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Paper Citation Record · LEDGER

Constraining accretion efficiency in massive binary stars with LIGO-Virgo black holes

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2010.11220.

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

pith.paper-citation-record.v1
2010.11220 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 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 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T22:52:12.296201Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-19T04:37:03.771734Z

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 5d00063a-66dc-492e-b1e6-ba9c82d11db7 · inbound

Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop cites this paper.

Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Constraining accretion efficiency in massive binary stars with LIGO-Virgo black holes

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-06T22:52:12.296201Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 01f1c463-431c-4543-afb3-57a3199a363b · inbound

Comparing astrophysical models to gravitational-wave data in the observable space cites this paper.

Comparing astrophysical models to gravitational-wave data in the observable space Constraining accretion efficiency in massive binary stars with LIGO-Virgo black holes

Reference 12

Resolution
verified exact
arxiv_id, observed 2026-05-19T04:37:03.774210Z

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=2026-05-19T04:36:12.661648Z digest=sha256:3f0042a991776975191a3314f649978cf03f42544115f0c4ace63d7c8ea40a07

Observation 491da678-a690-49f3-b5b1-b3726884607c · inbound

Exploring the astrophysical origins of binary black holes using normalising flows cites this paper.

Exploring the astrophysical origins of binary black holes using normalising flows Constraining accretion efficiency in massive binary stars with LIGO-Virgo black holes

Reference 23

Resolution
unresolved
no resolver link, observed 2026-08-05T15:53:34.517100Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T15:53:34.517100Z digest=sha256:98a5cfa5aac6f4331237254d908acd0848c0f7b33f5f7adbd00f2378e2e93a64