Pith. sign in

Paper Citation Record · LEDGER

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

As of 21 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 2026-08-21T06:32:19.484+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
  • malformed identifier0
  • metadata mismatch0

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:10.926075Z digest=sha256:150317561e3cbe47ea81addfb3d8a06e5f7281dfe6d9ecebc38d352ad6336d2d

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:10.929992Z digest=sha256:ec8aaad1932a4f3de438d81e7cd06a7b0b45b47e90a7c08d8209040647440b6b

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:10.933619Z digest=sha256:37352941d51f5a7579f5b0d9d114f6019859b08cdc2830067aabfc8c8a30c954

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:10.937549Z digest=sha256:72158c1cc7de34d95a77fe70737e8d66c2df7e19fb121c2248725676746bdc16

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:10.941311Z digest=sha256:efc761d840e3324779bceffd87566f5caf28b40728c4e398bc3cf6b4dc1ae698

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:10.945049Z digest=sha256:8b66c02feedd931ad463aaec243c18bb2854062131abcb83d9f80ffce4eb7cf8

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:10.948912Z digest=sha256:9369379adb32450e250840b03971d8a7b1d7d86489bb42a55ccf55c2e6f7487e

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:10.952164Z digest=sha256:ce548e5ab3883849405a5a5d431602aa916dda204834a48723e30c42707c6259

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.

source=pdf_text observed=2026-08-12T19:55:10.955563Z digest=sha256:3e671c8a98f041fd32f10a37d4d63206d04a608080bffed1ebc9ad81dffc8a12

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.

source=pdf_text observed=2026-08-12T19:55:10.959225Z digest=sha256:01a8acc3061fe2a05b8ca184e09ba6aeaa9747b85f158e9b23119b02b352108f

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:10.963277Z digest=sha256:d21bbe25521b4e2942a4293342a494b1d671d1d99e527bc827fb5e24b2cfdfe6

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.

source=pdf_text observed=2026-08-12T19:55:10.966816Z digest=sha256:a3381ea0ab2e968e0ba59cae5c5c7d247e9f41f5a0adb03b083730d05c205c56

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.

source=pdf_text observed=2026-08-12T19:55:10.970396Z digest=sha256:69904b05abe534b791b238ebe674ba3ab1999d2b7fa7dd426fbe5761de55023a

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:10.974031Z digest=sha256:af2863ed83b02c355097dc3f67282a006ec4cb08d622ad83990d67988d16f1c1

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:10.977182Z digest=sha256:50f9fb3d63a8876f1b5ebc859195cb8d1fa1b8a8fc0fc6c8b62a58de66e51838

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.

source=pdf_text observed=2026-08-12T19:55:10.980914Z digest=sha256:1cfd00b8c07d412cdd226a8ed74e292e79f131a3465cc84c95b629751161efc0

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:10.984571Z digest=sha256:9ba4fbb9e1ae6abdfdc03e52d2e440a7221e1a47f4f46e4a2a0c295b2d4fd9db

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:10.987784Z digest=sha256:d5aab1af5edb09d12ca9aa3af5f37a7f9d183a82b45021ce79afb7efd381ea57

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:10.990600Z digest=sha256:fe765fab3c2a7fd52b3865eb6032fb17964c64d0805007bd4a0e4726d1eef93c

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:10.993941Z digest=sha256:ec938aad2d8b25b387d3bb75ee39bee7fb9b955528175a1a1a3ac43543247974

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.

source=pdf_text observed=2026-08-12T19:55:10.996849Z digest=sha256:b2ccdd69bba2e8b7b42924397993d1fe2ef0851fdd595a1a33582de41718ed54

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:11.000396Z digest=sha256:ee77de3bc020a7bbecf47633e31c18f30799236a86aa5aab30d42a14dac2b4c0

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.

source=pdf_text observed=2026-08-12T19:55:11.003484Z digest=sha256:06152e2fc44c65d17361df96bd5d26555f9c8a2906eb1104ad5b213005548c02

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.

source=pdf_text observed=2026-08-12T19:55:11.006807Z digest=sha256:72dcfd272a2d900b0c37b7dd25a6b3b0ebb7aa06476bb09defd112217632215e

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.

source=pdf_text observed=2026-08-12T19:55:11.010551Z digest=sha256:79d0b1267f05bf7c7730c3f82be750fc45f06a5eb8ffa017be8b5077ad766194

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:11.014022Z digest=sha256:921277a78eb72d1b5e650807e42459ccdc4994d9ea607b939894e536f54b5e6f

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.

source=pdf_text observed=2026-08-12T19:55:11.017182Z digest=sha256:92c1ddc9c4bb66550d07194fde7a2fbd91c0051d5d4af4b47a598925187c2002

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:11.021006Z digest=sha256:96ba2a4bf648e9fe546ec0c87da28a0a3ff4432f142d38570df7d000fbe233c7

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.

source=pdf_text observed=2026-08-12T19:55:11.024225Z digest=sha256:c6d93f165061218094363e1904ae013de3d25af98713b25d87b3379d6a536805

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:11.027648Z digest=sha256:7be2935b9d88fbebbc09caddd558829271010e8bec912ac66a7470fa8b8d6bcd

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:11.030881Z digest=sha256:17b9192c435a7e926625eb470e4869251bd009f3b436402da5df8628d58d61f0

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-12T19:55:11.033921Z digest=sha256:6d2a7f7941eb6f79441ab6384e159e93288ca52f4a3d6d1633c23b4a77be4cd0

Pith citing papers

No inbound Pith citation observations are available.