Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-11T11:38:58.948485Z
Paper Citation Record · LEDGER
Accurate method for ultralight axion CMB and matter power spectra
As of 11 August 2026, this Paper Citation Record lists 63 of 63 outbound references and 6 inbound Pith citation observations for arXiv:2412.15192.
A citation records a reference. It does not transfer a finding from one paper to another.
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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T04:22:44.388067Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-02T15:27:05.305873Z
Reference resolution
63 of 63 outbound references displayed
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External citation measurements
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Outbound references
Observation 058d85c1-bea1-4fd2-a26d-6a953b95ff4c · outbound
This paper cites number of ways.
Accurate method for ultralight axion CMB and matter power spectra number of ways
Reference 1
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Observation db8978f2-4683-4aa9-9469-2858b1f98bff · outbound
This paper cites The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters.
Accurate method for ultralight axion CMB and matter power spectra The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters
Reference 2
- Resolution
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Source-reported events for the cited work
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Observation 60896e88-5710-462f-a2d2-2cb87fe47bb6 · outbound
This paper cites Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework.
Accurate method for ultralight axion CMB and matter power spectra Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework
Reference 4
- Resolution
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Source-reported events for the cited work
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Observation 4e8a671b-9073-4c53-bd5f-de7445130511 · outbound
This paper cites Cosmology From CMB Lensing and Delensed EE Power Spectra Using 2019-2020 SPT-3G Polarization Data.
Accurate method for ultralight axion CMB and matter power spectra Cosmology From CMB Lensing and Delensed EE Power Spectra Using 2019-2020 SPT-3G Polarization Data
Reference 5
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Observation 9e13aaaa-118f-4470-be21-fb3a76f70322 · outbound
This paper cites DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations.
Accurate method for ultralight axion CMB and matter power spectra DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
Reference 6
- Resolution
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Source-reported events for the cited work
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Observation 6da82217-e7be-4a03-9684-c9d2465cca5a · outbound
This paper cites The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset.
Accurate method for ultralight axion CMB and matter power spectra The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset
Reference 7
- Resolution
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Source-reported events for the cited work
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Observation 19e6067d-c26b-4cb8-9173-0daf226acc1c · outbound
This paper cites KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints.
Accurate method for ultralight axion CMB and matter power spectra KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints
Reference 8
- Resolution
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Source-reported events for the cited work
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Observation 53042029-4dfc-4914-b88d-ae036805d1ac · outbound
This paper cites Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing.
Accurate method for ultralight axion CMB and matter power spectra Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
Reference 9
- Resolution
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Source-reported events for the cited work
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Observation 37ecef42-c7db-42a6-bacb-5f0fd4f78dd2 · outbound
This paper cites Small Magellanic Cloud Cepheids Observed with the Hubble Space Telescope Provide a New Anchor for the SH0ES Distance Ladder.
Accurate method for ultralight axion CMB and matter power spectra Small Magellanic Cloud Cepheids Observed with the Hubble Space Telescope Provide a New Anchor for the SH0ES Distance Ladder
Reference 10
- Resolution
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Source-reported events for the cited work
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Observation a8bad013-e5ec-4cc7-b8ad-3f1b9b444481 · outbound
This paper cites Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Emulator Based Halo Model.
Accurate method for ultralight axion CMB and matter power spectra Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Emulator Based Halo Model
Reference 11
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Observation 87a704c6-0c24-4590-8fd6-8ee6e489cb50 · outbound
This paper cites The $H_0$ Olympics: A fair ranking of proposed models.
Accurate method for ultralight axion CMB and matter power spectra The $H_0$ Olympics: A fair ranking of proposed models
Reference 12
- Resolution
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Observation 4402dbd4-f8af-428f-a878-9111d2c0ba58 · outbound
This paper cites Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopes.
Accurate method for ultralight axion CMB and matter power spectra Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopes
Reference 13
- Resolution
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Observation 0dcbc5b7-13e9-4437-9e06-10def696b34a · outbound
This paper cites Axions In String Theory.
Accurate method for ultralight axion CMB and matter power spectra Axions In String Theory
Reference 14
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Observation d4e0e8e6-52cd-45b7-bb81-4679f97748c8 · outbound
This paper cites In the Realm of the Hubble tension $-$ a Review of Solutions.
Accurate method for ultralight axion CMB and matter power spectra In the Realm of the Hubble tension $-$ a Review of Solutions
Reference 15
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Observation 1738a331-d099-42a7-a73f-68355fbf455e · outbound
This paper cites String Axiverse.
Accurate method for ultralight axion CMB and matter power spectra String Axiverse
Reference 16
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Observation 5f391d35-19bd-4246-a50b-3314a8020596 · outbound
This paper cites an unresolved cited work.
Accurate method for ultralight axion CMB and matter power spectra Unresolved cited work
Reference 17
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Observation c641c21c-d829-41c3-85c9-211e3ba864d7 · outbound
This paper cites The Spectrum of the Axion Dark Sector.
Accurate method for ultralight axion CMB and matter power spectra The Spectrum of the Axion Dark Sector
Reference 18
- Resolution
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Source-reported events for the cited work
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Observation 03ece217-bfd4-4352-8f81-2a2fe1a523b5 · outbound
This paper cites The type IIB string axiverse and its low-energy phenomenology.
Accurate method for ultralight axion CMB and matter power spectra The type IIB string axiverse and its low-energy phenomenology
Reference 19
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Source-reported events for the cited work
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Observation ee837690-3b90-4925-859e-2a958d9599f0 · outbound
This paper cites Vector Dark Matter from Inflationary Fluctuations.
Accurate method for ultralight axion CMB and matter power spectra Vector Dark Matter from Inflationary Fluctuations
Reference 20
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Observation 1601b194-9775-4555-8847-a7c8e03658cd · outbound
This paper cites Glimmers from the Axiverse.
Accurate method for ultralight axion CMB and matter power spectra Glimmers from the Axiverse
Reference 21
- Resolution
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Observation 5a1bf317-7abf-4fd7-b4ac-65e50a5b3603 · outbound
This paper cites an unresolved cited work.
Accurate method for ultralight axion CMB and matter power spectra Unresolved cited work
Reference 22
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Observation 1df28fc3-f103-4971-b368-5f8dca6ff869 · outbound
This paper cites Small-scale structure in vector dark matter.
Accurate method for ultralight axion CMB and matter power spectra Small-scale structure in vector dark matter
Reference 23
- Resolution
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Observation 0e46eb88-0b76-43e5-9d56-0d862b68aa12 · outbound
This paper cites Ultra-Light Scalar Fields and the Growth of Structure in the Universe.
Accurate method for ultralight axion CMB and matter power spectra Ultra-Light Scalar Fields and the Growth of Structure in the Universe
Reference 24
- Resolution
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Observation 8d4dcb36-2a67-42cc-bc99-deccd85e055a · outbound
This paper cites Choi, Phys.
Accurate method for ultralight axion CMB and matter power spectra Choi, Phys
Reference 25
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Observation a2ec11ac-6718-4a74-b6ef-08a7a9e8cc71 · outbound
This paper cites an unresolved cited work.
Accurate method for ultralight axion CMB and matter power spectra Unresolved cited work
Reference 26
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Observation 49f85ab0-96f8-4442-8f13-4977db1fef4e · outbound
This paper cites Axion Cosmology.
Accurate method for ultralight axion CMB and matter power spectra Axion Cosmology
Reference 27
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Observation 219fd667-b771-4d0f-9c21-7cd7ad371de9 · outbound
This paper cites Too big to fail? The puzzling darkness of massive Milky Way subhaloes.
Accurate method for ultralight axion CMB and matter power spectra Too big to fail? The puzzling darkness of massive Milky Way subhaloes
Reference 28
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Observation a80af037-6f71-4cd1-879c-7c51c309220a · outbound
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Accurate method for ultralight axion CMB and matter power spectra The Core-Cusp Problem
Reference 29
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Observation 568e5df5-0f34-407d-a4cd-b4e2e22a780b · outbound
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Accurate method for ultralight axion CMB and matter power spectra Cold and Fuzzy Dark Matter
Reference 30
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Observation 89982a42-c304-4851-93b7-e0cb283c4072 · outbound
This paper cites Small-Scale Challenges to the $\Lambda$CDM Paradigm.
Accurate method for ultralight axion CMB and matter power spectra Small-Scale Challenges to the $\Lambda$CDM Paradigm
Reference 31
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Observation 4a18e4f3-c455-4e16-a7bc-41a0deccf46a · outbound
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Accurate method for ultralight axion CMB and matter power spectra Unresolved cited work
Reference 32
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Observation 37e12af2-5202-49ce-acb6-be36f342de95 · outbound
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Accurate method for ultralight axion CMB and matter power spectra Ultralight scalars as cosmological dark matter
Reference 33
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Observation c47a0846-658c-49ea-bba2-c30cbe9ac8c8 · outbound
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Accurate method for ultralight axion CMB and matter power spectra Acoustic Dark Energy: Potential Conversion of the Hubble Tension
Reference 34
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Observation d931943d-8720-4f6b-9ee3-b2c6803028bb · outbound
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Accurate method for ultralight axion CMB and matter power spectra Cosmological implications of ultra-light axion-like fields
Reference 35
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Observation cd75783f-725b-48f2-ac51-340cd3dfdd6e · outbound
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Accurate method for ultralight axion CMB and matter power spectra CMB-S4 Science Case, Reference Design, and Project Plan
Reference 36
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This paper cites Ultra-light axions and the $S_8$ tension: joint constraints from the cosmic microwave background and galaxy clustering.
Accurate method for ultralight axion CMB and matter power spectra Ultra-light axions and the $S_8$ tension: joint constraints from the cosmic microwave background and galaxy clustering
Reference 37
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Observation a33b6af8-e77a-44a5-ac35-d69d8d90b578 · outbound
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Accurate method for ultralight axion CMB and matter power spectra LSST Science Book, Version 2.0
Reference 38
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Accurate method for ultralight axion CMB and matter power spectra LSST: from Science Drivers to Reference Design and Anticipated Data Products
Reference 39
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Observation f5f028dc-3f55-4d66-b206-68f55be5b53f · outbound
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Accurate method for ultralight axion CMB and matter power spectra Cosmology and Fundamental Physics with the Euclid Satellite
Reference 40
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Accurate method for ultralight axion CMB and matter power spectra The LSST Dark Energy Science Collaboration (DESC) Science Requirements Document
Reference 41
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Observation a31d0a11-947d-498e-8677-fd7db66e2e9a · outbound
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Accurate method for ultralight axion CMB and matter power spectra A search for ultra-light axions using precision cosmological data
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Observation 2687960f-631f-42c6-9589-5edc1bd018ca · outbound
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Accurate method for ultralight axion CMB and matter power spectra The DESI Experiment Part I: Science,Targeting, and Survey Design
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Observation 642e9068-9852-4766-bd3d-91227e39f61b · outbound
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Accurate method for ultralight axion CMB and matter power spectra How sound are our ultra-light axion approximations?
Reference 44
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Observation f891e271-410b-4852-8d95-2583ce511092 · outbound
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Accurate method for ultralight axion CMB and matter power spectra Ratra, Phys
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Observation 44f7a7bd-23fa-4285-b038-f2d8bdb68a3e · outbound
This paper cites Implications of multi-axion dark matter on structure formation.
Accurate method for ultralight axion CMB and matter power spectra Implications of multi-axion dark matter on structure formation
Reference 46
- Resolution
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Observation 8fce5de9-d33a-4abb-8dbc-a386f1b287d2 · outbound
This paper cites Accurate effective fluid approximation for ultralight axions.
Accurate method for ultralight axion CMB and matter power spectra Accurate effective fluid approximation for ultralight axions
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- Resolution
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Observation a9a5aa9e-49f0-4ed7-b550-b0326141ec22 · outbound
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Accurate method for ultralight axion CMB and matter power spectra Cosmology with varying fundamental constants from hyperlight, coupled scalars
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- Resolution
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Accurate method for ultralight axion CMB and matter power spectra The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
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- Resolution
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Observation 57ff70be-7406-4e01-8167-077a0f4a13eb · outbound
This paper cites Cosmological signatures of ultralight dark matter with an axionlike potential.
Accurate method for ultralight axion CMB and matter power spectra Cosmological signatures of ultralight dark matter with an axionlike potential
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- Resolution
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Observation f5fadf41-f204-49ec-b58f-38adb9a22dc3 · outbound
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Accurate method for ultralight axion CMB and matter power spectra Towards accurate cosmological predictions for rapidly oscillating scalar fields as dark matter
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- Resolution
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Source-reported events for the cited work
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Accurate method for ultralight axion CMB and matter power spectra Planck 2018 results. VI. Cosmological parameters
Reference 52
- Resolution
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Source-reported events for the cited work
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This paper cites On the cosmological evolution of Scalar Field Dark Matter in the $\texttt{CLASS}$ code: accuracy and precision of numerical solutions.
Accurate method for ultralight axion CMB and matter power spectra On the cosmological evolution of Scalar Field Dark Matter in the $\texttt{CLASS}$ code: accuracy and precision of numerical solutions
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Unavailable: canonical work link unavailable.
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Accurate method for ultralight axion CMB and matter power spectra Separating the Universe into the Real and Fake
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Source-reported events for the cited work
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This paper cites Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges.
Accurate method for ultralight axion CMB and matter power spectra Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges
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Accurate method for ultralight axion CMB and matter power spectra Fast and accurate CMB computations in non-flat FLRW universes
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Observation dc06bc52-9820-43d8-8f2d-d699beb05db1 · outbound
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Accurate method for ultralight axion CMB and matter power spectra Hu, Astrophys
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Observation ab3545b5-afd0-4561-8da3-8018a1772ef0 · outbound
This paper cites switch source.
Accurate method for ultralight axion CMB and matter power spectra switch source
Reference 58
- Resolution
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- raw_fallback, observed 2026-08-11T11:39:00.099861Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 46baa0ee-e4a7-472f-8bee-adcd7a078a68 · outbound
This paper cites A Complete Treatment of CMB Anisotropies in a FRW Universe.
Accurate method for ultralight axion CMB and matter power spectra A Complete Treatment of CMB Anisotropies in a FRW Universe
Reference 59
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T11:38:58.930210Z
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Observation 99afaa37-2954-418d-9c13-89be5af8918d · outbound
This paper cites A Line of Sight Approach to Cosmic Microwave Background Anisotropies.
Accurate method for ultralight axion CMB and matter power spectra A Line of Sight Approach to Cosmic Microwave Background Anisotropies
Reference 60
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T11:38:58.933901Z
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Observation 827a7001-be6c-4328-b7a7-ff7776ee8354 · outbound
This paper cites The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview.
Accurate method for ultralight axion CMB and matter power spectra The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview
Reference 61
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T11:38:58.937578Z
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Observation 5272aabc-c2c4-4f10-b363-5765531194b1 · outbound
This paper cites Cosmic Complementarity: Joint Parameter Estimation from CMB Experiments and Redshift Surveys.
Accurate method for ultralight axion CMB and matter power spectra Cosmic Complementarity: Joint Parameter Estimation from CMB Experiments and Redshift Surveys
Reference 62
- Resolution
- verified exact
- local_arxiv, observed 2026-08-11T11:38:59.008951Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation da11d578-583d-4b0e-821f-8bdfec74d999 · outbound
This paper cites Strong bound on canonical ultra-light axion dark matter from the Lyman-alpha forest.
Accurate method for ultralight axion CMB and matter power spectra Strong bound on canonical ultra-light axion dark matter from the Lyman-alpha forest
Reference 63
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T11:38:58.944861Z
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Observation 11f935a8-9bd1-4b79-8f94-efe1514965b2 · outbound
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Accurate method for ultralight axion CMB and matter power spectra Dark Matter from an ultra-light pseudo-Goldsone-boson
Reference 64
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T11:38:58.948485Z
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Pith citing papers
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A Fast and Accurate Implementation of the Effective Fluid Approximation for Ultralight Axions Accurate method for ultralight axion CMB and matter power spectra
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T15:47:01.419967Z
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Observation 1dc2a2a9-24ef-4bbf-a87a-14c9d5ef79de · inbound
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Ultralight fuzzy dark matter review Accurate method for ultralight axion CMB and matter power spectra
Reference 150
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T21:18:59.210017Z
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Observation 84990f65-209d-4c57-ac2e-41324bace7e5 · inbound
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Reference 14
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T20:39:28.872834Z
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Observation ddbbaa05-34c0-44c7-b8d2-93bac0775b3f · inbound
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Wavelet-Scattering Signatures of Fuzzy Dark Matter in Simulated 21 cm Brightness-Temperature Maps Accurate method for ultralight axion CMB and matter power spectra
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T19:30:09.411332Z
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Observation 811b352f-1367-4ffe-bff8-cadf090cd9be · inbound
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Reference 68
- Resolution
- verified exact
- arxiv_id, observed 2026-07-27T00:19:42.406886Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation a1d58d98-23d3-4796-aa34-9ca514772948 · inbound
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Inflationary Axion Isocurvature in the CMB across All Ultralight Masses Accurate method for ultralight axion CMB and matter power spectra
Reference 40
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T04:22:44.388067Z
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