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Paper Citation Record · LEDGER

Inferring binary black holes stellar progenitors with gravitational wave sources

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2207.00374.

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

pith.paper-citation-record.v1
2207.00374 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 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 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T22:52:12.289712Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T15:53:42.506261Z

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 13557c2e-fe15-4341-826d-6bfb630754be · 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 Inferring binary black holes stellar progenitors with gravitational wave sources

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-06T22:52:12.289712Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T22:52:12.289712Z digest=sha256:23cf478076bee929bd072a058f4f93b24cc2bfabbd45e240e8b37aeaf6fec5a7

Observation 337e5d5f-d039-43ef-ab22-544db44c8f50 · 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 Inferring binary black holes stellar progenitors with gravitational wave sources

Reference 25

Resolution
verified exact
local_arxiv, observed 2026-08-05T15:53:42.700293Z

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=2026-08-05T15:53:34.768873Z digest=sha256:9eddcbb768d6586bfa70299d1d4f5b70451c9ca1b0be8f95cd44e8afb6fee95e