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Paper Citation Record · LEDGER

Formation Rate of Extreme Mass Ratio Inspirals in Active Galactic Nuclei

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2101.09146.

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

pith.paper-citation-record.v1
2101.09146 v6

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measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 9 of 9 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T19:32:09.829925Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-24T05:23:56.827023Z

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0 of 0 outbound references displayed

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 76383742-50d7-4cc9-a7e4-679d9bb81989 · inbound

Waveform Modelling for the Laser Interferometer Space Antenna cites this paper.

Waveform Modelling for the Laser Interferometer Space Antenna Formation Rate of Extreme Mass Ratio Inspirals in Active Galactic Nuclei

Reference 79

Resolution
verified exact
arxiv_id, observed 2026-05-24T05:23:56.829910Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

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Observation a765ef76-eaff-4c0f-9b7b-c0885069631c · inbound

The implications of stochastic gas torques for asymmetric binaries in the LISA band cites this paper.

The implications of stochastic gas torques for asymmetric binaries in the LISA band Formation Rate of Extreme Mass Ratio Inspirals in Active Galactic Nuclei

Reference 45

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unresolved
no resolver link, observed 2026-08-07T19:32:09.829925Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 1538716c-7299-4306-ab13-67d3ea1ed64d · inbound

A pipeline for searching and fitting instrumental glitches in LISA data cites this paper.

A pipeline for searching and fitting instrumental glitches in LISA data Formation Rate of Extreme Mass Ratio Inspirals in Active Galactic Nuclei

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-07T14:14:26.395144Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 8e002686-eff5-4ed7-8df7-454e5b462bd0 · inbound

Extreme mass-ratio inspiral within an ultralight scalar cloud I. Scalar radiation cites this paper.

Extreme mass-ratio inspiral within an ultralight scalar cloud I. Scalar radiation Formation Rate of Extreme Mass Ratio Inspirals in Active Galactic Nuclei

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-06T21:02:47.298480Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:02:47.298480Z digest=sha256:5a475ed2fd9818b36fa9a41a77668c76370bf855c08ba0e15317c4f15c591e8a

Observation 591c23f0-f399-4f2e-aa9e-a0cea269d895 · inbound

Constraints on the extreme mass-ratio inspiral population from LISA data cites this paper.

Constraints on the extreme mass-ratio inspiral population from LISA data Formation Rate of Extreme Mass Ratio Inspirals in Active Galactic Nuclei

Reference 17

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verified exact
arxiv_id, observed 2026-05-18T21:46:51.663842Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-05-18T21:45:55.600867Z digest=sha256:445cf2a39f413efdb17754e5ee91213e7e7c90ecea920e29d97915653a1e958d

Observation 0f9ce5cd-64a0-4d95-b005-aea608df4363 · inbound

Probing Kerr Symmetry Breaking with LISA Extreme-Mass-Ratio Inspirals cites this paper.

Probing Kerr Symmetry Breaking with LISA Extreme-Mass-Ratio Inspirals Formation Rate of Extreme Mass Ratio Inspirals in Active Galactic Nuclei

Reference 40

Resolution
verified exact
arxiv_id, observed 2026-05-10T23:10:54.346673Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

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Observation 4129c870-6828-4f6d-9fc7-c707d31189c4 · 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 Formation Rate of Extreme Mass Ratio Inspirals in Active Galactic Nuclei

Reference 12

Resolution
verified exact
arxiv_id, observed 2026-05-11T09:31:05.405295Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-05-10T15:58:14.292439Z digest=sha256:41655e37419432de1b091e43a5f9ef7d10a9beca1f9c43c291ed8746bc1d8c2d

Observation e07ee4e5-acda-48b2-8643-1dcde062db74 · inbound

Eccentricity-Modulated Phase Degeneracy and Distinguishability between Dark Matter and Accretion Disk Environmental Effects in EMRIs cites this paper.

Eccentricity-Modulated Phase Degeneracy and Distinguishability between Dark Matter and Accretion Disk Environmental Effects in EMRIs Formation Rate of Extreme Mass Ratio Inspirals in Active Galactic Nuclei

Reference 80

Resolution
unresolved
no resolver link, observed 2026-07-13T04:38:50.936878Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-13T04:38:50.936878Z digest=sha256:6e6d0aa6a7ea83f541d1b947259633700697c9d831052ca7d1ae6fd5bb592516

Observation 072815bf-962c-49db-b424-48a9f9ebcaaf · 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 Formation Rate of Extreme Mass Ratio Inspirals in Active Galactic Nuclei

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-01T00:50:14.683295Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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