Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Axion Emission Can Explain a New Hard $X$-ray Excess from Nearby Isolated Neutron Stars
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1910.04164.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T15:00:24.109152Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-18T15:51:34.571154Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 e5a52d56-ceec-4c5c-bf1e-a9369f5a457d · inbound
Mass-Gap Neutron Stars from Vector \texorpdfstring{$f(R)$}{f(R)} Gravity Inflationary Deformations cites this paper.
Mass-Gap Neutron Stars from Vector \texorpdfstring{$f(R)$}{f(R)} Gravity Inflationary Deformations Axion Emission Can Explain a New Hard $X$-ray Excess from Nearby Isolated Neutron Stars
Reference 33
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T15:00:24.109152Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3a7894f9-0ed6-4fef-a67a-17d7df3b49e1 · inbound
Axion lines from nuclear de-excitations in galactic stellar populations cites this paper.
Axion lines from nuclear de-excitations in galactic stellar populations Axion Emission Can Explain a New Hard $X$-ray Excess from Nearby Isolated Neutron Stars
Reference 26
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T10:57:49.131914Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f7ac3013-5651-430b-93f7-d84afe9ed4a7 · inbound
Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities cites this paper.
Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities Axion Emission Can Explain a New Hard $X$-ray Excess from Nearby Isolated Neutron Stars
Reference 107
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T15:51:34.572980Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.