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Paper Citation Record · LEDGER

Ideal E/IMRI vs Real E/IMRI system : Observable signature in LISA

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2307.12144.

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

pith.paper-citation-record.v1
2307.12144 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 2026-08-10T06:31:04.303077+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T17:33:37.083166Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T09:31:05.388525Z

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 9fdb01f4-094c-4c8a-99cb-58932be0273d · inbound

Secondary spins of extreme mass ratio inspirals: A probe to the formation channels cites this paper.

Secondary spins of extreme mass ratio inspirals: A probe to the formation channels Ideal E/IMRI vs Real E/IMRI system : Observable signature in LISA

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-09T17:33:37.083166Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T17:33:37.083166Z digest=sha256:0b1de360838c961930a47629b299608dd9d0102c15b215cc820b6fd9a4178c47

Observation 044d879e-bbf0-4417-b842-2aa1ff7ae504 · inbound

Probing Active Galactic Nuclei and Measuring the Hubble constant with Extreme-Mass-Ratio Inspirals cites this paper.

Probing Active Galactic Nuclei and Measuring the Hubble constant with Extreme-Mass-Ratio Inspirals Ideal E/IMRI vs Real E/IMRI system : Observable signature in LISA

Reference 19

Resolution
verified exact
arxiv_id, observed 2026-05-11T09:31:05.396716Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-10T15:58:14.292439Z digest=sha256:ff04782116f941515c1510cbbb1a7280750aa537535d33f01e0831891121adf2