Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Collective pulsational velocity broadening due to gravity modes as a physical explanation for macroturbulence in hot massive stars
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:0909.3585.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-05T20:04:16.086649Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-12T07:08:35.622816Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 3959235f-9509-4453-8c84-4f8e0d9b40b8 · inbound
The Stellar Observations Network Group (SONG) -- A Legacy Archive of Stellar Time-Domain Spectroscopy cites this paper.
The Stellar Observations Network Group (SONG) -- A Legacy Archive of Stellar Time-Domain Spectroscopy Collective pulsational velocity broadening due to gravity modes as a physical explanation for macroturbulence in hot massive stars
Reference 88
- Resolution
- verified exact
- local_arxiv, observed 2026-07-12T07:08:35.624933Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation f06ec259-1b0c-4271-bade-6dc5dd1c4b30 · 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 Collective pulsational velocity broadening due to gravity modes as a physical explanation for macroturbulence in hot massive stars
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T20:04:16.086649Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.