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Paper Citation Record · LEDGER

Binary evolution models with rotation

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0302232.

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

pith.paper-citation-record.v1
astro-ph/0302232 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 2026-08-09T06:31:02.800959+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T15:35:16.324749Z

measured 1 of 1 external citation measurements

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

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

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 2054236d-ee41-4c97-b2d8-903e83da53ce · inbound

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions cites this paper.

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions Binary evolution models with rotation

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:16.324749Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:35:16.324749Z digest=sha256:35677c87bf04d66238d957b42aeca2e44b3abb8c082fdc4fbcfa6a6c680894ac

Observation dc1deb0a-6e45-4155-8fbc-54d2d5520f30 · inbound

You're Gonna Need a Bigger Core: Calibrating Massive Star Models against Galactic OB-type Stars cites this paper.

You're Gonna Need a Bigger Core: Calibrating Massive Star Models against Galactic OB-type Stars Binary evolution models with rotation

Reference 276

Resolution
metadata mismatch
local_arxiv, observed 2026-08-04T05:09:39.743962Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-08-04T05:08:03.888155Z digest=sha256:9ef18ad224b0d01a0706219539678ead1e05bc3119e270bd87bc01163317ef73