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Paper Citation Record · LEDGER

An `Analytic Dynamical Magnetosphere' formalism for X-ray and optical emission from slowly rotating magnetic massive stars

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1607.08568.

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

pith.paper-citation-record.v1
1607.08568 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 2026-08-15T15:19:16.573344Z

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

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  • verified fuzzy0
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External citation measurements

57
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation e3578139-baf9-427a-a5d1-3ad955f5f4de · 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 An `Analytic Dynamical Magnetosphere' formalism for X-ray and optical emission from slowly rotating magnetic massive stars

Reference 248

Resolution
verified exact
local_arxiv, observed 2026-05-25T02:50:15.240013Z

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=sha256:17fb7c294822d6346fabcbbc5cf88bdf6bde97313ff5c43cd17c2a8bc2903e42

Observation 69997a28-20ba-413a-ba59-7230907527b5 · 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 An `Analytic Dynamical Magnetosphere' formalism for X-ray and optical emission from slowly rotating magnetic massive stars

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.573344Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.573344Z digest=sha256:22146dd9b4d6dae6ace3bda4020672017cdf29fbab7d2fc64d988d93d9eebdc9