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Paper Citation Record · LEDGER

Oscillatory convective modes in red giants: a possible explanation of the long secondary periods

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1507.03430.

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

pith.paper-citation-record.v1
1507.03430 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 2026-08-16T06:30:59.297886+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T14:31:40.328671Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-27T15:10:59.246684Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
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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 f5db3d60-55b4-4658-94ae-238cefc84678 · inbound

CORALIE radial-velocity search for companions around evolved stars (CASCADES) V. Three planetary companions and achievable precision cites this paper.

CORALIE radial-velocity search for companions around evolved stars (CASCADES) V. Three planetary companions and achievable precision Oscillatory convective modes in red giants: a possible explanation of the long secondary periods

Reference 101

Resolution
verified exact
local_arxiv, observed 2026-06-27T15:10:59.248242Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:a69bbe8f34c4a879b998a8d276eb755d73cfdce07fcb1214e4294f08ebbd4a61

Observation 28da363c-dbba-4b3b-9147-a9bba5f54631 · inbound

Origin of the Long-Period Radial Velocity Variation in the Red Supergiant HD 216946 (V424 Lac) cites this paper.

Origin of the Long-Period Radial Velocity Variation in the Red Supergiant HD 216946 (V424 Lac) Oscillatory convective modes in red giants: a possible explanation of the long secondary periods

Reference 200

Resolution
unresolved
no resolver link, observed 2026-08-01T11:43:04.863009Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T11:43:04.863009Z digest=sha256:2e3466f908774495db656d70784c1911548afcc9f8684c141cd3d897d33d7a41

Observation da12d3cd-d0e0-4898-8e05-296ec3dfcb6f · inbound

White Dwarf Kicks via Episodic Mass Ejection from Red Giant Stars cites this paper.

White Dwarf Kicks via Episodic Mass Ejection from Red Giant Stars Oscillatory convective modes in red giants: a possible explanation of the long secondary periods

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-15T14:31:40.328671Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T14:31:40.328671Z digest=sha256:fcb08c6fa00ee7cca7e863508d7f9b6ec1c1c01726edba03c65b1bc3b23f8a5f