Paper Citation Record · LEDGER

Machine-assisted discovery of relationships in astronomy

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1302.5129.

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

pith.paper-citation-record.v1
1302.5129 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 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 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 1 of 1 external citation measurements

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

Source: pith, 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

40
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 948fd8b7-8a23-4604-adb6-a233012c5d7f · inbound

Into the Gompverse: A robust Gompertzian reionization model for CMB analyses cites this paper.

Into the Gompverse: A robust Gompertzian reionization model for CMB analyses Machine-assisted discovery of relationships in astronomy

Reference 17

Resolution: verified exact; arxiv_id, observed 2026-05-10T13:45:28.903055Z

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 77ca8dd5-5b73-4c31-911b-be92cdb69bbf · inbound

Predicting intermediate-mass black hole formation in star clusters with machine learning cites this paper.

Predicting intermediate-mass black hole formation in star clusters with machine learning Machine-assisted discovery of relationships in astronomy

Reference 88

Resolution: verified exact; local_arxiv, observed 2026-05-22T09:21:21.219629Z

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 3fb34e29-859c-4715-930d-30d1738ca5ae · inbound

pop-cosmos: Disentangling galaxy properties from observables using data-driven approaches cites this paper.

pop-cosmos: Disentangling galaxy properties from observables using data-driven approaches Machine-assisted discovery of relationships in astronomy

Reference 51

Resolution: verified exact; local_arxiv, observed 2026-06-27T13:40:58.121405Z

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 e9d7f151-6199-4455-a28e-a37639122f67 · inbound

pop-cosmos: Galaxy size evolution across structural and star-formation classifications in COSMOS-Web cites this paper.

pop-cosmos: Galaxy size evolution across structural and star-formation classifications in COSMOS-Web Machine-assisted discovery of relationships in astronomy

Reference 53

Resolution: verified exact; local_arxiv, observed 2026-06-30T01:04:08.731587Z

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.