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Paper Citation Record · LEDGER

Theory and Diagnostics of Hot Star Mass Loss

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2109.08164.

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

pith.paper-citation-record.v1
2109.08164 v4

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T13:35:03.100181Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T00:05:50.383899Z

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 99f618f0-d3ce-4216-b13c-968e690a1575 · inbound

Evolution and final fates of low- and intermediate-mass stars cites this paper.

Evolution and final fates of low- and intermediate-mass stars Theory and Diagnostics of Hot Star Mass Loss

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-11T13:35:03.100181Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T13:35:03.100181Z digest=sha256:cb10e415baf16af93ff32e988a11e0e97f231080c192f9d1d96e828f1ef6446d

Observation 4cdc5557-d1ed-4b94-ab43-9a7f87d531b0 · inbound

How many VHE gamma-ray binaries with young pulsars can be observed? cites this paper.

How many VHE gamma-ray binaries with young pulsars can be observed? Theory and Diagnostics of Hot Star Mass Loss

Reference 66

Resolution
verified exact
arxiv_id, observed 2026-05-11T00:05:50.385704Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-10T18:42:16.317215Z digest=sha256:66274585f0a68f86c8eabbee7884af7cad083a5e0ed35eaf8489a6c04e4e47ae

Observation b46ae495-c893-4685-bc87-382494b22be4 · inbound

The Stellar Winds Atlas II: Black Hole Formation at Solar Metallicity cites this paper.

The Stellar Winds Atlas II: Black Hole Formation at Solar Metallicity Theory and Diagnostics of Hot Star Mass Loss

Reference 284

Resolution
unresolved
no resolver link, observed 2026-08-01T00:42:46.573552Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T00:42:46.573552Z digest=sha256:cff62026d2cff4403919026119516dc43c3ac56de4c436253b40cdbb380955f4