Paper Citation Record · LEDGER

Clustering in Massive Neutrino Cosmologies via Eulerian Perturbation Theory

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2106.13771.

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

pith.paper-citation-record.v1
2106.13771 v2

Coverage vector

measured 0 of 0 reference resolution

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measured 11 of 11 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T04:59:58.804936Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T06:27:41.763658Z

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 33f8b87a-570b-4019-b71a-a3f29d4f1925 · inbound

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

DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Clustering in Massive Neutrino Cosmologies via Eulerian Perturbation Theory

Reference 137

Resolution: verified exact; arxiv_id, observed 2026-05-17T06:00:49.888796Z

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Observation 5fc54375-1586-4a38-a0fe-922ef7da6a93 · inbound

Fullshape power spectrum for the Symmetron modified gravity model cites this paper.

Fullshape power spectrum for the Symmetron modified gravity model Clustering in Massive Neutrino Cosmologies via Eulerian Perturbation Theory

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-07T04:59:58.804936Z

Source-reported events for the cited work

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Observation 0dc17b87-143a-4301-b62d-21634324406d · inbound

Tracing Signatures of Modified Gravity in Redshift-Space Galaxy Bispectrum Multipoles: Prospects for Euclid cites this paper.

Tracing Signatures of Modified Gravity in Redshift-Space Galaxy Bispectrum Multipoles: Prospects for Euclid Clustering in Massive Neutrino Cosmologies via Eulerian Perturbation Theory

Reference 115

Resolution: verified exact; arxiv_id, observed 2026-05-18T21:31:52.129473Z

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Observation a0bd828a-47ef-4cbd-b5d0-c39086870260 · inbound

Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy cites this paper.

Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy Clustering in Massive Neutrino Cosmologies via Eulerian Perturbation Theory

Reference 143

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Source-reported events for the cited work

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Observation d8be63b6-47a1-4d2e-9ea3-955051680169 · inbound

FolpsD: combining EFT and phenomenological approaches for joint power spectrum and bispectrum analyses cites this paper.

FolpsD: combining EFT and phenomenological approaches for joint power spectrum and bispectrum analyses Clustering in Massive Neutrino Cosmologies via Eulerian Perturbation Theory

Reference 60

Resolution: verified exact; arxiv_id, observed 2026-05-11T06:25:59.313950Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation a9f00086-c8b8-4998-8df0-7f41f29ede2d · inbound

Forecasting neutrino mass constraints from the Nancy Grace Roman Space Telescope cites this paper.

Forecasting neutrino mass constraints from the Nancy Grace Roman Space Telescope Clustering in Massive Neutrino Cosmologies via Eulerian Perturbation Theory

Reference 22

Resolution: verified exact; arxiv_id, observed 2026-05-10T10:49:56.983710Z

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No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation b3d3717c-4f76-46b2-8030-9c833420fbeb · inbound

Testing Scale-Dependent Modified Gravity with DESI DR1 cites this paper.

Testing Scale-Dependent Modified Gravity with DESI DR1 Clustering in Massive Neutrino Cosmologies via Eulerian Perturbation Theory

Reference 63

Resolution: verified exact; arxiv_id, observed 2026-05-12T09:21:26.272107Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 6fee8006-c367-4a34-82c2-f9d1fbb9e494 · inbound

Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges cites this paper.

Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges Clustering in Massive Neutrino Cosmologies via Eulerian Perturbation Theory

Reference 72

Resolution: metadata mismatch; arxiv_id, observed 2026-05-11T17:56:05.833629Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation e9b16065-5bb7-4729-ba76-5e1fadf68ecf · inbound

Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges cites this paper.

Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges Clustering in Massive Neutrino Cosmologies via Eulerian Perturbation Theory

Reference 80

Resolution: metadata mismatch; arxiv_id, observed 2026-06-30T23:25:07.669584Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation a0f7b58d-fd7e-4470-8d9c-852637e00342 · inbound

Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization cites this paper.

Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization Clustering in Massive Neutrino Cosmologies via Eulerian Perturbation Theory

Reference 56

Resolution: verified exact; arxiv_id, observed 2026-07-03T06:27:41.768889Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation b7c5a5ee-660b-4108-ae71-2fccf8535878 · inbound

Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization cites this paper.

Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization Clustering in Massive Neutrino Cosmologies via Eulerian Perturbation Theory

Reference 56

Resolution: unresolved; no resolver link, observed 2026-07-12T08:00:27.085537Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.