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Paper Citation Record · LEDGER

The Heavier the Faster: A Sub-population of Heavy, Rapidly Spinning and Quickly Evolving Binary 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:2406.03257.

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

pith.paper-citation-record.v1
2406.03257 v1

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 2026-08-04T08:07:40.212654Z

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

1
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 312e7d0f-7b8e-40c7-aee4-953861d93fbc · inbound

A new group of low-spin $50-70M_\odot$ Black Holes and the high pair-instability mass cutoff cites this paper.

A new group of low-spin $50-70M_\odot$ Black Holes and the high pair-instability mass cutoff The Heavier the Faster: A Sub-population of Heavy, Rapidly Spinning and Quickly Evolving Binary Black Holes

Reference 22

Resolution
verified exact
arxiv_id, observed 2026-05-22T12:41:33.128623Z

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=2026-05-22T12:40:21.857869Z digest=sha256:31535b1add4470066c15d991e58e8e8523f05f1b04079542d41b70df8c4a29c8

Observation 7e682b81-33e7-4055-9baa-d62c9b2a84a7 · inbound

A new group of low-spin $50-70M_\odot$ Black Holes and the high pair-instability mass cutoff cites this paper.

A new group of low-spin $50-70M_\odot$ Black Holes and the high pair-instability mass cutoff The Heavier the Faster: A Sub-population of Heavy, Rapidly Spinning and Quickly Evolving Binary Black Holes

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-04T08:07:40.212654Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T08:07:40.212654Z digest=sha256:05d3d2b9e26bae819543833fd79fa0a445a8879aeea049213677a724b4d25b78

Observation 1078efc5-5b0f-4656-82c1-296004cf71e6 · inbound

How do the LIGO-Virgo-KAGRA's Heavy Black Holes Form? No evidence for core-collapse Intermediate-mass black holes in GWTC-4 cites this paper.

How do the LIGO-Virgo-KAGRA's Heavy Black Holes Form? No evidence for core-collapse Intermediate-mass black holes in GWTC-4 The Heavier the Faster: A Sub-population of Heavy, Rapidly Spinning and Quickly Evolving Binary Black Holes

Reference 138

Resolution
metadata mismatch
arxiv_id, observed 2026-05-08T23:14:24.716402Z

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=arxiv_source observed=2026-05-08T06:31:36.774997Z digest=sha256:7efbbe8be443445f79816248a707ac696d2c987a81b2b55058fea899bcd7b2b7