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Paper Citation Record · LEDGER

Observational signatures of convectively driven waves in massive stars

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1505.06648.

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

pith.paper-citation-record.v1
1505.06648 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T14:18:47.069166Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-19T19:42:43.941347Z

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 59c49f19-b1b5-418a-9430-8eba8357aa9b · inbound

Binarity at LOw Metallicity (BLOeM): massive star variability revealed using a novel software tool for point-spread function fitting of TESS images cites this paper.

Binarity at LOw Metallicity (BLOeM): massive star variability revealed using a novel software tool for point-spread function fitting of TESS images Observational signatures of convectively driven waves in massive stars

Reference 80

Resolution
verified exact
local_arxiv, observed 2026-05-19T19:42:43.942957Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:03118d647ffe6fa626f81b252e6a3caee17d195a55465f9e8bbf4be964f3c979

Observation 5e9f7ae1-da54-4621-8635-0942d622c951 · inbound

The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry cites this paper.

The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry Observational signatures of convectively driven waves in massive stars

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-05T20:04:16.578906Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T20:04:16.578906Z digest=sha256:32f529f105b86326d0784207457cbf5bfac92ce644bcdc9ef55651e1f3831677

Observation 1633f3cc-539b-403f-ac66-359fe83ce740 · inbound

Characterization of the variability of the blue supergiant HD 14134 cites this paper.

Characterization of the variability of the blue supergiant HD 14134 Observational signatures of convectively driven waves in massive stars

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-06T18:25:19.419121Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T18:25:19.419121Z digest=sha256:5035768c74652538f6a57cf36e08dfee8b8bb553f0ae0966d4cdd88b6e50a2f9

Observation 20367887-ef00-4707-a758-06d1d47b7320 · inbound

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants cites this paper.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Observational signatures of convectively driven waves in massive stars

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-12T12:11:54.400377Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T12:11:54.400377Z digest=sha256:861a21c4af92c1d1752f2e6092e5cd0c9eafe9a0e660ca1cb139539ac7891ff1

Observation 802c9fb5-c26d-4738-af95-62f1681a65f7 · inbound

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants cites this paper.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Observational signatures of convectively driven waves in massive stars

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-15T14:18:47.069166Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T14:18:47.069166Z digest=sha256:5905b6e1ff844e0edab8f83887b30992883f9a3bbfd88aa9badbdc33b397f4cf