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Paper Citation Record · LEDGER

The more accurately the metal-dependent star formation rate is modeled, the larger the predicted excess of binary black hole mergers

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2410.21401.

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

pith.paper-citation-record.v1
2410.21401 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 2026-08-05T06:32:48.257954+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-06-28T13:01:54.102298Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation cf642016-f9df-41aa-a3f7-f095613482dc · inbound

Emergent structure in the binary black hole mass distribution and implications for population-based cosmology cites this paper.

Emergent structure in the binary black hole mass distribution and implications for population-based cosmology The more accurately the metal-dependent star formation rate is modeled, the larger the predicted excess of binary black hole mergers

Reference 36

Resolution
metadata mismatch
arxiv_id, observed 2026-05-11T11:51:01.836227Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-05-10T12:31:50.358428Z digest=sha256:ea01fb6211815c4c6d4c8d61e151024aeee3ad902265948b665bccc555e5f841

Observation f3ca6d52-b4fa-4295-95e1-d4d441cb23f5 · inbound

Massquerade: Impacts of Mass Ratio Reversals on Binary Black Hole Merger Rates and Mass Distributions cites this paper.

Massquerade: Impacts of Mass Ratio Reversals on Binary Black Hole Merger Rates and Mass Distributions The more accurately the metal-dependent star formation rate is modeled, the larger the predicted excess of binary black hole mergers

Reference 194

Resolution
verified exact
arxiv_id, observed 2026-05-22T09:31:21.570731Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-05-22T09:28:59.560434Z digest=sha256:11a3a35866b3aa4febd8866f30d27d64982f0904f2867d3563fc07a72310b170

Observation 59a1b618-1849-43b6-a49a-bfeeee9bad4b · inbound

Can current models predict the local black hole merger rate? cites this paper.

Can current models predict the local black hole merger rate? The more accurately the metal-dependent star formation rate is modeled, the larger the predicted excess of binary black hole mergers

Reference 48

Resolution
verified exact
arxiv_id, observed 2026-06-28T13:02:10.456453Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-28T13:01:54.102298Z digest=sha256:6f56d9fb7ab7d469e388b08f1c4c5411ccfbae5b3efd37d435caa6e363fd76c6