Paper Citation Record · LEDGER

New constraints on the central mass contents of Omega Centauri from combined stellar kinematics and pulsar timing

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2408.00939.

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

pith.paper-citation-record.v1
2408.00939 v6

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measured 0 of 0 reference resolution

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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 2026-08-05T06:32:48.257954+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 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-08T15:15:03.214985Z

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Outbound references

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Pith citing papers

Observation 1471942d-21fa-4a17-89d4-aa67933ca685 · 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 New constraints on the central mass contents of Omega Centauri from combined stellar kinematics and pulsar timing

Reference 32

Resolution: verified exact; arxiv_id, observed 2026-06-19T17:10:15.756437Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 271a3574-5c5f-4b8e-aa44-108d7dced5ab · inbound

Dark Matter in Draco and Bo\"otes I: Hints of a Core in an Ultra-Faint Dwarf from Simulation-Based Inference cites this paper.

Dark Matter in Draco and Bo\"otes I: Hints of a Core in an Ultra-Faint Dwarf from Simulation-Based Inference New constraints on the central mass contents of Omega Centauri from combined stellar kinematics and pulsar timing

Reference 14

Resolution: verified exact; local_arxiv, observed 2026-06-26T01:58:54.828593Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 70a8c9b5-1f4e-4420-a390-7acb2ba46a5b · inbound

Too shy to spin? Cosmic wallflowers as proto-globular clusters cites this paper.

Too shy to spin? Cosmic wallflowers as proto-globular clusters New constraints on the central mass contents of Omega Centauri from combined stellar kinematics and pulsar timing

Reference 97

Resolution: verified exact; local_arxiv, observed 2026-06-29T02:13:00.383206Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation dd01f2b6-1406-455f-a643-b154f1c693cd · inbound

Pulsars in Globular Clusters With the SKAO cites this paper.

Pulsars in Globular Clusters With the SKAO New constraints on the central mass contents of Omega Centauri from combined stellar kinematics and pulsar timing

Reference 28

Resolution: verified exact; local_arxiv, observed 2026-07-08T15:15:03.216400Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.