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Paper Citation Record · LEDGER

Enhanced Extreme Mass Ratio Inspiral Rates into Intermediate Mass Black Holes

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2304.13062.

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

pith.paper-citation-record.v1
2304.13062 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T00:50:16.830616Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T15:58:38.277812Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • 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 7cb3d888-1046-4f79-a726-0b68d8d23ef9 · inbound

Gravitational radiation from hyperbolic orbits: comparison between self-force, post-Minkowskian, post-Newtonian, and numerical relativity results cites this paper.

Gravitational radiation from hyperbolic orbits: comparison between self-force, post-Minkowskian, post-Newtonian, and numerical relativity results Enhanced Extreme Mass Ratio Inspiral Rates into Intermediate Mass Black Holes

Reference 116

Resolution
verified exact
arxiv_id, observed 2026-05-17T02:13:52.485113Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-17T02:11:46.560266Z digest=sha256:df64c4bc27525974075ce66882b7f6c0b4bd7d038d7a47b865198711564b60f6

Observation 2de50be6-d631-4ce6-b948-3a158cea5d15 · inbound

Gravitational wave background from extreme-mass-ratio inspirals cites this paper.

Gravitational wave background from extreme-mass-ratio inspirals Enhanced Extreme Mass Ratio Inspiral Rates into Intermediate Mass Black Holes

Reference 26

Resolution
verified exact
arxiv_id, observed 2026-07-03T15:58:38.279232Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-06-27T06:13:43.701245Z digest=sha256:e69a41adf20890bda1a9979acc24a36de3b9d2dafae424bc78c867ee39f9e3ad

Observation 429e47fc-c01f-4b2d-9f79-d81f755fce5c · inbound

From S2 to LISA: Astrometric Bounds on Extreme-Mass-Ratio Inspirals and Bursts cites this paper.

From S2 to LISA: Astrometric Bounds on Extreme-Mass-Ratio Inspirals and Bursts Enhanced Extreme Mass Ratio Inspiral Rates into Intermediate Mass Black Holes

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-01T00:50:16.830616Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:50:16.830616Z digest=sha256:e280a67a5d06ee246ffd37a6a33994d230cb6cc46aaa8ce8ff3299187974329e