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Paper Citation Record · LEDGER

Dynamics of binary black holes in young star clusters: the impact of cluster mass and long-term evolution

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2203.08163.

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

pith.paper-citation-record.v1
2203.08163 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 2026-08-07T06:34:17.273281+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T23:08:01.831675Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T19:40:06.496401Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • parse uncertain0
  • malformed identifier0
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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 605fc640-7883-4865-8a77-087aa3f53942 · inbound

The impact of the formation channel on gravitational-wave-galaxy cross-correlations cites this paper.

The impact of the formation channel on gravitational-wave-galaxy cross-correlations Dynamics of binary black holes in young star clusters: the impact of cluster mass and long-term evolution

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-02T23:08:01.831675Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T23:08:01.831675Z digest=sha256:23ac19c9d7589a3d7e6266613e97c637d20080d0322acf5bbbbd81bb7efa1820

Observation 85ebed27-b722-48f4-b51e-6c4523ab0942 · inbound

How lonely are the Binary Compact Objects Detected by the LIGO-Virgo-KAGRA Collaboration? cites this paper.

How lonely are the Binary Compact Objects Detected by the LIGO-Virgo-KAGRA Collaboration? Dynamics of binary black holes in young star clusters: the impact of cluster mass and long-term evolution

Reference 29

Resolution
verified exact
arxiv_id, observed 2026-05-11T20:01:11.367132Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-08T10:30:09.499209Z digest=sha256:f7215c356ec3c2cc0dc35505fe25da276f206ea8d1b6beaf2c42154750697311

Observation 14126478-2e08-4660-8e27-a6dcce8db425 · inbound

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

Constraints on Line-of-Sight Acceleration from O1-O4 Dynamics of binary black holes in young star clusters: the impact of cluster mass and long-term evolution

Reference 24

Resolution
verified exact
arxiv_id, observed 2026-07-04T19:40:06.497793Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-06-25T21:10:34.484784Z digest=sha256:0f48a29cd3894ffd2c9a89a35a5ada2b587c2b18ee0995661f45a2f997a065fa

Observation dc081f61-3bbf-4144-95a4-4d4dd6580ca0 · inbound

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

Constraints on Line-of-Sight Acceleration from O1-O4 Dynamics of binary black holes in young star clusters: the impact of cluster mass and long-term evolution

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-02T10:17:27.015203Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T10:17:27.015203Z digest=sha256:33ec0f87298557850ffed8cb8e6f9dbb42bfb63668e332558b087b1a162e5330

Observation 63635a9b-05ec-4088-8262-f4a6150f1ba7 · inbound

Modes in Transitional Millisecond Pulsars: Evidence of Pulsar Wind-Induced Disk Heating from GRMHD and Radiative Transfer cites this paper.

Modes in Transitional Millisecond Pulsars: Evidence of Pulsar Wind-Induced Disk Heating from GRMHD and Radiative Transfer Dynamics of binary black holes in young star clusters: the impact of cluster mass and long-term evolution

Reference 163

Resolution
unresolved
no resolver link, observed 2026-08-01T13:29:43.103807Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T13:29:43.103807Z digest=sha256:e7f110f1e86b16c0ae3d294cbcbb7e00d2446471745c9e1930ca198574b2021b