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Paper Citation Record · LEDGER

Identification of Gravitational-waves from Extreme Mass Ratio Inspirals

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2310.03520.

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

pith.paper-citation-record.v1
2310.03520 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T14:59:16.445913Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-01T13:25:45.729985Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 74f1c863-62ab-4638-9405-5c75423c4683 · inbound

Sequential simulation-based inference for extreme mass ratio inspirals cites this paper.

Sequential simulation-based inference for extreme mass ratio inspirals Identification of Gravitational-waves from Extreme Mass Ratio Inspirals

Reference 90

Resolution
unresolved
no resolver link, observed 2026-08-07T14:59:16.445913Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation b96afb3a-7796-429e-8656-5811c64a02d9 · inbound

Searching for extreme mass ratio inspirals in LISA: from identification to parameter estimation cites this paper.

Searching for extreme mass ratio inspirals in LISA: from identification to parameter estimation Identification of Gravitational-waves from Extreme Mass Ratio Inspirals

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-07T14:43:24.229897Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:43:24.229897Z digest=sha256:012b1e2e8b11de6de8f4df1f7c7b17f8a7c2eef0e929e83f3b6ac4b2d5f6b9e4

Observation fa116278-349a-43a9-8717-ee3dc46c8c53 · inbound

Global time-frequency search for stellar-mass binary black holes in LISA cites this paper.

Global time-frequency search for stellar-mass binary black holes in LISA Identification of Gravitational-waves from Extreme Mass Ratio Inspirals

Reference 25

Resolution
verified exact
arxiv_id, observed 2026-05-25T08:05:31.173157Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-25T08:01:49.461171Z digest=sha256:d21fac9d3451487e16b8e27c07a39ecd6c5353668fdd6d4ae22797ecb0bed28b

Observation 0cc7f6db-9cf0-4201-81d3-15e5d11bffce · inbound

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals cites this paper.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Identification of Gravitational-waves from Extreme Mass Ratio Inspirals

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-03T06:36:31.105761Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T06:36:31.105761Z digest=sha256:aff88669ee7066e2f15a542151df698fe8ec2e1109c870b10c092e0f49c9cdab

Observation 55e56ca2-ed6d-478d-84e5-e95a8008ed65 · inbound

Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals cites this paper.

Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals Identification of Gravitational-waves from Extreme Mass Ratio Inspirals

Reference 19

Resolution
verified exact
arxiv_id, observed 2026-05-11T18:21:07.875989Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-08T16:15:50.585102Z digest=sha256:ca1b504e459905dc6714575ff46da16bc66916a7f9737aee436336ebda27b693

Observation e3a7371b-a63e-4143-88af-8c3ba7903ec1 · inbound

Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals cites this paper.

Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals Identification of Gravitational-waves from Extreme Mass Ratio Inspirals

Reference 19

Resolution
verified exact
arxiv_id, observed 2026-05-11T04:36:00.396653Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-11T01:12:19.470529Z digest=sha256:23bca9ba670a4ab52e8a7e3d225660da2bb1445fbc32b399db079a44de9d4788

Observation f2dc4c6d-8f2e-4240-b6e2-07c13106c00f · inbound

Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals cites this paper.

Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals Identification of Gravitational-waves from Extreme Mass Ratio Inspirals

Reference 20

Resolution
verified exact
arxiv_id, observed 2026-07-01T13:25:45.731474Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-06-30T23:15:57.036633Z digest=sha256:4e38cf15719b7992553f759f1a3f6f84997d396ba390453a0590ed82d227c53b