Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data

Abstract

This paper focuses on cosmological constraints derived from analysis of WMAP data alone. A simple LCDM cosmological model fits the five-year WMAP temperature and polarization data. The basic parameters of the model are consistent with the three-year data and now better constrained: Omega_b h^2 = 0.02273+-0.00062, Omega_c h^2 = 0.1099+-0.0062, Omega_L = 0.742+-0.030, n_s = 0.963+0.014- 0.015, tau = 0.087+-0.017, sigma_8 = 0.796+-0.036. With five years of polarization data, we have measured the optical depth to reionization, tau>0, at 5 sigma significance. The redshift of an instantaneous reionization is constrained to be z_reion = 11.0+-1.4 with 68% confidence. This excludes a sudden reionization of the universe at z=6 at more than 3.5 sigma significance, suggesting that reionization was an extended process. Using two methods for polarized foreground cleaning we get consistent estimates for the optical depth, indicating an error due to foreground treatment of tau~0.01. This cosmological model also fits small-scale CMB data, and a range of astronomical data measuring the expansion rate and clustering of matter in the universe. We find evidence for the first time in the CMB power spectrum for a non-zero cosmic neutrino background, or a background of relativistic species, with the standard three light neutrino species preferred over the best-fit LCDM model with N_eff=0 at >99.5% confidence, and N_eff > 2.3 (95% CL) when varied. The five-year WMAP data improve the upper limit on the tensor-to-scalar ratio to r < 0.43 (95% CL), for power-law models. With longer integration we find no evidence for a running spectral index, with dn_s/dlnk = -0.037+-0.028.

49 pages, 18 figures, version accepted by ApJS. Original Section 2 moved to separate paper. For higher quality figs, see version on http://lambda.gsfc.nasa.gov

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• Cold flows and the first quasars
• Planck 2015 results. X. Diffuse component separation: Foreground maps
• Extreme Feedback and the Epoch of Reionization: Clues in the Local Universe
• Dynamics of interacting dark energy
• The primordial abundance of 4He: evidence for non-standard big bang nucleosynthesis
• Can Neutron stars constrain Dark Matter?
• The Observed Growth of Massive Galaxy Clusters II: X-ray Scaling Relations
• On the redshift-evolution of the Lyman-alpha escape fraction and the dust content of galaxies
• Semi-Analytic Galaxy Evolution (SAGE): Model Calibration and Basic Results
• Searching for modified growth patterns with tomographic surveys
• A lower bound on the mass of Dark Matter particles
• Improved measurements of the temperature and polarization of the CMB from QUaD
• Signatures of intrinsic Li depletion and Li-Na anti-correlation in the metal-poor globular cluster NGC6397
• Radiation pressure from massive star clusters as a launching mechanism for super-galactic winds
• Constraining Asymmetric Dark Matter through observations of compact stars
• Constraining the Milky Way's Hot Gas Halo with OVII and OVII Emission Lines
• Cosmology and Astrophysics from Relaxed Galaxy Clusters II: Cosmological Constraints
• The neutron and its role in cosmology and particle physics
• Fibre Inflation: Observable Gravity Waves from IIB String Compactifications
• The metal-poor end of the Spite plateau. 1: Stellar parameters, metallicities and lithium abundances
• Cosmological Constraints from a Combination of Galaxy Clustering and Lensing -- I. Theoretical Framework
• Planck intermediate results. XLVII. Planck constraints on reionization history
• Primordial Black Holes as All Dark Matter
• Damped Lyman Alpha Systems in Galaxy Formation Simulations
• A quantitative explanation of the observed population of Milky Way satellite galaxies
• The MICE Grand Challenge Lightcone Simulation I: Dark matter clustering
• Estimators for CMB Statistical Anisotropy
• Dark Radiation constraints on minicharged particles in models with a hidden photon
• Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes
• Big Bang Nucleosynthesis as a Probe of New Physics
• The cluster gas mass fraction as a cosmological probe: a revised study
• The impact of priors and observables on parameter inferences in the Constrained MSSM
• Do Hot Haloes Around Galaxies Contain the Missing Baryons?
• Simulations of the Microwave Sky
• Impact of Cluster Physics on the Sunyaev-Zel'dovich Power Spectrum
• The Contribution of High Redshift Galaxies to Cosmic Reionization: New Results from Deep WFC3 Imaging of the Hubble Ultra Deep Field
• On the Stellar Populations and Evolution of Star-Forming Galaxies at 6.3 < z < 8.6
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Foreground Emission
• ACTPol: A polarization-sensitive receiver for the Atacama Cosmology Telescope
• Massive hidden photons as lukewarm dark matter
• Generalised constraints on the curvature perturbation from primordial black holes
• Dark coupling
• Moving mesh cosmology: numerical techniques and global statistics
• General Relativity and Cosmology: Unsolved Questions and Future Directions
• A robust sample of galaxies at redshifts 6.0<z<8.7: stellar populations, star-formation rates and stellar masses
• Lyman-Alpha-Emitting Galaxies at z = 2.1 in ECDF-S: Building Blocks of Typical Present-day Galaxies?
• Realistic sterile neutrino dark matter with keV mass does not contradict cosmological bounds
• The GMRT-EoR Experiment: A new upper limit on the neutral hydrogen power spectrum at z~8.6
• Inside-out or Outside-in: The topology of reionization in the photon-starved regime suggested by Lyman-alpha forest data
• The Atacama Cosmology Telescope: likelihood for small-scale CMB data
• Cosmic Flows on 100 Mpc/h Scales: Standardized Minimum Variance Bulk Flow, Shear and Octupole Moments
• Upper Bound of 0.28 eV on the Neutrino Masses from the Largest Photometric Redshift Survey
• Deuterium Abundance in the Most Metal-Poor Damped Lyman alpha System: Converging on Omega_baryons
• Measurements of Secondary Cosmic Microwave Background Anisotropies with the South Pole Telescope
• Cosmological Constraints from a Combination of Galaxy Clustering and Lensing -- III. Application to SDSS Data
• Observables sensitive to absolute neutrino masses. II
• Testing General Relativity with Current Cosmological Data
• The HETDEX Pilot Survey. II. The Evolution of the Ly-alpha Escape Fraction from the UV Slope and Luminosity Function of 1.9<z<3.8 LAEs
• Primordial Curvature Fluctuation and Its Non-Gaussianity in Models with Modulated Reheating
• Current experimental constraints on the lightest Higgs boson mass in the constrained MSSM
• Dependence of Interstellar Turbulent Pressure on Supernova Rate
• Jet-regulated cooling catastrophe
• Detection of a Hot Gaseous Halo Around the Giant Spiral Galaxy NGC 1961
• The EFIGI catalogue of 4458 nearby galaxies with detailed morphology
• Semi-annihilation of Dark Matter
• Analytical solution of the geodesic equation in Kerr-(anti) de Sitter space-times
• Cosmic flow from 2MASS redshift survey: The origin of CMB dipole and implications for LCDM cosmology
• Implications of High-Resolution Simulations on Indirect Dark Matter Searches
• Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements
• Cosmological and Astrophysical Neutrino Mass Measurements
• The Kinematic Connection Between Galaxies and Dark Matter Haloes
• Constraining the Scatter in the Mass-Richness Relation of maxBCG Clusters With Weak Lensing and X-ray Data
• Spectroscopy of z ~ 7 candidate galaxies: Using Lyman-alpha to constrain the neutral fraction of hydrogen in the high-redshift universe
• Discovery of a Giant Lya Emitter Near the Reionization Epoch
• The X-ray Cluster Normalization of the Matter Power Spectrum
• On the Orbits of Infalling Satellite Halos
• Galaxies in X-ray Groups I: Robust Membership Assignment and the Impact of Group Environments on Quenching
• Observational evidence for a broken Li Spite plateau and mass-dependent Li depletion
• Hidden On-Shell Mediators for the Galactic Center Gamma-Ray Excess
• Radiative Transfer Modeling of Lyman Alpha Emitters. I. Statistics of Spectra and Luminosity
• The Impact of Feedback on Disk Galaxy Scaling Relations
• Probing modifications of General Relativity using current cosmological observations
• The Bimodal Galaxy Stellar Mass Function in the COSMOS Survey to z~1: A Steep Faint End and a New Galaxy Dichotomy
• Constraints on f(R) gravity from probing the large-scale structure
• The Fast Fourier Transform Telescope
• LoCuSS: the connection between brightest cluster galaxy activity, gas cooling and dynamical disturbance of X-ray cluster cores
• Planck early results. XXI. Properties of the interstellar medium in the Galactic plane
• Self-Consistent Cosmological Simulations of DGP Braneworld Gravity
• What determines satellite galaxy disruption?
• Microwave Background Constraints on Mixing of Photons with Hidden Photons
• The stellar mass fraction and baryon content of galaxy clusters and groups
• Constraints on the induced gravitational wave background from primordial black holes
• Probing the First Stars and Black Holes in the Early Universe with the Dark Ages Radio Explorer (DARE)
• Observing Neutral Hydrogen Above Redshift 6: The "Global" Perspective
• The Nature of Double-Peaked [O III] Active Galactic Nuclei
• A Grand Rotation Curve and Dark Matter Halo in the Milky Way Galaxy
• Constraining the high redshift formation of black hole seeds in nuclear star clusters with gas inflows
• ELUCID - Exploring the Local Universe with reConstructed Initial Density field III: Constrained Simulation in the SDSS Volume
• Galaxies in X-ray Groups. II. A Weak Lensing Study of Halo Centering
• Kinematics of Milky Way Satellites in a Lambda Cold Dark Matter Universe
• Robust Neutrino Constraints by Combining Low Redshift Observations with the CMB
• Cosmological parameter constraints from SDSS luminous red galaxies: a new treatment of large-scale clustering
• The Shift of the Baryon Acoustic Oscillation Scale: A Simple Physical Picture
• On the Baryon Fractions in Clusters and Groups of Galaxies
• Constraints on Dark Matter annihilations from reionization and heating of the intergalactic gas
• CMB polarization features from inflation versus reionization
• The Growth of Structure in Interacting Dark Energy Models
• Is the dark-matter halo spin a predictor of galaxy spin and size?
• Testing the Low-Mass End of X-Ray Scaling Relations with a Sample of Chandra Galaxy Groups
• Reconstructing the Distortion Function for Nonlocal Cosmology
• XMASS detector
• Gluon contribution to the dark matter direct detection
• The Atacama Cosmology Telescope: A Measurement of the 600< ell <8000 Cosmic Microwave Background Power Spectrum at 148 GHz
• First-year Sloan Digital Sky Survey-II (SDSS-II) supernova results: consistency and constraints with other intermediate-redshift datasets
• On the Origin of Exponential Galaxy Disks
• Nonlocal Models of Cosmic Acceleration
• The Parameter Space of Galaxy Formation
• The Carnegie-Chicago Hubble Program. I. An Independent Approach to the Extragalactic Distance Scale Using only Population II Distance Indicators
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Signs of neutrino mass in current cosmological datasets
• Hot X-ray coronae around massive spiral galaxies: a unique probe of structure formation models
• Cosmological Constraints on $f(G)$ Dark Energy Models
• LUNA: a Laboratory for Underground Nuclear Astrophysics
• Scaling Relations and Overabundance of Massive Clusters at z>~1 from Weak-Lensing Studies with HST
• The integrated stellar content of dark matter halos
• Primordial features due to a step in the inflaton potential
• Measuring the escape velocity and mass profiles of galaxy clusters beyond their virial radius
• Second and third season QUaD CMB temperature and polarization power spectra
• Six more quasars at redshift 6 discovered by the Canada-France High-z Quasar Survey
• Gas Motion Study of Lya Emitters at z~2 Using UV and Optical Spectral Lines
• What Does Clustering Tell Us About the Buildup of the Red Sequence?
• Updated constraints on the cosmic string tension
• Hubble Space Telescope Weak-lensing Study of the Galaxy Cluster XMMU J2235.3-2557 at z=1.4: A Surprisingly Massive Galaxy Cluster when the Universe is One-third of its Current Age
• The Epoch of Reionization
• Signatures of Non-Gaussianity in the Curvaton Model
• Planck pre-launch status: the Planck-LFI programme
• Anomalous parity asymmetry of the Wilkinson Microwave Anisotropy Probe power spectrum data at low multipoles
• Was reionization complete by z ~ 5-6?
• The Dark Universe
• Likelihood Functions for Supersymmetric Observables in Frequentist Analyses of the CMSSM and NUHM1
• XMM-Newton Detects a Hot Gaseous Halo in the Fastest Rotating Spiral Galaxy UGC 12591
• Extended Hot Halos Around Isolated Galaxies Observed in the ROSAT All-Sky Survey
• High-redshift formation and evolution of central massive objects II: The census of BH seeds
• Planck pre-launch status: High Frequency Instrument polarization calibration
• An updated Gamma Ray Bursts Hubble diagram
• The Impact of Modeling Assumptions in Galactic Chemical Evolution Models
• Mass and Hot Baryons in Massive Galaxy Clusters from Subaru Weak Lensing and AMiBA SZE Observations
• A dark matter disc in three cosmological simulations of Milky Way mass galaxies
• Cluster Density Profiles as a Test of Modified Gravity
• SuperIso Relic: A program for calculating relic density and flavor physics observables in Supersymmetry
• The diphoton signal of the light Higgs boson in Natural NMSSM
• Radio imaging of the Subaru/XMM-Newton Deep Field - III. Evolution of the radio luminosity function beyond z=1
• SPT-CL J0546-5345: A Massive z > 1 Galaxy Cluster Selected Via the Sunyaev-Zel'dovich Effect with the South Pole Telescope
• Massive black holes lurking in Milky Way satellites
• Galaxy formation in the Planck Millennium: the atomic hydrogen content of dark matter halos
• No Evolution in the IR-Radio Relation for IR-Luminous Galaxies at z<2 in the COSMOS Field
• A Comparison between Semi-Analytic Model Predictions for the CANDELS Survey
• The VLA-COSMOS Perspective on the IR-Radio Relation. I. New Constraints on Selection Biases and the Non-Evolution of the IR/Radio Properties of Star Forming and AGN Galaxies at Intermediate and High Redshift
• A Bayesian approach to the semi-analytic model of galaxy formation: methodology
• Cosmological Constraints on DGP Braneworld Gravity with Brane Tension
• Halo masses for optically-selected and for radio-loud AGN from clustering and galaxy-galaxy lensing
• Nucleosynthesis Constraints on a Massive Gravitino in Neutralino Dark Matter Scenarios
• Constraint on Coupled Dark Energy Models from Observations
• Templates for the Sunyaev-Zel'dovich Angular Power Spectrum
• Ly-alpha Emitting Galaxies at z = 2.1: Stellar Masses, Dust and Star Formation Histories from Spectral Energy Distribution Fitting
• The first (nearly) model-independent constraint on the neutral hydrogen fraction at z~5--6
• Constraints on cosmic hemispherical power anomalies from quasars
• The stellar-to-halo mass relation for Local Group galaxies
• On the Origin of the Galaxy Star-Formation-Rate Sequence: Evolution and Scatter
• High Redshift Metals I.: The Decline of C IV at z > 5.3
• On the Kennicutt-Schmidt relation of low-metallicity high-redshift galaxies
• Kerr-de Sitter Universe
• Collapse Barriers and Halo Abundance: Testing the Excursion Set Ansatz
• Properties of the scale factor measure
• Archipelagian Cosmology: Dynamics and Observables in a Universe with Discretized Matter Content
• Reconstructing the Cosmic Velocity and Tidal Fields with Galaxy Groups Selected from the Sloan Digital Sky Survey
• Cosmic web alignments with the shape, angular momentum and peculiar velocities of dark matter haloes
• Spherical Collapse and the Halo Model in Braneworld Gravity
• Galactic Globular and Open Clusters in the Sloan Digital Sky Survey. II. Test of Theoretical Stellar Isochrones
• Phantom Black Holes in Einstein-Maxwell-Dilaton Theory
• Robust Cosmological Bounds on Neutrinos and their Combination with Oscillation Results
• Indirect Evidence for Escaping Ionizing Photons in Local Lyman Break Galaxy Analogs
• BINGO: A code for the efficient computation of the scalar bi-spectrum
• The COS-Halos Survey: Keck LRIS and Magellan MagE Optical Spectroscopy
• CMB spectral distortions from small-scale isocurvature fluctuations
• Galaxy Formation Spanning Cosmic History
• Naturalness and Focus Points with Non-Universal Gaugino Masses
• Big Bang nucleosynthesis revisited via Trojan Horse Method measurements
• A Substantial Mass of Cool, Metal-Enriched Gas Surrounding the Progenitors of Modern-Day Ellipticals
• The extended ROSAT-ESO Flux Limited X-ray Galaxy Cluster Survey (REFLEX II) IV. X-ray Luminosity Function and First Constraints on Cosmological Parameters
• Voids as a Precision Probe of Dark Energy
• Measuring cosmological parameters with Gamma-Ray Bursts
• Cosmological parameter constraints for Horndeski scalar-tensor gravity
• A Scale-Dependent Power Asymmetry from Isocurvature Perturbations
• Hubble tension or a transition of the Cepheid SnIa calibrator parameters?
• Gamma rays from the annihilation of singlet scalar dark matter
• Measurement of the Crab nebula polarization at 90 GHz as a calibrator for CMB experiments
• Polarized CMB power spectrum estimation using the pure pseudo-cross-spectrum approach
• Investigating dark energy experiments with principal components
• Probing Majorana neutrinos in rare K and D, D_s, B, B_c meson decays
• Thermal history of the plasma and high-frequency gravitons
• Constraints on leptonically annihilating Dark Matter from reionization and extragalactic gamma background
• Constraining the evolutionary history of Newton's constant with gravitational wave observations
• Flavored Quantum Boltzmann Equations
• CosmoHammer: Cosmological parameter estimation with the MCMC Hammer
• De-Rotation of the Cosmic Microwave Background Polarization: Full-Sky Formalism
• The Evolution of the M_BH-sigma relation Inferred from the Age Distribution of Local Early-Type Galaxies and AGN Evolution
• Resolving the high redshift Lyman-alpha forest in smoothed particle hydrodynamics simulations
• MSSM Baryogenesis and Electric Dipole Moments: An Update on the Phenomenology
• The impact of supernovae driven winds on stream-fed protogalaxies
• Radiative Transfer Modeling of Lyman Alpha Emitters. II. New Effects in Galaxy Clustering
• Estimation of cosmological parameters using adaptive importance sampling
• A Profile Likelihood Analysis of the Constrained MSSM with Genetic Algorithms
• The SWELLS survey. II. Breaking the disk-halo degeneracy in the spiral galaxy gravitational lens SDSS J2141-0001
• On the Evolution of the Velocity-Mass-Size Relations of Disk-Dominated Galaxies over the Past 10 Billion Years
• Direct Constraints on Minimal Supersymmetry from Fermi-LAT Observations of the Dwarf Galaxy Segue 1
• Varying the Universality of Supersymmetry-Breaking Contributions to MSSM Higgs Boson Masses
• Metal-Poor Lithium-Rich Giants in the Radial Velocity Experiment Survey
• Can we discover dual-component thermal WIMP dark matter?
• A Model of Universe Anisotropization
• Observational Evidence of the Accelerated Expansion of the Universe
• The age problem in $\Lambda$CDM model
• Effects of Dark Matter Annihilation on the Cosmic Microwave Background
• A generalized equation of state for dark energy
• How flat can you get? A model comparison perspective on the curvature of the Universe
• The VIRUS-P Exploration of Nearby Galaxies (VENGA): Survey Design, Data Processing, and Spectral Analysis Methods
• A first direct measurement of the intergalactic medium temperature around a quasar at z=6
• Observations of Galactic and Extragalactic Novae
• Sterile Neutrinos in Light of Recent Cosmological and Oscillation Data: a Multi-Flavor Scheme Approach
• Directional detection as a strategy to discover Galactic Dark Matter
• Tests of Gravity from Imaging and Spectroscopic Surveys
• Super Luminous Supernovae as standardizable candles and high redshift distance probes
• ΔY/ ΔZ from the analysis of local K dwarfs
• The GMRT EoR Experiment: Limits on Polarized Sky Brightness at 150 MHz
• z~7-10 Galaxies behind Lensing Clusters: Contrast with Field Search Results
• New constraints on Parity Symmetry from a re-analysis of the WMAP-7 low resolution power spectra
• Right-handed sneutrino dark matter in the NMSSM
• A Census of Baryons and Dark Matter in an Isolated, Milky Way-sized Elliptical Galaxy
• No Evidence for Dark Energy Dynamics from a Global Analysis of Cosmological Data
• The past and future dynamics of quintom dark energy models
• New Constraints on the Primordial Magnetic Field
• Eddington-Born-Infeld gravity and the large scale structure of the Universe
• The evolution of Lyman-break galaxies in CDM
• Anomalous parity asymmetry of WMAP power spectrum data at low multpoles: is it cosmological or systematics?
• Structure formation in a nonlocally modified gravity model
• The rise and fall of star-formation in $\mathbf{z}\sim 0.2$ merging galaxy clusters
• Discovery of a redshift 6.13 quasar in the UKIRT Infrared Deep Sky Survey
• Model-independent cosmological constraints from the CMB
• Exploring Cosmic Origins with CORE: B-mode Component Separation
• Non-Gaussianity and the Cosmic Microwave Background Anisotropies
• Eight-Dimensional Mid-Infrared/Optical Bayesian Quasar Selection
• Cosmic variance of the local Hubble flow in large-scale cosmological simulations
• Horizon Run 4 Simulation: Coupled Evolution of Galaxies and Large-scale Structures of the Universe
• The Search for a Primordial Magnetic Field
• Discovery of spectral curvature in the shock downstream region: CIZA J2242.8+5301
• An Intensive HST Survey for z>1 Supernovae by Targeting Galaxy Clusters
• Delensing Gravitational Wave Standard Sirens with Shear and Flexion Maps
• Constraints on the Dark Side of the Universe and Observational Hubble Parameter Data
• Candidate z~8-9 Galaxies from WFC3 Imaging
• An Empirical Model for the Star Formation History in Dark Matter Halos
• Thinking Outside the Box: Effects of Modes Larger than the Survey on Matter Power Spectrum Covariance
• Di-photon Higgs signal at the LHC: a comparative study for different supersymmetric models
• The cosmological analysis of X-ray cluster surveys: II- Application of the CR-HR method to the XMM archive
• CMB Polarization Systematics, Cosmological Birefringence and the Gravitational Waves Background
• 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
• The Non-Gaussian Halo Mass Function with fNL, gNL and tauNL
• Simple foreground cleaning algorithm for detecting primordial B-mode polarization of the cosmic microwave background
• Improved Constraints on the Gravitational Lens Q0957+561. II. Strong Lensing
• Topology and Geometry of Gaussian random fields I: on Betti Numbers, Euler characteristic and Minkowski functionals
• Estimating the impact of recombination uncertainties on the cosmological parameter constraints from cosmic microwave background experiments
• 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
• Accretion Shocks in Clusters of Galaxies and their SZ Signature from Cosmological Simulations
• Probing natural SUSY from stop pair production at the LHC
• Cosmological constraints on dark matter models with velocity-dependent annihilation cross section
• Observation of interstellar lithium in the low-metallicity Small Magellanic Cloud
• The number density of a charged relic
• Majorana Phases and Leptogenesis in See-Saw Models with A_4 Symmetry
• Optical Redshift and Richness Estimates for Galaxy Clusters Selected with the Sunyaev-Zel'dovich Effect from 2008 South Pole Telescope Observations
• Cosmic transparency: A test with the baryon acoustic feature and type Ia supernovae
• WIMP Dark Matter and Baryogenesis
• Quintessence with quadratic coupling to dark matter
• Discussing direct search of dark matter particles in the Minimal Supersymmetric extension of the Standard Model with light neutralinos
• Dynamics of dark energy models and centre manifolds
• Fossil remnants of reionization in the halo of the Milky Way
• Tidal alignments as a contaminant of redshift space distortions
• Results from the Wilkinson Microwave Anisotropy Probe
• Spectral age modelling of the `Sausage' cluster radio relic
• Oscillations in the inflaton potential: Complete numerical treatment and comparison with the recent and forthcoming CMB datasets
• The scalar bi-spectrum in the Starobinsky model: The equilateral case
• How the Scalar Field of Unified Dark Matter Models Can Cluster
• The Observed Growth of Massive Galaxy Clusters III: Testing General Relativity on Cosmological Scales
• Do WMAP data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
• Confronting Dark Energy Models using Galaxy Cluster Number Counts
• A Constraint on Planck-scale Modifications to Electrodynamics with CMB polarization data
• How Dark Matter Reionized The Universe
• Positron/Gamma-Ray Signatures of Dark Matter Annihilation and Big-Bang Nucleosynthesis
• Dark-Matter Decays and Self-Gravitating Halos
• Relic density at one-loop with gauge boson pair production
• Wet Compaction to a Blue Nugget: a Critical Phase in Galaxy Evolution
• Confronting General Relativity with Further Cosmological Data
• Reconstruction of the primordial power spectrum of curvature perturbations using multiple data sets
• A critical analysis of the UV Luminosity Function at redshift~7 from deep WFC3 data
• Quark mass variation constraints from Big Bang nucleosynthesis
• Effect of quark-mass variation on big bang nucleosynthesis
• Machine learning cosmological structure formation
• The Chandra Survey of Extragalactic Sources in the 3CR Catalog: X-ray Emission from Nuclei, Jets, and Hotspots in the Chandra Archival Observations
• Ultradeep Near-Infrared Observations of GOODS 850-5
• The XMM-LSS survey: optical assessment and properties of different X-ray selected cluster classes
• Faraday rotation, stochastic magnetic fields and CMB maps
• KiDS+2dFLenS+GAMA: Testing the cosmological model with the $E_{\mathrm{G}}$ statistic
• The Equation of State of the Intergalactic Medium After Hydrogen Reionization
• iCosmo: an Interactive Cosmology Package
• The Little Review on Leptogenesis
• The Effect of Galactic Properties on the Escape Fraction of Ionizing Photons
• Dark halo response and the stellar initial mass function in early-type and late-type galaxies
• Stochastic backgrounds of relic gravitons: a theoretical appraisal
• Numerical resolution limits on subhalo abundance matching
• Betti numbers of Gaussian fields
• Photo-heating and the fate of hard photons during the reionisation of HeII by quasars
• Genetically modified halos: towards controlled experiments in $\Lambda$CDM galaxy formation
• Gravitational waves: Classification, Methods of detection, Sensitivities, and Sources
• Constraints on amplitudes of curvature perturbations from primordial black holes
• BayeSED: A General Approach to Fitting the Spectral Energy Distribution of Galaxies
• Constraining dark energy with gamma-ray bursts
• Metastable GeV-scale particles as a solution to the cosmological lithium problem
• Distant galaxy clusters in the XMM Large Scale Structure survey
• Probabilistic selection of high-redshift quasars
• Efficient Wiener filtering without preconditioning
• Precision cosmology with a wide area XMM cluster survey
• Conversion of relic gravitational waves into photons in cosmological magnetic fields
• Resurrecting No-Scale Supergravity Phenomenology
• Statistics of extreme objects in the Juropa Hubble Volume simulation
• Dark matter annihilation and its effect on CMB and Hydrogen 21 cm observations
• Thermodynamics of phantom black holes in Einstein-Maxwell-Dilaton theory
• Cosmology: small scale issues revisited
• Runaway Stars and the Escape of Ionizing Radiation from High-Redshift Galaxies
• Kaluza-Klein Dark Matter: Direct Detection vis-a-vis LHC
• Unveiling the nature of the unidentified gamma-ray sources III: gamma-ray blazar-like counterparts at low radio frequencies
• From the LHC to Future Colliders
• The clustering of Ly-alpha emitters in a LambdaCDM Universe
• Large-Scale Structure of the Universe as a Cosmic Standard Ruler
• The Interplay Between the "Low" and "High" Energy CP-Violation in Leptogenesis
• A three-phase amplification of the cosmic magnetic field in galaxies
• Probing Particle Physics with IceCube
• Alleviation of Cosmic Age Problem In Interacting Dark Energy Model
• The Growth of Central and Satellite Galaxies in Cosmological Smoothed Particle Hydrodynamics Simulations
• Host galaxy-active galactic nucleus alignments in the SDSS-DR7
• The relationship between star formation rate and radio synchrotron luminosity at 0 < z < 2
• Constraints from muon g-2 and LFV processes in the Higgs Triplet Model
• Thermodynamics of phantom Reissner-Nordstrom-AdS black hole
• Biased Dark Energy Constraints from Neglecting Reduced Shear in Weak Lensing Surveys
• The Star Formation History in The Far Outer Disc of M33
• Low Variance at large scales of WMAP 9 year data
• Singlet Fermionic Dark Matter explains DAMA signal
• Stochastic backgrounds of relic gravitons, T$\Lambda$CDM paradigm and the stiff ages
• A New Moment Method for Continuum Radiative Transfer in Cosmological Reionization
• The High Redshift Integrated Sachs-Wolfe Effect
• Anisotropic dark energy and CMB anomalies
• An analytical model for the accretion of dark matter subhalos
• How primordial magnetic fields shrink galaxies
• Testing pre-main sequence models: the power of a Bayesian approach
• Forecasted 21 cm constraints on compensated isocurvature perturbations
• The Cosmic Near Infrared Background II: Fluctuations
• A revised thermonuclear rate of ${}^7$Be($n$,$\alpha$)${}^4$He relevant to Big-Bang nucleosynthesis
• Early-type galaxies in the PEARS survey: Probing the stellar populations at moderate redshift
• Higher D or Li: Probes of Physics beyond the Standard Model
• Constraints from CMB on Spacetime Noncommutativity and Causality Violation
• Compatibility of Planck and BICEP2 in the Light of Inflation
• The role of cluster mergers and travelling shocks in shaping the H$\alpha$ luminosity function at $\mathbf{z}\sim 0.2$: `sausage' and `toothbrush' clusters
• Constraining the expansion rate of the Universe using low-redshift ellipticals as cosmic chronometers
• SUSY Constraints, Relic Density, and Very Early Universe
• Tracing the Gas to the Virial Radius (R100) in a Fossil Group
• The solar, exoplanet and cosmological lithium problems
• Multi-frequency imaging of the galaxy cluster Abell 2163 using the Sunyaev-Zel'dovich Effect
• The non-Gaussianity of the cosmic shear likelihood - or: How odd is the Chandra Deep Field South?
• Tachyon Field in Intermediate Inflation
• Cosmic string parameter constraints and model analysis using small scale Cosmic Microwave Background data
• Novel Higgs Decays and Dark Matter in the E(6)SSM
• Phenomenology of light neutralinos in view of recent results at the CERN Large Hadron Collider
• Sharpening the Precision of the Sunyaev-Zel'dovich Power Spectrum
• Dark Energy and Neutrino Masses from Future Measurements of the Expansion History and Growth of Structure
• Phantom wormholes in Einstein-Maxwell-dilaton theory
• Warm inflationary model in loop quantum cosmology
• High redshift formation and evolution of central massive objects I: model description
• On the consistency of warm inflation in the presence of viscosity
• The escape of ionizing photons from supernova-dominated primordial galaxies
• Detecting Gamma-Ray Anisotropies from Decaying Dark Matter: Prospects for Fermi LAT
• Chandra Observations of 3C Radio Sources with z<0.3 II: completing the snapshot survey
• SUSY Breaking Constraints on Modular flavor $S_3$ Invariant $SU(5)$ GUT Model
• The Observed Growth of Massive Galaxy Clusters IV: Robust Constraints on Neutrino Properties
• Inflation and Reheating in Induced Gravity
• BL Lac candidates for TeV observations
• Thermohaline instability and rotation-induced mixing II- Yields of 3He for low- and intermediate-mass stars
• The Top Window for dark matter
• $w$-cosmological singularities
• Large Scale Extragalactic Jets in the Chandra era I: data reduction and analysis
• Bayesian optimal reconstruction of the primordial power spectrum
• Distinguishing interacting dark energy from wCDM with CMB, lensing, and baryon acoustic oscillation data
• On Adiabatic Renormalization of Inflationary Perturbations
• Future CMB cosmological constraints in a dark coupled universe
• Equilibrium configurations of 11eV sterile neutrinos in MONDian galaxy clusters
• Cosmological evolution and statefinder diagnostic for new holographic dark energy model in non flat universe
• Cosmological constraints on a light non-thermal sterile neutrino
• A new look at microlensing limits on dark matter in the Galactic halo
• Oscillations in the dark energy EoS: new MCMC lessons
• Light mixed sneutrinos as thermal dark matter
• Features in the primordial power spectrum? A frequentist analysis
• Incorporating Photometric Redshift Probability Density Information into Real-Space Clustering Measurements
• Interpreting the Clustering of Distant Red Galaxies
• Supergauge interactions and electroweak baryogenesis
• Limits on Isocurvature Perturbations from Non-Gaussianity in WMAP Temperature Anisotropies
• Electroweak Resonant Leptogenesis in the Singlet Majoron Model
• GUT Inflation and Proton Decay after WMAP5
• Information Gains from Cosmic Microwave Background Experiments
• E6 inspired SUSY models with exact custodial symmetry
• Constraining Fundamental Physics with Future CMB Experiments
• From Big to Little Rip in modified F(R,G) gravity
• Black hole solutions in massive gravity
• Does the Universe Accelerate Equally in all Directions?
• Tachyacoustic Cosmology: An Alternative to Inflation
• Radio galaxy feedback in X-ray selected groups from COSMOS: the effect on the ICM
• The nature of HI absorbers in GRB afterglows: clues from hydrodynamic simulations
• CFHTLS weak-lensing constraints on the neutrino masses
• Dirac Neutralinos and Electroweak Scalar Bosons of N=1/N=2 Hybrid Supersymmetry at Colliders
• Leptogenesis with Linear, Inverse or Double Seesaw
• Non-universal scalar-tensor theories and big bang nucleosynthesis
• The axis of evil - a polarization perspective
• 3D Genus Topology of Luminous Red Galaxies
• Cross-correlating WMAP5 with 1.5 million LRGs: a new test for the ISW effect
• Fine-tuning implications for complementary dark matter and LHC SUSY searches
• On Possible Variation in the Cosmological Baryon Fraction
• Applications of Bayesian model averaging to the curvature and size of the Universe
• Relic Gravitational Waves with A Running Spectral Index and Its Constraints at High Frequencies
• Elucidating Galaxy Assembly Bias in SDSS
• New Optimised Estimators for the Primordial Trispectrum
• Testable dark energy predictions from current data
• A combined measurement of cosmic growth and expansion from clusters of galaxies, the CMB and galaxy clustering
• Cosmic Strings as the Source of Small-Scale Microwave Background Anisotropy
• The Jubilee ISW Project II: observed and simulated imprints of voids and superclusters on the cosmic microwave background
• Impact of Primordial Ultracompact Minihaloes on the Intergalactic Medium and First Structure Formation
• Mapping the allowed parameter space for decaying dark matter models
• The cosmological BCS mechanism and the Big Bang Singularity
• On the scalar consistency relation away from slow roll
• Constraining SUSY models with Fittino using measurements before, with and beyond the LHC
• Exclusion limits from data of directional Dark Matter detectors
• Halo clustering and g_{NL}-type primordial non-Gaussianity
• Non-parametric modeling of the intra-cluster gas using APEX-SZ bolometer imaging data
• Constraining reionization using 21 cm observations in combination with CMB and Lyman-alpha forest data
• Probing the Effective Number of Neutrino Species with Cosmic Microwave Background
• Constraints on modified gravity from the observed X-ray luminosity function of galaxy clusters
• The Quijote CMB Experiment
• Cosmological Limits on Hidden Sector Dark Matter
• Statistical methods for cosmological parameter selection and estimation
• A Multi-Parameter Investigation of Gravitational Slip
• Galaxy evolution from strong lensing statistics: the differential evolution of the velocity dispersion function in concord with the LambdaCDM paradigm
• Exploring the Diversity of Groups at 0.1<z<0.8 with X-ray and Optically Selected Samples
• Probing Primordial Chirality with Galaxy Spins
• New estimates of the CMB angular power spectra from the WMAP 5 yrs low resolution data
• Non-Gaussianity and Baryonic Isocurvature Fluctuations in the Curvaton Scenario
• Dirac gaugino as leptophilic dark matter
• Interacting Cosmological Fluids and the Coincidence Problem
• Dark matter-dark energy interaction for a time-dependent equation of state
• Toward More Realistic Forecasting of Dark Energy Constraints from Galaxy Redshift Surveys
• Star-formation efficiency and metal enrichment of the intracluster medium in local massive clusters of galaxies
• Cosmological constraints on generalized Chaplygin gas model: Markov Chain Monte Carlo approach
• Probing the IGM/Galaxy Connection IV: The LCO/WFCCD Galaxy Survey of 20 Fields Surrounding UV Bright Quasars
• Local stochastic non-Gaussianity and N-body simulations
• Probing the Astrophysics of Cluster Outskirts
• The Quasar SDSS J1536+0441: An Unusual Double-Peaked Emitter
• The Contribution Of Inverse Compton Scattering To The Diffuse Extragalactic Gamma-Ray Background From Annihilating Dark Matter
• Early Dark Energy at High Redshifts: Status and Perspectives
• The UK Infrared Telescope M33 monitoring project. V. The star formation history across the galactic disc
• Baryogenesis in non-extensive Tsallis Cosmology
• Constraining chameleon field theories using the GammeV afterglow experiments
• Cosmology with Equivalence Principle Breaking in the Dark Sector
• Constraints on the anisotropy of dark energy
• An interpretable machine learning framework for dark matter halo formation
• Pseudo-Majoron as Dark Matter
• Cascade Events at IceCube+DeepCore as a Definitive Constraint on the Dark Matter Interpretation of the PAMELA and Fermi Anomalies
• Investigating light neutralinos at neutrino telescopes
• Annihilation vs. Decay: Constraining dark matter properties from a gamma-ray detection
• Unified Dark Matter models with fast transition
• Mainly axion cold dark matter in the minimal supergravity model
• Spherical Collapse and Cluster Counts in Modified Gravity Models
• Cosmological parameters after WMAP5: forecasts for Planck and future galaxy surveys
• A Phenomenological Model for the Early Universe
• Baryon Asymmetry from the Generalized Uncertainty Principle
• Lepton-mediated electroweak baryogenesis
• Sneutrino NLSP Scenarios in the NUHM with Gravitino Dark Matter
• Lyman-alpha transfer in primordial hydrogen recombination
• Fractal initial conditions and natural parameter values in hybrid inflation
• A Chandra Snapshot Survey for 3C Radio Galaxies with redshifts between 0.3 and 0.5
• Estimating relic magnetic fields from CMB temperature correlations
• Gamma-ray bursts as cosmological probes: LambdaCDM vs. conformal gravity
• Multicomponent and Variable Velocity Galactic Outflow in Cosmological Hydrodynamic Simulations
• Accretion, Growth of Supermassive Black Holes, and Feedback in Galaxy Mergers
• The Jubilee ISW Project I: simulated ISW and weak lensing maps and initial power spectra results
• The discovery of a typical radio galaxy at z = 4.88
• Single-field inflation constraints from CMB and SDSS data
• Inert-Sterile Neutrino: Cold or Warm Dark Matter Candidate
• The ELIXR Galaxy Survey. II: Baryons and Dark Matter in an Isolated Elliptical Galaxy
• Bayesian component separation and CMB estimation for the 5-year WMAP temperature data
• Forecasts for Dark Energy Measurements with Future HI Surveys
• Analytic Spectra of CMB Anisotropies and Polarization Generated by Relic Gravitational Waves with Modification due to Neutrino Free-Streaming
• Power Asymmetries in the Cosmic Microwave Background Temperature and Polarization patterns
• Hierarchical Galaxy Growth and Scatter in the Stellar Mass - Halo Mass Relation
• Probing magnetic turbulence by synchrotron polarimetry: statistics and structure of magnetic fields from Stokes correlators
• TEASING: a fast and accurate approximation for the low multipole likelihood of the Cosmic Microwave Background temperature
• The Hubble Space Telescope Cluster Supernova Survey: III. Correlated Properties of Type Ia Supernovae and Their Hosts at 0.9 < z < 1.46
• A Chandra view of the z=1.62 galaxy cluster IRC-0218A
• The signature of dark energy perturbations in galaxy cluster surveys
• Small Angular Scale Measurements of the CMB Temperature Power Spectrum from QUaD
• Observational constraints on K-inflation models
• What the small angle CMB really tells us about the curvature of the Universe
• Luminous Red Galaxy Halo Density Field Reconstruction and Application to Large Scale Structure Measurements
• Interpreting the Global 21-cm Signal from High Redshifts. I. Model Independent Constraints
• The extreme limit of the generalized Chaplygin gas
• Efficient reconstruction of CMSSM parameters from LHC data - A case study
• Constraints on dark energy from the lookback time versus redshift test
• The clustering of galaxy clusters in cosmological models with non-Gaussian initial conditions: Predictions for future surveys
• Diffuse light in the young cluster of galaxies CL J1449+0856 at z=2.07
• Blazars spectral properties at 74 MHz
• A Re-analysis of Gravitino Dark Matter in the Constrained MSSM
• The cosmological analysis of X-ray cluster surveys: I- A new method for interpreting number counts
• Cosmic Antiproton Constraints on Effective Interactions of the Dark Matter
• Cold Dark Matter Isocurvature Perturbations: Constraints and Model Selection
• KiDS-Legacy calibration: unifying shear and redshift calibration with the SKiLLS multi-band image simulations
• Neutrino Mass, Sneutrino Dark Matter and Signals of Lepton Flavor Violation in the MRSSM
• Neutralino Dark Matter in the USSM
• What if Supersymmetry Breaking Unifies beyond the GUT Scale?
• From the early to the late time universe within $f(T,\mathcal{T})$ gravity
• The luminosity of supernovae of type Ia from TRGB distances and the value of H_0
• WMAP 7 year constraints on CPT violation from large angle CMB anisotropies
• Phenomenology of SUSY SU(5) with type I+III seesaw
• Effect of Long-lived Strongly Interacting Relic Particles on Big Bang Nucleosynthesis
• The evolution of the helium-ionizing background at z ~ 2-3
• Large curvature perturbations near horizon crossing in single-field inflation models
• Relating the structure of dark matter halos to their assembly and environment
• Unraveling the origin of magnetic fields in galaxies
• Indirect detection of gravitino dark matter including its three-body decays
• Spitzer observations of a gravitationally lensed quasar, QSO 2237+0305
• On using the WMAP distance priors in constraining the time evolving equation of state of dark energy
• Maximum likelihood, parametric component separation and CMB B-mode detection in suborbital experiments
• Weak lensing signal in Unified Dark Matter models
• HectoMAP and Horizon Run 4: Dense Structures and Voids in the Real and Simulated Universe
• Neutralino Dark Matter with Inert Higgsinos and Singlinos
• Probing the time dependence of dark energy
• Bayesian inferences of galaxy formation from the K-band luminosity and HI mass functions of galaxies: constraining star formation and feedback
• Double Type-II Seesaw, Baryon Asymmetry and Dark Matter for Cosmic e^\pm Excesses
• Galaxy Satellites and the Weak Equivalence Principle
• A Comparison of Algorithms for the Construction of SZ Cluster Catalogues
• Cosmological concordance or chemical coincidence? Deuterated molecular hydrogen abundances at high redshift
• Dark Matter Signatures in the Anisotropic Radio Sky
• The ACS Nearby Galaxy Survey Treasury IV. The Star Formation History of NGC 2976
• A Dark Matter Model with Non-Abelian Gauge Symmetry
• Including birefringence into time evolution of CMB: current and future constraints
• The 21 cm Forest as a Probe of the Reionization and the Temperature of the Intergalactic Medium
• Curvaton reheating in logamediate inflationary model
• Observational constraints on cosmic neutrinos and dark energy revisited
• Dark Energy Survey Year 1 Results: the lensing imprint of cosmic voids on the Cosmic Microwave Background
• Higgs decay to dark matter in low energy SUSY: is it detectable at the LHC ?
• Cosmic age, Statefinder and $Om$ diagnostics in the decaying vacuum cosmology
• Structure and substructure analysis of DAFT/FADA galaxy clusters in the [0.4-0.9] redshift range
• Fluctuations in the Ionizing Background During and After Helium Reionization
• Probing the Epoch of Reionization with the Lyman Alpha Forest at z~4-5
• Bimetric structure formation: non-Gaussian predictions
• Figures of merit for present and future dark energy probes
• A dynamical approach to link low energy phases with leptogenesis
• Observable effects of anisotropic bubble nucleation
• Transit cosmological models with observational constraints in f(Q, T) gravity
• Hybrid natural inflation from non Abelian discrete symmetry
• ${\rm Y}$ Decays into Light Scalar Dark Matter
• Properties and use of CMB power spectrum likelihoods
• Mixed dark matter: matter power spectrum and halo mass function
• Flavon Inflation
• Neutrino Oscillations, Lorentz/CPT Violation, and Dark Energy
• Primordial Helium Abundance from CMB: a constraint from recent observations and a forecast
• Cosmological constraints on the Hu-Sawicki modified gravity scenario
• The reanalysis of spectra of GRB 080913 to estimate the neutral fraction of the IGM at a redshift of 6.7
• MSSM Forecast for the LHC
• An X-ray selected catalog of extended galaxy clusters from the ROSAT All-Sky Survey (RXGCC)
• Ultra light bosonic dark matter and cosmic microwave background
• Low-Scale Leptogenesis and the Domain Wall Problem in Models with Discrete Flavor Symmetries
• Explaining the DAMPE data with scalar dark matter and gauged $U(1{)}_{L_e-L_{\mu }}$ interaction
• Angular momentum transfer to a Milky Way disk at high redshift
• The Most Bound Halo Particle-Galaxy Correspondence Model: Comparison between Models with Different Merger Timescales
• Analytical solutions of accreting black holes immersed in a Lambda-CDM model
• Non-canonical generalizations of slow-roll inflation models
• Light Neutralino in the MSSM: a playground for dark matter, flavor physics and collider experiments
• Studying the Sources of Cosmic Reionization with 21-cm Fluctuations
• Bright Lyman-alpha Emitters at z~9: constraints on the luminosity function from HiZELS
• First stars and the extragalactic background light: How recent gamma-ray observations constrain the early universe
• Averaging Robertson-Walker Cosmologies
• Reionization constraints from five-year WMAP data
• Two-point Correlation Function of WMAP 9 year data
• Mass and Metallicity Requirement in Stellar Models for Galactic Chemical Evolution Applications
• Neutrino masses from clustering of red and blue galaxies: a test of astrophysical uncertainties
• Influence of Population III stars on cosmic chemical evolution
• Structure formation in the Deser-Woodard nonlocal gravity model: a reappraisal
• Constraining resonant dark matter with combined LHC electroweakino searches
• ELUCID. VI: Cosmic variance of galaxy distribution in the local Universe
• Mapping the Escape Fraction of Ionizing Photons Using Resolved Stars: A Much Higher Escape Fraction for NGC 4214
• Measuring the reionization optical depth without large-scale CMB polarization
• Fine-tuning favors mixed axion/axino cold dark matter over neutralinos in the minimal supergravity model
• Gamma-ray Constraints on Hadronic and Leptonic Activities of Decaying Dark Matter
• The impact of a strongly first-order phase transition on the abundance of thermal relics
• Probing the Anisotropy of the Milky Way Gaseous Halo-II: sightline toward Mrk509
• Robustness of cosmic neutrino background detection in the cosmic microwave background
• CLARA's view on the escape fraction of Lyman-Alpha photons in high redshift galaxies
• The FRB 121102 host is atypical among nearby FRBs
• Resonant Dirac leptogenesis on throats
• Review of scientific topics for Millimetron space observatory
• Highlights and Discoveries from the Chandra X-ray Observatory
• Parameter dependence of magnetized CMB observables
• Detecting and distinguishing topological defects in future data from the CMBPol satellite
• Forecast Constraints on Inflation from Combined CMB and Gravitational Wave Direct Detection Experiments
• Gravitational waves and stability of cosmological solutions in the theory with anomaly-induced corrections
• Polytropic dark matter flows illuminate dark energy and accelerated expansion
• The Deuterium Abundance in the Local Interstellar Medium
• Strong lensing of submillimetre galaxies: A tracer of foreground structure?
• Optimal constraint on g_NL from CMB
• Turbulence in the Intergalactic Medium
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): ${\Omega }_{{\mathrm{m}}_0}$ from the galaxy clustering ratio measured at $z\sim 1$
• The EFIGI catalogue of 4458 nearby galaxies with morphology II. Statistical properties along the Hubble sequence
• Signatures of clumpy dark matter in the global 21 cm background signal
• Constraining the time variation of the coupling constants from cosmic microwave background: effect of Λ_{QCD}
• Production of Primordial Black Holes via Single Field Inflation and Observational Constraints
• Large contributions to dark matter annihilation from three-body final states
• Disk Galaxy Scaling Relations in the SFI++: Intrinsic Scatter and Applications
• Probing Dark Energy Dynamics from Current and Future Cosmological Observations
• Effects of power law primordial magnetic field on big bang nucleosynthesis
• Rivers of Gas I.: Unveiling The Properties of High Redshift Filaments
• X-ray spectral curvature of High Frequency Peaked BL Lacs: a predictor for the TeV flux
• A Left-Right Symmetric Model for Neutrino Masses, Baryon Asymmetry and Dark Matter
• A New X-ray Selected Sample of Very Extended Galaxy Groups from the ROSAT All-Sky Survey
• Update on the Direct Detection of Dark Matter in MSSM Models with Non-Universal Higgs Masses
• Combining Semi-analytic Models with Simulations of Galaxy Clusters: the Need for Heating from Active Galactic Nuclei
• Revealing the cosmic web dependent halo bias
• The Gentle Growth of Galaxies at High Redshifts in Overdense Environments
• Emerging Universe from Scale Invariance
• Hybrid Natural Low Scale Inflation
• A cosmological context for compact massive galaxies
• Gravitational waves, dark energy and inflation
• Resolving the baryon-fraction profile in lensing galaxies
• Approximate Analytic Spectra of Reionized CMB Anisotropies and Polarization generated by Relic Gravitational Waves
• Distinguishing standard reionization from dark matter models
• Intermediate inflation in Gauss-Bonnet braneworld
• Prospects for dark matter detection with IceCube in the context of the CMSSM
• Detected fluctuations in SDSS LRG magnitudes: Bulk flow signature or systematic?
• Inert Doublet Dark Matter and Mirror/Extra Families after Xenon100
• Large scale alignment anomalies of CMB anisotropies: a new test for residuals applied to WMAP 5yr maps
• Hadronic production of squark-squark pairs: The electroweak contributions
• Detections of Faint Lyman-alpha Emitters at z = 5.7: Galaxy Building Blocks and Engines of Reionization
• Three-Point Correlations in f(R) Models of Gravity
• The distribution of Omega_k from the scale-factor cutoff measure
• CMB Temperature and Matter Power Spectrum in a Decay Vacuum Dark Energy Model
• Spheroidal post-mergers in the local Universe
• Updated void catalogs of the SDSS DR7 main sample
• 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
• Galaxy Formation in Heavily Overdense Regions at z~10: the Prevalence of Disks in Massive Halos
• Hemispherical power asymmetries in the WMAP 7-year low-resolution temperature and polarization maps
• Tensors, non-Gaussianities, and the future of potential reconstruction
• Interpreting the Transmission Windows of Distant Quasars
• ELUCID V. Lighting dark matter halos with galaxies
• Revival of the Deser-Woodard nonlocal gravity model: Comparison of the original nonlocal form and a localized formulation
• Magellan/MMIRS near-infrared multi-object spectroscopy of nebular emission from star forming galaxies at 2<z<3
• The Effect of Fluctuations on the Helium-Ionizing Background
• Dark Matter Assimilation into the Baryon Asymmetry
• Flaring Patterns in Blazars
• The Hubble rate in averaged cosmology
• Large scale directional anomalies in the WMAP 5yr ILC map
• Dark matter detection in the BMSSM
• Electric-magnetic duality and the conditions of inflationary magnetogenesis
• The V-mode polarization of the Cosmic Microwave Background
• Coupling between cold dark matter and dark energy from neutrino mass experiments
• Flavoured Soft Leptogenesis
• Limits on a muon flux from Kaluza-Klein dark matter annihilations in the Sun from the IceCube 22-string detector
• Time Dependent Quark Masses and Big Bang Nucleosynthesis Revisited
• The Dark Side of QSO Formation at High Redshifts
• Grand Rip and Grand Bang/Crunch cosmological singularities
• Complete one-loop effects of SUSY QCD in $b\bar{b}h$ production at the LHC under current experimental constraints
• The dusty, albeit ultraviolet bright infancy of galaxies
• The Effects of Varying Cosmological Parameters on Halo Substructure
• Cosmological Alfvén waves in the recent CMB data, and the observational bound on the primordial vector perturbation
• How accurate is it to update the cosmology of your halo catalogues?
• A Multiwavelength Spectral and Polarimetric Study of the Jet of 3C 264
• Observational constraints on phantom power-law cosmology
• The evolution of the Lyman-alpha forest effective optical depth following HeII reionisation
• Thermal inflation and baryogenesis in heavy gravitino scenario
• Weak lensing and dark energy: the impact of dark energy on nonlinear dark matter clustering
• A Bayesian Analysis of the Constrained NMSSM
• Chemistry of heavy elements in the Dark Ages
• Unifying cosmological and recent time variations of fundamental couplings
• Cosmological data analysis of f(R) gravity models
• K2: A new method for the detection of galaxy clusters based on CFHTLS multicolor images
• Bino Dark Matter and Big Bang Nucleosynthesis in the Constrained E6SSM with Massless Inert Singlinos
• Planck intermediate results. XXIII. Galactic plane emission components derived from Planck with ancillary data
• Impact of Systematics on SZ-Optical Scaling Relations
• Implications of CDMS II result on Higgs sector in the MSSM
• Stau relic density at the Big-Bang nucleosynthesis era consistent with the abundance of the light element nuclei in the coannihilation scenario
• Constraint on noncommutative spacetime from PLANCK data
• Constraining the Lorentz-Violating Bumblebee Vector Field with Big Bang Nucleosynthesis and Gravitational Baryogenesis
• Supersymmetric Leptogenesis and the Gravitino Bound
• Observational constraints on decaying vacuum dark energy model
• CP violation Beyond the MSSM: Baryogenesis and Electric Dipole Moments
• Dark Energy from Large-Scale Structure Lensing Information
• Leptogenesis without violation of B-L
• GARROTXA Cosmological Simulations of Milky Way-sized Galaxies: General Properties, Hot Gas Distribution, and Missing Baryons
• Helium reionization and the thermal proximity effect
• New results on catalyzed BBN with a long-lived negatively-charged massive particle
• Constraints upon the spectral indices of relic gravitational waves by LIGO S5
• Tachyon Field in Intermediate Inflation on the Brane
• Warm-Intermediate inflationary universe model
• Model independent constraints on mass-varying neutrino scenarios
• Understanding the origin of CMB constraints on Dark Energy
• Geometrothermodynamics of phantom AdS black holes
• CMB Temperature Polarization Correlation and Primordial Gravitational Waves
• Consistency check of ΛCDM phenomenology
• Dirac Born Infeld (DBI) Cosmic Strings
• Constraining Cosmology with Big Data Statistics of Cosmological Graphs
• Einstein-Maxwell-Dilatonic phantom black holes: Thermodynamics and geometrothermodynamics
• Bayesian Model Averaging in Astrophysics: A Review
• Changes in the halo formation rates due to features in the primordial spectrum
• Acceleration of Galactic Supershells by Lyman Alpha Radiation
• Massive Dark Matter Halos at High Redshift: Implications for Observations in the JWST Era
• Nonlinear Effects in the Amplitude of Cosmological Density Fluctuations
• Optimal Binning of the Primordial Power Spectrum
• An optimal estimator for the CMB-LSS angular power spectrum and its application to WMAP and NVSS data
• The global mass - to - light ratio of SLACS lenses
• BMSSM Implications for Cosmology
• Physics of the cosmic microwave background anisotropy
• Constraints on cosmological birefringence from Planck and Bicep2/Keck data
• Identifying galaxy groups at high redshift from incomplete spectroscopic data: I. The group finder and application to zCOSMOS
• CMB constraints on mass and coupling constant of light pseudoscalar particles
• Bayesian model comparison in cosmology with Population Monte Carlo
• VLT/XSHOOTER & Subaru/MOIRCS Spectroscopy of HUDF-YD3: No Evidence for Lyman-alpha Emission at z=8.55
• Cosmological Parameters from the QUaD CMB polarization experiment
• Charged Lepton Flavour Violating Radiative Decays ${\ell }_i\to {\ell }_j+\gamma$ in See-Saw Models with $A_4$ Symmetry
• MillimeterDL: Deep Learning Simulations of the Microwave Sky
• Big-Bang nucleosynthyesis: constraints on nuclear reaction rates, neutrino degeneracy, inhomogeneous and Brans-Dicke models
• Quantum Gravity inspired nonlocal gravity model
• A conventional approach to the dark-energy concept
• Testing the (generalized) Chaplygin gas model with the Lookback time-Redshift data
• Ten More New Sightlines for the Study of Intergalactic Helium, and Hundreds of Far-UV-Bright Quasars, from SDSS, GALEX, and HST
• Ly alpha emissters at z=6.5 in the SSA22 field: An area more neutral or void at the end of the reionization epoch
• Primordial Magnetic Field Effects on the CMB and Large Scale Structure
• Satellite Survival in Highly Resolved Milky Way Class Halos
• Constraints of dark matter direct detection experiments on the MSSM and implications for LHC Higgs searches
• Constraints on the High-l Power Spectrum of Millimeter-wave Anisotropies from APEX-SZ
• Peculiar velocities into the next generation: cosmological parameters from the SFI++ survey
• The BINGO Project VI: HI Halo Occupation Distribution and Mock Building
• Generalized modified gravity with the second order acceleration equation
• Heavy colored SUSY partners from deflected anomaly mediation
• Reionization on Large Scales II: Detecting Patchy Reionization through Cross Correlation of the Cosmic Microwave Background
• Coincidence Problem in $f(R)$ Gravity Models
• Large-scale Structure and Dynamics of the Most X-ray Luminous Galaxy Cluster Known -- RX J1347-1145
• Resonant high energy graviton to photon conversion at post recombination epoch
• The phenomenology of beyond Horndeski gravity
• On the contribution of active galactic nuclei to reionization (Research Note)
• Axinos in Cosmology and at Colliders
• Sequestering the Gravitino: Neutralino Dark Matter in Gauge Mediation
• The ACS Nearby Galaxy Survey Treasury VI. The Ancient Star Forming disk of NGC 404
• Evidence for the Fifth Element Astrophysical status of Dark Energy
• Understanding the redshift evolution of the luminosity functions of Lyman-alpha emitters
• The Radius of Baryonic Collapse in Disc Galaxy Formation
• Stückelino Dark Matter in Anomalous U(1)' Models
• A deep Chandra observation of the hot gaseous halo around a rare, extremely massive and relativistic jet launching spiral galaxy
• Explain DAMPE Results by Dark Matter With Hierarchical Lepton-Specific Yukawa Interactions
• Phase transition and heat engine efficiency of phantom AdS black holes
• Observational signatures of a non-singular bouncing cosmology
• Negative vacuum energy densities and the causal diamond measure
• The History of Star Formation in Galaxy Disks in the Local Volume as Measured by the ACS Nearby Galaxy Survey Treasury
• Expanding the search for galaxies at z ~7-10 with new NICMOS Parallel Fields
• Exploring the Luminosity Evolution and Stellar Mass Assembly of 2SLAQ Luminous Red Galaxies Between Redshift 0.4 and 0.8
• Should we doubt the cosmological constant?
• Radiative Feedback in Relic HII Regions at High-Redshift
• Comparison of the properties of two fossil groups of galaxies with the normal group NGC 6034 based on multiband imaging and optical spectroscopy
• Virialization of high redshift dark matter haloes
• Measuring Planck beams with planets
• Neutrino mass from cosmology: Impact of high-accuracy measurement of the Hubble constant
• Long gamma-ray burst rate at very high redshift
• Constraints on the neutrino mass and the primordial magnetic field from the matter density fluctuation parameter ${\sigma }_8$
• Cosmology of F-theory GUTs
• Higher-Order Gauss-Bonnet Cosmology
• Searching for super-WIMPs in leptonic heavy meson decays
• Searching for a cosmological preferred direction with 147 rotationally supported galaxies
• Numerical evaluation of the three-point scalar-tensor cross-correlations and the tensor bi-spectrum
• The nonlinear biasing of the 10k zCOSMOS galaxies up to z~1
• Non-Gaussian Scatter in Cluster Scaling Relations
• Constraints on Star Forming Galaxies at z> 6.5 from HAWK-I Y-band Imaging of GOODS-South
• Sources of contamination to weak lensing tomography: redshift-dependent shear measurement bias
• Neutron spectroscopic factors of 7Li and astrophysical 6Li(n,g)7Li reaction rates
• Dynamical Effect of the Turbulence of IGM on the Baryon Fraction Distribution
• A comparison of CMB Angular Power Spectrum Estimators at Large Scales: the TT case
• Scintillation-only Based Pulse Shape Discrimination for Nuclear and Electron Recoils in Liquid Xenon
• Rare Z-decay into light CP-odd Higgs bosons: a comparative study in different new physics models
• Constraints on neutrino masses from WMAP5 and BBN in the lepton asymmetric universe
• A Yukawa coupling parameterization for type I+ II seesaw formula and applications to lepton flavor violation and leptogenesis
• Non-Gaussianity in WMAP Data Due to the Correlation of CMB Lensing Potential with Secondary Anisotropies
• The ACS Nearby Galaxy Survey Treasury VII. The NGC 4214 Starburst and the Effects of Star Formation History on Dwarf Morphology
• Inverse problem: Reconstruction of modified gravity action in Palatini formalism by Supernova Type Ia data
• HST/COS Detection of Deuterated Molecular Hydrogen in a DLA at z = 0.18
• Dissecting the spin distribution of Dark Matter halos
• Detectability of large-scale power suppression in the galaxy distribution
• Solving the muon g-2 anomaly in deflected AMSB with messenger-matter interactions
• CMB-Galaxy correlation in Unified Dark Matter Scalar Field Cosmologies
• Implications for constrained supersymmetry of combined H.E.S.S. observations of dwarf galaxies, the Galactic halo and the Galactic Centre
• Evidence for horizon-scale power from CMB polarization
• The cosmological free-free signal from galaxy groups and clusters
• Effects of the size of cosmological N-Body simulations on physical quantities - III: Skewness
• Extreme data compression for the CMB
• Primordial beryllium as a big bang calorimeter
• The effect of asymmetric beams in the Wilkinson Microwave Anisotropy Probe experiment
• Insights into the origin of halo mass profiles from machine learning
• New decay modes of gravitino dark matter
• The degenerate gravitino scenario
• Astrophysical foregrounds and primordial tensor-to-scalar ratio constraints from CMB B-mode polarization observations
• New blazars from the cross-match of recent multi-frequency catalogs
• Higher order statistics of shear field: a machine learning approach
• Heavy Right-Handed Neutrinos and Dark Matter in the $\nu$CMSSM
• Observations of the Corona Borealis supercluster with the superextended Very Small Array: further constraints on the nature of the non-Gaussian CMB cold spot
• Scalar dark matter explanation of the DAMPE data in the minimal Left-Right symmetric model
• 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
• Test of conformal gravity with astrophysical observations
• The C-Band All-Sky Survey (C-BASS): Template Fitting of Diffuse Galactic Microwave Emission in the Northern Sky
• The Mass Function of Void Groups as a Probe of the Primordial non-Gaussianity
• Constraints on dark energy models from radial baryon acoustic scale measurements
• Symmetry and anti-symmetry of the CMB anisotropy pattern
• Constraining Dark Matter Properties with Gamma-Rays from the Galactic Center with Fermi-LAT
• Dark Matter Decay and the Abundance of Ultracompact Minihalos
• Optimising cosmic shear surveys to measure modifications to gravity on cosmic scales
• Power for dry BL Lacertae objects
• A useful guide for gravitational wave observers to test modified gravity models
• Reconciling low multipole anomalies and reheating in single field inflationary models
• Large Lepton Asymmetry for Small Baryon Asymmetry and Warm Dark Matter
• Constraints on Dark Energy Parameters from Correlations of CMB with LSS
• Universe opacity and CMB
• Identification of Cosmic Voids as Massive Cluster Counterparts
• Alcock-Paczynski Test with the Evolution of Redshift-Space Galaxy Clustering Anisotropy
• Reconstructing Cosmological Matter Perturbations using Standard Candles and Rulers
• Circular dichroism, magnetic knots and the spectropolarimetry of the Cosmic Microwave Background
• Phantom black holes and critical phenomena
• Study of the Spectrum of Inflaton Perturbations
• Identifying Ionized Regions in Noisy Redshifted 21 cm Data Sets
• Future CMB ISW-Lensing bispectrum constraints on modified gravity in the Parameterized Post-Friedmann formalism
• Averaging in cosmological models using scalars
• Modification of the 21-cm power spectrum by X-rays during the epoch of reionisation
• Annihilations of superheavy dark matter in superdense clumps
• Quantum Fields on Noncommutative Spacetimes: Theory and Phenomenology
• Cosmological Parameter Estimation Using the Genus Amplitude - Application to Mock Galaxy Catalogs
• Cosmic string induced CMB maps
• Cosmological Information from the Small-scale Redshift Space Distortions
• Cosmological Constraints on the Higgs Boson Mass
• Revisiting The Coincidence Problem in $f(R)$ Gravitation
• Spin and structural halo properties at high redshift in a LCDM Universe
• A 125 GeV Higgs and its di-photon signal in different SUSY models: a mini review
• Application of Bayesian model averaging to measurements of the primordial power spectrum
• Brightest group galaxies-II: the relative contribution of BGGs to the total baryon content of groups at z<1.3
• Bianchi Type-I Universe Models with Nonlinear Viscosity
• The Breakdown Scale of HI Bias Linearity
• Single-field inflation à la generalized Chaplygin gas
• Two fossil groups of galaxies at z~0.4 in the COSMOS: accelerated stellar-mass build-up, different progenitors
• Cosmic polarimetry in magnetoactive plasmas
• Landscape of Supersymmetric Particle Mass Hierarchies in Deflected Mirage Mediation
• A Critique of the Spite Plateau, and the Astration of Primordial Lithium
• Superweakly interacting dark matter from the Minimal Walking Technicolor
• Implementation of a Fourier Matched Filter in CMB Analyses. Application to ISW Studies
• Determination of the abundance of cosmic matter via the cell count moments of the galaxy distribution (1)
• A simple model for particle physics and cosmology
• Reheating Temperature and Gauge Mediation Models of Supersymmetry Breaking
• The ALHAMBRA survey: Discovery of a faint QSO at z = 5.41
• Explaining Excess Dipole in NVSS Data Using Superhorizon Perturbation
• Search for Majorana Neutrino Signal in $B_c$ Meson Rare Decay
• Statefinder parameters for quantum effective Yang-Mills condensate dark energy model
• A split SUSY model from SUSY GUT
• Structure formation in $f(R)$ gravity: A distinguishing probe between the dark energy and modified gravity
• Cosmological Perturbations and the Running Cosmological Constant Model
• On Gaugino Contributions to Soft Leptogenesis
• The $\gamma$-ray sky seen at X-ray energies I. Searching for the connection between X-rays and $\gamma$-rays in Fermi BL Lac objects
• Phenomenology of Supersymmetric Gauge-Higgs Unification
• Alignments of the Galaxies in and around the Virgo Cluster with the Local Velocity Shear
• Planck and reionization history: a model selection view
• Initial directional singularity in inflationary models
• Curvature Perturbation from Supersymmetric Flat Directions
• Novel traversable wormhole in General Relativity and Einstein-Scalar-Gauss-Bonnet theory supported by nonlinear electrodynamics
• Estimating the tensor-to-scalar ratio and the effect of residual foreground contamination
• An FLRW interacting dark energy model of the Universe
• Dark energy, integrated Sachs-Wolfe effect and large-scale magnetic fields
• Model independent approaches to reionization in the analysis of upcoming CMB data
• The Effects of the Ionizing Radiation Background on Galaxy Evolution
• Lensed Cosmic Microwave Background Constraints on Post-General Relativity Parameters
• ELUCID VII: Using Constrained Hydro Simulations to Explore the Gas Component of the Cosmic Web
• Dynamics of interacting scalar field model in the realm of chiral cosmology
• A Multi-Wavelength Study of Low Redshift Clusters of Galaxies I. Comparison of X-ray and Mid-Infrared Selected AGNs
• Dark Energy Nature in Logarithmic $f(R,T)$ Cosmology
• Local Group Analogs in $\Lambda$CDM cosmological simulations
• Hybrid dark energy
• Decoupling Dark Energy from Matter
• An efficient phase-shifting scheme for bolometric additive interferometry
• The lensing efficiencies of MACS X-ray selected versus RCS optically selected galaxy clusters
• Electron EDM and soft leptogenesis in supersymmetric B-L extension of the standard model
• Radiative natural SUSY spectrum from deflected AMSB scenario with messenger-matter interactions
• The dark side of curvature
• Split Supersymmetry Under GUT and Current Dark Matter Constraints
• Two-dimensional Topology of Cosmological Reionization
• Dark sector evolution in Horndeski models
• Ohmic currents and pre-decoupling magnetism
• An analytic approach to perturbations from an initially anisotropic universe
• Models of high redshift luminosity functions and galactic outflows: The dependence on halo mass function
• FRW dark energy cosmological model with hybrid expansion law
• Birefringence, CMB polarization and magnetized B-mode
• Large-Scale Gas Dynamics in the Adhesion Model: Implications for the Two-Phase Massive Galaxy Formation Scenario
• Leptogenesis in a model with Friedberg-Lee symmetry
• CMBPol Mission Concept Study: Reionization Science with the Cosmic Microwave Background
• A Sneutrino NLSP in the $\nu$CMSSM
• The $\gamma$-ray sky seen at X-ray energies II: the Swift hunt of Fermi BL Lac objects among unidentified gamma-ray sources
• Phenomenology of a Light Cold Dark Matter Two-Singlet Model
• Revised Mass-to-Light Ratios For Nearby Galaxy Groups and Clusters
• The Lyman-alpha forest at redshifts 0.1 -- 1.6: good agreement between a large hydrodynamic simulation and HST spectra
• Genus statistics using the Delaunay tessellation field estimation method: (I) tests with the Millennium Simulation and the SDSS DR7
• Enhanced X-ray emission from candidate Lyman continuum emitting galaxies
• Prospects in Constraining the Dark Energy Potential
• Observables for FRW model with cosmological constant in the framework of loop cosmology
• GECO: Galaxy Evolution COde - A new semi-analytical model of galaxy formation
• Globular clusters as probes of dark matter cusp-core transformations
• Exploring $0\nu \beta \beta$ and Leptogenesis in the Alternative Left-Right Model
• Higher-order generalized uncertainty principle applied to gravitational baryogenesis
• Exotic Smoothness in Four Dimensions and Euclidean Quantum Gravity
• Analytic Spectra of CMB Anisotropies and Polarization Generated by Scalar Perturbations in Synchronous Gauge
• Scalar field power-law cosmology with spatial curvature and dark energy-dark matter interaction
• Dark Matter Astrophysics
• Bianchi type-I string cosmological model in the presence of a magnetic field: classical versus loop quantum cosmology approaches
• IceCube: physics, status, and future
• The first spectral line surveys searching for signals from the Dark Ages
• Resolving the Ultra-Luminous X-ray Sources in the Ly$\alpha$ Emitting Galaxy Haro 11
• Statistical properties of substructures around Milky Way-sized haloes and their implications for the formation of stellar streams
• Correlation of supernova redshifts with temperature fluctuations of the Cosmic Microwave Background
• Measurement of Galaxy Cluster Integrated Comptonization and Mass Scaling Relations with the South Pole Telescope
• Naturality, unification and dark matter
• Simulated stellar kinematics studies of high-redshift galaxies with the HARMONI Integral Field Spectrograph
• Testing for spectral index variations in polarised CMB foregrounds
• The contribution of the kinematic Sunyaev-Zel'dovich Effect from the Warm Hot Intergalactic Medium to the Five-Year WMAP Data
• MAHGIC: A Model Adapter for the Halo-Galaxy Inter-Connection
• Relic gravitational waves in the frame of slow-roll inflation with a power-law potential and the detection
• Foreground removal from WMAP 5yr temperature maps using an MLP neural network
• Adiabatic versus Isocurvature Non--Gaussianity
• Deep learning insights into cosmological structure formation
• Dynamical evolutin of quintessence dark energy in collapsing dark matter halos
• Cosmic microwave anisotropies in an inhomogeneous compact flat universe
• Thermal abundance of non-relativistic relics with Sommerfeld enhancement
• Revisit relic gravitational waves based on the latest CMB observations
• Connections between the Seesaw and Dark Matter Searches
• The optimal redshift for detecting ionized bubbles in HI 21-cm maps
• Forecasts on neutrino mass constraints from the redshift-space two-point correlation function
• An Introduction into the Theory of Cosmological Structure Formation
• Parametric tension between even and odd multipole data of WMAP power spectrum: unaccounted contamination or missing parameters?
• The Chandra X-Ray Observatory: Progress Report and Highlights
• Designing Decisive Detections
• X-ray Clusters of Galaxies as Cosmological Tools
• Textures and Semi-Local Strings in SUSY Hybrid Inflation
• Galactic Fly-Bys: New Source of Lithium Production
• Natural SUSY from SU(5) Orbifold GUT
• Screening maps of the local Universe I -- Methodology
• Stormy weather in 3C 196.1: nuclear outbursts and merger events shape the environment of the hybrid radio galaxy 3C 196.1
• General relativistic density perturbations
• Flavoured soft leptogenesis and natural values of the B term
• Modeling missing transverse energy in V+jets at CERN LHC
• Decaying Dark Matter in Supersymmetric SU(5) Models
• Is the misalignment of the Local Group velocity and the 2MASS Redshift Survey dipole typical in a LambdaCDM model?
• Scalar field exact solutions for non-flat FLRW cosmology: A technique from non-linear Schrödinger-type formulation
• Split-SUSY dark matter in light of direct detection limits
• Constraining Intra-cluster Gas Models with AMiBA13
• Constraints from CMB in the intermediate Brans-Dicke inflation
• Upper Limit on Dimming of Cosmological Sources by Intergalactic Grey Dust from the Soft X-ray Background
• The Impact of Secondary non-Gaussianities in the CMB on Cosmological Parameter Estimation
• Probing Cosmology and Galaxy Cluster Structure with the Sunyaev-Zel'dovich Decrement vs. X-ray Temperature Scaling Relation
• An Extended Zel'dovich Model for the Halo Mass Function
• Quark-Novae, cosmic reionization, and early r-process element production
• Collider signatures of the Gauge-Higgs Dark Matter
• Exact Solutions in Modified Gravity Models
• Detection of Hot Gas in Galaxy Groups via the Sunyaev-Zel'dovich Effect
• Probing the Warm Dark Matter with High-z Quasar Luminosity Function
• The Baryon Cycle at High Redshifts: Effects of Galactic Winds on Galaxy Evolution in Overdense and Average Regions
• Neutralino relic density from ILC measurements in the CPV MSSM
• Optimal and fast E/B separation with a dual messenger field
• Do Bound Structures Brake Cosmic Acceleration?
• Probing the primordial power spectra with inflationary priors
• Clustering and descendants of MUSYC galaxies at z<1.5
• A Solution to Lithium Problem by Long-Lived Stau
• Spatial Correlations in the Helium-Ionizing Background
• Efficient Mass Estimate at the Core of Strong Lensing Galaxy Clusters Using the Einstein Radius
• Beyond the Higgs boson at the Tevatron: detecting gluinos from Yukawa-unified SUSY
• The coevolution of the velocity and mass functions of galaxies and dark haloes
• Cosmic shear statistics in cosmologies with non-Gaussian initial conditions
• Next-to-Minimal Supersymmetric Model Higgs Scenarios for Partially Universal GUT Scale Boundary Conditions
• $\mu -e$ Conversion With Four Generations
• Search at the CERN LHC for a light neutralino of cosmological interest
• Nonstandard Higgs Decays and Dark Matter in the E6SSM
• Simulated vs. observed UV emission at high redshift: a hint for a clumpy ISM?
• The parameter-free Finger-Of-God model and its application to 21cm intensity mapping
• Coupled scalar field cosmology with effects of curvature
• Tailoring galaxies: size-luminosity-surface brightness relations of bulges and disks along the morphological sequence
• Early search for supersymmetric dark matter models at the LHC without missing energy
• Galaxy Statistics in Pencil-beam Surveys at High Redshifts
• AMiBA: Sunyaev-Zel'dovich effect derived properties and scaling relations of massive galaxy clusters
• Cosmological Constraints on Rapid Roll Inflation
• Power Spectra of CMB Polarization by Scattering in Clusters
• Optimising Boltzmann codes for the Planck era
• Assumptions of the primordial spectrum and cosmological parameter estimation
• Dark matter direct detection in the MSSM with heavy scalars
• Modelling ultra-fine structure in dark matter halos
• The primordial "f_NL" non-Gaussianity, and perturbations beyond the present horizon
• The long-lived stau as a thermal relic
• Beyond the Standard Model for Montaneros
• Polytropic dark halos of elliptical galaxies
• The Evolution of Early-type Galaxies Selected by Their Spatial Clustering
• The Cosmology of Asymmetric Brane Modified Gravity
• Reheating constraints on modified quadratic chaotic inflation
• The BINGO project VIII: On the recoverability of the BAO signal on HI intensity mapping simulations
• Primordial density perturbations with running spectral index: impact on non-linear cosmic structures
• Probing the Primordial Power Spectrum with Cluster Number Counts
• Graviton creation from the CMB in large scale magnetic fields
• Narrow Band X-ray Photometry as a Tool for Studying Galaxy and Cluster Mass Distributions
• When galaxies collide: understanding the broad absorption-line radio galaxy 4C +72.26
• Brans-Dicke model constrained from Big Bang nucleosynthesis and magnitude redshift relations of Supernovae
• Null geodesics and observational cosmology
• Turn-off of Deuterium Astration in the Recent Star Formation of the Galaxy Disk
• Cosmic Rays during BBN as Origin of Lithium Problem
• Electromagnetic leptogenesis at the TeV scale
• Probing intergalactic radiation fields during cosmic reionization through gamma-ray absorption
• The Ks-band Tully-Fisher Relation - A Determination of the Hubble Parameter from 218 ScI Galaxies and 16 Galaxy Clusters
• Improved Cosmological Parameter Constraints from CMB and H(z) Data
• Variograms of the Cosmic Microwave Background Temperature Fluctuations: Confirmation of Deviations from Statistical Isotropy
• Finding proto-clusters to trace galaxy evolution: I. The finder and its performance
• Cosmological Parameters from a re-analysis of the WMAP-7 low resolution maps
• Implications of Higgs to diphoton decay rate in the bilinear R-parity violating supersymmetric model
• On the star formation efficiency in high redshift Lyman-α emitters
• Demonstration of the spike phenomenon using the LTB models
• Massive Galaxies at High-z: Assembly Patterns, Structure & Dynamics in the Fast Phase of Galaxy Formation
• Relics of spatial curvature in the primordial non-gaussianity
• Focusing on the extended X-ray emission in 3C 459 with a Chandra follow-up observation
• Extended X-ray emission associated with the radio lobes and the environments of 60 radio galaxies
• New Lithium Measurements in Metal-Poor Stars
• Interplay between the muon $g-2$ anomaly and the PTA nHZ gravitational waves from domain walls in next-to minimal supersymmetric standard model
• DESIVAST: A Catalog of Low-Redshift Voids using Data from the DESI DR1 Bright Galaxy Survey
• A spiral galaxy's mass distribution uncovered through lensing and dynamics
• MultiCAM: A multivariable framework for connecting the mass accretion history of haloes with their properties
• Is a Dissipative Regime During Inflation in Agreement with Observations?
• Gravitino dark matter in hybrid gauge-gravity models
• A Multi-messenger view of Cosmic Dawn: Conquering the Final Frontier
• New Black Holes Solutions in a Modified Gravity
• Inverse decays and the relic density of the sterile sneutrino
• Realistic f(T) model describing the de Sitter epoch of the dark energy dominated universe
• Constant-roll Inflation in Brane Induced Gravity Cosmology
• Beyond the Standard Model of Physics with Astronomical Observations
• A Multi-Wavelength Study of Low Redshift Cluster of Galaxies II. Environmental Impact on Galaxy Growth
• Scalar Triplet Leptogenesis with a CP violating phase
• Primordial Nucleosynthesis: an updated comparison of observational light nuclei abundances with theoretical predictions
• Gravitational waves during inflation from a 5D large-scale repulsive gravity model
• New Results from the Magellan IMACS Spectroscopic Lyman Alpha Survey: NICMOS Observations of Lyman Alpha emitters at z=5.7
• Estimation of the Hubble Constant and Constraint on Descriptions of Dark Energy
• Cosmic positron and antiproton constraints on the gauge-Higgs Dark Matter
• Brane cosmology in the Horava-Witten heterotic M-Theory on $S^1/Z_2$
• Observing Higgs Dark Matter at the CERN LHC
• Contamination of the Central Sunyaev--Zel'dovich Decrements in AMiBA Galaxy Cluster Observations
• A High Throughput Workflow Environment for Cosmological Simulations
• Supersymmetric Baryogenesis from Exotic Quark Decays
• Probing cosmology via the clustering of critical points
• Evolution of proto-galaxy-clusters to their present form: theory and observations
• Anisotropy and characteristic scales in halo density gradient profiles
• Second order invariants and holography
• On the abundance of gravitational arcs produced by submillimeter galaxies at radio and submm wavelengths
• Quasi-linear static solutions in massive gravity
• Explaining the Muon g-2 Anomaly in Deflected AMSB for NMSSM
• Evaluating the origins of the secondary bias based on the correlation of halo properties with the linear density field
• Statistical and dynamical decoupling of the IGM from Dark Matter
• Full sky Integrated Sachs-Wolfe maps for the MICE Grand Challenge lightcone simulation
• Implication of the PAMELA antiproton data for dark matter indirect detection at LHC
• Primordial Nucleosynthesis After WMAP
• Neutrons and the New Standard Model
• The curvaton scenario in Brane cosmology: model parameters and their constraints
• Reheating constraints to modulus mass for single field inflationary models
• A study of the galaxy redshift distribution toward the cosmic microwave background cold spot in the Corona Borealis supercluster
• Enhanced Tau Lepton Signatures at LHC in Constrained Supersymmetric Seesaw
• Multiple Main Sequence of Globular Clusters as a Result of Inhomogeneous Big Bang Nucleosynthesis
• Estimates of unresolved point sources contribution to WMAP 5
• Metal Enrichment and Reionization Constraints on Early Star Formation
• Galaxy systems in the optical and infrared
• Electrodynamics on Cosmological Scales
• Cosmology in One Dimension: The Two Component Universe
• Effect of phantom dark energy on the holographic thermalization
• Constraining Modified Gravity with Large non-Gaussianities
• Turbulence and turbulent mixing in natural fluids
• Wash-Out in N_2-dominated leptogenesis
• Cosmic Acceleration from Causal Backreaction in a Smoothly Inhomogeneous Universe
• Quantum of volume in de Sitter space
• Some aspects of neutrino mixing and oscillations
• Thermodynamics of black plane solution
• NMSSM with generalized deflected mirage mediation
• Primordial vorticity and gradient expansion
• Signals of the cosmological reionization in the radio sky through C and O fine structure lines
• Little Higgs model with new Z-parity and Dark matter
• Magnetized matter effects on dilaton photon mixing
• Observational signatures of lithium depletion in the metal-poor globular cluster NGC6397
• Surprising phenomena in a rich new class of inflationary models
• Lithium detection in red supergiant stars of the Perseus complex
• Weak lensing forecasts for dark energy, neutrinos and initial conditions
• A Study of Universal Thermodynamics in Massive Gravity: Modified Entropy on the Horizons
• Observational constraints on a Yang-Mills condensate dark energy model
• Crossing the cosmological constant barrier with kinetically interacting double quintessence
• Cluster-counterpart Voids: Void Identification from Galaxy Density Field
• A Swift X-ray view of the SMS4 sample -- X-ray properties of 31 quasars and radio galaxies
• Measuring the mass profile of galaxy clusters beyond their virial radius
• Peaks in the cosmological density field: parameter constraints from 2dF Galaxy Redshift Survey data
• Cosmic microwave background constraints on the tensor-to-scalar ratio
• Constraining Extended Reionization Models Through Arcminute-Scale CMB Measurements
• The BRAIN experiment, a bolometric interferometer dedicated to the CMB B-mode measurement
• Measuring galaxy abundance and clustering at high redshift from incomplete spectroscopic data: Tests on mock catalogs
• A Monster in the early Universe
• Higher order spectra from an initially anisotropic universe
• CMB constraints on noncommutative geometry during inflation
• Lagrangian Volume Deformations around Simulated Galaxies
• Muon (g-2) from the bulk neutrino field in a warped extra dimensional model
• Minimal Yukawa deflection of AMSB from the Kahler potential
• Friedmann equations from GUP-modified equipartition law
• The Gravitational Lensing Imprints of DES Y3 Superstructures on the CMB: A Matched Filtering Approach
• Cosmic Acceleration and a New Concordance from Causal Backreaction
• $f(T)$ gravity from holographic Ricci dark energy model with new boundary conditions
• Inflation from a Non-Local Theory of Gravity
• Warm constant-roll inflation in brane-world cosmology
• Dark matter and the LHC
• Sunyaev-Zel'dovich contribution in CMB analysis
• Accelerating and decelerating cosmology from spinor and scalar fields non-minimally coupled with f(R) gravity
• Spectator stresses and CMB observables
• How To Determine SUSY Mass Scales Now
• Anomalies, U(1)' and the MSSM
• RDM-stars and galactic rotation curves
• Building a Better mSUGRA: WIMP Dark Matter Without Flavor Violation
• Non-adiabatic instability in coupled dark sectors
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• Closed inflationary universe in Patch Cosmology
• Constraints on the three-fluid model of curvaton decay
• A new test for the Galactic formation and evolution -- prediction for the orbital eccentricity distribution of the halo stars
• The Primordial Helium Abundance
• Axion hot dark matter bounds
• XMM-Newton follow-up of a sample of apparent low surface brightness galaxy groups detected in the ROSAT All-Sky Survey
• How does Inflation Depend Upon the Nature of Fluids Filling Up the Universe in Brane World Scenario
• Decoupling of Higgs boson from the inflationary stage of Universe evolution
• Degeneracy and Discreteness in Cosmological Model Fitting
• Higgs mass from cosmological and astrophysical measurements
• A Swift X-ray view of the SMS4 sample -- II: X-ray properties of 17 bright radio sources
• Measurements of 4He in Metal-Poor Extragalactic HII Regions: the Primordial Helium Abundance and the Delta Y / Delta O Ratio
• Spinor-Unit Field Representation of Electromagnetism Applied to a Model Inflationary Cosmology
• A non-singular universe with vacuum energy
• Spectroscopic Confirmation of Two X-ray Diffuse and Massive Galaxy Clusters at Low Redshift
• Two spectroscopically confirmed galaxy structures at z=0.61 and 0.74 in the CFHTLS Deep~3 field
• Observations of General Relativity at strong and weak limits
• Logamediate inflation in DGP cosmology driven by a non-canonical scalar field
• Constraints on the Epoch of Reionization with Roman Space Telescope and the Void Probability Function of Lyman-Alpha Emitters
• Constraining super-critical string/brane cosmologies with astrophysical data
• Constraining primordial non-Gaussianity using Neural Networks
• Cross-correlating the patchy screening and kinetic Sunyaev-Zel'dovich effects as a new probe of reionization
• Lagrangian space remapping and the angular momentum reconstruction from cosmic structures
• Dark Energy and Dark Matter
• Triplet scalar flavored leptogenesis with spontaneous CP violation
• Dynamical suppression of non-adiabatic modes
• K-Inflation with a Dark Energy Coupling
• Neutralino dark matter detection beyond the MSSM
• Physics at Underground Laboratories: Direct Detection of Dark Matter
• Lensing Without Borders. I. A Blind Comparison of the Amplitude of Galaxy-Galaxy Lensing Between Independent Imaging Surveys
• Neutralino Dark Matter in MSSM Models with Non-Universal Higgs Masses
• Gravity heats the Universe
• Testing gravity on large scales. The skewness of the galaxy distribution at z~1
• Extracting cosmological signals from foregrounds in deep mm maps of the sky
• Inflation with the right-handed sneutrino revisited
• RDM-stars as sources of fast radio bursts
• High redshift galaxy surveys
• Big Bang Nucleosynthesis with long-lived strongly interacting relic particles
• Dark energy constraints and correlations with systematics from CFHTLS weak lensing, SNLS supernovae Ia and WMAP5
• Area products for ${\mathcal{H}}^{\pm }$ in AdS space
• From WMAP to Planck: Exact reconstruction of 4- and 5-dimensional inflationary potential from high precision CMB measurements
• Outlook for Charged Higgs Physics
• Minimal Lepton Flavor Violation and Renormalization Group Evolution of Lepton Masses and Mixing
• Adiabatic fluctuations from cosmic strings in a contracting universe
• Probing the last scattering surface through the recent and future CMB observations
• Forecasting isocurvature models with CMB lensing information: axion and curvaton scenarios
• Recent results in the search for dark matter with noble liquid detectors
• Cosmological bootstrap
• Measuring CMB non-Gaussianity as a probe of Inflation and Cosmic Strings
• Tachyonic Universes in Patch Cosmologies with $\Omega >1$
• Curvaton reheating and intermediate inflation in brane cosmology
• How Does Feedback Affect Milky Way Satellite Formation?
• Constraining Planck scale physics with CMB and Reionization Optical Depth
• A high-significance detection of primordial tidal torque imprints
• CMB polarization anisotropies from cosmological reionization: extension to B-modes
• Gravitino Production after Inflation in No-Scale Supergravity
• Turbulent formation of protogalaxies at the end of the plasma epoch: theory and observations
• Optimisation of the Population Monte Carlo algorithm: Application to constraining isocurvature models with cosmic microwave background data
• Stability of 2-body orbits in retarded gravitation theory (RGT)
• Supernova constraints on higher-dimensional cosmology with a phantom field
• The Effects of Gravitational Slip on the Higher-Order Moments of the Matter Distribution
• Turbulent formation of protogalaxies at the plasma to gas transition
• Galactic evolution of D, 3He and 4He
• A New Approach to Flatness, Horizon and Late-time Accelerating Expansion Problems on the basis of Mach Principle
• Primordial Nucleosynthesis: A Cosmological Probe
• Integrated Markov Chain Monte Carlo (MCMC) analysis of primordial non-Gaussianity (f_NL) in the recent CMB data
• Ringing Non-Gaussianity from inflation with a step in the second derivative of the potential
• Towards convergence of turbulent dynamo amplification in cosmological simulations of galaxies
• Nonlinear Spinors as the Candidate of Dark Matter
• The violent Universe: the Big Bang
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• Leptogenesis with Friedberg-Lee Symmetry
• Quantum Boltzmann equations in resonant leptogenesis
• The nonlinear equation of correlation function of galaxies in the expanding universe and the solution in linear approximation
• Primordial Fluctuations in String Cosmology
• Theoretical calculation of nuclear reactions of interest for Big Bang Nucleosynthesis
• Linearized Treatment of Scalar perturbations in the Asymptotic Cosmological Model
• $G_3$ -- interacting scalar tensor dark energy
• Optimizing Observational Strategy for Future Fgas Constraints
• Impact of the low solar abundance on the ages of globular clusters
• Relations between Neutrino and Charged Fermion Masses
• Non-Gaussian Distribution and Clustering of Hot and Cold Pixels in the WMAP Five-Year Sky
• Luminosities, Masses and Star Formation Rates of Galaxies at High Redshift (IAU279 conference proceedings)
• Sunyaev-Zel'dovich Effect Observations of the Bullet Cluster (1E 0657-56) with APEX-SZ