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Paper Citation Record · LEDGER

The ubiquity of variable radio emission and spin-down rates in pulsars

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2501.03500.

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

pith.paper-citation-record.v1
2501.03500 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T16:38:01.982666Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-12T09:28:41.161713Z

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 8c632c89-2733-4b93-9c5a-2e650b4954a9 · inbound

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years cites this paper.

Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years The ubiquity of variable radio emission and spin-down rates in pulsars

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-05T16:38:01.982666Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T16:38:01.982666Z digest=sha256:1e5841e2e6ff9617133b4d5af3b64ade29f0234abbb83017b746e49bbcf21aa0

Observation 721b9422-28a7-4dfb-a796-8f44276bfa4f · inbound

Probing Neutron Star Interiors and the Properties of Cold Ultra-dense Matter with the SKAO cites this paper.

Probing Neutron Star Interiors and the Properties of Cold Ultra-dense Matter with the SKAO The ubiquity of variable radio emission and spin-down rates in pulsars

Reference 216

Resolution
verified exact
local_arxiv, observed 2026-07-12T09:28:41.163894Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-12T09:19:35.429829Z digest=sha256:d4d25fb4ad9f3a07466131c18319d35f2f8991066c69a0c67f0f548d6ca970eb

Observation 5d9645b5-55b9-4272-b9ad-a1beab75f298 · inbound

The SKAO Pulsar Timing Array cites this paper.

The SKAO Pulsar Timing Array The ubiquity of variable radio emission and spin-down rates in pulsars

Reference 122

Resolution
unresolved
no resolver link, observed 2026-07-12T05:10:13.912506Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T05:10:13.912506Z digest=sha256:79ec0b6501bd8532dcd429e48343f0360b6134d9289bd716cc09fe1478c6a3f3

Observation 293058c6-8c1e-4772-b146-5c0cb1f8f1ad · inbound

Understanding the Neutron Star Population with the SKAO Telescopes cites this paper.

Understanding the Neutron Star Population with the SKAO Telescopes The ubiquity of variable radio emission and spin-down rates in pulsars

Reference 161

Resolution
unresolved
no resolver link, observed 2026-07-12T05:00:29.237939Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T05:00:29.237939Z digest=sha256:00730965a59bbb3e1030e39a85f27c6552b7cbe2976a1aa00ec0f92570d1d876