Paper Citation Record · LEDGER

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions

As of 14 August 2026, this Paper Citation Record lists 32 of 32 outbound references and 0 inbound Pith citation observations for arXiv:2411.10223.

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

pith.paper-citation-record.v1
2411.10223 v1

Coverage vector

measured 32 of 32 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-12T19:55:11.033921Z

measured 32 of 32 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

32 of 32 outbound references displayed

verified exact6
verified fuzzy10
unresolved16
parse uncertain0
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 7077db4c-adc5-4121-9a08-3530632e0192 · outbound

This paper cites We denote theselectedeventsas {( ˜Ei, ˜Xmax,i, δ˜Xmax,i)}ℓ, with i = 1,.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions We denote theselectedeventsas {( ˜Ei, ˜Xmax,i, δ˜Xmax,i)}ℓ, with i = 1,

Reference 1

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T19:55:11.536269Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 9d42e0da-0fca-481b-8f00-d9fa97b7a69a · outbound

This paper cites an unresolved cited work.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Unresolved cited work

Reference 2

Resolution: unresolved; raw_fallback, observed 2026-08-12T19:55:11.526306Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation cfaf4217-18fc-46af-9447-4379171c9b30 · outbound

This paper cites an unresolved cited work.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Unresolved cited work

Reference 3

Resolution: unresolved; raw_fallback, observed 2026-08-12T19:55:11.516679Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 94a81266-b979-4860-abd4-eaef0a71270b · outbound

This paper cites an unresolved cited work.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Unresolved cited work

Reference 4

Resolution: unresolved; raw_fallback, observed 2026-08-12T19:55:11.508262Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 632b1558-d14d-4de1-85fa-ac0ed2116672 · outbound

This paper cites an unresolved cited work.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Unresolved cited work

Reference 5

Resolution: unresolved; raw_fallback, observed 2026-08-12T19:55:11.499012Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 4ff91f6f-ec1d-4aef-abf4-3de58ab2e0b8 · outbound

This paper cites Ultra-High Energy Heavy Nuclei Propagation in Extragalactic Magnetic Fields.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Ultra-High Energy Heavy Nuclei Propagation in Extragalactic Magnetic Fields

Reference 6

Resolution: verified exact; local_arxiv, observed 2026-08-12T19:55:11.385598Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 5456c810-3818-4682-8bfb-01c728911245 · outbound

This paper cites an unresolved cited work.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Unresolved cited work

Reference 7

Resolution: verified exact; raw_fallback, observed 2026-08-12T19:55:11.370156Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 9ab29cbf-3e51-4d75-a221-0387eb7cacae · outbound

This paper cites Andringa, R.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Andringa, R

Reference 8

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T19:55:11.488319Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 4112e6fa-a3d5-417f-a248-632d5c4e2a04 · outbound

This paper cites The Pierre Auger Cosmic Ray Observatory.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions The Pierre Auger Cosmic Ray Observatory

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-12T19:55:10.955563Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5f731559-4d7c-4c77-b68d-380f2d9af25f · outbound

This paper cites AugerPrime -- The upgrade of the Pierre Auger Observatory.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions AugerPrime -- The upgrade of the Pierre Auger Observatory

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-12T19:55:10.959225Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ee0a64e4-13b8-469e-88c7-22edad42ad7c · outbound

This paper cites Kawai, S.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Kawai, S

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T19:55:11.477614Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 2940c1c7-60fd-433e-b16a-de0ceac7a2d3 · outbound

This paper cites QGSJET-III model of high energy hadronic interactions: II. Particle production and extensive air shower characteristics.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions QGSJET-III model of high energy hadronic interactions: II. Particle production and extensive air shower characteristics

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-12T19:55:10.966816Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 04334a5b-4b9d-4501-b706-eff825acfebb · outbound

This paper cites Constraining models for the origin of ultra-high-energy cosmic rays with a novel combined analysis of arrival directions, spectrum, and composition data measured at the Pierre Auger Observatory.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Constraining models for the origin of ultra-high-energy cosmic rays with a novel combined analysis of arrival directions, spectrum, and composition data measured at the Pierre Auger Observatory

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-12T19:55:10.970396Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 67a53a72-264f-4701-a7fc-49d6957710d3 · outbound

This paper cites Blazek, J.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Blazek, J

Reference 14

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T19:55:11.466411Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation b6aefcb9-64e3-4c2f-9d6f-a800f7afc040 · outbound

This paper cites On the model uncertainties for the predicted maximum depth of extensive air showers.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions On the model uncertainties for the predicted maximum depth of extensive air showers

Reference 15

Resolution: verified exact; local_arxiv, observed 2026-08-12T19:55:11.173852Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation f83eb1dd-94dd-4c7c-95ac-135d875b24b5 · outbound

This paper cites Working Group Report on the Combined Analysis of Muon Density Measurements from Eight Air Shower Experiments.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Working Group Report on the Combined Analysis of Muon Density Measurements from Eight Air Shower Experiments

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-12T19:55:10.980914Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0f1d6fe3-91d1-4616-835f-48c547882faa · outbound

This paper cites Learning the Composition of Ultra High Energy Cosmic Rays.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Learning the Composition of Ultra High Energy Cosmic Rays

Reference 17

Resolution: verified exact; local_arxiv, observed 2026-08-12T19:55:11.150673Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 005cd042-eb03-4cfa-89c2-37a48f76c6c4 · outbound

This paper cites Improving the Composition of Ultra High Energy Cosmic Rays with Ground Detector Data.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Improving the Composition of Ultra High Energy Cosmic Rays with Ground Detector Data

Reference 18

Resolution: verified exact; local_arxiv, observed 2026-08-12T19:55:11.137219Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 822b58ad-4644-4500-8c6a-0ecc6f979126 · outbound

This paper cites Resolution of (Heavy) Primaries in Ultra High Energy Cosmic Rays.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Resolution of (Heavy) Primaries in Ultra High Energy Cosmic Rays

Reference 19

Resolution: verified exact; local_arxiv, observed 2026-08-12T19:55:11.123329Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 61897035-829c-4e68-80e6-c6532c15efe3 · outbound

This paper cites Pierre auger observatory 2021 open data,.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Pierre auger observatory 2021 open data,

Reference 20

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T19:55:11.456099Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation d360e7cd-1eb0-4604-8e7f-e9f1bb6a34a3 · outbound

This paper cites Depth of Maximum of Air-Shower Profiles at the Pierre Auger Observatory: Measurements at Energies above 10^17.8 eV.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Depth of Maximum of Air-Shower Profiles at the Pierre Auger Observatory: Measurements at Energies above 10^17.8 eV

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-12T19:55:10.996849Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f9f019f3-88bb-4b36-b0b6-646b2217826c · outbound

This paper cites CORSIKA: A Monte Carlo code to simulate extensive air showers,.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions CORSIKA: A Monte Carlo code to simulate extensive air showers,

Reference 22

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T19:55:11.446214Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 2ee81010-54dc-41a7-8594-e1b9370b3916 · outbound

This paper cites EPOS LHC : test of collective hadronization with LHC data.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions EPOS LHC : test of collective hadronization with LHC data

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-12T19:55:11.003484Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0b41f806-ab73-4867-9196-228e5f2464d0 · outbound

This paper cites Sibyll$^{\bigstar}$.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Sibyll$^{\bigstar}$

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-12T19:55:11.006807Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9e8f17cb-d442-4768-b3d4-b70f72bd08f5 · outbound

This paper cites Monte Carlo treatment of hadronic interactions in enhanced Pomeron scheme: I. QGSJET-II model.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Monte Carlo treatment of hadronic interactions in enhanced Pomeron scheme: I. QGSJET-II model

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-12T19:55:11.010551Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4cf51c9f-16bc-48d5-8291-90fd60c77856 · outbound

This paper cites an unresolved cited work.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Unresolved cited work

Reference 26

Resolution: unresolved; raw_fallback, observed 2026-08-12T19:55:11.435996Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 6ddd9d85-78d8-4b2d-ba5d-e178814b4987 · outbound

This paper cites EPOS4: New theoretical concepts for modeling proton-proton and ion-ion scattering at very high energies.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions EPOS4: New theoretical concepts for modeling proton-proton and ion-ion scattering at very high energies

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-12T19:55:11.017182Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8e80313b-dd68-41ac-a71d-66b11667672b · outbound

This paper cites Efron and R.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Efron and R

Reference 28

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T19:55:11.424301Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 21bd3d6e-cfa7-4117-a613-f73c4efa155f · outbound

This paper cites Skilling, AIP Conference Proceedings735, 395 (2004), https://aip.scitation.org/doi/pdf/10.1063/1.1835238.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Skilling, AIP Conference Proceedings735, 395 (2004), https://aip.scitation.org/doi/pdf/10.1063/1.1835238

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-12T19:55:11.024225Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c2209b6c-1d02-48ef-be2a-8de5a851bc7c · outbound

This paper cites Buchner, Statistics and Computing26, 383 (2014).

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Buchner, Statistics and Computing26, 383 (2014)

Reference 30

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T19:55:11.415015Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation db72754a-5059-4b14-8cb1-470c68333cbe · outbound

This paper cites Collaborative nested sampling: Big data vs. complex physical models,.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Collaborative nested sampling: Big data vs. complex physical models,

Reference 31

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T19:55:11.405643Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 49662038-3331-473b-a104-e7f82401e273 · outbound

This paper cites Ultranest – a robust, general purpose bayesian inference engine,.

Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions Ultranest – a robust, general purpose bayesian inference engine,

Reference 32

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T19:55:11.396672Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Pith citing papers

No inbound Pith citation observations are available.