Paper Citation Record · LEDGER

How much information can be extracted from galaxy clustering at the field level?

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 17 inbound Pith citation observations for arXiv:2403.03220.

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

pith.paper-citation-record.v1
2403.03220 v3

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measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 17 of 17 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 17 of 17 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T05:50:31.640171Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

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External citation measurements

5
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 3150e3df-53c9-4c47-8e76-56f8dce1a98d · inbound

Renormalized Perturbation Theory at Field-level: the LSS bootstrap in GridSPT cites this paper.

Renormalized Perturbation Theory at Field-level: the LSS bootstrap in GridSPT How much information can be extracted from galaxy clustering at the field level?

Reference 33

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Observation c7e36254-7807-48ed-b316-6b70830a3760 · inbound

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors cites this paper.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors How much information can be extracted from galaxy clustering at the field level?

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-06T21:30:54.695470Z

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Observation 06008e1c-5177-4962-99da-7291c759b23a · inbound

Modeling the Cosmological Lyman-$\alpha$ Forest at the Field Level cites this paper.

Modeling the Cosmological Lyman-$\alpha$ Forest at the Field Level How much information can be extracted from galaxy clustering at the field level?

Reference 59

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Observation c6502973-84ab-49ce-8fdd-42e11359b7f0 · 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 How much information can be extracted from galaxy clustering at the field level?

Reference 36

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Observation f34d5994-1dcb-41f1-9594-415c438d8c65 · inbound

Two-loop renormalization and running of galaxy bias cites this paper.

Two-loop renormalization and running of galaxy bias How much information can be extracted from galaxy clustering at the field level?

Reference 29

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Observation d90bad49-25c2-4bec-8921-e998727c9d9f · 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 How much information can be extracted from galaxy clustering at the field level?

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-06T13:22:38.718671Z

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Observation 8f6a79a9-ab29-4af4-ac5d-b8c7f2e70a3a · inbound

DISCO-DJ II: a differentiable particle-mesh code for cosmology cites this paper.

DISCO-DJ II: a differentiable particle-mesh code for cosmology How much information can be extracted from galaxy clustering at the field level?

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-04T11:25:25.514689Z

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Observation d5aa0274-2149-4fc1-ada5-4c647561f743 · inbound

Field-level likelihood for projected fields: Evolved projected fields from initial projected fields cites this paper.

Field-level likelihood for projected fields: Evolved projected fields from initial projected fields How much information can be extracted from galaxy clustering at the field level?

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-04T09:46:17.103168Z

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Observation d4e7a9a8-51f4-481e-80af-b2abf52747a2 · inbound

Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation cites this paper.

Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation How much information can be extracted from galaxy clustering at the field level?

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-03T23:38:16.829576Z

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Observation 033123f8-800a-4fd3-b280-7881265a5feb · inbound

On the Relation Between Field-Level Posteriors, Correlators, and their Likelihoods cites this paper.

On the Relation Between Field-Level Posteriors, Correlators, and their Likelihoods How much information can be extracted from galaxy clustering at the field level?

Reference 23

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Observation 0b5e89fb-0412-4506-94f0-aa725eaf3b2b · inbound

Probing nonlinear structure formation beyond $\Lambda$CDM with the LSS bootstrap: a joint power spectrum and bispectrum analysis cites this paper.

Probing nonlinear structure formation beyond $\Lambda$CDM with the LSS bootstrap: a joint power spectrum and bispectrum analysis How much information can be extracted from galaxy clustering at the field level?

Reference 58

Resolution: verified exact; arxiv_id, observed 2026-05-14T17:42:32.802578Z

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 abf1f01f-267e-45f6-9bbe-546cb53b0aac · inbound

Field-level vs summaries: convergence of information in non-Gaussian density fields cites this paper.

Field-level vs summaries: convergence of information in non-Gaussian density fields How much information can be extracted from galaxy clustering at the field level?

Reference 13

Resolution: verified exact; arxiv_id, observed 2026-07-03T22:49:01.233759Z

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Observation 574ebee4-39cc-4e5b-b247-63a71700b921 · inbound

Lyman-Alpha Forest and its Cross-Correlation with High-Redshift Galaxies in Effective Field Theory at the Field Level cites this paper.

Lyman-Alpha Forest and its Cross-Correlation with High-Redshift Galaxies in Effective Field Theory at the Field Level How much information can be extracted from galaxy clustering at the field level?

Reference 204

Resolution: verified exact; arxiv_id, observed 2026-07-04T15:19:57.117120Z

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 526a854f-bb53-41b5-9f27-23181445859c · inbound

First full-shape joint analysis of the two- and three-point correlation functions on real data: $\Lambda$CDM cosmological constraints from BOSS DR12 cites this paper.

First full-shape joint analysis of the two- and three-point correlation functions on real data: $\Lambda$CDM cosmological constraints from BOSS DR12 How much information can be extracted from galaxy clustering at the field level?

Reference 227

Resolution: metadata mismatch; arxiv_id, observed 2026-06-26T01:38:51.631934Z

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 6660cf96-bacf-4e86-8ca2-7a3afb7b6a92 · inbound

Emulating Cosmic Structure Formation with a Lagrangian Neural Cellular Automaton cites this paper.

Emulating Cosmic Structure Formation with a Lagrangian Neural Cellular Automaton How much information can be extracted from galaxy clustering at the field level?

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-01T09:37:45.309457Z

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Observation 5a31f242-3922-43d3-bb19-0c17c92a6677 · inbound

GGI Lectures on Large-Scale Structure Perturbation Theory (Effective Field Theory) cites this paper.

GGI Lectures on Large-Scale Structure Perturbation Theory (Effective Field Theory) How much information can be extracted from galaxy clustering at the field level?

Reference 152

Resolution: unresolved; no resolver link, observed 2026-07-31T11:32:44.916759Z

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Observation 04236630-a759-48ba-9515-ff0ad903070a · inbound

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation cites this paper.

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation How much information can be extracted from galaxy clustering at the field level?

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-03T00:28:17.443304Z

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Unavailable: canonical work link unavailable.