Paper Citation Record · LEDGER

Space-based Gravitational Wave Observatories Will Be Able to Use Eccentricity to Unveil Stellar-mass Binary Black Hole Formation

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2304.10340.

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

pith.paper-citation-record.v1
2304.10340 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:15:05.529087Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-25T08:05:30.837927Z

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 b2565178-624b-42e1-816b-03aafd2e1fb3 · inbound

Multiband parameter estimation with phase coherence and extrinsic marginalization: Extracting more information from low-SNR CBC signals in LISA data cites this paper.

Multiband parameter estimation with phase coherence and extrinsic marginalization: Extracting more information from low-SNR CBC signals in LISA data Space-based Gravitational Wave Observatories Will Be Able to Use Eccentricity to Unveil Stellar-mass Binary Black Hole Formation

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-07T11:37:22.516020Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d7b1dacf-fc49-409d-b757-f2d26e78b4ce · 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 Space-based Gravitational Wave Observatories Will Be Able to Use Eccentricity to Unveil Stellar-mass Binary Black Hole Formation

Reference 33

Resolution: verified exact; arxiv_id, observed 2026-05-25T08:05:30.840178Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 8211041c-e509-4448-9d46-874fcfb2eff6 · inbound

Can Eccentric Binary Black Hole Signals Mimic Gravitational-Wave Microlensing? cites this paper.

Can Eccentric Binary Black Hole Signals Mimic Gravitational-Wave Microlensing? Space-based Gravitational Wave Observatories Will Be Able to Use Eccentricity to Unveil Stellar-mass Binary Black Hole Formation

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-03T18:57:07.865329Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 348e59f7-daa1-4c1f-b32b-3f14cd21e6ae · inbound

Constraining Dipole Radiation with Multiband Gravitational Waves from Eccentric Binary Black Holes cites this paper.

Constraining Dipole Radiation with Multiband Gravitational Waves from Eccentric Binary Black Holes Space-based Gravitational Wave Observatories Will Be Able to Use Eccentricity to Unveil Stellar-mass Binary Black Hole Formation

Reference 34

Resolution: verified exact; arxiv_id, observed 2026-05-12T10:21:28.594640Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation a63799d8-52e4-4c98-8fb3-78e8783ad1fd · inbound

Constraining Dipole Radiation with Multiband Gravitational Waves from Eccentric Binary Black Holes cites this paper.

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-02T15:13:24.177193Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2ffe484c-a479-475c-bbb5-4cc0a43e52ad · inbound

A parametrized test of general relativity for inspiralling eccentric binaries in LISA cites this paper.

A parametrized test of general relativity for inspiralling eccentric binaries in LISA Space-based Gravitational Wave Observatories Will Be Able to Use Eccentricity to Unveil Stellar-mass Binary Black Hole Formation

Reference 111

Resolution: unresolved; no resolver link, observed 2026-08-14T04:15:05.529087Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.