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Paper Citation Record · LEDGER

Extensions to models of the galaxy-halo connection

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2008.04913.

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

pith.paper-citation-record.v1
2008.04913 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T05:21:13.573747Z

measured 0 of 1 external citation measurements

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

Source: cited_works

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 3b235751-cce1-4213-86c6-413af4bdc320 · 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 Extensions to models of the galaxy-halo connection

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-16T05:21:13.573747Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T05:21:13.573747Z digest=sha256:5f79a8b0350f1ab97d0b00f85bb0573cc93e52cefa34452bcd72c3c54e7836ea

Observation b2374e31-2e5c-4c33-a23e-8feffa8522b0 · inbound

Interpreting the stacked kinetic SZ effect I: velocity reconstruction and non-linear velocity effects cites this paper.

Interpreting the stacked kinetic SZ effect I: velocity reconstruction and non-linear velocity effects Extensions to models of the galaxy-halo connection

Reference 108

Resolution
unresolved
no resolver link, observed 2026-07-31T23:49:26.817095Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T23:49:26.817095Z digest=sha256:b41810e7ec83531198e3b548a74b7528534ed221ab9b9df6cc267d3db3f39159