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Paper Citation Record · LEDGER

Massive stars at low metallicity: Evolution and surface abundances of O dwarfs in the SMC

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1304.6923.

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

pith.paper-citation-record.v1
1304.6923 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 2026-08-21T06:32:19.484+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-28T13:02:10.517761Z

Reference resolution

0 of 0 outbound references displayed

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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 e732847d-f1a0-45da-8947-33410a746160 · inbound

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

Can current models predict the local black hole merger rate? Massive stars at low metallicity: Evolution and surface abundances of O dwarfs in the SMC

Reference 198

Resolution
verified exact
local_arxiv, observed 2026-06-28T13:02:10.519024Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:7962ea8d0812a5baa8c59d8ab50d1d8bbe0e2cd35a47332d1ab7e32b2260dd9c

Observation b15eef83-4faa-4e67-b2f7-25c287d4fe36 · inbound

Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI cites this paper.

Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI Massive stars at low metallicity: Evolution and surface abundances of O dwarfs in the SMC

Reference 155

Resolution
verified exact
local_arxiv, observed 2026-06-26T18:09:41.429031Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:bd04c03d221705ec4fd3c111ef520da3f165376b1be7723d8449f528f7b9859c