Paper Citation Record · LEDGER

Heavy QCD axion model in light of pulsar timing arrays

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2307.12385.

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

pith.paper-citation-record.v1
2307.12385 v2

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 2026-08-16T06:30:59.297886+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T20:02:43.055303Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T18:11:06.702141Z

Reference resolution

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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 093836a8-aeb3-45b0-9e9e-d805b3750335 · inbound

Glueball Axion-Like Particles cites this paper.

Glueball Axion-Like Particles Heavy QCD axion model in light of pulsar timing arrays

Reference 120

Resolution: unresolved; no resolver link, observed 2026-08-12T18:22:42.604123Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dcd52cf5-dd22-46e6-9bd9-334b0791949b · inbound

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise cites this paper.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Heavy QCD axion model in light of pulsar timing arrays

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.055303Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9aec7b11-44ec-4b43-9a65-7924d200c627 · inbound

NANOGrav 15-year gravitational-wave signals from binary supermassive black-holes seeded by primordial black holes, and implications for the origins of Little Red Dots cites this paper.

NANOGrav 15-year gravitational-wave signals from binary supermassive black-holes seeded by primordial black holes, and implications for the origins of Little Red Dots Heavy QCD axion model in light of pulsar timing arrays

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-03T23:49:28.578170Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 66eb5411-81ce-41d9-a1ee-4a26e354c869 · inbound

Constraints on the inflationary vacuum and reheating era from NANOGrav cites this paper.

Constraints on the inflationary vacuum and reheating era from NANOGrav Heavy QCD axion model in light of pulsar timing arrays

Reference 19

Resolution: verified exact; arxiv_id, observed 2026-05-11T18:11:06.704587Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.