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Paper Citation Record · LEDGER

Cosmic Rates of Black Hole Mergers and Pair-Instability Supernovae from Chemically Homogeneous Binary Evolution

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2002.11630.

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

pith.paper-citation-record.v1
2002.11630 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 2026-08-21T06:32:19.484+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T22:52:12.181264Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T12:58:07.880065Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • 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 44f65799-545a-45be-81ab-d1ca31f2ae60 · inbound

GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run cites this paper.

GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run Cosmic Rates of Black Hole Mergers and Pair-Instability Supernovae from Chemically Homogeneous Binary Evolution

Reference 69

Resolution
verified exact
arxiv_id, observed 2026-05-11T09:30:26.390600Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-05-11T09:30:24.998354Z digest=sha256:417ac9efcb8b9bf166a20b0f79568b872c2d66d3131da3eb5501d96a226a3570

Observation ae186cc1-5746-4c1c-81f8-fa955ddfa355 · 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 Cosmic Rates of Black Hole Mergers and Pair-Instability Supernovae from Chemically Homogeneous Binary Evolution

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-06T22:52:12.181264Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T22:52:12.181264Z digest=sha256:aca41c594c3b0e33b489238dca8de47d214b11f862cfc7b960fb6037eb652c77

Observation 20c7061d-fe50-4149-9121-e9467428ed38 · 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 Cosmic Rates of Black Hole Mergers and Pair-Instability Supernovae from Chemically Homogeneous Binary Evolution

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-05T15:53:37.336841Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T15:53:37.336841Z digest=sha256:9f8c196a7244d8aea9d74d5a296143e2bf2f8197dbfa72f7174ecb5c31ef3748

Observation 21a16a87-a4bc-4de0-8905-c2825251bbc4 · inbound

Very Massive, Rapidly Spinning Binary Black Hole Progenitors through Chemically Homogeneous Evolution -- The Case of GW231123 cites this paper.

Very Massive, Rapidly Spinning Binary Black Hole Progenitors through Chemically Homogeneous Evolution -- The Case of GW231123 Cosmic Rates of Black Hole Mergers and Pair-Instability Supernovae from Chemically Homogeneous Binary Evolution

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-05T13:59:04.833803Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T13:59:04.833803Z digest=sha256:de20c9911bbb99a08b2598ab55be227b136b9ae5fd671429fd3bb666555dcd80

Observation 36bfbe1b-6b3c-4a4e-bbb1-178defc869cf · inbound

Evidence for additional structure in the effective spin distribution hints at multiple formation pathways in GWTC-5.0 cites this paper.

Evidence for additional structure in the effective spin distribution hints at multiple formation pathways in GWTC-5.0 Cosmic Rates of Black Hole Mergers and Pair-Instability Supernovae from Chemically Homogeneous Binary Evolution

Reference 38

Resolution
verified exact
arxiv_id, observed 2026-07-03T12:58:07.881481Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-06-27T08:41:37.044992Z digest=sha256:bc6ea37ae14cd934c58fb3ab9b0acb7e09541cd38263837c984f9454208b207e