• Can cosmic acceleration be caused by exotic massless particles?
• New parameterization for unified dark matter and dark energy
• The Age-Redshift Relationship of Old Passive Galaxies
• Quasar variability limits on cosmological density of cosmic strings
• Emergent Universe in the Braneworld Scenario
• Cosmic Chemical Evolution with an Early Population of Intermediate Mass Stars
• Properties of the exact analytic solution of the growth factor and its applications
• Lepton number asymmetry via inflaton decay in a modified radiative seesaw model
• Crossing the Phantom divide line in the Chaplygin gas model
• Cosmological reconstruction and {\it Om} diagnostic analysis of Einstein-Aether Theory
• CFT driven cosmology and conformal higher spin fields
• Curvature and Entropy Perturbations in Generalized Gravity
• Ewald Sums for One Dimension
• An updated analysis of two classes of f(R) theories of gravity
• Magnetogenesis and the primordial non-gaussianity
• Cosmologically viable generalized Einstein-Aether theories
• Planck and reionization history: a model selection view
• The Impact of Assuming Flatness in the Determination of Neutrino Properties from Cosmological Data
• Analysis of $f(R)$ Theory Corresponding to NADE and NHDE
• Annihilation of NMSSM neutralinos in the Sun and neutrino telescope limits
• Periodic Cosmological Evolutions of Equation of State for Dark Energy
• Using pulsar timing arrays and the quantum normalization condition to constrain relic gravitational waves
• What kind of science is cosmology?
• Interacting Viscous Dark Energy in Bianchi Type-I Universe
• Hybrid inflation with moduli stabilization and low scale supersymmetry breaking
• Dark energy, integrated Sachs-Wolfe effect and large-scale magnetic fields
• Constraining the WMAP9 bispectrum and trispectrum with needlets
• Implications of Two Type Ia Supernova Populations for Cosmological Measurements
• Simulating the Anisotropic Clustering of Luminous Red Galaxies with Subhalos: A Direct Confrontation with Observation and Cosmological Implications
• Decoupling Dark Energy from Matter
• No-go theorem for bimetric gravity with positive and negative mass
• Expected properties of the Two-Point Autocorrelation Function of the IGM
• Flat Universe with Hyperbolic Voids
• Complete Hamiltonian analysis of cosmological perturbations at all orders
• Lensed Cosmic Microwave Background Constraints on Post-General Relativity Parameters
• Ricci Dark Energy in Brans-Dicke theory
• An FLRW interacting dark energy model of the Universe
• Improved Constraints on Anisotropic Birefringent Lorentz Invariance and CPT Violation from Broadband Optical Polarimetry of High Redshift Galaxies
• Foreground influence on primordial non-Gaussianity estimates: needlet analysis of WMAP 5-year data
• keV Warm Dark Matter via the Supersymmetric Higgs Portal
• Large-scale collective motion of RFGC galaxies
• Nearly scale-invariant curvature modes from entropy perturbations during graceful exit
• Initial directional singularity in inflationary models
• Electron EDM and soft leptogenesis in supersymmetric B-L extension of the standard model
• Cosmology based on $f(R)$ gravity with $\mathcal{O}(1)$ eV sterile neutrino
• Extra dimensions and Seesaw Neutrinos at the International Linear Collider
• CMB bounds on tensor-scalar-scalar inflationary correlations
• Non-Local Gravity from Hamiltonian Point of View
• A detailed view of filaments and sheets in the warm-hot intergalactic medium. I. Pancake formation
• An optimal basis system for cosmology: data analysis and new parameterisation
• An effective theory of accelerated expansion
• Barrow entropic Quintessence and Dilation dark energy Models with Generalized HDE cut-off
• A Terminal Velocity on the Landscape: Particle Production near Extra Species Loci in Higher Dimensions
• Is dark energy evolving?
• Do intergalactic magnetic fields imply an open universe?
• Warm Inflation in $f(R,T)$ gravity
• A dark energy view of inflation
• Dark Energy Nature in Logarithmic $f(R,T)$ Cosmology
• Measurement of the matter-radiation equality scale using the extended Baryon Oscillation Spectroscopic Survey Quasar Sample
• Small field models with gravitational wave signature supported by CMB data
• A generalized mass-to-horizon relation: a new global approach to entropic cosmologies and its connection to $\Lambda$CDM
• Trispectrum versus Bispectrum in Single-Field Inflation
• Erratum: Statistical anisotropy in the inflationary universe
• The Integrated Sachs-Wolfe Effect in Time Varying Vacuum Model
• Coupled quintessence with a possible transient accelerating phase
• Probing the course of cosmic expansion with a combination of observational data
• Cosmic Microwave Background Bispectrum from the Lensing--Rees-Sciama Correlation Reexamined: Effects of Non-linear Matter Clustering
• SUSY breaking scales in the gauge-Higgs unification
• The probability distribution for non-Gaussianity estimators constructed from the CMB trispectrum
• Physics of galactic colliders: high speed satellites in LCDM vs MONDian cosmology
• Can Relic Superhorizon Inhomogeneities be Responsible for Large-Scale CMB Anomalies?
• Curvature Constraints from the Causal Entropic Principle
• Cosmological constraints from low-redshift data
• Luminosity Distribution of Gamma-Ray Burst Host Galaxies at redshift z=1 in Cosmological Smoothed Particle Hydrodynamic Simulations: Implications for the Metallicity Dependence of GRBs
• BDM Dark Matter: CDM with a core profile and a free streaming scale
• A gravitational lensing explanation for the excess of strong Mg-II absorbers in GRB afterglow spectra
• Figures of Merit for Testing Standard Models: Application to Dark Energy Experiments in Cosmology
• Reconciling the cosmic age problem in the R_h=ct Universe
• Project Dinos II: Redshift evolution of dark and luminous matter density profiles in strong-lensing elliptical galaxies across 0.1 < z < 0.9
• MFV Reductions of MSSM Parameter Space
• Inflation without self-reproduction in $F(R)$ gravity
• The First Billion Years project: gamma-ray bursts at z>5
• Quantum cosmological consistency condition for inflation
• Search for a dark vector gauge boson decaying to ${\pi }^{+}{\pi }^{-}$ using $\eta \to {\pi }^{+}{\pi }^{-}\gamma$ decays
• On the dark matter haloes inner structure and galaxy morphology
• What determines the observational differences of blazars?
• Simultaneous determination of the cosmic birefringence and miscalibrated polarisation angles from CMB experiments
• Whether Lyra's Manifold Itself is a Hidden Source of Dark Energy
• The impact of the Universe's expansion rate on constraints on modified growth of structure
• Astrophysical and Cosmological Searches for Lorentz Invariance Violation
• DE models with combined $H_0\cdot r_d$ from BAO and CMB dataset and friends
• Time variability of the core-shift effect in the blazar 3C 454.3
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines II. [C II], [O I], [O III], [N II] and [N III] up to z=6
• Quintom fields from chiral K-essence cosmology
• Dynamical systems of cosmological models for different possibilities of $G$ and ${\rho }_{\Lambda }$
• Minisuperspace Quantization of $f\left(T,B\right)$ Cosmology
• How much primordial tensor mode is allowed?
• FRW dark energy cosmological model with hybrid expansion law
• Triplet Leptogenesis, Type-II Seesaw Dominance, Intrinsic Dark Matter, Vacuum Stability and Proton Decay in Minimal SO(10) Breakings
• Non-commutative effects on gravitational measurements
• SPMHD simulations of Structure Formation
• On the possibility of braneworld quintessential inflation
• Inflation with Planck: a survey of some "exotic" inflationary models
• Repulsive gravity model for dark energy
• Supernova, baryon acoustic oscillations, and CMB surface distance constraints on f(G) higher order gravity models
• The ACS LCID Project XI. On the early time resolution of LG dwarf galaxy SFHs: Comparing the effects of reionization in models with observations
• Quadra-Spectrum and Quint-Spectrum from Inflation and Curvaton Models
• On the Hojman conservation quantities in Cosmology
• Discovery of off-axis jet structure of TeV blazar Mrk 501 with mm-VLBI
• Detection of Molecular Gas in Void Galaxies : Implications for Star Formation in Isolated Environments
• Detecting relic gravitational waves in the CMB: The contamination caused by the cosmological birefringence
• High Redshift Investigation On The Dark Energy Equation of State
• Geometric and dynamic distortions in anisotropic galaxy clustering
• Exploring SUSY light Higgs boson scenarios via dark matter experiments
• The Observable Thermal and Kinetic Sunyaev-Zel'dovich Effect in Merging Galaxy Clusters
• One-loop effects on MSSM parameter determination via chargino production at the LC
• Decaying Dark Matter in the Supersymmetric Standard Model with Freeze-in and Seesaw mechanims
• Bianchi type-V dark energy model with varying EoS parameter
• Cold Dark Matter Hypotheses in the MSSM
• Scalar field dark energy perturbations and the Integrated Sachs Wolfe effect
• Expected constraints on the Galactic magnetic field using PLANCK data
• Hierarchies of Susy Splittings and Invisible Photinos as Dark Matter
• Neutralino-Sbottom Coannihilation in SU(5)
• Observational Constraints on the Normal Branch of a Warped DGP Cosmology
• Application of cross correlations between CMB and large scale structure to constraints on the primordial non-Gaussianity
• A gauge-invariant approach to interactions in the dark sector
• An analytic approach to perturbations from an initially anisotropic universe
• The lessons from the running of the tensor-to-scalar ratio
• Needatool: A Needlet Analysis Tool for Cosmological Data Processing
• CP Violating Lepton Asymmetry from B Decays in Supersymmetric Grand Unified Theories
• On the optimality of the spherical Mexican hat wavelet estimator for the primordial non-Gaussianity
• Probing Dark Energy with the Kunlun Dark Universe Survey Telescope
• Long-lived stops in MSSM scenarios with a neutralino LSP
• Power-law solutions and accelerated expansion in scalar-tensor theories
• Non-Gaussianity constrains hybrid inflation
• Optical variability of radio-intermediate quasars
• The dark side of curvature
• When Should We Treat Galaxies as Isolated?
• Coupled currents in cosmic strings
• From CFT Spectra to CMB Multipoles in Quantum Gravity Cosmology
• Remote Inflation: Hybrid-like inflation without hybrid-type potential
• Tracking Quintessence and Cold Dark Matter Candidates
• Dynamical Dark Energy model parameters with or without massive neutrinos
• Curvatons in Warped Throats
• Ohmic currents and pre-decoupling magnetism
• Superbradyons and some possible dark matter signatures
• Clumpiness enhancement of charged cosmic rays from dark matter annihilation with Sommerfeld effect
• CMB Polarization and Temperature Power Spectra Estimation using Linear Combination of WMAP 5-year Maps
• Angular-planar CMB power spectrum
• Precision Measurements of Little Higgs Parameters at the International Linear Collider
• Birefringence, CMB polarization and magnetized B-mode
• CMBPol Mission Concept Study: Reionization Science with the Cosmic Microwave Background
• Dark Matter Decaying into a Fermi Sea of Neutrinos
• Formation of globular clusters induced by external ultraviolet radiation
• A prototype of a directional detector for non-baryonic dark matter search: MIMAC (Micro-TPC Matrix of Chambers)
• Non-Perturbative Yang-Mills Condensate as Dark Energy
• Nonlinear reconstruction of features in the primordial power spectrum from large-scale structure
• Observational constraints on the energy scale of inflation
• Large Blue Spectral Isocurvature Spectral Index Signals Time-Dependent Mass
• Quantum cosmology with symmetry analysis for quintom dark energy model
• Study of the observational compatibility of an inhomogeneous cosmology with linear expansion according to SNe Ia
• Codimension-2 brane inflation
• Trans-Planckian enhancements of the primordial non-Gaussianities
• Relaxing the Cosmological Constraints on Unparticle Dark Component
• Spatially-Resolved Medium Resolution Spectroscopy of an Interacting E+A (post-starburst) System with the Subaru telescope
• Assessment of the Systematic Uncertainties in the Cosmological Analysis of the SDSS Supernovae Photometric Sample
• Scalar field power-law cosmology with spatial curvature and dark energy-dark matter interaction
• Prospects in Constraining the Dark Energy Potential
• Chain Inflation Reconsidered
• Spider Optimization II: Optical, Magnetic and Foreground Effects
• Comparison of neutralino and sneutrino dark matter in a model with spontaneous CP violation
• Constraining the history of reheating with the NANOGrav 15-year data
• Neutron star mass in dark matter clumps
• Modelling the stochasticity of high-redshift halo bias
• Gravitational Waves from Incomplete Inflationary Phase Transitions
• Constraints on the Phase Plane of the Dark Energy Equation of State
• Observation constraints on scalar field cosmological model in Anisotropic universe
• Perturbative stability of SFT-based cosmological models
• Dark Energy Cosmology with the Alternative Cosmic Microwave Background Data
• Similarity solutions for the Wheeler-DeWitt equation in $f\left(R\right)$-cosmology
• The first spectral line surveys searching for signals from the Dark Ages
• CMBR Weak Lensing and HI 21-cm Cross-correlation Angular Power Spectrum
• Probing CMB Cold Spot through Local Minkowski Functionals
• Multi-Field Inflation from String Theory
• A phenomenological study of 5d supersymmetry
• Inclusive Constraints on Unified Dark Matter Models from Future Large-Scale Surveys
• Power-Law and Logarithmic Entropy-Corrected Ricci Viscous Dark Energy and Dynamics of Scalar Fields
• Fractal Structure of Isothermal Lines and Loops on the Cosmic Microwave Background
• Consistency of Equations in the Second-order Gauge-invariant Cosmological Perturbation Theory
• Orbital perturbations due to massive rings
• Observational tests for oscillating expansion rate of the Universe
• Constraints on Models with a Break in the Primordial Power Spectrum
• Subdegree Sunyaev-Zel'dovich Signal from Multifrequency BOOMERanG observations
• A model of nonsingular universe
• Bounds from ISW-galaxy cross-correlations on generalized covariant Galileon models
• Generalized models of unification of dark matter and dark energy
• Bianchi type-VI anisotropic dark energy model with varying EoS parameter
• Parametrizing the transition to the phantom epoch with Supernovae Ia and Standard Rulers
• Signatures of Dark Matter in Inert Triplet Models
• Parametrization for the Scale Dependent Growth in Modified Gravity
• Natural scaling for dark energy
• Analytic Spectra of CMB Anisotropies and Polarization Generated by Scalar Perturbations in Synchronous Gauge
• UVIT view of Centaurus A; a detailed study on positive AGN feedback
• On probing the properties of QSOs through their proximity effects on the intergalactic medium
• Anisotropic Massive Gauge-flation
• Statistical Determination of Bulk Flow Motions
• Baryon asymmetry and lower bound on right handed neutrino mass in fast expanding Universe: an analytical approach
• ISW-LSS cross-correlation in coupled Dark Energy models with massive neutrinos
• On existence of a possible Lorentz invariant modified gravity in Weitzenböck spacetime
• Spin-$1/2$ invisible particles in heavy meson decays
• Environmental dependence of AGN activity and star formation in galaxy clusters from Magneticum simulations
• Next-to-leading order QCD predictions for the signal of Dark Matter and photon associated production at the LHC
• Viable inflationary models ending with a first-order phase transition
• Varying constants entropic--$\Lambda$CDM cosmology
• Cosmic Ray Anomalies from the MSSM?
• Revisiting non-Gaussianity of multiple-field inflation from the field equation
• Exploring the Cosmological Model in $f(R,T^{\varphi })$ Gravity with Observational Constraints
• Cross-correlations of the Lyman-alpha forest with weak lensing convergence I: Analytical Estimates of S/N and Implications for Neutrino Mass and Dark Energy
• Observational tests of backreaction with recent data
• Effects of P-wave Annihilation on the Angular Power Spectrum of Extragalactic Gamma-rays from Dark Matter Annihilation
• Quintom cosmological model and some possible solutions using Lie and Noether symmetries
• Frequentist comparison of CMB local extrema statistics in the five-year WMAP data with two anisotropic cosmological models
• The effect of inhomogeneities on dark energy constraints
• Cosmological models of generalized ghost pilgrim dark energy (GGPDE) in the gravitation theory of Saez-Ballester
• Constraining Holographic Dark Energy and Analyzing Cosmological Tensions
• Modeling and Analyzing Stability of Hybrid Stars within $f(Q)$ Gravity
• Fluid inflation with brane correction
• Inverse problem - reconstruction of dark energy models
• Cosmological Birefringence: an Astrophysical test of Fundamental Physics
• $f(Q,T)$ gravity: From early to late-time cosmic acceleration
• The Past History of Galaxy Clusters told by their present neighbors
• A small Universe
• Combining Optical and X-ray Observations of Galaxy Clusters to Constrain Cosmological Parameters
• An Effective Selection Method for Low-Mass Active Black Holes and First Spectroscopic Identification
• A Clipping Method to Mitigate the Impact of Catastrophic Photometric Redshift Errors on Weak Lensing Tomography
• Probing a Mixed Neutralino Dark Matter Model at the 7 TeV LHC
• Evolution of CIV Absorbers. II. Where does CIV live?
• Multi-scalar field cosmology from SFT: an exactly solvable approximation
• Time Variable Cosmological Constants from the Age of Universe
• Revisiting cosmic acceleration with DESI BAO
• Stochastic Samples versus Vacuum Expectation Values in Cosmology
• Measuring dark matter ellipticity of Abell 901/902 using Particle Based Lensing
• Figure of Merit and Different Combinations of Observational Data Sets
• Dark Energy and Inflation in a Gravitational Wave Dominated Universe
• New type of hill-top inflation
• Reconstructing the growth index $\gamma$ with Gaussian Processes
• CLEAN imaging systematics of M87 radio jet
• Neutrino phenomenology in the flavored NMSSM without domain wall problems
• Universe Inflation Based on Nonlinear Electrodynamics
• Correlation of supernova redshifts with temperature fluctuations of the Cosmic Microwave Background
• Enhanced Dark Matter Annihilation Rate for Positron and Electron Excesses from Q-ball Decay
• Implications of JLA data for $k-$essence model of dark energy with given equation of state
• Using Cold Atoms to Measure Neutrino Mass
• Observationally constrained accelerating cosmological model with higher power of non-metricity and squared trace
• Impact of the 1/f noise and the asymmetric beam on non-Gaussianity searches with Planck
• $f(T,B)$ gravity in a Friedmann-Lema\^ıtre-Robertson-Walker universe with nonzero spatial curvature
• Gravitino dark matter and the lithium primordial abundance within a pre-BBN modified expansion
• Adiabatic versus Isocurvature Non--Gaussianity
• Deep Correlation Between Cosmic-Ray Anomaly and Neutrino Masses
• Thermal abundance of non-relativistic relics with Sommerfeld enhancement
• Seesaw Neutrino Signals at the Large Hadron Collider
• Non-Gaussianity from false vacuum inflation: Old curvaton scenario
• Neutralino and Chargino Production in U(1)' at the LHC
• Dark Energy Perturbations Revisited
• Multiple $\Lambda$CDM cosmology with string landscape features and future singularities
• Is $w\ne -1$ evidence for a dynamical dark energy equation of state ?
• Modulated preheating and isocurvature perturbations
• Crossing the Phantom Divide in Extended Dvali-Gabadadze-Porrati Gravity
• G.A.S. I: A prescription for turbulence-regulated star formation and its impact on galaxy properties
• Balancing the Baryon Budget: The fraction of the IGM due to Galaxy Mergers
• Predictions for BAO distance estimates from the cross-correlation of the Lyman-alpha forest and redshifted 21-cm emission
• CDMS II result and Light Higgs Boson Scenario of the MSSM
• Dynamical evolutin of quintessence dark energy in collapsing dark matter halos
• Brightness temperature - obtaining physical properties of non-equipartition plasma
• Decaying dark matter mimicking time-varying dark energy
• Cosmological dynamics of a non-minimally coupled bulk scalar field in DGP setup
• Cosmic acceleration and phantom crossing in $f(T)$-gravity
• Quadratic Isocurvature Cross-Correlation, Ward Identity, and Dark Matter
• Relaxing a large cosmological constant in the astrophysical domain
• Designing Future Dark Energy Space Missions: II. Photometric Redshift of Space Weak Lensing Optimized Survey
• Crossing the Cosmological Constant Line on a Warped DGP Brane
• The CMBR ISW and HI 21-cm Cross-correlation Angular Power Spectrum
• Cosmological constraints on Agegraphic dark energy in DGP braneworld gravity
• Examining leptogenesis with lepton flavor violation and the dark matter abundance
• Constraints on neutrino masses from the lensing dispersion of Type Ia supernovae
• Models of supersymmetric dark matter and their predictions in light of CDMS
• Complete Hamiltonian analysis of cosmological perturbations at all orders II: Non-canonical scalar field
• Smooth crossing of $w_{\Lambda }=-1$ line in a single scalar field model
• A Phase Transition between Small and Large Field Models of Inflation
• Stop-mass prediction in naturalness scenarios within MSSM-25
• Extended FLRW Models: dynamical cancellation of cosmological anisotropies
• The optimal redshift for detecting ionized bubbles in HI 21-cm maps
• Quintessential and phantom power-law solutions in scalar tensor model of dark energy
• Generalizing thawing dark energy models: the standard vis-à-vis model independent diagnostics
• Brane inflation revisited after WMAP five-year results
• Distinguishing reionization models using the largest cluster statistics of the 21-cm maps
• Modified Gravity or Dark Matter?
• An Introduction into the Theory of Cosmological Structure Formation
• Results on photon-mediated dark matter-nucleus interactions from the PICO-60 C${}_3$F${}_8$ bubble chamber
• Gravity- and temperature-driven phase transitions in a model for collapsed axionic condensates
• Late-time acceleration driven by shift-symmetric Galileon in the presence of Torsion
• Biases to primordial non-Gaussianity measurements from CMB secondary anisotropies
• Constraining the physics of star formation from CIB-cosmic shear cross-correlations
• The interacting generalized Ricci dark energy model in non-flat universe
• Constraints on primordial non-Gaussianity from WMAP7 and Luminous Red Galaxies power spectrum and forecast for future surveys
• Dynamical System Analysis of Quintessence Models with Exponential Potential -- Revisited
• Dynamical analysis for a scalar-tensor model with kinetic and non-minimal couplings
• Gluon condensate, modified gravity, and the accelerating Universe
• Testing a Phenomenologically Extended DGP Model with Upcoming Weak Lensing Surveys
• Constraint on dark matter annihilation with dark star formation using Fermi extragalactic diffuse gamma-ray background data
• An original constraint on the Hubble constant: h>0.74
• Power suppression from disparate mass scales in effective scalar field theories of inflation and quintessence
• Reconstructing Single Field Inflationary Actions From CMBR Data
• Constraining Perturbative Early Dark Energy with Current Observations
• Correlation function of quasars in real and redshift space from the Sloan Digital Sky Survey Data Release 7
• Anisotropy effects on Baryogenesis in $f(R)$-Theories of Gravity
• Effects of Chameleon Scalar Field on Rotation Curves of the Galaxies
• Matter Parity Violating Dark Matter Decay in Minimal SO(10), Unification, Vacuum Stability and Verifiable Proton Decay
• Modification of the halo mass function by kurtosis associated with primordial non-Gaussianity
• Non-linear mode coupling and the growth of perturbations in LCDM
• Constraining dark matter sub-structure with the dynamics of astrophysical systems
• Solar System Tests in Brans-Dicke and Palatini f(R)-theories
• Parameterization Effects in the analysis of AMI Sunyaev-Zel'dovich Observations
• Discrimination of New Physics Models with the International Linear Collider
• Quantum Yang--Mills Dark Energy
• Isophote Shapes of Early-Type Galaxies in Massive Clusters at $z\sim 1$ and 0
• Detecting the Elusive Blazar Counter-Jets
• A weak lensing view on primordial non-Gaussianities
• Cosmology in doubly coupled massive gravity: constraints from SNIa, BAO and CMB
• Searching for Dark Matter in Messier 33
• CMB anisotropies induced by tensor modes in Massive Gravity
• Direct Collapse to Supermassive Black Hole Seeds: Comparing the AMR and SPH Approaches
• Short Distance Physics and Initial State Effects on the CMB Power Spectrum
• Non-linear cosmological collapse of quintessence
• Cosmological nonlinear density and velocity power spectra including nonlinear vector and tensor modes
• Last scattering, relic gravitons and the circular polarization of the CMB
• Connecting the Dots: Tracking Galaxy Evolution Using Constant Cumulative Number Density at 3<z<7
• Long-lived charged Higgs at LHC as a probe of scalar Dark Matter
• Cosmic microwave background anomalies viewed via Gumbel Statistics
• 30 GHz observations of sources in the VSA fields
• Can a void mimic the $\Lambda$ in $\Lambda$CDM?
• Scale invariant jets: from blazars to microquasars
• Cosmological constant in F(R) supergravity
• Orthogonal BipoSH measures : Scrutinizing sources of isotropy violation
• The effect of the linear term on the wavelet estimator of primordial non-Gaussianity
• Statistical Isotropy violation of the CMB brightness fluctuations
• Numerical Relativity as a New Tool for Fundamental Cosmology
• New features in curvaton model
• The tilting rate of the Milky Way's disc
• Chargino reconstruction in supersymmetry with long-lived staus
• Reconstructing $f(T)$ modified gravity from ECHDE and ECNADE models
• F-term Braneworld inflation in Light of Five-year WMAP observations
• Neutralino Dark Matter in Gauge Mediation in Light of CDMS-II
• WMAP5 Observationnal Constraints on Braneworld New Inflation Model
• Average Dark Matter Halo Sparsity Relations as Consistency Check of Mass Estimates in Galaxy Cluster Samples
• Damping of the baryon acoustic oscillations in the matter power spectrum as a probe of the growth factor
• Constraints on Cardassian universe from Gamma ray bursts
• Quasi-linear regime and rare-event tails of decaying Burgers turbulence
• On primordial trispectrum from exchanging scalar modes in general multiple field inflationary models
• Parametric tension between even and odd multipole data of WMAP power spectrum: unaccounted contamination or missing parameters?
• Recent developments in astrophysical and cosmological exploitation of microwave surveys
• Scalar field exact solutions for non-flat FLRW cosmology: A technique from non-linear Schrödinger-type formulation
• Evolution in bouncing quantum cosmology
• The Extended Analysis On New Generalized Chaplygin Gas
• Catalog of Radio Galaxies with z>0.3. II: Photometric Data
• Cosmological constraints on $f(Q)$ gravity models in the non-coincident formalism
• Forecasts of cosmological constraints from Type Ia supernovae including the weak-lensing convergence
• Discord in Concordance Cosmology and Anomalously Massive Early Galaxies
• Cluster-lensing: A Python Package for Galaxy Clusters & Miscentering
• Viscous Dark Energy and Phantom Field in An Anisotropic Universe
• The GMRT archive atomic gas survey -- II. Mass modelling and dark matter halo properties across late-type spirals
• Anisotopic inflation with a non-abelian gauge field in Gauss-Bonnet gravity
• Constraints on Cosmological Models from Hubble Parameters Measurements
• Gravitational Lensing Effects on the Baryonic Acoustic Oscillation Signature in the Redshift-Space Correlation Function
• Observational Constraints on Visser's Cosmological Model
• Dissecting Galaxies with Quantitative Spectroscopy of the Brightest Stars in the Universe
• The universe is accelerating. Do we need a new mass scale?
• Multi-photon signal in supersymmetry comprising non-pointing photon(s) at the LHC
• Small steps towards Grand Unification and the electron/positron excesses in cosmic-ray experiments
• The nonlinear redshift space probability distribution function in models with local primordial non-Gaussianity
• Constraining Thawing Dark Energy using Galaxy Cluster Number Counts
• Detection of Dark Matter Decay in the X-ray
• The Standard model Higgs as the inflaton
• Spatial Correlations in the Helium-Ionizing Background
• Some Uncomfortable Thoughts on the Nature of Gravity, Cosmology, and the Early Universe
• Age problem in holographic dark energy
• Interacting warm dark matter
• Constraints from CMB in the intermediate Brans-Dicke inflation
• Phantom dark energy with tachyonic instability: metric perturbations
• The HeI 584 A Forest as a Diagnostic of Helium Reionization
• Improved parametrization of the growth index for dark energy and DGP models
• Clustering of Superstring Loops
• Reconstructions of $f(\mathcal{P})$ and $f(\mathcal{Q})$ gravity models from $(m,n)$-type Barrow Holographic Dark Energy: Analysis and Observational Constraints
• Detection of relic gravitational waves in the CMB: Prospects for CMBPol mission
• Dynamics of Magnetized Bulk Viscous Strings in Brans-Dicke Gravity
• The influence of mergers on the cluster temperature function and cosmological parameters derived from it
• Joint Minkowski Functionals and Bispectrum Constraints on Non-Gaussianity in the CMB
• Do Bound Structures Brake Cosmic Acceleration?
• SFT non-locality in cosmology: solutions, perturbations and observational evidences
• Signatures from an extra-dimensional seesaw model
• A simple model of pointlike spacetime defects and implications for photon propagation
• Primordial non-Gaussianity with Angular correlation function: Integral constraint and validation for DES
• Effect of low anisotropy on cosmological models by using supernova data
• Phantom-Like Behavior of a DGP-Inspired Scalar-Gauss-Bonnet Gravity
• Mixed fluid cosmological model in $f(R,T)$ gravity
• An Application of Wiener Hermite Expansion to Non-linear Evolution of Dark Matter
• Manufacturing cosmic rays in the evolving dynamical states of galaxy clusters
• Tachyon-Dilaton-induced Inflation as an alpha'-resummed String Background
• Generalized Model of Interacting Dark Energy and Dark Matter : Phase Portrait Analysis of Evolving Universe
• Fast generation of mock galaxy catalogues with COLA
• Neutralino dark matter annihilation to monoenergetic gamma rays as a signal of low mass superstrings
• Perturbed dark energy: classical scalar field versus tachyon
• Galactic outflows and the kinematics of damped Lyman alpha absorbers
• Probing the primordial power spectra with inflationary priors
• Cosmology with a Continuous Tower of Scalar Fields
• Molecular hydrogen in Lyman Alpha Emitters
• Generalized Scaling Ansatz and Minimal Seesaw Mechanism
• AstroFit: An Interface Program for Exploring Complementarity in Dark Matter Research
• Upper Limit on Dimming of Cosmological Sources by Intergalactic Grey Dust from the Soft X-ray Background
• How low-scale Trinification sheds light in the flavour hierarchies, neutrino puzzle, dark matter and leptogenesis
• Phase space analysis for a scalar-tensor model with kinetic and Gauss-Bonnet couplings
• Search for inelastic dark matter in events with two displaced muons and missing transverse momentum in proton-proton collisions at $\sqrt{s}$ = 13 TeV
• Discriminating Electroweak-ino Parameter Ordering at the LHC and Its Impact on LFV Studies
• Degree-scale anomalies in the CMB: localizing the first peak dip to a small patch of the north ecliptic sky
• Thermal Fluctuations of Dark Matter in Bouncing Cosmology
• UV/IR mode mixing and the CMB
• Gravitationally induced particle production and its impact on structure formation
• The Scale Factor in the Universe with Dark Energy
• Quantum corrections during inflation and conservation of adiabatic perturbations
• Inhomogeneous fluids for warm inflation
• Knot Universes in Bianchi Type I Cosmology
• A semi-analytic model of pairwise velocity distribution between dark matter halos
• WMAP Constraints On K-Inflation
• Non-Gaussian error bars in galaxy surveys -- II
• Detection of Hot Gas in Galaxy Groups via the Sunyaev-Zel'dovich Effect
• On the separation between baryonic and dark matter: evidence for phantom dark matter?
• The kinetic Sunyaev-Zel'dovich tomography II: probing the circumgalactic medium
• Implementing Hilltop F-term Hybrid Inflation in Supergravity
• MOJAVE -- XXII. Brightness temperature distributions and geometric profiles along parsec-scale AGN jets
• Momentum dependence of the bispectrum in two-field inflation
• Probing Cosmology and Galaxy Cluster Structure with the Sunyaev-Zel'dovich Decrement vs. X-ray Temperature Scaling Relation
• Characterizing SL2S galaxy groups using the Einstein radius
• Quantum Modifications to Gravity Waves in de Sitter Spacetime
• Non-minimal coupling of the phantom field and cosmic acceleration
• CP-violating inflation and its cosmological imprints
• Higgs-Inflaton Potential in Higher-Dimensional SUSY Gauge Theories
• Impact of Cosmology on Lorentz Invariance Violation Constraints from GRB Time-Delays
• Nonsingular Chaplygin gas cosmologies in universes connected by wormhole
• The effective Equation of State in Palatini $f(R)$ cosmology
• Impact of freeze-in on dark matter isocurvature
• An unbiased method of measuring the ratio of two data sets
• Cosmological Constraints on Rapid Roll Inflation
• Fuzzy Supernova Templates II: Parameter Estimation
• Constraining Decaying Dark Matter
• Modelling Time-varying Dark Energy with Constraints from Latest Observations
• Ellipticity of Structures in CMB Sky Maps
• Statistics of the excursion sets in models with local primordial non-Gaussianity
• Primordial gravitational wave of BICEP2 from dynamical double hybrid inflation
• What do we learn from CMB observations
• MSSM dark matter measurements at the LHC without squarks and sleptons
• Local Scale-Dependent Non-Gaussian Curvature Perturbations at Cubic Order
• $\mu -e$ Conversion With Four Generations
• Particle Spectroscopy of Supersymmetric SO(10) with Non-Universal Gaugino Masses
• On the coldness of the local Hubble flow: the role of baryons
• Origin of the Chemical Elements
• Ultra-fine dark matter structure in the Solar neighbourhood
• Direct measurement of the angular power spectrum of cosmic microwave background temperature anisotropies in the WMAP Data
• Aspects of Some New Versions of Pilgrim Dark Energy in DGP Braneworld
• Log-Poisson Non-Gaussianity of Ly$\alpha$ Transmitted Flux Fluctuations at High Redshift
• The Impact of HI in Galaxies on 21-cm Intensity Fluctuations During the Reionisation Epoch
• Relating information entropy and mass variance to measure bias and non-Gaussianity
• Stability analysis of agegraphic dark energy in Brans-Dicke cosmology
• Testing the gaugino AMSB model at the Tevatron via slepton pair production
• The Interstellar Medium: The Key Component in Galactic Evolution and Modern Cosmology
• Spiral galaxies rotation curves in the Horava - Lifshitz gravity theory
• Reconstruction of the equation of state for the cyclic universes in homogeneous and isotropic cosmology
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• The Type Ia Supernova Rate in Radio and Infrared Galaxies from the CFHT Supernova Legacy Survey
• Gravitationally Lensed Quasar SDSS J1442+4055: Redshifts of Lensing Galaxies, Time Delay, Microlensing Variability, and Intervening Metal System at z ~ 2
• Quadratic integrals of a multi-scalar cosmological model
• Cosmic shear statistics in cosmologies with non-Gaussian initial conditions
• Radio-relic and the diffuse emission trail discovered in a low mass galaxy cluster Abell 1697
• On solutions of loop quantum cosmology
• Luminous satellite galaxies in gravitational lenses
• A Novel Approach to Constrain the Escape Fraction and Dust Content at High Redshift Using the Cosmic Infrared Background Fractional Anisotropy
• A rapidly declining transient discovered with Subaru/Hyper Suprime-Cam
• Constraints on Dark Energy state equation with varying pivoting redshift
• The WHIQII Survey: Metallicities and Spectroscopic Properties of Luminous Compact Blue Galaxies
• Fast estimation of aperture-mass statistics I: aperture mass variance and an application to the CFHTLenS data
• Physical and kinematic conditions of the local merging galaxy NGC 1487
• Periods of the Long-Term Variability of the Blazar 0716+714 and Their Inter-Correlations in a Helical Jet Model
• Extra relativistic degrees of freedom without extra particles using Planck data
• Parabolic jet shape on parsec scales in high redshift AGN
• Reconstructing quintom from WMAP 5-year observations: Generalized ghost condensate
• New Tests of Millilensing in the Blazar PKS 1413+135
• Superparticle Signatures: from PAMELA to the LHC
• Einstein Static Universe and its Stability in Generalized Rastall Gravity
• Anisotropic inflation in non-minimal kinetic coupling model
• Noether Symmetry analysis in Chameleon Field Cosmology
• Imprints of dynamical dark energy on weak-lensing measurements
• Non-Gaussianity in Island Cosmology
• Reconciling inverse-Compton Doppler factors with variability Doppler factors in blazar jets
• Power Spectra of CMB Polarization by Scattering in Clusters
• Accelerating the Universe with Gravitational Waves
• Probing departures from $\Lambda$CDM by late-time datasets
• $\Lambda$-CDM type Heckmann - Suchuking model and union 2.1 compilation
• Can we distinguish early dark energy from a cosmological constant?
• Addressing μ-b_μand proton lifetime problems and active neutrino masses in a U(1)^\prime-extended supergravity model
• Statistics of the Sunyaev-Zel'dovich Effect power spectrum
• Looking into the Jet Cone of the Neutrino-Associated Very High Energy Blazar PKS 1424+240
• Reconstructing FHDE with Scalar and Gauge Fields
• Statistical nature of non-Gaussianity from cubic order primordial perturbations: CMB map simulations and genus statistic
• Latest Observational Constraints on Cardassian Models
• Are we seeing the beginnings of Inflation?
• Modified Bekenstein-Hawking system in $f(R)$ gravity
• On the dwarf galaxies rotation curves diversity problem
• Stable $f(Q)$ gravity model through non-trivial connection
• The primordial "f_NL" non-Gaussianity, and perturbations beyond the present horizon
• Deformation of the quintom cosmological model and its consequences
• Testing the consistency of early and late cosmological parameters with BAO and CMB data
• Cosmic evolution in the background of non-minimal coupling in $f(R,T,R_{\mu \nu }{T}^{\mu \nu })$ Gravity
• Searching for the earliest galaxies in the 21 cm forest
• The study of light invisible particles in $B_c$ decays
• Dwarf Galaxies without Dark Matter: constraints on Modified Gravity
• Coupled Quintessence scalar field model in light of observational datasets
• Galaxy Statistics in Pencil-beam Surveys at High Redshifts
• The integrated angular bispectrum
• The Physics of Q-balls
• Some anisotropic universes in the presence of imperfect fluid coupling with spatial curvature
• Comments on SUSY inflation models on the brane
• Radio spectral properties of cores and extended regions in blazars in the MHz regime
• Vacuum Energy Density in the Quantum Yang - Mills Theory
• Environmental dependence of 8um luminosity functions of galaxies at z~0.8: Comparison between RXJ1716.4+6708 and the AKARI NEP deep field
• Purely Triplet Seesaw and Leptogenesis within Cosmological Bound, Dark Matter and Vacuum Stability
• Goodness-of-fit analysis of the Cosmicflows-2 database of velocities
• Towards an Observational Appraisal of String Cosmology
• The Cosmology of Asymmetric Brane Modified Gravity
• Time variable cosmological constant of holographic origin with interaction in Brans-Dicke theory
• Constraining the Lattice Fluid Dark Energy from SNe Ia, BAO and OHD
• CMB map restoration
• 1/R Correction to Gravity in the Early Universe
• The blazar OJ 287 jet from parsec- to kiloparsec-scales
• Constraining graviton non-Gaussianity through the CMB bispectra
• Possible Enhancement of High Frequency Gravitational Waves
• Reconstruction of the interaction term between dark matter and dark energy using SNe Ia
• Enhanced One-Loop Corrections to WIMP Annihilation and their Thermal Relic Density in the Coannihilation Region
• Cold stream stability during minor mergers
• Impact of the Epoch of Reionization sources on the 21-cm bispectrum
• Emergent gravity fails to explain color-dependent galaxy-galaxy lensing signals from SDSS Dr7
• Probing interaction in the dark sector
• On Dark Energy Isocurvature Perturbation
• Dark energy density predicted and explained
• Let there be Light: the Emergence of Structure out of the Dark Ages in the Early Universe
• Cosmological flux noise and measured noise power spectra in SQUIDs
• Structure formation in clustering DBI dark energy model with constant sound speed
• Primordial power spectrum versus extension parameters beyond the standard model
• Non-minimally coupled scalar field in Kantowski--Sachs model and symmetry analysis
• Andromeda XXV -- a dwarf galaxy with a low central dark matter density
• Unveiling the Bent Jet Structure and Polarization of OJ 287 at 1.7 GHz with Space VLBI
• The role of domain wall junctions in Carter's pentahedral model
• The TeV-mass curvaton
• Modified gravity in a viscous and non-isotropic background
• Towards a warped inflationary brane scanning
• The Berry phase in inflationary cosmology
• Cosmic Rays during BBN as Origin of Lithium Problem
• The Structure of Cold Dark Matter Halos: Recent Insights from High Resolution Simulations
• High-precision spectra for dynamical Dark Energy cosmologies from constant-w models
• Imprints of a hemispherical power asymmetry in the seven-year WMAP data due to non-commutativity of space-time
• Perturbation Theory Remixed: Improved Nonlinearity Modeling beyond Standard Perturbation Theory
• Cosmological perturbations in the $\Lambda$CDM-like limit of a polytropic dark matter model
• Improvements in the X-ray luminosity function and constraints on the Cosmological parameters from X-ray luminous clusters
• Scalar Dark Energy Models and Scalar-Tensor Gravity: Theoretical Explanations for the Accelerated Expansion of Present Universe
• Primordial density perturbations with running spectral index: impact on non-linear cosmic structures
• Concentrating the Dark Matter in Galaxy Clusters through Tidal Stripping of Baryonically-Compressed Galactic Halos
• Re-examining the role of curvature in the slowing down acceleration scenario
• Unparticle-Higgs Mixing: MSW Resonances, See-saw Mechanism and Spinodal Instabilities
• Electromagnetic vacuum fluctuations around a cosmic string in de Sitter spacetime
• The formation of the first galaxies and the transition to low-mass star formation
• Hubble drift in Palatini $f(\mathcal{R})$-theories
• Thermal relics in cosmology with bulk viscosity
• Scalar field description of a parametric model of dark energy
• Curvaton preheating revisited
• Distances to Galaxies from the Brightest Stars in the Universe
• Turbulence-induced deviation between baryonic field and dark matter field in the spatial distribution of the Universe
• Redshift evolution of the 1.4 GHz volume averaged radio luminosity function in clusters of galaxies
• Observational constraint on dynamical evolution of dark energy
• Constraints on the Combined Models with $R^{2-q}$ Inflation and Viable $f(R)$ Dark Energy
• A minimal set of invariants as a systematic approach to higher order gravity models: Physical and Cosmological Constraints
• Inflation and CMB Anisotropy from Quantum Metric Fluctuations
• Primordial Gravitational Waves Measurements and Anisotropies of CMB Polarization Rotation
• U(1)_R-mediated supersymmetry breaking from a six-dimensional flux compactification
• Hard X-ray Bursts from Collapse of the Super Massive Stars
• The Atacama Cosmology Telescope: Delensed Power Spectra and Parameters
• QUIET - Measuring the CMB polarization with coherent detector arrays
• Dark matter annihilation and non-thermal Sunyaev-Zel'dovich effect: I. galaxy cluster
• Hidden Photons from the Sun
• Beyond the Standard Model for Montaneros
• The distribution of annihilation luminosities in dark matter substructure
• Minimal and non-minimal Universal Extra Dimension models in the light of LHC data at 13 TeV
• Inhomogeneous spacetimes in Einstein-æther Cosmology
• There is no vacuum zero-point energy in our universe for massive particles within the scope of relativistic quantum mechanics
• Computation of inflationary cosmological perturbations in chaotic inflationary scenarios using the phase-integral method
• Probing the Primordial Power Spectrum with Cluster Number Counts
• The impossibility of heavy neutrino dark matter in the Littlest Higgs Model with T-parity: constraints from direct search
• Contradiction between strong lensing statistics and a feedback solution to the cusp/core problem
• Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae
• Searching for Dark Matter- Theoretical Rates and Exclusion Plots due to the Spin
• New Constraints on Lorentz Invariance Violation from Combined Linear and Circular Optical Polarimetry of Extragalactic Sources
• Higher order terms in the inflaton potential and the lower bound on the tensor to scalar ratio r
• Foreground Maps in WMAP frequency bands
• The Big Bang as the Ultimate Traffic Jam
• The Origin of the X-ray Emission from the High-velocity Cloud MS30.7-81.4-118
• Local reionizations histories with merger tree of HII regions
• Evidence for evolving dark energy from DESI DR2 BAO and Pantheon${}^{+}$, DES-Dovekie, and Union3
• Warped Hybrid Inflation
• Estimating small angular scale CMB anisotropy with high resolution N-body simulations: weak lensing
• Realistic f(T) model describing the de Sitter epoch of the dark energy dominated universe
• Over-cooled haloes at z > 10: a route to form low-mass first stars
• High accuracy power spectra including baryonic physics in dynamical Dark Energy models
• Coupled scalar fields in the late Universe: The mechanical approach and the late cosmic acceleration
• An Interacting Scenario for Dark Energy in Bianchi Type-I Universe
• Improved Photometric Redshifts with Surface Luminosity Priors
• Axion cold dark matter revisited
• Dynamics of tachyon field in spatially curved FRW universe
• The potential of advanced ground-based gravitational wave detectors to detect generic deviations from general relativity
• Double SSA Spectrum and Magnetic Field Strength of the FSRQ 3C 454.3
• Cosmological acceleration from a gas of strings
• The Glow of Axion Quark Nugget Dark Matter: (I) Large Scale Structures
• Reheating in Chaotic D-Term Inflation
• Baryogenesis and Asymmetric Dark Matter from The Left-Right Mirror Symmetric Model
• Impact of the matter density uncertainty on the dark energy reconstruction
• New cosmological solutions in hybrid metric-Palatini gravity from dynamical symmetries
• Non-Gaussianities from isocurvature modes
• Power spectrum response of large-scale structure in 1D and in 3D: tests of prescriptions for post-collapse dynamics
• Angular momentum in cluster Spherical Collapse Model
• On SUSY GUTs with a degenerate Higgs mass matrix
• Bouncing Universe with a Nonminimally Coupled Scalar Field on a Moving Domain Wall
• Cosmological model dependence of the galaxy luminosity function: far-infrared results in the Lemaitre-Tolman-Bondi model
• One-loop contribution to the neutrino mass matrix in NMSSM with right-handed neutrinos and tri-bimaximal mixing
• Probing the cosmic acceleration from combinations of different data sets
• Comprehensive Analysis on the Light Higgs Boson Scenario
• Yet another sample of RFGC galaxies
• Probing Precise Location of Radio Core in TeV Blazar Mrk 501 with VERA at 43 GHz
• Phenomenological Consequences of Supersymmetric Theories from Dimensional Reduction and Reduction of Couplings
• Statistically significant length scale of filaments as a robust measure of galaxy distribution
• Implications of Higgs to diphoton decay rate in the bilinear R-parity violating supersymmetric model
• Adiabatic Media Inflation
• Comparing the Predictions of two Mixed Neutralino Dark Matter Models with the Recent CDMS II Candidate Events
• Multifrequency VLBI Observations of the Broad Absorption Line Quasar J1020+4320: Recently Restarted Jet Activity?
• A Pair of Early- and Late-Forming Galaxy Cluster Samples: a Novel Way of Studying Halo Assembly Bias Assisted by a Constrained Simulation
• Is a Dissipative Regime During Inflation in Agreement with Observations?
• Saas-Fee Lecture Notes: Multi-messenger Astronomy and Dark Matter
• Endowing $\mathbf{\Lambda }$ with a dynamic nature: constraints in a spatially curved Universe
• The five dimensional universal hypermultiplet and the cosmological constant problem
• The 21cm Signature of Early Relic \HII Regions
• Holographic dark energy at the Ricci scale
• Interpreting the HI 21-cm cosmology maps through Largest Cluster Statistics -- I: Impact of the synthetic SKA1-Low observations
• Can A Higgs Portal Dark Matter be Compatible with the Anti-proton Cosmic-ray?
• Gödel and Gödel-type solutions in the Palatini $f(R,T)$ gravity theory
• Constraints on the pMSSM from searches for squarks and gluinos by ATLAS
• Relics of spatial curvature in the primordial non-gaussianity
• The Halo Occupation Distribution of HI Galaxies
• The Ks-band Tully-Fisher Relation - A Determination of the Hubble Parameter from 218 ScI Galaxies and 16 Galaxy Clusters
• Testing Inflation: A Bootstrap Approach
• An Expanding Locally Anisotropic (ELA) Metric Describing Matter in an Expanding Universe
• The X-Ray Zurich Environmental Study (X-ZENS). II. X-ray Observations of the Diffuse Intragroup Medium in Galaxy Groups
• Constraints on cosmic birefringence using $E$-mode polarisation
• Tau neutrinos from ultracompact dark matter minihalos and constraints on the primordial curvature perturbations
• Observational constraints to a unified cosmological model
• The Degeneracy of Galaxy Formation Models
• Relative baryon-dark matter velocities in cosmological zoom simulations
• The primordial non-Gaussianity of local type (f_NL) in the WMAP 5-year data: the length distribution of CMB skeleton
• Equilibrium boundary conditions, dynamic vacuum energy, and the Big Bang
• A note on second-order perturbations of non-canonical scalar fields
• Testing the Nambu-Goldstone Hypothesis for Quarks and Leptons at the LHC
• Time Variable Cosmological Constant from Renormalization Group Equations
• Measuring H0 from the 6dF Galaxy Survey and future low-redshift surveys
• Inflation with a stringy minimal length, reworked
• Explosive particle production in non-commutative inflation
• B-L assisted Anomaly Mediation and the radiative B-L symmetry breaking
• Cosmological Model-independent Gamma-ray Bursts Calibration and its Cosmological Constraint to Dark Energy
• Ultra High Energy Neutrinos: Absorption, Thermal Effects and Signatures
• Improved Cosmological Parameter Constraints from CMB and H(z) Data
• Vortical Motions of Baryonic Gas in the Cosmic Web: Growth History and Scaling Relation
• Cluster contribution to the X-ray background as a cosmological probe
• Magnetic fields and Sunyaev-Zel'dovich effect in galaxy clusters
• Fast and Flexible Neutrino Decoupling Part I: The Standard Model
• Dark Matter Halos: The Dynamical Basis of Effective Empirical Models
• A Model of Four Generation Fermions and Cold Dark Matter and Matter-Antimatter Asymmetry
• A procedure for making high dynamic-range radio images: Deep imaging of the kiloparsec-scale radio structures of a distant blazar, NRAO 530, with JVLA data
• A spectroscopically confirmed z=1.327 galaxy-scale deflector magnifying a z~8 Lyman-Break galaxy in the Brightest of Reionizing Galaxies survey
• Non-Gaussianity in String Cosmology: A Case Study
• Analysis of recent type Ia supernova data based on evolving dark energy models
• Search for fast radio transients using Arecibo drift-scan observations at 1.4 GHz
• Can the coincidence problem be solved by a cosmological model of coupled dark energy and dark matter?
• CDMS II Inspired Neutralino Dark Matter in Flipped SU(5)
• Gravitational Wave Detection Using Redshifted 21-cm Observations
• Brane cosmology in the Horava-Witten heterotic M-Theory on $S^1/Z_2$
• Reconstructing matter profiles of spherically compensated cosmic regions in $\Lambda$CDM cosmology
• Non-universal SUGRA at LHC: Prospects and Discovery Potential
• Testing Dvali-Gabadadze-Porrati Gravity with Planck
• The magnitude-redshift relation in a realistic inhomogeneous universe
• Computation of the Power Spectrum in Chaotic $1/4\lambda {\varphi }^4$ Inflation
• Reheating constraints to modulus mass for single field inflationary models
• Conformal Inflation, Modulated Reheating, and WMAP5
• Probing Quintessence using BAO imprint on the cross-correlation of weak lensing and post-reionization HI 21 cm signal
• Distinguishing between inhomogeneous model and $\Lambda \text{CDM}$ model with the cosmic age method
• The Physics Case for Axions, WIMPs, WISPs and Other Weird Stuff
• D-term assisted Anomaly Mediation in E6 motivated models
• The curvaton scenario in Brane cosmology: model parameters and their constraints
• Constraining hybrid potential scalar field cosmological model in Lyra's geometry with recent observational data
• Cosmic Birefringence as a probe of dark matter nature: Sterile neutrino and dipolar dark matter
• Lambda-CDM and the WMAP power spectrum beam profile sensitivity
• Two active states of the narrow-line gamma-ray-loud AGN GB 1310+487
• Symmetries of Differential equations and Applications in Relativistic Physics
• Constraining Neutrinos and Dark Energy with Galaxy Clustering in the Dark Energy Survey
• Possible Anthropic Support for a Decaying Universe: A Cosmic Doomsday Argument
• The Impact of Non-Equipartition on Cosmological Parameter Estimation from Sunyaev-Zel'dovich Surveys
• Precision Cosmology from X-ray AGN clustering
• Affine Connections in Quantum Gravity and New Scalar Fields
• Multiple Main Sequence of Globular Clusters as a Result of Inhomogeneous Big Bang Nucleosynthesis
• Implication of Spatial and Temporal Variations of the Fine-Structure Constant
• Testing the Lorentz and CPT Symmetry with CMB polarizations and a non-relativistic Maxwell Theory
• Metal Enrichment and Reionization Constraints on Early Star Formation
• Primordial Nucleosynthesis After WMAP
• The follow-up EVN observations of twelve GPS radio sources at 5 GHz
• Estimates of unresolved point sources contribution to WMAP 5
• The near-infrared radiation background, gravitational wave background and star formation rate of Pop III and Pop II during cosmic reionization
• Quintessential Kination and Thermal Production of SUSY e-WIMPs
• A new signature of primordial non-Gaussianities from the abundance of galaxy clusters
• Estimation of the Hubble Constant and Constraint on Descriptions of Dark Energy
• Generalizing the ADM Computation to Quantum Field Theory
• Estimating the distribution of rest-frame timescales for blazar jets: a statistical approach
• Dark matter vorticity and velocity dispersion from truncated Dyson$\unicode{x2013}$Schwinger equations
• Expressing the equation of state parameter in terms of the three dimensional cosmic shear
• Short Gamma Ray Bursts as possible electromagnetic counterpart of coalescing binary systems
• Ratchet Model of Baryogenesis
• Electromagnetic Casimir densities for a cylindrical shell on de Sitter space
• Observational constraints using Bayesian statistics and Deep Learning in $f(Q)$ gravity
• Signature of short distance physics on inflation power spectrum and CMB anisotropy
• Reconstruction of the isocurvaton scenario
• Interacting Viscous Dark Energy in Bianchi Type-III Universe
• The coincidence problem in $f(R)$ gravity models
• Constraining Modified Gravity with Large non-Gaussianities
• Ionized bubble number count as a probe of non-Gaussianity
• Detecting unresolved moving sources in a diffuse background
• Deep CFHT Y-band Imaging of VVDS-F22 Field: II. Quasar Selection and Quasar Luminosity Function
• Neutrino Mass, Coupling Unification, Verifiable Proton Decay, Vacuum Stability and WIMP Dark Matter in SU(5)
• The torsion cosmology in Kaluza-Klein theory
• On the abundance of gravitational arcs produced by submillimeter galaxies at radio and submm wavelengths
• Reconstruction of the left-chiral tau-sneutrino in supersymmetry with a right-sneutrino as the lightest supersymmetric particle
• Dynamical system analysis in multiscalar-torsion cosmology
• Scalar Triplet Leptogenesis with a CP violating phase
• Constraints on pseudoscalar-photon interaction from CMB polarization observation
• Primordial black hole formation from non-Gaussian curvature perturbations
• Void or Dark Energy?
• Analysis of defect formation in semiconductor cryogenic bolometric detectors created by heavy dark matter
• Simultaneous determination of the cosmic birefringence and miscalibrated polarization angles II: Including cross frequency spectra
• Phenomenological Aspects of Gauge Mediation with Sequestered Supersymmetry Breaking in light of Dark Matter Detection
• Statistical and dynamical decoupling of the IGM from Dark Matter
• Constraints on the primordial gravitational waves with variable sound speed from current CMB data
• A Search for Neutron Star Precession and Interstellar Magnetic Field Variations via Multiepoch Pulsar Polarimetry
• Supernatural A-term Inflation
• Halo Density Profiles Consistent with Asymmetric M-B Velocity Distributions-Implications on Direct Dark Matter Searches
• The Connection between Radio and Gamma Ray Emission in Fermi/LAT Blazars
• Consistent cosmology with Higgs thermal inflation in a minimal extension of the MSSM
• On Semi-classical Degravitation and the Cosmological Constant Problems
• Non-linear Matter Spectrum for a Variable Equation of State
• Time parallel gravitational collapse simulation
• A gauge mediation scenario with hidden sector renormalization in MSSM
• Simulating Galaxy Clusters
• Cosmic Acceleration from Causal Backreaction in a Smoothly Inhomogeneous Universe
• Shapes of dark matter haloes with discrete globular cluster dynamics: The example of NGC 5128 (Centaurus A)
• A tentative derivation of the main cosmological parameters
• The viability of low-mass subhaloes as targets for gamma-ray dark matter searches
• Dynamical Oscillations in Dark Energy: Joint Constraints on the $w_{sin}$CDM Model from DESI, OHD, and Supernova Samples
• Distance-Redshift Relations in an Anisotropic Cosmological Model
• Crossing the cosmological constant barrier with kinetically interacting double quintessence
• Scaling of the 1-halo terms with bias
• Fermionic and scalar fields as sources of interacting dark matter-dark energy
• The Friedmann equations in deformed Hořava-Lifshitz gravity and Debye model
• A light Scalar Dark Matter for CoGeNT and DAMA in D_6 Flavor Symmetric Model
• $\Lambda$CDM and early dark energy in latent space: a data-driven parametrization of the CMB temperature power spectrum
• Gauge Mediated Supersymmetry Breaking in Five Dimensions
• Sunyaev-Zel'dovich observations of LoCuSS clusters with the Arcminute Microkelvin Imager: moderate X-ray luminosity sample
• A non-perturbative study of the evolution of cosmic magnetised sources
• The power spectrum of the cosmic microwave background Kolmogorov maps: possible clue to correlation of voids
• The R-axion and non-Gaussianity
• Optimal estimator for the amplitude of the bispectrum from IR sources
• Modified Dark Matter in Galaxies and Galaxy Clusters
• Magnetic contributions in Bekenstein type models
• Infrared divergence of pure Einstein gravity contributions to cosmological density power spectrum
• CP-phase effects on the effective neutrino mass $m_{ee}$ in the case of quasi-degenerate neutrinos
• Energy Conditions in Extended $f(R,G,T)$ Gravity
• Observational Constraints on Phantom Crossing DGP Gravity
• Using rates to measure mixed modulus-anomaly mediated supersymmetry breaking at the LHC
• Cosmological constraints on Lorentz invariance violation in the neutrino sector
• Probing the bias of radio sources at high redshift
• A CMB Gibbs sampler for localized secondary anisotropies
• A New Multi-Scale Structure Finding Algorithm to Identify Cosmological Structure
• Observational constraints on a Yang-Mills condensate dark energy model
• SUSY SU(5) $\times S_4$ GUT Flavor Model for Fermion Masses and Mixings with Adjoint, Large ${\theta }_{13}^{PMNS}$
• VLBI Imagings of Kilo-parsec Knot in 3C 380
• Dependence on the environment of the abundance function of light-cone simulation dark matter haloes
• Probing for Lorentz Invariance Violation in Pantheon Plus Dominated Cosmology
• Large-scale collective motion of RFGC galaxies in curved space-time
• WISDOM project -- XVIII. Molecular gas distributions and kinematics of three megamaser galaxies
• A class of regular bouncing cosmologies
• Bound to bounce: a coupled scalar-tachyon model for a smooth bouncing/cyclic universe
• Attractor Solutions in Tachyacoustic Cosmology
• Generalized particle dynamics in anti de Sitter spaces: A source for dark energy
• Cluster mass estimation through Fair Galaxies
• Dark Energy and Inflation from Gravitational Waves
• Effective cosmological constant from TeV-scale physics
• Renormalization Group Evolution of the Non-Unitary operator
• Experimental status of particle and astroparticle searches for supersymmetry
• Speakable and unspeakable in cosmology: dark matter vs. gravitational self energies. Hubble's constant, the cosmological term and all that
• Cosmological aspects of a vector field model
• Gauss-Bonnet Braneworld Cosmology with Modified Induced Gravity on the Brane
• The Carnegie Supernova Project II. Early observations and progenitor constraints of the Type Ib supernova LSQ13abf
• Multiplicity distributions in gravitational and strong interactions
• Detecting intermediate mass black holes in midiquasars with current and future surveys
• Lepton-number-violating decays of singly-charged Higgs bosons in the minimal type-(I+II) seesaw model at the TeV scale
• Direct determination of Neutrino Mass from Tritium Beta Spectrum
• Leptogenesis Scenarios via Non-Thermally Produced Right-handed Neutrino and Sneutrino in Supersymmetric Seesaw Model
• Weak lensing forecasts for dark energy, neutrinos and initial conditions
• Some aspects of neutrino mixing and oscillations
• Exact solutions in a scalar-tensor model of dark energy
• Large non-Gaussianity generated at the end of Extended D-term Hybrid Inflation
• Inverse Compton Scattering of the Central Source Photons as an X-ray Emission Mechanism on Kiloparsec Scales in PKS 1127-145
• Correlation between direct dark matter detection and Br(B_s -> mu mu) with a large phase of B_s - anti-B_s mixing
• Propagating Uncertainties in the SALT3 Model Training Process to Cosmological Constraints
• Large-scale magnetic fields from inflation in teleparallel gravity
• Kickstarting Reionization with the First Black Holes: the effects of second-order perturbation theory in pre-reionization volumes
• Decomposition of linear metric perturbations on generic background spacetime -- Toward higher-order general-relativistic gauge-invariant perturbation theory
• Inflation of Universe by Nonlinear Electrodynamics
• Reconstructions of Einstein-Aether Gravity from Barrow Agegraphic and New Barrow Agegraphic Dark Energy models: Examinations and Observational Limits
• Constraining cosmology with thermal Sunyaev-Zel'dovich maps: Minkowski functionals, peaks, minima, and moments
• Degree of randomness: numerical experiments for astrophysical signals
• Magnetized matter effects on dilaton photon mixing
• Cluster formation and the Sunyaev-Zel'dovich power spectrum in modified gravity: the case of a phenomenologically extended DGP model
• Unification Predictions With or Without Supersymmetry
• Primordial vorticity and gradient expansion
• $k$-essence for warm inflation on the brane
• Correlation between flavour violating decay of long-lived slepton and tau in the coannihilation scenario with Seesaw mechanism
• Geometric Tachyon and Warm Inflation
• Effect of Priomordial non-Gaussianities on Galaxy Clusters Scaling Relations
• Dark Matters in Gauged B-3L_i Model
• Quasi-degenerate Neutrino mass models and their significance: A model independent investigation
• Spinor quintom cosmology with intrinsic spin
• Dark Matter in SuperGUT Unification Models
• Slow-roll Natural & Hilltop Inflation in Rastall Gravity
• Realistic Four-Generation MSSM in Type II String Theory
• Non-relativistic Matrix Inflation
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• DBI Lifshitz Inflation
• Testing Gaussianity in the WMAP data of OT foreground reduced map
• On the prior dependence of constraints on the tensor-to-scalar ratio
• The Sunyaev-Zel'dovich effect due to hyper-starburst galaxy winds
• Schwarzschild and de Sitter solutions from the argument by Lenz and Sommerfeld
• On the Detectability of the Hydrogen 3-cm Fine Structure Line from the EoR
• Mass Varying Neutrinos in Supernovae
• A Brachistochrone Approach to Reconstruct the Inflaton Potential
• How Future Space-Based Weak Lensing Surveys Might Obtain Photometric Redshifts Independently
• Asymptotically Static Universe
• Holographic unification of dark matter and dark energy
• The Abnormally Weighting Energy Hypothesis: The origin of the cosmic acceleration
• Spontaneous parity breaking and supersymmetry breaking in metastable vacua with consistent cosmology
• Dark matter, mu problem and neutrino mass with gauged R-symmetry
• The Hubble constant and dark energy
• Radiative corrections to neutralino annihilation: Recent developments
• Particle asymmetries in the early universe
• On the cosmological viability of the Hu-Sawicki type modified induced gravity
• Constraints on Decaying Dark Matter
• Scalar Field, Four Dimensional Spacetime Volume and the Holographic Dark Energy
• Multiple Lorentz groups - a toy model for superluminal muon neutrinos
• Axions in Cold Dark Matter and Inflation Models
• Gluino, wino and Higgsino-like particles without supersymmetry
• Detection of CO(J=1-0) Emission from Barred Spiral Galaxies at z~0.1
• Gravitino dark matter with neutralino NLSP in the constrained NMSSM
• Moderate Galaxy-Galaxy Lensing
• Implications of SUSY Searches at the LHC for the ILC
• Constraining decaying dark energy density models with the CMB temperature-redshift relation
• Coincidence Problem in Cyclic Phantom Models of the Universe
• The inhomogeneous equation of state and the road towards the solution of the cosmological constant problem
• Higher order spectra from an initially anisotropic universe
• Effects of Variable Newton Constant During Inflation
• A model of the anisotropic correlation function xi(rp, pi) in redshift space including redshift errors
• Thermodynamics in Little Rip cosmology in the framework of a type of f(R,T) gravity
• CP Violating Asymmetry in Stop Decay into Bottom and Chargino
• Compactification driven Hilltop Inflation in Einstein-Yang-Mills
• Particle-antiparticle asymmetry from magnetogenesis through the Landau mechanism
• Growth of matter perturbations for realistic $F(R)$ models
• Non-adiabatic primordial fluctuations
• The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIRE
• Measuring the Hubble Constant with the Hubble Space Telescope
• Supersymmetry after the Higgs discovery and its LHC phenomenology
• Delayed Enrichment by Unseen Galaxies: Explaining the Rapid Rise in IGM CIV Absorption from z = 6-5
• Type Ia supernovae and the acceleration of the universe: results from the ESSENCE Supernova Survey
• Simulations and Observations of the Microwave Universe
• Testing cosmological models with the brightness profile of distant galaxies
• Single Past Null Geodesic in the Lemaitre-Tolman-Bondi Cosmology
• Power-law expansion and Higgs-type potential in a scalar-tensor model
• 'Constraint consistency' at all orders in Cosmological perturbation theory
• Gauss Bonnet dark energy Chaplygin Gas Model
• A general method for the construction of stable Galileon models consistent with the Planck data results
• A numerical study of primordial magnetic field amplification by inflation-produced gravitational waves
• Constraining Extended Reionization Models Through Arcminute-Scale CMB Measurements
• Warm Ekpyrosis
• Non-Gaussianity in the HILC foreground-reduced three-year WMAP CMB map
• Cosmic evolution with a general Gaussian type scale factor
• Modelling the environmental dependence of the growth rate
• Constraining Chaplygin models using diffuse supernova neutrino background
• Influence of the correlation prior on reconstruction of the dark energy equation of state
• Cosmology in a model with Lagrange multiplier, and Gauss-Bonnet and non-minimal kinetic couplings
• Exact Solutions and Constraints on the Dark Energy Model in FRW Universe
• An overview of the current status of CMB observations
• Reconstructing the Peculiar Velocity of the Local Group with Modified Gravity and 2MASS
• Measuring galaxy abundance and clustering at high redshift from incomplete spectroscopic data: Tests on mock catalogs
• Mixed perturbations from an Inflaton and Two Curvatons - towards understanding non-gaussianity in more complicated curvaton scenarios
• Dependence of the dynamical properties of light-cone simulation dark matter halos on their environment
• Direct Detection of the Primordial Inflationary Gravitational Waves
• Hubble Space Telescope Captures UGC~12591: Bulge/Disc Properties, Star Formation and `Missing Baryons' Census in a Very Massive and Fast Spinning Hybrid Galaxy
• Machine-guided Exploration and Calibration of Astrophysical Simulations
• Vacuum polarization by a scalar field in de Sitter spacetime in the presence of global monopole
• Large non-Gaussianity generated after D-term Inflation by Right-Handed Sneutrino Curvaton
• Gravitational Lensing of Dark Energy Models and $\Lambda$CDM Using Observational data in Loop Quantum Cosmology
• Studies of stationary features in jets: BL Lacertae II. Trajectory reversals and superluminal speeds on sub-parsec scales
• Soft X-ray excess of clusters: a thermal filament model, and the strong lensing of background galaxy groups
• Barions and $\Lambda$CDM Model Problems
• Jet formation studies in AGN: a search for new targets
• A helical magnetic field in quasar NRAO150 revealed by Faraday rotation
• Integral field spectroscopy with SINFONI of VVDS galaxies. I. Galaxy dynamics and mass assembly at 1.2 < z < 1.6
• CMB constraints on noncommutative geometry during inflation
• Nearly Full-Sky Low-Multipole Cosmic Microwave Background Temperature Anisotropy: III. CMB Temperature Anomalies
• Hubble Tension and Dark Energy in Teleparallel Gauss-Bonnet Gravity: New Constraints from DESI BAO, Pantheon${}^{+}$ and Hubble Data
• Anisotropic cosmology using observational datasets: exploring via machine learning approaches
• Observational constraints in late time for an axially symmetric transitioning model with bulk viscous fluid
• The Simons Observatory: Design, Optimization, and Performance of Low Frequency Detectors
• FBQ 0951+2635: time delay and structure of the main lensing galaxy
• Can MONDian vector theories explain the cosmic speed up ?
• Neutrino Masses, Dark Energy and the Gravitational Lensing of Pregalactic HI
• Active galactic nucleus feedback in NGC 3982
• Is non-particle dark matter equation of state parameter evolving with time?
• Cluster density slopes from Dark Matter-Baryons Energy Transfer
• Current observational constraints on holographic dark energy model
• Is cosmology just a plausibility argument?
• $\Lambda CDM$ periodic cosmology
• NESSiE: The Experimental Sterile Neutrino Search in Short-Base-Line at CERN
• A New Approach to Testing Dark Energy Models by Observations
• Dynamical analysis for a scalar-tensor model with Gauss-Bonnet and non-minimal couplings
• Gravitational interaction of celestial bodies and black holes with particle dark matter
• Mapping possible non-Gaussianity in the Planck maps
• Light Higgs boson scenario in the SUSY seesaw model
• Muon (g-2) from the bulk neutrino field in a warped extra dimensional model
• Supernovae at the cosmic dawn
• Parameterizing the flattening of galaxies rotation curves on an expanding locally anisotropic background
• Dark Matter Isocurvature from Curvature
• On the evolution of Betti curves in the Cosmic web
• Probability distribution and statistical properties of spherically compensated cosmic regions in $\Lambda$CDM cosmology
• Cosmological constraints on parameters of one-brane models with extra dimension
• Axi-Higgs portal Dark Matter via Wess-Zumino mechanism
• The connection between cosmology and neutrino physics
• The Size of Local Bispectrum and Trispectrum in a Non-Minimal Inflation
• Method for Determining AGN Accretion Phase in Field Galaxies
• The effect of the cosmological constant on gravitational wave quadrupole signal
• Quinstant Dark Energy Predictions for Structure Formation
• Dark Matter Internal Pair Production -- A Novel Direct Detection Mechanism
• A Proposal for Constraining Initial Vacuum by CMB
• Axion hot dark matter bounds
• Cosmological correlation functions in scalar and vector inflationary models
• Helical magnetic field structure in 3C 273. A Faraday rotation analysis using multi-frequency polarimetric VLBA data
• Sunyaev-Zel'dovich contribution in CMB analysis
• Relativistic stars in $f(Q)$-gravity: Exact analytic solution for the power-law case $f(Q)=Q+b{Q}^{\nu }$
• The Infancy of Cosmic Reionization
• The Cosmic Evolution of CIV Absorbers at $1.4<z<4.5$: Insights from $100,000$ Systems in DESI Quasars
• Implications of pulsar timing arrays for Gauss-Bonnet Inflation
• Emergent Universe as an interaction in the dark sector
• Geometric sigma model of the Universe
• Anomalies, U(1)' and the MSSM
• Relic density and future colliders: inverse problem(s)
• Degeneracy and Discreteness in Cosmological Model Fitting
• QCD-scale modified-gravity universe
• Unified Brane Gravity: Cosmological Dark Matter from Scale Dependent Newton Constant
• Observational constraints on thawing quintessence scalar field model
• Coupled fluids model in FRW space-time
• Photo-z optimization for measurements of the BAO radial direction
• A class of transient acceleration models consistent with Big Bang Cosmology
• Direct and Indirect Detection of Neutralino Dark Matter and Collider Signatures in an $SO(10)$ Model with Two Intermediate Scales
• Inflation and Preheating in Supergravity with MSSM Flat Directions
• Cosmological dynamics with modified induced gravity on the normal DGP branch
• A simulation experiment of a pipeline based on machine learning for neutral hydrogen intensity mapping surveys
• The Virtues of Frugality - Why cosmological observers should release their data slowly
• Constraint on the growth factor of the cosmic structure from the damping of the baryon acoustic oscillation signature
• Observable predictions of generalised inflationary scenarios
• Dark aspects of massive spinor electrodynamics
• Conservation Laws in Gravitation and Cosmology
• An Optimal and Model-Independent Measurement of the Intracluster Pressure Profile I: Methodology and First Applications
• The inhomogeneous equation of state and the speed of convergence to a small cosmological constant
• Metallicity and kinematical clues to the formation of the Local Group
• Inverse Compton gamma-rays from Galactic dark matter annihilation: Anisotropy signatures
• Particle Dark Matter: the state of the art
• Cosmo-Particle Searches for Supersymmetry at the Collider Detector at Fermilab
• Effective Theories and Modifications of Gravity
• Higgs mass from cosmological and astrophysical measurements
• Observable Gravitational Waves and Spectral Index Running in Small Single Field Inflationary Models
• A worldsheet perspective on string inflation
• Recent Progress in Formal Theory
• Gamma Ray and Neutrino Flux from Annihilation of Neutralino Dark Matter at Galactic Halo Region in mAMSB Model
• Planetary motion on an expanding locally anisotropic background
• Dark matter as a localized scalar in the extra dimension
• Exact solution and exotic fluid in cosmology
• Curvaton decay into relativistic matter
• Braneworlds with timelike extra-dimension
• Spectator stresses and CMB observables
• Finite scale factor and future singularities
• Non-oscillation probes of neutrino masses
• Constraints on scalar-tensor theories from observations
• Explanations of the DAMPE high energy electron/positron spectrum in the dark matter annihilation and pulsar scenarios
• Possible origin of CMB temperature fluctuations: Vacuum fluctuations of Kaluza-Klein and string states during inflationary era
• Cosmographic applications of Gamma Ray Bursts
• Tracking Quintessence, WIMP Relic Density, PAMELA and Fermi LAT
• Approximate $w_{\varphi }\sim {\Omega }_{\varphi }$ Relations in Quintessence Models
• On the Viability of a Non-Analytical f(R)-Theory
• Cascade Hierarchy in SUSY SU(5) GUT
• Li isotopes in metal-poor halo dwarfs, a more and more complicated story
• Dark matter in natural supersymmetric extensions of the Standard Model
• New frontiers in Numerical Relativity
• Calculating a confidence interval on the sum of binned leakage
• Zero Cosmological Constant and Nonzero Dark Energy from Holographic Principle
• The degenerate scenario in the NMSSM: Direct singlino-like neutralino searches with a gravitino LSP
• M-flation and its spectators
• Supersymmetry Signals at the LHC under the most favorable SUGRA scenario
• Models for the Clustering of Far-Infrared and Sub-millimetre selected Galaxies
• Modelling non-Gaussianity from foreground contaminants
• Effective Field Theory for Inflation
• Simple Model of Propagating Flame Pulsations
• Galaxy Rotation Curves from String Theory
• Classical, quantum, and phenomenological aspects of dark energy models
• Noether symmetry approach in non-minimal derivative coupling gravity
• Dark Energy Survey Year 3 Results: Galaxy mock catalogs for BAO analysis
• GRBs luminosity function synthesized from \textit{Swift/BAT}, \textit{Fermi/GBM} and \textit{Konus-Wind} data
• SU(5) unification of two triplet seesaw and leptogenesis with dark matter and vacuum stability
• Constraints on Multicomponent Dark Energy from Cosmological Observations
• Confronting Grand Unification with Lepton Flavour Violation, Dark Matter and LHC Data
• Collins in Wonderland
• CMB delensing with deep learning
• Generalized Semi-Holographic Universe
• Impact of SUSY-QCD corrections on neutralino-stop co-annihilation and the neutralino relic density
• Effects of Multi-Field Phantom Inflation in Big Rip
• The Quantum Origin of Cosmic Structure
• Dark Energy and Dark Matter
• How accurately is the property of the Little Higgs Dark Matter determined at the ILC?
• O-V-S-Z and friends: Non-Gaussianity from inhomogeneous reionization
• Correlations in the matter distribution in CLASH galaxy clusters
• Shedding Light on the Symmetries of Dark Matter
• Confronting SUSY GUT with Dark Matter, Sparticle Spectroscopy and Muon $(g-2)$
• Physics requirements for Scalar Muons searches at CLIC
• Searching for Particle Physics Beyond the Standard Model at the LHC and Elsewhere
• Isochronous solutions of Einstein's equations and their Newtonian limit
• Inflation and Cosmological Constant
• Triplet scalar flavored leptogenesis with spontaneous CP violation
• Cosmological Constraints on a Massive Neutrino
• A Nonminimal Coupling Model and its Short-Range Solar System Impact
• Bianchi type-III THDE quintessence model with hybrid expansion law
• CMB polarization induced by stochastic magnetic fields
• Anomalous Lorentz and CPT violation
• Consistency relations between the source terms in the second-order Einstein equations for cosmological perturbations
• Long-wavelength gravitational waves and cosmic acceleration
• Constraining fast-roll inflation
• Reheating Temperature after Inflation in No-Scale Supergravity
• Observational constraints on massive gravity
• Experimental and Theoretical Evidence for Extended Particle Models
• Cluster number counts in quintessence models
• Symmetry restoration due to preheating and lepton number asymmetry
• The Active Universe
• Initial Conditions in the Effective Field Theory of Inflation
• Holographic Dark Energy with Torsion
• Orbifold construction of the modes of the Poincare dodecahedral space
• Racetrack Inflation and Cosmic Strings
• Perturbation Theory Remixed II: Improved Modeling of Nonlinear Bispectrum
• EUROnu-WP6 2010 Report
• Dilatonic Inflation, Gravitino and Reheating in Modified Modular invariant Supergravity
• Constraining primordial non-Gaussianity using Neural Networks
• SO(4,1) Yang-Mills theory of quantum gravity
• Adiabatic fluctuations from cosmic strings in a contracting universe
• Geometry vs growth: Internal consistency of the flat ΛCDM model with KiDS-1000
• How large is the contribution of cosmic web to ${\Omega }_{\Lambda }$ ? A preliminary study on a novel inhomogenous model
• Exploring the Latest Pantheon SNIa Dataset by Using Three Kinds of Statistics Techniques
• Neutrino masses and the Cabibbo expansion
• Minimal Lepton Flavor Violation and Renormalization Group Evolution of Lepton Masses and Mixing
• Accelerating Universe from Modified Kasner Model in Extra Dimensions
• Cosmic Four-Fermion Neutrino Secret Interactions, Enhancement and Total Cross Section
• A Toy Model For Single Field Open Inflation
• On the universality of the halo mass function beyond $\Lambda$CDM cosmology
• Impact on Astrophysics and Elementary Particle Physics of recent and future solar neutrino data
• Identification of new physics and general WIMP search at the ILC
• Constraining the expansion history of the universe from the red shift evolution of cosmic shear
• Fomin's conception of quantum cosmogenesis
• Muons from Neutralino Annihilations in the Sun: Flipped SU(5)
• Adaptive friends-of-friends algorithm for identifying gravitationally bound cosmological structures
• Model Independent Constraints on Solar Neutrinos
• Remarks on non-gaussian fluctuations of the inflaton and constancy of ζoutside the horizon
• Direct neutralino searches in the NMSSM with gravitino LSP in the degenerate scenario
• Structure Formation independent of Cold Dark Matter
• "Ab initio" models of galaxy formation: successes and open problems
• Where galaxies really come from
• Towards the unification of late-time acceleration and inflation by k-essence model
• SUSY Enhancement of Heavy Higgs Production
• Cluster optical depth and pairwise velocity estimation using machine learning
• Inverse Compton Scattering of Radiation from a Central Source as a Possible Mechanism for the Formation of X-Ray Radiation from Kiloparsec Jets of Core-Dominated Quasars
• Analytic expressions for the kinetic decoupling of WIMPs
• Status of Constraints on Supersymmetry
• Gamma rays from dark matter
• Studies of stationary features in jets: 3C 279 quasar I. On-sky scattering and dynamics
• Gravitational potential wells and the cosmic bulk flow
• Generalized Second Law of Thermodynamics on the Event Horizon for Interacting Dark Energy
• Observational constraints on inflation with the nonlinear sigma fields in light of Plank 2015
• Chandra Studies of the X-ray Gas Properties of Fossil Systems
• Gravitino dark matter in the constrained next-to-minimal supersymmetric standard model with neutralino next-to-lightest superpartner
• CMB two- and three-point correlation functions from Alfvén waves
• On the four-dimensional effective theories in brane-worlds
• Dynamical suppression of non-adiabatic modes
• Cosmological bootstrap
• Possible Bubbles of Spacetime Curvature in the South Pacific
• Dark energy constraints and correlations with systematics from CFHTLS weak lensing, SNLS supernovae Ia and WMAP5
• Long-Range Models of Modified Gravity and Their Agreement with Solar System and Double Pulsar Data
• Soft supersymmetry breaking with tiny cosmological constant in flux compactified N=1 Supergravity
• Holographic Ricci DE as running vacuum with nonlinear interactions
• Measuring CMB non-Gaussianity as a probe of Inflation and Cosmic Strings
• High precision spectra at large redshift for dynamical DE cosmologies
• Have we found conclusive evidence for dark matter through direct detection experiments?
• From WMAP to Planck: Exact reconstruction of 4- and 5-dimensional inflationary potential from high precision CMB measurements
• Spinor-Unit Field Representation of Electromagnetism Applied to a Model Inflationary Cosmology
• Cosmological constraints on the big bang quantum cosmology model
• "Observing and Analyzing" Images From a Simulated High Redshift Universe
• Viable f(R) gravity and future cosmological evolution
• Intermittence of the Map of Kinetic Sunyaev-Zel'dovich Effect and Turbulence of IGM
• Curvaton reheating and intermediate inflation in brane cosmology
• Lagrangian-space Gaussian ansatz for the matter redshift-space power spectrum and correlation function
• Minicharged Particle Sensitivity of the MAPP Outrigger Detector
• The holographic principle and the cosmological constant
• Cosmological perturbation theory with trinity of scalar fields
• Suppression of galactic outflows by cosmological infall and circumgalactic medium
• Interpreting the HI 21-cm cosmology maps through Largest Cluster Statistics. Part II. Impact of the realistic foreground and instrumental noise on synthetic SKA1-Low observations
• Ringing Non-Gaussianity from inflation with a step in the second derivative of the potential
• Identification of high-redshift X-ray active galactic nuclei in the 4XMM-DR11 serendipitous catalogue using DES data: Comparative analysis with optically-selected QSOs
• The Primordial Magnetic Field (PMF) Generated in Large Field Inflation (LFI), Natural Inflation (NI) and $R^2$-Inflation by $f^{2}FF$ Model
• Matter Field, Dark Matter and Dark Energy
• Baryogenesis from a CP-violating inflation
• Precision Measurements of the model parameters in the Littlest Higgs model with T-parity
• MOND's Problem in Local Group
• Machine learning analysis of Photometric data from the Dark Energy Survey
• Is the $\Lambda$CDM Model in Crisis?
• Retrofitting Models of Inflation
• The stability of the de-Sitter universe in nonlocal gravity
• Forecasts of constraining isotropic cosmic birefringence on AliCPT-1
• Measurement of Heavy Gauge Bosons in Little Higgs Model with T-parity at ILC
• An extended Higgs sector for neutrino mass, dark matter and baryon asymmetry
• Tracing the evolution of brightest galaxies and diffuse light in galaxy groups
• "An Era of Precision Astrophysics: Connecting Stars, Galaxies and the Universe," an Astro2010 Science White Paper
• Similar Fermi-GBM sGRBs to GW/sGRB 170817A in MeV-GeV energies
• Large-angle non-Gaussianity in simulated high-resolution CMB maps
• Manifestations of String Theory in Astrophysical Data and at the LHC
• FlowSN: Neural Simulation-Based Inference under Realistic Selection Effects applied to Supernova Cosmology
• A Ring of Fire Orphan γ-Ray Flare in the Neutrino Candidate 3C 120
• CP Violation in Dual Dark Matter
• Millimeter VLBI constraints on the central magnetic field and symmetric jet production in the twin-jet galaxy NGC 1052
• The Higgs Sector and CoGeNT/DAMA-Like Dark Matter in Supersymmetric Models
• Cosmology in the presence of diffeomorphism-violating, nondynamical background fields
• Structure formation in a non-canonical scalar field model of clustering dark energy
• $\Lambda$CDM, $\Lambda$DGP and extended phantom-like cosmologies
• The violent Universe: the Big Bang
• Cosmological signatures of brane inflation
• Energy conditions and entropy density of the universe
• Measurements of the model parameter in the littlest Higgs model with T-parity
• Electromagnetic Origin for Planck Mass and Dark Energy
• Some Aspects of New CDM Models and CDM Detection Methods
• A heuristic solution for the Pioneer anomaly employing an ELA metric with dark matter in the outskirts of the Solar system
• A novel test of Lorentz violation in the photon sector with an LC circuit
• Coupling dark-baryonic matter density profile for vacuum decay scenarios
• A possible explanation for NuTeV's anomalous dimuon events
• Simulation study of ZHAH mode in Littlest Higgs Model with T-Parity
• Elliptic solutions of generalized Brans-Dicke gravity with a non-universal coupling
• The inner regions of disk galaxies: a constant baryonic fraction?
• Large-Angle Anomalies in the Microwave Background
• Generating Gravitational Waves After Inflation
• Constraining the Charged Higgs Mass in the MSSM: A Low-Energy Approach
• Dark Matter and Electroweak Symmetry Breaking from $SO(10)$
• Possible consistent extra time dimensions in the early universe
• Analysis of Little Higgs Model with T-parity at ILC
• The effect of the curvature-scalar mixing on the annihilation cross sections of dark matter scalar and unparticle dark matter
• Breaking down the link between luminous and dark matter in massive galaxies
• The Standard-smooth Variant of Hybrid Inflation
• Asymmetry and non-random orientation of the inflight effective beam pattern in the WMAP Data
• Scaling Relations Between Low-mass Black Holes and Their Host Galaxies
• Discrete dark matter mechanism
• How dark matter cares about topological superstrings
• Prospects of Focus Point Supersymmetry for Snowmass 2013
• Annihilation cross sections and interaction couplings of the dark matter candidates in the warped and flat extra dimensions
• Neutrinos from the Early Universe and Physics Beyond Standard Models
• Identifying changing jets through their radio variability
• Developments in Leptogenesis
• Loop Quantum Cosmology on a Torus
• Characteristic Scales of Initial Density and Velocity Fields
• Physical vacuum as the source of the standard model particle masses
• The limits of cosmology
• Theory MOND in a Friedmann-Robertson-Walker Cosmology as alternative to the Nonbaryonic Dark Matter paradigm
• Dynamical dark energy and variation of fundamental "constants"
• Nature of Clustering of Large Scale Structures
• Applied Nanofabrication for X-ray Grating Spectroscopy
• High-Energy Neutrino Production in Clusters of Galaxies
• Chaotic inflation on the Randall-Sundrum 2-brane model
• Quantum gravity and mass of gauge field: a four-dimensional unified quantum theory
• Susy Seesaw Inflation and NMSO(10)GUT
• On the absence of a universal surface density, and a maximum Newtonian acceleration in dark matter haloes: consequences for MOND
• A Chi-Squared Analysis of the Measurements of Two Cosmological Parameters Over Time
• Neutralino dark matter with a Light Higgs
• Detecting relic gravitational waves in the CMB: A statistical bias
• Cosmological solutions of Tensor-Vector theories of gravity with varying the space-time-matter coupling constant
• Integrated Markov Chain Monte Carlo (MCMC) analysis of primordial non-Gaussianity (f_NL) in the recent CMB data
• Asymmetry at LHC for an U(1)' anomalous extension of MSSM
• Minimal gauge inflation
• Effective Approaches in and Beyond the MSSM : applications to Higgs Physics and Dark Matter observables
• Fundamental physics in observational cosmology
• Early Universe: inflation and cosmological perturbations
• Effects of Radiation on Primordial Non-Gaussianity
• Modified Power law Inflation: solution to the graceful exit problem and improvement of dark energy models
• The Mystery of Parity
• Primordial density fluctuations generated by wormholes
• Higgs, di-Higgs and tri-Higgs production via SUSY processes at the LHC with 14 TeV
• A Mass Dependent Density Profile from Dwarfs to Clusters
• $\Lambda$CDM-like models with future singularities
• Phase space analysis of Rényi Holographic dark energy model
• Dark Matter Experimental Overview
• Isocurvature Constraints and Gravitational Ward Identity
• Probing the correlations in composite signals
• Confidence Level Estimator for cosmological model (Research Note)
• Unstable Axion Quintessence Revisited
• Beyond the power spectrum: primordial and secondary non-Gaussianity in the microwave background
• A New Strategy For Solving Two Cosmological Problems in Hadron Physics
• Spontaneous Symmetry Breaking Vacuum Energy in Cosmology
• Non-Gaussianity and finite length inflation
• Non-canonical scalar field in low anisotropy universe with intermediate inflation
• On the validity of cosmic no-hair conjecture in an anisotropic inflationary model
• Gravitino Production after Inflation in No-Scale Supergravity
• Non-Gaussian Distribution and Clustering of Hot and Cold Pixels in the WMAP Five-Year Sky
• Unweaving the Fabric of the Universe: The Interplay between Mathematics and Physics
• 30 parameter version of the MSSM in light of the $B_s\to {\mu }^{+}{\mu }^{-}$ observation
• Light and compressed gluinos at the LHC via string theory
• Upper limits on Einstein's weak equivalence principle placed by uncertainties of dispersion measures of fast radio bursts
• The Invisible Tension of the Universe from Astrophysical Black Holes: a Solution to the Coincidence Problem of the Accelerated Expansion
• Linearized Treatment of Scalar perturbations in the Asymptotic Cosmological Model
• Phase space analysis and cosmography of a two-fluid cosmological model
• Probing the innermost regions of AGN jets and their magnetic fields with RadioAstron. V. Space and ground millimeter-VLBI imaging of OJ 287
• Supersymmetry Breaking and Gravitino Production after Inflation in Modular Invariant Supergravity
• Looking up at seesaw and GUT scales from TeV
• A revisited Correction to the Halo Mass Function for local-type Primordial non-Gaussianity
• Does gravity prefer the Poincare dodecahedral space?
• Electromagnetic vacuum stresses and energy fluxes induced by a cosmic string in de Sitter spacetime
• An Adynamical, Graphical Approach to Quantum Gravity and Unification
• Flavor Mixing Phenomenology in Supersymmetric Models
• Studying the spectral properties of Active Galactic Nuclei in the JWST era
• Casting Light on Dark Matter