Paper Citation Record · LEDGER

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities

As of 7 August 2026, this Paper Citation Record lists 21 of 21 outbound references and 0 inbound Pith citation observations for arXiv:2509.05422.

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

pith.paper-citation-record.v1
2509.05422 v1

Coverage vector

measured 21 of 21 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-05T05:30:26.015679Z

measured 21 of 21 standing notices

One-hop event checks from named stored sources.

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measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

21 of 21 outbound references displayed

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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 9a08e36e-5213-427e-a651-1c27564da509 · outbound

This paper cites Large-scale structure of the universe and cosmological perturbation theory,.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities Large-scale structure of the universe and cosmological perturbation theory,

Reference 1

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T05:30:26.280884Z

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No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 2546a689-041c-4ddb-a825-593222a244e3 · outbound

This paper cites Non-Gaussian covariance of the matter power spectrum in the effective field theory of large scale structure,.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities Non-Gaussian covariance of the matter power spectrum in the effective field theory of large scale structure,

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T05:30:26.270003Z

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No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 710150d5-edb4-45b1-b710-1a8834d4d730 · outbound

This paper cites Isotropic N-point basis functions and their properties,.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities Isotropic N-point basis functions and their properties,

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T05:30:26.259406Z

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Observation ce42e379-67ea-40e7-b492-f207af95ad8c · outbound

This paper cites Test for Cosmological Parity Violation Using the 3D Distribution of Galaxies,.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities Test for Cosmological Parity Violation Using the 3D Distribution of Galaxies,

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T05:30:26.247513Z

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Observation 92d5c0d7-5193-4721-8211-d47f9ee3235b · outbound

This paper cites Triple-spherical Bessel function integrals with exponential and Gaussian damping: towards an analytic N-point correlation function covariance model,.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities Triple-spherical Bessel function integrals with exponential and Gaussian damping: towards an analytic N-point correlation function covariance model,

Reference 5

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T05:30:26.236040Z

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No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 67947a91-9e3c-491d-b66b-1f3310f4b202 · outbound

This paper cites DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-05T05:30:25.962500Z

Source-reported events for the cited work

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Observation b3d74592-c0e6-4e90-8575-59272c1cc216 · outbound

This paper cites http://dlmf.nist.gov/.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities http://dlmf.nist.gov/

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T05:30:26.223297Z

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Observation 22b8b825-6db0-4c3f-889e-f500f4e1890d · outbound

This paper cites Analytic Gaussian covariance matrices for galaxy N -point correlation functions,.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities Analytic Gaussian covariance matrices for galaxy N -point correlation functions,

Reference 8

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T05:30:26.211763Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation d158110b-83d9-40a0-b59c-bd13e5e67866 · outbound

This paper cites an unresolved cited work.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities Unresolved cited work

Reference 9

Resolution: unresolved; raw_fallback, observed 2026-08-05T05:30:26.199975Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation c7a0429d-6796-47e4-be64-8646e62a91d9 · outbound

This paper cites Study of the Connected Four-Point Correlation Function of Galaxies from DESI Data Release 1 Luminous Red Galaxy Sample.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities Study of the Connected Four-Point Correlation Function of Galaxies from DESI Data Release 1 Luminous Red Galaxy Sample

Reference 10

Resolution: verified exact; local_arxiv, observed 2026-08-05T05:30:26.094750Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation e1d62158-dedd-4a47-9863-358e1205752b · outbound

This paper cites Neutrino Mass Signatures in the Galaxy Bispectrum.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities Neutrino Mass Signatures in the Galaxy Bispectrum

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-05T05:30:25.981979Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c999b97d-03bd-4dc4-aa6d-5fde19845439 · outbound

This paper cites Perturbative approach to covariance matrix of the matter power spectrum,.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities Perturbative approach to covariance matrix of the matter power spectrum,

Reference 12

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T05:30:26.188305Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation e2cb66a6-7e40-435c-9be4-b59b6b02fff8 · outbound

This paper cites A Model for the Redshift-Space Galaxy 4-Point Correlation Function.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities A Model for the Redshift-Space Galaxy 4-Point Correlation Function

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-05T05:30:25.989136Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9334209a-6c96-40c9-aaad-b265d9681358 · outbound

This paper cites Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field I: 1-Loop Corrections with Second-Order Densities,.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field I: 1-Loop Corrections with Second-Order Densities,

Reference 14

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T05:30:26.176292Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation c1a0e7e4-bf3b-47c6-8e6e-446044310d45 · outbound

This paper cites A First Detection of the Connected 4-Point Correlation Function of Galaxies Using the BOSS CMASS Sample.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities A First Detection of the Connected 4-Point Correlation Function of Galaxies Using the BOSS CMASS Sample

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-05T05:30:25.995833Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 50199ee0-d35b-4c80-810e-e371dc853a0f · outbound

This paper cites Probing parity violation with the four-point correlation function of BOSS galaxies,.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities Probing parity violation with the four-point correlation function of BOSS galaxies,

Reference 16

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T05:30:26.163731Z

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No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 3b9979bc-a605-43ce-99a7-7515bf93d8f1 · outbound

This paper cites The Bispectrum as a Signature of Gravitational Instability in Redshift Space,.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities The Bispectrum as a Signature of Gravitational Instability in Redshift Space,

Reference 17

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T05:30:26.150979Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 71607c0d-6c35-40cf-a71b-9fdc2e2f36b5 · outbound

This paper cites On a generating function for the isotropic basis functions and other connected results,.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities On a generating function for the isotropic basis functions and other connected results,

Reference 18

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T05:30:26.139958Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 14a703f9-556a-4852-a8ae-e9b4d60549e1 · outbound

This paper cites Modeling the large-scale redshift-space 3-point correlation function of galaxies,.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities Modeling the large-scale redshift-space 3-point correlation function of galaxies,

Reference 19

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T05:30:26.128739Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 19bb9ceb-7191-40f9-b8c6-c0758fea1c8e · outbound

This paper cites Measurement of Parity-Violating Modes of the Dark Energy Spectroscopic Instrument (DESI) Year 1 Luminous Red Galaxies' 4-Point Correlation Function.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities Measurement of Parity-Violating Modes of the Dark Energy Spectroscopic Instrument (DESI) Year 1 Luminous Red Galaxies' 4-Point Correlation Function

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-05T05:30:26.012194Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f1874520-d998-4d2b-962b-5ab62de366e2 · outbound

This paper cites Galaxy power spectrum multipoles covariance in perturbation theory,.

Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm II}$: 1-Loop Corrections with Third-Order Densities Galaxy power spectrum multipoles covariance in perturbation theory,

Reference 21

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T05:30:26.117514Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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