The Simons Observatory: Science goals and forecasts

Abstract

The Simons Observatory (SO) is a new cosmic microwave background experiment being built on Cerro Toco in Chile, due to begin observations in the early 2020s. We describe the scientific goals of the experiment, motivate the design, and forecast its performance. SO will measure the temperature and polarization anisotropy of the cosmic microwave background in six frequency bands: 27, 39, 93, 145, 225 and 280 GHz. The initial configuration of SO will have three small-aperture 0.5-m telescopes (SATs) and one large-aperture 6-m telescope (LAT), with a total of 60,000 cryogenic bolometers. Our key science goals are to characterize the primordial perturbations, measure the number of relativistic species and the mass of neutrinos, test for deviations from a cosmological constant, improve our understanding of galaxy evolution, and constrain the duration of reionization. The SATs will target the largest angular scales observable from Chile, mapping ~10% of the sky to a white noise level of 2 $\mu$K-arcmin in combined 93 and 145 GHz bands, to measure the primordial tensor-to-scalar ratio, $r$, at a target level of $\sigma (r)=0.003$. The LAT will map ~40% of the sky at arcminute angular resolution to an expected white noise level of 6 $\mu$K-arcmin in combined 93 and 145 GHz bands, overlapping with the majority of the LSST sky region and partially with DESI. With up to an order of magnitude lower polarization noise than maps from the Planck satellite, the high-resolution sky maps will constrain cosmological parameters derived from the damping tail, gravitational lensing of the microwave background, the primordial bispectrum, and the thermal and kinematic Sunyaev-Zel'dovich effects, and will aid in delensing the large-angle polarization signal to measure the tensor-to-scalar ratio. The survey will also provide a legacy catalog of 16,000 galaxy clusters and more than 20,000 extragalactic sources.

This paper presents an overview of the Simons Observatory science goals, details about the instrument will be presented in a companion paper. The author contribution to this paper is available at https://simonsobservatory.org/publications.php (Abstract abridged) -- matching version published in JCAP

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• The Physics of Galaxy Cluster Outskirts
• Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data
• The Impact of the First Galaxies on Cosmic Dawn and Reionization
• Observational Constraints on the Physical Properties of Interstellar Dust in the Post-Planck Era
• An Improved Measurement of the Secondary Cosmic Microwave Background Anisotropies from the SPT-SZ + SPTpol Surveys
• Dark Energy at early times and ACT: a larger Hubble constant without late-time priors
• Scalar-tensor theories of gravity, neutrino physics, and the $H_0$ tension
• Cosmology with the Wide-Field Infrared Survey Telescope -- Multi-Probe Strategies
• Dark Photon Oscillations in Our Inhomogeneous Universe
• The Websky Extragalactic CMB Simulations
• Restoring cosmological concordance with early dark energy and massive neutrinos?
• Using the Marked Power Spectrum to Detect the Signature of Neutrinos in Large-Scale Structure
• The Atacama Cosmology Telescope: Component-separated maps of CMB temperature and the thermal Sunyaev-Zel'dovich effect
• CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope
• Do we have any hope of detecting scattering between dark energy and baryons through cosmology?
• Hints of Early Dark Energy in Planck, SPT, and ACT data: new physics or systematics?
• Gravitational Waves from Domain Walls in Pulsar Timing Array Datasets
• Dark energy in light of the early JWST observations: case for a negative cosmological constant?
• Constraining local non-Gaussianities with kSZ tomography
• First Cosmological Constraint on the Effective Theory of Dark Matter-Proton Interactions
• The Novel Probes Project -- Tests of Gravity on Astrophysical Scales
• Testing Screened Modified Gravity
• Consistent lensing and clustering in a low-$S_8$ Universe with BOSS, DES Year 3, HSC Year 1 and KiDS-1000
• Evidence for suppression of structure growth in the concordance cosmological model
• Constraints on Cosmological Parameters from the 500 deg${}^2$ SPTpol Lensing Power Spectrum
• The growth of density perturbations in the last $\sim$10 billion years from tomographic large-scale structure data
• Constraints on $\Lambda$CDM Extensions from the SPT-3G 2018 $EE$ and $TE$ Power Spectra
• Joint constraints on cosmology and the impact of baryon feedback: combining KiDS-1000 lensing with the thermal Sunyaev-Zeldovich effect from Planck and ACT
• Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations
• Direct detection of dark energy: the XENON1T excess and future prospects
• Updated constraints on amplitude and tilt of the tensor primordial spectrum
• Recombination-independent determination of the sound horizon and the Hubble constant from BAO
• Measurement of the Splashback Feature around SZ-selected Galaxy Clusters with DES, SPT and ACT
• Foreground-immune CMB lensing with shear-only reconstruction
• The Sigma-8 Tension is a Drag
• The Simons Observatory: Astro2020 Decadal Project Whitepaper
• Constraining neutrino mass with tomographic weak lensing one-point probability distribution function and power spectrum
• $Euclid$ preparation: XV. Forecasting cosmological constraints for the $Euclid$ and CMB joint analysis
• The state of the dark energy equation of state circa 2023
• Cosmology with kSZ: breaking the optical depth degeneracy with Fast Radio Bursts
• DeepCMB: Lensing Reconstruction of the Cosmic Microwave Background with Deep Neural Networks
• Peeling off foregrounds with the constrained moment ILC method to unveil primordial CMB $B$-modes
• A Measurement of the Degree Scale CMB B-mode Angular Power Spectrum with POLARBEAR
• A Review of X-ray Microcalorimeters Based on Superconducting Transition Edge Sensors for Astrophysics and Particle Physics
• Fractional attractors in light of the latest ACT observations
• Lower bias, lower noise CMB lensing with foreground-hardened estimators
• The Origin of Parity Violation in Polarized Dust Emission and Implications for Cosmic Birefringence
• Time-dependence of the astrophysical stochastic gravitational wave background
• Searching for Anisotropic Cosmic Birefringence with Polarization Data from SPTpol
• Tracing the high energy theory of gravity: an introduction to Palatini inflation
• Quadratic estimators for CMB weak lensing
• Dawn of the dark: unified dark sectors and the EDGES Cosmic Dawn 21-cm signal
• Massive neutrinos and cosmic composition
• $\Lambda$CDM or self-interacting neutrinos? - how CMB data can tell the two models apart
• Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies
• Revealing the effects of curvature on the cosmological models
• CMB/kSZ and Compton-$y$ Maps from 2500 square degrees of SPT-SZ and Planck Survey Data
• The Gravitino and the Swampland
• Primordial Features from Linear to Nonlinear Scales
• Tomographic measurement of the intergalactic gas pressure through galaxy-tSZ cross-correlations
• Bayesian delensing delight: sampling-based inference of the primordial CMB and gravitational lensing
• Observational constraints on dark matter scattering with electrons
• Testing AdS early dark energy with Planck, SPTpol and LSS data
• Finding cosmic voids and filament loops using topological data analysis
• Isotropic cosmic birefringence from early dark energy
• Colliding Ghosts: Constraining Inflation with the Parity-Odd Galaxy Four-Point Function
• The Atacama Cosmology Telescope: Detection of the Pairwise Kinematic Sunyaev-Zel'dovich Effect with SDSS DR15 Galaxies
• The Benefits of CMB Delensing
• DESI luminous red galaxy samples for cross-correlations
• A tale of two (or more) $h$'s
• Intensity Mapping as a Probe of Axion Dark Matter
• Health checkup test of the standard cosmological model in view of recent Cosmic Microwave Background Anisotropies experiments
• Trans-Planckian Censorship, Inflation and Dark Matter
• Future CMB constraints on cosmic birefringence and implications for fundamental physics
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• Multidimensionality of the Hubble tension: the roles of ${\Omega }_m$ and ${\omega }_c$
• Optimal CMB Lensing Reconstruction and Parameter Estimation with SPTpol Data
• Thermalization of large energy release in the early Universe
• HYREC-2: a highly accurate sub-millisecond recombination code
• Constraints on Scalar and Tensor spectra from $N_{eff}$
• Future Constraints on Dynamical Dark-Energy using Gravitational-Wave Standard Sirens
• Determining the Hubble Constant without the Sound Horizon: A $3.6\%$ Constraint on $H_0$ from Galaxy Surveys, CMB Lensing and Supernovae
• Gravitational Wave from Graviton Bremsstrahlung during Reheating
• QUIJOTE scientific results -- IV. A northern sky survey in intensity and polarization at 10-20GHz with the Multi-Frequency Instrument
• Constraining the Baryon Abundance with the Kinematic Sunyaev-Zel'dovich Effect: Projected-Field Detection Using Planck, WMAP, and unWISE
• Combining pre- and post-recombination new physics to address cosmological tensions: case study with varying electron mass and sign-switching cosmological constant
• ALP Dark Matter in a Primordial Black Hole Dominated Universe
• The large scale polarization explorer (LSPE) for CMB measurements: performance forecast
• Cosmological Constraints on Light (but Massive) Relics
• Evidence for Line-of-Sight Frequency Decorrelation of Polarized Dust Emission in $Planck$ Data
• The Atacama Large Aperture Submillimetre Telescope (AtLAST)
• Primordial Gravitational Waves from Galaxy Intrinsic Alignments
• Joint CMB and BBN Constraints on Light Dark Sectors with Dark Radiation
• New constraint on the tensor-to-scalar ratio from the $Planck$ and BICEP/Keck Array data using the profile likelihood
• Cosmological Signatures of Superheavy Dark Matter
• Cosmology with the Wide-Field Infrared Survey Telescope -- Synergies with the Rubin Observatory Legacy Survey of Space and Time
• Indications for a Nonzero Lepton Asymmetry from Extremely Metal-Poor Galaxies
• Can we neglect relativistic temperature corrections in the Planck thermal SZ analysis?
• The Simons Observatory microwave SQUID multiplexing detector module design
• Cosmological Constraints on First-Order Phase Transitions
• Observational constraints of a new unified dark fluid and the $H_0$ tension
• Is cosmic birefringence due to dark energy or dark matter? A tomographic approach
• The Atacama Cosmology Telescope: Two-season ACTPol Extragalactic Point Sources and their Polarization properties
• Constraints on the redshift evolution of astrophysical feedback with Sunyaev-Zeldovich effect cross-correlations
• Cosmology with dropout selection: Straw-man surveys and CMB lensing
• The Simons Observatory Large Aperture Telescope Receiver
• CMB targets after the latest Planck data release
• Probing galaxy evolution in massive clusters using ACT and DES: splashback as a cosmic clock
• A Demonstration of Improved Constraints on Primordial Gravitational Waves with Delensing
• Primordial lepton asymmetries in the precision cosmology era: Current status and future sensitivities from BBN and the CMB
• Probing Dark Matter with Future CMB Measurements
• Exploring Early Dark Energy solution to the Hubble tension with Planck and SPTPol data
• Scale independent $R^2$ inflation
• Probing Axion-like Particles via CMB Polarization
• Single field inflation in the light of Pulsar Timing Array Data: Quintessential interpretation of blue tilted tensor spectrum through Non-Bunch Davies initial condition
• Dark Matter properties through cosmic history
• Bayesian evidence for the tensor-to-scalar ratio $r$ and neutrino masses $m_{\nu }$: Effects of uniform vs logarithmic priors
• Consistency of Planck, ACT and SPT constraints on magnetically assisted recombination and forecasts for future experiments
• Messengers from the Early Universe: Cosmic Neutrinos and Other Light Relics
• Constraints on Pre-Recombination Early Dark Energy from SPT-3G Public Data
• Stellar Property Statistics of Massive Halos from Cosmological Hydrodynamics Simulations: Common Kernel Shapes
• Hints of dark matter-neutrino interactions in Lyman-$\alpha$ data
• QUBIC I: Overview and ScienceProgram
• Bridging the gap: spectral distortions meet gravitational waves
• Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory
• Planck and BICEP/Keck Array 2018 constraints on primordial gravitational waves and perspectives for future B-mode polarization measurements
• Constraints On Scalar-Induced Gravitational Waves Up To Third Order From Joint Analysis of BBN, CMB, And PTA Data
• Quijote-PNG: Simulations of primordial non-Gaussianity and the information content of the matter field power spectrum and bispectrum
• Power spectrum of domain-wall network and its implications for isotropic and anisotropic cosmic birefringence
• Neutrino non-standard interactions meet precision measurements of $N_{\mathrm{eff}}$
• Impact of polarised extragalactic sources on the measurement of CMB B-mode anisotropies
• Characterizing hydrostatic mass bias with Mock-X
• Sensitivity of the Prime-Cam Instrument on the CCAT-prime Telescope
• Constraining Cluster Virialization Mechanism and Cosmology using Thermal-SZ-selected clusters from Future CMB Surveys
• Cosmic Neutrino Background Detection in Large-Neutrino-Mass Cosmologies
• Dust Polarization Maps from TIGRESS: E/B power asymmetry and TE correlation
• Recent Progress in Modeling the Macro- and Micro-Physics of Radio Jet Feedback in Galaxy Clusters
• Cosmological implications of $n_s\approx 1$ in light of the Hubble tension
• Internal delensing of Cosmic Microwave Background polarization B-modes with the POLARBEAR experiment
• The Simons Observatory: Constraining inflationary gravitational waves with multi-tracer B-mode delensing
• Natural inflation with a nonminimal coupling to gravity
• Non-universality of the mass function: dependence on the growth rate and power spectrum shape
• Light Dirac neutrino portal dark matter with observable $\Delta N_{\mathrm{eff}}$
• Revealing the Cosmic History with Gravitational Waves
• A minimal power-spectrum-based moment expansion for CMB B-mode searches
• Statistical description of dust polarized emission from the diffuse interstellar medium -- A RWST approach
• Cosmic Birefringence Test of the Hubble Tension
• Cosmological Implications of Axion-Matter Couplings
• CMB constraints on the early universe independent of late time cosmology
• Constraining Single-Field Inflation with MegaMapper
• Uncovering the History of Cosmic Inflation from Anomalies in Cosmic Microwave Background Spectra
• Cosmology with varying fundamental constants from hyperlight, coupled scalars
• Constraints on primordial magnetic fields from magnetically-induced perturbations: current status and future perspectives with LiteBIRD and future ground based experiments
• CMB-S4: Iterative Internal Delensing and $r$ Constraints
• Quantifying the global "CMB tension" between the Atacama Cosmology Telescope and the Planck satellite in extended models of cosmology
• Transverse Velocities with the Moving Lens Effect
• Primordial Non-Gaussianity
• Self-Interacting Neutrinos in Light of Large-Scale Structure Data
• Limits on the cosmic neutrino background
• Improved cosmic microwave background (de-)lensing using general spherical harmonic transforms
• Microwave Spectro-Polarimetry of Matter and Radiation across Space and Time
• The Simons Observatory: gain, bandpass and polarization-angle calibration requirements for B-mode searches
• Cosmological constraints on the gravitational constant
• Precise dark matter relic abundance in decoupled sectors
• The Atacama Cosmology Telescope DR6 and DESI: Structure formation over cosmic time with a measurement of the cross-correlation of CMB Lensing and Luminous Red Galaxies
• Varying fundamental constants principal component analysis: additional hints about the Hubble tension
• Mitigating the optical depth degeneracy using the kinematic Sunyaev-Zel'dovich effect with CMB-S4
• Performance forecasts for the primordial gravitational wave detection pipelines for AliCPT-1
• Enhancing gravitational wave anisotropies with peaked scalar sources
• Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
• Neutrino Properties with Ground-Based Millimeter-Wavelength Line Intensity Mapping
• Small-scale clumping at recombination and the Hubble tension
• AMICO galaxy clusters in KiDS-DR3: Constraints on cosmological parameters and on the normalisation of the mass-richness relation from clustering
• Shocks in the Stacked Sunyaev-Zel'dovich Profiles of Clusters I: Analysis with the Three Hundred Simulations
• Can small-scale baryon inhomogeneities resolve the Hubble tension? An investigation with ACT DR4
• Mass Calibration of Optically Selected DES clusters using a Measurement of CMB-Cluster Lensing with SPTpol Data
• BeyondPlanck III. Commander3
• Foreground-immune CMB lensing reconstruction with polarization
• Impact of Polarized Galactic Foreground Emission on CMB Lensing Reconstruction and Delensing of B-Modes
• Searching for axion-like particles through CMB birefringence from string-wall networks
• Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe
• Confronting interacting dark radiation scenarios with cosmological data
• Neutrino Mass from Cosmology: Probing Physics Beyond the Standard Model
• Determination of miscalibrated polarization angles from observed CMB and foreground $EB$ power spectra: Application to partial-sky observation
• CosmoPower-JAX: high-dimensional Bayesian inference with differentiable cosmological emulators
• Do you smell something decaying? Updated linear constraints on decaying dark matter scenarios
• Constraining primordial non-Gaussianity from DESI quasar targets and Planck CMB lensing
• Shocks in the Stacked Sunyaev-Zel'dovich Profiles of Clusters II: Measurements from SPT-SZ + Planck Compton-y Map
• Warm Little Inflaton becomes Dark Energy
• CosmoBit: A GAMBIT module for computing cosmological observables and likelihoods
• Machine Learning for Observational Cosmology
• Mapping the relativistic electron gas temperature across the sky
• CoLoRe: fast cosmological realisations over large volumes with multiple tracers
• The Atacama Cosmology Telescope: Probing the Baryon Content of SDSS DR15 Galaxies with the Thermal and Kinematic Sunyaev-Zel'dovich Effects
• Baryonic feedback biases on fundamental physics from lensed CMB power spectra
• Primordial Standard Clock Models and CMB Residual Anomalies
• Capse.jl: efficient and auto-differentiable CMB power spectra emulation
• The Atacama Cosmology Telescope: Microwave Intensity and Polarization Maps of the Galactic Center
• Precision CMB constraints on eV-scale bosons coupled to neutrinos
• $S_8$ Tension in the Context of Dark Matter-Baryon Scattering
• $5\sigma$ tension between Planck cosmic microwave background and eBOSS Lyman-alpha forest and constraints on physics beyond $\Lambda$CDM
• Beating the Lyth bound by parametric resonance during inflation
• Inflationary Potential as seen from Different Angles: Model Compatibility from Multiple CMB Missions
• The impact of modified gravity on the Sunyaev-Zel'dovich effect
• Projected-Field Kinetic Sunyaev-Zel'dovich Cross-Correlations: Halo Model and Forecasts
• Inferring the impact of feedback on the matter distribution using the Sunyaev Zel'dovich effect: Insights from CAMELS simulations and ACT+DES data
• Learning to Concentrate: Multi-tracer Forecasts on Local Primordial Non-Gaussianity with Machine-Learned Bias
• The Signatures of Self-Interacting Dark Matter and Subhalo Disruption on Cluster Substructure
• Quintessential $\alpha$-attractor inflation: forecasts for Stage IV galaxy surveys
• Astrophysics & Cosmology from Line Intensity Mapping vs Galaxy Surveys
• Probing correlated compensated isocurvature perturbations using scale-dependent galaxy bias
• The Second Radio Synchrotron Background Workshop: Conference Summary and Report
• On the superstring-inspired quantum correction to the Starobinsky model of inflation
• Axion-Gauge Field Dynamics with Backreaction
• The Simons Observatory: Modeling Optical Systematics in the Large Aperture Telescope
• Towards testing CMB anomalies using the kinetic and polarized Sunyaev Zel'dovich effects
• Cosmology with the moving lens effect
• Fractional Polarisation of Extragalactic Sources in the 500-square-degree SPTpol Survey
• The Gravitational Lensing Signatures of BOSS Voids in the Cosmic Microwave Background
• Exploring KSZ velocity reconstruction with $N$-body simulations and the halo model
• Using the cosmological recombination radiation to probe early dark energy and fundamental constant variations
• The Simons Observatory: Galactic Science Goals and Forecasts
• Likelihood methods for CMB experiments
• Simulations and observational tests of primordial magnetic fields from Cosmic Microwave Background constraints
• CMB lensing power spectrum estimation without instrument noise bias
• The weak, the strong and the ugly -- A comparative analysis of interacting stepped dark radiation
• Partially Constrained Internal Linear Combination: a method for low-noise CMB foreground mitigation
• The Atacama Cosmology Telescope: Detection of mm-wave transient sources
• Probing cosmic birefringence with polarized Sunyaev-Zel'dovich tomography
• On the consistency of $\Lambda$CDM with CMB measurements in light of the latest Planck, ACT, and SPT data
• Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation
• Slow-Roll Inflation at N3LO
• Discordances in cosmology and the violation of slow-roll inflationary dynamics
• Bayesian estimation of our local motion from the Planck-2018 CMB temperature map
• Monopoles, Strings and Gravitational Waves in Non-minimal Inflation
• B-mode Targets
• Cross-correlation between Subaru Hyper Suprime-Cam Galaxy Weak Lensing and Planck Cosmic Microwave Background Lensing
• Fundamental limits on constraining primordial non-Gaussianity
• Improved upper limit on degree-scale CMB B-mode polarization power from the 670 square-degree POLARBEAR survey
• Foreground Separation and Constraints on Primordial Gravitational Waves with the PICO Space Mission
• Including massive neutrinos in thermal Sunyaev Zeldovich power spectrum and cluster counts analyses
• ForSE: a GAN based algorithm for extending CMB foreground models to sub-degree angular scales
• Forecast of Neutrino Cosmology from the CSST Photometric Galaxy Clustering and Cosmic Shear Surveys
• Minimizing gravitational lensing contributions to the primordial bispectrum covariance
• A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
• Small Aperture Telescopes for the Simons Observatory
• Euclid: The search for primordial features
• Assessing the Importance of Noise from Thermal Sunyaev-Zel{'}dovich Signals for CMB Cluster Surveys and Cluster Cosmology
• Probing Lorentz-violating electrodynamics with CMB polarization
• Searching for Oscillations in the Primordial Power Spectrum with CMB and LSS Data
• Twenty years of PWV measurements in the Chajnantor Area
• Probing ultra-light axions with the 21-cm Signal during Cosmic Dawn
• Scaling Transformations and the Origins of Light Relics Constraints from Cosmic Microwave Background Observations
• candl: Cosmic Microwave Background Analysis with a Differentiable Likelihood
• Recovering the CMB Signal with Machine Learning
• Novel constraints on fifth forces and ultralight dark sector with asteroidal data
• Polarized primordial gravitational waves in spatial covariant gravities
• High $H_0$ Values from CMB E-mode Data: A Clue for Resolving the Hubble Tension?
• Impact of internal-delensing biases on searches for primordial B-modes of CMB polarisation
• Probing neutrino interactions and dark radiation with gravitational waves
• Improved constraint on primordial gravitational waves in light of the Hubble tension and BICEP/Keck
• Constraints on Primordial Magnetic Fields from their impact on the ionization history with Planck 2018
• Global view of neutrino interactions in cosmology: The freestreaming window as seen by Planck
• Impact of the Hubble tension on the $r$-$n_s$ contour
• Measuring the Inflaton Coupling in the CMB
• Testing General Relativity on cosmological scales at redshift z ~ 1.5 with quasar and CMB lensing
• Probing Stochastic Gravitational Wave Background from $SU(5)\times U(1{)}_{\chi }$ Strings in Light of NANOGrav 15-Year Data
• Cosmological constraints on nonphantom dynamical dark energy with DESI Data Release 2 Baryon Acoustic Oscillations: A 3$\sigma$+ lensing anomaly
• Understanding the relation between thermal Sunyaev-Zeldovich decrement and halo mass using the SIMBA and TNG simulations
• On the number of $e$-folds in the Jordan and Einstein frames
• The 21 cm-kSZ-kSZ Bispectrum during the Epoch of Reionization
• Improved Mixed Dark Matter Halo Model for Ultralight Axions
• Multiple point criticality principle and Coleman-Weinberg inflation
• Retrieving cosmological information from small-scale CMB foregrounds II. The kinetic Sunyaev Zel'dovich effect
• Constraining the properties of gaseous halos via cross-correlations of upcoming galaxy surveys and thermal Sunyaev-Zel'dovich maps
• Limitations of CMB B-mode template delensing
• The Simons Observatory: Metamaterial Microwave Absorber (MMA) and its Cryogenic Applications
• Non-Gaussianity constraints from Planck spectral distortion cross-correlations
• Constraints on primordial lepton asymmetries with full neutrino transport
• First Constraints on the Epoch of Reionization Using the non-Gaussianity of the Kinematic Sunyaev-Zel{'}dovich Effect from the South Pole Telescope and {\it Herschel}-SPIRE Observations
• Novel higher-curvature variations of $R^2$ inflation
• What does cosmology tell us about the mass of thermal-relic dark matter?
• Dark Radiation from Neutrino Mixing after Big Bang Nucleosynthesis
• Optimal multifrequency weighting for CMB lensing
• Baryogenesis from neutron-dark matter oscillations
• First Identification of a CMB Lensing Signal Produced by $1.5$ Million Galaxies at $z\sim$4: Constraints on Matter Density Fluctuations at High Redshift
• An improved Compton parameter map of thermal Sunyaev-Zeldovich effect from Planck PR4 data
• Prospects of Future CMB Anisotropy Probes for Primordial Black Holes
• Pairwise Transverse Velocity Measurement with the Rees-Sciama Effect
• Removing the giants and learning from the crowd: a new SZ power spectrum method and revised Compton $y$-map analysis
• Transition Edge Sensors: Physics and Applications
• LiteBIRD Science Goals and Forecasts. A Case Study of the Origin of Primordial Gravitational Waves using Large-Scale CMB Polarization
• Multi-Clustering Needlet-ILC for CMB B-modes component separation
• Framework for analysis of next generation, polarised CMB data sets in the presence of galactic foregrounds and systematic effects
• Cleaning our own Dust: Simulating and Separating Galactic Dust Foregrounds with Neural Networks
• Hint of a truncated primordial spectrum from the CMB large-scale anomalies
• The Cosmological Heavy Ion Collider: Fast Thermalization after Cosmic Inflation
• Full-sky Models of Galactic Microwave Emission and Polarization at Sub-arcminute Scales for the Python Sky Model
• Non-Gaussian modelling and statistical denoising of Planck dust polarization full-sky maps using scattering transforms
• Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6
• CMB constraints on a physical model of reionization
• MillimeterDL: Deep Learning Simulations of the Microwave Sky
• Joint velocity and density reconstruction of the Universe with nonlinear differentiable forward modeling
• Simons Observatory Microwave SQUID Multiplexing Readout -- Cryogenic RF Amplifier and Coaxial Chain Design
• Deep XMM-Newton Observations of the Most Distant SPT-SZ Galaxy Cluster
• The role of CMB spectral distortions in the Hubble tension: a proof of principle
• BCS in the Sky: Signatures of Inflationary Fermion Condensation
• Comparison of delensing methodologies and assessment of the delensing capabilities of future experiments
• The Atacama Cosmology Telescope: A search for Planet 9
• Kinetic Sunyaev-Zel'dovich tomography with line-intensity mapping
• When FIMPs Decay into Neutrinos: The $N_{\mathrm{eff}}$ Story
• PSZSPT: a joint Planck and SPT-SZ cluster catalog
• Modified recombination and the Hubble tension
• Neutrino effects on the morphology of cosmic large-scale structure
• Optimal filters for the moving lens effect
• Astrophysical Tests of Dark Matter Self-Interactions
• CMB lensing reconstruction biases from masking extragalactic sources
• Simulated catalogs and maps of radio galaxies at millimeter wavelengths in Websky
• In-flight polarization angle calibration for LiteBIRD: blind challenge and cosmological implications
• Sensitivity forecasts for the cosmological recombination radiation in the presence of foregrounds
• Velocity reconstruction with the cosmic microwave background and galaxy surveys
• On chromonatural inflation in string theory
• Back to the features: assessing the discriminating power of future CMB missions on inflationary models
• Towards a full description of MeV dark matter decoupling: a self-consistent determination of relic abundance and $N_{\mathrm{eff}}$
• Characterizing fast radio bursts through statistical cross-correlations
• Primordial trispectrum from kSZ tomography
• Freeze-in Dark Matter via Light Dirac Neutrino Portal
• LiteBIRD Science Goals and Forecasts: Improving Sensitivity to Inflationary Gravitational Waves with Multitracer Delensing
• Scatter in Sunyaev--Zel'dovich effect scaling relations explained by inter-cluster variance in mass accretion histories
• Inevitable imprints of patchy reionization on the cosmic microwave background anisotropy
• Dark matter models for the 511 keV galactic line predict keV electron recoils on Earth
• Inpainting Galactic Foreground Intensity and Polarization maps using Convolutional Neural Network
• Cosmic birefringence tomography with polarized Sunyaev Zel'dovich effect
• Extragalactic Millimeter Transients in the Era of Next Generation CMB Surveys
• Electromagnetic probes of primordial black holes as dark matter
• Baryonic effects on CMB lensing and neutrino mass constraints
• Optimal filtering for CMB lensing reconstruction
• Principal component analysis of the primordial tensor power spectrum
• Density reconstruction from biased tracers and its application to primordial non-Gaussianity
• Dark Sectors with Mass Thresholds Face Cosmological Datasets
• Reconstructing large scales at cosmic dawn
• Avoiding baryonic feedback effects on neutrino mass measurements from CMB lensing
• Single frequency CMB B-mode inference with realistic foregrounds from a single training image
• Unified and consistent structure growth measurements from joint ACT, SPT and \textit{Planck} CMB lensing
• Minkowski Functionals of CMB polarisation intensity with Pynkowski: theory and application to Planck and future data
• Mass Estimation of Galaxy Clusters with Deep Learning II: CMB Cluster Lensing
• Dirac neutrino mass generation from Majorana messenger
• Developing a unified pipeline for large-scale structure data analysis with angular power spectra -- II. A case study for magnification bias and radio continuum surveys
• Reconstructing Patchy Reionization with Deep Learning
• Full-sky, arcminute-scale, 3D models of Galactic microwave foreground dust emission based on filaments
• Pseudoscalar sterile neutrino self-interactions in light of Planck, SPT and ACT data
• Cosmology from weak lensing alone and implications for the Hubble tension
• Dust polarization spectral dependence from Planck HFI data. Turning point on CMB polarization foregrounds modelling
• Measuring ${\sigma }_8$ using DESI Legacy Imaging Surveys Emission-Line Galaxies and Planck CMB Lensing and the Impact of Dust on Parameter Inference
• Cosmology from Clustering, Cosmic Shear, CMB Lensing, and Cross Correlations: Combining Rubin Observatory and Simons Observatory
• Warm Inflation with the Standard Model
• Improving models of the cosmic infrared background using CMB lensing mass maps
• YOLO-CL: Galaxy cluster detection in the SDSS with deep machine learning
• QUIJOTE scientific results -- VIII. Diffuse polarized foregrounds from component separation with QUIJOTE-MFI
• What is the amplitude of the Gravitational Waves background expected in the Starobinsky model ?
• Testing the $n_s-H_0$ scaling relation with Planck-independent CMB data
• Constraints on axion-like polarization oscillations in the cosmic microwave background with POLARBEAR
• Searching for anisotropic stochastic gravitational-wave backgrounds with constellations of space-based interferometers
• Squeezing $f_{\mathrm{NL}}$ out of the matter bispectrum with consistency relations
• 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
• Calibration of Transition-edge Sensor (TES) Bolometer Arrays with Application to CLASS
• An Accurate Analytic Model for the Thermal Sunyaev-Zel'dovich One-Point PDF
• A Survey of Neutrino Flavor Models and the Neutrinoless Double Beta Decay Funnel
• Bias to CMB lensing from lensed foregrounds
• Probing Cosmology with 92 Localized Fast Radio Bursts and DESI BAO
• Current constraints on cosmological scenarios with very low reheating temperatures
• Generalized Hilltop Inflation
• Probing cosmic strings by reconstructing polarization rotation of the cosmic microwave background
• The Cross-correlation of KSZ Effect and 21 cm Intensity Mapping with Tidal Reconstruction
• Instrumental systematics biases in CMB lensing reconstruction: a simulation-based assessment
• Delensing the CMB with the cosmic infrared background: the impact of foregrounds
• Cosmological radiation density with non-standard neutrino-electron interactions
• Cosmological parameter forecasts by a joint 2D tomographic approach to CMB and galaxy clustering
• Several Problems in Particle Physics and Cosmology Solved in One SMASH
• Characterising cosmic birefringence in the presence of galactic foregrounds and instrumental systematic effects
• An Inpainting Approach to Tackle the Kinematic and Thermal SZ Induced Biases in CMB-Cluster Lensing Estimators
• Atacama Cosmology Telescope measurements of a large sample of candidates from the Massive and Distant Clusters of WISE Survey: Sunyaev-Zeldovich effect confirmation of MaDCoWS candidates using ACT
• LiteBIRD and CMB-S4 Sensitivities to Reheating in Plateau Models of Inflation
• Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey: I. Evidence for thermal energy anisotropy using oriented stacking
• The Simons Observatory 220 and 280 GHz Focal-Plane Module: Design and Initial Characterization
• Cosmology from weak lensing, galaxy clustering, CMB lensing and tSZ: I. 10x2pt Modelling Methodology
• Extended Analysis of Neutrino-Dark Matter Interactions with Small-Scale CMB Experiments
• The Impacts of Modeling Choices on the Inference of the Circumgalactic Medium Properties from Sunyaev-Zeldovich Observations
• Backlighting extended gas halos around luminous red galaxies: kinematic Sunyaev-Zel'dovich effect from DESI Y1 x ACT
• Primordial power spectrum at N3LO in effective theories of inflation
• Determination of Polarization Angles in CMB Experiments and Application to CMB Component Separation Analyses
• Velocity reconstruction in the era of DESI and Rubin (part I): Exploring spectroscopic, photometric & hybrid samples
• Gravitational wave constraints on the observable inflation
• Constraining gravity with a new precision $E_G$ estimator using Planck + SDSS BOSS
• The QCD Axion: Some Like It Hot
• Forecast constraints on Anisotropic Stress in Dark Energy using gravitational-waves
• Patchy Screening of the CMB from Dark Photons
• Cosmological Probes of Structure Growth and Tests of Gravity
• Improving constraints on primordial non-Gaussianity using neural network based reconstruction
• The Kinematic Sunyaev-Zel'dovich Effect with ACT, DES, and BOSS: a Novel Hybrid Estimator
• Robust and efficient CMB lensing power spectrum from polarization surveys
• Constraints on new physics around the MeV scale with cosmological observations
• The Atacama Cosmology Telescope: Systematic Transient Search of 3-Day Maps
• Revisiting progenitor-age dependence of type Ia supernova luminosity standardization process
• Impact of half-wave plate systematics on the measurement of cosmic birefringence from CMB polarization
• Real-world CMB lensing quadratic estimator power spectrum response
• Baryon Physics and Tight Coupling Approximation in Boltzmann Codes
• Importance of being nonminimally coupled: Scalar Hawking radiation from regular black holes
• QUBIC II: Spectro-Polarimetry with Bolometric Interferometry
• Improved Galactic Foreground Removal for B-Modes Detection with Clustering Methods
• Understanding matched filters for precision cosmology
• BeyondPlanck VI. Noise characterization and modelling
• Constraints on $f(R)$ and nDGP Modified Gravity Model Parameters with Cluster Abundances and Galaxy Clustering
• The Atacama Cosmology Telescope: limits on dark matter-baryon interactions from DR4 power spectra
• Target Neutrino Mass Precision for Determining the Neutrino Hierarchy
• A Generative Model of Galactic Dust Emission Using Variational Inference
• Quijote-PNG: The Information Content of the Halo Mass Function
• Machine Learning and Cosmology
• High-resolution CMB bispectrum estimator with flexible modal basis
• Full-sky beam convolution for cosmic microwave background applications
• Prospects for kSZ${}^2$-Galaxy Cross-Correlations during Reionization
• Transitioning from Stage-III to Stage-IV: Cosmology from galaxy$\times$CMB lensing and shear$\times$CMB lensing
• Testing scale-invariant inflation against cosmological data
• Primordial Black Holes and Scalar-induced Gravitational Waves in Radiative Hybrid Inflation
• Thomson scattering: One rate to rule them all
• Optimization of foreground moment deprojection for semi-blind CMB polarization reconstruction
• Accelerating cosmological inference with Gaussian processes and neural networks -- an application to LSST Y1 weak lensing and galaxy clustering
• Characterization of Transition Edge Sensors for the Simons Observatory
• Standard model Higgs field and hidden sector cosmology
• Probing Hot Gas Components of Circumgalactic Medium in Cosmological Simulations with the Thermal Sunyaev-Zel'dovich Effect
• The $R^2$-Higgs inflation: $R^3$ contribution and preheating after ACT and SPT data
• Cosmology from Cross-Correlation of ACT-DR4 CMB Lensing and DES-Y3 Cosmic Shear
• CMB lensing with shear-only reconstruction on the full sky
• Optimal Inflationary Potentials
• Super-sample covariance of the thermal Sunyaev-Zel'dovich effect
• M-theory Cosmology, Octonions, Error Correcting Codes
• CMB-HD: Astro2020 RFI Response
• Cosmology from the kinetic polarized Sunyaev Zel'dovich effect
• Constraining Cosmic Inflation with Observations: Prospects for 2030
• Violation of slow-roll in non-minimal inflation
• Brane inflation and the robustness of the Starobinsky inflationary model
• Low redshift calibration of the Amati relation using galaxy clusters
• Disentangling Doppler modulation, aberration and the temperature dipole in the CMB
• Back to the phase space: thermal axion dark radiation via couplings to standard model fermions
• Gravitational Wave from Axion-SU(2) Gauge Fields: Effective Field Theory for Kinetically Driven Inflation
• A new probe of the high-redshift Universe: nulling CMB lensing with interloper-free "LIM-pair" lensing
• Chasing cosmic inflation: constraints for inflationary models and reheating insights
• A numerical study of observational systematic errors in lensing analysis of CMB polarization
• Constraining CMB temperature evolution with Sunyaev-Zel'dovich galaxy clusters from the Atacama Cosmology Telescope
• The hunt for extraterrestrial high-energy neutrino counterparts
• Detectability of the cross-correlation between CMB lensing and stochastic GW background from compact object mergers
• Third-order corrections to the slow-roll expansion: calculation and constraints with Planck, ACT, SPT, and BICEP/Keck
• The Simons Observatory: A fully remote controlled calibration system with a sparse wire grid for cosmic microwave background telescopes
• Mitigating Foreground Bias to the CMB Lensing Power Spectrum for a CMB-HD Survey
• The Simons Observatory: the Large Aperture Telescope (LAT)
• How much primordial tensor mode is allowed?
• Analysis of NILC performance on B-modes data of sub-orbital experiments
• Asteroid Measurements at Millimeter Wavelengths with the South Pole Telescope
• Morphological Analysis of the Polarized Synchrotron Emission with WMAP and Planck
• Gravitational Waves From Dark Sectors, Oscillating Inflatons, and Mass Boosted Dark Matter
• Non-unitary three-neutrino mixing in the early Universe
• Requirements for future CMB satellite missions: photometric and band-pass response calibration
• A hybrid map-$C_{\ell }$ component separation method for primordial CMB $B$-mode searches
• Is patchy reionization an obstacle in detecting the primordial gravitational wave signal?
• Extragalactic CO emission lines in the CMB experiments: a forgotten signal and a foreground
• Hierarchical Bayesian CMB Component Separation with the No-U-Turn Sampler
• Inference of gravitational lensing and patchy reionization with future CMB data
• Investigation of CMB constraints for dark matter-helium scattering
• Probing parity-odd bispectra with anisotropies of GW $V$ modes
• An Examination of Galactic Polarization with Application to the Planck TB Correlation
• Cosmology with the thermal-kinetic Sunyaev-Zel'dovich effect
• ECLIPSE: a fast Quadratic Maximum Likelihood estimator for CMB intensity and polarization power spectra
• Revisiting signatures of thermal axions in nonstandard cosmologies
• Reconstructing Cosmic Polarization Rotation with ResUNet-CMB
• Efficient ILC analysis on polarization maps after EB leakage correction
• The star formation history in the last 10 billion years from CIB cross-correlations
• Primordial neutrinos and new physics: novel approach to solving neutrino Boltzmann equation
• Analytical model of the readout power and SQUID hysteresis parameter dependence of the resonator characteristics of microwave SQUID multiplexers
• Perfectly parallel cosmological simulations using spatial comoving Lagrangian acceleration
• CMB-S4 forecast on the primordial non-Gaussianity parameter of feature models
• Joint measurement of the galaxy cluster pressure profile with Planck and SPT-SZ
• Dark Radiation from the Primordial Thermal Bath in Momentum Space
• Large neutrino mass in cosmology and keV sterile neutrino dark matter from a dark sector
• Spin characterisation of systematics in CMB surveys -- a comprehensive formalism
• CMB polarization as a tool to constrain the optical properties of the Universe
• LiteBIRD Science Goals and Forecasts: A full-sky measurement of gravitational lensing of the CMB
• Exact joint likelihood of pseudo-$C_{\ell }$ estimates from correlated Gaussian cosmological fields
• CHANCES, the Chilean Cluster Galaxy Evolution Survey: Selection and initial characterisation of clusters and superclusters
• Fast computation of angular power spectra and covariances of high-resolution cosmic microwave background maps using the Toeplitz approximation
• Dark matter coupled to radiation: Limits from the Milky Way satellites
• Demonstration of 220/280 GHz Multichroic Feedhorn-Coupled TES Polarimeter
• Mitigating the impact of the CIB on galaxy cluster SZ detection with spectrally constrained matched filters
• Joint constraints on reionization: a framework for combining the global 21cm signal and the kinetic Sunyaev-Zel'dovich effect
• Probing early structure and model-independent neutrino mass with high-redshift CMB lensing mass maps
• Uncorrelated Compensated Isocurvature Perturbations from kSZ Tomography
• Fresh Look at Neutrino Self-Interactions With the Lyman-$\alpha$ Forest: Constraints from EFT and PRIYA Simulations
• Galaxy cluster rotation revealed in the MACSIS simulations with the kinetic Sunyaev-Zeldovich effect
• Neutrino mass constraints beyond linear order: cosmology dependence and systematic biases
• BeyondPlanck XVI. Limits on Large-Scale Polarized Anomalous Microwave Emission from Planck LFI and WMAP
• XLSSC 122 caught in the act of growing up: Spatially resolved SZ observations of a z=1.98 galaxy cluster
• Quintessential Inflation in Palatini Gravity
• Harmonic Hybrid Inflation
• Inflation and Dark Energy from spectroscopy at $z>2$
• Recovering Cosmic Microwave Background Polarization Signals with Machine Learning
• Flaring Stars in a Non-targeted mm-wave Survey with SPT-3G
• Painting baryons onto N-body simulations of galaxy clusters with image-to-image deep learning
• Impact of Anisotropic Birefringence on Measuring Cosmic Microwave Background Lensing
• Joint cosmology and mass calibration from tSZ cluster counts and cosmic shear
• Emulating Sunyaev-Zeldovich Images of Galaxy Clusters using Auto-Encoders
• Quantum Discrete Levels of the Universe from the Early Trans-Planckian Vacuum to the Late Dark Energy
• Generative models of astrophysical fields with scattering transforms on the sphere
• Constraining Holographic Dark Energy and Analyzing Cosmological Tensions
• Light Dark Matter Annihilation and Scattering in LHC Detectors
• Looking for a twist: probing the cosmological gravitomagnetic effect via weak lensing-kSZ cross correlations
• QUIJOTE Scientific Results -- VII. Galactic AME sources in the QUIJOTE-MFI Northern Hemisphere Wide-Survey
• Abundance and properties of dark radiation from the cosmic microwave background
• New insights on $\nu$-DM Interactions
• The Simons Observatory: Characterizing the Large Aperture Telescope Receiver with Radio Holography
• Cosmological Tests of Gravity: A Future Perspective
• Imprint of baryons and massive neutrinos on velocity statistics
• Optical modeling of systematic uncertainties in detector polarization angles for the Atacama Cosmology Telescope
• S.M.A.S.H.E.D.: Standard Model Axion Seesaw Higgs Inflation Extended for Dirac Neutrinos
• Modeling parity-violating spectra in Galactic dust polarization with filaments and its applications to cosmic birefringence searches
• Symmetrically Tuned Large-Volume Conic Shell-Cavities for Axion Searches
• Robust constraints on tensor perturbations from cosmological data: a comparative analysis from Bayesian and frequentist perspectives
• Using large scale structure data and a halo model to constrain Generalised Dark Matter
• LimberJack.jl: auto-differentiable methods for angular power spectra analyses
• Hypersensitive tunable Josephson escape sensor for gigahertz astronomy
• Free-Streaming Neutrinos and Their Phase Shift in Current and Future CMB Power Spectra
• Testing for spectral index variations in polarised CMB foregrounds
• Characterizing line-of-sight variability of polarized dust emission with future CMB experiments
• Zoology of Graviton non-Gaussianities
• Solar chameleons: Novel channels
• Gauge-Invariant Tensor Perturbations Induced from Baryon-CDM Relative Velocity and the B-mode Polarization of the CMB
• Precipitable water vapour measurement using GNSS data in the Atacama Desert for millimetre and submillimetre astronomical observations
• Searching for local features in primordial power spectrum using genetic algorithms
• Constraining the physics of star formation from CIB-cosmic shear cross-correlations
• Biases to primordial non-Gaussianity measurements from CMB secondary anisotropies
• Connecting Cosmic Inflation to Particle Physics with LiteBIRD, CMB-S4, EUCLID and SKA
• Probing Feedback in Galaxy Formation with Millimeter-wave Observations
• A representation learning approach to probe for dynamical dark energy in matter power spectra
• New Horizons in Cosmology with Spectral Distortions of the Cosmic Microwave Background
• Assembly development for the Simons Observatory focal plane readout module
• Radiative Plateau Inflation with Conformal Invariance: Dynamical Generation of Electroweak and Seesaw Scales
• Freeze-In of radiative keV-scale neutrino dark matter from a new $\text{U}(1{)}_{\text{B-L}}$
• The thermal and gravitational energy densities in the large-scale structure of the Universe
• High resolution tomography for galaxy spectroscopic surveys with angular redshift fluctuations
• Reconstruction with velocities
• Cosmology with the kinetic Sunyaev-Zeldovich effect: Independent of the optical depth and ${\sigma }_8$
• Is the formation of primordial black holes from single-field inflation compatible with standard cosmology?
• How new physics affects primordial neutrinos decoupling: Direct Simulation Monte Carlo approach
• Lensed CMB power spectrum biases from masking extragalactic sources
• Imprints of screened dark energy on nonlocal quantum correlations
• Theoretical and Experimental Challenges in the Measurement of Neutrino Mass
• New physics decaying into metastable particles: impact on cosmic neutrinos
• Information Theoretic Bounds on Cosmic String Detection in CMB Maps with Noise
• The skewness of the distance-redshift relation in $\Lambda$CDM
• Probing Dark Relativistic Species and Their Interactions with Dark Matter through CMB and 21cm surveys
• New Interpretations of the Cosmological Preference for a Negative Neutrino Mass
• An exploration of the properties of cluster profiles for the thermal and kinetic Sunyaev-Zel'dovich effects
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• Generative Models of Multi-channel Data from a Single Example -- Application to Dust Emission
• Natural Inflation with Exponentially Small Tensor-To-Scalar Ratio
• Absolute reference for microwave polarization experiments -- The COSMOCal project and its proof of concept
• Inverse-Compton Scattering of the Cosmic Infrared Background
• Improved Modeling of the Kinematic Sunyaev-Zel'dovich Projected-Fields signal and its Cosmological Dependence
• Boundless baryons: how diffuse gas contributes to anisotropic tSZ signal around simulated Three Hundred clusters
• $\mu$-Hybrid Inflation and Metastable Cosmic Strings in $\mathbf{SU}(3{)}_{\mathbf{c}}\times \mathbf{SU}(2{)}_{\mathbf{L}}\times \mathbf{SU}(2{)}_{\mathbf{R}}\times \mathbf{U}(1{)}_{\mathbf{B}-\mathbf{L}}$
• Running effects on QCD axion phenomenology
• Skewing the CMB$\times$LSS: a Fast Method for Bispectrum Analysis
• Introducing constrained matched filters for improved separation of point sources from galaxy clusters
• Remote Dipole Field Reconstruction with Dusty Galaxies
• Sound-Horizon-Agnostic Inference of the Hubble Constant and Neutrino Mass from BAO, CMB Lensing, and Galaxy Weak Lensing and Clustering
• B-mode constraints from Planck low multipole polarisation data
• Galaxy cluster SZ detection with unbiased noise estimation: an iterative approach
• Power Spectra of Slow-Roll inflation in the consistent $D\to 4$ Einstein-Gauss-Bonnet gravity
• Improving Constraints on Models Addressing the Hubble Tension with CMB Delensing
• The Simons Observatory: Development and Optical Evaluation of Achromatic Half-Wave Plates
• Gravitational waves, CMB polarization, and the Hubble tension
• Impact of nonlinear growth of the large-scale structure on CMB B-mode delensing
• Probing the Weak Gravity Conjecture in the Cosmic Microwave Background
• Analysis of Polarized Dust Emission Using Data from the First Flight of SPIDER
• Probing the origin of our Universe through cosmic microwave background constraints on gravitational waves
• A general framework to test gravity using galaxy clusters VI: Realistic galaxy formation simulations to study clusters in modified gravity
• Primordial Black Holes and Scalar-induced Gravitational Waves in Sneutrino Hybrid Inflation
• Constraints on the Optical Depth to Reionization from Balloon-Borne CMB Measurements
• Starobinsky inflation beyond the leading order
• $\tilde{\xi }$-attractors in metric-affine gravity
• Pairwise kSZ signal extraction efficacy and optical depth estimation
• Impact of Galactic dust non-Gaussianity on searches for B-modes from inflation
• Forecast of cross-correlation of CSST cosmic shear tomography with AliCPT-1 CMB lensing
• Large and small field inflation from hyperbolic sigma models
• Bounds on Velocity-Dependent Dark Matter-Baryon Scattering from Large-Scale Structure
• Probing helium reionization with kinetic Sunyaev Zel'dovich tomography
• Challenges in Constraining Gravity with Cosmic Voids
• Exact CMB B-mode power spectrum from anisotropic cosmic birefringence
• The velocity structure of the intracluster medium during a major merger: simulated microcalorimeter observations
• Selecting samples of galaxies with fewer Fingers-of-God
• The reconstructed CMB lensing bispectrum
• Foreground removal with ILC methods for AliCPT-1
• Probing departures from $\Lambda$CDM by late-time datasets
• Dynamics of metastable Standard Model particles from long-lived particle decays in the MeV primordial plasma
• Imprint of massive neutrinos on Persistent Homology of large-scale structure
• Computing Microwave Background Polarization Power Spectra from Cosmic Birefringence
• eV Hubble Scale Inflation with Radiative Plateau: Very light Inflaton, Reheating & Dark Matter in B-L Extensions
• The effect of quantum decoherence on inflationary gravitational waves
• Cross-correlation of POLARBEAR CMB Polarization Lensing with High-$z$ Sub-mm Herschel-ATLAS galaxies
• Cold Dark Matter Based on an Analogy with Superconductivity
• A power spectrum approach to the search for Axion-like Particles from resolved galaxy clusters using CMB as a backlight
• Finding Evidence for Inflation and the Origin of Galactic Magnetic Fields with CMB Surveys
• Impact of half-wave plate systematics on the measurement of CMB $B$-mode polarization
• The Atacama Cosmology Telescope: DR6 Power Spectrum Foreground Model and Validation
• Dynamical Inflection Point Inflation
• Material survey for millimeter-wave absorber using 3-D printed mold
• Correlations of Dark Matter, Gas and Stellar Profiles in Dark Matter Halos
• A general framework to test gravity using galaxy clusters V: A self-consistent pipeline for unbiased constraints of $f(R)$ gravity
• Understanding large scale CMB anomalies with the generalized non-minimal derivative coupling during inflation
• The HalfDome Multi-Survey Cosmological Simulations: N-body Simulations
• Impact of freeze-in on dark matter isocurvature
• Searching for dilaton fields in the Ly$\alpha$ forest
• Radiative Symmetry breaking, Cosmic Strings and Observable Gravity Waves in $U(1{)}_R$ symmetric $SU(5)\times U(1{)}_{\chi }$
• A framework to mitigate patchy reionization contamination on the primordial gravitational wave signal
• An Analytical Study of the Primordial Gravitational-Wave-Induced Contribution to the Large-Scale Structure of the Universe
• The cosmological collider in $R^2$ inflation
• Scalar Dark Energy Models and Scalar-Tensor Gravity: Theoretical Explanations for the Accelerated Expansion of Present Universe
• Inference of the optical depth to reionization $\tau$ from $\text{Planck}$ CMB maps with convolutional neural networks
• Strong cosmological constraints on the neutrino magnetic moment
• Accurate estimation of angular power spectra for maps with correlated masks
• Cuscuton Bounce Beyond the Linear Regime: Bispectrum and Strong Coupling Constraints
• Prospects and Limitations for Constraining Light Relics with Primordial Abundance Measurements
• Measurement and Modeling of Polarized Atmosphere at the South Pole with SPT-3G
• Improving Constraints on Fundamental Physics Parameters with the Clustering of Sunyaev-Zeldovich Selected Galaxy Clusters
• Non-parametric maximum likelihood component separation for CMB polarization data
• Anatomy of Parity-violating Trispectra in Galaxy Surveys
• Revisiting model-independent constraints on spatial curvature and cosmic ladders calibration: updated and forecast analyses
• Crosstalk effects in microwave SQUID multiplexed TES bolometer readout
• Addressing the $H_0$ tension through matter with pressure and no early dark energy
• The Atacama Cosmology Telescope: Delensed Power Spectra and Parameters
• A Simulation-Based Method for Correcting Mode Coupling in CMB Angular Power Spectra
• Consistency of CMB experiments beyond cosmic variance
• Growth and Geometry Split in Light of the DES-Y3 Survey
• Cosmology Large Angular Scale Surveyor (CLASS): 90 GHz Telescope Pointing, Beam Profile, Window Function, and Polarization Performance
• Forecast of foreground cleaning strategies for AliCPT-1
• The primordial information content of Rayleigh Anisotropies
• A new "temperature inversion" estimator to detect CMB patchy screening by large-scale structure
• A Diffused Background from Axion-like Particles in the Microwave Sky
• Thermal emission from the amorphous dust: An alternative possibility of the origin of the anomalous microwave emission
• Fast scalar quadratic maximum likelihood estimators for the CMB B-mode power spectrum
• Fast and Flexible Neutrino Decoupling Part I: The Standard Model
• Prospects for disentangling dark matter with weak lensing
• Constraints on ultra-low-frequency gravitational waves with statistics of pulsar spin-down rates
• Astro2020 Decadal Science White Paper: The state of gravitational-wave astrophysics in 2020
• Predicting CMB dust foreground using galactic 21 cm data
• The Atacama Cosmology Telescope: Flux Upper Limits from a Targeted Search for Extragalactic Transients
• Looking beyond lambda
• Suppressing the thermal SZ-induced variance in CMB-cluster lensing estimators
• A forecast of the sensitivity on the measurement of the optical depth to reionization with the GroundBIRD experiment
• Simons Observatory Focal-Plane Module: In-lab Testing and Characterization Program
• Controlling systematics in ground-based CMB surveys with partial boresight rotation
• Total power horn-coupled 150 GHz LEKID array for space applications
• Constraining Cosmology With the CMB $\times$ LIM-Nulling Convergence
• On the contributions of extragalactic CO emission lines to ground-based CMB observations
• Measuring cosmic filament spin with the kinetic Sunyaev-Zel'dovich effect
• A New Probe of the High-z BAO scale: BAO tomography With CMB $\times$ LIM-Nulling Convergence
• Enhancing Cosmological Model Selection with Interpretable Machine Learning
• Exploring Early and Late Cosmology with Next Generation Surveys
• Probing light relics through cosmic dawn
• Relic Cosmological Vector Fields and Inflationary Gravitational Waves
• Inpainting hydrodynamical maps with deep learning
• Cluster profiles from beyond-the-QE CMB lensing mass maps
• Brane inflation driven by an arctan potential: CMB constraints and Reheating
• Non-thermal Sunyaev-Zeldovich signal from radio galaxy lobes
• AI for Scientific Discovery is a Social Problem
• Effective Field Theory of Chiral Gravitational Waves
• CMB Shadows: The Effect of Interstellar Extinction on Cosmic Microwave Background Polarization and Temperature Anisotropy
• Predictive Dirac and Majorana Neutrino Mass Textures from $SU(6)$ Grand Unified Theories
• Tomographic constraint on anisotropic cosmic birefringence
• Current and Future constraints on single-field $\alpha$-Attractor model
• Quantum Trans-Planckian Physics inside Black Holes and its Spectrum
• Constraints on cosmic birefringence using $E$-mode polarisation
• Cosmoglobe DR1. III. First full-sky model of polarized synchrotron emission from all WMAP and Planck LFI data
• Big Bang Nucleosynthesis and Neutrino Cosmology
• The Integration and Testing Program for the Simons Observatory Large Aperture Telescope Optics Tubes
• MAPPRAISER: A massively parallel map-making framework for multi-kilo pixel CMB experiments
• Cross-correlation between soft X-rays and galaxies A new benchmark for galaxy evolution models
• Unified dark fluid with null sound speed as an alternative to phantom dark energy
• The Simons Observatory: Assessing the Impact of Dust Complexity on the Recovery of Primordial $B$-modes
• Demonstration of a 1820 channel multiplexer for transition-edge sensor bolometers
• Sensitivity of the Global 21-cm Signal to Dark Matter-Baryon Scattering
• PROTOCALC, A W-band polarized calibrator for CMB Telescopes: application to Simons Observatory and CLASS
• Investigating the Origin of CMB Large-Scale Features Using LiteBIRD and CMB-S4
• Massive $\nu$s through the CNN lens: interpreting the field-level neutrino mass information in weak lensing
• Cosmological Parameter Estimation with a Joint-Likelihood Analysis of the Cosmic Microwave Background and Big Bang Nucleosynthesis
• Clocking the End of Cosmic Inflation
• Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Resolving the Hot and Ionized Universe through the Sunyaev-Zeldovich effect
• Cosmic Neutrino Decoupling and its Observable Imprints: Insights from Entropic-Dual Transport
• A measurement of cluster masses using Planck and SPT-SZ CMB lensing
• Supersymmetric Hybrid Inflation in Light of CMB Experiments and Swampland Conjectures
• Coherent states of quantum spacetimes for black holes and de Sitter spacetime
• Observational Constraints on Extended Starobinsky and Weyl Gravity Model of Inflation
• Relaxing cosmological constraints on current neutrino masses
• Identifying frequency decorrelated dust residuals in B-mode maps by exploiting the spectral capability of bolometric interferometry
• A Constrained NILC method for CMB B mode observations
• Lensing reconstruction from the cosmic microwave background polarization with machine learning
• Transverse velocities and matter gradient correlations: a new signal and a new challenge to moving-lens analyses
• Unraveling the CMB lack-of-correlation anomaly with the cosmological gravitational wave background
• New probe of inflationary gravitational waves: cross-correlations of lensed primary CMB B-modes with large-scale structure
• The Simons Observatory: Beam characterization for the Small Aperture Telescopes
• Scale-invariant inflation
• Tilted non-spatially-flat inflation
• MeV Dark Matter with MeV Dark Photons in Abelian Kinetic Mixing Theories
• Dark Energy with a Triplet of Classical U(1) Fields
• Numerical solution of the exact background collisional Boltzmann equation for dark matter-baryon scattering
• Blind Map Level Systematics Cleaning: A Quadratic Estimator Approach
• The Statistics of Extended Debris Disks Measured with Gaia and Planck
• The T-E correlation coefficient of Planck legacy data
• CMB-HD: An Ultra-Deep, High-Resolution Millimeter-Wave Survey Over Half the Sky
• The Simons Observatory: Project Overview
• $\Lambda$CDM and early dark energy in latent space: a data-driven parametrization of the CMB temperature power spectrum
• Introducing the Descriptive Parametric Model: Gaseous Profiles for Galaxies, Groups, and Clusters
• Non-Gaussianities as a Signature of Quantumness of Quantum Cosmology
• The Power of the Cosmic Web
• Doppler boosted dust emission and CIB-galaxy cross-correlations: a new probe of cosmology and astrophysics
• Scale and redshift dependent limits on cosmic neutrino properties
• Signature of Massive Neutrinos from the Clustering of Critical Points. I. Density-threshold-based Analysis in Configuration Space
• Conversations in the dark: cross-correlating birefringence and LSS to constrain axions
• Characterization of Extragalactic Point-Sources on E- and B-mode Maps of the CMB Polarization
• The Atacama Cosmology Telescope: SZ-based masses and dust emission from IR-selected cluster candidates in the SHELA survey
• Calibrating baryonic effects in cosmic shear with external data in the LSST era
• A search for super-imposed oscillations to the primordial power spectrum in Planck and SPT-3G 2018 data
• The Simons Observatory: impact of bandpass, polarization angle and calibration uncertainties on small-scale power spectrum analysis
• Examining statistical isotropy of CMB low multipoles from Planck PR4 data
• Constraining the average magnetic field in galaxy clusters with current and upcoming CMB surveys
• Cool dark sector, concordance, and a low ${\sigma }_8$
• Structure Formation in Dark Matter Particle Production Cosmology
• Primordial black holes save $R^2$ inflation
• Determining our peculiar velocity from the aberration in the cosmic microwave background
• Cosmic variance mitigation in measurements of the integrated Sachs-Wolfe effect
• The Simons Observatory: Magnetic Shielding Measurements for the Universal Multiplexing Module
• Classifying CMB time-ordered data through deep neural networks
• A flexible parameterization to test early physics solutions to the Hubble tension with future CMB data
• Return of the Lepton Number: Sterile Neutrino Dark Matter Production and the Revival of the Shi-Fuller Mechanism
• Constraining cosmology with thermal Sunyaev-Zel'dovich maps: Minkowski functionals, peaks, minima, and moments
• The radio SZ effect as a probe of the cosmological radio background
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• The parity-odd Intrinsic Bispectrum
• Beware of the running $n_s$ when producing heavy primordial black holes
• Breaking the degeneracy between polarization efficiency and cosmological parameters in CMB experiments
• YOLO-CL cluster detection in the Rubin/LSST DC2 simulation
• Constraints on primordial non-Gaussianity from Quaia
• QUIJOTE scientific results -- XVIII. New constraints on the polarization of the Anomalous Microwave Emission in bright Galactic regions: $\rho$\,Ophiuchi, Perseus and W43
• Modelling TES non-linearity induced by a rotating HWP in a CMB polarimeter
• Constraining primordial tensor features with the anisotropies of the Cosmic Microwave Background
• Beyond Fisher Forecasting for Cosmology
• Novel Cosmological Tests from Combining Galaxy Lensing and the Polarized Sunyaev-Zel'dovich Effect
• A short review on Quintom dark energy theory
• Improving CMB constraints on early Universe physics with LSS: A multi-probe forecast including cross-covariance
• Measuring lensing ratios with future cosmological surveys
• Limits on Polarized Dust Spectral Index Variations for CMB Foreground Analysis
• Maximum likelihood kinetic Sunyaev Zel'dovich velocity reconstruction
• Precision calculation of $N_{\text{eff}}$ with Neutrino Direct Simulation Monte Carlo
• A quasi-matter bounce equivalent to Starobinsky inflation
• Cosmic Census: Relative Distributions of Dark Matter, Galaxies and Diffuse Gas
• Detecting deviations from Gaussianity in high-redshift CMB lensing maps
• Self-supervised component separation for the extragalactic submillimeter sky
• Galactic foreground constraints on primordial $B$-mode detection for ground-based experiments
• Cross-correlating radial peculiar velocities and CMB lensing convergence
• Model independent variance cancellation in CMB lensing cross-correlations
• Cosmology with Planck T-E correlation coefficient
• The impact of halo concentration on the Sunyaev Zel'dovich effect signal from massive galaxy clusters
• Prospects for studying the mass and gas in protoclusters with future CMB observations
• Effects of boosting on extragalactic components: methods and statistical studies
• The Hydrogen Intensity and Real-time Analysis eXperiment: 256-Element Array Status and Overview
• Projected two- and three-point statistics: Forecasts and mitigation of non-linear RSDs
• The Simons Observatory: Large-Scale Characterization of 90/150 GHz TES Detector Modules
• Anti-reflection coating with mullite and Duroid for large-diameter cryogenic sapphire and alumina optics
• Interacting light thermal-relic dark matter: self-consistent cosmological bounds
• kSZ Pairwise Velocity Reconstruction with Machine Learning
• Impact of Dark Sector Preheating on CMB Observables
• Smooth $\mu$-Hybrid and Non-Minimal Higgs Inflation in $SU(4{)}_C\times SU(2{)}_L\times SU(2{)}_R$ With Observable Gravitational Waves
• Consequences of constant elevation scans for instrumental systematics in Cosmic Microwave Background Experiments
• The Gravitational Lensing Imprints of DES Y3 Superstructures on the CMB: A Matched Filtering Approach
• Probing Inflation with Precision Bispectra
• Improved Gibbs samplers for Cosmic Microwave Background power spectrum estimation
• The Moving Lens Effect: Simulations, Forecasts and Foreground Mitigation
• SpectrAx: Spectral Search of Axion-Like Particles Using Multi-Band Observations of Galaxy Clusters from SKA, SO, CMB-S4 and eROSITA
• The Atacama Cosmology Telescope: Quantifying Atmospheric Emission above Cerro Toco
• Reconstructing inflationary potential from NANOGrav 15-year Data: A robust study using Non-Bunch Davies initial condition
• A Novel Bispectrum Estimator of the Kinematic Sunyaev-Zel'dovich Effect using Projected Fields
• Stage IV CMB forecasts for warm inflation
• Filtering in CMB data analysis with application to ACT DR4 and Planck observations
• Towards a multi-tracer neutrino mass measurement with line-intensity mapping
• ForSE+: Simulating non-Gaussian CMB foregrounds at 3 arcminutes in a stochastic way based on a generative adversarial network
• The Simons Observatory: Studies of Detector Yield and Readout Noise From the First Large-Scale Deployment of Microwave Multiplexing at the Large Aperture Telescope
• The Simons Observatory: Design, Optimization, and Performance of Low Frequency Detectors
• The Simons Observatory: Validation of reconstructed power spectra from simulated filtered maps for the Small Aperture Telescope survey
• Neural Network Reconstruction of Non-Gaussian Initial Conditions from Dark Matter Halos
• Improving Cosmic Birefringence Constraints via Delensing
• Impact of Galactic non-Gaussian foregrounds on CMB lensing measurements
• Natural inflation in Palatini $F(R,X)$
• Curvature perturbations from kinetic preheating after $\alpha$-attractor inflation
• CMB polarization analysis on circular scans
• The Atacama Cosmology Telescope: Systematic Transient Search of Single Observation Maps
• Small Correlated Against Large Estimator (SCALE) for Cosmic Microwave Background Lensing
• The Simons Observatory: Design and Measured Performance of a Carbon Fiber Strut for a Cryogenic Truss
• Magnetic Fields in the Shapley Supercluster Core with POSSUM: Challenging Model Predictions
• From Dark Radiation to Dark Energy: Unified Cosmological Evolution in K-essence Models
• Aemulus $\nu$: Precision halo mass functions in w$\nu$CDM cosmologies
• Delensing for Precision Cosmology: Optimizing Future CMB B-mode Surveys to Constrain r
• Direct correlation of line intensity mapping and CMB lensing from evolution along the lightcone
• Observations of compact sources in galaxy clusters using MUSTANG2
• Mapping luminous and dark matter in the Universe
• Probing Primordial Symmetry Breaking with Cosmic Microwave Background Anisotropy
• Cosmological Implications of a Neutrino Mass Detection
• Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics
• Turbulence Induced Non-Gaussian Spectral Distortion in the Microwave Sky from Photon-Axion Conversion in Galaxy Clusters
• On Gauge Theories of Neutrino Masses and Dark Matter
• CMB delensing with deep learning
• Results and forecasts on cosmic inflation from weak lensing
• Vibration characteristics of a continuously rotating superconducting magnetic bearing and potential influence to TES and SQUID
• Constraining the primordial power spectrum using a differentiable likelihood
• Breaking degeneracies with the Sunyaev-Zeldovich full bispectrum
• Accelerating spherical harmonic transforms for a large number of sky maps
• Signatures of Solar Chameleons in the Earth's Magnetic Field
• Fast map-based simulations of systematics in CMB surveys including effects of the scanning strategy
• The Circumgalactic Medium from the CAMELS Simulations: Forecasting Constraints on Feedback Processes from Future Sunyaev-Zeldovich Observations
• Spinning Guest Fields during Inflation: Leftover Signatures
• The LSPE-Strip Pointing Reconstruction and Star Tracker
• Sensitive 3mm Imaging of Discrete Sources in the Fields of tSZ-Selected Galaxy Clusters
• Post-inflationary production of particle Dark Matter: Hilltop and Coleman-Weinberg inflation
• Characterizing Extra-solar Oort Clouds with Submillimeter-wave Observations
• Forecasts of effects of beam systematics and deprojection on the third-generation ground-based cosmic microwave background experiment
• Improved cosmological constraints on axion-lepton interactions
• Dark matter search with CMB: a study of foregrounds
• E and B modes of the CMB y-type distortions: polarised kinetic Sunyaev-Zeldovich effect from the reionisation and post-reionisation eras
• Energy Recovery System for Large Telescopes
• The Atacama Cosmology Telescope: A Test of the Gravitational Force Law on Cosmological Scales Using the Kinematic Sunyaev-Zeldovich Effect
• Polarization fraction of Planck Galactic cold clumps and forecasts for the Simons Observatory
• Stirring the cosmic pot: how black hole feedback shapes the matter power spectrum in the Fable simulations
• Estimators for the cross-pairwise kSZ effect: forecasts for the dark energy and modified gravity parameters with Simons Observatory and CMB-S4
• Distinguishing Primordial Magnetic Fields from Inflationary Tensor Perturbations in the Cosmic Microwave Background
• Nonminimal Couplings and the Forgotten Field of Axion Inflation
• Cosmic Strings-induced CMB anisotropies in light of Weighted Morphology
• A measurement of atmospheric circular polarization with POLARBEAR
• The intrinsic bispectrum of the CMB from isocurvature initial conditions
• (P)reheating Effects of the Kähler Moduli Inflation I Model
• The non-thermal secondary CMB anisotropies from a cosmic distribution of radio galaxy lobes
• New tests of dark sector interactions from the full-shape galaxy power spectrum
• Estimating the Impact of foregrounds on the Future Detection of Rayleigh scattering
• Correlating Visual Characteristics and Cryogenic Performance of Superconducting Detectors
• Searching for Extremal Spots in Planck Lensing Maps
• The Simons Observatory: Differentiating Thermal and Optical Effects in Superconducting Transition-Edge Sensing Bolometers
• Dissecting the Thermal SZ Power Spectrum by Halo Mass and Redshift in SPT-SZ Data and Simulations
• Systematic effects on the upcoming NIKA2 LPSZ scaling relation
• A Closer Look in the Mirror: Reflections on the Matter/Dark Matter Coincidence
• Refitting cosmological data with neutrino mass and degeneracy
• Implications of scattering for CMB foreground emission modelling
• The Simons Observatory: A Minimum-Cost Matching Algorithm for Pairing Measured Resonances with Designed Detectors
• High-Efficiency and Low-Noise Detectors for the Upgraded CLASS 90 GHz Focal Plane
• Strongly-interacting massive particle and dark photon in the era of intensity frontier
• Revisiting the Chern-Simons interaction during inflation with a non-canonical pseudo-scalar
• Optimizing the hunt for extraterrestrial high-energy neutrino counterparts
• Cosmic topology. Part IIIb. Eigenmodes and correlation matrices of spin-2 perturbations in orientable Euclidean manifolds
• Big Bang Nucleosynthesis as a probe of non-standard neutrino interactions and non-unitary three-neutrino mixing
• Atacama Cosmology Telescope: Observations of supermassive black hole binary candidates. Strong sinusoidal variations at 95, 147 and 225 GHz in PKS 2131$-$021 and PKS J0805$-$0111
• Cluster optical depth and pairwise velocity estimation using machine learning
• Axion Dark Matter Archaeology with Primordial Gravitational Waves
• Forecasting Constraints on Non-Thermal Light Massive Relics from Future CMB Experiments (CMB-S4/Simons Observatory)
• Requirements on bandpass resolution and measurement precision for LiteBIRD
• Power Spectrum Emulators from Neural Networks and Tree-Based Methods
• Measuring the Hubble Constant Near and Far in the Era of ELT's
• LiteBIRD science goals and forecasts: improved full-sky reconstruction of the gravitational lensing potential through the combination of Planck and LiteBIRD data
• Delensing CMB B-modes using galaxy surveys: the effect of galaxy bias and matter clustering non-linearities
• Bias in the tensor-to-scalar ratio from self-interacting dark radiation
• Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future
• Unbiased Primordial Gravitational Wave Inference from the CMB with SMICA
• Constraining Power of Wavelet vs. Power Spectrum Statistics for CMB Lensing and Weak Lensing with Learned Binning
• Machine Learning-Driven Analysis of kSZ Maps to Predict CMB Optical Depth $\tau$
• Constraints on the normal branch of DGP gravity from SPT galaxy clusters with DES and HST weak-lensing mass calibration and from Planck PR4 CMB anisotropies
• Axions at the meV Crossroads: Theory, Cosmology, Astrophysics, and Experiments
• Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization
• Constraining primordial non-Gaussianity using Neural Networks
• Thermal Sunyaev-Zeldovich measurements and cosmic infrared background leakage mitigation combining upcoming ground-based telescopes
• Detection likelihood of cluster-induced CMB polarization
• Enabling Discoveries: Thirty Years of Advanced Technologies and Instrumentation at the National Science Foundation
• Information content in mean pairwise velocity and mean relative velocity between pairs in a triplet
• The Atacama Cosmology Telescope: A demonstration of CMB lensing measurement from daytime data
• Foreground Mitigation for CMB Lensing with the Global Minimum Variance Quadratic Estimator
• QUIJOTE-TFGI polarization calibration -- Ground characterization and on-sky validation with Tau A and the Moon
• The frame-dragging vector potential on galaxy scales from Dark-Matter-only Newtonian $N$-body simulations
• Bias on Tensor-to-Scalar Ratio Inference With Estimated Covariance Matrices
• Controlled Tension Forecasting: Quantifying Cross-Probe Biases in ${\omega }_0{\omega }_a$CDM
• Cosmic Collider Gravitational Waves sourced by Right-handed Neutrino production from Bubbles: Testing Seesaw, Leptogenesis and Dark Matter
• Constraining the inflaton potential with gravitational waves from oscillons
• Reheating in geometric Weyl-invariant Einstein-Cartan gravity
• The Hydrostatic Mass Bias and the ${\sigma }_8$ Tension: A Multi-Probe Forecast for Stage-IV/V Surveys
• Beyond thermal approximations: Precise cosmological bounds on Axion-Like Particles
• Accurate and efficient likelihood modeling for large-scale CMB data
• ABCMB: A Python+JAX Package for the Cosmic Microwave Background Power Spectrum
• Fast computation of temperature and polarization coupling matrices
• Intracluster Medium Fluctuations on Scales up to 1 Mpc: A Combined eROSITA and SPT/Planck Analysis of Abell 3266
• Cosmological gravity on all scales V: MCMC forecasts combining large scale structure and CMB lensing for binned phenomenological modified gravity
• CCAT-prime: Characterization of the First 280 GHz MKID Array for Prime-Cam
• Cold vs. Hot Gas Accretion and Angular Momentum in FIRE Simulations: From Halo to Galaxy Scales
• The hidden circumgalactic medium
• AliCPT Sensitivity to Cosmic Reheating
• Extending Galactic foreground emission with neural networks
• The Simons Observatory: Quantifying the impact of beam chromaticity on large-scale B-mode science
• Probing CMB Polarization Gaussianity with the Statistics of Unpolarized Points: Non-Gaussianity of Planck Data and Prospects for Future B-Mode Measurements
• Quantum measurement systems and applications to particle physics and cosmology
• Understanding galaxy formation and evolution through an all-sky submillimetre spectroscopic survey
• Cosmological radiation density with non-standard neutrino-electron interactions
• The Atacama Cosmology Telescope: Machine Learning Driven Tools for Detecting Millimeter Sources in Timestream Pre-processing
• CMB lensing tomography with clustering estimation of lens redshift distributions
• The Simons Observatory: laboratory beam characterization for the first small aperture telescope
• Chern-Simons gravitational term coupled to a spectator field
• The Simons Observatory: Design, Integration, and Current Status of Small Aperture Telescopes
• Impact of particle production during inflation on the CMB detection
• BrahMap: A scalable and modular map-making framework for the CMB experiments
• Non-Gaussianity from explicit $U(1)$-breaking interactions
• Systematic effects on lensing reconstruction from a patchwork of CMB polarization maps
• Towards detecting Primordial non-Gaussianity in the CMB using Spherical Convolutional Neural Networks
• The case for an all-sky millimetre survey at sub-arcminute resolution
• Impact of the calibration of the Halo Mass Function on galaxy cluster number count cosmology
• The Bias to Cosmic Microwave Background Lensing Reconstruction from the Kinematic Sunyaev-Zel'dovich Effect at Reionization
• Running the small-correlated-against-large estimator at scale: Applications of small-scale CMB lensing estimators on realistic simulations
• Mitigating Cosmic Microwave Background Shadow Degradation of Tensor-to-scalar Ratio Measurements through Map-based Studies
• Forecasting Galaxy Cluster HI Mass Recovery with CHIME at Redshifts z = 1 and 2 via the IllustrisTNG Simulations
• Imprints of light dark matter on the evolution of cosmic neutrinos
• Wide Field High Cadence CMB Survey Designs for Chilean Telescopes
• Extragalactic astrophysics with next-generation CMB experiments
• The Atacama Cosmology Telescope: Extragalactic Point Sources in the Southern Surveys at 150, 220 and 280 GHz observed between 2008-2010
• Cosmology with the Roman Space Telescope -- Synergies with CMB lensing
• Multi-frequency point source detection with fully convolutional networks: Performance in realistic microwave sky simulations
• Optimal map-making with singularities
• Testing magnetic interference between TES detectors and the telescope environment for future CMB satellite missions
• Secondary CMB anisotropies from magnetized halos --I: Power spectra of the Faraday rotation angle and conversion rate
• A new approach of estimating the Galactic thermal dust and synchrotron polarized emission template in the microwave bands
• Polarization angle requirements for CMB B-mode experiments. Application to the LiteBIRD satellite
• Finite inflation in curved space
• The Simons Observatory: HoloSim-ML: machine learning applied to the efficient analysis of radio holography measurements of complex optical systems
• Mitigating point-source contamination in CMB polarization: a Generalized Point Spread Function fitting approach
• Feedback-Controlled Beam Pattern Measurement Method Using a Power-Variable Calibration Source for Cosmic Microwave Background Telescopes
• A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
• The Simons Observatory: Studies of Phase Drift in RF Transmission Lines from the First Large-Scale Deployment of Microwave Frequency Multiplexing for Cosmology
• Time-dependent deflection reconstruction: new technique to search for gravitational waves with the cosmic microwave background
• Identifying changing jets through their radio variability
• A general framework for unbiased tests of gravity using galaxy clusters
• How to embed any likelihood into SBI: Application to Planck + Stage IV galaxy surveys and Dynamical Dark Energy
• Beyond general relativity: gravitational waves in non-minimally coupled theories
• Forecasting ground-based sensitivity to the Rayleigh scattering of the CMB in the presence of astrophysical foregrounds
• High-precision polarization measurements with Lumped Element Kinetic Inductance Detectors