Planck 2018 results. I. Overview and the cosmological legacy of Planck

Abstract

The European Space Agency's Planck satellite, which was dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013, producing deep, high-resolution, all-sky maps in nine frequency bands from 30 to 857GHz. This paper presents the cosmological legacy of Planck, which currently provides our strongest constraints on the parameters of the standard cosmological model and some of the tightest limits available on deviations from that model. The 6-parameter LCDM model continues to provide an excellent fit to the cosmic microwave background data at high and low redshift, describing the cosmological information in over a billion map pixels with just six parameters. With 18 peaks in the temperature and polarization angular power spectra constrained well, Planck measures five of the six parameters to better than 1% (simultaneously), with the best-determined parameter (theta_*) now known to 0.03%. We describe the multi-component sky as seen by Planck, the success of the LCDM model, and the connection to lower-redshift probes of structure formation. We also give a comprehensive summary of the major changes introduced in this 2018 release. The Planck data, alone and in combination with other probes, provide stringent constraints on our models of the early Universe and the large-scale structure within which all astrophysical objects form and evolve. We discuss some lessons learned from the Planck mission, and highlight areas ripe for further experimental advances.

arXiv comment61 pages, 40 figures, matches version accepted by A&A

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• Constraining Primordial Black Hole Formation from Single-Field Inflation
• Galaxy clustering in the DESI Legacy Survey and its imprint on the CMB
• Dark matter from an even lighter QCD axion: trapped misalignment
• Simulations and symmetries
• Cosmology Intertwined I: Perspectives for the Next Decade
• An overview of what current data can (and cannot yet) say about evolving dark energy
• Cosmic Shear Cosmology Beyond 2-Point Statistics: A Combined Peak Count and Correlation Function Analysis of DES-Y1
• Neutrino Mass Bounds in the era of Tension Cosmology
• Quantifying the global parameter tensions between ACT, SPT and Planck
• Cosmological Analysis of Three-Dimensional BOSS Galaxy Clustering and Planck CMB Lensing Cross Correlations via Lagrangian Perturbation Theory
• The Simons Observatory: Astro2020 Decadal Project Whitepaper
• The state of the dark energy equation of state circa 2023
• Cosmology in Extended Parameter Space with DESI Data Release 2 Baryon Acoustic Oscillations: A 2$\sigma$+ Detection of Nonzero Neutrino Masses with an Update on Dynamical Dark Energy and Lensing Anomaly
• Cosmological constraints on post-Newtonian parameters in effectively massless scalar-tensor theories of gravity
• A Consistent View of Interacting Dark Energy from Multiple CMB Probes
• A new technique for finding galaxies leaking Lyman-continuum radiation: [SII]-deficiency
• A New RASS Galaxy Cluster Catalog with Low Contamination Extending to $z\sim 1$ in the DES Overlap Region
• Regular rotation and low turbulence in a diverse sample of z ~ 4.5 galaxies observed with ALMA
• Cosmology From CMB Lensing and Delensed EE Power Spectra Using 2019-2020 SPT-3G Polarization Data
• A Measurement of the Degree Scale CMB B-mode Angular Power Spectrum with POLARBEAR
• Bounds on light sterile neutrino mass and mixing from cosmology and laboratory searches
• Cosmological Bound on the QCD Axion Mass, Redux
• Concentrations of Dark Haloes Emerge from Their Merger Histories
• The Origin of Parity Violation in Polarized Dust Emission and Implications for Cosmic Birefringence
• Search for dark matter produced in association with a leptonically decaying Z boson in proton-proton collisions at $\sqrt{s}=$ 13 TeV
• The observed galaxy power spectrum in General Relativity
• Microwave Background Temperature at a Redshift of 6.34 from H2O Absorption
• Can redshift errors bias measurements of the Hubble Constant?
• The star formation history of Upper Scorpius and Ophiuchus
• The Sloan Digital Sky Survey Peculiar Velocity Catalogue
• COMAP Early Science: I. Overview
• Explaining Cosmological Anisotropy: Evidence for Causal Horizons from CMB data
• Mapping the viable parameter space for testable leptogenesis
• Baryogenesis, Primordial Black Holes and MHz-GHz Gravitational Waves
• SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field
• Cosmic Shear Covariance Matrix in $w$CDM: Cosmology Matters
• Primordial black holes from stochastic tunnelling
• Data-driven Reconstruction of the Late-time Cosmic Acceleration with f(T) Gravity
• Quantifying the $S_8$ tension and evidence for interacting dark energy from redshift-space distortion measurements
• CMB spectral distortions revisited: a new take on $\mu$ distortions and primordial non-Gaussianities from FIRAS data
• An unusually low density ultra-short period super-Earth and three mini-Neptunes around the old star TOI-561
• Strongly lensed SNe Ia in the era of LSST: observing cadence for lens discoveries and time-delay measurements
• The Benefits of CMB Delensing
• Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements
• DESI luminous red galaxy samples for cross-correlations
• Inflation and Early Dark Energy with a Stage II Hydrogen Intensity Mapping Experiment
• Health checkup test of the standard cosmological model in view of recent Cosmic Microwave Background Anisotropies experiments
• Eryn : A multi-purpose sampler for Bayesian inference
• New Roads to the Small-Scale Universe: Measurements of the Clustering of Matter with the High-Redshift UV Galaxy Luminosity Function
• Dirac neutrinos and $N_{\mathrm{eff}}$ II: the freeze-in case
• Cosmological constraints on slow-roll inflation: an update
• New cosmological bounds on hot relics: Axions $\&$ Neutrinos
• Hot Extended Galaxy Halos Around Local L* Galaxies From Sunyaev-Zeldovich Measurements
• Constraining primordial non-Gaussianity using two galaxy surveys and CMB lensing
• Note on the bispectrum and one-loop corrections in single-field inflation with primordial black hole formation
• The Road to Precision Cosmology
• Mass bias evolution in tSZ cluster cosmology
• Cosmological parameter estimation for dynamical dark energy models with future fast radio burst observations
• Quantum fluctuations masquerade as halos: Bounds on ultra-light dark matter from quadruply-imaged quasars
• The resilience of the Etherington-Hubble relation
• A fake Interacting Dark Energy detection?
• QUIJOTE scientific results -- IV. A northern sky survey in intensity and polarization at 10-20GHz with the Multi-Frequency Instrument
• A new way to test the Cosmological Principle: measuring our peculiar velocity and the large scale anisotropy independently
• Sterile neutrino self-interactions: $H_0$ tension and short-baseline anomalies
• The large scale polarization explorer (LSPE) for CMB measurements: performance forecast
• Cosmological constraints from the BOSS DR12 void size function
• Improving Galaxy Clustering Measurements with Deep Learning: analysis of the DECaLS DR7 data
• Baryonic effects on the matter bispectrum
• Large scale anomalies in the CMB and non-Gaussianity in bouncing cosmologies
• Probing Cosmic Reionization and Molecular Gas Growth with TIME
• HETDEX Public Source Catalog 1: 220K Sources Including Over 50K Lyman Alpha Emitters from an Untargeted Wide-area Spectroscopic Survey
• Synergy between CSST galaxy survey and gravitational-wave observation: Inferring the Hubble constant from dark standard sirens
• Inhomogeneous Reionization Models in Cosmological Hydrodynamical Simulations
• Breakdown of chiral perturbation theory for the axion hot dark matter bound
• Full-sky Cosmic Microwave Background Foreground Cleaning Using Machine Learning
• Constrained realizations of 2MRS density and peculiar velocity fields: growth rate and local flow
• Revealing the late-time transition of $H_0$: relieve the Hubble crisis
• Data reconstruction of the dynamical connection function in $f(Q)$ cosmology
• ADM formulation and Hamiltonian analysis of $f(Q)$ gravity
• Is the Harrison-Zel'dovich spectrum coming back? ACT preference for $n_s\sim 1$ and its discordance with Planck
• A Bayesian direct method implementation to fit emission line spectra: Application to the primordial He abundance determination
• Inference of the cosmic rest-frame from supernovae Ia
• Search for new phenomena in final states with $b$-jets and missing transverse momentum in $\sqrt{s}=13$ TeV $pp$ collisions with the ATLAS detector
• Constraints on modified gravity from the BOSS galaxy survey
• Primordial lepton asymmetries in the precision cosmology era: Current status and future sensitivities from BBN and the CMB
• Bayesian inflationary reconstructions from Planck 2018 data
• The full Boltzmann hierarchy for dark matter-massive neutrino interactions
• Spectroscopically Confirmed Lyman-Alpha Emitters from Redshift 5 to 7 Behind Ten Galaxy Cluster Lenses
• Tightening the reins on non-minimal dark sector physics: Interacting Dark Energy with dynamical and non-dynamical equation of state
• Pressure Parametrization of Dark Energy: First and Second-Order Constraints with Latest Cosmological Data
• Hints of dark energy anisotropic stress using Machine Learning
• Evolutionary behaviour of cosmological parameters with dynamical system analysis in f (Q, T) gravity
• Quijote-PNG: Simulations of primordial non-Gaussianity and the information content of the matter field power spectrum and bispectrum
• Exploring the evidence for a large local void with supernovae Ia data
• The primordial matter power spectrum on sub-galactic scales
• Inflation, the Hubble Tension and Early Dark Energy: an alternative overview
• SIBELIUS-DARK: a galaxy catalogue of the Local Volume from a constrained realisation simulation
• Implications of the NANOGrav result on primordial gravitational waves in nonstandard cosmologies
• Optimal 1D Ly$\alpha$ Forest Power Spectrum Estimation -- II. KODIAQ, SQUAD & XQ-100
• Swampland conjecture in $f(R)$ gravity by the Noether Symmetry Approach
• Impact of polarised extragalactic sources on the measurement of CMB B-mode anisotropies
• TDCOSMO III: Dark matter substructure meets dark energy -- the effects of (sub)halos on strong-lensing measurements of $H_0$
• Reheating ACTs on Starobinsky and Higgs inflation
• Calibrating Gamma-Ray Bursts by Using a Gaussian Process with Type Ia Supernovae
• Fast computation of non-linear power spectrum in cosmologies with massive neutrinos
• Unveiling the Intrinsic Alignment of Galaxies with Self-Calibration and DECaLS DR3 data
• Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions
• General framework for cosmological dark matter bounds using $N$-body simulations
• Gravelamps: Gravitational Wave Lensing Mass Profile Model Selection
• The cosmic radio dipole: Bayesian estimators on new and old radio surveys
• From Dark Matter to Galaxies with Convolutional Networks
• Leptogenesis and fermion mass fit in a renormalizable $SO(10)$ model
• Gamma ray burst constraints on cosmological models from the improved Amati correlation
• Testing Dark Energy Models with Gamma-Ray Bursts Calibrated from the Observational $H(z)$ Data through a Gaussian Process
• Quantifying the global "CMB tension" between the Atacama Cosmology Telescope and the Planck satellite in extended models of cosmology
• Electroweak Phase Transition with an SU(2) Dark Sector
• Clustering in Massive Neutrino Cosmologies via Eulerian Perturbation Theory
• Transfer learning for radio galaxy classification
• Positivity Bounds without Boosts
• Observational Constraints on Warm Natural Inflation
• Cosmology with fast radio bursts in the era of SKA
• Cross-Correlation of Planck CMB Lensing with DESI-Like LRGs
• What can CMB observations tell us about the neutrino distribution function?
• The future search for low-frequency axions and new physics with the FLASH resonant cavity experiment at Frascati National Laboratories
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Bumblebee field as a source of cosmological anisotropies
• Evidence for a high-z ISW signal from supervoids in the distribution of eBOSS quasars
• Small-scale clumping at recombination and the Hubble tension
• Varying fundamental constants principal component analysis: additional hints about the Hubble tension
• Revisiting the distance to radio Loops I and IV using Gaia and radio/optical polarization data
• Performance forecasts for the primordial gravitational wave detection pipelines for AliCPT-1
• Real-space entanglement in the Cosmic Microwave Background
• Uses of Complex Metrics in Cosmology
• Probing dark matter particles at CEPC
• Extracting the cold neutral medium from HI emission with deep learning: Implications for Galactic foregrounds at high latitude
• String Cosmology backgrounds from Classical String Geometry
• Distances to the Supernova Remnants in the Inner Disk
• PACT I: Combining ACT and Planck data for optimal detection of tSZ signal
• Perturbative description of bias tracers using consistency relations of LSS
• Testing the standard model of cosmology with the SKA: the cosmic radio dipole
• BeyondPlanck III. Commander3
• Constraining the spatial curvature with cosmic expansion history in a cosmological model with a non-standard sound horizon
• Transit cosmological models with observational constraints in f(Q, T) gravity
• HOLISMOKES -- III. Achromatic Phase of Strongly Lensed Type Ia Supernovae
• N-body simulations of dark matter with frequent self-interactions
• An X-ray selected catalog of extended galaxy clusters from the ROSAT All-Sky Survey (RXGCC)
• Constraining primordial non-Gaussianity from DESI quasar targets and Planck CMB lensing
• Cosmological Constraints on sub-horizon scales modified gravity theories with MGCLASS II
• On higher derivative corrections to the $R+R^2$ inflationary model
• A void in the Hubble tension? The end of the line for the Hubble bubble
• WarmSPy: a numerical study of cosmological perturbations in warm inflation
• Primordial Standard Clock Models and CMB Residual Anomalies
• Baryonic feedback biases on fundamental physics from lensed CMB power spectra
• Observational constraints and predictions of the interacting dark sector with field-fluid mapping
• The Atacama Cosmology Telescope: Probing the Baryon Content of SDSS DR15 Galaxies with the Thermal and Kinematic Sunyaev-Zel'dovich Effects
• Constraining cosmology with a new all-sky Compton parameter map from the Planck PR4 data
• Measuring the reionization optical depth without large-scale CMB polarization
• Dark sector searches with the CMS experiment
• Proca in the sky
• On the origin of matter in the Universe
• Precise Calibration of the One-Loop Bispectrum in the Effective Field Theory of Large Scale Structure
• Exotic Compact Objects: The Dark White Dwarf
• New Limit on Axion-Like Dark Matter using Cold Neutrons
• First Constraints on Small-Scale Non-Gaussianity from UV Galaxy Luminosity Functions
• Inflationary Potential as seen from Different Angles: Model Compatibility from Multiple CMB Missions
• SICRET: Supernova Ia Cosmology with truncated marginal neural Ratio EsTimation
• Observational Constraints on $f(T)$ Gravity from Model-Independent Data
• Projected-Field Kinetic Sunyaev-Zel'dovich Cross-Correlations: Halo Model and Forecasts
• Planck intermediate results. LVI. Detection of the CMB dipole through modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove II
• Theoretical systematics in testing the Cosmological Principle with the kinematic quasar dipole
• Planck constraints on cross-correlations between anisotropic cosmic birefringence and CMB polarization
• Exploration at the high-energy frontier: ATLAS Run~2 searches investigating the exotic jungle beyond the Standard Model
• [CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST
• Tomographic Alcock-Paczynski Test with Redshift-Space Correlation Function: Evidence for the Dark Energy Equation of State Parameter w>-1
• Curvature of magnetic field lines in compressible magnetized turbulence: Statistics, magnetization predictions, gradient curvature, modes and self-gravitating media
• The improved Amati correlations from Gaussian copula
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• The Second Radio Synchrotron Background Workshop: Conference Summary and Report
• Phenomenological implications of modified loop cosmologies: an overview
• A high space density of L* Active Galactic Nuclei at z~4 in the COSMOS field
• The Simons Observatory: Galactic Science Goals and Forecasts
• Stacked CMB lensing and ISW signals around superstructures in the DESI Legacy Survey
• Using the cosmological recombination radiation to probe early dark energy and fundamental constant variations
• The multipole expansion of the local expansion rate
• Precise and Accurate Cosmology with CMBxLSS Power Spectra and Bispectra
• No rungs attached: A distance-ladder free determination of the Hubble constant through type II supernova spectral modelling
• Modelling the Accelerating Universe with $f(Q)$ Gravity: Observational Consistency
• A comparison of template vs. direct model fitting for redshift-space distortions in BOSS
• Holographic dark energy through Kaniadakis entropy in non flat universe
• The Atacama Cosmology Telescope: Summary of DR4 and DR5 Data Products and Data Access
• The perspective of voids on rising cosmology tensions
• Bayesian estimation of our local motion from the Planck-2018 CMB temperature map
• Effect of evolutionary physical constants on type-1a supernova luminosity
• Why Cosmic Voids Matter: Nonlinear Structure & Linear Dynamics
• Cosmic Purity Lost: Perturbative and Resummed Late-Time Inflationary Decoherence
• $B$-mode forecast of CMB-Bh$\overline{a}$rat
• Slow-Roll Inflation at N3LO
• Forecast of Neutrino Cosmology from the CSST Photometric Galaxy Clustering and Cosmic Shear Surveys
• Systematic-free inference of the cosmic matter density field from SDSS3-BOSS data
• Search for dark matter particles produced in association with a Higgs boson in proton-proton collisions at $\sqrt{s}=$ 13 TeV
• One- and Two-point Source Statistics from the LOFAR Two-metre Sky Survey First Data Release
• ForSE: a GAN based algorithm for extending CMB foreground models to sub-degree angular scales
• Stellar Accelerations and the Galactic Gravitational Field
• A forecast of using fast radio burst observations to constrain holographic dark energy
• Tests of Gravity with Galaxy Clusters
• Phantom scalar-tensor models and cosmological tensions
• Cosmology inference at the field level from biased tracers in redshift-space
• Massive neutrino self-interactions with a light mediator in cosmology
• Euclid: The search for primordial features
• Probing Lorentz-violating electrodynamics with CMB polarization
• Learning how to surf: Reconstructing the propagation and origin of gravitational waves with Gaussian Processes
• Search for dark matter produced in association with a single top quark in $\sqrt{s}=13$ TeV $pp$ collisions with the ATLAS detector
• Peculiar motion of Solar system from the Hubble diagram of supernovae Ia and its implications for cosmology
• Rapid build-up of the stellar content in the protocluster core SPT2349$-$56 at $z=4.3$
• Measuring the evolution of intergalactic gas from z=0 to 5 using the kinematic Sunyaev-Zel'dovich effect
• Comparing sharp and smooth transitions of the second slow-roll parameter in single-field inflation
• BeyondPlanck I. Global Bayesian analysis of the Planck Low Frequency Instrument data
• Modeling features in the redshift-space halo power spectrum with perturbation theory
• Dark energy in multi-fractional spacetimes
• The effect of inhomogeneous reionisation on the Lyman-$\alpha$ forest power spectrum at redshift $z>4$: implications for thermal parameter recovery
• Testing $\Lambda$CDM cosmology in a binned universe: anomalies in the deceleration parameter
• Constraints on Primordial Magnetic Fields from their impact on the ionization history with Planck 2018
• Testing General Relativity on cosmological scales at redshift z ~ 1.5 with quasar and CMB lensing
• Cosmological constraints on nonphantom dynamical dark energy with DESI Data Release 2 Baryon Acoustic Oscillations: A 3$\sigma$+ lensing anomaly
• Detection of Spectral Variations of Anomalous Microwave Emission with QUIJOTE and C-BASS
• Retrieving cosmological information from small-scale CMB foregrounds II. The kinetic Sunyaev Zel'dovich effect
• Gravitational lensing $H_0$ tension from ultralight axion galactic cores
• Uphill inflation
• Cosmological constraints on non-adiabatic dark energy perturbations
• The HETDEX Survey: Emission Line Exploration and Source Classification
• Stringy Running Vacuum Model and current Tensions in Cosmology
• Probability distribution function of the aperture mass field with large deviation theory
• Improved Mixed Dark Matter Halo Model for Ultralight Axions
• Enhanced power on small scales and evolution of quantum state of perturbations in single and two field inflationary models
• Dispu$\tau$able: the high cost of a low optical depth
• The Resolved Sunyaev--Zel'dovich Profiles of Nearby Galaxy Groups
• Clusters of galaxies up to z=1.5 identified from photometric data of the Dark Energy Survey and unWISE
• The Cosmic Dipole in the Quaia Sample of Quasars: A Bayesian Analysis
• Empirical constraints on the turbulence in QSO host nebulae from velocity structure function measurements
• BeyondPlanck XIII. Intensity foreground sampling, degeneracies, and priors
• Precise Calibration of the One-Loop Trispectrum in the Effective Field Theory of Large Scale Structure
• Investigating the XENON1T Low-Energy Electronic Recoil Excess Using NEST
• A first estimate of the Milky Way dark matter halo spin
• J0107a: A Barred Spiral Dusty Star-forming Galaxy at $z=2.467$
• The quadrupole in the local Hubble parameter: first constraints using Type Ia supernova data and forecasts for future surveys
• HOLISMOKES -- VII. Time-delay measurement of strongly lensed Type Ia supernovae using machine learning
• Extracting cosmological parameters from N-body simulations using machine learning techniques
• Tensor-to-scalar ratio forecasts for extended LiteBIRD frequency configurations
• Dynamical stability in models where dark matter and dark energy are non-minimally coupled to curvature
• Detailed study of the ELAIS N1 field with the uGMRT - I. Characterizing the 325 MHz foreground for redshifted 21 cm observations
• A study of collider signatures for two Higgs doublet models with a Pseudoscalar mediator to Dark Matter
• Gravitational waves from the remnants of the first stars in nuclear star clusters
• z-GAL -- A NOEMA spectroscopic redshift survey of bright Herschel galaxies: [II] Dust properties
• Probing primordial non-Gaussianity with the power spectrum and bispectrum of future 21cm intensity maps
• Molecular Chemistry for Dark Matter II: Recombination, Molecule Formation, and Halo Mass Function in Atomic Dark Matter
• A note on interacting holographic dark energy with a Hubble-scale cutoff
• In-flight polarization angle calibration for LiteBIRD: blind challenge and cosmological implications
• Why Must Primordial Non-Gaussianity Be Very Small?
• Constraints on the spectral index of polarized synchrotron emission from WMAP and Faraday-corrected S-PASS data
• The Cosmic Evolution of Magnesium Isotopes
• Dark Matter Candidates and Searches
• Testing CCC+TL Cosmology with Observed BAO Features
• Sensitivity forecasts for the cosmological recombination radiation in the presence of foregrounds
• Clarifying transfer function approximations for the large-scale gravitational wave background in $\Lambda$CDM
• Characterization of the polarized synchrotron emission from Planck and WMAP data
• Strong electroweak phase transition in $t$-channel simplified dark matter models
• Back to the features: assessing the discriminating power of future CMB missions on inflationary models
• The deceleration parameter in `tilted' universes: generalising the Friedmann background
• Two sides of the same coin: sterile neutrinos and dark radiation. Status and perspectives
• One-Electron Quantum Cyclotron as a Milli-eV Dark-Photon Detector
• The Atacama Cosmology Telescope: Map-Based Noise Simulations for DR6
• A general study of chameleon fifth force in gravity space experiments
• HAWC+/SOFIA Polarimetry in L1688: Relative Orientation of Magnetic Field and Elongated Cloud Structure
• Optimal constraints on primordial gravitational waves from the lensed CMB
• Gravitational waves from neutrino mass and dark matter genesis
• Most of the cool CGM of star-forming galaxies is not produced by supernova feedback
• Constraints on galileons from the positions of supermassive black holes
• Extracting HI Astrophysics from Interferometric Intensity Mapping
• Two Year Cosmology Large Angular Scale Surveyor (CLASS) Observations: Long Timescale Stability Achieved with a Front-End Variable-delay Polarization Modulator at 40 GHz
• Improved constraints on reionisation from CMB observations: A parameterisation of the kSZ effect
• First Results from a Broadband Search for Dark Photon Dark Matter in the $44$ to $52\mu$eV range with a coaxial dish antenna
• Axion-pion thermalization rate in unitarized NLO chiral perturbation theory
• Role of Extended Gravity Theory in Matter Bounce Dynamics
• Cosmology of Supercooled Universe
• Cosmological foundations revisited with Pantheon+
• Source anisotropies and pulsar timing arrays
• The de Broglie-Bohm Quantum Theory and its Application to Quantum Cosmology
• Enhanced curvature perturbations from spherical domain walls nucleated during inflation
• Post-inflationary axion isocurvature perturbations facing CMB and large-scale structure
• Cosmology in the presence of multiple light moduli
• Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
• Non-minimally coupled curvaton
• The cosmic shallows I: interaction of CMB photons in extended galaxy halos
• Nonlinear Redshift-Space Distortions in the Harmonic-space Galaxy Power Spectrum
• Ultra-light axions and the kinetic Sunyaev-Zel'dovich Effect
• Raychaudhuri equation in $k$-essence geometry: conditional singular and non-singular cosmological models
• BeyondPlanck VII. Bayesian estimation of gain and absolute calibration for CMB experiments
• Thermal axions with multi-eV masses are possible in low-reheating scenarios
• Ultra-large-scale approximations and galaxy clustering: debiasing constraints on cosmological parameters
• Dark Matter Direct Detection of Classical WIMPs
• COMAP Early Science: VI. A First Look at the COMAP Galactic Plane Survey
• The Extinction and Distance of the MBM Molecular Clouds at High Galactic Latitude
• Primordial Black Hole Dark Matter in the Context of Extra Dimensions
• Inferring the Intermediate Mass Black Hole Number Density from Gravitational Wave Lensing Statistics
• Testing cosmic anisotropy with Pade approximation and Pantheon+ sample
• MADYS: the Manifold Age Determination for Young Stars
• Primordial power spectrum and cosmology from black-box galaxy surveys
• Measuring ${\sigma }_8$ using DESI Legacy Imaging Surveys Emission-Line Galaxies and Planck CMB Lensing and the Impact of Dust on Parameter Inference
• Large-scale cosmic ray anisotropies with 19 years of data from the Pierre Auger Observatory
• QUIJOTE scientific results -- VIII. Diffuse polarized foregrounds from component separation with QUIJOTE-MFI
• Oscillating dark energy in light of the latest observations and its impact on the Hubble tension
• Growth-rate measurement with type-Ia supernovae using ZTF survey simulations
• Discordance of dipole asymmetries seen in recent large radio surveys with the Cosmological Principle
• Resonant neutrino self-interactions and the $H_0$ tension
• Sweeping Horndeski Canvas: New Growth-Rate Parameterization for Modified-Gravity Theories
• Constraining dark matter decays with cosmic microwave background and weak lensing shear observations
• The 7% Rule: A Maximum Entropy Prediction on New Decays of the Higgs Boson
• A novel CMB polarization likelihood package for large angular scales built from combined WMAP and Planck LFI legacy maps
• The impact of extragalactic foregrounds on internal delensing of CMB B-mode polarization
• CENN: A fully convolutional neural network for CMB recovery in realistic microwave sky simulations
• The unified history of the viscous accelerating universe and phase transitions
• Statistics of biased tracers in variance-suppressed simulations
• The C-Band All-Sky Survey (C-BASS): Template Fitting of Diffuse Galactic Microwave Emission in the Northern Sky
• BeyondPlanck X. Bandpass and beam leakage corrections
• Constraining the anisotropy of the Universe with the X-ray and UV fluxes of quasars
• Scalar-Tensor Gravity and DESI 2024 BAO data
• Delensing the CMB with the cosmic infrared background: the impact of foregrounds
• Dust polarization modeling at large-scale over the Northern Galactic cap using EBHIS and Planck data
• Instrumental systematics biases in CMB lensing reconstruction: a simulation-based assessment
• COMAP Early Science: III. CO Data Processing
• $f\left(R,{\nabla }_{{\mu }_1}R,\dots ,{\nabla }_{{\mu }_1}\dots {\nabla }_{{\mu }_n}R\right)$ theories of gravity in Einstein frame: A higher order modified Starobinsky inflation model in the Palatini approach
• Tracking the Multifield Dynamics with Cosmological Data: A Monte Carlo approach
• Discovery of a coherent, wave-like velocity pattern for the Radcliffe Wave
• Targeted search for the kinematic dipole of the gravitational-wave background
• 21cmFirstCLASS I. Cosmological tool for $\Lambda$CDM and beyond
• Observing the Reionization : Effect of Calibration and Position Errors on Realistic Observation Conditions
• Constraints from Fermi observations of Long Gamma-Ray Bursts on cosmological parameters
• The C-Band All-Sky Survey (C-BASS): Constraining diffuse Galactic radio emission in the North Celestial Pole region
• BeyondPlanck XI. Bayesian CMB analysis with sample-based end-to-end error propagation
• Cosmography of the Local Universe by Multipole Analysis of the Expansion Rate Fluctuation Field
• Wake forces in a background of quadratically coupled mediators
• BeyondPlanck XII. Cosmological parameter constraints with end-to-end error propagation
• KiDS-1000: cross-correlation with Planck cosmic microwave background lensing and intrinsic alignment removal with self-calibration
• Magnification Bias Estimators for Realistic Surveys: an Application to the BOSS Survey
• Impact of Population III homogeneous stellar evolution on early cosmic reionisation
• A novel model-marginalized cosmological bound on the QCD axion mass
• Extended Analysis of Neutrino-Dark Matter Interactions with Small-Scale CMB Experiments
• Cosmoglobe DR1 results. I. Improved Wilkinson Microwave Anisotropy Probe maps through Bayesian end-to-end analysis
• Anisotropy in Pantheon+ supernovae
• On the relationship between mean observations, spatial averages and the Dyer-Roeder approximation in Einstein-Straus models
• From BeyondPlanck to Cosmoglobe: Preliminary $WMAP$ $Q$-band analysis
• Determination of Polarization Angles in CMB Experiments and Application to CMB Component Separation Analyses
• Interacting dark energy after DESI DR2: a challenge for $\Lambda$CDM paradigm?
• WALLABY Pre-Pilot and Pilot Survey: the Tully Fisher Relation in Eridanus, Hydra, Norma and NGC4636 fields
• A viable varying speed of light model in the RW metric
• Cosmological forecasts on thermal axions, relic neutrinos and light elements
• Dark Matter and $(g-2{)}_{\mu ,e}$ in radiative Dirac neutrino mass models
• Sterile Neutrino. A short introduction
• Understanding matched filters for precision cosmology
• The Milky Way, Coming into Focus: Precision Astrometry Probes its Evolution, and its Dark Matter
• Testing Quintessence Axion Dark Energy with Recent Cosmological Results
• The physical properties of Cluster Chains
• Experimental targets for dark photon dark matter
• Phase-space analysis of dark energy models in non-minimally coupled theories of gravity
• Constraining gravity with a new precision $E_G$ estimator using Planck + SDSS BOSS
• Gravito-electromagnetic perturbations of MOG black holes with a cosmological constant: Quasinormal modes and Ringdown waveforms
• Exploring the Growth Index ${\gamma }_L$: Insights from Different CMB Dataset Combinations and Approaches
• The Kinematic Sunyaev-Zel'dovich Effect with ACT, DES, and BOSS: a Novel Hybrid Estimator
• The Atacama Cosmology Telescope: Systematic Transient Search of 3-Day Maps
• Machine learning cosmic inflation
• Impact of half-wave plate systematics on the measurement of cosmic birefringence from CMB polarization
• Probing dark matter interactions with 21cm observations
• Polarized Synchrotron Foreground Assessment for CMB Experiments
• On estimating the cosmic molecular gas density from CO Line Intensity Mapping observations
• BeyondPlanck VI. Noise characterization and modelling
• Evaporation of dynamical horizon with the Hawking temparature in the {\bf K-}essence emergent Vaidya spacetime
• Hybrid-basis inference for large-scale galaxy clustering: combining spherical and Cartesian Fourier analyses
• Revised estimates of CMB $B$-mode polarization induced by patchy reionization
• The interacting multiverse and its effect on the cosmic microwave background
• Explaining Excess Dipole in NVSS Data Using Superhorizon Perturbation
• Challenging the Stability of Light Millicharged Dark Matter
• Multi-messenger Gravitational Lensing
• Dynamical modelling and origin of gas turbulence in z $\sim$ 4.5 galaxies
• Not All Subhaloes Are Created Equal: Modelling the Diversity of Subhalo Density Profiles in TNG50
• Optical depth to reionization from perturbative 21cm clustering
• Leptogenesis from the Asymmetric Texture
• Density matrix calculation of the dark matter abundance in the Higgs induced right-handed neutrino mixing model
• Constraints from High-Precision Measurements of the Cosmic Microwave Background: The Case of Disintegrating Dark Matter with $\Lambda$ or Dynamical Dark Energy
• Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions
• Detecting the HI Power Spectrum in the Post-Reionization Universe with SKA-Low
• Loop quantum cosmology: relation between theory and observations
• Inflation and the cosmological (not-so) constant in unimodular gravity
• Fraudulent White Noise: Flat power spectra belie arbitrarily complex processes
• Two 100 TeV neutrinos coincident with the Seyfert galaxy NGC 7469
• Varying physical constants and the lithium problem
• Cosmology before noon with multiple galaxy populations
• Probing the cold neutral medium through HI emission morphology with the scattering transform
• Milky Way and M31 rotation curves: $\Lambda$CDM vs. MOND
• Disentangling Doppler modulation, aberration and the temperature dipole in the CMB
• Mean Estimate Distances for Galaxies with Multiple Estimates in NED-D
• Multi-component DHOST analysis in galaxy clusters
• UNCOVERing the High-redshift AGN Population among Extreme UV Line Emitters
• Neutron-Mirror-Neutron Oscillation and Neutron Star Cooling
• Primordial perturbations in the Dapor-Liegener model of hybrid loop quantum cosmology
• The Sejong Suite: Cosmological Hydrodynamical Simulations with Massive Neutrinos, Dark Radiation, and Warm Dark Matter
• Cosmology of an Axion-Like Majoron
• Interacting tachyonic scalar field
• An X-ray and SZ bright diffuse source toward M31: a Local Hot Bridge
• Constraints on Dark Energy Models Using Late Universe Probes
• Super-sample covariance of the thermal Sunyaev-Zel'dovich effect
• Observable Primordial Gravitational Waves from Non-minimally Coupled $R^2$ Palatini Modified Gravity
• The CMB Cold Spot as predicted by foregrounds around nearby galaxies
• Lattice simulations of axion-U(1) inflation: gravitational waves, magnetic fields, and scalar statistics
• Constraints on interacting dark energy revisited: implications for the Hubble tension
• Large gas inflow driven by a matured galactic bar in the early Universe
• A new probe of the high-redshift Universe: nulling CMB lensing with interloper-free "LIM-pair" lensing
• The Impact of Anisotropic Redshift Distributions on Angular Clustering
• Asymmetric Self-interacting Dark Matter via Dirac Leptogenesis
• Cosmological consequences of first-order general-relativistic viscous fluid dynamics
• Anisotropic universe with anisotropic dark energy
• The Integrated Sachs-Wolfe Effect in 4D Einstein-Gauss-Bonnet Gravity
• ECLIPSE: a fast Quadratic Maximum Likelihood estimator for CMB intensity and polarization power spectra
• Leptophilic Composite Asymmetric Dark Matter and its Detection
• On the asymptotic connection between full- and flat-sky angular correlators
• Requirements for future CMB satellite missions: photometric and band-pass response calibration
• Analysis of NILC performance on B-modes data of sub-orbital experiments
• $H_0$ Tension on the Light of Supermassive Black Hole Shadows Data
• How much primordial tensor mode is allowed?
• Hemispherical Power Asymmetry in intensity and polarization for Planck PR4 data
• The galaxy power spectrum from TGSS ADR1 and the effect of flux calibration systematics
• Mapping the inhomogeneous Universe with Standard Sirens: Degeneracy between inhomogeneity and modified gravity theories
• The ACCEL2 Project: Precision Measurements of EFT Parameters and BAO Peak Shifts for the Lyman-$\alpha$ Forest
• Optical polarization and spectral properties of the H-poor superluminous supernovae SN 2021bnw and SN 2021fpl
• Third-order corrections to the slow-roll expansion: calculation and constraints with Planck, ACT, SPT, and BICEP/Keck
• Irregular universe in the Nieh-Yan modified teleparallel gravity
• Detection of WHIM in the Planck data using Stack First approach
• Evolution of Primordial Neutrino Helicities in Cosmic Gravitational Inhomogeneities
• New Physics Search at the CEPC: a General Perspective
• Separating the Intrinsic Alignment Signal and the Lensing Signal using Self-Calibration in Photo-z Surveys with KiDS450 and KV450 Data
• Inflow of low-metallicity cool gas in the halo of the Andromeda galaxy
• Non-thermal neutrino-like hot dark matter in light of the $S_8$ tension
• Clouds accreting from the IGM are not able to feed the star formation of low-redshift disc galaxies
• Probing gravity with redshift-space distortions: effects of tracer bias and sample selection
• Retrieving cosmological information from small-scale CMB foregrounds I. The thermal Sunyaev Zel'dovich effect
• The Anisotropic Circumgalactic Medium of Massive Early-Type Galaxies
• The PSZ-MCMF catalogue of Planck clusters over the DES region
• Reassessment of the dipole in the distribution of quasars on the sky
• Constraints on the scalar-field potential in warm inflation
• The ACT-DR5 MCMF Galaxy Cluster Catalog
• Approximate Bayesian Neural Doppler Imaging
• Filamentary Dust Polarization and the Morphology of Neutral Hydrogen Structures
• Bounds from ISW-galaxy cross-correlations on generalized covariant Galileon models
• Muon g-2, Neutralino Dark Matter and Stau NLSP
• Monopole Fluctuation of the CMB and its Gauge Invariance
• Fast computation of angular power spectra and covariances of high-resolution cosmic microwave background maps using the Toeplitz approximation
• Constraints on Neutron-Mirror-Neutron Oscillation from Neutron Star Cooling
• Pursuit of paired dijet resonances in the Run 2 dataset with ATLAS
• A search for candidate strongly-lensed dusty galaxies in the Planck satellite catalogues
• Application of Contour Minkowski Tensor and $\mathcal{D}$ Statistic to the Planck $E$-mode data
• Perturbative region on non-Gaussian parameter space in single-field inflation
• KiDS+VIKING+GAMA: Halo occupation distributions and correlations of satellite numbers with a new halo model of the galaxy-matter bispectrum for galaxy-galaxy-galaxy lensing
• Post maximum light and late time optical imaging polarimetry of type I superluminous supernova 2020znr
• The spectral index of polarized diffuse Galactic emission between 30 and 44 GHz
• Constraining Chameleon screening using galaxy cluster dynamics
• Joint constraints on reionization: a framework for combining the global 21cm signal and the kinetic Sunyaev-Zel'dovich effect
• Schrödinger Connections: From Mathematical Foundations Towards Yano-Schrödinger Cosmology
• Quantifying effects of inhomogeneities and curvature on gravitational wave standard siren measurements of $H(z)$
• Galactic satellite systems in CDM, WDM and SIDM
• Constraining the neutrino mass using a multi-tracer combination of two galaxy surveys and CMB lensing
• Mixed Warm Dark Matter Constraints using Milky Way Satellite Galaxy Counts
• Unveiling cosmological information on small scales with line intensity mapping
• How robust are the parameter constraints extending the $\Lambda$CDM model?
• Quantum gravitational signatures in next-generation gravitational wave detectors
• Sommerfeld-enhanced dark matter searches with dwarf spheroidal galaxies
• Cosmological Tests of Gravity: A Future Perspective
• Testing $\alpha$-attractor quintessential inflation against CMB and low-redshift data
• Cosmological effects of the Galileon term in Scalar-Tensor Theories
• Learning neutrino effects in Cosmology with Convolutional Neural Networks
• A Novel CMB Component Separation Method: Hierarchical Generalized Morphological Component Analysis
• New insights on $\nu$-DM Interactions
• When Leaving the Solar System: Dark Matter Makes a Difference
• Highly Excited Electron Cyclotron for QCD Axion and Dark-Photon Detection
• Modeling parity-violating spectra in Galactic dust polarization with filaments and its applications to cosmic birefringence searches
• If dark matter is fuzzy, the first stars form in massive pancakes
• Right-Handed Neutrino Dark Matter with Forbidden Annihilation
• Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Cross-correlation with the cosmic microwave background
• Bouncing cosmology from nonlinear dark energy with two cosmological constants
• Study of the thermal and nonthermal emission components in M31: the Sardinia Radio Telescope view at 6.6 GHz
• Neural network reconstruction of density and velocity fields from the 2MASS Redshift Survey
• Squeezing the Axion
• Baryogenesis through Asymmetric Hawking Radiation from Primordial Black Holes as Dark Matter
• QUIJOTE Scientific Results -- VII. Galactic AME sources in the QUIJOTE-MFI Northern Hemisphere Wide-Survey
• Signatures of Light Massive Relics on nonlinear structure formation
• Length-preserving biconnection gravity and its cosmological implications
• Tomographic redshift dipole: Testing the cosmological principle
• Constraints on power law cosmology from cosmic chronometer, standard ruler, and standard candle data
• First Axion-Like Particle Results from a Broadband Search for Wave-Like Dark Matter in the 44 to 52 $\mu$eV Range with a Coaxial Dish Antenna
• Dynamical features of $f(T,B)$ cosmology
• Constraints on ${\tau }_{\mathrm{NL}}$ from Planck temperature and polarization
• Cross-correlation between $Planck$ CMB lensing potential and galaxy catalogues from HELP
• Angular correlations of causally-coherent primordial quantum perturbations
• The kinematic contribution to the cosmic number count dipole
• Dissipative quintessence, and its cosmological implications
• Data-driven and Almost Model-independent Reconstruction of Modified Gravity
• Runaway dilaton models: improved constraints from the full cosmological evolution
• The low multipoles in the Pantheon+SH0ES data
• A multishock scenario for the formation of radio relics
• Faraday tomography of LoTSS-DR2 data: II. Multi-tracer analysis in the high-latitude outer Galaxy
• BBN constraints on dark radiation isocurvature
• Alternative approach to the Starobinsky model for inflation scenarios
• HETDEX Public Source Catalog 1 -- Stacking 50K Lyman Alpha Emitters
• Biases to primordial non-Gaussianity measurements from CMB secondary anisotropies
• Decay of $f(R)$ quintessence into dark matter: mitigating the Hubble tension?
• Gravitational-wave event rates as a new probe for dark matter microphysics
• Constraints on extended Bekenstein models from cosmological, astrophysical, and local data
• Magnetic Field of Molecular Gas Measured with the Velocity Gradient Technique I. Orion A
• Cosmological Boundary Flux Parameter
• How new physics affects primordial neutrinos decoupling: Direct Simulation Monte Carlo approach
• The role of $T_0$ in CMB anisotropy measurements
• The first molecules in the intergalactic medium and halos of the Dark Ages and Cosmic Dawn
• Systematic effects induced by Half Wave Plate precession into Cosmic Microwave Background polarization measurements
• Direct Optimal Mapping for 21cm Cosmology: A Demonstration with the Hydrogen Epoch of Reionization Array
• New physics decaying into metastable particles: impact on cosmic neutrinos
• Dark Radiation and the Hagedorn Phase
• Collapsing scenarios of K-essence generalized Vaidya spacetime under $f(\bar{R},\bar{T})$ gravity
• Inferring subhalo effective density slopes from strong lensing observations with neural likelihood-ratio estimation
• Interpreting Internal Consistency of DES Measurements
• Generative Models of Multi-channel Data from a Single Example -- Application to Dust Emission
• Rejuvenating the hope of a swampland consistent inflated multiverse with tachyonic inflation in the high energy RS-II Braneworld
• A measurement of the Integrated Sachs-Wolfe Effect with the Rapid ASKAP Continuum Survey
• Beyond Two Parameters: Revisiting Dark Energy with the Latest Cosmic Probes
• A study of Dipolar Signal in distant Quasars with various observables
• Covariant formulation of refracted gravity
• Deviation from Tribimaximal mixing using $A_4$ flavour model with five extra scalars
• An Empirical Determination of the Dependence of the Circumgalactic Mass Cooling Rate and Feedback Mass Loading Factor on Galactic Stellar Mass
• Optimising Inflationary Features the Bayesian Way
• Search for dark matter produced in association with a single top quark and an energetic $W$ boson in $\sqrt{s}=$ 13 TeV $pp$ collisions with the ATLAS detector
• Low-scale Resonant Leptogenesis in $SU(5)$ GUT with ${\mathcal{T}}_{13}$ Family Symmetry
• Effects of feedback-free starburst galaxies on the 21-cm signal and reionization history
• BeyondPlanck X. Planck LFI frequency maps with sample-based error propagation
• ALETHEIA: Hunting for Low-mass Dark Matter with Liquid Helium TPCs
• Cosmological effects on $f(\bar{R},\bar{T})$ gravity through a non-standard theory
• CMB foreground measurements through broad-band radio spectro-polarimetry: prospects of the SKA-MPG telescope
• Cosmology from Planck CMB Lensing and DESI DR1 Quasar Tomography
• A local infall from a cosmographic analysis of Pantheon+
• Constraints on the Optical Depth to Reionization from Balloon-Borne CMB Measurements
• Running effects on QCD axion phenomenology
• Absolute reference for microwave polarization experiments -- The COSMOCal project and its proof of concept
• Simultaneous Millimeter-wave, Gamma-ray, and Optical Monitoring of the Blazar PKS 2326-502 During a Flaring State
• QUIJOTE Scientific Results -- XVII. Studying the Anomalous Microwave Emission in the Andromeda Galaxy with QUIJOTE-MFI
• Spatial Curvature in Cosmology Revisited
• Constraints on Equivalence Principle Violation from Gamma Ray Bursts
• Kinetic Field Theory for Cosmic Structure Formation
• On Wigner Degeneracy in Elko theory: Hermiticity and Dark Matter
• A power spectrum approach to the search for Axion-like Particles from resolved galaxy clusters using CMB as a backlight
• Spherical Collapse Approach for Non-standard Dark Matter Models and Enhanced Early Galaxy Formation in JWST
• Planck intermediate results. LV. Reliability and thermal properties of high-frequency sources in the Second Planck Catalogue of Compact Sources
• Two-body lepton-flavour-violating decays in a 2HDM with soft family-lepton-number breaking
• QUIJOTE scientific results -- V. The microwave intensity and polarisation spectra of the Galactic regions W49, W51 and IC443
• Evidence of Extended Dust and Feedback around z$\approx$1 Quiescent Galaxies via Millimeter Observations
• Footprints of Doppler and Aberration Effects in CMB Experiments: Statistical and Cosmological Implications
• Foreground removal with ILC methods for AliCPT-1
• Constraints on Cosmological Models with Gamma-Ray Bursts in Cosmology-Independent Way
• Testing the Cosmological Principle: On the Time Dilation of Distant Sources
• Gravitational Fluctuations as an Alternative to Inflation
• Cosmic dipoles of active galactic nuclei at optical and radio wavelengths display much larger amplitudes than the cosmic microwave background dipole
• Relative alignment between gas structures and magnetic field in Orion A at different scales using different molecular gas tracers
• The proper motion of stars in dwarf galaxies: distinguishing central density cusps from cores
• A Pixel Space Method for Testing Dipole Modulation in the CMB Polarization
• Mapping the Universe in HD
• Resolution of the incongruency of dipole asymmetries within various large radio surveys -- implications for the Cosmological Principle
• Constraining the $3-3-1$ model with heavy neutral leptons using $(g-2{)}_{\mu }$ and dark matter observables
• Baryogenesis from sphaleron decoupling
• Impact of half-wave plate systematics on the measurement of CMB $B$-mode polarization
• BeyondPlanck VIII. Efficient Sidelobe Convolution and Correction through Spin Harmonics
• Dynamics of metastable Standard Model particles from long-lived particle decays in the MeV primordial plasma
• Two models unifying warm inflation with dark matter and dark energy
• Halo formation and evolution in scalar field dark matter and cold dark matter: New insights from the fluid approach
• Dependence of accessible dark matter annihilation cross-sections on the density profiles of dwarf spheroidal galaxies with the Cherenkov Telescope Array
• Enlightening the CSL model landscape in inflation
• Dark Twilight Joined with the Light of Dawn to Unveil the Reionization History
• How bad could it be? Modelling the 3D complexity of the polarised dust signal using moment expansion
• FlexKnot as a Generalised Model of the Sky-averaged 21-cm Signal at z ~ 6-30 in the Presence of Systematics
• The LSPE-Strip feed horn array
• CHEX-MATE: pressure profiles of 6 galaxy clusters as seen by SPT and Planck
• Scalar Quasi-Normal Modes of a Loop Quantum Black Hole
• Modern Cosmology, an Amuse-Gueule
• Growth and Geometry Split in Light of the DES-Y3 Survey
• The C-Band All-Sky Survey (C-BASS): New Constraints on the Integrated Radio Spectrum of M 31
• A horseshoe-shaped ring of diffuse emission detected at 1.4 GHz
• Effects of a Late Gravitational Transition on Gravitational Waves and Anticipated Constraints
• A comparative analysis of dissipation coefficients in warm inflation
• Isolating the linear signal when making redshift space distortion measurements
• Spatial Curvature from Super-Hubble Cosmological Fluctuations
• Constraints on the non-thermal desorption of methanol in the cold core LDN 429-C
• Quantum initial conditions for curved inflating universes
• Tachyonic vs Quintessence dark energy: linear perturbations and CMB data
• An Informational Approach to Cosmological Parameter Estimation
• Incompatibility of fine-structure constant variations at recombination with local observations
• What if the universe expands linearly? A local general relativity to solve the "zero active mass" problem
• Cosmic dipole tensions: confronting the cosmic microwave background with infrared and radio populations of cosmological sources
• Perturbation Theory Remixed: Improved Nonlinearity Modeling beyond Standard Perturbation Theory
• Characteristic Functions for Cosmological Cross-Correlations
• Embedded Domain Walls and Electroweak Baryogenesis
• Cosmology at high redshift -- a probe of fundamental physics
• Examining the local Universe isotropy with galaxy cluster velocity dispersion scaling relations
• BeyondPlanck IV. On end-to-end simulations in CMB analysis -- Bayesian versus frequentist statistics
• An Analytical Study of the Primordial Gravitational-Wave-Induced Contribution to the Large-Scale Structure of the Universe
• Resistive Heating Induced by Streaming Cosmic Rays Around a Galaxy in the Early Universe
• Interacting Barrow Holographic Dark Energy in Non-flat Universe
• A Novel Estimator for the Equation of State of the IGM by Ly$\alpha$ Forest Tomography
• Resilience and implications of adiabatic CMB cooling
• Probing the Anisotropy and Non-Gaussianity in the Redshift Space through the Conditional Moments of the First Derivative
• Low Fine-Tuning with Heavy Higgsinos in Yukawa Unified SUSY GUTs
• Observational Constraints on Early Coupled Quintessence
• Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory
• Search for inelastic WIMP-iodine scattering with COSINE-100
• Field-level multiprobe analysis of the CMB, integrated Sachs-Wolfe effect, and the galaxy density maps
• Forecast of CMB TB and EB correlations for AliCPT-1
• Scalar-Induced Gravitational Waves in a $\Lambda$CDM Cosmology
• Form Invariance of Raychaudhuri equation in the presence of Inflaton-type fields
• Mass Modeling and Kinematics of Galaxy Clusters in Modified Gravity
• An Independent Measure of the Kinematic Dipole from SDSS
• Euclid: Relativistic effects in the dipole of the 2-point correlation function
• Constraints on cosmic birefringence using $E$-mode polarisation
• Anomalies in the topology of the temperature fluctuations in the cosmic microwave background: An analysis of the $\text{NPIPE}$ and $\text{FFP10}$ data releases
• Cryogenic SiPMs for the Optical Readout of DarkSide-20k
• Baryon acoustic oscillations from HI intensity mapping: the importance of cross-correlations in the monopole and quadrupole
• Prospects for disentangling dark matter with weak lensing
• Expansion-contraction duality breaking in a Planck-scale sensitive cosmological quantum simulator
• Cosmological test of an extended quintessence model
• One Extension to Explain Them All, One Scale-Invariant Spectrum to Test Them All, and in One Model Bind Them
• Evaluation of the single-component thermal dust emission model in CMB experiments
• Cosmography of the minimally extended Varying Speed of Light Model
• General analysis of Noether symmetries in Horndeski gravity
• Reconstruction of inflationary scenarios in non-conservative unimodular gravity
• QUIJOTE scientific results -- VI. The Haze as seen by QUIJOTE
• Hemispherical Variance Anomaly and Reionization Optical Depth
• Probing the Cosmological Principle with the CSST Photometric Survey
• What does a cosmological experiment really measure? Covariant posterior decomposition with normalizing flows
• Comparison of hydrostatic and lensing cluster mass estimates:a pilot study in MACS J0647.7+7015
• Controlling systematics in ground-based CMB surveys with partial boresight rotation
• Predicting CMB dust foreground using galactic 21 cm data
• Revised planet brightness temperatures using the Planck/LFI 2018 data release
• Planet cartography with neural learned regularization
• Little Rip, Pseudo Rip and bounce cosmology with generalized equation of state in non-standard backgrounds
• Constraints on Bianchi-I type universe with SH0ES anchored Pantheon+ SNIa data
• Stellar tidal streams around nearby spiral galaxies with deep imaging from amateur telescopes
• A Comprehensive All-Sky Catalog of 3345 Molecular Clouds from Three-dimensional Dust Extinction
• Bayesian decomposition of the Galactic multi-frequency sky using probabilistic autoencoders
• Unveiling polarized emission from interstellar dust of the Large Magellanic Cloud with Planck
• Dark Energy: is it `just' Einstein's Cosmological Constant Lambda?
• Unexplained correlation between the Cosmic Microwave Background temperature and the local matter density distribution
• Kick-alignment: matter asymmetry sourced dark matter
• Blind Map Level Systematics Cleaning: A Quadratic Estimator Approach
• A Constrained NILC method for CMB B mode observations
• Dynamical Dark Energy and the Unresolved Hubble Tension: Multi-model Constraints from DESI 2025 and Other Probes
• Dressing rotating black holes with anisotropic matter
• Combination and summary of ATLAS dark matter searches interpreted in a 2HDM with a pseudo-scalar mediator using 139 fb${}^{-1}$ of $\sqrt{s}=13$ TeV $pp$ collision data
• Constraining cosmic reionization by combining the kinetic Sunyaev-Zel'dovich and the 21 cm power spectra
• Phenomenology of a minimal extension of the standard model with a family-dependent gauge symmetry
• KiDS+VIKING+GAMA: Testing semi-analytic models of galaxy evolution with galaxy-galaxy-galaxy lensing
• Testing the local supervoid solution to the Hubble tension with direct distance tracers
• Probing Long-Range Forces Between Neutrinos with Cosmic Structures
• Enhancing CMB map reconstruction and power spectrum estimation with convolutional neural networks
• New probe of inflationary gravitational waves: cross-correlations of lensed primary CMB B-modes with large-scale structure
• Emergent universe revisited through the CSL theory
• The anomaly of the CMB power with the latest Planck data
• Resonant neutrino self-interactions: Insights from the full shape galaxy power spectrum
• The Simons Observatory: Beam characterization for the Small Aperture Telescopes
• The effect of cosmic variance on the characteristics of dust polarization power spectra
• Cosmoglobe DR1. III. First full-sky model of polarized synchrotron emission from all WMAP and Planck LFI data
• The environmental dependence of the baryon acoustic peak in the Baryon Oscillation Spectroscopic Survey CMASS sample
• MAPPRAISER: A massively parallel map-making framework for multi-kilo pixel CMB experiments
• Improved Weak Lensing Photometric Redshift Calibration via StratLearn and Hierarchical Modeling
• Null geodesic structure for the Barriola-Vilenkin spacetime via $k$-essence
• Investigating the Origin of CMB Large-Scale Features Using LiteBIRD and CMB-S4
• A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter
• Central concentration of warm and dense molecular gas in a strongly lensed submillimeter galaxy at z=6
• NEC violation in $f(\bar{R},\bar{T})$ gravity in the context of a non-canonical theory via modified Raychaudhuri equation
• Point Source Detection with Fully-Convolutional Networks: Performance in Realistic Simulations
• Dipole Anisotropy in Gravitational Wave Source Distribution
• Neutron stars as probes of dark matter
• The Statistics of Extended Debris Disks Measured with Gaia and Planck
• A measurement of cluster masses using Planck and SPT-SZ CMB lensing
• Sparse image reconstruction on the sphere: a general approach with uncertainty quantification
• Combining chirp mass, luminosity distance and sky localisation from gravitational wave events to detect the cosmic dipole
• Statistical estimation of full-sky radio maps from 21cm array visibility data using Gaussian constrained realizations
• QCD axion dark matter and the cosmic dipole problem
• The Orion-Taurus ridge: a synchrotron radio loop at the edge of the Orion-Eridanus superbubble
• Signal in the Hyperfine Structure Line of the Ground State of Atomic Hydrogen from the Dark Ages as a Cosmological Test
• Gamma-Ray Bursts Calibrated from the Observational $H(z)$ Data in Artificial Neural Network Framework
• Clustering properties of the CatWISE2020 quasar catalogue and their impact on the cosmic dipole anomaly
• The parity-odd Intrinsic Bispectrum
• Reaching small scales with low frequency imaging: applications to the Dark Ages
• Ionospheric effect on the synthetic Epoch of Reionization observations with the SKA1-Low
• Measuring our peculiar velocity from spectroscopic redshift surveys
• Scalar Dark Matter and Electroweak Stability
• Euclid preparation. The impact of relativistic redshift-space distortions on two-point clustering statistics from the Euclid wide spectroscopic survey
• Determining our peculiar velocity from the aberration in the cosmic microwave background
• FaVeST: Fast Vector Spherical Harmonic Transforms
• Polarization and variability of compact sources measured in Planck time-ordered data
• Star-Crossed Labours: Checking Consistency Between Current Supernovae Compilations
• Breaking the degeneracy between polarization efficiency and cosmological parameters in CMB experiments
• QUIJOTE scientific results -- XVIII. New constraints on the polarization of the Anomalous Microwave Emission in bright Galactic regions: $\rho$\,Ophiuchi, Perseus and W43
• Non-Singular Bouncing cosmology from Phantom Scalar-Gauss-Bonnet Coupling: Reconstruction with Observational Insights
• Towards a theory of machine learning
• Conversations in the dark: cross-correlating birefringence and LSS to constrain axions
• Constraining the average magnetic field in galaxy clusters with current and upcoming CMB surveys
• Euclid: performance on main cosmological parameter science
• AMICO galaxy clusters in KiDS-DR3: constraints on $\Lambda$CDM from extreme value statistics
• A Bayesian Method to Mitigate the Effects of Unmodelled Time-Varying Systematics for 21-cm Cosmology Experiments
• Scale and redshift dependent limits on cosmic neutrino properties
• Primordial Power Spectrum of Five Dimensional Uniform Inflation
• Higher-Order Spectra of Weak Lensing Convergence Maps in Parameterized Theories of Modified Gravity
• The Velocity Field Olympics: Assessing velocity field reconstructions with direct distance tracers
• Global signal in the redshifted hydrogen 21-cm line from the Dark Ages and Cosmic Dawn: Dependence on the nature of dark matter and modeling of first light
• N-body simulations of dark matter-baryon interactions
• Study on the filters of atmospheric contamination in ground based CMB observation
• Updated observational constraints on $\varphi$CDM dynamical dark energy cosmological models
• Effects of observer peculiar motion on the isotropic background frequency spectrum: from monopole to higher multipoles
• Matter Dipole and Hubble Tension due to Large Wavelength Perturbations
• Euclid: Photometric redshift calibration with self-organising maps
• Host group degeneracy in gravitational lensing time delay determination of $H_0$
• Including topology change in Loop Quantum Gravity with topspin network formalism with application to homogeneous and isotropic cosmology
• Generating large primordial fluctuations in single-field inflation for PBH formation
• Morphometry on the sphere: Cartesian and irreducible Minkowski tensors explained and implemented
• No slow-roll inflation à la Generalized Chaplygin Gas in General Relativity
• The End of the Road for Far-infrared Reddening Maps? Evidence for Reddening Errors Driven by Changes in PAH Abundance
• Using Lyman Alpha Absorption to Measure the Intensity and Variability of $z\sim 2.4$ Ultraviolet Background Light
• Dark matter spiral arms in Milky Way-like halos
• The establishment of the Standard Cosmological Model through observations
• A Monte Carlo comparison between template-based and Wiener-filter CMB dipole estimators
• Impact of primordial black holes on the formation of the first stars and galaxies
• On CMB B-modes and the Onset of Inflation
• A unique window into the Epoch of Reionisation: A double-peaked Lyman-$\alpha$ emitter in the proximity zone of a quasar at $z\sim 6.6$
• Dark Matter Annihilation via Breit-Wigner Enhancement with Heavier Mediator
• Probing the global 21-cm background by velocity-induced dipole and quadrupole anisotropies
• Sustaining quasi de-Sitter inflation with bulk viscosity
• The Three Hundred: Gas Properties Outside of Galaxy Cluster with the WHIM Contribution and Detection
• Improving CMB constraints on early Universe physics with LSS: A multi-probe forecast including cross-covariance
• Towards a multi-tracer neutrino mass measurement with line-intensity mapping
• Cosmological Non-Gaussianity from Neutrino Seesaw Mechanism
• Cosmological Signatures of Neutrino Seesaw Mechanism
• Disentangling the Halo: Joint Model for Measurements of the Kinetic Sunyaev-Zeldovich Effect and Galaxy-Galaxy Lensing
• Filtering in CMB data analysis with application to ACT DR4 and Planck observations
• New Constraints on Anisotropic Expansion from Supernovae Type Ia
• Solar system peculiar motion from the Hubble diagram of quasars and testing the Cosmological Principle
• Stage IV CMB forecasts for warm inflation
• Quantum Sensing Using Atomic Clocks for Nuclear and Particle Physics
• Dark Matter constraints from Planck observations of the Galactic polarized synchrotron emission
• Testing Refracted Gravity with kinematics of galaxy clusters
• No evidence for local $H_0$ anisotropy from Tully--Fisher or supernova distances
• Inverse Tritium Beta Decay with Relic Neutrinos, Solar Neutrinos, and a 51Cr Source
• The choice of Planck CMB likelihood in cosmological analyses
• Application of Genetic Algorithm to Estimate the Large Angular Scale Features of Cosmic Microwave Background
• The Universe is Brighter in the Direction of Our Motion: Galaxy Counts and Fluxes are Consistent with the CMB Dipole
• Master variables and Darboux symmetry for axial perturbations of the exterior and interior of black hole spacetimes
• The Relation Between Transverse and Radial Velocity Distributions for Observations of an Isotropic Velocity Field
• Statistical exploration of halo anisotropic clustering and intrinsic alignments with the mass-Peak Patch algorithm
• Regularization of Single Field Inflation Models
• Radiative seesaw corrections and charged-lepton decays in a model with soft flavour violation
• Covariant Predictions for Planck-Scale Features in Primordial Power Spectra
• L-BASS: a project to produce an absolutely calibrated 1.4 GHz sky map, I -- Scientific rationale and system overview
• The Simons Observatory: Design, Optimization, and Performance of Low Frequency Detectors
• On the Possibility of Detecting a Global Signal in the Line of the Hyperfine Structure of Hydrogen from the Dark Ages
• Neutrino masses, leptogenesis and dark matter
• Clusternets: A deep learning approach to probe clustering dark energy
• Linear perturbations spectra for dynamical dark energy inspired by modified gravity
• Inflating without a flat potential: Viscous inflation
• Reconciling cosmic dipolar tensions with a gigaparsec void
• Statistical properties of Galactic synchrotron temperature and polarization maps -- a multi-frequency comparison
• Self-supervised component separation for the extragalactic submillimeter sky
• Stellar Profile Independent Determination of the Dark Matter Distribution of the Fornax Local Group Dwarf Spheroidal Galaxy
• Fast and spurious: a robust determination of our peculiar velocity with future galaxy surveys
• A Minkowski Functional Analysis of the Cosmic Microwave Background Weak Lensing Convergence
• Common Origin of Warm Dark Matter and Dark Radiation
• Enhancement of the Higgs decay into a $Z^{\prime }$ pair in models with $U(1{)}_X$ gauge symmetry
• Dark energy and spontaneous mirror symmetry breaking
• Cosmological nanolensing by dense gas clouds
• Cauchy-compact flat spacetimes with extreme BTZ
• Distribution of Phantom Dark Matter in Dwarf Spheroidals
• Deep Needlet: A CNN based full sky component separation method in Needlet space
• Gravitational Fluctuations as an Alternative to Inflation II. CMB Angular Power Spectrum
• Impact of Calibration and Position Errors on Astrophysical Parameters of the HI 21cm Signal
• Testing the dark origin of neutrino masses with oscillation experiments
• Dark energy model with very large-scale inhomogeneity
• Small Correlated Against Large Estimator (SCALE) for Cosmic Microwave Background Lensing
• A New Probe of Gaussianity and Isotropy applied to the CMB Maps
• Degrees of Freedom of New General Relativity I: Type 2, Type 3, Type 5, and Type 8
• Polarization fraction of Planck Galactic cold clumps and forecasts for the Simons Observatory
• Enhancing the Sensitivity to Seesaw Predictions in Gauged $B-L$ Scenarios
• Theoretical priors in scalar-tensor cosmologies: Shift-symmetric Horndeski models
• Unimodular Theory of Gravity in Light of the Latest Cosmological Data
• Deconfusing intensity maps with neural networks
• Observational constraints on the second-order primordial power spectrum: Exploring a Continuous Spontaneous Localization inspired inflationary model
• Quantum fluctuations and semiclassicality in an inflaton-driven evolution
• Model-independent constraints on clustering and growth of cosmic structures from BOSS DR12 galaxies in harmonic space
• Gamma-ray signature of superluminous supernovae: Fermi-LAT GeV detection of SN 2017egm and evidence of a central engine
• Robust laboratory limits on a cosmological spatial gradient in the electromagnetic fine-structure constant from accelerometer experiments
• Quantum Gravity, Hydrodynamics and Emergent Cosmology: A Collection of Perspectives
• Messier 90 galactic halo rotation in the microwaves
• Gluino Search with Stop and Top in Nonuniversal Gaugino Mass Models at LHC and Future Colliders
• Cosmic Strings-induced CMB anisotropies in light of Weighted Morphology
• $A_5$ symmetry and deviation from Golden Ratio mixing with charged lepton flavor violation
• Is natural inflation in agreement with CMB data?
• Nearly Full-Sky Low-Multipole Cosmic Microwave Background Temperature Anisotropy: II. Angular Power Spectra and Likelihood
• Horizon, homogeneity and flatness problems -- do their resolutions really depend upon inflation?
• Theoretical Radio Signals from Radio-Band Gravitational Waves Converted from the Neutron Star Magnetic Field
• Metamorphosis of dwarf halo density profile under dark matter decays
• Viable Curvaton Models from the $f_{NL}$ Parameter
• A universal and physically motivated threshold for Hessian-based cosmic web identification: V-Web case
• 3-3-1 Self Interacting Dark Matter and the Galaxy Core-Cusp problem
• Exploiting the high-resolution NIKA2 data to study the intracluster medium and dynamical state of ACT-CL J0240.0+0116
• ADF22+: a declining faint end in the far-infrared luminosity function in the SSA22 protocluster at z=3.09
• Violation of Bell inequalities from Cosmic Microwave Background data
• Holographic description of the dissipative model of universe with curvature
• Constraining the primordial power spectrum using a differentiable likelihood
• Gravitational Wave Memory Imprints on the CMB from Populations of Massive Black Hole Mergers
• Anomalies of Cosmic Anisotropy from Holographic Universality of Great-Circle Variance
• Gamma-Ray Bursts Calibrated by Using Artificial Neural Networks from the Pantheon+ Sample
• Noether symmetry approach in non-minimal derivative coupling gravity
• Infrared galaxies detected by the Atacama Cosmology Telescope
• Particle production during inflation: constraints expected from redshifted 21 cm observations from the epoch of reionization
• Helium emission from Balmer-dominated shocks in Type Ia supernova remnants provides constraints to their progenitor systems
• Multi-Scale Perturbation Theory II: Solutions and Leading-Order Bispectrum in the $\Lambda$CDM Universe
• Distributed filtered hyperinterpolation for noisy data on the sphere
• Evolution of Cosmic Voids in the Schrodinger-Poisson Formalism
• BeyondPlanck V. Minimal ADC Corrections for Planck LFI
• Homology reveals significant anisotropy in the cosmic microwave background
• Gravitational and electromagnetic Cherenkov radiation constraints in modified dispersion relations
• Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics
• Scalar and vector modes in inflation with antisymmetric tensor field
• Exploring the connection between compact object mergers and fast X-ray transients: The cases of LXT 240402A and EP250207b
• HETDEX Public Data Release 1: Source Catalog 2 and Data Cubes from ~90 sq deg of Integral-Field Optical Spectroscopy
• Curvature perturbations from vacuum transition during inflation
• Large-scale acoustic peak shift in the Planck CMB data
• Exploring the Origin of Supermassive Black Holes with Coherent Neutrino Scattering
• The cosmological Mass Varying Neutrino model in the late universe
• Investigating star-formation activity towards the southern HII region RCW 42
• Cosmic tango between the very small and the very large: Addressing CMB anomalies through Loop Quantum Cosmology
• Ricci cosmology in light of astronomical data
• The Hubble Tension: Relativistic Dark Matter Production from Long-lived Particles
• Disk fraction among free-floating planetary-mass objects in Upper Scorpius
• Origin of Weak MgII and Higher Ionization Absorption Lines in an Outflow from an Intermediate-Redshift Dwarf Satellite Galaxy
• How light can ALP dark matter be?
• LiteBIRD science goals and forecasts: improved full-sky reconstruction of the gravitational lensing potential through the combination of Planck and LiteBIRD data
• Search for resonances decaying to an anomalous jet and a Higgs boson in proton-proton collisions at $\sqrt{s}$ = 13 TeV
• Enhancement of the Axion Decay Constant in Inflation and the Weak Gravity Conjecture
• Catching TeV emission from GRB 221009A and alike with LHAASO, LACT and SWGO
• Inflation Story: slow-roll and beyond
• Impact of the cosmological expansion on spectral energy density of radiation in the intergalactic medium and once more about Olbers' paradox
• Power Suppression and Lensing Anomaly -- A phenomenological investigation
• Mathematical Singularities in the Farthest Confines of the Universe -- And a Brief Report on Its Evolutionary History
• Perturbation Theory Remixed II: Improved Modeling of Nonlinear Bispectrum
• Using thermodynamics to learn gravitational wave physics
• Statistical Isotropy of the CMB E-mode signal
• Lensing Without Borders. I. A Blind Comparison of the Amplitude of Galaxy-Galaxy Lensing Between Independent Imaging Surveys
• Accelerating BAO Scale Fitting Using Taylor Series
• Characterizing CO Emitters in the SSA22-AzTEC26 Field
• The Right-Handed Slepton Bulk Region for Dark Matter in Generalized No-scale $\mathcal{F}$-$SU(5)$ with Effective Super-Natural Supersymmetry
• On the generalized Faber-Jackson relation for galaxy clusters
• Geometric distances between closed universes
• Exploring the cosmic microwave background dipole direction using gamma-ray bursts
• Improving NASA/IPAC Extragalactic Database Redshift Calculations
• Pulsar scattering as a probe for structures in the interstellar medium
• MNTES: Modeling Nonlinearity of TES detectors for Enhanced Cosmic Microwave Background measurements with LiteBIRD
• Constraining the polarisation flux density and angle of point sources by training a convolutional neural network
• The large-scale monopole of the power spectrum in a Euclid-like survey: wide-angle effects, lensing, and the `finger of the observer'
• Neutrino mass limits and decaying dark matter: background evolution versus perturbations
• Flat Space, Dark Energy, and the Cosmic Microwave Background
• The Hawking Energy in a Perturbed Friedmann-Lemaître Universe
• Optimal bolometer transfer function deconvolution for CMB experiments through maximum likelihood mapmaking
• Implications of single field inflation in general cosmological scenarios on the nature of dark energy given the swampland conjectures
• Requirements on bandpass resolution and measurement precision for LiteBIRD
• Cosmic backgrounds from the radio to the far-infrared: recent results and perspectives from cosmological and astrophysical surveys
• Horndeski in motion
• Primordial perturbations in kinetically dominated regimes of general relativity and hybrid quantum cosmology
• Critical Analysis of Replacing Dark Matter and Dark Energy with a Model of Stochastic Spacetime
• Bayesian inference methodology to characterize the dust emissivity at far-infrared and submillimeter frequencies
• Evidence against Ryskin's model of cosmic acceleration
• Cosmological measurements from the CMB and BAO are insensitive to the tail probability in the assumed likelihood
• Self-similar cosmological solutions in f(R,T) gravity theory
• Exploring Cosmological Implications of the Modified Raychaudhuri Equation in Non-Gravitating Vacuum Energy Theory
• The Herschel-SPIRE Dark Field -- II. A P(D) fluctuation analysis of the deepest Herschel image of the submillimetre universe
• Timing Mass of the Local Group
• Curvature perturbations from preheating with scale dependence
• Implications of scattering for CMB foreground emission modelling
• GRB 260310A / SN 2026fgk: A Multi-Wavelength Study of a Nearby Underluminous Long GRB and SN with a Complex Afterglow
• Light right-handed Smuons at the LHC: Natural dark matter and $g_{\mu }-2$ in an unexplored realm of the pMSSM
• The Ellis and Baldwin test of the Cosmic Dipole: Exploring the impact of multiple flux density cuts
• Testing the cosmological principle with quasars
• The Manticore Project II: Bayesian digital twins of cosmic structure across the SDSS and BOSS volumes
• Non-singular Bouncing Cosmology in $f(R,G,T)$--Quintom model
• Geometric Matching of Local Static Regions in Cosmological Spacetimes with an Evolving Lapse
• Neural network emulator to constrain the high-$z$ IGM thermal state from Lyman-$\alpha$ forest flux auto-correlation function
• Measuring peculiar velocity and tomographic redshift dipole with DESI DR1 catalogs
• Local bandpower diagnostics for the hemispherical power asymmetry in CMB E-mode polarization
• Asymptotic analysis of the Boltzmann equation for dark matter relic abundance
• Do We Have Sufficient Knowledge of the Galactic Foreground Emission in Cosmic Microwave Background Science?
• Advancing weak lensing mass mapping with a mask-aware HEALPix transformer
• The ViSta method for stacking in the Fourier domain and its application to the dusty star-forming galaxies in the ALMA Science Archive
• Disentangling the Cosmic/Comoving Duality: The Cognitive Stability and Typicality Tests
• SKA and the Cosmic Radio Dipole
• Mitigating gain calibration errors from EoR observations with SKA1-Low AA*
• Distinct radial acceleration relations of galaxies and galaxy clusters supports hyperconical modified gravity
• Oscillating scalar field as dark matter through the cosmological epochs
• Circumventing Cosmic Variance via Remote Quadrupole Measurements
• From Geometry to Observation: Gravitational Waves and the Raychaudhuri Equation
• Stop Search in SUSY SO(10) GUTs with Nonuniversal Gaugino Masses
• A new approach of estimating the Galactic thermal dust and synchrotron polarized emission template in the microwave bands
• Linking Young Stellar Object Morphology to Evolutionary Stages with Self-Organizing Maps
• Center-of-mass recoil effects on the annihilation and formation of dark matter bound pairs
• Towards detecting Primordial non-Gaussianity in the CMB using Spherical Convolutional Neural Networks
• Clustering analysis of medium-band selected high-redshift galaxies
• Overview of the ESCAPE Dark Matter Test Science Project for Astronomers
• Living on the Fermi Edge: On Baryon Transport and Fermi Condensation
• Asymmetries in invisible Dark Matter mediator production associated with $t\bar{t}$ final states
• Lagrangian Perturbation Theory for Biased Tracers: Significance of the Number Conservation
• Galaxy number-count dipole and superhorizon fluctuations
• Combining Planck and SPT cluster catalogs: cosmological analysis and impact on Planck scaling relation calibration
• Redshift and gauge choice
• Stochastic gravitational wave background from the collisions of dark matter halos
• Background stability and annual modulation test using PICOLON ultra-pure NaI(Tl) detector
• Confusing dark matter particle properties with modifications to General Relativity
• Addressing Dipole Tension via Clustering in $\Lambda$CDM and beyond
• On the computational feasibility of Bayesian end-to-end analysis of LiteBIRD simulations within Cosmoglobe
• Cosmic Dipoles from Large-Scale Structure Surveys
• The Kaiser-Rocket effect: three decades and counting
• First Light: Switching on Stars at the Dawn of Time
• The Parameter-Level Performance of Covariance Matrix Conditioning in Cosmic Microwave Background Data Analyses
• Cosmological structure formation in complex scalar field dark matter versus real ultralight axions: a comparative study using CLASS
• Streaming Velocity Effects on the Post-reionization 21 cm Baryon Acoustic Oscillation Signal
• Stability Analysis of Four $f(Q)$ Gravity Models : A Cosmological Review in the Background of Bianchi-I Anisotropy
• Multi-frequency point source detection with fully convolutional networks: Performance in realistic microwave sky simulations
• Particle production during inflation: A Bayesian analysis with CMB data from Planck 2018
• AGN-host interaction in IC 5063. I. Large-scale X-ray morphology and spectral analysis
• Towards a de Sitter quintom-like cosmology from a reduction of a 7-dimensional $BF$ theory
• Sample Variance in Cosmological Observations with a Narrow Field-of-View
• Evidence of Two-Source King Plot Nonlinearity in Spectroscopic Search for New Boson
• The CMB bispectrum from bouncing cosmologies
• Unitary evolution and cosmic acceleration in Loop Quantum Cosmology
• A Fuzzy Situation Eased: Cold Dark Matter with Multipoles Can Explain The Double Radio Quad Lens HS 0810+2554
• Physics beyond the Standard Model with the DSA-2000
• Beam-deconvolved Planck LFI maps
• Optimal map-making with singularities
• Consistency of Planck Data With Power-Law Primordial Scalar Power Spectrum
• Lectures on the Bondi--Metzner--Sachs group and related topics in infrared physics
• Forecasting ground-based sensitivity to the Rayleigh scattering of the CMB in the presence of astrophysical foregrounds
• Free Cosmic Density Bispectrum on Small Scales
• Finite inflation in curved space
• The quantum de Sitter root of quasi de Sitter observables: a pedagogical review
• A global view on star formation: The GLOSTAR Galactic plane survey XII. Effelsberg's continuum view and data release
• Search for dark matter produced in association with a Higgs boson decaying to bottom quarks in proton-proton collisions at $\sqrt{s}$ = 13 TeV
• What is Known About the Polarization of Starlight in the Southern Hole
• Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension
• Structure Formation with Dark Magnetohydrodynamics
• Marked statistics across the cosmic web: Environmental dependent clustering in modified gravity simulations
• The BINGO project X. Cosmological parameter constraints from HI Intensity Mapping lognormal simulations
• Weak Lensing Low Multipoles
• Seeing Wiggles without Seeing Wiggles: BAO Recovery in 21 cm Intensity Mapping with Deep Learning
• Our Peculiar Motion Inferred from Number Counts of Mid Infra Red AGNs and the Discordance Seen with the Cosmological Principle
• Background dynamics and observational constraints of flat and non-flat $\Lambda (t)$CDM models from $H(z)$ and DESI DR2 BAO measurements
• Detecting dark matter substructure with lensed quasars in optical bands
• First constraints on the intrinsic CMB dipole and our velocity with Doppler and aberration
• Spectral Map Making with SPHEREx
• In-depth analysis of the clustering of dark matter particles around primordial black holes. Part III: CMB constraints
• The read-out electronics for the FLASH experiment
• Expected redshift drift for tilted observers