Pith. sign in

Paper Citation Record · LEDGER

General constraints on sources of high-energy cosmic rays from the interaction losses

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2212.03483.

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

pith.paper-citation-record.v1
2212.03483 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 2026-08-04T18:04:16.219697Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-23T18:55:46.433887Z

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 2f8513ca-6d06-4d50-89fb-852865a5c2d3 · inbound

TeV to PeV neutrinos from AGN coronae cites this paper.

TeV to PeV neutrinos from AGN coronae General constraints on sources of high-energy cosmic rays from the interaction losses

Reference 18

Resolution
verified exact
arxiv_id, observed 2026-05-23T18:55:46.437481Z

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=2026-05-23T18:55:13.328874Z digest=sha256:0d67a81b9c65653a53ba398d340930d4e52a16cb374048bd753ef837f143a0ee

Observation e57003ac-bfe2-4b2a-9699-4d46010dfc3d · 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 General constraints on sources of high-energy cosmic rays from the interaction losses

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-04T18:04:16.219697Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T18:04:16.219697Z digest=sha256:b3b97955b7d58dd3d14ba5655ec0f4144e3af59c99bdd98028b1d40f93fb30a7