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Paper Citation Record · LEDGER

A Magnetic Confinement vs. Rotation Classification of Massive-Star Magnetospheres

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1211.0282.

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

pith.paper-citation-record.v1
1211.0282 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T15:19:16.649442Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-25T02:50:15.055017Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • 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 1996f90d-1d5e-4673-a16c-61d16b55937c · inbound

GMRT Survey of Radio Emission from Magnetic Massive Stars -- I: Emission from Single Stars at sub-GHz Frequencies cites this paper.

GMRT Survey of Radio Emission from Magnetic Massive Stars -- I: Emission from Single Stars at sub-GHz Frequencies A Magnetic Confinement vs. Rotation Classification of Massive-Star Magnetospheres

Reference 253

Resolution
verified exact
local_arxiv, observed 2026-05-25T02:50:15.057178Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:ea08f488b1623115f9a1c59f4a4db3c5e104fc10ba10c0e9f3704202dec0a30b

Observation c09f619b-4c67-463f-a3a4-a3db665ed04c · inbound

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir cites this paper.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir A Magnetic Confinement vs. Rotation Classification of Massive-Star Magnetospheres

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.649442Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.649442Z digest=sha256:24959252e3ae787655bceef8638c6f42bf3e76f31b5e54898145df6b74616b96