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Paper Citation Record · LEDGER

Gamma-ray halos around pulsars as the key to understanding cosmic ray transport in the Galaxy

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2202.06899.

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

pith.paper-citation-record.v1
2202.06899 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T04:55:36.251896Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-24T06:49:02.002015Z

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 5813ac93-07e9-4aac-84a1-37c376969156 · inbound

Constraining the slow-diffusion zone size and electron injection spectral index for the Geminga pulsar halo cites this paper.

Constraining the slow-diffusion zone size and electron injection spectral index for the Geminga pulsar halo Gamma-ray halos around pulsars as the key to understanding cosmic ray transport in the Galaxy

Reference 5

Resolution
verified exact
arxiv_id, observed 2026-05-24T06:49:02.004383Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-05-24T06:48:57.946124Z digest=sha256:9278add1142db07b925e29a34d9f4ee1954e8bdbc134dcceeb2e2f6a47b8c012

Observation 590d0eeb-017e-4e64-a3ce-2529f396dec8 · inbound

Extended TeV Halos May Commonly Exist around Middle-Aged Pulsars cites this paper.

Extended TeV Halos May Commonly Exist around Middle-Aged Pulsars Gamma-ray halos around pulsars as the key to understanding cosmic ray transport in the Galaxy

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-16T04:54:30.177578Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:54:30.177578Z digest=sha256:fbf4a5243116273be5a8b6102ed1d28bcf2df3801a9528f8036b81a448179228

Observation cec1e270-611a-4e37-9a9e-c6108138853b · inbound

Absence of TeV halos around millisecond pulsars cites this paper.

Absence of TeV halos around millisecond pulsars Gamma-ray halos around pulsars as the key to understanding cosmic ray transport in the Galaxy

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-16T04:55:36.251896Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:55:36.251896Z digest=sha256:fd3ad910dee83c765cc4399ce99384fb58c90c0fbb5ff08b44833e004a67f454

Observation 0569c35b-391d-451d-9670-8a316d562d6a · inbound

PHECT: A lightweight computation tool for pulsar halo emission cites this paper.

PHECT: A lightweight computation tool for pulsar halo emission Gamma-ray halos around pulsars as the key to understanding cosmic ray transport in the Galaxy

Reference 11

Resolution
verified exact
arxiv_id, observed 2026-05-18T23:02:52.321733Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-05-18T23:02:15.483780Z digest=sha256:9bb02d3bc3f867e7b5e00b1ddb85cf915289d5cb1f8ec6b6f1e90961a1857513

Observation e4e85f86-7e12-46fc-b1a5-ed9222130f1b · inbound

Resolving diffusion signatures in distant pulsar halos with current and future experiments cites this paper.

Resolving diffusion signatures in distant pulsar halos with current and future experiments Gamma-ray halos around pulsars as the key to understanding cosmic ray transport in the Galaxy

Reference 8

Resolution
verified exact
arxiv_id, observed 2026-05-21T12:14:11.668567Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-05-21T12:11:58.523346Z digest=sha256:4bf45368e0f9759606415cd7d56b492b87b2dfca835983b236a1126400f8edc2

Observation 59737545-0a1c-47ba-8fc5-bb93962eaf71 · inbound

Search for TeV emission from spider millisecond pulsars with HAWC cites this paper.

Search for TeV emission from spider millisecond pulsars with HAWC Gamma-ray halos around pulsars as the key to understanding cosmic ray transport in the Galaxy

Reference 7

Resolution
verified exact
arxiv_id, observed 2026-05-14T01:23:34.799557Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-05-14T01:22:04.712990Z digest=sha256:d26d7062ffacdeeafead2c36bc82b23092a7842d1e9d8522b9fb16dc045c8493