Paper Citation Record · LEDGER

Evolution of rapidly rotating metal-poor massive stars towards gamma-ray bursts

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:astro-ph/0508242.

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

pith.paper-citation-record.v1
astro-ph/0508242 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T13:05:39.589001Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-28T13:22:15.691659Z

Reference resolution

0 of 0 outbound references displayed

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verified fuzzy0
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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation dc254665-0c4f-4299-b159-d1feb8138a15 · inbound

Stable mass transfer in massive binaries leading to merging black holes cites this paper.

Stable mass transfer in massive binaries leading to merging black holes Evolution of rapidly rotating metal-poor massive stars towards gamma-ray bursts

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-03T14:34:24.372389Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f4cdeb0d-8c6d-4f19-9878-1a3de5e68076 · inbound

Mergers via failed common envelope as a route towards intermediate-mass stripped stars cites this paper.

Mergers via failed common envelope as a route towards intermediate-mass stripped stars Evolution of rapidly rotating metal-poor massive stars towards gamma-ray bursts

Reference 139

Resolution: verified exact; local_arxiv, observed 2026-05-25T02:20:13.709005Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 1445f30a-4a9b-44e3-96eb-0361ca210c7e · inbound

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

Can current models predict the local black hole merger rate? Evolution of rapidly rotating metal-poor massive stars towards gamma-ray bursts

Reference 136

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.623458Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation dee10233-4fa0-42c2-b824-224e57d9fa14 · inbound

Accretion of Primordial Black Holes in Stellar Interiors cites this paper.

Accretion of Primordial Black Holes in Stellar Interiors Evolution of rapidly rotating metal-poor massive stars towards gamma-ray bursts

Reference 294

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:22:15.692886Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 3e992f17-cc8d-4c06-a94c-9dba98cad576 · inbound

Fast Radio Bursts Trace Cosmic Star Formation with Little Delay cites this paper.

Fast Radio Bursts Trace Cosmic Star Formation with Little Delay Evolution of rapidly rotating metal-poor massive stars towards gamma-ray bursts

Reference 60

Resolution: unresolved; no resolver link, observed 2026-07-13T05:21:16.491609Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 59267153-2dd1-469c-a6f8-0452e208e69a · inbound

3D simulations of a complete convective silicon shell burning phase cites this paper.

3D simulations of a complete convective silicon shell burning phase Evolution of rapidly rotating metal-poor massive stars towards gamma-ray bursts

Reference 116

Resolution: unresolved; no resolver link, observed 2026-08-06T13:05:39.589001Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.