Pith. sign in

Paper Citation Record · LEDGER

Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2501.04778.

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

pith.paper-citation-record.v1
2501.04778 v1

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 2026-08-07T05:02:01.157340Z

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 704e3b52-c5c1-4f82-87e0-ebf524412e7d · inbound

Inferring the pair-instability mass gap from gravitational wave data cites this paper.

Inferring the pair-instability mass gap from gravitational wave data Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations

Reference 89

Resolution
unresolved
no resolver link, observed 2026-08-07T05:02:01.157340Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T05:02:01.157340Z digest=sha256:06fcceb31a1ac9aed7354b0c026ad6e0b0d9952edd73a360ccce32dad09445c3

Observation f17df02b-a237-44a1-a886-fe737f7706d1 · inbound

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

Can current models predict the local black hole merger rate? Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations

Reference 150

Resolution
verified exact
arxiv_id, observed 2026-06-28T13:02:10.881769Z

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=2026-06-28T13:01:54.102298Z digest=sha256:b87bca90e91d46319f28a47850e73d23ba85d780430badd8414cc7ea808ef449