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Paper Citation Record · LEDGER

Cosmic Rays IV. The spectrum and chemical composition above $10^4$ GeV

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/9303006.

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

pith.paper-citation-record.v1
astro-ph/9303006 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 2026-08-23T06:30:58.430688+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T12:09:20.111162Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-13T00:16:21.800782Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • 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 a62222ce-bae1-4e83-9f70-b7263055b94b · inbound

Cosmic ray contributions from rapidly rotating stellar mass black holes: Cosmic Ray GeV to EeV proton and anti-proton sources cites this paper.

Cosmic ray contributions from rapidly rotating stellar mass black holes: Cosmic Ray GeV to EeV proton and anti-proton sources Cosmic Rays IV. The spectrum and chemical composition above $10^4$ GeV

Reference 106

Resolution
metadata mismatch
local_arxiv, observed 2026-08-12T18:51:59.172719Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-08-12T18:51:59.121779Z digest=sha256:d1e6f83d31d366a3b52795da1e4e091a0e559a8e3b33b3f62c4b1814b221e254

Observation 6b29fd36-4246-4116-b93f-93d688e88471 · inbound

A two-step strategy to identify episodic sources of gravitational waves and high energy neutrinos in starburst galaxies cites this paper.

A two-step strategy to identify episodic sources of gravitational waves and high energy neutrinos in starburst galaxies Cosmic Rays IV. The spectrum and chemical composition above $10^4$ GeV

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-16T12:09:20.111162Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T12:09:20.111162Z digest=sha256:f6b33af82e97e3a6ba73924a50cedcaabbe51e98968d14dcca28076f9969cdfd