Paper Citation Record · LEDGER

Analysis of Unified Galaxy Power Spectrum Multipole Measurements

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2307.07475.

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

pith.paper-citation-record.v1
2307.07475 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T22:24:26.829326Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T06:27:41.770221Z

Reference resolution

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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 2bc19a5b-ddeb-4336-8f4b-860dc26f5c5f · 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 Analysis of Unified Galaxy Power Spectrum Multipole Measurements

Reference 157

Resolution: verified exact; arxiv_id, observed 2026-05-17T06:00:49.966497Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation e1c4437e-c4bd-4a99-add2-5e9b89a38d69 · inbound

DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements cites this paper.

DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements Analysis of Unified Galaxy Power Spectrum Multipole Measurements

Reference 44

Resolution: verified exact; arxiv_id, observed 2026-05-15T21:36:41.870334Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation d6ba88b7-99c3-43c5-87de-ea552f5d2958 · inbound

Reducing nuisance prior sensitivity via non-linear reparameterization, with application to EFT analyses of large-scale structure cites this paper.

Reducing nuisance prior sensitivity via non-linear reparameterization, with application to EFT analyses of large-scale structure Analysis of Unified Galaxy Power Spectrum Multipole Measurements

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-11T22:24:26.829326Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 323b3788-46bb-430b-abdf-5b16702974ba · inbound

$\Lambda$CDM and early dark energy in latent space: a data-driven parametrization of the CMB temperature power spectrum cites this paper.

$\Lambda$CDM and early dark energy in latent space: a data-driven parametrization of the CMB temperature power spectrum Analysis of Unified Galaxy Power Spectrum Multipole Measurements

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-07T20:33:58.302756Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9f062b8e-e2b8-4c01-aedb-e3e7dfbea6ab · inbound

Debiasing inference in large-scale structure with non-flat volume measures cites this paper.

Debiasing inference in large-scale structure with non-flat volume measures Analysis of Unified Galaxy Power Spectrum Multipole Measurements

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-06T13:22:38.602224Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d3971ca6-49c6-4377-bab2-1929320164c3 · inbound

The simple way to measure evolving dark energy without prior-volume effects cites this paper.

The simple way to measure evolving dark energy without prior-volume effects Analysis of Unified Galaxy Power Spectrum Multipole Measurements

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-04T18:59:15.458972Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8c04a651-1421-4a7b-8ff8-9bfb33a2886c · inbound

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

Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization Analysis of Unified Galaxy Power Spectrum Multipole Measurements

Reference 96

Resolution: verified exact; arxiv_id, observed 2026-07-03T06:27:41.772454Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation f1a87149-e7cf-4876-8f66-e6bb5ec728ce · inbound

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

Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization Analysis of Unified Galaxy Power Spectrum Multipole Measurements

Reference 96

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.