Planck 2013 results. I. Overview of products and scientific results

Abstract

The ESA's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14 May 2009 and has been scanning the microwave and submillimetre sky continuously since 12 August 2009. This paper gives an overview of the mission and its performance, the processing, analysis, and characteristics of the data, the scientific results, and the science data products and papers in the release. The science products include maps of the CMB and diffuse extragalactic foregrounds, a catalogue of compact Galactic and extragalactic sources, and a list of sources detected through the SZ effect. The likelihood code used to assess cosmological models against the Planck data and a lensing likelihood are described. Scientific results include robust support for the standard six-parameter LCDM model of cosmology and improved measurements of its parameters, including a highly significant deviation from scale invariance of the primordial power spectrum. The Planck values for these parameters and others derived from them are significantly different from those previously determined. Several large-scale anomalies in the temperature distribution of the CMB, first detected by WMAP, are confirmed with higher confidence. Planck sets new limits on the number and mass of neutrinos, and has measured gravitational lensing of CMB anisotropies at greater than 25 sigma. Planck finds no evidence for non-Gaussianity in the CMB. Planck's results agree well with results from the measurements of baryon acoustic oscillations. Planck finds a lower Hubble constant than found in some more local measures. Some tension is also present between the amplitude of matter fluctuations derived from CMB data and that derived from SZ data. The Planck and WMAP power spectra are offset from each other by an average level of about 2% around the first acoustic peak.

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• The Cosmic Microwave Background: The history of its experimental investigation and its significance for cosmology
• Testing deviations from $\Lambda$CDM with growth rate measurements from 6 Large Scale Structure Surveys at $\mathbf{z}=0.06$ to 1
• An extensive investigation of the Generalised Dark Matter model
• Quantifying Tensions between CMB and Distance Datasets in Models with Free Curvature or Lensing Amplitude
• Bayesian inflationary reconstructions from Planck 2018 data
• Does Current Data Prefer a Non-minimally Coupled Inflaton?
• The Knotted Sky I: Planck constraints on the primordial power spectrum
• The Jubilee ISW Project II: observed and simulated imprints of voids and superclusters on the cosmic microwave background
• Constraining f(R) gravity with PLANCK data on galaxy cluster profiles
• BICEP2/Keck Array IV: Optical Characterization and Performance of the BICEP2 and Keck Array Experiments
• Modified Dust and the Small Scale Crisis in CDM
• The reconstruction of inflationary potentials
• Evolution of the cold gas properties of simulated post-starburst galaxies
• SEDIGISM: The kinematics of ATLASGAL filaments
• Constraints and tensions in testing general relativity from Planck and CFHTLenS including intrinsic alignment systematics
• GALExtin: An alternative online tool to determine the interstellar extinction in the Milky Way
• A machine learning approach to mapping baryons onto dark matter haloes using the EAGLE and C-EAGLE simulations
• Early Cosmology Constrained
• A review of unsupervised learning in astronomy
• SIBELIUS-DARK: a galaxy catalogue of the Local Volume from a constrained realisation simulation
• Dark matter and U(1)' symmetry for the right-handed neutrinos
• Covariance of CMB anomalies
• Latest NIKA results and the NIKA-2 project
• Predicting accreted satellite galaxy masses and accretion redshifts based on globular cluster orbits in the E-MOSAICS simulations
• The evolution of the oxygen abundance gradients in star-forming galaxies in the EAGLE simulations
• Search for dark Higgsstrahlung in e+ e- -> mu+ mu- and missing energy events with the KLOE experiment
• On stability of exponential cosmological solutions with non-static volume factor in the Einstein-Gauss-Bonnet model
• Maps of the Southern Millimeter-wave Sky from Combined 2500 deg${}^2$ SPT-SZ and Planck Temperature Data
• Testing General Relativity with Growth rate measurement from Sloan Digital Sky Survey III Baryon Oscillations Spectroscopic Survey galaxies
• Combined analysis of galaxy cluster number count, thermal Sunyaev-Zel'dovich power spectrum, and bispectrum
• The Jubilee ISW Project I: simulated ISW and weak lensing maps and initial power spectra results
• An application of machine learning techniques to galaxy cluster mass estimation using the MACSIS simulations
• The Cluster-EAGLE project: velocity bias and the velocity dispersion - mass relation of cluster galaxies
• Constraints on the Nambu-Goto cosmic string contribution to the CMB power spectrum in light of new temperature and polarisation data
• Cosmological distance indicators
• Stochastic Background of Gravitational Waves from Fermions -- Theory and Applications
• Measuring Baryon Acoustic Oscillations from the clustering of voids
• Low redshift observational constraints on tachyon models of dark energy
• The origin of compact galaxies with anomalously high black hole masses
• The 80 Ms follow-up of the X-ray afterglow of GRB 130427A challenges the standard forward shock model
• The abundance and physical properties of O VII and O VIII X-ray absorption systems in the EAGLE simulations
• Young star cluster populations in the E-MOSAICS simulations
• Updated measurements of the dark matter halo masses of obscured quasars with improved WISE and Planck data
• Quintessence with Yukawa Interaction
• Revealing the properties of void galaxies and their assembly using the EAGLE simulation
• Planck intermediate results. XVI. Profile likelihoods for cosmological parameters
• Search for a light charged Higgs boson in the H${}^{\pm }$ $\to$ cs channel in proton-proton collisions at $\sqrt{s}=$ 13 TeV
• The diversity of rotation curves of simulated galaxies with cusps and cores
• iPTF13beo: The Double-Peaked Light Curve of a Type Ibn Supernova Discovered Shortly after Explosion
• Solution of Dirac equation and greybody radiation around a regular Bardeen black hole surrounded by quintessence
• The aftermath of the Great Collision between our Galaxy and the Large Magellanic Cloud
• A LOFAR-IRAS cross-match study: the far-infrared radio correlation and the 150-MHz luminosity as a star-formation rate
• Sommerfeld enhancements with vector, scalar and pseudoscalar force-carriers
• The Spectral Energy Distributions of Active Galactic Nuclei
• The Spectral Energy Distributions of Active Galactic Nuclei
• Comparison between hemisphere comparison method and dipole-fitting method in tracing the anisotropic expansion of the Universe use the Union2 dataset
• The Survey of Centaurus A's Baryonic Structures (SCABS). II. The Extended Globular Cluster System of NGC5128 and its Nearby Environment
• Constraining the anisotropy of the Universe via Pantheon supernovae sample
• Inflaton dark matter from incomplete decay
• The Evolving Block Universe and the Meshing Together of Times
• On the proper kinetic quadrupole CMB removal and the quadrupole anomalies
• Visualizing probabilistic models: Intensive Principal Component Analysis
• Squeezed Bispectrum in the $\delta N$ Formalism: Local Observer Effect in Field Space
• Deconstructing Thermal Sunyaev-Zel'dovich - Gravitational Lensing Cross-Correlations: Implications for the Intracluster Medium
• BeyondPlanck III. Commander3
• Cosmic evolution of dark energy in a generalized Rastall gravity
• The High Fraction of Thin Disk Galaxies Continues to Challenge ΛCDM Cosmology
• Higgs Phenomenology in the Two-Singlet Model
• The Secret Lives of Cepheids: Evolutionary Changes and Pulsation-Induced Shock Heating in the Prototype Classical Cepheid δ Cep
• Beyond Minimal Lepton Flavored Dark Matter
• Quantifying Concordance in Cosmology
• Top-philic Scalar Dark Matter with a Vector-like Fermionic Top Partner
• Diagnostics of Stellar Modelling from Spectroscopy and Photometry of Globular Clusters
• Constraining the evolution of the CMB temperature with SZ measurements from Planck data
• Including birefringence into time evolution of CMB: current and future constraints
• Energy Constraints and Phenomenon of Cosmic Evolution in $f(T,B)$ Framework
• Absolute Calibration of the Radio Astronomy Flux Density Scale at 22 to 43 GHz Using Planck
• Gravitational-wave constraints on the GWTC-2 events by measuring the tidal deformability and the spin-induced quadrupole moment
• Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe
• Galaxy formation in the PLANCK cosmology - III. The high-redshift universe
• Nonabelian Dark Matter with Resonant Annihilation
• Constraints on $\gamma$-CDM interactions matching the Planck data precision
• Hyperbolic Inflation in the Light of Planck 2015 data
• The Flavour Portal to Dark Matter
• How Unusual is the Milky Way's Assembly History?
• Reconstruction of constant slow-roll inflation
• Cosmological reconstruction and energy bounds in $f(R,R_{\alpha \beta }{R}^{\alpha \beta },\varphi )$ gravity
• Pre-inflationary primordial perturbations
• Constraining anisotropy of the universe from different groups of type-Ia supernovae
• Relativistic SZ temperature scaling relations of groups and clusters derived from the BAHAMAS and MACSIS simulations
• MultiDarkLens Simulations: weak lensing light-cones and data base presentation
• Constraining the kinetically dominated Universe
• Unexpected Topology of the Temperature Fluctuations in the Cosmic Microwave Background
• The Deep Diffuse Extragalactic Radio Sky at 1.75 GHz
• Detailed study of geodesics in the Kerr-Newman-(A)dS spactime and the rotating charged black hole spacetime in $f(R)$ gravity
• Synthetic CO, H2 and HI surveys of the Galactic 2nd Quadrant, and the properties of molecular gas
• Inflation and leptogenesis in the 3-3-1-1 model
• Holographic Dark Energy with Cosmological Constant
• Reanalysis of the binary neutron star mergers GW170817 and GW190425 using numerical-relativity calibrated waveform models
• The Atacama Cosmology Telescope: Microwave Intensity and Polarization Maps of the Galactic Center
• Shortcomings of New Parametrizations of Inflation
• Cosmic Inflation at the Crossroads
• CMB power spectrum of Nambu-Goto cosmic strings
• Search for Early Gamma-ray Production in Supernovae Located in a Dense Circumstellar Medium with the Fermi LAT
• C-Band All-Sky Survey: A First Look at the Galaxy
• H.E.S.S. and Suzaku observations of the Vela X pulsar wind nebula
• Polarimetry at millimeter wavelengths with the NIKA camera: calibration and performance
• Two-point Correlation Function of WMAP 9 year data
• Information Gains from Cosmological Probes
• Searching for Cosmic Strings in CMB Anisotropy Maps using Wavelets and Curvelets
• Inflation Model Selection meets Dark Radiation
• Light propagation in inhomogeneous and anisotropic cosmologies
• The New Numerical Galaxy Catalogue (ν^2 GC): Properties of Active Galactic Nuclei and Their Host Galaxies
• Constraining the redshift evolution of the Cosmic Microwave Background black-body temperature with PLANCK data
• Dark Radiation and Inflationary Freedom after Planck 2015
• The Herschel Virgo Cluster Survey. XX. Dust and gas in the foreground Galactic cirrus
• Inflation via Gravitino Condensation in Dynamically Broken Supergravity
• The nonlinear dynamical stability of infrared modifications of gravity
• Projected-Field Kinetic Sunyaev-Zel'dovich Cross-Correlations: Halo Model and Forecasts
• Post-Newtonian Approximation of Teleparallel Gravity Coupled with a Scalar Field
• Late-time backreaction from inflationary fluctuations of a non-minimally coupled massless scalar
• Mapping the Integrated Sachs-Wolfe Effect
• Adaptive mesh refinement simulations of a galaxy cluster merger - I. Resolving and modelling the turbulent flow in the cluster outskirts
• Investigation of Dark Matter in Minimal 3-3-1 Models
• Is there evidence for additional neutrino species from cosmology?
• HERschel Observations of Edge-on Spirals (HEROES). IV. Dust energy balance problem
• First Light And Reionisation Epoch Simulations (FLARES) VII: The Star Formation and Metal Enrichment Histories of Galaxies in the early Universe
• Calibrated, cosmological hydrodynamical simulations with variable IMFs I: Method and effect on global galaxy scaling relations
• Remarks on the weak cosmic censorship conjecture of RN-AdS black holes with cloud of strings and quintessence under the scalar field
• Electron EDM as a Sensitive Probe of PeV Scale Physics
• Cosmological constraints to dark matter with two- and many-body decays
• Do the observational data favor a local void?
• Multifrequency study of GHz-peaked spectrum sources
• Optical validation and characterization of Planck PSZ1 sources at the Canary Islands observatories. I. First year of ITP13 observations
• AMICO galaxy clusters in KiDS-DR3: cosmological constraints from large-scale stacked weak lensing profiles
• Out of the White Hole: A Holographic Origin for the Big Bang
• Effective Potential and Topological Photon Spheres: A Novel Approach to Black Hole Parameter Classification
• Electroweak Baryogenesis and Dark Matter via a Pseudoscalar vs. Scalar
• Neutrino masses, leptogenesis, and sterile neutrino dark matter
• Constraining Curvatonic Reheating
• The Ellipsoidal Universe in the Planck Satellite Era
• Constraining the dynamical dark energy parameters: Planck-2013 vs WMAP9
• Measurement of detector-corrected observables sensitive to the anomalous production of events with jets and large missing transverse momentum in $pp$ collisions at $\sqrt{s}=13$ TeV using the ATLAS detector
• Evidence for galaxy dynamics tracing background cosmology below the de Sitter scale of acceleration
• A Combined View of Sterile-Neutrino Constraints from CMB and Neutrino Oscillation Measurements
• Probing hot gas around luminous red galaxies through the Sunyaev-Zel'dovich effect
• Fermionic Semi-Annihilating Dark Matter
• Scalar and tensor perturbations in loop quantum cosmology: High-order corrections
• Non-linear curvature perturbation in multi-field inflation models with non-minimal coupling
• The chemical structure of young high-mass star-forming clumps: (II) parsec-scale CO depletion and deuterium fraction of $\mathrm{HC}{\mathrm{O}}^{+}$
• The effect of gas accretion on the radial gas metallicity profile of simulated galaxies
• Methods for pixel domain correction of EB leakage
• Energy Conditions in Higher Derivative $f(R,\square R,T)$ Gravity
• Primordial perturbations with pre-inflationary bounce
• All-sky census of Galactic high-latitude molecular intermediate-velocity clouds
• Probing Modified Gravity Theories with ISW and CMB Lensing
• Parameter splitting in dark energy: is dark energy the same in the background and in the cosmic structures?
• Reverse Shock Emission Revealed in Early Photometry in the Candidate Short GRB 180418A
• Modified Brans-Dicke cosmology with matter-scalar field interaction
• Developing a unified pipeline for large-scale structure data analysis with angular power spectra -- I. The importance of redshift-space distortions for galaxy number counts
• The connection between the parsec-scale radio jet and gamma-ray flares in the blazar 1156+295
• Quantum dynamics of the black hole interior in LQC
• Nonthermal production of dark radiation and dark matter
• Exploring Cosmic Origins with CORE: Cluster Science
• Calibrating Cluster Number Counts with CMB lensing
• On the detectability of visible-wavelength line emission from the local circumgalactic and intergalactic medium
• BeyondPlanck I. Global Bayesian analysis of the Planck Low Frequency Instrument data
• Random spherical hyperbolic diffusion
• Gravitino LSP and leptogenesis after the first LHC results
• Radio-Gamma-ray connection and spectral evolution in 4C +49.22 (S4 1150+49): the Fermi, Swift and Planck view
• ZOMG II: Does the halo assembly history influence central galaxies and gas accretion?
• Kinematic analysis of EAGLE simulations: Evolution of ${\lambda }_{Re}$ and its connection with mergers and gas accretion
• Testing the Dipole Modulation Model in CMBR
• The Cosmic Equation of State
• The formation of early-type galaxies through monolithic collapse of gas clouds in Milgromian gravity
• Vacuum and Gravitons of Relic Gravitational Waves, and Regularization of Spectrum and Energy-Momentum Tensor
• The lensing properties of subhaloes in massive elliptical galaxies in sterile neutrino cosmologies
• Fast Bayesian inference for slow-roll inflation
• The Effects of Rayleigh Scattering on the CMB and Cosmic Structure
• Fluctuations of the total number of critical points of random spherical harmonics
• Planck intermediate results. XLV. Radio spectra of northern extragalactic radio sources
• Hot WHIM counterparts of FUV OVI absorbers: Evidence in the line-of-sight towards quasar 3C 273
• Reducing biases on $H_0$ measurements using strong lensing and galaxy dynamics: results from the EAGLE simulation
• A novel sampling theorem on the rotation group
• Baryon Number, Lepton Number, and Operator Dimension in the SMEFT with Flavor Symmetries
• Cosmological evidence for leptonic asymmetry after Planck
• Reheating temperature in non-minimal derivative coupling model
• X-ray Line from the Dark Transition Electric Dipole
• Using ALMA to resolve the nature of the early star-forming large-scale structure PLCK G073.4-57.5
• The detection of the imprint of filaments on cosmic microwave background lensing
• Constraining light sterile neutrino mass with the BICEP2/Keck Array 2014 B-mode polarization data
• Feeding cosmic star formation: Exploring high-redshift molecular gas with CO intensity mapping
• Primordial non-Gaussianity in the bispectra of large-scale structure
• Late-time quantum backreaction of a very light nonminimally coupled scalar
• Baryons Shaping Dark Matter Haloes
• High significance detection of the tSZ effect relativistic corrections
• Discovery of kpc-scale line emission in barred galaxies, not linked to AGN or star formation
• The Resolved Sunyaev--Zel'dovich Profiles of Nearby Galaxy Groups
• Sound speed of scalar field dark energy: weak effects and large uncertainties
• Planck intermediate results. XLIV. The structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap
• LHC Phenomenology of SO(10) Models with Yukawa Unification II
• Boltzmann-Fokker-Planck formalism for dark-matter--baryon scattering
• Role of magnetic fields in fueling Seyfert nuclei
• The information content of cosmic microwave background anisotropies
• GalWeight Application: A publicly-available catalog of dynamical parameters of 1,800 galaxy clusters from SDSS-DR13, ($GalWCat19$)
• Emergent universe scenario and the low CMB multipoles
• Cosmological Magnetogenesis: The Biermann Battery during the Epoch of Reionization
• Impact of particles on the Planck HFI detectors: Ground-based measurements and physical interpretation
• Modified Lyth bound and implications of BICEP2 results
• A new calibration method of sub-halo orbital evolution for semi-analytic models
• Dark-matter-deficient galaxies in hydrodynamical simulations
• Energy and momentum of Bianchi Type VI_h Universes
• Probing neutrino physics with a self-consistent treatment of the weak decoupling, nucleosynthesis, and photon decoupling epochs
• Constraints on the dark matter and dark energy interactions from weak lensing bispectrum tomography
• The orbital phase space of contracted dark matter halos
• Physics of the cosmic microwave background anisotropy
• Colloquium: Time-reversal violation with quantum-entangled B mesons
• Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
• New radio observations of anomalous microwave emission in the HII region RCW175
• Redshift evolution of the dark matter haloes shapes
• A Comparison of Maps and Power Spectra Determined from South Pole Telescope and Planck Data
• The warm-hot circumgalactic medium around EAGLE-simulation galaxies and its detection prospects with X-ray line emission
• The $I\kappa \epsilon \alpha$ model of feedback-regulated galaxy formation
• Assessing Consistency Between WMAP 9-year and Planck 2015 Temperature Power Spectra
• The phenomenology of beyond Horndeski gravity
• Gaussian Approximation of Peak Values in the Integrated Sachs-Wolfe Effect
• Anisotropic Spheres Via Embedding Approach in $f(R,\varphi ,X)$ Gravity
• On the Origin of Flux Ratio Anomaly in Quadruple Lens Systems
• Radiative Decays of Cosmic Background Neutrinos in Extensions of MSSM with a Vector Like Lepton Generation
• The evolution of the UV luminosity function of globular clusters in the E-MOSAICS simulations
• Separating astrophysical sources from indirect dark matter signals
• Non-equilibrium thermodynamics of gravitational screens
• Cosmological anisotropy from non-comoving dark matter and dark energy
• Constraints on a seesaw model leading to quasidegenerate neutrinos and signatures at the LHC
• Galaxy and Mass Assembly (GAMA): Formation and Growth of Elliptical Galaxies in the Group Environment
• Light of Planck-2015 on Non-Canonical Inflation
• The metallicity distribution of HI systems in the EAGLE cosmological simulation
• The SAMI Galaxy Survey: bulge and disk stellar population properties in cluster galaxies
• Circumstellar Dust, PAHs, and Stellar Populations in Early-Type Galaxies: Insights from GALEX and WISE
• SILC: a new Planck Internal Linear Combination CMB temperature map using directional wavelets
• Galaxy properties in the cosmic web of EAGLE simulation
• Large Neutrino Magnetic Dipole Moments in MSSM Extensions
• Photometric Observations of Supernova 2013cq Associated with GRB 130427A
• The SAMI-Fornax Dwarfs Survey III: Evolution of [$\alpha$/Fe] in dwarfs, from Galaxy Clusters to the Local Group
• Testing CPT Symmetry with Current and Future CMB Measurements
• The assembly of spheroid-dominated galaxies in the EAGLE simulation
• Reconstructing QCD ghost $f(R,T)$ models
• The bispectra of galactic CMB foregrounds and their impact on primordial non-Gaussianity estimation
• Microwave Background Polarization as a Probe of Large-Angle Correlations
• Imprints of dark matter on the structural properties of minimally deformed compact stars
• A comparison of CMB Angular Power Spectrum Estimators at Large Scales: the TT case
• A Neural-Network based estimator to search for primordial non-Gaussianity in Planck CMB maps
• Calibrated, cosmological hydrodynamical simulations with variable IMFs III: Spatially-resolved properties and evolution
• Probing the statistical properties of CMB $B$-mode polarization through Minkowski Functionals
• GalWeight: A New and Effective Weighting Technique for Determining Galaxy Cluster and Group Membership
• Interacting $F(R,T)$ gravity with modified Chaplygin gas
• Early dark energy and its interaction with dark matter
• North-South non-Gaussian asymmetry in PLANCK CMB maps
• Status and prospects of the nMSSM after LHC Run-1
• Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
• The Cosmic Dispersion Measure in the EAGLE Simulations
• Effects of overlapping sources on cosmic shear estimation: Statistical sensitivity and pixel-noise bias
• Dissipative Universe-Inflation with Soft Singularity
• On stable exponential cosmological solutions in the EGB model with a $\Lambda$-term in dimensions D = 5,6,7,8
• Kasner solutions, climbing scalars and big-bang singularity
• Revised bounds on local cosmic strings from NANOGrav observations
• Observational Constraints on Varying-alpha Domain Walls
• Relating the inhomogeneous power spectrum to the CMB hemispherical anisotropy
• The Local Value of $H_0$ in an Inhomogeneous Universe
• Constraining cosmology with the cosmic microwave and infrared backgrounds correlation
• Evolution of Cluster of Stars in f(R) Gravity
• Investigation of the Origin of the Anomalous Microwave Emission in Lambda Orionis
• Characterization and Physical Explanation of Energetic Particles on Planck HFI Instrument
• Joint Analysis of Galaxy-Galaxy Lensing and Galaxy Clustering: Methodology and Forecasts for DES
• The Cosmology Large Angular Scale Surveyor Receiver Design
• The Impact of Non-Gaussianity upon Cosmological Forecasts
• Breaking Be: a sterile neutrino solution to the cosmological lithium problem
• Elementary Theorems Regarding Blue Isocurvature Perturbations
• Optical validation and characterization of Planck PSZ2 sources at the Canary Islands observatories. II. Second year of LP15 observations
• TASI 2014 Lectures: The Hunt for Dark Matter
• Can Self-Ordering Scalar Fields explain the BICEP2 B-mode signal?
• Light Sterile Neutrinos and Inflationary Freedom
• On the Detection of CMB B-modes from Ground at Low Frequency
• Riemann-Eddington theory: Incorporating matter, degravitating the cosmological constant
• On Electroweak Phase Transition and Di-photon Excess with a 750 GeV Scalar Resonance
• Orion revisited III. The Orion Belt population
• A high-resolution cosmological simulation of a strong gravitational lens
• Testing approximate predictions of displacements of cosmological dark matter halos
• Characterising Tidal Features Around Galaxies in Cosmological Simulations
• Compactly supported linearised observables in single-field inflation
• Phenomenological approaches of inflation and their equivalence
• On the stability of satellites at unstable libration points of sun-planet-moon systems
• Theoretical reevaluations of the black hole mass - bulge mass relation - I. Effect of the seed black hole mass
• A unified scenario for the origin of spiral and elliptical galaxy structural scaling laws
• The mass-size plane of EAGLE galaxies
• On the consistency of tachyon warm inflation with viscous pressure
• The dearth of difference between central and satellite galaxies II. Comparison of observations with L-GALAXIES and EAGLE in star formation quenching
• Dark Matter from Conformal Sectors
• Deciphering the unusual stellar progenitor of GRB 210704A
• Stellar Mass Assembly of Brightest Cluster Galaxies at Late Times
• BeyondPlanck X. Bandpass and beam leakage corrections
• The present-day gas content of simulated field dwarf galaxies
• Cosmic Variance of the Spectral Index from Mode Coupling
• Velocity dispersion and dynamical masses for 388 Galaxy Clusters and groups. Calibrating the $M_{\mathrm{SZ}}$--$M_{\mathrm{dyn}}$ scaling relation for the PSZ2 sample
• Disentangling redshift-space distortions and nonlinear bias using the 2D power spectrum
• BeyondPlanck XII. Cosmological parameter constraints with end-to-end error propagation
• Novel Collider and Dark Matter Phenomenology of a Top-philic Z'
• Sun-Earth Lagrange reference for fundamental physics and navigation
• A new polarisation amplitude bias reduction method
• Determination of Polarization Angles in CMB Experiments and Application to CMB Component Separation Analyses
• From BeyondPlanck to Cosmoglobe: Preliminary $WMAP$ $Q$-band analysis
• Brane SUSY Breaking and Inflation: Implications for Scalar Fields and CMB Distorsion
• On exponential cosmological type solutions in the model with Gauss-Bonnet term and variation of gravitational constant
• Distances to nearby molecular clouds traced by young stars
• Sparse image reconstruction on the sphere: analysis and synthesis
• The Borg Cube Simulation: Cosmological Hydrodynamics with CRK-SPH
• The Kullback-Leibler Divergence as an Estimator of the Statistical Properties of CMB Maps
• BeyondPlanck XI. Bayesian CMB analysis with sample-based end-to-end error propagation
• $f(T)$ non-linear massive gravity and the cosmic acceleration
• Forecast constraints on Anisotropic Stress in Dark Energy using gravitational-waves
• BeyondPlanck VI. Noise characterization and modelling
• The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations
• Cosmologically probing ultra-light particle dark matter using 21 cm signals
• Flavor changing in the flipped trinification
• The Cluster-EAGLE project: a comparison of dynamical mass estimators using simulated clusters
• On the Viability of Thermal Well-Tempered Dark Matter in SUSY GUTs
• The "Maggie" filament: Physical properties of a giant atomic cloud
• Azimuthal variations of oxygen abundance profiles in star-forming regions of disc galaxies in the EAGLE simulations
• Temperature in warm inflation in non minimal kinetic coupling model
• Stable exponential cosmological solutions with zero variation of $G$ and three different Hubble-like parameters in the Einstein-Gauss-Bonnet model with a $\Lambda$-term
• Modified Gauss-Bonnet Gravity with Radiating Fluids
• General Relativistic corrections in density-shear correlations
• Planck/SDSS Cluster Mass and Gas Scaling Relations for a Volume-Complete redMaPPer Sample
• On the Trispectrum of Galileon Inflation
• The redshift-space galaxy two-point correlation function and baryon acoustic oscillations
• Baryonic properties of nearby galaxies across the stellar-to-total dynamical mass relation
• Red, Straight, no bends: primordial power spectrum reconstruction from CMB and large-scale structure
• Vector dark energy models with quadratic terms in the Maxwell tensor derivatives
• Super-Natural MSSM
• More on the Hypercharge Portal into the Dark Sector
• Bounds on Higher Derivative $f(R,\square R,T)$ Models from Energy Conditions
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines I. The [C II] 158 microns line at z~0
• Theoretical terms of contemporary cosmology as intellectual artifacts
• Cosmological Evolution of Pilgrim Dark Energy
• Chameleon Field Dynamics During Inflation
• Studying the Intervention of an Unusual Term in $f(T)$ Gravity via Noether Symmetry
• Skewness and Kurtosis as Indicators of Non-Gaussianity in Galactic Foreground Maps
• Maps of the Magellanic Clouds from Combined South Pole Telescope and Planck Data
• Tilt and Tensor-to-Scalar Ratio in Multifield Monodromy Inflation
• The Higgs Boson is found: What is next?
• HI, star formation and tidal dwarf candidate in the Arp 305 system
• Constraining dark sector perturbations I: cosmic shear and CMB lensing
• Multi-fluid cosmology in Einstein gravity: analytical solutions
• Calibrated, cosmological hydrodynamical simulations with variable IMFs II: Correlations between the IMF and global galaxy properties
• AFGL 5180 and AFGL 6366S: sites of hub-filament systems at the opposite edges of a filamentary cloud
• Detecting the neutral IGM in filaments with the SKA
• Cosmology based on $f(R)$ gravity with $\mathcal{O}(1)$ eV sterile neutrino
• Constraining Dark Energy With Stacked Concave Lenses
• Standard Model and Graviweak Unification with (Super)Renormalizable Gravity. Part I: Visible and Invisible Sectors of the Universe
• Polymer inflation
• CMASS galaxy sample and the ontological status of the cosmological principle
• Evaluating hydrodynamical simulations with green valley galaxies
• Rotation of the CMB polarisation by foreground lensing
• Non-virialised clusters for detection of Dark Energy-Dark Matter interaction
• Superconducting dark energy
• Bayesian approach to radio frequency interference mitigation
• Ram pressure statistics for bent tail radio galaxies
• Requirements for future CMB satellite missions: photometric and band-pass response calibration
• Investigation of Dark Matter in the 3-2-3-1 Model
• Emergence of new oscillation modes in dark matter admixed neutron stars
• The Next Generation X-ray Galaxy Survey with eROSITA
• The Q/U Imaging ExperimenT: Polarization Measurements of the Galactic Plane at 43 and 95 GHz
• Fourier-space combination of Planck and Herschel images
• Marginalised Normal Regression: Unbiased curve fitting in the presence of x-errors
• Generation of Circular Polarization of CMB via Polarized Compton Scattering
• Supersymmetric Partially Interacting Dark Matter
• Polarimetric and photometric investigation of a dark globule LDN 1225: distance, extinction law, and magnetic fields
• Unveiling the main sequence of galaxies at $z\ge 5$ with the James Webb Space Telescope: predictions from simulations
• Cosmological fluids in the equivalence between Rastall and Einstein gravity
• Removing beam asymmetry bias in precision CMB temperature and polarisation experiments
• Constraining the baryon fraction in the Warm Hot Intergalactic Medium at low redshifts with PLANCK data
• Clustering in the Simulated H$\alpha$ Galaxy Redshift Survey from Nancy Grace Roman Space Telescope
• Cosmo++: An Object-Oriented C++ Library for Cosmology
• The Multi-Tracer Optimal Estimator applied to VIPERS
• Cosmic Acceleration and Anisotropic models with Magnetic field
• Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Our Galaxy
• Non-Gaussian CMB and LSS statistics beyond polyspectra
• Impact of Primordial Black Hole Dark Matter on Gas Properties at Very High Redshift: A Semi-Analytical Model
• Twin Cogenesis
• CosmoDM and its application to Pan-STARRS data
• Andreev Current for low temperature thermometry
• Dealing with missing data: An inpainting application to the MICROSCOPE space mission
• Galaxy cluster rotation revealed in the MACSIS simulations with the kinetic Sunyaev-Zeldovich effect
• First Light And Reionisation Epoch Simulations (FLARES) XII: The consequences of star-dust geometry on galaxies in the EoR
• Quantum corrections to the dynamics of the expanding universe
• Implications of Fermionic Dark Matter on recent neutrino oscillation data
• Detection capabilities of the Athena X-IFU for the warm-hot intergalactic medium using gamma-ray burst X-ray afterglows
• Galactic satellite systems in CDM, WDM and SIDM
• Large Blue Spectral Isocurvature Spectral Index Signals Time-Dependent Mass
• Spinning Bar and a Star-formation Inefficient Repertoire: Turbulence in Hickson Compact Group NGC7674
• The Cosmological Parameters (2023)
• The minimal adjoint-SU(5)xZ_4 GUT model
• Revisiting constraints on (pseudo)conformal Universe with Planck data
• Cosmological constraints on the neutron lifetime
• Optimizing future experiments of cosmic far-infrared background: a principal component approach
• Relic photon temperature versus redshift and the cosmic neutrino background
• An Inventory of Bispectrum Estimators for Redshift Space Distortions
• Is there a connection between "dark" and "light" physics?
• Selfish Dark Matter
• Abundance and group coalescence timescales of compact groups of galaxies in the EAGLE simulation
• A Novel CMB Component Separation Method: Hierarchical Generalized Morphological Component Analysis
• Black string surrounded by a static anisotropic quintessence fluid
• Imprint of baryons and massive neutrinos on velocity statistics
• Exploiting flux ratio anomalies to probe warm dark matter in future large scale surveys
• Weak Lensing Measurement of Filamentary Structure with the SDSS BOSS and Subaru Hyper Suprime-Cam Data
• Large-scale gauge spectra and pseudoscalar couplings
• SU(2)${}_{\mathrm{CMB}}$ and the cosmological model: angular power spectra
• Candidate high-redshift protoclusters and lensed galaxies in the Planck list of high-z sources overlapping with Herschel-SPIRE imaging
• Constraining Cosmological Parameters using the Cluster Mass-Richness Relation
• Testing anthropic reasoning for the cosmological constant with a realistic galaxy formation model
• A Quantum Window Onto Early Inflation
• High-Resolution Spectroscopy of Extremely Metal-Poor Stars from SDSS/SEGUE: II. Binary Fraction
• Linearized iterative least-squares (LIL): A parameter fitting algorithm for component separation in multifrequency CMB experiments such as Planck
• Maximum Likelihood Analysis of Low Energy CDMS II Germanium Data
• First Detection of ${}^3$He${}^{+}$ in the Planetary Nebula IC418
• Realization of Power-Law Inflation & Variants via Variation of the Strong Coupling Constant
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• A new map-making algorithm for CMB polarisation experiments
• How much cosmological information can be measured?
• The Transition from Diffuse Molecular Gas to Molecular Cloud Material in Taurus
• Holographic Ricci dark energy as running vacuum
• Relating galaxies across different redshift to study galaxy evolution
• Star formation histories of Coma Cluster galaxies matched to simulated orbits hint at quenching around first pericenter
• Characterising Strong Lensing Galaxy Clusters using the Millennium-XXL and MOKA simulations
• Evolution of the cosmic matter density field with a primordial magnetic field
• A radiation transfer model for the Milky Way. II The global properties and large scale structure
• Unveiling the environment and faint features of the isolated galaxy CIG 96 with deep optical and HI observations
• History of the gas fuelling star formation in eagle galaxies
• A cosmological model from emergence of space
• SZ Scaling Relations of Galaxy Groups and Clusters Near the North Ecliptic Pole
• Cosmic metal invaders: Intergalactic OVII as a tracer of the warm-hot intergalactic medium within cosmic filaments in the EAGLE simulation
• Connecting the Cosmic Star Formation Rate with the Local Star Formation
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• Testing isotropy of cosmos with WMAP and PLANCK data
• Modeling the cross power spectrum of Sunyaev-Zel'dovich and X-ray surveys
• A Study of Dirac Fermionic Dark Matters
• Improving Planck calibration by including frequency-dependent relativistic corrections
• X-Ray-to-Radio Offset Inference from Low-Count X-Ray Jets
• Probing Particle Physics from Top Down with Cosmic Strings
• The Herschel Virgo Cluster Survey. XV. Planck submillimetre sources in the Virgo Cluster
• CMB statistical anisotropy from noncommutative gravitational waves
• The Galactic Center Excess from Z3 Scalar Semi-Annihilations
• Average Energy Expended Per e-h Pair and Energy Scale Function for Germanium-Based Dark Matter Experiments
• Non-linear matter bispectrum in general relativity
• Anisotropies in Non-Thermal Distortions of Cosmic Light from Photon-Axion Conversion
• Test the Weak Cosmic Supervision Conjecture in Dark Matter-Black Hole System
• Supersymmetric SU(5) Grand Unification for a Post Higgs Boson Era
• Reconstructions of $f(\mathcal{P})$ and $f(\mathcal{Q})$ gravity models from $(m,n)$-type Barrow Holographic Dark Energy: Analysis and Observational Constraints
• Gravitational Lensing of Spherically Symmetric Black Holes in Dark Matter Halos
• Optimized Large-Scale CMB Likelihood And Quadratic Maximum Likelihood Power Spectrum Estimation
• Dark Matter with Topological Defects in the Inert Doublet Model
• Pairwise kSZ signal extraction efficacy and optical depth estimation
• BeyondPlanck X. Planck LFI frequency maps with sample-based error propagation
• Cogeneration of Dark Matter and Baryons by Non-Standard-Model Sphalerons in Unified Models
• Follow-up analyses of the binary-neutron-star signals GW170817 and GW190425 by using post-Newtonian waveform models
• Perturbation level interacting dark energy model and its consequence on late-time cosmological parameters
• Emergence of space and expansion of universe
• Perturbations in Tachyon Dark Energy and their Effect on Matter Clustering
• Birth of de Sitter Universe from time crystal
• Effective Field Theory of Anisotropic Inflation and Beyond
• Vacuum contribution of photons in the theory with Lorentz and CPT-violating terms
• Optical validation and characterisation of Planck PSZ1 sources at the Canary Islands observatories. II. Second year of ITP13 observations
• Dust extinction map of the Galactic plane based on the VVV survey data
• Fundamental Physics and Cosmology with TianQin
• Measuring inflaton couplings via dark radiation as $\Delta N_{\mathrm{eff}}$ in CMB
• CHEX-MATE: pressure profiles of 6 galaxy clusters as seen by SPT and Planck
• Using EAGLE simulations to study the effect of observational constraints on the determination of HI asymmetries in galaxies
• The effect of local universe constraints on halo abundance and clustering
• Ray tracing the integrated Sachs-Wolfe effect through the light cones of the Dark Energy Universe Simulation -- Full Universe Runs
• Rapid numerical solutions for the Mukhanov-Sasaki equation
• Dark Energy Constraints on Masses and Sizes of Large Scale Cosmic Structures
• Finslerian dipolar modulation of the CMB power spectra at scales $2<l<600$
• The abundance of satellite galaxies in the inner region of $\Lambda$CDM Milky Way sized haloes
• Cosmic evolution in the background of non-minimal coupling in $f(R,T,R_{\mu \nu }{T}^{\mu \nu })$ Gravity
• Testing the Cubic Galileon Gravity model by the Milky Way rotation curve and SPARC data
• The SAMI Galaxy Survey: understanding observations of large-scale outflows at low redshift with EAGLE simulations
• Features in single field slow-roll inflation
• Very light dilaton and naturally light Higgs boson
• SU(2)$_{\tiny\mbox{CMB}}$ at high redshifts and the value of $H_0$
• Cosmic Sculpture: A new way to visualise the Cosmic Microwave Background
• SZ/X-ray scaling relations using X-ray data and Planck Nominal maps
• Limits on Entanglement Effects in the String Landscape from Planck and BICEP/Keck Data
• A new estimator of the deceleration parameter from galaxy rotation curves
• Stable exponential cosmological solutions with zero variation of G in the Einstein-Gauss-Bonnet model with a Lambda-term
• The low mass end of the neutral gas mass and velocity width functions of galaxies in $\Lambda$CDM
• The CIB-lensing bispectrum: impact on primordial non-Gaussianity and detectability for the Planck mission
• Cosmological constraints on superconducting dark energy models
• Towards the geometry of the universe from data
• The AGN Hubble Diagram and Its Implications for Cosmology
• Interacting parametrized post-Friedmann method
• Possible signature of distant foreground in the Planck data
• Mapping the temperature of the intra-cluster medium with the tSZ effect
• Fully renormalized stress tensor correlator in flat space
• Hubble flow variations as a test for inhomogeneous cosmology
• Sparse Inpainting and Isotropy
• BeyondPlanck IV. On end-to-end simulations in CMB analysis -- Bayesian versus frequentist statistics
• Evidence for Inflation in an Axion Landscape
• Excess in the High Frequency Radio Background: Insights from Planck
• Dynamics of dwarf galaxies in $f(R)$ gravity
• Physics of the Cosmic Microwave Background Radiation
• A sparse regression approach to modeling the relation between galaxy stellar masses and their host halos
• Geometrical measures of non-Gaussianity generated from single field Inflationary models
• N-body lensed CMB maps: lensing extraction and characterization
• Design and Calibration of the 34 GHz Yale Microwave Cavity Experiment
• Supersymmetric SO(10) Grand Unification at the LHC and Beyond
• Cosmic dipole tensions: confronting the cosmic microwave background with infrared and radio populations of cosmological sources
• Examples of stable exponential cosmological solutions with three factor spaces in EGB model with a $\Lambda$-term
• Self-Calibrating the Look-Elsewhere Effect: Fast Evaluation of the Statistical Significance Using Peak Heights
• Distribution of star formation rates during the rapid assembly of NGC 1399 as deduced from its globular cluster system
• Time-ordered data simulation and map-making for the PIXIE Fourier transform spectrometer
• Constraining the population of intermediate mass black holes by gamma-ray data of the Fornax cluster
• $Spitzer$-selected $z>1.3$ protocluster candidates in the LSST Deep Drilling Fields
• Bubble Universes With Different Gravitational Constants
• A new variable in scalar cosmology with exponential potential
• HP2 Survey V. Ophiuchus: Filament formation in a dispersing cloud complex
• Gamma rays from dark matter spikes in EAGLE simulations
• Evaluating the variance of individual halo properties in constrained cosmological simulations
• Galaxy interactions in filaments and sheets: insights from EAGLE simulations
• Statistical imprints of CMB B-type polarization leakage in an incomplete sky survey analysis
• On the application of dimensionality reduction and clustering algorithms for the classification of kinematic morphologies of galaxies
• More about a successful vector-tensor theory of gravitation
• Baryogenesis and Dark Matter in $U(1)$ Extensions
• Thermal gravitational-wave background in the general pre-inflationary scenario
• The QCD mass gap and quark deconfinement scales as mass bounds in strong gravity
• Observations of Galactic star-forming regions with the Cosmic Background Imager at 31 GHz
• Revised planet brightness temperatures using the Planck/LFI 2018 data release
• Simulated Predictions for HI at $z=3.35$ with the Ooty Wide Field Array (OWFA) -- II: Foreground Avoidance
• Revisiting the Birkhoff theorem from a dual null point of view
• The decisive future of inflation
• Dynamic Dark Energy Equation of State (EoS) and Hubble Constant analysis using type Ia supernovae from Union 2.1 dataset
• A spectroscopically confirmed z=1.327 galaxy-scale deflector magnifying a z~8 Lyman-Break galaxy in the Brightest of Reionizing Galaxies survey
• Suppressing the primordial tensor amplitude without changing the scalar sector in quadratic curvature gravity
• Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
• Emergent universe revisited through the CSL theory
• Tracing the magnetic field morphology of the LDN 1172/1174 cloud complex
• Advanced technologies for future ground-based, laser-interferometric gravitational wave detectors
• Direct detection of dark matter with resonant annihilation
• Entropy methods for CMB analysis of anisotropy and non-Gaussianity
• A study of 90 GHz dust emissivity on molecular cloud and filament scales
• Taller in the saddle: constraining CMB physics using saddle points
• Non-Linear Resonance in Relativistic Preheating
• Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
• Null geodesic structure for the Barriola-Vilenkin spacetime via $k$-essence
• Observing EAGLE galaxies with JWST: predictions for Milky Way progenitors and their building blocks
• Weak Lensing by Minifilament or Minivoid as the Origin of Flux-ratio Anomalies in Lensed Quasar MG0414+0534
• Orbits and adiabatic contraction in scalar field dark matter halos: revisiting the cusp-core problem in dwarf galaxies
• Decaying Fermionic Dark Matter Search with CALET
• Similarity dark energy models in Bianchi type - I space-time
• Some effects of different coordinate systems in cosmology
• Influence of dark matter on the structure of strange quark stars in one-fluid model
• Nonparametric test of consistency between cosmological models and multiband CMB measurements
• Searching for non-diagonal Mass varying mechanism in the ${\nu }_{\mu }$-${\nu }_{\tau }$ system
• Early-Matter-Like Dark Energy and the Cosmic Microwave Background
• A non-perturbative study of the evolution of cosmic magnetised sources
• Early Universe in the SU(3)_L X U(1)_X electroweak models
• A spatial-correlation analysis of the cubic 3-torus topology based on the Planck 2013 data
• Analytic Study of Cosmological Perturbations in a Unified Model of Dark Matter and Dark Energy with a Sharp Transition
• Bandpass mismatch error for satellite CMB experiments II: Correcting for the spurious signal
• Unveiling acoustic physics of the CMB using nonparametric estimation of the temperature angular power spectrum for Planck
• Constraints on primordial magnetic fields from the optical depth of the cosmic microwave background
• Planck and WMAP constraints on generalised Hubble flow inflationary trajectories
• A Potentially Detectable Gamma-Ray Line in the Fermi Galactic Center Excess -- In Light of One-Step Cascade Annihilations of Secluded (Vector) Dark Matter via the Higgs Portal
• Scaling Hydrodynamical Evolution of a Gravitating Dark-fluid Universe
• Fast radio bursts as probes of feedback from active galactic nuclei
• Polarization and variability of compact sources measured in Planck time-ordered data
• An atomic probe of dark matter differential interactions with elementary particles
• Unveiling galaxy pair alignment in cosmic filaments: A 3D exploration using EAGLE simulation
• Reconstructions of Einstein-Aether Gravity from Barrow Agegraphic and New Barrow Agegraphic Dark Energy models: Examinations and Observational Limits
• Testing and Combining Transient Spectral Classification Tools on 4MOST-like Blended Spectra
• The Velocity Field Olympics: Assessing velocity field reconstructions with direct distance tracers
• Andromeda's asymmetric satellite system as a challenge to cold dark matter cosmology
• String Theory clues for the low-$\ell$ CMB ?
• AMICO galaxy clusters in KiDS-DR3: constraints on $\Lambda$CDM from extreme value statistics
• Diffuse LINER-type emission from extended disc regions of barred galaxies
• Is the Cosmological Constant of Topological Origin?
• Simulations of cm-wavelength Sunyaev-Zel'dovich galaxy cluster and point source blind sky surveys and predictions for the RT32/OCRA-f and the Hevelius 100-m radio telescope
• An Introduction to the Planck Mission
• Dark Energy from Topology
• The NIKA polarimeter on science targets. Crab nebula observations at 150 GHz and dual-band polarization images of Orion Molecular Cloud OMC-1
• Impact of the vector dark matter on polarization of the CMB photon
• Time-like geodesic structure for the K-essence Emergent Barriola-Vilenkin type spacetime
• Reminiscences of my work with Richard Lewis Arnowitt
• Einstein-aether models III: conformally static metrics, perfect fluid and scalar fields
• Scalar field vs hydrodynamic models in the homogeneous isotropic cosmology
• Stellar initial mass function variation in massive early-type galaxies: the potential role of the deuterium abundance
• Dynamical analysis for a scalar-tensor model with Gauss-Bonnet and non-minimal couplings
• Quadrant asymmetry in the angular distribution of the Cosmic Microwave Background in the Planck satellite data
• Particle Physics after the Higgs-Boson Discovery: Opportunities for the Large Hadron Collider
• Covariant Predictions for Planck-Scale Features in Primordial Power Spectra
• Towards reconstruction of unlensed, intrinsic CMB power spectra from lensed map
• The roles of environment and interactions on the evolution of red and blue galaxies in the EAGLE simulation
• Flavor phenomenology of an extended 2HDM with inverse seesaw mechanism
• Black holes in $f(R)$ gravity coupled to nonlinear electromagnetic fields
• Filtering in CMB data analysis with application to ACT DR4 and Planck observations
• Stellar-gas kinematic misalignments in EAGLE: lifetimes and longevity of misaligned galaxies
• The impact of cosmic ray feedback during the epoch of reionisation
• CMB lensing forecasts for constraining the primordial perturbations: adding to the CMB temperature and polarization information
• A critical value for dark energy
• The Cold Dust Content of the Nearby Galaxies IC 5325, NGC 7496, NGC 7590, and NGC 7599
• Nonlinear evolution of anisotropic matter configurations under higher-order curvature corrections
• Low-$\ell$ CMB from String-Scale SUSY Breaking?
• Chaplygin Gas of Tachyon Nature Imposed by Symmetry and Constrained via H(z) Data
• Discovery of two quasars at $z=5$ from the OGLE Survey
• Dark Matter Directionality Revisited with a High Pressure Xenon Gas Detector
• A new mechanism for dark energy: the adaptive screening
• The Day the Universes Interacted: Quantum Cosmology without a Wave function
• Needlet estimation of cross-correlation between CMB lensing maps and LSS
• Tackling tangledness of cosmic strings by knot polynomial topological invariants
• DUNE potential for sub-GeV dark matter in proton beam dump mode
• Evolution equations dynamical system of the Lemaître--Tolman--Bondi metric containing coupled dark energy
• Subdominant Dark Matter sterile neutrino resonant production in the light of Planck
• Barboza-Alcaniz Equation of State Parametrization : Constraining the Parameters in Different Gravity Theories
• Interpreting Millimeter Emission from IMEGIN galaxies NGC 2146 and NGC 2976
• Gravitational Pressure and the Accelerating Universe
• From top-hat masking to smooth transitions: P-filter and its application to polarized microwave sky maps
• Single scalar cosmology
• Homology reveals significant anisotropy in the cosmic microwave background
• Scalar and tensor perturbation in vacuum inflation
• A sparse regression approach for populating dark matter halos and subhalos with galaxies
• Spectral Variations of the Sky: Constraints on Alternate Universes
• Infrared galaxies detected by the Atacama Cosmology Telescope
• Large Scale Cosmological Anomalies and Inhomogeneous Dark Energy
• Ultraviolet Extinction at High Galactic Latitudes II: The Ultraviolet Extinction Function
• The weird side of the Universe: Preferred axis
• Challenges and prospects for better measurements of the CMB intensity spectrum
• Hypergeometric viable models in $f(R)$ gravity
• Violation of Bell inequalities from Cosmic Microwave Background data
• First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmic dawn
• Scale-free power spectrums in the delayed cosmology
• Neutrino masses from CMB B-mode polarization and cosmic growth rate
• The Edges of Our Universe
• Thermal Sunyaev-Zeldovich measurements and cosmic infrared background leakage mitigation combining upcoming ground-based telescopes
• Irreversible Thermodynamics of the Universe: Constraints from Planck Data
• Tests of Modified Gravity Theories in the Solar System
• The long road to the Green Valley: Tracing the evolution of the Green Valley galaxies in the EAGLE simulation
• Primordial Black Holes Formed during Magneto-Hydrodynamic Turbulence in The Early Universe as Dominant Part of Dark Matter
• The expansion rate of the intermediate Universe in light of Planck
• The Radiowave Hunt for Young Stellar Object Emission and Demographics (RADIOHEAD): A Radio Luminosity$-$Spectral Type Dependence in Taurus$-$Auriga YSOs
• Direct measurement of evolving dark energy density and super-accelerating expansion of the universe
• Baryon-driven decontraction in Milky Way mass haloes
• Stability of horizon with pressure and volume of d-dimensional charged AdS black holes with cloud of strings and quintessence
• Improving Dark Matter Searches by Measuring the Nucleon Axial Form Factor: Perspectives from MicroBooNE
• Thermodynamics of irreversible particle creation phenomena and its cosmological consequence
• A Nonminimal Coupling Model and its Short-Range Solar System Impact
• Decoupled Sectors and Wolf-Rayet Galaxies
• Fundamental fields around compact objects: Massive spin-2 fields, Superradiant instabilities and Stars with dark matter cores
• Notes on f(R) Theories of Gravity
• Emulating the Non-Linear Matter Power-Spectrum in Mixed Axion Dark Matter Models
• Estimating the dense gas mass of molecular clouds using spatially unresolved 3 mm line observations
• First Light And Reionization Epoch Simulations (FLARES) -- XIX: Supermassive black hole mergers in the early Universe and their environmental dependence
• Spatial Curvature and Large Scale Lorentz Violation
• Gauge-independent Gravitational Waves from Cogenesis in a $B-L$ Conserving Universe
• A Cosmological Bragg Law: Interpreting the CMB as a Diffractogram of Foliated Spacetime
• Velocity dispersion functions of pressure-supported galaxies in EAGLE simulations with varying active galactic nucleus feedback
• Robustness of cosmological axion mass limits
• The Planck Catalogue of Compact Sources
• Geometry and General Relativity in the Groupoid Model with a Finite Structure Group
• Impact on Astrophysics and Elementary Particle Physics of recent and future solar neutrino data
• Fluids in cosmology
• Absorption of Fermionic Dark Matter in the PICO-60 C${}_3$F${}_8$ Bubble Chamber
• Constraining the $\gamma$-ray Emission Region for Fermi-Detected FSRQs by the Seed Photon Approach
• Simultaneous Estimation of Large-Scale Structure and Milky Way Dust Extinction from Galaxy Surveys
• Testing for directionality in the Planck polarization and lensing data
• Thermodynamics and overcharging problem in the extended phase spaces of charged AdS black holes with cloud of strings and quintessence under charged particle absorption
• Optimal bolometer transfer function deconvolution for CMB experiments through maximum likelihood mapmaking
• Gravitational attraction of ultra-relativistic matter: A new testbed for modified gravity at the Large Hadron Collider
• A new mechanism of realizing inflationary universe with recourse to backreaction of quantized free fields -- Inflation without inflaton --
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• The Simons Observatory: HoloSim-ML: machine learning applied to the efficient analysis of radio holography measurements of complex optical systems
• A Non-Local Reality: Is there a Phase Uncertainty in Quantum Mechanics?
• LYRA II: Cosmological dwarf galaxy formation with inhomogeneous Population III enrichment
• Categorizing models using Self-Organizing Maps: an application to modified gravity theories probed by cosmic shear
• Recent Progress in Cosmology and Particle Astrophysics
• ${}^3$He Abundances in Planetary Nebulae
• Relativistic Angular Redshift Fluctuations embedded in Large Scale Varying Gravitational Potentials
• Existence of Minkowski space
• Finite inflation in curved space
• Weak Lensing the non-Linear Ly-alpha Forest
• Asymmetry and non-random orientation of the inflight effective beam pattern in the WMAP Data
• Inflationary study of non-Gaussianity using two-dimensional geometrical measures of CMB temperature maps
• Recent results and perspectives on cosmology and fundamental physics from microwave surveys
• Strong Local Nondeterminism and Exact Modulus of Continuity for Spherical Gaussian Fields
• Cosmic Web-Halo Connection Between Twin Universes
• Dark Radiation and Inflationary Freedom
• Evaluation of multi-parameter likelihoods through iteration of two-dimensional slices
• The Continuous Tower of Scalar Fields as a System of Interacting Dark Matter -- Dark Energy
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
• Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window
• Constraints on the general solutions of Einstein cosmological equations by Hubble parameter times cosmic age: a historical perspective
• Attraction Induced by Mutual Quantum Measurements of Velocity
• CMB lensing tomography with clustering estimation of lens redshift distributions
• Quintessence with Hybrid Potential
• Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling
• Theoretical deduction of the Hubble law beginning with a MoND theory in context of the $\Lambda$FRW-Cosmology
• High resolution SZ observations at the IRAM 30-m telescope with NIKA
• Dynamical Models of the Milky Way in Action Space with LAMOST DR8 and GAIA EDR3
• Mocking IFU observations and metallicity diagnostics from cosmological simulations
• The Nature of High-Redshift Massive Quiescent Galaxies -- Searching for RUBIES-UDS-QG-z7 in FLARES
• Fluctuation of the Hubble parameter
• "Niñas Atómicas" (Atomic Girls): An initiative that generates opportunities for young girls in STEM
• Do We Have Sufficient Knowledge of the Galactic Foreground Emission in Cosmic Microwave Background Science?
• Dark Radiation and Inflationary Freedom
• Probing the Majorana Nature in Radiative Neutrino mass models with the same-sign dilepton final states at future colliders
• Accidental deep field bias in CMB T and SNe $z$ correlation
• Propagation of gravitational waves in a universe with slowly-changing equation of state
• Modeling Long-Wavelength Amorphous Dust Emission Based on the Physically Motivated Soft-Potential Model
• Quantum dynamics of the early universe
• Searches for Exotic Phenomena at ATLAS and CMS
• Stable exponential cosmological solutions with three factor spaces of dimensions $m=3$, $k_1=k$ and $k_2=k$ in the Einstein-Gauss-Bonnet model with a $\Lambda$-term
• Correlation Analysis between Tibet AS-$\gamma$ TeV Cosmic Ray and WMAP Nine-year Data
• A non-relativistic theory of quantum mechanics with local modulus symmetry
• A topological origin for Dark Energy
• Exploring the halo occupation distribution for moderate X-ray luminosity active galactic nuclei in the EAGLE cosmological simulation