Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The Renormalization Group for Large-Scale Structure: Origin of Galaxy Stochasticity
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2404.16929.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T16:23:48.142736Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
0
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 fd526bf4-fb8e-42da-b422-0188c1a5b60b · inbound
Two-loop renormalization and running of galaxy bias cites this paper.
Two-loop renormalization and running of galaxy bias The Renormalization Group for Large-Scale Structure: Origin of Galaxy Stochasticity
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:23:48.142736Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 32b99c66-f563-428e-baad-14ca075a8b65 · inbound
Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation cites this paper.
Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation The Renormalization Group for Large-Scale Structure: Origin of Galaxy Stochasticity
Reference 4
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T23:38:16.376174Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f5f0b455-a060-428a-8552-b88ea32607ac · 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 The Renormalization Group for Large-Scale Structure: Origin of Galaxy Stochasticity
Reference 26
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T00:31:19.470534Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.
Observation 955b7f33-1e97-48b7-a9a0-5c1a5e775ae9 · 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 The Renormalization Group for Large-Scale Structure: Origin of Galaxy Stochasticity
Reference 185
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-06-26T01:38:51.696159Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.
Observation 62a39176-22e2-4d65-b1c5-f3d9a4b47c1f · inbound
Galaxy bias renormalization: Two-loop Power Spectrum, One-loop Trispectrum and Bispectrum cites this paper.
Galaxy bias renormalization: Two-loop Power Spectrum, One-loop Trispectrum and Bispectrum The Renormalization Group for Large-Scale Structure: Origin of Galaxy Stochasticity
Reference 18
- Resolution
- verified exact
- arxiv_id, observed 2026-07-01T11:05:42.616618Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.