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Paper Citation Record · LEDGER

Data-driven model of the cosmic-ray flux and mass composition from 10 GeV to $10^{11}$ GeV

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1711.11432.

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

pith.paper-citation-record.v1
1711.11432 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T11:45:35.529151Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T02:57:35.302035Z

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 2ba05099-f955-47f3-ae02-3daee5f85a6e · inbound

A New Method for Measuring the Pion-Air Cross Section at Multi-TeV Energies Using Muon Bundle Properties in Deep Underground Detectors cites this paper.

A New Method for Measuring the Pion-Air Cross Section at Multi-TeV Energies Using Muon Bundle Properties in Deep Underground Detectors Data-driven model of the cosmic-ray flux and mass composition from 10 GeV to $10^{11}$ GeV

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-06T11:45:35.529151Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T11:45:35.529151Z digest=sha256:d1d77e1a1ea5c1dac9a141c8f026aa677c886f57500ab4d266b89c27d21d2e39

Observation 37ba7773-5720-4355-bde5-af8a9f5cbc12 · inbound

Exploring New Propagation Scales With Galactic Neutrinos cites this paper.

Exploring New Propagation Scales With Galactic Neutrinos Data-driven model of the cosmic-ray flux and mass composition from 10 GeV to $10^{11}$ GeV

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-03T17:08:36.111670Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T17:08:36.111670Z digest=sha256:1193adc0a1795921d56d7a29c31fcb6323d151178c5ccb5727655c8170cb55f7

Observation 880a28e9-1895-45a7-9ba1-f385944e7d11 · inbound

Mountain Muography for China Jinping Underground Laboratory cites this paper.

Mountain Muography for China Jinping Underground Laboratory Data-driven model of the cosmic-ray flux and mass composition from 10 GeV to $10^{11}$ GeV

Reference 27

Resolution
verified exact
local_arxiv, observed 2026-07-02T16:07:08.599109Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-06-27T23:03:40.799637Z digest=sha256:78581b856ac2aac9ada3fc1b00e431ee0d40c137ca24a60400153d01b7701fd5

Observation 69dbf327-6fe8-40de-9d29-5fcb9d16c465 · 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 Data-driven model of the cosmic-ray flux and mass composition from 10 GeV to $10^{11}$ GeV

Reference 62

Resolution
verified exact
local_arxiv, observed 2026-07-03T02:57:35.303761Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-06-27T15:39:48.644607Z digest=sha256:c2dec0167b61fe46817d0352f26f97d08702317de43407d7ecf6d870935a141b