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Paper Citation Record · LEDGER

Exact Modeling of Power Spectrum Multipole through Spherical Fourier-Bessel Basis

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2404.04812.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2404.04812 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T05:21:13.711412Z

measured 1 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

0
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation e810f4dc-7835-437b-8aaf-c6e66c17ac4c · inbound

Primordial non-Gaussianity -- the effects of relativistic and wide-angle corrections to the power spectrum cites this paper.

Primordial non-Gaussianity -- the effects of relativistic and wide-angle corrections to the power spectrum Exact Modeling of Power Spectrum Multipole through Spherical Fourier-Bessel Basis

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-11T19:40:39.048758Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T19:40:39.048758Z digest=sha256:bd4113925d01afe407eb93c10f90c051ec1dc068b8128b03a7a91f9db641ad76

Observation f6ea0ca8-57a4-44df-a96e-8b8ab4111328 · inbound

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation cites this paper.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Exact Modeling of Power Spectrum Multipole through Spherical Fourier-Bessel Basis

Reference 85

Resolution
unresolved
no resolver link, observed 2026-08-16T05:21:13.711412Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T05:21:13.711412Z digest=sha256:a8510e37855ff9a276520b35960a235357bbcc93f05491bcd6203546869483e6

Observation 8d290482-0828-454f-9504-1f9ed4824b9b · inbound

Separating Angular and Radial Modes with Spherical-Fourier Bessel Power Spectrum on All Scales and Implications for Systematics Mitigation cites this paper.

Separating Angular and Radial Modes with Spherical-Fourier Bessel Power Spectrum on All Scales and Implications for Systematics Mitigation Exact Modeling of Power Spectrum Multipole through Spherical Fourier-Bessel Basis

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-07T05:55:49.308368Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T05:55:49.308368Z digest=sha256:cab2bc9981b2b4690abe72d77fa03dab648d630c7aa5d51dd6f930b0384c2c3b

Observation 52cc1290-73a4-4668-952f-061e914a585d · inbound

Large-scale Modeling of the Observed Power Spectrum Multipoles cites this paper.

Large-scale Modeling of the Observed Power Spectrum Multipoles Exact Modeling of Power Spectrum Multipole through Spherical Fourier-Bessel Basis

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-04T06:23:22.493842Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T06:23:22.493842Z digest=sha256:89c0c2b70f891afe4514ee0672a7a1ba2762b9827c788c21f3de2cc41e5cc483

Observation d1260d01-9699-45b7-bf2c-56f0c5d255f7 · inbound

The observer power spectrum for lightcone statistics, integrated relativistic observables and wide angle effects cites this paper.

The observer power spectrum for lightcone statistics, integrated relativistic observables and wide angle effects Exact Modeling of Power Spectrum Multipole through Spherical Fourier-Bessel Basis

Reference 34

Resolution
verified exact
arxiv_id, observed 2026-06-29T14:53:32.218070Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-06-29T06:12:10.521465Z digest=sha256:b026dae1155f832bea8974c7c47900f5ecf8d39f47de772f0cef1201a4cfa7bf

Observation 5d3aa311-ef6b-4e56-9a7f-cc30659d3709 · inbound

The observer power spectrum for lightcone statistics, integrated relativistic observables and wide angle effects cites this paper.

The observer power spectrum for lightcone statistics, integrated relativistic observables and wide angle effects Exact Modeling of Power Spectrum Multipole through Spherical Fourier-Bessel Basis

Reference 34

Resolution
unresolved
no resolver link, observed 2026-07-14T18:39:20.634979Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T18:39:20.634979Z digest=sha256:8f5757ec77035fe64832d09bd1a7703a3ba1993f7b0bed48c72f339478946898

Observation 020d079f-ee44-44d1-b47b-fad5fc456d55 · inbound

First full-shape joint analysis of the two- and three-point correlation functions on real data: $\Lambda$CDM cosmological constraints from BOSS DR12 cites this paper.

First full-shape joint analysis of the two- and three-point correlation functions on real data: $\Lambda$CDM cosmological constraints from BOSS DR12 Exact Modeling of Power Spectrum Multipole through Spherical Fourier-Bessel Basis

Reference 190

Resolution
metadata mismatch
arxiv_id, observed 2026-06-26T01:38:51.689394Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-06-26T01:35:05.451125Z digest=sha256:1b3d9c3efaec00b4d4481400bb5d094905a148c431eb6df62f6805276ce3c136

Observation de7fca30-dc59-4747-85ae-a145699fb5f6 · inbound

Optimal and exact wide-angle power spectrum estimation cites this paper.

Optimal and exact wide-angle power spectrum estimation Exact Modeling of Power Spectrum Multipole through Spherical Fourier-Bessel Basis

Reference 34

Resolution
unresolved
no resolver link, observed 2026-07-11T06:32:08.971654Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-11T06:32:08.971654Z digest=sha256:143d70bd8d2e7cfda0ea9761ee352cc1ebd05cc5a52a68b2d987801b02d696fd

Observation 43ae758a-6c59-4378-886e-2a2515f2f562 · inbound

Impact and measurability of linear relativistic effects in galaxy surveys cites this paper.

Impact and measurability of linear relativistic effects in galaxy surveys Exact Modeling of Power Spectrum Multipole through Spherical Fourier-Bessel Basis

Reference 131

Resolution
verified exact
local_arxiv, observed 2026-07-10T23:17:42.383465Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-07-10T23:12:29.350615Z digest=sha256:c8b43a74851af8736365fd5bb68f189de086a1a625de65d3f2818d8decd7eabd

Observation 53d10cba-f478-4260-bed8-85b8a8875019 · inbound

Beyond {\Lambda}CDM with the SKA Observatory -- II: Unveiling the Secrets of the Early Universe cites this paper.

Beyond {\Lambda}CDM with the SKA Observatory -- II: Unveiling the Secrets of the Early Universe Exact Modeling of Power Spectrum Multipole through Spherical Fourier-Bessel Basis

Reference 23

Resolution
metadata mismatch
local_arxiv, observed 2026-07-10T04:46:46.011218Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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