Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
High-energy gamma-ray and neutrino emissions from interacting supernovae based on radiation hydrodynamic simulations: a case of SN 2023ixf
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2409.18935.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T18:34:13.803786Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-02T11:16:54.129070Z
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 510a1f67-ce7a-458a-b3e8-71926d9a5941 · inbound
SN 2023ixf: The Closest Supernova of the Decade cites this paper.
SN 2023ixf: The Closest Supernova of the Decade High-energy gamma-ray and neutrino emissions from interacting supernovae based on radiation hydrodynamic simulations: a case of SN 2023ixf
Reference 63
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T18:34:13.803786Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 201d2bda-95d0-4f33-9498-f81b0dae4268 · inbound
Exploring the properties of newborn pulsars with high-energy neutrinos cites this paper.
Exploring the properties of newborn pulsars with high-energy neutrinos High-energy gamma-ray and neutrino emissions from interacting supernovae based on radiation hydrodynamic simulations: a case of SN 2023ixf
Reference 54
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T15:18:11.654538Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a52d6150-b830-4904-ab52-b31c59dc5032 · inbound
Observational signatures of thermonuclear electron-capture supernovae -- Ne II line strengthening and color evolution as traces of the explosion mechanism cites this paper.
Observational signatures of thermonuclear electron-capture supernovae -- Ne II line strengthening and color evolution as traces of the explosion mechanism High-energy gamma-ray and neutrino emissions from interacting supernovae based on radiation hydrodynamic simulations: a case of SN 2023ixf
Reference 246
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T11:16:54.130415Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.