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 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 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 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T21:32:15.906178Z

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 ad937445-a247-475b-b859-3ba5d55c830f · inbound

Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations cites this paper.

Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations The more accurately the metal-dependent star formation rate is modeled, the larger the predicted excess of binary black hole mergers

Reference 107

Resolution: unresolved; no resolver link, observed 2026-08-10T21:32:15.906178Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 94008b7a-7c9c-4080-b479-a26d38aab7fc · inbound

Candidate intermediate-mass black hole discovered in an extremely young low-metallicity cluster in the tadpole galaxy KUG 1138+327 cites this paper.

Candidate intermediate-mass black hole discovered in an extremely young low-metallicity cluster in the tadpole galaxy KUG 1138+327 The more accurately the metal-dependent star formation rate is modeled, the larger the predicted excess of binary black hole mergers

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-08T13:16:52.400971Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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 2026-08-13T06:32:02.005865+00:00.

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 2026-08-13T06:32:02.005865+00:00.

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 2026-08-13T06:32:02.005865+00:00.