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Paper Citation Record · LEDGER

The maximum mass of a black hole which can tidally disrupt a star: measuring black hole spins with tidal disruption events

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2312.00557.

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

pith.paper-citation-record.v1
2312.00557 v2

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 2026-08-22T06:32:14.747728+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T22:18:53.870074Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-16T12:02:50.796008Z

Reference resolution

0 of 0 outbound references displayed

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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 666ee1af-1144-4f56-a392-39a692580455 · inbound

Stepping Up Superradiance Constraints on Axions cites this paper.

Stepping Up Superradiance Constraints on Axions The maximum mass of a black hole which can tidally disrupt a star: measuring black hole spins with tidal disruption events

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-11T22:18:53.870074Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 0fea6ef7-f1d4-4896-9df5-1f01956dea2a · inbound

Black hole supercolliders cites this paper.

Black hole supercolliders The maximum mass of a black hole which can tidally disrupt a star: measuring black hole spins with tidal disruption events

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-07T11:54:00.604813Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T11:54:00.604813Z digest=sha256:5c0c79d21b579950a7409b34e58253d96948f3863e77a5f3c22523d4d93b6bc9

Observation f08d4c86-a18e-4e17-b75a-ce86633e24f9 · inbound

Mass Determination of Supermassive Black Holes Governing Evolution of Radio Emitters cites this paper.

Mass Determination of Supermassive Black Holes Governing Evolution of Radio Emitters The maximum mass of a black hole which can tidally disrupt a star: measuring black hole spins with tidal disruption events

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-06T11:21:10.574113Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T11:21:10.574113Z digest=sha256:ab242c1a922aef805522479d83d4cac474f78ad5aa403b5dfdcf4dd4c9c1391a

Observation c856db07-4390-450b-a456-10593ec5e6b2 · inbound

Roche limit and stellar disruption in the Simpson--Visser spacetime cites this paper.

Roche limit and stellar disruption in the Simpson--Visser spacetime The maximum mass of a black hole which can tidally disrupt a star: measuring black hole spins with tidal disruption events

Reference 96

Resolution
verified exact
arxiv_id, observed 2026-05-16T12:02:50.798189Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-16T12:01:27.699618Z digest=sha256:5ef7b1d62060b85e2049812655b93d423c59ee82a799f430c6ec8e64056cf5fd

Observation 0a793ae8-f22e-4031-91c7-7ee56aee2c68 · inbound

One year of broadband radio monitoring of the enigmatic transient GRB 250702B reveals the evolution of the relativistic jet cites this paper.

One year of broadband radio monitoring of the enigmatic transient GRB 250702B reveals the evolution of the relativistic jet The maximum mass of a black hole which can tidally disrupt a star: measuring black hole spins with tidal disruption events

Reference 4

Resolution
unresolved
no resolver link, observed 2026-08-05T23:39:12.965753Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T23:39:12.965753Z digest=sha256:814279f29fedfd88474f77a8d04b9927ad964ce12bc689ba84bef37866c7e7e6