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Paper Citation Record · LEDGER

New full-sky studies of the distribution of ultra-high-energy cosmic-ray arrival directions

As of 12 August 2026, this Paper Citation Record lists 10 of 10 outbound references and 0 inbound Pith citation observations for arXiv:2507.10441.

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

pith.paper-citation-record.v1
2507.10441 v1

Coverage vector

measured 10 of 10 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-06T17:36:00.617098Z

measured 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+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

10 of 10 outbound references displayed

  • verified exact4
  • verified fuzzy1
  • unresolved5
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 2ecfac2f-f97e-45fa-a302-5ec7386568a1 · outbound

This paper cites How isotropic can the UHECR flux be?.

New full-sky studies of the distribution of ultra-high-energy cosmic-ray arrival directions How isotropic can the UHECR flux be?

Reference 1

Resolution
verified exact
local_arxiv, observed 2026-08-06T17:36:01.576646Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-08-06T17:35:59.672485Z digest=sha256:2f16475e320e2816d2c4caa8ccec43ede82b094c4f12408055f8c712da0ef5a7

Observation 2bb8f78e-8faa-4e7d-b4b5-1e78ba8f864a · outbound

This paper cites an unresolved cited work.

New full-sky studies of the distribution of ultra-high-energy cosmic-ray arrival directions Unresolved cited work

Reference 2

Resolution
unresolved
raw_fallback, observed 2026-08-06T17:36:02.143783Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-08-06T17:35:59.767543Z digest=sha256:3903685f5caa25bcda4c618046318602b3be2414eb139b8c527eaf9904a473a0

Observation 5cc802e7-e574-41d1-9b5b-41a320d76a27 · outbound

This paper cites Large-scale cosmic ray anisotropies with 19 years of data from the Pierre Auger Observatory.

New full-sky studies of the distribution of ultra-high-energy cosmic-ray arrival directions Large-scale cosmic ray anisotropies with 19 years of data from the Pierre Auger Observatory

Reference 3

Resolution
unresolved
no resolver link, observed 2026-08-06T17:35:59.900396Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T17:35:59.900396Z digest=sha256:037ba92e1f434b14f0073c8ec316170dade722f10672b64543661af9c6c30349

Observation 0f24b5e8-c864-4e1c-860f-65fece2bcab3 · outbound

This paper cites Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory.

New full-sky studies of the distribution of ultra-high-energy cosmic-ray arrival directions Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory

Reference 4

Resolution
unresolved
no resolver link, observed 2026-08-06T17:36:00.015501Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T17:36:00.015501Z digest=sha256:0538bf1d55bd0dd2189281d90028cf41518ec22b8c36344ba61e5c7d83036a86

Observation e6ef2081-4347-43b2-8b30-0e26e21292d2 · outbound

This paper cites Searches for Large-Scale Anisotropy in the Arrival Directions of Cosmic Rays Detected above Energy of $10^{19}$ eV at the Pierre Auger Observatory and the Telescope Array.

New full-sky studies of the distribution of ultra-high-energy cosmic-ray arrival directions Searches for Large-Scale Anisotropy in the Arrival Directions of Cosmic Rays Detected above Energy of $10^{19}$ eV at the Pierre Auger Observatory and the Telescope Array

Reference 5

Resolution
verified exact
local_arxiv, observed 2026-08-06T17:36:01.255628Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-08-06T17:36:00.104398Z digest=sha256:7ee5e3841f18828a821dc520df11be9180e6c03f688fe8589d6384da1e9cf233

Observation 5e5d5ac4-ed20-4671-aa31-b77b06193532 · outbound

This paper cites Indications of Intermediate-Scale Anisotropy of Cosmic Rays with Energy Greater Than 57 EeV in the Northern Sky Measured with the Surface Detector of the Telescope Array Experiment.

New full-sky studies of the distribution of ultra-high-energy cosmic-ray arrival directions Indications of Intermediate-Scale Anisotropy of Cosmic Rays with Energy Greater Than 57 EeV in the Northern Sky Measured with the Surface Detector of the Telescope Array Experiment

Reference 6

Resolution
unresolved
no resolver link, observed 2026-08-06T17:36:00.185793Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T17:36:00.185793Z digest=sha256:09e21ecb35be37442150026f098d6287c4224266528cdede58484d10c52c9e4f

Observation 4f61ec80-e616-415e-8870-b081209ac998 · outbound

This paper cites Tinyakov et al.

New full-sky studies of the distribution of ultra-high-energy cosmic-ray arrival directions Tinyakov et al

Reference 7

Resolution
verified fuzzy
raw_fallback, observed 2026-08-06T17:36:01.890577Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-08-06T17:36:00.298813Z digest=sha256:a0d2eb122d925a769c3e77048506eebd2afb883ce178ba786760f3f70a835e6d

Observation 3df9af20-242c-4e27-a955-014365a91165 · outbound

This paper cites Combined fit of spectrum and composition data as measured by the Pierre Auger Observatory.

New full-sky studies of the distribution of ultra-high-energy cosmic-ray arrival directions Combined fit of spectrum and composition data as measured by the Pierre Auger Observatory

Reference 8

Resolution
unresolved
no resolver link, observed 2026-08-06T17:36:00.411699Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T17:36:00.411699Z digest=sha256:0453e493963d21b6ee8983ff4c16c143241c4a25a4fd9152ce5ed42be1673c85

Observation 534b4a2b-e247-4599-92b1-e669083197f3 · outbound

This paper cites Likelihood methods for the combined analysis of CMB temperature and polarisation power spectra.

New full-sky studies of the distribution of ultra-high-energy cosmic-ray arrival directions Likelihood methods for the combined analysis of CMB temperature and polarisation power spectra

Reference 9

Resolution
verified exact
local_arxiv, observed 2026-08-06T17:36:00.987689Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-08-06T17:36:00.485869Z digest=sha256:c037f7c2499f1c29bbfff61d29a0068e40e21410c465a9266a83d3b2496996f9

Observation 8ac1539f-e798-4873-a3ea-5c66a4392a66 · outbound

This paper cites Detecting ultra-high energy cosmic ray anisotropies through cross-correlations.

New full-sky studies of the distribution of ultra-high-energy cosmic-ray arrival directions Detecting ultra-high energy cosmic ray anisotropies through cross-correlations

Reference 10

Resolution
verified exact
local_arxiv, observed 2026-08-06T17:36:00.791260Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-08-06T17:36:00.617098Z digest=sha256:b05c8d7ed72722df084021d84483f74e497236fb4e39e4994d1b595d4acbc34a

Pith citing papers

No inbound Pith citation observations are available.