Paper Citation Record · LEDGER

Constraints on the distribution of supernova remnants with Galactocentric radius

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1508.02931.

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

pith.paper-citation-record.v1
1508.02931 v1

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 2026-08-18T06:34:40.430872+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T05:31:18.452843Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T02:57:35.306649Z

Reference resolution

0 of 0 outbound references displayed

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verified fuzzy0
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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 3c136c08-eed2-4dc8-8fba-16a9a70f5c7c · inbound

A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz cites this paper.

A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz Constraints on the distribution of supernova remnants with Galactocentric radius

Reference 187

Resolution: verified exact; local_arxiv, observed 2026-05-25T03:56:35.607436Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation ec06df3a-bbc5-47c8-8b87-12484e74d483 · inbound

Modelling Galactic neutrino emission: contributions from massive star clusters and interstellar cosmic rays cites this paper.

Modelling Galactic neutrino emission: contributions from massive star clusters and interstellar cosmic rays Constraints on the distribution of supernova remnants with Galactocentric radius

Reference 55

Resolution: verified exact; local_arxiv, observed 2026-07-03T02:57:35.307858Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 4e67cb55-9f31-4336-a643-2be6bb66eaa2 · inbound

TeV-PeV Gamma-ray and Neutrino Emission in the Galactic Plane cites this paper.

TeV-PeV Gamma-ray and Neutrino Emission in the Galactic Plane Constraints on the distribution of supernova remnants with Galactocentric radius

Reference 168

Resolution: verified exact; local_arxiv, observed 2026-06-26T07:29:08.249351Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation f489e59f-46bc-43ed-9e51-6f4fdfeed643 · inbound

The Galactic Neutrino Sky: Predictions from Gamma-ray Source Populations cites this paper.

The Galactic Neutrino Sky: Predictions from Gamma-ray Source Populations Constraints on the distribution of supernova remnants with Galactocentric radius

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-11T05:31:18.452843Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.