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Paper Citation Record · LEDGER

Predictions for the flux of high-energy cosmogenic neutrinos and the influence of the extragalactic magnetic field

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1810.03769.

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

pith.paper-citation-record.v1
1810.03769 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 2026-08-15T06:32:42.880941+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T19:10:39.736459Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-14T05:10:37.285981Z

Reference resolution

0 of 0 outbound references displayed

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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 93e67f91-2d3f-47ba-9350-06ce730e3d8f · inbound

Current constraints from cosmogenic neutrinos on the fraction of protons in UHECRs cites this paper.

Current constraints from cosmogenic neutrinos on the fraction of protons in UHECRs Predictions for the flux of high-energy cosmogenic neutrinos and the influence of the extragalactic magnetic field

Reference 23

Resolution
verified exact
local_arxiv, observed 2026-08-14T05:10:37.290596Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T05:10:37.131882Z digest=sha256:cfa9be86ef52cf46268118b7e751eb07cd8ba98630851c2da54fbdd274c61459

Observation 85b479a9-2ee2-4eca-bc91-e6e4c0250256 · inbound

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos cites this paper.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Predictions for the flux of high-energy cosmogenic neutrinos and the influence of the extragalactic magnetic field

Reference 111

Resolution
unresolved
no resolver link, observed 2026-08-15T19:10:39.736459Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T19:10:39.736459Z digest=sha256:454902e75481719cc0918394f81efd1c4f8c9ed123a6d6e28a292586a7fa85bb