Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-15T16:34:58.318429Z
Paper Citation Record · LEDGER
Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm I}$: 1-Loop Corrections involving Second-Order Densities
As of 18 August 2026, this Paper Citation Record lists 21 of 21 outbound references and 0 inbound Pith citation observations for arXiv:2509.05419.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
21 of 21 outbound references displayed
- verified exact0
- verified fuzzy2
- unresolved19
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation ddde20f7-30dc-4bf6-b686-28e1115d4305 · 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 ${\rm I}$: 1-Loop Corrections involving Second-Order Densities Large-scale structure of the universe and cosmological perturbation theory,
Reference 1
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T16:34:58.220058Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a2cc96bc-1f4f-47f1-9fbd-fd88db3d3c01 · 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 ${\rm I}$: 1-Loop Corrections involving Second-Order Densities Non-Gaussian covariance of the matter power spectrum in the effective field theory of large scale structure,
Reference 2
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T16:34:58.224668Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 85a483d1-929b-41a0-b217-0c75669bd3d9 · 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 ${\rm I}$: 1-Loop Corrections involving Second-Order Densities Isotropic N-point basis functions and their properties,
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T16:34:58.229085Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ff74ecbb-cb55-4d75-82d2-5825f8124ec1 · 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 ${\rm I}$: 1-Loop Corrections involving Second-Order Densities Test for Cosmological Parity Violation Using the 3D Distribution of Galaxies,
Reference 4
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T16:34:58.233435Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b4fd85c9-6842-496c-87cf-4375c18d5e66 · 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 ${\rm I}$: 1-Loop Corrections involving Second-Order Densities Triple-spherical Bessel function integrals with exponential and Gaussian damping: towards an analytic N-point correlation function covariance model,
Reference 5
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T16:34:58.238380Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9597d369-9da7-4d5f-b136-c42037e057ab · 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 ${\rm I}$: 1-Loop Corrections involving Second-Order Densities DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 6
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T16:34:58.242708Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c974350e-fe5c-43ee-b0d2-b766849602a5 · outbound
This paper cites http://dlmf.nist.gov/.
Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm I}$: 1-Loop Corrections involving Second-Order Densities http://dlmf.nist.gov/
Reference 7
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T16:34:58.248408Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 75d200b8-e127-43ae-9f47-71d82cdaf443 · 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 ${\rm I}$: 1-Loop Corrections involving Second-Order Densities Analytic Gaussian covariance matrices for galaxy N -point correlation functions,
Reference 8
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T16:34:58.253298Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4b63520b-6e87-4fdf-ae6a-500dcd529578 · outbound
This paper cites an unresolved cited work.
Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm I}$: 1-Loop Corrections involving Second-Order Densities Unresolved cited work
Reference 9
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T16:34:58.257416Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 24806b2c-db52-4d23-a32e-af42eb424c0f · 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 ${\rm I}$: 1-Loop Corrections involving Second-Order Densities Study of the Connected Four-Point Correlation Function of Galaxies from DESI Data Release 1 Luminous Red Galaxy Sample
Reference 10
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T16:34:58.261194Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c97dc458-aa10-486a-a1b2-49a37283cb54 · 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 ${\rm I}$: 1-Loop Corrections involving Second-Order Densities Neutrino Mass Signatures in the Galaxy Bispectrum
Reference 11
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T16:34:58.265327Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f9eabb96-d874-4c1b-9dd3-4c14f6d06bde · 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 ${\rm I}$: 1-Loop Corrections involving Second-Order Densities Perturbative approach to covariance matrix of the matter power spectrum,
Reference 12
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T16:34:58.272490Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7df591c2-728d-4284-a074-e4ec7ce5af8b · 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 ${\rm I}$: 1-Loop Corrections involving Second-Order Densities A Model for the Redshift-Space Galaxy 4-Point Correlation Function
Reference 13
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T16:34:58.276684Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7d4bfcb7-0578-4309-8b39-f18ee73cb788 · outbound
This paper cites Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field II: 1-loop Corrections with Third-Order Densities,.
Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field ${\rm I}$: 1-Loop Corrections involving Second-Order Densities Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field II: 1-loop Corrections with Third-Order Densities,
Reference 14
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T16:34:58.530574Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 99a5e639-10ac-44e8-955e-e6b89bb9ecba · 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 ${\rm I}$: 1-Loop Corrections involving Second-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 2026-08-15T16:34:58.289299Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9c05526b-07a4-4318-9ea3-520bebdeb8d6 · 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 ${\rm I}$: 1-Loop Corrections involving Second-Order Densities Probing parity violation with the four-point correlation function of BOSS galaxies,
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T16:34:58.294059Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6dc5b4c3-650e-4ee7-a918-87e24adf5f18 · 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 ${\rm I}$: 1-Loop Corrections involving Second-Order Densities The Bispectrum as a Signature of Gravitational Instability in Redshift Space,
Reference 17
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T16:34:58.299152Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d7bf81a3-bb8d-423e-953d-8da82e40640b · 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 ${\rm I}$: 1-Loop Corrections involving Second-Order Densities On a generating function for the isotropic basis functions and other connected results,
Reference 18
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T16:34:58.303464Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7f8cda0c-4211-4e24-82fa-ac3d76d0be12 · 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 ${\rm I}$: 1-Loop Corrections involving Second-Order Densities Modeling the large-scale redshift-space 3-point correlation function of galaxies,
Reference 19
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T16:34:58.308512Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d875017b-82a0-4cd9-a313-2596e254644b · 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 ${\rm I}$: 1-Loop Corrections involving Second-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 2026-08-15T16:34:58.313123Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 021dd1d4-a623-490d-b611-bbc4f243b6d7 · 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 ${\rm I}$: 1-Loop Corrections involving Second-Order Densities Galaxy power spectrum multipoles covariance in perturbation theory,
Reference 21
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T16:34:58.478365Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Pith citing papers
No inbound Pith citation observations are available.