Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
C$^3$-Cluster Clustering Cosmology II. First detection of the BAO peak in the three-point correlation function of galaxy clusters
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2011.04665.
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 2026-08-16T06:30:59.297886+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T05:21:13.530989Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-23T22:35:50.505575Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 6e247ac3-418a-4e87-9cb9-df96e4ee8f8b · 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 C$^3$-Cluster Clustering Cosmology II. First detection of the BAO peak in the three-point correlation function of galaxy clusters
Reference 52
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T22:35:50.508298Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 4b2952dc-bb6f-49e1-8370-e8fd209a3e55 · inbound
Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation cites this paper.
Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation C$^3$-Cluster Clustering Cosmology II. First detection of the BAO peak in the three-point correlation function of galaxy clusters
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T05:21:13.530989Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.