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Paper Citation Record · LEDGER

Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars

As of 22 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:1510.06960.

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

pith.paper-citation-record.v1
1510.06960 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-07-20T06:30:07.809122+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-02T06:26:43.465960Z

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 8b54e886-749b-4eab-9c24-01c5b0f628f9 · inbound

Asteroseismology of solar-type stars cites this paper.

Asteroseismology of solar-type stars Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars

Reference 174

Resolution
verified exact
local_arxiv, observed 2026-05-25T14:15:54.710051Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-20T06:30:07.809122+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:f639bf08e4979910ae0ab0a4a32da099b68be28313d62c840c4e4c1bc2dd0b31

Observation f199d942-ddcd-4895-a557-33d8cf151312 · inbound

Asteroseismology cites this paper.

Asteroseismology Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars

Reference 10

Resolution
verified exact
local_arxiv, observed 2026-05-23T20:13:24.414392Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-20T06:30:07.809122+00:00.

source=pdf_text observed=2026-07-11T11:50:26.030339Z digest=sha256:8cff86690e5fd96c30aa5db0d490ae6b6a976bf6e36099687ba762db03a39424

Observation 22d982f0-5348-44e4-98c2-f6bc71674829 · inbound

Seismic signature of a magnetic field in the $\gamma$ Doradus star KIC 2309579 cites this paper.

Seismic signature of a magnetic field in the $\gamma$ Doradus star KIC 2309579 Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars

Reference 8

Resolution
metadata mismatch
local_arxiv, observed 2026-05-22T03:54:33.828049Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-20T06:30:07.809122+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:bbd95b6adff0aa7cf86eb58bfb7ef9664c0376e7df9c87f3a0ad1530f475ec6a

Observation e5ccd01d-f0d2-458e-8890-0ed99074f751 · inbound

Non-linear Dynamical Stability of Magnetic Polytropes cites this paper.

Non-linear Dynamical Stability of Magnetic Polytropes Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars

Reference 28

Resolution
metadata mismatch
local_arxiv, observed 2026-06-28T18:52:30.557008Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-20T06:30:07.809122+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:26929faee6e837e11d773258e55b88d0dd1e0861455751fbdfb81a352bb8f0fa

Observation ed39607c-6e07-4c54-8dbd-3ef761a00935 · inbound

Extending asteroseismic magnetometry across the diverse landscape of magnetic structures cites this paper.

Extending asteroseismic magnetometry across the diverse landscape of magnetic structures Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars

Reference 10

Resolution
metadata mismatch
local_arxiv, observed 2026-06-27T20:41:14.469842Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-20T06:30:07.809122+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b765533e45c2046d41b77e00f04a628ca62d7a3fc998b2a64a0a68863aebc9be

Observation c2c6080a-a355-4784-ad33-1de9a9b416a3 · inbound

Oscillations of red giant stars with magnetic damping in the core. II. Mixed mode visibilities on the red-giant branch cites this paper.

Oscillations of red giant stars with magnetic damping in the core. II. Mixed mode visibilities on the red-giant branch Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars

Reference 124

Resolution
metadata mismatch
local_arxiv, observed 2026-06-28T03:31:30.822544Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-20T06:30:07.809122+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:5da8bc16df114a83393c1b782aa57aa68d641826b19a50854940a13034ac4725

Observation bae1a321-56f7-43b0-99b6-8a8223738ef0 · inbound

The effect of near-core mixing on rejuvenation and the asteroseismic properties of massive accretors cites this paper.

The effect of near-core mixing on rejuvenation and the asteroseismic properties of massive accretors Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars

Reference 104

Resolution
metadata mismatch
local_arxiv, observed 2026-06-27T05:40:36.413143Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-20T06:30:07.809122+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:34abfcde17926ebe03c6e751f0db7429dc4e9b8334b09832607310001dfec8f8

Observation a03d8e34-4396-4146-a536-ce348aba4e87 · inbound

Constraining the model-based uncertainties of asteroseismic magnetic field measurements in red giants cites this paper.

Constraining the model-based uncertainties of asteroseismic magnetic field measurements in red giants Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars

Reference 73

Resolution
metadata mismatch
local_arxiv, observed 2026-07-02T06:26:43.467164Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-20T06:30:07.809122+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:33686503ea36daacf3082450be6127a6c75dd4a8342824f3890c4a670166e2b9