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Paper Citation Record · LEDGER

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays

As of 11 August 2026, this Paper Citation Record lists 24 of 24 outbound references and 0 inbound Pith citation observations for arXiv:2502.08747.

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

pith.paper-citation-record.v1
2502.08747 v2

Coverage vector

measured 24 of 24 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-07T23:52:04.402453Z

measured 24 of 24 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+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

24 of 24 outbound references displayed

  • verified exact1
  • verified fuzzy6
  • unresolved17
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 46b4c446-c2dc-4e0c-bcdd-3f003d979e50 · outbound

This paper cites The Pierre Auger Cosmic Ray Observatory.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays The Pierre Auger Cosmic Ray Observatory

Reference 1

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 4fc6a254-c65c-4c24-b590-5c42c0d32c01 · outbound

This paper cites Pierog, I.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays Pierog, I

Reference 2

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation e8cc638f-9429-4464-a57a-1cf0224a50cc · outbound

This paper cites Ostapchenko,Phys.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays Ostapchenko,Phys

Reference 3

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation 50d93328-3cfd-4182-b509-baa473f253c8 · outbound

This paper cites Riehn, R.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays Riehn, R

Reference 4

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation 5396cf7c-584d-4447-bf59-124b7551b27a · outbound

This paper cites an unresolved cited work.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays Unresolved cited work

Reference 5

Resolution
unresolved
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation 6ac7dd9a-5917-441a-a66e-8a08f8c6ccda · outbound

This paper cites an unresolved cited work.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays Unresolved cited work

Reference 6

Resolution
unresolved
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation 24f7446e-fd18-4a0e-bf16-2e55b39b5d80 · outbound

This paper cites Pierog and K.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays Pierog and K

Reference 7

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation a1fc2b37-222e-4d86-ac10-8a6854020afa · outbound

This paper cites Ebr et al.,PoS ICRC2023(2023) 245.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays Ebr et al.,PoS ICRC2023(2023) 245

Reference 8

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation c899e132-47af-48b0-9c6e-dbec9ce12e34 · outbound

This paper cites Testing Hadronic-Model Predictions of Depth of Maximum of Air-Shower Profiles and Ground-Particle Signals using Hybrid Data of the Pierre Auger Observatory.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays Testing Hadronic-Model Predictions of Depth of Maximum of Air-Shower Profiles and Ground-Particle Signals using Hybrid Data of the Pierre Auger Observatory

Reference 9

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 00234da7-5907-4737-b52d-d79367f8c4d7 · outbound

This paper cites an unresolved cited work.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays Unresolved cited work

Reference 10

Resolution
unresolved
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation 4287889d-c4eb-4b6d-bf36-219bbb201ff9 · outbound

This paper cites Measurement of the Depth of Maximum of Air-Shower Profiles with energies between $\mathbf{10^{18.5}}$ and $\mathbf{10^{20}}$ eV using the Surface Detector of the Pierre Auger Observatory and Deep Learning.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays Measurement of the Depth of Maximum of Air-Shower Profiles with energies between $\mathbf{10^{18.5}}$ and $\mathbf{10^{20}}$ eV using the Surface Detector of the Pierre Auger Observatory and Deep Learning

Reference 11

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 7105b32f-ecd5-4f90-b56d-30d4da592aaf · outbound

This paper cites an unresolved cited work.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays Unresolved cited work

Reference 12

Resolution
unresolved
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation 2c2b1457-ea3c-4001-ad62-2d54f4fc6c7c · outbound

This paper cites Evidence for a mixed mass composition at the `ankle' in the cosmic-ray spectrum.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays Evidence for a mixed mass composition at the `ankle' in the cosmic-ray spectrum

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-07T23:52:04.349164Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T23:52:04.349164Z digest=sha256:081709215a02351f74d97308b9e18122a38ad3db767f92148b467761f9c8345b

Observation 67dead61-2eae-49b0-927a-909f51c1d5f8 · outbound

This paper cites an unresolved cited work.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays Unresolved cited work

Reference 14

Resolution
unresolved
raw_fallback, observed 2026-08-07T23:52:04.659967Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation 7e5a48c3-ef51-40e9-a7b6-73b95c9a6db1 · outbound

This paper cites an unresolved cited work.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays Unresolved cited work

Reference 15

Resolution
unresolved
raw_fallback, observed 2026-08-07T23:52:04.645330Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation aa477e1e-f6d7-41c4-9eed-cd3205854af4 · outbound

This paper cites an unresolved cited work.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays Unresolved cited work

Reference 16

Resolution
unresolved
raw_fallback, observed 2026-08-07T23:52:04.630407Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-08-07T23:52:04.363297Z digest=sha256:98dbe67bb01b65c47fa6e729ea636a79f3144224f2ffd2fda31dd4b47764bfe1

Observation c55f31bb-3453-48a1-9cae-1de4674fa83f · outbound

This paper cites Observation of a Large-scale Anisotropy in the Arrival Directions of Cosmic Rays above $8 \times 10^{18}$ eV.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays Observation of a Large-scale Anisotropy in the Arrival Directions of Cosmic Rays above $8 \times 10^{18}$ eV

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-07T23:52:04.367977Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation a3fddb34-d9c6-4895-8bca-ce3b88b6659a · outbound

This paper cites A Catalog of the Highest-Energy Cosmic Rays Recorded During Phase I of Operation of the Pierre Auger Observatory.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays A Catalog of the Highest-Energy Cosmic Rays Recorded During Phase I of Operation of the Pierre Auger Observatory

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-07T23:52:04.373099Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T23:52:04.373099Z digest=sha256:d24bf1f7f401668350c11ef91c6915197ab01dba47eb4d100d1e1f1946b2f23e

Observation 99622eb3-c4f4-49b1-9c8d-420fbb5dfb94 · outbound

This paper cites CRPropa 3.2 -- an advanced framework for high-energy particle propagation in extragalactic and galactic spaces.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays CRPropa 3.2 -- an advanced framework for high-energy particle propagation in extragalactic and galactic spaces

Reference 19

Resolution
unresolved
no resolver link, observed 2026-08-07T23:52:04.378180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation fa76bd36-5df1-4c59-958b-bf63c87dd52c · outbound

This paper cites The Coherent Magnetic Field of the Milky Way.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays The Coherent Magnetic Field of the Milky Way

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-07T23:52:04.382995Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation bbd5d58d-42b4-4492-b929-d5436d8c6ae9 · outbound

This paper cites A New Model of the Galactic Magnetic Field.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays A New Model of the Galactic Magnetic Field

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-07T23:52:04.388020Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T23:52:04.388020Z digest=sha256:f7cd9581eda8f8e8b34f46bb2b4b49220d08a0e35acd0970fe42f4903ad16e57

Observation 6267854b-5556-4c75-b60f-192365a65ae5 · outbound

This paper cites Planck intermediate results. XLII. Large-scale Galactic magnetic fields.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays Planck intermediate results. XLII. Large-scale Galactic magnetic fields

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-07T23:52:04.393027Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T23:52:04.393027Z digest=sha256:e2dc8dee6f439e9a439eab3ac499f9f24e9d8df33cdba421057e143b27f8ddfd

Observation 849acdb4-0396-4a85-bcea-09098db254e6 · outbound

This paper cites Sommers,Astroparticle Physics14(2001) 271.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays Sommers,Astroparticle Physics14(2001) 271

Reference 23

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-08-07T23:52:04.397678Z digest=sha256:088718376345e7ac071d40d5df2b0be82dcfdf48e32c3b7a3418f9f14cb6f557

Observation d219aa55-7579-4c22-9a61-722bc3a86413 · outbound

This paper cites Modification of the Dipole in Arrival Directions of Ultra-high-energy Cosmic Rays due to the Galactic Magnetic Field.

Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays Modification of the Dipole in Arrival Directions of Ultra-high-energy Cosmic Rays due to the Galactic Magnetic Field

Reference 24

Resolution
verified exact
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Pith citing papers

No inbound Pith citation observations are available.