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Paper Citation Record · LEDGER

Quantitative spectroscopy of late O-type main-sequence stars with a hybrid non-LTE method

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2301.09462.

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

pith.paper-citation-record.v1
2301.09462 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 2026-08-08T13:33:06.266147Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

No source-named external measurement is stored.

Outbound references

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Pith citing papers

Observation e32b71c9-14b5-41db-9016-32ea479f9cb0 · inbound

3D Non-LTE radiation transfer: theory and applications to stars, exoplanets, and kilonovae cites this paper.

3D Non-LTE radiation transfer: theory and applications to stars, exoplanets, and kilonovae Quantitative spectroscopy of late O-type main-sequence stars with a hybrid non-LTE method

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-03T23:48:48.664483Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-03T23:48:48.664483Z digest=sha256:24edc71557558a8d53a2fdc0e6579a5b2180ecd2da15009d129c23137af8cf19

Observation d6dced30-9ae7-43fd-8c9e-f2556a981d7e · inbound

The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars cites this paper.

The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars Quantitative spectroscopy of late O-type main-sequence stars with a hybrid non-LTE method

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-08T13:33:06.266147Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T13:33:06.266147Z digest=sha256:7f102a17457e33423420e37210bbacdaffac42c6b99d74e1fe154f68db298a5c