Paper Citation Record · LEDGER

New Black Hole Spin Values for Sagittarius A* Obtained with the Outflow Method

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2310.12108.

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

pith.paper-citation-record.v1
2310.12108 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T06:36:31.871081Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T04:26:36.156759Z

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 2523ecd6-d3ad-4179-85c8-4c0cfced82fd · inbound

Redshifted civilizations, galactic empires, and the Fermi paradox cites this paper.

Redshifted civilizations, galactic empires, and the Fermi paradox New Black Hole Spin Values for Sagittarius A* Obtained with the Outflow Method

Reference 28

Resolution: verified exact; arxiv_id, observed 2026-05-18T11:31:19.338553Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 3ca27fe8-3a4f-4abd-9b4d-ecc230f8ec70 · inbound

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals cites this paper.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals New Black Hole Spin Values for Sagittarius A* Obtained with the Outflow Method

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:31.871081Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6f8f1e4a-e874-4044-a079-5351ba2a5efc · inbound

Multimessenger Signatures of Tilted, Self-Gravitating, Black Hole Disks cites this paper.

Multimessenger Signatures of Tilted, Self-Gravitating, Black Hole Disks New Black Hole Spin Values for Sagittarius A* Obtained with the Outflow Method

Reference 10

Resolution: verified exact; arxiv_id, observed 2026-05-13T18:28:06.697838Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation f6ae3108-5428-4156-9450-2cc7f1d0b998 · inbound

Multimessenger Signatures of Tilted, Self-Gravitating, Black Hole Disks cites this paper.

Multimessenger Signatures of Tilted, Self-Gravitating, Black Hole Disks New Black Hole Spin Values for Sagittarius A* Obtained with the Outflow Method

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-02T16:51:29.602664Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b942e9d2-f688-4861-b2c3-a79d17645fc7 · inbound

A Plunge into the Chasm: Surviving Tidal Effects in Kerr Spacetime cites this paper.

A Plunge into the Chasm: Surviving Tidal Effects in Kerr Spacetime New Black Hole Spin Values for Sagittarius A* Obtained with the Outflow Method

Reference 9

Resolution: verified exact; arxiv_id, observed 2026-07-02T04:26:36.158063Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.