Paper Citation Record · LEDGER

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

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 18 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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measured 18 of 18 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 18 of 18 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T04:39:47.184947Z

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 dace2466-9200-4180-9b92-17b4ea7677ea · inbound

Towards characterizing dark matter subhalo perturbations in stellar streams with graph neural networks cites this paper.

Towards characterizing dark matter subhalo perturbations in stellar streams with graph neural networks How much information can be extracted from galaxy clustering at the field level?

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-09T04:39:47.184947Z

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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

Resolution: unresolved; no resolver link, observed 2026-08-07T05:50:31.640171Z

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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

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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

Resolution: unresolved; no resolver link, observed 2026-08-06T19:34:06.286855Z

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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

Resolution: unresolved; no resolver link, observed 2026-08-06T16:23:47.257707Z

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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

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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

Resolution: verified exact; arxiv_id, observed 2026-05-12T00:31:19.780960Z

Source-reported events for the cited work

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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

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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 2026-08-08T06:32:00.761636+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

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No event found in the named queried sources as of 2026-08-08T06:32:00.761636+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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