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Paper Citation Record · LEDGER

On the Differential Rotation of Massive Main Sequence Stars

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1511.03809.

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

pith.paper-citation-record.v1
1511.03809 v1

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 2026-08-18T06:34:40.430872+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T14:18:47.098153Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

86
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 687b52f6-29fb-404f-a4b7-cf929981c561 · 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 On the Differential Rotation of Massive Main Sequence Stars

Reference 120

Resolution
verified exact
local_arxiv, observed 2026-05-19T19:42:44.028865Z

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:ca3cf83737651f8e34b81ede7d49e4a1a126e55ae92f3c9424163c05b6e41179

Observation 28daf1c6-f612-4432-a1e2-a78cc29a3db5 · 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 On the Differential Rotation of Massive Main Sequence Stars

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-12T12:11:54.407417Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T12:11:54.407417Z digest=sha256:37eec1024d7fd6beeefd5a9c177dc24e364f40412541a19683a4ed25c7ab8545

Observation f51f8175-265f-4d8a-a04e-3bf1e5115566 · 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 On the Differential Rotation of Massive Main Sequence Stars

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-15T14:18:47.098153Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T14:18:47.098153Z digest=sha256:31895489fde8b17006ce7b7d9856f5832b3b071bb30334ab0b773c0ebc0871da