Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis

Abstract

We present new full-sky temperature maps in five frequency bands from 23 to 94 GHz, based on the first three years of the WMAP sky survey. The new maps, which are consistent with the first-year maps and more sensitive, incorporate improvements in data processing made possible by the additional years of data and by a more complete analysis of the polarization signal. These include refinements in the gain calibration and beam response models. We employ two forms of multi-frequency analysis to separate astrophysical foreground signals from the CMB, each of which improves on our first-year analyses. First, we form an improved 'Internal Linear Combination' map, based solely on WMAP data, by adding a bias correction step and by quantifying residual uncertainties in the resulting map. Second, we fit and subtract new spatial templates that trace Galactic emission; in particular, we now use low-frequency WMAP data to trace synchrotron emission. The WMAP point source catalog is updated to include 115 new sources. We derive the angular power spectrum of the temperature anisotropy using a hybrid approach that combines a maximum likelihood estimate at low l (large angular scales) with a quadratic cross-power estimate for l>30. Our best estimate of the CMB power spectrum is derived by averaging cross-power spectra from 153 statistically independent channel pairs. The combined spectrum is cosmic variance limited to l=400, and the signal-to-noise ratio per l-mode exceeds unity up to l=850. The first two acoustic peaks are seen at l=220.8 +- 0.7 and l=530.9 +- 3.8, respectively, while the first two troughs are seen at l=412.4 +- 1.9 and l=675.1 +- 11.1, respectively. The rise to the third peak is unambiguous; when the WMAP data are combined with higher resolution CMB measurements, the existence of a third acoustic peak is well established.

116 pgs, 24 figs. Accepted version of the 3-year paper as posted to http://lambda.gsfc.nasa.gov/product/map/dr2/map_bibliography.cfm in January 2007

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• Basics of inflationary cosmology
• CMB Temperature and Matter Power Spectrum in a Decay Vacuum Dark Energy Model
• Follow-up observations at 16 and 33 GHz of extragalactic sources from WMAP 3-year data: I - Spectral properties
• Modeling of accelerating Universe with bulk viscous fluid in Bianchi V space-time
• Optimal filters on the sphere
• How to make a clean separation between CMB E and B modes with proper foreground masking
• A novel method for measuring the extragalactic background light: Fermi application to the lobes of Fornax A
• CMB polarization map derived from the WMAP 5 year data through Harmonic Internal Linear Combination
• Complementing the ground-based CMB Stage-4 experiment on large scales with the PIXIE satellite
• Non-Gaussianity analysis on local morphological measures of WMAP data
• Foreground Separation and Constraints on Primordial Gravitational Waves with the PICO Space Mission
• Constraints on standard and non-standard early Universe models from CMB B-mode polarization
• Non-Gaussian Signatures in the five-year WMAP data as identified with isotropic scaling indices
• Point Source Contamination in CMB Non-Gaussianity Analyses
• Late-time acceleration and Phantom Divide Line Crossing with Non-minimal Coupling and Lorentz Invariance Violation
• Instability of reconstruction of the low CMB multipoles
• A novel multi-frequency technique for the detection of point sources in Cosmic Microwave Background maps
• Isocurvature modes and Baryon Acoustic Oscillations
• Constraints on scalar and tensor perturbations in phenomenological and two-field inflation models: Bayesian evidences for primordial isocurvature and tensor modes
• Parameter Inference for Weak Lensing using Gaussian Processes and MOPED
• Submillimetre Detection of the z=2.83 Lyman-Break Galaxy, Westphal-MM8, and Implications for SCUBA2
• Cosmological Alfvén waves in the recent CMB data, and the observational bound on the primordial vector perturbation
• The study of topology of the universe using multipole vectors
• Understanding the WMAP Cold Spot mystery
• Limits on high-frequency gravitational wave background from its interplay with large scale magnetic fields
• The dynamical viability of scalar-tensor gravity theories
• CMB likelihood approximation by a Gaussianized Blackwell-Rao estimator
• Constraints on the Primordial Magnetic Field from ${\sigma }_8$
• WMAP 5-year constraints on time variation of $\alpha$ and $m_e$ in a detailed recombination scenario
• The Linearity of the Cosmic Expansion Field from 300 to 30,000 km/s and the Bulk Motion of the Local Supercluster with Respect to the CMB
• Anomalous SZ Contribution to 3 Year WMAP Data
• Observational constraints on decaying vacuum dark energy model
• Efficiency of pseudo-spectrum methods for estimation of Cosmic Microwave Background B-mode power spectrum
• Re-examining the Too-Big-To-Fail Problem for Dark Matter Haloes with Central Density Cores
• Removal of two large scale Cosmic Microwave Background anomalies after subtraction of the Integrated Sachs Wolfe effect
• Statistical correlation between the distribution of Ly$\alpha$ emitters and IGM HI at $z\sim 2.2$ mapped by Subaru/Hyper Suprime-Cam
• Exploring the evolution of color-luminosity parameter $\beta$ and its effects on parameter estimation
• A characteristic observable signature of preferred frame effects in relativistic binary pulsars
• Bayesian Model Averaging in Astrophysics: A Review
• Searching for non-Gaussianity in the WMAP data
• Design, development and verification of the 30 and 44 GHz front-end modules for the Planck Low Frequency Instrument
• Cosmological constraints from the observed angular cross-power spectrum between Sunyaev-Zel'dovich and X-ray surveys
• How to constrain inflationary parameter space with minimal priors
• Effects of modified theories of gravity on neutrino pair annihilation energy deposition near neutron stars
• Kinematic Sunyaev-Zeldovich Cosmic Microwave Background Temperature Anisotropies Generated by Gas in Cosmic Structures
• Physics of the cosmic microwave background anisotropy
• Wavelet domain Bayesian denoising of string signal in the cosmic microwave background
• A Braneworld Dark Energy Model with Induced Gravity and the Gauss-Bonnet Effect
• Modified GBIG Scenario as an Alternative for Dark Energy
• Observation number correlation in WMAP data
• Holographic kinetic k-essence model
• Contamination cannot explain the lack of large-scale power in the cosmic microwave background radiation
• Structures in the microwave background radiation
• Probing for the Cosmological Parameters with PLANCK Measurement
• Primordial Magnetic Field Effects on the CMB and Large Scale Structure
• Explicit Bayesian treatment of unknown foreground contaminations in galaxy surveys
• Cosmic strings interacting with dark strings
• Assessing Consistency Between WMAP 9-year and Planck 2015 Temperature Power Spectra
• The number counts, luminosity functions and evolution of microwave-selected (WMAP) blazars and radio galaxies
• Full-sky Models of Galactic Microwave Emission and Polarization at Sub-arcminute Scales for the Python Sky Model
• Dynamical systems analysis of phantom models
• Faraday Rotation as a diagnostic of Galactic foreground contamination of CMB maps
• Crossing of the Phantom Divided Barrier with Lorentz Invariance Violating Fields
• Comparison of Frames: Jordan vs Einstein Frame for a Non-minimal Dark Energy Model
• Non-gaussianity in the foreground-reduced CMB maps
• Poincare dodecahedral space parameter estimates
• Non-Gaussianity of secondary anisotropies from ACTPol and Planck
• Angular Power Spectra with Finite Counts
• Effects of CMB temperature uncertainties on cosmological parameter estimation
• The scalar perturbation spectral index n_s: WMAP sensitivity to unresolved point sources
• Measuring the Largest Angular Scale CMB B-mode Polarization with Galactic Foregrounds on a Cut Sky
• Measuring Planck beams with planets
• Isocurvature modes and Baryon Acoustic Oscillations II: gains from combining CMB and Large Scale Structure
• Is the cold spot responsible for the CMB North-South asymmetry?
• A framework for testing isotropy with the cosmic microwave background
• Relating the inhomogeneous power spectrum to the CMB hemispherical anisotropy
• Too few spots in the cosmic microwave background
• The One-dimensional Fourier Representation and Large Angular Scale Foreground Contamination in the 3-year Wilkinson Microwave Anisotropy Probe data
• Detectability of large-scale power suppression in the galaxy distribution
• The effect of dark strings on semilocal strings
• Pseudo-Dipole Signal Removal from WMAP Data
• Extreme data compression for the CMB
• Multibaseline gravitational wave radiometry
• The Evolution of the Cosmic Microwave Background
• Neutrino spin oscillations in conformally gravity coupling models and quintessence surrounding a black hole
• An Improved Diffuse Foreground Subtraction by ILC method: CMB Map and Angular Power Spectrum using Planck and WMAP Observations
• The effect of asymmetric beams in the Wilkinson Microwave Anisotropy Probe experiment
• Improved calculation of relic gravitational waves
• Symmetry and anti-symmetry of the CMB anisotropy pattern
• Dominant Multipoles in WMAP5 Mosaic Data Correlation Maps
• On Preferred Axes in WMAP Cosmic Microwave Background Data after Subtraction of the Integrated Sachs-Wolfe Effect
• Generalized holographic Ricci dark energy and generalized second law of thermodynamics in Bianchi Type I universe
• Extragalactic Point Source Search in WMAP 61 and 94 GHz Data
• Large-scale anomalies of the CMB in the curvaton scenario
• Cosmoglobe DR1 results. I. Improved Wilkinson Microwave Anisotropy Probe maps through Bayesian end-to-end analysis
• Observational Constraints on Hybrid Scale Factor in f(Q,T) Gravity with Anisotropic Space-Time
• Is Cosmology Compatible with Blue Gravity Waves ?
• WMAP anomalous signal in the ecliptic plane
• Impact of Point Source Clustering on Cosmological Parameters with CMB Anisotropies
• Residual noise covariance for Planck low-resolution data analysis
• Searching for primordial non-Gaussianity in Planck CMB maps using a combined estimator
• CMB component separation in the pixel domain
• Bayesian power-spectrum inference with foreground and target contamination treatment
• Are There Echoes From The Pre-Big Bang Universe? A Search for Low Variance Circles in the CMB Sky
• WMAP Observations of Planck ESZ Clusters
• Determining the motion of the solar system relative to the cosmic microwave background using type Ia supernovae
• Multi-frequency spectral analysis of extragalactic radio sources in the 33-GHz VSA catalogue: sources with flattening and upturn spectrum
• Bianchi VII_h models and the cold spot texture
• Thermal and non-thermal emission in the Cygnus X region
• New insights into foreground analysis of the WMAP five-year data using FASTICA
• The effect of reionization on the CMB-density correlation
• Neutrino pair annihilation ($\nu \bar{\nu }\to e^{-}{e}^{+}$) in the presence of quintessence surrounding a black hole
• Mapping the large-angle deviation from Gaussianity in simulated CMB maps
• Harmonic Inpainting of the Cosmic Microwave Background Sky: Formulation and Error Estimate
• Hybrid-basis inference for large-scale galaxy clustering: combining spherical and Cartesian Fourier analyses
• Application of Bayesian model averaging to measurements of the primordial power spectrum
• The Hot and Cold Spots in Five-Year WMAP Data
• Peculiarities of phases of the WMAP quadrupole
• Local properties of WMAP Cold Spot
• Searching for planar signatures in WMAP
• Correlation between galactic HI and the Cosmic Microwave Background
• Flat Tree-level Inflationary Potentials in Light of CMB and LSS Data
• Interacting entropy-corrected holographic Chaplygin gas model
• Isotropy statistics of CMB hot and cold spots
• Hemispherical power asymmetry: parameter estimation from CMB WMAP5 data
• A Global ILC Approach in Pixel Space over Large Angular Scales of the Sky using CMB Covariance Matrix
• Dynamical-Screening and the Phantom-Like Effects in a DGP-Inspired $F(R,\varphi )$ Model
• Effects of a time-varying color-luminosity parameter $\beta$ on the cosmological constraints of modified gravity models
• Consistency Condition of Spherically Symmetric Solutions in $f(R)$ Gravity
• CMB low multipole alignments in the $\mathbf{\Lambda }$CDM and Dipolar models
• The local dust foregrounds in the microwave sky: I. Thermal emission spectra
• Weighing neutrinos in the presence of a running primordial spectral index
• A multifrequency method based on the Matched Multifilter for the detection of point sources in CMB maps
• Real space tests of the statistical isotropy and Gaussianity of the WMAP CMB data
• Inflaton Two-Point Correlation in the Presence of a Cosmic String
• Observational Scan Induced Artificial CMB Anisotropy
• Likelihood, Fisher information, and systematics of cosmic microwave background experiments
• Data compression on the sphere
• Tomography of the Reionization Epoch with Multifrequency CMB Observations
• Non-linear Preheating with Scalar Metric Perturbations
• A Dark Energy Model in Lyra Manifold
• Effect of Foregrounds on the CMBR Multipole Alignment
• Hemispherical Power Asymmetry in intensity and polarization for Planck PR4 data
• Baryonic matter perturbations in decaying vacuum cosmology
• Cosmo++: An Object-Oriented C++ Library for Cosmology
• Expected constraints on the Galactic magnetic field using PLANCK data
• Probability Density of the Multipole Vectors for a Gaussian Cosmic Microwave Background
• Does Planck mass run on the cosmological horizon scale?
• Quintom dark energy in DGP braneworld cosmology
• Time-Periodic Solutions of the Einstein's Field Equations
• Angular-planar CMB power spectrum
• Foreground removal from CMB temperature maps using an MLP neural network
• Covariant and infrared-free graviton two-point function in de Sitter spacetime II
• Dynamical system analysis of LRS-BI Universe with f(Q) gravity theory
• Fractal Structure of Isothermal Lines and Loops on the Cosmic Microwave Background
• Observational tests of backreaction with recent data
• Large scale vector modes and the first CMB temperature multipoles
• Frequentist comparison of CMB local extrema statistics in the five-year WMAP data with two anisotropic cosmological models
• A robust constraint on cosmic textures from the cosmic microwave background
• CMB-S4 and the Hemispherical Variance Anomaly
• Analytic Spectra of CMB Anisotropies and Polarization Generated by Scalar Perturbations in Synchronous Gauge
• Constraints on Generalized Dark Energy from Recent Observations
• Holographic dilatonic model of dark energy
• Foreground removal from WMAP 5yr temperature maps using an MLP neural network
• Morphology of CMB fields -- effect of weak gravitational lensing
• Spatial Periodicity of Galaxy Number Counts, CMB Anisotropy, and SNIa Hubble Diagram Based on the Universe Accompanied by a Non-Minimally Coupled Scalar Field
• Scale dependence of the primordial spectrum from combining the three-year WMAP, Galaxy Clustering, Supernovae, and Lyman-alpha forests
• Dynamical features of $f(T,B)$ cosmology
• Likelihood of the Power Spectrum in Cosmological Parameter Estimation
• A Statistical Analysis of the "Internal Linear Combination" Method in Problems of Signal Separation as in CMB Observations
• Smooth crossing of $w_{\Lambda }=-1$ line in a single scalar field model
• CMB anisotropies from acausal scaling seeds
• Analytic formulae for the off-center CMB anisotropy in a general spherically symmetric universe
• Phase analysis of the cosmic microwave background from an incomplete sky coverage
• Time-Periodic Solutions of the Einstein's Field Equations II
• Detecting baryon acoustic oscillations by 3d weak lensing
• de Sitter Harmonies: Cosmological Spacetimes as Resonances
• Testing fundamental physics with photon frequency shift
• Marginal distributions for cosmic variance limited CMB polarization data
• A Perturbative Analysis of Synchrotron Spectral Index Variation over Microwave Sky
• X-ray Clusters of Galaxies as Cosmological Tools
• CMB power spectrum estimation with non-circular beam and incomplete sky coverage
• Recent developments in astrophysical and cosmological exploitation of microwave surveys
• Testing isotropy of cosmos with WMAP and PLANCK data
• Leakage of power from dipole to higher multipoles due to non-symmetric WMAP beam
• Filling in the Gaps in the 4.85 GHz Sky
• Bayesian analysis of white noise levels in the 5-year WMAP data
• Direct reconstruction of spherical harmonics from interferometer observations of the CMB polarization
• The interacting generalized Ricci dark energy model in non-flat universe
• Testing the statistical isotropy of large scale structure with multipole vectors
• Local patch analysis for testing statistical isotropy of the Planck convergence map
• Interacting holographic tachyon model of dark energy
• White dwarf binary modulation can help stochastic gravitational wave background search
• Statistical isotropy violation in WMAP CMB maps resulting from non-circular beams
• Scalar Field as Dark Energy Accelerating Expansion of the Universe
• Sunyaev-Zel'dovich effect in the Virgo cluster from WMAP and ROSAT data
• Improved parametrization of the growth index for dark energy and DGP models
• Global neutrino parameter estimation using Markov Chain Monte Carlo
• Braneworld Isotropization and Magnetic Fields
• Detection of Dipole Modulation in CMB Temperature Anisotropy Maps from WMAP and Planck using Artificial Intelligence
• Constraints on the Optical Depth to Reionization from Balloon-Borne CMB Measurements
• CMB Telescopes and Optical Systems
• Optimal and fast E/B separation with a dual messenger field
• Degree-scale anomalies in the CMB: localizing the first peak dip to a small patch of the north ecliptic sky
• Higher-order gravity in higher dimensions: Geometrical origins of four-dimensional cosmology?
• Influence of Planck foreground masks in the large angular scale quadrant CMB asymmetry
• The Simultaneous Medicina-Planck Experiment (SiMPlE): data acquisition, reduction and first results
• Low-frequency line temperatures of the CMB
• Probing the circumgalactic baryons through cross-correlations
• Noncommutative Geometry and the Primordial Dipolar Imaginary Power Spectrum
• Phantom-Like Behavior of a DGP-Inspired Scalar-Gauss-Bonnet Gravity
• Age problem in holographic dark energy
• Measuring and calibrating Galactic synchrotron emission
• Inhomogeneous Cosmology, Inflation and Late-Time Accelerating Universe
• Ray tracing the integrated Sachs-Wolfe effect through the light cones of the Dark Energy Universe Simulation -- Full Universe Runs
• Decoherence Problem in Ekpyrotic Phase
• Probing the creatable character of perturbed Friedmann-Robertson-Walker universes
• Anisotropic Born-Infeld-f(R) Cosmologies
• The primordial "f_NL" non-Gaussianity, and perturbations beyond the present horizon
• Direct measurement of the angular power spectrum of cosmic microwave background temperature anisotropies in the WMAP Data
• The Atacama Cosmology Telescope: DR6 Power Spectrum Foreground Model and Validation
• Biparametric Adaptive Filter: detection of compact sources in complex microwave backgrounds
• The uncorrelated long term gamma-ray and X-ray variability of blazars and its implications on disk-jet coupling
• Testing for foreground residuals in the Planck foreground cleaned maps: A new method for designing confidence masks
• Two Component Baryonic-Dark Matter Structure Formation in Top-Hat Model
• Cosmic Covariance and the Low Quadrupole Anisotropy of the Wilkinson Microwave Anisotropy Probe (WMAP) Data
• Camouflaged galactic CMB foregrounds: total and polarized contributions of the kinetic Sunyaev Zeldovich effect
• Model of the polarized foreground diffuse Galactic emissions from 33 to 353 GHz
• Diffuse source separation in CMB observations
• Evolution of the CMB Power Spectrum Across WMAP Data Releases: A Nonparametric Analysis
• Two-photon approximation in the theory of the electron recombination in hydrogen
• On the Apparent Associations between Interstellar Neutral Hydrogen Structure and (WMAP) High Frequency Continuum Emission
• Cosmic ray backgrounds for dark matter indirect detection
• Modelling the WMAP large-angle anomalies as an effect of a local density inhomogeneity
• Imprint of Distortions in the Oort Cloud on the CMB Anisotropies
• Cosmological and Particle Physics Constraints on a New Non-Abelian SU(3) Gauge Model for Ordinary/Dark Matter Interaction
• Constraints on non-thermal Dark Matter from Planck lensing extraction
• Observing the evolution of the CMB
• Correlation properties of the maps of the NVSS survey and WMAP ILC
• Fast, exact (but unstable) spin spherical harmonic transforms
• ISW in $\Lambda$CDM or something else?
• Scalar quadratic maximum likelihood estimators for the CMB cross power spectrum
• Cosmological implications of the KATRIN experiment
• Fast scalar quadratic maximum likelihood estimators for the CMB B-mode power spectrum
• Search for non-Gaussianities in the WMAP data with the Scaling Index Method
• Probing for cosmological parameters with LAMOST measurement
• Hemispherical Variance Anomaly and Reionization Optical Depth
• Cosmological Parameters from a re-analysis of the WMAP-7 low resolution maps
• The primordial non-Gaussianity of local type (f_NL) in the WMAP 5-year data: the length distribution of CMB skeleton
• The Kinetic Sunyaev-Zel'dovich Effect Due to the Electrons of Our Galaxy
• Constraining Slow-Roll Inflation in the Presence of Dynamical Dark Energy
• From Analogue Models to Gravitating Vacuum
• Estimating SI violation in CMB due to non-circular beam and complex scan in minutes
• Conditions for spontaneous homogenization of the Universe
• CMB Angular Power Spectrum from Correlated Primordial Fluctuation
• Variograms of the Cosmic Microwave Background Temperature Fluctuations: Confirmation of Deviations from Statistical Isotropy
• Covariant Quantization of the Partially Massless Graviton Field in de Sitter Spacetime
• Bouncing Universe with a Nonminimally Coupled Scalar Field on a Moving Domain Wall
• On 1 + 3 covariant perturbations of the quasi-Newtonian space-time in modified Gauss-Bonnet gravity
• Constraints on the SZ Power Spectrum on Degree Angular Scales in WMAP Data
• Natural inflation in 5D warped backgrounds
• Allan Sandage and the Cosmic Expansion
• Limits on Semiclassical Fluctuations in the Primordial Universe
• Cosmic microwave background constraints on cosmological models with large-scale isotropy breaking
• The White Mountain Polarimeter Telescope and an Upper Limit on CMB Polarization
• Significant foreground unrelated non-acoustic anisotropy on the one degree scale in WMAP 5-year observations
• The Simons Observatory: Assessing the Impact of Dust Complexity on the Recovery of Primordial $B$-modes
• The spectral energy distribution of the Carina nebula from far infrared to radio wavelengths
• Microwave Emission from the Edgeworth-Kuiper Belt and the Asteroid Belt Constrained from WMAP
• Statistics of WMAP ILC map temperature fluctuations towards distant radio galaxies
• The nonlinear anisotropic model of the Universe with the linear potential
• The Accelerated Recombination, and the ACBAR and WMAP data
• Phantom Mimicry on the Normal Branch of a DGP-inspired Braneworld Scenario with Curvature Effect
• Effect of noncircularity of experimental beam on CMB parameter estimation
• Cosmic Acceleration from Causal Backreaction in a Smoothly Inhomogeneous Universe
• Study on the filters of atmospheric contamination in ground based CMB observation
• Cross-Power Spectrum and Its Application on Window Functions in the WMAP data
• Gauss-Bonnet Braneworld Cosmology with Modified Induced Gravity on the Brane
• Representation of signals as series of orthogonal functions
• Allan Sandage and the Distance Scale
• Examining statistical isotropy of CMB low multipoles from Planck PR4 data
• Extension of the sum rule for the transition rates between multiplets to the multiphoton case
• Model Independent Foreground Power Spectrum Estimation using WMAP 5-year Data
• Cosmic microwave background constraints on a decaying cosmological term related to the thermal evolution
• The two-and three-point correlation functions of the polarized five-year WMAP sky maps
• On the Critical Ionization Velocity Effect in Interstellar Space and Possible Detection of Related Continuum Emission
• Interacting Galactic Neutral Hydrogen Filaments and Associated High-Frequency Continuum Emission
• Observational constraints on cosmological parameters in the Bianchi type III Universe with f(R,T) gravity theory
• Anisotropic cosmology in Bumblebee gravity theory
• CMB Anomalies from Imperfect Dark Energy: Confrontation with the Data
• Investigation of the electromagnetically induced transparency in era of cosmological hydrogen recombination
• CMB lensing forecasts for constraining the primordial perturbations: adding to the CMB temperature and polarization information
• Application of Genetic Algorithm to Estimate the Large Angular Scale Features of Cosmic Microwave Background
• A Model of Large Quintessence Isocurvature Fluctuations and Low CMB Quadrupole
• Anisotropic cosmology using observational datasets: exploring via machine learning approaches
• An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$
• Quadrant asymmetry in the angular distribution of the Cosmic Microwave Background in the Planck satellite data
• On the Impact of Random Residual Calibration Error on the Gibbs ILC Estimates over Large Angular Scales
• Orientation of galaxies in structures
• CMB low multipole alignments across WMAP and \emph{Planck} data releases
• Excessive shift of the CMB acoustic peaks of the Cold Spot area
• Violation of Bell inequalities from Cosmic Microwave Background data
• Gravastar-like black hole solutions in $q$-theory
• QED model of the radiation escape from the matter
• Imprints of Anisotropy on the Power Spectrum in Matter Dominated Bouncing Universe as Background
• Bayesian analysis of the backreaction models
• Cosmological Constraints on Radion Evolution in the Universal Extra Dimension Model
• RMS Radio Source Contributions to the Microwave Sky
• Anisotropic cosmology in $q$-deformed entropic gravity
• Dark energy constraints and correlations with systematics from CFHTLS weak lensing, SNLS supernovae Ia and WMAP5
• Improved Method for Detecting Local Discontinuities in CMB data by Finite Differencing
• The effect of primordial fluctuations on neutrino oscillations
• Constraints on the Cosmological Constant in a Static Geometry from Periodicity in a Compact Fifth-Dimension
• A Search for X-Ray Reionization Signatures from Cross-Correlation of Wmap and ROSAT Rass Data
• A Partial-Sky Gibbs ILC Approach for the Estimation of CMB Posterior over Large Angular Scales of the Sky
• A Foreground Model Independent Bayesian CMB Temperature and Polarization Signal Reconstruction and Cosmological Parameter Estimation over Large Angular Scales
• An approach for the detection of point-sources in very high resolution microwave maps
• Baryon Acoustic Oscillations from galaxy surveys
• Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future
• A characterization of the diffuse Galactic emissions in the anti-center of the Galaxy
• A Cosmological Bragg Law: Interpreting the CMB as a Diffractogram of Foliated Spacetime
• Non-Gaussianities in the local curvature of the 5-year WMAP data
• Quintessence reconstruction of interacting HDE in a non-flat universe
• Birth and Growth of Two-dimensional Universe
• Integrated Markov Chain Monte Carlo (MCMC) analysis of primordial non-Gaussianity (f_NL) in the recent CMB data
• Testing the effects from dark radiation
• Asymmetry and non-random orientation of the inflight effective beam pattern in the WMAP Data
• Conformal General Relativity -- Unified Theory of the Standard Models of Elementary Particles and Modern Cosmology
• A New Description of Cosmic Strings in Brane World Scenario
• Torsion-Induced Modification to Friedmann Equations in $AdS{L}_4$ Gauged Gravity
• The quintessence field as a perfect cosmic fluid of constant pressure
• Correlation Analysis between Tibet AS-$\gamma$ TeV Cosmic Ray and WMAP Nine-year Data
• A 43-GHz Survey in the ELAIS N2 Area
• `Standard' Cosmological model & beyond with CMB
• Role of the companion lensing galaxy in the CLASS gravitational lens B1152+199
• CMB in nonstandard cosmology: A first look
• Observational constraints on a decaying cosmological term
• Phase space analysis of Bianchi III Universe with $f(R,T)$ gravity theory
• The Conformal Universe III: Basic Mechanisms of Matter Generation