Paper Citation Record · LEDGER

The origin of power-law spectra in relativistic magnetic reconnection

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2302.12269.

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

pith.paper-citation-record.v1
2302.12269 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T04:39:37.709255Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-22T10:16:22.630006Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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malformed identifier0
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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 90831e85-e4db-46e4-93e9-cf72d4c368ab · inbound

Gamma-ray bursts: what do we know today that we did not know 10 years ago? cites this paper.

Gamma-ray bursts: what do we know today that we did not know 10 years ago? The origin of power-law spectra in relativistic magnetic reconnection

Reference 206

Resolution: unresolved; no resolver link, observed 2026-08-11T04:39:37.709255Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6e22153f-3211-4b9e-8b77-2f25dde515c8 · 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? The origin of power-law spectra in relativistic magnetic reconnection

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.395604Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 81a0b921-4ada-4eae-ac04-ae743e1d744f · 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? The origin of power-law spectra in relativistic magnetic reconnection

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.426656Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 90b65545-5e0e-4d40-b724-a34763e41f9e · inbound

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

Single-source-class interpretation of the diffuse astrophysical neutrino flux The origin of power-law spectra in relativistic magnetic reconnection

Reference 32

Resolution: verified exact; arxiv_id, observed 2026-05-22T10:16:22.632757Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.