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Paper Citation Record · LEDGER

The origin of high-energy astrophysical neutrinos: new results and prospects

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2311.00281.

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

pith.paper-citation-record.v1
2311.00281 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 2026-08-11T06:34:44.6726+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T15:43:23.199801Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-07T15:43:35.682886Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 1e021812-3f67-4179-8ea6-3b9b5ccfb889 · inbound

Constraints on Neutrino Secret Interactions from Multi-messenger Neutrinos Scattering on C$\nu$B cites this paper.

Constraints on Neutrino Secret Interactions from Multi-messenger Neutrinos Scattering on C$\nu$B The origin of high-energy astrophysical neutrinos: new results and prospects

Reference 56

Resolution
verified exact
local_arxiv, observed 2026-08-07T15:43:35.778816Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-07T15:43:23.199801Z digest=sha256:e2fa050696e749be61d8ad7a4a2c3c20c4661c820399dff755f7b76e565958dd

Observation 07e43f3b-dc5c-48f6-8933-ac51a500cef3 · inbound

Can a gamma-ray dim radio blazar produce a 200-PeV neutrino? The case of PMN J0606$-$0724 and KM3-230213A cites this paper.

Can a gamma-ray dim radio blazar produce a 200-PeV neutrino? The case of PMN J0606$-$0724 and KM3-230213A The origin of high-energy astrophysical neutrinos: new results and prospects

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-04T18:04:11.260210Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T18:04:11.260210Z digest=sha256:c7131996256e27d7ee98ed61f7d4c1112c98eaab6cf77ebc52cd1285389850e6