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Paper Citation Record · LEDGER

Rates and Characteristics of Intermediate Mass Ratio Inspirals Detectable by Advanced LIGO

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:0705.0285.

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

pith.paper-citation-record.v1
0705.0285 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T04:25:35.462805Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-22T09:21:20.793329Z

Reference resolution

0 of 0 outbound references displayed

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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 b69a1e79-c970-4a20-8b61-edc55c72527b · inbound

Dark matter minispike: a significant enhancement of eccentricity for intermediate-mass-ratio-inspirals cites this paper.

Dark matter minispike: a significant enhancement of eccentricity for intermediate-mass-ratio-inspirals Rates and Characteristics of Intermediate Mass Ratio Inspirals Detectable by Advanced LIGO

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-14T10:57:42.143084Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:57:42.143084Z digest=sha256:cbc063faea1b592def4d9ea0e70e3f411a316baa89ce92f2b949d87cefc9814f

Observation a6664511-1199-4091-a0eb-8df72992d9c8 · 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 Rates and Characteristics of Intermediate Mass Ratio Inspirals Detectable by Advanced LIGO

Reference 104

Resolution
unresolved
no resolver link, observed 2026-08-10T13:27:10.742311Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T13:27:10.742311Z digest=sha256:6a13d56a4ab87948cb13c1f2789be4a3b201c14a8abe30ab057d5131730ba974

Observation d9e34d6d-b5e1-49de-bb5f-728da77574a8 · inbound

Evolution of a black hole cluster in full general relativity cites this paper.

Evolution of a black hole cluster in full general relativity Rates and Characteristics of Intermediate Mass Ratio Inspirals Detectable by Advanced LIGO

Reference 210

Resolution
unresolved
no resolver link, observed 2026-08-16T04:25:35.462805Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:25:35.462805Z digest=sha256:4632768f8fddb8df9427f852537c6de145d3b8ca9493f0476c165bb7a736ad1d

Observation 92b4b79d-9af5-4853-8817-b31100a3ce4b · inbound

Searching for intermediate mass ratio binary black hole mergers in the third observing run of LIGO-Virgo-KAGRA cites this paper.

Searching for intermediate mass ratio binary black hole mergers in the third observing run of LIGO-Virgo-KAGRA Rates and Characteristics of Intermediate Mass Ratio Inspirals Detectable by Advanced LIGO

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-06T21:08:37.372763Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:08:37.372763Z digest=sha256:ee3f4dd97c5a88d5b5c88f5bb237cc61494c895230a5eca4e8b463ceb74ad3c6

Observation b927dd42-9003-4503-a3f5-c9ce0da89d03 · inbound

Predicting intermediate-mass black hole formation in star clusters with machine learning cites this paper.

Predicting intermediate-mass black hole formation in star clusters with machine learning Rates and Characteristics of Intermediate Mass Ratio Inspirals Detectable by Advanced LIGO

Reference 72

Resolution
verified exact
local_arxiv, observed 2026-05-22T09:21:20.795909Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-05-22T09:20:09.976842Z digest=sha256:191a54bbb4ce80f15d869246bb41d3e72164977907c62d28390e1c981b6a3d94