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Paper Citation Record · LEDGER

Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2405.14945.

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

pith.paper-citation-record.v1
2405.14945 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 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 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T04:41:35.523878Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T19:40:06.417160Z

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 77195ac5-19b7-40ab-b109-dd87afce2f31 · inbound

Population Synthesis of Gravitational Wave Sources cites this paper.

Population Synthesis of Gravitational Wave Sources Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-09T04:41:35.523878Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 88889351-ca89-438a-bac3-9e331dca9d38 · inbound

Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries cites this paper.

Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-09T00:23:46.606799Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation d45406c5-4e01-4d53-afab-2834471bebb1 · inbound

Non-adiabatic dynamics of eccentric black-hole binaries in post-Newtonian theory cites this paper.

Non-adiabatic dynamics of eccentric black-hole binaries in post-Newtonian theory Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes

Reference 86

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verified exact
arxiv_id, observed 2026-05-23T03:25:20.746199Z

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 2bb6836d-724c-423d-aaa0-0787351a3c03 · inbound

PRECESSION 2.1: black-hole binary spin precession on eccentric orbits cites this paper.

PRECESSION 2.1: black-hole binary spin precession on eccentric orbits Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes

Reference 7

Resolution
verified exact
arxiv_id, observed 2026-05-18T20:26:51.077653Z

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=2026-05-18T20:26:46.191637Z digest=sha256:c5e2478a2886472ec5e9b774430371997058df149c20cb100353078e533bc6e5

Observation 6739f9a8-2b01-4bc2-a5ea-444ad0c3d840 · inbound

Constraints on Line-of-Sight Acceleration from O1-O4 cites this paper.

Constraints on Line-of-Sight Acceleration from O1-O4 Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes

Reference 43

Resolution
verified exact
arxiv_id, observed 2026-07-04T19:40:06.418659Z

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=2026-06-25T21:10:34.484784Z digest=sha256:bdf06a85d5625dac1074007eb8fc4c4d83321867c0967f27a3488e7bf87113a3

Observation a2491895-64f9-493f-ab59-c4485c8e3454 · inbound

Constraints on Line-of-Sight Acceleration from O1-O4 cites this paper.

Constraints on Line-of-Sight Acceleration from O1-O4 Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-02T10:17:29.507023Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 578d20cc-0010-46b5-8c9b-01fa03193546 · inbound

High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms cites this paper.

High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-04T21:28:07.261577Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T21:28:07.261577Z digest=sha256:667bbd1efea7d60b6f0eced65a5ab31139a9b629d5d68f8430f6d222428a069a

Observation 2aa51eca-be52-4355-a1ec-4846e79e9b81 · inbound

High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms cites this paper.

High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:12.862930Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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