Pith. sign in

Paper Citation Record · LEDGER

Expectations for high energy diffuse galactic neutrinos for different cosmic ray distributions

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1606.04489.

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

pith.paper-citation-record.v1
1606.04489 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T06:00:45.814185Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

36
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 91f61d75-ba1f-4500-9c4e-be10c5ac6057 · inbound

LHAASO protons versus LHAASO diffuse gamma-rays: a consistency check cites this paper.

LHAASO protons versus LHAASO diffuse gamma-rays: a consistency check Expectations for high energy diffuse galactic neutrinos for different cosmic ray distributions

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-07T06:00:45.814185Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T06:00:45.814185Z digest=sha256:a0d5448ceee2bc9b32771f5814bcda2a20aecd29659148d792a8133257486400

Observation d7567575-e0dc-4bcb-9f35-397571b33818 · inbound

Modelling Galactic neutrino emission: contributions from massive star clusters and interstellar cosmic rays cites this paper.

Modelling Galactic neutrino emission: contributions from massive star clusters and interstellar cosmic rays Expectations for high energy diffuse galactic neutrinos for different cosmic ray distributions

Reference 45

Resolution
verified exact
local_arxiv, observed 2026-07-03T02:57:35.358049Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-06-27T15:39:48.644607Z digest=sha256:cfc318bd02f2f66f9c09d660c88ff7c0097804e8d166f0da896baab704f588d0

Observation dd4f1c21-6796-4108-95b5-82d1b93e23e7 · inbound

TeV-PeV Gamma-ray and Neutrino Emission in the Galactic Plane cites this paper.

TeV-PeV Gamma-ray and Neutrino Emission in the Galactic Plane Expectations for high energy diffuse galactic neutrinos for different cosmic ray distributions

Reference 141

Resolution
verified exact
local_arxiv, observed 2026-06-26T07:29:08.372613Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:62c7f05307c48cc56cf10267fc07fbd1ac09578c0081e6a662d97b999ee16419