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Paper Citation Record · LEDGER

High-Energy Radiation and Ion Acceleration in Three-dimensional Relativistic Magnetic Reconnection with Strong Synchrotron Cooling

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2305.02348.

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

pith.paper-citation-record.v1
2305.02348 v2

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 2026-08-13T06:32:02.005865+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T14:44:29.072941Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-22T10:16:22.688770Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • 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 2249582b-deec-4350-841c-c9b2eec7bbe7 · inbound

Can the neutrinos from TXS 0506+056 have a coronal origin? cites this paper.

Can the neutrinos from TXS 0506+056 have a coronal origin? High-Energy Radiation and Ion Acceleration in Three-dimensional Relativistic Magnetic Reconnection with Strong Synchrotron Cooling

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-09T14:44:29.072941Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-09T14:44:29.072941Z digest=sha256:e68d74a4ff18927a81ede1f8eff81392d8b8809a55510ef53581f43751bceb9e

Observation 9b0e7fee-6636-4bbc-a08c-4626fcac2aca · inbound

Single-source-class interpretation of the diffuse astrophysical neutrino flux cites this paper.

Single-source-class interpretation of the diffuse astrophysical neutrino flux High-Energy Radiation and Ion Acceleration in Three-dimensional Relativistic Magnetic Reconnection with Strong Synchrotron Cooling

Reference 33

Resolution
verified exact
arxiv_id, observed 2026-05-22T10:16:22.691429Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-05-22T10:15:07.047534Z digest=sha256:4033a491362f04d7cc8774579610bf60afddd29838bfbf166fa5066acf653f83