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Paper Citation Record · LEDGER

Magnetic fields of non-degenerate stars

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:0904.1938.

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

pith.paper-citation-record.v1
0904.1938 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 12 of 12 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 12 of 12 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T17:19:39.453433Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-04T18:50:04.512610Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 d3276893-dfd2-44f3-b722-d65e40726c25 · inbound

Stripped-Envelope Supernovae for QCD Axion Detection cites this paper.

Stripped-Envelope Supernovae for QCD Axion Detection Magnetic fields of non-degenerate stars

Reference 57

Resolution
verified exact
local_arxiv, observed 2026-05-17T21:40:17.900269Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-17T21:37:41.394551Z digest=sha256:b56acaaa10c58c8c567a2fa91c7139e3badd016b6cc88732cbf62594c24bccb2

Observation ff5a7038-1fc8-4bd0-a244-bdc38aa6d8fc · inbound

Testing the reliability of magnetic field strength measurements for M dwarfs cites this paper.

Testing the reliability of magnetic field strength measurements for M dwarfs Magnetic fields of non-degenerate stars

Reference 40

Resolution
verified exact
local_arxiv, observed 2026-05-20T00:47:54.685440Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:7ccef1b7280720c8ad24b8dde00bb035816be2d7e90882210c159a8064c354d2

Observation 6f1608e8-6a98-4689-bf86-854ecd2275c6 · 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 Magnetic fields of non-degenerate stars

Reference 124

Resolution
verified exact
local_arxiv, observed 2026-06-27T05:40:36.212559Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:7137a94185ad66fa1352ccc459975da5e5f56d0fe2da6b6443f26b42d16fbfd0

Observation 0b2501d7-5a2d-4277-91b3-630a47261f8b · inbound

Ultra-High-Resolution Astronomy with the Solar Gravitational Lens cites this paper.

Ultra-High-Resolution Astronomy with the Solar Gravitational Lens Magnetic fields of non-degenerate stars

Reference 25

Resolution
verified exact
local_arxiv, observed 2026-07-03T22:49:01.564411Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-06-26T23:16:41.283331Z digest=sha256:6c9d3cacae4cc036b85134dce43b0605d94835be9f481d9af05e8ebfdc90135a

Observation 70944ea7-bf3e-4b8c-b8f1-583940ed14e4 · inbound

Beyond the Tayler instability: A new global instability of toroidal magnetic fields in stars cites this paper.

Beyond the Tayler instability: A new global instability of toroidal magnetic fields in stars Magnetic fields of non-degenerate stars

Reference 2

Resolution
verified exact
local_arxiv, observed 2026-07-04T18:50:04.513886Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-06-25T22:31:24.799621Z digest=sha256:fd4da150ad0e622e28d70e63c5f1046b4dea6f20e5e29d2063bdb87cfceed7be

Observation 2b2f0d90-a44b-425e-bdc7-216f4b79e294 · inbound

Exploring Activity Across the Stellar Main Sequence with the Sun as a Benchmark cites this paper.

Exploring Activity Across the Stellar Main Sequence with the Sun as a Benchmark Magnetic fields of non-degenerate stars

Reference 10

Resolution
verified exact
local_arxiv, observed 2026-06-25T21:18:24.839737Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:bdae5111f917612c2f85da8d5a6f2978b55052ff31cf41979c75bacbca8c0b76

Observation 5e40e8f4-d595-48b4-92b4-fabaa159b88f · inbound

Magnetic activity in cool stars: manifestations and relevance to exoplanets cites this paper.

Magnetic activity in cool stars: manifestations and relevance to exoplanets Magnetic fields of non-degenerate stars

Reference 293

Resolution
verified exact
local_arxiv, observed 2026-07-01T03:05:19.437649Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:5e822ec4da60ac562c363af816201f85fdb430ba991357d8e54ab74c0b5ec524

Observation 5a747bc6-fede-4777-9efe-becb59c147fc · inbound

Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations cites this paper.

Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations Magnetic fields of non-degenerate stars

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-03T12:59:18.031200Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-03T12:59:18.031200Z digest=sha256:3fc78b459ee2d95a68421089787cad0f1f2c0a87c2c85864ef9b1ca568d180c0

Observation 2d47f841-dee6-4bb8-95fb-d49d2a0b81fb · inbound

Pollux UV & FUV polarimeters: first lab results cites this paper.

Pollux UV & FUV polarimeters: first lab results Magnetic fields of non-degenerate stars

Reference 25

Resolution
unresolved
no resolver link, observed 2026-08-04T14:53:29.931214Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T14:53:29.931214Z digest=sha256:861530183627cf7659fcf825c3020dffbb556811165c65b675dda053713f199c

Observation f3536180-19ea-4229-839c-6ccfe4175ced · 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 Magnetic fields of non-degenerate stars

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-05T20:04:22.594010Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T20:04:22.594010Z digest=sha256:88a3cd203718f2abf2a616b8d765f4aeb503f335e6aedec18a942c5d59b1ba54

Observation 12cc9f4f-eba4-49f2-9a83-665e1866e0e7 · inbound

3D simulations of a complete convective silicon shell burning phase cites this paper.

3D simulations of a complete convective silicon shell burning phase Magnetic fields of non-degenerate stars

Reference 186

Resolution
unresolved
no resolver link, observed 2026-08-06T13:05:39.761701Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T13:05:39.761701Z digest=sha256:b26c0a9e098af1cbe6825bc24a1e51098a1dd1141ba6795797eb879ee97c1140

Observation c6a6ce6e-5562-4b0e-898b-85c41b5e8a12 · inbound

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation cites this paper.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Magnetic fields of non-degenerate stars

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-10T17:19:39.453433Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T17:19:39.453433Z digest=sha256:92646760b5fe89bbf7ec1b33bcc5671a2f821b2c6393e1d9cb51c2a76adeccb1