CAMB v2: cosmological power spectra for high-precision surveys | Paper Citation Record

Observation 818ecdaf-3437-4d38-87a2-9ddc7616b4ca · outbound

This paper cites For evaluating the curved action ana- lytically it is useful to definex K =αS K(χ).

CAMB v2: cosmological power spectra for high-precision surveys For evaluating the curved action ana- lytically it is useful to definex K =αS K(χ)

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Observation 34666682-3fe8-4de3-a9ff-c2d6528cd6f1 · outbound

This paper cites (4.18), the constant-map (shifted-ν) limit.

CAMB v2: cosmological power spectra for high-precision surveys (4.18), the constant-map (shifted-ν) limit

Reference 2

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This paper cites Forl≤2 it uses phi_recurs.

CAMB v2: cosmological power spectra for high-precision surveys Forl≤2 it uses phi_recurs

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This paper cites The resulting parity factor is the closed-space sign applied to allK= +1 evaluations, including the Olver map of Eq.

CAMB v2: cosmological power spectra for high-precision surveys The resulting parity factor is the closed-space sign applied to allK= +1 evaluations, including the Olver map of Eq

Reference 4

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This paper cites COSMICS: Cosmological Initial Conditions and Microwave Anisotropy Codes.

CAMB v2: cosmological power spectra for high-precision surveys COSMICS: Cosmological Initial Conditions and Microwave Anisotropy Codes

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Observation aecda905-bd1d-4518-889c-f4c2c72652f8 · outbound

This paper cites A Complete Treatment of CMB Anisotropies in a FRW Universe.

CAMB v2: cosmological power spectra for high-precision surveys A Complete Treatment of CMB Anisotropies in a FRW Universe

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This paper cites Efficient Computation of CMB anisotropies in closed FRW models.

CAMB v2: cosmological power spectra for high-precision surveys Efficient Computation of CMB anisotropies in closed FRW models

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

CAMB v2: cosmological power spectra for high-precision surveys The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes

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Observation 1a161d1f-bb8e-41d0-8f9e-f16c320bf930 · outbound

This paper cites A Line of Sight Approach to Cosmic Microwave Background Anisotropies.

CAMB v2: cosmological power spectra for high-precision surveys A Line of Sight Approach to Cosmic Microwave Background Anisotropies

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Observation 5d12e45d-3641-4dfc-88e7-9de8fe07b4af · outbound

This paper cites Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges.

CAMB v2: cosmological power spectra for high-precision surveys Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges

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Observation 46d15f23-0248-445d-9872-697d2c4eab27 · outbound

This paper cites Weak Gravitational Lensing of the CMB.

CAMB v2: cosmological power spectra for high-precision surveys Weak Gravitational Lensing of the CMB

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Observation 7947adf0-c788-4874-bc5a-df075c3e70ed · outbound

This paper cites Efficient Computation of Hyperspherical Bessel Functions.

CAMB v2: cosmological power spectra for high-precision surveys Efficient Computation of Hyperspherical Bessel Functions

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Observation 029a5e65-e5ad-4035-85fe-fddd9534d09f · outbound

This paper cites Integral Solution for the Microwave Background Anisotropies in Non-fl at Universes.

CAMB v2: cosmological power spectra for high-precision surveys Integral Solution for the Microwave Background Anisotropies in Non-fl at Universes

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Observation 095771b9-e04c-43b5-a977-05ef3c549bf4 · outbound

This paper cites Microwave background polarization in cosmological models.

CAMB v2: cosmological power spectra for high-precision surveys Microwave background polarization in cosmological models

Reference 14

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Observation 16e4d9f6-f734-43f4-95a8-076781211a01 · outbound

This paper cites CMB power spectrum parameter degeneracies in the era of precision cosmology.

CAMB v2: cosmological power spectra for high-precision surveys CMB power spectrum parameter degeneracies in the era of precision cosmology

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This paper cites The Simons Observatory: Science goals and forecasts.

CAMB v2: cosmological power spectra for high-precision surveys The Simons Observatory: Science goals and forecasts

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This paper cites The General Primordial Cosmic Perturbation.

CAMB v2: cosmological power spectra for high-precision surveys The General Primordial Cosmic Perturbation

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Observation f651fb8a-f83c-4f02-8a0f-60209242f879 · outbound

This paper cites Photons and Baryons before Atoms: Improving the Tight-Coupling Approximation.

CAMB v2: cosmological power spectra for high-precision surveys Photons and Baryons before Atoms: Improving the Tight-Coupling Approximation

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This paper cites Computation of hyperspherical Bessel functions.

CAMB v2: cosmological power spectra for high-precision surveys Computation of hyperspherical Bessel functions

Reference 19

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Observation ce26208b-f4d0-4a3a-a83b-de1b60b8eb4c · outbound

This paper cites Fast and accurate CMB computations in non-flat FLRW universes.

CAMB v2: cosmological power spectra for high-precision surveys Fast and accurate CMB computations in non-flat FLRW universes

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This paper cites Lewis, Phys.

CAMB v2: cosmological power spectra for high-precision surveys Lewis, Phys

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This paper cites Lewis,https://cosmologist.info/notes/CAMB.pdf.

CAMB v2: cosmological power spectra for high-precision surveys Lewis,https://cosmologist.info/notes/CAMB.pdf

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This paper cites Lewis (2026),https://github.com/cmbant/ CAMB/blob/master/docs/changelog/flat_bessel_ approximations.pdf.

CAMB v2: cosmological power spectra for high-precision surveys Lewis (2026),https://github.com/cmbant/ CAMB/blob/master/docs/changelog/flat_bessel_ approximations.pdf

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CAMB v2: cosmological power spectra for high-precision surveys Unresolved cited work

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CAMB v2: cosmological power spectra for high-precision surveys Precision big bang nucleosynthesis with improved Helium-4 predictions

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CAMB v2: cosmological power spectra for high-precision surveys Constraining the helium abundance with CMB

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CAMB v2: cosmological power spectra for high-precision surveys Using BBN in cosmological parameter extraction from CMB: a forecast for Planck

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CAMB v2: cosmological power spectra for high-precision surveys PArthENoPE: Public Algorithm Evaluating the Nucleosynthesis of Primordial Elements

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CAMB v2: cosmological power spectra for high-precision surveys PArthENoPE reloaded

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CAMB v2: cosmological power spectra for high-precision surveys Towards a complete treatment of the cosmological recombination problem

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CAMB v2: cosmological power spectra for high-precision surveys Ultrafast effective multi-level atom method for primordial hydrogen recombination

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CAMB v2: cosmological power spectra for high-precision surveys Planck 2018 results. VI. Cosmological parameters

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CAMB v2: cosmological power spectra for high-precision surveys A new tension in the cosmological model from primordial deuterium?

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CAMB v2: cosmological power spectra for high-precision surveys How exactly did the Universe become neutral?

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CAMB v2: cosmological power spectra for high-precision surveys How well do we understand cosmological recombination?

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CAMB v2: cosmological power spectra for high-precision surveys HyRec: A fast and highly accurate primordial hydrogen and helium recombination code

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CAMB v2: cosmological power spectra for high-precision surveys HYREC-2: a highly accurate sub-millisecond recombination code

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CAMB v2: cosmological power spectra for high-precision surveys Radiative transfer effects during primordial helium recombination

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CAMB v2: cosmological power spectra for high-precision surveys A New Calculation of the Recombination Epoch

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CAMB v2: cosmological power spectra for high-precision surveys Cosmological parameters from WMAP 5-year temperature maps

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CAMB v2: cosmological power spectra for high-precision surveys Precise cosmological parameter estimation using CosmoRec

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CAMB v2: cosmological power spectra for high-precision surveys Reionization inference from the CMB optical depth and E-mode polarization power spectra

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CAMB v2: cosmological power spectra for high-precision surveys Planck intermediate results. XLVII. Planck constraints on reionization history

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CAMB v2: cosmological power spectra for high-precision surveys Hydrogen reionisation ends by $z=5.3$: Lyman-$\alpha$ optical depth measured by the XQR-30 sample

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CAMB v2: cosmological power spectra for high-precision surveys Observational constraints on Cosmic Reionization

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CAMB v2: cosmological power spectra for high-precision surveys Quantitative Constraints on the Reionization History from the IGM Damping Wing Signature in Two Quasars at z > 7

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CAMB v2: cosmological power spectra for high-precision surveys The Universe is Reionizing at z~7: Bayesian Inference of the IGM Neutral Fraction Using Ly$\alpha$ Emission from Galaxies

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CAMB v2: cosmological power spectra for high-precision surveys Crossing the Phantom Divide with Parameterized Post-Friedmann Dark Energy

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CAMB v2: cosmological power spectra for high-precision surveys Cosmological implications of ultra-light axion-like fields

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CAMB v2: cosmological power spectra for high-precision surveys A new parameterization of the reionisation history

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CAMB v2: cosmological power spectra for high-precision surveys Evolution of cosmological dark matter perturbations

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This paper cites The Cosmic Linear Anisotropy Solving System (CLASS) IV: Efficient implementation of non-cold relics.

CAMB v2: cosmological power spectra for high-precision surveys The Cosmic Linear Anisotropy Solving System (CLASS) IV: Efficient implementation of non-cold relics

Reference 63

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Observation 9b95db98-1626-494b-9fd9-f1ee0e934733 · outbound

This paper cites Parametrized Post-Friedmann Signatures of Acceleration in the CMB.

CAMB v2: cosmological power spectra for high-precision surveys Parametrized Post-Friedmann Signatures of Acceleration in the CMB

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-02T00:56:19.648514Z

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Observation e871fef2-f918-4248-a980-a34937a13632 · outbound

This paper cites Impact of post-Born lensing on the CMB.

CAMB v2: cosmological power spectra for high-precision surveys Impact of post-Born lensing on the CMB

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-02T00:56:20.024230Z

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Observation 91a92c79-bd3f-41ae-930d-03390f281097 · outbound

This paper cites The shape of the CMB lensing bispectrum.

CAMB v2: cosmological power spectra for high-precision surveys The shape of the CMB lensing bispectrum

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-02T00:56:20.082108Z

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Observation 2f568412-ac2b-4085-a559-605f00e55d6f · outbound

This paper cites Oscillating scalar fields and the Hubble tension: a resolution with novel signatures.

CAMB v2: cosmological power spectra for high-precision surveys Oscillating scalar fields and the Hubble tension: a resolution with novel signatures

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-02T00:56:19.828734Z

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Observation 1fd56f61-4db9-4346-a8be-090379022338 · outbound

This paper cites Lensed CMB power spectra from all-sky correlation functions.

CAMB v2: cosmological power spectra for high-precision surveys Lensed CMB power spectra from all-sky correlation functions

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-02T00:56:19.880198Z

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Observation ea93cea3-9838-47fd-bd01-c1404bdfa28f · outbound

This paper cites A Small-Scale Modification to the Lensing Kernel.

CAMB v2: cosmological power spectra for high-precision surveys A Small-Scale Modification to the Lensing Kernel

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-02T00:56:19.917445Z

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Observation 3c65e413-0487-490b-a426-61b369da526b · outbound

This paper cites perturbations.

CAMB v2: cosmological power spectra for high-precision surveys perturbations

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-02T00:56:14.468535Z

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Observation cd3ae3a2-db99-41fe-8e90-185df6e0a5a6 · outbound

This paper cites Emission-angle and polarization-rotation effects in the lensed CMB.

CAMB v2: cosmological power spectra for high-precision surveys Emission-angle and polarization-rotation effects in the lensed CMB

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-02T00:56:19.959925Z

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Observation 5e910dfd-000c-401e-a6fa-33a20dd40f03 · outbound

This paper cites Casaset al.(Euclid), Astron.

CAMB v2: cosmological power spectra for high-precision surveys Casaset al.(Euclid), Astron

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-02T00:56:20.542922Z

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Observation 203c5cd9-9caf-4a83-9c33-ebc3f1f04ca2 · outbound

This paper cites Revising the Halofit Model for the Nonlinear Matter Power Spectrum.

CAMB v2: cosmological power spectra for high-precision surveys Revising the Halofit Model for the Nonlinear Matter Power Spectrum

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-02T00:56:20.140321Z

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Observation d3bba61c-b2cb-4908-9ed0-c2d5323ff539 · outbound

This paper cites HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback.

CAMB v2: cosmological power spectra for high-precision surveys HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-02T00:56:20.239945Z

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Observation 78416919-4ead-4738-91c7-242d04c8d9b4 · outbound

This paper cites SP(k) -- A hydrodynamical simulation-based model for the impact of baryon physics on the non-linear matter power spectrum.

CAMB v2: cosmological power spectra for high-precision surveys SP(k) -- A hydrodynamical simulation-based model for the impact of baryon physics on the non-linear matter power spectrum

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-02T00:56:20.275539Z

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Observation 1513254e-cfa0-46eb-90cf-45ac2b8f017a · outbound

This paper cites The Cosmic Linear Anisotropy Solving System (CLASS) III: Comparision with CAMB for LambdaCDM.

CAMB v2: cosmological power spectra for high-precision surveys The Cosmic Linear Anisotropy Solving System (CLASS) III: Comparision with CAMB for LambdaCDM

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-02T00:56:20.344796Z

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Observation b6dd6f31-aac4-48d0-8258-a6b91ff1d6dc · outbound

This paper cites Baryonic feedback biases on fundamental physics from lensed CMB power spectra.

CAMB v2: cosmological power spectra for high-precision surveys Baryonic feedback biases on fundamental physics from lensed CMB power spectra

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-02T00:56:20.486742Z

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Observation 85789398-55f6-4f3a-a0ab-c4f3e6a2e74c · outbound

This paper cites High-accuracy emulators for observables in $\Lambda$CDM, $N_\mathrm{eff}$, $\Sigma m_\nu$, and $w$ cosmologies.

CAMB v2: cosmological power spectra for high-precision surveys High-accuracy emulators for observables in $\Lambda$CDM, $N_\mathrm{eff}$, $\Sigma m_\nu$, and $w$ cosmologies

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-02T00:56:20.597256Z

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Observation 3f81c39f-aee5-4fa6-9fb7-122bebd61a8e · outbound

This paper cites Lewis (2026),https://github.com/cmbant/CAMB/ blob/master/docs/changelog/hyperspherical_ bessels.pdf.

CAMB v2: cosmological power spectra for high-precision surveys Lewis (2026),https://github.com/cmbant/CAMB/ blob/master/docs/changelog/hyperspherical_ bessels.pdf

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-02T00:56:20.699784Z

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Observation 6a439260-e3fc-4703-b2a5-3e477f6fef1d · outbound

This paper cites The Simons Observatory: Science Goals and Forecasts for the Enhanced Large Aperture Telescope.

CAMB v2: cosmological power spectra for high-precision surveys The Simons Observatory: Science Goals and Forecasts for the Enhanced Large Aperture Telescope

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-02T00:56:20.851290Z

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Observation 906bae7e-7e67-4875-a8fd-7afd9a8900d8 · outbound

This paper cites These thresh- olds are calibrated on peak-normalized error, keeping the raw Olver envelope near 10 −4 on the validation grid.

CAMB v2: cosmological power spectra for high-precision surveys These thresh- olds are calibrated on peak-normalized error, keeping the raw Olver envelope near 10 −4 on the validation grid

Reference 500

Resolution: unresolved; no resolver link, observed 2026-08-02T00:56:14.882417Z

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