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Paper Citation Record · LEDGER

Constructing EOB dynamics with numerical energy flux for intermediate-mass-ratio inspirals

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1108.0995.

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

pith.paper-citation-record.v1
1108.0995 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 2026-08-18T06:34:40.430872+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T00:30:58.748019Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T18:35:58.881646Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
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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 ab878ef4-7cb8-4381-a956-e0f91d802b5b · inbound

GW250114 reveals black hole horizon signatures cites this paper.

GW250114 reveals black hole horizon signatures Constructing EOB dynamics with numerical energy flux for intermediate-mass-ratio inspirals

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-04T13:25:27.330056Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T13:25:27.330056Z digest=sha256:aede74652dc09f456333359cb58936d7a276facd720309cdc3342164daf30997

Observation 62587039-f711-4e94-9bf5-80bf5e1275f6 · inbound

Massive scalar fields in eccentric regime: Detectability and constraints from LISA observations of extreme mass-ratio inspirals cites this paper.

Massive scalar fields in eccentric regime: Detectability and constraints from LISA observations of extreme mass-ratio inspirals Constructing EOB dynamics with numerical energy flux for intermediate-mass-ratio inspirals

Reference 14

Resolution
verified exact
local_arxiv, observed 2026-07-01T18:35:58.882845Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-06-29T01:52:24.227372Z digest=sha256:18422fdac56b7d434bd05a725c0114bcfcf16a8597fbb8aa6915d1361ef92286

Observation 49f34867-3947-461f-8479-fad7f4d67756 · inbound

Taiji Resolving Power for the Transverse Scalar Mode of Gravitational Waves cites this paper.

Taiji Resolving Power for the Transverse Scalar Mode of Gravitational Waves Constructing EOB dynamics with numerical energy flux for intermediate-mass-ratio inspirals

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-16T00:30:58.748019Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T00:30:58.748019Z digest=sha256:6078bb075b2922e5fae0930a21c4c577f7f796ee7bfa03f4306984196c256c05