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Paper Citation Record · LEDGER

A Semi-Analytical Model for Stellar Evolution in AGN Disks

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2409.02981.

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

pith.paper-citation-record.v1
2409.02981 v1

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 2026-08-19T06:32:44.657259+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T20:16:00.106614Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T05:30:23.456663Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

1
pith, observed 2026-08-10T05:30:23.456663Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 0e502a4b-33f7-4a42-b2b5-1ad8362f57b8 · inbound

Prompt gravitational-wave mergers aided by gas in Active Galactic Nuclei: The hydrodynamics of binary-single black hole scatterings cites this paper.

Prompt gravitational-wave mergers aided by gas in Active Galactic Nuclei: The hydrodynamics of binary-single black hole scatterings A Semi-Analytical Model for Stellar Evolution in AGN Disks

Reference 32

Resolution
unresolved
no resolver link, observed 2026-08-10T20:16:00.106614Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:16:00.106614Z digest=sha256:33ad98957c7c48ee04a53a12f3ff150537645cf73725e863bc1ba01096ed4341

Observation 3d8d68d9-163c-4296-838f-194e4d90ba71 · inbound

Population Synthesis of Gravitational Wave Sources cites this paper.

Population Synthesis of Gravitational Wave Sources A Semi-Analytical Model for Stellar Evolution in AGN Disks

Reference 54

Resolution
verified exact
local_arxiv, observed 2026-08-09T04:41:36.525797Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-08-09T04:41:35.454329Z digest=sha256:ef86f793fa057a2197ac808fdbb1c06ff9200d0711dc0e2e97cfab31be7556e9