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Paper Citation Record · LEDGER

Cosmological parameters from the likelihood analysis of the galaxy power spectrum and bispectrum in real space

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2108.03204.

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

pith.paper-citation-record.v1
2108.03204 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T22:58:55.305549Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-23T22:35:50.803500Z

Reference resolution

0 of 0 outbound references displayed

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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 11df7995-d5bb-429f-9309-cbf938ba0f38 · inbound

Modeling and measuring the anisotropic halo 3-point correlation function: a coordinated study cites this paper.

Modeling and measuring the anisotropic halo 3-point correlation function: a coordinated study Cosmological parameters from the likelihood analysis of the galaxy power spectrum and bispectrum in real space

Reference 88

Resolution
verified exact
arxiv_id, observed 2026-05-23T22:35:50.806310Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

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Observation 3b12ff23-77f4-48d1-886f-065a367460d3 · inbound

Boosting galaxy clustering analyses with non-perturbative modelling of redshift-space distortions cites this paper.

Boosting galaxy clustering analyses with non-perturbative modelling of redshift-space distortions Cosmological parameters from the likelihood analysis of the galaxy power spectrum and bispectrum in real space

Reference 122

Resolution
unresolved
no resolver link, observed 2026-08-09T22:58:55.305549Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T22:58:55.305549Z digest=sha256:fa5dd5b96cfb95f98eeaa940509c1a1b1374ce3081206f90d79cc09d4347b30a

Observation 0b21aced-9ee3-454b-a162-0df17a16ed8f · inbound

Equivalence of the field-level inference and conventional analyses on large scales cites this paper.

Equivalence of the field-level inference and conventional analyses on large scales Cosmological parameters from the likelihood analysis of the galaxy power spectrum and bispectrum in real space

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-06T19:34:10.689472Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation b64daefb-7c5a-420d-ad48-ecb95e19c8dd · inbound

One-Loop Galaxy Bispectrum: Consistent Theory, Efficient Analysis with COBRA, and Implications for Cosmological Parameters cites this paper.

One-Loop Galaxy Bispectrum: Consistent Theory, Efficient Analysis with COBRA, and Implications for Cosmological Parameters Cosmological parameters from the likelihood analysis of the galaxy power spectrum and bispectrum in real space

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-06T12:12:39.620851Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T12:12:39.620851Z digest=sha256:5cdf88fcec35f942a364077d0eb7a4f6d34adfcc10747be23f87aab1f723eb1f

Observation 6f126e97-4457-4a8a-8358-52c23b2c92f5 · 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 Cosmological parameters from the likelihood analysis of the galaxy power spectrum and bispectrum in real space

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-04T18:59:20.243398Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T18:59:20.243398Z digest=sha256:f8d13249b515efe95b770846aa0e01fa26a95e9ef7fd6ae2ab71b20ffd2a4f28