Efficient Computation of CMB anisotropies in closed FRW models | Paper Citation Record

Observation db2d2a07-96d0-45e7-bf46-cb3af442903e · inbound

The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes cites this paper.

The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes Efficient Computation of CMB anisotropies in closed FRW models

Reference 3

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Planck 2018 results. VI. Cosmological parameters cites this paper.

Planck 2018 results. VI. Cosmological parameters Efficient Computation of CMB anisotropies in closed FRW models

Reference 221

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The angular scale of homogeneity in the Local Universe with the SDSS blue galaxies cites this paper.

The angular scale of homogeneity in the Local Universe with the SDSS blue galaxies Efficient Computation of CMB anisotropies in closed FRW models

Reference 34

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Cosmological constraints in extended parameter space from the Planck 2018 Legacy release cites this paper.

Cosmological constraints in extended parameter space from the Planck 2018 Legacy release Efficient Computation of CMB anisotropies in closed FRW models

Reference 65

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Toward a robust inference method for the galaxy bispectrum: likelihood function and model selection cites this paper.

Toward a robust inference method for the galaxy bispectrum: likelihood function and model selection Efficient Computation of CMB anisotropies in closed FRW models

Reference 29

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Probing the independence within the dark sector in the fluid approximation cites this paper.

Probing the independence within the dark sector in the fluid approximation Efficient Computation of CMB anisotropies in closed FRW models

Reference 106

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Fractional Dark Matter decay: cosmological imprints and observational constraints cites this paper.

Fractional Dark Matter decay: cosmological imprints and observational constraints Efficient Computation of CMB anisotropies in closed FRW models

Reference 71

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Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions cites this paper.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Efficient Computation of CMB anisotropies in closed FRW models

Reference 284

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Gravitational waves, CMB polarization, and the Hubble tension cites this paper.

Gravitational waves, CMB polarization, and the Hubble tension Efficient Computation of CMB anisotropies in closed FRW models

Reference 64

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Reionization optical depth determination from Planck HFI data with ten percent accuracy cites this paper.

Reionization optical depth determination from Planck HFI data with ten percent accuracy Efficient Computation of CMB anisotropies in closed FRW models

Reference 24

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Modelling the matter bispectrum at small scales in modified gravity cites this paper.

Modelling the matter bispectrum at small scales in modified gravity Efficient Computation of CMB anisotropies in closed FRW models

Reference 121

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Cobaya: Code for Bayesian Analysis of hierarchical physical models cites this paper.

Cobaya: Code for Bayesian Analysis of hierarchical physical models Efficient Computation of CMB anisotropies in closed FRW models

Reference 12

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Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing cites this paper.

Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing Efficient Computation of CMB anisotropies in closed FRW models

Reference 179

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Galaxy and halo angular clustering in LCDM and Modified Gravity cosmologies cites this paper.

Galaxy and halo angular clustering in LCDM and Modified Gravity cosmologies Efficient Computation of CMB anisotropies in closed FRW models

Reference 65

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Observation b0416f81-680b-439f-8e6d-f5d4ade1d1c3 · inbound

CMB power spectra and cosmological parameters from Planck PR4 with CamSpec cites this paper.

CMB power spectra and cosmological parameters from Planck PR4 with CamSpec Efficient Computation of CMB anisotropies in closed FRW models

Reference 1

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The Hubble Tension and Early Dark Energy cites this paper.

The Hubble Tension and Early Dark Energy Efficient Computation of CMB anisotropies in closed FRW models

Reference 100

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Observation 66f8361a-cb8e-47ee-8f74-78bb86386b7e · inbound

DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations cites this paper.

DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations Efficient Computation of CMB anisotropies in closed FRW models

Reference 178

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Observation 2446ef6a-84bb-4d30-94c8-6890737f8731 · inbound

MUltiplexed Survey Telescope (MUST) Science White Paper I: Overview of Large-Scale Structure Cosmology in the Era of Stage-V Spectroscopic Surveys cites this paper.

MUltiplexed Survey Telescope (MUST) Science White Paper I: Overview of Large-Scale Structure Cosmology in the Era of Stage-V Spectroscopic Surveys Efficient Computation of CMB anisotropies in closed FRW models

Reference 287

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Observation 81a74cc2-647c-45e2-8a4e-6495420c451e · inbound

Constraints on local primordial non-Gaussianity with 3d Velocity Reconstruction from the Kinetic Sunyaev-Zeldovich Effect cites this paper.

Constraints on local primordial non-Gaussianity with 3d Velocity Reconstruction from the Kinetic Sunyaev-Zeldovich Effect Efficient Computation of CMB anisotropies in closed FRW models

Reference 45

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The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes cites this paper.

The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes Efficient Computation of CMB anisotropies in closed FRW models

Reference 90

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Observation aa600f37-91f1-4b57-bac5-bc727cd97f84 · inbound

DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements cites this paper.

DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements Efficient Computation of CMB anisotropies in closed FRW models

Reference 130

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Observation 4f4cf45e-69b9-4919-8c89-4c7bdfadc8f5 · inbound

Do Observations Prefer Thawing Quintessence? cites this paper.

Do Observations Prefer Thawing Quintessence? Efficient Computation of CMB anisotropies in closed FRW models

Reference 61

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Modified recombination and the Hubble tension cites this paper.

Modified recombination and the Hubble tension Efficient Computation of CMB anisotropies in closed FRW models

Reference 43

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Observation 5637acd7-5472-4738-af90-93e66aa7bb71 · inbound

Multi-Agent System for Cosmological Parameter Analysis cites this paper.

Multi-Agent System for Cosmological Parameter Analysis Efficient Computation of CMB anisotropies in closed FRW models

Reference 12

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Reducing nuisance prior sensitivity via non-linear reparameterization, with application to EFT analyses of large-scale structure cites this paper.

Reducing nuisance prior sensitivity via non-linear reparameterization, with application to EFT analyses of large-scale structure Efficient Computation of CMB anisotropies in closed FRW models

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DeepWiener: Neural Networks for CMB polarization maps and power spectrum computation cites this paper.

DeepWiener: Neural Networks for CMB polarization maps and power spectrum computation Efficient Computation of CMB anisotropies in closed FRW models

Reference 40

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Playground of Lognormal Seminumerical Simulations of~the~Lyman~$\alpha$ Forest: Thermal History of the Intergalactic Medium cites this paper.

Playground of Lognormal Seminumerical Simulations of~the~Lyman~$\alpha$ Forest: Thermal History of the Intergalactic Medium Efficient Computation of CMB anisotropies in closed FRW models

Reference 24

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Observation 508f603e-7770-4e60-8182-3767beb227e4 · inbound

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ cites this paper.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Efficient Computation of CMB anisotropies in closed FRW models

Reference 37

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Impact of DESI BAO Data on Inflationary Parameters: stability against late-time new physics cites this paper.

Impact of DESI BAO Data on Inflationary Parameters: stability against late-time new physics Efficient Computation of CMB anisotropies in closed FRW models

Reference 89

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Impact of reionization history on constraining primordial gravitational waves in future all-sky cosmic microwave background experiments cites this paper.

Impact of reionization history on constraining primordial gravitational waves in future all-sky cosmic microwave background experiments Efficient Computation of CMB anisotropies in closed FRW models

Reference 69

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Probing Long-Range Forces Between Neutrinos with Cosmic Structures cites this paper.

Probing Long-Range Forces Between Neutrinos with Cosmic Structures Efficient Computation of CMB anisotropies in closed FRW models

Reference 194

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Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? cites this paper.

Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? Efficient Computation of CMB anisotropies in closed FRW models

Reference 81

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Effort: a fast and differentiable emulator for the Effective Field Theory of the Large Scale Structure of the Universe cites this paper.

Effort: a fast and differentiable emulator for the Effective Field Theory of the Large Scale Structure of the Universe Efficient Computation of CMB anisotropies in closed FRW models

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Cosmic Large-Scale Structure Formation from Newtonian Particle Dynamics cites this paper.

Cosmic Large-Scale Structure Formation from Newtonian Particle Dynamics Efficient Computation of CMB anisotropies in closed FRW models

Reference 40

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A Fast and Accurate Implementation of the Effective Fluid Approximation for Ultralight Axions cites this paper.

A Fast and Accurate Implementation of the Effective Fluid Approximation for Ultralight Axions Efficient Computation of CMB anisotropies in closed FRW models

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Uncertainties in the Hubble Constant from Peculiar Velocities cites this paper.

Uncertainties in the Hubble Constant from Peculiar Velocities Efficient Computation of CMB anisotropies in closed FRW models

Reference 48

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Impact of light sterile neutrinos on cosmological large scale structure cites this paper.

Impact of light sterile neutrinos on cosmological large scale structure Efficient Computation of CMB anisotropies in closed FRW models

Reference 51

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Exploring generalized Starobinsky Model of Inflation: Observational Constraints cites this paper.

Exploring generalized Starobinsky Model of Inflation: Observational Constraints Efficient Computation of CMB anisotropies in closed FRW models

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Searching for Inflationary Physics with the CMB Trispectrum: 2. Code & Validation cites this paper.

Searching for Inflationary Physics with the CMB Trispectrum: 2. Code & Validation Efficient Computation of CMB anisotropies in closed FRW models

Reference 74

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Reconstructing the shape of the non-linear matter power spectrum using CMB lensing and cosmic shear cites this paper.

Reconstructing the shape of the non-linear matter power spectrum using CMB lensing and cosmic shear Efficient Computation of CMB anisotropies in closed FRW models

Reference 40

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Generalized Uncertainty Principle mimicking dynamical Dark Energy: matter perturbations and gravitational wave data analysis cites this paper.

Generalized Uncertainty Principle mimicking dynamical Dark Energy: matter perturbations and gravitational wave data analysis Efficient Computation of CMB anisotropies in closed FRW models

Reference 84

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An overview of what current data can (and cannot yet) say about evolving dark energy cites this paper.

An overview of what current data can (and cannot yet) say about evolving dark energy Efficient Computation of CMB anisotropies in closed FRW models

Reference 256

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DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints cites this paper.

DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints Efficient Computation of CMB anisotropies in closed FRW models

Reference 124

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Extended Dark Energy analysis using DESI DR2 BAO measurements cites this paper.

Extended Dark Energy analysis using DESI DR2 BAO measurements Efficient Computation of CMB anisotropies in closed FRW models

Reference 86

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Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape cites this paper.

Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape Efficient Computation of CMB anisotropies in closed FRW models

Reference 135

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DEMNUni: the Sunyaev-Zel'dovich effect in the presence of massive neutrinos and dynamical dark energy cites this paper.

DEMNUni: the Sunyaev-Zel'dovich effect in the presence of massive neutrinos and dynamical dark energy Efficient Computation of CMB anisotropies in closed FRW models

Reference 55

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Shapes and orientations of massive halos in the statistically anisotropic universe cites this paper.

Shapes and orientations of massive halos in the statistically anisotropic universe Efficient Computation of CMB anisotropies in closed FRW models

Reference 26

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Teleparallel dark energy in a nonflat universe cites this paper.

Teleparallel dark energy in a nonflat universe Efficient Computation of CMB anisotropies in closed FRW models

Reference 63

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Cosmic Strings as Dynamical Dark Energy: Novel Constraints cites this paper.

Cosmic Strings as Dynamical Dark Energy: Novel Constraints Efficient Computation of CMB anisotropies in closed FRW models

Reference 64

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Attention-based Neural Network Emulators for Multi-Probe Data Vectors Part III: Modeling The Next Generation Surveys cites this paper.

Attention-based Neural Network Emulators for Multi-Probe Data Vectors Part III: Modeling The Next Generation Surveys Efficient Computation of CMB anisotropies in closed FRW models

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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics cites this paper.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Efficient Computation of CMB anisotropies in closed FRW models

Reference 21

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Constraining the Baryon Fraction in Extragalactic Diffuse Ionized Gas with 124 Localized Fast Radio Bursts cites this paper.

Constraining the Baryon Fraction in Extragalactic Diffuse Ionized Gas with 124 Localized Fast Radio Bursts Efficient Computation of CMB anisotropies in closed FRW models

Reference 77

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Topological defects as effective dynamical dark energy cites this paper.

Topological defects as effective dynamical dark energy Efficient Computation of CMB anisotropies in closed FRW models

Reference 65

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Patchy Helium and Hydrogen Reionization from the Kinetic Sunyaev-Zel'dovich Effect and Galaxies cites this paper.

Patchy Helium and Hydrogen Reionization from the Kinetic Sunyaev-Zel'dovich Effect and Galaxies Efficient Computation of CMB anisotropies in closed FRW models

Reference 100

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Bayesian and frequentist perspectives agree on dynamical dark energy cites this paper.

Bayesian and frequentist perspectives agree on dynamical dark energy Efficient Computation of CMB anisotropies in closed FRW models

Reference 55

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Observation 6ea1e5ef-2ca3-473e-ba9e-c01e1f30a7e1 · inbound

Simple quintessence models in light of DESI-BAO observations cites this paper.

Simple quintessence models in light of DESI-BAO observations Efficient Computation of CMB anisotropies in closed FRW models

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-07T00:43:08.423847Z

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Observation d60d4cdd-401c-483d-823d-2b1d04842c54 · inbound

Cosmology from Planck CMB Lensing and DESI DR1 Quasar Tomography cites this paper.

Cosmology from Planck CMB Lensing and DESI DR1 Quasar Tomography Efficient Computation of CMB anisotropies in closed FRW models

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-06T22:09:12.201602Z

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Observation bb9fe7a8-a73e-41d6-a514-ca4a3af71d41 · inbound

Quantum stress-energy at timelike boundaries: testing a new beyond-$\Lambda$CDM parameter with cosmological data cites this paper.

Quantum stress-energy at timelike boundaries: testing a new beyond-$\Lambda$CDM parameter with cosmological data Efficient Computation of CMB anisotropies in closed FRW models

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-06T21:34:30.948703Z

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Observation fcd7ab35-d550-42c7-92d9-e4012b8259a4 · inbound

Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration cites this paper.

Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration Efficient Computation of CMB anisotropies in closed FRW models

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-06T21:02:33.789577Z

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Observation cf398bcc-7098-4e89-8c11-1c39aa54025c · inbound

Cosmology and Source Redshift Constraints from Galaxy Clustering and Tomographic Weak Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model cites this paper.

Cosmology and Source Redshift Constraints from Galaxy Clustering and Tomographic Weak Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model Efficient Computation of CMB anisotropies in closed FRW models

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-06T20:59:59.033881Z

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Observation 3dd1a343-43f8-4646-a2b4-5242a99c838f · inbound

Cosmological Simulations of Galaxies cites this paper.

Cosmological Simulations of Galaxies Efficient Computation of CMB anisotropies in closed FRW models

Reference 185

Resolution: unresolved; no resolver link, observed 2026-08-06T18:16:10.592197Z

Source-reported events for the cited work

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Observation 8bfed45e-b36e-42e6-9a5c-a640fac1eea5 · inbound

Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints cites this paper.

Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints Efficient Computation of CMB anisotropies in closed FRW models

Reference 152

Resolution: unresolved; no resolver link, observed 2026-08-06T18:14:22.553260Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2da24161-141b-426f-bbcb-25923dbabb01 · inbound

New Insights into Dark Energy from DESI DR2 with CMB and SNIa cites this paper.

New Insights into Dark Energy from DESI DR2 with CMB and SNIa Efficient Computation of CMB anisotropies in closed FRW models

Reference 79

Resolution: verified exact; local_arxiv, observed 2026-05-19T05:22:06.187837Z

Source-reported events for the cited work

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Observation 2d1ee379-401d-4b28-a1c5-97ccf1ce5699 · inbound

Cosmological neutrino mass: a frequentist overview in light of DESI cites this paper.

Cosmological neutrino mass: a frequentist overview in light of DESI Efficient Computation of CMB anisotropies in closed FRW models

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-06T16:55:44.281419Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b6257c5b-52f3-422f-b491-08e37e4135d9 · inbound

The BAO-CMB Tension and Implications for Inflation cites this paper.

The BAO-CMB Tension and Implications for Inflation Efficient Computation of CMB anisotropies in closed FRW models

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-06T16:53:11.269932Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ec145a05-e061-4d81-b046-2b1f13477134 · inbound

Investigating $f(R)$-Inflation: background evolution and constraints cites this paper.

Investigating $f(R)$-Inflation: background evolution and constraints Efficient Computation of CMB anisotropies in closed FRW models

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-06T16:26:13.375124Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a2388c67-a604-4246-ae4f-4eb3a1ef8354 · inbound

Cosmological preference for a positive neutrino mass at 2.7$\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data cites this paper.

Cosmological preference for a positive neutrino mass at 2.7$\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data Efficient Computation of CMB anisotropies in closed FRW models

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-06T15:12:38.771038Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a9a4c16b-f970-45d5-bb80-fa28d18b2c8d · inbound

CMB constraints on $U(1)$ axion warm inflation cites this paper.

CMB constraints on $U(1)$ axion warm inflation Efficient Computation of CMB anisotropies in closed FRW models

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-06T15:00:52.404454Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1d47c652-fe29-45c2-bc3b-1106fe84d09c · inbound

Resolving the Planck-DESI tension by nonminimally coupled quintessence cites this paper.

Resolving the Planck-DESI tension by nonminimally coupled quintessence Efficient Computation of CMB anisotropies in closed FRW models

Reference 75

Resolution: verified exact; local_arxiv, observed 2026-05-19T01:36:58.416529Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation a1ce021a-b978-4fdc-b310-4070fdfb798d · inbound

$\texttt{GENGARS}$: Accurate non-Gaussian initial conditions with arbitrary bispectrum for N-body simulations cites this paper.

$\texttt{GENGARS}$: Accurate non-Gaussian initial conditions with arbitrary bispectrum for N-body simulations Efficient Computation of CMB anisotropies in closed FRW models

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-06T05:30:11.430346Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 50481e21-8c1e-4003-b79c-56f79e56e636 · inbound

Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO cites this paper.

Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO Efficient Computation of CMB anisotropies in closed FRW models

Reference 130

Resolution: unresolved; no resolver link, observed 2026-08-05T16:03:01.482094Z

Source-reported events for the cited work

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Observation 131a9cb8-f75c-43be-bf14-6c4cee6eacd0 · inbound

Deep Learning for CMB Foreground Removal and Beam Deconvolution: A U-Net GAN Approach cites this paper.

Deep Learning for CMB Foreground Removal and Beam Deconvolution: A U-Net GAN Approach Efficient Computation of CMB anisotropies in closed FRW models

Reference 16

Resolution: verified exact; local_arxiv, observed 2026-05-18T20:06:50.370265Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation c61ad294-e874-4218-94ac-875954f62f75 · inbound

Probing the limits of cosmological information from the Lyman-$\alpha$ forest 2-point correlation functions cites this paper.

Probing the limits of cosmological information from the Lyman-$\alpha$ forest 2-point correlation functions Efficient Computation of CMB anisotropies in closed FRW models

Reference 65

Resolution: verified exact; local_arxiv, observed 2026-05-18T15:41:33.646745Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 31aadee4-7bd6-41ca-9a46-06f0fd840f1c · inbound

Updated observational constraints on $\phi$CDM dynamical dark energy cosmological models cites this paper.

Updated observational constraints on $\phi$CDM dynamical dark energy cosmological models Efficient Computation of CMB anisotropies in closed FRW models

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-04T13:43:12.330326Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7157ac1d-01f4-45b8-a69e-59d1ba3531c6 · inbound

The superclustering of hot gas: cosmological sensitivity in the Websky simulations cites this paper.

The superclustering of hot gas: cosmological sensitivity in the Websky simulations Efficient Computation of CMB anisotropies in closed FRW models

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-04T10:50:55.323902Z

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Unavailable: canonical work link unavailable.

Observation c098f26a-6436-4410-a345-0a0fe2aeb6a0 · inbound

Constraints of dynamical dark energy models from different observational datasets cites this paper.

Constraints of dynamical dark energy models from different observational datasets Efficient Computation of CMB anisotropies in closed FRW models

Reference 45

Resolution: verified exact; local_arxiv, observed 2026-05-18T08:21:06.493245Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 20e3001e-7fd8-4fb3-af2e-97427c950646 · inbound

Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 cites this paper.

Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 Efficient Computation of CMB anisotropies in closed FRW models

Reference 185

Resolution: unresolved; no resolver link, observed 2026-08-04T09:59:30.666517Z

Source-reported events for the cited work

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Observation d8889185-d6ce-4677-b9fc-7e0dbb074c56 · inbound

Modeling nonlinear scales for dynamical dark energy cosmologies with COLA cites this paper.

Modeling nonlinear scales for dynamical dark energy cosmologies with COLA Efficient Computation of CMB anisotropies in closed FRW models

Reference 140

Resolution: verified exact; local_arxiv, observed 2026-05-18T06:15:58.592470Z

Source-reported events for the cited work

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Observation 054a30d8-6df3-4bed-a98d-d01662d376af · inbound

The implications of inflation for the last ACT cites this paper.

The implications of inflation for the last ACT Efficient Computation of CMB anisotropies in closed FRW models

Reference 76

Resolution: verified exact; local_arxiv, observed 2026-05-21T20:40:36.044508Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation a31cba02-190f-450b-a2d8-b4cc0019f3a9 · inbound

Running of the spectral index: Reconciling the CMB with the Lyman-$\alpha$ Forest cites this paper.

Running of the spectral index: Reconciling the CMB with the Lyman-$\alpha$ Forest Efficient Computation of CMB anisotropies in closed FRW models

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-04T00:26:07.092392Z

Source-reported events for the cited work

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Observation 56443d9a-da77-4043-97fa-5fdd3ee68ac1 · inbound

Quantifying Weighted Morphological Content of Large-Scale Structures via Simulation-Based Inference cites this paper.

Quantifying Weighted Morphological Content of Large-Scale Structures via Simulation-Based Inference Efficient Computation of CMB anisotropies in closed FRW models

Reference 113

Resolution: verified exact; local_arxiv, observed 2026-05-18T01:12:15.294836Z

Source-reported events for the cited work

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Observation 786ed3bb-de44-459b-8161-0ac665491b81 · inbound

unimpeded: A Public Grid of Nested Sampling Chains for Cosmological Model Comparison and Tension Analysis cites this paper.

unimpeded: A Public Grid of Nested Sampling Chains for Cosmological Model Comparison and Tension Analysis Efficient Computation of CMB anisotropies in closed FRW models

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-03T23:41:00.531856Z

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Observation 96be64e4-89bf-4624-b56d-82c067938ec0 · inbound

A Bayesian Perspective on Evidence for Evolving Dark Energy cites this paper.

A Bayesian Perspective on Evidence for Evolving Dark Energy Efficient Computation of CMB anisotropies in closed FRW models

Reference 21

Resolution: verified exact; local_arxiv, observed 2026-05-17T22:10:22.790537Z

Source-reported events for the cited work

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Observation 2c77ca22-e93e-4d21-890f-a6f8acfa5b62 · inbound

On the bin sensitivity of the transverse BAO cites this paper.

On the bin sensitivity of the transverse BAO Efficient Computation of CMB anisotropies in closed FRW models

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-03T20:50:04.658881Z

Source-reported events for the cited work

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Observation a371ff6b-f0b2-476c-a8f4-81d178ed591e · inbound

Cosmological tensions in Proca-Nuevo theory cites this paper.

Cosmological tensions in Proca-Nuevo theory Efficient Computation of CMB anisotropies in closed FRW models

Reference 91

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c2e12ccd-b177-432a-8a48-1cecd89e3671 · inbound

Observational constraints on 3-forms dark energy cites this paper.

Observational constraints on 3-forms dark energy Efficient Computation of CMB anisotropies in closed FRW models

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-03T17:24:59.362077Z

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Unavailable: canonical work link unavailable.

Observation 1505a535-249e-470d-9e16-d82ee9292680 · inbound

CLiENT: A new tool for emulating cosmological likelihoods using deep neural networks cites this paper.

CLiENT: A new tool for emulating cosmological likelihoods using deep neural networks Efficient Computation of CMB anisotropies in closed FRW models

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-03T15:17:37.024148Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 38a1a9d0-1e46-4ce1-88a4-63e3316c1d3f · inbound

Implicit Likelihood Inference of the Neutrino Mass Hierarchy from Cosmological Data cites this paper.

Implicit Likelihood Inference of the Neutrino Mass Hierarchy from Cosmological Data Efficient Computation of CMB anisotropies in closed FRW models

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-03T15:16:07.719134Z

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Observation 1a488ebd-ccff-4fdd-9620-943dab992363 · inbound

Thawing Quintessence: Priors, evidence, and likely trajectories cites this paper.

Thawing Quintessence: Priors, evidence, and likely trajectories Efficient Computation of CMB anisotropies in closed FRW models

Reference 50

Resolution: verified exact; local_arxiv, observed 2026-05-16T19:53:21.800443Z

Source-reported events for the cited work

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Observation 30ccc18b-56b3-493b-a6bc-9334f9cd55fe · inbound

Robust Preference for Dark Sector Interactions cites this paper.

Robust Preference for Dark Sector Interactions Efficient Computation of CMB anisotropies in closed FRW models

Reference 119

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.921211Z

Source-reported events for the cited work

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Observation 09766cfa-01d2-4738-9bab-e120b79c3657 · inbound

An essential building block for cosmological zoom-in perturbation theory cites this paper.

An essential building block for cosmological zoom-in perturbation theory Efficient Computation of CMB anisotropies in closed FRW models

Reference 55

Resolution: verified exact; local_arxiv, observed 2026-05-16T10:50:51.701451Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 7392432c-e893-4699-9139-dc11c4f35294 · inbound

Cosmological analysis of the DESI DR1 Lyman alpha 1D power spectrum cites this paper.

Cosmological analysis of the DESI DR1 Lyman alpha 1D power spectrum Efficient Computation of CMB anisotropies in closed FRW models

Reference 100

Resolution: verified exact; local_arxiv, observed 2026-05-16T10:07:43.803596Z

Source-reported events for the cited work

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Observation 1cd0460e-ce47-4b91-80b5-af68a24bad7d · inbound

A Variable-Slope Smooth-$k$ Filter for Modeling Halo Abundances with Damped and Oscillatory Power Spectra cites this paper.

A Variable-Slope Smooth-$k$ Filter for Modeling Halo Abundances with Damped and Oscillatory Power Spectra Efficient Computation of CMB anisotropies in closed FRW models

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-03T05:48:45.777090Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7a1f1a92-365f-4c50-8bc3-2ccda92745a3 · inbound

ACT DR6+Planck impact on inflation with non-zero vacuum expectation value and the post-inflationary behavior cites this paper.

ACT DR6+Planck impact on inflation with non-zero vacuum expectation value and the post-inflationary behavior Efficient Computation of CMB anisotropies in closed FRW models

Reference 51

Resolution: verified exact; local_arxiv, observed 2026-05-21T13:40:12.358439Z

Source-reported events for the cited work

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Observation cb8d9a5f-dc3e-4b4e-92e6-4838b89f7e0c · inbound

Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology cites this paper.

Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology Efficient Computation of CMB anisotropies in closed FRW models

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-03T03:05:15.449313Z

Source-reported events for the cited work

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Observation 7de4d59d-23db-4dc4-8130-f32f2096cc4b · inbound

DESI DR2 Baryon Acoustic Oscillations from the Lyman Alpha Forest Multipoles cites this paper.

DESI DR2 Baryon Acoustic Oscillations from the Lyman Alpha Forest Multipoles Efficient Computation of CMB anisotropies in closed FRW models

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-02T18:54:33.735206Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c0cc731f-77f2-4837-956c-4a018aec13a4 · inbound

The Bayesian view of DESI DR2 with unimpeded: Evidence and tension in a combined analysis with CMB and supernovae across cosmological models cites this paper.

The Bayesian view of DESI DR2 with unimpeded: Evidence and tension in a combined analysis with CMB and supernovae across cosmological models Efficient Computation of CMB anisotropies in closed FRW models

Reference 32

Resolution: verified exact; local_arxiv, observed 2026-05-21T11:34:09.256553Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 004a494b-b7f3-49e5-a722-3d3317c4e2dd · inbound

Constraining Neutrino Mass with the Void Weak Lensing Effect cites this paper.

Constraining Neutrino Mass with the Void Weak Lensing Effect Efficient Computation of CMB anisotropies in closed FRW models

Reference 80

Resolution: verified exact; local_arxiv, observed 2026-05-21T12:35:07.924037Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation eb7a25d5-7565-4a47-a336-dd9aeaa03604 · inbound

Measuring neutrino mass in light of ACT DR6 and DESI DR2 cites this paper.

Measuring neutrino mass in light of ACT DR6 and DESI DR2 Efficient Computation of CMB anisotropies in closed FRW models

Reference 185

Resolution: verified exact; local_arxiv, observed 2026-05-15T13:15:50.375056Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 140097b6-3f9a-452e-9325-3b844ddd242d · inbound

Blind mitigation of foreground-induced biases on primordial $B$ modes for ground-based CMB experiments cites this paper.

Blind mitigation of foreground-induced biases on primordial $B$ modes for ground-based CMB experiments Efficient Computation of CMB anisotropies in closed FRW models

Reference 36

Resolution: verified exact; local_arxiv, observed 2026-05-15T12:39:59.993017Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

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