Paper Citation Record · LEDGER

Chaotic Loss Cones, Black Hole Fueling and the M-Sigma Relation

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0302296.

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

pith.paper-citation-record.v1
astro-ph/0302296 v2

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 2026-08-11T06:34:44.6726+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T13:27:10.541145Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T17:18:52.756032Z

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 af9f2c18-1c1f-438b-a488-bab4cc4b6a2d · inbound

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers cites this paper.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Chaotic Loss Cones, Black Hole Fueling and the M-Sigma Relation

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.541145Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8f238bac-7551-4242-a78b-fb45b27d4328 · inbound

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster cites this paper.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Chaotic Loss Cones, Black Hole Fueling and the M-Sigma Relation

Reference 23

Resolution: verified exact; local_arxiv, observed 2026-08-06T17:18:52.834747Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.