Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results

Abstract

We present the final nine-year maps and basic results from the WMAP mission. We provide new nine-year full sky temperature maps that were processed to reduce the asymmetry of the effective beams. Temperature and polarization sky maps are examined to separate CMB anisotropy from foreground emission, and both types of signals are analyzed in detail. The WMAP mission has resulted in a highly constrained LCDM cosmological model with precise and accurate parameters in agreement with a host of other cosmological measurements. When WMAP data are combined with finer scale CMB, baryon acoustic oscillation, and Hubble constant measurements, we find that Big Bang nucleosynthesis is well supported and there is no compelling evidence for a non-standard number of neutrino species (3.84+/-0.40). The model fit also implies that the age of the universe is 13.772+/-0.059 Gyr, and the fit Hubble constant is H0 = 69.32+/-0.80 km/s/Mpc. Inflation is also supported: the fluctuations are adiabatic, with Gaussian random phases; the detection of a deviation of the scalar spectral index from unity reported earlier by WMAP now has high statistical significance (n_s = 0.9608+/-0.0080); and the universe is close to flat/Euclidean, Omega_k = -0.0027 (+0.0039/-0.0038). Overall, the WMAP mission has resulted in a reduction of the cosmological parameter volume by a factor of 68,000 for the standard six-parameter LCDM model, based on CMB data alone. For a model including tensors, the allowed seven-parameter volume has been reduced by a factor 117,000. Other cosmological observations are in accord with the CMB predictions, and the combined data reduces the cosmological parameter volume even further. With no significant anomalies and an adequate goodness-of-fit, the inflationary flat LCDM model and its precise and accurate parameters rooted in WMAP data stands as the standard model of cosmology.

177 pages, 44 figures, v3: Version accepted to Astrophysical Journal Supplement Series. Includes improvements in clarity of presentation and Fig 43 revised to include WMAP-only solutions, in response to referee and community. See the Legacy Archive for Microwave Background Data Analysis (LAMBDA): http://lambda.gsfc.nasa.gov/product/map/current/ for further detail

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• Hierarchical progressive surveys. Multi-resolution HEALPix data structures for astronomical images, catalogues, and 3-dimensional data cubes
• Constraints on secret neutrino interactions after Planck
• The Cosmic Thermal History Probed by Sunyaev-Zeldovich Effect Tomography
• Inflationary Steps in the Planck Data
• NIHAO XIX: How supernova feedback shapes the galaxy baryon cycle
• Future CMB constraints on cosmic birefringence and implications for fundamental physics
• Hot Extended Galaxy Halos Around Local L* Galaxies From Sunyaev-Zeldovich Measurements
• Distinguishing models of reionization using future radio observations of 21-cm 1-point statistics
• Dark Energy and Dark Matter from an additional adiabatic fluid
• The Galactic Faraday depth sky revisited
• Searching for Oscillations in the Primordial Power Spectrum: Perturbative Approach (Paper I)
• Galilean Creation of the Inflationary Universe
• Bi-layer Kinetic Inductance Detectors for space observations between 80-120 GHz
• Compatibility of Planck and BICEP2 in the Light of Inflation
• Nonlocal Gravity and Structure in the Universe
• Anisotropy of the Universe via the Pantheon supernovae sample revisited
• Trans-Planckian censorship and other swampland bothers addressed in warm inflation
• Effective field theory search for high-energy nuclear recoils using the XENON100 dark matter detector
• Polyspectra searches for sharp oscillatory features in cosmic microwave sky data
• Anisotropic inflation reexamined: upper bound on broken rotational invariance during inflation
• Faraday Tomography of the North Polar Spur: Constraints on the distance to the Spur and on the Magnetic Field of the Galaxy
• QUIJOTE scientific results -- IV. A northern sky survey in intensity and polarization at 10-20GHz with the Multi-Frequency Instrument
• Distinguishing interacting dark energy from wCDM with CMB, lensing, and baryon acoustic oscillation data
• Reconstructing cosmic growth with kSZ observations in the era of Stage IV experiments
• Dark matter and halo bispectrum in redshift space: theory and applications
• Constraining the Baryon Abundance with the Kinematic Sunyaev-Zel'dovich Effect: Projected-Field Detection Using Planck, WMAP, and unWISE
• Two Loop Neutrino Model and Dark Matter Particles with Global $B-L$ Symmetry
• Modelling of the Spectral Energy Distribution of Fornax A: Leptonic and Hadronic Production of High Energy Emission from the Radio Lobes
• Constraining anisotropic models of the early Universe with WMAP9 data
• Constraining Supersymmetry using the relic density and the Higgs boson
• Existence of bulk viscous universe in $f(R,T)$ gravity and confrontation with observational data
• Searching for Modified Gravity: Scale and Redshift Dependent Constraints from Galaxy Peculiar Velocities
• Large-Scale Structure Observables in General Relativity
• How Cold is Cold Dark Matter?
• Constraints on the Distance Moduli, Helium and Metal Abundances, and Ages of Globular Clusters from their RR Lyrae and Non-Variable Horizontal-Branch Stars. I. M3, M15, and M92
• Information Gains from Cosmic Microwave Background Experiments
• Supervoids in the WISE-2MASS catalogue imprinting Cold Spots in the Cosmic Microwave Background
• Observational Constraints on Monomial Warm Inflation
• Phantom cosmological model with observational constraints in $f(Q)$ gravity
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for the eBOSS Emission Line Galaxy Sample
• Model-independent determination of curvature parameter by using $H(z)$ and $D_A(z)$ data pair from BAO measurement
• Baryons do trace dark matter 380,000 years after the big bang: Search for compensated isocurvature perturbations with WMAP 9-year data
• Precise Measurements of Primordial Power Spectrum with 21 cm Fluctuations
• Cosmological Parameters from pre-Planck CMB Measurements: a 2017 Update
• Radiogenic p-isotopes from SNIa, nuclear physics uncertainties and Galactic chemical evolution compared with values in primitive meteorites
• Observed parity-odd CMB temperature bispectrum
• Dipolar modulation in number counts of WISE-2MASS sources
• Latest astronomical constraints on some nonlinear parametric dark energy models
• Testing gravity on large scales by combining weak lensing with galaxy clustering using CFHTLenS and BOSS CMASS
• Order out of Randomness : Self-Organization Processes in Astrophysics
• Cosmogenic Activation of Materials Used in Rare Event Search Experiments
• Analytical models of supermassive black holes in galaxies surrounded by dark matter halos
• A 3-D model of polarised dust emission in the Milky Way
• The Cosmic Microwave Background: The history of its experimental investigation and its significance for cosmology
• Pole Inflation - Shift Symmetry and Universal Corrections
• Constraints on modified gravity from Planck 2015: when the health of your theory makes the difference
• Connecting neutrino physics with dark matter
• The Simons Observatory Large Aperture Telescope Receiver
• The significance of anisotropic signals hiding in the type Ia supernovae
• On the scalar consistency relation away from slow roll
• Testing statistics of the CMB B-mode polarization toward unambiguously establishing quantum fluctuation of vacuum
• Planck constraints on scalar-tensor cosmology and the variation of the gravitational constant
• Benchmark ages for the Gaia benchmark stars
• Quantifying Tensions between CMB and Distance Datasets in Models with Free Curvature or Lensing Amplitude
• Warm-hot Gas in X-ray Bright Galaxy Clusters and the H I-deficient Circumgalactic Medium in Dense Environments
• Does Current Data Prefer a Non-minimally Coupled Inflaton?
• The Knotted Sky I: Planck constraints on the primordial power spectrum
• Weighing obscured and unobscured quasar hosts with the CMB
• Testing deviations from $\Lambda$CDM with growth rate measurements from 6 Large Scale Structure Surveys at $\mathbf{z}=0.06$ to 1
• Radiative Lepton Model and Dark Matter with Global $U(1{)}^{\prime }$ Symmetry
• Localisation of directional scale-discretised wavelets on the sphere
• KiDS & Euclid: Cosmological implications of a pseudo angular power spectrum analysis of KiDS-1000 cosmic shear tomography
• First-order thermodynamics of Horndeski gravity
• Bayesian inflationary reconstructions from Planck 2018 data
• Using Large Scale Structure to test Multifield Inflation
• Spectroscopically Confirmed Lyman-Alpha Emitters from Redshift 5 to 7 Behind Ten Galaxy Cluster Lenses
• Constraining f(R) gravity with PLANCK data on galaxy cluster profiles
• Suite of Hydrodynamical Simulations for the Lyman-Alpha Forest with Massive Neutrinos
• Planck intermediate results. XXV. The Andromeda Galaxy as seen by Planck
• Large-scale CMB temperature and polarization cross-spectra likelihoods
• First Results from COPSS: The CO Power Spectrum Survey
• Consistency of Planck, ACT and SPT constraints on magnetically assisted recombination and forecasts for future experiments
• Constraints and tensions in testing general relativity from Planck and CFHTLenS including intrinsic alignment systematics
• Pressure Parametrization of Dark Energy: First and Second-Order Constraints with Latest Cosmological Data
• Star formation history and metallicity in the Galactic inner bulge revealed by the red giant branch bump
• Generating primordial features at large scales in two field models of inflation
• Implications of Feebly Interacting Dark Sector on Neutron Star Properties and Constraints from GW170817
• A review of unsupervised learning in astronomy
• Accelerated Universes from type IIA Compactifications
• Limits on primordial non-Gaussianities from BOSS galaxy-clustering data
• Planck CMB Anomalies: Astrophysical and Cosmological Secondary Effects and the Curse of Masking
• Cosmic troublemakers: the Cold Spot, the Eridanus Supervoid, and the Great Walls
• Comprehensive analysis of the simplest curvaton model
• Inflation, the Hubble Tension and Early Dark Energy: an alternative overview
• One-loop corrections to neutralino-stop coannihilation revisited
• The Positron Puzzle
• On the dissection of degenerate cosmologies with machine learning
• Search for features in the spectrum of primordial perturbations using Planck and other datasets
• Practical Modeling of Large-Scale Galactic Magnetic Fields: Status and Prospects
• Quijote-PNG: Simulations of primordial non-Gaussianity and the information content of the matter field power spectrum and bispectrum
• 2MTF V. Cosmography, Beta, and the residual bulk flow
• Light Sterile Neutrinos in Cosmology and Short-Baseline Oscillation Experiments
• Robust Field-level Likelihood-free Inference with Galaxies
• The trouble with Hubble: Local versus global expansion rates in inhomogeneous cosmological simulations with numerical relativity
• Alleviating both $H_0$ and ${\sigma }_8$ tensions in Tsallis cosmology
• G181.1+9.5, a new high-latitude low-surface brightness supernova remnant
• On Recent Claims Concerning the R_h=ct Universe
• The flickering nuclear activity of Fornax A
• Strong Planck constraints on braneworld and non-commutative inflation
• A three-loop radiative neutrino mass model with dark matter
• Conformally Friedmann-Lemaitre-Robertson-Walker cosmologies
• Three problems about multi-scale modelling in cosmology
• Four-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: On-sky Receiver Performance at 40, 90, 150, and 220 GHz Frequency Bands
• Cosmological distance indicators
• Probing Compressed Sleptons at the LHC using Vector Boson Fusion Processes
• Anomalous Dimensions and Non-Gaussianity
• Integrated Sachs-Wolfe effect in massive bigravity
• On Modeling and Measuring the Temperature of the z~5 IGM
• Model-independent analyses of non-Gaussianity in Planck CMB maps using Minkowski Functionals
• Joint resonant CMB power spectrum and bispectrum estimation
• Realistic estimation for the detectability of dark matter sub-halos with Fermi-LAT
• Testing General Relativity with Growth rate measurement from Sloan Digital Sky Survey III Baryon Oscillations Spectroscopic Survey galaxies
• Complex Scalar DM in a B-L Model
• On the stability and causality of scalar-vector theories
• Anisotropic Inflation with the non-Vacuum Initial State
• Supermassive black holes in disk-dominated galaxies outgrow their bulges and co-evolve with their host galaxies
• Constraints on dark radiation from cosmological probes
• Friction in Gravitational Waves: a test for early-time modified gravity
• Evidence of a truncated spectrum in the angular correlation function of the cosmic microwave background
• Chasing Lyman alpha-emitting galaxies at z = 8.8
• SUSY-QCD corrections to stop annihilation into electroweak final states including Coulomb enhancement effects
• A minimal power-spectrum-based moment expansion for CMB B-mode searches
• Non-universal gaugino masses and semi-natural supersymmetry in view of the Higgs boson discovery
• Quintessence with Yukawa Interaction
• Probing gravity at large scales through CMB lensing
• Quantifying the global "CMB tension" between the Atacama Cosmology Telescope and the Planck satellite in extended models of cosmology
• Interpreting the Global 21-cm Signal from High Redshifts. I. Model Independent Constraints
• Electroweak Phase Transition in Non-Minimal Higgs Sectors
• Characterization of Population III Stars with Stellar Atmosphere and Evolutionary Modeling and Predictions of their Observability with the James Webb Space Telescope
• Parametrized modified gravity constraints after Planck
• The isotropic radio background revisited
• Gravitational wave spectra from oscillon formation after inflation
• CMB Scale Dependent Non-Gaussianity from Massive Gravity during Inflation
• Erasing the variable: Empirical foreground discovery for global 21 cm spectrum experiments
• Chandra Survey of Nearby Highly Inclined Disc Galaxies - III: Comparison with Hydrodynamical Simulations of Circumgalactic Coronae
• The BINGO telescope: a new instrument exploring the new 21-cm cosmology window
• Limit on the population of repeating fast radio bursts from the ASKAP/CRAFT lat50 survey
• The galaxy cluster outskirts probed by Chandra
• Spin-dependent exotic interactions
• The bispectrum of polarized galactic foregrounds
• Limits on the cosmic neutrino background
• The DES view of the Eridanus supervoid and the CMB Cold Spot
• The Spectral Energy Distributions of Active Galactic Nuclei
• The Simons Observatory: gain, bandpass and polarization-angle calibration requirements for B-mode searches
• Anisotropy of the galaxy cluster X-ray luminosity-temperature relation
• Foreground Biases on Primordial Non-Gaussianity Measurements from the CMB Temperature Bispectrum: Implications for Planck and Beyond
• Comparison between hemisphere comparison method and dipole-fitting method in tracing the anisotropic expansion of the Universe use the Union2 dataset
• Constraining the anisotropy of the Universe via Pantheon supernovae sample
• Constraining the initial conditions of the Universe using large scale structure
• On the distribution of the critical values of random spherical harmonics
• The cosmological impact of future constraints on $H_0$ from gravitational-wave standard sirens
• Measuring Infrared Surface Brightness Fluctuation Distances with HST WFC3: Calibration and Advice
• The Spectral Energy Distributions of Active Galactic Nuclei
• What is the Halo Mass Function in a Fuzzy Dark Matter Cosmology?
• The 500 ks Chandra observation of the z = 6.31 QSO SDSS J1030+0524
• Large-scale Cosmic Flows from Cosmicflows-2 Catalog
• Primordial Anisotropies in Gauged Hybrid Inflation
• Evidence for a high-z ISW signal from supervoids in the distribution of eBOSS quasars
• Large angular scale multipoles at redshift ~0.8
• The Contribution of Halos with Different Mass Ratios to the Overall Growth of Cluster-Sized Halos
• Revisiting the distance to radio Loops I and IV using Gaia and radio/optical polarization data
• QuickPol: Fast calculation of effective beam matrices for CMB polarization
• Theoretical uncertainty of the supersymmetric dark matter relic density from scheme and scale variations
• Can small-scale baryon inhomogeneities resolve the Hubble tension? An investigation with ACT DR4
• Cosmic inflation in a landscape of heavy-fields
• Leptogenesis in SO(10)
• Probing spatial homogeneity with LTB models: a detailed discussion
• Varying fundamental constants principal component analysis: additional hints about the Hubble tension
• Big Bang Nucleosynthesis with an Inhomogeneous Primordial Magnetic Field Strength
• BeyondPlanck III. Commander3
• $H_0$ Tension and the Phantom Regime: A Case Study In Terms of an Infrared $f(T)$ Gravity
• Quantifying Concordance in Cosmology
• CMB reconstruction from the WMAP and Planck PR2 data
• Impact of Polarized Galactic Foreground Emission on CMB Lensing Reconstruction and Delensing of B-Modes
• A CubeSat for Calibrating Ground-Based and Sub-Orbital Millimeter-Wave Polarimeters (CalSat)
• Dynamical dark energy confronted with multiple CMB missions
• Including birefringence into time evolution of CMB: current and future constraints
• Planck intermediate results. LII. Planet flux densities
• Primordial spectra from sudden turning trajectory
• Constraining anisotropy of the universe from different groups of type-Ia supernovae
• Complementarity of Dark Matter Searches at Resonance
• Galaxy clustering, CMB and supernova data constraints on $\varphi$CDM model with massive neutrinos
• Constraints on the temperature of the intergalactic medium at z=8.4 with 21-cm observations
• Limits on statistical anisotropy from BOSS DR12 galaxies using bipolar spherical harmonics
• LHC search for di-Higgs decays of stoponium and other scalars in events with two photons and two bottom jets
• Comparing Planck and WMAP: Maps, Spectra, and Parameters
• Spherically symmetric Einstein-aether perfect fluid models
• An effective description of Laniakea: impact on cosmology and the local determination of the Hubble constant
• FLRW cosmology with EDSFD parametrization
• Cosmic Inflation at the Crossroads
• Two-point Correlation Function of WMAP 9 year data
• C-Band All-Sky Survey: A First Look at the Galaxy
• Impact of anisotropic stress of free-streaming particles on gravitational waves induced by cosmological density perturbations
• A Projected Estimate of the Reionization Optical Depth Using the CLASS Experiment's Sample-Variance Limited E-Mode Measurement
• Starobinsky-Type Inflation from ${\alpha }^{\prime }$-Corrections
• First detection of a virial shock with SZ data: implication for the mass accretion rate of Abell 2319
• The Atacama Cosmology Telescope: Microwave Intensity and Polarization Maps of the Galactic Center
• Polarized anisotropic spectral distortions of the CMB: Galactic and extragalactic constraints on photon-axion conversion
• Testing cosmic anisotropy with Pantheon sample and quasars at high redshifts
• Cosmoglobe DR1 results. II. Constraints on isotropic cosmic birefringence from reprocessed WMAP and Planck LFI data
• Robustness of cosmic neutrino background detection in the cosmic microwave background
• Baryonic feedback biases on fundamental physics from lensed CMB power spectra
• Dark sector searches with the CMS experiment
• Primordial Magnetic Helicity Constraints from WMAP Nine-Year Data
• Measuring the reionization optical depth without large-scale CMB polarization
• Searching for primordial localized features with CMB and LSS spectra
• Cosmological solutions to the Lithium problem: Big-bang nucleosynthesis with photon cooling, $X$-particle decay and a primordial magnetic field
• Imprint of entanglement entropy in the power spectrum of inflationary fluctuations
• Simulated forecasts for primordial B-mode searches in ground-based experiments
• Kantowski-Sachs Einstein-Aether Scalar Field Cosmological Models
• Pre - Inflationary Clues from String Theory ?
• The Tip of the Red Giant Branch Distances to Type Ia Supernova Host Galaxies. III. NGC 4038/39 and NGC 5584
• Polytropic dark matter flows illuminate dark energy and accelerated expansion
• The Atacama Cosmology Telescope: Cross Correlation with Planck maps
• SBI++: Flexible, Ultra-fast Likelihood-free Inference Customized for Astronomical Applications
• Measurement of the pairwise kinematic Sunyaev-Zeldovich effect with Planck and BOSS data
• Dark Radiation and Inflationary Freedom after Planck 2015
• Constraints on the Early and Late Integrated Sachs-Wolfe effects from Planck 2015 Cosmic Microwave Background Anisotropies angular power spectra
• Prediction of Supernova Rates in Known Galaxy-galaxy Strong-lens Systems
• Alignments of parity even/odd-only multipoles in CMB
• Constraints on hidden photons from current and future observations of CMB spectral distortions
• Signals of Leptophilic Dark Matter at the ILC
• Light propagation in inhomogeneous and anisotropic cosmologies
• First Constraints on Compact Dark Matter from Fast Radio Burst Microstructure
• Lagrangian Formulation of Stochastic Inflation: A Recursive Approach
• Foreground-Induced Biases in CMB Polarimeter Self-Calibration
• Inflationary Potential as seen from Different Angles: Model Compatibility from Multiple CMB Missions
• Information Gains from Cosmological Probes
• Prospects for the Detection of Fast Radio Bursts with the Murchison Widefield Array
• The intrinsic B-mode polarisation of the Cosmic Microwave Background
• A paradigm of warm quintessential inflation and production of relic gravity waves
• Scale-invariant helical magnetic field evolution and the duration of inflation
• The WISE-2MASS Survey: Red Quasars Into the Radio Quiet Regime
• Is there evidence for additional neutrino species from cosmology?
• Spatially Homogeneous Einstein-Aether Cosmological Models: Scalar Fields with a Generalized Harmonic Potential
• Disentangling the $f(R)$ - Duality
• The Cosmology Large Angular Scale Surveyor (CLASS): 38 GHz detector array of bolometric polarimeters
• Brane inflation driven by noncanonical scalar field
• ALMA photometry of extragalactic radio sources
• Baryon acoustic oscillations reconstruction using convolutional neural networks
• Feeble DM-SM Interaction via New Scalar and Vector Mediators in Rotating Neutron Stars
• Non-local bias in the halo bispectrum with primordial non-Gaussianity
• Search for anomalous alignments of structures in Planck data using Minkowski Tensors
• Cosmological constraints to dark matter with two- and many-body decays
• The multipole expansion of the local expansion rate
• Strong evidence of Anomalous Microwave Emission from the flux density spectrum of M31
• Absolutely calibrated radio polarimetry of the inner Galaxy at 2.3 GHz and 4.8 GHz
• Masses, mixing angles and phases of general Majorana neutrino mass matrix
• On the current status of Modified Gravity
• An optimal estimator for resonance bispectra in the CMB
• Multifrequency study of GHz-peaked spectrum sources
• The Simons Observatory: Galactic Science Goals and Forecasts
• Inflationary Freedom and Cosmological Neutrino Constraints
• The Ellipsoidal Universe in the Planck Satellite Era
• Constraining the dynamical dark energy parameters: Planck-2013 vs WMAP9
• Cross-correlation of galaxies and galaxy clusters in the Sloan Digital Sky Survey and the importance of non-Poissonian shot noise
• Examining the consistency relations describing the three-point functions involving tensors
• Power Spectra Based Planck Constraints on Compensated Isocurvature, and Forecasts for LiteBIRD and CORE Space Missions
• AMICO galaxy clusters in KiDS-DR3: cosmological constraints from large-scale stacked weak lensing profiles
• Neutrino mu-tau reflection symmetry and its breaking in the minimal seesaw
• Using the cosmological recombination radiation to probe early dark energy and fundamental constant variations
• Probing cosmic birefringence with polarized Sunyaev-Zel'dovich tomography
• CMB Anomalies and the Hubble Tension
• First observational constraints on tensor non-Gaussianity sourced by primordial magnetic fields from cosmic microwave background
• Efficient sampling of constrained high-dimensional theoretical spaces with machine learning
• The Global Magneto-Ionic Medium Survey: A Faraday Depth Survey of the Northern Sky Covering 1280-1750 MHz
• Testing the Prediction of Fuzzy Dark Matter Theory in the Milky Way Center
• Polarized accretion shocks from the cosmic web
• Parameter splitting in dark energy: is dark energy the same in the background and in the cosmic structures?
• Modelling the Accelerating Universe with $f(Q)$ Gravity: Observational Consistency
• No scale SUGRA SO(10) derived Starobinsky Model of Inflation
• Fast Weak Lensing Simulations with Halo Model
• Multicomponent dark matter in extended $U(1{)}_{B-L}$: neutrino mass and high scale validity
• Is Dark Energy Dynamical in the DESI Era? A Critical Review
• $B$-mode forecast of CMB-Bh$\overline{a}$rat
• Cosmological Structure Formation in Decaying Dark Matter Models
• Statistical tests of sterile neutrinos using cosmology and short-baseline data
• Baryons still trace dark matter: probing CMB lensing maps for hidden isocurvature
• Cosmological Solutions in Multiscalar Field Theory
• Determination of the Cosmic Infrared Background from COBE/FIRAS and Planck HFI Observations
• High precision modeling of polarized signals: Moment expansion method generalized to spin-2 fields
• A stabilization mechanism for excited fermion-boson stars
• Lectures on Inflation
• Searching for features of a string-inspired inflationary model with cosmological observations
• Tests of Gravity with Galaxy Clusters
• The Cosmic Equation of State
• Circular polarization of the CMB: Foregrounds and detection prospects
• The lensing properties of subhaloes in massive elliptical galaxies in sterile neutrino cosmologies
• Gravitino LSP and leptogenesis after the first LHC results
• New thresholds for Primordial Black Hole formation during the QCD phase transition
• The Fan Region at 1.5 GHz. I: Polarized synchrotron emission extending beyond the Perseus Arm
• Vacuum and Gravitons of Relic Gravitational Waves, and Regularization of Spectrum and Energy-Momentum Tensor
• Magneto-reheating constraints from curvature perturbations
• Fast Bayesian inference for slow-roll inflation
• The Effects of Varying Cosmological Parameters on Halo Substructure
• Anomalies in the CMB from a cosmic bounce
• A particle dark matter footprint on the first generation of stars
• A systematic procedure to build the beyond generalized Proca field theory
• Magnetic field spectrum at cosmological recombination revisited
• CMB anisotropies generated by a stochastic background of primordial magnetic fields with non-zero helicity
• Reaffirming the Cosmic Acceleration without Supernova and CMB
• Axion cold dark matter: status after Planck and BICEP2
• Measuring a Charge-Coupled Device Point Spread Function: Euclid Visible Instrument CCD273-84 PSF Performance
• Exotic see-saw mechanism for neutrinos and leptogenesis in a Pati-Salam model
• Massive quiescent galaxies at $z\sim 3$: a comparison of selection, stellar population and structural properties with simulation predictions
• Connecting inflation with late cosmic acceleration by particle production
• The refractive index of relic gravitons
• BeyondPlanck I. Global Bayesian analysis of the Planck Low Frequency Instrument data
• Fluctuations of the total number of critical points of random spherical harmonics
• Cosmological evidence for leptonic asymmetry after Planck
• Local analyses of Planck maps with Minkowski Functionals
• Detection of Spectral Variations of Anomalous Microwave Emission with QUIJOTE and C-BASS
• Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: 40 GHz Telescope Pointing, Beam Profile, Window Function, and Polarization Performance
• Tensor Minkowski Functionals for random fields on the sphere
• Star clusters in M33: updated UBVRI photometry, ages, metallicities, and masses
• High $H_0$ Values from CMB E-mode Data: A Clue for Resolving the Hubble Tension?
• Optimal scan strategies for future CMB satellite experiments
• Leptogenesis in an SU(5) x A5 Golden Ratio Flavour Model
• Testing the homogeneity of the Universe using gamma-ray bursts
• Probing the thermal history during reionization using a semi-numerical photon-conserving code SCRIPT
• Inflation in a two 3-form fields scenario
• The Effect of Large-Scale Structure on the Magnification of High-Redshift Sources by Cluster-Lenses
• Polarization Predictions for Inflationary CMB Power Spectrum Features
• Surfing gravitational waves: can bigravity survive growing tensor modes?
• One-loop corrections to gaugino (co-)annihilation into quarks in the MSSM
• Inflating an Inhomogeneous Universe
• Neutrino phenomenology and scalar Dark Matter with $A_4$ flavor symmetry in Inverse and type II seesaw
• A direct measure of free electron gas via the Kinematic Sunyaev-Zel'dovich effect in Fourier-space analysis
• The information content of cosmic microwave background anisotropies
• The Resolved Sunyaev--Zel'dovich Profiles of Nearby Galaxy Groups
• Sound speed of scalar field dark energy: weak effects and large uncertainties
• Non-Gaussian Error Distributions of LMC Distance Moduli Measurements
• Cosmological signatures of tilted isocurvature perturbations: reionization and 21cm fluctuations
• A Bayesian analysis of inflationary primordial spectrum models using Planck data
• Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension
• A search for cosmic topology in the final WMAP data
• Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: A Measurement of Circular Polarization at 40 GHz
• On-sky performance of the CLASS Q-band telescope
• Dispu$\tau$able: the high cost of a low optical depth
• Joint Planck and WMAP Assessment of Low CMB Multipoles
• Post LHC8 SUSY benchmark points for ILC physics
• Measurement of the integrated Sachs-Wolfe effect using the AllWISE data release
• One line to run them all: SuperEasy massive neutrino linear response in $N$-body simulations
• BeyondPlanck XIII. Intensity foreground sampling, degeneracies, and priors
• Vector dark boson mediated feeble interaction between fermionic dark matter and strange quark matter in quark stars
• Millicharged Relics Reveal Massless Dark Photons
• Cluster counts: calibration issue or new physics?
• Physics of the cosmic microwave background anisotropy
• LiteBIRD Science Goals and Forecasts. A Case Study of the Origin of Primordial Gravitational Waves using Large-Scale CMB Polarization
• Bayesian analysis of inflationary features in Planck and SDSS data
• Study of the Inflationary Spectrum in the Presence of Quantum Gravity Corrections
• A model-independent fit to Planck and BICEP2 data
• Cosmic Decoherence: Massive Fields
• BICEP2 / Keck Array XI: Beam Characterization and Temperature-to-Polarization Leakage in the BK15 Dataset
• Corpuscular slow-roll inflation
• A Comparison of Maps and Power Spectra Determined from South Pole Telescope and Planck Data
• Multi-Clustering Needlet-ILC for CMB B-modes component separation
• Multi-resolution Bayesian CMB component separation through Wiener-filtering with a pseudo-inverse preconditioner
• Revisiting the impact of neutrino mass hierarchies on neutrino mass constraints in light of recent DESI data
• De Sitter vacua from a D-term generated racetrack potential in hypersurface Calabi-Yau compactifications
• Constraints on the Distance Moduli, Helium and Metal Abundances, and Ages of Globular Clusters From Their RR Lyrae and Non-Variable Horizontal-Branch Stars. III. M55 and NGC 6362
• A cryogenic continuously rotating half-wave plate for the POLARBEAR-2b cosmic microwave background receiver
• A Model for Pseudo-Dirac Neutrinos: Leptogenesis and Ultra-High Energy Neutrinos
• Molecular Chemistry for Dark Matter II: Recombination, Molecule Formation, and Halo Mass Function in Atomic Dark Matter
• Dark Energy: The Shadowy Reflection of Dark Matter?
• Observational Constraints on Warm Inflation in Loop Quantum Cosmology
• A deep Parkes HI survey of the Sculptor group and filament: HI mass function and environment
• Magnetic Misalignment of Interstellar Dust Filaments
• A new probe of Axion-Like Particles: CMB polarization distortions due to cluster magnetic fields
• Assessing Consistency Between WMAP 9-year and Planck 2015 Temperature Power Spectra
• de Sitter Space is Unstable in Quantum Gravity
• Constraining holographic cosmology using Planck data
• Tight framelets and fast framelet filter bank transforms on manifolds
• MCSED: A flexible spectral energy distribution fitting code and its application to $z\sim 2$ emission-line galaxies
• Determining thermal dust emission from Planck HFI data using a sparse, parametric technique
• Derivation of an Analytical Approximation of the Spectrum of Spinning Dust Emission
• Constraints on the spectral index of polarized synchrotron emission from WMAP and Faraday-corrected S-PASS data
• Reconciling galaxy cluster shapes, measured by theorists vs observers
• Separating astrophysical sources from indirect dark matter signals
• Direction dependence of cosmological parameters due to cosmic hemispherical asymmetry
• In-flight polarization angle calibration for LiteBIRD: blind challenge and cosmological implications
• Recovery of Large Angular Scale CMB Polarization for Instruments Employing Variable-delay Polarization Modulators
• Globular Clusters and Spur Clusters in NGC 4921, the Brightest Spiral Galaxy in the Coma Cluster
• Dark chiral symmetry breaking and the origin of the electroweak scale
• Light of Planck-2015 on Non-Canonical Inflation
• Tsallis holographic model of dark energy: Cosmic behaviour, statefinder analysis and ${\omega }_D-{\omega }_D^{\prime }$ pair in the non-flat universe
• A note on interacting holographic dark energy with a Hubble-scale cutoff
• Characterization of the polarized synchrotron emission from Planck and WMAP data
• The paradigm of warm quintessential inflation and spontaneous baryogenesis
• The Feasibility of Magnetic Reconnection Powered Blazar Flares from Synchrotron Self-Compton Emission
• A framework for testing isotropy with the cosmic microwave background
• Constraining the mass of fermionic dark matter from its feeble interaction with hadronic matter via dark mediators in neutron stars
• SUSY-QCD corrections for the direct detection of neutralino dark matter and correlations with the relic density
• HIFLUGCS: X-ray luminosity -- dynamical mass relation and its implications for mass calibrations with the SPIDERS and 4MOST surveys
• Peering through the dust II: $XMM-Newton$ observations of two additional FIRST-2MASS red quasars
• Inner radius and energy conditions of dark matter halos surrounding Schwarzschild black holes
• Bispectrum from open inflation
• Disentangling the Faraday rotation sky
• A comparison of CMB Angular Power Spectrum Estimators at Large Scales: the TT case
• North-South non-Gaussian asymmetry in PLANCK CMB maps
• Numerical evaluation of the three-point scalar-tensor cross-correlations and the tensor bi-spectrum
• Dark Matter on Top
• A tomographic test of cosmological principle using the JLA compilation of type Ia supernovae
• Leptogenesis in an SU(5) x A5 Golden Ratio Flavour Model: Addendum
• Measuring the Largest Angular Scale CMB B-mode Polarization with Galactic Foregrounds on a Cut Sky
• Spatial Curvature in $f(R)$ Gravity
• Living with Neighbors. II. Statistical Analysis of Flybys and Mergers of Dark Matter Halos in Cosmological Simulations
• Angular Correlation Functions for Models with Logarithmic Oscillations
• Angular Power Spectra with Finite Counts
• Interacting $F(R,T)$ gravity with modified Chaplygin gas
• Primordial features from ekpyrotic bounces
• Are $R^2$- and Higgs-inflations really unlikely?
• The deep Chandra survey in the SDSS J1030+0524 field
• Plane symmetric model in $f(R,T)$ gravity
• Imprints of interacting dark energy on cosmological perturbations
• The bispectra of galactic CMB foregrounds and their impact on primordial non-Gaussianity estimation
• A Neural-Network based estimator to search for primordial non-Gaussianity in Planck CMB maps
• Deciphering Residual Emissions: Time-Dependent Models for the Non-Thermal Interstellar Radiation from the Milky Way
• The Cosmology Large Angular Scale Surveyor Receiver Design
• Analytical investigation of pre-inflationary effects in the primordial power spectrum: From General Relativity to hybrid Loop Quantum Cosmology
• Modified theory of gravity and the history of cosmic evolution
• The traces of anisotropic dark energy in light of Planck
• Minkowski Functionals of CMB polarisation intensity with Pynkowski: theory and application to Planck and future data
• Role of trans-Planckian modes in cosmology
• Relating the inhomogeneous power spectrum to the CMB hemispherical anisotropy
• The $z<1.2$ optical luminosity function from a sample of $\sim 410000$ galaxies in bootes
• Inflationary susceptibilities, duality and large-scale magnetic fields generation
• Observational Constraints on Varying-alpha Domain Walls
• The cosmic shallows I: interaction of CMB photons in extended galaxy halos
• Stochastic gravitational-wave background from spin loss of black holes
• Effect of Template Uncertainties on the WMAP and Planck Measures of the Optical Depth Due To Reionization
• Primordial Non-Gaussianity and Reionization
• Modified cosmology from quantum deformed entropy
• The impact of line-of-sight structures on measuring $H_0$ with strong lensing time-delays
• Angular dependence of primordial trispectra and CMB spectral distortions
• Neutrino Masses and Leptogenesis in Type I+II Seesaw Models
• Reduced modified Chaplygin gas cosmology
• Integrated Sachs-Wolfe-galaxy cross-correlation bounds on the two branches of the minimal theory of massive gravity
• Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
• CMB constraints on running non-Gaussianity
• Characterizing unknown systematics in large scale structure surveys
• No evidence for dynamical dark energy in two models
• Phenomenological approaches of inflation and their equivalence
• UV completion of the Starobinsky model, tensor-to-scalar ratio, and constraints on non-locality
• An Improved Diffuse Foreground Subtraction by ILC method: CMB Map and Angular Power Spectrum using Planck and WMAP Observations
• Baryon content and dynamic state of galaxy clusters: XMM-Newton observations of A1095 and A1926
• Improvement of energy-momentum tensor and non-Gaussianities in holographic cosmology
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• BeyondPlanck VII. Bayesian estimation of gain and absolute calibration for CMB experiments
• Non-Gaussian Error Distribution of ${}^7\mathrm{Li}$ Abundance Measurements
• A global view on star formation: The GLOSTAR Galactic plane survey VIII. Formaldehyde absorption in Cygnus~X
• Preference for a Vanishingly Small Cosmological Constant in Supersymmetric Vacua in a Type IIB String Theory Model
• Light Sterile Neutrinos and Inflationary Freedom
• COMAP Early Science: VI. A First Look at the COMAP Galactic Plane Survey
• Testing cosmic anisotropy with Pade approximation and Pantheon+ sample
• Cosmic-rays, gas, and dust in nearby anti-centre clouds : III -- Dust extinction, emission, and grain properties
• Progress in the Global Modeling of the Galactic Magnetic Field
• The Impact of Non-Gaussianity upon Cosmological Forecasts
• QUIJOTE scientific results -- VIII. Diffuse polarized foregrounds from component separation with QUIJOTE-MFI
• Testing the $n_s-H_0$ scaling relation with Planck-independent CMB data
• Dust polarization spectral dependence from Planck HFI data. Turning point on CMB polarization foregrounds modelling
• Exploring cosmic origins with CORE: mitigation of systematic effects
• Phenomenological study of neutrino mass, dark matter and baryogenesis within the framework of minimal extended seesaw
• Reionization Histories of Milky Way Mass Halos
• Late-time vacuum phase transitions: Connecting sub-eV scale physics with cosmological structure formation
• The coherent magnetic field of the Milky Way halo, Local Bubble and Fan Region
• Evolution of the Stellar Mass Function and Infrared Luminosity Function of Galaxies since $z=1.2$
• Imprint of Inhomogeneous and Anisotropic Primordial Power Spectrum on CMB Polarization
• Regge calculus models of closed lattice universes
• Probing frequency-dependent half-wave plate systematics for CMB experiments with full-sky beam convolution simulations
• Accretion History of AGN III: Radiative Efficiency and AGN Contribution to Reionization
• The C-Band All-Sky Survey (C-BASS): Template Fitting of Diffuse Galactic Microwave Emission in the Northern Sky
• Calibration of Transition-edge Sensor (TES) Bolometer Arrays with Application to CLASS
• Lack-of-correlation anomaly in CMB large scale polarisation maps
• Constraining isocurvature perturbations with the 21cm emission from minihaloes
• BICEP / Keck XII: Constraints on axion-like polarization oscillations in the cosmic microwave background
• A novel CMB polarization likelihood package for large angular scales built from combined WMAP and Planck LFI legacy maps
• Model-Independent Measurements of Cosmic Expansion and Growth at z=0.57 Using the Anisotropic Clustering of CMASS Galaxies From the Sloan Digital Sky Survey Data Release 9
• Foreground model recognition through Neural Networks for CMB B-mode observations
• $\mu$-Hybrid Inflation with Low Reheat Temperature and Observable Gravity Waves
• Understanding the environment around the intermediate mass black hole candidate ESO 243-49 HLX-1
• Pure E and B polarization maps via Wiener filtering
• On the impact of large angle CMB polarization data on cosmological parameters
• Breaking cosmic degeneracies: Disentangling neutrinos and modified gravity with kinematic information
• Constraining the anisotropy of the Universe with the X-ray and UV fluxes of quasars
• Power Spectrum of Inflationary Attractors
• Analytic Formulae for Inflationary Correlators with Dynamical Mass
• Sun-Earth Lagrange reference for fundamental physics and navigation
• Quantifying the Origin and Distribution of Intracluster Light in a Fornax-like Cluster
• Constraints on non-resonant photon-axion conversion from the Planck satellite data
• Scaling ansatz with texture zeros in linear seesaw
• Cosmoglobe DR1 results. I. Improved Wilkinson Microwave Anisotropy Probe maps through Bayesian end-to-end analysis
• BeyondPlanck XI. Bayesian CMB analysis with sample-based end-to-end error propagation
• A new polarisation amplitude bias reduction method
• Sharp inflaton potentials and bi-spectra: Effects of smoothening the discontinuity
• Combined constraints on deviations of dark energy from an ideal fluid from Euclid and Planck
• The Kullback-Leibler Divergence as an Estimator of the Statistical Properties of CMB Maps
• Searching for primordial non-Gaussianity in Planck CMB maps using a combined estimator
• The SRG-eROSITA All-Sky Survey : Constraints on f(R) Gravity from Cluster Abundance
• Split NMSSM with electroweak baryogenesis
• High-resolution spectroscopy of gaseous ${}^{83m}$Kr conversion electrons with the KATRIN experiment
• A magnetised Galactic halo from inner Galaxy outflows
• Flavored leptogenesis with quasi degenerate neutrinos in a broken cyclic symmetric model
• BeyondPlanck XII. Cosmological parameter constraints with end-to-end error propagation
• Universe opacity and CMB
• An ultra-deep multi-band VLA survey of the faint radio sky (COSMOS-XS): New constraints on the cosmic star formation history
• Evidence of isotropy at large-scale from polarizations of radio sources
• From BeyondPlanck to Cosmoglobe: Preliminary $WMAP$ $Q$-band analysis
• Running primordial perturbations: Inflationary Dynamics and Observational Constraints
• Dark Energy Constraints in light of Pantheon SNe Ia, BAO, Cosmic Chronometers and CMB Polarization and Lensing Data
• Testing the cosmic distance duality relation with Type Ia supernova and transverse BAO measurements
• Cool-Core Cycles and Phoenix
• Current constraints on early and stressed dark energy models and future 21 cm perspectives
• The relation between cosmological redshift and scale factor for photons
• Lumped element kinetic inductance detectors maturity for space-borne instruments in the range between 80 and 180 GHz
• The C-Band All-Sky Survey (C-BASS): Constraining diffuse Galactic radio emission in the North Celestial Pole region
• Removing the ISW-lensing bias from the local-form primordial non-Gaussianity estimation
• The redshift-space galaxy two-point correlation function and baryon acoustic oscillations
• Cosmological Constraints on Ghost Dark Energy in the Brans-Dicke Theory by Using MCMC Approach
• Corrections to $n_s$ and $n_t$ from high scale physics
• Gamma-ray burst cosmology: Hubble diagram and star formation history
• Constraining the cosmic UV background at z>3 with MUSE Lyman-α emission observations
• The VVV survey: Long-period variable stars I. Photometric catalog of ten VVV/OGLE tiles
• Cosmological Probes of Structure Growth and Tests of Gravity
• Exploring the Growth Index ${\gamma }_L$: Insights from Different CMB Dataset Combinations and Approaches
• Impact of half-wave plate systematics on the measurement of cosmic birefringence from CMB polarization
• Polarized Synchrotron Foreground Assessment for CMB Experiments
• BeyondPlanck VI. Noise characterization and modelling
• Deconstructing the Planck TT Power Spectrum to Constrain Deviations from $\Lambda$CDM
• Calibration of a star formation and feedback model for cosmological simulations with Enzo
• Post-inflationary thermal histories and the refractive index of relic gravitons
• Determining $H_0$ with the latest HII galaxy measurements
• Optimal CMB estimators for bispectra from excited states
• Inflation including collapse of the wave function: The quasi-de Sitter case
• Consistent Cosmic Microwave Background Spectra from Quantum Depletion
• Generic inference of inflation models by non-Gaussianity and primordial power spectrum reconstruction
• Probing a cosmological model with a $\Lambda ={\Lambda }_0+3\beta H^2$ decaying-vacuum
• Thermal and non-thermal emission in the Cygnus X region
• A multi-level solver for Gaussian constrained CMB realizations
• Improving estimates of the growth rate using galaxy-velocity correlations: a simulation study
• Isocurvature perturbations and tensor mode in light of Planck and BICEP2
• Consistency of Pantheon+ supernovae with a large-scale isotropic universe
• SUSY-QCD corrected and Sommerfeld enhanced stau annihilation into heavy quarks with scheme and scale uncertainties
• Discovering strongly lensed quasar candidates with catalogue-based methods from DESI Legacy Surveys
• Optimization of foreground moment deprojection for semi-blind CMB polarization reconstruction
• High-resolution CMB bispectrum estimator with flexible modal basis
• Estimating the uncorrelated dark energy evolution in the Planck era
• Probing cold dark matter subhalos with simulated ALMA observations of macrolensed sub-mm galaxies
• Anisotropic constant-roll inflation for the Dirac-Born-Infeld model
• CMB with the background primordial magnetic field
• Searching for a possible dipole anisotropy on acceleration scale with 147 rotationally supported galaxies
• Constraining Primordial Non-Gaussianity with Moments of the Large Scale Density Field
• The tension on the cosmological parameters from different observational data
• Isotropy statistics of CMB hot and cold spots
• Impact of the damping tail on neutrino mass constraints
• Emergent Universe Scenario, Bouncing and Cyclic Universes in Degenerate Massive Gravity
• A Global ILC Approach in Pixel Space over Large Angular Scales of the Sky using CMB Covariance Matrix
• Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions
• Semi-blind Bayesian inference of CMB map and power spectrum
• Cosmic backgrounds of relic gravitons and their absolute normalization
• Chameleon Field Dynamics During Inflation
• CMB low multipole alignments in the $\mathbf{\Lambda }$CDM and Dipolar models
• Searching for an elusive charged Higgs at the Large Hadron Collider
• Bandpass mismatch error for satellite CMB experiments I: Estimating the spurious signal
• The Galaxy Stellar Mass Function and Low Surface Brightness Galaxies from Core-Collapse Supernovae
• Anisotropic universe with anisotropic dark energy
• Anisotropic power-law inflation for a model of two scalar and two vector fields
• Warm Inflation in $f(R,T)$ gravity
• Gravitational Magnus effect
• CMB bounds on tensor-scalar-scalar inflationary correlations
• Non-virialised clusters for detection of Dark Energy-Dark Matter interaction
• Constraints on Dark Energy Models Using Late Universe Probes
• An X-ray and SZ bright diffuse source toward M31: a Local Hot Bridge
• Prospects for discovery and spin discrimination of dark matter in Higgs portal DM models and their extensions at 100 TeV $pp$ collider
• Polarised radio emission associated with HESS J1912+101
• Cosmology based on $f(R)$ gravity with $\mathcal{O}(1)$ eV sterile neutrino
• Particle decay in post inflationary cosmology
• Quantifying the CMB Degeneracy Between the Matter Density and Hubble Constant in Current Experiments
• First comprehensive constraints on the Finslerian models using cosmological observations
• The scalar modes of the relic gravitons
• The Peculiar Velocity Correlation Function
• Constraining dark sector perturbations I: cosmic shear and CMB lensing
• Testing a theoretical prediction for bar formation in galaxies with bulges
• Constraining the WMAP9 bispectrum and trispectrum with needlets
• Generalized Brans-Dicke theories in light of evolving dark energy
• Mean Estimate Distances for Galaxies with Multiple Estimates in NED-D
• Screening corrections to Electron Capture Rates and resulting constraints on Primordial Magnetic Fields
• Analysis of NILC performance on B-modes data of sub-orbital experiments
• CMB B-mode auto-bispectrum produced by primordial gravitational waves
• Inflationary magnetogenesis, derivative couplings and relativistic Van der Waals interactions
• Post-Newtonian celestial mechanics in scalar-tensor cosmology
• The ages of (the oldest) stars
• Peering into the Milky Way by FAST: III. Magnetic fields in the Galactic halo and farther spiral arms revealed by the Faraday effect of faint pulsars
• The ESO's VLT Type Ia supernova spectral set of the final two years of SNLS
• An Examination of Galactic Polarization with Application to the Planck TB Correlation
• Shape of Dark Energy: Constraining Its Evolution with a General Parametrization
• The Integrated Sachs-Wolfe Effect in 4D Einstein-Gauss-Bonnet Gravity
• Cosmic Voids in Evolving Dark Sector Cosmologies: the Low Redshift Universe
• Constraining dark sector perturbations II: ISW and CMB lensing tomography
• Wyman's "other" scalar field solution, Sultana's generalization, and their Brans-Dicke and $R^2$ relatives
• High-precision nuclear chronometer for the cosmos
• A hybrid map-$C_{\ell }$ component separation method for primordial CMB $B$-mode searches
• Spinning nano-carbon grains: Viable origin for anomalous microwave emission
• The Q/U Imaging ExperimenT: Polarization Measurements of the Galactic Plane at 43 and 95 GHz
• Measurement of the Anisotropy Power Spectrum of the Radio Synchrotron Background
• Scalar Triplet Flavor Leptogenesis with Dark Matter
• The galaxy power spectrum from TGSS ADR1 and the effect of flux calibration systematics
• Warm inflation with an oscillatory inflaton in the non-minimal kinetic coupling model
• Local probes strongly favor $\Lambda$CDM against power-law and $R_h=ct$ universe
• What initial condition of inflation would suppress the large-scale CMB spectrum?
• Hierarchical Bayesian CMB Component Separation with the No-U-Turn Sampler
• Inflation in f(R,T) gravity with Double-Well potential
• The impact of magnetic fields on cosmological galaxy mergers -- II. Modified angular momentum transport and feedback
• Morphological Analysis of the Polarized Synchrotron Emission with WMAP and Planck
• QUIJOTE Scientific results. III. Microwave spectrum of intensity and polarization in the Taurus molecular cloud Complex and L1527
• Material models of dark energy
• Ages of 70 dwarfs of three populations in the solar neighborhood: considering O and C abundances in stellar models
• Fuzzy Aquarius: evolution of a Milky-way like system in the Fuzzy Dark Matter scenario
• Improved binary pulsar constraints on the parameterized post-Einsteinian framework
• The nature of non-Gaussianity and statistical isotropy of the 408 MHz Haslam synchrotron map
• LiteBIRD Science Goals and Forecasts: A full-sky measurement of gravitational lensing of the CMB
• Forecasts of cosmological constraints from HI intensity mapping with FAST, BINGO & SKA-I
• Foreground Bias From Parametric Models of Far-IR Dust Emission
• Glauber theory and the quantum coherence of curvature inhomogeneities
• LRS Bianchi I model with bulk viscosity in f(R,T) gravity
• Non-sphericity of ultralight axion dark matter haloes in the Galactic dwarf spheroidal galaxies
• Application of Contour Minkowski Tensor and $\mathcal{D}$ Statistic to the Planck $E$-mode data
• Monopole Fluctuation of the CMB and its Gauge Invariance
• Blasting away a dwarf galaxy: The "tail" of ESO 324-G024
• Supersymmetry Searches in GUT Models with Non-Universal Scalar Masses
• Magnetic fields of the W4 superbubble
• Exact joint likelihood of pseudo-$C_{\ell }$ estimates from correlated Gaussian cosmological fields
• Cosmic Voids in Evolving Dark Sector Cosmologies: the High Redshift Universe
• Helicity in the Large-Scale Galactic Magnetic Field
• Constancy of the Cluster Gas Mass Fraction in the R_h=ct Universe
• Relic Abundance of Asymmetric Dark Matter and the Scalar--Tensor Model
• The link between E-B polarization modes and gas column density from interstellar dust emission
• Axion inflation with cross-correlated axion isocurvature perturbations
• Probing dark energy via galaxy cluster outskirts
• A LEKID-based CMB instrument design for large-scale observations in Greenland
• Constraining the reionization history with CMB and spectroscopic observations
• Primordial power spectrum of tensor perturbations in Finsler spacetime
• Thermal power spectrum in the CFT driven cosmology
• Constraining the history of reheating with the NANOGrav 15-year data
• Searching for Cosmological Preferred Axis using cosmographic approach
• Inflation scenario driven by a low energy physics inflaton
• Resolved observations at 31 GHz of spinning dust emissivity variations in $\rho$ Oph
• Cosmological constraints on a unified dark matter-energy scalar field model with fast transition
• On SUSY Restoration in Single-Superfield Inflationary Models of Supergravity
• BeyondPlanck XVI. Limits on Large-Scale Polarized Anomalous Microwave Emission from Planck LFI and WMAP
• Cosmic acceleration from coupling of baryonic and dark matter components: Analysis and diagnostics
• An exact model of a gravitational wave in the Bianchi III universe based on Shapovalov II wave spacetime and the quadratic theory of gravity
• The spectral index of polarized diffuse Galactic emission between 30 and 44 GHz
• QUIJOTE scientific results -- X. Spatial variations of Anomalous Microwave Emission along the Galactic plane
• Type I+III Seesaw Mechanism and CP Violation for Leptogenesis
• A Novel CMB Component Separation Method: Hierarchical Generalized Morphological Component Analysis
• Supersymmetric B-L inflation near the conformal coupling
• Abundance and properties of dark radiation from the cosmic microwave background
• The Hierarchy Problem and the Cosmological Constant Problem Revisited -- A new view on the SM of particle physics
• Do we need wavelets in the late Universe?
• CMB all-scale blackbody distortions induced by linearizing temperature
• Constraints on Brane-World Inflation from the CMB Power Spectrum: Revisited
• Validating the methodology for constraining the linear growth rate from clustering anisotropies
• Two per cent measurement of $H_0$ from Cepheids alone
• If dark matter is fuzzy, the first stars form in massive pancakes
• Structure of Kähler potential for D-term inflationary attractor models
• The first observations of wide-band interferometers and the spectra of relic gravitons
• Non-Gaussian Shape Discrimination with Spectroscopic Galaxy Surveys
• de Sitter Harmonies: Cosmological Spacetimes as Resonances
• CMB all-scale blackbody distortions induced by linearizing temperature
• Dark matter imprint on ${}^8$B neutrino spectrum
• Modeling parity-violating spectra in Galactic dust polarization with filaments and its applications to cosmic birefringence searches
• No-hair conjectures, primordial shear and protoinflationary initial conditions
• The Structural and Kinematic Evolution of Central Star Clusters in Dwarf Galaxies and Their Dependence on Dark Matter Halo Profiles
• Quantum Discrete Levels of the Universe from the Early Trans-Planckian Vacuum to the Late Dark Energy
• The History of Inflation from Microwave Background Polarimetry and Laser Interferometry
• Likelihood of the Power Spectrum in Cosmological Parameter Estimation
• CMB imprints of non-canonical anisotropic inflation
• Probing Radiative Neutrino Mass Generation through Monotop Production
• Antisymmetric galaxy cross-correlations as a cosmological probe
• Constraining Hybrid Natural Inflation with recent CMB data
• On the Origin of Metal-poor Stars in the Solar Neighborhood
• QUIJOTE Scientific Results -- VII. Galactic AME sources in the QUIJOTE-MFI Northern Hemisphere Wide-Survey
• Deviation of geodesics and particle trajectories in a gravitational wave of the Bianchi type VI universe
• Deep redshift topological lensing: strategies for the T^3 candidate
• Evaluation of cosmogenic production of ${}^{39}Ar$ and ${}^{42}Ar$ for rare-event physics using underground argon
• Linearized iterative least-squares (LIL): A parameter fitting algorithm for component separation in multifrequency CMB experiments such as Planck
• Tensor Perturbations in Anisotropically Curved Cosmologies
• Probing modified gravity in cosmic filaments
• Self-consistent redshift estimation using correlation functions without a spectroscopic reference sample
• Angular correlations of causally-coherent primordial quantum perturbations
• Testing backreaction effects with observational Hubble parameter data
• Testing isotropy of cosmos with WMAP and PLANCK data
• Direct Optimal Mapping for 21cm Cosmology: A Demonstration with the Hydrogen Epoch of Reionization Array
• The Hantzsche-Wendt Manifold in Cosmic Topology
• Emergent Universe in f(Q) gravity theories
• Prospecting bipartite Dark Matter through Gravitational Waves
• Using the Modified Nearest Neighbor Method to Correct Fiber-collision Effects on Galaxy Clustering
• Gravitational Waves of Type III Shapovalov Spacetimes: Particle Trajectories, Geodesic Deviation and Tidal Accelerations
• Averaged Energy Conditions and Bouncing Universes
• Simultaneous Dependence of Matter Clustering on Scale and Environment
• Quantifying the Interstellar Medium and Cosmic Rays in the MBM 53, 54, and 55 Molecular Clouds and the Pegasus Loop using Fermi-LAT Gamma-ray Observations
• Sensitivity of inflationary predictions to pre-inflationary phases
• No stable dissipative phantom scenario in the framework of a complete cosmological dynamics
• Evolution of the cosmic matter density field with a primordial magnetic field
• Relativistic and nonrelativistic annihilation of dark matter: a sanity check using an effective field theory approach
• Extended anisotropic models in noncompact Kaluza-Klein theory
• A Perturbative Analysis of Synchrotron Spectral Index Variation over Microwave Sky
• Asymmetric capture of Dirac dark matter by the Sun
• Hidden Sector Dark Matter with Global $U(1{)}_X$-symmetry and Fermi-LAT 130 GeV $\gamma$-ray Excess
• CMB foreground measurements through broad-band radio spectro-polarimetry: prospects of the SKA-MPG telescope
• Least response method to separate CMB spectral distortions from foregrounds
• Novae: An Important Source of Lithium in the Galaxy
• Optimized Large-Scale CMB Likelihood And Quadratic Maximum Likelihood Power Spectrum Estimation
• Estimation of Inflation parameters for Perturbed Power Law model using recent CMB measurements
• Modelling the spinning dust emission from LDN 1780
• Quantum collapse as source of the seeds of cosmic structure during the radiation era
• Statistical properties of polarized CMB foreground maps
• Compact objects and the swampland
• Scale-Invariant Curvature Fluctuations from an Extended Semiclassical Gravity
• Inflationary Twin Models
• The gravitational and lensing-ISW bispectrum of 21cm radiation
• On the influence of environment on star forming galaxies
• Testing the ABS method with the simulated Planck temperature maps
• Gamma-ray and Synchrotron Radiation from Dark Matter annihilations in Ultra-faint Dwarf Galaxies
• Dark Matter, Sparticle Spectroscopy and Muon $(g-2)$ in $SU(4{)}_c\times SU(2{)}_L\times SU(2{)}_R$
• Modified Baryonic Dynamics: two-component cosmological simulations with light sterile neutrinos
• Fingerprint of Galactic Loop I on polarized microwave foregrounds
• Supergravity, $\alpha$-attractors and primordial non-Gaussianity
• Non-linear matter bispectrum in general relativity
• Constraints on the Optical Depth to Reionization from Balloon-Borne CMB Measurements
• Nonthermal $CP$ violation in soft leptogenesis
• Detection of Dipole Modulation in CMB Temperature Anisotropy Maps from WMAP and Planck using Artificial Intelligence
• The variation of the fine structure constant: testing the dipole model with thermonuclear supernovae
• Stringy bounces and gradient instabilities
• Simple numerical implementation of general dark energy models
• QUIJOTE Scientific Results -- XVII. Studying the Anomalous Microwave Emission in the Andromeda Galaxy with QUIJOTE-MFI
• Testing theories of Gravity and Supergravity with inflation and observations of the cosmic microwave background
• Improved Modeling of the Kinematic Sunyaev-Zel'dovich Projected-Fields signal and its Cosmological Dependence
• Tunable Rectangular Resonant Cavities for Axion Haloscopes
• A note on the semiclassicality of cosmological perturbations
• A Solution to Lithium Problem by Long-Lived Stau
• Effective Field Theory of Anisotropic Inflation and Beyond
• Mirage Models Confront the LHC: II. Flux-Stabilized Type IIB String Theory
• Nuclear Spin Metrology with Nitrogen Vacancy Center in Diamond for Axion Dark Matter Detection
• General modal estimation for cross-bispectra
• Statistical isotropy violation in WMAP CMB maps resulting from non-circular beams
• New Quantum Phase of the Universe before Inflation and its Cosmological and Dark Energy Implications
• Symmetries of CMB Temperature Correlation at Large Angular Separations
• Cosmological Parameters from CMB Maps without Likelihood Approximation
• Damped Lyman-$\alpha$ absorbers and atomic hydrogen in galaxies: the view of the GAEA model
• Two-field inflation with non-minimal coupling
• The PICASSO map-making code: application to a simulation of the QUIJOTE northern sky survey
• Symmetries and unitary interactions of mass dimension one fermionic dark matter
• Noncommutative Geometry and the Primordial Dipolar Imaginary Power Spectrum
• Very metal-poor stars in the solar vicinity: age determination
• Forecasts of CMB lensing reconstruction of AliCPT-1 from the foreground cleaned polarization data
• The Effect of $\alpha$-Vacua on the Scalar and Tensor Spectral Indices: Slow-Roll Approximation
• Fastcc: fast colour corrections for broadband radio telescope data
• Salvaging Power-Law Inflation through Warming
• Ray tracing the integrated Sachs-Wolfe effect through the light cones of the Dark Energy Universe Simulation -- Full Universe Runs
• Very light dilaton and naturally light Higgs boson
• Missing dust signature in the cosmic microwave background
• QUIJOTE scientific results -- V. The microwave intensity and polarisation spectra of the Galactic regions W49, W51 and IC443
• Phenomenology of $keV$ sterile neutrino in minimal extended seesaw
• Features in single field slow-roll inflation
• Reconstruction of the dark energy scalar field potential by Gaussian process
• The Stochastic Properties of ${\ell }^1$-Regularized Spherical Gaussian Fields
• A power spectrum approach to the search for Axion-like Particles from resolved galaxy clusters using CMB as a backlight
• Scale and shape dependent non-Gaussianity in the presence of inflationary vector fields
• The Huge Magnetic Toroids in the Milky Way Halo
• Noncommutative Universe and Chameleon Field Dynamics
• Perturbations in Bouncing and Cyclic Models, a General Study
• Sparse point-source removal for full-sky CMB experiments: application to WMAP 9-year data
• Constraints on the multi-lognormal magnetic fields from the observations of the cosmic microwave background and the matter power spectrum
• Two Dynamical Scenarios for Binned Master Sample Interpretation
• Dark Matter perspective of Left-Right symmetric gauge model
• The Atacama Cosmology Telescope: DR6 Power Spectrum Foreground Model and Validation
• Towards conformal cosmology
• Implications for cosmology from Ground-based Cosmic Microwave Background observations
• Holographic Dark Energy from Acceleration of Particle Horizon
• Modern Cosmology, an Amuse-Gueule
• Scalar - Tensor gravity with scalar -matter direct coupling and its cosmological probe
• Exploring Modified Gravity: Constraints on the $\mu$ and $\Sigma$ Parametrization with WMAP, ACT, and SPT
• No-scale SUGRA Inflation and Type-I seesaw
• Determining $H_0$ using a model-independent method
• On Weak Lensing Shape Noise
• Effect of gravitational field self-interaction on large structure formation
• Palatini approach and large-scale magnetogenesis
• Foreground removal with ILC methods for AliCPT-1
• Hidden from view: Coupled Dark Sector Physics and Small Scales
• Constraining Galileon Inflation
• Testing for foreground residuals in the Planck foreground cleaned maps: A new method for designing confidence masks
• Data driven foreground clustering approach to component separation in multifrequency CMB experiments: A new Planck CMB map
• Contribution of Galactic free-free emission to the foreground for EoR signal in SKA experiments
• Hubble law: measure and interpretation
• Impact of half-wave plate systematics on the measurement of CMB $B$-mode polarization
• Spectral-line Observations Using a Phased Array Feed on the Parkes Telescope
• The aspherical explosions of the 03fg-like Type Ia supernovae 2021zny and 2022ilv revealed by polarimetry
• Evolution of density and velocity profiles of dark matter and dark energy in spherical voids
• Pattern of perturbations from a coherent quantum inflationary horizon
• Higgs inflation model with non-minimal coupling in hybrid Palatini approach
• Anisotropic hyperbolic inflation for a model of two scalar and two vector fields
• Fermi-Boltzmann statistics of neutrinos and relativistic effective degrees of freedom
• The Diffuse Light of the Universe - On the microwave background before and after its discovery: open questions
• Testing the anisotropy of the Universe with the distance duality relation
• A Fast and Accurate Algorithm for Spherical Harmonic Analysis on HEALPix Grids with Applications to the Cosmic Microwave Background Radiation
• Bayesian inference on the sphere beyond statistical isotropy
• Estimation of Full Sky Power Spectrum between Intermediate to Large Angular Scales from Partial Sky CMB Anisotropies using Artificial Neural Network
• Cosmology Large Angular Scale Surveyor (CLASS): 90 GHz Telescope Pointing, Beam Profile, Window Function, and Polarization Performance
• Reconciling BICEP2 and Planck results with right-handed Dirac neutrinos in the fundamental representation of grand unified E_6
• Cosmological perturbations in the $\Lambda$CDM-like limit of a polytropic dark matter model
• Is interacting vacuum viable?
• Likelihood analysis of small field polynomial models of inflation yielding a high Tensor-to-Scalar ratio
• Topological pseudodefects of a supersymmetric $SO(10)$ model and cosmology
• Joint Bayesian estimation of tensor and lensing B-modes in the power spectrum of CMB polarization data
• Forecast of foreground cleaning strategies for AliCPT-1
• Violation of consistency relations and the protoinflationary transition
• Plateau Inflation from Random Non-Minimal Coupling
• Analytic Calculation of Covariance between Cosmological Parameters from Correlated Data Sets, with an Application to SPTpol
• Measuring Stellar Masses of Emission Line Galaxies at 1.2<z<1.9
• Cosmological decay of Higgs-like scalars into a fermion channel
• Anisotropic Cosmology in the Local Limit of Nonlocal Gravity
• Sparse Inpainting and Isotropy
• Exact theory of freeze out
• The 1.4 GHz Cosmic Star Formation History at z < 1.3
• Testing primordial non-Gaussianities on galactic scales at high redshift
• Confirming ALMA Calibration using Planck and ACT Observations
• The measurements of matter density perturbations amplitude from cosmological data
• Finsler space-time can explain both parity asymmetry and power deficit seen in CMB temperature anisotropies
• New natural shapes of non-Gaussianity from high-derivative interactions and their optimal limits from WMAP 9-year data
• Effects of dark boson mediated feeble interaction between dark matter (DM) and quark matter on $f$-mode oscillation of DM admixed quark stars
• Constraining graviton non-Gaussianity through the CMB bispectra
• The C-Band All-Sky Survey (C-BASS): New Constraints on the Integrated Radio Spectrum of M 31
• Ghost of a Shell: Magnetic Fields of Galactic Supershell GSH 006$-$15$+$7
• Modeling the Intergalactic Medium during the Epoch of Reionization
• Correlations between $\gamma$-ray luminosity and magnetization of the jet as well as relativistic electron injection power:cases for Mrk 421, 3C 454.3 and 3C 279
• Stochastic determination of matrix determinants
• An Informational Approach to Cosmological Parameter Estimation
• Does spatial flatness forbid the turnaround epoch of collapsing structures?
• Gradient expansion of superhorizon perturbations in G-inflation
• ISW in $\Lambda$CDM or something else?
• Correlation between U/Th and Pb/Os abundance ratios and its application in nuclear cosmochronology
• Classical Gravitational Back-Reaction
• CMB statistical isotropy confirmation at all scales using multipole vectors
• The biparametric Fisher-Rényi complexity measure and its application to the multidimensional blackbody radiation
• BeyondPlanck IV. On end-to-end simulations in CMB analysis -- Bayesian versus frequentist statistics
• Three-Dimensional Aquila Rift: Magnetized HI Arch Anchored by Molecular Complex
• Geometrical measures of non-Gaussianity generated from single field Inflationary models
• Curvaton scenarios with inflaton decays into curvatons
• Feeling de Sitter
• Is there evidence for CIDER in the Universe?
• Perturbation Theory Remixed: Improved Nonlinearity Modeling beyond Standard Perturbation Theory
• Correlating Fourier phase information with real-space higher order statistics
• Polarization of Sunyaev-Zeldovich signal due to electron pressure anisotropy in galaxy clusters
• QUIJOTE scientific results -- VI. The Haze as seen by QUIJOTE
• Chaotic interactions between dark matter and dark energy
• Estimating SI violation in CMB due to non-circular beam and complex scan in minutes
• Science-driven 3D data compression
• Neutralino Dark Matter in Gauge Mediation After Run I of LHC and LUX
• Evaluation of the single-component thermal dust emission model in CMB experiments
• BFORE: The B-mode Foreground Experiment
• Exact model of gravitational wave and pure radiation
• Parity in Planck full-mission CMB temperature maps
• Dynamics of dark energy in the gravitational fields of matter inhomogeneities
• Einstein gravity with torsion induced by the scalar field
• Analysis of the Amplitude of the Sunyaev-Zel'dovich Effect out to Redshift z=0.8
• Looking for non-Gaussianity in all the right places: A new basis for non-separable bispectra
• Revised planet brightness temperatures using the Planck/LFI 2018 data release
• Constraints on Bianchi-I type universe with SH0ES anchored Pantheon+ SNIa data
• Biparametric complexities and the generalized Planck radiation law
• Lensing amplitude anomaly and varying electron mass alleviate the Hubble and $S_8$ tensions
• Trial by FIRE: Probing the dark matter density profile of dwarf galaxies with GraphNPE
• Searching for velocity-dependent dark matter annihilation signals from extragalactic halos
• The Q/U Imaging Experiment: Polarization Measurements of Radio Sources at 43 and 95 GHz
• Anomalies in the topology of the temperature fluctuations in the cosmic microwave background: An analysis of the $\text{NPIPE}$ and $\text{FFP10}$ data releases
• Dynamic Dark Energy Equation of State (EoS) and Hubble Constant analysis using type Ia supernovae from Union 2.1 dataset
• The Two-Point Correlation Function of Gamma-ray Bursts
• Qualitative analysis for viscous cosmologies in a non linear regime of the Israel-Stewart formalism
• The Effect of Interplanetary Scintillation on Epoch of Reionisation Power Spectra
• Observational constraints on Tsallis holographic dark energy with Ricci horizon cutoff
• Stellar, Gas, and Dust Emission of Star Forming Galaxies out to z~2
• Inflaton fluctuations in the presence of cosmological defects
• The Glow of Axion Quark Nugget Dark Matter: (II) Galaxy Clusters
• Consistency Tests for Comparing Astrophysical Models and Observations
• Principal component analysis of the reionization history from Planck 2015 data
• Coincidence problem within dark energy as a coupled self-interacting Bose-Einstein gas
• Large Scale Anomalies in the Microwave Background: Causation and Correlation
• Quantum Trans-Planckian Physics inside Black Holes and its Spectrum
• Endowing $\mathbf{\Lambda }$ with a dynamic nature: constraints in a spatially curved Universe
• Time-ordered data simulation and map-making for the PIXIE Fourier transform spectrometer
• Is de Sitter space always excluded in semiclassical f(R) gravity?
• Improved cosmological fits with quantized primordial power spectra
• Reviewing the prospect of fermion triplets as dark matter and source of baryon asymmetry in non-standard cosmology
• The C-Band All-Sky Survey (C-BASS): Simulated parametric fitting in single pixels in total intensity and polarization
• The active nucleus of the ULIRG IRAS F00183-7111 viewed by NuSTAR
• One Extension to Explain Them All, One Scale-Invariant Spectrum to Test Them All, and in One Model Bind Them
• Closing in on the large-scale CMB power asymmetry
• Asymmetric Dark Matter in the Shear--dominated Universe
• Controlling systematics in ground-based CMB surveys with partial boresight rotation
• Status of Natural Supersymmetry from the GmSUGRA in Light of the current LHC Run-2 and LUX data
• An Independent Measure of the Kinematic Dipole from SDSS
• Hubble Space Telescope Astrometry of the Metal-Poor Visual Binary $\mu$ Cassiopeiae: Dynamical Masses, Helium Content, and Age
• Approaches to relativistic positioning around Earth and error estimations
• Venus Observations at 40 and 90 GHz with CLASS
• Statistical anisotropy from inflationary magnetogenesis
• The H$\alpha$ and [O III] $\lambda 5007$ Luminosity Functions of $1.2<z<1.9$ Emission-Line Galaxies from HST Grism Spectroscopy
• Impact of Low ell's on Large Scale Structure Anomalies
• Is there a resting frame in the universe? A proposed experimental test based on a precise measurement of particle mass
• Electric dipole moments of the nucleon and light nuclei
• Canonical equivalence, quantization and anisotropic inflation in higher order theory of gravity
• Observations of Galactic star-forming regions with the Cosmic Background Imager at 31 GHz
• Faraday scaling and the Bicep2 observations
• Analysis of Dark Matter Halo Structure Formation in $N$-body Simulations with Machine Learning
• Cosmoglobe DR1. III. First full-sky model of polarized synchrotron emission from all WMAP and Planck LFI data
• Initial conditions of the universe: A sign of the sine mode
• Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
• Statistically-Anisotropic Tensor Bispectrum from Inflation
• A new way to test the WIMP dark matter models
• Blind Map Level Systematics Cleaning: A Quadratic Estimator Approach
• Orbifold Line Topology and the Cosmic Microwave Background
• Polytropic Inspired Inflation on the Brane
• Constraining Ultra Light Dark Matter with the Galactic Nuclear Star Cluster
• Modeling Cosmic Expansion, and Possible Inflation, As a Thermodynamic Heat Engine
• Angular correlations on causally-coherent inflationary horizons
• The Formulation of Scaling Expansion in an Euler-Poisson Dark-fluid Model
• The Simons Observatory: Beam characterization for the Small Aperture Telescopes
• Unraveling the CMB lack-of-correlation anomaly with the cosmological gravitational wave background
• Lensing reconstruction from the cosmic microwave background polarization with machine learning
• Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
• Cosmological Perturbations without Inflation
• Cosmic Birefringence from CP-Violating Axion Interactions
• Coherent states of quantum spacetimes for black holes and de Sitter spacetime
• Discovery of the Goat Horn complex: a $\sim 1000$ deg${}^2$ diffuse X-ray source connected to radio loop XII
• On the recovery of ISW fluctuations using large-scale structure tracers and CMB temperature and polarization anisotropies
• A Bayesian estimate of the CMB-large-scale structure cross-correlation
• Observing the Epoch of Reionization with the Cosmic Microwave Background
• Footprints of Loop I on Cosmic Microwave Background Maps
• Influence of dark matter on the structure of strange quark stars in one-fluid model
• Can an Anti-de Sitter Vacuum in the Dark Energy Sector Explain JWST High-Redshift Galaxy and Reionization Observations?
• An Actinide-boost Star Discovered in the Gaia-Sausage-Enceladus
• Reconstruction of the scalar field potential in nonmetricity gravity through Gaussian processes
• Optical cavity resonator in an expanding universe
• Galactic diffuse emission from radio to ultra-high-energy gamma rays in light of up-to-date cosmic ray measurements
• Testing the coincidence problem with strong gravitational lens, Type Ia supernovae and Hubble parameter observational data
• Living with Neighbors. IV. Dissecting the Spin$-$Orbit Alignment of Dark Matter Halos: Interacting Neighbors and the Local Large-scale Structure
• The Thermal Sunyaev-Zeldovich Effect of Primordial Recombination Radiation
• One-loop considerations for coexisting vacua in the CP conserving 2HDM
• Pole inflation in Jordan frame supergravity
• Spectral Distortion in a Radially Inhomogeneous Cosmology
• Calculated WIMP signals at the ANDES laboratory: comparison with northern and southern located dark matter detectors
• A consistent scalar-tensor cosmology for inflation, dark energy and the Hubble parameter
• Fast and precise way to calculate the posterior for the local non-Gaussianity parameter $f_{\text{nl}}$ from cosmic microwave background observations
• Lyman-alpha Heating of Inhomogeneous High-redshift Intergalactic Medium
• Principal Components of CMB non-Gaussianity
• A test of the Suyama-Yamaguchi inequality from weak lensing
• BICEP's acceleration
• A Maximum Likelihood Approach to Estimating Correlation Functions
• Cosmic perturbations, baryon asymmetry and dark matter from the minimal supersymmetric standard model
• Conditional Colour-Magnitude Distribution of Central Galaxies in Galaxy Formation Models
• The establishment of the Standard Cosmological Model through observations
• Radio Observations as a Probe of Cosmic Web Magnetism
• Polarization Calibration of a Microwave Polarimeter with Near-Infrared Up-Conversion for Optical Correlation and Detection
• Effects of observer peculiar motion on the isotropic background frequency spectrum: from monopole to higher multipoles
• The Polarization Signature of Local Bulk Flows
• Optimal bispectrum constraints on single-field models of inflation
• Accelerated expansion of the Universe a la the Stueckelberg mechanism
• The consistency test on the cosmic evolution
• Cosmological Signatures of Dark Sector Physics: The Evolution of Haloes and Spin Alignment
• Spectator Higgs, large-scale gauge fields and the non-minimal coupling to gravity
• One spectrum to rule them all?
• Does fractal Universe favour warm inflation: Observational support?
• Characterisation of Dark Matter in Direct Detection Experiments: Singlino Versus Higgsino
• Cosmic variance mitigation in measurements of the integrated Sachs-Wolfe effect
• QUIJOTE scientific results -- XVIII. New constraints on the polarization of the Anomalous Microwave Emission in bright Galactic regions: $\rho$\,Ophiuchi, Perseus and W43
• Examining statistical isotropy of CMB low multipoles from Planck PR4 data
• LRS Bianchi I model with perfect fluid equation of state
• Effect of noncircularity of experimental beam on CMB parameter estimation
• WIMP dark matter in bulk viscous non-standard cosmologies
• Exploring the deviation of cosmological constant by a generalized pressure dark energy model
• Breaking the degeneracy between polarization efficiency and cosmological parameters in CMB experiments
• Gravitational waves in a cyclic Universe: resilience through cycles and vacuum state
• Can Hubble tension be eased by invoking a finite range for gravity?
• Sound Horizon Independent Constraints on Early Dark Energy: The Role of Supernova Data
• Non-linear curvature inhomogeneities and backreaction for relativistic viscous fluids
• Natural inflation with natural number of e-foldings
• Reionization and CMB non-Gaussianity
• Primordial Power Spectrum of Five Dimensional Uniform Inflation
• Hypermagnetic knots and gravitational radiation at intermediate frequencies
• Asymptotic symmetries and memories of gauge theories in FLRW spacetimes
• Entropy Production in the Inflationary Epoch Using the Gouy-Stodola Theorem
• The Microwave Thermal Emission from the Zodiacal Dust Cloud Predicted with Contemporary Meteoroid Models
• Constraining primordial vector mode from B-mode polarization
• A new look at the integrated radio/microwave continuum spectrum of Galactic supernova remnant IC443
• Multiscalar field cosmological model and possible solutions using Noether symmetry approach
• Spin-$0^{\pm }$ portal induced Dark Matter
• CMB two-point angular correlation function in the Ellipsoidal Universe
• A spatial-correlation analysis of the cubic 3-torus topology based on the Planck 2013 data
• Thermodynamics of the Primordial Universe
• Recent Developments in Degenerate Higher Order Scalar Tensor Theories
• Evolving beyond z=0: insights about the future of stars and the intergalactic medium
• Origin Of The Cosmic Ray Positrons Observed Near Earth- Meson Decay Or Dark Matter Decay?
• Planck and WMAP constraints on generalised Hubble flow inflationary trajectories
• Newtonian cosmology and Evolution of kappa-deformed universe
• Nonparametric test of consistency between cosmological models and multiband CMB measurements
• The parity-odd Intrinsic Bispectrum
• Entropy Production in a Lepton-Photon Universe
• Energy conditions in a modified Brans-Dicke theory
• Tantalizing New Physics from the Cosmic Purview
• Quadrant asymmetry in the angular distribution of the Cosmic Microwave Background in the Planck satellite data
• Extended Delta-map: a map-based foreground removal method for CMB polarization observations
• Is the Cosmological Constant of Topological Origin?
• L-BASS: a project to produce an absolutely calibrated 1.4 GHz sky map, I -- Scientific rationale and system overview
• QUIJOTE scientific results -- IX. Radio sources in the QUIJOTE-MFI wide survey maps
• Machine-guided Exploration and Calibration of Astrophysical Simulations
• Big-bang nucleosynthesis through bound-state effects with a long-lived slepton in the NMSSM
• All-sky reconstruction of the primordial scalar potential from WMAP temperature data
• Dark energy model with very large-scale inhomogeneity
• New Constraints on Anisotropic Expansion from Supernovae Type Ia
• Electroweak Phase Transitions with BSM Fermions
• The CMB Derivatives of Planck's Beam Asymmetry
• A Dynamic Dark Information Energy Consistent with Planck Data
• Galactic foreground constraints on primordial $B$-mode detection for ground-based experiments
• Limits on Polarized Dust Spectral Index Variations for CMB Foreground Analysis
• DARKSKIES: A suite of super-sampled zoom-in simulations of galaxy clusters with self-interacting dark matter
• The cross correlation of the ABS and ACT maps
• Nearly Full-Sky Low-Multipole Cosmic Microwave Background Temperature Anisotropy: III. CMB Temperature Anomalies
• Hemispheric handedness in the Galactic synchrotron polarization foreground
• ForSE+: Simulating non-Gaussian CMB foregrounds at 3 arcminutes in a stochastic way based on a generative adversarial network
• Dark energy explained by a bias in the measurements
• Effects of boosting on extragalactic components: methods and statistical studies
• CMB lensing forecasts for constraining the primordial perturbations: adding to the CMB temperature and polarization information
• Low-$\ell$ CMB from String-Scale SUSY Breaking?
• Baryon Acoustic Oscillations from Integrated Neutral Gas Observations: an instrument to observe the 21cm hydrogen line in the redshift range 0.13 $<$ z $<$ 0.45 -- status update
• A Bayesian ILC method for CMB B-mode posterior estimation and reconstruction of primordial gravity wave signal
• Parameterizing the SFC Baryogenesis Model
• Cosmic microwave background constraints on the tensor-to-scalar ratio
• Constraints on primordial non-Gaussianity from Planck PR4 data
• Filtering in CMB data analysis with application to ACT DR4 and Planck observations
• FIMP Dark Matter in bulk viscous non-standard cosmologies
• Reducing the Tension Between the BICEP2 and the Planck Measurements: A Complete Exploration of the Parameter Space
• Magnetization of fluid phonons and large-scale curvature perturbations
• Einstein-aether models III: conformally static metrics, perfect fluid and scalar fields
• Domestic Corpuscular Inflaton
• Viable Anisotropic Inflation and Reheating in the Tachyon Model
• Study of the Cosmic Rays and Interstellar Medium in Local HI Clouds using Fermi-LAT Gamma-Ray Observations
• A precessing jet from an active galactic nucleus drives gas outflow from a disk galaxy
• A quasi-matter bounce equivalent to Starobinsky inflation
• The prospects of gravitational waves on constraining the anisotropy of the Universe
• Cosmic Ray contribution to the WMAP polarization data on the Cosmic Microwave Background
• Quasiadiabatic modes from viscous inhomogeneities
• Design and Performance of 30/40 GHz Diplexed Focal Plane for BICEP Array
• Baryon Acoustic Oscillations analyses with Density-Split Statistics
• CMB Polarization by the Asymmetric Template of Scalar Perturbations
• The C-Band All-Sky Survey (C-BASS): Total intensity point-source detection over the northern sky
• Dark Energy from Topology
• Constraining the Anomalous Microwave Emission Mechanism in the S140 Star Forming Region with Spectroscopic Observations Between 4 and 8 GHz at the Green Bank Telescope
• Late evolution of relic gravitational waves in coupled dark energy models
• Chaplygin Gas of Tachyon Nature Imposed by Symmetry and Constrained via H(z) Data
• Evaluating a Sigmoid Dark Energy Model to Explain the Hubble Tension
• Application of Genetic Algorithm to Estimate the Large Angular Scale Features of Cosmic Microwave Background
• A comparison of cosmological models with high-redshift quasars
• Statistical properties of Galactic synchrotron temperature and polarization maps -- a multi-frequency comparison
• On the Size and Mass of Photo-ionized Clouds in Extended Spiral Galaxy Halos
• Sparse estimation of model-based diffuse thermal dust emission
• Assessment of Models of Galactic Thermal Dust Emission Using COBE/FIRAS and COBE/DIRBE Observations
• Testing cosmological models with large-scale power modulation using microwave background polarization observations
• A Radiative Model of Quark Masses with Binary Tetrahedral Symmetry
• On-sky performance of new 90 GHz detectors for the Cosmology Large Angular Scale Surveyor (CLASS)
• Waves on accelerating dodecahedral universes
• Dark matter search with CMB: a study of foregrounds
• Nearly Full-Sky Low-Multipole Cosmic Microwave Background Temperature Anisotropy: II. Angular Power Spectra and Likelihood
• Interpreting the Cosmic History of the Universe Through Five-Dimensional Supergravity
• Spinodal Backreaction During Inflation and Initial Conditions
• Viscous modes, isocurvature perturbations and CMB initial conditions
• Accounting for Correlations When Fitting Extra Cosmological Parameters
• Microwave Observations of Venus with CLASS
• CMB low multipole alignments across WMAP and \emph{Planck} data releases
• The adiabatic/entropy decomposition in $P({\varphi }^I,X^{IJ})$ theories with multiple sound speeds
• Analytic Correlation of Inflationary Potential to Power Spectrum Shape: Limits of Validity, and `No-Go' for Small Field Model Analytics
• Polarized CMB recovery with sparse component separation
• Baryon density extraction and isotropy analysis of Cosmic Microwave Background using Deep Learning
• Subdominant Dark Matter sterile neutrino resonant production in the light of Planck
• An Optimally Weighted Estimator of the Linear Power Spectrum Disentangling the Growth of Density Perturbations Across Galaxy Surveys
• Polarization fraction of Planck Galactic cold clumps and forecasts for the Simons Observatory
• Observational constraints on the second-order primordial power spectrum: Exploring a Continuous Spontaneous Localization inspired inflationary model
• The optimisation of low-acceleration interstellar relativistic rocket trajectories using genetic algorithms
• Dynamics of clusters of galaxies with extended $f(\chi )$ gravity
• Lensed fast radio bursts as a probe of time-varying gravitational potential induced by wave dark matter
• Curvaton: Perturbations and reheating
• Violation of Bell inequalities from Cosmic Microwave Background data
• Constraining Recent Oscillations in Quintessence Models with Euclid
• A Comparative Test of the LCDM and R_h=ct Cosmologies Based on Upcoming Redshift Drift Measurements
• SIToolBox : A package for Bayesian estimation of the isotropy violation in the CMB sky
• Toward accurate measurement of property-dependent galaxy clustering I. Comparison of the Vmax method and the "shuffled" method
• A Proposal for Constraining Initial Vacuum by CMB
• EDGES of the dark forest: A new absorption window into the composite dark matter and large scale structure
• Galaxies and Cluster of Galaxies as Peak Patches of the Density Field
• Bayesian analysis for a class of $\alpha$-attractor inflationary models
• Seeing Relativity -- III. Journeying within the Kerr metric toward the negative gravity region
• Coupled Dark Energy field variation
• Impact of redshift distribution uncertainties on Lyman-break galaxy cosmological parameter inference
• Cosmic microwave background constraints on coupled dark matter
• Confirmation of the detection of B-modes in the Planck polarization maps
• Cosmoglobe: Towards end-to-end CMB cosmological parameter estimation without likelihood approximations
• Non-vacuum relativistic extensions of MOND using metric theories of gravity with curvature-matter couplings and their applications to the accelerated expansion of the Universe without dark components
• Reheating constraints and the $H_0$ tension in Quintessential Inflation
• Shockingly Effective: Cluster Winds as Engines of Feedback in Starburst Galaxy VV 114
• Forecasts of effects of beam systematics and deprojection on the third-generation ground-based cosmic microwave background experiment
• Nearly Full-Sky Low-Multipole Cosmic Microwave Temperature Anisotropy: I. Foreground Cleaned Maps
• Cosmological scenario based on the particle creation and holographic equipartition
• On the Impact of Random Residual Calibration Error on the Gibbs ILC Estimates over Large Angular Scales
• Constraint on the cosmic age from the solar $r$-process abundances
• On the possibility of Baryon Acoustic Oscillation measurements at redshift $z>7.6$ with the Roman Space Telescope
• A Homogeneous and Isotropic Universe in Lorentz Gauge Theory of Gravity
• Application of beyond $\delta N$ formalism -- Varying sound speed
• CP violation in bilinear R-parity violation and its consequences for the early universe
• Inflation and late time acceleration designed by Stueckelberg massive photon
• Photometric variability in star-forming galaxies as evidence for low-mass AGN and a precursor to quenching
• Primordial perturbations in kinetically dominated regimes of general relativity and hybrid quantum cosmology
• Effects of the quantum vacuum at a cosmic scale and of dark energy
• Observables for the Effect of Gravity on Electromagnetic Polarization
• An Instrument Error Budget for Space-Based Absolute Flux Measurements of the Sky Synchrotron Spectrum Below 20 MHz
• Partial Ly$\alpha$ thermalization in an analytic nonlinear diffusion model
• Inflation and Primordial Perturbations in Fractal Cosmology
• Simulating gravitational motion, gas dynamics, and structure in the cosmos
• Bayesian recalibration of flux scale factors in diffuse radio maps using low-resolution absolute radiometers
• Cluster environment quenches the star formation of low-mass satellite galaxies from the inside-out
• Probing the Type 3 interacting dark-energy model using matter pairwise velocity
• LiteBIRD science goals and forecasts: improved full-sky reconstruction of the gravitational lensing potential through the combination of Planck and LiteBIRD data
• The Python Sky Model 3 software
• Emulating the Non-Linear Matter Power-Spectrum in Mixed Axion Dark Matter Models
• High-Efficiency and Low-Noise Detectors for the Upgraded CLASS 90 GHz Focal Plane
• Fast Luminous Blue Transients in the Reionization Era and Beyond
• Flat Space, Dark Energy, and the Cosmic Microwave Background
• Cosmic rays from multiwavelength observations of the Galactic diffuse emission
• Hidden in the background: a local approach to CMB anomalies
• Excess B-modes extracted from the Planck polarization maps
• Perturbation Theory Remixed II: Improved Modeling of Nonlinear Bispectrum
• Implications of scattering for CMB foreground emission modelling
• The Precursor Small Aperture Telescope (PreSAT) CMB polarimeter
• Galaxy clustering in modified gravity from full-physics simulations. I: two-point correlation functions
• Modified hybrid inflation in no-scale SUGRA with suppressed $R$-symmetry breaking
• MNTES: Modeling Nonlinearity of TES detectors for Enhanced Cosmic Microwave Background measurements with LiteBIRD
• The Effects of Spatial Curvature on Cosmic Evolution
• Squeezed relic photons beyond the horizon
• Number counts, confusion, mapping issues and sky coverage analysis for radio continuum surveys through EMU Early Science, EMU-ASKAP, and WODAN especially for cosmology science goals
• Development of a model to investigate the effect of the bias in SNIa measurements related to the inhomogeneity of space
• Toward accurate measurement of property-dependent galaxy clustering: II. Tests of the smoothed density-corrected $V_{\max }$ method
• A Foreground Model Independent Bayesian CMB Temperature and Polarization Signal Reconstruction and Cosmological Parameter Estimation over Large Angular Scales
• Origin of neutrino masses, dark matter, leptogenesis, and inflation in a seesaw model with triplets
• Does History Repeat Itself? Periodic Time Cosmology
• Importance of the X-ray edge singularity for the detection of relic neutrinos in the PTOLEMY project
• ILC sensitivity for leptophilic scalar dark matter
• A Partial-Sky Gibbs ILC Approach for the Estimation of CMB Posterior over Large Angular Scales of the Sky
• FIMP DM in the Extended Hyperchargeless Higgs Triplet Model
• Far-infrared to centimeter emission of very nearby galaxies with archival data
• Cosmology with Type II Supernovae
• Cosmology, astrobiology, and the RNA world. Just add quintessential water
• Is PLANCK consistent with primordial deuterium measurements ?
• Artificial Neural Network Spectral Light Curve Template for Type Ia Supernovae and its Cosmological Constraints
• Robustness of cosmological axion mass limits
• Extreme Digitisation For Ground-Based Cosmic Microwave Background Experiments
• Absorption of Fermionic Dark Matter in the PICO-60 C${}_3$F${}_8$ Bubble Chamber
• An Interpretable AI Framework to Disentangle Self-Interacting and Cold Dark Matter in Galaxy Clusters: The CKAN Approach
• L-BASS: A project to produce an absolutely calibrated 1.4 GHz sky map. II -- Technical Description of the System
• Quantum Gravity Effective Action Provides Entropy of The Universe
• Recent results and perspectives on cosmology and fundamental physics from microwave surveys
• Anomaly Induced Inflation in the Minimal Quartic Extension of Einstein's Gravity
• Generalized Noether Theorem for Gauss-Bonnet Cosmology
• Dark Radiation and Inflationary Freedom
• Accidental deep field bias in CMB T and SNe $z$ correlation
• Correlation Analysis between Tibet AS-$\gamma$ TeV Cosmic Ray and WMAP Nine-year Data
• The Distortion of the Cosmic Microwave Background by the Milky Way
• Weak Lensing Effect on CMB in the Presence of a Dipole Anisotropy
• Condensate decay in a radiation dominated cosmology
• A revisited Correction to the Halo Mass Function for local-type Primordial non-Gaussianity
• Circumventing Cosmic Variance via Remote Quadrupole Measurements
• Constraints on polynomial inflation under power-law perturbations
• Nonrelativistic superfluids in cosmology from a relativistic approach: Revisiting two formulations of superfluidity
• Uniformity of Cosmic Microwave Background as a Non-Inflationary Geometrical Effect
• $keV$ sterile neutrino as dark matter in doublet left-right symmetric model with $A_4$ modular symmetry
• Dark Radiation and Inflationary Freedom
• Optimisation of the Population Monte Carlo algorithm: Application to constraining isocurvature models with cosmic microwave background data
• Accurate and efficient likelihood modeling for large-scale CMB data
• On the computational feasibility of Bayesian end-to-end analysis of LiteBIRD simulations within Cosmoglobe
• Inflationary study of non-Gaussianity using two-dimensional geometrical measures of CMB temperature maps
• Generic inference of inflation models by local non-Gaussianity
• Yellow Post-Asymptotic-Giant-Branch Stars as Standard Candles. I. Calibration of the Luminosity Function in Galactic Globular Clusters
• Bayes' Theorem, Inflation, and the Ekpyrotic Universe
• Mitigating point-source contamination in CMB polarization: a Generalized Point Spread Function fitting approach
• Spectroscopic galaxy redshifts in the Peanut cluster -- a massive nearly head-on cluster merger shortly after pericenter passage
• Bouncing Cosmologies in modified gravity with space time torsion
• The Universe Originating from an Empty Planck-Size Torus
• Gravitational wave of the Bianchi VII universe: particle trajectories, geodesic deviation and tidal accelerations
• Quantum dynamics of the early universe
• Secondary gravitational waves against a strong gravitational wave in the Bianchi VI universe
• Mitigating Cosmic Microwave Background Shadow Degradation of Tensor-to-scalar Ratio Measurements through Map-based Studies
• QUIJOTE-TFGI polarization calibration -- Ground characterization and on-sky validation with Tau A and the Moon
• Two fluid CFL strange quark stars with scalar dark matter: critical mass and mass gap implications
• Probing CMB Polarization Gaussianity with the Statistics of Unpolarized Points: Non-Gaussianity of Planck Data and Prospects for Future B-Mode Measurements
• A global view on star formation: The GLOSTAR Galactic plane survey XII. Effelsberg's continuum view and data release
• Modeling Long-Wavelength Amorphous Dust Emission Based on the Physically Motivated Soft-Potential Model
• Local bandpower diagnostics for the hemispherical power asymmetry in CMB E-mode polarization
• Investigation of homogeneity and matter distribution on large scales using large quasar groups
• Initial Investigations of the Outskirts of XLSSC 122
• Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension
• Brane induced cosmological acceleration and crossing of w_{eff}=-1
• Linear perturbations of an exact gravitational wave in the Bianchi IV universe
• Do We Have Sufficient Knowledge of the Galactic Foreground Emission in Cosmic Microwave Background Science?
• A new approach of estimating the Galactic thermal dust and synchrotron polarized emission template in the microwave bands
• A new approach to the thermodynamics of scalar-tensor gravity
• Investigating non-Gaussianity in Cosmic Microwave Background Temperature Maps using Spherical Harmonic Phases
• Asymmetry and non-random orientation of the inflight effective beam pattern in the WMAP Data
• Temperature Anisotropy of the CMBR and the Non-zero Cosmological Constant
• Anisotropic evolution of D-dimensional FRW spacetime
• Detectability of Galactic Faraday Rotation in Multi-wavelength CMB Observations: A Cross-Correlation Analysis of CMB and Radio Maps
• B-mode polarization forecasts for GreenPol
• Ciii]$\lambda 1909$ emission as an alternative to Ly$\alpha$ in the reionization era: the dependence of Ciii] and Ly$\alpha$ at $3<z<4$ from the VANDELS survey